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1

Presentations & Testimony  

Office of Science (SC) Website

presentations-and-testimony/ The Office of presentations-and-testimony/ The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of national importance. It oversees - and is the principal federal funding agency of - the Nation's research programs in high-energy physics, nuclear physics, and fusion energy sciences. en {C6485D5D-3C27-4B21-961B-5075074695E9}http://science.energy.gov/~/media/sc-1/pdf/2013/103013_dehmer_csst.pdf Statement of the Acting Director of the Office of Science, Patricia Dehmer to the House Science, Space and Technology Committee Subcommittee on Energy The Office of Science's Role in Providing Tools for Scientific Discovery and Basic Energy Research. Wed, 30 Oct 2013 00:00:00 -0400

2

Presentations & Testimony | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Presentations & Testimony Presentations & Testimony News Featured Articles Science Headlines Presentations & Testimony 2013 2012 2011 2010 2009 2008 News Archives Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Presentations & Testimony Print Text Size: A A A Subscribe FeedbackShare Page Below are Presentations & Testimony for the Director of the Office of Science. Additional Presentations & Testimony can be found here. 10.30.13Presentations & Testimony Statement of the Acting Director of the Office of Science, Patricia Dehmer to the House Science, Space and Technology Committee Subcommittee on Energy .pdf file (132KB) The Office of Science's Role in Providing Tools for Scientific Discovery

3

Presentations & Testimony | U.S. DOE Office of Science (SC)  

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

Presentations & Testimony Presentations & Testimony Deputy Director for Science Programs Deputy Director Home Mission & Functions Deputy Director Biography Organization Staff Presentations & Testimony Federal Advisory Committees Committees of Visitors Contact Information Deputy Director for Science Programs U.S. Department of Energy SC-2/Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 F: (202) 586-4120 E: sc.science@science.doe.gov U.S. Department of Energy SC-2/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-5316 F: (301) 903-7780 E: sc.science@science.doe.gov Presentations & Testimony Print Text Size: A A A RSS Feeds FeedbackShare Page Office of Science Overview 2-pager .pdf file (10.8MB) Office of Science 2-page Fact Sheet .pdf file (10.8MB)

4

EERE Testimonials  

Office of Energy Efficiency and Renewable Energy (EERE)

These video testimonials capture what a variety of CEOs and business leaders have to say about the difference the Office of Energy Efficiency and Renewable Energy (EERE) is making in the clean energy economy.

5

Special Presentation: Key Findings from the Barrier Immune Radio  

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

Special Presentation: Key Findings from the Barrier Immune Radio Special Presentation: Key Findings from the Barrier Immune Radio Communications Project Speaker(s): Francis Rubinstein Girish Ghatikar Peter Haugen Date: November 29, 2007 - 12:00pm Location: 90-3122 The Barrier Immune Radio Communications (BIRC) Project was established in January 2007 by the Demand Response Emerging Technologies Program (DRETD) to identify radio frequency technologies that could enable the widespread deployment of Demand Response strategies in buildings. Researchers from Lawrence Berkeley National Laboratory and Lawrence Livermore National Laboratory will present the key findings from this project in a one-hour presentation. Researchers found that several of the RF technologies tested at LBNL's Molecular Foundry building were able to provide sufficiently

6

Ernest Moniz Senate Testimony Power Point  

Broader source: Energy.gov [DOE]

This is the slide presentation used by Secretary Ernest Moniz during his testimony before the U.S. Senate Appropriations committee on spurring innovation through federal funding given April 29, 2014.

7

Testimony Before Senate Energy & Water Development Committee...  

Energy Savers [EERE]

Reports Testimony Testimony Before Senate Energy & Water Development Committee Testimony Before Senate Energy & Water Development Committee March 21, 2012 Fiscal Year 2013...

8

Testimonials | National Nuclear Security Administration  

National Nuclear Security Administration (NNSA)

Testimonials | National Nuclear Security Administration Testimonials | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Testimonials Home > Federal Employment > Working at NNSA > Testimonials Testimonials At the NNSA, you will have the opportunity to work with some of the brightest professionals in the world who routinely tackle highly complex

9

Testimonials | Department of Energy  

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

Testimonials Testimonials Testimonials Read what some employees of the Office of Energy Efficiency and Renewable Energy (EERE) are saying about their work. Photo of EERE employee Kristina of the Education and Workforce Development office. "It is largely believed that creating a clean energy economy relies on three main components: 1) The right technologies; 2) the right policies; and 3) the right politics. However, a critical ingredient is missing from this equation-the right people. "The U.S. is confronted by a serious shortage of scientists and engineers. In fact, DOW CEO Andrew Liveris recently stated that there are 'one million science, technology, engineering, and math jobs available in [the U.S.] and only 200,000 graduates qualified to fill them.' This figure challenges the

10

Testimony of Michael G  

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

Testimony of Larry Dickerman, Director or Distribution Engineering Services, Testimony of Larry Dickerman, Director or Distribution Engineering Services, American Electric Power before the House Energy and Commerce Committee March 20 th 2007 American Electric Power (AEP) is one of the nation's largest electricity generators with over 5 million retail consumers in 11 states. AEP is the leader among US utilities for deployment of large-scale battery-based energy storage. .... AEP supports the adoption of incentives for deployment of distributed stationary energy storage for improvement in security, reliability and performance of the American electric grid infrastructure. ... Testimony of Larry Dickerman Director, Distribution Engineering Services American Electric Power Before the House Science and Technology ???? Committee October 3

11

FE Speeches and Testimony  

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

speeches-and-testimony Office of Fossil Energy speeches-and-testimony Office of Fossil Energy Forrestal Building 1000 Independence Avenue, SW Washington, DC 20585202-586-6503 en DOE's Coal Research and Development http://energy.gov/fe/articles/does-coal-research-and-development-0 DOE's Coal Research and Development

12

MARKETING PORTFOLIO TESTIMONIAL*  

E-Print Network [OSTI]

MARKETING PORTFOLIO TESTIMONIAL* As a Business Marketing student at California State University Fullerton, I was required to submit a portfolio containing several marketing projects from my college career to spend some time in creating a portfolio that highlighted my marketing projects from various classes

de Lijser, Peter

13

Testimony of Jay Hakes  

Gasoline and Diesel Fuel Update (EIA)

Testimony of Jay Hakes Testimony of Jay Hakes Administrator, Energy Information Administration U.S. Department of Energy before the U.S. Senate Committee on Energy and Natural Resources on Senate Bills S.882 and S.1776 and Their Impact on EIA's Programs March 30, 2000 Thank you for the opportunity to testify on S.882 and S.1776. I will be testifying on how these Bills relate to Energy Information Administration (EIA) programs, particularly the Voluntary Reporting of Greenhouse Gases Program. The 1605(b) Program, as it is sometimes called, can be viewed as an early step in reporting voluntary efforts to reduce greenhouse gas emissions and in calculating and reporting those emissions and reductions. As the program is entirely voluntary, the fact that over 230 companies and organizations have reported on more than 1,500 projects should be viewed as

14

Congressional Testimony | Department of Energy  

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

Congressional Testimony Congressional Testimony Congressional Testimony House Energy & Water Development February 29, 2012 Fiscal Year 2013 President's Budget Request By: Thomas P. D'Agostino, Undersecretary for Nuclear Security and Administrator National Nuclear Security Administration, U.S. Department of Energy Before: House Appropriations Committee Subcommittee on Energy and Water Development February 28, 2012 FY 2013 Budget Hearing By: Secretary Steven Chu, U.S. Department of Energy Before: Subcommittee on Energy and Water Development, and Related Agencies Committee on Appropriations U.S. House of Representatives More testimony Senate Energy & Water Development March 21, 2012 Fiscal Year 2013 President's Budget Request By: Thomas P. D'Agostino, Undersecretary for Nuclear Security and

15

Oak Ridge Centers for Manufacturing Technology ? testimonials  

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

testimonials The first testimonial for the successful Oak Ridge Centers for Manufacturing Technology came from Mitchell Burnett. Mitch was among the first hourly paid employees, an...

16

Testimony before the House Appropriations Committee, Subcommittee...  

National Nuclear Security Administration (NNSA)

... Testimony before the House Appropriations Committee, Subcommittee on Energy and Water Congressional Testimony Mar 4, 2010 Administrator Thomas D'Agostino As Prepared for...

17

Systems Oriented Epistemology and Testimony Theories of testimony | A simulation model | Conclusions  

E-Print Network [OSTI]

Systems Oriented Epistemology and Testimony Theories of testimony | A simulation model.S. Zollman Carnegie Mellon University Problem of testimony Theories of testimony | A simulation model University Three views Theories of testimony | A simulation model | Conclusions The views | Two methods in SE

Zollman, Kevin

18

Congressional Testimony | Department of Energy  

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

Congressional Testimony Congressional Testimony Congressional Testimony October 2, 2013 Before the Subcommittee on Energy and Power -- House Energy and Commerce Committee Subject: Obama Administration's Climate Change Policy By: Ernest Moniz, Secretary of Energy October 2, 2013 Before the Subcommittee on Environment and the Economy -- House Energy and Commerce Committee Subject: Implementing the Nuclear Waste Policy Act -- Next Steps By: Peter Lyons, Assistant Secretary, Nuclear Energy October 2, 2013 Before the Subcommittee on Energy -- House Science, Space, and Technology Committee Subject: The Future of Coal: Utilizing America's Abundant Energy Resources By: Christopher Smith, Acting Assistant Secretary, Office of Fossil Energy August 1, 2013 Before House Committee on Oversight and Government Reform

19

Testimony Before the House Energy & Water Development Committee...  

Energy Savers [EERE]

Testimony Testimony Before the House Energy & Water Development Committee Testimony Before the House Energy & Water Development Committee February 29, 2012 Fiscal Year 2013...

20

Congressional Testimony | Department of Energy  

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

Center » Congressional Testimony Center » Congressional Testimony Congressional Testimony Testimony to Congress by various members of OE. (Some of the documents in this section require Adobe Acrobat Reader. You can download a free copy of the Reader by visiting Adobe.) Assistant Secretary Pat Hoffman before the United States House of Representatives Energy and Commerce Subcommittee on Energy and Power on DOE's emergency authority under section 202(c) of the Federal Power Act - May 9, 2012 Assistant Secretary Pat Hoffman before the United States Senate Committee on Energy and Natural Resources on the DOE's role in managing weather related electrical outages - April 26, 2012 Assistant Secretary Pat Hoffman before the United States House of Representatives Appropriations Subcommittee on Energy and Water

Note: This page contains sample records for the topic "testimony presentations radio" 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

Congressional Testimony | National Nuclear Security Administration  

National Nuclear Security Administration (NNSA)

Congressional Testimony | National Nuclear Security Administration Congressional Testimony | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog The National Nuclear Security Administration Congressional Testimony Home > Media Room > Congressional Testimony Congressional Testimony NNSA officials frequently testify before Congressional committees and subcommittees on matters of nuclear and national security.

22

Testimonial to Major-General Sir J. F. D. Donnelly, K.C.B.  

Science Journals Connector (OSTI)

... , and by men of science and artists who have been connected with it, Sir John Gorst presented, on the behalf of some five hundred subscribers, the testimonial to Sir ... Gorst presented, on the behalf of some five hundred subscribers, the testimonial to Sir John Donnelly. This consisted of a silver salver, a set of library furniture, a ...

1899-12-07T23:59:59.000Z

23

Systems Oriented Epistemology and Testimony Theories of testimony | A simulation model | Conclusions  

E-Print Network [OSTI]

Systems Oriented Epistemology and Testimony Theories of testimony | A simulation model | A simulation model | Conclusions Two questions What is our epistemic warrant for believing testimony? Who.S. Zollman Carnegie Mellon University Three views Theories of testimony | A simulation model | Conclusions

Zollman, Kevin

24

Congressional Testimony | Department of Energy  

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

About Us » News » Congressional Testimony About Us » News » Congressional Testimony Congressional Testimony October 6, 2011 Statement Before the Subcommittee on Children's Health and Environmental Responsibility, Committee on Environment and Public Works, United States Senate (10/6/2011) Statement Before the Subcommittee on Children's Health and Environmental Responsibility, Committee on Environment and Public Works, United States Senate By: David Geiser, Director, Office of Legacy Management, Department of Energy Subject: UMTRCA March 16, 2010 Statement Before the Subcommittee on Energy and Water Development, Committee on Appropriations (3/16/2010) Statement Before the Subcommittee on Energy and Water Development, Committee on Appropriations, United States House of Representatives By David Geiser, Director, Office of Legacy Management, Department of

25

Testimony of James J. Anderson  

E-Print Network [OSTI]

and Wildlife Service on the operation of the Federal Columbia River Power System and the Federal Caucus Draft to testify in this hearing on the Draft Biological Opinion. In my testimony, I first put the salmon decline salmon involved the interplay of climate/ocean fluctuations and the cumulative impact of human activities

Washington at Seattle, University of

26

Worker Testimonials | Department of Energy  

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

Worker Worker Testimonials Worker Testimonials Rick Hurrelbrink, Pipefitters Local 392, Fernald Former Worker "I'm glad I got tested because it gave me peace of mind that I had no serious health problems. Construction workers get exposed to so many different materials on job sites that you never know how you will be affected. I also was able to take care of a few minor things I wouldn't have known about." Edna Brackey, Portsmouth Gaseous Diffusion Plant Former Worker "This is a thank you statement to the WHPP (Worker Health Protection Program) program and especially to the early detection CT Scan. The scan revealed a lung nodule that turned out to be malignant and was removed while it was tiny with no further treatment needed. THANK YOU FOR MY LIFE."

27

Political Interference with Government Climate Change Science Testimony of  

E-Print Network [OSTI]

Political Interference with Government Climate Change Science Testimony of James E. Hansen;2 Political Interference with Government Climate Change Science Contents 1. Rationale of Presentation 2. My by NASA Office of Public Affairs C. Executive Control of Purse Strings 3. Practical Impact of Political

Hansen, James E.

28

Testimony & Speeches | Department of Energy  

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

Blog » Testimony & Speeches Blog » Testimony & Speeches Testimony & Speeches Testimony & Speeches 2011 Statement of David Sandalow, Assistant Secretary of Energy for Policy and International Affairs, Before the Subcommittee on Energy and the Environment, Committee on Science, Space, and Technology, United States House of Representatives, December 7, 2011. Statement of David Sandalow, Assistant Secretary of Energy for Policy and International Affairs Before the Subcommittee on Investigations and Oversight, Committee on Science, Space, and Technology, United States House of Representatives, June 14, 2011. Statement of David Sandalow, Assistant Secretary of Energy for Policy and International Affairs, Before the Subcommittee on Energy, Committee on Energy and Natural Resources, United States Senate, June 9, 2011.

29

WRITTEN TESTIMONY OF DR. ROBERT J. WOOD  

E-Print Network [OSTI]

WRITTEN TESTIMONY OF DR. ROBERT J. WOOD DIRECTOR OF THE COOPERATIVE OXFORD LABORATORY NATIONAL Robert Wood, Director of the Cooperative Oxford Laboratory, a cooperative scientific research laboratory

30

EERE Partner Testimonials - Phil Roberts, California Lithium...  

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

Phil Roberts, California Lithium Battery (CalBattery) EERE Partner Testimonials - Phil Roberts, California Lithium Battery (CalBattery) Addthis Text Version The words "Office of...

31

FE Speeches and Testimony | Department of Energy  

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

March 28, 2012 Testimony of Christopher Smith before the House Committee on Energy and Commerce Statement of Christopher Smith, Deputy Assistant Secretary for Oil and Natural Gas,...

32

Testimony Before the House Appropriations Subcommittee on Energy...  

Energy Savers [EERE]

Testimony Before the House Appropriations Subcommittee on Energy and Water Development Testimony Before the House Appropriations Subcommittee on Energy and Water Development...

33

Press Room - Radio - U.S. Energy Information Administration (EIA)  

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

Press Room Press Room Glossary › FAQS › Overview Press Releases Testimony Presentations Radio Events Radio Spots Ready-to-broadcast news stories. Transcripts provided so radio spots can be re-recorded in whole or in part. Residential heating oil prices virtually unchanged mp3 Date: December 18, 2013 Description: The average retail price for home heating oil fell 4-tenths of a penny from a week ago to $3.95 per gallon. That's down 8-tenths of a penny from a year ago, based on the residential heating fuel survey by the U.S. Energy Information Administration. Heating oil prices in the New England region rose 3.92 per gallon, up 3-tenths of a cent from last week, and up 3 cents from a year ago. Contact/Author: Amerine Woodyard, 202-586-1256 Transcript: http://www.eia.gov/radio/transcript/heating_oil_prices_12182013.pdf

34

Testimony  

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

Energy Storage Technologies: State of Development for Stationary and Vehicular Applications Thomas S. Key Technical Leader, Renewables and Distributed Generation Electric Power Research Institute October 3, 2007 Thank you, Mr. Chairman and Members of the Subcommittee. I am Thomas Key, Technical Leader, Renewable and Hydropower Generation for the Electric Power Research Institute (EPRI), a non-profit, collaborative organization conducting electricity related R&D in the public interest. EPRI has been supported voluntarily by the electric industry since our founding in 1973. Our members, public and private, account for more than 90% of the kilowatt-hours sold in the U.S., and we now serve more than 1000 energy and governmental organizations in more that 40 countries.

35

Congressional Testimony | Department of Energy  

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

18, 2012 18, 2012 Testimony Before the House Subcommittee on Oversight and Investigations - Committee on Energy and Commerce Subject: FY 2013 Budget Process for the American Recovery and Reinvestment Act By: Christopher Johns, Director, Office of Budget March 28, 2012 Before House Subcommittee on Energy and Power - Committee on Energy and Commerce Subject: Strategic Energy Production Act of 2012 and Gasoline Regulations Act of 2012 By: Chris Smith, Deputy Assistant Secretary for Oil and Natural Gas March 27, 2012 Before House Subcommittee on Oversight and Investigations - Committee on Energy and Commerce Subject: IT Supply Chain Security By: Gil Vega, Associate Chief Information Officer for Cybersecurity and Chief Informtion Security Officer March 20, 2012 Before the Subcommittee on Water and Power - Committee on Natural Resources

36

Testimony of Dr. Hermann A. Grunder  

E-Print Network [OSTI]

Testimony of Dr. Hermann A. Grunder Director Argonne National Laboratory before the Subcommittee knowledge for the sake of knowledge set the stage for nuclear medicine, nuclear energy, and many other

37

Anderson Testimony to Water Power Subcommittee, Lewiston Idaho, May 31 1997 Page 1 Testimony of  

E-Print Network [OSTI]

of reservoir drawdown through funding from the Bonneville Power Administration and the Army Corps of EngineersAnderson Testimony to Water Power Subcommittee, Lewiston Idaho, May 31 1997 Page 1 Testimony before the U.S. House of Representatives Subcommittee on Water and Power in Lewiston Idaho May 31, 1997

Washington at Seattle, University of

38

Testimonials: Presidents Management Council Interagency Rotational Program  

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

Testimonials: Presidents Management Council Interagency Rotational Testimonials: Presidents Management Council Interagency Rotational Program Testimonials: Presidents Management Council Interagency Rotational Program Diane Turchetta - Department of Transportation My rotation in EERE's Clean Cities Program has helped me to better understand how the program works and the great strides it is making, though it's coalitions, to reduce petroleum use across the country. The rotation has also provided me with an opportunity to learn more about the other efforts and initiatives underway in the Vehicle Technology Program including wireless charging for electric vehicles, research on materials technologies, and technology improvements for both light-duty and heavy-duty vehicles. I plan to use the information and knowledge I have

39

FE Speeches and Testimony | Department of Energy  

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

Speeches and Testimony Speeches and Testimony FE Speeches and Testimony RSS July 25, 2013 DOE's Coal Research and Development Statement of Christopher Smith, Acting Assistant Secretary for Fossil Energy, before the House Committee on Science, Space and Technology Subcommittee on Energy June 18, 2013 DOE's Program Regulating Liquefied Natural Gas Export Applications Statement of Christopher Smith, Acting Assistant Secretary for Fossil Energy, before the House Committee on Energy and Commerce Subcommittees on Energy and Power April 26, 2013 DOE's Shale Gas and Hydraulic Fracturing Research Statement of Guido DeHoratiis Acting Deputy Assistant Secretary for Oil and Natural Gas before the House Committee on Science, Space, and Technology Subcommittees on Energy and Environment March 19, 2013

40

Testimony before the House Appropriations Committee, Subcommittee on Energy  

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

House Appropriations Committee, Subcommittee on Energy House Appropriations Committee, Subcommittee on Energy and Water | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > Testimony before the House Appropriations Committee, Subcommittee ... Congressional Testimony Testimony before the House Appropriations Committee, Subcommittee on Energy

Note: This page contains sample records for the topic "testimony presentations radio" 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

FY 2012 Budget Hearing Testimony House Armed Services Committee,  

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

House Armed Services Committee, House Armed Services Committee, Subcommittee on Strategic Forces | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony House Armed ... Congressional Testimony FY 2012 Budget Hearing Testimony House Armed Services Committee,

42

FY 2012 Budget Hearing Testimony before the House Appropriations Committee,  

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

House Appropriations Committee, House Appropriations Committee, Energy and Water Development Subcommittee | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony before the ... Congressional Testimony FY 2012 Budget Hearing Testimony before the House Appropriations Committee,

43

Testimony before the Senate Committee on Energy & Natural Resources |  

National Nuclear Security Administration (NNSA)

Senate Committee on Energy & Natural Resources | Senate Committee on Energy & Natural Resources | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > Testimony before the Senate Committee on Energy ... Congressional Testimony Testimony before the Senate Committee on Energy & Natural Resources

44

FY 2012 Budget Hearing Testimony before the House Appropriations Committee,  

National Nuclear Security Administration (NNSA)

House Appropriations Committee, House Appropriations Committee, Energy and Water Development Subcommittee | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony before the ... Congressional Testimony FY 2012 Budget Hearing Testimony before the House Appropriations Committee,

45

Testimony before the House Appropriations Committee, Subcommittee on Energy  

National Nuclear Security Administration (NNSA)

House Appropriations Committee, Subcommittee on Energy House Appropriations Committee, Subcommittee on Energy and Water | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > Testimony before the House Appropriations Committee, Subcommittee ... Congressional Testimony Testimony before the House Appropriations Committee, Subcommittee on Energy

46

FY 2012 Budget Hearing Testimony House Armed Services Committee,  

National Nuclear Security Administration (NNSA)

House Armed Services Committee, House Armed Services Committee, Subcommittee on Strategic Forces | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony House Armed ... Congressional Testimony FY 2012 Budget Hearing Testimony House Armed Services Committee,

47

WRITTEN TESTIMONY OF DR. JAMES S. FAMIGLIETTI  

E-Print Network [OSTI]

to provide testimony on the state of our water supply and water supply monitoring in California, including beneath Orange County. Nearly 80 percent of the fresh water used in the United States is for agriculture.S. In short, it the second most pumped aquifer in the United States. The current water crisis in California

George, Steven C.

48

WRITTEN TESTIMONY BY SAMUEL D. RAUCH III  

E-Print Network [OSTI]

.S.) as a recognized global leader in responsibly managed fisheries and sustainable seafood. My testimony today recreational catch remained stable. U.S. commercial fishermen landed 9.9 billion pounds of seafood valued at $5.1 The seafood industry--harvesters, seafood processors and dealers, seafood wholesalers and seafood

49

Presented at "RFI2004: Workshop on Mitigation of Radio Frequency Interference in Radio Astronomy"; Penticton, Canada, 16-18 July 2004  

E-Print Network [OSTI]

"; Penticton, Canada, 16-18 July 2004 "Quiet, please!" - regulatory protection strategies for the SKA Wim van of the large financial investment foreseen in the Square Kilometre Array (SKA) radio telescope, it will need sensitive observations outside the frequency bands allocated by the International Telecommunication Union

Ellingson, Steven W.

50

Press Room - Testimony - U.S. Energy Information Administration (EIA)  

Gasoline and Diesel Fuel Update (EIA)

Previous Years: 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004 2003 2002 Previous Years: 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004 2003 2002 2001 2000 1999 1998 1997 2013 Congressional Testimony U.S. petroleum supply system pdf Subject: EIA, Petroleum Presented by: Adam Sieminski, Administrator Presented to: Committee on Energy and Natural Resources U.S. Senate Washington, DC-July 16, 2013 Renewable Fuel Standard (RFS) program pdf Subject: EIA, Renewable, Forecasts Presented by: Adam Sieminski, Administrator Presented to: Subcommittee on Energy and Power Committee on Energy and Commerce U.S. House of Representatives Washington, DC-June 26, 2013 U.S. Energy Outlook pdf Subject: EIA, Energy Markets, Forecasts Presented by: Adam Sieminski, Administrator Presented to: Subcommittee on Energy Committee on Science, Space and Technology

51

Deputy Assistant Secretary Matt Moury's Written Testimony Before...  

Office of Environmental Management (EM)

Matt Moury's Written Testimony Before the Subcommittee on Financial and Contracting Oversight Committee on Homeland Security and Government Affairs (March 11, 2014) Deputy...

52

Principal Deputy Chief William A. Eckroade's Written Testimony...  

Office of Environmental Management (EM)

William A. Eckroade's Written Testimony Before the Subcommittee on Financial and Contracting Oversight Committee on Homeland Security and Governmental Affairs (March 11, 2014)...

53

Testimony Before the House Energy and Commerce Subcommittee on...  

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

Energy and Commerce Subcommittee on Energy and Environment Testimony Before the House Energy and Commerce Subcommittee on Energy and Environment Before the House Energy and...

54

Presentations  

Office of Science (SC) Website

Presentations Presentations Basic Energy Sciences (BES) BES Home About Research Facilities Science Highlights Benefits of BES Funding Opportunities Basic Energy Sciences Advisory Committee (BESAC) News & Resources Program Summaries Brochures Reports Accomplishments Presentations BES and Congress Science for Energy Flow Seeing Matter Scale of Things Chart Contact Information Basic Energy Sciences U.S. Department of Energy SC-22/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-3081 F: (301) 903-6594 E: sc.bes@science.doe.gov More Information » News & Resources Presentations Print Text Size: A A A RSS Feeds FeedbackShare Page Provided here are selected presentations given by the Director of BES since 2001 and some other related presentations. These are often large Powerpoint

55

Presentations  

Broader source: Energy.gov [DOE]

This page provides links to the presentations given at DOE Solid-State Lighting workshops and major conferences, as well as links to reference materials. Some of the following documents are...

56

Presentations  

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

Meeting Goals & Process Meeting Goals & Process December 26, 2012 | Author(s): Harvey Wasserman | Download File: LogisticsHarveyWasserman.pdf | pdf | 1.3 MB Meeting Goals & Process Liz Sexton---Kennedy: Present and Future Computing Requirements for CMS and ATLAS November 27, 2012 | Author(s): Liz Sexton---Kennedy (Fermilab) | Download File: LHC-Sexton-Kennedy.pdf | pdf | 638 KB Present and Future Computing Requirements for CMS and ATLAS Rob Roser and Tom LeCompte: Detector Simulations using GEANT 4 November 27, 2012 | Author(s): Rob Roser (Fermi National Accelerator Laboratory) and Tom LeCompte (ANL) | Download File: ROSER-NERSC.pdf | pdf | 2.2 MB Detector Simulations using GEANT 4 Scott Dodelson: The Dark Energy Survey (DES) November 27, 2012 | Author(s): Scott Dodelson (Fermilab) | Source: The Dark

57

PRESENT:  

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

PUBLIC MEETING PUBLIC MEETING + + + + + FRIDAY NOVEMBER 14, 1997 + + + + + WASHINGTON, D.C. The Committee met in the Clark Room of the Capital Holiday Inn, 550 C Street, S.W., at 10:30 a.m., G. Campbell Watkins, Chair, presiding. PRESENT: G. CAMPBELL WATKINS, Chair DANIEL A. RELLES, Vice Chair DAVID R. BELLHOUSE R. SAMPRIT CHATTERJEE BRENDA G. COX CAROL A. GOTWAY CRAWFORD PHILIP HANSEN CALVIN KENT GRETA M. LJUNG ROY W. WHITMORE INVITED GUESTS: SEYMOUR SUDMAN RICHARD TABORS EIA STAFF PRESENT: JAY HAKES, EIA Administrator BILL WEINIG LYNDA CARLSON DAVID MOREHOUSE JOHN WOOD ART ANDERSON BOB MANICKE I N D E X Item: Page: World Oil Supply; Evidence from 4 Estimating Supply Functions by Country Questions from the Committee 54 Public Comments 62 Closing Comments by the Chair 67 P-R-O-C-E-E-D-I-N-G-S

58

Presentations  

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

Cameron Geddes: Plasma Accelerator Simulation Using Laser and Particle Cameron Geddes: Plasma Accelerator Simulation Using Laser and Particle Beam Drivers Author(s): Cameron Geddes (LBNL) | Download File: Geddes-LPA.pdf | pdf | 7.5 MB Plasma Accelerator Simulation Using Laser and Particle Beam Drivers Liz Sexton---Kennedy: Present and Future Computing Requirements for CMS and ATLAS November 27, 2012 | Author(s): Liz Sexton---Kennedy (Fermilab) | Download File: LHC-Sexton-Kennedy.pdf | pdf | 638 KB Present and Future Computing Requirements for CMS and ATLAS Rob Roser and Tom LeCompte: Detector Simulations using GEANT 4 November 27, 2012 | Author(s): Rob Roser (Fermi National Accelerator Laboratory) and Tom LeCompte (ANL) | Download File: ROSER-NERSC.pdf | pdf | 2.2 MB Detector Simulations using GEANT 4 Scott Dodelson: The Dark Energy Survey (DES)

59

Testimony Before the Senate Armed Services Committee, New START Treaty  

National Nuclear Security Administration (NNSA)

Before the Senate Armed Services Committee, New START Treaty Before the Senate Armed Services Committee, New START Treaty Hearing | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > Testimony Before the Senate Armed Services Committee, ... Congressional Testimony Testimony Before the Senate Armed Services Committee, New START Treaty

60

Presentations  

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

NERSC Role in Biological and Environmental Research NERSC Role in Biological and Environmental Research September 12, 2012 | Author(s): Kathy Yelick | Download File: NERSC-BER-Yelick.ppt | ppt | 35 MB Present and Future Computing Requirements for Computational Prediction of Protein-DNA Binding September 12, 2012 | Author(s): Mohammed AlQuraishi | Download File: AlQuraishi.pdf | pdf | 1 MB KBASE: Data and Modeling for Predictive Biology September 12, 2012 | Author(s): Tom Brettin and Shane Canon | Download File: KBaseBrettin.pdf | pdf | 5.9 MB DOE Joint Genome Institute September 11, 2012 | Download File: JGI.pdf | pdf | 8.4 MB 20th Century Reanalysis September 11, 2012 | Author(s): Gil Compo | Download File: Compo.pdf | pdf | 2.4 MB Molecular Dynamics Simulation of Protein Dynamics and Lignocellulosic Biomass

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


61

Presented  

Office of Scientific and Technical Information (OSTI)

l* l* t , f , q.o Presented at the 20th International Pyrotechnics Seminar Colorado Springs, Colorado July 24-29, 1994 COMMENTS ON TNT EQUIVALENCE Paul W. Cooper Sandia National Laboratories Albuquerque, New Mexico U.S.A. 87185-1156 ABSTRACT The term "TNT Equivalence" is used throughout the explosives and related industries to compare the effects of the output of a given explosive to that of TNT. This is done for technical design reasons in scaling calculations such as for the prediction of blast waves, craters, and structural response, and is also used as a basis for government regulations controlling the shipping, handling and storage Of explosive materials, as well as for the siting and design of explosive facilities. TNT equivalence is determined experimentally by several different types of tests, the most common of which include: plate dent, ballistic mortar, trauzl,

62

Presentations  

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

Molecular Dynamics Simulation of Protein Dynamics and Lignocellulosic Molecular Dynamics Simulation of Protein Dynamics and Lignocellulosic Biomass September 11, 2012 | Download File: PetridisNERSC12.pdf | pdf | 2.8 MB Subsurface Flow and Reactive Transport September 11, 2012 | Author(s): Tim Scheibe | Download File: Scheibe.pdf | pdf | 7.5 MB 20th Century Reanalysis September 11, 2012 | Author(s): Gil Compo | Download File: Compo.pdf | pdf | 2.4 MB Present and Future Computing Requirements for Computational Prediction of Protein-DNA Binding September 12, 2012 | Author(s): Mohammed AlQuraishi | Download File: AlQuraishi.pdf | pdf | 1 MB Climate Science for a Sustainable Energy Future September 11, 2012 | Author(s): David Bader | Download File: CSSEFBader.pdf | pdf | 21 MB KBASE: Data and Modeling for Predictive Biology September 12, 2012 | Author(s): Tom Brettin and Shane Canon |

63

Presenters  

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

October 16 October 16 Presenters 7:30 Registration 8:30 Welcome Remarks Pilar Thomas, Department of Energy (DOE), Office of Indian Energy Policy and Programs Introductions All 9:00 DOE Tribal Grant Program Overview Lizana Pierce, Department of Energy, Golden Field Office Alaska START Program Overview Alex Dane, National Renewable Energy Laboratory (NREL) Denali Commission Overview Joel Niemeyer, Denali Commission 9:45 Pathways to Native Village Energy Development Village Energy Planning and Project Development Pilar Thomas, DOE Office of Indian Energy 10:30 -- Break 11:00 Native Village Energy Planning Community Project Development Principles Alex Dane (Moderator), NREL Tribal Energy Planning for the Organized Village of Kasaan Glenn "Stormy" Hamar , Organized Village of Kasaan

64

FY 2012 Budget Hearing Testimony on Nuclear Nonproliferation and Naval  

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

on Nuclear Nonproliferation and Naval on Nuclear Nonproliferation and Naval Reactor Programs before the House Appropriations Committee, Energy and Water Development Subcommittee | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony on Nuclear ...

65

FY 2012 Budget Hearing Testimony on Nuclear Nonproliferation and Naval  

National Nuclear Security Administration (NNSA)

on Nuclear Nonproliferation and Naval on Nuclear Nonproliferation and Naval Reactor Programs before the House Appropriations Committee, Energy and Water Development Subcommittee | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Congressional Testimony > FY 2012 Budget Hearing Testimony on Nuclear ...

66

Final Testimony Poneman September 22, 2011  

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

Testimony of Deputy Secretary Daniel Poneman U.S. Department of Energy Before the Committee on Oversight and Government Reform U.S. House of Representatives September 22, 2011 Chairman Issa, Ranking Member Cummings, and Members of the Committee, thank you for the opportunity to appear before you today to discuss the Department of Energy's (DOE) programs to strengthen our energy security, to advance clean energy innovation, to create jobs for the American people, and to make the U.S. more competitive in the global economy. In the U.S., we spend more than a trillion dollars a year on primary energy. 1 Worldwide, between five and ten trillion dollars are spent on energy every year. Energy represents a large and growing segment of the global economy.

67

BrinkmanFinal_Testimony(8).pdf  

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

STATEMENT OF STATEMENT OF DR. WILLIAM F. BRINKMAN DIRECTOR OF THE OFFICE OF SCIENCE FOR THE U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON INVESTIGATIONS AND OVERSIGHT COMMITTEE ON SCIENCE AND TECHNOLOGY U.S. HOUSE OF REPRESENTATIVES APRIL 22, 2010 Thank you Mr. Chairman, Ranking Member Broun, and Members of the Committee. I appreciate the opportunity to appear before you to provide testimony on the DOE's role and reaction to the national Helium-3 ( 3 He) shortage. Both the National Nuclear Security Administration (NNSA), and the DOE Isotope Development and Production for Research and Applications Program (Isotope Program) recently transferred to the Office of Science in the FY 2009 Appropriation, play a role in Helium-3 production and distribution. I

68

Testimony by the Inspector General | Department of Energy  

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

Testimony by the Inspector General Testimony by the Inspector General Testimony by the Inspector General Testimony by the Inspector General May 1, 2002 Gregory H. Friedman: Before the U.S. House of Representatives Committee on Energy and Commerce Subcommittee on Oversight and Investigations Statement of Gregory H. Friedman, Inspector General U.S. Department of Energy Subject: U.S. Department of Energy's Purchase Card Programs-Lessons Learned March 15, 2001 Gregory H. Friedman: Before the Subcommittee on National Security, Veterans Affairs, and International Relations of the Committee on Government Reform U.S. House of Representatives Statement of Gregory H. Friedman Inspector General Department of Energy Subject: Performance and management challenges confronting the Department of Energy June 10, 1999

69

Testimony Before the House Committee on Science, Space, and Technology |  

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

Testimony Before the House Committee on Science, Space, and Testimony Before the House Committee on Science, Space, and Technology Testimony Before the House Committee on Science, Space, and Technology June 18, 2013 - 11:03am Addthis Dr. Ernest Moniz Dr. Ernest Moniz Secretary of Energy Media: Watch archived video footage of the testimony. Chairman Smith, Ranking Member Johnson, and Members of the Committee, thank you for the opportunity to appear before you today to lay out my vision for the Department of Energy. I have had the opportunity to meet with several members of the Committee during my first four weeks on the job and I look forward to meeting with and working with this Committee in the coming weeks, months, and years. Indeed, I look forward to continuing my engagement with members of Congress from both parties and both chambers to constructively illuminate our

70

Summary of Testimony of Larry Dickerman, Director or Distribution  

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

Summary of Testimony of Larry Dickerman, Director or Distribution Summary of Testimony of Larry Dickerman, Director or Distribution Engineering Services, American Electric Power before the House Energy and Commerce Committee March 20th 2007 Summary of Testimony of Larry Dickerman, Director or Distribution Engineering Services, American Electric Power before the House Energy and Commerce Committee March 20th 2007 Summary of Testimony of Larry Dickerman, Director or Distribution Engineering Services, American Electric Power before the House Energy and Commerce Committee March 20th 2007. American Electric Power (AEP) is one of the nation's largest electricity generators with over 5 million retail consumers in 11 states. AEP is the leader among US utilities for deployment of large-scale battery-based energy storage. AEP supports the adoption of

71

Secretary Chu Testimony to Senate Armed Services Committee | Department of  

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

Testimony to Senate Armed Services Committee Testimony to Senate Armed Services Committee Secretary Chu Testimony to Senate Armed Services Committee June 17, 2010 - 12:00am Addthis Washington, DC -- Secretary Steven Chu testified today before the Senate Armed Services Committee on the New START Treaty. His prepared testimony is below: Chairman Levin, Ranking Member McCain, and Members of the Committee, thank you for the opportunity to testify on the Treaty between the United States of America and the Russian Federation on Measures for the Further Reduction and Limitation of Strategic Offensive Arms, known as "New START." In Prague last April, President Obama outlined a comprehensive agenda for addressing nuclear dangers in the 21st century. He pledged to take concrete steps toward a world without nuclear weapons, while maintaining

72

Testimony Before the House Committee on Science, Space, and Technology |  

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

Testimony Before the House Committee on Science, Space, and Testimony Before the House Committee on Science, Space, and Technology Testimony Before the House Committee on Science, Space, and Technology June 18, 2013 - 11:03am Addthis Dr. Ernest Moniz Dr. Ernest Moniz Secretary of Energy Media: Watch archived video footage of the testimony. Chairman Smith, Ranking Member Johnson, and Members of the Committee, thank you for the opportunity to appear before you today to lay out my vision for the Department of Energy. I have had the opportunity to meet with several members of the Committee during my first four weeks on the job and I look forward to meeting with and working with this Committee in the coming weeks, months, and years. Indeed, I look forward to continuing my engagement with members of Congress from both parties and both chambers to constructively illuminate our

73

Testimony by the Inspector General | Department of Energy  

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

Testimony by the Inspector General Testimony by the Inspector General Testimony by the Inspector General Testimony by the Inspector General August 1, 2013 Gregory H. Friedman: Provided for The Committee on Oversight and Government Reform U.S. House of Representatives Gregory H. Friedman: Provided for The Committee on Oversight and Government Reform U.S. House of Representatives July 24, 2013 Gregory H. Friedman: Provided for the Subcommittee on Oversight and Investigations Committee on Energy and Commerce U.S. House of Representatives Statement of Gregory H. Friedman Inspector General U.S. Department of Energyon Oversight and Investigations Committee on Energy and Commerce U.S. House of Representatives June 27, 2013 Gregory H. Friedman: Provided for the Subcommittee on Financial and Contracting Oversight Committee on Homeland Security and Governmental

74

WP-07 IP Direct Testimony (wp07/initial)  

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

Initial Proposal Direct Testimony documents were provided to rate case parties on CD-ROM at the Prehearing Conference and filed with the hearing clerk via the Rate Case Parties...

75

Testimony on Impacts of Proposed LPG Tank Development in Searsport, Maine on Property Values and Tourism-based Economic Activity  

E-Print Network [OSTI]

Testimony on Impacts of Proposed LPG Tank Development in Searsport, Maine on Property Values and Tourism-based Economic Activity Prepared for Thanks But No Tank (TBNT) for Presentation to the Searsport At the request of Counsel for Thanks But No Tanks (TBNT) and the Islesboro Island Trust (IIT), I have reviewed

Thomas, Andrew

76

EIA - Energy Conferences & Presentations.  

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

Presentations, Testimony, Events Presentations, Testimony, Events EIA Conference 2009 Tuesday, April 7 See each session for audio and video presentations! Plenary Session Welcome - Howard Gruenspecht Acting Administrator, Energy Information Administration Keynote Address; The Energy Problem - Dr. Steven Chu, Secretary of Energy The Economics of an Integrated World Oil Market - William D. Nordhaus, Sterling Professor of Economics, Yale University Energy in a Carbon-Constrained World - John W. Rowe, Chairman and Chief Executive Officer, Exelon Corporation Concurrent Sessions 1. The Future for Transport Demand 2. What's Ahead for Natural Gas Markets? Moderator: Andy Kydes (EIA) Moderator: Steve Harvey (EIA) Speakers: Lew Fulton (International Energy Agency) David Greene (Oak Ridge National Laboratory)

77

Testimony Before the House Committee on Energy and Commerce Subcommittee on Energy and Power  

Broader source: Energy.gov [DOE]

Secretary Moniz's full written testimony prepared for the House Committee on Energy and Commerce, Subcommittee on Energy and Power.

78

Secretary Chu's Written Testimony before the House Committee on Oversight  

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

Secretary Chu's Written Testimony before the House Committee on Secretary Chu's Written Testimony before the House Committee on Oversight and Government Reform Secretary Chu's Written Testimony before the House Committee on Oversight and Government Reform March 19, 2012 - 4:44pm Addthis Chairman Issa, Ranking Member Cummings, and Members of the Committee, thank you for the opportunity to discuss the Department of Energy's work through the American Recovery and Reinvestment Act to strengthen the U.S. economy and promote a secure energy future. When President Obama took office, the United States was in the midst of the greatest economic crisis since the Great Depression. More than 800,000 jobs were lost in January of 2009, and nearly 3 million jobs were lost in the six months before that. To meet this challenge, we had to respond quickly and forcefully. In

79

Secretary Chu's Testimony to Senate Energy and Water Development  

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

Chu's Testimony to Senate Energy and Water Development Chu's Testimony to Senate Energy and Water Development Subcommittee Secretary Chu's Testimony to Senate Energy and Water Development Subcommittee April 28, 2010 - 12:00am Addthis Washington, DC -- Secretary Steven Chu testified today before the Senate Subcommittee on Energy and Water Development on current energy policies and future energy goals. His opening statement is below: Chairman Dorgan, Ranking Member Bennett, and Members of the Committee, thank you for the opportunity to appear before you to discuss our nation's energy policy. We are driven to change our energy habits by several serious challenges. America is highly dependent on oil. Our climate is changing as a result of our carbon emissions. In order to mitigate the considerable risks of climate change, the world must transition to a sustainable energy future,

80

WRITTEN TESTIMONY OF JANE LUBCHENCO, Ph.D.  

E-Print Network [OSTI]

, including those in ocean-dependent industries such as fishing, marine transportation, and coastal tourismWRITTEN TESTIMONY OF JANE LUBCHENCO, Ph.D. UNDER SECRETARY OF COMMERCE FOR OCEANS AND ATMOSPHERE NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION U.S. DEPARTMENT OF COMMERCE LEGISLATIVE HEARING

Note: This page contains sample records for the topic "testimony presentations radio" 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

WRITTEN TESTIMONY OF ROBERT E. MAGNIEN, Ph.D.  

E-Print Network [OSTI]

1 WRITTEN TESTIMONY OF ROBERT E. MAGNIEN, Ph.D. DIRECTOR CENTER FOR SPONSORED COASTAL OCEAN and livelihoods of Americans, and providing products and services that benefit the economy, environment River Basin, we are witnessing some of these complex factors that drive HABs and hypoxia. NOAA

82

OUTLINE OF TESTIMONY FOR PBI/RF/NV  

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

TESTIMONY TESTIMONY STATEMENT OF JOHN C. LAYTON INSPECTOR GENERAL DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON OVERSIGHT AND INVESTIGATIONS UNITED STATES HOUSE OF REPRESENTATIVES 10:00 A.M. October 23, 1997 SUMMARY OF STATEMENT BY JOHN C. LAYTON The Office of Inspector General, Department of Energy (DOE), has identified deficiencies in the administration of performance-based contracts. For example, we found: Incentive fees were excessive in relation to the cost of the work. * An incentive fee of $225,000 was paid to replace a ventilation fan when the cost of this work for the year was only $25,000. Incentive fees were paid for work completed before the establishment of the performance objective. * A $776,000 incentive fee was paid for work completed on experiments before the

83

3-5-09_Final_Testimony_(EIA)_(Gruenspecht).pdf  

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

TESTIMONY OF TESTIMONY OF DR. HOWARD GRUENSPECHT ACTING ADMINISTRATOR ENERGY INFORMATION ADMINISTRATION BEFORE THE SUBCOMMITTEE ON ENERGY AND MINERAL RESOURCES COMMITTEE ON NATURAL RESOURCES U. S. HOUSE OF REPRESENTATIVES MARCH 5, 2009 2 Mr. Chairman and Members of the Committee, I appreciate the opportunity to appear before you today to discuss the U.S. energy outlook to 2030, focusing on the role of the Outer Continental Shelf (OCS) in current and projected energy production. The Energy Information Administration (EIA) is the independent statistical and analytical agency within the Department of Energy that produces objective, timely, and relevant data, projections, and analyses to assist policymakers, help markets function efficiently, and inform the public. We do not promote, formulate, or take positions on policy issues,

84

5_13_09_HSS_Fin_Testimony.pdf  

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

Written Testimony of Glenn S. Podonsky Written Testimony of Glenn S. Podonsky Chief Health, Safety and Security Officer U.S. Department of Energy FY 2010 Appropriation Hearing Before the Subcommittee on Strategic Forces Committee on Armed Services U.S. House of Representatives May 13, 2009 INTRODUCTION Chairman Tauscher, Ranking Member Turner, and members of the subcommittee, thank you for inviting me to testify today on the Fiscal Year (FY) 2010 Budget Request for the Office of Health, Safety and Security (HSS). As the central organization within the Department of Energy (Department or DOE) responsible for health, safety, security, and environment, HSS provides the Department with effective and consistent policy, technical assistance, professional development and training, complex-wide independent oversight, and enforcement. As the Chief Health,

85

2007 Wholesale Power Rate Case Initial Proposal : Direct Testimony.  

SciTech Connect (OSTI)

The purpose of our testimony is to sponsor the rate design portions of Bonneville Power Administration's (BPA) Wholesale Power Rate Development Study (WPRDS), WP-07-E-BPA-05, and associated portions of the Wholesale Power Rate Schedules and GRSPs (WP-07-E-BPA-07). Our testimony is organized in eight sections. The first section outlines the purpose of our testimony. Section 2 describes BPA's Demand Rates, including subsections on the definition of the Demand Rate, the method for computing the Demand Rates, and differences from the currently effective WP-02 Demand Rate. Section 3 describes BPA's Load Variance Rate, with subsections on the definition and purpose of the Load Variance Rate, application of the Load Variance Rate, how the Load Variance Rate is calculated, and the differences from the WP-02 Load Variance Rate. Section 4 describes the steps involved in developing BPA's energy rates and differences from the WP-02 rate case. Section 5 discusses discontinuation of the Stepped Up Multi-Year Block Rate. Section 6 describes a minor change to the Unauthorized Increase Rates and the Excess Factoring Rates. Section 7 describes the Targeted Adjustment Charge. Section 8 addresses the Operating Reserves Credit.

United States. Bonneville Power Administration.

2005-11-01T23:59:59.000Z

86

2-26-09_Final_Testimony_(Gruenspect)EIA.pdf  

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

before the Subcommittee on Energy and Environment Committee on Energy and Commerce U.S. House of Representatives February 26, 2009 Mr. Chairman, and members of the Committee, I appreciate the opportunity to appear before you today. My testimony reviews the role of renewable electricity generation in the Energy Information Administration's (EIA) Annual Energy Outlook 2009 (AEO2009) projections, provides a brief overview of the renewable resource base, and discusses key findings from earlier EIA analyses of proposals for a Federal renewable portfolio standard. EIA is the independent statistical and analytical agency within the Department of Energy. We are charged with providing objective, timely, and relevant data, analyses, and projections for the use

87

Radio Observations of High Redshift Radio Galaxies  

E-Print Network [OSTI]

We review some aspects of radio continuum polarimetric imaging of high redshift radio galaxies. The correlation between extreme values of Faraday rotation observed toward radio emitting structures in nearby radio galaxies, and X-ray emitting cluster atmospheres, is presented as a method for targeting objects at high redshift for deep X-ray searches. We present an X-ray detection of the extreme rotation measure radio galaxy PKS 1138-262 at z = 2.156, and we argue that the X-ray emission is from a cluster atmosphere with a luminosity of 1.7x10^{44} h^{-2} ergs sec^{-1}. We also present results on the correlation between size and redshift for a sample of ultra-luminous radio galaxies between 0 < z < 4.3. Source sizes decrease systematically with redshift, suggesting either denser environments, or younger sources, at high redshift. An alternative explanation is significant inverse Compton losses off the microwave background at high redshift.

C. L. Carilli; H. J. A. Rottgering; G. K. Miley L. Pentericci; D. E. Harris

1998-02-18T23:59:59.000Z

88

2007 Wholesale Power Rate Case Initial Proposal : Direct Testimony  

SciTech Connect (OSTI)

The purpose of this testimony is to provide the context and background to the financial and risk policy objectives for BPA's WP-07 Initial Proposal. The testimony contains eight sections. The first is this introduction. Section 2 provides background regarding BPA's Subscription Strategy and the Subscription contracts to which the WP-07 rates will apply. Section 3 describes the financial policy objectives considered when establishing the WP-07 rates. Section 4 describes BPA's risk profile, the risk mitigation tools used in prior rate periods, those proposed here, and additional tools under consideration for the FY 2007-2009 rate period. Section 5 describes financial policy directives and decisions that have shaped the WP-07 Initial Proposal. Section 6 describes the uncertainties of the current litigation regarding the National Marine Fisheries Service (NMFS) Federal Columbia River Power System (FCRPS) Biological Opinion and how it is addressed in this proposal. Section 7 briefly discusses the risk mitigation package in the WP-07 Initial Proposal. Finally, Section 8 describes some liquidity tools that may be incorporated into final studies if circumstances allow.

United States. Bonneville Power Administration.

2005-11-01T23:59:59.000Z

89

7-30-09_Final_Testimony_(Boswell).pdf  

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

DR. RAY BOSWELL DR. RAY BOSWELL NATIONAL ENERGY TECHNOLOGY LABORATORY U.S. DEPARTMENT OF ENERGY BEFORE THE COMMITTEE ON NATURAL RESOURCES SUBCOMMITTEE ON ENERGY AND MINERAL RESOURCES U.S. HOUSE OF REPRESENTATIVES JULY 30, 2009 Thank you, Mr. Chairman and Members of the Subcommittee. I appreciate this opportunity to provide testimony on the status of the United States Department of Energy's (DOE's) research efforts in naturally-occurring gas hydrates. INTRODUCTION Since 2000, DOE, through the Office of Fossil Energy's National Energy Technology Laboratory (NETL), has led the national research program in gas hydrates. The program is conducted through partnerships with private institutions and universities, and supported using the unique capabilities of DOE's National Laboratories.

90

9-10-09_Final_Testimony_(Gillo).pdf  

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

JEHANNE GILLO JEHANNE GILLO DIRECTOR FOR FACILITIES AND PROJECT MANAGEMENT DIVISION OFFICE OF NUCLEAR PHYSICS OFFICE OF SCIENCE U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON ENERGY AND ENVIRONMENT COMMITTEE ON SCIENCE AND TECHNOLOGY U.S. HOUSE OF REPRESENTATIVES SEPTEMBER 10, 2009 Thank you Mr. Chairman, Ranking Member Inglis, and Members of the Committee. I appreciate the opportunity to appear before you to provide testimony on the DOE Office of Science's Isotope Development and Production for Research and Applications program within the Office of Nuclear Physics. The Isotope Program was transferred from the Office of Nuclear Energy to the Office of Nuclear Physics within the Office of Science in March 2009, and, specifically, to the Nuclear Physics Facilities and Project

91

10-29-09_Final_Testimony_(Synakowski).pdf  

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

Statement of Statement of Dr. Edmund Synakowski Associate Director for Fusion Energy Sciences Office of Science U.S. Department of Energy Before the Subcommittee on Energy and Environment Committee on Science and Technology U.S. House of Representatives October 29, 2009 Thank you Mr. Chairman, Ranking Member Inglis, and Members of the Committee for the opportunity to appear before you to provide testimony on the Fusion Energy Sciences program in the Department of Energy's (DOE's) Office of Science (SC). I have been Director of the Office of Fusion Energy Science since June 7 th of this year. It is a privilege to lead the nation's fusion energy sciences program following a career of scientific research and service at two national laboratories and in research collaborations

92

3-10-09_Final_Testimony_(Meeks).pdf  

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

TIMOTHY J. MEEKS TIMOTHY J. MEEKS ADMINISTRATOR WESTERN AREA POWER ADMINISTRATION U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES MARCH 10, 2009 I am Timothy J. Meeks, Administrator of the Western Area Power Administration (Western). This is my testimony for the March 10 oversight hearing on "Federal Power Marketing Administration Borrowing Authority: Defining Success." Good afternoon and thank you, Madame Chairwoman and Subcommittee members. It's a privilege to update you on the actions Western is taking right now to deliver the results envisioned under Section 402 of the American Recovery and Reinvestment Act of 2009 (Recovery Act). Section 402 grants borrowing authority to Western, which is a tremendous

93

3-4-10_Final_Testimony_(BPA)_(Wright).pdf  

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

STATEMENT OF STATEMENT OF STEPHEN J. WRIGHT ADMINISTRATOR BONNEVILLE POWER ADMINISTRATION U. S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U. S. HOUSE OF REPRESENTATIVES MARCH 4, 2010 1 Madam Chairman and Members of the Subcommittee, I appreciate the opportunity to testify here today. My name is Steve Wright; I am the Administrator of the Bonneville Power Administration (Bonneville). I am pleased to be here today to discuss the President's Fiscal Year (FY) 2011 Budget as it relates to Bonneville. In my testimony today, I will share with the Committee Bonneville's significant successes over the past year, how we are addressing the considerable challenges we are facing, and an overview of the FY 2011 budget.

94

3-15-11_Final_Testimony_(Wright)_(BPA).pdf  

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

STEPHEN J. WRIGHT STEPHEN J. WRIGHT ADMINISTRATOR BONNEVILLE POWER ADMINISTRATION U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES MARCH 15, 2011 EXAMINING THE SPENDING, PRIORITIES AND THE MISSIONS OF THE BONNEVILLE POWER ADMINISTRATION, THE WESTERN AREA POWER ADMINISTRATION, THE SOUTHWESTERN POWER ADMINISTRATION AND THE SOUTHEASTERN POWER ADMINISTRATION Mr. Chairman and Members of the Subcommittee, I appreciate the opportunity to testify here today. My name is Steve Wright. I am the Administrator of the Bonneville Power Administration (Bonneville). I am pleased to be here today to discuss the President's Fiscal Year (FY) 2012 Budget as it relates to Bonneville. In my testimony today, I will share with the Committee Bonneville's significant

95

October 21, 2003, Board Public Meeting Testimony - Attachment 2  

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

' ' TESTIMONY Kyle E. McSlarrow, Deputy Secretary of Energy Defense Nuclear Facilities Safety Board Public hearing October 21,2003 Thank you, Mr. Chairman, and members of the Board for providing me the opportunity to address you today. In my role as the Deputy Secretary of Energy, I serve as the Department's Chief Operating Officer and have responsibility for providing direction to all DOE organizations, including NNSA. The subject of today's hearing - safety oversight - is a critical component of the Department's management system. The Secretary and I take our responsibility to ensure the Department's missions are performed safely very seriously, and the Secretary has made this clear from his first year in office. For example, the Secretary stated, in remarks at the 2001 Executive Safety

96

October 21, 2003, Board Public Meeting Testimony - Attachment 6  

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

Glenn Podonsky Glenn Podonsky Director, Office of Independent Oversight and Performance Assurance U.S. Department of Energy Before the DFfense Nuclear Facilities Safety Board October 21,2003 Introductory Remarks Thank you, Mr. Chairman, for inviting me to testify today. My office - the Office of Independent Oversight and Performance Assurance - was established by the Secretary of Energy as the independent evaluation element of the Department's integrated oversight system. We are responsible for evaluating environment, safety, and health; emergency management; cyber security; and safeguards and security programs at Department of Energy sites. Consistent with the scope of this hearing, I will focus my testimony today on our safety oversight role. Role of Independent Oversight

97

7-9-09_Final_Testimony_(USJohnson).pdf  

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

KRISTINA M. JOHNSON KRISTINA M. JOHNSON UNDER SECRETARY OF ENERGY U.S. DEPARTMENT OF ENERGY BEFORE THE COMMITTEE ON SCIENCE AND TECHNOLOGY SUBCOMMITTEE ON ENERGY AND ENVIRONMENT U.S. HOUSE OF REPRESENTATIVES JULY 9, 2009 Thank you, Mr. Chairman and Members of the Committee. I appreciate this opportunity to provide testimony on the U.S. Department of Energy's (DOE's) programs for developing water-efficient environmentally-sustainable energy-related technologies and DOE strategies for coordinating these activities. Energy production of all types affects and is affected by the natural water cycle, and increasingly, water-efficient technologies are being developed to reduce these impacts. Interactions with Others/ R&D Selection It is, of course, important to point out that a number of other Federal Agencies also have

98

5-14-09_Final_Testimony_(Vic_Der).pdf  

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

VICTOR K. DER VICTOR K. DER ACTING ASSISTANT SECRETARY OFFICE OF FOSSIL ENERGY U.S. DEPARTMENT OF ENERGY BEFORE THE ENERGY AND NATURAL RESOURCES COMMITTEE UNITED STATES SENATE MAY 14, 2009 Thank you, Mr. Chairman and members of the Committee. I appreciate this opportunity to provide testimony on the United States Department of Energy's (DOE's) research efforts in carbon capture and storage. The Department of Energy has not had an opportunity to fully analyze S. 1013, and therefore, cannot take a position on the bill at this time. INTRODUCTION Fossil fuel resources represent a tremendous national asset. An abundance of fossil fuels in North America has contributed to our Nation's economic prosperity. Based upon current rates of consumption, the United States probably has sufficient coal to meet its need for the next

99

3-10-09_Final_Testimony_(Bauer)_(NETL).pdf  

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

CARL O. BAUER CARL O. BAUER DIRECTOR NATIONAL ENERGY TECHNOLOGY LABORATORY U.S. DEPARTMENT OF ENERGY BEFORE THE ENERGY AND NATURAL RESOURCES COMMITTEE UNITED STATES SENATE MARCH 10, 2009 Thank you, Mr. Chairman and Members of the Committee. I appreciate the opportunity to provide testimony on the U.S. Department of Energy's (DOE's) research program directed at reducing power plant water use as it relates to carbon capture efficiency and optimization. Of particular concern is the potential implication on freshwater requirements in a future in which carbon dioxide (CO 2 ) capture technology is required to be installed on coal-based power systems. DOE's National Energy Technology Laboratory (NETL) projects that, in the absence of successful development of new advanced CO

100

Microsoft Word - 4.16.13 Final WAPA Testimony  

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

STATEMENT OF STATEMENT OF MR. MARK GABRIEL ADMINISTRATOR WESTERN AREA POWER ADMINISTRATION U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES APRIL 16, 2013 EXAMINING THE PROPOSED FISCAL YEAR 2014 SPENDING, PRIORITIES AND THE MISSIONS OF BUREAU OF RECLAMATION, THE FOUR POWER MARKETING ADMINISTRATIONS AND THE U.S.GEOLOGICAL SURVEY'S WATER PROGRAM Thank you, Mr. Chairman and Members of the Committee. My name is Mark Gabriel. I am the new Administrator of the Western Area Power Administration (Western). I am pleased to represent Western today as we discuss Western's portion of the President's Fiscal Year (FY) 2014 Budget. In this testimony, I will highlight Western's accomplishments and progress in delivering clean,

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


101

10-21-09_Final_Testimony_(Klara)_(NETL).pdf  

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

SCOTT M. KLARA SCOTT M. KLARA DIRECTOR, STRATEGIC CENTER FOR COAL NATIONAL ENERGY TECHNOLOGY LABORATORY U.S. DEPARTMENT OF ENERGY HEARING ON "BIOMASS FOR THERMAL ENERGY AND ELECTRICITY: A RESEARCH AND DEVELOPMENT PORTFOLIO FOR THE FUTURE" BEFORE THE COMMITTEE ON SCIENCE AND TECHNOLOGY SUBCOMMITTEE ON ENERGY AND ENVIRONMENT U. S. HOUSE OF REPRESENTATIVES October 21, 2009 Thank you, Mr. Chairman and Members of the Subcommittee. I appreciate this opportunity to provide testimony on the United States Department of Energy's (DOE) Clean Coal Research Program, particularly those activities related to co-feeding biomass materials with coal that reduce the life-cycle carbon intensity of electric power generation and large industrial processes. Biomass can be introduced to our Nation's energy mix as a feedstock input to thermal

102

6-7-11_Final_Testimony_(Kelly).pdf  

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

John E. Kelly John E. Kelly Deputy Assistant Secretary for Reactor Technologies Office of Nuclear Energy U.S. Department of Energy Before the Committee on Energy and Natural Resources U.S. Senate S. 512, the Nuclear Power 2021 Act and S. 1067, the Nuclear Energy Research Initiative Improvement Act June 7, 2011 Introduction Thank you, Chairman Bingaman, Ranking Member Murkowski, and Members of the Committee. This is my first testimony before Congress and it is a particular pleasure to be discussing small modular reactors (SMRs) with you, as they have been an area of great interest to me for some time. Before joining the Department of Energy, I co-chaired an American Nuclear Society special committee that was developing solutions to generic licensing issues for small

103

10-1-09_Final_Testimony_(Kovar).pdf  

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

Dr. Dennis Kovar Associate Director for High Energy Physics Office of Science U.S. Department of Energy Before the Subcommittee on Energy and Environment Committee on Science and Technology U.S. House of Representatives October 1, 2009 Thank you Mr. Chairman, Ranking Member Inglis, and Members of the Committee for the opportunity to appear before you to provide testimony on the High Energy Physics and Nuclear Physics programs in the Department of Energy's (DOE's) Office of Science (SC). I served as Director of the Nuclear Physics program for nine years, from 1998 to October 2007, and I have been Director of the Office of High Energy Physics since October 2007. I am pleased to be here today to share with you my perspectives on these

104

4-28-09_Final_Testimony_(Chalk).pdf  

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

STEVEN CHALK STEVEN CHALK PRINCIPAL DEPUTY ASSISTANT SECRETARY OFFICE OF ENERGY EFFICIENCY AND RENEWABLE ENERGY U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON ENERGY AND ENVIRONMENT COMMITTEE ON SCIENCE AND TECHNOLOGY U.S. HOUSE OF REPRESENTATIVES APRIL 28, 2009 1 Chairman Baird, Ranking Member Inglis, Members of the Subcommittee, thank you for the opportunity to appear before you today to discuss the U.S. Department of Energy's (DOE) Building Technologies Program activities and the enormous potential for energy savings in the buildings sector. I have included, as an appendix to this testimony, an update on the Department's progress in implementing sections of the Energy Policy Act of 2005 (EPACT 05) and the Energy Independence and Security Act of 2007 (EISA), as requested by the

105

October 21, 2003, Board Public Meeting Testimony - Attachment 3  

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

Linton Brooks, Administrator Linton Brooks, Administrator National Nuclear Security Administration W .S. Department of Energy Before the Defense Nuclear Facilities Safety Board October 2 1,2003 Mr. Chairman and Members of the Defense Nuclear Facilities Safety Board, Thank you for this opportunity to provide testimony on the National Nuclear Security Administration's (NNSA) current practices for oversight and management of the contracts and contractors that accomplish the mission assigned to NNSA under the Atomic Energy Act of 1954. We understand that the Board particularly wants to focus on the impact NNSA's reengineering may have on assuring adequate protection of the health and safety of the public and workers at NNSA's defense nuclear facilities. I fully understand my personal responsibility for assuring the safety of NNSA's

106

3-11-09_Final_Testimony_(Der).pdf  

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

VICTOR K. DER VICTOR K. DER ACTING ASSISTANT SECRETARY OFFICE OF FOSSIL ENERGY U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON ENERGY AND ENVIRONMENT COMMITTEE ON SCIENCE AND TECHNOLOGY U.S. HOUSE OF REPRESENTATIVES MARCH 11, 2009 Thank you, Mr. Chairman and Members of the Committee. I appreciate this opportunity to provide testimony on the U.S. Department of Energy's (DOE's) advanced coal research, development, and demonstration program to develop low-carbon emission coal technologies. INTRODUCTION Fossil fuel resources represent a tremendous national asset. An abundance of fossil fuels in North America has contributed to our Nation's economic prosperity. Based upon current rates of consumption, the United States probably has sufficient coal to meet its need for the next

107

My Testimony to the House Energy and Commerce Committee | Department of  

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

My Testimony to the House Energy and Commerce Committee My Testimony to the House Energy and Commerce Committee My Testimony to the House Energy and Commerce Committee November 16, 2011 - 5:38pm Addthis Secretary Chu Secretary Chu Former Secretary of Energy Tomorrow morning, I'll be appearing before the House Energy and Commerce Committee to discuss the choice we face in competing for the clean energy jobs of tomorrow. I know that many of you share my strong feelings on this crucial issue, so I wanted to share my testimony with you. What follows are my remarks, as I have prepared them for delivery: Thank you Chairman Stearns, Ranking Member DeGette, and members of the Subcommittee for the opportunity to speak with you today. Investments in clean energy reached a record $243 billion last year. Solar photovoltaic systems alone represent a global market worth more than $80

108

Cognitive Radio and Smart Grid Dr. Robert C. Qiu  

E-Print Network [OSTI]

Cognitive Radio and Smart Grid Dr. Robert C. Qiu Professor Wireless Networking Systems Laboratory Presented at IEEE Chapter, Huntsville, AL Email: rqiu@tntech.edu http://iweb.tntech.edu/rqiu #12;Cognitive RadioCognitive Radio 2 2/23/2010 #12;Outline Cognitive Radio Cognitive Radio @ Tennessee Tech

Qiu, Robert Caiming

109

Intelligent Spectrum Sensor Radio.  

E-Print Network [OSTI]

??A cognitive radio is a radio with built-in intelligence that makes it able to utilize the radio frequency spectrum more efficiently by adapting to the (more)

Mian, Omer

2008-01-01T23:59:59.000Z

110

Invited Testimony on the Report from the Panama Canal Stakeholder Working Group 1 Texas Senate Transportation Committee  

E-Print Network [OSTI]

Invited Testimony on the Report from the Panama Canal Stakeholder Working Group 1 Texas Senate Transportation Committee Public Hearing December 18, 2012 Invited Testimony Report from the Panama Canal terminals in Texas generated $277 billion in economic value to the state in 2011. The Panama Canal

111

Testimony of Christopher Smith before the House Committee on Energy and  

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

Testimony of Christopher Smith before the House Committee on Energy Testimony of Christopher Smith before the House Committee on Energy and Commerce Testimony of Christopher Smith before the House Committee on Energy and Commerce March 28, 2012 - 1:06pm Addthis Statement of Christopher Smith, Deputy Assistant Secretary for Oil and Natural Gas, Office of Fossil Energy, before the House Committee on Energy and Commerce, Subcommittee on Energy and Power. Chairman Whitfield, Ranking Member Rush, and Members of the subcommittee, thank you for the opportunity to discuss the Department of Energy's (DOE) perspective on two legislative proposals -the discussion drafts of the "Strategic Energy Production Act of 2012" and the "Gasoline Regulations Act of 2012." We share the concern of the Members regarding the burden that the rising

112

UPDATED: Oral Testimony of Energy Secretary Steven Chu at the Subcommittee  

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

Oral Testimony of Energy Secretary Steven Chu at the Oral Testimony of Energy Secretary Steven Chu at the Subcommittee on Energy and Water Development of the House Committee on Appropriations - As Prepared for Delivery UPDATED: Oral Testimony of Energy Secretary Steven Chu at the Subcommittee on Energy and Water Development of the House Committee on Appropriations - As Prepared for Delivery March 15, 2011 - 12:00am Addthis Chairman Frelinghuysen, Mr. Pastor, Chairman Rogers, Ranking Member Dicks, Mr. Visclosky, and Members of the Committee, thank you for the opportunity to discuss the President's Fiscal Year 2012 budget request for the Department of Energy. Your support is critical to our mission, and I look forward to continuing our relationship with this committee. I want to begin by expressing the Administration's support for the people

113

U.S. Distillate Market Testimony for New York Assembly Hearing  

Gasoline and Diesel Fuel Update (EIA)

Market Testimony for New York Assembly Hearing Market Testimony for New York Assembly Hearing 2/4/2000 Click here to start Table of Contents U.S. Distillate Market Testimony for New York Assembly Hearing U.S. Residential Heating Oil Prices Regional Residential Heating Oil Prices Selected State Residential Heating Oil Prices Spot Distillate & Crude Oil Prices (Prices thru Jan 31, 2000) Low Distillate Stocks Set Stage for Price Volatility PADD 1 (East Coast) Heating Oil Stocks Low New England & Mid-Atlantic Weekly Total Distillate Stocks Low World Crude Production Not Keeping Pace with Demand OECD Stocks Reflect S/D Imbalance Distillate Stocks Are Important Part of Northeast Winter Supply Distillate Problem Likely to be Resolved Soon, But Recurrence Possible East Coast Distillate Production

114

Testimony of Jonathan Silver, Executive Director Loan Programs Office, U.S.  

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

Testimony of Jonathan Silver, Executive Director Loan Programs Testimony of Jonathan Silver, Executive Director Loan Programs Office, U.S. Department of Energy Before the Subcommittee on Oversight and Investigations Committee on Energy and Commerce U.S. House of Representatives Testimony of Jonathan Silver, Executive Director Loan Programs Office, U.S. Department of Energy Before the Subcommittee on Oversight and Investigations Committee on Energy and Commerce U.S. House of Representatives September 14, 2011 - 12:01am Addthis As prepared for delivery Thank you Chairman Stearns, Ranking Member DeGette, and members of the Subcommittee. My name is Jonathan Silver, and I have served as Executive Director of the Loan Programs Office at the Department of Energy since November 2009. For most of my career, I have worked in the private sector, analyzing,

115

Oral Testimony of Energy Secretary Steven Chu at the House Energy and  

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

Oral Testimony of Energy Secretary Steven Chu at the House Energy Oral Testimony of Energy Secretary Steven Chu at the House Energy and Commerce Committee - As Prepared for Delivery Oral Testimony of Energy Secretary Steven Chu at the House Energy and Commerce Committee - As Prepared for Delivery March 16, 2011 - 12:00am Addthis Chairman Upton, Ranking Member Waxman, Mr. Barton, Mr. Dingell and Members of the Committee, thank you for the opportunity to discuss the President's Fiscal Year 2012 budget request for the Department of Energy. I want to begin by expressing the Administration's support for the people of Japan, as well as American citizens in Japan, as they respond to and recover from the tragic events of the past few days. Officials from the Department of Energy, the Nuclear Regulatory Commission, and other agencies have maintained close contact with Japanese officials

116

Radio Data  

Science Journals Connector (OSTI)

... abacs provided now cover wave-lengths down to five metres, while provision is made for audio-frequencies over the range 20-10,000 cycles a second. This publication contains a ... the means for obtaining the inductance, capacitance and reactance of coils and condensers at both audio- and radio-frequencies, charts are given for obtaining the efficiency and time constant of ...

1935-12-21T23:59:59.000Z

117

Radio Monitoring Birds of Prey  

Science Journals Connector (OSTI)

Abstract This paper is a consideration of field techniques rather than of equipment design. The first of three parts reviews applications of radio monitoring in bird of prey studies, with suggestions concerning terminology. There has been some radio telemetry of activity and incubation parameters, but most monitoring of raptors has involved radio tracking. This has included location of birds for investigation of movements, ranges, habitat utilization and roost sites, but could also be used for surveillance of what birds were doing. The second section describes techniques used in radio surveillance of a particularly secretive raptor, the goshawk, and presents original data on prey selection which were collected during studies of predation on woodpigeons and pheasants. Finally, there is an outline of how selection data were combined with predation rate measurements and hawk density estimates, obtained using radio tags as a Lincoln Index marker during hawk sightings, to determine the impact of predation on these economically important prey.

R.E. KENWARD

1980-01-01T23:59:59.000Z

118

Testimony Regarding Fiscal Year 2012 Funding for Federal Science and Technology Programs  

E-Print Network [OSTI]

necessary than ever. Federally-funded scientific research and development (R&D) produces innovationsTestimony Regarding Fiscal Year 2012 Funding for Federal Science and Technology Programs Submitted of delivering energy, food, and water in more sustainable ways. In short, NSF, NASA and NOAA help meet

119

Testimony on the Role of Marine Freight Transportation in the Economic  

E-Print Network [OSTI]

economies · How using marine transportation can possibly reduce "wear and tear" of the state's highways 1 Testimony on the Role of Marine Freight Transportation in the Economic Development concerning aspects of the role of marine freight transportation in the economic development of the State

120

United States Senate Committee on Indian Affairs Testimony for the September 18, 2009 Roundtable on  

E-Print Network [OSTI]

(RAEL) has experience in the design and implementation of clean energy building systems (both new to energy, marine energy, wind and hydro power) in over 20 countries (detailed online at http and implement low-carbon, pro- growth energy and economic plans. In the case of this testimony I am truly

Kammen, Daniel M.

Note: This page contains sample records for the topic "testimony presentations radio" 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

Ocean conditions and Columbia River salmon Testimony provided for the House Subcommittee on Power and Water  

E-Print Network [OSTI]

Ocean conditions and Columbia River salmon Testimony provided for the House Subcommittee on Power Institute for the Study of the Atmosphere and Oceans/School of Marine Affairs Climate Impacts Group Box controlling salmon marine survival in the Pacific Northwest, several ocean-climate events have been linked

Mantua, Nathan

122

Testimony of Dr. Stewart C. Prager Director, Princeton Plasma Physics Laboratory  

E-Print Network [OSTI]

1 Testimony of Dr. Stewart C. Prager Director, Princeton Plasma Physics Laboratory you for this opportunity to discuss fusion energy. I am Director of the Princeton Plasma Physics Laboratory ­ a Department of Energy national lab, managed by Princeton University, dedicated

123

Non-thermal radio astronomy  

Science Journals Connector (OSTI)

Abstract This presentation starts with Karl Janskys discovery of cosmic radio emission in 1933 and notes the striking similarities to Hesss discovery of cosmic-rays in 1912. At first it was assumed that this radio emission was thermal but in 1939 Grote Reber discovered that it was stronger at longer wavelengths, requiring a non-thermal emission process. These discoveries had a revolutionary impact on astronomy and radio astronomy was born. The interpretation of this non-thermal radiation as synchrotron emission from high energy particles in the interstellar medium did not occur until the late 1940s but then it provided the link between radio astronomy and cosmic-ray research. Ginzburg, in particular, saw that cosmic-ray astrophysics was now possible using radio waves to trace sources of cosmic-rays. We discuss the discovery of extragalactic active galactic nuclei leading to the discovery of quasars and the first evidence for black holes in the nuclei of galaxies. We summarise the present status and future of some of the main radio telescopes used to image the non-thermal emission from external galaxies. Finally, we include a short description of the use of radio signals for the direct detection of cosmic-rays and UHE neutrinos.

R.D. Ekers

2014-01-01T23:59:59.000Z

124

Recycling for radio astronomy  

Science Journals Connector (OSTI)

......research-article Features Recycling for radio astronomy Melvin Hoare Professor of Astrophysics at the...space missions, carry out single-dish radio astronomy and boost existing radio-astronomy interferometer arrays, objectives that bring......

Melvin Hoare

2012-02-01T23:59:59.000Z

125

PREPARED TESTIMONY OF ROBERT B. WEISENMILLER, PH.D. Qualifying Facilities: Resource Planning and Avoided Costs Methodology ................................ 1  

E-Print Network [OSTI]

Planning and Avoided Costs Methodology ................................ 1 Energy and Capacity Payments............................................................................. 15 Qualifying Facilities: Resource Planning and Avoided Costs Methodology 1. CPUC Order Instituting Testimony on Long Run Avoided Cost Methodology for the California Manufacturers Association, Department

126

Secretary Chu's Testimony to the Senate Committee on Environment and Public  

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

the Senate Committee on Environment the Senate Committee on Environment and Public Works - As Prepared for Delivery Secretary Chu's Testimony to the Senate Committee on Environment and Public Works - As Prepared for Delivery October 27, 2009 - 12:00am Addthis Washington, DC -- Secretary Steven Chu testified this morning before the Senate Committee on Environment and Public Works on S. 1733, the Clean Energy Jobs and American Power Act. His prepared testimony is below: Chairman Boxer, Ranking Member Inhofe, Members of the Committee, thank you for the opportunity to testify today. When I appeared before you in July, I focused on the energy challenge and the grave threat from climate change. The Intergovernmental Panel on Climate Change found in 2007 that the best estimate for the rise in average

127

Planck early results: Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources  

E-Print Network [OSTI]

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact Source Catalog (ERCSC) and simultaneous multifrequency data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous observations ranging from radio to gamma-rays. This is the first extensive frequency coverage in the radio and millimetre domains for an essentially complete sample of extragalactic radio sources, and it shows how the individual shocks, each in their own phase of development, moving in the relativistic jet, shape the radio spectra. The SEDs presented in this paper were fitted with second and third degree polynomials to estimate the frequencies of the synchrotron and inverse Compton (IC) peaks, and the spectral indices of low and high frequency radio data, including the Planck ERCSC data, were calculated. SED modelling methods are discussed, with an emphasis on proper, physical modelli...

Aatrokoski, J; Aghanim, N; Aller, H D; Aller, M F; Angelakis, E; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Balbi, A; Banday, A J; Barreiro, R B; Bartlett, J G; Battaner, E; Benabed, K; Benot, A; Berdyugin, A; Bernard, J -P; Bersanelli, M; Bhatia, R; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Burrows, D N; Cabella, P; Capalbi, M; Cappellini, B; Cardoso, J -F; Catalano, A; Cavazzuti, E; Cayn, L; Challinor, A; Chamballu, A; Chary, R -R; Chiang, L -Y; Christensen, P R; Clements, D L; Colafrancesco, S; Colombi, S; Couchot, F; Coulais, A; Cutini, S; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Gasperis, G; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Dickinson, C; Dole, H; Donzelli, S; Dor, O; Drl, U; Douspis, M; Dupac, X; Efstathiou, G; Enlin, T A; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Fuhrmann, L; Galeotta, S; Ganga, K; Gargano, F; Gasparrini, D; Gehrels, N; Giard, M; Giardino, G; Giglietto, N; Giommi, P; Giordano, F; Giraud-Hraud, Y; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Harrison, D; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hovest, W; Hoyland, R J; Huffenberger, K M; Jaffe, A H; Juvela, M; Keihnen, E; Keskitalo, R; King, O; Kisner, T S; Kneissl, R; Knox, L; Krichbaum, T P; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Laureijs, R J; Lavonen, N; Lawrence, C R; Leach, S; Leonardi, R; Len-Tavares, J; Linden-V\\ornle, M; Lindfors, E; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maffei, B; Maino, D; Mandolesi, N; Mann, R; Maris, M; Martnez-Gonzlez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Max-Moerbeck, W; Mazziotta, M N; Mazzotta, P; Melchiorri, A; Mendes, L; Mennella, A; Michelson, P F; Mingaliev, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Monte, C; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, A; Naselsky, P; Natoli, P; Nestoras, I; Netterfield, C B; Nieppola, E; Nilsson, K; N\\orgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; O'Dwyer, I J; Osborne, S; Pajot, F; Partridge, B; Pasian, F; Patanchon, G; Pavlidou, V; Pearson, T J; Perdereau, O; Perotto, L; Perri, M; Perrotta, F; Piacentini, F; Piat, M; Plaszczynski, S; Platania, P; Pointecouteau, E; Polenta, G; Ponthieu, N; Poutanen, T; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rain, S; Reach, W T; Readhead, A; Rebolo, R; Reeves, R; Reinecke, M; Reinthal, R; Renault, C; Ricciardi, S; Richards, J; Riller, T; Riquelme, D; Ristorcelli, I; Rocha, G; Rosset, C; Rowan-Robinson, M; Rubi\; Rusholme, B; Saarinen, J; Sandri, M; Savolainen, P; Scott, D; Seiffert, M D; Sievers, A; Sillanp, A; Smoot, G F; Sotnikova, Y; Starck, J -L; Stevenson, M; Stivoli, F; Stolyarov, V; Sudiwala, R; Sygnet, J -F; Takalo, L; Tammi, J; Tauber, J A; Terenzi, L; Thompson, D J; Toffolatti, L; Tomasi, M; Tornikoski, M; Torre, J -P; Tosti, G; Tramacere, A; Tristram, M; Tuovinen, J; Trler, M; Turunen, M; Umana, G; Ungerechts, H; Valenziano, L; Valtaoja, E; Varis, J; Verrecchia, F; Vielva, P; Villa, F; Vittorio, N; Wandelt, B D; Wu, J; Yvon, D; Zacchei, A; Zensus, J A; Zhou, X; Zonca, A

2011-01-01T23:59:59.000Z

128

Outline of Radio Astronomy  

Science Journals Connector (OSTI)

... about when a technique developed for one type of investigation is applied to another. Radio astronomy is an excellent example of this. During the past seven years the use of ... radio stars' which emit strongly in the radio-frequency portion of the spectrum."Radio Astronomy", by A. C. B. Lovell and J. A. Clegg, gives an ...

J. A. RATCLIFFE

1953-07-11T23:59:59.000Z

129

MULTIMOMENT RADIO TRANSIENT DETECTION  

SciTech Connect (OSTI)

We present a multimoment technique for signal classification and apply it to the detection of fast radio transients in incoherently dedispersed data. Specifically, we define a spectral modulation index in terms of the fractional variation in intensity across a spectrum. A signal whose intensity is distributed evenly across the entire band has a lower modulation index than a spectrum whose intensity is localized in a single channel. We are interested in broadband pulses and use the modulation index to excise narrowband radio frequency interference by applying a modulation index threshold above which candidate events are removed. The technique is tested both with simulations and using data from known sources of radio pulses (RRAT J1928+15 and giant pulses from the Crab pulsar). The method is generalized to coherent dedispersion, image cubes, and astrophysical narrowband signals that are steady in time. We suggest that the modulation index, along with other statistics using higher order moments, should be incorporated into signal detection pipelines to characterize and classify signals.

Spitler, L. G.; Cordes, J. M.; Chatterjee, S. [Astronomy Department and NAIC, Cornell University, Ithaca, NY 14853 (United States); Stone, J., E-mail: lspitler@astro.cornell.edu [Department of Physics and Astronomy, Barnard College, New York, NY 10027 (United States)

2012-04-01T23:59:59.000Z

130

Software-defined Radio based Wireless Tomography: Experimental Demonstration and  

E-Print Network [OSTI]

1 Software-defined Radio based Wireless Tomography: Experimental Demonstration and Verification presents an experimental demonstration of Software-Defined Radio (SDR) based wireless tomography us- ing follows our vision and previous theoretical study of wireless tomography which combines wireless

Qiu, Robert Caiming

131

Secretary Moniz's Written Testimony on the President's FY2016 Budget Before the U.S. House of Representatives Committee on Energy and Commerce Subcommittee on Energy and Power  

Broader source: Energy.gov [DOE]

Secretary Moniz's written testimony on the budget before the House Committee on Energy and Commerce, Energy and Power Subcommittee on February 11, 2015.

132

Deputy Assistant Secretary Matt Moury's Written Testimony Before the Subcommittee on Financial and Contracting Oversight Committee on Homeland Security and Government Affairs (March 11, 2014)  

Broader source: Energy.gov [DOE]

Written statement of Deputy Assistant Secretary Matt Moury's Written Testimony Before the Subcommittee on Financial and Contracting Oversight Committee on Homeland Security and Government Affairs...

133

Energy Efficient Radio Resource  

E-Print Network [OSTI]

Energy Efficient Radio Resource Management in a Coordinated Multi-Cell Distributed Antenna System Omer HALILOGLU Introduction System Model Performance Evaluation Conclusion References Energy Efficient Hacettepe University 5 September 2014 Omer HALILOGLU (Hacettepe University) Energy Efficient Radio Resource

Yanikomeroglu, Halim

134

Radio Research During 1959  

Science Journals Connector (OSTI)

... range of work carried out at the Radio Research Station, Slough, and at the substation in Singapore*.

W. J. G. BEYNON

1961-02-18T23:59:59.000Z

135

Intelligent Radio Frequency (RF) Monitoring  

E-Print Network [OSTI]

? Intelligent Radio Frequency (RF) Monitoring ? 2009 Armstrong International, Inc. www.armstronginternational.com 2 ?Expect many enjoyable experiences!? David M. Armstrong Present Process Challenges ? Identifying a failure ? Procedure.... Armstrong Steam Trap Challenges ? Identifying a failure ? Manpower ? Location ? Magnitude of failure ? Energy loss ? Loss of heat transfer ? Justification for repair ? ?Speed of Implementation? ? Environmental concerns Manpower Location 4...

Kimbrough, B.

136

Success for radio astronomy  

Science Journals Connector (OSTI)

......August 2000 news News Success for radio astronomy Jim Cohen of Jodrell Bank Observatory...mm-wave spectrum. As a result, radio astronomy is now officially allocated most of the...International Mobile Telecommunications). Radio astronomy made its gains in the mm-wave region......

Jim Cohen

2000-08-01T23:59:59.000Z

137

4-22-09_Final_Testimony_(Triay).pdf  

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

Inés Triay Inés Triay Acting Assistant Secretary for Environmental Management United States Department of Energy Before the Subcommittee on Strategic Forces Committee on Armed Services United States Senate April 22, 2009 Good morning, Chairman Nelson and Members of the Subcommittee. I am pleased to be here today to answer your questions on the integration of American Recovery and Reinvestment Act of 2009 (Recovery Act) funding within the Department of Energy's Office of Environmental Management (EM) program. As you are aware, in January 2009, the Department completed and presented to Congress a comprehensive report assessing initiatives to accelerate the reduction of environmental risks and challenges posed by the legacy of the Cold War. The report, "Status of Environmental

138

5-19-09_Final_Testimony_(Chu).pdf  

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

Steven Chu Steven Chu Secretary, U.S. Department of Energy Before the Senate Committee on Appropriations Subcommittee on Energy and Water Development, and Related Agencies FY 2010 Appropriations Hearing May 19, 2009 Chairman Dorgan, Ranking Member Bennett, members of the Committee, I am pleased to be before you today to present President Obama's fiscal year 2010 budget request for the Department of Energy. The President's 2010 Budget seeks to usher in a new era of responsibility - an era in which we invest to create new jobs and lift our economy out of recession, while laying a new foundation for our long-term growth and prosperity. The FY 2010 budget request of $26.4 billion provides the next critical investment in a multi-year effort to address the interconnected challenges of economic uncertainty,

139

8-3-09_Final_Testimony_(Simpson).pdf  

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

EDWARD R. SIMPSON EDWARD R. SIMPSON DIRECTOR, OFFICE OF PROCUREMENT AND ASSISTANCE MANAGEMENT U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON FEDERAL FINANCIAL MANAGEMENT, GOVERNMENT INFORMATION, FEDERAL SERVICES, AND INTERNATIONAL SECURITY COMMITTEE ON HOMELAND SECURITY AND GOVERNMENTAL AFFAIRS UNITED STATES SENATE AUGUST 3, 2009 Mr. Chairman, and members of the Committee, thank you for the opportunity to come before you today to present the Department of Energy's (DOE) views and perspectives on the recent U.S. Government Accountability Office Report entitled "Federal Contracting: Guidance on Award Fees Has Led to Better Practices but is Not Consistently Applied" (GAO-09-630). I am pleased to be here today to address how the Department is effectively using cost-plus-award-fee contracts to incentivize excellent

140

December 3, 2003, Board Public Meeting Speaker Presentations  

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

7 7 TESTIMONY Daniel E. Glenn, Manager Pantex Site Office National Nuclear Security Administration U. S. Department of Energy Before the Defense Nuclear Facilities Safety Board December 3 and 4, 2003 Mr. Chairman and Members of the Defense Nuclear Facilities Safety Board, Thank you for this opportunity to provide testimony on the Pantex Site Office's (PXSO) current practices for oversight and management of the Management and Operating contractor activities at the Pantex Plant. Transition from the long-standing roles and responsibilities to the re-engineered NNSA presents some challenges, but these changes are needed as we strive to improve the effectiveness, efficiency, and most importantly the safety of our site operations. I fully support the NNSA Reengineering effort and believe that appropriate level of Contractor

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


141

Mills 2.2.00 Testimony before Subcommittee on National Economic Growth, Natural Resources, and Regulatory Affairs  

E-Print Network [OSTI]

, and Regulatory Affairs "Kyoto and the Internet: The Energy Implications of the Digital Economy" Testimony of Mark P. Mills Science Advisor, The Greening Earth Society Senior Fellow, The Competitive Enterprise. Chairman and distinguished Members of the Subcommittee for inviting me to speak about the energy

142

Testimony of R. E. Smalley to the Senate Committee on Energy and Natural Resources; Hearing on sustainable , low emission,  

E-Print Network [OSTI]

, for example, hundreds of gigawatts of electrical power to be transported from solar farms in New Mexico1 Testimony of R. E. Smalley to the Senate Committee on Energy and Natural Resources; Hearing on sustainable , low emission, electricity generation, April 27, 2004 Energy is the single most important

143

Hoffman Testimony  

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

R&D, Office of Electricity Delivery & Energy Reliability R&D, Office of Electricity Delivery & Energy Reliability Department of Energy Committee on Science and Technology Energy and Environment Subcommittee U.S. House of Representatives October 3, 2007 Mr. Chairman and Members of the Subcommittee thank you for this opportunity to testify on behalf of the Department of Energy (DOE) on "Energy Storage Technologies: State of Development for Stationary and Vehicular Applications." The Department of Energy places great emphasis on the promise of energy storage and is researching a variety of storage technologies. Within DOE, applied research into energy storage technologies primarily occurs within two offices: the Office of Energy Efficiency and Renewable Energy (EERE) and the Office of Electricity Delivery and Energy

144

Hoffman Testimony  

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

of R&D and Acting Chief Operating Officer of R&D and Acting Chief Operating Officer Office of Electricity Delivery & Energy Reliability Department of Energy Committee on Energy and Natural Resources United States Senate November 6, 2007 Mr. Chairman and Members of the Committee, thank you for this opportunity to testify on behalf of the Department of Energy (DOE) on the nation's domestic energy sector workforce. Our nation's technical workforce is the backbone of our economy. These individuals have accumulated a wealth of experience and knowledge that cannot be duplicated overnight. If America is to remain the world's leader in science and technology and continue to lead the world in energy innovation, the energy industry needs to invest in a vibrant workforce. Given looming retirements in the energy workforce, success in ensuring America's future

145

THE COMPACT RADIO STRUCTURE OF RADIO-LOUD NARROW LINE SEYFERT 1 GALAXIES  

SciTech Connect (OSTI)

We present the compact radio structure of three radio-loud narrow line Seyfert 1 galaxies from the Very Long Baseline Array archive data at 2.3, 5, and 8.4 GHz. In RXS J16290+4007, the radio structure is mostly unresolved. The combination of compact radio structure, high brightness temperature, and inverted spectrum between simultaneous 2.3 and 8.4 GHz strongly favors jet relativistic beaming. Combined with the very long baseline interferometry data at 1.6 and 8.4 GHz from the literature, we argue that RXS J16333+4718 also may harbor a relativistic jet, with resolved core-jet structure in 5 GHz. B3 1702+457 is clearly resolved with a well-defined jet component. The overall radio steep spectrum indicates that B3 1702+457 is likely a source optically defined as NLS1 with radio definition of compact steep spectrum sources. From these three sources, we found that radio loud NLS1s can be either intrinsically radio loud (e.g., B3 1702+457) or apparently radio loud due to jet beaming effects (e.g., RXS J16290+4007 and RXS J16333+4718).

Gu Minfeng; Chen Yongjun, E-mail: gumf@shao.ac.c [Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030 (China)

2010-06-15T23:59:59.000Z

146

EIA Radio test  

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

September 10, 2012 September 10, 2012 Test of Energy News Radio Service This is a test audio file of the U.S. Energy Information Administration's energy news radio service to be launched on Tuesday, September 11 th with the release of EIA's monthly Short-Term Energy Outlook. EIA's radio service will provide free short broadcast stories on EIA energy data reports and analysis to radio stations nationwide. The stories will be recorded in MP3 format and can be downloaded from EIA's radio service webpage at www.eia.gov/radio. The first broadcast stories will be posted around noon Eastern Time on Sept. 11 after the release of EIA's monthly Short Term Energy Outlook forecast. These initial stories will focus on the outlook for U.S. gasoline prices, crude oil production and natural gas production.

147

Baruch Plan Presented | National Nuclear Security Administration  

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

Baruch Plan Presented | National Nuclear Security Administration Baruch Plan Presented | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > About Us > Our History > NNSA Timeline > Baruch Plan Presented Baruch Plan Presented June 14, 1946 New York, NY Baruch Plan Presented Bernard Baruch presents the American plan for international control of

148

Solar Radio Burst Effects on Global Positioning System Receivers .  

E-Print Network [OSTI]

??This thesis presents a series of studies investigating solar radio burst effects on Global Positioning System (GPS) receivers along with supporting instrumentation and analysis techniques. (more)

Cerruti, Alessandro Paolo

2007-01-01T23:59:59.000Z

149

Microsoft Word - FINAL Testimony - Gregory H Friedman - March 19 2009.doc  

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

Statement of Gregory H. Friedman Statement of Gregory H. Friedman Inspector General U.S. Department of Energy Before the Subcommittee on Investigations and Oversight Committee on Science and Technology U.S. House of Representatives FOR RELEASE ON DELIVERY 10:00 AM March 19, 2009 1 Mr. Chairman and Members of the Subcommittee: I appreciate the opportunity to testify today on accountability and transparency issues related to the American Recovery and Reinvestment Act of 2009 (Recovery Act). My testimony focuses on the efforts of my office to provide effective oversight of Recovery Act funds at the Department of Energy, which will receive approximately $40 billion for various science, energy, and environmental programs and initiatives. Furthermore, based on the Recovery Act and

150

Microsoft Word - 9-22-11 Final Testimony _Delwiche_ _BPA Statement for the Record_.doc  

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

GREGORY K. DELWICHE GREGORY K. DELWICHE SENIOR VICE PRESIDENT OF POWER SERVICES BONNEVILLE POWER ADMINISTRATION BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES SEPTEMBER 22, 2011 Mr. Chairman and Members of the Committee, I appreciate the opportunity to offer this statement regarding H.R. 1719 which would, if enacted, direct the Administrators of the Federal Power Marketing Administrations (PMA) to include on customers' monthly bills information about the costs the PMAs are incurring to comply with the Endangered Species Act (ESA). This statement is similar to my testimony provided on March 16, 2006 (H.R. 4857). ESA compliance costs incurred by Bonneville Power Administration (Bonneville) include the power share of debt service and operations and maintenance expense for fish passage facilities at

151

Frequencies for Radio Astronomy  

Science Journals Connector (OSTI)

... must therefore be achieved through the combined action of three international scientific unions, IAU (astronomy), COSPAR (space) and URSI (radio), which jointly delegate members to an ... jointly delegate members to an Inter-Union Commission for the Allocation of Frequencies for Radio Astronomy and Space Science (IUCAF). This Commission discusses the scientific case for protecting various ...

F. G. SMITH

1970-10-31T23:59:59.000Z

152

Telecommunications Radio Lease  

E-Print Network [OSTI]

Telecommunications Radio Lease 1. Fax completed form to 979.847.1111. 2. If you do not receive to any of the radios, chargers and accessories until signed back over to the Telecommunications office Telecommunications Office Use Only Service Due Date Installation Cost (NRC) Billed To Telephone/Circuit Number

153

Telecommunications Radio Rental  

E-Print Network [OSTI]

Telecommunications Radio Rental 1. Fax completed form to 979.847.1111. 2. If you do not receive of the radios, chargers and accessories until signed back over to the Telecommunications office. Amount Work Order Prepared Departmental Approval Signature Date Service Date Desired Telecommunications Office

154

Stabilized radio frequency quadrupole  

DOE Patents [OSTI]

Disclosed is a long-vane stabilized radio frequency resonator for accelerating charged particles and including means defining a radio frequency resonator cavity, a plurality of long vanes mounted in the defining means for dividing the cavity into sections, and means interconnecting opposing ones of the plurality of vanes for stabilizing the resonator. 5 figs.

Lancaster, H.D.; Fugitt, J.A.; Howard, D.R.

1984-12-25T23:59:59.000Z

155

Smart Radio Spectrum Management for Cognitive Radio  

E-Print Network [OSTI]

Today's wireless networks are characterized by fixed spectrum assignment policy. The limited available spectrum and the inefficiency in the spectrum usage necessitate a new communication paradigm to exploit the existing wireless spectrum opportunistically. Cognitive radio is a paradigm for wireless communication in which either a network or a wireless node changes its transmission or reception parameters to communicate efficiently avoiding interference with licensed or unlicensed users. In this work, a fuzzy logic based system for spectrum management is proposed where the radio can share unused spectrum depending on some parameters like distance, signal strength, node velocity and availability of unused spectrum. The system is simulated and is found to give satisfactory results.

Bhattacharya, Partha Pratim; Gera, Rishita; Agarwal, Anjali

2011-01-01T23:59:59.000Z

156

Need a Classroom Stimulus? Introduce Radio Astronomy  

Science Journals Connector (OSTI)

Silently invisibly ceaselessly our planet Earth is showered by radio waves from every direction and from every region of space. This radio energy originates in our solar system throughout the Milky Way galaxy and far beyond out to the remotest reaches of the universe. Detecting and unraveling the origins of these invisible signals is what radio astronomy is all about. This ever?present radiation provides astronomers with an alternate non?optical window to the universe revealing exotic and unfamiliar phenomena previously undetected by even the most powerful optical telescopes. For physics teachers a classroom discussion of these radio discoveries however brief offers an opportunity for igniting interest (and possibly a career option) in even the most apathetic of students. This paper describes first the background of some of these events and second (in the appendixes) a selection of numerical problems so that students can derive for themselves the truly mind?stretching features of these celestial objects.

Samuel Derman

2010-01-01T23:59:59.000Z

157

On the black-hole mass -- radio luminosity relation for flat-spectrum radio-loud quasars  

E-Print Network [OSTI]

A new analysis of the connection between black-hole mass and radio luminosity in radio-selected flat-spectrum quasars (FSQ) is presented. In contrast to recent claims in the literature, we find no evidence that the black-hole masses of radio-selected FSQ are systematically lower that those of luminous optically-selected radio-loud quasars. The black-hole masses of the FSQ are estimated via the virial black-hole mass estimator which utilizes the line-width of the H$\\beta$ emission line as a tracer of the central gravitational potential. By correcting for the inevitable effects of inclination, incurred due to the FSQ being viewed close to the line of sight, we find that the black-hole masses of the FSQ with intrinsically powerful radio jets are confined, virtually exclusively, to M_bh > 10^8 M_solar. This is in good agreement with previous studies of optically selected FSQ and steep-spectrum radio-loud quasars. Finally, following the application of a realistic Doppler boosting correction, we find that the FSQ occupy a wide range in intrinsic radio luminosity, and that many sources would be more accurately classified as radio-intermediate or radio-quiet quasars. This range in radio luminosity suggests that the FSQ are fully consistent with an upper boundary on radio power of the form L_5GHz \\propto M_bh^2.5.

Matt J. Jarvis; Ross J. McLure

2002-08-21T23:59:59.000Z

158

Conference on Advances in Materials Science - Presentations | National  

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

in Materials Science - Presentations | National in Materials Science - Presentations | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Feature Bottom Conference on Advances in Materials Science - Presentations Home > About Us > Our Programs > Defense Programs > Future Science & Technology Programs > Office of Advanced Simulation and Computing and

159

Conference on Advances in Materials Science - Presentations | National  

National Nuclear Security Administration (NNSA)

in Materials Science - Presentations | National in Materials Science - Presentations | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Feature Bottom Conference on Advances in Materials Science - Presentations Home > About Us > Our Programs > Defense Programs > Future Science & Technology Programs > Office of Advanced Simulation and Computing and

160

Abell 1033: birth of a radio phoenix  

E-Print Network [OSTI]

Extended steep-spectrum radio emission in a galaxy cluster is usually associated with a recent merger. However, given the complex scenario of galaxy cluster mergers, many of the discovered sources hardly fit into the strict boundaries of a precise taxonomy. This is especially true for radio phoenixes that do not have very well defined observational criteria. Radio phoenixes are aged radio galaxy lobes whose emission is reactivated by compression or other mechanisms. Here, we present the detection of a radio phoenix close to the moment of its formation. The source is located in Abell 1033, a peculiar galaxy cluster which underwent a recent merger. To support our claim, we present unpublished Westerbork Synthesis Radio Telescope and Chandra observations together with archival data from the Very Large Array and the Sloan Digital Sky Survey. We discover the presence of two sub-clusters displaced along the N-S direction. The two sub-clusters probably underwent a recent merger which is the cause of a moderately per...

de Gasperin, F; van Weeren, R J; Dawson, W A; Brggen, M; Bonafede, A; Simionescu, A

2015-01-01T23:59:59.000Z

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


161

A SAMPLE OF CANDIDATE RADIO STARS IN FIRST AND SDSS  

SciTech Connect (OSTI)

We conduct a search for radio stars by combining radio and optical data from the FIRST survey and the Sloan Digital Sky Survey (SDSS). The faint limit of SDSS makes possible a homogeneous search for radio emission from stars of low optical luminosity. We select a sample of 112 candidate radio stars in the magnitude range 15 < i {approx}< 19.1 and with radio flux S {sub 20} {>=} 1.25 mJy, from about 7000 deg{sup 2} of sky. The selection criteria are positional coincidence within 1'', radio and optical point source morphology, and an SDSS spectrum classified as stellar. The sample contamination is estimated by random matching to be 108 {+-} 13, suggesting that at most a small fraction of the selected candidates are genuine radio stars. Therefore, we rule out a very rare population of extremely radio-loud stars: no more than 1.2 of every million stars in the magnitude range 15 < i < 19.1 stars has radio flux S {sub 20} {>=} 1.25 mJy. We investigate the optical and radio colors of the sample to find candidates that show the largest likelihood of being real radio stars. The significant outliers from the stellar locus, as well as the magnetically active stars, are the best candidates for follow-up radio observations. We conclude that, while the present wide-area radio surveys are not sensitive enough to provide homogeneous samples of the extremely rare radio stars, upcoming surveys that exploit the great sensitivity of current and planned telescopes do have sufficient sensitivity and will allow the properties of this class of object to be investigated in detail.

Kimball, Amy E.; Ivezic, Zeljko; Plotkin, Richard M. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195-1580 (United States); Knapp, Gillian R.; Gordon, Michael S. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); West, Andrew A.; Bochanski, John J. [Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)], E-mail: akimball@astro.washington.edu

2009-08-10T23:59:59.000Z

162

Low Cost Radio Telescope  

Science Journals Connector (OSTI)

A radio interferometer has been constructed at Haverford College as an aid to learning the fundamentals of radio astronomy. Its cost both in cash outlay and in construction time make it a feasible year-long project for an undergraduate. Its simplicity does not prevent it from being a useful instrument for instruction at the college or high-school level; among its capabilities are the measurement of the positions of at least four of the strongest discrete cosmic-noisesources and the diameter of the radio sun.

Joseph H. Taylor Jr.

1964-01-01T23:59:59.000Z

163

CRAF Handbook for Radio Astronomy  

E-Print Network [OSTI]

CRAF Handbook for Radio Astronomy EUROPEAN SCIENCE FOUNDATION Committee on Radio Astronomy. It represents all scientific disciplines: physical and engineering sciences, life, earth and environmental Handbook for Radio Astronomy, 3rd edition". #12;CRAF Handbook for Radio Astronomy Edited by Jim Cohen

Rodriguez, Luis F.

164

NIOSH testimony on Kuwait before the subcommittee on hospitals and health care, committee on veterans' affairs by J. S. Andrews, September 16, 1992  

SciTech Connect (OSTI)

The testimony summarizes potential adverse health effects related to service in the Persian Gulf as presented by the Department of Health and Human Services. An estimated 9,000 workers from 43 different countries battled the burning oil wells in Kuwait from February 1991 through early November 1991 when the last was capped. Exposures and health effects in US military personnel, Kuwaiti citizens, and fire fighters were described. The hazards to the soldiers were largely dependent on the concentration of the pollutants in the air near the camps. Fortunately, the plume from the fires rose up to 10,000 and 12,000 feet, mixed with the air and then dispersed for several thousand miles downwind over a period of several weeks. The particles and gases contained in the plume were diluted as the plume travelled. Even so, some minor respiratory problems were present among the soldiers. Some of the hydrocarbons measured at low concentrations have been shown to produce cancer in laboratory animals only when present at higher levels of exposure. Based on the exposure information gathered, the author concludes that there will not likely be a detectable increase in lung cancer in Gulf War Veterans as a result of the oil well fires.

Not Available

1992-09-16T23:59:59.000Z

165

Radio and Spectrum Management | Department of Energy  

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

Radio and Spectrum Management Radio and Spectrum Management DOE Radio and Spectrum Workshop 43.pdf More Documents & Publications ICAM Workshop Ad Hoc Meetings Spectrum Technology...

166

Cognitive Radio Networks as Sensor Networks  

E-Print Network [OSTI]

is used, assuming the cognitive radios know their ownfor Embedded Networked Sensing Cognitive Radio Networks AsJ. Pottie Introduction: Cognitive Radio (CR) Networks The

Bandari, Dorna; Yang, Seung R.; Zhao, Yue; Pottie, Gregory

2007-01-01T23:59:59.000Z

167

Radio Recombination Lines: A New Observational Tool in Astrophysics  

Science Journals Connector (OSTI)

...2.0.30Av/MHz Fig. 4. (a...not significantly larger than the noise...25" HPBW V(MHz) 18hhM 18hOOm...construction of large radio telescopes...The hatched area labeled HPBW is...the meantime both larger radio telescopes...present maps of an area of the galactic...

P. G. Mezger; Patrick Palmer

1968-04-05T23:59:59.000Z

168

Optical and Near-IR Imaging of Ultra Steep Spectrum Radio Sources - The K-z diagram of radio and optically selected galaxies  

E-Print Network [OSTI]

We present optical and/or near-IR images of 128 ultra steep spectrum (USS) radio sources. Roughly half of the objects are identified in the optical images (R 94% are detected at K5). The major axes of the identifications in K-band are preferentially oriented along the radio axes, with half of them having compact morphologies. The 22 sources with spectroscopic redshifts and K-band magnitudes follow the K-z relation found from previous radio samples, but with a larger scatter. We argue that this may be due to a dependence of K-magnitude on the radio power, with the highest radio power sources inhabiting the most massive host galaxies. We present a composite K-z diagram of radio-loud and radio-quiet galaxies, selected from the HDF-North and the Hawaii surveys. Out to z radio-loud galaxies trace the bright envelope of the radio quiet galaxies, while at z >~ 1, the radio-loud galaxies are >~ 2 magnitudes brighter. We argue that this is not due to a contribution from the AGN or emission lines. This difference strongly suggests that radio galaxies pinpoint the most massive systems out to the highest known redshifts, probably due to the mutual correlation of the mass of the galaxy and the radio power on the mass of the central black hole.

Carlos De Breuck; Wil van Breugel; Adam Stanford; Huub Rottgering; George Miley; Daniel Stern

2001-09-28T23:59:59.000Z

169

The Enigmatic Radio Afterglow of GRB 991216  

E-Print Network [OSTI]

We present wide-band radio observations spanning from 1.4 GHz to 350 GHz of the afterglow of GRB 991216, taken from 1 to 80 days after the burst. The optical and X-ray afterglow of this burst were fairly typical and are explained by a jet fireball. In contrast, the radio light curve is unusual in two respects: (a) the radio light curve does not show the usual rise to maximum flux on timescales of weeks and instead appears to be declining already on day 1 and (b) the power law indices show significant steepening from the radio through the X-ray bands. We show that the standard fireball model, in which the afterglow is from a forward shock, is unable to account for (b) and we conclude that the bulk of the radio emission must arise from a different source. We consider two models, neither of which can be ruled out with the existing data. In the first (conventional) model, the early radio emission is attributed to emission from the reverse shock as in the case of GRB 990123. We predict that the prompt optical emission would have been as bright (or brighter) than 8th magnitude. In the second (exotic) model, the radio emission originates from the forward shock of an isotropically energetic fireball (10^54 erg) expanding into a tenuous medium (10^-4 cm^-3). The resulting fireball would remain relativistic for months and is potentially resolvable with VLBI techniques. Finally, we note that the near-IR bump of the afterglow is similar to that seen in GRB 971214 and no fireball model can explain this bump.

D. A. Frail; E. Berger; T. Galama; S. R. Kulkarni; G. H. Moriarty-Schieven; G. G. Pooley; R. Sari; D. S. Shepherd; G. B. Taylor; F. Walter

2000-03-09T23:59:59.000Z

170

TRIESTE: A Trusted Radio Infrastructure for Enforcing SpecTrum Etiquettes  

E-Print Network [OSTI]

1 TRIESTE: A Trusted Radio Infrastructure for Enforcing SpecTrum Etiquettes Wenyuan Xu Pandurang presents a framework, known as TRIESTE (Trusted Radio Infrastructure for Enforcing SpecTrum Etiquettes), which can ensure that radio devices are only able to access/use the spectrum in a manner that conforms

Xu, Wenyuan

171

Extended emission around GPS radio sources  

E-Print Network [OSTI]

Extended radio emission detected around a sample of GHz Peaked Spectrum (GPS) radio sources is discussed. Evidence for extended emission which is related to the GPS source is found in 6 objects out of 33. Three objects are associated with quasars with core-jet pc-scale morphology, and three are identified with galaxies with symmetric (CSO) radio morphology. We conclude that the core-jet GPS quasars are likely to be beamed objects with a continuous supply of energy from the core to the kpc scale. It is also possible that low surface brightness extended radio emission is present in other GPS quasars but the emission is below our detection limit due to the high redshifts of the objects. On the other hand, the CSO/galaxies with extended large scale emission may be rejuvenated sources where the extended emission is the relic of previous activity. In general, the presence of large scale emission associated with GPS galaxies is uncommon, suggesting that in the context of the recurrent activity model, the time scale between subsequent bursts is in general longer than the radiative lifetime of the radio emission from the earlier activity.

C. Stanghellini; C. P. O'Dea; D. Dallacasa; P. Cassaro; S. A. Baum; R. Fanti; C. Fanti

2005-07-21T23:59:59.000Z

172

LOFAR, a new low frequency radio telescope  

E-Print Network [OSTI]

LOFAR, the Low Frequency Array, is a large radio telescope consisting of approximately 100 soccer-field sized antenna stations spread over a region of 400 km in diameter. It will operate at frequencies from ~10 to 240 MHz, with a resolution at 240 MHz of better than an arcsecond. Its superb sensitivity will allow for studies of a broad range of astrophysical topics, including reionisation, transient radio sources and cosmic rays, distant galaxies and AGNs. In this contribution a status rapport of the LOFAR project and an overview of the science case is presented.

H. J. A. Rottgering

2003-09-19T23:59:59.000Z

173

Cognitive Radio: Fundamentals and Opportunities  

E-Print Network [OSTI]

Cognitive Radio: Fundamentals and Opportunities Robert H. Morelos-Zaragoza Department of Electrical Engineering San Jose State University October 12, 2007 #12;Cognitive Radio - RHMZ - 2007 Slide 2 of 18 Outline. Cognitive radio (CR) a) Definition and overview (Mitola) b) CR features (FCC) 3. Unlicensed TV spectrum

Morelos-Zaragoza, Robert H.

174

Electronics, Radio and Telecommunications  

Science Journals Connector (OSTI)

... a grant-in-aid from the United States National Science Foundation. One of these is Telecommunications (No. 1, 1957. Pp. 1-94. First English issue. Issued in ... the official publication of the A. S. Popov Technical Society of Radio Engineering and Telecommunications. ...

1958-10-11T23:59:59.000Z

175

PRESENTATION TITLE  

Energy Savers [EERE]

Hydroelectric Design Center "Leaders in Hydropower Engineering" 11 March 2013 Presentation for Southeastern Federal Power Alliance Steven R. Miles, PE, PMP Director, HDC BUILDING...

176

For Presentation  

Office of Scientific and Technical Information (OSTI)

For Presentation at 7th Fluidization Conference CONF-920502--I f May 3,, 1992 DE92 002879 HYDRODYNAMICS OF CIRCULATING FLUIDIZED BEDS" KINETIC THEORY APPROACH by i Dimitri...

177

Presentation Title  

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

Overview for Newcomers R. Arnold, NV R. Pinney, NJ M. Wangler, DC N. Weber, NM National Transportation Stakeholders Forum 14 May 2013 www.energy.gov/EM 2 Orientation Format * Overview presentation by M. Wangler. * Experiential discussions by R. Arnold, R. Pinney and N. Weber. * Q & A by participants. www.energy.gov/EM 3 Overview Presentation Topics * History of External Coordination * Transportation External Coordination Working Group (TEC) * Background * Some founding principles * Historical issues * Performance goals * Key accomplishments of TEC * National Transportation Stakeholders Forum * Information sharing * Addressing issues and concerns * Working Groups * Continuing focus * 2013 NTSF Meeting * Newsletter www.energy.gov/EM 4 History * Forums existed for addressing issues with communities

178

Testimony to the United States Senate Committee on Environment and Public Works Legislative Hearing on America's Climate Security Act of 2007  

E-Print Network [OSTI]

Testimony to the United States Senate Committee on Environment and Public Works Legislative Hearing Fellow Engineering Science and Technology Division Oak Ridge National Laboratory Good afternoon. Thank sector was responsible for 28% of total U.S. greenhouse gas emissions in 2005 (USEPA, 2007a, table 2

179

Testimony to the United States Senate Committee on Energy and Natural Resources POLICIES TO INCREASE PASSENGER CAR AND LIGHT TRUCK FUEL  

E-Print Network [OSTI]

a course toward a sustainable energy system. For the past twenty years we have spent the technologyTestimony to the United States Senate Committee on Energy and Natural Resources POLICIES Division Oak Ridge National Laboratory Good afternoon. Thank you for inviting me to discuss the need

180

A Sensing Error Aware MAC Protocol for Cognitive Radio Networks  

E-Print Network [OSTI]

Cognitive radios (CR) are intelligent radio devices that can sense the radio environment and adapt to changes in the radio environment. Spectrum sensing and spectrum access are the two key CR functions. In this paper, we present a spectrum sensing error aware MAC protocol for a CR network collocated with multiple primary networks. We explicitly consider both types of sensing errors in the CR MAC design, since such errors are inevitable for practical spectrum sensors and more important, such errors could have significant impact on the performance of the CR MAC protocol. Two spectrum sensing polices are presented, with which secondary users collaboratively sense the licensed channels. The sensing policies are then incorporated into p-Persistent CSMA to coordinate opportunistic spectrum access for CR network users. We present an analysis of the interference and throughput performance of the proposed CR MAC, and find the analysis highly accurate in our simulation studies. The proposed sensing error aware CR MAC p...

Hu, Donglin

2011-01-01T23:59:59.000Z

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


181

Presentation Schedule  

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

Presentation Schedule Presentation Schedule (30 Min) Dave Wade - Dose Comparisons of once-thru and closed fuel cycles. (30 Min) Ralph Bennett - Roadmap Overview (15 Min) Neil Todreas - GRNS Perspectives and Recommendations (75 Min) Neil Todreas / - NERAC DISCUSSION Sal Levy 2 Generation IV Roadmap NERAC Subcommittee (GRNS) Bobby Abrams* Duke Engineering Douglas Chapin MPR Associates B. John Garrick Independent Consultant Dan Kammen University of California- Berkeley 3 Salomon Levy ** Levy & Associates Ted Marston Electrical Power Research Institute Bill Naughton Exelon Neil Todreas ** Massachusetts Institute of Technology * Resigned, July 2002 ** Co-chair GRNS Recruited Working Group Co-Chairs Jack Devine TWG-1 Water Cooled Phil Hildebrandt TWG-2 Gas Cooled Steve Rosen TWG-3 Metal Cooled Bill Rasin

182

PRESENTATION TITLE  

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

PORTLAND DISTRICT PORTLAND DISTRICT 1 Corps of Engineers Hydro Optimization in the Pacific Northwest Presentation for: Southwestern Federal Hydropower Conference Kansas City, Missouri 16 June 2011 By Charlie Allen Hydroelectric Design Center US Army Corps of Engineers BUILDING STRONG ® PORTLAND DISTRICT 2 PRESENTATION OUTLINE  HOT INTRODUCTION AND HISTORY  TYPE I (Unit) OPTIMIZATION ► Cam Curve Verification ► 3-D Cam Controllers ► Inputs and Telemetry ► Gate-Blade Optimizer  TYPE II (Powerhouse) OPTIMIZATION ► Economic Dispatch ► Unit Commitment ► Absolute Flow Measurement ► Benefits Summary  QUESTIONS BUILDING STRONG ® PORTLAND DISTRICT 3 Hydropower Optimization Team (HOT) HOT is joint effort between BPA, COE, and BOR to maximize use of available water for hydropower

183

Radio Astronomy Fundamentals I John Simonetti  

E-Print Network [OSTI]

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

Ellingson, Steven W.

184

Presentation title  

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

Meeting Transmission Meeting Transmission Challenges in the Rocky Mountain Region Jeff Hein June 21, 2011 Western Renewable Energy Zones Composite photo created by NREL Presentation Outline * WREZ Vision * Chronology * WREZ Initiative Overview * Generation and Transmission Model * Lessons Learned * Future Activities National Renewable Energy Laboratory WREZ Vision * Western Governor's Association and U.S. Department of Energy initiated effort to develop renewable energy resources and reduce GHG emissions * Develop a high level "screening tool" to identify potential projects that allows industry stakeholders to analyze and compare economics of

185

basic exchange telecommunications radio service  

Science Journals Connector (OSTI)

A service that extends telecommunications service to rural, outlying, and remote...Common abbreviation BETRS. Note: In the basic exchange telecommunications radio service (BETRS), the (a)....

2001-01-01T23:59:59.000Z

186

SIMULTANEOUS X-RAY AND RADIO OBSERVATIONS OF ROTATING RADIO TRANSIENT J1819-1458  

SciTech Connect (OSTI)

We present the results of simultaneous radio and X-ray observations of PSR J18191458. Our 94 ks XMM-Newton observation of the high magnetic field (?5 10{sup 13} G) pulsar reveals a blackbody spectrum (kT ? 130 eV) with a broad absorption feature, possibly composed of two lines at ?1.0 and ?1.3 keV. We performed a correlation analysis of the X-ray photons with radio pulses detected in 16.2 hr of simultaneous observations at 1-2 GHz with the Green Bank, Effelsberg, and Parkes telescopes, respectively. Both the detected X-ray photons and radio pulses appear to be randomly distributed in time. We find tentative evidence for a correlation between the detected radio pulses and X-ray photons on timescales of less than 10 pulsar spin periods, with the probability of this occurring by chance being 0.46%. This suggests that the physical process producing the radio pulses may also heat the polar-cap.

Miller, J. J.; McLaughlin, M. A. [Department of Physics, West Virginia University, Morgantown, WV 26506 (United States); Rea, N. [Institut de Cincies de l'Espai (IEEC-CSIC) Campus UAB, Fac. de Cincies, Torre C5, parell, 2a planta, E-08193 Barcelona (Spain); Lazaridis, K.; Keane, E. F.; Kramer, M. [Max Planck Institut fr Radioastronomie, Auf dem Hgel 69, D-53121 Bonn (Germany); Lyne, A. [Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester M13 9PL (United Kingdom)

2013-10-20T23:59:59.000Z

187

Montblanc: GPU accelerated Radio Interferometer Measurement Equations in support of Bayesian Inference for Radio Observations  

E-Print Network [OSTI]

We present Montblanc, a GPU implementation of the Radio interferometer measurement equation (RIME) in support of the Bayesian inference for radio observations (BIRO) technique. BIRO uses Bayesian inference to select sky models that best match the visibilities observed by a radio interferometer. To accomplish this, BIRO evaluates the RIME multiple times, varying sky model parameters to produce multiple model visibilities. Chi-squared values computed from the model and observed visibilities are used as likelihood values to drive the Bayesian sampling process and select the best sky model. As most of the elements of the RIME and chi-squared calculation are independent of one another, they are highly amenable to parallel computation. Additionally, Montblanc caters for iterative RIME evaluation to produce multiple chi-squared values. Only modified model parameters are transferred to the GPU between each iteration. We implemented Montblanc as a Python package based upon NVIDIA's CUDA architecture. As such, it is ea...

Perkins, Simon; Zwart, Jonathan; Natarajan, Iniyan; Smirnov, Oleg

2015-01-01T23:59:59.000Z

188

Multiple Radios for Fast Rendezvous in Cognitive Radio Networks  

E-Print Network [OSTI]

--cognitive radio, blind rendezvous, channel hopping ! 1 INTRODUCTION WITH the traditional static spectrum managemen- t, a significant portion of the licensed spectrum is underutilized in most of time while the unlicensed spectrum is over-crowded due to the growing de- mand for wireless radio spectrum from exponen

Chu, Xiaowen

189

Multiple Radios for Effective Rendezvous in Cognitive Radio Networks  

E-Print Network [OSTI]

portions of the spectrum of the licensed users (or primary users, PUs). In cognitive radio networks (CRNs With the traditional static spectrum management, a majority of the licensed spectrum is underutilized in most of time while the unlicensed spectrum is over-crowded due to the growing demand for wireless radio spectrum from

Chu, Xiaowen

190

The spectral structure and energetics of powerful radio sources  

E-Print Network [OSTI]

Determining the energy spectrum of an electron population can give key insights into the underlying physics of a radio source; however, the lack of high resolution, broad-bandwidth observations has left many ambiguities in our understanding of radio galaxies. The improved capabilities of telescopes such as the JVLA and LOFAR mean that within the bandwidth of any given observation, a detailed spectral shape can now be produced. We present recent investigations of powerful FR-II radio galaxies at GHz and MHz frequencies and show for the first time their small-scale spectral structure. We highlight problems in traditional methods of analysis and demonstrate how these issues can now be addressed. We present the latest results from low frequency studies which suggest a potential increase in the total energy content of radio galaxy lobes with possible implications for the energetics of the population as a whole.

Harwood, J J; Croston, J H; Stroe, A; Morganti, R; Orru, E

2014-01-01T23:59:59.000Z

191

X-Ray Emission from a Radio Hotspot in 3C 390.3: Evidence for the Deflection of a Radio Jet by a Neighboring Galaxy  

E-Print Network [OSTI]

By summing a large number of ROSAT High Resolution Imager (HRI) observations of the variable radio galaxy 3C 390.3, we demonstrate that the X-ray emission associated with the northern radio lobe (reported by Prieto 1997) can be identified with hotspot B. None of the other hotspots have been detected. We present evidence that the anomalous X-ray emission is the consequence of a strong shock produced where the northern radio jet impinges onto an external galaxy.

D. E. Harris; K. M. Leighly; J. P. Leahy

1998-04-20T23:59:59.000Z

192

radioCherenkov.dvi  

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

. . Coherent radio Cherenkov radiation detectors: Revised February 2013 by S.R. Klein (LBNL/UC Berkeley) 100 10 10 -4 10 -3 10 -5 1.0 0.1 0.01 E 2 I(E ν ) [GeV m -2 s -1 sr -1 ] E ν [GeV] ν NuMoon 10 9 10 10 10 11 10 12 10 13 10 14 10 15 ATCA (no SSR) ATCA (SSR incl.) RICE ANITA Central GZK ν flux predictions Central GZK ν flux predictions Figure 1: Representative ν flux limits from radio-detection experiments, illustrating the energy ranges for different techniques. Shown are limits from the Rice, ANITA, NuMoon and Lunaska (ATCA) collaborations. NuMoon and Lunaska are low and high frequency lunar scans respectively, showing the strengths of the two different frequency bands. The two limits for ATCA are for different models of the lunar regolith; their separation is a measure of the resultant uncertainty. Also shown, for comparison is the mid-range of flux predictions

193

Radio frequency (RF) heated supersonic flow laboratory  

SciTech Connect (OSTI)

A unique supersonic flow apparatus which employs an inductively-coupled, radio frequency (RF) torch to supply high enthalpy source gas to the nozzle inlet is described. The main features of this system are the plasma tube, a cooled nozzle assembly, and a combustion/expansion chamber with a heat exchanger. A description of these components with current test data is presented. In addition, a discussion of anticipated experiments utilizing this system is included.

Wantuck, P.; Watanabe, H.

1990-01-01T23:59:59.000Z

194

The future for radio astronomy  

Science Journals Connector (OSTI)

......research-article Features The future for radio astronomy Rene P Breton Tom Hassall Rene P Breton and Tom Hassall, School of Physics and Astronomy, University of Southampton, UK; r...Tom Hassall argue that, while radio astronomy has always involved transient phenomena......

Rene P Breton; Tom Hassall

2013-12-01T23:59:59.000Z

195

Stabilized radio-frequency quadrupole  

DOE Patents [OSTI]

A long-vane stabilized radio frequency resonator for accelerating charged particles and including means defining a radio frequency resonator cavity, a plurality of long vanes mounted in the defining means for dividing the cavity into sections, and means interconnecting opposing ones of the plurality of vanes for stabilizing the resonator.

Lancaster, H.D.; Fugitt, J.A.; Howard, D.R.

1982-09-29T23:59:59.000Z

196

Cooperation in Cognitive Radio Networks  

Science Journals Connector (OSTI)

The operation of cognitive radio (CR) networks involves opportunistic access to the spectrum licensed to primary users (PUs) by secondary users (SUs). Traditionally, this access is performed in such a way that the PUs suffer minimal interference to their ... Keywords: cognitive radio networks, cooperation, cooperative relays

Pedro Smith Coutinho, Jos Ferreira de Rezende, Valmir Carneiro Barbosa

2014-05-01T23:59:59.000Z

197

The diffuse radio emission around NGC 5580 and NGC 5588  

E-Print Network [OSTI]

The galaxy pair NGC 5580 and NGC 5588 are part of a loose group of galaxies. They are surrounded by steep-spectrum, extended radio emission which was previously suggested to be a down-scaled example of Mpc-size radio haloes present in galaxies clusters. We present a multi-frequency study of the radio-emission aimed to clarify its nature. The source has been observed with the Giant Meterwave Radio Telescope at 235, 325 and 610 MHz and the images obtained were combined with archival data to cover the frequency range 150-1400 MHz. The new observations revealed the presence of a second, fainter lobe on the South-East of NGC 5580. The spectral index study of the source shows a flattening of the spectrum (which implies a younger particle population) close to the two galaxies. We argue that the extended radio emission is the remnant of a past activity cycle of the active galactic nucleus present in NGC 5580 and therefore a notable example of a dying radio galaxy located outside a dense environments.

de Gasperin, F; Williams, W; Brggen, M; Murgia, M; Beck, R; Bonafede, A

2014-01-01T23:59:59.000Z

198

UCLAComputerScienceDepartmentTechnicalReportTR-080024-2008 Spectrum Aware Routing in Cognitive Radio Mesh  

E-Print Network [OSTI]

spectrum opportunistically. In this paper we present SAMER, a routing solution for cognitive radio mesh spectrum and results in higher end-to-end performance. Index Terms--Cognitive Radio, Spectrum Aware Routing cognitive radio architectures that assume a central controller to lease spectrum to users, while KNOWS [1

Lu, Songwu

199

Spectrum Management for Cognitive Radio based on Genetics Algorithm  

E-Print Network [OSTI]

Spectrum scarceness is one of the major challenges that the present world is facing. The efficient use of existing licensed spectrum is becoming most critical as growing demand of the radio spectrum. Different researches show that the use of licensed are not utilized inefficiently. It has been also shown that primary user does not use more than 70% of the licensed frequency band most of the time. Many researchers are trying to found the techniques that efficiently utilize the under-utilized licensed spectrum. One of the approaches is the use of "Cognitive Radio". This allows the radio to learn from its environment, changing certain parameters. Based on this knowledge the radio can dynamically exploit the spectrum holes in the licensed band of the spectrum. This paper w i l l focus on the performance of spectrum allocation technique, based on popular meta-heuristics Genetics Algorithm and analyzing the performance of this technique using Mat Lab.

Singh, Santosh Kumar; Pathak, Vibhakar; Roy, Dr Krishna Chandra

2011-01-01T23:59:59.000Z

200

The jet-disk symbiosis. I. Radio to X-ray emission models for quasars  

E-Print Network [OSTI]

Starting from the assumption that radio jets and accretion disks are symbiotic features present in radio loud and radio quiet quasars we scale the bulk power of radio jets with the accretion power by adding mass- and energy conservation of the whole jet-disk system to the standard Blandford \\& K\\"onigl theory for compact radio cores. The model depends on only few parameters and can be constrained by observations. Thus we are able to show that radio and X-ray fluxes (SSC emission) of cores and lobes and typical dimensions of radio loud quasars are consistent with a jet being produced in the central engine. We present a synthetic broadband spectrum from radio to X-ray for a jet-disk system. The only way to explain the high efficiency of radio loud objects is to postulate that these objects consist of `maximal jets' with `total equipartition' where the magnetic energy flow of the jet is comparable to the kinetic jet power and the total jet power is a large fraction of the disk power. As the number of electrons is limited by the accretion flow, this is only possible when the minimum Lorentz factor of the electron distribution is $\\gamma_{\\rm e,min}\\ga100$ ($E\\ga 50 {\\rm MeV}$) or/and a large number of pairs are present. Such an electron/positron population would be a necessary consequence of hadronic interactions and may lead to some interesting effects in the low frequency self-absorbed spectrum. Emission from radio weak quasars can be explained with an initially identical jet. The difference between radio loud and radio weak could be due to a different efficiency in accelerating relativistic electrons on the sub-parsec scale. Finally we demonstrate that in order to appease the ravenous hunger of radio loud jets its production must be somehow linked to the dissipation process in the inner part of the disk.

Heino Falcke; Peter L. Biermann

1994-11-23T23:59:59.000Z

Note: This page contains sample records for the topic "testimony presentations radio" 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

Cosmological origin of anomalous radio background  

SciTech Connect (OSTI)

The ARCADE 2 collaboration has reported a significant excess in the isotropic radio background, whose homogeneity cannot be reconciled with clustered sources. This suggests a cosmological origin prior to structure formation. We investigate several potential mechanisms and show that injection of relativistic electrons through late decays of a metastable particle can give rise to the observed excess radio spectrum through synchrotron emission. However, constraints from the cosmic microwave background (CMB) anisotropy, on injection of charged particles and on the primordial magnetic field, present a challenge. The simplest scenario is with a ?>9 GeV particle decaying into e{sup +}e{sup ?} at a redshift of z ? 5, in a magnetic field of ? 5?G, which exceeds the CMB B-field constraints, unless the field was generated after decoupling. Decays into exotic millicharged particles can alleviate this tension, if they emit synchroton radiation in conjunction with a sufficiently large background magnetic field of a dark U(1)' gauge field.

Cline, James M. [Department of Physics, McGill University, 3600 Rue University, Montral, Qubec, H3A 2T8 Canada (Canada); Vincent, Aaron C., E-mail: jcline@physics.mcgill.ca, E-mail: vincent@ific.uv.es [Instituto de Fsica Corpuscular, Universitat de Valncia - CSIC, 46071, Valencia (Spain)

2013-02-01T23:59:59.000Z

202

Spectrum Sensing and Reconstruction for Cognitive Radio  

E-Print Network [OSTI]

Spectrum Sensing and Reconstruction for Cognitive Radio Amanpreet S Saini, Zhen Hu, Robert Qiu with spectrum sensing and spectrum reconstruction under the umbrella of cognitive radio which is the smart radio to explore and exploit the free spectrum. Spectrum analyzer is used to emulate cognitive radio to do spectrum

Qiu, Robert Caiming

203

Cognitive Radio Technology [from THE GUEST EDITORS  

E-Print Network [OSTI]

Cognitive Radio Technology [from THE GUEST EDITORS] Maria Gabriella di Benedetto, Yingbo Hua of cognitive radio. Perhaps the most pressing of them is improved utilization of the electromagnetic radio addressing a multitude of cognitive radio topics were recently approved with a total budget of more than 50

Di Benedetto, Maria-Gabriella

204

Radio galaxies and local quasars  

Science Journals Connector (OSTI)

... through the gas and magnetic fields near the galaxy which ejected them. This would produce synchroton radio emission in great strength and over a long time, drawing its power from ...

JAMES TERRELL

1975-11-13T23:59:59.000Z

205

Microwave and Radio Frequency Workshop  

Broader source: Energy.gov [DOE]

At the Microwave and Radio Frequency Workshop (held in Long Beach, CA, on July 25, 2012), academic and industry experts discussed the existing and emerging electrotechnologies such as microwave ...

206

Deep ATLAS radio observations of the CDFS-SWIRE field  

E-Print Network [OSTI]

We present the first results from the Australia Telescope Large Area Survey (ATLAS), which consist of deep radio observations of a 3.7 square degree field surrounding the Chandra Deep Field South, largely coincident with the infrared Spitzer Wide-Area Extragalactic (SWIRE) Survey. We also list cross-identifications to infrared and optical photometry data from SWIRE, and ground-based optical spectroscopy. A total of 784 radio components are identified, corresponding to 726 distinct radio sources, nearly all of which are identified with SWIRE sources. Of the radio sources with measured redshifts, most lie in the redshift range 0.5-2, and include both star-forming galaxies and active galactic nuclei (AGN). We identify a rare population of infrared-faint radio sources which are bright at radio wavelengths but are not seen in the available optical, infrared, or X-ray data. Such rare classes of sources can only be discovered in wide, deep surveys such as this.

Ray P. Norris; Jose Afonso; Phil N. Appleton; Brian J. Boyle; Paolo Ciliegi; Scott M. Croom; Minh T. Huynh; Carole A. Jackson; Anton M. Koekemoer; Carol J. Lonsdale; Enno Middelberg; Bahram Mobasher; Seb J. Oliver; Mari Polletta; Brian D. Siana; Ian Smail; Maxim A. Voronkov

2006-10-18T23:59:59.000Z

207

Radio and near-infrared observations of the steep spectrum Galactic plane radio source WKB 0314+57.8  

E-Print Network [OSTI]

Radio and near-infared observations towards the steep spectrum Galactic plane radio source WKB 0314+57.8 are presented, in order to clarify the nature of this source. The radio observations include archival and survey data, together with new Giant Metrewave Radio Telescope observations at 617 MHz. The near-infrared observations are in the J and K bands, from the Gemini instrument on the Shane 3-m telescope. The radio observations show that WKB 0314+57.8 is extended, with an very steep spectrum (with flux density proportional to frequency to -2.5 power between 40 MHz and 1.5 GHz). The colour--magnitude diagram constructed from near-infrared observations of the field suggests the presence of a z approx 0.08 galaxy cluster behind the Galactic plane, reddened by about 6 magnitudes of visual extinction. Although the steep spectrum source has no obvious identification, two other radio sources in the field covered by the near-infrared observations have tentative identifications with galaxies. These observations indicate that WKB 0314+57.8 is a relic source in a cluster of galaxies, not a pulsar.

D. A. Green; M. Lacy; S. Bhatnagar; E. L. Gates; P. J. Warner

2004-08-06T23:59:59.000Z

208

Large Scale Impact of the Cosmological Population of Expanding Radio Galaxies  

E-Print Network [OSTI]

We seek to compute the fraction of the volume of the Universe filled by expanding cocoons of the cosmological population of radio galaxies over the Hubble time as well as the magnetic field infused by them, in order to assess their importance in the cosmic evolution of the Universe. Using N-body $\\Lambda$CDM simulations, radio galaxies distributed according to the observed radio luminosity function are allowed to evolve in a cosmological volume as using well defined prescriptions for their expansion. We find that the radio galaxies permeate $10 - 30%$ of the total volume with $\\sim 10^{-8}$ G magnetic field by the present epoch.

Paramita Barai

2008-06-11T23:59:59.000Z

209

Large Scale Impact of the Cosmological Population of Expanding Radio Galaxies  

E-Print Network [OSTI]

We seek to compute the fraction of the volume of the Universe filled by expanding cocoons of the cosmological population of radio galaxies over the Hubble time as well as the magnetic field infused by them, in order to assess their importance in the cosmic evolution of the Universe. Using N-body $\\Lambda$CDM simulations, radio galaxies distributed according to the observed radio luminosity function are allowed to evolve in a cosmological volume as using well defined prescriptions for their expansion. We find that the radio galaxies permeate $10 - 30%$ of the total volume with $\\sim 10^{-8}$ G magnetic field by the present epoch.

Barai, Paramita

2008-01-01T23:59:59.000Z

210

Low frequency radio spectrum and spectral turnover of LS 5039  

E-Print Network [OSTI]

LS 5039, a possible black hole x-ray binary, was recently observed with Giant Meterwave Radio Telescope. The observed spectrum presented here shows that the spectrum is inverted at the low frequency. When combined with the archival data with orbital phase similar to the present observations, it shows a clear indication of a spectral turnover. The combined data are fitted with a broken power-law and the break frequency signifies a possible spectral turnover of the spectrum around 964 MHz. Truly simultaneous observations in radio wavelength covering a wide range of frequencies are required to fix the spectrum and the spectral turn over which will play a crucial role in developing a deeper understanding of the radio emitting jet in LS 5039.

Sagar Godambe; Subir Bhattacharyya; Nilay Bhatt; Manojendu Choudhury

2008-07-15T23:59:59.000Z

211

Evolution of Cygnus X-3 through its Radio and X-ray States  

SciTech Connect (OSTI)

Based on X-ray spectra and studies of the long-term correlated behavior between radio and soft X-ray, we present a detailed evolution of Cyg X-3 through its radio and X-ray states. We comment on the nature of the hard X-ray tail and possible Simbol X contribution in constraining the models.

Szostek, A. [Laboratoire d'Astrophysique de Grenoble, CNRS, Universite Joseph Fourier, Grenoble (France); Astronomical Observatory, Jagiellonian University, Krakow (Poland); Zdziarski, A. A. [Centrum Astronomiczne im. M. Kopernika, Warszawa (Poland); McCollough, M. L. [Smithsonian Astrophysical Observatory, Cambridge (United States)

2009-05-11T23:59:59.000Z

212

A Coordinated Radio Afterglow Program  

E-Print Network [OSTI]

We describe a ground-based effort to find and study afterglows at centimeter and millimeter wavelengths. We have observed all well-localized gamma-ray bursts in the Northern and Southern sky since BeppoSAX first started providing rapid positions in early 1997. Of the 23 GRBs for which X-ray afterglows have been detected, 10 have optical afterglows and 9 have radio afterglows. A growing number of GRBs have both X-ray and radio afterglows but lack a corresponding optical afterglow.

D. A. Frail; S. R. Kulkarni; M. H. Wieringa; G. B. Taylor; G. H. Moriarty-Schieven; D. S. Shepherd; R. M. Wark; R. Subrahmanyan; D. McConnell; S. J. Cunningham

1999-12-08T23:59:59.000Z

213

Towards Cognitive Radio Networks: Spectrum Utilization Measurements in Suburb Environment  

E-Print Network [OSTI]

Towards Cognitive Radio Networks: Spectrum Utilization Measurements in Suburb Environment Václav in an opportunistic way. Cognitive radio concept for better spectrum utilization is introduced here along -- Cognitive radio, radio spectrum management, spectrum sensing, spectrum utilization. I. INTRODUCTION

Paris-Sud XI, Université de

214

Radio Receiver Design  

Science Journals Connector (OSTI)

... local oscillator and then through the intermediate-frequency amplifier to the second detector giving an audio-frequency output. The present volume ends at this stage, leaving ... -frequency output. The present volume ends at this stage, leaving audio-frequency amplifiers and power supplies to be dealt with in Part 2. ...

1943-06-12T23:59:59.000Z

215

RASDR: Benchtop Demonstration of SDR for Radio Astronomy  

SciTech Connect (OSTI)

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

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

2012-01-01T23:59:59.000Z

216

ELECTRON-BEAM-INDUCED RADIO EMISSION FROM ULTRACOOL DWARFS  

SciTech Connect (OSTI)

We present the numerical simulations for an electron-beam-driven and loss-cone-driven electron-cyclotron maser (ECM) with different plasma parameters and different magnetic field strengths for a relatively small region and short timescale in an attempt to interpret the recent discovered intense radio emission from ultracool dwarfs. We find that a large amount of electromagnetic (EM) field energy can be effectively released from the beam-driven ECM, which rapidly heats the surrounding plasma. A rapidly developed high-energy tail of electrons in velocity space (resulting from the heating process of the ECM) may produce the radio continuum depending on the initial strength of the external magnetic field and the electron beam current. Both significant linear polarization and circular polarization of EM waves can be obtained from the simulations. The spectral energy distributions of the simulated radio waves show that harmonics may appear from 10 to 70{nu}{sub pe} ({nu}{sub pe} is the electron plasma frequency) in the non-relativistic case and from 10 to 600{nu}{sub pe} in the relativistic case, which makes it difficult to find the fundamental cyclotron frequency in the observed radio frequencies. A wide frequency band should therefore be covered by future radio observations.

Yu, S.; Doyle, J. G.; Kuznetsov, A. [Armagh Observatory, College Hill, Armagh BT61 9DG (United Kingdom); Hallinan, G. [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Antonova, A. [Department of Astronomy, St. Kliment Ohridski University of Sofia, 5 James Bourchier Blvd., 1164 Sofia (Bulgaria); MacKinnon, A. L. [School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ (United Kingdom); Golden, A., E-mail: syu@arm.ac.uk [Price Center, Albert Einstein College of Medicine, Yeshiva University, Bronx, NY 10461 (United States)

2012-06-10T23:59:59.000Z

217

Current Problems for X-ray Emission from Radio Jets  

E-Print Network [OSTI]

A list is presented of known extragalactic radio jets which also have associated X-ray emission. The canonical emission processes for the production of X-rays are reviewed and the sources are categorized on the basis of our current understanding. Although it seems clear that the X-ray emission is non-thermal, the two competing processes, synchrotron and inverse Compton emissions, arise from extremely high energy (synchrotron) or extremely low energy (beaming models with IC emission), relativistic electrons. Only synchrotron self-Compton emission from a few hotspots provides information on the `normal' energy range of the electrons responsible for the observed radio emission.

D. E. Harris

2000-12-17T23:59:59.000Z

218

RADIO EMISSION FROM INSTABILITIES IN SPACE PLASMAS: MARGINAL STABILITY,  

E-Print Network [OSTI]

I t RADIO EMISSION FROM INSTABILITIES IN SPACE PLASMAS: MARGINAL STABILITY, 4TOCHASTIC GROWTH emission, hich is an indirect emission process first discussed by Ginaburg and Zhe/eznyakoe, 9581, and electron cyclotron maser emission (ECME), which is a direct emission ess first discussed in the presently

Melrose, Don

219

On the Radio-activity of Natural Gas  

Science Journals Connector (OSTI)

... Physical Science Series, an account is given of some experiments with a highly radio-active gas obtained from crude petroleum. In this investigation it was found that air drawn through ... emanation from radium. The present writer has extended this investigation to an examination of the natural ...

J. C. MCLENNAN

1904-06-16T23:59:59.000Z

220

Spectrum Characterization for Opportunistic Cognitive Radio Systems  

E-Print Network [OSTI]

1 Spectrum Characterization for Opportunistic Cognitive Radio Systems Tevfik Y¨ucek and H challenging problems in cognitive radio systems. The spectrum of interest needs to be characterized and unused initial network entry is also discussed as a case study. Index Terms-- Cognitive radio, spectrum sensing

Arslan, Hüseyin

Note: This page contains sample records for the topic "testimony presentations radio" 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

System Design for Cognitive Radio Communications  

E-Print Network [OSTI]

about an increasing demand for frequency spectrum. Cognitive radio offers a tempting solution, in which frequency bands that are not being used by their licensed users are utilized by cognitive radios. Since cognitive radios do not need to have a license and since they do not affect the operation

Arslan, Hüseyin

222

METHODS OF RADIO-FREQUENCY CURRENT DRIVE  

E-Print Network [OSTI]

METHODS OF RADIO-FREQUENCY CURRENT DRIVE N. J. FISCH* Princeton Plasma Physics Laboratory-670 Radio-frequency waves can penetrate thermonuclear plasmas, depositing momentum and energy with great. INTRODUCTION Using radio-frequency (rf) waves to drive the toroidal current in tokamak reactors is attractive

223

The environments of FRII radio sources  

Science Journals Connector (OSTI)

......radio-emitting plasma, as argued by Kaiser...used total 178-MHz flux densities from...about the external atmosphere. 1 As discussed...radio-emitting plasma altogether from...X-ray-emitting atmospheres. Although many...radio-emitting plasma. It is then a coincidence......

M. J. Hardcastle; D. M. Worrall

2000-12-01T23:59:59.000Z

224

Electron beam induced radio emission from ultracool dwarfs  

E-Print Network [OSTI]

We present the numerical simulations for an electron-beam-driven and loss-cone-driven electron-cyclotron maser (ECM) with different plasma parameters and different magnetic field strengths for a relatively small region and short time-scale in an attempt to interpret the recent discovered intense radio emission from ultracool dwarfs. We find that a large amount of electromagnetic field energy can be effectively released from the beam-driven ECM, which rapidly heats the surrounding plasma. A rapidly developed high-energy tail of electrons in velocity space (resulting from the heating process of the ECM) may produce the radio continuum depending on the initial strength of the external magnetic field and the electron beam current. Both significant linear polarization and circular polarization of electromagnetic waves can be obtained from the simulations. The spectral energy distributions of the simulated radio waves show that harmonics may appear from 10 to 70$\

Yu, S; Kuznetsov, A; Hallinan, G; Antonova, A; MacKinnon, A L; Golden, A

2012-01-01T23:59:59.000Z

225

Hybrid spread spectrum radio system  

DOE Patents [OSTI]

Systems and methods are described for hybrid spread spectrum radio systems. A method, includes receiving a hybrid spread spectrum signal including: fast frequency hopping demodulating and direct sequence demodulating a direct sequence spread spectrum signal, wherein multiple frequency hops occur within a single data-bit time and each bit is represented by chip transmissions at multiple frequencies.

Smith, Stephen F. (London, TN) [London, TN; Dress, William B. (Camas, WA) [Camas, WA

2010-02-09T23:59:59.000Z

226

GEOL 5303 Project Presentations Presenter name: ______________________________________________  

E-Print Network [OSTI]

GEOL 5303 Project Presentations Presenter name: ______________________________________________ Project title: ___________________________________________________________ Project content Superb Effective Weak Absent Introduction: What is your project topic? Presenter provides a clear introduction

Smith-Konter, Bridget

227

MULTI-FREQUENCY STUDIES OF RADIO RELICS IN THE GALAXY CLUSTERS A4038, A1664, AND A786  

SciTech Connect (OSTI)

We present a multi-frequency study of radio relics associated with the galaxy clusters A4038, A1664, and A786. Radio images, integrated spectra, spectral index maps, and fits to the integrated spectra in the framework of the adiabatic compression model are presented. Images of the relic in A4038 at 150, 240, and 606 MHz with the Giant Meterwave Radio Telescope have revealed extended ultra-steep spectrum ({alpha} {approx} -1.8 to -2.7) emission of extent 210 Multiplication-Sign 80 kpc{sup 2}. The model of passively evolving radio lobes compressed by a shock fits the integrated spectrum best. The relic with a circular morphology at the outskirts of the cluster A1664 has an integrated spectral index of {approx} - 1.10 {+-} 0.06 and is best fit by the model of radio lobes lurking for {approx}4 Multiplication-Sign 10{sup 7} yr. The relic near A786 has a curved spectrum and is best fit by a model of radio lobes lurking for {approx}3 Multiplication-Sign 10{sup 7} yr. At 4.7 GHz, a compact radio source, possibly the progenitor of the A786 relic, is detected near the center of the radio relic. The A786 radio relic is thus likely a lurking radio galaxy rather than a site of cosmological shock as has been considered in earlier studies.

Kale, Ruta; Dwarakanath, K. S., E-mail: ruta@iucaa.ernet.in [Raman Research Institute, C. V. Raman Avenue, Sadashivanagar, Bangalore 560 080 (India)

2012-01-01T23:59:59.000Z

228

3-4-10_Final_Testimony_28SEPA29_28Legg29.pdf  

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

KENNETH E. LEGG ADMINISTRATOR SOUTHEASTERN POWER ADMINISTRATION U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON WATER AND POWER COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES MARCH 4, 2010 2 Madam Chairwoman and members of the Subcommittee, I am Kenneth Legg, Administrator of the Southeastern Power Administration (Southeastern), and I appreciate this opportunity to present a written statement today on the Fiscal Year 2011 Budget Request for the Southeastern Power Administration. PROFILE OF SOUTHEASTERN POWER ADMINISTRATION The mission of Southeastern is to market and deliver Federal hydroelectric power at the lowest possible cost consistent with sound business principles to public bodies and cooperatives in accordance with Section 5 of the Flood Control Act of 1944 (16 U.S.C. 825s).

229

Radio Sources in Low-Luminosity Active Galactic Nuclei.IV. Radio Luminosity Function, Importance of Jet Power, and Radio Properties of the Complete Palomar Sample  

E-Print Network [OSTI]

We present the completed results of a high resolution radio imaging survey of all (~200) low-luminosity active galactic nuclei (LLAGNs) and AGNs in the Palomar Spectroscopic Sample. The high incidences of pc-scale radio nuclei, with T(brightness) >=10^7 K, and sub-parsec jets argue for accreting black holes in >=50% of all LINERs and low-luminosity Seyferts; there is no evidence against all LLAGNs being mini-AGNs. The radio luminosity function (RLF) of Palomar Sample LLAGNs and AGNs extends three orders of magnitude below, and is continuous with, that of `classical' AGNs. We find marginal evidence for a low-power turnover in the RLF; nevertheless LLAGNs are responsible for a significant fraction of present day mass accretion. Adopting the jet model of Falcke & Biermann, we show that the accretion energy output in LLAGNs is dominated by the energy in the observed jets rather than the radiated bolometric luminosity. The Palomar LLAGNs and AGNs follow the same scaling between jet power and narrow line region (NLR) luminosity as the pc to kpc jets in powerful radio galaxies. Eddington ratios of <= 10^{-1} - 10^{-5} are implied in jet models of the radio emission. We find evidence that, in analogy to Galactic black hole candidates, LINERs are in a `low/hard' state (gas poor nuclei, low Eddington ratio, ability to launch collimated jets) while low-luminosity Seyferts are in a `high' state (gas rich nuclei, higher Eddington ratio, less likely to launch collimated jets). The jets are energetically more significant than supernovae in the LLAGN host galaxies, and are potentially able to deposit sufficient energy into the innermost parsecs to significantly slow the gas supply to the accretion disk.

Neil M. Nagar; Heino Falcke; Andrew S. Wilson

2005-02-25T23:59:59.000Z

230

Software-defined Radio Based Wireless Tomography: Experimental Demonstration and Verification  

SciTech Connect (OSTI)

This letter presents an experimental demonstration of software-defined-radio-based wireless tomography using computer-hosted radio devices called Universal Software Radio Peripheral (USRP). This experimental brief follows our vision and previous theoretical study of wireless tomography that combines wireless communication and RF tomography to provide a novel approach to remote sensing. Automatic data acquisition is performed inside an RF anechoic chamber. Semidefinite relaxation is used for phase retrieval, and the Born iterative method is utilized for imaging the target. Experimental results are presented, validating our vision of wireless tomography.

Bonior, Jason D [ORNL; Hu, Zhen [Tennessee Technological University; Guo, Terry N. [Tennessee Technological University; Qiu, Robert C. [Tennessee Technological University; Browning, James P. [United States Air Force Research Laboratory, Wright-Patterson Air Force Base; Wicks, Michael C. [University of Dayton Research Institute

2015-01-01T23:59:59.000Z

231

Impact of Infrared, Microwave, and Radio Occultation Satellite Observations on Operational Numerical Weather Prediction  

Science Journals Connector (OSTI)

A comparison of the impact of infrared (IR), microwave (MW), and radio occultation (RO) observations on NCEPs operational global forecast model over the month of March 2013 is presented. Analyses and forecasts with only IR, MW, and RO ...

L. Cucurull; R. A. Anthes

2014-11-01T23:59:59.000Z

232

Enhancement of electromagnetic propagation through complex media for Radio Frequency Identification  

E-Print Network [OSTI]

In this thesis, I present and examine the fundamental limitations involved in Radio Frequency Identification (RFID) as well as provide a means to improve reader-tag communication in ultra high frequency RFID systems. The ...

Marti, Uttara P

2005-01-01T23:59:59.000Z

233

ATLBS EXTENDED SOURCE SAMPLE: THE EVOLUTION IN RADIO SOURCE MORPHOLOGY WITH FLUX DENSITY  

SciTech Connect (OSTI)

Based on the Australia Telescope Low Brightness Survey (ATLBS) we present a sample of extended radio sources and derive morphological properties of faint radio sources. One hundred nineteen radio galaxies form the ATLBS Extended Source Sample (ATLBS-ESS) consisting of all sources exceeding 30'' in extent and integrated flux densities exceeding 1 mJy. We give structural details along with information on galaxy identifications and source classifications. The ATLBS-ESS, unlike samples with higher flux-density limits, has almost equal fractions of FR-I and FR-II radio galaxies, with a large fraction of the FR-I population exhibiting 3C31-type structures. Significant asymmetry in lobe extents appears to be a common occurrence in the ATLBS-ESS FR-I sources compared with FR-II sources. We present a sample of 22 FR-Is at z > 0.5 with good structural information. The detection of several giant radio sources, with size exceeding 0.7 Mpc, at z > 1 suggests that giant radio sources are not less common at high redshifts. The ESS also includes a sample of 28 restarted radio galaxies. The relative abundance of dying and restarting sources is indicative of a model where radio sources undergo episodic activity in which an active phase is followed by a brief dying phase that terminates with restarting of the central activity; in any massive elliptical a few such activity cycles wherein adjacent events blend may constitute the lifetime of a radio source and such bursts of blended activity cycles may be repeated over the age of the host. The ATLBS-ESS includes a 2 Mpc giant radio galaxy with the lowest surface brightness lobes known to date.

Saripalli, L.; Subrahmanyan, R.; Thorat, K.; Ekers, R. D. [Raman Research Institute, C. V. Raman Avenue, Sadashivanagar, Bangalore 560080 (India); Hunstead, R. W.; Johnston, H. M.; Sadler, E. M., E-mail: lsaripal@rri.res.in [Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006 (Australia)

2012-04-01T23:59:59.000Z

234

Poster Presentations 1 Poster Presentation Basics  

E-Print Network [OSTI]

Basics Poster Presentations 1 Poster Presentation Basics #12;Poster presentations involve two things Poster Presentation Basics2 Creating an effective poster The oral presentation you do standing by your poster #12;Effective posters A poster should convey the basic, most crucial points of your work

Texas at Arlington, University of

235

A Present . . . And A Future | U.S. DOE Office of Science (SC)  

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

A Present . . A Present . . . And A Future News Featured Articles 2014 2013 2012 2011 2010 2009 2008 2007 2006 2005 Science Headlines Presentations & Testimony News Archives Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 12.12.12 A Present . . . And A Future Students are hitting the books - instead of the mall - in preparation for the 2013 National Science Bowl. Print Text Size: A A A Subscribe FeedbackShare Page Click to enlarge photo. Enlarge Photo 2013 National Science Bowl Thousands of middle- and high-school students across the country are headed for a slightly unusual holiday season. Instead of hitting the mall, they'll be hitting the books. And instead of trying to figure out which movie to see, they'll instead be trying to remember answers to questions such as:

236

Statement of Charles G. Groat Director, U.S. Geological Survey, U.S. Depa...rce and Agency Organization, On The Yucca Mountain Project, April 5, 2005 Congressional Testimony, 2005  

E-Print Network [OSTI]

Organization, On The Yucca Mountain Project, April 5, 2005 Congressional Testimony, 2005 Statement of Charles G on Government Reform, Subcommittee on the Federal Workforce and Agency Organization On The Yucca Mountain's (DOE) Yucca Mountain Project. Let me emphasize from the outset how seriously USGS takes this situation

Torgersen, Christian

237

Pat Hoffman Testimony  

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

PATRICIA HOFFMAN PATRICIA HOFFMAN ACTING ASSISTANT SECRETARY FOR ELECTRICITY DELIVERY AND ENERGY RELIABILITY U.S. DEPARTMENT OF ENERGY BEFORE THE COMMITTEE ON ENERGY AND NATURAL RESOURCES U.S. SENATE MAY 7, 2009 Mr. Chairman and members of the Committee, thank you for this opportunity to testify before you on the cyber security issues facing the electric industry and on emergency authorities to protect critical electric infrastructure. All of us here today share a common concern that vulnerabilities exist within the electric system and that the government and the private sector must do everything we can to address it. This is particularly true for smart grid systems, which by their very nature involve the use of information technologies in areas and applications on the

238

TESTIMONY OF ARPAD A  

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

OF ARPAD A. BERGH, OF ARPAD A. BERGH, PRESIDENT OF THE OPTOELECTRONICS INDUSTRY DEVELOPMENT ASSOCIATION to the SENATE COMMITTEE ON ENERGY AND NATURAL RESOURCES JULY 18, 2001 "S. 1166 - THE NEXT GENERATION LIGHTING INITIATIVE ACT" * * * On behalf of the Optoelectronics Industry Development Association ("OIDA"), I would like to offer support for a government-industry initiative to develop a new form of energy efficient lighting based on solid state optoelectronics. In particular, OIDA en- dorses legislation recently introduced by Senators Jeff Bingaman and Mike DeWine -- S. 1166 -- that would establish a government-industry initiative to accelerate the develop- ment of solid state lighting. The "Next Generation Lighting Initiative Act" would create a 10-year program for

239

SG Testimony for March  

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

PATRICIA HOFFMAN ACTING ASSISTANT SECRETARY FOR ELECTRICITY DELIVERY AND ENERGY RELIABILITY U.S. DEPARTMENT OF ENERGY BEFORE THE SUBCOMMITTEE ON ENERGY AND ENVIRONMENT COMMITTEE ON SCIENCE AND TECHNOLOGY U.S. HOUSE OF REPRESENTATIVES JULY 23, 2009 Thank you Mr. Chairman and members of the Subcommittee for the opportunity to provide an update on the current status of smart grid activities at the Department of Energy as well as our future directions and priorities. The Energy Independence and Security Act of 2007 (EISA) and the American Recovery and Reinvestment Act of 2009 (Recovery Act) expand the role of the Federal Government substantially in research,

240

Testimony | Department of Energy  

Office of Environmental Management (EM)

of Information Resources Public Roundtable- Data Access and Privacy Issues Related to Smart Grid Technologies Public Meeting Transcript: Sustainable Design Standards for...

Note: This page contains sample records for the topic "testimony presentations radio" 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

"Human Life" Testimony  

Science Journals Connector (OSTI)

...Evanston, Illinois 60201 Hubbert's...article "How much oil? It de-pends...427) of the oil and gas estimates...expert in the field, M. King Hubbert...of ultimate production of crude oil from the lower-48...repre-sent cumulative production...

BENJAMIN LIBET

1981-07-10T23:59:59.000Z

242

FE Speeches and Testimony  

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

property"content:encoded" class"field-item odd">

Statement by Christopher Smith, Principal Deputy Assistant Secretary for Fossil Energy before the House Committee on...

243

Radio frequency overview of the high explosive radio telemetry project  

SciTech Connect (OSTI)

High explosive radio telemetry (HERT) is a project that is being developed jointly by Los Alamos National Laboratory and AlliedSignal Federal Manufacturing and Technologies. The ultimate goal is to develop a small, modular telemetry system capable of high-speed detection of explosive events, with an accuracy on the order of 10 nanoseconds. The reliable telemetry of this data, from a high-speed missile trajectory, is a very challenging opportunity. All captured data must be transmitted in less than 20 microseconds of time duration. This requires a high bits/Hertz microwave telemetry modulation code to insure transmission of the data with the limited time interval available.

Bracht, R. [Los Alamos National Lab., NM (United States); Dimsdle, J.; Rich, D.; Smith, F. [AlliedSignal Federal Manufacturing and Technologies, Kansas City, MO (United States)

1998-12-31T23:59:59.000Z

244

The radio spectrum of Sgr A*  

E-Print Network [OSTI]

We discuss the radio spectrum of Sgr A* \\index{Sgr A*, radio spectrum} in the frequency range between $\\approx 1\\,{\\rm GHz}$ and $\\approx 1\\,000\\,{\\rm GHz}$, show that it can be explained by optically thin synchrotron radiation \\index{Sgr A*, synchrotron radiation, optically thin} of relativistic electrons, and point toward a possible correlation between the spectrum of Sgr A* and larger-scale ($\\la 50\\,{\\rm pc}$) radio emission from the Galactic Center \\index{Galactic Center} region.

Wolfgang J. Duschl; Harald Lesch

1994-11-03T23:59:59.000Z

245

The Late-Time Radio Spectrum of SN1993J  

E-Print Network [OSTI]

We present VLA radio continuum measurements of SN1993J in M81 at the frequencies of 0.32 (P-band), 1.3 and 1.7 (L-band), 4.9 (C-band), 8.5 (X-band), and 14.9 (U-band) GHz carried out on December 17 and 21, 2000, about 2820 days after the supernova explosion. We find that a power-law spectrum, free-free absorbed by an homogeneous, or clumpy, distribution of ionized gas yields the best fit to the radio data. A combined homogeneous-clumpy model is not favored, but neither totally excluded. This result contrasts with the modeling of the early ($t \\lessim $230 days) radio emission from SN1993J, where a mixture of homogeneous and clumpy absorbers appeared to be necessary to adequately describe the behavior of the light curves. The radio spectrum of supernova SN1993J between 0.32 and 14.9 GHz is well characterized by $\\alpha = -0.67 \\pm 0.02 $ ($S_\

M. A. Perez-Torres; A. Alberdi; J. M. Marcaide

2002-05-14T23:59:59.000Z

246

Radio galaxies and the star formation history of the universe  

E-Print Network [OSTI]

Multi-wavelength observations made in the last decade suggest that the universe underwent an intense phase of star formation in the past (z > 1). This intensive activity is commonly attributed to a higher galaxy merger rate when the universe was a fraction of its present age. We examine the role of the powerful radio sources whose comoving density is known to be a few orders of magnitude higher at z ~ 2, the `quasar era'. Taking into account recent models for the temporal evolution of the size and luminosity of a powerful double radio source, as well as Lambda-CDM simulations of the cosmic web of baryonic material at different redshifts, we argue that during the quasar era a high fraction of the volume of the web was occupied by the lobes of double radio sources. Widespread compression of protostellar clouds, triggered by the high pressure of the synchrotron plasma of the radio lobes, can thus be expected to have played a significant role in the global star formation history of the universe. These lobes can also yield a rather high level of magnetization of the intergalactic medium at these early cosmic epochs.

Gopal-Krishna; Paul J. Wiita; M. Angela Osterman

2002-11-20T23:59:59.000Z

247

CXAllenRadioTower2.pdf  

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

Southwestern Power Administration proposes to modify and reconstruct its Allen Radio Tower communications site as part of the Spectrum Relocation project. Categorical...

248

Spectrum Decision for Cognitive Radio Networks.  

E-Print Network [OSTI]

??Cognitive Radio Networks (CRNs) are a key technology suggested to be part of 4G and beyond. The fundamental concept is to let Secondary Users (SUs) (more)

Yao, Yong; Erman, David

2011-01-01T23:59:59.000Z

249

Compressive Spectrum Sensing for Cognitive Radio Networks.  

E-Print Network [OSTI]

??Spectrum sensing is the most important part in cognitive radios. Wideband spectrum sensing requires high speed and large data samples. It makes sampling process challenging (more)

Nakarmi, Ukash

2011-01-01T23:59:59.000Z

250

Agile Testing Methods for IC Radios.  

E-Print Network [OSTI]

??This thesis concentrates on the development of a new testing procedure for the radio used in Broadcom?s WLAN and cellular chips. Verification and hardware testing (more)

Martinez, Luis

2011-01-01T23:59:59.000Z

251

Remarks From the 2010 Linton Brooks Medal for Public Service Presentation  

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

From the 2010 Linton Brooks Medal for Public Service Presentation From the 2010 Linton Brooks Medal for Public Service Presentation Ceremony | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Speeches > Remarks From the 2010 Linton Brooks Medal ... Speech Remarks From the 2010 Linton Brooks Medal for Public Service Presentation

252

Remarks From the 2010 Linton Brooks Medal for Public Service Presentation  

National Nuclear Security Administration (NNSA)

From the 2010 Linton Brooks Medal for Public Service Presentation From the 2010 Linton Brooks Medal for Public Service Presentation Ceremony | National Nuclear Security Administration Our Mission Managing the Stockpile Preventing Proliferation Powering the Nuclear Navy Emergency Response Recapitalizing Our Infrastructure Continuing Management Reform Countering Nuclear Terrorism About Us Our Programs Our History Who We Are Our Leadership Our Locations Budget Our Operations Media Room Congressional Testimony Fact Sheets Newsletters Press Releases Speeches Events Social Media Video Gallery Photo Gallery NNSA Archive Federal Employment Apply for Our Jobs Our Jobs Working at NNSA Blog Home > Media Room > Speeches > Remarks From the 2010 Linton Brooks Medal ... Speech Remarks From the 2010 Linton Brooks Medal for Public Service Presentation

253

Hybrid spread spectrum radio system  

DOE Patents [OSTI]

Systems and methods are described for hybrid spread spectrum radio systems. A method includes modulating a signal by utilizing a subset of bits from a pseudo-random code generator to control an amplification circuit that provides a gain to the signal. Another method includes: modulating a signal by utilizing a subset of bits from a pseudo-random code generator to control a fast hopping frequency synthesizer; and fast frequency hopping the signal with the fast hopping frequency synthesizer, wherein multiple frequency hops occur within a single data-bit time.

Smith, Stephen F. (London, TN); Dress, William B. (Camas, WA)

2010-02-02T23:59:59.000Z

254

AN ULTRA-STEEP-SPECTRUM RADIO RELIC IN THE GALAXY CLUSTER A2443  

SciTech Connect (OSTI)

We present newly discovered radio emission in the galaxy cluster A2443 which (1) is diffuse, (2) has an extremely steep spectrum, (3) is offset from the cluster center, (4) is of irregular morphology, and (5) is not clearly associated with any of the galaxies within the cluster. The most likely explanation is that this emission is a cluster radio relic associated with a cluster merger. We present deep observations of A2443 at multiple low frequencies (1425, 325, and 74 MHz) which help characterize the spectrum and morphology of this relic. Based on the curved spectral shape of the relic emission and the presence of small-scale structure, we suggest that this new source is likely a member of the radio phoenix class of radio relics.

Cohen, A. S.; Clarke, T. E., E-mail: aaron_cohen@alum.mit.edu [Naval Research Laboratory, Code 7213, Washington, DC 20375 (United States)

2011-05-15T23:59:59.000Z

255

X-RAYS FROM A RADIO-LOUD COMPACT BROAD ABSORPTION LINE QUASAR 1045+352 AND THE NATURE OF OUTFLOWS IN RADIO-LOUD BROAD ABSORPTION LINE QUASARS  

SciTech Connect (OSTI)

We present new results on X-ray properties of radio-loud broad absorption line (BAL) quasars and focus on broadband spectral properties of a high-ionization BAL (HiBAL) compact steep spectrum (CSS) radio-loud quasar 1045+352. This HiBAL quasar has a very complex radio morphology indicating either strong interactions between a radio jet and the surrounding interstellar medium or a possible re-start of the jet activity. We detected 1045+352 quasar in a short 5 ksec Chandra ACIS-S observation. We applied theoretical models to explain spectral energy distribution of 1045+352 and argue that non-thermal, inverse-Compton (IC) emission from the innermost parts of the radio jet can account for a large fraction of the observed X-ray emission. In our analysis, we also consider a scenario in which the observed X-ray emission from radio-loud BAL quasars can be a sum of IC jet X-ray emission and optically thin corona X-ray emission. We compiled a sample of radio-loud BAL quasars that were observed in X-rays to date and report no correlation between their X-ray and radio luminosity. However, the radio-loud BAL quasars show a large range of X-ray luminosities and absorption columns. This is consistent with the results obtained earlier for radio-quiet BAL quasars and may indicate an orientation effect in BAL quasars or more complex dependence between X-ray emission, radio emission, and an orientation based on the radio morphology.

Kunert-Bajraszewska, Magdalena; Katarzynski, Krzysztof [Torun Centre for Astronomy, N. Copernicus University, Gagarina 11, 87-100 Torun (Poland); Siemiginowska, Aneta [Harvard Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States); Janiuk, Agnieszka [N. Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw (Poland)

2009-11-10T23:59:59.000Z

256

Centralized Collaborative Compressed Sensing of Wideband Spectrum for Cognitive Radios  

E-Print Network [OSTI]

1 Centralized Collaborative Compressed Sensing of Wideband Spectrum for Cognitive Radios Hessam, spectrum sensing, cognitive radio, distri- bution discontinuities, algebraic detection, wideband. I technique for cognitive radio systems which combines algebraic tools and compressive sampling techniques

Paris-Sud XI, Université de

257

Spectrum Auction Framework for Access Allocation in Cognitive Radio Networks  

E-Print Network [OSTI]

1 Spectrum Auction Framework for Access Allocation in Cognitive Radio Networks Gaurav S. Kasbekar does not exist. Index Terms Cognitive Radio Networks, Spectrum Auctions, Algorithms I. INTRODUCTION, Wireless Meteropolitan Area networks etc., demand for radio spectrum is increasing. Currently, spectrum

Sarkar, Saswati

258

Optimal Classifier Based Spectrum Sensing in Cognitive Radio Wireless Systems  

E-Print Network [OSTI]

Optimal Classifier Based Spectrum Sensing in Cognitive Radio Wireless Systems Siddharth Sharma tolerance. General Terms Algorithms, Theory, Reliability. Keywords Cognitive Radio; Cooperative Spectrum Cognitive radio (CR) networks have been proposed as a revolutionary breakthrough to enhance spectrum

Jagannatham, Aditya K.

259

Ngociation de spectre dans les rseaux de radio cognitive  

E-Print Network [OSTI]

1 Négociation de spectre dans les réseaux de radio cognitive Rapport de recherche - Juin 2013 ................................................................................................................................... 4 I. Chapitre I : Réseaux de radio cognitive)............................................................................................... 6 I.3 Radio cognitive

Paris-Sud XI, Université de

260

Cognitive Radio Network {swjang, sbahk}@netlab.snu.ac.kr  

E-Print Network [OSTI]

2010 Cognitive Radio Network , , {swjang, sbahk}@netlab.snu.ac.kr Analysis of Average Opportunities in Cognitive Radio Networks Seowoo Jang, Saewoong Bahk INMC, EECS, Seoul National University Cognitive Radio Network . Primary user

Bahk, Saewoong

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


261

The Identification of EGRET Sources with Flat-Spectrum Radio Sources  

E-Print Network [OSTI]

We present a method to assess the reliability of the identification of EGRET sources with extragalactic radio sources. We verify that EGRET is detecting the blazar class of AGN. However, many published identifications are found to be questionable. We provide a table of 42 blazars which we expect to be robust identifications of EGRET sources. This includes one previously unidentified EGRET source, the lensed AGN PKS 1830-210 near the direction of the Galactic center. We provide the best available positions for 16 more radio sources which are also potential identifications for previously unidentified EGRET sources. All high Galactic latitude EGRET sources (b>3 degrees) which demonstrate significant variability can be identified with flat spectrum radio sources. This suggests that EGRET is not detecting any type of AGN other than blazars. This identification method has been used to establish with 99.998% confidence that the peak gamma-ray flux of a blazar is correlated with its average 5 GHz radio flux. An even better correlation is seen between gamma-ray flux and the 2.29 GHz flux density measured with VLBI at the base of the radio jet. Also, using high confidence identifications, we find that the radio sources identified with EGRET sources have larger correlated VLBI flux densities than the parent population of flat radio spectrum sources.

J. R. Mattox; J. Schachter; L. Molnar; R. C. Hartman; A. R. Patnaik

1996-12-18T23:59:59.000Z

262

THE 5 GHz ARECIBO SEARCH FOR RADIO FLARES FROM ULTRACOOL DWARFS  

SciTech Connect (OSTI)

We present the results of a 4.75 GHz survey of 33 brown dwarfs and one young exoplanetary system for flaring radio emission, conducted with the 305 m Arecibo radio telescope. The goal of this program was to detect and characterize the magnetic fields of objects cooler than spectral type L3.5, the coolest brown dwarf detected prior to our survey. We have also attempted to detect flaring radio emission from the HR 8799 planetary system, guided by theoretical work indicating that hot, massive exoplanets may have strong magnetic fields capable of generating radio emission at GHz frequencies. We have detected and confirmed radio flares from the T6.5 dwarf 2MASS J10475385+2124234. This detection dramatically extends the temperature range over which brown dwarfs appear to be at least sporadic radio-emitters, from 1900 K (L3.5) down to 900 K (T6.5). It also demonstrates that the utility of radio detection as a unique tool to study the magnetic fields of substellar objects extends to the coolest dwarfs, and, plausibly to hot, massive exoplanets. We have also identified a single, 3.6{sigma} flare from the L1 dwarf, 2MASS J1439284+192915. This detection is tentative and requires confirmation by additional monitoring observations.

Route, Matthew; Wolszczan, Alexander, E-mail: mroute@astro.psu.edu, E-mail: alex@astro.psu.edu [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States)

2013-08-10T23:59:59.000Z

263

DISCOVERY OF THE DISTURBED RADIO MORPHOLOGY IN THE INTERACTING BINARY QUASAR FIRST J164311.3+315618  

SciTech Connect (OSTI)

We report the high-resolution radio observations and the subsequent analysis of the radio-loud compact steep spectrum quasar FIRST J164311.3+315618, one of the members of a binary system. The second component of the system is a radio-quiet active galactic nucleus. The projected separation of this pair is 2.''3 (15 kpc); it is one of the smallest-known-separation binary quasars. The multi-band images of this binary system made with the Hubble Space Telescope show that the host galaxy of the radio-loud quasar is highly disturbed. The radio observations presented here were made with the Multi-Element Radio-Linked interferometer network (MERLIN) at 1.66 GHz and 5 GHz. We show that the radio morphology of FIRST J164311.3+315618 is complex on both frequencies and exhibits four components that indicate the intermittent activity with a possible rapid change of the jet direction and/or restarting of the jet due to the interaction with the companion. The radio components that are no longer powered by the jet can quickly fade away. We suggest that this makes the potential distortions of the radio structure short-lived phenomena. Our numerical simulations show that the influence of the companion can lead to prolonged current and future activities. FIRST J164311.3+315618 is an unusual and statistically very rare low redshift binary quasar wherein the first close encounter is probably just taking place.

Kunert-Bajraszewska, Magdalena [Torun Centre for Astronomy, Nicolaus Copernicus University, 87-100 Torun (Poland); Janiuk, Agnieszka, E-mail: magda@astro.uni.torun.pl [Center for Theoretical Physics, Polish Academy of Sciences, Aleja Lotnikow 32/46, 02-668 Warsaw (Poland)

2011-08-01T23:59:59.000Z

264

Telecommunications Emergency Alert System (EAS) Radio  

E-Print Network [OSTI]

Telecommunications Emergency Alert System (EAS) Radio 1. Send completed form to Mail Stop will be charged for a replacement. If the radio malfunctions, please contact Telecommunications. Texas A Departmental Approval Signature Date Service Date Desired Telecommunications Office Use Only Service Due Date

265

Spectrum Sensing Techniques in Cognitive Radio Communications  

E-Print Network [OSTI]

1 Spectrum Sensing Techniques in Cognitive Radio Communications Mario Bkassiny*, Yang Li, Georges for CR's. Index Terms-- Cognitive radio, cooperative spectrum sensing, dynamic spectrum access, energy, jayaweera, christos}@ece.unm.edu Abstract-- In this paper, we review some of the recent patents on spectrum

Jayaweera, Sudharman K.

266

Broadband Wireless Cognitive Radio-I  

E-Print Network [OSTI]

spectrum usage! #12;CMPE 591 - Broadband Wireless Networks 6 Cognitive Radio "Cognitive Radio" is the key portions of the spectrum is available and detect the presence of licensed users when a user operates in a licensed band. (Spectrum Sensing) 2. Select the best available channel. (Spectrum Decision) 3. Coordinate

Tuðcu, Tuna

267

Commercial Mobile Radio Service (WRI CMRS)  

E-Print Network [OSTI]

Commercial Mobile Radio Service (WRI ­ CMRS) Commercial Motor Vehicle Roadside Technology Corridor · Improved safety of CMVs and their operation · Reductions in accidents · Increased productivity and mobility · CMRS ­ Commercial Mobile Radio Services · Includes telematics devices (such as electronic on

268

NATIONAL RADIO ASTRONOMY OBSERVATORY CHARLOTTESVILLE, VIRGINIA  

E-Print Network [OSTI]

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

Groppi, Christopher

269

A survey for high-redshift radio-loud quasars: optical spectroscopy of S > 0.2 Jy, flat-spectrum radio sources  

E-Print Network [OSTI]

We present optical spectroscopic data for a complete sample of 161 S_5GHz >= 0.2 Jy, flat-spectrum radio sources. The sources were observed as part of a survey for high redshift, radio-loud quasars, and were selected for spectroscopic follow-up based on criteria of red optical colour and unresolved optical counterpart, as measured from APM scans of POSS-I plates. 13 objects from the spectroscopic sample were found to be radio-loud quasars with z > 3, of which two were previously known. We give positions, E (red) magnitudes, O-E colours, 5GHz radio fluxes, radio spectral indices, optical spectra and redshifts where possible for the spectroscopic sample. We also give finding charts for the z > 3 QSOs. The highest redshift object found is a QSO with z = 4.30 (GB1508+5714, the subject of an earlier Letter). The sample also contains a z = 3.05 QSO, GB1759+7539, which is optically very luminous (E=16.1). In addition, spectra are given for 18 S_5GHz >= 0.2 Jy, flat-spectrum radio sources that do not form part of the complete sample.

I. M. Hook; R. G. McMahon; M. J. Irwin; C. Hazard

1996-08-20T23:59:59.000Z

270

PowerPoint Presentation  

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

Carlos Apache Tribe Carlos Apache Tribe San Carlos Apache Mission Statement The Apache People will live a balanced life in harmony with spirituality, culture, language, and family unity in an ever-changing world. The Apache People shall create a strategic framework for our tribe to grow and prosper. San Carlos Apache Tribe And Reservation * Membership: approx 15,000 * Unemployment rate: 67% * 11 member tribal council * Apache Gold Casino * 1.83 million acres. * 800,000+ acres wooded/forested. * 1M ac. riparian/ grasslands/desert. * 2nd highest rated level of solar resource potential San Carlos Apache Reservation S a n C a r l o s A p a c h e T r i b e 2008 - 2013 Energy Initiatives * 2008: DOE ARRA Energy grant (TA/Energy Plan/lighting retrofits, solar at radio station/1 st

271

Spectrum hole identification and exploitation in cognitive radio networks.  

E-Print Network [OSTI]

??Cognitive radio networks are envisaged as the solution for effective spectrum management for the future communications. In a cognitive radio network, the unlicensed users are (more)

Vamsi Krishna Tumuluru.

2011-01-01T23:59:59.000Z

272

PowerPoint Presentation  

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

Presented by: Upgrades to Engineering Controls, Administrative Controls, Worker Training, Industrial Hygiene Procedures, Occupational Medicine Programs and Oversight 2009-Present...

273

The Radio Afterglow From GRB 980519: A Test of the Jet and Circumstellar Models  

E-Print Network [OSTI]

We present multi-frequency radio observations from the afterglow of GRB 980519 beginning 7.2 hours after the gamma-ray burst and ending 63 days later. The fast decline in the optical and X-ray light curves for this burst has been interpreted either as afterglow emission originating from a collimated outflow -- a jet -- or the result of a blast wave propagating into a medium whose density is shaped by the wind of an evolved massive star. These two models predict divergent behavior for the radio afterglow, and therefore, radio observations are capable, in principle, of discriminating between the two. We show that a wind model describes the subsequent evolution of the radio afterglow rather well. However, we see strong modulation of the light curve, which we interpret as diffractive scintillation. These variations prevent us from decisively rejecting the jet model.

D. A. Frail; S. R. Kulkarni; R. Sari; G. B. Taylor; D. S. Shepherd; J. S. Bloom; C. H. Young; L. Nicastro; N. Masetti

1999-10-04T23:59:59.000Z

274

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network [OSTI]

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

J. L. Payne; M. D. Filipovi?; E. J. Crawford; A. Y. De Horta; G. L. White; F. H. Stootman

2008-04-29T23:59:59.000Z

275

Optical Spectra of Radio Planetary Nebulae in the Small Magellanic Cloud  

E-Print Network [OSTI]

We present preliminary results from spectral observations of four candidate radio sources co-identified with known planetary nebulae (PNe) in the Small Magellanic Cloud (SMC). These were made using the Radcliffe 1.9-meter telescope in Sutherland, South Africa. These radio PNe were originally found in Australia Telescope Compact Array (ATCA) surveys of the SMC at 1.42 and 2.37 GHz, and were further confirmed by new high resolution ATCA images at 6 and 3 cm (4"/2"). Optical PNe and radio candidates are within 2" and may represent a subpopulation of selected radio bright objects. Nebular ionized masses of these objects may be 2.6 MSol or greater, supporting the existence of PNe progenitor central stars with masses up to 8 MSol.

Payne, J L; Crawford, E J; De Horta, A Y; White, G L; Stootman, F H

2008-01-01T23:59:59.000Z

276

VIRTUAL PRESENTERS: TOWARDS INTERACTIVE VIRTUAL PRESENTATIONS  

E-Print Network [OSTI]

the interesting parts of a sculpture or painting, addressing one, several or all persons in his or her audience be a painting, displayed and explained in a virtual museum environment. There are many examples of research they aim at giving the presentation task to a robot or virtual agent. In the latter case we can have one

Nijholt, Anton

277

High power radio frequency attenuation device  

DOE Patents [OSTI]

A resistor device for attenuating radio frequency power includes a radio frequency conductor connected to a series of fins formed of high relative magnetic permeability material. The fins are dimensional to accommodate the skin depth of the current conduction therethrough, as well as an inner heat conducting portion where current does not travel. Thermal connections for air or water cooling are provided for the inner heat conducting portions of each fin. Also disclosed is a resistor device to selectively alternate unwanted radio frequency energy in a resonant cavity.

Kerns, Quentin A. (Bloomingdale, IL); Miller, Harold W. (Winfield, IL)

1984-01-01T23:59:59.000Z

278

The 2dF Galaxy Redshift Survey: Clustering properties of radio galaxies  

E-Print Network [OSTI]

The clustering properties of local, S_{1.4 GHz} > 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the FIRST and 2dF Galaxy Redshift surveys. To this aim, we present 271 new bj < 19.45 spectroscopic counterparts of FIRST radio sources to be added to those already introduced in Magliocchetti et al. (2002). The two-point correlation function for the local radio population is found to be entirely consistent with estimates obtained for the whole sample of 2dFGRS galaxies. We estimate the parameters of the real-space correlation function xi(r)=(r/r_0)^{-\\gamma}, r_0=6.7^{+0.9}_{-1.1} Mpc and \\gamma=1.6\\pm 0.1, where h=0.7 is assumed. Different results are instead obtained if we only consider sources that present signatures of AGN activity in their spectra. These objects are shown to be very strongly correlated, with r_0=10.9^{+1.0}_{-1.2} Mpc and \\gamma=2\\pm 0.1, a steeper slope than has been claimed in other recent works. No difference is found in the clustering properties of radio-AGNs of different radio luminosity. These results show that AGN-fuelled sources reside in dark matter halos more massive than \\sim 10^{13.4} M_{\\sun}},higher the corresponding figure for radio-quiet QSOs. This value can be converted into a minimum black hole mass associated with radio-loud, AGN-fuelled objects of M_{BH}^{min}\\sim 10^9 M_{\\sun}. The above results then suggest -at least for relatively faint radio objects -the existence of a threshold black hole mass associated with the onset of significant radio activity such as that of radio-loud AGNs; however, once the activity is triggered, there appears to be no evidence for a connection between black hole mass and level of radio output. (abridged)

Manuela Magliocchetti; Steve J. Maddox; Ed Hawkins; John A. Peacock; Joss Bland-Hawthorn; Terry Bridges; Russell Cannon; Shaun Cole; Matthew Colless; Chris Collins; Warrick Couch; Gavin Dalton; Roberto de Propris; Simon P. Driver; George Efstathiou; Richard S. Ellis; Carlos S. Frenk; Karl Glazebrook; Carole A. Jackson; Bryn Jones; Ofer Lahav; Ian Lewis; Stuart Lumsden; Peder Norberg; Bruce A. Peterson; Will Sutherland; Keith Taylor

2004-02-21T23:59:59.000Z

279

Spectrum Leasing via Distributed Cooperation in Cognitive Radio  

E-Print Network [OSTI]

Spectrum Leasing via Distributed Cooperation in Cognitive Radio Igor Stanojev1 , Osvaldo Simeone1 for cognitive radio. I. INTRODUCTION Cognitive radio is a debated new paradigm for efficient spectrum or unlicensed model [1], requires secondary users to first sense the radio environment in search of spectrum

Yener, Aylin

280

Spectrum Leasing via Distributed Cooperation in Cognitive Radio  

E-Print Network [OSTI]

Spectrum Leasing via Distributed Cooperation in Cognitive Radio Igor Stanojev1, Osvaldo Simeone1 for cognitive radio. I. INTRODUCTION Cognitive radio is a debated new paradigm for efficient spectrum or unlicensed model [1], requires secondary users to first sense the radio environment in search of spectrum

Simeone, Osvaldo

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


281

Collaborative Spectrum Sensing from Sparse Observations in Cognitive Radio Networks  

E-Print Network [OSTI]

1 Collaborative Spectrum Sensing from Sparse Observations in Cognitive Radio Networks Jia (Jasmine for the implementation of cognitive radio. Collaborative spectrum sensing among the cognitive radio nodes is expected to improve the ability of checking complete spectrum usage. Due to hardware limitations, each cognitive radio

Yin, Wotao

282

Demonstration of Real-time Spectrum Sensing for Cognitive Radio  

E-Print Network [OSTI]

Demonstration of Real-time Spectrum Sensing for Cognitive Radio Zhe Chen, Nan Guo, and Robert C sensing detects the availability of the radio frequency spectrum in a real-time fashion, which is essen Cognitive radio (CR) has been put forward to make effi- cient use of scarce radio frequency spectrum

Qiu, Robert Caiming

283

Two Phase Spectrum Sharing for Frequency-Agile Radio Networks  

E-Print Network [OSTI]

1 Two Phase Spectrum Sharing for Frequency-Agile Radio Networks Zhenhua Feng and Yaling Yang of modern radios. We solve a joint spectrum sharing and end-to-end rate control problems for general technologies (e.g. software defined radio and cognitive radios) enable more flexible spectrum access through

Ha, Dong S.

284

SAMER: Spectrum Aware Mesh Routing in Cognitive Radio Networks  

E-Print Network [OSTI]

SAMER: Spectrum Aware Mesh Routing in Cognitive Radio Networks SHORT PAPER Ioannis Pefkianakis1 in licensed bands, to meet the increasing demand for radio spectrum. The new open spectrum operation--Cognitive Radio, Spectrum Aware Routing I. INTRODUCTION Cognitive radio networks (CORNET) are an emerging multihop

Lu, Songwu

285

Partial Cooperation for Spectrum Sharing in Cognitive Radio Network  

E-Print Network [OSTI]

Partial Cooperation for Spectrum Sharing in Cognitive Radio Network Lok Man Law1, Fen Hou2, Jianwei that many licensed radio spectrums are heavily under-utilized. Cognitive radio technology can improve spectrum, without affecting the normal communications of the primary licensed users. In cognitive radio

Paris-Sud XI, Université de

286

Partial Cooperation for Spectrum Sharing in Cognitive Radio Network  

E-Print Network [OSTI]

that many licensed radio spectrums are heavily under-utilized. Cognitive radio technology can improve spectrum, without affecting the normal communications of the primary licensed users. In cognitive radioPartial Cooperation for Spectrum Sharing in Cognitive Radio Network Lok Man Law1, Fen Hou2, Jianwei

Huang, Jianwei

287

Cooperative Opportunistic Large Array Approach for Cognitive Radio Networks  

E-Print Network [OSTI]

clearly shows that the licensed radio spectrum is underutilized continuously across time and space [1 to the radio spectrum congestion problem by opportunistic uses of the spectral holes to achieve efficient use created huge demand of radio spectrum. The radio spectrum is a scarce natural resource. Due

Hansen, René Rydhof

288

Utilisation des Protocoles HARQ pour la Radio Cognitive  

E-Print Network [OSTI]

Utilisation des Protocoles HARQ pour la Radio Cognitive Romain Tajan encadré/01/2012 #12;Plan 1 Introduction 2 La Radio Cognitive Techniques de la Radio Cognitive Méthodes d'accès 3 performances du protocole IR-HARQ 4 Utilisation des protocoles HARQ pour la Radio Cognitive Utilisation de l

Dobigeon, Nicolas

289

Energy Efficient Transmissions In MIMO Cognitive Radio Networks  

E-Print Network [OSTI]

Energy Efficient Transmissions In MIMO Cognitive Radio Networks Liqun Fu The Institute of Network@ie.cuhk.edu.hk Abstract-In this paper, we consider energy efficient transmis sions for MIMO cognitive radio networks. Index Terms-Cognitive radio networks, MIMO, Energy efficiency. I. INTRODUCTION Cognitive radio, which

Huang, Jianwei

290

ERAD 2014 Presentations  

Broader source: Energy.gov [DOE]

2014 ENVIRONMENTAL/RADIOLOGICAL ASSISTANCE DIRECTORY (ERAD) PRESENTATIONS Below are the presentations presented during the 2014 Environmental/Radiological Assistance Directory (ERAD) meetings: Visual Sample Plan (VSP), DOECAP, Radiological and Environmental Sciences Laboratory (RESL) MAPEP

291

Owens Valley Radio ObsevatoryOwens Valley Radio Obsevatory David Woody  

E-Print Network [OSTI]

Owens Valley Radio ObsevatoryOwens Valley Radio Obsevatory David Woody Owens Valley Radio · [Need pictures of the telescopes] 1/24/2008 2Woody #12;The Owens ValleyThe Owens Valley 1/24/2008 3Woody in the future · 40 m ­ 1960s ­ 1-20 GHz ­ Long history single dish and VLBI · VLBA antenna, 25 m dia · Misc. ­ 5

Weinreb, Sander

292

Bisfuel links - Presentations  

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

Presentations Devens Gust - Lecture at American Chemical Society Meeting EFRC 2011 Summit and Forum Materials (presentations and videos) Pat Dehmer - talk at the Science for our...

293

IACT Publications and Presentations  

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

Publications and Presentations Peer-Reviewed Publications Conference Proceedings, Abstracts, Presentations, and Poster Sessions IACT-funded Master and Doctoral Theses September...

294

First Spectroscopic Imaging Observations of the Sun at Low Radio Frequencies with the Murchison Widefield Array Prototype  

E-Print Network [OSTI]

We present the first spectroscopic images of solar radio transients from the prototype for the Murchison Widefield Array, observed on 2010 March 27. Our observations span the instantaneous frequency band 170.9201.6 MHz. ...

Oberoi, Divya

295

Public safety radios must pool spectrum  

E-Print Network [OSTI]

The dynamic-spectrum-access research and development community is maturing technologies that will enable radios to share RF spectrum much more intensively. The adoption of DSA technologies by the public-safety community ...

Lehr, William Herndon

296

Spectral radio observations of a solar eclipse  

Science Journals Connector (OSTI)

Measurements were made of the 7 March, 1970 solar eclipse by the AFCRL Sagamore Hill Radio Observatory in Hamilton, Massachusetts, on the wavelengths of 0.86,...m...=0.96) occurred at eclipse maximum. Source flux...

R. M. Straka

1971-12-01T23:59:59.000Z

297

Radio Frequency Identification : regulating information privacy protection  

E-Print Network [OSTI]

As applications of Radio Frequency Identification (RFID) become more profuse, the technology itself is stirring up some controversy. Due to its potential for amassing large amounts of information about both people and ...

Laufer, Deanna (Deanna Raquel)

2007-01-01T23:59:59.000Z

298

Radio Wavelength Observatories within the Exploration Architecture  

E-Print Network [OSTI]

Observations at radio wavelengths address key problems in astrophysics, astrobiology, and lunar structure including the first light in the Universe (the Epoch of Reionization), the presence of magnetic fields around extrasolar planets, particle acceleration mechanisms, and the structure of the lunar ionosphere. Moreover, achieving the performance needed to address these scientific questions demands observations at wavelengths longer than those that penetrate the Earth's ionosphere, observations in extremely "radio quiet" locations such as the Moon's far side, or both. We describe a series of lunar-based radio wavelength interferometers of increasing capability. The Radio Observatory for Lunar Sortie Science (ROLSS) is an array designed to be deployed during the first lunar sorties (or even before via robotic rovers) and addressing particle acceleration and the lunar ionosphere. Future arrays would be larger, more capable, and deployed as experience is gained in working on the lunar surface.

J. Lazio; R. J. Macdowall; J. Burns; L. Demaio; D. L. Jones; K. W. Weiler

2007-01-26T23:59:59.000Z

299

Radio Sources in Low-Luminosity Active Galactic Nuclei. I. VLA Detections of Compact, Flat-Spectrum Cores  

E-Print Network [OSTI]

We report a 0.2" resolution, 15 GHz survey of a sample of 48 low-luminosity active galactic nuclei with the Very Large Array. Compact radio emission has been detected in 57% (17 of 30) of LINERs and low-luminosity Seyferts, at least 15 of which have a flat to inverted radio spectrum (alpha > -0.3). The compact radio cores are found in both type 1 (i.e. with broad Halpha) and type 2 (without broad Halpha) nuclei. The 2 cm radio power is significantly correlated with the emission-line ([OI] lambda6300) luminosity. While the present observations are consistent with the radio emission originating in star-forming regions, higher resolution radio observations of 10 of the detected sources, reported in a companion paper (Falcke et al. 2000), show that the cores are very compact (= 10^8K) and probably synchrotron self-absorbed, ruling out a starburst origin. Thus, our results suggest that at least 50% of low-luminosity Seyferts and LINERs in the sample are accretion powered, with the radio emission presumably coming from jets or advection-dominated accretion flows. We have detected only 1 of 18 `transition' (i.e. LINER + HII) nuclei observed, indicating their radio cores are significantly weaker than those of `pure' LINERs.

Neil M. Nagar; Heino Falcke; Andrew S. Wilson; Luis C. Ho

2000-05-18T23:59:59.000Z

300

EARS (Enhancing Access to the Radio Spectrum) PROGRAM: The radio spectrum is a finite but exceedingly valuable natural resource that  

E-Print Network [OSTI]

EARS (Enhancing Access to the Radio Spectrum) PROGRAM: The radio spectrum is a finite communications, among a multitude of others. During the last two decades, the use of the radio spectrum has on the topic of Enhancing Access to the Radio Spectrum. The charge to the workshop was "to identify

Cetiner, Bedri A.

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


301

Low Luminosity Radio Loud Active Galactic Nuclei  

E-Print Network [OSTI]

I review observational properties of low power radio loud AGN. High resolution VLBI observations allow the estimate of the jet velocity and orientation with respect to the line of sight and the determination of the Doppler factor. These data reveal rich structures, including two-sided jets and secondary components. New results on 1144+35, a giant radio source with superluminal motion are shown in detail.

G. Giovannini; M. Giroletti

2007-08-30T23:59:59.000Z

302

STEP Partner Presentation  

Broader source: Energy.gov [DOE]

STEP Partner Presentation, from the Tool Kit Framework: Small Town University Energy Program (STEP).

303

On the Possibility of Curvature Radiation from Radio Pulsars  

E-Print Network [OSTI]

We consider the widespread hypothesis that coherent curvature radiation is responsible for the radio emission of pulsars. The comparison of energy conservation and the published data and luminosities explicitely proves that coherent curvature radiation cannot be the source for the radio emission of pulsars for frequencies below a few GHz. At higher frequencies coherent curvature radiation can be ruled out because neither the observationally deduced emission heights nor the observed radius to frequency mapping can be reproduced by this mechanism. Our argumentation is in accordance with the more general critics (e.g. Melrose 1992) that no adequate bunching mechanism has been identified for coherent curvature radiation. We present 5 examples (0329+29, 0355+54, 0540+23, 1133+16, 1916+10) of pulsars whose high frequency (larger than 1.4. GHz, up to 32 GHz) luminosities are well known, and as a low frequency example the faintest radio pulsar 0655+64 of the Taylor et al (1993) sample.

H. Lesch; A. Jessner; M. Kramer; Th. Kunzl

1998-01-26T23:59:59.000Z

304

Radio detection of high-energy cosmic rays at the Pierre Auger Observatory  

E-Print Network [OSTI]

The southern Auger Observatory provides an excellent test bed to study the radio detection of extensive air showers as an alternative, cost-effective, and accurate tool for cosmic-ray physics. The data from the radio setup can be correlated with those from the well-calibrated baseline detectors of the Pierre Auger Observatory. Furthermore, human-induced radio noise levels at the southern Auger site are relatively low. We have started an R&D program to test various radio-detection concepts. Our studies will reveal Radio Frequency Interferences (RFI) caused by natural effects such as day-night variations, thunderstorms, and by human-made disturbances. These RFI studies are conducted to optimise detection parameters such as antenna design, frequency interval, antenna spacing and signal processing. The data from our initial setups, which presently consist of typically 3 - 4 antennas, will be used to characterise the shower from radio signals and to optimise the initial concepts. Furthermore, the operation of a large detection array requires autonomous detector stations. The current design is aiming at stations with antennas for two polarisations, solar power, wireless communication, and local trigger logic. The results of this initial phase will provide an important stepping stone for the design of a few tens kilometers square engineering array

A. M. van den Berg; for the Pierre Auger Collaboration

2007-08-13T23:59:59.000Z

305

Testing Relativistic Gravity with Radio Pulsars  

E-Print Network [OSTI]

Before the 1970s, precision tests for gravity theories were constrained to the weak gravitational fields of the Solar system. Hence, only the weak-field slow-motion aspects of relativistic celestial mechanics could be investigated. Testing gravity beyond the first post-Newtonian contributions was for a long time out of reach. The discovery of the first binary pulsar by Russell Hulse and Joseph Taylor in the summer of 1974 initiated a completely new field for testing the relativistic dynamics of gravitationally interacting bodies. For the first time the back reaction of gravitational wave emission on the binary motion could be studied. Furthermore, the Hulse-Taylor pulsar provided the first test bed for the orbital dynamics of strongly self-gravitating bodies. To date there are a number of pulsars known, which can be utilized for precision test of gravity. Depending on their orbital properties and their companion, these pulsars provide tests for various different aspects of relativistic dynamics. Besides tests of specific gravity theories, like general relativity or scalar-tensor gravity, there are pulsars that allow for generic constraints on potential deviations of gravity from general relativity in the quasi-stationary strong-field and the radiative regime. This article presents a brief overview of this modern field of relativistic celestial mechanics, reviews some of the highlights of gravity tests with radio pulsars, and discusses their implications for gravitational physics and astronomy, including the upcoming gravitational wave astronomy.

Norbert Wex

2014-02-23T23:59:59.000Z

306

Radio Planetary Nebulae in the Magellanic Clouds  

E-Print Network [OSTI]

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

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

2009-01-01T23:59:59.000Z

307

X-Ray Observations of Radio Galaxies  

E-Print Network [OSTI]

We review some of the ways that X-ray observations provide unique information on radio galaxies. Thermal bremsstrahlung X-ray emission provides detailed data on ambient densities and temperatures. These parameters in turn can be used for pressure balance calculations and can demonstrate how the ambient gas affects radio source structure. Additionally, many signatures of the interaction of radio jets and lobes with the hot gas are found in high resolution X-ray maps. Non-thermal X-ray emission from knots and hotspots of radio jets can give us constraints on the relativistic electron population for energies greater that that normally sampled in the radio (in the case of synchrotron emission) or can give us an independent estimate of the average magnetic field strength (if inverse Compton emission is the origin of the X-rays). From recent ROSAT HRI observations of 3C 390.3 and 3C 120, we show evidence that X-ray emission from knots and hotspots appears to be associated with regions of large gradients in the radio surface brightness; i.e. at the location of powerful shocks.

D. E. Harris

1998-04-20T23:59:59.000Z

308

Senior Debt Fastball Presentation  

Broader source: Energy.gov [DOE]

Plenary III: Project Finance and Investment Senior Debt Fastball Presentation Phillip Thomas, Senior Vice President of Commercial Lending, Heartland Bank

309

Portfolio Manager Overview Presentation  

Broader source: Energy.gov [DOE]

This presentation, given through the DOE's Technical Assitance Program (TAP), provides information on the Portfolio Manager Overview

310

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. This presentation was presented in a Wind Powering America webinar on August 15, 2012 and is now available through the Wind Powering America website.

Mai, T.

2012-08-01T23:59:59.000Z

311

Giant Metrewave Radio Telescope observations of X-shaped radio sources  

Science Journals Connector (OSTI)

......obtained GMRT data at 240 and 610 MHz for almost all the known X-shaped...all the sources at 240 and 610 MHz show the characteristic X-shape...supersonic or buoyant flow of radio plasma in an asymmetric gas distribution...the lobe into an elliptical atmosphere and that all radio galaxies......

Dharam Vir Lal; A. Pramesh Rao

2007-01-21T23:59:59.000Z

312

Deep Spitzer observations of infrared-faint radio sources: high-redshift radio-loud AGN?  

E-Print Network [OSTI]

Oliver,5 Nick Seymour15 and Jason Surace6 1 CSIRO Australia Telescope National Facility, PO Box 76 Telescope Large Area Survey (ATLAS: Norris et al. 2006) as radio sources with no observable IR counterpart) and Middelberg et al. (2008a) have identified 51 such sources out of 2002 radio sources in the ATLAS survey. So

Norris, Ray

313

Observing, modeling and predicting the effects of solar radio bursts on radio communications  

Science Journals Connector (OSTI)

The Sun is a source of broadband radio noise which can reach significantly high levels during outbursts associated with the time evolution of the activity cycle. The statistics point out that the maximum occurrence frequency and intensity of solar radio bursts (SRBs) are observed in the proximity of the activity maximum but relevant phenomena can occur also in the raising and declining phases of the cycle. Both theoretical estimations based on extensive statistical analyses carried out in recent years and direct observations performed in the past solar activity cycle indicate that solar radio bursts can interfere wireless communications as well as Global Navigation Satellite Systems (GNSS). In this work we briefly review the theoretical basis and the experimental evidences to date and we show the effectiveness of fast multichannel solar radiopolarimeters like the Trieste Solar Radio System in monitoring and predicting solar radio noise increase in the framework of Space Weather applications.

Mauro Messerotti

2008-01-01T23:59:59.000Z

314

Contamination of Cluster Radio Sources in the Measurement of the Thermal Sunyaev-Zel'dovich Angular Power Spectrum  

E-Print Network [OSTI]

We present a quantitative estimate of the confusion of cluster radio halos and galaxies in the measurement of the angular power spectrum of the thermal Sunyaev-Zel'dovich (SZ) effect. To achieve the goal, we use a purely analytic approach to both radio sources and dark matter of clusters by incorporating empirical models and observational facts together with some theoretical considerations. It is shown that the correction of cluster radio halos and galaxies to the measurement of the thermal SZ angular power spectrum is no more than 20% at $l>2000$ for observing frequencies $\

Wei Zhou; Xiang-Ping Wu

2003-09-26T23:59:59.000Z

315

EOS Land Validation Presentations  

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

EOS Land Validation Presentations EOS Land Validation Presentations Meeting: Land Cover Validation Workshop Date: February 2, 2004 Place: Boston, MA Title: Validation Data Support Activities at the ORNL DAAC (Power Point) Presenter: Bob Cook Meeting: Fall 2003 American Geophysical Union (AGU) Meeting Date: December 9, 2003 Place: San Francisco, CA Title: Ground-Based Data Supporting the Validation of MODIS Land Products (Power Point) Presenter: Larry Voorhees Meeting: Terra and Aqua Products Review Date: March 2003 Place: NASA HQ Title: Supporting the Validation of MODIS Land Products (Power Point) Presenter: Larry Voorhees Meeting: Terra and Aqua Products Review Date: March 2003 Place: NASA HQ Title: MODIS Land Summary (Power Point) Presenter: Chris Justice, University of Maryland Meeting: Spring 2002 American Geophysical Union (AGU) Meeting

316

PowerPoint Presentation  

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

Working Session Working Session Presented to: Transportation External Coordination Rail Topic Group Transportation External Coordination Rail Topic Group Presented by: Presented by: Chair, Jay Jones Office of National Transportation March 15 2006 March 15 2006 Washington, DC Washington, DC 2 Agenda * Welcome and Introduction * Roll Call * Status/Update on Rail Topic Group at large * Update/Discussion from Individual Subgroups * Summary of CSG/Midwest Routing Project * Update of CSG/NE Routing Project * TRAGIS Update * Wrap Up * Subgroup Breakout

317

PowerPoint Presentation  

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

Update Update Presented to: Presented to: Transportation External Coordination Working Group Transportation External Coordination Working Group Presented by: Presented by: Jay Jones Jay Jones Office of National Transportation Office of National Transportation September 21, 2005 September 21, 2005 Pueblo, CO Pueblo, CO 2 Summary * Summary of Previous Transportation External Coordination (TEC) Rail Topic Group meeting * Summary of meeting with rail industry * Proposed Topic Group activities * Current issues and next steps 3 Summary Previous TEC Rail Topic Group Meeting * Request the Office of National Transportation to wait for SRGs to submit individual routing recommendations * Update from SRGs on their routing process * Topic Group recommendations: - Identified the need for Federal Railroad Administration

318

General Presentation Template  

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

Steve Pfaff August 8, 2013 Safety Culture Improvement: Past, Present, and Future PAST DNFSB Recommendation 2011-1, June 9, 2011, Safety Culture at the Waste Treatment and...

319

PowerPoint Presentation  

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

Demonstrate Engineering Design Process Illustrate Math and Science Concepts Explore Robot Concepts, Designs and Functions Exhibit and Vendor Area Presentation Nine Different...

320

SALC 2014 Presentations  

Broader source: Energy.gov [DOE]

This page provides links to DOE presentations given at the 2014 Illuminating Engineering Society Street and Area Lighting Conference (SALC), held September 14-17 in Nashville, TN.

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


321

Poster Presentation Purpose  

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

are usually done in groups, with observers milling around a large room of posters, the presentations are relaxed and more conducive to the exchange of ideas and...

322

Renewable Hydrogen (Presentation)  

SciTech Connect (OSTI)

Presentation about the United State's dependence on oil, how energy solutions are challenging, and why hydrogen should be considered as a long-term alternative for transportation fuel.

Remick, R. J.

2009-11-16T23:59:59.000Z

323

CEES Publications and Presentations  

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

CEES-Authored and Co-Authored Cover Stories Peer-Reviewed Publications Conference Proceedings, Abstracts, Presentations, and Poster Sessions Patents Frontiers in Energy Research...

324

Papers & Presentations- 2014  

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

Outlines Fiscal Year 2015 Goals Chris Barty Presents Talk at TIFR Colloquium September NIF Experiments Mimic Atmospheric Blast Effects Surrogate Capsule Experiments Study...

325

PowerPoint Presentation  

Energy Savers [EERE]

Priorities Presentation to the Commission to Review the Effectiveness of the National Energy Laboratories Dr. David T. Danielson September 15, 2014 2 DOE Mission: Enhance U.S....

326

Cognitive Radio will revolutionize American transportation  

ScienceCinema (OSTI)

Cognitive Radio will revolutionize American transportation. Through smart technology, it will anticipate user needs; detect available bandwidths and frequencies then seamlessly connect vehicles, infrastructures, and consumer devices; and it will support the Department of Transportation IntelliDrive Program, helping researchers, auto manufacturers, and Federal and State officials advance the connectivity of US transportation systems for improved safety, mobility, and environmental conditions. Using cognitive radio, a commercial vehicle will know its driver, onboard freight and destination route. Drivers will save time and resources communicating with automatic toll booths and know ahead of time whether to stop at a weigh station or keep rolling. At accident scenes, cognitive radio sensors on freight and transportation modes can alert emergency personnel and measure on-site, real-time conditions such as a chemical leak. The sensors will connect freight to industry, relaying shipment conditions and new delivery schedules. For industry or military purposes, cognitive radio will enable real-time freight tracking around the globe and its sensory technology can help prevent cargo theft or tampering by alerting shipper and receiver if freight is tampered with while en route. For the average consumer, a vehicle will tailor the transportation experience to the passenger such as delivering age-appropriate movies via satellite. Cognitive radio will enhance transportation safety by continually sensing what is important to the user adapting to its environment and incoming information, and proposing solutions that improve mobility and quality of life.

None

2013-12-06T23:59:59.000Z

327

Cognitive Radio will revolutionize American transportation  

SciTech Connect (OSTI)

Cognitive Radio will revolutionize American transportation. Through smart technology, it will anticipate user needs; detect available bandwidths and frequencies then seamlessly connect vehicles, infrastructures, and consumer devices; and it will support the Department of Transportation IntelliDrive Program, helping researchers, auto manufacturers, and Federal and State officials advance the connectivity of US transportation systems for improved safety, mobility, and environmental conditions. Using cognitive radio, a commercial vehicle will know its driver, onboard freight and destination route. Drivers will save time and resources communicating with automatic toll booths and know ahead of time whether to stop at a weigh station or keep rolling. At accident scenes, cognitive radio sensors on freight and transportation modes can alert emergency personnel and measure on-site, real-time conditions such as a chemical leak. The sensors will connect freight to industry, relaying shipment conditions and new delivery schedules. For industry or military purposes, cognitive radio will enable real-time freight tracking around the globe and its sensory technology can help prevent cargo theft or tampering by alerting shipper and receiver if freight is tampered with while en route. For the average consumer, a vehicle will tailor the transportation experience to the passenger such as delivering age-appropriate movies via satellite. Cognitive radio will enhance transportation safety by continually sensing what is important to the user adapting to its environment and incoming information, and proposing solutions that improve mobility and quality of life.

None

2013-07-22T23:59:59.000Z

328

Molecular gas in nearby powerful radio galaxies  

E-Print Network [OSTI]

We report the detection of CO(1-0) and CO(2-1) emission from the central region of nearby 3CR radio galaxies (z$gas content is below 10$^9$ \\msun. Their individual CO emission exhibit, for 5 cases, a double-horned line profile that is characteristic of an inclined rotating disk with a central depression at the rising part of its rotation curve. The inferred disk or ring distributions of the molecular gas is consistent with the observed presence of dust disks or rings detected optically in the cores of the galaxies. We reason that if their gas originates from the mergers of two gas-rich disk galaxies, as has been invoked to explain the molecular gas in other radio galaxies, then these galaxies must have merged a long time ago (few Gyr or more) but their remnant elliptical galaxies only recently (last 10$^7$ years or less) become active radio galaxies. Instead, we argue the the cannibalism of gas-rich galaxies provide a simpler explanation for the origin of molecular gas in the elliptical hosts of radio galaxies (Lim et al. 2000). Given the transient nature of their observed disturbances, these galaxies probably become active in radio soon after the accretion event when sufficient molecular gas agglomerates in their nuclei.

S. Leon; J. Lim; F. Combes; D. Van-Trung

2001-07-26T23:59:59.000Z

329

A REVIEW OF THE HISTORY, PRESENT STATUS, AND COURSE OF AMERICAN RADIO ASTRONOMY  

Science Journals Connector (OSTI)

...rapidly growing. In solar research, a vast amount...and some important solar-terrestrial relationships...particles, their initial energies, nor the precise means...Pulkovo telescope, as energy collectors. It will...this design is extremely economical, but the price paid...

F. D. Drake

1963-01-01T23:59:59.000Z

330

Money Matters Parent Presentation  

E-Print Network [OSTI]

Money Matters Parent Presentation Presented by Becky Lore June 7, 2014 #12;Money Matters · Dates.fcac-acfc.gc.ca · Gail Vaz-Oxlade My Money, My Choices www.gailvazoxlade.com · Money Mentors www.moneymentors.ca/ · Money

Seldin, Jonathan P.

331

Training Needs Assessment Presentation  

Broader source: Energy.gov [DOE]

The TNA PowerPoint Presentation is targeted for the training points of contacts whose organization's participate in the DOE training needs assessment (TNA). This presentation goes over how the training needs assessment (TNA) is done and the components of the TNA data collection tool.

332

Scientific Poster Presentations  

E-Print Network [OSTI]

Creating Scientific Poster Presentations Visual Rhetoric/Visual Literacy Series Overview: What go into constructing or manipulating an image. Definition of Genre: Scientific poster presentations proceedings. Keep text between 700 and 800 words for a standard 3-foot-by-5-foot poster. This amount of text

Ferrari, Silvia

333

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It is being presented at the Utility Variable-Generation Integration Group Fall Technical Workshop on October 24, 2012.

Hand, M.

2012-10-01T23:59:59.000Z

334

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented in a Power Systems Engineering Research Center webinar on September 4, 2012.

Mai, T.

2012-08-01T23:59:59.000Z

335

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented in an Union of Concerned Scientists webinar on June 12, 2012.

Hand, M.; Mai, T.

2012-08-01T23:59:59.000Z

336

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented in a webinar given by the California Energy Commission.

Hand, M. M.

2012-08-01T23:59:59.000Z

337

Radio Towers Geothermal Area | Open Energy Information  

Open Energy Info (EERE)

Radio Towers Geothermal Area Radio Towers Geothermal Area Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermal Resource Area: Radio Towers Geothermal Area Contents 1 Area Overview 2 History and Infrastructure 3 Regulatory and Environmental Issues 4 Exploration History 5 Well Field Description 6 Geology of the Area 7 Geofluid Geochemistry 8 NEPA-Related Analyses (0) 9 Exploration Activities (0) 10 References Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":6,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"500px","height":"300px","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":43.03666667,"lon":-115.4566667,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

338

PowerPoint Presentation  

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

Topic Group Summary Topic Group Summary Presented to: Transportation External Coordination Working Group Presented by: Presented by: Dan King, Oneida Nation, Tribal Topic Group Member Dan King, Oneida Nation, Tribal Topic Group Member April 5, 2005, Spring 2005 April 5, 2005, Spring 2005 Phoenix, AZ Phoenix, AZ 2 Funding Issues - Considerations * Examination of overlapping jurisdictions * Reconsider half-mile limit * Include all public safety officials in training * Ongoing training - turnover of personnel * Recovery of money spent responding to accidents * Cultural resources cannot be replaced - used to sustain communities 3 Funding Issues - Recommendations * Lessons Learned from Department of Homeland Security * Provide direct funding to Tribes * Create simple application process * Appoint Tribal representatives on application

339

ON THE EVOLUTION OF THE CORES OF RADIO SOURCES AND THEIR EXTENDED RADIO EMISSION  

SciTech Connect (OSTI)

The work in this paper aims at determining the evolution and possible co-evolution of radio-loud active galactic nuclei (AGNs) and their cores via their radio luminosity functions (i.e., total and core RLFs, respectively). Using a large combined sample of 1063 radio-loud AGNs selected at low radio frequency, we investigate the RLF at 408 MHz of steep-spectrum radio sources. Our results support a luminosity-dependent evolution. Using core flux density data of the complete sample 3CRR, we investigate the core RLF at 5.0 GHz. Based on the combined sample with incomplete core flux data, we also estimate the core RLF using a modified factor of completeness. Both results are consistent and show that the comoving number density of radio cores displays a persistent decline with redshift, implying a negative density evolution. We find that the core RLF is obviously different from the total RLF at the 408 MHz band which is mainly contributed by extended lobes, implying that the cores and extended lobes could not be co-evolving at radio emission.

Yuan Zunli; Wang Jiancheng, E-mail: yuanzunli@ynao.ac.cn [National Astronomical Observatories, Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 (China)

2012-01-10T23:59:59.000Z

340

DETECTION OF FAST TRANSIENTS WITH RADIO INTERFEROMETRIC ARRAYS  

SciTech Connect (OSTI)

Next-generation radio arrays, including the Square Kilometre Array (SKA) and its pathfinders, will open up new avenues for exciting transient science at radio wavelengths. Their innovative designs, comprising a large number of small elements, pose several challenges in digital processing and optimal observing strategies. The Giant Metre-wave Radio Telescope (GMRT) presents an excellent test-bed for developing and validating suitable observing modes and strategies for transient experiments with future arrays. Here we describe the first phase of the ongoing development of a transient detection system for GMRT that is planned to eventually function in a commensal mode with other observing programs. It capitalizes on the GMRT's interferometric and sub-array capabilities, and the versatility of a new software backend. We outline considerations in the plan and design of transient exploration programs with interferometric arrays, and describe a pilot survey that was undertaken to aid in the development of algorithms and associated analysis software. This survey was conducted at 325 and 610 MHz, and covered 360 deg{sup 2} of the sky with short dwell times. It provides large volumes of real data that can be used to test the efficacies of various algorithms and observing strategies applicable for transient detection. We present examples that illustrate the methodologies of detecting short-duration transients, including the use of sub-arrays for higher resilience to spurious events of terrestrial origin, localization of candidate events via imaging, and the use of a phased array for improved signal detection and confirmation. In addition to demonstrating applications of interferometric arrays for fast transient exploration, our efforts mark important steps in the roadmap toward SKA-era science.

Bhat, N. D. R. [International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102 (Australia)] [International Centre for Radio Astronomy Research, Curtin University, Bentley, WA 6102 (Australia); Chengalur, J. N.; Gupta, Y.; Prasad, J.; Roy, J.; Kudale, S. S. [National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune 411007 (India)] [National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune 411007 (India); Cox, P. J.; Bailes, M.; Burke-Spolaor, S.; Van Straten, W. [Centre for Astrophysics and Supercomputing, Swinburne University, Hawthorn, Victoria 3122 (Australia)] [Centre for Astrophysics and Supercomputing, Swinburne University, Hawthorn, Victoria 3122 (Australia)

2013-05-01T23:59:59.000Z

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


341

Publications and Presentations  

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

Publications and Presentations Publications and Presentations News & Publications ESnet in the News ESnet News Publications and Presentations Galleries ESnet Awards and Honors Contact Us Technical Assistance: 1 800-33-ESnet (Inside the US) 1 800-333-7638 (Inside the US) 1 510-486-7600 (Globally) 1 510-486-7607 (Globally) Report Network Problems: trouble@es.net Provide Web Site Feedback: info@es.net Publications and Presentations Sort by: Date | Author | Type 2013 Dart E., Rotman L., Tierney B., Hester M., and Zurawski J., "The Science DMZ: A Network Design Pattern for Data-Intensive Science", IEEE/ACM Annual SuperComputing Conference (SC13), Denver CO, USA, November 19, 2013, LBNL LBNL-6366E Download File: sc13sciDMZ-final.pdf (pdf: 952 KB) Ezra Kissel, Martin Swany, Brian Tierney and Eric Pouyoul, "Efficient

342

ARM - 2008 STM Presentations  

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

Presentations Presentations 2008 Meeting 2008 Meeting Home Proceedings Sorted by Author Proceedings Sorted by Title Pictures Posters Presentations Meeting Archives ARM Science Team Meeting Proceedings Past Science Team Meetings 2008 STM Presentations Monday, March 10 ARM Orientation for New and Current PIs Chief Scientist's Perspective (PDF, 5.7MB) Warren Wiscombe ARM Instruments (PDF, 14.7MB) Jimmy Voyles Infrastructure (PDF, 643KB) Jim Mather How to Get Data (PDF, 2MB) Raymond McCord Working Group Sessions Cloud Modeling Working Group 2008 ARM STM Cloud Modeling Working Group Session Agenda (PDF, 11KB) Understanding and Improving CRM and GCM Simulations of Cloud Systems with ARM Observations (PDF, 272KB) Xiaoqing Wu and Qilong Min Interactions of Cumulus Convection and the Boundary Layer at the

343

Roadmap Integration Team Presentation  

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

Presentation Presentation NP03-00 Slide 1 Generation IV Technology Roadmap NERAC Meeting: Washington, D.C. September 30, 2002 Roadmap Integration Team Presentation NP03-00 Slide 2 NERAC Meeting September 30, 2002 Generation IV Technology Roadmap * Identifies systems deployable by 2030 or earlier * Specifies six systems that offer significant advances towards: - Sustainability - Economics - Safety and reliability - Proliferation resistance and physical protection * Summarizes R&D activities and priorities for the systems * Lays the foundation for Generation IV R&D program plans Roadmap Integration Team Presentation NP03-00 Slide 3 NERAC Meeting September 30, 2002 The Technical Roadmap Report * Discusses the benefits, goals and challenges, and the importance of the fuel cycle * Describes evaluation and selection process

344

Presentations | MMSNF 2013 Chicago  

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

Privacy and Security Notice Presentations Available Presentations from the Materials Modeling and Simulation of Nuclear Fuels (MMSNF) 2013 workshop. Presented on Presentation Title Authors Session Oct. 14, 2013 Welcome and announcements Ewing, Tom (ANL, USA) and Rosner, Robert (UC, USA) Opening Oct. 14, 2013 First-principles DFT+U modeling of paramagnetic UO2 and (U,Pu) mixed oxides [366KB, posted: Oct. 13, 2013 ] Dorado, Boris (CEA, DAM, DIF, France), Garcia, Philippe (CEA, DEN, DEC, France) Atomistic Models and Simulations Oct. 14, 2013 Computational study of energetics and defect-ordering tendencies for rare earth elements in uranium dioxide [1.5MB, posted: Oct. 28, 2013 ] Solomon, Jonathan M. (UC Berkeley, USA), Alexandrov, Vitaly (UC Berkeley, UC Davis, USA), Sadigh, Babak (LLNL, USA), Navrotsky, Alexandra (UC Davis, USA), Asta, Mark (UC Berkeley, UC Davis, USA) Atomistic Models and Simulations

345

NERSC Science Highlights Presentations  

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

User Surveys User Surveys HPC Requirements for Science HPC Workshop Reports NERSC Staff Publications & Presentations Journal Cover Stories Galleries Home » News & Publications » Publications & Reports » Science Highlights Presentations Science Highlights Presentations NERSC collects highlights of recent scientific work carried out by its users. If you are a user and have work that you would like us to highlight please send e-mail to consult@nersc.gov. December 2013 Presentation [PDF] Model Shows Arrangement of Proteins in Photosynthetic Membranes [Geissler] How Many Earths are There? [Petigura] Read more... IceCube is 2013 Physics Breakthrough of the Year [Gerhardt] Read more... Simulation Couples with Experiment to Boost Energy Research [Smith] Simulation Captures the Essence of Carbonate Crystallization [Whitelam]

346

Control the Present  

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

Control the Present Image of water sampling trip embarking downstream from Otowi Bridge onto the Rio Grande with text overlay of 'How does LANL minimize the impacts from ongoing...

347

Papers and Presentations - 2014  

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

and Presentations NIF&PS People In the News Press Kit S&TR Articles Contact LLNL Lawrence Livermore National Laboratory 7000 East Avenue * Livermore, CA 94550 Operated by...

348

CFSES Blue Team Presentations  

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

take you to the slides used in the presentation. Constraints on the Magnitude and Rate of CO2 Dissolution at Bravo Dome Natural Gas Field Marc Hesse (May, 2014) Nanoscale...

349

Presentations for Industry  

Broader source: Energy.gov [DOE]

Industrial energy managers, utilities, and energy management professionals can find online trainings and information dissemination at no-cost. AMO has provided these energy-saving strategies from leading manufacturing companies and energy experts through several different presentation series.

350

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050.

Mai, T.

2012-10-01T23:59:59.000Z

351

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050.

Mai, T.

2012-11-01T23:59:59.000Z

352

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050.

Mai, T.

2013-04-01T23:59:59.000Z

353

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050.

Hand, M. M.

2012-09-01T23:59:59.000Z

354

PowerPoint Presentation  

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

Presented by: Larry Romine, DOE-RL Mike Swartz, CHPRC 2 Problem Statement On 1213, ten individuals working in Room 232 and 235A-3 of Building 234-5Z were potentially exposed...

355

Hydrogen Fuel Quality (Presentation)  

SciTech Connect (OSTI)

Jim Ohi of NREL's presentation on Hydrogen Fuel Quality at the 2007 DOE Hydrogen Program Annual Merit Review and Peer Evaluation on May 15-18, 2007 in Arlington, Virginia.

Ohi, J.

2007-05-17T23:59:59.000Z

356

GIS TRANSFORMATIONS Conference Presentation  

E-Print Network [OSTI]

GIS TRANSFORMATIONS Conference Presentation Waldo Tobler Geography Department University, line, area, or field phenomena, then the sixteen common classes of transformation are: point -> point (scalar, vector, tensor) data, to obtain eighty distinct possible classes of transformation. The common

Tobler, Waldo

357

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented to the 2012 Western Conference of Public Service Commissioners, during their June, 2012, meeting. The Western Conference of Public Service Commissioners is a regional association within the National Association of Regulatory Utility Commissioners (NARUC).

Hand, M. M.

2012-08-01T23:59:59.000Z

358

Burst Radio-Frequency Excited Pulsed Hollow-Cathode Lamp  

Science Journals Connector (OSTI)

Transient emission characteristics of a hollow-cathode lamp driven by a pulsed current in combination with a radio-frequency burst signal are described. The radio-frequency field...

Araki, Tsutomu; Walters, John P; Minami, Shigeo

1980-01-01T23:59:59.000Z

359

Meeting Notes and Presentations  

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

Board Notes and Slides Board Notes and Slides Notes from EM Corporate QA Board Tele-Conference - February 22, 2010 1 of 2 General: Attendance of voting board members was documented. All members were present or had a representative present on the call. Previous 5 Focus Areas: Dave Tuttel presented the proposed closeout of the previous 5 focus areas for the EM Corporate Board. * Focus Area 1 (Requirements Flow Down) - Board voted to close the focus area (unanimous) * Focus Area 2 (Adequate NQA-1 Suppliers) - Board voted to close the focus area (unanimous) * Focus Area 3 (CGI and Services Dedication) - Board voted to close the focus area (unanimous) * Focus Area 4 (Graded Approach to QA) -Discussion noted that the area as a whole may need more work in the future focus areas even though the procurement piece is ready to close out. The discussion also noted

360

Calculating the probability of detecting radio signals from alien civilizations  

E-Print Network [OSTI]

Although it might not be self-evident, it is in fact entirely possible to calculate the probability of detecting alien radio signals by understanding what types of extraterrestrial radio emissions can be expected and what properties these emissions can have. Using the Drake equation as the obvious starting point, and logically identifying and enumerating constraints of interstellar radio communications can yield the probability of detecting a genuine alien radio signal.

Marko Horvat

2007-07-14T23:59:59.000Z

Note: This page contains sample records for the topic "testimony presentations radio" 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

Calculating the probability of detecting radio signals from alien civilizations  

E-Print Network [OSTI]

Although it might not be self-evident, it is in fact entirely possible to calculate the probability of detecting alien radio signals by understanding what types of extraterrestrial radio emissions can be expected and what properties these emissions can have. Using the Drake equation as the obvious starting point, and logically identifying and enumerating constraints of interstellar radio communications can yield the probability of detecting a genuine alien radio signal.

Horvat, Marko

2006-01-01T23:59:59.000Z

362

PowerPoint Presentation  

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

Department of Energy Department of Energy Transportation External Working Group (TEC) EDWARDS MOVING & RIGGING, INC. Heavy Transport Presentation Presented By What kind of projects do we do? Heavy Transport Heavy Rigging Focus today is Heavy Transport Focus today is Heavy Transport Turbine Generator Transformer Boilers Vessel Press Bridge Duct work Railroad Engine Tank Relocation 440T Building Solid Masonry Even a building facade "These guys can move anything" Pressurizer RA Movement of Hazardous Cargo Major Plant Components & Casks Cask Movement Shipment by Road Shipment by Road Shipment by Railroad Shipments by Barge What makes Transport Contactors Suited for these projects? Complete Package *Engineering *Planning *State-of-the-art-equipment

363

PowerPoint Presentation  

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

Rail Topic Group Transportation External Coordination Rail Topic Group Rail Topic Group Transportation External Coordination Rail Topic Group Presented by: Presented by: Cort Richardson Council of State Governments- Eastern Regional Conference March 15 2006 March 15 2006 Washington, DC Washington, DC 2 Rail Topic Group Summary * Since the last TEC meeting in September, the approach of the Topic Group was to divide into subgroups to address activities important to the Topic Group as a whole * The subgroups are: - Inspections - Tracking and Radiation Monitoring - Planning - Lessons Learned - TRAGIS - Legal Weight Truck Shipments

364

PowerPoint Presentation  

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

Transportation External Coordination Working Group Transportation External Coordination Working Group Presented by: Presented by: Jay Jones Jay Jones Office of National Transportation Office of National Transportation September 21, 2005 September 21, 2005 Pueblo, CO Pueblo, CO Tribal Topic Group Update 2 Summary * 2005 Tribal program priorities * Key Transportation External Coordination Tribal (TEC) Topic Group topics * TEC Tribal Topic Group meetings update * TEC Tribal Topic Group recommendations * Next steps -Tribal interaction approaches 3 2005 Tribal Program Priorities * Initiate consultation with Native American Tribes along potential transportation corridors Issue notification letter Contact Tribal leaders regarding notification letter - Begin holding discussions and/or meetings with Tribal

365

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented at Wind Powering America States Summit. The Summit, which follows the American Wind Energy Association's (AWEA's) annual WINDPOWER Conference and Exhibition, provides state Wind Working Groups, state energy officials, U.S. Energy Department and national laboratory representatives, and professional and institutional partners an opportunity to review successes, opportunities, and challenges for wind energy and plan future collaboration.

DeMeo, E.

2012-08-01T23:59:59.000Z

366

Renewable Electricity Futures (Presentation)  

SciTech Connect (OSTI)

This presentation library summarizes findings of NREL's Renewable Electricity Futures study, published in June 2012. RE Futures investigated the challenges and impacts of achieving very high renewable electricity generation levels in the contiguous United States by 2050. It was presented at the 2012 RE AMP Annual Meeting. RE-AMP is an active network of 144 nonprofits and foundations across eight Midwestern states working on climate change and energy policy with the goal of reducing global warming pollution economy-wide 80% by 2050.

Mai, T.

2012-08-01T23:59:59.000Z

367

No Radio Afterglow from the Gamma-Ray Burst of February 28, 1997  

E-Print Network [OSTI]

We present radio observations of the gamma-ray burster GRB 970228 made with the Very Large Array (VLA) and the Owens Valley Radio Observatory (OVRO) spanning a range of postburst timescales from one to 300 days. A search for a time-variable radio source was conducted covering an area which included a fading X-ray source and an optical transient, both of which are thought to be the long wavelength counterparts to the gamma-ray burst. At the position of the optical transient sensitive limits between 10 uJy and 1 mJy can be placed on the absence of a radio counterpart to GRB 970228 between 1.4 and 240 GHz. We apply a simple formulation of a fireball model which has been used with some success to reproduce the behavior of the optical and X-ray light curves. Using this model we conclude that the radio non-detections are consistent with the peak flux density of the afterglow lying between 20-40 uJy and it requires that the optical flux peaked between 4 and 16 hours after the burst.

D. A. Frail; S. R. Kulkarni; D. S. Shepherd; E. Waxman

1998-04-16T23:59:59.000Z

368

The number counts, luminosity functions and evolution of microwave-selected (WMAP) blazars and radio galaxies  

E-Print Network [OSTI]

(Abridged) We carried out an extensive search to identify the counterparts of all the sources listed in the WMAP 3-yr catalogue using literature and archival data. Our work led to the identification of 309 WMAP sources, 98% of which are blazars, radio quasars or radio galaxies. At present, 15 objects still remain without identification due to the lack of optical spectroscopic data or a clear radio counterpart. Our results allow us to define a flux limited sample of 203 high Galactic latitude microwave sources ($f_{41GHz} \\ge 1$ Jy, $|b_{\\rm II}| > 15^\\circ$) which is virtually completely identified (99%). The microwave band is ideally suited for blazar statistical studies since this is the part of the em spectrum that is least affected by the superposition of spectral components of different origin. Using this data-set we derived number counts, luminosity functions and cosmological evolution of blazars and radio galaxies at microwave frequencies. Our results are in good agreement with those found at radio fre...

Giommi, P; Padovani, P; Gasparrini, D; Cavazzuti, E; Cutini, S

2009-01-01T23:59:59.000Z

369

Molecular Gas in the Powerful Radio Nucleus of the Ultraluminous Infrared Galaxy PKS 1345+12  

E-Print Network [OSTI]

Millimeter CO(1-0) interferometry and high resolution, Hubble Space Telescope (HST) 1.1, 1.6, and 2.2 micron imaging of the radio compact galaxy PKS 1345+12 are presented. With an infrared luminosity of 2x10^{12} L_sun, PKS 1345+12 is a prime candidate for studying the link between the ultraluminous infrared galaxy phenomenon and radio galaxies. These new observations probe the molecular gas distribution and obscured nuclear regions of PKS 1345+12 and provide morphological support for the idea that the radio activity in powerful radio galaxies is triggered by the merger of gas rich galaxies. Two nuclei separated by 2" (4.0 kpc) are observed in the near-infrared; the extended southeastern nucleus has colors consistent with reddened starlight, and the compact northwestern nucleus has extremely red colors indicative of an optical quasar with a warm dust component. Further, the molecular gas, 3mm continuum, and radio emission are coincident with the redder nucleus, confirming that the northwestern nucleus is the site of the AGN and that the molecular gas is the likely fuel source.

A. S. Evans; D. -C. Kim; J. M. Mazzarella; N. Z. Scoville; D. B. Sanders

1999-07-28T23:59:59.000Z

370

A Comparison of the Extra Nuclear X-ray and Radio Features in M87  

E-Print Network [OSTI]

ROSAT High Resolution Imager (HRI) data from eight observations have been co-added to obtain an effective exposure of 230 ksec. We have identified a number of features and regions with excess X-ray brightness over that from a circularly symmetric model of the well known hot gas component. A prominent `spur' extends 4' from the vicinity of knot A towards the south-west. The brightness to the south and east of this spur is significantly higher than that to the north and west. Excess brightness is also found to the East of the nucleus, with a local maximum centered on the eastern radio lobe 3' from the core. There are two well known relationships between radio and x-ray emission for radio galaxies in clusters: coincidence of emissions because the X-rays come from inverse Compton or synchrotron processes; and anti-coincidence caused by exclusion of hot gas from radio entities. We present a radio/X-ray comparison to determine if either of these relationships can be isolated in M87. The greatest obstacle we face is the unknown projection which affects both bands.

D. E. Harris; F. Owen; J. A. Biretta; W. Junor

2000-02-24T23:59:59.000Z

371

High-Resolution Radio Imaging of Gravitational Lensing Candidates in the 1 Jansky BL Lac Sample  

E-Print Network [OSTI]

While BL Lacertae objects are widely believed to be highly beamed, low-luminosity radio galaxies, many radio-selected BL Lacs have extended radio power levels and optical emission lines that are too luminous to be low-luminosity radio galaxies. Also, Stocke & Rector discovered an excess of MgII absorption systems along BL Lac sightlines compared to quasars, suggesting that gravitational lensing may be another means of creating the BL Lac phenomenon in some cases. We present a search for gravitationally-lensed BL Lacs with deep, high-resolution, two-frequency VLA radio maps of seven lensing candidates from the 1 Jansky BL Lac sample. We find that none of these objects are resolved into an Einstein ring like B 0218+357, nor do any show multiple images of the core. All of the lensing candidates that were resolved show a flat-spectrum core and very unusual, steep-spectrum extended morphology that is incompatible with a multiply lensed system. Thus, while these observations do not rule out microlensing, no macrolensing is observed.

T. A. Rector; J. T. Stocke

2003-02-19T23:59:59.000Z

372

Powerful Radio Galaxies with Simbol-X: Lobes and Hot Spots  

SciTech Connect (OSTI)

We present here the first Simbol-X simulations of the extended components, lobes and hot spots, of the radio galaxies. We use the paradigmatic case of Pictor A to test the capabilities of Simbol-X in this field of studies. Simulations demonstrate that Simbol-X will be able not only to perform spatially resolved studies on the lobes of radio galaxies below 10 keV but also to observe, for the first time, hard X-ray emission from the hot spots. These extremely promising results show the considerable potentiality of Simbol-X in studying interaction phenomena between relativistic plasma and surrounding environment.

Migliori, G. [SISSA/ISAS, via Beirut 2-4, I-34014 Trieste (Italy); Grandi, P.; Raimondi, L.; Torresi, E. [INAF/IASF Bologna, viale Gobetti 101, I-40129 Bologna (Italy); Angelini, L. [NASA/Goddard Space Flight Center (United States); Palumbo, G. G. C. [Dipartimento di Astronomia, Universita di Bologna, via Ranzani 1, I-40127 Bologna (Italy)

2009-05-11T23:59:59.000Z

373

Characteristics of radio-frequency, atmospheric-pressure glow discharges with air using bare metal electrodes  

SciTech Connect (OSTI)

In this letter, an induced gas discharge approach is proposed and described in detail for obtaining a uniform atmospheric-pressure glow discharge with air in a {gamma} mode using water-cooled, bare metal electrodes driven by radio-frequency (13.56 MHz) power supply. A preliminary study on the discharge characteristics of the air glow discharge is also presented in this study. With this induced gas discharge approach, radio-frequency, atmospheric-pressure glow discharges using bare metal electrodes with other gases which cannot be ignited directly as the plasma working gas, such as nitrogen, oxygen, etc., can also be obtained.

Wang Huabo; Sun Wenting; Li Heping; Bao Chengyu; Zhang Xiaozhang [Department of Engineering Physics, Tsinghua University, Beijing 100084 (China)

2006-10-16T23:59:59.000Z

374

CHANDRA OBSERVATIONS OF 3C RADIO SOURCES WITH z < 0.3. II. COMPLETING THE SNAPSHOT SURVEY  

SciTech Connect (OSTI)

We report on the second round of Chandra observations of the 3C snapshot survey developed to observe the complete sample of 3C radio sources with z < 0.3 for 8 ks each. In the first paper, we illustrated the basic data reduction and analysis procedures performed for the 30 sources of the 3C sample observed during Chandra Cycle 9, while here we present the data for the remaining 27 sources observed during Cycle 12. We measured the X-ray intensity of the nuclei and of any radio hot spots and jet features with associated X-ray emission. X-ray fluxes in three energy bands, i.e., soft, medium, and hard, for all the sources analyzed are also reported. For the stronger nuclei, we also applied the standard spectral analysis, which provides the best-fit values of the X-ray spectral index and absorbing column density. In addition, a detailed analysis of bright X-ray nuclei that could be affected by pile-up has been performed. X-ray emission was detected for all the nuclei of the radio sources in our sample except for 3C 319. Among the current sample, there are two compact steep spectrum radio sources, two broad-line radio galaxies, and one wide angle tail radio galaxy, 3C 89, hosted in a cluster of galaxies clearly visible in our Chandra snapshot observation. In addition, we also detected soft X-ray emission arising from the galaxy cluster surrounding 3C 196.1. Finally, X-ray emission from hot spots has been found in three FR II radio sources and, in the case of 3C 459, we also report the detection of X-ray emission associated with the eastern radio lobe as well as X-ray emission cospatial with radio jets in 3C 29 and 3C 402.

Massaro, F. [SLAC National Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, 2575 Sand Hill Road, Menlo Park, CA 94025 (United States); Tremblay, G. R. [European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei Muenchen (Germany); Harris, D. E.; O'Dea, C. P. [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States); Kharb, P.; Axon, D. [Department of Physics, Rochester Institute of Technology, Carlson Center for Imaging Science 76-3144, 84 Lomb Memorial Dr., Rochester, NY 14623 (United States); Balmaverde, B.; Capetti, A. [INAF-Osservatorio Astrofisico di Torino, Strada Osservatorio 20, I-10025 Pino Torinese (Italy); Baum, S. A. [Carlson Center for Imaging Science 76-3144, 84 Lomb Memorial Dr., Rochester, NY 14623 (United States); Chiaberge, M.; Macchetto, F. D.; Sparks, W. [Space Telescope Science Institute, 3700 San Martine Drive, Baltimore, MD 21218 (United States); Gilli, R. [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Giovannini, G. [INAF-Istituto di Radioastronomia di Bologna, Via Gobetti 101, I-40129 Bologna (Italy); Grandi, P.; Torresi, E. [INAF-IASF-Istituto di Astrofisica Spaziale e fisica Cosmica di Bologna, Via P. Gobetti 101, I-40129 Bologna (Italy); Risaliti, G. [INAF-Osservatorio Astronomico di Arcetri, Largo E. Fermi 5, I-50125 Firenze (Italy)

2012-12-15T23:59:59.000Z

375

Generalized Formalisms of the Radio Interferometer Measurement Equation  

E-Print Network [OSTI]

The Radio Interferometer Measurement Equation (RIME) is a matrix-based mathematical model that describes the response of a radio interferometer. The Jones calculus it employs is not suitable for describing the analogue components of a telescope. This is because it does not consider the effect of impedance mismatches between components. This paper aims to highlight the limitations of Jones calculus, and suggests some alternative methods that are more applicable. We reformulate the RIME with a different basis that includes magnetic and mixed coherency statistics. We present a microwave network inspired 2N-port version of the RIME, and a tensor formalism based upon the electromagnetic tensor from special relativity. We elucidate the limitations of the Jones-matrix-based RIME for describing analogue components. We show how measured scattering parameters of analogue components can be used in a 2N-port version of the RIME. In addition, we show how motion at relativistic speed affects the observed flux. We present r...

Price, Danny C

2015-01-01T23:59:59.000Z

376

FastForward: High-Throughput Dual-Radio Streaming Gholamhossein Ekbatanifard  

E-Print Network [OSTI]

amount of data at high throughput and/or low latency. For example, structural health of the Golden Gate end-to-end throughput is limited to 1/2 the radio capacity. To bridge this performance gap we present Bridge was sampled at 1 KHz in [1]. Brimon, a railway monitoring system, generates about 7 KB in each

Kuzmanov, Georgi

377

Policy-Based Cognitive Radios David Wilkins, Grit Denker, Mark-Oliver Stehr,  

E-Print Network [OSTI]

Policy-Based Cognitive Radios David Wilkins, Grit Denker, Mark-Oliver Stehr, Daniel Elenius, Rukman: firstname.lastname@sri.com April 2, 2007 Abstract We present a new language for expressing policies that unanticipated policy types can be encoded. We also describe a Policy Reasoner that reasons about CoRaL policies

378

Deep ATLAS radio observations of the CDFS-SWIRE field Ray P. Norris1  

E-Print Network [OSTI]

1 Deep ATLAS radio observations of the CDFS-SWIRE field Ray P. Norris1 , José Afonso5 , Phil N, UK #12;2 Abstract We present the first results from the Australia Telescope Large Area Survey (ATLAS to detect highly-obscured, ultraluminous infrared galaxies (ULIRGs) at z>>1. SWIRE's goal is to trace

Norris, Ray

379

Multi-Link Level Simulation Model of Indoor Peer-to-Peer Radio Channels  

E-Print Network [OSTI]

1 Multi-Link Level Simulation Model of Indoor Peer-to-Peer Radio Channels Paolo Castiglione, Claude presents a link-simulation model for cooperative indoor communication systems at 2.4 GHz, based of this paper is to propose a multi-link simulation model for peer-to-peer cooperative (a.k.a. distributed

Gesbert, David

380

Fraud Awareness Short Presentation  

E-Print Network [OSTI]

Fraud Awareness Overview A Short Presentation From Your Internal Audit Department With assistance from the Office of the State Controller and the EAGLE Training Team #12;What is Fraud? #12;#12;What are some examples of fraud? #12;#12;Who commits fraud and why? #12;Management Manipulation

Howitt, Ivan

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


381

Ethics & Integrity Presented by  

E-Print Network [OSTI]

Ethics & Integrity Presented by Chris Loschiavo Assistant Dean and Director Student Conduct · Ethics Activity · Introduction to Ethics · Case Studies · Conclusions/ Questions #12;UF Student Code;Introduction to Ethics #12;Defining the Term "Ethics" · The term "ethics" comes from the Latin word "ethica

Roy, Subrata

382

Presented by Information Fusion  

E-Print Network [OSTI]

Presented by Information Fusion: Science and Engineering of Combining Information from Multiple's Office of Science #12;2 Managed by UT-Battelle for the U.S. Department of Energy Rao_InfoFusion_SC10 Information Fusion at ORNL � ORNL Instrumental in formulating and fostering this multi-disciplinary area

383

Architecture Overview Presented  

E-Print Network [OSTI]

Pentium Pro Architecture Overview Presented by David T.Wang #12; ``New'' To the 80x86 world and 1 MIS . PatchableMicrocode . fetches past unresolved branches based on prediction . large register past unresolved branches are also executed speculatively. #12; Retirement . uops recombined at ROB

Jacob, Bruce

384

An assessment of presentism  

E-Print Network [OSTI]

that no past or future things exist now. Socrates does not now exist, though he did in the past; my future daughter does not now exist, though she may in the future. Ontologically, the present is distinct, serving to demarcate all that currently has existence...

McDaniel, Brannon David

2004-09-30T23:59:59.000Z

385

Programme, Abstracts, Presentations & Proceedings  

E-Print Network [OSTI]

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

386

National Radio Astronomy Observatory Electronics Division Technical Note No. 219  

E-Print Network [OSTI]

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

Groppi, Christopher

387

1 Spectrum Sharing Games of Network Operators and Cognitive Radios  

E-Print Network [OSTI]

Contents 1 Spectrum Sharing Games of Network Operators and Cognitive Radios Mohammad Hossein advances in radio technology, the spectrum regulators have opened some parts of the available spectrum operators and cognitive radios. Because of the dynamic nature of spectrum sharing, it is difficult

Bencsáth, Boldizsár

388

THE COMPACT STEEP SPECTRUM AND GHZ PEAKED SPECTRUM RADIO SOURCES  

E-Print Network [OSTI]

THE COMPACT STEEP SPECTRUM AND GHZ PEAKED SPECTRUM RADIO SOURCES Christopher P. O'Dea Space@stsci.edu ABSTRACT I review the radio to X­ray properties of GHz Peaked Spectrum (GPS) and Compact Steep Spectrum The GHz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources make up significant fractions

389

Sequential Detection based Cooperative Spectrum Sensing Algorithms in Cognitive Radio  

E-Print Network [OSTI]

Sequential Detection based Cooperative Spectrum Sensing Algorithms in Cognitive Radio Arun considers the problem of Spectrum Sensing in Cognitive Radio Networks. For this we use a recently developed is not experienced by our algorithm. Keywords-Cognitive Radio, Cooperative Spectrum Sensing, Decentralized Sequential

Sharma, Vinod

390

Competitive Interference-aware Spectrum Access in Cognitive Radio Networks  

E-Print Network [OSTI]

Competitive Interference-aware Spectrum Access in Cognitive Radio Networks Jocelyne Elias, Fabio studies the spectrum access problem in cognitive radio networks from a game theoretical perspective. Finally, we provide numerical results of the proposed spectrum access game in several cognitive radio

Boyer, Edmond

391

High Throughput Spectrum-aware Routing for Cognitive Radio Networks  

E-Print Network [OSTI]

High Throughput Spectrum-aware Routing for Cognitive Radio Networks Ashwin Sampath, Lei Yang, Lili, wireless nodes equipped with cognitive radios [11] do not operate on statically as- signed spectrum who own the spectrum, e.g. analog TV broadcast stations. Such flexibility means cognitive radios can

Zhao, Ben Y.

392

Censored Truncated Sequential Spectrum Sensing for Cognitive Radio Networks  

E-Print Network [OSTI]

1 Censored Truncated Sequential Spectrum Sensing for Cognitive Radio Networks Sina Maleki Geert Leus Abstract Reliable spectrum sensing is a key functionality of a cognitive radio network. Cooperative spectrum sensing improves the detection reliability of a cognitive radio system but also increases

Leus, Geert

393

A Framework for Radio Frequency Spectrum Measurement and Analysis  

E-Print Network [OSTI]

A Framework for Radio Frequency Spectrum Measurement and Analysis V. Rory Petty ITTC-FY2008-TR allocation and the burgeoning problem of spectrum scarcity have prompted an examination of how the radio frequency spectrum is utilized. The radio frequency spectrum is an important national resource that impacts

Kansas, University of

394

Robust Performance of Spectrum Sensing in Cognitive Radio Networks  

E-Print Network [OSTI]

1 Robust Performance of Spectrum Sensing in Cognitive Radio Networks Shimin Gong, Ping Wang) in cognitive radio networks requires SUs to be spectrum aware and know which spectrum bands are occupied by PUs and reduces the system sensitivity on decision variables. Index Terms Cognitive radio network, spectrum

Huang, Jianwei

395

: Correlation-Based Cooperative Spectrum Sensing in Cognitive Radio Networks  

E-Print Network [OSTI]

(CORN)2 : Correlation-Based Cooperative Spectrum Sensing in Cognitive Radio Networks Dongyue Xue is referred to as cognitive radio networks (CRNs) [2]. Based on the ambient spectrum information, cognitive for cognitive radio networks to minimize energy consumption. A sensing quality metric is defined as a measure

Paris-Sud XI, Université de

396

Reputation Aware Collaborative Spectrum Sensing for Mobile Cognitive Radio Networks  

E-Print Network [OSTI]

Reputation Aware Collaborative Spectrum Sensing for Mobile Cognitive Radio Networks Abstract ­ The task of spectrum sensing for Dynamic Spectrum Access in Cognitive Radio Networks (CRNs) is very of Cognitive Radio (CR) operation is the opportunistic utilization of licensed spectrum bands by the Secondary

Zou, Cliff C.

397

Throughput Enhancing Cooperative Spectrum Sensing Strategies for Cognitive Radios  

E-Print Network [OSTI]

Throughput Enhancing Cooperative Spectrum Sensing Strategies for Cognitive Radios Kyounghwan Lee growth of wireless services continues to accelerate the exhaustion of usable radio spectrum. The radio channels licensed to the primary users. A main chal- lenge in this case is to design a spectrum sensing

Yener, Aylin

398

Cryptographic Link Signatures for Spectrum Usage Authentication in Cognitive Radio  

E-Print Network [OSTI]

Cryptographic Link Signatures for Spectrum Usage Authentication in Cognitive Radio Xi Tan, Kapil frequency spectrum was inefficiently utilized. To fully use these spectrums, cognitive radio networks have of cognitive radio is to enable the current fixed spectrum channels assigned by Federal Communica- tions

Du, Wenliang "Kevin"

399

Quickest Spectrum Detection Using Hidden Markov Model for Cognitive Radio  

E-Print Network [OSTI]

Quickest Spectrum Detection Using Hidden Markov Model for Cognitive Radio Zhe Chen, Zhen Hu, Robert and recognition under the umbrella of cognitive radio. In the procedure of spectrum recognition, a frequency) opened free white space spectrum on November 4, 2008 [1]. Cognitive radio has been put forward as a more

Qiu, Robert Caiming

400

Robust Distributed Spectrum Sensing in Cognitive Radio Networks  

E-Print Network [OSTI]

unlicensed radios to operate in licensed spectrum, provided no harmful interference is expe- riencedRobust Distributed Spectrum Sensing in Cognitive Radio Networks Ruiliang Chen, Jung-Min Park {rlchen, jungmin, kgbian}@vt.edu Abstract--Distributed spectrum sensing (DSS) enables a Cog- nitive Radio

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


401

SOME UNSOLVED CHALLENGES IN RADIO-FREQUENCY HEATING AND  

E-Print Network [OSTI]

SOME UNSOLVED CHALLENGES IN RADIO-FREQUENCY HEATING AND CURRENT DRIVE N. J. FISCH* Princeton Plasma in the electronic version. I. INTRODUCTION There are many methods by which radio-frequency (rf) waves drive, 2013 doi:10.13182/FST13-682 Several unsolved challenges in radio-frequency heating and current drive

402

Rotating-radio-frequency ion traps T. Hasegawa*  

E-Print Network [OSTI]

rf ion trap, the rotating-radio-frequency rotating-rf trap, in which the motion of a charged particleRotating-radio-frequency ion traps T. Hasegawa* Department of Physics, Keio University, Kanagawa and Technology, Boulder, Colorado 80305, USA Received 9 July 2005; published 20 October 2005 We discuss a radio-frequency

403

GROUND-BASED AND SPACE-BASED RADIO OBSERVATIONS OF  

E-Print Network [OSTI]

discharge/flash consists of many consecutive strokes) [e.g. Gibbard et al., 1997] LightningGROUND-BASED AND SPACE-BASED RADIO OBSERVATIONS OF PLANETARY LIGHTNING P. Zarka1 , W. Farrell2 , G; Lightning's radio signature Space-based radio observations of planetary lightning Lightning

Demoulin, Pascal

404

Data Analysis in the Radio Astr 257: Modern Astronomical Techniques  

E-Print Network [OSTI]

Data Analysis in the Radio Emma Storm Astr 257: Modern Astronomical Techniques May 28th, 2013 Storm (Astr257) Radio Data Analysis 05/28/13 1 / 36 #12;Radio Data Analysis interferometers measure antenna to raw, uncalibrated data need to manually calibrate image processing depends on science goals Storm

California at Santa Cruz, University of

405

Energy Efficient Transmissions in MIMO Cognitive Radio Networks  

E-Print Network [OSTI]

Energy Efficient Transmissions in MIMO Cognitive Radio Networks Liqun Fu The Institute of Network@ie.cuhk.edu.hk Abstract--In this paper, we consider energy efficient transmis- sions for MIMO cognitive radio networks on the traffic load of the secondary system. Index Terms--Cognitive radio networks, MIMO, Energy- efficiency. I

Huang, Jianwei

406

Photonic Radio-Frequency Phase Detector based on Radio-Frequency to Intermediate-Frequency Phase Mapping  

Science Journals Connector (OSTI)

A photonic radio-frequency phase detector based on radio-frequency (RF) to intermediate-frequency mapping is demonstrated, and the theoretical principle of the design is explained.

Sun, Dongning; Dong, Yi; Wang, Siwei; Xia, Zongyang; Xie, Weilin; Shi, Hongxiao; Yi, Lilin; Hu, Weisheng

407

Multi-radio medium access control protocol for wireless sensor networks  

Science Journals Connector (OSTI)

This paper describes a dual-radio based medium access control protocol for wireless sensor networks. Our protocol combines the advantages of the two radios operating in different frequency bands to result in highly energy-efficient operation. The design effectively addresses the two dominant sources of energy consumption in sensor network communication, namely the idle listening and the ephemeral burst data traffic. This paper presents the design rationale and extensive empirical performance evaluation of the protocol in terms of power consumption and latency under various traffic loads and duty cycles. Experimental performance comparison with B-MAC show high gains of our approach. We derive analytical expression for the optimum transmit power level ratio of the two radios giving minimum energy consumption. We also model the mathematical relationship for the optimal duty cycle of the nodes to a given network traffic load and validate it through the prototype implementation on commercially available sensor nodes.

Junaid Ansari; Xi Zhang; Petri Mahonen

2010-01-01T23:59:59.000Z

408

Optical Synchrotron Precursors of Radio Hypernovae  

E-Print Network [OSTI]

Some hypernova (HN) explosions accompany much brighter radio afterglows than those of ordinary core-collapse supernovae (SNe), which we here term radio HNe. Due to their association with low-luminosity gamma-ray bursts (llGRBs), and with implied relativistic ejecta velocities, previous studies suggested that the enhanced radio emissions are essentially energized by relativistic jets. By re-examining some observed radio HNe based on the refreshed shock model, we find, however, that they can be consistently explained by afterglow emissions from spherical HN explosions without jet component. In this model, a sequence of shock breakout shells interacts with the circumstellar wind medium and induces multi-band synchrotron emission. Our model can be confirmed by optical synchrotron precursors from ~ 1000 s to 1 day after shock breakouts, which are detectable by current and future high-cadence wide-field surveys. They can be also associated with ordinary HNe with an event rate of ~ 0.32/yr from <~ 40 Mpc. Most of...

Nakauchi, Daisuke; Nagakura, Hiroki; Suwa, Yudai; Nakamura, Takashi

2014-01-01T23:59:59.000Z

409

Radio Astronomy with Very Large Arrray  

Science Journals Connector (OSTI)

...construction of the Very Large Array of radio telk...role of the Very Large Array in c research...control building. atmosphere is transpi mainly...their wave-00. Large optical V,Iu...radia-tion to the area ofthe sky covered...Neutral H: 1420.4 MHz H, He, and so on...

R. M. Hjellming; R. C. Bignell

1982-06-18T23:59:59.000Z

410

Buoyant radio plasma in clusters of galaxies  

Science Journals Connector (OSTI)

......calculated maps of the radio surface brightness resulting from synchroton radiation. These maps were compiled for two different assumptions...find that some of these processes may prolong the phase of synchroton emission but if so, the bubbles will be exceedingly faint......

M. Brggen; C.R. Kaiser

2001-08-01T23:59:59.000Z

411

Reliable Link Maintenance in Cognitive Radio Systems  

E-Print Network [OSTI]

resources and overcome the under-utilization of licensed spectrum. Since the licensed user still keeps) have to vacate the spectrum in case the licensed user claims it. In order to maintain the qualityReliable Link Maintenance in Cognitive Radio Systems Daniel Willkomm, James Gross and Adam Wolisz

Gross, James

412

The Rapidly Pulsating Radio Source in Vulpecula  

Science Journals Connector (OSTI)

...ob-served frequencies (Table 1...the pulse radio frequency as a function...is the % plasma frequency...near 100 Mhz are given...fre-quency (RF) as a function of frequency. The straight...those at 430 Mhz by 0.279...than the plasma and cyclotron...arrival time at high frequency. High Low...

F. D. Drake; E. J. Gundermann; D. L. Jauncey; J. M. Comella; G. A. Zeissig; H. D. Craft Jr.

1968-05-03T23:59:59.000Z

413

Buoyant radio plasma in clusters of galaxies  

Science Journals Connector (OSTI)

......observing frequency of 330 MHz. In these maps the major...observing frequency is 330 MHz and for the redshift...volume-filling factor of the radio plasma is unity. The units...to note that the hot plasma remains confined within...explosions in the Earth's atmosphere. In their wake the bubbles......

M. Brggen; C.R. Kaiser

2001-08-01T23:59:59.000Z

414

Chameleonic Radio Technical Memo No. 11  

E-Print Network [OSTI]

Chameleonic Radio Technical Memo No. 11 An Audio System for the Blackfin S.M. Shajedul Hasan and S Institute & State University Blacksburg, VA 24061 #12;An Audio System for the Blackfin S.M. Shajedul Hasan Institute & State University, Blacksburg VA 24061 USA. E-mail: hasan@vt.edu 1 #12;1 Introduction

Ellingson, Steven W.

415

Chameleonic Radio Technical Memo No. 15  

E-Print Network [OSTI]

Receiver based on USRP and OSSIE," S.M. Shajedul Hasan and P. Balister, December 14, 2005. [3] 2. "An Hasan and S.W. Ellingson, January 24, 2006. [4] 3. "Implementation Status of the SCA-Based FM Radio," P Interface," S.M. Shajedul Hasan and Kyehun Lee, July 23, 2006

Ellingson, Steven W.

416

Chameleonic Radio Technical Memo No. 23  

E-Print Network [OSTI]

Hasan, M. Harun, and C.R. Anderson October 5, 2007 Bradley Dept. of Electrical & Computer Engineering S.W. Ellingson , S.M. Shajedul Hasan, M. Harun, and C.R. Anderson October 7, 2007 Contents 1 Wideband RF Downconverter for the NIJ Public Safety Radio," S.M. Shajedul Hasan and S.W. Ellingson

Ellingson, Steven W.

417

Determination, Control & Improvement of an SKA Radio  

E-Print Network [OSTI]

SKA core sites were chosen in a sparsely populated part of South Africa, in the Northern Cape ProvinceDetermination, Control & Improvement of an SKA Radio Environment in South Africa Three potential -200 -150 -100 -50 0 Frequency spectrum 150 to 174 MHz Spectralpowerflux-density Agg Signal Kalahari

Ellingson, Steven W.

418

A current circuit model of pulsar radio emission  

E-Print Network [OSTI]

We present the outline of a new model for the coherent radio emission of pulsars that succeeds in reproducing the energetics and brightness temperatures of the observed radio emission from the observationally deduced distances of 50-100 pulsar radii above the neutron star in a narrow region. The restrictions imposed by energy conservation, plasma dynamics of the coherent radiation process and propagation effects are used to apply the action of a plasma process like coherent inverse Compton scattering (CICS) (see Benford, 1992). In accordance with our findings (Kunzl et al. 1998a) this process requires Lorentz factors of about 10 which are lower than in most other radio emission models. This implies that no significant pair production can take place near the surface and we expect charge densities close to the Goldreich-Julian value (Goldreich & Julian (1969)). To fulfill the energetic and electrodynamic constraints the model requires constant re-acceleration in dissipation regions which can be interpreted as a voltage drop similar to that in a resistive current circuit built of a battery, connecting copper wires and a resistive load. Using the emission heights for PSR 0329+54 published by Mitra and Rankin (2002) and the spectral data from Malofeev et al. (1994) we find that a constant depth of the dissipation region of about 2 r_NS can account for the observed luminosities and spectral behavior. The extremely high peak fluxes in the substructures of single pulses can be explained by beaming effects as discussed in Kunzl et al. (1998b).

Th. Kunzl; H. Lesch; A. Jessner

2002-08-30T23:59:59.000Z

419

2010 Raj JainCSE574sWashington University in St. Louis Radio FrequencyRadio Frequency  

E-Print Network [OSTI]

. Louis RFID ReadersRFID Readers Sends a pulse of radio energy and listens for tags response Readers may24-1 ©2010 Raj JainCSE574sWashington University in St. Louis Radio FrequencyRadio Frequency;24-3 ©2010 Raj JainCSE574sWashington University in St. Louis What is RFID?What is RFID? Radio Frequency

Jain, Raj

420

PowerPoint Presentation  

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

National Laboratory Mentor-Protégé Program Business Success Stories Presented by Cassandra McGee Stuart ORNL Small Business Programs Office May 23, 2013 2 Presentation name Today, ORNL is DOE's largest science and energy laboratory 2 Managed by UT-Battelle for the U.S. Department of Energy $1.65B budget World's most intense neutron source 4,400 employees World-class research reactor 3,000 research guests annually $500M modernization investment Nation's largest materials research portfolio Most powerful open scientific computing facility Nation's most diverse energy portfolio Managing billion-dollar U.S. ITER project 3 Managed by UT-Battelle for the U.S. Department of Energy ORNL is managed by UT-Battelle, LLC * A 65-year relationship with DOE

Note: This page contains sample records for the topic "testimony presentations radio" 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

PowerPoint Presentation  

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

Greenhouse Gas Reporting Program: Greenhouse Gas Reporting Program: Geologic Sequestration and Injection of Carbon Dioxide Mark de Figueiredo Climate Change Division U.S. Environmental Protection Agency Presentation for: DOE/NETL Carbon Storage Program Infrastructure Annual Review Meeting November 15, 2011 Outline * Background of Greenhouse Gas Reporting Program * Summary of Subpart UU (Injection of CO 2 ) * Summary of Subpart RR (Geologic Sequestration of CO 2 ) 2 This presentation is provided solely for informational purposes. It does not provide legal advice, have legally binding effect, or expressly or implicitly create, expand, or limit any legal rights, obligations, responsibilities, expectations, or benefits in regard to any person. Background of GHG Reporting Program * In response to the FY2008 Consolidated Appropriations Act, EPA

422

PowerPoint Presentation  

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

Presentation Presentation * CAES Aquifer Technology * Geological Framework of Iowa * Dallas Center Structure * Results of CAES Feasibility Simulation * ISEP CAES Development Plan How Does CAES Work? CAES Turbo-Machinery Operating Requirements Equipment Manufacturer Plant Size (MW) Min. Inlet Pressure (psi) Min. Flow Rate (lbs/MW/hr) Total Min. Flow Rate (lb/hr) Allison 15 200 9500 142,500 MAN Turbo 50 50 9500 475,000 Dresser Rand 134 830 9500 1,273,000 Alston 300 900 9500 2,850,000 Westinghouse (501D5) 350 750 9500 3,325,000 Westinghouse (501F) 450 750 9500 3,275,000 Earth Storage System Designs All based on the concept of multiple geologic and hydrologic barriers. DESIGN CRITERIA * Capacity: 5 to 10 BCF Total Vessel Volume * Integrity of Vessel: <4% of Volume over a year * Fluid Deliverability - 400#/sec = 464 MMscfd

423

PowerPoint Presentation  

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

Projects Projects Characterization of Most Promising Carbon Capture and Sequestration Formations in the Central Rocky Mountain Region (RMCCS) RCSP Annual Review Meeting October 5-7, 2010 Pittsburgh, PA Acknowledgements I * Many thanks to the U.S. Department of Energy and NETL for supporting this project * We express our gratitude also to our many industry partners, who have committed a great deal of time, funding and other general support for this project * The work presented today is co-authored by many partners in the RMCCS project * Project Team (Who) * Major Goals (Why) * Work Plan (How) * Progress to Date (What) Presentation Outline Partners The project team consists of the geological surveys in each state of the region, some invaluable industry partners, and of course NETL.

424

PowerPoint Presentation  

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

This presentation was given for the This presentation was given for the Navigant Research Webinar on Fast DC Charging for Electric Vehicles * http://www.navigantresearch.com/webinar/fast-dc-charging-for-electric-vehicles * April 9, 2013 1 Lessons Learned on the EV Project and DC Fast Charging Garrett Beauregard Executive Vice President and General Manager, eTec Labs April 9, 2013 ECOtality Company Overview Leading Hardware, Software and R&D for electric transportation Diversified revenue base of 3 complementary business segments Blink * Residential, public & commercial EV charging solutions * Contracted by U.S. Dept. of Energy for The EV Project (~$115M) * Over 11,000 chargers installed as of April 2013 Minit-Charger * Fast charging electric material handling and ground support equipment

425

PowerPoint Presentation  

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

FWP-FEW0174 - Task 5 Presenter: Megan Smith PI: Susan Carroll Yue Hao U.S. Department of Energy National Energy Technology Laboratory Carbon Storage R&D Project Review Meeting Developing the Technologies and Building the Infrastructure for CO 2 Storage August 20-22, 2013 This work performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344 Lawrence Livermore National Laboratory 2 Presentation Outline  Benefit to Program  Project Overview  Technical Status  Accomplishments  Summary  Appendix Lawrence Livermore National Laboratory 3 Benefit to the Program  This research project quantifies relationships between fluid flow, heterogeneity, and reaction rates specific to

426

PowerPoint Presentation  

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

in Western Utility Energy Efficiency in Western Utility in Western Utility Energy Efficiency in Western Utility Resource Plans Resource Plans Implications for Regional Assessments and Implications for Regional Assessments and Initiatives Initiatives Charles Goldman Nicole Hopper Lawrence Berkeley National Laboratory CREPC Meeting San Diego, CA September 28, 2006 Overview of Presentation Overview of Presentation * LBNL/CREPC Resource Assessment Project - Overview - Data Sources * Treatment of Energy Efficiency (EE) in Resource Plans - Why does it matter? * Energy Efficiency in Recent Resource Plans: - Common Inconsistencies and Data Problems - Levels of EE Proposed in Recent Utility Resource Plans * Recommendations and tools for tracking and reporting EE in future resource plans to support West-wide goals and analysis LBNL/CREPC Resource Assessment Project LBNL/CREPC Resource Assessment Project

427

MDM Tech Day Presentation  

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

Mega Project Mega Project Risk Analysis Model Oak Ridge Tennessee November 5, 2009 2 Content - Objectives - Risk Assessment Approach - Nuclear Risk Assessment Model Overview - Lessons Learned 3 Objectives ■ Present a new approach to analyzing risks of large and complex projects that may be directly applied to DOE ■ Discuss an example of how this methodology was recently used in a nuclear project, and how this can fit DOE's unique challenges ■ Present the benefits of using a risk assessment for protecting the government's interests and reduce risk exposure 4 Content - Objectives - Risk Assessment Approach - Nuclear Risk Assessment Model Overview - Lessons Learned 5 Approach to risk assessment follows a logical progression of risk identification, impact, and mitigation analysis Risk

428

PowerPoint Presentation  

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

Administration FAA Air Traffic Organization Presented to: Department of Energy Presented by: Mark DeNicuolo, Manager, Performance & Analyses, FAA ATO Safety and Technical Training Date: September 20, 2012 Safety Management 2 * Approximately 50,000 flights per day * En Route centers handle 40.5 million aircraft per year * FAA/contract towers handle: - 51.2 million airport operations - 39 million instrument operations * 732 million passenger enplanements * Over 5,000 civil, public-use airports * Approximately 33,300 ATO employees - More than 15,000 air traffic controllers - More than 7,000 technicians and engineers * 21 ARTCCs, 513 ATCTs, 17 FSSs, 3 AFSSs National Airspace System (NAS) 3 Discipline Domains En Route Terminal FSS Support NDP Totals

429

PowerPoint Presentation  

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

Evolution of Risk Management at NASA in Evolution of Risk Management at NASA in the Context of Achieving Adequate Safety Presented at the DOE 2012 Nuclear Safety Workshop Bethesda, Maryland September 20, 2012 Homayoon Dezfuli, Ph.D. NASA Technical Fellow for System Safety Office of Safety and Mission Assurance NASA Headquarters Outline * Historical Perspective on NASA Risk Management (RM) * RM Approach After 2008 * Future Direction of RM at NASA - The Concept of "Adequate Safety" - The Issue of Risk Analysis Completeness (Rationale for Future Trends in RM) * Summary 2 Acknowledgments This presentation is partly derived from the following sources: 3 NASA NPR 8000.4A NASA/SP-2010-576 NASA/SP-2011-3422 NASA/SP-2010-580 Historical Perspective on NASA Risk

430

PowerPoint Presentation  

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

Lawrence Livermore National Laboratory Lawrence Livermore National Laboratory LL-WCI-U-2011-522763 Monthly Performance Review Director's Office March 21, 2008 Monthly Performance Weapons and Complex Integration (WCI) High Energy Density Experiments on NIF in FY2011 (A Joint WCI-NIF Success) Presented to SEAB Oct. 12, 2011 Lawrence Livermore National Laboratory This work performed under the auspices of the U.S. Department of Energy by

431

FLARE-ASSOCIATED TYPE III RADIO BURSTS AND DYNAMICS OF THE EUV JET FROM SDO/AIA AND RHESSI OBSERVATIONS  

SciTech Connect (OSTI)

We present a detailed description of the interrelation between the Type III radio bursts and energetic phenomena associated with the flare activities in active region AR11158 at 07:58 UT on 2011 February 15. The timing of the Type III radio burst measured by the radio wave experiment on Wind/WAVE and an array of ground-based radio telescopes coincided with an extreme-ultraviolet (EUV) jet and hard X-ray (HXR) emission observed by SDO/AIA and RHESSI, respectively. There is clear evidence that the EUV jet shares the same source region as the HXR emission. The temperature of the jet, as determined by multiwavelength measurements by Atmospheric Imaging Assembly, suggests that Type III emission is associated with hot, 7 MK, plasma at the jet's footpoint.

Chen Naihwa; Ip, Wing-Huen [Graduate Institute of Astronomy, National Central University, Jhongli 32001, Taiwan (China); Innes, Davina, E-mail: d949001@astro.ncu.edu.tw, E-mail: wingip@astro.ncu.edu.tw, E-mail: innes@mps.mpg.de [Max-Planck-Institut fuer Sonnensystemforschung, D-37191 Katlenburg-Lindau (Germany)

2013-06-01T23:59:59.000Z

432

Abstract--Reconfigurable Radio Systems (RRS), based on Software Defined Radio (SDR) and Mobile Ad-hoc Network  

E-Print Network [OSTI]

Abstract--Reconfigurable Radio Systems (RRS), based on Software Defined Radio (SDR) and Mobile Ad-hoc by the proposed scheme, while keeping the important false positive rate at a very low level. Keywords--Mobile ad-hoc (SDR), Mobile Ad-hoc Networks (MANETs) and Cognitive Radio (CR). Research on these technologies has

433

PowerPoint Presentation  

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

Budget and TYCP Process Budget and TYCP Process Discussion Bob Harris UGP Regional Manager and PM 1 Preliminary 10-Year Capital Budget/Funding Establish Programmatic Asset Management/Capital Funding Process Asset Management Customer Networking Sustainable Funding Discussion Utilize Programmatic Asset Management/Capital Funding AMPIP WESTERN'S ROADMAP ROBUST ASSET MANAGEMENT PROGRAM/WESTERN-WIDE CAPITAL BUDGET 2013 2014 NOV MAY ... ... ... 2 Rates Presentation Jack Murray DSW Rates Manager 3 P-DP Rate Discussion * Transmission rates experiencing long-term upward pressure. * Cost of rebuilding aging infrastructure a key component responsible for potential rate increases. * As additional plant completed and placed in service, annual costs to service debt increase,

434

P9 Summary Presentation  

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

Learned Learned WTP Prototypic Mixing and Sampling System Vijay Jain Manager, Research & Technology (Vitrification) May 18-21, 2009 Waste Treatment & Immobilization Plant Project Presented at EM-21 Technical Exchange Denver, CO Jain 04102009 2 Outline Background Test requirements and system design Test status Technical issues during testing Test results Summary Jain 04102009 3 Highlights Testing system is prototypic Major technical and design issues resolved LAW report (3 simulants) - issued HLW & LAW tests - complete Data analyses - 08/09 Reports - 12/09 Jain 04102009 4 Background Compliance to waste specifications is critical to the success of WTP vitrification operations: - Mixing and sampling of waste and melter feed is an integral part

435

Meeting and Presentation Materials  

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

1) Agenda 2) Presentations: a. Welcome, Agenda and any High Priority Issues b. Issuance of DOE O 414.1D - How it Affects EM Sites c. EM Commercial Grade Dedication Guide d. Integration of QA in Design Guidance Document e. Draft Revision to the Standard QA Contract Language f. Operational Awareness - Basic QA Profile Associated with EM Hazard Category 2 and 3 Nuclear Operations g. EFCOG Current Efforts & Relationship to the EM QA Corporate Board Priorities & Focus Areas 3) Commercial Grade Dedication Guidance Document 4) Integration of QA in Design Guidance Document 5) Draft Revision to Standard QA Contract Language 6) Status of Actions from the February 2011 Board Meeting

436

PowerPoint Presentation  

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

Fleet Card Program Review Fleet Card Program Review Presented to: U.S. Department of Energy Wright Express Corporation June 25, 2012 2012 Wright Express Corporation. Confidential & Proprietary. 1 2012 Wright Express Corporation. Confidential & Proprietary. 2 Table of Contents I. Wright Express Fleet Card I. Program Statistics II. What's New II. Questions? 2012 Wright Express Corporation. Confidential & Proprietary. 3 Program Statistics 2012 Wright Express Corporation. Confidential & Proprietary. 4 Portfolio Snapshot * 13 Month Overview Month Total Gross Dollars Total Transactions Total Unleaded Gallons Total Unleaded Dollars Total Diesel Gallons Total Diesel Dollars Total Gallons (all Fuel) Total Non-Fuel Transactions Total Non-Fuel Dollars Total Cards

437

PowerPoint Presentation  

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

IOGCC/SSEB PTTF REPORT IOGCC/SSEB PTTF REPORT THE PIPELINE PROJECT: Analysis of potential pipeline infrastructure, transportation & storage of CO 2 Presented at DOE's Carbon Storage Program Infrastructure Annual Review Meeting Nov. 15, 2011 Acknowledgement * This material is based upon work supported by the U.S. Department of Energy's National Energy Technology Laboratory. The Report Four sections: 1. Overview 2. Background 3. Analysis 4. Recommendations PART 1: OVERVIEW * Pipeline Transportation Task Force * Collaborative Work Group Model * Task Force Objectives IOGCC-SSEB CO 2 Pipeline Transportation Task Force (PTTF) * Offshoot of IOGCC's Carbon Capture and Geologic Storage Task Force * Southeast Regional Carbon Sequestration Partnership Focus Area * Collaboration: Task Force Composition

438

PowerPoint Presentation  

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

INDUSTRY DAY INDUSTRY DAY Emergency Operations Training Academy Support Services James (Jim) Cochran Headquarters Support Section Headquarters Acquisition Branch Business Services Division January 6, 2012 2 Agenda * 0900 - Arrival/Registration * 0915 - Opening Remarks - Jim Cochran, Contracting Officer * 0925 - Emergency Operations Training Academy's (EOTA) Overview - Paul Jenkins, Director, EOTA * 0950 - Review of EOTA Request for Proposals * 1030 -EOTA Server Facility * 1100 - Questions * 1130 - Closing Comments 3 Notice * Presentation is based upon current information and plan of action * Input may be considered * Request for Proposal is the only document that is to be relied upon in determining the Government's needs 4 Overview * Purpose of Industry Day

439

PowerPoint Presentation  

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

and Validating Ternary Pd Alloys and Validating Ternary Pd Alloys Designing and Validating Ternary Pd Alloys for Optimum Sulfur/Carbon Resistance for Optimum Sulfur/Carbon Resistance in Hydrogen Separation in Hydrogen Separation and Carbon Capture Membrane Systems and Carbon Capture Membrane Systems Using High Using High - - Throughput Combinatorial Methods Throughput Combinatorial Methods Dan Henkel Rick kleiner November 12, 2009 This presentation does not contain any proprietary or confidential information 2 Participating Organizations Pall Corporation Pall Cortland Research and Development (PRDC) Cornell University Cornell Center for Materials Research (CCMR) Georgia Institute of Technology Dept. of Materials Science and Engineering Oak Ridge National Laboratory High Temperature Materials Lab (HTML)

440

TITLE OF PRESENTATION HERE  

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

Claiming Savings from Claiming Savings from Building Codes Activities Presented by Carolyn Sarno April 4, 2012 DOE Code Compliance Meeting FOR TODAY'S DISCUSSION * Background * Claimed Savings Report * Best Practice - Rhode Island 1 RECENT TRENDS 2 Aggressive new goals directing capture of all cost- effective efficiency * CT, MA, NY, RI VT * $2.5 billion committed to efficiency programs in New England, New York and Mid-Atlantic in 2012 * Multiple funding sources: SBC, RGGI, FCM, rate factors * Next generation of efficiency plans going broader & deeper ATTRIBUTING ENERGY CODE SAVINGS ENERGY EFFICIENCY PROGRAMS * Convene stakeholder advisory group * Identify issues related to PA support for codes (and standards) * Provide procedural guidance for

Note: This page contains sample records for the topic "testimony presentations radio" 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

Presentation title goes here  

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

Future of DR Future of DR March 3, 2011 Sila Kiliccote, Mary Ann Piette, Dave Watson, Rish Ghatikar Deputy, DRRC Program Manager, LBNL SKiliccote@lbl.gov 2 Presentation Overview * Trends * Policy * Technology * Implementations * Load As Resource in Ancillary Services Markets * Future directions towards responsive buildings 3 Trends Policy Dynamic Rates - Large C&I, residential, small commercial Codes and Standards -Title 24, US Green Building Council's LEED Credits Smart Grid Standards effort Ancillary Services Technology Integration of Renewables Energy Storage Technologies - Can DR replace storage? PHEVs and EVs Implementation Linking Energy Efficiency and DR Utility Implementations Smart Grid Investment and Demonstration Grants 4 Demand Side Management and Automated DR Future

442

PowerPoint Presentation  

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

China China Energy Statistics 2012 Lawrence Berkeley National Laboratory The LBNL China Energy Group The China Energy Group at Lawrence Berkeley National Laboratory (LBNL) was established in 1988. Over the years the Group has gained recognition as an authoritative source of China energy statistics through the publication of its China Energy Databook (CED). The Group has published seven editions to date of the CED (http://china.lbl.gov/research/china- energy-databook). This handbook summarizes key statistics from the CED and is expressly modeled on the International Energy Agency's "Key World Energy Statistics" series of publications. The handbook contains timely, clearly-presented

443

Norms of Presentational Force  

E-Print Network [OSTI]

://www.americanforensics.org/uploaded-files/tc_41_3_w05.pdf. Open Access version: http://kuscholarworks.ku.edu/dspace/. 15 hope to illustrate the close connection between emotional appeal and premise adequacy. After arguing that the Declaration of Independence and Constitution secure...Innocenti Manolescu, Beth. "Norms of Presentational Force." Argumentation and Advocacy 41 (2005): 139-51. Official publishers version: http://www.americanforensics.org/uploaded-files/tc_41_3_w05.pdf. 1 Citation: Innocenti Manolescu, Beth...

Innocenti, Beth

2005-01-01T23:59:59.000Z

444

FCC Lab Presentation  

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

Introduction to Introduction to Spectrum Engineering Julius Knapp, Chief Office of Engineering and Technology U.S. Federal Communications Commission Department of Energy Seminar on Spectrum Policy for the Utility Sector December 8, 2010 Note: The views expressed in this presentation are those of the author and may not necessarily represent the views of the Federal Communications Commission Why We Are Here: Utility Wireless Applications Use Spectrum Voice Dispatcher to Crews Crew to Crew Emergency Call "Talk Around" Interconnect Trunked Operation Mutual Aid/Interoperability Data: System Monitoring and Control, Reports and Status Messaging Telemetry, Protective Relaying SCADA (Supervisory Control and Data Acquisition) Automated Meter Reading Home Automation

445

PowerPoint Presentation  

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

Market Monitoring Market Monitoring Tools Bernie Lesieutre - LBNL Bob Thomas - Cornell October 18, 2006 Washington, D.C. OE Visualization and Controls Peer Review Market Monitoring Tools: Overview Approach: Use dispatch, profit, revenue/offer price, withholding sensitivities to identify opportunities for local advantage that give some participants market power potential. 2006 Technical Work: Extend prior results to large, RTO-scale systems. Initiate large-scale analysis with RTO (PJM). Evaluate reactive power effects on energy markets. Publication and presentation of results. Market Power: Substitutability Market power boils down to the issue of substitutability Locational Advantage: "Load Pockets" Physical network constraints limit supply to certain loads, so that the incremental demand

446

ILLUMINATING THE DARKEST GAMMA-RAY BURSTS WITH RADIO OBSERVATIONS  

SciTech Connect (OSTI)

We present X-ray, optical, near-infrared (IR), and radio observations of gamma-ray bursts (GRBs) 110709B and 111215A, as well as optical and near-IR observations of their host galaxies. The combination of X-ray detections and deep optical/near-IR limits establish both bursts as ''dark''. Sub-arcsecond positions enabled by radio detections lead to robust host galaxy associations, with optical detections that indicate z {approx}< 4 (110709B) and z Almost-Equal-To 1.8-2.9 (111215A). We therefore conclude that both bursts are dark due to substantial rest-frame extinction. Using the radio and X-ray data for each burst we find that GRB 110709B requires A{sub V}{sup host}{approx}>5.3 mag and GRB 111215A requires A{sub V}{sup host}{approx}>8.5 mag (assuming z = 2). These are among the largest extinction values inferred for dark bursts to date. The two bursts also exhibit large neutral hydrogen column densities of N{sub H,{sub int}} {approx}> 10{sup 22} cm{sup -2} (z = 2) as inferred from their X-ray spectra, in agreement with the trend for dark GRBs. Moreover, the inferred values are in agreement with the Galactic A{sub V} -N{sub H} relation, unlike the bulk of the GRB population. Finally, we find that for both bursts the afterglow emission is best explained by a collimated outflow with a total beaming-corrected energy of E{sub {gamma}} + E{sub K} Almost-Equal-To (7-9) Multiplication-Sign 10{sup 51} erg (z = 2) expanding into a wind medium with a high density, M Almost-Equal-To (6-20) Multiplication-Sign 10{sup -5} M{sub Sun} yr{sup -1} (n Almost-Equal-To 100-350 cm{sup -3} at Almost-Equal-To 10{sup 17} cm). While the energy release is typical of long GRBs, the inferred density may be indicative of larger mass-loss rates for GRB progenitors in dusty (and hence metal rich) environments. This study establishes the critical role of radio observations in demonstrating the origin and properties of dark GRBs. Observations with the JVLA and ALMA will provide a sample with sub-arcsecond positions and robust host associations that will help to shed light on obscured star formation and the role of metallicity in GRB progenitors.

Zauderer, B. A.; Berger, E.; Margutti, R.; Fong, W.; Laskar, T.; Chornock, R.; Soderberg, A. M. [Department of Astronomy, Harvard University, Cambridge, MA 02138 (United States); Levan, A. J. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Olivares E, F.; Greiner, J. [Max-Planck-Institut fuer extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching (Germany); Perley, D. A.; Horesh, A.; Carpenter, J. [Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA 91225 (United States); Updike, A. C. [Department of Chemistry and Physics, Roger Williams University, Bristol, RI 02809 (United States); Tanvir, N. R. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Menten, K. M. [Max-Planck-Institut fuer Radioastronomie, D-53121 Bonn (Germany); Nakar, E. [Department of Astrophysics, Sackler School of Physics and Astronomy, Tel Aviv University, 69978 Tel Aviv (Israel); Chandra, P. [National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune University Campus, Ganeshkhind, Pune 411007 (India); Castro-Tirado, A. J. [Instituto de Astrofisica de Andalucia (IAA-CSIC), P.O. Box 03004, E-18080 Granada (Spain); Bremer, M. [Institut de Radioastronomie Millimetrique, 300 rue de la Piscine, F-38406 Saint Martin d'Heres (France); and others

2013-04-20T23:59:59.000Z

447

PowerPoint Presentation  

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

Tolerance and Mechanical Properties of Tolerance and Mechanical Properties of Nanostructured Ceramic/Metal Composites Michael Nastasi Nebraska Center for Energy Sciences Research and Mechanical and Materials Engineering University of Nebraska-Lincoln Collaborators : UNL: Juan Colon Santana MIT: Mike Demkowicz , R. E. Baumer, Kan-Ju Lin TAMU: Lin Shao, Lloyd Price Work supported by DOE, NE, Nuclear Energy Enabling Technologies Presented at: Materials-Cross-Cut NEET Webinar August 20 th , 2013 Vacancies Interstitials Atomic defects produced by irradiation Embrittlement Defects that do NOT recombine aggregate into vacancy or interstitial clusters D.L. Porter and F. A. Garner, J. Nuclear Materials, 159, p. 114 (1988) D.J. Bacon and Y.N. Osetsky, Int. Mater. Rev., 47, p. 233 (2002).

448

PowerPoint Presentation  

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

Cleanup Project _____________________ September 21, 2005 FRR Rail Shipment to Idaho Presentation to the DOE Transportation External coordination Working Group (TEC) Mark R. Arenaz DOE-ID Idaho Cleanup Project U.S. Department of Energy Idaho Operations Office 2 DOE - Idaho Operations Office FRR Rail Shipment * Overview of Shipment * Operational Aspects * Emergency Response Preparation * Institutional Program * Route Determination * Lessons Learned * Pictures Idaho Cleanup Project U.S. Department of Energy Idaho Operations Office 3 Overview of Shipment * First shipment of Foreign Research Reactor (FRR) Spent Nuclear Fuel (SNF) * Spent Fuel originated in So. Korea * Transport by dedicated ship to Naval Weapons Station - Concord (NWSCo) * Transport by dedicated rail from NWSCo to Idaho National Laboratory Site

449

PowerPoint Presentation  

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

Stirling A. Colgate has been a staff physicist at Lawrence Livermore National Lab. (1952-1965) Stirling A. Colgate has been a staff physicist at Lawrence Livermore National Lab. (1952-1965) and was a staff member at Los Alamos National Laboratory, [LANL] from 1976 to 1991 and from then to present has been an adjunct physicist at LANL. From 1965 through 1974 he was president of New Mexico Institute of Mining and Technology. He was elected to the National Academy of Science in 1985. In 1990 he received the Rossi prize for work in astrophysics; having predicted in 1963 the emission of neutrinos from supernovae, recently observed from the nearby Supernovae 1987A. He is a Senior fellow at LANL, a Fellow of the American Physical Society, and co-shared the Los Alamos Medal. More important for this proposal is his experience in nuclear weapons, both design and

450

Title of Presentation  

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

A Process Approach to Management of Operational Cyber Security Risks Antione Manson, DHS Jim Cebula, CERT DOE Cyber Security Conference Atlanta - May 2010 2 NO WARRANTY THIS MATERIAL OF CARNEGIE MELLON UNIVERSITY AND ITS SOFTWARE ENGINEERING INSTITUTE IS FURNISHED ON AN -AS-IS" BASIS. CARNEGIE MELLON UNIVERSITY MAKES NO WARRANTIES OF ANY KIND, EITHER EXPRESSED OR IMPLIED, AS TO ANY MATTER INCLUDING, BUT NOT LIMITED TO, WARRANTY OF FITNESS FOR PURPOSE OR MERCHANTABILITY, EXCLUSIVITY, OR RESULTS OBTAINED FROM USE OF THE MATERIAL. CARNEGIE MELLON UNIVERSITY DOES NOT MAKE ANY WARRANTY OF ANY KIND WITH RESPECT TO FREEDOM FROM PATENT, TRADEMARK, OR COPYRIGHT INFRINGEMENT. Use of any trademarks in this presentation is not intended in any way to infringe on the rights of the

451

PowerPoint Presentation  

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

1 campaign statistics 1 campaign statistics and plans presented by R. Granetz Alcator C-Mod quarterly review 2011/05/05 C-Mod FY2011 operation * Budgeted for 15 research run weeks (60 run days) * 14.5 research run weeks have been completed to date * 1719 plasma discharges (I p > 0.1 MA and τ pulse > 0.1 s) > 90% plasma initiation success rate * 54 different miniproposals have received run time so far, with emphasis on: * pedestal studies (FY2011 joint facility research topic, J Hughes) * characterization and optimization of I-mode (E. Marmar) * lower hybrid density limit (G. Wallace) * rotation reversal (J. Rice) * 30 full or half run days led by grad students (i.e. session leaders) 2/5 C-Mod FY2011 operation, cont. * 10 PhD students obtained the bulk of their thesis data and/or completed their research

452

Oral Presentation Guidance  

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

Revised 04/01/2011 Page 1 of 2 Revised 04/01/2011 Page 1 of 2 09 ORAL PRESENTATION GUIDANCE The following guidance is not intended to replace or circumvent any existing agency-level guidance or regulation; the guidance is intended to enhance the agency's effectiveness when interviewing potential Energy Service Company (ESCOs). NOTE: Use for down selection of two or more ESCOs INSTRUCTIONS * Preplan your interview(s) * Be prepared o Decide whether to have video conference; webinar, telephonically or face-to-face interview (recommended). o Meet with the Acquisition Team (including your DOE Project Facilitator) at least one hour prior to the first ESCO interview. o Prepare questions and discussion issues based on the Team's comments and concerns. * Be brief o Recommend scheduling a 1 or 1-1/2 hour for each interview.

453

PowerPoint Presentation  

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

Bipolar Nickel Metal Hydride Battery Bipolar Nickel Metal Hydride Battery Development and Testing DOE ENERGY STORAGE SYSTEMS RESEARCH PROGRAM ANNUAL PEER REVIEW November 2 - 3, 2006, Washington, D.C. James Landi jlandi@electroenergyinc.com 203-797-2699 Program Objectives and Benefits  The objective of this program is to further develop the bipolar NiMH battery design to be used in high-energy and high-power energy storage applications. - Build and demonstrate large-format batteries - Demonstrate these batteries in present and future applications  The bipolar NiMH battery could provide the following benefits: - Improve efficiencies by reducing transmission peaking losses and shifting peak demands. - Reduce power and voltage sag to users. - Provide an efficient method to distribute backup energy/power

454

PowerPoint Presentation  

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

nd nd Energy & Innovation Conference November 28-29, 2012 Partnering for Innovation: Critical Materials Roe-Hoan Yoon, Lead Paul King, Business Development Critical Materials Strategic Growth Area NETL-Regional University Allience 2 o Critical: * Intrinsically rare, low grade, or currently unavailable in the United States. o Energy Critical Elements: * Chemical elements that are essential for the deployment of transformative energy technologies. Critical Materials-Definition 3 Application of Critical Materials 3 4  Short Term (present t - 2015) Criticality Matrix Your Logo  Mid Term (2015 - 2025) 5  Essential for the U.S. leading the 6 th wave of technology innovation o Renewable energy development o High-tech industry o Sustainability

455

PowerPoint Presentation  

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

We'd like to hear from you..." We'd like to hear from you..." "We'd like to hear from you..." * Encourage greater use of ARM data by the modeling community * Create highly polished datasets suitable for modelers * Possible future availability of statistical summaries for all standard ARM products (plots and/or datasets) * Possible future 'on the fly' calculation of statistical quantities, integrated into ARM archive interface The Purpose The Purpose This work was performed under the auspices of the U.S. Department of Energy by University of California Lawrence Livermore National Laboratory under contract No. W-7405-Eng-48. CRL-POST-229191 We present a prototype statistical summary of ARM observations designed for use by climate modelers. LLNL developed this prototype as a way of obtaining

456

PowerPoint Presentation  

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

BOEM Lower 48 Assessment BOEM Lower 48 Assessment Matthew Frye BOEM - Herndon, VA 6 June 2013 Update on BOEM Lower 48 Assessment A presentation to the Methane Hydrate Advisory Committee Matthew Frye Resource Evaluation Division BOEM - Herndon, VA matt.frye@boem.gov 6 June 2013 BOEM Resource Evaluation Division gas hydrate webpage: http://www.boem.gov/Oil-and-Gas-Energy-Program/Resource- Evaluation/Gas-Hydrates/index.aspx Update on BOEM Lower 48 Assessment Matthew Frye BOEM - Herndon, VA 6 June 2013 Update on BOEM Lower 48 Assessment Matthew Frye BOEM - Herndon, VA 6 June 2013 Oil and Gas Production on the US OCS Reserve Estimation Exploratory & Development Well Drilling Lease / Tract Award ("fair market value determination")

457

PowerPoint Presentation  

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

Implementation of Implementation of EPA's Class VI Geologic Sequestration Program Bruce Kobelski and Mary Rose Bayer Pittsburgh, PA November 15, 2011 U.S. Environmental Protection Agency UIC Program Background * 1974 Safe Drinking Water Act (SDWA; reauthorized in 1996) - Federal regulations to ensure protection of Underground Sources of Drinking Water (USDWs) * USDWs are defined as - Any aquifer or portion of an aquifer that contains water that is less than 10,000 ppm total dissolved solids or contains a volume of water such that it is a present, or viable future source for a Public Water Supply System * The UIC Program regulates injection of all fluids - liquid, gas, or slurry - Some natural gas storage, oil and gas production, and hydraulic fracturing fluids are exempted

458

PowerPoint Presentation  

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

Requirements Requirements for NERSC repository m327: "Parallel Simulation of Electron Cooling Physics and Beam Transport" Work supported by the US DOE Office of Science, Office of Nuclear Physics, including grant No.'s DE-FC02-07ER41499 and DE-SC0000835. Resources of NERSC were used. Workshop: Large Scale Computing and Storage Requirements for Nuclear Physics May 26, 2011 Presenter: D.L. Bruhwiler, 1 Contributors: B.T. Schwartz, 1 V.H. Ranjbar, 1 G.I. Bell 1 Other m327 users: J. Qiang, 4 S. White, 2 Y. Luo 2 Collaborators: R. Ryne, 4 V.N. Litvinenko, 2 W. Fischer, 2 G. Wang, 2 Y. Hao, 2 K. Paul, 1 I. Pogorelov 1 1. Tech-X Corporation 2. Brookhaven National Lab 3. Thomas Jefferson National Lab

459

PowerPoint Presentation  

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

Utility-Scale Solar 2012 Utility-Scale Solar 2012 An Empirical Analysis of Project Cost, Performance, and Pricing Trends in the United States Mark Bolinger & Samantha Weaver Lawrence Berkeley National Laboratory September 2013 1 This research was supported by funding from the U.S. Department of Energy's SunShot Initiative. Presentation Outline * Recent market growth has resulted in a critical mass of project-level data ripe for analysis * Key findings from this inaugural edition  Installed Costs/Prices  Operating (O&M) Costs  Performance (Capacity Factors)  Power Purchase Agreement ("PPA") Prices 2 A few background notes about this first edition: * Certain data (e.g., O&M costs) were still rather limited for this first edition, but are

460

PowerPoint Presentation  

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

Cloud Life Cycle and Structure Cloud Life Cycle and Structure A.M. Vogelmann, E. Luke, M.P. Jensen, P. Kollias, Brookhaven National Laboratory, Upton, New York and E.R. Boer LUEBEC, San Diego, CA SUMMARY SUMMARY * * Cloud tracking using geostationary satellite data provides a context of the cloud state observed at the ARM Sites, including the cloud's life-cycle stage and its representativeness of the region. * * Examples are presented of the duration and paths of mesoscale convective systems within the Tropical Western Pacific. * * This information will be used to interpret the cloud microphysical retrievals and overlap structure measured at the ARM sites. Reference Reference Boer, E. R., and V. Ramanathan, 1997: Lagrangian approach for deriving cloud characteristics from satellite observations and its implications to cloud

Note: This page contains sample records for the topic "testimony presentations radio" 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

PowerPoint Presentation  

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

ProActive DNS ProActive DNS Blacklisting Gene Rackow Argonne National Laboratory The Basics of DNS Hostname to IP mapping and back Host aliases Mail server locations Services Security records What is DNS Blacklisting? DNS Blacklist also known as a DNS Blackhole. Local server fakes zones know to contain: Malware Spyware Command/Control Advertising Political Issues What are DNS Blacklist Benefits Preventing hosts from getting to bad stuff. If you are not presented with the malware, Chances are you are not going to be infected. Estimates are that blocking Advertising sites stops 85% of infections. DNS Blacklist Sources of information Bad News about DNS Blacklisting Typically It's ReActive. Entries are added AFTER something happened. Some machines have already been

462

PowerPoint Presentation  

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

SEISMO-ACOUSTIC IMAGERY OF A SEISMO-ACOUSTIC IMAGERY OF A CARBONATE/HYDRATE MOUND IN THE GULF OF MEXICO Thomas McGee and Leonardo Macelloni Center for Marine Resources and Environmental Technology University of Mississippi Presented to the American Geophysical Union Fall Meeting San Francisco, California 11-15 December 2006 BACKGROUND INFORMATION In the northern Gulf of Mexico, hydrates outcrop within carbonate mounds precipitated by microbial action at sites of hydrocarbon venting from cold seeps. Such seeps are located along faults that act as pathways for fluids migrating upward from deep reservoirs. Location of MC118 The Gulf of Mexico Hydrate Research Consortium has begun to install a sea-floor observatory at such a mound in federal lease block Mississippi Canyon 118. Thanks for your attention.

463

PowerPoint Presentation  

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

Nanostructured Electrode and Electrolyte Nanostructured Electrode and Electrolyte Development for Energy Storage Devices Presented by Karen Waldrip Sandia National Laboratories Albuquerque, NM Funded by the Energy Storage Systems Program of the U.S. Department Of Energy (DOE/ESS) and by the Small Business Innovation Research (SBIR) program, and managed by Sandia National Laboratories (SNL). Sandia is a multi-program laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy's National Nuclear Security Administration, under contract DE-AC04-94AL85000. - SNL, GINER, and ADA - Electrochemical Storage Program Reviews - Capacitor Development Activities D. Ingersoll, F.M. Delnick, and K.E. Waldrip Sandia National Laboratories PO Box 5800 Albuquerque, NM 87185-0614

464

PowerPoint Presentation  

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

PUMP CANYON TEST SITE PUMP CANYON TEST SITE Prepared For: 2009 Regional Carbon Sequestration Partnerships Annual Review Meeting Prepared By: George J. Koperna, Jr. Advanced Resources International, Inc. Pittsburgh, November 16-19, 2009 1 1 2 RCSP SP111709 Presentation Outline * Introduction * Operations * Reservoir Characterization and Modeling * Monitoring, Verification and Accounting * Next Steps 3 RCSP SP111709 Objectives * Field-test the effectiveness of CO 2 sequestration in deep, unmineable coal seams via a small-scale geologic sequestration demonstration * Develop a better understanding of the efficacy of enhanced coalbed methane recovery processes via carbon dioxide injection (CO 2 -ECBM) into a pressure-depleted reservoir * Monitor plume migration to prevent any leakage 4 RCSP SP111709

465

PowerPoint Presentation  

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

Ingersoll, F.M. Delnick, and K.E. Waldrip Ingersoll, F.M. Delnick, and K.E. Waldrip Sandia National Laboratories PO Box 5800 Albuquerque, NM 87185-0614 High Voltage Electrochemical Capacitor presented at EESAT 2007 September 23-27, 2007 PEER Review San Francisco, CA Sandia is a multi-program laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000. 2 Objective * New Start - 7/07 * Increasing the energy of the system * Energy = 1/2 CV 2 * Four general means to increasing energy - Increased surface area - most common approach * A - active area of electrode - high surface area materials (carbon - typically > 1000 m 2 /g) - nanomaterials (e.g. carbon multiwalled nanotube) - Employ Faradaic processes -

466

PowerPoint Presentation  

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

NATIONAL CHAIRS MEETING NATIONAL CHAIRS MEETING Deer Creek State Park, Mt. Sterling, Ohio November 5-7, 2013 U.S. Department of Energy Practices Related to Public Input Presented by Greg Simonton Federal Coordinator Portsmouth SSAB EM SSAB NATIONAL CHAIRS MEETING Deer Creek State Park, Mt. Sterling, Ohio November 5-7, 2013 DOE Appreciation  The Department recognizes the members of the Site Specific Advisory Boards and Citizens Advisory Boards are volunteers and dedicate a lot of time to this work.  The Department also recognizes that members are asked to weigh in on complex and sometimes controversial issues that can have dramatic impacts on their communities.  The Department acknowledges that careful thought goes into recommendations and other input and that members bring a vital perspective to DOE operations.

467

PowerPoint Presentation  

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

Productivity Dispersion Productivity Dispersion Productivity Dispersion Productivity Dispersion and Input Prices: and Input Prices: The Case of Electricity The Case of Electricity Steven J. Davis - University of Chicago and NBER Cheryl Grim - U.S. Census Bureau John Haltiwanger - University of Maryland and NBER April 8, 2008 Disclaimer: This work is unofficial and thus has not undergone the review accorded to official U.S. Census Bureau publications. The views expressed are those of the authors and not necessarily those of the Census Bureau. This presentation has been screened to ensure no confidential data are revealed. Background Background * Prior research (Davis and Haltiwanger, 2001) shows that it is important to consider aggregate and allocative effects of oil price shocks - Positive oil shocks have adverse aggregate effect

468

Oral Presentation Guidance  

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

Revised 04/01/2011 Page 1 of 2 Revised 04/01/2011 Page 1 of 2 09 ORAL PRESENTATION GUIDANCE The following guidance is not intended to replace or circumvent any existing agency-level guidance or regulation; the guidance is intended to enhance the agency's effectiveness when interviewing potential Energy Service Company (ESCOs). NOTE: Use for down selection of two or more ESCOs INSTRUCTIONS * Preplan your interview(s) * Be prepared o Decide whether to have video conference; webinar, telephonically or face-to-face interview (recommended). o Meet with the Acquisition Team (including your DOE Project Facilitator) at least one hour prior to the first ESCO interview. o Prepare questions and discussion issues based on the Team's comments and concerns. * Be brief o Recommend scheduling a 1 or 1-1/2 hour for each interview.

469

X-ray Emission Processes in Radio Jets  

E-Print Network [OSTI]

The emission processes responsible for the observed X-rays from radio jets are commonly believed to be non-thermal, but in any particular case, it is unclear if synchrotron emission or one or more varieties of inverse Compton emission predominates. We present a formulation of inverse Compton emission from a relativistically moving jet (``IC/beaming'') which relies on radio emitting synchrotron sources for which the energy densities in particles and fields are comparable. We include the non-isotropic nature of inverse Compton scattering of the relativistic electrons on photons of the cosmic microwave background (CMB) and provide beaming parameters for a number of jets. A list of X-ray emitting jets is given and the jets are classified on the basis of their morphology and spectral energy distribution to determine their likely emission process. We conclude that these jets have significant bulk relativistic velocities on kpc scales; that higher redshift sources require less beaming because the energy density of the CMB is significantly greater than locally; and that for some nearby sources, synchrotron X-ray emission predominates because the jet makes a large angle to the line of sight.

D. E. Harris; H. Krawczynski

2001-09-27T23:59:59.000Z

470

Hermetic aluminum radio frequency interconnection and method for making  

DOE Patents [OSTI]

The present invention provides a light-weight, hermetic coaxial radio-frequency (RF) interconnection having an electrically conductive outer housing made of aluminum or an aluminum alloy, a central electrical conductor made of ferrous or non-ferrous material, and a cylinder of dielectric material comprising a low-melting-temperature, high-thermal-expansion aluminophosphate glass composition for hermetically sealing between the aluminum-alloy outer housing and the ferrous or non-ferrous center conductor. The entire RF interconnection assembly is made permanently hermetic by thermally fusing the center conductor, glass, and housing concurrently by bringing the glass to the melt point by way of exposure to an atmospheric temperature sufficient to melt the glass, less than 540.degree. C., but that does not melt the center conductor or the outer aluminum or aluminum alloy housing. The composition of the glass used is controlled to provide a suitable low dielectric constant so that an appropriate electrical characteristic impedance, for example 50 ohms, can be achieved for an electrical interconnection that performs well at high radio frequencies and also provides an interconnection maintaining a relatively small physical size.

Kilgo, Riley D. (Albuquerque, NM); Kovacic, Larry (Albuquerque, NM); Brow, Richard K. (Rolla, MO)

2000-01-01T23:59:59.000Z

471

A high frequency radio study of G11.2-0.3, a historical supernova remnant with a flat spectrum core  

E-Print Network [OSTI]

We present radio maps of the historical supernova remnant G11.2-0.3 in the frequency range from 4.85 GHz to 32 GHz. The integrated spectrum with \\alpha = -0.50 (S ~ \

R. Kothes; W. Reich

2001-04-24T23:59:59.000Z

472

Radio-Ecological Situation in River Basins of Central Asia Syrdarya and Amudarya According to the Results of the Project Navruz  

Science Journals Connector (OSTI)

The results of investigations of radio-ecological situation in river basins of Central Asia Syrdarya and Amudarya have been presented. The work has been fulfilled under the International project "Navruz" (USA,...

D. S. Barber; B. S. Yuldashev

2003-01-01T23:59:59.000Z

473

PowerPoint Presentation  

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

William Gausman William Gausman Sr. Vice President Asset Management & Planning DOE Energy Information Administration Washington, DC April 7, 2010 PHI's Smart Grid Vision and Investment Grant Awards 1 Presentation Overview * PHI Company overview * PHI's Smart Grid Vision * SGIG Awards - Scope, Costs, Benefits and Schedules * Distribution Automation * Key Next Steps 2 Combined Service Territory Transmission & Distribution Competitive Energy / Other Who is Pepco Holdings, Inc. PHI Investments 2 Regulated transmission and distribution is PHI's core business. 3 Business Overview Gas Customers ►778,000 ►498,000 ►123,000 ►547,000 GWh ►26,549 ►12,494 ► N/A ►9,659 Mcf (000's) ► N/A ► N/A ►19,044 ► N/A Service Area ►640 ►5,000 ►275 ►2,700 (square miles)

474

PowerPoint Presentation  

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

974 1 974 1 Introducing SAM (Sun and Aureole Measurement), a New, Ground-based Capability for Measuring Cloud Optical Properties Presented to Cloud Properties Working Group IRF Working Group ARM Science Team Meeting John DeVore (devore@visidyne.com) A.T. Stair (ats@visidyne.com) Bob McClatchey 1 (RMcClatchey@msn.com) Visidyne, Inc. 781-273-2820 March 2006 1 Consultant VI-4974 2 Space-Based Sun-Tracking Zenith-Viewing Cirrus (Ice Columns) Solar elevation = 45 deg Sat depression = 45 deg Surface albedo = 0.2 10 +4 10 +2 10 +0 10 -2 550 nm Radiance (W/cm 2 /sr/μm) 0.1 1.0 100. 10. Optical Depth Space-Based Sun-Tracking Zenith-Viewing Cirrus (Ice Columns) Solar elevation = 45 deg Sat depression = 45 deg Surface albedo = 0.2 10 +4 10 +2 10 +0 10 -2 550 nm Radiance (W/cm 2 /sr/μm) 0.1 1.0 100. 10. Optical Depth

475

RADIoLOGICALsURvEY AT  

Office of Legacy Management (LM)

RADIoLOGICALsURvEY RADIoLOGICALsURvEY AT 1411 CENTRAL AVENUE DETROIT, MICHIGAN Prepared by M.R. LANDIS Environmental Survey and Site Assessment Program Energy/Environment Systems Division Oak Ridge Associated Universities Oak Ridge, TN 37831-0117 Project Staff J.D. Berger H.J. Laudeman C.H. Searcy T.J. Sowell D.A. Gibson E.A. Powell S.M. Shanmugan C.F. Weaver Prepared for U.S. Department of Energy as part of the Formerly Utilized Sites - Remedial Action Program FINAL REPORT FEBRUARY 1990 This report is based on work performed under contract number DE-AC05-760R00033 with the U.S. Department of Energy. TABLE OF CONTENTS ListofFigures .......................... List of Tables. ........................... Introduction ............................ Facility Description. ........................

476

Radio bursts from Solar System planets  

E-Print Network [OSTI]

interaction · Kinetic energy flux on obstacle cross-section : Pk ~ NmV2 V Robs 2 N=No/d2 No=5 cm-3 m~1.1?mp RobsP 2 #12;Flow Obstacle Weakly/Not magnetized (Solar wind) Strongly magnetized (Jovian magnetosphereRadio bursts from Solar System planets and Extrasolar planets Philippe Zarka Observatoire de Paris

Demoulin, Pascal

477

Radio Source Evolution on Galactic Scales  

E-Print Network [OSTI]

profile external atmosphere. Key words: galaxies: jets radiation mechanisms: non-thermal galaxies: active 1 INTRODUCTION Understanding the detailed evolution of radio-loud jets and co- coons as they propagate through the intragalactic and intracluster... shocks the IGM/ICM at the hotspot, and once the jet material becomes under-dense, a backflow of material at the hotspot inflates enormous cocoons filled with a plasma of particles and magnetic fields. The jet pushes forward and the co- coon expands...

Maciel, T.; Alexander, P.

2014-01-01T23:59:59.000Z

478

Preparing a public database of radio sources  

E-Print Network [OSTI]

We have collected the largest existing set of radio source lists in machine-readable form: 320 tables with 1.75 million records. Only a minor fraction of these is accessible via public databases. We describe our plans to make this huge amount of heterogeneous data accessible in a homogeneous way via the World Wide Web, with reliable cross-identifications, and searchable by various observables.

H. Andernach; S. A. Trushkin; A. G. Gubanov; O. V. Verkhodanov; V. B. Titov; A. Micol

1996-07-22T23:59:59.000Z

479

Barrier Immune Radio Communications for Demand Response  

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

Barrier Immune Radio Communications for Demand Response Barrier Immune Radio Communications for Demand Response Title Barrier Immune Radio Communications for Demand Response Publication Type Report LBNL Report Number LBNL-2294e Year of Publication 2009 Authors Rubinstein, Francis M., Girish Ghatikar, Jessica Granderson, Paul Haugen, Carlos Romero, and David S. Watson Keywords technologies Abstract Various wireless technologies were field-tested in a six-story laboratory building to identify wireless technologies that can scale for future DR applications through very low node density power consumption, and unit cost. Data analysis included analysis of the signal-to-noise ratio (SNR), packet loss, and link quality at varying power levels and node densities. The narrowband technologies performed well, penetrating the floors of the building with little loss and exhibiting better range than the wideband technology. 900 MHz provided full coverage at 1 watt and substantially complete coverage at 500 mW at the test site. 900 MHz was able to provide full coverage at 100 mW with only one additional relay transmitter, and was the highest-performing technology in the study. 2.4 GHz could not provide full coverage with only a single transmitter at the highest power level tested (63 mW). However, substantially complete coverage was provided at 2.4 GHz at 63 mW with the addition of one repeater node.

480

Cosmology with SKA Radio Continuum Surveys  

E-Print Network [OSTI]

Radio continuum surveys have, in the past, been of restricted use in cosmology. Most studies have concentrated on cross-correlations with the cosmic microwave background to detect the integrated Sachs-Wolfe effect, due to the large sky areas that can be surveyed. As we move into the SKA era, radio continuum surveys will have sufficient source density and sky area to play a major role in cosmology on the largest scales. In this chapter we summarise the experiments that can be carried out with the SKA as it is built up through the coming decade. We show that the SKA can play a unique role in constraining the non-Gaussianity parameter to \\sigma(f_NL) ~ 1, and provide a unique handle on the systematics that inhibit weak lensing surveys. The SKA will also provide the necessary data to test the isotropy of the Universe at redshifts of order unity and thus evaluate the robustness of the cosmological principle.Thus, SKA continuum surveys will turn radio observations into a central probe of cosmological research in th...

Jarvis, Matt J; Blake, Chris; Brown, Michael L; Lindsay, Sam N; Raccanelli, Alvise; Santos, Mario; Schwarz, Dominik

2015-01-01T23:59:59.000Z

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481

Particle acceleration in double radio sources  

Science Journals Connector (OSTI)

Further study has been made of a model of extragalactic double radio sources in which the magnetized accretion disc of a massive black hole acts as an electric dynamo producing oppositely directed beams of relativistic particles. An empty region of small angular sizea vortice coreis shown to be a possible consequence of the hydrodynamics of accretion of gas with angular momentum. An ambient magnetic field in the gas tends to accumulate in the core region. The acceleration of electrons in the dynamo electric field gives rise to oppositely directed electron beams which in turn produce synchroton gamma rays collimated along the core. Collisions between the gamma rays and low energy photons caN initiate an electromagnetic cascade shower. The cascade acts to produce a collimated relativistic electron?positron beam. If the current flow in the dynamo occurs in surges then the outward propagation of the head of the electronpositron beams may produce expanding compact radio components. The electronpositron beam is ballistic in nature and it is electrically neutral and carries no current. Such a beam appears to have favorable stability properties. The beam is eventually stopped and spread out in pitch angle by the ram pressure of the external medium. Synchrotron radiated lobes of double radio sources.

R. V. E. Lovelace; J. MacAuslan; M. Burns

1979-01-01T23:59:59.000Z

482

Discovery of a Radio Flare from GRB 990123  

E-Print Network [OSTI]

We report the discovery of a radio counterpart to GRB 990123. In contrast to previous well-studied radio afterglows which rise to peak flux on a timescale of a week and then decay over several weeks to months, the radio emission from this GRB was clearly detected one day after the burst, after which it rapidly faded away. The simplest interpretation of this ``radio flare'' is that it arises from the reverse shock. In the framework of the afterglow models discussed to date, a forward shock origin for the flare is ruled out by our data. However, at late times, some radio afterglow emission (commensurate with the observed late-time optical emission, the optical afterglow) is expected from the forward shock. The relative faintness of the observed late-time radio emission provides an independent indication for a jet-like geometry in this GRB. We use the same radio observations to constrain two key parameters of the forward shock, peak flux and peak frequency, to within a factor of two. These values are inconsistent with the notion advocated by several authors that the prompt optical emission detected by ROTSE smoothly joins the optical afterglow emission. Finally, with hindsight we now recognize another such radio flare and this suggests that one out of eight GRBs has a detectable radio flare. This abundance coupled with the reverse shock interpretation suggests that the radio flare phenomenon has the potential to shed new light into the physics of reverse shocks in GRBs.

S. R. Kulkarni; D. A. Frail; R. Sari; G. H. Moriarty-Schieven; D. S. Shepherd; P. Udomprasert; A. C. S. Readhead; J. S. Bloom; M. Feroci; E. Costa

1999-03-30T23:59:59.000Z

483

RESEARCH POSTER PRESENTATION DESIGN 2011 www.PosterPresentations.com  

E-Print Network [OSTI]

RESEARCH POSTER PRESENTATION DESIGN © 2011 www.PosterPresentations.com Entangled Phenomena: Literac

Amin, S. Massoud

484

State-Level Energy-Related Carbon Dioxide Emissions, 2000-2009  

Annual Energy Outlook 2013 [U.S. Energy Information Administration (EIA)]

Press Releases Presentations Congressional Testimony Radio Spots Enter Search Term(s): Search eia.gov A-Z Index A-Z Index A B C D E F G H I J K L M N O P Q R S T U...

485

December 3, 2003, Board Public Meeting Speaker Presentations  

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

from Mike Mallory Before the DNFSB December 3, 2003 from Mike Mallory Before the DNFSB December 3, 2003 Page 0 Testimony of Mike Mallory, BWXT Pantex President and General Manager Before the Defense Nuclear Facilities Safety Board Regarding Contractor Assurance System at Pantex Plant December 3, 2003 Testimony from Mike Mallory Before the DNFSB December 3, 2003 Page 1 The Contractor Assurance System at BWXT Pantex Introduction Thank you for the opportunity to speak today regarding the Contractor Assurance System at BWXT Pantex. I am Mike Mallory, the President and General Manager of BWXT Pantex, the M&O contractor of the Pantex Plant for the Department of Energy's National Nuclear Security Administration. BWXT Pantex is responsible for five core missions at Pantex. 1) We evaluate, retrofit and repair

486

Radio-frequency glow discharge spectrometry:: A critical review  

Science Journals Connector (OSTI)

This paper presents a critical review of analytical radio frequency glow discharge spectrometry (rf-GDS). The historical foundations of rf-GDS are described, and current knowledge of the fundamental physics of analytical rf glow discharges is discussed. Additionally, instrumentation, methodologies, and applications of rf glow discharge optical emission spectrometry (rf-GDOES) and mass spectrometry (rf-GDMS) are reviewed. Although other rf-GDS techniques have appeared [e.g. rf glow discharge atomic absorption spectrophotometry (rf-GDAAS)], the emphasis is placed upon rf-GDOES and rf-GDMS, because they have received by far the most interest from analytical chemical metrologists. This review also provides explanations of some developments that are needed for further progress in the field of analytical rf-GDS.

Michael R. Winchester; Richard Payling

2004-01-01T23:59:59.000Z

487

Congressional Testimony | Department of Energy  

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

October 13, 2011 October 13, 2011 Before the House Science, Space, and Technology Subcommittee on Energy and Environment Subject: Coal Research and Development By: Scott Klara, Deputy Director National Energy Technology Laboratory September 22, 2011 Before the House Subcommittee on Water and Power Subject: Western Area Power Administration's Borrowing Authority (H.R. 2915) By: Lauren Azar, 
Senior Advisor, 
Office Of The Secretary Of Energy, U.S. Department Of Energy September 22, 2011 Before the House Subcommittee on Water and Power Subject: H.R. 1719 By: Gregory K. Delwiche, Senior Vice President Of Power Services, Bonneville Power Administration September 22, 2011 Before the House Committee on Oversight and Government Reform By: Deputy Secretary Daniel Poneman, U.S. Department of Energy

488

Pete_Lyons_Nomination_Testimony  

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

Peter B. Lyons Peter B. Lyons Assistant Secretary for Nuclear Energy Designee Before the Committee on Energy and Natural Resources United States Senate March 8, 2011 Chairman Bingaman, Ranking Member Murkowski, and distinguished Members of the Committee, it is an honor and a privilege to appear before you today as President Obama's nominee for Assistant Secretary for Nuclear Energy within the Department of Energy. It is a special honor for me to appear before this Committee. I worked with the Members and staff of this Committee for eight years while I was in Senator Domenici's personal office, and later when I served on the staff of this Committee. I originally came to the Senate on a detail from Los Alamos National Laboratory, where I worked for nearly 30 years.

489

Congressional Testimony | Department of Energy  

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

August 6, 2009 August 6, 2009 Office of Policy and International Affairs Before the Senate Environment an Public Works Committee Subject: Climate Change and Ensuring that America Leads the Clean Energy Transformation By: David Sandalow, Assistant Secretary August 5, 2009 Before the Senate Homeland Security and Governmental Affairs Subcommittee on Oversight of Government Management, the Workforce, and the District of Columbia Subject: Strengthening the Federal Acquisition Workforce: Government-wide Leadership and Initiatives By: John Bashista, Deputy Director, Office of Procurement and Assistance Management, Office of Management July 30, 2009 Before the House Natural Resources Subcommittee on Energy and Mineral Resources Subject: Unconventional Fuels, Part II: The Promise of Methane Hydrates

490

Final_Poneman_Testimony.pdf  

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

Daniel Poneman Daniel Poneman Deputy Secretary of Energy U.S. Department of Energy before the House Energy and Commerce Committee on H.R. 2054, the Energy and Revenue Enrichment Act of 2011 June 13, 2011 Introduction Thank you, Mr. Chairman, Ranking Member Waxman, and Members of the Committee. I appreciate this opportunity to appear before you and comment on legislation under consideration by the Committee, as well as to provide information on management and disposition of the Department of Energy's depleted uranium. The Administration continues to view nuclear power as an important element in its strategy to increase energy security and combat climate change. We join the

491

Microsoft Word - ML Final Testimony  

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

Michael W. Locatis, III Michael W. Locatis, III Chief Information Officer U.S. Department of Energy Before the Subcommittee on Technology, Information Policy, Intergovernmental Relations and Procurement Reform of the Committee on Oversight and Government Reform U.S. House of Representatives February 17, 2012 Good morning, Chairman Lankford, Ranking Member Connolly and other members of the Subcommittee. Thank you for this opportunity to testify today on the Government Accountability Office's (GAO) report on potentially duplicative IT investments. The Department of Energy (DOE) appreciates the work performed by the GAO to identify opportunities to improve mission effectiveness and fiscal efficiency. The DOE is dedicated to improving our overall IT portfolio management and to address areas identified in the GAO

492

Final_Testimony(20).pdf  

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

1 1 1 Chairman Bingaman, Ranking Member Murkowski, Members of the Committee, thank you for the opportunity to discuss the Implementation of National Consensus Appliance Agreements Act of 2011 (S.398) and the Better Use of Light Bulbs Act (S.395). In June 2009, President Obama said, "One of the fastest, easiest, and cheapest ways to make our economy stronger and cleaner is to make our economy more energy efficient." 1 Energy-conserving appliance standards are one of the significant steps the Administration has taken to save energy in homes and businesses nationwide, and pave the way toward a clean energy future for our country. 2 Since January 2009, the Department of Energy has finalized new efficiency standards for more than twenty household and commercial

493

Congressional Testimony | Department of Energy  

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

April 23, 2009 April 23, 2009 Before the Senate Energy and Natural Resources Committee Subject: Nomination Hearing By: Steven E. Koonin, Nominee for Under Secretary for Science April 23, 2009 Before the Senate Committee on Energy and Natural Resources Subject: Nomination Hearing By: Kristina M. Johnson, Under Secretary for Energy Designee April 22, 2009 Before the House Energy and Commerce Committee Subject: American Clean Energy and Security Act of 2009 By: Secretary Steven Chu April 22, 2009 Before the House Small Business Committee Subject: SBIR Reauthorization By: Larry James, Technology Transfer Program Manager, Office of Science April 22, 2009 Before the Senate Armed Services, Subcommittee on Strategic Forces Subject: EM Activities under the American Recovery and Reinvestment Act

494

Congressional Testimony | Department of Energy  

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

9, 2013 9, 2013 Before Senate Committee on Energy and Natural Resources Subject: Nomination for Secretary of Energy By: Ernest J. Moniz, Nominee for Secretary of Energy March 19, 2013 Before the Subcommittee on Energy Policy, Health Care, and Entitlements - House Oversight and Government Reform Committee Subject: Natural Gas Exports By: Christopher Smith, Acting Assistant Secretary for Fossil Energy March 13, 2013 Before the Subcommittee on Oversight and Investigations - House Energy and Commerce Committee Subject: Y-12 Security Event By: Daniel B. Poneman, Deputy Secretary of Energy February 28, 2013 Before the Subcommittee on Strategic Forces - House Armed Services Committee Subject: Security Incident at Y-12 National Security Complex By: Daniel B. Poneman, Deputy Secretary of Energy

495

Final_Testimony(26).pdf  

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

NATURAL RESOURCES NATURAL RESOURCES UNITED STATES SENATE May 5, 2011 2 Chairman Bingaman, Ranking Member Murkowski and members of the Committee, thank you for this opportunity to discuss the cyber security issues facing the electric industry, as well as proposed legislation intended to strengthen protection of the bulk power system and electric infrastructure from cyber security threats. Title XIII of the Energy Independence and Security Act of 2007 (EISA) states, "It is the policy of the United States to support the modernization of the Nation's electricity transmission and distribution system to maintain a reliable and secure electricity infrastructure." The protection and resilience of critical national infrastructures is a shared responsibility of the private sector,

496

Final_Testimony_JSilver.pdf  

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

Jonathan Silver Jonathan Silver Executive Director of the Loan Programs Office U.S. Department of Energy Before the Committee on Energy and Natural Resources United States Senate June 9, 2011 Introduction Chairman Bingaman, Ranking Member Murkowski, and members of the Committee, thank you for the opportunity to testify today. My name is Jonathan Silver, and I am the Executive Director of the Department of Energy's (DOE) Loan Programs Office (LPO). DOE's loan programs provide critical support for the nation's commercial deployment of clean energy technologies, and the jobs and economic growth that come with them. I welcome the opportunity to discuss the Advanced Technology Vehicles Manufacturing (ATVM) Loan Program with you and to highlight our significant accomplishments.

497

Congressional Testimony | Department of Energy  

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

May 5, 2011 May 5, 2011 Before the House Energy and Commerce Subcommittee on Energy and Power Subject: Alternative Transportation Fuels and Vehicles By: Patrick Davis, Program Manager Office of Energy Efficiency and Renewable Energy May 5, 2011 Before the House Energy and Commerce Subcommittee on Energy and Power Subject: Alternative Transportation Fuels and Vehicles By: Howard Gruenspecht, Deputy Administrator Energy Information Administration May 3, 2011 Before the Senate Energy and Natural Resources Committee Subject: Clean Energy Legislation By: Jonathan Silver, Director Office of Loan Guarantee Program April 13, 2011 Before the Senate Environment and Public Works Committee Subject: Domestic Renewable Fuels By: Henry Kelly, Acting Assistant Secretary Office of Energy Efficiency and

498

Final_Testimony(6).pdf  

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

Senior Advisor to the Secretary of Energy Before the Committee on Ways and Means United States House of Representatives April 14, 2010 Putting Americans to work, building a clean energy economy, and reducing our dependence on oil. Chairman Levin, Ranking Member Camp, and Members of the Committee, thank you for the opportunity to appear before you today to report on the progress of "The American Recovery and Reinvestment Act's"(Recovery Act) energy tax credit and grant programs. The Section 48C clean energy manufacturing tax credit and Section 1603 payments in lieu of tax credit programs have been among the most successful energy job creation and innovation programs under the Recovery Act to date, putting America back to work and positioning the US to regain leadership

499

Final_Testimony(21).pdf  

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

RICHARD NEWELL RICHARD NEWELL ADMINISTRATOR ENERGY INFORMATION ADMINISTRATION U.S. DEPARTMENT OF ENERGY before the COMMITTEE ON NATURAL RESOURCES U.S. HOUSE OF REPRESENTATIVES March 17, 2011 2 Mr. Chairman and Members of the Committee: I appreciate the opportunity to appear before you today to address the issue of rising gasoline prices and the role of available domestic oil and natural gas resources. The Energy Information Administration (EIA) is the statistical and analytical agency within the U.S. Department of Energy. EIA collects, analyzes, and disseminates independent and impartial energy information to promote sound policymaking, efficient markets, and public understanding regarding energy and its interaction with the economy and the environment. EIA is the Nation's

500

Final_Testimony_(Chalk).pdf  

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

STEVEN G. CHALK DEPUTY ASSISTANT SECRETARY FOR RENEWABLE ENERGY OFFICE OF ENERGY EFFICIENCY AND RENEWABLE ENERGY U.S. DEPARTMENT OF ENERGY BEFORE THE COMMITTEE ON ENERGY AND NATURAL RESOURCES UNITED STATES SENATE JUNE 7, 2011 1 Chairman Bingaman, Ranking Member Murkowski and Members of the Committee, thank you for the opportunity to discuss the Department of Energy's (DOE's) efforts to research, develop and deploy the next generation of alternative fuels and electric vehicles. I will also briefly discuss some areas of S. 937, the American Alternative Fuels Act of 2011, sponsored by Senator Barrasso. However, the Administration is still reviewing the bill and we do not have a position on the bill at this time. Alternative Fuels