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1

Institute of Geophysics, Planetary Physics, and Signatures  

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

Opportunities » Opportunities » Institute of Geophysics, Planetary Physics, and Signatures Institute of Geophysics, Planetary Physics, and Signatures Promoting and supporting high-quality, cutting-edge science in the areas of astrophysics, space physics, solid planetary geoscience, and climate science. Contact Director Harald Dogliani (505) 663-5309 Email Deputy and Signatures Jon Schoonover (505) 665-0772 Email Professional Staff Assistant Georgia Sanchez (505) 663-5291 Email Astophysics and Cosmology Ed Fenimore (505) 667-7371 Email Climate Manvendra K. Dubey (505) 665-3128 Email Geophysics Scott Baldridge (505) 667-4338 Email Space Physics Josef Koller (505) 665-7395 Email Expanding the frontiers of astrophysical, space, earth, and climate sciences and their signatures The Institute of Geophysics, Planetary Physics, and Signatures at Los

2

Institute of Geophysics and Planetary Physics 1993 annual report, October 1, 1992--September 30, 1993  

SciTech Connect

This report contains brief papers on the research being conducted at the Institute of Geophysics and Planetary Physics in 1993 in Geosciences, High-Pressure sciences, and Astrophysics.

Ryerson, F.J.; Budwine, C.M. [eds.

1994-06-15T23:59:59.000Z

3

LANL Institutes - Institute of Geophysics and Planetary Physics  

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

Expanding the Frontiers of Astrophysical, Space, Earth, & Climate Sciences & Their Signatures The Institute of Geophysics, Planetary Physics, and Signatures at Los Alamos National Laboratory is committed to promoting and supporting high quality, cutting-edge science in the areas of astrophysics, space physics, solid planetary geoscience, and climate science. These subject areas are selected based on their breadth of scientific challenges facing the international scientific community, as well as relevance to the strategic objective to extend Laboratory scientific excellence. IGPPS/LANL makes a special effort to promote and support new research ideas, which can be further developed through seed funding into major programs supported by federal or other funding sources. IGPPS also supports

4

LANL Institutes - Institute of Geophysics and Planetary Physics  

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

Geophysics Geophysics Focus Leader: Scott Baldridge sbaldridge@lanl.gov This focus supports a breadth of basic research concerning planetary surfaces and interiors, including numerical, experimental, and field studies of the structure, properties, processes, and dynamics of terrestrial and giant planets. It is strongly recommended that proposals exploit unique LANL resources (e.g., LANL high-performance computing resources; the Los Alamos Neutron Science Center (LANSCE); geochemical analyses facilities resident in EES and C divisions; and/or sensor technology capabilities resident in C, EES, ISR, and N divisions). We are particularly interested in innovative research projects in areas of current, strong international scientific interest such as the following: New techniques in passive (imaging) or active (e.g., lidar, radar)

5

LANL Institutes - Institute of Geophysics and Planetary Physics  

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

Summer of Applied Geophysical Experience (SAGE) Summer of Applied Geophysical Experience (SAGE) Application Form A complete application includes: An on-line application Letter of Interest two (2) references (download reference form in PDF or Word format). Referee must submit by email to georgia@lanl.gov or fax to: 505-663-5225 proof of health insurance complete transcripts (unofficial is acceptable) Foreign students, please contact Georgia Sanchez at georgia@lanl.gov regarding your application. Cost is $500, $100.00 is due with the application. Please mail deposit with a copy of your application to: SAGE IGPPS, MS-T001 Los Alamos National Laboratory Los Alamos, NM 87545 USA Email: georgia@lanl.gov Voice: 505-663-5291 Note: Course credit may be possible by prior arrangement with your university (please check with your advisor) but cannot be awarded directly

6

LANL Institutes - Institute of Geophysics and Planetary Physics  

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

Space Physics' Space Physics' Focus Leader: Josef Koller jkoller@lanl.gov Proposals are solicited that advance theoretical research, computational research, and/or observational research into the plasma environment of the Earth's atmosphere, the magnetosphere, and into processes that affect these environments. Research on the transport of plasma and energy from the Sun through interplanetary space to the Earth and other planets is also encouraged. These include the interaction of various plasma populations and the coupling of microscopic and macroscopic phenomena. The following topics are covered: solar dynamics responsible for the solar wind magnetohydrodynamics of the magnetosphere and thermosphere magnetospheric substorms Ionosphere lightening magnetotail current sheet dynamics

7

Institute of Geophysics and Planetary Physics at Lawrence Livermore National Laboratory: 1986 annual report  

SciTech Connect

The purpose of the Institute of Geophysics and Planetary Physics (IGPP) at LLNL is to enrich the opportunities of University of California campus researchers by making available to them some of the Laboratory's unique facilities and expertise, and to broaden the scientific horizon of LLNL researchers by encouraging collaborative or interdisciplinary work with other UC scientists. The IGPP continues to emphasize three fields of research - geoscience, astrophysics, and high-pressure physics - each administered by a corresponding IGPP Research Center. Each Research Center coordinates the mini-grant work in its field, and also works with the appropriate LLNL programs and departments, which frequently can provide supplementary funding and facilities for IGPP projects. 62 refs., 18 figs., 2 tabs.

Max, C.E. (ed.)

1987-07-01T23:59:59.000Z

8

Institute of Geophysics and Planetary Physics (IGPP), Lawrence Livermore National Laboratory (LLNL): Quinquennial report, November 14-15, 1996  

SciTech Connect

This Quinquennial Review Report of the Lawrence Livermore National Laboratory (LLNL) branch of the Institute for Geophysics and Planetary Physics (IGPP) provides an overview of IGPP-LLNL, its mission, and research highlights of current scientific activities. This report also presents an overview of the University Collaborative Research Program (UCRP), a summary of the UCRP Fiscal Year 1997 proposal process and the project selection list, a funding summary for 1993-1996, seminars presented, and scientific publications. 2 figs., 3 tabs.

Tweed, J.

1996-10-01T23:59:59.000Z

9

Planetary Physics  

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

Planetary Physics Some of the most intriguing NIF experiments test the physics believed to determine the structures of planets down to their cores, both in our solar system and...

10

Physics and Astronomy Geophysics Concentration  

E-Print Network (OSTI)

Physics and Astronomy Geophysics Concentration Strongly recommended courses Credits Term Dept. to Geophysics 3 PHY 3230 Thermal Physics 3 CHE 1101 Introductory Chemistry - I 3 CHE 1110 Introductory Chemistry Laboratory - I 1 GLY 1101 Intro. to Physical Geology 4 GLY 2250 Evolution of the Earth 4 GLY 4705 Adv

Thaxton, Christopher S.

11

Institute of geophysics and planetary physics  

SciTech Connect

This report contains brief discussions on topics of high-pressure sciences, astrophysics, and geosciences. (LSP)

Ryerson, F.; Budwine, C.M. (eds.)

1991-05-10T23:59:59.000Z

12

Geophysics  

Science Journals Connector (OSTI)

... illustration of its phenomena is rarely possible. The inclusion of this book in a handbook of experimental ... of experimental physics is therefore slightly anomalous, but the volume is none the less welcome. Geophysics is ...

1929-05-18T23:59:59.000Z

13

Institute of Geophyics and Planetary Physics. Annual report for FY 1994  

SciTech Connect

The Institute of Geophysics and Planetary Physics (IGPP) is a Multicampus Research Unit of the University of California (UC). IGPP was founded in 1946 at UC Los Angeles with a charter to further research in the earth and planetary sciences and in related fields. The Institute now has branches at UC campuses in Los Angeles, San Diego, Riverside, and Irvine and at Los Alamos and Lawrence Livermore national laboratories. The University-wide IGPP has played an important role in establishing interdisciplinary research in the earth and planetary sciences. For example, IGPP was instrumental in founding the fields of physical oceanography and space physics, which at the time fell between the cracks of established university departments. Because of its multicampus orientation, IGPP has sponsored important interinstitutional consortia in the earth and planetary sciences. Each of the six branches has a somewhat different intellectual emphasis as a result of the interplay between strengths of campus departments and Laboratory programs. The IGPP branch at Lawrence Livermore National Laboratory (LLNL) was approved by the Regents of the University of California in 1982. IGPP-LLNL emphasizes research in seismology, geochemistry, cosmochemistry, high-pressure sciences, and astrophysics. It provides a venue for studying the fundamental aspects of these fields, thereby complementing LLNL programs that pursue applications of these disciplines in national security and energy research. IGPP-LLNL is directed by Charles Alcock and is structured around three research centers. The Center for Geosciences, headed by George Zandt and Frederick Ryerson, focuses on research in geophysics and geochemistry. The Center for High-Pressure Sciences, headed by William Nellis, sponsors research on the properties of planetary materials and on the synthesis and preparation of new materials using high-pressure processing.

Ryerson, F.J. [ed.

1995-09-29T23:59:59.000Z

14

Planetary, Atmospheric, and Environmental Applications of Physics Frank Mills  

E-Print Network (OSTI)

solar energy production Evaluating, forecasting, and managing suburb-scale distributed solar electricity of clouds on the production of solar energy. Most of my research is done in collaboration with other groups production My research applies physics to a range of problems in planetary, atmospheric, and environmental

Chen, Ying

15

Z .Physics of the Earth and Planetary Interiors 119 2000 2536 www.elsevier.comrlocaterpepi  

E-Print Network (OSTI)

Z .Physics of the Earth and Planetary Interiors 119 2000 25­36 www a Department of Earth and Planetary Physics, Faculty of Science, Tokyo Uni?ersity, Hongo 7-3-1, Bunkyo algorithms, Phys. Earth Planet. Inter., this issue . q 2000 Elsevier Science B.V. All rights reserved

Geller, Robert

16

Role of borehole geophysics in defining the physical characteristics of the  

Open Energy Info (EERE)

Role of borehole geophysics in defining the physical characteristics of the Role of borehole geophysics in defining the physical characteristics of the Raft River geothermal reservoir, Idaho Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: Role of borehole geophysics in defining the physical characteristics of the Raft River geothermal reservoir, Idaho Details Activities (4) Areas (1) Regions (0) Abstract: Numerous geophysical logs have been made in three deep wells and in several intermediate depth core holes in the Raft River geothermal reservoir, Idaho. Laboratory analyses of cores from the intermediate depth holes were used to provide a qualitative and quantitative basis for a detailed interpretation of logs from the shallow part of the reservoir. A less detailed interpretation of logs from the deeper part of the reservoir

17

Internal geophysics (Physics of Earth's interior) Jump conditions and dynamic surface tension at permeable  

E-Print Network (OSTI)

Internal geophysics (Physics of Earth's interior) Jump conditions and dynamic surface tension of momentum across the interface, a possibly anisotropic surface tension and terms including an inter- face equals the jump of pressure; and in the presence of surface tension defined as a capillary action due

18

Z .Physics of the Earth and Planetary Interiors 117 2000 111121 www.elsevier.comrlocaterpepi  

E-Print Network (OSTI)

Z .Physics of the Earth and Planetary Interiors 117 2000 111­121 www rotation rate of the outer core fluid. Modulations in the rotation rate are produced as the inner core passes through successive gravitational wells. These modulations occur over roughly 90 year timescales

19

Physics of Atmospheres and Oceans: Class Question Sheets COMPARATIVE PLANETARY ATMOSPHERES  

E-Print Network (OSTI)

is the mass of Jupiter and R its radius. Assuming this is all converted to thermal energy, give a crudePhysics of Atmospheres and Oceans: Class Question Sheets COMPARATIVE PLANETARY ATMOSPHERES PLA.1 for discounting the less popular of these? Show that the energy liberated during the collapse of a sphere of mass

Read, Peter L.

20

Institute of Geophysics and Planetary Physics, 1992. Annual report, October 1, 1991--September 30, 1992  

SciTech Connect

This report contains brief discussions on topics in the following areas: High-pressure sciences; astrophysics; and geosciences.

Ryerson, F.J.; Budwine, C.M. [eds.

1993-06-14T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Space Plasma Physics  

Science Journals Connector (OSTI)

...W.D., BEAM-PLASMA DISCHARGE - BUILDUP...DURING ELECTRON BEAM-PLASMA INTERACTIONS, GEOPHYSICAL...ELECTRON-BEAM IN THE ATMOSPHERE, PLANETARY AND SPACE...1980 ). Space plasma physics: electron...regula' occurred at large pitch angles. Note...in quite different areas. (i) There is...

KLAUS WILHELM; WOLFGANG STDEMANN; WILLIBALD RIEDLER

1984-07-13T23:59:59.000Z

22

Emission line profiles as a probe of physical conditions in planetary nebulae  

E-Print Network (OSTI)

We present an analysis of physical conditions in planetary nebulae (PNe) in terms of collisionally-excited line (CEL) and optical-recombination line (ORL) profiles. We aim to investigate whether line profiles could be used to study the long-standing CEL/ORL abundance-discrepancy problem in nebular astrophysics. Using 1D photoionization models and their assumed velocity fields, we simulate the line profiles of various ionic species. We attempt to use our model to account for the observed CEL and ORL profiles. As a case study we present a detailed study of line profiles of the low-excitation planetary nebula (PN) IC 418. Our results show that the profiles of classical temperature and density diagnostic lines, such as [O III] 4363,5007, [S II] 6716,6731, and [Ar IV] 4711,4740, provide a powerful tool to study nebular temperature and density variations. The method enables the CEL/ORL abundance-discrepancy problem to be studied more rigorously than before. A pure photoionization model of a chemically-homogeneous nebula seems to explain the observed disagreements in the profiles for the [O III] 4363 and the 5007 lines, but cannot account for the differences between the [O III] CELs and the O II ORLs. We also investigate the temperature and density variations in the velocity space of a sample of PNe, which are found to be insignificant.

Yong Zhang

2008-05-15T23:59:59.000Z

23

Physics of the Earth and Planetary Interiors xxx (2004) xxxxxx High pressure crystal chemistry of hydrous ringwoodite  

E-Print Network (OSTI)

Physics of the Earth and Planetary Interiors xxx (2004) xxx­xxx High pressure crystal chemistry of hydrous ringwoodite and water in the Earth's interior Joseph R. Smytha,, Christopher M. Holla, Daniel J November 2002; received in revised form 12 May 2003; accepted 18 August 2003 Abstract The crystal chemistry

Smyth, Joseph R.

24

Physics of the Earth and Planetary Interiors 143144 (2004) 271278 High pressure crystal chemistry of hydrous ringwoodite  

E-Print Network (OSTI)

Physics of the Earth and Planetary Interiors 143­144 (2004) 271­278 High pressure crystal chemistry of hydrous ringwoodite and water in the Earth's interior Joseph R. Smytha,, Christopher M. Holla, Daniel J November 2002; received in revised form 12 May 2003; accepted 18 August 2003 Abstract The crystal chemistry

Jacobsen, Steven D.

25

Physics of the Earth and Planetary Interiors 176 (2009) 143156 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

's dynamic system. In this paper we review recent progresses in relevant fields and suggest that the EarthDirect Physics of the Earth and Planetary Interiors journal homepage: www.elsevier.com/locate/pepi Review has illustrated convincingly the whole-mantle nature of mantle convection, and the lower mantle origin

Zhong, Shijie

26

Physics of the Earth and Planetary Interiors 153 (2005) 12 Studies of the Earth's Deep Interior--Eighth Symposium  

E-Print Network (OSTI)

Physics of the Earth and Planetary Interiors 153 (2005) 1­2 Editorial Studies of the Earth's Deep Interior--Eighth Symposium The Eighth Symposium on the Study of the Earth's Deep Interior (SEDI) was held. On this occasion attention was also turned to the deep interior of other planets as well as the Earth. To decipher

Garnero, Ed

27

Physics of the Earth and Planetary Interiors 133 (2002) 127146 Palaeomagnetic study of Oligocene (2430 Ma) lava flows from  

E-Print Network (OSTI)

Physics of the Earth and Planetary Interiors 133 (2002) 127­146 Palaeomagnetic study of Oligocene previously obtained radiometric dates to correlate the sections [J. Petrol. 39 (4) (1998) 711; Earth Planet the composi- tion and dynamics of the Earth's core directly, one indirect method is to study the Earth

Demouchy, Sylvie

28

Physical properties of the WASP-67 planetary system from multi-colour photometry  

E-Print Network (OSTI)

The extrasolar planet WASP-67 b is the first hot Jupiter definitively known to undergo only partial eclipses. The lack of the second and third contact point in this planetary system makes it difficult to obtain accurate measurements of its physical parameters. Aims. By using new high-precision photometric data, we confirm that WASP-67 b shows grazing eclipses and compute accurate estimates of the physical properties of the planet and its parent star. Methods. We present high-quality, multi-colour, broad-band photometric observations comprising five light curves covering two transit events, obtained using two medium-class telescopes and the telescope-defocussing technique. One transit was observed through a Bessel-R filter and the other simultaneously through filters similar to Sloan griz. We modelled these data using jktebop. The physical parameters of the system were obtained from the analysis of these light curves and from published spectroscopic measurements. Results. All five of our light curves satisfy t...

Mancini, L; Ciceri, S; Novati, S Calchi; Dominik, M; Henning, Th; Jorgensen, U G; Korhonen, H; Nikolov, N; Alsubai, K A; Bozza, V; Bramich, D M; D'Ago, G; Jaimes, R Figuera; Galianni, P; Gu, S -H; Harpsoe, K; Hinse, T C; Hundertmark, M; Juncher, D; Kains, N; Popovas, A; Rabus, M; Rahvar, S; Skottfelt, J; Snodgrass, C; Street, R; Surdej, J; Tsapras, Y; Vilela, C; Wang, X -B; Wertz, O

2014-01-01T23:59:59.000Z

29

Geophysical Techniques | Open Energy Information  

Open Energy Info (EERE)

Geophysical Techniques Geophysical Techniques Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Technique: Geophysical Techniques Details Activities (2) Areas (1) Regions (0) NEPA(4) Exploration Technique Information Exploration Group: Geophysical Techniques Exploration Sub Group: None Parent Exploration Technique: Exploration Techniques Information Provided by Technique Lithology: may be inferred Stratigraphic/Structural: may be inferred Hydrological: may be inferred Thermal: may be inferred Dictionary.png Geophysical Techniques: Geophysics is the study of the structure and composition of the earth's interior. Other definitions:Wikipedia Reegle Introduction Geophysical techniques measure physical phenomena of the earth such as gravity, magnetism, elastic waves, electrical and electromagnetic waves.

30

Geophysical Methods | Open Energy Information  

Open Energy Info (EERE)

Geophysical Methods Geophysical Methods Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Technique: Geophysical Methods Details Activities (0) Areas (0) Regions (0) NEPA(1) Exploration Technique Information Exploration Group: Geophysical Techniques Exploration Sub Group: Geophysical Techniques Parent Exploration Technique: Information Provided by Technique Lithology: Stratigraphic/Structural: Hydrological: Thermal: Dictionary.png Geophysical Methods: Methods used to measure the physical properties of the earth Other definitions:Wikipedia Reegle Introduction There are five main types of geophysical methods used for geothermal resource discovery: Seismic Methods (active and passive) Electrical Methods Magnetic Methods Gravity Methods Radiometric Methods Seismic methods dominates oil and gas exploration, and probably accounts

31

Research overview 2009 Department of Geophysics, belonging to the Faculty of Mathematics and Physics,  

E-Print Network (OSTI)

also planetary aspects. Research is tightly coupled with education at the bachelor, master and doctoral microearthquakes induced by drilling for oil. Preparations were also carried to join one new European project

Cerveny, Vlastislav

32

Research overview 2008 Department of Geophysics, belonging to the Faculty of Mathematics and Physics,  

E-Print Network (OSTI)

also planetary aspects. Research is tightly coupled with education at the bachelor, master and doctoral microearthquakes induced by drilling for oil. We were invited to join also three new European project proposals

Cerveny, Vlastislav

33

Definition: Geophysical Techniques | Open Energy Information  

Open Energy Info (EERE)

Definition Definition Edit with form History Facebook icon Twitter icon » Definition: Geophysical Techniques Jump to: navigation, search Dictionary.png Geophysical Techniques Geophysics is the study of the structure and composition of the earth's interior.[1] View on Wikipedia Wikipedia Definition Exploration geophysics is the applied branch of geophysics which uses surface methods to measure the physical properties of the subsurface Earth, along with the anomalies in these properties, in order to detect or infer the presence and position of ore minerals, hydrocarbons, geothermal reservoirs, groundwater reservoirs, and other geological structures. Exploration geophysics is the practical application of physical methods (such as seismic, gravitational, magnetic, electrical and electromagnetic)

34

PHYSICAL STRUCTURE OF THE PLANETARY NEBULA NGC 3242 FROM THE HOT BUBBLE TO THE NEBULAR ENVELOPE  

SciTech Connect

One key feature of the interacting stellar winds model of the formation of planetary nebulae (PNe) is the presence of shock-heated stellar wind confined in the central cavities of PNe. This so-called hot bubble should be detectable in X-rays. Here we present XMM-Newton observations of NGC 3242, a multiple-shell PN whose shell morphology is consistent with the interacting stellar winds model. Diffuse X-ray emission is detected within its inner shell with a plasma temperature of {approx}2.35 x 10{sup 6} K and an intrinsic X-ray luminosity of {approx}2 x 10{sup 30} erg s{sup -1} at the adopted distance of 0.55 kpc. The observed X-ray temperature and luminosity are in agreement with 'ad hoc' predictions of models including heat conduction. However, the chemical abundances of the X-ray-emitting plasma seem to imply little evaporation of cold material into the hot bubble, whereas the thermal pressure of the hot gas is unlikely to drive the nebular expansion as it is lower than that of the inner shell rim. These inconsistencies are compounded by the apparent large filling factor of the hot gas within the central cavity of NGC 3242.

Ruiz, Nieves; Guerrero, MartIn A. [Instituto de Astrofisica de Andalucia, CSIC, Granada 18008 (Spain); Chu, You-Hua; Gruendl, Robert A., E-mail: nieves@iaa.es, E-mail: mar@iaa.es, E-mail: yhchu@astro.illinois.edu, E-mail: gruendl@astro.illinois.edu [Astronomy Department, University of Illinois at Urbana-Champaign, Urbana, IL 61801 (United States)

2011-09-15T23:59:59.000Z

35

Future gravitational physics tests from ranging to the BepiColombo Mercury planetary orbiter  

SciTech Connect

Milani et al. recently have published careful and fundamental studies of the accuracy with which both gravitational physics information and the solar quadrupole moment can be obtained from Earth-Mercury distance data. To complement these results, a quite different analysis method is used in the present paper. We calculate the first-order corrections to the Keplerian motion of a single planet around the Sun due to the parameterized post-Newtonian theory parameters {beta}, {gamma}, {alpha}{sub 1}, {alpha}{sub 2}, and {xi}, as well as corrections due to the solar quadrupole moment J{sub 2} and a possible secular change in GM{sub {center_dot}}. The Nordtvedt parameter {eta} that is used in tests of the strong equivalence principle also is included in this analysis. The expected accuracies are given for 1 yr, 2 yr, and 8 yr mission durations, assuming that the planet-planet and asteroid-planet perturbations are accurately known. The ''modified worst-case'' error analysis method that we use is quite different from the usual covariance analysis method based on assumed uncorrelated random errors, plus a bias that is fixed or that changes in a prescribed way. We believe this is appropriate because systematic measurement errors are likely to be the main limitation on the accuracy of the results. Our final estimated uncertainties are one-third of the errors that would result if a 4.5-cm rms systematic error had the most damaging possible variation with time. We discuss the resulting uncertainties for several different subsets of orbital and relativity parameters.

Ashby, Neil; Bender, Peter L.; Wahr, John M. [Department of Physics, University of Colorado, Boulder, Colorado 80309-0390 (United States); JILA, University of Colorado, Boulder, Colorado 80309-0440 (United States) and National Institute of Science and Technology, Boulder, Colorado 80309-0440 (United States); Department of Physics, University of Colorado, Boulder, Colorado 80309-0390 (United States)

2007-01-15T23:59:59.000Z

36

Variability of geophysical log data and the signature of crustal heterogeneities at the KTB  

Science Journals Connector (OSTI)

......variations in geophysical borehole data reflect geological...Continental Deep Drilling Program (KTB...heterogeneities. borehole geophysics|crustal...Introduction The large-scale structure...several geo-physical borehole data from the German Continental Deep Drilling Program (KTB......

Sabrina Leonardi; Hans-Joachim Kmpel

1998-12-01T23:59:59.000Z

37

Does the Sun work as a nuclear fusion amplifier of planetary tidal forcing? A proposal for a physical mechanism based on the mass-luminosity relation  

E-Print Network (OSTI)

Empirical evidences show that planetary tides may influence solar activity: 1) the 11-yr Schwabe sunspot number cycle is constrained between the spring tidal period of Jupiter and Saturn, 9.93 yr, and the tidal orbital period of Jupiter, 11.86 yr, and a model based on these cycles reconstructs solar dynamics at multiple time ; 2) a measure of the alignment of Venus, Earth and Jupiter reveals quasi 11.07-yr cycles well correlated to the 11-year Schwabe solar cycles; 3) there exists a 11.08 yr cyclical recurrence in the solar jerk-shock vector, which is induced mostly by Mercury and Venus. However, Newtonian classical physics fails to explain the phenomenon. Only by means of a significant nuclear fusion amplification of the tidal gravitational potential energy released in the Sun, may planetary tides produce irradiance output oscillations with a sufficient magnitude to influence solar dynamo processes. Here we use an adaptation of the well-known mass-luminosity relation to calculate a conversion factor between ...

Scafetta, Nicola

2012-01-01T23:59:59.000Z

38

Asteroseismic determination of the physical characteristics of the planetary system host HR\\,8799 ($\\lambda$ Bootis nature and age)  

E-Print Network (OSTI)

HR\\,8799 is a $\\lambda$ Bootis, $\\gamma$ Doradus star hosting a planetary system and a debris disk with two rings. This makes this system a very interesting target for asteroseismic studies. In particular, this work is devoted to the determination of the internal metallicity of this star, linked with its $\\lambda$ Bootis nature, and its age, taking the advantage of its $\\gamma$ Doradus-type pulsations. To do so we have used the equilibrium code CESAM and the non-adiabatic pulsational code GraCo. We have applied the Frequency Ratio Method and the Time Dependent Convection theory to estimate the mode identification, the Brunt-Va\\"is\\"al\\"a frequency integral and the mode instability, making a selection of the possible models fulfilling all observational constraints. Using the position of the star in the HR diagram, the solar metallicity models is discarded. This result contradicts one of the main assumptions of the most accepted hypothesis explaining the $\\lambda$ Bootis nature, the accretion/diffusion of gas f...

Moya, A; Barrado, D; Hernndez, A Garc\\'\\ia; Aberasturi, M; Montesinos, B; Aceituno, F

2010-01-01T23:59:59.000Z

39

Fiber optic geophysical sensors  

DOE Patents (OSTI)

A fiber optic geophysical sensor in which laser light is passed through a sensor interferometer in contact with a geophysical event, and a reference interferometer not in contact with the geophysical event but in the same general environment as the sensor interferometer. In one embodiment, a single tunable laser provides the laser light. In another embodiment, separate tunable lasers are used for the sensor and reference interferometers. The invention can find such uses as monitoring for earthquakes, and the weighing of objects.

Homuth, Emil F. (Los Alamos, NM)

1991-01-01T23:59:59.000Z

40

LANL | Solid Earth Geophysics | EES-17  

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

LANL : Earth & Environmental Sciences : Solid Earth Geophysics (EES-17) LANL : Earth & Environmental Sciences : Solid Earth Geophysics (EES-17) Home Publications Collaboration & Links Staff Research Highlights Ground-Based Nuclear Explosion Monitoring Geodynamics & National Security Nonlinear Elasticity Time Reversal Los Alamos Seismic Network Stimulated Porous Fluid Flow Resource Recovery Seismic & Acoustic Imaging Exploration Geophysics Induced Seismicity Volcanoes & Earthquakes Other Research CONTACTS Group Leader Ken Rehfeldt Administrative Contacts Jody Benson Cecilia Gonzales Geophysics (EES-17) The Geophysics Group supports the national security mission of Los Alamos National Laboratory by providing technical expertise to monitor movement of Earth's crust while predicting the effects of these events on the environment. Though our focus is on seismic monitoring, we also apply electric, magnetic, radionuclide, and acoustic technologies to monitor underground explosions, maintain our ability to conduct tests, and develop the Yucca Mountain Project. In addition, we study the nonlinear properties of earth materials, imaging with seismic waves, how seismic waves affect the interaction of porous rocks and fluids, use of seismic waves to characterize underground oil reservoirs, volcanology and volcanic seismicity, advanced computational physics of earth materials, and using drilling technology to study the crust of the earth. These tasks are complemented by our extensive background in both conventional and hot dry rock geothermal energy development and geophysical support of the Nevada Test Site.

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Cluster Dynamics of Planetary Waves  

E-Print Network (OSTI)

The dynamics of nonlinear atmospheric planetary waves is determined by a small number of independent wave clusters consisting of a few connected resonant triads. We classified the different types of connections between neighboring triads that determine the general dynamics of a cluster. Each connection type corresponds to substantially different scenarios of energy flux among the modes. The general approach can be applied directly to various mesoscopic systems with 3-mode interactions, encountered in hydrodynamics, astronomy, plasma physics, chemistry, medicine, etc.

Elena Kartashova; Victor S. L'vov

2008-11-05T23:59:59.000Z

42

An introduction to electrical resistivity in geophysics | Open Energy  

Open Energy Info (EERE)

An introduction to electrical resistivity in geophysics An introduction to electrical resistivity in geophysics Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: An introduction to electrical resistivity in geophysics Abstract Physicists are finding that the skills they have learned in their training may be applied to areas beyond traditional physics topics. One such field is that of geophysics. This paper presents the electrical resistivity component of an undergraduate geophysics course at Radford University. It is taught from a physics perspective, yet the application of the theory to the real world is the overriding goal. The concepts involved in electrical resistivity studies are first discussed in a general sense, and then they are studied through the application of the relevant electromagnetic theory.

43

Fiber optic geophysical sensors  

DOE Patents (OSTI)

A fiber optic geophysical sensor is described in which laser light is passed through a sensor interferometer in contact with a geophysical event, and a reference interferometer not in contact with the geophysical event but in the same general environment as the sensor interferometer. In one embodiment, a single tunable laser provides the laser light. In another embodiment, separate tunable lasers are used for the sensor and reference interferometers. The invention can find such uses as monitoring for earthquakes, and the weighing of objects. 2 figures.

Homuth, E.F.

1991-03-19T23:59:59.000Z

44

Geophysics and the Internet  

Science Journals Connector (OSTI)

...Article Special Section: New technology/vendor spotlight Geophysics...com Mercury International Technology, Tulsa, Oklahoma, U.S...highlights to the company intranet, and stockholders can get...However, Mercury International Technology is betting that that there...

Ralph Gobeli

45

Earth and Planetary Science Letters 381 (2013) 127137 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

Direct Earth and Planetary Science Letters www.elsevier.com/locate/epsl Frictional strength and wear-rate of carbonate faults during high-velocity, steady-state sliding Yuval Boneh a,1 , Amir Sagy b , Ze'ev Reches a, a School of Geology and Geophysics, University of Oklahoma, Norman, OK 73019, United States b Geological

Ze'ev, Reches

46

Classification of planetary nebulae by their departure from axisymmetry  

Science Journals Connector (OSTI)

......ac.il Department of Physics, University of Haifa at Oranim, Oranim, Tivon 36006, Israel Permanent address: West Valley High School, Kibbutz Yifat, 30069, Israel. We propose a scheme to classify planetary nebulae (PNe) according to......

Noam Soker; Ron Hadar

2002-04-01T23:59:59.000Z

47

COLLOQUIUM: The NASA Planetary Science Program | Princeton Plasma...  

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

February 25, 2015, 4:00pm to 6:30pm Colloquia MBG Auditorium COLLOQUIUM: The NASA Planetary Science Program Dr. James Green NASA Colloquium Committee: The Princeton Plasma Physics...

48

Planetary science comes to Nantes  

Science Journals Connector (OSTI)

......research-article Features Planetary science comes to Nantes Meeting...the European Planetary Science Congress (EPSC) and...Secretary Media, Policy, Education Outreach for the RAS...centre of planetary science in the first week of...around 650 talks and 850 posters on planetary bodies......

Robert Massey

2011-12-01T23:59:59.000Z

49

ESTIMATING UNCERTAINTIES FOR GEOPHYSICAL  

E-Print Network (OSTI)

to directly measure the amount of oil in an area is to drill several wells, but drilling is a very expensive procedure, and the whole idea of geophysics is to predict the amount of oil without drilling in all possible are: to locate minerals (oil, gas, fresh and saline water, etc); to locate and predict earthquakes

Kreinovich, Vladik

50

Near-surface geophysics:  

Science Journals Connector (OSTI)

...plants, chemical plants, refineries, and waste-disposal...vulnerable to noise from power lines, pipelines, electrical...the variations in the electric field. Among these is...GPS-determined locations, demands information about soil...Schlumberger and Wenner sounding curves by Zohdy (Geophysics...

Don W. Steeples

51

GEOPHYSICS, VOL. 66, NO. 3 (MAY-JUNE 2001); P. 904910, 7 FIGS., 3 TABLES. Velocity analysis for tilted transversely isotropic media: A physical  

E-Print Network (OSTI)

in conventional imaging, it is important to be able to recon- struct the velocity model suitable for anisotropic depth migration. Here, we discuss the results of anisotropic pa- rameter estimation on a physical and the anisotropic parameters and . The coefficient is obtained using the travel- times of a wave that crosses

Tsvankin, Ilya

52

Planetary radar astronomy  

Science Journals Connector (OSTI)

Radar is a powerful technique that has furnished otherwise unavailable information about solar system bodies for three decades. The advantages of radar in planetary astronomy result from (1) the observer's control of all the attributes of the coherent signal used to illuminate the target, especially the wave form's time/frequency modulation and polarization; (2) the ability of radar to resolve objects spatially via measurements of the distribution of echo power in time delay and Doppler frequency; (3) the pronounced degree to which delay-Doppler measurements constrain orbits and spin vectors; and (4) centimeter-to-meter wavelengths, which easily penetrate optically opaque planetary clouds and cometary comae, permit investigation of near-surface macrostructure and bulk density, and are sensitive to high concentrations of metal or, in certain situations, ice. Planetary radar astronomy has primarily involved observations with Earth-based radar telescopes, but also includes some experiments with a spaceborne transmitter or receiver. In addition to providing a wealth of information about the geological and dynamical properties of asteroids, comets, the inner planets, and natural satellites, radar experiments have established the scale of the solar system, have contributed significantly to the accuracy of planetary ephemerides, and have helped to constrain theories of gravitation. This review outlines radar astronomical techniques and describes principal observational results.

Steven J. Ostro

1993-10-01T23:59:59.000Z

53

Planetary Magnetospheric Philippe Zarka  

E-Print Network (OSTI)

, philippe.zarka@obspm.fr Rencontres de Blois - 2006 · Solar Wind / Solar Wind - Obstacle interaction = magnetosphere MP = magnetopause B = magnetic field · Solar Wind / Solar Wind - Obstacle interaction · Planetary Wind - dominated by bulk energy density : NmV2/2 - carries away solar B rooted in the Sun ! ballerina

Demoulin, Pascal

54

Planetary Nebulae Detection  

E-Print Network (OSTI)

layers develop deep convective zone, surface expands, mass loss due to stellar wind · Star moves from tip1 Planetary Nebulae · Detection · Distribution in the Galaxy · Central Stars · Evolution · Bipolar to dust) · Difficult to detect in radio (fainter than H II regions) · Projected number based on surveys

Crenshaw, Michael

55

Astronomy, geophysics and the media  

Science Journals Connector (OSTI)

......August-September 1997 research-article Features Astronomy, geophysics and the media Jacqueline...message from the RAS Discussion Meeting on Astronomy and Geophysics in the Media, held on...She is often asked why there are so few astronomy documentaries. It's not for want of......

Jacqueline Mitton; Peter Bond

1997-01-01T23:59:59.000Z

56

Physics  

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

Physics Physics1354608000000PhysicsSome of these resources are LANL-only and will require Remote Access.No Physics Some of these resources are LANL-only and will require Remote...

57

Computational physical oceanography -- A comprehensive approach based on generalized CFD/grid techniques for planetary scale simulations of oceanic flows. Final report, September 1, 1995--August 31, 1996  

SciTech Connect

The original intention for this work was to impart the technology that was developed in the field of computational aeronautics to the field of computational physical oceanography. This technology transfer involved grid generation techniques and solution procedures to solve the governing equations over the grids thus generated. Specifically, boundary fitting non-orthogonal grids would be generated over a sphere taking into account the topography of the ocean floor and the topography of the continents. The solution methodology to be employed involved the application of an upwind, finite volume discretization procedure that uses higher order numerical fluxes at the cell faces to discretize the governing equations and an implicit Newton relaxation technique to solve the discretized equations. This report summarizes the efforts put forth during the past three years to achieve these goals and indicates the future direction of this work as it is still an ongoing effort.

Beddhu, M.; Jiang, M.Y.; Whitfield, D.L.; Taylor, L.K.; Arabshahi, A.

1997-02-20T23:59:59.000Z

58

Numerical Simulation in Applied Geophysics. From the Mesoscale to ...  

E-Print Network (OSTI)

Instituto del Gas y del Petroleo, Facultad de Ingenier?a UBA. ,. Facultad de ... hydrocarbon exploration geophysics, mining and reservoir characterization and production. Local variations in the fluid ... physical process of wave propagation can be inspected during the experiment. ..... Black-Oil simulator. CO2 saturation...

2013-07-05T23:59:59.000Z

59

Available Energy of Geophysical Systems  

Science Journals Connector (OSTI)

An alternative derivation of the available energy for a geophysical fluid system is presented. It is shown that determination of the equilibrium temperature of the system by the minimization of an energy availability function is equivalent to that ...

Peter R. Bannon

2013-08-01T23:59:59.000Z

60

Laboratory Measurement of Geophysical Properties for Monitoring of CO2 Sequestration  

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

Laboratory Measurement of Geophysical Properties for Monitoring of Laboratory Measurement of Geophysical Properties for Monitoring of CO 2 Sequestration Larry R. Myer (LRMyer@lbl.gov; 510/486-6456) Lawrence Berkeley National Laboratory Earth Science Division One Cyclotron Road, MS 90-1116 Berkeley, CA 94720 Introduction Geophysical techniques will be used in monitoring of geologic sequestration projects. Seismic and electrical geophysical techniques will be used to map the movement of CO 2 in the subsurface and to establish that the storage volume is being efficiently utilized and the CO 2 is being safely contained within a known region. Rock physics measurements are required for interpretation of the geophysical surveys. Seismic surveys map the subsurface velocities and attenuation while electrical surveys map the conductivity. Laboratory measurements are required to convert field

Note: This page contains sample records for the topic "geophysics planetary physics" 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

GEOPHYSICAL RESEARCH LETTERS, VOL. 28, NO. 18, PAGES 3545-3548, SEPTEMBER 15, 2001 A method for estimating 2D wrinkle ridge strain  

E-Print Network (OSTI)

on the central Columbia Plateau are a succession of thrusted anticlines thought to be analogs of planetary in the inner Solar Sys- tem [e.g., Watters, 1988], and the conclusion that developing a method for estimating Copyright 2001 by the American Geophysical Union. Paper number 2001GL012934. 0094-8276/01/2001GL012934

Mege, Daniel

62

Physics  

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

Physics Physics Physics Print Because a large proportion of ALS experiments are "physics" experiments, it's useful to separate them into two categories - one focused on Materials/Condensed Matter, and this one, with a dual focus on AMO (atomic, molecular, and optical) physics and accelerator physics. Light sources such as the ALS have opened up research frontiers that may hold the answers to fundamental questions about structure and dynamics in AMO physics. The advanced spectroscopies that have been developed here provide the ability to control and probe atomic and molecular processes with unprecedented precision. In particular, the spectral resolution, brightness, broad tunability, and polarization control generate novel avenues for the study of tailored states, inner-shell processes, and nonperturbative electron interactions. Driven by the high brightness of the ALS, a whole new world of vacuum ultraviolet (VUV) and soft x-ray physics has emerged through the development of combined techniques to excite, select, and probe atoms, molecules, and clusters.

63

Physics  

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

Physics Print Physics Print Because a large proportion of ALS experiments are "physics" experiments, it's useful to separate them into two categories - one focused on Materials/Condensed Matter, and this one, with a dual focus on AMO (atomic, molecular, and optical) physics and accelerator physics. Light sources such as the ALS have opened up research frontiers that may hold the answers to fundamental questions about structure and dynamics in AMO physics. The advanced spectroscopies that have been developed here provide the ability to control and probe atomic and molecular processes with unprecedented precision. In particular, the spectral resolution, brightness, broad tunability, and polarization control generate novel avenues for the study of tailored states, inner-shell processes, and nonperturbative electron interactions. Driven by the high brightness of the ALS, a whole new world of vacuum ultraviolet (VUV) and soft x-ray physics has emerged through the development of combined techniques to excite, select, and probe atoms, molecules, and clusters.

64

Identifying Chemicals That Are Planetary Boundary Threats  

Science Journals Connector (OSTI)

Identifying Chemicals That Are Planetary Boundary Threats ... Our point of departure to develop profiles for chemicals that are potential planetary boundary threats is to identify scenarios in which a chemical could fulfill each of the three conditions for being a planetary boundary threat. ... Note that chemicals named as examples do not necessarily represent planetary boundary threats since at least one scenario from each of the three conditions must be fulfilled for a chemical to pose a planetary boundary threat. ...

Matthew MacLeod; Magnus Breitholtz; Ian T. Cousins; Cynthia A. de Wit; Linn M. Persson; Christina Rudn; Michael S. McLachlan

2014-09-02T23:59:59.000Z

65

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

66

Planetary Microlensing Perturbations: True Planets or Binary Sources?  

E-Print Network (OSTI)

A planetary microlensing event is characterized by a short-lived perturbation to the standard Paczy\\'nski curve. Planetary perturbations typically last from a few hours to a day, and have maximum amplitudes, $\\dmax$, of $5-20%$ of the standard curve. There exist a subset of binary-source events that can reproduce these main features, and thus masquerade as planetary events. These events require a binary source with a small flux ratio, $\\epsil \\sim 10^{-2}-10^{-4}$, and a small impact parameter for the fainter source, $\\beta_2 \\lsim \\epsil / \\dmax$. The detection probability of events of this type is $\\sim \\beta_2$, and can be as high as $\\sim 30%$; this is comparable to planetary detection rates. Thus a sample of planetary-like perturbations could be seriously contaminated by binary-source events, and there exists the possibility that completely meaningless physical parameters would be derived for any given perturbation. Here I derive analytic expressions for a binary-source event in the extreme flux ratio limit, and use these to demonstrate the basic degeneracy between binary source and planet perturbations. I describe how the degeneracy can be broken by dense and accurate sampling of the perturbation, optical/infrared photometry, or spectroscopic measurements.

B. Scott Gaudi

1997-06-26T23:59:59.000Z

67

UNIVERSITY COLLEGE LONDON Department of Physics and Astronomy  

E-Print Network (OSTI)

UNIVERSITY COLLEGE LONDON Department of Physics and Astronomy COURSE HANDBOOK MSc in Planetary Science Course Organiser: Nicholas Achilleos Session: 2012-2013 Planetary Science MSc at UCL/2012 Handbook 1Planetary Science MSc at UCL/2012 Handbook 1 #12;Dates of College Terms 2012-2013 First Term

Thompson, Samantha

68

Physics  

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

B C D E F G H I J K L M N O P Q R S T U V W X Y Z A'Hearn, Michael F. - Department of Astronomy, University of Maryland at College Park Aalberts, Daniel P. - Department of Physics,...

69

Geophysical Exploration (Montana) | Department of Energy  

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

Geophysical Exploration (Montana) Geophysical Exploration (Montana) Geophysical Exploration (Montana) < Back Eligibility Utility Fed. Government Commercial Investor-Owned Utility State/Provincial Govt Industrial Construction Municipal/Public Utility Local Government Installer/Contractor Rural Electric Cooperative Tribal Government Retail Supplier Institutional Fuel Distributor Savings Category Buying & Making Electricity Program Info State Montana Program Type Siting and Permitting Provider Montana Department of Natural Resources and Conservation An exploration permit is required for any entity conducting geophysical exploration within the state of Montana. Such entities are also required to follow rules adopted by the Board of Oil and Gas Conservation, including those pertaining to: (a) Adequate identification of seismic exploration crews operating in this

70

Leasing and Exploration * Seismic geophysical surveys  

E-Print Network (OSTI)

#12;Leasing and Exploration * Seismic geophysical surveys * Exploratory drilling using various.S. citizens engaged in a specific activity (other than commercial fishing) in a specified geographical region

71

Regional geophysics, Cenozoic tectonics and geologic resources...  

Open Energy Info (EERE)

and adjoining regions Jump to: navigation, search OpenEI Reference LibraryAdd to library Conference Proceedings: Regional geophysics, Cenozoic tectonics and geologic resources of...

72

Planetary formation theory developed, tested: predicts timeline for life  

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

Planetary formation theory developed, tested: predicts timeline for Planetary formation theory developed, tested: predicts timeline for life After the Big Bang: Theory suggests first planets formed after first generations of stars The researchers' calculations predict properties of first planet and timeline for life. May 3, 2012 image description The researchers state that the formation of Earth-like planets is not itself a sufficient prerequisite for life. Early galaxies contained strong sources of life-threatening radiation, such as supernovae and black holes. Therefore, they conclude that the conditions for life emerged only after the earliest epoch of galaxy formation. Get Expertise Jarrett Johnson Nuclear and Particle Physics, Astrophysics and Cosmology Email Hui Li Nuclear and Particle Physics, Astrophysics and Cosmology

73

A small RTG for future planetary missions  

SciTech Connect

A design study was conducted to characterize conceptual designs for a small Radioisotope Thermoelectric Generator (RTG), one that might be suitable for future planetary missions. Conceptual design configurations were derived from the General Purpose Heat Source{emdash}RTG (GPHS-RTG), with the design goal of providing 70 watts of electrical power at the end of a ten year mission life. Design improvements for mass minimization were evaluated, considering also the technical risk of the corresponding engineering development required. It was concluded that an RTG mass of 18 kg could be achieved with moderate risk. Further studies are recommended to define in detail the testing and other development activities that would be required to bring the conceptual design for such an RTG to reality. {copyright} {ital 1997 American Institute of Physics.}

Cockfield, R.D.; Kull, R.A. [Lockheed Martin Missiles Space P.O. Box 8555 Philadelphia, Pennsylvania19101 (United States)

1997-01-01T23:59:59.000Z

74

Geochemical and Geophysical Changes during Ammonia Gas Treatment...  

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

Geophysical Changes during Ammonia Gas Treatment of Vadose Zone Sediments for Uranium Remediation. Geochemical and Geophysical Changes during Ammonia Gas Treatment of Vadose Zone...

75

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource...  

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

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization Advanced...

76

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource...  

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

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization DOE...

77

Merging high resolution geophysical and geochemical surveys to...  

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

high resolution geophysical and geochemical surveys to reduce exploration risk at Glass Buttes, Oregon Merging high resolution geophysical and geochemical surveys to reduce...

78

Z .Global and Planetary Change 20 1999 93123 Global sea level rise and glacial isostatic adjustment  

E-Print Network (OSTI)

adjustment W.R. Peltier ) Department of Physics, Uni?ersity of Toronto, 60 St. George Street, Toronto-mail: peltier@atmosp.physics.utoronto.ca Z .rather recently Peltier and Tushingham, 1989 , it was not clearly;( )W.R. PeltierrGlobal and Planetary Change 20 1999 93­12394 Z .existed at that time e.g., Peltier

Peltier, W. Richard

79

Astronomy and geophysics in the secondary curriculum  

Science Journals Connector (OSTI)

......December 2006 research-article Education Astronomy and geophysics in the secondary curriculum...Committee, examines the ways in which astronomy and geophysics figure in secondary-school...Committee, Principal Moderator for GCSE Astronomy with Edexcel and Head of Science at Helena......

Julien King

2006-12-01T23:59:59.000Z

80

Geophysical muon imaging: feasibility and limits  

Science Journals Connector (OSTI)

......Gaussian with mean N and standard deviation N. However...interval is obtained through standard procedure and we have...made very constructive reviews of a former version of...2010. Muon tomography: plans for observations in the...measurements with application in mining geophysics, Geophysics......

N. Lesparre; D. Gibert; J. Marteau; Y. Dclais; D. Carbone; E. Galichet

2010-12-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Category:Geophysical Techniques | Open Energy Information  

Open Energy Info (EERE)

Techniques Techniques Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermalpower.jpg Looking for the Geophysical Techniques page? For detailed information on Geophysical Techniques as exploration techniques, click here. Category:Geophysical Techniques Add.png Add a new Geophysical Techniques Technique Subcategories This category has the following 4 subcategories, out of 4 total. E [+] Electrical Techniques‎ (2 categories) 5 pages G [×] Gravity Techniques‎ 3 pages M [×] Magnetic Techniques‎ 3 pages S [+] Seismic Techniques‎ (2 categories) 2 pages Pages in category "Geophysical Techniques" The following 5 pages are in this category, out of 5 total. D DC Resistivity Survey (Mise-Á-La-Masse) E Electrical Techniques G Gravity Techniques M Magnetic Techniques

82

SURFACE GEOPHYSICAL EXPLORATION - COMPENDIUM DOCUMENT  

SciTech Connect

This report documents the evolution of the surface geophysical exploration (SGE) program and highlights some of the most recent successes in imaging conductive targets related to past leaks within and around Hanford's tank farms. While it is noted that the SGE program consists of multiple geophysical techniques designed to (1) locate near surface infrastructure that may interfere with (2) subsurface plume mapping, the report will focus primarily on electrical resistivity acquisition and processing for plume mapping. Due to the interferences from the near surface piping network, tanks, fences, wells, etc., the results of the three-dimensional (3D) reconstruction of electrical resistivity was more representative of metal than the high ionic strength plumes. Since the first deployment, the focus of the SGE program has been to acquire and model the best electrical resistivity data that minimizes the influence of buried metal objects. Toward that goal, two significant advances have occurred: (1) using the infrastructure directly in the acquisition campaign and (2) placement of electrodes beneath the infrastructure. The direct use of infrastructure was successfully demonstrated at T farm by using wells as long electrodes (Rucker et al., 2010, 'Electrical-Resistivity Characterization of an Industrial Site Using Long Electrodes'). While the method was capable of finding targets related to past releases, a loss of vertical resolution was the trade-off. The burying of electrodes below the infrastructure helped to increase the vertical resolution, as long as a sufficient number of electrodes are available for the acquisition campaign.

RUCKER DF; MYERS DA

2011-10-04T23:59:59.000Z

83

Course: Numerical Simulation in Applied Geophysics. From the Mesoscale to the Macroscale  

E-Print Network (OSTI)

exploration geophysics, mining and reservoir characterization and production, among other fields. Local of wave-induced fluid pressure gradients via a slow-wave diffusion process that can be analyzed using inexpensive and informative, allowing to inspect the physical process of wave propagation using alternative

Santos, Juan

84

Charles University Prague Faculty of Mathematics and Physics  

E-Print Network (OSTI)

Charles University Prague Faculty of Mathematics and Physics an abstract of the thesis submittedD. Department of Geophysics Faculty of Mathematics and Physics Charles University Prague V Holesovick´ach 2 180

Cerveny, Vlastislav

85

GEOPHYSICS  

E-Print Network (OSTI)

?nite-element formulation (Smith. I975). handle any kind of waves in complex media but are limited mainly because nu- merical dispersion prevents them from

86

COSPAR Planetary Protection Policy COSPAR PLANETARY PROTECTION POLICY (20 October 2002; Amended 24 March 2005)  

E-Print Network (OSTI)

policy statement: Although the existence of life elsewhere in the solar system may be unlikelyCOSPAR Planetary Protection Policy COSPAR PLANETARY PROTECTION POLICY (20 October 2002; Amended 24) therefore, COSPAR maintains and promulgates this planetary protection policy for the reference

87

Mercury Geochemical, Groundwater Geochemical, And Radiometric Geophysical  

Open Energy Info (EERE)

Geochemical, Groundwater Geochemical, And Radiometric Geophysical Geochemical, Groundwater Geochemical, And Radiometric Geophysical Signatures At Three Geothermal Prospects In Northern Nevada Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Mercury Geochemical, Groundwater Geochemical, And Radiometric Geophysical Signatures At Three Geothermal Prospects In Northern Nevada Details Activities (14) Areas (3) Regions (0) Abstract: Ground water sampling, desorbed mercury soil geochemical surveys and a radiometric geophysical survey was conducted in conjunction with geological mapping at three geothermal prospects in northern Nevada. Orientation sample lines from 610 m (2000 ft.) to 4575 m (15,000 ft.) in length were surveyed at right angles to known and suspected faults. Scintillometer readings (gamma radiation - total counts / second) were also

88

Geophysical Fluid Dynamics Laboratory Presented by  

E-Print Network (OSTI)

Dynamics Laboratory Outline: · Introduction · Software Infrastructure Projects: Completed Current consortium for climate-weather community 3 #12;Geophysical Fluid Dynamics Laboratory Software Infrastructure Projects ­ Completed: · Flexible Modeling System (FMS) · FMS Model: Hybrid programming model Memory

89

Engineering and environmental geophysics at the millennium  

Science Journals Connector (OSTI)

...locations such as power plants, chemical plants, refineries, and waste-disposal...variations in the electric field. Among these...GPS-determined locations, demands information about...and Wenner sounding curves: Geophysics, 54...

Don W. Steeples

90

Non-Seismic Geophysical Approaches to Monitoring  

SciTech Connect

This chapter considers the application of a number of different geophysical techniques for monitoring geologic sequestration of CO2. The relative merits of the seismic, gravity, electromagnetic (EM) and streaming potential (SP) geophysical techniques as monitoring tools are examined. An example of tilt measurements illustrates another potential monitoring technique, although it has not been studied to the extent of other techniques in this chapter. This work does not represent an exhaustive study, but rather demonstrates the capabilities of a number of geophysical techniques on two synthetic modeling scenarios. The first scenario represents combined CO2 enhance oil recovery (EOR) and sequestration in a producing oil field, the Schrader Bluff field on the north slope of Alaska, USA. The second scenario is of a pilot DOE CO2 sequestration experiment scheduled for summer 2004 in the Frio Brine Formation in South Texas, USA. Numerical flow simulations of the CO2 injection process for each case were converted to geophysical models using petrophysical models developed from well log data. These coupled flow simulation geophysical models allow comparrison of the performance of monitoring techniques over time on realistic 3D models by generating simulated responses at different times during the CO2 injection process. These time-lapse measurements are used to produce time-lapse changes in geophysical measurements that can be related to the movement of CO2 within the injection interval.

Hoversten, G.M.; Gasperikova, Erika

2004-09-01T23:59:59.000Z

91

James L. Green Director, Planetary Science  

E-Print Network (OSTI)

Comet Hartley 2 * November 19 Launch of O/OREOS * December 7 Venus Climate Orbiter (JAXA) 2011 * February 14 Stardust NExT encounters comet Tempel 1 * March 7 ­ Planetary Science Decadal Survey released to Ceres August 5 MSL lands on Mars * Completed #12;Planetary Science Division Overview · Overarching

Rathbun, Julie A.

92

Energy and Energy Flux in Planetary Waves  

Science Journals Connector (OSTI)

...research-article Energy and Energy Flux in Planetary Waves V. T. Buchwald The propagation...a thorough study of the energy of these waves in the plane approximation...case of divergent planetary waves, the total energy density being E = T + U...

1972-01-01T23:59:59.000Z

93

Bulgarian Geophysical Journal, 2006, Vol. 32 Geophysical Institute, Bulgarian Academy of Sciences  

E-Print Network (OSTI)

Geophysical Journal, 2006, Vol. 32 Thermal water is a source of renewable energy and its utilization distribution maps at three depth levels below the surface - 50, 100 and 150m and geothermal gradient map have been prepared and analyzed together with existing geophysical results of gravity, magnetic, electric

Harinarayana, T.

94

Geophysical Studies in the Vicinity of Blue Mountain and Pumpernickel  

Open Energy Info (EERE)

the Vicinity of Blue Mountain and Pumpernickel the Vicinity of Blue Mountain and Pumpernickel Valley near Winnemucca, North-Central Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: Geophysical Studies in the Vicinity of Blue Mountain and Pumpernickel Valley near Winnemucca, North-Central Nevada Abstract From May 2008 to September 2009, the U.S. Geological Survey (USGS) collected data from more than 660 gravity stations, 100 line-km of truck-towed magnetometer traverses, and 260 physical-property sites in the vicinity of Blue Mountain and Pumpernickel Valley, northern Nevada (fig. 1). Gravity, magnetic, and physical-property data were collected to study regional crustal structures as an aid to understanding the geologic framework of the Blue Mountain and Pumpernickel Valley areas, which in

95

E-Print Network 3.0 - artificial geomagnetic field Sample Search...  

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

of Geophysics and Planetary Physics, Scripps Institution of Oceanography,University of California at San Diego Collection: Geosciences 2 Annales Geophysicae, 23, 29692974, 2005...

96

Nehru Fellow  

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

Office of Science, climate work at the Institute for Geophysics and Planetary Physics, a climate monitoring project combining multi-scale measurements and models to infer...

97

Manvendra Dubey selected as Fulbright-Nehru Fellow  

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

Office of Science, climate work at the Institute for Geophysics and Planetary Physics, a climate monitoring project combining multi-scale measurements and models to infer...

98

Contribution of Geophysical Prospecting to Geohazard Evaluation  

SciTech Connect

The physical properties of the subsoil are studied using geophysical methods. These studies are always indirect, such as gravimetric, magnetometric, magnetotelluric or reflection-refraction seismic surveys and are often combined to obtain more accurate and reliable results. With these tools the oil industry commonly investigates the sedimentary basins to localize structures that may favor the accumulation of hydrocarbons. Above all, seismic prospecting allow the understanding of the underground geology, defining boundaries of the geological formations as well as mechanical and physical properties of the rocks. New cutting-edge techniques allow high quality data to be obtained in almost all geological contexts and make reflection seismic the most powerful tool in subsurface observations. The seismic method was utilized in geothermal resources investigation, research of water strategic resources, volcanic risks assessment, etc. The refraction method was the first to be used in the exploration of oil reservoirs. At present the industry employs mainly refraction seismics to study shallow formations. Conversely, university researchers have applied wide-angle reflection-refraction surveys to localize deep crustal interfaces analyzing the high amplitudes of the wide-angle reflections and the velocities obtained from the refracted signals. Moho discontinuity and velocity distribution within the crust were mapped out, indicating thickness and boundary conditions in different geological settings. The maps have been used in the analysis of geodynamical behavior and of active movements within the crust, useful for seismotectonic investigations. The further addition of the seismic reflection imaging, with deep penetration and long transects, completed multidisciplinary programs to unravel the structure of the crust with clear seismic images and models. High-resolution application of seismic has a central role in the identification and characterization of seismotectonic and seismogenetic zones and of the related capable faults. The earthquakes represent an important external risk for key constructions and nuclear power plants and capable faults cause near-surface displacements being considered to be the more critical for site safety. A close cooperation among geophysicists, geologists and seismologists is recommended in the hazards evaluation, alike in macrozoning for location of seismic sources and in microzoning for the measure of terrains mechanical properties and dynamic responses. Here I present and discuss the results of integrated multidisciplinary studies to unravel the peculiarity of the crustal structures and seismicity in Southern Tuscany, Italy.

Nicolich, Rinaldo [Department of Civil Engineering, University of Trieste, via Valerio 10, I-34127 Trieste (Italy)

2006-03-23T23:59:59.000Z

99

Spatial correlation structure estimation using geophysical and hydrogeological data  

E-Print Network (OSTI)

Spatial correlation structure estimation using geophysical and hydrogeological data Susan S investigate the use of tomographic geophysical data in combination with hydrogeological data in the spatial of data having different support scales and spatial sampling windows was facilitated. Comparison

Hubbard, Susan

100

Geophysical Exploration Technologies | Open Energy Information  

Open Energy Info (EERE)

Geophysical Exploration Technologies Geophysical Exploration Technologies Jump to: navigation, search Geothermal ARRA Funded Projects for Geophysical Exploration Technologies Loading map... {"format":"googlemaps3","type":"ROADMAP","types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"limit":200,"offset":0,"link":"all","sort":[""],"order":[],"headers":"show","mainlabel":"","intro":"","outro":"","searchlabel":"\u2026 further results","default":"","geoservice":"google","zoom":false,"width":"600px","height":"350px","centre":false,"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":"","icon":"","visitedicon":"","forceshow":true,"showtitle":true,"hidenamespace":false,"template":false,"title":"","label":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"locations":[{"text":"

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Terrain identification methods for planetary exploration rovers  

E-Print Network (OSTI)

Autonomous mobility in rough terrain is becoming increasingly important for planetary exploration rovers. Increased knowledge of local terrain properties is critical to ensure a rover's safety, especially when driving on ...

Brooks, Christopher Allen, 1978-

2004-01-01T23:59:59.000Z

102

ARM - Measurement - Planetary boundary layer height  

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

govMeasurementsPlanetary boundary layer height govMeasurementsPlanetary boundary layer height ARM Data Discovery Browse Data Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Measurement : Planetary boundary layer height Top of the planetary boundary layer; also known as depth or height of the mixing layer. Categories Atmospheric State Instruments The above measurement is considered scientifically relevant for the following instruments. Refer to the datastream (netcdf) file headers of each instrument for a list of all available measurements, including those recorded for diagnostic or quality assurance purposes. ARM Instruments VCEIL : Vaisala Ceilometer External Instruments NCEPGFS : National Centers for Environment Prediction Global Forecast System Field Campaign Instruments

103

Geophysical Monitoring of Hydrological and Biogeochemical  

E-Print Network (OSTI)

explored the use of geophysical approaches for monitoring the spatiotemporal distribution of hydrological and biogeochemical transformations associated with a Cr(VI) bioremediation experiment performed at Hanford, WA. We: the spatial distribution of injected electron donor; the evolution of gas bubbles; variations in total

Hubbard, Susan

104

Statistical Analysis of EXTREMES in GEOPHYSICS  

E-Print Network (OSTI)

Statistical Analysis of EXTREMES in GEOPHYSICS Zwiers FW and Kharin VV. 1998. Changes in the extremes of the climate simulated by CCC GCM2 under CO2 dou- bling. J. Climate 11:2200­2222. http://www.ral.ucar.edu/staff/ericg/readinggroup.html #12;Outline · Some background on Extreme Value Statistics ­ Extremal Types Theorem ­ Max

Gilleland, Eric

105

Geophysical Method At Raft River Geothermal Area (1977) | Open Energy  

Open Energy Info (EERE)

Geophysical Method At Raft River Geothermal Area (1977) Geophysical Method At Raft River Geothermal Area (1977) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Geophysical Method At Raft River Geothermal Area (1977) Exploration Activity Details Location Raft River Geothermal Area Exploration Technique Geophysical Techniques Activity Date 1977 Usefulness not indicated DOE-funding Unknown Notes Borehole geophysics were completed at the Raft River valley, Idaho. References Applegate, J.K.; Donaldson, P.R.; Hinkley, D.L.; Wallace, T.L. (1 February 1977) Borehole geophysics evaluation of the Raft River geothermal reservoir, Idaho Retrieved from "http://en.openei.org/w/index.php?title=Geophysical_Method_At_Raft_River_Geothermal_Area_(1977)&oldid=594349" Category: Exploration Activities

106

JournalofGeophysicalResearch: SpacePhysics RESEARCH ARTICLE  

E-Print Network (OSTI)

the radar signal returns from various ground-based radar facilities. Finally, simulated backscattered of relativistic electrons, injected from a balloon, rocket, or spacecraft could be used for field line tracing on the ATLAS-1 mission [e.g., Burch et al., 1993] included a 6.25 keV electron beam of up to 1.2 A current

107

Planetary Emissions Management | Open Energy Information  

Open Energy Info (EERE)

Planetary Emissions Management Planetary Emissions Management Jump to: navigation, search Name Planetary Emissions Management Place Cambridge, Massachusetts Sector Carbon Product US-based, company offering measurements of carbon budgets using laser technology. Coordinates 43.003745°, -89.017499° 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":43.003745,"lon":-89.017499,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

108

Automatic Detection of Craters in Planetary Images: An Embedded Framework  

E-Print Network (OSTI)

, and Tianyu Cao5 University of Massachusetts Boston, Boston, Massachusetts1 Lunar and Planetary Institute with planetary surfaces, are among the most stud- ied geomorphic features in the solar system because they yield

Ding, Wei

109

Mission design for safe traverse of planetary hoppers  

E-Print Network (OSTI)

Planetary hoppers are a new class of vehicle being developed that will provide planetary surface mobility by reusing the landing platform and its actuators to propulsively ascend, translate, and descend to new landing ...

Cohanim, Babak, 1980-

2013-01-01T23:59:59.000Z

110

Hypervelocity impacts and the evolution of planetary surfaces and interiors  

E-Print Network (OSTI)

The thesis consists of five studies relating impact processes to the evolution of planetary interiors as well as impact structures on planetary surfaces. Chapter 2 is concerned with developing methods for estimating the ...

Watters, Wesley Andrs, 1976-

2009-01-01T23:59:59.000Z

111

Geophysical investigation, Salmon Site, Lamar County, Mississippi  

SciTech Connect

Geophysical surveys were conducted in 1992 and 1993 on 21 sites at the Salmon Site (SS) located in Lamar County, Mississippi. The studies are part of the Remedial Investigation/Feasibility Study (RI/FS) being conducted by IT Corporation for the U.S. Department of Energy (DOE). During the 1960s, two nuclear devices and two chemical tests were detonated 826 meters (in) (2710 feet [ft]) below the ground surface in the salt dome underlying the SS. These tests were part of the Vela Uniform Program conducted to improve the United States capability to detect, identify, and locate underground nuclear detonations. The RI/FS is being conducted to determine if any contamination is migrating from the underground shot cavity in the salt dome and if there is any residual contamination in the near surface mud and debris disposal pits used during the testing activities. The objective of the surface geophysical surveys was to locate buried debris, disposal pits, and abandoned mud pits that may be present at the site. This information will then be used to identify the locations for test pits, cone penetrometer tests, and drill hole/monitor well installation. The disposal pits were used during the operation of the test site in the 1960s. Vertical magnetic gradient (magnetic gradient), electromagnetic (EM) conductivity, and ground-penetrating radar (GPR) surveys were used to accomplish these objectives. A description of the equipment used and a theoretical discussion of the geophysical methods are presented Appendix A. Because of the large number of figures relative to the number of pages of text, the geophysical grid-location maps, the contour maps of the magnetic-gradient data, the contour maps of the EM conductivity data, and the GPR traverse location maps are located in Appendix B, Tabs I through 22. In addition, selected GPR records are located in Appendix C.

NONE

1995-02-01T23:59:59.000Z

112

BSU Geophysics Field Camp Report 2012 | Open Energy Information  

Open Energy Info (EERE)

BSU Geophysics Field Camp Report 2012 BSU Geophysics Field Camp Report 2012 Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: BSU Geophysics Field Camp Report 2012 Abstract Neal Hot Springs (NHS) is an active geothermal site and home to a new binary power plant built by U.S. Geothermal and funded through the Department of Energy. Power production is scheduled to begin in late 2012 and is proposed to generate 25 mega-watts of power to its customer Idaho Power. The project has also served Boise State University as an ideal location for geophysical exploration and research. Research began in spring of 2011 during BSU's annual geophysics field camp. Students and faculty conducted various geophysical surveys to gain insight into the controlling geological structure of the area. Studies of the site continued into 2012

113

UNIVERSITY OF CALIFORNIA, SANTA CRUZ EARTH AND PLANETARY SCIENCES  

E-Print Network (OSTI)

UNIVERSITY OF CALIFORNIA, SANTA CRUZ EARTH AND PLANETARY SCIENCES Ongoing Lecturer Pool The Department of Earth & Planetary Sciences at the University of California, Santa Cruz, is developing a short of instruction in areas of earth and planetary sciences. Outstanding candidates with teaching experience in all

California at Santa Cruz, University of

114

Borehole geophysics evaluation of the Raft River geothermal reservoir,  

Open Energy Info (EERE)

reservoir, reservoir, Idaho Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: Borehole geophysics evaluation of the Raft River geothermal reservoir, Idaho Details Activities (1) Areas (1) Regions (0) Abstract: GEOTHERMAL ENERGY; GEOTHERMAL FIELDS; GEOPHYSICAL SURVEYS; RAFT RIVER VALLEY; GEOTHERMAL EXPLORATION; BOREHOLES; EVALUATION; HOT-WATER SYSTEMS; IDAHO; MATHEMATICAL MODELS; WELL LOGGING; CAVITIES; EXPLORATION; GEOTHERMAL SYSTEMS; HYDROTHERMAL SYSTEMS; NORTH AMERICA; PACIFIC NORTHWEST REGION; USA Author(s): Applegate, J.K.; Donaldson, P.R.; Hinkley, D.L.; Wallace, T.L. Published: Geophysics, 2/1/1977 Document Number: Unavailable DOI: Unavailable Source: View Original Journal Article Geophysical Method At Raft River Geothermal Area (1977) Raft River Geothermal Area

115

Numerical Simulation in Applied Geophysics. From the Mesoscale to ...  

E-Print Network (OSTI)

Instituto del Gas y del Petrleo, Facultad de Ingenie? a UBA ... Seismic wave propagation is a common technique used in hydrocarbon exploration geophysics

116

Ch. VI, The geophysical environment around Waunita Hot Springs...  

Open Energy Info (EERE)

Ch. VI, The geophysical environment around Waunita Hot Springs Author A. L. Lange Editor T. G. Zacharakis Published Colorado Geological Survey in Cooperation with the U.S....

117

Course: Numerical Simulation in Applied Geophysics. From the ...  

E-Print Network (OSTI)

ration geophysics, mining and reservoir characterization and production. ... [5] T. Bourbie and O. Coussy and B. Zinszner, Acoustics of Porous Media, Editions ... [

2013-10-09T23:59:59.000Z

118

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization  

E-Print Network (OSTI)

We describe the ongoing development of joint geophysical imaging methodologies for geothermal site characterization and demonstrate their potential in two regions: Krafla volcano and associated geothermal fields in ...

Zhang, Haijiang

2012-01-01T23:59:59.000Z

119

Use of Geophysical Techniques to Characterize Fluid Flow in a...  

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

to Geothermal Prospecting Joint inversion of electrical and seismic data for Fracture char. and Imaging of Fluid Flow in Geothermal Systems Use of Geophysical Techniques...

120

Use of Geophysical Techniques to Characterize Fluid Flow in a...  

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

and test combined geophysical techniques to characterize fluid flow, in relation to fracture orientations and fault distributions in a geothermal system. Average Overall Score:...

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization  

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

DOE Geothermal Peer Review 2010 - Presentation. This project aims to develop improved geophysical imaging method for characterizing subsurface structure, identify fluid locations, and characterize fractures.

122

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization  

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

Advanced 3D Geophysical Imaging Technologies for Geothermal Resource Characterization presentation at the April 2013 peer review meeting held in Denver, Colorado.

123

Use of Geophysical Techniques to Characterize Fluid Flow in a...  

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

or otherwise restricted information. Self-potential 2 | US DOE Geothermal Program eere.energy.gov * Use of Geophysical Techniques to Characterize Fluid Flow in a Geothermal...

124

Crustal Geophysics and Geochemistry Science Center | Open Energy...  

Open Energy Info (EERE)

Science Center Jump to: navigation, search OpenEI Reference LibraryAdd to library Web Site: Crustal Geophysics and Geochemistry Science Center Author USGS Published...

125

Merging high resolution geophysical and geochemical surveys to...  

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

high resolution geophysical and geochemical surveys to reduce exploration risk at Glass Buttes, Oregon Patrick Walsh Ormat Nevada Inc. Innovative technologies May 19, 2010...

126

3D-Spectroscopy of extragalactic planetary nebulae as diagnostic probes for galaxy evolution  

E-Print Network (OSTI)

In addition to study extragalactic stellar populations in their integrated light, the detailed analysis of individual resolved objects has become feasible, mainly for luminous giant stars and for extragalactic planetary nebulae (XPNe) in nearby galaxies. A recently started project at the Astrophysical Institute Potsdam (AIP), called ``XPN--Physics'', aims to verify if XPNe are useful probes to measure the chemical abundances of their parent stellar population. The project involves theoretical and observational work packages.

Andreas Kelz; Ana Monreal-Ibero; Martin M. Roth; Christer Sandin; Detlef Schoenberner; Matthias Steffen

2006-07-21T23:59:59.000Z

127

Six Hot Topics in Planetary Astronomy  

E-Print Network (OSTI)

Six hot topics in modern planetary astronomy are described: 1) lightcurves and densities of small bodies 2) colors of Kuiper belt objects and the distribution of the ultrared matter 3) spectroscopy and the crystallinity of ice in the outer Solar system 4) irregular satellites of the giant planets 5) the Main Belt Comets and 6) comets and meteor stream parents.

David Jewitt

2008-11-14T23:59:59.000Z

128

Director, Planetary Science October 13, 2011  

E-Print Network (OSTI)

in science mode ·November 4 - EPOXI encounters Comet Hartley 2 2011 ·February 14 - Stardust NExT encounters comet Tempel 1 ·March 7 ­ Planetary Science Decadal Survey released ·March 17 - MESSENGER orbit leaves Vesta starts on its journey to Ceres ·August ­ Curiosity Rover lands on Mars · Completed http

Rathbun, Julie A.

129

Use of Geophysical Techniques to Characterize Fluid Flow in a Geothermal Reservoir  

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

Project objectives: Joint inversion of geophysical data for ground water flow imaging; Reduced the cost in geothermal exploration and monitoring; & Combined passive and active geophysical methods.

130

DEVELOPING GIS VISUALIZATION WEB SERVICES FOR GEOPHYSICAL APPLICATIONS  

E-Print Network (OSTI)

DEVELOPING GIS VISUALIZATION WEB SERVICES FOR GEOPHYSICAL APPLICATIONS A. Sayar a,b. *, M. Pierce Commission II, WG II/2 KEY WORDS: GIS, Geophysics, Visualization, Internet/Web, Interoperability, Networks Information System (GIS) community. In this paper we will describe our group's efforts to implement GIS

131

Geophysical Method At Raft River Geothermal Area (1975) | Open Energy  

Open Energy Info (EERE)

Method At Raft River Geothermal Area (1975) Method At Raft River Geothermal Area (1975) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Geophysical Method At Raft River Geothermal Area (1975) Exploration Activity Details Location Raft River Geothermal Area Exploration Technique Geophysical Techniques Activity Date 1975 Usefulness not indicated DOE-funding Unknown Notes Geologic and geophysics studies were completed at the Raft River valley. References Williams, P.L.; Mabey, D.R.; Pierce, K.L.; Zohdy, A.A.R.; Ackermann, H.; Hoover, D.B. (1 May 1975) Geological and geophysical studies of a geothermal area in the southern Raft river valley, Idaho Retrieved from "http://en.openei.org/w/index.php?title=Geophysical_Method_At_Raft_River_Geothermal_Area_(1975)&oldid=59434

132

Integrated Surface Geophysical Methods for Characterization of the Naval  

Open Energy Info (EERE)

Integrated Surface Geophysical Methods for Characterization of the Naval Integrated Surface Geophysical Methods for Characterization of the Naval Air Warfare Center, New Jersey Jump to: navigation, search OpenEI Reference LibraryAdd to library Web Site: Integrated Surface Geophysical Methods for Characterization of the Naval Air Warfare Center, New Jersey Author USGS Published Publisher Not Provided, 2013 DOI Not Provided Check for DOI availability: http://crossref.org Online Internet link for Integrated Surface Geophysical Methods for Characterization of the Naval Air Warfare Center, New Jersey Citation USGS. Integrated Surface Geophysical Methods for Characterization of the Naval Air Warfare Center, New Jersey [Internet]. 2013. [updated 2013/01/03;cited 2013/11/22]. Available from: http://water.usgs.gov/ogw/bgas/toxics/NAWC-surface.html

133

Geology and Geophysics at the University of Utah Advisors for Undergraduate Geology & Geophysics Students (2014-15 academic year)  

E-Print Network (OSTI)

Geology and Geophysics at the University of Utah Advisors for Undergraduate Geology & Geophysics Martinez (email: judy.martinez@utah.edu, office: 383 FASB, phone: 801-581-6553) Faculty Advisors-581-7250) Faculty Advisor for Environmental Science Emphasis, Geoscience Major ­ Prof. Dave Dinter (email: david

Johnson, Cari

134

Geology and Geophysics at the University of Utah Advisors for Undergraduate Geology & Geophysics Students (2013-14 academic year)  

E-Print Network (OSTI)

Geology and Geophysics at the University of Utah Advisors for Undergraduate Geology & Geophysics Martinez (email: judy.martinez@utah.edu, office: 383 FASB, phone: 801-581-6553) Faculty Advisors Advisor for Environmental Science Emphasis, Geoscience Major ­ Prof. Dave Dinter (email: david

Johnson, Cari

135

JournalofGeophysicalResearch: Atmospheres RESEARCH ARTICLE  

E-Print Network (OSTI)

National Institute of Polar Research, Tachikawa, Japan, 5Physics and Astronomy, Ohio Wesleyan University

Vadas, Sharon

136

Volatiles as a link between planetary interiors and the environment  

E-Print Network (OSTI)

Volatiles derived from planetary interiors influence magma evolution and environmental processes. Over appropriate timescales, Earth's mantle, crust, ocean, and atmosphere constitute coupled systems. The apparently synchronous ...

Black, Benjamin A. (Benjamin Alexander)

2013-01-01T23:59:59.000Z

137

Frontiers in Planetary and Stellar Magnetism through High-Performance...  

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

Hwang, project co-PI Frontiers in Planetary and Stellar Magnetism through High-Performance Computing PI Name: Jonathan Aurnou PI Email: aurnou@ucla.edu Institution: University...

138

Geology and geophysics of the Beata Ridge - Caribbean  

E-Print Network (OSTI)

GEOLOGY AND GEOPHYSICS OF THE BEATA RIDGE - CARIBBEAN A Thesis by LANAR BURTON ROEMER Submitted to the Graduate College of Texas Ak? University in partial fu1fillment of the requirement for the degree of MASTER OF SCIENCE August 1973 Ma...)or Subject: Oceanography GEOLOGY AND GEOPHYSICS OF THE BEATA RIDGE ? CARIBBEAN A Thesis by LAMAR BURTON ROEMER Approved as to style and content by: o-Chairman o C it ee -Car f o ee ea o Dep r e Member August 1973 ABSTRACT Geology and Geophysics...

Roemer, Lamar Burton

1973-01-01T23:59:59.000Z

139

Monitoring Vadose Zone Desiccation with Geophysical Methods  

SciTech Connect

Soil desiccation was recently field tested as a potential vadose zone remediation technology. Desiccation removes water from the vadose zone and significantly decreases the aqueous-phase permeability of the desiccated zone, thereby decreasing movement of moisture and contaminants. The 2-D and 3-D distribution of moisture content reduction over time provides valuable information for desiccation operations and for determining when treatment goals have been reached. This type of information can be obtained through use of geophysical methods. Neutron moisture logging, cross-hole electrical resistivity tomography, and cross-hole ground penetrating radar approaches were evaluated with respect to their ability to provide effective spatial and temporal monitoring of desiccation during a treatability study conducted in the vadose zone of the DOE Hanford Site in WA.

Truex, Michael J.; Johnson, Timothy C.; Strickland, Christopher E.; Peterson, John E.; Hubbard, Susan S.

2013-05-01T23:59:59.000Z

140

Integrated Geophysical Exploration of a Known Geothermal Resource: Neal Hot  

Open Energy Info (EERE)

Geophysical Exploration of a Known Geothermal Resource: Neal Hot Geophysical Exploration of a Known Geothermal Resource: Neal Hot Springs Jump to: navigation, search OpenEI Reference LibraryAdd to library Book Section: Integrated Geophysical Exploration of a Known Geothermal Resource: Neal Hot Springs Abstract We present integrated geophysical data to characterize a geothermal system at Neal Hot Springs in eastern Oregon. This system is currently being developed for geothermal energy production. The hot springs are in a region of complex and intersecting fault trends associated with two major extensional events, the Oregon-Idaho Graben and the Western Snake River Plain. The intersection of these two fault systems, coupled with high geothermal gradients from thin continental crust produces pathways for surface water and deep geothermal water interactions at Neal Hot Springs.

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Rules and Regulations Governing Geophysical, Seismic or Other Type  

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

Rules and Regulations Governing Geophysical, Seismic or Other Type Rules and Regulations Governing Geophysical, Seismic or Other Type Exploration on State-Owned Lands Other Than State-Owned Marine Waters (Mississippi) Rules and Regulations Governing Geophysical, Seismic or Other Type Exploration on State-Owned Lands Other Than State-Owned Marine Waters (Mississippi) < Back Eligibility Commercial Developer Fuel Distributor General Public/Consumer Industrial Investor-Owned Utility Municipal/Public Utility Utility Program Info State Mississippi Program Type Environmental Regulations Siting and Permitting Provider Mississippi Development Authority The Rules and Regulations Governing Geophysical, seismic or Other Type Exploration on State-Owned Lands Other than State-Owned Marine Waters is applicable to the Natural Gas Sector and the Coal with CCS Sector. This law

142

Geological and geophysical analysis of Coso Geothermal Exploration Hole No.  

Open Energy Info (EERE)

and geophysical analysis of Coso Geothermal Exploration Hole No. and geophysical analysis of Coso Geothermal Exploration Hole No. 1 (CGEH-1), Coso Hot Springs KGRA, California Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Report: Geological and geophysical analysis of Coso Geothermal Exploration Hole No. 1 (CGEH-1), Coso Hot Springs KGRA, California Details Activities (5) Areas (1) Regions (0) Abstract: The Coso Geothermal Exploration Hole number one (CGEH-1) was drilled in the Coso Hot Springs KGRA, California, from September 2 to December 2, 1977. Chip samples were collected at ten foot intervals and extensive geophysical logging surveys were conducted to document the geologic character of the geothermal system as penetrated by CGEH-1. The major rock units encountered include a mafic metamorphic sequence and a

143

Numerical Simulation in Applied Geophysics. From the Mesoscale to ...  

E-Print Network (OSTI)

Instead of solving the global problem associated with the above model, we obtained the solution using a parallel FE ... Black-Oil simulator. .... used in hydrocarbon exploration geophysics, mining and reservoir characterization and production.

144

Accepted to the Journal Geophysical Research Laboratory measurements of electrical  

E-Print Network (OSTI)

1 Accepted to the Journal Geophysical Research Laboratory measurements of electrical conductivities measurements of electrical conductivities of natural magma compositions. The electrical conductivities of three. The electrical conductivity increases with temperature and is higher in the order tephrite, phonotephrite

Paris-Sud XI, Université de

145

Seeing the Invisible: Educating the Public on Planetary Magnetic Fields and How they Affect Atmospheres  

E-Print Network (OSTI)

Seeing the Invisible: Educating the Public on Planetary Magnetic Fields and How they Affect to visualize ­ invisible · But planetary magnetic field and charged particle environments (magnetospheres

Fillingim, Matthew

146

Energetic neutral atoms at Mars 4. Imaging of planetary oxygen  

E-Print Network (OSTI)

Energetic neutral atoms at Mars 4. Imaging of planetary oxygen S. Barabash and M. Holmstro of the Martian oxygen exosphere/corona results in the production of planetary oxygen ions. The newborn ions start. The oxygen ions can then charge exchange with the neutral gases (H, H2, and O) of the Martian exosphere

Lukyanov, Alex

147

LANL | Physics | Nuclear Physics  

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

Leaders in nuclear physics Physics Division scientists and engineers play an important role in the Laboratory's Nuclear Physics program, funded by the Department of Energy's Office...

148

Planetary nebulae abundances and stellar evolution  

E-Print Network (OSTI)

A summary is given of planetary nebulae abundances from ISO measurements. It is shown that these nebulae show abundance gradients (with galactocentric distance), which in the case of neon, argon, sulfur and oxygen (with four exceptions) are the same as HII regions and early type star abundance gradients. The abundance of these elements predicted from these gradients at the distance of the Sun from the center are exactly the solar abundance. Sulfur is the exception to this; the reason for this is discussed. The higher solar neon abundance is confirmed; this is discussed in terms of the results of helioseismology. Evidence is presented for oxygen destruction via ON cycling having occurred in the progenitors of four planetary nebulae with bilobal structure. These progenitor stars had a high mass, probably greater than 5 solar masses. This is deduced from the high values of He/H and N/H found in these nebulae. Formation of nitrogen, helium and carbon are discussed. The high mass progenitors which showed oxygen destruction are shown to have probably destroyed carbon as well. This is probably the result of hot bottom burning.

S. R. Pottasch; J. Bernard-Salas

2006-07-31T23:59:59.000Z

149

The (In)Stability of Planetary Systems  

E-Print Network (OSTI)

We present results of numerical simulations which examine the dynamical stability of known planetary systems, a star with two or more planets. First we vary the initial conditions of each system based on observational data. We then determine regions of phase space which produce stable planetary configurations. For each system we perform 1000 ~1 million year integrations. We examine upsilon And, HD83443, GJ876, HD82943, 47UMa, HD168443, and the solar system (SS). We find that the resonant systems, 2 planets in a first order mean motion resonance, (HD82943 and GJ876) have very narrow zones of stability. The interacting systems, not in first order resonance, but able to perturb each other (upsilon And, 47UMa, and SS) have broad regions of stability. The separated systems, 2 planets beyond 10:1 resonance, (we only examine HD83443 and HD168443) are fully stable. Furthermore we find that the best fits to the interacting and resonant systems place them very close to unstable regions. The boundary in phase space between stability and instability depends strongly on the eccentricities, and (if applicable) the proximity of the system to perfect resonance. In addition to million year integrations, we also examined stability on ~100 million year timescales. For each system we ran ~10 long term simulations, and find that the Keplerian fits to these systems all contain configurations which may be regular on this timescale.

Rory Barnes; Thomas Quinn

2004-01-09T23:59:59.000Z

150

Hydromechanical transmission with compound planetary assembly  

DOE Patents (OSTI)

A power transmission having three distinct ranges: (1) hydrostatic, (2) simple power-split hydromechanical, and (3) compound power-split hydromechanical. A single compound planetary assembly has two sun gears, two ring gears, and a single carrier with two sets of elongated planet gears. The two sun gears may be identical in size, and the two ring gears may be identical in size. A speed-varying module in driving relationship to the first sun gear is clutchable, in turn, to (1) the input shaft and (2) the second sun gear. The speed-varying means may comprise a pair of hydraulic units hydraulically interconnected so that one serves as a pump while the other serves as a motor and vice versa, one of the units having a variable stroke and being the one clutchable to either the input shaft or to the second sun gear. The other unit, which may have a fixed stroke, is connected in driving relation to the first sun gear. A brake grounds the carrier in the first range and in reverse and causes drive to be delivered to the output shaft through the first ring gear in a hydrostatic mode, the first ring gear being rigidly connected to the output shaft. The input shaft is also clutchable to the second ring gear of the compound planetary assembly.

Orshansky, Jr., deceased, Elias (late of San Francisco, CA); Weseloh, William E. (San Diego, CA)

1980-01-01T23:59:59.000Z

151

APPLIED PHYSICS APPLIED PHYSICS  

E-Print Network (OSTI)

MSc APPLIED PHYSICS #12;MSc APPLIED PHYSICS This taught Masters course is based on the strong research in Applied Physics in the University's Department of Physics. The department has an impressive photonics and quantum optics, Physics and the Life Sciences, and solid state physics. The knowledge gained

Mottram, Nigel

152

Understanding biogeobatteries: Where geophysics meets microbiology  

SciTech Connect

Although recent research suggests that contaminant plumes behave as geobatteries that produce an electrical current in the ground, no associated model exists that honors both geophysical and biogeochemical constraints. Here, we develop such a model to explain the two main electrochemical contributions to self-potential signals in contaminated areas. Both contributions are associated with the gradient of the activity of two types of charge carriers, ions and electrons. In the case of electrons, bacteria act as catalysts for reducing the activation energy needed to exchange the electrons between electron donor and electron acceptor. Possible mechanisms that facilitate electron migration include iron oxides, clays, and conductive biological materials, such as bacterial conductive pili or other conductive extracellular polymeric substances. Because we explicitly consider the role of biotic processes in the geobattery model, we coined the term 'biogeobattery'. After theoretical development of the biogeobattery model, we compare model predictions with self-potential responses associated with laboratory and field-scale conducted in contaminated environments. We demonstrate that the amplitude and polarity of large (>100 mV) self-potential signatures requires the presence of an electronic conductor to serve as a bridge between electron donors and acceptors. Small self-potential anomalies imply that electron donors and electron acceptors are not directly interconnected, but instead result simply from the gradient of the activity of the ionic species that are present in the system.

Revil, A.; Mendonca, C.A.; Atekwana, E.A.; Kulessa, B.; Hubbard, S.S.; Bohlen, K.

2009-08-15T23:59:59.000Z

153

Mon. Not. R. Astron. Soc. 000, 113 (2014) Printed 10 November 2014 (MN LATEX style file v2.2) On the Stability of Extrasolar Planetary Systems  

E-Print Network (OSTI)

. Bloch3 1Physics Department, University of Michigan, Ann Arbor, MI 48109 2Astronomy Department, University of Michigan, Ann Arbor, MI 48109 3Mathematics Department, University of Michigan, Ann Arbor, MI). Many extra- solar planetary systems with Hot Jupiters (apparently) do not have an equilibrium state

Bloch, Anthony

154

871 The Meteoritical Society, 2009. Printed in USA. Meteoritics & Planetary Science 44, Nr 6, 871878 (2009)  

E-Print Network (OSTI)

871 © The Meteoritical Society, 2009. Printed in USA. Meteoritics & Planetary Science 44, Nr 6, 871

Perfect, Ed

155

Planetary Fuels LLC | Open Energy Information  

Open Energy Info (EERE)

Fuels LLC Fuels LLC Jump to: navigation, search Name Planetary Fuels, LLC Place Seattle, Washington Product Seattle-based start-up dedicated to the production of biodiesel. Coordinates 47.60356°, -122.329439° 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":47.60356,"lon":-122.329439,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

156

The energy transfer process in planetary flybys  

Science Journals Connector (OSTI)

We illustrate the energy transfer during planetary flybys as a function of time using a number of flight mission examples. The energy transfer process is rather more complicated than a monotonic increase (or decrease) of energy with time. It exhibits temporary maxima and minima with time which then partially moderate before the asymptotic condition is obtained. The energy transfer to angular momentum is exhibited by an approximate Jacobi constant for the system. We demonstrate this with flybys that have shown unexplained behaviors: (i) the possible onset of the Pioneer anomaly with the gravity assist of Pioneer 11 by Saturn to hyperbolic orbit (as well as the Pioneer 10 hyperbolic gravity assist by Jupiter) and (ii) the Earth flyby anomalies of small increases in energy in the geocentric system (Galileo-I, NEAR, and Rosetta, in addition discussing the Cassini and Messenger flybys). Perhaps some small, as yet unrecognized effect in the energy-transfer process can shed light on these anomalies.

John D. Anderson; James K. Campbell; Michael Martin Nieto

2007-01-01T23:59:59.000Z

157

Space Research and Planetary Sciences Division of  

E-Print Network (OSTI)

Physics Space Research and Planetology Climate and Environmental Physics High Energy Physics. (*The cosmic ray group is an independent sub-group but formally connected to the theoretical planetology will provide you with the STADTANZEIGER (the local paper of the city of Bern) if you request them to. If you

Richner, Heinz

158

On the Selection of Photometric Planetary Transits  

E-Print Network (OSTI)

We present a new method for differentiating between planetary transits and eclipsing binaries based on the presence of the ellipsoidal light variations. These variations can be used to detect stellar secondaries with masses ~0.2 M_sun orbiting sun-like stars at a photometric accuracy level which has already been achieved in transit surveys. By removing candidates exhibiting this effect it is possible to greatly reduce the number of objects requiring spectroscopic follow up with large telescopes. Unlike the usual candidate selection method, which are primarily based on the estimated radius of the orbiting object, this technique is not biased against bona-fide planets and brown dwarfs with large radii, because the amplitude of the effect depends on the transiting object's mass and orbital distance. In many binary systems, where a candidate planetary transit is actually due to the partial eclipse of two normal stars, the presence of flux variations due to the gravity darkening effect will show the true nature of these systems. We show that many of the recent OGLE-III photometric transit candidates exhibit the presence of significant variations in their light curves and are likely to be due to stellar secondaries. We find that the light curves of white dwarf transits will generally not mimic those of small planets because of significant gravitationally induced flux variations. We discuss the relative merits of methods used to detect transit candidates which are due to stellar blends rather than planets. We outline how photometric observations taken in two bands can be used to detect the presence of stellar blends.

A. J. Drake

2003-01-15T23:59:59.000Z

159

NATIONAL GEOPHYSICAL RESEARCH INSTITUTE, HYDERABAD, INDIA. Induction Workshop: (18 -23 October, 2004)  

E-Print Network (OSTI)

. 13. Open session · Venue:: National Geophysical Research Institute (An ISO 9001 Organisation in different sectors of the Himalaya. #12;· Venue:: National Geophysical Research Institute (An ISO 9001

Harinarayana, T.

160

Advances in borehole geophysics for hydrology  

SciTech Connect

Borehole geophysical methods provide vital subsurface information on rock properties, fluid movement, and the condition of engineered borehole structures. Within the first category, salient advances include the continuing improvement of the borehole televiewer, refinement of the electrical conductivity dipmeter for fracture characterization, and the development of a gigahertz-frequency electromagnetic propagation tool for water saturation measurements. The exploration of the rock mass between boreholes remains a challenging problem with high potential; promising methods are now incorporating high-density spatial sampling and sophisticated data processing. Flow-rate measurement methods appear adequate for all but low-flow situations. At low rates the tagging method seems the most attractive. The current exploitation of neutron-activation techniques for tagging means that the wellbore fluid itself is tagged, thereby eliminating the mixing of an alien fluid into the wellbore. Another method uses the acoustic noise generated by flow through constrictions and in and behind casing to detect and locate flaws in the production system. With the advent of field-recorded digital data, the interpretation of logs from sedimentary sequences is now reaching a sophisticated level with the aid of computer processing and the application of statistical methods. Lagging behind are interpretive schemes for the low-porosity, fracture-controlled igneous and metamorphic rocks encountered in the geothermal reservoirs and in potential waste-storage sites. Progress is being made on the general problem of fracture detection by use of electrical and acoustical techniques, but the reliable definition of permeability continues to be an elusive goal.

Nelson, P.H.

1982-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Geophysical Journal International Geophys. J. Int. (2013) doi: 10.1093/gji/ggt482  

E-Print Network (OSTI)

Kalscheuer2 and Jasper A. Vrugt3,4 1Applied and Environmental Geophysics Group, Faculty of Geosciences

Vrugt, Jasper A.

162

Time-lapse Joint Inversion of Geophysical Data and its Applications...  

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

Objectives of the project * Forward modeling geophysical response with fluid flowheat modeling * Joint inversion (stochasticdeterministic) for ground water flow imaging *...

163

Geophysical monitoring of foam used to deliver remediation treatments within the vadose zone  

E-Print Network (OSTI)

relationships observed for unconsolidated sediments. Wateron unsaturated, unconsolidated sands. Geophysics 69:762-771.saturated and unsaturated unconsolidated samples (Vanhala

Wu, Y.

2013-01-01T23:59:59.000Z

164

Chiara Piccolo, Anu Dudhia Atmospheric, Oceanic and Planetary Physics, Department of Physics, Oxford University, Oxford, UK  

E-Print Network (OSTI)

) above 10 pmol/mol for CF4 above 100 mol/mol for C2F6 (50 pmol/mol after 2011) Air /Air modified CCQM-P41.06 at 6 pmol/mol for SF6 0.01 at 1 nmol/mol for NF3 0.1 at 10 pmol/mol for CF4 Air /Air modified CCQM-K68 SF6, N2, O2 NF3, N2, O2 Air /Air modified CCQM-K15, Paper preparation CF4 (C2F6), N2, O2 Air /Air

Oxford, University of

165

Characterization Of Geothermal Resources Using New Geophysical Technology |  

Open Energy Info (EERE)

Using New Geophysical Technology Using New Geophysical Technology Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Characterization Of Geothermal Resources Using New Geophysical Technology Details Activities (2) Areas (2) Regions (0) Abstract: This paper presents a geothermal case history using a relatively new but proven technology that can accurately map groundwater at significant depths (up to 1,000 meters) over large areas (square kilometers) in short periods of time (weeks). Understanding the location and extent of groundwater resources is very important to the geothermal industry for obvious reasons. It is crucial to have a cost-effective method of understanding where concentrations of geothermal water are located as well as the preferential flow paths of the water in the subsurface. Such

166

Reconnaissance geophysical studies of the geothermal system in southern  

Open Energy Info (EERE)

geophysical studies of the geothermal system in southern geophysical studies of the geothermal system in southern Raft River Valley, Idaho Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: Reconnaissance geophysical studies of the geothermal system in southern Raft River Valley, Idaho Details Activities (4) Areas (1) Regions (0) Abstract: Gravity, aeromagnetic, and telluric current surveys in the southern Raft River have been used to infer the structure and the general lithology underlying the valley. The gravity data indicate the approximate thickness of the Cenozoic rocks and location of the larger normal faults, and the aeromagnetic data indicate the extent of the major Cenozoic volcanic units. The relative ellipse area contour map compiled from the telluric current survey generally conforms to the gravity map except for

167

Well casing-based geophysical sensor apparatus, system and method  

DOE Patents (OSTI)

A geophysical sensor apparatus, system, and method for use in, for example, oil well operations, and in particular using a network of sensors emplaced along and outside oil well casings to monitor critical parameters in an oil reservoir and provide geophysical data remote from the wells. Centralizers are affixed to the well casings and the sensors are located in the protective spheres afforded by the centralizers to keep from being damaged during casing emplacement. In this manner, geophysical data may be detected of a sub-surface volume, e.g. an oil reservoir, and transmitted for analysis. Preferably, data from multiple sensor types, such as ERT and seismic data are combined to provide real time knowledge of the reservoir and processes such as primary and secondary oil recovery.

Daily, William D. (Livermore, CA)

2010-03-09T23:59:59.000Z

168

An Integrated Traverse Planner and Analysis Tool for Planetary Exploration  

E-Print Network (OSTI)

Future planetary explorations will require surface traverses of unprecedented frequency, length, and duration. As a result, there is need for exploration support tools to maximize productivity, scientific return, and safety. ...

Johnson, Aaron William

169

ChemCam data abundant at Planetary Conference  

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

Mars Science Laboratory Curiosity rover ChemCam team will present more than two dozen posters and talks during the 44th Lunar and Planetary Science Conference. March 15, 2013 This...

170

A unified vision and inertial navigation system for planetary hoppers  

E-Print Network (OSTI)

In recent years, considerable attention has been paid to hopping as a novel mode of planetary exploration. Hopping vehicles provide advantages over traditional surface exploration vehicles, such as wheeled rovers, by ...

Steiner, Theodore J., III (Theodore Joseph)

2012-01-01T23:59:59.000Z

171

CURRICULUM VITAE TARJE NISSEN-MEYER address: ETH Zurich, Institute of Geophysics  

E-Print Network (OSTI)

CURRICULUM VITAE TARJE NISSEN-MEYER address: ETH Zurich, Institute of Geophysics Sonneggstrasse 5 of Geophysics, ETH Zurich, Switzerland 2008 - 2010 Postdoctoral Research Associate, Dept. of Geosciences, Institute of Geophysics, ETH Zurich 2008 ­ 2010 Ph.D. student co-superviser: Andrea Colombi, Percy Galvez

Nissen-Meyer, Tarje

172

Geological and geophysical studies of a geothermal area in the southern  

Open Energy Info (EERE)

Geological and geophysical studies of a geothermal area in the southern Geological and geophysical studies of a geothermal area in the southern Raft river valley, Idaho Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Proceedings: Geological and geophysical studies of a geothermal area in the southern Raft river valley, Idaho Details Activities (1) Areas (1) Regions (0) Abstract: areal geology; Cassia County Idaho; Cenozoic; clastic rocks; clasts; composition; conglomerate; economic geology; electrical methods; evolution; exploration; faults; folds; geophysical methods; geophysical surveys; geothermal energy; gravity methods; Idaho; igneous rocks; lithostratigraphy; magnetic methods; pyroclastics; Raft River Valley; resources; sedimentary rocks; seismic methods; stratigraphy; structural geology; structure; surveys; tectonics; United States; volcanic rocks

173

Radio Planetary Nebulae in the Magellanic Clouds  

E-Print Network (OSTI)

We report the extragalactic radio-continuum detection of 15 planetary nebulae (PNe) in the Magellanic Clouds (MCs) from recent Australia Telescope Compact Array+Parkes mosaic surveys. These detections were supplemented by new and high resolution radio, optical and IR observations which helped to resolve the true nature of the objects. Four of the PNe are located in the Small Magellanic Cloud (SMC) and 11 are located in the Large Magellanic Cloud (LMC). Based on Galactic PNe the expected radio flux densities at the distance of the LMC/SMC are up to ~2.5 mJy and ~2.0 mJy at 1.4 GHz, respectively. We find that one of our new radio PNe in the SMC has a flux density of 5.1 mJy at 1.4 GHz, several times higher than expected. We suggest that the most luminous radio PN in the SMC (N S68) may represent the upper limit to radio peak luminosity because it is ~3 times more luminous than NGC 7027, the most luminous known Galactic PN. We note that the optical diameters of these 15 MCs PNe vary from very small (~0.08 pc or ...

Filipovi?, M D; Reid, W A; Payne, J L; Parker, Q A; Crawford, E J; Boji?i?, I S; De Horta, A Y; Hughes, A; Dickel, J; Stootman, F

2009-01-01T23:59:59.000Z

174

Advanced forecast of coal seam thickness variation by integrated geophysical method in the laneway  

Science Journals Connector (OSTI)

Coal seam thickness variation has a direct relationship with coal mine design and mining, and the mutation locations of the thickness are generally the gas accumulation area. In order to justify the feasibility and validity of advanced forecast about the thickness change, we carried out geophysical numerical simulation. Utilizing generalized Radon transform migration, coal-rock interface can be identified with an error of less than 2%. By the calculation of 2.5D finite difference method, transient electric magnetic response characteristics of the thickness variation is conspicuous. In a coal mine the case study indicated that: the reflected wave energy anomaly offer interface information of the thickness change point; the apparent resistivity provide the physical index of the thick or thin coal seam area; synthesizing two kinds of information can predict the thickness variation tendency ahead of the driving face, which can ensure the safety of driving efficiency.

Wang Bo; Liu Sheng-dong; Jiang Zhi-hai; Huang Lan-ying

2011-01-01T23:59:59.000Z

175

Merging High Resolution Geophysical and Geochemical Surveys to Reduce  

Open Energy Info (EERE)

Merging High Resolution Geophysical and Geochemical Surveys to Reduce Merging High Resolution Geophysical and Geochemical Surveys to Reduce Exploration Risk at Glass Buttes, Oregon Geothermal Project Jump to: navigation, search Last modified on July 22, 2011. Project Title Merging High Resolution Geophysical and Geochemical Surveys to Reduce Exploration Risk at Glass Buttes, Oregon Project Type / Topic 1 Recovery Act: Geothermal Technologies Program Project Type / Topic 2 Validation of Innovative Exploration Technologies Project Description This program will combine detailed gravity, high resolution aeromagnetic, and LIDAR data, all of which will be combined for structural modeling, with hyperspectral data, which will identify and map specific minerals and mineral assemblages that may point to upflow zones. The collection of these surveys and analyses of the merged data and model will be used to site deeper slim holes. Slim holes will be flow tested to determine whether or not Ormat can move forward with developing this resource. An innovative combination of geophysical and geochemical tools will significantly reduce risk in exploring this area, and the results will help to evaluate the value of these tools independently and in combination when exploring for blind resources where structure, permeability, and temperature are the most pressing questions. The slim holes will allow testing of models and validation of methods, and the surveys within the wellbores will be used to revise the models and site production wells if their drilling is warranted.

176

Seismic petrophysics: An applied science for reservoir geophysics  

E-Print Network (OSTI)

Seismic petrophysics: An applied science for reservoir geophysics WAYNE D. PENNINGTON, Michigan a number of seismic attributes, using either prestack or poststack data, or even both in combination's intuition and, per- haps, wishful thinking, as a guide. This short paper introduces a new term "seismic

177

Deborah K. Smith Department of Geology and Geophysics, MS 22  

E-Print Network (OSTI)

Deborah K. Smith Department of Geology and Geophysics, MS 22 Woods Hole Oceanographic Institution: Jordan, T. H., H. W. Menard, and D.K. Smith, Density and size distribution of seamounts in the eastern. Smith, H. W. Menard, J. A. Orcutt and T. H. Jordan, Seismic reflection site survey: correlation

Smith, Deborah K.

178

High Precision Geophysics & Detailed Structural Exploration & Slim Well  

Open Energy Info (EERE)

Precision Geophysics & Detailed Structural Exploration & Slim Well Precision Geophysics & Detailed Structural Exploration & Slim Well Drilling Geothermal Project Jump to: navigation, search Last modified on July 22, 2011. Project Title High Precision Geophysics & Detailed Structural Exploration & Slim Well Drilling Project Type / Topic 1 Recovery Act: Geothermal Technologies Program Project Type / Topic 2 Validation of Innovative Exploration Technologies Project Description Existing geologic data show that the basalt has been broken by complex intersecting fault zones at the hot springs. Natural state hot water flow patterns in the fracture network will be interpreted from temperature gradient wells and then tested with moderate depth core holes. Production and injection well tests of the core holes will be monitored with an innovative combination of Flowing Differential Self-Potential (FDSP) and resistivity tomography surveys. The cointerpretation of all these highly detailed geophysical methods sensitive to fracture permeability patterns and water flow during the well tests will provide unprecedented details on the structures and flow in a shallow geothermal aquifer and support effective development of the low temperature reservoir and identification of deep up flow targets.

179

Geophysical Research Abstracts Vol. 12, EGU2010-11992, 2010  

E-Print Network (OSTI)

, geological maps were focussed on solid geology. Present societal needs increasingly require knowledge of regolith properties: superficial studies combining geology, geochemistry and geophysics become essential km. This method provides maps of potassium (K), uranium (U) and thorium (Th) which are the only

Paris-Sud XI, Université de

180

GFDLs ESM2 Global Coupled ClimateCarbon Earth System Models. Part I: Physical Formulation and Baseline Simulation Characteristics  

Science Journals Connector (OSTI)

The physical climate formulation and simulation characteristics of two new global coupled carbonclimate Earth System Models, ESM2M and ESM2G, are described. These models demonstrate similar climate fidelity as the Geophysical Fluid Dynamics ...

John P. Dunne; Jasmin G. John; Alistair J. Adcroft; Stephen M. Griffies; Robert W. Hallberg; Elena Shevliakova; Ronald J. Stouffer; William Cooke; Krista A. Dunne; Matthew J. Harrison; John P. Krasting; Sergey L. Malyshev; P. C. D. Milly; Peter J. Phillipps; Lori T. Sentman; Bonita L. Samuels; Michael J. Spelman; Michael Winton; Andrew T. Wittenberg; Niki Zadeh

2012-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Aerial remote sensing surveys, geophysical characterization. Final report  

SciTech Connect

The application of helicopter electromagnetic (HEM) and magnetic methods to the requirements of the environmental restoration of the Oak Ridge Reservation (ORR) demand the use of advanced, nontraditional methods of data acquisition, processing and interpretation. The cooperative study by the U.S. Geological Survey (USGS), Oak Ridge National Laboratory (ORNL), and University of California (UCB) has resulted in the planning and supervision of data acquisition, the development of tools for data processing and interpretation, and an intensive application of the methods developed. This final report consists of a series of publications which the USGS collaborated with the ORNL technical staff. These reports represent the full scope of the USGS assistance. Copies of the reports and papers are included in the Appendix. The primary goals of this effort were to quantify the effectiveness of the geophysical methods applied in the survey of the ORR for the identification of buried waste, hydrogeologic pathways by which contamination could migrate through or off the site, and for the more accurate geologic mapping of the ORR. The objectives in buried waste identification are the accurate description of the source of the geophysical anomaly and the determination of the limits of resolution of the geophysical methods to acknowledge what we might have missed. The study of hydrogeologic pathways concentrated on the identification of karst features in the limestone underlying much of the ORR. Work in this study has indicated to the ORNL staff that these karst features can be located from the airborne geophysics. The defining characteristic of this helicopter geophysical study is the collaborative nature of the effort. Each task in which the USGS was involved has included a designated staff member from the Oak Ridge National Laboratory.

Labson, V.F.; Pellerin, L.; Anderson, W.L.

1998-06-01T23:59:59.000Z

182

Core Analysis For The Development And Constraint Of Physical Models Of  

Open Energy Info (EERE)

For The Development And Constraint Of Physical Models Of For The Development And Constraint Of Physical Models Of Geothermal Reservoirs Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Report: Core Analysis For The Development And Constraint Of Physical Models Of Geothermal Reservoirs Details Activities (2) Areas (2) Regions (0) Abstract: Effective reservoir exploration, characterization, and engineering require a fundamental understanding of the geophysical properties of reservoir rocks and fracture systems. Even in the best of circumstances, spatial variability in porosity, fracture density, salinity, saturation, tectonic stress, fluid pressures, and lithology can all potentially produce and/or contribute to geophysical anomalies. As a result, serious uniqueness problems frequently occur when interpreting

183

Hierarchical aggregation in percolation model  

E-Print Network (OSTI)

a Institute of Geophysics and Planetary Physics, University of California Los ... constitutive set of a few fundamental equations. .... The connecting node of the tree in this case does ...... International Handbook of Earthquake and Engineering

2006-01-17T23:59:59.000Z

184

JOURNAL OF MATHEMATICAL PHYSICS 54, 123303 (2013) A stochastic perturbation theory for non-autonomous  

E-Print Network (OSTI)

JOURNAL OF MATHEMATICAL PHYSICS 54, 123303 (2013) A stochastic perturbation theory for non-autonomous order nonlinear non-autonomous stochastic ordinary differential equations that arise in climate physics be autonomous or non-autonomous (see Refs. 3 a)Present address: Institute of Theoretical Geophysics, Department

Wettlaufer, John S.

185

History of geophysical studies at the Waste Isolation Pilot Plant (WIPP), southeastern New Mexico  

SciTech Connect

A variety of geophysical methods including the spectrum of seismic, electrical, electromagnetic and potential field techniques have supported characterization, monitoring and experimental studies at the Waste Isolation Pilot Plant (WIPP). The geophysical studies have provided significant understanding of the nature of site deformation, tectonics and stability. Geophysical methods have delineated possible brine reservoirs beneath the underground facility and have defined the disturbed rock zone that forms around underground excavations. The role of geophysics in the WIPP project has evolved with the project. The early uses were for site characterization to satisfy site selection criteria or factors. As the regulatory framework for WIPP grew since 1980, the geophysics program supported experimental and field programs such as Salado hydrogeology and underground room systems and excavations. In summary, the major types of issues that geophysical studies addressed for WIPP are: Site Characterization; Castile Brine Reservoirs; Rustler/Dewey Lake Hydrogeology; Salado Hydrogeology; and Excavation Effects. The nature of geophysics programs for WIPP has been to support investigation rather than being the principal investigation itself. The geophysics program has been used to define conceptual models (e.g., the Disturbed Rock Zone-DRZ) or to test conceptual models (e.g., high transmissivity zones in the Rustler Formation). The geophysics program primarily supported larger characterization and experimental programs. Funding was not available for the complete documentation and interpretation. Therefore, a great deal of the geophysics survey information resides in contractor reports.

Borns, D.J. [Sandia National Labs., Albuquerque, NM (United States). Geophysics Dept.

1997-03-05T23:59:59.000Z

186

Optimizing the Ptolemaic Model of Planetary and Solar Motion  

E-Print Network (OSTI)

Ptolemy-s planetary model is an ancient geocentric astronomical model, describing the observed motion of the Sun and the planets. Ptolemy accounted for the deviations of planetary orbits from perfect circles by introducing two small and equal shifts into his model. We show that Ptolemy-s choice of shifts allowed him to approximate the true eccentricity of planetary orbits only in the first order, linear in eccentricity. We show that, if the shifts were tuned in the ratio 5/3, the model precision could be improved substantially, perhaps delaying its rejection. The best achievable precision is quadratic in eccentricities. Although, to achieve it fully, one would have to introduce Ptolemaic shifts in the epicycles as well as in deferents the planets.

Rushkin, Ilia

2015-01-01T23:59:59.000Z

187

E-Print Network 3.0 - aspherical planetary nebulae Sample Search...  

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

objects called planetary nebulae. M57 is located in Lyra, south of its brightest star Vega... ,300 light-years from Earth. It has a visual magnitude of 8.8. Planetary...

188

Mechanical alloying of Si and Ge in a planetary ball mill: Milling parameters and microscopic evolution of alloy formation  

SciTech Connect

The external parameters geometry and frequency of a planetary ball mill were adjusted in order to minimize the duration of mechanically induced Si-Ge alloy formation. Experimental results were compared with theoretical calculations on impact energies and milling power. It was found that a planetary ball mill with a ratio of the planetary to the system wheel`s frequency of {minus}3 delivers the best milling performance for vial sizes between 0.2 and 0.33 that of the system wheel size. Microstructural investigations on powder compacts revealed that a solid state diffusion mechanism of Ge into the harder Si seems to be the responsible process for realizing a homogeneous Si-Ge alloy. Crystallite sizes of the processed powders were 30 nm. The knowledge of the influence of external milling parameters on the comminution and alloying behavior of substances and the resulting internal structure of the processed ingots may help in a future correlation between thermoelectrical properties and microstructure. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

Schilz, J.; Pixius, K.; Amend, W. [Institute of Materials Research, German Aerospace Research Establishment (DLR), Linder Hoehe, 51147 Koehn (Germany); Plate, M.; Meyer, H. [Retsch Co., Rheinische Str. 36, 42781 Haan (Germany)

1994-08-10T23:59:59.000Z

189

Geophysical Characterization of a Geothermal System Neal Hot Springs,  

Open Energy Info (EERE)

Characterization of a Geothermal System Neal Hot Springs, Characterization of a Geothermal System Neal Hot Springs, Oregon, USA Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: Geophysical Characterization of a Geothermal System Neal Hot Springs, Oregon, USA Abstract Neal Hot Springs is an active geothermal area that is also the proposed location of a binary power plant, which is being developed by US Geothermal Inc. To date, two production wells have been drilled and an injection well is in the process of being completed. The primary goal of this field camp was to provide a learning experience for students studying geophysics, but a secondary goal was to characterize the Neal Hot Springs area to provide valuable information on the flow of geothermal fluids through the subsurface. This characterization was completed using a variety of

190

Borehole geophysics evaluation of the Raft River geothermal reservoir |  

Open Energy Info (EERE)

reservoir reservoir Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Book: Borehole geophysics evaluation of the Raft River geothermal reservoir Details Activities (1) Areas (1) Regions (0) Abstract: Borehole geophysics techniques were used in evaluating the Raft River geothermal reservoir to establish a viable model for the system. The assumed model for the hot water (145/sup 0/C) reservoir was a zone of higher conductivity, increased porosity, decreased density, and lower sonic velocity. It was believed that the long term contact with the hot water would cause alteration producing these effects. With this model in mind, cross-plots of the above parameters were made to attempt to delineate the reservoir. It appears that the most meaningful data include smoothed and

191

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF EARTH AND PLANETARY SCIENCES  

E-Print Network (OSTI)

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF EARTH AND PLANETARY SCIENCES Assistant Professor in Planetary Sciences The Department of Earth and Planetary Sciences at the University of California, Santa (tenure-track) level. Applicants' research should focus primarily on processes and bodies in this solar

California at Santa Cruz, University of

192

General overview of geophysical studies at Cerro Prieto  

SciTech Connect

Geophysical investigations by the CFE in the Mexicali Valley near the Cerro Prieto volcano began nearly 20 years ago. Initially, gravity and seismic refraction methods were used for structural information related to faults and basement configuration. Supplemented by ground magnetic and gravity measurements, the resistivity data are being interpreted to yield a detailed picture of the structure concealed by valley fill and to identify promising areas for future exploration. 18 refs.

Goldstein, N.E.; Razo, A.M.

1980-01-01T23:59:59.000Z

193

Geophysics-based method of locating a stationary earth object  

DOE Patents (OSTI)

A geophysics-based method for determining the position of a stationary earth object uses the periodic changes in the gravity vector of the earth caused by the sun- and moon-orbits. Because the local gravity field is highly irregular over a global scale, a model of local tidal accelerations can be compared to actual accelerometer measurements to determine the latitude and longitude of the stationary object.

Daily, Michael R. (Albuquerque, NM); Rohde, Steven B. (Corrales, NM); Novak, James L. (Albuquerque, NM)

2008-05-20T23:59:59.000Z

194

An Integrated Model For The Geothermal Field Of Milos From Geophysical  

Open Energy Info (EERE)

Milos From Geophysical Milos From Geophysical Experiments Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: An Integrated Model For The Geothermal Field Of Milos From Geophysical Experiments Details Activities (0) Areas (0) Regions (0) Abstract: The results of geophysical experiments carried out by eight teams on the island of Milos as part of an integrated project under the European Commission's geothermal R & D programme are considered. The combination of these data with earlier studies on the geology and geophysics of Milos allow the compilation of a possible model of the geothermal reservoir and its surroundings in the central eastern part of the island. The reservoir is fed by convection of hot fluids from a depth of several kilometres, but the geophysical data provide no strong support for the earlier hypothesis

195

Geophysical Fluid Dynamics Laboratory Portal | Data.gov  

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

Geophysical Fluid Dynamics Laboratory Portal Geophysical Fluid Dynamics Laboratory Portal Agriculture Community Menu DATA APPS EVENTS DEVELOPER STATISTICS COLLABORATE ABOUT Agriculture You are here Data.gov » Communities » Agriculture » Data Geophysical Fluid Dynamics Laboratory Portal Dataset Summary Description Output and documentation from a set of multi-century experiments performed using NOAA/GFDL's climate models. Users can download files, display data file attributes, and graphically display the data. Data sets include those from CM2.X experiments associated with the Intergovernmental Panel on Climate Change Assessment Report (IPCC) and the US Climate Change Science Program (US CCSP). Tags {climate,IPCC,CCSP,pressure,SLP," sea ice","upper-level winds",ozone,"meridional winds","zonal winds",u-wind,v-wind," carbon dioxide"," volcanic",aerosol,grids,"soil moisture"," IPCC",flux,"radiation flux",thickness,radiation,emissivity,longwave,sensible,"latent heat",downwelling,upwelling,temperature,convective,runoff,"water vapor",humidity,cloudiness,transport,"geopotential height",assimilation,salinity,evaporation,freshwater}

196

E-Print Network 3.0 - air force geophysics Sample Search Results  

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

(1,141) GEOCHEMISTRY & GEOPHYSICS (775... of sea surface temperature, sea ice, and night marine air temperature since the late nineteenth century Source: Jimenez, Jose-Luis -...

197

E-Print Network 3.0 - accurate world-wide geophysical Sample...  

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

of Edinburgh, EH9 3JW, UK Summary: the geophysical monitorability of injected supercritical CO2 stored in subsurface saline aquifers. We use... the information expected to be...

198

Time-lapse Joint Inversion of Geophysical Data and its Applications to Geothermal Prospecting  

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

Time-lapse Joint Inversion of Geophysical Data and its Applications to Geothermal Prospecting presentation at the April 2013 peer review meeting held in Denver, Colorado.

199

Jim Green, Kristen Erickson, Stephen Edberg NASA, Planetary Science  

E-Print Network (OSTI)

, Land, Rove, and Return Samples""Flyby, Orbit, Land, Rove, and Return Samples" NASA's 3 #12;2010 Year 4 EPOXI encounters Comet Hartley 2 * November 19 Launch of O/OREOS 2011 * Completed * February 14 Stardust NExT encounters comet Tempel 1 * March 7 ­ Planetary Science Decadal Survey released

200

EROSION AND DEPOSITION ON PLANETARY SURFACES BY WIND,  

E-Print Network (OSTI)

. · Huygens Probe landed near the equator by the edge of a dried up lake. ­ The ground was "squishy" · Cobbles;descent images #12;For the materials observed at the Huygens landing site, the minimum precipitation rate and periglacial features #12;#12;MINOR BODIES (ASTEROIDS, COMETS) ASTR/GEOL 5800 Planetary Surfaces & Interiors 24

Mojzsis, Stephen J.

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Ab initio theory of planetary materials Artem R. Oganov*, I  

E-Print Network (OSTI)

) density (r), and pressure (P) as a function of depth. Seismic tomography gives 3D-variations of seismicAb initio theory of planetary materials Artem R. Oganov*, I , G. David PriceII and Sandro Scandolo and Neptune), referring the reader to an excellent book [1] for more details. Internal structure For the Earth

Oganov, Artem R.

202

Calculation of Synthetic Ionizing Spectra for Planetary Nebulae  

E-Print Network (OSTI)

We present a new grid (solar and halo abundance ratios) of state-of-the-art fully line-blanketed NLTE model atmospheres which covers the parameter range of central stars of planetary nebulae. The grid is available at the WWW.

T. Rauch

2002-01-17T23:59:59.000Z

203

DEPARTMENT OF PHYSICS Physics 21900  

E-Print Network (OSTI)

DEPARTMENT OF PHYSICS Syllabus Physics 21900 Physics for Architecture Students Designation suggested material: Giancoli, Physics, Principles with Applications (6th ed.) (required), Prentice Hall Giancoli, Physics, Principles with Applications, Student Guide (6th ed.) (optional), Prentice Hall Course

Lombardi, John R.

204

DEPARTMENT OF PHYSICS Physics 20300  

E-Print Network (OSTI)

DEPARTMENT OF PHYSICS Syllabus Physics 20300 General Physics Designation: Required Undergraduate Catalog description: For majors in the life sciences (biology, medicine, dentistry, psychology, physical therapy) and for liberal arts students. Fundamental ideas and laws of physics from mechanics to modern

Lombardi, John R.

205

Northern Thailand Geophysics Field Camp: Overview of Activities Lee M. Liberty  

E-Print Network (OSTI)

Northern Thailand Geophysics Field Camp: Overview of Activities Lee M. Liberty Boise State and industries with communities in need using applied geophysics projects as a means to benefit people and the environment around the world. Our GWB project was developed to educate and connect local geophysicists

Barrash, Warren

206

Preliminary Characterization of a NAPL-Contaminated Site using Borehole Geophysical Techniques  

E-Print Network (OSTI)

preliminary results from an on-going geophysical investigation of the former DOE Pinel- las site, a site and side-effects from previous remediation activities. Continuing research at the Pinellas site will focus presents preliminary results from our on-going geophysical investigation of a former U.S. Department

Ajo-Franklin, Jonathan

207

Leveraging the power of local spatial autocorrelation in geophysical interpolative clustering  

Science Journals Connector (OSTI)

Nowadays ubiquitous sensor stations are deployed worldwide, in order to measure several geophysical variables (e.g. temperature, humidity, light) for a growing number of ecological and industrial processes. Although these variables are, in general, measured ... Keywords: Clustering, Geophysical data stream, Inverse distance weighting, Spatial autocorrelation

Annalisa Appice; Donato Malerba

2014-09-01T23:59:59.000Z

208

GEOCHEMISTRY, GEOPHYSICS, GEOSYSTEMS, VOL. ???, XXXX, DOI:10.1029/, The influence of non-uniform ambient noise on1  

E-Print Network (OSTI)

, Institute of Geophysics, ETH Zurich, Sonneggstrasse 5, Zurich, Switzerland. T. Nissen-Meyer, Institute of Geophysics, ETH Zurich, Sonneggstrasse 5, Zurich, Switzerland. Olaf Schenk, Institute of Computational of Geophysics, ETH Zurich, Sonneggstrasse 5, Zurich, Switzerland. 3 ISTEP, UMR 7193, UPMC Universite Paris 6

Paris-Sud XI, Université de

209

Geophysical logging case history of the Raft River geothermal system, Idaho  

Open Energy Info (EERE)

Geophysical logging case history of the Raft River geothermal system, Idaho Geophysical logging case history of the Raft River geothermal system, Idaho Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Report: Geophysical logging case history of the Raft River geothermal system, Idaho Details Activities (1) Areas (1) Regions (0) Abstract: Drilling to evaluate the geothermal resource in the Raft River Valley began in 1974 and resulted in the discovery of a geothermal reservoir at a depth of approximately 1523 m (500 ft). Several organizations and companies have been involved in the geophysical logging program. There is no comprehensive report on the geophysical logging, nor has there been a complete interpretation. The objectives of this study are to make an integrated interpretation of the available data and compile a case history. Emphasis has been on developing a simple interpretation

210

A Geothermal Field Model Based On Geophysical And Thermal Prospectings In  

Open Energy Info (EERE)

Model Based On Geophysical And Thermal Prospectings In Model Based On Geophysical And Thermal Prospectings In Nea Kessani (Ne Greece) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: A Geothermal Field Model Based On Geophysical And Thermal Prospectings In Nea Kessani (Ne Greece) Details Activities (0) Areas (0) Regions (0) Abstract: The present study completes a study by Thanassoulas et al. (1986) Geophys. Prosp.34, 83-97 and deals with geophysical exploration for geothermal resources in Nea Kessani area, NE Greece. The results of some deep electrical soundings (AB = 6000 m) with the interpretation of a gravity profile crossing the investigated area are considered together with thermal investigations. All subsequent information, along with the conclusions of an earlier paper dealing with a reconnaissance geophysical

211

Long-term planetary integration with individual time steps  

E-Print Network (OSTI)

We describe an algorithm for long-term planetary orbit integrations, including the dominant post-Newtonian effects, that employs individual timesteps for each planet. The algorithm is symplectic and exhibits short-term errors that are $O(\\epsilon\\Omega^2\\tau^2)$ where $\\tau$ is the timestep, $\\Omega$ is a typical orbital frequency, and $\\epsilon\\ll1$ is a typical planetary mass in solar units. By a special starting procedure long-term errors over an integration interval $T$ can be reduced to $O(\\epsilon^2\\Omega^3\\tau^2T)$. A sample 0.8 Myr integration of the nine planets illustrates that Pluto can have a timestep more than 100 times Mercury's, without dominating the positional error. Our algorithm is applicable to other $N$-body systems.

Prasenjit Saha; Scott Tremaine

1994-03-24T23:59:59.000Z

212

Planetary systems based on a quantum-like model  

E-Print Network (OSTI)

Planetary systems have their origin in the gravitational collapse of a cloud of gas and dust. Through a process of accretion, is formed a massive star and a disk of planetesimals orbiting the star. Using a formalism analogous to quantum mechanics (quantum-like model), the star-planetesimal system is described and the flow quantizing the gravitational field theoretical model parameters are obtained. Goodness of fit (chi-square) of the observed data with model quantum-like, to the solar system, satellites, exoplanets and protoplanetary disk around HL Tauri is determined. Shows that the radius, eccentricity, energy, angular momentum and orbital inclination of planetary objects formed take discrete values depending only on the mass star.

T., N Poveda; C, N Y Buitrago

2015-01-01T23:59:59.000Z

213

History of geophysical studies at the Waste Isolation Pilot Plant (WIPP), southeastern New Mexico  

SciTech Connect

A variety of geophysical methods including the spectrum of seismic, electrical, electromagnetic and potential field techniques have used support characterization, monitoring and experimental studies at the Waste Isolation Pilot Plant (WIPP). The geophysical studies have provided significant understanding of the nature of site deformation, tectonics and stability. Geophysical methods have delineated possible brine reservoirs beneath the underground facility and have defined the disturbed rock zone that forms around underground excavations. The role of geophysics in the WIPP project has evolved with the project. The early uses were for site characterization to satisfy site selection criteria or factors. As the regulatory framework for WIPP grew since 1980, the geophysics program was focused on support of experimental and field programs such as Salado hydrogeology and underground room systems and excavations. In summary, the major types of issues that geophysical studies addressed for WIPP are: Issue 1: Site Characterization; Issue 2: Castile Brine Reservoirs; Issue 3: Rustler /Dewey Lake Hydrogeology; Issue 4: Salado Hydrogeology; and Issue 5: Excavation Effects. The nature of geophysics program for WIPP has been to support investigation rather than being the principal investigation itself. The geophysics program has been used to define conceptual models (e.g., the Disturbed Rock Zone-DRZ) or to test conceptual models (e.g., high transmissivity zones in the Rustler Formation). An effect of being a support program is that as new project priorities arose the funding for the geophysics program was limited and withdrawn. An outcome is that much of the geophysics survey information resides in contractor reports since final interpretation reports were not funded.

Borns, D.J. [Sandia National Labs., Albuquerque, NM (United States)

1997-10-01T23:59:59.000Z

214

Cosmogonic aspects of the evolution of planetary systems  

SciTech Connect

Fundamental approaches to the problem of the formation of planetary and satellite systems are considered. Emphasis is placed on the hetegony principle and its proposed generalization to a formation principle including the central body, and a restricted actualistic principle. Relevant characteristic parameters (i.e., energy levels of orbits, mass distribution in satellite systems, and angular momentum) for identifying the formation processes are examined, and possible future planetological tasks that should be undertaken in the foregoing framework are discussed.

Stiller, H. (Deutsche Akademie der Wissenschaften, Forschungsbereich Geo- und Kosmoswissenschaften, Potsdam, East Germany); Moehlmann, D. (Deutsche Akademie der Wissenschaften, Zentralinstitut fuer Astrophysik, Potsdam, East Germany)

1981-01-01T23:59:59.000Z

215

@Why Physics Comprehensive Physics Major.  

E-Print Network (OSTI)

@Why Physics Comprehensive Physics Major. From the basic laws of physics to the resulting emergent behavior, physics studies what the universe is made of and how it works. As a Physics major that surrounds us, to the structure and evolution of the entire universe. We offer three degrees in Physics

Yoo, S. J. Ben

216

NASAs Space Lidar Measurements of Earth and Planetary Surfaces  

Science Journals Connector (OSTI)

This presentation will give an overview of history, ongoing work, and plans for using space lidar for measurements of planetary surfaces.

Abshire, James B

217

are exploring planet Earth is the part of earth science dealing with the physical processes and  

E-Print Network (OSTI)

GeoKids are exploring planet Earth Geophysics is the part of earth science dealing with the physical processes and characteristics of the Earth and its environment. Volcanism, earthquakes of earth processes. Children are fully involved in measuring processes, data collection, analysis

Brückl, Ewald

218

Physical response of mid-ocean ridge hydrothermal systems to local earthquakes  

E-Print Network (OSTI)

: Heat flow (benthic) and hydrothermal processes; 3035 Marine Geology and Geophysics: Midocean ridge processes; 8135 Tectonophysics: Hydrothermal systems (8424). Received 23 January 2004; Revised 9 July 2004Physical response of mid-ocean ridge hydrothermal systems to local earthquakes William S. D

Wilcock, William

219

Capabilities for measuring physical and chemical properties of rocks at high pressure  

SciTech Connect

The Experimental Geophysics Group of the Earth Sciences Department at Lawrence Livermore National Laboratory (LLNL) has experimental equipment that measures a variety of physical properties and phase equilibria and kinetics on rocks and minerals at extreme pressures (to 500 GPa) and temperatures (from 10 to 2800 K). These experimental capabilities are described in this report in terms of published results, photographs, and schematic diagrams.

Durham, W.B. (comp.)

1990-01-01T23:59:59.000Z

220

Paper Publishing is Here to Stay: The Cambridge Planetary Handbook by Michael E Bakich, 1999, Cambridge University Press, 19.95, hbk, ISBN 0 521 63280 3  

Science Journals Connector (OSTI)

......Stay: The Cambridge Planetary Handbook by Michael E Bakich, 1999...stay The Cambridge Planetary Handbook by Michael E Bakich, 1999...Bakich's Cambridge Planetary Handbook is a scholarly guide to the...presentations compare? What does the electronic presentation......

Sue Bowler

2000-04-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

DEPARTMENT OF PHYSICS Physics 32300  

E-Print Network (OSTI)

DEPARTMENT OF PHYSICS Syllabus Physics 32300 Quantum Mechanics for Engineers Designation: required for Physics majors in the Applied Physics Option Undergraduate Catalog description: Basic experiments, wave: Physics 20700 and 20800, Math 39100 and Math 39200 Textbook and other suggested material: Scherrer

Lombardi, John R.

222

DEPARTMENT OF PHYSICS Physics 42200  

E-Print Network (OSTI)

DEPARTMENT OF PHYSICS Syllabus Physics 42200 Biophysics Designation: Undergraduate Catalog and membranes. In depth study of the physical basis of selected systems including vision, nerve transmission. Prerequisites: Prereq.: 1 yr. of Math, 1 yr. of Physics (elective for Physics Majors and Biomedical Engineering

Lombardi, John R.

223

Research overview 2007 Department of Geophysics, belonging to the Faculty of Mathematics and Physics,  

E-Print Network (OSTI)

aspects. Research is tightly coupled with education at the bachelor, master and doctoral levels. In 2007 and applied geophysicists (Schlumberger Cambridge Research), studying microearthquakes induced by oil drilling

Cerveny, Vlastislav

224

Research overview 2005 Department of Geophysics, belonging to the Faculty of Mathematics and Physics, Charles  

E-Print Network (OSTI)

aspects. Research is tightly coupled with education at bachelor, master and doctoral levels. In 2005 Cambridge Research), studying microearthquakes induced by oil drilling. In 2005, we participated and prediction. Fruitful cooperation with several major oil companies, lasting since 1993, has continued in 2005

Cerveny, Vlastislav

225

Testing gravitational physics with superconducting gravimeters  

E-Print Network (OSTI)

Superconducting gravimeters are the most sensitive instruments to measure surface gravity changes at low frequencies. Currently, about twenty five superconducting gravimeters are operating in the world and their global network has been developed. We investigate possible applications of the superconducting gravimeters to tests of gravitational physics. Previous experimental searches for spatial anisotropies in the gravitational constant G and for gravitational waves, performed with gravimeters in 1960's to 1970's, can be improved by applications of the current superconducting gravimeters. Also, we describe other proposed applications of testing the universality of free-fall and searching for composition-dependent dilatonic waves, and discuss future works necessary for these geophysical tests.

Sachie Shiomi

2009-02-24T23:59:59.000Z

226

Geophysical investigation of concealed faults near Yucca Mountain, southwest Nevada  

SciTech Connect

Detailed gravity and ground magnetic data collected along surveyed traverses across Midway Valley, on the eastern flank of Yucca Mountain, Nevada reveal that these methods can be used to delineate concealed faults. These studies are part of an effort to evaluate faulting in the vicinity of the proposed surface facilities for a potential nuclear waste repository at Yucca Mountain. The largest gravity and magnetic anomaly in the vicinity of Midway Valley is associated with the Paintbrush fault on the west flank of Alice Ridge. Geophysical data infer a vertical offset of about 200 m (650 ft). Another prominent gravity and magnetic anomaly is associated with the Bow Ridge fault in the western part of Midway Valley.

Ponce, D.A. [Geological Survey, Menlo Park, CA (United States)

1993-12-31T23:59:59.000Z

227

Geophysical interpretation of the PASSCAL Ouachita experiment: southern part  

E-Print Network (OSTI)

'riends in this department for correcting my writting. TADLE OF' CONTENTS CIIAP'I'L'R Pnge I LNTRODUCTION ll ('L'OI. OCICAL SL'T'I'liVC III PREVIOUS STUDIES I V D A'I' f A C ( ) U I S I'I'10 N A N D P RO C E SS I iN G Dntn Acquisitioii Dntn Processing '. iIODI. 'I... the geophysical view point. The result is a two-dimensioanl velocity model that extends from the northern shot point 12 (lat. 33. 5'X. long. 93. 5"'Hr) to the southern shot point 19 (lat. 33'X, long. 93. 5" IF) and from sea level to a depth of about 34 km...

Wang, Wen-Kung

1989-01-01T23:59:59.000Z

228

Clean enough for industry? An airborne geophysical case study  

SciTech Connect

Data from two airborne geophysical surveys of the Department of Energy`s Oak Ridge Reservation (ORR) were extremely valuable in deciding whether a 1000-acre (400 hectare) parcel of the ORR should be released to the City of Oak Ridge for industrial development. Our findings, based on electromagnetic and magnetic data, were incorporated in the federally mandated Environmental Assessment Statement (EAS), and in general supported claims that this land was never used as a hazardous waste disposal site. We estimated the amount of iron required to produce each anomaly using a simple dipole model. All anomalies with equivalent sources greater than approximately 1000 kg of iron were checked in the field, and the source of all but one identified as either a bridge, reinforced concrete debris, or a similarly benign object. Additionally, some smaller anomalies (equivalent sources of roughly 500 kg) have been checked; thus far, these also have innocuous sources. Airborne video proved invaluable in identifying logging equipment as the source of some of these anomalies. Geologic noise may account for some of the remaining anomalies. Naturally occurring accumulations of magnetic minerals in the soil on the ORR have been shown to produce anomalies which, at a sensor height of 30 m, are comparable to the anomaly produced by about 500 kg of iron. By comparison, the electronic noise of the magnetic gradiometer, 0.01--0.02 nT/m, is equivalent to only about 50--100 kg of iron at a 30 m sensor height. The electromagnetic data, combined with field mapping of karst structures, provided evidence of a northeast-southwest striking conduit spanning the parcel. The possible existence of a karst conduit led the EAS authors to conclude that this is a ``sensitive hydrologic setting.`` We conclude that aerial geophysics is an extremely cost-effective, and efficient technique for screening large tracts of land for environmental characterization.

Nyquist, J.E.; Beard, L.P.

1996-02-01T23:59:59.000Z

229

Anisotropy and coherent vortex structures in planetary turbulence  

SciTech Connect

High-resolution numerical simulations were made of unforced, planetary-scale fluid dynamics. In particular, the simulation was based on the quasi-geostrophic equations for a Boussinesq fluid in a uniformly rotating and stably stratified environment, which is an idealization for large regions of either the atmosphere or ocean. The solutions show significant discrepancies from the long-standing theoretical prediction of isotropy. The discrepancies are associated with the self-organization of the flow into a large population of coherent vortices. Their chaotic interactions govern the subsequent evolution of the flow toward a final configuration that is nonturbulent.

McWilliams, J.C. (National Center for Atmospheric Research, Boulder, CO (United States)); Weiss, J.B. (Univ. of Colorado, Boulder, CO (United States)); Yavneh, I. (Technion, Hafia (Israel))

1994-04-15T23:59:59.000Z

230

ADVANCED RADIOISOTOPE HEAT SOURCE AND PROPULSION SYSTEMS FOR PLANETARY EXPLORATION  

SciTech Connect

The exploration of planetary surfaces and atmospheres may be enhanced by increasing the range and mobility of a science platform. Fundamentally, power production and availability of resources are limiting factors that must be considered for all science and exploration missions. A novel power and propulsion system is considered and discussed with reference to a long-range Mars surface exploration mission with in-situ resource utilization. Significance to applications such as sample return missions is also considered. Key material selections for radioisotope encapsulation techniques are presented.

R. C. O'Brien; S. D. Howe; J. E. Werner

2010-09-01T23:59:59.000Z

231

Upcoming Events | Princeton Plasma Physics Lab  

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

Upcoming Events Upcoming Events University Physics Events Upcoming Events Events Calendar Event Type - Any - Colloquia Conference Geophysical Fluid Dynamics Laboratory Open House Princeton University Research Seminar Science Education Science On Saturday Apply Reset There are no Ongoing Events. Check back soon! January 11, 2014, 9:00am to 11:00am MBG Auditorium Containing A Star On Earth: Understanding Turbulence At 100 Million Degrees Dr. Walter Guttenfelder, Research Physicist Princeton Plasma Physics Laboratory January 15, 2014, 4:00pm to 5:30pm MBG Auditorium COLLOQUIUM: The Global Carbon Cycle and Earth's Climate Professor David Archer University of Chicago January 18, 2014, 9:30am to 11:00am MBG Auditorium Physics of Cancer Professor Wolfgang Losert, Associate Professor, and Director, Partnership

232

LANL | Physics | High Energy Physics  

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

high energy physics frontiers as defined by the Department of Energy's Office of High Energy Physics. Exploring the intensity frontier On the trail of one of the greatest...

233

Geologic And Geophysical Evidence For Intra-Basin And Footwall Faulting At  

Open Energy Info (EERE)

Geophysical Evidence For Intra-Basin And Footwall Faulting At Geophysical Evidence For Intra-Basin And Footwall Faulting At Dixie Valley, Nevada Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Geologic And Geophysical Evidence For Intra-Basin And Footwall Faulting At Dixie Valley, Nevada Details Activities (1) Areas (1) Regions (0) Abstract: A 'nested graben' structural model, in which multiple faults successively displace rocks downward to the deepest part of the basin, is supported by recent field geologic analysis and correlation of results to geophysical data for Dixie Valley. Aerial photographic analysis and detailed field mapping provide strong evidence for a deep graben separated from the ranges to the east and west by multiple normal faults that affect the Tertiary/Quaternary basin-fill sediments. Correlation with seismic

234

Electromagnetic geophysics: Notes from the past and the road ahead | Open  

Open Energy Info (EERE)

Electromagnetic geophysics: Notes from the past and the road ahead Electromagnetic geophysics: Notes from the past and the road ahead Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Electromagnetic geophysics: Notes from the past and the road ahead Abstract During the last century, electrical geophysics has been transformed from a simple resistivity method to a modern technology that uses complex data-acquisition systems and high-performance computers for enhanced data modeling and interpretation. Not only the methods and equipment have changed but also our ideas about the geoelectrical models used for interpretation have been modified tremendously. This paper describes the evolution of the conceptual and technical foundations of EM methods. Author Michael S. Zhdanov Published Journal

235

Merging high resolution geophysical and geochemical surveys to reduce exploration risk at Glass Buttes, Oregon  

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

DOE Geothermal Technologies Peer Review - 2010. The primary objective of this project is to combine a suite of high resolution geophysical and geochemical techniques to reduce exploration risk by characterizing hydrothermal alteration, fault geometries and relationships.

236

Applying petroleum geophysics to astrophysics: Quantitative 4D seismic study of the solar interior  

E-Print Network (OSTI)

Applying petroleum geophysics to astrophysics: Quantitative 4D seismic study of another new branch of seismology recently developed in petroleum reservoir seismology is commonly known in the petroleum industry, differs from earlier

Crawford, Ian

237

A GEOLOGICAL AND GEOPHYSICAL STUDY OF THE BACA GEOTHERMAL FIELD, VALLES CALDERA, NEW MEXICO  

E-Print Network (OSTI)

Rio Arriba Counties, New Mexico. Union Oil Internal ReportGoil Company of California, and Public Service Company of New Mexico,New Mexico. Private geophysical survey for Union Oil Co.

Wilt, M.

2011-01-01T23:59:59.000Z

238

Geophysical applications of nuclear resonant spectroscopy Wolfgang Sturhahn and Jennifer M. Jackson*  

E-Print Network (OSTI)

Geophysical applications of nuclear resonant spectroscopy Wolfgang Sturhahn and Jennifer M. Jackson* 17th August 2007 Advanced Photon Source, Argonne National Laboratory, 9700 South Cass Ave, Argonne summarize recent developments of nuclear resonant spectroscopy methods like nuclear resonant inelastic x

Jackson, Jennifer M.

239

Geophysical Surveying with Marine Networked Mobile Robotic Systems: The WiMUST Project  

E-Print Network (OSTI)

Underwa- ter Sonar Technology) has been favorably evaluated by the European Commission and the project a group of research institutions, geophysical surveying com- panies and SMEs with a well proven track

Jesus, Sérgio M.

240

A GEOLOGICAL AND GEOPHYSICAL STUDY OF THE BACA GEOTHERMAL FIELD, VALLES CALDERA, NEW MEXICO  

E-Print Network (OSTI)

oil Company of California, and Public Service Company of New Mexico,Rio Arriba Counties, New Mexico. Union Oil Internal ReportGNew Mexico. Private geophysical survey for Union Oil Co.

Wilt, M.

2011-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Reduced rank filtering in chaotic systems with application in geophysical sciences  

E-Print Network (OSTI)

Recent technological advancements have enabled us to collect large volumes of geophysical noisy measurements that need to be combined with the model forecasts, which capture all of the known properties of the underlying ...

Ahanin, Adel, 1977-

2008-01-01T23:59:59.000Z

242

Assessment of various geophysical techniques for Plains Indian archaeological site investigations  

E-Print Network (OSTI)

of various geophysical techniques for non-intrusive location of Plains Indian archaeological features. Plains Indian cultural resources are being lost because of the rapidly eroding shorelines and the lack of a quick and cost-effective method for locating...

Klaff, Tamir Lee

2012-06-07T23:59:59.000Z

243

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

244

Electrical conductivity of continental lithospheric mantle from integrated geophysical and petrological modeling  

E-Print Network (OSTI)

Electrical conductivity of continental lithospheric mantle from integrated geophysical; published 11 October 2011. [1] The electrical conductivity of mantle minerals is highly sensitive, and compositional variations. The bulk electrical conductivity model has been integrated into the software package

Jones, Alan G.

245

Interactions between mantle plumes and mid-ocean ridges : constraints from geophysics, geochemistry, and geodynamical modeling  

E-Print Network (OSTI)

This thesis studies interactions between mid-ocean ridges and mantle plumes using geophysics, geochemistry, and geodynamical modeling. Chapter 1 investigates the effects of the Marion and Bouvet hotspots on the ultra-slow ...

Georgen, Jennifer E

2001-01-01T23:59:59.000Z

246

GRR/Section 4-AK-b - Geophysical Exploration Permit | Open Energy  

Open Energy Info (EERE)

4-AK-b - Geophysical Exploration Permit 4-AK-b - Geophysical Exploration Permit < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 4-AK-b - Geophysical Exploration Permit 04AKBGeophysicalExplorationPermit.pdf Click to View Fullscreen Contact Agencies Alaska Department of Natural Resources Alaska Division of Oil and Gas Regulations & Policies Alaska Statutes Alaska Administrative Code Triggers None specified Click "Edit With Form" above to add content 04AKBGeophysicalExplorationPermit.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative A Geophysical Exploration Permit is necessary for conducting seismic

247

Search for gravitational waves associated with the InterPlanetary Network short gamma ray bursts  

E-Print Network (OSTI)

Search for gravitational waves associated with the InterPlanetary Network short gamma ray bursts V with short gamma ray bursts detected by the InterPlanetary Network (IPN) during LIGO's fifth science run and Virgo's first science run. The IPN localisation of short gamma ray bursts is limited to extended error

California at Berkeley, University of

248

A dynamical stability study of Kepler Circumbinary planetary systems with one planet  

Science Journals Connector (OSTI)

......intrinsic interest, the study of such systems is an opportunity to test our understanding of planetary system formation and evolution...into formation studies in stellar binaries, which is also a test field for theories of planetary formation around single stars......

C. E. Chavez; N. Georgakarakos; S. Prodan; M. Reyes-Ruiz; H. Aceves; F. Betancourt; E. Perez-Tijerina

2015-01-01T23:59:59.000Z

249

Transient chaos and fractal structures in planetary feeding zones  

E-Print Network (OSTI)

The circular restricted three body problem is investigated in the context of accretion and scattering processes. In our model a large number of identical non-interacting mass-less planetesimals are considered in planar case orbiting a star-planet system. This description allows us to investigate in dynamical systems approach the gravitational scattering and possible captures of the particles by the forming planetary embryo. Although the problem serves a large variety of complex motion, the results can be easily interpreted because of the low dimensionality of the phase space. We show that initial conditions define isolated regions of the disk, where accretion or escape of the planetesimals occur, these have, in fact, a fractal structure. The fractal geometry of these "basins" implies that the dynamics is very complex. Based on the calculated escape rates and escape times, it is also demonstrated that the planetary accretion rate is exponential for short times and follows a power-law for longer integration. A new numerical calculation of the maximum mass that a planet can reach (described by the expression of the isolation mass) is also derived.

Tams Kovcs; Zsolt Regly

2014-12-03T23:59:59.000Z

250

Spectroscopic Coronagraphy for Planetary Radial Velocimetry of Exoplanets  

E-Print Network (OSTI)

We propose to apply the coronagraphic techniques to the spectroscopic direct detection of exoplanets via the Doppler shift of planetary molecular lines. Even for unresolved close-in planetary system, we show that a combination of a visible nuller and an extreme adaptive optics system can reduce photon noise of a main star and increases total signal-to-noise ratio of the molecular absorptions of exoplanetary atmosphere: it works as spectroscopic coronagraph. Assuming a 30 m telescope, we demonstrate the benefit of these high-contrast instruments for nearby close-in planets that mimic 55 Cnc b ($0.6 \\lambda/D$ of the angular separation in the K-band). We find that the tip-tilt error is the most crucial factor, however, low-order speckles also contribute to the noise. Assuming relatively conservative estimates for future wavefront control technique, the spectroscopic coronagraph can increase the contrast to $ \\sim 50-130$ times and enable us to obtain a $\\sim 3-6 $ times larger S/N for warm Jupiters and Neptunes...

Kawahara, Hajime; Matsuo, Taro; Kotani, Takayuki

2014-01-01T23:59:59.000Z

251

The frequency of planetary debris around young white dwarfs  

E-Print Network (OSTI)

(Abridged) We present the results of the first unbiased survey for metal pollution among H-atmosphere (DA) white dwarfs with cooling ages of 20-200 Myr and 17000K 0.8 Msun is found to be currently accreting, which suggests a large fraction are double-degenerate mergers, and the merger discs do not commonly reform large planetesimals or otherwise pollute the remnant. We reconfirm our previous finding that two white dwarf Hyads are currently accreting rocky debris. At least 27%, and possibly up to ~50%, of all white dwarfs with cooling ages 20-200 Myr are accreting planetary debris. At Teff > 23000K, the luminosity of white dwarfs is likely sufficient to vaporize circumstellar dust, and hence no stars with strong metal-pollution are found. However, planetesimal disruption events should occur in this cooling age and Teff range as well, and likely result in short phases of high mass transfer rates. It appears that the formation of rocky planetary material is common around 2-3 Msun late B- and A-type stars.

Koester, Detlev; Farihi, Jay

2014-01-01T23:59:59.000Z

252

Application of borehole geophysics to fracture identification and characterization in low porosity limestones and dolostones  

SciTech Connect

Geophysical logging was conducted in exploratory core holes drilled for geohydrological investigations at three sites used for waste disposal on the US Department of Energy's Oak Ridge Reservation. Geophysical log response was calibrated to borehole geology using the drill core. Subsequently, the logs were used to identify fractures and fractured zones and to characterize the hydrologic activity of such zones. Results of the study were used to identify zones of ground water movement and to select targets for subsequent piezometer and monitoring well installation. Neutron porosity, long- and short-normal resistivity, and density logs exhibit anomalies only adjacent to pervasively fractured zones and rarely exhibit anomalies adjacent to individual fractures, suggesting that such logs have insufficient resolution to detect individual fractures. Spontaneous potential, single point resistance, acoustic velocity, and acoustic variable density logs, however, typically exhibit anomalies adjacent to both individual fractures and fracture zones. Correlation is excellent between fracture density logs prepared from the examination of drill core and fractures identified by the analysis of a suite of geophysical logs that have differing spatial resolution characteristics. Results of the study demonstrate the importance of (1) calibrating geophysical log response to drill core from a site, and (2) running a comprehensive suite of geophysical logs that can evaluate both large- and small-scale rock features. Once geophysical log responses to site-specific geological features have been established, logs provide a means of identifying fracture zones and discriminating between hydrologically active and inactive fracture zones. 9 figs.

Haase, C.S.; King, H.L.

1986-01-01T23:59:59.000Z

253

DEPARTMENT OF PHYSICS Physics 35400  

E-Print Network (OSTI)

DEPARTMENT OF PHYSICS Syllabus Physics 35400 Electricity and Magnetism II Designation potentials and radiation, special relativity. 3 HR./WK.; 3 CR. Prerequisites: Prereq.: Physics 35300; pre- or coreq.: Math 39200 (required for Physics majors, except those in the Biomedical Option). Textbook

Lombardi, John R.

254

Chaotic dynamics in accelerator physics. [Dept. of Astrophysical, Planetary, and Atmospheric Sciences, Univ. of Colorado, Boulder  

SciTech Connect

Substantial progress was in several areas of accelerator dynamics. For developing understanding of longitudinal adiabatic dynamics, and for creating efficiency enhancements of recirculating free-electron lasers, was substantially completed. A computer code for analyzing the critical KAM tori that bound the dynamic aperture in circular machines was developed. Studies of modes that arise due to the interaction of coating beams with a narrow-spectrum impedance have begun. During this research educational and research ties with the accelerator community at large have been strengthened.

Cary, J.R.

1992-11-30T23:59:59.000Z

255

Physics Division: Subatomic Physics Group  

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

Subatomic Physics Subatomic Physics Physics home » Subatomic Physics Site Home About Us Groups Applied Modern Physics, P-21 Neutron Science and Technology, P-23 Plasma Physics, P-24 Subatomic Physics, P-25 CONTACTS Group Leader Jon Kapustinsky (Acting) Deputy Group Leader Andy Saunders Office Administration Irene Martinez Miquela Sanchez Group Office (505) 667-6941 Physics Links Jobs in Physics Human Resources Working at Los Alamos Los Alamos resources Who we are, what we do We conduct basic research in nuclear and particle physics, applying this expertise to solve problems of national importance. By pushing the limits of our understanding of the smallest building blocks of matter through diverse experiments probing aspects of subatomic reactions, we aim to provide a more thorough understanding of the basic

256

NATURE PHYSICS | VOL 9 | JUNE 2013 | www.nature.com/naturephysics 325 news & views  

E-Print Network (OSTI)

of emission can be envisaged, and have even been observed to occur naturally in outer space and in planetaryNATURE PHYSICS | VOL 9 | JUNE 2013 | www.nature.com/naturephysics 325 news & views LASERS Amplified atmospheres1,2 . For instance, stellar gases are known to emit surprisingly strong radiation on certain

Loss, Daniel

257

Electroweak Physics  

E-Print Network (OSTI)

Work on electroweak precision calculations and event generators for electroweak physics studies at current and future colliders is summarized.

W. Hollik

2005-01-26T23:59:59.000Z

258

Living Rev. Solar Phys., 5, (2008), 3 http://www.livingreviews.org/lrsp-2008-3 in solar physics  

E-Print Network (OSTI)

Living Rev. Solar Phys., 5, (2008), 3 http://www.livingreviews.org/lrsp-2008-3 in solar physics L I V I N G REVIEWS A History of Solar Activity over Millennia Ilya G. Usoskin Sodankyl¨a Geophysical here is a review of present knowledge of the long-term behavior of solar activity on a multi

Usoskin, Ilya G.

259

Laser Ranging for Gravitational, Lunar, and Planetary Science  

E-Print Network (OSTI)

More precise lunar and Martian ranging will enable unprecedented tests of Einstein's theory of General Relativity and well as lunar and planetary science. NASA is currently planning several missions to return to the Moon, and it is natural to consider if precision laser ranging instruments should be included. New advanced retroreflector arrays at carefully chosen landing sites would have an immediate positive impact on lunar and gravitational studies. Laser transponders are currently being developed that may offer an advantage over passive ranging, and could be adapted for use on Mars and other distant objects. Precision ranging capability can also be combined with optical communications for an extremely versatile instrument. In this paper we discuss the science that can be gained by improved lunar and Martian ranging along with several technologies that can be used for this purpose.

Stephen M. Merkowitz; Philip W. Dabney; Jeffrey C. Livas; Jan F. McGarry; Gregory A. Neumann; Thomas W. Zagwodzki

2007-12-20T23:59:59.000Z

260

Molecular line observations of proto-planetary nebulae  

E-Print Network (OSTI)

We present our recent results on mm-wave CO observations of proto-planetary nebulae. These include high-resolution interferometric maps of various CO lines in three well known bipolar PPNe: M1-92, M2-56 and OH231.8+4.2. The global properties of the high velocity molecular emission in post-AGB sources have been also studied, by means of high-sensitivity single dish observations of the J=1-0 and 2-1 lines of 12CO and 13CO. We discuss the implications of these results to constrain the origin of the post-AGB molecular high-velocity winds and the shaping of bipolar PPNe and PNe. In addition, we also present the results of an interferometric map of the molecular envelope around the luminous high-latitude star 89 Her, a low mass post-AGB source which is also a close binary system.

J. Alcolea; V. Bujarrabal; A. Castro-Carrizo; C. Sanchez Contreras; R. Neri; J. Zweigle

1999-10-05T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

An atlas of synthetic line profiles of planetary nebulae  

E-Print Network (OSTI)

We have constructed a grid of photoionization models of spherical, elliptical and bipolar planetary nebulae. Assuming different velocity fields, we have computed line profiles corresponding to different orientations, slit sizes and positions. The atlas is meant both for didactic purposes and for the interpretation of data on real nebulae. As an application, we have shown that line profiles are often degenerate, and that recovering the geometry and velocity field from observations requires lines from ions with different masses and different ionization potentials. We have also shown that the empirical way to measure mass-weighted expansion velocities from observed line widths is reasonably accurate if considering the HWHM. For distant nebulae, entirely covered by the slit, the unknown geometry and orientation do not alter the measured velocities statistically. The atlas is freely accessible from internet. The Cloudy_3D suite and the associated VISNEB tool are available on request.

C. Morisset; G. Stasinska

2008-01-31T23:59:59.000Z

262

MHD Stellar and Disk Winds: Application to Planetary Nebulae  

E-Print Network (OSTI)

MHD winds can emanate from both stars and surrounding accretion disks. It is of interest to know how much wind power is available and which (if either) of the two rotators dominates that power. We investigate this in the context of multi-polar planetary nebulae (PNe) and proto-planetary nebulae (PPNe), for which recent observations have revealed the need for a wind power source in excess of that available from radiation driving, and a possible need for magnetic shaping. We calculate the MHD wind power from a coupled disk and star, where the former results from binary disruption. The resulting wind powers depend only on the accretion rate and stellar properties. We find that if the stellar envelope were initially slowly rotating, the disk wind would dominate throughout the evolution. If the envelope of the star were rapidly rotating, the stellar wind could initially be of comparable power to the disk wind until the stellar wind carries away the star's angular momentum. Since an initially rapidly rotating star can have its spin and magnetic axes misaligned to the disk, multi-polar outflows can result from this disk wind system. For times greater than a spin-down time, the post-AGB stellar wind is slaved to the disk for both slow and rapid initial spin cases and the disk wind luminosity dominates. We find a reasonably large parameter space where a hybrid star+disk MHD driven wind is plausible and where both or either can account for PPNe and PNe powers. We also speculate on the morphologies which may emerge from the coupled system. The coupled winds might help explain the shapes of a number of remarkable multi-shell or multi-polar nebulae. Magnetic activity such as X-ray flares may be associated with the both central star and the disk and would be a valuable diagnostic for the dynamical role of MHD processes in PNe.

Eric G. Blackman; Adam Frank; Carl Welch

2000-05-12T23:59:59.000Z

263

The R/H SabvabaaA research hovercraft for marine geophysical work in the most inaccessible area of the Arctic Ocean  

Science Journals Connector (OSTI)

...research hovercraft for marine geophysical work in the...use of a hovercraft for marine geophysical, geological...installed, together with marine and aircraft VHF radios...water-cooled Deutz 440-hp diesel engine. About 40 of the power...

John K. Hall; Yngve Kristoffersen

264

Multi-geophysical Investigation of Geological Structures in a Pre-selected High-level Radioactive Waste Disposal Area in Northwestern China  

Science Journals Connector (OSTI)

...Science Foundation for funding support (no.-41104045...level radioactive waste disposal: Acta Geoscientica Sinica...geophysical studies at Yucca Mountain, Nevada and vicinity...potential radioactive waste disposal site: Geophysics, 65...

Zhiguo An; Qingyun Di; Ruo Wang; Miaoyue Wang

265

Geophysical Evidence through a CSAMT Survey of the Deep Geological Structure at a Potential Radioactive Waste Site at Beishan, Gansu, China  

Science Journals Connector (OSTI)

...Foundation for funding support (no...geophysical studies at Yucca Mountain, Nevada and vicinity...radioactive waste disposal site: Geophysics...waste (HLRW) disposal site in northwestern...models underground disposal waste disposal...

Zhiguo An; Qingyun Di; Changmin Fu; Cheng Xu; Bo Cheng

266

Geophysical review of Trans-Pecos area of west Texas  

SciTech Connect

The Trans-Pecos has intrigued and baffled the oil industry, and all exploratory efforts so far have remained fruitless. Our geophysical findings along with other geologic information allow us to analyze the overall hydrocarbon potential for this area. Gravity and magnetic data were helpful in regional mapping but were unreliable for localized information owing to numerous extrusive and intrusive rocks. Seismic mapping shows many undrilled structures. However, the success ratio for the structures already drilled is disappointing (e.g., on the Diablo platform, out of 22 structural leads, 11 have been drilled and all were dry, and in the Marfa basin 17 out of 41 leads were drilled without success). Results were similar in Salt-Flat graben. Many of these wells had good hydrocarbon shows and almost all yielded fresh water. Tectonically the area has undergone several periods of orogeny, the result of the latest being numerous Basin and Range faults. The area is still seismically active and shows appreciable geodetic movement. It is suggested that the traps were destroyed with subsequent leakage of hydrocarbon and repeated induction of fresh water. Trap destruction is apparently beyond the scope of seismic detection. The Chihuahua trough (US), in spite of many discouraging facts, such as high heat flow, thermal waters, etc, shows some promise because seismic data reveal large thrust anticlines in the lower Paleozoic rocks (approximately 15,000 ft) that are yet to be adequately tested. Other small undamaged stratigraphic traps (reefs, truncations, pinch-outs, etc) are possibly present and could be targets for future exploration.

Addy, S.K.; DeJong, H.W.; Whitney, G.W.; Worthington, R.E.

1985-02-01T23:59:59.000Z

267

The Young Sun and Its Influence on Planetary Atmospheres M. Gdel1,2  

E-Print Network (OSTI)

, and causing corresponding increases in temperature and the rate of nuclear fusion. At the same time, and hence the short-wavelength radiative input into planetary atmospheres diminished with time. (By contrast

Guedel, Manuel

268

An implementation of terrain geomorphing in the vertex shader for synthetic planetary surfaces  

E-Print Network (OSTI)

The purpose of this research is to develop the three-dimensional models of planetary surfaces which can be used in the test environments for the Vision-Based Navigation Systems' (VBNS) terrain recognition and navigation ...

Colagiovanni, Lawrence W. (Lawrence William)

2008-01-01T23:59:59.000Z

269

Planetary population synthesis coupled with atmospheric escape: a statistical view of evaporation  

E-Print Network (OSTI)

We apply hydrodynamic evaporation models to different synthetic planet populations that were obtained from a planet formation code based on a core-accretion paradigm. We investigated the evolution of the planet populations using several evaporation models, which are distinguished by the driving force of the escape flow (X-ray or EUV), the heating efficiency in energy-limited evaporation regimes, or both. Although the mass distribution of the planet populations is barely affected by evaporation, the radius distribution clearly shows a break at approximately 2 $R_{\\oplus}$. We find that evaporation can lead to a bimodal distribution of planetary sizes (Owen & Wu 2013) and to an "evaporation valley" running diagonally downwards in the orbital distance - planetary radius plane, separating bare cores from low-mass planet that have kept some primordial H/He. Furthermore, this bimodal distribution is related to the initial characteristics of the planetary populations because low-mass planetary cores can only acc...

Jin, Sheng; Parmentier, Vivien; van Boekel, Roy; Henning, Thomas; Ji, Jianghui

2014-01-01T23:59:59.000Z

270

Meteoritics & Planetary Science 38, Nr 6, 871885 (2003) Abstract available online at http://meteoritics.org  

E-Print Network (OSTI)

Meteoritics & Planetary Science 38, Nr 6, 871­885 (2003) Abstract available online at http://meteoritics.org 871 © Meteoritical Society, 2003. Printed in USA. Searching for the source regions of martian

Hamilton, Victoria E.

271

Dynamic Analysis of Wind Turbine Planetary Gears Using an Extended Harmonic Balance Approach: Preprint  

SciTech Connect

The dynamics of wind turbine planetary gears with gravity effects are investigated using an extended harmonic balance method that extends established harmonic balance formulations to include simultaneous internal and external excitations. The extended harmonic balance method with arc-length continuation and Floquet theory is applied to a lumped-parameter planetary gear model including gravity, fluctuating mesh stiffness, bearing clearance, and nonlinear tooth contact to obtain the planetary gear dynamic response. The calculated responses compare well with time domain integrated mathematical models and experimental results. Gravity is a fundamental vibration source in wind turbine planetary gears and plays an important role in system dynamics, causing hardening effects induced by tooth wedging and bearing-raceway contacts. Bearing clearance significantly reduces the lowest resonant frequencies of translational modes. Gravity and bearing clearance together lowers the speed at which tooth wedging occurs lower than the resonant frequency.

Guo, Y.; Keller, J.; Parker, R. G.

2012-06-01T23:59:59.000Z

272

A Comparison of Data Assimilation Methods Using a Planetary Geostrophic Model  

Science Journals Connector (OSTI)

Assimilating hydrographic observations into a planetary geostrophic model is posed as a problem in control theory. The cost functional is the sum of weighted model and data residuals. Model errors are assumed to be spatially correlated, and ...

Edward D. Zaron

2006-04-01T23:59:59.000Z

273

Development of a mechanical counter pressure Bio-Suit System for planetary exploration  

E-Print Network (OSTI)

Extra-vehicular activity (EVA) is critical for human spaceflight and particularly for human planetary exploration. The MIT Man Vehicle Laboratory is developing a Bio-Suit EVA System, based on mechanical counterpressure ...

Sim, Zhe Liang

2006-01-01T23:59:59.000Z

274

Expansion Parallax for the Compact Planetary Nebula M2-43  

E-Print Network (OSTI)

We present high quality radio continuum observations made with the Very Large Array (VLA) at 3.6 cm at two epochs toward the planetary nebula M2-43. The comparison of the two epochs, obtained with a time separation of 4.07 years, clearly shows the expansion of the planetary nebula with an angular rate of 0.61 +/- 0.09 mas/year.Assuming that the expansion velocity in the plane of the sky (determined from these measurements) and the expansion velocity in the line of sight (determined from optical spectroscopy available in the literature) are equal, we find a distance to the planetary nebula of 6.9 +/- 1.5 kpc. This is the largest distance for a planetary nebula measured up to now with this technique.

L. Guzman; Y. Gomez; L. F. Rodriguez

2006-02-19T23:59:59.000Z

275

Rough-terrain mobile robot planning and control with application to planetary exploration  

E-Print Network (OSTI)

Future planetary exploration missions will require mobile robots to perform difficult tasks in highly challenging terrain, with limited human supervision. Current motion planning and control algorithms are not well suited ...

Iagnemma, Karl David

2001-01-01T23:59:59.000Z

276

Parcel EulerianLagrangian fluid dynamics of rotating geophysical flows  

Science Journals Connector (OSTI)

...J. 1981 Hamiltonian field description of two-dimensional vortex fluids and guiding center plasmas. Plasma Physics Laboratory report, Princeton University. PPPL-1793, p. 20. Morrison, P.J 1998Hamiltonian description of the ideal...

2006-01-01T23:59:59.000Z

277

Physics Fellow  

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

as Institute of Physics Fellow January 18, 2011 LOS ALAMOS, New Mexico, January 18, 2011-Alan Bishop, Los Alamos National Laboratory's associate director for theory, simulation,...

278

A near-surface geophysical investigation of the effects of measured and repeated removal of overlying soil on instrument response  

E-Print Network (OSTI)

A geophysical survey presents many challenges. A scientist must be able to not only understand the theory and nature of the geophysics being applied but must also be able to identify features of interest in a dataset. It is also of extreme...

Long, Zachary Ryan

2005-11-01T23:59:59.000Z

279

EETD Researchers at the American Geophysical Union Meeting in San Francisco  

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

EETD Researchers at the American Geophysical Union Meeting in San Francisco EETD Researchers at the American Geophysical Union Meeting in San Francisco December 9-13 December 2013 A number of scientists from the Environmental Energy Technologies Division are presenting papers and posters at the American Geophysical Union Meeting next week in San Francisco. Here are brief descriptions of one talk and two posters by EETD scientists and their colleagues. For more information, go to the AGU meeting site at the link below, where you can look up presentations by scientists from EETD and other divisions of Lawrence Berkeley National Laboratory. Energy-Water Integrated Assessment of the Sacramento Area and a Demonstration of WEAP-LEAP Capability Poster Monday, December 9, 2013, 8 AM - 12 PM Hall A-C Moscone South Researchers from EETD and partner institutions report on a new basin-scale

280

A Geological And Geophysical Appraisal Of The Baca Geothermal Field, Valles  

Open Energy Info (EERE)

Geological And Geophysical Appraisal Of The Baca Geothermal Field, Valles Geological And Geophysical Appraisal Of The Baca Geothermal Field, Valles Caldera, New Mexico Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: A Geological And Geophysical Appraisal Of The Baca Geothermal Field, Valles Caldera, New Mexico Details Activities (10) Areas (2) Regions (0) Abstract: The Baca location #1 geothermal field is located in north-central New Mexico within the western half of the Plio-Pleistocene Valles Caldera. Steam and hot water are produced primarily from the northeast-trending Redondo Creek graben, where downhole temperatures exceed 260°C at depths of less than 2 km. Stratigraphically the reservoir region can be described as a five-layer sequence that includes Tertiary and Quaternary volcanic rocks, and Mesozoic and Tertiary sediments overlying Precambrian granitic

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Physical Properties of Gas Hydrates: A Review  

SciTech Connect

Methane gas hydrates in sediments have been studied by several investigators as a possible future energy resource. Recent hydrate reserves have been estimated at approximately 1016?m3 of methane gas worldwide at standard temperature and pressure conditions. In situ dissociation of natural gas hydrate is necessary in order to commercially exploit the resource from the natural-gas-hydrate-bearing sediment. The presence of gas hydrates in sediments dramatically alters some of the normal physical properties of the sediment. These changes can be detected by field measurements and by down-hole logs. An understanding of the physical properties of hydrate-bearing sediments is necessary for interpretation of geophysical data collected in field settings, borehole, and slope stability analyses; reservoir simulation; and production models. This work reviews information available in literature related to the physical properties of sediments containing gas hydrates. A brief review of the physical properties of bulk gas hydrates is included. Detection methods, morphology, and relevant physical properties of gas-hydrate-bearing sediments are also discussed.

Gabitto, Jorge [Prairie View A& M University; Tsouris, Costas [ORNL

2010-01-01T23:59:59.000Z

282

Space Research and Planetary Sciences Division of the  

E-Print Network (OSTI)

Research and Planetology Climate and Environmental Physics High Energy Physics Physikalisches Institut ray group is an independent sub-group but formally connected to the theoretical planetology group secretaries will provide you with the STADTANZEIGER (the local paper of the city of Bern) if you request them

Richner, Heinz

283

Probing long-period companions to planetary hosts. VLT and CFHT near infrared coronographic imaging surveys  

E-Print Network (OSTI)

We present the results of a deep imaging survey of stars surrounded by planets detected with the radial velocity technique. The purpose is to search for and to characterize long-period stellar and substellar companions. The sample contains a total of 26 stars, among which 6 exhibit additional radial velocity drifts. We used NACO, at the ESO Very Large Telescope, and PUEO-KIR, at the Candian French Hawaiian Telescope, to conduct a near-infrared coronographic survey with adaptive optics of the faint circumstellar environment of the planetary hosts. The domain investigated ranges between 0.1 to 15" (i.e. about 3 to 500 AU, according to the mean distance of the sample). The survey is sensitive to companions within the stellar and the substellar domains, depending on the distance to the central stars and on the star properties. The images of 14 stars do not reveal any companions once the field objects are removed. 8 stars have close potential companions that need to be re-observed within 1-2 years to check for physical companionship. 4 stars are surrounded by faint objects which are confirmed or very probable companions. The companion to HD13445 (Gliese 86) is already known. The HD196885 star is a new close visual binary system with a high probability of being bound. The 2 newly discovered companions, HD1237 B and HD27442 B, share common proper motions with the central stars. Orbital motion is detected for HD1237 B. HD1237 B is likely a low-mass M star, located at 70 AU (projected distance) from the primary. HD27442 B is most probably a white dwarf companion located at about 240 AU (projected distance).

G. Chauvin; A. -M. Lagrange; S. Udry; T. Fusco; F. Galland; D. Naef; J. -L. Beuzit; M. Mayor

2006-06-07T23:59:59.000Z

284

Age determination of the HR8799 planetary system using asteroseismology  

E-Print Network (OSTI)

Discovery of the first planetary system by direct imaging around HR8799 has made the age determination of the host star a very important task. This determination is the key to derive accurate masses of the planets and to study the dynamical stability of the system. The age of this star has been estimated using different procedures. In this work we show that some of these procedures have problems and large uncertainties, and the real age of this star is still unknown, needing more observational constraints. Therefore, we have developed a comprehensive modeling of HR8799, and taking advantage of its gamma Doradus-type pulsations, we have estimated the age of the star using asteroseismology. The accuracy in the age determination depends on the rotation velocity of the star, and therefore an accurate value of the inclination angle is required to solve the problem. Nevertheless, we find that the age estimate for this star previously published in the literature ([30,160] Myr) is unlikely, and a more accurate value ...

Moya, A; Barrado, D; Hernndez, A Garca; Aberasturi, M; Montesinos, B; Aceituno, F

2010-01-01T23:59:59.000Z

285

VISCOSITY IN PLANETARY RINGS WITH SPINNING SELF-GRAVITATING PARTICLES  

SciTech Connect

Using local N-body simulation, we examine viscosity in self-gravitating planetary rings. We investigate the dependence of viscosity on various parameters in detail, including the effects of particle surface friction. In the case of self-gravitating rings with low optical depth, viscosity is determined by particle random velocity. Inclusion of surface friction slightly reduces both random velocity and viscosity when particle random velocity is determined by inelastic collisions, while surface friction slightly increases viscosity when gravitational encounters play a major role in particle velocity evolution, so that viscous heating balances with increased energy dissipation at collisions due to surface friction. We find that including surface friction changes viscosity in dilute rings up to a factor of about two. In the case of self-gravitating dense rings, viscosity is significantly increased due to the effects of gravitational wakes, and we find that varying restitution coefficients also change viscosity in such dense rings by a factor of about two. We confirm that our numerical results for viscosity in dense rings with gravitational wakes can be well approximated by a semianalytic expression that is consistent with a previously obtained formula. However, we find that this formula seems to overestimate viscosity in dense rings far from the central planet, where temporary gravitational aggregates form. We derive semianalytic expressions that reproduce our numerical results well for the entire range of examined parameters.

Yasui, Yuki; Ohtsuki, Keiji [Department of Earth and Planetary Sciences, Kobe University, Kobe 657-8501 (Japan); Daisaka, Hiroshi [Graduate School of Commerce and Management, Hitotsubashi University, Tokyo 186-8601 (Japan)

2012-05-15T23:59:59.000Z

286

Hydrogen civilisation concept: historical and all-planetary aspects  

Science Journals Connector (OSTI)

This paper discusses the novel Hydrogen Civilisation (HyCi) concept of the International Association for Hydrogen Energy. The HyCi concept states that at this demanding period in history, humanity still has the ability to save the biosphere and make the continuation of the human race possible. This objective can be achieved only by way of all-planetary cooperation along the direction of the ecologically clean vector 'hydrogen energy ? hydrogen economy ? hydrogen civilisation'. The HyCi concept includes three constituent, mutually conditional parts: industrial??ecological, humanitarian??cultural and geopolitical??internationally legislative. The legislative??economical mechanism of the transition to HyCi is formulated, and the most important stages are indicated and discussed. Special attention is paid to the future noospheric role of the world scientific??cultural community, to the fundamental importance of purposeful forming 'hydrogen??ecological' mass consciousness, to the role and responsibility of international and regional legal and political organisations, national parliaments and governments.

Victor A. Goltsov; T. Nejat Veziroglu; Lyudmila F. Goltsova

2006-01-01T23:59:59.000Z

287

Probing AGB nucleosynthesis via accurate Planetary Nebula abundances  

E-Print Network (OSTI)

The elemental abundances of ten planetary nebulae, derived with high accuracy including ISO and IUE spectra, are analysed with the aid of synthetic evolutionary models for the TP-AGB phase. Model prescriptions are varied until we achieve the simultaneous reproduction of all elemental features, which allows placing important constraints on the characteristic masses and nucleosynthetic processes experienced by the stellar progenitors. First of all, it is possible to separate the sample into two groups of PNe, one indicating the occurrence of only the third dredge-up during the TP-AGB phase, and the other showing also the chemical signature of hot-bottom burning. The former group is reproduced by stellar models with variable molecular opacities (see Marigo 2002), adopting initial solar metallicity, and typical efficiency of the third dredge-up 0.3-0.4. The latter group of PNe, with extremely high He content 0.15 4.5-5.0 Mo) with LMC composition have suffered a number of very efficient, carbon-poor, dredge-up eve...

Marigo, P; Pottasch, S R; Tielens, A G G M; Wesselius, P R

2003-01-01T23:59:59.000Z

288

Probing AGB nucleosynthesis via accurate Planetary Nebula abundances  

E-Print Network (OSTI)

The elemental abundances of ten planetary nebulae, derived with high accuracy including ISO and IUE spectra, are analysed with the aid of synthetic evolutionary models for the TP-AGB phase. Model prescriptions are varied until we achieve the simultaneous reproduction of all elemental features, which allows placing important constraints on the characteristic masses and nucleosynthetic processes experienced by the stellar progenitors. First of all, it is possible to separate the sample into two groups of PNe, one indicating the occurrence of only the third dredge-up during the TP-AGB phase, and the other showing also the chemical signature of hot-bottom burning. The former group is reproduced by stellar models with variable molecular opacities (see Marigo 2002), adopting initial solar metallicity, and typical efficiency of the third dredge-up 0.3-0.4. The latter group of PNe, with extremely high He content 0.15TP-AGB progenitors (M > 4.5-5.0 Mo) with LMC composition have suffered a number of very efficient, carbon-poor, dredge-up events. Finally, the neon abundances of the He-rich PNe can be recovered by invoking a significant production of 22Ne during thermal pulses, which would imply a reduced role of the 22Ne(alpha,n)25Mg reaction as neutron source to the s-process nucleosynthesis in these stars.

P. Marigo; J. Bernard-Salas; S. R. Pottasch; A. G. G. M. Tielens; P. R. Wesselius

2003-07-11T23:59:59.000Z

289

Vol.3 No.10 October 2007 www.nature.com/naturephysics nature physics | vol 3 | oCToBER 2007  

E-Print Network (OSTI)

. Annual Subscription Rates: US/Canada US$2730 (Canada add 6% GST) (institutional/corporate), US$137 (Canada add 6% GST) (personal 1 year); US$94, (Canada add 6% GST) (student/post doc 1 year); UK physics | vol 3 | oCToBER 2007 contents PLANETARY DYNAMICS Does chaos reign in the outer Solar System

Loss, Daniel

290

New Geophysical Technique for Mineral Exploration and Mineral Discrimination Based on Electromagnetic Methods  

SciTech Connect

The research during the first two years of the project was focused on developing the foundations of a new geophysical technique for mineral exploration and mineral discrimination, based on electromagnetic (EM) methods. The developed new technique is based on examining the spectral induced polarization effects in electromagnetic data using effective-medium theory and advanced methods of 3-D modeling and inversion. The analysis of IP phenomena is usually based on models with frequency dependent complex conductivity distribution. In this project, we have developed a rigorous physical/mathematical model of heterogeneous conductive media based on the effective-medium approach. The new generalized effective-medium theory of IP effect (GEMTIP) provides a unified mathematical method to study heterogeneity, multi-phase structure, and polarizability of rocks. The geoelectrical parameters of a new composite conductivity model are determined by the intrinsic petrophysical and geometrical characteristics of composite media: mineralization and/or fluid content of rocks, matrix composition, porosity, anisotropy, and polarizability of formations. The new GEMTIP model of multi-phase conductive media provides a quantitative tool for evaluation of the type of mineralization, and the volume content of different minerals using electromagnetic data. We have developed a 3-D EM-IP modeling algorithm using the integral equation (IE) method. Our IE forward modeling software is based on the contraction IE method, which improves the convergence rate of the iterative solvers. This code can handle various types of sources and receivers to compute the effect of a complex resistivity model. We have demonstrated that the generalized effective-medium theory of induced polarization (GEMTIP) in combination with the IE forward modeling method can be used for rock-scale forward modeling from grain-scale parameters. The numerical modeling study clearly demonstrates how the various complex resistivity models manifest differently in the observed EM data. These modeling studies lay a background for future development of the IP inversion method, directed at determining the electrical conductivity and the intrinsic chargeability distributions, as well as the other parameters of the relaxation model simultaneously. The new technology introduced in this project can be used for the discrimination between uneconomic mineral deposits and the location of zones of economic mineralization and geothermal resources.

Michael S. Zhdanov

2009-03-09T23:59:59.000Z

291

Course MA59800: Numerical Simulation in Applied Geophysics. From the Mesoscale to the Macroscale.  

E-Print Network (OSTI)

Description Wave propagation is a common technique used in hydrocarbon exploration geophysics, mining and reservoir characterization and production, among other fields. Local variations in the fluid and solid gradients via a slow-wave diffusion process that can be analyzed using numerical experiments. Numerical rock

Santos, Juan

292

Charles A. Stock Research Oceanographer, NOAA/Geophysical Fluid Dynamics Laboratory  

E-Print Network (OSTI)

Change Impacts on Living Marine Resources", 2012 Ocean Sciences Meeting, Salt Lake City 2012-13 MemberCharles A. Stock Research Oceanographer, NOAA/Geophysical Fluid Dynamics Laboratory Princeton-mail: Charles.Stock@noaa.gov Education 2005 Ph.D., Woods Hole Oceanographic Institution/MIT Joint Program Civil

293

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, A bootstrap algorithm for deriving the1  

E-Print Network (OSTI)

-squares method combined13 with a bootstrap algorithm. Given a particular set of archeomagnetic data14 associated;X - 4 THEBAULT AND GALLET: A BOOTSTRAP ALGORITHM 2. Fundamentals We have a discrete set of data fGEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, A bootstrap algorithm for deriving the1

Thébault, Erwan

294

Carbon Sequestration and Its Role in the Global Carbon Cycle Geophysical Monograph Series 183  

E-Print Network (OSTI)

73 Carbon Sequestration and Its Role in the Global Carbon Cycle Geophysical Monograph Series 183. Blaine Metting2 The purpose of this chapter is to review terrestrial biological carbon sequestration Northwest National Laboratory, Richland, Washington, USA. #12;74 TERRESTRIAL BIOLOGICAL CARBON SEqUESTRATION

Pennycook, Steve

295

In this article, I suggest a new style of geophysics as a critical system, which  

E-Print Network (OSTI)

geophysics for the oil industry is that the high-resolution details of fluid-sat- urated reservoirs and rocks effects. Those proven to date include: (1) oil production that has been shown by Heffer et al the virtual reality!). We extract oil from an integrated crack-critical rock mass. Future advances depend

296

GEOPHYSICS & GEODYNAMICS D. McKenzie, J.A. Jackson, R.S. White, A. Deuss,  

E-Print Network (OSTI)

models based on land-, marine- and space-based observations. Theoretical and geophysical analyses. The COMET project on modelling and observation of earthquakes and tectonics has developed further our strong to regional investigations of large continental areas. This effort is coordinated within the COMET group (http://comet

Cambridge, University of

297

Major results of geophysical investigations at Yucca Mountain and vicinity, southern Nevada  

SciTech Connect

In the consideration of Yucca Mountain as a possible site for storing high level nuclear waste, a number of geologic concerns have been suggested for study by the National Academy of Sciences which include: (1) natural geologic and geochemical barriers, (2) possible future fluctuations in the water table that might flood a mined underground repository, (3) tectonic stability, and (4) considerations of shaking such as might be caused by nearby earthquakes or possible volcanic eruptions. This volume represents the third part of an overall plan of geophysical investigation of Yucca Mountain, preceded by the Site Characterization Plan (SCP; dated 1988) and the report referred to as the Geophysical White Paper, Phase 1, entitled Status of Data, Major Results, and Plans for Geophysical Activities, Yucca Mountain Project (Oliver and others, 1990). The SCP necessarily contained uncertainty about applicability and accuracy of methods then untried in the Yucca Mountain volcano-tectonic setting, and the White Paper, Phase 1, focused on summarization of survey coverage, data quality, and applicability of results. For the most part, it did not present data or interpretation. The important distinction of the current volume lies in presentation of data, results, and interpretations of selected geophysical methods used in characterization activities at Yucca Mountain. Chapters are included on the following: gravity investigations; magnetic investigations; regional magnetotelluric investigations; seismic refraction investigations; seismic reflection investigations; teleseismic investigations; regional thermal setting; stress measurements; and integration of methods and conclusions. 8 refs., 60 figs., 2 tabs.

Oliver, H.W.; Ponce, D.A. [eds.] [Geological Survey, Menlo Park, CA (United States); Hunter, W.C. [ed.] [Geological Survey, Denver, CO (United States). Yucca Mountain Project Branch

1995-12-31T23:59:59.000Z

298

American Geophysical Union Fall Meeting, San Francisco, 12/14/07 Analyzing Regional Climate Experiments  

E-Print Network (OSTI)

of future climate and produce high resolution climate change projections using multiple GCM/RCM simulations for weight- ing models and improved projections of regional climate and climate change. · RecognizingAmerican Geophysical Union Fall Meeting, San Francisco, 12/14/07 Analyzing Regional Climate

Sain, Steve

299

An edited version of this paper was published by AGU. Copyright 2005 American Geophysical Union.  

E-Print Network (OSTI)

Atlantic Ocean- Atmosphere Interaction, Geophysical Research Letters 32, L24619, doi: 10.1029/2005GL024871 et al., 2005 1 Observations of SST, Heat Flux and North Atlantic Ocean-Atmosphere Interaction# Na Wen is generated largely by the surface heat flux, and then forces the early winter atmosphere through the release

Wisconsin at Madison, University of

300

Global Land Ice Measurements from Space Publisher: Springer Praxis Books, Subseries: Geophysical Sciences  

E-Print Network (OSTI)

Global Land Ice Measurements from Space Publisher: Springer Praxis Books, Subseries: Geophysical perceptions about the importance of fluctuations of glaciers and ice sheets (Jeffrey S. Kargel) 1.1Early.2.2. Modern impacts of changing glaciers and ice sheets on people 0.2.3. Recent public perceptions about

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Optimisation of seismic network design: Application to a geophysical international lunar network  

E-Print Network (OSTI)

Optimisation of seismic network design: Application to a geophysical international lunar network. Informations about lunar seismicity and seismic subsurface models from the Apollo missions are used as a priori information in this study to optimise the geometry of future lunar seismic networks in order to best resolve

Sambridge, Malcolm

302

Geophysical Monitoring of Foam used to Deliver Remediation1 Treatments within the Vadose Zone2  

E-Print Network (OSTI)

for transport of pollutants from the ground surface37 to ground water. Contaminants in the vadose zone1 Geophysical Monitoring of Foam used to Deliver Remediation1 Treatments within the Vadose Zone2 3 amendments into the vadose zone for in situ11 remediation; it is an approach being considered for in situ

Hubbard, Susan

303

Geophysical constraints on contaminant transport modeling in a heterogeneous fluvial aquifer  

E-Print Network (OSTI)

of Geological Sciences, University of Alabama, Box 870338, Tuscaloosa, AL 35487, USA b Institute of Marine log­log relationship. Application of this relationship, using site-specific empirical constants supplemented with geophysical data at least as well as previous models of the site using purely hydrologic data

Zheng, Chunmiao

304

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. , XXXX, DOI:10.1029/, Magnetic Flux Emergence in the Sun  

E-Print Network (OSTI)

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. , XXXX, DOI:10.1029/, Magnetic Flux Emergence in the Sun V­dimensional evolution of solar eruptions as they leave the Sun and move into the interplanetary space. One of the most important processes, responsible for many dynamical phenomena ob­ served in the Sun, is the emergence

Sengun, Mehmet Haluk

305

GEON: Geophysical data add the 3rd dimension in geospatial studies  

E-Print Network (OSTI)

in the search for natural resources (water, oil, gas, minerals, geothermal energy). Such studies provide of Texas at El Paso, GEON and PACES Research Teams Abstract A major trend in GIS is the addition projects has required the development of many sophisticated tools to allow users to utilize geophysical

Kreinovich, Vladik

306

EMSL - physics  

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

physics en 15N2 formation and fast oxygen isotope exchange during pulsed 15N18O exposure of MnOxCeO2. http:www.emsl.pnl.govemslwebpublications15n2-formation-and-fast-oxygen-i...

307

Flavor Physics  

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

Flavor Physics and CP Violation Conference, Bled, 2007 1 The Search for e Oscillations at MiniBooNE H. A. Tanaka, for the MiniBooNE collaboration Department of...

308

Physical Scientist  

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

The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of...

309

Physical Scientist  

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

A successful candidate in this position will serve as the Senior Headquarters (HQ) Physical Scientist for the Carbon Storage Program. The Carbon Storage Program focuses on the development of...

310

Investigation of novel geophysical techniques for monitoring CO2 movement during sequestration  

SciTech Connect

Cost effective monitoring of reservoir fluid movement during CO{sub 2} sequestration is a necessary part of a practical geologic sequestration strategy. Current petroleum industry seismic techniques are well developed for monitoring production in petroleum reservoirs. The cost of time-lapse seismic monitoring can be born because the cost to benefit ratio is small in the production of profit making hydrocarbon. However, the cost of seismic monitoring techniques is more difficult to justify in an environment of sequestration where the process produces no direct profit. For this reasons other geophysical techniques, which might provide sufficient monitoring resolution at a significantly lower cost, need to be considered. In order to evaluate alternative geophysical monitoring techniques we have undertaken a series of numerical simulations of CO{sub 2} sequestration scenarios. These scenarios have included existing projects (Sleipner in the North Sea), future planned projects (GeoSeq Liberty test in South Texas and Schrader Bluff in Alaska) as well as hypothetical models based on generic geologic settings potentially attractive for CO{sub 2} sequestration. In addition, we have done considerable work on geophysical monitoring of CO{sub 2} injection into existing oil and gas fields, including a model study of the Weyburn CO{sub 2} project in Canada and the Chevron Lost Hills CO{sub 2} pilot in Southern California (Hoversten et al. 2003). Although we are specifically interested in considering ''novel'' geophysical techniques for monitoring we have chosen to include more traditional seismic techniques as a bench mark so that any quantitative results derived for non-seismic techniques can be directly compared to the industry standard seismic results. This approach will put all of our finding for ''novel'' techniques in the context of the seismic method and allow a quantitative analysis of the cost/benefit ratios of the newly considered methods compared to the traditional, more expensive, seismic technique. The Schrader Bluff model was chosen as a numerical test bed for quantitative comparison of the spatial resolution of various geophysical techniques being considered for CO{sub 2} sequestration monitoring. We began with a three dimensional flow simulation model provided by BP Alaska of the reservoir and developed a detailed rock-properties model from log data that provides the link between the reservoir parameters (porosity, pressure, saturations, etc.) and the geophysical parameters (velocity, density, electrical resistivity). The rock properties model was used to produce geophysical models from the flow simulations.

Hoversten, G. Michael; Gasperikova, Erika

2003-10-31T23:59:59.000Z

311

Physics Based on Physical Monism  

E-Print Network (OSTI)

Based on a physical monism, which holds that the matter and space are classified by not a difference of their kind but a difference of magnitude of their density, I derive the most fundamental equation of motion, which is capable of providing a deeper physical understanding than the known physics. For example, this equation answers to the substantive reason of movement, and Newton's second law, which has been regarded as the definition of force, is derived in a substantive level from this equation. Further, the relativistic energy-mass formula is generalized to include the potential energy term, and the Lorentz force and Maxwell equations are newly derived.

Seong-Dong Kim

2005-09-08T23:59:59.000Z

312

A physical model to estimate snowfall over land using AMSU-B observations  

E-Print Network (OSTI)

. Weinman,3 W. S. Olson,4,5 D.-E. Chang,6 G. Skofronick-Jackson,7 and J. R. Wang7 Received 26 February 2007.-J., J. A. Weinman, W. S. Olson, D.-E. Chang, G. Skofronick-Jackson, and J. R. Wang (2008), A physical; Skofronick-Jackson et al., 2004; Liu, 2004; Noh et al., JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113, D09201

Houze Jr., Robert A.

313

Geophysical Laboratory/CDAC*Geophysical Laboratory/CDAC* Carnegie Institution of WashingtonCarnegie Institution of Washington  

E-Print Network (OSTI)

advantages has been tapped for high-pressure geoscience · Brilliance · High energy · Energy resolution and bodies outside our solar system · New observations and space missions · Implications for life elsewhere, with the discovery..." The Physics of High Pressure" (1931). #12;2 x 2.5 mm diamonds Radial Energy (keV) Axial 2 mm

Hemley, Russell J.

314

Events Calendar | Princeton Plasma Physics Lab  

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

Events Calendar Events Calendar University Physics Events Upcoming Events Events Calendar Type of Event - Any - Colloquia Conference Geophysical Fluid Dynamics Laboratory Open House Princeton University Research Seminar Science Education Science On Saturday Apply COLLOQUIUM: "The Usefulness of Useless Knowledge": The History of the Institute for Advanced Study, Christine Di Bella, Institute for Advanced Study Wednesday, January 29, 2014 - 16:00 to 18:30 COLLOQUIUM: Addressing Big Data Challenges in Simulation-based Science, Professor Manish Prashar, Rutgers University Wednesday, January 22, 2014 - 16:00 to 17:30 COLLOQUIUM: The Global Carbon Cycle and Earth's Climate, Professor David Archer, University of Chicago Wednesday, January 15, 2014 - 16:00 to 17:30 COLLOQUIUM: On Tracing the Origins of the Solar Wind, Dr. Sarah McGregor,

315

REVIEW OF PARTICLE PHYSICS  

E-Print Network (OSTI)

ONLINE PARTICLE PHYSICS INFORMATION 1.3. Particle Physics Information Platforms . . . . . . . . .14. Particle Physics Education and Outreach

Beringer, Juerg

2013-01-01T23:59:59.000Z

316

Review of Particle Physics  

E-Print Network (OSTI)

11. Particle Physics Education Sites . . . . . . . . .ONLINE PARTICLE PHYSICS INFORMATION 1.11. Particle Physics Education Sites . . . . . . . . . . 12.

Nakamura, Kenzo

2010-01-01T23:59:59.000Z

317

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook  

E-Print Network (OSTI)

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook Edition 1.4 2007/2008 Contents 1 Introduction 7 1.1 Physics at Lancaster . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14 2 Organisation of Physics Teaching 15 2.1 Departmental Committees

Low, Robert

318

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook  

E-Print Network (OSTI)

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook For 3rd & 4th Year Students on Old . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 1.2 Points of contact within the Physics Department . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17 2 Physics at Lancaster 18 2.1 Pastoral Care and Development

Low, Robert

319

NAC Ad-Hoc Task Force on Planetary Defense August 17 and 20, 2010 1 NASA ADVISORY COUNCIL (NAC)  

E-Print Network (OSTI)

NAC Ad-Hoc Task Force on Planetary Defense August 17 and 20, 2010 1 NASA ADVISORY COUNCIL (NAC) Ad-Hoc Task Force on Planetary Defense MINUTES Meeting Date: August 17 and 20, 2010 AGENDA: · Ad-Hoc Task Force Final Report and Recommendations ATTENDING: Ad-Hoc Task Force: Tom Jones (Co-Chair), Rusty

Waliser, Duane E.

320

Physical Protection  

Directives, Delegations, and Requirements

This Manual establishes requirements for the physical protection of interests under the U.S. Department of Energys (DOEs) purview ranging from facilities, buildings, Government property, and employees to national security interests such as classified information, special nuclear material (SNM), and nuclear weapons. Cancels Section A of DOE M 470.4-2 Chg 1. Canceled by DOE O 473.3.

2009-07-23T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Physics Handbook  

Science Journals Connector (OSTI)

... mechanics, acoustics, optics, heat, electricity, magnetism and electro-magnetism, atomic and nuclear physics, and strength of materials, 120 to 128. Decimal numbers denote the sections and ... they should be recommended to use it with care and only in conjunction with other handbooks and encyclopaedias. The trouble is that too much has been attempted-a dictionary, ...

S. WEINTROUB

1968-10-19T23:59:59.000Z

322

The role of H3+in planetary atmospheres  

Science Journals Connector (OSTI)

...constituent of this atmospheric region a quarter...determining the thermal structure of the...consisting of plasma, physically coexist...Jupiter to the plasma sheet; this is...was in `quasi-thermal equilibrium...explain are the non-auroral temperatures...the equatorial plasma sheet. But rst...

2000-01-01T23:59:59.000Z

323

The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution  

E-Print Network (OSTI)

of fields in stellar physics benefit this extremely precise time-series photometry. CoRoT flies on PROTEUS of metallicity but also in terms of age, as thin and thick disk populations appear not mixed in exactly the same

Bordé, Pascal J.

324

Falsification Of The Atmospheric CO2 Greenhouse Effects Within The Frame Of Physics  

E-Print Network (OSTI)

The atmospheric greenhouse effect, an idea that authors trace back to the traditional works of Fourier 1824, Tyndall 1861 and Arrhenius 1896 and is still supported in global climatology essentially describes a fictitious mechanism in which a planetary atmosphere acts as a heat pump driven by an environment that is radiatively interacting with but radiatively equilibrated to the atmospheric system. According to the second law of thermodynamics such a planetary machine can never exist. Nevertheless, in almost all texts of global climatology and in a widespread secondary literature it is taken for granted that such mechanism is real and stands on a firm scientific foundation. In this paper the popular conjecture is analyzed and the underlying physical principles are clarified. By showing that (a) there are no common physical laws between the warming phenomenon in glass houses and the fictitious atmospheric greenhouse effects, (b) there are no calculations to determine an average surface temperature of a planet, ...

Gerlich, Gerhard

2007-01-01T23:59:59.000Z

325

Comprehensive Approaches to Multiphase Flows in Geophysics - Application to nonisothermal, nonhomogenous, unsteady, large-scale, turbulent dusty clouds I. Hydrodynamic and Thermodynamic RANS and LES Models  

SciTech Connect

The objective of this manuscript is to fully derive a geophysical multiphase model able to ''accommodate'' different multiphase turbulence approaches; viz., the Reynolds Averaged Navier-Stokes (RANS), the Large Eddy Simulation (LES), or hybrid RANSLES. This manuscript is the first part of a larger geophysical multiphase project--lead by LANL--that aims to develop comprehensive modeling tools for large-scale, atmospheric, transient-buoyancy dusty jets and plume (e.g., plinian clouds, nuclear ''mushrooms'', ''supercell'' forest fire plumes) and for boundary-dominated geophysical multiphase gravity currents (e.g., dusty surges, diluted pyroclastic flows, dusty gravity currents in street canyons). LES is a partially deterministic approach constructed on either a spatial- or a temporal-separation between the large and small scales of the flow, whereas RANS is an entirely probabilistic approach constructed on a statistical separation between an ensemble-averaged mean and higher-order statistical moments (the so-called ''fluctuating parts''). Within this specific multiphase context, both turbulence approaches are built up upon the same phasic binary-valued ''function of presence''. This function of presence formally describes the occurrence--or not--of any phase at a given position and time and, therefore, allows to derive the same basic multiphase Navier-Stokes model for either the RANS or the LES frameworks. The only differences between these turbulence frameworks are the closures for the various ''turbulence'' terms involving the unknown variables from the fluctuating (RANS) or from the subgrid (LES) parts. Even though the hydrodynamic and thermodynamic models for RANS and LES have the same set of Partial Differential Equations, the physical interpretations of these PDEs cannot be the same, i.e., RANS models an averaged field, while LES simulates a filtered field. In this manuscript, we also demonstrate that this multiphase model fully fulfills the second law of thermodynamics and fulfills the necessary requirements for a well-posed initial-value problem. In the next manuscripts, we will further develop specific closures for multiphase RANS, LES, and hybrid-LES.

S. Dartevelle

2005-09-05T23:59:59.000Z

326

Application of the Earth's Natural Electromagnetic Noise to Geophysical Prospecting and Seraching for Oil  

E-Print Network (OSTI)

When applying the Earth's natural pulse electromagnetic fields to geophysical prospecting one should take into account characteristics of their spatial and temporal variations. ENPEMF is known to include both pulses attributed to atmospheric thunderstorms and pulses generated in the lithosphere by mechanic-to-electric energy conversion in rocks. It is evident that the most valuable information on the geophysical structure of a certain area is obviously contained in pulses originated from this area. This article covers a method of recording spatial variations of the Earth's natural pulse electromagnetic fields which is able to take due account of spatial and temporal variations of EM fields and suits to reveal crustal structural and lithologic heterogeneities including hydrocarbon pools. We use a system of several stations recording the ENPEMF concurrently to erase the temporal variations from ENPEMF records and to sort out the pulses of local and remote origin. Some stations are fixed (reference) and record o...

Malyshkov, Sergey Yu; Gordeev, Vasily F; Shtalin, Sergey G; Polivach, Vitaly I; Bazhanov, Yury Yu; Hauan, Terje

2011-01-01T23:59:59.000Z

327

Interpretive geophysical fault map across the central block of Yucca Mountain, Nevada  

SciTech Connect

Geophysical data collected along 29 traverses across the central block of Yucca Mountain in southwest Nevada reveal anomalies associated with known fault sand indicate a number of possible concealed faults beneath the eastern flank of Yucca Mountain. Geophysical interpretations indicate that Midway Valley is characterized by several known and previously unknown faults, that the existence of the Yucca Wash fault is equivocal, and that the central part of the eastern flank of Yucca Mountain is characterized by numerous low-amplitude anomalies that probably reflect numerous small-scale faults. Gravity and magnetic data also reveal several large-amplitude anomalies that reflect larger-scale faulting along the margins of the central block.

Ponce, D.A.

1996-12-31T23:59:59.000Z

328

Application of high-resolution geophysical methods in submarine pipeline inspection  

Science Journals Connector (OSTI)

High-resolution marine geophysical equipment employed includes single beam echo sounder (SBES), multi-beam echo sounder (MBES), sub-bottom profiler (SBP) and side scan sonar (SSS). By employing SBES, the reflection curve in shallow water reveals the real condition of pipeline; while in deep water, the reflection or diffraction curve can't reveal the real condition. Compared with SBES, MBES is characterised by intuition, efficiency and high resolution. But the same as SBES, the beam angle affects its detecting ability seriously. As for the SBP, system employing Chirp technology can detect the buried conditions of pipelines. Ship speed and water depth can affect the detection. The SSS can detect the plane position, exposed height, spanning state and pipeline trench, but buried pipelines. In order to understand the whole in-situ conditions of submarine pipeline, multiple geophysical methods should be employed.

Lai Xianghua; Ye Yincan; Pan Guofu; Li Dong

2011-01-01T23:59:59.000Z

329

Experiments in Physics Physics 1291  

E-Print Network (OSTI)

of the Laboratory The laboratory experiments described in this manual are an important part of your physics course-3 Velocity, Acceleration, and g 35 1-4 Projectile Motion and Conservation of Energy 45 1-5 Conservation. Whenever possible, the material will have been discussed in lecture before you come to the laboratory

Columbia University

330

Experiments in Physics Physics 1291  

E-Print Network (OSTI)

and Conservation of Energy 97 1-9 Standing Waves 105 1-10 Specific Heat and Mechanical Equivalent of Heat 115 #12;#12;Introduction 1-0 General Instructions 1 Purpose of the Laboratory The laboratory experiments described in this manual are an important part of your physics course. Most of the experiments are designed to illustrate

Columbia University

331

Experiments in Physics Physics 1291  

E-Print Network (OSTI)

The laboratory experiments described in this manual are an important part of your physics course. Most-8 Projectile Motion and Conservation of Energy 97 1-9 Standing Waves 105 1-10 Specific Heat and Mechanical Equivalent of Heat 115 #12;#12;Introduction 1-0 General Instructions 1 Purpose of the Laboratory

Columbia University

332

Of Physics & Astronomy. MEDICAL PHYSICS  

E-Print Network (OSTI)

, Department of Cardiovascular Science: Academic contact: Dr John Fenner, O-floor, Room OU142 (Hallamshire of the University, and 0114 2713687 from outside, email j.w.fenner@sheffield.ac.uk Medical Physics office contact JWF - Dr John Fenner, Undergrad course director, RHH, O floor, OU142, Tel x 13687, j.w.fenner

Crowther, Paul

333

Physics Folklore  

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

Physics Folklore Physics Folklore By Lynne Zielinski       Sometime after World War II physicists began to change their way of giving names to theoretical ideas. Before then, new ideas were given titles such as "special relativity theory" or "neutrons." A precursor of the new kinds of names came in 1953 when Murray Gell-Mann and Kazuhiko Hishijima decided to name one of the properties of subatomic particles "strangeness." Gell-Mann accelerated the trend in 1961 by calling his group-theoretic way of explaining the properties of particles "The Eightfold Way." Gell-Mann's crazy names finally reached the consciousness of the general public in 1964 when he described the particles involved in the next stage of his thinking as "quarks." p. 508, source B

334

Crump Geyser: High Precision Geophysics & Detailed Structural Exploration & Slim Well Drilling  

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

DOE Geothermal Peer Review 2010 - Presentation. Project objectives: Discover new 260F and 300F geothermal reservoirs in Oregon. To demonstrate the application of high precision geophysics for well targeting. Demonstrate a combined testing approach to Flowing Differential Self Potential (FDSP) and electrical tomography resistivity as a guide to exploration and development. Demonstrate utility and benefits of sump-less drilling for a low environmental impact. Create both short and long term employment through exploration, accelerated development timeline and operation.

335

Physical Protection  

Directives, Delegations, and Requirements

Establishes requirements for the physical protection of safeguards and security interests. Copies of Section B, Safeguards and Security Alarm Management System, which contains Unclassified Controlled Nuclear Information, and Appendix 1, Security Badge Specifications, which contains Official Use Only information, are only available, by request, from the program manager, Protection Program Operations, 301-903-6209. Cancels: DOE M 473.1-1 and DOE M 471.2-1B.

2005-08-26T23:59:59.000Z

336

Physical Protection  

Directives, Delegations, and Requirements

This Manual establishes requirements for the physical protection of safeguards and security interests. Copies of Section B, Safeguards and Security Alarm Management System, which contains Unclassified Controlled Nuclear Information, and Appendix 1, Security Badge Specifications, which contains Official Use Only information, are only available, by request, from the program manager, Protection Program Operations, 301-903-6209. Chg 1, dated 3/7/06. Cancels: DOE M 473.1-1 and DOE M 471.2-1B

2005-08-26T23:59:59.000Z

337

Highlights of the 2009 SEG summer research workshop on"CO2 Sequestration Geophysics"  

SciTech Connect

The 2009 SEG Summer Research Workshop on CO2 Sequestration Geophysics was held August 23-27, 2009 in Banff, Canada. The event was attended by over 100 scientists from around the world, which proved to be a remarkably successful turnout in the midst of the current global financial crisis and severe corporate travel restrictions. Attendees included SEG President Larry Lines (U. Calgary), and CSEG President John Downton (CGG Veritas), who joined SRW Chairman David Lumley (UWA) in giving the opening welcome remarks at the Sunday Icebreaker. The workshop was organized by an expert technical committee (see side bar) representing a good mix of industry, academic, and government research organizations. The format consisted of four days of technical sessions with over 60 talks and posters, plus an optional pre-workshop field trip to the Columbia Ice Fields to view firsthand the effects of global warming on the Athabasca glacier (Figures 1-2). Group technical discussion was encouraged by requiring each presenter to limit themselves to 15 minutes of presentation followed by a 15 minute open discussion period. Technical contributions focused on the current and future role of geophysics in CO2 sequestration, highlighting new research and field-test results with regard to site selection and characterization, monitoring and surveillance, using a wide array of geophysical techniques. While there are too many excellent contributions to mention all individually here, in this paper we summarize some of the key workshop highlights in order to propagate new developments to the SEG community at large.

Lumley, D.; Sherlock, D.; Daley, T.; Huang, L.; Lawton, D.; Masters, R.; Verliac, M.; White, D.

2010-01-15T23:59:59.000Z

338

Earth and Planetary Science Letters 390 (2014) 175185 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

of materials such as (Mg, Fe)SiO3 perovskite and post-perovskite found in D . However, the thermal conductivity. Historically, estimates of thermal conductivities at the CMB from low pres- sure or low temperature experimentsDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Variation of thermal conductivity

339

Year of the Solar System Planetary Science Mission Events as of 11/28/11  

E-Print Network (OSTI)

­ Lunar Reconnaissance Orbiter in PSD * November 4 - EPOXI encounters Comet Hartley 2 * November 19T encounters comet Tempel 1 * March 7 ­ Planetary Science Decadal Survey released * March 17 - MESSENGER orbit starts on its journey to Ceres August 5 - MSL lands on Mars * Completed http://solarsystem.nasa.gov #12;

Christian, Eric

340

Year of the Solar System Planetary Science Mission Events as of 08/09/11  

E-Print Network (OSTI)

­ Lunar Reconnaissance Orbiter in PSD * November 4 - EPOXI encounters Comet Hartley 2 * November 19T encounters comet Tempel 1 * March 7 ­ Planetary Science Decadal Survey released * March 17 - MESSENGER orbit journey to Ceres August 5 - MSL lands on Mars 1 * Completed http://solarsystem.nasa.gov #12;

Christian, Eric

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Year of the Solar System Planetary Science Mission Events as of 05/27/11  

E-Print Network (OSTI)

­ Lunar Reconnaissance Orbiter in PSD * November 4 - EPOXI encounters Comet Hartley 2 * November 19 - Stardust NExT encounters comet Tempel 1 * March 7 ­ Planetary Science Decadal Survey released * March 17 Vesta starts on its journey to Ceres August - MSL lands on Mars 1 * Completed http

Christian, Eric

342

Calculation of Planetary Precession from Quantum-corrected Newton's Gravitation Law  

E-Print Network (OSTI)

With consideration of quantization of space, we relate Newton's gravitation with the Second Law of thermodynamics. This leads to a correction to its original form, which takes into consideration the role of classical measurement. Our calculation shows this corrected form of gravitation can give explanation for planetary precession.

Zhen Wang

1998-04-29T23:59:59.000Z

343

Lattice Boltzmann solutions of the three-dimensional planetary geostrophic equations  

E-Print Network (OSTI)

Lattice Boltzmann solutions of the three-dimensional planetary geostrophic equations by Rick Salmon1 ABSTRACT We use the lattice Boltzmann method as the basis for a three-dimensional, numerical ocean. By the special nature of its construction,the lattice Boltzmann model resolves upwelling boundarylayers

Salmon, Rick

344

Improved Neutron-Capture Element Abundances in Planetary N. C. SterlingA,I  

E-Print Network (OSTI)

Improved Neutron-Capture Element Abundances in Planetary Nebulae N. C. SterlingA,I , H. L of neutron(n)-capture elements that cannot be detected in asymptotic giant branch (AGB) stars. However Approximately half of the neutron(n)-capture elements (atomic number Z > 30) in the Universe are created by slow

Royer, Dana

345

C.14 PLANETARY SCIENCE & TECHNOLOGY THROUGH ANALOG RESEARCH 1. Scope of Program  

E-Print Network (OSTI)

) Science Operations: PSTAR seeks systems-level terrestrial field campaigns which are conducted exploration requires the development of relevant, miniaturized instrumentation capable of extensive operations environments on Earth in order to develop a sound technical and scientific basis to conduct planetary research

Rathbun, Julie A.

346

Earth and Planetary Science Letters 404 (2014) 8997 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

M. Tikoo a,, Benjamin P. Weiss a , William S. Cassata b , David L. Shuster c,d , Jérôme Gattacceca a,e and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA g University of Hawaii at Manoa

Shuster, David L.

347

Stability of Earth-Mass Planets in the Habitable Zones of Extrasolar Planetary Systems  

E-Print Network (OSTI)

Stability of Earth-Mass Planets in the Habitable Zones of Extrasolar Planetary Systems Dr. Ravi Kumar Kopparapu Dept. of Geosciences, College of Earth and Mineral Science Over 500 planets orbiting and Saturn but in the last couple of years several "super-earths", planets with mass less than 10 times Earth

Bjørnstad, Ottar Nordal

348

EFFECT OF THE HADLEY CIRCULATION ON THE REFLECTION OF PLANETARY WAVES IN THREE-DIMENSIONAL  

E-Print Network (OSTI)

EFFECT OF THE HADLEY CIRCULATION ON THE REFLECTION OF PLANETARY WAVES IN THREE-equation model that includes a representation of the Hadley circulation. The Hadley circulation is forced symmetric component of the ow. To quantify the e#11;ect of the Hadley circulation on wave propagation

Magnusdottir, Gudrun

349

The Influence of Meridional Shear on Planetary Waves. Part 2: Critical Latitudes  

Science Journals Connector (OSTI)

With the simplifying assumption that the mean zonal wind is a function of latitude only, numerical and analytical methods are applied to study the effects of critical latitudes (where the Doppler-shifted frequency is 0) on planetary waves. On the ...

John P. Boyd

1982-04-01T23:59:59.000Z

350

The Influence of Meridional Shear on Planetary Waves. Part 1: Nonsingular Wind Profiles  

Science Journals Connector (OSTI)

Using a simple separable model in which the mean wind U(y) is assumed to be a function of latitude only, those effects of latitudinal shear which do not depend on the vanishing of U(y) are examined for planetary waves in the middle atmosphere (...

John P. Boyd

1982-04-01T23:59:59.000Z

351

Meteoritics & Planetary Science 38, Nr 2, 197224 (2003) Abstract available online at http://meteoritics.org  

E-Print Network (OSTI)

, New York 11235, USA; Department of Earth and Planetary Sciences, American Museum of Natural History, Central Park West, New York, New York 10024, USA; and Department of Geological Sciences, Rutgers-aluminum-rich inclusions (CAIs) were among the first igneous rocks produced within our solar system. These cm-sized spheres

Connolly Jr, Harold C.

352

TWO WIDE PLANETARY-MASS COMPANIONS TO SOLAR-TYPE STARS IN UPPER SCORPIUS  

SciTech Connect

At wide separations, planetary-mass and brown dwarf companions to solar-type stars occupy a curious region of parameter space not obviously linked to binary star formation or solar system scale planet formation. These companions provide insight into the extreme case of companion formation (either binary or planetary), and due to their relative ease of observation when compared to close companions, they offer a useful template for our expectations of more typical planets. We present the results from an adaptive optics imaging survey for wide ({approx}50-500 AU) companions to solar-type stars in Upper Scorpius. We report one new discovery of a {approx}14 M{sub J} companion around GSC 06214-00210and confirm that the candidate planetary-mass companion 1RXS J160929.1-210524 detected by Lafreniere et al. is in fact comoving with its primary star. In our survey, these two detections correspond to {approx}4% of solar-type stars having companions in the 6-20 M{sub J} mass and {approx}200-500 AU separation range. This figure is higher than would be expected if brown dwarfs and planetary-mass companions were drawn from an extrapolation of the binary mass function. Finally, we discuss implications for the formation of these objects.

Ireland, M. J. [Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006 (Australia); Kraus, A. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Martinache, F. [National Astronomical Observatory of Japan, Subaru Telescope, Hilo, HI 96720 (United States); Law, N. [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto M5S 3H4, Ontario (Canada); Hillenbrand, L. A. [Department of Astrophysics, California Institute of Technology, MC 105-24, Pasadena, CA 91125 (United States)

2011-01-10T23:59:59.000Z

353

Physics and Astronomy Engineering/Physics Concentration  

E-Print Network (OSTI)

Physics and Astronomy Engineering/Physics Concentration Strongly recommended courses Credits Term Electromagnetic Fields & Waves 3 PHY 3230 Thermal Physics 3 PHY 4020 Computational Methods in Physics.) taken Grade PHY 4620 Optics 4 PHY 3211 Modern Physics II 3 PHY 4730 Analog Circuits 3 PHY 4640 Quantum

Thaxton, Christopher S.

354

Physics and Astronomy Radiation Safety Physics Concentration  

E-Print Network (OSTI)

Physics and Astronomy Radiation Safety Physics Concentration Strongly recommended courses Credits Environucleonics Lab 1 PHY 3211 Modern Physics II 3 PHY 3230 Thermal Physics 3 PHY 4330 Digital Electronics 3 PHY 4820 Medical Physics 3 CHE 1101 Intro. Chemistry I 3 CHE 1110 Intro. Chemistry I Lab 1 CHE 1102 Intro

Thaxton, Christopher S.

355

PHYSICS OF BURNING PHYSICS INACCESSIBLE TO  

E-Print Network (OSTI)

PHYSICS OF BURNING PLASMAS: PHYSICS INACCESSIBLE TO PRESENT FACILITIES FIRE Physics Workshop May 2000 F. Perkins and N. Sauthoff Princeton Plasma Physics Laboratory FIRE Workshop 1 May 2000 #12;OUTLINE · Introduction · Three Classes of Burning Plasma Physics inaccessable to contemporary tokamak

356

Department of Physics Department of Physics  

E-Print Network (OSTI)

Department of Physics Department of Physics Life Sciences Building 3101 S. Dearborn St. Chicago, IL 60616 312.567.3480 www.iit.edu/csl/physics Chair: Grant Bunder The Department of Physics offers B.S., M.S., and Ph.D. degrees in physics. Within the department, there are many opportunities for interdisciplinary

Heller, Barbara

357

314 Department of Physics Department of Physics  

E-Print Network (OSTI)

314 Department of Physics Department of Physics Physics, one of the basic sciences, has its origin led to the detailed understanding of a remarkable variety of physical phenomena. Our knowledge now comprehension of the physical world forms an impressive part of the intellectual and cultural heritage of our

Nagle, John F.

358

Physics (Phys) (Department of Physics and Engineering)  

E-Print Network (OSTI)

229Physics Physics (Phys) (Department of Physics and Engineering) McCormick Foundation PROFESSORSILU INSTRUCTOR CUMMING VISITING PROFESSOR BOLLER MAJORS A major in physics leading to a Bachelor of Science degree requires completion of 50 credits including the following: 1. Physics 111, 112, 113, 114, 210, 215

Dresden, Gregory

359

Department of Physics Department of Physics  

E-Print Network (OSTI)

Department of Physics Department of Physics Life Sciences Building 3101 S. Dearborn St. Chicago, IL 60616 312.567.3480 www.iit.edu/csl/physics Chair: Christopher White The Department of Physics offers B.S., M.S., and Ph.D. degrees in physics. Within the department, there are many opportunities

Heller, Barbara

360

Large Scale Computing Requirements for Basic Energy Sciences (An BES / ASCR / NERSC Workshop) Hilton Washington DC/Rockville Meeting Center, Rockville MD 3D Geophysical Imaging  

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

Requirements Requirements for Basic Energy Sciences (An BES / ASCR / NERSC Workshop) Hilton Washington DC/Rockville Meeting Center, Rockville MD 3D Geophysical Modeling and Imaging G. A. Newman Lawrence Berkeley National Laboratory February 9 - 10 , 2010 Talk Outline * SEAM Geophysical Modeling Project - Its Really Big! * Geophysical Imaging (Seismic & EM) - Its 10 to 100x Bigger! - Reverse Time Migration - Full Waveform Inversion - 3D Imaging & Large Scale Considerations - Offshore Brazil Imaging Example (EM Data Set) * Computational Bottlenecks * Computing Alternatives - GPU's & FPGA's - Issues Why ? So that the resource industry can tackle grand geophysical challenges (Subsalt imaging, land acquisition, 4-D, CO2, carbonates ......) SEAM Mission Advance the science and technology of applied

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Blind Geothermal System Exploration in Active Volcanic Environments; Multi-phase Geophysical and Geochemical Surveys in Overt & Subtle Volcanic Systems, Hawaii & Maui  

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

DOE Geothermal Technologies Peer Review 2010 - Presentation. Project Objective: To use a combination of traditional geophysical and geochemical tools with exploration suites not typically used in geothermal exploration.

362

ARE PLANETARY SYSTEMS FILLED TO CAPACITY? A STUDY BASED ON KEPLER RESULTS  

SciTech Connect

We used a sample of Kepler candidate planets with orbital periods less than 200 days and radii between 1.5 and 30 Earth radii (R{sub Circled-Plus }) to determine the typical dynamical spacing of neighboring planets. To derive the intrinsic (i.e., free of observational bias) dynamical spacing of neighboring planets, we generated populations of planetary systems following various dynamical spacing distributions, subjected them to synthetic observations by the Kepler spacecraft, and compared the properties of observed planets in our simulations with actual Kepler detections. We found that, on average, neighboring planets are spaced 21.7 mutual Hill radii apart with a standard deviation of 9.5. This dynamical spacing distribution is consistent with that of adjacent planets in the solar system. To test the packed planetary systems hypothesis, the idea that all planetary systems are dynamically packed or filled to capacity, we determined the fraction of systems that are dynamically packed by performing long-term (10{sup 8} years) numerical simulations. In each simulation, we integrated a system with planets spaced according to our best-fit dynamical spacing distribution but containing an additional planet on an intermediate orbit. The fraction of simulations exhibiting signs of instability provides an approximate lower bound on the fraction of systems that are dynamically packed; we found that {>=}31%, {>=}35%, and {>=}45% of two-planet, three-planet, and four-planet systems are dynamically packed, respectively. Such sizeable fractions suggest that many planetary systems are indeed filled to capacity. This feature of planetary systems is another profound constraint that formation and evolution models must satisfy.

Fang, Julia; Margot, Jean-Luc [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)

2013-04-20T23:59:59.000Z

363

Physics Applications  

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

Applications Applications Technetium-99m radioisotope generator developed at Brookhaven. Numerous physics-related programs at Brookhaven have yielded major advances in medicine and various technologies. Brookhaven's nuclear medicine program, which began in the 1950s, uses the Brookhaven Linac Isotope Producer to make radioisotopes for nuclear medicine diagnostics and treatment throughout the world. Today, more than 85 percent of all imaging examinations worldwide use one of the radioisotopes developed at Brookhaven. At Brookhaven's Center for Translational Neuroimaging, researchers can peer into a living brain through the use of various imaging modalities, including positron emission tomography (PET), magnetic resonance imaging (MRI), and optical imaging. Such research has led to a new understanding of

364

Kaon physics  

E-Print Network (OSTI)

At present, the main topics addressed by kaon physics are the unitarity test of CKM matrix via precision measurements of the Cabibbo angle as well as precision tests of discrete symmetries: in particular, study of possible CPT violations in a model-independent way through the Bell-Steinberger relation, or through the measurement of charge asymmetries. Other interesting topics are related to the test of predictions from chiral perturbation theory. Also status and prospects of the $K^\\pm \\to \\pi^\\pm\

B. Sciascia

2006-10-14T23:59:59.000Z

365

Physics Topics - MST - UW Plasma Physics  

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

Physics Topics UW Madison Madison Symmetric Torus Physics Topics MST HomeGraduate Student InformationLinksTourControl and Auxiliary SystemsPhysics TopicsDeviceResearch MissionMST...

366

Particle Physics Booklet 2008  

E-Print Network (OSTI)

212 25. Accelerator physics of colliders ? 26. High-energythe full Review. PARTICLE PHYSICS BOOKLET TABLE OF CONTENTSrev. ) Summary Tables of Particle Physics Gauge and Higgs

et al., C. Amsler

2008-01-01T23:59:59.000Z

367

Center for Beam Physics  

E-Print Network (OSTI)

for Heavy Ion Fusion," Research Trends in Physics, La JollaInternational School of Physics, New York, New York (1992),Professor and Chairman Physics Department University of

Chattopadhyay, S.

2010-01-01T23:59:59.000Z

368

Research overview 2006 Department of Geophysics, belonging to the Faculty of Mathematics and Physics, Charles University in  

E-Print Network (OSTI)

aspects. Research is tightly coupled with education at the bachelor, master and doctoral levels. In 2006 microearthquakes induced by oil drilling. An important contribution related to our participation in the SPICE continued successfully in 2006. The project has been supported by 6 oil companies (BP America Inc., U

Cerveny, Vlastislav

369

International Union of Geodesy and Geophysics - Association of Seismology and The Physics of the Interior of the Earth  

Science Journals Connector (OSTI)

...seismoaraphs are in operation at the observatory...Mountain area are fairly cold. In the rugged area...Hallo Lagoon are in operation. Vol. XXI EARTHQUAKE...ionosphere specialists, a weather man, three glaciologists...comfortably at 70 by oil heaters. The men slapt two...every type. Hot and cold running water ware...

370

A multi-physics, integrated approach to formation evaluation using borehole geophysical measurements and 3D seismic data  

E-Print Network (OSTI)

in the immediate vicinity of the wellbore. Examples are shown of the estimation of porosity, absolute permeability, effective porosity, and absolute permeability. Similarly, sonic logs are used to assess mechanical, permeability anisotropy, and initial water saturation using combinations of electromagnetic logs, formation

Torres-Verdín, Carlos

371

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, A Physical Model for Seismic Noise Generation from Sediment  

E-Print Network (OSTI)

Generation from Sediment Transport in Rivers Victor C. Tsai1,2 , Brent Minchew1,2 , Michael P. Lamb2 , and Jean-Paul Ampuero1,2 Measuring sediment flux in rivers remains a significant problem in studies provide such mea- surements, but the lack of models linking observed seismic quan- tities to sediment flux

Ampuero, Jean Paul

372

Physics Illinois Undergraduate Programs  

E-Print Network (OSTI)

Physics Illinois Undergraduate Programs Department of Physics College of Engineering University to undergraduate education. Over the last 15 years, in collaboration with our nationally recognized Physics Education Research Group, our faculty has reinvented the way undergraduate physics courses are taught

Gilbert, Matthew

373

Physics 6321 Coastal oceanography  

E-Print Network (OSTI)

Physics 6321 Coastal oceanography · Instructor: Dr. Iakov Afanassiev · Office: Physics C-4065 · email: yakov@physics.mun.ca · Course Times: TBD Room TBD · Office Hours: unlimited · Web Page: http://www.physics

deYoung, Brad

374

Effect of the Hadley Circulation on the Reflection of Planetary Waves in Three-Dimensional Tropospheric Flows  

Science Journals Connector (OSTI)

The nonlinear behavior of quasi-stationary planetary waves excited by midlatitude orographic forcing is considered in a three-dimensional primitive equation model that includes a representation of the Hadley circulation. The Hadley circulation is ...

Christopher C. Walker; Gudrun Magnusdottir

2002-10-01T23:59:59.000Z

375

High Energy Physics  

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

Basic Energy Science Biological and Environmental Research Fusion Energy Sciences High Energy Physics Nuclear Physics Advanced Scientific Computing Research Pioneering...

376

People's Physics Book The People's Physics Book  

E-Print Network (OSTI)

#12;People's Physics Book The People's Physics Book Authors James H. Dann, Ph.D. James J. Dann. All rights reserved. Textbook Website http://scipp.ucsc.edu/outreach/index2.html #12;People's Physics) "Each discovery, each advance, each increase in the sum of human riches, owes its being to the physical

California at Santa Cruz, University of

377

Physics Procedia 00 (2013) 16 Physics Procedia  

E-Print Network (OSTI)

Physics Procedia 00 (2013) 1­6 Physics Procedia Educating the next generation of Computational Physicists Joan Adler Physics Department, Technion -IIT, Haifa, Israel, 32000 Abstract Many "senior" Computational Physics researchers began their careers perched on of the other vertices of the Landau triangle

Adler, Joan

378

People's Physics Book The People's Physics Book  

E-Print Network (OSTI)

People's Physics Book The People's Physics Book Authors James H. Dann, Ph.D. James J. Dann. All rights reserved. Textbook Website http://scipp.ucsc.edu/outreach/index2.html #12;People's Physics) "Each discovery, each advance, each increase in the sum of human riches, owes its being to the physical

California at Santa Cruz, University of

379

Physics and Astronomy Chemical Physics Concentration  

E-Print Network (OSTI)

Physics and Astronomy Chemical Physics Concentration Strongly recommended courses Credits Term Dept Fields & Waves 3 PHY 3230 Thermal Physics 3 PHY 4640 Quantum Mechanics 3 PHY 4020 Computational Methods in Physics & Engineering 3 PHY 4330 Digital Electronics 3 CHE 1101 Intro. Chemistry I 3 CHE 1110 Intro

Thaxton, Christopher S.

380

Physics Procedia 00 (2013) 15 Physics Procedia  

E-Print Network (OSTI)

Physics Procedia 00 (2013) 1­5 Physics Procedia Educating the next generation of Computational Physicists Joan Adler Physics Department, Technion -IIT, Haifa, Israel, 32000 Abstract Many "senior" Computational Physics researchers began their careers perched on of the other vertices of the Landau triangle

Adler, Joan

Note: This page contains sample records for the topic "geophysics planetary physics" 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

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook  

E-Print Network (OSTI)

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook For 4th Year Students only on Old Regulations Old Edition 1.1 2012/2013 1 #12;Contents 1 Introduction 6 1.1 Points of contact within the Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14 2 Physics at Lancaster 15 2.1 Pastoral Care and Development

Low, Robert

382

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook  

E-Print Network (OSTI)

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook For 1st & 2nd Year Students on New . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 1.2 Points of contact within the Physics Department . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 2 #12;2 Physics at Lancaster 26 2.1 Pastoral Care and Development

Low, Robert

383

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook  

E-Print Network (OSTI)

DEPARTMENT of PHYSICS Physics Undergraduate Courses Handbook For 1st , 2nd & 3rd Year Students . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12 1.2 Points of contact within the Physics Department . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 2 #12;2 Physics at Lancaster 26 2.1 Pastoral Care and Development

Low, Robert

384

LARGE SCALE CHANGES IN THE HIGHLY ENERGETIC CHARGED PARTICLES IN THE REGION OF THE IO TORUS  

E-Print Network (OSTI)

that they are caused by energetic trapped particles. On the C22 pass through the torus region the count rates were pass, the background count rate was low until inside the orbit of Io with a dip in the count rate 1 Institute of Geophysics and Planetary Physics, University of California Los Angeles, CA 90095

Russell, Christopher T.

385

Mirror Mode Structures in the Solar Wind: STEREO Observations  

E-Print Network (OSTI)

Mirror Mode Structures in the Solar Wind: STEREO Observations O. Enríquez-Rivera1 , X. Blanco-Cano1 Autónoma de México, Coyoacán, D.F., 04510, MEXICO 2. Institute of Geophysics and Planetary Physics of California, Berkeley, CA 94720, USA Abstract. Mirror mode structures occur in the solar wind either

California at Berkeley, University of

386

Fluid Imaging of Enhanced Geothermal Systems through Joint 3D Geophysical  

Open Energy Info (EERE)

Imaging of Enhanced Geothermal Systems through Joint 3D Geophysical Imaging of Enhanced Geothermal Systems through Joint 3D Geophysical Inverse Modeling Geothermal Lab Call Project Jump to: navigation, search Last modified on July 22, 2011. Project Title Fluid Imaging of Enhanced Geothermal Systems through Joint 3D Geophysical Inverse Modeling Project Type / Topic 1 Laboratory Call for Submission of Applications for Research, Development and Analysis of Geothermal Technologies Project Type / Topic 2 Fluid Imaging Project Description EGS has been defined as enhanced reservoirs that have been created to extract economical amounts of heat from low permeability and/or porosity geothermal resources. Critical to the success of EGS is the successful manipulation of fluids in the subsurface to enhance permeability. Knowledge in the change in volume and location of fluids in the rocks and fractures (both natural and induced) will be needed to manage injection strategies such as the number and location of step out wells, in-fill wells and the ratio of injection to production wells. The key difficulty in manipulating fluids has been our inability to reliably predict their locations, movements and concentrations. We believe combining data from MEQ and electrical surveys has the potential to overcome these problems and can meet many of the above needs, economically. Induced seismicity is currently viewed as one of the essential methods for inferring the success of creating fracture permeability and fluid paths during large scale EGS injections. Fluids are obviously playing a critical role in inducing the seismicity, however, other effects such as thermal, geochemical and stress redistribution, etc. may also play a role.

387

Fault diagnosis for wind turbine planetary gearboxes via demodulation analysis based on ensemble empirical mode decomposition and energy separation  

Science Journals Connector (OSTI)

Planetary gearboxes play an important role in wind turbine drive trains. Fault diagnosis of planetary gearboxes is a key topic for maintenance of wind turbines. Considering the spectral complexity of planetary gearbox vibration signals as well as their amplitude modulation and frequency modulation (AMFM) nature, we propose a simple yet effective method to diagnose planetary gearbox faults based on amplitude and frequency demodulations. We use the energy separation algorithm to estimate the amplitude envelope and instantaneous frequency of modulated signals for further demodulation analysis, by exploiting the adaptability of Teager energy operator to instantaneous changes in signals and the fine time resolution. However, the energy separation algorithm requires signals to be mono-components. To satisfy this requirement, we decompose signals into intrinsic mode functions (IMFs) using the ensemble empirical mode decomposition (EEMD) method as it can decompose any signal into mono-components. We further propose a criterion to guide the selection of the most relevant IMF for demodulation analysis according to the wavelet-like filter nature of EEMD and the AMFM characteristics of the planetary gearbox vibration signals. By matching the dominant peaks in the Fourier spectra of the obtained amplitude envelope and instantaneous frequency with the theoretical characteristic frequency of each gear, we can diagnose planetary gearbox faults. The principle and effectiveness of the proposed method are illustrated by simulation and the experimental analysis of signals from a planetary gearbox of a wind turbine test rig. With the proposed method, both the wear and chipping faults can be detected and located for a sun gear of the planetary gearbox test rig.

Zhipeng Feng; Ming Liang; Yi Zhang; Shumin Hou

2012-01-01T23:59:59.000Z

388

Southeast Asia applied geophysics workshop: Geoscientists without borders Lee M. Liberty*, Spencer H. Wood, Emily A. Hinz, and Dylan Mikesell, Boise State University, Fongsaward  

E-Print Network (OSTI)

Southeast Asia applied geophysics workshop: Geoscientists without borders Lee M. Liberty*, Spencer in need using applied geophysics projects as a means to benefit people and the environment around the world. Our project was developed to educate and connect local geophysicists and students in Southeast

Barrash, Warren

389

Student-based archaeological geophysics in northern Thailand Emily A. Hinz*, Lee M. Liberty, and Spencer H. Wood, Boise State University, Fongsaward Singharajawarapan  

E-Print Network (OSTI)

Student-based archaeological geophysics in northern Thailand Emily A. Hinz*, Lee M. Liberty participants to evaluate the practicality and effectiveness of various geophysical techniques: seismic methods including refraction and reflection (not discussed here), ground- penetrating-radar (GPR), DC resistivity

Barrash, Warren

390

Geological and geophysical investigation of the Mid-Cayman Spreading Centre: seismic velocity measurements and implications for the constitution of layer 3  

Science Journals Connector (OSTI)

......Geophysics of the Pacific Ocean Basin and its Margin, eds Sutton...velocities of rocks from the Ming's Bight-Betts Cove Ophiolite Complex...spreading rates, in marginal basins, at different distances from...Geophysics of the Pacific Ocean Basin and its Margin, eds Sutton......

J. A. Karson; P. J. Fox

1986-04-01T23:59:59.000Z

391

Averaging over fast gravity waves for geophysical flows with arbitrary potential vorticity  

SciTech Connect

Here a mathematically rigorous framework is developed for deriving new reduced simplified dynamical equations for geophysical flows with arbitrary potential vorticity interacting with fast gravity waves. The examples include the rotating Boussinesq and rotating shallow water equations in the quasigeostrophic limit with vanishing Rossby number. For the spatial periodic case the theory implies that the quasi-geostrophic equations are valid limiting equations in the weak topology for arbitrary initial data. Furthermore, simplified reduced equations are developed for the fashion in which the vortical waves influence the gravity waves through averaging over specific gravity wave/vortical resonances. 18 refs.

Embid, P.F. [Princeton Univ., NJ (United States); Majda, A.J. [New York Univ., New York, NY (United States)

1996-12-31T23:59:59.000Z

392

LOW Mg/Si PLANETARY HOST STARS AND THEIR Mg-DEPLETED TERRESTRIAL PLANETS  

SciTech Connect

Simulations have shown that a diverse range of extrasolar terrestrial planet bulk compositions are likely to exist based on the observed variations in host star elemental abundances. Based on recent studies, it is expected that a significant proportion of host stars may have Mg/Si ratios below 1. Here we examine this previously neglected group of systems. Planets simulated as forming within these systems are found to be Mg-depleted (compared to Earth), consisting of silicate species such as pyroxene and various feldspars. Planetary carbon abundances also vary in accordance with the host star C/O ratio. The predicted abundances are in keeping with observations of polluted white dwarfs, lending validity to this approach. Further studies are required to determine the full planetary impacts of the bulk compositions predicted here.

Carter-Bond, Jade C.; O'Brien, David P. [Planetary Science Institute, 1700 E. Fort Lowell, Tucson, AZ 85719 (United States); Delgado Mena, Elisa; Israelian, Garik; Gonzalez Hernandez, Jonay I. [Instituto de Astrofisica de Canarias, 38200 La Laguna, Tenerife (Spain); Santos, Nuno C., E-mail: j.bond@unsw.edu.au [Centro de Astrofisica, Universidade do Porto, Rua das Estrelas, 4150-762 Porto (Portugal)

2012-03-15T23:59:59.000Z

393

A DOUBLE PLANETARY SYSTEM AROUND THE EVOLVED INTERMEDIATE-MASS STAR HD 4732  

SciTech Connect

We report the detection of a double planetary system orbiting around the evolved intermediate-mass star HD 4732 from precise Doppler measurements at Okayama Astrophysical Observatory and Australian Astronomical Observatory. The star is a K0 subgiant with a mass of 1.7 M {sub Sun} and solar metallicity. The planetary system is composed of two giant planets with minimum mass of msin i = 2.4 M {sub J}, orbital period of 360.2 days and 2732 days, and eccentricity of 0.13 and 0.23, respectively. Based on dynamical stability analysis for the system, we set the upper limit on the mass of the planets to be about 28 M {sub J} (i > 5 Degree-Sign ) in the case of coplanar prograde configuration.

Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Nagasawa, Makiko; Ida, Shigeru [Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan)] [Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Wittenmyer, Robert A. [Department of Astrophysics, School of Physics, University of NSW 2052 (Australia)] [Department of Astrophysics, School of Physics, University of NSW 2052 (Australia); Izumiura, Hideyuki; Kambe, Eiji [Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata, Okayama 719-0232 (Japan)] [Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata, Okayama 719-0232 (Japan); Takeda, Yoichi; Kokubo, Eiichiro [The Graduate University for Advanced Studies, Shonan Village, Hayama, Kanagawa 240-0193 (Japan)] [The Graduate University for Advanced Studies, Shonan Village, Hayama, Kanagawa 240-0193 (Japan); Yoshida, Michitoshi [Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)] [Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Itoh, Yoichi [Nishi-Harima Astronomical Observatory, Center for Astronomy, University of Hyogo, 407-2, Nishigaichi, Sayo, Hyogo 679-5313 (Japan)] [Nishi-Harima Astronomical Observatory, Center for Astronomy, University of Hyogo, 407-2, Nishigaichi, Sayo, Hyogo 679-5313 (Japan); Ando, Hiroyasu, E-mail: satobn@geo.titech.ac.jp [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)] [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

2013-01-01T23:59:59.000Z

394

PLANETARY TRANSITS WITH THE ATACAMA LARGE MILLIMETER/SUBMILLIMETER ARRAY RADIO INTERFEROMETER  

SciTech Connect

Planetary transits are commonly observed at visible wavelengths. Here we investigate the shape of a planetary transit observed at radio wavelengths. Solar maps at 17 GHz are used as a proxy for the stellar eclipse by several sizes of planets from super-Earths to hot Jupiters. The relative depth at mid-transit is the same as observed at visible wavelengths, but the limb brightening of the stellar disk at 17 GHz is clearly seen in the shape of the transit light curve. Moreover, when the planet occults an active region the depth of the transit decreases even further, depending on the brightness of the active region relative to the surrounding disk. For intense active region, with 50 times the brightness temperature of the surrounding disk, the decrease can supercede the unperturbed transit depth depending on the size of the eclipsing planet. For a super-Earth (R{sub p} = 0.02 R{sub s} ) crossing, the decrease in intensity is 0.04%, increasing to 0.86% in the case when a strong active region is present. On the other hand, for a hot Jupiter with R{sub p} = 0.17R{sub s} , the unperturbed transit depth is 3% increasing to 4.7% when covering this strong active region. This kind of behavior can be verified with observation of planetary transits with the Atacama Large Millimeter/submillimeter Array radio interferometer.

Selhorst, C. L.; Barbosa, C. L. [IP and D, Universidade do Vale do Paraba (UNIVAP), So Jos dos Campos, SP (Brazil)] [IP and D, Universidade do Vale do Paraba (UNIVAP), So Jos dos Campos, SP (Brazil); Vlio, Adriana, E-mail: caius@univap.br [CRAAM, Universidade Presbiteriana Mackenzie, So Paulo, SP (Brazil)] [CRAAM, Universidade Presbiteriana Mackenzie, So Paulo, SP (Brazil)

2013-11-10T23:59:59.000Z

395

N-body calculations of cluster growth in proto-planetary disks  

E-Print Network (OSTI)

We investigated numerically the dust growth driven by Brownian motion in a proto-planetary disc around a solar-type young stellar object. This process is considered as the first stage in the transformation of the initially micron-sized solid particles to a planetary system. In contrast to earlier studies the growth was investigated at the small particle number densities typical for the conditions in a proto-planetary disc. Under such circumstances, the mean particle distance exceeds the typical aggregate diameter by orders of magnitude, and a collision will be a very rare event. We derived a criterion which allows an efficient detection of candidates for imminent collisions. The N-particle-method we used is based upon an adaptive time step scheme respecting the individual dynamical states of the aggregates. Its basic concept is to perform on average constant ``length steps'', instead of using constant time steps. The numerical cost of the algorithm scales with the particle number better than N log N. In order to minimise the influence of the decreasing number of particles within the simulation box, a new rescaling method is used throughout the aggregation process. Our numerical results indicate that at very low number densities, the growth process is influenced by spatial number density fluctuations.

S. Kempf; S. Pfalzner; Th. Henning

1999-02-12T23:59:59.000Z

396

Periodic Flux Variability of Stars due to the Reflex Doppler Effect Induced by Planetary Companions  

E-Print Network (OSTI)

Upcoming space-based photometric satellites offer the possibility of detecting continuum flux variability at the micro-magnitude level. We show that the Doppler flux variability induced by the reflex motion of stars due to planetary companions has an amplitude of (3-alpha)K/c, where K is the reflex radial velocity amplitude and alpha is the logarithmic slope of source spectral flux in the observed frequency band. For many of the known close-in planetary systems with periods less than ~0.2 years, the periodic Doppler variability is of order a micromagnitude, and is significant relative to the variability caused by reflected light from the planetary companion. For companions with periods greater than ~0.2 years, the Doppler signal is larger than the reflected light signal. We show that the future photometric satellites should reach the sensitivity to detect this Doppler variability. In particular, the Kepler satellite should have the photon-noise sensitivity to detect at a signal-to-noise ratio > 5, all planets with minimum mass greater than 5 Jupiter masses, and periods less than 0.1 years around the 10,000 main-sequence stars with spectral types A through K and apparent magnitude V<12 in its field-of-view.

Abraham Loeb; B. Scott Gaudi

2003-03-10T23:59:59.000Z

397

The Strengths of Near-Infrared Absorption Features Relevant to Interstellar and Planetary Ices  

E-Print Network (OSTI)

The abundances of ices in planetary environments have historically been obtained through measurements of near-infrared absorption features (lambda = 1.0-2.5 microns), and near-IR transmission measurements of materials present in the interstellar medium are becoming more common. For transmission measurements, the band strength (or absorption intensity) of an absorption feature must be known in order to determine the column density of an ice component. In the experiments presented here, we have measured the band strengths of the near-IR absorption features for several molecules relevant to the study of interstellar icy grain mantles and icy planetary bodies: CO (carbon monoxide), CO2 (carbon dioxide), C3O2 (carbon suboxide), CH4 (methane), H2O (water), CH3OH (methanol), and NH3 (ammonia). During a vacuum deposition, the sizes of the near-IR features were correlated with that of a studied mid-IR feature whose strength is well known from previous ice studies. These data may be used to determine ice abundances from observed near-IR spectra of interstellar and planetary materials or to predict the sizes of near-IR features in spectral searches for these molecules in astrophysical environments.

P. A. Gerakines; J. J. Bray; A. Davis; C. R. Richey

2005-02-16T23:59:59.000Z

398

Technical Sessions S. Lovejoy, A. Davis, Y. Tessier Physics Department  

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

S. Lovejoy, A. Davis, Y. Tessier S. Lovejoy, A. Davis, Y. Tessier Physics Department McGill University Montreal, Quebec, Canada D. Schertzer, R. Borde laboratoire de Meteorologie Dynamique Universite Pierre et Marie Curie Paris, France R. Frouin Scripps Institution of Oceanography University of California, San Diego La Jolla, CA 92093-0221 C. Gautier, D. Lavallee Earth Space Research Group University of California Santa Barbara, CA size. It is now clear that the relevant scale changes can be quite general, involving not only stratification (e.g., because of gravity), but also differential rotation (the Coriolis force), and other more complex operations. Between the inner viscous scale and the outer planetary scale, the fundamental dynamical equations of the atmosphere involve no char- acteristic length; this is the physical basis of the scaling.

399

Three-Dimensional Surface Geophysical Exploration of the 200-Series Tanks at the 241-C Tank Farm  

SciTech Connect

A surface geophysical exploration (SGE) survey using direct current electrical resistivity was conducted within the C Tank Farm in the vicinity of the 200-Series tanks at the Hanford Site near Richland, Washington. This survey was the second successful SGE survey to utilize the Geotection(TM)-180 Resistivity Monitoring System which facilitated a much larger survey size and faster data acquisition rate. The primary objective of the C Tank Farm SGE survey was to provide geophysical data and subsurface imaging results to support the Phase 2 RCRA Facility Investigation, as outlined in the Phase 2 RCRA Facility Investigation / Corrective Measures work plan RPP-PLAN-39114.

Crook, N. [HydroGEOPHYSICS, Inc., Tuscon, AZ (United States); McNeill, M. [HydroGEOPHYSICS, Inc., Tuscon, AZ (United States); Dunham, Ralph [Columbia Energy and Environmental Services, Inc. (United States); Glaser, Danney R. [Washington River Protection Solutions, LLC (United States)

2014-02-26T23:59:59.000Z

400

Physics of the Earth and Planetary Interiors 172 (2009) 235240 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

as it approaches the transition to the CaCl2-type phase. The bounds on the aggregate adi- abatic bulk and shear to an orthorhombic CaCl2-type structure around 50 GPa (Cohen, 1992; Kingma et al., 1995). This transition may12)/2 (Cohen, 1992). Many AX2 com- pounds with the rutile structure undergo a transition to CaCl2

Duffy, Thomas S.

Note: This page contains sample records for the topic "geophysics planetary physics" 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

Physics of the Earth and Planetary Interiors 184 (2011) 194207 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

Drive, La Jolla, CA 92093-0225, USA a r t i c l e i n f o Article history: Received 11 September 2010 coast effect model study illustrate that the anomalous phases are associated with energy diffusing back (Jones and Price, 1970). It was also rec- ognized early on that the land-side coast effect may depend

Key, Kerry

402

Physics of the Earth and Planetary Interiors 175 (2009) 12 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

(French Ministry of Research and Higher Education), and MAE (French Min- istry of Foreign Affairs and the associated investigations were entrusted to Fernand de Montessus de Ballore, a French seis- mologist an automatic and real-time system for the processing of broad- band seismometer wavefield implemented at ERI

Clouard, Valerie

403

Physics of the Earth and Planetary Interiors 170 (2008) 156169 Contents lists available at ScienceDirect  

E-Print Network (OSTI)

are on powder samples and the stress was measured by X-ray peak broadening. In the deforming powder sample preparation and characterization A wadsleyite sample was synthesized from San Carlos olivine powder at P = 15 GPa and T 1400 K for 1 h and an olivine sample was hot-pressed from San Carlos olivine powder at P

404

A field test of electromagnetic geophysical techniques for locating simulated in situ mining leach solution  

SciTech Connect

The US Bureau of Mines, The University of Arizona, Sandia National Laboratories, and Zonge Engineering and Research Organization, Inc., conducted cooperative field tests of six electromagnetic (EM) geophysical methods to compare their effectiveness in locating a brine solution simulating in situ leach solution or a high-conductivity plume of contamination. The brine was approximately 160 m below the surface. The testsite was the University's San Xavier experimental mine near Tucson, AZ. Geophysical surveys using surface and surface-borehole, time-domain electromagnetic (TEM) induction; surface controlled-source audiofrequency magnetotellurics (CSAMT); surface-borehole, frequency-domain electromagnetic (FEM) induction; crosshole FEM; and surface magnetic field ellipticity were conducted before and during brine injection. The surface TEM data showed a broad decrease in resistivity. CSAMT measurements with the conventional orientation did not detect the brine, but measurements with another orientation indicated some decrease in resistivity. The surface-borehole and crosshole methods located a known fracture and other fracture zones inferred from borehole induction logs. Surface magnetic field ellipticity data showed a broad decrease in resistivity at depth following brine injection.

Tweeton, D.R.; Hanson, J.C.; Friedel, M.J.; Sternberg, B.K.; Dahl, L.J.

1994-01-01T23:59:59.000Z

405

Environmental geophysics at Kings Creek Disposal Site and 30th Street Landfill, Aberdeen Proving Ground, Maryland  

SciTech Connect

Geophysical studies on the Bush River Peninsula in the Edgewood Area of Aberdeen Proving Ground, Maryland, delineate landfill areas and provide diagnostic signatures of the hydrogeologic framework and possible contaminant pathways. These studies indicate that, during the Pleistocene Epoch, alternating stands of high and low seal levels resulted in a complex pattern of shallow channel-fill deposits in the Kings Creek area. Ground-penetrating radar studies reveal a paleochannel greater than 50 ft deep, with a thalweg trending offshore in a southwest direction into Kings Creek. Onshore, the ground-penetrating radar data indicate a 35-ft-deep branch to the main channel, trending to the north-northwest directly beneath the 30th Street Landfill. Other branches are suspected to meet the offshore paleochannel in the wetlands south and east of the 30th Street Landfill. This paleochannel depositional system is environmentally significant because it may control the shallow groundwater flow regime beneath the site. Electromagnetic surveys have delineated the pre-fill lowland area currently occupied by the 30th Street Landfill. Magnetic and conductive anomalies outline surficial and buried debris throughout the study area. On the basis of geophysical data, large-scale dumping has not occurred north of the Kings Creek Disposal Site or east of the 30th Street Landfill.

Davies, B.E.; Miller, S.F.; McGinnis, L.D.; Daudt, C.R.; Thompson, M.D.; Stefanov, J.E.; Benson, M.A.; Padar, C.A.

1995-01-01T23:59:59.000Z

406

Physics & Astronomy Degree options  

E-Print Network (OSTI)

148 Physics & Astronomy Degree options BSc (Single Honours Degrees) Astrophysics Physics MPhys AND HL7 in Mathematics Physics and Astronomy (Gateway and International Gateway) Entry For UK students. Physics&Astronomy Subject enquiries Dr Kenny Wood E: physics@st-andrews.ac.uk Features * The nature

Brierley, Andrew

407

B Physics (Experiment)  

E-Print Network (OSTI)

In past few years the flavor physics made important transition from the work on confirmation the standard model of particle physics to the phase of search for effects of a new physics beyond standard model. In this paper we review current state of the physics of b-hadrons with emphasis on results with a sensitivity to new physics.

Michal Kreps

2010-08-02T23:59:59.000Z

408

Physics Resources for Teachers  

E-Print Network (OSTI)

Physics Resources for Teachers University of Wisconsin ­ Madison Department of Physics 1150 University Ave. Madison, WI 53706 wonders@physics.wisc.edu (608) 262-2927 Plasma Physics Web Resources Center Plasma Physics Lab http://science-education.pppl.gov/ Coalition for Plasma Science http

Collar, Juan I.

409

Department of Physics High Energy Physics Group  

E-Print Network (OSTI)

Department of Physics High Energy Physics Group Electrical Engineer (Job ref: 0004) The High Energy and experience. A job description and an application form can be obtained from http

410

1. Physical constants 1 1. PHYSICAL CONSTANTS  

E-Print Network (OSTI)

1. Physical constants 1 1. PHYSICAL CONSTANTS Table 1.1. Reviewed 2011 by P.J. Mohr (NIST). Mainly in parentheses after the values give the 1-standard-deviation uncertainties in the last digits; the corresponding also P.J. Mohr and D.B. Newell, "Resource Letter FC-1: The Physics of Fundamental Constants," Am. J

411

Physics 4: Introductory Physics Electromagnetism and Light  

E-Print Network (OSTI)

Physics 4: Introductory Physics Electromagnetism and Light Professor Jeffrey D. Richman Department: Electromagnetism and Light Welcome to Physics 4! What is your goal in life? If it is to become an engineer or to pursue a career in science, this is a key class for you. Understanding electromagnetism and light

Fygenson, Deborah Kuchnir

412

Geophysical Fluid Dynamics I P.B. Rhines Notes on the Boussinesq Approximation -I. 27 ii 2004  

E-Print Network (OSTI)

Geophysical Fluid Dynamics ­ I P.B. Rhines Notes on the Boussinesq Approximation - I. 27 ii 2004 compare with the full equations for a compressible fluid in Gill section 6.4. The Boussinesq approximation to the depth of the fluid layer. The Boussinesq equations most often used in the literature are accurate only

413

GEOPHYSICS, VOL. 62, NO. 4 (JULY-AUGUST 1997); P. 12921309, 6 FIGS. Anisotropic parameters and P-wave  

E-Print Network (OSTI)

GEOPHYSICS, VOL. 62, NO. 4 (JULY-AUGUST 1997); P. 1292­1309, 6 FIGS. Anisotropic parameters and P models. By design, this notation provides a uniform description of anisotropic media with both or- thorhombic and TI symmetry. The dimensionless anisotropic parameters introduced here preserve all attractive

Tsvankin, Ilya

414

Long-period fading in atmospherics during severe meteorological activity and associated solar geophysical phenomena at low latitudes  

E-Print Network (OSTI)

Long-period fading in atmospherics during severe meteorological activity and associated solar activity with the solar geophysical phenomena was studied. The results are indicative of an interesting sequence of solar- terrestrial events. A tentative conclusion is reached, suggesting an origin

Boyer, Edmond

415

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Climate Impacts of Cirrus Ice Nucleation1  

E-Print Network (OSTI)

in the climate system. Ice clouds reflect solar radiation23 back to space, cooling the planet. However, cold ice finely balanced between warming and cooling, with warming thought to be slightly larger.27 Changes to iceJOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Climate Impacts of Cirrus Ice

Gettelman, Andrew

416

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Energy Transfer and Flow in the Solar1  

E-Print Network (OSTI)

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Energy Transfer and Flow TENFJORD AND ?STGAARD: ENERGY TRANSFER AND FLOW Abstract. In this paper we describe and quantify the energy data. We employ what we consider to be the best es-6 timates for energy sinks, and relate

?stgaard, Nikolai

417

Environmental geophysics deals with issues ranging from local-scale fluid-rock changes to large-scale climatic  

E-Print Network (OSTI)

Environmental geophysics deals with issues ranging from local-scale fluid-rock changes to large and quarries, military bases, oil and gas fields, petroleum refineries, etc. Many derelict sites such as crankcase oils), mine spoils, and other inorganic pollutants. Accidental spills or poor disposal practice

Meju, Max

418

Geophysical modeling of two willemite deposits, Vazante (Brazil) and Beltana (Australia) Richard A. Krahenbuhl* and Murray Hitzman  

E-Print Network (OSTI)

of ore bodies or through imaging of associated hydrothermal alteration. Introduction Due to recent technological advances in developing solvent-extraction and electro-winning processes for treatment of zinc by conventional processing techniques and geophysical inversion. Vazante deposit in Brazil The Vazante willemite

419

GEOPHYSICAL RESEARCH LETTERS, VOL. 27, NO. 3, PAGES 377-380, FEBRUARY 1, 2000 Anomalous scaling of mesoscale tropospheric humidity  

E-Print Network (OSTI)

GEOPHYSICAL RESEARCH LETTERS, VOL. 27, NO. 3, PAGES 377-380, FEBRUARY 1, 2000 Anomalous scaling will take up to 20 s to respond. In this paper we report the first sci- entific results using the full 20-Hz on the idea of chaotic isentropic lateral mixing [e.g., Emanuel and Pierrehumbert, 1996]. Our present study

Cho, John Y. N.

420

GEOPHYSICS, VOL. 64, NO. 1 (JANUARY-FEBRUARY 1999); P. 3347, 17 FIGS. Simultaneous reconstruction of 1-D susceptibility  

E-Print Network (OSTI)

; revised manuscript received June 16, 1998. Formerly UBC-Geophysical Inversion Facility, 2219 Main Mall, Vancouver, BC, Canada V6T 1Z4; currently Western Atlas Logging Services, 10201 Westheimer, Houston, TX 77042 Facility, 2219 Main Mall, Vancouver, BC, Canada V6T 1Z4; E-mail: doug@geop.ubc.ca. c 1999 Society

Oldenburg, Douglas W.

Note: This page contains sample records for the topic "geophysics planetary physics" 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

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, Global energy conversion rate from geostrophic flows into  

E-Print Network (OSTI)

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, Global energy conversion rate from estimate of the energy conversion rate from geostrophic flows into internal lee waves in the ocean that linear lee wave theory gives a good prediction of the energy conversion rate at sub-critical and critical

Ferrari, Raffaele

422

The Portland Hills Fault: uncovering a hidden fault in Portland, Oregon using high-resolution geophysical methods  

Science Journals Connector (OSTI)

The Portland metropolitan area historically is the most seismically active region in Oregon. At least three potentially active faults are located in the immediate vicinity of downtown Portland, with the Portland Hills Fault (PHF) extending directly beneath downtown Portland. The faults are poorly understood, and the surface geologic record does not provide the information required to assess the seismic hazards associated with them. The limited geologic information stems from a surface topography that has not maintained a cumulative geologic record of faulting, in part, due to rapid erosion and deposition from late Pleistocene catastrophic flood events and a possible strike-slip component of the faults. We integrated multiple high-resolution geophysical techniques, including seismic reflection, ground penetrating radar (GPR), and magnetic methods, with regional geological and geophysical surveys to determine that the Portland Hills Fault is presently active with a zone of deformation that extends at least 400 m. The style of deformation is consistent with at least two major earthquakes in the last 1215 ka, as confirmed by a sidehill excavation trench. High-resolution geophysical methods provide detailed images of the upper 100 m across the active fault zone. The geophysical images are critical to characterizing the structural style within the zone of deformation, and when integrated with a paleoseismic trench, can accurately record the seismic history of a region with little surface geologic exposure.

Lee M. Liberty; Mark A. Hemphill-Haley; Ian P. Madin

2003-01-01T23:59:59.000Z

423

Nonlinear Processes in Geophysics (2005) 12: 311320 SRef-ID: 1607-7946/npg/2005-12-311  

E-Print Network (OSTI)

Processes in Geophysics Forced versus coupled dynamics in Earth system modelling and prediction B. Knopf1, H, a crucial element of Earth System modelling. Since the cur- rently preferred strategy for simulating. Such a simplifying tech- nique is often employed in Earth System models in order to save computing resources

Paris-Sud XI, Université de

424

GEOPHYSICAL RESEARCH LETTERS, VOL. 0, NO. 0, PAGES 0-0, M 0, 2001 On the Pacific Ocean regime shift  

E-Print Network (OSTI)

GEOPHYSICAL RESEARCH LETTERS, VOL. 0, NO. 0, PAGES 0-0, M 0, 2001 On the Pacific Ocean regime shift variability of Pacific Ocean upper ocean heat content is examined for the 1948-1998 period using gridded-wide phenomenon affecting the thermal structure from 60 S to 70 N. EOF analysis of the Pacific Ocean heat content

425

GEOPHYSICAL RESEARCH LETTERS, VOL. 27, NO. 15, PAGES 22452248, AUGUST 1, 2000 Subsurface nuclear tests monitoring through the  

E-Print Network (OSTI)

nuclear tests down to 1 kiloton (kt) TNT equivalent anywhere on the planet. The IMS is based upon four waves will help check for underground, under­water and atmospheric nuclear tests. The fourth networkGEOPHYSICAL RESEARCH LETTERS, VOL. 27, NO. 15, PAGES 2245­2248, AUGUST 1, 2000 Sub­surface nuclear

Hourdin, Chez Frédéric

426

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, Interactions between the Hadley cell and the1  

E-Print Network (OSTI)

GEOPHYSICAL RESEARCH LETTERS, VOL. ???, XXXX, DOI:10.1029/, Interactions between the Hadley cell - 2 P. PAGA AND J. KIDSTON: HADLEY CELL AND LATITUDE OF WESTLIES The correlation between unforced variability in the latitude of the edge of6 the Hadley cell (Hadley) and latitude of the surface westerlies

Kidston, Joseph

427

Geophysical exploration:  

Science Journals Connector (OSTI)

...combustion of fossil fuels produces carbon dioxide, the main greenhouse gas that produces global warming. As a result the development...and wind are more amenable to fixed uses such as heating and lighting. Transportation, on the other hand, requires a fuel that...

Enders A. Robinson

428

Lowx physics  

Science Journals Connector (OSTI)

...experiment led to the concept of the nuclear atom (Geiger & Marsden 1909...stronger y dependence at the cost of involving derivatives of r...collider physics. Cambridge Mono- graphs on Particle Physics, Nuclear Physics and Cosmology, vol...

2001-01-01T23:59:59.000Z

429

Geophysical monitoring and reactive transport modeling of ureolytically-driven calcium carbonate precipitation  

SciTech Connect

Ureolytically-driven calcium carbonate precipitation is the basis for a promising in-situ remediation method for sequestration of divalent radionuclide and trace metal ions. It has also been proposed for use in geotechnical engineering for soil strengthening applications. Monitoring the occurrence, spatial distribution, and temporal evolution of calcium carbonate precipitation in the subsurface is critical for evaluating the performance of this technology and for developing the predictive models needed for engineering application. In this study, we conducted laboratory column experiments using natural sediment and groundwater to evaluate the utility of geophysical (complex resistivity and seismic) sensing methods, dynamic synchrotron x-ray computed tomography (micro-CT), and reactive transport modeling for tracking ureolytically-driven calcium carbonate precipitation processes under site relevant conditions. Reactive transport modeling with TOUGHREACT successfully simulated the changes of the major chemical components during urea hydrolysis. Even at the relatively low level of urea hydrolysis observed in the experiments, the simulations predicted an enhanced calcium carbonate precipitation rate that was 3-4 times greater than the baseline level. Reactive transport modeling results, geophysical monitoring data and micro-CT imaging correlated well with reaction processes validated by geochemical data. In particular, increases in ionic strength of the pore fluid during urea hydrolysis predicted by geochemical modeling were successfully captured by electrical conductivity measurements and confirmed by geochemical data. The low level of urea hydrolysis and calcium carbonate precipitation suggested by the model and geochemical data was corroborated by minor changes in seismic P-wave velocity measurements and micro-CT imaging; the latter provided direct evidence of sparsely distributed calcium carbonate precipitation. Ion exchange processes promoted through NH{sub 4}{sup +} production during urea hydrolysis were incorporated in the model and captured critical changes in the major metal species. The electrical phase increases were potentially due to ion exchange processes that modified charge structure at mineral/water interfaces. Our study revealed the potential of geophysical monitoring for geochemical changes during urea hydrolysis and the advantages of combining multiple approaches to understand complex biogeochemical processes in the subsurface.

Wu, Y.; Ajo-Franklin, J.B.; Spycher, N.; Hubbard, S.S.; Zhang, G.; Williams, K.H.; Taylor, J.; Fujita, Y.; Smith, R.

2011-07-15T23:59:59.000Z

430

Saturday Morning Physics - Talks  

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

are now asking. pdf print version (pdf) Further information online Contemporary Physics Education Project The Particle Adventure Particle Physics - Education and Outreach...

431

B Physics: Theory Overview  

E-Print Network (OSTI)

This is an overview of B physics that can be done at the LHC with the purpose of searching for new physics.

David London

2012-07-19T23:59:59.000Z

432

Project X: Physics Opportunities  

E-Print Network (OSTI)

Part 2 of "Project X: Accelerator Reference Design, Physics Opportunities, Broader Impacts". In this Part, we outline the particle-physics program that can be achieved with Project X, a staged superconducting linac for intensity-frontier particle physics. Topics include neutrino physics, kaon physics, muon physics, electric dipole moments, neutron-antineutron oscillations, new light particles, hadron structure, hadron spectroscopy, and lattice-QCD calculations. Part 1 is available as arXiv:1306.5022 [physics.acc-ph] and Part 3 is available as arXiv:1306.5024 [physics.acc-ph].

Andreas S. Kronfeld; Robert S. Tschirhart; Usama Al-Binni; Wolfgang Altmannshofer; Charles Ankenbrandt; Kaladi Babu; Sunanda Banerjee; Matthew Bass; Brian Batell; David V. Baxter; Zurab Berezhiani; Marc Bergevin; Robert Bernstein; Sudeb Bhattacharya; Mary Bishai; Thomas Blum; S. Alex Bogacz; Stephen J. Brice; Joachim Brod; Alan Bross; Michael Buchoff; Thomas W. Burgess; Marcela Carena; Luis A. Castellanos; Subhasis Chattopadhyay; Mu-Chun Chen; Daniel Cherdack; Norman H. Christ; Tim Chupp; Vincenzo Cirigliano; Pilar Coloma; Christopher E. Coppola; Ramanath Cowsik; J. Allen Crabtree; Andr de Gouva; Jean-Pierre Delahaye; Dmitri Denisov; Patrick deNiverville; Ranjan Dharmapalan; Alexander Dolgov; Georgi Dvali; Estia Eichten; Jrgen Engelfried; Phillip D. Ferguson; Tony Gabriel; Avraham Gal; Franz Gallmeier; Kenneth S. Ganezer; Susan Gardner; Douglas Glenzinski; Stephen Godfrey; Elena S. Golubeva; Stefania Gori; Van B. Graves; Geoffrey Greene; Cory L. Griffard; Ulrich Haisch; Thomas Handler; Brandon Hartfiel; Athanasios Hatzikoutelis; Ayman Hawari; Lawrence Heilbronn; James E. Hill; Patrick Huber; David E. Jaffe; Christian Johnson; Yuri Kamyshkov; Daniel M. Kaplan; Boris Kerbikov; Brendan Kiburg; Harold G. Kirk; Andreas Klein; Kyle Knoepfel; Boris Kopeliovich; Vladimir Kopeliovich; Joachim Kopp; Wolfgang Korsch; Graham Kribs; Ronald Lipton; Chen-Yu Liu; Wolfgang Lorenzon; Zheng-Tian Lu; Naomi C. R. Makins; David McKeen; Geoffrey Mills; Michael Mocko; Rabindra Mohapatra; Nikolai V. Mokhov; Guenter Muhrer; Pieter Mumm; David Neuffer; Lev Okun; Mark A. Palmer; Robert Palmer; Robert W. Pattie Jr.; David G. Phillips II; Kevin Pitts; Maxim Pospelov; Vitaly S. Pronskikh; Chris Quigg; Erik Ramberg; Amlan Ray; Paul E. Reimer; David G. Richards; Adam Ritz; Amit Roy; Arthur Ruggles; Robert Ryne; Utpal Sarkar; Andy Saunders; Yannis K. Semertzidis; Anatoly Serebrov; Hirohiko Shimizu; Arindam K. Sikdar; Robert Shrock; Pavel V. Snopok; William M. Snow; Aria Soha; Stefan Spanier; Sergei Striganov; Zhaowen Tang; Lawrence Townsend; Jon Urheim; Arkady Vainshtein; Richard Van de Water; Ruth S. Van de Water; Richard J. Van Kooten; Bernard Wehring; Lisa Whitehead; Robert J. Wilson; Elizabeth Worcester; William C. Wester III; Albert R. Young; Geralyn Zeller

2013-06-20T23:59:59.000Z

433

Office of Physical Protection  

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

The Office of Physical Protection is comprised of a team of security specialists engaged in providing Headquarters-wide physical protection.

434

ORISE: Health physics services  

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

Health physics services Nuclear power plant The Oak Ridge Institute for Science and Education (ORISE) offers comprehensive health physics services in a number of technical areas...

435

Carl A. Gagliardi PHYSICS  

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

Physical Society Joseph B. Natowitz CHEMISTRY Heavy-ion reaction dynamics and thermodynamics - ACS Award in Nuclear Chemistry - Fellow, American Physical Society Ralf Rapp...

436

EVOLUTION OF PLANETARY ORBITS WITH STELLAR MASS LOSS AND TIDAL DISSIPATION  

SciTech Connect

Intermediate mass stars and stellar remnants often host planets, and these dynamical systems evolve because of mass loss and tides. This paper considers the combined action of stellar mass loss and tidal dissipation on planetary orbits in order to determine the conditions required for planetary survival. Stellar mass loss is included using a so-called Jeans model, described by a dimensionless mass loss rate ? and an index ?. We use an analogous prescription to model tidal effects, described here by a dimensionless dissipation rate ? and two indices (q, p). The initial conditions are determined by the starting value of angular momentum parameter ?{sub 0} (equivalently, the initial eccentricity) and the phase ? of the orbit. Within the context of this model, we derive an analytic formula for the critical dissipation rate ?, which marks the boundary between orbits that spiral outward due to stellar mass loss and those that spiral inward due to tidal dissipation. This analytic result ? = ?(?, ?, q, p, ?{sub 0}, ?) is essentially exact for initially circular orbits and holds to within an accuracy of ?50% over the entire multi-dimensional parameter space, where the individual parameters vary by several orders of magnitude. For stars that experience mass loss, the stellar radius often displays quasi-periodic variations, which produce corresponding variations in tidal forcing; we generalize the calculation to include such pulsations using a semi-analytic treatment that holds to the same accuracy as the non-pulsating case. These results can be used in many applications, e.g., to predict/constrain properties of planetary systems orbiting white dwarfs.

Adams, Fred C. [Physics Department, University of Michigan, Ann Arbor, MI 48109 (United States)] [Physics Department, University of Michigan, Ann Arbor, MI 48109 (United States); Bloch, Anthony M. [Math Department, University of Michigan, Ann Arbor, MI 48109 (United States)] [Math Department, University of Michigan, Ann Arbor, MI 48109 (United States)

2013-11-10T23:59:59.000Z

437

The Kinematics and Dynamics of the Globular Clusters and the Planetary Nebulae of NGC 5128  

E-Print Network (OSTI)

A new kinematic and dynamic study of the halo of the giant elliptical galaxy, NGC 5128, is presented. From a spectroscopically confirmed sample of 340 globular clusters and 780 planetary nebulae, the rotation amplitude, rotation axis, velocity dispersion, and the total dynamical mass are determined for the halo of NGC 5128. The globular cluster kinematics were searched for both radial dependence and metallicity dependence by subdividing the globular cluster sample into 158 metal-rich ([Fe/H] > -1.0) and 178 metal-poor ([Fe/H] < -1.0) globular clusters. Our results show the kinematics of the metal-rich and metal-poor subpopulations are quite similar. The kinematics are compared to the planetary nebula population where differences are apparent in the outer regions of the halo. The total mass of NGC 5128 is found using the Tracer Mass estimator (Evans et al. 2003), to determine the mass supported by internal random motions, and the spherical component of the Jeans equation to determine the mass supported by rotation. We find a total mass of (1.0+/-0.2) x 10^(12) Msun from the planetary nebulae data out to a projected radius of 90 kpc and (1.3+/-0.5) x 10^(12) Msun from the globular clusters out to a projected radius of 50 kpc. Lastly, we present a new and homogeneous catalog of known globular clusters in NGC 5128. This catalog combines all previous definitive cluster identifications from radial velocity studies and HST imaging studies, as well as 80 new globular clusters from a study of M.A. Beasley et al. (2007, in preparation).

Kristin A. Woodley; William E. Harris; Michael A. Beasley; Eric W. Peng; Terry J. Bridges; Duncan A. Forbes; Gretchen L. H. Harris

2007-04-10T23:59:59.000Z

438

Geophysical Study of Basin-Range Structure Dixie Valley Region, Nevada |  

Open Energy Info (EERE)

of Basin-Range Structure Dixie Valley Region, Nevada of Basin-Range Structure Dixie Valley Region, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Report: Geophysical Study of Basin-Range Structure Dixie Valley Region, Nevada Abstract The study aims to determine the subsurface structure and origin ofa tectonically active part of the Basin and Range province, which hasstructural similarities to the ocean ridge system and to continental blockfaultstructure such_;s the Rift Valleys of East Africa. A variety oftechniques was utilized, including seismic refraction, gravity measurements,magnetic measurements, photogeologic mapping, strain analysis of existinggeodetic data, and elevation measurements on shorelines of ancient lakes.Dixie Valley contains more than 10,000 feet of Cenozoic deposits andis underlain by a complex fault trough concealed within the

439

An Integrated Geophysical Study Of The Geothermal Field Of Tule Chek, Bc,  

Open Energy Info (EERE)

Tule Chek, Bc, Tule Chek, Bc, Mexico Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: An Integrated Geophysical Study Of The Geothermal Field Of Tule Chek, Bc, Mexico Details Activities (0) Areas (0) Regions (0) Abstract: A method is described to determine bounds characterizing axisymmetric bodies from a set of gravity data. Bounds on the density contrast as a function of depth to the top and thickness of the anomalous source are obtained by using Parker's ideal body theory and linear programming algorithms. Such bounds are given in terms of trade-off diagrams, where regions of feasible solutions compatible with the observed data can be assured. Gravity data from the Tule Chek, B.C., Mexico, geothermal area were used to compute such trade-off diagrams. Seismic

440

An Integrated Geophysical Study Of The Northern Kenya Rift | Open Energy  

Open Energy Info (EERE)

Kenya Rift Kenya Rift Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: An Integrated Geophysical Study Of The Northern Kenya Rift Details Activities (0) Areas (0) Regions (0) Abstract: The Kenyan part of the East African rift is among the most studied rift zones in the world. It is characterized by: (1) a classic rift valley, (2) sheer escarpments along the faulted borders of the rift valley, (3) voluminous volcanics that flowed from faults and fissures along the rift, and (4) axial and flank volcanoes where magma flow was most intense. In northern Kenya, the rift faults formed in an area where the lithosphere was weakened and stretched by Cretaceous-Paleogene extension, and in central and southern Kenya, it formed along old zones of weakness at the

Note: This page contains sample records for the topic "geophysics planetary physics" 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

An Integrated Geophysical Analysis Of The Upper Crust Of The Southern Kenya  

Open Energy Info (EERE)

Upper Crust Of The Southern Kenya Upper Crust Of The Southern Kenya Rift Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: An Integrated Geophysical Analysis Of The Upper Crust Of The Southern Kenya Rift Details Activities (0) Areas (0) Regions (0) Abstract: Previous interpretations of seismic data collected by the Kenya Rift International Seismic Project (KRISP) experiments indicate the presence of crustal thickening within the rift valley area beneath the Kenya dome, an uplift centred on the southern part of the Kenya rift. North of the dome, these interpretations show thinning of the crust and an increase in crustal extension. To the south near the Kenya/Tanzania border, crustal thinning associated with the rift is modest. Our study was aimed at further investigating crustal structure from this dome southwards via a

442

Geophysical Setting of the Blue Mountain Geothermal Area, North-Central  

Open Energy Info (EERE)

Setting of the Blue Mountain Geothermal Area, North-Central Setting of the Blue Mountain Geothermal Area, North-Central Nevada and Its Relationship to a Crustal-Scale Fracture Associated with the Inception of the Yellowstone Hotspot Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Geophysical Setting of the Blue Mountain Geothermal Area, North-Central Nevada and Its Relationship to a Crustal-Scale Fracture Associated with the Inception of the Yellowstone Hotspot Abstract The Blue Mountain geothermal field, located about 35 km northwest of Winnemucca, Nevada, is situated along a prominent crustal-scale fracture interpreted from total intensity aeromagnetic and gravity data. Aeromagnetic data indicate that this feature is related to the intrusion of mafic dikes, similar to the Northern Nevada Rift (Zoback et al.,1994), and

443

Stratified Rotating Boussinesq Equations in Geophysical Fluid Dynamics: Dynamic Bifurcation and Periodic Solutions  

E-Print Network (OSTI)

The main objective of this article is to study the dynamics of the stratified rotating Boussinesq equations, which are a basic model in geophysical fluid dynamics. First, for the case where the Prandtl number is greater than one, a complete stability and bifurcation analysis near the first critical Rayleigh number is carried out. Second, for the case where the Prandtl number is smaller than one, the onset of the Hopf bifurcation near the first critical Rayleigh number is established, leading to the existence of nontrivial periodic solutions. The analysis is based on a newly developed bifurcation and stability theory for nonlinear dynamical systems (both finite and infinite dimensional) by two of the authors [16].

Chun-Hsiung Hsia; Tian Ma; Shouhong Wang

2006-10-31T23:59:59.000Z

444

GEOPHYSICAL INVESTIGATIONS OF THE ARCHAEOLOGICAL RESOURCES AT THE POWELL STAGE STATION  

SciTech Connect

Within the boundaries of the Idaho National Laboratory, an ongoing archaeological investigation of a late 19th century stage station was expanded with the use of Electro-Magnetic and Magnetic geophysical surveying. The station known as the Powell Stage Station was a primary transportation hub on the Snake River Plain, bridging the gap between railroad supply depots in Blackfoot, Idaho and booming mining camps throughout Central Idaho. Initial investigations have shown a strong magnetic signature from a buried road and previously unknown features that were not detected by visual surface surveys. Data gained from this project aids in federally directed cultural resource and land management and use requirements and has contributed additional information for archeological interpretation and cultural resource preservation.

Hollie K. Gilbert; Julie B. Braun; Brenda R. Pace; Gail Heath; Clark Scott

2009-04-01T23:59:59.000Z

445

A Feasibility Study of Non-Seismic Geophysical Methods forMonitoring Geologic CO2 Sequestration  

SciTech Connect

Because of their wide application within the petroleumindustry it is natural to consider geophysical techniques for monitoringof CO2 movement within hydrocarbon reservoirs, whether the CO2 isintroduced for enhanced oil/gas recovery or for geologic sequestration.Among the available approaches to monitoring, seismic methods are by farthe most highly developed and applied. Due to cost considerations, lessexpensive techniques have recently been considered. In this article, therelative merits of gravity and electromagnetic (EM) methods as monitoringtools for geological CO2 sequestration are examined for two syntheticmodeling scenarios. The first scenario represents combined CO2 enhancedoil recovery (EOR) and sequestration in a producing oil field, theSchrader Bluff field on the north slope of Alaska, USA. The secondscenario is a simplified model of a brine formation at a depth of 1,900m.

Gasperikova, Erika; Hoversten, G. Michael

2006-07-01T23:59:59.000Z

446

Search for gravitational waves associated with the InterPlanetary Network short gamma ray bursts  

E-Print Network (OSTI)

We outline the scientific motivation behind a search for gravitational waves associated with short gamma ray bursts detected by the InterPlanetary Network (IPN) during LIGO's fifth science run and Virgo's first science run. The IPN localisation of short gamma ray bursts is limited to extended error boxes of different shapes and sizes and a search on these error boxes poses a series of challenges for data analysis. We will discuss these challenges and outline the methods to optimise the search over these error boxes.

V. Predoi; for the LIGO Scientific Collaboration; for the Virgo Collaboration; K. Hurley; for IPN

2011-12-07T23:59:59.000Z

447

Identification of potential groundwater flow paths using geological and geophysical data  

SciTech Connect

This project represents the first phase in the development of a methodology for generating three-dimensional equiprobable maps of hydraulic conductivity for the Nevada Test Site (NTS). In this study, potential groundwater flow paths were investigated for subsurface tuffs at Yucca Flat by studying how these units are connected. The virtual absence of site-specific hydraulic conductivity data dictates that as a first step a surrogate attribute (geophysical logs) be utilized. In this first phase, the connectivity patterns of densely welded ash-flow tuffs were studied because these tuffs are the most likely to form zones of high hydraulic conductivity. Densely welded tuffs were identified based on the response shown on resistivity logs and this information was transformed into binary indicator values. The spatial correlation of the indicator data was estimated through geostatistical methods. Equiprobable three-dimensional maps of the distribution of the densely-welded and nonwelded tuffs (i.e., subsurface heterogeneity) were then produced using a multiple indicator simulation formalism. The simulations demonstrate that resistivity logs are effective as soft data for indicating densely welded tuffs. The simulated welded tuffs reproduce the stratigraphic relationships of the welded tuffs observed in hydrogeologic cross sections, while incorporating the heterogeneity and anisotropy that is expected in this subsurface setting. Three-dimensional connectivity of the densely welded tuffs suggests potential groundwater flow paths with lengths easily over 1 km. The next phase of this investigation should incorporate other geophysical logs (e.g., gamma-gamma logs) and then calibrate the resulting soft data maps with available hard hydraulic conductivity data. The soft data maps can then augment the hard data to produce the final maps of the spatial distribution of hydraulic conductivity that can be used as input for numerical solution of groundwater flow and transport.

Pohlmann, K.; Andricevic, R.

1994-09-01T23:59:59.000Z

448

GEOPHYSICAL RESEARCHLETTERS, VOL. 17, NO.6, PAGES 869-872, MAY 1990 A MODEL OF THE ION WAKE OF MARS  

E-Print Network (OSTI)

picked up by the solar wind in the dayside exosphere. The results suggest that low energy « 10 ke, the planetary exospheres can extend into the magnetosheath and solar wind because the effective "obstacles magnetosheath and adjacent solar wind. The latter has a finite gyroradius related spatial asymmetry controlled

California at Berkeley, University of

449

DownloadedBy:[UniversityofCaliforniaLosAngeles]At:16:419December2007 Geophysical and Astrophysical Fluid Dynamics,  

E-Print Network (OSTI)

and convective heat transfer scalingy J. M. AURNOU* Department of Earth and Space Sciences, University shell to generate larger-scale zonal flows. Comparing quantitative results, heat transfer data at high heat transfer rates. Keywords: Core dynamics; Convection; Heat transfer; Planetary dynamos 1

450

PHYSICS 106 Summer 2011  

E-Print Network (OSTI)

PHYSICS 106 Summer 2011 Instructor: Stephanie Magleby (sam25@physics.byu.edu) Office Hours: MWF 2 -3 pm, N311 ESC Office Phone (physics): 422-7056 Office Phone (engineering): 422-8319 TA: Corbin Jacobs [corbinjacobs@gmail.com] Email Corbin with any reading quiz questions or Mastering Physics issues

Hart, Gus

451

Aspects of Unparticle Physics  

E-Print Network (OSTI)

We review some theoretical and experimental issues in unparticle physics, focusing mainly on collider signatures.

Arvind Rajaraman

2008-09-29T23:59:59.000Z

452

Fundamentals of Plasma Physics  

E-Print Network (OSTI)

Fundamentals of Plasma Physics James D. Callen University of Wisconsin, Madison June 28, 2006 #12;PREFACE Plasma physics is a relatively new branch of physics that became a mature science over the last half of the 20th century. It builds on the fundamental areas of classical physics: mechanics

Callen, James D.

453

NAC Ad-Hoc Task Force on Planetary Defense July 8-9, 2010 CORRECTED 9/15/10 1 NASA ADVISORY COUNCIL (NAC)  

E-Print Network (OSTI)

NAC Ad-Hoc Task Force on Planetary Defense July 8-9, 2010 ­ CORRECTED 9/15/10 1 NASA ADVISORY COUNCIL (NAC) Ad-Hoc Task Force on Planetary Defense CORRECTED MINUTES Meeting Date: July 8 - 9, 2010 AGENDA: · Ad-Hoc Task Force Timeline · Fact Finding Report · Next Generation Ground-Based Search · Space

Waliser, Duane E.

454

NAC Ad-Hoc Task Force on Planetary Defense Apr 15-16, 2010 CORRECTED 6/10/10 1 NASA ADVISORY COUNCIL (NAC)  

E-Print Network (OSTI)

NAC Ad-Hoc Task Force on Planetary Defense Apr 15-16, 2010 ­ CORRECTED 6/10/10 1 NASA ADVISORY COUNCIL (NAC) Ad-Hoc Task Force on Planetary Defense CORRECTED MINUTES Meeting Date: April 15-16, 2010 AGENDA: · Ad-Hoc Task Force Terms of Reference · NASA Near Earth Objects Observation (NEOO) Program

Waliser, Duane E.

455

Particle Physics Education Sites  

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

쭺-¶ 쭺-¶ Particle Physics Education Sites ¡]¥H¤U¬°¥~¤åºô¯¸¡^ quick reference Education and Information - National Laboratory Education Programs - Women and Minorities in Physics - Other Physics Sites - Physics Alliance - Accelerators at National Laboratories icon Particle Physics Education and Information sites: top Introduction: The Particle Adventure - an interactive tour of particle physics for everyone: the basics of theory and experiment. Virtual Visitor Center of the Stanford Linear Accelerator Center. Guided Tour of Fermilab, - overviews of several aspects of Particle Physics. Also check out Particle Physics concepts. Probing Particles - a comprehensive and straight-forward introduction to particle physics. Big Bang Science - approaches particle physics starting from the theoretical origin of the universe.

457

Publications of the Hawaii Institute of Geophysics and Planetology University of Hawaii  

E-Print Network (OSTI)

scattering and X-ray diffraction study of the thermal decomposition of an ettringite-group crystal., Physics

458

Geologic, geophysical, and geochemical aspects of site-specific studies of the geopressured-geothermal energy resource of southern Louisiana. Final report  

SciTech Connect

The report consists of four sections dealing with progress in evaluating geologic, geochemical, and geophysical aspects of geopressured-geothermal energy resources in Louisiana. Separate abstracts have been prepared for the individual sections. (ACR)

Pilger, R.H. Jr. (ed.)

1985-01-01T23:59:59.000Z

459

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 94, NO. D13, PAGES 16,417-16,421,NOVEMBER 20, 1989 Greenhouse Effect of Chlorofluorocarbons and Other Trace Gases  

E-Print Network (OSTI)

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 94, NO. D13, PAGES 16,417-16,421,NOVEMBER 20, 1989 Greenhouse Effect of Chlorofluorocarbons and Other Trace Gases JAMESHANSEN,ANDREW LACIS,AND MICHAEL PRATHER NASA

Fridlind, Ann

460

TRANSIT TIMING VARIATION OF NEAR-RESONANCE PLANETARY PAIRS: CONFIRMATION OF 12 MULTIPLE-PLANET SYSTEMS  

SciTech Connect

We extract transit timing variation (TTV) signals for 12 pairs of transiting planet candidates that are near first-order mean motion resonances (MMR), using publicly available Kepler light curves (Q0-Q14). These pairs show significant sinusoidal TTVs with theoretically predicted periods, which demonstrate these planet candidates are orbiting and interacting in the same system. Although individual masses cannot be accurately extracted based only on TTVs because of the well-known degeneracy between mass and eccentricity, TTV phases and amplitudes can still place upper limits on the masses of the candidates, confirming their planetary nature. Furthermore, the mass ratios of these planet pairs can be relatively tightly constrained using these TTVs. The planetary pair in KOI 880 seems to have particularly high mass and density ratios, which might indicate very different internal compositions of these two planets. Some of these newly confirmed planets are also near MMR with other candidates in the system, forming unique resonance chains (e.g., KOI 500)

Xie, Ji-Wei, E-mail: xiejiwei@gmail.com, E-mail: jwxie@astro.utoronto.ca [Department of Astronomy and Key Laboratory of Modern Astronomy and Astrophysics in Ministry of Education, Nanjing University, Nanjing 210093 (China)

2013-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

The planetary system host HR\\,8799: On its $\\lambda$ Bootis nature  

E-Print Network (OSTI)

HR\\,8799 is a $\\lambda$ Bootis, $\\gamma$ Doradus star hosting a planetary system and a debris disk with two rings. This makes this system a very interesting target for asteroseismic studies. This work is devoted to the determination of the internal metallicity of this star, linked with its $\\lambda$ Bootis nature (i.e., solar surface abundances of light elements, and subsolar surface abundances of heavy elements), taking advantage of its $\\gamma$ Doradus pulsations. This is the most accurate way to obtain this information, and this is the first time such a study is performed for a planetary-system-host star. We have used the equilibrium code CESAM and the non-adiabatic pulsational code GraCo. We have applied the Frequency Ratio Method (FRM) and the Time Dependent Convection theory (TDC) to estimate the mode identification, the Brunt-Va\\"is\\"al\\"a frequency integral and the mode instability, making the selection of the possible models. When the non-seismological constraints (i.e its position in the HR diagram)...

Moya, A; Barrado, D; Hernndez, A Garca; Aberasturi, M; Montesinos, B; Aceituno, F

2010-01-01T23:59:59.000Z

462

The separation of the stars in the binary nucleus of the planetary nebula Abell 35  

E-Print Network (OSTI)

Using the Planetary Camera on board the Hubble Space Telescope we have measured the projected separation of the binary components in the nucleus of the planetary nebula Abell 35 to be larger than 0.08 arcsecs but less than 0.14 arcsecs. The system was imaged in three filters centered at 2950, 3350 and 5785 Ang. The white dwarf primary star responsible for ionizing the nebula is half as bright as its companion in the 2950 Ang filter causing the source to be visibly elongated. The 3350 Ang setting, on the other hand, shows no elongation as a result of the more extreme flux ratio. The F300W data allows the determinination of the binary's projected separation. At the minimum distance of 160 parsec to the system, our result corresponds to 18+/-5 AU. This outcome is consistent with the wind accretion induced rapid rotation hypothesis, but cannot be reconciled with the binary having emerged from a common-envelope phase.

A. A. Gatti; J. E. Drew; R. D. Oudmaijer; T. R. Marsh; A. E. Lynas-Gray

1998-09-25T23:59:59.000Z

463

Planetary companions in K giants beta Cancri, mu Leonis, and beta Ursae Minoris  

E-Print Network (OSTI)

Auns. The aim of our paper is to investigate the low-amplitude and long-period variations in evolved stars with a precise radial velocity (RV) survey. Methods. The high-resolution, the fiber-fed Bohyunsan Observatory Echelle Spectrograph (BOES) was used from 2003 to 2013 for a radial velocity survey of giant stars as part of the exoplanet search program at Bohyunsan Optical Astronomy Observatory (BOAO). Results. We report the detection of three new planetary companions orbiting the K giants beta Cnc, mu Leo, and beta UMi. The planetary nature of the radial velocity variations is supported by analyzes of ancillary data. The HIPPARCOS photometry shows no variations with periods close to those in RV variations and there is no strong correlation between the bisector velocity span (BVS) and the radial velocities for each star. Furthermore, the stars show weak or no core reversal in Ca II H lines indicating that they are inactive stars. The companion to beta Cnc has a minimum mass of 7.8 M_Jup in a 605-day orbit wi...

Lee, B -C; Park, M -G; Mkrtichian, D E; Hatzes, A P; Kim, K -M

2014-01-01T23:59:59.000Z

464

THE HYADES CLUSTER: IDENTIFICATION OF A PLANETARY SYSTEM AND ESCAPING WHITE DWARFS  

SciTech Connect

Recently, some hot DA-type white dwarfs have been proposed to plausibly be escaping members of the Hyades. We used hydrogen Balmer lines to measure the radial velocities of seven such stars and confirm that three, and perhaps two others, are/were indeed cluster members and one is not. The other candidate Hyad is strongly magnetic and its membership status remains uncertain. The photospheres of at least one quarter of field white dwarf stars are ''polluted'' by elements heavier than helium that have been accreted. These stars are orbited by extended planetary systems that contain both debris belts and major planets. We surveyed the seven classical single Hyades white dwarfs and the newly identified (escaping) Hyades white dwarfs and found calcium in the photosphere of LP 475-242 of type DBA (now DBAZ), thus implying the presence of an orbiting planetary system. The spectrum of white dwarf GD 31, which may be, but probably is not, an escaping member of the Hyades, displays calcium absorption lines; these originate either from the interstellar medium or, less likely, from a gaseous circumstellar disk. If GD 31 was once a Hyades member, then it would be the first identified white dwarf Hyad with a cooling age >340 Myr.

Zuckerman, B.; Xu, S.; Klein, B.; Jura, M., E-mail: ben@astro.ucla.edu, E-mail: sxu@astro.ucla.edu, E-mail: kleinb@astro.ucla.edu, E-mail: jura@astro.ucla.edu [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)

2013-06-20T23:59:59.000Z

465

Planetary balloons  

Science Journals Connector (OSTI)

Since the temperature is inferior to 100K in the 070km altitude range (94K at surface), the key factor for a Titan balloon mission is the power supply. RTG are needed both for thermal power since steady st...

Jacques Blamont

2008-10-01T23:59:59.000Z

466

Physics | More Science | ORNL  

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

Physics Physics ORNL Physics More Science Home | Science & Discovery | More Science | Physics SHARE Physics Bottom view of the 25 million volt tandem electrostatic accelerator of the Holifield Heavy Ion Research Facility. Physics researchers at ORNL seek to answer fascinating questions about our Universe: What are the nuclear reactions that drive stellar explosions? How does nuclear matter organize itself? What are the properties of nuclear interactions? Why is there more matter than antimatter in the universe? Is the neutrino its own antiparticle? What are the properties of matter that existed just after the Big Bang? Our research staff address these questions by developing experimental techniques and detector systems, performing experiments at national and

467

NEAR-INFRARED BAND STRENGTHS OF MOLECULES DILUTED IN N{sub 2} AND H{sub 2}O ICE MIXTURES RELEVANT TO INTERSTELLAR AND PLANETARY ICES  

SciTech Connect

The relative abundances of ices in astrophysical environments rely on accurate laboratory measurements of physical parameters, such as band strengths (or absorption intensities), determined for the molecules of interest in relevant mixtures. In an extension of our previous study on pure-ice samples, here we focus on the near-infrared absorption features of molecules in mixtures with the dominant components of interstellar and planetary ices, H{sub 2}O and N{sub 2}. We present experimentally measured near-infrared spectral information (peak positions, widths, and band strengths) for both H{sub 2}O- and N{sub 2}-dominated mixtures of CO (carbon monoxide), CO{sub 2} (carbon dioxide), CH{sub 4} (methane), and NH{sub 3} (ammonia). Band strengths were determined during sample deposition by correlating the growth of near-infrared features (10,000-4000 cm{sup -1}, 1-2.5 {mu}m) with better-known mid-infrared features (4000-400 cm{sup -1}, 2.5-25 {mu}m) at longer wavelengths.

Richey, C. R.; Gerakines, P. A., E-mail: christina.r.richey@nasa.gov, E-mail: gerak@uab.edu [Astro- and Solar-System Physics Program, Department of Physics, University of Alabama at Birmingham, Birmingham, AL 35294-1170 (United States)

2012-11-01T23:59:59.000Z

468

Kepler photometry and optical spectroscopy of the ZZ Lep central star of the Planetary Nebula NGC 6826: rotational and wind variability  

E-Print Network (OSTI)

We present three years of long-cadence and over one year of short-cadence photometry of the central star of the Planetary Nebula NGC 6826 obtained with the Kepler spacecraft, and temporally coinciding optical spectroscopy. The light curves are dominated by incoherent variability on time scales of several hours, but contain a lower-amplitude periodicity of 1.23799 d. The temporal amplitude and shape changes of this signal are best explicable with a rotational modulation, and are not consistent with a binary interpretation. We argue that we do not observe stellar pulsations within the limitations of our data, and show that a binary central star with an orbital period less than seven days could only have escaped our detection in the case of low orbital inclination. Combining the photometric and spectroscopic evidence, we reason that the hourly variations are due to a variable stellar wind, and are global in nature. The physical cause of the wind variability of NGC 6826 and other ZZ Leporis stars is likely relate...

Handler, G; Urbaneja, M A; Antoci, V; Twicken, J D; Barclay, T

2013-01-01T23:59:59.000Z

469

Chemical Abundances and Dust in the Halo Planetary Nebula K648 in M15: Its Origin and Evolution based on an Analysis of Multiwavelength Data  

E-Print Network (OSTI)

We report an investigation of the extremely metal-poor and C-rich planetary nebula (PN) K648 in the globular cluster M15 using the UV to far-IR data obtained using the Subaru, HST, FUSE, Spitzer, and Herschel. We determined the nebular abundances of ten elements. The enhancement of F ([F/H]=+0.96) is comparable to that of the halo PN BoBn1. The central stellar abundances of seven elements are determined. The stellar C/O ratio is similar to the nebular C/O ratios from recombination line and from collisionally excited line (CEL) within error, and the stellar Ne/O ratio is also close to the nebular CEL Ne/O ratio. We found evidence of carbonaceous dust grains and molecules including Class B 6-9 um and 11.3 um polycyclic aromatic hydrocarbons and the broad 11 um feature. The profiles of these bands are similar to those of the C-rich halo PNe H4-1 and BoBn1. Based on the theoretical model, we determined the physical conditions of the gas and dust and their masses, i.e., 0.048 Msun and 4.95x10^{-7} Msun, respective...

Otsuka, Masaaki; Tajitsu, Akito

2015-01-01T23:59:59.000Z

470

Imaging the transition between pre-planetary and planetary nebulae: Integral Field Spectroscopy of hot post-AGB stars with NIFS  

E-Print Network (OSTI)

We present 2 to 2.4 micron integral field spectroscopy of a sample of hot post-AGB stars with early-B spectral types, using the NIFS instrument on Gemini North. These stars are just beginning to ionize their immediate environments and turn into planetary nebulae (PNe).We use molecular hydrogen emission lines together with hydrogen and helium recombination lines to explore the distribution of molecular and atomic gas and the extent of the developing ionized region. We see a range of evolutionary stages: IRAS 18062+2410 and IRAS 18379-1707 have recently developed compact and unresolved regions of photoionized H within axisymmetric molecular envelopes, with the former object increasing its Br-Gamma flux by a factor of 5.3 in 14 years; IRAS 22023+5249 and IRAS 20462+3416 have extended Br-Gamma nebulae and in the latter object only weak H2 emission remains; IRAS 19336-0400 is at a more advanced stage of PN formation where H2 is mostly dissociated and we see structure in both the H and He recombination line nebulae...

Gledhill, T M

2014-01-01T23:59:59.000Z

471

An Analysis of Wind Power Development in the Town of Hull, MA_Appendix 4_Geophysical Survey Report  

SciTech Connect

CR Environmental, Inc. (CR) was contracted by GZA GeoEnvironmental, Inc. (GZA) to perform hydrographic and geophysical surveys of an approximately 3.35 square mile area off the eastern shore of Hull, Massachusetts. Survey components included: Single-beam bathymetry; 100-kHz and 500-kHz side scan sonar; Magnetometry; and Low to mid-frequency sub-bottom profiling.

Adams, Christopher

2013-06-30T23:59:59.000Z

472

Earth and Planetary Science Letters, 116(1993) 1-8 1 Elsevier Science Publishers B.V., Amsterdam  

E-Print Network (OSTI)

Earth and Planetary Science Letters, 116(1993) 1-8 1 Elsevier Science Publishers B.V., Amsterdam as the axialbody rotation. An observed magnetic superchron seems to end when a new hotspot migration cycle,rotating and magnetized mantles, in which the characteristic surface tracers are believed to reflect the patterns

Fridlind, Ann

473

Internal variability of the tropical Pacific ocean Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA  

E-Print Network (OSTI)

Internal variability of the tropical Pacific ocean M. Jochum Earth, Atmospheric and Planetary model of the tropical Pacific ocean is analyzed to quantify the interannual variability caused by internal variability of ocean dynamics. It is found that along the Pacific cold tongue internal variability

Jochum, Markus

474

Probing new physics with flavor physics (and probing flavor physics with new physics)  

E-Print Network (OSTI)

This is a written version of a series of lectures aimed at graduate students and postdoctoral fellows in particle theory/string theory/particle experiment familiar with the basics of the Standard Model. We begin with an overview of flavor physics and its implications for new physics. We emphasize the "new physics flavor puzzle". Then, we give four specific examples of flavor measurements and the lessons that have been (or can be) drawn from them: (i) Charm physics: lessons for supersymmetry from the upper bound on $\\Delta m_D$. (ii) Bottom physics: model independent lessons on the KM mechanism and on new physics in neutral B mixing from $S_{\\psi K_S}$. (iii) Top physics and beyond: testing minimal flavor violation at the LHC. (iv) Neutrino physics: interpreting the data on neutrino masses and mixing within flavor models.

Yosef Nir

2007-08-14T23:59:59.000Z

475

Physics Flash Newsletter  

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

Physics Links Jobs in Physics Human Resources Working at Los Alamos Los Alamos resources To read past issues, please see the: 2012 archive page 2011 archive page December 2013 | In...

476

Elementary Reactor Physics  

Science Journals Connector (OSTI)

... THERE are few subjects which have developed at the rate at which reactor physics and ... physics and reactor theory have done. This, of course, is largely due to the circumstances in ...

J. F. HILL

1962-02-10T23:59:59.000Z

477

Physics, complexity and causality  

Science Journals Connector (OSTI)

... physics theory that explains the nature of, or even the existence of, football matches, teapots, or jumbo-jet aircraft. The human mind is physically based, but there is ...

George F. R. Ellis

2005-06-08T23:59:59.000Z

478

Physics 151 Lecture 1 Physics 207: Lecture 1, Pg 1  

E-Print Network (OSTI)

Page 1 Physics 151 ­ Lecture 1 Physics 207: Lecture 1, Pg 1 Physics 207, Sections: 301/601Physics 207, Sections: 301/601 ­­ 314/614314/614 General Physics IGeneral Physics I MichaelMichael Winokur of the courseScope of the course Begin chapter 1Begin chapter 1 Homepage:Homepage: http://romano.physics

Winokur, Michael

479

Physical Probability Patrick Maher  

E-Print Network (OSTI)

Physical Probability Patrick Maher University of Illinois at Urbana-Champaign October 13, 2007 ABSTRACT. By "physical probability" I mean the empirical concept of probability in or- dinary language-extreme physical probabilities are compatible with determin- ism. Two principles, called specification

Fitelson, Branden

480

Whither Nuclear Physics ?  

E-Print Network (OSTI)

Nuclear Physics has had its ups and downs. However in recent years, bucked up by some new and often puzzling data, it has become a potentially very rich field. We review some of these exciting developments in a few important sectors of nuclear physics. Emphasis shall be on the study of exotic nuclei and the new physics that these nuclei are teaching us.

Syed Afsar Abbas

2008-01-07T23:59:59.000Z

Note: This page contains sample records for the topic "geophysics planetary physics" 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

in Condensed Matter Physics  

E-Print Network (OSTI)

Master in Condensed Matter Physics ­ Master académique #12;2 #12;3 Students at the University. Condensed matter physics is about explaining and predicting the relationship between the atomic, and broad education in the field of condensed matter physics · introduce you to current research topics

van der Torre, Leon

482

PHYSICS, QUALITATIVE BIBLIOGRAPHY  

E-Print Network (OSTI)

PHYSICS, QUALITATIVE C BIBLIOGRAPHY D. G. Bobrow and R J. Hayes, eds., Artif. Intell. 24," in Gentner and Stevens, 1983, pp. 155--190. J. de Kleer and J. S. Brown "A Qualitative Physics Based.J., 1983. P. Hayes, "The Naive Physics Manifesto," in Hobbs and Moore, 1985, pp 1--36 J R Hobbs and R C

de Kleer, Johan

483

B Physics at LHCb  

E-Print Network (OSTI)

LHCb is a dedicated detector for b physics at the LHC. In this article we present a concise review of the detector design and performance together with the main physics goals and their relevance for a precise test of the Standard Model and search of New Physics beyond it.

Monica Pepe Altarelli; Frederic Teubert

2008-02-13T23:59:59.000Z

484

Nuclear Physics with trapped  

E-Print Network (OSTI)

Nuclear Physics with trapped atoms and ions #12;2/2/2013Dan Melconian #12;2/2/2013Dan Melconian Outline · Scope and applications of nuclear physics precision frontier compliments LHC properties and aquifers in the Sahara #12;2/2/2013Dan Melconian What is Nuclear Physics? · Began with the study

Boas, Harold P.

485

Meteoritics & Planetary Science 39, Nr 8, 14091411 (2004) Abstracts available online at http://meteoritics.org  

E-Print Network (OSTI)

contributions to particle physics, nuclear physics (the discovery of nuclear particle tracks and the invention this technique to diverse problems in meteoritics, neutron dosimetry and cosmic rays, as well as archaeology

486

Particle Physics, Nuclear Physics and Nuclear Energy  

Science Journals Connector (OSTI)

Particle physics is a frontier subject which studies the smallest constituents of matter and the laws governing their interactions. It plays an important role in studying the origin and evolution of the univer...

Hesheng Chen

2011-01-01T23:59:59.000Z

487

Physics of Cancer | Princeton Plasma Physics Lab  

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

18, 2014, 9:30am to 11:00am Science On Saturday MBG Auditorium Physics of Cancer Professor Wolfgang Losert, Associate Professor, and Director, Partnership for Cancer Technology...

488

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network (OSTI)

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

J. L. Payne; M. D. Filipovi?; E. J. Crawford; A. Y. De Horta; G. L. White; F. H. Stootman

2008-04-29T23:59:59.000Z

489

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network (OSTI)

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

Payne, J L; Crawford, E J; De Horta, A Y; White, G L; Stootman, F H

2008-01-01T23:59:59.000Z

490

Attitude determination of planetary exploration rovers using solar panels characteristics and accelerometer  

Science Journals Connector (OSTI)

Abstract In this study, we propose a new attitude determination system, which we call Irradiance-based Attitude Determination (IRAD). IRAD employs the characteristics and geometry of solar panels. First, the sun vector is estimated using data from solar panels including current, voltage, temperature, and the normal vectors of each solar panel. Because these values are obtained using internal sensors, it is easy for rovers to provide redundancy for IRAD. The normal vectors are used to apply to various shapes of rovers. Second, using the gravity vector obtained from an accelerometer, the attitude of a rover is estimated using a three-axis attitude determination method. The effectiveness of IRAD is verified through numerical simulations and experiments that show IRAD can estimate all the attitude angles (roll, pitch, and yaw) within a few degrees of accuracy, which is adequate for planetary explorations.

Takayuki Ishida; Masaki Takahashi

2014-01-01T23:59:59.000Z

491

Thermal Control Architecture for a Planetary and Lunar Surface Exploration Micro?Robot  

Science Journals Connector (OSTI)

A thermal control architecture design study is conducted for a novel robotic planetary and lunar surface exploration concept. The concept is based on the deployment of a large number of small spherical mobile robots over large areas which employ hopping bouncing and rolling as means of locomotion. The aim of the research is to prevent freezing and overheating of the robots without compromising their mechanical and thermal reliability and stability. The proposed thermal control architecture relies on a low emissive silver surface coating and a low conductive silica aerogel insulation layer. This enables a single design to be used for several important potential explorations. The effects of a thermal control heat rejection mechanism composed of a variable emittance coating and heat switch are also studied in order to increase mission flexibility.

Brian R. Burg; Steven Dubowsky; John H. Lienhard V.; Dimos Poulikakos

2007-01-01T23:59:59.000Z

492

Accurately Estimating the State of a Geophysical System with Sparse Observations: Predicting the Weather  

E-Print Network (OSTI)

Utilizing the information in observations of a complex system to make accurate predictions through a quantitative model when observations are completed at time $T$, requires an accurate estimate of the full state of the model at time $T$. When the number of measurements $L$ at each observation time within the observation window is larger than a sufficient minimum value $L_s$, the impediments in the estimation procedure are removed. As the number of available observations is typically such that $L \\ll L_s$, additional information from the observations must be presented to the model. We show how, using the time delays of the measurements at each observation time, one can augment the information transferred from the data to the model, removing the impediments to accurate estimation and permitting dependable prediction. We do this in a core geophysical fluid dynamics model, the shallow water equations, at the heart of numerical weather prediction. The method is quite general, however, and can be utilized in the analysis of a broad spectrum of complex systems where measurements are sparse. When the model of the complex system has errors, the method still enables accurate estimation of the state of the model and thus evaluation of the model errors in a manner separated from uncertainties in the data assimilation procedure.

Zhe An; Daniel Rey; Henry D. I. Abarbanel

2014-05-11T23:59:59.000Z

493

Non-invasive geophysical investigation and thermodynamic analysis of a palsa in Lapland, northwest Finland  

E-Print Network (OSTI)

Non-invasive geophysical prospecting and a thermodynamic model were used to examine the structure, depth and lateral extent of the frozen core of a palsa near Lake Peeraj\\"arvi, in northwest Finland. A simple thermodynamic model verified that the current climatic conditions in the study area allow sustainable palsa development. A ground penetrating radar (GPR) survey of the palsa under both winter and summer conditions revealed its internal structure and the size of its frozen core. GPR imaging in summer detected the upper peat/core boundary, and imaging in winter detected a deep reflector that probably represents the lower core boundary. This indicates that only a combined summer and winter GPR survey completely reveals the lateral and vertical extent of the frozen core of the palsa. The core underlies the active layer at a depth of ~0.6 m and extends to about 4 m depth. Its lateral extent is ~15 m x ~30 m. The presence of the frozen core could also be traced as minima in surface temperature and ground condu...

Kohout, Tom; Rasmus, Kai; Leppranta, Matti; Matero, Ilkka

2014-01-01T23:59:59.000Z

494

Geophysical investigation of burn pit, 128-H-1, 100-H Area  

SciTech Connect

The 128-H-1 burn pit is located in the northeast corner of 100-H Area. The objective of the survey was to delineate subsurface features in the 128-H-1 burn pit that may affect the emplacement of soil-gas probes. Ground-penetrating radar (GPR) and electromagnetic induction (EMI) were the two techniques used in the investigation. The methods were selected because they are non-intrusive, relatively fast, economical, and have been used successfully in other geophysical investigations on the Hanford Site. The GPR system used for this work utilized a 300-MHz antenna to transmit the Em energy into the ground. The transmitted energy is reflected back to a receiving antenna where variations in the return signal are recorded. Common reflectors include natural geologic conditions such as bedding, cementation, moisture, and clay, or man-made objects such as pipes, barrels, foundations, and buried wires. The studied depth, which varies from site to site, was 0--11 ft for this survey. The method is limited in depth by transmit power, receiver sensitivity, and attenuation of the transmitted energy. Depth of investigation is influenced by highly conductive material, such as metal drums, which reflect all the energy back to the receiver. Therefore, the method cannot ``see`` below such objects.

Szwartz, G.J.

1994-07-11T23:59:59.000Z

495

A Geological and Geophysical Study of the Geothermal Energy Potential of Pilgrim Springs, Alaska  

SciTech Connect

The Pilgrim Springs geothermal area, located about 75 km north of Nome, was the subject of an intensive, reconnaissance-level geophysical and geological study during a 90-day period in the summer of 1979. The thermal springs are located in a northeast-oriented, oval area of thawed ground approximately 1.5 km{sup 2} in size, bordered on the north by the Pilgrim River. A second, much smaller, thermal anomaly was discovered about 3 km northeast of the main thawed area. Continuous permafrost in the surrounding region is on the order of 100 m thick. Present surface thermal spring discharge is {approx} 4.2 x 10{sup -3} m{sup 3} s{sup -1} (67 gallons/minute) of alkali-chloride-type water at a temperature of 81 C. The reason for its high salinity is not yet understood because of conflicting evidence for seawater vs. other possible water sources. Preliminary Na-K-Ca geothermometry suggests deep reservoir temperatures approaching 150 C, but interpretation of these results is difficult because of their dependence on an unknown water mixing history. Based on these estimates, and present surface and drill hole water temperatures, Pilgrim Springs would be classified as an intermediate-temperature, liquid-dominated geothermal system.

Turner, Donald L.; Forbes, Robert B. [eds.

1980-01-01T23:59:59.000Z

496

Physics at Strathclyde N. Langford  

E-Print Network (OSTI)

#12;Physics at Strathclyde N. Langford Department of Physics University of Strathclyde #12 and Misconceptions o "There's no money in physics" o "I like the idea of a physics degree but what actual jobs do physics degree is great ­ if you want to teach physics" Untrue Physics leads to engineering NO

Mottram, Nigel

497

CONSTRAINTS ON THE LIFETIMES OF DISKS RESULTING FROM TIDALLY DESTROYED ROCKY PLANETARY BODIES  

SciTech Connect

Spitzer IRAC observations of 15 metal-polluted white dwarfs reveal infrared excesses in the spectral energy distributions of HE 0110-5630, GD 61, and HE 1349-2305. All three of these stars have helium-dominated atmospheres, and their infrared emissions are consistent with warm dust produced by the tidal destruction of (minor) planetary bodies. This study brings the number of metal-polluted, helium and hydrogen atmosphere white dwarfs surveyed with IRAC to 53 and 38, respectively. It also nearly doubles the number of metal-polluted helium-rich white dwarfs found to have closely orbiting dust by Spitzer. From the increased statistics for both atmospheric types with circumstellar dust, we derive a typical disk lifetime of log [t{sub disk}(yr)] = 5.6 {+-} 1.1 (ranging from 3 Multiplication-Sign 10{sup 4} to 5 Multiplication-Sign 10{sup 6} yr). This assumes a relatively constant rate of accretion over the timescale where dust persists, which is uncertain. We find that the fraction of highly metal-polluted helium-rich white dwarfs that have an infrared excess detected by Spitzer is only 23%, compared to 48% for metal-polluted hydrogen-rich white dwarfs, and we conclude from this difference that the typical lifetime of dusty disks is somewhat shorter than the diffusion timescales of helium-rich white dwarf. We also find evidence for higher time-averaged accretion rates onto helium-rich stars compared to the instantaneous accretion rates onto hydrogen-rich stars; this is an indication that our picture of evolved star-planetary system interactions is incomplete. We discuss some speculative scenarios that can explain the observations.

Girven, J.; Gaensicke, B. T.; Marsh, T. R. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Brinkworth, C. S.; Hoard, D. W. [Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 (United States); Farihi, J. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Koester, D., E-mail: j.m.girven@warwick.ac.uk [Institut fuer Theoretische Physik und Astrophysik, University of Kiel, 24098 Kiel (Germany)

2012-04-20T23:59:59.000Z

498

Faculty Position Therapeutic Medical Physics  

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spectroscopy, fluoroscopy, ultrasound, digital radiography, and nuclear medicine. The Colorado State University of subjects in Radiation Therapy Physics, Medical Imaging Physics, and Radiological Physics and Dosimetry

499

Physical risks of landing on a cometary nucleus  

Science Journals Connector (OSTI)

Comets originate from the outer solar system where the density and temperature of the planetary nebula were rather low. They form a distinct class of small solar system bodies and their physical properties differ considerably from those of any other known objects. The present knowledge of the cometary nucleus is cursory and driven more by imagination than by observational facts. Landing on a cometary nucleus, as planned during the ROSETTA mission, is of high scientific interest and will substantially improve our knowledge of the nature and origin of comets. However, successful landing and operating the instruments is an extraordinary challenge to engineers and scientists. Even a close approach to an inactive nucleus may jeopardize the orbiter. A wide range of uncommon and risky environmental conditions such as outgassing, a fragile surface, deposition of dust grains, extreme temperature variations, and pronounced topography have to be considered. These are described in physical terms based on model calculations ranging from simple one-dimensional heat transfer to gas-dynamic acceleration of dust particles. Environmental constraints relevant for landing and operating instruments on a cometary nucleus are presented such as sublimation and recondensation of water on the cold parts of the lander and varying illumination conditions over the extent of the mission. Aspects of risk reduction are discussed. The paper also summarizes the present knowledge about physical and structural properties of cometary nuclei relevant for the development of landing strategies.

E. Khrt; J. Knollenberg; H.U. Keller

1997-01-01T23:59:59.000Z

500

Physics high-ranking Journals (category 2) Advances in Physics  

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Physics high-ranking Journals (category 2) Advances in Physics Annual Review of Astronomy and Astrophysics Annual Review of Nuclear and Particle Science Applied Physics Letters Astronomy & Astrophysics Astronomy and Astrophysics Review Astrophysical Journal European Physical Journal D. Atomic, Molecular