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Note: This page contains sample records for the topic "field discoveries estimated" 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

Colorado Dry Natural Gas New Reservoir Discoveries in Old Fields...  

Annual Energy Outlook 2012 (EIA)

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Colorado Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1 Year-2...

2

Colorado Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Colorado Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

3

Michigan Dry Natural Gas Reserves New Field Discoveries (Billion...  

Gasoline and Diesel Fuel Update (EIA)

New Field Discoveries (Billion Cubic Feet) Michigan Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

4

Utah Dry Natural Gas Reserves New Field Discoveries (Billion...  

Annual Energy Outlook 2012 (EIA)

New Field Discoveries (Billion Cubic Feet) Utah Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

5

Arkansas Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Arkansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

6

California Dry Natural Gas Reserves New Field Discoveries (Billion...  

Annual Energy Outlook 2012 (EIA)

New Field Discoveries (Billion Cubic Feet) California Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

7

Pennsylvania Dry Natural Gas Reserves New Field Discoveries ...  

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

New Field Discoveries (Billion Cubic Feet) Pennsylvania Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

8

Louisiana Dry Natural Gas Reserves New Field Discoveries (Billion...  

Annual Energy Outlook 2012 (EIA)

New Field Discoveries (Billion Cubic Feet) Louisiana Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

9

Mississippi Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Mississippi Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

10

Kansas Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Kansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

11

Oklahoma Dry Natural Gas Reserves New Field Discoveries (Billion...  

Annual Energy Outlook 2012 (EIA)

New Field Discoveries (Billion Cubic Feet) Oklahoma Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

12

Montana Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Montana Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

13

Virginia Dry Natural Gas Reserves New Field Discoveries (Billion...  

Annual Energy Outlook 2012 (EIA)

New Field Discoveries (Billion Cubic Feet) Virginia Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

14

Alabama Dry Natural Gas Reserves New Field Discoveries (Billion...  

Gasoline and Diesel Fuel Update (EIA)

New Field Discoveries (Billion Cubic Feet) Alabama Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

15

Wyoming Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Wyoming Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6...

16

Texas Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Texas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

17

Ohio Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Ohio Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

18

Alaska Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

New Field Discoveries (Billion Cubic Feet) Alaska Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7...

19

Miscellaneous States Shale Gas Proved Reserves New Field Discoveries...  

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

New Field Discoveries (Billion Cubic Feet) Miscellaneous States Shale Gas Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4...

20

Florida Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

2014 Next Release Date: 12312015 Referring Pages: New Field Discoveries of Dry Natural Gas Reserves Florida Dry Natural Gas Proved Reserves Dry Natural Gas Proved Reserves New...

Note: This page contains sample records for the topic "field discoveries estimated" 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

,"U.S. Coalbed Methane Proved Reserves New Field Discoveries...  

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

Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","U.S. Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",201...

22

,"New York Dry Natural Gas Reserves New Field Discoveries (Billion...  

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

Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","New York Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2012...

23

New Mexico Coalbed Methane Proved Reserves New Field Discoveries...  

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

Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0 0 0 - ...

24

Utah Coalbed Methane Proved Reserves New Field Discoveries (Billion...  

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

Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0 0 0 - ...

25

Wyoming Coalbed Methane Proved Reserves New Field Discoveries...  

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

Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0 0 0 - ...

26

Oklahoma Coalbed Methane Proved Reserves New Field Discoveries...  

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

Oklahoma Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0...

27

,"New York Dry Natural Gas New Reservoir Discoveries in Old Fields...  

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

Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","New York Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic...

28

Discovery of an isolated compact elliptical galaxy in the field  

E-Print Network (OSTI)

We present the discovery of an isolated compact elliptical (cE) galaxy, found during a search of SDSS DR7 for cEs, and for which we obtained WHT/ACAM imaging. It is ~900 kpc distant from its nearest neighbour, has an effective r-band radius of ~500 pc and a B-band mean surface brightness within its effective radius of 19.75 mag/arcsec. Serendipitous deep SuprimeCam imaging shows that there is no underlying disk. Its isolated position suggests that there is an alternative channel to the stripping scenario for the formation of compact ellipticals. We also report analysis of recent deeper imaging of the previous candidate free-flying cE, which shows that it is, in fact, a normal dwarf elliptical (dE). Hence the new cE reported here is the first confirmed isolated compact elliptical to be found in the field.

Huxor, Avon; Price, James

2013-01-01T23:59:59.000Z

29

Oklahoma Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Oklahoma Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 1970's 96 108 95 1980's 99 77 208 329 327 163 398 242 163 146 1990's 437 259 110 108 79 53 66 84 42 37 2000's 42 52 18 13 9 48 12 56 85 178 2010's 1 18 - = No Data Reported; -- = Not Applicable; NA = Not Available; W = Withheld to avoid disclosure of individual company data. Release Date: 8/1/2013 Next Release Date: 8/1/2014 Referring Pages: Dry Natural Gas New Reservoir Discoveries in Old Fields Oklahoma Dry Natural Gas Proved Reserves Dry Natural Gas New Reservoir Discoveries in Old Fields

30

,"Wyoming Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Wyoming Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18swy_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18swy_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

31

,"Pennsylvania Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Pennsylvania Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18spa_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18spa_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

32

,"Colorado Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Colorado Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sco_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sco_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

33

,"Virginia Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Virginia Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sva_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sva_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

34

,"Alabama Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Alabama Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sal_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sal_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

35

,"North Dakota Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","North Dakota Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18snd_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18snd_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

36

,"Florida Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Florida Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sfl_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sfl_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

37

,"New Mexico Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","New Mexico Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18snm_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18snm_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

38

,"Arkansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Arkansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sar_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sar_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

39

,"Montana Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Montana Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18smt_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18smt_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

40

,"Mississippi Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Mississippi Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sms_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sms_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

Note: This page contains sample records for the topic "field discoveries estimated" 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

,"Michigan Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Michigan Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18smi_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18smi_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

42

,"Oklahoma Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Oklahoma Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sok_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sok_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

43

,"West Virginia Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","West Virginia Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18swv_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18swv_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

44

,"Kentucky Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Kentucky Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sky_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sky_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov"

45

New Mexico--West Coalbed Methane Proved Reserves New Field Discoveries...  

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

Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0 0 0 - ...

46

U.S. Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)  

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

New Field Discoveries (Billion Cubic Feet) New Field Discoveries (Billion Cubic Feet) U.S. Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 1970's 3,173 3,860 3,188 1980's 2,539 3,731 2,687 1,574 2,536 999 1,099 1,089 1,638 1,450 1990's 2,004 848 649 899 1,894 1,666 1,451 2,681 1,074 1,568 2000's 1,983 3,578 1,332 1,222 759 942 409 796 1,170 1,372 2010's 850 947 - = No Data Reported; -- = Not Applicable; NA = Not Available; W = Withheld to avoid disclosure of individual company data. Release Date: 8/1/2013 Next Release Date: 8/1/2014 Referring Pages: New Field Discoveries of Dry Natural Gas Reserves U.S. Dry Natural Gas Proved Reserves Dry Natural Gas Proved Reserves New Field Discoveries

47

,"Utah Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Utah Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sut_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sut_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 6:11:13 PM"

48

,"Alaska Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Alaska Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sak_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sak_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 6:11:07 PM"

49

,"Kansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Kansas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18sks_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18sks_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 6:11:09 PM"

50

,"Ohio Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Ohio Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18soh_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18soh_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 6:11:11 PM"

51

,"Texas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)"  

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

New Field Discoveries (Billion Cubic Feet)" New Field Discoveries (Billion Cubic Feet)" ,"Click worksheet name or tab at bottom for data" ,"Worksheet Name","Description","# Of Series","Frequency","Latest Data for" ,"Data 1","Texas Dry Natural Gas Reserves New Field Discoveries (Billion Cubic Feet)",1,"Annual",2011 ,"Release Date:","8/1/2013" ,"Next Release Date:","8/1/2014" ,"Excel File Name:","rngr18stx_1a.xls" ,"Available from Web Page:","http://tonto.eia.gov/dnav/ng/hist/rngr18stx_1a.htm" ,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"12/12/2013 6:11:12 PM"

52

U.S. Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic  

Gasoline and Diesel Fuel Update (EIA)

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) New Reservoir Discoveries in Old Fields (Billion Cubic Feet) U.S. Dry Natural Gas New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 1970's 3,301 4,579 2,566 1980's 2,577 2,998 3,419 2,965 2,686 2,960 1,771 1,499 1,909 2,243 1990's 2,412 1,604 1,724 1,866 3,480 2,452 3,110 2,382 2,162 2,196 2000's 2,368 2,800 1,694 1,610 1,206 1,208 1,155 1,188 1,622 2,598 2010's 1,668 1,227 - = No Data Reported; -- = Not Applicable; NA = Not Available; W = Withheld to avoid disclosure of individual company data. Release Date: 8/1/2013 Next Release Date: 8/1/2014 Referring Pages: Dry Natural Gas New Reservoir Discoveries in Old Fields

53

U.S. Coalbed Methane Proved Reserves New Field Discoveries (Billion...  

Gasoline and Diesel Fuel Update (EIA)

U.S. Coalbed Methane Proved Reserves New Field Discoveries (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 2000's 0 2010's 0 0 0 0...

54

Magnetic Field based Heading Estimation for Pedestrian Navigation Environments  

E-Print Network (OSTI)

Magnetic Field based Heading Estimation for Pedestrian Navigation Environments Muhammad Haris Afzal held devices, these other sources are accelerometers for roll and pitch estimates and magnetic field sensors for the heading. In order to utilize the magnetic field sensors for heading estimation

Calgary, University of

55

Estimating Motor Efficiency in the Field  

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

Some utility companies and public agencies offer rebates to encourage customers to upgrade their existing standard efficiency motors to premium efficiency motors. It is important to know the efficiency of the existing motor and how it is being used to accurately estimate potential annual energy and dollar savings. This tip sheet provides suggested actions and estimates of savings from improved efficiency.

56

SEISMIC WAVES ESTIMATION AND WAVE FIELD DECOMPOSITION WITH FACTOR GRAPHS  

E-Print Network (OSTI)

SEISMIC WAVES ESTIMATION AND WAVE FIELD DECOMPOSITION WITH FACTOR GRAPHS Stefano Maranò Christoph, Dept. Information Technology & Electr. Eng., 8092 Zürich ABSTRACT Physical wave fields are often from sensors of different kinds. In this paper we propose a technique for the analysis of vector wave

Loeliger, Hans-Andrea

57

Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)  

E-Print Network (OSTI)

Context: Recent spectropolarimetric observations of Herbig Ae/Be stars have yielded new arguments in favour of a fossil origin for the magnetic fields of intermediate mass stars. Aims: To study the evolution of these magnetic fields, and their impact on the evolution of the angular momentum of these stars during the pre-main sequence phase, we observed Herbig Ae/Be members of young open clusters of various ages. Methods: We obtained high-resolution spectropolarimetric observations of Herbig Ae/Be stars belonging to the young open clusters NGC 6611 (< 6 Myr), NGC 2244 (~1.9 Myr), and NGC 2264 (~8 Myr), using ESPaDOnS at theCanada-France-Hawaii Telescope. Results: Here we report the discovery of strong magnetic fields in two massive pre-main sequence cluster stars. We detected, for the first time, a magnetic field in a pre-main sequence rapid rotator: the 10.2 Msun Herbig B1.5e star W601 (NGC 6611; v sin i ~ 190 km/s). Our spectropolarimetric observations yield a longitudinal magnetic field larger than 1 kG,...

Alecian, E; Catala, C; Bagnulo, S; Bhm, T; Bohlender, D; Bouret, J -C; Donati, J -F; Folsom, C P; Grunhut, J; Landstreet, J D

2008-01-01T23:59:59.000Z

58

Performance bounds on matched-field methods for source localization and estimation of ocean environmental parameters  

E-Print Network (OSTI)

Matched-field methods concern estimation of source location and/or ocean environmental parameters by exploiting full wave modeling of acoustic waveguide propagation. Typical estimation performance demonstrates two fundamental ...

Xu, Wen, 1967-

2001-01-01T23:59:59.000Z

59

Discovery of magnetic fields in the very young, massive stars W601 (NGC 6611) and OI 201 (NGC 2244)  

E-Print Network (OSTI)

Context: Recent spectropolarimetric observations of Herbig Ae/Be stars have yielded new arguments in favour of a fossil origin for the magnetic fields of intermediate mass stars. Aims: To study the evolution of these magnetic fields, and their impact on the evolution of the angular momentum of these stars during the pre-main sequence phase, we observed Herbig Ae/Be members of young open clusters of various ages. Methods: We obtained high-resolution spectropolarimetric observations of Herbig Ae/Be stars belonging to the young open clusters NGC 6611 (Hawaii Telescope. Results: Here we report the discovery of strong magnetic fields in two massive pre-main sequence cluster stars. We detected, for the first time, a magnetic field in a pre-main sequence rapid rotator: the 10.2 Msun Herbig B1.5e star W601 (NGC 6611; v sin i ~ 190 km/s). Our spectropolarimetric observations yield a longitudinal magnetic field larger than 1 kG, and imply a rotational period shorter than 1.7 days. The spectrum of this very young object (age ~ 0.017 Myr) shows strong and variable lines of He and Si. We also detected a magnetic field in the 12.1 Msun B1 star OI 201 (NGC 2244; v sin i = 23.5 km/s). The Stokes V profile of this star does not vary over 5 days, suggesting a long rotational period, a pole-on orientation, or aligned magnetic and rotation axes. OI 201 is situtated near the Zero-Age Main Sequence on the HR diagram, and exhibits normal chemical abundances and no spectrum variability.

E. Alecian; G. A. Wade; C. Catala; S. Bagnulo; T. Boehm; D. Bohlender; J. -C. Bouret; J. -F. Donati; C. P. Folsom; J. Grunhut; J. D. Landstreet

2008-02-27T23:59:59.000Z

60

Discovery and geology of the Desert Peak geothermal field: a case history. Bulletin 97  

SciTech Connect

A case history of the exploration, development (through 1980), and geology of the Desert Peak geothermal field is presented. Sections on geochemistry, geophysics, and temperature-gradient drilling are included.

Benoit, W.R.; Hiner, J.E.; Forest, R.T.

1982-09-01T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Discovery of a weak magnetic field in the photosphere of the single giant Pollux  

E-Print Network (OSTI)

Aims: We observe the nearby, weakly-active single giant, Pollux, in order to directly study and infer the nature of its magnetic field. Methods: We used the new generation spectropolarimeters ESPaDOnS and NARVAL to observe and detect circular polarization within the photospheric absorption lines of Pollux. Our observations span 18 months from 2007-2009. We treated the spectropolarimetric data using the Least-Squares Deconvolution method to create high signal-to-noise ratio mean Stokes V profiles. We also measured the classical activity indicator S-index for the Ca H&K lines, and the stellar radial velocity (RV). Results: We have unambiguously detected a weak Stokes V signal in the spectral lines of Pollux, and measured the related surface-averaged longitudinal magnetic field Bl. The longitudinal field averaged over the span of the observations is below one gauss. Our data suggest variations of the longitudinal magnetic field, but no significant variation of the S-index. We observe variations of RV which a...

Aurire, M; Konstantinova-Antova, R; Charbonnel, C; Catala, C; Weiss, W W; Roudier, T; Petit, P; Donati, J -F; Alecian, E; Cabanac, R; Van Eck, S; Folsom, C P; Power, J

2009-01-01T23:59:59.000Z

62

Discovery of the magnetic field in the pulsating B star beta Cephei  

E-Print Network (OSTI)

Although the star itself is not He enriched, the periodicity and the variability in the UV wind lines of the pulsating B1 IV star beta Cep are similar to what is observed in magnetic He-peculiar B stars, suggesting that beta Cep is magnetic. We searched for a magnetic field using spectropolarimetry. From UV spectroscopy, we analysed the wind variability and investigated the correlation with the magnetic data. Using 130 time-resolved circular polarisation spectra, obtained with the MuSiCoS spectropolarimeter at the 2m TBL from 1998 until 2005, we applied the least-squares deconvolution method on the Stokes V spectra and derived the longitudinal component of the integrated magnetic field over the visible hemisphere of the star. We performed a period analysis on the magnetic data and on EW measurements of UV wind lines obtained over 17 years. We also analysed the short- and long-term radial velocity variations, which are due to the pulsations and the 90-year binary motion. beta Cep hosts a sinusoidally varying m...

Henrichs, H F; Verdugo, E; Schnerr, R S; Neiner, C; Donati, J -F; Catala, C; Shorlin, S L S; Wade, G A; Veen, P M; Nichols, J S; Damen, E M F; Talavera, A; Hill, G M; Kaper, L; Tijani, A M; Geers, V C; Wiersema, K; Plaggenborg, B; Rygl, K L J

2013-01-01T23:59:59.000Z

63

Estimating of pulsed electric fields using optical measurements.  

SciTech Connect

We performed optical electric field measurements ion nanosecond time scales using the electrooptic crystal beta barium borate (BBO). Tests were based on a preliminary bench top design intended to be a proofofprinciple stepping stone towards a modulardesign optical Efield diagnostic that has no metal in the interrogated environment. The long term goal is to field a modular version of the diagnostic in experiments on large scale xray source facilities, or similarly harsh environments.

Flanagan, Timothy McGuire; Chantler, Gary R.

2013-09-01T23:59:59.000Z

64

Oklahoma Coalbed Methane Proved Reserves New Reservoir Discoveries...  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Oklahoma Coalbed Methane Proved Reserves New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0...

65

Wyoming Coalbed Methane Proved Reserves New Reservoir Discoveries...  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Wyoming Coalbed Methane Proved Reserves New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0...

66

Utah Coalbed Methane Proved Reserves New Reservoir Discoveries...  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Utah Coalbed Methane Proved Reserves New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1...

67

Fuzzy logic based ELF magnetic field estimation in substations  

Science Journals Connector (OSTI)

......field strength in a combined cycle gas turbine power station were described...Sebo S. A., Caldecott R. Development of a computer program for modeling...buildings. (1995) Stockholm Power Technology Conference, 18-22 June. Stockholm......

Ilhan Kosalay

2008-08-01T23:59:59.000Z

68

Estimated gas reserves and availability of the Viking-Kinsella Field, Alberta, Canada  

E-Print Network (OSTI)

-KINSELVL FEEI' . ~. . . . . . . . . . ~ ~ ~ - ~ 3 '3 CIASSIF ICATION of RESERVES Proved Reserves Probable Reserves Possible Reserves 5 6 6 6 FUTURE AVAIIJBXLITY of PIPELINE GAS. . . . . . . . . . . . . . . . 6 Estimation of' Projected Peri...'ormance of Free Gas . . . . . . . 7 Estimated Projected Performance of' the Viking-Kinaella Field . 9 CONCWS ION ACKNOWLZDGEbEN1'S REFERENCES 13 TABUIAT I 0 NS I - Estimated Natnral Gas Reserves--viking sand IX - Projected Perf'ormance--Viking Sand 15...

Meyer, Lawrence Joffre

1952-01-01T23:59:59.000Z

69

PHOTO-CONSISTENCY AND MULTIRESOLUTION METHODS FOR LIGHT FIELD DISPARITY ESTIMATION  

E-Print Network (OSTI)

PHOTO-CONSISTENCY AND MULTIRESOLUTION METHODS FOR LIGHT FIELD DISPARITY ESTIMATION Adam Bowen for light fields: a global method based on the idea of photo-consistency and a local method which employs. Experimental results demonstrate the effectiveness of the two methods as compared to other photo

Rajpoot, Nasir

70

Estimation of lignite reserve in the Kalburcayiri field, Kangal basin, Sivas, Turkey  

Science Journals Connector (OSTI)

This paper addresses a case study on global estimation of lignite reserve in the Kalburcayiri field from the SivasKangal basin, which is one of the most productive lignite basins in eastern Anatolia, Turkey. The two lignite seams, which were developed in a fresh-water lacustrine depositional environment during the Pliocene time, are currently being exploited in the Kalburcayiri open-cast mine for feed coal to a power plant with 300-MW capacity. Tonnage, thickness and quality parameters (ash yield, total sulphur content, and calorific value) of the lignite are variables considered in this study. The global estimates of these variables together with 95% confidence limits are obtained using the approximation principle of global estimation. A random stratified grid is fitted to available boreholes; the variograms for thickness and lignite quality parameters are estimated and modeled. The models are used in calculating estimation error variances that will later be used in constructing 95% confidence intervals for the true values.

A.Erhan Tercan; Ali Ihsan Karayigit

2001-01-01T23:59:59.000Z

71

Gas, liquids flow rates hefty at Galveston Bay discovery  

SciTech Connect

Extended flow tests indicate a large Vicksburg (Oligocene) gas, condensate, and oil field is about to be developed in western Galveston Bay. Internal estimates indicates that ultimate recovery from the fault block in which the discovery well was drilled could exceed 1 tcf of gas equivalent of proved, possible, and probable reserves. The paper discusses the test program for this field and other prospects in the Galveston Bay area.

Petzet, G.A.

1998-01-19T23:59:59.000Z

72

OXYGEN ABUNDANCES IN LOW- AND HIGH-{alpha} FIELD HALO STARS AND THE DISCOVERY OF TWO FIELD STARS BORN IN GLOBULAR CLUSTERS  

SciTech Connect

Oxygen abundances of 67 dwarf stars in the metallicity range -1.6 < [Fe/H] < -0.4 are derived from a non-LTE analysis of the 777 nm O I triplet lines. These stars have precise atmospheric parameters measured by Nissen and Schuster, who find that they separate into three groups based on their kinematics and {alpha}-element (Mg, Si, Ca, Ti) abundances: thick disk, high-{alpha} halo, and low-{alpha} halo. We find the oxygen abundance trends of thick-disk and high-{alpha} halo stars very similar. The low-{alpha} stars show a larger star-to-star scatter in [O/Fe] at a given [Fe/H] and have systematically lower oxygen abundances compared to the other two groups. Thus, we find the behavior of oxygen abundances in these groups of stars similar to that of the {alpha} elements. We use previously published oxygen abundance data of disk and very metal-poor halo stars to present an overall view (-2.3 < [Fe/H] < +0.3) of oxygen abundance trends of stars in the solar neighborhood. Two field halo dwarf stars stand out in their O and Na abundances. Both G53-41 and G150-40 have very low oxygen and very high sodium abundances, which are key signatures of the abundance anomalies observed in globular cluster (GC) stars. Therefore, they are likely field halo stars born in GCs. If true, we estimate that at least 3% {+-} 2% of the local field metal-poor star population was born in GCs.

Ramirez, I. [McDonald Observatory and Department of Astronomy, University of Texas at Austin, 1 University Station, C1400 Austin, TX 78712-0259 (United States); Melendez, J. [Departamento de Astronomia do IAG/USP, Universidade de Sao Paulo, Rua do Matao 1226, Sao Paulo 05508-900, SP (Brazil); Chaname, J. [Departamento de Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile, Av. Vicuna Mackenna 4860, 782-0436 Macul, Santiago (Chile)

2012-10-01T23:59:59.000Z

73

The Use of Tall Tower Field Data for Estimating Wind Turbine Power Performance , J. Chapman1  

E-Print Network (OSTI)

The Use of Tall Tower Field Data for Estimating Wind Turbine Power Performance A. Swift1 , J wind speed measurements on the TTU WISE 200m and 78m towers. A hypothetical wind turbine is shown. At potential wind turbine sites, it is uncommon to have wind measurements available at multiple heights. Then

Manuel, Lance

74

Observed oil and gas field size distributions: A consequence of the discovery process and prices of oil and gas  

Science Journals Connector (OSTI)

If observed oil and gas field size distributions are obtained ... should approximate that of the parent population of oil and gas fields. However, empirical evidence ... the observable size distributions change w...

Lawrence J. Drew; Emil D. Attanasi; John H. Schuenemeyer

1988-11-01T23:59:59.000Z

75

Analytic estimation of the Lyapunov exponent in a mean-field model undergoing a phase transition  

Science Journals Connector (OSTI)

The parametric instability contribution to the largest Lyapunov exponent ?1 is derived for a mean-field Hamiltonian model, with attractive long-range interactions. This uses a recent Riemannian approach to describe Hamiltonian chaos with a large number N of degrees of freedom. Through microcanonical estimates of suitable geometrical observables, the mean-field behavior of ?1 is analytically computed and related to the second-order phase transition undergone by the system. It predicts that chaoticity drops to zero at the critical temperature and remains vanishing above it, with ?1 scaling as N-(1/3) to the leading order in N.

Marie-Christine Firpo

1998-06-01T23:59:59.000Z

76

Discovery of a strong magnetic field on the O star HD 191612: new clues to the future of theta1 Orionis C?  

E-Print Network (OSTI)

From observations made with the ESPaDOnS spectropolarimeter, recently installed on the 3.6-m Canada--France--Hawaii Telescope, we report the discovery of a strong magnetic field in the Of?p spectrum variable HD 191612 -- only the second known magnetic O star (following theta1 Ori C). The stability of the observed Zeeman signature over four nights of observation, together with the non-rotational shape of line profiles, argue that the rotation period of HD 191612 is significantly longer than the 9-d value previously proposed. We suggest that the recently identified 538-d spectral-variability period is the rotation period, in which case the observed line-of-sight magnetic field of -220+-38 G implies a large-scale field (assumed dipolar) with a polar strength of about -1.5 kG. If confirmed, this scenario suggests that HD 191612 is, essentially, an evolved version of the near-ZAMS magnetic O star theta1 Ori C, but with an even stronger field (about 15 kG at an age similar to that of theta1Ori C). We suggest that t...

Donati, J F; Bouret, J C; Petit, P; Catala, C; Landstreet, J D; Donati, JF; Howarth, ID; Bouret, JC; Landstreet, JD

2006-01-01T23:59:59.000Z

77

Estimated human health risks of disposing of nonhazardous oil field waste in salt caverns  

SciTech Connect

Argonne National Laboratory (ANL) has completed an evaluation of the possibility that adverse human health effects (carcinogenic and noncarcinogenic) could result from exposure to contaminants released from nonhazardous oil field wastes (NOW) disposed in domal salt caverns. In this assessment, several steps were used to evaluate potential human health risks: identifying potential contaminants of concern, determining how humans could be exposed to these contaminants, assessing the contaminants` toxicities, estimating contaminant intakes, and, finally, calculating human cancer and noncancer risks.

Tomasko, D.; Elcock, D.; Veil, J.

1997-09-01T23:59:59.000Z

78

U.S. Coalbed Methane Proved Reserves New Reservoir Discoveries...  

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

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) U.S. Coalbed Methane Proved Reserves New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1...

79

Lab and field estimates of active time of chemical alarm cues of a cyprinid fish and an  

E-Print Network (OSTI)

Lab and field estimates of active time of chemical alarm cues of a cyprinid fish and an amphipod., 1999; Stankowich, 2008), seismic (Gregory et al., 1986) and vibratory mechanostimuli (Kirchner et al

Wisenden, Brian D.

80

Estimate of the risks of disposing nonhazardous oil field wastes into salt caverns  

SciTech Connect

Argonne National Laboratory (ANL) has completed an evaluation of the possibility that adverse human health effects (carcinogenic and noncarcinogenic) could result from exposure to contaminants released from nonhazardous oil field wastes (NOW) disposed in domal salt caverns. Potential human health risks associated with hazardous substances (arsenic, benzene, cadmium, and chromium) in NOW were assessed under four postclosure cavern release scenarios: inadvertent cavern intrusion, failure of the cavern seal, failure of the cavern through cracks or leaky interbeds, and a partial collapse of the cavern roof. To estimate potential human health risks for these scenarios, contaminant concentrations at the receptor were calculated using a one-dimensional solution to an advection/dispersion equation that included first order degradation. Assuming a single, generic salt cavern and generic oil-field wastes, the best-estimate excess cancer risks ranged from 1.7 {times} 10{sup {minus}12} to 1.1 {times} 10{sup {minus}8} and hazard indices (referring to noncancer health effects) ranged from 7 {times} 10{sup {minus}9} to 7 {times} 10{sup {minus}4}. Under worse-case conditions in which the probability of cavern failure is 1.0, excess cancer risks ranged from 4.9 {times} 10{sup {minus}9} to 1.7 {times} 10{sup {minus}5} and hazard indices ranged from 7.0 {times} 10{sup {minus}4} to 0.07. Even under worst-case conditions, the risks are within the US Environmental Protection Agency (EPA) target range for acceptable exposure levels. From a human health risk perspective, salt caverns can, therefore, provide an acceptable disposal method for NOW.

Tomasko, D.; Elcock, D.; Veil, J.

1997-12-31T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Estimation of expected human attention weights based on a decision field theory model  

Science Journals Connector (OSTI)

Abstract Modeling human decision making behavior is of great interest in understanding how a decision maker weights different decision attributes when making a decision. Such knowledge is critically important in helping predict future decisions, evaluating human decision performance, and improving the design of human and machine interface systems. Decision field theory (DFT) provides a psychological representation of the cognitive deliberation process, which is driven by the fluctuations of a persons attention among decision attributes. In this research area, the most common use of a DFT model is to estimate or predict the human decisions by using a set of pre-specified expected attention weights (EAWs) in the DFT model. Unlike other research, this paper extends the capabilities of DFT in a complementary direction, showing how to fit or train a DFT model by estimating the EAW based on sequentially obtained samples of decision trials. Furthermore, the inherent connection between the EAW and the decision choice uncertainty is investigated. The proposed modeling method is discussed in detail for a two-alternative decision scenario based on two attributes. Both simulations and a case study are conducted in the paper to demonstrate the effectiveness of the proposed modeling approach.

Andres G. Abad; Jionghua (Judy) Jin; Young-Jun Son

2014-01-01T23:59:59.000Z

82

Discoveries mount in E. Texas Cotton Valley pinnacle reef play  

SciTech Connect

Another sizable discovery and more operators are popping up in the expanding East Texas Jurassic Cotton Valley pinnacle reef gas play. Sonat Exploration Co., Houston, reported a large discovery and sizable participation in the play in late April. Sonat and its partners join Marathon Oil Co., which has dominated the play the past few years. Sonat started sales April from the 1 Fountain, a new field discovery in northwestern Leon County between McSwane and Branton gas fields. The discovery flowed at a rate of 30.3 MMcfd of gas with 5,060 psi flowing well-head pressure. TD is 14,379 ft. Sonat estimated reserves at the well, possibly the only one to be drilled into the reef, at 70--80 bcf of gas. Sonat in late April formed a joint venture to explore the trend with UMC Petroleum Corp., Houston, and two smaller private companies, Aspect Resources and MB Exploration. A map of the combined acreage was not available from Sonat at press time, but the accompanying map indicates UMC`s position as presented to financial analysts earlier this year.

Petzet, G.A.

1996-05-06T23:59:59.000Z

83

Coalbed Methane New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

0 0 0 2009-2011 0 0 0 2009-2011 Federal Offshore U.S. 0 0 0 2009-2011 Pacific (California) 0 0 0 2009-2011 Louisiana & Alabama 0 0 0 2009-2011 Texas 0 0 0 2009-2011 Alaska 0 0 0 2009-2011 Lower 48 States 0 0 0 2009-2011 Alabama 0 0 0 2009-2011 Arkansas 0 0 0 2009-2011 California 0 0 0 2009-2011 Coastal Region Onshore 0 0 0 2009-2011 Los Angeles Basin Onshore 0 0 0 2009-2011 San Joaquin Basin Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Colorado 0 0 0 2009-2011 Florida 0 0 0 2009-2011 Kansas 0 0 0 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 0 0 0 2009-2011 North 0 0 0 2009-2011 South Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Michigan 0 0 0 2009-2011 Mississippi 0 0 0 2009-2011 Montana 0 0 0 2009-2011 New Mexico

84

Coalbed Methane New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

0 0 0 2009-2011 0 0 0 2009-2011 Federal Offshore U.S. 0 0 0 2009-2011 Pacific (California) 0 0 0 2009-2011 Louisiana & Alabama 0 0 0 2009-2011 Texas 0 0 0 2009-2011 Alaska 0 0 0 2009-2011 Lower 48 States 0 0 0 2009-2011 Alabama 0 0 0 2009-2011 Arkansas 0 0 0 2009-2011 California 0 0 0 2009-2011 Coastal Region Onshore 0 0 0 2009-2011 Los Angeles Basin Onshore 0 0 0 2009-2011 San Joaquin Basin Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Colorado 0 0 0 2009-2011 Florida 0 0 0 2009-2011 Kansas 0 0 0 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 0 0 0 2009-2011 North 0 0 0 2009-2011 South Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Michigan 0 0 0 2009-2011 Mississippi 0 0 0 2009-2011 Montana 0 0 0 2009-2011 New Mexico

85

Stellar loci II. a model-free estimate of the binary fraction for field FGK stars  

E-Print Network (OSTI)

We propose a Stellar Locus OuTlier (SLOT) method to determine the binary fraction of main-sequence stars statistically. The method is sensitive to neither the period nor mass-ratio distributions of binaries, and able to provide model-free estimates of binary fraction for large numbers of stars of different populations in large survey volumes. We have applied the SLOT method to two samples of stars from the SDSS Stripe 82, constructed by combining the re-calibrated SDSS photometric data with respectively the spectroscopic information from the SDSS and LAMOST surveys. For the SDSS spectroscopic sample, we find an average binary fraction for field FGK stars of $41%\\pm2%$. The fractions decrease toward late spectral types, and are respectively $44%\\pm5%$, $43%\\pm3%$, $35%\\pm5%$, and $28%\\pm6%$ for stars of $g-i$ colors between 0.3 -- 0.6, 0.6 -- 0.9, 0.9 -- 1.2, and 1.2 - 1.6\\,mag. A modest metallicity dependence is also found. The fraction decreases with increasing metallicity. For stars of [Fe/H] between $-0.5$...

Yuan, Haibo; Xiang, Maosheng; Huang, Yang; Chen, Bingqiu

2014-01-01T23:59:59.000Z

86

Open-Source LCA Tool for Estimating Greenhouse Gas Emissions from Crude Oil Production Using Field Characteristics  

Science Journals Connector (OSTI)

Open-Source LCA Tool for Estimating Greenhouse Gas Emissions from Crude Oil Production Using Field Characteristics ... OPGEE models oil production emissions in more detail than previous transport LCA models. ... El-Houjeiri, H. and Brandt, A.Exploring the variation of GHG emissions from conventional oil production using an engineering-based LCA model. ...

Hassan M. El-Houjeiri; Adam R. Brandt; James E. Duffy

2013-05-01T23:59:59.000Z

87

UK now claims world's top discovery rate  

SciTech Connect

UK explorers are a bit more cheerful these days even though no one has discovered a giant field or anything elephant-sized. The reason is a benign tax regime and a growing confidence among industry explorers. This last has resulted in discovery of many smaller fields - particularly gas, some potentially commercial. It is claimed that the UK's discovery rate is now the highest in the world.

Not Available

1985-05-01T23:59:59.000Z

88

Field Validation of the Clean Power Estimator's Obstruction Analysis Algorithm Richard Perez  

E-Print Network (OSTI)

for obstruction analysis #12;the solar collector location (e.g., on an inaccessible, not- yet-built roof). Once produced by the Solar PathfinderTM (SPF). Results indicate that the Estimator provides acceptable estimates tables for two configurations: horizontal and south-facing at 30o-tilt. These tables are used to generate

Perez, Richard R.

89

,"U.S. Coalbed Methane Proved Reserves New Reservoir Discoveries...  

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

Name","Description"," Of Series","Frequency","Latest Data for" ,"Data 1","U.S. Coalbed Methane Proved Reserves New Reservoir Discoveries in Old Fields (Billion Cubic...

90

Quantum Field Theory & Gravity  

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

Field Theory & Gravity Quantum Field Theory & Gravity Understanding discoveries at the Energy, Intensity, and Cosmic Frontiers Get Expertise Rajan Gupta (505) 667-7664 Email...

91

Development of a potential field estimator for a path-planning application using neural networks  

E-Print Network (OSTI)

-field method[2]. This design has been modified for performance and for compatibility with &&ther aiialysis tools used at X~ASA's Johnson Spaceflight Center (JSC). The current focus of the research is i he addition of adapt; ability functions to the pot...-field method[2]. This design has been modified for performance and for compatibility with &&ther aiialysis tools used at X~ASA's Johnson Spaceflight Center (JSC). The current focus of the research is i he addition of adapt; ability functions to the pot...

Smith, Darin William

2012-06-07T23:59:59.000Z

92

Supercomputing | Knowledge Discovery | ORNL  

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

Mobile Applications Streaming/Real-time Data Data System Architectures for National Security Sensor Networks Visual Analytics Risk Analysis Materials Mathematics National Security Systems Modeling Engineering Analysis Behavioral Sciences Geographic Information Science and Technology Quantum Information Science Supercomputing and Computation Home | Science & Discovery | Supercomputing and Computation | Research Areas | Knowledge Discovery SHARE Knowledge Discovery The national level grand challenge in Computer Science is the ability to acquire, reduce, analyze and extract meaning from massive amounts of data. ORNL is studying methods for the discovery of "hidden laws and processes" underlying observable behaviors in complex systems. ORNL researchers are

93

Decades of Discovery  

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

of microwave background radiation, when combined with the eventual discovery of dark matter, will unify physics on the largest and smallest scales, fusing together the...

94

High-resolution stratospheric tracer fields estimated from satellite observations using Lagrangian trajectory calculations  

SciTech Connect

A technique is introduced by which high-resolution tracer fields may be constructed from low-resolution satellite observations. The technique relies upon the continual cascade of tracer variance from large to small scales and makes use of wind fields generated by a data assimilation scheme. To demonstrate its usefulness, the technique has been applied in a study of isentropic distributions of nitrous oxide in the winter midstratosphere, using measurements made by the Improved Stratospheric and Mesospheric Sounder (ISAMS) instrument on the Upper Atmosphere Research Satellite (UARS). The results show that the high-resolution fields significantly increase the amount of information that is available from the satellite observations. The fields give insights into the characteristic structure and evolution of tracer distributions at scales that are normally obscured from view. Two results are particularly noteworthy. First, at the interface between low and middle latitudes there is evidence of active mixing. This mixing occurs on the eastern, equatorward side of air that is being drawn toward high latitudes around the polar vortex. Second, in the anticyclone, a complex pattern of transport is revealed. Air drawn in from low latitudes spirals together with ambient midlatitude air. Small scales are generated relatively slowly in the organized flow, and persistent filamentary structures, with transverse scales of hundreds of kilometers or greater, are seen.

Sutton, R.T.; Maclean, H.; Swinbank, R.; O`Neill, A.; Taylor, F.W. [Oxford Univ., Oxford (United Kingdom)] [Oxford Univ., Oxford (United Kingdom); [Meteorological Office, Bracknell, Berkshire (United Kingdom); [Univ. of Reading, Reading (United Kingdom)

1994-10-01T23:59:59.000Z

95

Estimation of heat and chemical fluxes from a seafloor hydrothermal vent field using radon measurements  

Science Journals Connector (OSTI)

... exists at about 200 m above the depth of the vent field12'13. Distinct excess radon levels have been observed at Endeavour both in vent water and in the effluent plume ... vent water and in the effluent plume up to 17 km from the ridge axis14.Radon is a chemically inert gas with a radioactive half life of 3.85 days. ...

N. D. Rosenberg; J. E. Lupton; D. Kadko; R. Collier; M. D. Lilley; H. Pak

1988-08-18T23:59:59.000Z

96

Challenges of Antibacterial Discovery  

Science Journals Connector (OSTI)

...noninferiority standards. In late 2009...Pharma, which plans to continue development...detail in several reviews (5, 64, 97...terms of this review, even if we...discovery. Thus, if standard drug discovery...thrusts of this review have been 2-fold...problems are the standard, and considerable...

Lynn L. Silver

2011-01-01T23:59:59.000Z

97

Submillimetre sources in rich cluster fields - source counts, redshift estimates, and cooling flow limits  

E-Print Network (OSTI)

Recent submillimetre surveys have revealed a population of dusty, high redshift sources of great cosmological significance for understanding dust-enshrouded star formation in distant galaxies, and for determining the origin of the far-IR background. In this paper, we analyze nine rich cluster fields mapped at 850 and 450 microns with the SCUBA array on the James Clerk Maxwell telescope. Lensing models of the clusters are developed in order to derive accurate source counts for our sample. VLA maps of the same clusters are used to help constrain the redshift distribution of our SCUBA detections. Implications for high redshift galaxies and for the far-IR background are discussed. We also provide limits on distributed dust produced by cooling flows in these clusters.

Scott C. Chapman; Douglas Scott; Colin Borys; Gregory G. Fahlman

2000-09-05T23:59:59.000Z

98

The iron $K_?$ lines as a tool for magnetic field estimations in non-flat accretion flows  

E-Print Network (OSTI)

Observations of AGNs and microquasars by ASCA, RXTE, Chandra and XMM-Newton indicate the existence of broad X-ray emission lines of ionized heavy elements in their spectra. Such spectral lines were discovered also in X-ray spectra of neutron stars and X-ray afterglows of GRBs. Recently, Zakharov et al. (MNRAS, 2003, 342, 1325) described a procedure to estimate an upper limit of the magnetic fields in regions from which X-ray photons are emitted. The authors simulated typical profiles of the iron $K_\\alpha$ line in the presence of magnetic field and compared them with observational data in the framework of the widely accepted accretion disk model. Here we further consider typical Zeeman splitting in the framework of a model of non-flat accretion flows, which is a generalization of previous consideration into non-equatorial plane motion of particles emitting X-ray photons. Using perspective facilities of space borne instruments (e.g. Constellation-X mission) a better resolution of the blue peak structure of iron $K_\\alpha$ line will allow to evaluate the magnetic fields with higher accuracy.

A. F. Zakharov; Z. Ma; Y. Bao

2004-11-22T23:59:59.000Z

99

Investigation of the magnetic field characteristics of Herbig Ae/Be stars: Discovery of the pre-main sequence progenitors of the magnetic Ap/Bp stars  

E-Print Network (OSTI)

We are investigating the magnetic characteristics of pre-main sequence Herbig Ae/Be stars, with the aim of (1) understanding the origin and evolution of magnetism in intermediate-mass stars, and (2) exploring the influence of magnetic fields on accretion, rotation and mass-loss at the early stages of evolution of A, B and O stars. We have begun by conducting 2 large surveys of Herbig Ae/Be stars, searching for direct evidence of photospheric magnetic fields via the longitudinal Zeeman effect. From observations obtained using FORS1 at the ESO-VLT and ESPaDOnS at the Canada-France-Hawaii Telescope, we report the confirmed detection of magnetic fields in 4 pre-main sequence A- and B-type stars, and the apparent (but as yet unconfirmed) detection of fields in 2 other such stars. We do not confirm the detection of magnetic fields in several stars reported by other authors to be magnetic: HD 139614, HD 144432 or HD 31649. One of the most evolved stars in the detected sample, HD 72106A, shows clear evidence of stron...

Wade, G A; Bagnulo, S; Landstreet, J D; Mason, E; Silvester, J; Alecian, E; Bhm, T; Bouret, J C; Catala, C; Donati, J F; Folsom, C; Bale, K

2006-01-01T23:59:59.000Z

100

Investigation of the magnetic field characteristics of Herbig Ae/Be stars: Discovery of the pre-main sequence progenitors of the magnetic Ap/Bp stars  

E-Print Network (OSTI)

We are investigating the magnetic characteristics of pre-main sequence Herbig Ae/Be stars, with the aim of (1) understanding the origin and evolution of magnetism in intermediate-mass stars, and (2) exploring the influence of magnetic fields on accretion, rotation and mass-loss at the early stages of evolution of A, B and O stars. We have begun by conducting 2 large surveys of Herbig Ae/Be stars, searching for direct evidence of photospheric magnetic fields via the longitudinal Zeeman effect. From observations obtained using FORS1 at the ESO-VLT and ESPaDOnS at the Canada-France-Hawaii Telescope, we report the confirmed detection of magnetic fields in 4 pre-main sequence A- and B-type stars, and the apparent (but as yet unconfirmed) detection of fields in 2 other such stars. We do not confirm the detection of magnetic fields in several stars reported by other authors to be magnetic: HD 139614, HD 144432 or HD 31649. One of the most evolved stars in the detected sample, HD 72106A, shows clear evidence of strong photospheric chemical peculiarity, whereas many of the other (less evolved) stars do not. The magnetic fields that we detect appear to have surface intensities of order 1 kG, seem to be structured on global scales, and appear in about 10% of the stars studied. Based on these properties, these magnetic stars appear to be pre-main sequence progenitors of the magnetic Ap/Bp stars.

G. A. Wade; D. Drouin; S. Bagnulo; J. D. Landstreet; E. Mason; J. Silvester; E. Alecian; T. Bohm; J. -C. Bouret; C. Catala; J. -F. Donati; C. Folsom; K. Bale

2006-01-30T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Potential for CO2 storage in depleted fields on the Dutch Continental ShelfCost estimate for offshore facilities  

Science Journals Connector (OSTI)

A study was performed on capital and operational costs for offshore injection of CO2 into depleted fields. The main focus was on the design and costs of process requirements for injection, required conservation (hibernation) and modification of existing platforms between end of gas/oil production and start of CO2 injection. Also cost estimates for new platforms are provided. The study is high level and generic in nature as no specific target for CO2 storage has been selected. For the purpose of this study a simplified approach is used for determination of the required injection facilities and platform modifications. Nevertheless, the study provides a good indication on the level of expenditures that can be expected.

Floor Jansen; Rob Steinz; Boudewijn van Gelder

2011-01-01T23:59:59.000Z

102

900-MHz NMR: Accelerating Scientific Discovery  

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

00-MHz NMR: Accelerating Scientific 00-MHz NMR: Accelerating Scientific Discovery Scientific Innovation Through Integration 900-MHz NMR: Accelerating Scientific Discovery 900-MHz NMR: Accelerating Scientific Discovery Introduction When the U.S. Department of Energy's (DOE's) Office of Biological and Environmental Research approved the development and purchase of the world's first 900-MHz NMR (nuclear magnetic resonance) spectrometer in 1992, the highest magnetic field available was 750 MHz. DOE's decision and the ultimate success of its 900-MHz NMR spectrometer, which recently saw its five-year anniversary of operation at EMSL, catalyzed the development of a new generation of ultrahigh-field NMR spectrometers worldwide. Building new technology Building the magnet for the 900-MHz NMR spectrometer brought engineering challenges. Can the

103

Price discovery in crude oil futures  

Science Journals Connector (OSTI)

Abstract This study examines price discovery among the two most prominent price benchmarks in the market for crude oil, WTI sweet crude and Brent sweet crude. Using data on the most active futures contracts measured at the one-second frequency, we find that WTI maintains a dominant role in price discovery relative to Brent, with an estimated information share in excess of 80%, over a sample from 2007 to 2012. Our analysis is robust to different decompositions of the sample, over pit-trading sessions and non-pit trading sessions, segmentation of days associated with major economic news releases, and data measured to the millisecond. We find no evidence that the dominant role of WTI in price discovery is diminished by the price spread between Brent that emerged in 2008.

John Elder; Hong Miao; Sanjay Ramchander

2014-01-01T23:59:59.000Z

104

Discovery Research in Magnetic Fusion Energy  

E-Print Network (OSTI)

magnetic tori? � Fundamental study � Confinement science, heating, sustainment, heat flux to boundariesDiscovery Research in Magnetic Fusion Energy or "How we learn about magnetic containment the shape of the magnetic field � What can we learn by changing magnetic topology? Examples... � Stellarator

Mauel, Michael E.

105

field  

National Nuclear Security Administration (NNSA)

9%2A en Ten-Year Site Plans (TYSP) http:nnsa.energy.govaboutusouroperationsinfopsinfopstysp

field field-type-text field-field-page-name">

106

Science & Discovery | ORNL  

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

Advanced Materials Advanced Materials Clean Energy National Security Neutron Science Nuclear Science Supercomputing and Computation More Science Hubs, Centers and Institutes US ITER Mars 'Curiosity' has ORNL tech New family of tiny crystals glows bright in LED lights Home | Science & Discovery SHARE Science & Discovery As the US Department of Energy's largest multi-program laboratory, ORNL is engaged in a wide range of activities that support the department's mission of ensuring America's security and prosperity by addressing its energy and environmental challenges. To accomplish this, the laboratory applies a remarkable portfolio of scientific expertise and world-class scientific facilities and equipment to develop scientific and technological solutions. ORNL focuses these resources on delivering scientific discoveries and new

107

Natural Gas Liquids New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

35 26 32 16 30 65 1979-2008 35 26 32 16 30 65 1979-2008 Federal Offshore U.S. 25 7 21 6 24 22 1981-2008 Pacific (California) 0 0 0 0 0 0 1979-2008 Louisiana & Alabama 25 7 21 6 13 22 1981-2008 Texas 0 0 0 0 11 0 1981-2008 Alaska 0 0 0 0 0 0 1979-2008 Lower 48 States 35 26 32 16 30 65 1979-2008 Alabama 0 0 0 0 0 0 1979-2008 Arkansas 0 0 0 0 0 0 1979-2008 California 0 0 0 0 0 0 1979-2008 Coastal Region Onshore 0 0 0 0 0 0 1979-2008 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2008 San Joaquin Basin Onshore 0 0 0 0 0 0 1979-2008 State Offshore 0 0 0 0 0 0 1979-2008 Colorado 0 4 1 0 0 0 1979-2008 Florida 0 0 0 0 0 0 1979-2008 Kansas 0 0 0 0 0 0 1979-2008 Kentucky 0 0 1 0 0 0 1979-2008 Louisiana 0 0 0 1 0 3 1981-2008

108

Shale Natural Gas New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

868 557 232 2009-2011 868 557 232 2009-2011 Alaska 0 0 0 2009-2011 Lower 48 States 868 557 232 2009-2011 Alabama 0 0 2009-2010 Arkansas 0 0 0 2009-2011 California 0 2011-2011 San Joaquin Basin Onshore 0 2011-2011 Colorado 4 0 0 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 244 48 0 2009-2011 North 244 48 0 2009-2011 Michigan 0 2 0 2009-2011 Montana 0 0 0 2009-2011 New Mexico 0 0 0 2009-2011 East 0 0 0 2009-2011 West 0 0 0 2009-2011 North Dakota 6 8 2 2009-2011 Ohio 0 0 2009-2010 Oklahoma 0 54 37 2009-2011 Pennsylvania 120 49 162 2009-2011 Texas 353 396 31 2009-2011 RRC District 1 353 114 20 2009-2011 RRC District 2 Onshore 282 0 2010-2011 RRC District 3 Onshore 0 0 0 2009-2011 RRC District 4 Onshore 0 0 0 2009-2011 RRC District 5 0 0 0 2009-2011

109

Natural Gas Liquids New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

35 26 32 16 30 65 1979-2008 35 26 32 16 30 65 1979-2008 Federal Offshore U.S. 25 7 21 6 24 22 1981-2008 Pacific (California) 0 0 0 0 0 0 1979-2008 Louisiana & Alabama 25 7 21 6 13 22 1981-2008 Texas 0 0 0 0 11 0 1981-2008 Alaska 0 0 0 0 0 0 1979-2008 Lower 48 States 35 26 32 16 30 65 1979-2008 Alabama 0 0 0 0 0 0 1979-2008 Arkansas 0 0 0 0 0 0 1979-2008 California 0 0 0 0 0 0 1979-2008 Coastal Region Onshore 0 0 0 0 0 0 1979-2008 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2008 San Joaquin Basin Onshore 0 0 0 0 0 0 1979-2008 State Offshore 0 0 0 0 0 0 1979-2008 Colorado 0 4 1 0 0 0 1979-2008 Florida 0 0 0 0 0 0 1979-2008 Kansas 0 0 0 0 0 0 1979-2008 Kentucky 0 0 1 0 0 0 1979-2008 Louisiana 0 0 0 1 0 3 1981-2008

110

Shale Natural Gas New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

868 557 232 2009-2011 868 557 232 2009-2011 Alaska 0 0 0 2009-2011 Lower 48 States 868 557 232 2009-2011 Alabama 0 0 2009-2010 Arkansas 0 0 0 2009-2011 California 0 2011-2011 San Joaquin Basin Onshore 0 2011-2011 Colorado 4 0 0 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 244 48 0 2009-2011 North 244 48 0 2009-2011 Michigan 0 2 0 2009-2011 Montana 0 0 0 2009-2011 New Mexico 0 0 0 2009-2011 East 0 0 0 2009-2011 West 0 0 0 2009-2011 North Dakota 6 8 2 2009-2011 Ohio 0 0 2009-2010 Oklahoma 0 54 37 2009-2011 Pennsylvania 120 49 162 2009-2011 Texas 353 396 31 2009-2011 RRC District 1 353 114 20 2009-2011 RRC District 2 Onshore 282 0 2010-2011 RRC District 3 Onshore 0 0 0 2009-2011 RRC District 4 Onshore 0 0 0 2009-2011 RRC District 5 0 0 0 2009-2011

111

Real-time data processing and magnetic field pitch angle estimation of the JET motional Stark effect diagnostic based on Kalman filtering  

SciTech Connect

A novel technique for the real-time measurement of the magnetic field pitch angle in JET discharges using the motional Stark effect diagnostic is presented. Kalman filtering techniques are adopted to estimate the amplitude of the avalanche photodiode signals' harmonics that are relevant for the pitch angle calculation. The proposed technique {l_brace}for extended technical details of the generic algorithm see [R. Coelho and D. Alves, IEEE Trans. Plasma Sci. 37, 164 (2009)]{r_brace} is shown to be much more robust and provides less noisy estimates than an equivalent lock-in amplifier scheme, in particular when dealing with edge localized modes.

Coelho, R.; Alves, D. [Instituto de Plasmas e Fusao Nuclear, Associacao Euratom/IST, 1049-001 Lisboa (Portugal); Hawkes, N.; Brix, M. [Euratom/UKAEA Fusion Association, Culham Science Centre, Abingdon, Oxon, OX14 3DB (United Kingdom); Collaboration: JET EFDA Contributors

2009-06-15T23:59:59.000Z

112

Physiological observations validate finite element models for estimating subject-specific electric field distributions induced by transcranial magnetic stimulation of the human motor cortex  

Science Journals Connector (OSTI)

Abstract Recent evidence indicates subject-specific gyral folding patterns and white matter anisotropy uniquely shape electric fields generated by TMS. Current methods for predicting the brain regions influenced by TMS involve projecting the TMS coil position or center of gravity onto realistic head models derived from structural and functional imaging data. Similarly, spherical models have been used to estimate electric field distributions generated by TMS pulses delivered from a particular coil location and position. In the present paper we inspect differences between electric field computations estimated using the finite element method (FEM) and projection-based approaches described above. We then more specifically examined an approach for estimating cortical excitation volumes based on individualistic FEM simulations of electric fields. We evaluated this approach by performing neurophysiological recordings during MR-navigated motormapping experiments. We recorded motor evoked potentials (MEPs) in response to single pulse TMS using two different coil orientations (45 and 90 to midline) at 25 different locations (5נ5 grid, 1cm spacing) centered on the hotspot of the right first dorsal interosseous (FDI) muscle in left motor cortex. We observed that motor excitability maps varied within and between subjects as a function of TMS coil position and orientation. For each coil position and orientation tested, simulations of the TMS-induced electric field were computed using individualistic FEM models and compared to MEP amplitudes obtained during our motormapping experiments. We found FEM simulations of electric field strength, which take into account subject-specific gyral geometry and tissue conductivity anisotropy, significantly correlated with physiologically observed MEP amplitudes (rmax=0.91, p=1.8נ10-5 rmean=0.81, p=0.01). These observations validate the implementation of individualistic FEM models to account for variations in gyral folding patterns and tissue conductivity anisotropy, which should help improve the targeting accuracy of TMS in the mapping or modulation of human brain circuits.

Alexander Opitz; Wynn Legon; Abby Rowlands; Warren K. Bickel; Walter Paulus; William J. Tyler

2013-01-01T23:59:59.000Z

113

Price discovery in energy markets  

Science Journals Connector (OSTI)

Abstract In this study, we empirically analyze the price discovery process in the futures and spot markets for crude oil, heating oil and natural gas using daily closing prices. We use two different information share measures that are based on the methods proposed by Gonzalo and Granger (1995) and Lien and Shrestha (2014). Both measures indicate that almost all the price discovery takes place in the futures markets for the heating oil and natural gas. However, for the crude oil, the price discovery takes place both in the futures and spot markets. As a whole, our study indicates that futures markets play an important role in the price discovery process.

Keshab Shrestha

2014-01-01T23:59:59.000Z

114

Sample size requirements for estimating effective dose from computed tomography using solid-state metal-oxide-semiconductor field-effect transistor dosimetry  

SciTech Connect

Purpose: Effective dose (ED) is a widely used metric for comparing ionizing radiation burden between different imaging modalities, scanners, and scan protocols. In computed tomography (CT), ED can be estimated by performing scans on an anthropomorphic phantom in which metal-oxide-semiconductor field-effect transistor (MOSFET) solid-state dosimeters have been placed to enable organ dose measurements. Here a statistical framework is established to determine the sample size (number of scans) needed for estimating ED to a desired precision and confidence, for a particular scanner and scan protocol, subject to practical limitations. Methods: The statistical scheme involves solving equations which minimize the sample size required for estimating ED to desired precision and confidence. It is subject to a constrained variation of the estimated ED and solved using the Lagrange multiplier method. The scheme incorporates measurement variation introduced both by MOSFET calibration, and by variation in MOSFET readings between repeated CT scans. Sample size requirements are illustrated on cardiac, chest, and abdomenpelvis CT scans performed on a 320-row scanner and chest CT performed on a 16-row scanner. Results: Sample sizes for estimating ED vary considerably between scanners and protocols. Sample size increases as the required precision or confidence is higher and also as the anticipated ED is lower. For example, for a helical chest protocol, for 95% confidence and 5% precision for the ED, 30 measurements are required on the 320-row scanner and 11 on the 16-row scanner when the anticipated ED is 4 mSv; these sample sizes are 5 and 2, respectively, when the anticipated ED is 10 mSv. Conclusions: Applying the suggested scheme, it was found that even at modest sample sizes, it is feasible to estimate ED with high precision and a high degree of confidence. As CT technology develops enabling ED to be lowered, more MOSFET measurements are needed to estimate ED with the same precision and confidence.

Trattner, Sigal [Department of Medicine, Division of Cardiology, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York 10032 (United States)] [Department of Medicine, Division of Cardiology, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York 10032 (United States); Cheng, Bin [Department of Biostatistics, Columbia University Mailman School of Public Health, New York, New York 10032 (United States)] [Department of Biostatistics, Columbia University Mailman School of Public Health, New York, New York 10032 (United States); Pieniazek, Radoslaw L. [Center for Radiological Research, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York 10032 (United States)] [Center for Radiological Research, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York 10032 (United States); Hoffmann, Udo [Department of Radiology, Massachusetts General Hospital and Harvard Medical School, Boston, Massachusetts 02114 (United States)] [Department of Radiology, Massachusetts General Hospital and Harvard Medical School, Boston, Massachusetts 02114 (United States); Douglas, Pamela S. [Department of Medicine, Division of Cardiology, Duke University, Durham, North Carolina 27715 (United States)] [Department of Medicine, Division of Cardiology, Duke University, Durham, North Carolina 27715 (United States); Einstein, Andrew J., E-mail: andrew.einstein@columbia.edu [Department of Medicine, Division of Cardiology, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York and Department of Radiology, Columbia University Medical Center and New York-Presbyterian Hospital, New York, New York (United States)

2014-04-15T23:59:59.000Z

115

Estimation of the Residual Magnetic Field Strength Inside a Pipeline after Testing by a Magnetic Flaw Detector  

Science Journals Connector (OSTI)

The residual magnetic field strength inside a pipeline after testing by a magnetic flaw detector ... demagnetizing local joint-pipe sections in carrying out repair-welding works is proposed.

R. V. Zagidulin; V. F. Muzhitskii

2003-07-01T23:59:59.000Z

116

Decades of Discovery  

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

7 6/1/2011 7 6/1/2011 3.2 Discovery of One of the Smallest Particles of Matter Forces of nature are mediated by the interaction or exchange of particles called bosons. In 1989, experiments at Stanford Linear Accelerator Center and the European Laboratory for Particle Physics (also known as CERN) made precise measurements of the lifetime of the Z0 boson, which carries the "weak force" that allows particles to change form. The experiment was significant because it implied that only three families of fundamental particles exist. That's because the Z0 boson is short-lived and decays to certain other particles; the number of these particles influences the decay process. Precise measurement of the Z0 boson lifetime revealed that only three particles called neutrinos are produced. (If

117

Fluid pressure arrival time tomography: Estimation and assessment in the presence of inequality constraints, with an application to a producing gas field at Krechba, Algeria  

SciTech Connect

Deformation in the overburden proves useful in deducing spatial and temporal changes in the volume of a producing reservoir. Based upon these changes we estimate diffusive travel times associated with the transient flow due to production, and then, as the solution of a linear inverse problem, the effective permeability of the reservoir. An advantage an approach based upon travel times, as opposed to one based upon the amplitude of surface deformation, is that it is much less sensitive to the exact geomechanical properties of the reservoir and overburden. Inequalities constrain the inversion, under the assumption that the fluid production only results in pore volume decreases within the reservoir. We apply the formulation to satellite-based estimates of deformation in the material overlying a thin gas production zone at the Krechba field in Algeria. The peak displacement after three years of gas production is approximately 0.5 cm, overlying the eastern margin of the anticlinal structure defining the gas field. Using data from 15 irregularly-spaced images of range change, we calculate the diffusive travel times associated with the startup of a gas production well. The inequality constraints are incorporated into the estimates of model parameter resolution and covariance, improving the resolution by roughly 30 to 40%.

Rucci, A.; Vasco, D.W.; Novali, F.

2010-04-01T23:59:59.000Z

118

Abandoned oil fields in Oklahoma  

SciTech Connect

Data are presented for approximately 165 abandoned oil fields in Oklahoma that have produced 10,000 or more barrels of oil prior to abandonment. The following information is provided for each field: county; DOE field code; field name; AAPG geologic province code; discovery date of field; year of last production, if known; discovery well operator; proven acreage; formation thickness; depth of field; gravity of oil production; calendar year; yearly field oil production; yearly field gas production; cumulative oil production; cumulative gas production; number abandoned fields in county; cumulative production of oil from fields; and cumulative production of gas from fields. (ATT)

Chism, J.

1983-08-01T23:59:59.000Z

119

LBNL-41172 Discovery  

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

1172 1172 Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications S. Perlmutter, G. Aldering, M. Della Valle, S. Deustua, R. S. Ellis, S. Fabbro, A. Fruchter, G. Goldhaber, A. Goobar, D. E. Groom, 1. M. Hook, A. G. Kim, M. Y. Kim, R.A. Knop, C. Lidman, R. G. McMahon, P. Nugent, R. Pain, N. Panagia, C. R. Pennypacker, P. Ruiz-Lapuente, B. Schaefer & N. Walton (The Supernova Cosmology Project) This work was supported in part by the Director, Office of Science, Office of High Energy Physics, of the U.S. Department of Energy under Contract No. DE-AC03-76SF00098. DISCLAIMER This document was prepared as an account of work sponsored by the United States Government. While this document is believed to contain correct information, neither the United States Government nor any agency thereof, nor The Regents of the University of California, nor any of their

120

Discovery & Innovation  

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

The Office of Science The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of national importance. It oversees - and is the principal federal funding agency of - the Nation's research programs in high-energy physics, nuclear physics, and fusion energy sciences. en {8C4B6798-0A4D-4B36-AF69-02F3EFA94CD1}http://science.energy.gov/discovery-and-innovation/stories/2013/127045/ Observing the Sparks of Life EFRC researchers isolate a photosynthetic complex - arguably the most important bit of organic chemistry on the planet - in its complete

Note: This page contains sample records for the topic "field discoveries estimated" 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

One of the remarkable dis-coveries in astrophysics has  

E-Print Network (OSTI)

, the galaxies, and everything we know." With the discovery of dark energy ten years ago, a better understanding as dark energy, a uniform background field that is accelerating the expansion of the universe. The pres- ence of dark energy suggests a fundamental gap in our current understanding of the basic forces

122

Success Stories: Materials Discovery - Symyx  

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

Materials Discovery Materials Discovery Until Lawrence Berkeley National Laboratory scientist Peter Schultz thought of a better way, materials discovery was a costly, slow, and laborious process. In the early 1990s Dr. Schultz and colleagues invented a super efficient materials research process that combined minaturizing with parallel processing. In 1994 the start-up company Symyx Technologies, Inc. licensed the invention and began developing research tools that can create and screen new materials hundreds to thousands of times faster than traditional methods at a fraction of the cost. Combinatorial techniques had been successfully applied in the pharmaceutical industry to discover new drugs when Schultz and co-workers in the Molecular Design Institute of Berkeley Lab proposed that the same

123

Discovery of antivirals against smallpox  

Science Journals Connector (OSTI)

...and biotechnology companies in a poxvirus drug-discovery...require significant changes in the ways that...problems to study. A climate of apprehension...relationships with drug companies (Recommendation...government official and leaders of major pharmaceutical...and biotechnology companies to initiate and...

Stephen C. Harrison; Bruce Alberts; Ellie Ehrenfeld; Lynn Enquist; Harvey Fineberg; Steven L. McKnight; Bernard Moss; Michael O'Donnell; Hidde Ploegh; Sandra L. Schmid; K. Peter Walter; Julie Theriot

2004-01-01T23:59:59.000Z

124

Resource descriptions, ontology, and resource discovery  

Science Journals Connector (OSTI)

Resource discovery systems may assist scientists in the selection of bioinformatics resources suitable to implement scientific workflows. In this paper we address several problems related to resource discovery. They include resource publication formats, resource registration, and syntactic vs. semantic discovery. We analyse the BioMoby registry and present an algorithm that curates the BioMoby hierarchy into an ontology for use in semantic-driven resource discovery.

Zoe Lacroix; Maliha Aziz

2010-01-01T23:59:59.000Z

125

Estimating Methods  

Directives, Delegations, and Requirements

Based on the project's scope, the purpose of the estimate, and the availability of estimating resources, the estimator can choose one or a combination of techniques when estimating an activity or project. Estimating methods, estimating indirect and direct costs, and other estimating considerations are discussed in this chapter.

1997-03-28T23:59:59.000Z

126

Salt dome discoveries mounting in Mississippi  

SciTech Connect

Exploratory drilling around piercement salt domes in Mississippi has met with a string of successes in recent months. Exploration of these salt features is reported to have been initiated through the review of non-proprietary, 2D seismic data and subsurface control. This preliminary data and work were then selectively upgraded by the acquisition of additional, generally higher quality, conventional 2D seismic lines. This current flurry of successful exploration and ensuing development drilling by Amerada Hess Corp. on the flanks of salt domes in Mississippi has resulted in a number of significant Hosston discoveries/producers at: Carson salt dome in Jefferson Davis County; Dry Creek salt dome in Covington County, Midway salt dome in lamar County, Monticello salt dome in Lawrence County, and Prentiss salt dome in Jefferson Davis County. The resulting production from these fields is gas and condensate, with wells being completed on 640 acre production units.

Ericksen, R.L. [Mississippi Office of Geology, Jackson, MS (United States)

1996-06-17T23:59:59.000Z

127

The discovery of the electron, proton, and neutron  

Science Journals Connector (OSTI)

The discovery of the electron, proton, and neutron ... Brief history of the discovery of the electron, proton, and neutron. ...

Barrie M. Peake

1989-01-01T23:59:59.000Z

128

Abandoned oil fields in Kansas and Nebraska  

SciTech Connect

Data on approximately 400 abandoned oil fields in Kansas and 90 abandoned oil fields in Nebraska are presented. The following information is obtained on each field: county; DOE field code; field name; AAPG geologic province code; discovery date; year of last production; discovery well operator; proven acreage; formation thickness; depth of field; API gravity; calendar year; yearly field oil production; yearly field gas production; cumulative oil production; cumulative gas production; number abandoned fields in county; cumulative production of oil from fields; and cumulative production of gas from fields. (DMC)

Not Available

1982-12-01T23:59:59.000Z

129

LWD-0008 Motion for Discovery  

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

Ronald A. Sorri Ronald A. Sorri DECISION AND ORDER OF THE DEPARTMENT OF ENERGY Motions for Discovery Supplemental Order Name of Petitioner: Ronald A. Sorri L&M Technologies, Inc. Ronald A. Sorri Dates of Filing: September 24, 1993 September 27, 1993 October 12, 1993 Case Numbers: LWD-0008 LWD-0009 LWX-0011 This determination will consider two requests for discovery filed with the Office of Hearings and Appeals (OHA) on September 24 and 27, 1993, by Ronald A. Sorri (Sorri) and L&M Technologies, Inc. (L&M), respectively. These motions concern the hearing requested by Sorri under the Department of Energy's Contractor Employee Protection Program, 10 C.F.R. Part 708, on June 9, 1993 (OHA Case No. LWA-0001). The DOE Contractor Employee Protection Program and the Sorri proceeding are described in a

130

Particle Physics at Discovery's Horizon  

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

uslhc.us uslhc.us Particle Physics at Discovery's Horizon September 2012 Discoveries from the Compact Muon Solenoid experiment at the Large Hadron Collider at CERN in Geneva, Switzerland, promise to rev- olutionize our understanding of the universe. With more than 1000 participants from 49 institutions across the country, US CMS is the largest national group in the 3,600-member international CMS collaboration. Supported by the US Department of Energy's Office of Science and the National Science Foundation, the US CMS collaboration consists of more than 430 physicists, nearly 200 graduate students and more than 300 engineers, tech- nicians and computer scientists. The US CMS collaboration plays a vital role in the operation of the CMS detector and analysis of data from LHC collisions. US groups

131

Explanation and discovery in aerodynamics  

E-Print Network (OSTI)

The purpose of this paper is to discuss and clarify the explanations commonly cited for the aerodynamic lift generated by a wing, and to then analyse, as a case study of engineering discovery, the aerodynamic revolutions which have taken place within Formula 1 in the past 40 years. The paper begins with an introduction that provides a succinct summary of the mathematics of fluid mechanics.

Gordon McCabe

2005-12-22T23:59:59.000Z

132

Experimental Discovery of Topological Insulators and Related Superconductors  

SciTech Connect

Most quantum states of condensed matter are categorized by the symmetries they break. The remarkable discovery of charge Quantum Hall effects (1980s) revealed that there exists an organizational principle of matter based only on the topological distinctions, but in the presence of time-reversal symmetry breaking. In the past few years, theoretical developments suggest that new classes of topological states of matter might exist that are purely topological in nature in the sense that they do not break time-reversal symmetry, and hence can be realized without any applied magnetic field: "Quantum Hall-like effects without Magnetic Fields." This talk describes our discovery of new topologically ordered states of matter (topological insulators) and discusses the unusual electro-magnetic, spin, and superconducting properties this novel phase of quantum matter might exhibit and their potential applications.

Hasan, M. Zahid (Princeton) [Princeton

2010-09-15T23:59:59.000Z

133

Frontiers for Discovery in High Energy Density Physics  

SciTech Connect

The report is intended to identify the compelling research opportunities of high intellectual value in high energy density physics. The opportunities for discovery include the broad scope of this highly interdisciplinary field that spans a wide range of physics areas including plasma physics, laser and particle beam physics, nuclear physics, astrophysics, atomic and molecular physics, materials science and condensed matter physics, intense radiation-matter interaction physics, fluid dynamics, and magnetohydrodynamics

Davidson, R. C.; Katsouleas, T.; Arons, J.; Baring, M.; Deeney, C.; Di Mauro, L.; Ditmire, T.; Falcone, R.; Hammer, D.; Hill, W.; Jacak, B.; Joshi, C.; Lamb, F.; Lee, R.; Logan, B. G.; Melissinos, A.; Meyerhofer, D.; Mori, W.; Murnane, M.; Remington, B.; Rosner, R.; Schneider, D.; Silvera, I.; Stone, J.; Wilde, B.; Zajc. W.

2004-07-20T23:59:59.000Z

134

Testicular Cancer Discoveries and Updates  

Science Journals Connector (OSTI)

...-node dissection after chemotherapy can be avoided in approximately 95% of men if patients with a complete response on serologic and radiographic testing are followed with active surveillance. Stage III Testicular Cancer. The discovery of cis-diamminedichloroplatinum (known as cisplatin) in 1965, a landmark... The treatment of testicular cancer is a success story in oncology. With available methods, 95% of men with this condition can be cured. Emphasis is shifting toward maintaining high cure rates and reducing or effectively managing late effects of treatment.

Hanna N.H.; Einhorn L.H.

2014-11-20T23:59:59.000Z

135

Mexico's Luna discoveries are more than moonshine  

SciTech Connect

Just when it seemed that Mexico's petroleum reserves may have been overstated, the state oil company opened a new province. Petroleos Mexicanos (Pemex) geologists think the Luna area of Tabasco State and the Gulf of Mexico could add the condensate and gas equivalent of 20 billion bbl of light oil to Mexico's proven reserves. If true, this would be the largest discovery in Mexico since the Campeche Sound fields in 1976. To date, the new province stretches about 50 miles between the Caribbean coastal towns of Frontera and Puerto Ceiba in Tabasco State, and extends some 31 miles offshore (see map). Since the early 1970s, Pemex geologists have postulated that the entire Yucatan platform will prove productive. Luna finds reduce the distance between Campeche fields and onshore production to 93 miles. The Luna area is ideally suited for rapid development - it is about 40 miles northeast of Villahermosa, Tabasco, and within 60 miles of the export terminal at Dos Bocas near the border between Tabasco and Vera Cruz states. It is also less than 50 miles from the Cactus gas-processing and petrochemical plants in Chiapas State, which means that gas can be put into the country's trunk line that extends to the U.S. grid at Reynosa.

Stewart-Gordon, T.J.; Baker, G.T.

1987-05-01T23:59:59.000Z

136

COLDz: Karl G. Jansky Very Large Array discovery of a gas-rich galaxy in COSMOS  

E-Print Network (OSTI)

The broad spectral bandwidth at mm and cm-wavelengths provided by the recent upgrades to the Karl G. Jansky Very Large Array (VLA) has made it possible to conduct unbiased searches for molecular CO line emission at redshifts, z > 1.31. We present the discovery of a gas-rich, star-forming galaxy at z = 2.48, through the detection of CO(1-0) line emission in the COLDz survey, through a sensitive, Ka-band (31 to 39 GHz) VLA survey of a 6.5 square arcminute region of the COSMOS field. We argue that the broad line (FWHM ~570 +/- 80 km/s) is most likely to be CO(1-0) at z=2.48, as the integrated emission is spatially coincident with an infrared-detected galaxy with a photometric redshift estimate of z = 3.2 +/- 0.4. The CO(1-0) line luminosity is L'_CO = (2.2 +/- 0.3) x 10^{10} K km/s pc^2, suggesting a cold molecular gas mass of M_gas ~ (2 - 8)x10^{10}M_solar depending on the assumed value of the molecular gas mass to CO luminosity ratio alpha_CO. The estimated infrared luminosity from the (rest-frame) far-infrare...

Lentati, L; Carilli, C L; Riechers, D; Capak, P; Walter, F; Aravena, M; da Cunha, E; Hodge, J A; Ivison, R J; Smail, I; Sharon, C; Daddi, E; Decarli, R; Dickinson, M; Sargent, M; Scoville, N; Smolcic, V

2014-01-01T23:59:59.000Z

137

Materials Discovery Design, Synthesis & Processing | The Ames...  

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

Materials Discovery Design, Synthesis & Processing Vision: AMES will be the premier U.S. laboratory lusing an "atoms to applications" approach to discover and design new materials....

138

Accelerator Modeling for Discovery | Argonne Leadership Computing...  

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

three scientific drivers that require accelerator-based experiments (using the Higgs boson as a new tool for discovery, pursuing the physics associated with neutrino mass,...

139

Bioenergy Knowledge Discovery Framework Recognized at National...  

Energy Savers (EERE)

Knowledge Discovery Framework (KDF) is bringing together the bioenergy community through Web-based tools, and was presented by Bioenergy KDF team members from Oak Ridge National...

140

COLLOQUIUM: Laboratory Study of Magnetic Reconnection: Recent Discoveries  

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

March 27, 2013, 4:15pm to 5:30pm March 27, 2013, 4:15pm to 5:30pm Colloquia MBG Auditorium COLLOQUIUM: Laboratory Study of Magnetic Reconnection: Recent Discoveries on MRX Dr. Masaaki Yamada Princeton University Presentation: WC27MAR2013_MYamada.pptx Magnetic reconnection is a phenomenon of nature in which magnetic field lines change their topology in plasma and convert magnetic energy to particles by acceleration and heating. It is one of the most fundamental processes at work in laboratory and astrophysical plasmas. Magnetic reconnection occurs everywhere: in solar flares; coronal mass ejections; the earth's magnetosphere; in the star forming galaxies; and in plasma fusion devices. This talk focuses on recent discoveries in the fundamental research of magnetic reconnection on Magnetic Reconnection Experiment (MRX)

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141

Historical Evidence of the 1936 Mojokerto Skull Discovery, East Java  

Science Journals Connector (OSTI)

To resolve ambiguities in the literature, we detail the discovery history of the Mojokerto child's skull (Perning 1), employing letters, maps, photographs, reports, and newspaper accounts not previously used for this purpose. Andoyo, an experienced vertebrate-fossil collector with the Geological Survey of the Netherlands Indies, found the skull on February 13, 1936, while collecting for Johan Duyfjes, who had mapped the field area geologically. On February 1819 Andoyo sent the fossil and a 1:25,000-topographic map showing the discovery point to Survey headquarters. The locality lies between Perning and Sumbertengu villages, ?10km northeast of Mojokerto city, East Java. G.H. Ralph von Koenigswald, Survey paleontologist, identified the specimen as Pithecanthropus and then named it Homo modjokertensis (it is now accepted as Homo erectus). Unfortunately he confused the discovery record in a March 28 newspaper article by characterizing the skull as a surface find [Dutch: oppervlaktevondst] while also attributing it to ancient beds. von Koenigswald probably had insufficient basis for either assertion, having not yet talked to Andoyo or Duyfjes. Eugene Dubois challenged von Koenigswald on the surface-find issue, Andoyo was consulted, and Duyfjes went to the site. Duyfjes and von Koenigswald then published scientific papers stating that the skull was unearthed 1m deep from a hill-slope outcrop of conglomeratic sandstone in Duyfjes' Pucangan formation. A cross section by Andoyo, which may show the Mojokerto site, also indicates a skull at 1m depth in conglomeratic sandstone. Photographs taken in 19361938 show a shallow pit at a single field location that fits Duyfjes' site description and is identified as the Mojokerto-skull site in 19401943 publications. By WWII the scientific community accepted the skull as an early hominid. Although von Koenigswald's surface-find comment remains a source of doubt in the record, we consider in situ discovery for the Mojokerto skull to be very likely.

O. Frank Huffman; Pat Shipman; Christine Hertler; John de Vos; Fachroel Aziz

2005-01-01T23:59:59.000Z

142

11 - Discovery of Rich Resources  

Science Journals Connector (OSTI)

Abstract In the mid-twentieth century, constant diplomatic pressure during the Cold War by the Soviets against neighboring Afghanistan finally led to governmental acceptance of a major effort by some 250 Russian geologists to map the overall geology of the country, and to find valuable mineral resources that could be exploited, perhaps to the benefit of Afghanistan, but certainly to reward the finder Soviets. The two decades of Soviet mapping and analysis that took place in the 1960s and 1970s led directly to the discovery of resources that were rich by any standard. Valuable deposits of natural gas, oil, coal, cement, copper, and iron ores were all discovered and plans made for their future major exploitation.

John F. Shroder

2014-01-01T23:59:59.000Z

143

July 4, 2012: Discovery of a particle "consistent" with Higgs...  

Energy Savers (EERE)

July 4, 2012: Discovery of a particle "consistent" with Higgs Boson July 4, 2012: Discovery of a particle "consistent" with Higgs Boson July 4, 2012: Discovery of a particle...

144

ALFALFA DISCOVERY OF THE NEARBY GAS-RICH DWARF GALAXY LEO P. I. H I OBSERVATIONS  

SciTech Connect

The discovery of a previously unknown 21 cm H I line source identified as an ultra-compact high velocity cloud in the ALFALFA survey is reported. The H I detection is barely resolved by the Arecibo 305 m telescope {approx}4' beam and has a narrow H I linewidth (half-power full width of 24 km s{sup -1}). Further H I observations at Arecibo and with the Very Large Array corroborate the ALFALFA H I detection, provide an estimate of the H I radius, {approx}1' at the 5 Multiplication-Sign 10{sup 19} cm{sup -2} isophote, and show the cloud to exhibit a velocity field which, if interpreted as disk rotation, has an amplitude of {approx_equal}9.0 {+-} 1.5 km s{sup -1}. In other papers, Rhode et al. show the H I source to have a resolved stellar counterpart and ongoing star forming activity, while Skillman et al. reveal it as having extremely low metallicity: 12 + log (O/H) = 7.16 {+-} 0.04. The H I mass to stellar mass ratio of the object is found to be 2.6. We use the Tully-Fisher template relation in its baryonic form to obtain a distance estimate D{sub Mpc}=1.3{sup +0.9}{sub -0.5}. Additional constraints on the distance are also provided by the optical data of Rhode et al. and McQuinn et al., both indicating a distance in the range of 1.5 to 2.0 Mpc. The three estimates are compatible within their errors. The object appears to be located beyond the dynamical boundaries of, but still in close proximity to the Local Group. Its pristine properties are consistent with the sedate environment of its location. At a nominal distance of 1.75 Mpc, it would have an H I mass of {approx_equal} 1.0 Multiplication-Sign 10{sup 6} M {sub Sun }, a stellar mass of {approx_equal} 3.6 Multiplication-Sign 10{sup 5} M {sub Sun }, and a dynamical mass within the H I radius of {approx_equal} 1.5 Multiplication-Sign 10{sup 7} M {sub Sun }. This discovery supports the idea that optically faint-or altogether dark-low mass halos may be detectable through their non-stellar baryons.

Giovanelli, Riccardo; Haynes, Martha P.; Adams, Elizabeth A. K. [Center for Radiophysics and Space Research, Space Sciences Building, Cornell University, Ithaca, NY 14853 (United States); Cannon, John M.; Bernstein-Cooper, Elijah Z. [Department of Physics and Astronomy, Macalester College, Saint Paul, MN 55105 (United States); Rhode, Katherine L.; Salzer, John J. [Department of Astronomy, Indiana University, Bloomington, IN 47405 (United States); Skillman, Evan D.; McQuinn, Kristen B. W., E-mail: riccardo@astro.cornell.edu, E-mail: haynes@astro.cornell.edu, E-mail: betsey@astro.cornell.edu, E-mail: jcannon@macalester.edu, E-mail: ebernste@macalester.edu, E-mail: rhode@astro.indiana.edu, E-mail: slaz@astro.indiana.edu, E-mail: skillman@astro.umn.edu, E-mail: kmcquinn@astro.umn.edu [Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, MN 55455 (United States)

2013-07-01T23:59:59.000Z

145

Unsupervised Knowledge Discovery in Medical Databases Using Relevance Networks  

E-Print Network (OSTI)

Page 1 Unsupervised Knowledge Discovery in Medical Databases Using Relevance Networks Atul J Butte databases for unsupervised medical knowledge discovery without a prior model or information. Observations

Babu, M. Madan

146

Application of proteomics in the discovery of candidate protein...  

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

in the discovery of candidate protein biomarkers in a Diabetes Autoantibody Standardization Program Application of proteomics in the discovery of candidate protein...

147

Cost Estimator  

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

A successful candidate in this position will serve as a senior cost and schedule estimator who is responsible for preparing life-cycle cost and schedule estimates and analyses associated with the...

148

Methods to estimate on-field nitrogen emissions from crop production as an input to LCA studies in the agricultural sector  

Science Journals Connector (OSTI)

Nitrogen compounds emitted from the field are usually considered in Life Cycle Assessments (LCA) of agricultural products or processes. The environmentally most important of these N emissions are ammonia (NH3), n...

Frank Brentrup; Jrgen Ksters

2000-11-01T23:59:59.000Z

149

Stories of Discovery & Innovation  

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

stories/ The Office of stories/ The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of national importance. It oversees - and is the principal federal funding agency of - the Nation's research programs in high-energy physics, nuclear physics, and fusion energy sciences. en {8C4B6798-0A4D-4B36-AF69-02F3EFA94CD1}http://science.energy.gov/discovery-and-innovation/stories/2013/127045/ Observing the Sparks of Life EFRC researchers isolate a photosynthetic complex - arguably the most important bit of organic chemistry on the planet - in its complete

150

Los Alamos PC estimating system  

SciTech Connect

The Los Alamos Cost Estimating System (QUEST) is being converted to run on IBM personal computers. This very extensive estimating system is capable of supporting cost estimators from many different and varied fields. QUEST does not dictate any fixed method for estimating. QUEST supports many styles and levels of detail estimating. QUEST can be used with or without data bases. This system allows the estimator to provide reports based on levels of detail defined by combining work breakdown structures. QUEST provides a set of tools for doing any type of estimate without forcing the estimator to use any given method. The level of detail in the estimate can be mixed based on the amount of information known about different parts of the project. The system can support many different data bases simultaneously. Estimators can modify any cost in any data base.

Stutz, R.A.; Lemon, G.D.

1987-01-01T23:59:59.000Z

151

New Field Discoveries of Natural Gas, Wet After Lease Separation  

Gasoline and Diesel Fuel Update (EIA)

425 814 1,229 1,423 895 987 1979-2011 425 814 1,229 1,423 895 987 1979-2011 Federal Offshore U.S. 114 618 321 310 71 590 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 85 313 288 50 71 590 1981-2011 Texas 29 305 33 260 0 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 425 814 1,229 1,423 895 987 1979-2011 Alabama 0 0 2 0 3 2 1979-2011 Arkansas 7 0 0 0 0 0 1979-2011 California 0 0 0 1 1 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 0 1 1 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 15 15 18 8 23 19 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 10 0 4 0 1979-2011 Kentucky

152

Nonassociated Natural Gas New Field Discoveries, Wet After Lease Separation  

Gasoline and Diesel Fuel Update (EIA)

385 768 1,122 1,160 793 376 1979-2011 385 768 1,122 1,160 793 376 1979-2011 Federal Offshore U.S. 87 575 228 96 65 66 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 58 309 195 25 65 66 1981-2011 Texas 29 266 33 71 0 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 385 768 1,122 1,160 793 376 1979-2011 Alabama 0 0 2 0 1 0 1979-2011 Arkansas 7 0 0 0 0 0 1979-2011 California 0 0 0 1 1 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 0 1 1 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 15 15 18 8 23 19 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 6 0 3 0 1979-2011 Kentucky 0 0 0 0 0 2 1979-2011

153

Shale Natural Gas New Reservoir Discoveries in Old Fields  

Gasoline and Diesel Fuel Update (EIA)

1,613 1,149 699 2009-2011 1,613 1,149 699 2009-2011 Alaska 0 0 0 2009-2011 Lower 48 States 1,613 1,149 699 2009-2011 Alabama 0 0 2009-2010 Arkansas 0 0 0 2009-2011 California 0 2011-2011 San Joaquin Basin Onshore 0 2011-2011 Colorado 0 0 0 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 1,377 172 140 2009-2011 North 1,377 172 140 2009-2011 Michigan 0 0 0 2009-2011 Montana 0 0 1 2009-2011 New Mexico 0 0 0 2009-2011 East 0 0 0 2009-2011 West 0 0 0 2009-2011 North Dakota 1 1 2 2009-2011 Ohio 0 0 2009-2010 Oklahoma 162 0 0 2009-2011 Pennsylvania 0 871 319 2009-2011 Texas 65 36 93 2009-2011 RRC District 1 0 14 0 2009-2011 RRC District 2 Onshore 2 81 2010-2011 RRC District 3 Onshore 0 0 0 2009-2011 RRC District 4 Onshore 30 0 12 2009-2011 RRC District 5

154

Dry Natural Gas Proved Reserves New Field Discoveries (Summary)  

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

409 796 1,170 1,372 850 947 1977-2011 409 796 1,170 1,372 850 947 1977-2011 Alabama 0 0 2 0 3 2 1977-2011 Alaska 0 0 0 0 0 0 1977-2011 Arkansas 7 0 0 0 0 0 1977-2011 California 0 0 0 1 1 0 1977-2011 Colorado 14 15 17 8 22 18 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 0 0 9 0 4 0 1977-2011 Kentucky 0 0 0 0 0 1 1977-2011 Louisiana 27 0 191 257 48 47 1981-2011 Michigan 1 0 4 19 2 14 1977-2011 Mississippi 0 0 2 2 0 1 1977-2011 Montana 19 0 0 0 0 7 1977-2011 New Mexico 35 20 0 1 0 3 1977-2011 New York 45 7 0 0 56 0 1977-2011 North Dakota 1 0 6 6 25 10 1977-2011 Ohio 0 0 1 0 0 0 1977-2011 Oklahoma 0 6 21 0 51 47 1977-2011 Pennsylvania 13 7 61 128 50 165 1977-2011 Texas 80 78 472 476 519 69 1981-2011 Utah

155

New Field Discoveries of Natural Gas, Wet After Lease Separation  

Gasoline and Diesel Fuel Update (EIA)

425 814 1,229 1,423 895 987 1979-2011 425 814 1,229 1,423 895 987 1979-2011 Federal Offshore U.S. 114 618 321 310 71 590 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 85 313 288 50 71 590 1981-2011 Texas 29 305 33 260 0 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 425 814 1,229 1,423 895 987 1979-2011 Alabama 0 0 2 0 3 2 1979-2011 Arkansas 7 0 0 0 0 0 1979-2011 California 0 0 0 1 1 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 0 1 1 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 15 15 18 8 23 19 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 10 0 4 0 1979-2011 Kentucky

156

Nonassociated Natural Gas New Reservoir Discoveries in Old Fields, Wet  

Gasoline and Diesel Fuel Update (EIA)

1,132 1,171 858 2,487 1,515 1,100 1979-2011 1,132 1,171 858 2,487 1,515 1,100 1979-2011 Federal Offshore U.S. 388 325 248 186 95 38 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 329 294 169 150 83 38 1981-2011 Texas 59 31 79 36 12 0 1981-2011 Alaska 2 0 5 0 0 3 1979-2011 Lower 48 States 1,130 1,171 853 2,487 1,515 1,097 1979-2011 Alabama 7 17 1 0 0 0 1979-2011 Arkansas 33 27 41 36 27 23 1979-2011 California 4 1 7 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 1 1 7 0 0 0 1979-2011 State Offshore 3 0 0 0 0 0 1979-2011 Colorado 27 24 17 0 29 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 3 0 2 0 1 1 1979-2011

157

Dry Natural Gas Proved Reserves New Field Discoveries (Summary)  

Gasoline and Diesel Fuel Update (EIA)

409 796 1,170 1,372 850 947 1977-2011 409 796 1,170 1,372 850 947 1977-2011 Alabama 0 0 2 0 3 2 1977-2011 Alaska 0 0 0 0 0 0 1977-2011 Arkansas 7 0 0 0 0 0 1977-2011 California 0 0 0 1 1 0 1977-2011 Colorado 14 15 17 8 22 18 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 0 0 9 0 4 0 1977-2011 Kentucky 0 0 0 0 0 1 1977-2011 Louisiana 27 0 191 257 48 47 1981-2011 Michigan 1 0 4 19 2 14 1977-2011 Mississippi 0 0 2 2 0 1 1977-2011 Montana 19 0 0 0 0 7 1977-2011 New Mexico 35 20 0 1 0 3 1977-2011 New York 45 7 0 0 56 0 1977-2011 North Dakota 1 0 6 6 25 10 1977-2011 Ohio 0 0 1 0 0 0 1977-2011 Oklahoma 0 6 21 0 51 47 1977-2011 Pennsylvania 13 7 61 128 50 165 1977-2011 Texas 80 78 472 476 519 69 1981-2011 Utah

158

Natural Gas Liquids New Reservoir Discoveries in Old Fields  

Gasoline and Diesel Fuel Update (EIA)

72 54 42 53 58 68 1979-2008 72 54 42 53 58 68 1979-2008 Federal Offshore U.S. 37 32 21 19 16 18 1981-2008 Pacific (California) 0 0 0 0 0 0 1979-2008 Louisiana & Alabama 32 31 19 18 16 17 1981-2008 Texas 5 1 2 1 0 1 1981-2008 Alaska 0 0 0 0 0 0 1979-2008 Lower 48 States 72 54 42 53 58 68 1979-2008 Alabama 0 0 0 0 0 0 1979-2008 Arkansas 0 0 0 0 0 0 1979-2008 California 0 0 0 0 0 1 1979-2008 Coastal Region Onshore 0 0 0 0 0 0 1979-2008 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2008 San Joaquin Basin Onshore 0 0 0 0 0 1 1979-2008 State Offshore 0 0 0 0 0 0 1979-2008 Colorado 0 0 0 1 0 0 1979-2008 Florida 0 0 0 0 0 0 1979-2008 Kansas 0 0 0 0 0 0 1979-2008 Kentucky 0 0 0 0 0 0 1979-2008 Louisiana 16 6 12 14 10 31 1981-2008

159

Natural Gas Liquids New Reservoir Discoveries in Old Fields  

Gasoline and Diesel Fuel Update (EIA)

72 54 42 53 58 68 1979-2008 72 54 42 53 58 68 1979-2008 Federal Offshore U.S. 37 32 21 19 16 18 1981-2008 Pacific (California) 0 0 0 0 0 0 1979-2008 Louisiana & Alabama 32 31 19 18 16 17 1981-2008 Texas 5 1 2 1 0 1 1981-2008 Alaska 0 0 0 0 0 0 1979-2008 Lower 48 States 72 54 42 53 58 68 1979-2008 Alabama 0 0 0 0 0 0 1979-2008 Arkansas 0 0 0 0 0 0 1979-2008 California 0 0 0 0 0 1 1979-2008 Coastal Region Onshore 0 0 0 0 0 0 1979-2008 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2008 San Joaquin Basin Onshore 0 0 0 0 0 1 1979-2008 State Offshore 0 0 0 0 0 0 1979-2008 Colorado 0 0 0 1 0 0 1979-2008 Florida 0 0 0 0 0 0 1979-2008 Kansas 0 0 0 0 0 0 1979-2008 Kentucky 0 0 0 0 0 0 1979-2008 Louisiana 16 6 12 14 10 31 1981-2008

160

Dry Natural Gas New Reservoir Discoveries in Old Fields  

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

1,155 1,188 1,622 2,598 1,668 1,227 1977-2011 1,155 1,188 1,622 2,598 1,668 1,227 1977-2011 Federal Offshore U.S. 410 368 532 300 237 76 1990-2011 Pacific (California) 1 0 0 0 0 0 1977-2011 Louisiana & Alabama 343 330 379 223 213 76 1981-2011 Texas 66 38 153 77 24 0 1981-2011 Alaska 2 0 5 0 0 3 1977-2011 Lower 48 States 1,153 1,188 1,617 2,598 1,668 1,224 1977-2011 Alabama 7 17 1 0 0 0 1977-2011 Arkansas 32 27 41 36 27 23 1977-2011 California 4 1 14 0 0 0 1977-2011 Coastal Region Onshore 0 0 0 0 0 0 1977-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1977-2011 San Joaquin Basin Onshore 1 1 14 0 0 0 1977-2011 State Offshore 3 0 0 0 0 0 1977-2011 Colorado 26 23 17 0 27 0 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 3 0 2 0 1 1 1977-2011

Note: This page contains sample records for the topic "field discoveries estimated" 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

Crude Oil plus Lease Condensate New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

141 124 481 2009-2011 141 124 481 2009-2011 Federal Offshore U.S. 96 10 410 2009-2011 Pacific (California) 0 0 0 2009-2011 Louisiana & Alabama 34 10 410 2009-2011 Texas 62 0 0 2009-2011 Alaska 9 0 0 2009-2011 Lower 48 States 132 124 481 2009-2011 Alabama 0 1 1 2009-2011 Arkansas 0 0 0 2009-2011 California 0 0 0 2009-2011 Coastal Region Onshore 0 0 0 2009-2011 Los Angeles Basin Onshore 0 0 0 2009-2011 San Joaquin Basin Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Colorado 0 0 0 2009-2011 Florida 0 0 0 2009-2011 Illinois 0 0 0 2009-2011 Indiana 0 0 0 2009-2011 Kansas 2 2 2 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 0 0 1 2009-2011 North 0 0 0 2009-2011 South Onshore 0 0 1 2009-2011 State Offshore 0 0 0 2009-2011 Michigan 10 0 8 2009-2011

162

Dry Natural Gas New Reservoir Discoveries in Old Fields (Summary)  

Gasoline and Diesel Fuel Update (EIA)

,155 1,188 1,622 2,598 1,668 1,227 1977-2011 ,155 1,188 1,622 2,598 1,668 1,227 1977-2011 Alabama 7 17 1 0 0 0 1977-2011 Alaska 2 0 5 0 0 3 1977-2011 Arkansas 32 27 41 36 27 23 1977-2011 California 4 1 14 0 0 0 1977-2011 Colorado 26 23 17 0 27 0 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 3 0 2 0 1 1 1977-2011 Kentucky 4 0 0 0 0 0 1977-2011 Louisiana 185 134 650 1,542 279 167 1981-2011 Michigan 5 0 1 9 0 0 1977-2011 Mississippi 6 1 3 0 0 0 1977-2011 Montana 28 1 0 0 1 1 1977-2011 New Mexico 140 10 7 3 3 9 1977-2011 New York 0 0 0 0 0 27 1977-2011 North Dakota 3 3 5 5 2 17 1977-2011 Ohio 0 0 0 0 0 0 1977-2011 Oklahoma 12 56 85 178 1 18 1977-2011 Pennsylvania 0 3 32 0 904 322 1977-2011 Texas 253 535 178 425 122 425 1981-2011

163

Dry Natural Gas New Reservoir Discoveries in Old Fields  

Gasoline and Diesel Fuel Update (EIA)

1,155 1,188 1,622 2,598 1,668 1,227 1977-2011 1,155 1,188 1,622 2,598 1,668 1,227 1977-2011 Federal Offshore U.S. 410 368 532 300 237 76 1990-2011 Pacific (California) 1 0 0 0 0 0 1977-2011 Louisiana & Alabama 343 330 379 223 213 76 1981-2011 Texas 66 38 153 77 24 0 1981-2011 Alaska 2 0 5 0 0 3 1977-2011 Lower 48 States 1,153 1,188 1,617 2,598 1,668 1,224 1977-2011 Alabama 7 17 1 0 0 0 1977-2011 Arkansas 32 27 41 36 27 23 1977-2011 California 4 1 14 0 0 0 1977-2011 Coastal Region Onshore 0 0 0 0 0 0 1977-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1977-2011 San Joaquin Basin Onshore 1 1 14 0 0 0 1977-2011 State Offshore 3 0 0 0 0 0 1977-2011 Colorado 26 23 17 0 27 0 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 3 0 2 0 1 1 1977-2011

164

Crude Oil plus Lease Condensate New Field Discoveries  

Gasoline and Diesel Fuel Update (EIA)

141 124 481 2009-2011 141 124 481 2009-2011 Federal Offshore U.S. 96 10 410 2009-2011 Pacific (California) 0 0 0 2009-2011 Louisiana & Alabama 34 10 410 2009-2011 Texas 62 0 0 2009-2011 Alaska 9 0 0 2009-2011 Lower 48 States 132 124 481 2009-2011 Alabama 0 1 1 2009-2011 Arkansas 0 0 0 2009-2011 California 0 0 0 2009-2011 Coastal Region Onshore 0 0 0 2009-2011 Los Angeles Basin Onshore 0 0 0 2009-2011 San Joaquin Basin Onshore 0 0 0 2009-2011 State Offshore 0 0 0 2009-2011 Colorado 0 0 0 2009-2011 Florida 0 0 0 2009-2011 Illinois 0 0 0 2009-2011 Indiana 0 0 0 2009-2011 Kansas 2 2 2 2009-2011 Kentucky 0 0 0 2009-2011 Louisiana 0 0 1 2009-2011 North 0 0 0 2009-2011 South Onshore 0 0 1 2009-2011 State Offshore 0 0 0 2009-2011 Michigan 10 0 8 2009-2011

165

Nonassociated Natural Gas New Reservoir Discoveries in Old Fields, Wet  

Gasoline and Diesel Fuel Update (EIA)

1,132 1,171 858 2,487 1,515 1,100 1979-2011 1,132 1,171 858 2,487 1,515 1,100 1979-2011 Federal Offshore U.S. 388 325 248 186 95 38 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 329 294 169 150 83 38 1981-2011 Texas 59 31 79 36 12 0 1981-2011 Alaska 2 0 5 0 0 3 1979-2011 Lower 48 States 1,130 1,171 853 2,487 1,515 1,097 1979-2011 Alabama 7 17 1 0 0 0 1979-2011 Arkansas 33 27 41 36 27 23 1979-2011 California 4 1 7 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 1 1 7 0 0 0 1979-2011 State Offshore 3 0 0 0 0 0 1979-2011 Colorado 27 24 17 0 29 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 3 0 2 0 1 1 1979-2011

166

Coalbed Methane New Reservoir Discoveries in Old Fields  

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

91 0 13 0 0 2009-2013 Federal Offshore U.S. 0 0 0 0 0 2009-2013 Pacific (California) 0 0 0 0 0 2009-2013 Gulf of Mexico (Louisiana & Alabama) 0 0 0 0 0 2009-2013 Gulf of Mexico...

167

,"Arkansas Dry Natural Gas New Reservoir Discoveries in Old Fields...  

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

,"Source:","Energy Information Administration" ,"For Help, Contact:","infoctr@eia.doe.gov" ,,"(202) 586-8800",,,"1162014 3:41:34 PM" "Back to Contents","Data 1: Arkansas...

168

New Field Discoveries of Dry Natural Gas Reserves  

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

409 796 1,170 1,372 850 947 1977-2011 409 796 1,170 1,372 850 947 1977-2011 Federal Offshore U.S. 111 608 311 308 68 562 1990-2011 Pacific (California) 0 0 0 0 0 0 1977-2011 Louisiana & Alabama 82 304 279 48 68 562 1981-2011 Texas 29 304 32 260 0 0 1981-2011 Alaska 0 0 0 0 0 0 1977-2011 Lower 48 States 409 796 1,170 1,372 850 947 1977-2011 Alabama 0 0 2 0 3 2 1977-2011 Arkansas 7 0 0 0 0 0 1977-2011 California 0 0 0 1 1 0 1977-2011 Coastal Region Onshore 0 0 0 0 0 0 1977-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1977-2011 San Joaquin Basin Onshore 0 0 0 1 1 0 1977-2011 State Offshore 0 0 0 0 0 0 1977-2011 Colorado 14 15 17 8 22 18 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 0 0 9 0 4 0 1977-2011 Kentucky

169

New Field Discoveries of Dry Natural Gas Reserves  

Gasoline and Diesel Fuel Update (EIA)

409 796 1,170 1,372 850 947 1977-2011 409 796 1,170 1,372 850 947 1977-2011 Federal Offshore U.S. 111 608 311 308 68 562 1990-2011 Pacific (California) 0 0 0 0 0 0 1977-2011 Louisiana & Alabama 82 304 279 48 68 562 1981-2011 Texas 29 304 32 260 0 0 1981-2011 Alaska 0 0 0 0 0 0 1977-2011 Lower 48 States 409 796 1,170 1,372 850 947 1977-2011 Alabama 0 0 2 0 3 2 1977-2011 Arkansas 7 0 0 0 0 0 1977-2011 California 0 0 0 1 1 0 1977-2011 Coastal Region Onshore 0 0 0 0 0 0 1977-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1977-2011 San Joaquin Basin Onshore 0 0 0 1 1 0 1977-2011 State Offshore 0 0 0 0 0 0 1977-2011 Colorado 14 15 17 8 22 18 1977-2011 Florida 0 0 0 0 0 0 1977-2011 Kansas 0 0 9 0 4 0 1977-2011 Kentucky

170

Solar composition from the Genesis Discovery Mission  

Science Journals Connector (OSTI)

Solar composition from the Genesis Discovery Mission...gases differ in the Sun from other inner solar system objects. The N isotopic composition...discrepancies in the noble gas data from solar wind implanted in lunar soils. (ii) The...

D. S. Burnett; Genesis Science Team

2011-01-01T23:59:59.000Z

171

Computational Discovery of Communicable Scientific Knowledge  

Science Journals Connector (OSTI)

In this paper we distinguish between two computational paradigms for knowledge discovery that share the notion of heuristic search, but differ in the importance they place on using scientific formalisms to sta...

Pat Langley; Jeff Shrager; Kazumi Saito

2002-01-01T23:59:59.000Z

172

Applications of motif discovery in biological data  

E-Print Network (OSTI)

Sequential motif discovery, the ability to identify conserved patterns in ordered datasets without a priori knowledge of exactly what those patterns will be, is a frequently encountered and difficult problem in computational ...

Styczynski, Mark Philip-Walter

2007-01-01T23:59:59.000Z

173

Robust Subspace Discovery via Relaxed Rank Minimization  

E-Print Network (OSTI)

This letter examines the problem of robust subspace discovery from input data samples (instances) in the presence of overwhelming outliers and corruptions. A typical example is the case where we are given a set of images; ...

Wang, Xinggang

174

U.S. Natural Gas, Wet After Lease Separation New Reservoir Discoveries in  

Gasoline and Diesel Fuel Update (EIA)

New Reservoir Discoveries in Old Fields (Billion Cubic Feet) New Reservoir Discoveries in Old Fields (Billion Cubic Feet) U.S. Natural Gas, Wet After Lease Separation New Reservoir Discoveries in Old Fields (Billion Cubic Feet) Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 1970's 2,637 1980's 2,648 3,080 3,520 3,071 2,778 3,053 1,855 1,556 1,979 2,313 1990's 2,492 1,655 1,773 1,930 3,606 2,518 3,209 2,455 2,240 2,265 2000's 2,463 2,898 1,752 1,653 1,244 1,243 1,197 1,244 1,678 2,656 2010's 1,701 1,260 - = No Data Reported; -- = Not Applicable; NA = Not Available; W = Withheld to avoid disclosure of individual company data. Release Date: 8/1/2013 Next Release Date: 8/1/2014 Referring Pages: New Reservoir Discoveries in Old Fields of Natural Gas, Wet After

175

Hybrid approach for context-aware service discovery in healthcare domain  

Science Journals Connector (OSTI)

Context-awareness computing is a research field which often refers to healthcare as an interesting and rich area of application. Context aware computing attains environments monitoring by means of sensors to provide relevant information or services according ... Keywords: Clustering, Context-awareness, Fuzzy data analysis, Healthcare, Sensors, Service-discovery

G. Fenza; D. Furno; V. Loia

2012-07-01T23:59:59.000Z

176

VBD-0063- In the Matter of Bruce R. Field  

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

This determination will consider a Motion for Discovery filed with the Office of Hearings and Appeals (OHA) by Bruce R. Field (Field). This Motion, dated August 2, 2001, concerns the hearing...

177

Assessing the discovery potential of directional detection of dark matter  

Science Journals Connector (OSTI)

There is a worldwide effort toward the development of a large time projection chamber devoted to directional dark matter detection. All current projects are being designed to fulfill a unique goal: identifying weakly interacting massive particle (WIMP) as such by taking advantage of the expected direction dependence of WIMP-induced events toward the constellation Cygnus. However, such proof of discovery requires a careful statistical data treatment. In this paper, the discovery potential of forthcoming directional detectors is addressed by using a frequentist approach based on the profile likelihood ratio test statistic. This allows us to estimate the expected significance of a dark matter detection taking into account astrophysical and experimental uncertainties. We show that the energy threshold and the background contamination are key experimental issues for directional detection, while angular resolution and sense recognition efficiency only mildly affect the sensitivity and the energy resolution is unimportant. This way, we found that a 30kg.year CF4 directional experiment could reach a 3? sensitivity at 90%C.L. down to 10-5??pb and 3.10-4??pb for the WIMP-proton axial cross section in the most optimistic and pessimistic detector performance case, respectively.

J. Billard; F. Mayet; D. Santos

2012-02-07T23:59:59.000Z

178

Combinatorial Discovery of Fuel Cell Electrocatalysts  

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

Discovery of Fuel Cell Discovery of Fuel Cell Electrocatalysts Eugene S. Smotkin University of Puerto Rico @ Rio Piedras Non-Platinum Electrocatalysts Workshop March 21, 2003 Marriot courtyard - Convention Center New Orleans, Louisiana Combinatorial Discovery of Fuel Cell Electrocatalysts Eugene S. Smotkin University of Puerto Rico @ Rio Piedras Non-Platinum Electrocatalysts Workshop March 21, 2003 Marriot courtyard - Convention Center New Orleans, Louisiana Overview „ Parallel Screening methods „ Optical Screening method „ Array fuel cell „ Array synthetic methods „ Partial review of non-Pt cathode work Overview „ Parallel Screening methods „ Optical Screening method „ Array fuel cell „ Array synthetic methods „ Partial review of non-Pt cathode work Optical Screening of Electrocatalyst Libraries

179

Research towards a systematic signature discovery process  

SciTech Connect

In its most general form, a signature is a unique or distinguishing measurement, pattern, or collection of data that identifies a phenomenon (object, action, or behavior) of interest. The discovery of signatures is an important aspect of a wide range of disciplines from basic science to national security for the rapid and efficient detection and/or prediction of phenomena. Current practice in signature discovery is typically accomplished by asking domain experts to characterize and/or model individual phenomena to identify what might compose a useful signature. What is lacking is an approach that can be applied across a broad spectrum of domains and information sources to efficiently and robustly construct candidate signatures, validate their reliability, measure their quality, and overcome the challenge of detection -- all in the face of dynamic conditions, measurement obfuscation and noisy data environments. Our research has focused on the identification of common elements of signature discovery across application domains and the synthesis of those elements into a systematic process for more robust and efficient signature development. In this way, a systematic signature discovery process lays the groundwork for leveraging knowledge obtained from signatures to a particular domain or problem area, and, more generally, to problems outside that domain. This paper presents the initial results of this research by discussing a mathematical framework for representing signatures and placing that framework in the context of a systematic signature discovery process. Additionally, the basic steps of this process are described with details about the methods available to support the different stages of signature discovery, development, and deployment.

Baker, Nathan A.; Barr, Jonathan L.; Bonheyo, George T.; Joslyn, Cliff A.; Krishnaswami, Kannan; Oxley, Mark; Quadrel, Richard W.; Sego, Landon H.; Tardiff, Mark F.; Wynne, Adam S.

2013-06-04T23:59:59.000Z

180

The Centenary of the Discovery of Benzene  

Science Journals Connector (OSTI)

... the fame of Faraday rests almost entirely upon his striking contributions to scientific knowledge. His ambit was thus more circumscribed than that of Huxley, but his discoveries were more revolutionary, ... the nature of electricity and magnetism, and on the correlation of the different forms of energy, foreshadowed in a remarkable way the results of later investigations; but, as Helmholtz ...

MICHAEL FARADAY

1925-06-27T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

DIMENSIONS of DISCOVERY Sponsored Program Awards  

E-Print Network (OSTI)

Low-CostTechnologyfortheNextGeneration of High Efficiency Solar Cells; Modification 3 for Grant 105663." (a Discovery Park award -- Energy Center engineering, electrical & computer engineering, from U.S. Department of Energy, $25,999, "Development of-Throughput Pathogen RNA Detection System for Dairy Products." Bhunia,ArunK;foodscience,fromEmbassy oftheArabRepublicofEgypt

Ginzel, Matthew

182

COMBINATORIAL DISCOVERY OF PHOTOCATALYSTS FOR HYDROGEN PRODUCTION  

E-Print Network (OSTI)

the development of economical and environmentally benign hydrogen production methods and reliable storage systemsCOMBINATORIAL DISCOVERY OF PHOTOCATALYSTS FOR HYDROGEN PRODUCTION Theodore Mill, Albert Hirschon materials rapidly with appropriate band- gaps and screen them for efficient hydrogen production. The goal

183

Solar composition from the Genesis Discovery Mission  

E-Print Network (OSTI)

Solar composition from the Genesis Discovery Mission D. S. Burnett1 and Genesis Science Team2: the isoto- pic compositions of O, N, and noble gases differ in the Sun from other inner solar system objects in the noble gas data from solar wind implanted in lunar soils. (ii) The most advanced analytical instruments

184

Innovation. Discovery. Community. Excellence. Committed to  

E-Print Network (OSTI)

Innovation. Discovery. Community. Excellence. 2014 2015 Committed to Achievement #12;McGill has and around the world. McGill is committed to nurturing this innovation and entrepre- neurship businesses, social enterprises or novel collaborations. A McGill education isn't limited to the classroom. Mc

Kambhampati, Patanjali

185

False Discovery Rates John D. Storey  

E-Print Network (OSTI)

positives. The false discovery rate is designed to quantify this type of trade-off, making it particularly Hypothesis Testing In hypothesis testing, statistical significance is typically based on calculations involving p-values and Type I error rates. A p-value calculated from a single statistical hypothesis test

Storey, John D.

186

SRI International Discovery of Photocatalysts for  

E-Print Network (OSTI)

SRI International Discovery of Photocatalysts for Hydrogen Production 2003 DOE Hydrogen Review May for 2005 and 2010 involve sequential order of magnitude improvements in durability and modest improvements screening tools being developed in this project. Furthermore, the inclusion of a partner with the means

187

Exploratory Search Interfaces to Support Image Discovery  

E-Print Network (OSTI)

Director (1983-2000), Human-Computer Interaction Lab Professor, Department of Computer Science MemberExploratory Search Interfaces to Support Image Discovery Ben Shneiderman ben@cs.umd.edu Founding;Interdisciplinary research community - Computer Science & Psychology - Information Studies & Education (www

Shneiderman, Ben

188

Trawler: de novo regulatory motif discovery pipeline  

E-Print Network (OSTI)

Trawler: de novo regulatory motif discovery pipeline for chromatin immunoprecipitation Laurence, the fastest computational pipeline to date, to efficiently discover over-represented motifs in chromatin present the Trawler pipeline (Fig. 1a) that attempts the de novo identification of all over

Cai, Long

189

Unraveling the Higgs Boson Discovery - Rik Yoshida  

ScienceCinema (OSTI)

Argonne physicist Rik Yoshida explains what the Higgs boson is and what its discovery means for physics, the universe, and life. The third of Argonne's "OutLoud" public lecture series, held at the lab on September 27, 2012. Find out when the next one is at http://www.anl.gov/community/outloud

Rik Yoshida

2013-06-06T23:59:59.000Z

190

Targets for early discoveries at the LHC  

E-Print Network (OSTI)

Targets for early discoveries at the LHC Lian-Tao Wang University of Chicago 04/11/2011 Monday to emphasize less "well-known" or less "well-mentioned" but not "strange" channels. In the next year or so, LHC

191

Genomics-based drug discovery venture  

Science Journals Connector (OSTI)

Genomics-based drug discovery venture ... The Cambridge, Mass.-based company calls its DiscoverEase program "functional genomics"designed to isolate and rapidly determine not only genes but also the related functions of critical proteins. ... Other genomics programs sequence vast amounts of human genetic information. ...

ANN THAYER

1996-10-07T23:59:59.000Z

192

Genomics Rises To Drug Discovery Challenge  

Science Journals Connector (OSTI)

Genomics Rises To Drug Discovery Challenge ... Functional genomics and functional proteomics provide a set of powerful tools to help identify novel cellular targets ... With pharmaceutical companies and biotechnology firms always looking for ways to discover new medicines more quickly and more efficiently, they are increasingly turning to new genomics and proteomics technologies to speed things along. ...

STU BORMAN

1999-04-19T23:59:59.000Z

193

Lab Discovery: Water Leads to Chemical that "Gunks Up" Biofuels...  

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

Lab Discovery: Water Leads to Chemical that "Gunks Up" Biofuels Production Lab Discovery: Water Leads to Chemical that "Gunks Up" Biofuels Production November 20, 2014 - 12:16pm...

194

Causal Discovery for Climate Research Using Graphical Models  

Science Journals Connector (OSTI)

Causal discovery seeks to recover causeeffect relationships from statistical data using graphical models. One goal of this paper is to provide an accessible introduction to causal discovery methods for climate scientists, with a focus on ...

Imme Ebert-Uphoff; Yi Deng

2012-09-01T23:59:59.000Z

195

Single nucleotide polymorphism discovery in elite north american potato germplasm  

E-Print Network (OSTI)

Single nucleotide polymorphism discovery in elite north american potato germplasm Hamilton et al;RESEARCH ARTICLE Open Access Single nucleotide polymorphism discovery in elite north american potato breeding approaches in potato rely almost entirely on phenotypic evaluations; molecular markers

Douches, David S.

196

Microbial Impacts to the Near-Field Environment Geochemistry (MING): A Model for Estimating Microbial Communities in Repository Drifts at Yucca Mountain  

SciTech Connect

Geochemical and microbiological modeling was performed to evaluate the potential quantities and impact of microorganisms on the geochemistry of the area adjacent to and within nuclear waste packages in the proposed repository drifts at Yucca Mountain, Nevada. The microbial growth results from the introduction of water, ground support, and waste package materials into the deep unsaturated rock. The simulations, which spanned one million years, were accomplished using a newly developed computer code, Microbial Impacts to the Near-Field Environment Geochemistry (MING). MING uses environmental thresholds for limiting microbial growth to temperatures below 120 C and above relative humidities of 90 percent in repository drifts. Once these thresholds are met, MING expands upon a mass balance and thermodynamic approach proposed by McKinley and others (1997), by using kinetic rates to supply constituents from design materials and constituent fluxes including solubilized rock components into the drift, to perform two separate mass-balance calculations as a function of time. The first (nutrient limit) assesses the available nutrients (C, N, P and S) and calculates how many microorganisms can be produced based on a microorganism stoichiometry of C{sub 160}(H{sub 280}O{sub 80})N{sub 30}P{sub 2}S. The second (energy limit) calculates the energy available from optimally combined redox couples for the temperature, and pH at that time. This optimization maximizes those reactions that produce > 15kJ/mol (limit on useable energy) using an iterative linear optimization technique. The final available energy value is converted to microbial mass at a rate of 1 kg of biomass (dry weight) for every 64 MJ of energy. These two values (nutrient limit and energy limit) are then compared and the smaller value represents the number of microorganisms that can be produced over a specified time. MING can also be adapted to investigate other problems of interest as the model can be used in saturated and unsaturated environments and in laboratory situations to establish microbial growth limitations. Other projected uses include investigations of contaminated locations where monitored natural attenuation or engineered bioremediation could be employed.

D.M. Jolley; T.F. Ehrhorn; J. Horn

2002-03-19T23:59:59.000Z

197

Before, behind and beyond the discovery of the Higgs boson  

Science Journals Connector (OSTI)

...contributed to this discovery. Their paper also describes...its nature. The Higgs discovery is not only the culmination...may also provide the dark matter postulated by...perhaps driven by energy in space related to...issues posed by the discovery of the Higgs boson will...

2015-01-01T23:59:59.000Z

198

The discovery and measurements of a Higgs boson  

Science Journals Connector (OSTI)

...and beyond the discovery of the Higgs boson. organised and edited by John...discovery and measurements of a Higgs boson F. Gianotti 1 T. S. Virdee 2...and beyond the discovery of the Higgs boson . In July 2012, the ATLAS and...

2015-01-01T23:59:59.000Z

199

Before, behind and beyond the discovery of the Higgs boson  

Science Journals Connector (OSTI)

...and beyond the discovery of the Higgs boson. organised and edited by John...and beyond the discovery of the Higgs boson John Ellis e-mail: john.ellis...and beyond the discovery of the Higgs boson . The announcement on 4 July 2012...

2015-01-01T23:59:59.000Z

200

First Elements on Knowledge Discovery Guided by Domain Knowledge (KDDK)  

E-Print Network (OSTI)

First Elements on Knowledge Discovery Guided by Domain Knowledge (KDDK) Jean Lieber, Amedeo Napoli how knowledge discovery and knowl- edge processing may be combined. The knowledge discovery knowledge units. From a knowledge representa- tion perspective, the kdd process may take advantage of domain

Boyer, Edmond

Note: This page contains sample records for the topic "field discoveries estimated" 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

September 2009 Spotlight on Energy & the Environment Discovery Tour  

E-Print Network (OSTI)

of the farm's energy use is provided by more than 400 solar panels on the southern roof of his turkey barnSeptember 2009 Spotlight on Energy & the Environment Discovery Tour On September 21, dozens Discovery Tour: Energy and the Environment. Part of the Discovery Initiative launched earlier this year

Goodman, Robert M.

202

U.S. scientists celebrate Nobel Prize for Higgs discovery  

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

00813_higgs 00813_higgs 10/08/2013 High Resolution Image Lowering of the final element (YE-1) of the Compact Muon Solenoid (CMS) detector into its underground experimental cavern. U.S. scientists celebrate Nobel Prize for Higgs discovery Donald B Johnston, LLNL, (925) 423-4902, johnston19@llnl.gov Large Ion Collider Experiment, also known as ALICE, is a dedicated heavy-ion detector used to exploit the unique physics potential of nucleus-nucleus interactions at Large Hadron Collider energies. The Royal Swedish Academy of Sciences awarded the Nobel Prize in physics today to theorists Peter Higgs and Francois Englert to recognize their work developing the theory of what is now known as the Higgs field, which gives elementary particles mass. U.S. scientists, including researchers at Lawrence Livermore National

203

Abandoned oil fields in Alaska, California, Colorado, Montana, North Dakota, Utah and Wyoming  

SciTech Connect

This publication lists approximately 250 abandoned oil fields in Alaska, California, Colorado, Montana, North Dakota, Utah and Wyoming that have produced 10,000 or more barrels of oil before abandonment. The following information is provided for each field: county; DOE field code; field name; AAPG geologic province code; discovery data of field; year of last production; discovery well operator; proven acreage; formation thickness; depth of field; gravity of oil production; calendar year; yearly field oil production; yearly field gas production; cumulative oil production; cumulative gas production; number abandoned fields in county; cumulative production of oil from fields; cumulative production of gas from fields. (ATT)

Not Available

1983-04-01T23:59:59.000Z

204

DISCOVERY AND CHARACTERIZATION OF A FAINT STELLAR COMPANION TO THE A3V STAR zeta VIRGINIS  

SciTech Connect

Through the combination of high-order adaptive optics and coronagraphy, we report the discovery of a faint stellar companion to the A3V star zeta Virginis. This companion is {approx}7 mag fainter than its host star in the H band, and infrared imaging spanning 4.75 years over five epochs indicates this companion has common proper motion with its host star. Using evolutionary models, we estimate its mass to be 0.168{sup +0.012}{sub -0.016} M{sub sun}, giving a mass ratio for this system q = 0.082{sup +0.007}{sub -0.008}. Assuming the two objects are coeval, this mass suggests an M4V-M7V spectral type for the companion, which is confirmed through {integral} field spectroscopic measurements. We see clear evidence for orbital motion from this companion and are able to constrain the semimajor axis to be {approx}>24.9 AU, the period {approx}>124 yr, and eccentricity {approx}>0.16. Multiplicity studies of higher mass stars are relatively rare, and binary companions such as this one at the extreme low end of the mass ratio distribution are useful additions to surveys incomplete at such a low mass ratio. Moreover, the frequency of binary companions can help to discriminate between binary formation scenarios that predict an abundance of low-mass companions forming from the early fragmentation of a massive circumstellar disk. A system such as this may provide insight into the anomalous X-ray emission from A stars, hypothesized to be from unseen late-type stellar companions. Indeed, we calculate that the presence of this M-dwarf companion easily accounts for the X-ray emission from this star detected by ROSAT.

Hinkley, Sasha; Hillenbrand, Lynne [Department of Astronomy, California Institute of Technology, 1200 East California Boulevard, MC 249-17, Pasadena, CA 91125 (United States); Oppenheimer, Ben R.; Brenner, Douglas; Zimmerman, Neil; Sivaramakrishnan, Anand [Astrophysics Department, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); Roberts, Lewis C.; Roberts, Jennifer E.; Burruss, Rick; Shao, Michael; Vasisht, Gautam [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109 (United States); Parry, Ian R.; King, David L. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Soummer, Remi [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Simon, Michal [Stony Brook University, NY (United States); Perrin, Marshall D. [UCLA Department of Astronomy, CA (United States); Lloyd, James P. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Bouchez, Antonin; Dekany, Richard [Caltech Optical Observatories, California Institute of Technology, Pasadena, CA 91125 (United States); Beichman, Charles [NASA Exoplanet Science Institute, California Institute of Technology, Pasadena, CA 91125 (United States)

2010-03-20T23:59:59.000Z

205

Prediction and Estimation of Random Fields  

E-Print Network (OSTI)

"(t)g as: X(t) = 1X k=0 bk"(t k) + V (t); where fbkg are the MA parameters with b0 = 1, P1 k=1 jbkj 2 <1, bk = 0; k < 0 and f"(t)g is a white noise process with mean zero and variance 2 called the innovation process of fX(t)g. Here fV (t)g is a... deterministic process orthogonal to f"(t)g. For purely nonde- terministic (PND) process the Wold decomposition has no deterministic component such that X(t) = 1X k=0 bk"(t k): (2.1) It is well known that a necessary and sufficient condition for a process...

Kohli, Priya

2012-10-19T23:59:59.000Z

206

Challenges in Biomarker Discovery: Combining Expert Insights with Statistical Analysis of Complex Omics Data  

SciTech Connect

The advent of high throughput technologies capable of comprehensive analysis of genes, transcripts, proteins and other significant biological molecules has provided an unprecedented opportunity for the identification of molecular markers of disease processes. However, it has simultaneously complicated the problem of extracting meaningful signatures of biological processes from these complex datasets. The process of biomarker discovery and characterization provides opportunities both for purely statistical and expert knowledge-based approaches and would benefit from improved integration of the two. Areas covered In this review we will present examples of current practices for biomarker discovery from complex omic datasets and the challenges that have been encountered. We will then present a high-level review of data-driven (statistical) and knowledge-based methods applied to biomarker discovery, highlighting some current efforts to combine the two distinct approaches. Expert opinion Effective, reproducible and objective tools for combining data-driven and knowledge-based approaches to biomarker discovery and characterization are key to future success in the biomarker field. We will describe our recommendations of possible approaches to this problem including metrics for the evaluation of biomarkers.

McDermott, Jason E.; Wang, Jing; Mitchell, Hugh D.; Webb-Robertson, Bobbie-Jo M.; Hafen, Ryan P.; Ramey, John A.; Rodland, Karin D.

2013-01-01T23:59:59.000Z

207

Manhattan Project: Atomic Discoveries, 1890s-1939  

Office of Scientific and Technical Information (OSTI)

Excerpt from the comic book "Adventures Inside the Atom." Click on this image or visit the "Library" to view the whole comic book. ATOMIC DISCOVERIES Excerpt from the comic book "Adventures Inside the Atom." Click on this image or visit the "Library" to view the whole comic book. ATOMIC DISCOVERIES (1890s-1939) Events A Miniature Solar System, 1890s-1919 Exploring the Atom, 1919-1932 Atomic Bombardment, 1932-1938 The Discovery of Fission, 1938-1939 Fission Comes to America, 1939 Philosophers of Ancient Greece reasoned that all matter in the universe must be composed of fundamental, unchangeable, and indivisible objects, which they called "atoma" ("ατoµα"). The exact nature of these atoms remained elusive, however, despite centuries of attempts by alchemists to create a "philosopher's stone" that could transmute atoms of lead to gold, prove the Greeks wrong, and make its inventors Modern model of an atom very rich. It was only in the late 1890s and the early twentieth-century that this view of a solid atom, bouncing around the universe like a billiard ball, was replaced by an atom that resembled more a miniature solar system, its electrons orbiting around a small nucleus. Explorations into the nature of the atom from 1919 to 1932 confirmed this new model, especially with Ernest Rutherford's 1919 success in finally transmuting an atom of one substance into another and with James Chadwick's 1932 discovery of the elusive final basic particle of the atom, the neutron. From 1932 to 1938, scientists around the world learned a great deal more about atoms, primarily by bombarding the nuclei of atoms and using a variety of particle accelerators. In 1938, word came from Berlin of the most startling result of them all: the nucleus of an atom could actually be split in two, or "fissioned." This breakthrough was quickly confirmed in the United States and elsewhere. According to the theories of Albert Einstein, the fission of an atom should result in a release of energy. An "atomic bomb" was now no longer just science fiction -- it was a distinct possibility.

208

Single, Key Gene Discovery Could Streamline Production of Biofuels |  

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

Single, Key Gene Discovery Could Streamline Production of Biofuels Single, Key Gene Discovery Could Streamline Production of Biofuels Single, Key Gene Discovery Could Streamline Production of Biofuels August 11, 2011 - 3:51pm Addthis WASHINGTON, DC -- A team of researchers at the Department of Energy's BioEnergy Science Center (BESC) have pinpointed the exact, single gene that controls ethanol production capacity in a microorganism. This discovery could be the missing link in developing biomass crops that produce higher concentrations of ethanol at lower costs. "The Department of Energy relies on the scientific discoveries of its labs and research centers to improve the production of clean energy sources," said Energy Secretary Steven Chu. "This discovery is an important step in developing biomass crops that could increase yield of

209

NPP Estimation for Grasslands  

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

NPP for Grasslands NPP for Grasslands Introduction The Oak Ridge DAAC Net Primary Production (NPP) Database includes field measurements from grassland study sites worldwide. The following brief review and discussion is intended to explain the complexity of NPP estimates derived from grassland measurements. There is no single answer to the question, "What is the productivity of the ecosystem at study site A?"; rather there may be range of estimates of NPP, depending upon what data were actually collected and how these data are processed. Although some of these methods for determining NPP for grasslands may be applicable to other vegetation types (e.g., semi-deserts, tundra, or some crops), methods for forests, in particular, are significantly different. Nevertheless, it should be possible to answer the question, "Is this modelled value of NPP reasonable for this ecosystem type at this location?"

210

The Evolution of Giant Oil Field Production Behavior  

Science Journals Connector (OSTI)

The data for this study have been taken from the giant oil field database compiled by Robelius (2007...). AAPG was the main source for information about discovery year, year of first oil production, URR and cumulative

Mikael Hk; Bengt Sderbergh; Kristofer Jakobsson

2009-03-01T23:59:59.000Z

211

Stories of Discovery & Innovation: From Human Genome to Materials...  

Office of Science (SC) Website

of Science's Stories of Discovery & Innovation, was supported in part by the Center for Electrical Energy Storage, an EFRC led by Michael Thackeray at Argonne National Laboratory...

212

Supercomputers Drive Discovery of Materials for More Efficient...  

Office of Science (SC) Website

Supercomputers Drive Discovery of Materials for More Efficient Carbon Capture Advanced Scientific Computing Research (ASCR) ASCR Home About Research Facilities Science Highlights...

213

Cobalt discovery replaces precious metals as industrial catalyst  

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

replaces precious metals Cobalt discovery replaces precious metals as industrial catalyst Cobalt holds promise as an industrial catalyst with potential applications in such...

214

Cobalt discovery replaces precious metals as industrial catalyst  

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

Replaces Precious Metals Cobalt discovery replaces precious metals as industrial catalyst Cobalt holds promise as an industrial catalyst with potential applications in such...

215

Discovery of novel hydrogen storage materials: an atomic scale...  

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

Discovery of novel hydrogen storage materials: an atomic scale computational approach Home Author: C. Wolverton, D. J. Siegel, A. R. Akbarzadeh, V. Ozolins Year: 2008 Abstract:...

216

V-122: IBM Tivoli Application Dependency Discovery Manager Java...  

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

Tivoli Application Dependency Discovery Manager Java Multiple Vulnerabilities March 29, 2013 - 6:00am Addthis PROBLEM: IBM has acknowledged multiple vulnerabilities in IBM Tivoli...

217

Discovery of the Transuranium Elements (LBNL Summer Lecture Series)  

ScienceCinema (OSTI)

Summer Lecture Series 2006: Darleane Hoffman, a Berkeley Lab nuclear chemist, chronicles the discovery of the heaviest elements ? those much heavier than uranium and plutonium.

Hoffman, Darleane

2011-04-28T23:59:59.000Z

218

Slepton Discovery in Electroweak Cascade Decay  

E-Print Network (OSTI)

The LHC studies on the MSSM slepton sector have mostly been focused on direct slepton Drell-Yan pair production. In this paper, we analyze the case when the sleptons are lighter than heavy neutralinos and can appear in the on-shell decay of neutralino states. In particular, we have studied the \\chi_1^\\pm \\chi_2^0 associated production, with the consequent decays of \\chi_1^\\pm and \\chi_2^0 via on-shell sleptons. The invariant mass of the lepton pairs, m_{\\ell\\ell}, from the neutralino decay has a distinctive triangle shape with a sharp kinematic cutoff. We discuss the utilization of this triangle shape in m_{\\ell\\ell} distribution to identify the slepton signal. We studied the trilepton plus missing E_T signal and obtained the effective cross section, \\sigma \\times BR \\times acceptance, that is needed for a 5\\sigma discovery as a function of the cutoff mass for the LHC with center of mass energy 14 TeV and 100 fb^{-1} integrated luminosity. Our results are model independent such that they could be applied to other models with similar decay topology. When applied to the MSSM under simple assumptions, it is found that with 100 fb^{-1} integrated luminosity, a discovery reach in the left-handed slepton mass of about 600 GeV could be reached, which extends far beyond the slepton mass reach in the usual Drell-Yan studies.

Jonathan Eckel; William Shepherd; Shufang Su

2011-11-10T23:59:59.000Z

219

Discovery Mass Reach for Excited Quarks at Hadron Colliders  

E-Print Network (OSTI)

If quarks are composite particles then excited states are expected. We estimate the discovery mass reach as a function of integrated luminosity for excited quarks decaying to dijets at the Tevatron, LHC, and a Very Large Hadron Collider (VLHC). At the Tevatron the mass reach is 0.94 TeV for Run II (2 fb^-1) and 1.1 TeV for TeV33 (30 fb^-1). At the LHC the mass reach is 6.3 TeV for 100 fb^-1. At a VLHC with a center of mass energy, sqrt(s), of 50 TeV (200 TeV) the mass reach is 25 TeV (78 TeV) for an integrated luminosity of 10^4 fb^-1. However, an excited quark with a mass of 25 TeV would be discovered at a hadron collider with sqrt(s)=100 TeV and an integrated luminosity of 13 fb^-1, illustrating a physics example where a factor of 2 in machine energy is worth a factor of 1000 in luminosity.

Robert M. Harris

1996-09-11T23:59:59.000Z

220

General Critical Properties of the Dynamics of Scientific Discovery  

SciTech Connect

Scientific fields are difficult to define and compare, yet there is a general sense that they undergo similar stages of development. From this point of view it becomes important to determine if these superficial similarities can be translated into a general framework that would quantify the general advent and subsequent dynamics of scientific ideas. Such a framework would have important practical applications of allowing us to compare fields that superficially may appear different, in terms of their subject matter, research techniques, typical collaboration size, etc. Particularh' important in a field's history is the moment at which conceptual and technical unification allows widespread exchange of ideas and collaboration, at which point networks of collaboration show the analog of a percolation phenomenon, developing a giant connected component containing most authors. Here we investigate the generality of this topological transition in the collaboration structure of scientific fields as they grow and become denser. We develop a general theoretical framework in which each scientific field is an instantiation of the same large-scale topological critical phenomenon. We consider whether the evidence from a variety of specific fields is consistent with this picture, and estimate critical exponents associated with the transition. We then discuss the generality of the phenomenon and to what extent we may expect other scientific fields including very large ones to follow the same dynamics.

Bettencourt, L. M. A. (LANL); Kaiser, D. I. (MIT)

2011-05-31T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Conceptual Design For Interplanetary Spaceship Discovery  

Science Journals Connector (OSTI)

With the recently revived national interest in Lunar and Mars missions this design study was undertaken by the author in an attempt to satisfy the long?term space exploration vision of human travel to the Moon Mars and beyond with a single design or family of vehicles. This paper describes a conceptual design for an interplanetary spaceship of the not?to?distant future. It is a design that is outwardly similar to the spaceship Discovery depicted in the novel 2001 A Space Odyssey and film of the same name. Like its namesake this spaceship could one day transport a human expedition to explore the moons of Jupiter. This spaceship Discovery is a real engineering design that is capable of being implemented using technologies that are currently at or near the state?of?the?art. The ships main propulsion and electrical power are provided by bi?modal nuclear thermal rocket engines. Configurations are presented to satisfy four basic Design Reference Missions: (1) a high?energy mission to Jupiters moon Callisto (2) a high?energy mission to Mars (3) a low?energy mission to Mars and (4) a high?energy mission to the Moon. The spaceship design includes dual strap?on boosters to enable the high?energy Mars and Jupiter missions. Three conceptual lander designs are presented: (1) Two types of Mars landers that utilize atmospheric and propulsive braking and (2) a lander for Callisto or Earths Moon that utilizes only propulsive braking. Spaceship Discovery offers many advantages for human exploration of the Solar System: (1) Nuclear propulsion enables propulsive capture and escape maneuvers at Earth and target planets eliminating risky aero?capture maneuvers. (2) Strap?on boosters provide robust propulsive energy enabling flexibility in mission planning shorter transit times expanded launch windows and free?return abort trajectories from Mars. (3) A backup abort propulsion system enables crew aborts at multiple points in the mission. (4) Clustered NTR engines provide engine out redundancy. (5) The design efficiently implements galactic cosmic ray shielding using main propellant liquid hydrogen. (6) The design provides artificial gravity to mitigate crew physiological problems on long?duration missions. (7) The design is modular and can be launched using the proposed upgrades to the Evolved Expendable Launch Vehicles or Shuttle?derived heavy lift launch vehicles. (8) High value modules are reusable for Mars and Lunar missions. (9) The design has inherent growth capability and can be tailored to satisfy expanding mission requirements to enable an in?family progression to the Moon Mars and beyond.

Mark G. Benton Sr.

2006-01-01T23:59:59.000Z

222

The discovery and measurements of a Higgs boson  

Science Journals Connector (OSTI)

...candidate for dark matter in the...physics at the TeV energy scale as the SM...would also allow discovery of whatever else...diverges with energy, becoming unphysical...Summary The discovery of a Higgs boson...of the high-energy physics community...the identity of dark matter, the source...

2015-01-01T23:59:59.000Z

223

ORIGINAL PAPER Creativity and scientific discovery with infused design  

E-Print Network (OSTI)

ORIGINAL PAPER Creativity and scientific discovery with infused design and its analysis with C of a theory. As a first step, we use infused design (ID) method to generate new concepts and methods. Keywords Design theory Á Creativity Á Infused design Á C­K theory Á Scientific discovery 1 Introduction

Shai, Offer

224

Intelligent Mobile Agents for Information Retrieval and Knowledge Discovery from  

E-Print Network (OSTI)

or software agents for intelligent, selective, and context­sensitive data gathering and data assimilation assimilation, and knowl­ edge discovery using heterogeneous, distributed data and knowledge sources. (See [1Intelligent Mobile Agents for Information Retrieval and Knowledge Discovery from Distributed Data

Honavar, Vasant

225

Discovery and Early Development of Non-Suppressed Ion Chromatography  

Science Journals Connector (OSTI)

......ion pairing is a replacement process so that detection pre- diction...Comments on the Discovery Process We all derive considerable...contribute to the discovery process. The freedom to experiment...development and can help eventual commercialization of the technology. Summary......

James S. Fritz; Douglas T. Gjerde

2010-08-01T23:59:59.000Z

226

Secure neighbor discovery in wireless networks: formal investigation of possibility  

Science Journals Connector (OSTI)

Wireless communication enables a broad spectrum of applications, ranging from commodity to tactical systems. Neighbor discovery (ND), that is, determining which devices are within direct radio communication, is a building block of network protocols ... Keywords: relay attack, secure neighbor discovery, wireless networks security

Marcin Poturalski; Panos Papadimitratos; Jean-Pierre Hubaux

2008-03-01T23:59:59.000Z

227

Announcement Discoveries in Photosynthesis, Volume 20, Advances in Photosynthesis  

E-Print Network (OSTI)

Announcement Discoveries in Photosynthesis, Volume 20, Advances in Photosynthesis and Respiration I am delighted to announce the publication, in the Advances in Photosynthesis and Respiration (AIPH) series, of the first book that focuses on the historical aspects of photosynthesis research `Discoveries

Govindjee "Gov"

228

Brookhaven National Laboratory - a passion for discovery  

NLE Websites -- All DOE Office Websites

BNL People BNL People a passion for discovery 2013 Young Researcher Symposium Celebrating Brookhaven Lab's Up-and-Coming Scientists at 2013 Young Researcher Symposium Approximately 300 up-and-coming young researchers collaborating on groundbreaking research at Brookhaven Lab gathered in Berkner last month for the second-annual Young Researcher Symposium. More... Newsroom Video & Live Streaming Receive our weekly newsletter See all Latest News Adopt A Family BNLers Help Brighten Holidays for Local Families atomic-scale microscopy Opposing Phenomena Possible Key to High-Efficiency Electricity Delivery Steven Ritz Physicists Look Toward the High-Energy Horizon Our Mission We advance fundamental research in nuclear and particle physics to gain a deeper understanding of matter, energy, space, and time; apply photon

229

Discovery Potential of the Standard Model Higgs Boson Through H -> WW Decay Mode with the ATLAS Detector at LHC  

E-Print Network (OSTI)

We report results of a study of the Standard Model Higgs boson discovery potential through the W-pair leptonic decay modes with the ATLAS detector at LHC at 14 TeV center-of-mass energy. We used MC samples with full detector simulation and reconstruction of the ATLAS experiment to estimate the ATLAS detection sensitivity for the reaction of pp -> H -> WW -> e\

Hai-Jun Yang; for the ATLAS Collaboration

2009-10-01T23:59:59.000Z

230

Chapter 6 - Subsea Cost Estimation  

Science Journals Connector (OSTI)

Publisher Summary This chapter provides guidelines for cost estimation during a project feasibility study, where the accuracy range is between 30% for subsea field development projects. Subsea cost refers to the cost of the whole project, which generally includes the capital expenditures (CAPEX) and operation expenditures (OPEX) of the subsea field development. The feasibility studies are performed before execution of the project, which may include three phases as shown in the figure: prefield development; conceptual/feasibility study; and front-end engineering design (FEED). Cost estimations are made for several purposes, and the methods used for the estimations as well as the desired amount of accuracy will be different. The cost estimation classifications according to Association for the Advancement of Cost Engineering (AACE): level of project definition: expressed as percentage of complete definition; end usage: typical purpose of estimation; methodology: typical estimating method; expected accuracy range: typical range relative to best index of 1; and preparation effort: typical degree of effort relative to least cost index of 1.

Yong Bai; Qiang Bai

2010-01-01T23:59:59.000Z

231

Discoveries | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Discoveries Discoveries Basic Energy Sciences (BES) BES Home About Research Facilities Science Highlights Benefits of BES Funding Opportunities Basic Energy Sciences Advisory Committee (BESAC) News & Resources Program Summaries Brochures Reports Accomplishments Discoveries Nobel Prizes Vignettes Archives Presentations BES and Congress Science for Energy Flow Seeing Matter Scale of Things Chart Contact Information Basic Energy Sciences U.S. Department of Energy SC-22/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-3081 F: (301) 903-6594 E: sc.bes@science.doe.gov More Information » Accomplishments Discoveries Print Text Size: A A A RSS Feeds FeedbackShare Page The Office of Basic Energy Sciences (BES) has been at the forefront of scientific discovery for several decades. BES staff and colleagues in March

232

V-122: IBM Tivoli Application Dependency Discovery Manager Java Multiple  

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

2: IBM Tivoli Application Dependency Discovery Manager Java 2: IBM Tivoli Application Dependency Discovery Manager Java Multiple Vulnerabilities V-122: IBM Tivoli Application Dependency Discovery Manager Java Multiple Vulnerabilities March 29, 2013 - 6:00am Addthis PROBLEM: IBM has acknowledged multiple vulnerabilities in IBM Tivoli Application Dependency Discovery Manager PLATFORM: The vulnerabilities are reported in version 7.2.0.0 through 7.2.1.3 ABSTRACT: Multiple security vulnerabilities exist in the Java Runtime Environments (JREs) that can affect the security of IBM Tivoli Application Dependency Discovery Manager. REFERENCE LINKS: Secunia Advisory SA52829 IBM Security Bulletin 1631786 CVE-2012-1531 CVE-2012-3143 CVE-2012-3216 CVE-2012-4820 CVE-2012-4822 CVE-2012-5069 CVE-2012-5071 CVE-2012-5073 CVE-2012-5075 CVE-2012-5079

233

V-122: IBM Tivoli Application Dependency Discovery Manager Java Multiple  

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

2: IBM Tivoli Application Dependency Discovery Manager Java 2: IBM Tivoli Application Dependency Discovery Manager Java Multiple Vulnerabilities V-122: IBM Tivoli Application Dependency Discovery Manager Java Multiple Vulnerabilities March 29, 2013 - 6:00am Addthis PROBLEM: IBM has acknowledged multiple vulnerabilities in IBM Tivoli Application Dependency Discovery Manager PLATFORM: The vulnerabilities are reported in version 7.2.0.0 through 7.2.1.3 ABSTRACT: Multiple security vulnerabilities exist in the Java Runtime Environments (JREs) that can affect the security of IBM Tivoli Application Dependency Discovery Manager. REFERENCE LINKS: Secunia Advisory SA52829 IBM Security Bulletin 1631786 CVE-2012-1531 CVE-2012-3143 CVE-2012-3216 CVE-2012-4820 CVE-2012-4822 CVE-2012-5069 CVE-2012-5071 CVE-2012-5073 CVE-2012-5075 CVE-2012-5079

234

Role of Modeling and Simulation in Scientific Discovery | Department of  

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

Role of Modeling and Simulation in Scientific Discovery Role of Modeling and Simulation in Scientific Discovery Role of Modeling and Simulation in Scientific Discovery January 29, 2013 - 10:14am Addthis Role of Modeling and Simulation in Scientific Discovery What are the key facts? Modeling and simulation supplement theory and experimentation, improving the scientific method. Industry that has embraced modeling and simulation has realized huge savings in cost and time in getting thier products to market. Modeling and simulation should never be viewed as a substitute for real-world experimentation. Scientific discovery, or understanding, involves the formulation of theory to explain observed phenomena, the design and execution of experiments to test theory and the feedback of experimental results to evolve theory. This

235

DISCOVERY OF A PROTOCLUSTER AT z {approx} 6  

SciTech Connect

We report the discovery of a protocluster at z {approx} 6 containing at least eight cluster member galaxies with spectroscopic confirmations in the wide-field image of the Subaru Deep Field (SDF). The overdensity of the protocluster is significant at the 6{sigma} level, based on the surface number density of i'-dropout galaxies. The overdense region covers {approx}6' Multiplication-Sign 6' (14 Mpc Multiplication-Sign 14 Mpc in comoving units at z = 6) and includes 30 i'-dropout galaxies. Follow-up spectroscopy revealed that 15 of these are real z {approx} 6 galaxies (5.7 < z < 6.3). Of these 15, 8 are clustering in a narrow redshift range ({Delta}z < 0.05 centered at z = 6.01), corresponding to a seven-fold increase in number density over the average in redshift space. We found no significant difference in the observed properties, such as Ly{alpha} luminosities and UV continuum magnitudes, between the eight protocluster members and the seven non-members. The velocity dispersion of the eight protocluster members is 647 {+-} 124 km s{sup -1}, which is about three times higher than that predicted by the standard cold dark matter model. This discrepancy could be attributed to the distinguishing three-dimensional distribution of the eight protocluster members. We discuss two possible explanations for this discrepancy: either the protocluster is already mature, with old galaxies at the center, or it is still immature and composed of three subgroups merging to become a larger cluster. In either case, this concentration of z = 6.01 galaxies in the SDF may be one of the first sites of formation of a galaxy cluster in the universe.

Toshikawa, Jun; Kashikawa, Nobunari; Shibuya, Takatoshi; Ishizaki, Yoshifumi [Department of Astronomy, School of Science, Graduate University for Advanced Studies, Mitaka, Tokyo 181-8588 (Japan); Ota, Kazuaki; Nagao, Tohru [Department of Astronomy, Graduate School of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502 (Japan); Morokuma, Tomoki; Motohara, Kentaro [Institute of Astronomy, University of Tokyo, Mitaka, Tokyo 181-0015 (Japan); Hayashi, Masao [Optical and Infrared Astronomy Division, National Astronomical Observatory, Mitaka, Tokyo 181-8588 (Japan); Jiang, Linhua; Egami, Eiichi [Steward Observatory, University of Arizona, 933 North Chery Avenue, Tucson, AZ 85721 (United States); Malkan, Matthew A. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547 (United States); Shimasaku, Kazuhiro, E-mail: jun.toshikawa@nao.ac.jp [Department of Astronomy, University of Tokyo, Hongo, Tokyo 113-0033 (Japan)

2012-05-10T23:59:59.000Z

236

E-Print Network 3.0 - analysis accurate discovery Sample Search...  

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

of faster discovery and space increase... and discovery of service information in mobile ad hoc networks. By extending Bloom filter-based service... summarization scheme, our...

237

E-Print Network 3.0 - antimalarial drug discovery Sample Search...  

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

assessment for antiparasitic drug discovery Julie A. Frearson, Paul... G. Wyatt, Ian H. Gilbert and Alan H. Fairlamb Drug Discovery Unit, College of Life Sciences... , University...

238

E-Print Network 3.0 - antimicrobial drug discovery Sample Search...  

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

assessment for antiparasitic drug discovery Julie A. Frearson, Paul... G. Wyatt, Ian H. Gilbert and Alan H. Fairlamb Drug Discovery Unit, College of Life Sciences... , University...

239

A critical review of methods used in the estimation of natural gas reserves: Natural gas reserves in the state of Texas. Some educational prerequisites in the field of petroleum economics and evaluation.  

E-Print Network (OSTI)

-Associated Gas Reserves Volumetr ic Method Discussion of the Factors in tne Volumetri. Formula The Decline Curve Method 7 7 12 Ie Methods of Estimating Associated Gas Reserves Methods of Estimatmg Dissolved Gas Reserves Water Drive Constant Voluxne... Bibliography 58 TABLE of ILLUSTRATIONS ~Pa e A CRITICAI REVIEW OF METHODS USED IN THE ESTIMATION OF NATURAL GAS RESERVES Curves Curve No Curves Showing Change in the Compressi- bility Factor with Depth and Composition of the Wet Gas. Z4-A Curve No...

Crichton, John Alston

2012-06-07T23:59:59.000Z

240

Robust Semiparametric Regression Estimation Using Targeted Maximum Likelihood with Application to Biomarker Discovery and Epidemiology  

E-Print Network (OSTI)

testing, while for TMLE VIM there were 197 and 204 genesand has the second highest VIM values in both lists. Beyond3.4.1. SWI4?SWI6 Marginal VIM Many of the trends in Figure

Tuglus, Catherine Ann

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Internal Dose Estimates from  

E-Print Network (OSTI)

Appendix F Internal Dose Estimates from NTS Fallout F-1 #12;Radiation Dose to the Population;TABLE OF CONTENTS Page F- Part I. Estimates of Dose...........................................................................................40 Comparison to dose estimates from global fallout

242

Pantex night held at discovery center | National Nuclear Security  

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

night held at discovery center | National Nuclear Security night held at discovery center | 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 > Pantex night held at discovery center Pantex night held at discovery center Posted By Office of Public Affairs More than 500 Pantexans and their families attended Pantex Night at the Don

243

Pantex night held at discovery center | National Nuclear Security  

National Nuclear Security Administration (NNSA)

night held at discovery center | National Nuclear Security night held at discovery center | 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 > Pantex night held at discovery center Pantex night held at discovery center Posted By Office of Public Affairs More than 500 Pantexans and their families attended Pantex Night at the Don

244

A First in Combining Science Discovery Technologies: Federated Search and  

Office of Scientific and Technical Information (OSTI)

A First in Combining Science Discovery Technologies: Federated Search and A First in Combining Science Discovery Technologies: Federated Search and Speech-Indexed Multimedia Office of Scientific & Technical Information NEWS MEDIA CONTACT: Cathey Daniels, (865) 576-9539 FOR IMMEDIATE RELEASE June 8, 2011 A First in Combining Science Discovery Technologies: Federated Search and Speech-Indexed Multimedia Oak Ridge, TN - The DOE Office of Scientific and Technical Information (OSTI) announced today a new tool in scientific discovery technology. Now citizens and researchers alike can search for both written and spoken words in a whole range of media using OSTI's new, speech-indexed multimedia within large scientific search portals. To this point, online searches for scientific information have been limited to text, such as within scientific

245

2006 Department of Energy Strategic Plan - Scientific Discovery and  

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

Department of Energy Strategic Plan - Scientific Discovery and Department of Energy Strategic Plan - Scientific Discovery and Innovation 2006 Department of Energy Strategic Plan - Scientific Discovery and Innovation The United States has always been a Nation of innovators and the Department of Energy has been a major contributor to that legacy. DOE-supported basic research has produced Nobel Laureates, numerous paradigm-shifting scientific discoveries, and revolutionary technologies that have spawned entirely new industries. Such breakthroughs have created fundamentally new energy options, underpinned U.S. national security during challenging times, and contributed to the health of our citizenry and the stewardship of our Nation's environmental resources. This great engine of U.S. innovation has played an important role in fueling a strong economy and one

246

RIKEN Center for Sustainable Resource Science Gene Discovery Research Group  

E-Print Network (OSTI)

Research Team Biomass Research Platform Team Drug Discovery Platforms Cooperation Divison Chemical Bank Systems Research Group Plant Immunity Research Group Chemical Genomics Research Group Advanced Catalysis Integrated Genome Informatics Research Unit Chemical Biology Research Group Molecular Ligand Target Research

Fukai, Tomoki

247

Allele Discovery Platform (ADP) in Papaya (Carica papaya L.)  

Science Journals Connector (OSTI)

TILLING (targeting induced local lesion in genome)/ADP (allele discovery platform) is a tool for creating variability in ... species. For decades, plant breeders have used chemicals as well as fast-moving ionizin...

P. K. Anish Kumar; Anjanabha Bhattacharya; O. P. Dutta

2014-01-01T23:59:59.000Z

248

Paradise Found: Nature in America at the Time of Discovery  

E-Print Network (OSTI)

Review of Paradise Found: Nature in America at the Time of Discovery. Steve Nicholls. 2009. University of Chicago Press, New York and London. Pp. 536. ISBN10: 0226583406 ISBN13: 978-0226583402....

Pierotti, Raymond

2011-08-15T23:59:59.000Z

249

Our Water World 4-H Marine Science Discovery Project  

E-Print Network (OSTI)

Our Water World 4-H Marine Science Discovery Project Leader Guide OREGON STATE UNIVERSITY EXTENSION. In each activity, supporting information is provided in a background section or as part of the procedures

Tullos, Desiree

250

Anne LaPointe > Director, Catalyst Discovery and Development...  

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

Anne LaPointe Director, Catalyst Discovery and Development Laboratory aml329@cornell.edu Dr. LaPointe received her PhD from the Massachusetts Institute of Technology and then went...

251

Ontology-based methodology for e-service discovery  

Science Journals Connector (OSTI)

Service discovery is a critical aspect in the Service Oriented Computing approach. A model, a methodology and a tool environment based on ontologies are proposed in this paper. The requester and provider perspectives are discussed, both to support the ...

Devis Bianchini; Valeria De Antonellis; Barbara Pernici; Pierluigi Plebani

2006-06-01T23:59:59.000Z

252

Discovery of Ethanol-Responsive Small RNAs in Zymomonas mobilis  

Science Journals Connector (OSTI)

...Biotechnology Discovery of Ethanol-Responsive Small RNAs in...bacterium that can produce ethanol by fermentation. Due to its unique metabolism and efficient ethanol production, Z. mobilis has...special interest for biofuel energy applications; an important...

Seung Hee Cho; Roy Lei; Trey D. Henninger; Lydia M. Contreras

2014-05-02T23:59:59.000Z

253

Discovery of Ethanol-Responsive Small RNAs in Zymomonas mobilis  

Science Journals Connector (OSTI)

...research-article Biotechnology Discovery of Ethanol-Responsive Small RNAs in Zymomonas...mobilis is a bacterium that can produce ethanol by fermentation. Due to its unique metabolism and efficient ethanol production, Z. mobilis has attracted...

Seung Hee Cho; Roy Lei; Trey D. Henninger; Lydia M. Contreras

2014-05-02T23:59:59.000Z

254

Domain-specific Web Service Discovery with Service Class Descriptions  

SciTech Connect

This paper presents DynaBot, a domain-specific web service discovery system. The core idea of the DynaBot service discovery system is to use domain-specific service class descriptions powered by an intelligent Deep Web crawler. In contrast to current registry-based service discovery systems--like the several available UDDI registries--DynaBot promotes focused crawling of the Deep Web of services and discovers candidate services that are relevant to the domain of interest. It uses intelligent filtering algorithms to match services found by focused crawling with the domain-specific service class descriptions. We demonstrate the capability of DynaBot through the BLAST service discovery scenario and describe our initial experience with DynaBot.

Rocco, D; Caverlee, J; Liu, L; Critchlow, T J

2005-02-14T23:59:59.000Z

255

CONTENTS JIP Leg II Discovery .......................1 Alaska Seep Studies .....................6  

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

JIP Leg II Discovery .......................1 JIP Leg II Discovery .......................1 Alaska Seep Studies .....................6 Gas Hydrates Offshore Mexico 10 Alaska Reservoir Testing ...........12 Naval Research Laboratory Methane Hydrate Research .....17 Announcements ...................... 21 * Call for Papers * 2009 Hydrate Fellows * USGS Mendenhall Fellowship * AGU Annual Meeting * Moscow Conference * Gordon Research Conference Spotlight on Research .......... 24 Dan McConnell CONTACT Ray Boswell Technology Manager-Methane Hydrates, Strategic Center for Natural Gas & Oil 304-285-4541 ray.boswell@netl.doe.gov

256

Cost Estimation Package  

Directives, Delegations, and Requirements

This chapter focuses on the components (or elements) of the cost estimation package and their documentation.

1997-03-28T23:59:59.000Z

257

Check Estimates and Independent Costs  

Directives, Delegations, and Requirements

Check estimates and independent cost estimates (ICEs) are tools that can be used to validate a cost estimate. Estimate validation entails an objective review of the estimate to ensure that estimate criteria and requirements have been met and well documented, defensible estimate has been developed. This chapter describes check estimates and their procedures and various types of independent cost estimates.

1997-03-28T23:59:59.000Z

258

Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Camp Discovery Helps Camp Discovery Helps Kids Build an Electric Dune Buggy to someone by E-mail Share Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on Facebook Tweet about Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on Twitter Bookmark Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on Google Bookmark Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on Delicious Rank Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on Digg Find More places to share Alternative Fuels Data Center: Camp Discovery Helps Kids Build an Electric Dune Buggy on AddThis.com... Feb. 5, 2011 Camp Discovery Helps Kids Build an Electric Dune Buggy

259

Cobalt discovery replaces precious metals as industrial catalyst  

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

Cobalt Discovery Replaces Precious Metals Cobalt Discovery Replaces Precious Metals Cobalt discovery replaces precious metals as industrial catalyst Cobalt holds promise as an industrial catalyst with potential applications in such energy-related technologies such as production of biofuels and reduction of carbon dioxide. November 26, 2012 The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. Contact Nancy Ambrosiano Communications Office (505) 699-1149 Email Catalysts are also integral to thousands of industrial, synthetic, and

260

Melvin Schwartz and the Discovery of the Muon Neutrino  

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

Melvin Schwartz and the Discovery of the Muon Neutrino Melvin Schwartz and the Discovery of the Muon Neutrino Resources with Additional Information Melvin Schwartz Courtesy Brookhaven National Laboratory Melvin Schwartz was the co-winner of the 1988 Nobel Prize in Physics "for the neutrino beam method and the demonstration of the doublet structure of the leptons through the discovery of the muon neutrino". 'In 1962, Schwartz, with Leon Lederman and Jack Steinberger ... discovered the muon neutrino at the Alternating Gradient Synchrotron (AGS), the then brand-new accelerator at the U.S. Department of Energy's Brookhaven National Laboratory. ... First coming to Brookhaven in 1955, Schwartz performed his Ph.D. thesis research through 1956 at the Laboratory's first accelerator, the Cosmotron. While finishing his thesis, he was employed by the Laboratory from 1956-58.

Note: This page contains sample records for the topic "field discoveries estimated" 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

Creative Discovery Museum : BioEnergy Science Center  

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

The Creative Discovery Museum The Creative Discovery Museum BESC reaches thousands of students with 'Farming for Fuels' lessons The DOE BioEnergy Science Center and the Creative Discovery Museum in Chattanooga, TN, have developed a set of hands-on lesson plans on BioFuels aimed at students in fourth, fifth and sixth grades. These "Farming for Fuels" lessons educate students about the carbon cycle, the use of lignocellulosic biomass as a substrate for the production of biofuels and the technical and economic obstacles to a bio-based fuel economy. The nationally expanded outreach program has now reached more than 60,000 students, teachers and parents by partnering with museums and centers in Tennessee, Georgia, Texas, Michigan, Illinois, Florida, New York and Arizona. To extend use of the lessons to the general public we have assembled

262

Tools for Discovery Offer Potential Hope for Huntington's | Department of  

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

Tools for Discovery Offer Potential Hope for Huntington's Tools for Discovery Offer Potential Hope for Huntington's Tools for Discovery Offer Potential Hope for Huntington's May 25, 2011 - 3:24pm Addthis Flora Meilleur prepares protein solutions for structural investigation with neutrons. | Courtesy of ORNL Flickr / Jason Richards Flora Meilleur prepares protein solutions for structural investigation with neutrons. | Courtesy of ORNL Flickr / Jason Richards Charles Rousseaux Charles Rousseaux Senior Writer, Office of Science What does this mean for me? Scientists at ORNL's Center for Structural Molecular Biology are using Bio-SANS to see how biological structures look in their natural state ORNL's tools are leading to better targets and perhaps even potential treatments for diseases like Huntington's. Sometimes the right tool can shape the world . . . or even better, touch a

263

Cobalt discovery replaces precious metals as industrial catalyst  

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

Cobalt discovery replaces precious metals Cobalt discovery replaces precious metals Cobalt discovery replaces precious metals as industrial catalyst Cobalt holds promise as an industrial catalyst with potential applications in such energy-related technologies such as production of biofuels and reduction of carbon dioxide. November 26, 2012 The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. Contact Nancy Ambrosiano Communications Office (505) 699-1149 Email Catalysts are also integral to thousands of industrial, synthetic, and

264

Lab Breakthrough: Nanomaterials Discoveries Lead to Possible Cancer  

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

Lab Breakthrough: Nanomaterials Discoveries Lead to Possible Cancer Lab Breakthrough: Nanomaterials Discoveries Lead to Possible Cancer Treatment Lab Breakthrough: Nanomaterials Discoveries Lead to Possible Cancer Treatment June 4, 2012 - 3:05pm Addthis Argonne nanoscientist Elena Rozhkova is studying ways to enlist nanoparticles to treat brain cancer. This nano-bio technology may eventually provide an alternative form of therapy that targets only cancer cells and does not affect normal living tissue. View the entire Lab Breakthrough playlist. Michael Hess Michael Hess Former Digital Communications Specialist, Office of Public Affairs What is a nano-bio catalyst? A nanoparticle that triggers specific reactions in cells. The particle attaches to unwanted (tumor) cells, and when researchers shine light on them, they kill the cells through oxidation.

265

Cobalt discovery replaces precious metals as industrial catalyst  

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

Cobalt Discovery Replaces Precious Metals Cobalt Discovery Replaces Precious Metals Cobalt discovery replaces precious metals as industrial catalyst Cobalt holds promise as an industrial catalyst with potential applications in such energy-related technologies such as production of biofuels and reduction of carbon dioxide. November 26, 2012 The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. The artwork depicts the substitution of cobalt for precious metals in catalysis as a variation on the ancient alchemical theme of transmuting base metals into precious ones. Contact Nancy Ambrosiano Communications Office (505) 699-1149 Email Catalysts are also integral to thousands of industrial, synthetic, and

266

Flow cytometry aids basic cell biology research and drug discovery  

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

Flow cytometry aids basic cell biology research and drug discovery Flow cytometry aids basic cell biology research and drug discovery Flow cytometry aids basic cell biology research and drug discovery Life Technologies Corporation and LANL have released the Attune® Acoustic Focusing Cytometer, featuring a reduced footprint, reduced consumables, and an affordable price. April 3, 2012 Attune® Acoustic Focusing Cytometer The Attune® Acoustic Focusing Cytometer achieves sample throughput at rates over 10 times faster than other cytometers-up to 1,000 μL per minute. In December 2009, Life Technologies Corporation announced the release of the Attune® Acoustic Focusing Cytometer, a first-of-its-kind cytometer system based on technology developed at Los Alamos National Laboratory (LANL). Examining cells has never been clearer with LANL's use of acoustic waves

267

The Top Quark, Its Discovery, and Subsequent Research  

Office of Scientific and Technical Information (OSTI)

The Top Quark, Its Discovery, and Subsequent Research The Top Quark, Its Discovery, and Subsequent Research Resources with Additional Information 'Ever since the existence of the bottom (or b) quark was inferred from the discovery of the Upsilon family of resonances at Fermilab in 1977, particle physicists have been on the lookout for its partner, called top (or t). The long search, which occupied experimenters at laboratories around the world, came to a successful conclusion in February 1995 with the announcement that the top quark had been observed in two experiments at the Tevatron proton-antiproton collider at Fermilab. ... Top Quark Courtesy Fermilab Top is the last of the fundamental constituents of subnuclear matter that theories of the strong, weak, and electromagnetic interactions and a wealth of experimental information had led particle physicists to expect. Theoretically, top's existence was required to make the electroweak theory internally consistent.'1

268

Artificial neural network modeling and cluster analysis for organic facies and burial history estimation using well log data: A case study of the South Pars Gas Field, Persian Gulf, Iran  

Science Journals Connector (OSTI)

Intelligent and statistical techniques were used to extract the hidden organic facies from well log responses in the Giant South Pars Gas Field, Persian Gulf, Iran. Kazhdomi Formation of Mid-Cretaceous and Kangan-Dalan Formations of Permo-Triassic Data ... Keywords: Artificial neural network, Burial history, Cluster analysis, Organic facies, Rock-Eval pyrolysis, Well log data

Bahram Alizadeh; Saeid Najjari; Ali Kadkhodaie-Ilkhchi

2012-08-01T23:59:59.000Z

269

Radiation Dose Estimates from  

E-Print Network (OSTI)

Summary: Radiation Dose Estimates from Hanford Radioactive Material Releases to the Air- tantly, what radiation dose people may have received. An independent Technical Steering Panel (TSP, additionalProjectworkcouldresultin revisions of these dose estimates. April 21, 1994 Companion

270

State Energy Production Estimates  

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

State Energy Production Estimates 1960 Through 2012 2012 Summary Tables Table P1. Energy Production Estimates in Physical Units, 2012 Alabama 19,455 215,710 9,525 0 Alaska 2,052...

271

DISCOVERY OF THE SMALL-DIAMETER, YOUNG SUPERNOVA REMNANT G354.4+0.0  

SciTech Connect

We report the discovery of a shell-like structure G354.4+0.0 of size 1.'6 that shows the morphology of a shell supernova remnant (SNR). Part of the structure shows polarized emission in a NRAO VLA sky survey map. Based on 330 MHz and 1.4 GHz Giant Metrewave Radio Telescope observations and existing observations at higher frequencies, we conclude that the partial shell structure showing synchrotron emission is embedded in an extended H II region of size {approx}4'. The spectrum of the diffuse H II region turns over between 1.4 GHz and 330 MHz. The H I absorption spectrum shows this objected to be located more than 5 kpc from Sun. Based on its morphology, non-thermal polarized emission, and size, this object is one of the youngest SNRs discovered in the Galaxy with an estimated age of {approx}100-500 yr.

Roy, Subhashis [NCRA-TIFR, Pune 411007 (India); Pal, Sabyasachi, E-mail: roy@ncra.tifr.res.in, E-mail: sabya@csp.res.in [Indian Centre for Space Physics, Kolkata 700084 (India)

2013-09-10T23:59:59.000Z

272

Can a Single High-energy Neutrino from Gamma-ray Bursts be a Discovery?  

E-Print Network (OSTI)

Current emission models of GeV-PeV neutrinos from gamma-ray bursts (GRBs) predict a neutrino flux with $\\ll1$ detected neutrinos per GRB with kilometer-scale neutrino observatories. The detection of this flux will require the stacking of data from a large number of GRBs, leading to an increased background rate, decreasing the significance of a single neutrino detection. We show that utilizing the temporal correlation between the expected gamma-ray and neutrino fluxes, one can significantly improve the neutrino signal-to-noise ratio. We describe how this temporal correlation can be used. Using realistic GRB and atmospheric neutrino fluxes and incorporating temporal, spectral and directional information, we estimate the probability of a single detected GRB-neutrino being a 5-sigma discovery.

Bartos, Imre

2014-01-01T23:59:59.000Z

273

Machine-learning algorithm aims to accelerate materials discovery | Argonne  

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

Science Science Computing, Environment & Life Sciences Energy Engineering & Systems Analysis Photon Sciences Physical Sciences & Engineering Energy Frontier Research Centers Science Highlights Postdoctoral Researchers Machine-learning algorithm aims to accelerate materials discovery July 16, 2013 Tweet EmailPrint A research team led by Argonne Leadership Computing Facility computational chemist Anatole von Lilienfeld is developing an algorithm that combines quantum chemistry with machine learning (artificial intelligence) to enable atomistic simulations that predict the properties of new materials with unprecedented speed. From innovations in medicine to novel materials for next-generation batteries, this approach could greatly accelerate the pace of materials discovery, with high-performance

274

Types of Cost Estimates  

Directives, Delegations, and Requirements

The chapter describes the estimates required on government-managed projects for both general construction and environmental management.

1997-03-28T23:59:59.000Z

275

External Dose Estimates from  

E-Print Network (OSTI)

Appendix G External Dose Estimates from Global Fallout G-1 #12;External Radiation Exposure-MQ-003539 March 15, 2000 G-2 #12;Abstract This report provides estimates of the external radiation-62. Estimates are given on a county by county basis for each month from 1953-1972. The average population dose

276

External Dose Estimates from  

E-Print Network (OSTI)

Appendix E External Dose Estimates from NTS Fallout E-1 #12;External Radiation Exposure. 1, 1999) E-2 #12;Abstract This report provides estimates of the external radiation exposure of this report to: "Prepare crude estimates of the doses from external irradiation received by the American

277

Practice Field Practice Field  

E-Print Network (OSTI)

Courts Soccer Field Swimming pool Bandeen Hall Mountain House # 3 # 2 Golf Course Security Patterson Hall.B. Scott Arena Library Centennial Theater Mc Greer Hall Pollack Hall New Johnson Science Building Dewhurst Dining Hall Champlain Regional College # 4 Mackinnon Hall Residence # 6 Memorial House Retired Faculty

278

Reconstruction efficiency and discovery potential of a Mediterranean neutrino telescope: A simulation study using the Hellenic Open University Simulation & Reconstruction (HOURS) package  

E-Print Network (OSTI)

We report on the evaluation of the performance of a Mediterranean very large volume neutrino telescope. We present results of our studies concerning the capability of the telescope in detecting/discovering galactic (steady point sources) and extragalactic, transient (Gamma Ray Bursts) high energy neutrino sources as well as measuring ultra high energy diffuse neutrino fluxes. The neutrino effective area and angular resolution are presented as a function of the neutrino energy, and the background event rate (atmospheric neutrinos and muons) is estimated. The discovery potential of the neutrino telescope is evaluated and the experimental time required for a significant discovery of potential neutrino emitters (known from their gamma ray emission, assumedly produced by hadronic interactions) is estimated. For the simulation we use the HOU Reconstruction & Simulation (HOURS) software package.

Tsirigotis, A G; Tzamarias, S E

2012-01-01T23:59:59.000Z

279

A simple method to estimate interwell autocorrelation  

SciTech Connect

The estimation of autocorrelation in the lateral or interwell direction is important when performing reservoir characterization studies using stochastic modeling. This paper presents a new method to estimate the interwell autocorrelation based on parameters, such as the vertical range and the variance, that can be estimated with commonly available data. We used synthetic fields that were generated from stochastic simulations to provide data to construct the estimation charts. These charts relate the ratio of areal to vertical variance and the autocorrelation range (expressed variously) in two directions. Three different semivariogram models were considered: spherical, exponential and truncated fractal. The overall procedure is demonstrated using field data. We find that the approach gives the most self-consistent results when it is applied to previously identified facies. Moreover, the autocorrelation trends follow the depositional pattern of the reservoir, which gives confidence in the validity of the approach.

Pizarro, J.O.S.; Lake, L.W. [Univ. of Texas, Austin, TX (United States)

1997-08-01T23:59:59.000Z

280

The strength of galactic magnetic fields  

Science Journals Connector (OSTI)

... UK THE magnitudes of galactic magnetic fields are usually estimated from measurements of the radio synchroton emission arising from acceleration of cosmic-ray electrons in the magnetic field. To interpret ...

X. Chi; A. W. Wolfendale

1993-04-15T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Overlapping Community Discovery Methods: A Survey  

E-Print Network (OSTI)

The detection of overlapping communities is a challenging problem which is gaining increasing interest in recent years because of the natural attitude of individuals, observed in real-world networks, to participate in multiple groups at the same time. This review gives a description of the main proposals in the field. Besides the methods designed for static networks, some new approaches that deal with the detection of overlapping communities in networks that change over time, are described. Methods are classified with respect to the underlying principles guiding them to obtain a network division in groups sharing part of their nodes. For each of them we also report, when available, computational complexity and web site address from which it is possible to download the software implementing the method.

Amelio, Alessia

2014-01-01T23:59:59.000Z

282

Serendipitous discoveries in nonlocal gravity theory  

Science Journals Connector (OSTI)

We present a class of generally covariant nonlocal gravity models which have a flat-space general relativistic limit and also possess a stable deSitter or anti-deSitter (AdS) background with an arbitrary value of its cosmological constant. The nonlocal action of the theory is formulated in the Euclidean signature spacetime and is understood as an approximation to the quantum effective action (generating functional of one-particle irreducible diagrams) originating from fundamental quantum gravity theory. Using the known relation between the Schwinger-Keldysh technique for quantum expectation values and the Euclidean quantum field theory we derive from this action the causal effective equations of motion for mean value of the metric field in the physical Lorentzian-signature spacetime. Thus we show that the (A)dS background of the theory carries as free propagating modes massless gravitons having two polarizations identical to those of the Einstein theory with a cosmological term. The on-shell action of the theory is vanishing both for the flat-space and (A)dS backgrounds which play the role of stable vacua underlying, respectively, the ultraviolet and infrared phases of the theory. We also obtain linearized gravitational potentials of compact matter sources and show that in the infrared (A)dS phase their effective gravitational coupling Geff can be essentially different from the Newton gravitational constant GN of the short-distance general relativistic phase. When Geff?GN the (A)dS phase can be regarded as a strongly coupled infrared modification of Einstein theory not only describing the dark energy mechanism of cosmic acceleration but also simulating the dark matter phenomenon by enhanced gravitational attraction at long distances.

A. O. Barvinsky

2012-05-09T23:59:59.000Z

283

DISCOVERY OF MUTATED SUBNETWORKS ASSOCIATED WITH CLINICAL DATA IN CANCER  

E-Print Network (OSTI)

DISCOVERY OF MUTATED SUBNETWORKS ASSOCIATED WITH CLINICAL DATA IN CANCER FABIO VANDIN, PATRICK CLAY,pclay,eli,braphael}@cs.brown.edu A major goal of cancer sequencing projects is to identify genetic alterations that determine clinical phenotypes, such as survival time or drug response. Somatic mutations in cancer are typically very diverse

Raphael, Ben J.

284

Discovery of Fraud Rules for Telecommunications -Challenges and Solutions  

E-Print Network (OSTI)

Discovery of Fraud Rules for Telecommunications - Challenges and Solutions Saharon Rosset, Uzi'anana 43000, Israel uzimu, einatn, yizhaki }@amdocs.com ABSTRACT Many fraud analysis systemshave rules suitable for fraud analysis make this problem unique. Among themarethe following: the needto find

Shamir, Ron

285

AOC-by-self-discovery modeling and simulation for HIV  

Science Journals Connector (OSTI)

Among HIV, immune cell and drug, exhibit interactions that are usually not well understood and as a result, cannot be accurately modeled. In this paper, Modeling by AOC is to understand the dynamics of HIV infection and treatment. The use of AOC-by-self-discovery ...

Chunxiao Zhao; Ning Zhong; Ying Hao

2007-09-01T23:59:59.000Z

286

Discovery in Hydrating Plaster Using Multiple Machine Learning Methods  

E-Print Network (OSTI)

Discovery in Hydrating Plaster Using Multiple Machine Learning Methods Judith E. Devaney, John G plaster over multiple time periods. We use three dimensional data obtained through X-ray microtomography of the plaster datasets that had been labeled with their autoclass predictions. The rules were found to have both

Fernandez, Thomas

287

Historical review of californium-252 discovery and development  

SciTech Connect

This paper discusses the discovery and history of californium 252. This isotope may be synthesized by irradiating plutonium 239, plutonium 242, americium 243, or curium 244 with neutrons in a nuclear reactor. Various experiments and inventions involving /sup 252/Cf conducted at the Savannah River Plant are discussed. The evolution of radiotherapy using californium 252 is reviewed. (PLG)

Stoddard, D.H.

1985-01-01T23:59:59.000Z

288

Machine-assisted discovery of relationships in astronomy  

Science Journals Connector (OSTI)

......relationships in the HR diagram, the Fundamental Plane of elliptical galaxies and the...abilities such as not just relying on brute-force searches of feature spaces but being...The Data Mining and Knowledge Discovery Handbook-Maimon O., Rokach L., eds. (2010......

Matthew J. Graham; S. G. Djorgovski; Ashish A. Mahabal; Ciro Donalek; Andrew J. Drake

2013-01-01T23:59:59.000Z

289

Discovery of Rubidium, Strontium, Molybdenum, and Rhodium Isotopes  

E-Print Network (OSTI)

Currently, thirty-one rubidium, thirty-five strontium, thirty-five molybdenum and thirty-eight rhodium isotopes have been observed and the discovery of these isotopes is discussed here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented.

Parker, A M

2011-01-01T23:59:59.000Z

290

Discovery of rubidium, strontium, molybdenum, and rhodium isotopes  

SciTech Connect

Currently, 31 rubidium, 35 strontium, 35 molybdenum, and 38 rhodium isotopes have been observed and the discovery of these isotopes is described here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented.

Parker, A.M.; Thoennessen, M., E-mail: thoennessen@nscl.msu.edu

2012-07-15T23:59:59.000Z

291

Discovery of Rubidium, Strontium, Molybdenum, and Rhodium Isotopes  

E-Print Network (OSTI)

Currently, thirty-one rubidium, thirty-five strontium, thirty-five molybdenum and thirty-eight rhodium isotopes have been observed and the discovery of these isotopes is discussed here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented.

A. M. Parker; M. Thoennessen

2011-02-11T23:59:59.000Z

292

Classification and knowledge discovery in protein databases Predrag Radivojaca,1  

E-Print Network (OSTI)

structure [2], tertiary structure [3], protein disorder [4,5], relative solvent accessibility [6], switchClassification and knowledge discovery in protein databases Predrag Radivojaca,1 , Nitesh V Abstract We consider the problem of classification in noisy, high-dimensional, and class-imbalanced protein

Obradovic, Zoran

293

Fast top-k simple shortest paths discovery in graphs  

Science Journals Connector (OSTI)

With the wide applications of large scale graph data such as social networks, the problem of finding the top-k shortest paths attracts increasing attention. This paper focuses on the discovery of the top-k simple shortest paths (paths without ... Keywords: graphs, shortest path, top-k

Jun Gao; Huida Qiu; Xiao Jiang; Tengjiao Wang; Dongqing Yang

2010-10-01T23:59:59.000Z

294

Comparative Genomic Discovery of miRNAs Grad et al.  

E-Print Network (OSTI)

Comparative Genomic Discovery of miRNAs Grad et al. Computational and Experimental Identification throughout the adult life cycle (Feinbaum and Ambros, 1999; Lee et al., 1993; Reinhart et al., 2000 al., 1993; Wightman et al., 1993; Reinhart et al., 2000; Slack et al., 2000). Both lin-4 and let-7

Church, George M.

295

An Incremental, Probabilistic Rough Set Approach to Rule Discovery  

E-Print Network (OSTI)

1 An Incremental, Probabilistic Rough Set Approach to Rule Discovery Ning Zhong, Ju­Zhen Dong, Setsuo Ohsuga, Tsau Young Lin Abstract--- This paper introduces an incremental, proba­ bilistic rough set. The approach is based on the combination of Generaliza­ tion Distribution Table (GDT) and the rough set

Lin, Tsau Young

296

Molecular Fragment Mining for Drug Discovery Christian Borgelt1  

E-Print Network (OSTI)

Molecular Fragment Mining for Drug Discovery Christian Borgelt1 , Michael R. Berthold2 , and David will be active or inactive, so that future chemical tests can be focused on the most promis- ing candidates that discriminate between active and inactive molecules. In this paper we review this approach as well as two

Berthold, Michael R.

297

Automatic Discovery of API-Level Vulnerabilities Vinod Ganapathy  

E-Print Network (OSTI)

Automatic Discovery of API-Level Vulnerabilities Vinod Ganapathy , Sanjit A. Seshia , Somesh Jha-MADISON COMPUTER SCIENCES TECHNICAL REPORT: UW-CS-TR-1512, JULY 2004. Abstract A system is vulnerable to an API-level attack if its security can be compromised by invoking an allowed sequence of operations from its API. We

Ganapathy, Vinod

298

Discovery of Potent Isoxazoline Glycoprotein IIb/IIIa Receptor Antagonists  

Science Journals Connector (OSTI)

Using the isoxazoline as a common structural feature, three series of glycoprotein IIb/IIIa receptor antagonists were evaluated, culminating in the discovery of XR299 (30). In an in vitro assay of platelet inhibition, XR299 had an IC50 of 0.24 ?M and was ...

John Wityak; Thais M. Sielecki; Donald J. Pinto; George Emmett; Jean Y. Sze; Jie Liu; A. Ewa Tobin; Shuaige Wang; Biao Jiang; Philip Ma; Shaker A. Mousa; Ruth R. Wexler; Richard E. Olson

1997-01-03T23:59:59.000Z

299

Short Communication Discovery of a regionally important green turtle  

E-Print Network (OSTI)

Short Communication Discovery of a regionally important green turtle Chelonia mydas rookery and other Syrian beaches was undertaken to improve and update knowledge of Syria's marine turtle nesting populations. The survey confirmed that loggerhead turtles Caretta caretta nest in Syria (eight nests recorded

Exeter, University of

300

Linked Environments for Atmospheric Discovery Linked Environments for Atmospheric  

E-Print Network (OSTI)

Unidata Program Center #12;Linked Environments for Atmospheric Discovery The Team: 9 institutions and 105 MethodologyTraditional NWP Methodology STATIC OBSERVATIONS Radar Data Mobile Mesonets Surface Observations Satellites The Process is Entirely Prescheduled and Serial; It Does NOT Respond to the Weather! The Process

Note: This page contains sample records for the topic "field discoveries estimated" 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

Discovery of Cesium, Lanthanum, Praseodymium and Promethium Isotopes  

E-Print Network (OSTI)

Currently, forty-one cesium, thirty-five lanthanum, thirty-two praseodymium, and thirty-one promethium, isotopes have been observed and the discovery of these isotopes is discussed here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented.

May, E

2011-01-01T23:59:59.000Z

302

Discovery of Cesium, Lanthanum, Praseodymium and Promethium Isotopes  

E-Print Network (OSTI)

Currently, forty-one cesium, thirty-five lanthanum, thirty-two praseodymium, and thirty-one promethium, isotopes have been observed and the discovery of these isotopes is discussed here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented.

E. May; M. Thoennessen

2011-09-08T23:59:59.000Z

303

LHC $Z^`$ discovery potential for models with continuously distributed mass  

E-Print Network (OSTI)

We study the Large Hadron Collider (LHC) discovery potential for $Z^`$ models with continuously distributed mass for $\\sqrt{s} = 7, 10$ and 14 TeV centre-of-mass energies. One of possible LHC signatures for such models is the existence of broad resonance in Drell-Yan reaction $pp \\to Z^` + ... \\to l^+l^- + ...$.

N. V. Krasnikov

2010-04-22T23:59:59.000Z

304

Research at Princeton ContentsDISCOVERY Research at Princeton 2012  

E-Print Network (OSTI)

-Performance Computers Princeton's International Research Sun on Earth: the Princeton Plasma Physics Laboratory Faculty winners. We are privileged and honored to manage the nearby Princeton Plasma Physics Laboratory (PPPLResearch at Princeton #12;ContentsDISCOVERY Research at Princeton 2012 Research Briefs Research

Rowley, Clarence W.

305

Automated Discovery of Structural Signatures of Protein Fold and Function  

E-Print Network (OSTI)

Automated Discovery of Structural Signatures of Protein Fold and Function Marcel Turcotte1 sys- tematically for protein fold signatures, we have explored the use of Inductive Logic Programming fold. The work showed that signatures of protein folds exist, about half of rules discov- ered

Muggleton, Stephen H.

306

THE EINSTEIN-HOME SEARCH FOR RADIO PULSARS AND PSR J2007+2722 DISCOVERY  

SciTech Connect

Einstein-Home aggregates the computer power of hundreds of thousands of volunteers from 193 countries, to search for new neutron stars using data from electromagnetic and gravitational-wave detectors. This paper presents a detailed description of the search for new radio pulsars using Pulsar ALFA survey data from the Arecibo Observatory. The enormous computing power allows this search to cover a new region of parameter space; it can detect pulsars in binary systems with orbital periods as short as 11 minutes. We also describe the first Einstein-Home discovery, the 40.8 Hz isolated pulsar PSR J2007+2722, and provide a full timing model. PSR J2007+2722's pulse profile is remarkably wide with emission over almost the entire spin period. This neutron star is most likely a disrupted recycled pulsar, about as old as its characteristic spin-down age of 404 Myr. However, there is a small chance that it was born recently, with a low magnetic field. If so, upper limits on the X-ray flux suggest but cannot prove that PSR J2007+2722 is at least {approx}100 kyr old. In the future, we expect that the massive computing power provided by volunteers should enable many additional radio pulsar discoveries.

Allen, B.; Knispel, B.; Aulbert, C.; Bock, O.; Eggenstein, H. B.; Fehrmann, H.; Machenschalk, B. [Max-Planck-Institut fuer Gravitationsphysik, D-30167 Hannover (Germany); Cordes, J. M.; Brazier, A.; Chatterjee, S. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Deneva, J. S. [Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612 (United States); Hessels, J. W. T. [ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo (Netherlands); Anderson, D. [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States); Demorest, P. B. [NRAO (National Radio Astronomy Observatory), Charlottesville, VA 22903 (United States); Gotthelf, E. V. [Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027 (United States); Hammer, D. [Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, WI 53211 (United States); Kaspi, V. M. [Department of Physics, McGill University, Montreal, QC H3A2T8 (Canada); Kramer, M. [Max-Planck-Institut fuer Radioastronomie, D-53121 Bonn (Germany); Lyne, A. G. [Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, M13 9PL (United Kingdom); McLaughlin, M. A., E-mail: bruce.allen@aei.mpg.de [Department of Physics, West Virginia University, Morgantown, WV 26506 (United States); and others

2013-08-20T23:59:59.000Z

307

THE EARLY EARLY TYPE: DISCOVERY OF A PASSIVE GALAXY AT z{sub spec} {approx} 3  

SciTech Connect

We present the discovery of a massive, quiescent galaxy at z = 2.99. We have obtained an Hubble Space Telescope WFC3 spectrum of this object and measured its redshift from the detection of a deep 4000 A break consistent with an old population and a high metallicity. By stellar population modeling of both its grism spectrum and broadband photometry, we derive an age of {approx}0.7 Gyr, implying a formation redshift of z > 4, and a mass >10{sup 11} M{sub Sun }. Although this passive galaxy is the most distant confirmed so far, we find that it is slightly less compact than other z > 2 early types of similar mass, being overall more analogous to those z {approx} 1.6 field early-type galaxies. The discovery of this object shows that early-type galaxies are detectable to at least z = 3 and suggests that the diversity of structural properties found in z = 1.4-2 ellipticals to earlier epochs could have its origin in a variety of formation histories among their progenitors.

Gobat, R.; Strazzullo, V.; Daddi, E.; Bethermin, M. [Laboratoire AIM-Paris-Saclay, CEA/DSM-CNRS, Universite Paris Diderot, Irfu/Service d'Astrophysique, CEA Saclay, Orme des Merisiers, F-91191 Gif sur Yvette (France); Onodera, M.; Carollo, M. [Institute for Astronomy, ETH Zuerich Wolfgang-Pauli-strasse 27, CH-8093 Zuerich (Switzerland); Renzini, A. [INAF, Osservatorio Astronomico di Padova Vicolo dell'Osservatorio 5, I-35122 Padova (Italy); Dickinson, M. [National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ 85726 (United States); Cimatti, A. [Dipartimento di Astronomia, Universita di Bologna, Via Ranzani 1, I-40127 Bologna (Italy)

2012-11-10T23:59:59.000Z

308

New approaches to estimation of magnetotelluric parameters  

SciTech Connect

Fully efficient robust data processing procedures were developed and tested for single station and remote reference magnetotelluric (Mr) data. Substantial progress was made on development, testing and comparison of optimal procedures for single station data. A principal finding of this phase of the research was that the simplest robust procedures can be more heavily biased by noise in the (input) magnetic fields, than standard least squares estimates. To deal with this difficulty we developed a robust processing scheme which combined the regression M-estimate with coherence presorting. This hybrid approach greatly improves impedance estimates, particularly in the low signal-to-noise conditions often encountered in the dead band'' (0.1--0.0 hz). The methods, and the results of comparisons of various single station estimators are described in detail. Progress was made on developing methods for estimating static distortion parameters, and for testing hypotheses about the underlying dimensionality of the geological section.

Egbert, G.D.

1991-01-01T23:59:59.000Z

309

E-Print Network 3.0 - accelerating scientific discovery Sample...  

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

scientific discovery Page: << < 1 2 3 4 5 > >> 1 U.S. Department of Energy Scientific Discovery through Advanced Computing SciDAC 2010 Summary: U.S. Department of Energy Scientific...

310

Genomics-Guided Discovery of Endophenazines from Kitasatospora sp. HKI 714  

Science Journals Connector (OSTI)

Genomics-Guided Discovery of Endophenazines from Kitasatospora sp. ... In this study we report on the genomics-guided exploration of the metabolic potential of the newly discovered strain Kitasatospora sp. ... Genomics-inspired discovery of natural products ...

Daniel Heine; Karin Martin; Christian Hertweck

2014-03-11T23:59:59.000Z

311

Biomarker Discovery and Validation for Proteomics and Genomics: Modeling And Systematic Analysis  

E-Print Network (OSTI)

Discovery and validation of protein biomarkers with high specificity is the main challenge of current proteomics studies. Different mass spectrometry models are used as shotgun tools for discovery of biomarkers which is usually done on a small...

Atashpazgargari, Esmaeil

2014-08-27T23:59:59.000Z

312

"Quantum Field Theory and QCD"  

SciTech Connect

This grant partially funded a meeting, "QFT & QCD: Past, Present and Future" held at Harvard University, Cambridge, MA on March 18-19, 2005. The participants ranged from senior scientists (including at least 9 Nobel Prize winners, and 1 Fields medalist) to graduate students and undergraduates. There were several hundred persons in attendance at each lecture. The lectures ranged from superlative reviews of past progress, lists of important, unsolved questions, to provocative hypotheses for future discovery. The project generated a great deal of interest on the internet, raising awareness and interest in the open questions of theoretical physics.

Jaffe, Arthur M.

2006-02-25T23:59:59.000Z

313

Security Sciences Field Lab (SSFL) | ORNL  

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

Nuclear Science Nuclear Science Research Areas Research Highlights Facilities and Capabilities Educational Outreach Publications and Reports News and Awards Nuclear Science Home | Science & Discovery | Nuclear Science | Facilities and Capabilities SHARE Security Sciences Field Laboratory May 30, 2013 The Security Sciences Field Laboratory (SSFL) is designed to support testing and evaluation of a wide range of intrusion detection, assessment, surveillance, and peripheral physical security equipment including: sensors; cameras; alarm communication and display; power generation; access control; unattended stand-alone, remote communication; unmanned aerial and activated delay systems. At the heart of SSFL is a simulated border region of varied terrain such as open grassy fields, hilly wooded areas, sand

314

A Web of Possibilities: Network-Based Discovery of Protein Interaction Codes  

Science Journals Connector (OSTI)

A Web of Possibilities: Network-Based Discovery of Protein Interaction Codes ... Publication Date (Web): October 22, 2014 ...

Daniel L. Winter; Melissa A. Erce; Marc R. Wilkins

2014-10-22T23:59:59.000Z

315

The discovery of plutonium reorganized the periodic table and aided the discovery of new elements  

SciTech Connect

The modern Periodic Table derives principally from the work of the great Russian scientist Dimitri Mendeleev, who in 1869 enunciated a 'periodic law' that the properties of the elements are a periodic function of their atomic weights, and arranged the 65 known elements in a 'periodic table'. Fundamentally, every column in the main body of the Periodic Table is a grouping of elements that display similar chemical and physical behavior. Similar properties are therefore exhibited by elements with widely different mass. Chemical periodicity is central to the study of chemistry, and no other generalization comes close to its ability to systematize and rationalize known chemical facts. With the development of atomic theory, and an understanding of the electronic structure of atoms, chemical periodicity and the periodic table now find their natural explanation in the electronic structure of atoms. Moving from left to right along any row, the elements are arranged sequentially according to nuclear charge (the atomic number). Electrons counter balance that nuclear charge, hence each successive element has one more electron in its configuration. The electron configuration, or distribution of electrons among atomic orbitals, may be determined by application of the Pauli principle (paired spin in the same orbital) and the aufbau principle (which outlines the order of filling of electrons into shells of orbitals - s, p, d, f, etc.) such that in a given atom, no two electrons may have all four quantum numbers identical. In 1939, only three elements were known to be heavier than actinium: thorium, protactinium, and uranium. All three exhibited variable oxidation states and a complex chemistry. Thorium, protactinium and uranium were assumed to be d-transition metals and were placed in the Periodic Table under hafnium, tantalum, and tungsten, respectively. By 1940, McMillan and Abelson bombarded uranium atoms with slow neutrons and successfully identified atoms of element 93, which they named neptunium after the planet Neptune. This rapidly set the stage for the discovery of the next succeeding element, plutonium (Seaborg, McMillan, Kennedy, and Wahl, 1940), named after the next planet away from the Sun, Pluto. The newly discovered elements were presumed to fit comfortably in the Periodic Table under rhenium and osmium, respectively. However, subsequent tracer chemical experiments showed that neptunium and plutonium were closer in their chemical properties to uranium than their presumed homologues, rhenium and osmium. Spectroscopic evidence also indicated that the new elements were not typical transition elements, but had f-electrons in their valence shell. Thus, several researchers, including McMillan and Wahl, and Zachariasen at Los Alamos, suggested that these elements might be part of a second inner-transition series in which the 5f-electron subshell was being filled. It was not clear, however, where the new series would begin. McMillian had proposed a 'uraninide series' that started with neptunium, but attempts to isolate elements with atomic numbers 95 and 96 based on assumed similarities to uranium were unsuccessful. Both Wahl and Zacharias en had proposed a thoride series that started with protactinium. In 1944, Seaborg proposed that the series started with thorium, and that all of the elements heavier than actinium constituted an 'actinide' series similar to the lanthanides. Because the 5f-shell began filling in the same relative position as the 4f-shell, the electronic configuration of elements in the two series would be similar. Guided by the hypothesis that elements 95 and 96 were homologues of europium and gadolinium, new experiments were designed and the elements were uniquely synthesized and separated from all others. The new elements were subsequently named americium and curium. Seaborg's 'Actinide Concept' thus played a major role in the discovery of the transplutonium elements. It provided the framework that supported synthesis, isolation, and identification of the succeeding actinide elements berkelium through lawrenci

Clark, David L [Los Alamos National Laboratory

2009-01-01T23:59:59.000Z

316

Beyond the standard Higgs after the 125 GeV Higgs discovery  

Science Journals Connector (OSTI)

...behind and beyond the discovery of the Higgs boson...after the 125 GeV Higgs discovery C. Grojean e-mail...behind and beyond the discovery of the Higgs boson...Model up to very high energy, maybe as high as the...fill the universe with dark matter and does not...

2015-01-01T23:59:59.000Z

317

College of Engineering Discovery with Purpose www.engineering.iastate.edu  

E-Print Network (OSTI)

Discovery with Purpose www.engineering.iastate.edu Chemistry Placement Options · Chem 177: General ChemistryCollege of Engineering Discovery with Purpose www.engineering.iastate.edu Welcome to the College of Engineering! College of Engineering #12;College of Engineering Discovery with Purpose www.engineering

Lin, Zhiqun

318

Seymour Marine Discovery Center at Long Marine Lab 100 Shaffer Road * Santa Cruz, CA 95060  

E-Print Network (OSTI)

Seymour Marine Discovery Center at Long Marine Lab 100 Shaffer Road * Santa Cruz, CA 95060 (831) 459-3800 2014 Endowment Challenge to benefit Seymour Marine Discovery Center SANTA CRUZ, CA Discovery Center at Long Marine Lab 100 Shaffer Road * Santa Cruz, CA 95060 (831) 459-3800 Open

California at Santa Cruz, University of

319

Gateway Discovery Algorithm for Ad-Hoc Networks Using HELLO Messages Matthias Rosenschon a  

E-Print Network (OSTI)

Gateway Discovery Algorithm for Ad-Hoc Networks Using HELLO Messages Matthias Rosenschon studied in the literature up to now. This paper describes an approach for gateway discovery based on HELLO-hoc networks, MANET, gateway discovery, AODV, HELLO packets 1. INTRODUCTION Multihop wireless access networks

Rakocevic, Veselin

320

Discovery of two candidate pulsar wind nebulae in very-high-energy gamma rays  

E-Print Network (OSTI)

We present the discovery of two very-high-energy gamma-ray sources in an ongoing systematic search for emission above 100 GeV from pulsar wind nebulae in survey data from the H.E.S.S. telescope array. Imaging Atmospheric Cherenkov Telescopes are ideal tools for searching for extended emission from pulsar wind nebulae in the very-high-energy regime. H.E.S.S., with its large field of view of 5 degrees and high sensitivity, gives new prospects for the search for these objects. An ongoing systematic search for very-high-energy emission from energetic pulsars over the region of the Galactic plane between -60 degrees wind nebulae, HESS J1718-385 and HESS J1809-193. H.E.S.S. has proven to be a suitable instrument for pulsar wind nebula searches.

H. E. S. S. Collaboration; :; F. Aharonian

2007-05-11T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Abandoned oil fields in Alabama, Florida, Illinois, Indiana, Kentucky, Michigan, Missouri, New York, Tennessee and West Virginia  

SciTech Connect

Data are presented for approximately 240 abandoned oil fields in Alabama, Florida, Illinois, Indiana, Kentucky, Michigan, Missouri, New York, Tennessee, and West Virginia. Production data were not available on a majority of abandoned fields in New York, Missouri, and Kentucky. Consequently, some fields with less than 10,000 barrels cumulative production are included. The following information is presented for each field: county; DOE field code; field name; AAPG geologic province code; discovery date of field; year of last production; discovery well operator; proven acreage; formation thickness; depth of field; gravity of oil production; calendar year; yearly field oil production; yearly field gas production; cumulative oil production; cumulative gas production; number abandoned fields in county; cumulative production of oil from fields; cumulative production of gas from fields. (ATT)

Not Available

1983-04-01T23:59:59.000Z

322

Introduction Estimation paramtrique (exemples)  

E-Print Network (OSTI)

Introduction Estimation paramétrique (exemples) FARMAN : Laboratoire SATIE Jean-Pierre Barbot J.P. Barbot Séminaires FARMAN (Traitement du Signal) - 1/36 #12;Introduction Estimation paramétrique (exemples de paramètres de synchronisation (VDSL 2) J.P. Barbot Séminaires FARMAN (Traitement du Signal) - 2

323

Internal Dose Estimates from  

E-Print Network (OSTI)

Appendix H Internal Dose Estimates from Global Fallout H-1 #12;Radiation Dose to the Population. 263-MQ-008090 September 30, 2000 H-2 #12;Radiation Dose to the Population of the Continental United Site Part I. Estimates of Dose Lynn R. Anspaugh Lynn R. Anspaugh, Consulting Salt Lake City, UT Report

324

Estimating Specialty Costs  

Directives, Delegations, and Requirements

Specialty costs are those nonstandard, unusual costs that are not typically estimated. Costs for research and development (R&D) projects involving new technologies, costs associated with future regulations, and specialty equipment costs are examples of specialty costs. This chapter discusses those factors that are significant contributors to project specialty costs and methods of estimating costs for specialty projects.

1997-03-28T23:59:59.000Z

325

DISCOVERY OF THREE DISTANT, COLD BROWN DWARFS IN THE WFC3 INFRARED SPECTROSCOPIC PARALLELS SURVEY  

SciTech Connect

We present the discovery of three late-type ({>=}T4.5) brown dwarfs, including a probable Y dwarf, in the WFC3 Infrared Spectroscopic Parallels (WISP) survey. We use the G141 grism spectra to determine the spectral types of the dwarfs and derive distance estimates based on a comparison with nearby T dwarfs with known parallaxes. These are the most distant spectroscopically confirmed T/Y dwarfs, with the farthest at an estimated distance of {approx}400 pc. We compare the number of cold dwarfs found in the WISP survey with simulations of the brown dwarf mass function. The number found is generally consistent with an initial stellar mass function dN/dM{proportional_to}M{sup -{alpha}} with {alpha} = 0.0-0.5, although the identification of a Y dwarf is somewhat surprising and may be indicative of either a flatter absolute magnitude/spectral-type relation than previously reported or an upturn in the number of very-late-type brown dwarfs in the observed volume.

Masters, D.; Siana, B. [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); McCarthy, P.; Hathi, N. P.; Dressler, A. [Observatories of the Carnegie Institution of Washington, Pasadena, CA 91101 (United States); Burgasser, A. J. [Center for Astrophysics and Space Science, University of California, San Diego, La Jolla, CA 92093 (United States); Malkan, M.; Ross, N. R. [Department of Physics and Astronomy, UCLA, Los Angeles, CA 90095 (United States); Scarlata, C. [Astronomy Department, University of Minnesota, Minneapolis, MN 55455 (United States); Henry, A. [Department of Physics, University of California, Santa Barbara, CA 93106 (United States); Colbert, J.; Atek, H. [Spitzer Science Center, Caltech, Pasadena, CA 91125 (United States); Rafelski, M.; Teplitz, H. [Infrared Processing and Analysis Center, Caltech, Pasadena, CA 91125 (United States); Bunker, A. [Department of Physics, University of Oxford, Oxford (United Kingdom)

2012-06-10T23:59:59.000Z

326

Discovery Bay, California: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Discovery Bay, California: Energy Resources Discovery Bay, California: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 37.9085357°, -121.6002291° 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":37.9085357,"lon":-121.6002291,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

327

DOE Announces $60 Million in Projects to Accelerate Scientific Discovery  

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

0 Million in Projects to Accelerate Scientific 0 Million in Projects to Accelerate Scientific Discovery through Advanced Computing DOE Announces $60 Million in Projects to Accelerate Scientific Discovery through Advanced Computing September 7, 2006 - 8:53am Addthis WASHINGTON, D.C. - The U.S. Department of Energy's (DOE) Office of Science today announced approximately $60 million in new awards annually for 30 computational science projects over the next three to five years. The projects are aimed at accelerating research in designing new materials, developing future energy sources, studying global climate change, improving environmental cleanup methods and understanding physics from the tiniest particles to the massive explosions of supernovae. "Advanced computing is a critical element of President Bush's American

328

Visualizing the Future of Scientific Discovery - NERSC Science News June  

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

Visualizing the Visualizing the Future of Scientific Discovery Visualizing the Future of Scientific Discovery June 11, 2009 snVolRender-3.png A SUPERNOVA'S VOLUME: This volume rendering of supernova simulation data was generated by running the VisIt application on 32,000 processors on Franklin, a Cray XT4 supercomputer at NERSC. As computational scientists are confronted with increasingly massive datasets from supercomputing simulations and experiments, one of the biggest challenges is having the right tools to gain scientific insight from the data. A team of Department of Energy (DOE) researchers recently ran a series of experiments to determine whether VisIt, a leading scientific visualization application, is up to the challenge. Running on some of the world's most powerful supercomputers, VisIt achieved unprecedented levels of performance

329

Argonne licenses diamond semiconductor discoveries to AKHAN Technologies |  

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

licenses diamond semiconductor discoveries to AKHAN Technologies licenses diamond semiconductor discoveries to AKHAN Technologies By Joseph Bernstein * By Jared Sagoff * March 4, 2013 Tweet EmailPrint LEMONT, Ill. - The U.S. Department of Energy's Argonne National Laboratory announced today that the laboratory has granted AKHAN Technologies exclusive diamond semiconductor application licensing rights to breakthrough low-temperature diamond deposition technology developed by Argonne's Center for Nanoscale Materials (CNM). The Argonne-developed technology allows for the deposition of nanocrystalline diamond on a variety of wafer substrate materials at temperatures as low as 400 degrees Celsius. The combination of the Argonne's low-temperature diamond technology with AKHAN's Miraj Diamond(tm) process represents the state of the art in diamond semiconductor

330

View Discovery in OLAP Databases through Statistical Combinatorial Optimization  

SciTech Connect

The capability of OLAP database software systems to handle data complexity comes at a high price for analysts, presenting them a combinatorially vast space of views of a relational database. We respond to the need to deploy technologies sufficient to allow users to guide themselves to areas of local structure by casting the space of ``views'' of an OLAP database as a combinatorial object of all projections and subsets, and ``view discovery'' as an search process over that lattice. We equip the view lattice with statistical information theoretical measures sufficient to support a combinatorial optimization process. We outline ``hop-chaining'' as a particular view discovery algorithm over this object, wherein users are guided across a permutation of the dimensions by searching for successive two-dimensional views, pushing seen dimensions into an increasingly large background filter in a ``spiraling'' search process. We illustrate this work in the context of data cubes recording summary statistics for radiation portal monitors at US ports.

Joslyn, Cliff A.; Burke, Edward J.; Critchlow, Terence J.

2009-05-01T23:59:59.000Z

331

The LHC Higgs Boson Discovery: Implications for Finite Unified Theories  

E-Print Network (OSTI)

Finite Unified Theories (FUTs) are N = 1 supersymmetric Grand Unified Theories (GUTs) which can be made finite to all-loop orders, based on the principle of reduction of couplings, and therefore are provided with a large predictive power. We confront the predictions of an SU(5) FUT with the top and bottom quark masses and other low-energy experimental constraints, resulting in a relatively heavy SUSY spectrum, naturally consistent with the non-observation of those particles at the LHC. The light Higgs boson mass is automatically predicted in the range compatible with the Higgs discovery at the LHC. Requiring a light Higgs-boson mass in the precise range of M_h = 125.6 +- 2.1 GeV favors the lower part of the allowed spectrum, resulting in clear predictions for the discovery potential at current and future pp, as well as future e+e- colliders.

Heinemeyer, S; Zoupanos, G

2014-01-01T23:59:59.000Z

332

The discovery and measurements of a Higgs boson  

Science Journals Connector (OSTI)

The discovery of a Higgs-like boson with a mass of approximately 125GeV by the ATLAS and CMS experiments at the Large Hadron Collider was announced at CERN on 4 July 2012. The data-set of 5fb?1 of protonproton collisions with collected during 2011 and 6fb?1 with collected in 2012 up to the July discovery was supplemented by an additional 15fb?1 of data with collected during the rest of 2012. The measurements of the properties of the new boson with the combined data-set have substantially strengthened the evidence that this new particle is indeed the Higgs boson predicted to exist as a consequence of the BroutEnglertHiggs-mechanism that takes responsibility for generating masses of fundamental particles and for the electroweak symmetry breaking.

A L Read

2013-01-01T23:59:59.000Z

333

Discovery-Spring Garden, Maryland: Energy Resources | Open Energy  

Open Energy Info (EERE)

Discovery-Spring Garden, Maryland: Energy Resources Discovery-Spring Garden, Maryland: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 39.4614398°, -77.358284° 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":39.4614398,"lon":-77.358284,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

334

The LHC Higgs Boson Discovery: Implications for Finite Unified Theories  

E-Print Network (OSTI)

Finite Unified Theories (FUTs) are N = 1 supersymmetric Grand Unified Theories (GUTs) which can be made finite to all-loop orders, based on the principle of reduction of couplings, and therefore are provided with a large predictive power. We confront the predictions of an SU(5) FUT with the top and bottom quark masses and other low-energy experimental constraints, resulting in a relatively heavy SUSY spectrum, naturally consistent with the non-observation of those particles at the LHC. The light Higgs boson mass is automatically predicted in the range compatible with the Higgs discovery at the LHC. Requiring a light Higgs-boson mass in the precise range of M_h = 125.6 +- 2.1 GeV favors the lower part of the allowed spectrum, resulting in clear predictions for the discovery potential at current and future pp, as well as future e+e- colliders.

S. Heinemeyer; M. Mondragon; G. Zoupanos

2014-12-18T23:59:59.000Z

335

Manhattan Project: The Discovery of Fission, 1938-1939  

Office of Scientific and Technical Information (OSTI)

Lise Meitner and Otto Hahn, Kaiser-Wilhelm Institute, Berlin THE DISCOVERY OF FISSION Berlin, Germany (1938-1939) Events > Atomic Discoveries, 1890s-1939 A Miniature Solar System, 1890s-1919 Exploring the Atom, 1919-1932 Atomic Bombardment, 1932-1938 The Discovery of Fission, 1938-1939 Fission Comes to America, 1939 The English word "atom" derives from the Greek word "atomon" ("ατομον"), which means "that which cannot be divided." In 1938, the scientific community proved the Greek philosophers wrong by dividing the atom. Excerpt from the comic book "Adventures Inside the Atom." Click on this image or visit the "Library" to view the whole comic book. Fission, the basis of the atomic bomb, was discovered in Nazi Germany less than a year before the beginning of the Second World War. It was December 1938 when the radiochemists Otto Hahn (above, with Lise Meitner) and Fritz Strassmann, while bombarding elements with neutrons in their Berlin laboratory, made their unexpected discovery. They found that while the nuclei of most elements changed somewhat during neutron bombardment, uranium nuclei changed greatly and broke into two roughly equal pieces. They split and became not the new transuranic elements that some thought Enrico Fermi had discovered but radioactive barium isotopes (barium has the atomic number 56) and other fragments of the uranium itself. The substances Fermi had created in his experiments, that is, did more than resemble lighter elements -- they were lighter elements. The products of the Hahn-Strassmann experiment weighed less than that of the original uranium nucleus, and herein lay the primary significance of their findings. It folIowed from Albert Einstein's E=mc2 equation that the loss of mass resulting from the splitting process must have been converted into energy in the form of kinetic energy that could in turn be converted into heat.

336

Exploration and Empire: Iconographic Evidence of Iberian Ships of Discovery  

E-Print Network (OSTI)

.09????????????????????????. Figure 6 MA01; the caravel (MA01.02) is shown on the right.??????.?. Figure 7 One-masted caravel under sail (1C-2)?????????????? Figure 8 Two-masted caravels under sail (2C-6) and at anchor (2C-4)..???? Figure 9 Two-masted caravels under sail (2C...?????????????????????????? ix LIST OF TABLES??????????????????????????.. CHAPTER I INTRODUCTION?????????????????????. 1.1 Research Objectives and Parameters.??????????. II HISTORICAL CONTEXT OF IBERIAN CARTOGRAPHY AND SEAFARING IN THE AGE OF DISCOVERY...

Bojakowski, Katie

2011-08-08T23:59:59.000Z

337

Information discovery applied to a power generation database  

SciTech Connect

An information discovery system is presented that extracts knowledge from databases in a form that is much more compact and easy to understand than the original set of records. The system was tested with a subset of a real power generation database of the Federal Commission of Electricity in Mexico (CFE = Comision Federal de Electricidad). The paper discusses a machine learning algorithm for induction of rules and the heuristics used to obtain the simplest rules that define the knowledge hidden in a database.

Rodriguez, G.; Hernandez, V. [Electrical Research Inst., Cuernavaca (Mexico). Information Systems Dept.

1996-11-01T23:59:59.000Z

338

Materials Design and Discovery: Catalysis and Electrical Energy Storage  

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

and Discovery: Catalysis and Discovery: Catalysis and Electrical Energy Storage Presenter: N ichols A . R omero, A LCF ESP p ost---doc: Anouar B enali, A LCF PI: L arry C urAss, A NL M SD a nd C NM Comments from a reviewer on "Material Design and Discovery" from a proposal § How c ould t his m achine w ith t hese p rograms b e u sed t o d esign a n ew s olar c ell? Or a n ew c ure f or A IDS? O r a n ew h igh---T s uperconductor? T his i s n ot i ntended a s a trivial q uesAon. T he p resent m ethod o f D ISCOVERY r elies o n t he t rained h uman mind ( insight) a nd e xperiment ( serendipity). C omputaAonal s cience s o f ar h as n ot delivered a ny n ew d iscoveries b ecause i t l acks t he p ossibility o f s erendipity. T he greatest s uccess o f c omputaAonal c hemistry h as b een i mproved i nsight i nto t he way m aterial b ehaves

339

View discovery in OLAP databases through statistical combinatorial optimization  

SciTech Connect

OnLine Analytical Processing (OLAP) is a relational database technology providing users with rapid access to summary, aggregated views of a single large database, and is widely recognized for knowledge representation and discovery in high-dimensional relational databases. OLAP technologies provide intuitive and graphical access to the massively complex set of possible summary views available in large relational (SQL) structured data repositories. The capability of OLAP database software systems to handle data complexity comes at a high price for analysts, presenting them a combinatorially vast space of views of a relational database. We respond to the need to deploy technologies sufficient to allow users to guide themselves to areas of local structure by casting the space of 'views' of an OLAP database as a combinatorial object of all projections and subsets, and 'view discovery' as an search process over that lattice. We equip the view lattice with statistical information theoretical measures sufficient to support a combinatorial optimization process. We outline 'hop-chaining' as a particular view discovery algorithm over this object, wherein users are guided across a permutation of the dimensions by searching for successive two-dimensional views, pushing seen dimensions into an increasingly large background filter in a 'spiraling' search process. We illustrate this work in the context of data cubes recording summary statistics for radiation portal monitors at US ports.

Hengartner, Nick W [Los Alamos National Laboratory; Burke, John [PNNL; Critchlow, Terence [PNNL; Joslyn, Cliff [PNNL; Hogan, Emilie [PNNL

2009-01-01T23:59:59.000Z

340

Stories of Discovery & Innovation | U.S. DOE Office of Science (SC)  

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

Stories of Discovery & Stories of Discovery & Innovation Discovery & Innovation Stories of Discovery & Innovation Brief Science Highlights SBIR/STTR Highlights Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Stories of Discovery & Innovation Print Text Size: A A A Subscribe FeedbackShare Page The photosynthetic megacomplex from a cyanobacterium. 12.30.13Stories of Discovery & Innovation Observing the Sparks of Life EFRC researchers isolate a photosynthetic complex - arguably the most important bit of organic chemistry on the planet - in its complete functioning state. Read More » Scanning electron microscope image of sulfur graphene oxide. 11.27.13Stories of Discovery & Innovation

Note: This page contains sample records for the topic "field discoveries estimated" 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

North Dakota`s Dickinson Lodgepole discovery: A Preliminary exploration model  

SciTech Connect

Interest in the Mississippian Lodgepole formation of North Dakota has intensified since the successful completion of the Duncan Oil Inc. 1-11 Knopik flowing 2,707 b/d of oil and 1.55 MMcfd of gas 430 cu m of oil and 43,891 cu m of gas. The play began when Conoco drilled an in-field wildcat in an attempt to establish deeper production in Dickinson oil field. The discovery well, 74 Dickinson State, was completed in a clean lower Lodgepole limestone section that is thought to represent a Waulsortian mound. The most important questions asked concerning the Lodgepole play are whether or not it will step out of the Dickinson area, what are the factors that control the development of these mounds, what controlled the development of the reservoir and trap, and how it was charged with oil. Other than the reservoir section, the most significant feature observed from wireline logs of the area is the anomalously thick Bakken formation (Mississippian-Devonian). This observation is important to understanding the Lodgepole play and can be used to help explore for similar features elsewhere in the basin. The paper describes the regional setting, the Lodgepole stratigraphy, deposition, regional equivalents, and a salt collapse model that can readily explain the features observed at the Dickinson field.

LeFever, J.A. [North Dakota Geological Survey, Grand Forks, ND (United States); Halabura, S.P. [North Rim Exploration Ltd., Saskatoon, Saskatchewan (Canada); Martiniuk, C.D. [Manitoba Energy and Mines, Winnipeg, Manitoba (Canada); Fischer, D.W.

1995-08-14T23:59:59.000Z

342

Discovery of the pre-main sequence progenitors of the magnetic Ap/Bp stars?  

E-Print Network (OSTI)

We report the discovery, using FORS1 at the ESO-VLT and ESPaDOnS at the CFHT, of magnetic fields in the young A-type stars HD 101412, V380 Ori and HD 72106A. Two of these stars (HD 101412 and V380 Ori) are pre-main sequence Herbig Ae/Be (HAeBe) stars, while one (HD 72106A) is physically associated with a HAeBe star. Remarkably, evidence of surface abundance spots is detected in the spectra of HD 72106A. The magnetic fields of these objects display intensities of order 1 kG at the photospheric level, are ordered on global scales, and appear in approximately 10% of the stars studied. Based on these properties, the detected stars may well represent pre-main sequence progenitors of the magnetic Ap/Bp stars. The low masses inferred for these objects (2.6, 2.8 and 2.4 solar masses) represent additional contradictions to the hypothesis of Hubrig et al. (2000), who claim that magnetic fields appear in intermediate-mass stars only after 30% of their main sequence evolution is complete. Finally, we fail to confirm clai...

Wade, G A; Bagnulo, S; Landstreet, J D; Mason, E; Silvester, J; Alecian, E; Bhm, T; Bouret, J C; Catala, C; Donati, J F

2005-01-01T23:59:59.000Z

343

Associated-Dissolved Natural Gas New Reservoir Discoveries in Old Fields,  

Gasoline and Diesel Fuel Update (EIA)

65 73 820 169 186 160 1979-2011 65 73 820 169 186 160 1979-2011 Federal Offshore U.S. 32 54 297 122 150 42 1990-2011 Pacific (California) 1 0 0 0 0 0 1979-2011 Louisiana & Alabama 24 47 222 81 138 42 1981-2011 Texas 7 7 75 41 12 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 65 73 820 169 186 160 1979-2011 Alabama 0 0 0 0 0 0 1979-2011 Arkansas 0 0 0 0 0 0 1979-2011 California 0 0 9 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 9 0 0 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 0 0 0 0 0 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 1 0 0 0 1979-2011 Kentucky 0 0 0 0 0 0 1979-2011

344

New Reservoir Discoveries in Old Fields of Natural Gas, Wet After Lease  

Gasoline and Diesel Fuel Update (EIA)

1,197 1,244 1,678 2,656 1,701 1,260 1979-2011 1,197 1,244 1,678 2,656 1,701 1,260 1979-2011 Federal Offshore U.S. 420 379 545 308 245 80 1990-2011 Pacific (California) 1 0 0 0 0 0 1979-2011 Louisiana & Alabama 353 341 391 231 221 80 1981-2011 Texas 66 38 154 77 24 0 1981-2011 Alaska 2 0 5 0 0 3 1979-2011 Lower 48 States 1,195 1,244 1,673 2,656 1,701 1,257 1979-2011 Alabama 7 17 1 0 0 0 1979-2011 Arkansas 33 27 41 36 27 23 1979-2011 California 4 1 16 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 1 1 16 0 0 0 1979-2011 State Offshore 3 0 0 0 0 0 1979-2011 Colorado 27 24 17 0 29 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 3 0 3 0 1 1 1979-2011

345

Associated-Dissolved Natural Gas New Reservoir Discoveries in Old Fields,  

Gasoline and Diesel Fuel Update (EIA)

65 73 820 169 186 160 1979-2011 65 73 820 169 186 160 1979-2011 Federal Offshore U.S. 32 54 297 122 150 42 1990-2011 Pacific (California) 1 0 0 0 0 0 1979-2011 Louisiana & Alabama 24 47 222 81 138 42 1981-2011 Texas 7 7 75 41 12 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 65 73 820 169 186 160 1979-2011 Alabama 0 0 0 0 0 0 1979-2011 Arkansas 0 0 0 0 0 0 1979-2011 California 0 0 9 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 9 0 0 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 0 0 0 0 0 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 1 0 0 0 1979-2011 Kentucky 0 0 0 0 0 0 1979-2011

346

Associated-Dissolved Natural Gas New Field Discoveries, Wet After Lease  

Gasoline and Diesel Fuel Update (EIA)

40 46 107 263 102 611 1979-2011 40 46 107 263 102 611 1979-2011 Federal Offshore U.S. 27 43 93 214 6 524 1990-2011 Pacific (California) 0 0 0 0 0 0 1979-2011 Louisiana & Alabama 27 4 93 25 6 524 1981-2011 Texas 0 39 0 189 0 0 1981-2011 Alaska 0 0 0 0 0 0 1979-2011 Lower 48 States 40 46 107 263 102 611 1979-2011 Alabama 0 0 0 0 2 2 1979-2011 Arkansas 0 0 0 0 0 0 1979-2011 California 0 0 0 0 0 0 1979-2011 Coastal Region Onshore 0 0 0 0 0 0 1979-2011 Los Angeles Basin Onshore 0 0 0 0 0 0 1979-2011 San Joaquin Basin Onshore 0 0 0 0 0 0 1979-2011 State Offshore 0 0 0 0 0 0 1979-2011 Colorado 0 0 0 0 0 0 1979-2011 Florida 0 0 0 0 0 0 1979-2011 Kansas 0 0 4 0 1 0 1979-2011 Kentucky 0 0 0 0 0 0 1979-2011

347

Discovery of a strong magnetic field in the rapidly rotating B2 Vn star HR 7355  

Science Journals Connector (OSTI)

......domain. The primary benefit, however, is to reduce...telescope operated by the SMARTS 1 consortium with a 2048...used a comprehensive grid of metal line blanketed...comparison of several grid models to the observed...astro.yale.edu/smarts/ ). 2 http://nova......

M. E. Oksala; G. A. Wade; W. L. F. Marcolino; J. Grunhut; D. Bohlender; N. Manset; R. H. D. Townsend

2010-06-01T23:59:59.000Z

348

Discovery of two new Galactic candidate luminous blue variables with Wide-field Infrared Survey Explorer  

Science Journals Connector (OSTI)

......simbad/ 4 http://webviz.u-strasbg.fr/viz-bin/VizieR 5 http://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd 6 http://www.lsw.uni-heidelberg.de/users/ostahl/pcyg/ 7 We measured the EWs of DIBs in both spectra......

V. V. Gvaramadze; A. Y. Kniazev; A. S. Miroshnichenko; L. N. Berdnikov; N. Langer; G. S. Stringfellow; H. Todt; W.-R. Hamann; E. K. Grebel; D. Buckley; L. Crause; S. Crawford; A. Gulbis; C. Hettlage; E. Hooper; T.-O. Husser; P. Kotze; N. Loaring; K. H. Nordsieck; D. O?Donoghue; T. Pickering; S. Potter; E. Romero Colmenero; P. Vaisanen; T. Williams; M. Wolf; D. E. Reichart; K. M. Ivarsen; J. B. Haislip; M. C. Nysewander; A. P. LaCluyze

2012-04-21T23:59:59.000Z

349

Biofilms 2012: New Discoveries and Significant Wrinkles in a Dynamic Field  

Science Journals Connector (OSTI)

...on activated carbon particles for the remediation of polychlorinated biphenyls (PCBs...contamination may emerge as a useful water remediation approach. EMERGING TECHNOLOGIES IN...cutting-edge technologies, and innovative thinking. Published ahead of print...

Susanne Haussler; Clay Fuqua

2013-04-26T23:59:59.000Z

350

State Emissions Estimates  

Gasoline and Diesel Fuel Update (EIA)

Estimates of state energy-related carbon dioxide emissions Estimates of state energy-related carbon dioxide emissions Because energy-related carbon dioxide (CO 2 ) constitutes over 80 percent of total emissions, the state energy-related CO 2 emission levels provide a good indicator of the relative contribution of individual states to total greenhouse gas emissions. The U.S. Energy Information Administration (EIA) emissions estimates at the state level for energy-related CO 2 are based on data contained in the State Energy Data System (SEDS). 1 The state-level emissions estimates are based on energy consumption data for the following fuel categories: three categories of coal (residential/commercial, industrial, and electric power sector); natural gas; and ten petroleum products including-- asphalt and road oil, aviation gasoline, distillate fuel, jet fuel, kerosene, liquefied petroleum gases

351

Cost Estimating Guide  

Directives, Delegations, and Requirements

This Guide provides uniform guidance and best practices that describe the methods and procedures that could be used in all programs and projects at DOE for preparing cost estimates. No cancellations.

2011-05-09T23:59:59.000Z

352

: Helmholtz machine estimation .  

E-Print Network (OSTI)

: Helmholtz machine density estimation . . : . . . (supervised learning) , (active learning) (query learning) [1, 3]. . (unsupervised learning), . , [5]. . Helmholtz machine , . Helmholtz machine : Helmholtz machine [2] . Helmholtz machine (generative network) (recognition network) . , , . Helmholtz machine (self

353

On theoretical pricing of options with fuzzy estimators  

Science Journals Connector (OSTI)

In this paper we present an application of a new method of constructing fuzzy estimators for the parameters of a given probability distribution function, using statistical data. This application belongs to the financial field and especially to the section ... Keywords: Adaptive fuzzy numbers, Black-Scholes option pricing formula, Fuzzy estimators, Fuzzy volatility, Possibilistic mean

Konstantinos A. Chrysafis; Basil K. Papadopoulos

2009-01-01T23:59:59.000Z

354

Statistics and Discoveries at the LHC (2/4)  

ScienceCinema (OSTI)

The lectures will give an introduction to statistics as applied in particle physics and will provide all the necessary basics for data analysis at the LHC. Special emphasis will be placed on the the problems and questions that arise when searching for new phenomena, including p-values, discovery significance, limit setting procedures, treatment of small signals in the presence of large backgrounds. Specific issues that will be addressed include the advantages and drawbacks of different statistical test procedures (cut-based, likelihood-ratio, etc.), the look-elsewhere effect and treatment of systematic uncertainties.

None

2011-10-06T23:59:59.000Z

355

Statistics and Discoveries at the LHC (1/4)  

ScienceCinema (OSTI)

The lectures will give an introduction to statistics as applied in particle physics and will provide all the necessary basics for data analysis at the LHC. Special emphasis will be placed on the the problems and questions that arise when searching for new phenomena, including p-values, discovery significance, limit setting procedures, treatment of small signals in the presence of large backgrounds. Specific issues that will be addressed include the advantages and drawbacks of different statistical test procedures (cut-based, likelihood-ratio, etc.), the look-elsewhere effect and treatment of systematic uncertainties.

None

2011-10-06T23:59:59.000Z

356

Statistics and Discoveries at the LHC (4/4)  

ScienceCinema (OSTI)

The lectures will give an introduction to statistics as applied in particle physics and will provide all the necessary basics for data analysis at the LHC. Special emphasis will be placed on the the problems and questions that arise when searching for new phenomena, including p-values, discovery significance, limit setting procedures, treatment of small signals in the presence of large backgrounds. Specific issues that will be addressed include the advantages and drawbacks of different statistical test procedures (cut-based, likelihood-ratio, etc.), the look-elsewhere effect and treatment of systematic uncertainties.

None

2011-10-06T23:59:59.000Z

357

Statistics and Discoveries at the LHC (3/4)  

ScienceCinema (OSTI)

The lectures will give an introduction to statistics as applied in particle physics and will provide all the necessary basics for data analysis at the LHC. Special emphasis will be placed on the the problems and questions that arise when searching for new phenomena, including p-values, discovery significance, limit setting procedures, treatment of small signals in the presence of large backgrounds. Specific issues that will be addressed include the advantages and drawbacks of different statistical test procedures (cut-based, likelihood-ratio, etc.), the look-elsewhere effect and treatment of systematic uncertainties.

None

2011-10-06T23:59:59.000Z

358

GRR/Section 11-MT-c - Cultural Resource Discovery | Open Energy Information  

Open Energy Info (EERE)

c - Cultural Resource Discovery c - Cultural Resource Discovery < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 11-MT-c - Cultural Resource Discovery 11MTCCulturalResourceDiscoveryProcess (1).pdf Click to View Fullscreen Contact Agencies Montana Department of Natural Resources & Conservation Montana State Historic Preservation Office Regulations & Policies 36 CFR 800.16: NHPA Definitions MCA 22-3-421: Montana Antiquities Definitions MCA 22-3-429: Consultation, Notice, Appeal MCA 22-3-430: Mitigation MCA 22-3-435: Report of Discovery ARM 36.2.801-813: Antiquities Triggers None specified Click "Edit With Form" above to add content 11MTCCulturalResourceDiscoveryProcess (1).pdf Error creating thumbnail: Page number not in range.

359

NERSC User Day February 13 - Trends, Discovery, and Innovation in HPC  

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

Day February 13 - Trends, Discovery, and Innovation in HPC Day February 13 - Trends, Discovery, and Innovation in HPC NERSC User Day February 13 - Trends, Discovery, and Innovation in HPC February 10, 2013 by Francesca Verdier (0 Comments) All members of the Berkeley Lab community, as well as those who have registered for the NERSC Users Group meeting, are welcome to join us for the NERSC User Day this February 13, 2013, in the Building 50 auditorium at Berkeley Lab. The theme of the User Day is Trends, Discovery, and Innovation in High Performance Computing: Trends 9:00 - The Future of High Performance Scientific Computing, Kathy Yelick, Berkeley Lab Associate Director of Computing Science 9:45 - NERSC Today and in the Next 10 Years, Sudip Dosanjh, NERSC Director Discovery 11:00 - Discovery of the Higgs Boson and the role of LBNL and World-Wide

360

GRR/Section 11-TX-c - Cultural Resource Discovery Process | Open Energy  

Open Energy Info (EERE)

-TX-c - Cultural Resource Discovery Process -TX-c - Cultural Resource Discovery Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 11-TX-c - Cultural Resource Discovery Process 11TXCCulturalResourceDiscoveryProcess.pdf Click to View Fullscreen Contact Agencies Texas Historical Commission Regulations & Policies Sec. 191: Antiquities Code Triggers None specified Click "Edit With Form" above to add content 11TXCCulturalResourceDiscoveryProcess.pdf 11TXCCulturalResourceDiscoveryProcess.pdf Error creating thumbnail: Page number not in range. Error creating thumbnail: Page number not in range. Flowchart Narrative 11-TX-c.1 - Is the Project Located on State or Local Public Land? Before breaking ground at a project location on state or local public land,

Note: This page contains sample records for the topic "field discoveries estimated" 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

Kids at Camp Discovery Bond Over Building Electric Vehicle | Department of  

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

Kids at Camp Discovery Bond Over Building Electric Vehicle Kids at Camp Discovery Bond Over Building Electric Vehicle Kids at Camp Discovery Bond Over Building Electric Vehicle August 13, 2010 - 11:30am Addthis Campers at Camp Discovery put the finishing touches on a newly assembled electric vehicle they built to learn more about EV technology while sharing their experiences with battling cancer. | Photo courtesy of Craig Egan Campers at Camp Discovery put the finishing touches on a newly assembled electric vehicle they built to learn more about EV technology while sharing their experiences with battling cancer. | Photo courtesy of Craig Egan Joshua DeLung Each year, about 150 kids gather during the summer at Camp Discovery in Kerrville, Texas, to learn new things and have fun. But this isn't an ordinary summer camp - the attendees, ages seven to 16, all have been

362

Kids at Camp Discovery Bond Over Building Electric Vehicle | Department of  

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

Kids at Camp Discovery Bond Over Building Electric Vehicle Kids at Camp Discovery Bond Over Building Electric Vehicle Kids at Camp Discovery Bond Over Building Electric Vehicle August 13, 2010 - 11:30am Addthis Campers at Camp Discovery put the finishing touches on a newly assembled electric vehicle they built to learn more about EV technology while sharing their experiences with battling cancer. | Photo courtesy of Craig Egan Campers at Camp Discovery put the finishing touches on a newly assembled electric vehicle they built to learn more about EV technology while sharing their experiences with battling cancer. | Photo courtesy of Craig Egan Joshua DeLung Each year, about 150 kids gather during the summer at Camp Discovery in Kerrville, Texas, to learn new things and have fun. But this isn't an ordinary summer camp - the attendees, ages seven to 16, all have been

363

Weekly Coal Production Estimation Methodology  

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

Weekly Coal Production Estimation Methodology Step 1 (Estimate total amount of weekly U.S. coal production) U.S. coal production for the current week is estimated using a ratio...

364

REQUESTS FOR RETIREMENT ESTIMATE  

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

REQUEST FOR RETIREMENT ANNUITY ESTIMATE REQUEST FOR RETIREMENT ANNUITY ESTIMATE Instructions: Please read and answer the following questions thoroughly to include checking all applicable boxes. Unanswered questions may delay processing. Print and Fax back your request form to 202.586.6395 or drop request to GM-169. The request will be assigned to your servicing retirement specialist. They will confirm receipt of your request. SECTION A Request Submitted _____________________ ______________________ ________________________ _____________________ Name (last, first, middle) Last four SSN Date of Birth ___________________________ _________________________ __________________________ Organization Office Telephone Number Fax Number

365

Natural Gas Discovery and Development Impacts on Rio Vista and Its Community  

E-Print Network (OSTI)

1958. Legal Battle Over Rio Gas Rights Opens: 20 AttorneysRio Vista discovers gas..40 Part 1: Creationfor new economic avenues: The gas discovery..58 1. The

Gbedema, Tometi Koku

2006-01-01T23:59:59.000Z

366

E-Print Network 3.0 - array-based gene discovery Sample Search...  

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

2001 Summary: 1Mark-A. Krogel, Magdeburg University, Knowledge Discovery and Machine Learning Group KDD Cup 2001... : GeneProtein Function Prediction Using the Multirelational...

367

Price Discovery in Time and Space: The Course of Condominium Prices in Singapore  

E-Print Network (OSTI)

Method for Real Estate Price Index Construction, Journal ofAutocorrelation in House Prices, Journal of Real Estate1997), Quotes, Order Flow, and Price Discovery, Journal of

Hwang, Min; Quigley, John M.

2007-01-01T23:59:59.000Z

368

Search Method for Real-time Knowledge Discovery Modeled on the...  

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

Return to Search Search Method for Real-time Knowledge Discovery Modeled on the Human Brain Oak Ridge National Laboratory Contact ORNL About This Technology Publications: PDF...

369

E-Print Network 3.0 - anticancer drug discovery Sample Search...  

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

2 From the University of Mississippi Medical Center Division of Public Affairs ANTI-CANCER DRUG DISCOVERY PARTNERSHIP FORMED BETWEEN UMMC CANCER INSTITUTE AND Summary: From the...

370

The Discovery of the Tau and Its Major Properties: 1970--1985  

DOE R&D Accomplishments (OSTI)

This paper recounts the history of the discovery of the tau lepton and its major properties: its mass, its lifetime and its main decay modes.

Perl, M. L.

1990-09-00T23:59:59.000Z

371

Domain-Specific Languages for Composing Signature Discovery Workflows  

SciTech Connect

Domain-agnostic signature discovery entails investigation across multiple scientific disciplines. The breadth and cross-disciplinary nature of this work requires that existing executables be integrated with new capabilities into workflows, representing a wide range of user tasks. An algorithm may be written in multiple programming languages for various hardware platforms, and so workflow composition requires integrating executables from any number of remote hosts. This raises an engineering issue on how to generate web service wrappers for these heterogeneous executables and to compose them into a scientific workflow environment (e.g., Taverna). In this paper, we introduce two simple Domain-Specific Languages (DSLs) to automate these processes. Our Service Description Language (SDL) describes key elements of a signature discovery service and automatically generates its implementation code. The Workflow Description Language (WDL) describes the pipeline of services and generates deployable artifacts for the Taverna workflow management system. We demonstrate our approach with a real-world workflow composed of services wrapping remote executables.

Jacob, Ferosh; Gray, Jeff; Wynne, Adam S.; Liu, Yan (Jenny) [Jenny; Baker, Nathan A.

2012-10-23T23:59:59.000Z

372

Power load forecasting using data mining and knowledge discovery technology  

Science Journals Connector (OSTI)

Considering the importance of the peak load to the dispatching and management of the electric system, the error of peak load is proposed in this paper as criteria to evaluate the effect of the forecasting model. This paper proposes a systemic framework that attempts to use data mining and knowledge discovery (DMKD) to pretreat the data. And a new model is proposed which combines artificial neural networks with data mining and knowledge discovery for electric load forecasting. With DMKD technology, the system not only could mine the historical daily loading which had the same meteorological category as the forecasting day to compose data sequence with highly similar meteorological features, but also could eliminate the redundant influential factors. Then an artificial neural network is constructed to predict according to its characteristics. Using this new model, it could eliminate the redundant information, accelerate the training speed of neural network and improve the stability of the convergence. Compared with single BP neural network, this new method can achieve greater forecasting accuracy.

Yongli Wang; Dongxiao Niu; Ling Ji

2011-01-01T23:59:59.000Z

373

Estimating SCR installation costs  

SciTech Connect

The EUCG surveyed 72 separate US installations of selective catalytic reduction (SCR) systems at coal-fired units totalling 41 GW of capacity to identify the systems' major cost drivers. The results, summarized in this article, provide excellent first-order estimates and guidance for utilities considering installing the downstream emissions-control technology. 4 figs., 1 tab.

Marano, M.; Sharp, G. [American Electric Power (United States)

2006-01-15T23:59:59.000Z

374

SPACE TECHNOLOGY Actual Estimate  

E-Print Network (OSTI)

SPACE TECHNOLOGY TECH-1 Actual Estimate Budget Authority (in $ millions) FY 2011 FY 2012 FY 2013 FY.7 247.0 Exploration Technology Development 144.6 189.9 202.0 215.5 215.7 214.5 216.5 Notional SPACE TECHNOLOGY OVERVIEW .............................. TECH- 2 SBIR AND STTR

375

MOTION FIELD ESTIMATION BY COMBINED VECTOR RATIONAL AND BILINEAR  

E-Print Network (OSTI)

- mation. Bilinear interpolation, operating on a ner in- terpolation grid, takes neighbouring spatial selects the optimal motion vector with respect to the mini- mal boundary matching error 1], the motion exploit spatial correlations. Furthermore, a ner interpolation grid has been de ned according to which one

Gabbouj, Moncef

376

FIELD VALIDATION OF THE CLEAN POWER ESTIMATOR'S OBSTRUCTION ANALYSIS ALGORITHM  

E-Print Network (OSTI)

to provide obstruction profiles when it is difficult to be at the solar collector location (e) obstruction analysis algorithm based on results produced by the Solar PathfinderTM (SPF). Results indicate tables for two configurations: horizontal and south-facing at 30o -tilt. These tables are used

Perez, Richard R.

377

Mobile sensor systems for field estimation and "hot spot" identification  

E-Print Network (OSTI)

Robust, low-cost mobile sensing enables effective monitoring and management of urban environment and infrastructure which contributes towards a sustainable future. While mobile sensor systems have attracted significant ...

Kumar, Sumeet, Ph. D. Massachusetts Institute of Technology

2014-01-01T23:59:59.000Z

378

Estimating Velocity Fields on a Freeway from Low Resolution Video  

E-Print Network (OSTI)

] detects and tracks vehicles within a detection zone (roughly a rect- angle the size of a vehicle) and integrates their spatial and temporal signatures to measure their speeds. The ACTIONS system [4], detects camera. The TITAN system [6] uses mathematical morphology to extract individual vehicle features

Rice, John

379

MULTI-VALUED MOTION FIELDS ESTIMATION FOR TRANSPARENT  

E-Print Network (OSTI)

is with the Computer Science Department, Centro de Investigacion en Matematicas A.C., Apdo. Postal 402, Guanajuato, Gto Department, Centro de Investigacion en Matematicas A.C., Apdo. Postal 402, Guanajuato, Gto., 36000, Mexico. . . . . . . . . . . . . . . . . . . 8 2 The diffusion coefficients wi. The diffusion process is performed in the spatio

Rivera, Mariano

380

Estimate of the stress field in Kilauea's south flank, Hawaii  

Science Journals Connector (OSTI)

......is combined with gravity and seawater pressure to give the total...2 of Table 4, gravity and seawater pressure. The shear stress...The effects of gravity and seawater pressure have been removed...1984. Magma supply and storage at Kilauea volcano, Hawaii......

Beiyuan Liang; Carl Kisslinger; Carol Bryan

1995-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Gin Flat Snow Water Equivalent Estimation from Field Methods  

E-Print Network (OSTI)

Change, Atmospheric Rivers, and Floods in Cali- fornia Amelt leading to the risk of floods becom- ing more frequent

Vida, Jordan; Sa, Nathaniel; Lem, Dylan

2014-01-01T23:59:59.000Z

382

QUANTIFICATION MODEL FOR ESTIMATING TEMPERATURE FIELD DISTRIBUTIONS OF  

E-Print Network (OSTI)

process. It was related to the metabolism heat of plant body at any time. Keywords: apple fruit of Food Science and Technology, Shanghai Ocean University, Shanghai, P. R. China 201306 2 College of Urban Construction and Environment Engineering, University of Shanghai for Science and Technology, Shanghai, P. R

Boyer, Edmond

383

Discovery of Four Doubly Imaged Quasar Lenses from the Sloan Digital Sky Survey  

E-Print Network (OSTI)

We report the discovery of four doubly imaged quasar lenses. All the four systems are selected as lensed quasar candidates from the Sloan Digital Sky Survey data. We confirm their lensing hypothesis with additional imaging and spectroscopic follow-up observations. The discovered lenses are SDSS J0743+2457 with the source redshift z_s=2.165, the lens redshift z_l=0.381, and the image separation theta=1.034", SDSS J1128+2402 with z_s=1.608 and theta=0.844", SDSS J1405+0959 with z_s=1.810, z_l~0.66, and theta=1.978", and SDSS J1515+1511 with z_s=2.054, z_l=0.742, and theta=1.989". It is difficult to estimate the lens redshift of SDSS J1128+2402 from the current data. Two of the four systems (SDSS J1405+0959 and SDSS J1515+1511) are included in our final statistical lens sample to derive constraints on dark energy and the evolution of massive galaxies.

Inada, Naohisa; Rusu, Cristian E; Kayo, Issha; Morokuma, Tomoki

2014-01-01T23:59:59.000Z

384

THE DISCOVERY OF AN ULTRA-FAINT STAR CLUSTER IN THE CONSTELLATION OF URSA MINOR  

SciTech Connect

We report the discovery of a new ultra-faint globular cluster in the constellation of Ursa Minor, based on stellar photometry from the MegaCam imager at the Canada-France-Hawaii Telescope. We find that this cluster, Munoz 1, is located at a distance of 45 {+-} 5 kpc and at a projected distance of only 45' from the center of the Ursa Minor dwarf spheroidal galaxy. Using a maximum-likelihood technique we measure a half-light radius of 0.'5, or equivalently 7 pc, and an ellipticity consistent with being zero. We estimate its absolute magnitude to be M{sub V} -0.4 {+-} 0.9, which corresponds to L{sub V} = 120{sup +160}{sub -65} L{sub Sun} and we measure a heliocentric radial velocity of -137 {+-} 4 km s{sup -1} based on Keck/DEIMOS spectroscopy. This new satellite is separate from Ursa Minor by {approx}30 kpc and 110 km s{sup -1} suggesting the cluster is not obviously associated with the dSph, despite the very close angular separation. Based on its photometric properties and structural parameters we conclude that Munoz 1 is a new ultra-faint stellar cluster. Along with Segue 3 this is one of the faintest stellar clusters known to date.

Munoz, R. R.; Geha, M.; Vargas, L. C. [Astronomy Department, Yale University, New Haven, CT 06520 (United States); Cote, P.; Stetson, P. [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC V9E 2E7 (Canada); Santana, F. A. [Departamento de Astronomia, Universidad de Chile, Camino El Observatorio 1515, Las Condes, Santiago (Chile); Simon, J. D. [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Djorgovski, S. G., E-mail: rmunoz@das.uchile.cl [Astronomy Department, California Institute of Technology, Pasadena, CA 91125 (United States)

2012-07-01T23:59:59.000Z

385

The pharmaceutical value of marine biodiversity for anti-cancer drug discovery  

Science Journals Connector (OSTI)

Marine biodiversity is a resource of enormous importance to human societies that provides critical ecosystem services. Economic valuation of some services has been utilized to promote conservation initiatives by revealing a tangible and causative link between biodiversity declines and economic losses. Other ecosystem services have eluded valuation, including the value of the sea as a repository of novel pharmaceuticals. Here, we provide the first global estimate of the number, source and market value of undiscovered oncology drugs based on empirical data, industry statistics and conservative modelling assumptions. We report US$563billion5.69trillion attributable to anti-cancer drugs of marine origin pending discovery, revealing a new and substantial at-risk ecosystem service value. Our model predicted 253,120594,232 novel chemicals in marine organisms; 90.492.6% of these compounds remain undiscovered. A total of 55 to 214 new anti-cancer drugs were predicted to reach the market sourced primarily from animal phyla (Chordata, Mollusca, Porifera, and Byrozoa) and microbial phyla (Proteobacteria and Cyanobacteria). While no single aspect of extractive marine resource value should be relied upon to account for the opportunity costs of conservation initiatives, the application of valuation models to ecosystem services further reveals the true, irreversible economic cost of habitat degradation and biodiversity declines.

Patrick M. Erwin; Susanna Lpez-Legentil; Peter W. Schuhmann

2010-01-01T23:59:59.000Z

386

Methodology of Materials Discovery in Complex Metal Hydrides Using Experimental and Computational Tools  

SciTech Connect

We present a review of the experimental and theoretical methods used in the discovery of new metal-hydrogen materials systems for hydrogen storage applications. Rather than a comprehensive review of all new materials and methods used in the metal hydride community, we focus on a specific subset of successful methods utilizing theoretical crystal structure prediction methods, computational approaches for screening large numbers of compound classes, and medium-throughput experimental methods for the preparation of such materials. Monte Carlo techniques paired with a simplified empirical Hamiltonian provide crystal structure candidates that are refined using Density Functional Theory. First-principle methods using high-quality structural candidates are further screened for an estimate of reaction energetics, decomposition enthalpies, and determination of reaction pathways. Experimental synthesis utilizes a compacted-pellet sintering technique under high-pressure hydrogen at elevated temperatures. Crystal structure determination follows from a combination of Rietveld refinements of diffraction patterns and first-principles computation of total energies and dynamical stability of competing structures. The methods presented within are general and applicable to a wide class of materials for energy storage.

Majzoub, Eric H.; Ronnebro, Ewa

2012-02-22T23:59:59.000Z

387

Field Mapping | Open Energy Information  

Open Energy Info (EERE)

Field Mapping Field Mapping Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Technique: Field Mapping Details Activities (59) Areas (35) Regions (6) NEPA(0) Exploration Technique Information Exploration Group: Field Techniques Exploration Sub Group: Data Collection and Mapping Parent Exploration Technique: Data Collection and Mapping Information Provided by Technique Lithology: Map surface geology and hydrothermal alteration. Stratigraphic/Structural: Map fault and fracture patterns, kinematic information. Hydrological: Map surface manifestations of geothermal systems. Thermal: Map surface temperature. Cost Information Low-End Estimate (USD): 400.0040,000 centUSD 0.4 kUSD 4.0e-4 MUSD 4.0e-7 TUSD / hour Median Estimate (USD): 600.0060,000 centUSD

388

THE SOLAR NEIGHBORHOOD. XXIII. CCD PHOTOMETRIC DISTANCE ESTIMATES OF SCR TARGETS-77 M DWARF SYSTEMS WITHIN 25 pc  

SciTech Connect

We present CCD photometric distance estimates of 100 SCR (SuperCOSMOS RECONS) systems with {mu} {>=} 0.''18 yr{sup -1}, 29 of which are new discoveries previously unpublished in this series of papers. These distances are estimated using a combination of new VRI photometry acquired at CTIO and JHK magnitudes extracted from 2MASS. The estimates are improvements over those determined using photographic plate BRI magnitudes from SuperCOSMOS plus JHK, as presented in the original discovery papers. In total, 77 of the 100 systems investigated are predicted to be within 25 pc. If all 77 systems are confirmed to have {pi}{sub trig} {>=} 40 mas, this sample would represent a 23% increase in M dwarf systems nearer than 25 pc in the southern sky.

Winters, Jennifer G.; Henry, Todd J.; Jao, Wei-Chun [Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30302-4106 (United States); Subasavage, John P. [Cerro Tololo Inter-American Observatory, Casilla 603, La Serena (Chile); Finch, Charlie T. [United States Naval Observatory, Washington, DC 20392-5420 (United States); Hambly, Nigel C., E-mail: winters@chara.gsu.edu, E-mail: thenry@chara.gsu.edu, E-mail: jao@chara.gsu.edu, E-mail: jsubasavage@ctio.noao.edu, E-mail: finch@usno.navy.mil, E-mail: nch@roe.ac.uk [Scottish Universities Physics Alliance (SUPA), Institute of Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom)

2011-01-15T23:59:59.000Z

389

Quantum limits to estimation of photon deformation  

E-Print Network (OSTI)

We address potential deviations of radiation field from the bosonic behaviour and employ local quantum estimation theory to evaluate the ultimate bounds to precision in the estimation of these deviations using quantum-limited measurements on optical signals. We consider different classes of boson deformation and found that intensity measurement on coherent or thermal states would be suitable for their detection making, at least in principle, tests of boson deformation feasible with current quantum optical technology. On the other hand, we found that the quantum signal-to-noise ratio (QSNR) is vanishing with the deformation itself for all the considered classes of deformations and probe signals, thus making any estimation procedure of photon deformation inherently inefficient. A partial way out is provided by the polynomial dependence of the QSNR on the average number of photon, which suggests that, in principle, it would be possible to detect deformation by intensity measurements on high-energy thermal states.

Giovanni De Cillis; Matteo G. A. Paris

2014-07-08T23:59:59.000Z

390

DISCOVERY OF COLD, PRISTINE GAS POSSIBLY ACCRETING ONTO AN OVERDENSITY OF STAR-FORMING GALAXIES AT REDSHIFT z {approx} 1.6  

SciTech Connect

We report the discovery of large amounts of cold (T {approx} 10{sup 4} K), chemically young gas in an overdensity of galaxies at redshift z Almost-Equal-To 1.6 located in the Great Observatories Origins Deep Survey southern field. The gas is identified thanks to the ultra-strong Mg II {lambda}2800 absorption features it imprints onto the rest-frame UV spectra of galaxies in the background of the overdensity. There is no evidence that the optically thick gas is part of any massive galaxy (i.e., M{sub star} > 4 Multiplication-Sign 10{sup 9} M{sub Sun }), but rather is associated with the overdensity; less massive and fainter galaxies (25.5 mag < z < 27.5 mag) have too large an impact parameter to be causing ultra-strong absorption systems, based on our knowledge of such systems. The lack of corresponding Fe II absorption features, not detected even in co-added spectra, suggests that the gas is chemically more pristine than the interstellar medium and outflows of star-forming galaxies at similar redshift, including the galaxies of the overdensity itself, and comparable to the most metal-poor stars in the Milky Way halo. A crude estimate of the projected covering factor of the high-column-density gas (N{sub H} {approx}> 10{sup 20} cm{sup -2}) based on the observed fraction of galaxies with ultra-strong absorbers is C{sub F} Almost-Equal-To 0.04. A broad, continuum absorption profile extending to the red of the interstellar Mg II absorption line by {approx}< 2000 km s{sup -1} is possibly detected in two independent co-added spectra of galaxies belonging to the overdensity, consistent with a large-scale infall motion of the gas onto the overdensity and its galaxies. Overall, these findings provide the first tentative evidence of accretion of cold, chemically young gas onto galaxies at high redshift, possibly feeding their star formation activity. We suggest the fact that the galaxies are members of a large structure, as opposed to field galaxies, might play a significant role in our ability to detect the accreting gas.

Giavalisco, Mauro; Salimbeni, Sara; Tripp, Todd M.; Cassata, Paolo; Guo Yicheng; Tang Yuping [Astronomy Department, University of Massachusetts, Amherst, MA 01003 (United States); Vanzella, Eros; Nonino, Mario [INAF-Osservatorio Astronomico di Trieste, I-40131 Trieste (Italy); Dickinson, Mark [National Optical Astronomy Observatories, Tucson, AZ 85719 (United States); Renzini, Alvio [INAF-Osservatorio Astronomico di Padova, I-35122 Padova (Italy); Ferguson, Henry C. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Cimatti, Andrea [Dipartimento di Astronomia, Universita degli Studi di Bologna, I-40127 Bologna (Italy); Kurk, Jaron [Max Planck Institut fuer Extraterrestrische Physik, D-85748 Garching (Germany); Mignoli, Marco, E-mail: mauro@astro.umass.edu [INAF-Osservatorio Astronomico di Bologna, I-40127 Bologna (Italy)

2011-12-10T23:59:59.000Z

391

Use of Cost Estimating Relationships  

Directives, Delegations, and Requirements

Cost Estimating Relationships (CERs) are an important tool in an estimator's kit, and in many cases, they are the only tool. Thus, it is important to understand their limitations and characteristics. This chapter discusses considerations of which the estimator must be aware so the Cost Estimating Relationships can be properly used.

1997-03-28T23:59:59.000Z

392

Reinforcing floodrisk estimation  

Science Journals Connector (OSTI)

...publication of the Flood estimation handbook, studies of ood risk are now...especially for its neglect of the physics of catchment pro- cesses of...recommended in the Flood estimation handbook (Institute of Hydrology 1999...estimates. The Flood estimation handbook (Institute of Hydrology 1999...

2002-01-01T23:59:59.000Z

393

Multiple phase estimation in quantum cloning machines  

E-Print Network (OSTI)

Since the initial discovery of the Wootters-Zurek no-cloning theorem, a wide variety of quantum cloning machines have been proposed aiming at imperfect but optimal cloning of quantum states within its own context. Remarkably, most previous studies have employed the Bures fidelity or the Hilbert-Schmidt norm as the figure of merit to characterize the quality of the corresponding cloning scenarios. However, in many situations, what we truly care about is the relevant information about certain parameters encoded in quantum states. In this work, we investigate the multiple phase estimation problem in the framework of quantum cloning machines, from the perspective of quantum Fisher information matrix (QFIM). Focusing on the generalized d-dimensional equatorial states, we obtain the analytical formulas of QFIM for both universal quantum cloning machine (UQCM) and phase-covariant quantum cloning machine (PQCM), and prove that PQCM indeed performs better than UQCM in terms of QFIM. We highlight that our method can be generalized to arbitrary cloning schemes where the fidelity between the single-copy input and output states is input-state independent. Furthermore, the attainability of the quantum Cramer-Rao bound is also explicitly discussed.

Yao Yao; Li Ge; Xing Xiao; Xiao-guang Wang; Chang-pu Sun

2014-07-22T23:59:59.000Z

394

Field Sampling | Open Energy Information  

Open Energy Info (EERE)

form form View source History View New Pages Recent Changes All Special Pages Semantic Search/Querying Get Involved Help Apps Datasets Community Login | Sign Up Search Page Edit with form History Facebook icon Twitter icon » Field Sampling Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Technique: Field Sampling Details Activities (0) Areas (0) Regions (0) NEPA(0) Exploration Technique Information Exploration Group: Field Techniques Exploration Sub Group: Field Sampling Parent Exploration Technique: Field Techniques Information Provided by Technique Lithology: Rock samples are used to define lithology. Field and lab analyses can be used to measure the chemical and isotopic constituents of rock samples. Stratigraphic/Structural: Can reveal relatively high permeability zones. Provides information about the time and environment which formed a particular geologic unit. Microscopic rock textures can be used to estimate the history of stress and strain, and/or faulting.

395

24 METRO Monday, March 10, 2014 METROCOSM SCIENCE & DISCOVERY by BEN GILLILAND  

E-Print Network (OSTI)

of the greatest mysteries in science ­ what is dark matter and dark energy made of? #12;Monday, March 10, 2014 (levels) Neutron at lowest energy state 22 33 44 5511 METROCOSMSCIENCE & DISCOVERY by BEN GILLILAND24 METRO Monday, March 10, 2014 METROCOSM SCIENCE & DISCOVERY by BEN GILLILAND Follow @Gilli

Rotter, Stefan

396

Data Warehouse Design for Pharmaceutical Drug Discovery Research Melinda G. Axel and Il-Yeol Song  

E-Print Network (OSTI)

an analysis of the principal activities involved in drug discovery in the pharmaceutical industry, and a setData Warehouse Design for Pharmaceutical Drug Discovery Research Melinda G. Axel and Il-Yeol Song: axel@superlink.net, songiy@post.drexel.edu Abstract Pharmaceutical companies spend billions of dollars

Song, Il-Yeol

397

Hybrid Resource Discovery Mechanism in Ad Hoc Grid Using Structured Overlay  

E-Print Network (OSTI)

Hybrid Resource Discovery Mechanism in Ad Hoc Grid Using Structured Overlay Tariq Abdullah1, Luc.onana, david.calomme}@umh.ac.be Abstract. Resource management has been an area of research in ad hoc grids, decentralized or in a hybrid manner. In this paper, we discuss a micro economic based, hybrid resource discovery

Kuzmanov, Georgi

398

College of Engineering Discovery with Purpose www.engineering.iastate.edu  

E-Print Network (OSTI)

to the College of Engineering website. Hover over "Student Services" and you will see the `Scholarships' link12/6/2011 1 College of Engineering Discovery with Purpose www.engineering.iastate.edu College of Engineering Scholarship Program Joel Johnson, Director, ESS College of Engineering Discovery with Purpose www.engineering

Lin, Zhiqun

399

M2MI Service Discovery Middleware Framework Hans-Peter Bischof, Joel Varela Donado  

E-Print Network (OSTI)

M2MI Service Discovery Middleware Framework Hans-Peter Bischof, Joel Varela Donado Rochester.rit.edu Abstract. The Many-to-Many-Invocation (M2MI) Service Discovery Middleware Framework provides an API for publishing, providing, and using services in a serverless ad hoc network of devices imple- menting the M2MI

Bischof, Hans-Peter

400

Chapter Title Fundamentals of Spatial Data Warehousing for Geographic Knowledge Discovery  

E-Print Network (OSTI)

Chapter Title Fundamentals of Spatial Data Warehousing for Geographic Knowledge Discovery YVAN for spatial data warehousing) 2. Concepts and architectures of data warehouses 3. Spatial data warehousing 4. Conclusion: Challenges of spatial data warehousing for geographic knowledge discovery #12;1. Introduction

Note: This page contains sample records for the topic "field discoveries estimated" 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

Fast entropic profiler: an information theoretic approach for the discovery of patterns in genomes  

Science Journals Connector (OSTI)

Information theory has been used for quite some time in the area of computational biology. In this paper we present a pattern discovery method, named Fast Entropic Profiler, that is based on a local entropy function that captures the importance of a ... Keywords: computational biology, information theory, local entropy, pattern discovery

Matteo Comin, Morris Antonello

2014-05-01T23:59:59.000Z

402

An LDA-based Community Structure Discovery Approach for Large-Scale Social Networks  

E-Print Network (OSTI)

: {bqiu}@cse.psu.edu Abstract-- Community discovery has drawn significant re- search interests among even more attentions with the prevalence of social network websites, such as MySpace, Live of this paper include: (1) an LDA-based probabilistic community discovery model in large-sc

403

Evaluation of an integrated Knowledge Discovery and Data Mining process model  

Science Journals Connector (OSTI)

Data Mining projects are implemented by following the knowledge discovery process. This process is highly complex and iterative in nature and comprises of several phases, starting off with business understanding, and followed by data understanding, data ... Keywords: Analytical testing, CRISP-DM, Evaluation, IKDDM, Knowledge Discovery and Data Mining (KDDM) process models

Sumana Sharma; Kweku-Muata Osei-Bryson; George M. Kasper

2012-10-01T23:59:59.000Z

404

Multi-University Research to Advance Discovery Fusion Energy Science using a  

E-Print Network (OSTI)

Dept of Applied Physics and Applied Math, Columbia University, New York, NY Plasma Science and FusionMulti-University Research to Advance Discovery Fusion Energy Science using a Superconducting Center, MIT, Cambridge, MA Outline · Intermediate scale discovery fusion energy science needs support

405

False Discovery Control in Large-Scale Spatial Multiple Wenguang Sun  

E-Print Network (OSTI)

is one of the six criteria pollutants regulated by the US EPA under the Clean Air Act and has been linkedFalse Discovery Control in Large-Scale Spatial Multiple Testing Wenguang Sun University of Southern and computational framework for false discovery control in multiple testing of spatial signals. We consider both

Cai, T. Tony

406

Discovery of Cellulose as a Smart Material Jaehwan Kim* and Sungryul Yun  

E-Print Network (OSTI)

Discovery of Cellulose as a Smart Material Jaehwan Kim* and Sungryul Yun Center for EAPap Actuator in cellulose applications and technologies by reporting our discovery of cellulose as a smart material that can, however, the potential of cellulose as a smart lightweight material that can be used as a sensor

Ounaies, Zoubeida

407

Mr. Harold Snyder Chief, Discovery and Investigations Branch  

Office of Legacy Management (LM)

Harold Snyder Harold Snyder Chief, Discovery and Investigations Branch Hazardous Site Control Division Administration for Solid Waste and Emergency Response U. S. Environmental Protection Agency 401 M Street, S. W. Washington, D. C. 70460 Dear Mr. Snyder: The Department of Energy (DDE) has conducted a radiological survey at the Conserv Corporation (The former Virginia-Carolina Chemical Corporation), Nichols, Florida. This survey indicated that levels of residual radioactive material and associated radiation levels at the sfte are in excess c?f those used by DOE to determine if a site requires remedial actfon. The data did not indicate that, under the current use of the site, there was any hazard to the workers or the general public. However, changes fn site use or modifications to the facility could'possibly result

408

Photon Sciences Directorate | 2010 Annual Report | DISCOVERY at Light Speed  

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

BNL People BNL People 2010 ANNUAL REPORT Photon Sciences Directorate at Brookhaven National Laboratory Reflections on the Year Steve Dierker Steve Dierker, Associate Laboratory Director for Photon Sciences This is a very exciting period for photon sciences at Brookhaven National Laboratory. It is also a time of unprecedented growth for the Photon Sciences Directorate, which operates the National Synchrotron Light Source (NSLS) and is constructing NSLS-II, both funded by the Department of Energy's Office of Science. Reflecting the quick pace of our activities, we chose the theme "Discovery at Light Speed" for the directorate's 2010 annual report, a fiscal year bookended by October 2009 and September 2010. The year began with the news that NSLS users Venki Ramakrishnan of

409

A New Discovery Answers an Old Question | Advanced Photon Source  

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

Peering into the Interfaces of Nanoscale Polymeric Materials Peering into the Interfaces of Nanoscale Polymeric Materials Ironing Out the Details of the Earth's Core Science Highlights Archives: 2013 | 2012 | 2011 | 2010 2009 | 2008 | 2007 | 2006 2005 | 2004 | 2003 | 2002 2001 | 2000 | 1998 | Subscribe to APS Science Highlights rss feed A New Discovery Answers an Old Question JANUARY 25, 2012 Bookmark and Share Diffraction intensity contrast maps for Fe0.94O measured at 24.7 GPa. From Yang Ding et al., Appl. Phys.Lett. 100, 041903 (2012). The transition-metal monoxide FeO is an archetypal example of a Mott insulator-a material that should conduct electricity under conventional band theories but becomes an insulator when measured, especially at low temperatures-and a major iron-bearing component of the Earth's interior. Understanding the high-pressure behavior of this material is

410

Mr. Harold Snyder Chief, Discovery and Investigations Branch  

Office of Legacy Management (LM)

. 20545 . 20545 FEB 2 7 1985 Mr. Harold Snyder Chief, Discovery and Investigations Branch Hazardous Site Control Division Administration for Solid Waste and Emergency Response U. S. Environmental Protection Agency 401 M Street, S. W. Washington, D. C. 20460 Dear Mr. Snyder: The Department of Olin Corporation, Joliet, Illinois. Energy (DOE) has conducted a radiological survey at the Chemicals Group (The former Blockson Chemical Company), This survey indicated that levels of residual radioactive material and associated radiation levels at the site are in excess of those used by DOE to determine if a site requires remedial action. The data did not indicate that, under the current use of the site, there was any hazard to the workers or the general public. However,

411

BNL | Photon Sciences, Light as a Discovery Tool  

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

Photon Sciences Photon Sciences image Light as a Discovery Tool Brookhaven conducts scientific research using photons-particles of light-to probe the structure and makeup of materials. The National Synchrotron Light Source (NSLS) uses electrons accelerated along a high-tech ring at nearly the speed of light to create beams of light in the x-ray, ultraviolet, and infrared wavelengths, resulting in a kind of giant microscope. Revealing the Structure of Matter Scientists use beam lines at NSLS to probe the electronic and atomic structures of materials, analyze very small samples, or map surfaces with atomic-scale sensitivity. Researchers at NSLS use an array of sophisticated imaging techniques to get highly detailed "pictures" of a wide range of materials, from biological molecules to advanced electronics.

412

Mr. Harold Snyder, Chief Discovery and Investigation Branch  

Office of Legacy Management (LM)

Ofll s' Ofll s' :y 1: ,' :*,; / c- tii; 1 ;q' (/. 4 L Department of Energy Washington, D .C. 20545 Mr. Harold Snyder, Chief Discovery and Investigation Branch Hazardous Site Control Division Administration for Solid Waste and Emergency Response U.S. Environmental Protection Agency 401 M Street Washington, D.C. 20460 Dear Mr. Snyder: The Department of Energy (DOE) radiological survey at the former Horizons, Inc. facility at 2909 East 79th Street in Cleveland, Ohio, performed in 1977, indicated that levels of residual radioactive materials and associated radiation levels were in excess of those used by DOE to determine if a site requires remedial action. The radioactive contamination and elevated radiation levels on the site were found, for the most part, in storage areas, in drains, and under floors. These data did

413

Computer discovery of the mechanism of flow-induced sloshing  

SciTech Connect

A novel numerical method called physical component boundary fitted coordinate method (PC-BFC method) was applied to a recently discovered flow instability called in-vessel flow-induced sloshing. Then, with a spirit of computer discovery, a general procedure was developed and applied for solving the mechanism and condition for the occurrence of this sloshing. As a result, a nonlinear wave that never reflects at the wall was singled out numerically and was demonstrated to be the cause of the sloshing. In-vessel circulated free surface flow characterizes the flow of coolant in liquid metal cooled fast breeder reactor (LMFBR) during power generation; finding of the criteria for the occurrence of this sloshing has crucial importance for the safety operation of LMFBR.

Takizawa, Akihiko [Tokyo Electric Power Co., Yokohama (Japan). Nuclear Power R and D Center; Kondo, Shunsuke [Univ. of Tokyo (Japan). Dept. of Quantum Engineering and Systems Science

1995-11-01T23:59:59.000Z

414

Biofuel Distribution Datasets from the Bioenergy Knowledge Discovery Framework  

DOE Data Explorer (OSTI)

The Bioenergy Knowledge Discovery Framework invites users to discover the power of bioenergy through an interface that provides extensive access to research data and literature, GIS mapping tools, and collaborative networks. The Bioenergy KDF supports efforts to develop a robust and sustainable bioenergy industry. The KDF facilitates informed decision making by providing a means to synthesize, analyze, and visualize vast amounts of information in a relevant and succinct manner. It harnesses Web 2.0 and social networking technologies to build a collective knowledge system that can better examine the economic and environmental impacts of development options for biomass feedstock production, biorefineries, and related infrastructure. [copied from https://www.bioenergykdf.net/content/about] Holdings include datasets, models, and maps and the collections are growing due to both DOE contributions and individuals' data uploads.

415

Biofuel Production Datasets from DOE's Bioenergy Knowledge Discovery Framework (KDF)  

DOE Data Explorer (OSTI)

The Bioenergy Knowledge Discovery Framework invites users to discover the power of bioenergy through an interface that provides extensive access to research data and literature, GIS mapping tools, and collaborative networks. The Bioenergy KDF supports efforts to develop a robust and sustainable bioenergy industry. The KDF facilitates informed decision making by providing a means to synthesize, analyze, and visualize vast amounts of information in a relevant and succinct manner. It harnesses Web 2.0 and social networking technologies to build a collective knowledge system that can better examine the economic and environmental impacts of development options for biomass feedstock production, biorefineries, and related infrastructure. [copied from https://www.bioenergykdf.net/content/about]

Holdings include datasets, models, and maps and the collections arel growing due to both DOE contributions and data uploads from individuals.

416

Feedstock Production Datasets from the Bioenergy Knowledge Discovery Framework  

DOE Data Explorer (OSTI)

The Bioenergy Knowledge Discovery Framework invites users to discover the power of bioenergy through an interface that provides extensive access to research data and literature, GIS mapping tools, and collaborative networks. The Bioenergy KDF supports efforts to develop a robust and sustainable bioenergy industry. The KDF facilitates informed decision making by providing a means to synthesize, analyze, and visualize vast amounts of information in a relevant and succinct manner. It harnesses Web 2.0 and social networking technologies to build a collective knowledge system that can better examine the economic and environmental impacts of development options for biomass feedstock production, biorefineries, and related infrastructure. [copied from https://www.bioenergykdf.net/content/about] Holdings include datasets, models, and maps and the collections are growing due to both DOE contributions and data uploads from individuals.

417

Feedstock Logistics Datasets from DOE's Bioenergy Knowledge Discovery Framework (KDF)  

DOE Data Explorer (OSTI)

The Bioenergy Knowledge Discovery Framework invites users to discover the power of bioenergy through an interface that provides extensive access to research data and literature, GIS mapping tools, and collaborative networks. The Bioenergy KDF supports efforts to develop a robust and sustainable bioenergy industry. The KDF facilitates informed decision making by providing a means to synthesize, analyze, and visualize vast amounts of information in a relevant and succinct manner. It harnesses Web 2.0 and social networking technologies to build a collective knowledge system that can better examine the economic and environmental impacts of development options for biomass feedstock production, biorefineries, and related infrastructure. Holdings include datasets, models, and maps. [from https://www.bioenergykdf.net/content/about

418

7.27 - Advances in the Discovery of New Antimalarials  

Science Journals Connector (OSTI)

Malaria is a major parasitic infection that affects more than half of the world's population and causes over a million deaths each year. The resistance developed by the parasites to traditional drugs and decreasing effectiveness of insecticides towards mosquito vectors is seriously hindering malaria control programs. Discovery of new antimalarial agents or improving the effectiveness of existing ones is therefore urgently needed to face the health threat from this infection. This chapter gives a comprehensive overview of malaria epidemiology, with particular emphasis on progress made in the drug development efforts during the last decade. Modes of action of each class of drugs or the biosynthetic pathways they target, and details regarding drug resistance and prospects of combination therapy are discussed.

K.M. Muraleedharan; M.A. Avery

2007-01-01T23:59:59.000Z

419

Precipitable water structure in tropical systems as estimated from TOVS  

E-Print Network (OSTI)

and OLR . . . 28 67 85 6. Annual and semi-annual cycle effect estimates for selected areas . . . 89 LIST OF FIGURES Figure Page 1. PW fields from three models for 8 Feb 1988. Contour intervals are. 5 cm. . 34 2. PW fields from three models for 10... Feb 1988. Contour intervals are. 5 cm. 35 3. PW field for 9 Jan 1988. Contour intervals are . 5 cm. . 37 4. OLR field for 9 Jan 1988. Contour intervals are 25 Wm-2. . . . 38 5. PW fields from three models for 15 Aug 1990. Contour intervals are . 5...

Hatfield, Eric

2012-06-07T23:59:59.000Z

420

Global Discovery introduced at AAAS 2006 | OSTI, US Dept of Energy, Office  

Office of Scientific and Technical Information (OSTI)

Global Discovery introduced at AAAS 2006 Global Discovery introduced at AAAS 2006 Office of Scientific & Technical Information NEWS MEDIA CONTACT: Cathey Daniels, (865) 576-9539 FOR IMMEDIATE RELEASE February 17, 2006 Global Discovery introduced at AAAS 2006 Oak Ridge, TN - The U.S. Department of Energy Office of Scientific and Technical Information, a component of the Office of Science, is looking at new ways to disseminate science information. As tools and technologies rapidly become more sophisticated, OSTI is conducting applied research on a number of challenges related to this vision aimed at turning local discovery into Global Discovery. The benefits for researchers, for citizens, and for the U.S. economy could prove far-reaching as OSTI, through its Innovations in Scientific Knowledge and

Note: This page contains sample records for the topic "field discoveries estimated" 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

Discovery through Teamwork | U.S. DOE Office of Science (SC)  

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

Discovery through Teamwork Discovery through Teamwork Discovery & Innovation Stories of Discovery & Innovation Brief Science Highlights SBIR/STTR Highlights Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 07.29.13 Discovery through Teamwork By coordinating capabilities across institutions, DOE Bioenergy Research Center scientists identify a powerful new microbe for biofuel processing. Print Text Size: A A A Subscribe FeedbackShare Page Click to enlarge photo. Enlarge Photo An image of the bacterium Caldicellulosiruptor bescii, named for the DOE BioEnergy Science Center (BESC). Photo courtesy of Michael W. W. Adams The bacterium Caldicellulosiruptor bescii, named for the DOE BioEnergy Science Center (BESC).

422

Discovery of Dark Energy Ushered in a New Era in Computational Cosmology  

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

Discovery of Dark Discovery of Dark Energy Ushered in a New Era in Computational Cosmology Discovery of Dark Energy Ushered in a New Era in Computational Cosmology October 4, 2011 | Tags: Astrophysics, Awards John Hules, JAHules@lbl.gov, +1 510 486 6008 "If NERSC does not enable a major scientific discovery every few years, then we're not doing our job." That was the challenge issued by Bill McCurdy, then Lawrence Berkeley National Laboratory's Associate Laboratory Director for Computing Sciences, at the first all-hands meeting for staff of the National Energy Research Scientific Computing Center (NERSC) when the center reopened after moving to Berkeley Lab in spring of 1996. No one at that meeting could have guessed that the first major breakthrough enabled by NERSC would be a startling discovery in cosmology-that the

423

Comparison of discovery limits for extra Z bosons at future colliders  

Science Journals Connector (OSTI)

We study and compare the discovery potential for heavy neutral gauge bosons (Z) at various e+e- and pp(-) colliders that are planned or have been proposed. Typical discovery limits are for the Fermilab Tevatron ?1 TeV, Di-Tevatron ?2 TeV, CERN LHC ?4 TeV, LSGNA (a 60 TeV pp collider) ?13 TeV while the e+e- discovery limits are 210 ?s with the large variation reflecting the model dependence of the limits. While both types of colliders have comparable discovery limits the hadron colliders are generally less dependent on the specific Z model and provide more robust limits since the signal has little background. In contrast, discovery limits for e+e- limits are more model dependent and, because they are based on indirect inferences of deviations from standard model predictions, they are more sensitive to systematic errors.

Stephen Godfrey

1995-02-01T23:59:59.000Z

424

Discovery and Characterization of Radiation Mitigator Yel002  

E-Print Network (OSTI)

years at the time of the chernobyl accident. Int. J. Canceremergency workers of the chernobyl accident: Estimation ofS.E. Incidence of post-chernobyl leukemia and thyroid cancer

Rivina, Yelena Olegovna

2013-01-01T23:59:59.000Z

425

A hero's little horse: discovery of a dissolving star cluster in Pegasus  

E-Print Network (OSTI)

We report the discovery of an ultra-faint stellar system in the constellation of Pegasus. This concentration of stars was detected by applying our overdensity detection algorithm to the SDSS-DR10 and confirmed with deeper photometry from the Dark Energy Camera at the 4-m Blanco telescope. The best-fitting model isochrone indicates that this stellar system, Kim 1, features an old (12 Gyr) and metal-poor ([Fe/H]$\\sim-1.7$) stellar population at a heliocentric distance of $19.8\\pm0.9$ kpc. We measure a half-light radius of $6.9\\pm0.6$ pc using a Plummer profile. The small physical size and the extremely low luminosity are comparable to the faintest known star clusters Segue 3, Koposov 1 & 2, and Mu\\~noz 1. However, Kim 1 exhibits a lower star concentration and is lacking a well defined center. It also has an unusually high ellipticity and irregular outer isophotes, which suggests that we are seeing an intermediate mass star cluster being stripped by the Galactic tidal field. An extended search for evidence o...

Kim, Dongwon

2014-01-01T23:59:59.000Z

426

THE DISCOVERY OF THE MOST DISTANT KNOWN TYPE Ia SUPERNOVA AT REDSHIFT 1.914  

SciTech Connect

We present the discovery of a Type Ia supernova (SN) at redshift z = 1.914 from the CANDELS multi-cycle treasury program on the Hubble Space Telescope (HST). This SN was discovered in the infrared using the Wide-Field Camera 3, and it is the highest-redshift Type Ia SN yet observed. We classify this object as a SN Ia by comparing its light curve and spectrum with those of a large sample of Type Ia and core-collapse SNe. Its apparent magnitude is consistent with that expected from the {Lambda}CDM concordance cosmology. We discuss the use of spectral evidence for classification of z > 1.5 SNe Ia using HST grism simulations, finding that spectral data alone can frequently rule out SNe II, but distinguishing between SNe Ia and SNe Ib/c can require prohibitively long exposures. In such cases, a quantitative analysis of the light curve may be necessary for classification. Our photometric and spectroscopic classification methods can aid the determination of SN rates and cosmological parameters from the full high-redshift CANDELS SN sample.

Jones, David O.; Rodney, Steven A.; Riess, Adam G. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Dahlen, Tomas; Casertano, Stefano; Koekemoer, Anton [Space Telescope Science Institute, Baltimore, MD 21218 (United States); McCully, Curtis; Keeton, Charles R.; Patel, Brandon [Department of Physics and Astronomy, Rutgers, State University of New Jersey, Piscataway, NJ 08854 (United States); Frederiksen, Teddy F.; Hjorth, Jens [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen (Denmark); Strolger, Louis-Gregory [Department of Physics, Western Kentucky University, Bowling Green, KY 42101 (United States); Wiklind, Tommy G. [Joint ALMA Observatory, ESO, Santiago (Chile); Challis, Peter [Harvard/Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Graur, Or [School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978 (Israel); Hayden, Brian; Garnavich, Peter [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Weiner, Benjamin J. [Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States); Filippenko, Alexei V. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); and others

2013-05-10T23:59:59.000Z

427

No more gas from Egypt? Modeling offshore discoveries and import uncertainty of natural gas in Israel  

Science Journals Connector (OSTI)

Abstract Israel depends on natural gas imports from Egypt for about 40% of its domestic needs, with the remaining met from domestic production. Gas supplies from Egypt have been erratic since their initiation: disruptions have increased after the 2011 revolution in Egypt and have been further ignited by public discontent. Despite these developments, Israeli policy makers have viewed the Egyptian gas deal as a positive factor in preserving peace with Egypt and have had no better alternatives than relying upon it. This has changed, however, after recent discoveries of three major offshore fields that are expected to satisfy domestic demand for an indefinite period and to provide gas for exports. We use an extended global CGE modeling framework that incorporates multiple households and factor ownership to investigate the effects of reduced gas imports from Egypt and the evolvement of domestic gas production as an alternative. In case of reduced gas imports from Egypt, the Israeli economy would slightly retract mainly due to lower production in energy intensive sectors. Poor households would be the most negatively affected, due to the strongest relative decline in income and the strongest increase of their consumer price index. In the case of increasing domestic gas production, Israeli GDP and domestic absorption would rise by about 0.2% and 0.4%, respectively. Poor households would be more positively affected than rich ones due to their composition of factor income and their higher expenditure shares for energy intensive commodities.

Khalid Siddig; Harald Grethe

2014-01-01T23:59:59.000Z

428

Parameter Estimation Through Ignorance  

E-Print Network (OSTI)

Dynamical modelling lies at the heart of our understanding of physical systems. Its role in science is deeper than mere operational forecasting, in that it allows us to evaluate the adequacy of the mathematical structure of our models. Despite the importance of model parameters, there is no general method of parameter estimation outside linear systems. A new relatively simple method of parameter estimation for nonlinear systems is presented, based on variations in the accuracy of probability forecasts. It is illustrated on the Logistic Map, the Henon Map and the 12-D Lorenz96 flow, and its ability to outperform linear least squares in these systems is explored at various noise levels and sampling rates. As expected, it is more effective when the forecast error distributions are non-Gaussian. The new method selects parameter values by minimizing a proper, local skill score for continuous probability forecasts as a function of the parameter values. This new approach is easier to implement in practice than alternative nonlinear methods based on the geometry of attractors or the ability of the model to shadow the observations. New direct measures of inadequacy in the model, the "Implied Ignorance" and the information deficit are introduced.

Hailiang Du; Leonard A. Smith

2012-06-06T23:59:59.000Z

429

Field Techniques | Open Energy Information  

Open Energy Info (EERE)

Field Techniques Field Techniques Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Exploration Technique: Field Techniques Details Activities (0) Areas (0) Regions (0) NEPA(0) Exploration Technique Information Exploration Group: Field Techniques Exploration Sub Group: None Parent Exploration Technique: Exploration Techniques Information Provided by Technique Lithology: Map surface geology and hydrothermal alteration. Rock samples are used to define lithology. Field and lab analyses can be used to measure the chemical and isotopic constituents of rock samples. Bulk and trace element analysis of rocks, minerals, and sediments. Identify and document surface geology and mineralogy. Rapid and unambiguous identification of unknown minerals.[1] Stratigraphic/Structural: Locates active faults in the area of interest. Map fault and fracture patterns, kinematic information. Can reveal relatively high permeability zones. Provides information about the time and environment which formed a particular geologic unit. Microscopic rock textures can be used to estimate the history of stress and strain, and/or faulting.

430

DISCOVERY OF AN ENERGETIC PULSAR ASSOCIATED WITH SNR G76.9+1.0  

SciTech Connect

We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray Observatory, the Robert C. Byrd Green Bank Radio Telescope, and the Rossi X-ray Timing Explorer (RXTE). The pulsar's spin-down rate implies a rotation-powered luminosity E-dot = 1.2x10{sup 38} erg s{sup -1}, a surface dipole magnetic field strength B{sub s} = 1.0 x 10{sup 12} G, and a characteristic age of 8.9 kyr. PSR J2022+3842 is thus the second-most energetic Galactic pulsar known, after the Crab pulsar, as well as the most rapidly rotating young, radio-bright pulsar known. The radio pulsations are highly dispersed and broadened by interstellar scattering, and we find that a large ({delta}f/f {approx} 1.9 x 10{sup -6}) spin glitch must have occurred between our discovery and confirmation observations. The X-ray pulses are narrow (0.06 cycles FWHM) and visible up to 20 keV, consistent with magnetospheric emission from a rotation-powered pulsar. The Chandra X-ray image identifies the pulsar with a hard, unresolved source at the midpoint of the double-lobed radio morphology of G76.9+1.0 and embedded within faint, compact X-ray nebulosity. The spatial relationship of the X-ray and radio emissions is remarkably similar to the extended structure seen around the Vela pulsar. The combined Chandra and RXTE pulsar spectrum is well fitted by an absorbed power-law model with column density N{sub H} = (1.7 {+-} 0.3) x 10{sup 22} cm{sup -2} and photon index {Gamma} = 1.0 {+-} 0.2; this implies that the Chandra point-source flux is virtually 100% pulsed. For a distance of 10 kpc, the X-ray luminosity of PSR J2022+3842 is L{sub X}(2-10 keV) = 7.0 x 10{sup 33} erg s{sup -1}. Despite being extraordinarily energetic, PSR J2022+3842 lacks a bright X-ray wind nebula and has an unusually low conversion efficiency of spin-down power to X-ray luminosity, L{sub X}/ E-dot = 5.9x10{sup -5}.

Arzoumanian, Z. [Center for Research and Exploration in Space Science and Technology and X-ray Astrophysics Laboratory, NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771 (United States); Gotthelf, E. V. [Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027 (United States); Ransom, S. M. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22901 (United States); Safi-Harb, S. [Canada Research Chair, Department of Physics and Astronomy, University of Manitoba, Winnipeg, MB, R3T 2N2 (Canada); Kothes, R.; Landecker, T. L., E-mail: Zaven.Arzoumanian@nasa.gov [National Research Council of Canada, Herzberg Institute of Astrophysics, Dominion Radio Astrophysical Observatory, Box 248, Penticton, BC, V2A 6J9 (Canada)

2011-09-20T23:59:59.000Z

431

We can do better than effective dose for estimating or comparing low-dose radiation risks  

E-Print Network (OSTI)

We can do better than effective dose for estimating or comparing low-dose radiation risks D of exposure to different radiation fields. More commonly these days, it is used to estimate or compare radi. Keywords: Low dose risk estimation; Effective dose; Flawed definition; Effective risk 1. INTRODUCTION

Brenner, David Jonathan

432

Eddy mean flow decomposition and eddy diffusivity estimates in the tropical Pacific Ocean  

E-Print Network (OSTI)

Eddy mean flow decomposition and eddy diffusivity estimates in the tropical Pacific Ocean: 2] Eddy diffusivity of the surface velocity field in the tropical Pacific Ocean was estimated using diffusivity estimates in the tropical Pacific Ocean: 2. Results, J. Geophys. Res., 107(C10), 3154, doi:10

433

Magnetic Fields in Gamma-Ray Bursts: A Short Racah Institute for Physics, The Hebrew University, Jerusalem, 91904 Israel  

E-Print Network (OSTI)

Magnetic Fields in Gamma-Ray Bursts: A Short Overview Tsvi Piran Racah Institute for Physics Abstract. Magnetic fields play a crucial role in the physics of Gamma-Ray Bursts (GRBs). Strong thirty years, after the discovery of Gamma-Ray bursts (GRBs) we have now a reasonable GRB model

Jensen, Grant J.

434

900-MHz NMR: Accelerating Scientific Discovery Scientific Innovation Through Integration  

E-Print Network (OSTI)

When the U.S. Department of Energy's (DOE's) Office of Biological and Environmental Research approved, the highest magnetic field available was 750 MHz. DOE's decision and the ultimate success of its 900-MHz NMR. Influencing collaborators In addition to advancing many fields of fundamental research, the high-quality data

435

Dynamic Control of Autonomous Quadrotor Flight in an Estimated Nitin Sydney, Brendan Smyth, and Derek A. Paley  

E-Print Network (OSTI)

Dynamic Control of Autonomous Quadrotor Flight in an Estimated Wind Field Nitin Sydney, Brendan operating in an estimated, spatially varying, turbulent wind field. The quadrotor dynamics include and external wind fields. To control the quadrotor we use a dynamic input/output feedback linearization

Shapiro, Benjamin

436

D-branes in overcritical electric fields  

Science Journals Connector (OSTI)

We collect some arguments for treating a D-brane with overcritical electric field as a well-posed initial condition for a D-brane decay. Within the field theoretical toy model of Minahan and Zwiebach we give an estimate for the condensates of the related infinite tower of tachyonic excitations.

Harald Dorn; Mario Salizzoni; Alessandro Torrielli

2006-01-25T23:59:59.000Z

437

Arun field  

SciTech Connect

The Arun field is a giant gas-condensate field operated by Mobil and Pertamina with over 20,000 acres of closure at the top of the Arun reservoir. A middle-shelf patch reef complex of early to middle Miocene age is the producing facies at the Arun field. About 1,100 ft of porous limestones, encased in shales, create a stratigraphic trap for overpressure hydrocarbons. Three main carbonate lithologies were encountered during the examination of over 4,300 ft of core; (1) a reef facies consisting of vuggy, coral encrusting, red-algal boundstones, (2) a near-reef facies consisting of foraminiferal, mixed-skeletal packstones with gravel-size coral fragments, and (3) an interreef lagoonal facies consisting of benthonic-foram packstones. Twenty-two species of corals have been identified from Arun reef facies; major reef-forming coals, listed in order of decreasing abundance, are Porites cf P. Lutes, Cyphastrea microphthalma, Astreopora myriophthalma, Styloconiella gunetheri, Porites solida, and Acropora ssp. The Arun reef is comprised of limestones (with minor amounts of dolomite). No shale beds occur in the sequence, and all carbonate facies are in communication. A pervasive microporosity, occurring throughout the Arun Limestone, results from meteoric alteration of original carbonate mud to form a microrhombic porosity that accounts for about three-fourths of the field's total porosity.

Jordan, C.F. Jr.; Abdullah, M.

1988-01-01T23:59:59.000Z

438

DISCOVERY OF A NEW AM CVn SYSTEM WITH THE KEPLER SATELLITE  

SciTech Connect

We report the discovery of a new AM CVn system on the basis of broadband photometry obtained with the Kepler satellite supplemented by ground-based optical spectroscopy. Initially retained on Kepler target lists as a potential compact pulsator, the blue object SDSS J190817.07+394036.4 (KIC 004547333) has turned out to be a high-state AM CVn star showing the He-dominated spectrum of its accretion disk significantly reddened by interstellar absorption. We constructed new grids of NLTE synthetic spectra for accretion disks in order to analyze our spectroscopic observations. From this analysis, we infer preliminary estimates of the rate of mass transfer, the inclination angle of the disk, and the distance to the system. The AM CVn nature of the system is also evident in the Kepler light curve, from which we extracted 11 secure periodicities. The luminosity variations are dominated by a basic periodicity of 938.507 s, likely to correspond to a superhump modulation. The light curve folded on the period of 938.507 s exhibits a pulse shape that is very similar to the superhump wavefront seen in AM CVn itself, which is a high-state system and the prototype of the class. Our Fourier analysis also suggests the likely presence of a quasi-periodic oscillation similar to those already observed in some high-state AM CVn systems. Furthermore, some very low-frequency, low-amplitude aperiodic photometric activity is likely present, which is in line with what is expected in accreting binary systems. Inspired by previous work, we further looked for and found some intriguing numerical relationships between the 11 secure detected frequencies, in the sense that we can account for all of them in terms of only three basic clocks. This is further evidence in favor of the AM CVn nature of the system.

Fontaine, G.; Brassard, P.; Dufour, P.; Bergeron, P. [Departement de Physique, Universite de Montreal, Succ. Centre-Ville, C.P. 6128, Montreal, QC H3C 3J7 (Canada); Green, E. M.; Hubeny, I.; Guvenen, B.; O'Malley, C. J. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Charpinet, S.; Van Grootel, V. [Laboratoire d'Astrophysique de Toulouse-Tarbes, Universite de Toulouse, CNRS, 14 av. E. Belin, 31400 Toulouse (France); Steeghs, D.; Marsh, T. R. [Department of Astrophysics, University of Warwick, Coventry CV4 7AL (United Kingdom); Aerts, C.; Oestensen, R. H.; Bloemen, S. [Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, B-3001 Leuven (Belgium); Randall, S. K. [European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching (Germany); Silvotti, R. [INAF-Osservatorio Astronomico di Torino, Strada dell'Osservatorio 20, 10025 Pino Torinese (Italy); Howell, S. B. [National Optical Astronomy Observatory, Tucson, AZ 85719 (United States); Baran, A. [Krakow Pedagogical University, ul. Podchorazych 2, 30-084 Krakow (Poland); Kepler, S. O., E-mail: fontaine@astro.umontreal.ca [Instituto de Fisica, Universidade Federal do Rio Grande do Sul, Porto Alegre, RS (Brazil)

2011-01-10T23:59:59.000Z

439

Estimating Biomass in the Mountain Regions of Bwindi Impenetrable National Park, Uganda using Radar and Optical Remote Sensing  

E-Print Network (OSTI)

Field measured estimates of aboveground biomass (AGB) for 15 transects in Bwindi Impenetrable National Park (BINP), Uganda were used to generate a number of prediction models for estimating aboveground biomass (AGB) over the full extent of BINP. AGB...

Fedrigo, Melissa

2009-11-26T23:59:59.000Z

440

Cost Estimating, Analysis, and Standardization  

Directives, Delegations, and Requirements

To establish policy and responsibilities for: (a) developing and reviewing project cost estimates; (b) preparing independent cost estimates and analysis; (c) standardizing cost estimating procedures; and (d) improving overall cost estimating and analytical techniques, cost data bases, cost and economic escalation models, and cost estimating systems. Cancels DOE O 5700.2B, dated 8-5-1983; DOE O 5700.8, dated 5-27-1981; and HQ 1130.1A, dated 12-30-1981. Canceled by DOE O 5700.2D, dated 6-12-1992

1984-11-02T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Discovery of new material state counterintuitive to laws of physics |  

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

"It's like squeezing a stone and forming a giant sponge," said Argonne chemist Karena Chapman. "Materials are supposed to become denser and more compact under pressure. We are seeing the exact opposite." To view a larger version of the image, click on it. "It's like squeezing a stone and forming a giant sponge," said Argonne chemist Karena Chapman. "Materials are supposed to become denser and more compact under pressure. We are seeing the exact opposite." To view a larger version of the image, click on it. "It's like squeezing a stone and forming a giant sponge," said Argonne chemist Karena Chapman. "Materials are supposed to become denser and more compact under pressure. We are seeing the exact opposite." To view a larger version of the image, click on it. Discovery of new material state counterintuitive to laws of physics By Tona Kunz * June 11, 2013 Tweet EmailPrint LEMONT, Ill. - When you squeeze something, it gets smaller. Unless you're at Argonne National Laboratory.

442

Discovery of a Massive Protostar near IRAS 18507+0121  

E-Print Network (OSTI)

We have observed the massive star forming region, IRAS 18507+0121, at millimeter wavelengths in 3 mm continuum emission and H13CO+(J=1-0) and SiO(v=0, J=2-1) line emission, and at near-infrared wavelengths between 1.2 and 2.1 microns. Two compact molecular cores are detected: one north and one south separated by about 40". The northern molecular core contains a newly discovered, deeply embedded, B2 protostar surrounded by several hundred solar masses of warm gas and dust, G34.4+0.23 MM. Based on the presence of warm dust emission and the lack of detection at near-infrared wavelengths, we suggest that G34.4+0.23 MM may represent the relatively rare discovery of a massive protostar (e.g. analogous to a low-mass "Class 0" protostar). The southern molecular core is associated with a near-infrared cluster of young stars and an ultracompact (UC) HII region, G34.4+0.23, with a central B0.5 star. The fraction of near-infrared stars with excess infrared emission indicative of circumstellar material is greater than 50% which suggests an upper limit on the age of the IRAS 18507+0121 star forming region of 3 Myrs.

D. S. Shepherd; D. E. A. Nurnberger; L. Bronfman

2003-10-27T23:59:59.000Z

443

Discovery of a Radio Flare from GRB 990123  

E-Print Network (OSTI)

We report the discovery of a radio counterpart to GRB 990123. In contrast to previous well-studied radio afterglows which rise to peak flux on a timescale of a week and then decay over several weeks to months, the radio emission from this GRB was clearly detected one day after the burst, after which it rapidly faded away. The simplest interpretation of this ``radio flare'' is that it arises from the reverse shock. In the framework of the afterglow models discussed to date, a forward shock origin for the flare is ruled out by our data. However, at late times, some radio afterglow emission (commensurate with the observed late-time optical emission, the optical afterglow) is expected from the forward shock. The relative faintness of the observed late-time radio emission provides an independent indication for a jet-like geometry in this GRB. We use the same radio observations to constrain two key parameters of the forward shock, peak flux and peak frequency, to within a factor of two. These values are inconsistent with the notion advocated by several authors that the prompt optical emission detected by ROTSE smoothly joins the optical afterglow emission. Finally, with hindsight we now recognize another such radio flare and this suggests that one out of eight GRBs has a detectable radio flare. This abundance coupled with the reverse shock interpretation suggests that the radio flare phenomenon has the potential to shed new light into the physics of reverse shocks in GRBs.

S. R. Kulkarni; D. A. Frail; R. Sari; G. H. Moriarty-Schieven; D. S. Shepherd; P. Udomprasert; A. C. S. Readhead; J. S. Bloom; M. Feroci; E. Costa

1999-03-30T23:59:59.000Z

444

THE DISCOVERY OF PULSATING HOT SUBDWARFS IN NGC 2808  

SciTech Connect

We present the results of a Hubble Space Telescope program to search for pulsating hot subdwarfs in the core of NGC 2808. These observations were motivated by the recent discovery of such stars in the outskirts of ? Cen. Both NGC 2808 and ? Cen are massive globular clusters exhibiting complex stellar populations and large numbers of extreme horizontal branch stars. Our far-UV photometric monitoring of over 100 hot evolved stars has revealed six pulsating subdwarfs with periods ranging from 85 to 149 s and UV amplitudes of 2.0%-6.8%. In the UV color-magnitude diagram of NGC 2808, all six of these stars lie immediately below the canonical horizontal branch, a region populated by the subluminous 'blue-hook' stars. For three of these six pulsators, we also have low-resolution far-UV spectroscopy that is sufficient to broadly constrain their atmospheric abundances and effective temperatures. Curiously, and in contrast to the ? Cen pulsators, the NGC 2808 pulsators do not exhibit the spectroscopic or photometric uniformity one might expect from a well-defined instability strip, although they all fall within a narrow band (0.2 mag) of far-UV luminosity.

Brown, Thomas M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)] [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Landsman, Wayne B. [Adnet Systems, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Adnet Systems, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Randall, Suzanna K. [European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei Mnchen (Germany)] [European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei Mnchen (Germany); Sweigart, Allen V. [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Lanz, Thierry, E-mail: tbrown@stsci.edu, E-mail: Wayne.Landsman@nasa.gov, E-mail: srandall@eso.org, E-mail: allen.sweigart@gmail.com, E-mail: Thierry.Lanz@oca.eu [Laboratoire Lagrange, UMR7293, Universit de Nice Sophia-Antipolis, CNRS, Observatoire de la Cte dAzur, F-06304 Nice (France)] [Laboratoire Lagrange, UMR7293, Universit de Nice Sophia-Antipolis, CNRS, Observatoire de la Cte dAzur, F-06304 Nice (France)

2013-11-10T23:59:59.000Z

445

Knowledge Discovery and Data Mining (KDDM) survey report.  

SciTech Connect

The large number of government and industry activities supporting the Unit of Action (UA), with attendant documents, reports and briefings, can overwhelm decision-makers with an overabundance of information that hampers the ability to make quick decisions often resulting in a form of gridlock. In particular, the large and rapidly increasing amounts of data and data formats stored on UA Advanced Collaborative Environment (ACE) servers has led to the realization that it has become impractical and even impossible to perform manual analysis leading to timely decisions. UA Program Management (PM UA) has recognized the need to implement a Decision Support System (DSS) on UA ACE. The objective of this document is to research the commercial Knowledge Discovery and Data Mining (KDDM) market and publish the results in a survey. Furthermore, a ranking mechanism based on UA ACE-specific criteria has been developed and applied to a representative set of commercially available KDDM solutions. In addition, an overview of four R&D areas identified as critical to the implementation of DSS on ACE is provided. Finally, a comprehensive database containing detailed information on surveyed KDDM tools has been developed and is available upon customer request.

Phillips, Laurence R.; Jordan, Danyelle N.; Bauer, Travis L.; Elmore, Mark T. (Oak Ridge National Laboratory, Oak Ridge, TN); Treadwell, Jim N. (Oak Ridge National Laboratory, Oak Ridge, TN); Homan, Rossitza A.; Chapman, Leon Darrel; Spires, Shannon V.

2005-02-01T23:59:59.000Z

446

Discovery of hot supergiant stars near the Galactic center  

E-Print Network (OSTI)

We report new results of a campaign to find Wolf-Rayet and O (WR/O) stars and high-mass X-ray binaries (HMXBs) in the Galactic center. We searched for candidates by cross-correlating the 2MASS catalog with a deep Chandra catalog of X-ray point sources in the Radio Arches region. Following up with K-band spectroscopy, we found two massive stellar counterparts to CXOGC J174555.3-285126 and CXOGC J174617.0-285131, which we classify as a broad-lined WR star of sub-type WN6b and an O Ia supergiant, respectively. Their X-ray properties are most consistent with those of known colliding-wind binaries in the Galaxy and the Large Magellanic Cloud, although a scenario involving low-rate accretion onto a compact object is also possible. The O Ia star lies 4.4 pc in projection from the Quintuplet cluster, and has a radial velocity consistent with that of the Quintuplet, suggesting that this star might have escaped from the cluster. We also present the discovery of a B2 Ia supergiant, which we identified as a candidate massive star using 8 micron Spitzer maps of the Galactic center in a region near the known massive X-ray-emitting star CXOGC J174516.1-290315. We discuss the origin of these stars in the context of evolving stellar clusters in the Galactic center.

Jon C. Mauerhan; Michael P. Muno; Mark Morris

2007-03-08T23:59:59.000Z

447

DISCOVERY OF THE PIGTAIL MOLECULAR CLOUD IN THE GALACTIC CENTER  

SciTech Connect

This paper reports the discovery of a helical molecular cloud in the central molecular zone (CMZ) of our Galaxy. This 'pigtail' molecular cloud appears at (l, b, V{sub LSR}) {approx_equal} (-0.{sup 0}7, + 0.{sup 0}0, - 70 to -30 km s{sup -1}), with a spatial size of {approx}20 Multiplication-Sign 20 pc{sup 2} and a mass of (2-6) Multiplication-Sign 10{sup 5} M{sub Sun }. This is the third helical gaseous nebula found in the Galactic center region to date. Line intensity ratios indicate that the pigtail molecular cloud has slightly higher temperature and/or density than the other normal clouds in the CMZ. We also found a high-velocity wing emission near the footpoint of this cloud. We propose a formation model of the pigtail molecular cloud. It might be associated with a magnetic tube that is twisted and coiled because of the interaction between clouds in the innermost x{sub 1} orbit and ones in the outermost x{sub 2} orbit.

Matsumura, Shinji; Oka, Tomoharu; Tanaka, Kunihiko [Institute of Science and Technology, Keio University, 3-14-1 Hiyoshi, Yokohama, Kanagawa 223-8522 (Japan); Nagai, Makoto [Institute of Physics, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571 (Japan); Kamegai, Kazuhisa [Institute of Science and Technology, Tokyo University of Science, 2641 Yamazaki, Noda, Chiba (Japan); Hasegawa, Tetsuo [Joint ALMA Observatory, El Golf 40, Piso 18, Las Condes, Santiago (Chile)

2012-09-01T23:59:59.000Z

448

Discovery of a Neutron Star Oscillation Mode During a Superburst  

E-Print Network (OSTI)

Neutron stars are among the most compact objects in the universe and provide a unique laboratory for the study of cold ultra-dense matter. While asteroseismology can provide a powerful probe of the interiors of stars, for example, helioseismology has provided unprecedented insights about the interior of the sun, comparable capabilities for neutron star seismology have not yet been achieved. Here we report the discovery of a coherent X-ray modulation from the neutron star 4U 1636-536 during the February 22, 2001 thermonuclear superburst seen with NASA's Rossi X-ray Timing Explorer (RXTE) that is very likely produced by a global oscillation mode. The observed frequency is 835.6440 +- 0.0002 Hz (1.43546 times the stellar spin frequency of 582.14323 Hz) and the modulation is well described by a sinusoid ( A + Bsin(p - p0) ) with fractional half-amplitude of B/A = 0.19 +- 0.04% (4-15 keV). The observed frequency is consistent with the expected inertial frame frequency of a rotationally-modified surface g-mode, an ...

Strohmayer, Tod

2014-01-01T23:59:59.000Z

449

Biofuel Enduse Datasets from the Bioenergy Knowledge Discovery Framework (KDF)  

DOE Data Explorer (OSTI)

The Bioenergy Knowledge Discovery Framework invites users to discover the power of bioenergy through an interface that provides extensive access to research data and literature, GIS mapping tools, and collaborative networks. The Bioenergy KDF supports efforts to develop a robust and sustainable bioenergy industry. The KDF facilitates informed decision making by providing a means to synthesize, analyze, and visualize vast amounts of information in a relevant and succinct manner. It harnesses Web 2.0 and social networking technologies to build a collective knowledge system that can better examine the economic and environmental impacts of development options for biomass feedstock production, biorefineries, and related infrastructure. [copied from https://www.bioenergykdf.net/content/about]

Holdings include datasets, models, and maps. This is a very new resource, but the collections will grow due to both DOE contributions and individuals data uploads. Currently the Biofuel Enduse collection includes 133 items. Most of these are categorized as literature, but 36 are listed as datasets and ten as models.

450

Germanium: From Its Discovery to SiGe Devices  

SciTech Connect

Germanium, element No.32, was discovered in 1886 by Clemens Winkler. Its first broad application was in the form of point contact Schottky diodes for radar reception during WWII. The addition of a closely spaced second contact led to the first all-solid-state electronic amplifier device, the transistor. The relatively low bandgap, the lack of a stable oxide and large surface state densities relegated germanium to the number 2 position behind silicon. The discovery of the lithium drift process, which made possible the formation of p-i-n diodes with fully depletable i-regions several centimeters thick, led germanium to new prominence as the premier gamma-ray detector. The development of ultra-pure germanium yielded highly stable detectors which have remained unsurpassed in their performance. New acceptors and donors were discovered and the electrically active role of hydrogen was clearly established several years before similar findings in silicon. Lightly doped germanium has found applications as far infrared detectors and heavily Neutron Transmutation Doped (NTD) germanium is used in thermistor devices operating at a few milliKelvin. Recently germanium has been rediscovered by the silicon device community because of its superior electron and hole mobility and its ability to induce strains when alloyed with silicon. Germanium is again a mainstream electronic material.

Haller, E.E.

2006-06-14T23:59:59.000Z

451

DISCOVERY OF A NEW MEMBER OF THE INNER OORT CLOUD FROM THE NEXT GENERATION VIRGO CLUSTER SURVEY  

SciTech Connect

We report the discovery of 2010 GB{sub 174}, a likely new member of the Inner Oort Cloud (IOC). 2010 GB{sub 174} is 1 of 91 trans-Neptunian objects and Centaurs discovered in a 76 deg{sup 2} contiguous region imaged as part of the Next Generation Virgo Cluster Survey (NGVS)a moderate ecliptic latitude survey reaching a mean limiting magnitude of g' ? 25.5using MegaPrime on the 3.6 m Canada-France-Hawaii Telescope. 2010 GB{sub 174} is found to have an orbit with a semi-major axis of a ? 350.8 AU, an inclination of i ? 21.6, and a pericenter of q ? 48.5 AU. This is the second largest perihelion distance among known solar system objects. Based on the sky coverage and depth of the NGVS, we estimate the number of IOC members with sizes larger than 300 km (H{sub V} ? 6.2 mag) to be ? 11, 000. A comparison of the detection rate from the NGVS and the PDSSS (a characterized survey that 'rediscovered' the IOC object Sedna) gives, for an assumed a power-law luminosity function for IOC objects, a slope of ? ? 0.7 0.2. With only two detections in this region this slope estimate is highly uncertain.

Chen, Ying-Tung; Ip, Wing-Huen [Institute of Astronomy, National Central University, No. 300, Jhongda Road, Jhongli City, Taoyuan County 32001, Taiwan (China)] [Institute of Astronomy, National Central University, No. 300, Jhongda Road, Jhongli City, Taoyuan County 32001, Taiwan (China); Kavelaars, J. J.; Gwyn, Stephen; Ferrarese, Laura; Ct, Patrick [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC V9E 2E7 (Canada)] [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC V9E 2E7 (Canada); Jordn, Andrs; Suc, Vincent [Instituto de Astrofsica, Pontificia Universidad Catlica de Chile, Av. Vicua Mackenna 4860, Macul 7820436, Santiago (Chile)] [Instituto de Astrofsica, Pontificia Universidad Catlica de Chile, Av. Vicua Mackenna 4860, Macul 7820436, Santiago (Chile); Cuillandre, Jean-Charles, E-mail: charles@astro.ncu.edu.tw [Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Hwy., Kamuela, HI 96743 (United States)] [Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Hwy., Kamuela, HI 96743 (United States)

2013-09-20T23:59:59.000Z

452

Electric and Magnetic Fields (EMF) RAPID Engineering Program, Project 7: Development of Field Exposure Models  

SciTech Connect

The purpose of this project was to develop a conceptual model for estimating magnetic field (EMF) personal exposure (PE) of individuals or groups and construct a working model using existing data.

Bracken, T.D.; Rankin, R.F.; Wiley, J.A.

1999-05-01T23:59:59.000Z

453

Estimate steam-turbine losses to justify maintenance funds  

SciTech Connect

A procedure to estimate steam-turbine losses is described. The estimates are based on analytical calculations and field inspections of turbines with known performance deterioration resulting from their environment, not their construction. They are, therefore, applicable to many types of steam turbines. Common causes of deterioration are the following: solid particle erosion, deposits, increased clearances, and peening or damage from foreign material. Performance losses due to these factors are analyzed. An example of application is given.

Not Available

1982-05-01T23:59:59.000Z

454

Estimating demolition cost of plutonium buildings for dummies  

SciTech Connect

The primary purpose of the Rocky Flats Field Office of the US Department of Energy is to decommission the entire plant. In an effort to improve the basis and the accuracy of the future decommissioning cost, Rocky Flats has developed a powerful but easy-to-use tool to determine budget cost estimates to characterize, decontaminate, and demolish all its buildings. The parametric cost-estimating tool is called the Facilities Disposition Cost Model (FDCM).

Tower, S.E.

2000-07-01T23:59:59.000Z

455

Catalogue of Minor Planet Names and Discovery Circumstances  

Science Journals Connector (OSTI)

Smiley not only worked on the field of minor planet dynamics. He led 14 solar eclipse expeditions, in Peru, Canada, Brazil, Thailand, Pakistan, and the ... published in J.R. Astron. Soc. Canada, Vol. 72, p. 4647...

Lutz D. Schmadel

2014-09-01T23:59:59.000Z

456

Materials Discovery Design and Synthesis | U.S. DOE Office of Science (SC)  

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

Discovery Design and Synthesis Discovery Design and Synthesis Materials Sciences and Engineering (MSE) Division MSE Home About Research Areas Energy Frontier Research Centers (EFRCs) DOE Energy Innovation Hubs BES Funding Opportunities The Computational Materials and Chemical Sciences Network (CMCSN) Theoretical Condensed Matter Physics Scientific Highlights Reports and Activities Principal Investigators' Meetings BES Home Research Areas Materials Discovery Design and Synthesis Print Text Size: A A A RSS Feeds FeedbackShare Page Research is supported in the discovery and design of novel materials and the development of innovative materials synthesis and processing methods. This research is guided by applications of concepts learned from the interface between physics and biology and from nano-scale understanding of

457

Global Discovery introduced at AAAS 2006 | OSTI, US Dept of Energy, Office  

Office of Scientific and Technical Information (OSTI)

Global Discovery introduced at AAAS 2006 Global Discovery introduced at AAAS 2006 The Office of Scientific and Technical Information (OSTI) was a key participant in the symposium, Global Discovery on the Internet, at the American Association for the Advancement of Science (AAAS) 2006 Annual Meeting Feb. 16-20 in St. Louis, MO. The symposium introduced Global Discovery, which promises to increase the pace of science by searching all scientific communities at once for data, information, or methodological advances. "Imagine a Google-like search capability that returns results across the whole of science, giving scientists information on research they didn't even know existed," said Dr. Walter Warnick, director. "Except that this search would go further than traditional search engines. Rather than

458

Discovery of oxygen in atmosphere could mean life for Saturn's moon Dione  

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

Discovery of oxygen in atmosphere could mean life for Saturn's Discovery of oxygen in atmosphere could mean life for Saturn's moon Dione Discovery of oxygen in atmosphere could mean life for Saturn's moon Dione Discovery could mean ingredients for life are abundant on icy space bodies. March 5, 2012 Curiosity rover bears three LANL technologies Inside Titan: This artist's concept shows a possible scenario for the internal structure of Titan, as suggested by data from NASA's Cassini spacecraft. Scientists have been trying to determine what is under Titan's organic-rich atmosphere and icy crust. Data from the radio science experiment make the strongest case yet for a global subsurface ocean, sitting above a subsurface layer of high-pressure ice and a water-infused silicate core. Image credit: A. Tavani Get Expertise

459

What Was Your Surprising Energy-Saving Discovery? | Department of Energy  

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

Was Your Surprising Energy-Saving Discovery? Was Your Surprising Energy-Saving Discovery? What Was Your Surprising Energy-Saving Discovery? January 21, 2010 - 7:30am Addthis On Monday, Amy told you how her dog, Matilda, revealed that they were losing a lot of heated air from ducts damaged by a sleepy cat. Sometimes luck (like Matilda's unexpected heroics) or just a little spontaneous detective work can show potential energy savings in surprising places. What was your surprising energy-saving discovery? Each Thursday, you have the chance to share your thoughts on a question about energy efficiency or renewable energy for consumers. E-mail your responses to the Energy Saver team at consumer.webmaster@nrel.gov Addthis Related Articles Navigating the New EnergySaver.gov Our Dog Discovered Our Ducts Have Cats

460

Abstract 3728: A discovery platform for allosteric modulators of c-Abl kinase function  

Science Journals Connector (OSTI)

...discovery informatics platform allowing systematic target...of effects of RNAi and chemical screens on different...multidisciplinary cancer platform, canSAR (http...datapoints ranging from chemical and RNAi screening...

Prerna Grover and Thomas E. Smithgall

2014-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "field discoveries estimated" 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

Impact of Recent Discoveries on Petroleum and Natural Gas Exploration: Emphasis on India  

E-Print Network (OSTI)

Two discoveries have greatly impacted understanding relevant to the origination and emplacement of petroleum and natural gas deposits. One discovery, pertaining to hydrocarbon formation from methane broadens significantly potential regions where abiotic petroleum and natural gas deposits might be found. The other, discovery of the physical impossibility of Earth-mantle convection, restricts the range and domain of geodynamic behavior, and leads to new insights on the formation of petroleum and natural gas deposits. This article highlights the impact and implications of those discoveries, especially as they relate to petroleum and natural gas exploration in India and throughout the world. From the reasoning developed here, the generality of the considerations involved, the understanding developed with respect to the East African Rift System, and the experience garnered from the larger and older Siberian Traps, the prognosis and potential for the region beneath the Deccan Traps of India to eventually become a major source of petroleum and natural gas seems quite favorable.

J. Marvin Herndon

2010-03-23T23:59:59.000Z

462

Discovery of Genes and Genomes through Deep Metagenomic Sequencing of Cow Rumen (2010 JGI User Meeting)  

ScienceCinema (OSTI)

Director Eddy Rubin on "Discovery of Genes and Genomes through Deep Metagenomic Sequencing of Cow Rumen" on March 25, 2010 at the 5th Annual DOE JGI User Meeting

Rubin, Eddy

2011-04-25T23:59:59.000Z

463

Impact of Recent Discoveries on Petroleum and Natural Gas Exploration: Emphasis on India  

E-Print Network (OSTI)

Two discoveries have greatly impacted understanding relevant to the origination and emplacement of petroleum and natural gas deposits. One discovery, pertaining to hydrocarbon formation from methane broadens significantly potential regions where abiotic petroleum and natural gas deposits might be found. The other, discovery of the physical impossibility of Earth-mantle convection, restricts the range and domain of geodynamic behavior, and leads to new insights on the formation of petroleum and natural gas deposits. This article highlights the impact and implications of those discoveries, especially as they relate to petroleum and natural gas exploration in India and throughout the world. From the reasoning developed here, the generality of the considerations involved, the understanding developed with respect to the East African Rift System, and the experience garnered from the larger and older Siberian Traps, the prognosis and potential for the region beneath the Deccan Traps of India to eventually become a m...

Herndon, J Marvin

2010-01-01T23:59:59.000Z

464

Knowledge Discovery, Knowledge Management and Enterprise-Wide Information Technology Tools Final Report  

SciTech Connect

A final report on an ORNL task to establish a knowledge discovery and management tool to retrieve and recommend information from existing S&T documents for the Office of Naval Research Global.

Patton, Robert M [ORNL; Symons, Christopher T [ORNL; Gorman, Bryan L [ORNL; Treadwell, Jim N [ORNL

2012-04-01T23:59:59.000Z

465

Metagenomics for Etiologic Agent Discovery (Seventh Annual Sequencing, Finishing, Analysis in the Future (SFAF) Meeting 2012)  

ScienceCinema (OSTI)

Matthew Ross on "Metagenomics for etiological agent discovery" at the 2012 Sequencing, Finishing, Analysis in the Future Meeting held June 5-7, 2012 in Santa Fe, New Mexico.

Ross, Matthew [Baylor College of Medicine

2013-02-11T23:59:59.000Z

466

An empirical analysis of the price discovery function of Shanghai fuel oil futures market  

Science Journals Connector (OSTI)

This paper analyzes the role of price discovery of Shanghai fuel oil futures market by using methods, such ... there exists a strong relationship between the spot price of Huangpu fuel oil spot market and the fut...

Zhen Wang; Zhenhai Liu; Chao Chen

2007-08-01T23:59:59.000Z

467

Systematic Discovery of TLR Signaling Components Delineates Viral-Sensing Circuits  

E-Print Network (OSTI)

Deciphering the signaling networks that underlie normal and disease processes remains a major challenge. Here, we report the discovery of signaling components involved in the Toll-like receptor (TLR) response of immune ...

Chevrier, Nicolas

468

Discovery & Innovation | U.S. DOE Office of Science (SC)  

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

Innovation Innovation Discovery & Innovation Stories of Discovery & Innovation Brief Science Highlights SBIR/STTR Highlights Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Joint Bioenergy Institute Joint Bioenergy Institute Lawrence Berkeley National Laboratory Print Text Size: A A A Subscribe FeedbackShare Page Stories of Discovery & Innovation The photosynthetic megacomplex from a cyanobacterium. 12.30.13Stories of Discovery & Innovation Observing the Sparks of Life EFRC researchers isolate a photosynthetic complex - arguably the most important bit of organic chemistry on the planet - in its complete functioning state. Read More » Scanning electron microscope image of sulfur graphene oxide.

469

Exploration And Discovery In Yellowstone Lake- Results From High-Resolution  

Open Energy Info (EERE)

Exploration And Discovery In Yellowstone Lake- Results From High-Resolution Exploration And Discovery In Yellowstone Lake- Results From High-Resolution Sonar Imaging, Seismic Reflection Profiling, And Submersible Studies Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Journal Article: Exploration And Discovery In Yellowstone Lake- Results From High-Resolution Sonar Imaging, Seismic Reflection Profiling, And Submersible Studies Details Activities (1) Areas (1) Regions (0) Abstract: No portion of the American continent is perhaps so rich in wonders as the Yellow Stone' (F.V. Hayden, September 2, 1874) Discoveries from multi-beam sonar mapping and seismic reflection surveys of the northern, central, and West Thumb basins of Yellowstone Lake provide new insight into the extent of post-collapse volcanism and active hydrothermal

470

GRR/Section 11-WA-c - Archaeological Resource Discovery Process | Open  

Open Energy Info (EERE)

GRR/Section 11-WA-c - Archaeological Resource Discovery Process GRR/Section 11-WA-c - Archaeological Resource Discovery Process < GRR Jump to: navigation, search GRR-logo.png GEOTHERMAL REGULATORY ROADMAP Roadmap Home Roadmap Help List of Sections Section 11-WA-c - Archaeological Resource Discovery Process 11-WA-c - Archaeological Resource Discovery Process.pdf Click to View Fullscreen Triggers None specified In the state of Washington, cultural resource concerns are integrated as early as possible into the planning for capital projects and are protected if discovered during construction. Washington defines "Cultural resources" as archeological and historical sites and artifacts, and traditional areas or items of religious, ceremonial and social uses to affected tribes. Washington defines an "Archaeological resource" as any

471

Department of Engineering Sciences and Mechanics Spring 2012 Discovery Space Pendulum Exhibit  

E-Print Network (OSTI)

PENNSTATE Department of Engineering Sciences and Mechanics Spring 2012 Discovery Space Pendulum, a timer (counting in seconds) and an audio circuit in addition to the mechanics. In addition, the exhibit

Demirel, Melik C.

472

Nevada Field Office  

National Nuclear Security Administration (NNSA)

about NNSS

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473

Technology development for gene discovery and full-length sequencing  

SciTech Connect

In previous years, with support from the U.S. Department of Energy, we developed methods for construction of normalized and subtracted cDNA libraries, and constructed hundreds of high-quality libraries for production of Expressed Sequence Tags (ESTs). Our clones were made widely available to the scientific community through the IMAGE Consortium, and millions of ESTs were produced from our libraries either by collaborators or by our own sequencing laboratory at the University of Iowa. During this grant period, we focused on (1) the development of a method for preferential cloning of tissue-specific and/or rare transcripts, (2) its utilization to expedite EST-based gene discovery for the NIH Mouse Brain Molecular Anatomy Project, (3) further development and optimization of a method for construction of full-length-enriched cDNA libraries, and (4) modification of a plasmid vector to maximize efficiency of full-length cDNA sequencing by the transposon-mediated approach. It is noteworthy that the technology developed for preferential cloning of rare mRNAs enabled identification of over 2,000 mouse transcripts differentially expressed in the hippocampus. In addition, the method that we optimized for construction of full-length-enriched cDNA libraries was successfully utilized for the production of approximately fifty libraries from the developing mouse nervous system, from which over 2,500 full-ORF-containing cDNAs have been identified and accurately sequenced in their entirety either by our group or by the NIH-Mammalian Gene Collection Program Sequencing Team.

Marcelo Bento Soares

2004-07-19T23:59:59.000Z

474

DISCOVERY OF A SIGNIFICANT MAGNETIC CATACLYSMIC VARIABLE POPULATION IN THE LIMITING WINDOW  

SciTech Connect

We have discovered 10 periodic X-ray sources from the 1 Ms Chandra ACIS observation of the Limiting Window (LW), a low-extinction region (A{sub V} {approx} 3.9) at 1.{sup 0}4 south of the Galactic center. The observed periods ({approx}1.3-3.4 hr) and the X-ray luminosities (10{sup 31.8-32.9} erg s{sup -1} at 8 kpc) of the 10 periodic sources, combined with the lack of bright optical counterparts and thus high X-ray-to-optical flux ratios, suggest that they are likely accreting binaries, in particular, magnetic cataclysmic variables (MCVs). All of them exhibit a relatively hard X-ray spectrum ({Gamma} < 2 for a power-law model), and relatively high extinction observed in the X-ray spectra of at least five sources indicates some intrinsic absorption in the system, which is also a typical sign of MCVs. On close inspection, the period distribution of these sources resembles those of polars, whereas the relatively hard spectra suggest that they could be intermediate polars (IPs). These puzzling properties can be explained by unusual polars with buried magnetic fields or a rare sub-class of MCVs, nearly synchronous MCVs. These unusual MCVs may provide important clues in the evolutionary path of MCVs from IPs to polars. The completeness simulation indicates that {approx}>40% of the hard X-ray sources in the LW are periodic. Therefore, this discovery provides a first direct evidence of a large MCV population in the bulge and further supports the current view that MCVs constitute the majority of low-luminosity hard X-ray sources ({approx}10{sup 30-33} erg s{sup -1}) in the bulge.

Hong, JaeSub; Grindlay, Jonathan E.; Servillat, Mathieu; Zhao Ping [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Van den Berg, Maureen, E-mail: jaesub@head.cfa.harvard.edu [Astronomical Institute, Utrecht University, Princetonplein 5, Utrecht, 3508 TA (Netherlands)

2012-02-20T23:59:59.000Z

475

DISCOVERY OF THE Y1 DWARF WISE J064723.23623235.5  

SciTech Connect

We present the discovery of a very cold, very low mass, nearby brown dwarf using data from the NASA Wide-field Infrared Survey Explorer (WISE). The object, WISE J064723.23623235.5, has a very red WISE color of W1W2 > 3.77 mag and a very red Spitzer Space Telescope color of ch1ch2 = 2.82 0.09 mag. In J{sub MKO} ch2 color (7.58 0.27 mag) it is one of the two or three reddest brown dwarfs known. Our grism spectrum from the Hubble Space Telescope (HST) confirms it to be the seventeenth Y dwarf discovered, and its spectral type of Y1 0.5 makes it one of the four latest-type Y dwarfs classified. Astrometric imaging from Spitzer and HST, combined with data from WISE, provides a preliminary parallax of ? = 115 12 mas (d = 8.7 0.9 pc) and proper motion of ? = 387 25 mas yr{sup 1} based on 2.5 yr of monitoring. The spectrum implies a blue JH color, for which model atmosphere calculations suggest a relatively low surface gravity. The best fit to these models indicates an effective temperature of 350-400 K and a mass of ?5-30 M{sub Jup}. Kinematic analysis hints that this object may belong to the Columba moving group, which would support an age of ?30 Myr and thus an even lower mass of <2 M{sub Jup}, but verification would require a radial velocity measurement not currently possible for a J = 22.7 mag brown dwarf.

Kirkpatrick, J. Davy; Gelino, Christopher R.; Beichman, Charles A.; Mace, Gregory N. [Infrared Processing and Analysis Center, MS 100-22, California Institute of Technology, Pasadena, CA 91125 (United States); Cushing, Michael C.; Schneider, Adam [Department of Physics and Astronomy, MS 111, University of Toledo, 2801 West Bancroft Street, Toledo, OH 43606-3328 (United States); Tinney, C. G. [School of Physics, University of New South Wales, Sydney, NSW 2052 (Australia); Faherty, Jacqueline K., E-mail: davy@ipac.caltech.edu [Department of Astronomy, University of Chile, Camino El Observatorio 1515, Casilla 36-D Santiago (Chile)

2013-10-20T23:59:59.000Z

476

ON THE RELIABILITY OF POLARIZATION ESTIMATION USING ROTATION MEASURE SYNTHESIS  

SciTech Connect

We benchmark the reliability of the rotation measure (RM) synthesis algorithm using the 1005 Centaurus A field sources of Feain et al. The RM synthesis solutions are compared with estimates of the polarization parameters using traditional methods. This analysis provides verification of the reliability of RM synthesis estimates. We show that estimates of the polarization parameters can be made at lower signal-to-noise ratio (S/N) if the range of RMs is bounded, but reliable estimates of individual sources with unusual RMs require unconstrained solutions and higher S/N. We derive from first principles the statistical properties of the polarization amplitude associated with RM synthesis in the presence of noise. The amplitude distribution depends explicitly on the amplitude of the underlying (intrinsic) polarization signal. Hence, it is necessary to model the underlying polarization signal distribution in order to estimate the reliability and errors in polarization parameter estimates. We introduce a Bayesian method to derive the distribution of intrinsic amplitudes based on the distribution of measured amplitudes. The theoretically derived distribution is compared with the empirical data to provide quantitative estimates of the probability that an RM synthesis solution is correct as a function of S/N. We provide quantitative estimates of the probability that any given RM synthesis solution is correct as a function of measured polarized amplitude and the intrinsic polarization amplitude compared to the noise.

Macquart, J.-P.; Ekers, R. D. [ICRAR/Curtin University of Technology, Bentley, WA 6845 (Australia); Feain, I. [CSIRO Astronomy and Space Science, P.O. Box 76, Epping, NSW 1710 (Australia); Johnston-Hollitt, M., E-mail: J.Macquart@curtin.edu.au [School of Chemical and Physical Sciences, Victoria University of Wellington, P.O. Box 600, Wellington 6140 (New Zealand)

2012-05-10T23:59:59.000Z

477

Examples of Cost Estimation Packages  

Directives, Delegations, and Requirements

Estimates can be performed in a variety of ways. Some of these are for projects for an undefined scope, a conventional construction project, or where there is a level of effort required to complete the work. Examples of cost estimation packages for these types of projects are described in this appendix.

1997-03-28T23:59:59.000Z

478

5, 30473104, 2005 Estimates of  

E-Print Network (OSTI)

parametrisations, one relating convective preciptation (CP scheme) to lightning flash15 distributionsACPD 5, 3047­3104, 2005 Estimates of lightning NOx production K. F. Boersma et al. Title Page Discussions Estimates of lightning NOx production from GOME satellite observations K. F. Boersma, H. J. Eskes

Paris-Sud XI, Université de

479

Energy Expenditure Estimation DEMO Application  

E-Print Network (OSTI)

of accelerometry. An average smart phone contains an inertial sensor and today we hardly leave our home without itEnergy Expenditure Estimation DEMO Application Bozidara Cvetkovi´c1,2 , Simon Kozina1,2 , Bostjan://www.mps.si Abstract. The paper presents two prototypes for the estimation of hu- man energy expenditure during normal

Lu?trek, Mitja

480

Hybrid Recursive Energy-based Method for Robust Optical Flow on Large Motion Fields  

E-Print Network (OSTI)

Hybrid Recursive Energy-based Method for Robust Optical Flow on Large Motion Fields Jangheon Kim for optical flow estimation. The method efficiently combines the advantage of discrete motion estimation and optical flow estimation in a recursive block-to-pixel estimation scheme. Integrated local and global

Wichmann, Felix

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481

Mercury: An Example of Effective Software Reuse for Metadata Management, Data Discovery and Access  

SciTech Connect

Mercury is a federated metadata harvesting, data discovery and access tool based on both open source packages and custom developed software. Though originally developed for NASA, the Mercury development consortium now includes funding from NASA, USGS, and DOE. Mercury supports the reuse of metadata by enabling searching across a range of metadata specification and standards including XML, Z39.50, FGDC, Dublin-Core, Darwin-Core, EML, and ISO-19115. Mercury provides a single portal to information contained in distributed data management systems. It collects metadata and key data from contributing project servers distributed around the world and builds a centralized index. The Mercury search interfaces then allow the users to perform simple, fielded, spatial and temporal searches across these metadata sources. One of the major goals of the recent redesign of Mercury was to improve the software reusability across the 12 projects which currently fund the continuing development of Mercury. These projects span a range of land, atmosphere, and ocean ecological communities and have a number of common needs for metadata searches, but they also have a number of needs specific to one or a few projects. To balance these common and project-specific needs, Mercury's architecture has three major reusable components; a harvester engine, an indexing system and a user interface component. The harvester engine is responsible for harvesting metadata records from various distributed servers around the USA and around the world. The harvester software was packaged in such a way that all the Mercury projects will use the same harvester scripts but each project will be driven by a set of project specific configuration files. The harvested files are structured metadata records that are indexed against the search library API consistently, so that it can render various search capabilities such as simple, fielded, spatial and temporal. This backend component is supported by a very flexible, easy to use Graphical User Interface which is driven by cascading style sheets, which make it even simpler for reusable design implementation. The new Mercury system is based on a Service Oriented Architecture and effectively reuses components for various services such as Thesaurus Service, Gazetteer Web Service and UDDI Directory Services. The software also provides various search services including: RSS, Geo-RSS, OpenSearch, Web Services and Portlets, integrated shopping cart to order datasets from various data centers (ORNL DAAC, NSIDC) and integrated visualization tools. Other features include: Filtering and dynamic sorting of search results, book- markable search results, save, retrieve, and modify search criteria.

Devarakonda, Ranjeet [ORNL] [ORNL

2008-01-01T23:59:59.000Z

482

ARM - Evaluation Product - Quantitative Precipitation Estimates (QPE) from  

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

ProductsQuantitative Precipitation Estimates (QPE) ProductsQuantitative Precipitation Estimates (QPE) from the CSAPR Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Evaluation Product : Quantitative Precipitation Estimates (QPE) from the CSAPR Site(s) SGP TWP General Description Precipitation rates from cloud systems can give a fundamental insight into the processes occurring in-cloud. While rain gauges and disdrometers can give information at a single point, remote sensors such as radars can provide rainfall information over a defined area. The QPE value-added product (VAP) takes the Corrected Moments in Antenna Coordinates VAP and maps the Rain_rate_A field onto a Cartesian grid at the surface. This field is the rain rate as determined using the specific attenuation (A, dBZ/km) due to two-way liquid attenuation after Ryzhkov et

483

Integrating semantic web technologies and geospatial catalog services for geospatial information discovery and processing in cyberinfrastructure  

SciTech Connect

Abstract A geospatial catalogue service provides a network-based meta-information repository and interface for advertising and discovering shared geospatial data and services. Descriptive information (i.e., metadata) for geospatial data and services is structured and organized in catalogue services. The approaches currently available for searching and using that information are often inadequate. Semantic Web technologies show promise for better discovery methods by exploiting the underlying semantics. Such development needs special attention from the Cyberinfrastructure perspective, so that the traditional focus on discovery of and access to geospatial data can be expanded to support the increased demand for processing of geospatial information and discovery of knowledge. Semantic descriptions for geospatial data, services, and geoprocessing service chains are structured, organized, and registered through extending elements in the ebXML Registry Information Model (ebRIM) of a geospatial catalogue service, which follows the interface specifications of the Open Geospatial Consortium (OGC) Catalogue Services for the Web (CSW). The process models for geoprocessing service chains, as a type of geospatial knowledge, are captured, registered, and discoverable. Semantics-enhanced discovery for geospatial data, services/service chains, and process models is described. Semantic search middleware that can support virtual data product materialization is developed for the geospatial catalogue service. The creation of such a semantics-enhanced geospatial catalogue service is important in meeting the demands for geospatial information discovery and analysis in Cyberinfrastructure.

Yue, Peng [Wuhan University; Gong, Jianya [Wuhan University; Di, Liping [George Mason University; He, Lianlian [Hubei University; Wei, Yaxing [ORNL

2011-04-01T23:59:59.000Z

484

Estimation of static formation temperatures in geothermal wells | Open  

Open Energy Info (EERE)

Estimation of static formation temperatures in geothermal wells Estimation of static formation temperatures in geothermal wells Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Estimation of static formation temperatures in geothermal wells Abstract Stabilized formation temperatures were estimated at different depths in 40 wells from the Los Humeros geothermal field, Mexico, using the Horner and the spherical radial flow (SRF) methods. The results showed that the Horner method underestimates formation temperatures, while the SRF method gives temperatures that are closer to the true formation temperatures. This was supported by numerical simulation of a combined circulation and shut-in period in several wells, and results for well H-26 are presented. Numerical reproduction of logged temperature is more feasible if an initial

485

Reinforcing floodrisk estimation  

Science Journals Connector (OSTI)

...However, most ood-risk estimates support decisions...charac- ter. These are investment decisions, where the...current level of ood risk, making improvements...generated a national ood-risk map with a high political and societal impact...

2002-01-01T23:59:59.000Z

486

Estimation of resources and reserves  

E-Print Network (OSTI)

This report analyzes the economics of resource and reserve estimation. Current concern about energy problems has focused attention on how we measure available energy resources. One reads that we have an eight-year oil ...

Massachusetts Institute of Technology. Energy Laboratory.

1982-01-01T23:59:59.000Z

487

NREL: Solar Research - NREL Hydrogen Expert Sees Promise in New Discovery  

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

NREL Hydrogen Expert Sees Promise in New Discovery NREL Hydrogen Expert Sees Promise in New Discovery Photoelectrochemical pioneer John Turner says nickel film cracks the door for tandem artificial photosynthesis, greater efficiency January 8, 2014 Producing hydrogen directly from the sun -- and in a way that is commercially viable -- is more a reality, less a pipedream, thanks in part to a new discovery, renowned hydrogen water-splitting expert John Turner stated in a commentary in the journal Science. Turner, a research fellow at the Energy Department's National Renewable Energy Laboratory, demonstrated 15 years ago that he could use sunlight in a photoelectrochemical process to extract hydrogen from water at a remarkable 12.4% efficiency. Ever since, researchers have been trying to make that process more stable

488

Scientific Discovery through Advanced Computing (SciDAC) | U.S. DOE Office  

Office of Science (SC) Website

Scientific Scientific Discovery through Advanced Computing (SciDAC) Advanced Scientific Computing Research (ASCR) ASCR Home About Research Applied Mathematics Computer Science Next Generation Networking Scientific Discovery through Advanced Computing (SciDAC) Co-Design SciDAC Institutes Computational Science Graduate Fellowship (CSGF) ASCR SBIR-STTR Facilities Science Highlights Benefits of ASCR Funding Opportunities Advanced Scientific Computing Advisory Committee (ASCAC) News & Resources Contact Information Advanced Scientific Computing Research U.S. Department of Energy SC-21/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-7486 F: (301) 903-4846 E: sc.ascr@science.doe.gov More Information » Research Scientific Discovery through Advanced Computing (SciDAC)

489

Discovery of New Materials to Capture Methane | U.S. DOE Office of Science  

Office of Science (SC) Website

Discovery of New Materials to Capture Methane Discovery of New Materials to Capture Methane Basic Energy Sciences (BES) BES Home About Research Facilities Science Highlights Benefits of BES Funding Opportunities Basic Energy Sciences Advisory Committee (BESAC) News & Resources Contact Information Basic Energy Sciences U.S. Department of Energy SC-22/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-3081 F: (301) 903-6594 E: sc.bes@science.doe.gov More Information » April 2013 Discovery of New Materials to Capture Methane Predicted materials could economically produce high-purity methane from natural gas systems and separate methane from coal mine ventilation systems. Print Text Size: A A A Subscribe FeedbackShare Page Click to enlarge photo. Enlarge Photo Image courtesy of Berend Smit, UC-Berkeley

490

Two Real Discoveries That Bring Spider Powers to Our Universe | Department  

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

Two Real Discoveries That Bring Spider Powers to Our Universe Two Real Discoveries That Bring Spider Powers to Our Universe Two Real Discoveries That Bring Spider Powers to Our Universe July 3, 2012 - 10:36am Addthis Argonne Lab researchers used the Advanced Photon Source to look at the structure of spider's dragline silk, which allows arachnids to swing from branches and dangle from window frames, the Spiderman equivalent of swinging from high buildings and dangling from Gotham’s towers. | Creative Commons photo by Flickr user Djumbo. Argonne Lab researchers used the Advanced Photon Source to look at the structure of spider's dragline silk, which allows arachnids to swing from branches and dangle from window frames, the Spiderman equivalent of

491

Geek-Up[04.01.2011]: A Discovery to Fight Cancer and Other Diseases |  

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

4.01.2011]: A Discovery to Fight Cancer and Other Diseases 4.01.2011]: A Discovery to Fight Cancer and Other Diseases Geek-Up[04.01.2011]: A Discovery to Fight Cancer and Other Diseases April 1, 2011 - 5:52pm Addthis Two structures of the Mre11-Rad50 complex were solved independently and overlaid, further revealing a flexible hinge in Rad50 near the Mre11 binding site | Courtesy of Lawrence Berkeley National Laboratory Two structures of the Mre11-Rad50 complex were solved independently and overlaid, further revealing a flexible hinge in Rad50 near the Mre11 binding site | Courtesy of Lawrence Berkeley National Laboratory Niketa Kumar Niketa Kumar Public Affairs Specialist, Office of Public Affairs What does this mean for me? Researchers discovered that a cell's speedy ability to repair damaged DNA relies on the remarkable flexibility of a molecular motor.

492

#LabChat: Particle Accelerators, Lasers and Discovery Science, May 17 at  

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

Particle Accelerators, Lasers and Discovery Science, May Particle Accelerators, Lasers and Discovery Science, May 17 at 1pm EST #LabChat: Particle Accelerators, Lasers and Discovery Science, May 17 at 1pm EST May 15, 2012 - 2:03pm Addthis SLAC’s linac accelerates very short pulses of electrons to 99.9999999 percent the speed of light through a slalom that causes the electrons to emit X-rays, which become synchronized as they interact with the electron pulses and create the world’s brightest X-ray laser pulse. | Photo by Brad Plummer, SLAC. SLAC's linac accelerates very short pulses of electrons to 99.9999999 percent the speed of light through a slalom that causes the electrons to emit X-rays, which become synchronized as they interact with the electron pulses and create the world's brightest X-ray laser pulse. | Photo by

493

NNSA to bring together researchers to discuss discovery and innovation at  

National Nuclear Security Administration (NNSA)

to bring together researchers to discuss discovery and innovation at to bring together researchers to discuss discovery and innovation at LDRD Symposium | 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 > NNSA to bring together researchers to discuss ... NNSA to bring together researchers to discuss discovery and innovation at LDRD Symposium

494

Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt  

Open Energy Info (EERE)

1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt County, Nevada Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Conference Paper: Deep Blue No 1- A Slimhole Geothermal Discovery At Blue Mountain, Humboldt County, Nevada Details Activities (2) Areas (1) Regions (0) Abstract: The purpose of this paper is to provide a summary of the geology, drilling operations, and down-hole measurements obtained during the drilling of Deep Blue No.1. This well was sited on the basis of proximity to numerous gold exploration holes that indicated thermal water, high temperature gradients recorded in the 12 shallow gradient holes, and low resistivity values associated with certain interpreted major faults. The well was targeted to intersect fracture zones associated with the West and

495

Deep Blue No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt  

Open Energy Info (EERE)

No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt County, Nevada Jump to: navigation, search OpenEI Reference LibraryAdd to library Journal Article: Deep Blue No. 1-A Slimhole Geothermal Discovery at Blue Mountain, Humboldt County, Nevada Abstract The purpose of this paper is to provide a summary of the geology, drilling operations, and down-hole measurements obtained during the drilling of Deep Blue No.1. This well was sited on the basis of proximity to numerous gold exploration holes that indicated thermal water, high temperature gradients recorded in the 12 shallow gradient holes, and low resistivity values associated with certain interpreted major faults. The well was targeted to intersect fracture zones associated with the West and Central Faults, two

496

NNSA to bring together researchers to discuss discovery and innovation at  

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

to bring together researchers to discuss discovery and innovation at to bring together researchers to discuss discovery and innovation at LDRD Symposium | 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 > NNSA to bring together researchers to discuss ... NNSA to bring together researchers to discuss discovery and innovation at LDRD Symposium

497

THE OUTBURST DECAY OF THE LOW MAGNETIC FIELD MAGNETAR SGR 0418+5729  

SciTech Connect

We report on the long-term X-ray monitoring of the outburst decay of the low magnetic field magnetar SGR 0418+5729 using all the available X-ray data obtained with RXTE, Swift, Chandra, and XMM-Newton observations from the discovery of the source in 2009 June up to 2012 August. The timing analysis allowed us to obtain the first measurement of the period derivative of SGR 0418+5729: P-dot =4(1) Multiplication-Sign 10{sup -15} s s{sup -1}, significant at a {approx}3.5{sigma} confidence level. This leads to a surface dipolar magnetic field of B{sub dip} {approx_equal} 6 Multiplication-Sign 10{sup 12} G. This measurement confirms SGR 0418+5729 as the lowest magnetic field magnetar. Following the flux and spectral evolution from the beginning of the outburst up to {approx}1200 days, we observe a gradual cooling of the tiny hot spot responsible for the X-ray emission, from a temperature of {approx}0.9 to 0.3 keV. Simultaneously, the X-ray flux decreased by about three orders of magnitude: from about 1.4 Multiplication-Sign 10{sup -11} to 1.2 Multiplication-Sign 10{sup -14} erg s{sup -1} cm{sup -2}. Deep radio, millimeter, optical, and gamma-ray observations did not detect the source counterpart, implying stringent limits on its multi-band emission, as well as constraints on the presence of a fossil disk. By modeling the magneto-thermal secular evolution of SGR 0418+5729, we infer a realistic age of {approx}550 kyr, and a dipolar magnetic field at birth of {approx}10{sup 14} G. The outburst characteristics suggest the presence of a thin twisted bundle with a small heated spot at its base. The bundle untwisted in the first few months following the outburst, while the hot spot decreases in temperature and size. We estimate the outburst rate of low magnetic field magnetars to be about one per year per galaxy, and we briefly discuss the consequences of such a result in several other astrophysical contexts.

Rea, N.; Papitto, A.; Terreran, G.; Girart, J. M.; Palau, Aina; Caliandro, G. A. [Institute of Space Sciences (CSIC-IEEC), Campus UAB, Faculty of Science, Torre C5-parell, E-08193 Barcelona (Spain); Israel, G. L. [INAF/Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone (Italy); Pons, J. A.; Vigano, D. [Department de Fisica Aplicada, Universitat d'Alacant, Ap. Correus 99, E-03080 Alacant (Spain); Turolla, R. [Dipartimento di Fisica e Astronomia, Universita di Padova, via F. Marzolo 8, I-35131 Padova (Italy); Zane, S. [Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT (United Kingdom); Esposito, P.; Tiengo, A.; Salvetti, D. [INAF/Istituto di Astrofisica Spaziale e Fisica Cosmica-Milano, via E. Bassini 15, I-20133 Milano (Italy); Perna, R. [JILA and Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO 80309 (United States); Possenti, A.; Burgay, M. [INAF/Osservatorio Astronomico di Cagliari, localita Poggio dei Pini, strada 54, I-09012 Capoterra (Italy); Goegues, E. [Sabanc Latin-Small-Letter-Dotless-I University, Orhanl Latin-Small-Letter-Dotless-I -Tuzla, 34956 Istanbul (Turkey); Kouveliotou, C. [NASA Marshall Space Flight Center, Huntsville, AL 35812 (United States); Goetz, D. [AIM (UMR 7158 CEA/DSM-CNRS-Universite Paris Diderot) Irfu/Service d'Astrophysique, Saclay, F-91191 Gif-sur-Yvette Cedex (France); and others

2013-06-10T23:59:59.000Z

498

Magnetic Field Safety Training  

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

Safety Training Magnetic Field Safety Strong Magnetic Fields exist around energized magnets. High magnetic fields alone are a recognized hazard only for personnel with certain...

499

SLOPE ESTIMATES OF ARTIN-SCHREIER CURVES JASPER SCHOLTEN AND HUI JUNE ZHU  

E-Print Network (OSTI)

SLOPE ESTIMATES OF ARTIN-SCHREIER CURVES JASPER SCHOLTEN AND HUI JUNE ZHU Abstract. Let X polygon, zeta and L functions over finite fields. 1 #12;2 JASPER SCHOLTEN AND HUI JUNE ZHU b) If p > 2d

Zhu, Hui June

500

Estimation of fracture compliance from tubewaves generated at a fracture intersecting a borehole  

E-Print Network (OSTI)

Understanding fracture compliance is important for characterizing fracture networks and for inferring fluid flow in the subsurface. In an attempt to estimate fracture compliance in the field, we developed a new model to ...

Bakku, Sudhish Kumar

2011-01-01T23:59:59.000Z