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


1

Clean Cities: Margaret Smith  

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

about Clean Cities: Margaret Smith on Twitter Bookmark Clean Cities: Margaret Smith on Google Bookmark Clean Cities: Margaret Smith on Delicious Rank Clean Cities: Margaret Smith...

2

Clean Cities: Mark Smith  

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

Mark Smith to someone by E-mail Mark Smith to someone by E-mail Share Clean Cities: Mark Smith on Facebook Tweet about Clean Cities: Mark Smith on Twitter Bookmark Clean Cities: Mark Smith on Google Bookmark Clean Cities: Mark Smith on Delicious Rank Clean Cities: Mark Smith on Digg Find More places to share Clean Cities: Mark Smith on AddThis.com... Goals & Accomplishments Partnerships Hall of Fame Contacts Mark Smith Vehicle Technologies Deployment Manager Mark Smith is the vehicle technologies deployment manager for the Department of Energy's (DOE) national Clean Cities program. His responsibilities include developing outreach strategies for implementing new national partnerships between industry and the Clean Cities program to successfully deploy new vehicle technologies. Smith also works with the

3

Clean Cities: Margaret Smith  

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

West Technologies, Smith worked for Sustainable Energy Strategies, Inc., supporting biodiesel and ethanol projects that improve infrastructure, develop feedstocks, educate...

4

George DW Smith  

Science Conference Proceedings (OSTI)

Feb 17, 2012 ... Miller's first contact with Smith was during his interview process at ... in the development and commercialization of the techniques of atom probe...

5

Dennis A. Smith  

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

Dennis A. Smith is the National Clean Cities Director in the Vehicle Technologies Program, Office of Energy Efficiency and Renewable Energy at the Department of Energy.

6

BNL | Graham Smith  

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

Graham Smith Graham Smith Graham Smith Head of the Instrumentation Division photo of Graham Smith The mission of the Instrumentation Division, with a staff of around 40, is to develop state-of-the-art instrumentation required for experimental research programs at Brookhaven Lab and elsewhere, and to maintain the expertise and facilities in specialized high technology areas essential for this work. The focus is on three major research areas: radiation detectors (using solid, liquid, or gas media); microelectronics; and laser, optical, and microfabrication applications. Smith's major scientific accomplishments include measuring the fundamental limits of gas-filled detectors, which enables researchers using synchrotron light sources like the NSLS to obtain the highest resolution

7

William M. Smith  

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

Smith COO Infotility, Inc. wmsmith@epri.com This speaker was a visiting speaker who delivered a talk or talks on the date(s) shown at the links below. This speaker is not otherwise...

8

ORISE Research Team Experiences: Michael Smith  

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

Astrophysicist Uses Celestial Knowledge to Cultivate Rising Stars Michael Smith ORNL Nuclear Astrophysicist Michael Smith inspects the framework of what will eventually become...

9

FL J. Smith, Jr.  

Office of Legacy Management (LM)

ct. B. Duillap ct. B. Duillap (THPJJs L. Kassel) FL J. Smith, Jr. c c Kelley from R. 1. Cook, Kslley from R. 1. Cook, J J cit cit In accordawe with Secret memorandum dated October , 1951 ta IA. E. In accordawe with Secret rwmorandnn dated October , 1951 ta IA. E. Qapletad Uranium for HAA and ML," we are Ylepletad Uranium for HAA and ML," we are obligated to fill the following orders obligated to fill the following orders North American Aviation North American Aviation . . One Inch roes One Inch roes a. Depleted U nrptalj U-235 content= 0.&9 f O.O& Meterial must be homogenemsj uniformity of assay, O&Q5%. : b. Diemeterc 0.99P (1( O.ooOn, - 0.003")j de-hrmd. YI E ,g C* pwh b" f1/32" Classification Cancelled d. Humber of rods: 1800

10

Smith Purcell radiation from femtosecond electron bunches  

E-Print Network (OSTI)

We present theoretical and experimental results from a Smith-Purcell radiation experiment using the electron beam from a 17 GHz high gradient accelerator. Smith- Purcell radiation occurs when a charged particle travels ...

Korbly, Stephen E

2005-01-01T23:59:59.000Z

11

Christopher A. Smith | Department of Energy  

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

A. Smith A. Smith About Us Christopher A. Smith - Principal Deputy Assistant Secretary and Acting Assistant Secretary for Fossil Energy Photo of Christopher Smith Christopher Smith is Principal Deputy Assistant Secretary and Acting Assistant Secretary for Fossil Energy with responsibilities for office operations and managing the oversight of Fossil Energy's Research and Development program (encompassing coal, oil and natural gas) and the U.S. Petroleum Reserves. He was appointed to the Department of Energy in 2009 as Deputy Assistant Secretary for FE's Office of Oil and Natural Gas. Smith served as the Designated Federal Official for the National Commission on the BP Deepwater Horizon Oil Spill and Offshore Drilling, established by President Obama to investigate the root causes of the Gulf oil spill.

12

David E. Smith - Program Managers - FEERC  

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

Tennessee. Dr. Smith is a vehicle systems engineer with industry experience in hybrid electric vehicle powertrain modeling, simulation, and supervisory control system design and...

13

VITA -Kord S. Smith I. PERSONAL DATA  

E-Print Network (OSTI)

-23, Myrtle Beach, SC, (1997). 31. Kord S. Smith, "MOX Analysis Methods in SIMULATE-3," Trans. Am. Nuc. Soc, January 11-14, 1998. 36. M. Edenius, D. Knott, K. Smith, "CASMO-SIMULATE on MOX and Advanced Designs Corrections for MOX Calculations," Proc. Intl. Con- ference on Physics of Nuclear Science and Technology, Vol

Chen, Sow-Hsin

14

Environmental assessment: Deaf Smith County site, Texas  

SciTech Connect

In February 1983, the US Department of Energy (DOE) identified a location in Deaf Smith County, Texas, as one of nine potentially acceptable sites for a mined geologic repository for spent nuclear fuel and high-level radioactive waste. To determine their suitability, the Deaf Smith County site and the eight other potentially sites have been evaluated in accordance with the DOE's General Guidelines for the Recommendation of Sites for the Nuclear Waste Repositories. The Deaf Smith County site is in the Permian Basin, which is one of five distinct geohydrologic settings considered for the first repository. On the basis of the evaluations reported in this EA, the DOE has found that the Deaf Smith County site is not disqualified under the guidelines. On the basis of these findings, the DOE is nominating the Deaf Smith County site as one of the five sites suitable for characterization. 591 refs., 147 figs., 173 tabs.

1986-05-01T23:59:59.000Z

15

International Peirce-Smith Converting Centennial  

Science Conference Proceedings (OSTI)

... and G. Guzman D. Full Utilization of the Matte Converting Process Energy for Operatiing ... Injection Techniques, Modeling and Process Control. Peirce-Smith ... M. Marinigh. Increasing Capacity and Productivity in the Metals Markets through.

16

Environmental assessment: Deaf Smith County site, Texas  

Science Conference Proceedings (OSTI)

In February 1983, the US Department of Energy (DOE) identified a location in Deaf Smith County, Texas, as one of the nine potentially acceptable sites for mined geologic repository for spent nuclear fuel and high-level radioactive waste. To determine their suitability, the Deaf Smith County site and eight other potentially acceptable sites have been evaluated in accordance with the DOE's General Guidelines for the Recommendation of Sites for the Nuclear Waste Repositories. The Deaf Smith County site is in the Permian Basin, which is one of five distinct geohydrologic settings considered for the first repository. On the basis of the evaluations reported in this EA, the DOE has found that the Deaf Smith County site is not disqualified under the guidelines.

Not Available

1986-05-01T23:59:59.000Z

17

Environmental assessment, Deaf Smith County site, Texas  

SciTech Connect

The Nuclear Waste Policy Act of 1982 (42 USC sections 10101-10226) requires the environmental assessment of a proposed site to include a statement of the basis for nominating a site as suitable for characterization. Volume 2 provides a detailed statement evaluating the site suitability of the Deaf Smith County Site under DOE siting guidelines, as well as a comparison of the Deaf Smith County Site to the other sites under consideration. The evaluation of the Deaf Smith County Site is based on the impacts associated with the reference repository design, but the evaluation will not change if based on the Mission Plan repository concept. The second part of this document compares the Deaf Smith County Site to Davis Canyon, Hanford, Richton Dome and Yucca Mountain. This comparison is required under DOE guidelines and is not intended to directly support subsequent recommendation of three sites for characterization as candidate sites. 259 refs., 29 figs., 66 refs. (MHB)

Not Available

1986-05-01T23:59:59.000Z

18

A.O. Smith | Open Energy Information  

Open Energy Info (EERE)

A.O. Smith A.O. Smith Jump to: navigation, search Name A.O. Smith Place Milwaukee, WI Zip 53224 Sector Efficiency Stock Symbol AOS Number of employees 10,000 Phone number 414-359-4000 Website http://www.aosmith.com/ Coordinates 43.1676911°, -88.0411993° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.1676911,"lon":-88.0411993,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

19

Celebrating Black History Month with DOE's Christopher Smith | Department  

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

Celebrating Black History Month with DOE's Christopher Smith Celebrating Black History Month with DOE's Christopher Smith Celebrating Black History Month with DOE's Christopher Smith February 16, 2011 - 12:08pm Addthis Acting Assistant Secretary Smith Acting Assistant Secretary Smith Principal Deputy Assistant Secretary and Acting Assistant Secretary for Fossil Energy Throughout the month of February, we've been introducing remarkable African Americans who are working to advance the President's clean energy agenda. This week we're highlighting Christopher Smith, the Department's Deputy Assistant Secretary for Oil and Natural Gas in the Office of Fossil Energy. Below is a post he wrote that was featured on White House blog earlier this month. I'm lucky to have been raised by my parents, Raymond and Sue Ann Smith, who

20

Celebrating Black History Month with DOE's Christopher Smith | Department  

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

Christopher Smith Christopher Smith Celebrating Black History Month with DOE's Christopher Smith February 16, 2011 - 12:08pm Addthis Acting Assistant Secretary Smith Acting Assistant Secretary Smith Principal Deputy Assistant Secretary and Acting Assistant Secretary for Fossil Energy Throughout the month of February, we've been introducing remarkable African Americans who are working to advance the President's clean energy agenda. This week we're highlighting Christopher Smith, the Department's Deputy Assistant Secretary for Oil and Natural Gas in the Office of Fossil Energy. Below is a post he wrote that was featured on White House blog earlier this month. I'm lucky to have been raised by my parents, Raymond and Sue Ann Smith, who value education. As we celebrate Black History Month, I reflect on the

Note: This page contains sample records for the topic "young buz smith" 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

10 Questions for a Biophysicist: Jeremy Smith | Department of Energy  

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

a Biophysicist: Jeremy Smith a Biophysicist: Jeremy Smith 10 Questions for a Biophysicist: Jeremy Smith May 5, 2011 - 3:51pm Addthis Dr Jeremy Smith | Photo Courtesy of ORNL Dr Jeremy Smith | Photo Courtesy of ORNL Niketa Kumar Niketa Kumar Public Affairs Specialist, Office of Public Affairs "With regards to super-computing, those cheeky hardware guys keep building more and more powerful machines and challenging us to perform cutting-edge simulations that efficiently use their full capability." Jeremy Smith In 2006, Dr. Smith came to Oak Ridge National Laboratory (ORNL). Since then, he has led a wide-ranging spectrum of projects focusing on everything from biofuels to drug discovery. He recently gave us the download on his many projects, how neutron scattering advances his work and why this clip

22

RF engineering basic concepts: the Smith chart  

E-Print Network (OSTI)

The Smith chart is a very valuable and important tool that facilitates interpretation of S-parameter measurements. This paper will give a brief overview on why and more importantly on how to use the chart. Its definition as well as an introduction on how to navigate inside the chart are illustrated. Useful examples show the broad possibilities for use of the chart in a variety of applications.

Caspers, F

2011-01-01T23:59:59.000Z

23

Smith Newton Vehicle Performance Evaluation (Brochure)  

DOE Green Energy (OSTI)

The Fleet Test and Evaluation Team at the U.S. Department of Energy's National Renewable Energy Laboratory is evaluating and documenting the performance of electric and plug-in hybrid electric drive systems in medium-duty trucks across the nation. Through this project, Smith Electric Vehicles will build and deploy 500 all-electric medium-duty trucks. The trucks will be deployed in diverse climates across the country.

Not Available

2012-08-01T23:59:59.000Z

24

Brimacombe, Cohen, and Smith: New TMS Awards Honor Materials ...  

Science Conference Proceedings (OSTI)

Oct 15, 2010 ... Smith started his career as a research metallurgist at the American Brass Company in 1927 and later joined the Manhattan Project at Los...

25

Isotopic Analysis- Rock At Long Valley Caldera Area (Smith &...  

Open Energy Info (EERE)

Isotopic Analysis- Rock At Long Valley Caldera Area (Smith & Suemnicht, 1991) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Isotopic Analysis-...

26

Low Dose Radiation Research Program: Richard D. Smith  

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

W.J., Wang, H.X., Petyuk, V.A., Bloom, J.S., Sforza, D.M., Lacan, G., Liu, D., Khan, A.H., Cantor, R.M., Bigelow, D.J., Melega, W.P., Camp, D.G., Smith, R.D., and Smith, D.J....

27

Smith Electric Vehicles US SEV US | Open Energy Information  

Open Energy Info (EERE)

Electric Vehicles US SEV US Electric Vehicles US SEV US Jump to: navigation, search Name Smith Electric Vehicles US (SEV-US) Place Kansas City, Missouri Zip 64163 Product Kansas-based company owned by US investors and the Tanfield Group, which manufactures all-electric zero-emissions commercial trucks. References Smith Electric Vehicles US (SEV-US)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Smith Electric Vehicles US (SEV-US) is a company located in Kansas City, Missouri . References ↑ "Smith Electric Vehicles US (SEV-US)" Retrieved from "http://en.openei.org/w/index.php?title=Smith_Electric_Vehicles_US_SEV_US&oldid=351204" Categories: Clean Energy Organizations

28

Smith Creek Geothermal Project | Open Energy Information  

Open Energy Info (EERE)

Geothermal Project Geothermal Project Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Development Project: Smith Creek Geothermal Project Project Location Information Coordinates 39.311388888889°, -117.55083333333° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.311388888889,"lon":-117.55083333333,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

29

Testimony of Christopher Smith before the House Committee on...  

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

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...

30

Gilbert M. Smith, master boatbuilder of Long Island, New York  

E-Print Network (OSTI)

The second half of the 19th century in maritime America was an era marked by a rich variety of vernacular watercraft types adapted to a wide range of local needs and traditions. The Great South Bay, located off Long Island, New York, was home to several variants of small work and pleasure craft. This thesis is an examination of Long Island boatbuilding via a study of the career of the most prolific and best known local boatbuilder, Gilbert Monroe Smith (1843-1940). It is estimated that Gil Smith built four hundred vessels from the 1860s through the 1930s, the twilight of wooden boat- and shipbuilding in coastal southern New England. Smith's work represents the culmination of decades of traditional boatbuilding. This tradition, along with environmental and economic constraints, helped to shape Smith's hulls.

Merwin, Daria Elizabeth

2000-01-01T23:59:59.000Z

31

Microsoft Word - EMSSABChairs conferencecall Sept19.FINAL  

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

September 19, 2011 September 19, 2011 Participants Board Chairs/Representatives Site Support Staff Hanford Susan Leckband Idaho Nicki Karst Nevada Kathleen Bienenstein, Walt Wegst Kelly Snyder, Denise Rupp Northern New Mexico Ralph Phelps, Robert Gallegos Menice Santistevan Oak Ridge Maggie Owen, Ron Murphree Melyssa Noe, Pat Halsey, Pete Osborne, Spencer Gross Paducah Ralph Young Buz Smith, Eric Roberts, Lauren DeFazio Portsmouth Dick Snyder Julie Galloway Savannah River Don Bridges Erica Williams DOE-HQ Representatives EM-42 Catherine Alexander, Melissa Nielson, Elizabeth Schmitt EM-43 Christine Gelles EM-60 Joann Luczak EMAB Dennis Ferrigno Opening Remarks Ms. Catherine Alexander, Designated Federal Officer for the Environmental Management Site-

32

Microsoft PowerPoint - Smith.ppt  

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

Color Commentary for Color Commentary for WestConnect Paths Color Commentary for WestConnect Paths U.S. DOE 2009 Congestion Study Spring 2009 Technical Workshop Bob Smith Director Asset Management and Planning Arizona Public Service Company March 25, 2009 03/25/09 2 Four Corners West (Path 22) Owner: APS (SCE has all rights on FC-MK 500kV line through long term lease) TTC= 2325 MW Primary Use: Delivery of Four Corners generation and resources and New Mexico wind generation Four Corners Generation APS - 792.5 MW SCE - 744 MW PNM - 201.5 MW SRP - 155 MW EPE - 108.5 MW TEP - 108.5 MW TOTAL = 2110 MW 03/25/09 3 TOT 2A Owners: WAPA, PSCO, Tri-State TTC= 690 MW Primary Use: Delivery of CRSP hydro, Springerville generation and merchant activity 03/25/09 4 Southern New Mexico (Path 47) Owners: EPE, PNM, TRI TTC= 940 MW

33

Lauren Smith | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Lauren Smith Lauren Smith 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 Staff Lauren Smith Print Text Size: A A A RSS Feeds FeedbackShare Page Program Support Specialist Office of the Deputy Director for Science Programs SC-2/Germantown Building, Room H-208

34

Adam Smith and the Making of the Modern World  

E-Print Network (OSTI)

Preface 1. Adam Smiths Life and Work 2. Growth and Stasis 3. Of Wealth and Liberty 4. From Predation to Production Bibliography 3 ACKNOWLEDGEMENTS As with all books, this is a composite work and I would like to thank some... be potentially interested in one or two of the authors treated, but not all of them at once. So I have decided to re-issue each part as a downloadable electronic book, and add others parts of my exploration of the riddle of modernity in due course...

Macfarlane, Alan

2013-01-01T23:59:59.000Z

35

VEE-0085 - In the Matter of Smith Brothers Gas Company | Department of  

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

VEE-0085 - In the Matter of Smith Brothers Gas Company VEE-0085 - In the Matter of Smith Brothers Gas Company VEE-0085 - In the Matter of Smith Brothers Gas Company On April 18, 2002, Smith Brothers Gas Company (Smith) filed an Application for Exception with the Office of Hearings and Appeals (OHA) of the Department of Energy (DOE). Smith requests that it be relieved of the requirement to prepare and file the Energy Information Administration (EIA) form entitled "Resellers'/Retailers' Monthly Petroleum Product Sales Report," Form EIA-782B. As explained below, we have concluded that Smith has demonstrated that it is eligible for temporary exception relief. vee0085.pdf More Documents & Publications VEE-0081 - In the Matter of North Side Coal & Oil Co., Inc. VEE-0061 - In the Matter of Paul Smith Oil Company

36

VWA-0041 - In the Matter of Lucy B. Smith | Department of Energy  

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

41 - In the Matter of Lucy B. Smith 41 - In the Matter of Lucy B. Smith VWA-0041 - In the Matter of Lucy B. Smith This Decision involves a whistleblower complaint filed by Lucy B. Smith (Smith) under the Department of Energy's (DOE) Contractor Employee Protection Program. From September 1973 to March 1997, Smith was employed as a chemist at the DOE's Savannah River Site (SRS) by various contractors, the most recent of which was Westinghouse Savannah River Company (WSRC). At the time of her termination, Smith worked at WSRC's Waste Management Laboratory. Smith alleges that in retaliation for making a number of health and safety disclosures WSRC terminated her pursuant to a January 1997 Reduction-in-Force (1/97 Rif) and subsequently failed to rehire her. vwa0041.pdf More Documents & Publications

37

VEE-0061 - In the Matter of Paul Smith Oil Company | Department of Energy  

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

61 - In the Matter of Paul Smith Oil Company 61 - In the Matter of Paul Smith Oil Company VEE-0061 - In the Matter of Paul Smith Oil Company On May 24, 1999, Paul Smith Oil Company (Smith) filed an Application for Exception with the Office of Hearings and Appeals of the Department of Energy. In its Application, Smith asks that it be relieved of the requirement that it file the Energy Information Administration's (EIA) form entitled "Resellers'/Retailers' Monthly Petroleum Product Sales Report" (Form EIA-782B). As explained below, we have determined that the Application for Exception should be denied. vee0061.pdf More Documents & Publications VEE-0085 - In the Matter of Smith Brothers Gas Company VEE-0037 - In the Matter of W. Gordon Smith Company VEE-0060 - In the Matter of Blakeman Propane

38

James M. Coughlan Smith-Kettlewell Eye Research Institute  

E-Print Network (OSTI)

of the Problem 3-D lines in Manhattan scene project to lines on uv image plane. cr ar fu rr rr = cr br fv rr rrJames M. Coughlan Smith-Kettlewell Eye Research Institute Manhattan World: Orientation and Outlier Detection by Bayesian Inference #12;Application of the statistics of edges: Manhattan World Many scenes

Coughlan, James M.

39

DIFFERENTIAL OPERATORS ON AN AFFINE CURVE S. P. SMITH and J. T. STAFFORD  

E-Print Network (OSTI)

DIFFERENTIAL OPERATORS ON AN AFFINE CURVE S. P. SMITH and J. T. STAFFORD [Received 11 November 1986, 16A33. Proc. London Math. Soc. (3) 56 (1988) 229-259. #12;230 S. P. SMITH AND J. T. STAFFORD 0. #12;232 S. P. SMITH AND J. T. STAFFORD Given the above description of J, one may alternatively define

Smith, S. Paul

40

Clean Cities: Dennis A. Smith, P.E., C.E.M.  

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

Dennis A. Smith, P.E., C.E.M. to someone by E-mail Share Clean Cities: Dennis A. Smith, P.E., C.E.M. on Facebook Tweet about Clean Cities: Dennis A. Smith, P.E., C.E.M. on Twitter...

Note: This page contains sample records for the topic "young buz smith" 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

VEE-0085 - In the Matter of Smith Brothers Gas Company | Department of  

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

5 - In the Matter of Smith Brothers Gas Company 5 - In the Matter of Smith Brothers Gas Company VEE-0085 - In the Matter of Smith Brothers Gas Company On April 18, 2002, Smith Brothers Gas Company (Smith) filed an Application for Exception with the Office of Hearings and Appeals (OHA) of the Department of Energy (DOE). Smith requests that it be relieved of the requirement to prepare and file the Energy Information Administration (EIA) form entitled "Resellers'/Retailers' Monthly Petroleum Product Sales Report," Form EIA-782B. As explained below, we have concluded that Smith has demonstrated that it is eligible for temporary exception relief. vee0085.pdf More Documents & Publications VEE-0081 - In the Matter of North Side Coal & Oil Co., Inc. VEE-0082 - In the Matter of Fleischli Oil Company

42

Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Smith Dairy Deploys Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest to someone by E-mail Share Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest on Facebook Tweet about Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest on Twitter Bookmark Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest on Google Bookmark Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest on Delicious Rank Alternative Fuels Data Center: Smith Dairy Deploys Natural Gas Vehicles and Fueling Infrastructure in the Midwest on Digg

43

Chris Smith Deputy Assistant Secretary for Oil and Natural Gas  

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

Chris Smith Chris Smith Deputy Assistant Secretary for Oil and Natural Gas Office of Fossil Energy U.S. Department of Energy Before the Subcommittee on Energy and Power Committee on Energy and Commerce U.S. House of Representatives March 28, 2012 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 price of gasoline places on U.S. families and businesses. For decades, volatile energy prices have threatened economic security for millions of American households. That volatility has hit consumers hard

44

CNMS_UEC_19_Sep_2011_Smith.pptx  

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

Annual Annual Meeting of the CNMS User Executive Committee September 1 9, 2 011 a t 1 2:15P, ORNL Bldg 8600, Room C--152 UEC Members Attending: Mark Dadmun (Chair), Martyn McLachlan, Nina Balke, David Bucknall, Vivek Prabhu, Colin Wolden, Marco Nardelli, Michael Hickner, Tony Hmelo CNMS r epresentatives: Peter Cummings, Laura Edwards, Tony Haynes, Sean Smith Meeting C onvened 1 2:15P CNMS Update Provided by Sean Smith (slides attached) Discussion P oints * It was noticed that the total number of user publications for the current year through 9/9/11 appear to be down. Haynes explained that this is an artifact of the data collection cycle and that the year was not complete. * The number of active user projects appears to be leveling off at ~250 per year. CNMS

45

Energy System Integration(Smith 2001) | OpenEI Community  

Open Energy Info (EERE)

Energy System Integration(Smith 2001) Energy System Integration(Smith 2001) Home > Groups > Energy Systems Integration Qinsun's picture Submitted by Qinsun(35) Member 15 November, 2012 - 13:09 Literature Review This paper proposed the business analysis on energy system integration. It provided a procedure for the business analysis, and listed related techniques and technologies. It can be view as a first approach of business analysis on ESI The method used in the paper is Process Optimization Audit and One-Line Balance The paper financially analyzed ESI It did not provide clear definition No result is provided. Groups: Energy Systems Integration Login to post comments Latest documents Qinsun Research topics related to ESI Posted: 15 Nov 2012 - 13:55 by Qinsun Qinsun Prospects for Nuclear Power(Davis 2012)

46

Ms. Julie Smith Office of Electricity Delivery and Energy Reliability  

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

5, 2013 5, 2013 Ms. Julie Smith Office of Electricity Delivery and Energy Reliability Mail Code OE-20 U.S. Department of Energy 1000 Independence Avenue Washington, D.C. 20585 Juliea.smith@hq.doe.gov; Christopher.lawrence@hq.doe.gov Re: DOE RFI "Improving Performance of Federal Permitting and Review of Infrastructure Projects The American people support increased production and consumption of renewable energy according to credible public opinion polls. Too often the most appropriate sites for wind, solar, hydro, and other renewable generators are in rural areas that necessitate the construction of new high voltage transmission lines to deliver the energy to customer load centers. Siting such lines is a costly multi-year

47

Building Energy Audit Report for Camp Smith, HI  

Science Conference Proceedings (OSTI)

A detailed energy assessment was performed by a team of engineers from Pacific Northwest National Laboratory (PNNL) under contract to the Department of Energy/Federal Energy Management program (FEMP). The effort used the Facility Energy Decision System (FEDS) model to determine how energy is consumed at Camp Smith, identify the most cost-effective energy retrofit measures, and calculate the potential energy and cost savings. This report documents the results of that assessment.

Chvala, William D.; De La Rosa, Marcus I.; Brown, Daryl R.; Dixon, Douglas R.

2010-09-30T23:59:59.000Z

48

Smith Newton Vehicle Performance Evaluation - 3rd Quarter 2012 (Brochure)  

SciTech Connect

The Fleet Test and Evaluation Team at the U.S. Department of Energy's National Renewable Energy Laboratory is evaluating and documenting the performance of electric and plug-in hybrid electric drive systems in medium-duty trucks across the nation. Through this project, Smith Electric Vehicles will build and deploy 500 all-electric medium-duty trucks. The trucks will be deployed in diverse climates across the country.

Not Available

2013-03-01T23:59:59.000Z

49

Smith Creek Valley Geothermal Area | Open Energy Information  

Open Energy Info (EERE)

Smith Creek Valley Geothermal Area Smith Creek Valley Geothermal Area Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermal Resource Area: Smith Creek Valley 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":39.3128,"lon":-117.5493,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

50

Microsoft Word - EMSSABChairs.conferencecall.Jan21.FINAL  

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

January 21, 2010 January 21, 2010 Participants Chairs/Representatives: Idaho R.D. Maynard, John Bolliger, Bob Pence, Lisa Aldrich, Ceri Chapple Nevada Walt Wegst, Kelly Snyder, Denise Rupp NNM Ralph Phelps, Menice Santistevan Oak Ridge Ron Murphree, Kevin Westervelt, Pat Halsey, Spencer Gross, Pete Osborne Paducah Ralph Young, Buz Smith, Eric Roberts Portsmouth Richard Snyder, Larry Parker, Greg Simonton Richland/Hanford Susan Leckband, Bob Suyama, Shelley Cimon Savannah River Manuel Bettencourt, Donald Bridges, Sheron Smith, Erica Williams DOE representatives: EM-3.1 Cynthia Anderson, Thomas Johnson, John Mocknick EM-5 Shari Davenport EM-42 Melissa Nielson, Cate Brennan, Michelle Hudson, Allison Clark EM-43 Doug Tonkay EM-62 Ethan Merrill Congressional Update

51

VBA-0055 - In the Matter of Lucy Smith | Department of Energy  

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

VBA-0055 - In the Matter of Lucy Smith VBA-0055 - In the Matter of Lucy Smith VBA-0055 - In the Matter of Lucy Smith This Decision considers an Appeal of an Initial Agency Decision (IAD) issued on July 11, 2000, involving a Complaint filed by Lucy Smith (Smith or the Complainant) under the Department of Energy (DOE) Contractor Employee Protection Program, 10 C.F.R. Part 708. In her Complaint, Smith claims that her former employer, Westinghouse Savannah River Company (WSRC), a DOE contractor, terminated her employment during a reduction in force (RIF), and then failed to rehire her, in retaliation for making disclosures that are protected under Part 708. In the IAD, however, the Hearing Officer determined that WSRC had shown that it would have terminated the Complainant in the RIF, even in the absence of the protected

52

VEE-0037 - In the Matter of W. Gordon Smith Company | Department of Energy  

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

37 - In the Matter of W. Gordon Smith Company 37 - In the Matter of W. Gordon Smith Company VEE-0037 - In the Matter of W. Gordon Smith Company On December 24, 1996, the W. Gordon Smith Company (Smith), filed an Application for Exception with the Office of Hearings and Appeals (OHA) of the Department of Energy (DOE). In its Application, Smith requests that it be temporarily relieved of the requirement that it file the Energy Information Administration's (EIA) form entitled "Resellers'/Retailers' Monthly Petroleum Product Sales Report" (Form EIA-782B). As explained below, we have determined that the Application for Exception should be granted. vee0037.pdf More Documents & Publications VEE-0039 - In the Matter of Froman Oil Company VEE-0032 - In the Matter of Thomas Oil Company VEE-0017 - In the Matter of Visa Petroleum, Inc.

53

Modifications to Smith's Method for Deriving Normalised Relations from a Functional Dependency Diagram  

E-Print Network (OSTI)

Smith's method (Smith, 1985) is a formal technique for deriving a set of normalised relations from a functional dependency diagram (FDD). Smith's original rules for deriving these relations are incomplete, as they do not fully address the issue of determining the foreign key links between relations. In addition, one of the rules for deriving foreign keys can produce incorrect results, while the other rule is difficult to automate. In this paper are described solutions these issues.

Nigel Stanger

1999-01-01T23:59:59.000Z

54

Connie V. Smith General Attorney DOE-RL Office of Chief Counsel...  

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

damages, tribal relationships and cultural resource issues. She has dabbled in appropriations law because it seems to answer so many questions. Before joining DOE, Ms. Smith...

55

A.O. Smith Corporation Response to Preliminary Plan for Retrospective...  

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

Plan for Retrospective Analysis of A.O. Smith Corporation is the largest manufacturer of residential and commercial water heating equipment in the United States. We have the...

56

YOUNG RESEARCHER SYMPOSIUM  

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

2 BROOKHAVEN NATIONAL LABORATORY CALL FOR PAPERS YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG...

57

YOUNG RESEARCHER SYMPOSIUM  

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

3 BROOKHAVEN NATIONAL LABORATORY CALL FOR PAPERS YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG RESEARCHER SYMPOSIUM 2012 BROOKHAVEN NATIONAL LABORATORY YOUNG...

58

VBH-0025 - In the Matter of Alizabeth Aramowicz Smith | Department of  

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

5 - In the Matter of Alizabeth Aramowicz Smith 5 - In the Matter of Alizabeth Aramowicz Smith VBH-0025 - In the Matter of Alizabeth Aramowicz Smith This Initial Agency Decision concerns a whistleblower complaint filed by Alizabeth Aramowicz Smith, a former contractor employee at the Oak Ridge National Laboratory. As explained below, Smith's complaint should be denied. This case arises under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708, the "whistleblower" regulations. The whistleblower regulations prohibit a contractor from retaliating against a contractor employee who engages in protected conduct. Protected conduct includes disclosing information that the employee believes reveals 1) a substantial violation of a law, rule, or regulation; 2) a substantial and specific danger to employees or to public health or

59

First Measurements of the Longitudinal Bunch Profile at SLAC Using Coherent Smith-Purcell Radiation at 28GeV  

E-Print Network (OSTI)

First Measurements of the Longitudinal Bunch Profile at SLAC Using Coherent Smith-Purcell Radiation at 28GeV

Blackmore, V; Doucas, G; Kimmitt, M F; Molloy, S; Ottewell, B; Perry, C; Woods, M

2008-01-01T23:59:59.000Z

60

Deaf Smith Electric Coop, Inc | Open Energy Information  

Open Energy Info (EERE)

Electric Coop, Inc Electric Coop, Inc Jump to: navigation, search Name Deaf Smith Electric Coop, Inc Place Texas Utility Id 4939 Utility Location Yes Ownership C NERC Location SPP NERC SPP Yes Activity Transmission Yes Activity Distribution Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Farm & Home - Rate 01 Residential Industrial- Rate 08 Industrial Irrigation- Rate 03 Commercial Large Power- Rate 07 Commercial Lighting 100 HP sodium Lighting Lighting 1000 HP sodium Lighting Lighting 1000 MV Lighting Lighting 175 MV Lighting Lighting 250 HP sodium Lighting Lighting 400 HP sodium Lighting

Note: This page contains sample records for the topic "young buz smith" 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

LS-ll D. Y. Smith and A. E. Williamsont  

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

ll ll D. Y. Smith and A. E. Williamsont December 15, 1984 Optical Properties at X-ray Energies of Reflecting Elements for Synchrotron Radiation Sources* Summary Preliminary results are reported for the optical constants at x-ray wavelengths of elements commonly used for x-ray mirrors and multilayer reflectors. The data were derived from measured absorption spectra using a dispersion theory-sum rule analysis. Introduction The optical properties of materials in the x-ray range are of increasing interest in conjunction with the development of instrumentation for synchrotron radiation sources,l particularly for the design of mirrors 2 and mutlilayer 3 reflectors and filters. This letter is a preliminary report of a method for calculating these properties from presently available absorption

62

Smith School of Enterprise and the Environment | Open Energy Information  

Open Energy Info (EERE)

School of Enterprise and the Environment School of Enterprise and the Environment Jump to: navigation, search Name Smith School of Enterprise and the Environment Place Oxford, England, United Kingdom Product String representation "Oxford-based mu ... tal challenges." is too long. Coordinates 43.781517°, -89.571699° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":43.781517,"lon":-89.571699,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

63

09-03-10_Smith_Dawson_Andrews.pdf  

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

information on this form will be available to the public on the Executive Branch agency's recovery website. information on this form will be available to the public on the Executive Branch agency's recovery website. Written materials prepared by registered lobbyists should be attached to this form for posting o the website. To be completed by the employee contacted. Date and time of contact: Name of the Employee(s) Contacted (Name and Title) Brief description of the contact: (attach separate sheet if necessary) 09/3/2010 11:35 am EDT Mary C. Cronin Senior Legislative Associate Smith Dawson & Andrews Mary inquired about which program best matches her client's needs and how much money remains in the ATVM program.

64

Static Temperature Survey At U.S. South Region (Smith & Dees, 1982) | Open  

Open Energy Info (EERE)

Static Temperature Survey At U.S. South Region (Smith & Dees, 1982) Static Temperature Survey At U.S. South Region (Smith & Dees, 1982) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Static Temperature Survey At U.S. South Region (Smith & Dees, 1982) Exploration Activity Details Location U.S. South Region Exploration Technique Static Temperature Survey Activity Date Usefulness useful DOE-funding Unknown Notes (Louisiana & Mississippi): "cased, non-flowing boreholes at least 150 m deep were sought on an opportunistic basis through state geological surveys and U.S. Geological Survey offices. Representative samples of drill cuttings were used for laboratory measurements of thermal conductivity. A total of 38 new heat flow values, ranging from less than 1 heat flow unit (hfu) (41.8 mW/m 2) to more than 2 hfu, were determined (Smith and Dees, in

65

2010 DOE National Science Bowl® Photos - Smith Middle School | U.S. DOE  

Office of Science (SC) Website

Smith Middle School Smith Middle School National Science Bowl® (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past National Science Bowl Winners Past National Science Bowl Photos National Science Bowl Logos High School Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov 2010 National Science Bowl Photos 2010 DOE National Science Bowl® Photos - Smith Middle School Print Text Size: A A A RSS Feeds FeedbackShare Page Smith Middle School team members from Glastonbury, CT visit a variety of

66

Testimony of Christopher Smith before the House Committee on Energy and  

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

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

67

Isotopic Analysis- Rock At Long Valley Caldera Area (Smith & Suemnicht,  

Open Energy Info (EERE)

Isotopic Analysis- Rock At Long Valley Caldera Area (Smith & Suemnicht, Isotopic Analysis- Rock At Long Valley Caldera Area (Smith & Suemnicht, 1991) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Isotopic Analysis- Rock At Long Valley Caldera Area (Smith & Suemnicht, 1991) Exploration Activity Details Location Long Valley Caldera Area Exploration Technique Isotopic Analysis- Rock Activity Date Usefulness useful DOE-funding Unknown Notes This oxygen isotope and fluid inclusion study has allowed us to determine the pathways of fluid circulation, set limits on the thermal regime, and link the source of the heat to prolonged volcanic activity. At shallow depths in the caldera References Brian M. Smith, Gene A. Suemnicht (1991) Oxygen Isotope Evidence For Past And Present Hydrothermal Regimes Of Long Valley Caldera, California

68

Review: The Hanford Reach: A Land of Contrasts by Susan Zwinger and Stamford D. Smith  

E-Print Network (OSTI)

Review: The Hanford Reach: A Land of Contrasts By SusanSmith (Photographer).The Hanford Reach: A Land of Contrasts.addition. Simply put, The Hanford Reach: A Land of Contrasts

Sowards, Adam M.

2007-01-01T23:59:59.000Z

69

STATEMENT OF CONSIDERATIONS REQUEST BY A O. SMITH CORPORATION FOR AN ADVANCE WAIVER OF  

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

A O. SMITH CORPORATION FOR AN ADVANCE WAIVER OF A O. SMITH CORPORATION FOR AN ADVANCE WAIVER OF PATENT RIGHTS TO INV~NTIONS MADE UNDER SUBCONTRACT QZ001 UNDER COOPERATIVE AGREEMENT DE-EE0003985; W(A)-2010-066; CH-1588 A 0 Smith Corporation (Smith) requests an advance waiver of domestic and foreign patent rights for all subject inventions made under its subcontract under the referenced cooperative agreement between The Department of Energy and Stone Mountain Technologies entitled, "Development and Validation of a Gas Fired Residential Heat Pump Water Heater". The purpose of the cooperative agreement is to develop a gas- fired residential heat pump water heater (GHPWH) with a primary fuel efficiency 2.4 times higher than conventional gas storage water heaters, and 2.1 times higher than

70

Measuring short electron bunch lengths using coherent smith-purcell radiation  

DOE Patents (OSTI)

A method is provided for directly determining the length of sub-picosecond electron bunches. A metallic grating is formed with a groove spacing greater than a length expected for the electron bunches. The electron bunches are passed over the metallic grating to generate coherent and incoherent Smith-Purcell radiation. The angular distribution of the coherent Smith-Purcell radiation is then mapped to directly deduce the length of the electron bunches.

Nguyen, Dinh C. (Los Alamos, NM)

1999-01-01T23:59:59.000Z

71

Measuring short electron bunch lengths using coherent Smith-Purcell radiation  

DOE Patents (OSTI)

A method is provided for directly determining the length of sub-picosecond electron bunches. A metallic grating is formed with a groove spacing greater than a length expected for the electron bunches. The electron bunches are passed over the metallic grating to generate coherent and incoherent Smith-Purcell radiation. The angular distribution of the coherent Smith-Purcell radiation is then mapped to directly deduce the length of the electron bunches. 8 figs.

Nguyen, D.C.

1999-03-30T23:59:59.000Z

72

Smith River Rancheria's Development of an Energy Organization Investigation  

SciTech Connect

Smith River Rancheria (SRR), for some time, has had a strong commitment to attaining energy selfsufficiency, to reduce overall energy costs and concurrently initiate economic development within the community. Early on it was recognized that the development of an energy organization was important and for this reason was made part of the SRR's strategic review not only for economic development but also the reduction of energy costs. Towards this end, SRR retained Werner G. Buehler of W.G. Buehler & Associates to investigate the many phases or steps required to establish such an energy organization and determine, if in fact, it could benefit the Tribe. The basic phases are delineated as: (1) Identify potential sources of wholesale power and transmission paths; (2) Evaluating the various forms of energy organizations; (3) Determining the benefits (and disadvantages) of each form of organization; (4) Gathering costs to organize and operate the selected form or energy organization; (5) Performing an economic analysis of forming and operating an energy organization; and (6) Develop an implementation plan.

W.G Buehler & Associates

2007-08-27T23:59:59.000Z

73

Young Leaders Professional Development Award  

Science Conference Proceedings (OSTI)

YOUNG PROFESSIONAL LINKS. YOUNG PROFESSIONALS HOME [MORE]; YL INTERNATIONAL SCHOLAR AWARD Learn about the international scholar...

74

EM SSAB CHAIRS  

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

June 6, 2012 June 6, 2012 Participants Board Chairs/Representatives Site Support Staff Hanford Susan Leckband, Shelley Cimon Sharon Braswell, Dana Bryson, Tifany Nguyen Idaho Willie Preacher Nevada Kathleen Bienenstein Kelly Snyder, Denise Rupp Northern New Mexico Ralph Phelps, Carlos Valdez Ed Worth, Menice Santistevan, Oak Ridge Maggie Owen Spencer Gross Paducah Ralph Young, Buz Smith Eric Roberts Portsmouth Julie Galloway, Rick Greene Savannah River Don Bridges Bill Taylor, Terry Spears DOE-HQ Representatives EM-3.2 Catherine Alexander, Melissa Nielson, Michelle Hudson, Elizabeth Schmitt, Elizabeth Maksymonko EM-60 Connie Flohr Opening Remarks Ms. Catherine Alexander, Designated Federal Officer for the Environmental Management Site- Specific Advisory Board (EM SSAB), called the meeting to order.

75

EM SSAB CHAIRS Bi-Monthly Conference Call  

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

February 19, 2013 February 19, 2013 Participants Board Chairs/Representatives Site Staff Hanford Susan Leckband Kim Ballinger, Sharon Braswell Idaho Peggy Hinman Nevada Kathleen Bienenstein, Donna Hruska Kelly Snyder, Barb Ulmer Northern New Mexico Carlos Valdez Menice Santistevan Oak Ridge David Martin, David Hemelright Melyssa Noe, Spencer Gross, Pete Osborne Paducah Ralph Young Buz Smith, Eric Roberts Portsmouth Greg Simonton, Julie Galloway, Rick Greene, Savannah River Donald Bridges, Harold Simon Ashley Whitaker DOE-HQ Representatives EM-3.2 Catherine Alexander, Melissa Nielson, Michelle Hudson, Elizabeth Schmitt, Alexandra Gilliland, Sayoh Mansaray EM-31 Doug Tonkay EM-32 Mark Senderling EM-60 Terry Tyborowski Opening Remarks Ms. Catherine Alexander, Designated Federal Officer for the Environmental Management Site-

76

Microsoft Word - EMSSABChairs.conferencecall.May19.FINAL  

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

May 19, 2010 May 19, 2010 Participants Chairs/Representatives: Idaho Willie Preacher, Ceri Chapple Nevada Harold Sullivan, Kelly Snyder, Denise Rupp NNM Ralph Phelps, Lee Bishop, Menice Santistevan Oak Ridge Ron Murphree, Kevin Westervelt, Pete Osborne Paducah Judy Clayton, Ralph Young, Buz Smith, Eric Roberts Portsmouth Dick Snyder, Julie Galloway Richland/Hanford Susan Leckband, Lori Gamache Savannah River Manuel Bettencourt, Gerri Flemming DOE representatives: EM-3.1 John Mocknick, Colin Jones EM-42 Melissa Nielson, Cate Brennan, Michelle Hudson EM-62 Mark Janaskie Opening Remarks Ms. Cate Brennan, the Designated Federal Officer for the Environmental Management Site- Specific Advisory Board (EM SSAB), called the meeting to order. EM Budget and Strategic Planning Follow-Up

77

Barry F. Smith, 2011 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Barry F. Smith, 2011 Barry F. Smith, 2011 The Ernest Orlando Lawrence Award Lawrence Award Home Nomination & Selection Guidelines Award Laureates 2000's 1990's 1980's 1970's 1960's Ceremony The Life of Ernest Orlando Lawrence Contact Information The Ernest Orlando Lawrence Award U.S. Department of Energy SC-2/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-9395 E: lawrence.award@science.doe.gov 2000's Barry F. Smith, 2011 Print Text Size: A A A RSS Feeds FeedbackShare Page Computer, Information, and Knowledge Sciences: For scientific leadership in advancing the innovative and transformative numerical software package PETSc, which provides robust, efficient, scalable, and extensible tools that are the backbone of numerous high-performance DOE simulation computer

78

REQUEST BY SMITH INTERNATIONAL, INC. FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN RIGHTS  

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

SMITH INTERNATIONAL, INC. FOR AN SMITH INTERNATIONAL, INC. FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN RIGHTS IN SUBJECT INVENTIONS MADE IN THE COURSE OF OR UNDER DEPARTMENT OF ENERGY CONTRACT NO. DE- AC21-92MC28182, PHASE II; DOE WAIVER DOCKET W(A)- 96-019 [ORO-635] Smith International, Inc. has made a timely request for an advance waiver of worldwide rights in Subject Inventions made in the course of or under Phase II of Department of Energy (DOE) Contract No. DE-AC21-92MC28182. The scope of the work calls for the development, testing and tool hardening of a slim hole percussion air directional drilling system to be used with both conventional drill pipe and coiled tubing. The work is sponsored by the Office of Fossil Energy. The total value (including in-kind contributions) of Phase II of the contract is $1,926,862,

79

Field Mapping At Dixie Valley Geothermal Field Area (Smith, Et Al., 2001) |  

Open Energy Info (EERE)

Et Al., 2001) Et Al., 2001) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Field Mapping At Dixie Valley Geothermal Field Area (Smith, Et Al., 2001) Exploration Activity Details Location Dixie Valley Geothermal Field Area Exploration Technique Field Mapping Activity Date Usefulness not indicated DOE-funding Unknown References Richard P. Smith, Kenneth W. Wisianz, David D. BlackweIl (2001) Geologic And Geophysical Evidence For Intra-Basin And Footwall Faulting At Dixie Valley, Nevada Retrieved from "http://en.openei.org/w/index.php?title=Field_Mapping_At_Dixie_Valley_Geothermal_Field_Area_(Smith,_Et_Al.,_2001)&oldid=510735" Category: Exploration Activities What links here Related changes Special pages Printable version Permanent link

80

Young Researcher Symposium 2013  

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

Brookhaven National Laboratory Young Researcher Symposium 2013 Homepage Registration Talks Program Abstract Submission Sponsors Feedback Contact Us Symposium Information pulldown...

Note: This page contains sample records for the topic "young buz smith" 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

High performance computing and the simplex method Julian Hall, Qi Huangfu and Edmund Smith  

E-Print Network (OSTI)

High performance computing and the simplex method Julian Hall, Qi Huangfu and Edmund Smith School of Mathematics University of Edinburgh 12th April 2011 High performance computing and the simplex method #12;The... ... but methods for all three depend on it! High performance computing and the simplex method 1 #12;Overview · LP

Hall, Julian

82

UTILIZING GOOGLE EARTH AS A GIS PLATFORM FOR WEATHER APPLICATIONS Travis M. Smith1,2  

E-Print Network (OSTI)

UTILIZING GOOGLE EARTH AS A GIS PLATFORM FOR WEATHER APPLICATIONS Travis M. Smith1,2 and Valliappa Lakshmanan1,2 1 U. of Oklahoma/CIMMS; 2 NOAA/NSSL 1. Introduction Google Earth (formerly known as Keyhole; http://earth.google.com) is a free-for- personal-use application that streams high- resolution static

Smith, Travis

83

Fertilizing and Burning Flint Hills Bluestem CLENTON E. OWENSBY AND ED F. SMITH  

E-Print Network (OSTI)

Fertilizing and Burning Flint Hills Bluestem CLENTON E. OWENSBY AND ED F. SMITH Abstract Burned of nitrogen applied more than 80 lb N/acre did. Maintenance of good quality range was favored by burning and 0 and 40 lb N/acre compared to not burning and the same fertilizer rates. Eighty lb N/acre produced poor

Owensby, Clenton E.

84

Francis H. Smith: architect of antebellum southern military schools and educational reform  

E-Print Network (OSTI)

This study examines the historical significance of the Virginia Military Instituteâ??s (VMI) first superintendent, Francis Henney Smith, and his influence not only at his home institution but also on his broader social, educational, and political importance. Historiography neglects to credit or identify Smithâ??s contributions to the notable expansion of military education in the antebellum South and his influence beyond VMI. Not only did he play a key role in the developing of Southern military education, but overwhelming evidence indicates that the growth of these schools in the South would not have happened without Smith acting as an influential father figure. He provided the structure, ideology and pedagogical models of these institutions and advised, guided and inspired nearly every other Southern military school in the two decades preceding the Civil War. Moreover, his innovations spread far beyond those of military schools as he promoted a new vision for Virginia and the South, one in which independence could be established through intellectual solidarity by creating a society centered on education. As a West Point graduate, Smith structured VMI on the Sylvanus Thayer educational model and sought to promote this system throughout every school in Virginia and the South, both in military and non-military institutions. He also created a network of like-minded academics, mostly with alumni from the U.S. Military Academy who launched a movement to encourage a more practical education in the South, focusing on mathematics, engineering and the sciences. VMI graduates would also spread Smithâ??s academic gospel throughout the state and region as he encouraged them to serve their republic as teachers rather than soldiers. In spite of the popularity of his reforms and ideologies, Smith contended with the challenges of the volatile nature of antebellum Virginia politics as well as the social constructs of his native South, particularly in the forms of honor and masculinity demonstrated by his cadets. The outbreak of the Civil War in 1861 temporarily destroyed his dreams improving VMI on the model of the most advanced scientific institutions in Europe as the Institute converted to an exclusively military mission to serve the Confederacy.

Wineman, Bradford Alexander

2006-08-01T23:59:59.000Z

85

Young Scientist Research Award  

Science Conference Proceedings (OSTI)

Recognizing substantial research contributions by someone 36 years of age or younger. Young Scientist Research Award Divisions achievement agricultural analytical application award awards biotechnology detergents distinguished division Divisions

86

Comment submitted by A. O. Smith Corporation regarding the Energy Star Verification Testing Program  

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

From: Adams, Charlie From: Adams, Charlie Sent: Friday, May 06, 2011 03:38 PM To: Adams, Charlie Cc: Dana, Paul; Parker, Mike; Porter, Jerry; Schulz, Matt; Schuh, Darrell; Roy Smith; Ted Poulin; Berning, Dave; Dan Snyder Subject: Comments on ENERGY STAR verification testing program Hi, Ashley. A.O. Smith has the following comments in regard to DOE's ENERGY STAR® verification test program: * DOE and EPA appear to be working to pool the units tested under each program so that there is no double testing of units, and that all units tested count towards the total required for test during the specified period. This is great, and we appreciate their efforts. * In the selection for testing, we agree that new technologies and units that are above the Energy Star level of performance are of interest, but the majority of testing should be

87

Core Analysis At Long Valley Caldera Area (Smith & Suemnicht, 1991) | Open  

Open Energy Info (EERE)

Long Valley Caldera Area (Smith & Long Valley Caldera Area (Smith & Suemnicht, 1991) Exploration Activity Details Location Long Valley Caldera Area Exploration Technique Core Analysis Activity Date Usefulness useful DOE-funding Unknown Notes Sample for the present investigation consist of drill core and cuttings from all lithologic units identified in LVEW, cuttings from volcanic rocks in LV 13-21, core samples of Early Rhyolite and Bishop Tuff from LV13-26 and core samples of Bishop Tuff from SF38-32, LV48-29 and LV66-28 (Figs. 1 and 2). Surface samples of Early Rhyolite, Bishop Tuff and Paleozoic metasediments (Fig. 1) were also selected for comparative analysis and processed by the same procedures as the well samples. This oxygen isotope and fluid inclusion study has allowed us to determine the pathways of fluid

88

Cuttings Analysis At Long Valley Caldera Area (Smith & Suemnicht, 1991) |  

Open Energy Info (EERE)

Long Valley Caldera Area (Smith Long Valley Caldera Area (Smith & Suemnicht, 1991) Exploration Activity Details Location Long Valley Caldera Area Exploration Technique Cuttings Analysis Activity Date Usefulness useful DOE-funding Unknown Notes Sample for the present investigation consist of drill core and cuttings from all lithologic units identified in LVEW, cuttings from volcanic rocks in LV 13-21, core samples of Early Rhyolite and Bishop Tuff from LV13-26 and core samples of Bishop Tuff from SF38-32, LV48-29 and LV66-28 (Figs. 1 and 2). Surface samples of Early Rhyolite, Bishop Tuff and Paleozoic metasediments (Fig. 1) were also selected for comparative analysis and processed by the same procedures as the well samples. This oxygen isotope and fluid inclusion study has allowed us to determine the pathways of fluid

89

Mr. Christopher Lawrence and Ms. Julie Smith Office of Electricity Delivery and Energy Reliability  

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

Mr. Christopher Lawrence and Ms. Julie Smith Office of Electricity Delivery and Energy Reliability Mail Code: OE-20 U.S. Department of Energy 1000 Independence Avenue, SW Washington, D.C. 20585 Dear Mr. Lawrence and Ms. Smith, The Western Governors' Association (WGA) is submitting these comments in response to the Department of Energy's (DOE) Request for Information (RFI), dated August 29, 2013 1 . The RFI outlines a proposed process to establish a coordinated series of meetings and other actions for qualified transmission projects, via an Integrated, Interagency Pre-Application process (IIP). Western Governors appreciate efforts to streamline the siting and permitting process for transmission. Western Governors have a clear goal to site and permit transmission lines three years after a

90

Ms. Julie A. Smith Mr. Christopher Lawrence Office of Electricity Delivery and Energy Reliability  

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

October 30, 2013 October 30, 2013 Ms. Julie A. Smith Mr. Christopher Lawrence Office of Electricity Delivery and Energy Reliability Mail Code: OE-20 U.S. Department of Energy 1000 Independence Avenue, SW Washington, DC 20585 Dear Ms. Smith and Mr. Lawrence: The Association of Fish and Wildlife Agencies (AFWA) would like to provide comments on the Federal Register Notice Request for Information (RFI) on Improving Performance of Federal Permitting and Review of Infrastructure Projects, Federal Register Document 2013-21098. AFWA is the professional association that represents the collective voice of North America's state, provincial and territorial fish and wildlife agencies. The state fish and wildlife agencies (State agencies) have statutory authority

91

Cuttings Analysis At U.S. South Region (Smith & Dees, 1982) | Open Energy  

Open Energy Info (EERE)

& Dees, 1982) & Dees, 1982) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Activity: Cuttings Analysis At U.S. South Region (Smith & Dees, 1982) Exploration Activity Details Location U.S. South Region Exploration Technique Cuttings Analysis Activity Date Usefulness useful DOE-funding Unknown Notes (Louisiana & Mississippi): "cased, non-flowing boreholes at least 150 m deep were sought on an opportunistic basis through state geological surveys and U.S. Geological Survey offices. Representative samples of drill cuttings were used for laboratory measurements of thermal conductivity. A total of 38 new heat flow values, ranging from less than 1 heat flow unit (hfu) (41.8 mW/m 2) to more than 2 hfu, were determined (Smith and Dees, in

92

2013 Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM  

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

Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM 2013 BROOKHAVEN NATIONAL LABORATORY NOVEMBER 15, 2013 YRS LETTER FROM THE ORGANIZERS 2013 Dear Guest, Welcome...

93

Steve Young | Data.gov  

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

Steve Young Primary tabs View(active tab) Track Communities: Energy Display Name: Steve Young History Member for 1 year 1 week...

94

SSA Young Aspen Site  

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

Site (SSA-YA) The pole-tower at the YA site Closer look at the pole-tower at the YA site Solar panels powering the site, mounted on a folding ladder The young aspen canopy...

95

Jun-Young Choi  

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

Jun-Young Choi Korea Testing Laboratory NOTICE Due to the current lapse of federal funding, Berkeley Lab websites are accessible, but may not be updated until Congress approves...

96

Young Leaders Committee Bylaws  

Science Conference Proceedings (OSTI)

The vice chair is to be selected by the current chair/vice chair from Young Professionals who wish to serve in this capacity who have indicated a willingness to do...

97

Julie A. Smith and Christopher Lawrence Office of Electricity Delivery and Energy Reliability  

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

christopher.lawrence@hq.doe.gov christopher.lawrence@hq.doe.gov RE: Improving Performance of Federal Permitting and Review of Infrastructure Projects: Comments on a Draft Integrated, Interagency Pre-Application (IIP) Process Dear Ms. Smith and Mr. Lawrence: Please accept these comments on the draft Integrated, Interagency Pre-Application (IIP) Process on behalf of the Wyoming Infrastructure Authority (WIA), in response to your August 29, 2013, Request for Information (RFI) on "Improving Performance of Federal Permitting and Review of Infrastructure Projects." We are committed to state and federal cooperation to accelerate the statutory reviews, permits, and consultations

98

Christopher Smith  

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

Subcommittee on Energy and Power Subcommittee on Energy and Power Committee on Energy and Commerce United States House of Representatives The Department of Energy's Program Regulating Liquefied Natural Gas Export Applications June 18, 2013 Thank you Chairman Whitfield, Ranking Member Rush, and members of the Subcommittee; I appreciate the opportunity to be here today to discuss the Department of Energy's (DOE) program regulating the export of natural gas, including liquefied natural gas (LNG). Recent Developments in LNG Exports The boom in domestic shale gas provides unprecedented opportunities for the United States. Over the last several years, domestic natural gas production has increased significantly, outpacing consumption growth, resulting in declining natural gas and LNG imports. Production

99

Christopher Smith  

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

Oversight and Government Reform Committee Oversight and Government Reform Committee Subcommittee on Energy Policy, Health Care, and Entitlements United States House of Representatives The Department of Energy's Program Regulating Liquefied Natural Gas Export Applications March 19, 2013 Thank you Chairman Lankford, Ranking Member Speier, and members of the Committee; I appreciate the opportunity to be here today to discuss the Department of Energy's (DOE) program regulating the export of natural gas, including liquefied natural gas (LNG). Recent Developments in LNG Exports The boom in domestic shale gas provides unprecedented opportunities for the United States. Over the last several years, domestic natural gas production has increased significantly,

100

A REVISED METHOD FOR ESTIMATING OXIDE BASICITY PER THE SMITH SCALE WITH EXAMPLE APPLICATION TO GLASS DURABILITY  

SciTech Connect

Previous researchers have developed correlations between oxide electronegativity and oxide basicity. The present paper revises those correlations using a newer method of calculating electronegativity of the oxygen anion. Basicity is expressed using the Smith {alpha} parameter scale. A linear relation was found between the oxide electronegativity and the Smith {alpha} parameter, with an R{sup 2} of 0.92. An example application of this new correlation to the durability of high-level nuclear waste glass is demonstrated. The durability of waste glass was found to be directly proportional to the quantity and basicity of the oxides of tetrahedrally coordinated network forming ions.

REYNOLDS JG

2011-07-27T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

A Free Energy Model for Piezoceramic Materials Ralph C. Smith , Stefan Seelecke y and Zoubeida Ounaies z  

E-Print Network (OSTI)

A Free Energy Model for Piezoceramic Materials Ralph C. Smith #3; , Stefan Seelecke y and Zoubeida the development of a free energy model for quantifying the hysteresis and constitutive nonlinearities inherent to piezoceramic materials. In the #12;rst step of the development, free energy relations for a single crystal

102

Julie A. Smith and Christopher Lawrence Office of Electricity Delivery and Energy Reliability  

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

christopher.lawrence@hq.doe.gov christopher.lawrence@hq.doe.gov RE: Comments on a Draft Integrated, Interagency Pre-Application (IIP) Process Dear Ms. Smith and Mr. Lawrence: Please accept these Trout Unlimited (TU) comments on the draft Integrated, Interagency Pre-Application (IIP) Process. Trout Unlimited is concerned with expediting renewable development in a thoughtful and deliberate manner in order to protect and conserve fish and wildlife resources and sportsmen's interests. Trout Unlimited routinely participates in the Federal and state processes for environmental review of major energy projects and cooperates with State as well as Federal fish and wildlife and land management agencies. A well designed pre-application process could be instrumental in avoiding potential issues but Trout

103

Microsoft PowerPoint - 5_Pat Smith_NMMSS_2013_Presentation_NRC Reconciliation.pptx  

National Nuclear Security Administration (NNSA)

Reconciliation Reconciliation Pat Smith PSI NRC Lead NRC Reconciliation  NRC Reconciliation requirements per NUREG/BR-0007, Rev. 6  All RIS's must submit an MSR (Material Summary Report) (Form 742, 742C) to NMMSS under the following conditions: - A RIS has a reportable quantity as of their inventory date - A RIS has shipped or received a reportable quantity during the material balance reporting period NRC Reconciliation  All NRC licensees are required to report their physical inventory to NMMSS each year if they: - possess one gram or more of special nuclear material (SNM) (plutonium, uranium-233, or uranium-235 contained in enriched uranium) - one kilogram or more of foreign obligated source material (natural uranium, depleted uranium, or thorium) are required to report their physical inventory to NMMSS each

104

LS-ll1 J. A. Jendrzej czyk M. W. Wambsganss R. K. Smith  

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

ll1 ll1 J. A. Jendrzej czyk M. W. Wambsganss R. K. Smith March 1988 AMBIENT GROUND MOTION MEASUREMENTS AT ARGONNE NATIONAL LABORATORY OVER EXTENDED TIME PERIODS -1- BACKGROUND Successful operation of the APS facility requires a very stable particle beam. Vi brationcûupled thrûugh mechanical sy,stems, such as magnet suppûrts, beam tube supports, and other paths can cause deterioration of the particle beam. There are two sources of vibration: external, or far field, which is generated external to the APS site and internal, or near field, which is generated on site and associated with operation of the facility. Internal vibration sources can be controlled or minimized using good design practices to eliminate or reduce vibration amplitudes of machinery and equipment.

105

Electron Bunch Profile Reconstruction in the Few fs Regime using Coherent Smith-Purcell Radiation  

SciTech Connect

Advanced accelerators for fourth generation light sources based on high brightness linacs or laser-driven wakefield accelerators will operate with intense, highly relativistic electron bunches that are only a few fs long. Diagnostic techniques for the determination of temporal profile of such bunches are required to be non invasive, single shot, economic and with the required resolution in the fs regime. The use of a radiative process such as coherent Smith-Purcell radiation (SPR), is particularly promising with this respect. In this technique the beam is made to radiate a small amount of electromagnetic radiation and the temporal profile is reconstructed from the measured spectral distribution of the radiation. We summarise the advantages of SPR and present the design parameters and preliminary results of the experiments at the FACET facility at SLAC. We also discuss a new approach to the problem of the recovery of the 'missing phase', which is essential for the accurate reconstruction of the temporal bunch profile.

Bartolini, R.; /Oxford U., JAI /Diamond Light Source /SLAC; Clarke, C.; /SLAC; Delerue, N; /Oxford U., JAI /Diamond Light Source /SLAC; Doucas, G; Reichold, A; /Oxford U., JAI

2012-06-20T23:59:59.000Z

106

Final Report - Conservation & Renewable Energy Potential Study For Smith River Rancheria  

DOE Green Energy (OSTI)

In January 2006 the Smith River Rancheria (SRR), located in Smith River, California, contracted with the team of Strategic Energy Solutions (SES) and Evergreen NRG to conduct a study for the community. The objective of the study was to identify renewable generation opportunities that would facilitate Rancheria energy independence through SRR owned and operated power projects. These generation facilities were to be located either on or near the reservation. Specifically, the Rancheria was interested in the viability of generating electric power using biomass and wind fuel resources. Initial research identified that a very small portion of the community's energy could be offset by renewable energy generation due to the low solar resource in this area, and the lack of significant wind or biomass resources on or near reservation land. Some larger projects were identified which offered little or no benefit to the Rancheria. As a result, the scope of this study was changed in October 2006 to focus on energy efficiency opportunities for key reservation facilities, with a continued analysis of smaller renewable energy opportunities within reservation boundaries. The consulting team initially performed a resource analysis for biomass and solar generation opportunities in the region of the Rancheria. It was quickly concluded that none of these options would yield renewable power for the Rancheria at costs competitive with current utility sources, and that any larger installations would require substantial funding that may not be available. Having made these conclusions early on, the study effort was redirected and the team investigated each of the major Rancheria buildings to look for solar, wind and conservation opportunities. The buildings were audited for energy use and the roof areas were examined for exposure of solar radiation. Wind resources were also investigated to determine if smaller wind turbines would offer power generation at a reasonable cost.

Greg Retzlaff

2007-07-01T23:59:59.000Z

107

Won Young Park  

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

Won Park Won Park Won Young Park International Energy Studies Group Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 90R2002 Berkeley CA 94720 Office Location: 90-2144 (510) 495-2252 WYPark@lbl.gov Won Young Park is a senior research associate at Lawrence Berkeley National Laboratory (LBNL). He is working on technical analysis for televisions, computer monitors, and lighting for the Super-efficient Equipment and Appliance Deployment (SEAD) Initiative. In the studies, he assesses energy savings potential in efficiency improvement options, evaluates cost effectiveness of key technologies, and provides technical information and recommendations for policies and programs designed to accelerate the adoption of efficient technologies. He also supports a Korea project that

108

First Measurements of the Longitudinal Bunch Profile at SLAC Using Coherent Smith-Purcell Radiation at 28GeV  

Science Conference Proceedings (OSTI)

Coherent Smith-Purcell radiation has been demonstrated as a technique for measuring the longitudinal profile of charged particles bunches in the low to intermediate energy range. However, with the advent of the International Linear Collider, the need has arisen for a non-invasive method of measuring the bunch profile at extremely high energies. Smith-Purcell radiation has been used for the first time in the multi-GeV regime to measure the longitudinal profile of the 28GeV SLAC beam. The experiment has both successfully determined the bunch length, and has also demonstrated its sensitivity to bunch profile changes. The challenges associated with this technique, and its prospects as a diagnostic tool are reported here.

Blackmore, V.; Doucas, G.; Ottewell, B.; Perry, C.; /Oxford U.; Kimmitt, M.F.; /Essex U.; Arnold, R.; Molloy, S.; Woods, M.; /SLAC

2011-11-02T23:59:59.000Z

109

From: Adams, Charlie To: Regulatory.Review Cc: Stern, Jim; Parker, Mike; Dana, Paul; Josh Greene; Frank Stanonik; Neil Rolph; Schuh, Darrell; Roy Smith; Dan  

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

Adams, Charlie To: Regulatory.Review Cc: Stern, Jim; Parker, Mike; Dana, Paul; Josh Greene; Frank Stanonik; Neil Rolph; Schuh, Darrell; Roy Smith; Dan Snyder; Berning, Dave Subject: EO 13563 Preliminary Plan comments from A.O. Smith Corporation Date: Monday, August 01, 2011 2:59:51 PM A.O. Smith Corporation Response to Preliminary Plan for Retrospective Analysis of Existing Rules A.O. Smith Corporation is the largest manufacturer of residential and commercial water heating equipment in the United States. We have the following comments in response to the July 11, 2011, Notice of Availability in the Federal Register, in which DOE sought comments regarding its EO 13563 Preliminary Plan: · In general, we commend DOE's approach to review significant rules on an on-going basis in order

110

Mineralogy and geochemistry of Mariano Lake uranium deposit, Smith Lake district  

Science Conference Proceedings (OSTI)

The Mariano Lake uranium deposit is located on the west side of the Smith Lake district in the Grants mineral belt. Mineralization is restricted to a basal arkosic sandstone of the Brushy Basin Member of the Morrison Formation (Upper Jrassic). This sandstone is equivalent to the Poison Canyon sandstone of the Ambrosia Lake district and contains a series of paleochannels that have been mineralized. The ore displays a roll-type geometry and is located at an iron-sulfur redox interface. The deposit is chemically different from other deposits of the grants mineral belt. It is characterized by low total carbon dioxide, calcium, molybdenum, and selenium, whereas sulfur and vanadium are enriched. Arsenic and zinc exhibit regular zoning patterns across the deposit. The deposit contains an ubiquitous assemblage of pyrite, kaolinite, chlorite, illite, and illite-montmorillonite associated with vanadiferous ore mixed with organic carbon. No primary uranium minerals have been identified. Gypsum (variety selenite) is present, but calcite is absent. The age of mineralization is unknown. The ore has been remobilized, perhaps more than once, and mineralization may have occurred during mid-Cretaceous, Laramide, or post-Laramide time. Based on existing data, polygenetic models are as reasonable as a single stage of remobilization.

Place, J. (Gulf Oil Corp., Casper, WY); Della Valle, R.S.; Brookins, D.G.

1980-01-01T23:59:59.000Z

111

Torbett-Hutchings-Smith Memorial Hospital geothermal-system demonstration at Marlin, Texas. Final design report  

SciTech Connect

The final design and economics of the Torbett-Hutchings-Smith (THS) Memorial Hospital geothermal heating system at Marlin, Texas are outlined. A brief description of the existing heating system, an overview of the geothermal retrofit, and the results of an economic analysis are included. It is estimated that the geothermal heating system will displace approximately 84 percent of the hospital's average annual natural gas consumption. In summer conditions, approximately 45 gpm of geothermal fluid will be utilized at a wellhead temperature of 139/sup 0/F. In peak demand winter conditions, approximately 160 gpm will be utilized at a wellhead temperature of 148/sup 0/F. The geothermal fluid temperature drop across the system will range from about 5/sup 0/F in summer to over 45/sup 0/F during winter. Total capital costs for the system are estimated to be $673,000, including the production well, a geothermal equipment room, engineering and architectural costs, and all equipment. The average annual natural gas savings are expected to be $28,200 while average annual operating and maintenance costs are estimated to be $7750. A before tax life cycle economic analysis of the THS system shows the breakeven period (BEP) of 29 years falling slightly below the 30 year expected life. This BEP is significantly influenced by the developmental nature of this project and by its lack of tax incentives.

1980-09-17T23:59:59.000Z

112

Site study plan for Transportation, Deaf Smith County Site, Texas: Preliminary draft  

SciTech Connect

This site study plan describes transportation field studies to be conducted during the characterization of the Deaf Smith County, Texas, site for the US Department of Energy's Salt Repository Project. The studies are needed to identify and assess potential project impacts to transportation infrastructure and systems in the project vicinity and along potential transportation routes to the site across the State of Texas. The studies are also needed to locate and design project transportation facilities, and to evaluate and design impact mitigation. After identifying the transportation information requirements needed to comply with Federal, State, and local regulations and repository program requirements, the site study plan describes the study design and rationale, the field data collection procedures and equipment, the data analysis methods and application of results, the data management strategy, the schedule of field activities, the management of the study, and the study's quality assurance program. The field data collection activities are organized into programs for the characterization of site vicinity rail corridors and highway corridors, characterization of alternative statewide transportation routes, monitoring of site characterization effects on transportation, characterization of aircraft overflight patterns and hazardous material transportation patterns, and assessment of emergency response preparedness along alternative statewide transportation routes. 34 refs., 10 figs., 2 tabs.

1987-06-01T23:59:59.000Z

113

Community College Highlights Paducah Site Groundwater Model | Department of  

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

Community College Highlights Paducah Site Groundwater Model Community College Highlights Paducah Site Groundwater Model Community College Highlights Paducah Site Groundwater Model May 8, 2013 - 12:00pm Addthis Steve Hampson of the University of Kentucky, left to right, West Kentucky Community & Technical College President Dr. Barbara Veazey, Paducah Junior College Board of Trustees member Ken Wheeler and Buz Smith of the DOE Paducah Site Office examine a DOE Paducah Site groundwater model exhibit at the West Kentucky Community & Technical College Emerging Technology Center. Steve Hampson of the University of Kentucky, left to right, West Kentucky Community & Technical College President Dr. Barbara Veazey, Paducah Junior College Board of Trustees member Ken Wheeler and Buz Smith of the DOE Paducah Site Office examine a DOE Paducah Site groundwater model exhibit at

114

NREL: Energy Analysis - Katherine Young  

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

Katherine Young, P.E. Katherine Young, P.E. Photo of Katherine Young Katherine Young is a member of the Technology Systems and Sustainability Analysis Group in the Strategic Energy Analysis Center. Geothermal Energy Engineer On staff since June 2008 Phone number: 303-384-7402 E-mail: katherine.young@nrel.gov Areas of expertise Geothermal planning and opportunities Database planning and development Primary research interests Geothermal and hydroelectric energy opportunities U.S. DOE Geothermal Program Information Education and background training Continuing Education at University of Colorado in Boulder and Denver Groundwater modeling Quantitative methods in water resource engineering Water resource engineering and management Independent study in groundwater hydrology M.S. in geochemistry and isotope geology, 2002, University of

115

Young Americans | Department of Energy  

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

Young Americans Young Americans Young Americans Competitions 2013 EcoCar2 Challenge Primary Ed DOE 2013 National Science Bowl Primary Ed DOE Challenge Home Student Design University EERE 2013 National Clean Energy Business Plan University EERE 2013 Solar Decathlon University EERE/DOE 2013 National Collegiate Wind University DOE Better Buildings University DOE Energy Challenge University DOE Georgetown University Energy Prize University Georgetown Univ. P3: People, Prosperitym and the Planet University EPA National Clean Energy Business Plan University DOE National Geothermal Student University ORISE Hydrogen and Fuel Cell Competitions University NREL H2U Student Contest University HEF American Solar Challenge University ASC

116

MIKE TURNER ON SPOTTING YOUNG  

E-Print Network (OSTI)

BAE SYSTEMS MIKE TURNER ON SPOTTING YOUNG TALENT AND THE GROWTH OF HIS BUSINESS Success stories? Surely, it is about making lots of money, gaining power, status and prestige, and then using this wealth, the extinction of many animal and plant species, and global warming demonstrated that the raw materials

117

Feeding Young Horses For Sound Development  

E-Print Network (OSTI)

Horse owners must decide whether their young horses will be fed for moderate or rapid growth. One concern is the occurrence of bone and joint disorders in young horses that develop rapidly. Research has shown that this and other problems can be decreased by ensuring that young horses receive proper nutrition. Specific recommendations are included for creep feeding foals and for feeding weanlings and yearlings. Nutritional levels are discussed in relation to the amount of exercise young horses receive.

Gibbs, Pete G.; Potter, Gary D.

2005-05-25T23:59:59.000Z

118

Microsoft PowerPoint - 2013_2-22_Waste_Management_Symposium_-_T._Smith_ARI_Creating_a_2020_DOE  

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

Revitalization Initiative Revitalization Initiative Goals, Task Force, and Deliverables Tania Smith, DOE-EM ARI Task Force Leader February 2013 ARI Mission The Asset Revitalization Initiative (ARI) is a U.S. Department of Energy (DOE)-wide effort to advance the beneficial reuse of its unique and diverse mix of assets, including land, facilities, infrastructure, equipment, technologies, natural resources, and a highly skilled workforce. ARI promotes a more efficient business environment to encourage collaboration between public and private resources. This will maximize benefits to achieve energy and environmental goals, as well as to stimulate and diversify regional economies. 4/4/2013 2 ARI Vision for the DOE Complex * Site operations are conducted in a sustainable manner, facilities and transit are powered by clean

119

July 24, 2009, Visiting Speakers Program - Public-Private Partnerships and Technology Transfer by Dr. Ralph Taylor-Smith  

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

Tech-Transfer & the 21 Tech-Transfer & the 21 st Century Public-Private Partnership Ralph E. Taylor-Smith PhD MBA Battelle Venture Partners DOE-NAPA Forum Washington DC July 24, 2009 Commentary: Derived from Private-Sector Perspective on Tech-Commercialization * Active venture-capital (VC) industry player; various early-stage tech start-ups (federally-funded R&D) * University teaching as active adjunct Professor on Tech-Entrepreneurship & Industrial Innovation * Technology I-Banking (M&A, IPOs) on Wall-St * Prior decade-long industrial experience at Bell Labs as R&D scientist and technology manager * LLNL Industrial Advisory Board; NSF SBIR/STTR Focus on taking Federally-funded R&D to Commercial Market * DOE National Lab focus: LawrenceLivermore, OakRidge, Pacific Northwest, Brookhaven,

120

The Newsletter of the TMS Young Leaders Committee RESEARCH ...  

Science Conference Proceedings (OSTI)

Volume 3, Number 1. The Newsletter of the TMS Young Leaders Committee. RESEARCH, EXCHANGE, AND EXPLORATION: THE YOUNG LEADER...

Note: This page contains sample records for the topic "young buz smith" 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

October The Young Leader.indd  

Science Conference Proceedings (OSTI)

The award includes a $500 stipend from the Ford Motor Company and is open exclusively ... for young professionals in the oil and gas industry. In May, Csontos.

122

2013 Young Leader Meet the Candidate Poster Session  

Science Conference Proceedings (OSTI)

Jan 15, 2013... Young Leader Meet the Candidate Poster Session. Sponsorship, TMS: Young Leaders Committee. Organizer(s), Kinga A. Unocic, ORNL

123

Hopf Structures on Standard Young Tableaux  

SciTech Connect

We review the Poirier-Reutenauer Hopf structure on Standard Young Tableaux and show that it is a distinguished member of a family of Hopf structures. The family in question is related to deformed parastatistics.

Loday, Jean-Louis [IRMA, CNRS and Univ. Strasbourg, 7 rue Descartes, 67084 Strasbourg (France); Popov, Todor [INRNE, BAS, 72 Tsarigradsko Chaussee, 1784 Sofia (Bulgaria)

2010-06-17T23:59:59.000Z

124

Young Energy, LLC | Open Energy Information  

Open Energy Info (EERE)

Young Energy, LLC Place Texas Utility Id 56248 Utility Location Yes Ownership R NERC ERCOT Yes ISO Ercot Yes Activity Retail Marketing Yes References EIA Form EIA-861 Final Data...

125

Interview of Richard Smith  

E-Print Network (OSTI)

teacher, Ernst Wangerman, who subsequently went on to have a chair in European History at Leeds; he had been a pupil of Christopher Hill's and had published his Oxford DPhil in the Oxford series; I thought that quite exotic from the point of view...

Smith, Richard

2011-01-01T23:59:59.000Z

126

smith-98.pdf  

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

Studies Madison, Wisconsin H. B. Howell NOAA-National Environmental Satellite Data Information Service Madison, Wisconsin Introduction A new temperature and water vapor...

127

Smith-AM  

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

1999: Experimental and theoretical study of uncertainty in pyranometers for surface radiation. The EOSSPIE Symposium on Remote Sensing, September 20-24, 1999, Florence, Italy...

128

Scott Smith | BNL  

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

for the ground and rooftop stations, this included two Mini SODARs May 2009: Ameriflux Tall Tower Test. The lead BNL representative for the tracer release units for 2...

129

Microsoft PowerPoint - 6-01 Smith NGM Presentation_EM Tech Exchange-Session 6_Nov16-182010_FINAL.pptx  

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

Next Generation Waste Glass Melters Next Generation Waste Glass Melters Next Generation Waste Glass Melters The U.S. DOE Waste Processing Program The U.S. DOE Waste Processing Program Study Contributors: G.L. Smith, S.P. Schneider, Y.T. Collazo -- EM-30 W.G. Ramsey, T. Sams -- WRPS D.S. Kim, J.D. Vienna, G. Sevigny, M.J. Schweiger - PNNL E. Tchemitcheff, C. Veyer - AREVA B. Bowan, I. Joseph - ES D.E. Day -- MS&T I.L. Pegg, K.S. Matlack, W. Kot, I.S. Muller - CUA D.K. Peeler, F.R. Johnson, J.C. Marra - SRNL N. Soelberg, J. Roach - INL C.W. Kim - KHNP D. Lopukh - LETI S. Stefanovsky - RADON A. Aloy - KRI G.L. Smith, S.P. Schneider and Y.T. Collazo November 2010 Print Close U.S. National Academy of Sciences Roadmap U.S. National Academy of Sciences Roadmap Recommendations Recommendations  Recognizing the importance of melter technology to the

130

EM SSAB CHAIRS  

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

February 23, 2012 Participants Board Chairs/Representatives Site Support Staff Hanford Susan Leckband Paula Call, Tifany Nguyen, Sharon Braswell Idaho Willie Preacher Peggy Hinman Nevada Kathleen Bienenstein Kelly Snyder, Denise Rupp Northern New Mexico Ralph Phelps Ed Worth, Menice Santistevan Oak Ridge Ed Juarez Melyssa Noe, Pete Osborne, Spencer Gross Paducah Buz Smith, Eric Roberts, Jim Ethridge Portsmouth Dick Snyder Julie Galloway Savannah River Don Bridges Erica Williams DOE-HQ Representatives EM-3.2 Catherine Alexander, Melissa Nielson, Michelle Hudson, Dave Borak, Elizabeth Schmitt EM-10 Mark Gilbertson EM-60 Terry Tyborowski Opening Remarks Ms. Catherine Alexander, Designated Federal Officer for the Environmental Management Site-

131

2008 Rosalind Franklin Young Investigator Award  

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

The 2008 3-Way Meeting The 2008 3-Way Meeting In R&D, Super X-rays Mark Many Spots A New Gas Loading System for Diamond Anvil Cells at GSECARS Sidorowicz Named "Supervisor of the Year" SESS 2007: The School for Environmental Sciences with Synchrotrons APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed 2008 Rosalind Franklin Young Investigator Award APRIL 24, 2008 Bookmark and Share Oleg Shpyrko The Advanced Photon Source (APS) Users Organization has named Oleg G. Shpyrko of the University of California, San Diego, as the recipient of the 2008 Rosalind Franklin Young Investigator Award. The award recognizes an important technical or scientific accomplishment by a young investigator that depended on, or is beneficial to, the APS. Shpyrko will receive the

132

APSUO Announces Rosalind Franklin Young Investigator Award  

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

APSUO Announces Rosalind Franklin Young Investigator Award APSUO Announces Rosalind Franklin Young Investigator Award In conjunction with the Advanced Photon Source (APS), the APS Users Organization (APSUO) has established the APSUO Rosalind Franklin Young Investigator Award. The nomination deadline for this award is March 15, 2004. The award will be presented at the 2004 Users Meeting for the Advanced Photon Source, held at Argonne on May 3-6, 2004. Rosalind Franklin Born in 1920, Rosalind Franklin graduated from Cambridge University in 1941 in time to focus on a wartime problem: the composition of coal and charcoal and how to use them most efficiently. She published five papers on the subject before she was 26 years old, work that is still quoted today, and helped launch the field of high-strength carbon fibers. When Franklin had

133

Detecting Free-Mass Common-Mode Motion Induced by Incident Gravitational Waves: Testing General Relativity and Source Direction via Fox-Smith and Michelson Interferometers  

E-Print Network (OSTI)

In this paper we show that information on both the differential and common mode free-mass response to a gravitational wave can provide important information on discriminating the direction of the gravitational wave source and between different theories of gravitation. The conventional Michelson interferometer scheme only measures the differential free-mass response. By changing the orientation of the beam splitter, it is possible to configure the detector so it is sensitive to the common-mode of the free-mass motion. The proposed interferometer is an adaptation of the Fox-Smith interferometer. A major limitation to the new scheme is its enhanced sensitivity to laser frequency fluctuations over the conventional, and we propose a method of canceling these fluctuations. The configuration could be used in parallel to the conventional differential detection scheme with a significant sensitivity and bandwidth.

Michael Edmund Tobar; Toshikazu Suzuki; Kazuaki Kuroda

2009-03-29T23:59:59.000Z

134

Neural processes supporting young and older adults' emotional memories  

Science Conference Proceedings (OSTI)

Young and older adults are more likely to remember emotional information than neutral information. The present functional magnetic resonance imaging study examined the neural processes supporting young (ages 18--35) and older (ages 62--79) adults' successful ...

Elizabeth A. Kensinger; Daniel L. Schacter

2008-07-01T23:59:59.000Z

135

Mi-Young Kim - Research Staff - FEERC  

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

Mi-Young Kim Mi-Young Kim Post Doctoral Research Associate (F) 865-946-1354 kimm@ornl.gov Professional Highlights Education Ph.D., Applied Chemical Engineering, Chonnam National University, 2008 Miyoung joined the Oak Ridge National Laboratory (ORNL) as a post-doctoral researcher in 2010. She has worked at the Center for Development of Fine Chemicals and the Research Institute for Catalysis in Chonnam National University prior to joining the ORNL. Her research background is in heterogeneous catalysis and highly dispersed noble metal catalysts. She has extensive experience in characterizing catalysts using EXAFS, XPS, XRD, solid NMR and ESR. She is currently involved in automotive catalysis research with an emphasis on monolithic catalysts & materials relevant to lean NOx and cold start emissions controls

136

Women @ Energy: Young-Kee Kim | Department of Energy  

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

Young-Kee Kim Young-Kee Kim Women @ Energy: Young-Kee Kim March 19, 2013 - 3:37pm Addthis Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago Check out other profiles in the Women @ Energy series and share your favorites on Pinterest. Young-Kee Kim is the Deputy Director of Fermi National Accelerator Laboratory and a Louis Block Professor of Physics at the University of Chicago. As an experimental particle physicist, Young-Kee's research focuses on understanding the origin of mass for fundamental particles. Since July 2006, she has served as Deputy Director of Fermi National

137

TMS Young Leaders Committee Materials Week '97 Meeting Minutes  

Science Conference Proceedings (OSTI)

Sep 14, 1997 ... Each attendee participated in one of the focus groups established to focus on directives and goals of the Young Leaders Committee.

138

Combinatorics of Arc Diagrams, Ferrers Fillings, Young ... - CECM  

E-Print Network (OSTI)

Jul 22, 2009 ... I Generalization of permutation matrices: fill each row & column of a Ferrers shape ... Standard Young Tableaux. Arc Diagrams,. Nesting and.

139

Building Removal Ongoing at DOE's Paducah Site | Department of Energy  

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

Building Removal Ongoing at DOE's Paducah Site Building Removal Ongoing at DOE's Paducah Site Building Removal Ongoing at DOE's Paducah Site August 23, 2012 - 12:00pm Addthis Media Contact Buz Smith Robert.Smith@lex.doe.gov 270-441-6821 PADUCAH, KY - Work is ongoing at the Paducah Gaseous Diffusion Plant (PGDP) to raze a 65,000-square-foot facility known as the C-340 Metals Plant, which was used to make uranium metal during the Cold War. Department of Energy (DOE) cleanup contractor LATA Environmental Services of Kentucky began removing more than 1,500 panels of cement-asbestos siding from the Metals Plant complex Wednesday in anticipation of New Jersey-based LVI Services starting demolition Sept. 19. Demolition work is projected to last through the end of calendar 2012. "This is an important milestone because the C-340 Metals Plant is the

140

Microsoft Word - EMSSABChairs.conferencecall.Nov19.FINAL.doc  

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

SSAB CHAIRS SSAB CHAIRS Bi-Monthly Conference Call November 19, 2009 Participants Chairs/Representatives: Idaho R.D. Maynard, Lisa Aldrich Nevada Walt Wegst, Hal Sullivan, Denise Rupp NNM Ralph Phelps, Jeff Casalina, Menice Santistevan Oak Ridge Ron Murphree, Kevin Westervelt, Dave Adler, Pete Osborne Paducah Mark Sullivan, Maggie Morgan, Buz Smith, Eric Roberts Portsmouth Richard Snyder, Greg Simonton, Julie Galloway Richland/Hanford Susan Leckband, Shelley Cimon Savannah River Manuel Bettencourt, Sheron Smith DOE Representatives: EM-42 Melissa Nielson, Cate Brennan, Allison Clark EM-5 Shari Davenport EM-30 Joann Luczak EM-43 Christine Gelles EM-72 Kaye Sylvester, Tobie Juleau, James Powers Opening Remarks Ms. Brennan called the meeting to order at 3:00 pm EST and conducted a roll call by site.

Note: This page contains sample records for the topic "young buz smith" 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

New Directions in Gender and Sexuality Studies: Gayatri Chakravorty Spivak, Rebecca Jordan-Young, and Alondra Nelson Will Be Featured in Winter Quarter  

E-Print Network (OSTI)

Chakravorty Spivak, Rebecca Jordan-Young, and Alondra NelsonUniversity, Rebecca Jordan-Young, Associate Professor ofan embarrassment. Rebecca Jordan-Young Rebecca Jordan-Young

McLean, Lindsey; Johnson, Janea

2011-01-01T23:59:59.000Z

142

Computer game design and the imaginative play of young children  

Science Conference Proceedings (OSTI)

This paper discusses preliminary findings of the study of computer game design in relation to current understanding of imaginative play and its developmental value for young children. The crucial role of children's play in their development is well documented. ... Keywords: child development, computer games, design criteria, imaginative play, young children

Irina Verenikina; Jan Herrington

2009-06-01T23:59:59.000Z

143

HOW TO FIND YOUNG MASSIVE CLUSTER PROGENITORS  

SciTech Connect

We propose that bound, young massive stellar clusters form from dense clouds that have escape speeds greater than the sound speed in photo-ionized gas. In these clumps, radiative feedback in the form of gas ionization is bottled up, enabling star formation to proceed to sufficiently high efficiency so that the resulting star cluster remains bound even after gas removal. We estimate the observable properties of the massive proto-clusters (MPCs) for existing Galactic plane surveys and suggest how they may be sought in recent and upcoming extragalactic observations. These surveys will potentially provide a significant sample of MPC candidates that will allow us to better understand extreme star-formation and massive cluster formation in the Local Universe.

Bressert, E.; Longmore, S.; Testi, L. [European Southern Observatory, Karl Schwarzschild Str. 2, D-85748 Garching bei Muenchen (Germany); Ginsburg, A.; Bally, J.; Battersby, C. [Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309 (United States)

2012-10-20T23:59:59.000Z

144

EA-1974: Wallooskee-Youngs Confluence Restoration Project, Clatsop County,  

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

4: Wallooskee-Youngs Confluence Restoration Project, Clatsop 4: Wallooskee-Youngs Confluence Restoration Project, Clatsop County, Oregon EA-1974: Wallooskee-Youngs Confluence Restoration Project, Clatsop County, Oregon Summary Bonneville Power Administration is preparing an EA to assess the potential environmental impacts of the proposed restoration of a tidal marsh in the Columbia River Estuary, near Astoria in Clatsop County, Oregon. The project website is https://www.bpa.gov/goto/WallooskeeYoungs. Public Comment Opportunities Comments on the scope of the EA should be marked "Wallooskee-Youngs Confluence Restoration Project" and submitted by January 27, 2014, by one of the methods listed below. Comments will be posted in their entirety on BPA's website at www.bpa.gov/comments. Toll-free phone: 800-622-4519

145

Brigham Young University, Brigham Young University--Hawaii, BYU--Idaho, and LDS Business College exist to provide an  

E-Print Network (OSTI)

Brigham Young University, Brigham Young University--Hawaii, BYU--Idaho, and LDS Business College, and student body at BYU, BYU-- Hawaii, BYU--Idaho, and LDSBC are selected and retained from among those who represent BYU, BYU--Hawaii, BYU--Idaho, and LDSBC are to maintain the highest standards of honor, integrity

Hart, Gus

146

Training and Technology ? Janice Smiths story  

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

Janice and her desire to return to her roots. Janice says, "I graduated from the Training and Technology Physical Testing Program sponsored by Union Carbide in February, 1981....

147

Nonproliferation Graduate Fellowship Program Attracts High Caliber Young  

National Nuclear Security Administration (NNSA)

Graduate Fellowship Program Attracts High Caliber Young Graduate Fellowship Program Attracts High Caliber Young Professionals to Careers in Nonproliferation and National Security | 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 > NNSA Blog > Nonproliferation Graduate Fellowship Program Attracts High Caliber ... Nonproliferation Graduate Fellowship Program Attracts High Caliber Young

148

Research drilling in young silicic volcanoes  

DOE Green Energy (OSTI)

Magmatic activity, and particularly silicic magmatic activity, is the fundamental process by which continental crust forms and evolves. The transport of magma from deep crustal reservoirs to the surface is a neglected but important aspect of magmatic phenomena. It encompasses problems of eruptive behavior, hydrothermal circulation, and ore deposition, and must be understood in order to properly interpret deeper processes. Drilling provides a means for determining the relationship of shallow intrusive processes to eruption processes at young volcanoes where eruptions are best understood. Drilling also provides a means for directly observing the processes of heat and mass transfer by which recently emplaced intrusions approach equilibrium with their new environment. Drilling in the Inyo Chain, a 600-year-old chain of volcanic vents in California, has shown the close relationship of silicic eruption to shallow dike emplacement, the control of eruptive style by shallow porous-flow degassing, the origin of obsidian by welding, the development of igneous zonation by viscosity segregation, and the character and size of conduits in relation to well-understood magmatic and phreatic eruptions. 36 refs., 9 figs.

Eichelberger, J.C.

1989-06-30T23:59:59.000Z

149

The Young Open Cluster NGC 2129  

E-Print Network (OSTI)

The first CCD UBV(RI) photometric study in the area of the doubtful open cluster NGC 2129 is presented. Photometry of a field offset 15 arcmin northward is also provided, to probe the Galactic disk population toward the cluster. Using star counts, proper motions from the UCAC2 catalog, colour-magnitude and colour-colour diagrams we demonstrate that NGC 2129 is a young open cluster. The cluster radius is 2.5 arcmin, and across this region we find evidence of significant differential reddening, although the reddening law seems to be normal toward its direction. Updated estimates of the cluster fundamental parameters are provided. The mean reddening is found to be E(B-V)=0.80$\\pm$0.08 and the distance modulus is $(m-M)_o$= 11.70$\\pm0.30$. Hence, NGC 2129 is located at 2.2$\\pm$0.2 kpc from the Sun inside the Local spiral arm. The age derived from 37 photometrically selected members is estimated to be approximately 10 million years. These stars are used to provide new estimates of the cluster absolute proper motion components.

Giovanni Carraro; Brian Chaboyer; James Perencevich

2005-10-19T23:59:59.000Z

150

Jeff Smith | ornl.gov  

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

environment, safety, and health; business operations; security; human resources; communications; and technology transfer. In concert with the Deputy Director of Science...

151

Hanford Grows Young Minds Through Site Tours | Department of Energy  

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

Hanford Grows Young Minds Through Site Tours Hanford Grows Young Minds Through Site Tours Hanford Grows Young Minds Through Site Tours June 3, 2013 - 12:00pm Addthis John Britton, with Office of River Protection contractor Washington River Protection Solutions, explains the Hanford tank waste program to Western Washington University students in a recent tour of the Hanford site. John Britton, with Office of River Protection contractor Washington River Protection Solutions, explains the Hanford tank waste program to Western Washington University students in a recent tour of the Hanford site. RICHLAND, Wash. - It is harvest season for cherries, raspberries and rhubarb in Washington state. But employees at the Hanford site are helping grow the young minds of the nation's future science, technology,

152

Young Scientist Research Award The award recognizes a scienti  

Science Conference Proceedings (OSTI)

Young Scientist Research Award The award recognizes a scientist who has made a significant and substantial research contribution in one of the areas represented by the Divisions of AOCS.

153

Trends in the Health of Young Children in California  

E-Print Network (OSTI)

Research Brief October 2008 Trends in the Health of YoungThis brief examines trends in key health indicators forpoints (Exhibit 2). This trend has kept the overall health

Grant, David; Kurosky, Samantha

2008-01-01T23:59:59.000Z

154

Wave Breaking Dissipation in a Young Wind Sea  

Science Conference Proceedings (OSTI)

Coupled in situ and remote sensing measurements of young, strongly-forced, wind waves are applied to assess the role of breaking in an evolving wavefield. In situ measurements of turbulent energy dissipation from wave-following SWIFT drifters ...

Michael Schwendeman; Jim Thomson; Johannes R. Gemmrich

155

Using computer-based testing with young children  

Science Conference Proceedings (OSTI)

In this era of increased accountability in education, there is a need for tools to use in assessing the abilities and instructional levels of young children. Computers have been used successfully to assess older children and adults. However, ...

Susan Kubic Barnes / J. Christine Harmes

2010-01-01T23:59:59.000Z

156

The Martin Boundary Of The Young-Fibonacci Lattice  

E-Print Network (OSTI)

In this paper we find the Martin boundary for the Young-Fibonacci lattice YF. Along with the lattice of Young diagrams, this is the most interesting example of a differential partially ordered set. The Martin boundary construction provides an explicit Poisson-type integral representation of non-negative harmonic functions on YF. The latter are in a canonical correspondence with a set of traces on Okada locally semisimple algebra.

Frederick M. Goodman; Sergei V. Kerov

1997-01-01T23:59:59.000Z

157

Lithium: Measurement of Young's Modulus and Yield Strength  

Science Conference Proceedings (OSTI)

The Lithium Collection Lens is used for anti-proton collection. In analyzing the structural behavior during operation, various material properties of lithium are often needed. properties such as density, coefficient of thermal expansion, thermal conductivity, specific heat, compressability, etc.; are well known. However, to the authors knowledge there is only one published source for Young's Modulus. This paper reviews the results from the testing of Young's Modulus and the yield strength of lithium at room temperature.

Ryan P Schultz

2002-11-07T23:59:59.000Z

158

Linda Young of APS Elected Vice Chair of DAMOP  

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

Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award Moffat of BioCARS and U. of C. Receives 2011 ACA Patterson Award Argonne's Fenter Wins Warren Award for X-ray Diffraction Studies Lahsen Assoufid Elected a Fellow of SPIE 2011 Arthur H. Compton Award Announced by APSUO X-Ray Focusing: Techniques and Applications APS News Archives: 2012 | 2011 | 2010 | 2009 2008 | 2007 | 2006 | 2005 2004 | 2003 | 2002 | 2001 2000 Subscribe to APS News rss feed Linda Young of APS Elected Vice Chair of DAMOP JULY 14, 2011 Bookmark and Share Linda Young Argonne Distinguished Fellow and Argonne National Laboratory X-ray Science Division (XSD) Director Linda Young has been elected vice chair of the Division of Atomic, Molecular, and Optical Physics of the American Physical Society (DAMOP). The position became official at the 2011 DAMOP Meeting

159

Calling all Young Entrepreneurs: Deadline for Energy Department Business  

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

Calling all Young Entrepreneurs: Deadline for Energy Department Calling all Young Entrepreneurs: Deadline for Energy Department Business Plan Competition Approaching Calling all Young Entrepreneurs: Deadline for Energy Department Business Plan Competition Approaching December 1, 2011 - 12:08pm Addthis If you’re a university student interested in low-carbon technologies and entrepreneurship, then this is the premier opportunity for you to pitch your idea. The Regional Clean Energy Business Plan Competition is accepting business plan submissions from today until March 2, 2012. If you're a university student interested in low-carbon technologies and entrepreneurship, then this is the premier opportunity for you to pitch your idea. The Regional Clean Energy Business Plan Competition is accepting business plan submissions from today until March 2, 2012.

160

Why Has Home Ownership Fallen Among the Young? ?  

E-Print Network (OSTI)

We document that home ownership of households with heads aged 25 44 years fell substantially between 1980 and 2000 and recovered only partially during the 20012005 housing boom. The 19802000 decline in young home ownership occurred as improvements in mortgage opportunities made it easier to purchase a home. This paper uses an equilibrium life-cycle model calibrated to micro and macro evidence to understand why young home ownership fell over a period when it became easier to own a home. Our findings indicate that a trend toward marrying later and the increase in household earnings risk that occurred after 1980 account for 3/5 to 4/5 of the decline in young home ownership.

Jonas D. M. Fisher; Martin Gervais

2009-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Duck Young Chung - Argonne National Laboratories, Materials Sicence  

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

EM > Duck Young Chung EM > Duck Young Chung Duck Young Chung Principal Materials Engineer Bldg. 223, C-233 Phone: 630-252-4907 This e-mail address is being protected from spambots. You need JavaScript enabled to view it. Biography Duck Young Chung is a staff scientist in the Emerging Materials Group. After receiving his B.A. from DanKook University in 1984, M.S. and Ph.D from Kyungpook National University in 1991, he joined the group of Prof. Kanatzidis as a postdoc at Michigan State University in 1992 where later he became a research faculty, then moved to Argonne in 2006. His expertise includes exploratory synthesis, crystal growth, and characterization of a wide variety of bulk materials as well as development of synthesis techniques and methods in the areas of chalcogenides, pnictides, and intermetallic alloys for thermoelectrics, superconductivity, topological insulators, and semiconducting materials with interesting electronic or magnetic properties. He is the author of 80 peer-reviewed articles and patents published. Notable achievements include discovery of high performance thermoelectric semiconductor, CsBi4Te6, which holds the record of figure of merit for low temperature cooling applications (Science, 2000) and synthesis of an unconventional superconductors Ba1-xKxFe2As2 characterized by inelastic neutron scattering (Nature, 2008).

162

Young children's ability to use a computer mouse  

Science Conference Proceedings (OSTI)

Because there is little empirical data available on how well young children are able to use a computer mouse, the present study examined their proficiency in clicking on small objects at various positions on the screen and their skill in moving objects ... Keywords: Elementary education, Human-computer interaction, Interface, Media in education, Navigation

Afke Donker; Pieter Reitsma

2007-05-01T23:59:59.000Z

163

Young children's computer skills development from kindergarten to third grade  

Science Conference Proceedings (OSTI)

This investigation explores young children's computer skills development from kindergarten to third grade using the Early Childhood Longitudinal Study-Kindergarten (ECLS-K) dataset. The sample size of the study was 8642 children. Latent growth curve ... Keywords: Computer skills, Kindergarten, Latent growth curve modeling

Mesut Sakes; Kathy Cabe Trundle; Randy L. Bell

2011-09-01T23:59:59.000Z

164

THE FORMATION OF YOUNG DENSE STAR CLUSTERS THROUGH MERGERS  

SciTech Connect

Young star clusters such as NGC 3603 and Westerlund 1 and 2 in the Milky Way and R136 in the Large Magellanic Cloud are dynamically more evolved than expected based on their current relaxation times. In particular, the combination of a high degree of mass segregation, a relatively low central density, and the large number of massive runaway stars in their vicinity are hard to explain with the monolithic formation of these clusters. Young star clusters can achieve such a mature dynamical state if they formed through the mergers of a number of less massive clusters. The shorter relaxation times of less massive clusters cause them to dynamically evolve further by the time they merge, and the merger product preserves the memory of the dynamical evolution of its constituent clusters. With a series of N-body simulations, we study the dynamical evolution of single massive clusters and those that are assembled through merging smaller clusters together. We find that the formation of massive star clusters through the mergers of smaller clusters can reproduce the currently observed spatial distribution of massive stars, the density, and the characteristics (number and mass distribution) of the stars ejected as runaways from young dense clusters. We therefore conclude that these clusters and possibly other young massive star clusters formed through the mergers of smaller clusters.

Fujii, M. S.; Portegies Zwart, S. F. [Leiden Observatory, Leiden University, NL-2300RA Leiden (Netherlands); Saitoh, T. R. [Interactive Research Center of Science, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551 (Japan)

2012-07-01T23:59:59.000Z

165

Binary populations and stellar dynamics in young clusters  

E-Print Network (OSTI)

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (unconventionally formed objects) like intermediate mass black holes, Eta Carinae, Zeta Puppis, Gamma Velorum and WR 140.

D. Vanbeveren; H. Belkus; J. Van Bever; N. Mennekens

2008-01-17T23:59:59.000Z

166

Binary populations and stellar dynamics in young clusters  

E-Print Network (OSTI)

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (unconventionally formed objects) like intermediate mass black holes, Eta Carinae, Zeta Puppis, Gamma Velorum and WR 140.

Vanbeveren, D; Van Bever, J; Mennekens, N

2008-01-01T23:59:59.000Z

167

Young modulus dependence of nanoscopic friction coefficient in hard coatings  

E-Print Network (OSTI)

with miniature moving parts, such as micro- electromechanical systems and hard-disk drives.1,2 A betterYoung modulus dependence of nanoscopic friction coefficient in hard coatings Elisa Riedoa with varying hardness obtained by different growth temperatures. For the CrN films, we show that the changes

Brune, Harald

168

Microsoft Word - EMSSABChairs.conferencecall.March18.FINAL  

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

March 18, 2010 March 18, 2010 Participants Chairs/Representatives: Idaho Ceri Chapple Nevada Harold Sullivan, Kelly Snyder, Denise Rupp NNM Ralph Phelps Oak Ridge Ron Murphree, Spencer Gross, Pete Osborne Paducah Buz Smith Portsmouth Richard Snyder, Larry Parker, Greg Simonton Richland/Hanford Susan Leckband Savannah River Donald Bridges, Becky Craft DOE representatives: CI Betty Nolan EM-3.1 Thomas Johnson EM-42 Melissa Nielson, Cate Brennan, Michelle Hudson, Allison Clark EM-43 Doug Tonkay EM-60 Joann Luczak EM-62 Jay Rhoderick, Mark Janaskie Congressional Update Ms. Betty Nolan, Acting Assistant Secretary for the Office of Congressional and Intergovernmental Affairs, provided the Chairs with a Congressional update. The Department of Energy (DOE) is in the middle of the budget hearing season. Dr. Inés Triay,

169

Microsoft Word - EMSSABChairs conferencecall Jan22 FINAL.doc  

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

January 22, 2009 January 22, 2009 3:00 p.m. - 4:30 p.m. Participants Chairs/Representatives: Idaho Ceri Chapple Nevada Dave Hermann, Walter Wegst, Stacy Standley, Denise Rupp, Kelly Snyder NNM Ralph Phelps, Jeff Casalina, Menice Santistevan Oak Ridge Ted Lundy, Pat Halsey, Spencer Gross, Pete Osborne Paducah Judy Clayton, Eric Roberts, Buz Smith Portsmouth Val Francis, Richard Snyder, Julie Galloway, David Kozlowski, Greg Simonton Richland/Hanford Susan Leckband, Shelley Cimon Savannah River Donna Antonucci, Ranowul Jzar, Gerri Flemming, Mindy Mets DOE representatives: EM-13 Melissa Nielson, Cate Brennan, Michelle Hudson EM-5/6 James Fiore EM-12 Christine Gelles EM-20 Mark Gilbertson EM-31 Connie Flohr CI Betty Nolan OPENING REMARKS Cate Brennan welcomed participants to the call and reviewed the afternoon's agenda.

170

Microsoft Word - EMSSABChairs conferencecall Jan27.FINAL  

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

January 27, 2011 January 27, 2011 Participants Board Chairs/Representatives Site Support Staff Hanford Susan Leckband Idaho R.D. Maynard, Willie Preacher Nevada Walt Wegst, Kathleen Bienenstein Kelly Snyder, Denise Rupp Northern New Mexico Ralph Phelps, Robert Gallegos Lee Bishop, Menice Santistevan Oak Ridge Ron Murphree, Kevin Westervelt David Adler, Spencer Gross, Pete Osborne Paducah Buz Smith, Eric Roberts Portsmouth Dick Snyder, Larry Parker Rick Greene, Julie Galloway Savannah River Don Bridges Erica Williams DOE-HQ Representatives: EM-5 Shari Davenport EM-60 Joann Luczak EM-41 Tish O'Conor EM-42 Catherine Brennan, Michelle Hudson, Allison Clark EM-43 Arnie Edelman, Dave Mathes EM-3.1 Colin Jones Opening Remarks Ms. Catherine Brennan, Designated Federal Officer for the Environmental Management Site-

171

Microsoft Word - EMSSABChairs.conferencecall.May7.070809.doc  

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

May 7, 2009 May 7, 2009 3:00 p.m. - 4:30 p.m. Participants Chairs/Representatives: Idaho R.D. Maynard, Ceri Chapple Nevada Walter Wegst, Kelly Snyder, Denise Rupp NNM J.D. Campbell, Ralph Phelps, Menice Santistevan Oak Ridge Pete Osborne Paducah Bobby Ann Lee, Judy Clayton, Buz Smith, Eric Roberts, Suzanne Clinton Portsmouth Richard Snyder, David Kozlowski, Greg Simonton Richland/Hanford Susan Leckband, Shelley Cimon Savannah River Ranowul Jzar, Gerri Flemming, Mindy Mets DOE representatives: EM-13 Melissa Nielson, Cate Brennan, Michelle Hudson EM-3 John Mocknick EM-12 Christine Gelles EM-20 Mark Gilbertson EM-30 Merle Sykes Opening Remarks Ms. Cate Brennan welcomed participants to the call and reviewed the afternoon's agenda. American Recovery and Reinvestment Act Update

172

Microsoft Word - EMSSABChairs conferencecall July9 FINAL.doc  

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

July 9, 2009 July 9, 2009 3:00 p.m. - 4:30 p.m. Participants Chairs/Representatives: Idaho R.D. Maynard, Bob Pence Nevada Robert Gatliff, Harold Sullivan, Kelly Snyder, Denise Rupp NNM J.D. Campbell, Ralph Phelps, Jeff Casalina Oak Ridge Ted Lundy, Dave Adler, Spencer Gross, Pete Osborne Paducah Bobby Ann Lee, Judy Clayton, Buz Smith, Eric Roberts Portsmouth Richard Snyder, David Kozlowski, Greg Simonton, Julie Galloway Richland/Hanford Susan Leckband, Shelley Cimon, Lori Gamache Savannah River Manuel Bettencourt, Gerri Flemming, Mindy Mets DOE representatives: EM-13 Melissa Nielson, Cate Brennan, Michelle Hudson EM-2.1 John Mocknick, Kristine Cornils EM-12 Doug Tonkay, Gene Chou EM-31 Connie Flohr CI Katina Tsongas Opening Remarks Cate Brennan welcomed participants to the call and reviewed the afternoon's agenda.

173

The Paleo Project - Fossil, Oregon by Jenny Young, Rowell Brokaw Architects [EDRA/Places Awards 2006 -- Planning  

E-Print Network (OSTI)

courtesy of Rowell Brokaw Architects. Top: Construction ofYoung, Rowell Brokaw Architects In an economically bypassedYoung and Rowell Brokaw Architects / Paleo Project 2006

Moffat, David

2006-01-01T23:59:59.000Z

174

Proceedings Fourth European Young Researchers Workshop on Service Oriented Computing  

E-Print Network (OSTI)

Service-Oriented Computing (SOC) is an emerging new paradigm for distributed and object-oriented computing by allowing autonomous, platform-independent computational entities (called services) to be built (described, discovered, composed, orchestrated) within and across organizational boundaries. Like no other computing paradigm before, SOC is destined to exert a lasting influence on the business domain, among others (e-commerce, e-government, e-business, e-learning, e-health, etc.). The Young Researchers workshop series on Service-Oriented Computing is meant to be a platform for junior researchers from industry and academics alike. Its core objectives are to exchange information regarding advancements in the state of the art and practice of SOC, as well as to identify emerging research topics and the future trends in this domain. Following the success of the previous three workshops, the 4th European Young Researchers Workshop on Service-Oriented Computing (YR-SOC 2009) introduced two novelties: it was organ...

ter Beek, Maurice H

2009-01-01T23:59:59.000Z

175

No evidence for mass segregation in young clusters  

E-Print Network (OSTI)

Aims. We investigate the validity of mass segregation indicators commonly used in the analysis of young stellar clusters. Methods. We simulate observations by constructing synthetic seeing limited images of a 1000 massive clusters (10^4 Msun) with a standard IMF and a King density distribution function. Results. We find that commonly used indicators are highly sensitive to sample incompleteness in observational data, and that radial completeness determinations do not provide satisfactory corrections, rendering the studies of radial properties highly uncertain. On the other hand, we find that under certain conditions, the global completeness can be estimated accurately, allowing for the correction of the global luminosity and mass functions of the cluster. Conclusions. We argue that there is currently no observational evidence for mass segregation in young compact clusters since there is not a robust way to differentiate between true mass segregation and sample incompleteness effects. Caution should then be ex...

Ascenso, J; Lago, M T V T

2008-01-01T23:59:59.000Z

176

Young Professionals in Nuclear Industry Group Forms at Savannah River Site  

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

Young Professionals in Nuclear Industry Group Forms at Savannah Young Professionals in Nuclear Industry Group Forms at Savannah River Site Young Professionals in Nuclear Industry Group Forms at Savannah River Site January 1, 2012 - 12:00pm Addthis The Savannah River Chapter of North American – Young Generation in Nuclear is a new group forming at the Savannah River Site. The Savannah River Chapter of North American - Young Generation in Nuclear is a new group forming at the Savannah River Site. AIKEN, S.C. - Supporting the development of young nuclear professionals in the Central Savannah River Area (CSRA) is the purpose behind a new group forming at the Savannah River Site (SRS). The Savannah River Chapter of North American - Young Generation in Nuclear (SR-YGN) will hold a kick-off meeting Jan. 26 in Aiken and all

177

Warming mineralises young and old soil carbon equally  

E-Print Network (OSTI)

Abstract. The temperature sensitivity of soil organic carbon decomposition is critical for predicting future climate change because soils store 2-3 times the amount of atmospheric carbon. Of particular controversy is the question, whether temperature sensitivity differs between young or labile and old or more stable carbon pools. Ambiguities in experimental methodology have so far limited corroboration of any particular hypothesis. Here, we show in a clear-cut approach that differences in temperature sensitivity between young and old carbon are negligible. Using the change in stable isotope composition in transitional systems from C3 to C4 vegetation, we were able to directly distinguish the temperature sensitivity of carbon differing several decades in age. This method had several advantages over previously followed approaches. It allowed to identify release of much older carbon, avoided un-natural conditions of long-term incubations and did not require arguable curve-fitting. Our results demonstrate that feedbacks of the carbon cycle on climate change are driven equally by young and old soil organic carbon. 1

F. Conen; J. Leifeld; B. Seth; C. Alewell

2006-01-01T23:59:59.000Z

178

Mission of ITER and Challenges for the Young  

Science Conference Proceedings (OSTI)

It is recognized that the ongoing effort to provide sufficient energy for the wellbeing of the globe's population and to power the world economy is of the greatest importance. ITER is a joint international research and development project that aims to demonstrate the scientific and technical feasibility of fusion power. It represents the responsible actions of governments whose countries comprise over half the world's population, to create fusion power as a source of clean, economic, carbon dioxide-free energy. This is the most important science initiative of our time.The partners in the Project--the ITER Parties--are the European Union, Japan, the People's Republic of China, India, the Republic of Korea, the Russian Federation and the USA. ITER will be constructed in Europe, at Cadarache in the South of France. The talk will illustrate the genesis of the ITER Organization, the ongoing work at the Cadarache site and the planned schedule for construction. There will also be an explanation of the unique aspects of international collaboration that have been developed for ITER.Although the present focus of the project is construction activities, ITER is also a major scientific and technological research program, for which the best of the world's intellectual resources is needed. Challenges for the young, imperative for fulfillment of the objective of ITER will be identified. It is important that young students and researchers worldwide recognize the rapid development of the project, and the fundamental issues that must be overcome in ITER.The talk will also cover the exciting career and fellowship opportunities for young people at the ITER Organization.

Ikeda, Kaname [Director General, ITER Organization Cadarache Centre, 13108 St Paul lez Durance (France)

2009-02-19T23:59:59.000Z

179

Microsoft Word - SNOPUD_Youngs_Cr_Hydro_CX_+_Checklist.doc  

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

18, 2010 18, 2010 REPLY TO ATTN OF: KEC-4 SUBJECT: Environmental Clearance Memorandum James Hall Customer Service Engineer - TPC-TPP-4 Proposed Action: Interconnection of Snohomish County Public Utility District No.1 (SNOPUD) Young's Creek Hydro Small Generation Budget Information: WO# 00231295, Task 01 Categorical Exclusion Applied (from Subpart D, 10 C.F.R. Part 1021): B4.6 Additions or modifications to electric power transmission facilities that would not affect the environment beyond the previously developed facility area including, but not limited to, switchyard rock grounding upgrades, secondary containment projects, paving projects, seismic upgrading, tower modifications, changing insulators, and replacement of poles, circuit breakers, conductors,

180

Snowmass 2013 Young Physicists Science and Career Survey Report  

E-Print Network (OSTI)

From April to July 2013 the Snowmass Young Physicists (SYP) administered an online survey collecting the opinions and concerns of the High Energy Physics (HEP) community. The aim of this survey is to provide input into the long term planning meeting known as the Community Summer Study (CSS), or Snowmass on the Mississippi. In total, 1112 respondents took part in the survey including 74 people who had received their training within HEP and have since left for non-academic jobs. This paper presents a summary of the survey results including demographic, career outlook, planned experiments and non-academic career path information collected.

J. Anderson; J. Asaadi; B. Carls; R. Cotta; R. Guenette; B. Kiburg; A. Kobach; H. Lippincott; B. Littlejohn; J. Love; B. Penning; M. Soares Santos; T. Strauss; A. Szelc; E. Worcester; F. Yu

2013-07-30T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Physiological responses of young thoroughbred horses to intermittent high-intensity treadmill training  

E-Print Network (OSTI)

age or extent of previous training in young horses or theirat the outset of the training. Endnotes a Mustang 2200,References 1. Evans DL: Training thoroughbred racehorses. In

Ohmura, Hajime; Matsui, Akira; Hada, Tetsuro; Jones, James H

2013-01-01T23:59:59.000Z

182

Relationships among the personal fable, drug use and parental monitoring in adolescents and young adults.  

E-Print Network (OSTI)

??Relationships among the personal fable, drug use and parental monitoring in adolescents and young adults were tested in this study. Participants were 56 students, with (more)

Liu, Xin, 1986 Feb. 2-

2011-01-01T23:59:59.000Z

183

SENAI and the insertion of the young apprentice in the formal labor market.  

E-Print Network (OSTI)

??This study investigates the impact on the contribution of industrial learning for employability among young learners. The Government, through the Law of the Apprentice (10,097 (more)

Slon Nogueira de Lima

2009-01-01T23:59:59.000Z

184

A Real Reflection of How I Write: Young Adult Female Authors Seizing Agency Through Fan Fiction.  

E-Print Network (OSTI)

??This research project examines ""fan fiction"" (stories based upon existing texts such as movies, books, and video games) written by a young adult female and (more)

Coleman, Susanna

2008-01-01T23:59:59.000Z

185

book on theory and applications of MDS by Young and Hamer, [21 ...  

E-Print Network (OSTI)

book on theory and applications of MDS by Young and Hamer, [21] presents applications of MDS in such diverse fields as marketing.. sociology, physics,...

186

K-Ar dating of young volcanic rocks  

DOE Green Energy (OSTI)

Potassium-Argon (K-Ar) age dates were determined for forty-two young geologic samples by the Laboratory of Isotope Geochemistry, Department of Geosciences, in the period February 1, 1986 to June 30, 1989. Under the terms of Department of Energy Grant No. FG07-86ID12622, The University of Arizona was to provide state-of-the-art K-Ar age dating services, including sample preparation, analytical procedures, and computations, for forty-two young geologic samples submitted by DOE geothermal researchers. We billed only for forty samples. Age dates were determined for geologic samples from five regions with geothermal potential: the Cascade Mountains (Oregon); the Cascade Mountains (Washington); Ascension Island, South Atlantic Ocean; Cerro Prieto, Mexico; and Las Azufres, Mexico. The ages determined varied from 5.92 m.a. to 0.62 m.a. The integration of K-Ar dates with geologic data and the interpretation in terms of geologic and geothermal significance has been reported separately by the various DOE geothermal researchers. Table 1 presents a detailed listing of all samples dated, general sample location, researcher, researcher's organization, rock type, age, and probable error (1 standard deviation). Additional details regarding the geologic samples may be obtained from the respective geothermal researcher. 1 tab.

Damon, P.E.; Shafiqullah, M.

1991-01-31T23:59:59.000Z

187

Adopt, adapt, abandon: Understanding why some young adults start, and then stop, using instant messaging  

Science Conference Proceedings (OSTI)

Instant messaging (IM) has become a popular and important mode of staying in touch for teens and young adults. It allows for easy, frequent and lightweight interaction that contributes to building and sustaining friendships, as well as coordinating social ... Keywords: Adoption, Computer-mediated communication (CMC), Dropouts, Instant messaging, Young adults

Jeremy Birnholtz

2010-11-01T23:59:59.000Z

188

Young's modulus evaluation by SAWs for porous silica low-k film with cesium doping  

Science Conference Proceedings (OSTI)

Young's moduli of porous silica low-k films with cesium (Cs) doping are determined by surface acoustic waves (SAWs) in this study. Four low-k samples doped with 0-30ppmwt% Cs in the precursor solution are investigated to check the mechanical promotion ... Keywords: Cesium doping, Low-k film, Porous silica, Surface acoustic waves, Young's modulus

X. Xiao; X. M. Shan; Y. Kayaba; K. Kohmura; H. Tanaka; T. Kikkawa

2011-05-01T23:59:59.000Z

189

Aiming and clicking in young children's use of the computer mouse  

Science Conference Proceedings (OSTI)

The present study investigated the abilities of young children to aim and click with a computer mouse. Young children have not yet fully developed their motor skills and they are therefore more likely than adults to click next to targets on the computer ... Keywords: Elementary education, Human-computer interaction, Input device, Interface, Media in education, Navigation

Afke Donker; Pieter Reitsma

2007-11-01T23:59:59.000Z

190

Technology policy for the knowledge economy: Public support to young ICT service firms  

Science Conference Proceedings (OSTI)

Public intervention in high-tech sectors is often advocated to resolve market imperfections that may possibly limit the viability of young high-tech enterprises. Although some European countries have adopted national government support policies that ... Keywords: Horizontal direct public subsidies, Italy, Young ICT service firms

Massimo G. Colombo; Luca Grilli

2007-11-01T23:59:59.000Z

191

Baby Brutes: Simulations Help Solve the Mysteries of Massive Young  

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

Baby Brutes Baby Brutes Baby Brutes Simulations Help Solve the Mysteries of Massive Young Star-Forming Galaxies March 31, 2010 | Tags: Astrophysics Contact: Margie Wylie, mwylie@lbl.gov, +1 510 486 7421 Primack-fig1a.png Figure 1. In this model galactic plane (seen in cross section), the energy input of stellar superclusters causes gases to shoot out at speeds up to 1000 kilometers per second at temperatures reaching 100 million Kelvin. These appear as plumes or "chimneys," visible in the top three frames (showing density, temperature, and velocity; the bottom frame shows gas column density). Small bubbles of hot gas in the field (visible in the top two frames) are the result of stellar feedback from runaway stars. Astronomers have in recent years been surprised to find hulking brutes

192

Charles D. Young Project Engineer Government Support Directorate  

Office of Legacy Management (LM)

Please call if you have questions regarding the attached recommendation. i?&,o-o; Please call if you have questions regarding the attached recommendation. i?&,o-o; ~~~pApv $l$I Charles D. Young Project Engineer Government Support Directorate Architecture Planning and Technology Division CDY/smb Attachment cc: J. Fiore ;;,ewis (w/o) TH' E AEROSPACE CORPORATION i ' 0 A Suite 7900, 955 L' Enfam Plaza. S. W., Woshingron. D.C. 20024-2174. Tekphonc (202) 488-6000 7117-03.87.cdy.43 23 September 1987 CA Mr. Andrew Wallo, III, NE-23 Division of Facility & Site Decosunissioning Projects U.S. Department of Energy Germantown, Maryland 20545 Dear Mr. Wallo: ELIMINATION RECOMMENDATION -- COLLEGES AND UNIVERSITIES The attached elimination reconnnendation was prepared in accordance PC.o= with your suggestion during our meeting on 22 September. The recommendation flD.o-02

193

The Very Young Radio Pulsar J1357-6429  

E-Print Network (OSTI)

We report the discovery of a radio pulsar with a characteristic age of 7300 years, making it one of the 10 apparently youngest Galactic pulsars known. PSR J1357-6429, with a spin period of P = 166 ms and spin-down luminosity of 3.1e36 ergs/s, was detected during the Parkes multibeam survey of the Galactic plane. We have measured a large rotational glitch in this pulsar, with Delta P/P = -2.4e-6, similar in magnitude to those experienced occasionally by the Vela pulsar. At a nominal distance of only ~ 2.5 kpc, based on the measured free electron column density of 127 pc/cc and the electron distribution model of Cordes & Lazio, this may be, after the Crab, the nearest very young pulsar known. The pulsar is located near the radio supernova remnant candidate G309.8-2.6.

F. Camilo; R. N. Manchester; A. G. Lyne; B. M. Gaensler; A. Possenti; N. D'Amico; I. H. Stairs; A. J. Faulkner; M. Kramer; D. R. Lorimer; M. A. McLaughlin; G. Hobbs

2004-06-23T23:59:59.000Z

194

36 The Spectra, May 2012 Virginia Smith  

E-Print Network (OSTI)

, dual stage heat pump air conditioner. To study this setup, we collect data from a residential testbed of Computer Science Social Impact Heating, ventilation, and air conditioning (HVAC) systems are the greatest this research as part of a senior thesis for her computer science degree at the University of Virginia. She

Robins, Gabriel

195

Dual-Reality Objects Randall B. Smith  

E-Print Network (OSTI)

with each IUG. To move dual-reality object A into the virtual world, the IUG notifies the LOM of the RIFD that DROID and that RIFD tag value. Ownership of the object is passed directly from the originating LOM

Redmiles, David F.

196

Ray Smith | Y-12 National Security Complex  

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

new mission (4:10) Jack Case's impact on Y-12 and the world (2:18) Jack Case and the brass outhouse (1:27) Jack Case and the brass outhouse (restated) (1:19) Jack Case's can-do...

197

What's Driving Oil Prices? James L. Smith  

E-Print Network (OSTI)

$60 $80 1970 1975 1980 1985 1990 1995 2000 2005 Real Price ($2005) #12;2 Hubbert's Curve (Peak Oil) PEAK OIL QUIZ Instructions: With books closed and eyes on your own paper, please mark the single best answer. 1. Peak oil production indicates: a) Half gone. b) Running out. c) Starting out. d) None

O'Donnell, Tom

198

Microsoft PowerPoint - Smith.ppt  

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

New Mexico (Path 47) Owners: EPE, PNM, TRI TTC 940 MW Primary Use: Import Palo Verde Nuclear and Four Corners coal power into southern New Mexico 032509 5 East of the River...

199

AUGUST MEMBER NEWS FEATURE: Raymond Smith  

Science Conference Proceedings (OSTI)

Jul 31, 2009 ... While in Alaska, I first lived off the land and prospected for gold. ... I had become interested in solid state physics and ended up as technical...

200

A O Smith | Open Energy Information  

Open Energy Info (EERE)

Solar Product Wisconsin-based based company that makes both water heating equipment and electric motors and also is in the water treatment business. Its water heating focus...

Note: This page contains sample records for the topic "young buz smith" 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

Curriculum Vitae Address: 410 Smith Hall  

E-Print Network (OSTI)

Institute of Technology, Pasadena, CA Advisor: Prof. Alan Barr, Dr. David Breen AWARDS · 2010 Air Force Vision (ICCV 2011) · General Chair, ACM Interactive 3D Graphics (I3D 2013), proposed. Conference Program Committee Member · Interactive 3D Graphics, 2011 · ACM Multimedia, 2010 · IEEE Conference on Computer Vision

Taufer, Michela

202

MASS AND LUMINOSITY EVOLUTION OF YOUNG STELLAR OBJECTS  

SciTech Connect

A model of protostar mass and luminosity evolution in clusters gives new estimates of cluster age, protostar birthrate, accretion rate, and mean accretion time. The model assumes constant protostar birthrate, core-clump accretion, and equally likely accretion stopping. Its parameters are set to reproduce the initial mass function and to match protostar luminosity distributions in nearby star-forming regions. It obtains cluster ages and birthrates from the observed numbers of protostars and pre-main sequence (PMS) stars, and from the modal value of the protostar luminosity. In 31 embedded clusters and complexes, the global cluster age is 1-3 Myr, matching available estimates based on optical spectroscopy (OS) and evolutionary tracks. This method of age estimation is simpler than OS and is more useful for young embedded clusters where optical spectroscopy is not possible. In the youngest clusters, the protostar fraction decreases outward from the densest gas, indicating that the local star-forming age increases outward from a few 0.1 Myr in small protostar-dominated zones to a few Myr in large PMS-dominated zones.

Myers, Philip C., E-mail: pmyers@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-06-10T23:59:59.000Z

203

HUNTING FOR YOUNG DISPERSING STAR CLUSTERS IN IC 2574  

SciTech Connect

Dissolving stellar groups are very difficult to detect using traditional surface photometry techniques. We have developed a method to find and characterize non-compact stellar systems in galaxies where the young stellar population can be spatially resolved. By carrying out photometry on individual stars, we are able to separate the luminous blue stellar population from the star field background. The locations of these stars are used to identify groups by applying the HOP algorithm, which are then characterized using color-magnitude and stellar density radial profiles to estimate age, size, density, and shape. We test the method on Hubble Space Telescope Advanced Camera for Surveys archival images of IC 2574 and find 75 dispersed stellar groups. Of these, 20 highly dispersed groups are good candidates for dissolving systems. We find few compact systems with evidence of dissolution, potentially indicating that star formation in this galaxy occurs mostly in unbound clusters or groups. These systems indicate that the dispersion rate of groups and clusters in IC 2574 is at most 0.45 pc Myr{sup -1}. The location of the groups found with HOP correlate well with H I contour map features. However, they do not coincide with H I holes, suggesting that those holes were not created by star-forming regions.

Pellerin, Anne [Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843-4242 (United States); Meyer, Martin M. [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, CRAWLEY WA 6009 (Australia); Calzetti, Daniella [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Harris, Jason, E-mail: apellerin@mta.ca, E-mail: martin.meyer@uwa.edu.au, E-mail: calzetti@astro.umass.edu, E-mail: jharris@30doradus.org [Illumina, Inc., 25861 Industrial Blvd, Hayward, CA 94545 (United States)

2012-12-01T23:59:59.000Z

204

AFDC Benefits and Nonmarital Births to Young Women  

E-Print Network (OSTI)

Building on recent work by Rosenzweig (1999), this paper re-examines the effect of AFDC benefits on early non-marital childbearing. Unlike most previous work in this area, Rosenzweig finds a statistically significant and quantitatively large positive effect of AFDC benefits. Using data from the Panel Study of Income Dynamics, we replicate Rosenzweigs analysis and explore the reasons his findings differ from earlier research findings. We are able to reproduce his main finding that AFDC generosity influences non-marital childbearing when state and cohort fixed-effects are included. However, we find that model specification matters a great deal. An alternative specification of state fixed-effects yields no evidence of an AFDC effect, and when we focus on fertility only through age 19 (as in prior work), we also find no AFDC effect. This latter finding implies that the behavior of women in their early 20s may be far more sensitive to welfare In this paper, we replicate and extend recent research by Mark Rosenzweig (1999) on the relationship between AFDC benefits and non-marital childbearing by young women. Most previous work on the effects of AFDC benefit levels on a wide range of demographic behaviors, including non-marital childbearing, has found a relatively weak relationship. In some papers, benefits do have a statistically significant effect that is

Saul D. Hoffman; E. Michael Foster; David Neumark; Robert Moffitt; Rebecca Blank; Greg Duncan

2000-01-01T23:59:59.000Z

205

Linear spectropolarimetry of young and other emission line stars  

E-Print Network (OSTI)

The aim of this article is to demonstrate the useful role that can be played by spectropolarimetric observations of young and evolved emission line stars that analyse the linearly polarized component in their spectra. At the time of writing, this demonstration has to be made on the basis of optical data since there is no common-user infrared facility, in operation, that offers the desired combination of spectral resolution and sensitivity. Here we focus on what can be learned from linear spectropolarimetry alone at reasonably high spectral resolution and at $10^3 < $S/N$ < 10^4$. And we remind that the near infrared (1--2 micron) has the potential to out-perform the optical as a domain to work in because of the greatly reduced interstellar obscuration at these wavelengths. This point has been reached at a time when theory, exploiting flexible Monte Carlo methods, is fast becoming a powerful tool. In short we have the complex phenomena, and the rise of the modelling capability to match -- good data are the missing link.

Janet Drew; Jorick Vink; Tim Harries; Ryuichi Kurosawa; Rene Oudmaijer

2004-03-30T23:59:59.000Z

206

Evaluation of 1991-1992 Brood Overwinter-Reared Coho Released from Net Pens in Youngs Bay, Oregon : Final Completion Report Youngs Bay Terminal Fishery Project.  

DOE Green Energy (OSTI)

Funding from Bonneville Power Administration was provided to the Oregon Department of Fish and Wildlife and the Clatsop County Economic Development Council`s Fisheries Project to identify and develop terminal fishing opportunities. The 1991 and 1992 brood fingerling coho from Oregon Department of Fish and Wildlife hatcheries were successfully reared during the winter period to smolt stage in Youngs Bay utilizing floating net pens. Based on coded-wire-tag recoveries during 1991--93 from 2-week net-pen acclimation releases, total accountability of coho adults averaged 40,540 fish, with the Youngs Bay commercial harvest accounting for 39%. With reduced ocean harvest impacts during 1994 and 1995, 92% of 51,640 coho in 1994 and 68% of 23,599 coho in 1995 (based on coded-wire-tag recoveries) were accounted for in the Youngs Bay commercial fishery for combined 2-week and overwinter acclimation net-pen releases. Overwinter net-pen acclimation coho accounted for 35,063 and 15,775 coho adults in 1994 and 1995 with 93% and 68% accountable in the Youngs Bay commercial harvest. Based on coded-wire-tag recoveries, less than 1% of the adults resulting from releases at Youngs Bay net pens strayed to hatcheries, while none were recovered on spawning ground surveys during 1991--95. The highest survival rates were observed for 1991 and 1992 brood overwinter coho released in early May. Time of release, not rearing strategy, appears to be the determining factor affecting survival in Youngs Bay.

Hirose, Paul S.

1997-01-01T23:59:59.000Z

207

238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc  

Open Energy Info (EERE)

238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc 238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: 238U Decay Series Systematics Of Young Lavas From Batur Volcano, Sunda Arc Details Activities (0) Areas (0) Regions (0) Abstract: Activities of 238U decay series radioisotopes have been determined for both postcaldera basalts erupted between 1849 and 1974 and genetically related young precaldera dacites from Batur volcano, Bali, Sunda arc. All rocks possess (230Th/238U) = 1 within 2 sigma error indicating that little, if any, fractionation between Th and U occurred during their genesis, or in their source regions, within approximately the last 350 ka. Both the basaltic and the dacitic rocks possess (230Th/232U) ~

208

Bright Young Minds for a Clean Energy Future | Department of Energy  

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

Young Minds for a Clean Energy Future Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future August 16, 2011 - 12:11pm Addthis Bright Young Minds for a Clean Energy Future Sarah Jane Maxted Special Assistant, Office of Energy Efficiency & Renewable Energy How can I participate? Registration begins August 15 and ends on October 7, 2011. Students are encouraged to register with their teachers by September 30, 2011 to take advantage of the full energy savings period. It's that time again: Back to school season is officially here! Time for students to prepare for the new experiences and challenges that they will encounter throughout the upcoming school year. One such challenge-from the Energy Department in partnership with the National Science Teachers Association (NSTA)-aims to tap into the

209

Effects of acidic water on young-of-the-year smallmouth bass ...  

Science Conference Proceedings (OSTI)

Environmental Biology of Fishes Vol. 21, No. 3, pp. 223-229,1988. 0 Dr W. Junk Publishers, Dordrecht. Effects of acidic water on young-of-the-year smallmouth...

210

Hands to Work: The Practical Artistry of David DeYoung  

Science Conference Proceedings (OSTI)

Jun 4, 2009 ... Based on advice given to him by an architect at Children's Hospital of Pittsburgh, DeYoung devised an open floor plan in the living area that...

211

Molecular and Stellar Disks Galaxies Lisa Young (New Mexico Tech) and Martin Bureau (Oxford)  

E-Print Network (OSTI)

Molecular and Stellar Disks Galaxies Lisa Young (New Mexico Tech) and Martin Bureau (Oxford galaxies contain molecular disks. These internal structures evolution galaxies. to place observational constraints on the formation in early galaxies studying the relationships between embedded disks, molecular

Bureau, Martin

212

Bounded rationality and satisficing in young people's Web-based decision making  

Science Conference Proceedings (OSTI)

This study investigated Simon's behavioral decision-making theories of bounded rationality and satisficing in relation to young people's decision making in the World Wide Web, and considered the role of personal preferences in Web-based decisions. It ...

Denise E. Agosto

2002-01-01T23:59:59.000Z

213

Bright Young Minds for a Clean Energy Future | Department of Energy  

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

Bright Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future Bright Young Minds for a Clean Energy Future August 16, 2011 - 12:11pm Addthis Bright Young Minds for a Clean Energy Future Sarah Jane Maxted Special Assistant, Office of Energy Efficiency & Renewable Energy How can I participate? Registration begins August 15 and ends on October 7, 2011. Students are encouraged to register with their teachers by September 30, 2011 to take advantage of the full energy savings period. It's that time again: Back to school season is officially here! Time for students to prepare for the new experiences and challenges that they will encounter throughout the upcoming school year. One such challenge-from the Energy Department in partnership with the National Science Teachers Association (NSTA)-aims to tap into the

214

What causes the density effect in young forest plantations?  

DOE Green Energy (OSTI)

In young forest plantations, trees planted at high densities frequently show more rapid height and diameter growth than those plants at lower densities. This positive growth response to density (the ''density effect'') often manifests long before seedlings are tall enough to shade one another, so it is not a simple response to shade. The mechanism(s) which trigger and sustain this growth enhancement are unknown. Our objectives were to document the temporal dynamics of positive growth response to increasing density in Douglas-fir plantations and to test two hypotheses as potential mechanisms for this response. The hypotheses are (1) a canopy boundary layer effect, and (2) alterations in the quality of light reflected from neighboring trees. The ''boundary layer'' hypotheses proposes that changes in atmospheric mixing occur in high-density plantations, promoting increased concentrations of CO{sub 2} and H{sub 2}O vapor during early morning hours, which in turn would enhance carbon assimilation. The ''light quality'' hypothesis proposes that the presence of neighbors alters the ratio of red to far red light in the canopy environment. Plant sensors detect this change in light quality, and growth and development is altered in response. We found that boundary layer conductance was higher, as we predicted, in low-density Douglas-fir stands than in high-density stands five years after planting. The changes in boundary conductance were accompanied by higher CO{sub 2} and H{sub 2}O vapor during early morning hours. However, we also found that the primary manifestation of the density effect in Douglas-fir occurs two to four years after planting, and we were not able to measure differences in boundary conductance in different densities at that time. Also, we found no difference in carbon isotope composition of wood cellulose formed in high- vs. low-density stands two to three years after planting. We conclude that although stand density may have a significant impact on boundary layer conductance in young stands, it does not account for the ''density effect''. Our tests of the light quality hypothesis were slowed due to poor plantation establishment in the early phase of this study. In a variable density experiment we detected significant changes in R:FR related to density. Also in that study we measured a significant enhancement of tree height at high density. However, after three years of growth, the study trees did not show significant differences in stem diameter related to density. Experimenters at Weyerhaeuser therefore decided not to harvest the trees at the end of the 3rd growth year, as originally planned. In a 1-year study of seedlings planted in raised beds subjected to different light quality treatments using transparent plastic film, we found that tree height but not diameter increased in response to decreased R:FR. At this point, we conclude that R:FR remains a viable hypothesis for the ''density effect'', but evidence is not conclusive. We expect that continued measurements in the variable density test plot at Weyerhaeuser will add more evidence in the future.

Barbara J. Bond; Gary A. Ritchie

2002-07-21T23:59:59.000Z

215

X-ray chemistry in envelopes around young stellar objects  

E-Print Network (OSTI)

We present chemical models of the envelope of a young stellar object (YSO) exposed to a central X-ray source. The models are applied to the massive star-forming region AFGL 2591 for different X-ray fluxes. The total X-ray ionization rate is dominated by the `secondary' ionization rate of H2 resulting from fast electrons. The carbon, sulphur and nitrogen chemistries are discussed. It is found that He+ and H3+ are enhanced and trigger a peculiar chemistry. Several molecular X-ray tracers are found and compared to tracers of the far ultraviolet (FUV) field. Like ultraviolet radiation fields, X-rays enhance simple hydrides, ions and radicals. In contrast to ultraviolet photons, X-rays can penetrate deep into the envelope and affect the chemistry even at large distances from the source. Whereas the FUV enhanced species cover a region of 200-300 AU, the region enhanced by X-rays is >1000 AU. Best-fit models for AFGL 2591 predict an X-ray luminosity LX > 1e+31 ergs/s with a hard X-ray spectrum TX > 3e+07 K. Furthermore, we find LX/Lbol ~ 1e-6. The chemistry of the bulk of the envelope mass is dominated by cosmic-ray induced reactions rather than by X-ray induced ionization for X-ray luminosities LX < 1e+33 ergs/s. The calculated line intensities of HCO+ and HCS+ show that high-J lines are more affected than lower J lines by the presence of X-rays due to their higher critical densities, and that such differences are detectable even with large aperture single-dish telescopes. Future instruments such as Herschel-HIFI or SOFIA will be able to observe X-ray enhanced hydrides whereas the sensitivity and spatial resolution of ALMA is well-suited to measure the size and geometry of the region affected by X-rays.

P. Staeuber; S. D. Doty; E. F. van Dishoeck; A. O. Benz

2005-06-14T23:59:59.000Z

216

Water destruction by X-rays in young stellar objects  

E-Print Network (OSTI)

We study the H2O chemistry in star-forming environments under the influence of a central X-ray source and a central far ultraviolet (FUV) radiation field. The gas-phase water chemistry is modeled as a function of time, hydrogen density and X-ray flux. To cover a wide range of physical environments, densities between n_H = 10^4-10^9 cm^-3 and temperatures between T = 10-1000 K are studied. Three different regimes are found: For T water abundance is of order 10^-7-10^-6 and can be somewhat enhanced or reduced due to X-rays, depending on time and density. For 100 K 10^-3 ergs s-1 cm^-2 (t = 10^4 yrs) and for F_X > 10^-4 ergs s^-1 cm^-2 (t = 10^5 yrs). At higher temperatures (T > 250 K) and hydrogen densities, water can persist with x(H2O) ~ 10^-4 even for high X-ray fluxes. The X-ray and FUV models are applied to envelopes around low-mass Class 0 and I young stellar objects (YSOs). Water is destroyed in both Class 0 and I envelopes on relatively short timescales (t ~ 5000 yrs) for realistic X-ray fluxes, although the effect is less prominent in Class 0 envelopes due to the higher X-ray absorbing densities there. FUV photons from the central source are not effective in destroying water. The average water abundance in Class I sources for L_X > 10^27 ergs s^-1 is predicted to be x(H2O) < 10^-6.

P. Stauber; J. K. Jorgensen; E. F. van Dishoeck; S. D. Doty; A. O. Benz

2006-02-06T23:59:59.000Z

217

A Survey for Young Spectroscopic Binary K7-M4 Stars in Ophiuchus  

E-Print Network (OSTI)

This paper describes a high-resolution, infrared spectroscopic survey of young, low-mass stars designed to identify and characterize pre-main-sequence spectroscopic binaries. This is the first large infrared radial velocity survey of very young stars to date. The frequency and mass ratio distribution of the closest, low-mass binaries bear directly on models of stellar, brown dwarf, and planetary mass companion formation. Furthermore, spectroscopic binaries can provide mass ratios and ultimately masses, independent of assumptions, needed to calibrate models of young star evolution. I present the initial results from observations of a uniform sample of 33 T Tauri M stars in the Ophiuchus molecular cloud. The average mass of this sample is less than that of other young star radial velocity surveys of similar scope by a factor of ~2. Almost every star was observed at 3-4 epochs over 3 years with the 10 meter Keck II telescope and the facility infrared spectrometer NIRSPEC. An internal precision of 0.43 km/s was obtained with standard cross-correlation calibration techniques. Four of the targets are newly discovered spectroscopic binaries, one of which is located in a sub-arcsecond, hierarchical quadruple system. Three other sub-arcsecond visual binaries were also serendipitously identified during target acquisition. The spectroscopic multiplicity of the sample is comparable to that of earlier type, pre-main-sequence objects. Therefore, there is no dearth of young, low-mass spectroscopic binary stars, at least in the Ophiuchus region.

L. Prato

2006-11-20T23:59:59.000Z

218

AGE AND MASS STUDIES FOR YOUNG STAR CLUSTERS IN M31 FROM SEDS-FIT  

SciTech Connect

In this paper, we present photometry for young star clusters in M31, which are selected from Caldwell et al. These star clusters have been observed as part of the Beijing-Arizona-Taiwan-Connecticut (BATC) Multicolor Sky Survey from 1995 February to 2008 March. The BATC images including these star clusters are taken with 15 intermediate-band filters covering 3000-10000 A. Combined with photometry in the GALEX far- and near-ultraviolet, broadband UBV RI, SDSS ugriz, and infrared JHK{sub s} of Two Micron All Sky Survey, we obtain their accurate spectral energy distributions (SEDs) from 1538 to 20000 A. We derive these star clusters' ages and masses by comparing their SEDs with stellar population synthesis models. Our results are in good agreement with previous determinations. The mean value of age and mass of young clusters (<2 Gyr) is about 385 Myr and 2 Multiplication-Sign 10{sup 4} M{sub Sun }, respectively. There are two distinct peaks in the age distribution, a highest peak at age {approx}60 Myr and a secondary peak around 250 Myr, while the mass distribution shows a single peak around 10{sup 4} M{sub Sun }. A few young star clusters have two-body relaxation times greater than their ages, indicating that those clusters have not been well dynamically relaxed and therefore have not established the thermal equilibrium. There are several regions showing aggregations of young star clusters around the 10 kpc ring and the outer ring, indicating that the distribution of the young star clusters is well correlated with M31's star-forming regions. The young massive star clusters (age {<=}100 Myr and mass {>=}10{sup 4} M{sub Sun }) show apparent concentration around the ring splitting region, suggesting a recent passage of a satellite galaxy (M32) through M31 disk.

Wang Song; Ma Jun; Fan Zhou; Wu Zhenyu; Zhang Tianmeng; Zou Hu; Zhou Xu, E-mail: majun@nao.cas.cn [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)

2012-12-01T23:59:59.000Z

219

Measuring Liquid Volumes in Sub-nanoliter Wells Ian T. Young*1  

E-Print Network (OSTI)

Measuring Liquid Volumes in Sub-nanoliter Wells Ian T. Young*1 , Kari T. Hjelt2 , Richard van den. These wells can serve as bioreactors for studying a variety of biochemical reactions such as the enzymatic of liquid that has been deposited in a given well and/or to monitor the evaporation of the liquid. Using

van Vliet, Lucas J.

220

Texas Tech at TMEA 2013 Clinicians: Janice Killian & John Wayman, Young Harris College  

E-Print Network (OSTI)

Texas Tech at TMEA 2013 ,k9ki9o Clinicians: Janice Killian & John Wayman, Young Harris College Wood The Yin and Yang of Teaching Music Thurs. Feb 14 th 11:00 am ­ Noon / CC 212 Texas Tech Consortium Thurs. Feb 14 th 5:00-6:00 pm / CC 212 Concert: Texas Tech University Symphonic Wind Ensemble Conductor

Rock, Chris

Note: This page contains sample records for the topic "young buz smith" 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

Water harvesting for young trees using Peltier modules powered by photovoltaic solar energy  

Science Conference Proceedings (OSTI)

Young trees transplanted from nursery into open field require a minimum amount of soil moisture to successfully root in their new location, especially in dry-climate areas. One possibility is to obtain the required water from air moisture. This can be ... Keywords: DAQB, Dew condenser, EMF, ETc, Hr, Irrigation, SPV, SPVM, Solar photovoltaic energy, TD, Ta, Tdp, Thermoelectric effect, Ts, Water harvesting

M. A. MuOz-GarcA; G. P. Moreda; M. P. Raga-Arroyo; O. MarN-GonzLez

2013-04-01T23:59:59.000Z

222

Belowground and aboveground biomass in young postfire lodgepole pine forests of contrasting tree  

E-Print Network (OSTI)

Belowground and aboveground biomass in young postfire lodgepole pine forests of contrasting tree as 40% of live biomass in coniferous forests is located belowground, yet the effect of tree density on biomass allocation is poorly understood. We developed allometric equations using traditional harvesting

Turner, Monica G.

223

Homeless young people's experiences with information systems: life and work in a community technology center  

Science Conference Proceedings (OSTI)

This paper explores how homeless young people, aged 13-25, make use of information systems in daily life. Observed in a community technology center, four different examples of uses are described: i) Using digital tools to find employment, ii) Telling ... Keywords: digital media, homelessness, identity, youth

Jill Palzkill Woelfer; David G. Hendry

2010-04-01T23:59:59.000Z

224

We often think about energy in personal terms. People comment on the energy young children  

E-Print Network (OSTI)

Overview We often think about energy in personal terms. People comment on the energy young children seem to possess. Others mention that they don't feel they have enough energy to make it through the day. We've heard that the world is running out of certain types of energy. In spite of all of our everyday

Hardy, Darel

225

Modeling the Young Sun's Solar Wind and its Interaction with Earth's Paleomagnetosphere  

E-Print Network (OSTI)

We present a focused parameter study of solar wind - magnetosphere interaction for the young Sun and Earth, $~3.5$ Ga ago, that relies on magnetohydrodynamic (MHD) simulations for both the solar wind and the magnetosphere. By simulating the quiescent young Sun and its wind we are able to propagate the MHD simulations up to Earth's magnetosphere and obtain a physically realistic solar forcing of it. We assess how sensitive the young solar wind is to changes in the coronal base density, sunspot placement and magnetic field strength, dipole magnetic field strength and the Sun's rotation period. From this analysis we obtain a range of plausible solar wind conditions the paleomagnetosphere may have been subject to. Scaling relationships from the literature suggest that a young Sun would have had a mass flux different from the present Sun. We evaluate how the mass flux changes with the aforementioned factors and determine the importance of this and several other key solar and magnetospheric variables with respect t...

Sterenborg, M Glenn; Drake, Jeremy J; Gombosi, Tamas I; 10.1029/2010JA016036

2011-01-01T23:59:59.000Z

226

Probing the close environment of massive young stars with spectro-astrometry  

E-Print Network (OSTI)

Aims: We test the technique of spectro-astrometry as a potential method to investigate the close environment of massive young stars. Method: Archival VLT near infrared K band spectra (R=8900) of three massive young stellar objects and one Wolf-Rayet star are examined for spectro-astrometric signatures. The young stellar objects display emission lines such as Brackett gamma, CO 2-0 and CO 3-1 that are characteristic of ionised regions and molecular disks respectively. Two of the sample sources also display emission lines such as NIII and MgII that are characteristic of high temperatures. Results: Most of the emission lines show spectro-astrometric signal at various levels resulting in different positional displacements. The shapes and magnitudes of the positional displacements imply the presence of large disk/envelopes in emission and expanding shells of ionised gas. The results obtained for the source 18006-2422nr766 in particular provide larger estimates (> 300AU) on CO emitting regions indicating that in MYSOs CO may arise from inner regions of extended dense envelopes as well. Conclusions: The overall results from this study demonstrate the utility of spectro-astrometry as a potential method to constrain the sizes of various physical entities such as disks/envelopes, UCHII regions and/or ionised shells in the close environment of a massive young star.

J. M. C. Grave; M. S. N. Kumar

2006-12-05T23:59:59.000Z

227

Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site  

Office of Legacy Management (LM)

3-TAC 3-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project January through March 2003 Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site April 2003 Grand Junction Office U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy DE-AC13-02GJ79491 Approved for public release; distribution is unlimited. N0060800 GJO-2003-433-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project Quarterly Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site January through March 2003 April 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107

228

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

Young - Rainey Star Center Young - Rainey Star Center 110406202 Accutest Job Number: F30886 Sampling Date: 04/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

229

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

Young - Rainey Star Center Young - Rainey Star Center 110406202 Accutest Job Number: F35489 Sampling Date: 10/05/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable. Harry Behzadi, Ph.D.

230

S M Stoller Pinellas Environmental Restoration Project - Young- Rainey Star Center  

Office of Legacy Management (LM)

Pinellas Environmental Restoration Project - Young- Rainey Star Center Pinellas Environmental Restoration Project - Young- Rainey Star Center 7030-226 Accutest Job Number: F29125 Sampling Date: 01/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

231

Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainy STAR Center  

Office of Legacy Management (LM)

2-TAC 2-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project January through March 2003 Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center April 2003 Grand Junction Office Grand Junction Office Grand Junction Office U.S. Department of Energy Work Performed Under DOE Contract No. for the U.S. Department of Energy DE-AC13-02GJ79491 Approved for public release; distribution is unlimited. N0060700 GJO-2003-432-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center January through March 2003 April 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491

232

S M Stoller Pinellas Environmental Restoration Project - Young- Rainey Star Center  

Office of Legacy Management (LM)

Pinellas Environmental Restoration Project - Young- Rainey Star Center Pinellas Environmental Restoration Project - Young- Rainey Star Center 110406202 Accutest Job Number: F33039 Sampling Date: 07/06/05 Report to: S M Stoller Cathy.Kelleher@gjo.doe.gov ATTN: Cathy Kelleher Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference and/or state specific certification programs as applicable.

233

First principles study of the Young's modulus of Si <001> nanowires  

DOE Green Energy (OSTI)

We report the results of first-principles calculations of the Young's modulus and other mechanical properties of hydrogen-passivated Si <001> nanowires. The nanowires are taken to have predominantly {l_brace}100{r_brace} surfaces, with small {l_brace}110{r_brace} facets according to the Wulff shape. The Young's modulus, the equilibrium length and the constrained residual stress of a series of prismatic beams of differing sizes is found to have a size dependence that scales like the surface area to volume ratio for all but the smallest beam. The results are compared with two different models (and the results of classical atomistic calculations based on an empirical potential). We discuss the physics of the hydrogen interactions on the surface and the charge density variations within the beam that may account for the discrepancies of the models and the first principles results.

Lee, B; Rudd, R E

2006-07-03T23:59:59.000Z

234

Cooper minima and Young-type interferences in the photoionization of H{sub 2}{sup +}  

SciTech Connect

We present a detailed study of the partial and total cross sections for photon-induced electron emission from H{sub 2}{sup +}. By comparing the results employing exact and approximate, bounded and continuum wave functions, for one- and two-center basis functions, we find the origin and position of the Cooper-like minima in the partial cross sections and their relationship with the Young-type interference pattern.

Della Picca, R. [CONICET and Centro Atomico Bariloche, Comision Nacional de Energia Atomica, Avda E. Bustillo 9500, 8400 Bariloche (Argentina); UPMC Univ. Paris 6, UMR 7614, Laboratoire de Chimie Physique-Matiere et Rayonnement, 11 rue Pierre et Marie Curie, F-75231 Paris Cedex 05 (France); Fainstein, P. D. [CONICET and Centro Atomico Bariloche, Comision Nacional de Energia Atomica, Avda E. Bustillo 9500, 8400 Bariloche (Argentina); Dubois, A. [UPMC Univ. Paris 6, UMR 7614, Laboratoire de Chimie Physique-Matiere et Rayonnement, 11 rue Pierre et Marie Curie, F-75231 Paris Cedex 05 (France); CNRS UMR 7614, LCPMR, F-75005 Paris (France)

2011-09-15T23:59:59.000Z

235

Age distribution of young clusters and field stars in the SMC  

E-Print Network (OSTI)

In this paper we discuss the cluster and field star formation in the central part of the Small Magellanic Cloud. The main goal is to study the correlation between young objects and their interstellar environment. The ages of about 164 associations and 311 clusters younger than 1 Gyr are determined using isochrone fitting. The spatial distribution of the clusters is compared with the HI maps, with the HI velocity dispersion field, with the location of the CO clouds and with the distribution of young field stars. The cluster age distribution supports the idea that clusters formed in the last 1 Gyr of the SMC history in a roughly continuous way with periods of enhancements. The two super-shells 37A and 304A detected in the HI distribution are clearly visible in the age distribution of the clusters: an enhancement in the cluster formation rate has taken place from the epoch of the shell formation. A tight correlation between young clusters and the HI intensity is found. The degree of correlation is decreasing with the age of the clusters. Clusters older than 300 Myr are located away from the HI peaks. Clusters and associations younger than 10 Myr are related to the CO clouds in the SW region of the SMC disk. A positive correlation between the location of the young clusters and the velocity dispersion field of the atomic gas is derived only for the shell 304A, suggesting that the cloud-cloud collision is probably not the most important mechanism of cluster formation. Evidence of gravitational triggered episode due to the most recent close interaction between SMC and LMC is found both in the cluster and field star distribution.

E. Chiosi; A. Vallenari; E. V. Held; L. Rizzi; A. Moretti

2006-04-07T23:59:59.000Z

236

Bayesian analysis to identify very low-mass members of nearby young stellar kinematic groups  

E-Print Network (OSTI)

We describe our all-sky survey for >M4 candidate members to nearby, young associations from the 2MASS and WISE catalogs using bayesian inference. We report the first results, including 38 highly probable candidates showing spectroscopic signs of low-gravity (and thus youth). The latest of these objects would correspond to a 11 - 13 MJup object, around the limit of the planetary regime.

Gagn, Jonathan; Doyon, Ren; Malo, Lison; Faherty, Jacqueline; Artigau, tienne

2013-01-01T23:59:59.000Z

237

Hubble Space Telescope Imaging of the Young Planetary Nebula GL 618  

E-Print Network (OSTI)

We present narrow-band Hubble Space Telescope images of the young planetary nebula GL 618. These images have allowed us to study the detailed morphology of shock-excited emission present in the bipolar lobes of this object. These images reveal the presence of three highly collimated outflows emanating from the central regions of GL 618. We discuss the significance of the detection of these outflows and the possible origins of these features.

Susan R. Trammell

2000-01-10T23:59:59.000Z

238

Probing the close environment of massive young stars with spectro-astrometry  

E-Print Network (OSTI)

Aims: We test the technique of spectro-astrometry as a potential method to investigate the close environment of massive young stars. Method: Archival VLT near infrared K band spectra (R=8900) of three massive young stellar objects and one Wolf-Rayet star are examined for spectro-astrometric signatures. The young stellar objects display emission lines such as Brackett gamma, CO 2-0 and CO 3-1 that are characteristic of ionised regions and molecular disks respectively. Two of the sample sources also display emission lines such as NIII and MgII that are characteristic of high temperatures. Results: Most of the emission lines show spectro-astrometric signal at various levels resulting in different positional displacements. The shapes and magnitudes of the positional displacements imply the presence of large disk/envelopes in emission and expanding shells of ionised gas. The results obtained for the source 18006-2422nr766 in particular provide larger estimates (> 300AU) on CO emitting regions indicating that in MY...

Grave, J M C

2006-01-01T23:59:59.000Z

239

Moving the Goalposts: The Impact of Soccer on the Lives and Prospects of Girls and Young Women Rural Kenya  

E-Print Network (OSTI)

2004). Seventh lowest out of 69 districts in Kenya UNDP (2005) Fourth Kenya Human Development Report 2 MTGK (2005) 'Girls and Young Women in Rural Kenya Sarah Forde and Andrea

Forde, Sarah; Kendall-Taylor, Andrea

2007-01-01T23:59:59.000Z

240

Modulatory effects of levodopa on cognitive control in young but not in older subjects: A pharmacological fmri study  

Science Conference Proceedings (OSTI)

Older individuals show decline of prefrontal cortex (PFC) functions which may be related to altered dopaminergic neurotransmission. We investigated the effects of aging and dopaminergic stimulation in 15 young and 13 older healthy subjects on the neural ...

zgr A. Onur; Martina Piefke; Chuh-Hyoun Lie; Christiane M. Thiel; Gereon R. Fink

2011-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

"Young Town" growing up : four decades later : self-help housing and upgrading lessons from a squatter neighborhood in Lima  

E-Print Network (OSTI)

This thesis examines self-help housing policies in Peru by revisiting Independencia, one of Lima's young towns (squatter settlements), forty-five years after its founding. The study was designed to better understand how ...

Williams, Susana M. (Susana Maria)

2005-01-01T23:59:59.000Z

242

Young Scientist  

Science Conference Proceedings (OSTI)

Mar 14, 2012... Schmidt1; Mathis Ruppert1; Patrick Kndler1; Heinz Werner Hppel1; Mathias Gken1; 1Friedrich-Alexander-Universitt Erlangen-Nrnberg

243

Young Scientist  

Science Conference Proceedings (OSTI)

Feb 17, 2010 ... Unconventional ECAE Processing of Magnesium Alloys: David Foley1; Majid ... An examination of conventional and unconventional ECAE...

244

Scott Young  

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

Engineering, University of Toronto 2003, M.Sc. Biosystems Engineering, University of Manitoba 2000, B.Sc. Biosystems Engineering, University of Manitoba Vision & Mission...

245

Detection of steam in the circumstellar disk around a massive Young Stellar Object  

E-Print Network (OSTI)

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the infrared spectrometer ISAAC mounted on the VLT-ANTU. The water vapor is at a mean temperature of 1565+/-510 K, cooler than the hot CO found in the same object, which is at 1660K and the column density is N(H2O)=(2.5 +/- 0.4)x1E18 cm-2. The profile of both H2O and CO lines is best reproduced by the emission from a Keplerian disk. To interpret the data, we also investigate the formation of molecules and especially CO and water vapor in the inner hot and dense part of disks around young high mass stars using a pseudo time-dependent gas-phase chemical model. Molecules are rapidly photodissociated but this destruction is compensated by an efficient formation due to fast neutral-neutral reactions. The ability of CO molecules to self-shield significantly enhances its abundance. Water molecules are sufficiently abundant to be detectable. The observed H2O/CO ratio is reproduced by gas at 1600K and an enhanced UV field over gas density ratio I_UV/nH=1E(-4)- 1E(-6). The simulations support the presence of CO and H2O molecules in the inner disks around young massive stars despite the strong UV radiation and show that the OH radical plays an essential role in hot gas chemistry.

W. -F. Thi; A. Bik

2005-03-24T23:59:59.000Z

246

Quarterly Progress Report for the Young-Rainey STAR Center's 4.5 Acre Site  

Office of Legacy Management (LM)

600 600 GJO-2003-410-TAC GJO-PIN 25.5.1 Pinellas Environmental Restoration Project Quarterly Progress Report for the Young - Rainey STAR Center's 4.5 Acre Site October through December 2002 January 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0057600 Contents DOE/Grand Junction Office 4.5 Acre Site Quarterly Progress Report January 2003 Page iii Contents Acronyms and Abbreviations ..........................................................................................................v 1.0 Introduction ............................................................................................................................1

247

Passive solar water heating: breadbox design for the Fred Young Farm Labor Center in Indio  

SciTech Connect

An appropriate passive solar preheater for multifamily housing units in the Fred Young Farm Labor Center in Indio, California, was designed and analyzed. A brief summary of passive preheater systems and the key design features used in current designs is presented. The design features necessary for the site requirements are described. The eight preliminary preheater designs reviewed for the project are presented. The results of thermal performance simulation for the eight prototype systems are discussed. Alternative monitoring systems for the installation are described and evaluated. The consultants' recommendations, working drawings, and performance estimates of the system selected are presented. (MHR)

Melzer, B; Maeda, B

1979-10-01T23:59:59.000Z

248

The effects of stellar dynamics on the evolution of young dense stellar systems  

E-Print Network (OSTI)

In the present paper we report on first results of a project in Brussels where we study the effects of stellar dynamics on the evolution of young dense stellar systems using the 3 decades expertise in massive star evolution and our population (number and spectral) synthesis code. We highlight an unconventionally formed object scenario (UFO-scenario) for Wolf Rayet binaries and study the effects of a luminous blue variable-type instability wind mass loss formalism on the formation of intermediate mass black holes.

Belkus, H; Vanbeveren, D

2004-01-01T23:59:59.000Z

249

The effects of stellar dynamics on the evolution of young dense stellar systems  

E-Print Network (OSTI)

In the present paper we report on first results of a project in Brussels where we study the effects of stellar dynamics on the evolution of young dense stellar systems using the 3 decades expertise in massive star evolution and our population (number and spectral) synthesis code. We highlight an unconventionally formed object scenario (UFO-scenario) for Wolf Rayet binaries and study the effects of a luminous blue variable-type instability wind mass loss formalism on the formation of intermediate mass black holes.

H. Belkus; J. Van Bever; D. Vanbeveren

2004-10-21T23:59:59.000Z

250

A COMPREHENSIVE GALEX ULTRAVIOLET CATALOG OF STAR CLUSTERS IN M31 AND A STUDY OF THE YOUNG CLUSTERS  

Science Conference Proceedings (OSTI)

We present a comprehensive catalog of 700 confirmed star clusters in the field of M31 compiled from three major existing catalogs. We detect 418 and 257 star clusters in Galaxy Evolution Explorer near-ultraviolet and far-ultraviolet (FUV) imaging, respectively. Our final catalog includes photometry of star clusters in up to 16 passbands ranging from FUV to NIR as well as ancillary information such as reddening, metallicity, and radial velocities. In particular, this is the most extensive and updated catalog of UV-integrated photometry for M31 star clusters. Ages and masses of star clusters are derived by fitting the multi-band photometry with model spectral energy distribution (SED); UV photometry enables more accurate age estimation of young clusters. Our catalog includes 182 young clusters with ages less than 1 Gyr. Our estimated ages and masses of young clusters are in good agreement with previously determined values in the literature. The mean age and mass of young clusters are about 300 Myr and 10{sup 4} M{sub Sun }, respectively. We found that the compiled [Fe/H] values of young clusters included in our catalog are systematically lower (by more than 1 dex) than those from recent high-quality spectroscopic data and our SED-fitting result. We confirm that most of the young clusters' kinematics shows systematic rotation around the minor axis and association with the thin disk of M31. The young cluster distribution exhibits a distinct peak in the M31 disk around 10-12 kpc from the center and follows a spatial distributions similar to other tracers of disk structure such as OB stars, UV star-forming regions, and dust. Some young clusters also show concentration around the ring splitting regions found in the southern part of the M31 disk and most of them have systematically younger (star formation ring structure in the M31 disk. Consequently, we suggest that various properties of young clusters in M31 might be in line with the scenarios that a satellite galaxy had passed through the disk of M31 less than few hundred million years ago.

Kang, Yongbeom; Rey, Soo-Chang; Lee, Kyungsook; Kim, YoungKwang [Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764 (Korea, Republic of); Bianchi, Luciana [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Sohn, Sangmo Tony, E-mail: ybkang@cnu.ac.kr, E-mail: screy@cnu.ac.kr [Space Telescope Science Institute, Baltimore, MD 21218 (United States)

2012-04-01T23:59:59.000Z

251

ORIGINAL ARTICLE Low Motor Assessment: A Comparative Pilot Study with Young Children With and Without Motor  

E-Print Network (OSTI)

# The Author(s) 2009. This article is published with open access at Springerlink.com Abstract Most of the developmental instruments that measure cognitive development in children rely heavily on fine motor skills, especially for young children whose language skills are not yet well developed. This is problematic when evaluating the cognitive development of young children with motor impairment. The purpose of this study is to assess the need for a Low Motor adapation of a standardized instrument when testing children with motor impairment. To accomplish this, we have adapted the procedures, item instructions and play material of a widely used and standardized instrument, the Bayley Scales of Infant Development-Second Edition (BSID-II, Bayley 1993). The Original and the Low Motor versions were administered to 20 children experiencing typical development and 19 children with motor impairment within a period of two weeks. Results showed that children with motor impairments scored significantly higher on the Low Motor version of the Bayley Mental Scale than on the Original version: a difference of between 5 and 10 points when the score is expressed in terms of a developmental index score. Results from children with typical development support the assumption that item content and difficulty remain unchanged in the Low Motor version.

J Dev Phys Disabil; Selma Anne; Jos Ruiter; Han Nakken; Bieuwe F. Van Der Meulen; Carolien B. Lunenborg

2009-01-01T23:59:59.000Z

252

RADIO DETECTION OF GREEN PEAS: IMPLICATIONS FOR MAGNETIC FIELDS IN YOUNG GALAXIES  

Science Conference Proceedings (OSTI)

Green Peas are a new class of young, emission line galaxies that were discovered by citizen volunteers in the Galaxy Zoo project. Their low stellar mass, low metallicity, and very high star formation rates make Green Peas the nearby (z {approx} 0.2) analogs of the Lyman break galaxies which account for the bulk of the star formation in the early universe (z {approx} 2-5). They thus provide accessible laboratories in the nearby universe for understanding star formation, supernova feedback, particle acceleration, and magnetic field amplification in early galaxies. We report the first direct radio detection of Green Peas with low frequency Giant Metrewave Radio Telescope observations and our stacking detection with archival Very Large Array FIRST data. We show that the radio emission implies that these extremely young galaxies already have magnetic fields ({approx}> 30 {mu}G) even larger than that of the Milky Way. This is at odds with the present understanding of magnetic field growth based on amplification of seed fields by dynamo action over a galaxy's lifetime. Our observations strongly favor models with pregalactic magnetic fields at {mu}G levels.

Chakraborti, Sayan; Yadav, Naveen; Ray, Alak [Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai 400005 (India); Cardamone, Carolin, E-mail: sayan@tifr.res.in [Massachusetts Institute of Technology, 77 Massachusetts Avenue, Bldg. 26-331, Cambridge, MA 02139 (United States)

2012-02-10T23:59:59.000Z

253

Warm Gas in the Inner Disks around Young Intermediate Mass Stars  

E-Print Network (OSTI)

The characterization of gas in the inner disks around young stars is of particular interest because of its connection to planet formation. In order to study the gas in inner disks, we have obtained high-resolution K-band and M-band spectroscopy of 14 intermediate mass young stars. In sources that have optically thick inner disks, i.e. E(K-L)>1, our detection rate of the ro-vibrational CO transitions is 100% and the gas is thermally excited. Of the five sources that do not have optically thick inner disks, we only detect the ro-vibrational CO transitions from HD 141569. In this case, we show that the gas is excited by UV fluorescence and that the inner disk is devoid of gas and dust. We discuss the plausibility of the various scenarios for forming this inner hole. Our modeling of the UV fluoresced gas suggests an additional method by which to search for and/or place stringent limits on gas in dust depleted regions in disks around Herbig Ae/Be stars.

Sean Brittain; Theodore Simon; Joan Najita; Terrence Rettig

2006-12-08T23:59:59.000Z

254

Detection of steam in the circumstellar disk around a massive Young Stellar Object  

E-Print Network (OSTI)

We report on the observation of hot water vapor (steam) in the inner AU of a young massive star located in the star-forming region IRAS 08576-4334. The water lines are detected in a medium resolution (R=10,000) K-band spectrum taken by the infrared spectrometer ISAAC mounted on the VLT-ANTU. The water vapor is at a mean temperature of 1565+/-510 K, cooler than the hot CO found in the same object, which is at 1660K and the column density is N(H2O)=(2.5 +/- 0.4)x1E18 cm-2. The profile of both H2O and CO lines is best reproduced by the emission from a Keplerian disk. To interpret the data, we also investigate the formation of molecules and especially CO and water vapor in the inner hot and dense part of disks around young high mass stars using a pseudo time-dependent gas-phase chemical model. Molecules are rapidly photodissociated but this destruction is compensated by an efficient formation due to fast neutral-neutral reactions. The ability of CO molecules to self-shield significantly enhances its abundance. Wa...

Thi, W F

2005-01-01T23:59:59.000Z

255

A PAN-CARINA YOUNG STELLAR OBJECT CATALOG: INTERMEDIATE-MASS YOUNG STELLAR OBJECTS IN THE CARINA NEBULA IDENTIFIED VIA MID-INFRARED EXCESS EMISSION  

Science Conference Proceedings (OSTI)

We present a catalog of 1439 young stellar objects (YSOs) spanning the 1.42 deg{sup 2} field surveyed by the Chandra Carina Complex Project (CCCP), which includes the major ionizing clusters and the most active sites of ongoing star formation within the Great Nebula in Carina. Candidate YSOs were identified via infrared (IR) excess emission from dusty circumstellar disks and envelopes, using data from the Spitzer Space Telescope (the Vela-Carina survey) and the Two-Micron All Sky Survey. We model the 1-24 {mu}m IR spectral energy distributions of the YSOs to constrain physical properties. Our Pan-Carina YSO Catalog (PCYC) is dominated by intermediate-mass (2 M{sub sun} 2 x 10{sup 4} YSOs and a present-day star formation rate (SFR) of >0.008 M{sub sun} yr{sup -1}. The global SFR in the Carina Nebula, averaged over the past {approx}5 Myr, has been approximately constant.

Povich, Matthew S.; Getman, Konstantin V.; Townsley, Leisa K.; Broos, Patrick S. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Smith, Nathan [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Majewski, Steven R.; Indebetouw, Remy [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904-4325 (United States); Babler, Brian L.; Meade, Marilyn R.; Whitney, Barbara A. [Department of Astronomy, University of Wisconsin, 475 N. Charter Street, Madison, WI 53706 (United States); Robitaille, Thomas P. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Stassun, Keivan G. [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Yonekura, Yoshinori [Department of Physical Science, Osaka Prefecture University, 1-1 Gakuen-cho, Sakai, Osaka 599-8531 (Japan); Fukui, Yasuo, E-mail: povich@astro.psu.edu [Department of Astrophysics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 (Japan)

2011-05-01T23:59:59.000Z

256

Distribution Network Development (DND)  

Science Conference Proceedings (OSTI)

... Eli Lilly and Company 40. EMC2 41. Epic Games 42. Ernst & Young 43. ExxonMobil * 44. Facebook 45. Fluor 46. GE 47. GlaxoSmithKline 48. ...

2012-05-07T23:59:59.000Z

257

1  

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

Over the ARM CART Area from GOES Data P. Minnis, W. L. Smith, Jr., D. F. Young, and L. Nguyen Atmospheric Sciences National Aeronautics and Space Administration Langley Research...

258

1  

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

Multi-Resolution Imager Data to Account for Partially Cloud-Filled Pixels L. Nguyen, P. Minnis, D. V. Young, and W. L. Smith Jr. Atmospheric Sciences National Aeronautics Space...

259

ARM - Publications: Science Team Meeting Documents  

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

M.W. An Overview of ARM Satellite Cloud and Radiation Budget Datasets* Minnis, P., Nguyen, L., Smith Jr., W.L., Doelling, D.R., Heck, P.W., Khaiyer, M.M., Palikonda, R., Young,...

260

S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center  

Office of Legacy Management (LM)

6/06 6/06 Technical Report for S M Stoller Pinellas Environmental Restoration Project - Young - Rainey Star Center 110406202 Accutest Job Number: F43553 Sampling Date: 09/07/06 Report to: U.S. Dept of Energy, Grand Jct Office 2597 B 3/4 Road Grand Juction, CO 81503 ATTN: Contracts Department, PO# 24231 x Total number of pages in report: Certifications: FL (DOH E83510), NC (573), NJ (FL002), MA (FL946), IA (366), LA (03051), KS (E-10327), SC, AK This report shall not be reproduced, except in its entirety, without the written approval of Accutest Laboratories. Southeast * 4405 Vineland Road * Suite C-15 * Orlando, FL 32811 * tel: 407-425-6700 * fax: 407-425-0707 * http://www.accutest.com Test results contained within this data package meet the requirements of the National Environmental Laboratory Accreditation Conference

Note: This page contains sample records for the topic "young buz smith" 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

X-ray Chemistry in the Envelopes around Young Stellar Objects  

E-Print Network (OSTI)

We have studied the influence of X-rays from a massive young stellar object (YSO) on the chemistry of its own envelope by extending the models of Doty et al. (2002) and Staeuber et al. (2004). The models are applied to the massive star-forming region AFGL 2591 for different X-ray luminosities and plasma temperatures. Enhanced column densities for several species are predicted. In addition we present first detections of CO+ and SO+ toward AFGL 2591. These molecular ions are believed to be high-energy tracers. Herschel-HIFI will be able to observe other tracers like CH and CH+ whereas ALMA is well suited to measure the size and geometry of the emitting region.

P. Staeuber; A. O. Benz; S. D. Doty; E. F. van Dishoeck

2004-12-13T23:59:59.000Z

262

"I'm not perfect": an analysis of the narratives of young women's body image  

E-Print Network (OSTI)

Previous research has explored the influence of media on the development of feminine body image. Additional research has examined the influence of interpersonal relationships such as family and friends on body image. No research has yet examine the ways in which these factors are related and the effect they have on one another. This thesis examines the ways in which young women who are all members of the same sorority discuss their body image with one another, the stories that they tell about developing their own body image, and the factors that they find most influential to their body image. The girls speak about their body image in relation to mediated images; food, exercise, and diet; and clothing. The stories that they tell about developing body image either include the influence of friends and family or the influence of a particular activity that changes their body image. Finally, the girls' body image is most influenced by external situations such as interactions with others.

Dummer, Susan Ilene

2002-01-01T23:59:59.000Z

263

HST/NICMOS Imaging of Disks and Envelopes Around Very Young Stars  

E-Print Network (OSTI)

We present HST/NICMOS observations with 0.1" (15 AU) resolution of six young stellar objects in the Taurus star-formation region. The targets of our survey are three Class I IRAS sources (IRAS 04016+2610, IRAS 04248+2612, and IRAS 04302+2247) and three low-luminosity stars (DG Tau B, Haro 6-5B, and CoKu Tau/1) associated with Herbig Haro jets. The broad-band images show that the near-infrared radiation from these sources is dominated by light scattered from dusty circumstellar material distributed in a region 10 - 15 times the size of our solar system. Although the detailed morphologies of the individual objects are unique, the observed young stellar objects share common features. All of the circumstellar reflection nebulae are crossed by dark lanes from 500 - 900 AU in extent and from less than 50 to 350 AU in apparent thickness. The absorption lanes extend perpendicular to known optical and millimeter outflows in these sources. We interpret the dark lanes as optically thick circumstellar disks seen in silhouette against bright reflection nebulosity. The bipolar reflection nebulae extending perpendicular to the dust lanes appear to be produced by scattering from the upper and lower surfaces of the disks and from dusty material within or on the walls of the outflow cavities. Out of five objects in which the central source is directly detected, two are found to be subarcsecond binaries. This mini-survey is the highest resolution near-infrared study to date of circumstellar environments around solar-type stars with age <= 1 Myr.

Deborah L. Padgett; Wolfgang Brandner; Karl R. Stapelfeldt; Stephen E. Strom; Susan Terebey; David Koerner

1999-02-06T23:59:59.000Z

264

A CORRELATION BETWEEN SURFACE DENSITIES OF YOUNG STELLAR OBJECTS AND GAS IN EIGHT NEARBY MOLECULAR CLOUDS  

SciTech Connect

We report the discovery and characterization of a power-law correlation between the local surface densities of Spitzer-identified, dusty young stellar objects (YSOs) and the column density of gas (as traced by near-IR extinction) in eight molecular clouds within 1 kpc and with 100 or more known YSOs. This correlation, which appears in data smoothed over size scales of {approx}1 pc, varies in quality from cloud to cloud; those clouds with tight correlations, MonR2 and Ophiuchus, are fit with power laws of slope 2.67 and 1.87, respectively. The spread in the correlation is attributed primarily to local gas disruption by stars that formed there or to the presence of very young subregions at the onset of star formation. We explore the ratio of the number of Class II to Class I sources, a proxy for the star formation age of a region, as a function of gas column density; this analysis reveals a declining Class II to Class I ratio with increasing column density. We show that the observed star-gas correlation is consistent with a star formation law where the star formation rate per area varies with the gas column density squared. We also propose a simple picture of thermal fragmentation of dense gas in an isothermal, self-gravitating layer as an explanation for the power law. Finally, we briefly compare the star-gas correlation and its implied star formation law with other recent proposed of star formation laws at similar and larger size scales from nearby star-forming regions.

Gutermuth, R. A. [Five College Astronomy Department, Smith College, Northampton, MA 01063 (United States); Pipher, J. L. [Department of Physics and Astronomy, University of Rochester, Rochester, NY (United States); Megeath, S. T.; Allen, T. S. [Department of Physics and Astronomy, University of Toledo, Toledo, OH (United States); Myers, P. C. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Allen, L. E. [National Optical Astronomy Observatories, Tucson, AZ (United States)

2011-10-01T23:59:59.000Z

265

TAYouKi: A Sketch-Based Tutoring System for Young Kids  

E-Print Network (OSTI)

Intelligent tutoring systems (ITS) have proven to be effective tools for aiding in the instruction of new skills for young kids; however, interaction methods that employ traditional input devices such as the keyboard and mouse may present barriers to children who have yet learned how to write. Existing applications which utilize pen-input devices better mimic the physical act of writing, but few provide useful feedback to the users. This thesis presents a system specifically designed to serve as a useful tool in teaching children how to draw basic shapes, and helping them develop basic drawing and writing skills. The system uses a combination of sketch recognition techniques to interpret the handwritten strokes from sketches of the children, and then provides intelligent feedback based on what they draw. Our approach provides a virtual coach to assist teachers teaching the critical skills of drawing and handwriting. We do so by guiding children through a set of exercises of increasing complexity according to their progress, and at the same time keeping track of students' performance and engagement, giving them differentiated instruction and feedback. Our system would be like a virtual Teaching Assistant for Young Kids, hence we call it TAYouKi. We collected over five hundred hand-drawn shapes from grownups that had a clear understanding of what a particular geometric shape should look like. We used this data to test the recognition of our system. Following, we conducted a series of case studies with children in age group three to six to test the interactivity efficacy of the system. The studies served to gain important insights regarding the research challenges in different domains. Results suggest that our approach is appealable and engaging to children and can help in more effectively teach them how to draw and write.

Vides Ceron, Francisco

2012-08-01T23:59:59.000Z

266

Effect of synthetic ANP on renal and loop of Henle functions in the young rat  

SciTech Connect

The present studies were undertaken to determine, by recollection micropuncture, the effect of a synthetic atrial natriuretic peptide (ANP) on the absolute and fractional deliveries of water and sodium to the juxtamedullary end-descending limb. Two groups of young female Munich-Wistar rats were studied: 1) control received the vehicle only; and 2) ANP received a prime followed by the constant infusion of a synthetic rat atrial peptide (28 amino acids). With the infusion of ANP, clearance of p-( UC)aminohippurate (( UC(PAH) and glomerular filtration rate (GFR) fell significantly. Despite this fall in GFR and renal plasma flow, ANP produced a 2-fold increase in urine volume and a 10-fold increase in sodium excretion. Absolute and fractional sodium deliveries to the end-descending limb increased by approx.30% in the ANP group, whereas mean juxtamedullary single-nephron glomerular filtration rate (SNGFR) remained stable. In three additional rats prepared for micropuncture of the superficial end-accessible proximal tubule, ANP reduced cortical SNGFR by approx.15%. By contrast, GFR did not decline in response to ANP in larger rats, when treated identically. The authors conclude that 1) in young rats ANP can produce a natriuresis in the absence of a rise in GFR; 2) the fall in GFR observed following ANP is due presumably to the immaturity of the animals used in these studies; and 3) ANP produces a rise in absolute and fractional water and sodium deliveries to the end-descending limb that cannot be attributed to a change in SNGFR. The relatively small rise in fractional sodium delivery to the end-descending limb, most probably due to inhibition of sodium and water reabsorption in the juxtamedullary proximal tubule and/or thin descending limb, accounts for only a smallproportion of sodium excretion in the final urine.

Roy, D.R.

1986-08-01T23:59:59.000Z

267

CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters  

E-Print Network (OSTI)

We present CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters namely NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2006, SL 538, NGC 2011, NGC 2098 and NGC 2136. The BVRI data reaching down to V ~ 21 mag, are collected from 3.5-meter NTT/EFOSC2 in sub-arcsec seeing conditions. For NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2011 and NGC 2136, broad band photometric CCD data are presented for the first time. Seven of the 9 clusters have ages between 16 to 25 Myr while remaining two clusters have ages $32\\pm4$ Myr (NGC 2098) and $90\\pm10$ Myr (NGC 2136). For 7 younger clusters, the age estimates based on a recent model and the integrated spectra are found to be systematically lower ($\\sim$ 10 Myr) from the present estimate. In the mass range of $\\sim 2 - 12$ $M_{\\odot}$, the MF slopes for 8 out of nine clusters were found to be similar with the value of $\\gamma$ ranging from $-1.90\\pm0.16$ to $-2.28\\pm0.21$. For NGC 1767 it is flatter with $\\gamma = -1.23\\pm0.27$. Mass segregation effects are observed for NGC 2002, NGC 2006, NGC 2136 and NGC 2098. This is consistent with the findings of Kontizas et al. for NGC 2098. Presence of mass segregation in these clusters could be an imprint of star formation process as their ages are significantly smaller than their dynamical evolution time. Mean MF slope of $\\gamma = -2.22\\pm0.16$ derived for a sample of 25 young ($\\le 100$ Myr) dynamically unevolved LMC stellar systems provide support for the universality of IMF in the intermediate mass range $\\sim 2-12 M_{\\odot}$.

B. Kumar; R. Sagar; J. Melnick

2008-01-07T23:59:59.000Z

268

Comprehensive tables giving physical data and thermal energy estimates for young igneous systems of the United States  

DOE Green Energy (OSTI)

Two tables are presented. The first is a comprehensive table of 157 young igneous systems in the western United States, giving locations, physical data, and thermal energy estimates, where appropriate for each system. The second table is a list of basaltic fields probably less than 10,000 years old in the western United States.

Smith, R.L.; Shaw, H.R.; Leudke, R.G.; Russell, S.L.

1978-01-01T23:59:59.000Z

269

Nonlinear Dynamics in an OLG Growth Model with Young and Old Age Labour Supply: The Role of Public Health Expenditure  

Science Conference Proceedings (OSTI)

This study analyses the dynamics of a two-dimensional overlapping generations economy with young and old age labour supply. We show that the public provision of investments in health, which, in turn, affects the demand for material consumption of the ... Keywords: C62, C68, Chaos, I18, J22, Labour supply, O41, OLG model, Public health expenditure

Luca Gori; Mauro Sodini

2011-10-01T23:59:59.000Z

270

COMPARISON OF CONVECTIVE OVERSHOOTING MODELS AND THEIR IMPACT ON ABUNDANCES FROM INTEGRATED LIGHT SPECTROSCOPY OF YOUNG (<3 Gyr) STAR CLUSTERS  

Science Conference Proceedings (OSTI)

As part of an ongoing program to measure detailed chemical abundances in nearby galaxies, we use a sample of young- to intermediate-age clusters in the Large Magellanic Cloud with ages of 10 Myr-2 Gyr to evaluate the effect of isochrone parameters, specifically core convective overshooting, on Fe abundance results from high-resolution, integrated light spectroscopy. In this work we also obtain fiducial Fe abundances from high-resolution spectroscopy of the cluster individual member stars. We compare the Fe abundance results for the individual stars to the results from isochrones and integrated light spectroscopy to determine whether isochrones with convective overshooting should be used in our integrated light analysis of young- to intermediate-age (10 Myr-3 Gyr) star clusters. We find that when using the isochrones from the Teramo group, we obtain more accurate results for young- and intermediate-age clusters over the entire age range when using isochrones without convective overshooting. While convective overshooting is not the only uncertain aspect of stellar evolution, it is one of the most readily parameterized ingredients in stellar evolution models, and thus important to evaluate for the specific models used in our integrated light analysis. This work demonstrates that our method for integrated light spectroscopy of star clusters can provide unique tests for future constraints on stellar evolution models of young- and intermediate-age clusters.

Colucci, Janet E.; Bernstein, Rebecca A., E-mail: jcolucci@ucolick.org, E-mail: rab@ucolick.org [Department of Astronomy and Astrophysics, 1156 High Street, UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States)

2012-04-20T23:59:59.000Z

271

An Underwater Communication and Sensing Testbed in Marina del Rey Andrew Goodney, Young H. Cho, John Heidemann, John Wroclawski  

E-Print Network (OSTI)

An Underwater Communication and Sensing Testbed in Marina del Rey Andrew Goodney, Young H. Cho, and communication underwater is increasingly important to scientists who study the oceans, rivers, and lakes, as government and industry seek to observe, protect, exploit, and control resources underwater. With growing

Heidemann, John

272

Smith Village, Oklahoma: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

4508947°, -97.4572591° 4508947°, -97.4572591° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":35.4508947,"lon":-97.4572591,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

273

Smith County, Kansas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

9°, -98.7481167° 9°, -98.7481167° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":39.7333849,"lon":-98.7481167,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

274

Smith County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

95.3102505° 95.3102505° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.3352505,"lon":-95.3102505,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

275

Smith County, Tennessee: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

°, -85.971322° °, -85.971322° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.2388468,"lon":-85.971322,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

276

Smith County, Mississippi: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

9.4742177° 9.4742177° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":32.0826588,"lon":-89.4742177,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

277

Deaf Smith County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

5.0017354°, -102.5298028° 5.0017354°, -102.5298028° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":35.0017354,"lon":-102.5298028,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

278

Modeling and Reasoning about Everyday Events Dustin Arthur Smith  

E-Print Network (OSTI)

that is inexpensive (and what price is "expensive"?).For example, the way one travels to an event (e.g., taxi, foot already filled in, or searching for alternative restaurants in the expected neigh- borhood and price range- ing context aware assistance, us- ing information from the calen- dar program and the cellphone (e

279

experiment actually sees," Smith says. "When we were  

E-Print Network (OSTI)

,200 pieces of music from record companies and various artists, and that number is still growing. "As more of ceremonies for a number of nationally known gospel artists' concerts and have produced a CD titled Thank You components. The students' main robot features customized parts made with a titanium powder manufacturing

280

The Structure of Peirce-Smith Converting Schedules  

Science Conference Proceedings (OSTI)

Transfer and Consumption of Oxygen in Gold-bearing Sulfide Ores: Agnico-eagle Mines Trials Tundish Process Performance Improvement: Some Indian Case...

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


281

Presenter: Shawn Carson Principal Investigator: Stephen F. Smith ...  

Presentation_namefor the U.S. Department of Energy ... Very low power consumption ... Production Chips Partnership(s)

282

Takeeda Smith | U.S. DOE Office of Science (SC)  

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

Programs U.S. Department of Energy SC-2Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 F: (202) 586-4120 E: sc.science@science.doe.gov...

283

Formal development of self-organising systems Graeme Smith1  

E-Print Network (OSTI)

, the gradients, avoiding collisions, and so on. However it does not add to our understanding of atomic

Smith, Graeme

284

Sensor validation with machine learning Matt Smith1  

E-Print Network (OSTI)

. Sensors are used in buildings to analyze variables affecting energy use and efficiency. Given our reliance from five of the sensors of one house: (1) outside temperature, (2) outside humidity, (3) refrigerator energy, (4) heat pump water flow, (5) and heat pump liquid line pressure.These are called our target

Wang, Xiaorui "Ray"

285

an interview with Richard Alba Extraordinary Lives: Patti Smith  

E-Print Network (OSTI)

luxurious dress." This view is corroborated in lit- erature and in real-life examples. In Shakespeare

Dennehy, John

286

2010 DOE National Science Bowl Photos - Smith Middle School...  

Office of Science (SC) Website

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

287

Ants (Formicidae): Models for Social Complexity Chris R. Smith,1  

E-Print Network (OSTI)

August 1999 A Cooperative Effort By: Office of Radiation and Indoor Air Office of Solid Waste of a cooperative effort between the EPA Office of Radiation and Indoor Air, Office of Solid Waste and Emergency for prioritizing site remediation and waste management decisions. Volume I discusses the technical issues

Tschinkel, Walter R.

288

aime robert lansing hardy, application to practice, cyril stanley smith ...  

Science Conference Proceedings (OSTI)

wood frame with glass. Winners of this award may be eligible for AIME Honorary. Membership, Acta Materialia Materials & Society, and TMS/ASM Materials...

289

Testimony of Christopher Smith before the House Committee on...  

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

Through the President's all-of-the-above energy strategy, we are working to reduce oil imports, save families and businesses money at the pump, expand the choices available...

290

Modular Internet Programming with Cells Ran Rinat and Scott Smith  

E-Print Network (OSTI)

or remote invocations. Cells may be dynamically loaded, unloaded, copied, and moved. Cells serve the sizable burden of remote invocation. In- stead we advocate the use of cells in the place of remote objects: one cell may easily invoke a service on a remote cell to which it holds a reference. In this sense

Smith, Scott F.

291

A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFS  

SciTech Connect

We present a near-infrared (0.9-2.4 {mu}m) spectroscopic study of 73 field ultracool dwarfs having spectroscopic and/or kinematic evidence of youth ( Almost-Equal-To 10-300 Myr). Our sample is composed of 48 low-resolution (R Almost-Equal-To 100) spectra and 41 moderate-resolution spectra (R {approx}> 750-2000). First, we establish a method for spectral typing M5-L7 dwarfs at near-IR wavelengths that is independent of gravity. We find that both visual and index-based classification in the near-IR provides consistent spectral types with optical spectral types, though with a small systematic offset in the case of visual classification at J and K band. Second, we examine features in the spectra of {approx}10 Myr ultracool dwarfs to define a set of gravity-sensitive indices based on FeH, VO, K I, Na I, and H-band continuum shape. We then create an index-based method for classifying the gravities of M6-L5 dwarfs that provides consistent results with gravity classifications from optical spectroscopy. Our index-based classification can distinguish between young and dusty objects. Guided by the resulting classifications, we propose a set of low-gravity spectral standards for the near-IR. Finally, we estimate the ages corresponding to our gravity classifications.

Allers, K. N. [Department of Physics and Astronomy, Bucknell University, Lewisburg, PA 17837 (United States); Liu, Michael C., E-mail: k.allers@bucknell.edu [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

2013-08-01T23:59:59.000Z

292

Study of Four Young TeV Pulsar Wind Nebulae with a Spectral Evolution Model  

E-Print Network (OSTI)

We study four young Pulsar Wind Nebulae (PWNe) detected in TeV gamma-rays, G21.5-0.9, G54.1+0.3, Kes 75, and G0.9+0.1, using the spectral evolution model developed and applied to the Crab Nebula in our previous work. We model the evolution of magnetic field and particle distribution function inside a uniformly expanding PWN considering a time-dependent injection from the pulsar and radiative and adiabatic losses. Considering uncertainties in the interstellar radiation field (ISRF) and their distance, we study two cases for each PWN. Because TeV PWNe have a large TeV gamma-rays to X-rays flux ratio, the magnetic energy of the PWNe accounts for only a small fraction of the total energy injected (typically a few x 10^{-3}). The gamma-ray emission is dominated by inverse Compton scattering off the infrared photons of the ISRF. A broken power-law distribution function for the injected particles reproduces the observed spectrum well, except for G0.9+0.1. For G0.9+0.1, we do not need a low energy counterpart because...

Tanaka, Shuta J

2011-01-01T23:59:59.000Z

293

The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos  

E-Print Network (OSTI)

The energetic balance of the Standard Solar Model (SSM) results from an equilibrium between nuclear energy production, energy transfer, and photospheric emission. In this letter, we derive an order of magnitude of several % for the loss of energy in kinetic energy, magnetic energy, and X or UV radiation during the whole solar lifetime from the observations of the present Sun. We also estimate the mass loss from the observations of young solar analogs which could reach up to 30% of the current mass. We deduce new models of the present Sun, their associated neutrino fluxes, and their internal sound-speed profile. This approach sheds quantitative lights on the disagreement between the sound speed obtained by helioseismology and the sound speed derived from the SSM including the updated photospheric CNO abundances, based on recent observations. We conclude that about 20% of the present discrepancy could come from the incorrect description of the early phases of the Sun, its activity, its initial mass and mass-loss history. This study has obvious consequences on the solar system formation and the early evolution of the closest planets.

Sylvaine Turck-Chieze; Laurent Piau; Sbastien Couvidat

2011-03-14T23:59:59.000Z

294

CLOSE STELLAR ENCOUNTERS IN YOUNG, SUBSTRUCTURED, DISSOLVING STAR CLUSTERS: STATISTICS AND EFFECTS ON PLANETARY SYSTEMS  

SciTech Connect

Both simulations and observations indicate that stars form in filamentary, hierarchically clustered associations, most of which disperse into their galactic field once feedback destroys their parent clouds. However, during their early evolution in these substructured environments, stars can undergo close encounters with one another that might have significant impacts on their protoplanetary disks or young planetary systems. We perform N-body simulations of the early evolution of dissolving, substructured clusters with a wide range of properties, with the aim of quantifying the expected number and orbital element distributions of encounters as a function of cluster properties. We show that the presence of substructure both boosts the encounter rate and modifies the distribution of encounter velocities compared to what would be expected for a dynamically relaxed cluster. However, the boost only lasts for a dynamical time, and as a result the overall number of encounters expected remains low enough that gravitational stripping is unlikely to be a significant effect for the vast majority of star-forming environments in the Galaxy. We briefly discuss the implications of this result for models of the origin of the solar system, and of free-floating planets. We also provide tabulated encounter rates and orbital element distributions suitable for inclusion in population synthesis models of planet formation in a clustered environment.

Craig, Jonathan; Krumholz, Mark R., E-mail: krumholz@ucolick.org [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)

2013-06-01T23:59:59.000Z

295

High-resolution spectropolarimetric of k Cet: A proxy for the young Sun  

E-Print Network (OSTI)

Among the solar proxies studied in the Sun in Time k Cet (HD 20630) stands out as potentially having a mass very close to solar and a young age. On this study, we monitored the magnetic field and the chromospheric activity from the Ca II H & K lines of k Cet. We used the Least-Square-Deconvolution (LSD, Donati et al. 1997) by simultaneously extracting the information contained in all 8,000 photospheric lines of the echelogram (K1 type star). To reconstruct a reliable magnetic map and characterize the surface differential rotation of k Cet we used 14 exposures spread over 2 months, in order to cover at least two rotational cycles (Prot ~ 9.2 days). The LSD technique was applied to detect the Zeeman signature of the magnetic field in each of our 14 observations and to measure its longitudinal component. In order to reconstruct the magnetic field geometry of k Cet, we applied the Zeeman Doppler Imaging (ZDI) inversion method. ZDI revealed a structure in the radial magnetic field consisting of a polar magneti...

Nascimento, J D do; Marsden, S; de Mello, G F Porto; Ribas, I; Jeffers, S; Castro, M; Guinan, E

2013-01-01T23:59:59.000Z

296

NEW BROWN DWARF COMPANIONS TO YOUNG STARS IN SCORPIUS-CENTAURUS  

Science Conference Proceedings (OSTI)

We present the discoveries of three faint companions to young stars in the Scorpius-Centaurus region, imaged with the NICI instrument on Gemini South. We have confirmed all three companions through common proper motion tests. Follow-up spectroscopy has confirmed two of them, HIP 65423 B and HIP 65517 B, to be brown dwarfs, while the third, HIP 72099 B, is more likely a very low mass star just above the hydrogen burning limit. The detection of wide companions in the mass range of {approx}40-100 M{sub jup} complements previous work in the same region, reporting detections of similarly wide companions with lower masses, in the range of {approx}10-30 M{sub jup}. Such low masses near the deuterium burning limit have raised the question of whether those objects formed like planets or stars. The existence of intermediate objects as reported here could represent a bridge between lower-mass companions and stellar companions, but in any case demonstrate that mass alone may not provide a clear-cut distinction for the formation of low-mass companions to stars.

Janson, Markus [Department of Astrophysical Sciences, Princeton University, Princeton, NJ (United States); Jayawardhana, Ray; Bonavita, Mariangela [Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON (Canada); Girard, Julien H. [European Southern Observatory, Santiago (Chile); Lafreniere, David [Department of Physics, University of Montreal, Montreal, QC (Canada); Gizis, John [Department of Physics and Astronomy, University of Delaware, Newark, DE (United States); Brandeker, Alexis, E-mail: janson@astro.princeton.edu [Department of Astronomy, Stockholm University, Stockholm (Sweden)

2012-10-10T23:59:59.000Z

297

Can gas in young debris disks be constrained by their radial brightness profiles?  

E-Print Network (OSTI)

Disks around young stars are known to evolve from optically thick, gas-dominated protoplanetary disks to optically thin, almost gas-free debris disks. It is thought that the primordial gas is largely removed at ages of ~10 Myr, but it is difficult to discern the true gas densities from gas observations. This suggests using observations of dust: it has been argued that gas, if present with higher densities, would lead to flatter radial profiles of the dust density and surface brightness than those actually observed. However, here we show that these profiles are surprisingly insensitive to variation of the parameters of a central star, location of the dust-producing planetesimal belt, dustiness of the disk and - most importantly - the parameters of the ambient gas. This result holds for a wide range of gas densities (three orders of magnitude), for different radial distributions of the gas temperature, and different gas compositions. The brightness profile slopes of -3...-4 we find are the same that were theore...

Krivov, Alexander V; Brandeker, Alexis; Thbault, Philippe

2009-01-01T23:59:59.000Z

298

Difficulty Accessing Syringes Mediates the Relationship Between Methamphetamine Use and Syringe Sharing Among Young Injection Drug Users  

E-Print Network (OSTI)

The Author(s) 2010. This article is published with open access at Springerlink.com Abstract Injection drug users (IDU) who use methamphetamine (MA) are at an increased risk of HIV infection due to engagement in injection-related risk behavior including syringe sharing. In this cohort study of young IDU aged 18-30, we investigated the relationship between injection MA use and syringe sharing, and whether difficulty accessing sterile syringes mediated this association. Behavioral questionnaires were completed by 384 IDU in Vancouver, Canada between October 2005 and May 2008. Generalized estimating equations were used to estimate direct and indirect effects. The median age of participants was 24 (IQR: 2227) and 214 (55.7%) were male. Injecting MA was independently associated with syringe sharing. Mediation analyses revealed that difficulty accessing sterile syringes partially mediated the association between injecting MA and syringe sharing. Interventions to reduce syringe sharing among young methamphetamine injectors

Evan Wood; Thomas L. Patterson; Thomas Kerr; E. Wood; T. Kerr; T. L. Patterson

2011-01-01T23:59:59.000Z

299

Overcoming Obstacles to Mobility for Apprentices and Other Young People in Vocational Education and Training Final Report  

E-Print Network (OSTI)

This document acts as the final report of the Study on the obstacles to transnational mobility faced apprentices and other young people in initial vocational training and on ways of overcoming them also referred to as the MoVE-iT project. The report was financed and prepared for the use of the European Commission, Directorate-General for Education and Culture under contract nr 2005-4579/001 PIL-PILOTP.

unknown authors

2007-01-01T23:59:59.000Z

300

The Meaning of Success: Young Women and High Academic Achievement in Rapidly Developed Areas. A Comparative Study of Contemporary Rural Vermont, USA and Leinster, Ireland.  

E-Print Network (OSTI)

??This thesis is an in-depth, comparative international study on young womens high academic achievement in rural Leinster (Ireland) and Vermont (USA). The research analyses how (more)

Fuller, Wendy Irene

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Peluchi : product development of a programmable robotic toy to stimulate interest in the fields of science and technology amongst young girls  

E-Print Network (OSTI)

Statistically speaking, science, technology, and engineering are male dominated fields. Peluchi is a second-generation prototype of a programmable robotic toy targeted towards young girls in hope of promoting more interest ...

Vu, My (My H.)

2011-01-01T23:59:59.000Z

302

Shaking things up: young infants' use of sound information for object individuation  

E-Print Network (OSTI)

Object individuation, the capacity to determine whether two perceptual encounters belong to the same object or two different objects, is one of the most basic cognitive abilities and provides a foundation for infants understanding of the physical world. Yet very little work has been done to explore infants use of auditory information to individuate objects. The first research to investigate infants use of sound information to individuate objects was reported by Wilcox et al. (2006), who used a violation-ofexpectation task to examine the extent to which 4.5-month-olds use differences in sound to individuate objects. The results suggested that 4.5-month-olds use property-rich sounds (sounds intimately related to an objects physical, amodal properties) but not property-poor sounds (sounds that are more contrived) to distinguish the identity of objects involved in occlusion events. The current study investigated infants sensitivity to these two types of sounds within the context of a search task. Three experiments were conducted with infants aged 5 to 7 months. The outcome of these experiments builds and extends on the findings of Wilcox et al. in three ways. First, converging evidence was obtained, using a search task, that young infants are more sensitive to property-rich than property-poor sounds. Second, more detailed information was obtained on infants interpretation of samesounds events (two identical, rather than two different, sounds). Finally, possible explanations for infants greater sensitivity to property-rich sounds were assessed. The outcome of these studies, collectively, provides insight into the types of sounds that infants use to identify objects and the reasons why some sounds are more salient to infants than others.

Smith, Tracy Rebecca

2007-12-01T23:59:59.000Z

303

A PAN-STARRS + UKIDSS SEARCH FOR YOUNG, WIDE PLANETARY-MASS COMPANIONS IN UPPER SCORPIUS  

SciTech Connect

We have combined optical and NIR photometry from Pan-STARRS 1 and UKIDSS to search the young (5-10 Myr) star-forming region of Upper Scorpius for wide ( Almost-Equal-To 400-4000 AU) substellar companions down to {approx}5 M{sub Jup}. Our search is Almost-Equal-To 4 mag deeper than previous work based on the Two Micron All Sky Survey. We identified several candidates around known stellar members using a combination of color selection and spectral energy distribution fitting. Our follow-up spectroscopy has identified two new companions as well as confirmed two companions previously identified from photometry, with spectral types of M7.5-M9 and masses of {approx}15-60 M{sub Jup}, indicating a frequency for such wide substellar companions of {approx}0.6% {+-} 0.3%. Both USco 1610-1913B and USco 1612-1800B are more luminous than expected for their spectral type compared with known members of Upper Sco. HIP 77900B has an extreme mass ratio (M{sub 2}/M{sub 1} Almost-Equal-To 0.005) and an extreme separation of 3200 AU. USco 1602-2401B also has a very large separation of 1000 AU. We have also confirmed a low-mass stellar companion, USco 1610-2502B (730 AU, M5.5). Our substellar companions appear both non-coeval with their primary stars according to evolutionary models and, as a group, are systematically more luminous than the Upper Sco cluster sequence. One possible reason for these luminosity discrepancies could be different formation processes or accretion histories for these objects.

Aller, Kimberly M.; Kraus, Adam L.; Liu, Michael C.; Burgett, William S.; Chambers, Kenneth C.; Hodapp, Klaus W.; Kaiser, Nick; Magnier, Eugene A. [Institute of Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Price, Paul A. [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States)

2013-08-10T23:59:59.000Z

304

Application of composted pulp and paper mill sludge to a young pine plantation  

SciTech Connect

Disposing of sludge recovered from the effluent stream of pulp and paper mills has traditionally involved landfilling. Shortages in landfill space and increasingly stringent environmental regulations in many countries have forced the industry to seek alternative disposal options. The authors assessed the feasibility of compost-recycling a primary pulp and paper mill sludge (PMS) for use as a nutrient-releasing mulch in plantation forestry. The effects of the composted PMS on the growth, nutrition, water relations, and week suppression in a 3-yr-old plantation of radiata pine (Pinus radiata D.Don) on an infertile sandy soil in southern Tasmania were assessed. Compost was applied to the surface without incorporation in 0.5-m wide bands in tree rows at rates of 0, 20, 40, and 60 metric t ha{sup {minus}1} (dry matter). One year after application of compost, the percentage increase in stem diameter was 40 to 66% greater than that achieved in untreated plots, with better growth at the highest compost application rate. Improved growth of radiata pine after application of compost was primarily attributable to a 17 to 37% increase in the concentration of foliar N and to decreased water stress in amended plots. Nitrogen released from the compost was mostly absorbed by plant roots within the first 20 cm of the soil profile, with no significant movement beyond this depth range. Application of compost prepared from PMS to young stands of radiata pine was found to be acceptable recycling alternative for this material, capable of improving plantation productivity.

Jackson, M.J.; Line, M.A.; Wilson, S.; Hetherington, S.J.

2000-04-01T23:59:59.000Z

305

Report on enhancing young scholars in science and technology the Center for Excellence in Education  

Science Conference Proceedings (OSTI)

The present stock and flow of highly talented young persons engaged in the global discovery and application of science and technology are critical to the future pace of innovation. Historically, the world`s largest reservoirs of scientists and engineers have been in the Western economies. Overtime, however, Asia has begun to build equivalent pools of scientists and engineers among their university graduates. According to 1993 data from the National Science Foundation and the UNESCO World Science Report, Germany leads all economies with a 67% ratio of science and engineering degrees to total first university degrees compared to the United States with a distant fifth place at 32% behind Italy, Mexico and Poland. If the nation is to keep its scientific and technological prowess, it must capture its very best talent in the science and technology fields. The question is then raised as to the source within the United States of the science and technology talent pool. While between 1978 and 1991 there was an overall decline in male participation in undergraduate (-9%) and graduate degrees (-12%), the number of women receiving undergraduate (+8%) and graduate degrees (+34%) rose dramatically. These numbers are encouraging for women`s participation overall, however, women earn only a small percentage of physical science and engineering degrees. Why are there so few women in mathematics, engineering, and the physical sciences? The answers are complex and begin early in a woman`s exposure to science and mathematics. This report presents results on a study of careers of alumni from the Research Science Institute. Investigations were concerned with the timing of decision processes concerned with the sciences and math and factors that influenced people to turn away from or proceed with careers in science and math.

NONE

1996-09-30T23:59:59.000Z

306

OPTICAL PHOTOMETRIC GTC/OSIRIS OBSERVATIONS OF THE YOUNG MASSIVE ASSOCIATION CYGNUS OB2  

Science Conference Proceedings (OSTI)

In order to fully understand the gravitational collapse of molecular clouds, the star formation process, and the evolution of circumstellar disks, these phenomena must be studied in different Galactic environments with a range of stellar contents and positions in the Galaxy. The young massive association Cygnus OB2, in the Cygnus-X region, is a unique target to study how star formation and the evolution of circumstellar disks proceed in the presence of a large number of massive stars. We present a catalog obtained with recent optical observations in the r, i, z filters with OSIRIS, mounted on the 10.4 m Gran Telescopio CANARIAS telescope, which is the deepest optical catalog of Cyg OB2 to date. The catalog consists of 64,157 sources down to M = 0.15 M{sub Sun} at the adopted distance and age of Cyg OB2. A total of 38,300 sources have good photometry in all three bands. We combined the optical catalog with existing X-ray data of this region, in order to define the cluster locus in the optical diagrams. The cluster locus in the r - i versus i - z diagram is compatible with an extinction of the optically selected cluster members in the 2.64{sup m} < A{sub V} < 5.57{sup m} range. We derive an extinction map of the region, finding a median value of A{sub V} = 4.33{sup m} in the center of the association, decreasing toward the northwest. In the color-magnitude diagrams, the shape of the distribution of main-sequence stars is compatible with the presence of an obscuring cloud in the foreground {approx}850 {+-} 25 pc from the Sun.

Guarcello, M. G.; Wright, N. J.; Drake, J. J.; Aldcroft, T.; Kashyap, V. L. [Smithsonian Astrophysical Observatory, MS-67, 60 Garden Street, Cambridge, MA 02138 (United States); Garcia-Alvarez, D. [Instituto de Astrofisica de Canarias, E-38205 La Laguna, Tenerife (Spain); Drew, J. E. [CAR/STRI, University of Hertfordshire, College Lane, Hatfield, AL10 9AB (United Kingdom)

2012-10-15T23:59:59.000Z

307

A Sample of Very Young Field L Dwarfs and Implications for the Brown Dwarf "Lithium Test" at Early Ages  

E-Print Network (OSTI)

Using a large sample of optical spectra of late-type dwarfs, we identify a subset of late-M through L field dwarfs that, because of the presence of low-gravity features in their spectra, are believed to be unusually young. From a combined sample of 303 field L dwarfs, we find observationally that 7.6+/-1.6% are younger than 100 Myr. This percentage is in agreement with theoretical predictions once observing biases are taken into account. We find that these young L dwarfs tend to fall in the southern hemisphere (Dec < 0 deg) and may be previously unrecognized, low-mass members of nearby, young associations like Tucana-Horologium, TW Hydrae, beta Pictoris, and AB Doradus. We use a homogeneously observed sample of roughly one hundred and fifty 6300-10000 Angstrom spectra of L and T dwarfs taken with the Low-Resolution Imaging Spectrometer at the W. M. Keck Observatory to examine the strength of the 6708-A Li I line as a function of spectral type and further corroborate the trends noted by Kirkpatrick et al. (2000). We use our low-gravity spectra to investigate the strength of the Li I line as a function of age. The data weakly suggest that for early- to mid-L dwarfs the line strength reaches a maximum for a few 100 Myr, whereas for much older (few Gyr) and much younger (<100 Myr) L dwarfs the line is weaker or undetectable. We show that a weakening of lithium at lower gravities is predicted by model atmosphere calculations, an effect partially corroborated by existing observational data. Larger samples containing L dwarfs of well determined ages are needed to further test this empirically. If verified, this result would reinforce the caveat first cited in Kirkpatrick et al. (2006) that the lithium test should be used with caution when attempting to confirm the substellar nature of the youngest brown dwarfs.

J. Davy Kirkpatrick; Kelle L. Cruz; Travis S. Barman; Adam J. Burgasser; Dagny L. Looper; C. G. Tinney; Christopher R. Gelino; Patrick J. Lowrance; James Liebert; John M. Carpenter; Lynne A. Hillenbrand; John R. Stauffer

2008-08-22T23:59:59.000Z

308

Sitewide Environmental Monitoring Quarterly Progress Report for the Young-Rainey STAR Center, October through December 2002  

Office of Legacy Management (LM)

7500 7500 GJO-2003-409-TAC GJO-PIN 11.6.2 Pinellas Environmental Restoration Project Sitewide Environmental Monitoring Quarterly Progress Report for the Young - Rainey STAR Center October through December 2002 January 2003 Prepared by U.S. Department of Energy Grand Junction Office Grand Junction, Colorado Work Performed Under DOE Contract Number DE-AC13-02GJ79491 Task Order Number ST03-107 Document Number N0057500 Contents DOE/Grand Junction Office Pinellas Environmental Restoration Project January 2003 Page iii Contents Page Acronyms and Abbreviations ..........................................................................................................v 1.0 Introduction ............................................................................................................................1

309

2MASS J035523.37+113343.7: A YOUNG, DUSTY, NEARBY, ISOLATED BROWN DWARF RESEMBLING A GIANT EXOPLANET  

SciTech Connect

We present parallax and proper motion measurements, near-infrared spectra, and Wide-field Infrared Survey Explorer photometry for the low surface gravity L5{gamma} dwarf 2MASS J035523.37+113343.7 (2M0355). We use these data to evaluate photometric, spectral, and kinematic signatures of youth as 2M0355 is the reddest isolated L dwarf yet classified. We confirm its low-gravity spectral morphology and find a strong resemblance to the sharp triangular shaped H-band spectrum of the {approx}10 Myr planetary-mass object 2M1207b. We find that 2M0355 is underluminous compared to a normal field L5 dwarf in the optical and Mauna Kea Observatory J, H, and K bands and transitions to being overluminous from 3 to 12 {mu}m, indicating that enhanced photospheric dust shifts flux to longer wavelengths for young, low-gravity objects, creating a red spectral energy distribution. Investigating the near-infrared color-magnitude diagram for brown dwarfs confirms that 2M0355 is redder and underluminous compared to the known brown dwarf population, similar to the peculiarities of directly imaged exoplanets 2M1207b and HR8799bcd. We calculate UVW space velocities and find that the motion of 2M0355 is consistent with young disk objects (<2-3 Gyr) and it shows a high likelihood of membership in the AB Doradus association.

Faherty, Jacqueline K. [Department of Astronomy, Universidad de Chile Cerro Calan, Las Condes (Chile); Rice, Emily L.; Cruz, Kelle L.; Nunez, Alejandro [Department of Astrophysics , American Museum of Natural History, Central Park West at 79th Street, New York, NY 10034 (United States); Mamajek, Eric E., E-mail: jfaherty17@gmail.com, E-mail: jfaherty@amnh.org [Cerro Tololo Inter-American Observatory, Casilla 603, La Serena (Chile)

2013-01-01T23:59:59.000Z

310

Local Industry Tours - NXS 2009  

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

SMITHS Rutvik Mehta ALCOA Jian Liu SMITHS Caitlin Murphy ALCOA Yang Liu SMITHS lam nguyen ALCOA nicholas mauro SMITHS Rachel Pollock ALCOA KUN MO SMITHS Steven Remsen ALCOA...

311

Weight-related Beliefs, Behaviors, and Social Networks of Obese, Young Adult African- American Women: Implications for Healthy Weight Interventions  

E-Print Network (OSTI)

Obesity is a public health concern that affects over 30% of Americans. Approximately 78% of African-American women are overweight/obese, as compared to 46% of Caucasian women. Obese African-American women are at higher risk for associated morbidities (e.g., hypertension, type II diabetes, select cancers, and early mortality) as compared to non-Hispanic whites. Weight gain after young adulthood (ages 20-35) is associated with an increased risk of cardiovascular disease and other health problems later in life. Research that seeks to explain, predict, or control obesity among African-American women has focused on individual behavior change. Few studies have addressed the social contexts within which these behaviors occur. The purpose of this exploratory study was to examine the weight-related beliefs, behaviors, and social network characteristics of obese, young adult African-American women. A conceptual framework based on social support and social network theory guided the design of the study. Ten African-American women between the ages of 20 and 35, self-described as plus-size or full-figured, completed initial informal conversations about weight-related issues and concerns and semi-structured, in-depth face-to-face interviews. Five participants were randomly selected to complete social network profiles to identify potential social influences on weight-related beliefs and behaviors. Results of the initial conversations revealed approximately half of the participants were class III obesity (BMI > 40), reported overall good health, and 70% participated in physical activity at least one day a week. Semi-structured interviews results disclosed two primary reasons for unsuccessful long-term weight loss: (a) inconsistent weight loss behaviors and (b) lack of accountability. Weight-related beliefs and behaviors of study participants were similar to those reported for older adult African-American women. Similarities included (a) mixed levels of body satisfaction; (b) the belief that health is not determined by weight; (c) sedentary lifestyles and; (d) social support from family and friends impacts long-term weight loss success. The five social network profiles indicated participants networks are small, comprised of at least two overweight/obese females, and exhibited positive social support behaviors. Social networks included positive, negative, and non-positive relationships. Social support for weight loss is shared among network members through face-to-face interactions, phone conversations, and use of social media tools such as Facebook, Twitter, and text messaging. Future healthy weight studies would benefit from comprehensive analyses of the social networks of obese, young adult African-American women, inclusive of interviews with social network members. Culture-based healthier weight interventions that organize social support networks through social media tools are promising strategies for promoting healthy weight management among obese, young adult African-American women.

Rollins, Brandy 1982-

2012-12-01T23:59:59.000Z

312

Internationalization of a Talking Head Ouni, S. Massaro, D.W., Cohen, M.M., Young, K. & Jesse, A.(2003). Internationalization  

E-Print Network (OSTI)

Internationalization of a Talking Head Ouni, S. Massaro, D.W., Cohen, M.M., Young, K. & Jesse, A and providing the test facilities. REFERENCES [1] D.W. Massaro, Perceiving Talking Faces, From Speech Perception to a Behavioral Principle, MIT Press, 1998. [2] A. Bosseler and D.W. Massaro, "Development and Evaluation

Cohen, Michael M.

313

H2 carrier gas dependence of Young's modulus and hardness of chemical vapor deposited polycrystalline 3C-SiC thin films  

Science Conference Proceedings (OSTI)

This paper presents the mechanical properties of poly (polycrystalline) 3C-SiC thin films according to 0%, 7%, and 10% carrier gas (H"2) concentrations using nano-indentation. When H"2 concentration was 10%, it has been proved that the mechanical properties, ... Keywords: AFM, Hardness, Nano-indentation, Poly 3C-SiC, Young's modulus

Gwiy-Sang Chung; Ki-Bong Han

2008-12-01T23:59:59.000Z

314

Similar Survival With Breast Conservation Therapy or Mastectomy in the Management of Young Women With Early-Stage Breast Cancer  

Science Conference Proceedings (OSTI)

Purpose: To evaluate survival outcomes of young women with early-stage breast cancer treated with breast conservation therapy (BCT) or mastectomy, using a large, population-based database. Methods and Materials: Using the Surveillance, Epidemiology, and End Results (SEER) database, information was obtained for all female patients, ages 20 to 39 years old, diagnosed with T1-2 N0-1 M0 breast cancer between 1990 and 2007, who underwent either BCT (lumpectomy and radiation treatment) or mastectomy. Multivariable and matched pair analyses were performed to compare overall survival (OS) and cause-specific survival (CSS) of patients undergoing BCT and mastectomy. Results: A total of 14,764 women were identified, of whom 45% received BCT and 55% received mastectomy. Median follow-up was 5.7 years (range, 0.5-17.9 years). After we accounted for all patient and tumor characteristics, multivariable analysis found that BCT resulted in OS (hazard ratio [HR], 0.93; 95% confidence interval [CI], 0.83-1.04; p = 0.16) and CSS (HR, 0.93; CI, 0.83-1.05; p = 0.26) similar to that of mastectomy. Matched pair analysis, including 4,644 BCT and mastectomy patients, confirmed no difference in OS or CSS: the 5-, 10-, and15-year OS rates for BCT and mastectomy were 92.5%, 83.5%, and 77.0% and 91.9%, 83.6%, and 79.1%, respectively (p = 0.99), and the 5-, 10-, and 15-year CSS rates for BCT and mastectomy were 93.3%, 85.5%, and 79.9% and 92.5%, 85.5%, and 81.9%, respectively (p = 0.88). Conclusions: Our analysis of this population-based database suggests that young women with early-stage breast cancer have similar survival rates whether treated with BCT or mastectomy. These patients should be counseled appropriately regarding their treatment options and should not choose a mastectomy based on the assumption of improved survival.

Mahmood, Usama, E-mail: usama.mahmood@gmail.com [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States); Morris, Christopher; Neuner, Geoffrey [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States); Koshy, Matthew [Department of Cellular and Radiation Oncology, University of Chicago, Chicago, Illinois (United States)] [Department of Cellular and Radiation Oncology, University of Chicago, Chicago, Illinois (United States); Kesmodel, Susan; Buras, Robert [Department of Surgery, University of Maryland, Baltimore, Maryland (United States)] [Department of Surgery, University of Maryland, Baltimore, Maryland (United States); Chumsri, Saranya; Bao Ting; Tkaczuk, Katherine [Department of Medicine, University of Maryland, Baltimore, Maryland (United States)] [Department of Medicine, University of Maryland, Baltimore, Maryland (United States); Feigenberg, Steven [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)] [Department of Radiation Oncology, University of Maryland, Baltimore, Maryland (United States)

2012-08-01T23:59:59.000Z

315

Localization of shallow gas deposits and uncontrolled gas flows in young and unconsolidated sediments by geophysical methods  

SciTech Connect

The great mass of Neogene sediments in the Hungarian basin, where several hydrocarbon accumulations are known, is affected by Pliocene strike-slip movements, resulting in many [open quotes]flower structures.[close quotes] The gas may migrate from the reservoirs upward to the surface along the faults. Thus, shallow gas deposits can be located in the young, unconsolidated sands. There are also several shallow gas deposits derived from uncontrolled gas flows. In Hungary, the shallow gas reservoirs, which are small but increasingly important, have not yet been explored properly. However, the depleting gas may pollute the water in the soil as well as cause explosions. Our purpose is to develop inexpensive, complete, and highly sophisticated field- and data-processing techniques and an integrated complex of geophysical methods in order to define the limits of shallow gas deposits. To avoid anomalous behavior on seismic sections of the depleting gas, we started from uncontrolled gas flows which require special velocity and amplitude vs. offset analyses. In addition, natural and controlled source electromagnetic/electric surveys with various parameters were applied. An industrial-scale seismic section over an uncontrolled gas flow, special sections over flower structures and geoelectric sections, and a magnetic map are presented. The integrated complex of geophysical methods outlined above is being developed in order to establish the conditions for the exploration of gas reservoirs which have been used close to their locality and which could be recovered inexpensively.

Csoergei, J.; Kummer, I.; Papa, A.; Sipos, J.; Solyom, I.; Takacs, E.; Timar, Z. (Eotvos Lorand Geophysical Institute of Hungary, Budapest (Hungary)); Keresztes, T. (MOL RT, Budapest (Hungary))

1993-09-01T23:59:59.000Z

316

Estimation of Young's modulus and of hardness by ultra-low load hardness tests with a Vickers indenter  

SciTech Connect

The evaluation of the elastic-plastic properties of a material by using an ultra-low load hardness test requires a geometrical calibration that must take into account the imperfect form of the diamond indenter. In the present work, the Vickers indenter offset of the microindentation equipment was estimated using differently heat-treated steel samples. To this end, the dimensions of the indentations have been evaluated by two different methods: optical measurement of the diagonals and direct measurement of the penetration depth during the test. The elastic-plastic properties are then calculated from the analysis of the penetration depth/indentation load curves. The Young's modulus values determined for the different high-speed steel samples were very similar and close to the literature value for steel if the appropriate corrections are performed. The hardness values decrease when the determination procedure includes the geometrical correction of the indenter offset, and still further when using the total correction obtained by means of optical measurements of the indenter diagonal. Variation of the hardness values with the applied load is much less when the corrections are carried out.

Trindade, A.C. (Instituto Politecnico de Viseu (Portugal). Escola Superior de Tecnologia); Cavaleiro, A.; Fernandes, J.V. (Univ. de Coimbra (Portugal). Dept. de Engenharia Mecanica)

1994-07-01T23:59:59.000Z

317

The near-IR Surface Brightness Method applied to six Cepheids in the young LMC cluster NGC1866  

E-Print Network (OSTI)

We present new near-IR light curves for six Cepheids in the young blue LMC cluster NGC1866 as well as high precision radial velocity curves for ten Cepheids in NGC1866 and two in NGC2031. For the six Cepheids in NGC1866 with new J and K light curves we determine distances and absolute magnitudes by applying the near-IR surface brightness method. We find that the formal error estimates on the derived distances are underestimated by about a factor of two. We find excellent agreement between the absolute magnitudes for the low metallicity LMC Cepheids with the Period-Luminosity (P-L) relation determined by the near-IR surface brightness (ISB) method for Galactic Cepheids suggesting that the slope of the P-L relations for low metallicity and solar metallicity samples could be very similar in contrast to other recent findings. Still there appears to be significant disagreement between the observed slopes of the OGLE based apparent P-L relations in the LMC and the slopes derived from ISB analysis of Galactic Cepheids, and by inference for Magellanic Cloud Cepheids, indicating a possible intrinsic problem with the ISB method itself. Resolving this problem could reaffirm the P-L relation as the prime distance indicator applicable as well to metallicities significantly different from the LMC value.

Jesper Storm; Wolfgang P. Gieren; Pascal Fouque; Thomas G. Barnes III; Matias Gomez

2005-06-06T23:59:59.000Z

318

Herschel/PACS observations of young sources in Taurus: the far-infrared counterpart of optical jets  

E-Print Network (OSTI)

Observations of the atomic and molecular line emission associated with jets and outflows emitted by young stellar objects can be used to trace the various evolutionary stages they pass through as they evolve to become main sequence stars. To understand the relevance of atomic and molecular cooling in shocks, and how accretion and ejection efficiency evolves with the source evolutionary state, we will study the far-infrared counterparts of bright optical jets associated with Class I and II sources in Taurus (T Tau, DG Tau A, DG Tau B, FS Tau A+B, and RW Aur). We have analysed Herschel/PACS observations of a number of atomic ([OI]63um, 145um, [CII]158um) and molecular (high-J CO, H2O, OH) lines, collected within the OTKP GASPS. To constrain the origin of the detected lines we have compared the FIR emission maps with the emission from optical-jets and millimetre-outflows, and the line fluxes and ratios with predictions from shock and disk models. All of the targets are associated with extended emission in the at...

Podio, L; Flower, D; Howard, C; Sandell, G; Mora, A; Aresu, G; Brittain, S; Dent, W F R; Pinte, C; White, G J

2012-01-01T23:59:59.000Z

319

Clumpy stellar winds and high-energy emission in high-mass binaries hosting a young pulsar  

E-Print Network (OSTI)

High-mass binaries hosting young pulsars can be powerful gamma-ray emitters. The stellar wind of the massive star in the system is expected to be clumpy. Since the high-energy emission comes from the pulsar-star wind interaction, the presence of clumps can affect the spectrum and variability of this radiation. We look for the main effects of the clumps on the two-wind interaction region and on the non-thermal radiation. A simple analytical model for the two-wind interaction dynamics was developed accounting for the lifetime of clumps under the pulsar-wind impact. This time plays a very important role with regard to the evolution of the clump, the magnetic field in the clump-pulsar wind interaction region, and the non-radiative and radiative cooling of the non-thermal particles. We also computed the high-energy emission produced at the interaction of long-living clumps with the pulsar wind. For reasonable parameters, the clumps will induce small variability on the X-ray and gamma-ray radiation. Sporadically, l...

Bosch-Ramon, V

2013-01-01T23:59:59.000Z

320

The young's modulus of 1018 steel and 67061-T6 aluminum measured from quasi-static to elastic precursor strain-rates  

Science Conference Proceedings (OSTI)

The assumption that Young's modulus is strain-rate invariant is tested for 6061-T6 aluminium alloy and 1018 steel over 10 decades of strain-rate. For the same billets of material, 3 quasi-static strain-rates are investigated with foil strain gauges at room temperature. The ultrasonic sound speeds are measured and used to calculate the moduli at approximately 10{sup 4} s{sup -1}. Finally, ID plate impact is used to generate an elastic pre-cursor in the alloys at a strain-rate of approximately 10{sup 6} s{sup -1} from which the longitudinal sound speed may be obtained. It is found that indeed the Young's modulus is strain-rate independent within the experimental accuracy.

Rae, Philip J [Los Alamos National Laboratory; Trujillo, Carl [Los Alamos National Laboratory; Lovato, Manuel [Los Alamos National Laboratory

2009-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Anomalies in the Young modulus at structural phase transitions in rare-earth cobaltites RBaCo{sub 4}O{sub 7} (R = Y, Tm-Lu)  

SciTech Connect

The elastic properties of rare-earth cobaltites RBaCo{sub 4}O{sub 7} (R = Y, Tm-Lu) have been experimentally studied in the temperature range of 80-300 K. The strong softening of the Young modulus {Delta}E(T)/E{sub 0} Almost-Equal-To -(0.1-0.2) of cobaltites with Lu and Yb ions has been revealed, which is due to the instability of the crystal structure upon cooling and is accompanied by an inverse jump at the second-order structural phase transition. The softening of the Young modulus and the jump at the phase transition decrease by an order of magnitude and the transition temperature T{sub s} and hysteresis {Delta}T{sub s} increase from a compound with Lu to that with Tm. A large softening of the Young modulus at the structural transition in Lu- and Yb cobaltites indicates that the corresponding elastic constant goes to zero, whereas this constant in Tm cobaltite is not a 'soft' mode of the phase transition. It has been found that the structural phase transition in Lu- and Yb cobaltites is accompanied by a large absorption maximum at the phase transition point and an additional maximum in the low-temperature phase and absorption anomalies in Tm cobaltite is an order of magnitude smaller.

Kazei, Z. A., E-mail: kazei@plms.phys.msu.ru; Snegirev, V. V.; Andreenko, A. S. [Moscow State University (Russian Federation); Kozeeva, L. P. [Russian Academy of Sciences, Nikolaev Institute of Inorganic Chemistry, Siberian Branch (Russian Federation)

2011-08-15T23:59:59.000Z

322

Abstract for Ross Young  

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

Model has proven an extremely successful theory in describing the behaviour of nuclear and particle physics. The theoretical desire to restore simplicity in the fundamental...

323

YOUNG LEADER the - TMS  

Science Conference Proceedings (OSTI)

responsibility and ethics; multicultural, gender, and generational communication; and conflict resolution. Before and after the workshop, participants will have...

324

Young Jong Lee  

Science Conference Proceedings (OSTI)

... used to provide 3D chemical and orientational information for other ... Entropy and Time-Domain Kramers-Kronig Phase Retrieval Approaches are ...

2013-11-26T23:59:59.000Z

325

Young Professionals Program  

Science Conference Proceedings (OSTI)

Vice Chair Kinga Unocic, Past Chair Oak Ridge National Lab UnocicKA@ornl. gov, Saryu Fensin, Secretary Los Alamos National Lab saryuj@lanl.gov...

326

Young Jack Pine Site  

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

NSA-YJP) The hut, tent, and dirt road from the flux tower The sun photometer on top of the hut The bottom of the YJP flux tower NSA-YJP taken at a low sun angle to show the subtle...

327

Won Young Park  

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

designed to accelerate the adoption of efficient technologies. He also supports a Korea project that is to demonstrate economic potential for energy efficiency improvement in...

328

Young Leaders Tutorial Lecture  

Science Conference Proceedings (OSTI)

Presented by: Dr. F.H. (Sam) Froes, University of Idaho Location: 230C, Orange County Convention Center When: Monday, February 10, 12:00 noon-1:30 p.m..

329

Distribution of toenail selenium levels in young adult Caucasians and African Americans in the United States: The CARDIA Trace Element Study  

SciTech Connect

Background: Data on selenium (Se) levels in American young adults, especially in African Americans, are lacking. Objective: This study presented toenail Se distributions in American young adults of both genders, including both Caucasians and African Americans; and explored potential predictors of toenail Se levels. Data and methods: Data from the Coronary Artery Risk Development in Young Adults study among 4252 American young adults, aged 20-32 in 1987 was used to examine toenail Se levels by instrumental neutron-activation analysis. The distribution of Se levels was described and multivariable linear regression was used to examine potential modifiers of toenail Se concentration within ethnicity-gender subgroups. Results: The geometric mean of toenail Se in this cohort was 0.844 {mu}g/g (95% CI, 0.840-0.849 {mu}g/g) and the median was 0.837 {mu}g/g (95% CI, 0.833-0.844 {mu}g/g). Median levels from lowest to highest quintile were 0.691, 0.774, 0.838, 0.913 and 1.037 {mu}g/g. Se levels varied geographically, and were generally in accordance with its concentrations in local soil. Males, African Americans, current smokers, heavy drinkers and less educated participants were more likely to have low Se levels. Conclusion: This study suggests that toenail Se levels vary geographically depending on soil Se concentrations. In addition to gender, ethnicity and education level, smoking status and alcohol consumption are two important indicators of Se status since they are modifiable lifestyle factors. Findings from this study might aid public health professionals in identifying people at relatively high or low Se levels, so that chronic disease prevention efforts can be directed toward these subgroups. - Research highlights: {yields} Average of toenail Se levels in this cohort was 0.844 {mu}g/g (95% CI, 0.840-0.849 {mu}g/g). {yields} Toenail Se levels vary geographically depending on soil Se concentrations. {yields} Males, African Americans and less educated participants have low Se levels. {yields} Smoking status and alcohol consumption are two important indicators of Se status.

Xun, Pengcheng; Bujnowski, Deborah [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States) [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); Department of Epidemiology, Gillings School of Global Public Health, University of North Carolina at Chapel Hill, Chapel Hill, NC (United States); Liu, Kiang [Department of Preventive Medicine, Feinberg School of Medicine, Northwestern University, Chicago, IL (United States)] [Department of Preventive Medicine, Feinberg School of Medicine, Northwestern University, Chicago, IL (United States); Steve Morris, J. [Research Reactor Center, University of Missouri-Columbia, Columbia, MO (United States)] [Research Reactor Center, University of Missouri-Columbia, Columbia, MO (United States); Guo, Zhongqin [Department of Epidemiology and Biostatistics, School of Public Health, Ningxia Medical University, Ningxia (China) [Department of Epidemiology and Biostatistics, School of Public Health, Ningxia Medical University, Ningxia (China); Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); He, Ka, E-mail: kahe@unc.edu [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States) [Department of Nutrition, Gillings School of Global Public Health and School of Medicine, University of North Carolina at Chapel Hill, 2221 McGavran-Greenberg, Campus Box: 7461, Chapel Hill, NC (United States); Department of Epidemiology, Gillings School of Global Public Health, University of North Carolina at Chapel Hill, Chapel Hill, NC (United States)

2011-05-15T23:59:59.000Z

330

The long term dynamics of the solar radiative zone associated to new results from SoHO and young solar analogs  

E-Print Network (OSTI)

The Standard Solar Model (SSM) is no more sufficient to interpret all the observations of the radiative zone obtained with the SoHO satellite. We recall our present knowledge of this internal region and compare the recent results to models beyond the SSM assumptions. Then we discuss the missing processes and quantify some of them in using young analog observations to build a more realistic view of our star. This progress will be useful for solar-like stars observed by COROT and KEPLER.

Sylvaine Turck-Chieze; Sebastien Couvidat; Antonio Eff-Darwich; Vincent Duez; Rafael A. Garcia; Stephane Mathis; Savita Mathur; Laurent Piau; David Salabert

2011-09-19T23:59:59.000Z

331

THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A CLOSE SUBSTELLAR COMPANION TO THE YOUNG DEBRIS DISK STAR PZ Tel  

SciTech Connect

We report the discovery of a tight substellar companion to the young solar analog PZ Tel, a member of the {beta} Pic moving group observed with high-contrast adaptive optics imaging as part of the Gemini Near-Infrared Coronagraphic Imager Planet-Finding Campaign. The companion was detected at a projected separation of 16.4 {+-} 1.0 AU (0.''33 {+-} 0.''01) in 2009 April. Second-epoch observations in 2010 May demonstrate that the companion is physically associated and shows significant orbital motion. Monte Carlo modeling constrains the orbit of PZ Tel B to eccentricities >0.6. The near-IR colors of PZ Tel B indicate a spectral type of M7 {+-} 2 and thus this object will be a new benchmark companion for studies of ultracool, low-gravity photospheres. Adopting an age of 12{sup +8} {sub -4} Myr for the system, we estimate a mass of 36 {+-} 6 M {sub Jup} based on the Lyon/DUSTY evolutionary models. PZ Tel B is one of the few young substellar companions directly imaged at orbital separations similar to those of giant planets in our own solar system. Additionally, the primary star PZ Tel A shows a 70 {mu}m emission excess, evidence for a significant quantity of circumstellar dust that has not been disrupted by the orbital motion of the companion.

Biller, Beth A.; Liu, Michael C.; Wahhaj, Zahed; Dupuy, Trent J.; Ftaclas, Christ [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Nielsen, Eric L.; Close, Laird M.; Males, Jared; Skemer, Andrew [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Hayward, Thomas L.; Hartung, Markus [Gemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena (Chile); Burrows, Adam [Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States); Chun, Mark [Institute for Astronomy, 640 North Aohoku Place, 209, Hilo, HI 96720-2700 (United States); Clarke, Fraser; Tecza, Matthias; Thatte, Niranjan [Department of Astronomy, University of Oxford, DWB, Keble Road, Oxford OX1 3RH (United Kingdom); Reid, I. Neill [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Shkolnik, Evgenya L. [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015 (United States); Alencar, Silvia H. P. [Departamento de Fisica-ICEx-Universidade Federal de Minas Gerais, Av. Antonio Carlos, 6627, 30270-901, Belo Horizonte, MG (Brazil); Artymowicz, Pawel [University of Toronto at Scarborough, 1265 Military Trail, Toronto, Ontario M1C 1A4 (Canada)

2010-09-01T23:59:59.000Z

332

INDEPENDENT TECHNICAL REVIEW OF THE BUILDING 100 PLUME, FORMER DOE PINELLAS SITE (YOUNG - RAINEY STAR CENTER), LARGO, FLORIDA  

SciTech Connect

Contaminated groundwater associated with Building 100 at the Young-Rainey Science, Technology, and Research Center, formerly the DOE Pinellas plant, is the primary remedial challenge that remains to be addressed at the site. Currently, Building 100 is an active industrial facility that is now owned and operated by the Pinellas county government. Groundwater samples collected from monitoring wells recently installed near the southern boundary of the site suggest that contaminated groundwater has migrated off the plant site. In response to the challenges presented by the Building 100 plume, the Office of Legacy Management (LM) requested assistance from the DOE Office of Groundwater and Soil Remediation (EM-32) to provide a review team to make technical recommendations so that they can efficiently and effectively address characterization and remediation of the plume. The review team was unanimous in the conclusion that a dynamic strategy that combines a phased implementation of direct push samplers, sensors, and tools can be used to better delineate the extent of contamination, control plume migration, and rapidly remediate the contaminated groundwater at the site. The initial efforts of the team focused on reviewing the site history and data, organizing the information into a conceptual model, identifying appropriate technologies, and recommending an integrated strategy. The current groundwater data from the site indicate a two-lobed plume extending to the east and south. To the east vinyl chloride is the primary contaminant of concern, to the south, vinyl chloride and cis1, 2-DCE are the primary contaminants. The limited data that are available suggest that reductive dechlorination of the TCE is already occurring but is not sufficient to prevent offsite migration of low concentrations of TCE daughter products. The team recommends that DOE pursue a strategy that builds on the natural cleansing capacity of the subsurface with reductive methods including biostimulation and/or bioaugmentation to provide a sustainable remediation system within the flow path of the plume. Additional data will be required to implement this approach and will include: (1) Better delineation of the nature and extent of contamination; (2) Demonstration the plume is currently stable or shrinking; and (3) Demonstration the full reductive dechlorination is occurring. The technical team recommends that DOE use a phased approach to identify residual contamination and to provide rapid installation of remedies. Matrices of characterization and remediation sensors, technologies, and tools were developed by the team in order to match the specific conditions and requirements of the site. The team provides a specific example of remedy that includes the incorporation of a dynamic characterization strategy moving from minimally invasive to more aggressive field techniques, the consideration of multiple complementary remediation approaches based on a spatiotemporally phased approach keyed to the different demands of different parts of the plume, and the integration and sequencing of the characterization and remediation activities.

Eddy-Dilek, C.; Rossabi, J.; Amidon, M.; Riha, B.; Kaback, D.

2010-07-30T23:59:59.000Z

333

ESCHERICHIA COLI ISOLATED FROM CALVES WITH DIARRHA: MANNOSE-RESISTANT HAEMAGGLUTINATION  

E-Print Network (OSTI)

ESCHERICHIA COLI ISOLATED FROM CALVES WITH DIARRHA: MANNOSE-RESISTANT HAEMAGGLUTINATION the important characteristic of virulence in its ability to proliferate in the small intestine of young animals (Smith and Linggood, 1972). This kind of activity has also been demonstrated in vitro (Burrows et a

Recanati, Catherine

334

WILLIAM L. FOURNEY Keystone Professor and Associate Dean  

E-Print Network (OSTI)

.C. Holloway and D.B. Barker, Chapter 8, Mechanics of Oil Shale, Edited by K.P. Chong and J.W. Smith, Elsevier of Geotechnical Engineering, Vol. 120, No. 10, pp. 1684- 1703, 1994. 46. "Response of Oil Shale to Fragmentation;35."Fracture Control Blasting Techniques for Oil Shale Mining", with Chapman Young, 1983 Eastern Oil Shale

Celi, Roberto

335

Influence of an Intra-articular Lipopolysaccharide Challenge on Markers of Inflammation and Cartilage Metabolism and the Ability of Oral Glucosamine to Mitigate these Alterations in Young Horses  

E-Print Network (OSTI)

This project established an in vivo method to identify and manipulate expression of markers of osteoarthritis (OA). Specifically, strategies that predictably induce joint inflammation to evaluate dietary methods of OA prevention in young horses have yet to be accomplished. Therefore, the 3 studies described herein were conducted to determine effectiveness of an intra-articular lipopolysaccharide (LPS) challenge on markers of inflammation and cartilage metabolism in young horses and potential of dietary glucosamine hydrochloride (HCl) to mitigate these alterations. In the first study, horses were challenged with 0.25 ng or 0.50 ng of intra-articular LPS solution or lactated ringers solution (control). Injection of LPS increased inflammation based on synovial prostaglandin E2 (PGE2) concentrations. Carboxypeptide of type II collagen (CPII), a maker of type II collagen synthesis, also increased in a dose-dependent manner. However, clinical parameters of health were not influenced and remained within normal ranges. Carpal circumference increased in response to repeated arthrocentesis. Lameness scores increased with LPS injection when compared to controls. This model of joint inflammation (0.5 ng LPS) was used in the second study to evaluate potential chondroprotective effects of oral glucosamine HCl supplementation in yearling horses. Specifically, the oral absorption of glucosamine HCl versus saline was determined by nasogastric dosing and incorporation of dietary glucosamine HCl into plasma and synovial fluid over time. Plasma and synovial fluid concentrations of glucosamine tended to increase over the 98-d period. In the third study, yearlings were challenged with intra-articular LPS to determine the potential of glucosamine HCl to mitigate inflammation when compared to contralateral joints. Injection of LPS increased synovial PGE2 and cartilage biomarkers CPII and collagenase cleavage neopeptide (C2C), a marker of type II collagen degradation. Oral glucosamine HCl decreased PGE2 and C2C concentrations, but increased levels of CPII. Results of these 3 studies provide a clearer understanding of joint inflammation and cartilage turnover in young horses and demonstrated a potential role of oral glucosamine to mitigate these effects and possibly prevent OA in horses.

Lucia, Jessica Lauren

2013-05-01T23:59:59.000Z

336

Rsdometty C.M.R. Platt, J. W. Bennett, S. A. Young, M. D. Fenwick, P. J. Manson, G. R. Patterson, and B. Petraitis  

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

Rsdometty Rsdometty C.M.R. Platt, J. W. Bennett, S. A. Young, M. D. Fenwick, P. J. Manson, G. R. Patterson, and B. Petraitis CSIRO Division of Atmospheric Research Station Street Aspendale, Victoria, Australia Introduction a suitable detector, such a radiometer can yield a response time of about one second, which will follow most cl6ud fluctuations with minimum lag. The LIRAD Method The use of narrow beam filter radiometers with lidars goes back some considerable time. The CSIRO Marl< I radiometer was designed and constructed in 1970 (Platt 1971). Since then, improved versions (Marl< II and Marl< 111) have been constructed (Platt et al. 1987). Using the URAD method, much information has been obtained on the optical properties of cirrus (e.g., Platt et al. 1987, Platt and

337

GAS SURFACE DENSITY, STAR FORMATION RATE SURFACE DENSITY, AND THE MAXIMUM MASS OF YOUNG STAR CLUSTERS IN A DISK GALAXY. I. THE FLOCCULENT GALAXY M 33  

Science Conference Proceedings (OSTI)

We analyze the relationship between maximum cluster mass M{sub max} and surface densities of total gas ({Sigma}{sub gas}), molecular gas ({Sigma}{sub H{sub 2}}), and star formation rate ({Sigma}{sub SFR}) in the flocculent galaxy M 33, using published gas data and a catalog of more than 600 young star clusters in its disk. By comparing the radial distributions of gas and most massive cluster masses, we find that M{sub max}{proportional_to}{Sigma}{sup 4.7{+-}0.4}{sub gas}, M{sub max}{proportional_to}{Sigma}{sup 1.3{+-}0.1}{sub H{sub 2}}, and M{sub max}{proportional_to}{Sigma}{sup 1.0{+-}0.1}{sub SFR}. We rule out that these correlations result from the size of the sample; hence, the change of the maximum cluster mass must be due to physical causes.

Gonzalez-Lopezlira, Rosa A.; Pflamm-Altenburg, Jan; Kroupa, Pavel, E-mail: r.gonzalez@crya.unam.mx [Argelander Institut fuer Astronomie, Universitaet Bonn, Auf dem Huegel 71, D-53121 Bonn (Germany)

2012-12-20T23:59:59.000Z

338

United States Patent 8,298,667 Smith , et al. October 30, 2012  

E-Print Network (OSTI)

Patent D668,213 Barron October 2, 2012 Horizontal solar energy collector Claims CLAIM I claim the ornamental design for a horizontal solar energy collector, as shown and described. Inventors: Barron; Andrew Ross (Houston, TX) Assignee: Natcore Technology, Inc. (Red Bank, NJ) Appl. No.: D/368,952 Filed: August

Alvarez, Pedro J.

339

Postnikov Sections of Formal and Hyperformal Space Author(s): Samuel B. Smith  

E-Print Network (OSTI)

on the screen or printed page of such transmission. JSTOR is a not-for-profit organization founded in 1995. We provethat X is formalprovided Hq(Xn, Q) is additively generatedby decomposablesfor all q and n by Deligne et al., it seems plausible that a space is formal provided Hq(Xn, Q) is additivelygeneratedby

Smith, Sam

340

User Interface for the Control of the Gemini Telescopes S. S. Smith and K. Gillies  

E-Print Network (OSTI)

on the science detectors is a primary goal. Keywords: Gemini Telescope Control User Interface Tcl/Tk EPICS 1 are being built using Tcl/Tk 1 and are implemented to follow the ESO Graphical User Interface Common

Note: This page contains sample records for the topic "young buz smith" 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

User Interface for the Control of the Gemini Telescopes S. S. Smith and K. Gillies  

E-Print Network (OSTI)

detectors is a primary goal. Keywords: Gemini Telescope Control User Interface Tcl/Tk EPICS 1. INTRODUCTION software to cover the requirements of both. Applications are being built using Tcl/Tk1 and are implemented

342

Planning with Problems Requiring Temporal Coordination Andrew Coles, Maria Fox, Derek Long and Amanda Smith  

E-Print Network (OSTI)

will use in this paper is the fol- lowing. Suppose that we have two actions OPERATE MINE and MINE FOR COAL. The OPERATE MINE action causes a coal mine to be operational at the start of its execution, but closes the mine at its end. The MINE FOR COAL action #12;requires the coal mine to be operational throughout its

Coles, Andrew

343

Microsoft PowerPoint - 6-04 Bowan-Smith_r1.ppt  

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

system Completed HLW Melters Completed LAW Melter Print Close AJHM Program * Goal: Increase glass production rate for existing melter foot-print with minimal impact on WTP:...

344

Simulation of the Gas Flow in a Peirce-Smith Converter  

Science Conference Proceedings (OSTI)

ChemSheet as a Simulation Platform for Pyrometallurgical Processes ... Recent Developments in FactSage Thermochemical Software and Databases.

345

Hierarchical Diagnosis C.-Y.J. Kao and W. S. Smith Earth and...  

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

were associated with surface high-pressure systems, we include large-scale subsidence rates linearly increasing from zero at the surface up to 0.5 cm.s-1 at 1000 m, and...

346

Robust Control of a Magnetostrictive Actuator James M. Nealis 1 and Ralph C. Smith 2  

E-Print Network (OSTI)

and hybrid motor design. Such application utilize magnetostrictive transducers operating in hysteretic 111111 111111 End Mass Spring Washer Wound Wire Solenoid Permanent Magnet Direction of Rod Motion magnet which provides a biasing field to obtain bi­directional strains and a mechanism for flux shaping

347

James L. Smith, 1986 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Orlando Lawrence Contact Information The Ernest Orlando Lawrence Award U.S. Department of Energy SC-2Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301)...

348

fMRI measurements of color in macaque and human Smith-Kettlewell Eye Research Center,  

E-Print Network (OSTI)

College Web Sites and E-Mail College Searches on the Web U.S. College Fairs and Visits Visiting Campuses Sites Overviews of the U.S. Education System http://www.ed.gov/NLE/USNEI/toc.html http College Search Site http://www.usnews.com/usnews/edu/college/communit/ commsrch.htm C H A P T E R 3 C O M

Wandell, Brian A.

349

Francis Smith and the Opposition Press in England, 1660-1688  

E-Print Network (OSTI)

.R. Privy Council Re g isters in the Public Record Office State Papers Domestic in the Public Record Office A Transcript of the Registers of the Stationers 1640-1708, ed. G.E.B. Eyre and C.R. Rivington, London, 1913-4. Note on Dates and Style...

Crist, Timothy John

1977-10-25T23:59:59.000Z

350

Microsoft PowerPoint - 5_Pat Smith_NMMSS_2013_Presentation_NRC...  

National Nuclear Security Administration (NNSA)

physical inventories require a licensee to complete and submit both a Material Balance Report (DOENRC Form- 742) and Physical Inventory Listing (DOENRC Form742C) NRC...

351

User Adaptation: Good Results from Poor Systems Catherine L. Smith & Paul B. Kantor  

E-Print Network (OSTI)

.3 [Information Search and Retrieval]: Search process General Terms Experimentation, Human Factors. Keywords search" and saw the search interface. Using it, subjects entered queries in the search box, received prior to search and (2) the experimental search interface, which was entered from the first

352

User Adaptation: Good Results from Poor Systems Catherine L. Smith & Paul B. Kantor  

E-Print Network (OSTI)

.3 [Information Search and Retrieval]: Search process General Terms Experimentation, Human Factors. Keywords logged, including: (a) the beginning timestamp for each search, (b) each query entered (with timestamp characteristics of 416 topic searches Variable Mean S.E.M. Min. Max. ETTime 6.53 .158 1.53 22.73 Queries Entered 5

353

Targeted Eneregy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

354

Efficient, Automatic Web Resource Harvesting Michael L. Nelson, Joan A. Smith and  

E-Print Network (OSTI)

}@cs.odu.edu Herbert Van de Sompel and Xiaoming Liu Los Alamos National Laboratory Research Library Los Alamos NM 87545

Nelson, Michael L.

355

Targeted Energy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA  

SciTech Connect

This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

2013-03-01T23:59:59.000Z

356

Aging in Place: Smith, Media Texts and the Invisible Gendered Caregiver  

E-Print Network (OSTI)

Timonen. 2007. Home Care for Aging Populations. Northampton,and John A Krout. 2004. ?Aging in Place in Different HousingFederal Interagency Forum on Aging-Related Statistics. 2008.

Storelli, Elizangela

2010-01-01T23:59:59.000Z

357

Review: The Hanford Reach: A Land of Contrasts by Susan Zwinger and Stamford D. Smith  

E-Print Network (OSTI)

Professor, Department of History, University of Idaho,Moscow, Idaho 83844-3175 USA.M. Sowards University of Idaho, USA Susan Zwinger, Stamford

Sowards, Adam M.

2007-01-01T23:59:59.000Z

358

Component Assemblies and Component Runtimes Yu David Liu Ran Rinat Scott F. Smith  

E-Print Network (OSTI)

the cable analogy, cells are also designed to allow "hot-plugging", cables that may be connected invocation between connected cells, and full distributed functionality, including formation of remote cell different ways of handling parameters de- pending on inter-cell communication and intra-cell commu- nication

Smith, Scott F.

359

Louisville, KY Led by Debbie Grusenmeyer (Extension Associate/ PRO-DAIRY Youth Specialist) and Matt Young (Cornell Animal Science '02) a team of New York 4-H youth recently won the National 4-H  

E-Print Network (OSTI)

) and Matt Young (Cornell Animal Science '02) a team of New York 4-H youth recently won the National 4-H Dairy Quiz Bowl Championship title for the 10th time. The 33rd annual North American Invitational 4-H Dairy Quiz Bowl Contest was held at the North American International Livestock Exposition in Louisville

Keinan, Alon

360

Study at the UW this summer Summer is aspecial time to learn at the University of Washington. There is no summer  

E-Print Network (OSTI)

peptides and/or proteins. A database search of the human proteome on the basis of the BUZ domain added to the coupling reaction mixtures of Nle (24, 25). After synthesis of the random region-R-aminobutyrate (Abu or U, used as a Cys replacement), L-norleucine (Nle or M, used as a Met replacement), or 18

Queitsch, Christine

Note: This page contains sample records for the topic "young buz smith" 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

pubs.acs.org/BiochemistryPublished on Web 11/19/2010r 2010 American Chemical Society Biochemistry 2010, 49, 1073710746 10737  

E-Print Network (OSTI)

peptides and/or proteins. A database search of the human proteome on the basis of the BUZ domain added to the coupling reaction mixtures of Nle (24, 25). After synthesis of the random region-R-aminobutyrate (Abu or U, used as a Cys replacement), L-norleucine (Nle or M, used as a Met replacement), or 18

Richardson, David

362

The Architecture and Implementation of a Distributed Hypermedia Storage System  

E-Print Network (OSTI)

. Shackelford John B. Smith F. Donelson Smith The University of North Carolina at Chapel Hill Department

North Carolina at Chapel Hill, University of

363

SPECTRAL TYPING OF LATE-TYPE STELLAR COMPANIONS TO YOUNG STARS FROM LOW-DISPERSION NEAR-INFRARED INTEGRAL FIELD UNIT DATA  

Science Conference Proceedings (OSTI)

We used the Project 1640 near-infrared coronagraph and integral field spectrograph to observe 19 young solar-type stars. Five of these stars are known binary stars and we detected the late-type secondaries and were able to measure their JH spectra with a resolution of R {approx} 30. The reduced, extracted, and calibrated spectra were compared to template spectra from the IRTF spectral library. With this comparison, we test the accuracy and consistency of spectral-type determination with the low-resolution near-infrared spectra from P1640. Additionally, we determine effective temperature and surface gravity of the companions by fitting synthetic spectra calculated with the PHOENIX model atmosphere code. We also present several new epochs of astrometry of each of the systems. Together, these data increase our knowledge and understanding of the stellar make up of these systems. In addition to the astronomical results, the analysis presented helps validate the Project 1640 data reduction and spectral extraction processes and the utility of low-resolution, near-infrared spectra for characterizing late-type companions in multiple systems.

Roberts, Lewis C.; Beichman, Charles A.; Burruss, Rick; Ligon, E. Robert; Lockhart, Thomas G.; Roberts, Jennifer E.; Shao, Michael [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Rice, Emily L.; Brenner, Douglas; Oppenheimer, Ben R. [American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); Crepp, Justin R.; Dekany, Richard G.; Hillenbrand, Lynne A.; Hinkley, Sasha [California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States); King, David; Parry, Ian R. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA (United Kingdom); Metchev, Stanimir [Department of Physics and Astronomy, State University of New York, Stony Brook, NY 11794-3800 (United States); Pueyo, Laurent; Sivaramakrishnan, Anand; Soummer, Remi, E-mail: lewis.c.roberts@jpl.nasa.gov [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); and others

2012-07-15T23:59:59.000Z

364

Radiation for Hodgkin's Lymphoma in Young Female Patients: A New Technique to Avoid the Breasts and Decrease the Dose to the Heart  

SciTech Connect

Purpose: To demonstrate how, in young female patients with Hodgkin's lymphoma, using an inclined board technique can further decrease the volume of breasts and heart in the treatment field. Methods and Materials: An inclined board was constructed with the ability to mount an Aquaplast face mask, a Vacu-Lock, and a hip stopper. Eight female patients with early-stage Hodgkin's lymphoma were planned and compared using the conventional flat position and the inclined board position. All patients on the inclined board were planned with 90{sup o} degree table position and 15{sup o} gantry angle rotation to compensate for the beam divergence resulting from the patient's position on the inclined board. Dose-volume histograms were generated, as well as the mean V30 and V5 of both breasts and heart using both treatment positions. Results: The mean value of V30 of the right breast, left breast, and heart decreased from 3%, 3%, and 13%, respectively, using the flat position to 0, 0.4%, and 5%, respectively, using the inclined board. The mean value of V5 of the right breast, left breast, and heart decreased from 6%, 13%, and 36%, respectively, using the flat position to 2%, 8%, and 29%, respectively, using the inclined board. Conclusions: Compared with conventional flat positioning, this simple device and technique allows better sparing of the breasts and the heart while maintaining comparable target coverage and total lung dose.

Dabaja, Bouthaina S., E-mail: bdabaja@mdanderson.or [Department of Radiation Oncology, University of Texas M. D. Anderson Cancer Center, Houston, TX (United States); Rebueno, Neal C.S.; Mazloom, Ali; Thorne, Scott; Perrin, Kelly J.; Tolani, Naresh; Das, Pragnan; Delclos, Marc E.; Iyengar, Puneeth; Reed, Valerie K.; Horace, Patrecia; Salehpour, Mohammad R. [Department of Radiation Oncology, University of Texas M. D. Anderson Cancer Center, Houston, TX (United States)

2011-02-01T23:59:59.000Z

365

Sowing the seeds of massive black holes in small galaxies: Young clusters as the building blocks of Ultra-Compact-Dwarf Galaxies  

E-Print Network (OSTI)

Interacting galaxies often have complexes of hundreds of young stellar clusters of individual masses ~ 10^{4-6} Msun in regions that are a few hundred parsecs across. These cluster complexes interact dynamically, and their coalescence is a candidate for the origin of some ultracompact dwarf galaxies (UCDs). Individual clusters with short relaxation times are candidates for the production of intermediate-mass black holes of a few hundred solar masses, via runaway stellar collisions prior to the first supernovae in a cluster. It is therefore possible that a cluster complex hosts multiple intermediate-mass black holes that may be ejected from their individual clusters due to mergers or binary processes, but bound to the complex as a whole. Here we explore the dynamical interaction between initially free-flying massive black holes and clusters in an evolving cluster complex. We find that, after hitting some clusters, it is plausible that the massive black hole will be captured in an ultracompact dwarf forming near the center of the complex. In the process, the hole typically triggers electromagnetic flares via stellar disruptions, and is also likely to be a prominent source of gravitational radiation for the advanced ground-based detectors LIGO and VIRGO. We also discuss other implications of this scenario, notably that the central black hole could be considerably larger than expected in other formation scenarios for ultracompact dwarfs.

Pau Amaro-Seoane; Symeon Konstantinidis; Marc Dewi Freitag; M. Coleman Miller; Frederic A. Rasio

2012-11-28T23:59:59.000Z

366

A Catalog of Extended Green Objects (EGOs) in the GLIMPSE Survey: A new sample of massive young stellar object outflow candidates  

E-Print Network (OSTI)

Using images from the Spitzer GLIMPSE Legacy survey, we have identified more than 300 extended 4.5 micron sources (abbreviated EGO, Extended Green Object, for the common coding of the [4.5] band as green in 3-color composite IRAC images). We present a catalog of these EGOs, including integrated flux density measurements at 3.6, 4.5, 5.8, 8.0, and 24 microns from the GLIMPSE and MIPSGAL surveys. The average angular separation between a source in our sample and the nearest IRAS point source is >1 arcminute. The majority of EGOs are associated with infrared dark clouds (IRDCs), and where high-resolution 6.7 GHz methanol maser surveys overlap the GLIMPSE coverage, EGOs and 6.7 GHz methanol masers are strongly correlated. Extended 4.5 micron emission is thought to trace shocked molecular gas in protostellar outflows; the association of EGOs with IRDCs and 6.7 GHz methanol masers suggests that extended 4.5 micron emission may pinpoint outflows specifically from massive protostars. The mid-infrared colors of EGOs lie in regions of color-color space occupied by young protostars still embedded in infalling envelopes.

C. J. Cyganowski; B. A. Whitney; E. Holden; E. Braden; C. L. Brogan; E. Churchwell; R. Indebetouw; D. F. Watson; B. L. Babler; R. Benjamin; M. Gomez; M. R. Meade; M. S. Povich; T. P. Robitaille; C. Watson

2008-10-02T23:59:59.000Z

367

X-ray flares observed from six young stars located in the region of star clusters NGC 869 and IC 2602  

E-Print Network (OSTI)

We present an analysis of seven intense X-ray flares observed from six stars (LAV 796, LAV 1174, SHM2002 3734, 2MASS 02191082+5707324, V553 Car, V557 Car) for the first time. These stars are located in the region of young open star clusters NGC 869 and IC 2602. These flares detected in the XMM-Newton data show a rapid rise (10-40 minutes) and a slow decay (20-90 minutes). The X-ray luminosities during the flares in the energy band 0.3-7.5 keV are in the range of $10^{29.9}$ to $10^{31.7}$ erg s$^{-1}$. The strongest flare was observed with the ratio $\\sim 13$ for count rates at peak of the flare to the quiescent intensity. The maximum temperature during the flares has been found to be $\\sim$100 MK. The semi loop lengths for the flaring loops are estimated to be of the order of $\\rm{10^{10}}$ cm. The physical parameters of the flaring structure, the peak density, pressure, and minimum magnetic field required to confine the plasma have been derived and found to be consistent with flares from pre-main sequence s...

Bhatt, Himali; Singh, K P; Sagar, Ram; Kumar, Brijesh

2013-01-01T23:59:59.000Z

368

PLANETS AROUND LOW-MASS STARS (PALMS). II. A LOW-MASS COMPANION TO THE YOUNG M DWARF GJ 3629 SEPARATED BY 0.''2  

SciTech Connect

We present the discovery of a 0.''2 companion to the young M dwarf GJ 3629 as part of our high-contrast adaptive optics imaging search for giant planets around low-mass stars with the Keck-II and Subaru telescopes. Two epochs of imaging confirm that the pair is comoving and reveal signs of orbital motion. The primary exhibits saturated X-ray emission which, together with its UV photometry from GALEX, points to an age younger than {approx}300 Myr. At these ages the companion lies below the hydrogen burning limit with a model-dependent mass of 46 {+-} 16 M{sub Jup} based on the system's photometric distance of 22 {+-} 3 pc. Resolved YJHK photometry of the pair indicates a spectral type of M7 {+-} 2 for GJ 3629 B. With a projected separation of 4.4 {+-} 0.6 AU and an estimated orbital period of 21 {+-} 5 yr, GJ 3629 AB is likely to yield a dynamical mass in the next several years, making it one of only a handful of brown dwarfs to have a measured mass and an age constrained from the stellar primary.

Bowler, Brendan P.; Liu, Michael C. [Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Shkolnik, Evgenya L. [Lowell Observatory, 1400 W. Mars Hill Road, Flagstaff, AZ 86001 (United States); Tamura, Motohide, E-mail: bpbowler@ifa.hawaii.edu [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

2012-09-01T23:59:59.000Z

369

High-Energy Processes in Young Stars: Chandra X-ray Spectroscopy of HDE 283572, RY Tau, and LkCa 21  

E-Print Network (OSTI)

Weak-lined T Tauri stars (WTTS) represent the important stage of stellar evolution between the accretion phase and the zero-age main sequence. At this stage, the star decouples from its accretion disk, and spins up to a higher rotation rate than in the preceding classical T Tauri phase. Consequently, dynamo processes can be expected to become even stronger at this stage. High energy processes can have effects on the remaining circumstellar material, possibly including protoplanets and planetesimals, and these effects may account for certain observable properties of asteroids in the current solar system. Chandra observed for 100 ks the WTTS HDE 283572 which probes the PMS stage of massive A-type stars. We present first results of the analysis of its high-resolution X-ray spectrum obtained with the High-Energy Transmission Grating Spectrometer. A wide range of Fe lines of high ionization states are observed, indicating a continuous emission measure distribution. No significant signal is detected longward of the O \\textsc{viii} Ly$\\alpha$ line because of the high photoelectric absorption. We also report on the preliminary analysis of the zeroth order spectra of RY Tau and LkCa21. In particular, we show evidence of an emission line in RY Tau at 6.4 keV that we identify as fluorescent emission by neutral Fe caused by a strong X-ray flare which illuminated some structure in (or surrounding) the CTTS. A comparison of X-ray spectra of classical T Tau stars, other WTTS, and young main-sequence stars is made.

Marc Audard; Stephen L. Skinner; Kester W. Smith; Manuel Guedel; Roberto Pallavicini

2004-09-13T23:59:59.000Z

370

DEEP X-RAY OBSERVATIONS OF THE YOUNG HIGH-MAGNETIC-FIELD RADIO PULSAR J1119-6127 AND SUPERNOVA REMNANT G292.2-0.5  

SciTech Connect

High-magnetic-field radio pulsars are important transition objects for understanding the connection between magnetars and conventional radio pulsars. We present a detailed study of the young radio pulsar J1119-6127, which has a characteristic age of 1900 yr and a spin-down-inferred magnetic field of 4.1 Multiplication-Sign 10{sup 13} G, and its associated supernova remnant G292.2-0.5, using deep XMM-Newton and Chandra X-ray Observatory exposures of over 120 ks from each telescope. The pulsar emission shows strong modulation below 2.5 keV with a single-peaked profile and a large pulsed fraction of 0.48 {+-} 0.12. Employing a magnetic, partially ionized hydrogen atmosphere model, we find that the observed pulse profile can be produced by a single hot spot of temperature 0.13 keV covering about one-third of the stellar surface, and we place an upper limit of 0.08 keV for an antipodal hot spot with the same area. The non-uniform surface temperature distribution could be the result of anisotropic heat conduction under a strong magnetic field, and a single-peaked profile seems common among high-B radio pulsars. For the associated remnant G292.2-0.5, its large diameter could be attributed to fast expansion in a low-density wind cavity, likely formed by a Wolf-Rayet progenitor, similar to two other high-B radio pulsars.

Ng, C.-Y.; Kaspi, V. M. [Department of Physics, McGill University, Montreal, QC H3A 2T8 (Canada); Ho, W. C. G. [School of Mathematics, University of Southampton, Southampton SO17 1BJ (United Kingdom); Weltevrede, P. [Jodrell Bank Centre for Astrophysics, University of Manchester, Alan Turing Building, Manchester M13 9PL (United Kingdom); Bogdanov, S. [Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027 (United States); Shannon, R. [CSIRO Astronomy and Space Sciences, Australia Telescope National Facility, Marsfield, NSW 2210 (Australia); Gonzalez, M. E., E-mail: ncy@physics.mcgill.ca [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1 (Canada)

2012-12-10T23:59:59.000Z

371

2012 Young Researcher Symposium PROGRAM YOUNG RESEARCHER SYMPOSIUM  

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

of Cost-Effective and Environmentally-Benign Biogas Purification Technology Using Biochar Saurabh Patel, D. Mahajan YRS POSTERS 2012 10 36. Synthesis and...

372

Young Leaders Award Winner Summaries  

Science Conference Proceedings (OSTI)

... to participate in a wide variety of social function events, including Yong Leaders Tutorial Luncheon, EMPMD council meeting, and TMS-AIME Awards Banquet.

373

SSA Young Jack Pine Site  

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

View an aerial photo-map of the SSA-YJP site. Beginning of the "flagged path" to the tower, from the road The "new trail" to the YJP site, looking towards the site The hut and...

374

Young Leader International Scholar Program  

Science Conference Proceedings (OSTI)

TMS ESSENTIALS. MEMBERS ... The chosen International Scholars also spend a few days visiting select industrial facilities, research labs, or universities.

375

Diagnostics for Kenneth M. Young  

E-Print Network (OSTI)

remote handled waste activities and $23 million for the central characterization project. The bill million for the LANL CMR Wing 9 hot cells, and $5 million for LANSCE materials test station at LANL

376

FIRE Diagnostics Kenneth M. Young  

E-Print Network (OSTI)

Facility h ardware integration, mock-ups & in stallation Shielding/Remote Handling Integration Physics, ­ Effective change in numerical aperture. · Running fibers hot only affects the long-term absorption. · Great° Vacuum Vessel Test Cell Floor Quartz coherent fiber optic bundles Radiation Shielding Enclosure Detector

377

Fermilab Today  

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

Fermilab Today classifieds SubscribeUnsubscribe to Fermilab Today Photographer Lindy Smith Visits Fermilab Lindy Smith Lindy Smith at Fermilab arranging prairie plants on paper...

378

Effects of Drama on the Use of Reading Comprehension Strategies and on Attitudes Toward Reading  

E-Print Network (OSTI)

Press. Smith, J. L. , & Herring, J. D. (1993). Using dramaJackson, 2000; Smith & Herring, 1993) propagating theONeill, 1985; Smith & Herring, 1993). Moreover, drama helps

Gngr, Arzu

2008-01-01T23:59:59.000Z

379

Questions may be addressed via e-mail to Carl Salvaggio at salvaggio@cis.rit.edu, to Lon E. Smith at smith@cis.rit.edu, and to Emily J. Antoine at eja7248@rit.edu.  

E-Print Network (OSTI)

. For sensing systems working in what is generally referred to as the visible, near infrared, and shortwave is a composite of the radiance leaving the surface, composed of reflected direct solar, scattered solar s + LD ( ) + LB ( ) ( , , , s, s) ( , ) + Lu( , ) (4) where Es is the spectral exoatmospheric solar

Salvaggio, Carl

380

Quantitative textural analysis of packings of elongate crystals John F. Rudge Marian B. Holness Graham C. Smith  

E-Print Network (OSTI)

, for example, Barth and Wunsch (1990), Atkinson and Donev 868 Curtis and Snieder #12;(1992), Maurer and Boerner is offered in the ®eld of Bayesian statistical experimental design (e.g., Atkinson and Donev, 1992; Maurer

Rudge, John

Note: This page contains sample records for the topic "young buz smith" 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

CURRICULUM VITAE: LAURENCE C. SMITH My scientific research examines the impacts of climatic and environmental change upon  

E-Print Network (OSTI)

. to develop and optimize a sparkignited CNG Powered Refuse Truck Photo Credit: Cummings Westport, Inc. 11.9 liter CNG engine suitable for refuse and other vocational Class 8 applications. The engine conventional CNG engine to a more efficient and higher performance engine, and integrate it into a refuse

Smith, Laurence C.

382

Social organization of schools of the Scalloped Hammerhead shark, Sphyrna lewini (Griffith and Smith), in the Gulf of California  

E-Print Network (OSTI)

line), two standard errors (stip- pled bar), one standardline), two standard errors (stip- pled bar), one standardsolid), and females (stip- pled) I I I I I O Unidentified

Klimley, A Peter

1983-01-01T23:59:59.000Z

383

Nonlinear Pricing in Markets with Interdependent Demand Author(s): Shmuel S. Oren, Stephen A. Smith and Robert B. Wilson  

E-Print Network (OSTI)

being dropped, based on few simulations run, we set the Time-To-Live (TTL) value to 64 hops. 5. Number

Oren, Shmuel S.

384

L.C. Smith College Of Engineering And Computer Science Laura J. Ste inbe rg, De an  

E-Print Network (OSTI)

Materials for nuclear energy system, fission reactors, nuclear fuels, energy policy, sustainability & Engineering Nanomaterials growth and characterization; piezoelectric nanogenerators and piezotronics; photovoltaic and photoelectrochemical devices; nanomaterials for energy storage; nanoelectronics; nano

Raina, Ramesh

385

L.C. Smith College Of Engineering And Computer Science Laura J. Ste inbe rg, De an  

E-Print Network (OSTI)

deaths from wind turbine blades. Capparella A, Loew S, Meyerholz DK. Nature. 2012 Aug 2;488(7409):32. doi among the rare non-aligned sequences, they discovered a single sequence with high homology to the largeG antibodies can be detected particularly during the acute phase, but in most patients IgG antibodies are short

Raina, Ramesh

386

AR Ins. Lic. #245544 CA Ins. Lic. #0633005 d/b/a in CA Seabury & Smith Insurance Program Management  

E-Print Network (OSTI)

services · Emergency services · Hospitalization · Maternity and newborn care · Mental health/substance abuse treatments · Prescription drugs · Rehabilitative services · Laboratory services · Preventive-swing with the heftiest legislation set for 2014 -- when health insurance will become available to millions of Americans

Miami, University of

387

Molecular-level Monte Carlo simulation at fixed entropy William R. Smith a,*, Martin Lisal b,c  

E-Print Network (OSTI)

can be applied to the design of isentropic processes important in refrigeration and heat pump cycles for isentropic processes is an important consideration in the design of refrigeration and heat pump cycles its application for isentropic calculations involving compression of the alternative refrigerant HFC

Lisal, Martin

388

Flow Centralities: Do they Predict the Economic Rise and Fall of States? Douglas R. White and David Smith  

E-Print Network (OSTI)

eventually move down. Several major competing theories about mobility and centrality are tested here using and of the market depends on the ability to insert new processes into transaction chains in which products by Kaldor (1985), would suggest that the measure of centrality most relevant to mobility would

White, Douglas R.

389

Two-Dimensional Photonic Crystal Surfactant Detection Jian-Tao Zhang, Natasha Smith, and Sanford A. Asher*  

E-Print Network (OSTI)

al hierro. ¿Qué es lo que hace posible que materiales con tanta solera sigan estando de permanente

Asher, Sanford A.

390

A Distributed Graph Storage System for Artifacts in Group Collaborations  

E-Print Network (OSTI)

Douglas E. Shackelford John B. Smith F. Donelson Smith The University of North Carolina at Chapel Hill

North Carolina at Chapel Hill, University of

391

Visiting Brookhaven National Laboratory | Young Researcher Symposium...  

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

looks like a giant fish, with a forked tail on the "East End" -- the North Fork is rural, and the South Fork has many famous "Hamptons" resort towns. The Peconic Bay and...

392

General Information, Young Researcher Symposium 2012  

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

looks like a giant fish, with a forked tail on the "East End" -- the North Fork is rural, and the South Fork has many famous "Hamptons" resort towns. The Peconic Bay and...

393

Holmberg Ix: The Nearest Young Galaxy  

E-Print Network (OSTI)

Deep images taken with the Wide Field Channel of the Advanced Camera for Surveys on board the Hubble Space Telescope provide the basis for study the resolved stellar population of the M81 companion dwarf irregular galaxy Holmberg IX. Based on color-magnitude diagrams the stellar population toward Holmberg IX contains numerous stars with ages of <~200 Myr as well as older red giant stars. By charting the spatial distribution of the red giant stars and considering their inferred metallicities, we concluded that most of these older stars are associated with M81 or its tidal debris. At least 20% of the stellar mass in Holmberg IX was produced in the last ~200 Myr, giving it the youngest stellar populations if any nearby galaxy. The location of Holmberg IX, its high gas content, and its youthful stellar population suggests that it is a tidal dwarf galaxy, perhaps formed during the last close passage of M82 around M81.

Sabbi, E; Smith, L J; De Mello, D F; Mountain, M

2008-01-01T23:59:59.000Z

394

Celebrating 20 Years of Outstanding Young Leaders  

E-Print Network (OSTI)

Beesley 2001 Brent Heber Olson 2001 Kara Turner 2000 Richard Gurgel 2000 John Patrick Torgenson 1999 Eryn MaryLou Leyba 1991 Paula Quenemoen Bowman #12;NEENA PACK (2012) is a junior studying political science in 2008. He served as Campaign Finance Counsel for McCain-Palin 2008, Senator John McCain's presidential

Provancher, William

395

LEARNING FAITH YOUNG CHRISTIANS AND CATECHISM  

E-Print Network (OSTI)

Christians. The catechism handbooks were presented in a dialogue form borrowed from the first catechisms it fundamentally is. In other words, it is a relational involvement between different beings. According to him to the divergent theologies of the Lord's Supper. For the Catholics, the Eucharist holds a central and fundamental

Paris-Sud XI, Université de

396

TMS Young Leaders Professional Development Award Application  

Science Conference Proceedings (OSTI)

leadership positions in the society in the future. Funding ... $500 travel allowance toward airfare and round-trip transportation from airport to hotel. . Tickets to...

397

TMS Young Leaders International Scholar Application Form  

Science Conference Proceedings (OSTI)

Zip: Country: Birth Date: Telephone Number: E-mail: Supervisor's Name: 2. EDUCATIONAL BACKGROUND (most recent). College or University: City: State:

398

The Young Leader August 09.indd  

Science Conference Proceedings (OSTI)

als Science and Toyota Central R&D Labs. Travel expenses were paid for by the TMS Foundation. Applications for the 2010 International Scholar Award must in...

399

TMS Young Leaders Committee Meeting Minutes  

Science Conference Proceedings (OSTI)

Feb 4, 1996... are certain questions and answers that would be sensitive and should not be placed on the general bulletin board; i.e., a salary question.

400

TMS Young Leaders Committee 1998 Meeting Minutes  

Science Conference Proceedings (OSTI)

Feb 5, 1998 ... Thoughts included advanced refractories (including NASA work), nuclear fuels ( including burning weapons grade plutonium--swords into...

Note: This page contains sample records for the topic "young buz smith" 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

The Young Leader February 09.indd  

Science Conference Proceedings (OSTI)

Srikanth Bontha is a milling systems engineer at Kennametal Inc. in Latrobe, Pennsylvania, where he leads product development projects in the area of cutting...

402

EMPMD 2014 Technical Division Young Professional Poster ...  

Science Conference Proceedings (OSTI)

InGaN light-emitting diode (LED) epitaxial layer was separated from undoped GaN/sapphire structures through a chemical lift-off process. A 0.2 m-thick...

403

References - Hydrate dissolution influence on the Young's ...  

Science Conference Proceedings (OSTI)

... LMT-ENS de Cachan, France, PhD Thesis. Lide, DR 1997. CRC Handbook of Chemistry and Physics. 78 th Edition. CRC ...

2004-07-27T23:59:59.000Z

404

February The Young Leader 269 5783.indd  

Science Conference Proceedings (OSTI)

p.m. as part of the 2006 TMS Annual Meeting in San Antonio, Texas. Professional and student members alike are welcome to attend the tutorial free of charge.

405

Young's Modulus Measurements in Standard IC CMOS ...  

Science Conference Proceedings (OSTI)

... 3, pp. 689699, Mar. 1987. [3] D. Zeng et al., Residual stress and strain in CdZnTe wafer examined by X-ray diffraction methods, Appl. Phys. ...

2013-05-03T23:59:59.000Z

406

February 2010 Young Leader Revised 3.indd  

Science Conference Proceedings (OSTI)

University of Kentucky. Rachel DeLucas. Extraction & Processing Division. Rachel DeLucas is a process engineer in the melting operations and SGQ plant at...

407

Lithium Depletion of Nearby Young Stellar Associations  

E-Print Network (OSTI)

We estimate cluster ages from lithium depletion in five pre-main-sequence groups found within 100 pc of the Sun: TW Hydrae Association, Eta Chamaeleontis Cluster, Beta Pictoris Moving Group, Tucanae-Horologium Association and AB Doradus Moving Group. We determine surface gravities, effective temperatures and lithium abundances for over 900 spectra through least squares fitting to model-atmosphere spectra. For each group, we compare the dependence of lithium abundance on temperature with isochrones from pre-main-sequence evolutionary tracks to obtain model dependent ages. We find that the Eta Chamaelontis Cluster and the TW Hydrae Association are the youngest, with ages of 12+/-6 Myr and 12+/-8 Myr, respectively, followed by the Beta Pictoris Moving Group at 21+/-9 Myr, the Tucanae-Horologium Association at 27+/-11 Myr, and the AB Doradus Moving Group at an age of at least 45 Myr (where we can only set a lower limit since the models -- unlike real stars -- do not show much lithium depletion beyond this age). Here, the ordering is robust, but the precise ages depend on our choice of both atmospheric and evolutionary models. As a result, while our ages are consistent with estimates based on Hertzsprung-Russell isochrone fitting and dynamical expansion, they are not yet more precise. Our observations do show that with improved models, much stronger constraints should be feasible: the intrinsic uncertainties, as measured from the scatter between measurements from different spectra of the same star, are very low: around 10 K in effective temperature, 0.05 dex in surface gravity, and 0.03 dex in lithium abundance.

Erin Mentuch; Alexis Brandeker; Marten H. van Kerkwijk; Ray Jayawardhana; Peter H. Hauschildt

2008-08-26T23:59:59.000Z

408

Diagnostics for FIRE Kenneth M. Young  

E-Print Network (OSTI)

&D and Integration Facility h ardware integration, mock-ups & in stallation Shielding/Remote Handling Integration. · Running fibers hot only affects the long-term absorption. · Great disparity in radiation effects in an -diagnostic Plasma 90° 60° 45° 20° Vacuum Vessel Test Cell Floor Quartz coherent fiber optic bundles Radiation

409

SSRL BEAM PORT SCHEDULE  

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

7-1 7-1 Oct. 26, 2009 Oct. 27, 2009 Oct. 28, 2009 Oct. 29, 2009 Oct. 30, 2009 Oct. 31, 2009 Nov. 01, 2009 CHANGE/8803* C.SMI 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH 8803* C.SMITH BEAM LINE 9-1 Oct. 26, 2009 Oct. 27, 2009 Oct. 28, 2009 Oct. 29, 2009 Oct. 30, 2009 Oct. 31, 2009 Nov. 01, 2009 CHANGE/8861* I.MAT 8861* I.MATHEWS 8861* I.MATHEWS 8861* I.MATHEWS 8861* I.MATHEWS 8861* I.MATHEWS 8861* I.MATHEWS

410

LOW TECHNOLOGY HIGH TRITIUM BREEDING BLANKET CONCEPT* Y. Gohar, C. C. Baker, D. L. Smith, M. C. Billone, Y. S. Cha,  

E-Print Network (OSTI)

Code Costs of Decommissioning a Rederence Pressurized Water Reactor Power Station," NUREG/CR-0130 (June

Harilal, S. S.

411

M.J. Smith and G. Salvendy (Eds.): Human Interface, Part I, HCII 2009, LNCS 5617, pp. 628637, 2009. Springer-Verlag Berlin Heidelberg 2009  

E-Print Network (OSTI)

Hug, HaptiTickler, HaptiCooler, and HaptiWarmer) integrated into iFeel_IM! The implemented system can consid

Tachi, Susumu

412

Ambient Backscatter: Wireless Communication Out of Thin Air Vincent Liu, Aaron Parks, Vamsi Talla, Shyamnath Gollakota, David Wetherall, Joshua R. Smith  

E-Print Network (OSTI)

Ambient Backscatter: Wireless Communication Out of Thin Air Vincent Liu, Aaron Parks, Vamsi Talla owned by others than ACM must be honored. Abstracting with credit is permitted. To copy otherwise. Request permissions from permissions@acm.org. SIGCOMM'13, August 12­16, 2013, Hong Kong, China. Copyright

Hochberg, Michael

413

B R I G H A M YOUNG UNIVERSITY BRIGHAM YOUNG UNIVERSITY  

E-Print Network (OSTI)

borings in brachiopod shells from the Caradoc Oil Shale of Estonia. Olev VINN 1 Abstract: Abundant worm (Caradoc) oil shale in North Estonia. 9 of 21 brachiopod genera (43 %) have been bored. Excluding the size. Key Words: Ordovician; Estonia; oil shale; Brachiopoda; Trypanites; palaeoecology Citation: VINN O

Seamons, Kent E.

414

Youngs Modulus of Al/Sicp/Mgal2o4 Composites with Different ...  

Science Conference Proceedings (OSTI)

Results show that with increase in particles size distribution, residual .... Using the Computational Modelling to Improve Durability of Diesel Engine Elements.

415

Assessing the massive young Sun hypothesis to solve the warm young Earth puzzle  

E-Print Network (OSTI)

A moderately massive early Sun has been proposed to resolve the so-called faint early Sun paradox. We calculate the time-evolution of the solar mass that would be required by this hypothesis, using a simple parametrized energy-balance model for Earth's climate. Our calculations show that the solar mass loss rate would need to have been 2-3 orders of magnitude higher than present for a time on the order of ~2 Gy. Such a mass loss history is significantly at variance (both in timescale and in the magnitude of the mass loss rates) with that inferred from astronomical observations of mass loss in younger solar analogues. While suggestive, the astronomical data cannot completely rule out the possibility that the Sun had the required mass loss history; therefore, we also examine the effects of the hypothetical historical solar mass loss on orbital dynamics in the solar system, with a view to identifying additional tests of the hypothesis. Planetary and satellite orbits provide a few tests, but these are weak or non-unique.

David A. Minton; Renu Malhotra

2006-12-12T23:59:59.000Z

416

U. S. Department of Energy Savannah River Operations Office ...  

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

T. Zack Smith Deputy Manager U. S. Department of Energy Savannah River Operations Office T. Zack Smith Mr. Smith is the Deputy Manager for the U. S. Department of Energy...

417

Illustrating an error in "An equivalent condition for a uniform space to be coverable"  

E-Print Network (OSTI)

Berestovskii and Plaut introduced the concept of a coverable space when developing their theory of generalized universal covering maps for uniform spaces. If a space is coverable and chain connected then it has a generalized universal covering map. Brodskiy, Dydak, LaBuz, and Mitra introduced the concept of a uniformly joinable space when developing a theory of generalized uniform covering maps. It is easy to see that a chain connected coverable space is uniformly joinable. This paper discusses the attempt in Plaut's "An equivalent condition for a uniform space to be coverable" to prove that a uniformly joinable chain connected space is coverable.

Labuz, B

2009-01-01T23:59:59.000Z

418

Microsoft PowerPoint - UTSRWorkshop-Oct2010-Bons.pptx  

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

DESIGNING TURBINE ENDWALLS DESIGNING TURBINE ENDWALLS DESIGNING TURBINE ENDWALLS DESIGNING TURBINE ENDWALLS FOR DEPOSITION RESISTANCE WITH 1400C COMBUSTOR EXIT TEMPERATURES AND SYNGAS WATER VAPOR LEVELS Ch i S ith B tt B k P h th Sh k Chris Smith, Brett Barker, Prashanth Shankaran Josh Webb, Brian Casaday Dr. Ali Ameri, Dr. Jeffrey Bons "THE" OHIO STATE UNIVERSITY THE OHIO STATE UNIVERSITY Robert Laycock, Dr. Thomas Fletcher "THE" BRIGHAM YOUNG UNIVERSITY "THE" BRIGHAM YOUNG UNIVERSITY (3-year grant awarded Oct 2009) 1 MOTIVATION/NEED * Operational Issues -Fuel flexibility (range of feedstock heat release) y ( g ) -Diluent use (e.g. steam) -Filtration requirements * Technical Challenges - Higher firing temperature I d h t t f ( t dil t) - Increased heat transfer (steam diluent) - Potential for increased levels of airborne contaminants

419

Chuck Schadl  

Science Conference Proceedings (OSTI)

... Industrial Resource Center (PA IRC) Don Olszewski don@nepirc.com Mid ... Oklahoma Manufacturing Alliance Bob Smith bob.smith@okalliance.com ...

2013-03-08T23:59:59.000Z

420

Assessing the cleanliness of surfaces: Innovative molecular approaches vs. standard spore assays  

E-Print Network (OSTI)

N. D. Fields, C. M. Herring, and L. S. Smith. 1973.N. D. Fields, C. M. Herring, and L. S. Smith. 1973.

Cooper, M.

2012-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Chicago Office 9800 South Cass Avenue  

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

SEP 29 2010 Mr. Ian Smith Research Assistant, Laboratory Investigations Division People for Ethical Treatment of Animals 501 Front Street Norfolk, VA 23510 Dear Mr. Smith:...

422

Page not found | Department of Energy  

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

complaint filed by Alizabeth Aramowicz Smith, a former contractor employee at the Oak Ridge National Laboratory. As explained below, Smith's... http:energy.govohadownloads...

423

Page not found | Department of Energy  

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

filed by Alizabeth Aramowicz Smith, a former contractor employee at the Oak Ridge National Laboratory. As explained below, Smith's... http:energy.govohadownloads...

424

Development of a New Controlled Thermal Expansion Superalloy ...  

Science Conference Proceedings (OSTI)

Aerospace Structural Metals Handbook, (1991) Vol 4, Code 4103, page 36. 9. D. F. Smith and J. S. Smith, A Silicon-Containing, Low-Expansion Alloy with.

425

Bayesian Analysis in Applications of Hierarchical Models: Issues and Methods  

E-Print Network (OSTI)

A. S. Smith (Eds. ), Bayesian statistics 4 (pp. 336-338).Smith, A. F. (1993). Bayesian inference for generalizedat UCLA on May 23, 2011 Bayesian Analysis for Hierarchical

Michael Seltzer; Wing H. Wong; Anthony S. Bryk

2011-01-01T23:59:59.000Z

426

Temperature-Dependent Young's modulus, shear modulus and Poisson's ratio of p-type Ce0.9Fe3.5Co0.5Sb12 and n-type Co0.95Pd0.05Te0.05Sb3 Skutterudite Thermoelectric Materials  

Science Conference Proceedings (OSTI)

Effective models of the mechanical behavior of thermoelectric materials under device conditions require knowledge of the temperature-dependent elastic properties.Between room temperature and 600 K, Resonant Ultrasound Spectroscopy (RUS) measurements of the Young s and shear moduli of three skutterudite thermoelectric materials, n-type Co0.95Pd0.05Te0.05Sb3(both with and without 0.1 atomic % cerium dopant) and p-type Ce0.9Fe3.5Co0.5Sb12, decreased linearly with temperature at a rate between -0.011 GPa/K and -0.013 GPa/K. In contrast the Poisson s ratio was approximately 0.22 for the three materials and was relatively insensitive to temperature.For temperatures > 600 K, the elastic moduli decreased more rapidly and resonance peaks broadened indicating the onset of viscoelastic behavior.The viscoelastic relaxation of the moduli was least for Ce-doped n-type material, for which grain boundary precipitates may inhibit grain boundary sliding which in turn has important implications concerning creep resistance. In addition, powder processing of the n- and p-type materials should be done cautiously since submicron-sized powders of both the n- and p-type powders were pyrophoric

Schmidt, Robert [Michigan State University, East Lansing; Case, Eldon D [Michigan State University, East Lansing; Ni, Jennifer E. [Michigan State University, East Lansing; Trejo, Rosa M [ORNL; Lara-Curzio, Edgar [ORNL

2012-01-01T23:59:59.000Z

427

UNIVERSITE MONTPELLIER I INSTITUT DES SCIENCES DE L'ENTREPRISE ET DU MANAGEMENT (ISEM)  

E-Print Network (OSTI)

; Porter, 1980 ; Heil & Robertson, 1991 ; Smith & al., 1992) ou le limit pricing (ou pratique de prix

Paris-Sud XI, Université de

428

Volume Editor  

Science Conference Proceedings (OSTI)

...W. Sizek Air Force Research Laboratory Philip Smith Alcoa Technical Center Krishna Srivastava Haynes International

429

NBS FREQUENCY AND TIME BROADCAST SERVICES  

Science Conference Proceedings (OSTI)

... CR SMITH, Secretary ... observed solar or geophysical events. ... FLARES expected PROTON FLARE expected MAGSTORM expected sss (... ...

2003-01-30T23:59:59.000Z

430

WIRMS 2003: International workshop on infrared microscopy and spectroscopy with accelerator-based sources  

E-Print Network (OSTI)

Coherent THz Pulses at the NSLS DUV-FEL G.L. Carr, H. Loos,synchrotron radiation at the NSLS R.J. Smith, G.D. Smith,synchrotron radiation at the NSLS R.J. Smith 1 , G.D. Smith

Martin, Michael C.; Smith, Todd I.; McKinney, Wayne R.; Palanker, Daniel

2003-01-01T23:59:59.000Z

431

SDSU General Catalog 2010-2011 371 In the College of Sciences  

E-Print Network (OSTI)

., Shackelford, Shore, Smith, Teasdale, Templin, Wallace, Wolter Chair: Sinha Professors: Davis, Goldberg

Gallo, Linda C.

432

376 SDSU General Catalog 2012-2013 In the College of Sciences  

E-Print Network (OSTI)

, Roeder, S., Shackelford, Shore, Smith, Teasdale, Templin, Wallace, Wolter Chair: Sinha Professors: Davis

Gallo, Linda C.

433

SDSU General Catalog 2011-2012 371 In the College of Sciences  

E-Print Network (OSTI)

, Roeder, S., Shackelford, Shore, Smith, Teasdale, Templin, Wallace, Wolter Chair: Sinha Professors: Davis

Gallo, Linda C.

434

382 SDSU General Catalog 2013-2014 In the College of Sciences  

E-Print Network (OSTI)

, Roeder, S., Shackelford, Shore, Smith, Templin, Wallace, Wolter Chair: Sinha Professors: Davis, Johnson

Gallo, Linda C.

435

SEPTEMBER 201224 B OR DE R L A N D S N E WS  

E-Print Network (OSTI)

Article by COLIN SHACKELFORD, FORREST SMITH, AND BONNIE J. WARNOCK A NATIVE PLANT RESTORATION REVOLUTION

436

Young County, Texas: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

0087°, -98.7481167° 0087°, -98.7481167° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.2200087,"lon":-98.7481167,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

437

Envirodevonomics: A Research Agenda for a Young Field  

E-Print Network (OSTI)

Environmental quality in many developing countries is poor and generates substantial health and productivity costs. However, existing measures of willingness to pay for environmental quality improvements indicate low ...

Greenstone, Michael

2013-09-03T23:59:59.000Z

438

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part I  

E-Print Network (OSTI)

. Abstract- A Pliocene oil shale (Pula, Hungary), a C3 plant Triticum aestivum and a C4 plant Zea mays were-alkane, n-alkene, Pula oil shale, Botryococcus braunii, alga, plant, waxes, sediment. INTRODUCTION n-rich, Pliocene deposit from Pula (Hungary). The bulk carbon isotope ratio of this oil shale was also determined

Seamons, Kent E.

439

Combinatorics of Arc Diagrams, Ferrers Fillings, Young ... - CECM  

E-Print Network (OSTI)

partition can be reinterpreted as a cycle, as demonstrated in Figure 1.10. 1. 2. 3. 4. 5. 6. 7 ...... The two theorems can be combined to give the following corollary.

440

Framtidens lantbruk / Future Agriculture Young Researchers' Forum invites to free  

E-Print Network (OSTI)

quality and composition of the fodder it is possible to reduce greenhouse gas emissions considerably at the Swedish University of Agricul- tural Sciences that adress the sustai- nable use of natural resources

Note: This page contains sample records for the topic "young buz smith" 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

Evolution of emission line activity in intermediate mass young stars  

E-Print Network (OSTI)

We present optical spectra of 45 intermediate mass Herbig Ae/Be stars. Together with the multi-epoch spectroscopic and photometric data compiled for a large sample of these stars and ages estimated for individual stars by using pre-main sequence evolutionary tracks, we have studied the evolution of emission line activity in them. We find that, on average, the H_alpha emission line strength decreases with increasing stellar age in HAeBe stars, indicating that the accretion activity gradually declines during the PMS phase. This would hint at a relatively long-lived (a few Myr) process being responsible for the cessation of accretion in Herbig Ae/Be stars. We also find that the accretion activity in these stars drops substantially by ~ 3 Myr. This is comparable to the timescale in which most intermediate mass stars are thought to lose their inner disks, suggesting that inner disks in intermediate mass stars are dissipated rapidly after the accretion activity has fallen below a certain level. We, further find a relatively tight correlation between strength of the emission line and near-infrared excess due to inner disks in HAeBe stars, indicating that the disks around Herbig Ae/Be stars cannot be entirely passive. We suggest that this correlation can be understood within the frame work of the puffed-up inner rim disk models if the radiation from the accretion shock is also responsible for the disk heating.

P. Manoj; H. C. Bhatt; G. Maheswar; S. Muneer

2006-08-25T23:59:59.000Z

442

Young, Gifted & Black: Reflections, Commentaries and Girl Talk  

E-Print Network (OSTI)

Girl Talk By Carah L. B. Herring UC Berkeley Graduate Schoolfor my household, The Herring Insider (Circulation: 4. Well

Herring, Carah L

2011-01-01T23:59:59.000Z

443

Improving leadership capabilities for young employers at Kirin  

E-Print Network (OSTI)

My employer, Kirin Holding Company (Kirin), turned 100 years old in 2007. At the same year, Kirin changed its company structure into a holding company from Kirin Brewery Company Limited. As the former company name indicates, ...

Onuki, Hiroshi, M.B.A. Massachusetts Institute of Technology

2008-01-01T23:59:59.000Z

444

TMS Names 2013 Young Leader Professional Development Award  

Science Conference Proceedings (OSTI)

Mar 6, 2013 ... Angela Fenwick Strategic Communications Campaign Manager The Minerals ... Guang Sheng, Scientific Forming Technology Corp. Extraction...

445

The Young Leader August 2010 version2.indd - TMS  

Science Conference Proceedings (OSTI)

Babu is currently an associate professor at. The Ohio State University and a Distinguished. Scholar of Edison Welding Institute, both based in Columbus, Ohio.

446

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 27, Part 3  

E-Print Network (OSTI)

by Spieker and Ree- side (1925, p. 443) for exposures near the Blackhawk coal mine On the eastern front Huntington Creek, just south of Little Swens Canyon. East of the mapped area, where coal is being mined fromTertiary floodplains. Nonmarine limestone and thin layen of coal occur in the lacustrine middle pan of the formation

Seamons, Kent E.

447

CNST's Kartik Srinivasan Receives Sigma Xi Young Scientist ...  

Science Conference Proceedings (OSTI)

... achievements within 10 years of obtaining an advanced degree, was presented by the NIST Chapter of Sigma Xi at their annual banquet on June ...

2013-04-10T23:59:59.000Z

448

Linda Young Named to Head X-ray Science Division  

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

to the APS Hard X-ray Nanoprobe Earns an R&D 100 Award Winans of XSD Elected to ACS Fellowship Gluskin of Photon Sciences named Argonne Distinguished Fellow UChicago...

449

TMS 2014: Annual Meeting & Exhibition - For Young Professionals  

Science Conference Proceedings (OSTI)

To submit a poster for the competition, click on the button below that best describes your work: - Submit a poster in the Electronic, Magnetic & Photonic Materials...

450

BRIGHAM YOUNG UNIVERSITY GEOLOGY STUDIES Volume 26, Part 4  

E-Print Network (OSTI)

to )/( nmn + & . This result is in agreement with experimental data of oil shale (Grady et al., 1980, 1972, p. 129-140. Grady D.E., Kipp M.E., « Continuum Modeling of Explosive Fracture in Oil Shale », Int

Seamons, Kent E.

451

Brigham Young University Geology Studies Volume 27, Part 2  

E-Print Network (OSTI)

along the Southern Wasatch, Fish Springs, and House Ranges Wah Wah Range, Beaver County, Utah .................. Richard F. Wheeler Publications and Maps. Ccntrdl W d h Wdh Range. R e a ~ e r('ount~.1itah Ah\\trac r Inr~odurtlon #12

Seamons, Kent E.

452

Brigham Young University Geology Studies Volume 28, Part 3  

E-Print Network (OSTI)

, Southern Pavant Range, Utah December 1981 12-81600 52593 #12;CONTENTS Three Creeks Caldera. Southern Pavant Range. Utah ..............................................Dacite of Shauntie Hills ............................................Needles Range Formation Wah Wah

Seamons, Kent E.

453

Early Childbearing among Mexican-American Young Women: Place Matters  

E-Print Network (OSTI)

County Teen Birth Rates by Zip Code. Alameda County Publicteenagers in California zip code areas. Family Planningteenagers in California zip code areas. Family Planning

Richardson, Dawn Michele

2010-01-01T23:59:59.000Z

454

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

objects such as airplanes, nuclear power plants, rotor blades of wind turbines, damage detecting Application of the integral approach and wavelet transform in simulating and analysis of guided waves and numerical results. Keywords: guided waves; Lamb wave; debonding; structural health monitoring; piezoactuator

455

Serving the Brigham Young University Community universe.byu.edu  

E-Print Network (OSTI)

, and embroidered with the words, "Florida Python Hunters." Then the hike back to their Toyota Prius, which

Seamons, Kent E.

456

NOW OPEN: Young Professional "Meet the Candidate" Poster Session  

Science Conference Proceedings (OSTI)

There will be a master board, which will indicate the name of the candidate, the title of their poster and the location and times for their oral presentations (if...

457

Biomedical Research Mentorship: The Young Investigators' Innovative High School Program  

E-Print Network (OSTI)

Hill V, Goodchild F. (1993) Apprentice Researchers at QUEST.Santa Barbara, the Apprentice Researchers at QUEST Program (Biotechnology Program, and the Apprentice Research at QUEST

Pham, Laura; Bragg, Richard; Uchio, Ken; Husted, Cynthia A. Ph.D.

2006-01-01T23:59:59.000Z

458

Eye-In-Hand Visual Servoing Curriculum for Young Students  

E-Print Network (OSTI)

It is never too early to introduce students to robotics. Inspired by courses that use Lego Mindstorms as platform, by the huge success of the FIRST competition, and by the interest and enthusiasm of many local robotics ...

Rus, Daniela L.

459

THE DYNAMIC EVOLUTION OF YOUNG EXTRAGALACTIC RADIO SOURCES  

SciTech Connect

The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth stages of the radio luminosity versus size of the source. The interaction of the jet with the ambient medium results in the formation and evolution of sources with non-standard (flaring) morphology. In addition, cessation or restarting of the jet power and obstruction of the jet will also result in distinct morphological structures. The radio source population may thus be classified in morphological types that indicate the prevailing physical processes. Compact symmetric objects (CSOs) occupy the earliest evolutionary phase of symmetric radio sources and their dynamical behavior is fundamental for any further evolution. Analysis of CSO dynamics is presented for a sample of 24 CSOs with known redshift and hotspot separation velocity and with a large range of radio power. Observables such as radio power, separation between two hotspots, hotspot separation velocity, and kinematic age of the source are found to be generally consistent with the self-similar predictions for individual sources that reflect the varying density structure of the ambient interstellar medium. Individual sources behave different from the group as a whole. The age and size statistics confirm that a large fraction of CSOs does not evolve into extended doubles.

An Tao [Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai (China); Baan, Willem A., E-mail: antao@shao.ac.cn, E-mail: baan@astron.nl [ASTRON, P.O. Box 2, 7990-AA Dwingeloo (Netherlands)

2012-11-20T23:59:59.000Z

460

GRAVITATIONAL SLINGSHOT OF YOUNG MASSIVE STARS IN ORION  

SciTech Connect

The Orion Nebula Cluster (ONC) is the nearest region of massive star formation and thus a crucial testing ground for theoretical models. Of particular interest among the ONC's {approx}1000 members are: {theta}{sup 1} Ori C, the most massive binary in the cluster with stars of masses 38 and 9 M{sub Sun }; the Becklin-Neugebauer (BN) object, a 30 km s{sup -1} runaway star of {approx}8 M{sub Sun }; and the Kleinmann-Low (KL) nebula protostar, a highly obscured, {approx}15 M{sub Sun} object still accreting gas while also driving a powerful, apparently 'explosive' outflow. The unusual behavior of BN and KL is much debated: How did BN acquire its high velocity? How is this related to massive star formation in the KL nebula? Here, we report the results of a systematic survey using {approx}10{sup 7} numerical experiments of gravitational interactions of the {theta}{sup 1}C and BN stars. We show that dynamical ejection of BN from this triple system at its observed velocity leaves behind a binary with total energy and eccentricity matching those observed for {theta}{sup 1}C. Five other observed properties of {theta}{sup 1}C are also consistent with it having ejected BN and altogether we estimate that there is only a {approx}< 10{sup -5} probability that {theta}{sup 1}C has these properties by chance. We conclude that BN was dynamically ejected from the {theta}{sup 1}C system about 4500 years ago. BN then plowed through the KL massive star-forming core within the last 1000 years causing its recently enhanced accretion and outflow activity.

Chatterjee, Sourav; Tan, Jonathan C., E-mail: s.chatterjee@astro.ufl.edu, E-mail: jt@astro.ufl.edu [Department of Astronomy, University of Florida, Gainesville, FL 32611 (United States)

2012-08-01T23:59:59.000Z

Note: This page contains sample records for the topic "young buz smith" 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

Disk Planet Interactions and Early Evolution in Young Planetary Systems  

E-Print Network (OSTI)

We study and review disk protoplanet interactions using local shearing box simulations. These suffer the disadvantage of having potential artefacts arising from periodic boundary conditions but the advantage, when compared to global simulations, of being able to capture much of the dynamics close to the protoplanet at high resolution for low computational cost. Cases with and without self sustained MHD turbulence are considered. The conditions for gap formation and the transition from type I migration are investigated and found to depend on whether the single parameter M_p R^3/(M_* H^3), with M_p, M_*, R and H being the protoplanet mass, the central mass, the orbital radius and the disk semi-thickness respectively exceeds a number of order unity. We also investigate the coorbital torques experienced by a moving protoplanet in an inviscid disk. This is done by demonstrating the equivalence of the problem for a moving protoplanet to one where the protoplanet is in a fixed orbit which the disk material flows through radially as a result of the action of an appropriate external torque. For sustainable coorbital torques to be realized a quasi steady state must be realized in which the planet migrates through the disk without accreting significant mass. In that case although there is sensitivity to computational parameters, in agreement with earlier work by Masset & Papaloizou (2003) based on global simulations, the coorbital torques are proportional to the migration speed and result in a positive feedback on the migration, enhancing it and potentially leading to a runaway. This could lead to a fast migration for protoplanets in the Saturn mass range in massive disks and may be relevant to the mass period correlation for extrasolar planets which gives a preponderance of sub Jovian masses at short orbital period.

J. C. B. Papaloizou

2004-12-30T23:59:59.000Z

462

Brigham Young University Geology Studies Volume 30, Part 1  

E-Print Network (OSTI)

hear the Baltimore oriole saying "here, here, come right here, dear" and the yel- lowhammer saying "a

Seamons, Kent E.

463

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

. Javakhishvili Tbilisi State University 3 I. Tchavtchavadze Ave., 0179, Tbilisi, Georgia b School of Informatics, Engineering and Mathematics, University of Georgia 77a M. Kostava Str., 0175, Tbilisi, Georgia * gavalish

464

University of Florida Performing Arts Young Concert Artist  

E-Print Network (OSTI)

. Doch hast du das Mahl genossen, den Durst gestillt, Dann verlasse der lauten Genossen festfreudiges

Roy, Subrata

465

Three-Fold Increase in the Young's Modulus of Graphite ...  

Science Conference Proceedings (OSTI)

... Microstructures into Li-ion battery ... EV: Need double the energy density of presently available Li batteries ... Atomic Charges in Li-GIC Structures a3 ...

2012-10-04T23:59:59.000Z

466

Anatomy of a young giant component in the random graph  

E-Print Network (OSTI)

We provide a complete description of the giant component of the Erd\\H{o}s-R\\'enyi random graph $G(n,p)$ as soon as it emerges from the scaling window, i.e., for $p = (1+\\epsilon)/n$ where $\\epsilon^3 n \\to \\infty$ and $\\epsilon=o(1)$. Our description is particularly simple for $\\epsilon = o(n^{-1/4})$, where the giant component $C_1$ is contiguous with the following model (i.e., every graph property that holds with high probability for this model also holds w.h.p. for $C_1$). Let $Z$ be normal with mean $\\frac23 \\epsilon^3 n$ and variance $\\epsilon^3 n$, and let $K$ be a random 3-regular graph on $2\\lfloor Z\\rfloor$ vertices. Replace each edge of $K$ by a path, where the path lengths are i.i.d. geometric with mean $1/\\epsilon$. Finally, attach an independent Poisson($1-\\epsilon$)-Galton-Watson tree to each vertex. A similar picture is obtained for larger $\\epsilon=o(1)$, in which case the random 3-regular graph is replaced by a random graph with $N_k$ vertices of degree $k$ for $k\\geq 3$, where $N_k$ has mean...

Ding, Jian; Lubetzky, Eyal; Peres, Yuval

2009-01-01T23:59:59.000Z

467

What could infant and young child nutrition learn from sweatshops?  

E-Print Network (OSTI)

: accounting for ethical, social, cultural and commercialization issues. J Technol Manag Innov 2009, 4(3):24-33. Pre-publication history The pre-publication history for this paper can be accessed here: http://www.biomedcentral.com/1471-2458/11/276/prepub doi:10...

Singer, Peter A; Ansett, Sean; Sagoe-Moses, Isabella

2011-05-05T23:59:59.000Z

468

Understanding Wye Using Traditional Timber to Connect Young People  

E-Print Network (OSTI)

Biblins Youth Campsite accessible to groups from all backgrounds and abilities by improving facilities constructed. · Solar powered toilets and shower facilities will be installed before the end of 2007 and opened to follow for successful projects. · Joined-up thinking is essential between FC staff, stakeholders

469

NETL: News Release - Brigham Young University Professor Named...  

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

Fossil Fuel Combustion in Announcing 25,000 Award WASHINGTON, DC - Secretary of Energy Spencer Abraham today announced that the Department of Energy's 2002 Homer H. Lowry...

470

SMD 2013 Technical Division Young Professional Poster Contest  

Science Conference Proceedings (OSTI)

Mar 4, 2013... candidate materials for structural applications in nuclear reactors as .... Yield Point: Amit Pandey1; Robert Wheeler2; Amit Shyam1; 1ORNL;...

471

Young: The Ute Indians of Colorado in the Twentieth Century  

E-Print Network (OSTI)

The Ute Indians of Colorado in the Twentieth Century.Bibliography of the Ute In- dians of Colorado.Beulder: University of Colorado Studies, Series in

Knack, Martha C.

1999-01-01T23:59:59.000Z

472

MPMD 2014 Technical Division Young Professional Poster Contest  

Science Conference Proceedings (OSTI)

Graphics should be simple, colorful, well labeled and clear. The title should be written in letters 2 cm (3/4") to 5 cm (2") high, and all material should be readable ...

473

2013 Young Leader "Meet the Candidate" Poster Session  

Science Conference Proceedings (OSTI)

Mar 3, 2013 ... Materials Master Student Looks for a Full-time Engineer Job: Shuai Wan1; ... Liquid Metal Batteries for Large Scale Energy Storage Applications: ... feature of these batteries is the continuous creation and annihilation of the...

474

2006 Young Leader International Scholar Experience By: W. Jud ...  

Science Conference Proceedings (OSTI)

May 18, 2006 ... lab visits and arranging hosts in various cities. ... times when traveling between cities. ... $25 payable to City of Atlanta can perhaps go on our.

475

Young's Modulus and Poisson's Ratio on Piezoelectric Ceramics to ...  

Science Conference Proceedings (OSTI)

... of the Localized Temperature during a Back Grinding Process for TSV Wafers ... Porosification of CaO-B2O3-SiO2 Glass Ceramics by Selective Etching for...

476

NEWS ON THE s PROCESS FROM YOUNG OPEN CLUSTERS  

SciTech Connect

Recent spectroscopic measurements in open clusters younger than the Sun with [Fe/H] {approx}> 0 showed that the abundances of neutron-rich elements have continued to increase in the Galaxy after the formation of the Sun, roughly maintaining a solar-like distribution. This growth requires neutron fluences larger than those so far assumed, as these would have too few neutrons per iron seed. We suggest that the observed enhancements can be produced by nucleosynthesis in asymptotic giant branch (AGB) stars of low mass (M < 1.5 M{sub Sun }) if they release neutrons from the {sup 13}C({alpha},n){sup 16}O reaction in reservoirs larger by a factor of four than assumed in more massive AGB stars (M > 1.5 M{sub Sun }). Adopting such a stronger neutron source as a contributor to the abundances at the time of formation of the Sun, we show that this also affects the solar s-process distribution, so that its main component is well reproduced, without the need to assume ad hoc primary sources for the synthesis of s elements up to A {approx} 130, contrary to suggestions from other works. The changes in the expected abundances that we find are primarily due to the following reasons. (1) Enhancing the neutron source increases the efficiency of the s process, so that the ensuing stellar yields now mimic the solar distribution at a metallicity higher than before ([Fe/H ] {approx}> -0.1). (2) The age-metallicity relation is rather flat for several Gyr in that metallicity regime, so that those conditions remain stable and the enhanced nuclear yields, which are necessary to maintain a solar-like abundance pattern, can dominate the composition of the interstellar medium from which subsequent stars are formed.

Maiorca, Enrico; Busso, Maurizio; Palmerini, Sara; Trippella, Oscar [Department of Physics, University of Perugia, Via Pascoli, 06122 Perugia (Italy); Magrini, Laura; Randich, Sofia, E-mail: emaiorca@gmail.com [INAF, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, 50125 Firenze (Italy)

2012-03-01T23:59:59.000Z

477

Brigham Young University Geology Studies Volume 27, Part 2  

E-Print Network (OSTI)

geological deposits, such as oil shale, to extract hydrocarbons for energy needs. The apparatus provides more. The apparatus allows the liquid metal to distribute heat evenly throughout the oil shale. This reduces by providing more even heat distribution ·· Reduces costs associated with in situ heat extraction of oil shale

Seamons, Kent E.

478

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

of weak intensity using synchrotron radiation to reduce the exposure time to 1 s. It is also noted in section 2 from an adequate choice of free energy and internal variables. The model is then validated

479

Second ECCOMAS Young Investigators Conference 26 September 2013, Bordeaux, France  

E-Print Network (OSTI)

both among scientists and environmentalists and even among politicians. A wake behind a modern heavy planes Boeing-737. The main aim of the work was to study the influence of computational domain

480

The awarded young adult novel in Greece (1985-2004).  

E-Print Network (OSTI)

??The purpose of this study was to examine the adolescent novels that were awarded in Greece from 1985 till 2005 by four major organizations. The (more)

Komninou, Nikolitsa

2006-01-01T23:59:59.000Z

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


481

The effect of young biochar on soil respiration  

Science Conference Proceedings (OSTI)

The low temperature pyrolysis of organic material produces biochar, a charcoal like substance. Biochar is being promoted as a soil amendment to enhance soil quality, it is also seen as a mechanism of lomg-term sequestration of carbon. Our experiments tested the hypothesis that biochar is inert in soil. However, we measured an increase in CO2 production from soils after biochar amendment which increased with increasing rates of biochar. The ?13C signature of the CO2 evolved in the first several days of the incubation was the same as the ?13C signature of the biochar, confirming that biochar contributed to the CO2 flux. This effect diminished by day 6 of the incubation suggesting that most of the biochar C is slowly decomposing. Thus, aside from this short term mineralization increasing soil C with biochar may indeed be a long term C storage mechanism.

Smith, Jeffery L.; Collins, Harold P.; Bailey, Vanessa L.

2010-12-01T23:59:59.000Z

482

BRIGHAM YOUNG UNIVERSITY 2BYU 20122013 Graduate Catalog  

E-Print Network (OSTI)

include: pyrolysis, gasification, anaerobic digestion, mixed waste composting, plasma arc, and chemical ..................................................................................17 4.2 Gasification.4 Mixed Waste Composting............................................................21 4.5 Plasma Arc

Crandall, Keith A.

483

William E. and Diane M. Spicer Young Investigator Award | Stanford...  

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

esteemed member of the international scientific community as a teacher and researcher in electrical engineering, applied physics and materials science. Bill spent the past 40...

484

TMS Foundation Focus, 1 (1): Young Leaders Program  

Science Conference Proceedings (OSTI)

Jon Kellar (not pictured)--South Dakota School of Mines, Rapid City, South Dakota; Jennifer Lewis (not pictured)--University of Illinois, Urbana, Illinois; Thomas...

485

Who Creates Jobs? Small vs. Large vs. Young* By John ...  

Science Conference Proceedings (OSTI)

... less rapidly with firm age than does job destruction ... Birch, David L., 1981, Who Creates Jobs? The ... Sue, 1984, "Find the Firm", Proceedings of the ...

2013-12-24T23:59:59.000Z

486

ARM - Publications: Science Team Meeting Documents  

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

Improved Surface Emissivities Derived from Multispectral Satellite Data Improved Surface Emissivities Derived from Multispectral Satellite Data Over the ARM SGP Smith, W.L., Jr., Minnis, P., and Young, D.F., NASA Langley Research Center Eleventh Atmospheric Radiation Measurement (ARM) Science Team Meeting Surface emissivity is an important parameter for many remote sensing applications but is difficult to determine because it requires an accurate specification of the surface skin temperature. Because of this, laboratory estimates of the emissivity of pure surfaces are often relied on which generally do not adequately simulate the Earth's natural surfaces as seen from a satellite imager in space. A technique has been developed to derive surface emissivity from clear-sky, multispectral satellite data for three infrared channels (3.9 or 3.7, 10.8 and 12.0 um) common to many of today's

487

ARM - Publications: Science Team Meeting Documents  

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

Cloud and Radiative Properties Derived Over the ARM NSA Domain From AVHRR Cloud and Radiative Properties Derived Over the ARM NSA Domain From AVHRR Data Heck, P.W., Nguyen, L., Smith, W. L., Jr., Ayers, J.K., Doelling, D.R., and Spangenberg, D.A., Analytical Services and Materials, Inc.; Minnis, P., and Young, D.F., National Aeronautics and Space Administration-Langley Research Center Ninth Atmospheric Radiation Measurement (ARM) Science Team Meeting The Atmospheric Radiation Measurement (ARM) Program's polar sites on the North Slope of Alaska (NSA) measure time series of various atmospheric, cloud and radiative properties over a few selected areas. Satellite data are needed to provide measurements of similar properties between the sites and to estimate the radiation budget at the top of the atmosphere. Over the other ARM sites in the central United States and the Pacific, geostationary

488

ARM - Publications: Science Team Meeting Documents  

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

Diurnal Cycle of Cloud Microphysical Properties from GOES Over the ARM Diurnal Cycle of Cloud Microphysical Properties from GOES Over the ARM Southern Great Plains Minnis, P., and Young, D.F., National Aeronautics and Space Administration-Langley Research Center; Smith, W.L., Jr., and Heck, P.W., Analytical Services and Materials, Inc. Ninth Atmospheric Radiation Measurement (ARM) Science Team Meeting Cloud coverage, height and optical depth have been derived from the Geostationary Operational Environmental Satellite (GOES) data taken over the Atmospheric Radiation Measurement (ARM) Program's Southern Great Plains (SGP) domain since 1994. While these parameters provide a valuable basis for understanding the interaction of clouds with the radiation budget, they do not provide a complete characterization of the cloud field. Phase

489

ARM - Publications: Science Team Meeting Documents  

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

An Overview of ARM Satellite Cloud and Radiation Budget Datasets An Overview of ARM Satellite Cloud and Radiation Budget Datasets Minnis, P.(a), Nguyen, L.(a), Smith Jr., W.L.(a), Doelling, D.R.(b), Heck, P.W.(c), Khaiyer, M.M.(b), Palikonda, R.(b), Young, D.F.(a), Spangenberg, D.A.(b), Chakrapani, V.(b), Walter, B.J.(b), and Nowicki, G.D.(b), NASA Langley Research Center (a), Analytical Services and Materials, Inc. (b), CIMSS/University of Wisconsin-Madison (c) Fourteenth Atmospheric Radiation Measurement (ARM) Science Team Meeting The derivation of cloud properties from satellite data has been greatly enhanced by the availability of new multispectral satellite imagers, the validation power of ARM instruments and IOPs, and increases in computer processing speeds. Likewise, the recent availability of broadband radiation

490

Section 66  

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

Comparisons of Cloud Heights Derived from Satellite and Comparisons of Cloud Heights Derived from Satellite and Atmospheric Radiation Measurement Surface Lidar Data W.L. Smith, Jr., L. Nguyen, D.P. Garber, D.F. Young Analytical Services and Materials, Inc. Hampton, Virginia P. Minnis Atmospheric Sciences Division NASA Langley Research Center Hampton, Virginia J. Spinhirne NASA Goddard Space Flight Center Greenbelt, Maryland Introduction Cloud heights derived from single-channel, satellite infrared data can be relatively uncertain under certain conditions such as overlapped or optically thin clouds. During the daytime, optical depths derived from 0.63 µm visible (VIS) reflec- tances are used to adjust the altitude of optically thin clouds. Without the adjustment, the cloud heights are significantly underestimated diminishing the reliability and utility of the

491

Fire is the Enemy of Field and Forest  

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

Fire is the Enemy of Field and Forest Fire is the Enemy of Field and Forest Nature Bulletin No. 10 April 14, 1945 Forest Preserve District of Cook County Clayton F. Smith, President Roberts Mann, Superintendent of Conservation FIRE IS THE ENEMY OF FIELD AND FOREST There have been 112 fires in the forest preserves since January 1, burning over 612 acres, including 150 acres of fine woodland and young forest plantings. There need not have been ONE if people only understood the damage done by forest and grass fires. Every spring and every fall, thousands of acres of prairie and vacant subdivisions are burnt off. Some of these fires jump over into forest preserves. Many fires start inside the preserves, or along their highway borders, from matches, cigarettes or pipe bottle thrown aside by careless people. Some start from picnic fires. A few are kindled by boys who have seen their parents or neighbors do the same thing at home.

492

Easter Bunnies  

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

Easter Bunnies Easter Bunnies Nature Bulletin No. 61 April 13, 1946 Forest Preserve District of Cook County Clayton F. Smith, President Roberts Mann, Supt. of Conservation EASTER BUNNIES Rabbits do have eggs. But they are only 1/300 of an inch in diameter and develop into young which are born and nursed like other mammals. Molly Cottontail has already had the first of the three or four litters she produces per year in this climate. Each litter numbers from 4 to 6 little rabbits born in a nest which is a shallow hole dug in the ground by the mother, usually in an open field, padded with grass and with fur which she plucks from herself. Their ears are small at first, their eyes are closed, and they have only a coat of fuzz. After about a month they leave the nest and soon are shifting for themselves.

493

ARM - Publications: Science Team Meeting Documents  

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

Evaluation of Day-Night Continuity in Retrievals of Cloud Properties from Evaluation of Day-Night Continuity in Retrievals of Cloud Properties from GOES Heck, P.W.(a), Minnis, P.(b), Khaiyer, M.M.(a), Smith, Jr., W.L.(b), Young, D.F.(b), and Nguyen, L.(b), Analytical Services & Materials, Inc. (a), NASA Langley Research Center (b) Thirteenth Atmospheric Radiation Measurement (ARM) Science Team Meeting Currently, multi-spectral algorithms are being used to retrieve microphysical and radiative cloud p roperties from Geostationary Operational Environmental Satellite (GOES) imagery in a near-real time over a domain that includes the ARM Southern Great Plains (SGP) site. The Visible-Infrared-Solar i nfrared-Split window Technique (VISST) and Solar infrared- Infrared-Split window Technique (SIST) a re applied to half-hourly GOES data. The VISST is utilized during daylight hours while

494

B U S I N E S SB U S I N E S S ROBERT H. SMITH SCHOOL OF BUSINESS UNIVERSITY OF MARYLAND SPRING 2011 VOL. 12 NO. 1  

E-Print Network (OSTI)

and cellphone products. Employees were asked daily over a period of 10 work- ing days to list any incidents

Milchberg, Howard

495

An examination of major works for wind band and brass ensemble: Funeral march for brass choir by Edvard Grieg, Dance mix by Rob Smith, and An original suite by Gordon Jacob.  

E-Print Network (OSTI)

??The following report is research and analysis of major wind band literature for the Graduate Conducting Recital performed by the Kansas State University Wind Ensemble (more)

Sobba, Lyle Andrew

2011-01-01T23:59:59.000Z

496

FROM: STEPHEN M. SMITH, DIRECTOR OFFICE OF MANAGEMENT COMMUNICATIONS, ME-43 TO: DIRECTIVES POINTS OF CONTACT SUBJECT: DRAFT DOE G 430.1-1X, DOE Cost Estimating Guidefor Program  

E-Print Network (OSTI)

This is to notify you that the subject draft Guide has been posted in the Draft section of the DOE Directives Portal system for simultaneous use and coordination. The purpose of this Guide is to provide uniform guidance and best practices that describe the methods and procedures used in all programs and projects at DOE for preparing cost estimates. Comments in the Guide are due June 15, 2004. Comments on Guides should not be designated major or suggested, they should be simply labeled as comments. Because Guides provide nonmandatory, supplemental information about acceptable methods for implementing requirements, comments supplied will be considered advisory in nature The following procedures should be followed for the submission of comments:

unknown authors

2004-01-01T23:59:59.000Z

497

Those early days as we remember them (part VI) - Met Lab and...  

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

that the man you thought was Dr. Smith might not be Dr. Smith at all. When the atomic bomb was dropped on Japan and when the government released the famous Smythe Report, I...

498

Policy Flash 2013-47 Management and Security of Personally Identifiable Information  

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

Questions concerning this policy flash should be directed to Kevin M. Smith, of the Contract and Financial Assistance Policy Division, at Kevin.M.Smith@hq.doe.gov, or at (202) 287-1614.

499

NETL F 451.1-1/1 Categorical Exclusion (CX) Designation Form  

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

EE0002614 Smith Electric Vehicles EE DE-EE0002614 PMC - PVT Division 2010 John Jason Conley 02012010 - 10312013 Kansas City, Missouri Smith Electric Vehicles (SEV-US) Medium...

500

ARPA-E Announces 2012 Energy Innovation Summit Featuring Bill...  

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

Announces 2012 Energy Innovation Summit Featuring Bill Gates, Fred Smith and Lee Scott ARPA-E Announces 2012 Energy Innovation Summit Featuring Bill Gates, Fred Smith and Lee Scott...