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1

Jefferson Lab | Jefferson Lab  

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

News item slideshow News item slideshow Final Piece Final Piece Workers install a section of the pre-shower calorimeter, or PCAL, which is part of the CLAS12 detector package in Jefferson Lab's Experimental Hall B. The new equipment is being installed for the 12 GeV Upgrade project. <<< Installation of PCAL in Hall B. Upgraded Detector Upgraded Detector Work on the 12 GeV Upgrade project continues at Jefferson Lab. Shown here is the new CLAS12 detector in Experimental Hall B after the recent installation of the pre-shower calorimeter, or PCAL. <<< Installation work on Hall B detector. Neutron Stopper Neutron Stopper Jefferson Lab engineer Paul Brindza holds up samples of a new system of concrete products designed to stop neutrons and other particles from harming sensitive scientific computers and detectors. The new system was

2

Jefferson Lab Technology Transfer  

For more information about Intellectual Property and Inventions, please see the Jefferson Lab Employee Handbook, the Jefferson Lab Administrative ...

3

Jefferson Lab Coloring Book  

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

Programs and Events Search Education Privacy and Security Notice Jefferson Lab Coloring Book The Jefferson Lab Coloring Book, Quarks - More Than Meets the Eye, was written to help...

4

Jefferson Lab Treasure Hunt  

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

Jefferson Lab Treasure Hunt Students tour Jefferson Lab's site while searching for answers to challenging questions. Teacher Overview Download this Activity Lab Pages Questions...

5

Jefferson Lab Contract to be Awarded to Jefferson Science Associates...  

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

Awarded to Jefferson Science Associates, LLC for Management and Operation of World-Class Office of Science Laboratory Jefferson Lab Contract to be Awarded to Jefferson Science...

6

Jefferson Lab Technology Transfer  

What is Technology Transfer at Jefferson Lab? The transfer of technology (intellectual property) developed at JLab to the private sector is an ...

7

Jefferson Lab Technology Transfer  

Tool for Breast Cancer Research - Reducing the need for Biopsy. ... Jefferson Lab is a Department of Energy national laboratory for nuclear physics re ...

8

Jefferson Lab Technology Transfer  

List the name (s) of Thomas Jefferson National Accelerator Facility's technology of interest: * Does any foreign entity (company, person, ... Select license type:

9

Jefferson Lab Coloring Book  

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

Programs and Events Search Education Privacy and Security Notice Jefferson Lab Coloring Book Use the multi-colored crayon on the left-hand side of the screen to select a color....

10

Jefferson Lab's Open House  

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

Currently, the date for Jefferson Lab's next Open House hasn't been announced. If you would like to be notified when a date has been set, you can subscribe to the Science Education...

11

The BEAMS Program at Jefferson Lab  

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

the Thomas Jefferson National Accelerator Facility and Newport News City Public Schools The Thomas Jefferson National Accelerator Facility (Jefferson Lab) is a U.S....

12

Science Education at Jefferson Lab  

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

regional and national education community. Jefferson Lab's long-term commitment to science education continues to focus on increasing the number and quality of undergraduate...

13

Undergraduate Research at Jefferson Lab  

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

As a Department of Energy National Lab, Jefferson Lab has a responsibility to help train the next generation of scientists. See the research projects students participating in the...

14

Jefferson Lab Technology Transfer - JLab  

What is Technology Transfer at Jefferson Lab? The transfer of technology (intellectual property) developed at JLab to the private sector is an important element of ...

15

SF6 Emissions Management at Jefferson Lab  

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

SF 6 Emissions Management at Jefferson Lab Kevin Jordan PE Jefferson Lab November 16, 2010 Emissions Management Overview * SF 6 Gas Usage * SF 6 Transfer System * Remote Cesiator *...

16

Jefferson Lab Treasure Hunt - Teacher Overview  

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

a chance to see more of Jefferson Lab. Objectives: In this activity students will: - tour Jefferson Lab - collect information to answer questions in the BEAMS Lab Book Notes: -...

17

Marshall Newton  

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

Marshall D. Newton Marshall D. Newton Senior Chemist Emeritus Chemistry Department Building 555 Brookhaven National Laboratory P.O. Box 5000 Upton, NY 11973-5000 Phone: (631) 344-4366 FAX: (631) 344-5815 e-mail Marshall D. Newton Named Senior Scientist Emeritus Thermal, Photo- and Radiation-Induced Reactions in Condensed Media Injection of Electrons and Holes into Nanostructures RESEARCH INTERESTS Mechanistic analysis of electron transfer kinetics: thermal and photoinitiated; intra- and intermolecular; homogeneous and interfacial. Calculation of nonequilibrium solvation thermodynamics for electron transfer ( free energies and entropies) using quantum chemical techniques, molecular-level force fields, and dielectric continuum models. Formulation of compact electronic state spaces for modeling electron transfer, using optical spectroscopic data

18

Neutron Transversity at Jefferson Lab  

SciTech Connect

Nucleon transversity and single transverse spin asymmetries have been the recent focus of large efforts by both theorists and experimentalists. On-going and planned experiments from HERMES, COMPASS and RHIC are mostly on the proton or the deuteron. Presented here is a planned measurement of the neutron transversity and single target spin asymmetries at Jefferson Lab in Hall A using a transversely polarized {sup 3}He target. Also presented are the results and plans of other neutron transverse spin experiments at Jefferson Lab. Finally, the factorization for semi-inclusive DIS studies at Jefferson Lab is discussed.

Jian-Ping Chen; Xiaodong Jiang; Jen-chieh Peng; Lingyan Zhu

2005-09-07T23:59:59.000Z

19

Citing NEWTON!  

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

NEWTON Ask A Scientist program is not copyrighted formally. However, in any written work, a citation should be given to validate and give credence to the written work as well as credit the source of information. NEWTON Ask A Scientist program is not copyrighted formally. However, in any written work, a citation should be given to validate and give credence to the written work as well as credit the source of information. The best approach should follow the suggested formats below: MLA Format: APA Format: The MLA Style includes these components: Author's name. Title of document. Online posting date. Online posting. Name of the forum. Date of access ‹URL›. MLA Example: Trach, Bob. "What Is Nanotechnology?" Online posting. 19 Sept. 2003. NEWTON Ask a Scientist. 10 Jan. 2010 ‹http://www.newton.dep.anl.gov /askasci/chem03/chem03104.htm›. The APA Style includes these components: Author's name. (date of posting). Title of document. Message posted to URL

20

2013 Annual Planning Summary for the Thomas Jefferson Site Office...  

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

Thomas Jefferson Site Office 2013 Annual Planning Summary for the Thomas Jefferson Site Office 2013 Annual Planning Summary for the Thomas Jefferson Site Office The ongoing and...

Note: This page contains sample records for the topic "newton orange jefferson" 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

Thomas Jefferson National Accelerator Facility  

Science Conference Proceedings (OSTI)

The Thomas Jefferson National Accelerator Facility (Jefferson Lab) in Newport News, Virginia, USA, is one of ten national laboratories under the aegis of the Office of Science of the U.S. Department of Energy (DOE). It is managed and operated by Jefferson Science Associates, LLC. The primary facility at Jefferson Lab is the Continuous Electron Beam Accelerator Facility (CEBAF) as shown in an aerial photograph in Figure 1. Jefferson Lab was created in 1984 as CEBAF and started operations for physics in 1995. The accelerator uses superconducting radio-frequency (srf) techniques to generate high-quality beams of electrons with high-intensity, well-controlled polarization. The technology has enabled ancillary facilities to be created. The CEBAF facility is used by an international user community of more than 1200 physicists for a program of exploration and study of nuclear, hadronic matter, the strong interaction and quantum chromodynamics. Additionally, the exceptional quality of the beams facilitates studies of the fundamental symmetries of nature, which complement those of atomic physics on the one hand and of high-energy particle physics on the other. The facility is in the midst of a project to double the energy of the facility and to enhance and expand its experimental facilities. Studies are also pursued with a Free-Electron Laser produced by an energy-recovering linear accelerator.

Joseph Grames, Douglas Higinbotham, Hugh Montgomery

2010-09-01T23:59:59.000Z

22

Jefferson Offshore | Open Energy Information  

Open Energy Info (EERE)

Jefferson Offshore Jefferson Offshore Facility Jefferson Offshore Sector Wind energy Facility Type Offshore Wind Facility Status Proposed Owner Coastal Point Energy LLC Developer Coastal Point Energy LLC Location Gulf of Mexico TX Coordinates 29.568°, -93.957° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.568,"lon":-93.957,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

23

Teacher Night at Jefferson Lab  

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

Night at Jefferson Lab Night at Jefferson Lab Region II Physical Science Teacher Night for Elementary and Middle School Teachers April 2nd, 2014 6:30 pm - 8:00 pm Come for the FUN! You won't want to miss the annual Virginia Region II Teacher Night at Jefferson Lab! This year's focus is on physical science activities for upper elementary and middle school teachers. Format for the Evening Think of a Science Fair with enthusiactic students lined up at tables waiting to show you their projects... Teacher Night will be similar, except enthusiactic teachers will be waiting to share one of their favorite classroom activities with YOU! All teachers will have handouts and many will have starter supplies to accompany the handouts - that's right, FREE MATERIALS! Activity Topics Friction - Electrolysis - Water Cycle - Engineering Design Challenge -

24

What's used to steer Jefferson Lab's...  

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

What's used to steer Jefferson Lab's electron beam? Although it may not look like it at first, the Jefferson Lab accelerator really works much like your TV set. Electrons are...

25

Osage Orange Mulch  

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

Osage Orange Mulch Name: David Location: NA Country: NA Date: NA Question: Can wood chips from hedge trees (osage orange) be used as mulch in the garden? I know that the wood...

26

Independent Oversight Inspection, Thomas Jefferson National Accelerator  

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

Thomas Jefferson National Thomas Jefferson National Accelerator Facility - August 2008 Independent Oversight Inspection, Thomas Jefferson National Accelerator Facility - August 2008 August 2008 Inspection of Environment, Safety and Health Programs at the Thomas Jefferson National Accelerator Facility The U.S. Department of Energy (DOE) Office of Independent Oversight, within the Office of Health, Safety and Security (HSS), inspected environment, safety, and health (ES&H) programs at the DOE Thomas Jefferson Site Office (TJSO) and the Thomas Jefferson National Accelerator Facility (TJNAF) during May through July 2008. The ES&H inspection was performed by Independent Oversight's Office of Environment, Safety and Health Evaluations. In coordination with TJSO, TJNAF has taken a number of actions to develop a

27

Jefferson Lab Contract to be Awarded to Jefferson Science Associates, LLC  

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

Jefferson Lab Contract to be Awarded to Jefferson Science Jefferson Lab Contract to be Awarded to Jefferson Science Associates, LLC for Management and Operation of World-Class Office of Science Laboratory Jefferson Lab Contract to be Awarded to Jefferson Science Associates, LLC for Management and Operation of World-Class Office of Science Laboratory April 12, 2006 - 10:17am Addthis OAK RIDGE , TN - The U.S. Department of Energy has selected Jefferson Science Associates, LLC, as the contractor for management and operation of the Thomas Jefferson National Accelerator Facility. The contract, which has a potential value of $2 billion, becomes effective on April 17, 2006. "We have selected the team that we believe is best equipped to lead this important Office of Science laboratory for the department, and we look

28

High School Research at Jefferson Lab  

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

As a Department of Energy National Lab, Jefferson Lab has a responsibility to help train the next generation of scientists. See the research projects students participating in the...

29

Thomas Jefferson National Accelerator Facility Technologies ...  

Jefferson Lab also conducts a variety of research using its Free-Electron Laser, which is based on the same electron-accelerating technology used in CEBAF.

30

The NEWTON Archive  

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

Now you can with our general search page Type in your question below, and see what a google search would return. Then, at the top, click NEWTON Search to see what a NEWTON...

31

Electroweak Physics at Jefferson Lab  

SciTech Connect

The Continuous Electron Beam Accelerator Facility (CEBAF) at the Thomas Jefferson National Accelerator Facility provides CW electron beams with high intensity, remarkable stability, and a high degree of polarization. These capabilities offer new and unique opportunities to search for novel particles and forces that would require extension of the standard model. CEBAF is presently undergoing an upgrade that includes doubling the energy of the electron beam to 12 GeV and enhancements to the experimental equipment. This upgraded facility will provide increased capability to address new physics beyond the standard model.

R. D. McKeown

2012-03-01T23:59:59.000Z

32

Thomas Jefferson High School for Science & Technology National...  

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

Thomas Jefferson High School for Science & Technology National Science Bowl Champion Thomas Jefferson High School for Science & Technology National Science Bowl Champion May 2,...

33

Vascular Flora of the Rocky Flats Area, Jefferson County, Colorado...  

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

Vascular Flora of the Rocky Flats Area, Jefferson County, Colorado, USA Vascular Flora of the Rocky Flats Area, Jefferson County, Colorado, USA August 2010 Jody K. Nelson Vascular...

34

Jefferson Utilities | Open Energy Information  

Open Energy Info (EERE)

Jefferson Utilities Jefferson Utilities Place Wisconsin Utility Id 9690 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes ISO MISO Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Cp-1 Small Power Service between 50kW and 200kW Demand with Parallel Generation(20kW or less) Industrial Cp-1 Small Power Service between 50kW and 200kW Demand Industrial Cp-1 TOD Small Power Service between 50kW and 200kW Demand Optional Time-of-Day Service 7am-9pm with Parallel Generation(20kW or less) Industrial Cp-1 TOD Small Power Service between 50kW and 200kW Demand Optional

35

JeffersonSTM09.ppt  

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

AOS: Measurements of Aerosol Optical and AOS: Measurements of Aerosol Optical and AOS: Measurements of Aerosol Optical and Cloud-forming Properties Cloud-forming Properties Anne Jefferson and John Ogren NOAA Environmental Science Research Laboratory CIRES, University of Colorado ARM STM 2009 Aerosol Observing Systems In-situ surface measurements of aerosol optical, chemical, size, hygroscopic and cloud-forming properties * SGP - ARM central facility Lamont, OK *AMF - Pt Reyes, CA 3/2005 - 9/2005 - Niamey, Niger 12/2005-1/2007 - Murg Valley, Germany 4/2007 -1/2008 - Shouxian China 5/2008 - 12/2008 - Graciosa Island, Azores 4/2009 *BRW/NSA - Barrow Alaska *AMF2 ? Darwin? - What instruments support the science? AMF deployment in Shouxian China, HFE HFE was located at a rural, agricultural area ~120 km from Hefei, ~200 km from Nanking

36

Marshall D. Newton Publications  

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

Marshall D. Newton Marshall D. Newton Recent Publications 138. Modeling Donor/Acceptor Interactions: Combined Roles of Theory and Computation M. D. Newton Int. J. Quant. Chem. 77, 255-263 (2000) 139. Estimation of Electron Transfer Distances from AM1 Calculations S. F. Nelson and M. D. Newton J. Phys. Chem. A104, 10023-31 (2000) 140. An Informative Subtlety of Temperature-Jump or Coulostatic Responses for Surface-Attached Species J. F. Smalley, M. D. Newton and S. W. Fledberg Electrochem. Commun. 2, 832-38 (2000) 141. Electron Transfer: Theoretical Models and Computational Implementation M. D. Newton In Electron Transfer in Chemistry, Vol I, Ed., V. Balzani .; Wiley-VCH Verlag GmbH: Weinhein, Germany, 2001, p3 142. Adiabatic Interfacial Electron Transfer over 26 Å through

37

Math and Science Activities from Jefferson Lab  

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

BEAMS is a program in which classes of 6th, 7th and 8th grade students are exposed to the scientific environment of Jefferson Lab. For five consecutive days during school hours, classes of 6th grade students and their teachers participate in science and math activities conducted with Jefferson Lab staff. The students return to the lab in the 7th and 8th grades for additional activities which reinforce their 6th grade experience. Feel free to copy and alter these activities for use in your class. 6th Grade Background Materials Vocabulary List What is Matter? What is Jefferson Lab? Careers at Jefferson Lab Periodic Table of Elements Puzzles and Games BEAMS Word Search Element Word Search Geometry Word Search BEAMS Bingo Element Bingo BEAMS Crossword Puzzle BEAMS Cryptograph

38

The NEWTON Archive  

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

NEWTON Ask-A-Scientist - Archive Search NEWTON Ask-A-Scientist - Archive Search * If you need help with web-engine searching practices, please see our hints below. Loading... Please wait... * Want to do a general web search and compare with NEWTON, please click here! Archive Areas by Subject Astronomy Archive Astronomy Botany Archive Botany Chemistry Archive Chemistry Computer Science Archive Computer Science Engineering Archive Engineering Environmental and Earth Science Archive Environmental and Earth Science General Science Archive General Science Topics Material Science Archive Material Science Mathematics Archive Mathematics Molecular Biology Archive Molecular Biology Physics Archive Physics Veterinary Science Archive Veterinary Science Weather Archive Weather Zoology Archive Zoology

39

Jefferson Power Biomass Facility | Open Energy Information  

Open Energy Info (EERE)

Biomass Facility Biomass Facility Jump to: navigation, search Name Jefferson Power Biomass Facility Facility Jefferson Power Sector Biomass Owner Jefferson Power LLC Location Monticello, Florida Coordinates 30.5452022°, -83.8701636° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.5452022,"lon":-83.8701636,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

40

Marshall D. Newton  

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

Marshall D. Newton Marshall D. Newton Picture of Marshall D. Newton Senior Chemist Mechanistic analysis of electron transfer kinetics: thermal and photoinitiated; intra- and intermolecular; homogeneous and interfacial. Calculation of nonequilibrium solvation thermodynamics for electron transfer ( free energies and entropies) using quantum chemical techniques, molecular-level force fields, and dielectric continuum models. Formulation of compact electronic state spaces for modeling electron transfer, using optical spectroscopic data Telephone #: (631) 344-4366 newton@bnl.gov B.A. Dartmouth College, 1961; M.A. Dartmough College, 1963; Ph.D. Harvard University, 1966 NSF Postdoctoral Fellow, Oxford University, Oxford, England, 1966-67; NIH Postdoctoral Fellow, Carnegie-Mellon University, Pittsburgh, PA, 1967-68;

Note: This page contains sample records for the topic "newton orange jefferson" 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

Causal Newton Gravity Law  

E-Print Network (OSTI)

The equations of the relativistic causal Newton gravity law for the planets of the solar system are studied in the approximation when the Sun rests at the coordinates origin and the planets do not iteract between each other.

Yury M. Zinoviev

2012-01-17T23:59:59.000Z

42

JEFFERSON LAB HIGH SCHOOL SUMMER HONORS PROGRAM Application Procedure  

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

JEFFERSON LAB HIGH SCHOOL SUMMER HONORS PROGRAM JEFFERSON LAB HIGH SCHOOL SUMMER HONORS PROGRAM Application Procedure Dear Student Applicant: To be eligible to participate in the Jefferson Lab High School Summer Honors Program, you must attend a local high school (within 60 miles of Jefferson Lab), be at least 16 years old by the start date of the program, be in good academic standing, and maintain at least a 3.3 grade point average. Students who are selected to participate in the Jefferson Lab High School Summer Honors Program are chosen on the basis of demonstrated skills and merit. Dependents of Jefferson Lab employees are not eligible for this program. The 2014 Jefferson Lab High School Summer Honors Program begins on June 23, 2014 and concludes on August 1, 2014. To apply to the Jefferson Lab High School Summer Honors Program, follow the

43

Jefferson Lab Guided Tour - What is an accelerator?  

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

What is an accelerator? Welcome to Jefferson Lab Why was Jefferson Lab built? How do scientists study quarks? What is an accelerator? How does the accelerator work? Why use...

44

Jefferson Lab Guided Tour - How does the accelerator work?  

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

How does the accelerator work? Welcome to Jefferson Lab Why was Jefferson Lab built? How do scientists study quarks? What is an accelerator? How does the accelerator work? Why use...

45

2012 Annual Planning Summary for Thomas Jefferson Site Office  

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

The ongoing and projected Environmental Assessments and Environmental Impact Statements for 2012 and 2013 within Thomas Jefferson Site Office.

46

UNITED STATES DEPARTMENT OF ENERGY (DOE) THOMAS JEFFERSON NATIONAL ACCELERATOR FACILITY (JEFFERSON LAB)  

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

- 2014 JSAT Application Package - 2014 JSAT Application Package Page 1 of 6 UNITED STATES DEPARTMENT OF ENERGY (DOE) THOMAS JEFFERSON NATIONAL ACCELERATOR FACILITY (JEFFERSON LAB) JLAB SCIENCE ACTIVITIES FOR TEACHERS (JSAT) ATTENTION ALL 5 th , 6 th AND 8 th GRADE MIDDLE SCHOOL SCIENCE TEACHERS! THIS PROGRAM IS FOR YOU! What is it? JSAT is an after school program for 5 th , 6 th and 8 th grade science teachers designed to build teachers' skills in the physical sciences, funded by the Jefferson Science Associates Initiatives Fund. What will I do? The 2013-2014 program will include interactive activities to enhance physical science instruction at the middle school level and lectures by Jefferson Lab staff on the applications of science. And, yes, teachers WILL receive class sets of some activities!

47

Nucleon spin structure at Jefferson Lab  

Science Conference Proceedings (OSTI)

In the past decade an extensive experimental program to measure the spin structure of the nucleon has been carried out in the three halls at Jefferson Lab. Using a longitudinally polarized beam scattering off longitudinally or transversely polarized 3 He NH 3 and ND 3 targets

The CLAS collaboration

2011-01-01T23:59:59.000Z

48

Baryon spectroscopy with CLAS at Jefferson Lab  

Science Conference Proceedings (OSTI)

A substantial part of the experimental efforts at the experimental Hall-B of Jefferson Laboratory is dedicated to this studies of light baryon spectroscopy. In this report a general overview of the experimental capabilities in the Experimental Hall-B will be presented together with preliminary results of recent double polarization measurements and finally overall status of the program.

Eugene Pasyuk, CLAS Collaboration

2012-04-01T23:59:59.000Z

49

Petabyte Class Storage at Jefferson Lab (CEBAF)  

E-Print Network (OSTI)

By 1997, the Thomas Jefferson National Accelerator Facility will collect over one Terabyte of raw information per day of Accelerator operation from three concurrently operating Experimental Halls. When post-processing is included, roughly 250 TB of raw and formatted experimental data will be generated each year. By the year 2000, a total of one Petabyte will be stored on-line.

Rita Chambers Mark; Mark Davis

1996-01-01T23:59:59.000Z

50

12 GeV Upgrade | Jefferson Lab  

NLE Websites -- All DOE Office Websites

Science Science A Schematic of the 12 GeV Upgrade The 12 GeV Upgrade will greatly expand the research capabilities of Jefferson Lab, adding a fourth experimental hall, upgrading existing halls and doubling the power of the lab's accelerator. A D D I T I O N A L L I N K S: 12 GeV Home Public Interest Scientific Opportunities Hall D Status Updates Contacts Three-Year Accelerator Schedule 2014 - 2016 top-right bottom-left-corner bottom-right-corner 12 GeV Upgrade Physicists at Jefferson Lab are trying to find answers to some of nature's most perplexing questions about the universe by exploring the nucleus of the atom. Their goal is to answer such questions as: "What is the universe made of?" and "What holds everyday matter together?" In their search for answers, physicists smash electrons into atoms using

51

Overview of Nuclear Physics at Jefferson Lab  

E-Print Network (OSTI)

The Continuous Electron Beam Accelerator Facility (CEBAF) and associated experimental equipment at Jefferson Lab comprise a unique facility for experimental nuclear physics. This facility is presently being upgraded, which will enable a new experimental program with substantial discovery potential to address important topics in nuclear, hadronic, and electroweak physics. Further in the future, it is envisioned that the Laboratory will evolve into an electron-ion colliding beam facility.

R. D. McKeown

2013-03-26T23:59:59.000Z

52

Overview of Nuclear Physics at Jefferson Lab  

E-Print Network (OSTI)

The Continuous Electron Beam Accelerator Facility (CEBAF) and associated experimental equipment at Jefferson Lab comprise a unique facility for experimental nuclear physics. This facility is presently being upgraded, which will enable a new experimental program with substantial discovery potential to address important topics in nuclear, hadronic, and electroweak physics. Further in the future, it is envisioned that the Laboratory will evolve into an electron-ion colliding beam facility.

McKeown, R D

2013-01-01T23:59:59.000Z

53

Newton.mws - CECM  

E-Print Network (OSTI)

The su m of these two is 1/6 of a circle with radius=1/2 which has area 1/6 ...... 6 "" 1 "" {TEXT -1 51 "Newton: \\+ 1/2*3^(1/2) term 3 -781250000000000" }}{PARA 6...

54

The Future of Mr. Jefferson's Laboratory (nee CEBAF)  

E-Print Network (OSTI)

We present one viewpoint plus some general information on the plans for energy upgrades and physics research at the Jefferson Laboratory.

Carl E. Carlson

1997-01-27T23:59:59.000Z

55

EA-1937: Pacific Direct Intertie Upgrade Project, Lake, Jefferson...  

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

Lake, Jefferson, Crook, Deschutes, and Wasco Co, OR SUMMARY This project would replace aging equipment at BPA's Celilo converter station and to upgrade equipment on the...

56

Abstract for William Newton  

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

Newton Newton Texas A&M University - Commerce The physics and observational consequences of the neutron star crust-core boundary layer A neutron star, of order 10km in radius, is believed to have a mostly solid outer layer, the crust, about 1km thick, and a fluid core comprising the remaining depth to the center. The theoretical study of the properties of matter at the boundary layer between crust and core is crucial to understanding certain observational phenomena such as pulsar glitches, quasi-periodic oscillations in the X-ray tails of SGR light curves, and potential gravitational waves from neutron star oscillation modes and deviations from axial symmetry from material accreted onto the surface. I will introduce the various ingredients to such studies: nuclei and exotic

57

Jefferson Lab Science Videos on YouTube  

DOE Data Explorer (OSTI)

Jefferson Lab, a DOE physics research lab located in Virgina, has approximately 100 lab-produced videos on YouTube. These include selected presentations from the Jefferson Lab Science Series, short clips of simple experiments for educational purposes, clips from Frostbite Theater, and clips from the Physics Out Loud series.

58

Jefferson Lab Science Series - Current Schedule  

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

Current Science Series Schedule Current Science Series Schedule Lectures are free and open to students and adults with an interest in science. All lectures begin at 7:00 pm in CEBAF Center Auditorium [Download a Map] [Locate Jefferson Lab on Google Maps] [Display a QR Code for Scanning] and last for about an hour. Seating in the CEBAF Center Auditorium and overflow area is limited to about 300 people. Seating is on a first come, first served basis. Unfortunately, people arriving once capacity has been reached will be turned away. A live video stream will be available for those not able to attend in person. Lectures will be added to the video archive for on-demand viewing upon approval from the presenter. NOTICE: For security purposes, everyone over 16 is asked to carry a photo I.D. Security guards may inspect vehicles, book bags and purses.

59

Jefferson Renewable Energy | Open Energy Information  

Open Energy Info (EERE)

Renewable Energy Renewable Energy Jump to: navigation, search Name Jefferson Renewable Energy Place Warwick, Rhode Island Zip 2886 Product Rhode Island-based waste-to-energy and biofuel project developer. Coordinates 41.698591°, -71.461686° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.698591,"lon":-71.461686,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

60

The Jefferson Lab Frozen Spin Target  

SciTech Connect

A frozen spin polarized target, constructed at Jefferson Lab for use inside a large acceptance spectrometer, is described. The target has been utilized for photoproduction measurements with polarized tagged photons of both longitudinal and circular polarization. Protons in TEMPO-doped butanol were dynamically polarized to approximately 90% outside the spectrometer at 5 T and 200-300 mK. Photoproduction data were acquired with the target inside the spectrometer at a frozen-spin temperature of approximately 30 mK with the polarization maintained by a thin, superconducting coil installed inside the target cryostat. A 0.56 T solenoid was used for longitudinal target polarization and a 0.50 T dipole for transverse polarization. Spin relaxation times as high as 4000 hours were observed. We also report polarization results for deuterated propanediol doped with the trityl radical OX063.

Christopher Keith, James Brock, Christopher Carlin, Sara Comer, David Kashy, Josephine McAndrew, David Meekins, Eugene Pasyuk, Joshua Pierce, Mikell Seely

2012-08-01T23:59:59.000Z

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61

JEFFERSON LAB 12 GEV CEBAF UPGRADE  

Science Conference Proceedings (OSTI)

The existing continuous electron beam accelerator facility (CEBAF) at Thomas Jefferson National Accelerator Facility (TJNAF) is a 5-pass, recirculating cw electron Linac operating at approx6 GeV and is devoted to basic research in nuclear physics. The 12 GeV CEBAF Upgrade is a $310 M project, sponsored by the Department of Energy (DOE) Office of Nuclear Physics, that will expand its research capabilities substantially by doubling the maximum energy and adding major new experimental apparatus. The project received construction approval in September 2008 and has started the major procurement process. The cryogenic aspects of the 12 GeV CEBAF Upgrade includes: doubling the accelerating voltages of the Linacs by adding ten new high-performance, superconducting radiofrequency (SRF) cryomodules (CMs) to the existing 42 1/4 cryomodules; doubling of the 2 K cryogenics plant; and the addition of eight superconducting magnets.

Rode, C. H. [Thomas Jefferson National Accelerator Facility, Newport News, Virginia, 23606 (United States)

2010-04-09T23:59:59.000Z

62

The Jefferson Lab High Power Light Source  

Science Conference Proceedings (OSTI)

Jefferson Lab has designed, built and operated two high average power free-electron lasers (FEL) using superconducting RF (SRF) technology and energy recovery techniques. Between 1999-2001 Jefferson Lab operated the IR Demo FEL. This device produced over 2 kW in the mid-infrared, in addition to producing world record average powers in the visible (50 W), ultraviolet (10 W) and terahertz range (50 W) for tunable, short-pulse (power demonstration of an accelerator configuration that is being exploited for a number of new accelerator-driven light source facilities that are currently under design or construction. The driver accelerator for the IR Demo FEL uses an Energy Recovered Linac (ERL) configuration that improves the energy efficiency and lowers both the capital and operating cost of such devices by recovering most of the power in the spent electron beam after optical power is extracted from the beam. The IR Demo FEL was de-commissioned in late 2001 for an upgraded FEL for extending the IR power to over 10 kW and the ultraviolet power to over 1 kW. The FEL Upgrade achieved 10 kW of average power in the mid-IR (6 microns) in July of 2004, and its IR operation currently is being extended down to 1 micron. In addition, we have demonstrated the capability of on/off cycling and recovering over a megawatt of electron beam power without diminishing machine performance. A complementary UV FEL will come on-line within the next year. This paper presents a summary of the FEL characteristics, user community accomplishments with the IR Demo, and planned user experiments.

James R. Boyce

2006-01-01T23:59:59.000Z

63

Frostbite Theater - Just for Fun - Jefferson Lab Open House (2010)  

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

Nitrogen Viewer Requests! Nitrogen Viewer Requests! Previous Video (Liquid Nitrogen Viewer Requests!) Frostbite Theater Main Index Next Video (Season One Bloopers) Season One Bloopers Jefferson Lab Open House (2010) Highlights from Jefferson Lab's 2010 Open House including portions of our electron accelerator, a peek inside an end station, and a visit to the Free Electron Laser. [ Show Transcript ] Announcer: Frostbite Theater presents... Cold Cuts! No baloney! Joanna and Steve: Just science! Joanna: Hi! I'm Joanna! Steve: And I'm Steve! Joanna: And we're here at Jefferson Lab's Open House! If you're interested in science, this is the place to be! Steve: Thousands of people have come to Jefferson Lab today to learn more about science, what we do here and to just have fun! Joanna: So what are some of the things that people can do when they're

64

Thomas Jefferson High School for Science & Technology National Science  

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

Thomas Jefferson High School for Science & Technology National Thomas Jefferson High School for Science & Technology National Science Bowl® Champion Thomas Jefferson High School for Science & Technology National Science Bowl® Champion May 2, 2005 - 12:40pm Addthis WASHINGTON, DC -- "The Incompleteness Theorem" was the answer to a question on mathematics that today clinched the 2005 National Science Bowl® championship for the Thomas Jefferson High School for Science & Technology team from Alexandria, Va. The team received its championship trophy after triumphing over 62 other regional team champions this weekend. The team members are: Logan Kearsley, Matthew Isakowitz, Sam Lederer, Lisa Marrone, Charlotte Seid and coach Sharon Baker. The team also won a research trip to Alaska, three Computer Based Laboratories and $1,000 for their school's science

65

Jefferson Lab Contract to be Awarded to Jefferson Science Associates, LLC for Management and Operation of World-Class Office of Science Laboratory  

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

OAK RIDGE , TN - The U.S. Department of Energy has selected Jefferson Science Associates, LLC, as the contractor for management and operation of the Thomas Jefferson National Accelerator Facility....

66

Thomas Jefferson National Accelerator Facility Site Tour - Accelerator Map  

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

Counting House Free Electron Accelerator Facility Machine Control Center Physics Storage Building North Linear Accelerator South Linear Accelerator VEPCO Substation Machine Control Center Annex Machine Control Center Annex II North Access Building South Access Building Central Helium Liquefier Injector Hall A Truck Ramp Hall B Truck Ramp Hall C Truck Ramp Experimental Hall A Experimental Hall B Experimental Hall C East Arc West Arc Counting House Free Electron Accelerator Facility Machine Control Center Physics Storage Building North Linear Accelerator South Linear Accelerator VEPCO Substation Machine Control Center Annex Machine Control Center Annex II North Access Building South Access Building Central Helium Liquefier Injector Hall A Truck Ramp Hall B Truck Ramp Hall C Truck Ramp Experimental Hall A Experimental Hall B Experimental Hall C East Arc West Arc Science Education Jefferson Lab Jefferson Lab Home Search Jefferson Lab Contact Jefferson Lab Science Education Home Teacher Resources Student Zone Games and Puzzles Science Cinema Programs and Events Search Education Privacy and Security Notice Jefferson Lab Site Tour Guided Tour Site Map Accelerator Area Map Administrative Area Map Tour Index

67

Orange and Rockland Case Study  

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

0 2012 0 2012 Orange and Rockland Case Study 1 Voltage Control Device A "Model-Centric" Approach to Smarter Electric Distribution Systems Orange and Rockland Utilities (ORU), is an investor-owned utility and a subsidiary of Consolidated Edison Incorporated (Con Edison), and is located in suburban New York, New Jersey, and Pennsylvania, west of New York City. ORU is a key participant in Con Edison's $272 million Smart Grid Investment Grant (SGIG) project to modernize electric distribution systems. With $136 million in Recovery Act funding from the U.S. Department of Energy, Con Edison and ORU expect to install smart grid technologies that provide: (1) lower frequency and duration of outages, (2)

68

NEWTON Teachers - Classroom and Curriculum Development  

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

Feel free to click on the banner to explore the site. Welcome to the NEWTON Teachers NEWTON Teachers was developed by teachers for teachers. Here you can explore educational...

69

Leavenworth-Jefferson E C, Inc | Open Energy Information  

Open Energy Info (EERE)

Leavenworth-Jefferson E C, Inc Leavenworth-Jefferson E C, Inc Jump to: navigation, search Name Leavenworth-Jefferson E C, Inc Place Kansas Utility Id 10801 Utility Location Yes Ownership C NERC Location SPP Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Outdoor Area Lighting Service (HPS 100 W) Lighting Outdoor Area Lighting Service (HPS 250 W) Lighting Outdoor Area Lighting Service (HPS 400 W) Lighting Outdoor Area Lighting Service (MH 100 W) Lighting Outdoor Area Lighting Service (MH 250 W) Lighting Outdoor Area Lighting Service (MH 400 W) Lighting Outdoor Area Lighting Service (MV 175 W) Lighting

70

EA-1937: Pacific Direct Intertie Upgrade Project, Lake, Jefferson, Crook,  

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

37: Pacific Direct Intertie Upgrade Project, Lake, Jefferson, 37: Pacific Direct Intertie Upgrade Project, Lake, Jefferson, Crook, Deschutes, and Wasco Co, OR EA-1937: Pacific Direct Intertie Upgrade Project, Lake, Jefferson, Crook, Deschutes, and Wasco Co, OR SUMMARY This project would replace aging equipment at BPA's Celilo converter station and to upgrade equipment on the Celilo-Sylmar 500-kilovolt (kV) transmission line from the Celilo converter station in The Dalles, Oregon to the Nevada-Oregon border. As part of the project, BPA would remove and salvage the converter terminals 1 and 2 at its Celilo converter station and install a new two-converter terminal. A 20-acre expansion of the existing substation would accommodate the new terminal equipment. About 265 miles of transmission towers on the Celilo-Sylmar 500-kV transmission line would be

71

The 12 GeV Energy Upgrade at Jefferson Laboratory  

SciTech Connect

Two new cryomodules and an extensive upgrade of the bending magnets at Jefferson Lab has been recently completed in preparation for the full energy upgrade in about one year. Jefferson Laboratory has undertaken a major upgrade of its flagship facility, the CW re-circulating CEBAF linac, with the goal of doubling the linac energy to 12 GeV. I will discuss here the main scope and timeline of the upgrade and report on recent accomplishments and the present status. I will then discuss in more detail the core of the upgrade, the new additional C100 cryomodules, their production, tests and recent successful performance. I will then conclude by looking at the future plans of Jefferson Laboratory, from the commissioning and operations of the 12 GeV CEBAF to the design of the MEIC electron ion collider.

Pilat, Fulvia C. [JLAB

2012-09-01T23:59:59.000Z

72

An Overview of Dark Matter Experiments at Jefferson Lab  

Science Conference Proceedings (OSTI)

Dark Matter research at Jefferson Lab started in 2006 with the LIght Pseudoscalar and Scalar Search (LIPSS) collaboration to check the validity of results reported by the PVLAS collaboration. In the intervening years interest in dark matter laboratory experiments has grown at Jefferson Lab. Current research underway or in planning stages probe various mass regions covering 14 orders of magnitude: from 10{sup -6} eV to 100 MeV. This presentation will be an overview of our dark matter efforts, three of which focus on the hypothesized A' gauge boson.

James Boyce

2012-09-01T23:59:59.000Z

73

Labs at-a-Glance: Thomas Jefferson National Accelerator Facility | U.S. DOE  

Office of Science (SC) Website

Thomas Jefferson Thomas Jefferson National Accelerator Facility Laboratories Ames Laboratory Argonne National Laboratory Brookhaven National Laboratory Fermi National Accelerator Laboratory Lawrence Berkeley National Laboratory Oak Ridge National Laboratory Pacific Northwest National Laboratory Princeton Plasma Physics Laboratory SLAC National Accelerator Laboratory Thomas Jefferson National Accelerator Facility Laboratory Policy and Evaluation Safety, Security and Infrastructure Laboratory Science Highlights Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Labs at-a-Glance: Thomas Jefferson National Accelerator Facility Print Text Size: A A A RSS Feeds FeedbackShare Page Thomas Jefferson National Accelerator Facility Logo

74

VEE-0086 - In the Matter of Jefferson City Oil Co., Inc. | Department of  

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

6 - In the Matter of Jefferson City Oil Co., Inc. 6 - In the Matter of Jefferson City Oil Co., Inc. VEE-0086 - In the Matter of Jefferson City Oil Co., Inc. On April 18, 2002, Jefferson City Oil Co., Inc. (Jefferson City Oil) filed an Application for Exception with the Office of Hearings and Appeals (OHA) of the Department of Energy (DOE). Jefferson City Oil requests that it be relieved of the requirement to prepare and file the Energy Information Administration's (EIA) form entitled "Resellers'/Retailers' Monthly Petroleum Product Sales Report" (Form EIA-782(b)). As explained below, we have concluded that Jefferson City Oil has not demonstrated that it is entitled to exception relief. vee0086.pdf More Documents & Publications VEE-0074 - In the Matter of H.A. Mapes, Inc. VEE-0081 - In the Matter of North Side Coal & Oil Co., Inc.

75

Thomas Jefferson Site Office Homepage | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Home Home Thomas Jefferson Site Office (TJSO) TJSO Home About Current Projects Contract Management Environment, Safety and Health (ES&H) Resources Contact Information Thomas Jefferson Site Office U.S. Department of Energy 12000 Jefferson Avenue Newport News, VA 23606 P: (757) 269-7140 Thomas Jefferson Site Office Pictured Right: Thomas Jefferson Site Office Staff TJSO Staff Photo 1 of 2 Print Text Size: A A A RSS Feeds FeedbackShare Page The Thomas Jefferson Site Office (TJSO) is an organization within the U.S. Department of Energy's Office of Science with responsibility to oversee and manage the Management and Operating (M&O) contract for the Thomas Jefferson National Accelerator Facility (TJNAF) in Newport News, Virginia. TJNAF is one of ten Office of Science Laboratories and is a single program

76

Strategic Petroleum Reserve Texoma Complex distribution enhancements: Orange and Jefferson Counties, Texas; Calcasieu and Cameron Parishes, Louisiana: Environmental assessment  

Science Conference Proceedings (OSTI)

The Department of Energy is proposing to construct and operate two buried crude oil pipelines to provide for unconstrained drawdown of three Strategic Petroleum Reserve (SPR) crude oil storage facilities of the Texoma Complex located in portions of Louisiana and Texas. The project is required to provide a crude oil distribution system capable of meeting a planned increase in the Texoma Complex drawdown rate to 2,340,000 barrels-per-day (bpd). The EA addresses a no-action alternative and alternative pipeline routes. Potential impacts from pipeline construction concern disturbances to prime farmlands, floodplains and wetlands. A very small acreage of prime farmlands is involved; the total is not considered significant. The Floodplain/Wetlands Assessment states that the effects of pipeline construction and operation on floodplains and associated wetlands will be temporary and localized. DOE determined in a Floodplain Statement of Findings that for the project as a whole there is no practicable alternative to locating in a floodplain, and that the proposal conforms to appropriate state and local floodplain protection standards. Potential impacts from pipeline operation are primarily concerned with accidental releases of crude oil to the environment. Because the pipelines will be buried, the probability of a major pipeline break releasing large quantities of crude oil is small and pipeline testing and the development of an oil spill contingency plan will reduce the seriousness of any oil spill. The proposed pipelines are expected to involve no other environmental concerns. It is the determination of DOE that the proposed Texoma Complex Distribution Enhancements do not constitute a major federal action significantly affecting the quality of the human environment; therefore an environmental impact statement will not be prepared. 27 refs., 3 tabs.

Not Available

1987-03-01T23:59:59.000Z

77

Undergraduate Research at Jefferson Lab - Analysis of Contamination Levels  

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

Compton Scattering Chamber Compton Scattering Chamber Previous Project (Compton Scattering Chamber) Undergraduate Research Main Index Next Project (Non-linear Multidimensional Optimization) Non-linear Multidimensional Optimization Analysis of Contamination Levels of Jefferson Laboratory SRF Clean Room Facilities during Power Outage Using FE-SEM/EDX Studies of Copper Coupons Student: Kaitlyn M. Fields School: College of William and Mary Mentored By: Ari D. Palczewski and Charles E. Reece Superconducting radiofrequency (SRF) accelerating cavities at Thomas Jefferson National Accelerator Facility support high surface electric and magnetic fields with minimal energy dissipation and resistance. The performance of these cavities can be limited by particulate contamination, which can become a source of enhanced field emission. Clean cavity assembly

78

Old Jefferson, Louisiana: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Jefferson, Louisiana: Energy Resources Jefferson, Louisiana: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 30.3826922°, -91.0170468° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.3826922,"lon":-91.0170468,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

79

Jefferson West High School Wind Project | Open Energy Information  

Open Energy Info (EERE)

High School Wind Project High School Wind Project Jump to: navigation, search Name Jefferson West High School Wind Project Facility Jefferson West High School Sector Wind energy Facility Type Community Wind Location KS Coordinates 39.193382°, -95.560616° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.193382,"lon":-95.560616,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

80

A dynamically polarized hydrogen and deuterium target at Jefferson Lab  

DOE Green Energy (OSTI)

Polarized electron beams have been successfully used at Jefferson Lab for over a year. The authors now report the successful achievement of polarized targets for nuclear and particle physics experiments using the dynamic nuclear polarization (DNP)technique. The technique involves initial irradiation of frozen ammonia crystals (NH{sub 3} and ND{sub 3}) using the electron beam from the new Free Electron Laser (FEL) facility at Jefferson Lab, and transferring the crystals to a special target holder for use in Experimental Halls. By subjecting the still ionized and frozen ammonia crystals to a strong magnetic field and suitably tuned RF, the high electron polarization is transmitted to the nucleus thus achieving target polarization. Details of the irradiation facility, the target holder, irradiation times, ionized crystal shelf life, and achieved polarization are discussed.

Boyce, J.R.; Keith, C.; Mitchell, J.; Seely, M.

1998-07-01T23:59:59.000Z

Note: This page contains sample records for the topic "newton orange jefferson" 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

Jefferson County, Alabama: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Jefferson County, Alabama: Energy Resources Jefferson County, Alabama: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 33.4914122°, -86.9824288° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.4914122,"lon":-86.9824288,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

82

Newton, Utah: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

| Sign Up Search Page Edit with form History Facebook icon Twitter icon Newton, Utah: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates...

83

Recent Results from Jefferson Lab RSS Spin Physics Program  

Science Conference Proceedings (OSTI)

The spin physics program in Jefferson Labs Hall C concentrates on high precision and high resolution studies of the nucleon spin structure that can be extracted from inclusive polarized scattering experiments. The Resonances Spin Structure RSS experiment has measured nucleon spin structure functions in the resonances region at an intermediate four?momentum transfer Q 2 ?1.3? GeV 2 . The polarized target in Hall C could be polarized longitudinally and transversely

Mahbub Khandaker; the RSS Collaboration

2009-01-01T23:59:59.000Z

84

Spin Asymmetries on Nucleon Experiment at Jefferson Lab  

SciTech Connect

The Spin Asymmetries of the Nucleon Experiment (SANE) of Jefferson Lab is a comprehensive measurement of double spin asymmetries of the proton for both parallel and almost perpendicular spin configurations of the proton spin and the electron beam polarization directions. The experiment will provide both spin structure functions, g2 and g1 and spin observable A2 and A1 of the proton over Q2 region from 2.5 to 6.5 GeV2/c2 and Bjorken x region of 0.3 to 0.8. Using the polarized electron beam of Thomas Jefferson National Accelerator Facility and the polarized frozen NH3 target, the data were taken early 2009 in Hall C of Jefferson Lab. Scattered electrons from the inclusive reaction were detected by the Big Electron Telescope Array (BETA), a new non-magnetic detector with a large acceptance of 194 msr. The current analysis effort is focused on the proton spin structure functions g2 and g1. Physics motivations with the experimental methods will be presented with an overvew of the current status of the data analysis.

Seonho Choi

2011-10-01T23:59:59.000Z

85

Spin Asymmetries on Nucleon Experiment at Jefferson Lab  

SciTech Connect

The Spin Asymmetries of the Nucleon Experiment (SANE) of Jefferson Lab is a comprehensive measurement of double spin asymmetries of the proton for both parallel and almost perpendicular spin configurations of the proton spin and the electron beam polarization directions. The experiment will provide both spin structure functions, g{sub 2} and g{sub 1} and spin observable A{sub 2} and A{sub 1} of the proton over Q{sup 2} region from 2.5 to 6.5 GeV{sup 2}/c{sup 2} and Bjorken x region of 0.3 to 0.8. Using the polarized electron beam of Thomas Jefferson National Accelerator Facility and the polarized frozen NH{sub 3} target, the data were taken early 2009 in Hall C of Jefferson Lab. Scattered electrons from the inclusive reaction were detected by the Big Electron Telescope Array (BETA), a new non-magnetic detector with a large acceptance of 194 msr. The current analysis effort is focused on the proton spin structure functions g{sub 2} and g{sub 1}. Physics motivations with the experimental methods will be presented with an overview of the current status of the data analysis.

Choi, Seonho [Department of Physics, Seoul National University, Seoul 151-747 (Korea, Republic of)

2011-10-21T23:59:59.000Z

86

NEWTON, Ask a Scientist at Argonne National Labs  

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

Questions Referencing NEWTON About NEWTON About Ask A Scientist Education At Argonne Dog Licking Behavior Name: Faith Status: other Grade: other Location: NA Country: South...

87

North Newton School Corp | Open Energy Information  

Open Energy Info (EERE)

Newton School Corp Newton School Corp Jump to: navigation, search Name North Newton School Corp Facility North Newton School Corp Sector Wind energy Facility Type Community Wind Facility Status In Service Owner North Newton School Corp Developer Performance Services Energy Purchaser Net-metered Location Morocco IN Coordinates 41.03259745°, -87.42682815° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.03259745,"lon":-87.42682815,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

88

SBOT VIRGINIA THOMAS JEFFERSON LAB POC Danny Llyod Telephone  

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

VIRGINIA VIRGINIA THOMAS JEFFERSON LAB POC Danny Llyod Telephone (757) 269-7121 Email lloyd@jlab.org ADMINISTATIVE / WASTE / REMEDIATION Facilities Support Services 561210 Employment Placement Agencies 561311 Travel Agencies 561510 Locksmiths 561622 Exterminating and Pest Control Services 561710 Janitorial Services 561720 Landscaping Services 561730 Carpet and Upholstery Cleaning Services 561740 Hazardous Waste Collection 562112 CONSTRUCTION Industrial Building Construction 236210 Commercial and Institutional Building Construction 236220 Water and Sewer Line and Related Structures Construction 237110 Power and Communication Line and Related Structures Construction 237130 Highway, Street, and Bridge Construction 237310 Other Heavy and Civil Engineering Construction 237990 Other Foundation, Structure, and Building Exterior Contractors

89

Light Baryon Spectroscopy using the CLAS Spectrometer at Jefferson Laboratory  

Science Conference Proceedings (OSTI)

Baryons are complex systems of confined quarks and gluons and exhibit the characteristic spectra of excited states. The systematics of the baryon excitation spectrum is important to our understanding of the effective degrees of freedom underlying nucleon matter. High-energy electrons and photons are a remarkably clean probe of hadronic matter, providing a microscope for examining the nucleon and the strong nuclear force. Current experimental efforts with the CLAS spectrometer at Jefferson Laboratory utilize highly-polarized frozen-spin targets in combination with polarized photon beams. The status of the recent double-polarization experiments and some preliminary results are discussed in this contribution.

Volker Crede

2011-12-01T23:59:59.000Z

90

The Jefferson Lab 12 GeV Upgrade  

Science Conference Proceedings (OSTI)

A major upgrade of the Continuous Electron Beam Accelerator Facility (CEBAF) at the Thomas Jefferson National Accelerator Facility is in progress. Construction began in 2008 and the project should be completed in 2015. The upgrade includes doubling the energy of the electron beam to 12 GeV, the addition of a new fourth experimental hall, and new experimental equipment in three of the experimental halls. A brief overview of this upgrade project is presented along with some highlights of the anticipated experimental program.

R.D. McKeown

2011-10-01T23:59:59.000Z

91

EM Calorimeters for SoLID at Jefferson Lab  

SciTech Connect

Several approved experiments at Jefferson Lab for the 12 GeV era will use the proposed Solenoid Large Intensity Device (SoLID) spectrometer. Two EM calorimeters with a total area of 15 square meters are required for electron identification and electron-pion separation. The challenge is to build calorimeters that can withstand high radiation doses in high magnetic field region and bring photon signals to low field region for readout. Several types of calorimeters were considered and we are favoring Shashlyk type as a result of balancing performance and cost. Our preliminary design and simulation of SoLID EM calorimeters are presented.

Z.W. Zhao, J. Huang, M. Meziane, X. Zheng, P.E. Reimer, D. Armstrong, T. Averett, W. Deconinck

2012-12-01T23:59:59.000Z

92

RF Power Upgrade for CEBAF at Jefferson Laboratory  

Science Conference Proceedings (OSTI)

Jefferson Laboratory (JLab) is currently upgrading the 6GeV Continuous Electron Beam Accelerator Facility (CEBAF) to 12GeV. As part of the upgrade, RF systems will be added, bringing the total from 340 to 420. Existing RF systems can provide up to 6.5 kW of CW RF at 1497 MHZ. The 80 new systems will provide increased RF power of up to 13 kW CW each. Built around a newly designed and higher efficiency 13 kW klystron developed for JLab by L-3 Communications, each new RF chain is a completely revamped system using hardware different than our present installations. This paper will discuss the main components of the new systems including the 13 kW klystron, waveguide isolator, and HV power supply using switch-mode technology. Methodology for selection of the various components and results of initial testing will also be addressed. Notice: Authored by Jefferson Science Associates, LLC under U.S. DOE Contract No. DE-AC05-06OR23177. The U.S. Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce this manuscript for U.S. Government purposes.

Andrew Kimber,Richard Nelson

2011-03-01T23:59:59.000Z

93

EMC effect for light nuclei: new results from Jefferson Lab  

Science Conference Proceedings (OSTI)

High energy lepton scattering has been the primary tool for mapping out the quark distributions of nucleons and nuclei. Measurements of deep inelastic scattering in nuclei show that the quark distributions in heavy nuclei are not simply the sum of the quark distributions of the constituent proton and neutron, as one might expect for a weakly bound system. This modification of the quark distributions in nuclei is known as the EMC effect. I will discuss the results from Jefferson Lab (JLab) experiment E03-103, a precise measurement of the EMC effect in few-body nuclei with emphasis on the large x region. Data from the light nuclei suggests that the nuclear dependence of the high x quark distribution may depend on the nucleon's local environment, rather than being a purely bulk effect. In addition, I will also discuss about a future experiment at the upgraded 12 GeV Jefferson Lab facility which will further investigate the role of the local nuclear environment and the influence of detailed nuclear structure to the modification of quark distributions.

Daniel, A. [Dept. of Physics and Astronomy, Ohio University, Athens OH 45701 (United States)

2011-10-24T23:59:59.000Z

94

Optical modeling of the Jefferson Laboratory IR Demo FEL  

Science Conference Proceedings (OSTI)

The Thomas Jefferson National Accelerator Facility (Jefferson Lab) is in the process of building a 1 kW free-electron laser operates at 3 microns. The details of the accelerator driver are given in other papers in these proceedings. The optical cavity consists of a near-concentric resonator with transmissive outcoupling. Though several free-electron lasers have used similar designs, they have not had to confront the high average-power loading present in this laser. It is useful to know the limits of this type of optical cavity design. The optical system of the laser has been modeled using the commercial code GLAD{reg_sign} by using a Beer`s-law region to mimic the FEL interaction. The effects of mirror heating have been calculated and compared with analytical treatments. The magnitude of the distortion for several materials and wave-lengths has been estimated. The model developed here allows one to quickly determine whether the mirror substrates and coatings are adequate for operation at a given optical power level once the absorption of the coatings, substrate, and transmission are known. Results of calculations of the maximum power level expected using several different sets of mirrors will be presented. Measurements of the distortion in calcium fluoride from absorption of carbon dioxide laser light are planned to benchmark the simulations. Multimode simulations using the code ELIXER have been carried out to characterize the saturated optical mode quality. The results will be presented.

Benson, S.V.; Davidson, P.S.; Jain, R.; Kloeppel, P.K.; Neil, G.R.; Shinn, M.D.

1997-11-01T23:59:59.000Z

95

Jefferson Lab Science Series - Understanding Flight: A Physical Description  

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

Physics of Stock Car Racing Physics of Stock Car Racing Previous Video (The Physics of Stock Car Racing) Science Series Video Archive Next Video (The Hidden World of Technology) The Hidden World of Technology Understanding Flight: A Physical Description of How Airplanes Fly Dr. Scott Eberhardt - University of Washington March 23, 2004 Did you ever wonder how a Boeing 747, weighing 910,000 lbs at takeoff can possibly get off the ground? Or, did you ever wonder how airplanes fly upside down? Why is there a "backside of the power curve?" What makes a wing efficient? These questions can be answered when lift is developed in terms of Newton's laws. A Newtonian description of lift gives an intuitive feel for how airplanes fly, without the need for complicated analysis or approximations. Through the application of Newton's three laws, we will

96

Jefferson Davis Elec Coop, Inc | Open Energy Information  

Open Energy Info (EERE)

Davis Elec Coop, Inc Davis Elec Coop, Inc Jump to: navigation, search Name Jefferson Davis Elec Coop, Inc Place Louisiana Utility Id 9682 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes RTO SPP Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png All Electric Farm and Home Service Residential All Electric Farm and Home Service - Seasonal Residential Commercial and Industrial Services Commercial Extra Large Power Service Commercial Farm and Rice Dryers Residential Flood Lighting Service: 1000 watt- 140,000 Lumen High Pressure Sodium Lighting

97

Jefferson Lab Science Series - You Already Know This Physics!  

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

Living and Working in the Freezer Living and Working in the Freezer Previous Video (Living and Working in the Freezer) Science Series Video Archive Next Video (The Origin of the Elements) The Origin of the Elements You Already Know This Physics! Mr. Jack McKisson - Jefferson Lab, Detector and Imaging Group October 9, 2012 From a research path that includes a little bit of rocket science, under sea measurements, radiation detection and measurement, space experimentation and two expeditions to the Antarctic, Mr. McKisson brings a different view of how much physics most people already know from observing the world around them. With a minimal amount of math, attendees will learn a little of the history of physics and may discover that they know more than they thought about what some view as an inscrutable subject

98

Undergraduate Research at Jefferson Lab - Determining Electron Beam Energy  

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

Pretzelosity Distribution Pretzelosity Distribution Previous Project (Pretzelosity Distribution) Undergraduate Research Main Index Next Project (Buffered Chemical Polishing) Buffered Chemical Polishing Determining Electron Beam Energy through Spin Precession Methods Student: Gina Mayonado School: McDaniel College Mentored By: Douglas Higinbotham Nuclear physics experiments at Jefferson Lab require that the beam energy of the Continuous Electron Beam Accelerator Facility (CEBAF) accelerator be known to 0.01%. The g-2 spin precession of the electrons as they circulate in the machine can be used to determine the beam energy without relying on the absolute calibration of magnets and devices required for other methods. The precision of this approach needed to be fully investigated. Spin precession methods were investigated by writing an Apple application to

99

A LIMITED LIABILITY PARTNERSHIP 1050 Thomas Jefferson Street, NW  

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

A LIMITED LIABILITY PARTNERSHIP A LIMITED LIABILITY PARTNERSHIP 1050 Thomas Jefferson Street, NW Seventh Floor Washington, DC 20007 (202) 298-1800 Phone (202) 338-2416 Fax MEMORANDUM TO: DOE Office of General Counsel FROM: Doug Smith DATE: August 29, 2013 RE: Record of Communication Concerning Ceiling Fan and Ceiling Fan Light Kit Framework Document-Docket No. EERE-2012-BT-STD-0045 This memo provides an overview of communications made to DOE staff on the subject of possible changes to standards and test procedures for ceiling fans and ceiling fan light kits. The communications occurred at a meeting held at 10:30 a.m. on August 20, 2013, following the close of the comment period on the initial framework document for ceiling fans and light kits. The meeting attendees included:

100

Probing the nucleon structure with SIDIS at Jefferson Lab  

Science Conference Proceedings (OSTI)

In recent years, measurements of azimuthal moments of polarized hadronic cross sections in hard processes have emerged as a powerful tool to probe nucleon structure. Many experiments worldwide are currently trying to pin down various effects related to nucleon structure through Semi-Inclusive Deep-Inelastic Scattering (SIDIS). Azimuthal distributions of final-state particles in semi-inclusive deep inelastic scattering, in particular, are sensitive to the orbital motion of quarks and play an important role in the study of Transverse Momentum Dependent parton distribution functions (TMDs) of quarks in the nucleon. The CLAS spectrometer, installed in Hall-B at Jefferson Lab, has collected semi-inclusive data using the CEBAF 6 GeV polarized electron beam on polarized solid NH{sub 3} and ND{sub 3} targets. An overview of these measurements is presented.

Pereira, Sergio Anafalos [INFN-Frascati

2013-01-01T23:59:59.000Z

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101

Status of Jefferson Lab's Load Locked Polarized Electron Beam  

DOE Green Energy (OSTI)

A new 100 kV load locked polarized electron gun has been built at Jefferson Lab. The gun is installed in a test stand on a beam line that resembles the first few meters of the CEBAF nuclear physics photoinjector. With this gun, a GaAs photocathode can be loaded from atmosphere, hydrogen cleaned, activated and taken to high voltage in less than 8 hours. The gun is a three chamber design, with all of the moving parts remaining at ground potential during gun operation. Studies of gun performance, photocathode life times, transverse emittance at high bunch charge, helicity correlated effects and beam polarizations from new photocathode samples will all be greatly facilitated by the use of this load locked gun.

M.L. Stutzman; P. Adderley; M. Baylac; J. Clark; A. Day; J. Grames; J. Hansknecht; M. Poelker

2002-09-01T23:59:59.000Z

102

Jefferson Lab 12 GeV CEBAF Upgrade  

Science Conference Proceedings (OSTI)

The existing continuous electron beam accelerator facility (CEBAF) at Thomas Jefferson National Accelerator Facility (TJNAF) is a 5-pass, recirculating cw electron Linac operating at ~6 GeV and is devoted to basic research in nuclear physics. The 12 GeV CEBAF Upgrade is a $310 M project, sponsored by the Department of Energy (DOE) Office of Nuclear Physics, that will expand its research capabilities substantially by doubling the maximum energy and adding major new experimental apparatus. The project received construction approval in September 2008 and has started the major procurement process. The cryogenic aspects of the 12 GeV CEBAF Upgrade includes: doubling the accelerating voltages of the Linacs by adding ten new high-performance, superconducting radiofrequency (SRF) cryomodules (CMs) to the existing 42 1/4 cryomodules; doubling of the 2 K cryogenics plant; and the addition of eight superconducting magnets.

Claus Rode

2010-04-01T23:59:59.000Z

103

ELECTROSTATIC MODELING OF THE JEFFERSON LABORATORY INVERTED CERAMIC GUN  

SciTech Connect

Jefferson Laboratory (JLab) is currently developing a new 500kV DC electron gun for future use with the FEL. The design consists of two inverted ceramics which support a central cathode electrode. This layout allows for a load-lock system to be located behind the gun chamber. The electrostatic geometry of the gun has been designed to minimize surface electric field gradients and also to provide some transverse focusing to the electron beam during transit between the cathode and anode. This paper discusses the electrode design philosophy and presents the results of electrostatic simulations. The electric field information obtained through modeling was used with particle tracking codes to predict the effects on the electron beam.

P. Evtushenko ,F.E. Hannon, C. Hernandez-Garcia

2010-05-01T23:59:59.000Z

104

RICH detector at Jefferson Lab, design, performance and physics results  

Science Conference Proceedings (OSTI)

Since 2004 the hadron spectrometer of Hall A at Jefferson Lab is equipped with a proximity focusing RICH. This detector is capable of identify kaon from pion and proton with an angular separation starting from 6 sigma at 2 GeV/c. The RICH design is conceptually similar to the ALICE HMPID RICH; it uses a C6F14 liquid radiator and a 300 nm layer of CsI deposited on the cathode pad plane of an asymmetric MWPC. The RICH has operated for the Hypernuclear Spectroscopy Experiment E94-107, which took data in the last two years. Design details and performance along with first physics results from the hypernuclear experiment are shortly presented.

E. Cisbani; S. Colilli; F. Cusanno; S. Frullani; R. Frantoni; F. Garibaldi; F. Giuliani; M. Gricia; M. Lucentini; M.L. Magliozzi; L. Pierangeli; F. Santavenere; P. Veneroni; G.M. Urciuoli; M. Iodice; G. De Cataldo; R. De Leo; L. Lagamba; S. Marrone; E. Nappi; V. Paticchio; R. Feuerbach; D. Higinbotham; J. Lerose; B. Kross; R. Michaels; Y. Qiang; B. Reitz; J. Segal; B. Wojtsekhowski; C. Zorn; A. Acha; P. Markowitz; C.C. Chang; H. Breuer

2006-04-01T23:59:59.000Z

105

Studies of the Electromagnetic Structure of Mesons at Jefferson Lab  

SciTech Connect

The Jefferson Laboratory Hall B PrimEx Collaboration is using tagged photons to perform an absolute 1.4% level cross section measurement of the photoproduction of neutral pions in the Coulomb field of a nucleus. The absolute cross section for this process is directly proportional to the neutral pion radiative decay width and consequently the uncertainty in the luminosity is directly reflected in the final error bar of the measurement. The PI has taken primary responsibility for the photon flux determination and in this technical report, we outline the steps taken to limit the uncertainty in the tagged photon flux to the 1% level. These include the use of a total absorption counter for absolute flux calibration, a pair spectrometer for online relative flux monitoring, and updated procedures for postbremsstrahlung electron counting. The photon tagging technique has been used routinely in its various forms to provide quasimonochromatic photons for absolute photonuclear cross section measurements. The analysis of such experiments in the context of bremsstrahlung photon tagging was summarized by Owens in 1990. Since then, a number of developments have made possible significant improvements in the implementation of this technique. Here, we describe the steps taken by the PrimEx Collaboration in Hall B of Jefferson Laboratory to limit the systematic uncertainty in the absolute photon flux to 1%. They include an absolute flux calibration at low intensity with a total absorption counter, online relative flux monitoring with a pair spectrometer, and the use of multihit time to digital converters for post bremsstrahlung electron counting during production data runs. While this discussion focuses on the analysis techniques utilized by the PrimEx Collaboration which involves a bremsstrahlung based photon tagging system to measure the neutral pion lifetime, the methods described herein readily apply to other types of photon tagging systems.

Dale, Daniel, S.

2012-11-11T23:59:59.000Z

106

Orange and Rockland Utilities (Gas) - Residential Efficiency Program |  

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

Orange and Rockland Utilities (Gas) - Residential Efficiency Orange and Rockland Utilities (Gas) - Residential Efficiency Program Orange and Rockland Utilities (Gas) - Residential Efficiency Program < Back Eligibility Commercial Industrial Residential Savings Category Heating & Cooling Commercial Heating & Cooling Heating Appliances & Electronics Home Weatherization Commercial Weatherization Sealing Your Home Ventilation Construction Water Heating Program Info State New York Program Type Utility Rebate Program Rebate Amount Furnace: $140 - $420 Water Boiler: $350 or $700 Steam Boiler: $350 Boiler Reset Control: $70 Indirect Water Heater: $210 Programmable Thermostat: $18 Duct and Air Sealing: up to $420 Provider Orange and Rockland Utilities, Inc. Orange and Rockland Utilities provides rebates for residential customers

107

Newton County Rural E M C | Open Energy Information  

Open Energy Info (EERE)

Newton County Rural E M C Jump to: navigation, search Name Newton County Rural E M C Place Indiana Utility Id 13566 Utility Location Yes Ownership C NERC Location RFC NERC RFC Yes...

108

NEWTON, Ask a Scientist at Argonne National Labs  

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

NEWTON About NEWTON About Ask A Scientist Education At Argonne Hot Air Balloon Shape and Altitude Name: Brit Status: student Grade: 6-8 Location: CO Country: USA Date:...

109

A Newton-CG Augmented Lagrangian Method for Semidefinite Programming  

E-Print Network (OSTI)

We consider a Newton-CG augmented Lagrangian method for solving semidefinite programming (SDP) problems from the perspective of approximate semismooth Newton methods. In order to analyze the rate of convergence of our ...

Toh, Kim Chuan

110

NEWTON, Ask a Scientist at Argonne National Labs  

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

Questions Referencing NEWTON About NEWTON About Ask A Scientist Education At Argonne Dog Circling Name: Kalpak Status: student Grade: 9-12 Location: Outside U.S. Country: India...

111

Questions and Answers - Why did it take so long to build Jefferson Lab? Why  

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

are the Halls inbio-dome shapes? are the Halls in<br>bio-dome shapes? Previous Question (Why are the Halls in bio-dome shapes?) Questions and Answers Main Index Next Question (What would happen if part of the accelerator were to break?) What would happen if part ofthe accelerator were to break? Why did it take so long to build Jefferson Lab? Why was Jefferson Lab built in Newport News? Newport News was one of several places around the nation that competed for Jefferson Lab. The Southeastern Universities Research Association (SURA) won the contract to build and run Jefferson Lab in Newport News. A couple reasons helped bring the Lab to this area: 1) The city and state governments worked hard with SURA to earn the Department of Energy's approval to bring the Lab here. (Good teamwork means

112

Finding of No Significant Impact Improvements at the Thomas Jefferson National Accelerator Facility Newsport News, Virginia  

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

IMPROVEMENTS AT THE THOMAS JEFFERSON NATIONAL ACCELERATOR FACILITY IMPROVEMENTS AT THE THOMAS JEFFERSON NATIONAL ACCELERATOR FACILITY NEWPORT NEWS, VIRGINIA AGENCY: U.S. DEPARTMENT OF ENERGY ACTION: FINDING OF NO SIGNIFICANT IMPACT SUMMARY: The U.S. Department of Energy (DOE) has completed an Environmental Assessment (DOE/EA-1384) for proposed Improvements at the Thomas Jefferson National Accelerator Facility (Jefferson Lab). Newport News, Virginia. Based on the results of the impacts analysis reported in the EA, DOE has determined that the proposed action is not a major Federal action that would significantly affect the quality of the human environment within the context of the National Environmental Policy Act of 1969 (NEPA). Therefore, preparation of an environmental impact statement (EIS) is not necessary, and DOE is issuing this Finding of No

113

Jefferson Park : case study of a public housing project in transformation  

E-Print Network (OSTI)

This study focuses on the redevelopment of Jefferson Park, a public housing project in Cambridge, Massachusetts. The work establishes the historical political, social, and physical context in which that redevelopment takes ...

Powers, David Thomas

1984-01-01T23:59:59.000Z

114

Evolution of the Generic Lock System at Jefferson Lab  

SciTech Connect

The Generic Lock system is a software framework that allows highly flexible feedback control of large distributed systems. It allows system operators to implement new feedback loops between arbitrary process variables quickly and with no disturbance to the underlying control system. Several different types of feedback loops are provided and more are being added. This paper describes the further evolution of the system since it was first presented at ICALEPCS 2001 and reports on two years of successful use in accelerator operations. The framework has been enhanced in several key ways. Multiple-input, multiple-output (MIMO) lock types have been added for accelerator orbit and energy stabilization. The general purpose Proportional-Integral-Derivative (PID) locks can now be tuned automatically. The generic lock server now makes use of the Proxy IOC (PIOC) developed at Jefferson Lab to allow the locks to be monitored from any EPICS Channel Access aware client. (Previously clients had to be Cdev aware.) The dependency on the Qt XML parser has been replaced with the freely available Xerces DOM parser from the Apache project.

Brian Bevins; Yves Roblin

2003-10-13T23:59:59.000Z

115

The proton form factor ratio results from Jefferson Lab  

Science Conference Proceedings (OSTI)

The ratio of the proton form factors, GE p/GMp, has been measured extensively, from Q2 of 0.5 GeV2 to 8.5 GeV2, at the Jefferson Laboratory, using the polarization transfer method. This ratio is extracted directly from the measured ratio of the transverse and longitudinal polarization components of the recoiling proton in elastic electron-proton scattering. The polarization transfer results are of unprecedented high precision and accuracy, due in large part to the small systematic uncertainties associated with the experimental technique. There is an approved experiment at JLab, GEP(5), to continue the ratio measurements to 12 GeV2. A dedicated experimental setup, the Super Bigbite Spectrometer (SBS), will be built for this purpose. It will be equipped with a focal plane polarimeter to measure the polarization of the recoil protons. The scattered electrons will be detected in an electromagnetic calorimeter. In this presentation, I will review the status of the proton elastic electromagnetic form factors and discuss a number of theoretical approaches to describe nucleon form factors.

Vina Punjabi

2012-09-01T23:59:59.000Z

116

Optical modeling of the Jefferson Lab IR Demo FEL  

Science Conference Proceedings (OSTI)

The Thomas Jefferson National Accelerator Facility (formerly known as CEBAF) has embarked on the construction of a 1 kW free-electron laser operating initially at 3 microns that is designed for laser-material interaction experiments and to explore the feasibility of scaling the system in power and wavelength for industrial and Navy defense applications. The superconducting radio-frequency linac, and single-pass transport which accelerates the beam from injector to wiggler, followed by energy-recovery deceleration to a dump. The electron and optical beam time structure in the design consists of a train of pecosecond pulses at a 37.425 MHz pulse repetition rate. The initial optical configuration is a conventional near-concentric resonator with transmissive outcoupling. Future upgrades of the system will increase the power and shorten the operating wavelength, and utilize a more advanced resonator system capable of scaling to high powers. The optical system of the laser has been mode led using the GLAD code by using a Beer's-law region to mimic the FEL interaction. Effects such as mirror heating have been calculated and compared with analytical treatments. The magnitude of the distorium for several materials and wavelengths has been estimated. The advantages as well as the limitations of this approach are discussed.

G. Neil; S. Benson; Michelle D. Shinn; P. Davidson; P. Kloppel

1997-01-01T23:59:59.000Z

117

Observer and Particle Transformations and Newton's Laws  

E-Print Network (OSTI)

A frequently confused point in studies of symmetry violation is the distinction between observer and particle transformations. In this work, we consider a model in which a coefficient in the Standard-Model Extension leads to violations of rotation invariance in Newton's second law. The model highlights the distinction between observer and particle transformations.

T. H. Bertschinger; Natasha A. Flowers; Jay D. Tasson

2013-08-14T23:59:59.000Z

118

Using Newton's Law for Dark Energy  

E-Print Network (OSTI)

A model is introduced in which Newton's law is modified between matter and dark energy corpuscles (DECs). The model predicts that the DEC component is presently decelerating in its expansion at 14% of the magnitude of the matter expansion acceleration. In the future, expansion of the DEC universe will continue to decelerate.

Paul Frampton

2012-09-24T23:59:59.000Z

119

Orange and Rockland Utilities (Electric)- Residential Appliance Recycling Program  

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

Orange and Rockland Utilities provides rebates for residential customers for recycling older, inefficient refrigerators and freezers. All appliances must meet the program requirements listed on the...

120

Orange and Rockland Utilities (Electric)- Residential Efficiency Program (New York)  

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

Orange and Rockland Utilities provides rebates for residential customers for recycling older, inefficient refrigerators and freezers. All appliances must meet the program requirements listed on the...

Note: This page contains sample records for the topic "newton orange jefferson" 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

Blue, green, orange, and red upconversion laser  

DOE Patents (OSTI)

A laser for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr.sup.3+ ions and Yb.sup.3+ ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output.

Xie, Ping (San Jose, CA); Gosnell, Timothy R. (Sante Fe, NM)

1998-01-01T23:59:59.000Z

122

Blue, green, orange, and red upconversion laser  

DOE Patents (OSTI)

A laser is disclosed for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr{sup 3+} ions and Yb{sup 3+} ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output. 11 figs.

Xie, P.; Gosnell, T.R.

1998-09-08T23:59:59.000Z

123

Charged Pion Photoproduction from Hydrogen and Deuterium at Jefferson Lab  

DOE Green Energy (OSTI)

The {gamma}n {yields} {pi}{sup -}p and {gamma}p {yields} {pi}{sup +}n reactions are essential probes of the transition from meson-nucleon degrees of freedom to quark-gluon degrees of freedom in exclusive processes. The cross sections of these processes are also, advantageous, for the investigation of oscillatory behavior around the quark counting prediction, since they decrease relatively slower with energy compared with other photon-induced processes. Moreover, these photoreactions in nuclei can probe the QCD nuclear filtering and color transparency effects. In this talk, I discuss the preliminary results on the {gamma}p {yields} {pi}{sup +}n and {gamma}n {yields} {pi}{sup -}p processes at a center-of-mass angle of 90{sup o} from Jefferson Lab experiment E94-104. I also discuss a new experiment in which singles {gamma}p {yields} {pi}{sup +}n measurement from hydrogen, and coincidence {gamma}n {yields} {pi}{sup -}p measurements at the quasifree kinematics from deuterium and {sup 12}C for photon energies between 2.25 GeV to 5.8 GeV in fine steps at a center-of-mass angle of 90{sup o} are planned. The proposed measurement will allow a detailed investigation of the oscillatory scaling behavior in photopion production processes and the study of the nuclear dependence of rather mysterious oscillations with energy that previous experiments have indicated. The various nuclear and perturbative QCD approaches, ranging from Glauber theory, to quark-counting, to Sudakov-corrected independent scattering, make dramatically different predictions for the experimental outcomes.

Haiyan Gao

2003-02-01T23:59:59.000Z

124

Newton, Massachusetts: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

(Redirected from Newton, MA) (Redirected from Newton, MA) Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.3370413°, -71.2092214° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.3370413,"lon":-71.2092214,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

125

Modernizing Newton, to work at any speed  

E-Print Network (OSTI)

Modification of three ideas underlying Newton's original world view, with only minor changes in context, might offer two advantages to introductory physics students. First, the students will experience less cognitive dissonance when they encounter relativistic effects. Secondly, the map-based Newtonian tools that they spend so much time learning about can be extended to high speeds, non-inertial frames, and even (locally, of course) to curved-spacetime.

P. Fraundorf

2001-10-07T23:59:59.000Z

126

Orange County REMC - Energy Efficient Equipment Rebate Program | Department  

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

Orange County REMC - Energy Efficient Equipment Rebate Program Orange County REMC - Energy Efficient Equipment Rebate Program Orange County REMC - Energy Efficient Equipment Rebate Program < Back Eligibility Commercial Industrial Low-Income Residential Multi-Family Residential Residential Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Heat Pumps Appliances & Electronics Commercial Lighting Lighting Water Heating Program Info State Indiana Program Type Utility Rebate Program Rebate Amount Electric Water Heaters: $25 - $150 Hybrid Heat Pump Water Heater: $300 - $400 Central Air Conditioning: $100 - $200 Air-Source Heat Pumps: $200 - $800 Geothermal Heat Pumps: $1,000 ETS Systems: varies CFL bulbs: see program web site Provider Orange County REMC Orange County REMC offers incentives for members to improve the energy

127

Thomas Jefferson Site Office CX Determinations | U.S. DOE Office of Science  

Office of Science (SC) Website

Thomas Jefferson Site Office CX Thomas Jefferson Site Office CX Determinations Integrated Support Center (ISC) ISC Home About Services Freedom of Information Act (FOIA) Privacy Act Categorical Exclusion Determinations Contact Information Integrated Support Center Roxanne Purucker U.S. Department of Energy 9800 S. Cass Avenue Argonne, IL 60439 P: (630) 252-2110 Larry Kelly U.S. Department of Energy 200 Administration Road Oak Ridge, TN 37830 P: (865) 576-0885 Categorical Exclusion (CX) Determinations Thomas Jefferson Site Office CX Determinations Print Text Size: A A A RSS Feeds FeedbackShare Page As of October 31, 2010, there have been no CX determinations made. Categorical Exclusion Determination Documents (CX Determinations): * Determination Date Name of Action: Description Categorical Exclusion Number External link

128

Thomas Jefferson Site Office CX Determinations | U.S. DOE Office of Science  

Office of Science (SC) Website

Thomas Jefferson Site Office CX Determinations Thomas Jefferson Site Office CX Determinations Safety, Security and Infrastructure (SSI) SSI Home Facilities and Infrastructure Safeguards & Security Environment, Safety and Health (ES&H) Organization Chart .pdf file (82KB) Phone Listing .pdf file (129KB) SC HQ Continuity of Operations (COOP) Implementation Plan .pdf file (307KB) Categorical Exclusion Determinations SLI & SS Budget Contact Information Safety, Security and Infrastructure U.S. Department of Energy SC-31/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-4097 F: (301) 903-7047 Categorical Exclusion (CX) Determinations Thomas Jefferson Site Office CX Determinations Print Text Size: A A A RSS Feeds FeedbackShare Page As of October 31, 2010, there have been no CX determinations made.

129

Questions and Answers - What did Thomas Jefferson do as a scientist?  

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

Who invented magnets? Who invented magnets? Previous Question (Who invented magnets?) Questions and Answers Main Index Next Question (Why does the U.S. use Fahrenheit instead of Celsius?) Why does the U.S. useFahrenheit instead of Celsius? What did Thomas Jefferson do as a scientist? It's true that Thomas Jefferson contributed some new knowledge directly to science and technology. But his main scientific contribution was as a statesman of science. For half a century in public office and in private life, he led the growth of American optimism about science, technology, and the future. Jefferson wished he could be a scientist all the time. When he was leaving the presidency in early 1809, he wrote, "Nature intended me for the tranquil pursuits of science, by rendering them my supreme delight." In

130

VEE-0091 - In the Matter of Jefferson Smurfit Corp. | Department of Energy  

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

1 - In the Matter of Jefferson Smurfit Corp. 1 - In the Matter of Jefferson Smurfit Corp. VEE-0091 - In the Matter of Jefferson Smurfit Corp. This Decision decides the merits of five Applications for Exception filed with the Office of Hearings and Appeals (OHA) of the U.S. Department of Energy (DOE) under the provisions of 10 C.F.R. § 1003.20. See infra Appendix. These Applications concern annual revenues and sales data pertaining to each firm's sale of electricity that the DOE Energy Information Administration (EIA) collects through Form EIA-861, "Annual Electric Power Industry Report." EIA publishes this data, by state, in firm-specific form. The present exception request seeks to have the Applicants' data withheld as confidential. In their Applications for Exception, the Applicants incorporated an Application for Stay to prevent release of some of the

131

SPIN Effects, QCD, and Jefferson Laboratory with 12 GeV electrons  

Science Conference Proceedings (OSTI)

QCD and Spin physics are playing important role in our understanding of hadron structure. I will give a short overview of origin of hadron structure in QCD and highlight modern understanding of the subject. Jefferson Laboratory is undergoing an upgrade that will increase the energy of electron beam up to 12 GeV. JLab is one of the leading facilities in nuclear physics studies and once operational in 2015 JLab 12 will be crucial for future of nuclear physics. I will briefly discuss future studies in four experimental halls of Jefferson Lab.

Prokudin, Alexey [JLAB

2013-11-01T23:59:59.000Z

132

Recirculating Beam Breakup Study for the 12 GeV Upgrade at Jefferson Lab  

Science Conference Proceedings (OSTI)

Two new high gradient C100 cryomodules with a total of 16 new cavities were installed at the end of the CEBAF south linac during the 2011 summer shutdown as part of the 12-GeV upgrade project at Jefferson Lab. We surveyed the higher order modes (HOMs) of these cavities in the Jefferson Lab cryomodule test facility and CEBAF tunnel. We then studied recirculating beam breakup (BBU) in November 2011 to evaluate CEBAF low energy performance, measure transport optics, and evaluate BBU thresholds due to these HOMs. This paper discusses the experiment setup, cavity measurements, machine setup, optics measurements, and lower bounds on BBU thresholds by new cryomodules.

Ilkyoung Shin, Todd Satogata, Shahid Ahmed, Slawomir Bogacz, Mircea Stirbet, Haipeng Wang, Yan Wang, Byung Yunn, Ryan Bodenstein

2012-07-01T23:59:59.000Z

133

Nonconvergence of the plain Newton-min algorithm for linear ...  

E-Print Network (OSTI)

Apr 7, 2010 ... accounts on the use of interior point methods to solve linear ...... mineral precipitation-dissolution reactions by a semismooth Newton method.

134

Environmental Assessment Proposed Improvements at the Thomas Jefferson National Accelerator Facility Newport News, Virginia  

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

84 84 Environmental Assessment Proposed Improvements at the Thomas Jefferson National Accelerator Facility Newport News, Virginia June 2002 U. S. Department of Energy Oak Ridge Operations Oak Ridge, Tennessee DOE/EA-1384 i TABLE OF CONTENTS Executive Summary.....................................................................................................................1 1. INTRODUCTION..................................................................................................................... 6 1.1 PREVIOUS ACTIONS ............................................................................................................................................. 6 1.2 SCOPE OF THIS PROPOSED ACTION..............................................................................................................

135

Cornell Cooperative Extension of Jefferson County Saving $6,000 per Year on Lighting  

E-Print Network (OSTI)

,000 square foot building. The building was formerly a manufacturing plant for air freshenersCornell Cooperative Extension of Jefferson County Saving $6,000 per Year on Lighting Energy comfort and client experience throughout the building · More money to spend on other things Project Cost

Keinan, Alon

136

Remark on Algorithm 702the updated truncated Newton minimization package  

Science Conference Proceedings (OSTI)

A truncated Newton minimization package, TNPACK, was described in ACM Transactions on Mathematical Software 14, 1 (Mar. 1992), pp.46111. Modifications to enhance performance, especially for large-scale minimization of molecular ... Keywords: indefinite preconditioner, modified Cholesky factorization, molecular potential minimization, truncated Newton method

Dexuan Xie; Tamar Schlick

1999-03-01T23:59:59.000Z

137

Orange & Rockland Utils Inc | Open Energy Information  

Open Energy Info (EERE)

Orange & Rockland Utils Inc Orange & Rockland Utils Inc (Redirected from Orange & Rockland) Jump to: navigation, search Name Orange & Rockland Utils Inc Place New York Utility Id 14154 Utility Location Yes Ownership I NERC Location NPCC NERC NPCC Yes Activity Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png SC1 Residential (Multiple Bills, Full Service) Residential SC1 Residential (Multiple Bills, Retail Service) SC1 Residential (Single Bill, Retail Service) SC1 Residential - Residential SC15 Buyback Service SC15 Buyback Service SC16 Flood Lighting Sodium Vapor Overhead and Underground 250w (Customer

138

Orange County - Wind Permitting Standards | Department of Energy  

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

Orange County - Wind Permitting Standards Orange County - Wind Permitting Standards Orange County - Wind Permitting Standards < Back Eligibility Agricultural Commercial Residential Savings Category Wind Buying & Making Electricity Program Info State California Program Type Solar/Wind Permitting Standards Provider OC Planning In December 2010, the County of Orange Board of Supervisors adopted small wind performance and development standards (Ord. No. 10-020) in order to promote distributed generation systems in non-urbanized areas (as defined in Government Code Section 65944(d)(2)) within the unincorporated territory. Permitting standards are for systems of 50 kW or less per customer site, for which the energy is primarily for on-site consumption. Height: For systems 45 feet tall or less, a use permit must be approved by

139

OPERATION AND COMMISSIONING OF THE JEFFERSON LAB UV FEL USING AN SRF DRIVER ERL  

Science Conference Proceedings (OSTI)

We describe the operation and commissioning of the Jefferson Lab UV FEL using a CW SRF ERL driver. Based on the same 135 MeV linear accelerator as the Jefferson Lab 10 kW IR Upgrade FEL, the UV driver ERL uses a bypass geometry to provide transverse phase space control, bunch length compression, and nonlinear aberration compensation necessitating a unique set of commissioning and operational procedures. Additionally, a novel technique to initiate lasing is described. To meet these constraints and accommodate a challenging installation schedule, we adopted a staged commissioning plan with alternating installation and operation periods. This report addresses these issues and presents operational results from on-going beam operations.

R. Legg; S. Benson; G. Biallas; K. Blackburn; J. Boyce; D. Bullard; J. Coleman; C. Dickover; D. Douglas; F. Ellingsworth; P. Evtushenko; F. Hannon; C. Hernandez-Garcia; C. Gould; J. Gubeli; D. Hardy; K. Jordan; M. Klopf; J. Kortze; M. Marchlik; W. Moore; G. Neil; T. Powers; D. Sexton; Michelle D. Shinn; C. Tennant; R. Walker; G. Wilson

2011-03-01T23:59:59.000Z

140

ADVANTAGES OF THE PROGRAM-BASED LOGBOOK SUBMISSION GUI AT JEFFERSON LAB  

Science Conference Proceedings (OSTI)

DTlite is a Tcl/Tk script that is used as the primary interface for making entries into Jefferson Lab's electronic logbooks. DTlite was originally written and implemented by a user to simplify submission of entries into Jefferson Lab?s electronic logbook, but has subsequently been maintained and developed by the controls software group. The use of a separate, script-based tool for logbook submissions (as opposed to a web-based submission tool bundled with the logbook database/interface) provides many advantages to the users, as well as creating many challenges to the programmers and maintainers of the electronic logbook system. The paper describes the advantages and challenges of this design model and how they have affected the development lifecycle of the electronic logbook system.

T. McGuckin

2006-10-24T23:59:59.000Z

Note: This page contains sample records for the topic "newton orange jefferson" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

NEWTON, Ask a Scientist at Argonne National Labs  

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

About NEWTON About Ask A Scientist Education At Argonne Zoonotic Diseases between Cats and Humans Name: Steve Status: student Grade: 4-5 Location: NC Country: USA Date: Fall...

142

Investigating the Site of Newton's Laboratory in Trinity College, Cambridge  

E-Print Network (OSTI)

s Das Alche- mistenlaboratorium von Oberstockstall Ein Vor- bericht zum Stand des Forschungsprojekts. Mitteilungen der Fachgruppe der Geschichte der Chemie 7, 1992, 1119.] 15. Edleston J. (1850). Correspondence of Sir Isaac Newton and Professor Cotes...

Spargo, P E

143

Orange and Rockland Utilities (Electric) - Commercial Efficiency Programs |  

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

Orange and Rockland Utilities (Electric) - Commercial Efficiency Orange and Rockland Utilities (Electric) - Commercial Efficiency Programs Orange and Rockland Utilities (Electric) - Commercial Efficiency Programs < Back Eligibility Commercial Fed. Government Industrial Institutional Local Government Multi-Family Residential Nonprofit Schools State Government Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Other Heat Pumps Appliances & Electronics Commercial Lighting Lighting Maximum Rebate Prescriptive Rebates: 50% of cost Program Info Funding Source System Benefits Charge Start Date 4/1/2010 State New York Program Type Utility Rebate Program Rebate Amount Small Business Lighten Up Energy Savings Evaluation and CFLs: Free A/C A/C > 65 kBTU/h: $35/ton (11.5 EER); $55 (12 EER) Heat Pumps 14 SEER or 11.5 EER: $50-$65/ton

144

Hadronic Multi-Particle Final State Measurements with CLAS at Jefferson Lab  

E-Print Network (OSTI)

Precision measurements in the neutrino sector are becoming increasingly feasible due to the development of relatively high-rate experimental capabilities. These important developments command renewed attention to the systematic corrections needed to interpret the data. Hadronic multi-particle final state measurements made using CLAS at Jefferson Lab, together with a broad theoretical effort that links electro-nucleus and neutrino-nucleus data, will address this problem, and will elucidate long-standing problems in intermediate energy nuclear physics. This new work will ultimately enable precision determinations of fundamental quantities such as the neutrino mixing matrix elements in detailed studies of neutrino oscillations.

W. K. Brooks

2003-11-04T23:59:59.000Z

145

The GlueX experiment: Search for gluonic excitations via photoproduction at Jefferson Lab  

Science Conference Proceedings (OSTI)

Studies of meson spectra via strong decays provide insight regarding QCD at the confinement scale. These studies have led to phenomenological models for QCD such as the constituent quark model. However, QCD allows for a much richer spectrum of meson states which include extra states such as exotics, hybrids, multi-quarks, and glueballs. First discussion of the status of exotic meson searches is given followed by an overview of the progress at Jefferson Lab to double the energy of the machine to 12 GeV, which will allow us to access photoproduction of mesons in search for gluonic excited states.

Eugenio, Paul [Florida State U.

2013-07-01T23:59:59.000Z

146

The study of the elementary photo- and electro-production of kaons at Jefferson Lab  

DOE Green Energy (OSTI)

The subject of electromagnetic production of strangeness, covers an important part of the planned CEBAF experimental program at Jefferson Lab. In this review we will mainly focus on those experiments aiming to investigate the elementary mechanism of the associated production of kaon--hyperon pairs, on hydrogen target, induced by electron and by real photon beams. Complementary experiments, proposed for all the three experimental halls, allow to access a wide kinematical region where different theoretical approaches can be used for the interpretation of the (upcoming) data.

M. Iodice; E. Cisbani; S. Frullani; F. Garibaldi; G.M. Urciuoli; R. De Leo; R. Perrino; M. Sotona

1996-10-01T23:59:59.000Z

147

Jasper-Newton Elec Coop, Inc | Open Energy Information  

Open Energy Info (EERE)

Jasper-Newton Elec Coop, Inc Jasper-Newton Elec Coop, Inc Jump to: navigation, search Name Jasper-Newton Elec Coop, Inc Place Texas Utility Id 9668 Utility Location Yes Ownership C NERC Location SERC NERC ERCOT Yes NERC SERC Yes Activity Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Churches and Schools Service Commercial Farm and Home Services Residential General Service Commercial Large Power Service Industrial Security Lighting-100 W high pressure sodium Lighting Security Lighting-150 W high pressure sodium Lighting Security Lighting-400 W high pressure sodium Lighting

148

City of Newton, Illinois (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Newton Newton Place Illinois Utility Id 13560 Utility Location Yes Ownership M NERC Location RFC NERC RFC Yes ISO MISO Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Commercial Commercial Residential Residential Average Rates Residential: $0.0886/kWh Commercial: $0.0824/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from "http://en.openei.org/w/index.php?title=City_of_Newton,_Illinois_(Utility_Company)&oldid=410028" Categories: EIA Utility Companies and Aliases Utility Companies Organizations

149

Characteristics and fabrication of a 499 MHz superconducting deflecting cavity for the Jefferson Lab 12 geV Upgrade  

Science Conference Proceedings (OSTI)

A 499 MHz parallel bar superconducting deflecting cavity has been designed and optimized for a possible implementation at the Jefferson Lab. Previously the mechanical analysis, mainly stress, was performed. Since then pressure sensitivity was studied further and the cavity parts were fabricated. The prototype cavity is not completed due to the renovation at Jefferson Lab which resulted in the temporary shutdown of the electron beam welding facility. This paper will present the analysis results and facts encountered during fabrication. The unique geometry of the cavity and its required mechanical strength present interesting manufacturing challenges.

HyeKyoung Park, S.U. De Silva, J.R. Delayen

2012-07-01T23:59:59.000Z

150

Thomas Jefferson  

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

2 inches, with a freckled face, rather angular features, hazel-gray eyes, and thick sandy- red hair of silky texture. Although a bit awkward, he had an unusually intelligent...

151

City of Orange City, Iowa (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Orange City Orange City Place Iowa Utility Id 14159 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes Activity Distribution Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Commercial Rate Commercial Industrial Rate Industrial Residential Rate Residential Security Lighting 150 W Lighting Security Lighting 175W Lighting Security Lighting 400 W Lighting Average Rates Residential: $0.0858/kWh Commercial: $0.0863/kWh Industrial: $0.0735/kWh References ↑ "EIA Form EIA-861 Final Data File for 2010 - File1_a" Retrieved from

152

South Orange, New Jersey: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Orange, New Jersey: Energy Resources Orange, New Jersey: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.7489897°, -74.2612583° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.7489897,"lon":-74.2612583,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

153

September/October 1999 Operating in the Red Newton Apiaries  

E-Print Network (OSTI)

September/October 1999 Operating in the Red Newton Apiaries Varroa and Apimondia Sticky Boards Pollinators Booklet UCD Trailer Warning Operating in the Red As with any other business, you cannot operate paralysis virus (SPV), deformed wing virus (DWV), and cloudy wing virus (CWV) all were involved

Hammock, Bruce D.

154

Quantum Corrections to Newton's Law in Resummed Quantum Gravity  

E-Print Network (OSTI)

We present the elements of resummed quantum gravity, a new approach to quantum gravity based on the work of Feynman using the simplest example of a scalar field as the representative matter. We show that we get a UV finite quantum correction to Newton's law.

B. F. L. Ward

2004-11-03T23:59:59.000Z

155

Fast LMS/Newton algorithms for stereophonic acoustic echo cancelation  

Science Conference Proceedings (OSTI)

This paper presents a new class of adaptive filtering algorithms to solve the stereophonic acoustic echo cancelation (AEC) problem in teleconferencing systems. While stereophonic AEC may be seen as a simple generalization of the well-known single-channel ... Keywords: LMS/Newton, adaptive filters, lattice orthogonalization, stereo acoustic echo cancellation (AEC)

Harsha I. K. Rao; Behrouz Farhang-Boroujeny

2009-08-01T23:59:59.000Z

156

Baryon Resonances in the Double Pion Channel at Jefferson Lab (CEBAF): Experimental and Physical Analysis Status and Perspectives  

E-Print Network (OSTI)

Decay of light quark excited baryons in the double pion channel is discussed, as a particular way of investigating poorly know baryon resonances and searching for "missing states" predicted by quark models. A possible approach to the data analysis is discussed and some preliminary data from the CLAS collaboration at Jefferson Laboratory are presented.

Marco Ripani

1999-02-18T23:59:59.000Z

157

High School Research at Jefferson Lab - The Setup and Monitoring of a  

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

12 GeV Safety Systems 12 GeV Safety Systems Previous Project (12 GeV Safety Systems) High School Research Main Index Next Project (Computational Physics) Computational Physics The Setup and Monitoring of a Honeypot at Jefferson Lab A honeypot is software that emulates an operating system and therefore can be used in many projects that should not be tested on a computer that could lose data. For my project it was put onto the network unprotected to see what hackers would do to it. This way we can research what the new or common methods of hacking are. Also, the honeypot does not install any of the malicious software, yet it saves a copy for further analysis. This allows Systems Security to see what bug the program exploits and the information found gives them the ability to fix the issue before hackers

158

The New 2nd-Generation SRF R&D Facility at Jefferson Lab: TEDF  

Science Conference Proceedings (OSTI)

The US Department of Energy has funded a near-complete renovation of the SRF-based accelerator research and development facilities at Jefferson Lab. The project to accomplish this, the Technical and Engineering Development Facility (TEDF) Project has completed the first of two phases. An entirely new 3,100 m{sup 2} purpose-built SRF technical work facility has been constructed and was occupied in summer of 2012. All SRF work processes with the exception of cryogenic testing have been relocated into the new building. All cavity fabrication, processing, thermal treatment, chemistry, cleaning, and assembly work is collected conveniently into a new LEED-certified building. An innovatively designed 800 m2 cleanroom/chemroom suite provides long-term flexibility for support of multiple R&D and construction projects as well as continued process evolution. The characteristics of this first 2nd-generation SRF facility are described.

Reece, Charles E.; Reilly, Anthony V.

2012-09-01T23:59:59.000Z

159

Coherent photoproduction of pi+ from He-3 with CLAS at Jefferson Laboratory  

Science Conference Proceedings (OSTI)

We have measured the differential cross section for the {gamma}{sup 3}He {yields} t{pi}{sup +} reaction. This reaction was studied using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab. Real photons produced with the Hall-B bremsstrahlung tagging system in the energy range from 0.5 to 1.55 GeV were incident on a cryogenic liquid {sup 3}He target. The differential cross sections for the {gamma}{sup 3}He {yields} i{pi}{sup +}t reaction were measured as a function of photon-beam energy and pion-scattering angle Theoretical predictions to date cannot explain the large cross sections except at backward angles, showing that additional components must be added to the model.

Rakhsha Nasseripour, Barry Berman

2011-09-01T23:59:59.000Z

160

Options for an 11 GeV RF Beam Separator for the Jefferson Lab CEBAF Upgrade  

Science Conference Proceedings (OSTI)

The CEBAF accelerator at Jefferson Lab has had, since first demonstration in 1996, the ability to deliver a 5-pass electron beam to experimental halls (A, B, and C) simultaneously. This capability was provided by a set of three, room temperature 499 MHz rf separators in the 5th pass beamline. The separator was two-rod, TEM mode type resonator, which has a high shunt impedance. The maximum rf power to deflect the 6 GeV beams was about 3.4kW. The 12 GeV baseline design does not preserve the capability of separating the 5th pass, 11 GeV beam for the 3 existing halls. Several options for restoring this capability, including extension of the present room temperature system or a new superconducting design in combination with magnetic systems, are under investigation and are presented.

Jean Delayen, Michael Spata, Haipeng Wang

2009-05-01T23:59:59.000Z

Note: This page contains sample records for the topic "newton orange jefferson" 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

Recent Results of Target Single-Spin Asymmetry Experiments at Jefferson Lab  

SciTech Connect

We report recent results from Jefferson Lab Hall A Neutron Transversity experiment (E06-010). Transversely polarized target single-spin asymmetry AUT and beam-target double-spin asymmetry A{sub LT} have been measured in semi-inclusive deep-inelastic scattering (SIDIS) reactions on a polarized neutron ({sup 3}He) target. Collins-type and Sivers-type asymmetries have been extracted from A{sub UT} for charged pion SIDIS productions, which are sensitive to quark transversity and Sivers distributions, correspondingly. Double spin asymmetry A{sub LT} is sensitive to a specific quark transverse momentum dependent parton distribution (TMD), the so-called transverse helicity (g{sub 1T} ) distributions. In addition, target single-spin asymmetries A{sub y} in inclusive electron scattering on a transversely polarized {sup 3}He target in quasi-elastic and deep inelastic kinematics were also measured in Hall A.

Jiang, Xiaodong [Los Alamos National Lab

2013-08-01T23:59:59.000Z

162

Performance and results of the RICH detector for kaon physics in Hall A at Jefferson Lab  

SciTech Connect

A proximity focusing RICH detector has been constructed for the hadron High Resolution Spectrometer (HRS) of Jefferson Lab Experimental Hall-A. This detector is intended to provide excellent hadron identification up to a momentum of 2.5 GeV/c. The RICH uses a 15 mm thick liquid perfluorohexane radiator in proximity focusing geometry to produce Cherenkov photons traversing a 100 mm thick proximity gap filled with pure methane and converted into electrons by a thin film of CsI deposited on the cathode plane of a MWPC. The detector has been successfully employed in the fixed target, high luminosity and high resolution hypernuclear spectroscopy experiment. With its use as a kaon identifier in the 2 GeV/c region, the very large contribution from pions and protons to the hypernuclear spectrum was reduced to a negligible level. The basic parameters and the resulting performance obtained during the experiment are reported in this paper.

M. Iodice; E. Cisbani; S. Colilli; F. Cusanno; S. Frullani; R. Fratoni; F. Garibaldi; M. Gricia; M. Lucentini; L. Pierangeli; F. Santavenere; G.M. Urciuoli; P. Veneroni; G. De Cataldo; R. De Leo; D. Di Bari; L. Lagamba; E. Nappi; S. Marrone; B. Kross; J.J. LeRose; B. Reitz; J. Segal; C. Zorn and H. Breuer

2005-11-01T23:59:59.000Z

163

An overview of the planned Jefferson Lab 12-GeV helium refrigerator upgrade  

SciTech Connect

In February 2006, Jefferson Laboratory in Newport News, VA, received Critical Decision 1 (CD-1) approval to proceed with the engineering and design of the long anticipated upgrade to increase the beam energy of CEBAF, the Continuous Electron Beam Accelerator Facility, from 6 GeV to 12 GeV. This will require the installation of 10 new cryomodules, and additional 2.1-K refrigeration beyond the available 4600 W to handle the increased heat loads. Additionally, a new experimental hall, Hall D, is planned that will require the installation of a small, available refrigerator. This paper will present an overview of the integration of the new proposed refrigeration system into CEBAF, the installation of the available refrigerator for Hall D, and includes planned work scope, current schedule plans and project status.

Arenius, Dana; Creel, Jonathan; Dixon, Kelly; Ganni, Venkatarao; Knudsen, Peter; Sidi-Yekhlef, Ahmed; Wright, Mathew

2008-03-01T23:59:59.000Z

164

Exploration of deeply virtual Compton scattering on the neutron in the Hall A of Jefferson Laboratory  

SciTech Connect

Generalized Parton Distributions (GPDs) are universal functions which provide a comprehensive description of hadron properties in terms of quarks and gluons. Deeply Virtual Compton Scattering (DVCS) is the simplest hard exclusive process involving GPDs. In particular, the DVCS on the neutron is mostly sensitive to E, the less constrained GPD, wich allows to access to the quark angular momentum. The first dedicated DVCS experiment on the neutron ran in the Hall A of Jefferson Lab in fall 2004. The high luminosity of the experiment and the resulting background rate recquired specific devices which are decribed in this document. The analysis methods and the experiment results, leading to preliminary constraints on the GPD E, are presented.

Malek Mazouz

2006-12-08T23:59:59.000Z

165

Preliminary Results from Integrating Compton Photon Polarimetry in Hall A of Jefferson Lab  

SciTech Connect

A wide range of nucleon and nuclear structure experiments in Jefferson Lab's Hall A require precise, continuous measurements of the polarization of the electron beam. In our Compton polarimeter, electrons are scattered off photons in a Fabry-Perot cavity; by measuring an asymmetry in the integrated signal of the scattered photons detected in a GSO crystal, we can make non-invasive, continuous measurements of the beam polarization. Our goal is to achieve 1% statistical error within two hours of running. We discuss the design and commissioning of an upgrade to this apparatus, and report preliminary results for experiments conducted at beam energies from 3.5 to 5.9 GeV and photon rates from 5 to 100 kHz.

D. Parno, M. Friend, F. Benmokhtar, G. Franklin, R. Michaels, S. Nanda, B. Quinn, P. Souder

2011-09-01T23:59:59.000Z

166

New photomultiplier active base for Hall C Jefferson Lab lead tungstate calorimeter  

Science Conference Proceedings (OSTI)

A new photomultiplier tube active base was designed and tested. The base combines active voltage division circuit and fast amplifier, powered by the current flowing through voltage divider. This base is developed to upgrade older photomultiplier bases of Jefferson Lab lead-tungsten calorimeter (about ?1200 crystals of PbWO{sub 4} from the PrimEx experimental setup). This is needed for the extension of detectors' rate capability to meet requirements of new Hall C proposal PR12-11-102 of measurements of the L/T separated cross sections and their ratio R = ?L/?T in neutral-pion p(e,e??0)p deep exclusive and p(p(e,e??{sup 0})p)X semi-inclusive scattering regions. New active base is direct replacement of older passive base circuit without adding of additional power or signal lines. However, it extends detectors rate capability with factor over 20. Moreover, transistorized voltage divider improves detector's amplitude resolution due to reduction of photomultiplier gain dependence from tube anode current. The PMT active base is the invention disclosed in V. Popov's U.S. Patent No. 6,791,269, which successfully works over ten years in several Jefferson Lab Cherenkov detectors. The following design is a new revised and improved electronic circuit with better gain stability and linearity in challenge to meet requirements of new Hall C experimental setup. New active base performance was tested using fast LED light source and Pr:LuAG scintillator and gamma sources. Electronics radiation hardness was tested on JLab accelerator. Results of testing R4125 Hamamatsu photomultiplier tube in new active base are presented.

Popov, Vladimir E. [JLAB; Mkrtchyan, Hamlet G. [Artem Alikhanian National Laboratory

2012-11-01T23:59:59.000Z

167

Orange County Great Park Welcomes U.S. Department of Energy...  

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

CONTACT: MARCUS GINNATY 949-724-6574 Orange County Great Park Welcomes U.S. Department of Energy Solar Decathlon 2013 Collegiate Teams * Representatives from 20 collegiate teams...

168

Orang-utan feeding behaviour in Sabangau, Central Kalimantan  

E-Print Network (OSTI)

, Andrea Hing, Alexandra Gray, Okto, Ella, Marie Hammard and many OuTrop volunteers. I would also like to thank Laura DArcy, Laura Graham, Angela viii Benton-Browne, Ben Buckley, Marc Dragiewicz, Carly Waterman and Rosalie Dench. The amazing Ibu... also Muir et al., 1998, 2000; Warren et al., 2001; Brandon-Jones et al., 2004). The different (sub-) species will hybridise in captivity, but survival rates among Sumatra- Borneo hybrids are much lower, and captive Bornean orang-utans, many...

Harrison, Mark Edward

2009-04-14T23:59:59.000Z

169

MHK Projects/Newton Bend Project | Open Energy Information  

Open Energy Info (EERE)

Newton Bend Project Newton Bend Project < MHK Projects Jump to: navigation, search << Return to the MHK database homepage Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":5,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"500px","height":"350px","centre":false,"title":"","label":"","icon":"File:Aquamarine-marker.png","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.218,"lon":-90.9891,"alt":0,"address":"","icon":"http:\/\/prod-http-80-800498448.us-east-1.elb.amazonaws.com\/w\/images\/7\/74\/Aquamarine-marker.png","group":"","inlineLabel":"","visitedicon":""}]}

170

City of Newton Falls, Ohio (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Newton Falls Newton Falls Place Ohio Utility Id 13563 Utility Location Yes Ownership M NERC Location RFC NERC RFC Yes Activity Distribution Yes Activity Bundled Services Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png COMM city owned equip inside city limits Commercial COMM city owned equip inside city limits interuptible electric service Commercial COMM city owned equip outside city limits Commercial COMM cust owned equip inside city limits Commercial COMM cust owned equip inside city limits interuptible electric service Commercial COMM cust owned equip outside city limits

171

NEWTON, Ask a Scientist at Argonne National Labs  

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

Hard Drive Field Separation Hard Drive Field Separation Name: Dan P. Status: other Age: 40s Location: NY Date: N/A Question: You have an excellent answer to the question of "How does a computers hard drive work...store and send data?" (see http://www.newton.dep.anl.gov/newton/askasci/1995/compsci/CSI36.HTM) but could you explain further... What separates the magnetic field so that the hard drive knows the difference between a magnetic field that is one bit in size and a magnetic field that is 100 bits long? Are there spaces between each magnetic field? If so how can it tell the difference between a non-magnetic field that is one bit in size and a non-magnetic field that is 100 bits long? Replies: That is a good question. What really happens on a hard disk is a little more complicated than the simple magnetized-bit picture.

172

Mpemba effect, Newton cooling law and heat transfer equation  

E-Print Network (OSTI)

In this work we suggest a simple theoretical solution of the Mpemba effect in full agreement with known experimental data. This solution follows simply as an especial approximation (linearization) of the usual heat (transfer) equation, precisely linearization of the second derivation of the space part of the temperature function (as it is well-known Newton cooling law can be considered as the effective approximation of the heat (transfer) equation for constant space part of the temperature function).

Vladan Pankovic; Darko V. Kapor

2010-05-06T23:59:59.000Z

173

Reflectance Vis/NIR spectroscopy for nondestructive taste characterization of Valencia oranges  

Science Conference Proceedings (OSTI)

The feasibility of reflectance Vis/NIR spectroscopy was investigated for taste characterization of Valencia oranges based on taste attributes including soluble solids content (SSC) and titratable acidity (TA), as well as taste indices including SSC to ... Keywords: BrimA, Nondestructive, Taste, Valencia orange, Vis/NIR spectroscopy

Bahareh Jamshidi; Saeid Minaei; Ezzedin Mohajerani; Hassan Ghassemian

2012-07-01T23:59:59.000Z

174

California Society of Professional Engineers and UCI Host Orange County MATHCOUNTS  

E-Print Network (OSTI)

California Society of Professional Engineers and UCI Host Orange County MATHCOUNTS Competition Juan Capistrano converged at the Student Union of the University of California at Irvine on Saturday was conducted by the Orange County Chapter of the California Society of Professional Engineers (CSPE

Russo, Bernard

175

On inverse scattering at high energies for the multidimensional Newton equation in electromagnetic field  

E-Print Network (OSTI)

We consider the multidimensional (nonrelativistic) Newton equation in a static electromagnetic field $$\\ddot x = F(x,\\dot x), F(x,\\dot x)=-\

Alexandre Jollivet

2007-09-29T23:59:59.000Z

176

Optimization Online - A New Full-Newton step $O(n)$ Infeasible ...  

E-Print Network (OSTI)

Jul 9, 2008 ... A New Full-Newton step $O(n)$ Infeasible Interior-Point Algorithm for Semidefinite Optimization. Hossein Mansouri (H.Mansouri ***at***...

177

Design of the Proposed Low Energy Ion Collider Ring at Jefferson Lab  

SciTech Connect

The polarized Medium energy Electron-Ion Collider (MEIC) envisioned at Jefferson Lab will cover a range of center-of-mass energies up to 65 GeV. The present MEIC design could also allow the accommodation of low energy electron-ion collisions (LEIC) for additional science reach. This paper presents the first design of the low energy ion collider ring which is converted from the large ion booster of MEIC. It can reach up to 25 GeV energy for protons and equivalent ion energies of the same magnetic rigidity. An interaction region and an electron cooler designed for MEIC are integrated into the low energy collider ring, in addition to other required new elements including crab cavities and ion spin rotators, for later reuse in MEIC itself. A pair of vertical chicanes which brings the low energy ion beams to the plane of the electron ring and back to the low energy ion ring are also part of the design.

Nissen, Edward W. [JLAB; Lin, Fanglei [JLAB; Morozov, Vasiliy [JLAB; Zhang, Yuhong [JLAB

2013-06-01T23:59:59.000Z

178

Natural radioactivity in geothermal waters, Alhambra Hot Springs and nearby areas, Jefferson County, Montana  

DOE Green Energy (OSTI)

Radioactive hot springs issue from a fault zone in crystalline rock of the Boulder batholith at Alhambra, Jefferson County, in southwestern Montana. The discharge contains high concentrations of radon, and the gross activity and the concentration of radium-226 exceed maximum levels recommended by the Environmental Protection Agency for drinking water. Part of the discharge is diverted for space heating, bathing, and domestic use. The radioactive thermal waters at measured temperatures of about 60/sup 0/C are of the sodium bicarbonate type and saturated with respect to calcium carbonate. Radium-226 in the rock and on fractured surfaces or coprecipitated with calcium carbonate probably is the principal source of radon that is dissolved in the thermal water and discharged with other gases from some wells and springs. Local surface water and shallow ground water are of the calcium bicarbonate type and exhibit low background radioactivity. The temperature, percent sodium, and radioactivity of mixed waters adjacent to the fault zone increase with depth. Samples from most of the major hot springs in southwestern Montana have been analyzed for gross alpha and beta. The high level of radioactivity at Alhambra appears to be related to leaching of radioactive material from fractured siliceous veins by ascending thermal waters, and is not a normal characteristic of hot springs issuing from fractured crystalline rock in Montana.

Leonard, R.B.; Janzer, W.J.

1977-08-01T23:59:59.000Z

179

Electroproduction de pions neutres dans le Hall A au Jefferson Laboratory  

SciTech Connect

The past decade has seen a strong evolution of the study of the hadron structure through exclusive processes, allowing to access to a more complete description of this structure. Exclusive processes include DVCS (Deeply Virtual Compton Scattering) as well as hard exclusive meson production. This document is particularly focussed on the latter, and more particularly on exclusive neutral pion production. In this thesis is described the analysis of triple coincidence events H(e, e'{gamma}{gamma})X, which were a consequent by-product of the DVCS experiment which occured during Fall 2004 at Jefferson Lab Hall A, to extract the ep {yields} ep{pi}{sup 0} cross section. This cross section has been measured at two values of four-momentum transfer Q{sup 2} = 1.9 GeV{sup 2} and Q{sup 2} = 2.3 GeV{sup 2}. The statistical precision for these measurements is achieved at better than 5 %. The kinematic range allows to study the evolution of the extracted cross section as a function of Q{sup 2} and W. Results are be confronted with Regge inspired calculations and Generalized (GPD) predictions. An intepretation of our data within the framework of semi-inclusive deep inelastic scattering is also discussed.

Eric Fuchey

2010-06-01T23:59:59.000Z

180

Orange & Rockland Utils Inc | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Jump to: navigation, search Name Orange & Rockland Utils Inc Place New York Utility Id 14154 Utility Location Yes Ownership I NERC Location NPCC NERC NPCC Yes Activity Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png SC1 Residential (Multiple Bills, Full Service) Residential SC1 Residential (Multiple Bills, Retail Service) SC1 Residential (Single Bill, Retail Service) SC1 Residential - Residential SC15 Buyback Service SC15 Buyback Service SC16 Flood Lighting Sodium Vapor Overhead and Underground 250w (Customer owned, retail service, single bill)

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181

Orange County Rural E M C | Open Energy Information  

Open Energy Info (EERE)

County Rural E M C County Rural E M C Jump to: navigation, search Name Orange County Rural E M C Place Indiana Utility Id 14160 Utility Location Yes Ownership C NERC Location RFC NERC RFC Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Rate 101- 2012 Rate Schedule for Standard Service Residential Rate 104 and 106- 2012 Rate Schedule for Electric Thermal Storage (ETS) Residential Rate 105- 2012 Rate Schedule for Dual Fuel Service Commercial Rate 177- 2012 Rate Schedule for Security Lighting, Security Lighting- 100 W HPS (45 kwh) Lighting Rate 177- 2012 Rate Schedule for Security Lighting, Security Lighting- 175W

182

Nine Years of XMM-Newton Pipeline: Experience and Feedback  

Science Conference Proceedings (OSTI)

The Strasbourg Astronomical Observatory is member of the Survey Science Centre (SSC) of the XMM-Newton satellite. Among other responsibilities, we provide a database access to the 2XMMi catalogue and run the part of the data processing pipeline performing the cross-correlation of EPIC sources with archival catalogs. These tasks were all developed in Strasbourg. Pipeline processing is flawlessly in operation since 1999. We describe here the work load and infrastructure setup in Strasbourg to support SSC activities. Our nine year long SSC experience could be used in the framework of the Simbol-X ground segment.

Michel, Laurent; Motch, Christian [CNRS, Universite de Strasbourg, Observatoire Astronomique, 11 rue de l'Universite, 67000 Strasbourg (France)

2009-05-11T23:59:59.000Z

183

Rippled Cosmological Dark Matter from Damped Oscillating Newton Constant  

E-Print Network (OSTI)

Let the reciprocal Newton 'constant' be an apparently non-dynamical Brans-Dicke scalar field damped oscillating towards its General Relativistic VEV. We show, without introducing additional matter fields or dust, that the corresponding cosmological evolution averagely resembles, in the Jordan frame, the familiar dark radiation -> dark matter -> dark energy domination sequence. The fingerprints of our theory are fine ripples, hopefully testable, in the FRW scale factor; they die away at the General Relativity limit. The possibility that the Brans-Dicke scalar also serves as the inflaton is favorably examined.

Aharon Davidson

2004-09-15T23:59:59.000Z

184

Application of a New Adjoint Newton Algorithm to the 3D ARPS Storm-Scale Model Using Simulated Data  

Science Conference Proceedings (OSTI)

The adjoint Newton algorithm (ANA) is based on the first- and second-order adjoint techniques allowing one to obtain the Newton line search direction by integrating a tangent linear model backward in time (with negative time steps). Moreover, ...

Zhi Wang; Kelvin K. Droegemeier; L. White; I. M. Navon

1997-10-01T23:59:59.000Z

185

A Newton method using exact jacobians for solving fluid-structure coupling  

Science Conference Proceedings (OSTI)

This paper aims at introducing a partitioned Newton based method for solving nonlinear coupled systems arising in the numerical approximation of fluid-structure interaction problems. We provide a method which characteristic lies in the use of exact cross ... Keywords: ALE formulation, Fluid-structure interaction, Full coupled schemes, Haemodynamics, Navier-Stokes equations, Newton methods, Shape sensitivity analysis

Miguel ngel Fernndez; Marwan Moubachir

2005-01-01T23:59:59.000Z

186

Physics Opportunities with the 12 GeV Upgrade at Jefferson Lab  

SciTech Connect

We are at the dawn of a new era in the study of hadronic nuclear physics. The non-Abelian nature of Quantum Chromodynamics (QCD) and the resulting strong coupling at low energies represent a significant challenge to nuclear and particle physicists. The last decade has seen the development of new theoretical and experimental tools to quantitatively study the nature of confinement and the structure of hadrons comprised of light quarks and gluons. Together these will allow both the spectrum and the structure of hadrons to be elucidated in unprecedented detail. Exotic mesons that result from excitation of the gluon field will be explored. Multidimensional images of hadrons with great promise to reveal the dynamics of the key underlying degrees of freedom will be produced. In particular, these multidimensional distributions open a new window on the elusive spin content of the nucleon through observables that are directly related to the orbital angular momenta of quarks and gluons. Moreover, computational techniques in Lattice QCD now promise to provide insightful and quantitative predictions that can be meaningfully confronted with, and elucidated by, forthcoming experimental data. In addition, the development of extremely high intensity, highly polarized and extraordinarily stable beams of electrons provides innovative opportunities for probing (and extending) the Standard Model, both through parity violation studies and searches for new particles. Thus the 12 GeV upgrade of the Continuous Electron Beam Accelerator Facility (CEBAF) at Jefferson Lab will enable a new experimental program with substantial discovery potential to address these and other important topics in nuclear, hadronic and electroweak physics.

Dudek, Jozef; Essig, Rouven; Kumar, Krishna; Meyer, Curtis; McKeown, Robert; Meziani, Zein Eddine; Miller, Gerald A; Pennington, Michael; Richards, David; Weinstein, Larry

2012-08-01T23:59:59.000Z

187

The Jefferson Lab program: From 6 GeV operations to the 12 GeV upgrade  

Science Conference Proceedings (OSTI)

The Thomas Jefferson National Laboratory and the CEBAF accelerator operated for more than a decade, running a comprehensive scientific program that improved our understanding of the strong interaction. The facility is now moving toward an upgrade of the machine, from 6 to 12 GeV; a new experimental hall will be added and the equipment of the three existing halls will be enhanced. In this contribution some selected results from the rich physics program run at JLab, as well as the prospects for the near future, will be presented.

Marco Battaglieri

2012-04-01T23:59:59.000Z

188

Feasibility Test Run of C-12(e,e'K{sup +}) Reaction at Thomas Jefferson National Accelerator Facility  

DOE Green Energy (OSTI)

The high quality and high duty factor (100%) electron beam at Jefferson Lab offers an opportunity to broaden their view of hypernuclear physics by studying the (e,e{prime}K{sup +}) reaction with high resolution. The present data represent a feasibility study of such a reaction on a carbon target. The test run was carried out during experiments E91-16 (Electroproduction of Kaons and Light Hypernuclei) and E93-18 (Kaon Electroproduction on p(e,e{prime}K{sup +})Y). These two experiments used liquid deuterium and hydrogen targets, respectively. There exist data on an aluminum target for the background calibration of the liquid targets which are suitable also for a feasibility study of electroproduction of hypernuclei. These data are still under analysis. The goal of this test run is to evaluate issues concerned with the electroproduction of hypernuclei. These issues include: (1) the quasi-free production rate, which had not been measured previously, (2) random coincidence background, (3) keon identification over a possibly large hadronic background, and (4) possible evaluation of the production rate of the bound hypernuclear structures. This test run will supply significant knowledge for running high quality hypernuclear experiments at Jefferson Lab. The spectroscopy of hypernuclei has been studied mainly in two ways: the strangeness-exchange reaction (K{sup -}, {pi}{sup -}), and associated strangeness production ({pi}{sup +}, K{sup +}). The (e,e{prime}K{sup +}) reaction has the advantage of exciting both natural- and unnatural-parity states and the possibility of obtaining good energy resolution. The cross section for the (e,e{prime}K{sup +}) reaction is about a hundred times smaller than for the corresponding hadronic production reactions but it is compensated for by the availability of high intensity and high duty factor electron beams. In order to optimize the production rate, the kinematic setting requires both the scattered electron and kaon to be detected at very forward angles. The test run was not optimized for hypernuclear production, but it serves as an important technical evaluation for future hypernuclear programs at Jefferson Lab. The first high-resolution spectroscopy experiment on p-shell lambda hypernuclei is tentatively scheduled to run in 1999 in Hall C at Jefferson Lab.

Wendy Hinton

1998-08-01T23:59:59.000Z

189

The search for gluonic degrees of freedom in QCD using the GlueX facility at Jefferson Lab  

Science Conference Proceedings (OSTI)

The search for gluonic degrees of freedom in mesons is an experimental challenge. The most promising approach is to look for mesons with exotic quantum numbers that can not be described by quark degrees of freedom only. The GlueX experiment at Jefferson Lab in Hall-D, currently under construction, will search for such hybrid mesons with exotic quantum numbers by scattering a linearly polarized high energetic photon beam off a liquid hydrogen target. An amplitude analysis will be employed to search for such resonances in the data and determine their quantum numbers.

Benedikt Zihlmann

2011-05-01T23:59:59.000Z

190

Light Vector Meson Photoproduction off of H at Jefferson Lab and rho-omega Interference in the Leptonic Decay Channel  

SciTech Connect

Recent studies of light vector meson production in heavy nuclear targets has generated interest in {rho}-{omega} interference in the leptonic e{sup +}e{sup -} decay channel. An experimental study of the elementary process provides valuable input for theoretical models and calculations. In experiment E04-005 (g12), high statistics photoproduction data has been taken in Jefferson Lab's Hall B with the Cebaf Large Acceptance Spectrometer (CLAS). The invariant mass spectrum is fitted with two interfering relativistic Breit-Wigner functions to determine the interference phase. Preliminary analysis indicate a measurable {rho}-{omega} interference.

Chaden Djalali

2011-12-01T23:59:59.000Z

191

The design and performance of the electromagnetic calorimeters in Hall C at Jefferson Lab  

Science Conference Proceedings (OSTI)

The design and performance of the electromagnetic calorimeters in the magnetic spectrometers in Hall C at Jefferson Lab are presented. For the existing HMS and SOS spectrometers, construction information and comparisons of simulated and experimental results are presented. The design and simulated performance for a new calorimeter to be used in the new SHMS spectrometer is also presented. We have developed and constructed electromagnetic calorimeters from TF-1 type lead-glass blocks for the HMS and SOS magnetic spectrometers at JLab Hall C. The HMS/SOS calorimeters are of identical design and construction except for their total size. Blocks of dimension 10 cm 10 cm 70 cm are arranged in four planes and stacked 13 and 11 blocks high in the HMS and SOS respectively. The energy resolution of these calorimeters is better than 6%/?E, and pion/electron (?/e) separation of about 100:1 has been achieved in energy range 15 GeV. Good agreement has been observed between the experimental and GEANT4 simulated energy resolutions. The HMS/SOS calorimeters have been used nearly in all Hall C experiments, providing good energy resolution and a high pion suppression factor. No significant deterioration in their performance has been observed in the course of use since 1994. For the SHMS spectrometer, presently under construction, details on the calorimeter design and accompanying GEANT4 simulation efforts are given. A Preshower+Shower design was selected as the most cost-effective among several design choices. The preshower will consist of a layer of 28 modules with TF-1 type lead glass radiators, stacked in two columns. The shower part will consist of 224 modules with F-101 type lead glass radiators, stacked in a fly's eye configuration of 14 columns and 16 rows. The active area of 120 130 cm(2) will encompass the beam envelope at the calorimeter. The anticipated performance of the new calorimeter is simulated over the full momentum range of the SHMS, predicting resolution and yields similar to the HMS calorimeter. Good electron/hadron separation can be achieved by using energy deposition in the Preshower along with total energy deposition in the calorimeter. In this case the PID capability is similar to or better than that attainable with HMS calorimeter, with a pion suppression factor of a few hundreds predicted for 99% electron detection efficiency.

Vardan Tadevosyan, Hamlet Mkrtchyan, Arshak Asaturyan, Arthur Mkrtchyan, Simon Zhamkochyan

2012-12-01T23:59:59.000Z

192

NEWTON, Ask a Scientist at Argonne National Labs  

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

Jeff Buzby Ph.D. Jeff Buzby Ph.D. I am a Senior Scientist in Molecular Immunology with a Biochemistry Ph.D., and have studied gene expression in cyanobacteria, plants, and humans. I'm investigating developmental regulation of the immune & coagulation responses at Children's Hospital of Orange County, CA. Previously, I worked on identifying genetic factors that control the response of plants to light as a postdoctoral fellow at UCLA. My Ph.D. dissertation designed a gene transfer system for cyanobacteria (blue-green algae) at Penn State Univ., and my first postdoctoral project utilized this system to find cyanobacterial genes that confer herbicide-resistance in plants. I am also developing a WWW-based biotechnology consultanting service, Molecular Biotech Consultants (http://www.molecularbiotech.com).

193

NEWTON, Ask a Scientist at Argonne National Labs  

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

Nathan A. Unterman M.S. Nathan A. Unterman M.S. Email: nunterman@newton.dep.anl.gov FORMAL EDUCATION M.S. Science Teaching, 1988, DePaul University. Concentration in Secondary Science Curriculum Design. Courses included science content as well as curriculum design. B.S. Astronomy, 1975, University of Michigan. Minor in Physics and Mathematics, with courses including geology, meteorology, and chemistry. CONTINUING EDUCATION Illinois Oil and Natural Gas Education Conference 2012 Illinois Crude Oil and Natural Gas Core Energy Science and Math Curriculum Workshop 2012 Illinois Association of Aggregate Producers Rocks, Minerals, and Mining in Today's Society 2012 Illinois Coal Education Conference 2012 CERN High School Teachers International Program in high energy physics and physics education. Geneva, Switzerland 2011 Purdue University, Calumet ASM International Materials Science Camp 2011

194

NEWTON, Ask a Scientist at Argonne National Labs  

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

Beets and Bacteria Beets and Bacteria Name: Arlene Status: other Grade: 6-8 Location: IL Country: USA Date: Fall 2011 Question: I found an experiment at the pbs.org/teachers website that evaluates different handwashing techniques by swabbing palms, nails, and in between fingers after different types of handwashing. These swabs are then "plated" on canned beets placed inside of a petri dish. Does this sound like a realistic and safe experiment for middle school students? NEWTON BBS does not recommend growing/culturing bacteria without the supervision of a microbiologist, and a properly equipped microbiology laboratory. Safety is our main concern! Growing dangerous bacteria species unknowingly is a real possibility and serious illness may occur without proper handling techniques. Furthermore, without proper bacterial disposal procedures such as an autoclave can guarantee, there is a danger to anyone who comes in contact after disposal.

195

The perihelion of Mercury advance calculated in Newton's theory  

E-Print Network (OSTI)

Three radii are associated with a circle: the "geodesic radius" R_1 which is the distance from circle's center to its perimeter, the "circumferential radius" R_2 which is the length of the perimeter divided by 2 pi and the "curvature radius" R_3 which is circle's curvature radius in the Frenet sense. In the flat Euclidean geometry it is R_1 = R_2 = R_3, but in a curved space these three radii are different. I show that although Newton's dynamics uses Euclidean geometry, its equations that describe circular motion in spherical gravity always unambiguously refer to one particular radius of the three --- geodesic, circumferential, or curvature. For example, the gravitational force is given by F = -GMm/(R_2)^2, and the centrifugal force by mv^2/R_3. Building on this, I derive a Newtonian formula for the perihelion of Mercury advance.

Marek A. Abramowicz

2012-11-22T23:59:59.000Z

196

NEWTON, Ask a Scientist at Argonne National Labs  

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

Plant Phases Plant Phases Name: Mansi Status: student Grade: other Location: Outside U.S. Country: India Date: Spring 2012 Question: What is the period between 2 reproductive phase of a perennial plant called? What happens in this phase?does plant after reproductive phase re-enters vegetative phase in perennial plants? Replies: Right, the question is ambiguous. Perhaps referring to vegetative and reproductive periods in plants? Of course, this all depends upon the plant species in question, and different for ferns and mosses (alternation of generations) vs. angiosperms and gymnosperms. The following might be helpful to the individual: http://www.jstor.org/stable/1514428 http://www.nios.ac.in/srsec314newE/PDFBIO.EL19.pdf NEWTON BBS Ask A Scientist service receives about 200-300 requests per day. If you did not receive an answer it could be due to one of the following reasons:

197

An XMM-Newton Observation of Abell 2597  

E-Print Network (OSTI)

We report on a 120 ks XMM-Newton observation of the galaxy cluster Abell 2597. Results from both the European Photon Imaging Camera (EPIC) and the Reflection Grating Spectrometer (RGS) are presented. From EPIC we obtain radial profiles of temperature, density and abundance, and use these to derive cooling time and entropy. We illustrate corrections to these profiles for projection and point spread function (PSF) effects. At the spatial resolution available to XMM-Newton, the temperature declines by around a factor of two in the central 150 kpc or so in radius, and the abundance increases from about one-fifth to over one-half solar. The cooling time is less than 10 Gyr inside a radius of 130 kpc. EPIC fits to the central region are consistent with a cooling flow of around 100 solar masses per year. Broad-band fits to the RGS spectra extracted from the central 2 arcmin are also consistent with a cooling flow of the same magnitude; with a preferred low-temperature cut-off of essentially zero. The data appear to suggest (albeit at low significance levels below formal detection limits) the presence of the important thermometer lines from Fe XVII at 15, 17 Angstrom rest wavelength, characteristic of gas at temperatures ~ 0.3 keV. The measured flux in each line is converted to a mass deposition estimate by comparison with a classical cooling flow model, and once again values at the level of 100 solar masses per year are obtained. These mass deposition rates, whilst lower than those of previous generations of X-ray observatories, are consistent with those obtained from UV data for this object. This raises the possibility of a classical cooling flow, at the level of around 100 solar masses per year, cooling from 4 keV by more than two orders of magnitude in temperature.

R. Glenn Morris; A. C. Fabian

2005-01-17T23:59:59.000Z

198

Depleted uranium risk assessment for Jefferson Proving Ground using data from environmental monitoring and site characterization. Final report  

SciTech Connect

This report documents the third risk assessment completed for the depleted uranium (DU) munitions testing range at Jefferson Proving Ground (JPG), Indiana, for the U.S. Army Test and Evaluation command. Jefferson Proving Ground was closed in 1995 under the Base Realignment and Closure Act and the testing mission was moved to Yuma Proving Ground. As part of the closure of JPG, assessments of potential adverse health effects to humans and the ecosystem were conducted. This report integrates recent information obtained from site characterization surveys at JPG with environmental monitoring data collected from 1983 through 1994 during DU testing. Three exposure scenarios were evaluated for potential adverse effects to human health: an occasional use scenario and two farming scenarios. Human exposure was minimal from occasional use, but significant risk were predicted from the farming scenarios when contaminated groundwater was used by site occupants. The human health risk assessments do not consider the significant risk posed by accidents with unexploded ordnance. Exposures of white-tailed deer to DU were also estimated in this study, and exposure rates result in no significant increase in either toxicological or radiological risks. The results of this study indicate that remediation of the DU impact area would not substantially reduce already low risks to humans and the ecosystem, and that managed access to JPG is a reasonable model for future land use options.

Ebinger, M.H.; Hansen, W.R.

1996-10-01T23:59:59.000Z

199

A High-Energy High-Luminosity p+-p* Collider David V. Neuffer, CEBAF', 12000 Jefferson Avenue, Newport News VA 23692  

E-Print Network (OSTI)

A High-Energy High-Luminosity p+-p* Collider David V. Neuffer, CEBAF', 12000 Jefferson Avenue be costly and does not use our ability to recirculate p's. A recirculating linac (RLA) like CEBAF" can and M. S. Zolotorev, Phys. Rev. Lett.71, 4146 (1993). 11. CEBAF Design Report, CEBAF, Newport News VA

McDonald, Kirk

200

NEWTON, Ask a Scientist at Argonne National Labs  

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

Fruit Battery and Current Fruit Battery and Current Name: Rahil Status: student Grade: 4-5 Location: MN Country: USA Date: Winter 2011-2012 Question: Hello, I am a 5th grade student and doing "Fruit Battery" experiment for my science fair. My question is "What produce requires the least amount (in mass) to make a battery that lasts the longest?" I set up trials using potato, apple, orange and lemon. For all these produces when I created the first voltaic cell and measured the open and closed circuit voltages using multimeter, they were same, I am using 2.6V LED to light up which has no resistance. I also did not use any other external resistor. After adding 2nd voltaic cell to the circuit in series, the open and closed voltages differ by some amount. I want to know the reason behind the difference in the open and closed circuit voltages when there is more than one voltaic cell.. Also I tried to measure the current but it always started with one value and kept going down and never got stabilized at one value. May I know the reason for this as well?

Note: This page contains sample records for the topic "newton orange jefferson" 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

Large area, high spatial resolution tracker for new generation of high luminosity experiments in Hall A at Jefferson Lab  

Science Conference Proceedings (OSTI)

In 2014 the CEBAF electron accelerator at Jefferson Lab (JLab) will deliver a longitudinally polarized (up to 85%), high intensity (up to 100 ?A) beam with maximum energy of 12 GeV, twice the present value. To exploit the new opportunities that the energy upgrade will offer, a new spectrometer (Super BigBite - SBS) is under development, featuring very forward angle, large acceptance and ability to operate in high luminosity environment. The tracking system of SBS will consist of large area (40150 cm2 and 50200 cm2), high spatial resolution (better than 100 ?m) chambers based on the GEM technology and 2 small (1020 cm) Silicon Strip Detector planes. The design of the GEM chambers and its sub-components such as the readout electronics is resented here.

Bellini, V; Castelluccio, D; Colilli, S; Cisbani, E; De Leo, R; Fratoni, R; Frullani, S; Garibaldi, F; Guiliani, F; Guisa, A; Gricia, M; Lucentini, M; Meddi, F; Minutoli, S; Musico, P; Noto, F; De Oliveira, R; Santavenere, F; Sutera, M C

2011-06-01T23:59:59.000Z

202

HDice, Highly-Polarized Low-Background Frozen-Spin HD Targets for CLAS experiments at Jefferson Lab  

Science Conference Proceedings (OSTI)

Large, portable frozen-spin HD (Deuterium-Hydride) targets have been developed for studying nucleon spin properties with low backgrounds. Protons and Deuterons in HD are polarized at low temperatures (~10mK) inside a vertical dilution refrigerator (Oxford Kelvinox-1000) containing a high magnetic field (up to 17T). The targets reach a frozen-spin state within a few months, after which they can be cold transferred to an In-Beam Cryostat (IBC). The IBC, a thin-walled dilution refrigerator operating either horizontally or vertically, is use with quasi-4? detector systems in open geometries with minimal energy loss for exiting reaction products in nucleon structure experiments. The first application of this advanced target system has been used for Spin Sum Rule experiments at the LEGS facility in Brookhaven National Laboratory. An improved target production and handling system has been developed at Jefferson Lab for experiments with the CEBAF Large Acceptance Spectrometer, CLAS.

Wei, Xiangdong [JLAB; Bass, Christopher [JLAB; D'Angelo, Annalisa [INFN-Roma Tor Vegata; Deur, Alexandre P. [JLAB; Dezern, Gary L. [JLAB; Ho, Dao Hoang [Carnegie Mellon U.; Kageya, Tsuneo [JLAB; Khandaker, Mahbubul A, [Idaho State U.; Kashy, David H. [JLAB; Laine, Vivien Eric [Universite de Clermont Ferrand; Lowry, Michael M. [JLAB; O'Connell, Thomas Robert [University of Connecticut; Sandorfi, Andrew M. [JLAB; Teachey, II, Robert W. [JLAB; Whisnant, Charles Steven [James Madison U.; Zarecky, Michael R. [JLAB

2012-12-01T23:59:59.000Z

203

NEWTON, Ask a Scientist at Argonne National Labs  

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

Longest Day in Tropics Longest Day in Tropics Name: Owen Status: other Grade: other Country: Australia Date: Spring 2012 Question: I have checked the archive and it is not really answered there. http://www.newton.dep.anl.gov/askasci/gen01/gen01052.htm isthe closest link but does not really get to the crux of what I amasking below. Is the solstice still the longest day (in either hemisphere) if your location is between the Tropics? Some friends and I have been debating this. One faction argues that the solstice on 21 December is the longest day here in Cairns, QLD, Australia. the other faction claims that the longest days here are when the sun is directly overhead (we believe the days to be 28 November and 12 January here in Cairns) and that the days shorten between 28 November (zenith in CNS) and 21 December (solstice) ... then graduate/lengthen back to the maximum between 22 December until 12 January (our other zenith day as the sun moves back North) ... after which, they shorten again. can you please settle the debate (with an explanation).

204

Notes on Newton-Krylov based Incompressible Flow Projection Solver  

SciTech Connect

The purpose of the present document is to formulate Jacobian-free Newton-Krylov algorithm for approximate projection method used in Hydra-TH code. Hydra-TH is developed by Los Alamos National Laboratory (LANL) under the auspices of the Consortium for Advanced Simulation of Light-Water Reactors (CASL) for thermal-hydraulics applications ranging from grid-to-rod fretting (GTRF) to multiphase flow subcooled boiling. Currently, Hydra-TH is based on the semi-implicit projection method, which provides an excellent platform for simulation of transient single-phase thermalhydraulics problems. This algorithm however is not efficient when applied for very slow or steady-state problems, as well as for highly nonlinear multiphase problems relevant to nuclear reactor thermalhydraulics with boiling and condensation. These applications require fully-implicit tightly-coupling algorithms. The major technical contribution of the present report is the formulation of fully-implicit projection algorithm which will fulfill this purpose. This includes the definition of non-linear residuals used for GMRES-based linear iterations, as well as physics-based preconditioning techniques.

Robert Nourgaliev; Mark Christon; J. Bakosi

2012-09-01T23:59:59.000Z

205

XMM-Newton study of 0.012thermodynamics  

E-Print Network (OSTI)

We study the thermodynamic properties of the hot gas in a sample of groups in the 0.012-0.024 redshift range, using XMM-Newton observations. We present measurements of temperature, entropy, pressure and iron abundance. Non-parametric fits are used to derive the mean properties of the sample and to study dispersion in the values of entropy and pressure. The scaling of the entropy at 0.2r500 matches well the results of Ponman et al. (2003). However, compared to cool clusters, the groups in our sample reveal larger entropy at inner radii and a substantially flatter slope in the entropy in the outskirts, compared to both the prediction of pure gravitational heating and to observations of clusters. This difference corresponds to the systematically flatter group surface brightness profiles, reported previously. The scaled pressure profiles can be well approximated with a Sersic model with n=4. We find that groups exhibit a systematically larger dispersion in pressure, compared to clusters of galaxies, while the dispersion in entropy is similar.

A. Finoguenov; T. J. Ponman; J. P. F. Osmond; M. Zimer

2006-11-28T23:59:59.000Z

206

FIA-12-0061 - In the Matter of John P. Newton | Department of Energy  

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

2-0061 - In the Matter of John P. Newton 2-0061 - In the Matter of John P. Newton FIA-12-0061 - In the Matter of John P. Newton On October 31, 2012, the Office of Hearings and Appeals (OHA) issued a decision denying an appeal (Appeal) from two Freedom of Information Act (FOIA) determinations issued by the Department of Energy's Office of Information Resources (OIR). Specifically, the Appellant appealed OIR's decisions not to grant him a fee waiver and expedited processing of his FOIA requests. The OHA decided that the Appellant did not demonstrate that the information he sought from his FOIA request would contribute significantly to public understanding of government operations or activities or that the information concerned a time-sensitive matter. Therefore, the OHA denied the Appeal for expedited processing of the FOIA

207

A Newton-Krylov solution to the porous medium equations in the agree code  

Science Conference Proceedings (OSTI)

In order to improve the convergence of the AGREE code for porous medium, a Newton-Krylov solver was developed for steady state problems. The current three-equation system was expanded and then coupled using Newton's Method. Theoretical behavior predicts second order convergence, while actual behavior was highly nonlinear. The discontinuous derivatives found in both closure and empirical relationships prevented true second order convergence. Agreement between the current solution and new Exact Newton solution was well below the convergence criteria. While convergence time did not dramatically decrease, the required number of outer iterations was reduced by approximately an order of magnitude. GMRES was also used to solve problem, where ILU without fill-in was used to precondition the iterative solver, and the performance was slightly slower than the direct solution. (authors)

Ward, A. M.; Seker, V.; Xu, Y.; Downar, T. J. [Dept. of Nuclear Engineering and Radioligical Sciences, Univ. of Michigan, 2355 Bonisteel Blvd, Ann Arbor, MI 48109 (United States)

2012-07-01T23:59:59.000Z

208

The 12 GeV CEBAF Upgrade Project at Thomas Jefferson National Accelerator Facility, OAS-RA-L-11-13  

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

12 GeV CEBAF Upgrade 12 GeV CEBAF Upgrade Project at Thomas Jefferson National Accelerator Facility OAS-RA-L-11-13 September 2011 Department of Energy Washington, DC 20585 September 30, 2011 MEMORANDUM FOR THE DEPUTY DIRECTOR FOR SCIENCE PROGRAMS, OFFICE OF SCIENCE DIRECTOR, OFFICE OF RISK MANAGEMENT AND FINANCIAL POLICY, OFFICE OF THE CHIEF FINANCIAL OFFICER FROM: David Sedillo, Director NNSA & Science Audits Division Office of Inspector General SUBJECT: INFORMATION: Audit Report on "The 12 GeV CEBAF Upgrade Project at Thomas Jefferson National Accelerator Facility" Audit Report Number: OAS-RA-L-11-13 BACKGROUND In September 2008, the Department of Energy's (Department) Office of Science approved a construction project to double the electron beam energy of the Continuous Electron Beam

209

A Beginner's Guide to Newton INTRODUCTION There are two main library catalogues currently in use, the online  

E-Print Network (OSTI)

precise results, use a combination of search terms. Once the text has been entered you then need to select SEARCHING IN NEWTON A Newton Guided Search allows searching for combinations of search terms whilst below. This has three lines of boxes to enter the text you wish to search for. To retrieve the most

Keeler, James

210

New Inventions - Jefferson Lab | Jefferson Lab  

Invention Disclosure; CRADA/WFO Routing; Fairness of Opportunity; America Invents Act Summary; Achievements at JLab. Patents; New Inventions; New ...

211

Jefferson Lab Technology Transfer - Thomas Jefferson National ...  

Invention Disclosure; CRADA/WFO Routing; Fairness of Opportunity; America Invents Act Summary; Achievements at JLab. Patents; New Inventions; New ...

212

Jefferson Lab Technology Transfer - Thomas Jefferson National ...  

JSA Invention Disclosure; Technology Transfer Issues (Ombudsman) Programs and Facilities. Free-Electron Laser Program (FEL) Applied Research Center ...

213

Solving Nonlinear Solid Mechanics Problems with the Jacobian-Free Newton Krylov Method  

Science Conference Proceedings (OSTI)

The solution of the equations governing solid mechanics is often obtained via Newton's method. This approach can be problematic if the determination, storage, or solution cost associated with the Jacobian is high. These challenges are magnified for multiphysics applications with many coupled variables. Jacobian-free Newton-Krylov (JFNK) methods avoid many of the difficulties associated with the Jacobian by using a finite difference approximation. BISON is a parallel, object-oriented, nonlinear solid mechanics and multiphysics application that leverages JFNK methods. We overview JFNK, outline the capabilities of BISON, and demonstrate the effectiveness of JFNK for solid mechanics and solid mechanics coupled to other PDEs using a series of demonstration problems.

J. D. Hales; S. R. Novascone; R. L. Williamson; D. R. Gaston; M. R. Tonks

2012-06-01T23:59:59.000Z

214

The Search for Exotic Mesons in gamma p -> pi+pi+pi-n with CLAS at Jefferson Lab  

E-Print Network (OSTI)

The $\\pi_1(1600)$, a $J^{PC} = 1^{-+}$ exotic meson has been observed by experiments using pion beams. Theorists predict that photon beams could produce gluonic hybrid mesons, of which the $\\pi_1(1600)$ is a candidate, at enhanced levels relative to pion beams. The g12 rungroup at Jefferson Lab's CEBAF Large Acceptance Spectrometer (CLAS) has recently acquired a large photoproduction dataset, using a liquid hydrogen target and tagged photons from a 5.71 GeV electron beam. A partial-wave analysis of 502K $\\gamma p \\to \\pi^+\\pi^+\\pi^-n$ events selected from the g12 dataset has been performed, and preliminary fit results show strong evidence for well-known states such as the $a_1(1260)$, $a_2(1320)$, and $\\pi_2(1670)$. However, we observe no evidence for the production of the $\\pi_1(1600)$ in either the partial-wave intensities or the relative complex phase between the $1^{-+}$ and the $2^{-+}$ (corresponding to the $\\pi_2$) partial waves.

Craig Bookwalter

2011-08-31T23:59:59.000Z

215

The Search for Exotic Mesons in gammap-->pi+pi+pi?n with CLAS at Jefferson Lab  

DOE Green Energy (OSTI)

In addition to ordinary qq-bar pairs, quantum chromodynamics (QCD) permits many other possibilities in meson spectra, such as gluonic hybrids, glueballs, and tetraquarks. Experimental discovery and study of these exotic states provides insight on the nonperturbative regime of QCD. Over the past twenty years, some searches for exotic mesons have met with controversial results, especially those obtained in the three-pion system. Prior theoretical work indicates that in photoproduction one should find gluonic hybrids at significantly enhanced levels compared to that found in pion production. To that end, the CLAS g12 run was recently completed at Jefferson Lab, using a liquid hydrogen target and tagged photons from a 5.71 GeV electron beam. The CLAS experimental apparatus was modified to maximize forward acceptance for peripheral production of mesons. The resulting data contains the world's largest 3pi photoproduction dataset, with gammap-->pi+pi+pi?n events numbering in the millions. Early results describing the data quality, kinematics, and dysnamics will be shown.

Craig Bookwalter

2010-08-01T23:59:59.000Z

216

The Search for Exotic Mesons in gamma p -> pi+pi+pi-n with CLAS at Jefferson Lab  

DOE Green Energy (OSTI)

The {pi}{sub 1}(1600), a J{sup PC} = 1{sup {-+}} exotic meson has been observed by experiments using pion beams. Theorists predict that photon beams could produce gluonic hybrid mesons, of which the {pi}{sub 1}(1600) is a candidate, at enhanced levels relative to pion beams. The g12 rungroup at Jefferson Lab's CEBAF Large Acceptance Spectrometer (CLAS) has recently acquired a large photoproduction dataset, using a liquid hydrogen target and tagged photons from a 5.71 GeV electron beam. A partial-wave analysis of 502K {gamma}p {yields} {pi}{sup +}{pi}{sup +}{pi}{sup -}n events selected from the g12 dataset has been performed, and preliminary fit results show strong evidence for well-known states such as the a{sub 1}(1260), a{sub 2}(1320), and {pi}{sub 2}(1670). However, we observe no evidence for the production of the {pi}{sub 1}(1600) in either the partial-wave intensities or the relative complex phase between the 1{sup {-+}} and the 2{sup {-+}} (corresponding to the {pi}{sub 2}) partial waves.

Craig Bookwalter

2011-12-01T23:59:59.000Z

217

EPRI Transmission Line Reference Book: Wind-Induced Conductor Motion (Orange Book) Revision  

Science Conference Proceedings (OSTI)

This report is an updated edition of the longtime industry standard on vibration, EPRI Transmission Line Reference Book: Wind-Induced Conductor Motion, the "Orange Book," which was last issued in 1979. Publication of this new edition is the culmination of three years of research by an international team of experts in the field. The report includes the latest information on research, technology, and materials and represents a significant contribution to the global industry of electric power transmission.

2009-03-27T23:59:59.000Z

218

The XMM-Newton observation of GRB 040106 : evidence for an afterglow in a wind environment  

E-Print Network (OSTI)

We present the XMM-Newton observation of GRB 040106. From the X-ray spectral index and temporal decay, we argue that the afterglow is consistent with a fireball expanding in a wind environment. A constant density environment is excluded by the data. This is one of the very few cases in which this conclusion can be drawn.

B. Gendre; L. Piro; M. De Pasquale

2004-07-29T23:59:59.000Z

219

A Newton-based approach for attributing tumor lethality in animal carcinogenicity studies  

Science Conference Proceedings (OSTI)

A new Newton-based approach is proposed for finding the global maximum of a nonlinear function subject to various inequality constraints. This method can be applied to nonparametric maximum likelihood estimation problems to attribute tumor lethality ... Keywords: Cause of death, Inequality constraint, Maximum likelihood, Optimization, Sacrifice

Hongshik Ahn; Hojin Moon; Sunyoung Kim; Ralph L. Kodell

2002-01-01T23:59:59.000Z

220

On inverse problems for the multidimensional relativistic Newton equation at fixed energy  

E-Print Network (OSTI)

In this paper, we consider inverse scattering and inverse boundary value problems at sufficiently large and fixed energy for the multidimensional relativistic Newton equation with an external potential $V$, $V\\in C^2$. Using known results, we obtain, in particular, theorems of uniqueness.

Alexandre Jollivet

2006-07-03T23:59:59.000Z

Note: This page contains sample records for the topic "newton orange jefferson" 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

Landau energy levels for twisted N-enlarged Newton-Hooke space-time  

E-Print Network (OSTI)

We derive the Landau energy levels for twisted N-enlarged Newton-Hooke space-time, i.e. we find the time-dependent energy spectrum and the corresponding eigenstates for an electron moving in uniform magnetic as well as in uniform electric external fields.

Daszkiewicz, Marcin

2013-01-01T23:59:59.000Z

222

A modified smoothing and regularized Newton method for monotone second-order cone complementarity problems  

Science Conference Proceedings (OSTI)

In this paper, we propose a globally and quadratically convergent Newton-type algorithm for solving monotone second-order cone complementarity problems (denoted by SOCCPs). This algorithm is based on smoothing and regularization techniques by incorporating ... Keywords: Convergence analysis, Numerical results, Regularization, Second-order cone complementarity problem, Smoothing method

Linjie Chen; Changfeng Ma

2011-03-01T23:59:59.000Z

223

Model of hydrogen atom for twisted acceleration-enlarged Newton-Hooke space-times  

E-Print Network (OSTI)

We define the model of hydrogen atom for twist-deformed acceleration-enlarged Newton-Hooke space-time. Further, using time-dependent perturbation theory, we find in first step of iteration procedure the solution of corresponding Schroedinger equation as well as the probability of transition between two different energy-eigenstates.

Marcin Daszkiewicz

2013-12-09T23:59:59.000Z

224

Geology and geothermal resources of the Santiam Pass area of the Oregon Cascade Range, Deschutes, Jefferson and Linn Counties, Oregon  

DOE Green Energy (OSTI)

This open-file report presents the results of the Santiam Pass drilling program. The first phase of this program was to compile all available geological, geophysical and geothermal data for the Santiam Pass area and select a drill site on the basis of these data (see Priest and others, 1987a), A summary of the drilling operations and costs associated with the project are presented in chapter 1 by Hill and Benoit. An Overview of the geology of the Santiam Pass area is presented by Hill and Priest in chapter 2. Geologic mapping and isotopic age determinations in the Santiam Pass-Mount Jefferson area completed since 1987 are summarized in chapter 2. One of the more important conclusions reached in chapter 2 is that a minimum of 2 km vertical displacement has occurred in the High Cascade graben in the Santiam Pass area. The petrology of the Santiam Pass drill core is presented by Hill in chapter 3. Most of the major volcanic units in the core have been analyzed for major, minor, and trace element abundances and have been studied petrographically. Three K-Ar ages are interpreted in conjunction with the magnetostratigraphy of the core to show that the oldest rocks in the core are approximately 1.8 Ma. Geothermal and geophysical data collected from the Santiam Pass well are presented by Blackwell in chapter 4. The Santiam Pass well failed to penetrate beneath the zone of lateral groundwater flow associated with highly permeable Quaternary volcanic rocks. Calculated geothermal gradients range from about 50[degree]C/km at depth 700-900 m, to roughly 110[degree]C/km from 900 m to the bottom of the well at 929 m. Heat-flow values for the bottom part of the hole bracket the regional average for the High Cascades. Blackwell concludes that heat flow along the High Cascades axis is equal to or higher than along the western edge of the High Cascades.

Hill, B.E. (ed.)

1992-10-01T23:59:59.000Z

225

Parallel Jacobian-free Newton Krylov solution of the discrete ordinates method with flux limiters for 3D radiative transfer  

Science Conference Proceedings (OSTI)

The present study introduces a parallel Jacobian-free Newton Krylov (JFNK) general minimal residual (GMRES) solution for the discretized radiative transfer equation (RTE) in 3D, absorbing, emitting and scattering media. For the angular and spatial discretization ... Keywords: Collimated radiation, Discrete ordinates method (DOM) SN, Electromagnetic radiation, Flux limiters, General Minimal Residual (GMRES), Gram-Schmidt, Householder, Jacobian free Newton-Krylov (JFNK), Parallel MPI, Radiative transfer equation (RTE), TVD, Threads

William F. Godoy; Xu Liu

2012-06-01T23:59:59.000Z

226

Subspace accelerated inexact Newton method for large scale wave functions calculations in Density Functional Theory  

SciTech Connect

We describe an iterative algorithm to solve electronic structure problems in Density Functional Theory. The approach is presented as a Subspace Accelerated Inexact Newton (SAIN) solver for the non-linear Kohn-Sham equations. It is related to a class of iterative algorithms known as RMM-DIIS in the electronic structure community. The method is illustrated with examples of real applications using a finite difference discretization and multigrid preconditioning.

Fattebert, J

2008-07-29T23:59:59.000Z

227

Inverse scattering at fixed energy for the multidimensional Newton equation in short range radial potentials  

E-Print Network (OSTI)

We consider the inverse scattering problem at fixed and sufficiently large energy for the nonrelativistic and relativistic Newton equation in $\\R^n$, $n \\ge 2$, with a smooth and short range electromagnetic field $(V,B)$. Using results of [Firsov, 1953] or [Keller-Kay-Shmoys, 1956] we obtain a uniqueness result when $B$ is assumed to be zero in a neighborhood of infinity and $V$ is assumed to be spherically symmetric in a neighborhood of infinity.

Alexandre Jollivet

2012-10-24T23:59:59.000Z

228

Osage Orange  

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

hunt wild game, there have been herdsmen and farmers who have had to build fences. Fence building and fence repairing, whether they be stone walls, living thorn hedges, rail...

229

Jefferson Lab Technology Transfer  

This site's design is only visible in a graphical browser that supports web standards, but its content is accessible to any browser. Concerns? Technology Transfer.

230

Jefferson Lab Technology Transfer  

Invention Disclosure; CRADA/WFO Routing; Fairness of Opportunity; Achievements at JLab. Patents; New Inventions; New Technologies; New Advances; ...

231

Jefferson Lab Technology Transfer  

Title to invention of sponsor or laboratory operator goes to sponsor under class patent waiver and sponsor ... Disclosure to sponsor of laboratory ...

232

Jefferson Lab Technology Transfer  

Invention Disclosure; CRADA/WFO Routing; Fairness ... Every JLab employee who has an idea that may be patentable is encouraged to follow the simple In ...

233

Jefferson Lab Technology Transfer  

Research was done in collaboration with the Department of Biology at the College of William and Mary which obtained a grant from NSF and with the support of the ...

234

Jefferson Lab Technology Transfer  

Cryogenic Liquid Level Measuring Apparatus; Uniform Raster Pattern Generating System; ... Injection Mode-locking Ti-Sapphire Laser System; Radial ...

235

Structural Determinats Underlying Photoprotection in the Photoactive Orange Carotenoid Protein of Cyanobacteria  

SciTech Connect

The photoprotective processes of photosynthetic organisms involve the dissipation of excess absorbed light energy as heat. Photoprotection in cyanobacteria is mechanistically distinct from that in plants; it involves the Orange Carotenoid Protein (OCP), a water-soluble protein containing a single carotenoid. The OCP is a new member of the family of blue light photoactive proteins; blue-green light triggers the OCP-mediated photoprotective response. Here we report structural and functional characterization of the wildtype and two mutant forms of the OCP, from the model organism Synechocystis PCC6803. The structural analysis provides highresolution detail of the carotenoidprotein interactions that underlie the optical properties of the OCP, unique among carotenoid-proteins in binding a single pigment per polypeptide chain. Collectively, these data implicate several key amino acids in the function of the OCP and reveal that the photoconversion and photoprotective responses of the OCP to blue-green light can be decoupled.

Wilson, Adjele; Kinney, James N.; Zwart, Petrus H.; Punginelli, Claire; D'Haene, Sandrine; Perreau, Francois; Klein, Michael G.; Kirilovsky, Diana; Kerfeld, Cheryl

2010-04-01T23:59:59.000Z

236

XMM-Newton Observations of NGC 247 and a Supersoft Ultraluminous X-ray Source  

E-Print Network (OSTI)

We report on a new XMM-Newton observation of NGC 247 from December 2009. The galaxy contains a supersoft, ultraluminous X-ray source (ULX) whose spectrum consists of a thermal component with a temperature about 0.1 keV and a power-law tail with a photon index around 2.5. The thermal emission is absolutely the dominant component, contributing 96% of the total luminosity in the 0.3-10 keV band. Variability is detected at timescales of 100 s and longer with a $\

Jin, Jing; Kaaret, Philip; Zhang, Shuang-Nan

2011-01-01T23:59:59.000Z

237

From Cavendish to PLANCK: Constraining Newton's gravitational constant with CMB temperature and polarization anisotropy  

SciTech Connect

We present new constraints on cosmic variations of Newton's gravitational constant by making use of the latest CMB data from WMAP, BOOMERANG, CBI and ACBAR experiments and independent constraints coming from big bang nucleosynthesis. We found that current CMB data provide constraints at the {approx}10% level, that can be improved to {approx}3% by including big bang nucleosynthesis data. We show that future data expected from the Planck satellite could constrain G at the {approx}1.5% level while an ultimate, cosmic variance limited, CMB experiment could reach a precision of about 0.4%, competitive with current laboratory measurements.

Galli, Silvia; Melchiorri, Alessandro; Smoot, George F.; Zahn, Oliver [Physics Department, Universita di Roma 'La Sapienza', Ple Aldo Moro 2, 00185, Rome, Italy, and Laboratoire Astroparticule et Cosmologie (APC), Universite' Paris Diderot - 75205 PARIS cedex 13 (Italy); Physics Department and INFN, Universita di Roma 'La Sapienza', Ple Aldo Moro 2, 00185, Rome (Italy); Lawrence Berkeley National Laboratory and Berkeley Center for Cosmological Physics Physics Department, University of California, Berkeley California 94720 (United States)

2009-07-15T23:59:59.000Z

238

Dynamically polarized target for the g{sub 2}{sup p} and G{sub E}{sup p} experiments at Jefferson Lab  

SciTech Connect

Recently, two experiments were concluded in Hall A at Jefferson Lab which utilized a newly assembled, solid, polarized hydrogen target. The primary components of the target are a new, high cooling power {sup 4}He evaporation refrigerator, and a re-purposed, superconducting split-coil magnet. It has been used to polarize protons in irradiated NH{sub 3} at a temperature of 1 K and at fields of 2.5 and 5.0 tesla. Maximum polarizations of 55% and 95% were obtained at those fields, respectively. To satisfy the requirements of both experiments, the magnet had to be routinely rotated between angles of 0, 6, and 90 with respect to the incident electron beam.

Pierce, Joshua J. [JLAB; Maxwell, James D. [MIT; Keith, Christopher D. [JLAB

2014-01-01T23:59:59.000Z

239

The perihelion of Mercury advance and the light bending calculated in (enhanced) Newton's theory  

E-Print Network (OSTI)

We show that results of a simple dynamical gedanken experiment interpreted according to standard Newton's gravitational theory, may reveal that three-dimensional space is curved. The experiment may be used to reconstruct the curved geometry of space, i.e. its non-Euclidean metric. The perihelion of Mercury advance and the light bending calculated from the Poisson equation and the equation of motion in the curved geometry have the correct (observed) values. Independently, we also show that Newtonian gravity theory may be enhanced to incorporate the curvature of three dimensional space by adding an extra equation which links the Ricci scalar with the density of matter. Like in Einstein's general relativity, matter is the source of curvature. In the spherically symmetric (vacuum) case, the metric of space 3gik that follows from this extra equation agrees, to the expected accuracy, with the metric measured by the Newtonian gedanken experiment mentioned above.

M. A. Abramowicz; G. F. R. Ellis J. Horak; M. Wielgus

2013-03-21T23:59:59.000Z

240

Fluid preconditioning for Newton-Krylov-based, fully implicit, electrostatic particle-in-cell simulations  

E-Print Network (OSTI)

A recent proof-of-principle study proposes an energy- and charge-conserving, nonlinearly implicit electrostatic particle-in-cell (PIC) algorithm in one dimension [Chen et al, J. Comput. Phys., 230 (2011) 7018]. The algorithm in the reference employs an unpreconditioned Jacobian-free Newton-Krylov method, which ensures nonlinear convergence at every timestep (resolving the dynamical timescale of interest). Kinetic enslavement, which is one key component of the algorithm, not only enables fully implicit PIC a practical approach, but also allows preconditioning the kinetic solver with a fluid approximation. This study proposes such a preconditioner, in which the linearized moment equations are closed with moments computed from particles. Effective acceleration of the linear GMRES solve is demonstrated, on both uniform and non-uniform meshes. The algorithm performance is largely insensitive to the electron-ion mass ratio. Numerical experiments are performed on a 1D multi-scale ion acoustic wave test problem.

Chen, Guangye; Leibs, Christopher A; Knoll, Dana A; Taitano, William

2013-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "newton orange jefferson" 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

Multiple Attractor in Newton -Leipnik System, Peak to Peak dynamics and Chaos Control  

E-Print Network (OSTI)

The chaotic properties of Newton-Leipnik system are discussed from the view point of strange attractors. Previously, two strange attractors of this system were illustrated which occured from two different initial conditions under the same parameter condition. It is found that above system also exhibits multiple attractors under different parameter values but same initial condition and we have shown the existence of three other strange attractors with varying dimensionality under different parametric conditions. The properties of these attractors are then analyzed on the basis of Lyapunov exponents, power spectra, recurrence analysis and peak-to-peak dynamics. The peak-to-peak dynamics relies on the low dimensionality of the chaotic attractor and allows to approximately model the system. Peak-to-peak plot along with return-time plot are then effectively used to solve the optimal control problem of the system which reverts the system to a periodic situation.

Biswambhar Rakshit; Papri Saha; A. Roy Chowdhury

2005-01-07T23:59:59.000Z

242

Geology and geothermal resources of the Santiam Pass area of the Oregon Cascade Range, Deschutes, Jefferson and Linn Counties, Oregon. Final report  

DOE Green Energy (OSTI)

This open-file report presents the results of the Santiam Pass drilling program. The first phase of this program was to compile all available geological, geophysical and geothermal data for the Santiam Pass area and select a drill site on the basis of these data (see Priest and others, 1987a), A summary of the drilling operations and costs associated with the project are presented in chapter 1 by Hill and Benoit. An Overview of the geology of the Santiam Pass area is presented by Hill and Priest in chapter 2. Geologic mapping and isotopic age determinations in the Santiam Pass-Mount Jefferson area completed since 1987 are summarized in chapter 2. One of the more important conclusions reached in chapter 2 is that a minimum of 2 km vertical displacement has occurred in the High Cascade graben in the Santiam Pass area. The petrology of the Santiam Pass drill core is presented by Hill in chapter 3. Most of the major volcanic units in the core have been analyzed for major, minor, and trace element abundances and have been studied petrographically. Three K-Ar ages are interpreted in conjunction with the magnetostratigraphy of the core to show that the oldest rocks in the core are approximately 1.8 Ma. Geothermal and geophysical data collected from the Santiam Pass well are presented by Blackwell in chapter 4. The Santiam Pass well failed to penetrate beneath the zone of lateral groundwater flow associated with highly permeable Quaternary volcanic rocks. Calculated geothermal gradients range from about 50{degree}C/km at depth 700-900 m, to roughly 110{degree}C/km from 900 m to the bottom of the well at 929 m. Heat-flow values for the bottom part of the hole bracket the regional average for the High Cascades. Blackwell concludes that heat flow along the High Cascades axis is equal to or higher than along the western edge of the High Cascades.

Hill, B.E. [ed.

1992-10-01T23:59:59.000Z

243

The XMM-Newton bright serendipitous survey. Identification and optical spectral properties  

E-Print Network (OSTI)

AIMS: We present the optical classification and redshift of 348 X-ray selected sources from the XMM-Newton Bright Serendipitous Survey (XBS) which contains a total of 400 objects (identification level = 87%). About 240 are new identifications. In particular, we discuss in detail the classification criteria adopted for the Active Galactic Nuclei population. METHODS: By means of systematic spectroscopic campaigns and through the literature search we have collected an optical spectrum for the large majority of the sources in the XBS survey and applied a well-defined classification ``flow-chart''. RESULTS: We find that the AGN represent the most numerous population at the flux limit of the XBS survey (~10^-13 erg cm^-2 s^-1) constituting 80% of the XBS sources selected in the 0.5-4.5 keV energy band and 95% of the ``hard'' (4.5-7.5 keV) selected objects. Galactic sources populate significantly the 0.5-4.5 keV sample (17%) and only marginally (3%) the 4.5-7.5 keV sample. The remaining sources in both samples are c...

Caccianiga, A; Della Ceca, R; MacCacaro, T; Cocchia, F; Barcons, X; Carrera, F J; Matute, I; McMahon, R G; Page, M J; Pietsch, W; Sbarufatti, B; Schwope, A; Tedds, J A; Watson, M G

2007-01-01T23:59:59.000Z

244

Application of Newton's optimal power flow in voltage/reactive power control  

Science Conference Proceedings (OSTI)

This paper considers an application of Newton's optimal power flow to the solution of the secondary voltage/reactive power control in transmission networks. An efficient computer program based on the latest achievements in the sparse matrix/vector techniques has been developed for this purpose. It is characterized by good robustness, accuracy and speed. A combined objective function appropriate for various system load levels with suitable constraints, for treatment of the power system security and economy is also proposed. For the real-time voltage/reactive power control, a suboptimal power flow procedure has been derived by using the reduced set of control variables. This procedure is based on the sensitivity theory applied to the determination of zones for the secondary voltage/reactive power control and corresponding reduced set of regulating sources, whose reactive outputs represent control variables in the optimal power flow program. As a result, the optimal power flow program output becomes a schedule to be used by operators in the process of the real-time voltage/reactive power control in both normal and emergency operating states.

Bjelogrlic, M.; Babic, B.S. (Electric Power Board of Serbia, Belgrade (YU)); Calovic, M.S. (Dept. of Electrical Engineering, University of Belgrade, Belgrade (YU)); Ristanovic, P. (Institute Nikola Tesla, Belgrade (YU))

1990-11-01T23:59:59.000Z

245

The temperature and distribution of gas in CL 0016+16 measured with XMM-Newton  

E-Print Network (OSTI)

We present results of a 37 ks observation of CL 0016+16 with the XMM-Newton EPIC instrument. Within 1.5 arcmin of the cluster centre we measure a gas temperature of kT = 9.13^{+0.24}_{-0.22} keV and an abundance of 0.22^{+0.04}_{-0.03} times the solar value (1 sigma uncertainties). This significant improvement over previous measurements has allowed us to revise the estimate of the Hubble constant based on CL 0016+16 to 68 +/- 8 km s^{-1} Mpc^{-1} (random error only), close to the value from the Hubble Space Telescope distance-scale project. The total gravitating mass within a radius of 248 kpc of the cluster centre is in good agreement with that found from gravitational lensing over the same region, supporting the assumption of isothermal gas in hydrostatic equilibrium. The gas mass fraction of 0.13 +/- 0.02 is in remarkable agreement with that given by cosmological parameters for the Universe as a whole, suggesting that CL 0016+16 is a fair sample of the matter content of the Universe. While there is no spec...

Birkinshaw, M

2003-01-01T23:59:59.000Z

246

XMM-Newton observations of the Perseus Cluster I: The temperature and surface brightness structure  

E-Print Network (OSTI)

We present preliminary results of the XMM-Newton 50 ksec observation of the Perseus cluster. The global east/west asymmetry of the gas temperature and surface brightness distributions, approximately aligned with the chain of bright galaxies, suggests an ongoing merger, although the modest degree of the observed asymmetry certainly excludes a major merger interpretation. The chain of galaxies probably traces the filament along which accretion has started some time ago and is continuing at the present time. A cold and dense (low entropy) cluster core like Perseus is probably well "protected" against the penetration of the gas of infalling groups and poor clusters whereas in non-cooling core clusters like Coma and A1367, infalling subclusters can penetrate deeply into the core region. In Perseus, gas associated with infalling groups may be stripped completely at the outskirts of the main cluster and only compression waves (shocks) may reach the central regions. We argue that the passage of such a wave(s) can qualitatively explain the overall horseshoe shaped appearance of the gas temperature map (the hot horseshoe surrounds the colder, low entropy core) as well as other features of the Perseus cluster core. As compression waves traverse the cluster core, they can induce oscillatory motion of the cluster gas which can generate multiple sharp "edges", on opposite sides or the central galaxy. Gas motions induced by mergers may be a natural way to explain the high frequency of "edges" seen in clusters with cooling cores.

E. Churazov; W. Forman; C. Jones; H. Bhringer

2003-01-23T23:59:59.000Z

247

An XMM-Newton observation of the dynamically active binary cluster A1750  

E-Print Network (OSTI)

We present results from the XMM-Newton observation of the binary cluster A1750 at z = 0.086. We have performed a detailed study of the surface brightness, temperature and entropy distribution and confirm that the two main clusters of the system (A1750 N and A1750 C) have just started to interact. From the temperature distribution, we calculate that they are likely to merge sometime in the next 1 Gyr. The more massive cluster, A1750 C, displays a more complicated temperature structure than expected. We detect a hot region associated with a density jump ~450 kpc east of the cluster centre, which appears to be a shock wave. This shock is not connected with the binary merger, but it is intrinsic to A1750 C itself. From simple physical arguments and comparison with numerical simulations, we argue that this shock is related to a merging event that A1750 C has suffered in the past 1-2 Gyr. The larger scale structure around A1750 suggests that the system belongs to a rich supercluster, which would presumably increase...

Belsole, E; Sauvageot, J L; Bourdin, H

2004-01-01T23:59:59.000Z

248

The XMM-Newton view of AGN with intermediate mass black holes  

E-Print Network (OSTI)

We have observed with XMM-Newton four radiatively efficient active type 1 galaxies with black hole masses alternative scenarios for the nature of the soft excess (namely smeared ionized absorption and disc reflection) cannot be distinguished on a pure statistical basis, we point out that the absorption model produces a strong correlation between absorbing column density and ionization state, which may be difficult to interpret and is most likely spurious. As for reflection, it does only invoke standard ingredients of any accretion model for radiatively efficient sources such as a hard X-rays source and a relatively cold (though partially ionized) accretion disc, and therefore seems the natural choice to explain the soft excess in most (if not all) cases. The reflection model is also consistent with the additional presence of a thermal disc component with the theoretically expected temperature (although, again, with smaller-than-expected total luminosity). The observed active galaxies are among the most variable in X-rays and their excess variance is among the largest. This is in line with their relatively small black hole mass and with expectations from simple power spectra models. (abridged)

G. Miniutti; G. Ponti; J. E. Greene; L. C. Ho; A. C. Fabian; K. Iwasawa

2008-12-09T23:59:59.000Z

249

Evaluation of Orange and Rockland Utilities, Inc.`s competitive bidding program for demand-side resources. Final report  

SciTech Connect

The process evaluation reports on the implementation of Orange and Rockland Utilities demand-side bidding program in New York State during 1991 and 1992. The program is implemented by two energy service companies in Orange and rockland`s New York State service territory. The process evaluation methodology included interviews with utility staff (3), energy service company staff (2), and participating (6) and nonparticipating (7) utility customers. The two energy service companies had enrolled 14 customers in the program by summer 1992. One company had achieved 90% of their 2.75 MW bid and the other had achieved less than 90% of their 6.9 MW bid. Critical factors in success were determination of a reasonable bid amount for the market and marketing to the appropriate customers. Customers most interested in the program included those with limited access to capital and medium-sized firms with poor cash flows, particularly schools and hospitals. The findings also show that due to the incentive structure and associated need for substantial customer contributions, lighting measures dominate all installations. Customers, however, were interested in the potential savings and six of the nonparticipants chose to either install measures on their own or enroll in the utility`s rebate program.

Peters, J.S.; Stucky, L.; Seratt, P.; Darden-Butler, D. [Barakat and Chamberlin, Inc., Portland, OR (United States)

1993-02-01T23:59:59.000Z

250

Community Action Partnership of Orange County - Weatherization Assistance Program Funds Provided by the American Recovery and Reinvestment Act of 2009, OAS-RA-13-03  

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

Community Action Partnership of Community Action Partnership of Orange County - Weatherization Assistance Program Funds Provided by the American Recovery and Reinvestment Act of 2009 OAS-RA-13-03 October 2012 Department of Energy Washington, DC 20585 October 17, 2012 MEMORANDUM FOR THE ASSISTANT SECRETARY, ENERGY EFFICIENCY AND RENEWABLE ENERGY FROM: Rickey R. Hass Deputy Inspector General for Audit Services Office of Inspector General SUBJECT: INFORMATION: Examination Report on "Community Action Partnership of Orange County - Weatherization Assistance Program Funds Provided by the American Recovery and Reinvestment Act of 2009" BACKGROUND The attached report presents the results of an examination of the Community Action Partnership

251

First deep XMM-Newton observations of the LMC: Identifying LMC intrinsic source populations  

E-Print Network (OSTI)

The first X-ray survey of the Large Magellanic Cloud (LMC) was performed with the Einstein satellite, revealing diffuse X-ray emission from hot gas and discrete X-ray sources. The ROSAT observations between 1990 and 1998 supplied the most sensitive survey with imaging instruments in the soft X-ray band (0.1 - 2.4 keV). The PSPC and HRI observations covered 59 square degrees of the LMC and yielded a catalogue of about 1000 sources. Large efforts were undertaken to identify and classify the X-ray sources according to the nature of their X-ray emission. X-ray properties were used together with information from other electro-magnetic wavelength bands to screen out foreground stars and background objects from the LMC intrinsic X-ray source population which comprises X-ray binaries, supernova remnants and supersoft sources. However, the vast majority of sources still remains of unknown nature. First deep XMM-Newton observations of selected regions in the LMC demonstrate a large step forward in the identification of LMC X-ray sources. The large collecting area together with imaging detectors covering energies 0.1 - 15 keV with far improved spectral resolution allows to determine the nature of an object directly from the X-ray properties down to low flux levels of a few 10$^{-14}$ erg cm$^{-2}$ s$^{-1}$. First results of a deep observation north of LMC X-4 are presented, which reveal the presence of new supernova remnants and X-ray binaries.

F. Haberl

2002-03-14T23:59:59.000Z

252

The temperature and distribution of gas in CL 0016+16 measured with XMM-Newton  

E-Print Network (OSTI)

We present results of a 37 ks observation of CL 0016+16 with the XMM-Newton EPIC instrument. Within 1.5 arcmin of the cluster centre we measure a gas temperature of kT = 9.13^{+0.24}_{-0.22} keV and an abundance of 0.22^{+0.04}_{-0.03} times the solar value (1 sigma uncertainties). This significant improvement over previous measurements has allowed us to revise the estimate of the Hubble constant based on CL 0016+16 to 68 +/- 8 km s^{-1} Mpc^{-1} (random error only), close to the value from the Hubble Space Telescope distance-scale project. The total gravitating mass within a radius of 248 kpc of the cluster centre is in good agreement with that found from gravitational lensing over the same region, supporting the assumption of isothermal gas in hydrostatic equilibrium. The gas mass fraction of 0.13 +/- 0.02 is in remarkable agreement with that given by cosmological parameters for the Universe as a whole, suggesting that CL 0016+16 is a fair sample of the matter content of the Universe. While there is no spectral or spatial evidence to suggest a cooling flow in CL 0016+16, we find an asymmetrical central X-ray structure which may have a harder spectrum than the cluster as a whole, and be evidence for some merger activity, in addition to a previously reported asymmetry to the west of the cluster. The nearest companion cluster to CL 0016+16 is measured to have a gas temperature of kT = 3.8^{+0.3}_{-0.3} keV and an abundance of 0.6^{+0.3}_{-0.2} times the solar value (1 sigma uncertainties). We also present spectral data for the companion quasar whose spectrum was confused with CL 0016+16 in previous ASCA data.

D. M. Worrall; M. Birkinshaw

2003-01-07T23:59:59.000Z

253

X-RAY SUBSTRUCTURE STUDIES OF FOUR GALAXY CLUSTERS USING XMM-NEWTON DATA  

SciTech Connect

Mahdavi et al. find that the degree of agreement between weak lensing and X-ray mass measurements is a function of cluster radius. Numerical simulations also point out that X-ray mass proxies do not work equally well at all radii. The origin of the effect is thought to be associated with cluster mergers. Recent work presenting the cluster maps showed an ability of X-ray maps to reveal and study cluster mergers in detail. Here, we present a first attempt to use the study of substructure in assessing the systematics of the hydrostatic mass measurements using two-dimensional (2D) X-ray diagnostics. The temperature map is uniquely able to identify the substructure in an almost relaxed cluster which would be unnoticed in the intracluster medium electron number density and pressure maps. We describe the radial fluctuations in the 2D maps by a cumulative/differential scatter profile relative to the mean profile within/at a given radius. The amplitude indicates {approx}10% fluctuations in the temperature, electron number density, and entropy maps, and {approx}15% fluctuations in the pressure map. The amplitude of and the discontinuity in the scatter complement 2D substructure diagnostics, e.g., indicating the most disturbed radial range. There is a tantalizing link between the substructure identified using the scatter of the entropy and pressure fluctuations and the hydrostatic mass bias relative to the expected mass based on the M-Y{sub X} and M-M{sub gas} relations particularly at r{sub 500}. XMM-Newton observations with {approx}120,000 source photons from the cluster are sufficient to apply our substructure diagnostics via the spectrally measured 2D temperature, electron number density, entropy, and pressure maps.

Zhang Yuying; Reiprich, Thomas H.; Hudson, Daniel S. [Argelander Institut fuer Astronomie, Universitaet Bonn, Auf dem Huegel 71, 53121 Bonn (Germany); Finoguenov, Alexis [Max-Planck-Institut fuer extraterrestrische Physik, Giessenbachstrasse, 85748 Garching (Germany); Sarazin, Craig L. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States)

2009-07-10T23:59:59.000Z

254

Jacobian-free Newton Krylov discontinuous Galerkin method and physics-based preconditioning for nuclear reactor simulations  

Science Conference Proceedings (OSTI)

We present high-order accurate spatiotemporal discretization of all-speed flow solvers using Jacobian-free Newton Krylov framework. One of the key developments in this work is the physics-based preconditioner for the all-speed flow, which makes use of traditional semi-implicit schemes. The physics-based preconditioner is developed in the primitive variable form, which allows a straightforward separation of physical phenomena. Numerical examples demonstrate that the developed preconditioner effectively reduces the number of the Krylov iterations, and the efficiency is independent of the Mach number and mesh sizes under a fixed CFL condition.

HyeongKae Park; Robert R. Nourgaliev; Richard C. Martineau; Dana A. Knoll

2008-09-01T23:59:59.000Z

255

Jefferson Lab Technology Transfer - JLab  

Grants and cooperative agreements are entered into solely by the government with a recipient whereby money or property is transferred to the recipient to support ...

256

Jefferson Lab Technology Transfer - JLab  

Proponents say scintimammography could save patients or their health care providers a lot of money on biopsies.

257

Career Opportunities at Jefferson Lab  

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

more courses from time to time after they 'finish' school to improve or update their skills and knowledge. They know they must always be learning if they want to be successful....

258

Jefferson Lab Science Series - Holograms  

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

Clocks and Timekeeping Previous Video (Clocks and Timekeeping) Science Series Video Archive Next Video (Which Way is Up?) Which Way is Up? Holograms Mr. Paul Christie - Liti...

259

Jefferson Lab Technology Transfer - JLab  

Dual Design Resistor for High Voltage Conditioning and Transmission Lines; Anatomic and Functional Imaging of Tagged Molecules in Animals;

260

Jefferson Science Associates, LLC - JLab  

Chief Financial Officer & Business Operations Manager, be based on JLab Management view ... risk capital and expenses necessary to bring the invention to the point of ...

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261

Jefferson Lab Technology Transfer - JLab  

This control system must provide supervisory I/O, local feedback control, analysis capability, and operator interfaces for numerous accelerator ...

262

Flat Stanley visits Jefferson Lab!  

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

halls, helps with the filming of an episode of Frostbite Theater, watches a National Science Bowl competition and strolls the sands of nearby Virginia Beach Next Page ...

263

Jefferson Lab Technology Transfer - JLab  

Invention Disclosure; CRADA/WFO Routing; Fairness of Opportunity; America Invents Act Summary; Achievements at JLab. Patents; New Inventions; New ...

264

Jefferson Lab Technology Transfer - JLab  

.6. A brief description of the company's commitment and overall plans to successfully develop, manufacture and sell products under the proposed ...

265

Jefferson Lab Technology Transfer - JLab  

... Health Sciences Center will be conducting the test programs including phantom studies to identify the detector type with the ... such a facility ...

266

Science Education at Jefferson Lab  

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

Education Privacy and Security Notice Science Education Teacher Resources Student Zone Games and Puzzles Science Cinema Programs and Events Search Science Education As a...

267

REACTIVE TRANSPORT MODELING USING A PARALLEL FULLY-COUPLED SIMULATOR BASED ON PRECONDITIONED JACOBIAN-FREE NEWTON-KRYLOV  

SciTech Connect

Systems of multicomponent reactive transport in porous media that are large, highly nonlinear, and tightly coupled due to complex nonlinear reactions and strong solution-media interactions are often described by a system of coupled nonlinear partial differential algebraic equations (PDAEs). A preconditioned Jacobian-Free Newton-Krylov (JFNK) solution approach is applied to solve the PDAEs in a fully coupled, fully implicit manner. The advantage of the JFNK method is that it avoids explicitly computing and storing the Jacobian matrix during Newton nonlinear iterations for computational efficiency considerations. This solution approach is also enhanced by physics-based blocking preconditioning and multigrid algorithm for efficient inversion of preconditioners. Based on the solution approach, we have developed a reactive transport simulator named RAT. Numerical results are presented to demonstrate the efficiency and massive scalability of the simulator for reactive transport problems involving strong solution-mineral interactions and fast kinetics. It has been applied to study the highly nonlinearly coupled reactive transport system of a promising in situ environmental remediation that involves urea hydrolysis and calcium carbonate precipitation.

Luanjing Guo; Chuan Lu; Hai Huang; Derek R. Gaston

2012-06-01T23:59:59.000Z

268

Comparing the performance of neural networks developed by using Levenberg-Marquardt and Quasi-Newton with the gradient descent algorithm for modelling a multiple response grinding process  

Science Conference Proceedings (OSTI)

Monitoring and control of multiple process quality characteristics (responses) in grinding plays a critical role in precision parts manufacturing industries. Precise and accurate mathematical modelling of multiple response process behaviour holds the ... Keywords: Back propagation neural network, Gradient descent algorithm, Levenberg-Marquardt algorithm, Multiple response, Quasi-Newton algorithm

Indrajit Mukherjee; Srikanta Routroy

2012-02-01T23:59:59.000Z

269

SWIFT AND XMM-NEWTON OBSERVATIONS OF THE EXTRAORDINARY GAMMA-RAY BURST 060729: MORE THAN 125 DAYS OF X-RAY AFTERGLOW  

E-Print Network (OSTI)

SWIFT AND XMM-NEWTON OBSERVATIONS OF THE EXTRAORDINARY GAMMA-RAY BURST 060729: MORE THAN 125 DAYS:1 and absorption column density of 1 ; 1021 cm?2 . Subject headinggs: gamma rays: bursts -- X-rays: bursts Online material: color figure 1. INTRODUCTION Gamma-ray bursts (GRBs) are the most powerful explosions

Zhang, Bing

270

Improving existing facade insulation against railway J. A.E. Paris-Newton, D. Chapman, C. Luciani and R. G. Mackenzie  

E-Print Network (OSTI)

Improving existing fa¸cade insulation against railway noise J. A.E. Paris-Newton, D. Chapman, C. Luciani and R. G. Mackenzie Building Performance Centre, 42 Colinton Road, Edinburgh, EH10 7DT Edinburgh the insulation offered by existing dwelling façades on approximately a thousand properties subject to railway

Paris-Sud XI, Université de

271

Fe Emission And Ionized Excess Absorption in the Luminous Quasar 3C109 With XMM-Newton  

Science Conference Proceedings (OSTI)

We report results from an XMM-Newton observation of the broad-line radio galaxy 3C 109 (z=0.3056). Previous ASCA data revealed the presence of a broad iron line from the accretion disc with which the XMM-Newton spectrum is fully consistent. However, although improving the ASCA constraints on the line parameters, the quality of the data is not high enough to distinguish between an untruncated accretion disc extending down to small radii close to the black hole and a scenario in which the innermost 20-30 gravitational radii are missing. For this reason, our results are model-dependent and the hard data can be modeled equally well by considering an absorption scenario in which a large column of neutral gas partially covers the X-ray continuum source. However, the absorber would have to comprise hundreds/thousands very compact clouds close to the X-ray source, which seems rather extreme a requirement. The 2-10 keV intrinsic luminosity of 3C 109 is of the order of 2-3 x 10{sup 45} erg s{sup -1} regardless of the adopted model. A recent black hole mass estimate of {approx} 2 x 10{sup 8} M{sub {circle_dot}} implies that L{sub bol}/L{sub Edd} > 1. If partial covering is excluded, the observed reflection fraction (of the order of unity), steep photon index (1.86), and Fe line equivalent width (about 100 eV) all suggest to exclude that the X-ray continuum is strongly beamed indicating that the large Eddington ratio is associated with a radiatively efficient accretion process and making it unlikely that the innermost accretion disc is replaced by a thick radiatively inefficient medium such as in advection-dominated accretion models. We also confirm previous findings on the detection of low energy absorption in excess of the Galactic value, where we find excellent agreement with previous results obtained in X-rays and at other wavelengths (optical and infrared). The better quality of the XMM-Newton data enables us to attribute the excess absorption to slightly ionized gas in the line of sight, located at the redshift of 3C 109. The most likely interpretation for the excess absorption is that the line-of-sight is grazing the obscuring torus of unified models, which is consistent with the inclination inferred from the Fe line profile (about 40{sup o}) and with the hybrid radio-galaxy/quasar nature of 3C 109.

Miniutti, Giovanni; /Cambridge U., Inst. of Astron.; Ballantyne, D.R.; /Arizona U.; Allen, S.W.; /KIPAC, Menlo Park; Fabian, A.C.; /Cambridge U., Inst. of Astron.; Ross, R.R.; /Holy Cross Coll.

2006-06-09T23:59:59.000Z

272

A systematic analysis of X-ray afterglows of gamma-ray burst observed by XMM-Newton  

E-Print Network (OSTI)

This work is part of a systematic re-analysis program of all the data of Gamma-Ray Burst (GRB) X-ray afterglows observed so far, in order to constrain the GRB models. We present here a systematic analysis of those afterglows observed by XMM-Newton between January 2000 and March 2004. This dataset includes GRB 011211 and GRB 030329. We have obtained spectra, light curves and colors for these afterglows. In this paper we focus on the continuum spectral and temporal behavior. We compare these values with the theoretical ones expected from the fireball model. We derive constraints about the burst environment (absorption, density profile) and put constraints on their beaming angle. Key words: Gamma-ray: burst, X-ray: general 1

Bruce Gendre A; Luigi Piro A; Massimiliano De Pasquale A

2004-01-01T23:59:59.000Z

273

EA-1841: Department of Energy Loan Guarantee for the Taylor Biomass Montgomery Project in the Town of Montgomery, Orange County, New York  

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

Taylor Biomass, LLC (Taylor) submitted an application to DOE for a Federal loan guarantee to support the construction and startup of a biomass gasification-to energy facility at a 95-acre recycling facility in the Town of Montgomery, Orange County, NY. The Project would involve the construction of a Post-Collection Separation Facility, a Gasification System and a Combined Cycle Gas Turbine Power Island.

274

Identification and confirmation of molecular markers and orange flesh color associated with major QTL for high beta-carotene content in muskmelon  

E-Print Network (OSTI)

Beta-carotene presence or absence in muskmelon is controlled by two genes, green flesh gf and white flesh wf. In its dominant form the wf gene is responsible for orange flesh color; however, the epistatic interactions of gf and wf can create three flesh colors: orange, white and green. Two F2 populations, consisting of 77 greenhouse grown and 117 field grown plants, from the cross of Sunrise (white fleshed) by TAM Uvalde (orange fleshed), were used to examine the relationships of beta-carotene content, flesh color, and flesh color intensity. Bulk segregent analysis was used with RAPD markers to identify molecular markers associated with high beta-carotene content. Flesh color and flesh color intensity both had significant relationships with beta-carotene content. A significant correlation between total soluble solids and beta-carotene content was also found. Molecular markers were identified in both F2 populations and all significant, associated markers from TAM Uvalde were linked with WF. A single QTL was also found to be linked with the WF locus. The identified QTL can be used to screen potential breeding lines for high beta-carotene. It was also confirmed that the visual ratings of flesh color intensity can be reliably used to select high beta-carotene content melons.

Napier, Alexandra Bamberger

2006-12-01T23:59:59.000Z

275

Creating web applications for spatial epidemiological analysis and mapping in R using Rwui  

E-Print Network (OSTI)

, pink > 5000, orange 500, yellow 0.5%, pink > 0.05%, orange > 0.005%, yellow < 0.005%). Newton et al. Source Code for Biology and Medicine 2011, 6:6 http...

Newton, Richard; Deonarine, Andrew; Wernisch, Lorenz

2011-04-01T23:59:59.000Z

276

Assessment of HTGR Helium Compressor Analysis Tool Based on Newton-Raphson Numerical Application to Through-flow Analysis  

SciTech Connect

This study describes the development of a computer program for analyzing the off-design performance of axial flow helium compressors, which is one of the major concerns for the power conversion system of a high temperature gas-cooled reactor (HTGR). The compressor performance has been predicted by the aerodynamic analysis of meridional flow with allowances for losses. The governing equations have been derived from Euler turbomachine equation and the streamline curvature method, and then they have been merged into linearized equations based on the Newton-Raphson numerical method. The effect of viscosity is considered by empirical correlations to introduce entropy rises caused by primary loss sources. Use of the method has been illustrated by applying it to a 20-stage helium compressor of the GTHTR300 plant. As a result, the flow throughout the stages of the compressor has been predicted and the compressor characteristics have been also investigated according to the design specification. The program results show much better stability and good convergence with respect to other through-flow methods, and good agreement with the compressor performance map provided by JAEA. (authors)

Ji Hwan Kim; Hyeun Min Kim; Hee Cheon NO [Korea Advanced Institute of Science and Technology, 335 Gwahangno - 373-1 Guseong-dong, Yuseong-gu, Daejeon 305-701 (Korea, Republic of)

2006-07-01T23:59:59.000Z

277

Spherically symmetric solutions, Newton's Law, and the infrared limit {lambda}{yields}1 in covariant Horava-Lifshitz gravity  

SciTech Connect

In this note we examine whether spherically symmetric solutions in covariant Horava-Lifshitz gravity can reproduce Newton's Law in the IR limit {lambda}{yields}1. We adopt the position that the auxiliary field A is independent of the space-time metric [J. Alexandre and P. Pasipoularides, Phys. Rev. D 83, 084030 (2011).][J. Greenwald, V. H. Satheeshkumar, and A. Wang, J. Cosmol. Astropart. Phys. 12 (2010) 007.], and we assume, as in [A. M. da Silva, Classical Quantum Gravity 28, 055011 (2011).], that {lambda} is a running coupling constant. We show that under these assumptions, spherically symmetric solutions fail to restore the standard Newtonian physics in the IR limit {lambda}{yields}1, unless {lambda} does not run, and has the fixed value {lambda}=1. Finally, we comment on the Horava and Melby-Thompson approach [P. Horava and C. M. Melby-Thompson, Phys. Rev. D 82, 064027 (2010).] in which A is assumed as a part of the space-time metric in the IR.

Alexandre, Jean [King's College London, Department of Physics, London WC2R 2LS (United Kingdom); Pasipoularides, Pavlos [Department of Physics, National Technical University of Athens, Zografou Campus GR 157 73, Athens (Greece)

2011-10-15T23:59:59.000Z

278

Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data  

E-Print Network (OSTI)

We have analyzed XMM-Newton Optical Monitor (OM) UV (180-400 nm) data for a sample of 33 galaxies, of which 30 are cluster members. Nine of these are central cluster galaxies (CCGs) in cooling flow clusters, having mass deposition rates which span a range of 8 to 525 solar masses per year. Using the ratio of UV to 2MASS J band flux, we find a significant UV excess in many, but not all, cooling flow CCGs. This UV excess is a direct indication of the presence of young massive stars, and therefore recent star formation, in these galaxies. Using the Starburst99 spectral energy distribution (SED) model of continuous star formation over a 900 Myr period, we derive star formation rates of 0.2 to 219 solar masses per year for the cooling flow sample. For 2/3 of this sample it is possible to equate Chandra/XMM cooling flow mass deposition rates with UV inferred star formation rates, for a combination of starburst lifetime and IMF slope. This is a pilot study of the well populated XMM UV cluster archive and a more extensive follow up study is currently underway.

Amalia K. Hicks; Richard Mushotzky

2005-08-04T23:59:59.000Z

279

MODELING THE OXYGEN K ABSORPTION IN THE INTERSTELLAR MEDIUM: AN XMM-NEWTON VIEW OF Sco X-1  

Science Conference Proceedings (OSTI)

We investigate the X-ray absorption structure of oxygen in the interstellar medium by analyzing XMM - Newton observations of the low-mass X-ray binary Sco X-1. Simple models based on the O I atomic photoabsorption cross section from different sources are used to fit the data and evaluate the impact of the atomic data on the interpretation of the observations. We show that relatively small differences in the atomic calculations can yield spurious results, and that the most complete and accurate set of atomic cross sections successfully reproduce the observed data in the 21.0-24.5 A wavelength region of the spectrum. Our fits indicate that the absorption is mainly due to neutral gas with an ionization parameter of {xi} = 10{sup -4} erg cm s{sup -1} and an oxygen column density of N{sub O} {approx} (8-10) x 10{sup 17} cm{sup -2}. The models are able to reproduce both the K edge and the K{alpha} absorption line from O I which are the two main features in this region. We find no conclusive evidence for absorption by anything other than atomic oxygen.

GarcIa, J.; Bautista, M. A. [Department of Physics, Western Michigan University, Kalamazoo, MI 49008 (United States); RamIrez, J. M. [Astrophysikalisches Institut Potsdam, An der Sternwarte 16 D-14482 Potsdam (Germany); Kallman, T. R.; Witthoeft, M. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Mendoza, C. [Centro de Fisica, IVIC, Caracas 1020 (Venezuela, Bolivarian Republic of); Palmeri, P.; Quinet, P., E-mail: javier.garcia@wmich.edu, E-mail: manuel.bautista@wmich.edu, E-mail: timothy.r.kallman@nasa.gov, E-mail: michael.c.witthoeft@nasa.gov, E-mail: jramirez@aip.de, E-mail: claudio@ivic.gob.v, E-mail: palmeri@umh.ac.be, E-mail: quinet@umh.ac.be [Astrophysique et Spectroscopie, Universite de Mons-UMONS, B-7000 Mons (Belgium)

2011-04-10T23:59:59.000Z

280

Temperature structure of the intergalactic medium within seven nearby and bright clusters of galaxies observed with XMM-Newton  

E-Print Network (OSTI)

Aims. We map the temperature structure of the intra-cluster medium (ICM) within a nearly complete X-ray flux limited sample of galaxy clusters in the redshift range z=[0.045,0.096]. Our sample contains seven bright clusters of galaxies observed with XMM-Newton: Abell 399, Abell 401, Abell 478, Abell 1795, Abell 2029, Abell 2065, Abell 2256. Methods. We use a multi-scale spectral mapping algorithm especially designed to map spectroscopic observables from X-ray extended emission of the ICM. Derived from a former algorithm using Haar wavelets, our algorithm is now implemented with B-spline wavelets in order to perform a more regular analysis of the signal. Results. For the four clusters in our sample that are major mergers, we find a complex thermal structure with strong thermal variations consistent with their dynamics. For two of them, A2065 and A2256, we perform a 3-d analysis of cold front features evidenced from the gas temperature and brightness maps. Furthermore, we detect a significant non-radial thermal structure outside the cool core region of the other 3 more "regular" clusters, with relative amplitudes of about about 10%. We investigate possible implications of this structure on the mass estimates of the "regular" clusters A1795 and A2029, by extracting surface brightness and temperature profiles from sectors correspondings to the hottest and coldest regions in the maps. While compensating with surface brightness for A2029, leading to consistent mass profiles, the temperature structure leads to significant mass discrepancies in the innermost region of A1795.

H. Bourdin; P. Mazzotta

2008-02-13T23:59:59.000Z

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JLab Science Activities for Teachers - 2006-2007 PowerPoint Presentati...  

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What do we study at Jefferson Lab? Bohr Model Diagrams (Elements 1-36) Fusion and Fission A Wave Review Sound and Waves Newton's Laws of Motion Work and Simple Machines Who...

282

Implementation of a level 1 trigger system using high speed serial (VXS) techniques for the 12GeV high luminosity experimental programs at Thomas Jefferson National Accelerator Facility  

SciTech Connect

We will demonstrate a hardware and firmware solution for a complete fully pipelined multi-crate trigger system that takes advantage of the elegant high speed VXS serial extensions for VME. This trigger system includes three sections starting with the front end crate trigger processor (CTP), a global Sub-System Processor (SSP) and a Trigger Supervisor that manages the timing, synchronization and front end event readout. Within a front end crate, trigger information is gathered from each 16 Channel, 12 bit Flash ADC module at 4 nS intervals via the VXS backplane, to a Crate Trigger Processor (CTP). Each Crate Trigger Processor receives these 500 MB/S VXS links from the 16 FADC-250 modules, aligns skewed data inherent of Aurora protocol, and performs real time crate level trigger algorithms. The algorithm results are encoded using a Reed-Solomon technique and transmission of this Level 1 trigger data is sent to the SSP using a multi-fiber link. The multi-fiber link achieves an aggregate trigger data transfer rate to the global trigger at 8 Gb/s. The SSP receives and decodes Reed-Solomon error correcting transmission from each crate, aligns the data, and performs the global level trigger algorithms. The entire trigger system is synchronous and operates at 250 MHz with the Trigger Supervisor managing not only the front end event readout, but also the distribution of the critical timing clocks, synchronization signals, and the global trigger signals to each front end readout crate. These signals are distributed to the front end crates on a separate fiber link and each crate is synchronized using a unique encoding scheme to guarantee that each front end crate is synchronous with a fixed latency, independent of the distance between each crate. The overall trigger signal latency is <3 uS, and the proposed 12GeV experiments at Jefferson Lab require up to 200KHz Level 1 trigger rate.

C. Cuevas, B. Raydo, H. Dong, A. Gupta, F.J. Barbosa, J. Wilson, W.M. Taylor, E. Jastrzembski, D. Abbott

2009-11-01T23:59:59.000Z

283

NEWTON: Rules of Science  

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Rules of Science Rules of Science Name: Steven Status: other Grade: 12+ Location: WA Country: USA Date: Spring 2012 Question: What are the hard-and-fast rules of science? Are there any? How does science avoid becoming fiction? Replies: Interesting question. Since the question posed refers to some generic 'science', I would offer these few thoughts.... Science (to me) involves careful, precise observation of some natural or man-made phenomenon, accurately and objectively capturing the observation, honestly and objectively sharing of the captured data, fair and objective analysis of the captured data, and fair, honest, and objective efforts to test and thereby replicate the data in the interest of adding the gathered information to the ever-growing body of gathered, analyzed, tested and replicated knowledge we accept as the nearest thing to "fact" we know. Collection of the observed components of the phenomenon with integrity can help us to make predictions of future similar and dissimilar events

284

NEWTON's Weather Archive  

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Weather Archive: Weather Archive: Loading Most Recent Weather Questions: Acid Rain and Evaporation Effects Ground Temperature for Snow to 'Stick' Clouds and Time of Day Chart Scales on Vertical Velocity Chart Aneroid Barometers: Aircraft; Meteorology Air and Saturation Pressure Tornado Size and Vortex Spin Rate Polar Air Pressure Coldest Temperature in Atmosphere; Elevation Snow Clump Formation Relative Humidity, Temperature, Amount of Water Polar Weather Systems Bergeron Process Cloud Formation and Time of Day Hailstone Shape Threshold Values for Classifying Pressure Systems Rain Shadow Range Cloud Suspension Measuring Rainfall Why Does It Rain? Measuring Rainfall Dew Point and Dogs Size of Cloud from Shadow What is dBZ in Meteorology? Daily Temperature Lag To see all entries in the Weather

285

NEWTON's References About Mathematics  

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Math References Math References Do you have a great math reference link? Please click our Ideas page. Featured Reference Links: Steve Marsden's Chemistry Resources Discovery Education's Mathematics Guide Discovery Educators have provided a Mathematics Guide for Educators. Included are numerous links to sites that touch on almost every mathematic topic that you are interested in. The Ultimate Math Portal The Ultimate Math Portal Whether you are confused by multiplication, need extra practice with geometry proofs, find yourself struggling to understand logarithms, or you just want to know more about pi, you are sure to find what you need with this great list of math facts and resources. MathIsFun.com MathIsFun.com Here, math is explained in easy language, for your students to understand. Plus, there are puzzles, games, quizzes, worksheets and a forum for more exploration. This site is designed for K-12 kids, teachers and parents to enjoy.

286

NEWTON's Material Science Archive  

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Materials Science Archive: Materials Science Archive: Loading Most Recent Materials Science Questions: Hydrogen Compounds and Heat Conduction Weaving Carbon Nanotubes Metal as Electrical Conductor, Not Thermal Steel Changes with Age PETE, Ultraviolet Light, Benefits Strength of Yarn by Spinning Each Substance Unique Density Alloy versus Constituent Density Knowing When Material is Melted Crystalline Metal Versus Metallic Glass and Conduction Super Glue, Surgery, and Skin Silica Gel Teflon Non-Stick Property Salt Crystal Formation Lubricating Rubber Bands and Elasticity Materials for Venus Probe Crystalline Solids and Lowest Energy Sodium Polycarbonate and Salt Water Early Adhesives Surface Energy and Temperature Separating Polypropylene, Polyester, and Nylon Factors Effecting Polymer Flexibility

287

NEWTON's Material Science Videos  

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Material Science Videos Material Science Videos Do you have a great material science video? Please click our Ideas page. Featured Videos: University of Maryland - Material Science University of Maryland - Material Science The Department of Materials Science and Engineering offers a set of videos about various topics in material science to help students understand what material science is. Learn about plasma, polymers, liquid crystals and much more. LearnersTV.com - Material Science LearnersTV.com - Material Science LearnersTV.com offers a series of educational material science lectures that are available to the public for free. Learn about topics like polymers, non-crystalline solids, crystal geometry, phase diagrams, phase transformations and more. NanoWerk - Nanotechnology Videos NanoWerk - Nanotechnology Videos

288

NEWTON's Metric System Resources  

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Please select any link below. Search this page, using your web browser's search function. Please select any link below. Search this page, using your web browser's search function. Metric System References Do you have a great metric reference link? Please click our Ideas page. Featured Reference Links: Metric (SI) References Metric (SI) References Having trouble with the metric system? Visit the National Institute of Standards and Technology's site about the rules and style conventions of the International System of Units (SI). The Metric System The Metric System Need another reference? Try this site provided by Wikipedia that discusses the metric system and its history in depth. Metric Converter Metric Converter Need to convert to Metric? OnlineConversion.com allows you to convert just about anything to just about anything else. This will let you easily from metric to US Standard notation, and vice versa.

289

NEWTON: Determining Material Degradation  

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Determining Material Degradation Determining Material Degradation Name: Hamish Status: student Grade: 6-8 Location: CA Country: USA Date: Summer 2013 Question: I am working on a science project about photo-degradation of plastic film. My question is how much degraded a plastic film should be to say that it was 100% photo-degraded? The plastic film I am photo-degrading is turning into dust when I touch it, what level of degradation is that? Replies: Hi Hamish, Thanks for the question. You will need to define what you mean by photo-degraded. 100% photo-degraded could be that the film becomes translucent and lets through only blurry images. Or it could mean that the film turns to dust when you touch it. As long as you clearly state in your science project what you mean by 100% photo-degraded, you will be doing a good job.

290

NEWTON's Botany References  

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Botany References Botany References Do you have a great botany video? Please click our Ideas page. Featured Videos: AOL News AOL News - Botany Videos AOL news provides hundreds of botany videos from around the world. View informational and instructional videos as well as interviews about the latest botany topics and discoveries. NeoK12 Plant Videos NeoK12 - Every Plant Topic Imaginable Explore videos encompassing every category dealing with plants. Learn about photosynthesis, plant evolution, reproduction, and many more plant related videos. Fungus Image Fungi Videos BBC Nature provides informational videos about fugni and other organisms. Learn and explore a wide variety of topics concerning the fungus kingdom. Other Botany Videos: Botany Videos for Kids Look at various botany videos geared towards a younger audience.

291

NEWTON: What is Equilibrium  

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What is Equilibrium? What is Equilibrium? Name: Lisa Status: student Grade: 6-8 Location: CA Country: USA Date: Spring 2012 Question: What is equilibrium? Are molecules still moving at equilibrium? Replies: Lisa, Imagine a seesaw (teeter-totter). If we start the seesaw parallel to the ground, put two objects, one on each end, and the objects have the same mass, the seesaw does not move. This is what is considered a static equilibrium - a balance. Nothing is changing. The object may move around, but as long as they stay on the same side of the seesaw, the balance is maintained. There is another way for the balance to be maintained. Suppose we put two jugglers, one on each end of the seesaw. Let's say the jugglers have the same mass and each hold four balls. The seesaw will also not move, remain parallel to the ground, when the jugglers toss the balls to each other - as long as they pass the balls to each other at the same rate so that the weights essentially remains the same on both ends. This is considered a dynamic equilibrium - things are moving back and forth, but a balance is maintained. In dynamic equilibrium, there is change (there is transfer between the two jugglers), but there is no net change (each juggler still ends up with the same overall mass).

292

NEWTON's Material Science References  

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Material Science References Material Science References Do you have a great material science reference link? Please click our Ideas page. Featured Reference Links: Materials Research Society Materials Research Society The Materials Research Society has assembled many resources in its Materials Science Enthusiasts site. This site has information for the K-12 audience, general public, and materials science professionals. Material Science nanoHUB nanHUB.org is the place for nanotechnology research, education, and collaboration. There are Simulation Programs, Online Presentations, Courses, Learning Modules, Podcasts, Animations, Teaching Materials, and more. (Intened for high school and up) Materials Science Resources on the Web Materials Science Resources on the Web This site gives a good general introduction into material science. Sponsered by Iowa State, it talks about what material science is, ceramics and composites, and other topics.

293

NEWTON's Botany References  

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Botany References Botany References Do you have a great botany reference link? Please click our Ideas page. Featured Reference Links: Dave's Garden - Plant Database Dave's Garden - Plant Database Visit Dave's Garden with information and photos for 185,359 different plants! United States Department of Agriculture Plant Database USDA PLANTS Database The PLANTS Database provides standardized information about the vascular plants, mosses, liverworts, hornworts, and lichens of the U.S. and its territories. Search over 40,000 plant images of US plants. Botany.com Botany.com Botany.com offers an encyclopedia of flowers and plants and resources to help people learn how to identify any different kinds of plants. Plant Kingdom This is a good reference for looking at the plant kingdom.

294

NEWTON's Molecular Biology References  

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Molecular Biology References Molecular Biology References Do you have a great reference link? Please click our Ideas page. Featured Reference Links: The Vitual Museum of Bacteria The Vitual Museum of Bacteria Visit the virtual museum of bacteria to learn more about bacteria and germs! This site brings together many links on bacteria, bacteriology, and related topics available on the web. It also provides crystal-clear information about many aspects of bacteria. The American Society of Cell Biology Cell Biology Educational Resources This site, sponsered by the American Society of Cell Biology, provides additional web links to everything from, general educational sites, to biology course materials, to teaching tools and more. National Center for Biotechnology Information National Center for Biotechnology Information

295

NEWTON's General Science References  

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General Science References General Science References Do you have a great general science reference link? Please click our Ideas page. Featured Reference Links: First.gov Science and Technology First.gov Science and Technology This site, sponsered by the US Government provides reference links to topics on science, telecommunications, computers, research agencies, and news. NASA Science NASA Science NASA Science, is a website sponsered by NASA, that supplies resources for understanding our world and the world above. Topics include earth science, heliophysics, the planets, astrophysics and much more. There is also an educator page! Nobel Laueate Listings and Stories Nobel Laueate Listings and Stories See the official site for the Nobel Prize, and read biographies about all of the Nobel Laureates, and there life changing discoveries and accomplishments.

296

NEWTON's Weather Links  

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References Do you have a great weather reference link? Please click our Ideas page. Featured Reference Links: NOAA Teachers Support Page NOAA Teachers Support Page for Weather and...

297

NEWTON's Physics References  

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Physics References Do you have a great physics reference link? Please click our Ideas page. Featured Reference Links: Physics Links Physics Links from AAPT See the American...

298

NEWTON's Physics Videos  

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Physics Videos Do you have a great physics video? Please click our Ideas page. Featured Videos: How Stuff Works Videos - Physics How Stuff Works Videos - Physics The Physics...

299

NEWTON's Energy References  

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"Nuclear Energy" experts with supportive classroom materials. ICCI Illinois Clean Coal Institute The Illinois Clean Coal Institute (ICCI) was established in December 1982 as...

300

NEWTON's Chemistry Videos  

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Chemistry Videos Do you have a great chemistry videos? Please click our Ideas page. Featured Videos: Steve Marsden's Chemistry Resources The Periodic Table of Videos The University...

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301

NEWTON's Chemistry References  

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Chemistry References Do you have a great chemistry reference link? Please click our Ideas page. Featured Reference Links: Steve Marsden's Chemistry Resources Steve Marsden's...

302

NEWTON's Engineering References  

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engineering content for K-12 teachers. There are activities, lessons, and curriculum designed to introduce your students to engineering. ENGINEERING.com ENGINEERING.com...

303

NEWTON's Veterinary Science Archive  

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Sniffing and Breathing in Dogs Dog Licking Behavior Dog Teeth and Hearing Cat heart Size Mammal Teeth Animal Reactions to ChemicalsDrugs Dogs and Time Cat Heart Rate...

304

NEWTON's General Science Videos  

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General Science Videos Do you have a great general science video? Please click our Ideas page. Featured Videos: Videos from National Geographic Kids Videos from National Geographic...

305

NEWTON: Green Hot  

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to two different phenomena. The 'red-hot' or 'white-hot' designations are due to black body radiation, which you can read about on-line. The colors of flames are due to ionization...

306

NEWTON's Zoology Archive  

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Process Robins Nest Duck Behavior Desert Hair Migrating Robins and Breast Color Fish Nostrils Insect Gas Exchange Shrew Physiology Fish Respiration Rates Long-eared Owl...

307

NEWTON's Chemistry Archive  

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in Filter Evaporation Experiment Gain? Energy in a System "Apparent Melting" Steel Wool, Soap, Water Absorption Diamond Growth and Seeds Energy for Sublimation Diffusion and...

308

NEWTON's Physics Archive  

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Light of Early Universe Filing Iron and Magnetism of Filings Atomic Mass Units and Atomic Particle Mass Source of Magnetic Force Photon Mass and Gravitation Buoyant Force on...

309

NEWTON's Veterinary Science References  

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Hospital Association presents HealthlyPet.com which gives detailed information about dog care, cat care, referral hospitals, and other resources. Is a link broken? Please let...

310

NEWTON's Zoology Videos  

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Planet - Videos Section Animal Planet online lets you see videos about cat breeds, dog breeds, wild animals and pets and much more. See and learn about animals courtesy of...

311

NEWTON's Astronomy Archive  

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Feel free to search in the search box below, or scroll through all of the records below the search box. Search the Astronomy Archive: Loading Most Recent Astronomy Questions:...

312

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Computer Science References Do you have a great computer reference link? Please click our Ideas page. Featured Reference Links: w3schools.com w3schools.com The site, w3schools.com,...

313

NEWTON's Computer Science Archive  

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Computer Science Archive: Loading Most Recent Computer Science Questions: Preparation for Video Game Creator Most Common Programming and Web Script How Does Spell Check Work? How...

314

NEWTON's Computer Science Videos  

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Computer Science Videos Do you have a great computer science video? Please click our Ideas page. Featured Videos: Computer Science Videos from Purdue Computer Science Videos from...

315

NEWTON's Weather Videos  

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day. Learn about all sorts of weather phenomena or just get a video of your daily forecast. NOAA Weather Partner's Videos NOAA Weather Partner's Videos The National Oceanic and...

316

NEWTON's Botany Archive  

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Coloration and Energy Double Pine Cones Botanical Beard Carbon Dioxide Amounts and Photosynthesis Plant Phases Red Oak Reproduction Propagation of "Star Fish" Banana Placentation...

317

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Molecular Biology Videos Do you have a great molecular biology video? Please click our Ideas page. Featured Videos: University of Berkeley - Molecular Biology Lectures University...

318

NEWTON's Molecular Biology Archive  

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Molecular Biology Archive: Loading Most Recent Molecular Biology Questions: Cytoplasm pH DNA Extract and Cold Alcohol Albino Gene Loci Male Development Candy and Bacteria Revisited...

319

NEWTON's Engineering Archive  

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Transmission and Grounding Turbulence Modeling and Wing Design Rentricity Heat Shield and 120,000 Foot Fall Hydrogen Peroxide and Fuel Cells Aquatic Exercise and Buoyancy...

320

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Please click our Ideas page. Featured Reference Links: Free Math Video Lectures Mathematics Online Courses View 100s of free instructional math videos. FreeVideoLectures...

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321

NEWTON: Size of Infinity  

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if the infinity obtained by limits in calculus is the largest possible quantity in mathematics and calculus for the following reason. I think that the infinity obtained in...

322

NEWTON: Pigeon Landing Behavior  

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an apartment with a balcony. We are curious to know why pigeons alight on the balcony rail first and if that is not possible, because our rail is oversized and curved, they...

323

NEWTON's General Science Archive  

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General Science Archive: Loading Most Recent General Science Questions: What is Equilibrium? Banana and Human Genetics Hair Examination Body Buffer Action Jellyfish : Plant or...

324

NEWTON's Astronomy Videos  

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Astronomy References Astronomy References Do you have a great astronomy video? Please click our Ideas page. Featured Videos: Space.com NASA's Video Gallery NASA offers a vast multimedia gallery, including their own video gallery. Watch videos about exploration and other missions that NASA is doing right now. Watch and discover more about astronomy and our galaxy. European Space Agency - Video Gallery European Space Agency - Video Gallery The European Space Agency also offers a vast multimedia gallery. Look at images of deep space, see tons of videos about ESA missions, watch many animations, and much more! There is something for all! Astronomy Magazine Astronomy Magazine The editors of Astronomy Magazine bring you hundreds of different astronomy videos. New videos are added daily so there's always something new to watch.

325

NEWTON: Why Meat Eaters?  

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Eaters? Name: Alexandre Status: student Grade: 6-8 Location: Outside U.S. Country: Canada Date: Spring 2013 Question: How come we are omnivores and vegetables and fruits are so...

326

NEWTON's Mathematics Archive  

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Mathematics Archive: Mathematics Archive: Loading Most Recent Questions on Mathematics: Standard Deviations Discontinuous Function Integration Secant, Cosecant, and Cotangent Uses Least Overlap Combinations Elliptical Appearance and Viewing Angle Combinations in Rotations Three Heads in Row on Flips Pi and Rectangle Gaussian Curve Summations Decimal System and Double Digits Multiples of Nine, Digit Sum Mathematics Log Books Tutorial on the term Term Functions Origin of Theta Equation for Pi Origin of FOIL Method Arabic Numerals and Shape 45 Degrees Does Not Halve Gravitational Field Intensity Bar for Repeating Decimals Term Size of Infinity Estimating Contrail Height Correlation and Causation Cube and Sphere Surface Area and Relative Size Solving X^2 = 2^X To see all entries in the Mathematics

327

Jefferson Lab Science Series - Einstein for Everyone  

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The Restoration of the USS Monitor The Restoration of the USS <i>Monitor</i> Previous Video (The Restoration of the USS Monitor) Science Series Video Archive Next Video (The Mysterious Universe) The Mysterious Universe Einstein for Everyone Dr. Robert Piccioni October 5, 2010 Young Einstein was a rebel who seemed doomed to fail. How did he overcome rejection to become the most famous scientist in history? We will discuss and explain all his theories in plain English and without math, and we will discover how Einstein's achievements impact our lives through DVDs, GPS, iPods, computers and green energy. Is the space above this area blank? If so, there may be a problem loading the embedded version of the video from YouTube. Either their server is having issues or your school is actively blocking access to YouTube. If

328

Jefferson Lab Science Series - The Ultimate Speed  

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Higgs Boson and Our Life Higgs Boson and Our Life Previous Video (The Higgs Boson and Our Life) Science Series Video Archive Next Video (What Is CEBAF All About?) What Is CEBAF All About? The Ultimate Speed Dr. William Bertozzi - Massachusetts Institute of Technology Sometime in 1962 In his youth, Dr. William Bertozzi, an MIT professor who has long been a leader in experimental nuclear physics using beams of electrons, carried out an experiment in which he explored the relationship between the velocity of electrons and their kinetic energy by measurements over a range of accelerating voltages between 0.5 MeV and 15 MeV. The kinetic energy is measured using calorimetry and the velocity is measured by time-of-flight. This educational film, made in 1962, documents the experiment and shows

329

Jefferson, Virginia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

645565°, -77.1877587° 645565°, -77.1877587° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.8645565,"lon":-77.1877587,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

330

Jefferson Electric Member Corp | Open Energy Information  

Open Energy Info (EERE)

Electric Member Corp Electric Member Corp Place Georgia Utility Id 9689 Utility Location Yes Ownership C NERC Location SERC NERC SERC Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png GENERAL SERVICE SCHEDULE B Commercial HIGH LOAD FACTOR SERVICE SCHEDULE HLF-13-R Commercial PREPAID RESIDENTIAL SERVICE SCHEDULE APP Residential RESIDENTIAL SERVICE SCHEDULE A Residential SCHEDULE ARP-1 ALLOCATED RESOURCE PRICING Commercial SCHEDULE ARP-2 McE ALLOCATED RESOURCE PRICING Commercial SCHEDULE C TOU TIME-OF-USE SERVICE Commercial SCHEDULE I-8 - greater than 30 kVA (Single Phase - Time-of-Use Energy

331

Jefferson Lab Science Series - Adventures in Science  

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

Physics IQ Test Previous Video (Physics IQ Test) Science Series Video Archive Next Video (Polymers, Foams and Gels) Polymers, Foams and Gels Adventures in Science Professor Cynthia...

332

Jefferson Lab Science Series - Space Shuttle Science  

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

Atlantis in the Chesapeake? Previous Video (Atlantis in the Chesapeake?) Science Series Video Archive Next Video (Mechanical Properties of Soda Cans) Mechanical Properties of Soda...

333

New Advances - Jefferson Lab Technology Transfer  

The Detector Group is collaborating with University of Virginia, on a medical instumentation project to improve breast tumor detection. The ...

334

Jefferson Lab Science Series - Symmetry - From Kaleidoscopes...  

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

Detecting Einstein's Gravity Waves Previous Video (Detecting Einstein's Gravity Waves) Science Series Video Archive Next Video (Physics IQ Test) Physics IQ Test Symmetry - From...

335

New Advances - Jefferson Lab Technology Transfer  

New Advances Commercial Spin-offs Abound For New Free Electron Laser. The world of laser technology took a giant leap forward recently as researchers ...

336

Jefferson Lab Science Series - Comic Book Physics  

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

(Multi-Million Dollar Forgeries Exposed) Multi-Million Dollar Forgeries Exposed Comic Book Physics Dr. Jim Kakalios - University of Minnesota March 25, 2003 Even superheroes must...

337

Jefferson Lab Science Series - Where's the Beach?  

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

What Is CEBAF All About? Previous Video (What Is CEBAF All About?) Science Series Video Archive Next Video (Superconducting BAYCO Bits) Superconducting BAYCO Bits Where's the...

338

Jefferson Lab Science Series - What's for Dinner?  

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

lurking in your food? How are they produced and how harmful are they? Dr. Kristen Kulp, a cancer research scientist, will perform demonstrations to illustrate methods used to...

339

Jefferson Lab Science Series - Guesstimating the Environment  

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

Video (The Origin of the Elements) Science Series Video Archive Next Video (The Higgs Boson and Our Life) The Higgs Boson and Our Life Guesstimating the Environment Dr....

340

Thomas Jefferson National Accelerator Facility Technology ...  

Energy Innovation Portal Technologies. Search Help ... This invention can produce copious quantities of carbon nanotubes at rates near grams per hour.

Note: This page contains sample records for the topic "newton orange jefferson" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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341

Jefferson City - Property Assessed Clean Energy | Department...  

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

Lighting Insulation Other Bioenergy Manufacturing Buying & Making Electricity Solar Wind Program Information Missouri Program Type PACE Financing Property-Assessed Clean Energy...

342

Nucleon spin physics at Jefferson Lab  

Science Conference Proceedings (OSTI)

In this talk I shall review some of the important results from the spin physics program at JLab and give an outlook for the 12 GeV upgrade spin program.

Zein-Eddine Meziani

2006-06-05T23:59:59.000Z

343

Jefferson Lab Science Series - Investigating Earth's Atmosphere  

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

Byron Meadows - NASALangley Research Center May 14, 1991 Demonstrations of weather forecasting tools and techniques for experiments in the atmosphere and of lasers used to...

344

Jefferson Lab Science Series - Lowering the Boom!  

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

with Earth) Science Series Video Archive Next Video (Environmental Impact of Global Burning) Environmental Impact of Global Burning Lowering the Boom Dr. Christine Darden -...

345

Jefferson Lab Science Series - Volcanoes in Virginia!  

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

Dr. Elizabeth Baedke Johnson - James Madison University January 24, 2012 The recent earthquake may have you wondering what other surprises Virginia's geology may hold. Could there...

346

From Newton to Hawking and beyond: Why disability equality is relevant to the world of particle physics - by Dr T. Shakespeare  

E-Print Network (OSTI)

According to the recent World report on disability, 15% of the worlds population is disabled. Among that group could be numbered famous physicists such as Isaac Newton, Paul Dirac & Stephen Hawking. This presentation will provide some basic data about global disability, and the socially-imposed barriers which disabled people face.It will also offer some practical suggestions on how to respect and include people with disabilities in the workplace. Tom Shakespeare is a social scientist and ethicist with 25 years experience with the disability movement. Between 2008-2013, Tom worked in the Disability and Rehabilitation team at the World Health Organization, Geneva. He currently teaches medical sociology at the University of East Anglia Medical School, in Norwich, UK.

CERN. Geneva

2013-01-01T23:59:59.000Z

347

XMM-Newton and Chandra Spectroscopy of the Variable High-Energy Absorption of PG 1115+080: Refined Outflow Constraints  

E-Print Network (OSTI)

We present results from multi-epoch spectral analysis of XMM-Newton and Chandra observations of the mini broad absorption line (BAL) quasar PG 1115+080. This is one of the few X-ray detected mini-BAL quasars to date that is bright enough in the X-ray band, mostly due to large gravitational-lensing magnifications, to allow in-depth spectral analysis. The present XMM-Newton observations of PG 1115+080 have provided the highest signal-to-noise X-ray spectra of a mini-BAL quasar obtained to date. By modeling the spectra of PG 1115+080 we have obtained constraints on the column density and ionization state of its outflowing absorbing gas. A comparison between these constraints over several epochs indicates significant variability in the properties of the outflowing absorbers in PG 1115+080. The depths of the high-energy broad absorption features in PG 1115+080 show a significant decrease between the first two observation epochs separated by a rest-frame timescale of ~ 1 year. This variability supports the intrinsic nature of these absorbers. Assuming the interpretation that the high-energy absorption features arise from highly ionized Fe XXV we constrain the fraction of the total bolometric energy released by quasars PG 1115+080 and APM 08279+5225 into the IGM in the form of kinetic energy to be epsilon_k = 0.64(-0.40,+0.52) (68% confidence), and epsilon_k =0.09(-0.05,+0.07), respectively. According to recent theoretical studies this range of efficiencies is large enough to influence significantly the formation of the host galaxy and to regulate the growth of the central black hole.

G. Chartas; W. N. Brandt; S. C. Gallagher; D. Proga

2007-01-04T23:59:59.000Z

348

XMM-Newton observations of the Small Magellanic Cloud: X-ray outburst of the 6.85 s pulsar XTE J0103-728  

E-Print Network (OSTI)

A bright X-ray transient was seen during an XMM-Newton observation in the direction of the Small Magellanic Cloud (SMC) in October 2006. The EPIC data allow us to accurately locate the source and to investigate its temporal and spectral behaviour. X-ray spectra covering 0.2-10 keV and pulse profiles in different energy bands were extracted from the EPIC data. The detection of 6.85 s pulsations in the EPIC-PN data unambiguously identifies the transient with XTE J0103-728, discovered as 6.85 s pulsar by RXTE. The X-ray light curve during the XMM-Newton observation shows flaring activity of the source with intensity changes by a factor of two within 10 minutes. Modelling of pulse-phase averaged spectra with a simple absorbed power-law indicates systematic residuals which can be accounted for by a second emission component. For models implying blackbody emission, thermal plasma emission or emission from the accretion disk (disk-blackbody), the latter yields physically sensible parameters. The photon index of the power-law of ~0.4 indicates a relatively hard spectrum. The 0.2-10 keV luminosity was 2x10^{37} with a contribution of ~3% from the disk-blackbody component. A likely origin for the excess emission is reprocessing of hard X-rays from the neutron star by optically thick material near the inner edge of an accretion disk. From a timing analysis we determine the pulse period to 6.85401(1) s indicating an average spin-down of ~0.0017 s per year since the discovery of XTE J0103-728 in May 2003. The X-ray properties and the identification with a Be star confirm XTE J0103-728 as Be/X-ray binary transient in the SMC.

F. Haberl; W. Pietsch

2008-01-30T23:59:59.000Z

349

The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources  

E-Print Network (OSTI)

We present the first results of the measurements of angular auto-correlation functions (ACFs) of X-ray point sources detected in the XMM-Newton observations of the 2 deg2 COSMOS field (XMM-COSMOS). A significant positive signals have been detected in the 0.5-2 (SFT) band, in the angle range of 0.5-24 arcminutes, while the positive signals were at the 2 and 3 sigma levels in the 2-4.5 (MED) and 4.5-10 (UHD) keV bands respectively. Correctly taking integral constraints into account is a major limitation in interpreting our results. With power-law fits to the ACFs without the integral constraint term, we find correlation lengths of theta_c=1.9+-0.3, 0.8+0.5-0.4 and 6+-2 arcseconds for the SFT, MED, and UHD bands respectively for gamma=1.8. The inferred comoving correlation lengths, also taking into account the bias by the source merging due to XMM-Newton PSF, are 9.8+-0.7, 5.8+1.4-1.7 and 12+-2 h-1 Mpc at the effective redshifts of 1.1, 0.9, and 0.6 for the SFT, MED, and UHD bands respectively. If we include the integral constraint term in the fitting process,assuming that the power-law extends to the scale length of the entire XMM-COSMOSfield, the correlation lengths become larger by 20%-90%. Comparing the inferred rms fluctuations of the spatial distribution of AGNs with those of the underlying mass, the bias parameters of the X-ray source clustering at these effective redshifts are in the range b(AGN)=1.5-4. (Edited to simple ascii.)

Takamitsu Miyaji; Giovanni Zamorani; Nico Cappelluti; Roberto Gilli; Richard E. Griffiths; Andrea Comastri; Guenther Hasinger; Marcella Brusa; Fabrizio Fiore; Simonetta Puccetti; Luigi Guzzo; Alexis Finoguenov

2006-12-14T23:59:59.000Z

350

The XMM-Newton wide-field survey in the COSMOS field: V. Angular Clustering of the X-ray Point Sources  

E-Print Network (OSTI)

We present the first results of the measurements of angular auto-correlation functions (ACFs) of X-ray point sources detected in the XMM-Newton observations of the ? 2 deg2 COSMOS field (XMM-COSMOS). A significant positive signals have been detected in the 0.5-2 (SFT) band, in the angle range of 0.5-24 arcminutes, while the positive signals were at the ?2 and ? 3? levels in the 2-4.5 (MED) and 4.5-10 (UHD) keV bands respectively. Correctly taking integral constraints into account is a major limitation in interpreting our results. With power-law fits to the ACFs without the integral constraint term, we find correlation lengths of ?c = 1. ? ? 9 0. ? ? 3, 0. ? ? 8 +0.? ? 5 ?0. ? ? 4 and 6 ? ? 2 ? ? for the SFT, MED, and UHD bands respectively for ? = 1.8. The inferred comoving correlation lengths, also taking into account the bias by the source merging due to XMM-Newton PSF, are rc ? 9.8 0.7, 5.8 +1.4 ?1.7 and 12 2 h?1 Mpc at the effective redshifts of zeff ? 1.1, 0.9, and 0.6 for the SFT, MED, and UHD bands respectively. If we include the integral constraint term in the fitting process, assuming that the power-law extends to the scale length of the entire XMM-COSMOS field, the correlation lengths become larger by ? 20%90%. Comparing the inferred rms fluctuations of the spatial distribution of AGNs ?8,AGN with those of the underlying mass, the bias parameters of the X-ray source clustering at these effective redshifts are in the range bAGN = 1.5 ? 4.

Takamitsu Miyaji; Giovanni Zamorani; Roberto Gilli; Richard E; Andrea Comastri; Gnther Hasinger; Marcella Brusa; Simonetta Puccetti; Luigi Guzzo; Alexis Finoguenov

2006-01-01T23:59:59.000Z

351

Probing Unification With Chandra HETGS and XMM-Newton EPIC And RGS Spectroscopy of the Narrow Emission Line Galaxy NGC 2110  

E-Print Network (OSTI)

We present results from Chandra HETGS (250 ks over two epochs) and XMM-Newton EPIC and RGS (60 ks) observations of NGC 2110, which has been historically classified as a Narrow Emission Line Galaxy galaxy. Our results support the interpretation that the source is a Seyfert 2 viewed through a patchy absorber. The nuclear X-ray spectrum of the source is best described by a power law of photon index $\\Gamma$ ~1.7, modified by absorption from multiple layers of neutral material at a large distance from the central supermassive black hole. We report the strong detections of Fe K$\\alpha$ and Si K$\\alpha$ lines, which are marginally resolved with the Chandra HETGS, and we constrain the emission radius of the fluorescing material to >1 pc. There is some evidence for modest additional broadening at the base of the narrow Fe K$\\alpha$ core with a velocity ~4500 km s$^{-1}$. We find tentative evidence for ionized emission (O VIII Ly $\\alpha$, an O VIII RRC feature, and possibly a Ne IX forbidden line) in the Chandra MEG and XMM-Newton RGS spectra, which could be associated with the known extended X-ray emission that lies ~160 pc from the nucleus. We suggest that the $10^{23}$ cm$^{-2}$ partially covering absorber originates in broad-line region clouds in the vicinity of the AGN, and that the $3\\times10^{22}$ cm$^{-2}$ coverer is likely to have a more distant origin and have a flattened geometry in order to allow the small-scale radio jet to escape.

Daniel A. Evans; Julia C. Lee; T. Jane Turner; Kimberly A. Weaver; Herman L. Marshall

2007-08-30T23:59:59.000Z

352

A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray Source NGC 5408 X-1 with XMM-Newton  

E-Print Network (OSTI)

We present results of new XMM-Newton observations of the ultraluminous X-ray source (ULX) NGC 5408 X-1, one of the few ULXs to show quasi-periodic oscillations (QPO). We detect QPOs in each of four new (~ 100 ks) pointings, expanding the range of frequencies observed from 10 - 40 mHz. We compare our results with the timing and spectral correlations seen in stellar-mass black hole systems, and find that the qualitative nature of the timing and spectral behavior of NGC 5408 X-1 is similar to systems in the steep power-law state exhibiting Type-C QPOs. However, in order for this analogy to quantitatively hold we must only be seeing the so-called saturated portion of the QPO frequency - photon index (or disk flux) relation. Assuming this to be the case, we place a lower limit on the mass of NGC 5408 X-1 of > 800 solar masses. Alternatively, the QPO frequency is largely independent of the spectral parameters, in which case a close analogy with the Type-C QPOs in stellar systems is problematic. Measurement of the s...

Pasham, Dheeraj R

2013-01-01T23:59:59.000Z

353

Probing Unification With Chandra HETGS and XMM-Newton EPIC And RGS Spectroscopy of the Narrow Emission Line Galaxy NGC 2110  

E-Print Network (OSTI)

We present results from Chandra HETGS (250 ks over two epochs) and XMM-Newton EPIC and RGS (60 ks) observations of NGC 2110, which has been historically classified as a Narrow Emission Line Galaxy galaxy. Our results support the interpretation that the source is a Seyfert 2 viewed through a patchy absorber. The nuclear X-ray spectrum of the source is best described by a power law of photon index $\\Gamma$ ~1.7, modified by absorption from multiple layers of neutral material at a large distance from the central supermassive black hole. We report the strong detections of Fe K$\\alpha$ and Si K$\\alpha$ lines, which are marginally resolved with the Chandra HETGS, and we constrain the emission radius of the fluorescing material to >1 pc. There is some evidence for modest additional broadening at the base of the narrow Fe K$\\alpha$ core with a velocity ~4500 km s$^{-1}$. We find tentative evidence for ionized emission (O VIII Ly $\\alpha$, an O VIII RRC feature, and possibly a Ne IX forbidden line) in the Chandra MEG ...

Evans, Daniel A; Turner, T Jane; Weaver, Kimberly A; Marshall, Herman L

2007-01-01T23:59:59.000Z

354

Orange and Rockland Case Study  

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

west of New York City. ORU is a key participant in Con Edison's 272 million Smart Grid Investment Grant (SGIG) project to modernize electric distribution systems. With 136...

355

Three XMM-Newton observations of the Anomalous X-ray Pulsar 1E 1048.1-5937: long term variations in spectrum and pulsed fraction  

E-Print Network (OSTI)

We report the results of a recent (July 2004) XMM-Newton Target of Opportunity observation of the Anomalous X-ray pulsar 1E 1048.1-5937, together with a detailed re-analysis of previous observations carried out in 2000 and 2003. In July 2004 the source had a 2-10 keV flux of 6.2$\\times10^{-12}$ erg cm$^{-2}$ s$^{-1}$ and a pulsed fraction P$_F$=0.68. The comparison of the three data sets shows the presence of an anti-correlation between flux and pulsed fraction, implying that previous estimates of the source energetics based on the assumption of a large and constant pulsed fraction might be significantly underestimated. The source spectrum is well described by a power law plus blackbody model (kT~0.63 keV, photon index $\\Gamma$~2.7-3.5) or, alternatively, by the sum of two blackbodies of which the hotter is Comptonized by relativistic electrons. In this case the temperatures are kT${_1}$~0.2-0.3 keV and kT${_2}$~0.4-0.5 keV and the emitting area of the cooler component is consistent with the whole neutron star surface. The long term luminosity variation of a factor >~2 is accompanied by relatively small variations in the spectral shape. Phase resolved spectroscopy indicates a harder spectrum in correspondence of the pulse maximum. No spectral features have been detected with 4$\\sigma$ limits on the equivalent width in the range ~10-220 eV, depending on line energy and width.

A. Tiengo; S. Mereghetti; R. Turolla; S. Zane; N. Rea; L. Stella; G. L. Israel

2005-03-17T23:59:59.000Z

356

GOMA 6.0 : a full-Newton finite element program for free and moving boundary problems with coupled fluid/solid momentum, energy, mass, and chemical species transport : user%3CU%2B2019%3Es guide.  

SciTech Connect

Goma 6.0 is a finite element program which excels in analyses of multiphysical processes, particularly those involving the major branches of mechanics (viz. fluid/solid mechanics, energy transport and chemical species transport). Goma is based on a full-Newton-coupled algorithm which allows for simultaneous solution of the governing principles, making the code ideally suited for problems involving closely coupled bulk mechanics and interfacial phenomena. Example applications include, but are not limited to, coating and polymer processing flows, super-alloy processing, welding/soldering, electrochemical processes, and solid-network or solution film drying. This document serves as a user's guide and reference.

Schunk, Peter Randall; Rao, Rekha Ranjana; Chen, Ken Shuang; Labreche, Duane A.; Sun, Amy Cha-Tien; Hopkins, Matthew Morgan; Moffat, Harry K.; Roach, Robert Allen; Hopkins, Polly L.; Notz, Patrick K.; Roberts, Scott Alan; Sackinger, Philip A.; Subia, Samuel Ramirez; Wilkes, Edward Dean; Baer, Thomas A.; Noble, David R.; Secor, Robert B. [3M Engineering Systems and Technology, St. Paul, MN

2013-07-01T23:59:59.000Z

357

JOINT ANALYSIS OF CLUSTER OBSERVATIONS. II. CHANDRA/XMM-NEWTON X-RAY AND WEAK LENSING SCALING RELATIONS FOR A SAMPLE OF 50 RICH CLUSTERS OF GALAXIES  

SciTech Connect

We present a study of multiwavelength X-ray and weak lensing scaling relations for a sample of 50 clusters of galaxies. Our analysis combines Chandra and XMM-Newton data using an energy-dependent cross-calibration. After considering a number of scaling relations, we find that gas mass is the most robust estimator of weak lensing mass, yielding 15% {+-} 6% intrinsic scatter at r{sub 500}{sup WL} (the pseudo-pressure Y{sub X} yields a consistent scatter of 22% {+-} 5%). The scatter does not change when measured within a fixed physical radius of 1 Mpc. Clusters with small brightest cluster galaxy (BCG) to X-ray peak offsets constitute a very regular population whose members have the same gas mass fractions and whose even smaller (<10%) deviations from regularity can be ascribed to line of sight geometrical effects alone. Cool-core clusters, while a somewhat different population, also show the same (<10%) scatter in the gas mass-lensing mass relation. There is a good correlation and a hint of bimodality in the plane defined by BCG offset and central entropy (or central cooling time). The pseudo-pressure Y{sub X} does not discriminate between the more relaxed and less relaxed populations, making it perhaps the more even-handed mass proxy for surveys. Overall, hydrostatic masses underestimate weak lensing masses by 10% on the average at r{sub 500}{sup WL}; but cool-core clusters are consistent with no bias, while non-cool-core clusters have a large and constant 15%-20% bias between r{sub 2500}{sup WL} and r{sub 500}{sup WL}, in agreement with N-body simulations incorporating unthermalized gas. For non-cool-core clusters, the bias correlates well with BCG ellipticity. We also examine centroid shift variance and power ratios to quantify substructure; these quantities do not correlate with residuals in the scaling relations. Individual clusters have for the most part forgotten the source of their departures from self-similarity.

Mahdavi, Andisheh [Department of Physics and Astronomy, San Francisco State University, San Francisco, CA 94131 (United States); Hoekstra, Henk [Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden (Netherlands); Babul, Arif; Bildfell, Chris [Department of Physics and Astronomy, University of Victoria, Victoria, BC V8W 3P6 (Canada); Jeltema, Tesla [Santa Cruz Institute for Particle Physics, UC Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Henry, J. Patrick [Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

2013-04-20T23:59:59.000Z

358

AN XMM-NEWTON SURVEY OF THE SOFT X-RAY BACKGROUND. II. AN ALL-SKY CATALOG OF DIFFUSE O VII AND O VIII EMISSION INTENSITIES  

Science Conference Proceedings (OSTI)

We present an all-sky catalog of diffuse O VII and O VIII line intensities, extracted from archival XMM-Newton observations. This catalog supersedes our previous catalog, which covered the sky between l = 120 Degree-Sign and l = 240 Degree-Sign . We attempted to reduce the contamination from near-Earth solar wind charge exchange (SWCX) emission by excluding times of high solar wind proton flux from the data. Without this filtering, we were able to extract measurements from 1868 observations. With this filtering, nearly half of the observations became unusable, and only 1003 observations yielded measurements. The O VII and O VIII intensities are typically {approx}2-11 and {approx}10 L.U. were observed. We compared our measurements with models of the heliospheric and geocoronal SWCX. The heliospheric SWCX intensity is expected to vary with ecliptic latitude and solar cycle. We found that the observed oxygen intensities generally decrease from solar maximum to solar minimum, both at high ecliptic latitudes (which is as expected) and at low ecliptic latitudes (which is not as expected). The geocoronal SWCX intensity is expected to depend on the solar wind proton flux incident on the Earth and on the sightline's path through the magnetosheath. The intensity variations seen in directions that have been observed multiple times are in poor agreement with the predictions of a geocoronal SWCX model. We found that the oxygen lines account for {approx}40%-50% of the 3/4 keV X-ray background that is not due to unresolved active galactic nuclei, in good agreement with a previous measurement. However, we found that this fraction is not easily explainable by a combination of SWCX emission and emission from hot plasma in the halo. We also examined the correlations between the oxygen intensities and Galactic longitude and latitude. We found that the intensities tend to increase with longitude toward the inner Galaxy, possibly due to an increase in the supernova rate in that direction or the presence of a halo of accreted material centered on the Galactic center. The variation of intensity with Galactic latitude differs in different octants of the sky, and cannot be explained by a single simple plane-parallel or constant-intensity halo model.

Henley, David B.; Shelton, Robin L., E-mail: dbh@physast.uga.edu [Department of Physics and Astronomy, University of Georgia, Athens, GA 30602 (United States)

2012-10-15T23:59:59.000Z

359

NEWTON: Why Does It Rain  

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

Why Does It Rain? Why Does It Rain? Name: Drama Status: student Grade: K-3 Location: FL Country: USA Date: Fall 2011 Question: Why does it rain? Replies: Drama, When water is heated it evaporates into the air. You cannot see the water in the air, but sometimes you can feel it (especially when it is hot outside). Have you ever noticed that on some warm days it is really humid (sticky and sweaty) and other warm days it feels dry? You might have also noticed that in the morning, when the air is cool, you might find dew or mist on the leaves and grass. This occurs because cold air cannot hold much of moisture. There is a limit to the amount of water that air can hold. This limit is known as the saturation limit (or dew point). When the air is completely saturated and cannot hold any more water, then it comes down as rain (and leaves all that heat in the air).

360

NEWTON: Preventing Tire Dry Rot  

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

Preventing Tire Dry Rot Preventing Tire Dry Rot Name: Millard Status: student Grade: 9-12 Location: MD Country: USA Date: Spring 2013 Question: My dad has a classic car, and because it gets driven very little each year, the tires dry rot before he can get much tread wear on them. What could be used to protect the tires from dry rot and cracking? Replies: Hi Millard, Thanks for the question. I would recommend keeping the car on blocks so that there is no weight on the tires. Additionally, I would recommend that no electrical equipment (motors, switches, and other things that spark) be used around the car. The sparks generate ozone and ozone can cause rubber items such as tires, belts, and hoses to crack. I hope this helps. Please let me know if you have more questions. Thanks Jeff Grell

Note: This page contains sample records for the topic "newton orange jefferson" 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

NEWTON'S METHOD FOR MULTIOBJECTIVE OPTIMIZATION ...  

E-Print Network (OSTI)

estimations on the error of approximating F, ?Fj by its quadratic and ...... A subjective assessment of alternative mission architectures for the human ex- ploration...

362

NEWTON: Blood Group Systems Usage  

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

Blood Group Systems Usage Blood Group Systems Usage Name: Kishori Status: student Grade: n/a Location: Outside U.S. Country: India Date: Summer 2013 Question: What is the difference between MN blood group system and ABO bloodgroup system? Although, we nowadays prefer ABO blood groups why do we use MN blood groups in the forensic department? Replies: Humans actually have multiple blood antigens on the surface of our blood cells. Wikipedia says that there are over 50 different blood group antigens. ABO and Rh are just the most dominant. Rh actually has 3 alleles called C, D and E. So one could be CCddee, for example, but clinically, when referring to Rh, only the D antigen is considered. So MN is another system that is also present. The reason it would be considered in forensics is due to population genetics considerations. Certain combinations are found in different percentages depending on what ancestry a person is a part of. Humans evolved in isolation from each other and until relatively recently, were separated due to difficult travel/migration. But even though we can move around the planet easily now, we still carry the history of our ancestry in our DNA. M and N are codominant, like the ABO system.

363

CHANDRA AND XMM-NEWTON STUDIES OF THE SUPERNOVA REMNANT G292.2-0.5 ASSOCIATED WITH THE PULSAR J1119-6127  

SciTech Connect

We present the first detailed imaging and spatially resolved spectroscopic study of the Galactic supernova remnant (SNR) G292.2-0.5, associated with the high-magnetic field radio pulsar (PSR) J1119-6127, using Chandra and XMM-Newton. The high-resolution X-ray images reveal a partially limb-brightened morphology in the west, with diffuse emission concentrated toward the interior of the remnant unlike the complete shell-like morphology observed at radio wavelengths. The spectra of most of the diffuse emission regions within the remnant are best described by a two-component thermal+non-thermal model. The thermal component is described by a plane-parallel, non-equilibrium ionization plasma model with a temperature kT ranging from 1.3{sup +0.3}{sub -0.2} keV in the western side of the remnant to 2.3{sup +2.9}{sub -0.5} keV in the east, a column density increasing from 1.0{sup +0.1}{sub -0.6} Multiplication-Sign 10{sup 22} cm{sup -2} in the west to 1.8{sup +0.2}{sub -0.4} Multiplication-Sign 10{sup 22} cm{sup -2} in the east, and a low ionization timescale ranging from (5.7{sup +0.8}{sub -0.7}) Multiplication-Sign 10{sup 9} cm{sup -3} s in the SNR interior to (3.6{sup +0.7}{sub -0.6}) Multiplication-Sign 10{sup 10} cm{sup -3} s in the western side-suggestive of expansion of a young remnant in a low-density medium. The spatial and spectral differences across the SNR are consistent with the presence of a dark cloud in the eastern part of the SNR, absorbing the soft X-ray emission, as also revealed by the optical image of that region. The spectra from some of the regions also show slightly enhanced metal abundances from Ne, Mg, and Si, hinting at the first evidence for ejecta heated by the reverse shock. Comparing our inferred metal abundances to core-collapse nucleosynthesis models yields, we estimate a high progenitor mass of {approx}30 M{sub Sun} suggesting a Type Ib/c supernova. We confirm the presence of non-thermal X-ray emission from regions close to the pulsar, with the emission characterized by a power-law model with a hard photon index similar to that seen in the compact pulsar wind nebula. We estimate an SNR age range between 4.2 kyr (free expansion phase) and 7.1 kyr (Sedov phase) at an assumed distance of 8.4 kpc, a factor of a few higher than the measured pulsar's age upper limit of 1.9 kyr.

Kumar, Harsha S.; Safi-Harb, Samar [Department of Physics and Astronomy, University of Manitoba, Winnipeg, MB, R3T 2N2 (Canada); Gonzalez, Marjorie E., E-mail: harsha@physics.umanitoba.ca, E-mail: samar@physics.umanitoba.ca, E-mail: gonzalez@phas.ubc.ca [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z1 (Canada)

2012-08-01T23:59:59.000Z

364

Jefferson Hills, Pennsylvania: Energy Resources | Open Energy Information  

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9°, -79.9319942° 9°, -79.9319942° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.2911809,"lon":-79.9319942,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

365

Jefferson Valley-Yorktown, New York: Energy Resources | Open Energy  

Open Energy Info (EERE)

Valley-Yorktown, New York: Energy Resources Valley-Yorktown, New York: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.3138618°, -73.800734° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.3138618,"lon":-73.800734,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

366

Jefferson Lab Science Series - Proton Therapy - Accelerating Protons to  

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The Science of Chocolate The Science of Chocolate Previous Video (The Science of Chocolate) Science Series Video Archive Next Video (Adventures in Infectious Diseases) Adventures in Infectious Diseases Proton Therapy - Accelerating Protons to Save Lives Dr. Cynthia Keppel - Hampton University Proton Therapy Institute October 25, 2011 In 1946, physicist Robert Wilson first suggested that protons could be used as a form of radiation therapy in the treatment of cancer because of the sharp drop-off that occurs on the distal edge of the radiation dose. Research soon confirmed that high-energy protons were particularly suitable for treating tumors near critical structures, such as the heart and spinal column. The precision with which protons can be delivered means that more radiation can be deposited into the tumor while the surrounding healthy

367

Jefferson County, Pennsylvania: Energy Resources | Open Energy Information  

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°, -78.9288242° °, -78.9288242° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.147013,"lon":-78.9288242,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

368

Jefferson County, Tennessee: Energy Resources | Open Energy Information  

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°, -83.4643551° °, -83.4643551° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.0417825,"lon":-83.4643551,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

369

Jefferson Parish, Louisiana: Energy Resources | Open Energy Information  

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Parish, Louisiana: Energy Resources Parish, Louisiana: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 30.3911214°, -91.0634024° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.3911214,"lon":-91.0634024,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

370

Jefferson County, Missouri: Energy Resources | Open Energy Information  

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2310301°, -90.5257823° 2310301°, -90.5257823° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.2310301,"lon":-90.5257823,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

371

Jefferson County, Washington: Energy Resources | Open Energy Information  

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°, -123.3040062° °, -123.3040062° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":47.7424541,"lon":-123.3040062,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

372

Jefferson Lab Science Series - Science Series Video Archive  

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Science Series Video Archive Science Series Video Archive Couldn't make it to the last Science Series lecture? Did you like a lecture so much that you just had to see it again? Not to worry! Past lectures are now available on demand! The Higgs Boson and Our Life The Higgs Boson and Our Life On July 4th, 2012, the ATLAS and CMS experiments operating at the CERN Large Hadron Collider (LHC) announced the discovery of a new particle compatible with the Higgs boson (hunted for almost 50 years), which is a crucial piece for our understanding of fundamental physics and thus the structure and evolution of the universe. This lecture describes the unprecedented instruments and challenges that have allowed such an accomplishment, the meaning and relevance of this discovery to physics... April 30, 2013

373

West Jefferson, North Carolina: Energy Resources | Open Energy Information  

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364°, -81.4928829° 364°, -81.4928829° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.4037364,"lon":-81.4928829,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

374

Jefferson County, Iowa: Energy Resources | Open Energy Information  

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91.9099238° 91.9099238° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.0236358,"lon":-91.9099238,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

375

Jefferson County, Kansas: Energy Resources | Open Energy Information  

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5.3102505° 5.3102505° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.2827652,"lon":-95.3102505,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

376

Jefferson County, New York: Energy Resources | Open Energy Information  

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421°, -75.9927652° 421°, -75.9927652° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.0607421,"lon":-75.9927652,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

377

Jefferson County, Arkansas: Energy Resources | Open Energy Information  

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°, -91.9099238° °, -91.9099238° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.227351,"lon":-91.9099238,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

378

Jefferson County, Indiana: Energy Resources | Open Energy Information  

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1543°, -85.4788065° 1543°, -85.4788065° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.7751543,"lon":-85.4788065,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

379

Jefferson Lab Science Series - The Mysterious Universe: Exploring Our World  

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Einstein for Everyone Einstein for Everyone Previous Video (Einstein for Everyone) Science Series Video Archive Next Video (DNA: The Strand That Connects Us All) DNA: The Strand That Connects Us All The Mysterious Universe: Exploring Our World With Particle Accelerators Dr. James E. Brau - University of Oregon November 23, 2010 The universe is dark and mysterious, more so than even Einstein imagined. While modern science has established deep understanding of ordinary matter, unidentified elements ("Dark Matter" and "Dark Energy") dominate the structure of the universe, its behavior and its destiny. What are these curious elements? We are now working on answers to these and other challenging questions posed by the universe with experiments at particle accelerators on Earth. Results of this research may revolutionize our view

380

Jefferson Lab Science Series - Living and Working in the Freezer  

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Volcanoes in Virginia! Volcanoes in Virginia! Previous Video (Volcanoes in Virginia!) Science Series Video Archive Next Video (You Already Know This Physics!) You Already Know This Physics! Living and Working in the Freezer Dr. Victoria Hill - Old Dominion University, Bio-Optics Group February 7, 2012 Very little data of any kind exists from the early spring in the Arctic. The reason? It's extremely cold and that makes it difficult to survive, let alone conduct science. From March through the end of April, 2011, scientists from around the world braved temperatures of -48°C in the high Canadian Arctic in the name of science. At the Catlin Arctic Survey's floating 'Ice Base' off Ellef Ringnes Island, Dr. Victoria Hill was investigating how organic material in fresh water near the surface of the

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381

Jefferson County, Montana: Energy Resources | Open Energy Information  

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3°, -112.0752952° 3°, -112.0752952° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":46.1450553,"lon":-112.0752952,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

382

Jefferson County, Kentucky: Energy Resources | Open Energy Information  

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097°, -85.643487° 097°, -85.643487° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.1938097,"lon":-85.643487,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

383

Jefferson County, West Virginia: Energy Resources | Open Energy Information  

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1°, -77.8824596° 1°, -77.8824596° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.3059841,"lon":-77.8824596,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

384

Undergraduate Research at Jefferson Lab - Non-linear Multidimensional  

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Contamination Levels Contamination Levels Previous Project (Contamination Levels) Undergraduate Research Main Index Next Project (Data Acquisition Components) Data Acquisition Components Non-linear Multidimensional Optimization for use in Wire Scanner Fitting Student: Alyssa Henderson School: University of Virginia Mentored By: Alicia Hofler and Balša Terzić To ensure experiment efficiency and quality from the Continuous Electron Beam Accelerator, beam energy, size, and position must be measured. Wire scanners are inserted into the beamline to produce measurements which can obtain beam properties. Extracting physical information from wire scanner measurements begins by fitting Gaussian curves to the data. This study focuses on optimizing and automating this curve-fitting procedure. We use a

385

Jefferson Lab Science Series - The Higgs Boson and Our Life  

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Guesstimating the Environment Guesstimating the Environment Previous Video (Guesstimating the Environment) Science Series Video Archive Next Video (The Ultimate Speed) The Ultimate Speed The Higgs Boson and Our Life Dr. Fabiola Gianotti - European Organization for Nuclear Research (CERN) April 30, 2013 On July 4th, 2012, the ATLAS and CMS experiments operating at the CERN Large Hadron Collider (LHC) announced the discovery of a new particle compatible with the Higgs boson (hunted for almost 50 years), which is a crucial piece for our understanding of fundamental physics and thus the structure and evolution of the universe. This lecture describes the unprecedented instruments and challenges that have allowed such an accomplishment, the meaning and relevance of this discovery to physics, and

386

Port Jefferson, New York: Energy Resources | Open Energy Information  

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464875°, -73.0692732° 464875°, -73.0692732° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.9464875,"lon":-73.0692732,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

387

Port Jefferson Station, New York: Energy Resources | Open Energy  

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Station, New York: Energy Resources Station, New York: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 40.9253764°, -73.0473284° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.9253764,"lon":-73.0473284,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

388

Jefferson Lab Science Series - The Origin of the Elements  

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You Already Know This Physics! You Already Know This Physics! Previous Video (You Already Know This Physics!) Science Series Video Archive Next Video (Guesstimating the Environment) Guesstimating the Environment The Origin of the Elements Dr. Edward Murphy - University of Virginia, Department of Astronomy November 13, 2012 The world around us is made of atoms. Did you ever wonder where these atoms came from? How was the gold in our jewelry, the carbon in our bodies, and the iron in our cars made? In this lecture, we will trace the origin of a gold atom from the Big Bang to the present day, and beyond. You will learn how the elements were forged in the nuclear furnaces inside stars, and how, when they die, these massive stars spread the elements into space. You will learn about the origin of the building blocks of matter in the Big Bang,

389

Jefferson County, Nebraska: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

97.179026° 97.179026° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.1680732,"lon":-97.179026,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

390

Jefferson County, Wisconsin: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Wisconsin: Energy Resources Wisconsin: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 43.089927°, -88.7108964° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.089927,"lon":-88.7108964,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

391

Jefferson County, Oklahoma: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

7.87216° 7.87216° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":34.1672949,"lon":-97.87216,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

392

Jefferson County, Oregon: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

121.1785788° 121.1785788° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.6673324,"lon":-121.1785788,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

393

Jefferson County, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

8.864698° 8.864698° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.2267348,"lon":-88.864698,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

394

Jefferson, North Carolina: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

20403°, -81.4734376° 20403°, -81.4734376° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.420403,"lon":-81.4734376,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

395

Jefferson County, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

2°, -80.7657804° 2°, -80.7657804° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.3871722,"lon":-80.7657804,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

396

Jefferson County, Colorado: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

98°, -105.2662931° 98°, -105.2662931° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.5800298,"lon":-105.2662931,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

397

Jefferson Davis County, Mississippi: Energy Resources | Open Energy  

Open Energy Info (EERE)

281°, -89.8130356° 281°, -89.8130356° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":31.5825281,"lon":-89.8130356,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

398

Jefferson Davis Parish, Louisiana: Energy Resources | Open Energy  

Open Energy Info (EERE)

90.1500395° 90.1500395° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.9686923,"lon":-90.1500395,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

399

Jefferson County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

94.1513764° 94.1513764° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.8165398,"lon":-94.1513764,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

400

Jefferson Lab Science Series - Iceland: Dynamic Land of Ice and...  

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

Archive Next Video (The Physics of Baseball) The Physics of Baseball Iceland: Dynamic Land of Ice and Fire Dr. Richard S. Williams Jr. - U.S. Geological Survey February 8, 2002...

Note: This page contains sample records for the topic "newton orange jefferson" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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401

Jefferson Lab Science Series - Cloning: The Science Behind Jurassic...  

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

Subatomic Particles at CEBAF Previous Video (Finding Subatomic Particles at CEBAF) Science Series Video Archive Next Video (Pollution Sleuthing Using an Accelerator) Pollution...

402

Jefferson Lab Science Series - The Science and Technology Behind...  

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

Molecules are Everywhere Previous Video (Molecules are Everywhere) Science Series Video Archive Next Video (Iceland: Dynamic Land of Ice and Fire) Iceland: Dynamic Land of Ice and...

403

Bio-medical Applications of Jefferson Lab's Nuclear Physics ...  

Science Conference Proceedings (OSTI)

... contamination to crops Carbon sequestration Dual 15 cm x 20 cm Planar PET system ?3.03 mm step pixellated, 10 mm thick LGSO ...

2010-10-29T23:59:59.000Z

404

Jefferson Lab's Workbench Projects - The Ring Fling Machine ...  

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

iron core has been removed from the coil. The circuit starts at the hot side of the AC power line, passes through the fuse, then through the switch, then through the coil and...

405

Jefferson Lab Science Series - Detecting Einstein's Gravity Waves  

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Science Series Video Archive Next Video (Symmetry) Symmetry Detecting Einstein's Gravity Waves Dr. David Shoemaker - Massachusetts Institute of Technology March 18, 1997 LIGO...

406

Jefferson Lab Science Series - The Physics of Baseball  

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

Science Series Video Archive Next Video (Worlds Beyond the Matrix) Worlds Beyond the Matrix The Physics of Baseball Dr. Robert Adair - Yale University December 9, 2003 From...

407

Jefferson Lab Science Series - Chemistry - It's More Than Puffs...  

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

(Dinosaur Extinctions and Giant Asteroids) Dinosaur Extinctions and Giant Asteroids Chemistry - It's More Than Puffs and Bangs Dr. Joe Schwarcz - McGill Office for Chemistry and...

408

Generating Test Data from SOFL Specifications \\Lambda A. Jefferson Offutt  

E-Print Network (OSTI)

of Information Sciences Hiroshima City University Asaminami­ku, Hiroshima 731­31 Japan email: shaoying@cs.hiroshima

Offutt, Jeff

409

Jefferson Lab Science Series - A TACT-ful Chemical Musical  

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

Einstein's Biggest Blunder Previous Video (Einstein's Biggest Blunder) Science Series Video Archive Next Video (The Restoration of the USS Monitor) The Restoration of the USS...

410

Thomas Jefferson Site Office Categorical Exclusions | U.S. DOE...  

Office of Science (SC) Website

Safety & Health Organization Chart .pdf file (82KB) Phone Listing .pdf file (129KB) SC Categorical Exclusions and NEPA Documents SLI & SS Budget Contact Information Safety,...

411

HIGH INTENSITY LOW-ENERGY POSITRON SOURCE AT JEFFERSON  

SciTech Connect

We present a novel concept of a low-energy e{sup +} source with projected intensity on the order of 10{sup 10} slow e{sup +}/s. The key components of this concept are a continuous wave e{sup -} beam, a rotating positron-production target, a synchronized raster/anti-raster, a transport channel, and extraction of e{sup +} into a field-free area through a magnetic plug for moderation in a cryogenic solid. Components were designed in the framework of GEANT4-based (G4beamline) Monte Carlo simulation and TOSCA magnetic field calculation codes. Experimental data to demonstrate the effectiveness of the magnetic plug is presented.

Serkan Golge, Bogdan Wojtsekhowski, Branislav Vlahovic

2012-07-01T23:59:59.000Z

412

Jefferson Lab Science Series - What Is CEBAF All About?  

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

Science Series Video Archive Next Video (Where's the Beach?) Where's the Beach? What Is CEBAF All About? Dr. Beverly Hartline and Kathryn Strozak - CEBAF September 27, 1990 An...

413

Jefferson Lab Science Series - Magnets and Their Attractions...  

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

for the Teenager Magnets and Their Attractions for Technology Dr. Leigh Harwood - CEBAF December 11, 1991 How do scientists and engineers use magnets? What do magnets promise...

414

Jefferson Lab Science Series - Explore the World of Scientific...  

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

of Scientific Computing LIVE Dr. Roy Whitney, Ms. Rita Chambers and Dr. Chip Watson - CEBAF March 6, 1991 Simulations and demonstrations of the human interface for real-time data...

415

Jefferson Lab Science Series - Finding Subatomic Particles at...  

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

Jurassic Park) Cloning: The Science Behind Jurassic Park Finding Subatomic Particles at CEBAF Dr. Keith Baker - Hampton University and CEBAF November 16, 1993 How physicists detect...

416

Jefferson Lab Science Series - Neutrinos: Much Ado About (Almost...  

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

The Big Sting) Science Series Video Archive Next Video (Finding Subatomic Particles at CEBAF) Finding Subatomic Particles at CEBAF Neutrinos: Much Ado About (Almost) Nothing Dr....

417

Jefferson Lab Science Series - Mars Missions and the Search for...  

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

me?) Radiation: What is it and how can it affect me? Mars Missions and the Search for Life Dr. Robert Mitcheltree - NASA Langley Research Center February 15, 2000 How engineering...

418

The DVCS program in Hall A at Jefferson Lab  

Science Conference Proceedings (OSTI)

The DVCS Hall A/JLab experiments aim at providing data relevant to the '3-D structure of the nucleon' exploration by measuring precise absolute cross sections in the Deep Exclusive domain. Deeply Virtual Compton Scattering off the nucleon is the simplest process which is sensitive to the Generalized Parton Distribution functions. Currently, the DVCS in Hall A program is articulated in three steps. The first generation of experiments showed the power of precise measurement of absolute cross sections to test factorization of the DVCS amplitude. The second generation of experiments (data under analysis) will separate (at twist-2 order) all of the terms making up the unpolarized cross section. And the third generation of experiments (data to be taken with the 12 GeV beam at JLab) will provide measurements over an extended kinematic range. In this conference proceeding, the status of the DVCS in Hall A/JLab program is reviewed.

Julie Roche

2012-09-01T23:59:59.000Z

419

Jefferson Lab's Workbench Projects - Go Far Car Ramps - Component...  

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

(roughly 3 feet needed) 1 6 pine board (roughly 1 foot needed) 14" thick oak or poplar plywood (a section 4 feet long and 7 58" wide needed) 6 3 38" screw hook (2...

420

Jefferson Lab's Workbench Projects - Go Far Car Ramps - Overview  

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

spaced 5 centimeters apart. The ramp itself is made from a 4 foot long sheet of oak or poplar plywood. The smoothness of the plywood is the primary consideration when choosing a...

Note: This page contains sample records for the topic "newton orange jefferson" 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

Preliminary mode distortion measurements on the Jefferson Lab IRFEL  

SciTech Connect

We previously reported analytical calculations of mirror distortion in a high power FEL with a near-concentric cavity. Naive assumptions about the FEL power vs. distortion led us to believe that mirror losses were much lower than expected. Recently we have directly measured the mode size and beam quality as a function of power using a resonator with a center wavelength of 5 microns. The resonator mirrors were calcium fluoride. This material exhibits a large amount of distortion for a given power but, due to the negative slope of refractive index v temperature, adds almost no optical phase distortion on the laser output. The mode in the cavity can thus be directly calculated from the measurements at the resonator output. The presence of angular jitter produced results inconsistent with cold cavity expectations. Removing the effects of the angular jitter produces results in reasonable agreement with analytical models assuming mirror losses comparable to the original expectations.

Stephen V. Benson; Joe Gubeli; Michelle D. Shinn

2001-08-01T23:59:59.000Z

422

2010 DOE National Science Bowl Photos - Thomas Jefferson High...  

Office of Science (SC) Website

Facebook Facebook External link Share with Twitter Twitter External link Share with Google Bookkmarks Google Bookmarks External link Email a Friend Email link to: send 2010 DOE...

423

Jefferson Lab Science Series - Is Something Wrong With the Weatherman...  

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

LIVE Is Something Wrong With the Weatherman? Dr. Mike Kaplan - North Carolina State University January 22, 1991 What makes weather forecasting so hard? How can computers help?...

424

Jefferson Lab Science Series - Interactive Computer Games and...  

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

(Detecting Einstein's Gravity Waves) Detecting Einstein's Gravity Waves Interactive Computer Games and Animation Ms. Stephanie Barish - Shoah Foundation December 10, 1996...

425

Jefferson Lab Science Series - Multi-Million Dollar Forgeries...  

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

Comic Book Physics Previous Video (Comic Book Physics) Science Series Video Archive Next Video (Science Headlines from the 21st Century) Science Headlines from the 21st Century...

426

Jefferson Lab Science Series - Hidden Worlds - Hunting for Quarks...  

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

Extinctions and Giant Asteroids) Science Series Video Archive Next Video (Comic Book Physics) Comic Book Physics Hidden Worlds - Hunting for Quarks in Ordinary Matter Dr....

427

Very high power THz radiation at Jefferson Lab  

E-Print Network (OSTI)

AM Frequency (THz) JLab ERL NSLS Black Body Watts/cm 1E-4scientific program at the NSLS infrared beamline Nucl.The blackbody is at 2000K, the NSLS source is described in

Carr, G.L.; Martin, Michael C.; McKinney, Wayne R.; Jordan, K.; Neil, George R.; Williams, G.P.

2002-01-01T23:59:59.000Z

428

Jefferson Lab Science Series - Earth on Fire: The Environmental...  

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

Waste: You Can't Just Throw It Away Earth on Fire: The Environmental Impact of Global Burning Dr. Joel Levine - NASA Langely Research Center January 11, 1995 How human actions and...

429

Undergraduate Research at Jefferson Lab - Light Yield Measurements...  

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

Emission Characteristics) Field Emission Characteristics Light Yield Measurements of Heavy Photon Search (HPS) Muon Scintillator Hodoscopes Student: Marianne Skolnik School:...

430

Jefferson Lab's Workbench Projects - The Ring Fling Machine ...  

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

cord (18 AWG, 3 conductor) fuse holder (1" 14 " fuse, 20 amp capacity) 8 amp, 240 volt fast acting fuse (1 14" 14 ") 1 4 plank of white pine (roughly 4 feet needed)...

431

Jefferson Lab Science Series - Worlds Beyond the Matrix  

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

Video (The Physics of Baseball) Science Series Video Archive Next Video (The Physics of Stock Car Racing) The Physics of Stock Car Racing Worlds Beyond the Matrix Nigel Hey -...

432

Jefferson Lab Science Series - The Physics of Stock Car Racing...  

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

Archive Next Video (Understanding Flight) Understanding Flight The Physics of Stock Car Racing from a NASCAR Champion's Perspective Dr. Scott Winters - Lawrence Livermore...

433

Jefferson Lab's Workbench Projects - Go Far Car Ramps - Main...  

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

Go Far Car Ramps | Background | Overview | Component List | Ramp Construction | Support Arm Preparation | | Base Board Preparation | Top Board Preparation | Support Frame Assembly...

434

Jefferson Lab Science Series - The Restoration of the USS Monitor  

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

A TACT-ful Chemical Musical A TACT-ful Chemical Musical Previous Video (A TACT-ful Chemical Musical) Science Series Video Archive Next Video (Einstein for Everyone) Einstein for Everyone The Restoration of the USS Monitor David Krop - Conservation Project Manager, The Mariner's Museum March 2, 2010 The ongoing efforts to conserve and exhibit the iconic Civil War ironclad USS Monitor at The Mariners' Museum will be discussed. The presentation will cover past conservation accomplishments by conservators and NOAA specialists, current activities in the lab, and future plans to bring back to life one of the world's most famous warships. Learn about the complex methods and procedures used to treat the ship's revolving gun turret, steam engine, Dahlgren guns and carriages, as well as numerous small artifacts

435

Jefferson Lab Science Series - AIDS: The Science, The Impact  

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

Remote Control with Computers Previous Video (Remote Control with Computers) Science Series Video Archive Next Video (Exploring the Microwave Universe) Exploring the Microwave...

436

Jefferson Lab Science Series - Remote Control with Computers  

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

(AIDS: The Science, The Impact) AIDS: The Science, The Impact Remote Control with Computers Dr. Chip Watson - CEBAF March 14, 1995 Making hundreds of computers do your bidding...

437

Jefferson Lab Science Series - Strange Matters: Science Headlines...  

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

Lab Science Series | Current Lecture Schedule | Video Archive | Multi-Million Dollar Forgeries Exposed Previous Video (Multi-Million Dollar Forgeries Exposed) Science...

438

Jefferson County, Idaho: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

112.2493671° 112.2493671° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.7640903,"lon":-112.2493671,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

439

Jefferson County, Georgia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

82.4319405° 82.4319405° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.0740753,"lon":-82.4319405,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

440

Orange, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

7877944°, -117.8531119° 7877944°, -117.8531119° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.7877944,"lon":-117.8531119,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "newton orange jefferson" 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

Orange, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

758°, -81.4806744° 758°, -81.4806744° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.4497758,"lon":-81.4806744,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

442

Orange County - OCHEEP! (Florida) | Open Energy Information  

Open Energy Info (EERE)

CaulkingWeather-stripping, Ceiling Fan, Central Air conditioners, DuctAir sealing, Energy Mgmt. SystemsBuilding Controls, Heat pumps, Lighting, Programmable Thermostats,...

443

Trusted Computer System Evaluation Criteria ["Orange Book"  

Science Conference Proceedings (OSTI)

Page 1. DoD 5200.28-STD Supersedes CSC-STD-00l-83, dtd l5 Aug 83 Library No. S225,7ll DEPARTMENT OF DEFENSE STANDARD ...

2013-04-16T23:59:59.000Z

444

Orange and Rockland Utilities (Electric) - Residential Appliance...  

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

Recycling Program < Back Eligibility Residential Commercial Savings Category Appliances & Electronics Construction Commercial Heating & Cooling Program Info Funding Source...

445

Orange and Rockland Utilities (Electric) - Residential Efficiency...  

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

Program (New York) < Back Eligibility Commercial Residential Savings Category Appliances & Electronics Program Info State New York Program Type Utility Rebate Program Rebate...

446

THE XMM-NEWTON X-RAY SPECTRA OF THE MOST X-RAY LUMINOUS RADIO-QUIET ROSAT BRIGHT SURVEY-QSOs: A REFERENCE SAMPLE FOR THE INTERPRETATION OF HIGH-REDSHIFT QSO SPECTRA  

SciTech Connect

We present the broadband X-ray properties of four of the most X-ray luminous (L{sub X} {>=} 10{sup 45} erg s{sup -1} in the 0.5-2 keV band) radio-quiet QSOs found in the ROSAT Bright Survey. This uniform sample class, which explores the extreme end of the QSO luminosity function, exhibits surprisingly homogenous X-ray spectral properties: a soft excess with an extremely smooth shape containing no obvious discrete features, a hard power law above 2 keV, and a weak narrow/barely resolved Fe K{alpha} fluorescence line for the three high signal-to-noise ratio (S/N) spectra. The soft excess can be well fitted with only a soft power law. No signatures of warm or cold intrinsic absorbers are found. The Fe K{alpha} centroids and the line widths indicate emission from neutral Fe (E = 6.4 keV) originating from cold material from distances of only a few light days or further out. The well-constrained equivalent widths (EW) of the neutral Fe lines are higher than expected from the X-ray Baldwin effect which has been only poorly constrained at very high luminosities. Taking into account our individual EW measurements, we show that the X-ray Baldwin effect flattens above L{sub X} {approx} 10{sup 44} erg s{sup -1} (2-10 keV band) where an almost constant (EW) of {approx}100 eV is found. We confirm the assumption of having very similar X-ray active galactic nucleus properties when interpreting stacked X-ray spectra. Our stacked spectrum serves as a superb reference for the interpretation of low S/N spectra of radio-quiet QSOs with similar luminosities at higher redshifts routinely detected by XMM-Newton and Chandra surveys.

Krumpe, M.; Markowitz, A. [University of California, San Diego, Center for Astrophysics and Space Sciences, 9500 Gilman Drive, La Jolla, CA 92093-0424 (United States); Lamer, G. [Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam (Germany); Corral, A., E-mail: mkrumpe@ucsd.ed [INAF-Osservatorio Astronomico di Brera, via Brera 28, 20121 Milan (Italy)

2010-12-20T23:59:59.000Z

447

Newton, Alabama: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

°, -85.6052133° °, -85.6052133° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":31.3351716,"lon":-85.6052133,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

448

Newton, Massachusetts: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.3370413°, -71.2092214° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":42.3370413,"lon":-71.2092214,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

449

NEWTON's Environmental and Earth Science References  

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

Environmental and Earth Science References Environmental and Earth Science References Do you have a great reference link? Please click our Ideas page. Featured Reference Links: >NASA's Earth Science Division NASA's Earth Science Division Find the answers to the big questions of Earth Science such as "How is the World Changing?" The information and articles are provided by NASA's Earth Science Division Geology.com Resources Teaching Earth Science - Geology.com Geology.com provides news and information about Geology and Earth Science. It has a teacher resource section as well, which provides a collection of classroom activities and lesson plans, for earth science in the classroom. IRIS's Seismographs in Schools Program IRIS's Seismographs in Schools Program Discover tools to share seismic data in real-time, classroom activities, and technical support documents for seismic instruments.

450

NEWTON: Greenhouse Gas and Heat Transfer  

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

Greenhouse Gas and Heat Transfer Greenhouse Gas and Heat Transfer Name: Robert Status: teacher Grade: 9-12 Location: AK Country: USA Date: Summer 2013 Question: It would appear from a superficial reading that heat flows out of a greenhouse gas more slowly than heat flows into the same gas. This has to be an incorrect interpretation. It seems more likely that molecules with high heat capacities resist heat transfer-both into and out of such a molecular system. At a molecular level how does heat move out of a hot greenhouse gas? I have seen plots of Cv vs Tempt which indicates that heat moves from translational modes of motion-into rotational modes and finally into modes of vibration. The energy spacing of vibrations is generally grater that rotation which are greater than translation. Could it be that it is this quantization of the energy levels and the difference in energy between such quantum states that is the source of the resistance to heat flow or transfer?

451

NEWTON, TEACHERS, Classroom and Curriculum Development  

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

http:www.pisymphony.comtoothpicktoothpick1.htm http:www.yale.eduynhticurriculumunits2001501.05.04.x.html http:www.garrettsbridges.com http:...

452

NEWTON, TEACHERS, Classroom and Curriculum Development  

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

Argonne Science Fair Ideas The best ideas for science projects are learning about and investigating something in science that interests you. These Science Fair Help sites are...

453

NEWTON, TEACHERS, Classroom and Curriculum Development  

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

and Functions Listing of parts Arm and Base Body Tube Stage Clips Iris and Light Condenser Coarse Adjustment Knob Fine Adjustment Knob Rotating Head Light Source Mechanical...

454

Smith Newton Vehicle Performance Evaluation (Brochure)  

DOE Green Energy (OSTI)

The Fleet Test and Evaluation Team at the U.S. Department of Energy's National Renewable Energy Laboratory is evaluating and documenting the performance of electric and plug-in hybrid electric drive systems in medium-duty trucks across the nation. Through this project, Smith Electric Vehicles will build and deploy 500 all-electric medium-duty trucks. The trucks will be deployed in diverse climates across the country.

Not Available

2012-08-01T23:59:59.000Z

455

QUASI-NEWTON METHODS ON GRASSMANNIANS AND ...  

E-Print Network (OSTI)

machine learning [44, 41], neuroscience [45], quantum chemistry [35], signal processing. [10, 13 .... geodesic curves and transport of vectors on Grassmannians.

456

Updated 5-13 Garry R. Newton  

E-Print Network (OSTI)

specialized tools and procedures to assess weapons system effectiveness and efficiencies in both/military personnel located in headquarters, Naval Air Warfare Center Aircraft/Weapons Divisions, and Fleet Readiness,000 civilian and military personnel across 27 operational sites, with an annual budget of $5 billion. Mr

457

NEWTON's Environmental and Earth Science Archive  

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

Dissolving Rocks Eye of Hurricane Time Limit on Earthquake Aftershocks Oxygen in Underwater Cave Limnic Eruptions Extraterrestrial Plate Tectonics Earth's Core Hottest Layer...

458

A quasi-Newton proximal splitting method  

E-Print Network (OSTI)

Jun 20, 2012 ... common trend in modern science is the increase in size of datasets, which ..... complexity O(N log N) by simple sorting the absolute values.

459

Marshall Library of Economics Newton Library  

E-Print Network (OSTI)

holdings you want to search. 3. Basic Search 3.1 Basic Search Screen Insert search term(s) Select the type of search you want to use ­ in this example, a Boolean search has been selected and the search terms joined.g. by limiting your search to a specific library. #12;3.2 Types of basic search Do not enter words such as the

Talbot, James P.

460

NEWTON: Bacteria Survival in the Stomach  

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

Bacteria Survival in the Stomach Bacteria Survival in the Stomach Name: Lianne Status: other Grade: other Location: Outside U.S. Country: USA Date: Summer 2013 Question: Is H. Pylorii the only bacteria able to survive the acidic condition of the stomach, or are there others? Replies: Hi Lianne, Thanks for the question. Yes, other bacteria are able to survive the acidic conditions in the stomach. For instance, the bacteria that are present in acidopholus yougurt (and milk) are able to survive the stomach's acid and to repopulate the large intestine. These acidopholus bacteria are "good" bacteria and are useful in restoring bacterial colonies in the large intestine after a treatment of antibiotics. I hope this helps. Please let me know if you have more questions. Thanks Jeff I don't know, but I would be very surprised given the number of bacterial species, that H. Pylori is uniquely adapted to low pH environments.

Note: This page contains sample records for the topic "newton orange jefferson" 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

Complete genome sequence of the orange-red pigmented, radioresistant Deinococcus proteolyticus type strain (MRPT)  

SciTech Connect

Deinococcus proteolyticus (ex Kobatake et al. 1973) Brook and Murray 1981 is one of currently 47 species in the genus Deinococcus within the family Deinococcaceae. Strain MRPTT was isolated from faeces of Lama glama; it shares with various other species of the genus the extreme radiation resistance, with D. proteolyticus being resistant up to 1.5 Mrad of gamma radiation. Strain MRPT{sup T} is of further interest for its carotenoid pigment. The genome presented here is only the fifth completed genome sequence of a member of the genus Deinococcus (and the forth type strain) to be published, and will hopefully contribute to a better understanding of how members of this genus adapted to high gamma- or UV ionizing-radiation. Here we describe the features of this organism, together with the complete genome sequence and annotation. The 2,886,836 bp long genome with its four large plasmids of 97 kbp, 132 kbp, 196 kbp and 315 kbp harbours 2,741 protein-coding and 58 RNA genes and is a part of the Genomic Encyclopedia of Bacteria and Archaea project.

Copeland, A [U.S. Department of Energy, Joint Genome Institute; Zeytun, Ahmet [Los Alamos National Laboratory (LANL); Yasawong, Montri [HZI - Helmholtz Centre for Infection Research, Braunschweig, Germany; Nolan, Matt [U.S. Department of Energy, Joint Genome Institute; Lucas, Susan [U.S. Department of Energy, Joint Genome Institute; Hammon, Nancy [U.S. Department of Energy, Joint Genome Institute; Deshpande, Shweta [U.S. Department of Energy, Joint Genome Institute; Cheng, Jan-Fang [U.S. Department of Energy, Joint Genome Institute; Han, Cliff [Los Alamos National Laboratory (LANL); Tapia, Roxanne [Los Alamos National Laboratory (LANL); Goodwin, Lynne A. [Los Alamos National Laboratory (LANL); Pitluck, Sam [U.S. Department of Energy, Joint Genome Institute; Mavromatis, K [U.S. Department of Energy, Joint Genome Institute; Liolios, Konstantinos [U.S. Department of Energy, Joint Genome Institute; Pagani, Ioanna [U.S. Department of Energy, Joint Genome Institute; Ivanova, N [U.S. Department of Energy, Joint Genome Institute; Mikhailova, Natalia [U.S. Department of Energy, Joint Genome Institute; Pati, Amrita [U.S. Department of Energy, Joint Genome Institute; Chen, Amy [U.S. Department of Energy, Joint Genome Institute; Palaniappan, Krishna [U.S. Department of Energy, Joint Genome Institute; Land, Miriam L [ORNL; Hauser, Loren John [ORNL; Jeffries, Cynthia [Oak Ridge National Laboratory (ORNL); Brambilla, Evelyne-Marie [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Rohde, Manfred [HZI - Helmholtz Centre for Infection Research, Braunschweig, Germany; Sikorski, Johannes [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Pukall, Rudiger [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Goker, Markus [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Detter, J. Chris [U.S. Department of Energy, Joint Genome Institute; Woyke, Tanja [U.S. Department of Energy, Joint Genome Institute; Bristow, James [U.S. Department of Energy, Joint Genome Institute; Eisen, Jonathan [U.S. Department of Energy, Joint Genome Institute; Markowitz, Victor [U.S. Department of Energy, Joint Genome Institute; Hugenholtz, Philip [U.S. Department of Energy, Joint Genome Institute; Kyrpides, Nikos C [U.S. Department of Energy, Joint Genome Institute; Klenk, Hans-Peter [DSMZ - German Collection of Microorganisms and Cell Cultures GmbH, Braunschweig, Germany; Lapidus, Alla L. [U.S. Department of Energy, Joint Genome Institute

2012-01-01T23:59:59.000Z

462

Inexact Newton Methods, Newton-Krylov Methods, Extensions for Large-Scale Underdetermined Systems  

E-Print Network (OSTI)

(u) - F(u + s) pred F(u) - F(u) + F (u)s (actual reduction) ("predicted" reduction) Update a la Dennis on the first reduction, a cubic on subsequent reductions. IN/NK Methods & Extensions Oak Ridge National NOX nonlinear solver suite, with GMRES and domain-based (overlapping Schwarz) ILU preconditioners from

463

Frostbite Theater - Liquid Nitrogen Experiments - Shattering...  

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

Science Education Jefferson Lab Jefferson Lab Home Search Jefferson Lab Contact Jefferson Lab Science Education Home Teacher Resources Student Zone Games and Puzzles Science Cinema...

464

West Orange, New Jersey: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

987113°, -74.2390353° 987113°, -74.2390353° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.7987113,"lon":-74.2390353,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

465

Orange County, Indiana: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

4°, -86.4996546° 4°, -86.4996546° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.5169004,"lon":-86.4996546,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

466

Orange County, New York: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

3°, -74.3118212° 3°, -74.3118212° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.3911653,"lon":-74.3118212,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

467

Orange Cove, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

624394°, -119.3137301° 624394°, -119.3137301° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.624394,"lon":-119.3137301,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

468

Orange County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

033°, -93.8655303° 033°, -93.8655303° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":30.1484033,"lon":-93.8655303,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

469

Orange, New Hampshire: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

6545168°, -71.9714725° 6545168°, -71.9714725° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.6545168,"lon":-71.9714725,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

470

Orange County, Vermont: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

4186°, -72.4003713° 4186°, -72.4003713° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":44.0014186,"lon":-72.4003713,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

471

Orange County, Virginia: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

4°, -77.973865° 4°, -77.973865° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":38.2426674,"lon":-77.973865,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

472

Orange, New Jersey: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

706562°, -74.2326463° 706562°, -74.2326463° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.7706562,"lon":-74.2326463,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

473

Orange County, North Carolina: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

2°, -79.1096901° 2°, -79.1096901° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.0263022,"lon":-79.1096901,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

474

Orange County, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

County, California: Energy Resources County, California: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 33.7174708°, -117.8311428° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.7174708,"lon":-117.8311428,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

475

ESnet, Orange Silicon Valley, and Bay Microsystems Demonstrate...  

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

Microsystems Demonstrate the World's First Long Distance 40Gbps RDMA Data Transfer Public-Private Collaborative Demo Leveraged New ESnet Advanced Networking Initiative (ANI)...

476

Adsorptive Removal of Arsenic and Fluoride by Using Orange Juice ...  

Science Conference Proceedings (OSTI)

Aug 1, 2003 ... TMS Member price: 10.00. Non-member price: 25.00. TMS Student Member price : 10.00. Product In Stock. Description Industrial application of...

477

Orange County - Solar Hot Water Rebate Program (Florida) | Open...  

Open Energy Info (EERE)

Clean Energy Analysis Low Emission Development Strategies Oil & Gas Smart Grid Solar U.S. OpenLabs Utilities Water Wind Page Actions View form View source History View New...

478

The France Telecom Orange Labs (Beijing) Video Semantic ...  

Science Conference Proceedings (OSTI)

... Index Terms TRECVID, INS, Vocabulary Tree, Ap- proximate K-Means ... the highest low-level similarities and enter- s the interactive search loop ...

2012-11-29T23:59:59.000Z

479

Orange County, Florida: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

28.4844995°, -81.2518833° 28.4844995°, -81.2518833° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":28.4844995,"lon":-81.2518833,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

480

Kelp Wrack: Hopping with Life in Orange County  

E-Print Network (OSTI)

of mechanically removing it from sandy beaches. Results fromecology and sustainability of sandy beaches, many of whichthe animal species living on sandy beaches depend on wrack.

Dugan, Jenifer E.

2011-01-01T23:59:59.000Z

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


481

Undergraduate Research at Jefferson Lab - LabVIEW Software Based Program to  

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Data Acquisition Components Data Acquisition Components Previous Project (Data Acquisition Components) Undergraduate Research Main Index Next Project (Spin-Polarization of Helium-3 Target Cell) Spin-Polarization of Helium-3 Target Cell LabVIEW Software Based Program to Minimize Data File Size of the Slow Controls System (SCS) of the Silicon Vertex Tracker (SVT) Student: Zulqarnain M Jamal School: Georgia Institute of Technology Mentored By: Amrit Yegneswaran SVT is a detector, made of silicon modules. It tracks charged particles and helps to determine interaction vertices. SCS controls and monitors currents and voltages, and monitors temperatures and humidity. SCS produces large data files. Smart Logger, a LabVIEW program, has been developed in to minimize data file size. Smart Logger discards data-sets if any the

482

Undergraduate Research at Jefferson Lab - Designing a Multi-Purpose Dark  

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Noise Correlation Noise Correlation Previous Project (Noise Correlation) Undergraduate Research Main Index Next Project (Proton-Deuteron Drell-Yan Reaction) Proton-Deuteron Drell-Yan Reaction Designing a Multi-Purpose Dark Box Optimized for PMT Uniformity Testing Student: Nicholas M. Dowdle School: Emory & Henry College at Emory Mentored By: Jack McKisson This paper describes the process of designing a means for measuring the response uniformity for position-sensitive photomultiplier tubes (PSPMTs), a trait which, in the ideal case, suggests identical responses for every pixel on the face of a PSPMT in a field of uniform light. However, significant non-uniformities arise in the practical usage of PSPMTs, necessitating some form of compensation before or after experimentation. A

483

OPTIMIZING CENTRIFUGAL BARREL POLISHING FOR MIRROR FINISH SRF CAVITY AND RF TESTS AT JEFFERSON LAB  

SciTech Connect

We performed Centrifugal Barrel Polishing (CBP) on a 1.3 GHz fine grain TESLA single cell cavity and 1.5 GHz fine grain CEBAF high gradient superconducting radio frequency (SRF) single cell cavity following a modified recipe originally developed at Fermi National Accelerator Lab (FNAL). We were able to obtain a mirror like surface similar to that obtained at FNAL, while reducing the number of CBP steps and total processing time. This paper will discuss the change in surface and subsequent cavity performance post CBP, after a 800 C bake (no pre-bake chemistry) and minimal controlled electro-polishing (10 micron). In addition to Q vs. E{sub ACC} thermometry mapping with preheating characteristics and optical inspection of the cavity after CBP will also be shown.

Ari Palczewski, Rongli Geng, Hui Tian

2012-07-01T23:59:59.000Z

484

LEIC - A Polarized Low Energy Electron-ion Collider at Jefferson Lab  

Science Conference Proceedings (OSTI)

A polarized electron-ion collider is envisioned as the future nuclear science program at JLab beyond the 12 GeV CEBAF. Presently, a medium energy collider (MEIC) is set as an immediate goal with options for a future energy upgrade. A comprehensive design report for MEIC has been released recently. The MEIC facility could also accommodate electron and proton/ion collisions in a low CM energy range, covering proton energies from 10 to 25 GeV and ion energies with a similar magnetic rigidity, for additional science reach. In this paper, we present a conceptual design of this low energy collider, LEIC, showing its luminosity can reach above 10{sup 33} cm{sup -2}s{sup -1}. The design specifies that the large booster of the MEIC is converted to a low energy ion collider ring with an interaction region and an electron cooler integrated into it. The design provides options for either sharing the detector with the MEIC or a dedicated low energy detector in a third collision point, with advantages of either a minimum cost or extra detection parallel to the MEIC operation, respectively. The LEIC could be positioned as the first and low cost phase of a multi-stage approach to realize the full MEIC.

Derbenev, Yaroslav S. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Hutton, Andrew M. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Krafft, Geoffrey A. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Li, Rui [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Lin, Fanglei [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Morozov, Vasiliy [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Nissen, Edward W. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Yunn, Byung C. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Zhang, He [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Sullivan, Michael K. [SLAC National Accelerator Laboratory, Menlo Park, CA (United States); Zhang, Yuhong [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States)

2013-06-01T23:59:59.000Z

485

JLIFE: THE JEFFERSON LAB INTERACTIVE FRONT END FOR THE OPTICAL PROPAGATION CODE  

SciTech Connect

We present details on a graphical interface for the open source software program Optical Propagation Code, or OPC. This interface, written in Java, allows a user with no knowledge of OPC to create an optical system, with lenses, mirrors, apertures, etc. and the appropriate drifts between them. The Java code creates the appropriate Perl script that serves as the input for OPC. The mode profile is then output at each optical element. The display can be either an intensity profile along the x axis, or as an isometric 3D plot which can be tilted and rotated. These profiles can be saved. Examples of the input and output will be presented.

Watson, Anne M. [JLAB; Shinn, Michelle D. [JLAB

2013-08-01T23:59:59.000Z

486

Executive Summary The Eastern Panhandle (Berkeley, Jefferson, and Morgan counties) has been among the fastest  

E-Print Network (OSTI)

distance from Pittsburgh, PA, Cleveland, OH, Washington DC, and New York City. Within the state Orchestra, and conducted the University Choir in the Kennedy Center in Washington, D.C. During the last Graduate Reid Hartman at the Smithsonian Folklife Festival in Washington, DC 8 school of music | college

Mohaghegh, Shahab

487

Design and implementation of a slow orbit control package at Thomas Jefferson National Accelerator Facility  

SciTech Connect

The authors describe the design and implementation of a C++ client/server based slow orbit and energy control package based on the CDEV software control bus. Several client applications are described and operational experience is given.

Zeijts, J. van; Witherspoon, S.; Watson, W.A.

1997-06-01T23:59:59.000Z

488

High School Research at Jefferson Lab - 3D Model Creation for...  

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

these parts look simple, adding these essential pieces was an arduous task requiring human precision, error diagnostics, and critical thinking. It was no small feat creating...

489

Multipass Beam Breakup Study at Jefferson Lab for the 12 GeV CEBAF Upgrade.  

E-Print Network (OSTI)

?? Recirculating linear accelerators (linacs) provide a compact and efficient way of accelerating particle beams to medium and high energies by reusing the same linac (more)

SHIN, ILKYOUNG

2013-01-01T23:59:59.000Z

490

Jefferson Lab Science Series - Waste: You Can't Just Throw It...  

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

Environmental Impact of Global Burning Previous Video (Environmental Impact of Global Burning) Science Series Video Archive Next Video (Remote Control with Computers) Remote...

491

Results of Cavity Series Fabrication at Jefferson Laboratory for the Cryomodule R100  

SciTech Connect

A series production of eight superconducting RF cavities for the cryomodule R100 was conducted at JLab in 2010. The cavities underwent chemical post-processing prior to vertical high power testing and routinely exceeded the envisaged performance specifications. After cryomodule assembly, cavities were successfully high power acceptance tested. In this paper, we present the achievements paving the way for the first demonstration of 100 MV (and beyond) in a single cryomodule to be operated at CEBAF.

F. Marhauser, W.A. Clemens, M.A. Drury, D. Forehand, J. Henry, S. Manning, R.B. Overton, R.S. Williams

2011-09-01T23:59:59.000Z

492

High-Resolution Search for Pentaquark Partners in Hall A at Jefferson Lab  

DOE Green Energy (OSTI)

We have carried out a high-resolution search ({sigma} = 1.5 MeV) for narrow exotic resonances ({Gamma} < 10 MeV) in the mass range M {approx} 1500-1850 MeV in ep {yields} e'K{sup +}X, ep {yields} e'K{sup -}X and ep {yields} e'{pi}{sup +}X electroproduction at forward angles ({theta}{sup CM} {approx} 6-7 degrees). Such narrow resonances would be candidates for partner states of the speculative {Theta}{sup +}(1540) pentaquark. The experiment employed a 5 GeV CW electron beam incident on a liquid hydrogen target and two high-resolution magnetic spectrometers covering a total center-of-mass solid angle of {Delta}{Omega} {approx} 30-40 msr. We do not observe a statistically significant signal in any of the three reaction channels. Upper limits on the production cross sections were determined to be between 3 and 16 nb/sr, depending on the channel and the assumed width of the state. In addition, precise electroproduction data of the {Lambda}(1116), {Sigma}(1193) and {Lambda}(1520) resonances were obtained for calibration purposes.

Jens-ole Hansen

2005-08-26T23:59:59.000Z

493

Data acquisition system of Moeller polarimeter Hall A Jefferson Lab (in Russian)  

SciTech Connect

The structure, parameters and test results of a new data acquisition system for Moller polarimeter based on flash-ADC are presented. Flash-ADC is electronic module in VME format that consists of high-speed multichannel ADC piped type and FPGA unit on board. The use of flash-ADC has a lot of advantages: reduce of cable interconnections, events registration with higher rate, considerable decreases of system deadtime and, as result, the accuracy of polarization measurements is increases.

Roman Pomatsalyuk

2012-11-01T23:59:59.000Z

494

High School Research at Jefferson Lab - Development of the GRINCH Gas  

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

Nonlinear Particle Dynamics Nonlinear Particle Dynamics Previous Project (Nonlinear Particle Dynamics) High School Research Main Index Next Project (Fire Alarm Monitoring Systems) Fire Alarm Monitoring Systems Development of the GRINCH Gas Cherenkov Detector This project was done as a summation of all of the projects I have done referencing A1n and the GRINCH detector. To assist in the preparation of the A1n experiment, I helped develop and model a magnetic shielding box for an array of PMT's in the GRINCH detector. Using this box, as well as a compensation coil, seemed to provide ample shielding from the BigBite magnets magnetic field. The PMT's in the array were salvaged from a detector where they were submerged in water and sustained damage (micro-fractures) on their acceptance windows. By putting a layer of glue

495

Jefferson Lab Science Series - DNA: The Strand That Connects Us All  

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The Mysterious Universe The Mysterious Universe Previous Video (The Mysterious Universe) Science Series Video Archive Next Video (The Science of Chocolate) The Science of Chocolate DNA: The Strand That Connects Us All Dr. Matt Kaplan - University of Arizona Genetics Core March 29, 2011 Learn how the methods and discoveries of human population genetics are applied for personal genealogical reconstruction and anthropological testing. We will start with a short general review of human genetics and the biology behind this form of DNA testing. We will look at how DNA testing is performed and how samples are processed in our laboratory. We will also examine examples of personal genealogical results from Family Tree DNA and personal anthropological results from the Genographic Project. Finally, I will describe the newest project in our laboratory, the DNA

496

Questions and Answers - Can you explain why the United States uses  

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did Thomas Jeffersondo as a scientist? did Thomas Jefferson<br>do as a scientist? Previous Question (What did Thomas Jefferson do as a scientist?) Questions and Answers Main Index Next Question (How long would it take a person on a bicycle-type generator to create an atom?) How long would it take a person on abicycle-type generator to create an atom? Can you explain why the United States uses Fahrenheit instead of Celsius? Answer 1 The answer to the your question is in Sir Isaac Newton's first law of motion, which is more commonly known as inertia. That is, that when something gets going it is hard to stop it or change its direction. It would be a really good thing if we just bit the bullet and made the change to the metric system or, more properly, to International Units. Even NASA

497

NEWTON, Ask a Scientist at Argonne National Labs  

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

Current Oil Formation Current Oil Formation Name: Jerry Status: n/a Grade: other Country: USA Date: Winter 2011-2012 Question: Is oil still being formed in an ongoing fashion by geologic and physical processes just as it was millions of years ago? Replies: Jerry, The process of converting organic detritus into oil only requires that the organic material (dead plants, animals, etc) undergo decomposition in an oxygen poor environment. Long chain hydrocarbons are formed in this way. So in places where there is a lot of organic material buried under rock or below the pinocline of some body of water (a depth and temperature of water where little roiling happens and hence oxygen does not appreciably mix in), then the conversion of organic material into oil should be happening. This might lead you to wonder why are we concerned that fossil fuel is being depleted - and this goes to how much oil is being extracted and used, versus how much oil is being produced by the natural process.

498

NEWTON, Ask a Scientist at Argonne National Labs  

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

Radioactive Decay Products Radioactive Decay Products Name: Mary Status: educator Location: IL Country: USA Date: Spring 2012 Question: What happens to a radioactive isotope when it decays? Does the radioactive material disappear? How or why? Replies: Mary http://en.wikipedia.org/wiki/Isotope "Isotopes are variants of a particular chemical element. While all isotopes of a given element share the same number of protons, each isotope differs from the others in its number of neutrons." So if an isotope decays it simply becomes a different chemical element or the same element of a different atomic weight. http://en.wikipedia.org/wiki/Radioactive_decay Per the above Wikipedia article Uranium Atomic Wt: 238 loses an alpha particle to become Thorium 234 Thorium 234 loses a beta particle to become Protactinium 234 which loses another beta particle to become Uranium 234....and on and on and on.

499

NEWTON, Ask a Scientist at Argonne National Labs  

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

Aquatic Plans vs Land Plants and Nutrients Aquatic Plans vs Land Plants and Nutrients Name: Maaz Status: educator Grade: other Location: Outside U.S. Country: India Date: Summer 2011 Question: My students have many question about plants growth. Many plant need soil to grow and make food. What kind of soil need in aquatic plants to grow or this normal soil is used for the aquatic plant? Replies: Dear Maaz, You may recall the famous experiment by Jan Baptist van Helmont where he grew a tree in a large pot with a weighed amount of soil for five years and determined that the bulk dry weight of the tree did not come from the soil but rather from the carbon dioxide drawn from the air (with water contributing to the fresh weight). The experiment demonstrates that the soil is most critical for supplying physical support and trace minerals. In an aquatic environment, the trace minerals are found primarily in the water so the soil largely serves as a means to anchor the aquatic plant and keep it from drifting.

500

NEWTON, Ask a Scientist at Argonne National Labs  

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

Asteroids, Charge, and Magnetic Fields Asteroids, Charge, and Magnetic Fields Name: Daniel Status: student Grade: 12 Location: MD Country: USA Date: Spring 2012 Question: If a fragment from an asteroid falls to Earth and a static electric charge is built up in the fragment as it falls, does it generate a magnetic field? If so, why? Replies: Yes, it would. A moving electric charge creates a magnetic field. The "why" basically comes from relativity. When the charge moves, its electrical interaction with other charged objects changes because of the way spacetime distorts. That change manifests as a magnetic field. Richard E. Barrans Jr., Ph.D., M.Ed. Department of Physics and Astronomy University of Wyoming Daniel, Current is the motion of electric charge from one location to another. Current, as we usually think of it, is the movement of electrons within a wire, and this current will create a magnetic field surrounding the wire. Maxwell's equations define the strength of this field based on the value of this current (amount of charge flowing through the wire each second). Current is not confined to wires, however; electrons flowing in space will define a current (and associated magnetic field) as well. For a charged asteroid, you can define current associated with its charge moving through space and an associated magnetic field.