Powered by Deep Web Technologies
Note: This page contains sample records for the topic "broken bow ne" 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.


1

Broken Bow Wind Farm | Open Energy Information  

Open Energy Info (EERE)

Bow Wind Farm Bow Wind Farm Jump to: navigation, search Name Broken Bow Wind Farm Facility Broken Bow Wind Farm Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Midwest Wind Energy Developer Midwest Wind Energy Energy Purchaser Nebraska Public Power District Location Custer County, Nebraska Coordinates 41.400029°, -99.573412° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.400029,"lon":-99.573412,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

2

City of Broken Bow, Nebraska (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Bow, Nebraska (Utility Company) Bow, Nebraska (Utility Company) Jump to: navigation, search Name City of Broken Bow Place Nebraska Utility Id 2277 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes Operates Generating Plant Yes Activity Generation Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Area Lights (Metered) 175 W sod-vap - city Lighting Area Lights (Metered) 175 W sod-vap - rural Lighting Area Lights (Unmetered) 1000 W mer-vap - city Lighting Area Lights (Unmetered) 1500 W quartz - city Lighting Area Lights (Unmetered) 175 W sod-vap - city Lighting

3

Bows and Arrows -- Part One: The Bow  

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

One: The Bow One: The Bow Nature Bulletin No. 592 February 20, 1960 Forest Preserve District of Cook County Daniel Ryan, President Roberts Mann, Conservation Editor David H. Thompson, Senior Naturalist BOWS AND ARROWS: PART ONE THE BOW Primitive man, although at different times in various parts of the world, seems to have passed through three stages of development. During what is called the Old Stone Age he discovered how to make and use fire but had only clubs, stones and crudely shaped axes as weapons. During the Middle Stone Age he invented the spear, perhaps a throwing stick to hurl it, and finally the bow and arrow. Then man became a match for the mammoth, mastodon, cave bear, saber-toothed tiger or any predator. Then he was able to kill his food at a distance, or from a hiding place, with less risk of his life Then, too, he was enabled to ambush an enemy instead of meeting him in desperate hand-to-hand conflict.

4

Broken Symmetry  

ScienceCinema (OSTI)

- Physics, as we know it, attempts to interpret the diverse natural phenomena as particular manifestations of general laws. This vision of a world ruled by general testable laws is relatively recent in the history of mankind. Basically it was initiated by the Galilean inertial principle. The subsequent rapid development of large-scale physics is certainly tributary to the fact that gravitational and electromagnetic forces are long-range and hence can be perceived directly without the mediation of highly sophisticated technical devices. - The discovery of subatomic structures and of the concomitant weak and strong short-range forces raised the question of how to cope with short-range forces in relativistic quantum field theory. The Fermi theory of weak interactions, formulated in terms of point-like current-current interaction, was well-defined in lowest order perturbation theory and accounted for existing experimental data.However, it was inconsistent in higher orders because of uncontrollable divergent quantum fluctuations. In technical terms, in contradistinction to quantum electrodynamics, the Fermi theorywas not ?renormalizable?. This difficulty could not be solved by smoothing the point-like interaction by a massive, and therefore short-range, charged ?vector? particle exchange: theories with massive charged vector bosons were not renormalizable either. In the early nineteen sixties, there seemed to be insuperable obstacles to formulating a consistent theory with short-range forces mediated by massive vectors. - The breakthrough came from the notion of spontaneous symmetry breaking which arose in the study of phase transitions and was introduced in field theory by Nambu in 1960. - Ferromagnets illustrate the notion in phase transitions. Although no direction is dynamically preferred, the magnetization selects a global orientation. This is a spontaneous broken symmetry(SBS)of rotational invariance. Such continuous SBS imply the existence of ?massless? modes (here spin-waves), which are the ancestors of the NG bosons discussed below. Fluctuations of the order parameter (the magnetization) are described by a ?massive? SBS mode. - In field theory, Nambu showed that broken chiral symmetry from a spontaneous generation of hadron masses induces massless pseudoscalar modes (identified with a massless limit of pion fields). This illustrates a general phenomenon made explicit by Goldstone: massless Nambu-Goldstone (NG) bosons are a necessary concomitant of spontaneously broken continuous symmetries. Massive SBS scalars bosons describe, as in phase transitions, the fluctuations of the SBS order parameters. - In 1964, with Robert Brout, we discovered a mechanism based on SBS by which short range interactions are generated from long range ones. A similar proposal was then made independently by Higgs in a different approach. Qualitatively, our mechanism works as follows. The long range fundamental electromagnetic and gravitational interactions are governed by extended symmetries,called gauge symmetries, which were supposed to guarantee that the elementary field constituents which transmit the forces, photons or gravitons, be massless. We considered a generalization of the electromagnetic ?vector? field, known as Yang-Mills fields, and coupled them to fields which acquire from SBS constant values in the vacuum. These fields pervade space, as did magnetization, but they have no spatial orientation: they are ?scalar?? fields. The vector Yang-Mills fields which interact with the scalar fields become massive and hence the forces they mediate become short ranged. We also showed that the mechanism can survive in absence of elementary scalar fields. - Because of the extended symmetries, the nature of SBS is profoundly altered: the NG fields are absorbed into the massive vector Yang-Mills fields and restore the gauge symmetry. This has a dramatic consequence. To confront precision experiments, the mechanism should be consistent at the quantum mechanical level, or in technical terms, should yield a ?renormalizable? theory. From our analysi

None

2011-10-06T23:59:59.000Z

5

Broken Bow, Nebraska: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

9509°, -99.6392794° 9509°, -99.6392794° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.4019509,"lon":-99.6392794,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

6

NE Pacific St. NE Pacific St.  

E-Print Network (OSTI)

Lake W ashington Ship Canal NE Pacific St. NE Pacific St. NE Boat St. 15th Ave NE 15thAveNE UniversityWayNE BrooklynAveNE NE Pacific St. MontlakeBlvdNE MontlakeBlvdNE Pacific Place NE University Burke-Gilman Trail METRO NW A CD D EF F GHI H J RR BB CC EE AA Rotunda Cafe Ocean Sciences Hitchcock

7

BooNE: About BooNE  

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

Information BooNE Collaboration BooNE Experiment BooNE vs MiniBooNE Interesting Facts Posters Virtual Tour Picture Gallery News Articles BooNE photo montage Technical Information...

8

Broken baby Skyrmions  

Science Journals Connector (OSTI)

...centre of the soliton, and the three points on the equator midway between the equatorial vacua, such as phi =(1,0,0). In the broken baby Skyrme model, the potential at a midway point is greater than the potential at the soliton centre...

2012-01-01T23:59:59.000Z

9

Magnetically dominated MHD bow shock ows  

E-Print Network (OSTI)

Chapter 7 Magnetically dominated MHD bow shock ows: three-dimensional ow over a sphere spheres. Fig. 7.1 shows a 3D visualization of a bow shock ow around a sphere with magnetically dominated uniform upstream ow (switch-on shocks occur). In the 3D ow magnetic #12;eld lines can slip over

De Sterck, Hans

10

Reconnecting broken blood vessels  

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

Reconnecting broken blood vessels Reconnecting broken blood vessels Name: Catherine A Kraft Status: N/A Age: N/A Location: N/A Country: N/A Date: N/A Question: While watching the television program "Chicago Hope" the other day, I watched a doctor sew someone's ear back on using an elaborate microscope. I was wondering if a surgeon is required to reconnect all the broken blood vessels, and how you would accomplish this? Thanks for your time! Replies: I'm not a surgeon, but I think the answer to your question is "no." The blood will flow across the wound (out the end of one blood vessel and into the end of another), although not efficiently. I believe they sometimes use leeches sucking on the end of the reconnected part to help induce flow of blood in the right direction through the area. You probably do need to put the ends of the major vessels near each other, so the distribution of blood flow is reasonably like it was before the injury, and so the vessels can eventually reconnect. But probably the microscope is used mostly to be sure the various layers of muscle, connective tissue, and fat are connected together correctly.

11

NE-23,  

Office of Legacy Management (LM)

t:"'. ? - ' t:"'. ? - ' y5 NE-23, wk$& Dr. Joseph A. Warburton Chainnan, Radiological and Toxicological Safety Board University of Nevada System DRI/ASC, P.O. Box 60220 Reno, Nevada 89506 Dear Dr. Warburton: The Department of Energy (DOE), as part of its Formerly Utilized Sites Remedial Action Program (FUSRAP), has reviewed information on the Mackay School of M ines facility at the University of Nevada, Reno, Nevada, to determine whether it contains residual radioactivity traceable to activities conducted on behalf of the Atomic Energy Commission (a predecessor to DOE). A radiological survey indicated that the radiation levels at the involved portion of the facility are at or near background levtrls. Therefore, no remedial action is required, and DGE is eliminating

12

NE-24  

Office of Legacy Management (LM)

VW- VW- 50 "id AU6 3 1983 NE-24 .' . _ : ' : R&D Decontamination Projects Under the Formerly Utilized Sites Remedial Actlon Program (FUSRAP) '_ F .- ,: 'J,.LaGrone, Manager . Oak Ridge Operations Office As a result of the House-Senate Conference Report and the Energy and Water Appropriations Act for FY 1984, and based on the data in the attached reports indicating radioactive contamination in excess of acceptable guidelines, the sites listed in the attachment and their respective vicinity properties (contaminated with radioactive materials from these sites) are being designated as decontamination research and development projects under the FUSRAP. Each site and the associated vicinity properties should be treated as a separate project. The objective of each project is to decontaminate the vicinity properties

13

NE-20  

Office of Legacy Management (LM)

hi v. !&-2:. hi v. !&-2:. /qL lo 1 OCT 2 9 1984 NE-20 -. Authorization for Remedial Action of the Ashland 2 Site, Tonawanda, New York f! Joe LaGrone, Manager Oak Ridge Operations Office Based on the Aerial Radiological Survey (Attachment 1) and a "walk-on" radiologlcal survey (Attachment 2 , excerpted from the ORNL draft report "Ground-Level Investigation of Anomalous Gamma Radiation Levels in the Tonawanda, New York, Area," January 1980), the property identified as Ashland 2 is authorized for remedial action. It should be noted that the attached survey data are for designation purposes only and Bechtel National, Inc. (EM), should conduct appropriate comprehensive characterization surveys to determine the extent and magnitude of the

14

On the broken ray transform  

E-Print Network (OSTI)

This PhD thesis studies the broken ray transform, a generalization of the geodesic X-ray transform where geodesics are replaced with broken rays that reflect on a part of the boundary. The fundamental question is whether this transform is injective. We employ four different methods to approach this question, and each of them gives interesting results. Direct calculation can be used in a ball, where the geometry is particularly simple. If the reflecting part of the boundary is (piecewise) flat, a reflection argument can be used to reduce the problem to the usual X-ray transform. In some geometries one can use broken rays near the boundary to determine the values of the unknown function at the reflector, and even construct its Taylor series. One can also use energy estimates -- which in this context are known as Pestov identities -- to show injectivity in the presence of one convex reflecting obstacle. Many of these methods work also on Riemannian manifolds. We also discuss the periodic broken ray transform, where the integrals are taken over periodic broken rays. The broken ray transform and its periodic version have applications in other inverse problems, including Calder\\'on's problem and problems related to spectral geometry. A more detailed abstract can be found in the PDF file. This version only contains the introductory parts of the thesis. The full thesis also contains five articles.

Joonas Ilmavirta

2014-09-26T23:59:59.000Z

15

Classroom demonstration of the vibration of a bowed string  

Science Journals Connector (OSTI)

An overhead projector has been modified for stroboscopic illumination for the purpose of demonstrating the vibration of a string excited by a violinbow. The vibrational pattern is clearly delineated as are differences caused by insufficient or excessive bow force. A regime of oscillation is noted at high bow force and low speed in which alternate waves are reflected from the bow and the bridge so that the vibration transmitted to the bridge is about an octave below the fundamental frequency of the string.

E. Brock Dale

1976-01-01T23:59:59.000Z

16

How Do You Mend a Broken Heart?  

E-Print Network (OSTI)

Rebounding from a broken heart, then, may not so dissimilarHow Do You Mend a Broken Heart? It was seven hours into ourartists often do: they put their hearts on display. Cobbling

Service, Shannon

2012-01-01T23:59:59.000Z

17

How Do You Mend a Broken Heart?  

E-Print Network (OSTI)

Rebounding from a broken heart, then, may not so dissimilarHow Do You Mend a Broken Heart? It was seven hours into ourartists often do: they put their hearts on display. Cobbling

Service, Shannon

2011-01-01T23:59:59.000Z

18

BooNE: Picture Gallery  

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

Picture Gallery BooNE Collaboration Members of the BooNE collaboration Civil Construction Pictorial progress of BooNE civil construction work Detector Installation Pictorial...

19

BooNE Collaboration  

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

Collaboration The BooNE collaboration consists of approximately sixty-five physicists from 13 institutions. While small on the scale of high energy physics experiments, BooNE...

20

NE Blog Archive  

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

ne/blog-archive 1000 Independence Ave. SWWashington DC ne/blog-archive 1000 Independence Ave. SWWashington DC 20585202-586-5000 en Generation IV International Forum Updates Technology Roadmap and Builds Future Collaboration http://energy.gov/ne/articles/generation-iv-international-forum-updates-technology-roadmap-and-builds-future ne/articles/generation-iv-international-forum-updates-technology-roadmap-and-builds-future" class="title-link">Generation IV International Forum Updates Technology Roadmap and Builds Future Collaboration

Note: This page contains sample records for the topic "broken bow ne" 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

Medicine Bow Wind Farm I | Open Energy Information  

Open Energy Info (EERE)

Medicine Bow Wind Farm I Medicine Bow Wind Farm I Facility Medicine Bow Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Platte River Power Authority Developer Platte River Power Authority Energy Purchaser Platte River Power Authority Location Medicine Bow WY Coordinates 41.927554°, -106.371968° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.927554,"lon":-106.371968,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

22

Medicine Bow Wind Farm IV | Open Energy Information  

Open Energy Info (EERE)

Medicine Bow Wind Farm IV Medicine Bow Wind Farm IV Facility Medicine Bow Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Platte River Power Authority Developer Northern Alternative Energy Energy Purchaser Platte River Power Authority Location Medicine Bow WY Coordinates 41.927554°, -106.371968° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.927554,"lon":-106.371968,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

23

Bows and Arrows -- Part Two: Arrows and Archers  

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

Two: Arrows and Archers Two: Arrows and Archers Nature Bulletin No. 593 February 27, 1960 Forest Preserve District of Cook County Daniel Ryan, President Roberts Mann, Conservation Editor Richard Becker, Naturalist BOWS AND ARROWS - PART TWO: ARROWS AND ARCHERS Archery, and hunting with a bow, are sports increasingly popular in this country. Bows and arrows are still used by primitive tribes, such as the pigmies in Africa and the aborigines in South American jungles, who frequently tip their arrows with deadly poisons. The warlike Indians of the Great Plains used bows and arrows long after the introduction of firearms. Loading an old-fashioned musket took too much time and was difficult for a brave on a running horse. After repeating rifles appeared, they and cartridges for them were greatly prized but hard to get.

24

Medicine Bow Wind Farm III | Open Energy Information  

Open Energy Info (EERE)

Medicine Bow Wind Farm III Medicine Bow Wind Farm III Facility Medicine Bow Sector Wind energy Facility Type Small Scale Wind Facility Status In Service Owner Platte River Power Authority Developer Platte River Power Authority Energy Purchaser Platte River Power Authority Location Medicine Bow WY Coordinates 41.927554°, -106.371968° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.927554,"lon":-106.371968,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

25

Medicine Bow Wind Farm II | Open Energy Information  

Open Energy Info (EERE)

Medicine Bow Wind Farm II Medicine Bow Wind Farm II Jump to: navigation, search Name Medicine Bow Wind Farm II Facility Medicine Bow Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Platte River Power Authority Developer Platte River Power Authority Energy Purchaser Platte River Power Authority Location Medicine Bow WY Coordinates 41.927554°, -106.371968° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.927554,"lon":-106.371968,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

26

Elementary stability considerations for bowed?string motion  

Science Journals Connector (OSTI)

Using the approach first pioneered by Raman the Helmholtz motion of a bowed string is discussed as a special case of two?velocity motions in which a given point (at which the bow is located) alternates in the course of a cycle between two constant velocities. The fact that the bow typically presents a negative resistance to the string during the slipping part of the cycle is adduced as a reason for the duty cycle that is the fraction of the period that corresponds to slipping to try to become as short as possible. It is shown that for a string without dissipation or stiffness this duty cycle can be arbitrarily low for general bow positions; data obtained with the digital bow illustrate this behavior. It is shown theoretically and confirmed with computer simulations that instabilities arising from the negative slipping resistance cannot be eliminated by assigning a finite positive value to the sticking resistance. The apparent stability of Helmholtz motion observed in real playing situations remains a puzzle.

Gabriel Weinreich; Ren Causs

1991-01-01T23:59:59.000Z

27

BooNE: Posters  

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

Posters What's a Neutrino? How neutrinos fit into our understanding of the universe. Recipe for a Neutrino Beam Start with some protons... concocting the MiniBooNE beam. The...

28

20Ne 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 1983SC17 20Ne(, ): deduced S-factor of capture 0.55 - 3.2 X4 09152011...

29

EIS-0432: Medicine Bow Fuel & Power Coal-to-Liquid Facility in...  

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

2: Medicine Bow Fuel & Power Coal-to-Liquid Facility in Carbon County, WY EIS-0432: Medicine Bow Fuel & Power Coal-to-Liquid Facility in Carbon County, WY Documents Available for...

30

Eliyahu Ne'eman  

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

Eliyahu Ne'eman Eliyahu Ne'eman Consulting Engineer on Lighting and Daylighting Lawrence Berkeley National Laboratory This speaker was a visiting speaker who delivered a talk or talks on the date(s) shown at the links below. This speaker is not otherwise associated with Lawrence Berkeley National Laboratory, unless specifically identified as a Berkeley Lab staff member. Eliyahu Ne'eman is a leading international expert on lighting and daylighting. He has been involved in education, research and practice for over 40 years while working in Israel, UK, Germany and the US(LBNL). He has worked extensively in the area of occupant response in luminous spaces and he has been leading the CIE Task Group that has revised the CIE Museum Lighting Guide. This Speaker's Seminars Control of Damage to Museum Objects by Optical Radiation

31

20Ne Cross Section  

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

p, X) (Current as of 05152012) NSR Reaction Ep (MeV) Cross Section File X4 Dataset Date Added 1981DY03 20Ne(p, p'): for production of -rays threshold - 23 1.63-MeV -rays...

32

Bristol Heart Institute issue broken heart  

E-Print Network (OSTI)

Bristol Heart Institute issue Mending a broken heart The energy powerhouse Plaques, cracks and heart attacks re:search University of Bristol · June 2006 #12;BRISTOL HEART INSTITUTE ISSUE · JUNE 2006 THE BRISTOL HEART INSTITUTE 1 C ardiovascular disease is the UK's single biggest killer of both men and women

Bristol, University of

33

Broken Scale Invariance and Anomalous Dimensions  

DOE R&D Accomplishments (OSTI)

Mack and Kastrup have proposed that broken scale invariance is a symmetry of strong interactions. There is evidence from the Thirring model and perturbation theory that the dimensions of fields defined by scale transformations will be changed by the interaction from their canonical values. We review these ideas and their consequences for strong interactions.

Wilson, K. G.

1970-05-00T23:59:59.000Z

34

BooNE: Booster Neutrino Experiment  

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

Picture Gallery BooNE Collaboration Members of the BooNE collaboration Civil Construction Pictorial progress of BooNE civil construction work Detector Installation Pictorial...

35

BooNE: Booster Neutrino Experiment  

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

Collaboration Booster Neutrino Experiment (BooNE) BooNE vs MiniBooNE Interesting Facts Posters Virtual Tour Picture Gallery News Articles Technical Information BooNE Proposal...

36

Effective Field Theory of Broken Spatial Diffeomorphisms  

E-Print Network (OSTI)

We study the low energy effective theory describing gravity with broken spatial diffeomorphism invariance. In the unitary gauge, the Goldstone bosons associated with broken diffeomorphisms are eaten and the graviton becomes a massive spin-2 particle with 5 well-behaved degrees of freedom. In this gauge, the most general theory is built with the lowest dimension operators invariant under only temporal diffeomorphisms. Imposing the additional shift and SO(3) internal symmetries, we analyze the perturbations on a FRW background. At linear perturbation level, the observables of this theory are characterized by six parameters, including the usual cosmological parameters and two additional coupling constants for the symmetry-breaking scalars. We discuss several examples relevant to theories of massive gravity.

Lin, Chunshan

2015-01-01T23:59:59.000Z

37

How can R parity be broken?  

Science Journals Connector (OSTI)

The most popular model of spontaneous R-parity breaking is analyzed. It is shown that the extremum of the potential found in the model is, in fact, an unstable saddle point, while in the true minimum R parity is not broken. Other existing models involving R-parity breaking are briefly discussed and it is pointed out that none of them can describe successfully the existing experimental data.

M. Chaichian and A. V. Smilga

1992-03-09T23:59:59.000Z

38

Excitation functions of the Ne20+20Ne system  

Science Journals Connector (OSTI)

A differentially pumped windowless Ne20 gas target and a Ne20 beam produced with the ATLAS accelerator at Argonne National Laboratory were used to measure angle-averaged excitation functions for binary decay of Ne20+20Ne into low-lying states of Ne20+20Ne and Mg24+16O, in the region of excitation energy in Ca40 from 51.4 to 58.2 MeV (20Ne beam energies from 61.8 to 75.4 MeV). The Ne20+20Ne mass partition displays little correlated structure and there exists no evidence of intermediate width resonances in these channels with branching ratios comparable to those seen in the Mg24+24Mg system. Angular distributions for the elastic channel are consistent with those obtained using optical-model calculations. The exictation functions for the low-lying channels in Mg24+16O do contain some structures, with widths varying from 400 to 800 keV in the c.m. system.

S. P. Barrow; R.W. Zurmhle; J. T. Murgatroyd; N. G. Wimer; Y. Miao; K. R. Pohl; A. H. Wuosmaa; R. R. Betts; M. Freer; B. Glagola

1995-04-01T23:59:59.000Z

39

Category:Omaha, NE | Open Energy Information  

Open Energy Info (EERE)

Omaha, NE Omaha, NE Jump to: navigation, search Go Back to PV Economics By Location Media in category "Omaha, NE" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Omaha NE Omaha Public Power District.png SVFullServiceRestauran... 63 KB SVHospital Omaha NE Omaha Public Power District.png SVHospital Omaha NE Om... 61 KB SVLargeHotel Omaha NE Omaha Public Power District.png SVLargeHotel Omaha NE ... 61 KB SVLargeOffice Omaha NE Omaha Public Power District.png SVLargeOffice Omaha NE... 63 KB SVMediumOffice Omaha NE Omaha Public Power District.png SVMediumOffice Omaha N... 65 KB SVMidriseApartment Omaha NE Omaha Public Power District.png SVMidriseApartment Oma... 62 KB SVOutPatient Omaha NE Omaha Public Power District.png SVOutPatient Omaha NE ...

40

NE-23 W  

Office of Legacy Management (LM)

>:-1. ,- '"CC3 >:-1. ,- '"CC3 . ' NE-23 .+ W h itm~ l-l& Mr. Victor 3. Canilov, Director Museum of Science and Industry East 57th Street and Lake Shore Drive Chicago, Illinois 60037 Dear kr. Danilov: The Department of Energy (DOE), as part of its Formerly Utilized Sites Remedial Action Program (FUSPSIP), has reviewed information on the Museum cf Science and Industry, Chicago, Illinois, to determine whether it contains residual radioactivity traceable to activities conducted on behalf of the Manhattan Engineer District or the Atomic Energy C o m m ission (predecessors to DOE). A radiological survey indicated that the radiation levels are equal to natural background. Therefore, no remedial action is required, ant DOE is eliminating the Museum of Science and Industry from further

Note: This page contains sample records for the topic "broken bow ne" 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

Dual-Doppler analysis of the 17 June 1997 bow echo over southeast Texas  

E-Print Network (OSTI)

not shown in conceptual models of bow echoes however is a distinct, smaller-scale, cyclonic vortex present along the northern front edge of the bow echo. This vortex seems to have formed from the tilting and subsequent stretching of vorticity generated...

Moncla, Kerry Louis

2012-06-07T23:59:59.000Z

42

Bowed string synthesis with force feedback gesture interaction Jean-Loup Florens, Cyrille Henry  

E-Print Network (OSTI)

Introduction In sustained oscillation instruments (like bow string instruments, reed instrumentsBowed string synthesis with force feedback gesture interaction Jean-Loup Florens, Cyrille Henry string, which closely links the properties of the produced sounds to the gesture and energetic investment

Paris-Sud XI, Université de

43

CAUSAL/ANTICAUSAL DECOMPOSITION FOR MIXED-PHASE DESCRIPTION OF BRASS AND BOWED STRING SOUNDS  

E-Print Network (OSTI)

CAUSAL/ANTICAUSAL DECOMPOSITION FOR MIXED-PHASE DESCRIPTION OF BRASS AND BOWED STRING SOUNDS, in order to lo- cally model divergent oscillations in a steady way [4]. This mixed-phase representation- ous interaction instruments (CII): brass and bowed string. The aim of this work is to better

Dupont, Stéphane

44

MiniBooNE Collaboration MiniBooNE Collaboration Yale University  

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

at MiniBooNE at MiniBooNE B. T. Fleming for the B. T. Fleming for the MiniBooNE Collaboration MiniBooNE Collaboration Yale University Yale University The LSND experiment...

45

6.4 A BOW-ECHO EVENT ON A SQUALL LINE IN THE NETHERLANDS Rob Groenland  

E-Print Network (OSTI)

6.4 A BOW-ECHO EVENT ON A SQUALL LINE IN THE NETHERLANDS Rob Groenland Meteo Consult, Wageningen, The Netherlands (Europe) ABSTRACT In this study, the structure of a bow-echo on a squall line is investigated . It accelerated as it moved into the Netherlands. A bow-echo developed over extreme northern Belgium

Haak, Hein

46

BooNE: Booster Neutrino Experiment  

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

collaboration Find here collaboration lists of MiniBooNE at various stages of the experiment Current MiniBooNE-darkmatter collaboration Original MiniBooNE collaboration From script...

47

BooNE: Booster Neutrino Experiment  

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

Scrapbook Page 2 The BooNE collaboration in winter. A tour of the construction site. Working with the BooNE Horn. BooNE in the winter A tour of the construction site. A day with...

48

Posters Monte Carlo Simulation of Longwave Fluxes Through Broken...  

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

5 Posters Monte Carlo Simulation of Longwave Fluxes Through Broken Scattering Cloud Fields E. E. Takara and R. G. Ellingson University of Maryland College Park, Maryland To...

49

Spectral characterizations of sun graphs and broken sun graphs  

E-Print Network (OSTI)

Spectral characterizations of sun graphs and broken sun graphs Romain Boulet 10 Dec 2009 Abstract- cyclic graphs. An odd (resp. even) sun is a graph obtained by appending a pendant vertex to each vertex of an odd (resp. even) cycle. A broken sun is a graph obtained by deleting pendant vertices of a sun

Paris-Sud XI, Université de

50

For the MicroBooNE Collaboration IPA2013  

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

Status of MicroBooNE Christina Ignarra (MIT) For the MicroBooNE Collaboration IPA2013 May 14, 2013 Motivation for MicroBooNE: MiniBooNE Motivation for MiniBooNE: LSND * LSND...

51

EIS-0432: Department of Energy Loan Guarantee for Medicine Bow Gasification  

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

2: Department of Energy Loan Guarantee for Medicine Bow 2: Department of Energy Loan Guarantee for Medicine Bow Gasification and Liquefaction Coal-to-Liquids, Carbon County, Wyoming EIS-0432: Department of Energy Loan Guarantee for Medicine Bow Gasification and Liquefaction Coal-to-Liquids, Carbon County, Wyoming Summary DOE is assessing the potential environmental impacts for its proposed action of issuing a Federal loan guarantee to Medicine Bow Fuel & Power LLC (MBFP), a wholly-owned subsidiary of DKRW Advanced Fuels LLC. MBFP submitted an application to DOE under the Federal loan guarantee program pursuant to the Energy Policy Act of 2005 to support the construction and startup of the MBFP coal-to-liquids facility, a coal mine and associated coal handling facilities. Public Comment Opportunities No public comment opportunities available at this time.

52

Propeller design optimization for tunnel bow thrusters in the bollard pull condition  

E-Print Network (OSTI)

Tunnel bow thrusters are often used by large ships to provide low-speed lateral maneuverability when docking. Required to provide high thrust while essentially at a standstill, the design point for these thrusters is the ...

Wilkins, James R., IV

2012-01-01T23:59:59.000Z

53

Physics and learning based computational models for breaking bow waves based on new boundary immersion approaches  

E-Print Network (OSTI)

A ship moving on the free surface produces energetic breaking bow waves which generate spray and air entrainment. Present experimental, analytic, and numerical studies of this problem are costly, inaccurate and not robust. ...

Weymouth, Gabriel David

2008-01-01T23:59:59.000Z

54

Bow shocks formed by plasma collisions in laser irradiated semi-cylindrical cavities  

E-Print Network (OSTI)

the axis to form a dense bright plasma focus. Later in time a long lasting bow shock is observed to develop a location near the cavity axis, where it collides forming a bright high density plasma focus

Rocca, Jorge J.

55

US NE MA Site Consumption  

Gasoline and Diesel Fuel Update (EIA)

NE MA NE MA Site Consumption million Btu $0 $500 $1,000 $1,500 $2,000 $2,500 $3,000 US NE MA Expenditures dollars ALL ENERGY average per household (excl. transportation) 0 2,000 4,000 6,000 8,000 10,000 12,000 US NE MA Site Consumption kilowatthours $0 $250 $500 $750 $1,000 $1,250 $1,500 US NE MA Expenditures dollars ELECTRICITY ONLY average per household * Massachusetts households use 109 million Btu of energy per home, 22% more than the U.S. average. * The higher than average site consumption results in households spending 22% more for energy than the U.S. average. * Less reliance on electricity for heating, as well as cool summers, keeps average site electricity consumption in the state low relative to other parts of the U.S. However, spending on electricity is closer to the national average due to higher

56

US NE MA Site Consumption  

U.S. Energy Information Administration (EIA) Indexed Site

NE MA NE MA Site Consumption million Btu $0 $500 $1,000 $1,500 $2,000 $2,500 $3,000 US NE MA Expenditures dollars ALL ENERGY average per household (excl. transportation) 0 2,000 4,000 6,000 8,000 10,000 12,000 US NE MA Site Consumption kilowatthours $0 $250 $500 $750 $1,000 $1,250 $1,500 US NE MA Expenditures dollars ELECTRICITY ONLY average per household * Massachusetts households use 109 million Btu of energy per home, 22% more than the U.S. average. * The higher than average site consumption results in households spending 22% more for energy than the U.S. average. * Less reliance on electricity for heating, as well as cool summers, keeps average site electricity consumption in the state low relative to other parts of the U.S. However, spending on electricity is closer to the national average due to higher

57

A review of "Richard Brathwait: The First Lakeland Poet" by John Bowes  

E-Print Network (OSTI)

reviews 21 John Bowes. Richard Brathwait: The First Lakeland Poet. Great Britain: Hugill Publications Ltd, 2007. viii + 256pp. ?12.95. Review by siobh?n collins, university college cork. The merits of John Bowes?s biography of Richard..., extravagant dress, greed, and bad reviews 23 behaviour? (87), traits which he himself exhibits at various stages of his life. His love of extravagant dress is presumably what gave rise to his nickname ?Dapper Dick,? which appears as ?Dagger Dick...

Collins, Siobhan

2010-01-01T23:59:59.000Z

58

Calculation of the reactivity feedback due to core-assembly bowing in LMFBRs  

SciTech Connect

The nonuniformity of the temperature distribution in an LMFBR leads to differential thermal expansion of the walls of an assembly hexcan. These thermal expansion differentials cause the hexcan to distort or bow. Consequentially, the assembly experiences a spatial displacement, which results in a change in reactivity for the core. A computational model to calculate the reactivity feedback due to material displacements induced by assembly bowing effects has been developed.

Not Available

1983-01-01T23:59:59.000Z

59

Three-dimensional hydrodynamic simulations of asymmetric pulsar wind bow shocks  

E-Print Network (OSTI)

We present three-dimensional, nonrelativistic, hydrodynamic simulations of bow shocks in pulsar wind nebulae. The simulations are performed for a range of initial and boundary conditions to quantify the degree of asymmetry produced by latitudinal variations in the momentum flux of the pulsar wind, radiative cooling in the postshock flow, and density gradients in the interstellar medium (ISM). We find that the bow shock is stable even when travelling through a strong ISM gradient. We demonstrate how the shape of the bow shock changes when the pulsar encounters density variations in the ISM. We show that a density wall can account for the peculiar bow shock shapes of the nebulae around PSR J2124-3358 and PSR B0740-28. A wall produces kinks in the shock, whereas a smooth ISM density gradient tilts the shock. We conclude that the anisotropy of the wind momentum flux alone cannot explain the observed bow shock morphologies but it is instead necessary to take into account external effects. We show that the analytic (single layer, thin shell) solution is a good approximation when the momentum flux is anisotropic, fails for a steep ISM density gradient, and ap- proaches the numerical solution for efficient cooling. We provide analytic expressions for the latitudinal dependence of a vacuum-dipole wind and the associated shock shape, and compare the results to a split-monopole wind. We find that we are unable to distinguish between these two wind models purely from the bow shock morphology.

M. Vigelius; A. Melatos; S. Chatterjee; B. M. Gaensler; P. Ghavamian

2006-10-16T23:59:59.000Z

60

Using numerical models of bow shocks to investigate the circumstellar medium of massive stars  

E-Print Network (OSTI)

Many massive stars travel through the interstellar medium at supersonic speeds. As a result they form bow shocks at the interface between the stellar wind. We use numerical hydrodynamics to reproduce such bow shocks numerically, creating models that can be compared to observations. In this paper we discuss the influence of two physical phenomena, interstellar magnetic fields and the presence of interstellar dust grains on the observable shape of the bow shocks of massive stars. We find that the interstellar magnetic field, though too weak to restrict the general shape of the bow shock, reduces the size of the instabilities that would otherwise be observed in the bow shock of a red supergiant. The interstellar dust grains, due to their inertia can penetrate deep into the bow shock structure of a main sequence O-supergiant, crossing over from the ISM into the stellar wind. Therefore, the dust distribution may not always reflect the morphology of the gas. This is an important consideration for infrared observati...

van Marle, Allard Jan; Cox, Nick; Meliani, Zakaria

2014-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

Posters Mean Fluxes of Visible Solar Radiation in Broken Clouds  

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

7 Posters Mean Fluxes of Visible Solar Radiation in Broken Clouds V. E. Zuev, G. A. Titov, T. B. Zhuravleva, and S. Y. Popov Institute of Atmospheric Optics, Siberian Branch...

62

BooNE: Booster Neutrino Experiment  

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

CA A Search for numu Disappearance with SciBooNE and MiniBooNE PowerPoint Z. Pavlovic Low Energy Neutrino Oscillations G. Zeller Neutrino-Nucleus Cross Sections G. Mills Neutrino...

63

BooNE: Booster Neutrino Experiment  

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

J.L.Raaf NOON 2004 February 11-15, 2004 Tokyo, Japan MiniBooNE Status NA B. Louis 2004 Venice, Italy MiniBooNE NA G. Zeller 2nd International Workshop on Neutrino-Nucleus...

64

BooNE: Booster Neutrino Experiment  

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

a variety of experiments. image: neutrino event types in oil for the MiniBooNE flux This pie chart shows the resultant event fractions at MiniBooNE before any selection cuts. The...

65

NE  

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

h i n g t o n M u l t n o m a h C o . O r e g o n M u l t n o m a h C o . O r e g o n Troutdale N E I O N E L O O P SW PAR K ST NW IVY ST NW ELM ST N W 1 8 T H L O O P S W 5 T H A...

66

Anisotropy in Broken Cloud Fields Over Oklahoma from Ladsat Data  

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

Anisotropy in Broken Cloud Fields Over Oklahoma Anisotropy in Broken Cloud Fields Over Oklahoma from Landsat Data L. M. Hinkelman National Institute of Aerospace Hampton, Virginia K. F. Evans University of Colorado Boulder, Colorado Introduction Previously, it was shown (Hinkelman et al. 2002) that anisotropy, or the existence of a preferred direction, in cumulus fields significantly affects solar radiative transfer through these fields. In this poster, we investigate the occurrence of anisotropy in broken cloud fields near the Atmospheric Radiation Measurement (ARM) Program Southern Great Plains (SGP) site imaged by the Landsat 7 enhanced thematic mapper (ETM). Method Sample Landsat scenes of cumuloform clouds with different types of organization over Central Oklahoma, including the ARM Cloud and Radiation Testbed site to the northeast, were obtained from

67

Image upload with broken thumbnail image | OpenEI Community  

Open Energy Info (EERE)

Image upload with broken thumbnail image Image upload with broken thumbnail image Home > Groups > Developer Rmckeel's picture Submitted by Rmckeel(297) Contributor 20 July, 2012 - 07:55 bug images wiki OpenEI users can upload images to the wiki by typing a new file name http://en.openei.org/wiki/File:My_new_file.jpg However, due to a caching timing issue, right after upload, the 120px-wide thumbnail has not yet been created by the time the fetier cache goes after it. Thus, the thumbnail appears broken. Is anyone up for debugging? For users uploading images, this can be fixed by forcing a reload of the page: Windows: ctrl + F5 Mac/Apple: Apple + R or command + R Linux: F5 Thanks! DIAGNOSTIC INFORMATION: BROKEN THUMBNAIL IMAGE HEADERS (RIGHT IMAGE, BUT CACHED BEFORE THUMBNAIL CREATED): Request URL:http://prod-http-80-800498448.us-east-1.elb.amazonaws.com/w/images/thumb/4/44/Powered_by_OpenEI_196x49_sc.png/120px-Powered_by_OpenEI_196x49_sc.png

68

Overview of NE Research Programs  

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

NE Research Programs NE Research Programs Sue Lesica Office of Nuclear Energy U.S. Department of Energy July 31, 2013 2 R&D Budgets FY 2013 FY 2014 Congressional Request House Mark Senate Mark SMR Licensing Technical Support 62,999 70,000 110,000 70,000 Small Modular Reactor R&D 23,958 20,000 20,000 20,000 Next Generation Nuclear Plant 38,720 0 0 0 LWR Sustainability 24,218 21,500 21,500 21,500 Advanced Reactor Concepts 21,178 31,000 45,000 21,000 Reactor Concepts RD&D 108,075 72,500 86,500 62,500 Modeling and Simulation Hub 24,588 24,300 24,300 24,300 Crosscutting Technology Development 17,242 13,901 27,885 25,437 NEAMS 13,646 9,536 National Scientific Users Facility 14,563 14,563 14,563 14,563 Nuclear Energy Enabling Technologies 70,040 62,300 66,748 62,300

69

Specification of an Infinite-State Local Model Checker in Rewriting Logic Bow-Yaw Wang  

E-Print Network (OSTI)

Specification of an Infinite-State Local Model Checker in Rewriting Logic Bow-Yaw Wang Institute logic and use it to analyze an infinite-state system in this paper. In order not to pursue infinite computation path endlessly, we perform bounded proof search on the system. Inconclusive proofs occurred

Wang, Bow-Yaw

70

Larmor radius size density holes discovered in the solar wind upstream of Earth's bow shock  

E-Print Network (OSTI)

Larmor radius size density holes discovered in the solar wind upstream of Earth's bow shock G. K, University of New Brunswick, Canada M. L. Goldstein NASA Goddard Space Flight Center, Greenbelt, Maryland P that are five or more times the solar wind density. Particle distributions show the steepened edge can behave

California at Berkeley, University of

71

X-RAY EMISSION LINE PROFILES FROM WIND CLUMP BOW SHOCKS IN MASSIVE STARS  

SciTech Connect

The consequences of structured flows continue to be a pressing topic in relating spectral data to physical processes occurring in massive star winds. In a preceding paper, our group reported on hydrodynamic simulations of hypersonic flow past a rigid spherical clump to explore the structure of bow shocks that can form around wind clumps. Here we report on profiles of emission lines that arise from such bow shock morphologies. To compute emission line profiles, we adopt a two-component flow structure of wind and clumps using two 'beta' velocity laws. While individual bow shocks tend to generate double-horned emission line profiles, a group of bow shocks can lead to line profiles with a range of shapes with blueshifted peak emission that depends on the degree of X-ray photoabsorption by the interclump wind medium, the number of clump structures in the flow, and the radial distribution of the clumps. Using the two beta law prescription, the theoretical emission measure and temperature distribution throughout the wind can be derived. The emission measure tends to be power law, and the temperature distribution is broad in terms of wind velocity. Although restricted to the case of adiabatic cooling, our models highlight the influence of bow shock effects for hot plasma temperature and emission measure distributions in stellar winds and their impact on X-ray line profile shapes. Previous models have focused on geometrical considerations of the clumps and their distribution in the wind. Our results represent the first time that the temperature distribution of wind clump structures are explicitly and self-consistently accounted for in modeling X-ray line profile shapes for massive stars.

Ignace, R. [Department of Physics and Astronomy, East Tennessee State University, Johnson City, TN 37614 (United States); Waldron, W. L. [Eureka Scientific Inc., 2452 Delmer Street, Oakland, CA 94602 (United States); Cassinelli, J. P. [Department of Astronomy, University of Wisconsin-Madison, Madison, WI 53711 (United States); Burke, A. E., E-mail: ignace@etsu.edu, E-mail: wwaldron@satx.rr.com, E-mail: cassinelli@astro.wisc.edu, E-mail: burke.alexander@gmail.com [990 Washington Street 317, Dedham, MA 02026 (United States)

2012-05-01T23:59:59.000Z

72

Mach 5 bow shock control by a nanosecond pulse surface dielectric barrier discharge  

SciTech Connect

Bow shock perturbations in a Mach 5 air flow, produced by low-temperature, nanosecond pulse, and surface dielectric barrier discharge (DBD), are detected by phase-locked schlieren imaging. A diffuse nanosecond pulse discharge is generated in a DBD plasma actuator on a surface of a cylinder model placed in air flow in a small scale blow-down supersonic wind tunnel. Discharge energy coupled to the actuator is 7.3-7.8 mJ/pulse. Plasma temperature inferred from nitrogen emission spectra is a few tens of degrees higher than flow stagnation temperature, T = 340 {+-} 30 K. Phase-locked Schlieren images are used to detect compression waves generated by individual nanosecond discharge pulses near the actuator surface. The compression wave propagates upstream toward the baseline bow shock standing in front of the cylinder model. Interaction of the compression wave and the bow shock causes its displacement in the upstream direction, increasing shock stand-off distance by up to 25%. The compression wave speed behind the bow shock and the perturbed bow shock velocity are inferred from the Schlieren images. The effect of compression waves generated by nanosecond discharge pulses on shock stand-off distance is demonstrated in a single-pulse regime (at pulse repetition rates of a few hundred Hz) and in a quasi-continuous mode (using a two-pulse sequence at a pulse repetition rate of 100 kHz). The results demonstrate feasibility of hypersonic flow control by low-temperature, repetitive nanosecond pulse discharges.

Nishihara, M.; Takashima, K.; Rich, J. W.; Adamovich, I. V. [Michael A. Chaszeyka Nonequilibrium Thermodynamics Laboratories, Department of Mechanical and Aerospace Engineering, Ohio State University, Columbus, Ohio 43210 (United States)

2011-06-15T23:59:59.000Z

73

Discrete Applied Mathematics 121 (2002) 139153 NeST graphs  

E-Print Network (OSTI)

Discrete Applied Mathematics 121 (2002) 139­153 NeST graphs Ryan B. Haywarda; , Paul E. Kearneyb; received in revised form 14 March 2001; accepted 26 March 2001 Abstract We establish results on NeST graphs show the equivalence of proper NeST graphs and unit NeST graphs, the equivalence of ÿxed distance NeST

Hayward, Ryan B.

74

Broken Arrow, Oklahoma: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Broken Arrow, Oklahoma: Energy Resources Broken Arrow, Oklahoma: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 36.0525993°, -95.7908195° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.0525993,"lon":-95.7908195,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

75

Yoichiro Nambu and the Mechanism of Spontaneous Broken Symmetries in  

Office of Scientific and Technical Information (OSTI)

Yoichiro Nambu and the Mechanism of Yoichiro Nambu and the Mechanism of Spontaneous Broken Symmetries in Subatomic Physics Resources with Additional Information · Awards Yoichiro Nambu Credit: University of Chicago Yoichiro Nambu was awarded the 2008 Nobel Prize in Physics "for the discovery of the mechanism of spontaneous broken symmetry in subatomic physics". Nambu 'has revolutionized modern scientific ideas about the nature of the most fundamental particles and the space through which they move. His theories form an essential cornerstone of what physicists call the Standard Model, which explains in a unified way three of the four fundamental forces of nature: strong, weak and electromagnetic. He also has significantly influenced the development of quantum chromodynamics, a theory that describes certain interactions between quarks and between protons and neutrons.' 1

76

Consistency condition for inflation from (broken) conformal symmetry  

SciTech Connect

We investigate the symmetry constraints on the bispectrum, i.e. the three-point correlation function of primordial density fluctuations, in slow-roll inflation. It follows from the defining property of slow-roll inflation that primordial correlation functions inherit most of their structure from weakly broken de Sitter symmetries. Using holographic techniques borrowed from the AdS/CFT correspondence, the symmetry constraints on the bispectrum can be mapped to a set of stress-tensor Ward identities in a weakly broken 2+1-dimensional Euclidean CFT. We construct the consistency condition from these Ward identities using conformal perturbation theory. This requires a second order Ward identity and the use of the evolution equation. Our result also illustrates a subtle difference between conformal perturbation theory and the slow-roll expansion.

Schalm, Koenraad; Aalst, Ted van der [Instituut-Lorentz for Theoretical Physics, Universiteit Leiden, Niels Bohrweg 2, Leiden (Netherlands); Shiu, Gary, E-mail: kschalm@lorentz.leidenuniv.nl, E-mail: shiu@physics.wisc.edu, E-mail: vdaalst@lorentz.leidenuniv.nl [Department of Physics, University of Wisconsin-Madison, Madison, WI 53706 (United States)

2013-03-01T23:59:59.000Z

77

NE - Nuclear Energy - Energy Conservation Plan  

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

NUCLEAR ENERGY (NE) NUCLEAR ENERGY (NE) ENERGY CONSERVATION PLAN NE has heavily emphasized the use of flexiplace, both regular and situational. Since approximately 56 percent of NE staff use flexiplace, our plan is based on the Forrestal/Germantown (FORS/GTN) office spaces, and flexiplace office space. There are other common sense actions and policies that will be used to improve energy efficiency in the offices at both FORS and GTN. In the FORS/GTN office space: 1. Use flexiplace to the maximum extent possible. Saving an average of 1.5 gallons of gasoline per day per person (e.g., 13 miles per work x 2 = 26 miles, an average of 17 mpg), on a normal workday, NE employees save (56 percent of 145 = 71 times 1.2 days per pay period = 85.2 workdays x 1.5 gals = 127.8 gallons/pay

78

Particle-hole symmetry broken pseudogap in high temperature superconductors  

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

Particle-hole symmetry broken pseudogap in Particle-hole symmetry broken pseudogap in high temperature superconductors High-temperature (Tc) superconductivity is one of the most important topics in condensed matter physics. Despite extensive studies over more than two decades, the microscopic mechanism of high temperature superconductivity still remains elusive due to many unconventional properties that are not well understood. Among them, the most mysterious behavior of high-Tc superconductor is the nature of so called "pseudogap", which has been a focus of the field for many years. In conventional superconductors, a gap exists in the energy absorption spectrum only below Tc, corresponding to the energy price to pay for breaking a Cooper pair of electrons. In high-Tc cuprate superconductors, an energy gap called the pseudogap exists above Tc but below T*, and is controversially attributed either to pre-formed superconducting pairs or to competing phases. Recently, by carefully studying the "symmetry" of the gap, researchers Makoto Hashimoto and Rui-Hua He, along with their co-workers in Prof. Zhi-Xun Shen's group at Stanford University, have found crucial evidence suggesting that the particle-hole symmetry required by superconductivity is broken in the pseudogap state.

79

U of L Calgary Campus-Friday, August 31, 2012 Parking Information for Rocky Mountain Plaza and Bow Valley College  

E-Print Network (OSTI)

U of L Calgary Campus- Friday, August 31, 2012 Parking Information for Rocky Mountain Plaza and Bow daytime hours. The flat rate costs are as follows: Monday to Friday (evenings): $3.00 Weekends & Holidays

Morris, Joy

80

Hartford Neighborhood Healthy Homes Project (NeHHP) Checklist Definitions  

E-Print Network (OSTI)

Hartford Neighborhood Healthy Homes Project (NeHHP) Checklist Definitions Hartford Neighborhood Healthy Homes Project (NeEHP) Modified Visual Assessment from US DHHS Healthy Housing Inspection Manual or breaking stone or brick. #12;Hartford Neighborhood Healthy Homes Project (Ne

Oliver, Douglas L.

Note: This page contains sample records for the topic "broken bow ne" 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

Astrophysical bow shocks: An analytical solution for the hypersonic blunt body problem in the intergalactic medium  

E-Print Network (OSTI)

Aims: Bow shock waves are a common feature of groups and clusters of galaxies since they are generated as a result of supersonic motion of galaxies through the intergalactic medium. The goal of this work is to present an analytical solution technique for such astrophysical hypersonic blunt body problems. Methods: A method, developed by Schneider (1968, JFM, 31, 397) in the context of aeronautics, allows calculation of the galaxy's shape as long as the shape of the bow shock wave is known (so-called inverse method). In contrast to other analytical models, the solution is valid in the whole flow region (from the stagnation point up to the bow shock wings) and in particular takes into account velocity gradients along the streamlines. We compare our analytical results with two-dimensional hydrodynamical simulations carried out with an extended version of the VH-1 hydrocode which is based on the piecewise parabolic method with a Lagrangian remap. Results: It is shown that the applied method accurately predicts the...

Schulreich, Michael Mathias

2011-01-01T23:59:59.000Z

82

AKARI/FIS Mapping of the ISM-Wind Bow Shock around Alpha Ori  

E-Print Network (OSTI)

We present 10' x 50' scan maps around an M supergiant Alpha Ori at 65, 90, 140 and 160 microns obtained with the AKARI Infrared Astronomy Satellite. Higher spatial resolution data with the exact analytic solution permit us to fit the de-projected shape of the stellar wind bow shock around Alpha Ori to have the stand-off distance of 4.8', position angle of 55 degrees and inclination angle of 56 degrees. The shape of the bow shock suggests that the peculiar velocity of Alpha Ori with respect to the local medium is v_* = 40 (n_H)^(-1/2), where n_H is the hydrogen nucleus density at Alpha Ori. We find that the local medium is of n_H = 1.5 to 1.9 cm^(-3) and the velocity of the local flow is at 11 km s^(-1) by using the most recent astrometric solutions for Alpha Ori under the assumption that the local medium is moving away from the Orion OB 1 association. AKARI images may also reveal a vortex ring due to instabilities on the surface of the bow shock as demonstrated by numerical models. This research exemplifies the potential of AKARI All-Sky data as well as follow-up observations with Herschel Space Telescope and Stratospheric Observatory for Infrared Astronomy for this avenue of research in revealing the nature of interaction between the stellar wind and interstellar medium.

Toshiya Ueta; Hideyuki Izumiura; Issei Yamamura; Yoshikazu Nakada; Mikako Matsuura; Yoshifusa Ita; Toshihiko Tanabe; Hinako Fukushi; Noriyuki Matsunaga; Hiroyuki Mito

2008-08-20T23:59:59.000Z

83

BooNE: Booster Neutrino Experiment  

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

Posters What's a Neutrino? How neutrinos fit into our understanding of the universe. Recipe for a Neutrino Beam Start with some protons... concocting the MiniBooNE beam. The...

84

BooNE: Booster Neutrino Experiment  

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

linked in their own page with captions. Additional resources are the Talks, Slides and Posters page and the Publications page Experiment Details Data Releases BooNE photo montage...

85

BooNE: Booster Neutrino Experiment  

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

arXiv:0806.1449 General neutrino fluxes vs true neutrino energy, for MiniBooNE: image:muon neutrino flux image:electron neutrino flux image:final muon and electron neutrino...

86

BooNE: Booster Neutrino Experiment  

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

by the MiniBooNE Collaboration: A.A. Aguilar-Arevalo et al., First Measurement of the Muon Antineutrino Double Differential Charged Current Quasi-Elastic Cross Section,...

87

BooNE: Booster Neutrino Experiment  

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

BooNE will investigate the question of neutrino mass by searching for oscillations of muon neutrinos into electron neutrinos. This will be done by directing a muon neutrino beam...

88

A=18Ne (1995TI07)  

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

found. Astrophysical implications are discussed. 3. 14O(, )18Ne Qm 5.112 The thermonuclear reaction rates for this reaction have been estimated (1987WI11) using information...

89

MicroBooNE Proposal Addendum March  

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

by the growing interest in the Mini- BooNE low energy excess, demonstrated by new phenomenology papers appearing on the archive and by dedicated sessions at conferences such as...

90

BooNE: Booster Neutrino Experiment  

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

break the light barrier'' in the oil. Of course, nothing can travel faster than c, the speed of light in a vacuum, but for MiniBooNE light is traveling through oil. The oil...

91

MicroBooNE Detector Move  

ScienceCinema (OSTI)

On Monday, June 23, 2014 the MicroBooNE detector -- a 30-ton vessel that will be used to study ghostly particles called neutrinos -- was transported three miles across the Fermilab site and gently lowered into the laboratory's Liquid-Argon Test Facility. This video documents that move, some taken with time-lapse camerad, and shows the process of getting the MicroBooNE detector to its new home.

Flemming, Bonnie; Rameika, Gina

2014-07-15T23:59:59.000Z

92

N E A D A M S P L NE  

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

NE 349TH ST N E 29TH AV E NE 3 59 T H ST N E 2 6 T H A V E N E 36 4T H ST NE LA ND ER HO LM RD N E 33 4 TH S T N E B R O T H E R S R D NE 3 4 5 T H C I R NE 21S T AV E N E F I N A...

93

Parity-time symmetry broken by point-group symmetry  

SciTech Connect

We discuss a parity-time (PT) symmetric Hamiltonian with complex eigenvalues. It is based on the dimensionless Schrdinger equation for a particle in a square box with the PT-symmetric potential V(x, y) = iaxy. Perturbation theory clearly shows that some of the eigenvalues are complex for sufficiently small values of |a|. Point-group symmetry proves useful to guess if some of the eigenvalues may already be complex for all values of the coupling constant. We confirm those conclusions by means of an accurate numerical calculation based on the diagonalization method. On the other hand, the Schrdinger equation with the potential V(x, y) = iaxy{sup 2} exhibits real eigenvalues for sufficiently small values of |a|. Point group symmetry suggests that PT-symmetry may be broken in the former case and unbroken in the latter one.

Fernndez, Francisco M., E-mail: fernande@quimica.unlp.edu.ar; Garcia, Javier [INIFTA (UNLP, CCT La Plata-CONICET), Divisin Qumica Terica, Blvd. 113 S/N, Sucursal 4, Casilla de Correo 16, 1900 La Plata (Argentina)] [INIFTA (UNLP, CCT La Plata-CONICET), Divisin Qumica Terica, Blvd. 113 S/N, Sucursal 4, Casilla de Correo 16, 1900 La Plata (Argentina)

2014-04-15T23:59:59.000Z

94

On a Broken Formal Symmetry between Kinetic and Gravitational Energy  

E-Print Network (OSTI)

Historically, the discovery of symmetries has played an important role in the progress of our fundamental understanding of nature. This paper will demonstrate that there exists in Newtonian theory in a spherical gravitational field a formal symmetry between the kinetic (KE) and gravitational potential energy (GPE) of a test mass. Put differently, there exists a way of expressing GPE such that the form of the mathematical expression remains invariant under an interchange of KE and GPE. When extended to relativity by a suitable assumption, it leads to a framework that bridges the general relativistic and Newtonian conceptions of gravitational energy, even though the symmetry is broken except in the infinitesimal limit. Recognizing this symmetry at infinitesimal scales makes it possible to write a relativistic equation of an individual graviton, the properties of which under under one interpretation may be unexpected.

Armin Nikkhah Shirazi

2014-07-16T23:59:59.000Z

95

Ground-state magnetic phase diagram of bow-tie graphene nanoflakes in external magnetic field  

SciTech Connect

The magnetic phase diagram of a ground state is studied theoretically for graphene nanoflakes of bow-tie shape and various sizes in external in-plane magnetic field. The tight-binding Hamiltonian supplemented with Hubbard term is used to model the electronic structure of the systems in question. The existence of the antiferromagnetic phase with magnetic moments localized at the sides of the bow-tie is found for low field and a field-induced spin-flip transition to ferromagnetic state is predicted to occur in charge-undoped structures. For small nanoflake doped with a single charge carrier, the low-field phase is ferrimagnetic and a metamagnetic transition to ferromagnetic ordering can be forced by the field. The critical field is found to decrease with increasing size of the nanoflake. The influence of diagonal and off-diagonal disorder on the mentioned magnetic properties is studied. The effect of off-diagonal disorder is found to be more important than that of diagonal disorder, leading to significantly widened distribution of critical fields for disordered population of nanoflakes.

Sza?owski, Karol, E-mail: kszalowski@uni.lodz.pl, E-mail: kszalowski@wp.pl [Department of Solid State Physics, Faculty of Physics and Applied Informatics, University of ?d?, ul. Pomorska 149/153, 90-236 ?d? (Poland)

2013-12-28T23:59:59.000Z

96

NE SARE Arbuscular Mycorrhiza Research following canola  

E-Print Network (OSTI)

NE SARE Arbuscular Mycorrhiza Research Corn grown following canola Corn grown following soybeans The planting of canola, a non-mycorrhizal crop, has been shown to reduce arbuscular mycorrhizal fungi following canola. To address this problem, we intercropped canola with oats, a mycorrhizal crop

Kaye, Jason P.

97

Higgs boson physics and broken flavor symmetry -- LHC phenomenology  

E-Print Network (OSTI)

The LHC implications are presented of a simplified model of broken flavor symmetry in which a new scalar (a flavon) emerges with mass in the TeV range. We summarize the influence of the model on Higgs boson physics, notably on the production cross section and decay branching fractions. Limits are obtained on the flavon $\\varphi$ from heavy Higgs boson searches at the LHC at 7 and 8 TeV. The branching fractions of the flavon are computed as a function of the flavon mass and the Higgs-flavon mixing angle. We explore possible discovery of the flavon at 14 TeV, particularly via the $\\varphi \\rightarrow Z^0Z^0$ decay channel in the $2\\ell2\\ell'$ final state, and through standard model Higgs boson pair production $\\varphi \\rightarrow hh$ in the $b\\bar{b}\\gamma\\gamma$ final state. The flavon mass range up to $500$ GeV could probed down to quite small values of the Higgs-flavon mixing angle with 100 fb$^{-1}$ of integrated luminosity at 14 TeV.

Berger, Edmond L

2014-01-01T23:59:59.000Z

98

MiniBooNE QE Cross Section Data Release  

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

to the public: CCQE cross sections: MiniBooNE flux table of predicted MiniBooNE muon neutrino flux (Table V) flux-integrated double differential cross section (Figure 13)...

99

Mon. Not. R. Astron. Soc. 339, 524536 (2003) Anatomy of the HerbigHaro object HH7 bow shock  

E-Print Network (OSTI)

images as well as ISO data, the line profile, H2 position­velocity diagram, optical images and the proper-dynamics (MHD) in star-forming regions. The Herbig­Haro object HH7 is an extensively investigated bow shock

100

Pseudomorphic GeSn/Ge(001) quantum wells: Examining indirect band gap bowing  

SciTech Connect

A study of the bandgap character of compressively strained GeSn{sub 0.060-0.091}/Ge(001) quantum wells grown by molecular beam epitaxy is reported. The built-in strain in GeSn wells leads to an increased separation between L and {Gamma} conduction band minima. The prevalent indirect interband transitions in GeSn were probed by photoluminescence spectroscopy. As a result we could simulate the L-valley bowing parameter in GeSn alloys, b{sub L} = 0.80 {+-} 0.06 eV at 10 K. From this we conclude that even compressively strained GeSn/Ge(001) alloys could become direct band gap semiconductors at the Sn-fraction higher than 17.0 at. %.

Tonkikh, Alexander A. [Max Planck Institute of Microstructure Physics, Weinberg 2 D-06120, Halle (Saale) (Germany); Institute for Physics of Microstructures RAS, GSP-105, Nizhniy Novgorod (Russian Federation); Eisenschmidt, Christian; Schmidt, Georg [Institute of Physics, Martin Luther University Halle-Wittenberg, Von-Danckelmann-Platz 3 D-01620, Halle (Saale) (Germany); Talalaev, Vadim G. [Max Planck Institute of Microstructure Physics, Weinberg 2 D-06120, Halle (Saale) (Germany); ZIK SiLi-Nano, Martin Luther University Halle-Wittenberg, Karl-Freiherr-von-Fritsch-Str. 3 D-06120, Halle (Saale) (Germany); Zakharov, Nikolay D.; Werner, Peter [Max Planck Institute of Microstructure Physics, Weinberg 2 D-06120, Halle (Saale) (Germany); Schilling, Joerg [ZIK SiLi-Nano, Martin Luther University Halle-Wittenberg, Karl-Freiherr-von-Fritsch-Str. 3 D-06120, Halle (Saale) (Germany)

2013-07-15T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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.


101

On the absence of wind bow-shocks around OB-runaway stars: probing the physical conditions of the interstellar medium  

E-Print Network (OSTI)

High-resolution IRAS maps are used to search for the presence of stellar-wind bow-shocks around high-mass X-ray binaries (HMXBs). Their high space velocities, recently confirmed with Hipparcos observations, combined with their strong stellar winds should result in the formation of wind bow-shocks. Except for the already known bow-shock around Vela X-1 (Kaper et al. 1997), we do not find convincing evidence for a bow-shock around any of the other HMXBs. Also in the case of (supposedly single) OB-runaway stars, only a minority appears to be associated with a bow-shock (Van Buren et al. 1995). We investigate why wind bow-shocks are not detected for the majority of these OB-runaway systems: is this due to the IRAS sensitivity, the system's space velocity, the stellar-wind properties, or the height above the galactic plane? It turns out that none of these suggested causes can explain the low detection rate (~40%). We propose that the conditions of the interstellar medium mainly determine whether a wind bow-shock is formed or not. In hot, tenuous media (like inside galactic superbubbles) the sound speed is high (~100 km/s), such that many runaways move at subsonic velocity through a low-density medium, thus preventing the formation of an observable bow-shock. Superbubbles are expected (and observed) around OB associations, where the OB-runaway stars were once born. Turning the argument around, we use the absence (or presence) of wind bow-shocks around OB runaways to probe the physical conditions of the interstellar medium in the solar neighbourhood.

Fredrik Huthoff; Lex Kaper

2001-12-18T23:59:59.000Z

102

Compton profiles of Ne, Ar, and Kr  

Science Journals Connector (OSTI)

Compton profiles of Ne, Ar, and Kr are calculated from ground-state energies and wave functions with full correlation contributions included. The latter is carried out by regarding atoms as inhomogeneous interacting electron-gas systems using the Kohn-Sham self-consistent scheme in the local-density approximation. The calculated values are brought closer to the experimental values from Hartree-Fock results. There are numerical problems for large atoms.

B. Y. Tong and L. Lam

1978-08-01T23:59:59.000Z

103

NE Oregon Wildlife Project "Precious Lands"  

E-Print Network (OSTI)

NE Oregon Wildlife Project "Precious Lands" Managed by The Nez Perce Tribe Angela C. Sondenaa, Ph Oct 1996 Helm 10,306 $2,660,674.00 Sept 1998 Graham Tree farm 158 $402,453.00 Aug 1999 Beach Ranch 1 of shrub sub-canopy Project Goals: 40-70% tree canopy cover 35-65% shrub canopy cover > 3.5 snags 6-10" dbh

104

Ground Broken for New Job-Creating Accelerator Research Facility at DOE's  

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

Ground Broken for New Job-Creating Accelerator Research Facility at Ground Broken for New Job-Creating Accelerator Research Facility at DOE's Fermi National Accelerator Laboratory in Illinois Ground Broken for New Job-Creating Accelerator Research Facility at DOE's Fermi National Accelerator Laboratory in Illinois December 16, 2011 - 11:49am Addthis WASHINGTON, D.C. - Today, ground was broken for a new accelerator research facility being built at the Department of Energy's (DOE's) Fermi National Accelerator Laboratory (Fermilab) in Batavia, Illinois. Supported jointly by the state of Illinois and DOE, the construction of the Illinois Accelerator Research Center (IARC) will provide a state-of-the-art facility for research, development and industrialization of particle accelerator technology, and create about 200 high-tech jobs. DOE's Office

105

NE Blog Archive | Department of Energy  

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

Blog Archive Blog Archive NE Blog Archive RSS December 31, 2013 GIF Policy Group Meeting in Brussels, Belgium, November 2013 Generation IV International Forum Updates Technology Roadmap and Builds Future Collaboration The Generation IV International Forum (GIF) held its 36th Policy Group (PG) meeting on November 21-22 in Brussels, Belgium. The PG reviewed progress on a number of on-going actions and received progress reports from the GIF Experts Group (EG) and the GIF Senior Industry Advisory Panel (SIAP). December 12, 2013 The basics of small modular reactor technology explained. | Infographic by Sarah Gerrity, Energy Department. Advancing Small Modular Reactors: How We're Supporting Next-Gen Nuclear

106

Microsoft PowerPoint - NE- Milton  

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

University University Program (NEUP) Presentation to Vice Presidents of Research and Development of Historically Black Colleges and Universities Ingrid M. Milton Department of Energy Office of Nuclear Energy July 9, 2009 195725 (2) Overview The Office of Nuclear Energy (NE) is committed to strengthening the Nation's educational programs in nuclear science and engineering. * Established the Nuclear Energy University Program (NEUP). * Award grants and contracts through competitive selection process. NEUP enables universities to maintain and expand their nuclear science curriculum and programs to ensure future availability of technical experts for U.S. nuclear programs. * NEUP is managed by the Center for Advanced Energy Studies (CAES). 2 195725 (3) Nuclear Energy University Program -

107

EIS-0432: Department of Energy Loan Guarantee for Medicine Bow Gasification and Liquefaction Coal-to-Liquids, Carbon County, Wyoming  

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

DOE is assessing the potential environmental impacts for its proposed action of issuing a Federal loan guarantee to Medicine Bow Fuel & Power LLC (MBFP), a wholly-owned subsidiary of DKRW Advanced Fuels LLC. MBFP submitted an application to DOE under the Federal loan guarantee program pursuant to the Energy Policy Act of 2005 to support the construction and startup of the MBFP coal-to-liquids facility, a coal mine and associated coal handling facilities.

108

Microsoft PowerPoint - MiniBooNE Neutrino 2008  

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

Oscillation Searches Steve Brice (Fermilab) for the MiniBooNE Collaboration Neutrino 2008 Neutrino 2008 Steve Brice (FNAL) 2 Outline * Electron Neutrino Appearance - Oscillation...

109

NE Press Releases | Department of Energy  

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

Press Releases Press Releases NE Press Releases RSS December 12, 2013 Energy Department Announces New Investment in Innovative Small Modular Reactor The Energy Department tannounced an award to NuScale Power LLC to support a new project to design, certify and help commercialize innovative small modular reactors in the United States. November 12, 2013 Public Invited to Comment on Draft Environmental Assessment for the Resumption of Transient Testing of Nuclear Fuels and Materials The U.S. Department of Energy invites the public to read and comment on a draft environmental assessment it has prepared for a proposal to resume transient testing of nuclear fuels and materials at either Idaho National Laboratory (INL) or Sandia National Laboratories (SNL). November 4, 2013 Factsheet: Second Meeting of the United States-Japan Bilateral Commission

110

Notices 888 First Street, NE., Washington, DC  

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

11 Federal Register 11 Federal Register / Vol. 76, No. 122 / Friday, June 24, 2011 / Notices 888 First Street, NE., Washington, DC 20426. The filings in the above-referenced proceeding are accessible in the Commission's eLibrary system by clicking on the appropriate link in the above list. They are also available for review in the Commission's Public Reference Room in Washington, DC. There is an eSubscription link on the Web site that enables subscribers to receive e-mail notification when a document is added to a subscribed docket(s). For assistance with any FERC Online service, please e-mail FERCOnlineSupport@ferc.gov or call (866) 208-3676 (toll free). For TTY, call (202) 502-8659. Dated: June 20, 2011. Kimberly D. Bose, Secretary. [FR Doc. 2011-15859 Filed 6-23-11; 8:45 am]

111

Notices 888 First Street NE., Washington, DC  

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

53 Federal Register 53 Federal Register / Vol. 78, No. 56 / Friday, March 22, 2013 / Notices 888 First Street NE., Washington, DC 20426. This filing is accessible on-line at http://www.ferc.gov, using the ''eLibrary'' link and is available for review in the Commission's Public Reference Room in Washington, DC. There is an ''eSubscription'' link on the Web site that enables subscribers to receive email notification when a document is added to a subscribed docket(s). For assistance with any FERC Online service, please email FERCOnlineSupport@ferc.gov, or call (866) 208-3676 (toll free). For TTY, call (202) 502-8659. Comment Date: 5:00 p.m. Eastern Time on April 2, 2013. Dated: March 15, 2013. Kimberly D. Bose, Secretary. [FR Doc. 2013-06602 Filed 3-21-13; 8:45 am] BILLING CODE 6717-01-P

112

Mr. Andrew Wallo, III, NE-23  

Office of Legacy Management (LM)

suite 7900,955 L%l/onr Plaza, S. W., Washingion, D.C. 20024.?174,, Telephone: (202) 488.~ suite 7900,955 L%l/onr Plaza, S. W., Washingion, D.C. 20024.?174,, Telephone: (202) 488.~ Mr. Andrew Wallo, III, NE-23 Division of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland 20545 7117~03.87.dy.43 23 September 1987 I j / Dear Mr. Wallo: I ELIMINATION RECOMMENDATION -- COLLEGES AND UN&ITIES I . The attached elimination recommendation was prepared in accordance with your suggestion during our meeting on 22 September!. The recommend includes 26 colleges and universities identified,in Enclosure 4 to Aerospace letter subject: Status of Actions 27 May 1987; three institutions (Tufts and the University of Washington) currently list of sites under consideration; and six institutions tified during a search of Hanford records.

113

M r. Andrew Wallo, III, NE-23  

Office of Legacy Management (LM)

300.955 L*Enfom Plaza, S. Iv.. Washrhington. D.C. 200242174, Tekphonc (202) 300.955 L*Enfom Plaza, S. Iv.. Washrhington. D.C. 200242174, Tekphonc (202) 7117-03.87.cdy.43 23 September 1987 M r. Andrew Wallo, III, NE-23 Division of Facility & Site Deconnnissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear M r. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES The attached elimination recommendation was prepared in accordi with your suggestion during our meeting on 22 September. The reconu includes 26 colleges and universities identified.in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Sites List, da: 27 May 1987; three institutions.(Tufts College, University of Virgil and the University of Washington) currently identified'on the FUSFN list of sites under consideration; and six.institutions recently idI

114

Mr. Andrew Wallo, III, NE-23  

Office of Legacy Management (LM)

9% L'Enfam Plaza, S, W.. Warhin@on, D.C. 2002ijl74j Tekphow (202) 488ddO 9% L'Enfam Plaza, S, W.. Warhin@on, D.C. 2002ijl74j Tekphow (202) 488ddO 7117-03.87.cdy.'i3 23 September 1967 ~ s ~ Mr. Andrew Wallo, III, NE-23 Oivision of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear Mr. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND IJNIVFRSITIES , The attached elimination reconnnendation was prepar!ad in accordance with your suggestion during our meeting on 22 September! The recommendation includes 26 colleges and universities identified,in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Site List, dated 27 May 1987; three institutions (Tufts College, University of Virginia, and the University of Washington) currently identified!on ithe FUSRAP list of sites under consideration; and six institutions recently iden-

115

REPLY TO ATTN OF NE-301  

Office of Legacy Management (LM)

N\I&?' d,' g N\I&?' d,' g 4 DATE. fdov 2 5 1980 REPLY TO ATTN OF NE-301 .* - memoraadu SUBJECT Remedial Action for Linde Air Products Plant, Tonawanda, New York TO W. E. Mott, EV In view of the General Counsel's reconsideration of the authority to proceed with remedial action on this site and your determination that remedial action is needed to protect the public health and safety, we will include this site in our program for remedial action. of this memorandum. Oak Ridge is requested to do so by copy I am somewhat surprised at the urgency of remedial action which you implied in your memorandum since your previous memorandum designating this site stated that it has a low priority. The site radiological survey report DOE/EV-005/5 concludes that air and water contamination were below the non-occupational

116

MiniBooNE Oscillation Results 2011  

SciTech Connect

The MiniBooNE neutrino oscillation search experiment at Fermilab has recently updated results from a search for {bar {nu}}{sub {mu}} {yields} {bar {nu}}{sub e} oscillations, using a data sample corresponding to 8.58 x 10{sup 20} protons on target in anti-neutrino mode. This high statistics result represent an increase in statistics of 52% compared to result published in 2010. An excess of 57.7 {+-} 28.5 events is observed in the energy range 200 MeV < E{sub {nu}} < 3000 MeV. The data favor LSND-like {bar {nu}}{sub {mu}} {yields} {bar {nu}}{sub e} oscillations over a background only hypothesis at 91.1% confidence level in the energy range 475 < E{sub {nu}} < 3000 MeV.

Djurcic, Zelimir

2012-01-01T23:59:59.000Z

117

NE-23 List of California Sites NE-23 Hattie Car-well, SAN/NSQA Division  

Office of Legacy Management (LM)

NE-23 NE-23 Hattie Car-well, SAN/NSQA Division Attached for your information is the list of California sites we identified in our search of Manhattdn Engineer District records for the Formerly Utilized Sites Remedial Action Program (FUSRAP). None of the facilities listed qualified"fbr'FUSRAP:'~- The only site in California,that was included in FUSRAP was Gilman Hall on the University of California-Berkeley Campus. All California sites that are in our Surplus Facilities Management Prcgram are under San Francisco Operations and are at the Santa Susana Field Laboratory or the University of California-Davis. If you have questions on any of the sites on the list, please call me at FTS 233-5439. /ct( Andrew Walls III. Desiynation and Certification Manager

118

NE Pacific Basin --Tagging Data Kate Myers, Ph.D.  

E-Print Network (OSTI)

Ocean B: NE Pacific Basin --Tagging Data Kate Myers, Ph.D. Principal Investigator, High Seas Salmon ocean tagging research on Columbia River salmon and steelhead migrating in the NE Pacific Basin R. Basin in 1995-2004. Fisheries and Oceans Canada, Pacific Biological Station, Nanaimo, B

119

Oscillations results from the MiniBooNE experiment Alexis Aguilar...  

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

Alexis Aguilar-Arvalo (ICN-UNAM), for the MiniBooNE collaboration SILAFAE 2010 10 December 2010, Valparaso, Chile 2 Outlook MiniBooNE Motivation MiniBooNE Description...

120

Mr. Andrew Wallo, III, NE-23  

Office of Legacy Management (LM)

300, 955 L'E~~MI Phm.SW.:. Washin@on. LX. 200242174, T~kphonc(202)48ll. 5 300, 955 L'E~~MI Phm.SW.:. Washin@on. LX. 200242174, T~kphonc(202)48ll. 5 7117-03.87.cdy.43 23 September 1987 cA Mr. Andrew Wallo, III, NE-23 Division of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear Mr. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES M/).0-05 pl 0.0% The attached elimination recommendation was prepared in accordance ML.05 with your suggestion during our meeting on 22 September. The recommendation flD.o-02 includes 26 colleges and universities identified.in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Site List, dated NO.03. 27 May 1987; three institutions (Tufts College, University of Virginia, rJc..of and the University of Washington) currently identified on the FUSRAP

Note: This page contains sample records for the topic "broken bow ne" 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.


121

CA Mr. Andrew Wallo, III, NE-23  

Office of Legacy Management (LM)

?9OQ, 95.5 L'E&nt Plaza, SW.. W.ashin@.m, D.C. 20024.2174, Tekphone: (202) 488AQOO ?9OQ, 95.5 L'E&nt Plaza, SW.. W.ashin@.m, D.C. 20024.2174, Tekphone: (202) 488AQOO 7117-03.B7.cdy.43 23 September 1987 CA Mr. Andrew Wallo, III, NE-23 Division of Facility & Site Decommissioning Projects U.S. Oepartment of Energy Germantown, Maryland 20545 Dear Mr. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES zh/ ! o-01 lM!tl5 ML)!o-05 PI 77!0> The attached elimination recoannendation was prepared in accordance . -1 rlL.0~ with your suggestion during our meeting on 22 September. The recommendation flD.o-02 includes 26 colleges and universities identified~in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Site List, dated MO.07. 27 May 1987; three institutions (Tufts College, University of Virginia, UCIIOJ and the University of Washington) currently identified on the FUSRAP

122

MiniBooNE liner integrity study  

SciTech Connect

The civil construction for the MiniBooNE project includes a 50-m decay path and beam absorbers. The decay path is a six-foot diameter corrugated metal pipe (CMP). To prevent activation of the groundwater, the CMP and beam absorbers are surrounded by crushed aggregate, and enclosed in a double-walled geotextile membrane, referred to as the liner. The minimum distance from the beam centerline to the liner is 10 feet. The double-wall construction of the liner forms three regions, the containment volume, the interstitial volume, and the exterior. Each of these volumes is connected to monitoring wells at both the upstream and downstream ends of the decay volume, i.e. a total of six monitoring pipes extend to the surface. To confirm the integrity of the liner system following its placement, the firm Earth Tech was contracted to perform tests. Michael Williams was the primary contact with Earth Tech. The following is the report from Earth Tech, with minor changes in the interest of clarity. A sketch of the decay region is shown; only one of the layers of the liner is shown, and only one monitoring port. At the time of these tests, the excavation in general, but particularly in the vicinity of the monitoring wells had not been backfilled in the final grade, as indicated by the dashed lines.

Ray Stefanski, Phil Martin and Jeff Sims

2001-11-09T23:59:59.000Z

123

Pion inelastic scattering from sup 20 Ne  

SciTech Connect

Angular distributions for {sup 20}Ne({pi}{sup {plus minus}}, {pi}{sup {plus minus}}{prime}) were measured on the Energetic Pion Channel and Spectrometer (EPICS) at the Clinton P. Anderson Meson Physics Facility (LAMPF). Data were taken with both {pi}{sup {plus}} and {pi}{sup {minus}} over an angular range of 12{degree} to 90{degree} for T{sub {pi}}=180 MeV and with {pi}{sup +} from 15{degree} to 90{degree} for T{sub {pi}}=120 MeV. The data were analyzed using both the distorted-wave impulse approximation (DWIA) and the coupled-channels impulse approximation (CCIA) with collective transition densities. In addition, microscopic transition densities were used in the DWIA analysis for states in the lowest rotational bands. The transitions to the 6.73-MeV 0{sup +} and several 1{sup {minus}} states, including the states at 5.79 MeV and 8.71 MeV, were studied using several models for the transition density. Strong evidence for the importance of two-step routes in pion inelastic scattering was seen in several angular distributions, including the 5.79-MeV 1{sup {minus}}, the first three 4{sup +} states, and the 8.78-MeV 6{sup +}. 100 refs., 81 figs., 33 tabs.

Burlein, M. (Pennsylvania Univ., Philadelphia, PA (USA). Dept. of Physics)

1989-12-01T23:59:59.000Z

124

Exploring Neutrino Interactions with MicroBooNE  

E-Print Network (OSTI)

Recently, MiniBooNE observed an electromagnetic excess at low energy. What is the nature of this excess? What about the nature of the low-energy excess at LSND 20 years ago? The MicroBooNE detector will see neutrinos from the same Booster beam at Fermilab as used by MiniBooNE. MicroBooNE's design will enable us to discriminate photons from electrons elucidating the MiniBooNE and LSND low-energy electromagnetic excesses. MicroBooNE is a 170 ton liquid argon time projection chamber (LArTPC) capable of imaging neutrino interactions with the detail of a bubble chamber, but with electronic data acquisition and processing. In addition to shining light on the low-energy excesses and measuring low-energy neutrino cross sections, MicroBooNE is leading the way for a more extensive short-baseline neutrino physics program at Fermilab and it also serves as a R&D project towards a long-baseline multi-kiloton scale LArTPC detector.

Tia Miceli

2014-11-17T23:59:59.000Z

125

Exploring Neutrino Interactions with MicroBooNE  

E-Print Network (OSTI)

Recently, MiniBooNE observed an electromagnetic excess at low energy. What is the nature of this excess? What about the nature of the low-energy excess at LSND 20 years ago? The MicroBooNE detector will see neutrinos from the same Booster beam at Fermilab as used by MiniBooNE. MicroBooNE's design will enable us to discriminate photons from electrons elucidating the MiniBooNE and LSND low-energy electromagnetic excesses. MicroBooNE is a 170 ton liquid argon time projection chamber (LArTPC) capable of imaging neutrino interactions with the detail of a bubble chamber, but with electronic data acquisition and processing. In addition to shining light on the low-energy excesses and measuring low-energy neutrino cross sections, MicroBooNE is leading the way for a more extensive short-baseline neutrino physics program at Fermilab and it also serves as a R&D project towards a long-baseline multi-kiloton scale LArTPC detector.

Miceli, Tia

2014-01-01T23:59:59.000Z

126

Satellite observations of ship emission induced transitions from broken to closed cell marine stratocumulus  

E-Print Network (OSTI)

be related to the ship tracks, which is mainly coming from the cloud cover effect, may exceed ?100 Wm?2Satellite observations of ship emission induced transitions from broken to closed cell marine; accepted 3 August 2012; published 12 September 2012. [1] Documentation of the evolution of ship tracks

Daniel, Rosenfeld

127

Energy of the soliton internal modes and broken symmetries in nonlinear optics  

E-Print Network (OSTI)

Energy of the soliton internal modes and broken symmetries in nonlinear optics Dmitry V. Skryabin, in particular, of the negative energy of the internal modes are described in the context of nonlinear optics manuscript received October 3, 2001; accepted October 7, 2001 Applications of the concepts of the energy and

Skryabin, Dmitry

128

Mass scale effects for the Sudakov form factors in theories with the broken gauge symmetry  

E-Print Network (OSTI)

The off-shell and the on-shell Sudakov form factors in theories with broken gauge symmetry are calculated in the double-logarithmic approximation. We have used different infrared cut-offs, i.e. different mass scales, for virtual photons and weak gauge bosons.

A. Barroso; B. I. Ermolaev

2002-03-12T23:59:59.000Z

129

Property:EIA/861/IsoNe | Open Energy Information  

Open Energy Info (EERE)

IsoNe IsoNe Jump to: navigation, search Property Name ISO_NE Property Type Boolean Description Indicates that the organization conducts operations in the New England ISO region [1] References ↑ "EIA Form EIA-861 Final Data File for 2010 - 861 Webfile Layout for 2010.doc" Pages using the property "EIA/861/IsoNe" Showing 25 pages using this property. (previous 25) (next 25) B Bangor Hydro-Electric Co + true + Barton Village, Inc (Utility Company) + true + Bozrah Light & Power Company + true + C Central Maine Power Co + true + Central Vermont Pub Serv Corp + true + CinCap IV, LLC + true + CinCap V LLC + true + Cinergy Capital & Trading, Inc + true + City of Chicopee, Massachusetts (Utility Company) + true + City of Holyoke, Massachusetts (Utility Company) + true +

130

The Ne/O abundance ratio in the quiet Sun  

E-Print Network (OSTI)

Aims: To determine the neon-to-oxygen abundance in the quiet Sun, a proxy for the photospheric abundance ratio. Method: An emission measure method applied to extreme ultraviolet emission lines of Ne IV-VI and O III-V ions observed by the Coronal Diagnostic Spectrometer on the SOHO satellite. Results: The average Ne/O abundance ratio in supergranule cell centre regions is 0.18 +/- 0.05, while in supergranule network regions is 0.16 +/- 0.04. A photospheric Ne/O ratio of 0.17 +/- 0.05 is suggested, in good agreement with the most recent compilation of solar photospheric abundances, but discrepant with a recent Ne/O ratio derived from stellar X-ray spectra and revised neon abundances suggested from solar interior models.

P. R. Young

2005-10-10T23:59:59.000Z

131

The MicroBooNE Experiment - Conference Talks  

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

Short-Baseline Neutrion Oscillation Program Jonathan Asaadi PANIC 2014 August 24-29, 2014 Hamburg, Germany The MicroBooNE Experiment Mitch Soderberg FPC 2014 July 27-August 2,...

132

The coronal Ne/O abundance of alpha Centauri  

E-Print Network (OSTI)

Recent improvements in the modeling of solar convection and line formation led to downward revisions of the solar photospheric abundances of the lighter elements, which in turn led to changes in the radiative opacity of the solar interior and hence to conflicts with the solar convection zone depth as inferred from helioseismic oscillation frequencies. An increase of the solar Ne/O abundance to values as observed for nearby stars has been proposed as a solution. Because of the absence of strong neon lines in the optical, neon abundances are difficult to measure and the correct solar and stellar Ne/O abundances are currently hotly debated. Based on X-ray spectra obtained with XMM-Newton, we determine a reference value of Ne/O for the inactive, solar-like star alpha Cen (primarily alpha Cen B, which is the dominant component in X-rays), with three independent, line-based methods, using differential emission measure reconstruction and an emission measure-independent method. Our results indicate a value of approx. 0.28 for Ne/O in alpha Cen, approximately twice the value measured for the Sun, but still below the average value obtained for other stars. The low Ne/O abundance of the Sun is peculiar when compared to alpha Cen and other stars; our results emphasize the necessity to obtain more and accurate Ne/O abundance measurements of low activity stars.

C. Liefke; J. H. M. M. Schmitt

2006-09-01T23:59:59.000Z

133

Letter of Intent to Build a MiniBooNE Near Detector:BooNE  

SciTech Connect

There is accumulating evidence for a difference between neutrino and antineutrino oscillations at the {approx}1 eV{sup 2} scale. The MiniBooNE experiment observes an unexplained excess of electron-like events at low energies in neutrino mode, which may be due, for example, to either a neutral current radiative interaction, sterile neutrino decay, or to neutrino oscillations involving sterile neutrinos and which may be related to the LSND signal. No excess of electron-like events (-0.5 {+-} 7.8 {+-} 8.7), however, is observed so far at low energies in antineutrino mode. Furthermore, global 3+1 and 3+2 sterile neutrino fits to the world neutrino and antineutrino data suggest a difference between neutrinos and antineutrinos with significant (sin{sup 2} 2{theta}{sub {mu}{mu}} {approx} 35%) {bar {nu}}{sub {mu}} disappearance. In order to test whether the low-energy excess is due to neutrino oscillations and whether there is a difference between {nu}{sub {mu}} and {bar {nu}}{sub {mu}} disappearance, we propose building a second MiniBooNE detector at (or moving the existing MiniBooNE detector to) a distance of {approx}200 m from the Booster Neutrino Beam (BNB) production target. With identical detectors at different distances, most of the systematic errors will cancel when taking a ratio of events in the two detectors, as the neutrino flux varies as 1/r{sup 2} to a calculable approximation. This will allow sensitive tests of oscillations for both {nu}{sub e} and {bar {nu}} appearance and {nu}{sub {mu}} and {bar {nu}}{sub {mu}} disappearance. Furthermore, a comparison between oscillations in neutrino mode and antineutrino mode will allow a sensitive search for CP and CPT violation in the lepton sector at short baseline ({Delta}m{sup 2} > 0.1 eV{sup 2}). Finally, by comparing the rates for a neutral current (NC) reaction, such as NC {pi}{sup 0} scattering or NC elastic scattering, a direct search for sterile neutrinos will be made. The initial amount of running time requested for the near detector will be a total of {approx}2E20 POT divided between neutrino mode and antineutrino mode, which will provide statistics comparable to what has already been collected in the far detector. A thorough understanding of this short-baseline physics will be of great importance to future long-baseline oscillation experiments.

Stancu, I.; /Alabama U.; Djurcic, Z.; /Argonne; Smith, D.; /Embry-Riddle Aeronautical U.; Ford, R.; Kobilarcik, T.; Marsh, W.; Moore, C.D.; /Fermilab; Grange, J.; Osmanov, B.; Ray, H.; /Florida U.; Garvey, G.T.; /Los Alamos /Louisiana State U. /Michigan U. /Mexico U., ICN

2009-10-12T23:59:59.000Z

134

Production of heavy actinides from interactions of O16, O18, Ne20, and Ne22 with Cm248  

Science Journals Connector (OSTI)

We have measured cross sections for the production of isotopes of Bk through No in bombardments of Cm248 with O16, O18, Ne20, and Ne22 ions at energies near the Coulomb barrier. In general, the peak of the mass-yield curve for each element is about two mass units larger for O18 and Ne22 than for O16 and Ne20, reflecting the neutron excess of the projectiles. The production cross sections and maxima of the actinide isotopic distributions are at least as favorable for production of neutron-rich actinides as those measured for irradiation of U238 and Cm248 with very heavy ions. The observation of so many neutron-rich products between the masses of the target and compound nucleus suggests a direct transfer reaction in which the product nuclide is formed with relatively low excitation which minimizes depletion from prompt fission.NUCLEAR REACTIONS Cm248(O16,18,X), (Ne20,22,X) E(O16,18)=98,97 MeV, E(Ne20,22=115,116MeV); measured ? and isotopic distributions for Z=97-102.

Diana Lee; Hans von Gunten; Barbara Jacak; Matti Nurmia; Yuan-fang Liu; Cheng Luo; Glenn T. Seaborg; Darleane C. Hoffman

1982-01-01T23:59:59.000Z

135

D:\NE WEB Sites\NE\nerac\nov2001minutes.wpd  

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

November 5-6, 2001, DoubleTree Hotel, Arlington, Virginia November 5-6, 2001, DoubleTree Hotel, Arlington, Virginia NERAC members present: John Ahearne Robert Long Joseph Comfort Warren F. Miller, Jr. Michael L. Corradini Benjamin F. Montoya Jose Luis Cortez Sekazi Mtingwa Allen Croff Lura Powell James Duderstadt (Chair) Richard Reba Marvin Fertel Joy Rempe Beverly Hartline John Taylor Andrew Klein Charles E. Till Dale Klein (Monday only) Neil Todreas NERAC members absent: Thomas Cochran Allen Sessoms Maureen S. Crandall Daniel C. Sullivan Steve Fetter C. Bruce Tarter Leslie Hartz Ashok Thadani (ad hoc) J. Bennett Johnston Joan Woodard Linda C. Knight Also present: Robert Card, Under Secretary, USDOE Nancy Carder, NERAC Staff Charles Forsberg, Researcher, Oak Ridge National Laboratory Norton Haberman, Senior Technical Advisor, NE, USDOE

136

AE AURIGAE: FIRST DETECTION OF NON-THERMAL X-RAY EMISSION FROM A BOW SHOCK PRODUCED BY A RUNAWAY STAR  

SciTech Connect

Runaway stars produce shocks when passing through interstellar medium at supersonic velocities. Bow shocks have been detected in the mid-infrared for several high-mass runaway stars and in radio waves for one star. Theoretical models predict the production of high-energy photons by non-thermal radiative processes in a number sufficiently large to be detected in X-rays. To date, no stellar bow shock has been detected at such energies. We present the first detection of X-ray emission from a bow shock produced by a runaway star. The star is AE Aur, which was likely expelled from its birthplace due to the encounter of two massive binary systems and now is passing through the dense nebula IC 405. The X-ray emission from the bow shock is detected at 30'' northeast of the star, coinciding with an enhancement in the density of the nebula. From the analysis of the observed X-ray spectrum of the source and our theoretical emission model, we confirm that the X-ray emission is produced mainly by inverse Compton upscattering of infrared photons from dust in the shock front.

Lopez-Santiago, J.; Pereira, V.; De Castro, E. [Dpto. de Astrofisica y CC. de la Atmosfera, Universidad Complutense de Madrid, E-28040 Madrid (Spain); Miceli, M.; Bonito, R. [Dipartimento di Fisica, Universita di Palermo, Piazza del Parlamento 1, I-90134 Palermo (Italy); Del Valle, M. V.; Romero, G. E. [Instituto Argentino de Radioastronomia (IAR), CCT La Plata (CONICET), C.C.5, 1894 Villa Elisa, Buenos Aires (Argentina); Albacete-Colombo, J. F. [Centro Universitario Regional Zona Atlantica (CURZA), Universidad Nacional del COMAHUE, Monsenor Esandi y Ayacucho, 8500 Viedma, Rio Negro (Argentina); Damiani, F. [INAF-Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, I-90134 Palermo (Italy)

2012-09-20T23:59:59.000Z

137

NREL's PV Incubator: Where Solar Photovoltaic Records Go to be Broken |  

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

NREL's PV Incubator: Where Solar Photovoltaic Records Go to be NREL's PV Incubator: Where Solar Photovoltaic Records Go to be Broken NREL's PV Incubator: Where Solar Photovoltaic Records Go to be Broken June 28, 2011 - 11:44am Addthis NREL Principal Engineer Keith Emery prepares to load three-junction concentrator cells into NREL's
 High-Intensity Pulse Solar Simulator to test for efficiency. | Department of Energy Photo | Courtesy of National Renewable Energy Laboratory | Photo by Dennis Schroeder | Public Domain | NREL Principal Engineer Keith Emery prepares to load three-junction concentrator cells into NREL's
 High-Intensity Pulse Solar Simulator to test for efficiency. | Department of Energy Photo | Courtesy of National Renewable Energy Laboratory | Photo by Dennis Schroeder | Public Domain | Minh Le Minh Le

138

Language barrier broken with Multilingual WorldWideScience.org BETA | OSTI,  

Office of Scientific and Technical Information (OSTI)

Language barrier broken with Multilingual WorldWideScience.org BETA Language barrier broken with Multilingual WorldWideScience.org BETA Multilingual WordWideScience Officials at the June 11 launch of Multilingual WorldWideScience.org BETA at the International Council for Scientific and Technical Information (ICSTI) annual conference held in Helsinki, Finland. Pictured, from left, Dr. Walter Warnick, U.S. Department of Energy Office of Scientific and Technical Information (OSTI) Director; Yuri Arskiy, All-Russian Institute of Scientific and Technical Information (VINITI) Director; Tony Hey, Microsoft Research Corporate Vice-President; Richard Boulderstone of the British Library and the WorldWideScience Alliance Chairman; and Wu Yishan, Institute of Scientific and Technical Information of China (ISTIC) Chief Engineer OSTI Homepage

139

Broken gauge symmetry in a Bose gas with constant particle number  

E-Print Network (OSTI)

The existence of broken gauge symmetries in Bose-Einstein condensates is still controversially discussed in science, since it would not conserve the total number of particles. Here, it is shown for the first time that non-random condensate and non-condensate phase distributions may arise from local particle number breaking in a Bose gas with constant particle number, while the global U(1)-gauge symmetry of the system is preserved due to particle number conservation.

Alexej Schelle

2014-12-13T23:59:59.000Z

140

An Audiomagnetotelluric Survey Over The Chaves Geothermal Field (Ne  

Open Energy Info (EERE)

Page Page Edit History Facebook icon Twitter icon » An Audiomagnetotelluric Survey Over The Chaves Geothermal Field (Ne Portugal) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: An Audiomagnetotelluric Survey Over The Chaves Geothermal Field (Ne Portugal) Details Activities (0) Areas (0) Regions (0) Abstract: In an attempt to define the resistivity model of the Chaves geothermal field in NE Portugal, a detailed survey with scalar audiomagnetotelluric measurements was performed. The soundings were made in the frequency range from 2300 to 4.1 Hz. Electrical resistivity models were derived from the application of 1-D inversion, 2-D trial and error modeling and 2-D inversion procedures. The resistivities inside the geothermal field are low, reaching not more than 30 Ωm and increasing up to 60-150 Ωm

Note: This page contains sample records for the topic "broken bow ne" 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.


141

Municipal Energy Agency of NE | Open Energy Information  

Open Energy Info (EERE)

Municipal Energy Agency of NE Municipal Energy Agency of NE Jump to: navigation, search Name Municipal Energy Agency of NE Place Nebraska Utility Id 21352 Utility Location Yes Ownership P NERC Location MRO NERC MRO Yes NERC SPP Yes NERC WECC Yes RTO SPP Yes ISO MISO Yes Operates Generating Plant Yes Activity Generation Yes Activity Buying Transmission Yes Activity Wholesale Marketing Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png No rate schedules available. Average Rates No Rates Available References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from

142

Defect assistant band alignment transition from staggered to broken gap in mixed As/Sb tunnel field effect transistor heterostructure  

E-Print Network (OSTI)

.3As heterointerface. As a result, the band alignment was converted from staggered gap to broken gap-to-source voltage, VGS. As the SS of a MOSFET is governed by the transport mechanism of thermionic-emission over

Yener, Aylin

143

Ground Broken for New Job-Creating Accelerator Research Facility at DOEs Fermi National Accelerator Laboratory in Illinois  

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

WASHINGTON, D.C. Today, ground was broken for a new accelerator research facility being built at the Department of Energys (DOEs) Fermi National Accelerator Laboratory (Fermilab) in Batavia,...

144

Ne tak jsi mi pskal Kdyzs mi rucku stskal  

E-Print Network (OSTI)

Ne tak Ne tak jsi mi pískal Kdyzs mi rucku stískal A pravils mi svarnás je A traz m peres, mé srdecko dres A pravís mi spatnás je Vybil jsi mn zuby Z mojí slicné huby A pravís mi starás je Vybod jsi mi oci Na lzecku v noci A pravís mi slepás je Not so This is not the song you whistled to me When you

Zapletal, Jindrich

145

Generation of genuine $?$-type four-particle entangled state of superconducting artificial atoms with broken symmetry  

E-Print Network (OSTI)

We propose a scheme for generating a genuine $\\chi$-type four-particle entangled state of superconducting artificial atoms with broken symmetry by using one-dimensional transmission line resonator as a data bus. The $\\Delta$-type three-level artificial atom we use in the scheme is different from natural atom and has cyclic transitions. After suitable interaction time and simple operations, the desired entangled state can be obtained. Since artificial atomic excited states and photonic states are adiabatically eliminated, our scheme is robust against the spontaneous emissions of artificial atoms and the decays of transmission line resonator.

Chun-Ling Leng; Qi Guo; Xin Ji; Shou Zhang

2014-12-11T23:59:59.000Z

146

Broken symmetry and (1/2 statistics of spinons in (2+1)-dimensional antiferromagnets  

Science Journals Connector (OSTI)

We consider the Gutzwiller-projected Hofstadter-Slater determinant as a resonating-valence-bond wave function in a (2+1)-dimensional antiferromagnet. A strong case is made that spinons in the spin liquid state obey (1/2 statistics when a mass gap is present. We arrive at this conclusion from an effective continuum limit gauge theory. When a mass gap opens up, the parity symmetry is spontaneously broken resulting in twofold degeneracy of the ground state. The picture is consistent with that of the fractional quantum Hall state advocated by Laughlin.

Z. Zou

1989-08-01T23:59:59.000Z

147

Thermal gauge boson masses of the electroweak theory in the broken phase  

Science Journals Connector (OSTI)

Thermal effects in the broken phase of the electroweak theory are studied in the strongly interacting Higgs boson limit. In that limit and at the tree level the bosonic sector of the theory is a gauged non-linear sigma model. The associated one-loop thermal effective action for soft fields is then computed by using the background field method together with the Stueckelberg formalism. This effective action describes thermal corrections to the masses of the gauge bosons W, Z and the photon. It is the proper generalization of the hard thermal effective action of a Yang-Mills theory when there is a Higgs mechanism for a heavy Higgs particle.

Cristina Manuel

1998-05-19T23:59:59.000Z

148

Excited states in 104Cd described with the interacting boson model plus broken pairs  

Science Journals Connector (OSTI)

The high-spin structure of 104Cd has been studied through the 50Cr(58Ni,4p) reaction at a beam energy of 220 MeV. The level scheme has been extended up to an excitation energy of 11.9 MeV. Four collective structures have been identified based on two-quasineutron configurations. The low-lying states of both parities, as well as the main ?I=2 regular structures observed at high spin, are described in the framework of the interacting boson-fermion model with broken pairs.

G. de Angelis; C. Fahlander; D. Vretenar; S. Brant; A. Gadea; A. Algora; Y. Li; Q. Pan; E. Farnea; D. Bazzacco; G. Bonsignori; F. Brandolini; M. De Poli; D. De Acuna; S. Lunardi; G. Maron; D. R. Napoli; P. Pavan; C. M. Petrache; C. Rossi Alvarez; P. Spolaore; G. Vedovato

1999-06-17T23:59:59.000Z

149

Mercury Vapor Release from Broken Compact Fluorescent Lamps and In Situ Capture by New Nanomaterial Sorbents  

Science Journals Connector (OSTI)

There is one report of Hg poisoning (acrodynia) in a child exposed to broken tube-type fluorescents in a detailed case study presented by Tunnessen et al. (6). ... Similar release patterns but lower amounts were seen for spent bulbs (example result 90 ?g in 24 h) or from the fracture site of a new bulb after glass removal to simulate cleanup. ... Artificial lighting systems are transitioning from incandescent to compact fluorescent lamp (CFL) and light-emitting diode (LED) bulbs in response to the U.S. Energy Independence and Security Act and the EU Ecodesign Directive, which leads to energy ... ...

Natalie C. Johnson; Shawn Manchester; Love Sarin; Yuming Gao; Indrek Kulaots; Robert H. Hurt

2008-06-27T23:59:59.000Z

150

MICROBOONE PHYSICS Ben Carls Fermilab MicroBooNE Physics Outline  

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

PHYSICS Ben Carls Fermilab MicroBooNE Physics Outline * The detector and beam - MicroBooNE TPC - Booster and NuMI beams at Fermilab * Oscillation physics - Shed light on the...

151

E-Print Network 3.0 - api 20ne para Sample Search Results  

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

api 20ne para Search Powered by Explorit Topic List Advanced Search Sample search results for: api 20ne para Page: << < 1 2 3 4 5 > >> 1 Draft of 7282003 IBP Network Function...

152

ARM - Field Campaign - 2001 Philadelphia NE-OPS Air Quality Experiment  

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

Philadelphia NE-OPS Air Quality Experiment Comments? We would love to hear from you Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : 2001 Philadelphia NE-OPS Air...

153

The Mysterious Sickle Object in the Carina Nebula: A stellar wind induced bow shock grazing a clump?  

E-Print Network (OSTI)

Optical and near-infrared images of the Carina Nebula show a peculiar arc-shaped feature, which we call the "Sickle", next to the B-type star Trumpler 14 MJ 218. We use multi-wavelength observations to explore and constrain the nature and origin of the nebulosity. Using sub-mm data from APEX/LABOCA as well as Herschel far-infrared maps, we discovered a dense, compact clump with a mass of ~ 40 Msun located close to the apex of the Sickle. We investigate how the B-star MJ 218, the Sickle, and the clump are related. Our numerical simulations show that, in principle, a B-type star located near the edge of a clump can produce a crescent-shaped wind shock front, similar to the observed morphology. However, the observed proper motion of MJ 218 suggest that the star moves with high velocity (~ 100 km/s) through the ambient interstellar gas. We argue that the star is just about to graze along the surface of the clump, and the Sickle is a bow shock induced by the stellar wind, as the object moves supersonically through...

Ngoumou, Judith; Ratzka, Thorsten; Burkert, Andreas

2013-01-01T23:59:59.000Z

154

A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E0657-56  

E-Print Network (OSTI)

The Chandra image of the merging, hot galaxy cluster 1E0657-56 reveals a bow shock propagating in front of a bullet-like gas cloud just exiting the disrupted cluster core. This is the first clear example of a shock front in a cluster. From the jumps in the gas density and temperature at the shock, the Mach number of the bullet-like cloud is 2-3. This corresponds to a velocity of 3000-4000 km/s relative to the main cluster, which means that the cloud traversed the core just 0.1-0.2 Gyr ago. The 6-7 keV "bullet" appears to be a remnant of a dense cooling flow region once located at the center of a merging subcluster whose outer gas has been stripped by ram pressure. The bullet's shape indicates that it is near the final stage of being destroyed by ram pressure and gas dynamic instabilities, as the subcluster galaxies move well ahead of the cool gas. The unique simplicity of the shock front and bullet geometry in 1E0657-56 may allow a number of interesting future measurements. The cluster's average temperature is 14-15 keV but shows large spatial variations. The hottest gas (T>20 keV) lies in the region of the radio halo enhancement and extensive merging activity involving subclusters other than the bullet.

M. Markevitch; A. H. Gonzalez; L. David; A. Vikhlinin; S. Murray; W. Forman; C. Jones; W. Tucker

2001-10-22T23:59:59.000Z

155

THE MYSTERIOUS SICKLE OBJECT IN THE CARINA NEBULA: A STELLAR WIND INDUCED BOW SHOCK GRAZING A CLUMP?  

SciTech Connect

Optical and near-infrared images of the Carina Nebula show a peculiar arc-shaped feature, which we call the ''Sickle'', next to the B-type star Trumpler 14 MJ 218. We use multi-wavelength observations to explore and constrain the nature and origin of the nebulosity. Using submillimeter data from APEX/LABOCA as well as Herschel far-infrared maps, we discovered a dense, compact clump with a mass of {approx}40 M{sub Sun} located close to the apex of the Sickle. We investigate how the B star MJ 218, the Sickle, and the clump are related. Our numerical simulations show that, in principle, a B-type star located near the edge of a clump can produce a crescent-shaped wind shock front, similar to the observed morphology. However, the observed proper motion of MJ 218 suggests that the star moves with high velocity ({approx}100 km s{sup -1}) through the ambient interstellar gas. We argue that the star is just about to graze along the surface of the clump, and the Sickle is a bow shock induced by the stellar wind, as the object moves supersonically through the density gradient in the envelope of the clump.

Ngoumou, Judith; Preibisch, Thomas; Ratzka, Thorsten; Burkert, Andreas, E-mail: ngoumou@usm.lmu.de [Universitaets-Sternwarte Muenchen, Ludwig-Maximilians-Universitaet, Scheinerstr.1, D-81679 Muenchen (Germany)

2013-06-01T23:59:59.000Z

156

[NeII] emission line profiles from photoevaporative disc winds  

E-Print Network (OSTI)

I model profiles of the [NeII] forbidden emission line at 12.81um, emitted by photoevaporative winds from discs around young, solar-mass stars. The predicted line luminosities (~ 1E-6 Lsun) are consistent with recent data, and the line profiles vary significantly with disc inclination. Edge-on discs show broad (30-40km/s) double-peaked profiles, due to the rotation of the disc, while in face-on discs the structure of the wind results in a narrower line (~10km/s) and a significant blue-shift (5-10km/s). These results suggest that observations of [NeII] line profiles can provide a direct test of models of protoplanetary disc photoevaporation.

R. D. Alexander

2008-09-01T23:59:59.000Z

157

File:EIA-Williston-NE-Gas.pdf | Open Energy Information  

Open Energy Info (EERE)

Williston-NE-Gas.pdf Williston-NE-Gas.pdf Jump to: navigation, search File File history File usage Williston Basin, Northeast Part By 2001 Gas Reserve Class Size of this preview: 776 × 600 pixels. Full resolution ‎(6,600 × 5,100 pixels, file size: 5.95 MB, MIME type: application/pdf) Description Williston Basin, Northeast Part By 2001 Gas Reserve Class Sources Energy Information Administration Authors Samuel H. Limerick; Lucy Luo; Gary Long; David F. Morehouse; Jack Perrin; Robert F. King Related Technologies Oil, Natural Gas Creation Date 2005-09-01 Extent Regional Countries United States UN Region Northern America States Montana, North Dakota, South Dakota File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment

158

R i i R iReviving Russia Can a legacy of limited economic stability be broken?  

E-Print Network (OSTI)

R i i R iReviving Russia Can a legacy of limited economic stability be broken? #12;Hypothesis of economic (in)stability in Russia's past to determine whether or not Russia had become a `normal capitalist society' by the late 1990s. #12;· In 2001, Russia's GDP had fallen by more than half since 1991. · Living

New Hampshire, University of

159

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

160

Retrieval of Aerosol Optical Depth in Vicinity of Broken Clouds from Reflectance Ratios: Sensitivity Study  

SciTech Connect

We conducted a sensitivity study to better understand the potential of a new method for retrieving aerosol optical depth (AOD) under partly cloudy conditions. This method exploits reflectance ratios in the visible spectral range and provides an effective way to avoid three-dimensional (3D) cloud effects. The sensitivity study is performed for different observational conditions and random errors in input data. The results of the sensitivity study suggest that this ratio method has the ability to detect clear pixels even in close proximity to clouds. Such detection does not require a statistical analysis of the two-dimensional (2D) horizontal distribution of reflected solar radiation, and thus it could be customized for operational retrievals. In comparison with previously suggested approaches, the ratio method has the capability to increase the "harvest" of clear pixels. Similar to the traditional Independent Pixel Approximation (IPA), the ratio method has a low computational cost for retrieving AOD. In contrast to the IPA method, the ratio method provides much more accurate estimations of the AOD values under broken cloud conditions: pixel-based and domain-averaged estimations of errors in AOD are about 25% and 10%, respectively. Finally, both the ratio-based cloud screening and the accuracy of domain-averaged ratio-based AOD values do not suffer greatly when 5% random errors are introduced in the reflectances.

Kassianov, Evgueni I.; Ovtchinnikov, Mikhail; Berg, Larry K.; McFarlane, Sally A.; Flynn, Connor J.

2009-09-01T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

2013 Annual DOE-NE Materials Research Coordination Meeting | Department of  

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

2013 Annual DOE-NE Materials Research Coordination Meeting 2013 Annual DOE-NE Materials Research Coordination Meeting 2013 Annual DOE-NE Materials Research Coordination Meeting The Reactor Materials element of the Nuclear Energy Enabling Technologies (NEET) program conducted its FY 2013 coordination meeting as a series of four web-conferences to act as a forum for the nuclear materials research community. The purpose of this meeting was to report on current and planned nuclear materials research, identify new areas of collaboration and promote greater coordination among the various Office of Nuclear Energy (NE) programs. Currently, materials research is performed in several NE programs, including NE Advanced Modeling and Simulation (NEAMS), Fuel Cycle Research and Development (FCRD), Advanced Reactor Technologies

162

2013 Annual DOE-NE Materials Research Coordination Meeting | Department of  

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

2013 Annual DOE-NE Materials Research Coordination Meeting 2013 Annual DOE-NE Materials Research Coordination Meeting 2013 Annual DOE-NE Materials Research Coordination Meeting The Reactor Materials element of the Nuclear Energy Enabling Technologies (NEET) program conducted its FY 2013 coordination meeting as a series of four web-conferences to act as a forum for the nuclear materials research community. The purpose of this meeting was to report on current and planned nuclear materials research, identify new areas of collaboration and promote greater coordination among the various Office of Nuclear Energy (NE) programs. Currently, materials research is performed in several NE programs, including NE Advanced Modeling and Simulation (NEAMS), Fuel Cycle Research and Development (FCRD), Advanced Reactor Technologies

163

N.E. Leonard U. Pisa 18-20 April 2007Slide 1 Cooperative Control  

E-Print Network (OSTI)

1 N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 1 Cooperative Control and Mobile Sensor Networks.princeton.edu/~naomi N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 2 Outline and Key References A. Artificial Potentials-20 April 2007Slide 3 Outline and Key References D. Virtual Tensegrity Structures: B. Nabet and N.E. Leonard

Leonard, Naomi

164

N.E. Leonard U. Pisa 18-20 April 2007Slide 1 Cooperative Control  

E-Print Network (OSTI)

1 N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 1 Cooperative Control and Mobile Sensor Networks.princeton.edu/~naomi N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 2 Outline 1. Introduction to cooperative control.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 3 Reference 1. E. Fiorelli, N.E. Leonard, P. Bhatta, D. Paley, R

Leonard, Naomi

165

A Case Study For Geothermal Exploration In The Ne German Basin...  

Open Energy Info (EERE)

Geothermal Exploration In The Ne German Basin- Integrated Interpretation Of Seismic Tomography, Litho-Stratigraphy, Salt Tectonics, And Thermal Structure Jump to: navigation,...

166

Participants: William Naughton, COHMED Bill Sherman, NE HLRW Task Force  

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

conference call May 27, 1998 conference call May 27, 1998 Participants: William Naughton, COHMED Bill Sherman, NE HLRW Task Force Bob Fronczak, AAR Mike Butler, UETC Ray English, DOE-NR George Ruberg, UETC Kevin Blackwell, FRA Markus Popa, DOE-RW Sandy Covi, UP The Rail Topic Group is currently in a transitional mode, moving simultaneously toward closure of the two rail information matrices, Comparison of CVSA Recommended National Procedures and Out-Of-Service Criteria for the Enhanced Safety Inspection of Commercial Highway Vehicles Transporting Transuranics, Spent Nuclear Fuel, and High Level Waste to Rail Inspection Standards, and Rail and Highway Regulations Relative to the Transportation of Radioactive Materials and their Applicability to States, Tribes, Shippers, and Carriers, (both

167

EG&G SURVEY REPORT NE-F-003  

Office of Legacy Management (LM)

EBJG EBJG -ENERGY MEASUREMENTS GROUP EG&G SURVEY REPORT NE-F-003 FEBRUARY 1983 NJT& THE REMOTE SENSING lRtlORlllORY OF THE UNITED STATES DEPARTMENT OF ENERGY AN AERIAL RADIOLOGICAL SURVEY OF AN AREA SURROUNDING THE FORMER M IDDLESEX SAMPLING PLANT IN M IDDLESEX, N E W JERSEY DATE OF SURVEY: M A Y 1978 DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or

168

PNM Resources 2401 Aztec NE, MS-Z100  

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

PNM Resources PNM Resources 2401 Aztec NE, MS-Z100 Albuquerque, NM 87107 505-241-2025 Fax 505 241-2384 PNMResources.com October 29, 2013 Mr. Christopher Lawrence Office of Electricity Delivery and Energy Reliability (OE-20) U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 Submitted electronically via email to: Christopher.Lawrence@hq.doe.gov Dear Mr. Lawrence: Subject: Department of Energy (DOE)- Improving Performance of Federal Permitting and Review of Infrastructure Projects, Request for Information, 78 Fed. Reg. 53436 (Aug. 29, 2013) PNM Resources (PNMR) is an energy holding company with 2012 consolidated operating revenues of $1.3 billion. Through its regulated utilities, PNM and TNMP, PNMR serves electricity to more than 739,000 homes and businesses in New

169

CA M r. Andrew Wallo, III. NE-23  

Office of Legacy Management (LM)

i5W 95.5 L' i5W 95.5 L' E&nt plom. S. W.:. Washingr on. D.C. ZOOX2i74, Tekphm: (202) 488-6OGb 7II7-03.87.cdy.43 23 September 1987. Ii CA M r. Andrew Wallo, III. NE-23 Division of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear M r. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES pqq.0' 05 PI ;p.03- The attached elimination recommendation was prepared in accordance ,I ML.05 with your suggestion during our meeting on 22 September. The recommendation flO.O-02 includes 26 colleges and universities identified in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Site List, dated 27 May 1987; three institutions (Tufts College, University of Virginia, and the University of Washington) currently identified on the FUSRAP

170

Idaho National Laboratory DOE-NE's National Nuclear Capability-  

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

4-2023 4-2023 Idaho National Laboratory DOE-NE's National Nuclear Capability- Developing and Maintaining the INL Infrastructure TEN-YEAR SITE PLAN DOE/ID-11474 Final June 2012 Sustainable INL continues to exceed DOE goals for reduction in the use of petroleum fuels - running its entire bus fleet on biodiesel while converting 75% of its light-duty fleet to E85 fuel. The Energy Systems Laboratory (ESL), slated for completion this year, will be a state-of-the-art laboratory with high-bay lab space where leading bioenergy feedstock processing, advanced battery testing, and hybrid energy systems integration research will be conducted. The Advanced Test Reactor is the world's most advanced nuclear research capability - crucial to (1) the ongoing development of safe, efficient

171

NE-24 Unlverslty of Chicayo Remedial Action Plan  

Office of Legacy Management (LM)

(YJ 4 tlsj .?I2 (YJ 4 tlsj .?I2 416 17 1983 NE-24 Unlverslty of Chicayo Remedial Action Plan 22&d 7 IA +-- E. I.. Keller, Director Technical Services Division Oak Ridge Operations Ufflce In response to your memorandum dated July 29, 1983, the Field Task Proposal/Agreement (FTP/A) received frw Aryonne National Laboratory (ANL) appears to be satisfactory, and this office concurs in the use of ANL to provide the decontamination effort as noted in the FTP/A. The final decontaminatton report should Include the data needed for certiff- cation of the cleanup and any contamination left In place, e.g., sewer lines should be so documented in the permanent records of the University as well as the certification documents and reports. The remedial action to be conducted appears to be clearly InsIgnifIcant from an environmental

172

Photon-emission studies of slow C4+-Ne collisions  

Science Journals Connector (OSTI)

We present absolute term- and level-selective cross sections for specific single- and double-electron capture processes in slow (16 keV) C4+-Ne collisions. The results are deduced through a combined analysis of earlier translational energy-gain data and the present photon-emission cross sections in the region 40240 nm. We find that double-electron capture is dominated by processes in which two electrons appear to change orbitals in a single interaction of two diabatic quasimolecular potential curvesa type of process which rarely has been isolated before. Furthermore, we observe a strong preference for population of 2s2p over 2p2 configurations in these one-step two-electron capture reactions. This is a remarkable configuration selectivity, since reaction channels leading to 2s2p and 2p2 configurations cross with the incident channel at almost the same internuclear distances.

M.O. Larsson; A. Wnnstrm; M. Wang; A. Arnesen; F. Heijkenskjld; A. Langereis; B. Nystrm; R.W. McCullough; H. Cederquist

1997-03-01T23:59:59.000Z

173

Microsoft PowerPoint - NEAC Battelle NE Capabilities 062408.ppt  

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

R&D Facility Requirements NEAC Meeting Progress Report June 24, 2008 2 Facilitization of U.S. Nuclear R&D Infrastructure Three-step study process: * First, ASNE requested Battelle Memorial Institute to develop Industry- and-University-supported list of capabilities and facilities necessary to conduct a comprehensive nuclear R&D program. (Draft, June 12, 2008) * Second, INL, using input from all DOE and other sources, will determine current facilities and their condition and availability to support next 20 years of nuclear R&D. (Draft, June 30, 2008) * Third, recommendations will be made on priorities and on existing facilities to be maintained/preserved or otherwise supported by NE regardless of location or ownership. (Executive Team Meeting, July 1, 2008)

174

THE GENESIS SOLAR WIND CONCENTRATOR TARGET: MASS FRACTIONATION CHARACTERISED BY NE ISOTOPES  

SciTech Connect

The concentrator on Genesis provides samples of increased fluences of solar wind ions for precise determination of the oxygen isotopic composition of the solar wind. The concentration process caused mass fractionation as function of the radial target position. They measured the fractionation using Ne released by UV laser ablation along two arms of the gold cross from the concentrator target to compare measured Ne with modeled Ne. The latter is based on simulations using actual conditions of the solar wind during Genesis operation. Measured Ne abundances and isotopic composition of both arms agree within uncertainties indicating a radial symmetric concentration process. Ne data reveal a maximum concentration factor of {approx} 30% at the target center and a target-wide fractionation of Ne isotopes of 3.8%/amu with monotonously decreasing {sup 20}Ne/{sup 22}Ne ratios towards the center. The experimentally determined data, in particular the isotopic fractionation, differ from the modeled data. They discuss potential reasons and propose future attempts to overcome these disagreements.

WIENS, ROGER C. [Los Alamos National Laboratory; OLINGER, C. [Los Alamos National Laboratory; HEBER, V.S. [Los Alamos National Laboratory; REISENFELD, D.B. [Los Alamos National Laboratory; BURNETT, D.S. [Los Alamos National Laboratory; ALLTON, J.H. [Los Alamos National Laboratory; BAUR, H. [Los Alamos National Laboratory; WIECHERT, U. [Los Alamos National Laboratory; WIELER, R. [Los Alamos National Laboratory

2007-01-02T23:59:59.000Z

175

Sample Curriculum for EECS/NE Joint Major EECS and Nuclear Engineering  

E-Print Network (OSTI)

Sample Curriculum for EECS/NE Joint Major Year EECS and Nuclear Engineering Fall Spring FRESHMAN Math 1A (4 units) Math 1B (4 units) Chemistry 1A (4 units) CS 61B or 61 BL (4 units) Engineering 10 (3 (4 units) Electives (3 units) JUNIOR NE 101 (4 units) Stat 25/Stat134/EE 126 (3-4 units) Engineering

California at Irvine, University of

176

NeXus: A common format for the exchange of neutron and synchroton data  

Science Journals Connector (OSTI)

NeXus is a data format for the exchange of neutron and synchrotron scattering data between facilities and user institutions. It has been developed by an international team of scientists and computer programmers from neutron and X-ray facilities around the world. The NeXus format uses the hierarchical data format (HDF) which is portable, binary, extensible and self-describing. The NeXus format defines the structure and contents of these HDF files in order to facilitate the visualization and analysis of neutron and X-ray data. In addition, an application program interface (API) is being produced in order to simplify the reading and writing of NeXus files. The details of the format are available at ?http://www.neutron.anl.gov/NeXus/?.

P Klosowski; M Koennecke; J.Z Tischler; R Osborn

1997-01-01T23:59:59.000Z

177

EA-1909: South Table Wind Project, Kimball County, NE | Department of  

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

09: South Table Wind Project, Kimball County, NE 09: South Table Wind Project, Kimball County, NE EA-1909: South Table Wind Project, Kimball County, NE Summary DOE's Western Area Power Administration is preparing this EA to evaluate the environmental impacts of interconnecting the proposed South Table Wind Project, which would generate approximately 60 megawatts from about 40 turbines, to Western's existing Archer-Sidney 115-kV Transmission Line in Kimball County, Nebraska. Public Comment Opportunities None available at this time. Documents Available for Download August 28, 2012 EA-1909: Finding of No Significant Impact South Table Wind Project, Kimball County, NE July 16, 2012 EA-1909: Final Environmental Assessment South Table Wind Project, Kimball County, NE February 29, 2012 EA-1909: Draft Environmental Assessment

178

CA CAIOlf Mr. Andrew Wallo. III, NE-23  

Office of Legacy Management (LM)

kire 7900. 955 L*E,,fa,u PLUG S. W.. Washin@ on. D.C. 20024-2174, Tekphme: (202) 488-6000 kire 7900. 955 L*E,,fa,u PLUG S. W.. Washin@ on. D.C. 20024-2174, Tekphme: (202) 488-6000 7117-03.87.cdy.43 23 September 1987 CA CAIOlf Mr. Andrew Wallo. III, NE-23 Division of Facility & Site Decommissioning Projects U.S. Department of Energy Germantown, Maryland 20545 CT.05 FL .0-o/ lti.Ob id.Or Dear Mr. Wallo: In/. O-01 flA.05 ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES Mbj.o-03 I4 v.o+ The attached elimination recommendation was prepared in accordance ML.o= with your suggestion during our meeting on 22 September. The recommendation nO.O-02 includes 26 colleges and universities identified.in Enclosure 4 to Aerospace letter subject: Status of Actions - FUSRAP Site List, dated N0.63' 27 May 1987; three institutions (Tufts College, University of Virginia, kfC900

179

Using the NeWS window system in a Cray environment  

SciTech Connect

NeWS is structured as a single UNIX process, a network server that contains a PostScript interpreter. Client programs, which exist somewhere out on the network, talk to NeWS through byte streams. This paper describes the implementation of such a client interface on a Cray running the UNICOS operating system. With only a modest effort, it is possible to fit a simple PostScript interface to existing mainframe applications, which allows the user to graphically interact with the program from a remote workstation. Some typical applications, which have been structured as NeWS clients, have been described.

Phillips, R.L.; Forslund, D.W.

1987-06-01T23:59:59.000Z

180

EcoCAR: The NeXt Challenge | Department of Energy  

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

EcoCAR: The NeXt Challenge EcoCAR: The NeXt Challenge EcoCAR: The NeXt Challenge May 18, 2010 - 7:30am Addthis While most college students' experience with vehicles goes no further than the beater they picked up for a few thousand dollars, students participating in the EcoCAR: The NeXT Challenge competition get to experience the cutting-edge of driving technology. The competition, which was established by the U.S. Department of Energy and General Motors, is a three year advanced vehicle engineering contest. Yesterday, May 17, was the first day of their Year 2 judging sessions. In EcoCAR, students from 16 universities across North America are competing against each other to build the most environmentally sustainable and practical vehicle. This year's teams have adopted a number of advanced

Note: This page contains sample records for the topic "broken bow ne" 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 Case Study For Geothermal Exploration In The Ne German Basin- Integrated  

Open Energy Info (EERE)

Geothermal Exploration In The Ne German Basin- Integrated Geothermal Exploration In The Ne German Basin- Integrated Interpretation Of Seismic Tomography, Litho-Stratigraphy, Salt Tectonics, And Thermal Structure Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Proceedings: A Case Study For Geothermal Exploration In The Ne German Basin- Integrated Interpretation Of Seismic Tomography, Litho-Stratigraphy, Salt Tectonics, And Thermal Structure Details Activities (0) Areas (0) Regions (0) Abstract: Unavailable Author(s): K. Bauer, I. Moeck, B. Norden, A. Schulze, M. H. Weber Published: Publisher Unknown, 2009 Document Number: Unavailable DOI: Unavailable Retrieved from "http://en.openei.org/w/index.php?title=A_Case_Study_For_Geothermal_Exploration_In_The_Ne_German_Basin-_Integrated_Interpretation_Of_Seismic_Tomography,_Litho-Stratigraphy,_Salt_Tectonics,_And_Thermal_Structure&oldid=390106"

182

Fermilab | Newsroom | Press Releases | June 24, 2014: MicroBooNE...  

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

Res | Hi Res The massive MicroBooNE neutrino detector is gently lowered into the main cavern of the Liquid-Argon Test Facility at Fermilab on Monday, June 23. The banner on the...

183

HeNe and cw CO2 laser long-path systems for gas detection  

Science Journals Connector (OSTI)

This paper describes the design and testing of a laboratory prototype dual HeNe laser system for the detection of methane leaks from underground pipelines and solid-waste landfill...

Grant, William B

1986-01-01T23:59:59.000Z

184

REPLY TO ATTN OF: NE-24 L SUBJECT: Authorization to Conduct Remedial...  

Office of Legacy Management (LM)

|1 e0i78 DATE: OCT 9 1984 REPLY TO ATTN OF: NE-24 L SUBJECT: Authorization to Conduct Remedial Action at Vicinity Properties In Lodi, New Jersey TO: J. LaGrone, Manager...

185

Search for Muon Neutrino and Antineutrino Disappearance in MiniBooNE  

E-Print Network (OSTI)

The MiniBooNE Collaboration reports a search for ?[subscript ?] and ?? [subscript ?] disappearance in the ?m[superscript 2] region of 0.540 ??eV[superscript 2]. These measurements are important for constraining models ...

McGary, Van Thanh

186

MiniBooNE H. A. Tanaka Princeton University Neutrino Factory...  

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

H. A. Tanaka Princeton University Neutrino Factory 2004 Osaka, Japan The MiniBooNE Collaboration University of Alabama: Y.Liu, I.Stancu Bucknell University: S.Koutsoliotas...

187

Thomas-Ehrman effect in a three-body model: $^{16}$Ne case  

E-Print Network (OSTI)

The dynamic mechanism of the Thomas-Ehrman shift is studied in three-cluster systems by example of $^{16}$Ne and $^{16}$C isobaric mirror partners. We predict configuration mixings for $0^+$ and $2^+$ states in $^{16}$Ne and $^{16}$C. Large isospin symmetry breaking on the level of wave function component weights is demonstrated for these states and discussed as three-body mechanism of Thomas-Ehrman shift. It is shown that the description of the Coulomb displacement energies requires a consistency among three parameters: the $^{16}$Ne decay energy $E_T$, the $^{15}$F ground state energy $E_r$, and the configuration mixing parameters for the $^{16}$Ne/$^{16}$C $0^+$ and $2^+$ states. Basing on this analysis we infer the $^{15}$F $1/2^+$ ground state energy to be $E_r=1.39-1.42$ MeV.

Grigorenko, L V; Zhukov, M V

2014-01-01T23:59:59.000Z

188

Thomas-Ehrman effect in a three-body model: $^{16}$Ne case  

E-Print Network (OSTI)

The dynamic mechanism of the Thomas-Ehrman shift is studied in three-cluster systems by example of $^{16}$Ne and $^{16}$C isobaric mirror partners. We predict configuration mixings for $0^+$ and $2^+$ states in $^{16}$Ne and $^{16}$C. Large isospin symmetry breaking on the level of wave function component weights is demonstrated for these states and discussed as three-body mechanism of Thomas-Ehrman shift. It is shown that the description of the Coulomb displacement energies requires a consistency among three parameters: the $^{16}$Ne decay energy $E_T$, the $^{15}$F ground state energy $E_r$, and the configuration mixing parameters for the $^{16}$Ne/$^{16}$C $0^+$ and $2^+$ states. Basing on this analysis we infer the $^{15}$F $1/2^+$ ground state energy to be $E_r=1.39-1.42$ MeV.

L. V. Grigorenko; T. A. Golubkova; M. V. Zhukov

2014-11-07T23:59:59.000Z

189

Dirac Phenomenological Analyses of Unpolarized Proton Inelastic Scattering from $^{22}$Ne  

E-Print Network (OSTI)

Unpolarized 800 MeV proton inelastic scatterings from an s-d shell nucleus $^{22}$Ne are analyzed using phenomenological optical potentials in the Dirac coupled channel formalism. The first-order rotational collective model is used to obtain the transition optical potentials for the low lying excited collective states that belong to the ground state rotational band of the nucleus. The optical potential parameters of Woods-Saxon shape and the deformation parameters of the excited states are varied phenomenologically using the sequential iteration method to reproduce the experimental differential cross section data. The effective central and spin-orbit optical potentials are obtained by reducing the Dirac equations to the Schr\\"odinger-like second-order differential equations and the surface-peaked phenomena are observed at the real effective central potentials when the scattering from $^{22}$Ne is considered. The obtained deformation parameters of the excited states are compared with those of the nonrelativistic calculations and another s-d shell nucleus $^{20}$Ne. The deformation parameters for the $2^+$ and the $4^+$ states of the ground state rotational band at the nucleus $^{22}$Ne are found to be smaller than those of $^{20}$Ne, indicating that the couplings of those states to the ground state are weaker at the nucleus $^{22}$Ne compared to those at the nucleus $^{20}$Ne. The multistep channel coupling effect is confirmed to be important for the $4^+$ state excitation of the ground state rotational band at the proton inelastic scattering from the s-d shell nucleus $^{22}$Ne.

Moon-Won Kim; Sugie Shim

2015-01-04T23:59:59.000Z

190

N.E. Leonard U. Pisa 18-20 April 2007Slide 1 Cooperative Control  

E-Print Network (OSTI)

1 N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 1 Cooperative Control and Mobile Sensor Networks.princeton.edu/~naomi N.E. Leonard ­ U. Pisa ­ 18-20 April 2007Slide 2 Key References [1] Leonard, Paley, Lekien. Pisa ­ 18-20 April 2007Slide 3 5 Scripps Spray Gliders 10 WHOI Slocum Gliders AOSN-II Glider Plan N

Leonard, Naomi

191

Emission of F23 and Ne24 in cluster radioactivity of Pa231  

Science Journals Connector (OSTI)

Using a track-recording phosphate glass detector with a standard deviation ?Z=0.23 charge unit, we collected ?2100 tracks of energetic clusters emitted from Pa231. Of these, 1348 survived cuts on energy, angle of incidence to the detectors, and ?2. All but one of them are consistent with Ne24, and our measured branching ratio, B(Ne/?)=(13.41.7)10-12, for an alpha-decay half-life for Pa231 of 3.28104 yr. This value of B is a factor of 2.2 greater than was determined by Tretyakova et al., who observed 252 Ne decays. We identify one event as F23, the nucleus predicted by cluster emission models to have the second highest branching ratio for emission from Pa231. This corresponds to a branching ratio B(Ne/F)=1347-940+6440, the 1? limits being governed by inverse Poisson statistics. Published models predict lower values of B(Ne/F), ranging from 3 to 400. Our event, if its 4? deviation from Ne is regarded as sufficient evidence for F, would be the first example of emission of an odd-Z cluster in spontaneous cluster radioactivity.

P. B. Price; R. Bonetti; A. Guglielmetti; C. Chiesa; R. Matheoud; C. Migliorino; K. J. Moody

1992-11-01T23:59:59.000Z

192

Posters Brightness Fields of Broken Clouds V. E. Zuev, G. A. Titov, E. I. Kasyanov, and D. A. Zimin  

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

1 1 Posters Brightness Fields of Broken Clouds V. E. Zuev, G. A. Titov, E. I. Kasyanov, and D. A. Zimin Institute of Atmospheric Optics, Siberian Branch Russian Academy of Sciences Tomsk, Russia Introduction The radiation budget and brightness field of the system "atmosphere-underlying surface" are controlled, to a considerable degree, by the variety of forms and the strong space-time variability of cloud cover. The space and angle structure of the radiation fields of cloudy atmosphere together with their sensitivity to cloud variations provide an important source of information needed to formulate and solve problems of the remote optical sensing of cloudy atmosphere (e.g., King 1987; Yi et al. 1990) and of satellite meteorology, as well as for retrievals of the albedo from

193

Neutrino-nucleus neutral current elastic interactions measurement in MiniBooNE  

SciTech Connect

The MiniBooNE experiment at the Fermi National Accelerator Laboratory (Fermilab) was designed to search for {nu}{sub {mu}} {yields} {nu}{sub e} neutrino oscillations at {Delta}m{sup 2} {approx} 1 eV{sup 2} using an intense neutrino flux with an average energy E{sub {nu}} {approx} 700 MeV. From 2002 to 2009 MiniBooNE has accumulated more than 1.0 x 10{sup 21} protons on target (POT) in both neutrino and antineutrino modes. MiniBooNE provides a perfect platform for detailed measurements of exclusive and semiinclusive neutrino cross-sections, for which MiniBooNE has the largest samples of events up to date, such as neutral current elastic (NCE), neutral current {pi}{sup 0}, charged current quasi-elastic (CCQE), charged current {pi}{sup +}, and other channels. These measured cross-sections, in turn, allow to improve the knowledge of nucleon structure. This thesis is devoted to the study of NCE interactions. Neutrino-nucleus neutral current elastic scattering ({nu}N {yields} {nu}N) accounts for about 18% of all neutrino interactions in MiniBooNE. Using a high-statistics, high purity sample of NCE interactions in MiniBooNE, the flux-averaged NCE differential cross-section has been measured and is being reported here. Further study of the NCE cross-section allowed for probing the structure of nuclei. The main interest in the NCE cross-section is that it may be sensitive to the strange quark contribution to the nucleon spin, {Delta}s, this however requires a separation of NCE proton ({nu}p {yields} {nu}p) from NCE neutron ({nu}n {yields} {nu}n) events, which in general is a challenging task. MiniBooNE uses a Cherenkov detector, which imposes restrictions on the measured nucleon kinematic variables, mainly due to the impossibility to reconstruct the nucleon direction below the Cherenkov threshold. However, at kinetic energies above this threshold MiniBooNE is able to identify NCE proton events that do not experience final state interactions (FSI). These events were used for the {Delta}s measurement. In this thesis MiniBooNE reports the NCE (n+p) cross-section, the measurement of the axial mass, M{sub A}, and the {Delta}s parameter from the NCE data.

Perevalov, Denis; /Alabama U.

2009-12-01T23:59:59.000Z

194

First Direct Measurement of the 17F(p,gamma)18Ne Cross Section  

SciTech Connect

The rate of the {sup 17}F(p,{gamma}){sup 18}Ne reaction is of significant importance in astrophysical events like novae and x-ray bursts. The decay of {sup 17}F is thought to help drive the expansion of the nova envelope, and the {sup 17}F(p,{gamma}){sup 18}Ne reaction affects the production of {sup 18}F, a target of gamma-ray astronomy, as well as being an important link in the ({alpha},p) reaction chain during the ignition phase of x-ray bursts. A 3{sup +} state in {sup 18}Ne predicted to dominate the rate was found at 599.8 keV using the {sup 17}F(p,p){sup 17}F reaction [1], but the resonance strength was unknown. For the first time, the {sup 17}F(p,{gamma}){sup 18}Ne reaction has been measured directly with the Daresbury Recoil Separator, using a mixed beam of radioactive {sup 17}F and stable {sup 17}O from the Holifield Radioactive Ion Beam Facility at Oak Ridge National Laboratory. A {gamma} width was found for the 599.8 keV resonance in {sup 18}Ne, and an upper limit on the direct capture S factor was determined at an intermediate energy of 800 keV.

Chipps, Kelly A [ORNL; Bardayan, Daniel W [ORNL; Blackmon, Jeff C [ORNL; Chae, K. Y. [University of Tennessee, Knoxville (UTK); Greife, U. [Colorado School of Mines, Golden; Hatarik, Robert [Rutgers University; Kozub, R. L. [Tennessee Technological University; Matei, Catalin [Oak Ridge Associated Universities (ORAU); Moazen, Brian [University of Tennessee, Knoxville (UTK); Nesaraja, Caroline D [ORNL; Pain, Steven D [ORNL; Peters, W. A. [Rutgers University; Pittman, S. T. [University of Tennessee, Knoxville (UTK); ShrinerJr., J. F. [Tennessee Technological University; Smith, Michael Scott [ORNL

2008-01-01T23:59:59.000Z

195

DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term  

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

DOE-NE Light Water Reactor Sustainability Program and EPRI DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term Operations Program - Joint Research and Development Plan DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term Operations Program - Joint Research and Development Plan Nuclear power has contributed almost 20% of the total amount of electricity generated in the United States over the past two decades. High capacity factors and low operating costs make nuclear power plants (NPPs) some of the most economical power generators available. Further, nuclear power remains the single largest contributor (nearly 70%) of non-greenhouse gas-emitting electric power generation in the United States. Even when major refurbishments are performed to extend operating life, these plants continue to represent cost-effective, low-carbon assets to the nation's

196

DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term  

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

DOE-NE Light Water Reactor Sustainability Program and EPRI DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term Operations Program - Joint Research and Development Plan DOE-NE Light Water Reactor Sustainability Program and EPRI Long-Term Operations Program - Joint Research and Development Plan Nuclear power has contributed almost 20% of the total amount of electricity generated in the United States over the past two decades. High capacity factors and low operating costs make nuclear power plants (NPPs) some of the most economical power generators available. Further, nuclear power remains the single largest contributor (nearly 70%) of non-greenhouse gas-emitting electric power generation in the United States. Even when major refurbishments are performed to extend operating life, these plants continue to represent cost-effective, low-carbon assets to the nation's

197

ARM - Field Campaign - 1996 NARSTO Northeast Field Study (NARSTO-NE)  

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

6 NARSTO Northeast Field Study (NARSTO-NE) 6 NARSTO Northeast Field Study (NARSTO-NE) Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : 1996 NARSTO Northeast Field Study (NARSTO-NE) 1996.07.01 - 1996.07.28 Lead Scientist : Larry Kleinman For data sets, see below. Description The DOE G-1 aircraft was deployed in the New York City metropolitan area as part of the North American Research Strategy for Tropospheric Ozone-Northeast effort to determine the causes of elevated ozone levels in the northeastern United States. Measurements of ozone, ozone precursors, and other photochemically active trace gases were made upwind and downwind of New York City with the objective of characterizing the ozone formation process and its dependence on ambient levels of NOx and volatile organic

198

Microsoft PowerPoint - Freeze.NE PA Overview_052511.ppt  

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

Used Fuel Disposition Campaign Used Fuel Disposition Campaign Summary of DOE-NE PA Modeling for Storage and Disposal of Used Nuclear Fuel (UNF), High-Level Radioactive Waste (HLW), and Low-Level Waste (LLW) Geoff Freeze Sandia National Laboratories PA Community of Practice Technical Exchange May 25-26, 2011 Print Close Used Fuel Disposition 2 DOE-Nuclear Energy (NE) - PA Modeling Activities NE Advanced Modeling and Simulation (NEAMS) Waste Integrated Performance and Safety Codes (Waste IPSC) Used Fuel Disposition (UFD) Generic Performance Assessment Model (GPAM) *** Initial modeling focus in both campaigns in on UNF/HLW disposal Print Close Used Fuel Disposition 3  UFD GPAM  Short time horizon (2-3 yrs) - Simplified generic system models (i.e., PA-fidelity using GoldSim) - Current computing capabilities

199

Skåne County, Sweden: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Skåne County, Sweden: Energy Resources Skåne County, Sweden: Energy Resources Jump to: navigation, search Name Skåne County, Sweden Equivalent URI DBpedia GeoNames ID 3337385 Coordinates 55.98333°, 13.5° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":55.98333,"lon":13.5,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

200

Charged-Current Neutral Pion production at SciBooNE  

SciTech Connect

SciBooNE, located in the Booster Neutrino Beam at Fermilab, collected data from June 2007 to August 2008 to accurately measure muon neutrino and anti-neutrino cross sections on carbon below 1 GeV neutrino energy. SciBooNE is studying charged current interactions. Among them, neutral pion production interactions will be the focus of this poster. The experimental signature of neutrino-induced neutral pion production is constituted by two electromagnetic cascades initiated by the conversion of the {pi}{sup 0} decay photons, with an additional muon in the final state for CC processes. In this poster, I will present how we reconstruct and select charged-current muon neutrino interactions producing {pi}{sup 0}'s in SciBooNE.

Catala-Perez, J.; /Valencia U., IFIC

2009-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

Charged-Current Neutral Pion production at SciBooNE  

E-Print Network (OSTI)

SciBooNE, located in the Booster Neutrino Beam at Fermilab, collected data from June 2007 to August 2008 to accurately measure muon neutrino and anti-neutrino cross sections on carbon below 1 GeV neutrino energy. SciBooNE is studying charged current interactions. Among them, neutral pion production interactions will be the focus of this poster. The experimental signature of neutrino-induced neutral pion production is constituted by two electromagnetic cascades initiated by the conversion of the neutral pion decay photons, with an additional muon in the final state for CC processes. In this poster, I will present how we reconstruct and select charged-current muon neutrino interactions producing neutral pions in SciBooNE.

Catala-Perez, J

2009-01-01T23:59:59.000Z

202

N NE EX XT T G GE EN NE ER RA AT TI IO ON N S SA AF FE EG  

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

NE NE EX XT T G GE EN NE ER RA AT TI IO ON N S SA AF FE EG GU UA AR RD DS S I IN NI IT TI IA AT TI IV VE E ( (N NG GS SI I) ) O OP PP PO OR RT TU UN NI IT TI IE ES S F FO OR R S ST TU UD DE EN NT TS S A AN ND D Y YO OU UN NG G P PR RO OF FE ES SS SI IO ON NA AL LS S I IN NT TE ER RE ES ST TE ED D I IN N S SA AF FE EG GU UA AR RD DS S/ /N NO ON NP PR RO OL LI IF FE ER RA AT TI IO ON N The Next Generation Safeguards Initiative (NGSI) was launched by the National Nuclear Security Administration (NNSA) in FY 2008 to develop the policies, concepts, technologies, expertise, and infrastructure necessary to strengthen and sustain the international safeguards system as it evolves to meet new challenges over the next 25 years. NGSI's Human Capital Development subprogram 1 aims to revitalize and expand the international safeguards human capital base in the United States by attracting, educating, training, and retaining

203

Structure and heat capacity of Ne and Xe adsorbed on a bundle of carbon nanotubes  

E-Print Network (OSTI)

The structural and thermal properties of Ne and Xe gases adsorbed on the outer surface of a large nanotube bundle have been evaluated with computer simulation. The potential energy model and numerical techniques were used previously to study Ar [N. M. Urban, S. M. Gatica, M. W. Cole, and J. L. Riccardo, ``Correlation functions and thermal properties of Ar adsorbed on the external surface of a bundle of carbon nanotubes'', Phys. Rev. B 71, 245410 (2005)]. Heat capacity results for Ne and Xe exhibit peaks associated with reordering and ``stripe'' melting transitions for these gases.

Daniel E. Shai; Nathan M. Urban; Milton W. Cole

2007-02-08T23:59:59.000Z

204

MicroBooNE: A New Liquid Argon Time Projection Chamber Experiment  

SciTech Connect

Liquid Argon Time Projection Chamber detectors are well suited to study neutrino interactions, and are an intriguing option for future massive detectors capable of measuring the parameters that characterize neutrino oscillations. These detectors combine fine-grained tracking with calorimetry, allowing for excellent imaging and particle identification ability. In this talk the details of the MicroBooNE experiment, a 175 ton LArTPC which will be exposed to Fermilab's Booster Neutrino Beamline starting in 2011, will be presented. The ability of MicroBooNE to differentiate electrons from photons gives the experiment unique capabilities in low energy neutrino interaction measurements.

Soderberg, M.

2009-10-01T23:59:59.000Z

205

Transport phenomena in intrinsic semiconductors and insulators at high current densities: Suppression of the broken neutrality drift  

SciTech Connect

It is shown that, in addition to the diffusion and broken neutrality drift (BND) modes well-known for insulators and very lightly doped semiconductors, the quasineutral drift (QND) mode is possible. The transition from the BND to QND mode is accompanied by the appearance of a portion with a very sharp current rise in the current-voltage characteristic. This effect is observed in a new type of semiconductor detectors (CIDs, Current Injected Detectors) of high-intensity neutron and proton radiation, suggested, in particular, for Large Hadron Collider. The effect is unambiguously attributed now to the presence of radiation-induced deep centers in a semiconductor. It is shown, however, in this paper that the effect of a very sharp rise in current upon a slight increase in voltage is even possible when there are no deep centers. An equation adequately describing the possible transport modes in intrinsic semiconductors and insulators is derived. The results of an analytical study are confirmed by an adequate simulation.

Mnatsakanov, T. T.; Tandoev, A. G.; Yurkov, S. N. [All-Russia Electrotechnical Institute, Krasnokazarmennaya 12, 111250 Moscow (Russian Federation)] [All-Russia Electrotechnical Institute, Krasnokazarmennaya 12, 111250 Moscow (Russian Federation); Levinshtein, M. E. [The Ioffe Physico-Technical Institute, Politekhnicheskaya 26, 194021 St. Petersburg (Russian Federation)] [The Ioffe Physico-Technical Institute, Politekhnicheskaya 26, 194021 St. Petersburg (Russian Federation)

2013-08-14T23:59:59.000Z

206

Oil and Gas CDT Cenomanian-Turonian Palaeoenvironments of NE Brazil  

E-Print Network (OSTI)

Oil and Gas CDT Cenomanian-Turonian Palaeoenvironments of NE Brazil Margin University of Birmingham, biostratigraphy, Brazil, Cretaceous Overview The Late Cretaceous stratigraphy of the Equatorial margin of North East Brazil holds a unique record of the final stages of the opening of the South Atlantic. During

Henderson, Gideon

207

Cooperative Equilibrium Nash equilibrium (NE) assumes that players always make a  

E-Print Network (OSTI)

cooperative equilibrium (PCE). PCE may help explain players' behavior in games where cooper- ation is observed in practice. A player's payoff in a PCE is at least as high as in any NE. However, a PCE does not always exist. We thus consider -PCE, where takes into account the degree of cooperation; a PCE is a 0-PCE. Every

Halpern, Joseph Y.

208

Searches for new physics at MiniBooNE : sterile neutrinos and mixing freedom  

E-Print Network (OSTI)

The MiniBooNE experiment was designed to perform a search for Vu --> Ve oscillations in a region of A[delta]sin 2 20very different from that allowed by standard, three neutrino oscillations, as determined by solar and ...

Karagiorgi, Georgia S. (Georgia Stelios)

2010-01-01T23:59:59.000Z

209

MiniBooNE Charged Current Neutral Pion Cross Section Data Release  

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

Muon Neutrino Induced Charged Current Neutral Pion Cross Sections on Mineral Oil at Enu0.5-2.0 GeV" , arXiv:1010.3264 hep-ex The following MiniBooNE information for the 2010 CC...

210

COLUMBIA RIVER INTER-TRIBAL FISH COMMISSION 700 NE Multnomah Street, Suite 1200  

E-Print Network (OSTI)

COLUMBIA RIVER INTER-TRIBAL FISH COMMISSION 700 NE Multnomah Street, Suite 1200 Portland, Oregon 97232 F (503) 235-4228 (503) 238-0667 F (503) 235-4228 www.critfc.org Putting fish back in the rivers and protecting the watersheds where fish live September 17, 2013 Bill Bradbury, Chairman Northwest Power

211

CONGESTION IN THE ISO-NE ELECTRICITY MARKETS ANNA BARBARA IHRIG  

E-Print Network (OSTI)

CONGESTION IN THE ISO-NE ELECTRICITY MARKETS BY ANNA BARBARA IHRIG THESIS Advisor: Prof. George Gross Submitted in partial fulfillment of the requirements for the degree of "Diplom-Wirtschaftsingenieur, technische Fachrichtung Elektrotechnik" at Darmstadt University of Technology, Germany. G. Gross Thesis

Gross, George

212

Power broadening effects on Electromagnetically Induced Transparency in $^{20}$Ne vapor  

E-Print Network (OSTI)

We report here the first observation of electromagnetically induced transparency (EIT) in $^{20}$Ne. The power broadening of the EIT linewidth is measured as a function of neon pressure and RF excitation power. Doppler effects on the EIT broadening are found even at low pressures and low intensities, where the linewidth should be governed only by homogeneous effects.

Lubotzky, Boaz; Kong, Tao; Katz, Nadav; Ron, Guy

2014-01-01T23:59:59.000Z

213

Power broadening effects on Electromagnetically Induced Transparency in $^{20}$Ne vapor  

E-Print Network (OSTI)

We report here the first observation of electromagnetically induced transparency (EIT) in $^{20}$Ne. The power broadening of the EIT linewidth is measured as a function of neon pressure and RF excitation power. Doppler effects on the EIT broadening are found even at low pressures and low intensities, where the linewidth should be governed only by homogeneous effects.

Boaz Lubotzky; David Shwa; Tao Kong; Nadav Katz; Guy Ron

2014-02-25T23:59:59.000Z

214

High pressure measurements of the He-Ne binary phase diagram at 296 K: Evidence for the stability of a stoichiometric Ne(He)2 solid  

Science Journals Connector (OSTI)

The binary phase diagram of He-Ne mixtures has been measured at 296 K in a diamond anvil cell. It is of the eutectic type with no fluid-fluid separation of phases. A homogeneous solid mixture is shown to be stable for a mole fraction of He equal to 2/3. Single-crystal synchrotron x-ray measurements indicate that this solid is ordered with 12 atoms in the unit cell. Gibbs free energy calculations support the attribution to the MgZn2 type structure. It is the first Laves phase observed in a van der Waals molecular compound,

Paul Loubeyre; Michel Jean-Louis; Ren LeToullec; Lydie Charon-Grard

1993-01-11T23:59:59.000Z

215

Hidden Secrets, Broken Hearts  

E-Print Network (OSTI)

grace was that it was not Starsky's face. "You said soon, Hutch. And that was days ago," Starsky reminded him. "I know," Hutch admitted. "I'm your partner, ain't I, Hutch?" Starsky asked softly. Hutch cringed, knowing exactly where this was going. "Of... the park. "Okay," Starsky agreed, tucking the ball against his waist and moving in on his partner. Hutch held the advancing body at bay by catching the hand that was once again reaching for his towel. "Do you want to play, or do you want to play?" he asked...

Multiple Contributors

2004-01-01T23:59:59.000Z

216

PI Research Organisation Project Title NE/J024678/1 Dr Christopher Davis University of Reading Driving space weather forecasts with real data  

E-Print Network (OSTI)

Lead Grant Reference PI Research Organisation Project Title NE/J024678/1 Dr Christopher Davis Troposphere and the Routing of Aircraft (EXTRA)Professor Keith Shine University of Reading NE/J023760

217

Probing Ligand Effects on the Redox Energies of [4Fe-4S] Clusters Using Broken-Symmetry Density Functional Theory  

SciTech Connect

A central issue in understanding redox properties of iron-sulfur proteins is determining the factors that tune the reduction potentials of the Fe-S clusters. Recently, Solomon and coworkers have shown that the Fe-S bond covalency of protein analogs measured by %L, the percent ligand character of the Fe 3d orbitals, from ligand K-edge X-ray absorption spectroscopy (XAS) correlates with the electrochemical redox potentials. Also, Wang and coworkers have measured electron detachment energies for iron-sulfur clusters without environmental perturbations by gas-phase photoelectron spectroscopy (PES). Here the correlations of the ligand character with redox energy and %L character are examined in [Fe?S?L?]2? clusters with different ligands by broken symmetry density functional theory (BS-DFT) calculations using the B3LYP functional together with PES and XAS experimental results. These gas-phase studies assess ligand effects independently of environmental perturbations and thus provide essential information for computational studies of iron-sulfur proteins. The B3LYP oxidation energies agree well with PES data, and the %L character obtained from natural bond orbital analysis correlates with XAS values, although it systematically underestimates them because of basis set effects. The results show that stronger electron-donating terminal ligands increase %Lt, the percent ligand character from terminal ligands, but decrease %Sb, the percent ligand character from the bridging sulfurs. Because the oxidized orbital has significant Fe-Lt antibonding character, the oxidation energy correlates well with %Lt. However, because the reduced orbital has varying contributions of both Fe-Lt and Fe-Sb antibonding character, the reduction energy does not correlate with either %Lt or %Sb. Overall, BSDFT calculations together with XAS and PES experiments can unravel the complex underlying factors in the redox energy and chemical bonding of the [4Fe-4S] clusters in iron-sulfur proteins.

Niu, Shuqiang; Ichiye, Toshiko

2009-05-14T23:59:59.000Z

218

Searches for New Physics at MiniBooNE: Sterile Neutrinos and Mixing Freedom  

SciTech Connect

The MiniBooNE experiment was designed to perform a search for {nu}{sub {mu}} {yields} {nu}{sub e} oscillations in a region of {Delta}m{sup 2} and sin{sup 2} 2{theta} very different from that allowed by standard, three-neutrino oscillations, as determined by solar and atmospheric neutrino experiments. This search was motivated by the LSND experimental observation of an excess of {bar {nu}}{sub e} events in a {bar {nu}}{sub {mu}} beam which was found compatible with two-neutrino oscillations at {Delta}m{sup 2} {approx} 1 eV{sup 2} and sin{sup 2} 2{theta} < 1%. If confirmed, such oscillation signature could be attributed to the existence of a light, mostly-sterile neutrino, containing small admixtures of weak neutrino eigenstates. In addition to a search for {nu}{sub {mu}} {yields} {nu}{sub e} oscillations, MiniBooNE has also performed a search for {bar {nu}}{sub {mu}} {yields} {bar {nu}}{sub e} oscillations, which provides a test of the LSND two-neutrino oscillation interpretation that is independent of CP or CPT violation assumptions. This dissertation presents the MiniBooNE {nu}{sub {mu}} {yields} {nu}{sub e} and {bar {nu}}{sub {mu}} {yields} {bar {nu}}{sub e} analyses and results, with emphasis on the latter. While the neutrino search excludes the two-neutrino oscillation interpretation of LSND at 98% C.L., the antineutrino search shows an excess of events which is in agreement with the two-neutrino {bar {nu}}{sub {mu}} {yields} {bar {nu}}{sub e} oscillation interpretation of LSND, and excludes the no oscillations hypothesis at 96% C.L. Even though the neutrino and antineutrino oscillation results from MiniBooNE disagree under the single sterile neutrino oscillation hypothesis, a simple extension to the model to include additional sterile neutrino states and the possibility of CP violation allows for differences between neutrino and antineutrino oscillation signatures. In view of that, the viability of oscillation models with one or two sterile neutrinos is investigated in global fits to MiniBooNE and LSND data, with and without constraints from other oscillation experiments with similar sensitivities to those models. A general search for new physics scenarios which would lead to effective non-unitarity of the standard 3 x 3 neutrino mixing matrix, or mixing freedom, is also performed using neutrino and antineutrino data available from MiniBooNE.

Karagiorgi, Georgia S.; /MIT

2010-07-01T23:59:59.000Z

219

Origin of Ne Emission Line of Very Luminous Soft X-ray Transient MAXI J0158$-$744  

E-Print Network (OSTI)

We investigate the mechanism to reproduce notable spectral features at the ignition phase of nova explosion observed for a super-Eddington X-ray transient source MAXI J0158$-$744 in the Small Magellanic Cloud. These are a strong Ne IX emission line at 0.92 keV with a large equivalent width of $0.32^{+0.21}_{-0.11}$ keV and the absence of Ne X line at 1.02 keV. In this paper, we calculate the radiative transfer using a Monte Carlo code, taking into account the line blanketing effect due to transitions of N, O, Ne, Mg and Al ions in an accelerating wind emanating from a white dwarf with a structure based on a spherically symmetric stationary model. We found that the strong Ne IX line can be reproduced if the mass fraction of Ne is enhanced to $10^{-3}$ or more and that of O is reduced to $\\sim5\\times10^{-9}$ or less and that the absence of other lines including Ne X ions at higher energies can be also reproduced by the line blanketing effect. This enhancement of the Ne mass fraction indicates that the ejecta ar...

Ohtani, Yukari; Shigeyama, Toshikazu

2014-01-01T23:59:59.000Z

220

Neutron-induced gamma-ray production cross sections for the first excited-state transitions in Ne-20 and Ne-22  

E-Print Network (OSTI)

Background: Neutron-induced reactions are a significant concern for experiments that require extremely low levels of radioactive backgrounds. Measurements of gamma-ray production cross sections over a wide energy range will help to predict and identify neutron backgrounds in these experiments. Purpose: Determine partial gamma-ray production cross sections for neutron-induced reactions in natural neon. Methods: The broad-spectrum neutron beam at the Los Alamos Neutron Science Center (LANSCE) was used for the measurement. Gamma rays from neutron-induced reactions were detected using the GErmanium Array for Neutron Induced Excitations (GEANIE). Results: Partial gamma-ray cross sections were measured for the first excited-state transitions in Ne-20 and Ne-22. The measured cross sections were compared to the TALYS and CoH3 nuclear reaction codes. Conclusions: These are the first experimental data for (n,n') reactions in neon. In addition to providing data to aid in the prediction and identification of neutron backgrounds in low-background experiments, these new measurements will help refine cross-section predictions in a mass region where models are not well constrained.

S. MacMullin; M. Boswell; M. Devlin; S. R. Elliott; N. Fotiades; V. E. Guiseppe; R. Henning; T. Kawano; B. H. LaRoque; R. O. Nelson; J. M. O'Donnell

2012-10-03T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

Ronald E. Gill (NE), Scoville, ID - Level I Curtis Roth (EM), Idaho  

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

E. Gill (NE), E. Gill (NE), Scoville, ID - Level I Curtis Roth (EM), Idaho Falls, ID - Level I Jared T. Howerton (NNSA), Oak Ridge, TN - Level I Richard L. Person (NNSA), DOE HQ - Level I Phillip (Tony) A. Polk (EM), Aiken, SC (Savannah River) - Level IV Jane Powell-Dolan (LM), Cincinnati, OH - Level I Eric M. Thompson (NNSA), Oak Ridge, TN - Level II Congratulations to our newly certified FPDs! The Certification Review Board (CRB or 'the Board') convened on Friday, Sep- tember 24 to review certifi- cation candidates and dis- cuss several topics. The Department of Energy (DOE) met the FY2010 tar- gets for the Root Cause Analysis, Corrective Action Plan metrics 7 and 8, as fol- lows: DOE surpassed the target for Metric #7 (95% of pro-

222

DOE-NE-STD-1004-92; Root Cause Analysis Guidance Document  

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

NE-STD-1004-92 NE-STD-1004-92 DOE GUIDELINE ROOT CAUSE ANALYSIS GUIDANCE DOCUMENT February 1992 U.S. Department of Energy Office of Nuclear Energy Office of Nuclear Safety Policy and Standards Washington, D.C. 20585 ii ABSTRACT DOE Order 5000.3A, "Occurrence Reporting and Processing of Operations Information," investigation and reporting of occurrences (including the performance of root cause analysis) requires the and the selection, implementation, and follow-up of corrective actions. The level of effort expended should be based on the significance attached to the occurrence. Most off-normal occurrences need only a scaled- down effort while most emergency occurrences should be investigated using one or more of the formal analytical models. A discussion of methodologies, instructions, and worksheets in this document guides

223

File:USDA-CE-Production-GIFmaps-NE.pdf | Open Energy Information  

Open Energy Info (EERE)

NE.pdf NE.pdf Jump to: navigation, search File File history File usage Nebraska Ethanol Plant Locations Size of this preview: 776 × 600 pixels. Full resolution ‎(1,650 × 1,275 pixels, file size: 278 KB, MIME type: application/pdf) Description Nebraska Ethanol Plant Locations Sources United States Department of Agriculture Related Technologies Biomass, Biofuels, Ethanol Creation Date 2010-01-19 Extent State Countries United States UN Region Northern America States Nebraska External links http://www.nass.usda.gov/Charts_and_Maps/Ethanol_Plants/ File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 16:18, 27 December 2010 Thumbnail for version as of 16:18, 27 December 2010 1,650 × 1,275 (278 KB) MapBot (Talk | contribs) Automated bot upload

224

NE-23 Disposal of Offsite-Generated Defense Radioactive Waste, Ventron  

Office of Legacy Management (LM)

pi/L +3 pi/L +3 *3L 52. NE-23 Disposal of Offsite-Generated Defense Radioactive Waste, Ventron FUSRAP Site Jill E. Lytle, DP-12 NE-23 The Office of Remedial Action and Waste Technology has received a request from the Technical Services Division, DOE-Oak Ridge Operations Office, for a determination of the appropriate disposal location for the material which will result from remedial action of the Ventron site in Beverly, Massachusetts. The Ventron site was used from 1942 to 1948 under contract to the ME0 and AEC for converting uranium oxide to uranium metal powder, as well as later operations involving recovery of uranium from scrap uranium and turnings from the fuel fabrication plant at Hanford, Washington. Full-scale remedial action, anticipated to result in approximately 5,000

225

ANL/NE-13/9 SHARP Assembly-Scale Multiphysics Demonstration  

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

NE-13/9 NE-13/9 SHARP Assembly-Scale Multiphysics Demonstration Simulations Mathematics and Computation Division & Nuclear Engineering Division About Argonne National Laboratory Argonne is a U.S. Department of Energy laboratory managed by UChicago Argonne, LLC under contract DE-AC02-06CH11357. The Laboratory's main facility is outside Chicago, at 9700 South Cass Avenue, Argonne, Illinois 60439. For information about Argonne and its pioneering science and technology programs, see www.anl.gov. Availability of This Report This report is available, at no cost, at http://www.osti.gov/bridge. It is also available on paper to the U.S. Department of Energy and its contractors, for a processing fee, from: U.S. Department of Energy Office of Scientific and Technical Information

226

Neutron Transfer Studied with a Radioactive beam of 24Ne, using TIARA at SPIRAL  

E-Print Network (OSTI)

A general experimental technique for high resolution studies of nucleon transfer reactions using radioactive beams is briefly described, together with the first new physics results that have been obtained with the new TIARA array. These first results from TIARA are for the reaction 24Ne(d,p)25Ne, studied in inverse kinematics with a pure radioactive beam of 100,000 pps from the SPIRAL facility at GANIL. The reaction probes the energies of neutron orbitals relevant to very neutron rich nuclei in this mass region and the results highlight the emergence of the N=16 magic number for neutrons and the associated disappearance of the N=20 neutron magic number for the very neutron rich neon isotopes.

W. N. Catford; C. N. Timis; R. C. Lemmon; M. Labiche; N. A. Orr; L. Caballero; R. Chapman; M. Chartier; M. Rejmund; H. Savajols; for the TIARA Collaboration

2009-12-20T23:59:59.000Z

227

Neutral Current pi0 Production in the MiniBooNE Antineutrino Data  

E-Print Network (OSTI)

The single largest background to future numubar to nuebar (numu to nue) oscillation searches is neutral current pi0 production. MiniBooNE, which began taking antineutrino data in January 2006, has the world's largest sample of pi0's produced by antineutrinos in the 1 GeV energy range. These neutral pions are primarily produced through the delta resonance but can also be created through "coherent production." The latter process is the coherent sum of glancing scatters of (anti)neutrinos off a neutron or proton, in which the nucleus is kept intact but a pi0 is created. Current analysis of NC pi0 production in the MiniBooNE antineutrino data will be discussed.

V. T. Nguyen

2008-01-04T23:59:59.000Z

228

NC pi0 Production in the MiniBooNE Antineutrino Data  

E-Print Network (OSTI)

The single largest background to future numubar to nuebar (numu to nue) oscillation searches is neutral current pi0 production. MiniBooNE, which began taking antineutrino data in January 2006, has the world's largest sample of pi0's produced by antineutrinos in the 1 GeV energy range. These neutral pions are primarily produced through the delta resonance but can also be created through "coherent production." The latter process is the coherent sum of glancing scatters of (anti)neutrinos off a neutron or proton, in which the nucleus is kept intact but a pi0 is created. Current analysis of NC pi0 production in the MiniBooNE antineutrino data will be discussed.

V. T. Nguyen

2008-01-02T23:59:59.000Z

229

Conical Emission from Shock Waves in Ne(1-20 AGeV)+U Collisions  

E-Print Network (OSTI)

The formation and propagation of high-density compression waves, e.g. Mach shock waves, in cold nuclear matter is studied by simulating high-energy nucleus-nucleus collisions of Ne with U in the energy range from E_lab = 0.5 AGeV to 20 AGeV. In an ideal hydrodynamic approach, the high-density shock wave created by the small Ne nucleus passing through the heavy U nucleus is followed by a slower and more dilute Mach shock wave which causes conical emission of particles at the Mach cone angle. The conical emission originates from low-density regions with a small flow velocity comparable to the speed of sound. Moreover, it is shown that the angular distributions of emitted baryons clearly distinguish between a hydrodynamic approach and binary cascade processes used in the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) transport model.

Philip Rau; Jan Steinheimer; Barbara Betz; Hannah Petersen; Marcus Bleicher; Horst Stcker

2010-03-05T23:59:59.000Z

230

The thermonuclear rate for the 19F(a,p)22Ne reaction at stellar temperatures  

E-Print Network (OSTI)

The $^{19}$F($\\alpha$,p)$^{22}$Ne reaction is considered to be one of the main sources of fluorine depletion in AGB and Wolf-Rayet stars. The reaction rate still retains large uncertainties due to the lack of experimental studies available. In this work the yields for both exit channels to the ground state and first excited state of $^{22}$Ne have been measured and several previously unobserved resonances have been found in the energy range E$_{lab}$=792-1993 keV. The level parameters have been determined through a detailed R-matrix analysis of the reaction data and a new reaction rate is provided on the basis of the available experimental information.

Claudio Ugalde; Richard Azuma; Aaron Couture; Joachim Grres; Hye-Young Lee; Edward Stech; Elizabeth Strandberg; Wanpeng Tan; Michael Wiescher

2008-03-04T23:59:59.000Z

231

Dirac Phenomenological Analyses of Unpolarized Proton Inelastic Scattering from $^{22}$Ne  

E-Print Network (OSTI)

Unpolarized 800 MeV proton inelastic scatterings from an s-d shell nucleus $^{22}$Ne are analyzed using phenomenological optical potentials in the Dirac coupled channel formalism. The first-order rotational collective model is used to obtain the transition optical potentials for the low lying excited collective states that belong to the ground state rotational band of the nucleus. The optical potential parameters of Woods-Saxon shape and the deformation parameters of the excited states are varied phenomenologically using the sequential iteration method to reproduce the experimental differential cross section data. The effective central and spin-orbit optical potentials are obtained by reducing the Dirac equations to the Schr\\"odinger-like second-order differential equations and the surface-peaked phenomena are observed at the real effective central potentials when the scattering from $^{22}$Ne is considered. The obtained deformation parameters of the excited states are compared with those of the nonrelativist...

Kim, Moon-Won

2015-01-01T23:59:59.000Z

232

K-vacancy levels in Ne, Mg, Si, S, Ar, and Ca  

E-Print Network (OSTI)

The HFR and AUTOSTRUCTURE atomic structure codes are used to compute complete data sets of level energies, wavelengths, A-values, and radiative and Auger widths for K-vacancy states of the Ne, Mg, Si, S, Ar, and Ca isonuclear sequences. Ions with electron number N>9 are treated for the first time. Detailed comparisons with previous measurements and theoretical data for ions with N<=9 are carried out in order to estimate reliable accuracy ratings.

P. Palmeri; P. Quinet; C. Mendoza; M. A. Bautista; J. Garcia; T. R. Kallman

2008-04-04T23:59:59.000Z

233

Les Roms ? Ils ne sont pas encore prts se reprsenter eux-mmes !  

E-Print Network (OSTI)

401 « Les Roms ? Ils ne sont pas encore prêts à se représenter eux-mêmes ! » Les tensions entre groupes Roms et associations « gadjé » à Milan Tommaso VITALE et Laura BOSCHETTI Centre d en rectangle, la réunion du Tavolo Rom, la « Table Rom », a lieu un lundi sur deux à 18 h 00. Cela

Paris-Sud XI, Université de

234

Hole transport in the rare-gas solids Ne, Ar, Kr, and Xe  

Science Journals Connector (OSTI)

This paper reports an investigation of the drift mobility of excess holes in solid Ne, Ar, Kr, and Xe. Thin-crystal specimens (50-500 ?m thick) were grown from the liquid between parallel-plate electrodes in a chamber attached to a miniature cryostat after purification of the starting gas. As in previous work on the electron transport in rare-gas solids and liquids, an electron-beam technique was used to generate excess carriers near one of the electrodes. Holes were extracted by the applied field and their transit time was measured directly, leading to the drift mobility ?h. Close to the triple points, ?h values in the above crystals lie between 1 10-2 and 4 10-2 cm2 V-1 sec-1, several orders of magnitude lower than the corresponding electron mobilities. The form of the temperature dependence of ?h changes progressively from Xe(?h?T-1.6) to an essentially activated mobility in Ar and Ne. The experimental results have been analyzed in terms of small-polaron theory, using both the adiabatic and nonadiabatic approximations. The theory can account for the different forms of the temperature dependence and possible ranges of values for the predominant phonon energy, the polaron binding energy and the transfer energy for holes have been deduced in each case. These quantities, characterizing the hole hopping transport, vary systematically from Xe to Ne and their correlation is discussed in some detail.

P. G. Le Comber; R. J. Loveland; W. E. Spear

1975-04-15T23:59:59.000Z

235

The KM3NeT deep-sea neutrino telescope  

E-Print Network (OSTI)

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will host the next generation Cherenkov neutrino telescope and nodes for a deep sea multidisciplinary observatory, providing oceanographers, marine biologists, and geophysicists with real time measurements. The neutrino telescope will complement IceCube in its field of view and exceed it substantially in sensitivity. Its main goal is the detection of high energy neutrinos of astrophysical origin. The detector will have a modular structure with six building blocks, each consisting of about one hundred Detection Units (DUs). Each DU will be equipped with 18 multi-PMT digital optical modules. The first phase of construction has started and shore and deep-sea infrastructures hosting the future KM3NeT detector are being prepared offshore Toulon, France and offshore Capo Passero on Sicily, Italy. The technological solutions for the neutrino detector of KM3NeT and the expected performance of the neutrino telescope are present...

Margiotta, Annarita

2014-01-01T23:59:59.000Z

236

Neon Lights Up a Controversy: the Solar Ne/O Abundance  

E-Print Network (OSTI)

The standard solar model was so reliable that it could predict the existence of the massive neutrino. Helioseismology measurements were so precise that they could determine the depth of the convection zone. This agreement between theory and observation was the envy of all astrophysics -- until recently when sophisticated three-dimensional hydrodynamic calculations of the solar atmosphere reduced the metal content by a factor of almost two. Antia & Basu (2005) suggested that a higher value of the solar neon abundance, Ne/O = 0.52, would resolve this controversy. Drake & Testa (2005) presented strong evidence in favor of this idea from a sample of 21 Chandra stars with enhanced values of the neon abundance, Ne/O = 0.41. In this paper, we have analyzed solar active region spectra from the archive of the Flat Crystal Spectrometer on Solar Maximum Mission, a NASA mission from the 1980s, as well as full-Sun spectra from the pioneering days of X-ray astronomy in the 1960s. These data seem consistent with the standard neon-to-oxygen abundance value, Ne/O = 0.15 (Grevesse & Sauval 1998). If these results prove to be correct, than the enhanced-neon hypothesis will not resolve the current controversy.

J. T. Schmelz; K. Nasraoui; J. K. Roames; L. A. Lippner; J. W. Garst

2005-10-07T23:59:59.000Z

237

Conservation off the Port Bow  

E-Print Network (OSTI)

The Applied Biodiversity Sciences Perspectives Series is a student-directed collection of contributions from graduate student and faculty members of the integrative, NSF-IGERT Applied Biodiversity Sciences (ABS) program at Texas A&M University...

Woodman, Constance

2014-10-07T23:59:59.000Z

238

Overshoots in planetary bow shocks  

Science Journals Connector (OSTI)

... probed by planetary spacecraft so far. These shocks both deflect the supersonic, or supermagnetosonic, solar wind around the planets and heat the ... wind around the planets and heat the solar wind. Part of the incoming ...

C. T. Russell; M. M. Hoppe; W. A. Livesey

1982-03-04T23:59:59.000Z

239

Nuclear Structure Properties of Astrophysical Importance for 19Ne above the Proton Threshold Energy  

SciTech Connect

Knowledge of the 18F(p,a)15O and 18F(p,g)19Ne astrophysical reaction rates are important to understand -ray emission from nova explosions and heavy-element production in x-ray bursts. The rates for these reactions have been uncertain, in part due to a lack of a comprehensive examination of the available structure information in the compound nucleus 19Ne. We have examined the latest experimental measurements with radioactive and stable beams, collected all the structure information in the nucleus 19Ne and its mirror 19F, and made estimates of unmeasured 19Ne nuclear-level parameters. These parameters will be useful for future reaction rate calculations.

Nesaraja, Caroline D [ORNL; Shu, Nengchuan [ORNL; Bardayan, Daniel W [ORNL; Blackmon, Jeff C [ORNL; Chen, Y. S. [China Institute of Atomic Energy; Kozub, R. L. [Tennessee Technological University; Smith, Michael Scott [ORNL

2007-01-01T23:59:59.000Z

240

Effects of thermal pollution on the soft-bottoms surrounding a power station in the Canary Islands (NE Atlantic ocean)  

Science Journals Connector (OSTI)

The spatial and temporal effects of hot seawater (6070C) from a power station on nearby soft-bottom communities were ... coast of Tenerife, Canary Islands, NE Atlantic Ocean). The samples were taken during summ...

Rodrigo Riera; Jorge Nez; Daniel Martn

2011-12-01T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

NE-24  

Office of Legacy Management (LM)

the Bureau of Hines Site at Albany, Oregon, for Remedial the Bureau of Hines Site at Albany, Oregon, for Remedial Action Under the Formerly Utilized Sites Remedial Action Program I L@ _I' J.-La&one, Manager Oak Ridge Operations Office Based on the data in the attached draft reports, it has been determined that the subject site is contaminated with residual radioactive material ' as a result of Manhattan Engineer District/Atomic Energy Commission operations P * at this site. The contamination is in excess of the acceptable guidelines and warrants some form of remedial action under the Fornlerly Utilized Sites Reriledial Action Program. It should be noted that the attached reports are draft reports and although subject to change, the changes expected will not effect the designation of the site; therefore, the reports are Suitable for -

242

NE-23  

Office of Legacy Management (LM)

s,' s,' Whidd Pk. Yilljam West West Orange Tennis Club, Inc. 200 Pleasant Valley Way West Orange, New Jersey 07052 Dear Mr. West: The Department of Energy (DOE), as part of its Formerly Utilized Sites Remedial Action Program (FUSRAP), has reviewed information on Vitro Laboratories, formerly located on what is now property of the West Orange Tennis Club, to determine whether it contains residual radioactivity traceable to activities conducted on behalf of the Atomic Energy Commission (a predecessor to DOE). A radiological survey indicated that the radiation levels and radionuclide concentrations are at or near natural background levels. Therefore, no remedial action is required, and DOE is eliminating the former Vitro site from further consideration under FL&RAP.

243

NE-23:  

Office of Legacy Management (LM)

residual radioactivity traceable to activities conducted on behalf of the Manhattan Engineer District or the Atomic Energy Commission (predecessors to DOE). A radiological survey...

244

New Results from MiniBooNE: A Search for Electron Antineutrino Appearance at $\\sim$1 eV$^2$  

E-Print Network (OSTI)

These proceedings summarize the first MiniBooNE electron antineutrino appearance search results, corresponding to a data sample collected for 3.39$\\times10^{20}$ protons on target (POT). The search serves as a direct test of the LSND oscillation signature, and provides complementary information which can be used in studies addressing the MiniBooNE neutrino-mode low-energy excess.

G. Karagiorgi; for the MiniBooNE Collaboration

2009-10-01T23:59:59.000Z

245

Response to 'Comment on 'Heat capacity, enthalpy fluctuations, and configurational entropy in broken ergodic systems'' [J. Chem. Phys. 134, 147101 (2011)  

SciTech Connect

We show that Johari's critique of our work is based on a misunderstanding of ergodic theory and a disregard for the broken ergodic nature of glass. His analysis is in contradiction with well established experimental results in specific heat spectroscopy, shear-mechanical spectroscopy, and the vanishing of heat capacity in the limit of zero temperature. Based on these misinterpretations, Johari arrives at the erroneous conclusion that the residual entropy of glass is real. However, we show that Johari's result is an artifact in direct contradiction with both rigorous theory and experimental measurements.

Mauro, John C. [Science and Technology Division, Corning Incorporated, SP-FR-05-1, Corning, New York 14831 (United States); Loucks, Roger J. [Department of Physics and Astronomy, Alfred University, One Saxon Drive, Alfred, New York 14802 (United States); Sen, Sabyasachi [Department of Chemical Engineering and Materials Science, University of California-Davis, One Shields Avenue, Davis, California 95616 (United States)

2011-04-14T23:59:59.000Z

246

MiniBooNE Neutrino Physics at the University of Alabama  

SciTech Connect

This report summarizes the activities conducted by the UA group under the auspices of the DoE/EPSCoR grant number DE--FG02--04ER46112 since the date of the previous progress report, i.e., since November 2005. It also provides a final report of the accomplishments achieved during the entire period of this grant (February 2004 to January 2007). The grant has fully supported the work of Dr. Yong Liu (postdoctoral research assistant -- in residence at Fermilab) on the MiniBooNE reconstruction and particle identification (PID) algorithms.

Ion Stancu

2007-04-27T23:59:59.000Z

247

DOE-NE Proliferation and Terrorism Risk Assessment: FY12 Plans Update  

SciTech Connect

This presentation provides background information on FY12 plans for the DOE Office of Nuclear Energy Proliferation and Terrorism Risk Assessment program. Program plans, organization, and individual project elements are described. Research objectives are: (1) Develop technologies and other solutions that can improve the reliability, sustain the safety, and extend the life of current reactors; (2) Develop improvements in the affordability of new reactors to enable nuclear energy; (3) Develop Sustainable Nuclear Fuel Cycles; and (4) Understand and minimize the risks of nuclear proliferation and terrorism - Goal is to enable the use of risk information to inform NE R&D program planning.

Sadasivan, Pratap [Los Alamos National Laboratory

2012-06-21T23:59:59.000Z

248

Differential Cross Sections for the Excitation of Single Rotational Quantum Transitions: HD + Ne  

Science Journals Connector (OSTI)

Differential cross sections for the rotational excitation from j=0 to j=1 of HD molecules in collisions with Ne atoms have been measured in a crossed molecular beam experiment. The inelasticity is obtained by time-of-flight analysis of the scattered particles using the pseudorandom chopper method. The measured cross sections of 0.31 to 0.45 2/sr at energies of about 30 meV and angles between 40 and 80 prove very sensitive to the angle-dependent part of the interaction potential as shown by a comparison with calculated data.

U. Buck; F. Huisken; J. Schleusener; H. Pauly

1977-03-28T23:59:59.000Z

249

The response of NE 102 to 2.6-28.0 MeV neutrons  

E-Print Network (OSTI)

are not sufficiently precise for 1 detector efficiency de~tion in this region. Although the re~as 2-7 function of NE 102 has been studied by several groups ), the data are This paper follows the style and format of Nuclear Instr!ments and Nethods. tco sparse...V, was found to be about 3. 4%. The data of Gettner and Selove and of Czirr et al. were at tco low an ~ for direct comparison with the present data. They were, however, considered when calculating the zero ~lated curve. 'Ihe curve is a least squares fitted...

Martin, Stephen Dobie

2012-06-07T23:59:59.000Z

250

Thermonuclear reaction rate of $^{18}$Ne($?$,$p$)$^{21}$Na from Monte-Carlo calculations  

E-Print Network (OSTI)

The $^{18}$Ne($\\alpha$,$p$)$^{21}$Na reaction impacts the break-out from the hot CNO-cycles to the $rp$-process in type I X-ray bursts. We present a revised thermonuclear reaction rate, which is based on the latest experimental data. The new rate is derived from Monte-Carlo calculations, taking into account the uncertainties of all nuclear physics input quantities. In addition, we present the reaction rate uncertainty and probability density versus temperature. Our results are also consistent with estimates obtained using different indirect approaches.

P. Mohr; R. Longland; C. Iliadis

2014-12-09T23:59:59.000Z

251

Thermonuclear reaction rate of $^{18}$Ne($?$,$p$)$^{21}$Na from Monte-Carlo calculations  

E-Print Network (OSTI)

The $^{18}$Ne($\\alpha$,$p$)$^{21}$Na reaction impacts the break-out from the hot CNO-cycles to the $rp$-process in type I X-ray bursts. We present a revised thermonuclear reaction rate, which is based on the latest experimental data. The new rate is derived from Monte-Carlo calculations, taking into account the uncertainties of all nuclear physics input quantities. In addition, we present the reaction rate uncertainty and probability density versus temperature. Our results are also consistent with estimates obtained using different indirect approaches.

P. Mohr; R. Longland; C. Iliadis

2014-12-14T23:59:59.000Z

252

Thermonuclear reaction rate of $^{18}$Ne($\\alpha$,$p$)$^{21}$Na from Monte-Carlo calculations  

E-Print Network (OSTI)

The $^{18}$Ne($\\alpha$,$p$)$^{21}$Na reaction impacts the break-out from the hot CNO-cycles to the $rp$-process in type I X-ray bursts. We present a revised thermonuclear reaction rate, which is based on the latest experimental data. The new rate is derived from Monte-Carlo calculations, taking into account the uncertainties of all nuclear physics input quantities. In addition, we present the reaction rate uncertainty and probability density versus temperature. Our results are also consistent with estimates obtained using different indirect approaches.

Mohr, P; Iliadis, C

2014-01-01T23:59:59.000Z

253

Observation of quartet-state fine structures and lifetimes in lithiumlike Ne VIII  

Science Journals Connector (OSTI)

Wavelength and lifetime measurements for the fine-structure components of the 1s 2s 2p Po4-1s 2p2 P4 multiplet in lithiumlike Ne VIII have been made using foil excitation of a fast-ion beam. The results are compared with recent theoretical calculations and with previous measurements for other ions of the same isoelectronic squence. An apparent discrepancy between theory and experiment for the 1s 2p2 P324 lifetime is removed.

A. E. Livingston; J. E. Hardis; L. J. Curtis; R. L. Brooks; H. G. Berry

1984-10-01T23:59:59.000Z

254

Excitation of the giant quadrupole resonance in /sup 58/Ni with /sup 20/Ne  

E-Print Network (OSTI)

The heavy-ion induced excitation of the quadrupole resonance in /sup 58/Ni has been studied with /sup 20/Ne beams of 14.5 and 19.6 MeV/N incident energy. The broad resonance structure is clearly observed; the strength exhausts 44% and 60% of the energy weighted sum rule (EWSR) at the two incident energies, respectively. The background is partly explained by a three-body reaction mechanism, which is based on the one-nucleon pick-up reaction into unbound states followed by one- nucleon emission. The remaining part is interpreted as inelastic excitation of other multipoles. (11 refs).

Bohlen, H G; Ingold, G; Lettau, H; Ossenbrink, H; von Oertzen, W

1981-01-01T23:59:59.000Z

255

Impact of the uncertainty in ?-captures on {sup 22}Ne on the weak s-process in massive stars  

SciTech Connect

Massive stars at solar metallicity contribute to the production of heavy elements with atomic masses between A = 60 and A = 90 via the so-called weak s-process (which takes place during core He and shell C burning phases). Furthermore, recent studies have shown that rotation boosts the s-process production in massive stars at low metallicities, with a production that may reach the barium neutron-magic peak. These results are very sensitive to neutron source and neutron poison reaction rates. For the weak s-process, the main neutron source is the reaction {sup 22}Ne(?,n){sup 25}Mg, which is in competition with {sup 22}Ne(?,?){sup 26}Mg. The uncertainty of both rates strongly affects the nucleosynthesis predictions from stellar model calculations. In this study, we investigate the impact of the uncertainty in ?-captures on {sup 22}Ne on the s-process nucleosynthesis in massive stars both at solar and at very low metallicity. For this purpose, we post-process, with the Nugrid mppnp code, non-rotating and rotating evolutionary models 25M{sub ?} stars at two different metallicities: Z = Z{sub ?} and Z = 10{sup ?5}Z{sub ?}, respectively. Our results show that uncertainty of {sup 22}Ne(?,n){sup 25}Mg and {sup 22}Ne(?,?){sup 26}Mg rates have a significant impact on the final elemental production especially for metal poor rotating models. Beside uncertainties in the neutron source reactions, for fast rotating massive stars at low metallicity we revisit the impact of the neutron poisoning effect by the reaction chain {sup 16}O(n,?){sup 17}O(?,?){sup 21}Ne, in competition with the {sup 17}O(?,n){sup 20}Ne, recycling the neutrons captured by {sup 16}O.

Nishimura, N. [Astrophysics group, EPSAM, Keele University, Keele, ST5 1BH, UK and NuGrid Project (United Kingdom); Hirschi, R. [Astrophysics group, EPSAM, Keele University, Keele, ST5 1BH, UK and Kavli IPMU (WPI), University of Tokyo, Kashiwa, 277-8583 (Japan); Pignatari, M. [NuGrid Project and Department of Physics, University of Basel, Basel, CH-4056 (Switzerland); Herwig, F. [NuGrid Project and Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P5C2 (Canada); Beard, M. [NuGrid Project and Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Imbriani, G. [Dipartiment di Scienze Fisiche, Universita di Napoli Federico II, Napoli (Italy); Grres, J.; Boer, R. J. de; Wiescher, M. [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States)

2014-05-02T23:59:59.000Z

256

Measurement of the Atomic Scattering Factor of Ne, Ar, Kr, and Xe  

Science Journals Connector (OSTI)

To test the accuracy of the Hartree-Fock (HF) method and the reliability of x-ray measurements of the atomic scattering factor f, we have determined the scattering of Mo K? radiation by Ne, Ar, Kr, and Xe gases. Values of f were obtained on an absolute basis with an accuracy of about %. Results at small angle yield the mean-square radius of the electron cloud ?r2?av and the dispersion correction. For Ne, Ar, and Kr, the values of ?r2?av are in good agreement with HF calculations. For Xe, the experimental value is significantly lower. Susceptibility results yield about 6% lower values in each case. Our derived values of the dispersion correction are each more negative than those obtained from published absorption coefficients. At higher angles, our f values differ by less than 0.2 electron unit from the HF values for all the gases; even for Xe the approximate HF values presently available are more nearly accurate than the Thomas-Fermi-Dirac (TFD) values. We conclude that a 4% discrepancy between theory and experiment found by Batterman, Chipman, and DeMarco for metal powders arose from solid-state effects or from difficulties in sample preparation.

D. R. Chipman and L. D. Jennings

1963-10-15T23:59:59.000Z

257

Nature of the Configuration-Interaction Method in Ab Initio Calculations. I. Ne Ground State  

Science Journals Connector (OSTI)

A detailed study of the correlation energy of Ne has been made in order to analyze the nature of the configuration-interaction (CI) method in ab initio calculations. Both the Bethe-Goldstone method of Nesbet and the total-pair-excitation-block method (TPEB) were examined. A series of calculations was made using both "atom-centered" and "shell-centered" basis sets. The most detailed calculations gave - 0.333 a.u. (88%) for the correlation energy by the TPEB method, and - 0.396 a.u. (104%) by the sum-of-the-pairs technique. The difference between these two values is mainly the so-called pair-pair interactions, which have been considered too small to be important to other investigators. A series of perturbation calculations on the triple and quadruple excitations gives ? 1.5% of the total correlation energy. A complete CI calculation with a very limited basis set was done on the p block of Ne. The results of this calculation are in agreement with our total-atom calculation, except that now the TPEB calculation gave about 98.5%, and the sum of the pairs about 115% of the complete CI result. The effect on the pair correlation energy of a unitary transformation of the outer-shell occupied self-consistent-field orbitals was also studied. Only a small difference in the results was obtained.

Tery L. Barr and Ernest R. Davidson

1970-03-01T23:59:59.000Z

258

Evaluation of ne pitch p{on{n and n{on{n irradiated silicon microstrip detectors for the LHCb experiment  

E-Print Network (OSTI)

Evaluation of ne pitch p{on{n and n{on{n irradiated silicon microstrip detectors for the LHCb experiment

Libby, J

2001-01-01T23:59:59.000Z

259

Markus Popa, DOE (OCRWM) Bill Sherman, NE HLRW Task Force Robert Holden, NCAI  

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

Minutes Monday, November 3rd 2:00-3:00 p.m. (EST) Minutes Monday, November 3rd 2:00-3:00 p.m. (EST) Participants included: Markus Popa, DOE (OCRWM) Bill Sherman, NE HLRW Task Force Robert Holden, NCAI Mike Butler, UETC Bob Fronczak, AAR Kevin Blackwell, FRA Mike Butler (UETC) greeted participants and informed the group of previous notification by Robert Light (Mescalero Apache Tribe), Robert Centracco (FRA), and Mike Calhoun (FRA) that they would be unable to join the call. Mr. Butler began the call with a brief update on the status of Matrix 1, now entitled "Summary of Rail and Highway Regulations and their Applicability to States, Tribes, Shippers, and Carriers." He informed the group that he had completed an initial draft of the matrix, but that he was making substantial revisions to it and therefore he had not distributed it to the entire group for

260

NE-24 R&D Decontamination Projects Under the Formerly Utilized Sites Remedial  

Office of Legacy Management (LM)

" _ ,' ,:.' : " _ ,' ,:.' : NE-24 R&D Decontamination Projects Under the Formerly Utilized Sites Remedial Action Program (FUSRAP) '. * * ,~~'.'J.' L.aGrone, Manager Oak Ridge Operations O fffce As a result of the House-Senate Conference Report and the Energy and W a ter Appropriations Act for FY 1984, and based on the data in the attached reports indicating radioactive contamination In excess of acceptable guidelines, the sites listed In the attachment and their respectfve vicinity properties (contaminated with radioactive materials from these sites) are being designated as decontamination research and development projects under the FUSRAP. Each site and the associated vicinity properties should be treated as a separate project. . . -_ The objectjve of each project is to decontaminate the vicinity properties

Note: This page contains sample records for the topic "broken bow ne" 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

NE-23 Elimination of the Chupadera Mesa and Los Alamos County Industrial Waste  

Office of Legacy Management (LM)

AM? 2 2 1986 AM? 2 2 1986 NE-23 Elimination of the Chupadera Mesa and Los Alamos County Industrial Waste Line Sites from Further Consideration for FUSRAP Inclusion Carlos E. Garcia, Director Environmental Safety and Health Division Albuquerque Operations Office The enclosed material is being provided to you to document the final actions taken under the Department's Formerly Utilized Sites Remedial Action Program (FUSRAP) for the Chupadera Mesa area and the Los Alamos County Industrial Waste Lines, New Mexico. Copies of designation/ elimination reviews for each of the sites are enclosed for your records. We have determined that neither site warrants inclusion in the remedial action program. Primary sources of data for this determination were two survey reports prepared through your Division, LA-10256-MS, "Radiological

262

Laser Rock Drilling on the History Channel - The NE Multimedia Collection  

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

Departments > System Technologies & Diagnostics > Videos Departments > System Technologies & Diagnostics > Videos Laser Oil & Gas Well Drilling: Laser Rock Drilling on the History Channel Argonne's Laser Applications Lab and researcher Claude Reed (NE) appeared in the History Channel program "Modern Marvels: Drilling" (May 10, 2006). "Modern Marvels" relates the ingenuity, invention and imagination behind everyday items, technological breakthroughs and man-made wonders. :: Please wait until video loads completely :: Argonne Experts Dr. Claude B. Reed is one of the Experts featured in the Argonne Experts Guide. The video is in mp4 format. Closed Captioning Transcript Live Closed captioning of the video is not available; however -as an alternative- we provide a transcript of the audio portion of this video as a separate web page.

263

Ionization of the He, Ne, Ar, Kr, and Xe isoelectronic series by proton impact  

Science Journals Connector (OSTI)

In this paper we report ionization cross sections of positive Li+, Na+, K+, Rb+, neutral He, Ne, Ar, Kr, Xe, and negative F?, Cl?, Br?, I? ions by impact of protons with energies ranging from 25to1000keV. Cross sections of singly charged ions are relevant to the calculation of electron yields in collisions with insulator surfaces. Calculations were performed within the continuum distorted waveeikonal initial state method using an angular expansion in spherical harmonics and a numerical evaluation of the radial functions corresponding to both the initial (bound) and the final (continuum) states. The first Born approximation was used on an equal footing. We find that this first-order theory holds for proton energies larger than 300keV. For comparison, we also calculate the shellwise local plasma approximation. Our results show that it gives a good account of the cross sections for neutral targets.

J. E. Miraglia and M. S. Gravielle

2008-11-06T23:59:59.000Z

264

Distribution of products in the reaction /sup 20/Ne + Al. [118 and 167 MeV  

SciTech Connect

The measurement and preliminary analysis of the distribution of products with Z between 2 and 21 and A between 3 and 43 from 118- and 167-MeV reactions of /sup 20/Ne with Al are reported. Experimental conditions were adequate to allow resolution of individual isotopes over this entire range, and measurements were made at several angles for each bombarding energy. Measured relative cross sections of the heavier products were compared with predictions of a statistical-model evaporation calculation. The overall agreement between experiment and theory was rather good; however, certain discrepancies between calculation and experiment for low Z and A at 167 MeV may be troublesome. 3 figures. (RWR)

Ferguson, R.L.; Gavron, A.I.; Obenshain, F.E.; Plasil, F.; Robinson, R.L.; Shapira, D.; Snell, A.H.; Young, G.R.

1980-01-01T23:59:59.000Z

265

Superdeformed structures and low $?$ parity doublet in Ne$-$S nuclei near neutron drip-line  

E-Print Network (OSTI)

The structure of Ne, Na, Mg, Al, Si, P and S nuclei near the neutron drip-line region is investigated in the frame-work of relativistic mean field theory and non-relativistic Skyrme Hartree-Fock formalism. The recently discovered nuclei $^{40}$Mg and $^{42}$Al, which are beyond the drip-line predicted by various mass formulae are located within these models. We find many largely deformed neutron-rich nuclei, whose structures are analyzed. From the structure anatomy, we find that at large deformation, low $\\Omega$ orbits of opposite parities (e.g. $\\frac{1}{2}^+$ and $\\frac{1}{2}^-$) occur close to each other in energy.

Shailesh K. Singh; S. K. Patra; C. R. Praharaj

2014-01-24T23:59:59.000Z

266

Is w{ne}-1 evidence for a dynamical dark energy equation of state?  

SciTech Connect

Current constraints on the dark energy equation of state parameter, w, are expected to be improved by more than 1 order of magnitude in the next decade. If |w-1| > or approx. 0.01 around the present time, but the dark energy dynamics is sufficiently slow, it is possible that future constraints will rule out a cosmological constant while being consistent with a time-independent equation of state parameter. In this paper, we show that although models with such behavior can be constructed, they do require significant fine-tuning. Therefore, if the observed acceleration of the Universe is induced by a dark energy component, then finding w{ne}-1 would, on its own, constitute very strong evidence for a dynamical dark energy equation of state.

Avelino, P. P. [Centro de Fisica do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal); Departamento de Fisica da Faculdade de Ciencias da Universidade do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal); Trindade, A. M. M. [Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto (Portugal); Viana, P. T. P. [Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto (Portugal); Departamento de Matematica Aplicada da Faculdade de Ciencias da Universidade do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal)

2009-09-15T23:59:59.000Z

267

The Goldstone theorem protects naturalness, and the absence of Brout-Englert-Higgs fine-tuning, in spontaneously broken SO(2)  

E-Print Network (OSTI)

The Gell-Mann-Levy (GML), Schwinger and Standard Models were previously shown to lack a Brout-Englert-Higgs (BEH) fine-tuning problem due to quadratic divergences, with finite Euclidean cut-off \\Lambda, because of the symmetries obeyed by all O(\\Lambda^2) contributions. We extend those results to finite contributions from certain M_{Heavy}^2>> m_{BEH}^2 particles in SO(2) versions of GML and Schwinger. We demonstrate explicit 1-loop physical naturalness for two SO(2) singlet examples: a heavy real scalar S and a right-handed Type 1 see-saw Majorana neutrino. We prove that for low |q^2| the heavy degrees of freedom contribute, at worst, marginal operators in spontaneously broken SO(2) Schwinger. The key GML lesson from these examples is that the pseudo Nambu-Goldstone boson (NGB) mass-squared must be properly renormalized. A true NGB value, m_3^2 = 0, is then protected by the Goldstone theorem. For the Schwinger model, two crucial observations emerge: global Ward-Takahashi identities (WTI) force all relevant operators into the pseudo-NGB mass-squared; and WTI enforce the Goldstone theorem by forbidding all relevant operator contributions in the spontaneously broken Goldstone mode, \\pi_3 is a massless NGB there. Goldstone mode, with weak-scale m_{BEH}^2 \\& ^2, is not-fine-tuned even as a low-energy effective theory with certain high-mass-scale extensions. Its "Goldstone Exceptional Naturalness (GEN)," where all relevant operators vanish, a powerful suppression of fine-tuning, is simply another (albeit un-familiar) consequence of WTI, spontaneous symmetry breaking and the Goldstone theorem. If GEN can somehow be extended to the Standard Model (SM), there should be no expectation that LHC will discover any Beyond the SM physics unrelated to neutrino mixing, i.e. the only known experimentally necessary modification of the Standard Model plus General Relativity paradigm.

Bryan W. Lynn; Glenn D. Starkman

2014-11-11T23:59:59.000Z

268

BP Studentship* in the Department of Earth Sciences of the University of Oxford Tectonic evolution of the Parnaiba cratonic basin, NE Brazil  

E-Print Network (OSTI)

of the Parnaiba cratonic basin, NE Brazil Supervisors: Prof. A. B. Watts and Dr. M. Daly (BP) * Subject to funding structure and petroleum play. The focus will be on the Parnaiba basin in NE Brazil, one of the world in Brazil and the UK, will involve the acquisition of seismic reflection and refraction profile data along

269

Grant Holder Research Organisation Project Title Grant Reference Peter Bernath University of York Satellite Observations of Halogen-Containing Molecules NE/I022663/1  

E-Print Network (OSTI)

, Ice and Super-cooled Water Particles. NE/I023058/1 Gareth Chisham NERC British Antarctic Survey Quantifying the Effect of the Upper Atmospheric Electric Potential on Lower Atmospheric Temperature Orography) NE/I024984/1 Peter Jan van Leeuwen University of Reading Next generation Numerical Weather

270

Detailed microscopic calculation of stellar electron and positron capture rates on $^{24}$Mg for O+Ne+Mg core simulations  

E-Print Network (OSTI)

Few white dwarfs, located in binary systems, may acquire sufficiently high mass accretion rates resulting in the burning of carbon and oxygen under nondegenerate conditions forming a O+Ne+Mg core. These O+Ne+Mg cores are gravitationally less bound than more massive progenitor stars and can release more energy due to the nuclear burning. They are also amongst the probable candidates for low entropy r-process sites. Recent observations of subluminous Type II-P supernovae (e.g., 2005cs, 2003gd, 1999br, 1997D) were able to rekindle the interest in 8 -- 10 M$_{\\odot}$ which develop O+Ne+Mg cores. Microscopic calculations of capture rates on $^{24}$Mg, which may contribute significantly to the collapse of O+Ne+Mg cores, using shell model and proton-neutron quasiparticle random phase approximation (pn-QRPA) theory, were performed earlier and comparisons made. Simulators, however, may require these capture rates on a fine scale. For the first time a detailed microscopic calculation of the electron and positron captur...

Nabi, Jameel-Un

2014-01-01T23:59:59.000Z

271

Four Momentum Transfer Discrepancy in the Charged Current ? plus; Production in the MiniBooNE: Data vs. Theory  

Science Journals Connector (OSTI)

The MiniBooNE experiment has collected what is currently the worlds largest sample of v ? charged current single charged pion (CC1? + ) interactions roughly 46 000 events. The purity of the (CC1? + ) sample is 87% making this the purest event sample observed in the MiniBooNE detector [1]. The average energy of neutrinos producing (CC1? + ) interactions in MiniBooNE is about 1?GeV[2] therefore the study of these events can provide insight into both resonant and coherent pion production processes. In this talk we will discuss the long?standing discrepancy in four?momentum transfer observed between (CC1? + ) data and existing predictions. Several attempts to address this problem will be presented. Specifically the Rein?Sehgal [3 4] model has been extended to include muon mass terms for both resonant [5 6] and coherent [7] production. Using calculations from [8] an updated form for the vector form factor [9] has also been adopted. The results of this improved description of (CC1? + ) production will be compared to the high statistics MiniBooNE (CC1? + ) data and several existing parametrisations of the axial vector form factor [8 9 11].

Jaroslaw A. Nowak; MiniBooNE Collaboration

2009-01-01T23:59:59.000Z

272

Transport Diffusivities of CH4, CF4, He, Ne, Ar, Xe, and SF6 in Silicalite from Atomistic Simulations  

Science Journals Connector (OSTI)

We have used atomistic simulations to examine the adsorption isotherms, self diffusivity, and transport diffusivity of seven light gases, CH4, CF4, He, Ne, Ar, Xe, and SF6, adsorbed as single-components in silicalite at room temperature. By using ...

Anastasios I. Skoulidas; David S. Sholl

2002-04-23T23:59:59.000Z

273

Third harmonic cavity design and RF measurements for the Frascati DA?NE collider  

Science Journals Connector (OSTI)

Third harmonic passive RF cavities have been proposed for installation in both rings of the DA?NE factory collider to improve the Touschek lifetime and to increase the Landau damping. This paper illustrates the design of the harmonic cavities. The main requirements were to obtain a relatively low R/Q factor and a quality factor Q as high as possible to satisfy beam dynamics requirements and to damp all the higher order mode (HOM) to a harmless level in order to avoid multibunch instabilities. A spherical shape of the cavity central body has been chosen as an optimum compromise between a high Q resonator and a low R/Q factor. HOM suppression has been provided by a ferrite ring damper designed for the superconducting cavities of the high energy ring of the KEK-B factory. The design and electromagnetic properties of the resonant modes have been studied with MAFIA and HFSS codes. Cavities have been made of aluminum and the RF measurements have been performed to characterize them. The measurements are in a good agreement with numerical simulations results, demonstrating a satisfactory HOM damping.

David Alesini; Roberto Boni; Alessandro Gallo; Fabio Marcellini; Mikhail Zobov; Mauro Migliorati; Luigi Palumbo

2004-09-07T23:59:59.000Z

274

Geological characterization of a sandstone reservoir in Eastern Kansas: Savonburg NE field, Allen County, Kansas  

SciTech Connect

Production on the Nelson leases of the Savonburg NE oil field in eastern Kansas is from sandstone that is part of the fill of a paleovalley that was eroded after deposition of the Tebo coal but before deposition of the Scammon coal. Sandstone in this interval is called the Chelsea Sandstone; the interval is referred to as the Skinner interval. (That interval is part of the Cabaniss Formation, Cherokee Group, and assigned to the Desmoinesian stage of the Middle Pennsylvanian). In addition to determining the stratigraphic relationships of the reservoir, geological characterization helped to understand the distribution of the most productive areas of the field and led to specific recommendations for abandonment of wells, workovers, well treatments, well conversions from producers to injectors, and drilling of new wells, all with the aim of increasing productivity and decreasing costs for the operator. The reservoir characterization used information routinely gathered in the course of oil field operations in eastern Kansas. Gamma-neutron logs indicated lithology as well as stratigraphy, while core descriptions provided insight into stratigraphic distinctions and depositional processes. Core analysis of porosity, permeability, and fluid saturations permitted depiction of the distribution of such attributes throughout the productive region. Key geological concepts of regional marker intervals and incised valley fills provided the theoretical framework for analyzing the reservoir.

Walton, A.W.; Beaty, D.S.

1995-12-31T23:59:59.000Z

275

Flash pyrolysis of kerogens from algal rich oil shales from the Eocene Huadian Formation, NE China  

Science Journals Connector (OSTI)

Abstract The hydrocarbon composition of the kerogen fractions of two samples (HD-20 and HD-21) from oil shale layer 4 in the Eocene Huadian Formation, NE China were investigated by analytical flash pyrolysis (650C/10s) followed by gas chromatographymass spectrometry (PyGCMS). Organic petrography showed that the two kerogens were almost entirely derived from algal remains but contained very different algal maceral compositions, with 40% of the macerals in HD-20 being of macroalgal origin that were not present in HD-21. PyGCMS yielded high concentrations of n-alkanes from both kerogens, but with different molecular weight profiles due to the different algal contributors to the two kerogen samples. The hydrocarbon pyrolysates generated at 650C from HD-21 in which the green microalga Botryococcus braunii was identified showed a higher proportion of longer chain alkanes and alkenes presumably from cracking of the botryococcus algaenan. We also identified a C40 monoaromatic lycopane derivative, which was absent in the HD-20. The high hydrocarbon potential of both kerogens can be attributed to common microalgal sources, whereas the macroalgae, which is abundant in HD-20, makes only a minor contribution to the hydrocarbon products.

Zhirong Zhang; John K. Volkman; Paul F. Greenwood; Wenxuan Hu; Jianzhong Qin; Tenger Borjigin; Changbo Zhai; Weixin Liu

2014-01-01T23:59:59.000Z

276

Design and Performance of the Soft Gamma-ray Detector for the NeXT mission  

SciTech Connect

The Soft Gamma-ray Detector (SGD) on board the NeXT (Japanese future high energy astrophysics mission) is a Compton telescope with narrow field of view (FOV), which utilizes Compton kinematics to enhance its background rejection capabilities. It is realized as a hybrid semiconductor gamma-ray detector which consists of silicon and CdTe (cadmium telluride) detectors. It can detect photons in a wide energy band (0.05-1 MeV) at a background level of 5 x 10{sup -7} counts/s/cm{sup 2}/keV; the silicon layers are required to improve the performance at a lower energy band (<0.3 MeV). Excellent energy resolution is the key feature of the SGD, allowing it to achieve both high angular resolution and good background rejection capability. An additional capability of the SGD, its ability to measure gamma-ray polarization, opens up a new window to study properties of astronomical objects. We will present the development of key technologies to realize the SGD: high quality CdTe, low noise front-end ASIC and bump bonding technology. Energy resolutions of 1.7 keV (FWHM) for CdTe pixel detectors and 1.1 keV for Si strip detectors have been measured. We also present the validation of Monte Carlo simulation used to evaluate the performance of the SGD.

Tajima, Hiroyasu; Kamae, T.; Madejski, G.; Mitani, T.; Nakazawa, K.; Tanaka, T.; Takahashi, T.; Watanabe, S.; Fukazawa, Y.; Ikagawa, T.; Kataoka, J.; Kokubun, M.; Makishima, K.; Terada, Y.; Nomachi, M.; Tashiro, M.; /SLAC /Sagamihara, Inst. Space Astron. Sci. /Tokyo U. /Hiroshima U. /Tokyo Inst. Tech. /Wako, RIKEN /Osaka U. /Saitama U.

2006-04-19T23:59:59.000Z

277

Lead Grant Reference Lead Grant RO Grant Holder Last Name, First Name Project Title NE/K000071/1 Newcastle University Mr R Gaulton Dual-wavelength laser scanning for forest health  

E-Print Network (OSTI)

Newcastle University Mr R Gaulton Dual-wavelength laser scanning for forest health monitoring. NE/K000381/1Lead Grant Reference Lead Grant RO Grant Holder Last Name, First Name Project Title NE/K000071/1 and sensory mechanisms in bat navigation NE/K000403/1 University of Southampton Dr S Watt Emplacement dynamics

278

Detailed microscopic calculation of stellar electron and positron capture rates on $^{24}$Mg for O+Ne+Mg core simulations  

E-Print Network (OSTI)

Few white dwarfs, located in binary systems, may acquire sufficiently high mass accretion rates resulting in the burning of carbon and oxygen under nondegenerate conditions forming a O+Ne+Mg core. These O+Ne+Mg cores are gravitationally less bound than more massive progenitor stars and can release more energy due to the nuclear burning. They are also amongst the probable candidates for low entropy r-process sites. Recent observations of subluminous Type II-P supernovae (e.g., 2005cs, 2003gd, 1999br, 1997D) were able to rekindle the interest in 8 -- 10 M$_{\\odot}$ which develop O+Ne+Mg cores. Microscopic calculations of capture rates on $^{24}$Mg, which may contribute significantly to the collapse of O+Ne+Mg cores, using shell model and proton-neutron quasiparticle random phase approximation (pn-QRPA) theory, were performed earlier and comparisons made. Simulators, however, may require these capture rates on a fine scale. For the first time a detailed microscopic calculation of the electron and positron capture rates on $^{24}$Mg on an extensive temperature-density scale is presented here. This type of scale is more appropriate for interpolation purposes and of greater utility for simulation codes. The calculations are done using the pn-QRPA theory using a separable interaction. The deformation parameter, believed to be a key parameter in QRPA calculations, is adopted from experimental data to further increase the reliability of the QRPA results. The resulting calculated rates are up to a factor of 14 or more enhanced as compared to shell model rates and may lead to some interesting scenario for core collapse simulators.

Jameel-Un Nabi

2014-08-15T23:59:59.000Z

279

NatioNal academy of ScieNceS of UkraiNe iNStitUte of archaeology  

E-Print Network (OSTI)

NatioNal academy of ScieNceS of UkraiNe iNStitUte of archaeology crimeaN braNch doNetSk NatUral hi devoted to the publication of the materials from Palaeolithic site of Karabai I, Crimea, Ukraine cadre du projet "Funktionale Variabilität im späten Mittelpaläolithikum auf der Halbinsel Krim, Ukraine

Sheldon, Nathan D.

280

Neutrinos in IceCube/KM3NeT as probes of dark matter substructures in galaxy clusters  

Science Journals Connector (OSTI)

Galaxy clusters are one of the most promising candidate sites for dark matter (DM) annihilation. We focus on DM (?) with mass in the range of 10GeV100TeV, annihilating through the channels ????+?-, ?????, ???tt, or ???????, and forecast the expected sensitivity to the annihilation cross section into these channels by observing galaxy clusters at IceCube/KM3NeT. Optimistically, the presence of DM substructures in galaxy clusters is predicted to enhance the signal by 23 orders of magnitude over the contribution from the smooth component of the DM distribution. Optimizing for the angular size of the region of interest for galaxy clusters, the sensitivity to the annihilation cross section, ??v?, of heavy DM with mass in the range of 300GeV100TeV will be O(10-24??cm3?s-1) for full IceCube/KM3NeT live time of 10years, which is about one order of magnitude better than the best limit that can be obtained by observing the MilkyWay halo. We find that neutrinos from cosmic ray interactions in the galaxy cluster, in addition to the atmospheric neutrinos, are a source of background. We show that significant improvement in the experimental sensitivity can be achieved for lower DM masses in the range of 10300GeV if neutrino-induced cascades can be reconstructed to ?5 accuracy, as may be possible in KM3NeT. We, therefore, propose that a low-energy extension KM3NeT-Core, similar to DeepCore in IceCube, be considered for an extended reach at low DM masses.

Basudeb Dasgupta and Ranjan Laha

2012-11-01T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

AR-NE3A, a New Macromolecular Crystallography Beamline for Pharmaceutical Applications at the Photon Factory  

SciTech Connect

Recent advances in high-throughput techniques for macromolecular crystallography have highlighted the importance of structure-based drug design (SBDD), and the demand for synchrotron use by pharmaceutical researchers has increased. Thus, in collaboration with Astellas Pharma Inc., we have constructed a new high-throughput macromolecular crystallography beamline, AR-NE3A, which is dedicated to SBDD. At AR-NE3A, a photon flux up to three times higher than those at existing high-throughput beams at the Photon Factory, AR-NW12A and BL-5A, can be realized at the same sample positions. Installed in the experimental hutch are a high-precision diffractometer, fast-readout, high-gain CCD detector, and sample exchange robot capable of handling more than two hundred cryo-cooled samples stored in a Dewar. To facilitate high-throughput data collection required for pharmaceutical research, fully automated data collection and processing systems have been developed. Thus, sample exchange, centering, data collection, and data processing are automatically carried out based on the user's pre-defined schedule. Although Astellas Pharma Inc. has a priority access to AR-NE3A, the remaining beam time is allocated to general academic and other industrial users.

Yamada, Yusuke; Hiraki, Masahiko; Sasajima, Kumiko; Matsugaki, Naohiro; Igarashi, Noriyuki; Kikuchi, Takashi; Mori, Takeharu; Toyoshima, Akio; Kishimoto, Shunji; Wakatsuki, Soichi [Photon Factory, Institute of Materials Structure Science, High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki, 305-0801 (Japan); Amano, Yasushi; Warizaya, Masaichi; Sakashita, Hitoshi [Drug Discovery Research, Astellas Pharma Inc., 21, Miyukigaoka, Tukuba, Ibaraki, 300-8585 (Japan)

2010-06-23T23:59:59.000Z

282

A measurement of the neutral current neutrino-nucleon elastic cross section at MiniBooNE  

SciTech Connect

The neutral current neutrino-nucleon elastic interaction {nu} N {yields} {nu} N is a fundamental process of the weak interaction ideally suited for characterizing the structure of the nucleon neutral weak current. This process comprises {approx}18% of neutrino events in the neutrino oscillation experiment, MiniBooNE, ranking it as the experiment's third largest process. Using {approx}10% of MiniBooNE's available neutrino data, a sample of these events were identified and analyzed to determine the differential cross section as a function of the momentum transfer of the interaction, Q{sup 2}. This is the first measurement of a differential cross section with MiniBooNE data. From this analysis, a value for the nucleon axial mass M{sub A} was extracted to be 1.34 {+-} 0.25 GeV consistent with previous measurements. The integrated cross section for the Q{sup 2} range 0.189 {yields} 1.13 GeV{sup 2} was calculated to be (8.8 {+-} 0.6(stat) {+-} 0.2(syst)) x 10{sup -40} cm{sup 2}.

Cox, David Christopher; /Indiana U.

2008-02-01T23:59:59.000Z

283

Are oxygen and neon enriched in PNe and is the current solar Ne/O abundance ratio underestimated?  

E-Print Network (OSTI)

A thorough critical literature survey has been carried out for reliable measurements of oxygen and neon abundances of planetary nebulae (PNe) and HII regions. By contrasting the results of PNe and of HII regions, we aim to address the issues of the evolution of oxygen and neon in the interstellar medium (ISM) and in the late evolutionary phases of low- and intermediate-mass stars (LIMS), as well as the currently hotly disputed solar Ne/O abundance ratio. Through the comparisons, we find that neon abundance and Ne/O ratio increase with increasing oxygen abundance in both types of nebulae, with positive correlation coefficients larger than 0.75. The correlations suggest different enrichment mechanisms for oxygen and neon in the ISM, in the sense that the growth of neon is delayed compared to oxygen. The differences of abundances between PNe and HII regions, are mainly attributed to the results of nucleosynthesis and dredge-up processes that occurred in the progenitor stars of PNe. We find that both these alpha-elements are significantly enriched at low metallicity (initial oxygen abundance oxygen in intermediate mass stars (IMS) of low initial metallicities and in more massive stars, a conjecture that requires verification by further theoretical studies. This result also strongly suggests that both the solar neon abundance and the Ne/O ratio should be revised upwards by ~0.22 dex from the Asplund, Grevesse & Sauval values or by ~0.14 dex from the Grevesse & Sauval values.

W. Wang; X. -W. Liu

2008-06-13T23:59:59.000Z

284

Organic matter composition and macrofaunal diversity in sediments of the Condor Seamount (Azores, NE Atlantic)  

Science Journals Connector (OSTI)

Abstract In recent years increasing knowledge has been accumulated on seamounts ecology; however their sedimentary environments and associated biological communities remain largely understudied. In this study we investigated quantity and biochemical composition of organic matter and macrofaunal diversity in sediments of the Condor Seamount (NE Atlantic, Azores). In order to test the effect of the seamount on organic matter distribution, sediment samples were collected in 6 areas: the summit, the northern and southern flanks and bases, and in an external far field site. Macrofauna abundance and diversity were investigated on the summit, the southern flank and in the far field site. The organic matter distribution reflected the complex hydrodynamic conditions occurring on the Condor. Concentrations of organic matter compounds were generally lower on the whole seamount than in the far field site and on the seamount summit compared to flanks and bases. A clear difference was also evident between the northern and southern slopes of the Condor, suggesting a role of the seamount in conditioning sedimentation processes and distribution of food resources for benthic consumers. Macrofauna assemblages changed significantly among the three sampling sites. High abundance and dominance, accompanied by low biodiversity, characterized the macrofauna community on the Condor summit, while low dominance and high biodiversity were observed at the flank. Our results, although limited to five samples on the seamount and two off the seamount, do not necessarily support the paradigm that seamounts are more biodiverse than the surrounding seafloor. However, the abundance (and biomass), functional diversity and taxonomical distinctiveness of the macrofaunal assemblages from the Condor Seamount suggest that seamounts habitats may play a relevant role in adding to the regional biodiversity.

Lucia Bongiorni; Ascenso Ravara; Paola Parretti; Ricardo S. Santos; Clara F. Rodrigues; Teresa Amaro; Marina R. Cunha

2013-01-01T23:59:59.000Z

285

Redshift propagation equations in the {beta}{sup '{ne}}0 Szekeres models  

SciTech Connect

The set of differential equations obeyed by the redshift in the general {beta}{sup '{ne}}0 Szekeres spacetimes is derived. Transversal components of the ray's momentum have to be taken into account, which leads to a set of 3 coupled differential equations. It is shown that in a general Szekeres model, and in a general Lemaitre-Tolman (L-T) model, generic light rays do not have repeatable paths (RLPs): two rays sent from the same source at different times to the same observer pass through different sequences of intermediate matter particles. The only spacetimes in the Szekeres class in which all rays are RLPs are the Friedmann models. Among the proper Szekeres models, RLPs exist only in the axially symmetric subcases, and in each one the RLPs are the null geodesics that intersect each t=constant space on the symmetry axis. In the special models with a 3-dimensional symmetry group (L-T among them), the only RLPs are radial geodesics. This shows that RLPs are very special and in the real Universe should not exist. We present several numerical examples which suggest that the rate of change of positions of objects in the sky, for the studied configuration, is 10{sup -6}-10{sup -7} arc sec per year. With the current accuracy of direction measurement, this drift would become observable after approximately 10 years of monitoring. More precise future observations will be able, in principle, to detect this effect, but there are basic problems with determining the reference direction that does not change.

Krasinski, Andrzej [N. Copernicus Astronomical Centre, Polish Academy of Sciences, Bartycka 18, 00 716 Warszawa (Poland); Bolejko, Krzysztof [Astrophysics Department, University of Oxford, Oxford OX1 3RH (United Kingdom)

2011-04-15T23:59:59.000Z

286

Monte Carlo calculations for reference dosimetry of electron beams with the PTW Roos and NE2571 ion chambers  

SciTech Connect

Purpose: To investigate recommendations for reference dosimetry of electron beams and gradient effects for the NE2571 chamber and to provide beam quality conversion factors using Monte Carlo simulations of the PTW Roos and NE2571 ion chambers. Methods: The EGSnrc code system is used to calculate the absorbed dose-to-water and the dose to the gas in fully modeled ion chambers as a function of depth in water. Electron beams are modeled using realistic accelerator simulations as well as beams modeled as collimated point sources from realistic electron beam spectra or monoenergetic electrons. Beam quality conversion factors are calculated with ratios of the doses to water and to the air in the ion chamber in electron beams and a cobalt-60 reference field. The overall ion chamber correction factor is studied using calculations of water-to-air stopping power ratios. Results: The use of an effective point of measurement shift of 1.55 mm from the front face of the PTW Roos chamber, which places the point of measurement inside the chamber cavity, minimizes the difference betweenR{sub 50}, the beam quality specifier, calculated from chamber simulations compared to that obtained using depth-dose calculations in water. A similar shift minimizes the variation of the overall ion chamber correction factor with depth to the practical range and reduces the root-mean-square deviation of a fit to calculated beam quality conversion factors at the reference depth as a function of R{sub 50}. Similarly, an upstream shift of 0.34 r{sub cav} allows a more accurate determination of R{sub 50} from NE2571 chamber calculations and reduces the variation of the overall ion chamber correction factor with depth. The determination of the gradient correction using a shift of 0.22 r{sub cav} optimizes the root-mean-square deviation of a fit to calculated beam quality conversion factors if all beams investigated are considered. However, if only clinical beams are considered, a good fit to results for beam quality conversion factors is obtained without explicitly correcting for gradient effects. The inadequacy of R{sub 50} to uniquely specify beam quality for the accurate selection of k{sub Q} factors is discussed. Systematic uncertainties in beam quality conversion factors are analyzed for the NE2571 chamber and amount to between 0.4% and 1.2% depending on assumptions used. Conclusions: The calculated beam quality conversion factors for the PTW Roos chamber obtained here are in good agreement with literature data. These results characterize the use of an NE2571 ion chamber for reference dosimetry of electron beams even in low-energy beams.

Muir, B. R., E-mail: bmuir@physics.carleton.ca; Rogers, D. W. O., E-mail: drogers@physics.carleton.ca [Physics Department, Carleton Laboratory for Radiotherapy Physics, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario K1S 5B6 (Canada)] [Physics Department, Carleton Laboratory for Radiotherapy Physics, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario K1S 5B6 (Canada)

2013-12-15T23:59:59.000Z

287

Analysis of reaction cross sections of Ne and Mg isotopes at 240 MeV/u in the Dirac-Brueckner approach and Glauber model  

Science Journals Connector (OSTI)

Within a relativistic effective complex nucleon-nucleon interaction derived by solving the Dirac-Brueckner-Bethe-Goldstone equation, locally, starting from...20-36Ne , 24-38Mg + 12C reactions, recently observed a...

M. Rashdan

2014-09-01T23:59:59.000Z

288

2 | engineering neWs | spring 2010 coluMBia engineering | spring 2010 | 3 his issue of Columbia Engineering magazine focuses on engineering  

E-Print Network (OSTI)

2 | engineering neWs | spring 2010 coluMBia engineering | spring 2010 | 3 T his issue of Columbia as the inventor of the Pupin coil and father of long- distance telephony. His pupil and, later, faculty colleague

Hone, James

289

Measurement of K(+) production cross section by 8 GeV protons using high-energy neutrino interactions in the SciBooNE detector  

E-Print Network (OSTI)

The SciBooNE Collaboration reports K[superscript +] production cross section and rate measurements using high-energy daughter muon neutrino scattering data off the SciBar polystyrene (C[subscript 8]H[subscript 8]) target ...

Bugel, Leonard G.

290

The Broken Symmetry of Time  

SciTech Connect

This paper seeks to clarify features of time asymmetry in terms of symmetry breaking. It is observed that, in general, a contingent situation or event requires the breaking of an underlying symmetry. The distinction between the universal anisotropy of temporal processes and the irreversibility of certain physical processes is clarified. It is also proposed that the Transactional Interpretation of quantum mechanics offers an effective way to explain general thermodynamic asymmetry in terms of the time asymmetry of radiation, where prior such efforts have fallen short.

Kastner, Ruth E. [Department of Philosophy, University of Maryland, College Park, MD 20742 (United States)

2011-11-29T23:59:59.000Z

291

Biomarker evidence for Botryococcus and a methane cycle in the Eocene Huadian oil shale, NE China  

Science Journals Connector (OSTI)

Abstract The saturated and unsaturated hydrocarbons of two samples (HD-19 and HD-21) from the same section of the Middle Eocene lacustrine Huadian oil shale in NE China were identified and shown to be mainly from algal and bacterial sources. Comparison of the two samples provided an opportunity to explore the contribution from telalginite to the hydrocarbon profiles. Cells identified from microscopy as Botryococcus in the telalginite of HD-21 were confirmed as belonging to the L race of B. braunii from the presence of monoaromatic lycopane derivatives and small amounts of several lycopadienes. Lycopane was abundant and was probably derived from biohydrogenation of lycopadienes and related lipids on the basis of ?13C values. Hopane distributions showed a dominance of those with the biological 17?,21?-stereochemistry, as expected for an immature shale, with low amounts of 17?,21?-hopanes (moretanes) and 17?,21?-hopanes. Two hopenes were also abundant and assigned as C29 and C30 neohop-13(18)-enes, which occurred together with the C29 and C30 hop-17(21)-enes. These had depleted carbon isotope values (?43.7 to ?50.8), indicative of production by methane oxidizing bacteria (methanotrophs). The high proportion of hopanoids with carbon numbers

John K. Volkman; Zhirong Zhang; Xiaomin Xie; Jianzhong Qin; Tenger Borjigin

2015-01-01T23:59:59.000Z

292

Investigation of thermonuclear $^{18}$Ne($?$,$p$)$^{21}$Na rate via resonant elastic scattering of $^{21}$Na+$p$  

E-Print Network (OSTI)

The $^{18}$Ne($\\alpha$,$p$)$^{21}$Na reaction is thought to be one of the key breakout reactions from the hot CNO cycles to the rp-process in type I x-ray bursts. In this work, the resonant properties of the compound nucleus $^{22}$Mg have been investigated by measuring the resonant elastic scattering of $^{21}$Na+$p$. An 89 MeV $^{21}$Na radioactive beam delivered from the CNS Radioactive Ion Beam Separator bombarded an 8.8 mg/cm$^2$ thick polyethylene (CH$_{2}$)$_{n}$ target. The $^{21}$Na beam intensity was about 2$\\times$10$^{5}$ pps, with a purity of about 70% on target. The recoiled protons were measured at the center-of-mass scattering angles of $\\theta_{c.m.}$$\\approx$175.2${^\\circ}$, 152.2${^\\circ}$, and 150.5${^\\circ}$ by three sets of $\\Delta E$-$E$ telescopes, respectively. The excitation function was obtained with the thick-target method over energies $E_x$($^{22}$Mg)=5.5--9.2 MeV. In total, 23 states above the proton-threshold in $^{22}$Mg were observed, and their resonant parameters were determined via an $R$-matrix analysis of the excitation functions. We have made several new $J^{\\pi}$ assignments and confirmed some tentative assignments made in previous work. The thermonuclear $^{18}$Ne($\\alpha$,$p$)$^{21}$Na rate has been recalculated based on our recommended spin-parity assignments. The astrophysical impact of our new rate has been investigated through one-zone postprocessing x-ray burst calculations. We find that the $^{18}$Ne($\\alpha$,$p$)$^{21}$Na rate significantly affects the peak nuclear energy generation rate, reaction fluxes, as well as the onset temperature of this breakout reaction in these astrophysical phenomena.

L. Y. Zhang; J. J. He; A. Parikh; S. W. Xu; H. Yamaguchi; D. Kahl; S. Kubono; P. Mohr; J. Hu; P. Ma; S. Z. Chen; Y. Wakabayashi; H. W. Wang; W. D. Tian; R. F. Chen; B. Guo; T. Hashimoto; Y. Togano; S. Hayakawa; T. Teranishi; N. Iwasa; T. Yamada; T. Komatsubara; Y. H. Zhang; X. H. Zhou

2014-03-19T23:59:59.000Z

293

Measurement and ab initio calculation of the Ne photoabsorption spectrum in the region of the K edge  

Science Journals Connector (OSTI)

The Ne photoabsorption spectrum in the region of the K edge has been measured with unprecedented energy resolution. The results have been interpreted by using an ab initio method that predicts natural linewidths, as well as relative intensities and positions of the different 1s?np (3<~n<~6) transitions. The remarkable agreement between theory and experiment improves the spectroscopic characterization of these inner-shell excited states in an energy region where only electron-energy-loss spectroscopies were considered to provide accurate and high-resolution data.

M. Coreno; L. Avaldi; R. Camilloni; K. C. Prince; M. de Simone; J. Karvonen; R. Colle; S. Simonucci

1999-03-01T23:59:59.000Z

294

Quantum dynamics of solid Ne upon photo-excitation of a NO impurity: A Gaussian wave packet approach  

SciTech Connect

A high-dimensional quantum wave packet approach based on Gaussian wave packets in Cartesian coordinates is presented. In this method, the high-dimensional wave packet is expressed as a product of time-dependent complex Gaussian functions, which describe the motion of individual atoms. It is applied to the ultrafast geometrical rearrangement dynamics of NO doped cryogenic Ne matrices after femtosecond laser pulse excitation. The static deformation of the solid due to the impurity as well as the dynamical response after femtosecond excitation are analyzed and compared to reduced dimensionality studies. The advantages and limitations of this method are analyzed in the perspective of future applications to other quantum solids.

Unn-Toc, W.; Meier, C.; Halberstadt, N. [Laboratoire Collisions Agregats et Reactivite, IRSAMC, UMR CNRS 5589, Universite Paul Sabatier, 31062 Toulouse (France); Uranga-Pina, Ll. [Laboratoire Collisions Agregats et Reactivite, IRSAMC, UMR CNRS 5589, Universite Paul Sabatier, 31062 Toulouse (France); Facultad de Fisica, Universidad de la Habana, San Lazaro y L, Vedado, 10400 La Habana (Cuba); Rubayo-Soneira, J. [Instituto Superior de Tecnologias y Ciencias Aplicadas (InSTEC), Ave. Salvador Allende y Luaces, Habana 10600, AP 6163 La Habana (Cuba)

2012-08-07T23:59:59.000Z

295

A Measurement of the muon neutrino charged current quasielastic interaction and a test of Lorentz violation with the MiniBooNE experiment  

SciTech Connect

The Mini-Booster neutrino experiment (MiniBooNE) at Fermi National Accelerator Laboratory (Fermilab) is designed to search for {nu}{sub {mu}} {yields} {nu}{sub e} appearance neutrino oscillations. Muon neutrino charged-current quasi-elastic (CCQE) interactions ({nu}{sub {mu}} + n {yields} {mu} + p) make up roughly 40% of our data sample, and it is used to constrain the background and cross sections for the oscillation analysis. Using high-statistics MiniBooNE CCQE data, the muon-neutrino CCQE cross section is measured. The nuclear model is tuned precisely using the MiniBooNE data. The measured total cross section is {sigma} = (1.058 {+-} 0.003 (stat) {+-} 0.111 (syst)) x 10{sup -38} cm{sup 2} at the MiniBooNE muon neutrino beam energy (700-800 MeV). {nu}{sub e} appearance candidate data is also used to search for Lorentz violation. Lorentz symmetry is one of the most fundamental symmetries in modern physics. Neutrino oscillations offer a new method to test it. We found that the MiniBooNE result is not well-described using Lorentz violation, however further investigation is required for a more conclusive result.

Katori, Teppei; /Indiana U.

2008-12-01T23:59:59.000Z

296

Silver Bow County Secondary Data Analysis  

E-Print Network (OSTI)

Myocardial Infarction prevalence (Heart Attack) 5.3% 4.1% 6.0% All Sites Cancer 416.6 (Region 4) 455. Heart Disease 2. Cancer 3. CLRD* 1. Cancer 2. Heart Disease 3.CLRD* 1. Heart Disease 2. Cancer 3

Maxwell, Bruce D.

297

Origin of the Structures in the C-12(o-16,alpha) Reaction - Dominance of Ne-20-Star and O-16-Star Sequential Alpha-Decay Processes  

E-Print Network (OSTI)

of the ' C(' O,a) Mg reaction with good energy resolution in the bombarding energy range of 60 to 100 MeV. It turned out that peaks observed in the Mg excitation energy E =20?30 MeV did not have the same widths and decay branching ratios that the known... publication, " the movement of the structures in terms of the 2 Mg excita- tion as a function of the incident energy is well explained by sequential a-decay processes from Ne* and/or ' 0' through the narrow resonances at E?( Ne)=8. 8, 12.0, 14.3, 16.5, 20...

Murakami, T.; Ungricht, E.; Takahashi, N.; Lui, YW; Mihara, Y.; Neese, R. E.; Takada, E.; Tanner, D. M.; Tribble, Robert E.; Nagatani, K.

1984-01-01T23:59:59.000Z

298

Towards secondary ion mass spectrometry on the helium ion microscope: An experimental and simulation based feasibility study with He{sup +} and Ne{sup +} bombardment  

SciTech Connect

The combination of the high-brightness He{sup +}/Ne{sup +} atomic level ion source with secondary ion mass spectrometry detection capabilities opens up the prospect of obtaining chemical information with high lateral resolution and high sensitivity on the Zeiss ORION helium ion microscope. The analytical performance in terms of sputtering yield, useful yield, and detection limit is studied and subsequently optimized by oxygen and cesium flooding. Detection limits down to 10{sup -6} and 10{sup -5} can be obtained for silicon using Ne{sup +} and He{sup +}, respectively. A simulation based study reveals furthermore that a lateral resolution <10 nm can be obtained.

Wirtz, T.; Vanhove, N.; Pillatsch, L.; Dowsett, D. [Department of Science and Analysis of Materials (SAM), Centre de Recherche Public - Gabriel Lippmann, 41 rue du Brill, L-4422 Belvaux (Luxembourg); Sijbrandij, S.; Notte, J. [Carl Zeiss NTS LLC, One Corporation Way, Peabody, Massachusetts 01960 (United States)

2012-07-23T23:59:59.000Z

299

REP&V TO ATTNJF: NE-23 SUWECC Commercial Facilities Used by National Lead Company of Ohio in Support  

Office of Legacy Management (LM)

REP&V TO REP&V TO ATTNJF: NE-23 SUWECC Commercial Facilities Used by National Lead Company of Ohio in Support 'of FMPC Operations TO: Robert E. Lynch Procuresnent and CorXracts Division, AD-42 Oak Ridge Operations Office The Division of Facility and Site Decormnissioning Projects (DFSP) is responsible for managing the Department's Formerly Utilized Sites Remedial Action Program (FUSRAP). The purposes of FUSRAP are (1) to identify facilities formerly operated for or by the Manhattan Engineer District (NED) and Atomic Energy Commission (AEC) which may have been radioactively contaminated as a result of these operations, (2) to determine if the facilities require remedial action, and (3) where DOE has authority, to conduct the remedial action. Authority for remedial action under FUSRAP is

300

REP&V TO ATTNOF: NE-23 SUBJECT: Commercial Facilities Used by National Lead Company of Ohio in Support  

Office of Legacy Management (LM)

x:Y" x:Y" . .' 3023 I\ \ 'a' '. Unita? -&&s Coverament , ,Q,.l. ),&, ,(>.. Department of Energy riGmorandum / d6a 2/. $3 DATE: JL(L 2 8 ;;$5 co. /3 .-J/ co,/3 REP&V TO ATTNOF: NE-23 SUBJECT: Commercial Facilities Used by National Lead Company of Ohio in Support of FMPC Operations TO: Robert E. Lynch Procuremnent and Contracts Division, AD-42 Oak Ridge Operations Office The Division of Facility and Site Decommissioning Projects (DFSD) is responsible for managing the Department's Formerly Utilized Sites Remedial Action Program (FuSRAP). The purposes of FUSRAP are (1) to identify facilities formerly operated for or by the Manhattan Engineer District (NED) and Atomic Energy Commission (AEC) which may have been radioactively contaminated as a result of these operations, (2) to determine if the

Note: This page contains sample records for the topic "broken bow ne" 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

35 COFibE, Series A. U. S. ATOXIC ENERGY CCMMISSION r'C Cj NE# YORK OPERATIONS OFFICE  

Office of Legacy Management (LM)

COFibE, Series A. COFibE, Series A. - U. S. ATOXIC ENERGY CCMMISSION r'C Cj NE# YORK OPERATIONS OFFICE HEkLTH AND SAFETY DIVISION (Merril Eicsnbud, Dirsator) MONTHLY REPORT OF FIELD ACTIVITIES (This report%v,rs%~~~nth period) Indusorial Ii~iene Branoh m a . . 0 . . c . . . o W. B. Harris, Chief Radiation Branch . y y e 0e . e . e . . . . e . . . Hanson Blatz, Chief Fi:e and Accident Branch D e a o o . . . ..s . . B. J. Kehoe, Chief Medical Advioer, Dr. J. A. Quiglsy Siometrician, Dr. A. E. Brandt TABLF OF COEpTmS PRODUCTION COWTRACTORS ._ Feed Nabrlals Production Centor '$iiddlcsexSampling Plnnt Harshaw ChuoicalCompa~ Wlin&rodt Chen!icrl Works tie. Ontario Storage Area b Vit*o Mnufacturing CompaW B4ikhem Steel F'lrnt - IpcknuMnr Clifton Roducts CompvIy Drush Bcx@.Uun~ Company - Luckcy

302

Proposal to search for a dark photon in $e^+$ on target collisions at DA$?$NE linac  

E-Print Network (OSTI)

Photon-like particles are predicted in many extensions of the Standard Model. They have interactions similar to the photon, are vector bosons, and can be produced together with photons. The present paper proposes a search for such particles in the $ e^+e^- \\to U\\gamma$ process in a positron-on-target experiment, exploiting the positron beam of the DA$\\Phi$NE linac at the Laboratori Nazionali di Frascati, INFN. In one year of running a sensitivity in the relative interaction strength down to $\\sim10^{-6}$ is achievable, in the mass region from 2.5 MeV$

Mauro Raggi; Venelin Kozhuharov

2014-03-12T23:59:59.000Z

303

Effects of CP Violation from Neutral Heavy Fermions on Neutrino Oscillations, and the LSND/MiniBooNE Anomalies  

E-Print Network (OSTI)

Neutrinos may mix with ultralight fermions, which gives flavor oscillations, and with heavier fermions, which yields short distance flavor change. I consider the case where both effects are present. I show that in the limit where a single oscillation length is experimentally accessible, the effects of heavier fermions on neutrino oscillations can generically be accounted for by a simple formula containing four parameters, including observable CP violation. I consider the anomalous LSND and MiniBooNE results, and show that these can be fit in a model with CP violation and two additional sterile neutrinos, one in the mass range between 0.1 and 20 eV, and the other with mass between 33 eV and 40 GeV. I also show that this model can avoid conflict with constraints from existing null short baseline experimental results.

Ann E Nelson

2010-10-19T23:59:59.000Z

304

Using the X-FEL to photo-pump X-ray laser transitions in He-like Ne  

SciTech Connect

Nearly four decades ago H-like and He-like resonantly photo-pumped laser schemes were proposed for producing X-ray lasers. However, demonstrating these schemes in the laboratory has proved to be elusive because of the difficulty of finding a strong resonant pump line. With the advent of the X-ray free electron laser (X-FEL) at the SLAC Linac Coherent Light Source (LCLS) we now have a tunable X-ray laser source that can be used to replace the pump line in previously proposed laser schemes and allow researchers to study the physics and feasibility of resonantly photo-pumped laser schemes. In this paper we use the X-FEL at 1174 eV to photo-pump the singly excited 1s2p state of He-like Ne to the doubly excited 2p3p state and model gain on the 2p3p-2p2s transition at 175 eV and the 2p3p-1s3p transition at 1017 eV. One motivation for studying this scheme is to explore possible quenching of the gain due to strong non-linear coupling effects from the intense X-FEL beam We compare this scheme with photo-pumping the He-like Ne ground state to the 1s3p singly excited state followed by lasing on the 3p-2s and 3d-2p transitions at 158 and 151 eV. Experiments are being planned at LCLS to study these laser processes and coherent quantum effects.

Nilsen, J; Rohringer, N

2011-08-30T23:59:59.000Z

305

SciBooNE/MiniBooNE  

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

Scintillator tracking detector (15 tons) Neutrino target * Electron Catcher (EC) * Muon Range Detector (MRD) Physics goals: Precise measurements of and cross...

306

Grant Reference Grant Holder Research Organisation Project Title NE/I015299/1 Robert Upstill-Goddard Newcastle University Surfactant control of air-sea gas exchange in coastal waters  

E-Print Network (OSTI)

Grant Reference Grant Holder Research Organisation Project Title NE/I015299/1 Robert Upstill of Holocene Monsoon intensity from Central Asia NE/I016414/1 Michael James Lancaster University Quantifying's University of Belfast 14C as a tool to trace terrestrial carbon in a complex lake: implications for food

307

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

308

Proceedings of CELLmicrocosmos neXt 2014 (DOI: 10.2390/biecoll-next2014-2) 7 Towards a 3D Cell Model of Chlamydomonas reinhardtii  

E-Print Network (OSTI)

Proceedings of CELLmicrocosmos neXt 2014 (DOI: 10.2390/biecoll-next2014-2) 7 Towards a 3D Cell Photonics Group, Bielefeld University Universitätsstr. 25, 33615 Bielefeld, Germany 1 Introduction is the production of biofuels. 2 Cell Modeling A visualization approach of the interpretative abstraction level

Moeller, Ralf

309

Event Excess in the MiniBooNE Search for {nu}{sub {mu}{yields}{nu}e} Oscillations  

SciTech Connect

The MiniBooNE experiment at Fermilab reports results from a search for {nu}{sub {mu}{yields}{nu}e} oscillations, using a data sample corresponding to 5.66x10{sup 20} protons on target. An excess of 20.9{+-}14.0 events is observed in the energy range 475

Aguilar-Arevalo, A. A. [Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, D.F. 04510 (Mexico); Anderson, C. E.; Fleming, B. T.; Linden, S. K.; Spitz, J. [Yale University, New Haven, Connecticut 06520 (United States); Brice, S. J.; Brown, B. C.; Ford, R.; Garcia, F. G.; Kobilarcik, T.; Marsh, W.; Moore, C. D.; Polly, C. C.; Russell, A. D.; Stefanski, R. J.; Zeller, G. P. [Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (United States); Bugel, L.; Conrad, J. M.; Karagiorgi, G.; Nguyen, V. [Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)

2010-10-29T23:59:59.000Z

310

Study of Dissipative Collisions of $^{20}$Ne ($\\sim$7-11 MeV/nucleon) + $^{27}$Al  

E-Print Network (OSTI)

The inclusive energy distributions of complex fragments (3 $\\leq$Z $\\leq$ 9) emitted in the reactions $^{20}$Ne (145, 158, 200, 218 MeV) + $^{27}$Al have been measured in the angular range 10$^{o}$ - 50$^{o}$. The fusion-fission and the deep-inelastic components of the fragment yield have been extracted using multiple Gaussian functions from the experimental fragment energy spectra. The elemental yields of the fusion-fission component have been found to be fairly well exlained in the framework of standard statistical model. It is found that there is strong competition between the fusion-fission and the deep-inelastic processes at these energies. The time scale of the deep-inelastic process was estimated to be typically in the range of $\\sim$ 10$^{-21}$ - 10$^{-22}$ sec., and it was found to decrease with increasing fragment mass. The angular momentum dissipations in fully energy damped deep-inelastic process have been estimated from the average energies of the deep-inelastic components of the fragment energy spectra. It has been found that, the estimated angular momentum dissipations, for lighter fragments in particular, are more than those predicted by the empirical sticking limit.

Aparajita Dey; C. Bhattacharya; S. Bhattacharya; T. K. Rana; S. Kundu; K. Banerjee; S. Mukhopadhyay; S. R. Banerjee; D. Gupta; R. Saha

2006-08-22T23:59:59.000Z

311

Explosions of O-Ne-Mg Cores, the Crab Supernova, and Subluminous Type II-P Supernovae  

E-Print Network (OSTI)

We present results of simulations of stellar collapse and explosions in spherical symmetry for progenitor stars in the 8-10 solar mass range with an O-Ne-Mg core. The simulations were continued until nearly one second after core bounce and were performed with the Prometheus/Vertex code with a variable Eddington factor solver for the neutrino transport, including a state-of-the-art treatment of neutrino-matter interactions. Particular effort was made to implement nuclear burning and electron capture rates with sufficient accuracy to ensure a smooth continuation, without transients, from the progenitor evolution to core collapse. Using two different nuclear equations of state (EoSs), a soft version of the Lattimer & Swesty EoS and the significantly stiffer Wolff & Hillebrandt EoS, we found no prompt explosions, but instead delayed explosions, powered by neutrino heating and the neutrino-driven baryonic wind which sets in about 200 ms after bounce. The models eject little nickel ( 0.46, which suggests a chemical composition that is not in conflict with galactic abundances. No low-entropy matter with Ye << 0.5 is ejected. This excludes such explosions as sites of a low-entropy r-process. The low explosion energy and nucleosynthetic implications are compatible with the observed properties of the Crab supernova, and the small nickel mass supports the possibility that our models explain some subluminous Type II-P supernovae.

F. S. Kitaura; H. -Th. Janka; W. Hillebrandt

2005-12-02T23:59:59.000Z

312

Investigation of thermonuclear $^{18}$Ne($\\alpha$,$p$)$^{21}$Na rate via resonant elastic scattering of $^{21}$Na+$p$  

E-Print Network (OSTI)

The $^{18}$Ne($\\alpha$,$p$)$^{21}$Na reaction is thought to be one of the key breakout reactions from the hot CNO cycles to the rp-process in type I x-ray bursts. In this work, the resonant properties of the compound nucleus $^{22}$Mg have been investigated by measuring the resonant elastic scattering of $^{21}$Na+$p$. An 89 MeV $^{21}$Na radioactive beam delivered from the CNS Radioactive Ion Beam Separator bombarded an 8.8 mg/cm$^2$ thick polyethylene (CH$_{2}$)$_{n}$ target. The $^{21}$Na beam intensity was about 2$\\times$10$^{5}$ pps, with a purity of about 70% on target. The recoiled protons were measured at the center-of-mass scattering angles of $\\theta_{c.m.}$$\\approx$175.2${^\\circ}$, 152.2${^\\circ}$, and 150.5${^\\circ}$ by three sets of $\\Delta E$-$E$ telescopes, respectively. The excitation function was obtained with the thick-target method over energies $E_x$($^{22}$Mg)=5.5--9.2 MeV. In total, 23 states above the proton-threshold in $^{22}$Mg were observed, and their resonant parameters were determ...

Zhang, L Y; Parikh, A; Xu, S W; Yamaguchi, H; Kahl, D; Kubono, S; Mohr, P; Hu, J; Ma, P; Chen, S Z; Wakabayashi, Y; Wang, H W; Tian, W D; Chen, R F; Guo, B; Hashimoto, T; Togano, Y; Hayakawa, S; Teranishi, T; Iwasa, N; Yamada, T; Komatsubara, T; Zhang, Y H; Zhou, X H

2014-01-01T23:59:59.000Z

313

Efficient Implementation of MPI-2 Pas s iv e O ne-S id ed C ommu nication on InfiniB and  

E-Print Network (OSTI)

Efficient Implementation of MPI- 2 Pas s iv e O ne- S id ed C ommu nication on InfiniB and C lu # # $ a ( ) % % $ a a# $ a i n a $ + id d ' ( ini ia $ a i n , u$ $ # % i' % # # uni a i n $ a n u% d i-sided communications ... Access Epoch Origin Target window #12;n ini n . $ n indu ( anda d P + id ig

Panda, Dhabaleswar K.

314

Troisi`eme serie d'exercices Ne pas utiliser le theor`eme d'adequation pour faire ces exercices.  

E-Print Network (OSTI)

MAT 3060 Troisi`eme s´erie d'exercices Ne pas utiliser le th´eor`eme d'ad´equation pour faire ces bf A et B, alors les formules suivantes sont des th´eor`emes de L : (a) (A ((A))) ; (b) ((B A) ((A) (B)) (((A) B) A)) et L (((A) (B)) (B A)). En d´eduire que tout th´eor`eme de L est un th´eor

Rousseau, Christiane

315

Measurement of K+ production cross section by 8 GeV protons using high energy neutrino interactions in the SciBooNE detector  

SciTech Connect

The SciBooNE Collaboration reports K+ production cross section and rate measurements using high energy daughter muon neutrino scattering data off the SciBar polystyrene (C8H8) target in the SciBooNE detector. The K+ mesons are produced by 8 GeV protons striking a beryllium target in Fermilab Booster Neutrino Beam line (BNB). Using observed neutrino and antineutrino events in SciBooNE, we measure d2?/dpd? = (5.34 0.76) mb/(GeV/c x sr) for p + Be =K+ + X at mean K+ energy of 3.9 GeV and angle (with respect to the proton beam direction) of 3.7 degrees, corresponding to the selected K+ sample. Compared to Monte Carlo predictions using previous higher energy K+ production measurements, this measurement, which uses the NUANCE neutrino interaction generator, is consistent with a normalization factor of 0.85 0.12. This agreement is evidence that the extrapolation of the higher energy K+ measurements to an 8 GeV beam energy using Feynman scaling is valid. This measurement reduces the error on the K+ production cross section from 40% to 14%.

Cheng, G [Columbia U.; Mariani, C [Columbia U.; Alcaraz-Aunion, J L [Barcelona, IFAE; Brice, S J [Fermilab; Bugel, L [MIT; Catala-Perez, J [Valencia U.; Conrad, J M [MIT; Djurcic, Z [Columbia U.; Dore, U [Banca di Roma; INFN, Rome; Finley, D A [Fermilab; Franke, A J [Columbia U.; Banca di Roma; INFN, Rome

2011-07-28T23:59:59.000Z

316

Description of $?$-cluster tail in $^{8}$Be and $^{20}$Ne: Delocalization of $?$ cluster because of quantum penetration  

E-Print Network (OSTI)

We analyze the $\\alpha$-cluster wave functions in cluster states of $^8$Be and $^{20}$Ne by comparing the exact relative wave function obtained by the generator coordinate method (GCM) with various types of trial functions. For the trial functions, we adopt the fixed range shifted Gaussian of the Brink-Bloch (BB) wave function, the spherical Gaussian with the adjustable range parameter of the spherical Thosaki-Horiuchi-Schuck-R\\"opke (sTHSR), the deformed Gaussian of the deformed THSR (dTHSR), and a function with the Yukawa tail (YT). The quality of the description of the exact wave function with a trial function is judged by the squared overlap between the trial function and the GCM wave function. The better result is obtained with the sTHSR wave function than the BB wave function, and further improvement can be done with the dTHSR wave function because these wave functions can describe the outer tail better. The YT wave function gives almost the equal quality to or even better quality than the dTHSR wave function indicating that the outer tail of $\\alpha$ cluster states is characterized by the Yukawa-like tail rather than the Gaussian tail. In the weakly bound $\\alpha$ cluster states with the small $\\alpha$ separation energy and the low centrifugal and Coulomb barriers, the outer tail part is the slowly damping function described well by the quantum penetration through the effective barrier. This outer tail characterizes the almost zero-energy free $\\alpha$ gas behavior, i.e., the delocalization of cluster.

Yoshiko Kanada-En'yo

2014-07-11T23:59:59.000Z

317

Fragmentation of N14, O16, Ne20, and Mg24 nuclei at 290 to 1000 MeV/nucleon  

Science Journals Connector (OSTI)

We report fragmentation cross sections measured at 0 for beams of N14, O16, Ne20, and Mg24 ions, at energies ranging from 290 MeV/nucleon to 1000 MeV/nucleon. Beams were incident on targets of C, CH2, Al, Cu, Sn, and Pb, with the C and CH2 target data used to obtain hydrogen-target cross sections. Using methods established in earlier work, cross sections obtained with both large-acceptance and small-acceptance detectors are extracted from the data and, when necessary, corrected for acceptance effects. The large-acceptance data yield cross sections for fragments with charges approximately half of the beam charge and above, with minimal corrections. Cross sections for lighter fragments are obtained from small-acceptance spectra, with more significant, model-dependent corrections that account for the fragment angular distributions. Results for both charge-changing and fragment production cross sections are compared to the predictions of the Los Alamos version of the quark gluon string model (LAQGSM) as well as the NASA Nuclear Fragmentation (NUCFRG2) model and the Particle and Heavy Ion Transport System (PHITS) model. For all beams and targets, cross sections for fragments as light as He are compared to the models. Estimates of multiplicity-weighted helium production cross sections are obtained from the data and compared to PHITS and LAQGSM predictions. Summary statistics show that the level of agreement between data and predictions is slightly better for PHITS than for either NUCFRG2 or LAQGSM.

C. Zeitlin; J. Miller; S. Guetersloh; L. Heilbronn; A. Fukumura; Y. Iwata; T. Murakami; S. Blattnig; R. Norman; S. Mashnik

2011-03-24T23:59:59.000Z

318

NE Press Releases  

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

press-releases 1000 Independence Ave. SWWashington DC press-releases 1000 Independence Ave. SWWashington DC 20585202-586-5000 en Energy Department Announces New Investment in Innovative Small Modular Reactor http://energy.gov/articles/energy-department-announces-new-investment-innovative-small-modular-reactor Energy Department Announces New Investment in Innovative Small Modular Reactor

319

Interconnect Issues in NE  

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

Presentation covers interconnect issues in the Northeast and is given at the Spring 2010 Federal Utility Partnership Working Group (FUPWG) meeting in Providence, Rhode Island.

320

MicroBooNE  

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

we spearheaded the effort to resolve the fallen 25 m absorber plate problem caused by hydrogen embrittlement of high grade steel chains, and helped develop a new hanging...

Note: This page contains sample records for the topic "broken bow ne" 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

NE Press Releases  

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

field-type-text-with-summary field-label-hidden">

Energy Department Awards 5 Million to Support...

322

Low Energy Fission of {sup 256}No, {sup 270}Sg, {sup 271}Hs and {sup 286}112 Nuclei Formed in Reactions with {sup 22}Ne and {sup 48}Ca Ions  

SciTech Connect

The fusion-fission reactions {sup 22}Ne + {sup 248}Cm and {sup 22}Ne + {sup 249}Cf were investigated at projectile energies equal to 102 and 127 MeV. Mass-energy distributions and yields are shown. Two-dimensional plots of TKE vs fragment mass are also shown for {sup 48}Ca reactions at 230 MeV with {sup 208}Pb and {sup 238}U, leading to {sup 256}No and {sup 286}112.

Itkis, M.G.; Kondratiev, N.A.; Kozulin, E.M.; Krupa, L.; Oganessian, Yu. Ts.; Pokrovsky, I.V.; Prokhorova, E.V.; Rusanov, A. Ya.

1999-12-31T23:59:59.000Z

323

Table 2 -Lime use and practices on Corn, major producing states, 2001 CO GA IL IN IA KS KY MI MN MO NE NY NC ND OH PA SD TX WI Area  

E-Print Network (OSTI)

Table 2 - Lime use and practices on Corn, major producing states, 2001 CO GA IL IN IA KS KY MI MN.7 Table 2 - Lime use and practices on Corn, major producing states, 2000 CO IL IN IA KS KY MI MN MO NE NY use and practices on Corn, major producing states, 1999 CO IL IN IA KS KY MI MN MO NE NC OH SD TX WI

Kammen, Daniel M.

324

A survey of Existing V&V, UQ and M&S Data and Knowledge Bases in Support of the Nuclear Energy - Knowledge base for Advanced Modeling and Simulation (NE-KAMS)  

SciTech Connect

The Nuclear Energy - Knowledge base for Advanced Modeling and Simulation (NE-KAMS) is being developed at the Idaho National Laboratory in conjunction with Bettis Laboratory, Sandia National Laboratories, Argonne National Laboratory, Oak Ridge National Laboratory, Utah State University and others. The objective of this consortium is to establish a comprehensive knowledge base to provide Verification and Validation (V&V) and Uncertainty Quantification (UQ) and other resources for advanced modeling and simulation (M&S) in nuclear reactor design and analysis. NE-KAMS will become a valuable resource for the nuclear industry, the national laboratories, the U.S. NRC and the public to help ensure the safe operation of existing and future nuclear reactors. A survey and evaluation of the state-of-the-art of existing V&V and M&S databases, including the Department of Energy and commercial databases, has been performed to ensure that the NE-KAMS effort will not be duplicating existing resources and capabilities and to assess the scope of the effort required to develop and implement NE-KAMS. The survey and evaluation have indeed highlighted the unique set of value-added functionality and services that NE-KAMS will provide to its users. Additionally, the survey has helped develop a better understanding of the architecture and functionality of these data and knowledge bases that can be used to leverage the development of NE-KAMS.

Hyung Lee; Rich Johnson, Ph.D.; Kimberlyn C. Moussesau

2011-12-01T23:59:59.000Z

325

Orientation of tectonic stresses in central Kentucky during U. Devonian/L. Mississippian times: Evidence from quartz veins (after gypsum) in NE-trending, systematic joints in shales  

SciTech Connect

Quartz replacing fibrous gypsum and anhydrite pseudomorphically (QAS; quartz after sulfate''), and preserving characteristic crack-seal'' and chickenwire'' textures, occurs in extensional veins at four locations in central KY. The veins occupy a systematic set of NE-SW-trending, vertical joints within the essentially flat-lying shales of the Renfro Member of the Mississippian Borden Formation and the Late Devonian New Albany Shale. The four QAS occurrences discovered to date are located northeast of the Borden Front. At one site in the New Albany Shale, QAS veins show clear evidence of penecontemporaneous deformation. It is proposed that at all QAS locations, gypsum precipitated in incipient joints before complete lithification of the sediment, and grew perpendicular to the fractures to form extensional veins in the soft but firm muds. The orientations of the joints now marked by QAS veins are broadly consistent with regional patterns of NE-SW-trending systematic joints and lineaments in southern IN and in central and eastern KY. These systematic fracture patterns do not correspond directly to known basement faults or rift systems, although they are consistent with modern stress directions in eastern and western KY, measured in situ in wells and by earthquake fault-plane solutions. It is proposed that this systematic trend marks the regional tectonic stress pattern characteristic of southern IN and central and eastern KY at, and since the Late Devonian. The evidence of penecontemporaneous sedimentary deformation in joints of U. Devonian age, marked and preserved by quartz replacement of early gypsum, is sufficient to show that while the systematic NE-trending joint set in KY may also be modern it is not uniquely so.

Grover, J.; Dupuis-Nouille, E.M. (Univ. of Cincinnati, Cincinnati, OH (United States). Dept. of Geology)

1992-01-01T23:59:59.000Z

326

Sub-meV accuracy in first-principles computations of the ionization potentials and electron affinities of the atoms H to Ne  

SciTech Connect

Recent advances in coupled-cluster methods for the treatment of electron correlation in atoms (and molecules) have now made possible the computation of the ionization potentials and electron affinities of the atoms H through Ne with a mean absolute deviation of 0.35 meV with respect to experimental data. In this article, coupled-cluster wave functions are parametrized using orbital and Slater-type geminal basis functions. Many-body electron interactions are accounted for through connected quintuple excitations, and relativistic effects (spin-orbit as well as scalar) and diagonal Born-Oppenheimer corrections are included.

Klopper, Wim; Bachorz, Rafal A.; Tew, David P.; Haettig, Christof [Center for Functional Nanostructures (CFN) and Institute of Physical Chemistry, Karlsruhe Institute of Technology, KIT Campus South, Kaiserstrasse 12, D-76131 Karlsruhe (Germany); School of Chemistry, University of Bristol, Bristol BS8 1TS (United Kingdom); Lehrstuhl fuer Theoretische Chemie, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)

2010-02-15T23:59:59.000Z

327

Measurement of the half-life of the T=$\\frac{1}{2}$ mirror decay of $^{19}$Ne and its implication on physics beyond the standard model  

E-Print Network (OSTI)

The $\\frac{1}{2}^+ \\rightarrow \\frac{1}{2}^+$ superallowed mixed mirror decay of $^{19}$Ne to $^{19}$F is excellently suited for high precision studies of the weak interaction. However, there is some disagreement on the value of the half-life. In a new measurement we have determined this quantity to be $T_{1/2}$ = $17.2832 \\pm 0.0051_{(stat)}$ $\\pm 0.0066_{(sys)}$ s, which differs from the previous world average by 3 standard deviations. The impact of this measurement on limits for physics beyond the standard model such as the presence of tensor currents is discussed.

L. J. Broussard; H. O. Back; M. S. Boswell; A. S. Crowell; P. Dendooven; G. S. Giri; C. R. Howell; M. F. Kidd; K. Jungmann; W. L. Kruithof; A. Mol; C. J. G. Onderwater; R. W. Pattie Jr.; P. D. Shidling; M. Sohani; D. J. van der Hoek; A. Rogachevskiy; E. Traykov; O. O. Versolato; L. Willmann; H. W. Wilschut; A. R. Young

2014-05-28T23:59:59.000Z

328

Experimental measurements of the O15(alpha,gamma)Ne19 reaction rate and the stability of thermonuclear burning on accreting neutron stars  

E-Print Network (OSTI)

Neutron stars in close binary star systems often accrete matter from their companion stars. Thermonuclear ignition of the accreted material in the atmosphere of the neutron star leads to a thermonuclear explosion which is observed as an X-ray burst occurring periodically between hours and days depending on the accretion rate. The ignition conditions are characterized by a sensitive interplay between the accretion rate of the fuel supply and its depletion rate by nuclear burning in the hot CNO cycle and the rp-process. For accretion rates close to stable burning the burst ignition therefore depends critically on the hot CNO breakout reaction, O15(alpha,gamma)Ne19, that regulates the flow between the hot CNO cycle and the rapid proton capture process. Until recently, the O15(alpha,gamma)Ne19-reaction rate was not known experimentally and the theoretical estimates carried significant uncertainties. In this paper we perform a parameter study of the uncertainty of this reaction rate and determine the astrophysical consequences of the first measurement of this reaction rate. Our results corroborate earlier predictions and show that theoretically burning remains unstable up to accretion rates near the Eddington limit, in contrast to astronomical observations.

Jacob Lund Fisker; Wanpeng Tan; Joachim Goerres; Michael Wiescher; Randall L. Cooper

2007-05-07T23:59:59.000Z

329

How Do You Mend a Broken Heart?  

E-Print Network (OSTI)

so similar to a standard heart attack that the patient willEKG and conclude its a heart attack. Even at the Emergencygoing to treat you for a heart attack, Wittstein says. "It

Service, Shannon

2011-01-01T23:59:59.000Z

330

How Do You Mend a Broken Heart?  

E-Print Network (OSTI)

so similar to a standard heart attack that the patient willEKG and conclude its a heart attack. Even at the Emergencygoing to treat you for a heart attack, Wittstein says. "It

Service, Shannon

2012-01-01T23:59:59.000Z

331

Research Needs for Magnetic Fusion Energy Sciences. Report of the Research Needs Workshop (ReNeW) Bethesda, Maryland, June 8-12, 2009  

SciTech Connect

Nuclear fusion - the process that powers the sun - offers an environmentally benign, intrinsically safe energy source with an abundant supply of low-cost fuel. It is the focus of an international research program, including the ITE R fusion collaboration, which involves seven parties representing half the world's population. The realization of fusion power would change the economics and ecology of energy production as profoundly as petroleum exploitation did two centuries ago. The 21st century finds fusion research in a transformed landscape. The worldwide fusion community broadly agrees that the science has advanced to the point where an aggressive action plan, aimed at the remaining barriers to practical fusion energy, is warranted. At the same time, and largely because of its scientific advance, the program faces new challenges; above all it is challenged to demonstrate the timeliness of its promised benefits. In response to this changed landscape, the Office of Fusion Energy Sciences (OFES ) in the US Department of Energy commissioned a number of community-based studies of the key scientific and technical foci of magnetic fusion research. The Research Needs Workshop (ReNeW) for Magnetic Fusion Energy Sciences is a capstone to these studies. In the context of magnetic fusion energy, ReNeW surveyed the issues identified in previous studies, and used them as a starting point to define and characterize the research activities that the advance of fusion as a practical energy source will require. Thus, ReNeW's task was to identify (1) the scientific and technological research frontiers of the fusion program, and, especially, (2) a set of activities that will most effectively advance those frontiers. (Note that ReNeW was not charged with developing a strategic plan or timeline for the implementation of fusion power.) This Report presents a portfolio of research activities for US research in magnetic fusion for the next two decades. It is intended to provide a strategic framework for realizing practical fusion energy. The portfolio is the product of ten months of fusion-community study and discussion, culminating in a Workshop held in Bethesda, Maryland, from June 8 to June 12, 2009. The Workshop involved some 200 scientists from Universities, National Laboratories and private industry, including several scientists from outside the US. Largely following the Basic Research Needs model established by the Office of Basic Energy Sciences (BES ), the Report presents a collection of discrete research activities, here called 'thrusts.' Each thrust is based on an explicitly identified question, or coherent set of questions, on the frontier of fusion science. It presents a strategy to find the needed answers, combining the necessary intellectual and hardware tools, experimental facilities, and computational resources into an integrated, focused program. The thrusts should be viewed as building blocks for a fusion program plan whose overall structure will be developed by OFES , using whatever additional community input it requests. Part I of the Report reviews the issues identified in previous fusion-community studies, which systematically identified the key research issues and described them in considerable detail. It then considers in some detail the scientific and technical means that can be used to address these is sues. It ends by showing how these various research requirements are organized into a set of eighteen thrusts. Part II presents a detailed and self-contained discussion of each thrust, including the goals, required facilities and tools for each. This Executive Summary focuses on a survey of the ReNeW thrusts. The following brief review of fusion science is intended to provide context for that survey. A more detailed discussion of fusion science can be found in an Appendix to this Summary, entitled 'A Fusion Primer.'

None

2009-06-08T23:59:59.000Z

332

Data:1dfbc558-81fb-450f-b6c2-ef422f4bb34c | Open Energy Information  

Open Energy Info (EERE)

dfbc558-81fb-450f-b6c2-ef422f4bb34c dfbc558-81fb-450f-b6c2-ef422f4bb34c 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 Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: Choctaw Electric Coop Inc Effective date: 2012/10/21 End date if known: Rate name: Broken Bow Public Works Authority Sector: Commercial Description: * Avialable to the Broken Bow Public Works Authority for use or resale. Electric service shall be billed to and paid by Broken Bow Public Works Authority. Subject to all taxes, but not limited to gross receipts taxes. Source or reference: Rate binder # 4 Source Parent: Comments Applicability Demand (kW) Minimum (kW): Maximum (kW): History (months):

333

Dynamic screening x-ray energy shifts and collisional line broadening of 2p-1s transitions in 2 MeV/AMU H- and He-like Ne, Mg, and S ions traveling in solids  

E-Print Network (OSTI)

University in partial fulfillment of the requirements for the degree of BASTER OF SCIENCE December 1983 Na)or Sub)ect: Chemistry DYNAMIC SCREENING X-RAY ENERGY SHIFTS AND COLLISIONAL LINE BROADENING OF 2p-1s TRANSITIONS IN 2 Mev/AMU H- AND HE-LIKE NE...) December 1983 ABSTRACT Dynamic Screening X-Ray Energy Shifts and Collisional Line Broadening of 2p-1s Transitions in 2 Mev/AMU H- and He-like Ne, Mg, and S Tons Traveling in Solids (December 1983) Richard Jay Maurer, B. S. College of Charleston...

Maurer, Richard Jay

2012-06-07T23:59:59.000Z

334

REP&" TO A~NOF: NE-23 SUBJECT: Commercial Facilities Used by National Lead Company of Ohio iin Support  

Office of Legacy Management (LM)

tifr'itG!'l' &i&s Coverament tifr'itG!'l' &i&s Coverament --_ , ,&,.i +.&r, ,' ,T.L ' Department of Energy / REP&" TO A~NOF: NE-23 SUBJECT: Commercial Facilities Used by National Lead Company of Ohio iin Support of FMPC Operations TO: Robert E. Lynch Procuremnent and Contracts Division, AD-42 Oak Ridge Operations Office , / I I The Division of Facility and Site Oecomnissioning Projects (OF%) is responsible for managing the Department's Formerly Utilized Sites Remedial Action Program (FUSRAP). The purposes of FUSRAP are (1) to identify facilities formerly operated for or by the Manhattan Engineer District (WED) and Atomic Energy Commission (AEC) which may have been'radioactively contaminated as a result of these operations, (5) to determine if the

335

Clouds, Aerosols and Precipitation in the Marine Boundary Layer (CAP-MBL) AMF Deployment Graciosa Island, Azores, NE Atlantic Ocean May 2009-December 2010  

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

the Marine Boundary Layer (CAP-MBL) Graciosa Island, Azores, NE Atlantic Ocean May 2009-December 2010 Rob Wood, University of Washington CAP-MBL Proposal Team AMF Deployment Team Thanks to Mark Miller: AMF Site Scientist Kim Nitschke: AMF Site Manager Importance of Low-Clouds for Climate Imperative that we understand the processes controlling the formation, maintenance and dissipation of low clouds in order to improve their representation in climate models. Which clouds matter for climate sensitivity? Climate Feedbacks Model Intercomparison Project (CFMIP) 12 slab ocean models 2xCO 2 - control Correlation of global mean CRF with local values Mark Webb, Hadley Center 90 N 45 N 0 45 S 90S 0 90 E 180 90 W 0

336

Idaho National Laboratory Ten-year Site Plan (2012 through 2021) -- DOE-NE's National Nuclear Capability -- Developing and Maintaining the INL Infrastructure  

SciTech Connect

To meet long-term objectives to transform the Idaho National Laboratory (INL), we are providing an integrated, long-term vision of infrastructure requirements that support research, development and demonstration (RD&D) goals outlined in the DOE strategic plans, including the NE Roadmap and reports such as Facilities for the Future of Nuclear Energy Research: A Twenty-year Outlook. The goal of the INL Ten-year Site Plan (TYSP) is to clearly link RD&D mission goals and INL core capabilities with infrastructure requirements (single and multi-program), establish the 10-year end-state vision for INL complexes, identify and prioritize infrastructure and capability gaps, as well as the most efficient and economic approaches to closing those gaps.

Cal Ozaki

2010-06-01T23:59:59.000Z

337

PRESENTATION TITLE  

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

STRONG STRONG ® Projects Impacting Federal Power Tulsa District Dan Brueggenjohann 9 June 2010 BUILDING STRONG ® 303(d) Listing of Broken Bow Tailwaters Impairment Impaired Use Cadmium Fish and Wildlife Propagation - Trout Fishery Lead Fish and Wildlife Propagation - Trout Fishery Water Temperature* Fish and Wildlife Propagation - Trout Fishery The 303(d) List reports on waters identified as impaired. These waters: Have elevated portions of one or more pollutants. Do not meet one or more water quality standards. Portions of the Mountain Fork River below Broken Bow Dam are on the 2010 draft Oklahoma 303(d) list. * ODWC is currently working to implement a selective withdrawal

338

C O N TA C T > Lee Ann Ciarlette | 630.252.4835 | leeann@anl.gov | Nuclear Engineering Division | students.ne.anl.gov Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439 November 2012  

E-Print Network (OSTI)

C O N TA C T > Lee Ann Ciarlette | 630.252.4835 | leeann@anl.gov | Nuclear Engineering Division | students.ne.anl.gov Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439 November 2012 The Nuclear Engineering Division has hosted students from: Aalto University (Finland) · Auburn University

Kemner, Ken

339

Grant Reference Principal Investigator Research Organisation Project Title NE/J013544/1 Professor B Hubbard Aberystwyth University Extended-range optical televiewer imaging of the NEEM deep ice borehole, Greenland  

E-Print Network (OSTI)

Grant Reference Principal Investigator Research Organisation Project Title NE/J013544/1 Professor B Hubbard Aberystwyth University Extended-range optical televiewer imaging of the NEEM deep ice borehole/1 Dr A Bedford Edge Hill University Late Holocene temperature reconstruction from Hawes Water northwest

340

Broken hearts and the heart broken: living with, and dying from, heart failure in Scotland  

E-Print Network (OSTI)

Heart failure is a common and serious chronic condition, which can be as malignant as most forms of cancer (Stewart, MacIntyre, Hole, Capewell, & McMurray, 2001). Recent estimates are that around 40,000 men and 45,000 ...

Pratt, Rebekah Janet

2012-11-30T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

Longitudinal beam dynamics in the Frascati DA?NE e+e- collider with a passive third harmonic cavity in the lengthening regime  

Science Journals Connector (OSTI)

A high-harmonic rf system is going to be installed in both rings of the DA?NE ?-Factory collider to improve the Touschek lifetime. The main goal of this paper is to study the impact of the 3rd harmonic cavity on beam dynamics making a special emphasis on the dynamics of a bunch train with a gap. The shift of the coherent synchrotron frequencies of the coupled-bunch modes has been estimated. In the following we investigated the effect of magnification of the synchrotron phase spread and beam spectrum variation due to the gap. Besides we simulated the bunch lengthening for different bunches along the unevenly filled train and evaluated the Touschek lifetime enhancement taking into account the obtained bunch distributions. Finally, the cavity parking option is discussed. It can be considered as a reliable backup procedure consisting of tuning the cavity away from the 3rd harmonic frequency and in between two revolution harmonics. It allows recovering, approximately, the same operating conditions as were before the harmonic cavity installation.

David Alesini; Alessandro Gallo; Susanna Guiducci; Fabio Marcellini; Mikhail Zobov; Mauro Migliorati; Luigi Palumbo

2003-07-08T23:59:59.000Z

342

Plankton blooms, ocean circulation and the European slope current: Response to weather and climate in the Bay of Biscay and W English Channel (NE Atlantic)  

Science Journals Connector (OSTI)

Abstract The flow of upper-layer surface water and circulation for the Bay of Biscay, continental slope and in the wider region of the NE Atlantic is presented, as well as the seasonality of flow and internal tides. The marine plankton environments of Biscay Ocean, Biscay Eddies, Biscay Slope and Biscay Shelf are defined. The Shelf region (Armorican and Celtic) is further divided into Stratified Shelf, Frontal and Tidally Mixed. Seasonal distributions of chlorophyll a are given for all environment from in situ measurements and remote sensing data. Mixing and stabilisation of surface water in the euphotic layer for the start of the spring bloom using in situ profiling measurements is examined. Some regional responses for the slope current, dinoflagellate blooms and interannual variations in spring diatom numbers with respect to weather and climate in the Bay of Biscay and around the British Isles are suggested and discussed. An example of the Eastern European Ocean Margin continental slope response to winter weather (sea level atmospheric pressure forcing) resulting in warm winter water in the southern Bay of Biscay (Navidad, with eddy production) and off the Shetland continental slopes (the warm-water supply route to the Arctic) is given from the slope climate observation series.

Robin D. Pingree; Carlos Garcia-Soto

2014-01-01T23:59:59.000Z

343

Properties of resonant states in 18Ne relevant to key 14O(alpha,p)17F breakout reaction in type I x-ray bursts  

E-Print Network (OSTI)

The $^{14}$O($\\alpha$,$p$)$^{17}$F reaction is one of the key reactions involved in the breakout from the hot-CNO cycle to the rp-process in type I x-ray bursts. The resonant properties in the compound nucleus $^{18}$Ne have been investigated through resonant elastic scattering of $^{17}$F+$p$. The radioactive $^{17}$F beam was separated by the CNS Radioactive Ion Beam separator (CRIB) and bombarded a thick H$_2$ gas target at 3.6 MeV/nucleon. The recoiling light particles were measured by using three ${\\Delta}$E-E silicon telescopes at laboratory angles of $\\theta$$_{lab}$$\\approx$3$^\\circ$, 10$^\\circ$ and 18$^\\circ$, respectively. Five resonances at $E_{x}$=6.15, 6.28, 6.35, 6.85, and 7.05 MeV were observed in the excitation functions. Based on an $R$-matrix analysis, $J^{\\pi}$=1$^-$ was firmly assigned to the 6.15-MeV state. This state dominates the thermonuclear $^{14}$O($\\alpha$,$p$)$^{17}$F rate below 1 GK. We have also confirmed the existence and spin-parities of three states between 6.1 and 6.4 MeV. A...

Hu, J; Parikh, A; Xu, S W; Yamaguchi, H; Kahl, D; Ma, P; Su, J; Wang, H W; Nakao, T; Wakabayashi, Y; Teranishi, T; Hahn, K I; Moon, J Y; Sung, H S; Hashimoto, T; Chen, A A; Irvine, D; Lee, C S; Kubono, S

2014-01-01T23:59:59.000Z

344

Silver Bow County, Montana: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

804293°, -112.5843056° 804293°, -112.5843056° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":45.8804293,"lon":-112.5843056,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

345

Bow Mar, Colorado: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Colorado: Energy Resources Colorado: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 39.628321°, -105.0499841° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.628321,"lon":-105.0499841,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

346

Radio emission from the bow shock of G2  

Science Journals Connector (OSTI)

......E-mail: crumleyp@physics.utexas.edu -(PC...utexas.edu -(PK) 1 Physics Department, University...when the forward shock passes pericentre, possibly...with a high mass-loss rate as suggested by Scoville...passage. black hole physics|radiation mechanisms......

P. Crumley; P. Kumar

2013-01-01T23:59:59.000Z

347

Plasmonic eigenmodes in individual and bow-tie graphene nanotriangles  

E-Print Network (OSTI)

Serving as a new two-dimensional plasmonic material, graphene has stimulated an intensive study of its optical properties which benefit from the unique electronic band structure of the underlying honeycomb lattice of carbon atoms. In classical electrodynamics, nanostructured graphene is commonly modeled by the computationally demanding problem of a three-dimensional conducting film of atomic-scale thickness. Here, we propose an efficient alternative two-dimensional electrostatic approach where all the calculation procedures are restricted to the plane of the graphene sheet. To explore possible quantum effects, we perform tight-binding calculations, adopting a random-phase approximation. We investigate the multiple plasmon modes in triangles of graphene, treating the optical response classically as well as quantum mechanically in the case of both armchair and zigzag edge termination of the underlying atomic lattice. Compared to the classical plasmonic spectrum which is "blind" to the edge termination, we find ...

Wang, Weihua; Jauho, Antti-Pekka; Thygesen, Kristian S; Wubs, Martijn; Mortensen, N Asger

2014-01-01T23:59:59.000Z

348

The Heliospheres Interstellar Interaction: No Bow Shock  

Science Journals Connector (OSTI)

...solves magnetohydrodynamics (MHD) equations...We also performed kinetic/MHD simulations for the...heliosphere. Fig. 4 Schematic diagram of the current best understanding...position by three-dimensional MHD simulations . Astrophys...

D. J. McComas; D. Alexashov; M. Bzowski; H. Fahr; J. Heerikhuisen; V. Izmodenov; M. A. Lee; E. Mbius; N. Pogorelov; N. A. Schwadron; G. P. Zank

2012-06-08T23:59:59.000Z

349

Using Directionality in Mobile Routing Bow-Nan Cheng  

E-Print Network (OSTI)

) the need for line ofsight (LOS) and (ii) reduced transmission quality in adverse weather conditions. Yuksel Institute bownan@gmail.com Murat Yuksel CSE Department University of Nevada - Reno yuksem

Yuksel, Murat

350

Using Directionality in Mobile Routing Bow-Nan Cheng  

E-Print Network (OSTI)

Institute chengb@rpi.edu Murat Yuksel CSE Department University of Nevada - Reno yuksem compared to RF but suffers from (i) the need for line of sight (LOS) alignment and (ii) reduced transmission quality in adverse weather conditions. Yuksel et al. [13] proposed several ways to mitigate

Kalyanaraman, Shivkumar

351

Some conclusive considerations on the comparison of the ICARUS nu_mu to nu_e oscillation search with the MiniBooNE low-energy event excess  

E-Print Network (OSTI)

A sensitive search for anomalous LSND-like nu_mu to nu_e oscillations has been performed by the ICARUS Collaboration exposing the T600 LAr-TPC to the CERN to Gran Sasso (CNGS) neutrino beam. The result is compatible with the absence of additional anomalous contributions giving a limit to oscillation probability of 3.4E-3 and 7.6E-3 at 90% and 99% confidence levels respectively showing a tension between these new limits and the low-energy event excess (200 energy excess has been performed, including the energy resolution as obtained from the official MiniBooNE data release. As a result the previously reported tension is confirmed at 90% C.L., suggesting an unexplained nature or an otherwise instrumental effect for the MiniBooNE low energy event excess

Antonello, M; Benetti, P; Boffelli, F; Bubak, A; Calligarich, E; Centro, S; Cesana, A; Cieslik, K; Cline, D B; Cocco, A G; Dabrowska, A; Dermenev, A; Falcone, A; Farnese, C; Fava, A; Ferrari, A; Gibin, D; Gninenko, S; Guglielmi, A; Haranczyk, M; Holeczek, J; Kirsanov, M; Kisiel, J; Kochanek, I; Lagoda, J; Mania, S; Menegolli, A; Meng, G; Montanari, C; Otwinowski, S; Picchi, P; Pietropaolo, F; Plonski, P; Rappoldi, A; Raselli, G L; Rossella, M; Rubbia, C; Sala, P; Scaramelli, A; Sergiampietri, F; Stefan, D; Sulej, R; Szarska, M; Terrani, M; Torti, M; Varanini, F; Ventura, S; Vignoli, C; Wang, H; Yang, X; Zalewska, A; Zani, A; Zaremba, K

2015-01-01T23:59:59.000Z

352

B) Le rle de l'ocan et des aquifres La proximit de l'ocan Atlantique est telle qu'on ne peut occulter l'hypothse de sa  

E-Print Network (OSTI)

travers l'halite contenue dans la formation limono-argileuse du soubassement (cf. fig. 22). Mais quelle contiennent pas d'halite et d'autre part, le soubassement limono-argileux ne peut être d'origine éolienne vu, le gypse suit le même schéma que l'halite, c'est à dire qu'il est exclusivement contenu dans le

Paris-Sud XI, Université de

353

BANCROFTIANA NE W S L E T T E R O F T H E FR I E N D S O F T H E BA N C R O F T LI B R A RY  

E-Print Network (OSTI)

BANCROFTIANA NE W S L E T T E R O F T H E FR I E N D S O F T H E BA N C R O F T LI B R A RY N U M B-1836. In the role of offi- cial artist, Lewis had accompanied Tho- mas L. McKenney, Superintendent of the Bureau the portraits when he returned to Detroit. Learning that McKenney planned to publish a "Portrait Gallery

California at Berkeley, University of

354

Energy for the future with Ris from nuclear power to sustainable energy Ris NatioNal laboRatoRy foR sustaiNable eNeRgy  

E-Print Network (OSTI)

Energy for the future ­ with Risø from nuclear power to sustainable energy Risø NatioNal laboRatoRy foR sustaiNable eNeRgy edited by MoRteN JastRup #12;Energy for the future #12;Energy for the future ­ with Risø from nuclear power to sustainable energy Translated from 'Energi til fremtiden ­ med Risø fra

355

Research/Evaluate Restoration of NE Oregon Streams: Effects of Livestock Exclosures (Corridor Fencing) on Riparian Vegetation, Stream Geomorphic Features and Fish Populations; Final Report 2002.  

SciTech Connect

The Pacific Northwest Electric Power Planning and Conservation Act of 1980 indicated ''The council shall properly develop and adopt a program to protect, mitigate, and enhance fish and wildlife, including related spawning grounds and habitat on the Columbia River and its tributaries.'' As a result, the Bonneville Power Administration (BPA) has spent millions of dollars on various instream projects throughout the Columbia Basin with the goal of increasing system-wide production of anadromous fisheries through a combination of habitat restoration and enhancement measures. For two decades, numerous BPA-funded projects have been initiated in the upper Columbia River Basin for the express intent of improving the aquatic habitats of anadromous salmonids. Largely missing from most of these projects has been any rigorous evaluation of project success or failure. Some field reviews of some habitat projects have been undertaken (e.g., Beschta et al. 1991, Kauffman et al. 1993) and provide an overview of major problems and opportunities associated with selected projects. However, there continues to be a lack of quantifiable information, collected in a systematic manner that could be used as the basis for scientifically assessing the effects of individual projects on riparian/aquatic habitats, functions, or processes. Recent publications (e.g., NRC 1992, ISG 1996, NRC 1996, Beschta 1997, and Kauffman et al. 1997) have identified and summarized important concepts associated with the restoration and improvement of aquatic ecosystems. While such conceptual approaches provide an important structure for those undertaking restoration efforts, there remains a paucity of basic information throughout the upper Columbia Basin on the hydrologic, geomorphic, and biologic responses that occur from various enhancement approaches. Basic data on the spatial and temporal responses of restoration approaches would provide: (1) a better understanding of project effects upon aquatic habitats and associated riparian functions; (2) a means of determining rates of aquatic habitat improvement; and (3) a basis for projecting future trends of habitat recovery. The proposed research is intended to provide an improved understanding of both the effects and effectiveness of a commonly used habitat enhancement approach in the upper Columbia River Basin. This is the exclusion of domestic livestock from streamside communities and streams via corridor fencing (exclosures). This final report is broken into three separate chapters. The first chapter covers the vegetation change associated with livestock exclusion. The second chapter focuses on the physical geomorphic changes to the streambank and channel. The final chapter covers the response of salmonids and warmwater fishes to livestock exclusion at the spatial scales of exclosures as is commonly constructed today. It is expected that this study will provide an important scientific basis, currently lacking, for understanding the ecological principles of restoration/enhancement of sustainable aquatic habitats for salmonids. Thus, the results of this work are likely to have important ramifications for habitat improvement projects within and beyond the general geographic region of northeastern Oregon.

Kauffman, J. Boone

2002-09-17T23:59:59.000Z

356

HOTSPUR: gamma ray emission from spheres pulsed with D-T neutrons. I. Calibration of improved NE213 detector assembly. II. Comparison of TART/SANDYL electron recoil spectra to experiment; preliminary results  

SciTech Connect

The NE213 scintillator detector was modified so that the pulse height would be linear with electron energy over the full range of interest - up to 7.1 MeV. Absolute calibration was done with four different calibrated gamma sources. An average correction factor is obtained which normalizes SANDYL calculations with respect to the calibration experiments. The procedure for calculating neutron-induced gamma-ray output and electron recoil spectra is described, and experimental data from a number of spherical assemblies are given and compared to TART/SANDYL calculations. (LEW)

Goldberg, E.; Hansen, L.F.; Komoto, T.T.; Pohl, B.A.

1986-09-01T23:59:59.000Z

357

Some characteristics of waves broken by a longshore bar  

E-Print Network (OSTI)

V &t Cv. 2+. 1 ynz, , P C' ';, ', -VQ ;, Lli1 . . / 2. &7 . ;ec 'T n C fQ i "RC "9 . Cg C'"C ': / Sc'. C o ") "jwc~" y"v IQ o 3 c. ) , ! z, 29 sac V r. r q t / u L ?, rc:. " o";. ". t 'nav~ n 0 3? ! 1 P. '~n i-, = ~ / 3... V &t Cv. 2+. 1 ynz, , P C' ';, ', -VQ ;, Lli1 . . / 2. &7 . ;ec 'T n C fQ i "RC "9 . Cg C'"C ': / Sc'. C o ") "jwc~" y"v IQ o 3 c. ) , ! z, 29 sac V r. r q t / u L ?, rc:. " o";. ". t 'nav~ n 0 3? ! 1 P. '~n i-, = ~ / 3...

McNair, Ernest Clark

2012-06-07T23:59:59.000Z

358

Broken promises: solvency issues for defined benefit superannuation funds  

Science Journals Connector (OSTI)

......Benefit Superannuation Plans. Media release 21...Time Bomb. Business Review Weekly, 17 April...evidenced by an actuarial review in relation to a...arising from the plan trust deed or employment...commit- ments of the plan.73 To illustrate...expectations and relevant regulatory requirements......

Shauna Ferris

2006-01-01T23:59:59.000Z

359

BROKEN BOTTLENECKS AND THE FUTURE OF MOLECULAR QUANTUM MECHANICS  

Science Journals Connector (OSTI)

...quantitative success of the theory was attained, perhaps...well-known paper on the theory of the chemical bond...the rules of valence theory and the exceptions to...intermediates; toward a basic under- standing of activated...O. Lowdin, Ark. Fysik, 3, 147 (1951...

R. S. Mulliken; C. C. J. Roothaan

1959-01-01T23:59:59.000Z

360

A Broken Gauge Approach to Gravitational Mass and Charge  

E-Print Network (OSTI)

We argue that a spontaneous breakdown of local Weyl invariance offers a mechanism in which gravitational interactions contribute to the generation of particle masses and their electric charge. The theory is formulated in terms of a spacetime geometry whose natural connection has both dynamic torsion and non-metricity. Its structure illuminates the role of dynamic scales used to determine measurable aspects of particle interactions and it predicts an additional neutral vector boson with electroweak properties.

T. Dereli; R. W. Tucker

2001-12-14T23:59:59.000Z

Note: This page contains sample records for the topic "broken bow ne" 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

Solving the broken link problem in Walden's Paths  

E-Print Network (OSTI)

keeping track of all the documents that link to the page and notifying them with the page?s new location at migration time. The main drawback of the abovementioned methods 1http://www.ietf.com/html.charters/urn-charter.html 12 is that even... the lookup and returns the location of the page. Shafer, et al., [1996] describe PURL (Persistent Uniform Resource Locators). PURLs are designed to replace URLs except that they point to an intermediate lookup service instead of the page...

Dalal, Zubin Jamshed

2004-09-30T23:59:59.000Z

362

Born Broken: Fonts and Information Loss in Legacy Digital Documents  

E-Print Network (OSTI)

introduced improved APIs in Windows XP (moving from GDIto GDI+) and Windows 7 (with the development ofalgorithm implemented in GDI+ may be overridden within an

Brown, Geoffrey; Woods, Kam

2009-01-01T23:59:59.000Z

363

Ground Broken for New Job-Creating Accelerator Research Facility...  

Office of Environmental Management (EM)

our nation in the areas of sustainable energy, a cleaner environment, economic security, health care and national defense. The accelerators of tomorrow have the potential to make...

364

Original article Impact of broken cells of lactococci or propionibacteria  

E-Print Network (OSTI)

suspension (CBS), or cell-free extract (CFE), obtained after centrifugation, were added to UF-St Paulin was effectively provedusingimmunodetectionof lactococci cytoplasmic proteins.The additionof lactococci CBS or CFE increased free amino acid content (1.5 to 3 times) whereas propionibacteria CBS or CFE exhibited

Boyer, Edmond

365

Fluorescence microscopy with diffraction resolution barrier broken by stimulated emission  

Science Journals Connector (OSTI)

...intracavity frequency doubler. This system partly converted the Ti:Sapphire...the focused time-averaged power. The axial...processing. Computational image restoration can in addition improve...light. 1 Pawley J ( 1995 ) Handbook of Biological Confocal Microscopy...

Thomas A. Klar; Stefan Jakobs; Marcus Dyba; Alexander Egner; Stefan W. Hell

2000-01-01T23:59:59.000Z

366

SIMS zircon UPb and molybdenite ReOs geochronology, Hf isotope, and whole-rock geochemistry of the Wunugetushan porphyry CuMo deposit and granitoids in NE China and their geological significance  

Science Journals Connector (OSTI)

Abstract The geodynamic setting of magmatic rocks and geodynamic mechanism of CuMoFeSnPbZnAg polymetallic mineralization in northeastern (NE) China are attracting increasing attention. This study explores these issues by providing SIMS zircon UPb dating, whole-rock geochemical, Hf isotopic data of magmatic rocks, and molybdenite ReOs dating exposed in the Wunugetushan porphyry CuMo deposit, NE China. This deposit is located in the western part of the Great Xing'an Range, on the southeastern margin of the MongolOkhotsk Orogenic Belt. Molybdenite ReOs and SIMS zircon UPb dating of the host monzogranitic porphyry and the wall rock of biotite granite in the Wunugetushan porphyry CuMo deposit indicate that the ore-formation, host porphyry, and wall rock-emplacement occurred at 180.52.0Ma, 180.41.4Ma, and 203.51.6Ma, respectively, and the mineralization of the Wunugetushan porphyry CuMo deposit occurred during the same period as that of the host monzogranitic porphyry. Geochemically, the Wunugetushan granitoids are characterized by strong LREE/HREE fractionation, and pronounced negative Nb, Ta, and Ti anomalies, with slightly negative Eu anomalies (Eu/Eu*=0.710.97) of the host monzogranitic porphyry and pronounced negative Eu anomalies (Eu/Eu*=0.290.32) of the wall rock of biotite granite. In situ Hf isotopic analyses of zircons from the host monzogranitic porphyry and the wall rock of biotite granite yielded ?Hf(t) values ranging from 0.5 to 8.2, and from ?6.9 to 5.9, respectively. The geochemical and isotopic data for the Wunugetushan granitoids imply that the primary magmas of the host monzogranitic porphyry could have originated by partial melting of a thickened lower crust, with input of mantle components, while the primary magmas of the wall rock of biotite granite could have been derived by partial melting of a thickened lower crust that mixed with ancient crustal materials. Based on the regional geological history, geochemistry of the Wunugetushan granitoids, and new isotopic age data, we suggest that the formation of the Wunugetushan porphyry CuMo deposit was possibly induced in the Early Jurassic during the period of the southeastward subduction of the MongolOkhotsk oceanic plate beneath the Erguna Massif.

Yinhong Wang; Chunbo Zhao; Fangfang Zhang; Jiajun Liu; Jianping Wang; Runmin Peng; Bin Liu

2014-01-01T23:59:59.000Z

367

MODELS FOR METAL-POOR STARS WITH ENHANCED ABUNDANCES OF C, N, O, Ne, Na, Mg, Si, S, Ca, AND Ti, IN TURN, AT CONSTANT HELIUM AND IRON ABUNDANCES  

SciTech Connect

Recent work has shown that most globular clusters have at least two chemically distinct components, as well as cluster-to-cluster differences in the mean [O/Fe], [Mg/Fe], and [Si/Fe] ratios at similar [Fe/H] values. In order to investigate the implications of variations in the abundances of these and other metals for H-R diagrams and predicted ages, grids of evolutionary sequences have been computed for scaled solar and enhanced {alpha}-element metal abundances, and for mixtures in which the assumed [m/Fe] value for each of the metals C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti has been increased, in turn, by 0.4 dex at constant [Fe/H]. These tracks, together with isochrones for ages from Almost-Equal-To 5 to 14 Gyr, have been computed for -3.0 {<=} [Fe/H] {<=}-0.6, with helium abundances Y = 0.25, 0.29, and 0.33 at each [Fe/H] value, using upgraded versions of the Victoria stellar structure program and the Regina interpolation code, respectively. Turnoff luminosity versus age relations from isochrones are found to depend almost entirely on the importance of the CNO cycle, and thereby mainly on the abundance of oxygen. Since C, N, and O, as well as Ne and S, do not contribute significantly to the opacities at low temperatures and densities, variations in their abundances do not impact the predicted T{sub eff} scale of red giants. The latter is a strong function of the abundances of only Mg and Si (and Fe, possibly to a lesser extent) because they are so abundant and because they are strong sources of opacity at low temperatures. For these reasons, Mg and Si also have important effects on the temperatures of main-sequence stars. Due to their low abundances, Na, Ca, and Ti are of little consequence for stellar models. The effects of varying the adopted solar metals mixture and the helium abundance at a fixed [Fe/H] are also briefly discussed.

VandenBerg, Don A.; Dotter, Aaron [Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, B.C. V8W 3P6 (Canada); Bergbusch, Peter A. [Department of Physics, University of Regina, Regina, Saskatchewan S4S 0A2 (Canada); Ferguson, Jason W. [Department of Physics, Wichita State University, Wichita, KS 67260-0032 (United States); Michaud, Georges; Richer, Jacques [Departement de Physique, Universite de Montreal, Montreal, Quebec H3C 3J7 (Canada); Proffitt, Charles R., E-mail: vandenbe@uvic.ca, E-mail: Aaron.Dotter@gmail.com, E-mail: pbergbusch@accesscomm.ca, E-mail: proffitt@stsci.edu, E-mail: Jason.Ferguson@wichita.edu, E-mail: michaudg@astro.umontreal.ca, E-mail: jacques.richer@umontreal.ca [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)

2012-08-10T23:59:59.000Z

368

Microsoft PowerPoint - SW Fed Hydro Conference Jun 12 presentation Final [Compatibility Mode]  

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

Projects Projects Impacting Federal Projects Impacting Federal Power Tulsa District Tulsa District Beau Biffle Beau Biffle 13 June 2012 BUILDING STRONG ® Topics Topics  Interior Least Tern Operations and Habitat Creation  Tulsa Vision 2025  Dam Safety Issues ► Keystone ► Pine Creek ► Tenkiller  Lake Eufaula Advisory Committee  Lake Eufaula Advisory Committee  Tenkiller Downstream Fishery Issues  Broken Bow Seasonal Pool Update - Cultural Broken Bow Seasonal Pool Update Cultural Resources Impacts  Arkansas River Navigation Improvement BUILDING STRONG ®  Oklahoma Comprehensive Water Plan Update Interior Least Tern Operations and H bit t C ti Habitat Creation  2011 Breeding Season Survey Results: - Arkansas River System: 517 adults, 358 fledglings. Season totals exceeded

369

PRESENTATION TITLE  

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

Projects Impacting Federal Projects Impacting Federal Power Tulsa District Dan Brueggenjohann 12 June 2013 BUILDING STRONG ®  Interpretation/Application of CERM-F-2013-18  303(d) Listing of Broken Bow Tailwaters  Interior Least Tern Operations and Habitat Creation  Tulsa Vision 2025  Dam Safety Issues ► Keystone, Pine Creek, Robert S. Kerr, Denison  Lake Eufaula Advisory Committee  Tenkiller Downstream Fishery Issues  Broken Bow Seasonal Pool Update - Cultural Resources Impacts  Arkansas River Navigation Improvement  Oklahoma Comprehensive Water Plan Update BUILDING STRONG ® Interpretation/Application of CERM-F-2013-18  Situation - New Resource Management regulation to increase the capitalization threshold for power marketing agency assets.

370

CATEGORICAL EXCLUSION (CX) DETERMINATION BRIEF DESCRIPTION OF PROPOSED ACTION:  

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

Southwestern Power Administration (Southwestern) proposes to modify and/or construct several Arkansas, Southwestern Power Administration (Southwestern) proposes to modify and/or construct several Arkansas, Oklahoma, and Missouri communication tower facilities to facilitate the spectrum relocation of Federal communications systems in conjunction with the Commercial Spectrum Enhancement Act (CSEA, Title II of P.L. 108-494). Communication tower facility modifications and construction activities include 13 tower replacements, 16 tower removals, and 6 communication site dispositions. The 35 tower project locations, identified by state, include: ~ Arkansas- Hardy, Melbourne, Paragould, Piggott, Bethel, Bull Shoals, Norfork, Piggott, Poteau Mountain, Decatur, Sulphur Rock, Van Buren, Winesburg, and Humphrey ~ Oklahoma- Broken Bow Project Office, Broken Bow Powerhouse, Gore Substation, Lamar, Weleetka,

371

Reactions of He/sup +/, Ne/sup +/, and Ar/sup +/ with CH/sub 4/, C/sub 2/H/sub 6/, SiH/sub 4/, and Si/sub 2/H/sub 6/  

SciTech Connect

The rate coefficients and product-ion distributions for the reactions of He/sup +/ and Ar/sup +/ with silane and disilane have been measured in a drift tube, typically for collision energies of 0.01--1 eV. The total charge-exchange rate coefficients are found to be roughly independent of E/N, or collision energy, and are about equal to the Langevin values for the reactions of He/sup +/ with SiH/sub 4/ and C/sub 2/H/sub 6/ and Ar/sup +/ with CH/sub 4/ and C/sub 2/H/sub 6/. The He/sup +/ rate coefficients on CH/sub 4/ and Si/sub 2/H/sub 6/, and the Ne/sup +/ rate coefficients on SiH/sub 4/ and Si/sub 2/H/sub 6/ are 50% to 80% of the Langevin values, while the Ar/sup +/ rate coefficients on SiH/sub 4/ and Si/sub 2/H/sub 6/ are much smaller. Product ions tend to be hydrogen poor with very infrequent breaking of the C--C or Si--Si bonds. Furthermore, hydrogen stripping is more severe for the silanes than the alkanes. These product-ion distributions bear no resemblance to the product-ion distributions of either photoionization or electron collisional ionization.

Chatham, H.; Hils, D.; Robertson, R.; Gallagher, A.C.

1983-08-01T23:59:59.000Z

372

NE Press Releases | Department of Energy  

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

July 8, 2010 July 8, 2010 Department of Energy Announces more than $18 Million to Strengthen Nuclear Education at U.S. Universities and Colleges Awards $5 million for 117 scholarships and fellowships, and $13.2 million for infrastructure upgrades for university nuclear programs June 21, 2010 Global Nuclear Energy Partnership Steering Group Members Approve Transformation to the International Framework for Nuclear Energy Cooperation The Global Nuclear Energy Partnership Steering Group met in Accra, Ghana on June 16-17, 2010, and approved unanimously several transformative changes to reflect global developments that have occurred since the Partnership was established in 2007. June 2, 2010 International Working Group Meeting Focuses on Nuclear Power Infrastructure Development and Needs

373

NE Blog Archive | Department of Energy  

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

January 30, 2008 January 30, 2008 Artist's concept of the New Horizons spacecraft during its planned encounter with Pluto and its moon, Charon. The craft's miniature cameras, radio science experiment, ultraviolet and infrared spectrometers and space plasma experiments are run by the Department of Energy's Radioisotope Thermoelectric Generator (RTG). | Photo courtesy of Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute (JHUAPL/SwRI) New Horizons Mission Powered by Space Radioisotope Power Systems The New Horizons spacecraft utilized a Radioisotope Thermoelectric Generator (RTG) to provide electricity and heat to the science instruments and other spacecraft components. January 29, 2008 Mars Science Laboratory, aka Curiosity, is part of NASA's Mars Exploration Program, a long-term program of robotic exploration of the Red Planet. It's powered by the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG). Photo courtesy of NASA/JPL-Caltech.

374

NE Press Releases | Department of Energy  

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

September 29, 2011 September 29, 2011 United States and Czech Republic Join Together to Announce Bilateral Nuclear Energy Research and Development Efforts PRAGUE, Czech Republic - The U.S. Department of Energy recently joined with the Řež Nuclear Research Institute, the U.S. September 28, 2011 Department of Energy Issues FY 2012 Request for Pre-Applications from U.S. Universities for Nuclear Energy Research and Development Proposals The U.S. Department of Energy today announced that its Nuclear Energy University Programs is now accepting pre-applications from universities interested in conducting nuclear energy research and development projects. September 21, 2011 Department of Energy Announces $17 Million to Bolster University-Led Nuclear Energy Research and Development

375

NE Press Releases | Department of Energy  

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

March 23, 2010 March 23, 2010 DOE Announces Cooperative Agreement with USEC for American Centrifuge Demonstration Project The U.S. Department of Energy today announced that it finalized a cost-shared $90 million cooperative agreement with USEC Inc. to provide support for the continued development and demonstration of the American Centrifuge technology. March 17, 2010 U.S. and India hold the Third Meeting of the Indo-United States Civil Nuclear Energy Working Group India hosted the third meeting of the Indo-United States Civil Nuclear Energy Working Group in Mumbai, on Feb. 3-4, 2010. March 17, 2010 INL User Facility welcomes three new experiments The number of universities conducting nuclear energy experiments in Idaho National Laboratory's one-of-a-kind research reactor has now reached an

376

NE Press Releases | Department of Energy  

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

February 17, 2010 February 17, 2010 Deputy Secretary Poneman Addresses Nuclear Deterrence Summit Alexandria, VA - U.S. Deputy Secretary of Energy Daniel Poneman today addressed the opening session of the second annual Nuclear Deterrence Summit and discussed the Department of Energy's commitment to helping achieve the President's goals of reducing nuclear dangers and expanding the use of nuclear energy in a manner that minimizes the risks of proliferation. The Deputy Secretary also spoke about the Department's commitment to management excellence. February 16, 2010 Obama Administration Announces Loan Guarantees to Construct New Nuclear Power Reactors in Georgia President Obama today announced that the Department of Energy has offered conditional commitments for a total of $8.33 billion in loan guarantees for

377

NE Blog Archive | Department of Energy  

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

June 1, 2012 June 1, 2012 Navy personnel stationed in Idaho Falls, Idaho, in the mid 1950s learn how to operate the Nautilus S1W, the prototype of the Navy's first nuclear-powered submarine. | Photo courtesy of Idaho National Laboratory Veteran Leadership Strong at Idaho's Laboratory Idaho National Lab has played a large role in building fission reactors for Navy vessels - and then training those military personnel on how to use the equipment. February 15, 2012 Secretary Chu traveled to Waynesboro, Georgia, to visit the Vogtle nuclear power plant, the site of what will be the first new nuclear reactors to be built in the United States in three decades. | Image credit: Southern Company. Secretary Chu Visits Vogtle Nuclear Power Plant Secretary Chu traveled to Waynesboro, Georgia, to visit the Vogtle nuclear

378

NE Press Releases | Department of Energy  

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

April 15, 2011 April 15, 2011 Dr. Peter B. Lyons Confirmed as Assistant Secretary for Nuclear Energy Washington, D.C. - Dr. Peter B. Lyons was confirmed by the Senate on Thursday, April 14, as the Department of Energy's Assistant Secretary for Nuclear Energy. February 28, 2011 U.S. Department of Energy Issues Fiscal Year 2011 Funding Opportunity Announcements to Enhance Nuclear Energy Education Infrastructure The U.S. Department of Energy today announced two new fiscal year 2011 Funding Opportunity Announcements to support university and college efforts to build or expand their school's nuclear science and engineering basic research or education capabilities. February 18, 2011 Department of Energy Issues Call for Proposals to U.S. Universities for Nuclear Energy-Related Integrated Research Project Proposals

379

MiniBooNE darkmatter collaboration  

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

R. Ford,3 F.G. Garcia,3 G. T. Garvey,8 J. Grange,9 W. Huelsnitz,8 I. L. de Icaza Astiz,1 R.A. Johnson,10 G. Karagiorgi,4 T. Katori,11 T. Kobilarcik,3 W. Ketchum,8 Q. Liu,8 W.C....

380

BooNE: Booster Neutrino Experiment  

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

and tag it with the decay michel electron. These cubes can be used to study the energy deposited by muons, as well as angular effects. schematic of muon tracker and...

Note: This page contains sample records for the topic "broken bow ne" 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

Microsoft Word - CoyoteCreekNE_CX  

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

Project Manager - KEWM-4 Proposed Action: Coyote Creek Property Acquisition Funding Fish and Wildlife Project No.: 2011-003-00, Contract BPA-007521 Categorical Exclusion...

382

BooNE: Booster Neutrino Experiment  

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

Adventure An interactive tour of quarks, neutrinos, anti-matter, extra dimensions, dark matter, accelerators, and particle detectors. Developed by the Particle Data Group....

383

NE Press Releases | Department of Energy  

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

(RFA) for scholarships and fellowships as part of its efforts to recruit and train the next generation of nuclear scientists and engineers. March 9, 2010 Department of...

384

NE Press Releases | Department of Energy  

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

Material Transfer to Czech Republic for Advanced Reactor Research The U.S. Department of Energy recently joined with the U.S. Embassy in Prague and the Czech Republic's Ministry...

385

NE Press Releases | Department of Energy  

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

for nuclear energy in 2013, U.S. Secretary of Energy Steven Chu visited the Vogtle nuclear power plant in Waynesboro, Georgia. February 15, 2012 Chu Visits Site of America's First...

386

BooNE: Booster Neutrino Experiment  

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

linked in their own page with captions. Additional resources are the Talks, Slides and Posters page, Publications page, and Data Release page Beamline Flux Detector Cross sections...

387

NE Press Releases | Department of Energy  

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

2010 International team discovers element 117 An international team of scientists from Russia and the United States, including two Department of Energy national laboratories and...

388

Nucleosynthesis in O-Ne-Mg Supernovae  

SciTech Connect

We have studied detailed nucleosynthesis in the shocked surface layers of an oxygen-neon-magnesium core collapse supernova with an eye to determining whether the conditions are suitable for r-process nucleosynthesis. We find no such conditions in an unmodified model, but do find overproduction of N=50 nuclei (previously seen in early neutron-rich neutrino winds) in amounts that, if ejected, would pose serious problems for Galactic chemical evolution.

Hoffman, R D; Janka, H; Muller, B

2007-12-18T23:59:59.000Z

389

BooNE: Booster Neutrino Experiment  

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

Releases: Data Released with A.A. Aguilar-Arevalo et al., "First Measurement of the Muon Antineutrino Double-Differential Charged-Current Quasielastic Cross section",...

390

MiniBooNE Nuebar Data Release  

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

90% limit contour and 99% limit contour. Sensitivity and limit curves for a 2-neutrino muon-to-electron antineutrino oscillation fit. Frequentist studies were performed to...

391

NE Press Releases | Department of Energy  

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

For Irradiation Performance As part of the Office of Nuclear Energy's Next Generation Nuclear Plant (NGNP) Program, the Advanced Gas Reactor (AGR) Fuel Development Program has...

392

NE Press Releases | Department of Energy  

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

January 20, 2012 January 20, 2012 Energy Department Takes First Step to Spur U.S. Manufacturing of Small Modular Nuclear Reactors Through the draft Funding Opportunity Announcement announced today, the Department will establish cost-shared agreements with private industry to support the design and licensing of SMRs. January 20, 2012 Energy Department Takes First Step to Spur U.S. Manufacturing of Small Modular Nuclear Reactors New Funding Opportunity Announcement Will Support SMR Design and Licensing for Widespread Commercial Use December 22, 2011 Secretary Chu Statement on AP1000 Reactor Design Certification U.S. Energy Secretary Steven Chu issued the following statement today in support of the Nuclear Regulatory Commission's (NRC) decision to certify Westinghouse Electric's AP1000 nuclear reactor design, a significant step

393

Zero-order bows in radially inhomogeneous spheres: direct and inverse problems  

E-Print Network (OSTI)

number density, pressure, and temperature distributions for the Venusian atmo- sphere, amongst other known that sun-illuminated homogeneous raindrops cannot produce zero-order (or direct trans- mission

Adam, John A.

394

Numerical Simulations of Bow Echo Formation Following a Squall LineSupercell Merger  

Science Journals Connector (OSTI)

Output from idealized numerical simulations is used to investigate the storm-scale processes responsible for squall-line evolution following a merger with an isolated supercell. A simulation including a squall linesupercell merger is compared to ...

Adam J. French; Matthew D. Parker

2014-12-01T23:59:59.000Z

395

Extended red objects and stellar-wind bow shocks in the Carina Nebula  

Science Journals Connector (OSTI)

......exceeding the sound speed in their ambient medium (Castor, Abbott Klein 1975) and forming...supersonic velocity relative to the surrounding medium, ambient gas and dust can be swept around...the velocity of the ambient interstellar medium (ISM) relative to the driving stars......

Remington O. Sexton; Matthew S. Povich; Nathan Smith; Brian L. Babler; Marilyn R. Meade; Alexander L. Rudolph

2015-01-01T23:59:59.000Z

396

Exoplanet transit variability: bow shocks and winds around HD 189733b  

Science Journals Connector (OSTI)

......both cases, the maps show the distribution...2.2 Stellar wind model The magnetic surface maps are used as one...conditions in our stellar wind simulation. We...equations, for the wind mass density rhow, gas pressure p w, the velocity of the plasma and......

J. Llama; A. A. Vidotto; M. Jardine; K. Wood; R. Fares; T. I. Gombosi

2013-01-01T23:59:59.000Z

397

On the stability of bow shocks generated by red supergiants: the case of IRC10414  

Science Journals Connector (OSTI)

......between the wind and space velocities of the star...velocities and mass-loss rates...limitation on the mass-loss rate...The space velocity of IRC-10414...the stellar wind velocity...the space velocity of the star...most of the mass-loss prescriptions...presents a map of the surface...the shocked wind, which naturally......

D. M.-A. Meyer; V. V. Gvaramadze; N. Langer; J. Mackey; P. Boumis; S. Mohamed

2014-01-01T23:59:59.000Z

398

The electric potential at the Earth's quasi-parallel bow shock: Initial Cluster results  

E-Print Network (OSTI)

of reflected ions downstream again due to a slowly changing Bn. Incoming solar wind ions may interact with backstreaming, reflected ions. These interactions lead to the generation of low-frequency (ULF) waves [2] via. convected into the shock by the solar wind. Note that SLAMS are produced far upstream in this scenario

California at Berkeley, University of

399

Bow-tie antenna-coupled graphene FETs for direct detection at 0.6THz.  

E-Print Network (OSTI)

??The recent demonstration of the electric field effect in graphene, a two-dimensional carbon lattice, and the measurement of its extraordinary room-temperature properties have sparked enormous (more)

Zak, Audrey

2014-01-01T23:59:59.000Z

400

Interactions of the heliospheric current and plasma sheets with the bow shock: Cluster and Polar observations  

E-Print Network (OSTI)

Jack D. Scudder,3 Forrest S. Mozer,4 Christopher T. Russell,5 Henri Rème,6 Christopher Mouikis,1 and Keith D. Siebert7 Received 28 June 2010; revised 8 November 2010; accepted 16 November 2010; published

California at Berkeley, University of

Note: This page contains sample records for the topic "broken bow ne" 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 directionality in mobile routing Bow-Nan Cheng Murat Yuksel Shivkumar Kalyanaraman  

E-Print Network (OSTI)

, USA e-mail: bownan@gmail.com M. Yuksel Reno ECSE Department, University of Nevada, Reno, NV, USA S compared to RF but suffers from: (1) the need for line of sight (LOS) alignment and (2) reduced transmission quality in adverse weather conditions. Yuksel et al. [4] proposed several ways to mitigate

Yuksel, Murat

402

Quasi-Stationary Convective Systems Forming Perpendicular to, Above the Cold Pool of, Strong Bow Echoes  

E-Print Network (OSTI)

and Forecasting (WRF) model are analyzed in an attempt to understand the mechanisms responsible for initiating and maintaining the convective line. Due to coarse resolution, observational analyses are only useful for inspection of the synoptic-scale. Model...

Keene, Kelly M.

2012-10-19T23:59:59.000Z

403

Impact of Graupel Class in Microphysics Parameterizations on Bow Echo1 Simulations2  

E-Print Network (OSTI)

Research and Forecasting (WRF-ARW)13 model. Multiple simulations are performed, testing the sensitivity, by the environmental wind, and above and below the rear inflow40 into the system can act to ensure the longevity of the system (Weisman 1992). However,41 a temporary, local intensification of the cold pool and its associated

Johnson, Richard H.

404

Deformation and evolution of solar-wind discontinuities through their interactions with the Earth's bow shock  

E-Print Network (OSTI)

1 Deformation and evolution of solar-wind discontinuities through their interactions with the Earth Research Institute, Austrian Academy of Sciences, Graz, Austria. (2) Center for Solar-Terrestrial Research, Alberta, Canada. (5) Institut für Geophysik und extraterrestrische Physik, Technische Universität

405

Giotto measurements of cometary and solar wind plasma at the Comet Halley bow shock  

Science Journals Connector (OSTI)

... wind measurement takes 500ms and is repeated every two spacecraft spins or 8 s. The solar wind energy range covers one-quarter of the total energy range in 30 steps; the upper ...

A. J. Coates; R. P. Lin; B. Wilken; E. Amata; K. A. Anderson; H. Borg; D. A. Bryant; C. W. Carlson; D. W. Curtis; V. Formisano; K. Jockers; A. D. Johnstone; A. Korth; D. A. Mendis; H. Reme; A. K. Richter; H. Rosenbauer; J. A. Sauvaud; W. Stdemann; M. F. Thomsen; C. d'Uston; J. D. Winningham

1987-06-11T23:59:59.000Z

406

Joint MiniBooNE, SciBooNE Disappearance Analysis Gary Cheng ...  

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

Uncertainties * Results 3 Friday, August 31, 2012 4 Neutrino Oscillations e phenomenology of the neutrino oscillation, we generally defin e , , ) ( eL , ...

407

Gravitational waves from broken cosmic strings: The bursts and the beads  

Science Journals Connector (OSTI)

We analyze the gravitational wave signatures of a network of metastable cosmic strings. We consider the case of cosmic string instability to breakage, with no primordial population of monopoles. This scenario is well motivated from grand unified theories and string-theoretic models with an inflationary phase below the grand unified theories/string scale. The network initially evolves according to a scaling solution, but with breakage events resulting from confined monopoles (beads) being pair produced and accelerated apart. We find these ultrarelativistic beads to be a potent source of gravitational wave bursts, detectable by initial LIGO, advanced LIGO, and LISA. Indeed, advanced LIGO could observe bursts from strings with tensions as low as G??10-12. In addition, we find that ultrarelativistic beads produce a scale-invariant stochastic background detectable by LIGO, LISA, and pulsar timing experiments. The stochastic background is scale invariant up to the Planckian frequencies. This phenomenology provides new constraints and signatures of cosmic strings that disappear long before the present day.

Louis Leblond; Benjamin Shlaer; Xavier Siemens

2009-06-24T23:59:59.000Z

408

Retrieval of Aerosol Optical Depth in Vicinity of Broken Clouds from Reflectance Ratios: Case Study  

SciTech Connect

A recently developed reflectance ratio (RR) method for the retrieval of aerosol optical depth (AOD) is evaluated using extensive airborne and ground-based data sets collected during the Cloud and Land Surface Interaction Campaign (CLASIC) and the Cumulus Humilis Aerosol Processing Study (CHAPS), which took place in June 2007 over the U.S. Department of Energy (DOE) Atmospheric Radiation Measurement (ARM) Southern Great Plains site. A detailed case study is performed for a field of single-layer shallow cumuli observed on June 12, 2007. The RR method is applied to retrieve the spectral values of AOD from the reflectance ratios measured by the MODIS Airborne Simulator (MAS) for two pairs of wavelengths (660 and 470 nm and 870 and 470 nm) collected at a spatial resolution of 0.05 km. The retrieval is compared with an independent AOD estimate from three ground-based Multi-filter Rotating Shadowband Radiometers (MFRSRs). The interpolation algorithm that is used to project MFRSR point measurements onto the aircraft flight tracks is tested using AOD derived from NASA Langley High Spectral Resolution Lidar (HSRL). The RR AOD estimates are in a good agreement (within 5%) with the MFRSR-derived AOD values for the 660-nm wavelength. The AODs obtained from MAS reflectance ratios overestimate those derived from MFRSR measurements by 15-30% for the 470-nm wavelength and underestimate the 870-nm AOD by the same amount.

Kassianov, Evgueni I.; Ovchinnikov, Mikhail; Berg, Larry K.; McFarlane, Sally A.; Flynn, Connor J.; Ferrare, Richard; Hostetler, Chris A.; Alexandrov, Mikhail

2010-10-06T23:59:59.000Z

409

Postmortem computed tomography images of a broken piece of a weapon in the skull  

Science Journals Connector (OSTI)

The use of post-mortem radiological imaging is becoming increasing widespread in forensic medicine. These images can help improve the quality and safety of autopsy. We report two cases of homicide victims that ha...

Yusuke Kawasumi; Yoshiyuki Hosokai; Akihito Usui

2012-02-01T23:59:59.000Z

410

Broken axial symmetry as essential feature to predict radiative capture in heavy nuclei  

E-Print Network (OSTI)

Cross sections for neutron capture in the range of unresolved resonances are predicted for more than 140 spin-0 target nuclei with A > 50. Allowing the breaking of spherical and axial symmetry in nearly all these nuclei a combined parameterization for both, level density and photon strength is obtained which employs a surprisingly small number of parameters only. The strength functions used are based on a global fit to IVGDR shapes by the sum of three Lorentzians. They are based on theoretical predictions for the A-dependence of pole energies and spreading widths and add up to the TRK sum rule. For the small spins reached by capture resonance spacings are well described by a level density parameter close to the nuclear matter value; a significant collective enhancement is apparent due to the deviation from axial symmetry. Reliable predictions for compound nuclear reactions also outside the valley of stability (as important for nuclear astrophysics and for the transmutation of nuclear waste) are expected to result from the global parameterization presented.

Eckart Grosse; Arnd R. Junghans; Ralph Massarczyk

2015-01-14T23:59:59.000Z

411

Crude oil prices and petroleum inventories : remedies for a broken oil price forecasting model.  

E-Print Network (OSTI)

??The empirical relationship between crude oil prices and petroleum inventories has been exploited in a number of short-term oil price forecasting models. Some of the (more)

Grimstad, Dan

2007-01-01T23:59:59.000Z

412

Problematic p-benzyne: Orbital instabilities, biradical character, and broken symmetry  

E-Print Network (OSTI)

-Fock RHF and UHF , restricted Brueckner RB orbital, and Generalized Valence Bond GVB theory. RHF-restricted description is provided when using Brueckner orbitals at the RB-CCD T level. GVB leads to exaggerated

Crawford, T. Daniel

413

Stochastic Radiative Transfer in Multilayer Broken Clouds. Part II: Validation Tests  

SciTech Connect

In the second part of our two-part paper we estimated the accuracy and robustness of the approximated equations for the mean radiance that were derived in Part I. In our analysis we used the three-dimensional (3D) cloud fields provided by (i) the stochastic Boolean model, (ii) large-eddy simulation model and (iii) satellite cloud retrieval. The accuracy of the obtained equations was evaluated by comparing the ensemble-averaged radiative properties that were obtained by the numerical averaging method (reference) and the analytical averaging method (approximation). The robustness of these equations was estimated by comparing the domain-averaged radiative properties obtained by using (i) the full 3D cloud structure (reference) and (ii) the bulk cloud statistics (approximation). It was shown that the approximated equations could provide reasonable accuracy ({approx}15%) for both the ensemble-averaged and domain-averaged radiative properties.

Kassianov, Evgueni I.; Ackerman, Thomas P.; Marchand, Roger T.; Ovtchinnikov, Mikhail

2003-04-01T23:59:59.000Z

414

Broken axial symmetry as essential feature to predict radiative capture in heavy nuclei  

E-Print Network (OSTI)

Cross sections for neutron capture in the range of unresolved resonances are predicted for more than 140 spin-0 target nuclei with A > 50. Allowing the breaking of spherical and axial symmetry in nearly all these nuclei a combined parameterization for both, level density and photon strength is obtained which employs a surprisingly small number of parameters only. The strength functions used are based on a global fit to IVGDR shapes by the sum of three Lorentzians. They are based on theoretical predictions for the A-dependence of pole energies and spreading widths and add up to the TRK sum rule. For the small spins reached by capture resonance spacings are well described by a level density parameter close to the nuclear matter value; a significant collective enhancement is apparent due to the deviation from axial symmetry. Reliable predictions for compound nuclear reactions also outside the valley of stability (as important for nuclear astrophysics and for the transmutation of nuclear waste) are expected to result from the global parameterization presented.

Eckart Grosse; Arnd R. Junghans; Ralph Massarczyk

2014-09-06T23:59:59.000Z

415

Broken axial symmetry as essential feature to predict radiative capture in heavy nuclei  

E-Print Network (OSTI)

Cross sections for neutron capture in the range of unresolved resonances are predicted for more than 140 spin-0 target nuclei with A > 50. Allowing the breaking of spherical and axial symmetry in nearly all these nuclei a combined parameterization for both, level density and photon strength is obtained which employs a surprisingly small number of parameters only. The strength functions used are based on a global fit to IVGDR shapes by the sum of three Lorentzians. They are based on theoretical predictions for the A-dependence of pole energies and spreading widths and add up to the TRK sum rule. For the small spins reached by capture resonance spacings are well described by a level density parameter close to the nuclear matter value; a significant collective enhancement is apparent due to the deviation from axial symmetry. Reliable predictions for compound nuclear reactions also outside the valley of stability (as important for nuclear astrophysics and for the transmutation of nuclear waste) are expected to re...

Grosse, Eckart; Massarczyk, Ralph

2014-01-01T23:59:59.000Z

416

Penguins, trees and final state interactions in B decays in broken SU3  

Science Journals Connector (OSTI)

The availability of data on Bs decays to strange quasi-two-body final states, either with or without charmonium opens new possibilities for understanding different contributions of weak diagrams and in particular the relative contributions of tree and penguin diagrams. Corresponding Bd and Bs decays to charge conjugate final states are equal in the SU(3) symmetry limit and the dominant SU(3) breaking mechanism is given by ratios of CKM matrix elements. Final State Interactions effects should be small, because strong interactions conserve C and should tend to cancel in ratios between charge conjugate states. Particularly interesting implications of decays into final states containing ? and ?? are discussed.

Harry J. Lipkin

1997-01-01T23:59:59.000Z

417

Broken Bar Detection in Synchronous Machines Based Wind Energy Conversion System  

E-Print Network (OSTI)

Electrical machines are subject to different types of failures. Early detection of the incipient faults and fast maintenance may prevent costly consequences. Fault diagnosis of wind turbine is especially important because they are situated...

Rahimian, Mina Mashhadi

2012-10-19T23:59:59.000Z

418

Surfaces: a playground for physics with broken symmetry in reduced dimensionality  

SciTech Connect

With our crystal ball in front of us, we attempt to articulate the opportunities and challenges for a surface physicist in the beginning of the new millennium. The challenge is quite clear: to use the unique environment of a surface or interface to do fascinating physics, while taking full advantage of the skills the community has developed over the last 30 years. The opportunities appear to be endless! In this age of Nanotechnology where the promise is to shape the world atom by atom, leading to the next industrial revolution [Nanotechnology: shaping the world atom by atom, National Science and Technology Council, Committee on Technology, 1999], surface science should be at the very forefront of both technological and scientific advances. The smaller objects become, the more important their surfaces become. In this article we focus on the role of a surface physicist in the emergence of nanoscale collective phenomena in complex materials.

Plummer, E.W.

2001-07-11T23:59:59.000Z

419

Suppression of bulk conductivity in InAs/GaSb broken gap composite quantum wells  

SciTech Connect

The two-dimensional topological insulator state in InAs/GaSb quantum wells manifests itself by topologically protected helical edge channel transport relying on an insulating bulk. This work investigates a way of suppressing bulk conductivity by using gallium source materials of different degrees of impurity concentrations. While highest-purity gallium is accompanied by clear conduction through the sample bulk, intentional impurity incorporation leads to a bulk resistance over 1 M?, independent of applied magnetic fields. In addition, ultra high electron mobilities for GaAs/AlGaAs structures fabricated in a molecular beam epitaxy system used for the growth of Sb-based samples are reported.

Charpentier, Christophe; Flt, Stefan; Reichl, Christian; Nichele, Fabrizio; Nath Pal, Atindra; Pietsch, Patrick; Ihn, Thomas; Ensslin, Klaus; Wegscheider, Werner [Laboratory for Solid State Physics, ETH Zrich, 8093 Zrich (Switzerland)] [Laboratory for Solid State Physics, ETH Zrich, 8093 Zrich (Switzerland)

2013-09-09T23:59:59.000Z

420

History of AUV's Hull shape Typically, hull shape is based on a body of revolution with a rounded bow,  

E-Print Network (OSTI)

for calculating laminar/turbulent boundary layer thickness and for transition prediction. · To study of how and the results of transition point (xtran) and drag cofficient (CDA) at Re = 5?107 picture from Zedan (1978 techniques or the designer's experience. · The computer CFD software simulation is the main design tool

Sóbester, András

Note: This page contains sample records for the topic "broken bow ne" 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

Mesoscale Surface Pressure and Temperature Features Associated with Bow Echoes REBECCA D. ADAMS-SELIN AND RICHARD H. JOHNSON  

E-Print Network (OSTI)

-SELIN AND RICHARD H. JOHNSON Department of Atmospheric Science, Colorado State University, Fort Collins, Colorado

Johnson, Richard H.

422

Microsoft Word - N01221_NE Site IRAP final.doc  

Office of Legacy Management (LM)

Northeast Site Northeast Site August 2008 Office of Legacy Management LMS/PIN/N01221 Work Performed Under DOE Contract No. for the U.S. Department of Energy Office of Legacy Management. DE-AM01-07LM00060 Approved for public release; distribution is unlimited. Office of Legacy Management Office of Legacy Management Office of Legacy Management U.S. Department of Energy This page intentionally left blank LMS/PIN/N01221 Pinellas Environmental Restoration Project Interim Remedial Action Plan for Source Removal at the Northeast Site August 2008 This page intentionally left blank U.S. Department of Energy Interim Remedial Action Plan for Source Removal at the Northeast Site August 2008 Doc. No. N0122100 Page iii Contents Acronyms and Abbreviations .........................................................................................................

423

NE-20 ACTION: SSDP Project Charter Revision CONCURRENCES RTG SYMBOL  

Office of Legacy Management (LM)

0 0 ACTION: SSDP Project Charter Revision CONCURRENCES RTG SYMBOL James W. Vaughan, Jr. N-923 Acting Assistant Secretary . for Nuclear Energy Murphi Attached for your signature is a revised Project Charter for the 1/ 86 Shippingport Station Decommissioning Project (SSDP). Since our original M determination in July that there was a need to revise the SSDP Charter, we N K23 have been in discussion with the Richland Operations Field Office (RL). INe Significant differences in management philosophy surfaced between RL and DeLaney Headquarters that required discussions up to and including the RL Manager DAE/86 and myself. I now feel that the revised Charter reflects a mutually acceptable working arrangement between the appropriate organizations. The RTGSYMBOL general roles and responsibilities defined in this Charter will facilitate

424

File:EIA-Williston-NE-BOE.pdf | Open Energy Information  

Open Energy Info (EERE)

Northeast Part By 2001 BOE Reserve Class Northeast Part By 2001 BOE Reserve Class Size of this preview: 776 × 600 pixels. Full resolution ‎(6,600 × 5,100 pixels, file size: 5.94 MB, MIME type: application/pdf) Description Williston Basin, Northeast Part By 2001 BOE Reserve Class Sources Energy Information Administration Authors Samuel H. Limerick; Lucy Luo; Gary Long; David F. Morehouse; Jack Perrin; Robert F. King Related Technologies Oil, Natural Gas Creation Date 2005-09-01 Extent Regional Countries United States UN Region Northern America States Montana, North Dakota, South Dakota File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 18:49, 20 December 2010 Thumbnail for version as of 18:49, 20 December 2010 6,600 × 5,100 (5.94 MB) MapBot (Talk | contribs) Automated bot upload

425

File:EIA-Williston-NE-Liquids.pdf | Open Energy Information  

Open Energy Info (EERE)

Liquids.pdf Liquids.pdf Jump to: navigation, search File File history File usage Williston Basin, Northeast Part By 2001 Liquids Reserve Class Size of this preview: 776 × 600 pixels. Full resolution ‎(6,600 × 5,100 pixels, file size: 5.95 MB, MIME type: application/pdf) Description Williston Basin, Northeast Part By 2001 Liquids Reserve Class Sources Energy Information Administration Authors Samuel H. Limerick; Lucy Luo; Gary Long; David F. Morehouse; Jack Perrin; Robert F. King Related Technologies Oil, Natural Gas Creation Date 2005-09-01 Extent Regional Countries United States UN Region Northern America States Montana, North Dakota, South Dakota File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment

426

NE-24 Gilman Hall, University of California, Certification Documentation  

Office of Legacy Management (LM)

Gilman Hall, University of California, Gilman Hall, University of California, Certification Documentation Berkeley, California, Conditional Verlette Gatlin, MA-232 I am attaching for entry into the Public Document Room, two copies of the subject documentation. These documents are the backup data for the conditional certification that the site is radiologically acceptable for restricted use as noted in the certification statement published in the Federal Register. Inasmuch as the conditional certification is made public through the Federal Register, it is prudent that the attached backup documentation also be available to the public. The docket consists of: 1. Introduction: Introduction to the certification docket for Gilman Hall, University of California, Berkeley, California. 2. Exhibit I: Summary of activities at Gilman Hall, University of

427

Microsoft Word - 2.8.12 NE Final Testimony  

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

Peter Lyons Peter Lyons Assistant Secretary for Nuclear Energy U.S. Department of Energy Before the Committee on Science, Space, and Technology U.S. House of Representatives Assessing America's Nuclear Future- A review of the Blue Ribbon Commission's Report to the Secretary of Energy February 8, 2012 Chairman Hall, Ranking Member Johnson, and Members of the Committee, thank you for the opportunity to appear before you today to discuss the Blue Ribbon Commission's (BRC) Report to the Secretary of Energy. The Commissioners worked collaboratively and constructively - through a public, open and transparent process - on recommendations to support a new strategy for the back end of the nuclear fuel cycle. The Administration commends the Commission for its

428

NE-24 Designation of Universal Cyclops, Inc., Titusville Plant  

Office of Legacy Management (LM)

Universal Cyclops, Inc., Titusville Plant Universal Cyclops, Inc., Titusville Plant Pennsylvania, for Remedial iiction under the Formerly Uti Remedial Action Program (FUSRAP) J. LaGrone, Manager Oak Ridge Operations Office Aliquippa, iized Sites pg!. " * 1 ' j---' R , 7. Based on the data in the attached report, it has been determined that the subject site is contaminated with radioactive residues as a result of Manhattan Engineer District/Atomic Energy Commission operations at the site. The contamination is in excess of acceptable guidelines and warrants designation for remedial action under the FUSRAP, Although the contamirta- tion levels exceed guidelines, the risk of exposure and associated health effects are low under current use and/or potential future use of the site; therefore, the site is designated as a low priority site for remedial -

429

The MicroBooNE Experiment - About the Detector  

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

Ryan is power washing the cryostat Cryostat Roberto is power washing the cryostat PMT Rack The photomultiplier tube (PMT) rack is sitting in the cryostat Cryostat Jonathan and...

430

INTRODUCTION NE Forests 2100: A Synthesis of Climate  

E-Print Network (OSTI)

are increasing atmospheric concentra- tions of carbon dioxide and other greenhouse gases (e.g., ni- trous oxide (IPCC 2007). Observed changes in precipitation (i.e., quantity, frequency, intensity, type) have disciplines is required to more fully evaluate responses and reduce the uncertainty of future projected change

Mohan, Jacqueline E.

431

Aussie LNG players target NE Asia in expansion bid  

SciTech Connect

Australia's natural gas players, keen to increase their presence in world liquefied natural gas trade, see Asia as their major LNG market in the decades to come. That's despite the fact that two spot cargoes of Australian Northwest Shelf LNG were shipped to Europe during the last 12 months and more are likely in 1994. Opportunities for growth are foreseen within the confines of the existing Northwest Shelf gas project for the rest of the 1990s. But the main focus for potential new grassroots project developers and expansions of the existing LNG plant in Australia is the expected shortfall in contract volumes of LNG to Japan, South Korea, and Taiwan during 2000--2010. Traditionally the price of crude oil has been used as a basis for calculating LNG prices. This means the economics of any new 21st century supply arrangements are delicately poised because of the current low world oil prices, a trend the market believes is likely to continue. In a bid to lessen the effect of high initial capital outlays and still meet projected demand using LNG from new projects and expansion of the existing plant, Australia's gas producers are working toward greater cooperation with prospective Asian buyers.

Not Available

1994-02-28T23:59:59.000Z

432

High Precision Measurement of the 19Ne Lifetime  

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

. . . . . . . . . . . . . . . . . . . . . . . . . 106 viii List of Figures 1.1 Feynman diagram of neutron decay. . . . . . . . . . . . . . . . . . . . 4 1.2 V ud from independent...

433

Ion-trap electrode preparation with Ne$^+$ bombardment  

E-Print Network (OSTI)

We describe an ex-situ surface-cleaning procedure that is shown to reduce motional heating from ion-trap electrodes. This precleaning treatment, to be implemented immediately before the final assembly and vacuum processing of ion traps, removes surface contaminants remaining after the electrode-fabrication process. We incorporate a multi-angle ion-bombardment treatment intended to clean the electrode surfaces and interelectrode gaps of microfabricated traps. This procedure helps to minimize redeposition in the gaps between electrodes that can cause electrical shorts. We report heating rates in a stylus-type ion trap prepared in this way that are lower by one order of magnitude compared to a similar untreated stylus-type trap using the same experimental setup.

McKay, K S; Colombe, Y; Jrdens, R; Wilson, A C; Slichter, D H; Allcock, D T C; Leibfried, D; Wineland, D J; Pappas, D P

2014-01-01T23:59:59.000Z

434

Ion-trap electrode preparation with Ne$^+$ bombardment  

E-Print Network (OSTI)

We describe an ex-situ surface-cleaning procedure that is shown to reduce motional heating from ion-trap electrodes. This precleaning treatment, to be implemented immediately before the final assembly and vacuum processing of ion traps, removes surface contaminants remaining after the electrode-fabrication process. We incorporate a multi-angle ion-bombardment treatment intended to clean the electrode surfaces and interelectrode gaps of microfabricated traps. This procedure helps to minimize redeposition in the gaps between electrodes that can cause electrical shorts. We report heating rates in a stylus-type ion trap prepared in this way that are lower by one order of magnitude compared to a similar untreated stylus-type trap using the same experimental setup.

K. S. McKay; D. A. Hite; Y. Colombe; R. Jrdens; A. C. Wilson; D. H. Slichter; D. T. C. Allcock; D. Leibfried; D. J. Wineland; D. P. Pappas

2014-06-06T23:59:59.000Z

435

DOE-NE-STD-1004-92 | Department of Energy  

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

& Publications Type B Investigation Board Report on the June 19, 1997, Occupational Illness at the Y-12 Plant, Oak Ridge, Tennessee DOE-HDBK-1208-2012 Inspection Report: IG-044...

436

ne of the quirks of the Earth's stratigraphic recording system  

E-Print Network (OSTI)

. An alluvial river channel (one formed from its own sediment) and its adjoining flood plain are self in which the channel­flood-plain system organizes itself. In many alluvial rivers, sedimentation associated onto the flood plain once the levee is breached. So, rather than gradually inundatingthefloodplain

Paola, Chris

437

MiniBooNE Nue & Nuebar Data Release 2012  

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

90% limit contour and 99% limit contour. Sensitivity and limit curves for a 2-neutrino muon-to-electron neutrino and antineutrino oscillation fit. Frequentist studies were...

438

MiniBooNE Nue & Nuebar Data Release 2012  

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

limit contour and 3 sigma limit contour. Sensitivity and limit curves for a 2-neutrino muon-to-electron neutrino and antineutrino oscillation fit. Frequentist studies were...

439

Microsoft PowerPoint - USWIN - INL_NE_Overview.ppt  

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

* First Breeder Reactor * First Naval Propulsion Reactor * 52 Research, Development, Testing, and Demonstration Reactors * Worldwide Nuclear Safety Basis (LOFTRELAP5) DOE's...

440

The MicroBooNE Technical Design Report  

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

a dry, inert environment for as long as possible. The cabling from each PMT routs to a patch panel attached to the back of the support rack nearest to the open end of the...

Note: This page contains sample records for the topic "broken bow ne" 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.


441

The MicroBooNE Experiment - Getting Started  

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

between 7:30am - 4:45pm. Have your Fermilab ID number ready and call 1-630-840-4225. Bicycle Rental - inquire at the Housing Office. Public Transport - This varies, most people...

442

Fabry-Prot Interference in Gapped Bilayer Graphene with Broken Anti-Klein Tunneling Anastasia Varlet,1,*  

E-Print Network (OSTI)

the efficiency of sharp potential steps between the n- and p-type regions, which play the role, Tsukuba 305-0044, Japan (Received 13 June 2014; published 8 September 2014) We report the experimental or the particle energy is varied. In solid-state physics, graphene has proven to be a sui- table material

Schubart, Christoph

443

Functional approach for pairing in finite systems: How to define restoration of broken symmetries in Energy Density Functional theory ?  

E-Print Network (OSTI)

The Multi-Reference Energy Density Functional (MR-EDF) approach (also called configuration mixing or Generator Coordinate Method), that is commonly used to treat pairing in finite nuclei and project onto particle number, is re-analyzed. It is shown that, under certain conditions, the MR-EDF energy can be interpreted as a functional of the one-body density matrix of the projected state with good particle number. Based on this observation, we propose a new approach, called Symmetry-Conserving EDF (SC-EDF), where the breaking and restoration of symmetry are accounted for simultaneously. We show, that such an approach is free from pathologies recently observed in MR-EDF and can be used with a large flexibility on the density dependence of the functional.

Guillaume Hupin; Denis Lacroix; Michael Bender

2011-05-30T23:59:59.000Z

444

A BROKEN SOLAR TYPE II RADIO BURST INDUCED BY A CORONAL SHOCK PROPAGATING ACROSS THE STREAMER BOUNDARY  

SciTech Connect

We discuss an intriguing type II radio burst that occurred on 2011 March 27. The dynamic spectrum was featured by a sudden break at about 43 MHz on the well-observed harmonic branch. Before the break, the spectrum drifted gradually with a mean rate of about -0.05 MHz s{sup -1}. Following the break, the spectrum jumped to lower frequencies. The post-break emission lasted for about 3 minutes. It consisted of an overall slow drift which appeared to have a few fast-drift sub-bands. Simultaneous observations from the Solar TErrestrial RElations Observatory and the Solar Dynamics Observatory were also available and are examined for this event. We suggest that the slow-drift period before the break was generated inside a streamer by a coronal eruption driven shock, and the spectral break as well as the relatively wide spectrum after the break is a consequence of the shock crossing the streamer boundary where density drops abruptly. It is suggested that this type of radio bursts can be taken as a unique diagnostic tool for inferring the coronal density structure, as well as the radio-emitting source region.

Kong, X. L.; Chen, Y.; Li, G.; Feng, S. W.; Song, H. Q.; Jiao, F. R. [Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209 (China); Guo, F., E-mail: yaochen@sdu.edu.cn [Department of Planetary Sciences and Lunar and Planetary laboratory, University of Arizona, Tucson, AZ 85721 (United States)

2012-05-10T23:59:59.000Z

445

Parity Broken Chiral Spin Dynamics in Ba3NbFe3Si2O14 V. Simonet,1  

E-Print Network (OSTI)

by unpolarized and polarized inelastic neutron scattering. A dynamical fingerprint of the chiral ground state are equipopulated, the chirality is usually averaged to zero in centrosymmetric magnets. However, neutron scattering by means of polarized neutron scattering experiments. Our study provides evidence for a fully chiral spin

Boyer, Edmond

446

Los Angeles of My Broken Heart: Pocha Mobility in Mxico de mi corazn and Del otro lado del puente  

E-Print Network (OSTI)

Emilio Garca. Mxico de mi corazn. Historia documental372-373. Print. Films Mxico de mi corazn (Dos mexicanas enPocha Mobility in Mxico de mi corazn and Del otro lado del

Parades, Veronica

2012-01-01T23:59:59.000Z

447

Broken Information Feedback Loops Prevent Good Building Energy PerformanceIntegrated Technological and Sociological Fixes Are Needed  

E-Print Network (OSTI)

Trajectory Toward Zero Net Energy. In Proceedings of thethe New Scale for a Zero Net-Energy Future. Architecturalto a new campus goal of zero-net energy by 2020 (Elliott and

Arens, Edward; Brown, Karl

2012-01-01T23:59:59.000Z

448

Broken Information Feedback Loops Prevent Good Building Energy PerformanceIntegrated Technological and Sociological Fixes Are Needed  

E-Print Network (OSTI)

Summer Study on Energy Efficiency in Buildings, Monterey CAStudy of Energy Efficiency in Buildings. Panel 4 Paper 1130.Summer Study of Energy Efficiency in Buildings. 5:13-5:25.

Arens, Edward; Brown, Karl

2012-01-01T23:59:59.000Z

449

Broken Information Feedback Loops Prevent Good Building Energy PerformanceIntegrated Technological and Sociological Fixes Are Needed  

E-Print Network (OSTI)

Communication Toward Deep Efficiency. Presentation to the 2010 Behavior, Energy, and Climate Change (

Arens, Edward; Brown, Karl

2012-01-01T23:59:59.000Z

450

A broken material approach to modeling oil sand under dynamic load Tim Grain Joseph, Ph.D., P.Eng.,  

E-Print Network (OSTI)

.Eng., Asst. Professor, Mining, University of Alberta and Principal Engineer, JPi Ltd. and Ardeshir Demoobed example of strain softening material in the context of an underfoot environment for large mobile mining behaviour and its response to loading by the equipment. This was discussed by Joseph (2002

Joseph, Tim Grain

451

A modification of MacArthur's Broken Stick Model and its application to aquatic insect populations in a fishless pond  

E-Print Network (OSTI)

0 Enochrus ochzaceusl 2 0 0 0 0 18 1 4 0 1 ~Hd H va s 0 0 0 3 1 1 1 10 0 11 4 0 ~LH '? ~1 imus 1 1 1 1 1 0 0 14 1 0 t t silaris 1 2 0 0 0 0 0 10 0 ~dd thus iri- cojor 16 0 0 0 0 0 0 0 0 0 18 TABLE 1. (Continued) Oct ~ iVov. Dec. Jan... s . 0 1 4 7 0 0 0 0 3 1 0 0 ~hd us s . 1 1 1 0 1 0 0 2 0 2 4 1 ~Hdro- vatus ~us tu- latus 4 3 1 1 0 0 0 0 0 2 1 0 ~P sp. near confusus 2 0 0 0 1 1 1 1 1 0 0 ~Bd h rufi es 0 0 0 0 0 0 0 1 0 0 0 ~02 * cbevro- lati 2 2 0 0 0 0 1 2 0 1 0 0 ~EE d h...

Heitz, Nancy Jo

2012-06-07T23:59:59.000Z

452

Rade, Development, and the Broken Promise of Interdependence: A Buddhist Reflection on the Possibility of Post-market Economics  

E-Print Network (OSTI)

With the increasing sophistication of transportation technologies and infrastructure, lines of transmission for more durable goods quite early became long even by contemporary standards. For example, as early as the second century BCE, the tributary system fueling... function of steady traffic along preferred routes connecting separate localities that have been drawn into some kind of meaningful relationship. The localities might be two villages or family compounds, or they might be a human settlement and a...

Hershock, Peter D

2003-01-01T23:59:59.000Z

453

Data:Cd0e08f3-2fb2-41b3-b757-1686df5354c9 | Open Energy Information  

Open Energy Info (EERE)

f3-2fb2-41b3-b757-1686df5354c9 f3-2fb2-41b3-b757-1686df5354c9 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 Information 2. Demand 3. Energy << Previous 1 2 3 Next >> Basic Information Utility name: Choctaw Electric Coop Inc Effective date: 2008/10/21 End date if known: Rate name: Large Power 6 Sector: Commercial Description: * Available only to Tyson Processing,Broken Bow,Oklahama with installed capacity of 5,000kW.This rate will not be available for service as standby or auxiliary. Subject to only power factor adjustment and Gross Receipt tax. Source or reference: Rate binder # 4 Source Parent: Comments fixed monthly charge per metering point Applicability Demand (kW) Minimum (kW):

454

Excitation and kinematics in H2 bow shocks: near-infrared observations of HH 99 and VLA 1623A (HH 313)  

Science Journals Connector (OSTI)

......with two-dimensional MHD modelling of molecular...interpret excitation (CDR) diagrams and estimate the extinction...magnetohydrodynamic (MHD) shock properties...The velocity-position diagrams (centre and right...column density ratio diagram with large scatter......

Christopher J. Davis; Michael D. Smith; Jochen Eislffel; John K. Davies

1999-09-19T23:59:59.000Z

455

Effects of cumulus clouds on microclimate and shoot-level photosynthetic gas exchange in Picea engelmannii and Abies lasiocarpa at treeline, Medicine Bow Mountains, Wyoming, USA  

Science Journals Connector (OSTI)

Abstract Here we describe the dynamic effects of cumulus clouds on microclimate and shoot-level photosynthetic gas exchange in saplings of two treeline conifer speciesPicea engelmannii and Abies lasiocarpa. Measurements were made during both clear-sky and partly cloudy conditions (?1070% cumulus cloud cover) throughout the 2012 growing season within an alpine-treeline ecotone. Cumulus clouds generated dynamic fluctuations in photosynthetically active radiation (PAR), higher maximum PAR (>2500?molm?2s?1), 24 fold increases in diffuse PAR, reduced daily mean and cumulative PAR, lower needle temperatures, and reduced leaf-to-air vapor pressure differences relative to clear-sky conditions. Onset of cloud-shade corresponded with declines in photosynthesis, needle temperatures, and evapotranspiration, which were proportional to cloud duration and opacity. Despite increased diffuse light and greater sunlight intensity during cloud-gaps, photosynthesis was never higher on partly cloudy days compared to clear days in either species, during cloud-gaps or cloud-shade. However, reduced transpiration paired with photosynthesis comparable with clear-sky levels during cloud-gaps resulted in greater instantaneous water use efficiency relative to clear-sky measurements. There was no apparent photoinhibition of photosynthesis reflected in gas exchange measurements in response to abrupt and dramatic changes in PAR levels caused by cumulus clouds. We conclude that cumulus clouds reduce instantaneous and daily carbon gain, although lower needle temperatures and associated reductions in transpirational water loss may alleviate daily and seasonal water stress, thereby enhancing carbon gain over the growing season.

Nicole M. Hughes; Kaylyn L. Carpenter; David K. Cook; Timothy S. Keidel; Charlene N. Miller; Junior L. Neal; Adriana Sanchez; William K. Smith

2015-01-01T23:59:59.000Z

456

Integration of a 15-Element, VHF Bow-Tie Antenna Array into an Aerodynamic Fairing on a NASA P-3 Aircraft  

E-Print Network (OSTI)

Radar depth sounding and imaging of deep glaciers in Antarctica and Greenland yield results for better understanding a changing climate and improving glacier modeling. A 15-element, airborne antenna array with an increased ...

Byers, Kyle J.

2011-06-16T23:59:59.000Z

457

User Modelling in I-Help: What, Why, When and How Susan Bull, Jim Greer, Gordon McCalla, Lori Kettel, Jeff Bowes  

E-Print Network (OSTI)

User Modelling in I-Help: What, Why, When and How Susan Bull, Jim Greer, Gordon McCalla, Lori. This paper describes user modelling in I-Help, a system to facilitate communication amongst learners. There are two I-Help components: Private and Public Discussions. In the Private Discussions learners take part

Bull, Susan

458

Examination of Gravity Waves Associated with the 13 March 2003 Bow Echo REBECCA D. ADAMS-SELIN* AND RICHARD H. JOHNSON  

E-Print Network (OSTI)

-SELIN* AND RICHARD H. JOHNSON Department of Atmospheric Science, Colorado State University, Fort Collins, Colorado heat release from condensation, freezing, and deposition in the updraft (Houze 1982; Johnson and Young 1983; Gallus and Johnson 1991). The speed of these low- frequency waves is given by c 5 NH np , (1

Johnson, Richard H.

459

Asymptotic normalization coefficients from the (20)Ne((3)He, d)(21)Na reaction and astrophysical factor for (20)Ne(p,gamma)(21)Na  

E-Print Network (OSTI)

, diffuseness a = 0.65 fm, and the Coulomb radius parameter rC = 1.4 fm for comparison. Our spectroscopic factors are significantly lower than those determined in Ref. [1], since Rolfs et al. used a rectangular well in their analysis. The rectangular well... of the Czech Republic, and by the Robert A. Welch Foundation. [1] C. Rolfs, W. S. Rodney, M. S. Shapiro, and H. Winkler, Nucl. Phys. A241, 460 (1975). [2] A. M. Mukhamedzhanov and R. E. Tribble, Phys. Rev. C 59, 3418 (1999). [3] H. M. Xu, C. A. Gagliardi...

Mukhamedzhanov, AM; Bem, P.; Burjan, V.; Gagliardi, Carl A.; Irgaziev, BF; Kroha, V.; Novak, J.; Piskor, S.; Simeckova, E.; Tribble, Robert E.; Vesely, F.; Vincour, J.

2006-01-01T23:59:59.000Z

460

IOP PUBLISHING NANOTECHNOLOGY Nanotechnology 18 (2007) 495704 (7pp) doi:10.1088/0957-4484/18/49/495704  

E-Print Network (OSTI)

) nanostructures, such as helix, coil, ring, spring, bow, and so on, owing to their attractive properties

Wang, Zhong L.

Note: This page contains sample records for the topic "broken bow ne" 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

--No Title--  

U.S. Energy Information Administration (EIA) Indexed Site

Algerian| Brazilian| Canadian | Canadian | Canadian Month | Saharan | Marlim | Bow River | Light Sour | Lloydminster | Blend | | Heavy | Blend | ||...

462

Welcome to the second edition of C&W's Energy and Sustainability Task Force Ne  

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

second edition of C&W's Energy and Sustainability Task Force Newsletter. This second edition of C&W's Energy and Sustainability Task Force Newsletter. This publication illustrates how C&W is delivering on its commitment to enhance the environmental performance of commercial real estate. C&W Managed Properties Earn LEED Volume Certification In January 2010, 18 properties under C&W management earned LEED (Leadership in Energy and Environmental Design) certification utilizing the U.S. Green Building Council's (USGBC) Portfolio Program and volume certification process. More than half of the properties certified at the Platinum and Gold levels. Working closely with our clients, C&W is

463

Klein-NERAC NE education taskforce report 5-18-04  

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

Department of Department of Nuclear Engineering & Radiation Health Physics Report of the Nuclear Energy Research Advisory Committee Nuclear Power Engineering Curriculum Task Force April 7, 2004 Department of Nuclear Engineering & Radiation Health Physics Task Force Members * Andrew C. Klein, Chair, Oregon State University * James F. Stubbins, University of Illinois, Champaign-Urbana * Gilbert Brown, University of Massachusetts, Lowell * Harold Ray, Southern California Edison * Eugene S. Grecheck, Dominion Energy Department of Nuclear Engineering & Radiation Health Physics Primary Concern Expressed * Nuclear engineering curricula had changed over recent times * No longer producing engineers with training optimal to the needs of the power industry Department of Nuclear Engineering

464

Microsoft PowerPoint - NE FY2012 Budget, SMR, and BRC 121311.pptx  

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

Update Update Dr. Peter Lyons Assistant Secretary for Nuclear Energy U.S. Department of Energy Nuclear Energy Advisory Committee Washington, DC December 13, 2011 2 Overview of NEAC Rotation Policy NEAC Statistics * Prior to new members being added in 2009, the average term for the Committee was about 10 years * Reappointed all 16 members with 5 rotating out by September 30 th 2012 * Rotating Members: John Ahearne (Vice-Chair), Marv Fertel, Thomas Cochran, Allen Sessoms, and Neil Todreas * Added Members: Matthew Bunn, Margaret Chu, Susan Eisenhower, Mujid Kazimi, Regis Matzie, Richard Meserve, and Alfred Sattelberger * Disciplines of new members include: Applied Physics, Fuel Element Design, Energy Efficiency, National Security, Advanced Reactor Development, and Nuclear Non-proliferation Issues.

465

6-15-2010_NE_Final_Testimony_R-Shane-Johnson.pdf  

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

R. Shane Johnson R. Shane Johnson Chief Operating Officer for Nuclear Energy U.S. Department of Energy before the Subcommittee on Energy Senate Committee on Energy and Natural Resources on S. 3233, the Surplus Uranium Disposition Act of 2010 June 15, 2010 Introduction Thank you, Madam Chairman, Ranking Member Risch, and Members of the Subcommittee. I appreciate this opportunity to appear before you and comment on legislation under consideration by the Committee, as well as to provide information on the Department of Energy's management and disposition of its excess uranium. The Administration continues to view nuclear power as an important element in its strategy to increase energy security and combat climate change. A strong domestic nuclear industry supports the expansion of clean, carbon-free nuclear energy in the

466

NE-23 List of California Sites Hattie Carwell. SAN/NSQA Division  

Office of Legacy Management (LM)

Hattie Carwell. SAN/NSQA Division Hattie Carwell. SAN/NSQA Division Attached for your information is the list Of Callfornia sites we identified in our search of Manhattdn Engineer District records for the Formerly Utilized Sites Remedial Action Program (FUSRAP). None of the facilities listed qualified for FUSRAP. The only site in California that was included in FUSRAP was Gilman Hall on the University of California-Berkeley Campus. All California sites that are in our Surplus Facilities Management Program are under San Francisco Operations and are at the Santa Susana Field Laboratory or the University of California-Davis. If you have questions on any of the sites on th*? list, please call me at FTS 233-5439. Andrew Wallo III, Designation and Certification Manager Division of Facilitv and Site

467

Microsoft Word - N01401_NE and 4-5 Closure Mon Plan.doc  

Office of Legacy Management (LM)

Closure Monitoring Plan for the Closure Monitoring Plan for the Northeast Site and 4.5 Acre Site August 2009 LMS/PIN/N01401 This page intentionally left blank LMS/PIN/N01401 Pinellas Environmental Restoration Project Closure Monitoring Plan for the Northeast Site and 4.5 Acre Site August 2009 This page intentionally left blank U.S. Department of Energy Closure Monitoring Plan for the Northeast Site and 4.5 Acre Site July 2009 Doc. No. N01401 Page i Contents 1.0 Introduction......................................................................................................................... 1 2.0 Summary of Source Removal Activities............................................................................. 1 3.0 Delineation of Contaminant Plumes ...................................................................................

468

I. Neutrino Oscillations with the MiniBooNE Experiment at FNAL...  

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

and cosmology "Sterile" Neutrinos *Cosmology: o Dark matter o Baryogenisis o Dark energy *Core collapse supernova * Explosion processes * Heavy element formation * Pulsar...

469

Fluctuation Driven FirstOrder Pairing Transition of ChernSimons N.E. Bonesteel  

E-Print Network (OSTI)

­dimensional electron gas at Landau level filling factor š = 1=2 can be viewed as a `Fermi sea' of composite fermions 2 pairing for weak enough attraction and drive the pairing transition which occurs as the attraction natural to ask what effect the CS gauge field may have on BCS pairing. In this short note I introduce

Bonesteel, Nicholas E.

470

Lakes, groundwater and palaeohydrology in the Sahel of NE Nigeria: evidence from hydrogeochemistry  

Science Journals Connector (OSTI)

...contains significant renewable groundwater resources...improved management of the renewable waters in the shallow...International Atomic Energy Agency, Vienna. Technical...Cooling of tropical Brazil (5C) during the last...contains significant renewable groundwater resources...

W. M. EDMUNDS; E. FELLMAN; I. B. GONI

471

SESSIoNE DEL maTTINo 9.00 RegistRazione paRtecipanti  

E-Print Network (OSTI)

sociologo, ?cole des Hautes ?tudes en Sciences Sociales di Parigi] Dal castigo degli dèi ai diritti negati

Robbiano, Lorenzo

472

Kaon Monitoring in MiniBooNE: The LMC Detector E. D. Zimmerman  

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

1.5x1.5 cm 2 , x and y views Downstream: 2x12 cm 2 , only x view (for post-bend slope) Magnet: permanent (ferrite), 2.7 kG, field length 22.5 cm. Design rendering of fiber tracker...

473

E-Print Network 3.0 - astrophysically important 19ne Sample Search...  

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

scope (SXT Source: Bicknell, Geoff - Mt. Stromlo Observatory & Research School of Astronomy and Astrophysics, Australian National University Collection: Physics 2 Indirect...

474

Elastic scattering of low-energy electrons by Ne, Ar, Kr, and Xe  

Science Journals Connector (OSTI)

We treat low-energy electron scattering by atoms within a Kohn-Sham-type one-particle theory. In applying this theory, all many-body effects involved in the projectile-target interaction are absorbed into a one-particle potential. Hence, one merely has to solve an elementary potential-scattering problem. However, there are two crucial points to be observed in the construction of the scattering potential. (1) The Kohn-Sham-type exchange-correlation potential must be formed by using correlation factors which are required to have certain asymptotic and integral properties. (2) Since the scattering process is viewed as being quasistationary, the unbound projectile state must be modified by a bell-jar-type envelope function to account for the effect of a finite residence time in the target where the projectile causes a finite perturbation. During this time the entire system has to be treated as consisting of N+1 indistinguishable electrons which in a Kohn-Sham-type theory are described by only N+1 self-consistent one-particle states. Once the analytical forms of the correlation factors and the envelope function have been chosen, the calculational procedure is completely parameter-free. Although it is considerably simpler than well-established methods in this field, it provides comparably good results on differential cross sections and scattering-induced polarizations in a wide range of impact energies (5100 eV).

R. Haberland; L. Fritsche; J. Noffke

1986-04-01T23:59:59.000Z

475

Microsoft PowerPoint - TAUP_07_MiniBooNE.ppt  

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

(MeV) 15% E resolution at 53 MeV PRELIMINARY Spectrum of Michel electrons from stopping muons Energy vs. Range for events stopping in scintillator cubes 0 Mass Distribution ...

476

Measuring n-N Deep Inelastic Cross Sections at MiniBooNE  

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

fit likelihoods vs fit energy provides nice separation between electrons (top) and muons (bottom) Energy (GeV) 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 ) L e log(L 0.4...

477

Microsoft PowerPoint - NOW2004_MiniBooNE.ppt  

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

53 MeV PRELIMINARY Energy Calibration Checks Spectrum of Michel electrons from stopping muons Energy vs. Range for events stopping in scintillator cubes Mass distribution for...

478

RESULTS OF THE MiniBooNE NEUTRINO OSCILLATION SEARCH E. D. Zimmerman  

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

The Michel electron subevent provides muon tag as well as a very well- understood chargeenergy calibration * Muons capture on nucleus with 8% probability; these capture events...

479

Neobarroco Y erotismo en la poesi?a de Eduardo Espina Y Ne?stor Perlongher  

E-Print Network (OSTI)

apuntando al incesante m?todo de darle un giro al nivel de referencia creando otro para impedirle al lector una lectura lineal haciendo la lectura dif?cil, provocando el caos predicho por Calabrese. Esta tesis se apega a la idea de Calabrese respecto a...

Aregullin-Valdez, Rosalinda

2011-10-21T23:59:59.000Z

480

E-Print Network 3.0 - area ne china Sample Search Results  

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

Shenyang Beijing Fig.1 Growth of GHP in Different Regions in China The increased GHP heating area... heating in China had reached 150 million m2 of building ... Source:...

Note: This page contains sample records for the topic "broken bow ne" 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

Plate tectonics at an awkward junction: rules for the evolution of Sovanco Ridge area, NE Pacific  

Science Journals Connector (OSTI)

......Northern Juan de Fuca Ridge, (W) West Valley, (ES) East SovancoRidge...ately into the extension of the West Valley of the northern Juan de Fuca ridge...to the new spreading centre of West Valley (Fig. 2 and Davis & Lister 1977a......

C. R. B. Lister

1989-02-01T23:59:59.000Z

482

Private in Public - Public in Private: A Library on H Street NE Washington, DC.  

E-Print Network (OSTI)

??The thesis investigates private versus public space and the natural tendency for an individual to seek out its own place within a group. More specifically, (more)

Rutledge, Kathleen Anne

2011-01-01T23:59:59.000Z

483

JOURNAL DE PHYSIQUE Colloque C9, suppl6ment au ne12, Tome 48, decembre 1987  

E-Print Network (OSTI)

region. Due to the resolution obtainable with XPS, (e-2e) and synchroton radiation excited photoelectron

Paris-Sud XI, Université de

484

Autumn 2014 YoRK'S neW ReSeARCH StRAteGY  

E-Print Network (OSTI)

; Environmental Sustainability and Resilience; Health and Wellbeing; Justice and Equality; Risk, Evidence College ­ 4 a new student community Transforming the treatment 5 of cancer patients Pigs' unhappy balloon

485

2010 Sambamurti Lecture: ?Expecting the Unexpected: Neutrino Physics at MiniBooNE?  

ScienceCinema (OSTI)

For more than 50 years, neutrinos have surprised researchers, not only by their mere presence, but also by the recent revelation that these ghostlike particles can oscillate from one type to another. This discovery has opened up a host of new questions about neutrinos and their properties ? questions that scientists are currently in a global race to answer.

Geralyn ?Sam? Zeller

2010-09-01T23:59:59.000Z

486

Microsoft Word - N01357_NE Site Final LDA Report.doc  

Office of Legacy Management (LM)

of the site; a water treatment system that included two 21,000-gallon steel frac tanks, sand filters, and an air stripper located along the west boundary of the site; the...

487

Evaluation of the NCEP/NCAR reanalysis in the NE Pacific and the Bering Sea  

E-Print Network (OSTI)

Marine Environmental Laboratory, National Oceanic and Atmospheric Administration (NOAA), Seattle., 1999; Wang and McPhaden, 2001] or globally [e.g., Weare, 1997; Scott and Alexander, 1999; Yang et al

Ladd, Carol

488

Geophysical imaging methods for analysis of the Krafla Geothermal Field, NE Iceland  

E-Print Network (OSTI)

Joint geophysical imaging techniques have the potential to be reliable methods for characterizing geothermal sites and reservoirs while reducing drilling and production risks. In this study, we applied a finite difference ...

Parker, Beatrice Smith

2012-01-01T23:59:59.000Z

489

Validation of SO2 retrievals from the Ozone Monitoring Instrument over NE China  

E-Print Network (OSTI)

measurements on polluted days. The air mass­corrected collection 3 data still show positive bias. Most fossil fuel burning occurs near the surface where SO2 is released into the planetary boundary aerosol by reaction with OH in air or by reaction with H2O2 in aqueous solutions (clouds) [Seinfeld

Li, Zhanqing

490

Plate tectonics at an awkward junction: rules for the evolution of Sovanco Ridge area, NE Pacific  

Science Journals Connector (OSTI)

......offshorecompression in Winona basin. The spreading-centre terminating...fault does not strike into the bight of the Juan de Fuca strait...it occurs (such as in Winona basin: Davis & Riddihough 1982...Riddihough, R., 1982. The Winona basin: structure and tectonics......

C. R. B. Lister

1989-02-01T23:59:59.000Z

491

EcoCAR: The NeXt Challenge | Department of Energy  

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

electric, extended-range hybrid electric, all-electric, and fuel cell plug-in hybrid electric drives. The teams using plug-in hybrid electric and extended-range electric...

492

Mr. Trevor L. Cook NGNP Project Manager NE-33, Germantown Building  

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

in Area E that exhibited potential for listing. Today, these data could comprise the bulk of the identification phase of cultural resource compliance for any new project...

493

Resonances in the Photo-Ionization Continuum of Ne I (20-150 eV)  

Science Journals Connector (OSTI)

The absorption spectrum of neon in the region 20-150 eV has been studied photographically and photoelectrically, using synchrotron light as a background source. Discrete structure has been observed in three distinct energy ranges. The first is between the P?12,322 limits near 22 eV, involving resonances analogous to those observed by Beutler in Ar, Kr, and Xe; the second is the region between 44 and 60 eV, the structure here being classified as due to two types of excitation: (i) the excitation of a subshell 2s electron, (ii) the simultaneous excitation of two outer 2p electrons; the third region is near 80 eV, where two weak resonances are observed, due to the simultaneous excitation of a subshell 2s and a 2p electron. The resonance profiles of the states 2s 2p6 np P?11, where n=3,4,and5, and the two-electron excitation state 2p4 (P3) 3s 3p P?11 have been studied quantitatively and values of q, ?, and ? determined for each.

K. Codling; R. P. Madden; D. L. Ederer

1967-03-05T23:59:59.000Z

494

lingvasituacioSEFI Ne por publikigo La lingva situacio en Svedio kaj Finnlando  

E-Print Network (OSTI)

16 600 suda samea 2 500 2 500 5 000 lulea samea 2 000 2 000 2 000 pitea samea 1 000 1 000 1 000 umea

Kiselman, Christer

495

lingvasituacioSEFI Ne por publikigo La lingva situacio en Svedio kaj Finnlando  

E-Print Network (OSTI)

suda samea 2 500 2 500 5 000 lulea samea 2 000 2 000 2 000 pitea samea 1 000 1 000 1 000 umea samea 500

Kiselman, Christer

496

Power spectrum analysis of the annual rainfall series for Massachusetts (NE, U.S.A.)  

Science Journals Connector (OSTI)

Maximum Entropy Spectral Analysis of the annual rainfall series for 18871976 (90 years) for Massachusetts (northeastern USA.) shows T...= 17.8 (very near the 18.6 year luni-solar signal) as the most prominent pe...

R. P. Kane; N. R. Teixeira

1991-01-01T23:59:59.000Z

497

CHRIS ROBERTSON & ASSOCIATES, LLC Business and Policy Advisors 3707 NE16th Avenue, Portland, Oregon 97212  

E-Print Network (OSTI)

Resilience and Subduction Zone Earthquake Emergency Response: Impacts of Distributed Solar Energy (DG PV) Supply Systems Environmental cost benefit analyses are usually concerned with how the environment in the event the grid goes down. Distributed solar energy systems can now be built with modern inverters

498

Cas o les tfn (xa, o) ne dpendent pas de y et de z. --  

E-Print Network (OSTI)

dès que le courant anode dépasse 4. 1 o-13 A quelle que soit la tension d'alimentation [ 1]. Nous alimenté par une tension constante de 160o V (80 V par étages), le courant anode est enregistré en fonction. Pour un flux lumineux déterminé, le courant anode a une valeur supérieure au courant limite et le

Boyer, Edmond

499

Status of the MiniBooNE Quasi-Elastic Analysis  

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

Quasi-Elastic Events Chris Green Motivation and detector overview Flux and cross sections Reconstruction and results Summary and outlook DNP '04 Friday 29 th...

500

Synthetic studies toward palau򡭩ne and enantioselective total synthesis of biogenetically related (+)-phakellin and (+)-monobromophakellin  

E-Print Network (OSTI)

R CO 2 H 1.1:Oroidin 1.3:R=H,Br 1.2: AAPE Figure 1. Oroidin (1.1), the key to the pyrrole-imidazole alkaloids 2 B. Isolation and Biological Activity The pyrrole-imidazole alkaloids include an array of structurally diverse and complex secondary...). The phakellstatins (1.12, 1.13) are related members of this family bearing a cyclic urea rather than a cyclic guanidine (Figure 2). The isolation of (-)- dibromophakellstatin (1.13) was reported in 1997 by Pettit and co-workers. 18 The alkaloid was isolated from...

Wang, Shaohui

2009-05-15T23:59:59.000Z