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1

Monochromator Crystal Glitch Library  

DOE Data Explorer (OSTI)

SSRL's Monochromator Crystal Glitch Library allows users to view glitch spectra online, list specific crystal orientations, and download PDF files of the glitch spectra. (Specialized Interface)

2

Pulsed-neutron monochromator  

DOE Patents (OSTI)

In one aspect, the invention is an improved pulsed-neutron monochromator of the vibrated-crystal type. The monochromator is designed to provide neutron pulses which are characterized both by short duration and high density. A row of neutron-reflecting crystals is disposed in a neutron beam to reflect neutrons onto a common target. The crystals in the row define progressively larger neutron-scattering angles and are vibrated sequentially in descending order with respect to the size of their scattering angles, thus generating neutron pulses which arrive simultaneously at the target. Transducers are coupled to one end of the crystals to vibrate them in an essentially non-resonant mode. The transducers propagate transverse waves in the crystal which progress longitudinally therein. The waves are absorbed at the undriven ends of the crystals by damping material mounted thereon. In another aspect, the invention is a method for generating neutron pulses characterized by high intensity and short duration.

Mook, H.A. Jr.

1984-01-01T23:59:59.000Z

3

Pulsed-neutron monochromator  

DOE Patents (OSTI)

In one aspect, the invention is an improved pulsed-neutron monochromator of the vibrated-crystal type. The monochromator is designed to provide neutron pulses which are characterized both by short duration and high density. A row of neutron-reflecting crystals is disposed in a neutron beam to reflect neutrons onto a common target. The crystals in the row define progressively larger neutron-scattering angles and are vibrated sequentially in descending order with respect to the size of their scattering angles, thus generating neutron pulses which arrive simultaneously at the target. Transducers are coupled to one end of the crystals to vibrate them in an essentially non-resonant mode. The transducers propagate transverse waves in the crystal which progress longitudinally therein. The wave are absorbed at the undriven ends of the crystals by damping material mounted thereon. In another aspect, the invention is a method for generating neutron pulses characterized by high intensity and short duration.

Mook, Jr., Herbert A. (Oak Ridge, TN)

1985-01-01T23:59:59.000Z

4

High energy resolution, high angular acceptance crystal monochromator  

DOE Patents (OSTI)

A 4-bounce dispersive crystal monochromator reduces the bandpass of synchrotron radiation to a 10-50 meV range without sacrificing angular acceptance. The monochromator includes the combination of an asymmetrical channel-cut single crystal of lower order reflection and a symmetrical channel-cut single crystal of higher order reflection in a nested geometric configuration. In the disclosed embodiment, a highly asymmetrically cut (.alpha.=20) outer silicon crystal (4 2 2) with low order reflection is combined with a symmetrically cut inner silicon crystal (10 6 4) with high order reflection to condition a hard x-ray component (5-30 keV) of synchrotron radiation down to the .mu.eV-neV level. Each of the crystals is coupled to the combination of a positioning inchworm and angle encoder via a respective rotation stage for accurate relative positioning of the crystals and precise energy tuning of the monochromator.

Alp, Ercan E. (Bolingbrook, IL); Mooney, Timothy M. (Westmont, IL); Toellner, Thomas (Green Bay, WI)

1996-06-04T23:59:59.000Z

5

APS high heat load monochromator  

SciTech Connect

This document contains the design specifications of the APS high heat load (HHL) monochromator and associated accessories as of February 1993. It should be noted that work is continuing on many parts of the monochromator including the mechanical design, crystal cooling designs, etc. Where appropriate, we have tried to add supporting documentation, references to published papers, and calculations from which we based our decisions. The underlying philosophy behind performance specifications of this monochromator was to fabricate a device that would be useful to as many APS users as possible, that is, the design should be as generic as possible. In other words, we believe that this design will be capable of operating on both bending magnet and ID beamlines (with the appropriate changes to the cooling and crystals) with both flat and inclined crystal geometries and with a variety of coolants. It was strongly felt that this monochromator should have good energy scanning capabilities over the classical energy range of about 4 to 20 keywith Si (111) crystals. For this reason, a design incorporating one rotation stage to drive both the first and second crystals was considered most promising. Separate rotary stages for the first and second crystals can sometimes provide more flexibility in their capacities to carry heavy loads (for heavily cooled first crystals or sagittal benders of second crystals), but their tuning capabilities were considered inferior to the single axis approach.

Lee, W.K.; Mills, D.

1993-02-01T23:59:59.000Z

6

Thermal gradient crystals as tuneable monochromator for high energy X-rays  

SciTech Connect

At the high energy synchrotron radiation beamline BW5 at DORIS III at DESY a new monochromator providing broad energy bandwidth and high reflectivity is in use. On a small 10x10x5 mm{sup 3} silicon crystal scattering at the (311) reflection a thermal gradient is applied, which tunes the scattered energy bandwidth. The (311) reflection strongly suppresses the higher harmonics allowing the use of an image plate detector for crystallography. The monochromator can be used at photon energies above 60 keV.

Ruett, U.; Schulte-Schrepping, H.; Heuer, J.; Zimmermann, M. von [Hamburger Synchrotron Strahlungslabor (HASYLAB), at Deutsches Elektronensychrotron (DESY), Notkestr. 85, 22603 Hamburg (Germany)

2010-06-23T23:59:59.000Z

7

A dynamic focusing x-ray monochromator for a wiggler beam line at the SRS of the SERC Daresbury Laboratory  

SciTech Connect

A Si(220) double-crystal monochromator for the energy range 10--30 keV is presented. It will be used for EXAFS as well as powder diffraction measurements. To determine the requirements for this monochromator we looked, apart from mean considerations, at the requirements dictated by EXAFS in transmission mode. For good data analyses the proper shape, amplitude, and location at the energy axis of each wiggle is required. Moreover it is essential to separate the wiggles from background and noise. For the latter a high flux through the sample is desirable, which can be achieved by horizontal focusing of the beam. For that we have chosen to bend the second crystal sagitally. The sagittal bending radius is adjustable between 50 and 0.8 m, because for different energies different sagittal radii are necessary to focus the beam on the sample. The mean meridional radius of the second crystal is fixed at 130 m, which is an optimization for 20 keV. The meridional radius of the first crystal can be tuned between 100 and 500 m. When this radius is set to 130 m the energy resolution is calculated to be 6, 3, and 35 eV for 10, 20, and 30 keV (for perfectly bent crystals). By changing the meridional radius of the first crystal, future users of this monochromator can make the trade off between resolution and intensity. Movement of the monochromator exit beam, during a scan, will occur due to the monochromator geometry, but is reduced as much as possible by using an asymmetrically cut second crystal, with an asymmetry angle of 2.5{degree}. The average exit beam movement of the monochromator for a 1-keV scan is 20 {mu}m. For 40% of the energy range (10--30 keV) the exit beam position remains within 10 {mu}m. For the second crystal no translation stage is used.

De Bruijn, D.; Van Zuylen, P. (TNO Institute of Applied Physics, P.O. Box 155, 2600 AD Delft (Netherlands)); Kruizinga, G. (Netherlands Organization for Scientific Research (NWO), P.O. Box 93138, 2509 AC Den Haag (Netherlands) State University of Utrecht, Sorbonnelaan 16, 3508 TB Utrecht (Netherlands))

1992-01-01T23:59:59.000Z

8

Back-scattering channel-cut high-resolution monochromator for inelastic x-ray scattering  

SciTech Connect

We report on a design and on some experimental results for the performance of a new high energy resolution monochromator. It is a large channel-cut Si crystal with a 197 mm separation between the two faces designed to operate in a near-backscattering regime. The device was tested as a second monochromator on Sector 3 of the Synchrotron Radiation Instrumentation Collaborative Access Team (SRI-CAT) at the Advanced Photon Source using the Si(777) reflection at a photon energy of 13.84 keV. The same monochromator can be used for other energies with reflections of the type (hhh). Special care has been taken to equalize the temperature of the two faces by employing a Peltier heat pump. A Si(111) double-crystal pre-monochromator designed to withstand the high heat load of the undulator radiation was used upstream on the beamline. The measured throughput efficiency of the Si(777) channel-cut monochromator was less ideal by a factor of 1.9. Dynamical diffraction theory was used to calculate the throughput of an ideally perfect crystal.

Kushnir, V.I.; Abbamonte, P.M.; Macrander, A.T.; Schwoerer-Boehning, M.

1997-08-01T23:59:59.000Z

9

Highly asymmetric Laue focusing monochromator  

SciTech Connect

By using two highly asymmetric Laue crystals in a dispersive arrangement with a circular profile (Oe 8 mm) we have created a sagittaly focusing Laue system for the first time. The crystallographic planes (111) of the two Si crystals formed an angle of 7.95 deg. with the entrance surface. The crystals dimensions were 40 mmx20 mm and the diffracting surface was a 0.5 mm thick neck between the two circular profiles. The 15.35 keV diffracted beam formed an angle of 0.55 deg. with the exit surface. The calculated focusing distance of the Laue-Laue focusing system was 14 m.

Oberta, P. [Institute of Physics, Academy of Sciences of the Czech Republic v.v.i., Na Slovance 2, Praha 8 (Czech Republic); Swiss Light Source, Paul Scherrer Institut, Villigen (Switzerland); Mikulik, P. [Department of Condensed Matter Physics, Faculty of Science, Masaryk University, Kotlarska 2, Brno (Czech Republic); Hrdy, J.; Kittler, M. [Institute of Physics, Academy of Sciences of the Czech Republic v.v.i., Na Slovance 2, Praha 8 (Czech Republic)

2010-06-23T23:59:59.000Z

10

Categorical Exclusion Determinations: B5.16 | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

6 6 Categorical Exclusion Determinations: B5.16 Existing Regulations B5.16: Solar photovoltaic systems The installation, modification, operation, and removal of commercially available solar photovoltaic systems located on a building or other structure (such as rooftop, parking lot or facility, and mounted to signage, lighting, gates, or fences), or if located on land, generally comprising less than 10 acres within a previously disturbed or developed area. Covered actions would be in accordance with applicable requirements (such as local land use and zoning requirements) in the proposed project area and would incorporate appropriate control technologies and best management practices. DOCUMENTS AVAILABLE FOR DOWNLOAD July 17, 2013 CX-010763: Categorical Exclusion Determination

11

Categorical Exclusion Determinations: B5.16 | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

October 11, 2012 October 11, 2012 CX-009435: Categorical Exclusion Determination Town of Poughkeepsie NEPA Statement of Work CX(s) Applied: A9, A11, B1.35, B2.2, B5.1, B5.14, B5.16, B5.17, B5.18, B5.19 Date: 10/11/2012 Location(s): New York Offices(s): Golden Field Office September 21, 2012 CX-009238: Categorical Exclusion Determination Routine and Non-Routine Activities at the Grand Junction, Colorado, Office Site CX(s) Applied: B1.3, B1.4, B1.7, B1.13, B1.15, B1.16, B1.23, B1.24, B1.28, B2.1, B2.2, B2.4, B2.5, B3.1, B5.16, B6.1 Date: 09/21/2012 Location(s): Grand Junction Offices(s): Legacy Management September 21, 2012 CX-009340: Categorical Exclusion Determination Cost-Effective Treatment of Produced Water Using Co-Produced Energy Sources Phase II: Field Scale Demonstration and Commercialization

12

Investigation of pin-post monochromators for a wiggler beamline  

SciTech Connect

Three water-cooled pin-post monochromators, to be used on a wiggler beamline at the Advanced Photon Source (APS), were built with the heat exchanger engineered to provide very high heat transfer. The geometry of the heat exchanger as well as calculated data on the heat transfer will be presented. Before using the monochromators on the beamline, they were checked by x-ray diffraction topography. Reflections (333) and (220) in Bragg case were utilized. In all crystals, similar patterns of strain in the diffracting silicon layers were revealed, which can be attributed to the geometry of the heat exchangers, the bonding technology, and the thickness of the top layer. Conclusions about construction of future pin-post monochromators have been drawn.

Krasnicki, S.; Maj, J. [Argonne National Lab., IL (United States); Schildkamp, W. [Univ. of Chicago, IL (United States); Tonnessen, T. [Boeing North American, Albuquerque, NM (United States). Albuquerque Operations

1998-12-31T23:59:59.000Z

13

Synchronized monochromator and insertion device energy scans at SLS  

SciTech Connect

Synchronous monochromator and insertion device energy scans were implemented at the Surfaces/Interfaces:Microscopy (SIM) beamline in order to provide the users fast X-ray magnetic dichroism studies (XMCD). A simple software control scheme is proposed based on a fast monochromator run-time energy readback which quickly updates the insertion device requested energy during an on-the-fly X-ray absorption scan (XAS). In this scheme the Plain Grating Monochromator (PGM) motion control, being much slower compared with the insertion device (APPLE-II type undulator), acts as a 'master' controlling the undulator 'slave' energy position. This master-slave software implementation exploits EPICS distributed device control over computer network and allows for a quasi-synchronous motion control combined with data acquisition needed for the XAS or XMCD experiment.

Krempasky, J.; Flechsig, U.; Korhonen, T.; Zimoch, D.; Quitmann, Ch.; Nolting, F. [Paul Scherrer Institut, Villigen, Swiss Light Source, 5235 Villigen PSI (Switzerland)

2010-06-23T23:59:59.000Z

14

Optical system for high resolution spectrometer/monochromator  

DOE Patents (OSTI)

An optical system for use in a spectrometer or monochromator employing a mirror which reflects electromagnetic radiation from a source to converge with same in a plane is disclosed. A straight grooved, varied-spaced diffraction grating receives the converging electromagnetic radiation from the mirror and produces a spectral image for capture by a detector, target or like receiver. 11 figs.

Hettrick, M.C.; Underwood, J.H.

1988-10-11T23:59:59.000Z

15

Grating monochromator for electron cyclotron resonance ion source operation  

SciTech Connect

Recently, we started to observe optical line spectra from an ECR plasma using a grating monochromator with a photomultiplier. The light intensity of line spectrum from the ECR plasma had a strong correlation with ion beam intensity measured by a magnetic mass analyzer. This correlation is a significant information for beam tuning because it allows the extraction of the desired ion species from the ECR plasma. Separation of ion species of the same charge to mass ratio with an electromagnetic mass analyzer is known to be an exceptionally complex process, but this research gives new insights into its simplification. In this paper, the grating monochromator method for beam tuning of a Hyper-ECR ion source as an injector for RIKEN azimuthal varying field (AVF) cyclotron is described.

Muto, Hideshi [Center of General Education, Tokyo University of Science, Suwa, 5000-1 Toyohira, Chino Nagano 391-0292 (Japan)] [Center of General Education, Tokyo University of Science, Suwa, 5000-1 Toyohira, Chino Nagano 391-0292 (Japan); Ohshiro, Yukimitsu; Yamaka, Shouichi; Watanabe, Shin-ichi; Yamaguchi, Hidetoshi; Shimoura, Susumu [Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Riken Campus, Wako Saitama 351-0198 (Japan)] [Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Riken Campus, Wako Saitama 351-0198 (Japan); Oyaizu, Michihiro; Kase, Masayuki [RIKEN Nishina Center for Accelerator-Based Science, Wako Saitama 351-0198 (Japan)] [RIKEN Nishina Center for Accelerator-Based Science, Wako Saitama 351-0198 (Japan); Kubono, Shigeru [Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Riken Campus, Wako Saitama 351-0198 (Japan) [Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Riken Campus, Wako Saitama 351-0198 (Japan); RIKEN Nishina Center for Accelerator-Based Science, Wako Saitama 351-0198 (Japan); Institute of Modern Physics, Chinese Academy of Sciences, Nanchang Road 509, Lanzhou 730000 (China); Hattori, Toshiyuki [Heavy Ion Cancer Therapy Center, National Institute of Radiological Sciences, 4-9-1 Anagawa, Inage Chiba 263-855 (Japan)] [Heavy Ion Cancer Therapy Center, National Institute of Radiological Sciences, 4-9-1 Anagawa, Inage Chiba 263-855 (Japan)

2013-07-15T23:59:59.000Z

16

Design and analysis of a high heat load pin-post monochromator crystal with an integral water manifold  

SciTech Connect

Conventional minichannel water cooling geometry will not perform satisfactorily for x-radiation from a wiggler source at the Advanced Photon Source. For closed-gap wiggler operation, cryogenic silicon appears to be the only option for crystals in Bragg-Bragg geometry. For operation of the wiggler at more modest critical energies ({lt}17 keV), the first crystal can be cooled by a pin-post cooling scheme, using water at room temperature as a coolant. In order to limit the water consumption to 4 gpm and hence the risk of introducing vibrations to the crystal, the intensely cooled area of the crystal was matched to the footprint of the beam, leaving a less cooled area of the crystal subject to survival in a missteered beam but not to perform as a monochromator. The manifold design avoids large areas of high water pressure that would bow the crystal. We present here the design of a pin-post monochromator consisting of a four-layer silicon manifold system and an integrally bonded 39{percent} nickel-iron alloy base plate. A transparent prototype of the design will be exhibited. Fabrication techniques and design advantages will be discussed. {copyright} {ital 1996 American Institute of Physics.}

Schildkamp, W. [Consortium for Advanced Radiation Sources, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637 (United States)] [Consortium for Advanced Radiation Sources, University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637 (United States); Tonnessen, T. [Rocketdyne Albuquerque Operations, 2511 C. Broadbent Parkway, N.E., Albuquerque, NM 87107 (United States)] [Rocketdyne Albuquerque Operations, 2511 C. Broadbent Parkway, N.E., Albuquerque, NM 87107 (United States)

1996-09-01T23:59:59.000Z

17

Development of the Channel Cut Monochromator with Curved Reflecting Surfaces at NSRL  

SciTech Connect

To simplify the complicated mechanism of the traditional double crystal monochromator for synchrotron radiation, a kind of channel cut monochromator with curved reflecting surfaces to fix the exit beam position was successfully developed at NSRL. The performance of this monochromator, which includes the relative efficiency, diffraction bandwidth and deviation of the beam spot, was calculated and measured. The analysis of these results are presented in this paper.

Kang Le; Li Zhongliang; Feng Liangjie; Dong Xiaohao; Lu Lei; Zhao Feiyun; Xu Chaoyin [National Synchrotron Radiation Laboratory, University of Science and Technology of China, Hefei 230029, Anhui (China)

2010-06-23T23:59:59.000Z

18

[FIXED] perl 5.16.0 File::Glob() causes crashes  

NLE Websites -- All DOE Office Websites (Extended Search)

works, more complex cases fail. This is a known issue for perl 5.16.0, and there is a patch available. During the quarterly maintenance we will patch the perl installation to...

19

FS MTG. 4/8/03 Approved 5-16-03  

E-Print Network (OSTI)

FS MTG. 4/8/03 Approved 5-16-03 Faculty Senate Meeting April 8, 2003 4:30 P.M. SUB--Conference Room letter from Peter Rolnick was read by R. Smith. A. Preussner commented regarding the process the Faculty. An amendment proposed by V. Pultz in an email was discussed. V. Pultz #12;FS MTG. 4/8/03 Approved 5-16-03 moved

Gering, Jon C.

20

Quick-scanning x-ray absorption spectroscopy system with a servo-motor-driven channel-cut monochromator with a temporal resolution of 10 ms  

SciTech Connect

We have developed a quick-scanning x-ray absorption fine structure (QXAFS) system and installed it at the recently constructed synchrotron radiation beamline BL33XU at the SPring-8. Rapid acquisition of high-quality QXAFS data was realized by combining a servo-motor-driven Si channel-cut monochromator with a tapered undulator. Two tandemly aligned monochromators with channel-cut Si(111) and Si(220) crystals covered energy ranges of 4.0-28.2 keV and 6.6-46.0 keV, respectively. The system allows the users to adjust instantly the energy ranges of scans, the starting angles of oscillations, and the frequencies. The channel-cut crystals are cooled with liquid nitrogen to enable them to withstand the high heat load from the undulator radiation. Deformation of the reflecting planes is reduced by clamping each crystal with two cooling blocks. Performance tests at the Cu K-edge demonstrated sufficiently high data quality for x-ray absorption near-edge structure and extended x-ray absorption fine-structure analyses with temporal resolutions of up to 10 and 25 ms, respectively.

Nonaka, T.; Dohmae, K.; Araki, T.; Hayashi, Y.; Hirose, Y. [Toyota Central R and D Labs., Inc., Nagakute, Aichi 480-1192 (Japan); Uruga, T.; Yamazaki, H.; Tanida, H.; Goto, S. [JASRI/Spring-8, 1-1-1, Kouto, Sayo-cho, Sayo-gun, Hyogo 679-5198 (Japan); Mochizuki, T. [JASRI/Spring-8, 1-1-1, Kouto, Sayo-cho, Sayo-gun, Hyogo 679-5198 (Japan); Toyama Corp., Zama, Kanagawa 228-0003 (Japan)

2012-08-15T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

A Laboratory-based Hard X-ray Monochromator for High-Resolution X-ray Emission Spectroscopy and X-ray Absorption Near Edge Structure Measurements  

E-Print Network (OSTI)

We report the development of a laboratory-based Rowland-circle monochromator that incorporates a low poer x-ray (bremsstrahlung) tube source, a spherically-bent crystal analyzer (SBCA), and an energy-resolving solid-state detector. This relatively inexpensive, introductory level instrument achieves 1-eV energy resolution for photon energies of 5 keV to 10 keV while also dmeonstrating a net efficiency previously seen only in laboratory monochromators having much coarser energy resolution. Despite the use of only a compact, air-cooled 10 W x-ray tube, we find count rates for nonresonant x-ray emission spectroscopy (XES) comparable to those achived at monochromatized spectroscopy beamlines at synchrotron light sources. For x-ray absorption near edge structure (XANES), the monochromatized flux is small (due to the use of a low-powered x-ray generator) but still useful for routine transmission-mode studies of concentrated samples. These results indicate that upgrading to a standard commercial high-powered line-foc...

Seidler, G T; Remesnik, A J; Pacold, J I; Ball, N A; Barry, N; Styczinski, M; Hoidn, O R

2014-01-01T23:59:59.000Z

22

PERFORMANCE AND APPLICATION OF A DOUBLE CRYSTAL MONOCHROMATOR IN THE ENERGY REGION 800 < hv < 4500 eV  

E-Print Network (OSTI)

monochromator which is not UHV compatible and does not haveof this ultrahigh-vacuum (UHV) compatible constant deviationmonochromator, and (4) is UHV (~10~ torr) compatible. These

Hussain, Z.

2010-01-01T23:59:59.000Z

23

Inclined monochromator for high heat-load synchrotron x-ray radiation  

DOE Patents (OSTI)

A double crystal monochromator is described including two identical, parallel crystals, each of which is cut such that the normal to the diffraction planes of interest makes an angle less than 90 degrees with the surface normal. Diffraction is symmetric, regardless of whether the crystals are symmetrically or asymmetrically cut, enabling operation of the monochromator with a fixed plane of diffraction. As a result of the inclination of the crystal surface, an incident beam has a footprint area which is elongated both vertically and horizontally when compared to that of the conventional monochromator, reducing the heat flux of the incident beam and enabling more efficient surface cooling. Because after inclination of the crystal only a fraction of thermal distortion lies in the diffraction plane, slope errors and the resultant misorientation of the diffracted beam are reduced. 11 figures.

Khounsary, A.M.

1994-02-15T23:59:59.000Z

24

Precision mechanical design of an UHV-compatible artificial channel-cut x-ray monochromator.  

SciTech Connect

A novel ultra-high-vacuum (UHV)-compatible x-ray monochromator has been designed and commissioned at the undulator beamline 8-ID-I at the Advanced Photon Source (APS) for x-ray photon correlation spectroscopy applications. To meet the challenging stability and x-ray optical requirements, the monochromator integrates two new precision angular positioning mechanisms into its crystal optics motion control system: An overconstrained weak-link mechanism that enables the positioning of an assembly of two crystals to achieve the same performance as a single channel-cut crystal, the so called 'artificial channel-cut crystal'; A ceramic motor driven in-vacuum sine-bar mechanism for the double crystal combined pitch motion. The mechanical design of the monochromator, as well as the test results of its positioning performance are presented in this paper.

Shu, D.; Narayanan, S.; Sandy, A.; Sprung, M.; Preissner, C.; Sullivan, J.; APS Engineering Support Division

2007-01-01T23:59:59.000Z

25

Set-up of an XAFS beamline for measurements between 2.4-8 keV at DORIS III  

SciTech Connect

In this paper results from the commissioning phase and from first user experiments of a new EXAFS beamline at the DORIS III storage ring are presented. The bending magnet EXAFS beamline A1 underwent a complete rebuild and now covers the energy range 2.4-8 keV. A Ni-coated toroidal mirror, placed in a 2:1 focusing position and a plane mirror with one Ni coated stripe and one uncoated (SiO{sub 2}) stripe are used for effective higher harmonics suppression and focusing. The UHV-compatible fixed-exit Double Crystal Monochromator (DCM) is equipped with two Si(111) crystal pairs. The second crystal of one of the two crystal pairs is tilted by 90 deg. around the surface normal to shift the position of glitches. It allows Bragg angles between 5 deg. and 55.5 deg. and continuous scans in quick-EXAFS mode. Test measurements during the commissioning phase proved the excellent performance of the monochromator and a high quality of the XAFS spectra over the entire working range.

Welter, Edmund [Deutsches Elektronen-Synchrotron A Research Centre of the Helmholtz Association, Notkestrasse 85, D-22607 Hamburg (Germany)

2010-06-23T23:59:59.000Z

26

High-energy-resolution monochromator for aberration-corrected scanning transmission electron microscopy/electron energy-loss spectroscopy  

Science Journals Connector (OSTI)

...equal to the beam current per unit area per unit solid angle per unit energy interval, CFE electron sources with their...Monochromated, spatially resolved electron energy-loss spectroscopic measurements of gold nanoparticles in the plasmon range...

2009-01-01T23:59:59.000Z

27

Design and characterization of an UHV compatible artificial channel cut monochromator.  

SciTech Connect

We present design and characterization results of a novel ultra-high-vacuum-compatible artificial channel-cut monochromator that has been installed at the undulator beamline 8-ID-I at the Advanced Photon Source. The monochromator has been designed to meet the challenging stability and optical requirements of the x-ray photon correlation spectroscopy program hosted at this beamline. In particular, the device incorporates a novel in-vacuum sine-bar drive mechanism for the combined pitch motion of the two crystals and a flexure-based high-stiffness weak-link mechanism for fine tuning the pitch and roll of the second crystal relative to the first crystal.

Narayanan, S.; Shu, D.; Sandy, A.; Sprung, M.; Preissner, C.; Sullivan, J.; X-Ray Science Division

2006-01-01T23:59:59.000Z

28

Adaptation of UVSOR-Type Plane-Grating Monochromator in Saga  

SciTech Connect

The plane grating monochromator (PGM) is one of the most useful monochromators in the world. The design concept of the PGM originates from the characteristics of synchrotron radiation itself, namely parallel rays and small source size. Since the performance of the PGM depends on the beam emittance of the storage ring, it is expected that even the used PGM may be utilized in recent facility. Therefore, the UVSOR-type PGM that had been used for more than twenty years in UVSOR was adapted to the university's branch beamline in Saga-LS with several modifications. The performance tests were carried out with a photoelectron spectrometer, and the observed values were compared with the ray-tracing calculation. The results show that the adaptation of the UVSOR-type PGM is good enough to study new functional materials.

Sugiyama, H.; Takahashi, K.; Ogawa, K.; Azuma, J.; Kamada, M. [Synchrotron Light Application Center, Saga University, Saga 840-8502 (Japan)

2010-06-23T23:59:59.000Z

29

ANL/APS/TB-24 Diamond Monochromators for APS Undulator-A Beamlines  

NLE Websites -- All DOE Office Websites (Extended Search)

4 4 Diamond Monochromators for APS Undulator-A Beamlines R.C. Blasdell, L. A. Assoufid, and D. M. Mills TABLE OF CONTENTS 1. INTRODUCTION .................................................................................1 2. PHYSICAL PROPERTIES OF DIAMONDS ..................................................5 2.1 Varieties of Diamonds ....................................................................5 2.2 The Lattice Parameter .....................................................................5 2.3 Bulk Thermal and Mechanical Properties ...............................................6 2.4 Typical Surface and Lattice Plane Morphology ......................................8 2.5 The Liquid-GaIn/Diamond Interface ...................................................10 3. DIFFRACTION PROPERTIES OF DIAMOND

30

Improvement in Stability of SPring-8 Standard X-Ray Monochromators with Water-Cooled Crystals  

SciTech Connect

SPring-8 standard double-crystal monochromators containing water-cooled crystals were stabilized to a sufficient level to function as a part of optics components to supply stable microfocused x-ray beams, by determining causes of the instability and then removing them. The instability was caused by two factors--thermal deformation of fine stepper stages in the monochromator, which resulted in reduction in beam intensity with time, and vibrations of coolant supply units and vacuum pumps, which resulted in fluctuation in beam intensity. We remodeled the crystal holders to maintain the stage temperatures constant with water, attached x-ray and electron shields to the stages in order to prevent their warming up, introduced accumulators in the water circuits to absorb pressure pulsation, used polyurethane tubes to stabilize water flow, and placed rubber cushions under scroll vacuum pumps. As a result, the intensity reduction rate of the beam decreased from 26% to 1% per hour and the intensity fluctuation from 13% to 1%. The monochromators were also modified to prevent radiation damage to the crystals, materials used as a water seal, and motor cables.

Yamazaki, Hiroshi; Shimizu, Nobtaka; Kumasaka, Takashi; Koganezawa, Tomoyuki; Sato, Masugu; Hirosawa, Ichiro; Senba, Yasunori; Ohashi, Haruhiko; Goto, Shunji [Japan Synchrotron Radiation Research Institute (JASRI), 1-1-1, Kouto, Sayo-cho, Hyogo 679-5198 (Japan); Shimizu, Yasuhiro; Miura, Takanori; Tanaka, Masayuki; Kishimoto, Hikaru; Matsuzaki, Yasuhisa [Japan Synchrotron Radiation Research Institute (JASRI), 1-1-1, Kouto, Sayo-cho, Hyogo 679-5198 (Japan); SPring-8 Service Co., Ltd., 2-23-1, Kouto, Kamigori-cho, Ako-gun, Hyogo 678-1205 (Japan); Kawano, Yoshiaki; Yamamoto, Masaki; Ishikawa, Tetsuya [RIKEN SPring-8 Center, 1-1-1, Kouto, Sayo-cho, Hyogo 679-5148 (Japan)

2010-06-23T23:59:59.000Z

31

On the 17-keV neutrino  

SciTech Connect

A brief review on the status of the 17-keV neutrino is presented. Several different experiments found spectral distortions which were consistently interpreted as evidence for a heavy neutrino admixture in {beta} decay. Recent experiments, however, rule out the existence of a 17-keV neutrino as well as escaping criticisms of earlier null results. Moreover, the majority of positive results have been reinterpreted in terms of instrumental effects, despite the need for a different explanation in each case. Anomalies persist in the low energy region of the tritium spectrum which deserve further investigation.

Hime, A.

1993-04-01T23:59:59.000Z

32

On the 17-keV neutrino  

SciTech Connect

A brief review on the status of the 17-keV neutrino is presented. Several different experiments found spectral distortions which were consistently interpreted as evidence for a heavy neutrino admixture in [beta] decay. Recent experiments, however, rule out the existence of a 17-keV neutrino as well as escaping criticisms of earlier null results. Moreover, the majority of positive results have been reinterpreted in terms of instrumental effects, despite the need for a different explanation in each case. Anomalies persist in the low energy region of the tritium spectrum which deserve further investigation.

Hime, A.

1993-04-01T23:59:59.000Z

33

Time-delay compensated monochromator for the spectral selection of extreme-ultraviolet high-order laser harmonics  

SciTech Connect

The design and the characterization of a monochromator for the spectral selection of ultrashort high-order laser harmonics in the extreme ultraviolet are presented. The instrument adopts the double-grating configuration to preserve the length of the optical paths of different diffracted rays, without altering the extremely short duration of the pulse. The gratings are used in the off-plane mount to have high efficiency. The performances of the monochromator have been characterized in terms of spectral response, efficiency, photon flux, imaging properties, and temporal response. In particular, the temporal characterization of the harmonic pulses has been obtained using a cross-correlation method: Pulses as short as 8 fs have been measured at the output of the monochromators, confirming the effectiveness of the time-delay compensated configuration.

Poletto, Luca; Villoresi, Paolo; Frassetto, Fabio [Laboratory for UV and X-Ray Optical Research, CNR-INFM and Department of Information Engineering, University of Padova, Padova 35131 (Italy); Calegari, Francesca; Ferrari, Federico; Lucchini, Matteo; Sansone, Giuseppe; Nisoli, Mauro [National Laboratory for Ultrafast and Ultraintense Optical Science, CNR-INFM and Department of Physics, Politecnico di Milano, Milano 20133 (Italy)

2009-12-15T23:59:59.000Z

34

Periodic magnetic field as a polarized and focusing thermal neutron spectrometer and monochromator  

SciTech Connect

A novel periodic magnetic field (PMF) optic is shown to act as a prism, lens, and polarizer for neutrons and particles with a magnetic dipole moment. The PMF has a two-dimensional field in the axial direction of neutron propagation. The PMF alternating magnetic field polarity provides strong gradients that cause separation of neutrons by wavelength axially and by spin state transversely. The spin-up neutrons exit the PMF with their magnetic spins aligned parallel to the PMF magnetic field, and are deflected upward and line focus at a fixed vertical height, proportional to the PMF period, at a downstream focal distance that increases with neutron energy. The PMF has no attenuation by absorption or scatter, as with material prisms or crystal monochromators. Embodiments of the PMF include neutron spectrometer or monochromator, and applications include neutron small angle scattering, crystallography, residual stress analysis, cross section measurements, and reflectometry. Presented are theory, experimental results, computer simulation, applications of the PMF, and comparison of its performance to Stern-Gerlach gradient devices and compound material and magnetic refractive prisms.

Cremer, J. T.; Williams, D. L.; Fuller, M. J.; Gary, C. K.; Piestrup, M. A. [Adelphi Technology, Inc., 2003 East Bayshore Rd., Redwood City, California 94063 (United States); Pantell, R. H.; Feinstein, J. [Department of Electrical Engineering, Stanford University, Stanford, California 94305 (United States); Flocchini, R. G.; Boussoufi, M.; Egbert, H. P.; Kloh, M. D.; Walker, R. B. [Davis McClellan Nuclear Radiation Center, University of California, McClellan, California 95652 (United States)

2010-01-15T23:59:59.000Z

35

Data:07657709-0dbd-4f7d-9ba5-16de8191e070 | Open Energy Information  

Open Energy Info (EERE)

d-9ba5-16de8191e070 No revision has been approved for this page. It is currently under review by our subject matter experts. Jump to: navigation, search Loading... 1. Basic...

36

Hybrid diamond-silicon angular-dispersive x-ray monochromator with 0.25-meV energy bandwidth and high spectral efficiency  

Science Journals Connector (OSTI)

We report on the design, implementation, and performance of an x-ray monochromator with ultra-high energy resolution (?E/E ? 2.7 10?8) and...

Stoupin, S; Shvydko, Y V; Shu, D; Blank, V D; Terentyev, S A; Polyakov, S N; Kuznetsov, M S; Lemesh, I; Mundboth, K; Collins, S P; Sutter, J P; Tolkiehn, M

2013-01-01T23:59:59.000Z

37

Lifetime of 981-Kev State in Li-8  

E-Print Network (OSTI)

PHYSICAL REVIEW C VOLUME 3, NUMBER 2 FEBRUARY 1971 Lifetime of the 981-keV State in Li ~ M. J. Throop* University of Iosoa, Iozea City, Ious 52240 and D. H. Youngblood Texas A. @M University, College Station, Texas 77843 and G. C. Morrison...- tify contaminant peaks, spectra were obtained for C and 0 targets at a Liv energy of 7.4 MeV. In Fig. 2, the peaks from the Li7+ C reaction are those at 871 keV (from the 0.871 0.0-MeV trans- ition in 0") and at 960 keV (the double-escape peak from...

Throop, M. J.; Youngblood, David H.; Morrison, G. C.

1971-01-01T23:59:59.000Z

38

High-heat-load synchrotron tests of room-temperature, silicon crystal monochromators at the CHESS F-2 wiggler station  

SciTech Connect

This note summarizes the results of the single crystal monochromator high-heat-load tests performed at the CHESS F-2 wiggler station. The results from two different cooling geometries are presented: (1) the ``pin-post`` crystal and (2) the ``criss-cross`` crystal. The data presented were taken in August 1993 (water-cooled pin-post) and in April 1995 (water- and gallium-cooled pin-post crystal and gallium-cooled criss-cross crystal). The motivation for trying these cooling (or heat exchanger) geometries is to improve the heat transfer efficiency over that of the conventional slotted crystals. Calculations suggest that the pin-post or the microchannel design can significantly improve the thermal performance of the crystal. The pin-post crystal used here was fabricated by Rocketdyne Albuquerque Operations. From the performance of the conventional slotted crystals, it was thought that increased turbulence in the flow pattern may also enhance the heat transfer. The criss-cross crystal was a simple attempt to achieve the increased flow turbulence. The criss-cross crystal was partly fabricated in-house (cutting, etching and polishing) and bonded by RAO. Finally, a performance comparison among all the different room temperature silicon monochromators that have been tested by the APS is presented. The data includes measurements with the slotted crystal and the core-drilled crystals. Altogether, the data presented here were taken at the CHESS F-2 wiggler station between 1991 and 1995.

Lee, W.K.; Fernandez, P.B.; Graber, T.; Assoufid, L.

1995-09-08T23:59:59.000Z

39

Compact, maintainable 80-KeV neutral beam module  

DOE Patents (OSTI)

A compact, maintainable 80-keV arc chamber, extractor module for a neutral beam system immersed in a vacuum of <10.sup.-2 Torr, incorporating a nested 60-keV gradient shield located midway between the high voltage ion source and surrounding grounded frame. The shield reduces breakdown or arcing path length without increasing the voltage gradient, tends to keep electric fields normal to conducting surfaces rather than skewed and reduces the peak electric field around irregularities on the 80-keV electrodes. The arc chamber or ion source is mounted separately from the extractor or ion accelerator to reduce misalignment of the accelerator and to permit separate maintenance to be performed on these systems. The separate mounting of the ion source provides for maintaining same without removing the ion accelerator.

Fink, Joel H. (Livermore, CA); Molvik, Arthur W. (Livermore, CA)

1980-01-01T23:59:59.000Z

40

Relic keV sterile neutrinos and reionization  

E-Print Network (OSTI)

A sterile neutrino with mass of several keV can account for cosmological dark matter, as well as explain the observed velocities of pulsars. We show that X-rays produced by the decays of these relic sterile neutrinos can boost the production of molecular hydrogen, which can speed up the cooling of gas and the early star formation, which can, in turn, lead to a reionization of the universe at a high enough redshift to be consistent with the WMAP results.

Peter L. Biermann; Alexander Kusenko

2005-12-31T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Experimental results with cryogenically cooled, thin, silicon crystal x-ray monochromators on high-heat-flux beamlines  

SciTech Connect

A novel, silicon crystal monochromator has been designed and tested for use on undulator and focused wiggler beamlines at third-generation synchrotron sources. The crystal utilizes a thin, partially transmitting diffracting element fabricated within a liquid-nitrogen cooled, monolithic block of silicon. This report summarizes the results from performance tests conducted at the European Synchrotron Radiation Facility (ESRF) using a focused wiggler beam and at the Advanced Photon Source (APS) on an undulator beamline. These experiments indicate that a cryogenic crystal can handle the very high power and power density x-ray beams of modem synchrotrons with sub-arcsec thermal broadening of the rocking curve. The peak power density absorbed on the surface of the crystal at the ESRF exceeded go W/mm{sup 2} with an absorbed power of 166 W, this takes into account the spreading of the beam due to the Bragg angle of 11.4{degrees}. At the APS, the peak heat flux incident on the crystal was 1.5 W/mA/mm{sup 2} with a power of 6.1 W/mA for a 2.0 H x 2.5 V mm{sup 2} beam at an undulator gap of 11.1 mm and stored current up to 96 mA.

Rogers, C.S.; Mills, D.M.; Lee, W.K.; Fernandez, P.B.; Graber, T.

1996-08-01T23:59:59.000Z

42

Linac4 45 keV Proton Beam Measurements  

E-Print Network (OSTI)

Linac4 is a 160 MeV normal-conducting H- linear accelerator, which will replace the 50 MeV proton Linac2 as injector for the CERN proton complex. Commissioning of the low energy part - comprising the H - source, a 45 keV Low Energy Beam Transport line (LEBT), a 3 MeV Radiofrequency Quadrupole (RFQ) and a Medium Energy Beam Transport (MEBT) - will start in fall 2012 on a dedicated test stand installation. In preparation to this, preliminary measurements were taken using a 45 keV proton source and a temporary LEBT setup, with the aim of characterising the output beam by comparison with the predictions of simulations. At the same time this allowed a first verification of the functionalities of diagnostics instrumentation and acquisition software tools. Measurements of beam profile, emittance and intensity were taken in three different setups: right after the source, after the first and after the second LEBT solenoids respectively. Particle distributions were reconstructed from emittance scan...

Bellodi, G; Hein, L M; Lallement, J-B; Lombardi, A M; Midttun, O; Scrivens, R; Posocco, P A

2013-01-01T23:59:59.000Z

43

Hydrogen-Atom Excitation and Ionization by Proton Impact in 50-Kev to 200-Kev Energy Region  

E-Print Network (OSTI)

.1475 0.1291 0.0959 0.2654 0.2445 0.2092 0.1555 0.1048 0,0452 0.0452 0.0349 0.0197 0.0088 0.0248 0.0216 0.0168 0.0110 0.0063 I ' I ' I I I I 3.0? ~ PAGPM FSHB ~ GI I i I 20 60 I i I i I ) 100 140 180 E (kev) I 220 FIG. 3....1475 0.1291 0.0959 0.2654 0.2445 0.2092 0.1555 0.1048 0,0452 0.0452 0.0349 0.0197 0.0088 0.0248 0.0216 0.0168 0.0110 0.0063 I ' I ' I I I I 3.0? ~ PAGPM FSHB ~ GI I i I 20 60 I i I i I ) 100 140 180 E (kev) I 220 FIG. 3...

Fitchard, E.; Ford, A. Lewis; Reading, John F.

1977-01-01T23:59:59.000Z

44

High resolution 17 keV to 75 keV backlighters for High Energy Density experiments  

SciTech Connect

We have developed 17 keV to 75 keV 1-dimensional and 2-dimensional high-resolution (< 10 {micro}m) radiography using high-intensity short pulse lasers. High energy K-{alpha} sources are created by fluorescence from hot electrons interacting in the target material after irradiation by lasers with intensity I{sub L} > 10{sup 17} W/cm{sup 2}. We have achieved high resolution point projection 1-dimensional and 2-dimensional radiography using micro-foil and micro-wire targets attached to low-Z substrate materials. The micro-wire size was 10 {micro}m x 10 {micro}m x 300 {micro}m on a 300 {micro}m x 300 {micro}m x 5 {micro}m CH substrate. The radiography performance was demonstrated using the Titan laser at LLNL. We observed that the resolution is dominated by the micro-wire target size and there is very little degradation from the plasma plume, implying that the high energy x-ray photons are generated mostly within the micro-wire volume. We also observe that there are enough K{alpha} photons created with a 300 J, 1-{omega}, 40 ps pulse laser from these small volume targets, and that the signal-to-noise ratio is sufficiently high, for single shot radiography experiments. This unique technique will be used on future high energy density (HED) experiments at the new Omega-EP, ZR and NIF facilities.

Park, H; Maddox, B R; Giraldez, E; Hatchett, S P; Hudson, L; Izumi, N; Key, M H; Pape, S L; MacKinnon, A J; MacPhee, A G; Patel, P K; Phillips, T W; Remington, B A; Seely, J F; Tommasini, R; Town, R; Workman, J

2008-02-25T23:59:59.000Z

45

Inelastic Scattering of 20-kev Electrons in Metal Vapors  

Science Journals Connector (OSTI)

The low-energy losses of 20-kev electrons passing through the vapors of Zn, Cd, Hg, Na, K, Mg, Ca, Sb, Pb, and KCl, have been measured by using an electrostatic analyzer previously used for measuring electron energy losses in thin metal films. The atomic transitions corresponding to the measured energy losses are in many cases fairly easily established. However, there remain some which are questionable due to the fact that there is more than one feasible transition with energy differences of the order of the given energy loss. It is established that the principal interaction results in the excitation from the ground state of the neutral atom to the first excited levelthe resonance excitation. It is also found that dipole excitations predominate

Lewis B. Leder

1957-09-15T23:59:59.000Z

46

Commissioning of a Soft X-ray Beamline PF-BL-16A with a Variable-Included-Angle Varied-Line-Spacing Grating Monochromator  

SciTech Connect

The design and commissioning of a new soft X-ray beamline, BL-16A, at the Photon Factory is presented. The beamline consists of a pre-focusing mirror, an entrance slit, a variable-included-angle varied-line-spacing plane grating monochromator, and a post-focusing system as usual, and provides circularly and linearly polarized soft X rays in the energy range 200-1500 eV with an APPLE-II type undulator. The commissioning procedure for the beamline optics is described in detail, especially the check of the focal position for the zero-th order and diffracted X rays.

Amemiya, Kenta; Toyoshima, Akio; Kikuchi, Takashi; Kosuge, Takashi; Nigorikawa, Kazuyuki; Sumii, Ryohei; Ito, Kenji [Institute of Materials Structure Science, High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki 305-0801 (Japan)

2010-06-23T23:59:59.000Z

47

Plural Scattering of 20-kev Electrons in Aluminum  

Science Journals Connector (OSTI)

The angular and energy distribution of 20-kev electrons, scattered at very small angles (<10-2 rad) by transmission through aluminum foils, are compared with the theory of plural inelastic scattering, under the following assumptions: (a) The probability of elastic scattering at very small angles is negligibly small in comparison with the probability of inelastic scattering. (b) Inelastic scattering occurs predominantly through sharply defined "characteristic" energy losses, whose number follows a Poisson statistical distribution. (c) The angular distribution in each loss follows a simple law: ?(?)?(?E2+?2)-1. (d) The cumulative angular distribution from plural inelastic scattering is obtained by repeated "folding" of ?(?) with the angular spread of the incident beam. The angular distribution of zero-loss electrons is found to be substantially independent of the foil thickness; the normalized angular distributions of the first- and second-loss peaks are accurately fitted by the "folding" calculation; Poisson statistics gives a good approximation to the observed numbers of energy losses. The value of ? for five observations on foils of thicknesses 650-2580 A is approximately 810 A, independent of thickness; systematic errors in the method of observation may render this value up to 20% higher than the mean free path corresponding to the total cross section.

L. Marton; J. Arol Simpson; H. A. Fowler; N. Swanson

1962-04-01T23:59:59.000Z

48

Origin of The 871-keV Gamma Ray and the "Oxide" Attribute  

SciTech Connect

This brief paper concludes our study of the origin of the 871-keV observed for many plutonium oxide samples.

Peurrung, Anthony J.; Arthur, Richard J.; Geelhood, Bruce D.; Scheele, Randall D.; Elovich, Robert J.; Pratt, Sharon L.

2000-03-22T23:59:59.000Z

49

Sagittal focusing Laue monochromator  

SciTech Connect

An x-ray focusing device generally includes a slide pivotable about a pivot point defined at a forward end thereof, a rail unit fixed with respect to the pivotable slide, a forward crystal for focusing x-rays disposed at the forward end of the pivotable slide and a rearward crystal for focusing x-rays movably coupled to the pivotable slide and the fixed rail unit at a distance rearward from the forward crystal. The forward and rearward crystals define reciprocal angles of incidence with respect to the pivot point, wherein pivoting of the slide about the pivot point changes the incidence angles of the forward and rearward crystals while simultaneously changing the distance between the forward and rearward crystals.

Zhong; Zhong (Stony Brook, NY), Hanson; Jonathan (Wading River, NY), Hastings; Jerome (Stanford, CA), Kao; Chi-Chang (Setauket, NY), Lenhard; Anthony (Medford, NY), Siddons; David Peter (Cutchogue, NY), Zhong; Hui (Coram, NY)

2009-03-24T23:59:59.000Z

50

Multipole mixtures of gamma-ray transitions depopulating the 1318-keV (2-) and 1518-keV (6+ or 7-) states in Yb174  

Science Journals Connector (OSTI)

An E1+E3 (?1.9%M2) multipole mixture has been observed for the 1242-keV (2- ? 2+) transition depopulating the J?, K=2-,2 octupole vibrational level at 1318 keV in Yb174 following the decay of Lu174 and Lum174. The internal-conversion cfficient for this transition and the ?-? directional correlation for the 1242-76.5-keV cascade have been remeasured, and the results yield the unique set of multipole mixing ratios ?1(M2E1)=0.050.09 and ?2(E3E1)=0.190.08 which correspond to a multipole admixture of E1(96.3-2.6+1.7%)+M2(0.2-0.2+1.7%)+E3(3.5-2.1+3.8%). The M2 multipolarity of the 1318-keV (2- ? 0+) transition was also verified from the measured internal-conversion coefficient. A multipole admixture of E3 (<27%M2) for the 1065-keV transition was deduced from available data, and the ratios of reduced transition probabilities for the transitions depopulating the 1318-keV level were calculated and compared with rotational-model predictions. Using the previously measured half-life of the 2- level, absolute transition probabilities and hindrance factors were obtained for these transitions, and B(E3) values were compared with theoretical microscopic model calculations. Partial correlation coefficients for the 992-keV transition depopulating the 1518-keV isomeric state were determined using the ?-? directional correlation data. Multipole admixtures consistent with the correlation data (and internal conversion data for the 7- case) are E2+(278%)M1 for the choice of 6+ and E1(687%)+M2(52%)+E3(277%) for the choice of 7- for the 1518-keV level. Using the reported half-life for that level, the hindrance factors were obtained for the K-forbidden transitions depopulating the level for each choice of spin assignment and these are compared with hindrance factors observed for known K-forbidden transitions.[RADIOACTIVITY Lu174 [from Yb174(d,2n)] measured I?, ??(?), I(ce); deduced J, ?, ICC, ? mixing, B(E3).

A. G. Schmidt; J. W. Mihelich; E. G. Funk

1974-06-01T23:59:59.000Z

51

Performance and application of a double-crystal monochromator in the energy region 800 less than or equal to h. nu. less than or equal to 4500 eV  

SciTech Connect

The performance and application of an ultra-high-vacuum compatible constant-deviation double-crystal monochromator (JUMBO) in operation at SSRL is demonstrated. The monochromator can be operated with any of four pairs of crystals interchangeable in situ. An electronic-maximum-search feedback loop optimizes the intensity of the spatially fixed outgoing beam as the photon energy is scanned. The monochromatic beam is focussed (approx. 1.5 mm x 5 mm) onto the sample by a toroidal mirror. Monochromator crystals of beryl(10 anti 10), InSb(111) and Ge(111) have been tested in the energy regions 800 to 1540 eV, 1690 to 4000 eV and 1930 to 4500 eV, respectively. The performance of these crystals with regard to the resolution, the intensity, the level of scattered light, and the contribution of higher orders have been determined. Various effects arising from a radiation-induced temperature gradient in the monochromator crystals are discussed.

Hussain, Z.; Umbach, E.; Shirley, D.A.; Stoehr, V.; Feldhaus, J.

1981-07-01T23:59:59.000Z

52

Measurement of the differential neutron-deuteron scattering cross section in the energy range from 100 keV to 600 keV using a proportional counter  

E-Print Network (OSTI)

The angular distribution of neutron-deuteron scattering was investigated using the proportional counter P2 simultaneously as scattering target and detector for the recoil deuterons. The measurements were carried out using monoenergetic neutrons in the energy range from 150 keV to 500 keV. Various techniques were employed to reduce distortions of the experimental pulse-height distribution by photon-induced events. The experimental data were compared with realistic simulations which were carried out using different evaluated data sets. This comparison allows to conclude on inconsistencies in the evaluations.

Nolte, R; Plompen, A; Rttger, S

2014-01-01T23:59:59.000Z

53

Wireless Hacking Tools http://www.cse.wustl.edu/~jain/cse571-07/ftp/wireless_hacking/ 1 of 12 12/19/2007 5:16 PM  

E-Print Network (OSTI)

Wireless Hacking Tools http://www.cse.wustl.edu/~jain/cse571-07/ftp/wireless_hacking/ 1 of 12 12/19/2007 5:16 PM Wireless Hacking Tools Author: Michael Roche mroche@wustl.edu Abstract: This paper or application. #12;Wireless Hacking Tools http://www.cse.wustl.edu/~jain/cse571-07/ftp/wireless_hacking/ 2 of 12

Jain, Raj

54

Origin of the 871-keV gamma ray and the ``oxide'' attribute  

SciTech Connect

This work concludes the investigation of the oxide attribute of current interest for the characterization of stored plutonium. Originally it was believed that the presence of oxide could be ascertained by measurement of the 871-keV line in a high-resolution gamma-ray spectrum. However, recent work has suggested that the 871-keV gamma ray in plutonium oxide arises from the reaction {sup 14}N({alpha},p){sup 17}O rather than the inelastic scattering reaction {sup 17}O({alpha},{alpha}{prime}){sup 17}O*. This conclusion, though initially surprising, was obtained during efforts to determine the relative importance of americium and plutonium alpha-particle decay for the production of the 871-keV gamma ray. Several questions were raised by previous experiments: What role, if any does {sup 17}O have in the generation of the 871-keV gamma ray? How does sufficient nitrogen come to be present in plutonium oxide? Under what conditions is the 871-keV gamma ray measurable in plutonium oxide? This paper describes the answers to these questions.

AJ Peurrung; RJ Arthur; BD Geelhood; RD Scheele; RJ Elovich; SL Pratt

2000-03-22T23:59:59.000Z

55

Ion and photon emission from keV cluster impacts on surfaces  

E-Print Network (OSTI)

molecular SF6tx- (8 keV) tuojectiles than for the same energy monoatomic Cs+ beam. Monoatomic Cs+ was used for comparison because Cs atomic weight is close to the molecular weight of SF6 - 133 amu for Cs+ and 146 amu for SF6. The difference in projectile... molecular SF6tx- (8 keV) tuojectiles than for the same energy monoatomic Cs+ beam. Monoatomic Cs+ was used for comparison because Cs atomic weight is close to the molecular weight of SF6 - 133 amu for Cs+ and 146 amu for SF6. The difference in projectile...

Yau, Alice Yau-Lic

2012-06-07T23:59:59.000Z

56

A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line  

E-Print Network (OSTI)

Galaxy clusters can efficiently convert axion-like particles (ALPs) to photons. We propose that the recently claimed detection of a 3.55--3.57 keV line in the stacked spectra of a large number of galaxy clusters and the Andromeda galaxy may originate from the decay of either a scalar or fermionic $7.1$ keV dark matter species into an axion-like particle (ALP) of mass $m_{a} \\lesssim 6\\cdot 10^{-11}~{\\rm eV}$, which subsequently converts to a photon in the cluster magnetic field. In contrast to models in which the photon line arises directly from dark matter decay or annihilation, this can explain the anomalous line strength in the Perseus cluster. As axion-photon conversion scales as $B^2$ and cool core clusters have high central magnetic fields, this model can also explains the observed peaking of the line emission in the cool cores of the Perseus, Ophiuchus and Centaurus clusters, as opposed to the much larger dark matter halos. We describe distinctive predictions of this scenario for future observations.

Michele Cicoli; Joseph P. Conlon; M. C. David Marsh; Markus Rummel

2014-03-10T23:59:59.000Z

57

Study of photon attenuation coefficients of some multielement materials. [123-1250 keV  

SciTech Connect

Total photon mass attenuation of six multielement shielding materials (concrete, plaster of paris, quick lime, black cement, white cement, and silica) is measured in the 123- to 1,250-keV energy range. The experimental results are analyzed in terms of cross sections, effective atomic numbers, and electron densities. Considerable sensitivity of the total mass attenuation coefficients and effective atomic numbers to variations in oxygen content are found in these multielement materials.

Bhandal, G.S. (N.J.S.A. Government Coll., Punjab (India)); Singh, K. (Guru Nanak Dev Univ., Amritsar (India). Dept. of Physics)

1994-03-01T23:59:59.000Z

58

HELIOSPHERIC NEUTRAL ATOM SPECTRA BETWEEN 0.01 AND 6 keV FROM IBEX  

SciTech Connect

Since 2008 December, the Interstellar Boundary Explorer (IBEX) has been making detailed observations of neutrals from the boundaries of the heliosphere using two neutral atom cameras with overlapping energy ranges. The unexpected, yet defining feature discovered by IBEX is a Ribbon that extends over the energy range from about 0.2 to 6 keV. This Ribbon is superposed on a more uniform, globally distributed heliospheric neutral population. With some important exceptions, the focus of early IBEX studies has been on neutral atoms with energies greater than {approx}0.5 keV. With nearly three years of science observations, enough low-energy neutral atom measurements have been accumulated to extend IBEX observations to energies less than {approx}0.5 keV. Using the energy overlap of the sensors to identify and remove backgrounds, energy spectra over the entire IBEX energy range are produced. However, contributions by interstellar neutrals to the energy spectrum below 0.2 keV may not be completely removed. Compared with spectra at higher energies, neutral atom spectra at lower energies do not vary much from location to location in the sky, including in the direction of the IBEX Ribbon. Neutral fluxes are used to show that low energy ions contribute approximately the same thermal pressure as higher energy ions in the heliosheath. However, contributions to the dynamic pressure are very high unless there is, for example, turbulence in the heliosheath with fluctuations of the order of 50-100 km s{sup -1}.

Fuselier, S. A.; Ghielmetti, A. G.; Petrinec, S. M.; Trattner, K. J., E-mail: sfuselier@swri.edu, E-mail: fallegrini@swri.edu [Lockheed Martin Advanced Technology Center, Palo Alto, CA 94304 (United States); and others

2012-07-20T23:59:59.000Z

59

Total Neutron Cross Section for Uranium from 20 kev to 20 Mev  

Science Journals Connector (OSTI)

The total neutron cross section of normal uranium has been measured for neutron energies from 20 kev to 7.6 Mev and at 17, 19, and 20 Mev. When combined with other published work in the 7-14 Mev range, the result is a smooth cross-section curve up to 20 Mev. The curve fits smoothly on the surface showing total neutron cross section as a function of both atomic weight and neutron energy.

R. L. Henkel; L. Cranberg; G. A. Jarvis; R. Nobles; J. E. Perry; Jr.

1954-04-01T23:59:59.000Z

60

Low Dose Radiation Research Program: 12.5 keV Xray Microbeam Bystander  

NLE Websites -- All DOE Office Websites (Extended Search)

12.5 keV Xray Microbeam Bystander Studies With Human Mammary 12.5 keV Xray Microbeam Bystander Studies With Human Mammary Epithelial Cells and Fibroblasts Authors: E. A. Blakely1, R. I. Schwarz1, A. C. Thompson2, K. A. Bjornstad1, P. Y. Chang1,3 C.J. Rosen1, and D. Sudar1 Institutions: Divisions of 1Life Sciences and 2Advanced Light Source, Lawrence Berkeley National Laboratory, Berkeley, CA. and 3SRI International, Menlo Park, CA. We are using a novel x-ray Microprobe Beamline at the Advanced Light Source (ALS) at LBNL to investigate bystander effects of low doses in well characterized human mammary epithelial cells (HMEC) and human skin fibroblasts (HSF). The ALS facility is capable of producing a beam of 12.5 keV x-rays with a focussed spot size of __m_ and a wide range of doses and dose-rates. Unlike normal x-ray sources, this beam has a very small background of either low-

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Effective field theory and keV lines from dark matter  

E-Print Network (OSTI)

We survey operators that can lead to a keV photon line from dark matter decay or annihilation. We are motivated in part by recent claims of an unexplained 3.5 keV line in galaxy clusters and in Andromeda, but our results could apply to any hypothetical line observed in this energy range. We find that given the amount of flux that is observable, explanations in terms of decay are more plausible than annihilation, at least if the annihilation is directly to Standard Model states rather than intermediate particles. The decay case can be explained by a scalar or pseudoscalar field coupling to photons suppressed by a scale not far below the reduced Planck mass, which can be taken as a tantalizing hint of high-scale physics. The scalar case is particularly interesting from the effective field theory viewpoint, and we discuss it at some length. Because of a quartically divergent mass correction, naturalness strongly suggests the theory should be cut off at or below the 1000 TeV scale. The most plausible such natural UV completion would involve supersymmetry. These bottom-up arguments reproduce expectations from top-down considerations of the physics of moduli. A keV line could also arise from the decay of a sterile neutrino, in which case a renormalizable UV completion exists and no direct inference about high-scale physics is possible.

Rebecca Krall; Matthew Reece; Thomas Roxlo

2014-03-05T23:59:59.000Z

62

Microprocessorbased monochromator controller  

E-Print Network (OSTI)

I-- _z 5o- > :5- % IOO a) 75 ooooO eeeeeeee 65 6 .7 .8 o ee Ooooooo eeeeeeeee 9 656.0 .2 3 .4 .5 .6, (NM) >- 50 > 25 00 b) 0 e lil e e 655.8 .9 656.0 .I .2 .3 .4 .5 .6 (NM) Figure 4. Bidirectional scans of deuterium lamp emission line at 656.1 nm (e..., University of Illinois, Urbana, Illinois, USA, 1977. [3] Intel Corporation "MCS-85 USERS Manual," Santa Clara, California, USA, 1978. [4] Larsen D.G., Rony, P.R., Titus, J.A., and Titus, C.A.,Arnerican Laboratory, 1978, 10 (9), 88. [5] Ref. 3, p. A1 32. [6...

Dalle-Molle, Richard; Defreese, James D.

1980-04-01T23:59:59.000Z

63

Stopping Cross Sections of Some Hydrocarbon Gases for 40-200-keV Helium Ions  

Science Journals Connector (OSTI)

The stopping cross sections of air, CH4, C2H2, C2H4, C3H8, (CH2)3, and C3H6 have been measured for incident helium ions in the energy range 40 to 200 keV. The data are in good agreement with previous experiment work, and have standard deviations between 2 and 6%. They obey an energy dependence ?=?E12 in accord with the calculation of Lindhard and Scharff. It has been shown that while there is probably an effect due to chemical binding on the helium-ion stopping cross sections of hydrocarbons, this effect is small.

John T. Park

1965-05-31T23:59:59.000Z

64

Partial widths and gamma-ray decay of the 2883- and 5037-keV levels in Sc41  

Science Journals Connector (OSTI)

Proton and ?-ray decay widths for the 7/2+ resonance at 2883 keV excitation in Sc41 have been deduced from measurements of ??? and the (p,?) resonance strength. Our results are ??=0.0580.007 eV and ?p=0.0900.011 eV. Angular distributions measured for the 5037(92+)?2883 keV and 2883?0(72-) keV transitions confirm the J=72 assignment for the 2883-keV level. The linear polarization was measured for the 2883?0 keV transition and confirms the positive parity assignment. In addition, the (p,?) strength for the 5037-keV level was measured, and our strength results for both resonances are lower than those of Youngblood, Wildenthal, and Class by a factor of 1.4.[NUCLEAR REACTIONS Ca40(p,?), Ep=1.84,4.05 MeV; measured ?(E?,?), Q, P(90?), resonance strengths, I?. Sc41 deduced levels, J?, ??, ?p, CSp2. Enriched target.

R. L. Kozub; B. E. Cooke; J. R. Leslie; B. C. Robertson

1977-07-01T23:59:59.000Z

65

EMISSION LINES BETWEEN 1 AND 2 keV IN COMETARY X-RAY SPECTRA  

SciTech Connect

We present the detection of new cometary X-ray emission lines in the 1.0-2.0 keV range using a sample of comets observed with the Chandra X-Ray Observatory and ACIS spectrometer. We have selected five comets from the Chandra sample with good signal-to-noise spectra. The surveyed comets are C/1999 S4 (LINEAR), C/1999 T1 (McNaught-Hartley), 153P/2002 (Ikeya-Zhang), 2P/2003 (Encke), and C/2008 8P (Tuttle). We modeled the spectra with an extended version of our solar wind charge exchange (SWCX) emission model. Above 1 keV, we find Ikeya-Zhang to have strong emission lines at 1340 and 1850 eV which we identify as being created by SWCX lines of Mg XI and Si XIII, respectively, and weaker emission lines at 1470, 1600, and 1950 eV formed by SWCX of Mg XII, Mg XI, and Si XIV, respectively. The Mg XI and XII and Si XIII and XIV lines are detected at a significant level for the other comets in our sample (LS4, MH, Encke, 8P), and these lines promise additional diagnostics to be included in SWCX models. The silicon lines in the 1700-2000 eV range are detected for all comets, but with the rising background and decreasing cometary emission, we caution that these detections need further confirmation with higher resolution instruments.

Ewing, Ian; Christian, Damian J. [Department of Physics and Astronomy, California State University, 18111 Nordhoff Street, Northridge, CA 91330 (United States)] [Department of Physics and Astronomy, California State University, 18111 Nordhoff Street, Northridge, CA 91330 (United States); Bodewits, Dennis [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States)] [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States); Dennerl, Konrad [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1312, D-85741 Garching Germany (Germany)] [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1312, D-85741 Garching Germany (Germany); Lisse, Carey M. [Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723 (United States)] [Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723 (United States); Wolk, Scott J., E-mail: ian.ewing.794@my.csun.edu, E-mail: daman.christian@csun.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2013-01-20T23:59:59.000Z

66

Effective field theory and keV lines from dark matter  

E-Print Network (OSTI)

We survey operators that can lead to a keV photon line from dark matter decay or annihilation. We are motivated in part by recent claims of an unexplained 3.5 keV line in galaxy clusters and in Andromeda, but our results could apply to any hypothetical line observed in this energy range. We find that given the amount of flux that is observable, explanations in terms of decay are more plausible than annihilation, at least if the annihilation is directly to Standard Model states rather than intermediate particles. The decay case can be explained by a scalar or pseudoscalar field coupling to photons suppressed by a scale not far below the reduced Planck mass, which can be taken as a tantalizing hint of high-scale physics. The scalar case is particularly interesting from the effective field theory viewpoint, and we discuss it at some length. Because of a quartically divergent mass correction, naturalness strongly suggests the theory should be cut off at or below the 1000 TeV scale. The most plausible such natural...

Krall, Rebecca; Roxlo, Thomas

2014-01-01T23:59:59.000Z

67

Ion Source Development For The Proposed FNAL 750 keV Injector Upgrade  

SciTech Connect

Currently there is a Proposed FNAL 750 keV Injector Upgrade for the replacement of the 40 year old Fermi National Laboratory (FNAL) Cockcroft-Walton accelerators with a new ion source and 200 MHz Radio Frequency Quadruple (RFQ). The slit type magnetron being used now will be replaced with a round aperture magnetron similar to the one used at Brookhaven National Lab (BNL). Operational experience from BNL has shown that this type of source is more reliable with a longer lifetime due to better power efficiency. The current source development effort is to produce a reliable source with >60 mA of H{sup -} beam current, 15 Hz rep-rate, 100 {mu}s pulse width, and a duty factor of 0.15%. The source will be based on the BNL design along with development done at FNAL for the High Intensity Neutrino Source (HINS).

Bollinger, D. S. [Fermi National Accelerator Laboratory, Box 500, Batavia, IL 60543 (United States)

2011-09-26T23:59:59.000Z

68

Student research with 400keV beams: {sup 13}N radioisotope production target development  

SciTech Connect

The AN400 Van de Graaff accelerator at the Minnesota State University, Mankato, Applied Nuclear Science Lab has demonstrated utility as an accessible and versatile platform for student research. Despite the limits of low energy, the research team successfully developed projects with applications to the wider radioisotope production community. A target system has been developed for producing and extracting {sup 13}N by the {sup 12}C(d,n){sup 13}N reaction below 400keV. The system is both reusable and robust, with future applications to higher energy machines producing this important radioisotope for physiological imaging studies with Positron Emission Tomography. Up to 36({+-}1)% of the {sup 13}N was extracted from the graphite matrix when 35 A current was externally applied to the graphite target while simultaneously flushing the target chamber with CO{sub 2} gas.

Fru, L. Che; Clymer, J.; Compton, N.; Cotter, J.; Dam, H.; Lesko, Z.; Pautzke, J.; Prokop, C.; Swanson, L.; Roberts, A. D. [Department of Physics and Astronomy, Minnesota State University, Trafton Science Center N141, Mankato MN 56001 (United States)

2013-04-19T23:59:59.000Z

69

Photoeffect cross sections of several rare-earth elements for 323-keV photons  

Science Journals Connector (OSTI)

Total-attenuation cross sections of the oxides of rare-earth elements such as La, Ce, Pr, Nd, Sm, Gd, Dy, Ho, and Er, and also NaNO3 and NaNO2 have been measured in a narrow-beam geometry setup at 323 keV. The total-attenuation cross section for oxygen was obtained as the difference in NaNO3 and NaNO2 cross sections. Using this, the total-attenuation cross sections of the individual lanthanides have been obtained with the aid of the mixture rule. From these, the photoeffect cross sections were derived by subtracting the scattering contribution. These values are found to agree well with Scofields theoretical data [University of California Report No. UCRL 51326, 1973 (unpublished)].

T. K. Umesh, S. J. Anasuya, J. Shylaja Kumari, Channe Gowda, K. P. Gopinathan Nair, and Ramakrishna Gowda

1992-02-01T23:59:59.000Z

70

QUIET-TIME INTERPLANETARY {approx}2-20 keV SUPERHALO ELECTRONS AT SOLAR MINIMUM  

SciTech Connect

We present a statistical survey of {approx}2-20 keV superhalo electrons in the solar wind measured by the SupraThermal Electron instrument on board the two STEREO spacecraft during quiet-time periods from 2007 March through 2009 March at solar minimum. The observed superhalo electrons have a nearly isotropic angular distribution and a power-law spectrum, f{proportional_to}v{sup -{gamma}}, with {gamma} ranging from 5 to 8.7, with nearly half between 6.5 and 7.5, and an average index of 6.69 {+-} 0.90. The observed power-law spectrum varies significantly on a spatial scale of {approx}>0.1 AU and a temporal scale of {approx}>several days. The integrated density of quiet-time superhalo electrons at 2-20 keV ranges from {approx}10{sup -8} cm{sup -3} to 10{sup -6} cm{sup -3}, about 10{sup -9}-10{sup -6} of the solar wind density, and, as well as the power-law spectrum, shows no correlation with solar wind proton density, velocity, or temperature. The density of superhalo electrons appears to show a solar-cycle variation at solar minimum, while the power-law spectral index {gamma} has no solar-cycle variation. These quiet-time superhalo electrons are present even in the absence of any solar activity-e.g., active regions, flares or microflares, type III radio bursts, etc.-suggesting that they may be accelerated by processes such as resonant wave-particle interactions in the interplanetary medium, or possibly by nonthermal processes related to the acceleration of the solar wind such as nanoflares, or by acceleration at the CIR forward shocks.

Wang, Linghua [Department of Geophysics, Peking University, 100871 Beijing (China); Lin, Robert P.; Salem, Chadi; Pulupa, Marc; Larson, Davin E.; Luhmann, Janet G. [Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450 (United States); Yoon, Peter H., E-mail: wanglhwang@gmail.com [School of Space Research, Kyung Hee University, Yongin, Gyeonggi (Korea, Republic of)

2012-07-01T23:59:59.000Z

71

Isotopic Mo Neutron Total Cross Section Measurements in the Energy Range 1 to 620 keV  

Science Journals Connector (OSTI)

Abstract A series of new total cross section measurements for the stable molybdenum isotopes of 92,94,95,96,98,100Mo covering the energy range between 1 keV and 620 keV was performed at the Gaerttner LINAC Center at Rensselaer Polytechnic Institute. New high-accuracy resonance parameters were extracted from an analysis of the data using the multilevel R-matrix Bayesian code SAMMY. In the unresolved resonance region, average resonance parameters and fits to the total cross sections were obtained using the Bayesian Hauser-Feshbach statistical model code FITACS.

R. Bahran; D. Barry; G. Leinweber; M. Rapp; R. Block; A. Daskalakis; B. McDermott; S. Piela; E. Blain; Y. Danon

2014-01-01T23:59:59.000Z

72

Plasma focus based flash hard X-ray source in the 100 keV region with reproducible spectrum  

Science Journals Connector (OSTI)

A pulsed hard X-ray source with shot to shot reproducible spectrum, based on a 4.7 kJ small-chamber Mather-type plasma focus device, is presented. The hard X-ray output spectrum was measured in a single shot basis by differential absorption on metallic plates. The measured spectra have a single dominant peak around 75 keV and a spectral bandwidth covering the 40150 keV range. A hard X-ray dose of ( 53 3 ) ?Gy per shot was measured on axis at 53 cm from the source, and found to be uniform within a half aperture angle of 6.

V. Raspa; P. Knoblauch; F. Di Lorenzo; C. Moreno

2010-01-01T23:59:59.000Z

73

On the keV sterile neutrino search in electron capture  

E-Print Network (OSTI)

A joint effort of cryogenic microcalorimetry (CM) and high-precision Penning-trap mass spectrometry (PT-MS) in investigating atomic orbital electron capture (EC) can shed light on the possible existence of heavy sterile neutrinos with masses from 0.5 to 100 keV. Sterile neutrinos are expected to perturb the shape of the atomic de-excitation spectrum measured by CM after a capture of the atomic orbital electrons by a nucleus. This effect should be observable in the ratios of the capture probabilities from different orbits. The sensitivity of the ratio values to the contribution of sterile neutrinos strongly depends on how accurately the mass difference between the parent and the daughter nuclides of EC-transitions can be measured by, e.g., PT-MS. A comparison of such probability ratios in different isotopes of a certain chemical element allows one to exclude many systematic uncertainties and thus could make feasible a determination of the contribution of sterile neutrinos on a level below 1%. Several electron capture transitions suitable for such measurements are discussed.

P. E. Filianin; K. Blaum; S. A. Eliseev; L. Gastaldo; Yu. N. Novikov; V. M. Shabaev; I. I. Tupitsyn; J. Vergados

2014-02-18T23:59:59.000Z

74

Nonabelian dark matter models for 3.5 keV X-rays  

E-Print Network (OSTI)

A recent analysis of XXM-Newton data reveals the possible presence of an X-ray line at approximately 3.55 keV, which is not readily explained by known atomic transitions. Numerous models of eV-scale decaying dark matter have been proposed to explain this signal. Here we explore models of multicomponent nonabelian dark matter with typical mass ~ 1-10 GeV (higher values being allowed in some models) and eV-scale splittings that arise naturally from the breaking of the nonabelian gauge symmetry. Kinetic mixing between the photon and the hidden sector gauge bosons can occur through a dimension-5 or 6 operator. Radiative decays of the excited states proceed through transition magnetic moments that appear at one loop. The decaying excited states can either be primordial or else produced by upscattering of the lighter dark matter states. These models are significantly constrained by direct dark matter searches or cosmic microwave background distortions, and are potentially testable in fixed target experiments that s...

Cline, James M

2014-01-01T23:59:59.000Z

75

MULTI-KEV X-RAY YIELDS FROM HIGH-Z GAS TARGETS FIELDED AT OMEGA  

SciTech Connect

The authors report on modeling of x-ray yield from gas-filled targets shot at the OMEGA laser facility. The OMEGA targets were 1.8 mm long, 1.95 mm in diameter Be cans filled with either a 50:50 Ar:Xe mixture, pure Ar, pure Kr or pure Xe at {approx} 1 atm. The OMEGA experiments heated the gas with 20 kJ of 3{omega} ({approx} 350 nm) laser energy delivered in a 1 ns square pulse. the emitted x-ray flux was monitored with the x-ray diode based DANTE instruments in the sub-keV range. Two-dimensional x-ray images (for energies 3-5 keV) of the targets were recorded with gated x-ray detectors. The x-ray spectra were recorded with the HENWAY crystal spectrometer at OMEGA. Predictions are 2D r-z cylindrical with DCA NLTE atomic physics. Models generally: (1) underpredict the Xe L-shell yields; (2) overpredict the Ar K-shell yields; (3) correctly predict the Xe thermal yields; and (4) greatly underpredict the Ar thermal yields. However, there are spreads within the data, e.g. the DMX Ar K-shell yields are correctly predicted. The predicted thermal yields show strong angular dependence.

Kane, J O; Fournier, K B; May, M J; Colvin, J D; Thomas, C A; Marrs, R E; Compton, S M; Moody, J D; Bond, E J; Davis, J F

2010-11-04T23:59:59.000Z

76

0-600 kev Gamma-Ray Spectra from Thermal Neutron Capture in the Region A=104to198  

Science Journals Connector (OSTI)

The energies and absolute intensities of prominent peaks in the 0-600 kev region of the gamma-ray spectrum following thermal neutron capture have been measured with a single NaI(Tl) scintillation spectrometer. The elements investigated were rhodium, silver, cadmium, indium, antimony, tellurium, iodine, samarium, europium, gadolinium, terbium, dysprosium, holmium, erbium, thulium, hafnium, tantalum, rhenium, iridium, platinum, and gold.

James E. Draper

1959-04-01T23:59:59.000Z

77

Development of a modular CdTe detector plane for gamma-ray burst detection below 100 keV  

E-Print Network (OSTI)

We report on the development of an innovative CdTe detector plane (DPIX) optimized for the detection and localization of gamma-ray bursts in the X-ray band (below 100 keV). DPIX is part of an R&D program funded by the French Space Agency (CNES). DPIX builds upon the heritage of the ISGRI instrument, currently operating with great success on the ESA INTEGRAL mission. DPIX is an assembly of 200 elementary modules (XRDPIX) equipped with 32 CdTe Schottky detectors (4x4 mm2, 1 mm thickness) produced by ACRORAD Co. LTD. in Japan. These detectors offer good energy response up to 100 keV. Each XRDPIX is readout by the very low noise front-end electronics chip IDeF-X, currently under development at CEA/DSM/DAPNIA. In this paper, we describe the design of XRDPIX, the main features of the IDeF-X chip, and will present preliminary results of the reading out of one CdTe Schottky detector by the IDeF-X V1.0 chip. A low-energy threshold around 2.7 keV has been measured. This is to be compared with the 12-15 keV threshol...

Ehanno, M; Barret, D; Lacombe, K; Pons, R; Rouaix, G; Gevin, O; Limousin, O; Lugiez, F; Bardoux, A; Penquer, A

2007-01-01T23:59:59.000Z

78

Development of a modular CdTe detector plane for gamma-ray burst detection below 100 keV  

E-Print Network (OSTI)

We report on the development of an innovative CdTe detector plane (DPIX) optimized for the detection and localization of gamma-ray bursts in the X-ray band (below 100 keV). DPIX is part of an R&D program funded by the French Space Agency (CNES). DPIX builds upon the heritage of the ISGRI instrument, currently operating with great success on the ESA INTEGRAL mission. DPIX is an assembly of 200 elementary modules (XRDPIX) equipped with 32 CdTe Schottky detectors (4x4 mm2, 1 mm thickness) produced by ACRORAD Co. LTD. in Japan. These detectors offer good energy response up to 100 keV. Each XRDPIX is readout by the very low noise front-end electronics chip IDeF-X, currently under development at CEA/DSM/DAPNIA. In this paper, we describe the design of XRDPIX, the main features of the IDeF-X chip, and will present preliminary results of the reading out of one CdTe Schottky detector by the IDeF-X V1.0 chip. A low-energy threshold around 2.7 keV has been measured. This is to be compared with the 12-15 keV threshold of the ISGRI-INTEGRAL and BAT-SWIFT instruments, which both use similar detector material.

M. Ehanno; C. Amoros; D. Barret; K. Lacombe; R. Pons; G. Rouaix; O. Gevin; O. Limousin; F. Lugiez; A. Bardoux; A. Penquer

2007-01-15T23:59:59.000Z

79

Observational consistency and future predictions for a 3.5 keV ALP to photon line  

E-Print Network (OSTI)

Motivated by the possibility of explaining the 3.5 keV line through dark matter decaying to axion-like particles that subsequently convert to photons, we study ALP-photon conversion for sightlines passing within 50 pc of the galactic centre. Conversion depends on the galactic centre magnetic field which is highly uncertain. For fields at low or mid-range of observational estimates (10--100 $\\mu$G), no observable signal is possible. For fields at the high range of observational estimates (a pervasive poloidal mG field over the central 150 pc) it is possible to generate sufficient signal to explain recent observations of a 3.5 keV line in the galactic centre. In this scenario, the galactic centre line signal comes predominantly from the region with $z > 20$ pc, reconciling the results from the Chandra and XMM-Newton X-ray telescopes. The dark matter to ALP to photon scenario also naturally predicts the non-observation of the 3.5 keV line in stacked galaxy spectra. We further explore predictions for the line flux in galaxies and suggest a set of galaxies that is optimised for observing the 3.5 keV line in this model.

Pedro D. Alvarez; Joseph P. Conlon; Francesca V. Day; M. C. David Marsh; Markus Rummel

2014-10-07T23:59:59.000Z

80

3.55 keV photon lines from axion to photon conversion in the Milky Way and M31  

E-Print Network (OSTI)

We further explore a scenario in which the recently observed 3.55 keV photon line arises from dark matter decay to an axion-like particle (ALP) of energy 3.55 keV, which then converts to a photon in astrophysical magnetic fields. This ALP scenario is well-motivated by the observed morphology of the 3.55 keV flux. For this scenario we study the expected flux from dark matter decay in the galactic halos of both the Milky Way and Andromeda (M31). The Milky Way magnetic field is asymmetric about the galactic centre, and so the resulting 3.55 keV flux morphology differs significantly from the case of direct dark matter decay to photons. However the Milky Way magnetic field is not large enough to generate an observable signal, even with ASTRO-H. In contrast, M31 has optimal conditions for ALP to photon conversion and the intrinsic signal from M31 becomes two orders of magnitude larger than for the Milky Way, comparable to that from clusters and consistent with observations.

Joseph P. Conlon; Francesca V. Day

2014-04-30T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

Production of a keV X-Ray Beam from Synchrotron Radiation in Relativistic Laser-Plasma Interaction  

E-Print Network (OSTI)

Production of a keV X-Ray Beam from Synchrotron Radiation in Relativistic Laser-Plasma Interaction demonstrate that a beam of x-ray radiation can be generated by simply focusing a single high- intensity laser spectral range) [6]. Laser-driven K x-ray sources [7­9] radiate subnanometer wavelength radiation

Umstadter, Donald

82

First limits on the 3-200 keV X-ray spectrum of the quiet Sun using RHESSI  

E-Print Network (OSTI)

We present the first results using the Reuven Ramaty High-Energy Solar Spectroscopic Imager, RHESSI, to observe solar X-ray emission not associated with active regions, sunspots or flares (the quiet Sun). Using a newly developed chopping technique (fan-beam modulation) during seven periods of offpointing between June 2005 to October 2006, we obtained upper limits over 3-200 keV for the quietest times when the GOES12 1-8A flux fell below $10^{-8}$ Wm$^{-2}$. These values are smaller than previous limits in the 17-120 keV range and extend them to both lower and higher energies. The limit in 3-6 keV is consistent with a coronal temperature $\\leq 6$ MK. For quiet Sun periods when the GOES12 1-8A background flux was between $10^{-8}$ Wm$^{-2}$ and $10^{-7}$ Wm$^{-2}$, the RHESSI 3-6 keV flux correlates to this as a power-law, with an index of $1.08 \\pm 0.13$. The power-law correlation for microflares has a steeper index of $1.29 \\pm 0.06$. We also discuss the possibility of observing quiet Sun X-rays due to solar axions and use the RHESSI quiet Sun limits to estimate the axion-to-photon coupling constant for two different axion emission scenarios.

Iain G. Hannah; G. J Hurford; H. S. Hudson; R. P. Lin; K. van Bibber

2007-02-27T23:59:59.000Z

83

The INTEGRAL/SPI 511 keV Signal from Hidden Valleys  

SciTech Connect

We examine under what circumstances the INTEGRAL/SPI 511 keV signal can originate from decays of MeV-scale composite states produced by: (A) thermonuclear (type Ia) or (B) core collapse supernovae (SNe). The requisite dynamical properties that would account for the observed data are quite distinct, for cases (A) and (B). We determine these requirements in simple hidden valley models, where the escape fraction problem is naturally addressed, due to the long lifetime of the new composite states. A novel feature of scenario (A) is that the dynamics of type Ia SNe, standard candles for cosmological measurements, might be affected by our mechanism. In case (A), the mass of the state mediating between the hidden sector and the SM e{sup +}e{sup -} could be a few hundred GeV and within the reach of a 500GeV e{sup +}e{sup -} linear collider. We also note that kinetic mixing of the photon with a light vector state may provide an interesting alternate mediation mechanism in this case. Scenarios based on case (B) are challenged by the need for a mechanism to transport some of the produced positrons toward the Galactic bulge, due to the inferred distribution of core collapse sources. The mass of the mediator in case (B) is typically hundreds of TeV, leading to long-lived particles that could, under certain circumstances, include a viable dark matter candidate. The appearance of long-lived particles in typical models leads to cosmological constraints and we address how a consistent cosmic history may be achieved.

Davoudiasl, H.; Perez, G.

2009-12-01T23:59:59.000Z

84

Resolving the 1040 keV cosmic X-ray background with constellation-X  

Science Journals Connector (OSTI)

The energy density of the Cosmic X-ray background (XRB) peaks around 30 keV (see Figure 1) an energy not yet probed by focussing imaging instruments. The first hard X-ray telescope due to fly on a space mission will be that on board Constellation-X. The imaging capability besides providing an improvement of several orders of magnitude in sensitivity over current passively collimated detectors will permit for the first time to resolve a fraction of the XRB at this most crucial energy. Synthesis models of the XRB based on obscured AGN predict that at least 40% of the 1040 keV XRB will be resolved by Constellation-X.

Giorgio Matt; Fulvio Pompilio; Fabio La Franca

2001-01-01T23:59:59.000Z

85

First measurement of the 14N(p,gamma)15O cross section down to 70 keV  

E-Print Network (OSTI)

In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate is determined by the slowest process, the 14N(p,gamma)15O reaction. Deep underground in Italy's Gran Sasso laboratory, at the LUNA 400 kV accelerator, the cross section of this reaction has been measured at energies much lower than ever achieved before. Using a windowless gas target and a 4pi BGO summing detector, direct cross section data has been obtained down to 70 keV, reaching a value of 0.24 picobarn. The Gamow peak has been covered by experimental data for several scenarios of stable and explosive hydrogen burning. In addition, the strength of the 259 keV resonance has been remeasured. The thermonuclear reaction rate has been calculated for temperatures 90 - 300 *10^6 K, for the first time with negligible impact from extrapolations.

A. Lemut; D. Bemmerer; F. Confortola; R. Bonetti; C. Broggini; P. Corvisiero; H. Costantini; J. Cruz; A. Formicola; Zs. Fulop; G. Gervino; A. Guglielmetti; C. Gustavino; Gy. Gyurky; G. Imbriani; A. P. Jesus; M. Junker; B. Limata; R. Menegazzo; P. Prati; V. Roca; D. Rogalla; C. Rolfs; M. Romano; C. Rossi Alvarez; F. Schumann; E. Somorjai; O. Straniero; F. Strieder; F. Terrasi; H. P. Trautvetter

2006-02-09T23:59:59.000Z

86

Resolving the 10-40 keV Cosmic X-ray Background with Constellation-X  

E-Print Network (OSTI)

The energy density of the Cosmic X-ray background (XRB) peaks around 30 keV (see Figure 1), an energy not yet probed by focussing imaging instruments. The first hard X-ray telescope due to fly on a space mission will be that on board Constellation-X. The imaging capability, besides providing an improvement of several orders of magnitude in sensitivity over current passively collimated detectors, will permit for the first time to resolve a fraction of the XRB at this most crucial energy. Synthesis models of the XRB based on obscured AGN predict that at least 40% of the 10-40 keV XRB will be resolved by Constellation-X.

Giorgio Matt; Fulvio Pompilio; Fabio La Franca

2000-07-08T23:59:59.000Z

87

TIME-RESOLVED 1-10 keV CRYSTAL SPECTROMETER FOR THE Z MACHINE AT SANDIA NATIONAL LABORATORIES  

SciTech Connect

We have designed, fabricated, calibrated, and fielded a fast, time-resolved 1-10 keV crystal spectrometer to observe the evolution of wire pinch spectra at the Z machine at Sandia National Laboratories. The instrument has two convex cylindrical crystals (PET and KAP). Both crystals Bragg reflect x-rays into an array of ten silicon diodes, providing continuous spectral coverage in twenty channels from 1.0 to 10 keV. The spectral response of the instrument has been calibrated from 1.0 to 6.3 keV at beamline X8A at the National Synchrotron Light Source. The time response of the 1-mm2 silicon detectors was measured with the Pulsed X-ray Source at Bechtel Nevada's Los Alamos Operations, where 2-nanosecond full-width half-maximum (FWHM) waveforms with 700-picosecond rise times typically were observed. The spectrometer has been fielded recently on several experimental runs at the Z Machine. In this paper, we present the time-resolved spectra resulting from the implosions of double-nested tungsten wire arrays onto 5-mm diameter foam cylinders. We also show the results obtained for a double-nested stainless steel wire array with no target cylinder. The spectrometer was located at the end of a 7.1-meter beamline on line-of sight (LOS)21/22, at an angle 12{sup o} above the equatorial plane, and was protected from the debris field by a customized dual-slit fast valve. The soft detector channels below 2.0 keV recorded large signals at pinch time coinciding with signals recorded on vacuum x-ray diodes (XRDs). On experiment Z993, the spectrometer channels recorded a second pulse with a hard x-ray emission spectrum several nanoseconds after pinch time.

D. V. Morgan; S. Gardner; R. Liljestrand; M. Madlener; S. Slavin; M. Wu

2003-06-01T23:59:59.000Z

88

New Observations of the Solar 0.5-5 keV Soft X-ray Spectrum  

E-Print Network (OSTI)

The solar corona is orders of magnitude hotter than the underlying photosphere, but how the corona attains such high temperatures is still not understood. Soft X-ray (SXR) emission provides important diagnostics for thermal processes in the high-temperature corona, and is also an important driver of ionospheric dynamics at Earth. There is a crucial observational gap between ~0.2 and ~4 keV, outside the ranges of existing spectrometers. We present observations from a new SXR spectrometer, the Amptek X123-SDD, which measured the spatially-integrated solar spectral irradiance from ~0.5 to ~5 keV, with ~0.15 keV FWHM resolution, during sounding rocket flights on 2012 June 23 and 2013 October 21. These measurements show that the highly variable SXR emission is orders of magnitude greater than that during the deep minimum of 2009, even with only weak activity. The observed spectra show significant high-temperature (5-10 MK) emission and are well fit by simple power-law temperature distributions with indices of ~6, ...

Caspi, Amir; Warren, Harry P

2015-01-01T23:59:59.000Z

89

GALAXY CLUSTERS IN THE SWIFT/BAT ERA. II. 10 MORE CLUSTERS DETECTED ABOVE 15 keV  

SciTech Connect

We report on the discovery of 10 additional galaxy clusters detected in the ongoing Swift/Burst Alert Telescope (BAT) all-sky survey. Among the newly BAT-discovered clusters there are Bullet, A85, Norma, and PKS 0745-19. Norma is the only cluster, among those presented here, which is resolved by BAT. For all the clusters, we perform a detailed spectral analysis using XMM-Newton and Swift/BAT data to investigate the presence of a hard (non-thermal) X-ray excess. We find that in most cases the clusters' emission in the 0.3-200 keV band can be explained by a multi-temperature thermal model confirming our previous results. For two clusters (Bullet and A3667), we find evidence for the presence of a hard X-ray excess. In the case of the Bullet cluster, our analysis confirms the presence of a non-thermal, power-law-like, component with a 20-100 keV flux of 3.4 x 10{sup -12} erg cm{sup -2} s{sup -1} as detected in previous studies. For A3667, the excess emission can be successfully modeled as a hot component (kT {approx} 13 keV). We thus conclude that the hard X-ray emission from galaxy clusters (except the Bullet) has most likely a thermal origin.

Ajello, M.; Reimer, O. [SLAC National Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, 2575 Sand Hill Road, Menlo Park, CA 94025 (United States); Rebusco, P. [Kavli Institute for Astrophysics and Space Research, MIT, Cambridge, MA 02139 (United States); Cappelluti, N.; Boehringer, H. [Max Planck Institut fuer Extraterrestrische Physik, P.O. Box 1603, 85740, Garching (Germany); La Parola, V.; Cusumano, G., E-mail: majello@slac.stanford.ed [INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, via U. La Malfa 153, 90146 Palermo (Italy)

2010-12-20T23:59:59.000Z

90

Charge-Exchange Collisions Between Hydrogen Ions and Cesium Vapor in the Energy Range 0.5-20 keV  

Science Journals Connector (OSTI)

Charge-exchange collisions have been studied when H+ ions and ground state H0 atoms are incident on Cs vapor. Measurements of the positive, neutral, and negative beam components after passage through the target were made as a function of the Cs target thickness at several energies between 0.5 and 20 keV. All three beam components were found to approach charge equilibrium monotonically. The maximum H- equilibrium yield is (21 4)%, which occurs at an H+ energy of 0.75 keV. The H- yield decreases with increasing energy, and is 0.4% at 20 keV. At energies below 4 keV the H+ equilibrium yield is very small compared with the yield of H0 and H-. For energies greater than 10 kev the H- equilibrium yield is very small compared with the yield of H0 and H+. The cross sections ?+0, ?+-, ?0+, and ?0- were measured. The subscripts + and - refer to the H+ and H- ions, 0 as an initial subscript refers to a ground-state H0 atom, and 0 as a final subscript refers to an H0 atom in the particular states produced. The cross section ?+0 decreases with increasing energy, and ranges from (9.4 2.0) 10-15 cm2 at 1 keV to (7.5 1.1) 10-16 cm2 at 15 keV. The cross section ?+- decreases with increasing energy in the range 2-15 keV, and has the value (2.1 0.6) 10-17 cm2 at 5 keV. The cross section ?0+ increases with increasing energy, having the value (1.2 0.2) 10-17 cm2 at 2 keV, and (1.74 0.26) 10-16 cm2 at 15 keV. The cross section ?0- decreases with increasing energy, having the value (1.5 0.3) 10-16 cm2 at 2 keV and (1.4 0.2) 10-17 cm2 at 15 keV.

A. S. Schlachter; P. J. Bjorkholm; D. H. Loyd; L. W. Anderson; W. Haeberli

1969-01-05T23:59:59.000Z

91

Study of 18 keV K-? x-ray emission from high intensity femtosecond laser produced plasma  

SciTech Connect

We report an experimental study on the optimization of a laser plasma based x-ray source of ultra-short duration K-? line radiation. The interaction of pulses from a CPA based Ti:sapphire laser (10 TW, 45 fs, 10 Hz) system with magnesium, titanium, iron and copper solid target generates bright 1-8 keV K-? x-ray radiation. The x-ray yield was optimized with the laser pulse duration (at fixed fluence) which is varied in the range of 45 fs to 1.4 ps. It showed a maximum at laser pulse duration of ?740 fs, 420 fs, 350 and 250 fs for Mg (1.3 keV), Ti (4.5 keV), Fe (6.4 keV) and Cu (8.05 keV) respectively. The x-ray yield is observed to be independent of the sign of the chirp. The scaling of the K-? yield (I{sub x} ? I{sub L}{sup ?}) for 45 fs and optimized pulse duration were measured for laser intensities in the region of 3 10{sup 14} 8 10{sup 17}. The x-ray yield shows a much faster scaling exponent ? = 1.5, 2.1, 2.4 and 2.6 for Mg, Ti, Fe and Cu respectively at optimized pulse duration compared to scaling exponent of 0.65, 1.3, 1.5, and 1.7 obtained for 45 fs duration laser pulses. The laser to x-ray energy conversion efficiencies obtained for different target materials are ?{sub Mg} = 1.2 10{sup ?5}, ?{sub Ti} = 3.1 10{sup ?5}, ?{sub Fe} = 2.7 10{sup ?5}, ?{sub Cu} = 1.9 10{sup ?5}. The results have been explained from the efficient generation of optimal energy hot electrons at longer laser pulse duration. The faster scaling observed at optimal pulse duration indicates that the x-ray source is generated at the target surface and saturation of x-ray emission would appear at larger laser fluence. An example of utilization of the source for measurement of shock-wave profiles in a silicon crystal by time resolved x-ray diffraction is also presented.

Arora, V., E-mail: arora@rrcat.gov.in; Naik, P. A.; Chakera, J. A.; Bagchi, S.; Tayyab, M.; Gupta, P. D. [Laser Plasma Division, Raja Rammana Centre for Advanced Technology, Indore 452 013 (India)] [Laser Plasma Division, Raja Rammana Centre for Advanced Technology, Indore 452 013 (India)

2014-04-15T23:59:59.000Z

92

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics Single axis, air bearing goniometer; CCD detector, low-temperature system

93

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics Single axis, air bearing goniometer; CCD detector, low-temperature system

94

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics Single axis, air bearing goniometer; CCD detector, low-temperature system

95

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics Single axis, air bearing goniometer; CCD detector, low-temperature system

96

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

5.0.2 5.0.2 Beamline 5.0.2 Print Tuesday, 20 October 2009 08:35 Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics

97

Beamline 5.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-wavelength anomalous diffraction (MAD) and monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm period wiggler (W11) Energy range 5-16 keV Monochromator Double-crystal, Si(111) liquid N2 cooled Measured flux at 12.4 keV 8.0 x 1011 photons/s at 400-mA ring current, with 1.5-mrad convergence and 100-µm pinhole collimator Resolving power (E/ΔE) 7,000 Divergence at sample 3.0(h) x 0.4 (v) mrad (user selectable) Spot size 25-125 µm (user selectable) Endstations Standard hutch Characteristics Single axis, air bearing goniometer; CCD detector, low-temperature system

98

Curium-245 and curium-247 neutron cross sections between 10 keV and 10 MeV  

SciTech Connect

The optical model code 2PLUS and the statistical model codes COMNUC and CASCADE were used to compute neutron cross sections for Cm-245 and Cm-247 between 10 keV and 10 MeV. Cross sections for elastic and inelastic scattering, radiative capture, fission, and the (n,2n) reactions were computed. The parameters for the fission model were selected to yield agreement with the cross sections from the Physics-8 bomb shot. Pu-239 cross sections were calculated and compared with existing cross section evaluations to demonstrate the validity of the calculational methods.

Clifford, L.R.; McCrosson, F.J.

1982-07-01T23:59:59.000Z

99

Photon production from collisions of 100350-keV positive ions with CO, CF4, and CH4  

Science Journals Connector (OSTI)

Various photon emissions from collisions of H+, H2+, and He+ in the 100350-keV energy range with targets of CO, CF4, and CH4 were studied. The wavelength range of the investigation ran from 2000 to 7000 . Photon-emission cross sections were measured for all significant features. The cross-section data were compared to the Bethe-Born theory through the use of Fano plots. The results show that the theory could be applicable in the case of the CO target, but is probably not applicable to the tetrahedral molecular targets as the emissions are from dissociated atoms.

Eric J. Freeman; Elisabeth L. Bryan; Michael N. Monce

1992-07-01T23:59:59.000Z

100

Simulations of Microchannel Plate Sensitivity to <20 keV X-rays as a Function of Energy and Incident Angle  

SciTech Connect

We present results of Monte Carlo simulations of microchannel plate (MCP) response to x-rays in the 250 eV to 20 keV energy range as a function of both x-ray energy and impact angle. The model is based on the model presented in Rochau et al. (2006). However, while the Rochau et al. (2006) model was two-dimensional, and their results only went to 5 keV, our results have been expanded to 20 keV, and our model has been incorporated into a three-dimensional Monte Carlo MCP model that we have developed over the past several years (Kruschwitz et al. 2011). X-ray penetration through multiple MCP pore walls is increasingly important above 5 keV. The effect of x-ray penetration through multiple pores on MCP performance was studied and is presented.

Kruschwitz, Craig [NSTec; Wu, M. [SNL; Rochau, G. A. [SNL

2013-06-13T23:59:59.000Z

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to obtain the most current and comprehensive results.


101

Chain-oxygen ordering in twin-free YBa2Cu3O7-single crystals driven by 20-keV electron irradiation  

E-Print Network (OSTI)

Chain-oxygen ordering in twin-free YBa2Cu3O7- single crystals driven by 20-keV electron irradiation 2005 We have examined the effects of 20-keV electron irradiation on the -Cu 1 -O 1 - n chain-oxygen arrange- ments in oxygen-deficient but otherwise twin-free YBa2Cu3O7- single crystals. Comparison

Johansen, Tom Henning

102

Measurement of the neutron capture cross section of the s-only isotope 204Pb from 1 eV to 440 keV  

E-Print Network (OSTI)

The neutron capture cross section of 204Pb has been measured at the CERN n_TOF installation with high resolution in the energy range from 1 eV to 440 keV. An R-matrix analysis of the resolved resonance region, between 1 eV and 100 keV, was carried out using the SAMMY code. In the interval between 100 keV and 440 keV we report the average capture cross section. The background in the entire neutron energy range could be reliably determined from the measurement of a 208Pb sample. Other systematic effects in this measurement could be investigated and precisely corrected by means of detailed Monte Carlo simulations. We obtain a Maxwellian average capture cross section for 204Pb at kT=30 keV of 79(3) mb, in agreement with previous experiments. However our cross section at kT=5 keV is about 35% larger than the values reported so far. The implications of the new cross section for the s-process abundance contributions in the Pb/Bi region are discussed.

C. Domingo-Pardo

2006-10-24T23:59:59.000Z

103

Low-energy x-ray dosimetry studies (7 to 17.5 keV) with synchroton radiation  

SciTech Connect

Unique properties of synchrotron radiation (SR), such as its high intensity, brightness, polarization, and broad spectral distribution (extending from x-ray to infra-red wavelengths) make it an attractive light source for numerous experiments. As SR facilities are rapidly being built all over the world, they introduce the need for low-energy x-ray dosemeters because of the potential radiation exposure to experimenters. However, they also provide a unique opportunity for low-energy x-ray dosimetry studies because of the availability of monochromatic x-ray beams. Results of such studies performed at the Stanford Synchrotron Radiation Laboratory are described. Lithium fluoride TLDs (TLD-100) of varying thicknesses (0.015 to 0.08 cm) were exposed free in air to monochromatic x-rays (7 to 17.5 keV). These exposures were monitored with ionization chambers. The response (nC/Gy) was found to increase with increasing TLD thickness and with increasing beam energy. A steeper increase in response with increasing energy was observed with the thicker TLDs. The responses at 7 and 17.5 keV were within a factor of 2.3 and 5.2 for the 0.015 and 0.08 cm-thick TLDs, respectively. The effects of narrow (beam size smaller than the dosemeter) and broad (beam size larger than the dosemeter) beams on the response of the TLDs are also reported.

Ipe, N.E.; Bellamy, H.; Flood, J.R. [and others

1995-06-01T23:59:59.000Z

104

Measurement of the ionization yield of nuclear recoils in liquid argon at 80 and 233 keV  

E-Print Network (OSTI)

The energy calibration of nuclear recoil detectors is of primary importance to rare-event experiments such as those of direct dark matter search and coherent neutrino-nucleus scattering. In particular, such a calibration is performed by measuring the ionization yield of nuclear recoils in liquid Ar and Xe detection media, using neutron elastic scattering off nuclei. In the present work, the ionization yield for nuclear recoils in liquid Ar has for the first time been measured in the higher energy range, at 80 and 233 keV, using a two-phase Cryogenic Avalanche Detector (CRAD) and DD neutron generator. The ionization yield in liquid Ar at an electric field of 2.3 kV/cm amounted to 7.8+/-1.1 and 9.7+/-1.3 e-/keV at 80 and 233 keV respectively. The Jaffe model for nuclear recoil-induced ionization, in contrast to that Thomas-Imel, can probably consistently describe the energy dependence of the ionization yield.

A. Bondar; A. Buzulutskov; A. Dolgov; E. Grishnyaev; S. Polosatkin; L. Shekhtman; E. Shemyakina; A. Sokolov

2014-09-23T23:59:59.000Z

105

Revisiting the relationship between 6 {\\mu}m and 2-10 keV continuum luminosities of AGN  

E-Print Network (OSTI)

We have determined the relation between the AGN luminosities at rest-frame 6 {\\mu}m associated to the dusty torus emission and at 2-10 keV energies using a complete, X-ray flux limited sample of 232 AGN drawn from the Bright Ultra-hard XMM-Newton Survey. The objects have X-ray luminosities corrected for intrinsic absorption between 10^42 and 10^46 erg/s and redshifts from 0.05 to 2.8. The rest-frame 6 {\\mu}m luminosities were computed using data from the Wide-Field Infrared Survey Explorer and are based on a spectral energy distribution decomposition into AGN and galaxy emission. The best-fit relationship for the full sample is consistent with being linear, L_6 {\\mu}m $\\propto$ L_2-10 keV^0.99$\\pm$0.032, but has significant intrinsic scatter, ~0.35 dex in log L_6 {\\mu}m. Assuming a constant X-ray bolometric correction, the fraction of AGN bolometric luminosity reprocessed in the mid-IR decreases weakly, if at all, with the AGN luminosity, a finding at odds with simple receding torus models. Type 2 AGN have re...

Mateos, S; Alonso-Herrero, A; Rovilos, E; Hernn-Caballero, A; Barcons, X; Blain, A; Caccianiga, A; Della Ceca, R; Severgnini, P

2015-01-01T23:59:59.000Z

106

Differential cross sections for single ionization of H{sub 2} by 75-keV proton impact  

SciTech Connect

We have calculated triply differential cross sections (TDCS) and doubly differential cross sections (DDCS) for single ionization of H{sub 2} by 75-keV proton impact using the molecular three-body distorted-wave-eikonal initial-state (M3DW-EIS) approach. Previously published measured DDCS (differential in the projectile scattering angle and integrated over the ejected electron angles) found pronounced structures at relatively large angles that were interpreted as an interference resulting from the two-centered potential of the molecule. Theory treating H{sub 2} as atomic H multiplied by a molecular interference factor only predicts the observed structure when assumptions are made about the molecular orientation. Here we apply the M3DW-EIS method, which does not rely on such an ad hoc approach, but rather treats the interference from first principles.

Chowdhury, U.; Schulz, M.; Madison, D. H. [Missouri University of Science and Technology, Department of Physics and Laboratory for Atomic, Molecular, and Optical Research, Rolla, Missouri 65401 (United States)

2011-03-15T23:59:59.000Z

107

Effect of Degree of Orientation and Crystal Size on the Scattering of 20-kev Electrons by Aluminum  

Science Journals Connector (OSTI)

The energy distribution of 20-kev electrons scattered by aluminum has been measured as a function of degree of crystalline orientation and foil thickness. For equal physical thickness the foils with higher degree of orientation are electron-optically thinner. Over a range of thickness from 35 to 500 A, the values of the first two characteristic losses are 6.30.1 ev and 15.00.1 ev. They exhibit no systematic change with thickness greater than the experimental uncertainty. The intensity ratio between the two losses is essentially constant within this range. It is concluded that the low-lying (6.3 ev) loss is not due to the depolarization effect of grain boundaries.

L. Marton; J. Arol Simpson; J. A. Suddeth; M. D. Wagner; Hiroshi Watanabe

1958-06-01T23:59:59.000Z

108

Characteristic x-ray production by argon projectiles moving in graphite targets between 30 and 200 keV  

Science Journals Connector (OSTI)

Thick-target yields and x-ray spectra have been measured for argon ions impinging on graphite targets at energies between 30 and 200 keV. The thick-target yields of carbon K-shell and argon L-shell x rays are analyzed on the basis of a simple model involving multiple collisions and molecular-orbital promotions. The analysis results in average argon L-shell fluorescence yields and total decay rates for argon ions traversing the solid. These values are found to be substantially lower than those appropriate to argon ions traversing a gas target. An explanation for the differences is proposed, and found to be corroborated by analysis of the observed x-ray spectra. An approximate determination of the argon M-shell vacancy distribution is obtained and compared with beam-foil charge equilibrium measurements.

R. J. Fortner and J. D. Garcia

1975-09-01T23:59:59.000Z

109

The 14C(n,g) cross section between 10 keV and 1 MeV  

E-Print Network (OSTI)

The neutron capture cross section of 14C is of relevance for several nucleosynthesis scenarios such as inhomogeneous Big Bang models, neutron induced CNO cycles, and neutrino driven wind models for the r process. The 14C(n,g) reaction is also important for the validation of the Coulomb dissociation method, where the (n,g) cross section can be indirectly obtained via the time-reversed process. So far, the example of 14C is the only case with neutrons where both, direct measurement and indirect Coulomb dissociation, have been applied. Unfortunately, the interpretation is obscured by discrepancies between several experiments and theory. Therefore, we report on new direct measurements of the 14C(n,g) reaction with neutron energies ranging from 20 to 800 keV.

R. Reifarth; M. Heil; C. Forssen; U. Besserer; A. Couture; S. Dababneh; L. Doerr; J. Goerres; R. C. Haight; F. Kaeppeler; A. Mengoni; S. O'Brien; N. Patronis; R. Plag; R. S. Rundberg; M. Wiescher; J. B. Wilhelmy

2009-10-01T23:59:59.000Z

110

X-ray Filament with a Strong 6.7 keV Line in the Galactic Center Region  

E-Print Network (OSTI)

An elongated X-ray source with a strong K-shell line from He-like iron (Fe XXVI) is found at (RA, Dec)_{J2000.0}=(17h44m00s.0, -29D13'40''.9) in the Galactic center region. The position coincides with the X-ray thread, G359.55+0.16, which is aligned with the radio non-thermal filament. The X-ray spectrum is well fitted with an absorbed thin thermal plasma (apec) model. The best-fit temperature, metal abundance, and column density are 4.1^{+2.7}_{-1.8} keV, 0.58^{+0.41}_{-0.32} solar, and 6.1^{+2.5}_{-1.3}x10^{22} cm^{-2}, respectively. These values are similar to those of the largely extended Galactic center X-ray emission.

Yamauchi, Shigeo; Nakashima, Shinya; Nobukawa, Masayoshi; Tsuru, Takeshi Go; Koyama, Katsuji

2014-01-01T23:59:59.000Z

111

Absolute Calibration of Image Plate for electrons at energy between 100 keV and 4 MeV  

SciTech Connect

The authors measured the absolute response of image plate (Fuji BAS SR2040) for electrons at energies between 100 keV to 4 MeV using an electron spectrometer. The electron source was produced from a short pulse laser irradiated on the solid density targets. This paper presents the calibration results of image plate Photon Stimulated Luminescence PSL per electrons at this energy range. The Monte Carlo radiation transport code MCNPX results are also presented for three representative incident angles onto the image plates and corresponding electron energies depositions at these angles. These provide a complete set of tools that allows extraction of the absolute calibration to other spectrometer setting at this electron energy range.

Chen, H; Back, N L; Eder, D C; Ping, Y; Song, P M; Throop, A

2007-12-10T23:59:59.000Z

112

$?_R$ dark matter-philic Higgs for 3.5 keV X-ray signal  

E-Print Network (OSTI)

We suggest a new model in which a dark matter-philic Higgs is included to discriminate the interaction between dark matter and other particles, to explain the recent observation of the $7~ {\\rm keV}$ X-ray line signal by XMM-Newton observatory. The smallness of the vacuum expectation value of dark matter-philic Higgs can achieve the small mixing angle of the dark matter right-handed neutrino with the ordinary one. We show the range of the symmetry breaking scales as well as the observed dark matter properties are satisfied. In our model, the value of the vacuum expectation value of dark matter-philic Higgs should be about $0.17~ {\\rm GeV}$.

Naoyuki Haba; Hiroyuki Ishida; Ryo Takahashi

2014-08-05T23:59:59.000Z

113

Microsoft Word - Chap3 5-16-05.doc  

Office of Legacy Management (LM)

Three May 2005 Three May 2005 2004 Site Environmental Report 3-1 Results in Brief: 2004 Groundwater Pathway Groundwater Remedy - At the start of 2004, active restoration of the Great Miami Aquifer continued at the following five groundwater restoration modules: * South Plume Module, which became operational on August 27, 1993 * South Field Extraction (Phase I) Module, which became operational on July 13, 1998 * South Plume Optimization Module, which became operational on August 9, 1998 * Re-injection Module, which became operational on September 2, 1998 * Waste Storage Area Module, which became operational on May 8, 2002. The decision was made to convert the advanced wastewater treatment facility (AWWT) into a smaller facility that would remain after site closure in 2006. Construction to convert the facility began in the fall of 2004.

114

Accretion Properties of a Sample of Hard X-Ray (<60 keV) Selected Seyfert 1 Galaxies  

Science Journals Connector (OSTI)

We examine the accretion properties in a sample of 42 hard (3-60 keV) X-ray selected nearby broad-line active galactic nuclei (AGNs). The energy range in the sample is harder than that usually used in similar previous studies. These AGNs are mainly complied from the RXTE All Sky Survey, and complemented by the released INTEGRAL AGN catalog. The black hole masses, bolometric luminosities of AGN, and Eddington ratios are derived from their optical spectra in terms of the broad H? emission line. The tight correlation between the hard X-ray (3-20 keV) and bolometric/line luminosity is well identified in our sample. Also identified is a strong inverse Baldwin relationship of the H? emission line. In addition, all of these hard X-ray AGNs are biased toward luminous objects with a high Eddington ratio (mostly between 0.01 and 0.1) and a low column density (22 cm2), which is most likely due to the selection effect of the surveys. The hard X-ray luminosity is consequently found to be strongly correlated with the black hole mass. We believe the sample completeness will be improved in the next few years by the ongoing Swift and the International Gamma-Ray Astrophysics Laboratory missions, and by the next advanced missions, such as NuSTAR, Simbol-X, and NeXT. Finally, the correlation between RFe (= optical Fe II/H?) and disk temperature as assessed by T ? (L/L Edd)M 1 BH leads us to suggest that the strength of the Fe II emission is mainly determined by the shape of the ionizing spectrum.

J. Wang; Y. F. Mao; J. Y. Wei

2009-01-01T23:59:59.000Z

115

Multiple wavelength X-ray monochromators  

DOE Patents (OSTI)

An improved apparatus and method is provided for separating input x-ray radiation containing first and second x-ray wavelengths into spatially separate first and second output radiation which contain the first and second x-ray wavelengths, respectively. The apparatus includes a crystalline diffractor which includes a first set of parallel crystal planes, where each of the planes is spaced a predetermined first distance from one another. The crystalline diffractor also includes a second set of parallel crystal planes inclined at an angle with respect to the first set of crystal planes where each of the planes of the second set of parallel crystal planes is spaced a predetermined second distance from one another. In one embodiment, the crystalline diffractor is comprised of a single crystal. In a second embodiment, the crystalline diffractor is comprised of a stack of two crystals. In a third embodiment, the crystalline diffractor includes a single crystal that is bent for focusing the separate first and second output x-ray radiation wavelengths into separate focal points. 3 figs.

Steinmeyer, P.A.

1992-11-17T23:59:59.000Z

116

Two-axis sagittal focusing monochromator  

DOE Patents (OSTI)

An x-ray focusing device and method for adjustably focusing x-rays in two orthogonal directions simultaneously. The device and method can be operated remotely using two pairs of orthogonal benders mounted on a rigid, open frame such that x-rays may pass through the opening in the frame. The added x-ray flux allows significantly higher brightness from the same x-ray source.

Haas, Edwin G; Stelmach, Christopher; Zhong, Zhong

2014-05-13T23:59:59.000Z

117

Auger-electron and x-ray production in 50- to 2000-keV Ne+Ne collisions  

Science Journals Connector (OSTI)

The production of vacancies in the inner and outer shells of the target and projectile have been studied in Nei+ + Ne collisions in the incident energy range of 45 keV to 2.2 MeV through the observation of K x rays and Auger electrons. Data are given for incident charge states i=0,1,and2. Parameters necessary for the analysis of collision kinematics were extracted from previous data and used to investigate these effects on the observed Auger spectra. The kinematic line broadening in the Ne collisions is shown to obscure the peak structure characteristic of the multiple ionization states. The centroid energies and average energy widths of the Auger groups, together with absolute intensities, are reported as a function of the Nei+ energy and electron emission angle for both target and projectile. After kinematic corrections, it is found that target and projectile Auger-electron emission are isotropic to within 10% and that the K vacancy created is equally shared between the target and projectile. The average number nA of electrons removed from the L shell simultaneous with the K vacancy production is estimated from the centroid Auger-electron energies and compared with previously measured data. It is found that nA increases with the Ne+ energy from ?2.5-3.6 over the energy range studied. Absolute cross sections for x-ray and Auger-electron production are reported with an accuracy of about 15%, and mean fluorescence yields are determined from these cross-section data. The fluorescence yield increases with incident Ne+-ion energy, and is consistent with the observed degree of L-shell ionization. Total K-vacancy production cross sections agree well with available calculations below 200 keV, but the theoretical results underestimate the cross sections at higher energies. This reflects a breakdown of the two-state approximation made in the calculation. Information regarding the coupling of outer-shell molecular orbitals in the entrance channel is extracted from the comparison of the measured data and previous calculations.

N. Stolterfoht, D. Schneider, D. Burch, B. Aagaard, E. Bving, and B. Fastrup

1975-10-01T23:59:59.000Z

118

Capture of a neutron to excited states of a {sup 9}Be nucleus taking into account resonance at 622 keV  

SciTech Connect

Radiative capture of a neutron to the ground and excited states of the 9Be nucleus is considered using the potential cluster model with forbidden states and with classification of cluster states by the Young schemes taking into account resonance at 622 keV for thermal and astrophysical energies.

Dubovichenko, S. B., E-mail: dubovichenko@gmail.com [National Space Agency of the Republic of Kazakhstan, Fessenkov Astrophysical Institute, National Space Research and Technologies Center (Kazakhstan)

2013-10-15T23:59:59.000Z

119

Scattering of 64 eV to 3 keV Neutrons from Polyethylene and Graphite and the Coherence Length Problem  

E-Print Network (OSTI)

Scattering of 64 eV to 3 keV Neutrons from Polyethylene and Graphite and the Coherence Length 12180, USA (Received 31 August 2005; published 8 February 2006) We measured the neutron scattering by the neutron coherence length. The scattered intensity ratios were found to conform to conventional

Danon, Yaron

120

Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus  

E-Print Network (OSTI)

We test the origin of the 3.5 keV line photons by analyzing the morphology of the emission at that energy from the Galactic Center and from the Perseus cluster of galaxies. We employ a variety of different templates to model the continuum emission and analyze the resulting radial and azimuthal distribution of the residual emission. We then perform a pixel-by-pixel binned likelihood analysis including line emission templates and dark matter templates and assess the correlation of the 3.5 keV emission with these templates. We conclude that the radial and azimuthal distribution of the residual emission is incompatible with a dark matter origin for both the Galactic center and Perseus; the Galactic center 3.5 keV line photons trace the morphology of lines at comparable energy, while the Perseus 3.5 keV photons are highly correlated with the cluster's cool core, and exhibit a morphology incompatible with either dark matter decay or with axion-like particle conversions in the cluster's magnetic fields. The template...

Carlson, Eric; Profumo, Stefano

2014-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

Energy and fluence calibration of the neutron spectrometer ROSPEC at the IRSN AMANDE facility between 70 keV and 4.5 MeV  

Science Journals Connector (OSTI)

......spectrometer in the energy range 144 keV to 14.8 MeV with ISO energies. Radiat. Prot...eds. (1987) II. New York: Academic Press...Bolognese-Milstajn T. AMANDE: a new facility for monoenergetic...United Kingdom Atomic Energy Authority. AWRE......

M. Benmosbah; B. Asselineau

2009-07-01T23:59:59.000Z

122

Finite-Hilbert-basis-set calculations for the angular distribution of ionized electrons produced in p+H impact at 20 keV  

E-Print Network (OSTI)

We present a different method of extracting the angular distribution of ejected electrons in an ion-atom collision from a two-centered finite Hilbert basis-set calculation. We obtain good agreement with experiment for a p+H collision at 20 keV if we...

Reading, John F.; Fu, J.; Fitzpatrick, M. J.

2004-01-01T23:59:59.000Z

123

Beamline 8.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.5 (v) mrad Measured spot size (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K

124

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

125

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

126

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

127

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

128

Beamline 8.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.5 (v) mrad Measured spot size (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K

129

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

130

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

131

Beamline 8.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.5 (v) mrad Measured spot size (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K

132

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

133

Beamline 8.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0(h) x 0.5(v) mrad Measured spot size at sample (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K Special notes Computers for data processing and analysis are available

134

Beamline 8.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Multiple-Wavelength Anomalous Diffraction (MAD) and Macromolecular Crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 T, single pole) Energy range 5-16 keV Monochromator Double crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 3.0 x 1011 photons/sec Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.5 (v) mrad Measured spot size (FWHM) 100 µm Endstations Minihutch Detectors 3x3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available Sample environment Ambient or ~100 K

135

Experimental investigation of the 100 keV X-ray dose response of the high-temperature thermoluminescence in LiF:Mg,Ti (TLD-100): theoretical interpretation using the unified interaction model  

Science Journals Connector (OSTI)

......measured from 1 to 50 000 Gy using 100 keV X rays at the European Synchroton Radiation Facility. Glow curves were deconvoluted into component...from 1 to 50,000 Gy using 100 keV X rays at the European Synchroton Radiation Facility. Glow curves were deconvoluted into component......

J. Livingstone; Y. S. Horowitz; L. Oster; H. Datz; M. Lerch; A. Rosenfeld; A. Horowitz

2010-03-01T23:59:59.000Z

136

The response of a fast phosphor screen scintillator (ZnO:Ga) to low energy ions (0-60 keV)  

SciTech Connect

ZnO:Ga is a promising, high time resolution candidate for use as a fast-ion-loss detector in TJ-II. We compare its ionoluminescence with that of the standard fast-ion-loss detector material, SrGa{sub 2}S{sub 4}:Eu (also known as TG-Green), when irradiated by H{sup +} ions with a range of energies E{<=}60 keV using a dedicated laboratory setup. It is found that ZnO:Ga is a reasonably good candidate for detecting low energy (E<60 keV) ions as it has excellent time resolution; however, its sensitivity is about 100 times lower than TG-Green, potentially limiting it to applications with high energy ion loss signals.

Jimenez-Rey, D. [Centro de Micro-Analisis de Materiales, Universidad Autonoma de Madrid, C/ Faraday 3, Campus de Cantoblanco, E-28049 Madrid (Spain); Zurro, B.; Baciero, A.; Navarro, M. [Laboratorio Nacional de Fusion, Asociacion Euratom-CIEMAT, Av. Complutense 22, E-28040 Madrid (Spain); Rodriguez-Barquero, L. [Laboratorio de Metrologia de Radiaciones lonizantes, CIEMAT, Av. Complutense 22, E-28040 Madrid (Spain)

2010-10-15T23:59:59.000Z

137

Development of a soft x-ray diffractometer for a wideband multilayer grating with a novel layer structure in the 2-4 keV range  

SciTech Connect

We have been developing a wavelength-dispersive soft x-ray spectrograph covering an energy region of 50-4000 eV to attach to a conventional electron microscope. Observation of soft x-ray emission in the 2-4 keV range needs a multilayer coated grating. In order to evaluate the performance of the optical component in the energy region, a goniometric apparatus has been newly developed and the preliminary performance has been tested using synchrotron radiation.

Imazono, Takashi; Koike, Masato; Kawachi, Tetsuya; Hasegawa, Noboru; Koeda, Masaru; Nagano, Tetsuya; Sasai, Hiroyuki; Oue, Yuki; Yonezawa, Zeno; Kuramoto, Satoshi; Terauchi, Masami; Takahashi, Hideyuki; Handa, Nobuo; Murano, Takanori [Quantum Beam Science Directorate, Japan Atomic Energy Agency, 8-1-7 Umemidai, Kizugawa, Kyoto 619-0215 (Japan); Device Dept., Shimadzu Corp., 1 Nishinokyo-Kuwabara-cho, Nakagyo-ku, Kyoto 604-8511 (Japan); IMRAM, Tohoku University, 2-1-1 Katahira, Aoba-ku, Sendai 980-8577 (Japan); ECBU, JEOL Ltd., 3-1-2 Musashino, Akishima, Tokyo 196-8558 (Japan)

2012-07-11T23:59:59.000Z

138

Hard x-ray (>100 keV) imager to measure hot electron preheat for indirectly driven capsule implosions on the NIF  

SciTech Connect

We have fielded a hard x-ray (>100 keV) imager with high aspect ratio pinholes to measure the spatially resolved bremsstrahlung emission from energetic electrons slowing in a plastic ablator shell during indirectly driven implosions at the National Ignition Facility. These electrons are generated in laser plasma interactions and are a source of preheat to the deuterium-tritium fuel. First measurements show that hot electron preheat does not limit obtaining the fuel areal densities required for ignition and burn.

Doeppner, T.; Dewald, E. L.; Divol, L.; Thomas, C. A.; Burns, S.; Celliers, P. M.; Izumi, N.; LaCaille, G.; McNaney, J. M.; Prasad, R. R.; Robey, H. F.; Glenzer, S. H.; Landen, O. L. [Lawrence Livermore National Laboratory, Livermore, California 94551 (United States); Kline, J. L. [Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

2012-10-15T23:59:59.000Z

139

Angular scattering of 150 keV ions through graphene and thin carbon foils: Potential applications for space plasma instrumentation  

SciTech Connect

We present experimental results for the angular scattering of ?150 keV H, He, C, O, N, Ne, and Ar ions transiting through graphene foils and compare them with scattering through nominal ?0.5 ?g?cm{sup ?2} carbon foils. Thin carbon foils play a critical role in time-of-flight ion mass spectrometers and energetic neutral atom sensors in space. These instruments take advantage of the charge exchange and secondary electron emission produced as ions or neutral atoms transit these foils. This interaction also produces angular scattering and energy straggling for the incident ion or neutral atom that acts to decrease the performance of a given instrument. Our results show that the angular scattering of ions through graphene is less pronounced than through the state-of-the-art 0.5 ?g?cm{sup ?2} carbon foils used in space-based particle detectors. At energies less than 50 keV, the scattering angle half width at half maximum, ?{sub 1/2}, for ?35 atoms thick graphene is up to a factor of 3.5 smaller than for 0.5 ?g?cm{sup ?2} (?20 atoms thick) carbon foils. Thus, graphene foils have the potential to improve the performance of space-based plasma instruments for energies below ?50 keV.

Ebert, Robert W., E-mail: rebert@swri.edu [Southwest Research Institute, P. O. Drawer 28510, San Antonio, Texas 78228-0510 (United States); Allegrini, Frdric; Fuselier, Stephen A.; Nicolaou, Georgios [Southwest Research Institute, P. O. Drawer 28510, San Antonio, Texas 78228-0510 (United States) [Southwest Research Institute, P. O. Drawer 28510, San Antonio, Texas 78228-0510 (United States); Physics and Astronomy Department, University of Texas at San Antonio, One UTSA Circle, San Antonio, Texas 78249 (United States); Bedworth, Peter; Sinton, Steve [Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, California 94304 (United States)] [Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, California 94304 (United States); Trattner, Karlheinz J. [Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, California 94304 (United States) [Lockheed Martin Advanced Technology Center, 3251 Hanover Street, Palo Alto, California 94304 (United States); Laboratory for Atmospheric and Space Physics, University of Colorado, 1234 Innovation Drive, Boulder, Colorado 80303 (United States)

2014-03-15T23:59:59.000Z

140

Measurement of the 183 keV Resonance in 17O(p,alpha)14N using a Novel Technique  

SciTech Connect

We have developed a novel technique for measurements of low energy (p,alpha) reactions using heavy ion beams and a differentially-pumped windowless gas target. We applied this new approach to study the 183 keV resonance in the 17O(p,alpha)14}N reaction. We report a resonance energy (center-of-mass) of 183.5{+0.1}{-0.4} keV, a resonance strength of 1.70 +/- 0.15 meV, and set an upper limit (95\\% confidence) on the total width of the state of < 0.1 keV. This resonance is important for the 17O(p,alpha)14}N reaction rate, and we find that 18F production is significantly decreased in low mass ONeMg novae but less affected in more energetic novae. We also report the first determination of the stopping power for oxygen ions in hydrogen gas near the peak of the Bragg curve (E=193 keV/u) to be (63+/-1)e-15 eV-cm2.

Moazen, Brian H [ORNL; Bardayan, Daniel W [ORNL; Blackmon, Jeff C [ORNL; Chae, Kyung Yuk [ORNL; Chipps, Kelly A [ORNL; Domizioli, Carlo P [ORNL; Fitzgerald, Ryan [ORNL; Greife, Uwe [ORNL; Hix, William Raphael [ORNL; Grzywacz-Jones, Kate L [ORNL; KOZUB, RAYMOND L [ORNL; Lingerfelt, Eric J [ORNL; Livesay, Jake [ORNL; Nesaraja, Caroline D [ORNL; Pain, Steven D [ORNL; Roberts, Luke F [ORNL; Shriner, Jr., John F [ORNL; Smith, Michael Scott [ORNL; Thomas, Jeffrey S [ORNL

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
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to obtain the most current and comprehensive results.


141

Double-electron capture on {sup 112}Sn to the excited 1871 keV state in {sup 112}Cd: A possible alternative to double-{beta} decay  

SciTech Connect

We report the first use of a coincidence technique to study neutrinoless double-electron capture (0{nu}ECEC) to an excited state in the daughter nucleus. We investigated 0{nu}ECEC by {sup 112}Sn leading to the possibly degenerate 1871 keV excited state in {sup 112}Cd by searching for its deexcitation {gamma} rays of 1253 keV and 618 keV in coincidence. The experiment was performed at ground level. A sample of 3.91 g of tin enriched to 99.5% in {sup 112}Sn was placed between two high-purity germanium {gamma}-ray detectors. In order to enhance the sample material, rods of natural tin totaling 1.2 kg (natural abundance 0.97%{sup 112}Sn) surrounded the cylindrical surface of our two {gamma}-ray detectors. After an exposure of 1.59 kg x days of {sup 112}Sn, no decays were observed. From this null result we determine a lower limit for the half-life time of T{sub 1/2}>2.7(1.3)x10{sup 19} yr (68%(90%) CL). We hope to achieve a sensitivity in the 10{sup 23} to 10{sup 24} yr range with a sample of a few kg of {sup 112}Sn and improved {gamma}-ray detectors in an underground facility.

Kidd, M. F.; Esterline, J. H.; Tornow, W. [Department of Physics, Duke University and Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708-0308 (United States)

2008-09-15T23:59:59.000Z

142

New emission line at ~3.5 keV - observational status, connection with radiatively decaying dark matter and directions for future studies  

E-Print Network (OSTI)

Recent works of [1402.2301,1402.4119], claiming the detection of extra emission line with energy ~3.5 keV in X-ray spectra of certain clusters of galaxies and nearby Andromeda galaxy, have raised considerable interest in astrophysics and particle physics communities. A number of new observational studies claim detection or non-detection of the extra line in X-ray spectra of various cosmic objects. In this review I summarize existing results of these studies, overview possible interpretations of the extra line, including intriguing connection with radiatively decaying dark matter, and show future directions achievable with existing and planned X-ray cosmic missions.

Iakubovskyi, Dmytro

2014-01-01T23:59:59.000Z

143

Earth X-ray albedo for cosmic X-ray background radiation in the 1--1000 keV band  

E-Print Network (OSTI)

We present calculations of the reflection of the cosmic X-ray background (CXB) by the Earth's atmosphere in the 1--1000 keV energy range. The calculations include Compton scattering and X-ray fluorescent emission and are based on a realistic chemical composition of the atmosphere. Such calculations are relevant for CXB studies using the Earth as an obscuring screen (as was recently done by INTEGRAL). The Earth's reflectivity is further compared with that of the Sun and the Moon -- the two other objects in the Solar system subtending a large solid angle on the sky, as needed for CXB studies.

E. Churazov; S. Sazonov; R. Sunyaev; M. Revnivtsev

2008-02-11T23:59:59.000Z

144

Angular and energy dependence of cross sections for ejection of electrons from water vapor. III. 20150-keV neutral-hydrogen impact  

Science Journals Connector (OSTI)

Absolute values of cross sections for electron production in collisions of neutral hydrogen atoms of 20150 keV energy with water vapor molecules have been measured as a function of the ejection energy and angle. The range of angles was 10 to 160 and the electron energy range was 1300 eV. The doubly differential cross sections were integrated over angle and/or energy to obtain singly differential cross sections, total electron production cross sections, and average energies of ejection. The angular distribution of the electron loss peak was found to have some features in common with the cross section for elastic scattering of electrons.

M. A. Bolorizadeh and M. E. Rudd

1986-02-01T23:59:59.000Z

145

Reduction in the intensity of solar X-ray emission in the 2- to 15-keV photon energy range and heating of the solar corona  

SciTech Connect

The time profiles of the energy spectra of low-intensity flares and the structure of the thermal background of the soft X-ray component of solar corona emission over the period of January-February, 2003, are investigated using the data of the RHESSI project. A reduction in the intensity of X-ray emission of the solar flares and the corona thermal background in the 2- to 15-keV photon energy range is revealed. The RHESSI data are compared with the data from the Interball-Geotail project. A new mechanism of solar corona heating is proposed on the basis of the results obtained.

Mirzoeva, I. K., E-mail: colombo2006@mail.ru [Russian Academy of Sciences, Space Research Institute (Russian Federation)

2013-04-15T23:59:59.000Z

146

High aspect ratio hard x-ray (> 100 keV) imager to measure hot electron preheat for indirectly driven capsule implosions on the National Ignition Facility  

SciTech Connect

We have fielded a multi-pinhole, hard x-ray (> 100 keV) imager to measure the spatially-resolved bremsstrahlung emission from energetic electrons slowing in a plastic ablator shell during indirectly driven implosions at the National Ignition Facility. These electrons are generated in laser plasma interactions, and are a source of preheat to the deuterium-tritium fuel that could limit the compressibility required for ignition and burn. Our hard x-ray imaging measurements allow to set an upper limit to the DT fuel preheat, which we find is acceptable in current capsule implosions on the NIF.

Doppner, T; Dewald, E; Divol, L; Burns, S; Izumi, N; Kline, J; LaCaille, G; McNaney, J; Prasad, R; Thomas, C A; Glenzer, S H; Landen, O; Author, A; Author, S G; Author, T

2012-05-01T23:59:59.000Z

147

Facilities and techniques for x-ray diagnostic calibration in the 100-eV to 100-keV energy range  

SciTech Connect

The Lawrence Livermore National Laboratory (LLNL) has been a pioneer in the field of x-ray diagnostic calibration for more than 20 years. We have built steady state x-ray sources capable of supplying fluorescent lines of high spectral purity in the 100-eV to 100-keV energy range, and these sources have been used in the calibration of x-ray detectors, mirrors, crystals, filters, and film. This paper discusses our calibration philosophy and techniques, and describes some of our x-ray sources. Examples of actual calibration data are presented as well.

Gaines, J.L.; Wittmayer, F.J.

1986-06-01T23:59:59.000Z

148

Formation of submicron oxide widths on aluminum in the presence of keV electron beams and CO/sub 2/ or N/sub 2/O  

SciTech Connect

The purpose of this paper is to report the size of oxide islands or line widths that can be grown as smaller diameter electron beams are used for the oxidation. The implications of the potential lateral resolution available between oxide lines for electronic materials are discussed. The localize dioxide growth on thin Al films occurs in the presence of .5 to 10 keV electron beams and high vacuum level pressures of carbon dioxide or nitrous oxide. Auger electron spectroscopy shows saturation of the O (KLL) signal and depletion of the Al (LMM) signal after an exposure of 5000 l carbon dioxide with a 2 keV beam of 7 A/sq. cm. The oxide is spatially restricted to the beam impact region and is stable for long periods of time in vacuum. The most plausible mechanism for this oxide growth is dissociation of the carbon dioxide or the nitrous oxide by the electron beam in the region of impingement on or near the surface. Oxygen atoms thus formed can then react with the Al, and carbon monoxide or nitrogen desorbs.

Pitts, J.R.; Massopust, T.P.; Czanderna, A.W.; Kazmerski, L.L.

1986-03-01T23:59:59.000Z

149

Non-abelian Dark Matter Solutions for Galactic Gamma-ray Excess and Perseus 3.5 keV X-ray Line  

E-Print Network (OSTI)

We attempt to explain simultaneously the Galactic center gamma-ray excess and the 3.5 keV X-ray line from the Perseus cluster based on a class of non-abelian $SU(2)$ DM models, in which the dark matter and an excited state comprise a "dark" $SU(2)$ doublet. The non-abelian group kinetically mixes with the standard model gauge group via dimensions-5 operators. The dark matter particles annihilate into standard model fermions, followed by fragmentation and bremsstrahlung, and thus producing a continuous spectrum of gamma-rays. On the other hand, the dark matter particles can annihilate into a pair of excited states, each of which decays back into the dark matter particle and an X-ray photon, which has an energy equal to the mass difference between the dark matter and the excited state, which is set to be 3.5 keV. The large hierarchy between the required X-ray and $\\gamma$-ray annihilation cross-sections can be achieved by a very small kinetic mixing between the SM and dark sector, which effectively suppresses t...

Cheung, Kingman; Tsai, Yue-Lin Sming

2014-01-01T23:59:59.000Z

150

Energy and angular distribution of electrons ejected from argon by 5-keV to 1.5-MeV protons  

Science Journals Connector (OSTI)

Cross sections, differential in emission energy and angle, have been measured for the ejection of electrons in collisions of H+ with argon gas targets. Incident-proton energies studied were from 5 keV to 1.5 MeV and electron emission angles ranged from 10 to 160. Integration of the double-differential cross sections over emission angle and energy yield results in good agreement with direct measurement of total ionization cross sections. The electron distributions are compared to two plane-wave Born-approximation calculations, one using Hartree-Slater wave functions and the other using Hartree-Fock wave functions in the 3p-?d channel.

T. L. Criswell; L. H. Toburen; M. E. Rudd

1977-08-01T23:59:59.000Z

151

Charge transfer of 0.5-, 1.5-, and 5-keV protons with atomic oxygen: Absolute differential and integral cross sections  

Science Journals Connector (OSTI)

We report measurements of the absolute differential cross sections for charge-transfer scattering of 0.5-, 1.5-, and 5-keV protons by atomic oxygen at scattering angles between 0.01 and 2.6 in the laboratory frame. Absolute integral cross sections are also reported and compared with previously published total cross sections. The measurements were made using a flowing gas target, which consisted of a mixture of atomic and molecular oxygen produced by passage of O2 through a microwave discharge. The cross sections for atomic oxygen were obtained by appropriate subtraction of the signal due to molecular oxygen from that due to the mixture of O and O2. 1996 The American Physical Society.

B. G. Lindsay; D. R. Sieglaff; D. A. Schafer; C. L. Hakes; K. A. Smith; R. F. Stebbings

1996-01-01T23:59:59.000Z

152

Measurement of the x-ray mass attenuation coefficients of gold in the 38?50-keV energy range  

SciTech Connect

We used synchrotron x rays to measure the x-ray mass attenuation coefficients of gold at nine energies from 38 to 50 keV with accuracies of 0.1%. Our results are much more accurate than previous measurements in this energy range. A comparison of our measurements with calculated mass attenuation coefficients shows that our measurements fall almost exactly midway between the XCOM and FFAST calculated theoretical values, which differ from one another in this energy region by about 4%, even though the range includes no absorption edge. The consistency and accuracy of these measurements open the way to investigations of the x-ray attenuation in the region of the L absorption edge of gold.

Islam, M.T.; Rae, N.A.; Glover, J.L.; Barnea, Z.; de Jonge, M.D.; Tran, C.Q.; Wang, J.; Chantler, C.T. (Melbourne)

2010-11-12T23:59:59.000Z

153

A 3.55 keV line from $\\text{DM}\\rightarrow a \\rightarrow ?$: predictions for cool-core and non-cool-core clusters  

E-Print Network (OSTI)

We further study a scenario in which a 3.55 keV X-ray line arises from decay of dark matter to an axion-like particle (ALP), that subsequently converts to a photon in astrophysical magnetic fields. We perform numerical simulations of Gaussian random magnetic fields with radial scaling of the magnetic field magnitude with the electron density, for both cool-core `Perseus' and non-cool-core `Coma' electron density profiles. Using these, we quantitatively study the resulting signal strength and morphology for cool-core and non-cool-core clusters. Our study includes the effects of fields of view that cover only the central part of the cluster, the effects of offset pointings on the radial decline of signal strength and the effects of dividing clusters into annuli. We find good agreement with current data and make predictions for future analyses and observations.

Joseph P. Conlon; Andrew J. Powell

2014-06-20T23:59:59.000Z

154

Calibration of X-ray detectors in the 8 to 115 keV energy range and their application to diagnostics on the National Ignition Facility  

SciTech Connect

The calibration of X-ray diagnostics is of paramount importance to the National Ignition Facility (NIF) at Lawrence Livermore National Laboratory (LLNL). National Security Technologies LLC (NSTec) fills this need by providing a wide variety of calibration and diagnostic development services in support of the ongoing research efforts at NIF. The X-ray source in the High Energy X-ray lab utilizes induced fluorescence in a variety of metal foils to produce a beam of characteristic X rays ranging from 8 to 111 keV. Presented are the methods used for calibrating a High Purity Germanium detector, which has been absolutely calibrated using radioactive check sources, compared against a silicon photodiode calibrated at Physikalisch Technische Bundesanstalt (PTB). Also included is a limited presentation of results from the recent calibration of the upgraded Filter Fluorescer X ray Spectrometer.

J. J. Lee, M. J. Haugh, G. LaCaille, and P. Torres

2012-10-01T23:59:59.000Z

155

Differential elastic electron-scattering cross sections of pyrimidine in the energy range between 20 eV and 1 keV  

Science Journals Connector (OSTI)

Differential elastic electron-scattering cross sections of pyrimidine were absolutely measured for electron energies from 20 eV to 1 keV in the angular range between 5 and 135. The present results agree with the data of other groups within the experimental uncertainties at scattering angles below 75 while considerable differences among the data were found at higher scattering angles. The experimental values were compared to theoretical values calculated using the modified independent-atom model. The theoretical values reproduce the angular dependence of the experimental differential elastic scattering cross sections qualitatively well for electron energies above 60 eV. The sum of the integral elastic scattering cross sections, obtained by the integration of the differential elastic scattering cross sections, and ionization cross sections predicted by the binary-encounter-Bethe model agree with the previously measured total electron-scattering cross sections of pyrimidine to within 8%.

W. Y. Baek; M. U. Bug; H. Rabus

2014-06-24T23:59:59.000Z

156

Cross Sections for Electron Capture into the Excited Level n=6 of Hydrogen by 5- to 70-keV Protons in Mg Vapor and in Neon  

Science Journals Connector (OSTI)

An optical technique has been used to investigate electron capture into the excited level n=6 of hydrogen by 5- to 70-keV protons passing through magnesium vapor or neon. Photons from the Balmer H? transition which are emitted downstream of the target were analyzed with a grating spectrometer and counted. From these the population of the level n=6 and the cross section for electron capture into n=6 have been obtained. Cross-section estimates for ionization of the level n=6 collisions with Mg atoms are also presented. The electron-capture cross sections are consistent with n-3 extrapolations of electric-gap measurements for capture into higher quantum levels (n?9to15) reported by Il'in and co-workers, Futch and Moses, and Riviere. The results are compared with those of various theoretical models.

Klaus H. Berkner, William S. Cooper, III, Selig N. Kaplan, and Robert V. Pyle

1969-06-05T23:59:59.000Z

157

First result of the experimental search for the 9.4 keV solar axion reactions with Kr-83 in the copper proportional counter  

E-Print Network (OSTI)

The experimental search for solar hadronic axions is started at the Baksan Neutrino Observatory of the Institute for Nuclear Researches Russian Academy of Science. It is assumed that axions are created in the Sun during M1-transition between the first thermally excited level at 9.4 keV and the ground state in Kr-83. The experiment is based on axion detection via resonant absorption process by the same nucleus in the detector. The big copper proportional counter filled with krypton is used to detect signals from axions. The experimental setup is situated in the deep underground low background laboratory. No evidence of axion detection were found after the 26.5 days data collection. Resulting new upper limit on axion mass is m_{A} < 130 eV at 95% C.L.

Yu. M. Gavrilyuk; A. M. Gangapshev; A. V. Derbin; V. V. Kazalov; H. J. Kim; Y. D. Kim; V. V. Kobychev; V. V. Kuzminov; Luqman Ali; V. N. Muratova; S. I. Panasenko; S. S. Ratkevich; D. A. Semenov; D. A. Tekueva; S. P. Yakimenko; E. V. Unzhakov

2014-05-06T23:59:59.000Z

158

Search for 14.4-KeV Solar Axions Emitted in the M1-Transition of Fe-57 Nuclei with CAST  

SciTech Connect

We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of 57Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon g{sub ay}|-1.19g{sub aN}{sup 0}+g{sub aN}{sup 3}| < 1.36 x 10{sup -16} GeV{sup -1} for ma < 0.03 eV at the 95% confidence level.

Andriamonje, S.; Aune, S.; /DAPNIA, Saclay; Autiero, D.; /CERN /Lyon, IPN; Barth, K.; /CERN; Belov, A.; /Moscow, INR; Beltran, B.; /Zaragoza U. /Queen's U., Kingston; Brauninger, H.; /Garching, Max Planck Inst., MPE; Carmona, J.M.; Cebrian, S.; /Zaragoza U.; Collar, J.I.; /Chicago U., EFI /Chicago U., KICP; Dafni, T.; /DAPNIA, Saclay /Darmstadt, Tech. Hochsch. /Zaragoza U.; Davenport, M.; /CERN; Di Lella, L.; /CERN /Pisa, Scuola Normale Superiore; Eleftheriadis, C.; /Aristotle U., Thessaloniki; Englhauser, J.; /Garching, Max Planck Inst., MPE; Fanourakis, G.; /Democritos Nucl. Res. Ctr.; Ferrer-Ribas, E.; /DAPNIA, Saclay; Fischer, H.; Franz, J.; /Freiburg U.; Friedrich, P.; /Garching, Max Planck Inst., MPE; Geralis, T.; /Democritos Nucl. Res. Ctr. /DAPNIA, Saclay /Moscow, INR /Zaragoza U. /British Columbia U. /Freiburg U. /Darmstadt, Tech. Hochsch. /DAPNIA, Saclay /Zaragoza U. /Frankfurt U. /Boskovic Inst., Zagreb /Freiburg U. /Munich, Max Planck Inst. /Boskovic Inst., Zagreb /Democritos Nucl. Res. Ctr. /Darmstadt, Tech. Hochsch. /Garching, Max Planck Inst., MPE /Boskovic Inst., Zagreb /CERN /Aristotle U., Thessaloniki /Boskovic Inst., Zagreb /Munich, Max Planck Inst. /Zaragoza U. /Chicago U., EFI /Chicago U., KICP /Stanford U., Phys. Dept. /SLAC /Zaragoza U. /CERN /DAPNIA, Saclay /CERN /Munich, Max Planck Inst. /Darmstadt, Tech. Hochsch. /Zaragoza U. /Aristotle U., Thessaloniki /Patras U. /Brookhaven /CERN /Munich, Max Planck Inst. /CERN /Chicago U., EFI /Chicago U., KICP /Zaragoza U. /Freiburg U. /CERN /CERN /Patras U.

2011-12-02T23:59:59.000Z

159

Hidden axion dark matter decaying through mixing with QCD axion and the 3.5 keV X-ray line  

E-Print Network (OSTI)

Hidden axions may be coupled to the standard model particles through a kinetic or mass mixing with QCD axion. We study a scenario in which a hidden axion constitutes a part of or the whole of dark matter and decays into photons through the mixing, explaining the 3.5 keV X-ray line signal. Interestingly, the required long lifetime of the hidden axion dark matter can be realized for the QCD axion decay constant at an intermediate scale, if the mixing is sufficiently small. In such a two component dark matter scenario, the primordial density perturbations of the hidden axion can be highly non-Gaussian, leading to a possible dispersion in the X-ray line strength from various galaxy clusters and near-by galaxies. We also discuss how the parallel and orthogonal alignment of two axions affects their couplings to gauge fields.

Tetsutaro Higaki; Naoya Kitajima; Fuminobu Takahashi

2014-08-18T23:59:59.000Z

160

3-10 keV and 0. 1- to 2-MeV observations of four gamma-ray bursts  

SciTech Connect

Four catalogued ..gamma..-ray bursts that occurred between 79/3/7 and 79/7/31 have been observed over the 3 to 10 keV range by a joint NRL/Los Alamos experiment on the Air Force P78-1 satellite. The bursts were also well observed by members of the interplanetary network. In this paper we present hardness ratios, x-ray/..gamma..-ray luminosity ratios, and time histories. The most significant results presented herein can be summarized as follows: (1) gamma-ray bursters can emit fairly strongly at x-ray energies near the time of the ..gamma.. burst with L/sub x//L/sub ..gamma../ approx. .02 (L/sub x/ approx. 10/sup 37/ ergs s/sup -1/, 3 to 10 keV, assuming a distance of 1 kpc); (2) the centroid of the x-ray emission generally lags the ..gamma..-ray centroid, but there is also evidence for one or more types of x-ray precursor activity; (3) the ..gamma..-ray hardness ratios were not highly variable for these particular events. However, there is some evidence that the ..gamma..-ray spectra softened near the ends of the bursts when the x-ray/..gamma..-ray ratios were high; (4) the x-ray/..gamma..-ray power law number index during times of the strongest ..gamma..-ray emission ranged from 0.8 to approx. 1.1 for the four bursts; (5) the x-ray tail of GB790307 probably can be modeled as the cooling of hot plasma generated during the ..gamma..-ray burst. Simple versions of this model can be used to estimate various source parameters. These estimates imply a distance of a few hundred to a few thousand pc; (6) gamma-ray bursters probably do not produce events similar to classical x-ray bursts independently of the ..gamma..-ray emission.

Laros, J.G.; Evans, W.D.; Fenimore, E.E.; Klebesadel, R.W.; Shulman, S.; Fritz, G.

1983-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

A new study of the $^{22}$Ne(p,$?$)$^{23}$Na reaction deep underground: Feasibility, setup, and first observation of the 186 keV resonance  

E-Print Network (OSTI)

The $^{22}$Ne(p,$\\gamma$)$^{23}$Na reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle is active in asymptotic giant branch stars as well as in novae and contributes to the nucleosythesis of neon and sodium isotopes. In order to reduce the uncertainties in the predicted nucleosynthesis yields, new experimental efforts to measure the $^{22}$Ne(p,$\\gamma$)$^{23}$Na cross section directly at the astrophysically relevant energies are needed. In the present work, a feasibility study for a $^{22}$Ne(p,$\\gamma$)$^{23}$Na experiment at the Laboratory for Underground Nuclear Astrophysics (LUNA) 400\\,kV accelerator deep underground in the Gran Sasso laboratory, Italy, is reported. The ion beam induced $\\gamma$-ray background has been studied. The feasibility study led to the first observation of the $E_{\\rm p}$ = 186\\,keV resonance in a direct experiment. An experimental lower limit of 0.12\\,$\\times$\\,10$^{-6}$\\,eV has been obtained for the resonance strength. Informed by the feasibility study, a dedicated experimental setup for the $^{22}$Ne(p,$\\gamma$)$^{23}$Na experiment has been developed. The new setup has been characterized by a study of the temperature and pressure profiles. The beam heating effect that reduces the effective neon gas density due to the heating by the incident proton beam has been studied using the resonance scan technique, and the size of this effect has been determined for a neon gas target.

F. Cavanna; R. Depalo; M. -L. Menzel; M. Aliotta; M. Anders; D. Bemmerer; C. Broggini; C. G. Bruno; A. Caciolli; P. Corvisiero; T. Davinson; A. di Leva; Z. Elekes; F. Ferraro; A. Formicola; Zs. Flp; G. Gervino; A. Guglielmetti; C. Gustavino; Gy. Gyrky; G. Imbriani; M. Junker; R. Menegazzo; P. Prati; C. Rossi Alvarez; D. A. Scott; E. Somorjai; O. Straniero; F. Strieder; T. Szcs; D. Trezzi

2014-11-25T23:59:59.000Z

162

Nonthermal Two Component Dark Matter Model for Fermi-LAT $\\gamma$-ray excess and 3.55 keV X-ray Line  

E-Print Network (OSTI)

A two component model of nonthermal dark matter is formulated to simultaneously explain the Fermi-LAT results indicating a $\\gamma$-ray excess observed from our Galactic Centre in the 1-3 GeV energy range and the detection of an X-ray line at 3.55 keV from extra galactic sources. Two additional Standard Model singlet scalar fields $S_2$ and $S_3$ are introduced. These fields couple among themselves and with the Standard Model Higgs doublet $H$. The interaction terms among the scalar fields, namely $H$, $S_2$ and $S_3$, are constrained by the application of a discrete $\\mathbb{Z}_2\\times \\mathbb{Z}^\\prime_2$ symmetry which breaks softly to a remnant $\\mathbb{Z}^{\\prime \\prime}_2$ symmetry. This residual discrete symmetry is then spontaneously broken through an MeV order vacuum expectation value $u$ of the singlet scalar field $S_3$. The resultant physical scalar spectrum has the Standard Model like Higgs as $\\chi_{{}_{{}_1}}$ with $M_{\\chi_{{}_{{}_1}}}\\sim 125$ GeV, a moderately heavy scalar $\\chi_{{}_{{}_2}}$...

Biswas, Anirban; Roy, Probir

2015-01-01T23:59:59.000Z

163

Atom penetration from a thin film into the substrate during sputtering by polyenergetic Ar{sup +} ion beam with mean energy of 9.4 keV  

SciTech Connect

Penetration of alien atoms (Be, Ni) into Be, Al, Zr, Si and diamond was investigated under Ar{sup +} ion bombardment of samples having thermally evaporated films of 30--50 nm. Sputtering was carried out using a wide energy spectrum beam of Ar{sup +} ions of 9.4 keV to dose D = 1 {times} 10{sup 16}--10{sup 19} ion/cm{sup 2}. Implanted atom distribution in the targets was measured by Rutherford backscattering spectrometry (RBS) of H{sup +} and He{sup +} ions with energy of 1.6 MeV as well as secondary ion mass-spectrometry (SIMS). During the bombardment, the penetration depth of Ar atoms increases with dose linearly. This depth is more than 3--20 times deeper than the projected range of bombarding ions and recoil atoms. This is a deep action effect. The analysis shows that the experimental data for foreign atoms penetration depth are similar to the data calculated for atom migration through the interstitial site in a field of internal (lateral) compressive stresses created in the near-surface layer of the substrate as a result of implantation. Under these experimental conditions atom ratio r{sub i}/r{sub m} (r{sub i} -- radius of dopant, r{sub m} -- radius target of substrate) can play a principal determining role.

Kalin, B.A.; Gladkov, V.P.; Volkov, N.V.; Sabo, S.E. [Moscow Engineering Physics Inst. (Russian Federation)

1995-12-31T23:59:59.000Z

164

Angular distribution of thick-target bremsstrahlung produced by electrons with initial energies ranging from 10 to 20 keV incident on Ag  

Science Journals Connector (OSTI)

Experimental results are presented comparing the intensities of the bremsstrahlung produced by electrons with initial energies ranging from 10 to 20 keV incident on a thick Ag target, measured at forward angles in the range of 0 to 55. When the data are corrected for attenuation due to photon absorption within the target, the results indicate that the detected radiation is distributed anisotropically only at photon energies k that are approximately equal to the initial energy of the incident electrons E0. The results of our experiments suggest that, as k/E0 ? 0, the detected radiation essentially becomes isotropic due primarily to the scattering of electrons within the target. A comparison to the theory of Kissel et al. [At. Data Nucl. Data Tables 28, 381 (1983)] suggests that the angular distribution of bremsstrahlung emitted by electrons incident on thick targets is similar to the angular distribution of bremsstrahlung emitted by electrons incident on free-atom targets only when k/E0 ? 1. The experimental data also are in approximate agreement with the angular distribution predictions of the Monte Carlo program penelope.

D. Gonzales; B. Cavness; S. Williams

2011-11-29T23:59:59.000Z

165

Learning to Apply Metrology Principles to the Measurement of X-ray Intensities in the 500 eV to 110 keV Energy Range  

SciTech Connect

National Security Technologies, LLC (NSTec), Livermore Operations, has two optical radiation calibration laboratories accredited by the National Voluntary Laboratories Accreditation Program (NVLAP) which is the accrediting body of the National Institute of Standards and Technology (NIST), and is now working towards accreditation for its X-ray laboratories. NSTec operates several laboratories with X-ray sources that generate X-rays in the energy range from 50 eV to 115 keV. These X-ray sources are used to characterize and calibrate diagnostics and diagnostic components used by the various national laboratories, particularly for plasma analysis on the Lawrence Livermore National Laboratory (LLNL) National Ignition Facility (NIF). Because X-ray photon flux measurement methods that can be accredited, i.e., traceable to NIST, have not been developed for sources operating in these energy ranges, NSTec, NIST, and the National Voluntary Accreditation Program (NVLAP) together have defined a path toward the development and validation of accredited metrology methods for X-ray energies. The methodology developed for the high energy X-ray (HEX) Laboratory was NSTecs starting point for X-ray metrology accreditation and will be the basis for the accredited processes in the other X-ray laboratories. This paper will serve as a teaching tool, by way of this example using the NSTec X-ray sources, for the process and methods used in developing an accredited traceable metrology.

Haugh, M. J.; Pond, T.; Silbernagel, C.; Torres, P.; Marlett, K.; Goldin, F.; Cyr, S.

2011-02-08T23:59:59.000Z

166

Energy-Loss Spectra and Collision Cross Sections for Impact of 20-120-keV Positive Ions on Molecular Nitrogen  

Science Journals Connector (OSTI)

Inelastic energy-loss spectra induced by impact of H+, H2+, and Ar+ on N2 have been measured at incident ion energies of 20-120 keV, with an energy resolution of about 2 eV. Prominent peaks are observed at energy losses of 9.5 and 13.8 eV. The first of these is well resolved and is attributed to excitation of the Lyman-Birge-Hopfield (LBH) system of N2. The peak at 13.8 eV is believed due primarily to excitation of the b?u1 band of the Worley-Jenkins series. The locations of these features on the energy-loss scale do not agree with results of the electron impact work of others and, in general, show trends with projectile velocity that are consistent with an assumed enhancement of excitation to higher vibrational states with the heavier particles. Collision cross sections for excitation of the two peaks are presented, as well as the total ionization cross section and the cross section for total inelastic processes in the case of proton impact.

F. D. Schowengerdt and John T. Park

1970-03-01T23:59:59.000Z

167

Determination of the absolute K through O conversion coefficients of the 80-keV M4 transition in Irm193  

Science Journals Connector (OSTI)

We produced carrier-free, nearly isotopically pure Irm193 from thermal-neutron irradiation of Os192. From studies of the conversion-electron spectrum, the photon spectrum, and the absolute counting rates, we determined the absolute K, L1, L2, L3, M1, M3, M5, N, and O+P conversion coefficients for the first time. With possibly one exception, these values agree closely with theoretical calculations. The value for the energy of the unconverted gamma ray was found to be 80.220.02 keV. The half-life for Irm193 determined by absolute electron counting in a proportional counter of 100% counting efficiency (4??) was found to be 10.530.04 d. We have determined the L1 subshell fluorescence yield, ?1, to be 0.1200.003 for iridium. Based upon our measurements of initial and final L subshell vacancies together with a best-fit literature value for ?2, we have found a plausible value for the Coster-Kronig coefficient f12 to be 0.0910.011.

M. Lindner; R. Gunnink; R. J. Nagle

1987-09-01T23:59:59.000Z

168

First observation of {alpha} decay of {sup 190}Pt to the first excited level (E{sub exc}=137.2 keV) of {sup 186}Os  

SciTech Connect

The {alpha} decays of naturally occurring platinum isotopes, which are accompanied by the emission of {gamma} quanta, have been searched for deep underground (3600 m water equivalent) at the Gran Sasso National Laboratories of the INFN (Italy). A sample of Pt with a mass of 42.5 g and a natural isotopic composition has been measured with a low background HP Ge detector (468 cm{sup 3}) during 1815 h. The {alpha} decay of {sup 190}Pt to the first excited level of {sup 186}Os (J{sup {pi}}=2{sup +}, E{sub exc}=137.2 keV) has been observed for the first time, with the half-life determined as T{sub 1/2}=2.6{sub -0.3}{sup +0.4}(stat.){+-}0.6(syst.)x10{sup 14} yr. The T{sub 1/2} limits for the {alpha} decays of other Pt isotopes have been determined at the level of T{sub 1/2}{approx_equal}10{sup 16}-10{sup 20} yr. These limits have been set for the first time or they are better than those known from earlier experiments.

Belli, P. [INFN, Sezione di Roma Tor Vergata, I-00133 Rome (Italy); Bernabei, R. [INFN, Sezione di Roma Tor Vergata, I-00133 Rome (Italy); Dipartimento di Fisica, Universita di Roma Tor Vergata, I-00133 Rome (Italy); Cappella, F. [INFN, Sezione di Roma La Sapienza, I-00185 Rome (Italy); Dipartimento di Fisica, Universita di Roma La Sapienza, I-00185 Rome (Italy); Cerulli, R.; Laubenstein, M.; Nisi, S. [INFN, Laboratori Nazionali del Gran Sasso, 67010 Assergi (AQ) (Italy); Danevich, F. A.; Nagorny, S. S.; Polischuk, O. G.; Tretyak, V. I. [Institute for Nuclear Research, MSP 03680 Kyiv (Ukraine); Incicchitti, A. [INFN, Sezione di Roma La Sapienza, I-00185 Rome (Italy)

2011-03-15T23:59:59.000Z

169

Physics design of a 100 keV acceleration grid system for the diagnostic neutral beam for international tokamak experimental reactor  

SciTech Connect

This paper describes the physics design of a 100 keV, 60 A H{sup -} accelerator for the diagnostic neutral beam (DNB) for international tokamak experimental reactor (ITER). The accelerator is a three grid system comprising of 1280 apertures, grouped in 16 groups with 80 apertures per beam group. Several computer codes have been used to optimize the design which follows the same philosophy as the ITER Design Description Document (DDD) 5.3 and the 1 MeV heating and current drive beam line [R. Hemsworth, H. Decamps, J. Graceffa, B. Schunke, M. Tanaka, M. Dremel, A. Tanga, H. P. L. De Esch, F. Geli, J. Milnes, T. Inoue, D. Marcuzzi, P. Sonato, and P. Zaccaria, Nucl. Fusion 49, 045006 (2009)]. The aperture shapes, intergrid distances, and the extractor voltage have been optimized to minimize the beamlet divergence. To suppress the acceleration of coextracted electrons, permanent magnets have been incorporated in the extraction grid, downstream of the cooling water channels. The electron power loads on the extractor and the grounded grids have been calculated assuming 1 coextracted electron per ion. The beamlet divergence is calculated to be 4 mrad. At present the design for the filter field of the RF based ion sources for ITER is not fixed, therefore a few configurations of the same have been considered. Their effect on the transmission of the electrons and beams through the accelerator has been studied. The OPERA-3D code has been used to estimate the aperture offset steering constant of the grounded grid and the extraction grid, the space charge interaction between the beamlets and the kerb design required to compensate for this interaction. All beamlets in the DNB must be focused to a single point in the duct, 20.665 m from the grounded grid, and the required geometrical aimings and aperture offsets have been calculated.

Singh, M. J. [ITER-India, Institute for Plasma Research, Bhat, Gandhinagar, Gujarat 382428 (India); De Esch, H. P. L. [CEA-Cadarache, IRFM, F-13108 Saint-Paul-lez-Durance (France)

2010-01-15T23:59:59.000Z

170

Single- and double-electron capture by 1-100-keV protons in collisions with magnesium and barium atoms  

Science Journals Connector (OSTI)

Absolute total cross sections for single- and double-electron capture by H+ in collisions with Mg and Ba have been measured for energies between 1 and 100 keV. The single-electron-capture cross section has also been calculated with the Gryzinski formalism of the classical binary-encounter approximation. The measured cross sections exhibit both high- and low-energy structure. The high-energy behavior is in accord with the Brinkman-Kramers results and classical predictions for the energy at which inner-shell capture becomes important. The low-energy behavior is discussed in terms of a molecular picture of the collision. The cross sections are shown to be critically dependent on curve-crossing effects which occur at avoided crossings between potential curves. At low energies the double-electron-capture cross section in Mg shows pronounced structure consistent with a description of the collision in terms of transitions via the intermediate H (1s) state. It is shown that this mechanism is not important in Ba, since curve crossings are expected to take place at internuclear separations too large for transitions to occur. A possible explanation for the decrease in single-electron-capture cross section in Ba at low energies is suggested in terms of competition from direct target-excitation collisions. For single-electron capture in Mg, recent low-energy perturbed-stationary-state calculations and high-energy classical-trajectory Monte Carlo calculations by Olson and Liu are in good agreement with experiment. The present classical binary-encounter approximation results for single-electron capture in both Mg and Ba agree with experiment to within a factor of 2 over the entire energy range. Measurements of single- and double-electron capture are also reported for Ar targets. A pronounced second maximum in the double-electron-capture cross section is found.

T. J. Morgan and F. J. Eriksen

1979-04-01T23:59:59.000Z

171

High resolution bragg focusing optics for synchrotron monochromators and analyzers  

SciTech Connect

A number of different applications for high resolution Bragg Focusing Optics are reviewed. Applications include Sagittal Focusing, Energy Dispersive optics for x-ray absorption and diffraction, a curved analyzer-multichannel detector method for efficient acquisition of powder and small angle scattering data, the use of Backscattering Analyzers for very high resolution inelastic scattering, and curved crystals for high energy applications.

Knapp, G.S.; Beno, M.A.; Gofron, K.J.

1997-07-01T23:59:59.000Z

172

SPUTTERING AND MOLECULAR SYNTHESIS INDUCED BY 100 keV PROTONS IN CONDENSED CO{sub 2} AND RELEVANCE TO THE OUTER SOLAR SYSTEM  

SciTech Connect

We present results on sputtering and radiation chemistry of CO{sub 2} films induced by 100 keV H{sup +} at 25 and 50 K. Using a quartz crystal microbalance, we measure a sputtering yield (SY) between {approx}10 and 20 CO{sub 2} equivalent per ion at 25 K. The yield at 50 K is similar to that at 25 K at low fluences, but increases to {approx}2400 by mid-10{sup 14} H{sup +} cm{sup -2} and declines at higher fluence. Irradiation to 1 Multiplication-Sign 10{sup 15} H{sup +} cm{sup -2} depletes {approx}85%-90% of the initial film mass at 50 K, compared to 3% at 25 K. In both cases, mass spectrometry shows that CO is the dominant constituent in the sputtered flux, followed by O{sub 2}, O, and CO{sub 2}. Using infrared spectroscopy, we monitor the depletion of CO{sub 2} and the accumulation of CO and O{sub 2} and minor species as O{sub 3} and CO{sub 3}. We determine G(-CO{sub 2}) = 2.6 {+-} 0.3, the number of CO{sub 2} destroyed per 100 eV at 25 K. A significant fraction of the radiolyzed CO and O{sub 2} are retained in the film at 25 K; only those near the surface are removed during irradiation, contributing to a smaller SY. At 50 K, CO and O{sub 2} are unstable along the 'hot' ion track and are expelled possibly from the entire depth of the film. Our results, and the lack of detection of CO in the exospheres around Rhea and Dione, show that the CO{sub 2} does not originate from sputtering, since otherwise the exosphere would be dominated by CO, the main molecule in the sputtered flux. We suggest that the exospheric CO{sub 2} is thermally released from an endogenic source.

Raut, U.; Baragiola, R. A. [Laboratory for Atomic and Surface Physics, University of Virginia, Thornton Hall B103, Charlottesville, VA 22904 (United States)

2013-07-20T23:59:59.000Z

173

IonCCD for direct position-sensitive charged-particle detection: from electrons and keV ions to hyperthermal biomolecular ions  

SciTech Connect

A novel charged-particle sensitive, pixel based detector array is described and its usage is demonstrated for a variety of applications, from detection of elemental particles (electrons) to hyper-thermal large biomolecular positive and negative ions including keV light atomic and molecular ions. The array detector is a modified light-sensitive charged coupled device (CCD). The IonCCDTM was engineered for direct charged particle detection by replacing the semi-conductor part of the CCD pixel by a conductor1. In contrast with the CCD, where the semi-conductive pixel is responsible for electron-hole pair formation upon photon bombardment, the IonCCD uses a capacitor coupled to the conductive electrode for direct charge integration. The detector can be operated from atmospheric pressure to high vacuum since no high voltages are needed. The IonCCD, presented in this work is an array of 2126 active pixels with 21 um pixel width and 3 um pixel gap. The detection area is 1.5x51mm2 where 1.5 mm and 51 mm are pixel and detector array length, respectively. The result is a one-dimensional position-sensitive detector with 24 um spatial resolution and 88 % pixel area ratio (PAR). In this work we demonstrate the capabilities and the performance of the detector. For the first time we show the direct detection of 250 eV electrons providing linearity response and detection efficiency of the IonCCD as function of electron beam current. Using positive ions from and electron impact source (E-I), we demonstrate that the detection efficiency of the IonCCD is virtually independent of particle energy [250 eV, 1250 eV], particle impact angle [45o, 90o] and particle flux. By combining the IonCCD with a double focusing sector field of Mattauch-Herzog geometry (M-H), we demonstrate fast acquisition of mass spectra in direct air sniffing mode. A first step towards fast in vivo breath analysis is presented. Detection of hyper-thermal biomolecular ions produced using an electrospray ionization source (ESI) is presented. The IonCCD was used as beam profiler to characterize the beam shape and intensity of 15 eV protonated and deprotonated biomolecular ions at the exit of an RF only collisional quadrupole. We present simultaneous detection of 140 eV doubly protonated biomolecular ions when the IonCCD is combined with the M-H analyzer. The latter, demonstrates the possibility of simultaneous separation and micro-array deposition of biological material using a miniature sector field.

Hadjar, Omar; Johnson, Grant E.; Laskin, Julia; Kibelka, Gottfried; Shill, Scott M.; Kuhn, Ken; Cameron, Chad; Kassan, Scott

2011-04-01T23:59:59.000Z

174

Tables and graphs of photon-interaction cross sections from 0. 1 keV to 100 MeV derived from the LLL evaluated-nuclear-data library  

SciTech Connect

Energy-dependent evaluated photon interaction cross sections and related parameters are presented for elements H through Cf(Z = 1 to 98). Data are given over the energy range from 0.1 keV to 100 MeV. The related parameters include form factors and average energy deposits per collision (with and without fluorescence). Fluorescence information is given for all atomic shells that can emit a photon with a kinetic energy of 0.1 keV or more. In addition, the following macroscopic properties are given: total mean free path and energy deposit per centimeter. This information is derived from the Livermore Evaluated-Nuclear-Data Library (ENDL) as of October 1978.

Plechaty, E.F.; Cullen, D.E.; Howerton, R.J.

1981-11-11T23:59:59.000Z

175

[New OPinitial posting 5/16/11] Operating Policy and Procedure  

E-Print Network (OSTI)

an enterprise-wide web publication policy for Texas Tech University websites. REVIEW: This OP will be reviewed--The primary page or entry point of a website b. Primary public entry point--A Web page designed specifically public entry point for the university. c. Secondary public entry point--Any supplementary Web page

Rock, Chris

176

Measurement of the 238U neutron-capture cross section and gamma-emission spectra from 10 eV to 100 keV using the DANCE detector at LANSCE  

SciTech Connect

A careful new measurement of the {sup 238}U(n,{gamma}) cross section from 10 eV to 100 keV has been made using the DANCE detector at LANSCE. DANCE is a 4{pi} calorimetric scintillator array consisting of 160 BaF{sub 2} crystals. Measurements were made on a 48 mg/cm{sup 2} depleted uranium target. The cross sections are in general good agreement with previous measurements. The gamma-ray emission spectra, as a function of gamma multiplicity, were also measured and compared to model calculations.

Ullmann, John L [Los Alamos National Laboratory; Couture, A J [Los Alamos National Laboratory; Keksis, A L [Los Alamos National Laboratory; Vieira, D J [Los Alamos National Laboratory; O' Donnell, J M [Los Alamos National Laboratory; Jandel, M [Los Alamos National Laboratory; Haight, R C [Los Alamos National Laboratory; Rundberg, R S [Los Alamos National Laboratory; Kawano, T [Los Alamos National Laboratory; Chyzh, A [NORTH CAROLINA STATE UNIV; Baramsai, B [NORTH CAROLINA STATE UNIV; Wu, C Y [LLNL; Mitchell, G E [NORTH CAROLINA STATE UNIV; Becker, J A [LLNL; Krticka, M [CHARLES UNIV

2010-01-01T23:59:59.000Z

177

Internal electron conversion of the isomeric {sup 57}Fe nucleus state with an energy of 14.4 keV excited by the radiation of the plasma of a high-power femtosecond laser pulse  

SciTech Connect

We recorded the spectrum of delayed secondary electrons ejected from the target, which was coated with a layer of iron enriched with the {sup 57}Fe isotope to 98%, under its irradiation by fluxes of broadband X-ray radiation and fast electrons from the plasma produced by a femtosecond laser pulse at an intensity of 10{sup 17} W cm{sup -2}. Maxima were identified at energies of 5.6, 7.2, and 13.6 keV in the spectrum obtained for a delay of 90 - 120 ns. The two last-listed maxima owe their origin to the internal electron conversion of the isomeric level with an energy of 14.4 keV and a lifetime of 98 ns to the K and L shells of atomic iron, respectively; the first-named level arises from a cascade K - L{sub 2}L{sub 3} Auger process. Photoexcitaion by the X-ray plasma radiation is shown to be the principal channel of the isomeric level excitation. (interaction of laser radiation with matter)

Golovin, G V; Savel'ev-Trofimov, Andrei B; Uryupina, D S; Volkov, Roman V [International Laser Center, M. V. Lomonosov Moscow State University, Moscow (Russian Federation)

2011-03-31T23:59:59.000Z

178

The Millennium Gas project aims to undertake smoothed-particle hydrodynamic resimulations of the Millennium Simulation, providing many hundred massive galaxy clusters for comparison with X-ray surveys (170 clusters with kTsl > 3 keV). This paper looks at  

E-Print Network (OSTI)

. Abstract The Millennium Gas project aims to undertake smoothed-particle hydrodynamic-ray surveys (170 clusters with kTsl > 3 keV). This paper looks at the hot gas and stellar fractions-core systems but are successful in matching the hot gas profiles of non-cool-core clusters. Although

Thomas, Peter

179

BEAMLINE 4-1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray Absorption Spectroscopy MAIN SCIENTIFIC DISCIPLINES: Environmental / Materials / Chemistry / Biology % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 20-pole, 2.0-Tesla Wiggler, 0.75 mrad, side station BEAM LINE SPECIFICATIONS: energy range grating type resolution DE/E spot size flux angular acceptance unfocused 5,500-38,000eV 10-4 4x18mm 0.75 mrad OPTICS: M0 mirror: Flat, bent vertically collimating, 1 m, Si, Rh-coated, cutoff 9-23 keV, LN2-cooled monochromator. Energies over 22keV are run with the mirror out. MONOCHROMATOR: Si(220) f=0° or Si(220) f=90° double-crystal, non-fixed exit slit Monochromator Crystal Glitch Library

180

SustSciTeam_ProgramSummary_051611.xlsx.5/16/11 1Q 2Q 3Q Summer  

E-Print Network (OSTI)

-month) Orientation and Team Building Year 1 Sustainability Science ESS280A (4units) Independent Research XXX299 (4 units) Independent Research XXX299 (4 units) Summer Salary Sustainability Science Course; Define Team Report; Progress mtgs. Sustainability Science Team - Summary Schedule Apply to Sustainability Science

Rose, Michael R.

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

A novel X-ray diffractometer for studies of liquid-liquid interfaces  

Science Journals Connector (OSTI)

A dedicated liquid surface diffractometer employing a tilting double-crystal monochromator in Bragg geometry has been designed. This diffractometer allows reflectivity and grazing-incidence scattering measurements of an immobile mechanical completely decoupled liquid sample from 6.4 to 29.4 keV.

Murphy, B.M.

2013-11-29T23:59:59.000Z

182

E-Print Network 3.0 - acceptance crystal monochromator Sample...  

NLE Websites -- All DOE Office Websites (Extended Search)

... Source: Controlled Fusion Atomic Data Center (CFADC) Collection: Plasma Physics and Fusion 13 MACS -A New High Intensity Cold Neutron Spectrometer at NIST Summary: V (Ei2.1...

183

Neutron Diffraction Performance Based on Multiple Reflection Monochromator for High-Resolution Neutron Radiography  

Science Journals Connector (OSTI)

The effects of multiple Bragg reflections in single crystal can be observed when more than one set of planes are simultaneously operative for a given wavelength i.e. when more than two reciprocal lattice point...

Pavel Mikula; Miroslav Vrana

2007-01-01T23:59:59.000Z

184

BEAMLINE 7-3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray absorption spectroscopy MAIN SCIENTIFIC DISCIPLINES: Structural Biology % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 20-pole, 2-Tesla wiggler, 0.8 mrad beam, side station BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size (fwhm) flux* angular acceptance unfocused 4600-37000 eV 1 x 10-4 2 x 15 mm2 ~1 x 1012 0.8 mrad *ph/sec @100 mA / 9 keV w 2x15 mm aperture OPTICS: M0 mirror: Flat, bent, vertically collimating, 1 m, Si, Rh-coated, LN2-cooled monochromator MONOCHROMATOR: Si(220) phi=0°, Si(220) phi=90° double-crystal, non-fixed exit slit Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL

185

BEAMLINE 4-3  

NLE Websites -- All DOE Office Websites (Extended Search)

4-3 4-3 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray Absorption Spectroscopy MAIN SCIENTIFIC DISCIPLINES: Environmental / Materials / Biology % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 20-pole, 2.0-Tesla wiggler, 0.75 mrad, side station BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size flux angular acceptance unfocused 2400-14000 eV 10-4 3 x 16 mm 0.75 mrad OPTICS: M0 mirror: Flat, bent vertically collimating, 1 m, Si, Rh-coated, cutoff 4-14 keV, LN2-cooled monochromator MONOCHROMATOR: Si(111) f=0° or Si(111) f=90° double-crystal, non-fixed exit slit Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL

186

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 Beamline 12.3.1 Print Tuesday, 20 October 2009 09:33 Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000 Monochromator #2

187

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000 Monochromator #2 0.6% bandpass multilayers Calculated flux (1.9 GeV, 400 mA)

188

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000 Monochromator #2 0.6% bandpass multilayers Calculated flux (1.9 GeV, 400 mA)

189

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000 Monochromator #2 0.6% bandpass multilayers Calculated flux (1.9 GeV, 400 mA)

190

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

12.3.1 Print 12.3.1 Print Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000 Monochromator #2 0.6% bandpass multilayers Calculated flux (1.9 GeV, 400 mA)

191

Compton scattering of 20- to 40-keV photons  

Science Journals Connector (OSTI)

The scattered-energy spectra of monochronized synchrotron-radiation photons toward 90 by C, Al, Fe, Cu, Au, and Pb samples were measured using high-purity Ge detectors to obtain incoherent scattering function (S) in the 1.14

Y. Namito; S. Ban; H. Hirayama; N. Nariyama; H. Nakashima; Y. Nakane; Y. Sakamoto; N. Sasamoto; Y. Asano; S. Tanaka

1995-04-01T23:59:59.000Z

192

Secondary ion emission under keV carbon cluster bombardment  

E-Print Network (OSTI)

of the impact energy 52 4-3 (A) Negative secondary ion yield per amu of Phe as a function of impact velocity, (B) enlarged view of the secondary ion yield per amu of Phe as a function of impact velocity.... 53 4-4 Secondary ion yield per amu of H - as a function of projectile impact velocity from a phenylalanine sample 55 4-5 Secondary ion yield per amu of D - as a function of projectile impact velocity from a phenylalanine...

Locklear, Jay Edward

2006-10-30T23:59:59.000Z

193

DEVELOPMENT OF 120 keV NEUTRAL BEAM INJECTORS  

E-Print Network (OSTI)

heat load and the heat capacity of the grids determine thepulse. To measure the heat load to the grids we fabricated lines; the average heat load to each grid could thus be

Berkner, K.H.

2010-01-01T23:59:59.000Z

194

CoM Annual Meeting 5/16/05 The meeting began at 4:40 pm in the North Auditorium of the Coleman building, with  

E-Print Network (OSTI)

will graduate in May and another 2 in December. UT students taking the Step 1 board exam had a 91% pass rate and for the Step 2, had a 98.6% pass rate. The motion was made and passed to certify the class. Pres. Waters.g., what is the role of occupational therapy, physical therapy, etc). The second component is a series

Cui, Yan

195

Measurement of vibrational spectrum of liquid using monochromated scanning transmission electron microscopyelectron energy loss spectroscopy  

Science Journals Connector (OSTI)

......application to lithium-ion battery and hence has been well studied...Atom-by-atom spectroscopy at graphene edge. Nature (2010) 468...temperature molten salts as lithium battery electrolyte. Electrochim...additive systems as lithium-ion battery ionic liquid electrolytes......

Tomohiro Miyata; Mao Fukuyama; Akihide Hibara; Eiji Okunishi; Masaki Mukai; Teruyasu Mizoguchi

2014-10-01T23:59:59.000Z

196

High-energy-resolution monochromator for aberration-corrected scanning transmission electron microscopy/electron energy-loss spectroscopy  

Science Journals Connector (OSTI)

...R. F. 1996 Electron energy-loss spectroscopy in...microscope, 2nd edn. New York, NYPlenum. Egerton...Transmission electron energy loss spectrometry in materials...energy-gain spectroscopy. New J. Phys. 10, 1367-2630...

2009-01-01T23:59:59.000Z

197

An Energy-Stabilized Varied-Line-Space-Monochromator UndulatorBeam Line for PEEM Illumination and Magnetic Circular Dichroism  

SciTech Connect

A new undulator beam line has been built and commissioned at the Advanced Light Source for illumination of the PEEM3 microscope. The beam line delivers high flux beams over an energy range from C1s through the transition metals to include the M edges of the magnetic rare earth elements. We present details of the optical design, and data on the performance of the zero-order tracking of the photon energy.

Warwick, Tony; McKinney, Wayne; Domning, Ed; Doran, Andrew; Padmore, Howard

2006-06-01T23:59:59.000Z

198

X-ray Microscopy and Imaging: 2-BM  

NLE Websites -- All DOE Office Websites (Extended Search)

BM BM Introduction The 2-BM beamline offers measurement capabilities for x-ray microtomography, x-ray topography and x-ray microdiffraction. X-ray microtomography and x-ray diffraction instruments are installed on separate optical tables for independent operation with fast switch over time. Optically-coupled high-resolution CCD system is used for microtomography and topography with up to 1 micron spatial resolution. X-ray microdiffraction setup consists of KB microfocussing mirrors (~3 micron minimum spot), four-circle Huber diffractometer, high-precision translation sample stage, two orthogonally-mounted video cameras for viewing sample, fluorescence detector (Si-drift diode) and diffraction detector (a scintillation detector or a CCD). Three different levels of monochromaticity are available. Conventional monochromatic x-rays from a double-bounced Si (111) crystal monochromator (DCM, D E/E=1E-4), wide band-pass monochromatic x-rays from a double multilayer monochromator (DMM, D E/E=1~4E-2) and pink beam. The available x-ray range is from 5 keV to 30 keV. The lower limit is due to the x-ray windows and the upper limit is due to the critical angle of the x-ray mirror. Two different coatings (Cr and Pt) for the x-ray mirror allow either 20 keV or 30 keV energy cutoff.

199

BEAMLINE 9-3  

NLE Websites -- All DOE Office Websites (Extended Search)

9-3 9-3 CURRENT STATUS: Closed (Down-pending mirror repair) SUPPORTED TECHNIQUES: X-ray absorption spectroscopy Single crystal x-ray absorption spectroscopy MAIN SCIENTIFIC DISCIPLINES: Structural Biology % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 16-pole, 2-Tesla wiggler, 2 mrad beam BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size (fwhm) flux* angular acceptance focused 5000-30000 eV 1 x 10-4 0.4 x 3 mm2 ~2 x 1012 2.0 mrad *ph/sec @100 mA / 9 keV w 1x4 mm aperture OPTICS: M0 mirror: Flat, bent, vertically collimating, 1 m, Si, Rh-coated, LN2-cooled monochromator M1 mirror: Bent, cylindrical, 1.2 m, Zerodur, Rh-coated MONOCHROMATOR: Si(220) phi=0°, Si(220) phi=90° double-crystal,

200

BEAMLINE 2-1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 CURRENT STATUS: Open SUPPORTED TECHNIQUES: Powder diffraction Thin film diffraction MAIN SCIENTIFIC DISCIPLINES: Materials / Environmental % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 1.3 Tesla Bend Magnet BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size flux angular acceptance focused 4000-14500 eV ~5 x 10-4 .20 x 0.45 mm 1.5 mrad OPTICS: Bent cylinder, single-crystal Si, Rh-coated mirror Radii: 2900 m (adjustable) x 52 mm Mean angle of incidence: 4.2 milliradians Cut off energy: 14.5 keV, Magnification: 1.1 MONOCHROMATOR: Si(111), Si(220) Si(400), upward reflecting, double-crystal Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

BEAMLINE 7-2  

NLE Websites -- All DOE Office Websites (Extended Search)

7-2 7-2 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray scattering X-ray diffraction MAIN SCIENTIFIC DISCIPLINES: Materials / Environmental % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 20-pole, 2-Tesla Wiggler ID End Station BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size flux angular acceptance focused 4600 - 16500 eV 0.12 x 0.50 mm 0.4 mrad OPTICS: Bent cylinder, single crystal Si, Rh-coated M0 mirror Radii: 2945 m (adjustable) x 56.1 mm Mean angle of incidence: 3.81 mrad Cut off energy: 17.7 keV Magnification: 1.0 MONOCHROMATOR: LN2-cooled, sagitally focusing, double crystal Si(111) Upward reflecting Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL

202

Performance measurements at the SLS SIM beamline  

SciTech Connect

The Surface/Interface: Microscopy beamline of the Swiss Light Source started operation in 2001. In 2007 the beamline has been significantly upgraded with a second refocusing section and a blazed grating optimized for high photon flux. Two Apple II type undulators with a plane grating monochromator using the collimated light scheme deliver photons with an energy from 90eV to about 2keV with variable polarization for the photoemission electron microscope (PEEM) as the primary user station. We measured a focus of (45x60) {mu}m({nu}xh) and a photon flux > 10{sup 12} photon/s for all gratings. Polarization switching within a few seconds is realized with the small bandpass of the monochromator and a slight detuning of the undulator.

Flechsig, U.; Nolting, F.; Fraile Rodriguez, A.; Krempasky, J.; Quitmann, C.; Schmidt, T.; Spielmann, S.; Zimoch, D. [Paul Scherrer Institut, Swiss Light Source, 5232 Villigen PSI (Switzerland)

2010-06-23T23:59:59.000Z

203

Single shot spatial and temporal coherence properties of the SLAC linac coherent light source in the hard x-ray regime  

SciTech Connect

We measured the transverse and longitudinal coherence properties of the Linac Coherent Light Source (LCLS) at SLAC in the hard x-ray regime at 9 keV photon energy on a single shot basis. Speckle patterns recorded in the forward direction from colloidal nanoparticles yielded the transverse coherence properties of the focused LCLS beam. Speckle patterns from a gold nanopowder recorded with atomic resolution allowed us to measure the shot-to-shot variations of the spectral properties of the x-ray beam. The focused beam is in the transverse direction fully coherent with a mode number close to 1. The average number of longitudinal modes behind the Si(111) monochromator is about 14.5 and the average coherence time {tau}{sub c} = (2.0 {+-} 1.0) fs. The data suggest a mean x-ray pulse duration of (29 {+-} 14) fs behind the monochromator for (100 {+-} 14) fs long electron pulses.

Gutt, C.; Wochner, P.; Fischer, B.; Conrad, H.; Castro-Colin, M.; Lee, S.; Lehmkuhler, F.; Steinke, I.; Sprung, M.; Roseker, W.; Zhu, D.; Lemke, H.; Bogle, S.; Fuoss, P. H.; Stephenson, G. B.; Cammarata, M.; Fritz, D. M.; Robert, A.; Grubel, G. (Materials Science Division); (Deutsches Elektronen-Synchrotron); (Max-Planck-Institut fur Intelligene Systeme); (LCLS, SLAC Nat. Accelerator Lab.)

2012-01-01T23:59:59.000Z

204

Optical design and performance of the inelastic scattering beamline at the National Synchrotron Light Source  

SciTech Connect

Phase I of the X21 beamline at the National Synchrotron Light Source was commissioned during 1993. The research program at the X21 beamline is focused on the study of electronic excitations in condensed matter with total energy resolution of 0.1 eV to 1.0 eV. The source is a 27 pole hybrid wiggler. A water-cooled horizontal focusing Si(220) monochromator and a spherically bent Si(444) analyzer were installed and commissioned. At 8 keV the energy resolution of the monochromator is about 0.7 eV, and the energy resolution of the analyzer is about 0.1 eV. Results from several selected experiments are also discussed.

Kao, C.C.; Siddons, D.P.; Oversluizen, T.; Hastings, J.B. [Brookhaven National Lab., Upton, NY (United States); Hamalainen, K. [Helsinki Univ. (Finland). Dept. of Physics; Krisch, M. [European Synchrotron Radiation Facility, 38 - Grenoble (France)

1994-12-31T23:59:59.000Z

205

A New Tomography Beamline at a Wiggler Port at the Center for Advanced Microstructures and Devices (CAMD) Storage Ring  

Science Journals Connector (OSTI)

A new tomography beamline has been built and commissioned at the 7 T wiggler of the CAMD storage ring. This beamline is equipped with two monochromators that can be used interchangeably for X?ray absorption spectroscopy or high resolution X?ray tomography at best 23 ?m pixel size. The high?flux double multilayer?mirror monochromator (W?B4C multilayers) can be used in the energy range from 6 to 35 keV with a resolution (?E/E ) between 0.010.03. The second is a channel?cut Si(311)?crystal monochromator with a range of 15 to 36 keV and resolution of ca. 10?4 this is not yet tested. Tomography has the potential for high?throughput materials analysis; however there are some significant obstacles to be overcome in the areas of data acquisition reconstruction visualization and analysis. Data acquisition is facilitated by the multilayer monochromator as this provides high photon flux thus reducing measurement time. At the beamline Matlab routines provide simple x y z fly?throughs of the sample. Off?beamline processing with Amira can yield more sophisticated inspection of the sample. Standard data acquisition based on fixed angle increments is not optimal however new patterns based on Greek golden ratio angle increments offer faster convergence to a high signal?to?noise?ratio image. The image reconstruction has traditionally been done by back?projection reconstruction. In this presentation we will show first results from samples studied at the new beamline.

Kyungmin Ham; Heath A. Barnett; Leslie G. Butler; Clinton S. Willson; Kevin J. Morris; Roland C. Tittsworth; John D. Scott

2007-01-01T23:59:59.000Z

206

Beamline 10.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print X-ray fluorescence microprobe Scientific disciplines: Environmental science, detector development, low-dose radiation effects in cells GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-20 keV Monochromator White light, multilayer mirrors in Kirkpatrick-Baez configuration Calculated flux (1.9 GeV, 400 mA) 3 x 1010 photons/s at 12.5 keV Resolving power (E/ΔE) White light to 30 at 12 keV Endstations Large hutch with optical table Characteristics X-ray fluorescence analysis of samples with high elemental sensitivity and high spatial resolution Spatial resolution 10 x 10 µm Detectors Silicon drift detector Spot size at sample 1.0 x 1.2 µm Sample format Sample size flexible up to 30 cm x 1 meter depending on configuration.

207

Beamline 10.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print X-ray fluorescence microprobe Scientific disciplines: Environmental science, detector development, low-dose radiation effects in cells GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-20 keV Monochromator White light, multilayer mirrors in Kirkpatrick-Baez configuration Calculated flux (1.9 GeV, 400 mA) 3 x 1010 photons/s at 12.5 keV Resolving power (E/ΔE) White light to 30 at 12 keV Endstations Large hutch with optical table Characteristics X-ray fluorescence analysis of samples with high elemental sensitivity and high spatial resolution Spatial resolution 10 x 10 µm Detectors Silicon drift detector Spot size at sample 1.0 x 1.2 µm Sample format Sample size flexible up to 30 cm x 1 meter depending on configuration.

208

Beamline 10.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

0.3.1 0.3.1 Beamline 10.3.1 Print Tuesday, 20 October 2009 09:14 X-ray fluorescence microprobe Scientific disciplines: Environmental science, detector development, low-dose radiation effects in cells GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-20 keV Monochromator White light, multilayer mirrors in Kirkpatrick-Baez configuration Calculated flux (1.9 GeV, 400 mA) 3 x 1010 photons/s at 12.5 keV Resolving power (E/ΔE) White light to 30 at 12 keV Endstations Large hutch with optical table Characteristics X-ray fluorescence analysis of samples with high elemental sensitivity and high spatial resolution Spatial resolution 10 x 10 µm Detectors Silicon drift detector Spot size at sample 1.0 x 1.2 µm Sample format

209

Beamline 10.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print X-ray fluorescence microprobe Scientific disciplines: Environmental science, detector development, low-dose radiation effects in cells GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-20 keV Monochromator White light, multilayer mirrors in Kirkpatrick-Baez configuration Calculated flux (1.9 GeV, 400 mA) 3 x 1010 photons/s at 12.5 keV Resolving power (E/ΔE) White light to 30 at 12 keV Endstations Large hutch with optical table Characteristics X-ray fluorescence analysis of samples with high elemental sensitivity and high spatial resolution Spatial resolution 10 x 10 µm Detectors Silicon drift detector Spot size at sample 1.0 x 1.2 µm Sample format Sample size flexible up to 30 cm x 1 meter depending on configuration.

210

Beamline 10.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print X-ray fluorescence microprobe Scientific disciplines: Environmental science, detector development, low-dose radiation effects in cells GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-20 keV Monochromator White light, multilayer mirrors in Kirkpatrick-Baez configuration Calculated flux (1.9 GeV, 400 mA) 3 x 1010 photons/s at 12.5 keV Resolving power (E/ΔE) White light to 30 at 12 keV Endstations Large hutch with optical table Characteristics X-ray fluorescence analysis of samples with high elemental sensitivity and high spatial resolution Spatial resolution 10 x 10 µm Detectors Silicon drift detector Spot size at sample 1.0 x 1.2 µm Sample format Sample size flexible up to 30 cm x 1 meter depending on configuration.

211

Bent crystal analyzer without grooves for inelastic scattering -- first experimental results  

SciTech Connect

A new design of a bent crystal analyzer for high energy resolution inelastic X-ray scattering has been recently proposed. It has been theoretically predicted that an analyzer with reflecting planes at a certain angle with respect to a crystal surface, bent with two different radii of curvature, will have the same energy resolution as a perfect crystal. The first experimental measurement obtained at the Advanced Photon Source of a bandwidth of such an analyzer is presented. The overall energy resolution of the analyzer and monochromator observed with a narrow beam is equal to 16.4 meV (FWHM) at 13.84 KeV.

Kushnir, V.I.; Macrander, A.T.

1996-11-01T23:59:59.000Z

212

Power In Space: Time For A Biological Solution http://www.spacedaily.com/reports/Power_In_Space_Time_For_A_Bi... 1 of 4 5/16/2007 10:16 AM  

E-Print Network (OSTI)

on the hardest of hardware: photovoltaics (solar panels), hydrogen fuel cells, radioisotope thermal generators, microbial fuel cells, and algal growing compartments are all visible. Image by Chris Lund. Credit: Int are microbial fuel cells, which rely on microbes that release electrons during metabolism, and gadgets

Lovley, Derek

213

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 2.2 Beamline 12.2.2 Print Tuesday, 20 October 2009 09:31 High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating

214

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

215

Beamline 8.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Multiple-wavelength anomalous diffraction (MAD) and macromolecular crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 tesla, single pole) Energy range 5-17 keV (1% max flux) Monochromator Double flat crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 2.5 x 1011 at 11 keV Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.35 (v) mrad Endstations Minihutch Detectors 3 x 3 CCD array (ADSC Q315r) Measured spot size at sample (FWHM) 0.120 (h) x 0.108 (v) mm Sample format Single crystals of biological molecules. Crystallization tray goniometer available with prior arrangement.

216

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

217

Beamline 8.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Multiple-wavelength anomalous diffraction (MAD) and macromolecular crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 tesla, single pole) Energy range 5-17 keV (1% max flux) Monochromator Double flat crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 2.5 x 1011 at 11 keV Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.35 (v) mrad Endstations Minihutch Detectors 3 x 3 CCD array (ADSC Q315r) Measured spot size at sample (FWHM) 0.120 (h) x 0.108 (v) mm Sample format Single crystals of biological molecules. Crystallization tray goniometer available with prior arrangement.

218

Beamline 8.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Multiple-wavelength anomalous diffraction (MAD) and macromolecular crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 tesla, single pole) Energy range 5-17 keV (1% max flux) Monochromator Double flat crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 2.5 x 1011 at 11 keV Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.35 (v) mrad Endstations Minihutch Detectors 3 x 3 CCD array (ADSC Q315r) Measured spot size at sample (FWHM) 0.120 (h) x 0.108 (v) mm Sample format Single crystals of biological molecules. Crystallization tray goniometer available with prior arrangement.

219

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

220

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

3.1 3.1 Beamline 12.3.1 Print Tuesday, 20 October 2009 09:33 Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

222

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

223

Beamline 12.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.3.1 2.3.1 Beamline 12.3.1 Print Tuesday, 20 October 2009 09:33 Structurally Integrated Biology for Life Sciences (SIBYLS) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend Energy range 5-17 keV (1% max flux) Frequency range 2.5-0.73 Angstrom wavelength Beam size 100 µm round beam default 10 µm and 30 µm collimators available for small samples with flux reduced to 1% and 12%, respectively. 120 µm x 120 µm Gaussian uncollimated beam shape at sample. Scientific discipline Structural biology Monochromator #1 Si(111) Double crystal Calculated flux (1.9 GeV, 400 mA) 2.5 x 1011 photons/sec at 11 keV Resolving power (E/ΔE) 7000

224

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

225

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

Beamline 12.2.2 Beamline 12.2.2 Beamline 12.2.2 Print Tuesday, 20 October 2009 09:31 High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure

226

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

227

Beamline 8.3.1  

NLE Websites -- All DOE Office Websites (Extended Search)

3.1 Print 3.1 Print Multiple-wavelength anomalous diffraction (MAD) and macromolecular crystallography (MX) Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics Superbend magnet (5.0 tesla, single pole) Energy range 5-17 keV (1% max flux) Monochromator Double flat crystal, Si(111) Measured flux (1.9 GeV, 400 mA) 2.5 x 1011 at 11 keV Resolving power (E/ΔE) 7,000 Divergence (max at sample) 3.0 (h) x 0.35 (v) mrad Endstations Minihutch Detectors 3 x 3 CCD array (ADSC Q315r) Measured spot size at sample (FWHM) 0.120 (h) x 0.108 (v) mm Sample format Single crystals of biological molecules. Crystallization tray goniometer available with prior arrangement.

228

South pole bang-time diagnostic on the National Ignition Facility  

SciTech Connect

The south pole bang-time (SPBT) diagnostic views National Ignition Facility (NIF) implosions through the lower hohlraum laser entrance hole to measure the time of peak x-ray emission (peak compression) in indirect drive implosions. Five chemical-vapor-deposition (CVD) diamond photoconductive detectors (PCD's) with different filtrations and sensitivities record the time-varying x rays emitted by the target. Wavelength-selecting highly oriented pyrolytic graphite (HOPG) crystal mirror monochromators increase the x-ray signal-to-background ratio by filtering for 11-keV emission. Diagnostic timing and the in-situ temporal instrument response function are determined from laser impulse shots on the NIF. After signal deconvolution and background removal, the bang time is determined to 45-ps accuracy. The x-ray 'yield' (mJ/sr/keV at 11 keV) is determined from the total area under the peak.

MacPhee, A; Edgell, D; Bradley, D K; Bond, E J; Burns, S; Callahan, D A; Celeste, J; Kimbrough, J; Mackinnon, A J; Magoon, J; Eckart, M J; Glebov, V; Hey, D; Lacielle, G; Kilkenny, J; Parker, J; Sangster, T C; Shoup, M J; Stoeckl, C; Thomas, T

2012-05-01T23:59:59.000Z

229

Beamline 12.2.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2.2 Print 2.2 Print High-Pressure (California High-Pressure Science Observatory: Calipso) Endstations: Medium pressure High pressure laser heating GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for General Sciences Beamlines (6-month cycle) Source characteristics Superbend magnet, 1.9GeV, 5.29Tesla, 500mA Monochromator Si(111) or Multilayer Energy range 6-40 keV for Si(111), 14-28 keV for Multilayer Resolving power (E/ΔE) Si(111) = 7000, Multilayer =100 Beam size (HxV) Focused: 10 x 10 micron Unfocused: 90 x 100 micron Scientific applications High-pressure science Scientific disciplines Earth sciences, materials science, construction materials, chemistry, energy. Endstations Medium pressure High pressure laser heating Experimental techniques High pressure, diffraction, x-ray imaging, XAS, laser heating

230

E-Print Network 3.0 - attosecond kev x-ray Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

de Montral Collection: Engineering 3 Generation of Attosecond X-ray and gamma-ray via Compton backscattering Summary: Generation of Attosecond X-ray and gamma-ray via...

231

Phenomenological description of neutron capture cross sections at 30 keV  

E-Print Network (OSTI)

Studying published data of Maxwellian averaged neutron capture cross sections, we found simple phenomenological rules obeyed by the cross sections as a function of proton and neutron number. We use these rules to make predictions for cross sections of neutron capture on nuclei with proton number above 83, where very few data are available.

Miklos Kiss; Zoltan Trocsanyi

2011-04-01T23:59:59.000Z

232

Heliospheric Energetic Particle Reservoirs: Ulysses and ACE 175-315 keV Electron Observations  

E-Print Network (OSTI)

there is also the additional and dominant contribution from the radioisotope thermoelectric generator (RTG

Sanahuja, Blai

233

Supernova explosions, 511 keV photons, gamma ray bursts and mirror matter  

E-Print Network (OSTI)

There are three astroparticle physics puzzles which fire the imagination: the origin of the ``Great Positron Producer'' in the galactic bulge, the nature of the gamma-ray bursts central engine and the mechanism of supernova explosions. We show that the mirror matter model has the potential to solve all three of these puzzles in one beautifully simple strike.

R. Foot; Z. K. Silagadze

2004-04-27T23:59:59.000Z

234

A Beam line for Macromolecular Crystallography in ALBA  

SciTech Connect

ALBA is a third generation 3 GeV storage ring being built near Barcelona and foreseen to be operational in 2010. Out of the seven beamlines already funded in ALBA, one will be dedicated to macromolecular crystallography (MX). The beamline, dubbed XALOC, shall cope with a broad range of crystal structures and sizes. To this aim, a flexible optical design involving variable focusing optics has been incorporated into the beamline optics. The photon source will be a 2 m long, in-vacuum undulator with a period of 21.3 mm. The optics will consist in a Si(111), double-crystal monochromator cryogenically cooled, and a pair of mirrors placed in a Kirkpatrick-Baez configuration. The beamline will deliver a high flux beam in the 5-15 keV energy range, with an energy resolution of {delta}E/E {approx}2 x 10-4. In addition to the main beamline, it is being considered the possibility to use a diamond laue monochromator to provide photons at a fixed wavelength to an ancillary branch. This report shows the present status of the beamline design.

Juanhuix, Jordi; Ferrer, Salvador [CELLS -ALBA Synchrotron, Ed. Ciencies, Campus UAB, 08193 Bellaterra, Barcelona (Spain)

2007-01-19T23:59:59.000Z

235

Beamline 3.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.1 Print 2.1 Print Commercial deep-etch x-ray lithography (LIGA) GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-12 keV Monochromator None Endstations Hutch with automated scanner Calculated spot size at sample 100 x 10 mm Sample format 3- and 4-in. wafer format; x-ray mask and LIGA substrate Sample environment Ambient, air Scientific disciplines Applied science Scientific applications Deep-etch x-ray lithography (LIGA) Spokesperson This e-mail address is being protected from spambots. You need JavaScript enabled to view it Advanced Light Source, Berkeley Lab Phone: (510) 486-5527 Fax: (510) 486-4102 This e-mail address is being protected from spambots. You need JavaScript enabled to view it AXSUN Technology

236

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available

237

SUPERLATTICE OPTICAL ELEMENTS P. J. Viccaro and E. Ziegler L5-57  

NLE Websites -- All DOE Office Websites (Extended Search)

SUPERLATTICE OPTICAL ELEMENTS SUPERLATTICE OPTICAL ELEMENTS P. J. Viccaro and E. Ziegler L5-57 March, 1986 1 Superlattice Optical Elements Introduction The performance of state-of-the-art Layered Synthetic Microstructures (LSM)(l) or superlattices at x-ray energies even exceeding the soft x-ray domain is a promising sign that systems of this type may play an important role as x-ray optical elements in the energy region of interest to 6-GeV users. As will be discussed below, they are particularly attractive because of their large energy bandpass compared to crystals such as Si or Ge. In fact, they have been suggested recently as elements in high throughput large bandpass x-ray monochromators tunable in the interval of 5-30 keV.(2) For high flux applications, the hope is that LSM will prove to be stable in

238

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available

239

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available

240

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 Beamline 5.0.1 Print Tuesday, 20 October 2009 08:32 Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

Beamline 3.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.1 Print 2.1 Print Commercial deep-etch x-ray lithography (LIGA) GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-12 keV Monochromator None Endstations Hutch with automated scanner Calculated spot size at sample 100 x 10 mm Sample format 3- and 4-in. wafer format; x-ray mask and LIGA substrate Sample environment Ambient, air Scientific disciplines Applied science Scientific applications Deep-etch x-ray lithography (LIGA) Spokesperson This e-mail address is being protected from spambots. You need JavaScript enabled to view it Advanced Light Source, Berkeley Lab Phone: (510) 486-5527 Fax: (510) 486-4102 This e-mail address is being protected from spambots. You need JavaScript enabled to view it AXSUN Technology

242

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available

243

Beamline 5.0.1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 Print 1 Print Berkeley Center for Structural Biology (BCSB) Monochromatic protein crystallography Scientific discipline: Structural biology GENERAL BEAMLINE INFORMATION Operational Yes Proposal cycle Proposals for Structural Biology Beamlines (2-month cycle) Source characteristics 11.4-cm-period wiggler (W11) Energy range 12.7 keV (fixed) Monochromator Si(220) Asymmetric cut single crystal Measured flux 1.50 x 1011 photons/s at 400-mA ring current, with 1.5-mrad divergence and 100-µm pinhole collimator Resolving power (E/ΔE) ~10,000 Divergence at sample 3.0 (h) x 0.4 (v) mrad (user selectable) Spot size 100 µm Endstations Standard hutch Detectors 3 x 3 CCD array (ADSC Q315R) Sample format Single crystals of biological molecules Sample preparation Support labs available

244

BEAMLINE 10-2  

NLE Websites -- All DOE Office Websites (Extended Search)

0-2 0-2 CURRENT STATUS: Open SUPPORTED TECHNIQUES: 10-2a: X-ray absorption spectroscopy; XAS imaging 10-2b: X-ray scattering MAIN SCIENTIFIC DISCIPLINES: Biology / Materials / Environmental % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 30-pole, 1.45-Tesla Wiggler ID End Station BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size flux angular acceptance focused 4500 - 30000 eV 0.2 x .43 mm 1.5 mrad unfocused 4500 - 45000 eV 2.0 x 20.0 mm 1.5 mrad OPTICS: Bent cylinder, Rh-coated, single crystal Si, M0 mirror Radii: 1500 m (adjustable) x 32.9 mm Cut off energy: 22 keV, Mean angle of incidence: 2.7 mrad MONOCHROMATOR: Si(111) f=90° or Si(220) f=90° Liquid nitrogen-cooled,

245

Beamline 3.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.1 Print 2.1 Print Commercial deep-etch x-ray lithography (LIGA) GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-12 keV Monochromator None Endstations Hutch with automated scanner Calculated spot size at sample 100 x 10 mm Sample format 3- and 4-in. wafer format; x-ray mask and LIGA substrate Sample environment Ambient, air Scientific disciplines Applied science Scientific applications Deep-etch x-ray lithography (LIGA) Spokesperson This e-mail address is being protected from spambots. You need JavaScript enabled to view it Advanced Light Source, Berkeley Lab Phone: (510) 486-5527 Fax: (510) 486-4102 This e-mail address is being protected from spambots. You need JavaScript enabled to view it AXSUN Technology

246

Beamline 3.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.1 Print 2.1 Print Commercial deep-etch x-ray lithography (LIGA) GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-12 keV Monochromator None Endstations Hutch with automated scanner Calculated spot size at sample 100 x 10 mm Sample format 3- and 4-in. wafer format; x-ray mask and LIGA substrate Sample environment Ambient, air Scientific disciplines Applied science Scientific applications Deep-etch x-ray lithography (LIGA) Spokesperson This e-mail address is being protected from spambots. You need JavaScript enabled to view it Advanced Light Source, Berkeley Lab Phone: (510) 486-5527 Fax: (510) 486-4102 This e-mail address is being protected from spambots. You need JavaScript enabled to view it AXSUN Technology

247

Extreme ultraviolet diagnosis of a neutral-beam-heated mirror machine  

SciTech Connect

Extreme ultraviolet emissions from the LLL 2XIIB fusion research experiment have been studied. (2XIIB was a magnetic-mirror-plasma-confinement device; beams of high-energy (20 keV) neutral deuterium created a high-density, high-temperature plasma.) A normal-incidence concave-grating monochromator, equipped with a windowless photomultiplier tube, was used to measure emissions in the spectral region from 400 Angstrom to 1600 A. Emissions of oxygen, titanium, carbon, nitrogen, and deuterium were identified; the oxygen brightnesses at times exceeded 10/sup 18/ ph-s/sup -1/-cm/sup -2/-sr/sup -1/. A survey of the emission characteristics found the oxygen concentration was 3%, the other impurities had concentrations near 0.4%. The radiated power loss was about 5% of the deposited neutral beam power.

Drake, R.P.

1980-07-01T23:59:59.000Z

248

The Design of Superconducting Wiggler Beamline BL7 at SAGA-LS  

SciTech Connect

A new hard X-ray beamline has been designed at Saga Light Source. The beamline, named BL7, uses a newly developed 4-Tesla superconducting wiggler as a light source in order to cover a wide energy range to 30 keV. This beamline has a simple optics: a double-crystal monochromator and a Rh-coated bent-cylindrical mirror and can supply a focused beam with a photon flux about 1x10{sup 10} photons/s and a sub-millimeter size. Several experiments will be performed in the experimental station: e.g. protein crystallography; X-ray micro computed tomography; X-ray absorption fine structure measurement.

Kawamoto, M.; Sumitani, K.; Okajima, T. [Beamline Group, Kyushu Synchrotron Light Research Center, Tosu, Saga 841-0005 (Japan)

2010-06-23T23:59:59.000Z

249

Beamline 3.2.1  

NLE Websites -- All DOE Office Websites (Extended Search)

2.1 Print 2.1 Print Commercial deep-etch x-ray lithography (LIGA) GENERAL BEAMLINE INFORMATION Operational Yes, but not open to users Source characteristics Bend magnet Energy range 3-12 keV Monochromator None Endstations Hutch with automated scanner Calculated spot size at sample 100 x 10 mm Sample format 3- and 4-in. wafer format; x-ray mask and LIGA substrate Sample environment Ambient, air Scientific disciplines Applied science Scientific applications Deep-etch x-ray lithography (LIGA) Spokesperson This e-mail address is being protected from spambots. You need JavaScript enabled to view it Advanced Light Source, Berkeley Lab Phone: (510) 486-5527 Fax: (510) 486-4102 This e-mail address is being protected from spambots. You need JavaScript enabled to view it AXSUN Technology

250

Estimation of 235U concentration in some depleted uranium samples by high resolution gamma-ray spectrometry using 185 keV and 1001 keV gamma-energies of 235U and 234mPa  

Science Journals Connector (OSTI)

The identification of isotopic composition of depleted uranium obtained after the reprocessing of spent fuel...235U in the reprocessed uranium will be lower and their depletion depends ... of the reactor and burn...

S. Anilkumar; A. K. Deepa; K. Narayani

2007-10-01T23:59:59.000Z

251

ANL/APS/LS-313 Short-Period APPLE II Undulator for Generating 12-15 keV  

E-Print Network (OSTI)

Radiation Center, Higashi-Hiroshima, 739-0046, Japan Rev. 3, November 25, 2009: Edited by C. Eyberger a zero-emittance electron beam, all radiation on-axis above the first harmonic will be zero). However APPLE II design. In this note, we present magnet design calculations and radiation calculations

Kemner, Ken

252

Enhanced room temperature oxidation in silicon and porous silicon under 10 keV x-ray irradiation  

E-Print Network (OSTI)

is monitored by ellipsometry and interferometric reflectance spectroscopy. Fourier transform infrared FTIR samples used in this work were boron doped p-type Si 100 , 0.01­0.02 cm. Porous silicon films were solution to remove the native oxide and subse- quently rinsed with de-ionized water and dried under nitro

Weiss, Sharon

253

Versatile Silicon Photodiode Detector Technology for Scanning Electron Microscopy with High-Efficiency Sub-5 keV Electron Detection  

E-Print Network (OSTI)

Versatile Silicon Photodiode Detector Technology for Scanning Electron Microscopy with High for Scanning Electron Microscopy, based on ultrashallow p+ n boron-layer photodiodes, features nm-thin anodes, closely-packed photodiodes and through-wafer apertures allow flexible configurations for optimal material

Technische Universiteit Delft

254

Molecular dynamics simulation of radiation damage in CaCd6 quasicrystal cubic approximant up to 10 keV  

E-Print Network (OSTI)

, Finland 2 Department of Mathematics and Physics, Lappeenranta University of Technology, P.O. Box 20, FIN-53851 Lappeenranta, Finland 3 Science and Technology on Surface Physics and Chemistry Laboratory, P

Nordlund, Kai

255

The Determination of Absolute Intensity of 234mPa's 1001 keV Gamma Emission Using Monte Carlo Simulation  

Science Journals Connector (OSTI)

......Granulated glass with uranium content (chemical compo...2 Institute of Public Health Cluj Napoca, Louis Pasteur...composition of the glass with uranium content. Substance Molar...line intensities for depleted uranium. Radiat. Eff. and......

Robert-Csaba Begy; Constantin Cosma; Alida Timar; Dan Fulea

2009-05-01T23:59:59.000Z

256

Measurements of relativistic effects in collective Thomson scattering at electron temperatures less than 1 keV  

E-Print Network (OSTI)

Thomson scattering on the NIF . . 7.1.2 Electron featureon reduced-scale targets at the nif and omega lasers, Janparameter. . . . . . . Figure 1.2: A NIF Au hohlraum target

Ross, James Steven

2010-01-01T23:59:59.000Z

257

FHBS calculation of ionized electron angular and energy distribution following the p+H collision at 20 keV  

E-Print Network (OSTI)

the following Schr? equa- tion ( D2 1r ) c(r) = E c(r): (2.6) The solution to the 1s ground state wave function is j0 >= 2e r Y0;0: (2.7) 11 There are two solutions for a scattering state with momentum k, namely c(+)k (r) = ep=2kG(1 i=k)e ik rF(i=k;1;ikr +ik r... l0 and m0 in Eq. (2.38), thus = ?? l=0 Z ? 0 Cl rl eikr F(l +1+in;2l +2; 2ikr) il(2l +1) jl(Qr) ( 1)l 2e r p4p r2dr( 1)l (4p) 2 (2l +1)2 ?m= lY lm(Q)Ylm(k): (2.42) De ne integral Il(k;Q) = Z ? 0 rl eikr F(l +1+in...

Fu, Jun

2004-11-15T23:59:59.000Z

258

Measurements of relativistic effects in collective Thomson scattering at electron temperatures less than 1 keV  

E-Print Network (OSTI)

basis for laser- plasma interactions in ignition hohlraumslaser-beam propagation through high- temperature ignitionlaser-target coupling efficiency it significantly improves implosion symmetry. The indirect drive approach to ignition

Ross, James Steven

2010-01-01T23:59:59.000Z

259

INTEGRAL Cross-calibration Status: Crab observations between 3 keV and 1 MeV  

E-Print Network (OSTI)

We present results of Crab observations by the INTEGRAL instruments. A simultaneous fit allows us to demonstrate that INTEGRAL provides reliable spectra over its wide energy range.

E. Jourdain; D. Gotz; N. J. Westergaard; L. Natalucci; J. P. Roques

2008-10-03T23:59:59.000Z

260

INTEGRAL Cross-calibration Status: Crab observations between 3 keV and 1 MeV  

E-Print Network (OSTI)

We present results of Crab observations by the INTEGRAL instruments. A simultaneous fit allows us to demonstrate that INTEGRAL provides reliable spectra over its wide energy range.

Jourdain, E; Westergaard, N J; Natalucci, L; Roques, J P

2008-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

Construction of 144, 565 keV and 5.0 MeV monoenergetic neutron calibration fields at JAERI  

Science Journals Connector (OSTI)

......MV Van-de-Graaf accelerator. This paper describes...MV Van-de-Graaf accelerator is a 4UH-HC Pelletron...shown in Figure 1. The accelerator is installed in the...8529-1(1). The nuclear reactions employed for...reaction is made of thin vacuum-deposited LiF on a......

Y. Tanimura; M. Yoshizawa; J. Saegusa; K. Fujii; S. Shimizu; M. Yoshida; Y. Shibata; A. Uritani; K. Kudo

2004-08-01T23:59:59.000Z

262

Experimental aspects of ion acceleration and transport in the Earth's magnetosphere. [Plasmasphere (leV), exo-plasmasphere (leV-lkeV), plasma sheet (1-10 keV), ring current (10-300 keV), trapped radiation belts (>300 keV)  

SciTech Connect

Major particle population within the Earth's magnetosphere have been studied via ion acceleration processes. Experimental advances over the past ten to fifteen years have demonstrated the complexity of the processes. A review is given here for areas where composition experiments have expanded perception on magnetospheric phenomena. 64 refs., 6 figs., 1 tab. (WRF)

Young, D.T.

1985-01-01T23:59:59.000Z

263

A study of the response of a gas ionization chamber to different sources of ionizing radiation  

E-Print Network (OSTI)

ranged from a few keV to 20 MeV and peaked at 5 MeV. The neutrons were produced by the (n, n) reaction o(5. 16MeV)+ Be ~ C+n( 5MeV). A 2-in thick lead brick was placed in front of the chamber to absorb the soft 7-rays emitted from the source along... with the neutrons. The source was kept 9in away from the chamber during all runs. Data were taken for both gas mixtures with the cathode pad facing the source and also with the chamber turned around. In addition to these measurements, four more runs were made...

Zamble?-Die?guez, Filiberto Edmundo

2012-06-07T23:59:59.000Z

264

J. Phys. F : Metal Phys., Vol. 7, No. 12, 1977. Printed in Great Britain. @ 1977 LETTER TO THE EDITOR  

E-Print Network (OSTI)

with a silicon channel-cut crystal monochromator and synchrotron radiation from the 5GeV electron synchroton NINA

Gimzewski, James

265

Pushing high-heat-load optics to the limit  

Science Journals Connector (OSTI)

A cryogenically cooled silicon monochromator and a water-cooled diamond monochromator have been tested under twice the standard power load conditions at the Advanced Photon Source. Both monochromators performed satisfactorily under these extreme power loads (several hundred watts of incident power and up to 300 W/mm2 of incident normal peak power density). The experimental data and the parameters derived to predict the performance limits of the cryogenic silicon monochromator are presented.

P. B. Fernandez

2000-01-01T23:59:59.000Z

266

Sector 1 Frequently Asked Questions  

NLE Websites -- All DOE Office Websites (Extended Search)

Sector 1 - General Information Sector 1 - General Information Sector 1 Safety Plan (pdf) Useful X-Ray Related Numbers Si a0 = 5.4308 Angstrom CeO2 a0=5.411 Angstrom Cd-109 gamma = 88.036 keV X-ray energy/wavelength conversion constant = 12.39842 Angstrom/keV Useful 1-ID Operations Information Always set the undulator by closing from large to small gap. Always scan the Kohzu monochromator from high to low energy. A Cd-109 source that can be used to calibrate detectors can be obtained by contacting Ali. It has Ag flourescent lines and a 88.036 keV gamma line. Tim Mooney's telephone number is 2-5417. Frequently Asked Questions The following questions come up often when using the Sector 1 beamlines. If you have a question (and maybe answer) that would be of general interest to Sector 1 users, please give it to Jon or Greg for inclusion in this list.

267

First ?+SR studies on thin films with a new beam of low energy positive muons at energies below 20 keV  

Science Journals Connector (OSTI)

At the Paul Scherrer Institute slow positive muons (?+) with nearly 100% polarization and an energy of about 10 eV are generated by ... moderation of an intense secondary beam of surface muons in an appropriate c...

T. Prokscha; M. Birke; E. Forgan; H. Glckler; A. Hofer

268

New limit on the mass of 9.4-keV solar axions emitted in an M1 transition in $^{83}$Kr nuclei  

E-Print Network (OSTI)

A search for resonant absorption of the solar axion by $^{83}\\rm{Kr}$ nuclei was performed using the proportional counter installed inside the low-background setup at the Baksan Neutrino Observatory. The obtained model independent upper limit on the combination of isoscalar and isovector axion-nucleon couplings $|g_3-g_0|\\leq 1.69\\times 10^{-6}$ allowed us to set the new upper limit on the hadronic axion mass of $m_{A}\\leq 130$ eV (95\\% C.L.) with the generally accepted values $S$=0.5 and $z$=0.56.

Derbin, A V; Gavrilyuk, Yu M; Kazalov, V V; Kim, H J; Kim, Y D; Kobychev, V V; Kuzminov, V V; Ali, Luqman; Muratova, V N; Panasenko, S I; Ratkevich, S S; Semenov, D A; Tekueva, D A; Yakimenko, S P; Unzhakov, E V

2015-01-01T23:59:59.000Z

269

Cork Embedded Internal Features and Contrast Mechanisms with Del Using 18, 20, 30, 36 and 40 keV Synchrotron X-rays  

SciTech Connect

Images of the cork used for wine and other bottles are visualized with the use of diffraction-enhanced imaging (DEI) technique. Present experimental studies allowed us to identify the cracks, holes, porosity, and importance of soft-matter (soft-material) and associated biology by visualization of the embedded internal complex features of the biological material such as cork and its microstructure. Highlighted the contrast mechanisms above and below the K-absorption edge of iodine and studied the attenuation through a combination of weakly and strongly attenuating materials.

Rao, D.V.; Zhong, Z.; Akatsuka, T.; Yuasa, T.; Hasan, M.Z.; Takeda, T.

2010-01-01T23:59:59.000Z

270

Beryllium and Graphite High-Accuracy Total Cross-Section Measurements in the Energy Range from 24 to 900 keV  

E-Print Network (OSTI)

Beryllium and Graphite High-Accuracy Total Cross-Section Measurements in the Energy Range from 24 new measurements of the carbon and beryllium neutron total cross section in the energy range of 24 the measurement of the energy-dependent total cross section st ~Ei ! by applying Eq. ~1! for every TOF channel i

Danon, Yaron

271

Band mapping in x-ray photoelectron spectroscopy: An experimental and theoretical study of W(110) with 1.25 keV excitation  

Science Journals Connector (OSTI)

Angle-resolved photoemission spectroscopy (ARPES) has generally been carried out at energies below ?150eV, but there is growing interest in going to higher energies so as to achieve greater bulk sensitivity. To this end, we have measured ARPES spectra from a tungsten (110) crystal in a plane containing the [100], [110], and [010] directions with a photon energy of 1253.6 eV. The experimental data are compared to free-electron final-state calculations in an extended zone scheme with no inclusion of matrix elements, as well as highly accurate one-step theory including matrix elements. Both models provide further insight into such future higher-energy ARPES measurements. Special effects occurring in a higher-energy ARPES experiment, such as photon momentum, phonon-induced zone averaging effects, and the degree of cryogenic cooling required are discussed, together with qualitative predictions via appropriate Debye-Waller factors for future experiments with a number of representative elements being presented.

C. Papp; L. Plucinski; J. Minar; J. Braun; H. Ebert; C. M. Schneider; C. S. Fadley

2011-07-18T23:59:59.000Z

272

Synthesis and properties of layered synthetic microstructure (LSM) dispersion elements for 62 eV (200A) to 1. 24 keV (10A) radiation. Final report  

SciTech Connect

The opportunities offered by engineered synthetic multilayer dispersion elements for x-rays have been recognized since the earliest days of x-ray diffraction analysis. In this paper, application of sputter deposition technology to the synthesis of Layered Synthetic Microstructure (LSMs) of sufficient quality for use as x-ray dispersion elements is discussed. It will be shown that high efficiency, controllable bandwidth dispersion elements, with d spacings varying from 15 A to 180 A, may be synthesized onto both mechanically stiff and flexible substrates. Multilayer component materials include tungsten, niobium, molybdenum, titanium, vanadium, and silicon layers separated by carbon layers. Experimental observations of peak reflectivity in first order, integrated reflectivity in first order, and diffraction performance at selected photon energies in the range, 100 to 15,000 eV, will be reported and compared to theory.

Barbee, T.W. Jr.

1981-08-01T23:59:59.000Z

273

Near-Intrinsic Energy Resolution for 30 to 662 keV Gamma Rays in a High Pressure Xenon Electroluminescent TPC  

E-Print Network (OSTI)

The search for neutrinoless double beta decay, Riv. NuovoSearch for Neutrinoless Double-Beta Decay in Xe Xe with EXO-

Catal, J.M.

2014-01-01T23:59:59.000Z

274

Compact Fixed-exit UHV DCM for XAFS  

SciTech Connect

A double-crystal, UHV-compatible monochromator for XAFS applications at bending magnet beamlines has been designed. It uses two crystal sets, Si(111) and (311), on a common central rotation axis driven by an ex-vacuo goniometer. All mechanical and electrical components are mounted on a 400 mm UHV flange which is attached to a compact vacuum chamber. The first crystals are water cooled using connector- and bellowless tubing through the fluidic sealed feedthrough of the central rotation. The first crystal set is mounted off-axis and can be translated vertically to keep the fixed exit condition. The second crystal set uses small crystals of the same size as the first. In order to accept the reflected beam of the first crystal at small Bragg angles, it is tangentially translated along the beam. The angle can be varied from 5 deg. to 55.5 deg. resulting in a total energy range 2.4 - 43.4 keV for Si(111)/(311). Crystal sets are interchangeable by translating the vacuum chamber. Angle encoding is achieved by a Renishaw incremental optical encoder in vacuo.

Rickers, K.; Brueggmann, U.; Drube, W.; Herrmann, M.; Heuer, J.; Welter, E.; Schulte-Schrepping, H.; Schulz-Ritter, H. [Hamburger Synchrotronstrahlungslabor HASYLAB am Deutschen Elektronen-Synchrotron DESY, Notkestr. 85, D-22607 Hamburg (Germany)

2007-01-19T23:59:59.000Z

275

A Beamline for Fast Polarization Switching at NSLS-II  

SciTech Connect

The first XUV beamline (200-2000 eV) at NSLS-II will have two branches, one optimized for photon hungry experiments requiring high coherent flux and one optimized for studies of polarization sensitive materials and interfaces based on fast polarization switching. We describe here the branch designed for fast polarization switching with frequencies up to 1 kHz, high photon flux, and good energy resolution. The beamline will be served by two canted undulators and is based on the focusing variable line spacing grating monochromator. The two beams will be focused at the same spot of approximately 80x10 {mu}m (hor.xver.). The expected circular polarized flux at the sample from each device up to 1.4 keV will be higher than 10{sup 12} photons/s at a resolving power better than 10{sup 4}. An additional KB focusing system will deliver the two beams to a spot in the {mu}m range.

Reininger, R.; Sanchez-Hanke, C.; Hulbert, S. L. [NSLS and NSLS-II, Brookhaven National Laboratory, Upton, New York 11973 (United States)

2010-06-23T23:59:59.000Z

276

Time-Resolved Research at the Advanced Photon Source Beamline 7-ID  

SciTech Connect

The Sector 7 undulator beamline (7-ID) of the Advanced Photon Source (APS) is dedicated to time-resolved x-ray research and is capable of ultrafast measurements on the order of 100 ps. Beamline 7-ID has a laser laboratory featuring a Ti:Sapphire system (average power of 2.5W, pulse duration <50 fs, repetition rate 1-5 kHz) that can be synchronized to the bunch pattern of the storage ring. The laser is deliverable to x-ray enclosures, which contain diffractometers, as well as motorized optical tables for table-top experiments. Beamline 7-ID has a single APS Undulator A and uses a diamond (111) double-crystal monochromator, providing good energy resolution over a range of 6-24 keV. Available optics include Kirkpatrick-Baez (KB) mirrors to microfocus the x-ray beam. A variety of time-resolved diffraction and spectroscopy research is available at 7-ID, with experiments being done in the atomic, molecular, optical, chemistry, and solid state (bulk and surface) fields.

Dufresne, Eric M.; Adams, Bernhard; Arms, Dohn A.; Chollet, Matthieu; Landahl, Eric C.; Li, Yuelin; Walko, Donald A.; Wang, Jin

2010-08-02T23:59:59.000Z

277

Systematic intensity errors caused by spectral truncation: origin and remedy  

Science Journals Connector (OSTI)

X-ray absorption by the monochromator determines the wavelength dispersion in the monochromated X-ray beam and explains the values of 0.03, 0.14 and 0.16 for graphite(002)-monochromated Cu, Mo and Rh radiation. To eliminate the systematic intensity truncation errors, caused by the large wavelength dispersion, a correction is proposed based on the applied scan angle and the real beam spectrum.

Lenstra, A.T.H.

2001-10-26T23:59:59.000Z

278

Polarimetric performance of a Laue lens gamma-ray CdZnTe focal plane prototype  

SciTech Connect

A gamma-ray telescope mission concept [gamma ray imager (GRI)] based on Laue focusing techniques has been proposed in reply to the European Space Agency call for mission ideas within the framework of the next decade planning (Cosmic Vision 2015-2025). In order to optimize the design of a focal plane for this satellite mission, a CdZnTe detector prototype has been tested at the European Synchrotron Radiation Facility under an {approx}100% polarized gamma-ray beam. The spectroscopic, imaging, and timing performances were studied and in particular its potential as a polarimeter was evaluated. Polarization has been recognized as being a very important observational parameter in high energy astrophysics (>100 keV) and therefore this capability has been specifically included as part of the GRI mission proposal. The prototype detector tested was a 5 mm thick CdZnTe array with an 11x11 active pixel matrix (pixel area of 2.5x2.5 mm{sup 2}). The detector was irradiated by a monochromatic linearly polarized beam with a spot diameter of about 0.5 mm over the energy range between 150 and 750 keV. Polarimetric Q factors of 0.35 and double event relative detection efficiency of 20% were obtained. Further measurements were performed with a copper Laue monochromator crystal placed between the beam and the detector prototype. In this configuration we have demonstrated that a polarized beam does not change its polarization level and direction after undergoing a small angle (<1 deg.) Laue diffraction inside a crystal.

Curado da Silva, R. M. [Departmento de Fisica, Universidade de Coimbra, P-3000 Coimbra (Portugal); Center for Space Radiations, Univesite Catholique de Louvain (Belgium); Caroli, E.; Stephen, J. B.; Schiavone, F.; Donati, A.; Ventura, G. [Istituto di Astrofisica Spaziale e Fisica Cosmica-Bologna, Via Gobetti 101, I-40129 Bologna (Italy); Pisa, A.; Auricchio, N.; Frontera, F. [Dipartimento di Fisica, Universita di Ferrara, Ferrara (Italy); Del Sordo, S. [Istituto di Astrofisica Spaziale e Fisica Cosmica-Palermo, Via Ugo La Malfa 153, 90146 Palermo (Italy); Honkimaeki, V. [European Synchrotron Radiation Facility, Grenoble (France); Trindade, A. M. F. [Departmento de Fisica, Universidade de Coimbra, P-3000 Coimbra (Portugal)

2008-10-15T23:59:59.000Z

279

E-Print Network 3.0 - approaches neoadjuvant chemotherapy Sample...  

NLE Websites -- All DOE Office Websites (Extended Search)

of optical spectroscopy in early monitoring of neo-adjuvant... chemotherapy Xenon Arc Lamp + Monochromator Collection Fibers In vivo Breast Tissue Illumination Fibers Imaging...

280

Microsoft PowerPoint - IXD-NSLSII_Poster_Bai  

NLE Websites -- All DOE Office Websites (Extended Search)

crystal sagittal focusing monochromator (Bottom) IXD beamline layout Catalysis: Water gas shift reaction Real-Time Catalysis: In-Situ Structural Studies for Producing and...

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

Electrocatalysis in Alkaline Electrolytes - Research Overview  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Binding Site EXAFS (> 50 eV) * Geometric information * Bond length * Coordination number *BULK short range order Synchrotron Monochromator I o Spectro-electrochemical Cell...

282

Microsoft PowerPoint - FXI_NSLSII_Poster  

NLE Websites -- All DOE Office Websites (Extended Search)

of the FXI beamline. Storage Ring Shield Wall Damping Wiggler Collimating Mirror Toroidal Mirror Monochromator Condenser Sample Objective Detector Secondary Source Aperture Slit...

283

Analytical SuperSTEM for extraterrestrial materials research  

SciTech Connect

Electron-beam studies of extraterrestrial materials with significantly improved spatial resolution, energy resolution and sensitivity are enabled using a 300 keV SuperSTEM scanning transmission electron microscope with a monochromator and two spherical aberration correctors. The improved technical capabilities enable analyses previously not possible. Mineral structures can be directly imaged and analyzed with single-atomic-column resolution, liquids and implanted gases can be detected, and UV-VIS optical properties can be measured. Detection limits for minor/trace elements in thin (<100 nm thick) specimens are improved such that quantitative measurements of some extend to the sub-500 ppm level. Electron energy-loss spectroscopy (EELS) can be carried out with 0.10-0.20 eV energy resolution and atomic-scale spatial resolution such that variations in oxidation state from one atomic column to another can be detected. Petrographic mapping is extended down to the atomic scale using energy-dispersive x-ray spectroscopy (EDS) and energy-filtered transmission electron microscopy (EFTEM) imaging. Technical capabilities and examples of the applications of SuperSTEM to extraterrestrial materials are presented, including the UV spectral properties and organic carbon K-edge fine structure of carbonaceous matter in interplanetary dust particles (IDPs), x-ray elemental maps showing the nanometer-scale distribution of carbon within GEMS (glass with embedded metal and sulfides), the first detection and quantification of trace Ti in GEMS using EDS, and detection of molecular H{sub 2}O in vesicles and implanted H{sub 2} and He in irradiated mineral and glass grains.

Bradley, J P; Dai, Z R

2009-09-08T23:59:59.000Z

284

BEAMLINE 8-1  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 CURRENT STATUS: Open SUPPORTED TECHNIQUES: Photoemission spectroscopy MAIN SCIENTIFIC DISCIPLINES: BL8-1a: Materials / Surface Chemistry BL8-1b: Materials % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: Bending magnet station (vacuum ultraviolet) BEAM LINE SPECIFICATIONS: energy range grating type resolution DE/E spot size (FWHM) flux angular acceptance focused 15 - 185 eV ~1 x 10-3 0.1 mm2 8.0 mrad OPTICS: M0 mirror: Cylindrical, SiC M1 mirror: Spherical, Fused Silica MONOCHROMATOR: 6m toroidal grating monochromator (TGM) Grating Monochromator References Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL support staff.

285

Characterization of Mn-doped ZnO nanobelts by electron energy-loss spectroscopy  

Science Journals Connector (OSTI)

......energy resolution of EELS spectra: an alternative to the monochromator solution. Ultramicroscopy (2003) 96:385-400. 20 Overwijk M , Reefman D. Maximum-entropy deconvolution applied to electron energy-loss spectroscopy. Micron (2000) 31:325-331......

Jingmin Zhang; Chao Yu; Zhimin Liao; Xinzheng Zhang; Liping You; Dapeng Yu

2009-10-01T23:59:59.000Z

286

CAP 4401 / COT 5930 Digital Image Processing Spring 2013 Instructor: Dr. Oge Marques Dept: CEECS  

E-Print Network (OSTI)

processing software tools for lab assignments and projects. Prerequisites: COP 3530 and enhancement algorithms for monochrome as well as color images using MATLAB MATLAB" by Oge Marques Wiley/IEEE Press, 2011 ISBN-10: 0470048158 | ISBN

Marques, Oge

287

Microsoft PowerPoint - 1L35-brochure.ppt  

NLE Websites -- All DOE Office Websites (Extended Search)

* fitted with solar spectrum simulator and optical monochromator LakeShore HFTTP4 cryogenic probe station: * low-noise measurements from 4 K up to 400 K * in-plane field from 1...

288

New Mineral Names  

Science Journals Connector (OSTI)

...05 mm) with MoKa radiation, using a diffractometer...graphite-monochromated CuKa radiation) were obtained from...Gandolfi camera (CuKa radiation). Single-crystal...well to those of the naturally occuring material. Based on...

Paula C. Piilonen; Glenn Poirier; Kim T. Tait

289

2/21/11 11:08 AMOregon Quarterly Features Page 1 of 4http://www.oregonquarterly.com/winter2010/feature4.php  

E-Print Network (OSTI)

/feature4.php UO Home | Dept index Winter 2010 | Volume 90, Number 2 Donate to OQ | Past Issues:08 AMOregon Quarterly Features Page 2 of 4http://www.oregonquarterly.com/winter2010/feature4.php monochrome

Richmond, Geraldine L.

290

STUDIES OF ELECTRON CORRELATION IN THE PHOTOIONIZATION PROCESS  

E-Print Network (OSTI)

from the ultra-high vacuum (UHV ~10- torr) of the beam line,LiF window to separate the UHV and experi- mental chamber.Seya-Namioka monochromator (UHV Design, GCA/McPherson). The

Roseberg, Richard Allen

2011-01-01T23:59:59.000Z

291

Endodermal ABA Signaling Promotes Lateral Root Quiescence during Salt Stress in Arabidopsis Seedlings  

Science Journals Connector (OSTI)

...stage and MFC-2000 controller (Applied Scientific Instrumentation), samples were backlit using an infrared light-emitting diode panel, and images were captured using a digital monochrome camera (CoolSnap) fitted with an NF Micro-Nikor...

Lina Duan; Daniela Dietrich; Chong Han Ng; Penny Mei Yeen Chan; Rishikesh Bhalerao; Malcolm J. Bennett; José R. Dinneny

2013-01-22T23:59:59.000Z

292

Application of spherical gratings in synchrotron radiation spectroscopy  

SciTech Connect

The recent development in gracing incidence grating monochromator design is discussed and the performance limiting for such instruments are examined. Especially the aberrations of toroidal and spherical gratings are investigated using the optical path function concept. It is shown that large radius spherical gratings, which can be produced with better slope tolerances than aspherics, also yield smaller overall line curvature than toroids. Therefore, a new simple spherical grating monochromator design is proposed and its performance is analyzed.

Hogrefe, H.; Howells, M.R.; Hoyer, E.

1986-05-01T23:59:59.000Z

293

Heydemann Algorithm for Energy Scale Linearisation  

SciTech Connect

Many monochromators rely on quadrature encoders for positioning optical elements like gratings or mirrors. In most cases the required accuracy is significantly higher than the pitch of the encoders and an interpolation scheme becomes necessary. The accuracy of this procedure can be significantly enhanced, if signal errors in the detection systems are compensated. We report on the implementation of this technique at the BESSY monochromators and the impact on spectroscopic data.

Follath, Rolf; Balzer, Andreas [Helmholtz-Center Berlin, Electron Storage Ring BESSY II, Albert-Einstein-Strasse 15, 12489 Berlin (Germany)

2010-06-23T23:59:59.000Z

294

Structure and dynamics of the microbial communities underlying the carboxylate platform for biofuel production  

E-Print Network (OSTI)

community analysis of a biogas-producing completely stirredwaste into acids, alcohols, biogas, and hydrogen (5, 16, 25,

Hollister, E.B.

2012-01-01T23:59:59.000Z

295

BEAMLINE 8-2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray absorption spectroscopy, near edge Photoemission spectroscopy MAIN SCIENTIFIC DISCIPLINES: Materials % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: Bending magnet station (soft x-ray) BEAM LINE SPECIFICATIONS: energy range grating type resolution DE/E spot size (FWHM) flux angular acceptance focused 100 - 1300 eV ~4 x 10-4 >0.1 mm2 4.0 mrad OPTICS: M0 mirror: toroidal SiC MONOCHROMATOR: 6m spherical grating monochromator (TGM) Grating Monochromator References ABSORPTION: NA INSTRUMENTATION: User Chambers on VUV Lines DATA ACQUISITION AND ANALYSIS: SPEC For questions and issues related to SPEC, contact beam line staff or send

296

Time and spectrum-resolving mutiphoton correlator for 300-900 nm  

E-Print Network (OSTI)

We demonstrate a single-photon sensitive spectrometer in the visible range, which allows us to perform time-resolved and multi-photon spectral correlation measurements. It is based on a monochromator composed of two gratings, collimation optics and an array of single photon avalanche diodes. The time resolution can reach $110$ ps and the spectral resolution is $2$ nm/pixel, limited by the design of the monochromator. This technique can easily be combined with commercial monochromators, and can be useful for joint spectrum measurements of two photons emitted in the process of parametric down conversion, as well as time-resolved spectrum measurements in optical coherence tomography or medical physics applications.

Johnsen, Kelsey D; Scarcella, Carmelo; Thibault, Marilyne; Tosi, Alberto; Jennewein, Thomas

2014-01-01T23:59:59.000Z

297

Time and spectrum-resolving mutiphoton correlator for 300-900 nm  

E-Print Network (OSTI)

We demonstrate a single-photon sensitive spectrometer in the visible range, which allows us to perform time-resolved and multi-photon spectral correlation measurements. It is based on a monochromator composed of two gratings, collimation optics and an array of single photon avalanche diodes. The time resolution can reach $110$ ps and the spectral resolution is $2$ nm/pixel, limited by the design of the monochromator. This technique can easily be combined with commercial monochromators, and can be useful for joint spectrum measurements of two photons emitted in the process of parametric down conversion, as well as time-resolved spectrum measurements in optical coherence tomography or medical physics applications.

Kelsey D. Johnsen; Piotr Kolenderski; Carmelo Scarcella; Marilyne Thibault; Alberto Tosi; Thomas Jennewein

2014-06-17T23:59:59.000Z

298

For more information, contact  

NLE Websites -- All DOE Office Websites (Extended Search)

Tao Hong, hongt@ornl.gov, 865.574.8659 Tao Hong, hongt@ornl.gov, 865.574.8659 Adam Aczel, aczelaa@ornl.gov, 865.978.0118 neutrons.ornl.gov/cg4c The US/Japan Cold Neutron Triple-Axis Spectrometer is a conventional triple-axis spectrometer with variable incident energy and variable monochromator-sample and sample-analyzer distances. The cold guide 4 bender and guide hall shielding reduce 4C's vertically focusing monochromator PG (002). To enhance accommodation of strong magnetic position and to simplify future polarization analysis, the amount of ferromagnetic material has been minimized in

299

The Current Performance of the Wide Range (90-2500 eV) Soft X-ray Beamline at the Australian Synchrotron  

SciTech Connect

The Soft X-ray beamline at the Australian synchrotron has been constructed around a collimated light Plane Grating Monochromator taking light from an Elliptically Polarized Undulator (EPU). The beamline covers a wide photon energy range between 90 to 2500 eV, using two gratings of 250 l/mm and 1200 l/mm. At present the output from the monochromator is directed into one branchline with a dedicated UHV endstation. The measured performance of the beamline in flux and resolution is shown to be very close to that of theoretical calculations.

Cowie, B. C. C.; Tadich, A.; Thomsen, L. [Australian Synchrotron, 800 Blackburn Road, Clayton, Victoria (Australia)

2010-06-23T23:59:59.000Z

300

Development of heavy mineral and heavy element database of soil sediments in Japan using synchrotron radiation X-ray powder diffraction and high-energy (116keV) X-ray fluorescence analysis: 1. Case study of Kofu and Chiba region  

Science Journals Connector (OSTI)

We have started the construction of a nationwide forensic soil sediment database for Japan based on the heavy mineral and trace heavy element compositions of stream sediments collected at 3024 points all over Japan obtained by high-resolution synchrotron X-ray powder diffraction (SR-XRD) and high-energy synchrotron X-ray fluorescence analysis (HE-SR-XRF). In this study, the performance of both techniques was demonstrated by analyzing soil sediments from two different geological regions, the Kofu and Chiba regions in Kanto province, to construct database that can be applied in the future to provenance analysis of soil evidence from a crime scene. The sediments from the quaternary volcanic lithology of the Chiba region were found to be dominated by heavy minerals of volcanic origin orthopyroxene, clinopyroxene, and amphibole, and the \\{REEs\\} (rare earth elements) within the region showed similar geochemical behavior. On the other hand, four distinct heavy mineral groups were identified in the sediments of the Kofu region, where there is a great variety of underlying bedrock, and the geochemical behavior of the \\{REEs\\} in the sediments also varied accordingly to their geological origins. As such, our study shows that high-resolution SR-XRD data can provide information on the spatial distribution patterns of heavy minerals in stream sediments, playing an important role in determining their likely geographical origin. Meanwhile, the highly sensitive HE-SR-XRF data allow us to study the geochemical behavior of trace heavy elements, especially the \\{REEs\\} in the sediments, providing additional support to further constrain the likely geographical origin of the sediments determined by heavy minerals.

Willy Shun Kai Bong; Izumi Nakai; Shunsuke Furuya; Hiroko Suzuki; Yoshinari Abe; Keiichi Osaka; Takuya Matsumoto; Masayoshi Itou; Noboru Imai; Toshio Ninomiya

2012-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Whole-genome sequencing analysis of phenotypic heterogeneity and anticipation in LiFraumeni cancer predisposition syndrome  

Science Journals Connector (OSTI)

...17/10) C57Bl6 p53-/- Male 3 months (liver) 53 12484 (5/16/10) 129SvSL p53+/+ Female 3 months (liver) 54 12776 (5/16/10) C57Bl6/129SvSL p53+/- embryo (17.5 embryo) 55 pup191 (5/16/10) C57Bl6/129SvSL p53+/- embryo...

Hany Ariffin; Pierre Hainaut; Anna Puzio-Kuter; Soo Sin Choong; Adelyne Sue Li Chan; Denis Tolkunov; Gunaretnam Rajagopal; Wenfeng Kang; Leon Li Wen Lim; Shekhar Krishnan; Kok-Siong Chen; Maria Isabel Achatz; Mawar Karsa; Jannah Shamsani; Arnold J. Levine; Chang S. Chan

2014-01-01T23:59:59.000Z

302

Exploring the Neutrinoless Double Beta Decay in the Inverted Neutrino Hierarchy with Bolometric Detectors  

E-Print Network (OSTI)

keV] Light [keV] Energy [keV] / ndf p0 p1 4.518e-05 Light Detector Light Thermometer Energy release S1_LvsH S1_LvsH Po c) smeared ? source Energy [keV] Light [

Artusa, D. R.

2014-01-01T23:59:59.000Z

303

CX-012247: Categorical Exclusion Determination | Department of...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

Determination CX-012247: Categorical Exclusion Determination Installation of Solar Photovoltaic Systems CX(s) Applied: A9, B5.16 Date: 06182014 Location(s): Wisconsin, Wisconsin...

304

CX-009004: Categorical Exclusion Determination | Department of...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

04: Categorical Exclusion Determination CX-009004: Categorical Exclusion Determination "Solar Panels on Hudson County Facilities CX(s) Applied: B5.16 Date: 08272012 Location(s):...

305

E-Print Network 3.0 - abolina solvita jermacane Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

and Agricultural Engineering, Texas A&M University Collection: Engineering ; Renewable Energy 5 16. Pollitz, F. F. Transient rheology of the uppermost mantle beneath the Mojave...

306

Download  

Science Journals Connector (OSTI)

Norw. North Polar. Exped., 1893-1896, Sci. Results 5(16): l-22. RODHE, W. 1955. Can plankton production pro- ceed during winter darkness in subarctic lakes?

1999-12-25T23:59:59.000Z

307

CX-010763: Categorical Exclusion Determination | Department of...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

CX-010763: Categorical Exclusion Determination Nevada Desert Research Institute- Photovoltaic Installation CX(s) Applied: B5.16 Date: 07172013 Location(s): Nevada...

308

E-Print Network 3.0 - adenoma sweat gland Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

5-16 Lines of cleavage... - sweat glands - nails 5-18 Functions of Hair? Prevents heat loss UV Protection Protect eyes Touch... found in dermis Sebaceous (oil)...

309

CX-009542: Categorical Exclusion Determination  

Energy.gov (U.S. Department of Energy (DOE))

Solar Parks Project CX(s) Applied: B5.16 Date: 11/09/2012 Location(s): Florida Offices(s): Golden Field Office

310

Theoretical analysis and experiments on antireflection coatings for laser diodes  

E-Print Network (OSTI)

was set on dB, the time constant ivas 100 ms, and the sensitivity was 10 mV. A special controller was designed and constructed to operate the monochromator and to provide a, voltage proportional to the grating position. The X-axis of the plotter ivas...

Chin, Kai Jian

1987-01-01T23:59:59.000Z

311

Influence of the Morphology and Porosity of n-Hexane Films on the Electron-Stimulated Luminescence and Desorption of Metastable Argon from Adsorbed Argon  

Science Journals Connector (OSTI)

Groupe du Conseil de Recherches Mdicales en Sciences des Radiations, Facult de Mdecine, Universit de Sherbrooke, Sherbrooke, Qubec, Canada J1H 5N4 ... The instrument consists of an electrostatic electron monochromator, a cryogenically cooled Pt(111) substrate, hemispherical LEED grids, and a position sensitive detector. ...

E. Vichnevetski; L. Sanche

1999-08-31T23:59:59.000Z

312

Spectral restoration and energy resolution improvement of electron energy-loss spectra by Pixon reconstruction: I. Principle and test examples  

Science Journals Connector (OSTI)

......spectrometer and energy filter for use in combination with 200 kV monochromated (S)TEMs. Ultramicroscopy 96: 367-384. 2 Overwijk M H F and Reefman D. (2000) Maximum-entropy deconvolution applied to electron energy-loss spectroscopy. Micron 31......

Shunsuke Muto; Richard C. Puetter; Kazuyoshi Tatsumi

2006-08-01T23:59:59.000Z

313

Towards 0.1 nm resolution with the first spherically corrected transmission electron microscope  

Science Journals Connector (OSTI)

......defocus-modulation image processing. Ultramiaysco/y'41: 323-333. means of an appropriate monochromator. 24 Thust A, Overwijk M H, Coene W M J, and Lentzen M (1996) M. Haider et al. Corrected electron microscope 405 Numerical correction of lenaberrations......

Maximilian Haider; Herald Rose; Stephan Uhlemann; Bernd Kabius; Knut Urban

1998-01-01T23:59:59.000Z

314

UHV piezoelectric translator  

SciTech Connect

A UHV compatible piezoelectric translator has been developed to correct for angular misalignments in the crysals of a UHV x-ray monochromator. The unit is small, bakeable to 150/sup 0/C, and uses only ceramic materials for insulation. We report on the construction details, vacuum compatibility, mechanical properties, and uses of the device.

Oversluizen, T.; Watson, G.

1985-01-01T23:59:59.000Z

315

Correction of Emission Crosstalk for FRET sensors By Teng-Leong Chew and Rex L. Chisholm  

E-Print Network (OSTI)

1 Correction of Emission Crosstalk for FRET sensors By Teng-Leong Chew and Rex L. Chisholm Excerpt. The superscript "y" can be replaced by "b" to indicate that the monochrome image has been background subtracted. For example: b dF represents a background-subtracted image of the donor fluorophore taken using the FRET

Goldman, Robert D.

316

Streaming speech3: a framework for generating and streaming 3D text-to-speech and audio presentations to wireless PDAs as specified using extensions to SMIL  

Science Journals Connector (OSTI)

While monochrome unformatted text and richly colored graphical content are both capable of conveying a message, well designed graphical content has the potential for better engaging the human sensory system. It is our contention that the author of an ... Keywords: 3D audio, PDA, SMIL, accessibility, location-based, mobile, spatialization, speech synthesis, streaming, wireless

Stuart Goose; Sreedhar Kodlahalli; William Pechter; Rune Hjelsvold

2002-05-01T23:59:59.000Z

317

Auger resonance study for the C1s 2pi* excitation of CO  

E-Print Network (OSTI)

monochromator resolution it is now possible to study the Auger spectra of diatomic molecules such as carbon monoxide (CO) in great detail. Our current study of CO, focuses on the computation of photoionization cross sections for the auger decay of CO after...

Botting, Shaleen Kaye

1997-01-01T23:59:59.000Z

318

Artificial Microfossils: Experimental Studies of Permineralization of Blue-Green Algae in Silica  

Science Journals Connector (OSTI)

...microorganisms are comparable to naturally occurring fossil algae...processes, comparable to naturally occuring fossil algae, information...are cotinparable to naturally occurring fossil algae...bars for 2 weeks; CuKa radiation with a LiF mono-chromator...

John H. Oehler; J. William Schopf

1971-12-17T23:59:59.000Z

319

Accurate radiometry from space: an essential tool for climate studies  

Science Journals Connector (OSTI)

...calibration system again consists of three instruments, although one...grating. We have chosen to use three monochromators, each optimized...sufficient accuracy, is a central pillar to achieving this goal. The...efforts to ensure long-term sustainability and growth within an ever-changing...

2011-01-01T23:59:59.000Z

320

Beam line instrumentation proposed by an ORAU/ORNL consortium for the VUV ring at NSLS  

Science Journals Connector (OSTI)

The beam line configuration and monochromators proposed jointly by a consortium of universities organized through Oak Ridge Associated Universities and by workers at Oak Ridge National Labs for installation at the National Synchrotron Light Source (NSLS) at Brookhaven are described. The proposed system is an adaptation of designs developed at Brookhaven for the VUV storage ring of NSLS.

T.A. Callcott; P.A. Carlson

1980-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

Mitochondrial Matrix Ca2+ Accumulation Regulates Cytosolic NAD+/NADH Metabolism, Protein Acetylation, and Sirtuin Expression  

Science Journals Connector (OSTI)

...12). Repetitive Ca2+ oscillations are commonly observed in...Spectral analysis of Ca2+ oscillations was measured as described...microscope equipped with a xenon arc lamp and DeltaRamX monochromator...Receptor-mediated Ca2+ oscillations stimulate mitochondrial Ca2...

Raluca Marcu; Brian M. Wiczer; Christopher K. Neeley; Brian J. Hawkins

2014-05-27T23:59:59.000Z

322

A Quantitative Analysis of Disk Drive Power Management in Portable Computers  

E-Print Network (OSTI)

the question of power management begins with an analysis of where the energy is being consumed. Table 1 gives) Percent of Total Display Compaq monochrome lite25c 3.5 68% Disk Drive (105 Mbytes) Maxtor MXL­105 III 1 of inactivity. In this paper, we perform a quantitative analysis of the potential costs and benefits of spinning

Anderson, Tom

323

Supporting Information for: Hyperspectral imaging of structure and composition in atomically thin heterostructures  

E-Print Network (OSTI)

The central mirror of a Schwarzschild objective obscures the central portion of the collected light cone (see. Light exiting the monochromator is focused with parabolic mirrors into a solarization a reflective (Schwarzschild) objective with an N.A. of 0.65, an effective magnification of ~100?, and spatial

McEuen, Paul L.

324

Number: Revision: A LS-OPS-0065  

E-Print Network (OSTI)

in the upstream and downstream sections when bleeding up the monochromator. II Section between UHV Vat Valve1 and Beryllium Window A. Bleed up 1. Notify the Coordinator ( Beeper 5824) 2. Close and seal NSLS UHV front end valve 3. Close and seal UHV Vat Valve 1 4. Coordinator places Yellow tag on UHV Vat valve 1 5. Hook up

Ohta, Shigemi

325

holger.lange@physik.tu-berlin.de Oviedo/Spain -September, 2008  

E-Print Network (OSTI)

micrographs were taken by a Philips CM200-FEG- UT operated at 200 kV. Low-frequency vibrational mode clearly at liquid helium temperatures with the 514 nm line of an Ar+ laser and a Dilor-XY triple monochromator system. Nanorods were characterized with high resolution transmission electron microscopy . HRTEM

Nabben, Reinhard

326

Tomato Fruit and Seed Colonization by Clavibacter michiganensis subsp. michiganensis through External and Internal Routes  

Science Journals Connector (OSTI)

...michiganensis subsp. michiganensis strains used in this study Strain County of origin Yr collected Voltage (kV/cm) a Transformation...0690-FS Rensselaer, NY 2006 12.5 16 (18) This study 0767-FS Oneida, NY 2007 7.5 16 (27) This study 11015-FS Albany, NY...

Matthew A. Tancos; Laura Chalupowicz; Isaac Barash; Shulamit Manulis-Sasson; Christine D. Smart

2013-09-06T23:59:59.000Z

327

The A.J. Goddard: Reconstruction and Material Culture of a Klondike Gold Rush Sternwheeler  

E-Print Network (OSTI)

Page 5.16 2 in. angle iron clamp underneath deck...................................................... 140 5.17 Hatch locations ........................................................................................... 141 5.18 Chain... Page 5.16 2 in. angle iron clamp underneath deck...................................................... 140 5.17 Hatch locations ........................................................................................... 141 5.18 Chain...

Thomas, Lindsey Hall

2012-10-19T23:59:59.000Z

328

Resonance Raman spectroscopy in Si and C ion-implanted double-wall carbon nanotubes  

E-Print Network (OSTI)

The effect of 170 keV Si and 100 keV C ion bombardment on the structure and properties of highly pure, double-wall carbon nanotubes has been investigated using resonance Raman spectroscopy. The implantations were performed ...

Dresselhaus, Mildred

329

Center for Nanophase Materials Sciences - Newsletter January...  

NLE Websites -- All DOE Office Websites (Extended Search)

is an exciting addition to our imaging and analytical capabilities. It operates in the energy range between 60keV and 120keV which makes it the optimum choice for observing...

330

eCopy, Inc.  

NLE Websites -- All DOE Office Websites (Extended Search)

20 keV undulator. The rods are mevable *** 62 2 tic lux i1e ef a hal ried ef a 20-keV REC undula e1.6 * Dimensiens are in cm. The drawing...

331

Molecular Depth Profiling of Sucrose Films: A Comparative Study...  

NLE Websites -- All DOE Office Websites (Extended Search)

Cs and O Ions. Abstract: Time-of-flight secondary ion mass spectrometry (ToF-SIMS) depth profiling of sucrose thin films were investigated using 10 keV C60+, 20 keV...

332

UNIVERSITY OF CALIFORNIA, Velocity-space resolved fast-ion measurements in the DIII-D tokamak  

E-Print Network (OSTI)

=2830ms with central ion temperature Ti=5keV and NBI injection energy Einj=80keV. Linear color scale function for the vertically-viewing FIDA system calculated for E =45keV. The minimum energy curve combination of gyro-angle, energy, and pitch to contribute to the measured spectrum at E . Figure 1.6. FIDA

Heidbrink, William W.

333

Internal conversion coefficients in (134)Cs, (137)Ba, and (139)La: A precise test of theory  

E-Print Network (OSTI)

Recently we measured the ratio of K-shell internal conversion coefficients, alpha(K), for the 127.5-keV E3 transition in (134)Cs and the 661.7-keV M4 transition in (137)Ba. We here report a measurement of the 165.9-keV M1 transition in (139)La...

Nica, N.; Hardy, John C.; Iacob, V. E.; Balonek, C.; Trzhaskovskaya, M. B.

2008-01-01T23:59:59.000Z

334

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

335

eCopy, Inc.  

NLE Websites -- All DOE Office Websites (Extended Search)

I~~~~bmjtted I~~~~bmjtted manuscript has been authored i' vi c. cor: ',actOr of the U. S. Government un02r contract No. W¥31-109-ENG-38. Accordingly, the U. S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or allow others to do so, for U. S. Government purposes. LS--238 High-Heat-Load Studies of Silicon and Diamond Monochromators Using the APS/CHESS Prototype Undulator D. M. Mills, W.-K Lee, R. K. Smither, and P. B. Fernandez Experimental Facilities Division September 16, 1994 Advanced Photon Source Argonne National Laboratory High-Heat-Load Studies of Silicon and Diamond Monochromators Using the APS/CHESS Prototype Undulator D.M. Mills, W.-K. Lee, R.K. Smither and P. B. Fernandez

336

eCopy, Inc.  

NLE Websites -- All DOE Office Websites (Extended Search)

he submitted manuscript has been authored he submitted manuscript has been authored ria contractor of the U. S. Government under contract No. W·31·10S-ENG·38. Accordingly. the U. S. Government retains a nonexclusive, royalty·free license to publish or reproduce the published form of this contribution, or allow others to do so~ for U. S. Government purposes. IDENTIFICATION OF ROOT CAUSE OF VIBRATION OF A LIQUID .. GALLIUM .. COOLED SILICON MONOCHROMATOR AND RECOMMENDATIONS FOR ABATEMENT by S. S. Chen, S. Zhu, M. W. Wambsganss, and J. A. J endrzejczyk Energy Technology Division W.K.Lee Experimental Facilities Division August 1994 Work supported by U. S. DEPARTMENT OF ENERGY Office of Basic Energy Sciences LS-240 IDENTIFICATION OF ROOT CAUSE OF VIBRATION OF A LIQUID .. GALlIUM .. COOLED SILICON MONOCHROMATOR AND

337

BL 11  

NLE Websites -- All DOE Office Websites (Extended Search)

BL 11-2 Status and Scheduling Information BL 11-2 Status and Scheduling Information Third Run 2001 BL 11-2 user commissioning is in full swing. March and April activities have centered around debugging and characterizing major electromechanical and optical systems of the beam line (motors, mirrors, and the 11-2 LN-cooled monochromator). We are now preparing for the upcoming run, of which 5 1/2 weeks are scheduled for user beam. Further commissioning work and new system testing will be interspersed between user beam periods. Notably, this work will include feasibility tests using metal microcapillary microfocusing optics (2 to 10 mm range) and system tests on the BL 11-2 grazing-incidence XAS spectrometer. Several instrumental capabilities are still in the process of being brought on-line. We anticipate that the BL 11-2 monochromator will

338

Beamline 9.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

9.0.2 Print 9.0.2 Print Chemical Dynamics Scientific disciplines: Chemical dynamics, aerosol chemistry, imaging mass spectrometry, chemical kinetics, laser ablation and clusters, combustion and flames. Endstations: Molecular-beam photoelectron/photoion imaging and spectroscopy Flame chamber Ablation chamber Aerosol chamber Kinetics chamber GENERAL BEAMLINE INFORMATION Operational Yes Source characteristics 10-cm period undulator (U10) (fundamental) Energy range 7.4-30 eV Undulator beam White beam (straight undulator beam) Calculated flux (1.9 GeV, 400 mA) 1016 photons/s, 2.5%BW Spot size at sample 170 (h) x 50 (v) µm Monochromator #1 3-m Off-plane Eagle Calculated flux (1.9 GeV, 400 mA) 1014 photons/s, 0.1%BW Spot size at sample 400 (h) x 350 (v) µm Monochromator #2 3-m Off-plane Eagle

339

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

340

Beamline 9.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Chemical Dynamics Scientific disciplines: Chemical dynamics, aerosol chemistry, imaging mass spectrometry, chemical kinetics, laser ablation and clusters, combustion and flames. Endstations: Molecular-beam photoelectron/photoion imaging and spectroscopy Flame chamber Ablation chamber Aerosol chamber Kinetics chamber GENERAL BEAMLINE INFORMATION Operational Yes Source characteristics 10-cm period undulator (U10) (fundamental) Energy range 7.4-30 eV Undulator beam White beam (straight undulator beam) Calculated flux (1.9 GeV, 400 mA) 1016 photons/s, 2.5%BW Spot size at sample 170 (h) x 50 (v) µm Monochromator #1 3-m Off-plane Eagle Calculated flux (1.9 GeV, 400 mA) 1014 photons/s, 0.1%BW Spot size at sample 400 (h) x 350 (v) µm Monochromator #2 3-m Off-plane Eagle

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

342

NCEM National Center for Electron Microscopy: Microscopes and Facilities:  

NLE Websites -- All DOE Office Websites (Extended Search)

LIBRA LIBRA The 200kV Zeiss monochromated LIBRA 200MC is designed to produce high contrast imaging for TEM and STEM and either convergent beam or parallel beam diffraction using Koehler illumination.In addition, the incorporation of a monochromator into the field emission gun enables energy resolution of ~0.15eV for electron energy loss spectroscopy. The dedicated in-column Omega Filter implemented in this microscope also can be used for both spectroscopic analysis and energy-filtered imaging with a 2048x2048 CCD camera. The high tilt capability of the stage and pole piece accepts various types of analytical holders.This microscope is optimized for soft materials applications that require either the high contrast imaging performance or analytical methods such as EF-TEM and STEM.( Instrument

343

BEAMLINE 13-2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 CURRENT STATUS Open RESPONSIBLE STAFF: Dan Brehmer Hirohito Ogasawara EXPERIMENTS: Photoemission; NEXAFS (see also: Spectroscopic Techniques) SCHEDULING: BL13 Schedules Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: Elliptically polarized undulator OPTICS: M0 vertical deflecting spherical, water-cooled M2 horizontal deflecting spherical M3 vertical deflecting elliptical MONOCHROMATOR: Spherical Grating Monochromator (SGM) SLITS : 0-1000 µm. Entrance slit cooled and movable ± 200 mm along optical axis GRATINGS : 3 water-cooled interchangeable HORIZONTAL ANGULAR ACCEPTANCE : 0.25 mrad ENERGY RANGE : 300 l/mm: 150 - 400 E/DE 10000 600 l/mm: 250 - 700 E/DE 10000 1100 l/mm: 500 - 1200 E/DE 10000 SPOT SIZE : 0.01 x 0.075 mm2

344

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

345

eCopy, Inc.  

NLE Websites -- All DOE Office Websites (Extended Search)

S~ Government S~ Government under contract No. W·31·10S-ENG·38. Accordingly, the U. S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or allow others to do so, for U. S. Government purposes. LS-250 High-Heat-Load Synchrotron Tests of Room-Temperature, Silicon Crystal Monochromators at the CHESS F-2 Wiggler Station W.-K. Lee, P. B. Fernandez, T. Graber, and L. Assoufid Experimental Facilities Division, APS September 8, 1995 Advanced Photon Source Argonne National Laboratory HIGH~HEATwLOAD SYNCHROTRON TESTS OF ROOM~ TEMPERATURE, SILICON CRYSTAL MONOCHROMATORS AT THE CHESS F-2 WIGGLER STATION W. K. Lee, P. B. Fernandez, T. Graber, and L. Assoufid Experimental Facilities Division

346

FCD Instrument Team | ORNL Neutron Sciences  

NLE Websites -- All DOE Office Websites (Extended Search)

The Four-Circle Diffractometer at HFIR The Four-Circle Diffractometer at HFIR HB-3A Four-Circle Diffractometer (HB-3A). The Four-Circle Diffractometer goniometer has a full χ circle with a 4.5-450 K closed-cycle helium refrigerator. The detector is 3He with a 7-anode array in a honeycomb pattern. Currently, only the center anode is used. The upper 2Θ limit is 155°. A multilayer-[110]-wafer silicon monochromator with the reflection from planes of the zone ensures sharp diffraction peaks in specified ranges of detector angles by control of the horizontal radius of curvature. Any plane from the zone can be set in Bragg position, but only the (331), (220) with (440), and (111) with (333) reflections are of practical interest. For the fixed monochromator angle of 48°, these reflections provide principal incident wavelengths of

347

BEAMLINE 11-3 Materials Diffraction  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 CURRENT STATUS: Open SUPPORTED TECHNIQUES: X-ray scattering Thin film diffraction MAIN SCIENTIFIC DISCIPLINES: Materials / Environmental / Biology % TIME GENERAL USE: 100% SCHEDULING: Proposal Submittal and Scheduling Procedures Current SPEAR and Beam Line Schedules SOURCE: 26-pole, 2.0-Tesla ID Side Station BEAM LINE SPECIFICATIONS: energy range resolution DE/E spot size flux angular acceptance focused 12735 eV ~5 x 10-4 3.1 x 0.15 mm Usable 0.15 x 0.15 mm OPTICS: Single-crystal Si, Rh-coated - vertically focusing mirror MONOCHROMATOR: Bent cube-root I_beam Si(311), Side deflecting Monochromator Crystal Glitch Library Crystal changes need to be scheduled and coordinated in advance with BL support staff. ABSORPTION: INSTRUMENTATION: Standard detector: MAR345 Imaging Plate - 345 mm

348

Beamline 9.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

9.0.2 Print 9.0.2 Print Chemical Dynamics Scientific disciplines: Chemical dynamics, aerosol chemistry, imaging mass spectrometry, chemical kinetics, laser ablation and clusters, combustion and flames. Endstations: Molecular-beam photoelectron/photoion imaging and spectroscopy Flame chamber Ablation chamber Aerosol chamber Kinetics chamber GENERAL BEAMLINE INFORMATION Operational Yes Source characteristics 10-cm period undulator (U10) (fundamental) Energy range 7.4-30 eV Undulator beam White beam (straight undulator beam) Calculated flux (1.9 GeV, 400 mA) 1016 photons/s, 2.5%BW Spot size at sample 170 (h) x 50 (v) µm Monochromator #1 3-m Off-plane Eagle Calculated flux (1.9 GeV, 400 mA) 1014 photons/s, 0.1%BW Spot size at sample 400 (h) x 350 (v) µm Monochromator #2 3-m Off-plane Eagle

349

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

350

Beamline 9.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

2 Print 2 Print Chemical Dynamics Scientific disciplines: Chemical dynamics, aerosol chemistry, imaging mass spectrometry, chemical kinetics, laser ablation and clusters, combustion and flames. Endstations: Molecular-beam photoelectron/photoion imaging and spectroscopy Flame chamber Ablation chamber Aerosol chamber Kinetics chamber GENERAL BEAMLINE INFORMATION Operational Yes Source characteristics 10-cm period undulator (U10) (fundamental) Energy range 7.4-30 eV Undulator beam White beam (straight undulator beam) Calculated flux (1.9 GeV, 400 mA) 1016 photons/s, 2.5%BW Spot size at sample 170 (h) x 50 (v) µm Monochromator #1 3-m Off-plane Eagle Calculated flux (1.9 GeV, 400 mA) 1014 photons/s, 0.1%BW Spot size at sample 400 (h) x 350 (v) µm Monochromator #2 3-m Off-plane Eagle

351

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

352

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

353

CTAX: the US/Japan Cold Neutron Triple-Axis Spectromete at HFIR | ORNL  

NLE Websites -- All DOE Office Websites (Extended Search)

CTAX-US/Japan Cold Neutron Triple-Axis Spectrometer CTAX-US/Japan Cold Neutron Triple-Axis Spectrometer CTAX US/Japan Cold Neutron Triple-Axis Spectrometer (CG-4C). (larger image) The U.S.-Japan Cold Neutron Triple-Axis Spectrometer (CTAX) is a conventional triple-axis spectrometer with variable incident energy and variable monochromator-sample and sample-analyzer distances. The cold guide 4 bender and guide hall shielding reduce background levels at CG-4C, and the 15-cm-tall guide profile is well exploited by CG-4C's vertically focusing monochromator (PG 002). To enhance accommodation of strong magnetic fields at the sample position and to simplify future polarization analysis, the amount of ferromagnetic material has been minimized in the construction of this instrument. CG-4C is a collaboration of Oak Ridge National Laboratory, the Neutron

354

Beamline 4.0.3  

NLE Websites -- All DOE Office Websites (Extended Search)

3 Print 3 Print High-resolution spectroscopy of complex materials (MERLIN) Endstations: MERIXS: High-resolution inelastic scattering ARPES: Angle-resolved photoemission spectroscopy GENERAL BEAMLINE INFORMATION Operational 2011 Source characteristics 9.0-cm-period quasiperiodic elliptical polarization undulator (EPU9) Energy range 9eV-120eV with current gratings Monochromator Variable-included-angle spherical grating monochromator (SGM) Calculated flux (1.9 GeV, 400 mA) 1012 photons/s/0.01%BW at 100 eV Resolving power (E/ΔE) High flux 1200 lines/mm; ~1/25,000 Endstations High-resolution inelastic scattering (MERIXS) and ARPES Characteristics Milli-Electron-volt Resolution beamLINe (MERLIN): Ultrahigh-resolution inelastic scattering and angle-resolved photoemission

355

Beamline 9.0.2  

NLE Websites -- All DOE Office Websites (Extended Search)

9.0.2 Print 9.0.2 Print Chemical Dynamics Scientific disciplines: Chemical dynamics, aerosol chemistry, imaging mass spectrometry, chemical kinetics, laser ablation and clusters, combustion and flames. Endstations: Molecular-beam photoelectron/photoion imaging and spectroscopy Flame chamber Ablation chamber Aerosol chamber Kinetics chamber GENERAL BEAMLINE INFORMATION Operational Yes Source characteristics 10-cm period undulator (U10) (fundamental) Energy range 7.4-30 eV Undulator beam White beam (straight undulator beam) Calculated flux (1.9 GeV, 400 mA) 1016 photons/s, 2.5%BW Spot size at sample 170 (h) x 50 (v) µm Monochromator #1 3-m Off-plane Eagle Calculated flux (1.9 GeV, 400 mA) 1014 photons/s, 0.1%BW Spot size at sample 400 (h) x 350 (v) µm Monochromator #2 3-m Off-plane Eagle

356

Performance of an optimally contact-cooled high-heat-load mirror at the APS.  

SciTech Connect

X-ray undulator beamlines at third-generation synchrotrons facilities use either a monochromator or a mirror as the first optical element. In this paper, the thermal and optical performance of an optimally designed contact-cooled high-heat-load x-ray mirror used as the first optical element on the 2ID undulator beamline at the Advanced Photon Source (APS) is reported. It is shown that this simple and economical mirror design can comfortably handle the high heat load of undulator beamlines and provide good performance with long-term reliability and ease of operation. Availability and advantages of such mirrors can make the mirror-first approach to high-heat-load beamline design an attractive alternative to monochromator-first beamlines in many circumstances.

Cai, Z.; Khounsary, A.; Lai, B.; McNulty, I.; Yun, W.

1998-11-18T23:59:59.000Z

357

Higher Order Suppressor (HOS) for the PolLux Microspectroscope Beamline at the Swiss Light Source SLS  

SciTech Connect

The mechanical design and performance of a device to suppress higher orders of a spherical grating monochromator at a constant deviation angle is described. The higher order suppressor (HOS) is used for a scanning transmission x-ray microspectroscope beamline (PolLux) at a bending magnet of the Swiss Light Source (SLS). The instruments allow microspectroscopy in polymer science, of biological samples in the water window as well as the study of magnetic materials with circular or linear polarized light in a photon energy range of 200 eV to 1400 eV. The HOS uses three mirrors acting as a low pass filter for soft x-rays to improve the absorption spectroscopy of carbon, oxygen and nitrogen 1s core levels. The successful installation and operation of the HOS located after the monochromator is reported. First results obtained using samples from materials research and environmental sciences exemplify the improved spectroscopy capabilities of the instrument.

Frommherz, U.; Stefani, R.; Ellenberger, U. [Paul Scherrer Institut, Division of Mechanical Engineering Sciences, 5232 Villigen PSI (Switzerland); Raabe, J.; Watts, B. [Paul Scherrer Institut, Swiss Light Source, 5232 Villigen PSI (Switzerland)

2010-06-23T23:59:59.000Z

358

High resolution ion Doppler spectroscopy at Prairie View Rotamak  

SciTech Connect

A fast ion Doppler spectroscopy (IDS) diagnostic system is installed on the Prairie View Rotamak to measure ion temperature and plasma flow. The diagnostic employs a single channel photomultiplier tube and a Jarrell-Ash 50 monochromator with a diffraction grating line density of 1180 lines/mm, which allows for first order spectra of 200-600 nm. The motorized gear of the monochromator allows spectral resolution of 0.01 nm. Equal IDS measurements are observed for various impurity emission lines of which carbon lines exhibit stronger intensities. Furthermore, the diagnostics is examined in an experiment where plasma experiences sudden disruption and quick recovery. In this case, the IDS measurements show {approx}130% increase in ion temperature. Flow measurements are shown to be consistent with plasma rotation.

Houshmandyar, Saeid; Yang Xiaokang [Solar Observatory Department, Prairie View A and M University, Prairie View, Texas 77446 (United States); Magee, Richard [Department of Physics, West Virginia University, Morgantown, West Virginia 26506 (United States)

2012-10-15T23:59:59.000Z

359

An adaptive crystal bender for high power synchrotron radiation beams  

SciTech Connect

Perfect crystal monochromators cannot diffract x-rays efficiently, nor transmit the high source brightness available at synchrotron radiation facilities, unless surface strains within the beam footprint are maintained within a few arcseconds. Insertion devices at existing synchrotron sources already produce x-ray power density levels that can induce surface slope errors of several arcseconds on silicon monochromator crystals at room temperature, no matter how well the crystal is cooled. The power density levels that will be produced by insertion devices at the third-generation sources will be as much as a factor of 100 higher still. One method of restoring ideal x-ray diffraction behavior, while coping with high power levels, involves adaptive compensation of the induced thermal strain field. The design and performance, using the X25 hybrid wiggler beam line at the National Synchrotron Light Source (NSLS), of a silicon crystal bender constructed for this purpose are described.

Berman, L.E.; Hastings, J.B.

1992-01-01T23:59:59.000Z

360

1993 CAT workshop on beamline optical designs  

SciTech Connect

An Advanced Photon Source (APS) Collaborative Access Team (CAT) Workshop on Beamline Optical Designs was held at Argonne National Laboratory on July 26--27, 1993. The goal of this workshop was to bring together experts from various synchrotron sources to provide status reports on crystal, reflecting, and polarizing optics as a baseline for discussions of issues facing optical designers for CAT beamlines at the APS. Speakers from the European Synchrotron Radiation Facility (ESRF), the University of Chicago, the National Synchrotron Light Source, and the University of Manchester (England) described single- and double-crystal monochromators, mirrors, glass capillaries, and polarizing optics. Following these presentations, the 90 participants divided into three working groups: Crystal Optics Design, Reflecting Optics, and Optics for Polarization Studies. This volume contains copies of the presentation materials from all speakers, summaries of the three working groups, and a ``catalog`` of various monochromator designs.

Not Available

1993-11-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

An adaptive crystal bender for high power synchrotron radiation beams  

SciTech Connect

Perfect crystal monochromators cannot diffract x-rays efficiently, nor transmit the high source brightness available at synchrotron radiation facilities, unless surface strains within the beam footprint are maintained within a few arcseconds. Insertion devices at existing synchrotron sources already produce x-ray power density levels that can induce surface slope errors of several arcseconds on silicon monochromator crystals at room temperature, no matter how well the crystal is cooled. The power density levels that will be produced by insertion devices at the third-generation sources will be as much as a factor of 100 higher still. One method of restoring ideal x-ray diffraction behavior, while coping with high power levels, involves adaptive compensation of the induced thermal strain field. The design and performance, using the X25 hybrid wiggler beam line at the National Synchrotron Light Source (NSLS), of a silicon crystal bender constructed for this purpose are described.

Berman, L.E.; Hastings, J.B.

1992-10-01T23:59:59.000Z

362

Radiocarbon dating of a pictograph and a shell mask gorget  

E-Print Network (OSTI)

the general location of cave shelter 41VV75. . An example of a Pecos River style pictograph (Panther Cave site 41VV83). , 12 An example of a Red Linear style pictograph. . . . . 14 An example of a Red Monochrome style pictograph (41VV699) . . 16..., darts, fending sticks, and pouches hanging from their elbows. Also, serpents and panthers are recurring themes in this style of pictograph. Images are usually static figures, frontally posed shamanistic figures and panthers in profile, The pictographs...

Pace, Mary Fairfax Nichols

2012-06-07T23:59:59.000Z

363

The new very small angle neutron scattering spectrometer at Laboratoire Leon Brillouin  

E-Print Network (OSTI)

The design and characteristics of the new very small angle neutron scattering spectrometer under construction at the Laboratoire Leon Brillouin is described. Its goal is to extend the range of scattering vectors magnitudes towards 2x10{-4} /A. The unique feature of this new spectrometer is a high resolution two dimensional image plate detector sensitive to neutrons. The wavelength selection is achieved by a double reflection supermirror monochromator and the collimator uses a novel multibeam design.

Sylvain Desert; Vincent Thevenot; Julian Oberdisse; Annie Brulet

2007-06-12T23:59:59.000Z

364

Compact, self-contained optical spectrometer  

SciTech Connect

We describe the construction and performance of a self-contained, battery-operated, hand-held optical spectrometer. This unit contains an on-board optical excitation source, miniaturized monochromator, CCD detector, Peltier cooler, LCD display module, and microprocessor control. We demonstrate capabilities for qualitative fluorescence determinations and semiquantitative fluorescence and absorption measurements. Resolution is {lambda}/{delta}{lambda}{approx_equal}1200 at 434 nm. {copyright} {ital 1995 Society for Applied Spectroscopy.}

Baird, W.; Nogar, N.S. [Chemical Sciences and Technology, CST-1 MSJ565, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

1995-11-01T23:59:59.000Z

365

X-ray instrumentation for protein crystallography with SR (abstract)  

SciTech Connect

The station is intended for x-ray analysis of single crystals, primarily that of proteins with the beam of synchrotron radiation from the superconducting wiggler of a special storage ring {ital E}=2.0 GeV, {ital I}=0.3 A in the town of Zelenograd (TNK).{sup 1} The dimensions of the radiation source are 2.35{sup 2} {sigma}{sub {ital x}}{center dot}{sigma}{sub {ital z}}=1.5{times}0.05 mm{sup 2}, the brightness for {lambda}=1.5 A is 10{sup 15} photon/(s mm{sup 2} mrad.{sup 2} 0.1% ({Delta}{lambda}/{lambda})). The station comprises the device forming the monochromatized primary beam ({lambda}=0.5--2.2 A, {Delta}{lambda}/{lambda}{sup {minus}3}{similar to}10{sup {minus}4}) that consists of an asymmetric focusing monochromator with triangular-shaped Si or Ge crystal curved as a round cylinder,{sup 2} a segmented mirror of total external reflection placed behind the monochromator on a rotating bench consisting of 8 flat glass 200{times}50{times}25 mm{sup 2} segments that form a surface imitating an elliptical cylinder, three pairs of horizontal and vertical slits, monitor--ionization chamber, four-circle diffractometer with scintillation counter and horizontal main axis placed on the adjustable carriage that can turn about the monochromator axis; position-sensitive proportional chamber with spherical drift space, 512{times}512 elements of space resolution and time resolution of 10{sup 6} photons per second that can be vertically shifted and bent around the holder horizontal axis. The monochromator goniometer as well as the crystal bend and the mirror segments are driven by the multiple-turn potientiometers by the computer and CAMAC interface.

Popov, A.N.; Kheiker, D.M.; Harutunyan, E.G. (Institute of Crystallography of the USSR Academy of Sciences, Leninsky Prospect 59, Moscow, 117333 (USSR))

1992-01-01T23:59:59.000Z

366

Large-Area Zone Plate Fabrication with Optical Lithography  

SciTech Connect

Zone plates as condenser optics for x-ray microscopes offer simple optical designs for both illumination and spectral resolution when used as a linear monochromator. However, due to the long write times for electron beam lithography, both the availability and the size of zone plates for condensers have been limited. Since the resolution provided by the linear monochromator scales almost linearly with the diameter of the zone plate, the full potential for zone plate monochromators as illumination systems for x-ray microscopes has not been achieved. For example, the 10-mm-diameter zone plate has demonstrated a spectral resolution of E/{Delta}E = 700[1], but with a 26-mm-diameter zone plate, the calculated spectral resolution is higher than E/{Delta}E = 3000. These large-area zone plates are possible to fabricate with the leading edge semiconductor lithography tools such as those available at the College of Nanoscale Science and Engineering at the University at Albany. One of the lithography tools available is the ASML TWINSCAN XT: 1950i with 37-nm resolution [2]. A single 300-mm wafer can contain more than 60 fields, each with a large area condenser, and the throughput of the tool can be more than one wafer every minute.

Denbeaux, G. [College of Nanoscale Science and Engineering, University at Albany, 255 Fuller Road, Albany, NY 12203 (United States)

2011-09-09T23:59:59.000Z

367

Evidence for O+ and 1- Levels in U234 Populated in the One-Minute Beta Decay of Pa234  

Science Journals Connector (OSTI)

A directional correlation measurement has been performed on the 250-kev vs (751+795)-kev composite cascade in U234 following the 24-day beta decay of Th234 and the subsequent one-minute beta decay of Pa234. The "770"-kev (751+795 kev) composite photopeak spectrum coincident with the 250-kev gamma ray was displayed on a multichannel pulse-height analyzer for different positions of the scintillation counters. From these spectra the directional correlations between the 250-kev gamma ray and the lower and upper sides of the 770-kev composite line were measured. The results together with other measurements are consistent with assignments of multipolarity E1 to the 250-, 751-, and 795-kev gamma rays and spin and parity assignments 0+-1--2+ and 0+-1--0+ to the levels involved in the 250-751 kev and 250-795 kev gamma-gamma cascades, respectively. Thus new levels are proposed at 795 and 1046 kev with spin and parity 1- and 0+, respectively.

G. T. Wood

1960-09-15T23:59:59.000Z

368

Global Climate Change and National Security  

E-Print Network (OSTI)

5/16/2014 1 Global Climate Change and National Security RADM Jon White Oceanographer and Navigator months. · Oil, gas, and mineral resource exploitation expected to continue · Production/transportatio n

Howat, Ian M.

369

CX-012109: Categorical Exclusion Determination | Department of...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

Categorical Exclusion Determination CX-012109: Categorical Exclusion Determination Solar Energy Parking Canopy Demonstration Project CX(s) Applied: A9, B1.15, B5.16 Date: 0505...

370

CX-010269: Categorical Exclusion Determination  

Energy.gov (U.S. Department of Energy (DOE))

Renewable Energy Initiatives for Clark County, Nevada CX(s) Applied: A9, B5.16 Date: 05/16/2013 Location(s): Nevada Offices(s): Golden Field Office

371

Integrating Zooarchaeology and Modeling: Trans-Holocene Fishing in Monterey Bay, California  

E-Print Network (OSTI)

242 Table 5.16. Radiocarbon dates from SCR-Recovery Excavations at CA-SCR-60/130 for the Pajaro Valleyis the Scotts Valley site, SCR-177. It may date to 9500 BC [

Boone, Cristie

2012-01-01T23:59:59.000Z

372

CX-009007: Categorical Exclusion Determination | Department of...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

CX-009007: Categorical Exclusion Determination "Northeast Provider of Solar Photovoltaic Instructor Training CX(s) Applied: A9, A11, B5.16 Date: 08082012 Location(s): New...

373

CX-012014: Categorical Exclusion Determination  

Office of Energy Efficiency and Renewable Energy (EERE)

Deployable Commercial Rooftop Solar Electric System CX(s) Applied: A9, B3.6, B5.16 Date: 04/17/2014 Location(s): New York Offices(s): Golden Field Office

374

CX-010256: Categorical Exclusion Determination  

Energy.gov (U.S. Department of Energy (DOE))

Sherwood Valley Rancheria of Pomo Indians CX(s) Applied: B5.16 Date: 04/18/2013 Location(s): California Offices(s): Golden Field Office

375

E-Print Network 3.0 - arkadi ebber veiko Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

Annette Ebbers-Baumann1 , Ansgar Grune1... of Computer Science I, D-53117 Bonn, Germany ebbers, gruene, rolf.klein@cs.uni-bonn.de 2 University of Bonn... , pp. 5-16, 2005....

376

CX-010509: Categorical Exclusion Determination | Department of...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Exclusion Determination CX-010509: Categorical Exclusion Determination Plug & Play Solar Photovoltaic for American Homes CX(s) Applied: A9, B3.6, B5.16 Date: 06102013...

377

1999 Well Installation Report, Project Shoal Area, Churchill...  

Office of Legacy Management (LM)

. . . . . . . . . . . . . . . 5-14 5-10 Well HC-8 Tritium Activities During DevelopmentTest Pumping . . . . . . . . . . . . 5-16 5-11 Well HC-8 Summary of Drilling Parameters . ....

378

Intracellular Mechanisms of Adult Neural Progenitor Proliferation and Self-Renewal  

E-Print Network (OSTI)

Appl Biochem 40:5-16. 44. Peltier J, Schaffer DV. (2010).death. Nature 411:42-43. 49. Peltier J, O'Neill A, Schafferaccepted for publication as Peltier J, ONeill A, Schaffer

Peltier, Joseph Charles

2010-01-01T23:59:59.000Z

379

Co-infection with Schistosoma haematobium modulates the gene expression profile of malaria infection in schoolchildren in Gabon  

Science Journals Connector (OSTI)

We undertook a prospective study of schoolchildren aged 5-16 in an area endemic for schistosomiasis near Lambarn in Gabon. 425 children were recruited and demographic data...P. falciparum malaria infection (thi...

Katie Ewer; Julius Muller; Marielle Haks; Marguerite Massinga Loembe

2014-09-01T23:59:59.000Z

380

CX-007424: Categorical Exclusion Determination | Department of...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Exclusion Determination CX-007424: Categorical Exclusion Determination City of Houston Wind Project CX(s) Applied: B5.16, B5.18 Date: 12132011 Location(s): Texas Offices(s):...

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Potential Energy Savings and CO2 Emissions Reduction of China's Cement Industry  

E-Print Network (OSTI)

5.16 EJ in 2009. Primary energy consumption This article wasconsumption (EJ) Primary energy consumption Figure 2. Chinathat Chinas total primary energy consumption will rise

Ke, Jing

2013-01-01T23:59:59.000Z

382

CX-008596: Categorical Exclusion Determination  

Energy.gov (U.S. Department of Energy (DOE))

Northeast Provider of Solar Instructor Training - North CX(s) Applied: A9, A11, B5.16 Date: 07/16/2012 Location(s): Maine Offices(s): Golden Field Office

383

CX-010251: Categorical Exclusion Determination  

Energy.gov (U.S. Department of Energy (DOE))

University of Louisville- Sustainable Buildings CX(s) Applied: B1.15, B5.16, B5.17 Date: 03/20/2013 Location(s): Kentucky Offices(s): Golden Field Office

384

A Low-Carbon Fuel Standard for California, Part 1: Technical Analysis  

E-Print Network (OSTI)

biofuel) and bio-based and FT diesel fuels are indicated,Diesel Bio-Diesel Hydrogen Electric Figure 5-6: Fuel energyDiesel Bio-Diesel Hydrogen Electric Figure 5-16: Fuel energy

Farrell, Alexander E.; Sperling, Dan

2007-01-01T23:59:59.000Z

385

Foundations of Computer Science (Semester 2) 2014 Assessed Exercise Sheet 6 10% of Continuous Assessment Mark  

E-Print Network (OSTI)

this are said to be stable. For each of Bubble Sort, Insertion Sort, and Selection Sort say whether affect the stability of a Treesort algorithm based on it. Question 5 (16 marks) Sort the array [21, 26

Bullinaria, John

386

CX-008988: Categorical Exclusion Determination | Department of...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Categorical Exclusion Determination "The Institute for Energy, Environment, and Sustainability CX(s) Applied: A9, B5.16 Date: 08152012 Location(s): Kansas Offices(s): Golden...

387

The Radiations of Th231 (UY)  

Science Journals Connector (OSTI)

?-ray spectrum studies on a double-lens spectrometer of the electron spectrum of UY revealed a complex spectrum with three beta-components of 302 kev (44 percent), 216 kev (11 percent), and 94 kev (45 percent), and numerous conversion lines assignable to gammas of 22, 59, 63, 85, 122, 167, and 208 kev, each of these except the 122 kev also observed directly as gammas in a scintillation spectrometer. There is also evidence for a 107- and for a 230-kev gamma-ray. The samples were separated carrier-free from isotopically pure U235 (99.86 percent) by solvent extraction. A decay scheme is presented which gives a total disintegration energy of 324 kev.

Melvin S. Freedman; Arthur H. Jaffey; Frank Wagner; Jr.; Jack May

1953-01-01T23:59:59.000Z

388

Results of a Si/CdTe Compton Telescope  

E-Print Network (OSTI)

We have been developing a semiconductor Compton telescope to explore the universe in the energy band from several tens of keV to a few MeV. We use a Si strip and CdTe pixel detector for the Compton telescope to cover an energy range from 60 keV. For energies above several hundred keV, the higher efficiency of CdTe semiconductor in comparison with Si is expected to play an important role as an absorber and a scatterer. In order to demonstrate the spectral and imaging capability of a CdTe-based Compton Telescope, we have developed a Compton telescope consisting of a stack of CdTe pixel detectors as a small scale prototype. With this prototype, we succeeded in reconstructing images and spectra by solving the Compton equation from 122 keV to 662 keV. The energy resolution (FWHM) of reconstructed spectra is 7.3 keV at 511 keV and 3.1 keV at 122 keV, respectively. The angular resolution obtained at 511 keV is measured to be 12.2 degree (FWHM).

Kousuke Oonuki; Takaaki Tanaka; Shin Watanabe; Shin'ichiro Takeda; Kazuhiro Nakazawa; Takefumi Mitani; Tadayuki Takahashi; Hiroyasu Tajima; Yasushi Fukazawa; Masaharu Nomachi

2005-09-21T23:59:59.000Z

389

The Relative Probabilities and Absolute Cross Sections of the D D Reactions  

Science Journals Connector (OSTI)

Measurements with a gas target have been made of the relative probabilities and absolute cross sections of the two possible D D reactions, by simultaneously counting the helium and hydrogen nuclei produced by the reactions. The counters were separated from the target by a thin silica window. The ratio of the cross section of the neutron-producing reaction to that of the proton-producing reaction was found to increase from 0.95 at 120 kev to 1.06 at 250 kev. The "neutron" cross section was 0.019 barn at 120 kev and 0.038 barn at 250 kev while the "proton" cross section increased from 0.020 barn at 120 kev to 0.049 barn at 300 kev. The results can be fitted to an expression of the form ?E=?alPl and the values of the coefficients al are given.

K. G. McNeill and G. M. Keyser

1951-02-15T23:59:59.000Z

390

Re-publication of the data from the BILL magnetic spectrometer: The cumulative $?$ spectra of the fission products of $^{235}$U, $^{239}$Pu, and $^{241}$Pu  

E-Print Network (OSTI)

In the 1980s, measurements of the cumulative $\\beta$ spectra of the fission products following the thermal neutron induced fission of $^{235}$U, $^{239}$Pu, and $^{241}$Pu were performed at the magnetic spectrometer BILL at the ILL in Grenoble. This data was published in bins of 250 keV. In this paper, we re-publish the original data in a binning of 50 keV for $^{235}$U and 100 keV for $^{239}$Pu and $^{241}$Pu.

N. Haag; W. Gelletly; F. von Feilitzsch; L. Oberauer; W. Potzel; K. Schreckenbach; A. A. Sonzogni

2014-05-14T23:59:59.000Z

391

THE BURSTY NATURE OF SOLAR FLARE X-RAY EMISSION. II. THE NEUPERT EFFECT  

SciTech Connect

We carry out a novel statistical test of the Neupert effect based on multifractal spectra. The multifractal spectrum is the number distribution of the strengths (i.e., the Hlder exponents) of bursts in a signal. This is tested on simulations and carried out on RHESSI X-ray data from a well observed GOES X4.8 magnitude flare. The multifractal spectra is ideally suited to quantifying the relative smooth and bursty signals typically found in (thermal) soft X-ray and (non-thermal) hard X-ray data of solar flares. We show that light curves from all energies between 3 keV and 25 keV are statistically similar, suggesting that all these signals are dominated by the same (presumably thermal) emission. Emission lying between 25 keV and 100 keV probably contains some contribution from both thermal and non-thermal sources. The multifractal spectrum of a signal and that of its (cumulative) temporal integration are statistically similar (i.e., low residuals upon subtraction), but shifted by one in the peak Hlder exponent. We find the pairs of 3-6 keV and 100-300 keV emissions, the 6-12 keV and 100-300 keV emissions and the 12-25 keV and 100-300 keV emissions are all consistent with the Neupert effect. The best agreement with the Neupert effect is between the 12-25 keV and 100-300 keV pair, although possibly with some secondary source of thermal emission present.

McAteer, R. T. James [Department of Astronomy, New Mexico State University, MSC 4500, NM 88003-8001 (United States); Bloomfield, D. Shaun, E-mail: mcateer@nmsu.edu [Astrophysics Research Group, School of Physics, Trinity College Dublin, College Green, Dublin 2 (Ireland)

2013-10-20T23:59:59.000Z

392

DETERMINATION AND CHARACTERIZATION OF DEEP LEVELS IN p-CdTe(Cl)  

E-Print Network (OSTI)

photons de 122 keV (57Co) et de 5 keV pour des photons de 59 keV (241Am). Abstract. 2014 CdTe single doped CdTe single crystals grown from tellurium solvent have a good resolution for gamma-rays, when. The investigation of the energy levels system of charged centres in CdTe, as well as in other II-VI compounds

Paris-Sud XI, Université de

393

Columbia University X-Ray Measurements  

E-Print Network (OSTI)

V-720 keV · NaI 2x2x2" detector views an energy range of 1 keV-3 MeV Store signal in the tree. computer configuration. Plasmas were created using multi-frequency ECRH, and we find that most of the plasma energy is stored in the fast electrons. The energy spectrum of the x-ray emission below 740 keV is measured

394

RHESSI and SphinX Common Observations  

E-Print Network (OSTI)

) energy range: 3-8 keV (16 energy bands, E=0.3 keV) #12;Fluxes comparison SphinX DRM conversion factors possible. In 2009 we had three instruments that observed the Sun in similar energy band: SphinX, RHESSI, design & manufacture - energy range: 1.2 ­ 15 keV - time resolution: ~0.00001 s - sensitivity: 100x

Mrozek, Tomasz

395

First Hot Electron Measurements in Near-ignition Scale Hohlraums on the National Ignition Facility  

SciTech Connect

On the National Ignition Facility (NIF), the hot electrons generated in laser heated hohlraums are inferred from the >20 keV bremsstrahlung emission measured with the FFLEX broadband spectrometer. New high energy (>200 keV) time resolved channels were added to meet requirements for ignition and to infer the generated >170 keV hot electrons that can cause ignition capsule preheat. First hot electron measurements in near ignition scaled hohlraums heated by 96-192 NIF laser beams are presented.

Dewald, E L; Suter, L J; Thomas, C; Hunter, S; Meeker, D; Meezan, N; Glenzer, S H; Bond, E; Kauffman, R L; Kilkenny, J; Landen, O

2009-10-08T23:59:59.000Z

396

Hot electron measurements in ignition relevant Hohlraums on the National Ignition Facility  

SciTech Connect

On the National Ignition Facility (NIF), hot electrons generated in laser heated Hohlraums are inferred from the >20 keV bremsstrahlung emission measured with the time integrated FFLEX broadband spectrometer. New high energy (>200 keV) time resolved channels were added to infer the generated >170 keV hot electrons that can cause ignition capsule preheat. First hot electron measurements in near ignition scaled Hohlraums heated by 96-192 NIF laser beams are presented.

Dewald, E. L.; Thomas, C.; Hunter, S.; Divol, L.; Meezan, N.; Glenzer, S. H.; Suter, L. J.; Bond, E.; Celeste, J.; Bradley, D.; Bell, P.; Kauffman, R. L.; Landen, O. L. [Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550 (United States); Kline, J. L. [Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States); Kilkenny, J. [General Atomics, P.O. Box 85608, San Diego, California 92186 (United States)

2010-10-15T23:59:59.000Z

397

NIVEAUX EXCITS DU 50Sn11666 Par J. COLARD (*), P. GEPTS (**), L. GRENACS, A. JONES (***)  

E-Print Network (OSTI)

électrons de conversion externe ont été obtenus par effet photoélectrique dans une feuille d'uranium naturel transition de 1 756 keV. La méthode des conversions internes indique pour le niveau de 2 535 keV J = 4 et la the existence of the 1 756 keV transition. The internal conversion method indicates J = 4 and positive parity

Paris-Sud XI, Université de

398

Generating X-ray lines from annihilating dark matter  

E-Print Network (OSTI)

We propose different scenarios where a keV dark matter annihilates to produce a monochromatic signal. The process is generated through the exchange of a light scalar of mass of order 300 keV - 50 MeV coupling to photon through loops or higher dimensional operators. For natural values of the couplings and scales, the model can generate a gamma-ray line which can fit with the recently identified 3.5 keV X-ray line.

Emilian Dudas; Lucien Heurtier; Yann Mambrini

2014-05-08T23:59:59.000Z

399

Astronomy & Astrophysics manuscript no. h3933 December 20, 2002 (DOI: will be inserted by hand later)  

E-Print Network (OSTI)

.1+2221 and 1SAX J0618.0+2227) and a harder component up to 100 keV, indicating that a synchroton origin

400

E-Print Network 3.0 - annihilation coincidence peak Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

peak is seen at 3375 keV with 6000... . the annihilation spectra from the polyethylene and gold tar- ... Source: Golovchenko, Jene A. - Department of Physics, Harvard...

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

Using RSI format  

NLE Websites -- All DOE Office Websites (Extended Search)

first results of charge exchange recombination spectroscopy CHERS and motional Stark effect MSE measurements in the Madison Symmetric Torus reversed field pinch. A 30 keV,...

402

Gamma-ray lifetimes for parity doublets in K41, Ca41  

Science Journals Connector (OSTI)

Lifetimes have been measured by direct timing for the 1582 keV, 32- level of K41(?<38 ps) and the 2010 keV, 32+ level of Ca41(?=73018 ps). These levels are members of closely spaced parity doublets. The sensitivity of measurements to determine the parity mixing within these doublets is discussed.NUCLEAR REACTIONS K41(p,p?), Ex=1582 keV, measured ?; Ca40(d,p?), Ex=2010 keV, measured ?. Direct timing.

S. K. Saha; M. J. Maynard; B. C. Robertson; A. B. McDonald; E. D. Earle

1980-06-01T23:59:59.000Z

403

NEUTRAL BEAM INJECTOR RESEARCH AND DEVELOPMENT WORK IN THE USA  

E-Print Network (OSTI)

AND DEVELOPMENT WORK IN THE USA* R. V. Pylo, W. R. Baker, W.species 10 keV H beam us­ ing magnetic electron suppression

Pyle, R.V.

2011-01-01T23:59:59.000Z

404

Heliospheric shocks and sheaths John D. Richardson  

E-Print Network (OSTI)

wind speed. They have an initial thermal energy equal to the solar wind energy, about 1 keV. This paper

Richardson, John

405

Innovations in the design of mechanical components for a beamline -- The SRl`95 Workshop 2 summary  

SciTech Connect

The Synchrotron Radiation Instrumentation 1995 Conference (SRI`95) was hosted by the Advanced Photon Source (APS) at Argonne National Laboratory (ANL). Of the many workshops within the conference, the SRI`95 Workshop 2 was ``Innovations in the Design of Mechanical Components of a Beamline``. The workshop was attended well with over 140 registrants. The following topics were discussed. Industry`s perspective on the status and future was provided by Huber Diffrationtechnik, Oxford Instruments, and Kohzu Seiko Ltd. on goniometers/diffractometers, advanced manufacturing technique of high heat load components, such as the APS photon shutter, and the specialties of monochromators provided to the third-generation synchrotrons, respectively. This was followed by a description of the engineering of a dual function monochromator design for water-cooled diamond or cryogenically cooled silicon monochromators by CMC CAT/APS. Another category was the nagging problem of sensitivity of the photon beam position monitors (XBPM) to bending magnet radiation (``BM contamination``) and the undulator magnet gap changes. Problem descriptions and suggested solutions were provided by both the Advanced Light Source (ALS) and the APS. Other innovative ideas were the cooling schemes (enhanced cooling of beamline components using metallic porous meshes including cryo-cooled applications); Glidcop photon shutter design using microchannels at the ALS; and window/filter design, manufacture and operational experiences at CHESS and PETRA/HASYLAB. Additional discussions were held on designing for micromotions and precision in the optical support systems and smart user filter schemes. This is a summary of the presentations at the Workshop. 5 refs., 5 figs.

Kuzay, T.M. [Argonne National Lab., IL (United States); Warwick, T. [Lawrence Berkeley Lab., CA (United States)

1995-12-31T23:59:59.000Z

406

Characterization and calibration of compact array spectrometers in the ultraviolet spectral region  

SciTech Connect

Array-based spectrometers, with their compact size, low weight, low cost, and fast measurement time, are now frequently used in place of both conventional single-channel scanning monochromators, and broadband meters. Their rapid measurement capability makes them an attractive option for routine solar UV spectral measurements, where shortterm variability in signal is a challenge. However, compactness, portability, low cost and high speed are achieved at the expense of the spectrometer's optical and electronic performance. Thus such spectrometers are more prone to measurement error from environmental changes, and more prone to other intrinsic sources of error such as stray light and detector non-linearity, which significantly affect solar UV measurements, than a scanning monochromator. The effects of stray light and non-linearity can be reduced either by improved optical and detector design or by a detailed spectrometer characterization. We present in this paper our investigation of the performance of three different commercial array spectrometers: two mini-spectrometers, and a more elaborate array spectrometer with an on-board image amplifier device. These were tested for a subset of performance parameters: their wavelength accuracy and stability, electronic linearity, responsivity linearity, stray light sensitivity, and mechanical stability and repeatability. With all three spectrometers we found that these parameters, particularly but not limited to stray light, had a significant impact on the measurement of the incoming optical radiation. This meant that, without characterization, the instruments would be unable to accurately measure the UV component of any source with significant visible radiation. We discuss various simple and low-cost solutions for improving the performance of these instruments, and providing a rigorous calibration using a straightforward set-up including optical filters and the quasi-monochromatic light from a double monochromator.

Shindo, Francois [Measurement Standards Laboratory of New Zealand, Industrial Research, Lower Hutt (New Zealand); Woolliams, Emma; Scott, Barry; Harris, Subrena [National Physical Laboratory, Teddington (United Kingdom)

2013-05-10T23:59:59.000Z

407

SSRL HEADLINES Jan 2007  

NLE Websites -- All DOE Office Websites (Extended Search)

7 January, 2007 7 January, 2007 __________________________________________________________________________ Contents of this Issue: Science Highlight - Key Component of Malaria Parasite Invasion Motor Revealed Science Highlight - On the Role of Copper Regulation in a M. tuberculosis Repressor Science Highlight - Minding the Gaps: Explaining the Behavior of a High-Temperature Superconductor XAS Course for Structural Molecular Biology Applications in March New Hard X-ray Microscope Commissioned on Beam Line 6-2 Scanning the Microworld: SSRL's New Hard X-ray Microprobe Sagittal Focusing, LN-cooled Monochromator Installed on Beam Line 7-2 Workshop on New Directions in X-ray Scattering Photon Science Job Opportunities __________________________________________________________________________

408

Bacterial metabolite indole modulates incretin secretion from intestinal enteroendocrine L-cells  

E-Print Network (OSTI)

was used as a control measurement. The dish was mounted in a perfusion chamber on an Olympus IX71 microscope with x40 oil-immersion objective, and imaged using an Orca-ER CCD camera. A 75W Xenon arc lamp and a monochromator (Cairn Research) controlled... ) expressed on the plasma membrane of L-cells, enhancing L-cell number and secretion (Cani et al., 2013; Petersen et al., 2014; Plaisancie et al., 1995; Psichas et al., 2014; Tarini and Wolever, 2010; Tolhurst et al., 2012). Many other bacterial metabolites...

Chimerel, Catalin; Emery, Edward; Summers, David K.; Keyser, Ulrich; Gribble, Fiona M.; Reimann, Frank

2014-01-01T23:59:59.000Z

409

X-ray instrumentation for the photon factory  

SciTech Connect

The Photon Factory is one of the world's largest synchroton radiation light sources, the beam lines of which supply intense sources of vacuum UV, soft and hard X-rays. About 30 measuring instruments have been purpose-built, and this book describes the development and construction of the X-ray instrumentation. Given the multifunctional nature of the Photon Factory, it may be expected that the instrumentation serving it fulfills a variety of purposes including: reflection imaging systems; diffraction grating fabrication; monochromators; polarizers; analyzers; detectors; data collection systems; cameras; and goniometers.

Hosoya, S.; Iitaka, Y.; Hashizume, H.

1987-01-01T23:59:59.000Z

410

Plasmonic Dye-Sensitized Solar Cells Using Core?Shell Metal?Insulator Nanoparticles  

Science Journals Connector (OSTI)

Our spectroscopic investigation indicates that plasmon-enhanced photocarrier generation competes well with plasmons oscillation damping with in the first tens of femtoseconds following light absorption. ... The spectral response was measured using a 250 W xenon lamp filtered by a Princeton Instruments monochromator coupled to a Keithley 2636, both controlled by Labview and calibrated against a UV enhanced silicon reference diode. ... Probably in the same way as a laser generates stimulated emission of coherent photons, a spaser' could generate stimulated emission of surface plasmons (oscillations of free electrons in metallic nanostructures) in resonating metallic nanostructures adjacent to a gain medium. ...

Michael D. Brown; Teeraporn Suteewong; R. Sai Santosh Kumar; Valerio DInnocenzo; Annamaria Petrozza; Michael M. Lee; Ulrich Wiesner; Henry J. Snaith

2010-12-31T23:59:59.000Z

411

Xplot: XY plotting software for Sun Workstations  

SciTech Connect

A user friendly XY plotting package for Sun Workstations has been developed. Xplot is X-windows based and Open Look compliant. Running under an Open Look window manager, it supports the Drag Drop metaphor allowing the user to simply drag and drop a file icon into the plot window to create XY plots of multi-column ASCII data files. It supports color and monochrome PostScript hardcopy and re-sizeable windows. It has been designed to provide simple XY plots with minimal effort from the user. 7 figs.

Hess, B.V.

1991-06-01T23:59:59.000Z

412

The New Structural Materials Science Beamlines BL8A and 8B at Photon Factory  

SciTech Connect

BL8A and 8B are new beamlines for structural materials science at Photon Factory. The primary characteristics of both beamlines are similar. The incident beam is monochromatized by the Si(111) double-flat crystal monochromator and focused at the sample position by a Rh-coated bent cylindrical quartz mirror. The Weissenberg-camera-type imaging-plate (IP) diffractometers were installed. The X-ray diffraction experiments for structural studies of strongly correlated materials, such as transition metals, molecular conductors, endohedral fullerenes, nano-materials, etc, are conducted at these stations.

Nakao, A.; Sugiyama, H.; Koyama, A.; Watanabe, K. [Insttitute of Materials Science, High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki 305-0801 (Japan)

2010-06-23T23:59:59.000Z

413

The X-ray microscopy beamline UE46-PGM2 at BESSY  

SciTech Connect

The Max Planck Institute for Metal Physics in Stuttgart and the Helmholtz Center Berlin operate a soft X-ray microscopy beamline at the storage ring BESSY II. A collimated PGM serves as monochromator for a scanning X-ray microscope and a full field X-ray microscope at the helical undulator UE46. The selection between both instruments is accomplished via two switchable focusing mirrors. The scanning microscope (SM) is based on the ALS STXM microscope and fabricated by the ACCEL company. The full field microscope (FFM) is currently in operation at the U41-SGM beamline and will be relocated to its final location this year.

Follath, R.; Schmidt, J. S. [Helmholtz-Center Berlin, Albert-Einstein-Strasse 15, 12489 Berlin (Germany); Weigand, M. [Max Planck Institute for Metals Research, Heisenbergstrasse 3, 70569 Stuttgart (Germany); Fauth, K. [University Erlangen, Experimental Physics 4, Am Hubland, 97074 Wuerzburg (Germany)

2010-06-23T23:59:59.000Z

414

A KB-Focusing Mirror Pair for a VUV-Raman Spectrometer at FLASH - Mirror Metrology and Ray Tracing Results  

SciTech Connect

A plane mirror and two strongly curved plane elliptical mirrors comprising the refocusing system downstream the plane grating monochromator at FLASH in DESY have been characterized with the Nanometer Optical Component Measuring Machine at the BESSY-II Optics Laboratory of the Helmholtz Zentrum Berlin. Based on the measurement results the two elliptical cylinders were optimized by deterministic surface finishing technology (Ion Beam Finishing). The expected focusing performance was verified by ray tracings after each ion beam finish iteration using the measured topography results.

Siewert, Frank [Helmholtz Zentrum Berlin / BESSY II, Albert-Einstein-Str. 15, D-12489 Berlin (Germany); Reininger, Ruben [Scientific Answers and Solutions, 77 Constantine Way, Mount Sinai, NY 11766 (United States); Ruebhausen, Michael A. [CFEL, Center for Free Electron Laser Science, Notkestr. 15, 20355 Hamburg (Germany)

2010-06-23T23:59:59.000Z

415

Enhancement of the resolution of full-field optical coherence tomography by using a colour image sensor  

SciTech Connect

The influence of white balance in a colour image detector on the resolution of a full-field optical coherence tomograph (FFOCT) is studied. The change in the interference pulse width depending on the white balance tuning is estimated in the cases of a thermal radiation source (incandescent lamp) and a white light emitting diode. It is shown that by tuning white balance of the detector in a certain range, the FFOCT resolution can be increased by 20 % as compared to the resolution, attained with the use of a monochrome detector. (optical coherence tomography)

Kalyanov, A L; Lychagov, V V; Smirnov, I V; Ryabukho, V P [N.G. Chernyshevsky Saratov State University, Saratov (Russian Federation)

2013-08-31T23:59:59.000Z

416

Acquisition and reconstruction of brain tissue using knife-edge scanning microscopy  

E-Print Network (OSTI)

. As the sample passes under an individual photon receptor, the light intensity value is summed and passed to the next register. The final output pixel is the sum of the light intensity received by all TDI registers for a single sampled point... wide line is imaged along the leading edge of the knife. Our primary camera of choice is a DALSA CT-F3 High- Speed TDI Line Scan Camera. In order to get a high sensitivity at the speed at which we want to cut, the monochrome camera uses Time Delay...

Mayerich, David Matthew

2004-09-30T23:59:59.000Z

417

ELECTROCHEMICAL CORROSION STUDIES FOR TANK 241-AN-107 CORE 309 SEGMENTS 21R1 & 21R2  

SciTech Connect

Liquid waste in tank 241-AN-107 is below Technical Safety Requirements Administrative Control 5.16 (AC 5.16) limits. Electrochemical corrosion testing was performed on Core 309, Segments 21R1 and 21R2, to provide information on the conductivity and corrosive tendencies of the tank saltcake and interstitial liquid. This report describes data obtained under the execution of RPP-PLAN-29001, 'Electrochemical Corrosion Studies for Tank 241-AN-107 Core 309, Segments 21R1 and 21R2'. Analytical results are presented that show supernatant was within the limits while the interstitial liquid remained below the limits for the analytical cores. Applicable AC 5.16 chemistry control limits for AN-107 are presented.

DUNCAN JB

2007-11-13T23:59:59.000Z

418

Simultaneous determination of boron-10 and boron-11 under proton bombardment  

Science Journals Connector (OSTI)

Simultaneous determination of the two stable boron isotopes was carried out through the measurement of...11B and 428 keV or 718 keV gamma-rays from10B. Excitation functions were constructed and mean energies for ...

C. Olivier; H. A. Ras; M. Peisach

1982-01-01T23:59:59.000Z

419

Distribution in Angle of Protons from the D-D Reaction  

Science Journals Connector (OSTI)

The angular distribution of the disintegration protons from the D-D reaction has been investigated as a function of energy from 60 kev to 390 kev. The distribution was found to be well represented by I(?)=1+Acos2? at any one energy. The value of A increases smoothly with bombarding energy over the range investigated.

H. P. Manning; R. D. Huntoon; F. E. Myers; V. J. Young

1942-03-01T23:59:59.000Z

420

E-Print Network 3.0 - alpha spectrometry system Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

Tandem ion accelerator Proton beam: 200 keV to 6.4 MeV Alpha beam: 200 keV to 9.6 MeV Heavy ions: 200 ke... V to 20 MeV Beam currents: from pA to A (equivalent to mCi to...

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

E-Print Network 3.0 - alpha spectrometry measurement Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

Tandem ion accelerator Proton beam: 200 keV to 6.4 MeV Alpha beam: 200 keV to 9.6 MeV Heavy ions: 200 ke Source: Los Alamos National Laboratory, Theoretical Division, Condensed...

422

$^{180}$Ta production in the classical s-process  

E-Print Network (OSTI)

The production and survival of the quasistable isomer $^{180}$Ta during the stellar nucleosynthesis has remained a matter of discussion for years. A careful analysis of the available experimental data and theoretical calculations enabled us to reproduce the observed solar abundance of $^{180}$Ta in the classical s-process ($kT=28$ keV -- 33 keV).

Markus Loewe; Petr Alexa; Jorrit de Boer; Michael Wuerkner

2002-07-04T23:59:59.000Z

423

Precise measurement of alpha(K) for the M4 transition from Ir-193(m): A test of internal-conversion theory  

E-Print Network (OSTI)

The 10.5-day isomer in Ir-193 decays by a single 80.2-keV M4 transition directly to the ground state of that nucleus. We have measured the total intensity of K x rays relative to 80.2-keV gamma rays for this transition to be 98.7(6). With the K...

Nica, N.; Hardy, John C.; Iacob, VE; Raman, S.; Nestor, CW; Trzhaskovskaya, MB.

2004-01-01T23:59:59.000Z

424

Theoretical X-ray line profiles from colliding wind binaries  

Science Journals Connector (OSTI)

......106 Mo yr1 the lower energy lines (E 1 keV) are...Chandra Low- and High-Energy Transmission Grating...Skinner et al. 2001) and Car (Corcoran et al. 2001...it actually is. The alternative is to assume that all...noticeable for the lower energy lines (E 1 keV). These......

David B. Henley; Ian R. Stevens; Julian M. Pittard

2003-12-11T23:59:59.000Z

425

Getting Ready for the Technical Assessment at Snowmass "Go ahead, make my FIRE"  

E-Print Network (OSTI)

reactor - couple with burning plasma physics · Boundary Physics and Plasma Technology (coupled with above overall portfolio approach includes IFE) #12;Comparison of EU One Step to DEMO Power Plant(s) with ARIESV) LawsonFusionParameter,niTiE(1020m-3kevs) Central Ion Temperature (keV) Tokamaks 1993-99 Laser 1986 Direct

426

arXiv:1104.2624v1[astro-ph.SR]13Apr2011 Solar Physics  

E-Print Network (OSTI)

­15 keV, and 15­30 keV energy ranges for each event. In order to extract the height distribution from Northwestern Switzerland, Institute of 4D, Technologies, 5210 Windisch, Switzerland SOLA: paper.tex; 15 April

California at Berkeley, University of

427

Development of the Short Gap Undulators at the Photon Factory, KEK  

SciTech Connect

Very short-period and in-vacuum type undulators have been developed and installed in the 2.5-GeV Photon Factory storage ring, which was upgraded to enhance the straight sections for insertion devices in 2005. X rays ranging from 2 keV to 15 keV are covered by these undurators with their lower harmonics.

Yamamoto, Shigeru; Tsuchiya, Kimichika; Sasaki, Hiroyuki; Aoto, Tomohiro [Photon Factory, High Energy Accelerator Research Organization, KEK Oho, Tsukuba, Ibaraki 305-0801 (Japan); Department of Materials Structure Science, Graduate University for Advanced Studies, Oho, Tsukuba, Ibaraki 305-0801 (Japan); Shioya, Tatsuro [Photon Factory, High Energy Accelerator Research Organization, KEK Oho, Tsukuba, Ibaraki 305-0801 (Japan)

2010-06-23T23:59:59.000Z

428

Monte Carlo simulation of embedded 241Am activity in injured palm  

Science Journals Connector (OSTI)

......Pu isotopes (17.5 keV) and neptunium L X-rays (17.8 keV) of 241Am...uranium L X-rays due to Pu and neptunium L X-rays due to 241Am. Ratio...wounds incurred by former workers at rocky flats. Health Phys. (2006) 91(2......

M. Y. Nadar; H. K. Patni; D. K. Akar; Lokpati Mishra; I. S. Singh; D. D. Rao; P. K. Sarkar

2013-04-01T23:59:59.000Z

429

Development of Polarized Electron Source of GaAs-AlGaAs Superlattice and Strained GaAs  

Science Journals Connector (OSTI)

At Nagoya University, we have continued the development of GaAs polarized electron source (PES) for several years. Our test ... a gun producing (15) KeV polarized electrons and a standard 100 KeV Mott polarimete...

T. Nakanishi; S. Nakamura

1991-01-01T23:59:59.000Z

430

Formation of unsaturated hydrocarbons in interstellar ice analogues by cosmic rays  

Science Journals Connector (OSTI)

......facilities of the heavy-ion accelerator Grand Accelerateur National...were performed inside a high vacuum chamber which could be coupled...m) Electronic (keV m1) Nuclear (keV m1) Total [eV (molecules...Reimann C. T., 1984, Nuclear Instrum. Methods Phys. Res......

S. Pilling; D. P. P. Andrade; E. F. da Silveira; H. Rothard; A. Domaracka; P. Boduch

2012-07-01T23:59:59.000Z

431

ORIGAMIX, a CdTe-based spectro-imager development for nuclear applications  

E-Print Network (OSTI)

The Astrophysics Division of CEA Saclay has a long history in the development of CdTe based pixelated detection planes for X and gamma-ray astronomy, with time-resolved imaging and spectrometric capabilities. The last generation, named Caliste HD, is an all-in-one modular instrument that fulfills requirements for space applications. Its full-custom front-end electronics is designed to work over a large energy range from 2 keV to 1 MeV with excellent spectroscopic performances, in particular between 10 and 100 keV (0.56 keV FWHM and 0.67 keV FWHM at 13.9 and 59.5 keV). In the frame of the ORIGAMIX project, a consortium based on research laboratories and industrials has been settled in order to develop a new generation of gamma camera. The aim is to develop a system based on the Caliste architecture for post-accidental interventions or homeland security, but integrating new properties (advanced spectrometry, hybrid working mode) and suitable for industry. A first prototype was designed and tested to acquire feedback for further developments. In this study, we particularly focused on spectrometric performances with high energies and high fluxes. Therefore, our device was exposed to energies up to 700 keV (133Ba, 137Cs) and we measured the evolution of energy resolution (0.96 keV at 80 keV, 2.18 keV at 356 keV, 3.33 keV at 662 keV). Detection efficiency decreases after 150 keV, as Compton effect becomes dominant. However, CALISTE is also designed to handle multiple events, enabling Compton scattering reconstruction, which can drastically improve detection efficiencies and dynamic range for higher energies up to 1408 keV (22Na, 60Co, 152Eu) within a 1-mm thick detector. In particular, such spectrometric performances obtained with 152Eu and 60Co were never measured before with this kind of detector.

S. Dubos; H. Lemaire; S. Schanne; O. Limousin; F. Carrel; V. Schoepff; C. Blondel

2015-02-05T23:59:59.000Z

432

Measurements of Scintillation Efficiency and Pulse-Shape for Low Energy Recoils in Liquid Xenon  

E-Print Network (OSTI)

Results of observations of low energy nuclear and electron recoil events in liquid xenon scintillator detectors are given. The relative scintillation efficiency for nuclear recoils is 0.22 +/- 0.01 in the recoil energy range 40 keV - 70 keV. Under the assumption of a single dominant decay component to the scintillation pulse-shape the log-normal mean parameter T0 of the maximum likelihood estimator of the decay time constant for 6 keV < Eee < 30 keV nuclear recoil events is equal to 21.0 ns +/- 0.5 ns. It is observed that for electron recoils T0 rises slowly with energy, having a value ~ 30 ns at Eee ~ 15 keV. Electron and nuclear recoil pulse-shapes are found to be well fitted by single exponential functions although some evidence is found for a double exponential form for the nuclear recoil pulse-shape.

Akimov, D Y; Davidge, D; Dawson, J; Howard, A S; Ivaniouchenkov, Yu; Jones, W G; Joshi, M; Kudryavtsev, V A; Lawson, T B; Lebedenko, V; Lehner, M J; Lightfoot, P K; Liubarsky, I; Lscher, R; McMillan, J E; Peak, C D; Quenby, J J; Spooner, N J C; Sumner, T J; Tovey, Daniel R; Ward, C K

2002-01-01T23:59:59.000Z

433

Estimation of boron isotope ratios using high resolution continuum source atomic absorption spectrometry  

Science Journals Connector (OSTI)

In the production of 10B enriched steels, the productionrecycling process needs to be closely monitored for inadvertent mix-up of materials with different B isotope levels. A quick and simple method for the estimation of boron isotope ratios in high alloyed steels using high resolution continuum source flame AAS (HR-CS-FAAS) was developed. On the 208.9nm B line the wavelength of the peak absorption of 10B and 11B differs by 2.5pm. The wavelength of the peak absorption of boron was determined by fitting a Gauss function through spectra simultaneously recorded by HR-CS-FAAS. It was shown that a linear correlation between the wavelength of the peak absorption and the isotope ratio exists and that this correlation is independent of the total boron concentration. Internal spectroscopic standards were used to compensate for monochromator drift and monochromator resolution changes. Accuracy and precision of the analyzed samples were thereby increased by a factor of up to 1.3. Three steel reference materials and one boric acid CRM, each certified for the boron isotope ratio were used to validate the procedure.

Helmar Wiltsche; Karl Prattes; Michael Zischka; Gnter Knapp

2009-01-01T23:59:59.000Z

434

Neutron Polarization  

Science Journals Connector (OSTI)

The neutron polarization cross section of iron has been measured as a function of energy from 0.7 to 3.3A by two methods: using the single transmission effect in a block of polycrystalline iron at energies selected by a quartz crystal monochromator; and using a single crystal of magnetized magnetite to analyze the beam emerging from the iron polarizer, the magnetite crystal itself serving as monochromator. The measured values are compared with those of other observers and the theoretically expected values. These are found to agree fairly well within the limits of accuracy of the measurements and existing knowledge of the wave function of the iron 3d shell. The two techniques were used also to determine the average polarization (32 percent) as seen by a 1v detector in a beam of reactor neutrons emerging from a 4-cm thick polarizing block of iron. Problems and techniques associated with the measurement of the average polarization of a continuous spectrum are discussed. A simplified experimental treatment of the problem of beam "hardening" is described. A description is given of the use of the magnetic resonance method in conjunction with a single-crystal magnetite analyzer for the measurement of neutron polarization.

C. P. Stanford; T. E. Stephenson; L. W. Cochran; S. Bernstein

1954-04-15T23:59:59.000Z

435

Application of beam emission spectroscopy to NBI plasmas of Heliotron J  

SciTech Connect

This paper describes the application of the beam emission spectroscopy (BES) to Heliotron J, having the nonsymmetrical helical-magnetic-axis configuration. The spectral and spatial profile of the beam emission has been estimated by the numerical calculation taking the collisional excitation processes between plasmas (electrons/ions) and beam atoms. Two sets of the sightlines with good spatial resolution are presented. One is the optimized viewing chords which have 20 sightlines and observe the whole plasma region with the spatial resolution {Delta}{rho} less than {+-}0.055 using the newly designed viewing port. The other is 15 sightlines from the present viewing port of Heliotron J for the preliminary measurement to discuss the feasibility of the density fluctuation measurement by BES. The beam emission has been measured by a monochromator with a CCD camera. A good consistency has been obtained between the spectral profiles of the beam emission measured by the monochromator and the beam emission spectrum deduced by the model calculation. An avalanche photodiode with an interference filter system was also used to evaluate the signal-to-noise (S/N) ratio of the beam emission in the present experimental setup. The modification of the optical system is being planned to improve the S/N ratio, which will enable us to estimate the density fluctuation in Heliotron J.

Kobayashi, S.; Ohshima, S.; Mizuuchi, T.; Nagasaki, K.; Yamamoto, S.; Okada, H.; Minami, T.; Hanatani, K.; Konoshima, S.; Takeuchi, M.; Toushi, K.; Sano, F. [Institute of Advanced Energy, Kyoto University, Uji, Kyoto 611-0011 (Japan); Kado, S. [School of Engineering, The University of Tokyo, Bunkyo, Tokyo 113-8656 (Japan); Oishi, T. [Nagoya University, Chikusa-ku, Nagoya 464-8603 (Japan); Kagawa, T.; Lee, H. Y.; Minami, T.; Nakamura, Y. [Graduate School of Energy Science, Kyoto University, Uji, Kyoto 611-0011 (Japan); Murakami, S. [Graduate School of Engineering, Kyoto University, Kyoto, Kyoto 606-8501 (Japan)

2010-10-15T23:59:59.000Z

436

Low-Energy Nuclear Level Scheme of Rh104  

Science Journals Connector (OSTI)

Investigations of the low-energy level properties (level energies, spins, and parities) of Rh104 have been undertaken from studies of the coincidence relationships existing between the low-energy capture gamma rays produced by thermal neutron capture in Rh103 using NaI(Tl) scintillation crystals as detectors. It is known from the decay scheme of the 4.4-min Rh104m isomer that Rh104 has energy levels at 52, 96, and 129 keV with spins and parities of 2-, 2+, and 5+, respectively. The data obtained in these investigations have been combined with the isomeric level data in order to determine the properties of several additional levels. Additional levels in Rh104 have been determined at the following energies, with the level spin and parity in parenthesis after the energy; 184 keV (1), 192 keV (3+), 269 keV (3), 450 keV, and either 229 keV (3+) or 325 keV (4+). These spin and parity assignments were made on the basis of a K internal conversion coefficient analysis of the coincidence data together with consideration of the relative cascade intensities. On the basis of the possible odd-proton and odd-neutron configurations open to the 184- and 269-keV levels, and considering the transition intensities to the lower levels, it was determined that the negative-parity assignment is most probable for both of these levels, with the levels having configuration assignments of (p32)(d52). The 192-keV level together with the 229- or 325-keV level most probably have either [(g92)5]72(d52)n or (g92)5(d52)n configurations. In fact, if it is the 229-keV level which does exist, as the available evidence might seem to indicate, then, since they both have spins and parities of 3+, the 192-keV level would have one of these configurations while the 229-keV level would have the other.

R. C. Greenwood

1963-01-01T23:59:59.000Z

437

Cubane, Cuneane, and Their Carboxylates: A Calorimetric, Crystallographic, Calculational, and Conceptual Coinvestigation  

E-Print Network (OSTI)

Henares, Spain, Department of Chemistry & Biochemistry, University of Missouri St. Louis, 8001 Natural Bridge Road, St Louis, Missouri 63121-4499, Department of Chemistry & Biochemistry, University, fH°m(cr)/kJ,mol-1 ) -232.62 ( 5.84 and -413.02 ( 5.16, respectively. The enthalpies of sublimation

Chickos, James S.

438

Federal Guidance Report No. 13  

National Nuclear Security Administration (NNSA)

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439

untitled  

Gasoline and Diesel Fuel Update (EIA)

... 12,545.7 111,000.1 4,447.5 16,937.0 1,344.1 2,725.3 December ... 12,285.5 118,369.4 4,125.0 17,688.1 1,227.6 2,529.6...

440

HIGH ENERGY LUNCH PHYSICS SEMINAR, 19931996 1993 Seminars  

E-Print Network (OSTI)

Wilson, The University of Chicago 3/14 Nick Solomey, The University of Chicago 3/21 Bruce Winstein/2 Andre Turcot, CERN 5/9 Lincoln Wolfenstein, Carnegie Mellon University 5/16 Wyatt Merritt, Fermilab 5/25 Corbin Covault, The University of Chicago 8/1 Edward Blucher, The University of Chicago 8/8 Frank Merritt

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
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they are not comprehensive nor are they the most current set.
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to obtain the most current and comprehensive results.


441

Utilization and Fairness in Spectrum Assignment for Opportunistic Spectrum Access  

E-Print Network (OSTI)

. INTRODUCTION Wireless devices are becoming ubiquitous, placing increas- ing stress on the fixed radio spectrum by software defined radio (SDR) technology [5], [16], [24], Open Spectrum allows unlicensed (secondary) users1 Utilization and Fairness in Spectrum Assignment for Opportunistic Spectrum Access Chunyi Peng

Almeroth, Kevin C.

442

Natural Environment and Landscape Policy and Guidelines  

E-Print Network (OSTI)

(LEED) and Sustainability Tracking, Assessment & Rating System (STARS). LEED is a `Green Building Rating System' that promotes sustainable development and building practices through a number of standardized & furniture 5.14 Walls and fences 5.15 Signage 5.16 Outdoor lighting 5.17 Green roof #12;Dalhousie University

Brownstone, Rob

443

DALHOUSIE UNIVERSITY Natural Environment and Landscape Nov 2013  

E-Print Network (OSTI)

(LEED) and Sustainability Tracking, Assessment & Rating System (STARS). LEED is a `Green Building Rating System' that promotes sustainable development and building practices through a number of standardized & furniture 5.14 Walls and fences 5.15 Signage 5.16 Outdoor lighting 5.17 Green roof #12;Dalhousie University

Brownstone, Rob

444

--No Title--  

Annual Energy Outlook 2012 (EIA)

17 67 16 1,040 2,488 769 16.3 26.9 20.4 Heating Equipment (more than one may apply) Heat Pumps ... 4 64 9 339 3,677 542 12.9 17.5 16.8...

445

Global Stability Analysis of Fluid Flows using Sum-of-Squares  

E-Print Network (OSTI)

Jul 1, 2011 ... The first of these is the classical energy approach of [5, 16], which provides conservative ..... Standard software tools are freely available for posing and solving ... stability limit estimated by direct numerical simulation. ...... make assumptions identical to those in [9, 10] for the purposes of comparison.

2011-07-01T23:59:59.000Z

446

OHIO SEA GRANT AND STONE LABORATORY OHIO SEA GRANT AND STONE LABORATORY  

E-Print Network (OSTI)

5/16/2014 1 OHIO SEA GRANT AND STONE LABORATORY OHIO SEA GRANT AND STONE LABORATORY Climate Change Impacts on Lake Erie and Stone Lab Efforts to Address the Problem OHIO SEA GRANT AND STONE LABORATORY (CLEAR) ·1978--Ohio Sea Grant College Program ·1992--Great Lakes Aquatic Ecosystem Research Consortium

Howat, Ian M.

447

Dynamics of the Friedmann Universe Using Regge Calculus  

Science Journals Connector (OSTI)

Models for the Friedmann Universe are constructed from 5, 16, or 600 dust-filled tetrahedrons connected so as to form a closed space. Using the techniques of Regge calculus the time development of these model universes is determined and the results compared with the standard analytic solution for an isotropic dust-filled universe.

P. A. Collins and Ruth M. Williams

1973-02-15T23:59:59.000Z

448

Boundaries for Biofilm Formation: Humidity and Temperature  

Science Journals Connector (OSTI)

...Yucca Mountain is located at the Nevada Test Site, 100 miles northwest of Las...oxygenated volcanic tuff at the Nevada Test Site (1, 10, 11). When native...exist in the rock and soil of the Nevada Test Site (5, 16, 21). Studies by...

Terry Ann Else; Curtis R. Pantle; Penny S. Amy

2003-08-01T23:59:59.000Z

449

Y YEAR  

National Nuclear Security Administration (NNSA)

Female (AAPI,F) 0 0 0% Hispanic Male (H,M) 0 0 0% Hispanic Female (H,F) 0 0 0% White Male (W,M) 13 12 -7.69% White Female (W,F) 6 5 -16.67% Savannah River Field...

450

Office of Civil Rights, NNSA, NA 1.2, Albuquerque Complex  

National Nuclear Security Administration (NNSA)

1.71% Hispanic Male 6 5 -16.67% 6.41% 6.17% Hispanic Female 5 5 0.00% 6.41% 4.52% White Male 44 43 -2.27% 55.13% 39.03% White Female 15 14 -6.67% 17.95% 33.74% GENDER...

451

Y YEAR  

National Nuclear Security Administration (NNSA)

(AAPI,F) 2 2 0% Hispanic Male (H,M) 6 6 0% Hispanic Female (H,F) 6 5 -16.67% White Male (W,M) 50 46 -8.00% White Female (W,F) 13 12 -7.69% PAY PLAN Change...

452

Y YEAR  

National Nuclear Security Administration (NNSA)

0 0 0% Hispanic Male (H,M) 2 0 -100% Hispanic Female (H,F) 6 5 -16.67% White Male (W,M) 9 9 0% White Female (W,F) 3 3 0% PAY PLAN Change DIVERSITY Change...

453

CX-100151 Categorical Exclusion Determination  

Office of Energy Efficiency and Renewable Energy (EERE)

State of Illinois SEP: Continental Electrical Construction Company, LLC: Technology and Demonstration Grant No. 13-432003 Award Number: DE-EE0006225 CX(s) Applied: B5.16, B1.31 Date: 12/19/2014 Location(s): IL Office(s): Golden Field Office

454

Exchangeable sodium accumulation and replacement in Southeast Texas soils under turfgrass  

E-Print Network (OSTI)

accumulation but exchangeable Na also increased as a function of years of irrigation. The multiple regression equation: SARE =-5.16 + 0.53 SARiw + 4.04 In (yr) (R2 = 0.86) best predicted SARE to a depth of 30 cm. This study also compared gypsum, a common...

Najjar, Namir Fouad

1995-01-01T23:59:59.000Z

455

Helical poly(arginine) mimics with superior cell-penetrating and molecular transporting properties  

E-Print Network (OSTI)

permeability up to two orders of magnitude higher than that of HIV-TAT peptide and excellent DNA and si-rich CPPs is HIV-TAT, an 11-mer peptide containing 6 Arg residues.5,16 In addition to the critical roles superior membrane activities, up to two orders of magnitude higher than that of TAT, and remarkable DNA

Cheng, Jianjun

456

Kernel methods for phenotyping complex plant architecture  

E-Print Network (OSTI)

Kernel methods for phenotyping complex plant architecture Koji KAWAMURA1,2 ,Laurence HIBRAND´e, FRANCE , 2. Department of Environmental Engineering, Osaka Institute of Technology, 5-16-1 Ohmiya, Asahi architecture is a crit- ical step for understanding the genetic determinism of plant architecture. Previous

Paris-Sud XI, Université de

457

CX-100017: Categorical Exclusion Determination  

Office of Energy Efficiency and Renewable Energy (EERE)

U.S. Photovoltaic Manufacturing Consortium - Enabling America's Solar Revolution CX(s) Applied: A9, B3.6, B5.16 Date: 08/18/2014 Location(s): New York Offices(s): Golden Field Office Technology Office: Solar Energy Technologies Award Number: DE-EE0004947

458

The Proceedings of the 2008 International Conference on Mobile Data Xiaofeng Meng Hui Lei Stephane Grumbach Hong Va Leong  

E-Print Network (OSTI)

. 12. ,,. Deep Web . , 31(8): 1412-142120088. 13. ,,,: XML Twig . 45 ()354-359, 2008.10(, ) 14 . , 45 ()37-42, 2008.10. (, ) 17. TEXEM . 45 ()269-274, 2008.10 1 Deep Web Key Techniques on Deep Web Data Integration2008.5.16 2 Deep Web Study on Query Results Processing of Deep Web Data

459

A NuSTAR observation of the fast symbiotic nova V745 Sco in outburst  

E-Print Network (OSTI)

The fast recurrent nova V745 Sco was observed in the 3-79 keV X-rays band with NuSTAR 10 days after the optical discovery. The measured X-ray emission is consistent with a collisionally ionized optically thin plasma at temperature of about 2.7 keV. A prominent iron line observed at 6.7 keV does not require enhanced iron in the ejecta. We attribute the X-ray flux to shocked circumstellar material. No X-ray emission was observed at energies above 20 keV, and the flux in the 3-20 keV range was about 1.6 $\\times$ 10$^{-11}$ erg cm$^{-2}$ s$^{-1}$. The emission measure indicates an average electron density of order of 10$^7$ cm$^{-2}$. The X-ray flux in the 0.3-10 keV band almost simultaneously measured with Swift was about 40 times larger, mainly due to the luminous central supersoft source emitting at energy below 1 keV. The fact that the NuSTAR spectrum cannot be fitted with a power law, and the lack of hard X-ray emission, allow us to rule out Comptonized gamma rays, and to place an upper limit of the order of...

Orio, M; Page, K L; Sokoloski, J L; Harrison, F

2014-01-01T23:59:59.000Z

460

Level structure of Yb174 from the Yb173(n,?) reaction  

Science Journals Connector (OSTI)

The level structure of Yb174 has been studied using the Yb173(n,?) reaction with both thermal and 2-keV neutrons. Measurements of ?-ray energies and intensities were made using Ge(Li) detectors. From these data a neutron separation energy of 7464.80.5 keV has been determined for Yb174. A level scheme is proposed for Yb174 which contains 47 excited states, with identified de-excitation modes, below 2.35 MeV. Features of the proposed level scheme include: the K?=2-,0-,and3- octupole-vibrational bands with band-head energies of 1318, 1710, and 1851 keV, respectively; the ?-vibrational band at 1634 keV; three excited K?=0+ bands with band-head energies of 1487, 1885, and 2100 keV; and, several two-quasiparticle bands with band-head energies in keV (and K? assignments) of 1660(3+), 1624(1+), 2016(3+), and 2049(3-). Configuration assignments for these two-quasiparticle bands are discussed. The available data for the K?=3+ band at 1606 keV are not inconsistent with the assumption that it has collective character; and it is suggested that it, together with the lowest-lying 3+ band in Yb172 (at 1172 keV), might represent, in the framework of the interacting boson approximation model, examples of g-boson excitations.NUCLEAR REACTIONS Yb173(n,?), E=thermal, 2 keV; measured E?, I?; Yb174 deduced levels, J, ?. Enriched targets, Ge(Li) detectors.

R. C. Greenwood and C. W. Reich

1981-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

New astrophysical S factor for the (15)N(p,gamma)(16)O reaction via the asymptotic normalization coefficient (ANC) method  

E-Print Network (OSTI)

reaction have been reported by Rolfs and Rodney [1] down to proton energies of Ep #1; 155 keV and earlier by Hebbard [2] for proton energies down to Ep #1; 220 keV. These measurements disagree at energies below 300 keV by up to a factor of 2. To fit... their low-energy data to obtain an astrophysical S factor, Rolfs and Rodney included the interference of the two 1? resonant capture amplitudes with the nonresonant (direct) component to the ground state of 16O. The direct capture term plays an important...

Mukhamedzhanov, A. M.; Bem, P.; Burjan, V.; Gagliardi, Carl A.; Goldberg, V. Z.; Hons, Z.; La Cognata, M.; Kroha, V.; Mrazek, J.; Novak, J.; Piskor, S.; Pizzone, R. G.; Plunkett, A.; Romano, S.; Simeckova, E.; Spitaleri, C.; Trache, L.; Tribble, Robert E.; Vesely, F.; Vincour, J.

2008-01-01T23:59:59.000Z

462

Medium energy ion implantation of Germanium into heated Silicon  

E-Print Network (OSTI)

flange arranged in a standard Einsel lens arrangement and a set of 13 ++12 ~6 L, 1 - Source 2 - Acceleration Column 3. - Glass Cross and 6" Diffusion 4 - Separation Magnet 5 - Gate Valve 6 - Quadrupole 7 - Rear Collimator 8 - Deflection Plates... Analysis of a, 40 keV, SXIO" ions cm' Ge Implant into 420'C FZ &111& Si. 29 300 keV He RBS analysis of two, 60 keV, 3X10" ions cm' Ge implants, rastered and unrastered, into 300'C FZ &111& Si. 30 LIST OF TABLES Table Page Cntical thickness of a Ge...

McCoy, John Curtis

1993-01-01T23:59:59.000Z

463

Energy distribution of Compton-scattered gamma rays  

E-Print Network (OSTI)

of the experimental peaks, and is shown in Figs. 15, 17, 19, 21, and 22. The FNHM of these curves can be measured and the broaden- ing due to the Doppler effect calculated. The equation used is where D is the broadening due to the Doppler effect, E... of this corrected curve was found to fit a Gaussian curve of dispersion 6. 6 keV. The FWHM of the Gaussian corresponding to this is 15. 4 keV, From thi. s, the broadening due to the Doppler effect is found to be 10. 2-1 keV, + The uncertainty in the Doppler...

Moreland, Richard Wayne

2012-06-07T23:59:59.000Z

464

Average resonance capture study of Te124  

Science Journals Connector (OSTI)

An average resonance capture study of Te124 was carried out by bombarding samples of Te123 with 2- and 24-keV neutron beams. The complete set of 0+, 1+, 2+ states disclosed by the experiment is consistent with the data of Robinson, Hamilton, and Snelling, demonstrating that there are no undetected states of these spins (especially 0+ states) below about 2500 keV. In particular, proposed 0+ levels at 1156 and 1290 keV are ruled out. This impacts various attempted interpretations in terms of intruder states, U(5), and O(6) symmetries.

R. F. Casten; J.-Y. Zhang; B.-C. Liao

1991-07-01T23:59:59.000Z

465

A search for neutrinoless double beta decay of 130Te with a low temperature calorimeter  

Science Journals Connector (OSTI)

Possible impacts of the bolometric technique on Neutrinoless Double Beta Decay (0??DVD) search are discussed. In this approach the performances of two TeO2 low temperature calorimeters with masses of 73 g and 340 g are reported: the FWHM resolutions are respectively 6 keV and 20 keV at 2614 keV. The operation of these detectors in a low background environment in the Gran Sasso underground laboratory has allowed to set a limit on the half?life of 130Te 2??DBD of about 2.51021 and to study the residual radioactive background components.

A. Alessandrello; C. Brofferio; D. V. Camin; O. Cremonesi; G. Gervasio; E. Fiorini; A. Giuliani; M. Pavan; G. Pessina; E. Previtali; L. Zanotti

1992-01-01T23:59:59.000Z

466

Microsoft Word - bang_abstract  

NLE Websites -- All DOE Office Websites (Extended Search)

a few keV. When an energetic deuterium ion collides with another deuterium ion, a nuclear fusion reaction can occur, generating a 2.45 MeV neutron. By shooting cryogenically...

467

Edge effects caused by enhancement of DD/DT fusion reactions in metals at low energy of projectile particles in an ITER-type fusion reactor  

Science Journals Connector (OSTI)

Experimental data on enhancement of the yield of DD/DT reactions in metal targets at low energies of projectile deuterons (E d...< 5 keV) were analyzed. A semiempirical expression was obtained to ...

A. G. Lipson; A. S. Roussetski; B. F. Lyakhov; E. I. Saunin

2008-07-01T23:59:59.000Z

468

Muon-induced backgrounds in the CUORICINO experiment  

E-Print Network (OSTI)

code simulated the muon energy and angular distribution inthe direction and energy of the muons underground. The rangemuon and bolometer counts / 1 keV Low LowEnergyRegion Energy

Andreotti, E.

2010-01-01T23:59:59.000Z

469

Experiments with low-energy muons  

Science Journals Connector (OSTI)

Two experiments with low-energy muons are described: the determination of the stopping ... of C, Si, Ti and Au for muons at energies down to 2 keV and the measurement ... . A pronounced Barkas effect was found fo...

F. J. Hartmann; H. Daniel; Chr Maierl; M. Mhlbauer; W. Schott

1996-01-01T23:59:59.000Z

470

Two photon decay of neutral scalars below 1.5 GeV in a chiral model for bar{q}q and bar{q}bar{q}qq states  

E-Print Network (OSTI)

We study the two photon decay of neutral scalars below 1.5 GeV in the context of a recently proposed chiral model for bar{q}q and bar{q}bar{q}qq states. We find good agreement with experimental results for the a_{0}(980)->gamma gamma. Our calculations for f_{0}(980)->gamma gamma shows that further work is necessary in order to understand the structure of this meson. The model predicts Gamma(a_{0}(1450)->gamma gamma)=0.16+/-0.10KeV, Gamma(sigma->gamma gamma)=0.47+/-0.66 KeV, Gamma(f(1370)->gamma gamma)=0.07+/-0.15 KeV, Gamma(f(1500)->gamma gamma)=0.74+/-0.78 KeV.

Simon Rodriguez; Mauro Napsuciale

2004-11-10T23:59:59.000Z

471

State-of-the-art dosimetric methods for internal and external exposures: conclusions of a EURADOS action  

Science Journals Connector (OSTI)

......in Europe. An inventory of the internal...future study is highly recommended to...186keV) in lungs (enriched uranium); other MDA values...induced or KPA for uranium measurements...131I, and also uranium, thorium and plutonium......

M. A. Lopez; C. M. Castellani; L. Currivan; J. van Dijk; R. Falk; P. Olko; C. Wernli

2007-07-01T23:59:59.000Z

472

The neutron binding energy in the neutron-rich nucleus93Sr  

Science Journals Connector (OSTI)

The neutron binding energy in93Sr has been determined to (52306) keV from energy correspondences between levels defined by ?-ray transitions and ?-delayed neutron emission.

K. -L. Kratz; H. Ohm

1980-01-01T23:59:59.000Z

473

Performance of a Chamber for Studying the Liquid Xenon Response to Nuclear Recoils  

E-Print Network (OSTI)

The design and performance of a 1.2 liter liquid xenon chamber equipped with 7 two-inch photomultiplier tubes, with the purpose of studying the scintillation response of xenon to gamma-rays and neutrons, is described. Measurements with gamma-rays indicate a high VUV light collection efficiency resulting in ~5.5 photoelectrons per 1 keV of deposited energy. The energy resolution (FWHM) is 18% and 22%, for 122 keV and 511 keV gamma-rays, respectively. An algorithm for the reconstruction of the scintillation coordinates in (x,y) plane was developed and tested. The position resolution is estimated to be 6.9 mm (sigma) for 122 keV gamma-rays.

V. Chepel; F. Neves; V. Solovov; A. Pereira; M. I. Lopes; J. Pinto da Cunha; P. Mendes; A. Lindote; C. P. Silva; R. Ferreira Marques; A. J. P. L. Policarpo

2005-01-07T23:59:59.000Z

474

Influence of the magnetic phase transition on secondary ion emission from disordered Ni-Pd compounds of various compositions  

Science Journals Connector (OSTI)

Variations in secondary ion emission (SIE) from polycrystals of ferromagnetic disordered Ni-Pd compounds irradiated by argon ions with energy of 10 keV are studied experimentally. A considerable reduction in Ni+ ...

K. F. Minnebaev; K. A. Tolpin

2012-05-01T23:59:59.000Z

475

Clues to the origin of metal in Almahata Sitta EL and EH chondrites...  

NLE Websites -- All DOE Office Websites (Extended Search)

microanalyzer (EPMA) at the ICEM operated at 15 keV, a probe current of 15 nA, and 1 lm beam size. For metal analyses (Table 1), pure Astimex metal standards (Fe, Ni, Si, Co),...

476

Toward Understanding Dynamic Annealing Processes in Irradiated Ceramics  

E-Print Network (OSTI)

Scattering IBA Ion Beam Analysis vi IBM Ion Beam Modification IED Ionization Enhanced Diffusion IP Intermediate Defect Peak keV Kilo Electron Volt KP Kinchin-Pease Ld Diffusion Length LED Light Emitting Diode LLNL Lawrence Livermore National...

Myers, Michael

2013-03-04T23:59:59.000Z

477

The Disintegration of Radium D  

Science Journals Connector (OSTI)

The disintegration of radium D has been investigated using a gaseous source of lead tetramethyl in a proportional counter. The form of the low energy ?-spectrum coincident with the 46.7-kev ?-ray has been determined. The end point has been found to be 15.21 kev. The shape of the spectrum shows good agreement with the Fermi theory for an allowed transition, in which the effect of screening on the Coulomb factor is neglected. The results indicate that the number of ?-particles below 3 kev is somewhat less than than predicted by theory, neglecting screening. It is also concluded that the change in binding energy of the atomic electrons (about 10 kev) released in the decay, is included in the energy of disintegration of the ?-particles, and is shared between the ?-particle and neutrino.

A. A. Jaffe and S. G. Cohen

1953-01-15T23:59:59.000Z

478

Effect of Fe-ion implantation doping on structural and optical properties of CdS thin films  

Science Journals Connector (OSTI)

We report on effects of Fe implantation doping-induced changes in structural, optical, morphological, and vibrational properties of cadmium sulfide thin films. Films were implanted with 90keV Fe+ ions at room te...

S. Chandramohan; A. Kanjilal; S. N. Sarangi; S. Majumder

2010-06-01T23:59:59.000Z

479

Identification of the slow E3 transition {sup 136}Cs{sup m{yields}136}Cs with conversion electrons  

SciTech Connect

We performed at ISOLDE the spectroscopy of the decay of the 8{sup -} isomer in {sup 136}Cs by {gamma} and conversion-electron detection. For the first time the excitation energy of the isomer and the multipolarity of its decay have been measured. The half-life of the isomeric state was remeasured to T{sub 1/2}=17.5(2) s. This isomer decays via a very slow 518-keV E3 transition to the ground state. In addition to this, a much weaker decay branch via a 413-keV M4 and a subsequent 105-keV E2 transition has been found. Thus we have found a new level at 105 keV with spin 4{sup +} between the isomeric and the ground state. The results are discussed in comparison to shell-model calculations.

Wimmer, K. [Fakultaet fuer Physik, Ludwig-Maximilians-Universitaet Muenchen, D-85748 Garching (Germany); Physik Department E12, Technische Universitaet Muenchen, D-85748 Garching (Germany); Koester, U. [Institut Laue Langevin, F-38042 Grenoble Cedex 9 (France); Hoff, P. [Department of Chemistry, University of Oslo, N-0315 Oslo (Norway); Kroell, Th. [Physik Department E12, Technische Universitaet Muenchen, D-85748 Garching (Germany); Institut fuer Kernphysik, Technische Universitaet Darmstadt, D-64289 Darmstadt (Germany); Kruecken, R. [Physik Department E12, Technische Universitaet Muenchen, D-85748 Garching (Germany); Lutter, R.; Morgan, Th.; Schwerdtfeger, W.; Thirolf, P. G. [Fakultaet fuer Physik, Ludwig-Maximilians-Universitaet Muenchen, D-85748 Garching (Germany); Mach, H. [Department of Nuclear and Particle Physics, Uppsala University, S-75121 Uppsala (Sweden); Sarkar, S. [Department of Physics, Bengal Engineering and Science University, Shibpur, Howrah 711103 (India); Sarkar, M. Saha [Nuclear and Atomic Physics Division, Saha Institute of Nuclear Physics, Kolkata 700064 (India); Srivastava, P. C. [Grand Accelerateur National d'Ions Lourds, CEA/DSM-CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex 5 (France); Nuclear Physics Group, Department of Physics, University of Allahabad, Allahabad 211002 (India); Van Isacker, P. [Grand Accelerateur National d'Ions Lourds, CEA/DSM-CNRS/IN2P3, B.P. 55027, F-14076 Caen Cedex 5 (France)

2011-07-15T23:59:59.000Z

480

This content has been downloaded from IOPscience. Please scroll...  

NLE Websites -- All DOE Office Websites (Extended Search)

radius, filter polychromators with 6 to 8 channels (10 eV-5 keV range), avalanche photodiode detectors, and 1 GSampleschannel digitization. Use of the previous pulse-burst...

Note: This page contains sample records for the topic "5-16 kev monochromator" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

Neutron capture cross sections of /sup 178/,/sup 179/,/sup 180/Hf and the origin of nature's rarest stable isotope /sup 180/Ta  

SciTech Connect

The neutron capture cross sections of /sup 178/,/sup 179/,/sup 180/Hf were measured in the energy range 2.6 keV to 2 MeV. The average capture cross sections were derived and fitted in terms of strength functions. Resonance parameters for the observed resonances below 10 keV were determined by shape analysis. Maxwellian-averaged capture cross sections were computed for thermal energies with kT between 5 and 100 keV. The cross sections for kT = 30 keV were used to determine the population probability of the 8- isomeric level in /sup 180/Hf by neutron capture as (1.24 +- 0.06)% and the r-process abundance of /sup 180/Hf as 0.0290 (Si = 10/sup 6/). These quantities served to analyze s- and r-process nucleosynthesis of /sup 180/Ta, nature's rarest stable isotope.

Beer, H.; Macklin, R.L.

1982-01-01T23:59:59.000Z

482

Depth profiling studies of multilayer films with a C60 A.G. Sostarecza,*  

E-Print Network (OSTI)

0) at a C60 þ beam energy of 20 keV. The neutral atom yield was monitored via laser postionization Materials Research Institute Building, University Park, PA 16802, USA b Physics Department, University

Wucher, Andreas

483

Latitude Distribution of Interplanetary Magnetic Field Lines Rooted in Active Regions  

Science Journals Connector (OSTI)

Electrons, accelerated in solar active regions to ? 10 keV, escape along open magnetic field lines and generate plasma radiation (Type III bursts ... Here we describe the latitude distribution of the field lines ...

G. A. Dulk; J. L. Steinberg; S. Hoang

1986-01-01T23:59:59.000Z

484

The fabrication of high quality silicon junction detectors by low energy ion implantation  

Science Journals Connector (OSTI)

High quality silicon junction detectors have been made by implantation of boron and phosphorus ions into silicon wafers. Resolutions of 20 keV for Po ?-particles were obtained.

S. Kalbitzer; R. Bader; H. Herzer; K. Bethge

1967-01-01T23:59:59.000Z

485

Determination of Mass Attenuation Coefficients for CuInSe2 and CuGaSe2 Semiconductors  

SciTech Connect

This work presents mass attenuation coefficients values of CuInSe2 and CuGaSe2 semiconductor thin films commonly used in photovoltaic devices. The mass attenuation coefficients were measured at different energies from 11.9 to 37.3 keV by using the secondary excitation method. Monochromatic photons were obtained using the Br, Sr, Mo, Cd, Te, Ba and Nd secondary targets. 59.5 keV gamma rays emitted from an annular Am-241 radioactive source were used to excite secondary targets. Characteristic X-rays emitted from secondary target were counted by a Si(Li) detector with a resolution of 0.16 keV at 5.9 keV. The measured values were compared with theoretical values calculated using WinXCOM program.

Celik, Ahmet; Cevik, Ugur; Baltas, Hasan; Bacaksiz, Emin [Department of Physics, Faculty of Arts and Sciences, Karadeniz Technical University, 61080 Trabzon (Turkey)

2007-04-23T23:59:59.000Z

486

PHYSICAL REVIEW C 75, 044305 (2007) Global study of the spectroscopic properties of the first 2+  

E-Print Network (OSTI)

more than 2 orders of magnitude, ranging below 100 keV in deformed actinide nuclei to a few Me be used for the entire chart of nuclei. The Skyrme family of functionals that is used in the present study

Bertsch George F.

487

18O Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 05142012) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 2003DA19 18O(, ): deduced resonance strengths 470 - 770 keV X4 02132012...

488

7Li Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 05142012) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 2004GY02 7Li(, ): deduced absolute resonance strengths 810 - 820 keV X4 02...

489

15N Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 05142012) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 2002WI18 15N( ): 461 - 2642 keV X4 09122011 1997WI12 15N( ): 0.65...

490

19F Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 01212015) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 2008UG01 19F(, p): yield curves, 792 - 1993 keV X4 09142011 2005UG04...

491

11B Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 01212015) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 1991WA02 11B(, n): thick-target yield of E 411, 605 and 606 keV resonance...

492

3He Cross Section  

NLE Websites -- All DOE Office Websites (Extended Search)

, X) (Current as of 05142012) NSR Reaction E (MeV) Cross Section File X4 Dataset Date Added 1982KR05 3He(, ): Ecm 107 - 1266 keV X4 01052012 1969NA24 3He(, ):...

493

Disintegration of Boron-10 by Protons  

Science Journals Connector (OSTI)

... -particles from the disintegration of boron-11 were eliminated by using a target of separated boron-10. The accompanying graph shows the number of particles counted as a function of current ... (1) at 630 keV. proton energy, and

W. E. BURCHAM; JOAN M. FREEMAN

1949-01-29T23:59:59.000Z

494

Design and Performance of a Novel Instrument for Soft-Landing...  

NLE Websites -- All DOE Office Websites (Extended Search)

ions was performed using 15 keV Ga+ time-of-flight secondary ion mass spectrometry (TOF-SIMS) and grazing incidence infrared reflection-absorption spectroscopy (IRRAS). It will be...

495

Charge Retention by Peptide Ions Soft-Landed onto Self-Assembled...  

NLE Websites -- All DOE Office Websites (Extended Search)

spectrometry or ex situ 15 keV Ga+ time-of-flight secondary ion mass spectrometry (ToF-SIMS). The results demonstrate that a fraction of multiply protonated peptide ions retain...

496

First gaseous boronization during pulsed discharge cleaning  

NLE Websites -- All DOE Office Websites (Extended Search)

6 2 keV, and a pulse length of 60 ms. The vertical equilibrium field is provided by the image currents inside the 50 mm thick, high-conductivity aluminum (6061-T6) vacuum vessel...

497

Real-time RBS analysis of plasma erosion in DIONISOS  

E-Print Network (OSTI)

One of the primary scientific challenges still facing the development of commercial nuclear fusion reactors lies at the plasma-material boundary. Plasma temperatures greater than 10 million degrees Celsius (10 keV) require ...

Peterson, Ethan E. (Ethan Eric)

2013-01-01T23:59:59.000Z

498

E-Print Network 3.0 - axisymmetric electron beam Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

. Factors controlling the plasma electron temperature when heated by 18-20keV neutral beams with a power... from periphery, electron temperatures of 150-160eV were obtained with...

499

Patents -- Georges Charpak (1991-2000)  

Office of Scientific and Technical Information (OSTI)

elements. The primary electrons emitted by the radioelements are accelerated to an energy level lying between 20 keV and 1 MeV by means of an electric field E applied...

500

XMM-Newton study of the ULIRG NGC 6240  

E-Print Network (OSTI)

A recently performed XMM-Newton observation of the ULIRG NGC 6240 clearly indicates the presence of an AGN contribution to its X-ray spectrum. In the 5.0 - 7.0 keV energy range there is a clear signature of the fluorescent Fe K lines at 6.4, 6.7 and 6.9 keV, respectively. The line strength of the 6.4 keV line cannot be produced by a thermal component. The 0.3 - 10.0 keV spectral energy distribution is characterized by the following components: (I) two hot thermal components (the starburst), (II) one direct component (heavily absorbed; AGN is hidden), (III) one reflection component (the AGN), (IV) three narrow Fe lines. The model parameters for the broad-band spectral energy distribution are consistent with the results of previously works.

Ralf Keil; Th. Boller; R. Fujimoto

2001-06-12T23:59:59.000Z