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1

DEPARTMENT OF ASTRONOMY & ASTROPHYSICS Special Astronomy Seminar  

E-Print Network [OSTI]

DEPARTMENT OF ASTRONOMY & ASTROPHYSICS Special Astronomy Seminar October 13, 2011 Speaker : Mayukh) Abstract Black hole X-ray binaries (BHXBs) are widely observed sources in the X-ray and radio astronomy

Udgaonkar, Jayant B.

2

THE ASTRONOMY DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

THE ASTRONOMY MAJOR DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE September(2013(( #12;The Department of Physics and Astronomy website: http: //www.dartmouth.edu/~physics Upcoming colloquia://dartmouth.smartcatalogiq.com/en/2013/orc If you are thinking of majoring in astronomy, and have any questions, please contact any

3

THE ASTRONOMY DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

THE ASTRONOMY MAJOR DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE September 2013 #12;The Department of Physics and Astronomy website: http: //www.dartmouth.edu/~physics Upcoming, and Courses: http://dartmouth.smartcatalogiq.com/en/2013/orc If you are thinking of majoring in astronomy

4

COMPUTER USE AUTHORIZATION ASTRONOMY DEPARTMENT  

E-Print Network [OSTI]

COMPUTER USE AUTHORIZATION ASTRONOMY DEPARTMENT RADIO ASTRONOMY LABORATORY THEORETICALASTROPHYSICS authorized to support charges for the computer account. Please give the completed form to Bill Boyd in 401: ____________________________ User I.D.: ________________________ CONDITIONS OF USE The Astronomy Department provides computing

Militzer, Burkhard

5

UNDERGRADUATE PROGRAMS DEPARTMENT OF ASTRONOMY  

E-Print Network [OSTI]

UNDERGRADUATE PROGRAMS DEPARTMENT OF ASTRONOMY The UniversiTy of Texas aT aUsTin Astronomy is one richness of the universe. Join this adventure by exploring the astronomy program at the University of Texas at Austin. The Department of Astronomy at UT Austin is one of the top ten astronomy research programs

Jefferys, William

6

Yale University Department of Astronomy  

E-Print Network [OSTI]

Yale University Department of Astronomy Astronomy 110: Planets and Stars Course will be using selections from the following workbook: Lecture- Tutorials for Introductory Astronomy.93. It is available at the following website: http:// www.mypearsonstore.com/bookstore/lecture-tutorials-for-introductory-astronomy

7

DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE GRADUATE STUDENT HANDBOOK 2012-13 #12;2 TABLE .....................................................................27 #12;3 SECTION I PRACTICAL MATTERS 1. WELCOME AND OVERVIEW The Department of Physics and Astronomy with some undergraduate courses. The course requirements for physics and astronomy students are given

8

DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE GRADUATE STUDENT HANDBOOK 2014-15 #12;2 TABLE .....................................................................28 #12;3 SECTION I PRACTICAL MATTERS 1. WELCOME AND OVERVIEW The Department of Physics and Astronomy undergraduate courses. The course requirements for physics and astronomy students are given in Section II-1

9

PHYSICS & ASTRONOMY GRADUATE STUDENT HANDBOOK DEPARTMENT OF PHYSICS & ASTRONOMY  

E-Print Network [OSTI]

PHYSICS & ASTRONOMY GRADUATE STUDENT HANDBOOK DEPARTMENT OF PHYSICS & ASTRONOMY UNIVERSITY OF UTAH Fall 2012 Version 2012 .................................................................................... 11 3.1. Ph.D. in Physics 12 3.1.1. Astronomy & Astrophysics

Tipple, Brett

10

Strategic Plan Department of Physics and Astronomy  

E-Print Network [OSTI]

Strategic Plan Department of Physics and Astronomy University of Tennessee, Knoxville September (Ex Officio), and Hanno Weitering #12;Introduction The Department of Physics and Astronomy has over. Figure 1: Schematic diagram illustrating the Department of Physics and Astronomy's interactions

Dai, Pengcheng

11

June 18, 2013 1 Department of Astronomy  

E-Print Network [OSTI]

June 18, 2013 1 Department of Astronomy Harvard University _________________________________________________________________________________________ Harvard College Observatory 60 Garden Street, MS 46, Cambridge, MA 02138 SpecialAppointmentsintheFASDepartmentofAstronomy Harvard'sprograminastrophysicsisgreatlyenhancedbythealliancebetweentheHarvard Astronomy

12

University of Maryland Department of Astronomy  

E-Print Network [OSTI]

University of Maryland Department of Astronomy College Park, Maryland 20742 1. INTRODUCTION This report covers astronomical activities primarily within Maryland's Department of Astronomy but also AND INSTRUMENTATION 4.1 Laboratory for Millimeter-Wave Astronomy The Laboratory for Millimeter-wave Astronomy LMA

Gruner, Daniel S.

13

FAKULTT FR PHYSIK UND ASTRONOMIE DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

FAKULT√?T F√?R PHYSIK UND ASTRONOMIE DEPARTMENT OF PHYSICS AND ASTRONOMY DEKANAT / OFFICE OF THE DEAN beizuf√ľgen: 1. Die Angaben des Faches, f√ľr das die Habilitation erfolgen soll (Physik oder Astronomie). 1x 2

Heermann, Dieter W.

14

Strategic Plan Department of Physics and Astronomy  

E-Print Network [OSTI]

1 Strategic Plan Department of Physics and Astronomy University of Tennessee, Knoxville Fall 2011)........................................................... 46 #12;3 Introduction The Department of Physics and Astronomy has over the last two decades had

Dai, Pengcheng

15

DOUGLAS NATELSON Department of Physics and Astronomy  

E-Print Network [OSTI]

DOUGLAS NATELSON Department of Physics and Astronomy Rice University, MS: 61 6100 Main St. 3206 fabrication methods. PROFESSIONAL EXPERIENCE 7/10-present Professor, Department of Physics and Astronomy, Rice Engineering. 7/06-7/10 Associate Professor, Department of Physics and Astronomy, Rice University; member, Rice

Mellor-Crummey, John

16

University of Maryland Department of Astronomy  

E-Print Network [OSTI]

University of Maryland Department of Astronomy College Park, Maryland 20742 S0002-7537 98 07501-5 1. INTRODUCTION This report covers astronomical activities primarily within Maryland's Department of Astronomy students, was initiated this year from the Astronomy Department and the College of Computer, Mathematical

Gruner, Daniel S.

17

DOUGLAS NATELSON Department of Physics and Astronomy  

E-Print Network [OSTI]

DOUGLAS NATELSON Department of Physics and Astronomy Rice University, MS: 61 6100 Main St. 3115 fabrication methods. PROFESSIONAL EXPERIENCE 7/10-present Professor, Department of Physics and Astronomy, Rice/06-7/10 Associate Professor, Department of Physics and Astronomy, Rice University; member, Rice Quantum Institute

Natelson, Douglas

18

University of Maryland Department of Astronomy  

E-Print Network [OSTI]

University of Maryland Department of Astronomy College Park, Maryland 20742 S0002-7537 90 03801-X of the Theory and Computa- tion Panel of the Astronomy Decadal Survey, and Virginia Trimble part of the panel on Benefits to the Nation from Astronomy. The department was represented on advisory and users' committees

Gruner, Daniel S.

19

University of Maryland Department of Astronomy  

E-Print Network [OSTI]

University of Maryland Department of Astronomy College Park, Maryland 20742 S0002-7537 99 06701-3 This report covers astronomical activities primarily within Maryland's Department of Astronomy but also was elected to serve as chair of the Astronomy Section of the American Association for the Advancement

Gruner, Daniel S.

20

University of Maryland Department of Astronomy  

E-Print Network [OSTI]

University of Maryland Department of Astronomy College Park, Maryland 20742 S0002-7537 93 22641 . Recipients of PhD degrees and their current affiliations are Yanga Fernandez Inst. of Astronomy, U. Hawaii

Gruner, Daniel S.

Note: This page contains sample records for the topic "astronomy department abstract" 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

STATIA LUSZCZ-COOK Department of Astronomy  

E-Print Network [OSTI]

STATIA LUSZCZ-COOK Department of Astronomy University of California, Berkeley B-20 Hearst Field, University of California, Berkeley 2006 B.A. Astronomy with Honors, magna cum laude, Cornell University 2006 Graduate Student Instructor, Astronomy for Non-majors, U.C. Berke- ley 2004 - 2006 Undergraduate

Militzer, Burkhard

22

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS  

E-Print Network [OSTI]

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS Ongoing Lecture Pool in Astronomy and Astrophyics THE DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS at the University of California, the solar system, stellar structure and evolution, planets, high energy astrophysics, extragalactic

California at Santa Cruz, University of

23

he University of Texas at Austin Department of Astronomy is one of the largest astronomy  

E-Print Network [OSTI]

T he University of Texas at Austin Department of Astronomy is one of the largest astronomy programs virtually all of modern astronomy, placing the Department among the top few American astronomical institutions. The association between the Department of Astronomy and McDonald Observatory provides excellent

Jefferys, William

24

COLLOQUIUM SPEAKER SERIES Department of Physics and Astronomy  

E-Print Network [OSTI]

COLLOQUIUM SPEAKER SERIES Department of Physics and Astronomy Friday, Sept. 13, 2013 SB142 at 4 of Physics and Astronomy University of British Columbia Dr. Jens Dilling #12;

Calgary, University of

25

Physics and Astronomy Department Strategic Plan March 1, 2011  

E-Print Network [OSTI]

Physics and Astronomy Department Strategic Plan March 1, 2011 Executive Summary The Department of Physics & Astronomy performs world-class research and provides state-of-the-art training for students in astronomy, astrophysics, and gravitational physics; atomic/molecular/optical physics, quantum optics

Harms, Kyle E.

26

401-C Allen Hall Department of Physics and Astronomy  

E-Print Network [OSTI]

401-C Allen Hall Department of Physics and Astronomy 3941 O'Hara Street Pittsburgh, PA 15260 for these problems. A few years ago, a physics and astronomy graduate student, Brian Cherinka, took a course you between a few members of our department of Physics and Astronomy (Michael Wood-Vasey, Arthur Kosowsky

Marai, G. Elisabeta "Liz"

27

Giving Opportunities in the Department of Physics & Astronomy  

E-Print Network [OSTI]

Giving Opportunities in the Department of Physics & Astronomy _______________________________________________________________________ The Department of Physics and Astronomy has established different accounts to help us maintain our standard and astronomy laboratories. They are named in honor of Dr. Robert Lide, who served on the physics faculty for 35

Dai, Pengcheng

28

Mechanical Engineering Department technical abstracts  

SciTech Connect (OSTI)

The Mechanical Engineering Department publishes listings of technical abstracts twice a year to inform readers of the broad range of technical activities in the Department, and to promote an exchange of ideas. Details of the work covered by an abstract may be obtained by contacting the author(s). Overall information about current activities of each of the Department's seven divisions precedes the technical abstracts.

Denney, R.M. (ed.)

1982-07-01T23:59:59.000Z

29

Physics and Astronomy Department Withdrawal Policy In accordance with university policy, the Physics and Astronomy department permits withdrawals from  

E-Print Network [OSTI]

Physics and Astronomy Department Withdrawal Policy In accordance with university policy, the Physics and Astronomy department permits withdrawals from P&A courses up to the withdrawal deadline with associated, co-requisite labs. Physics 101/102, 111/112, 121/122, 220/222, 230/232/ 240/242 Astronomy 115

Bland, Roger

30

JOHN KORMENDY ADDRESS AND TELEPHONE NUMBER: Department of Astronomy  

E-Print Network [OSTI]

VITA JOHN KORMENDY ADDRESS AND TELEPHONE NUMBER: Department of Astronomy University of Texas@astro.as.utexas.edu (email) EDUCATION: B. Sc. 1970, Honours Mathematics, Physics and Chemistry (Astronomy Division), University of Toronto Ph. D. 1976, Astronomy, California Institute of Technology, Pasadena, CA POSITIONS: Apr

Kormendy, John

31

Astronomy Page 65Sonoma State University 2012-2013 Catalog DEPARTMENT OFFICE  

E-Print Network [OSTI]

Astronomy Page 65Sonoma State University 2012-2013 Catalog ASTRONOMY DEPARTMENT OFFICE Darwin Hall Hongtao Shi * Faculty Early Retirement Program Program Offered Minor in Astronomy Astronomy, offered as a minor in the Department of Physics and Astronomy, is the study of the planets, stars, and galaxies

Ravikumar, B.

32

Astronomy Page 63Sonoma State University 2014-2015 Catalog DEPARTMENT OFFICE  

E-Print Network [OSTI]

Astronomy Page 63Sonoma State University 2014-2015 Catalog ASTRONOMY DEPARTMENT OFFICE Darwin Hall Shi * Faculty Early Retirement Program Program Offered Minor in Astronomy Astronomy, offered as a minor in the Department of Physics and Astronomy, is the study of the planets, stars, and galaxies

Ravikumar, B.

33

Page 66 Astronomy Sonoma State University 2008-2010 Catalog Department Office  

E-Print Network [OSTI]

Page 66 Astronomy Sonoma State University 2008-2010 Catalog Department Office Darwin Hall 300 (707 minor in astronomy Astronomy, offered as a minor in the Department of Physics and Astronomy of Astronomy and Astrophysics, the application of physics principles to astronomical observations, today deal

Ravikumar, B.

34

BS in PHYSICSASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy  

E-Print Network [OSTI]

BS in PHYSICS­ASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy For students Astronomy Phscs 140 Electronics Lab Phscs 145 Experimental Methods in Physics Phscs 191 Intro to Physics Astronomy Phscs 228 Stellar and Extragalactic Astronomy Phscs 230 Computational Physics Lab 1 Phscs 291

Hart, Gus

35

BS in PHYSICSASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy  

E-Print Network [OSTI]

BS in PHYSICS­ASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy For students Phscs 127 Descriptive Astronomy Phscs 140 Electronics Lab Phscs 145 Experimental Methods in Physics* Modern Physics Phscs 227 Solar System Astronomy Phscs 228 Stellar and Extragalactic Astronomy Phscs 230

Olsen Jr., Dan R.

36

BS in PHYSICSASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy  

E-Print Network [OSTI]

BS in PHYSICS­ASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy For students 123 Intro to Waves, Optics, & Thermodynamics Phscs 127 Descriptive Astronomy Phscs 191 Intro Solar System Astronomy Phscs 228 Stellar and Extragalactic Astronomy Phscs 230 Computational Physics Lab

Olsen Jr., Dan R.

37

Astronomy Page 73Sonoma State University 2006-2008 Catalog Department Office  

E-Print Network [OSTI]

Astronomy Page 73Sonoma State University 2006-2008 Catalog Department Office Darwin Hall 300 (707 S. Tenn *Faculty Early Retirement Program Program Offered Minor in Astronomy Astronomy, offered as a minor in the Department of Physics and Astronomy, is the study of the planets, stars, and galaxies

Ravikumar, B.

38

Page 66 Astronomy Sonoma State University 2011-2012 Catalog Department Office  

E-Print Network [OSTI]

Page 66 Astronomy Sonoma State University 2011-2012 Catalog Department Office Darwin Hall 300 (707 Program Offered Minor in Astronomy Astronomy, offered as a minor in the Department of Physics and Astronomy, is the study of the planets, stars, and galaxies in the universe beyond the earth's atmosphere

Ravikumar, B.

39

DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE  

E-Print Network [OSTI]

environment, including the Van Allen Radiation Belts and their adverse effects on spacecraft and astronauts with application to development of nuclear fusion as an energy source. ·research many topics in astronomy; see astonishing effects of quantum physics and the transition between quantum and classical physics. (Lower right

40

DEPARTMENT OF PHYSICS AND ASTRONOMY DARTMOUTH COLLEGE  

E-Print Network [OSTI]

such as the origin of the universe and the nature of dark matter and dark energy. ∑study the solar system space and seminars: http://www.dartmouth.edu/~physics/news/calendar.html Organization, Regulations, and Courses: http with application to development of nuclear fusion as an energy source. ∑research many topics in astronomy; see

Note: This page contains sample records for the topic "astronomy department abstract" 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

John S. Colton Curriculum Vitae, Jun 2012 828 E 1080 N Department of Physics and Astronomy  

E-Print Network [OSTI]

JSC-1 John S. Colton ­ Curriculum Vitae, Jun 2012 828 E 1080 N Department of Physics and Astronomy University, Department of Physics and Astronomy, Provo UT. Duties include teaching, research, mentoring University, Department of Physics and Astronomy, Provo UT. Aug 2003 ­ Aug 2007 Assistant Professor

Hart, Gus

42

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy  

E-Print Network [OSTI]

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy 2011.1 Master of Science;Ruprecht-Karls-University Heidelberg 2 Department of Physics and Astronomy 2011.1 Versions: Version 2011 & organic electronics Module descriptions astronomy #12;Ruprecht-Karls-University Heidelberg 3 Department

Heermann, Dieter W.

43

BS in PHYSICSASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy  

E-Print Network [OSTI]

BS in PHYSICS­ASTRONOMY (694832) MAP Sheet Department of Physics and Astronomy For students Principles of Physics 2 Phscs 127 Descriptive Astronomy Phscs 140 Electronics Lab Phscs 145 Experimental semester. Phscs 220 Principles of Physics 3 Phscs 222 Modern Physics Phscs 227 Solar System Astronomy Phscs

Hart, Gus

44

THE UNIVERSITY OF NEW MEXICO PHYSICS & ASTRONOMY DEPARTMENT  

E-Print Network [OSTI]

THE UNIVERSITY OF NEW MEXICO PHYSICS & ASTRONOMY DEPARTMENT Recruitment of Part-Time Instructors faculty positions are submitted through UNMJobs, the University of New Mexico's on-line application form assistance with UNMJobs, please e-mail UNMJobs@unm.edu or call (505) 277-6947. The University of New Mexico

New Mexico, University of

45

Double Beta Decay Experiments Department of Physics and Astronomy  

E-Print Network [OSTI]

1 Double Beta Decay Experiments A. Piepkea a Department of Physics and Astronomy University. The experimen- tal investigation of the nuclear double beta decay is one of the key techniques for solving, such as the evaluation of the beta spec- tra near their endpoint, or neutrinoless double beta decay. The latter technique

Piepke, Andreas G.

46

Did you know that the University of Kansas Department of Physics and Astronomy . . .  

E-Print Network [OSTI]

Did you know that the University of Kansas Department of Physics and Astronomy . . . · has? · ranks in the top fifth of US university physics and astronomy departments in quality of productivity Physics and Astronomy (for students interested in the applica tion of computers to problem solving

47

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy  

E-Print Network [OSTI]

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy 20102/3 Master-Karls-University Heidelberg 2 Department of Physics and Astronomy 20102/3 1. The master degree in physics).............................................................18 3.1. Astronomy and Astrophysics

Heermann, Dieter W.

48

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy  

E-Print Network [OSTI]

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy 2012.1/v2 Master 2011) #12;Ruprecht-Karls-University Heidelberg 2 Department of Physics and Astronomy 2012.1/v2 Versions descriptions condensed matter & organic electronics Module descriptions astronomy Version 2012.1/v2

Heermann, Dieter W.

49

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy  

E-Print Network [OSTI]

Ruprecht-Karls-University Heidelberg 1 Department of Physics and Astronomy 2012.2/v3 Master 2011) #12;Ruprecht-Karls-University Heidelberg 2 Department of Physics and Astronomy 2012.2/v3 Versions descriptions condensed matter & organic electronics Module descriptions astronomy Version 2012.1/v2

Heermann, Dieter W.

50

PH.D. REQUIREMENTS IN THE DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

PH.D. REQUIREMENTS IN THE DEPARTMENT OF PHYSICS AND ASTRONOMY Completion of the Ph.D. requires (1 of Physics and Astronomy requires 36 hours of formal course work1 including: · Seven core courses covering the foundations of physics or astronomy, listed be- low, totaling 19 credit hours; · Two graduate-level courses

Bordenstein, Seth

51

OXYGEN ABUNDANCE OF OPEN CLUSTER DWARFS Department of Astronomy, Peking University, Beijing 100871, China; shenzx@bac.pku.edu.cn  

E-Print Network [OSTI]

OXYGEN ABUNDANCE OF OPEN CLUSTER DWARFS Z.-X. Shen Department of Astronomy, Peking University 100871, China Received 2005 June 30; accepted 2007 January 19 ABSTRACT We present oxygen abundances in the open cluster Pleiades derived from the [O i] k6300 forbidden line. Stellar parameters and oxygen

Liu, Xiaowei

52

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS  

E-Print Network [OSTI]

in Astronomy, Physics, or related field; demonstrated record of research PREFERRED QUALIFICATIONS: Postdoctoral

California at Santa Cruz, University of

53

Iowa State University Department of Physics and Astronomy  

E-Print Network [OSTI]

, black illuminated detector that can be cooled to -70 C with thermoelectric cooling. At the New- tonian-based astronomy modules, collectively known as ``the Polaris Project.'' These cover basic concepts that often at the freshman non-scientist, the first module has been tested by students with back- grounds ranging from none

54

2000 Astronomy Department, University of Texas at Austin Full Of Hot Air?  

E-Print Network [OSTI]

©2000 Astronomy Department, University of Texas at Austin Full Of Hot Air? Introduction Light has standing by a pool, the medium is air. If you are looking at the Moon from under water after you jump into the pool, the mediums are both air and water. The Moon would appear dif- ferent from underwater because

Hemenway, Mary Kay

55

BS in PHYSICS (694821) MAP Sheet Department of Physics and Astronomy  

E-Print Network [OSTI]

BS in PHYSICS (694821) MAP Sheet Department of Physics and Astronomy For students entering and 2 Arts Letters Scientific Principles & Reasoning Biological Science Physical Science Social Science of Physics 1 Phscs 123 Principles of Physics 2 Phscs 140 Electronics Lab Phscs 145 Experimental Methods

Hart, Gus

56

Physics and Astronomy Department San Francisco State University Physics Readiness Exam  

E-Print Network [OSTI]

Physics and Astronomy Department San Francisco State University Physics Readiness Exam Math Qualification Test for Introductory Physics ­ Physics 111 or Physics 220 In addition to meeting course prerequisites, students wishing to enroll in Physics 111 or Physics 220 must demonstrate adequate competence

Golterman, Maarten

57

The University of Michigan Department of Astronomy Exhibit Museum of Natural History  

E-Print Network [OSTI]

The University of Michigan Department of Astronomy Exhibit Museum of Natural History Student Astronomical Society and Michigan Center for Theoretical Physics present A distinguished speaker series solar system SouthwestResearchInstitute Friday Our local microcosmos CarlHeiles October5 Universityof

Oey, Sally

58

M.S. Astronomy Program M.S. in Astronomy  

E-Print Network [OSTI]

M.S. Astronomy Program M.S. in Astronomy Department(s) Physics and Astronomy College Sciences 1 for later reference. 1. understanding of a variety of fields of physics and astronomy at the graduate level 2*. performance of an astronomy research project suitable for a masters thesis 3*. ability

Hemmers, Oliver

59

Ph.D. Astronomy Program Ph.D. in Astronomy  

E-Print Network [OSTI]

Ph.D. Astronomy Program Ph.D. in Astronomy Department(s) Physics and Astronomy College Sciences 1 physics at the graduate level 4. understand observational astronomy techniques 5. understand astrophysics strong background of knowledge and expertise in physics and astronomy #12;2. Curriculum Alignment

Hemmers, Oliver

60

Curriculum Vitae: Michael Riley Brown Department of Physics and Astronomy  

E-Print Network [OSTI]

(spheromak and field reversed configuration). (9/94- Present) External Support U. S. Department of Energy and operation of a spheromak accelerator for the purposes of tokamak refueling and current drive on the ENCORE discharges for spheromak research. (6/87-5/89) Fellowship at Dartmouth College to study compressible MHD

Brown, Michael R.

Note: This page contains sample records for the topic "astronomy department abstract" 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

GLAS-PPE/2007-01 Department of Physics & Astronomy  

E-Print Network [OSTI]

administrative domain, in our case this is the ATLAS VO. A Resource Provider (RP) is a facility offering)141 330 5881 Integration of the ATLAS VOMS system with the ATLAS Metadata Interface T.Doherty Department This document provides an account of the development of a Javabased solution to integrate the ATLAS VOMS system

Glasgow, University of

62

IceCube: An Instrument for Neutrino Astronomy  

E-Print Network [OSTI]

An Instrument for Neutrino Astronomy Francis Halzen 1 andAn Instrument for Neutrino Astronomy Francis Halzen 1 and94720 Abstract Neutrino astronomy beyond the Sun was first

Halzen, F.

2010-01-01T23:59:59.000Z

63

ABSTRACT  

Broader source: Energy.gov (indexed) [DOE]

Conference on Building Commissioning Whitepaper on: Commissioning of Combined Heat and Power Systems Information was compiled with support from the U. S. Department of Energy and...

64

ABSTRACT  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary)morphinanInformation Desert SouthwestTechnologies |November 2011A FirstEMSLAEMSL341AACEii ABSTRACT This

65

Astronomy Department UC Berkeley B-20 Hearst Field Annex # 3411 Berkeley, CA 94720  

E-Print Network [OSTI]

are primary goals of the Astronomy Decadal Review. NASA, Goddard Space Flight Center, Greenbelt, MD NPP Fellow://ratir.astroscu.unam.mx/public/ · Support the construction (mechanical, cryogenic, optical, and electronic systems), commissioning

Militzer, Burkhard

66

University of Maryland Graduate Program in Astronomy  

E-Print Network [OSTI]

University of Maryland Graduate Program in Astronomy: A Handbook for Graduate Students Last revised student in the Department of Astronomy, a general overview of the graduate program in Astronomy of Astronomy. Information on University regulations and deadlines can be found at the Graduate School's website

Gruner, Daniel S.

67

Astronomy Major www.physicsandastronomy.pitt.edu  

E-Print Network [OSTI]

Astronomy Major www.physicsandastronomy.pitt.edu Revised: 03/2013 The University of Pittsburgh's internationally recognized Department of Physics and Astronomy has been an important leader at the frontier, chemistry, engineering, and computer science. Required courses for the Astronomy major The BA in astronomy

Jiang, Huiqiang

68

ASTRONOMY 104: UNDERGRADUATE ASTRONOMY SEMINAR  

E-Print Network [OSTI]

1 ASTRONOMY 104: UNDERGRADUATE ASTRONOMY SEMINAR SYLLABUS Unique Number 47750 Class Meetings together with fellow astronomy majors, and those in other majors who are keen on astronomy. We hope to discuss present and future pathways to success in and around astronomy, and to share with you some

69

THE NEWSLETTER OF THE UNIVERSITY OF TENNESSEE DEPARTMENT OF PHYSICS AND ASTRONOMY CROSS SECTIONS  

E-Print Network [OSTI]

of novice astronomy students have just been given control of nine brand new $3000 Meade LX 200R telescopes. Pfounts controls the camera using a laptop, which is displaying a fuzzy image of stars that she hopes are near the galaxy. Every second the camera sends an updated image to the screen so Petschulat can focus

Tennessee, University of

70

At the end of every Spring Semester the Physics & Astronomy Department recognizes the achievements of  

E-Print Network [OSTI]

greater than 3.9 and had participated in re- search before they entered the senior year). After leaving term's lectures. When he retired from the university in the late '60s the Thomas H. Osgood in Physics or Astronomy who was entering his/her senior year. The basis of the award, as designated by Ver

71

MITIGATING THE THREAT TO SOLAR SYSTEM SCIENCE IMPOSED BY MCT PROGRAMS. Michael H. Wong, Astronomy Department, University of California, Berkeley CA 94720-3411  

E-Print Network [OSTI]

MITIGATING THE THREAT TO SOLAR SYSTEM SCIENCE IMPOSED BY MCT PROGRAMS. Michael H. Wong, Astronomy Department, University of California, Berkeley CA 94720-3411 mikewong@astro.berkeley.edu A White Paper on HST's highly-productive solar system science program, which is characterized by projects with relatively small

72

Astronomy 9603B -Star Formation Star Formation: Astronomy 9603B (Winter 2012)  

E-Print Network [OSTI]

Astronomy 9603B - Star Formation Star Formation: Astronomy 9603B (Winter 2012) Lecturer: Prof below. Contact information: Martin Houde Associate Professor Department of Physics and Astronomy Room 207, Physics and Astronomy Building E-mail: mhoude2@uwo.ca Phone: (519) 661-2111 x: 86711 (office) Fax

Lennard, William N.

73

ABSENCE OF GEOMETRIC MODELS IN MEDIEVAL CHINESE ASTRONOMY  

E-Print Network [OSTI]

ABSENCE OF GEOMETRIC MODELS IN MEDIEVAL CHINESE ASTRONOMY JAYANT SHAH Abstract. In 718 A.D., Ch) on astronomy was entirely based on the Indian astronomy of the 7th century which in turn was based on the geometric astronomy of the Greeks. A few years later, the emperor asked I-hsing (Yixing in pinyin

Shah, Jayant M.

74

University of British Columbia Physics & Astronomy Outreach Program  

E-Print Network [OSTI]

University of British Columbia Physics & Astronomy Outreach Program Faraday Show is the Outreach Department of Physics & Astronomy, University of British Columbia Email: outreach@phas.ubc.ca; Phone: 604

Karczmarek, Joanna

75

Abstract--The U. S. Department of Energy (DOE) is studying Yucca Mountain, Nevada, to determine the mountain's suitability  

E-Print Network [OSTI]

183 Abstract--The U. S. Department of Energy (DOE) is studying Yucca Mountain, Nevada, to determine in the Yucca Mountain Project area. Fifty- seven study plots were established on disturbances in four pri- mary plans for site-specific disturbances at Yucca Mountain. In 1979, the Department of Energy identified

76

Astronomy 362: Observational Astronomy University of Montana  

E-Print Network [OSTI]

Astronomy 362: Observational Astronomy University of Montana Fall 2010 T/Th 2:10 ­ 3:30 pm CHCB 227://www.physics.umt.edu/~nate/astr362/ Course Description Observational astronomy relies heavily on application of advanced technology astronomy is dominated by the CCD and related pixel array detectors: digital devices with unprecedented

Vonessen, Nikolaus

77

Physics and Astronomy Scott Sommerfeldt, Chair  

E-Print Network [OSTI]

Physics and Astronomy Scott Sommerfeldt, Chair N-281A ESC, (801) 422-2205 College of Physical programs in the Department of Physics and Astronomy are open enrollment. However, special limitations apply principles that govern the structure and dynamics of matter and energy in the physical world, from subatomic

Hart, Gus

78

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

257 Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics and Astronomy offers undergraduate and graduate programs for a wide range of interests. The bachelor of arts degrees in physics and astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

79

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics and Astronomy offers undergraduate and graduate programs for a wide range of interests. The bachelor of arts degrees in physics and astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

80

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

1 Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics and Astronomy offers undergraduate and graduate programs for a wide range of interests. The bachelor of arts degrees in physics and astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

Note: This page contains sample records for the topic "astronomy department abstract" 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

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

233 Physics and Astronomy The Wiess School of Natural Sciences Chair F. Barry Dunning Professors of Physics and Astronomy offers undergraduate and graduate programs for a wide range of interests. The bachelor of arts degrees in physics and in #12;234 DEPARTMENTS / Physics and Astronomy All physics majors

Richards-Kortum, Rebecca

82

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

246 Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics and Astronomy offers undergraduate and graduate programs for a wide range of interests. The bachelor of arts degrees in physics and astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

83

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

234 Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics andAstronomy offers undergraduate and graduate pro- grams for a wide range of interests.The bachelor of arts degrees in physics and in astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

84

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

228 Physics and Astronomy The Wiess School of Natural Sciences Degrees Offered: BA, BS, MST, MS, PhD The Department of Physics andAstronomy offers undergraduate and graduate pro- grams for a wide range of interests.The bachelor of arts degrees in physics and in astronomy are suitable for students who wish to obtain a broad

Richards-Kortum, Rebecca

85

The Astronomy Freshman Prizes for Excellence (AFPE) typically range from $2,000 to $10,000 per student and will be awarded yearly to freshmen of outstanding promise admitted to the first year of the UT Astronomy  

E-Print Network [OSTI]

The Astronomy Freshman Prizes for Excellence (AFPE) typically range from $2,000 to $10,000 per Astronomy program. The AFPE awards are funded jointly by the Astronomy Department excellence funds@astro.as.utexas.edu Mailing address: Char Burke - Student Coordinator Department of Astronomy The University of Texas

Jefferys, William

86

Astronomy & Astrophysics manuscript no. 7834 c ESO 2008 February 1, 2008  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. 7834 c ESO 2008 February 1, 2008 Isotopic anomaly of Astronomy, University of Vienna, T¬®urkenschanzstra√?e 17, 1180 Vienna, Austria 2 Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48, 109017 Moscow, Russia 3 Department of Physics and Astronomy

87

NATIONAL RADIO ASTRONOMY OBSERVATORY CHARLOTTESVILLE, VIRGINIA  

E-Print Network [OSTI]

No. 186 A PROGRESS REPORT ON JOSEPHSON JUNCTION MIXERS FOR MILLIMETER WAVE RADIO ASTRONOMY D. R. DECKER FEBRUARY 1978 NUMBER OF COPIES: 150 #12;A PROGRESS REPORT ON JOSEPHSON JUNCTION MIXERS FOR MILLIMETER WAVE RADIO ASTRONOMY D. R. Decker ABSTRACT Interest in use of Josephson junction devices

Groppi, Christopher

88

Australian Aboriginal Astronomy in the International Year of Astronomy  

E-Print Network [OSTI]

1 Australian Aboriginal Astronomy in the International Year of Astronomy Ray P. Norris CSIRO Astronomy & Space Science, NSW, Australia Warawara Dept. The International year of Astronomy seemed an excellent opportunity to tell the wider

Norris, Ray

89

PROPOSED PORTHOLE FOR ASTRONOMY MAJORS Information for Astronomy Majors  

E-Print Network [OSTI]

PROPOSED PORTHOLE FOR ASTRONOMY MAJORS Information for Astronomy Majors The Astronomy Major sciences such as Astronomy, Physics, or Engineering. (Link to details on Astrophysics Concentration) The General Astronomy Concentration is intended for students who do not plan on research careers in astronomy

Richardson Jr., James E.

90

Astronomy & Astrophysics manuscript no. GJpraesepeII c ESO 2008 March 26, 2008  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. GJpraesepeII c ESO 2008 March 26, 2008 The effect Institut f¨ur Astronomie, Universit¨at Wien, T¨urkenschanzstrasse 17, 1180 Wien, Austria. e-mail: fossati-mail: sba@arm.ac.uk 3 Department of Physics & Astronomy, University of Western Ontario, London, N6A 3K7

91

New Astronomy Reviews 45 (2001) 663742 www.elsevier.com/locate/newar  

E-Print Network [OSTI]

New Astronomy Reviews 45 (2001) 663­742 www.elsevier.com/locate/newar Advective accretion disks Institute, Profsoyuznaya 84/32, Moscow 117810, Russia b Department of Astronomy, Cornell University, Ithaca-6473(01)00146-4 #12;664 G.S. Bisnovatyi-Kogan, R.V.E. Lovelace / New Astronomy Reviews 45 (2001) 663­742 infalling

92

Astronomy, Lund, 24 February, 2011 Twisting of Light around Spinning Black Holes  

E-Print Network [OSTI]

Astronomy, Lund, 24 February, 2011 Twisting of Light around Spinning Black Holes and other uses with contributions from Fabrizio Tamburini Department of Astronomy, University of Padova, Italy and LOFAR/LOIS project members Uppsala and elsewhere #12;Astronomy, Lund, February, 2011 Very readable paper on POAM

93

Astronomy & Astrophysics manuscript no. 9183 c ESO 2008 January 8, 2008  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. 9183 c ESO 2008 January 8, 2008 LETTER TO THE EDITOR. Ryabchikova2,3, S. Bagnulo4, and G. Lo Curto5 1 Department of Astronomy and Space Physics, Uppsala University, SE-751 20, Uppsala, Sweden 2 Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya 48

94

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014 The Hawk-I UDS for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK 3 Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA, SA 4 Max-Planck-Institut fur extraterrestrische Physik

Faraon, Andrei

95

David Tsiklauri, Astronomy Unit, School of Physics and Astronomy  

E-Print Network [OSTI]

David Tsiklauri, Astronomy Unit, School of Physics and Astronomy astro.qmul.ac.uk/~tsiklauri 19 Sep oscillations, waves in magnetised plasmas, elements of plasma kinetics. David Tsiklauri Astronomy Unit Queen, Astronomy Unit, School of Physics and Astronomy astro.qmul.ac.uk/~tsiklauri 19 Sep 2012 STFC summer school

96

ASTRONOMY AND ASTROLOGY IN THE  

E-Print Network [OSTI]

ASTRONOMY AND ASTROLOGY IN THE WORKS OF CHAUCER Done By: Ameerah Bte Po'ad Mattar Chew Yoke Wah in astronomy albeit the astronomy incorporated in his works are concealed in a way that it is difficult to extract his full knowledge of astronomy. Astronomy was not the key topic in Chaucer's works although his

Aslaksen, Helmer

97

arXiv:astro-ph/0106481v126Jun2001 MASSIVE DATASETS IN ASTRONOMY  

E-Print Network [OSTI]

arXiv:astro-ph/0106481v126Jun2001 Chapter 1 MASSIVE DATASETS IN ASTRONOMY Robert J. Brunner, S 21218 USA szalay@pha.jhu.edu Abstract Astronomy has a long history of acquiring, systematizing archives and services representing a new in- formation infrastructure for astronomy of the 21st century

Prince, Thomas A.

98

Astronomy in Argentina  

E-Print Network [OSTI]

This article analyses the current state of Astronomy in Argentina and describes its origins. We briefly describe the institutions where astronomical research takes place, the observational facilities available, the training of staff and professionals, and the role of the institutions in scientific promotion. We also discuss the outreach of Astronomy towards the general public, as well as amateur activities. The article ends with an analysis of the future prospects of astronomy in Argentina.

Muriel, HernŠn

2013-01-01T23:59:59.000Z

99

International Year of Astronomy: Join the yearlong astronomy party  

E-Print Network [OSTI]

International Year of Astronomy: Join the yearlong astronomy party To mark the 400th anniversary are having a yearlong party.The InternationalYear of Astronomy is organized by the United Nations Educational!feature local and regional events such as public telescope viewings and public lectures, astronomy-themed plays

Pedersen, Tom

100

Kriti 2010 Astronomy Design Problems Equinox, The Astronomy Club  

E-Print Network [OSTI]

Kriti 2010 Astronomy Design Problems Equinox, The Astronomy Club February 8, 2010 Introduction The Astronomy Design Problems constitute a new event introduced in Kriti this year. Below, you will nd two-trivial. While both certainly have solu- tions, to someone new to amateur astronomy, they would represent

Plotkin, Joshua B.

Note: This page contains sample records for the topic "astronomy department abstract" 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

CRAF Handbook for Radio Astronomy  

E-Print Network [OSTI]

CRAF Handbook for Radio Astronomy EUROPEAN SCIENCE FOUNDATION Committee on Radio Astronomy forum for science. The ESF Expert Committee on Radio Astronomy Frequencies, CRAF, was established Astronomy Service and other passive applications. Cover: The 76-m diameter Lovell Telescope at Jodrell Bank

Rodriguez, Luis F.

102

Superconducting Tunnel Junctions as Direct Detectors for Submillimeter Astronomy  

E-Print Network [OSTI]

Superconducting Tunnel Junctions as Direct Detectors for Submillimeter Astronomy A Dissertation 2008 by John Daniel Teufel. All rights reserved. #12;Abstract Superconducting Tunnel Junctions on the of performance of superconducting tunnel junctions (STJ) as direct detectors for submillimeter radiation. Over

103

atmospheric physics department: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

final paper in ACP if available. unknown authors 7 Department of Physics UCLA Physics and Astronomy Department Materials Science Websites Summary: Department of Physics...

104

astronomy: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

SEMINAR Physics Websites Summary: 1 ASTRONOMY 104: UNDERGRADUATE ASTRONOMY SEMINAR SYLLABUS Unique Number 47750 Class Meetings together with fellow astronomy majors, and those...

105

Astronomy in Ukraine  

E-Print Network [OSTI]

The current and prospective status of astronomical research in Ukraine is discussed. A brief history of astronomical research in Ukraine is presented and the system organizing scientific activity is described, including astronomy education, institutions and staff, awarding higher degrees/titles, government involvement, budgetary investments and international cooperation. Individuals contributing significantly to the field of astronomy and their accomplishments are mentioned. Major astronomical facilities, their capabilities, and their instrumentation are described. In terms of the number of institutions and personnel engaged in astronomy, and of past accomplishments, Ukraine ranks among major nations of Europe. Current difficulties associated with political, economic and technological changes are addressed and goals for future research activities presented.

Ya. V. Pavlenko; I. B. Vavilova; T. Kostiuk

2005-12-16T23:59:59.000Z

106

Physics & Astronomy Degree options  

E-Print Network [OSTI]

148 Physics & Astronomy Degree options BSc (Single Honours Degrees) Astrophysics Physics MPhys (Single Honours Degrees) Astrophysics Physics Theoretical Physics BSc (Joint Honours Degrees) Physics) Theoretical Physics and Mathematics MSci (Joint Honours Degree) Physics and Chemistry Entrance Requirements

Brierley, Andrew

107

CCD Astronomy Software User's Guide  

E-Print Network [OSTI]

CCDSoft CCD Astronomy Software User's Guide Version 5 Revision 1.11 Copyright © 1992­2006 SantaSky Astronomy Software, and AutomaDome are trademarks of Software Bisque. WindowsTM is a trademark of Microsoft

108

Research Review NOVA and Astronomy  

E-Print Network [OSTI]

Research Review NOVA and Astronomy 2010 October 2011 #12;2 QANU / Research Review NOVA and Astronomy Quality Assurance Netherlands Universities (QANU) Catharijnesingel 56 PO Box 8035 3503 RA Utrecht NOVA and Astronomy 3 Contents: Update 5 1. The Review Committee and Review Procedures 7 2. Remarks

van Rooij, Robert

109

Taught degrees MSc in Astronomy  

E-Print Network [OSTI]

Essentials Taught degrees MSc in Astronomy MSc in Cosmology Research degrees MPhil, PhD in Astronomy Related degrees MSc in Particle Physics (p135) MSc in Physics (p135) MSc in Physics (Euro-class undergraduate honours degree in a physics-, mathematics- or astronomy-based subject. Other degrees

Sussex, University of

110

Taught degrees MSc in Astronomy  

E-Print Network [OSTI]

Essentials Taught degrees MSc in Astronomy MSc in Cosmology Research degrees MPhil, PhD in Astronomy Related degrees MSc in Computational Mathematics (p119) MSc in Particle Physics (p137) MSc-class undergraduate honours degree in a physics-, mathematics- or astronomy-based subject. Other degrees

Sussex, University of

111

Gamma-ray Astronomy  

E-Print Network [OSTI]

The relevance of gamma-ray astronomy to the search for the origin of the galactic and, to a lesser extent, the ultra-high-energy cosmic rays has long been recognised. The current renaissance in the TeV gamma-ray field has resulted in a wealth of new data on galactic and extragalactic particle accelerators, and almost all the new results in this field were presented at the recent International Cosmic Ray Conference (ICRC). Here I summarise the 175 papers submitted on the topic of gamma-ray astronomy to the 30th ICRC in Merida, Mexico in July 2007.

Jim Hinton

2007-12-20T23:59:59.000Z

112

Cosmic Ray Astronomy  

E-Print Network [OSTI]

Cosmic ray astronomy attempts to identify and study the sources of ultrahigh energy cosmic rays. It is unique in its reliance on charged particles as the information carriers. While no discrete source of ultrahigh energy cosmic rays has been identified so far, a new generation of detectors is acquiring the huge exposure that is needed at the highest energies, where deflection by magnetic fields is minimized and the background from distant sources is eliminated by pion photoproduction. In this paper, we summarize the status of cosmic ray astronomy, describing the detectors and the analysis techniques.

Paul Sommers; Stefan Westerhoff

2008-02-09T23:59:59.000Z

113

Fifteenth annual U.S. Department of Energy low-level radioactive waste management conference: Agenda and abstracts  

SciTech Connect (OSTI)

The goal of the conference was to give the opportunity to identify and discuss low-level radioactive waste management issues, share lessons learned, and hear about some of the latest advances in technology. Abstracts of the presentations are arranged into the following topical sections: (1) Performance Management Track: Performance assessment perspectives; Site characterization; Modeling and performance assessment; and Remediation; (2) Technical Track: Strategic planning; Tools and options; Characterization and validation; Treatment updates; Technology development; and Storage; (3) Institutional Track: Orders and regulatory issues; Waste management options; Legal, economic, and social issues; Public involvement; Siting process; and Low-level radioactive waste policy amendment acts.

NONE

1993-12-31T23:59:59.000Z

114

M.S. Physics and Astronomy, University of Pittsburgh, 2005 Submitted to the Graduate Faculty of  

E-Print Network [OSTI]

M.S. Physics and Astronomy, University of Pittsburgh, 2005 Submitted to the Graduate Faculty of the Department of Physics and Astronomy in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Pittsburgh 2009 Andrew J. Mason B.S. Physics, State University of New York

Minnesota, University of

115

Neutrino Astronomy Scott Wilbur  

E-Print Network [OSTI]

V protons, which should be created with neutrinos, have been seen Can be used to observe possible dark Particle Physics Extremely long baseline for neutrino oscillation studies Dark Matter Searches Many dark Detector Picture from AMANDA II Web Site: http://www.amanda.uci.edu #12;Advantages of Neutrino Astronomy

Golwala, Sunil

116

Symposium on atomic spectroscopy (SAS-83): abstracts and program  

SciTech Connect (OSTI)

Abstracts of papers given at the symposium are presented. Session topics include: Rydbergs, optical radiators, and planetary atoms; highly ionized atoms; ultraviolet radiation; theory, ion traps, and laser cooling; beam foil; and astronomy. (GHT)

Not Available

1983-09-01T23:59:59.000Z

117

Abstract crystals Department of Mathematics  

E-Print Network [OSTI]

is a normal crystal define a bijection si : B B by sib = ~f wti(b) i b, if wti(b) 0, ~e -wti(b) i b, if wti, b2 B2} with wti(b1 b2) = wti(b1) + wti(b2), i(b1 b2) = max{i(b1), i(b2) - wt(b1), i }, i(b1 b2

Ram, Arun

118

Astronomy Beat No.32 September 21,2009 Page 1 ASTRONOMY BEAT  

E-Print Network [OSTI]

Astronomy Beat No.32 · September 21,2009 Page 1 ASTRONOMY BEAT ASTRONOMY BEAT Editor's Introduction questions on his web site. Astronomy Beat readers are sure to get such questions from friends and colleagues Institute Senior Scientist www.astrosociety.org The Ask an AstrobiologistWeb Site #12;Astronomy Beat No.32

Long, Nicholas

119

Radio Astronomy Fundamentals I John Simonetti  

E-Print Network [OSTI]

Radio Astronomy Fundamentals I John Simonetti Spring 2012 Radio astronomy provides a very different view of the universe than optical astronomy. Radio astronomers and optical astronomers use astronomy. Radio astronomers talk about sources of radio emission. Cas A is a strong source, for example

Ellingson, Steven W.

120

Cornell Astronomy Saturday November 9, 2013  

E-Print Network [OSTI]

Frontiers of Cornell Astronomy Saturday November 9, 2013 105 Space Sciences Building Cornell University #12;Frontiers of Cornell Astronomy Frontiers of Cornell Astronomy 9:00 am Martha Haynes Welcome 9 Astronomy 3:00 pm Astro Grad Network Liquid nitrogen ice cream party Image Credits: Quasar ULAS: Gemini

Richardson Jr., James E.

Note: This page contains sample records for the topic "astronomy department abstract" 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

Computational Intelligence in Astronomy A Win-Win Situation  

E-Print Network [OSTI]

TT, UK {P.Tino@cs,somak@star.sr}.bham.ac.uk http://www.birmingham.ac.uk Abstract. Large archives of the Virtual Observatory project. In order for such massive heteroge- neous data collections to be of use with deep domain knowledge is crucial. Both fields - Computer Science and Astronomy - can hugely benefit

Tino, Peter

122

Adaptive Optics in Astronomy Jay J. McCarthy  

E-Print Network [OSTI]

Adaptive Optics in Astronomy Jay J. McCarthy NW Computational Intelligence Laboratory Portland State University Abstract ­ The field of adaptive optics (AO) has developed as a means to correct for the phase disturbances of an optical signal by understanding the medium through which it passes. This paper

La Rosa, Andres H.

123

astronomy building capacity: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

SEMINAR Physics Websites Summary: 1 ASTRONOMY 104: UNDERGRADUATE ASTRONOMY SEMINAR SYLLABUS Unique Number 47750 Class Meetings together with fellow astronomy majors, and those...

124

airborne astronomy symposium: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

SEMINAR Physics Websites Summary: 1 ASTRONOMY 104: UNDERGRADUATE ASTRONOMY SEMINAR SYLLABUS Unique Number 47750 Class Meetings together with fellow astronomy majors, and those...

125

astronomy receiver systems: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Astronomy Phscs 228 Stellar and Extragalactic Astronomy Phscs 230 Olsen Jr., Dan R. 77 SCIENCE CHINA Physics, Mechanics & Astronomy Engineering Websites Summary: SCIENCE CHINA...

126

Abstracting Preparation  

E-Print Network [OSTI]

Guidelines & Review Manuscript Preparation Submit Your Manuscript Book Reviews Movies & Videos Contact of Biological and Chemical Sciences. Queen Mary, University of London, Mile End Road, London, UK. Abstract Two motive force for energy conversion, providing for metabolism, for active transport, and for synthesis

Allen, John F.

127

Electronics Lab Department of Physics and Astronomy  

E-Print Network [OSTI]

Hart to better suit the new clientele. It has been modified by Branton Campbell to adjust the labs red LEDs 1 2N3904, npn small-signal transistor 2 2N3906, pnp small-signal transistors 1 IRF3704, power inverter 1 7432, quad OR gate 2 7474, D-type flip-flops 1 74193, up-down counter 1 74154, 4-bit decoder 1

Hart, Gus

128

DEPARTMENT OF PHYSICS & ASTRONOMY DEPARTMENTAL CONFERENCE  

E-Print Network [OSTI]

coincidences between Gamma Ray Bursts and neutrino events detected in the RICE array. 12.15 ­ 12.25 Paul Miller

Hickman, Mark

129

DOUGLAS NATELSON Department of Physics and Astronomy  

E-Print Network [OSTI]

and acoustic measurements. Extended range of thermal conductivity investigations through novel experimental susceptibility; thermal transport measurements at low temperatures using resistive, dielectric, and 3 He melting INTERESTS Nanoscale and disordered materials; coherence and correlations in systems of reduced

130

Page 264 Courses: Astronomy (ASTR) Sonoma State University 2014-2015 Catalog Astronomy (ASTR)  

E-Print Network [OSTI]

Page 264 Courses: Astronomy (ASTR) Sonoma State University 2014-2015 Catalog Astronomy (ASTR) AStr 100 deSCriptiVe AStronoMy (3) Lecture, 3 hours. A survey designed primarily for non-science majors, including an introduction to historic astronomy, Newton's Laws, gravitation, atomic structure, light

Ravikumar, B.

131

STFC Astronomy Advisory Panel Report (October 2012) STFC Astronomy Advisory Panel report (October 2012) 1  

E-Print Network [OSTI]

#12;STFC Astronomy Advisory Panel Report (October 2012) STFC Astronomy Advisory Panel report (October 2012) 1 STFC Astronomy Advisory Panel 2012 Programmatic Review report to PPAN (October 2012) Executive summary This document provides a roadmap for UK astronomy and provides advice for future science

Crowther, Paul

132

E-Print Network 3.0 - abstract optical scattering Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

S. H. Eah, H. W. Kihm, Q. H. Kim, W. S. Bak, Dai... -Sik Kim Center for Subwavelength Optics, Department of Physics and Astronomy, Seoul National ... Source: Park, Namkyoo -...

133

*** TITLE *** Reports on Astronomy 2009-2012  

E-Print Network [OSTI]

*** TITLE *** Reports on Astronomy 2009-2012 ***NAME OF EDITORS*** c 2012 International on HISTORICAL RADIO ASTRONOMY CHAIR Kenneth Kellermann VICE-CHAIR Wayne Orchiston BOARD Rod Davies Leonid TRIENNIAL REPORT 2009-2012 1. Introduction The IAU Working Group on Historical Radio Astronomy (WGHRA

Groppi, Christopher

134

Cardiff School of Physics and Astronomy  

E-Print Network [OSTI]

Cardiff School of Physics and Astronomy Postgraduate Programmes www.astro.cardiff.ac.uk #12;Welcome to the Cardiff School of Physics and Astronomy 1 Director of PG Studies welcome 2 An Introduction to the Cardiff School of Physics and Astronomy 3 Cardiff: The City 4 Cardiff: The University 6 Research Groups 8

Davies, Christopher

135

Cardiff School of Physics and Astronomy  

E-Print Network [OSTI]

Cardiff School of Physics and Astronomy Undergraduate Degree Programmes www.astro.cardiff.ac.uk #12;Cardiff School of Physics and Astronomy SUPPORTIVE ENVIRONMENT FRIENDLY ON SITE FACILITIES TRANSFERABLE and Astronomy at Cardiff 10 Degree Programmes 13 Degree Programme Structures 17 Employability and Careers 20

Davies, Christopher

136

Astronomy 142: Spring 2008 The Evolving Universe  

E-Print Network [OSTI]

Astronomy 142: Spring 2008 The Evolving Universe: Recent Theories and Observations in Modern Astronomy INSTRUCTOR: Diane Friend E-MAIL: diane.friend@umontana.edu PHONE: 243-4299 (Phys./Astr. dept. office: 243-2073) OFFICE: CHCB 129 (inside the Physics/Astronomy dept. office) OFFICE HOURS: M 10-11 & 1

Vonessen, Nikolaus

137

Virtual Observatories A New Era for Astronomy  

E-Print Network [OSTI]

Virtual Observatories A New Era for Astronomy Reinaldo R. de Carvalho DAS-INPE/MCT 2010 Wednesday, April 7, 2010 #12;Virtual Observatories A New Era for Astronomy Reinaldo R. de Carvalho DAS!;#--&$G !!!$ ! ' !"#$%&'&#()*! !!!$#%& !( $ ' !%&$ $ ! (% +#&,&'- .'/0&#,& Wednesday, April 7, 2010 #12;Virtual Observatories A New Era for Astronomy Reinaldo R. de

138

Energy Research Abstracts. [DOE abstract journal  

SciTech Connect (OSTI)

Energy Research Abstracts (ERA) provides abstracting and indexing coverage of all scientific and technical reports, journal articles, conference papers and proceedings, books, patents, theses, and monographs originated by the US Department of Energy, its laboratories, energy centers, and contractors. ERA also covers other energy information prepared in report form by federal and state government organizations, foreign governments, and domestic and foreign universities and research organizations. ERA coverage of non-report literature is limited to that generated by Department of Energy activity. ERA is comprehensive in its subject scope, encompassing the DOE's research, development, demonstration, and technological programs resulting from its broad charter for energy sources, conservation, safety, environmental impacts, and regulation. Corporate, author, subject, report number, and contract number indexes are included. ERA is available on an exchange basis to universities, research intitutions, industrial firms, and publishers of scientific information. Federal, state, and municipal agencies concerned with energy development, conservation, and usage may obtain ERA free of charge. Inquiries should be directed to the Technical Information Center, P.O. Box 62, Oak Ridge, Tennessee 37830. ERA is available to the public on a subscription basis for 24 semimonthly issues including a semiannual index and an annual index. All citations announced in ERA exist as separate records in the DOE Energy Data Base.

Not Available

1981-01-01T23:59:59.000Z

139

SCIENCE CHINA Physics, Mechanics & Astronomy  

E-Print Network [OSTI]

SCIENCE CHINA Physics, Mechanics & Astronomy © Science China Press and Springer-Verlag Berlin for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China. Sci China-Phys Mech Astron, 2013, 56: 207221, doi: 10.1007/s11433-012-4970-8 1 Introduction

Zhang, Guangyu

140

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.

Note: This page contains sample records for the topic "astronomy department abstract" 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

Astronomy and the Fifth Dimension  

E-Print Network [OSTI]

Astronomy is a precise and relatively simple science because objects accelerate in a gravitational field at the same rate, irrespective of their composition. Galileo knew this, and Einstein took it as the basis for general relativity. Surprisingly, it is also a consequence of new theories that use a fifth dimension.

Paul S. Wesson

2013-01-01T23:59:59.000Z

142

Astronomy 4194 Group Studies Essential Radio Astronomy Syllabus for May Term 2014 Prof. Martini Page 1 of 2  

E-Print Network [OSTI]

Astronomy 4194 ­ Group Studies ­ Essential Radio Astronomy ­ Syllabus for May Term 2014 ­ Prof. Martini Page 1 of 2 Astronomy 4194 ­ Group Studies ­ Essential Radio Astronomy Syllabus for May Term 2014. Paul Martini, Dept. of Astronomy Office: 4021 McPherson Lab (4th floor), mailbox in 4055 McPherson Lab

Martini, Paul

143

High-Energy Neutrino Astronomy  

E-Print Network [OSTI]

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their multidisciplinary missions include the search for the particle nature of dark matter and for additional small dimensions of space. In the end, their conceptual design is very much anchored to the observational fact that Nature accelerates protons and photons to energies in excess of $10^{20}$ and $10^{13}$ eV, respectively. The cosmic ray connection sets the scale of cosmic neutrino fluxes. In this context, we discuss the first results of the completed AMANDA detector and the reach of its extension, IceCube. Similar experiments are under construction in the Mediterranean. Neutrino astronomy is also expanding in new directions with efforts to detect air showers, acoustic and radio signals initiated by super-EeV neutrinos.

F. Halzen

2004-02-03T23:59:59.000Z

144

High-Energy Neutrino Astronomy  

E-Print Network [OSTI]

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their multidisciplinary missions include the search for the particle nature of dark matter and for additional small dimensions of space. In the end, their conceptual design is very much anchored to the observational fact that Nature accelerates protons and photons to energies in excess of 10^{20} and 10^{13} eV, respectively. The cosmic ray connection sets the scale of cosmic neutrino fluxes. In this context, we discuss the first results of the completed AMANDA detector and the reach of its extension, IceCube. Similar experiments are under construction in the Mediterranean. Neutrino astronomy is also expanding in new directions with efforts to detect air showers, acoustic and radio signals initiated by neutrinos with energies similar to those of the highest energy cosmic rays.

F. Halzen

2005-01-26T23:59:59.000Z

145

ASTRONOMY BIOLOGY CHEMISTRY COMPUTER-SCIENCE GEOGRAPHY MATHEMATICS PHYSICS STATISTICS  

E-Print Network [OSTI]

ASTRONOMY BIOLOGY CHEMISTRY COMPUTER-SCIENCE GEOGRAPHY MATHEMATICS PHYSICS STATISTICS HEALTHCARE BIOMEDICAL-ENGINEERING ELECTRONIC- ENGINEERING ASTRONOMY BIOLOGY CHEMISTRY COMPUTER-SCIENCE GEOGRAPHY MATHEMATICS PHYSICS STATISTICS HEALTHCARE BIOMEDICAL-ENGINEERING ELECTRONIC-ENGINEERING ASTRONOMY BIOLOGY C H

Bernstein, Phil

146

Introduction Abstract reflection groups and abstract buildings  

E-Print Network [OSTI]

Introduction Abstract reflection groups and abstract buildings Their geometric realizations Compactly supported cohomology L2 -cohomology Cohomology of Coxeter groups and buildings Mike Davis (work groups and buildings #12;Introduction Abstract reflection groups and abstract buildings Their geometric

Vogtmann, Karen

147

Department ofDepartment of Astronomy and AstrophysicsAstronomy and Astrophysics  

E-Print Network [OSTI]

such as supernovae and gamma ray bursts Cosmology: gravitational lensing and dark energy Study of solar and stellar waves Explosive processes such as supernovae and gamma ray bursts Cosmology: gravitational lensing Puravankara A. R. Rao Alak K. Ray K. P. Singh T. P. Singh M. N. Vahia J. S. Yadav Faculty Members Devendra K

Shyamasundar, R.K.

148

Department  

Broader source: Energy.gov (indexed) [DOE]

Department of Energy Washington, DC 20585 MEMORANDUM FOR SCOTT BLAKE HARRIS GENERAL COUNSEL DAVID K. ZAB S Y ACTING PRINCI A EP DIRECTOR OFFICE OF CIV DIOACTIVE WASTE MANAGEMENT...

149

Department  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Nuclear Physics," on May 26-27,2011, in Bethesda, MD (Washington, DC area). This workshop is organized by the Department of Energy's Offices of Nuclear Physics (NP) and Advanced...

150

Department  

Energy Savers [EERE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector General Office of Audit Services Audit Report DepartmentRepresentative Of The Year | Department

151

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA ELECTRONICS DIVISION TECHNICAL NOTE R. Lacasse #12;NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia 140-ft CASSEGRAIN BAa

Groppi, Christopher

152

Astronomy & Astrophysics manuscript no. E1Cfin c ESO 2009 December 14, 2009  

E-Print Network [OSTI]

, Romania 4 University of Bucharest, Department of Physics, Platforma Magurele, Str. Fizicienilor nr. 1, CP Mg - 11, Bucharest-Magurele, 76900, Romania 5 The Romanian Society for Meteors and Astronomy (SARM), T^argovis¬łte, Romania 6 Astronomical Observatory "Admiral Vasile Urseanu", Bd. Lascar Catargiu, nr

Boyer, Edmond

153

Department  

Office of Legacy Management (LM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment ofDepartment ofof EnergyYou$0.C. 20545*. . : '* FEB1 Rev. 0IwellSite:u.s.

154

Xray Astronomy at SSL My personal perspective  

E-Print Network [OSTI]

Xray Astronomy at SSL My personal perspective Mike Lampton 29 August 2009 #12;Astronomical.Lampton 29 Aug 2009 4 The Quest ∑ 50 years SSL; 50 years of Xray astronomy ∑ New questions: what's out there between theory & observation ≠ SSL: observations ≠ Campus: theory ≠ Together: stronger than either would

California at Berkeley, University of

155

Tunable Imaging Filters in Astronomy  

E-Print Network [OSTI]

While tunable filters are a recent development in night time astronomy, they have long been used in other physical sciences, e.g. solar physics, remote sensing and underwater communications. With their ability to tune precisely to a given wavelength using a bandpass optimized for the experiment, tunable filters are already producing some of the deepest narrowband images to date of astrophysical sources. Furthermore, some classes of tunable filters can be used in fast telescope beams and therefore allow for narrowband imaging over angular fields of more than a degree over the sky.

J. Bland-Hawthorn

2000-06-05T23:59:59.000Z

156

Report to Congress on the U.S. Department of Energy`s Environmental Management Science Program: Research funded and its linkages to environmental cleanup problems, and Environmental Management Science Program research award abstracts. Volume 2 of 3 -- Appendix B  

SciTech Connect (OSTI)

The Department of Energy`s Environmental Management Science Program (EMSP) serves as a catalyst for the application of scientific discoveries to the development and deployment of technologies that will lead to reduction of the costs and risks associated with cleaning up the nation`s nuclear complex. Appendix B provides details about each of the 202 research awards funded by the EMSP. This information may prove useful to researchers who are attempting to address the Department`s environmental management challenges in their work, program managers who are planning, integrating, and prioritizing Environmental Management projects, and stakeholders and regulators who are interested in the Department`s environmental challenges. The research award information is organized by the state and institution in which the lead principal investigator is located. In many cases, the lead principal investigator is one of several investigators at a number of different institutions. In these cases, the lead investigator (major collaborator) at each of the additional institutions is listed. Each research award abstract is followed by a list of high cost projects that can potentially be impacted by the research results. High cost projects are Environmental Management projects that have total costs greater than $50 million from the year 2007 and beyond, based on the March 1998 Accelerating Cleanup: Paths to Closure Draft data, and have costs or quantities of material associated with an Environmental Management problem area. High cost projects which must remain active in the year 2007 and beyond to manage high risk are also identified. Descriptions of these potentially related high cost Environmental Management projects can be found in Appendix C. Additional projects in the same problem area as a research award can be located using the Index of High Cost Environmental Management Projects by Problem Area, at the end of Appendices B and C.

NONE

1998-04-01T23:59:59.000Z

157

What can I do with a degree in Astronomy?  

E-Print Network [OSTI]

What can I do with a degree in Astronomy? Science Planning your career Choosing a career involves.canterbury.ac.nz/liaison/best_prep.shtml What is Astronomy? Astronomy and astrophysics are concerned with the study of the nature and revealing observations. As a consequence, astronomy in recent years has been one of the most rapidly

Hickman, Mark

158

Astronomy and Ethics Mark A. Bullock 2/22/05  

E-Print Network [OSTI]

Astronomy and Ethics Mark A. Bullock 2/22/05 Astronomy, from the Greek astron, star, plus nomos, and thus as a challenge to ethics, so subsequent developments in astronomy deprived humans of an order" (Critique of Practical Reason, 288); but the achievements of modern astronomy have left the moral law within

Bullock, Mark A.

159

Transforming Abstract Interpretations by Abstract Interpretation  

E-Print Network [OSTI]

an instance of the same abstract interpretation frame- work lifted to higher types, i.e. where the objectsTransforming Abstract Interpretations by Abstract Interpretation New Challenges in Language - Verona, Italy (roberto.giacobazzi|isabella.mastroeni)@univr.it Abstract. In this paper we exploit

Giacobazzi, Roberto

160

Institute for Astronomy The Royal Observatory Edinburgh comprises the UK Astronomy Technology Centre of the Science and Technology  

E-Print Network [OSTI]

Institute for Astronomy The Royal Observatory Edinburgh comprises the UK Astronomy Technology Centre of the Science and Technology Facilities Council, the Institute for Astronomy of the University of Edinburgh and the ROE Visitor Centre. Undergraduate study at the IfA The Institute for Astronomy (If

Tittley, Eric

Note: This page contains sample records for the topic "astronomy department abstract" 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

E-Print Network 3.0 - angular resolution astronomy Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

astronomy Search Powered by Explorit Topic List Advanced Search Sample search results for: angular resolution astronomy Page: << < 1 2 3 4 5 > >> 1 Astronomy, Lund, 24 February,...

162

Department  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-UpHeat Pump Models | Department1 Prepared1217 Release NotesFinalDemonstration of= Energy

163

Energy Research Abstracts; (USA)  

SciTech Connect (OSTI)

Energy Research Abstracts (ERA) provides abstracting and indexing coverage of all scientific and technical reports and patent applications originated by the US Department of Energy, its laboratories, energy centers, and contractors, as well as theses and conference papers and proceedings issued by these organizations in report form. Audiovisual materials, computer media (magnetic tapes, diskettes, etc.), and engineering drawings are included in this definition. ERA also covers other energy information prepared in report form by federal and state government organizations, foreign governments, and domestic and foreign universities and research organizations, provided that the full text of the document has been received by OSTI. Foreign report information is obtained through the International Energy Agency's fourteen nation Energy Technology Data Exchange, the International Atomic Energy Agency's International Nuclear Information System, or nation-to-nation agreements. The purpose of this publication is to announce documents produced or obtained by DOE that are not so readily available as journal articles, books, or patents. ERA does not cover nonreport literature. The scope of ERA encompasses DOE's research, development, demonstration, and technology programs resulting from its broad charter for energy sources, supplies, safety, environmental impacts, and regulation.

Rutkowski, R.W.; Henline, D.M. (eds.)

1991-01-01T23:59:59.000Z

164

Program of Study Programs of study leading to the degrees of Master of Science, Master of Engineering (Engineering Physics), and Doctor of Philosophy are offered through the Department of Physics and Astronomy.  

E-Print Network [OSTI]

, electrical engineering, biology, chemistry, chemical engineering and Stem Education. Such cooperative rese of Engineering (Engineering Physics), and Doctor of Philosophy are offered through the Department of Physics to courses in physics and such allied fields as other sciences, mathematics, and engineering. However

Thomas, Andrew

165

Physics & Astronomy BSc (Single Honours Degrees)  

E-Print Network [OSTI]

138 Physics & Astronomy BSc (Single Honours Degrees) Astrophysics Physics MPhys (Single Honours Degrees) Astrophysics Physics Theoretical Physics BSc (Joint Honours Degrees) Physics and one of: Computer Science Logic and Philosophy of Science Mathematics MPhys (Joint Honours Degree) Theoretical Physics

Brierley, Andrew

166

Physics and Astronomy Engineering Electronics Concentration  

E-Print Network [OSTI]

Physics and Astronomy Engineering Electronics Concentration Strongly recommended courses Credits PHY 3230 Thermal Physics 2 PHY 4330 Digital Electronics 3 PHY 4635 Advanced Microprocessors Grade PHY 4020 Computational Methods in Physics & Engineering 3 PHY 4620 Optics 4 PHY 4735

Thaxton, Christopher S.

167

The HST contribution to neutron star astronomy  

E-Print Network [OSTI]

While isolated neutron stars (INSs) are among the brightest gamma-ray sources, they are among the faintest ones in the optical, and their study is a challenging task which require the most powerful telescopes. HST has lead neutron star optical astronomy yielding nearly all the identifications achieved since the early 1990s. Here, the major HST contributions in the optical studies of INSs and their relevance for neutron stars' astronomy are reviewed.

R. P. Mignani

2007-10-29T23:59:59.000Z

168

Abstracts - Department of Mathematics, Purdue University  

E-Print Network [OSTI]

May 27, 2007 ... Isoperimetric Inequalities Related to Mass and Energy in General Relativity ... Panagiota Daskalopoulos, Columbia University, New York, NY.

2007-05-18T23:59:59.000Z

169

Abstracts - Department of Mathematics, Purdue University  

E-Print Network [OSTI]

We investigate variational problems for an energy developed by the physicists Chen and ... I plan to present the main steps .... sciences domain. At least two†...

2009-05-25T23:59:59.000Z

170

Abstracts - Department of Mathematics, Purdue University  

E-Print Network [OSTI]

Apr 13, 2013 ... Stability and Approximation Results for Biomechanical Imaging ... We consider the scattering of a time-harmonic plane wave incident on a two†...

171

Call for Abstracts | Department of Energy  

Broader source: Energy.gov (indexed) [DOE]

Management Team Environmental Justice Environmental Management System Applied Studies and Technology Post-Closure Benefits Property Records Management Stakeholder Relations...

172

Abstract - Department of Mathematics, Purdue University  

E-Print Network [OSTI]

This work presents the numerical modeling of water flow in randomly heterogeneous ... finite element method for the spatial discretization combined with a backward Euler ... terize groundwater flow in highly heterogeneous soils and analyze the ... Introduction ..... may be regarded as a cell-centered finite difference scheme.

1910-20-30T23:59:59.000Z

173

Gravitational wave astronomy - astronomy of the 21st century  

E-Print Network [OSTI]

An enigmatic prediction of Einstein's general theory of relativity is gravitational waves. With the observed decay in the orbit of the Hulse-Taylor binary pulsar agreeing within a fraction of a percent with the theoretically computed decay from Einstein's theory, the existence of gravitational waves was firmly established. Currently there is a worldwide effort to detect gravitational waves with interferometric gravitational wave observatories or detectors and several such detectors have been built or being built. The initial detectors have reached their design sensitivities and now the effort is on to construct advanced detectors which are expected to detect gravitational waves from astrophysical sources. The era of gravitational wave astronomy has arrived. This article describes the worldwide effort which includes the effort on the Indian front - the IndIGO project -, the principle underlying interferometric detectors both on ground and in space, the principal noise sources that plague such detectors, the astrophysical sources of gravitational waves that one expects to detect by these detectors and some glimpse of the data analysis methods involved in extracting the very weak gravitational wave signals from detector noise.

S. V. Dhurandhar

2011-04-15T23:59:59.000Z

174

AbstractAbstract Improving efficiency of thermoelectric  

E-Print Network [OSTI]

-classical transport models used to predict ZT can effectively predict thermoelectric performance of bulk materials Material PerformanceThermoelectric Material Performance 0 0.5 1 1.5 2 2.5 3 1950 1960 1970 1980 1990 2000AbstractAbstract · Improving efficiency of thermoelectric energy conversion devices is a major

Walker, D. Greg

175

Statistical Abstract 2013  

E-Print Network [OSTI]

Kansas Statistical Abstract 2013 published exclusively online by Institute for Policy & Social,chapters,or the full Kansas Statistical Abstract are permitted on the condition that sources are cited. Kansas Statistical Abstract 2013 2 #12;Table of Contents Foreword

176

Department of Mechanical Engineering "Heat Under the Microscope  

E-Print Network [OSTI]

applications ranging from thermoelectric waste heat recovery to radio astronomy. BIOGRAPHY Austin MinnichDepartment of Mechanical Engineering presents "Heat Under the Microscope: Uncovering an essential role in nearly every technological application, ranging from space power generation to consumer

Militzer, Burkhard

177

ASTRONOMY 2895 TOPICS IN ASTROPHYSICS Autumn Semester 2012  

E-Print Network [OSTI]

ASTRONOMY 2895 ­ TOPICS IN ASTROPHYSICS SYLLABUS Autumn Semester 2012 Course coordinator: Professor Bradley Peterson Office: 4055 McPherson Laboratory, 292-2022 E-mail: peterson@astronomy.ohio-state.edu Webpage URL: http://www.astronomy.ohio-state.edu/~peterson/Ast2895/ Classroom: 3094 Smith Laboratory Class

Peterson, Bradley M.

178

Astronomy in room 309 with Professor David Cohen  

E-Print Network [OSTI]

Astronomy in room 309 with Professor David Cohen March 1, 2006 The Moon You can see the moon up these out on your computer, with your parents - Information and pictures about the moon and astronomy: http://www.calculatorcat.com/moon_phases/moon_phases.phtml http://antwrp.gsfc.nasa.gov/apod/astropix.html (Astronomy Picture of the Day ­ check out their "search

Cohen, David

179

Curriculum Vitae Casey J. Law Radio Astronomy Lab  

E-Print Network [OSTI]

Curriculum Vitae ­ Casey J. Law Radio Astronomy Lab University of California Hearst Field Annex ­ B://astro.berkeley.edu/claw 1 Education Northwestern University, Ph.D., Astrophysics (2007) Boston University, M.A., Astronomy: Radio Astronomy Lab Postdoctoral Fellow at UC Berkeley. Worked with Geoff Bower, Don Backer, and Carl

Militzer, Burkhard

180

PART 1: Astronomy and Society Monday, 10 June 2013  

E-Print Network [OSTI]

PART 1: Astronomy and Society Monday, 10 June 2013 09h00 Registration 09h30 10' Welcome Session 1 and their importance for astronomy Ron Ekers 11h00 Tea/coffee Break Session 2: Why should society fund big science projects and big astronomy projects in particular? 11h30 30' The benefits of basic research in general

Galis, Frietson

Note: This page contains sample records for the topic "astronomy department abstract" 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

GEM 1506 HEAVENLY MATHEMATICS: HIGHLIGHTS OF CULTURAL ASTRONOMY  

E-Print Network [OSTI]

GEM 1506 ­ HEAVENLY MATHEMATICS: HIGHLIGHTS OF CULTURAL ASTRONOMY TERM PROJECT THE NEW YEAR AND THE AUSPICIOUS HOURS......17 3.1 TERMS USED IN THE ASTRONOMY OF SRI LANKA signs (though, in reality the sun does not move). With a rich history behind the astronomy of Sri Lanka

Aslaksen, Helmer

182

Astronomy and its Role in Vedic Culture Subhash Kak  

E-Print Network [OSTI]

Astronomy and its Role in Vedic Culture Subhash Kak Louisiana State University Baton Rouge, LA, Part 1, edited by G.C. Pande, ICPR/Munshiram Manoharlal, Delhi, 2000, pp. 507-524. That astronomy to the calendar. Vedic astronomy was not based on the use of accurate clocks, but fine time units were defined

Koppelman, David M.

183

INTRA Programme B.Sc. Physics with Astronomy  

E-Print Network [OSTI]

INTRA Programme B.Sc. Physics with Astronomy The Objective of this four-year, full-time degree with a physics degree and associated skills in IT and mathematics, combined with a good background in astronomy and astrophysics as a specialisation (i.e. a physics "major", astronomy "minor"). The courses taught within

Humphrys, Mark

184

UNIVERSITY OF ST ANDREWS SCHOOL OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

UNIVERSITY OF ST ANDREWS SCHOOL OF PHYSICS AND ASTRONOMY Guidance notes for potential exchange and study abroad students The School of Physics and Astronomy is pleased to welcome exchange and study to the nature of the module it is not permitted to take this introductory module as well as any other astronomy

Greenaway, Alan

185

The University of Manchester School of Physics and Astronomy  

E-Print Network [OSTI]

The University of Manchester School of Physics and Astronomy www. The University of Manchester was my first choice because I knew it is at the forefront of astronomy research to help international students settle in. The School of Physics and Astronomy provided me with a mentor

186

Transactions IAU, Volume XXVIIIA Reports on Astronomy 2009-2012  

E-Print Network [OSTI]

Transactions IAU, Volume XXVIIIA Reports on Astronomy 2009-2012 Ian Corbett, ed. c 2012 GROUP ON HISTORICAL RADIO ASTRONOMY CHAIR Kenneth Kellermann VICE-CHAIR Wayne Orchiston BOARD Rod Davies Woerden TRIENNIAL REPORT 2009-2012 1. Introduction The IAU Working Group on Historical Radio Astronomy

Groppi, Christopher

187

National Radio Astronomy Observatory Electronics Division Technical Note No. 219  

E-Print Network [OSTI]

1 National Radio Astronomy Observatory Electronics Division Technical Note No. 219 Measurements of Automotive Radar Emissions received by a Radio Astronomy Observatory Darrel Emerson (National Radio Astronomy (Continental Corporation, A.D.C. Automotive Distance Control Systems GmbH, Germany), Juergen

Groppi, Christopher

188

Computer Models in Astronomy and Statistics Stellar Evolution  

E-Print Network [OSTI]

Computer Models in Astronomy and Statistics Stellar Evolution Calibration of X-ray Detectors Embedding Astronomical Computer Models into Complex Statistical Models David A. van Dyk Statistics Section Dyk Complex Analyses with Computer Models in Astronomy #12;Computer Models in Astronomy and Statistics

van Dyk, David

189

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK ) WEST VIRGINIA  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK ) WEST VIRGINIA ELECTRONICS DIVISION INTERNAL REPORT No. 159 INTERFERENCE POTENTIAL FOR RADIO ASTRONOMY OBSERVATIONS AT GREEN BANK, WEST VIRGINIA CRAIG ASTRONOMY OBSERVATIONS AT GREEN BANK, WEST VIRGINIA Craig R. Moore and James L. Dolan Introduction

Groppi, Christopher

190

From Modern Astronomy to Modern Finance: A New Theory 6.1. What Finance and Astronomy Have in Common?  

E-Print Network [OSTI]

Chapter 6 From Modern Astronomy to Modern Finance: A New Theory of Finance 6.1. What Finance and Astronomy Have in Common? Some theories, originated from a very technical area, because of their deep insight and analytical power, become the foundation of much broader fields. Modern astronomy, founded

Bolch, Tobias

191

abstract.tex  

E-Print Network [OSTI]

Seismic response of fractures and induced anisotropy in poroelastic media Juan E. Santos Department of Mathematics, Purdue University and Instituto del Gas y†...

192

Patricia Burchat Department of Physics  

E-Print Network [OSTI]

Patricia Burchat Department of Physics Stanford University Dark Matter, Dark Energy: Mysteries University Dark Matter, Dark Energy: Mysteries of the Universe Dark Energy 70% Dark Matter 26% Ordinary://janus.astro.umd.edu/javadir/orbits/ssv.html Planetary Motion Credit: The Astronomy Workshop A collection of interactive web-based programs

Osheroff, Douglas D.

193

VFITRG.SCH PhysicsAstronomy  

E-Print Network [OSTI]

: TRIGGER DELAY AND VETO Seattle, WA 98195­1560 University of Washington B208 Physics­Astronomy Bldg. Super 8 4 6 8 4 7 8 4 3 8 4 2 8 4 1 ... 5 1 5 0 4 9 4 8 4 7 4 6 4 5 supply bypass capacitors: 4 4 4 2 4 3

Berns, Hans-Gerd

194

NATIONAL RADIO ASTRONOMY OBSERVATORY CHARLOTTESVILLE) VA  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY CHARLOTTESVILLE) VA ELECTRONICS DIVISION INTERNAL REPORT No ' : : lg Measurement Programs DETECTO R1 . · · · · .· · · . · · · · · · · NOISEL3.B. . 9· · . · · · · · · · · . . . Automated ' : : lg Measurement Programs DETECTO R1

Groppi, Christopher

195

Lectures on Neutrino Astronomy: Theory and Experiment  

E-Print Network [OSTI]

1. Overview of neutrino astronomy: multidisciplinary science. 2. Cosmic accelerators: the highest energy cosmic rays. 3. Neutrino beam dumps: supermassive black holes and gamma ray bursts. 4. Neutrino telescopes: water and ice. 5. Indirect dark matter detection. 6. Towards kilometer-scale detectors.

F. Halzen

1998-10-22T23:59:59.000Z

196

Fly Through the Universe: Bring Real Astronomy  

E-Print Network [OSTI]

1998) Also: radiation (0.01%) Visible Matter (stars 0.4%, gas 3.6%) 5 #12;Sloan Digital Sky Survey #12;SDSS Data in Your Class · This is real, modern astronomy data ­ Exactly the same data pros get · Not cleaned up for students ­ "true to nature" · No "right answer" · No limit to topics students can

Collar, Juan I.

197

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.

198

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.

199

Physics and Astronomy Chair: Professor M. Vineyard  

E-Print Network [OSTI]

Physics and Astronomy Chair: Professor M. Vineyard Faculty: Professors S. Maleki, J. Newman, G for the Physics Major: Ten courses in physics (Physics 120, 121, 122, 123, 220, 230, 270, 300, 310, and 490 or 493 to gain an appreciation for current research in physics and related areas. For those students wishing

Koopmann, Rebecca A.

200

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.

Note: This page contains sample records for the topic "astronomy department abstract" 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

Mathematics and explanation in astronomy and astrophysics  

E-Print Network [OSTI]

The purpose of this paper is to expound and clarify the mathematics and explanations commonly employed in certain notable areas of astronomy and astrophysics. The first section concentrates upon the mathematics employed to represent and understand stellar structure and evolution. The second section analyses two different explanations for the structure of spiral galaxies.

Gordon McCabe

2007-02-16T23:59:59.000Z

202

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

203

Rutgers University Department of Physics and Astronomy Physics 110: Astronomy & Cosmology  

E-Print Network [OSTI]

: Fundamentals, 1st edition Authors: Bennett, Donohue, Schneider & Voit ISBN: 978-0321567048 Paperback COURSE WEB 13 9 8/6 (T) · Dark Matter & Dark Energy · Q7 14 10 8/8 (R) · Dark Matter & Dark Energy, con

Glashausser, Charles

204

Astronomy 111, Fall 2014 13 November 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 111, Fall 2014 13 November 2014 (c) University of Rochester 1 13 November 2014 Astronomy 111, Fall 2014 1 Astronomy 111 Lecture #20: rings and orbits qPerturbations and resonances q.7 (Tides), 13 (rings) Philae lander on Comet 67P 13 November 2014 Astronomy 111, Fall 2014 2 #12;Astronomy

Mamajek, Eric E.

205

BEMS: Abstract book  

SciTech Connect (OSTI)

This volume provides abstracts of presentations made at the Sixteenth Meeting of The Bioelectromagnetics Society held June 12-17, 1994 in Copenhagen, Denmark.

NONE

1995-06-01T23:59:59.000Z

206

TATA INSTITUTE OF FUNDAMENTAL RESEARCH DEPARTMENT OF ASTRONOMY & ASTROPHYSICS  

E-Print Network [OSTI]

-up projects in order to detect more of these massive YSOs which gives constraints about star formation rates models. Due to the rising of deep infrared data, much progress has been obtained during the last five of the inner few 2 square degrees of our Galaxy and will focus especially on the study of AGB stars using

Udgaonkar, Jayant B.

207

Iowa State University Department of Physics and Astronomy  

E-Print Network [OSTI]

projects under the NSF funded REU program. Appleton continued his term as AURA member represen- tative, which should have greater wave- length and readout efficiency. ISU's International Institute

208

Curriculum Vitae: Michael Riley Brown Department of Physics and Astronomy  

E-Print Network [OSTI]

- ids; dynamos; self-organization in turbulent systems; magnetic confinement fusion (spheromak and field of a spheromak accelerator for the purposes of tokamak refueling and current drive on the ENCORE tokamak for spheromak research. (6/87-5/89) Fellowship at Dartmouth College to study compressible MHD turbulence theory

Brown, Michael R.

209

Curriculum Vitae: Michael Riley Brown Department of Physics and Astronomy  

E-Print Network [OSTI]

; dy- namos; self-organization in turbulent systems; magnetic confinement fusion (spheromak and field. Bellan. Work included the design, construction and operation of a spheromak accelerator for the purposes voltage (10 kV), high current (100 kA), rapidly switched discharges for spheromak research. (6

Brown, Michael R.

210

MARK WHITTLE CURRICULUM VITAE ADDRESS : Department of Astronomy,  

E-Print Network [OSTI]

, Charlottesville, VA 22903, U.S.A. Tel. (434) 924 4900. e-mail : dmw8f@virginia.edu BORN : March 30, 1956

Whittle, Mark

211

Nature's Design Mark Whittle, Astronomy Department, University of Virginia  

E-Print Network [OSTI]

Brief History of Matter" which you can find on my web page at http://www.astro.virginia.edu/dmw8f under

Whittle, Mark

212

Ph.D. QUALIFYING EXAMINATION DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

, m = (j + m)(j - m + 1) |j, m - 1 . #12;2. (10 points): Calculate the efficiency of the Diesel cycle is the electric field inside the block? (6 pts.) (b) What is the electric charge density in the volume

Baskaran, Mark

213

Department of Physics & Astronomy Experimental Particle Physics Group  

E-Print Network [OSTI]

that the degradation of Si over the lifetime of a detector may be quite signi#12;cant [1]. Even with the use of defect material has increased, so research into applications has advanced. Presently the material is used in UV is due to surface changes, shown by the degradation i

Glasgow, University of

214

Department of Physics & Astronomy Experimental Particle Physics Group  

E-Print Network [OSTI]

in the future ATLAS experiment at the LHC imposes severe demands on the radiation hardness of the GaAs detectors were performed at the ISIS facility [2] for the neutron exposure, with a spectrum strongly peaked at 1 of the ATLAS semiconductor tracker. 3 Reverse Current The effect of all three types of irradiation

Glasgow, University of

215

Department of Physics & Astronomy Experimental Particle Physics Group  

E-Print Network [OSTI]

V pion and muon CERN SPS testbeam before irradition in the autumn of 2002 and post-irradiation in summer

Glasgow, University of

216

UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS  

E-Print Network [OSTI]

; demonstrated record of research. PREFERRED QUALIFICATIONS: Postdoctoral experience, potential to obtain

California at Santa Cruz, University of

217

Dan Martin Watson Department of Physics and Astronomy  

E-Print Network [OSTI]

panel. 2008, 2011, 2013 NASA: Research Opportunities in Space and Earth Science: Origins of Solar Postoctoral Fellowship Program review panel. 2012 NSF: Experimental Program to Stimulate Competitive Research review panel 2009-2011 National Academy of Sciences (NAS)/National Research Council (NRC) 2010 Decadal

218

DEPARTMENT OF PHYSICS AND ASTRONOMY GEORGE W. CRABTREE  

E-Print Network [OSTI]

economic, social and political future. The uncertainty of imported oil threatens global energy security security, environment or climate requires finding alternative sources of energy that are clean, abundant

Baskaran, Mark

219

George Hadjipanayis, Chairman, Department of Physics and Astronomy,  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-UpHeatMulti-Dimensional Subject: Guidance for naturalGeneralEnergy GeologicMexico

220

Nature's Design Mark Whittle, Astronomy Department, University of Virginia  

E-Print Network [OSTI]

, as opposed to energy? Again, if you have not heard of it, look up ''dark energy'' on the web. From (1) and (2 Brief History of Matter'' which you can find on my web page at http://www.astro.virginia.edu/#dmw8f is basically atomic (protons/neutrons/electons)? If you have not heard of it, look up ''dark matter

Whittle, Mark

Note: This page contains sample records for the topic "astronomy department abstract" 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

faculty of engineering and physical sciences School of Physics and Astronomy  

E-Print Network [OSTI]

faculty of engineering and physical sciences School of Physics and Astronomy Postgraduate Project....................................................................................................................................................2 Astronomy and Astrophysics available in the School of Physics & Astronomy from September 2013. The list of projects is by no means

222

STFC Astronomy Advisory Panel Draft 2012 Programmatic Review report to PPAN (October 2012)  

E-Print Network [OSTI]

#12;STFC Astronomy Advisory Panel Draft 2012 Programmatic Review report to PPAN (October 2012) Astronomy Advisory Panel: Richard Bower (Durham University), Michael Brown (University of Manchester), Anthony Challinor (University of Cambridge), Chris Evans (STFC United Kingdom Astronomy Technology Centre

Crowther, Paul

223

E-Print Network 3.0 - astronomy including observations Sample...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

142: fusion Summary: 2 February 2010 Astronomy 142, Spring 2010 1 Today in Astronomy 142: fusion Nuclear fusion... photo.) 12;2 February 2010 Astronomy 142, Spring 2010 2 The...

224

Astronomie, ťcologie et poťsie par Hubert Reeves  

ScienceCinema (OSTI)

Hubert ReevesL'astrophysicien donne une confťrence puis s'entretient avec l'ťcrivain FranÁois Bon autour de :"Astronomie, ťcologie et poťsie"Pour plus d'informations :†http://outreach.web.cern.ch/outreach/FR/evenements/conferences.htmlNombre de places limitť. Rťservation obligatoire ŗ la Rťception du CERN†: +41 22 767 76 76 †Soirťe diffusťe en direct sur le Web : http://webcast.cern.ch/††††††

None

2011-10-06T23:59:59.000Z

225

Testing Modified Gravity with Gravitational Wave Astronomy  

E-Print Network [OSTI]

The emergent area of gravitational wave astronomy promises to provide revolutionary discoveries in the areas of astrophysics, cosmology, and fundamental physics. One of the most exciting possibilities is to use gravitational-wave observations to test alternative theories of gravity. In this contribution we describe how to use observations of extreme-mass-ratio inspirals by the future Laser Interferometer Space Antenna to test a particular class of theories: Chern-Simons modified gravity.

Carlos F. Sopuerta; Nicolas Yunes

2010-10-01T23:59:59.000Z

226

Computer Abstractions and Technology  

E-Print Network [OSTI]

& wheel Supersedes roller-ball mechanical mouse #12;Chapter 1 -- Computer Abstractions and Technology to building sized Embedded computers Hidden as components of systems Stringent power of machine instructions executed per operation Processor and memory system Determine how fast instructions

Huang, Chun-Hsi

227

astronomy conference held: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

and cons of Globalization of scientific research. Communities like Astronomy, High Energy Physics and Statistics develop ideas separately, but also have frequent interaction....

228

Abstracts of contributed papers  

SciTech Connect (OSTI)

This volume contains 571 abstracts of contributed papers to be presented during the Twelfth US National Congress of Applied Mechanics. Abstracts are arranged in the order in which they fall in the program -- the main sessions are listed chronologically in the Table of Contents. The Author Index is in alphabetical order and lists each paper number (matching the schedule in the Final Program) with its corresponding page number in the book.

Not Available

1994-08-01T23:59:59.000Z

229

E-Print Network 3.0 - asteroid radar astronomy Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

radar astronomy Search Powered by Explorit Topic List Advanced Search Sample search results for: asteroid radar astronomy Page: << < 1 2 3 4 5 > >> 1 The Mechanics of Moving...

230

RESEARCH & DEVELOPMENT: PROGRAM ABSTRACTS  

E-Print Network [OSTI]

) 586-8061 Fax: (202) 586-9811 E-mail: patrick.davis@ee.doe.gov Fuel Cell Core Technology R&D JoAnn Milliken (202) 586-2480 Fax: (202) 586-9811 E-mail: joann.milliken@ee.doe.gov Fuel Cell System Development Donna Ho (202) 586-8000 Fax: (202) 586-9811 E-mail: donna.ho@ee.doe.gov Mailing Address U.S. Department

231

FROM THE BLOGOSPHERE Abstractions  

E-Print Network [OSTI]

.com/nautilus and see Peer-to-Peer for news for peer-reviewers and about peer review http://blogs.nature in semi- natural field conditions over 3 years was a lot of work. I was worried something might go wrongFROM THE BLOGOSPHERE Abstractions Visit Nautilus for regular news relevant to Nature authors http://blogs.nature

Wu, Zhigang

232

Programme, Abstracts, Presentations & Proceedings  

E-Print Network [OSTI]

Programme, Abstracts, Presentations & Proceedings 24th IAEA Fusion Energy Conference October 8. #12;QR Codes for Smartphone Conference App Scan relevant QR to download the conference app QR code for Android QR code for iPhone The Conference4me application provides a digital, mobile copy of the confer

233

Physics & Astronomy Open House Schedule UH Manoa Watanabe Hall  

E-Print Network [OSTI]

Physics & Astronomy Open House Schedule UH Manoa Watanabe Hall 22 November 2014 0830 - 1245 *** Physics & Astronomy info. available at www.phys.hawaii.edu *** Welcome & Overview: Prof. Pui Lam in Physical Science 217 at 0830 ** schedules for groups 1 to 10 below for 0900-1100 ** **solar observing

234

Physics and Astronomy The Wiess School of Natural Sciences  

E-Print Network [OSTI]

209 Physics and Astronomy The Wiess School of Natural Sciences Chair F. Barry Dunning Professors / Physics and Astronomy All physics majors must complete the following courses: PHYS 101 or 111 Mechanics Modern Physics PHYS 231 Elementary Physics Laboratory II PHYS 301 Intermediate Mechanics MATH 101

Richards-Kortum, Rebecca

235

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA ELECTRONICS DIVISION INTERNAL REPORT and Ionospheric Center, Arecibo, Puerto Rico by the National Radio Astronomy Observatory at Green Bank, West Virginia. The general design concept was taken from previous receivers assembled at NRAO. S. Weinreb and N

Groppi, Christopher

236

NATIONAL RADIO ASTRONOMY OBSERVATORY Green, Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green, Bank, West Virginia Electronics Division Internal Rep preformed by the Standard Receiver Section of the National Radio Astronomy Observatory at Green Bank, West Virginia. The following breakdown was used to divide the costs into various categories: (1) Emckajs.c1 . 1

Groppi, Christopher

237

Astronomy 241: Foundations of Astrophysics I. The Solar System  

E-Print Network [OSTI]

· Over 99.9% of solar system's mass · Largely H and He · Self-regulating nuclear furnace Tuesday, AugustAstronomy 241: Foundations of Astrophysics I. The Solar System Astronomy 241 is the first part the structure and evolution of the Solar System. Prerequisites: Physics 170, Physics 272 (or concurrent

Barnes, Joshua Edward

238

E-Print Network 3.0 - abstract orthographic codes Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

that the patient must have accessed abstract orthographic codes in order to perform the task, what he called... to construct abstract ... Source: Bowers, Jeff - Department of...

239

Astronomy with ultra high-energy particles  

E-Print Network [OSTI]

Recent measurements of the properties of cosmic rays above 10^17 eV are summarized and implications on our contemporary understanding of their origin are discussed. Cosmic rays with energies exceeding 10^20 eV have been measured, they are the highest-energy particles in the Universe. Particles at highest energies are expected to be only marginally deflected by magnetic fields and they should point towards their sources on the sky. Recent results of the Pierre Auger Observatory have opened a new window to the Universe - astronomy with ultra high-energy particles.

Joerg R. Hoerandel

2008-03-20T23:59:59.000Z

240

A versatile integral in physics and astronomy  

E-Print Network [OSTI]

This paper deals with a general class of integrals, the particular cases of which are connected to outstanding problems in astronomy and physics. Reaction rate probability integrals in the theory of nuclear reaction rates, Kr\\"atzel integrals in applied analysis, inverse Gaussian distribution, generalized type-1, type-2 and gamma families of distributions in statistical distribution theory, Tsallis statistics and Beck-Cohen superstatistics in statistical mechanics and the general pathway model are all shown to be connected to the integral under consideration. Representations of the integral in terms of generalized special functions such as Meijer's G-function and Fox's H-function are also pointed out.

A. M. Mathai; H. J. Haubold

2011-09-23T23:59:59.000Z

Note: This page contains sample records for the topic "astronomy department abstract" 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

Interchanging Interactive 3-d Graphics for Astronomy  

E-Print Network [OSTI]

We demonstrate how interactive, three-dimensional (3-d) scientific visualizations can be efficiently interchanged between a variety of mediums. Through the use of an appropriate interchange format, and a unified interaction interface, we minimize the effort to produce visualizations appropriate for undertaking knowledge discovery at the astronomer's desktop, as part of conference presentations, in digital publications or as Web content. We use examples from cosmological visualization to address some of the issues of interchange, and to describe our approach to adapting S2PLOT desktop visualizations to the Web. Supporting demonstrations are available at http://astronomy.swin.edu.au/s2plot/interchange/

C. J. Fluke; D. G. Barnes; N. T. Jones

2008-12-09T23:59:59.000Z

242

EBS Radionuclide Transport Abstraction  

SciTech Connect (OSTI)

The purpose of this report is to develop and analyze the engineered barrier system (EBS) radionuclide transport abstraction model, consistent with Level I and Level II model validation, as identified in Technical Work Plan for: Near-Field Environment and Transport: Engineered Barrier System: Radionuclide Transport Abstraction Model Report Integration (BSC 2005 [DIRS 173617]). The EBS radionuclide transport abstraction (or EBS RT Abstraction) is the conceptual model used in the total system performance assessment (TSPA) to determine the rate of radionuclide releases from the EBS to the unsaturated zone (UZ). The EBS RT Abstraction conceptual model consists of two main components: a flow model and a transport model. Both models are developed mathematically from first principles in order to show explicitly what assumptions, simplifications, and approximations are incorporated into the models used in the TSPA. The flow model defines the pathways for water flow in the EBS and specifies how the flow rate is computed in each pathway. Input to this model includes the seepage flux into a drift. The seepage flux is potentially split by the drip shield, with some (or all) of the flux being diverted by the drip shield and some passing through breaches in the drip shield that might result from corrosion or seismic damage. The flux through drip shield breaches is potentially split by the waste package, with some (or all) of the flux being diverted by the waste package and some passing through waste package breaches that might result from corrosion or seismic damage. Neither the drip shield nor the waste package survives an igneous intrusion, so the flux splitting submodel is not used in the igneous scenario class. The flow model is validated in an independent model validation technical review. The drip shield and waste package flux splitting algorithms are developed and validated using experimental data. The transport model considers advective transport and diffusive transport from a breached waste package. Advective transport occurs when radionuclides that are dissolved or sorbed onto colloids (or both) are carried from the waste package by the portion of the seepage flux that passes through waste package breaches. Diffusive transport occurs as a result of a gradient in radionuclide concentration and may take place while advective transport is also occurring, as well as when no advective transport is occurring. Diffusive transport is addressed in detail because it is the sole means of transport when there is no flow through a waste package, which may dominate during the regulatory compliance period in the nominal and seismic scenarios. The advective transport rate, when it occurs, is generally greater than the diffusive transport rate. Colloid-facilitated advective and diffusive transport is also modeled and is presented in detail in Appendix B of this report.

J. Prouty

2006-07-14T23:59:59.000Z

243

Astronomy 142, Spring 2013 26 February 2013 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 142, Spring 2013 26 February 2013 (c) University of Rochester 1 25 February 2014 Astronomy 142, Spring 2014 1 Today in Astronomy 142: interstellar dust Extinction, reddening Mellinger, Central Michigan U.) 25 February 2014 Astronomy 142, Spring 2014 2 How do we know

Mamajek, Eric E.

244

Astronomy 161 Syllabus for Winter Quarter 2010 Prof. Martini Page 1 of 4  

E-Print Network [OSTI]

Astronomy 161 ­ Syllabus for Winter Quarter 2010 ­ Prof. Martini Page 1 of 4 Astronomy 161 ­ Introduction to Solar System Astronomy Syllabus for Winter Quarter 2010 MTWRF, 9:30-10:18am, 1184 Postle Hall Prof. Paul Martini Course Objectives Astronomy 161 fulfills the physical science requirement

Martini, Paul

245

Figure 1: ATA 42 antenna array at Hat Creek ********ADAPTIVE REAL TIME IMAGING FOR RADIO ASTRONOMY*******  

E-Print Network [OSTI]

Figure 1: ATA 42 antenna array at Hat Creek ********ADAPTIVE REAL TIME IMAGING FOR RADIO ASTRONOMY --------------------------¬≠ ¬∑ Astronomers primarily interested in astronomy. ¬≠ Data reduction preoccupies radio astronomy specialists,f,p Bandpass( )f PolCal( )f,p Gains( )s,f,p S Beam Imager Astronomy Solver I2 ( ) )^(^, 2sVpfV - √• ¬Ļkj X Solver

Militzer, Burkhard

246

Astronomy 142, Spring 2014 27 February 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 142, Spring 2014 27 February 2014 (c) University of Rochester 1 27 February 2014 Astronomy 142, Spring 2014 1 Today in Astronomy 142: interstellar gas The Orion Nebula (M42 and NGC 1977 go along. TI Chelsea Jean will have a practice session (TBD) 27 February 2014 Astronomy 142, Spring

Mamajek, Eric E.

247

Astronomy 142, Spring 2014 30 January 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 142, Spring 2014 30 January 2014 (c) University of Rochester 1 30 January 2014 Astronomy 142, Spring 2014 1 Today in Astronomy 142: the Sun The structure of the Sun's outer layers: convection-rich active regions (TRACE/NASA). 30 January 2014 Astronomy 142, Spring 2014 2 The Sun's convection zone

Mamajek, Eric E.

248

Astronomy 111, Fall 2014 30 October 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 111, Fall 2014 30 October 2014 (c) University of Rochester 1 30 October 2014 Astronomy 111, Fall 2014 1 Astronomy 111 Lecture #16: planetary atmospheres qVertical density and pressure scattered by its upper atmosphere and rings (Galileo/ JPL/NASA) 30 October 2014 Astronomy 111, Fall 2014 2

Mamajek, Eric E.

249

Astronomy 142, Spring 2014 20 February 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 142, Spring 2014 20 February 2014 (c) University of Rochester 1 Today in Astronomy 142 evolution: the Hertzsprung-Russell diagrams of open and globular stellar clusters 20 February 2014 Astronomy February 2014 Astronomy 142, Spring 2014 2 Late stages of stellar evolution After the maximum mass fraction

Mamajek, Eric E.

250

Astronomy 142, Spring 2014 13 February 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 142, Spring 2014 13 February 2014 (c) University of Rochester 1 13 February 2014 Astronomy 142, Spring 2014 1 Today in Astronomy 142: stellar-mass black holes Figure: artist's conception (will not be accepted late) 13 February 2014 Astronomy 142, Spring 2014 2 Escape velocities from stars

Mamajek, Eric E.

251

Astronomy 111, Fall 2014 11 November 2014 (c) University of Rochester 1  

E-Print Network [OSTI]

Astronomy 111, Fall 2014 11 November 2014 (c) University of Rochester 1 11 November 2014 Astronomy, Australia, Aug 2009) 11 November 2014 Astronomy 111, Fall 2014 2 Jupiter's rings Discovered in 1979 be seen above and below the main ring, about a factor of ten fainter. #12;Astronomy 111, Fall 2014 11

Mamajek, Eric E.

252

Astronomy 161 Syllabus for Winter Quarter 2010 Prof. Martini Page 1 of 4  

E-Print Network [OSTI]

Astronomy 161 ­ Syllabus for Winter Quarter 2010 ­ Prof. Martini Page 1 of 4 Astronomy 161 ­ Introduction to Solar System Astronomy Syllabus for Winter Quarter 2010 MTWRF, 11:30am-12:18pm, 100 Stillman Hall Prof. Paul Martini Course Objectives Astronomy 161 fulfills the physical science requirement

Martini, Paul

253

ABSTRACTS OF PAPERS PUBLISHED  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary)morphinanInformation Desert SouthwestTechnologies |November 2011A FirstEMSLAEMSL341AACEii ABSTRACT This4 -

254

EBS Radionuclide Transport Abstraction  

SciTech Connect (OSTI)

The purpose of this report is to develop and analyze the engineered barrier system (EBS) radionuclide transport abstraction model, consistent with Level I and Level II model validation, as identified in ''Technical Work Plan for: Near-Field Environment and Transport: Engineered Barrier System: Radionuclide Transport Abstraction Model Report Integration'' (BSC 2005 [DIRS 173617]). The EBS radionuclide transport abstraction (or EBS RT Abstraction) is the conceptual model used in the total system performance assessment for the license application (TSPA-LA) to determine the rate of radionuclide releases from the EBS to the unsaturated zone (UZ). The EBS RT Abstraction conceptual model consists of two main components: a flow model and a transport model. Both models are developed mathematically from first principles in order to show explicitly what assumptions, simplifications, and approximations are incorporated into the models used in the TSPA-LA. The flow model defines the pathways for water flow in the EBS and specifies how the flow rate is computed in each pathway. Input to this model includes the seepage flux into a drift. The seepage flux is potentially split by the drip shield, with some (or all) of the flux being diverted by the drip shield and some passing through breaches in the drip shield that might result from corrosion or seismic damage. The flux through drip shield breaches is potentially split by the waste package, with some (or all) of the flux being diverted by the waste package and some passing through waste package breaches that might result from corrosion or seismic damage. Neither the drip shield nor the waste package survives an igneous intrusion, so the flux splitting submodel is not used in the igneous scenario class. The flow model is validated in an independent model validation technical review. The drip shield and waste package flux splitting algorithms are developed and validated using experimental data. The transport model considers advective transport and diffusive transport from a breached waste package. Advective transport occurs when radionuclides that are dissolved or sorbed onto colloids (or both) are carried from the waste package by the portion of the seepage flux that passes through waste package breaches. Diffusive transport occurs as a result of a gradient in radionuclide concentration and may take place while advective transport is also occurring, as well as when no advective transport is occurring. Diffusive transport is addressed in detail because it is the sole means of transport when there is no flow through a waste package, which may dominate during the regulatory compliance period in the nominal and seismic scenarios. The advective transport rate, when it occurs, is generally greater than the diffusive transport rate. Colloid-facilitated advective and diffusive transport is also modeled and is presented in detail in Appendix B of this report.

J.D. Schreiber

2005-08-25T23:59:59.000Z

255

Reasoning with Generic Cases in the Arithmetic of Abstract Matrices  

E-Print Network [OSTI]

Department of Computer Science, University of Western Ontario www.csd.uwo.ca/watt Abstract. In previous work specifying n. We call this working with "symbolic" or "abstract" values. In previous work we have givenReasoning with Generic Cases in the Arithmetic of Abstract Matrices Alan P. Sexton1 , Volker Sorge1

Sorge, Volker

256

Reasoning with Generic Cases in the Arithmetic of Abstract Matrices  

E-Print Network [OSTI]

Department of Computer Science, University of Western Ontario www.csd.uwo.ca/~watt Abstract. In previous work specifying n. We call this working with "symbolic" or "abstract" values. In previous work we have givenReasoning with Generic Cases in the Arithmetic of Abstract Matrices Alan P. Sexton1 , Volker Sorge1

Watt, Stephen M.

257

Abstract adiabatic charge pumping  

E-Print Network [OSTI]

This paper is devoted to the analysis of an abstract formula describing quantum adiabatic charge pumping in a general context. We consider closed systems characterized by a slowly varying time-dependent Hamiltonian depending on an external parameter $\\alpha$. The current operator, defined as the derivative of the Hamiltonian with respect to $\\alpha$, once integrated over some time interval, gives rise to a charge pumped through the system over that time span. We determine the first two leading terms in the adiabatic parameter of this pumped charge under the usual gap hypothesis. In particular, in case the Hamiltonian is time periodic and has discrete non-degenerate spectrum, the charge pumped over a period is given to leading order by the derivative with respect to $\\alpha$ of the corresponding dynamical and geometric phases.

A. Joye; V. Brosco; F. Hekking

2010-02-05T23:59:59.000Z

258

A Roadmap for Canadian Submillimetre Astronomy  

E-Print Network [OSTI]

We survey the present landscape in submillimetre astronomy for Canada and describe a plan for continued engagement in observational facilities to ~2020. Building on Canada's decadal Long Range Plan process, we emphasize that continued involvement in a large, single-dish facility is crucial given Canada's substantial investment in ALMA and numerous PI-led submillimetre experiments. In particular, we recommend: i) an extension of Canadian participation in the JCMT until at least the unique JCMT Legacy Survey program is able to realize the full scientific potential provided by the world-leading SCUBA-2 instrument; and ii) involvement of the entire Canadian community in CCAT, with a large enough share in the partnership for Canadian astronomers to participate at all levels of the facility. We further recommend continued participation in ALMA development, involvement in many focused PI-led submillimetre experiments, and partnership in SPICA.

Webb, Tracy; Di Francesco, James; Matthews, Brenda; Murray, Norm; Scott, Douglas; Wilson, Christine

2013-01-01T23:59:59.000Z

259

Inversions in astronomy and the SOLA method  

E-Print Network [OSTI]

This paper was presented at the Institute for Mathematics and its Applications workshop "Inverse problems in wave propagation" and will appear in the series IMA volumes (Springer). A brief overview of applications of inversions within astronomy is presented and also an inventory of techniques commonly in use. Most of this paper is focussed on the method of Subtractive Optimally Localized Averages (SOLA) which is an adaptation of the Backus and Gilbert method. This method was originally developed for use in helioseismology where the Backus and Gilbert method is computationally too slow. Since then it has also been applied to the problem of reverberation mapping of active galactic nuclei and the differences between this inverse problem and the ones of helioseismology are also discussed.

F. P. Pijpers

1995-06-14T23:59:59.000Z

260

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Elec-xonics Division Internal Report 140 MV The battery voltage as a function of temperature was also measured. The voltage was extremely

Groppi, Christopher

Note: This page contains sample records for the topic "astronomy department abstract" 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

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report with the calculator. It is constructed from CMOS logic for lowest power consumption and has a NiCad battery back

Groppi, Christopher

262

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report an opposition battery, a DC Null Voltmeter and a recorder. With this set-up a variation in temperature of .02 įC

Groppi, Christopher

263

Abstraction of Drift Seepage  

SciTech Connect (OSTI)

This model report documents the abstraction of drift seepage, conducted to provide seepage-relevant parameters and their probability distributions for use in Total System Performance Assessment for License Application (TSPA-LA). Drift seepage refers to the flow of liquid water into waste emplacement drifts. Water that seeps into drifts may contact waste packages and potentially mobilize radionuclides, and may result in advective transport of radionuclides through breached waste packages [''Risk Information to Support Prioritization of Performance Assessment Models'' (BSC 2003 [DIRS 168796], Section 3.3.2)]. The unsaturated rock layers overlying and hosting the repository form a natural barrier that reduces the amount of water entering emplacement drifts by natural subsurface processes. For example, drift seepage is limited by the capillary barrier forming at the drift crown, which decreases or even eliminates water flow from the unsaturated fractured rock into the drift. During the first few hundred years after waste emplacement, when above-boiling rock temperatures will develop as a result of heat generated by the decay of the radioactive waste, vaporization of percolation water is an additional factor limiting seepage. Estimating the effectiveness of these natural barrier capabilities and predicting the amount of seepage into drifts is an important aspect of assessing the performance of the repository. The TSPA-LA therefore includes a seepage component that calculates the amount of seepage into drifts [''Total System Performance Assessment (TSPA) Model/Analysis for the License Application'' (BSC 2004 [DIRS 168504], Section 6.3.3.1)]. The TSPA-LA calculation is performed with a probabilistic approach that accounts for the spatial and temporal variability and inherent uncertainty of seepage-relevant properties and processes. Results are used for subsequent TSPA-LA components that may handle, for example, waste package corrosion or radionuclide transport.

J.T. Birkholzer

2004-11-01T23:59:59.000Z

264

Page 262 Courses: Astronomy (ASTR) Sonoma State University 2013-2014 Catalog AStr 396 SeLeCted topiCS in AStronoMy (1-3)  

E-Print Network [OSTI]

Page 262 Courses: Astronomy (ASTR) Sonoma State University 2013-2014 Catalog AStr 396 SeLeCted topiCS in AStronoMy (1-3) Lecture, 1-3 hours. A course of lectures on a single topic or set of related topics not ordinarily covered in the Astronomy curriculum. The course may be repeated for credit with a different topic

Ravikumar, B.

265

Courses: Astronomy (ASTR) Page 259Sonoma State University 2012-2013 Catalog ASTR 482 Adv ObSeRvATiOnAl ASTROnOmy (2)  

E-Print Network [OSTI]

Courses: Astronomy (ASTR) Page 259Sonoma State University 2012-2013 Catalog ASTR 482 Adv ObSeRvATiOnAl ASTROnOmy (2) Lecture, 1 hour; laboratory, 3 hours. A study of advanced observing techniques including astronomy. Both written and oral presentations (including a demonstration of the experiment or activity

Ravikumar, B.

266

Page 262 Courses: Astronomy (ASTR) Sonoma State University 2010-2011 Catalog AStr 482 AdV OBSerVAtiOnAl AStrOnOMy (2)  

E-Print Network [OSTI]

Page 262 Courses: Astronomy (ASTR) Sonoma State University 2010-2011 Catalog AStr 482 AdV OBSerVAtiOnAl AStrOnOMy (2) Lecture, 1 hour; laboratory, 3 hours. A study of advanced observing techniques including astronomy. Both written and oral presentations (including a demonstration of the experiment or activity

Ravikumar, B.

267

Page 258 Courses: Astronomy (ASTR) Sonoma State University 2011-2012 Catalog AStr 482 AdV ObSerVAtiOnAl AStrOnOMy (2)  

E-Print Network [OSTI]

Page 258 Courses: Astronomy (ASTR) Sonoma State University 2011-2012 Catalog AStr 482 AdV ObSerVAtiOnAl AStrOnOMy (2) Lecture, 1 hour; laboratory, 3 hours. A study of advanced observing techniques including astronomy. Both written and oral presentations (including a demonstration of the experiment or activity

Ravikumar, B.

268

The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under a cooperative agreement by Associated Universities, Inc. Astronomy: The Visible and Invisible Universe  

E-Print Network [OSTI]

The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under a cooperative agreement by Associated Universities, Inc. Astronomy: The Visible and Invisible Universe #12;The National Radio Astronomy Observatory is a facility of the National Science Foundation

Groppi, Christopher

269

Abstract Data Types and UML Models* Heinrich Hussmann1  

E-Print Network [OSTI]

, Francoise Tort3 1 Department of Computer Science, Dresden University of Technology, Germany 2 DISI in order to find out to which extent it follows clean data abstraction principles. In this sense

Reggio, Gianna

270

E-Print Network 3.0 - astronomy-related rare books Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

astronomy-related rare books Search Powered by Explorit Topic List Advanced Search Sample search results for: astronomy-related rare books Page: << < 1 2 3 4 5 > >> 1 Rare Books...

271

Memory abstractions for parallel programming  

E-Print Network [OSTI]

A memory abstraction is an abstraction layer between the program execution and the memory that provides a different "view" of a memory location depending on the execution context in which the memory access is made. Properly ...

Lee, I-Ting Angelina

2012-01-01T23:59:59.000Z

272

Abstracts  

E-Print Network [OSTI]

cus on the classification of ancient solutions in the curve shortening flow and the Ricci flow on ... has applications in heat control at the boundary of a domain.

2012-05-26T23:59:59.000Z

273

ABSTRACT  

E-Print Network [OSTI]

A new online diagnostics system for the continuous condition monitoring of lubricating oils in industrial gearboxes is presented. Characteristic features of emerging component damage, such as wear, contamination or chemical aging, are identified in an early stage. The OilQSens ģ sensor effectively controls the proper operation conditions of bearings and cogwheels in gears. Also, the condition of insulating oils in transformers can be monitored. The online diagnostics system measures components of the specific complex impedance of oils. For instance, metal abrasion due to wear debris, broken oil molecules, forming acids or oil soaps result in an increase of the electrical conductivity, which directly

Manfred Mauntz; JŁrgen Gegner

274

Abstract  

Office of Scientific and Technical Information (OSTI)

One such site is SASOL in South Africa, which uses ATRs licensed by Lurgi out of Germany. As stated above, KBR-designed ATRs have been installed in ammonia plants in Kitimat,...

275

Abstracts  

E-Print Network [OSTI]

Nov 16, 2013 ... Moreover, various stability results for these waves will be addressed, .... Lewis and coauthors when the measure is p-harmonic and also for p†...

2013-11-13T23:59:59.000Z

276

Abstract  

E-Print Network [OSTI]

excite seismic body waves in the earth. One detects these waves at seismic stations distributed over the earth's surface. Wave-equation tomography is derived†...

2008-07-23T23:59:59.000Z

277

abstract  

E-Print Network [OSTI]

this environment. To find and ... offers researchers an environment where the entire problem ... ware architecture for the FFTĒ, Proceedings of ICASSP. 1998, vol†...

1910-00-82T23:59:59.000Z

278

Abstracts  

E-Print Network [OSTI]

Nov 1, 2014 ... The purpose of Wabash Seminar talks is to present surveys of interest to all analysts, including graduate students and scholars working in†...

2014-10-27T23:59:59.000Z

279

Abstract:  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc Documentation RUCProductstwrmrAre the Effects ofAbout ScienceAbout OakMeasurement of the őĹ

280

Abstract  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout the Building Technologies Office About theofAbout SHAREHands on

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While these samples are representative of the content of NLEBeta,
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to obtain the most current and comprehensive results.


281

Abstract  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout the Building Technologies Office About theofAbout SHAREHands onThis

282

Abstract:  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout the Building Technologies Office About theofAbout SHAREHandsJohn

283

Abstract:  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAbout the Building Technologies Office About theofAbout SHAREHandsJohnNew

284

ABSTRACT  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLasDelivered¬ČPNGExperience4AJ01) (See95TI07) (See4AJ01)59AJ76)74AJ01)

285

ABSTRACT  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsrucLasDelivered¬ČPNGExperience4AJ01) (See95TI07) (See4AJ01)59AJ76)74AJ01)BROWNE, MICHAEL CHARLES.

286

Transformations for Abstractions Eelco Visser  

E-Print Network [OSTI]

of Information and Computing Sciences Universiteit Utrecht July 2005 #12;This is an extended version: Department of Information and Computing Sciences Universiteit Utrecht P.O.Box 80089 3508 TB Utrecht Eelco Department of Information and Computing Sciences, Universiteit Utrecht PO Box 80.089, 3508 TB Utrecht

Utrecht, Universiteit

287

Astronomy & Astrophysics manuscript no. huang_resubm c ESO 2014 May 7, 2014  

E-Print Network [OSTI]

Astronomy & Astrophysics manuscript no. huang_resubm c ESO 2014 May 7, 2014 H spectroscopy of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Shandong. Ireland 3 Institute of Astronomy and National Astronomical Observatory, BAS, 72 Tsarigradsko Chaussee blvd

288

Experimental Astronomy (2004) 17: 261267 C Springer 2005 RFI MITIGATION AND THE SKA  

E-Print Network [OSTI]

Experimental Astronomy (2004) 17: 261­267 C Springer 2005 RFI MITIGATION AND THE SKA STEVEN W radio astronomy from its inception. The Workshop on the Mitigation of Radio Frequency Interference in Radio Astronomy (RFI2004) was held in Penticton, BC, Canada in July 2004 in order to consider

Ellingson, Steven W.

289

IAU DIVISION X, XII / COMMISSION 40, 41 / WORKING GROUP on HISTORICAL RADIO ASTRONOMY  

E-Print Network [OSTI]

IAU DIVISION X, XII / COMMISSION 40, 41 / WORKING GROUP on HISTORICAL RADIO ASTRONOMY CHAIR Kenneth. Introduction The IAU Working Group on Historical Radio Astronomy (WGHRA) was formed at the 2003 General Assembly of the IAU as a Joint Working Group of Commissions 40 (Radio Astronomy) and 41 (History

Groppi, Christopher

290

ASTRONOMY TO INSPIRE AND EDUCATE YOUNG CHILDREN EU-UNAWE Lorentz Center Workshop  

E-Print Network [OSTI]

ASTRONOMY TO INSPIRE AND EDUCATE YOUNG CHILDREN EU-UNAWE Lorentz Center Workshop Official Opening. Mitchell, MEP, Chair, EU Parliamentary Committee on Development Astronomy Research and Education in South Committee for Education, Culture and Science Video messages (5 min) Astronomy and Space collaborations

Galis, Frietson

291

Ivan De Mitri VHE Gamma Ray Astronomy 1 Very High Energy  

E-Print Network [OSTI]

~ 1/day Gamma Ray Bursts The X-ray counterpart detection with better pointing accuracy instrumentsIvan De Mitri VHE Gamma Ray Astronomy 1 Very High Energy Gamma Ray Astronomy Ivan De Mitri'Aquila, 11- Jun -2002 Photo F. Arneodo #12;Ivan De Mitri VHE Gamma Ray Astronomy 2 Seminar Outline Background

Harrison, Thomas

292

Assessment of the Research Institute of Physics and Astronomy of Utrecht  

E-Print Network [OSTI]

Assessment of the Research Institute of Physics and Astronomy of Utrecht University over the period Institute Physics and Astronomy Utrecht University. 1 Assessment of the Research Institute of Physics and Astronomy of Utrecht University over the period 1996-2002. 1 General information 1.1 Introduction

Utrecht, Universiteit

293

The Application of kd-tree in Astronomy  

E-Print Network [OSTI]

The basic idea of the kd-tree algorithm is to recursively partition a point set P by hyperplanes, and to store the obtained partitioning in a binary tree. Due to its immense popularity, many applications in astronomy have been implemented. The algorithm can been used to solve a near neighbor problem for cross-identification of huge catalogs and realize the classification of astronomical objects. Since kd-tree can speed up query and partition spaces, some approaches based on it have been applied for photometric redshift measurement. We give the case studies of kd-tree in astronomy to show its importance and performance.

Dan Gao; Yanxia Zhang; Yongheng Zhao

2008-01-14T23:59:59.000Z

294

Windows on Computer Science Department of Computer and Information Science  

E-Print Network [OSTI]

1 CSCI 120 Windows on Computer Science Department of Computer and Information Science IUPUI What is Computer Science? Is Computer Science the study of computers (Building computers, and writing computer programs) ? Computer Science is no more about computers than astronomy is about telescopes, or biology

Fang, Shiaofen

295

NAME ______________________ NAME ______________________ DEPARTMENT _______________________ DEPARTMENT _______________________  

E-Print Network [OSTI]

_______________________ DEPARTMENT _______________________ Personal Data Sheet Personal Data Sheet Employee fills out electronic I-9 _______________________ Personal Data Sheet Personal Data Sheet Employee fills out electronic I-9 Employee fills out electronic I-9 ______________________ DEPARTMENT _______________________ DEPARTMENT _______________________ Personal Data Sheet Personal Data Sheet

Van Stryland, Eric

296

Materials Department Annual Report 1992  

E-Print Network [OSTI]

Materials Department Annual Report 1992 Published by the Materials Department Ris√ł National and stone by Chr. Dahlgaard Larsen Materials Department Ris√ł National Laboratory, Roskilde, Denmark Tel.: +45 46 77 46 77 Fax: +4542351173 #12;Abstract Selected activities ot the Materials Department at Riso

297

ECOAS 2011 Titles and Abstracts  

E-Print Network [OSTI]

sociated to other families of representations, according to the so-called .... Abstract: We use the technology of linking algebras and linking groupoids to show.

2011-10-11T23:59:59.000Z

298

PROGRAM & ABSTRACTS 13. DANSKE HAVFORSKERMDE  

E-Print Network [OSTI]

Department, DK-4000 Roskilde 129 I (15.7 Ma) is a naturally occurring radioisotope of iodine. The ratio as A Oceanographic Tracer Xiaolin Hou, H. Dahlgaard, S.P. Nielsen Ris√ł National Laboratory, Radiation Research

299

The Open Astronomy Journal, 2008, 1, 1-26 1 1874-3811/08 2008 Bentham Science Publishers Ltd.  

E-Print Network [OSTI]

The Open Astronomy Journal, 2008, 1, 1-26 1 1874-3811/08 2008 Bentham Science Publishers Ltd. #12;2 The Open Astronomy Journal, 2008, Volume 1 Sultana N. Nahar #12;Electron-Ion Recombination Rate Coefficients The Open Astronomy Journal, 2008, Volume 1 3 #12;4 The Open Astronomy Journal, 2008, Volume 1

Nahar, Sultana Nurun

300

GRC 2009 Annual Meeting Announced, Call for Abstracts Issued | Department  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-UpHeatMulti-Dimensional Subject: Guidance for natural gas as aGEAGNEP PartnersGPS

Note: This page contains sample records for the topic "astronomy department abstract" 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

Clara Aldana (Nantes) Abstract: TBA  

E-Print Network [OSTI]

Program Clara Aldana (Nantes) TBA Abstract: TBA Ubertino Battisti (Torino) "Fourier integral operators on manifolds with boundary and index of symplectomorphisms on manifolds with boundary" Abstract using Egorov Theorem, that U is always Fredholm and set i() = i(U ). In a joint work with S. Coriasco

Baer, Christian

302

Technical abstracts: Mechanical engineering, 1990  

SciTech Connect (OSTI)

This document is a compilation of the published, unclassified abstracts produced by mechanical engineers at Lawrence Livermore National Laboratory (LLNL) during the calendar year 1990. Many abstracts summarize work completed and published in report form. These are UCRL-JC series documents, which include the full text of articles to be published in journals and of papers to be presented at meetings, and UCID reports, which are informal documents. Not all UCIDs contain abstracts: short summaries were generated when abstracts were not included. Technical Abstracts also provides descriptions of those documents assigned to the UCRL-MI (miscellaneous) category. These are generally viewgraphs or photographs presented at meetings. An author index is provided at the back of this volume for cross referencing.

Broesius, J.Y. (comp.)

1991-03-01T23:59:59.000Z

303

QANU Research Review11 NOVA and Astronomy 201012  

E-Print Network [OSTI]

), with appendices44 2. Copies of three key publications per research programme.45 46 Remarks concerning the overall to world astronomy far49 disproportionate to its population or GDP. These contributions include50 51 ­ best in the world in the fields of7 astrochemistry/astromineralogy8 Network 3: High-Energy Astrophysics

van Suijlekom, Walter

304

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report line. A 12 V stor- e battery may be attached to the battery connector with pin 1 ground and pin 2 +12 V DC nominal. When the primary power fails, the battery will supply power to the clock. About 1 1/2 amp

Groppi, Christopher

305

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY GREEN BANK, WEST VIRGINIA ELECTRONICS DIVISION TECHNICAL NOTE .:41; CLOCK INFORMATION FOR AST 286 COMPUTERS Ronald B. Weimer The battery backed clock is only read (which does not set the battery clock) the AST keeps time from a second crystal oscillator. A rough block

Groppi, Christopher

306

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report No. 109 BATTERY PACK FOR HEWLETT-PACKARD 5065A RUBIDIUM FREQUENCY STANDARD Michael Balister OCTOBER 1971 NUMBER OF COPIES: 150 #12;BATTERY PACK FOR HEWLETT-PACKARD 5065A RUBIDIUM FREQUENCY STANDARD

Groppi, Christopher

307

Physics and Astronomy Chair: Associate Professor C. Orzel  

E-Print Network [OSTI]

Physics and Astronomy Chair: Associate Professor C. Orzel Faculty: Professors R. Koopmann, S Assistant) Requirements for the Physics Major: Ten courses in physics (Physics 120, 121, 122, 123, 220, 230 departmental colloquium series to gain an appreciation for current research in physics and related areas

Koopmann, Rebecca A.

308

THE PHYSICS MAJOR (Physics and Astronomy & Astrophysics Streams)  

E-Print Network [OSTI]

THE PHYSICS MAJOR (Physics and Astronomy & Astrophysics Streams) Overview: Physics examines, to the behaviour of matter on the subatomic scale - and everything in between. Studying Physics at UWA gives you access to the frontiers of modern physics, built on the pillars of quantum physics and relativity. You

Tobar, Michael

309

Data needs for X-ray astronomy satellites  

SciTech Connect (OSTI)

I review the current status of atomic data for X-ray astronomy satellites. This includes some of the astrophysical issues which can be addressed, current modeling and analysis techniques, computational tools, the limitations imposed by currently available atomic data, and the validity of standard assumptions. I also discuss the future: challenges associated with future missions and goals for atomic data collection.

Kallman, T. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)

2013-07-11T23:59:59.000Z

310

IceCube: An Instrument for Neutrino Astronomy  

E-Print Network [OSTI]

Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it was realized that kilometer-scale neutrino detectors were required. The first such instrument, IceCube, is near completion and taking data. The IceCube project transforms a cubic kilometer of deep and ultra-transparent Antarctic ice into a particle detector. A total of 5,160 optical sensors are embedded into a gigaton of Antarctic ice to detect the Cherenkov light emitted by secondary particles produced when neutrinos interact with nuclei in the ice. Each optical sensor is a complete data acquisition system, including a phototube, digitization electronics, control and trigger systems and LEDs for calibration. The light patterns reveal the type (flavor) of neutrino interaction and the energy and direction of the neutrino, making neutrino astronomy possible. The scientific missions of IceCube include such varied tasks as the search for sources of cosmic rays, the observation of Galactic supernova explosions, the search for dark matter, and the study of the neutrinos themselves. These reach energies well beyond those produced with accelerator beams. The outline of this review is as follows: Neutrino Astronomy and Kilometer-Scale Detectors. High-Energy Neutrino Telescopes: Methodologies of Neutrino Detection. IceCube Hardware. High-Energy Neutrino Telescopes: Beyond Astronomy. Future Projects

Francis Halzen; Spencer R. Klein

2010-07-07T23:59:59.000Z

311

Computer Models in Astronomy and Statistics Stellar Evolution  

E-Print Network [OSTI]

Computer Models in Astronomy and Statistics Stellar Evolution Calibration of X-ray Detectors Embedding Astronomical Computer Models into Complex Statistical Models David A. van Dyk Statistics Section, Imperial College London UCLA, February 2012 David A. van Dyk Complex Analyses with Computer Models

van Dyk, David

312

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia ELECTRONICS DIVISION INTERNAL REPORT the earth's axis and perpendic- ular to the Greenwich Meridian, call it the east-west plane. A telescope's rectangular cordinate components (x,y,z) are X = 882880.0208m Distance from the east-west plane, Greenwich

Groppi, Christopher

313

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report which has been used on all systems mounted in the past at the 300-foot telescope. The East and West 14 are so made to allow the East and West 1410 MHz feeds to be positioned 2. 63, 5.24, 7.88 and 10. 52

Groppi, Christopher

314

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY Green Bank, West Virginia Electronics Division Internal Report (Polarization) Focus Declination Beam East on Sky (Feed West of Center) Beam North to West on Sky (Feed North to West on Sky) Feed moves down toward surface Beam South on Sky Position Read- out Sign 300-FOOT

Groppi, Christopher

315

Astronomy Advisory Panel Richard Bower, Michael Brown, Anthony  

E-Print Network [OSTI]

Astronomy Advisory Panel Richard Bower, Michael Brown, Anthony Challinor, Chris Evans, Paul O to provide large contracts for UK industry. · High Performance Computing access ­ fund hardware upgrades via over 10 years Many UK science areas: dark energy/matter, galactic structure, transients, solar system

Crowther, Paul

316

Abstract Algebra I Course Page  

E-Print Network [OSTI]

Abstract Algebra I. MW 4:35-5:55, Skiles 246. OFFICE HOURS: Tues 11-12 or by appointment. Textbook: Topics in Algebra by I.M. Herstein. Topics covered:.

317

International Pharmaceutical Abstracts (IPA) What is International Pharmaceutical Abstracts?  

E-Print Network [OSTI]

topic into the search box. #12;2 2. Click on Search to continue. 3. Enter terms to describe another in your search results. "Or" broadens your search by letting you search for related terms or synonyms. #12-related health topics. Searching International Pharmaceutical Abstracts The example below illustrates a step

Saskatchewan, University of

318

On the Present and Future of Pulsar Astronomy  

E-Print Network [OSTI]

To face recent observational results obtained in multi-wavelength studies from neutron stars and pulsars with the various theoretical models and to discuss on future perspectives on neutron star astronomy we organized a Joined Discussion (JD02) during the XXVI IAU General Assembly which took place in 2006 August in Prague. More than 150 scientists took actively part in this Joint Discussion. Fourteen invited review talks were presented to view the present and future of pulsar astronomy. Fifty three poster contributions displayed new and exciting results. In this summary we give an overview of the invited review talks and contributed posters. The review talks are subject of review articles which will be published elsewhere. More information on this will be available at http://www.mpe.mpg.de/IAU_JD02 in the near future.

W. Becker; J. Gil; B. Rudak

2007-02-09T23:59:59.000Z

319

Online Search Aids Petroleum Abstracts  

E-Print Network [OSTI]

to enter the words for the query. The center frame will display the list of terms resulting from the queryOnline Search Aids User Guide Petroleum Abstracts¬ģ A Division of The University of Tulsa July 1. A compilation of relevant E&P technical index terms and their relationships, covering the areas of geology

Reynolds, Albert C.

320

Resources Abstracts Input Transaction Form  

E-Print Network [OSTI]

#12;Resources Abstracts Input Transaction Form 4. Title 5. Report Date 6.Urban Aquaculture Covered The University of the District of Columbia 12. Sponsoring Organization Water Resources Research of the rainbow trout (Salmo gairdneri) in a closed recycling water system in an urban environment is described

District of Columbia, University of the

Note: This page contains sample records for the topic "astronomy department abstract" 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

Gamma-Ray Astronomy with ARGO-YBJ  

E-Print Network [OSTI]

ARGO-YBJ is a full coverage air shower array located at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l., 606 g/cm^2) recording data with a duty cycle $\\geq$85% and an energy threshold of a few hundred GeV. In this paper the latest results in Gamma-Ray Astronomy are summarized.

G. Di Sciascio; for the ARGO-YBJ Collaboration

2011-07-18T23:59:59.000Z

322

Hands-on astronomy activities for the elementary school  

SciTech Connect (OSTI)

We held a series of astronomy workshops for local school teachers using astronomy activities from a course we give for Elementary Education majors. The school teachers provide us with feedback about successes and failures. Then we try the revised activities in the classroom. Via this in-service and pre-service feedback, the astronomy laboratory activities in the course have been completely revised over the last three years. The activities we use are almost entirely hands-on. The activities include use of log book (or journal) for describing outside-of-class observations of sunsets, phases of the moon, portable sundial, and the somewhat unique method we use to teach the constellations. In addition, all laboratory activity records are kept in the log book. Laboratory activities cover the use of fists to measure degrees, constellations, phases of the moon, relative distances and size of planets, Invent an Alien, lenses, images and telescopes, and the making of a comet. In our poster, based roughly on the theme of the seasons, we will describe a portable, multi-user sundial, length of the day display using newspaper data, two temperature/season activities, and a model demonstration of why the sundial shadows behave as they do.

Lutz, T.E.; Horne, J.C. [Washington State Univ., Pullman, WA (United States)

1994-12-31T23:59:59.000Z

323

Demo Abstract: MARVEL: Multiple Antenna based Relative Vehicle Localizer  

E-Print Network [OSTI]

to install especially on existing vehicles and exhibit a tradeoff between accuracy and cost. Similarly, usingDemo Abstract: MARVEL: Multiple Antenna based Relative Vehicle Localizer Dong Li , Tarun Bansal , Zhixue Lu and Prasun Sinha Department of Computer Science and Engineering The Ohio State University

Sinha, Prasun

324

Human genome program report. Part 2, 1996 research abstracts  

SciTech Connect (OSTI)

This report contains Part 2 of a two-part report to reflect research and progress in the US Department of Energy Human Genome Program from 1994 through 1996, with specified updates made just before publication. Part 2 consists of 1996 research abstracts. Attention is focused on the following: sequencing; mapping; informatics; ethical, legal, and social issues; infrastructure; and small business innovation research.

NONE

1997-11-01T23:59:59.000Z

325

Merging DBMs E#ciently --Extended Abstract Alexandre David 1  

E-Print Network [OSTI]

Merging DBMs E#ciently -- Extended Abstract Alexandre David 1 Department of Computer Science to reduce the number of DBMs in federations by merging them. Federations are unions of DBMs and are used to represent non­convex zones. Inclusion checking between DBMs is a limited technique to reduce the size

David, Alexandre

326

Merging DBMs Efficiently Extended Abstract Alexandre David1  

E-Print Network [OSTI]

Merging DBMs Efficiently ­ Extended Abstract Alexandre David1 Department of Computer Science algorithms to reduce the number of DBMs in federations by merging them. Federations are unions of DBMs and are used to represent non-convex zones. Inclusion checking between DBMs is a limited technique to reduce

David, Alexandre

327

E-Print Network 3.0 - astronomy smithsonian institution Sample...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Search Powered by Explorit Topic List Advanced Search Sample search results for: astronomy smithsonian institution Page: << < 1 2 3 4 5 > >> 1 12 May 2011 Charles C. Steidel...

328

E-Print Network 3.0 - argentina exhibiting astronomy-related...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

search results for: argentina exhibiting astronomy-related Page: << < 1 2 3 4 5 > >> 1 Potato Research 36 (1993) 3 -12 Wild potato (Solanum sect. Petota) germplasm collecting...

329

DSNF AND OTHER WASTE FORM DEGRADATION ABSTRACTION  

SciTech Connect (OSTI)

The purpose of this analysis/model report (AMR) is to select and/or abstract conservative degradation models for DOE-(US. Department of Energy) owned spent nuclear fuel (DSNF) and the immobilized ceramic plutonium (Pu) disposition waste forms for application in the proposed monitored geologic repository (MGR) postclosure Total System Performance Assessment (TSPA). Application of the degradation models abstracted herein for purposes other than TSPA should take into consideration the fact that they are, in general, very conservative. Using these models, the forward reaction rate for the mobilization of radionuclides, as solutes or colloids, away from the waste fondwater interface by contact with repository groundwater can then be calculated. This forward reaction rate generally consists of the dissolution reaction at the surface of spent nuclear fuel (SNF) in contact with water, but the degradation models, in some cases, may also include and account for the physical disintegration of the SNF matrix. The models do not, however, account for retardation, precipitation, or inhibition of the migration of the mobilized radionuclides in the engineered barrier system (EBS). These models are based on the assumption that all components of the DSNF waste form are released congruently with the degradation of the matrix.

T.A. Thornton

2000-12-20T23:59:59.000Z

330

Materials Department Annual Report 1991  

E-Print Network [OSTI]

Materials Department Annual Report 1991 Published by the Materials Department Ris√ł National, iron and stone by Chr. Dahlgaard Larsen Materials Department Ris√ł National Laboratory, Roskilde, Denmark Tel.: +45 42 37 12 12 Fax: + 45 42 35 11 73 #12;Abstract Selected activities of the Materials

331

Fisherman's Guide to Astronomy 1 Four friends went out on a night fishing expedition.  

E-Print Network [OSTI]

#12;Fisherman's Guide to Astronomy 1 Preface Four friends went out on a night fishing expedition around them has a myriad of impacts on his fishing productivity. More importantly-water fishing. We hope with this short guide, some questions relating salt-water fishing and astronomy

Aslaksen, Helmer

332

Wide-field near-infrared all-reflecting camera with Fabry--Perot for astronomy  

E-Print Network [OSTI]

Wide-field near-infrared all-reflecting camera with Fabry--Perot for astronomy Yin-sheng Sun to small temperature differences in the optical system. Keywords: Fabry-Perot etalon, reflecting, near-infrared, imaging, astronomy 1 INTRODUCTION Our goal is to build a camera that can acquire near-infrared images

Ashley, Michael C. B.

333

South African SKA Project Postgraduate Scholarship Programme Postgraduate Projects for 2013 1. Radio Astronomy Science  

E-Print Network [OSTI]

. Radio Astronomy Science 1.2. Radio Astronomy Science - PhD topics Project Title Project Description Title Project Description Qualifications and Skills Required Link to MeerKAT and/ or SKA Science. This project is related to the MeerKAT continuum survey science and the SKA science theme `Magnetic fields

Jarrett, Thomas H.

334

faculty of engineering and physical sciences School of Physics and Astronomy  

E-Print Network [OSTI]

faculty of engineering and physical sciences School of Physics and Astronomy Visit/Interview Day into the School of Physics and Astronomy at the University of Manchester. The School receives approximately 1200 attributes that will allow them to thrive in our internationally renowned community of academics and students

335

Designing and Mining Multi-Terabyte Astronomy Archives: The Sloan Digital Sky Survey  

E-Print Network [OSTI]

will operate a data pump to support sweep searches touching most of the data. The anticipated queries will re management challenges. Keywords Database, archive, data analysis, data mining, astronomy, scaleable, InternetDesigning and Mining Multi-Terabyte Astronomy Archives: The Sloan Digital Sky Survey Alexander S

Narasayya, Vivek

336

High-Energy Neutrino Astronomy: from AMANDA to Icecube  

E-Print Network [OSTI]

Kilometer-scale neutrino detectors such as IceCube are discovery instruments covering nuclear and particle physics, cosmology and astronomy. Examples of their multidisciplinary missions include the search for the particle nature of dark matter and for additional small dimensions of space. In the end, their conceptual design is very much anchored to the observational fact that Nature accelerates protons and photons to energies in excess of 10^{20} and 10^{13} eV, respectively. The cosmic ray connection sets the scale of cosmic neutrino fluxes. In this context, we discuss the first results of the completed AMANDA detector and the reach of its extension, IceCube.

F. Halzen

2003-10-31T23:59:59.000Z

337

Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy  

E-Print Network [OSTI]

Amateur contributions to professional publications have increased exponentially over the last decades in the field of Planetary Astronomy. Here we review the different domains of the field in which collaborations between professional and amateur astronomers are effective and regularly lead to scientific publications. We discuss the instruments, detectors, softwares and methodologies typically used by amateur astronomers to collect the scientific data in the different domains of interest. Amateur contributions to the monitoring of planets and interplanetary matter, characterization of asteroids and comets, as well as the determination of the physical properties of Kuiper Belt Objects and exoplanets are discussed.

Mousis, O; Beaulieu, J -P; Bouley, S; Carry, B; Colas, F; Klotz, A; Pellier, C; Petit, J -M; Rousselot, P; Dib, M Ali; Beisker, W; Birlan, M; Buil, C; Delsanti, A; Frappa, E; Hammel, H B; Levasseur-Regourd, A -C; Orton, G S; Sanchez-Lavega, A; Santerne, A; Tanga, P; Vaubaillon, J; Zanda, B; Baratoux, D; Boehm, T; Boudon, V; Bouquet, A; Buzzi, L; Dauvergne, J -L; Decock, A; Delcroix, M; Drossart, P; Esseiva, N; Fischer, G; Fletcher, L N; Foglia, S; Gomez-Forrellad, J M; Guarro-Flo, J; Herald, D; Kugel, F; Lebreton, J -P; Lecacheux, J; Leroy, A; Maquet, L; Masi, G; Maury, A; Meyer, F; Pťrez-Hoyos, S; Rajpurohit, A S; Rinner, C; Rogers, J H; Roques, F; Schmude,, R W; Sicardy, B; Tregon, B; Vanhuysse, M; Wesley, A; Widemann, T

2013-01-01T23:59:59.000Z

338

Composite mirror facets for ground based gamma ray astronomy  

E-Print Network [OSTI]

Composite mirrors for gamma-ray astronomy have been developed to fulfill the specifications required for the next generation of Cherenkov telescopes represented by CTA (Cherenkov Telescope Array). In addition to the basic requirements on focus and reflection efficiency, the mirrors have to be stiff, lightweight, durable and cost efficient. In this paper, the technology developed to produce such mirrors is described, as well as some tests that have been performed to validate them. It is shown that these mirrors comply with the needs of CTA, making them good candidates for use on a significant part of the array.

Brun, P; Durand, D; Glicenstein, J-F; Jeanney, C; Medina, M C; Micolon, P; Peyaud, B

2013-01-01T23:59:59.000Z

339

Jefferson Lab Celebrates International Year of Astronomy with Founders of  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: Vegetation ProposedUsingFunInfraredJefferson Lab Click on theJames D.AnnouncesWorld Year ofAstronomy

340

A Guide to the Petroleum Abstracts  

E-Print Network [OSTI]

Petroleum Abstracts A Guide to the Petroleum Abstracts Information Service Serving the Exploration Conferences Covered #12;Petroleum Abstracts . . . your global information partner. Statement of Purpose Petroleum Abstracts is an abstracting and indexing service conducted as a not-for-profit operation

Reynolds, Albert C.

Note: This page contains sample records for the topic "astronomy department abstract" 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

High Energy Neutrino Astronomy: Towards Kilometer-Scale Detectors  

E-Print Network [OSTI]

Of all high-energy particles, only neutrinos can directly convey astronomical information from the edge of the universe---and from deep inside the most cataclysmic high-energy processes. Copiously produced in high-energy collisions, travelling at the velocity of light, and not deflected by magnetic fields, neutrinos meet the basic requirements for astronomy. Their unique advantage arises from a fundamental property: they are affected only by the weakest of nature's forces (but for gravity) and are therefore essentially unabsorbed as they travel cosmological distances between their origin and us. Many of the outstanding mysteries of astrophysics may be hidden from our sight at all wavelengths of the electromagnetic spectrum because of absorption by matter and radiation between us and the source. For example, the hot dense regions that form the central engines of stars and galaxies are opaque to photons. In other cases, such as supernova remnants, gamma ray bursters, and active galaxies, all of which may involve compact objects or black holes at their cores, the precise origin of the high-energy photons emerging from their surface regions is uncertain. Therefore, data obtained through a variety of observational windows---and especially through direct observations with neutrinos---may be of cardinal importance. In this talk, the scientific goals of high energy neutrino astronomy and the technical aspects of water and ice Cherenkov detectors are examined, and future experimental possibilities, including a kilometer-square deep ice neutrino telescope, are explored.

F. Halzen

2001-03-13T23:59:59.000Z

342

Gamma-ray Astronomy: Implications for Fundamental Physics  

E-Print Network [OSTI]

Gamma-ray Astronomy studies cosmic accelerators through their electromagnetic radiation in the energy range between ~100 MeV and ~100 TeV. The present most sensitive observations in this energy band are performed, from space, by the Large Area Telescope onboard the Fermi satellite and, from Earth, by the Imaging Air Cherenkov Telescopes MAGIC, H.E.S.S. and VERITAS. These instruments have revolutionized the field of Gamma-ray Astronomy, discovering different populations of gamma-ray emitters and studying in detail the non-thermal astrophysical processes producing this high-energy radiation. The scientific objectives of these observatories include also questions of fundamental physics. With gamma-ray instruments we study the origin of Galactic cosmic rays, testing the hypothesis or whether they are mainly produced in supernova explosions. Also, we obtain the most sensitive measurement of the cosmic electron-positron spectrum between 20 GeV and 5 TeV. By observing the gamma-ray emission from sources at cosmological distances, we learn about the intensity and evolution of the extragalactic background light, and perform tests of Lorentz Invariance. Moreover, we can search for dark matter by looking for gamma-ray signals produced by its annihilation or decay in over-density sites. In this paper, we review the most recent results produced with the current generation of gamma-ray instruments in these fields of research.

Javier Rico

2011-11-28T23:59:59.000Z

343

IceCube: An Instrument for Neutrino Astronomy  

SciTech Connect (OSTI)

Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it was realized that kilometer-scale neutrino detectors were required. The first such instrument, IceCube, is near completion and taking data. The IceCube project transforms a cubic kilometer of deep and ultra-transparent Antarctic ice into a particle detector. A total of 5,160 optical sensors are embedded into a gigaton of Antarctic ice to detect the Cherenkov light emitted by secondary particles produced when neutrinos interact with nuclei in the ice. Each optical sensor is a complete data acquisition system, including a phototube, digitization electronics, control and trigger systems and LEDs for calibration. The light patterns reveal the type (flavor) of neutrino interaction and the energy and direction of the neutrino, making neutrino astronomy possible. The scientific missions of IceCube include such varied tasks as the search for sources of cosmic rays, the observation of Galactic supernova explosions, the search for dark matter, and the study of the neutrinos themselves. These reach energies well beyond those produced with accelerator beams.

IceCube Collaboration; Halzen, F.; Klein, S.

2010-06-04T23:59:59.000Z

344

Abstract Scalable Performance Engineering Notation | ORNL  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Abstract Scalable Performance Engineering Notation May 01, 2013 Aspen (Abstract Scalable Performance Engineering Notation) is a domain specific language for performance modeling...

345

Arizona Department of Environmental Quality's Application Forms...  

Open Energy Info (EERE)

search OpenEI Reference LibraryAdd to library Web Site: Arizona Department of Environmental Quality's Application Forms and Guidance Website Abstract This site contains forms...

346

The Abstract Domain of Segmented Ranking Functions  

E-Print Network [OSTI]

function by abstract in- terpretation. We build our work on their proposed general framework, and we designThe Abstract Domain of Segmented Ranking Functions Caterina Urban ¬īEcole Normale Sup¬īerieure - CNRS - INRIA, Paris, France urban@di.ens.fr Abstract. We present a parameterized abstract domain for proving

Paris-Sud XI, Université de

347

Fundamentalist physics: why Dark Energy is bad for Astronomy  

E-Print Network [OSTI]

Astronomers carry out observations to explore the diverse processes and objects which populate our Universe. High-energy physicists carry out experiments to approach the Fundamental Theory underlying space, time and matter. Dark Energy is a unique link between them, reflecting deep aspects of the Fundamental Theory, yet apparently accessible only through astronomical observation. Large sections of the two communities have therefore converged in support of astronomical projects to constrain Dark Energy. In this essay I argue that this convergence can be damaging for astronomy. The two communities have different methodologies and different scientific cultures. By uncritically adopting the values of an alien system, astronomers risk undermining the foundations of their own current success and endangering the future vitality of their field. Dark Energy is undeniably an interesting problem to attack through astronomical observation, but it is one of many and not necessarily the one where significant progress is most likely to follow a major investment of resources.

Simon D. M. White

2007-04-18T23:59:59.000Z

348

Status of Neutrino Astronomy: The Quest for Kilometer-Scale Instruments  

E-Print Network [OSTI]

This is a (very) personal attempt to summarize the status of neutrino astronomy: its scientific motivations, our understanding of natural water and ice as particle detectors and, finally, the detector technology.

F. Halzen

1997-01-07T23:59:59.000Z

349

SCUBA-2 instrument: an application of large-format superconducting bolometer arrays for submillimetre astronomy  

E-Print Network [OSTI]

This thesis concerns technical aspects related to the design and operation of the submillimetre common-user bolometer array 2 (SCUBA-2) instrument, a new wide-field camera for submillimetre astronomy currently undergoing ...

Hollister, Matthew Ian

350

University of British Columbia Faraday Show is UBC Physics & Astronomy Outreach Program's  

E-Print Network [OSTI]

University of British Columbia Faraday Show is UBC Physics & Astronomy Outreach Program's annual Outreach Program University of British Columbia Email: outreach@phas.ubc.ca; Phone: 604-822-3675 #12;

Karczmarek, Joanna

351

Mechanical engineering department technical review  

SciTech Connect (OSTI)

The Mechanical Engineering Department Technical Review is published to: (1) inform the readers of various technical activities within the department, (2) promote exchange of ideas, and (3) give credit to the personnel who are achieving the results. The report is formatted into two parts: technical acievements and publication abstracts. The first is divided into eight sections, one for each division in the department providing the reader with the names of the personnel and the division accomplishing the work.

Carr, R.B. Denney, R.M. (eds.)

1981-01-01T23:59:59.000Z

352

United States Department of  

E-Print Network [OSTI]

as an offset, or for registering carbon dioxide reductions using the U.S. Department of Energy 1605(b Report NRS-18 Measurement Guidelines for the Sequestration of Forest Carbon Timothy R.H. Pearson Sandra L)368-0152 Abstract Measurement guidelines for forest carbon sequestration were developed to support reporting

353

Abstraction Layers for Scalable Microfluidic Biocomputers  

E-Print Network [OSTI]

Abstraction Layers for Scalable Microfluidic Biocomputers William Thies1 , John Paul Urbanski2 Hatsopoulos Microfluids Laboratory Massachusetts Institute of Technology {thies, urbanski, thorsen, saman}@mit.edu Abstract. Microfluidic devices are emerging as an attractive technol- ogy for automatically orchestrating

Amarasinghe, Saman

354

E-Print Network 3.0 - accreting brown dwarfs Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

<< < 1 2 3 4 5 > >> 1 The University of Western Ontario DEPARTMENT OF PHYSICS AND ASTRONOMY Summary: : Accretion and dusty disks" ABSTRACT Young brown dwarfs appear to share...

355

abstract newtonian frameworks and their applications  

E-Print Network [OSTI]

Key words: generalized equation, abstract Newton scheme, augmented Lagrangian, multiplier me- thod, local ... Specifically, in this work we concentrate on.

2012-12-05T23:59:59.000Z

356

FirstYear Progress Report for NSFPHY0073057 Department of Physics and Astronomy  

E-Print Network [OSTI]

accom¬≠ plishments include PRL's on two conclusive light supersymmetric particle searches, a study of √? search and the ffl 0 =ffl PRL's. Two propsective PRL's on the rare decays KL ! e + e \\Gamma ¬Į + ¬Į \\Gamma and KL ! e + e \\Gamma e + e \\Gamma have passed collaboration review, a PRL article on the radiative width

Devlin, Thomas J.

357

Internal State Cooling of Molecular Ions Department of Physics and Astronomy Northwestern University,Evanston,IL  

E-Print Network [OSTI]

University,Evanston,IL Introduction J.P.Marler, J.Nguyen,C-Y.Lien,Y-W.Lin, V.Rajagopal, C.Seck, D. A laboratory searches quite interesting. Chiral molecules with right- and left-handed configurations

Hensinger, Winfried

358

John A. Goree Department of Physics and Astronomy, The University of Iowa  

E-Print Network [OSTI]

and in Chip Manufacturing" 1995 Science "Plasma Physics Gets a Home" 28 Mar 1997 Physical Review Focus "Mach and Professional History Education Princeton University Ph.D. Plasma Physics 1985 Princeton University M.A. Plasma for Electrical and Electronic Engineers Research Interests Plasma physics experiments and modeling: Dusty plasmas

Goree, John

359

The Transportation System Inside a Living Cell Department of Physics and Astronomy  

E-Print Network [OSTI]

, or 32 nanometer steps depending on the load it is hauling or on the amount of ATP (fuel. It has workers (proteins), a power plant (mitochondria), roads (actin fibers and microtubules), trucks is the fuel that is used to power molecular motors. The second way is through active transport that works like

Yu, Clare C.

360

University of California, Irvine 2014-2015 1 Department of Physics and Astronomy  

E-Print Network [OSTI]

, to those in biological sciences, and to those in physics, engineering, and other sciences. Faculty members: Physics 3: Intended audience: Premedical students, Biological Sciences majors. Prerequisites: concurrent audience: Physical Sciences and Engineering majors. Prerequisite: concurrent enrollment in Mathematics 2

Stanford, Kyle

Note: This page contains sample records for the topic "astronomy department abstract" 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

Stone Age Distributed Computing (Extended Abstract)  

E-Print Network [OSTI]

on the first page. Copyrights for components of this work owned by others than ACM must be honored. AbstractingStone Age Distributed Computing (Extended Abstract) Yuval Emek Distributed Computing Group ETH wattenhofer@ethz.ch ABSTRACT A new model that depicts a network of randomized finite state machines operating

362

Hybrid Abstractions that Preserve Timed Languages  

E-Print Network [OSTI]

Hybrid Abstractions that Preserve Timed Languages Paulo Tabuada1 and George J. Pappas2 1 Instituto@ee.upenn.edu Abstract. In this paper we consider the problem of extracting an ab- straction from a hybrid control system that determine when trajectories of the original hybrid system can be generated by the abstracted hybrid system

Pappas, George J.

363

A Simple Guide to Backyard Astronomy Using Binoculars or a Small Telescope www.carolrpt.com/astroguide.htm P.1 A Simple Guide to Backyard AstronomyA Simple Guide to Backyard Astronomy  

E-Print Network [OSTI]

to anyone who wants to look upward and behold the magnificence of the night sky. Light pollution complicates information about curbing light pollution and saving money at the same time, or to see a light pollution map astronomy clubs have public outreach programs and advertise public viewing nights. Here is a list of local

Kiss, Emil

364

SRS scientific and technical abstracts, July--September 1992  

SciTech Connect (OSTI)

This document focuses on the scientific and technical information (STT) reports, articles, and presentations generated at the site by various authors and organizations of Westinghouse Savannah River Company and its subcontractors. Abstracts of these STI products are contained within this document. The abstracts have been compiled as they originally appeared in the source reports. No changes to the content have been made except as necessary to correct errors of spelling, to reduce abstract length, or to ensure that the information is unclassified. The abstracts are organized according to information categories ( UC'' categories) established by the Department of Energy's Office of Scientific and Technical Information (OSTI). When reports fall into more than one category, their abstract is included as an entry in the most applicable section of this document. UC-700 General, Miscellaneous, and Progress Reports, UC-701 Chemistry, UC-702 Environmental Sciences, UC-703 Geosciences, UC-704 Materials, UC-705 Mathematics and Computer Sciences, UC-706 Engineering, Equipment, and Instruments, UC-707 Health and Safety, UC-708 Biological Sciences, UC-711 Chemical Separation Processes for Plutonium and Uranium, UC-712 Inertial Confinement Fusion, UC-713 Radioisotope and Radiation Applications, UC-714 Criticality Studies, UC-715 Technology - Feed Materials, UC-721 Defense Waste Management, UC-722 Transportation of Nuclear Materials, UC-731 Nuclear Materials Production, UC-732 Special Isotope Separation (Plutonium), UC-733 Nuclear Raw Materials, UC-741 Chemical High Explosives, UC-742 Applications of Explosions, UC-743 Nuclear Propulsion Systems, UC-744 Aerospace Nuclear Safety, and Index 91.

Not Available

1992-10-01T23:59:59.000Z

365

SRS scientific and technical abstracts, July--September 1992  

SciTech Connect (OSTI)

This document focuses on the scientific and technical information (STT) reports, articles, and presentations generated at the site by various authors and organizations of Westinghouse Savannah River Company and its subcontractors. Abstracts of these STI products are contained within this document. The abstracts have been compiled as they originally appeared in the source reports. No changes to the content have been made except as necessary to correct errors of spelling, to reduce abstract length, or to ensure that the information is unclassified. The abstracts are organized according to information categories (``UC`` categories) established by the Department of Energy`s Office of Scientific and Technical Information (OSTI). When reports fall into more than one category, their abstract is included as an entry in the most applicable section of this document. UC-700 General, Miscellaneous, and Progress Reports, UC-701 Chemistry, UC-702 Environmental Sciences, UC-703 Geosciences, UC-704 Materials, UC-705 Mathematics and Computer Sciences, UC-706 Engineering, Equipment, and Instruments, UC-707 Health and Safety, UC-708 Biological Sciences, UC-711 Chemical Separation Processes for Plutonium and Uranium, UC-712 Inertial Confinement Fusion, UC-713 Radioisotope and Radiation Applications, UC-714 Criticality Studies, UC-715 Technology - Feed Materials, UC-721 Defense Waste Management, UC-722 Transportation of Nuclear Materials, UC-731 Nuclear Materials Production, UC-732 Special Isotope Separation (Plutonium), UC-733 Nuclear Raw Materials, UC-741 Chemical High Explosives, UC-742 Applications of Explosions, UC-743 Nuclear Propulsion Systems, UC-744 Aerospace Nuclear Safety, and Index 91.

Not Available

1992-10-01T23:59:59.000Z

366

WEST VIRGINIA UNIVERSITY and NATIONAL RADIO ASTRONOMY OBSERVATORY APPLICATION FOR RARECATS PROGRAM Deadline for postmark of this application and supporting  

E-Print Network [OSTI]

WEST VIRGINIA UNIVERSITY and NATIONAL RADIO ASTRONOMY OBSERVATORY APPLICATION FOR RARECATS PROGRAM 604 Allen Hall, PO Box 6122 West Virginia University Morgantown, WV 26506-6122 #12;

Groppi, Christopher

367

DlcSsoo |LI Metallurgy Department  

E-Print Network [OSTI]

DlcSsoo |£LI s TT^rrrc^ G en 2 L-V I 7 RisÝ-R-523 Metallurgy Department Progress Report;RisÝ-R-523 METALLURGY DEPARTMENT PROGRESS REPORT FOR THE PERIOD 1 JANUARY TO 31 DECEMBER 1984 Abstract. The activities of the Metallurgy Department at RisÝ during 1984 are described. The work is presented in three

368

Mechanical Engineering Department "The Lindbergh Lectures"  

E-Print Network [OSTI]

Mechanical Engineering Department "The Lindbergh Lectures" Thursday, October 17th, 2013 12:00 ­ 12:50 PM Room 1106 Mechanical Engineering Building 1513 University Avenue MECHANICAL AND NEURAL FACTORS Department of Mechanical Engineering Department of Biomedical Engineering Abstract: Human walking involves

Wisconsin at Madison, University of

369

Automation of Termination: Abstracting CCG through MWG Automation of Termination: Abstracting Calling  

E-Print Network [OSTI]

Automation of Termination: Abstracting CCG through MWG Automation of Termination: Abstracting of Termination: Abstracting CCG through MWG Motivation Termination analysis is a fundamental topic in computer science. While classical results state the undecidability of various termination problems, automated

Ayala-Rincůn, Mauricio

370

Abstracted publications related to the Hanford environment, 1980 to 1988  

SciTech Connect (OSTI)

This abstracted bibliography provides a reference to the diverse environmental activities conducted on the Hanford Site from 1980 through 1988. It includes 500 reports and articles that were prepared largely by onsite contractors and the Department of Energy. Documents contained here were separated into eight subject areas: air and atmosphere, aquatic ecology, effluents and wastes, geology and hydrology, Hanford Site, radioactivity, terrestrial ecology, and socioeconomics. These areas form the basis of a key word index, which is intended to help the reader locate subjects of interest. An author index is also included.

Becker, C.D.; Gray, R.H.

1989-05-01T23:59:59.000Z

371

Filtergraph: An Interactive Web Application for Visualization of Astronomy Datasets  

E-Print Network [OSTI]

Filtergraph is a web application being developed and maintained by the Vanderbilt Initiative in Data-intensive Astrophysics (VIDA) to flexibly and rapidly visualize a large variety of astronomy datasets of various formats and sizes. The user loads a flat-file dataset into Filtergraph which automatically generates an interactive data portal that can be easily shared with others. From this portal, the user can immediately generate scatter plots of up to 5 dimensions as well as histograms and tables based on the dataset. Key features of the portal include intuitive controls with auto-completed variable names, the ability to filter the data in real time through user-specified criteria, the ability to select data by dragging on the screen, and the ability to perform arithmetic operations on the data in real time. To enable seamless data visualization and exploration, changes are quickly rendered on screen and visualizations can be exported as high quality graphics files. The application is optimized for speed in t...

Burger, Dan; Pepper, Joshua; Siverd, Robert J; Paegert, Martin; De Lee, Nathan M

2013-01-01T23:59:59.000Z

372

RASDR: Benchtop Demonstration of SDR for Radio Astronomy  

SciTech Connect (OSTI)

The Society of Amateur Radio Astronomers (SARA) members present the benchtop version of RASDR, a Software Defined Radio (SDR) that is optimized for Radio Astronomy. RASDR has the potential to be a common digital receiver interface useful to many SARA members. This document describes the RASDR 0.0 , which provides digitized radio data to a backend computer through a USB 2.0 interface. A primary component of RASDR is the Lime Microsystems Femtocell chip which tunes from a 0.4-4 GHz center frequency with several selectable bandwidths from 0.75 MHz to 14 MHz. A second component is a board with a Complex Programmable Logic Device (CPLD) chip that connects to the Femtocell and provides two USB connections to the backend computer. A third component is an analog balanced mixer up conversion section. Together these three components enable RASDR to tune from 0.015 MHz thru 3.8GHz of the radio frequency (RF) spectrum. We will demonstrate and discuss capabilities of the breadboard system and SARA members will be able to operate the unit hands-on throughout the workshop.

Vacaliuc, Bogdan [ORNL] [ORNL; Oxley, Paul [Retired] [Retired; Fields, David [ORNL] [ORNL; Kurtz, Dr. Stan [Universidad Nacional Autonoma de Mexico (UNAM)] [Universidad Nacional Autonoma de Mexico (UNAM); Leech, Marcus [Shirleys Bay Radio Astronomy Consortium] [Shirleys Bay Radio Astronomy Consortium

2012-01-01T23:59:59.000Z

373

Analysis of complex networks using aggressive abstraction.  

SciTech Connect (OSTI)

This paper presents a new methodology for analyzing complex networks in which the network of interest is first abstracted to a much simpler (but equivalent) representation, the required analysis is performed using the abstraction, and analytic conclusions are then mapped back to the original network and interpreted there. We begin by identifying a broad and important class of complex networks which admit abstractions that are simultaneously dramatically simplifying and property preserving - we call these aggressive abstractions -- and which can therefore be analyzed using the proposed approach. We then introduce and develop two forms of aggressive abstraction: 1.) finite state abstraction, in which dynamical networks with uncountable state spaces are modeled using finite state systems, and 2.) onedimensional abstraction, whereby high dimensional network dynamics are captured in a meaningful way using a single scalar variable. In each case, the property preserving nature of the abstraction process is rigorously established and efficient algorithms are presented for computing the abstraction. The considerable potential of the proposed approach to complex networks analysis is illustrated through case studies involving vulnerability analysis of technological networks and predictive analysis for social processes.

Colbaugh, Richard; Glass, Kristin. [New Mexico Institute of Mining and Technology, Socorro, NM; Willard, Gerald [Department of Defense, Ft. Meade, MD

2008-10-01T23:59:59.000Z

374

DEPARTMENT OF ENERGY Privacy Awareness Training | Department...  

Energy Savers [EERE]

DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy...

375

Virtual Sensors: Abstracting Data from Physical Sensors  

E-Print Network [OSTI]

Virtual Sensors: Abstracting Data from Physical Sensors TR-UTEDGE-2006-001 Sanem Kabadayi Adam Pridgen Christine Julien © Copyright 2006 The University of Texas at Austin #12;Virtual Sensors: Abstracting Data from Physical Sensors Sanem Kabadayi, Adam Pridgen, and Christine Julien The Center

Julien, Christine

376

Semi-Autonomous Intersection Management (Extended Abstract)  

E-Print Network [OSTI]

Semi-Autonomous Intersection Management (Extended Abstract) Tsz-Chiu Au School of Electrical@cs.utexas.edu ABSTRACT Autonomous Intersection Management (AIM) is a reservation-based intersection control protocol. AIM was designed for the time when all, or most, of the vehicles on the road are fully autonomous

Au, Tsz-Chiu

377

Call for Abstracts-- 2014 National Environmental Justice Conference and Training Program, Deadline for Submission of Abstracts  

Broader source: Energy.gov [DOE]

Course Title:†††Call for Abstracts--2014 National Environmental Justice Conference and Training Program

378

A LIVELY ELECTRONIC COMPENDIUM OF RESEARCH, NEWS, RESOURCES, AND OPINION Astronomy Education Review2011, AER, 10, 010302-1, 10.3847/AER2011036  

E-Print Network [OSTI]

2011, AER, 10, 010302-1, 10.3847/AER2011036 Astronomy Apps for Mobile Devices, A First Catalog Andrew

Fillingim, Matthew

379

Research departments Materials Research Department  

E-Print Network [OSTI]

and alleviate atmospheric pollution in colla- boration with DMU (the National En- vironmental Research Institute Countries is also part of this department. Wind Energy and Atmospheric Physics Department (Formerly

380

Physics-Astronomy Library Permanent Reserve Collection -Loan Periods Vary (revised 8/27/2010) AUTHOR TITLE E-BOOK CALL NUMBER  

E-Print Network [OSTI]

Physics-Astronomy Library Permanent Reserve Collection - Loan Periods Vary (revised 8, 3rd ed. QA 931 L283 1986 Shu, F.H. Physical Universe QB 43.2 S54 1982 Chaisson, E., et al Astronomy: A Beginner's Guide to the Universe, 5th ed. QB 43.3 C43 2007 Chaisson, E., et al Astronomy Today, 5th ed. QB

Wurtele, Jonathan

Note: This page contains sample records for the topic "astronomy department abstract" 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

Research Science and Education: The NSF's Astronomy and Astrophysics Postdoctoral Fellowship  

E-Print Network [OSTI]

The NSF's Astronomy and Astrophysics Postdoctoral Fellowship (AAPF) is exceptional among the available postdoctoral awards in Astronomy and Astrophysics. The fellowship is one of the few that allows postdoctoral researchers to pursue an original research program, of their own design, at the U.S. institution of their choice. However, what makes this fellowship truly unique is the ability of Fellows to lead an equally challenging, original educational program simultaneously. The legacy of this singular fellowship has been to encourage and advance leaders in the field who are equally as passionate about their own research as they are about sharing that research and their passion for astronomy with students and the public. In this positional paper we address the importance of fellowships like the AAPF to the astronomical profession by identifying the science and educational contributions that Fellows have made to the community. Further, we recommend that fellowships that encourage leading postdoctoral researchers...

Norman, Dara; Brown, Timothy M; Browning, Matthew; Chakrabarti, Sukanya; Cobb, Bethany; Coble, Kim; Conselice, Christopher; Cruz, Kelle; Danly, Laura; Frinchaboy, Peter M; Gawiser, Eric; Gelfand, Joseph; Gonzalez, Anthony; Hoffman, Jennifer L; Huterer, Dragan; Johnson, John; Johnson, Roberta M; Kannappan, Sheila; de Naray, Rachel Kuzio; Lai, David; Leonard, Douglas C; Lystrup, Makenzie; Markoff, Sera; Menendez-Delmestre, Karin; Muchovej, Stephan; McSwain, M Virginia; Rhode, Katherine; Smecker-Hane, Tammy; Smith, Malcolm; Sokoloski, Jennifer; Tran, Kim-Vy

2009-01-01T23:59:59.000Z

382

Neutrino Astronomy and Cosmic Rays Spectroscopy at Horizons  

E-Print Network [OSTI]

A new air-showering physics may rise in next years at horizon, offering at different angles and altitudes a fine tuned filtered Cosmic Rays astrophysics and an upward Neutrino induced air-showering astronomy. Most of this opportunity arises because of neutrino masses, their mixing and the consequent replenishment of rarest tau flavor during its flight in Space. Horizontal air atmosphere act as a filter for High energy Cosmic Rays (CR) and as a beam dump for Ultra High Energy (UHE) neutrinos and a powerfull amplifier for its tau decay in air by its wide showering areas. Earth sharp shadows plays the role of a huge detector volume for UHE neutrino and a noise-free screen for upcoming EeVs tau air-showers (as well PeVs anti-neutrino electron air interactions). Projects for Tau Airshowers are growing at the top of a mountains or at the edge of a cliff. ASHRA in Hawaii and CRNTN in Utah are tracking fluorescence lights, while other novel projects on Crown array detectors on mountains, on balloons and satellites are elaborated for Cherenkov lights. AUGER, facing the Ande edges, ARGO located within a deep valley are testing inclined showers; MILAGRO (and MILAGRITO) may be triggered by horizontal up-going muon bundles from the Earth edges; HIRES and AUGER UHECR detectors, linking twin array telescopes along their axis may test horizontal Cerenkov blazing photons. MAGIC (Hess, Veritas) and Shalon Telescopes may act already like a detector for few PeVs and Glashow resonance neutrino events; MAGIC pointing downward to terrestrial ground acts as a massive tens of km^3 detector, making it the most sensitive dedicated neutrino telescope. MAGIC facing the sea edges must reveal mirrored downward UHECR Air-showers Cherenkov flashes. Magic-crown systems may lead to tens km^3, neutrino detectors.

D. Fargion

2006-04-20T23:59:59.000Z

383

06241 Abstracts Collection Human Motion -Understanding, Modeling,  

E-Print Network [OSTI]

06241 Abstracts Collection Human Motion - Understanding, Modeling, Capture and Animation. 13th Summary Human Motion - Understanding, Modeling, Capture and Animation. 13th Workshop Reinhard Klette 06241 Human Motion - Understanding, Modeling, Capture and Animation. 13th Workshop "Theoretical

384

Pulmonary toxicology of respirable particles. [Lead abstract  

SciTech Connect (OSTI)

Separate abstracts were prepared for the 44 papers presented in these proceedings. The last paper (Stannard) in the proceedings is an historical review of the field of inhalation toxicology and is not included in the analytics. (DS)

Sanders, C.L.; Cross, F.T.; Dagle, G.E.; Mahaffey, J.A. (eds.)

1980-09-01T23:59:59.000Z

385

Kansas Statistical Abstract 2005 (40th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on population, vital statistics and health, housing, elections, education, business and manufacturing, exports, employment, income, ...

Policy Research Institute

2008-10-21T23:59:59.000Z

386

Kansas Statistical Abstract 2007 (42nd Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on agriculture, banking and finance, business and exports, climate, communications and information, crime, education, employment and ...

Policy Research Institute

2008-10-21T23:59:59.000Z

387

Kansas Statistical Abstract 2001 (36th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on population, vital statistics and health, housing, elections, education, business and manufacturing, exports, employment, income, ...

2002-12-01T23:59:59.000Z

388

Kansas Statistical Abstract 2008 (43rd Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on agriculture, banking and finance, business and exports, climate, communications and information, crime, education, employment and ...

Policy Research Institute

2009-09-21T23:59:59.000Z

389

Kansas Statistical Abstract 2009 (44th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on agriculture, banking and finance, business and exports, climate, communications and information, crime, education, employment and ...

Policy Research Institute

2011-03-02T23:59:59.000Z

390

Kansas Statistical Abstract 2004 (39th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on population, vital statistics and health, housing, elections, education, business and manufacturing, exports, employment, income, ...

Policy Research Institute

2006-01-31T23:59:59.000Z

391

Kansas Statistical Abstract 2003 (38th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on population, vital statistics and health, housing, elections, education, business and manufacturing, exports, employment, income, ...

Policy Research Institute

2004-09-01T23:59:59.000Z

392

Kansas Statistical Abstract 2012 (47th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract 2012, contains the latest available state, county, and city-level data for Kansas on population, vital statistics and health, housing, education, business and manufacturing, exports, employment, ...

Institute for Policy & Social Research

2014-05-27T23:59:59.000Z

393

Kansas Statistical Abstract 2002 (37th Edition)  

E-Print Network [OSTI]

The Kansas Statistical Abstract contains state, county, and city-level data for Kansas on population, vital statistics and health, housing, elections, education, business and manufacturing, exports, employment, income, ...

2003-09-01T23:59:59.000Z

394

Sandia National Laboratories: Online Abstracts and Reports  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

of Page Abstract (16.KB PDF) Report (2.0MB PDF) "Simulation and Testing of Resin Infusion Manufacturing Processes for Large Composite Structures" D.B. Mastbergen October 2007...

395

Energy Blog | Department of Energy  

Broader source: Energy.gov (indexed) [DOE]

country to compete in a range of science disciplines, including biology, chemistry, earth science, physics, astronomy and math. The members of the winning team, from Roosevelt...

396

Submillimetre/TeraHertz Astronomy at Dome C with CEA filled bolometer array  

E-Print Network [OSTI]

Submillimetre/TeraHertz (e.g. 200, 350, 450 microns) astronomy is the prime technique to unveil the birth and early evolution of a broad range of astrophysical objects. A major obstacle to carry out submm observations from ground is the atmosphere. Preliminary site testing and atmospheric transmission models tend to demonstrate that Dome C could offer the best conditions on Earth for submm/THz astronomy. The CAMISTIC project aims to install a filled bolometer-array camera with 16x16 pixels on IRAIT at Dome C and explore the 200-$\\mu$m windows for potential ground-based observations.

Vincent Minier; Gilles Durand; Pierre-Olivier Lagage; Michel Talvard; Tony Travouillon; Maurizio Busso; Gino Tosti

2007-02-19T23:59:59.000Z

397

A Sustainable approach to large ICT Science based infrastructures; the case for Radio Astronomy  

E-Print Network [OSTI]

Large sensor-based infrastructures for radio astronomy will be among the most intensive data-driven projects in the world, facing very high power demands. The geographically wide distribution of these infrastructures and their associated processing High Performance Computing (HPC) facilities require Green Information and Communications Technologies (ICT). A combination is needed of low power computing, efficient data storage, local data services, Smart Grid power management, and inclusion of Renewable Energies. Here we outline the major characteristics and innovation approaches to address power efficiency and long-term power sustainability for radio astronomy projects, focusing on Green ICT for science.

Barbosa, Domingos; Boonstra, Albert-Jan; Aguiar, Rui; van Ardenne, Arnold; de Santander-Vela, Juande; Verdes-Montenegro, Lourdes

2014-01-01T23:59:59.000Z

398

Earth Sciences Division collected abstracts: 1980  

SciTech Connect (OSTI)

This report is a compilation of abstracts of papers, reports, and talks presented during 1980 at national and international meetings by members of the Earth Sciences Division, Lawrence Livermore National Laboratory. The arrangement is alphabetical (by author). For a given report, a bibliographic reference appears under the name of each coauthor, but the abstract itself is given only under the name of the first author (indicated in capital letters) or the first Earth Sciences Division author.

Henry, A.L.; Hornady, B.F. (eds.)

1981-10-15T23:59:59.000Z

399

Photoinduced Hydrogen Abstraction from Phenols by Aromatic Ketones. A New Mechanism for Hydrogen Abstraction by  

E-Print Network [OSTI]

Photoinduced Hydrogen Abstraction from Phenols by Aromatic Ketones. A New Mechanism for Hydrogen carried out of the kinetics of inter- and intramolecular phenolic hydrogen abstraction phenolic hydrogen, which yields the corresponding phenoxyl-hemipinacol biradical. The biradicals have also

Leigh, William J.

400

Abstract In the years since Charles Elton proposed that more diverse communities should be less susceptible to  

E-Print Network [OSTI]

: J.S. Dukes, Department of Biology, University of Utah, 257 S. 1400 East, Salt Lake City, UT 84112Abstract In the years since Charles Elton proposed that more diverse communities should be less

Dukes, Jeffrey

Note: This page contains sample records for the topic "astronomy department abstract" 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

Mechanical Engineering Department Technical Review  

SciTech Connect (OSTI)

The Mechanical Engineering Department Technical Review is published to inform readers of various technical activities within the Department, promote exchange of ideas, and give credit to personnel who are achieving the results. The report is presented in two parts: technical achievements and publication abstracts. The first is divided into seven sections, each of which reports on an engineering division and its specific activities related to nuclear tests, nuclear explosives, weapons, energy systems, engineering sciences, magnetic fusion, and materials fabrication.

Carr, R.B.; Denney, R.M. (eds.)

1981-07-01T23:59:59.000Z

402

HELSINKI UNIVERSITY OF TECHNOLOGY Department of Computer Science and Engineering  

E-Print Network [OSTI]

Licentiate's Thesis submitted in partial fulfillment of the requirements for the degree of Licentiate Korhonen #12;HELSINKI UNIVERSITY ABSTRACT OF OF TECHNOLOGY LICENTIATE THESIS Department of Computer Science

403

California Department of Fish and Wildlife Consistency Determination...  

Open Energy Info (EERE)

search OpenEI Reference LibraryAdd to library Web Site: California Department of Fish and Wildlife Consistency Determination Webpage Abstract This website explains the...

404

California Department of Fish and Wildlife Environmental Review...  

Open Energy Info (EERE)

search OpenEI Reference LibraryAdd to library Web Site: California Department of Fish and Wildlife Environmental Review and Permitting Webpage Abstract This website provides...

405

Bounds Analysis by Abstract Interpretation Xiaolei Qian Allen Goldberg  

E-Print Network [OSTI]

representations fo* *r these abstract types. In this work an abstract context, i.e. model, consists * Bounds Analysis by Abstract@csl.sri.com goldberg@kestrel.edu Abstract Abstract interpretation

Goldberg, Allen

406

Earth Sciences Division collected abstracts: 1979  

SciTech Connect (OSTI)

This report is a compilation of abstracts of papers, internal reports, and talks presented during 1979 at national and international meetings by members of the Earth Sciences Division, Lawrence Livermore Laboratory. The arrangement is alphabetical (by author). For a given report, a bibliographic reference appears under the name of each coauthor, but the abstract iself is given only under the name of the first author or the first Earth Sciences Division author. A topical index at the end of the report provides useful cross references, while indicating major areas of research interest in the Earth Sciences Division.

Henry, A.L.; Schwartz, L.L.

1980-04-30T23:59:59.000Z

407

Matlab Tutorial In association with Lab #3 of Phys 322, Observational Astronomy  

E-Print Network [OSTI]

Lab # 3 Matlab Tutorial In association with Lab #3 of Phys 322, Observational Astronomy Start IDL: To start Matlab, click on the Matlab icon on the left in the task bar. After a moment, a window will appear Matlab's current directory setting (using the text box at the top of the screen) to the directory where

Gary, Dale E.

408

NATIONAL RADIO ASTRONOMY OBSERVATORY TITLE: A REVISED VAX FARANT SPLOT ROUTINE AND RELATED APPLE  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY TITLE: A REVISED VAX FARANT SPLOT ROUTINE AND RELATED APPLE #12;A REVISED VAX FARANT SPLOT ROUTINE AND RELATED APPLE II PLOTTING PROGRAM. The purpose of this report is to describe some upgrades made to the VAX 1 SPLOT" routine and the related Apple plotting

Groppi, Christopher

409

226 Physics and Astronomy 227 All physics majors must complete the  

E-Print Network [OSTI]

226 Physics and Astronomy 227 All physics majors must complete the following courses: PHYS 101 and Optics PHYS 202 Modern Physics PHYS 231 Elementary Physics Laboratory II PHYS 301 Intermediate Mechanics 211/ MATH 212) Additional courses for the B.S. degree in physics: PHYS 302 Intermediate

Richards-Kortum, Rebecca

410

2013 University of Rochester 1 All rights reserved Astronomy 142: Elementary astrophysics  

E-Print Network [OSTI]

-165/171-174, and Astronomy 111. Professor: Dan Watson (B&L 418, 275-8576, dmw@pas.rochester.edu, www.pas.rochester.edu/~dmw. World Wide Web site: http://www.pas.rochester.edu/~dmw/ast142/ . In these pages one will find complete

411

Astronomy 202: Astrophysical Gas Dynamics LL = Fluid Mechanics by Landau & Lifshitz  

E-Print Network [OSTI]

Astronomy 202: Astrophysical Gas Dynamics LL = Fluid Mechanics by Landau & Lifshitz PP = Plasma Fluid Dynamics by D. J. Tritton You should start by reading the Feynman Lectures Vol II, Ch 40 & 41 (Shu Ch. 1) 2. Equations of Gas Dynamics: neutral ideal fluids (LL Ch. 1; esp. §1,2,5,6,7,8,10; Shu Ch

Wurtele, Jonathan

412

Roadmap for Ultra-High Energy Cosmic Ray Physics and Astronomy (whitepaper for Snowmass 2013)  

E-Print Network [OSTI]

We summarize the remarkable recent progress in ultra-high energy cosmic ray physics and astronomy enabled by the current generation of cosmic ray observatories. We discuss the primary objectives for future measurements and describe the plans for near-term enhancements of existing experiments as well as the next generation of observatories.

Anchordoqui, Luis A; Krizmanic, John F; Matthews, Jim; Mitchell, John W; Olinto, Angela V; Paul, Thomas C; Sokolsky, Pierre; Thomson, Gordon B; Weiler, Thomas J

2013-01-01T23:59:59.000Z

413

Science Programme Prioritisation 2010-2015 Report from the Particle Physics, Astronomy and Nuclear Physics Science  

E-Print Network [OSTI]

Astrophysics Advisory Panel (PAAP) as well as the Ground Based Facilities Review of Astronomy (GBFR Advanced LIGO ATLAS ATLAS UPGRADES CMS CMS UPGRADES GAIA post-launch support GridPP Ground Based-launch support Boulby underground facility JAI LHeC NG1df SUPER B Below Alpha MoonLITE #12;4 of 19 Development

Crowther, Paul

414

Directions to the National Radio Astronomy Observatory Green Bank, West Virginia  

E-Print Network [OSTI]

Directions to the National Radio Astronomy Observatory Green Bank, West Virginia From Charleston Roanoke, VA: Via I-64 West, exit at White Sulphur Springs (Exit 181) and take Rt. 92 North to Green Bank, then take Rt. 92 South to Green Bank. From Washington DC: Via I-66 West to I-81 South. Option 1: Take I-81

Groppi, Christopher

415

The Astronomy of the Kamilaroi People and their Neighbours Robert S. Fuller1,2  

E-Print Network [OSTI]

and 1838 in the region, many from historically known massacres of Aboriginal people. Sveiby and SkuthorpeThe Astronomy of the Kamilaroi People and their Neighbours Robert S. Fuller1,2 , Ray P. Norris1 The Kamilaroi people and their neighbours, the Euahlayi, Ngemba, and Murrawarri, are an Aboriginal cultural

Norris, Ray

416

Gamma Ray Astronomy with Air Shower Arrays A.I. Mincer 1  

E-Print Network [OSTI]

Gamma Ray Astronomy with Air Shower Arrays A.I. Mincer 1 New York University, New York, NY 10003 in the Jemez Mountains near Los Alamos, New Mexico and ARGO is under construction in Yangbajing these energies. When a primary energetic photon enters the earth's at­ mosphere, it interacts producing secondary

California at Santa Cruz, University of

417

Highlights of Astronomy, Volume 14 XXVIth IAU General Assembly, August 2006  

E-Print Network [OSTI]

. Battaglia1 1 Institute of Astronomy, ETH Zurich, 8092-Zurich, Switzerland email: benz of the coronal source for the first time (Battaglia & Benz 2006). We compare the time behaviour; Battaglia et al. 2005). The SHS behaviour thus constitutes a conspicuous property of the acceleration

418

Highlights of Astronomy, Volume 14 XXVIth IAU General Assembly, August 2006  

E-Print Network [OSTI]

. Battaglia 1 1 Institute of Astronomy, ETH Zurich, 8092­Zurich, Switzerland email: benz of the coronal source for the first time (Battaglia & Benz 2006). We compare the time behaviour; Battaglia et al. 2005). The SHS behaviour thus constitutes a conspicuous property of the acceleration

419

Property:Abstract | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector GeneralDepartmentAUDIT REPORTOpenWende New Energy CoFirstNovosPatriot Wind

420

Natural radiation environment III. [Lead Abstract  

SciTech Connect (OSTI)

Separate abstracts were prepared for the 52 research papers presented at this symposium in April 1978. The major topics in this volume deal with penetrating radiation measurements, radiation surveys and population exposure, radioactivity in the indoor environment, and technologically enhanced natural radioactivity. (KRM)

Gesell, T.F.; Lowder, W.M. (eds.)

1980-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "astronomy department abstract" 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

Book of Abstracts The Center for Nanoscience &  

E-Print Network [OSTI]

Book of Abstracts 5th Workshop The Center for Nanoscience & Nanotechnology Tel Aviv University: 5TH Workshop The Center for Nanoscience & Nanotechnology Tel Aviv University February 22-24, 2009 Ha: ... " S.E.C. SCIENTIFIC EQUIPMENT CO. LTD. 5TH Workshop The Center for Nanoscience & Nanotechnology Tel

Lifshitz, Ron

422

Abstract AndParallel Machines Nachum Dershowitz  

E-Print Network [OSTI]

Abstract And­Parallel Machines Nachum Dershowitz University of Illinois Urbana, IL 61801 U are introduced. The first of them, the And­ Parallel Turing Machine, can be viewed as a generalization of the deterministic Turing machine in which the infinite tape is replaced by an infinite tree­like tape on which

Dershowitz, Nachum

423

Equilibrium Pricing with Positive Externalities (Extended Abstract)  

E-Print Network [OSTI]

a product in the presence of historical externalities? A low introductory price may attract early adoptersEquilibrium Pricing with Positive Externalities (Extended Abstract) Nima Anari1 , Shayan Ehsani1 an item to strategic buyers in the pres- ence of positive historical externalities, where the value

Immorlica, Nicole

424

Colorado Natural Heritage Program 2003 Project Abstracts  

E-Print Network [OSTI]

Colorado Natural Heritage Program 2003 Project Abstracts #12;Cover photo: A CNHP researcher collects freshwater specimens (Pisidium spp.) at Long Slough Reservoir on the Grand Mesa of Colorado's West of Colorado's biodiversity, what efforts are underway to maintain it, and why more biological information

425

Abstract explanations in science Christopher Pincock  

E-Print Network [OSTI]

Introduction 2 2 A Case 3 3 Abstract and Causal Explanations 9 British Journal for the Philosophy of Science 22 1 Introduction In the philosophy of science discussions of explanation tend to assume that most of explanation.1 The risk of this approach is that it may turn out that explanations are not all of the same kind

Pincock, Chris

426

Transforming and Refining Abstract Constraint Specifications  

E-Print Network [OSTI]

Transforming and Refining Abstract Constraint Specifications Alan M. Frisch1 , Brahim Hnich2 , Ian choose model transformations to reduce greatly the amount of effort that is required to solve a problem by systematic search. It is a consid- erable challenge to automate such transformations. A problem may be viewed

Walsh, Toby

427

Managed Data: Modular Strategies for Data Abstraction  

E-Print Network [OSTI]

these mechanisms to define specific kinds of data. Managed Data allows program- mers to take control of many management mechanism, not properties of individ- ual data types. It is possible to define such featuresManaged Data: Modular Strategies for Data Abstraction Alex Loh University of Texas at Austin

Cook, William R.

428

ALGEBRA SEMINAR TALK Department of Computer Science  

E-Print Network [OSTI]

ALGEBRA SEMINAR TALK WITH LILA KARI Department of Computer Science The University of Western for Theoretical Computer Science" Abstract: We are now witnessing exciting interactions between computer science absorbing notions, techniques and methodologies intrinsic to computer science and mathematics, theoretical

Sinnamon, Gordon J.

429

Mechanical Engineering Department "The Lindbergh Lectures"  

E-Print Network [OSTI]

Mechanical Engineering Department "The Lindbergh Lectures" Thursday, November 14th, 2013 12:00 ­ 12:50 PM Room 1106 Mechanical Engineering Building MECHANICAL MICRO-MANUFACTURING RESEARCH @ CARNEGIE MELLON UNIVERSITY BURAK OZDOGANLAR, CARNEGIE MELLON UNIVERSITY Abstract: Mechanical

Wisconsin at Madison, University of

430

Proceedings of the 8th International Symposium on Cavitation CAV2012 -Abstract No. 198  

E-Print Network [OSTI]

Proceedings of the 8th International Symposium on Cavitation CAV2012 - Abstract No. 198 August 14-PHASE FLOW WITH CAVITATION Keh-Ming Shyue Department of Mathematics National Taiwan University Taipei, Taiwan for the efficient numerical simulation of compressible two-phase flow with cavitation. The algorithm uses a five

Shyue, Keh-Ming

431

Automatic identification of abstract online groups  

DOE Patents [OSTI]

Online abstract groups, in which members aren't explicitly connected, can be automatically identified by computer-implemented methods. The methods involve harvesting records from social media and extracting content-based and structure-based features from each record. Each record includes a social-media posting and is associated with one or more entities. Each feature is stored on a data storage device and includes a computer-readable representation of an attribute of one or more records. The methods further involve grouping records into record groups according to the features of each record. Further still the methods involve calculating an n-dimensional surface representing each record group and defining an outlier as a record having feature-based distances measured from every n-dimensional surface that exceed a threshold value. Each of the n-dimensional surfaces is described by a footprint that characterizes the respective record group as an online abstract group.

Engel, David W; Gregory, Michelle L; Bell, Eric B; Cowell, Andrew J; Piatt, Andrew W

2014-04-15T23:59:59.000Z

432

SATURATED ZONE FLOW AND TRANSPORT MODEL ABSTRACTION  

SciTech Connect (OSTI)

The purpose of the saturated zone (SZ) flow and transport model abstraction task is to provide radionuclide-transport simulation results for use in the total system performance assessment (TSPA) for license application (LA) calculations. This task includes assessment of uncertainty in parameters that pertain to both groundwater flow and radionuclide transport in the models used for this purpose. This model report documents the following: (1) The SZ transport abstraction model, which consists of a set of radionuclide breakthrough curves at the accessible environment for use in the TSPA-LA simulations of radionuclide releases into the biosphere. These radionuclide breakthrough curves contain information on radionuclide-transport times through the SZ. (2) The SZ one-dimensional (I-D) transport model, which is incorporated in the TSPA-LA model to simulate the transport, decay, and ingrowth of radionuclide decay chains in the SZ. (3) The analysis of uncertainty in groundwater-flow and radionuclide-transport input parameters for the SZ transport abstraction model and the SZ 1-D transport model. (4) The analysis of the background concentration of alpha-emitting species in the groundwater of the SZ.

B.W. ARNOLD

2004-10-27T23:59:59.000Z

433

Metallurgy Department Progress Report for the Period  

E-Print Network [OSTI]

Dlcfc^ooWS imsm "-"' Metallurgy Department Progress Report for the Period 1 January to 31 December 1962 (Uw National Laboratory, DK-4000 Roskilde, Denmark July 1963 #12;RisÝ-R-486 METALLURGY DEPARTMENT PROGRESS REPORT FOR THE PERIOD 1 JANUARY TO 31 DECEMBER 1982 Abstract. The activities of the Metallurgy

434

Mechanical Engineering Department "The Lindbergh Lectures"  

E-Print Network [OSTI]

Mechanical Engineering Department "The Lindbergh Lectures" Thursday, February 13th 12:00 ­ 12 Bart Raeymaekers Department of Mechanical Engineering, University of Utah, Abstract: Approximately 285 is Assistant Professor in the Dept. of Mechanical Engineering at the University of Utah. He received his M

Wisconsin at Madison, University of

435

Department of Economics and Business Aarhus University  

E-Print Network [OSTI]

Department of Economics and Business Aarhus University Fuglesangs Allé 4 DK-8210 Aarhus V Denmark@creates.au.dk Department of Economics and Business, and CREATES Aarhus University November 2013 Abstract This paper in Oviedo and the CDMA Workshop on DSGE models in St. Andrews for their helpful comments. I also thank Olaf

436

Small Business Innovation Research: Abstracts of Phase 1 awards, 1994  

SciTech Connect (OSTI)

The Small Business Innovation Research (SBIR) program enables DOE to obtain effective, innovative solutions to important problems through the private sector, which has a commercial incentive to pursue the resulting technology and bring it to the marketplace. The growing number of awardees, many of them started in business in response to SBIR solicitations, is becoming a significant resource for the solution of high risk, high technology problems for the Department. As detailed here, this publication describes the technical efforts for SBIR Phase 1 awards in 1994. It is intended for the educated layman, and may be of particular interest to potential investors who wish to get in on the ground floor of exciting opportunities. Contained in this booklet are abstracts of the Phase 1 awards made in FY 1994 under the DOE SBIR program. The 212 Phase 1 projects described here were selected in a highly competitive process from a total of 2,276 grant applications received in response to the 1994 DOE annual SBIR Solicitation. The selections for awards were made on scientific and technical merit, as judged against the specific criteria listed in the Solicitation. Conclusions were reached on the basis of detailed reports returned by reviewers drawn from DOE laboratories, universities, private industry, and government. (Any discrepancies noted in prior DOE releases naming the firms selected for awards are due either to the firm changing its name after the award selection or to the firm not proceeding to a signed grant.) It is expected that between one-third and one-half of the Phase 1 projects will be continued into Phase 2. The work described in the abstracts is novel, high-risk research, but the benefits will also be potentially high if the objectives are met. Brief comments on the potential applications are given after each abstract. Individuals and organizations with an interest in the research described are encouraged to contact the appropriate small business directly.

Not Available

1994-12-31T23:59:59.000Z

437

AbstractAbstract Vendors of high performance computers are converging towards an  

E-Print Network [OSTI]

AbstractAbstract Vendors of high performance computers are converging towards an architecture based full advantage of the available computing power, in order to achieve the best scalability.This new of computer time #12;Poloidal Grid: unstructured meshPoloidal Grid: unstructured mesh · Gives uniform

438

Science Education in a Nordic Welfare State Institute of Physics and Astronomy, University of Arhus, DK8000,  

E-Print Network [OSTI]

is no exception. In the 16th century the Danish Astronomer Tycho Brahe was the first to see a supernova (stella on the past, but only notice that already at the time of Tycho Brahe, astronomy was a highly international

Fynbo, Johan

439

Current Abstracts Nuclear Reactors and Technology  

SciTech Connect (OSTI)

This publication Nuclear Reactors and Technology (NRT) announces on a monthly basis the current worldwide information available from the open literature on nuclear reactors and technology, including all aspects of power reactors, components and accessories, fuel elements, control systems, and materials. This publication contains the abstracts of DOE reports, journal articles, conference papers, patents, theses, and monographs added to the Energy Science and Technology Database during the past month. Also included are US information obtained through acquisition programs or interagency agreements and international information obtained through acquisition programs or interagency agreements and international information obtained through the International Energy Agency`s Energy Technology Data Exchange or government-to-government agreements. The digests in NRT and other citations to information on nuclear reactors back to 1948 are available for online searching and retrieval on the Energy Science and Technology Database and Nuclear Science Abstracts (NSA) database. Current information, added daily to the Energy Science and Technology Database, is available to DOE and its contractors through the DOE Integrated Technical Information System. Customized profiles can be developed to provide current information to meet each user`s needs.

Bales, J.D.; Hicks, S.C. [eds.

1993-01-01T23:59:59.000Z

440

IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica  

E-Print Network [OSTI]

The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the "first light" in the nascent field of neutrino astronomy. The observed diffuse neutrino flux seems to suggest a much larger level of hadronic activity in the non-thermal universe than previously thought and suggests a rich discovery potential for a larger neutrino observatory. This document presents a vision for an substantial expansion of the current IceCube detector, IceCube-Gen2, including the aim of instrumenting a $10\\,\\mathrm{km}^3$ volume of clear glacial ice at the South Pole to deliver substantial increases in the astrophysical neutrino sample for all flavors. A detector of this size would have a rich physics program with the goal to resolve the sources of these astrophysical neutrinos, discover GZK neutrinos, and be a leading observatory in future multi-messenger astronomy programs.

IceCube-Gen2 Collaboration; :; M. G. Aartsen; M. Ackermann; J. Adams; J. A. Aguilar; M. Ahlers; M. Ahrens; D. Altmann; T. Anderson; G. Anton; C. Arguelles; T. C. Arlen; J. Auffenberg; S. Axani; X. Bai; I. Bartos; S. W. Barwick; V. Baum; R. Bay; J. J. Beatty; J. Becker Tjus; K. -H. Becker; S. BenZvi; P. Berghaus; D. Berley; E. Bernardini; A. Bernhard; D. Z. Besson; G. Binder; D. Bindig; M. Bissok; E. Blaufuss; J. Blumenthal; D. J. Boersma; C. Bohm; F. Bos; D. Bose; S. BŲser; O. Botner; L. Brayeur; H. -P. Bretz; A. M. Brown; N. Buzinsky; J. Casey; M. Casier; E. Cheung; D. Chirkin; A. Christov; B. Christy; K. Clark; L. Classen; F. Clevermann; S. Coenders; G. H. Collin; J. M. Conrad; D. F. Cowen; A. H. Cruz Silva; J. Daughhetee; J. C. Davis; M. Day; J. P. A. M. de Andrť; C. De Clercq; S. De Ridder; P. Desiati; K. D. de Vries; M. de With; T. DeYoung; J. C. DŪ andaz-Vťlez; M. Dunkman; R. Eagan; B. Eberhardt; T. Ehrhardt; B. Eichmann; J. Eisch; S. Euler; J. J. Evans; P. A. Evenson; O. Fadiran; A. R. Fazely; A. Fedynitch; J. Feintzeig; J. Felde; K. Filimonov; C. Finley; T. Fischer-Wasels; S. Flis; K. Frantzen; T. Fuchs; T. K. Gaisser; R. Gaior; J. Gallagher; L. Gerhardt; D. Gier; L. Gladstone; T. GlŁsenkamp; A. Goldschmidt; G. Golup; J. G. Gonzalez; J. A. Goodman; D. Gůra; D. Grant; P. Gretskov; J. C. Groh; A. GroŖ; C. Ha; C. Haack; A. Haj Ismail; P. Hallen; A. Hallgren; F. Halzen; K. Hanson; J. Haugen; D. Hebecker; D. Heereman; D. Heinen; K. Helbing; R. Hellauer; D. Hellwig; S. Hickford; J. Hignight; G. C. Hill; K. D. Hoffman; R. Hoffmann; A. Homeier; K. Hoshina; F. Huang; W. Huelsnitz; P. O. Hulth; K. Hultqvist; A. Ishihara; E. Jacobi; J. Jacobsen; G. S. Japaridze; K. Jero; O. Jlelati; B. J. P. Jones; M. Jurkovic; O. Kalekin; A. Kappes; T. Karg; A. Karle; T. Katori; U. F. Katz; M. Kauer; A. Keivani; J. L. Kelley; A. Kheirandish; J. Kiryluk; J. Klšs; S. R. Klein; J. -H. KŲhne; G. Kohnen; H. Kolanoski; A. Koob; L. KŲpke; C. Kopper; S. Kopper; D. J. Koskinen; M. Kowalski; C. B. Krauss; A. Kriesten; K. Krings; G. Kroll; M. Kroll; J. Kunnen; N. Kurahashi; T. Kuwabara; M. Labare; J. L. Lanfranchi; D. T. Larsen; M. J. Larson; M. Lesiak-Bzdak; M. Leuermann; J. LoSecco; J. LŁnemann; J. Madsen; G. Maggi; K. B. M. Mahn; S. Marka; Z. Marka; R. Maruyama; K. Mase; H. S. Matis; R. Maunu; F. McNally; K. Meagher; M. Medici; A. Meli; T. Meures; S. Miarecki; E. Middell; E. Middlemas; N. Milke; J. Miller; L. Mohrmann; T. Montaruli; R. W. Moore; R. Morse; R. Nahnhauer; U. Naumann; H. Niederhausen; S. C. Nowicki; D. R. Nygren; A. Obertacke; S. Odrowski; A. Olivas; A. Omairat; A. O'Murchadha; T. Palczewski; L. Paul; ÷. Penek; J. A. Pepper; C. Pťrez de los Heros; C. Pfendner; D. Pieloth; E. Pinat; J. L. Pinfold; J. Posselt; P. B. Price; G. T. Przybylski; J. PŁtz; M. Quinnan; L. Ršdel; M. Rameez; K. Rawlins; P. Redl; I. Rees; R. Reimann; M. Relich; E. Resconi; W. Rhode; M. Richman; B. Riedel; S. Robertson; J. P. Rodrigues; M. Rongen; C. Rott; T. Ruhe; B. Ruzybayev; D. Ryckbosch; S. M. Saba; H. -G. Sander; J. Sandroos; P. Sandstrom; M. Santander; S. Sarkar; K. Schatto; F. Scheriau; T. Schmidt; M. Schmitz; S. Schoenen; S. SchŲneberg; A. SchŲnwald; A. Schukraft; L. Schulte; O. Schulz; D. Seckel; Y. Sestayo; S. Seunarine; M. H. Shaevitz; R. Shanidze; M. W. E. Smith; D. Soldin; S. SŲldner-Rembold; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; N. A. Stanisha; A. Stasik; T. Stezelberger; R. G. Stokstad; A. StŲŖ andl; E. A. Strahler; R. StrŲm; N. L. Strotjohann; G. W. Sullivan; H. Taavola; I. Taboada; A. Taketa; A. Tamburro; H. K. M. Tanaka; A. Tepe; S. Ter-Antonyan; A. Terliuk; G. Teö; andi?; S. Tilav; P. A. Toale; M. N. Tobin; D. Tosi; M. Tselengidou; E. Unger; M. Usner; S. Vallecorsa; N. van Eijndhoven; J. Vandenbroucke; J. van Santen; S. Vanheule; M. Vehring; M. Voge; M. Vraeghe; C. Walck; M. Wallraff; Ch. Weaver; M. Wellons; C. Wendt; S. Westerhoff; B. J. Whelan; N. Whitehorn; C. Wichary; K. Wiebe; C. H. Wiebusch; D. R. Williams; H. Wissing; M. Wolf; T. R. Wood; K. Woschnagg; S. Wren; D. L. Xu; X. W. Xu; Y. Xu; J. P. Yanez; G. Yodh; S. Yoshida; P. Zarzhitsky; J. Ziemann; M. Zoll

2014-12-18T23:59:59.000Z

Note: This page contains sample records for the topic "astronomy department abstract" 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

* TOTT(^/Oi\\ Riso-R-402 Metallurgy Department  

E-Print Network [OSTI]

o o o o 00 U *∑ TOTT(^/Oi\\ Riso-R-402 ^ Metallurgy Department Progress Report for the period l METALLURGY DEPARTMENT PROGRESS REPORT FOR THE PERIOD 1 JANUARY TO 31 DECEMBER 1978 Abstract. The activities of the Metallurgy Department at RisÝ during 1978 are described. The work is presented in four chap- ters: General

442

Department Washington,  

Office of Legacy Management (LM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment ofDepartment ofof EnergyYou$0.C. 20545*. . : '* FEB1 Rev. 0IwellSite:u.s.

443

2013 LIST OF PUBLICATIONS REVIEWED BY PETROLEUM ABSTRACTS Petroleum Abstracts reviews the following publications on a regular basis and selects material for indexing and abstracting according to  

E-Print Network [OSTI]

2013 LIST OF PUBLICATIONS REVIEWED BY PETROLEUM ABSTRACTS Petroleum Abstracts reviews the following was used by Petroleum Abstracts through 2004. Beginning with 2005 issues, the Complete Title is used. TABLE OF CONTENTS SERVICE As a current-awareness service, Petroleum Abstracts Document Delivery Service (PADDS

Reynolds, Albert C.

444

Abstract--Electrocorticogram recordings for neuroprosthetics provide an intermediate level of abstraction between EEG and  

E-Print Network [OSTI]

tasks [5]. Therefore, harnessing both the inputs (dendritic activity) and outputs (action potentials, FL 32610 USA (e-mail: carnepr@peds.ufl.edu). J. C. Principe is with the Department of Electrical and/or field potentials can explain as much as 80 percent of the variance observed in motor control

Slatton, Clint

445

Verification of Parallel Garbage Collection by Abstract Model Checking  

E-Print Network [OSTI]

have a finite state space provided that the abstraction mapping is powerful. M¨uller and Nipkow's work working on abstract model checking. In Section 4, the abstractions we defined on garbage #12; collectionVerification of Parallel Garbage Collection by Abstract Model Checking (Extended Abstract) Masami

Hagiya, Masami

446

DOE NABIR PI Workshop: Abstracts 2002  

SciTech Connect (OSTI)

The mission of the NABIR program is to provide the fundamental science that will serve as the basis for the development of cost-effective bioremediation and long-term stewardship of radionuclides and metals in the subsurface at DOE sites. The focus of the program is on strategies leading to long-term immobilization of contaminants in place to reduce the risk to humans and the environment. Contaminants of special interest are uranium, technetium, plutonium, chromium, and mercury. The focus of the NABIR program is on the bioremediation of these contaminants in the subsurface below the root zone, including both vadose and saturated zones. The program is implemented through four interrelated scientific research elements (Biogeochemistry, Biomolecular Science and Engineering, Biotransformation, and Community Dynamics/Microbial Ecology); and through an element called Bioremediation and its Societal Implications and Concerns (BASIC), which addresses societal issues and potential concerns of stakeholders. The material presented at this year's workshop focuses on approximately 60 research projects funded in FY 2000-2002 by DOE's Office of Biological and Environmental Research (BER). Abstracts of NABIR research projects are provided in this book.

Hawkes (Editor), Dan

2002-01-09T23:59:59.000Z

447

DOE-NABIR PI Workshop: Abstracts 2003  

SciTech Connect (OSTI)

The mission of the NABIR program is to provide the fundamental science that will serve as the basis for the development of cost-effective bioremediation and long-term stewardship of radionuclides and metals in the subsurface at DOE sites. The focus of the program is on strategies leading to long-term immobilization of contaminants in situ to reduce the risk to humans and the environment. Contaminants of special interest are uranium, technetium, plutonium, chromium, and mercury. The focus of the NABIR program is on the bioremediation of these contaminants in the subsurface below the root zone, including both vadose and saturated zones. The program consists of four interrelated Science Elements (Biotransformation, Community Dynamics/Microbial Ecology, Biomolecular Science and Engineering, and Biogeochemistry). The program also has a cross-cutting Assessment Element that supports development of innovative approaches and technologies to support the science elements. An element called Bioremediation and its Societal Implications and Concerns (BASIC) addresses potential societal issues of implementing NABIR scientific findings. The material presented at this year's workshop focuses on approximately 60 research projects funded in FY 2000-2003 by the Environmental Remediation Sciences Division in DOE's Office of Biological and Environmental Research (BER) in the Office of Science. Abstracts of NABIR research projects are provided in this book.

Various

2003-01-28T23:59:59.000Z

448

DEPARTMENT CODE Department of Computer Science  

E-Print Network [OSTI]

DEPARTMENT CODE Department of Computer Science College of Natural Sciences Colorado State and Amendment of this Code 19 #12;1 MISSION AND OBJECTIVES 3 Preamble This Code of the Department of Computer

449

Department Safety Representatives Department Safety Representative  

E-Print Network [OSTI]

Department Safety Representatives Overview Department Safety Representative Program/Operations Guidance Document The Department Safety Representative (DSR) serves a very important role with implementation of safety, health, and environmental programs on campus. The role of the DSR is to assist

Pawlowski, Wojtek

450

Abstracts of Phase 1 awards, (fiscal year) 1987  

SciTech Connect (OSTI)

Contained in this booklet are abstracts of the Phase I awards made in Fiscal Year 1987 under the Small Business Innovation Research (SBIR) program in the Department of Energy (DOE). The program is designed for implementation in a three-phase process, with Phase I determining the scientific or technical merit and feasibility of ideas proposed for investigation. The period of performance in this initial phase is relatively brief, typically about 6 months, and the awards are limited to $50,000. Phase II is the principal research or research and development effort, and the awards are as high as $500,000 for work to be performed in periods of up to 2 years. Phase III is the commercial application. The 111 Phase I projects described were selected in a highly competitive process from a total of 942 proposals received in response to the 1987 Solicitation. They cover the fields of chemistry, materials, control systems, plant natural products, instrumentation, nuclear medicine, health and environmental effects, high energy physics, particle accelerators, nuclear physics, plasma diagnostics and confinement, fusion energy systems, robotics and remote systems, nuclear reactors, space nuclear power, fuel cycle, decontamination/decommissioning, commputers in nuclear plants, coal, enhanced oil recovery/tar sands, fossil energy, photovoltaics, solar thermal, ceramics for heat engines, and industrial separation, conversion and recovery processes. (DLC)

Not Available

1987-01-01T23:59:59.000Z

451

Selected Abstracts & Bibliography of International Oil Spill Research, through 1998  

E-Print Network [OSTI]

Quarterly. 7(3) Energy Research Abstracts. 1987. Spills-of-Energy Daily. 18:139. Energy Research Abstracts. 1987. FieldResponse. 96pp. ERA (Energy Research Abstracts), ETD (Energy

Louisiana Applied Oil Spill Research & Development Program Electronic Bibliography

1998-01-01T23:59:59.000Z

452

Process Abstraction in the Verification of Temporal Properties†  

E-Print Network [OSTI]

as abstraction operations. We show that an abstract process satisfies a property expressed as a temporal logic formula just if the original process satisfies a transformed formula. We define various abstraction operators and illustrate their use in verification...

Bruns, Glen R

453

ABSTRACT: Bioenergy Harvesting Technologies to Supply Crop Residues...  

Energy Savers [EERE]

ABSTRACT: Bioenergy Harvesting Technologies to Supply Crop Residues In a Densified Large Square Bale Format ABSTRACT: Bioenergy Harvesting Technologies to Supply Crop Residues In a...

454

Asymptotic almost-equivalence of abstract evolution systems ?  

E-Print Network [OSTI]

May 13, 2008 ... Abstract. We study the asymptotic behavior of almost-orbits of abstract .... In that sense our work is different but complementary to [12,11].

2008-05-13T23:59:59.000Z

455

abstracting code specific: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Poster: 4195B656 Abstract Title: Specification of Multiple Ganglion Cell Stimulation Codes for Engineering Websites Summary: ProgramPoster: 4195B656 Abstract Title:...

456

Clad Degradation- Summary and Abstraction for LA  

SciTech Connect (OSTI)

The purpose of this model report is to develop the summary cladding degradation abstraction that will be used in the Total System Performance Assessment for the License Application (TSPA-LA). Most civilian commercial nuclear fuel is encased in Zircaloy cladding. The model addressed in this report is intended to describe the postulated condition of commercial Zircaloy-clad fuel as a function of postclosure time after it is placed in the repository. Earlier total system performance assessments analyzed the waste form as exposed UO{sub 2}, which was available for degradation at the intrinsic dissolution rate. Water in the waste package quickly became saturated with many of the radionuclides, limiting their release rate. In the total system performance assessments for the Viability Assessment and the Site Recommendation, cladding was analyzed as part of the waste form, limiting the amount of fuel available at any time for degradation. The current model is divided into two stages. The first considers predisposal rod failures (most of which occur during reactor operation and associated activities) and postdisposal mechanical failure (from static loading of rocks) as mechanisms for perforating the cladding. Other fuel failure mechanisms including those caused by handling or transportation have been screened out (excluded) or are treated elsewhere. All stainless-steel-clad fuel, which makes up a small percentage of the overall amount of fuel to be stored, is modeled as failed upon placement in the waste packages. The second stage of the degradation model is the splitting of the cladding from the reaction of water or moist air and UO{sub 2}. The splitting has been observed to be rapid in comparison to the total system performance assessment time steps and is modeled to be instantaneous. After the cladding splits, the rind buildup inside the cladding widens the split, increasing the diffusion area from the fuel rind to the waste package interior. This model report summarizes the component models, developed for the two stages noted above, that are used as inputs to TSPA-LA. The model concludes that less than two percent of the fuel, including all of the stainless-steel clad fuel, received at the repository is failed (perforated) upon receipt at the repository. All failed fuel is assumed to axially split upon waste package failure exposing the fuel to oxidation from the in-package environment. TSPA-LA then calculates the release of radionuclides from the exposed volume of oxidized fuel.

D. Stahl

2004-10-01T23:59:59.000Z

457

DSNF AND OTHER WASTE FORM DEGRADATION ABSTRACTION  

SciTech Connect (OSTI)

Several hundred distinct types of DOE-owned spent nuclear fuel (DSNF) may potentially be disposed in the Yucca Mountain repository. These fuel types represent many more types than can be viably individually examined for their effect on the Total System Performance Assessment for the License Application (TSPA-LA). Additionally, for most of these fuel types, there is no known direct experimental test data for the degradation and dissolution of the waste form in repository groundwaters. The approach used in the TSPA-LA model is, therefore, to assess available information on each of 11 groups of DSNF, and to identify a model that can be used in the TSPA-LA model without differentiating between individual codisposal waste packages containing different DSNF types. The purpose of this report is to examine the available data and information concerning the dissolution kinetics of DSNF matrices for the purpose of abstracting a degradation model suitable for use in describing degradation of the DSNF inventory in the Total System Performance Assessment for the License Application. The data and information and associated degradation models were examined for the following types of DSNF: Group 1--Naval spent nuclear fuel; Group 2--Plutonium/uranium alloy (Fermi 1 SNF); Group 3--Plutonium/uranium carbide (Fast Flux Test Facility-Test Fuel Assembly SNF); Group 4--Mixed oxide and plutonium oxide (Fast Flux Test Facility-Demonstration Fuel Assembly/Fast Flux Test Facility-Test Demonstration Fuel Assembly SNF); Group 5--Thorium/uranium carbide (Fort St. Vrain SNF); Group 6--Thorium/uranium oxide (Shippingport light water breeder reactor SNF); Group 7--Uranium metal (N Reactor SNF); Group 8--Uranium oxide (Three Mile Island-2 core debris); Group 9--Aluminum-based SNF (Foreign Research Reactor SNF); Group 10--Miscellaneous Fuel; and Group 11--Uranium-zirconium hydride (Training Research Isotopes-General Atomics SNF). The analyses contained in this document provide an ''upper-limit'' (i.e., instantaneous degradation) model for use in the TSPA-LA model. ''Best-estimate'' models for the degradation of the fuels in each of the DSNF groups are discussed to provide a basis for selecting the upper limit model for use in the TSPA-LA model. The instantaneous degradation model is chosen for use in the TSPA-LA model because the available information shows that the degradation rate of the N Reactor fuel (which constitutes most of the DSNF inventory) is very high and because the available qualified information is insufficient to justify use of a less conservative approach. The commercial spent nuclear fuel model will be used for naval spent nuclear fuel because it has been shown to be conservative for representing naval spent nuclear fuel.

J. CUNNANE

2004-11-19T23:59:59.000Z

458

arXiv:1205.5114v1[astro-ph.SR]23May2012 370 Years of Astronomy at Utrecht  

E-Print Network [OSTI]

arXiv:1205.5114v1[astro-ph.SR]23May2012 370 Years of Astronomy at Utrecht ASP Conference Series in eclipse spectra taken in 1973. 1. Utrecht solar physics I spent 50 years in Utrecht astronomy, arriving as a student in the autumn of 1961 and cleaning out my desk at the near-defunct Sterrekundig Instituut Utrecht

Rutten, Rob

459

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

460

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

Note: This page contains sample records for the topic "astronomy department abstract" 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

Formal Proof of Abstract Model Checking of Concurrent Garbage Collection  

E-Print Network [OSTI]

, the correctness of abstraction is not always easy to verify. In our pre- vious work, we applied abstract model with that of proving the concrete system from scratch (not by abstract model checking). In our previous work [6], whichFormal Proof of Abstract Model Checking of Concurrent Garbage Collection Koichi Takahashi Masami

Hagiya, Masami

462

Abstract machines for game semantics, revisited Olle Fredriksson  

E-Print Network [OSTI]

: In this paper we are developing the line of work on PAM/IAM/JAM in order to define new abstract machines whichAbstract machines for game semantics, revisited Olle Fredriksson University of Birmingham, UK Dan R. Ghica University of Birmingham, UK Abstract--We define new abstract machines for game seman- tics which

Ghica, Dan

463

US Department  

Broader source: Energy.gov (indexed) [DOE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarly Career Scientists' Research Petroleum ReserveDepartment of Energy AtNotice forof Energy TheUS

464

Ultra High Energy Cosmic Rays, Z-Shower and Neutrino Astronomy by Horizontal-Upward Tau Air-Showers  

E-Print Network [OSTI]

Ultra High Cosmic Rays (UHECR) Astronomy may be correlated to a primary parental Neutrino Astronomy: indeed any far BL Lac Jet or GRB, sources of UHECR, located at cosmic edges, may send its signal, overcoming the severe GZK cut-off, by help of UHE ZeV energetic neutrino primary. These UHE neutrino scattering on relic light ones (spread on wide Hot Local Groups Halos) maybe fine-tuned : E_(nu) =(M_Z)^2/m_(nu) = 4 10^(22) eV *((0.1eV)/m_(nu)), to combine at once the observed light neutrino masses and the UHECR spectra, leading to a relativistic Z-Shower in Hot Dark Halos (e few tens Mpc wide) whose final nuclear component traces the UHECR event on Earth. Therefore UHECR (with no longer volme GZK constrains) may point to far BL Lac sources. This Z-Burst (Z-Shower) model calls for large neutrino fluxes. Even if Nature do not follow the present Z-model, UHECR while being cut-off by Big Bang Radiation, must produce a minimal UHE neutrino flux, the GZK neutrino secondaries. For both reasons such UHE Neutrino Astronomy must be tested on Earth. Lowest High Energy Astronomy is searched by AMANDA, ANTARES underground deterctors by muons tracks. We suggest a complementary higher energy Neutrino Tau Astronomy inducing Horizontal and Upward Tau AirShowers. Possible early evidence of such a New Neutrino UPTAUs (Upward Tau Showers at PeVs energies) Astronomy may be in BATSE records of Upward Terrestrial Gamma Flashes. Future signals must be found in detectors as EUSO, seeking Upward-Horizontal events: indeed even minimal, guaranteed, GZK neutrino fluxes may be better observed if EUSO threshold reaches 10^(19) eV by enlarging its telescope size.

D. Fargion

2003-06-24T23:59:59.000Z

465

White Paper on the Status and Future of Ground-based Gamma-ray Astronomy  

E-Print Network [OSTI]

In recent years, ground-based gamma-ray observatories have made a number of important astrophysical discoveries which have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical Society has requested the preparation of a white paper on the status and future of ground-based gamma-ray astronomy to define the science goals of the future observatory, to determine the performance specifications, and to identify the areas of necessary technology development. In this contribution we give a brief overview of the activities of the current white paper team and invite the international community to contribute to the white paper.

Krawczynski, H; Byrum, K; Dermer, C; Dingus, B; Falcone, A; Kaaret, Philip; Krennrich, F; Pohl, M; Vasilev, V; Williams, D A

2007-01-01T23:59:59.000Z

466

A fast photon counting camera for {gamma}-ray pulsar astronomy  

SciTech Connect (OSTI)

The Electron Multiplying CCD (EMCCD) astronomical camera, under development at the Institute of Astronomy UNAM, will be able to obtain images of faint optical objects with very low instrumental noise and short integration times. The EMCCD is a normal CCD with an additional multiplication register located before the input of the readout amplifier. This will be a very suitable instrument to search for optical pulsations of unidentified gamma-ray sources, specially with GLAST entering the realm of radio quiet gamma-ray loud pulsars.

Orozco, Benito; Carraminana, Alberto [Inst. Nacional de Astrofisica, Optica y Electronica, Luis Enrique Erro 1, Tonantzintla, Puebla 72840 (Mexico); Michel, Raul; Zazueta, Salvador [Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, A.P. 877, Ensenada, BC 22800 (Mexico); Fordham, John L. A. [Department of Physics and Astronomy, University College London, Gower Street, London (United Kingdom)

2007-07-12T23:59:59.000Z

467

Submm/FIR astronomy in Antarctica: Potential for a large telescope facility  

E-Print Network [OSTI]

Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500 micron regime, i.e. for far-infrared (FIR) and submillimetre (submm) astronomy. We present an overview of potential science cases that could be addressed with a large telescope facility at Dome C. This paper also includes a presentation of the current knowledge about the site characterics in terms of atmospheric transmission, stability, sky noise and polar constraints on telescopes. Current and future site testing campaigns are finally described.

Vincent Minier; V. Minier; L. Olmi; P. -O. Lagage; L. Spinoglio; G. A. Durand; E. Daddi; D. Galilei; H. Gallee; C. Kramer; D. Marrone; E. Pantin; L. Sabbatini; N. Schneider; N. Tothill; L. Valenziano; C. Veyssiere

2008-05-16T23:59:59.000Z

468

White Paper on the Status and Future of Ground-based Gamma-ray Astronomy  

E-Print Network [OSTI]

In recent years, ground-based gamma-ray observatories have made a number of important astrophysical discoveries which have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical Society has requested the preparation of a white paper on the status and future of ground-based gamma-ray astronomy to define the science goals of the future observatory, to determine the performance specifications, and to identify the areas of necessary technology development. In this contribution we give a brief overview of the activities of the current white paper team and invite the international community to contribute to the white paper.

H. Krawczynski; J. Buckley; K. Byrum; C. Dermer; B. Dingus; A. Falcone; P. Kaaret; F. Krennrich; M. Pohl; V. Vassiliev; D. A. Williams; for the White Paper Team

2007-09-05T23:59:59.000Z

469

NEWS RELEASE Contact: John G. Learned, 011-81-578-59-618 EMBARGOED UNTIL Department of Physics and Astronomy  

E-Print Network [OSTI]

of scientists, in collaboration with international partners, announced the first-ever positive identification been conducted because of the inability to access material from deep within the earth

Learned, John

470

Graduate Student Information Department of Physics & Astronomy Wayne State University College of Science Page 1 of 22  

E-Print Network [OSTI]

. Course Registration Requirements and PLAN OF WORK ......... 4 4. Annual Review......................................................................... 6 4. Course Registration Requirements and PLAN OF WORK......... 6 5. Annual Review details, consult with the Graduate Advisor. PHY 8991 will have 1-credit seminars on High Energy

Berdichevsky, Victor

471

On resonant heating below the cyclotron frequency Department of Physics and Astronomy, University of California, Irvine, California 92697  

E-Print Network [OSTI]

, University of California, Irvine, California 92697 Zhihong Lin and Roscoe White Plasma Physics Laboratory of the cyclotron frequency. This result may have relevance for the heating of ions in the solar corona

Lin, Zhihong

472

Directions to Petroleum Abstracts Petroleum Abstracts' main office is located in the basement of John Rogers Hall (JRH)  

E-Print Network [OSTI]

Directions to Petroleum Abstracts Petroleum Abstracts' main office is located in the basement approximately 2 blocks West of South Harvard Avenue. Petroleum Abstracts' office (Room 1520) is on the basement wish to visit Petroleum Abstracts and they will contact us to direct you to our office in the basement

Reynolds, Albert C.

473

Bundle: A Group Based Programming Abstraction for Cyber Physical Systems  

E-Print Network [OSTI]

). Similar to other programming abstractions, a Bun- dle creates logical collections of sensing devices on feedback from the current members. The Bun- dle abstraction is implemented in Java which ensures ease

Stankovic, John A.

474

On the Hardness of Optimal Auctions (Extended Abstract)  

E-Print Network [OSTI]

On the Hardness of Optimal Auctions (Extended Abstract) Amir Ronen #3; Amin Saberi y Abstract We Berkeley. Email: saberi@cc.gatech.edu. problem which is perhaps the most basic in optimal auction design

Saberi, Amin

475

Policy space abstraction for a lifelong learning agent†  

E-Print Network [OSTI]

This thesis is concerned with policy space abstractions that concisely encode alternative ways of making decisions; dealing with discovery, learning, adaptation and use of these abstractions. This work is motivated by ...

Hawasly, Majd

2014-11-27T23:59:59.000Z

476

Division of Environmental Control Technology Program, 1979. [Lead abstract  

SciTech Connect (OSTI)

Separate abstracts were prepared for the 10 sections in this progress report dealing with environmental engineering. (KRM)

None

1980-06-01T23:59:59.000Z

477

NATIONAL RADIO ASTRONOMY OBSERVATORY TITLE: USE OF THE VAX-11 FARANT MICROWAVE DESIGN PROGRAM FROM GREEN BANK  

E-Print Network [OSTI]

NATIONAL RADIO ASTRONOMY OBSERVATORY TITLE: USE OF THE VAX-11 FARANT MICROWAVE DESIGN PROGRAM FROM #12;USE OF THE VAX-il FARANT MICROWAVE DESIGN PROGRAM FROM GREEN BANK R. Norrod Recently, I have learned to use the FARANT microwave analysis and optimization program which resides on the VAX-11 in CV

Groppi, Christopher

478

The Universe Viewed in Gamma-Rays 1 Summary Talk: The Status of VHE Astronomy c2002  

E-Print Network [OSTI]

, the review will obviously be somewhat subjective. VHE gamma-ray astronomy came of age in the 1990's [2 measurements of energy spectra and flux variability were routine for the stronger sources. The last decade also-ray telescopes took place in a series of meetings entitled Towards a Major Atmospheric Cherenkov Detector

Enomoto, Ryoji

479

Astronomy 203/203W/403: astronomical instruments and techniques This document is available on the World Wide Web, at  

E-Print Network [OSTI]

is available on the World Wide Web, at http://www.pas.rochester.edu/~dmw/ast203/Syllabus.htm . Astronomy 203 and Lomb, 275-8576; lab: 485 Bausch and Lomb, 275-7162; Internet: dmw@isis.pas.rochester.edu; home page: http://www.pas.rochester.edu/~dmw/ . World Wide Web site: http://www.pas.rochester.edu/~dmw/ast203

480

COMPUTER SCIENCE EECS Department  

E-Print Network [OSTI]

COMPUTER SCIENCE EECS Department The Electrical Engineering and Computer Science (EECS) Department at WSU offers undergraduate degrees in electrical engineering, computer engineering and computer science. The EECS Department offers master of science degrees in computer science, electrical engineering

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to obtain the most current and comprehensive results.


481

ELECTRICAL ENGINEERING EECS Department  

E-Print Network [OSTI]

ELECTRICAL ENGINEERING EECS Department The Electrical Engineering and Computer Science (EECS) Department at WSU offers undergraduate degrees in electrical engineering, computer engineering and computer science. The EECS Department offers master of science degrees in computer science, electrical engineering

482

Mechanical engineering Department Seminar  

E-Print Network [OSTI]

and the Department of Mechanical Engineering Tufts University Retooling Our Energy Ecosystem: challengesMechanical engineering Department Seminar Robert J. Hannemann The Gordon Institute and Chair of the Tufts Department of Mechanical Engineering. His technical and academic interests

483

COMPUTER ENGINEERING EECS Department  

E-Print Network [OSTI]

COMPUTER ENGINEERING EECS Department The Electrical Engineering and Computer Science (EECS) Department at WSU offers undergraduate degrees in electrical engineering, computer engineering and computer science. The EECS Department offers Master of Science degrees in computer science, electrical engineering

484

Department of Biomedical Engineering  

E-Print Network [OSTI]

Department of Biomedical Engineering Undergraduate Studies Manual 2010­2011 #12;Biomedical Engineering Undergraduate Advising Manual 2010 | 1 Introduction 2 Biomedical Engineering at Washington University 4 Career Opportunities 6 Department Mission & Objective 7 Department of Biomedical Engineering 8

Stormo, Gary

485

Departement Umweltwissenschaften Department of Environmental Sciences  

E-Print Network [OSTI]

Departement Umweltwissenschaften Department of Environmental Sciences Environmental Sciences .......................................................................10 3 The impact of Environmental Sciences graduates on Swiss economy, public administration.............................................................................................................................................. 15 3.1 Four statements on the impact of Environmental Sciences graduates on Swiss economy, public

Fischlin, Andreas

486

Invited Editorial Manually structured digital abstracts: A scaffold for automatic  

E-Print Network [OSTI]

in the publication process, and authors will then use this out- put as a starting point to shape the digital abstractInvited Editorial Manually structured digital abstracts: A scaffold for automatic text mining In the past, we have advocated the adoption of the struc- tured digital abstract to bring scientific

Gerstein, Mark

487

The Impact of Distributed Programming Abstractions on Application Energy Consumption  

E-Print Network [OSTI]

The Impact of Distributed Programming Abstractions on Application Energy Consumption Young-Woo Kwon of their energy consumption patterns. By varying the abstractions with the rest of the functionality fixed, we measure and analyze the impact of distributed programming abstractions on application energy consumption

Tilevich, Eli

488

A certifying frontend for (sub)polyhedral abstract domains  

E-Print Network [OSTI]

of the overall abstract domain. The main contribution of the work described here is the design of the linkA certifying frontend for (sub)polyhedral abstract domains Alexis Fouilhe and Sylvain Boulmé Univ. Grenoble-Alpes, VERIMAG, F-38000 Grenoble, France {alexis.fouilhe,sylvain.boulme}@imag.fr Abstract. Convex

Paris-Sud XI, Université de

489

No. ___________ Reviewer: ______________________________ 2014 WSU Academic Showcase Abstract Evaluation Rubric  

E-Print Network [OSTI]

, or student A student-submitted abstract has either a faculty co-author or a faculty Sponsor All work mustNo. ___________ Reviewer: ______________________________ 2014 WSU Academic Showcase Abstract Evaluation Rubric Eligibility Criteria1 Does not meet criteria Abstract is submitted by a WSU faculty, staff

Collins, Gary S.

490

Abstract Local Reasoning for Concurrent Libraries: Mind the Gap  

E-Print Network [OSTI]

considerable work on combining lo- cal reasoning with abstraction. There are two main approaches. One approach, truly abstract reasoning of a tree module (such as DOM) works with predicates based on connecting treeMFPS 2014 Abstract Local Reasoning for Concurrent Libraries: Mind the Gap Philippa Gardner, Azalea

Gardner, Philippa

491

From Abstract to Concrete Norms in Agent Institutions  

E-Print Network [OSTI]

From Abstract to Concrete Norms in Agent Institutions Davide Grossi and Frank Dignum Utrecht accounts for how (abstract) norms can be incorporated in the (concrete) procedures constituting. This abstract is organized as follows. In Section 2 we make the problem we are focusing on concrete by means

Dignum, Frank

492

State of Alaska Department of Transportation and Public Facilities...  

Open Energy Info (EERE)

search OpenEI Reference LibraryAdd to library Form: State of Alaska Department of Transportation and Public Facilities - Utility Permit Abstract This document is an example of a...

493

Kentucky Department of Agriculture  

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

Kentucky Department Kentucky Department of Agriculture of Agriculture Motor Fuel and Pesticide Motor Fuel and Pesticide Testing Laboratory Testing Laboratory Introduction...

494

Mechanical engineering Department Seminar  

E-Print Network [OSTI]

Research Center. Currently he is an Assistant Prof. in the Aerospace and Ocean Engineering DepartmentMechanical engineering Department Seminar Cornel Sultan Virginia Tech Design for Control

495

Poster Abstract: Community Sensor Grids Deployment and Usage  

E-Print Network [OSTI]

and Informatics Arizona State University Tempe, AZ 85287 partha@asu.edu Amiya Bhattacharya Department of Computer Science New Mexico State University Las Cruces, NM 88003 amiya@nmsu.edu Meddage S. Fernando Department is that individuals or small community agencies may deploy sensors to cover their own property, but also make them

Bhattacharya, Amiya

496

Search Results Cite abstracts as Author(s) (2010), Title, Abstract xxxxx-xxxx presented at 2010 Fall  

E-Print Network [OSTI]

2010 Fall Meeting Search Results Cite abstracts as Author(s) (2010), Title, Abstract xxxxx will present results on the scaling of reconnection rate with S, as well as turbulence levels. This work

Ng, Chung-Sang

497

Baltic Astronomy,  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth (AOD)ProductssondeadjustsondeadjustAboutScience ProgramBackground High Energy Physics (HEP)BaerstronglyBaltic

498

On Optimal Inverters Department of Computer Science  

E-Print Network [OSTI]

On Optimal Inverters Yijia Chen Department of Computer Science Shanghai Jiaotong University yijia.flum@math.uni­freiburg.de Abstract Leonid Levin showed that every algorithm computing a function has an optimal inverter. Recently. An inverter I of F is an algorithm that for all y in the range of F computes a preimage I(y) of y, i.e., F

Chen, Yijia

499

On Optimal Inverters Department of Computer Science  

E-Print Network [OSTI]

On Optimal Inverters Yijia Chen Department of Computer Science Shanghai Jiaotong University yijia.flum@math.uni-freiburg.de Abstract Leonid Levin showed that every algorithm computing a function has an optimal inverter. Recently. An inverter I of F is an algorithm that for all y in the range of F computes a preimage I(y) of y, i.e., F

Chen, Yijia

500

Brock University Department of Computer Science  

E-Print Network [OSTI]

;Abstract Passive solar building design is the process of designing a building while considering sunlight exposure for receiving heat in winter and rejecting heat in summer. The main goal of a passive solarBrock University Department of Computer Science Passive Solar Building Design Using Genetic