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1

Calyxo USA Solar Fields LLC | Open Energy Information  

Open Energy Info (EERE)

Calyxo USA Solar Fields LLC Calyxo USA Solar Fields LLC Jump to: navigation, search Name Calyxo USA (Solar Fields LLC) Place Perrysburg, Ohio Zip 43551 Sector Solar Product Producer of cadmium telluride photovoltaic modules. Q-Cells acquired Solar Fields IP and assets which have been transferred into the US branch of Q-Cells subsidiary Calyxo GmbH Coordinates 41.55671°, -83.628899° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.55671,"lon":-83.628899,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

2

Scheuten Solar USA Inc | Open Energy Information  

Open Energy Info (EERE)

Scheuten Solar USA, Inc. Place: Rancho Santa Margarita, California Zip: 92688 Sector: Solar Product: Manufacturer of Solar PV systems References: Scheuten Solar USA, Inc.1 This...

3

Solar Unlimited USA | Open Energy Information  

Open Energy Info (EERE)

Logo: Solar Unlimited USA Name Solar Unlimited USA Address 2353 Park Ave. Place Cedar City, Utah Zip 84721 Sector Solar Product Solar energy systems Year founded 1998 Phone number 435-867-9876 Website http://solarunlimited.net/ Coordinates 37.6944762°, -113.0937928° 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":37.6944762,"lon":-113.0937928,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

4

Solar Systems USA | Open Energy Information  

Open Energy Info (EERE)

USA USA Jump to: navigation, search 200px Name Solar Systems USA Place Atlanta, Georgia Sector Renewable Energy Product Solar Panels Year founded 2010 Website http://solarsystemsusa.net Coordinates 33.7489954°, -84.3879824° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":33.7489954,"lon":-84.3879824,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

5

Solar World USA not SolarWorld AG | Open Energy Information  

Open Energy Info (EERE)

World USA not SolarWorld AG World USA not SolarWorld AG Jump to: navigation, search Name Solar World USA (not SolarWorld AG) Place Colorado Springs, Colorado Zip 80907 Sector Solar Product Solar World manufactures solar powered products for educational, consumer, electronic and custom OEM markets. References Solar World USA (not SolarWorld AG)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Solar World USA (not SolarWorld AG) is a company located in Colorado Springs, Colorado . References ↑ "Solar World USA (not SolarWorld AG)" Retrieved from "http://en.openei.org/w/index.php?title=Solar_World_USA_not_SolarWorld_AG&oldid=351350" Categories: Clean Energy Organizations

6

High Field Magnet R&D in the USA  

E-Print Network [OSTI]

Field Magnet R&D in the USA Stephen A. Gourlay Abstract··Laboratory, Berkeley, CA 94720 USA (telephone: 510-486-7156,

Gourlay, S.A.

2011-01-01T23:59:59.000Z

7

High Field Magnet R&D in the USA  

E-Print Network [OSTI]

High Field Magnet R&D in the USA Stephen A. Gourlay magnetLaboratory, Berkeley, CA 94720 USA (telephone: 510-486-7156,

Gourlay, Stephen A.

2003-01-01T23:59:59.000Z

8

2008 European PV Conference, Valencia, Spain COMPARISON OF SOLAR RADIATION FORECASTS FOR THE USA  

E-Print Network [OSTI]

2008 European PV Conference, Valencia, Spain COMPARISON OF SOLAR RADIATION FORECASTS FOR THE USA J, The University at Albany, 251 Fuller Rd, Albany, NY 12203, USA 3 University of Oldenburg, Institute of Physics for a half year period (summer 2007) at three different climates in the USA. ECMWF shows the best results

Perez, Richard R.

9

The Magnetic Field in the Solar Atmosphere  

E-Print Network [OSTI]

This publication provides an overview of magnetic fields in the solar atmosphere with the focus lying on the corona. The solar magnetic field couples the solar interior with the visible surface of the Sun and with its atmosphere. It is also responsible for all solar activity in its numerous manifestations. Thus, dynamic phenomena such as coronal mass ejections and flares are magnetically driven. In addition, the field also plays a crucial role in heating the solar chromosphere and corona as well as in accelerating the solar wind. Our main emphasis is the magnetic field in the upper solar atmosphere so that photospheric and chromospheric magnetic structures are mainly discussed where relevant for higher solar layers. Also, the discussion of the solar atmosphere and activity is limited to those topics of direct relevance to the magnetic field. After giving a brief overview about the solar magnetic field in general and its global structure, we discuss in more detail the magnetic field in active regions, the quie...

Wiegelmann, Thomas; Solanki, Sami K

2014-01-01T23:59:59.000Z

10

Solar magnetic fields and terrestrial climate  

E-Print Network [OSTI]

Solar irradiance is considered one of the main natural factors affecting terrestrial climate, and its variations are included in most numerical models estimating the effects of natural versus anthropogenic factors for climate change. Solar wind causing geomagnetic disturbances is another solar activity agent whose role in climate change is not yet fully estimated but is a subject of intense research. For the purposes of climate modeling, it is essential to evaluate both the past and the future variations of solar irradiance and geomagnetic activity which are ultimately due to the variations of solar magnetic fields. Direct measurements of solar magnetic fields are available for a limited period, but can be reconstructed from geomagnetic activity records. Here we present a reconstruction of total solar irradiance based on geomagnetic data, and a forecast of the future irradiance and geomagnetic activity relevant for the expected climate change.

Georgieva, Katya; Kirov, Boian

2014-01-01T23:59:59.000Z

11

Multi-objective optimization of solar tower heliostat fields  

E-Print Network [OSTI]

Multi-objective optimization of solar tower heliostat fields Pascal Richter, Martin Frank and Erika Introduction Solar tower plants generate electric power from sunlight by focusing concentrated solar radiation electricity. Fig. 1 Solar tower plant PS10, 11 MW in Andalusia, Spain. [Source: flickr] Solar tower plants

Ábrahám, Erika

12

SEP Success Story: Solar Field Powers Historic Garden Holiday...  

Energy Savers [EERE]

SEP Success Story: Solar Field Powers Historic Garden Holiday Display SEP Success Story: Solar Field Powers Historic Garden Holiday Display December 21, 2011 - 1:26pm Addthis This...

13

Sinocome Solar aka Perfect Field Investment | Open Energy Information  

Open Energy Info (EERE)

Solar aka Perfect Field Investment Solar aka Perfect Field Investment Jump to: navigation, search Name Sinocome Solar (aka Perfect Field Investment) Place China Product Chinese manufacturer of amorphous silicon thin-film cells and modules using technology patents owned by the Target Group, also a Chinese firm. References Sinocome Solar (aka Perfect Field Investment)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Sinocome Solar (aka Perfect Field Investment) is a company located in China . References ↑ "[ Sinocome Solar (aka Perfect Field Investment)]" Retrieved from "http://en.openei.org/w/index.php?title=Sinocome_Solar_aka_Perfect_Field_Investment&oldid=351122" Categories:

14

FRONIUS USA LLC | Open Energy Information  

Open Energy Info (EERE)

FRONIUS USA LLC Jump to: navigation, search Name: FRONIUS USA LLC Place: Brighton, Michigan 48116 USA, Michigan Sector: Solar Product: Focused on welding machines and solar...

15

Collector Field Maintenance: Distributed Solar Thermal Systems  

Science Journals Connector (OSTI)

This paper reports on recent operation and maintenance experiences with distributed solar thermal systems. Although some information on system-...

E. C. Boes; E. C. Cameron; E. L. Harley

1986-01-01T23:59:59.000Z

16

1 CONFIDENTIAL1 CONFIDENTIAL GreenField Solar  

E-Print Network [OSTI]

Driving solar energy into mainstream deployment, without subsidies Thank You! #12;1 CONFIDENTIAL1 CONFIDENTIAL GreenField Solar: Testing and Reliability needs of CPV Systems DrField's Dense array design advantages: · Simpler optical alignment & relaxed tracking tolerances => o Lower O

Rollins, Andrew M.

17

Recycling of the Solar Corona's Magnetic Field  

Science Journals Connector (OSTI)

Magnetic fields play a dominant role in the atmospheres of the Sun and other Sun-like stars. Outside sunspot regions, the photosphere of the so-called quiet Sun contains myriads of small-scale magnetic concentrations, with strengths ranging from the detection limit of ~1016 Mx up to ~3 ? 1020 Mx. The tireless motion of these magnetic flux concentrations, along with the continual appearance and disappearance of opposite-polarity pairs of fluxes, releases a substantial amount of energy that may be associated with a whole host of physical processes in the solar corona, not least the enigma of coronal heating. We find here that the timescale for magnetic flux to be remapped in the quiet-Sun corona is, surprisingly, only 1.4 hr (around 1/10 of the photospheric flux recycling time), implying that the quiet-Sun corona is far more dynamic than previously thought. Besides leading to a fuller understanding of the origins of magnetically driven phenomena in our Sun's corona, such a process may also be crucial for the understanding of stellar atmospheres in general.

R. M. Close; C. E. Parnell; D. W. Longcope; E. R. Priest

2004-01-01T23:59:59.000Z

18

Geometry of tower-type solar electric station heliostat field  

SciTech Connect (OSTI)

A general method is presented for calculating the angular positions of an arbitrary heliostat at an arbitrary position in a heliostat field surrounding a tower-type solar electric station as a function of solar position. A system of angular coordinates is used which rotates with the solar azimuth direction around the collecting tower, resulting in an expression for the proper orientation of heliostat mirrors that is independent of local latitude, solar declination and time of day. The lines on the horizontal plane of the heliostat field characterized by the same values of the angles governing the horizontal inclination of the corresponding heliostat for a given solar elevation form two families of hyperbolas with vertexes facing the center of the field. Such isoline drawings constructed from the calculations may be used to determine the limiting values of the heliostat angles during the daily and seasonal course of operation of the heliostat facility.

Tepliakov, D.I.; Aparisi, R.R.

1980-01-01T23:59:59.000Z

19

Suggested improvements to solar system maintenance based on field experience  

SciTech Connect (OSTI)

Field experience has shown that maintenance is a critical factor in determining the overall success of a solar system. This paper summarizes the field experience with the maintenance of over 30 solar installations, three of which contain more than 500 individual solar systems for residential housing. The field results show several severe problems, and an analysis indicates that a number of improvements can be made to help avoid them. These include (1) improving solar designs, (2) producing service documents, and (3) providing training for maintenance personnel. Specific technical improvements to solar designs are presented in this paper, the number and content of service documents are outlined, and suggestions for training of maintenance personnel are presented.

Johnson, D.L.; Hittle, D.C.; Joncich, D.M.

1983-06-01T23:59:59.000Z

20

Molecular Lines as Diagnostics of Solar and Stellar Magnetic Fields  

E-Print Network [OSTI]

Molecular Lines as Diagnostics of Solar and Stellar Magnetic Fields S.V. Berdyugina1, S.K. Solanki2 of different OH lines are reproduced without invoking any free parameters, except the magnetic field strength to significant improvements in the deduced magnetic field vector. Here we investigate how molecular lines can

Berdyugina, Svetlana

Note: This page contains sample records for the topic "usa solar fields" 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

Efficient solar anti-neutrino production in random magnetic fields  

E-Print Network [OSTI]

We have shown that the electron anti-neutrino appearance in the framework of the spin flavor conversion mechanism is much more efficient in the case of neutrino propagation through random than regular magnetic field. This result leads to much stronger limits on the product of the neutrino transition magnetic moment and the solar magnetic field based on the recent KamLAND data. We argue that the existence of the random magnetic fields in the solar convective zone is a natural sequence of the convective zone magnetic field evolution.

O. G. Miranda; T. I. Rashba; A. I. Rez; J. W. F. Valle

2004-05-12T23:59:59.000Z

22

S. Guha, J. Yang, A. Banerjee, K. Hoffman, S. Sugiyama, and J. Call United Solar Systems Corp., Troy, Michigan 48084 USA  

E-Print Network [OSTI]

Conversion Devices, Inc., Troy, Michigan 48084 USA spectral-splitting, triple-junction a-S alloy solar cell been achieved using a spectral-splitting, triple-junction cell technology incorporating i) high qualityS. Guha, J. Yang, A. Banerjee, K. Hoffman, S. Sugiyama, and J. Call United Solar Systems Corp

Deng, Xunming

23

Solar Field Powers Historic Garden Holiday Display | Department of Energy  

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

Field Powers Historic Garden Holiday Display Field Powers Historic Garden Holiday Display Solar Field Powers Historic Garden Holiday Display December 21, 2011 - 2:58pm Addthis This is part of the holiday light display at Longwood Gardens in Pennsylvania's Brandwine Valley. This year, they commissioned an American-made 1.2 megawatt, 10.7-acre solar field as part of their goal to generate three megawatts of renewable energy by 2018. | Photo courtesy of Longwood Gardens/W. Hill This is part of the holiday light display at Longwood Gardens in Pennsylvania's Brandwine Valley. This year, they commissioned an American-made 1.2 megawatt, 10.7-acre solar field as part of their goal to generate three megawatts of renewable energy by 2018. | Photo courtesy of Longwood Gardens/W. Hill Kristin Swineford Communication Specialist, Weatherization and Intergovernmental Programs

24

MAGNETIC FIELD CONFINEMENT IN THE SOLAR CORONA. II. FIELD-PLASMA INTERACTION B. Fornberg,2  

E-Print Network [OSTI]

MAGNETIC FIELD CONFINEMENT IN THE SOLAR CORONA. II. FIELD-PLASMA INTERACTION N. Flyer,1 B. Fornberg numerically to generate a continuum of solutions with two parameters to control the total azimuthal flux from the study to the solar corona and the energetics of coronal mass ejections and flares. Subject

Fornberg, Bengt

25

Magnetic fields in the solar photosphere  

Science Journals Connector (OSTI)

...magnetoconvection in the quiet Sun. Filled contours show the temperature variations in a horizontal...Sanchez Almeida2003Quiet-Sun magnetic fields at high...Almeida, and F Kneer2006The distribution of quiet Sun magnetic field strengths...

2008-01-01T23:59:59.000Z

26

MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS  

SciTech Connect (OSTI)

Solar flares and coronal mass ejections, the most catastrophic eruptions in our solar system, have been known to affect terrestrial environments and infrastructure. However, because their triggering mechanism is still not sufficiently understood, our capacity to predict the occurrence of solar eruptions and to forecast space weather is substantially hindered. Even though various models have been proposed to determine the onset of solar eruptions, the types of magnetic structures capable of triggering these eruptions are still unclear. In this study, we solved this problem by systematically surveying the nonlinear dynamics caused by a wide variety of magnetic structures in terms of three-dimensional magnetohydrodynamic simulations. As a result, we determined that two different types of small magnetic structures favor the onset of solar eruptions. These structures, which should appear near the magnetic polarity inversion line (PIL), include magnetic fluxes reversed to the potential component or the nonpotential component of major field on the PIL. In addition, we analyzed two large flares, the X-class flare on 2006 December 13 and the M-class flare on 2011 February 13, using imaging data provided by the Hinode satellite, and we demonstrated that they conform to the simulation predictions. These results suggest that forecasting of solar eruptions is possible with sophisticated observation of a solar magnetic field, although the lead time must be limited by the timescale of changes in the small magnetic structures.

Kusano, K.; Bamba, Y.; Yamamoto, T. T. [Solar-Terrestrial Environment Laboratory, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601 (Japan); Iida, Y.; Toriumi, S. [Department of Earth and Planetary Science, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Asai, A., E-mail: kusano@nagoya-u.jp [Unit of Synergetic Studies for Space, Kyoto University, 17 Kitakazan Ohmine-cho, Yamashina-ku, Kyoto 607-8471 (Japan)

2012-11-20T23:59:59.000Z

27

Solar Field Gives Tennessee Economy a Boost | Department of Energy  

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

Field Gives Tennessee Economy a Boost Field Gives Tennessee Economy a Boost Solar Field Gives Tennessee Economy a Boost September 14, 2010 - 6:24pm Addthis Efficient Energy of Tennessee installs panels at a 1-MW solar farm outside Knoxville in July. | Photo by Harvey Abouelata and courtesy of Efficient Energy of Tennessee Efficient Energy of Tennessee installs panels at a 1-MW solar farm outside Knoxville in July. | Photo by Harvey Abouelata and courtesy of Efficient Energy of Tennessee Lorelei Laird Writer, Energy Empowers Outside Knoxville, Tenn., a new construction project began raising eyebrows in May. The project was clearly visible from cars on the nearby Andrew Johnson Highway, but passers-by had no idea what to make of it at first, according to Robbie Thomas, president of Efficient Energy of Tennessee, a

28

Coriolis emf as the real generator of solar magnetic field and a new model of the reversal of the general solar magnetic field  

Science Journals Connector (OSTI)

Generation of general solar magnetic field as proposed by Cowling (1945, 1953) and Drobyshevski (1977) from the Coriolis emf is reconsidered and a new mechanism of the reversal of teh general solar magnetic fi...

L. Manihar Singh; L. Randhoni Devi

29

Solar Energy Applications Page 1 Rev. September 23, 2009 Field Office Serial  

E-Print Network [OSTI]

Solar Energy Applications Page 1 Rev. September 23, 2009 Field Office Serial Number Project Name) Located in Maricopa Co., north of Mobile AZ. Pending 9. AZA 034187 Sonoran Solar Energy Project Boulevard Co. South of Gila Bend Pending #12;Solar Energy Applications Page 2 Rev. September 23, 2009 Field

Laughlin, Robert B.

30

Solar Wind and Interplanetary Magnetic Field: A Tutorial C. T. Russell  

E-Print Network [OSTI]

Solar Wind and Interplanetary Magnetic Field: A Tutorial C. T. Russell Institute of Geophysics at the center of the sun to its radiation into space by the photosphere, but most importantly for the solar wind controls the properties of the solar wind. In this tutorial review we examine the properties of the fields

Russell, Christopher T.

31

Characterization of the solar light field within the ocean mesopelagic zone based on radiative transfer simulations  

E-Print Network [OSTI]

Characterization of the solar light field within the ocean mesopelagic zone based on radiative t The solar light field within the ocean from the sea surface to the bottom of the mesopelagic zone there is sufficient amount of solar light to support the process of photosynthesis, and below by the aphotic

Stramski, Dariusz

32

Impact of the solar wind dynamic pressure on the Region 2 field-aligned currents  

E-Print Network [OSTI]

Impact of the solar wind dynamic pressure on the Region 2 field-aligned currents S. Nakano,1,2 G and the solar wind dynamic pressure is investigated using magnetic field data from Defense Meteorological in the magnetosphere varies with the solar wind dynamic pressure. Therefore, we can expect that the Region 2 currents

Higuchi, Tomoyuki

33

Energy management in solar thermal power plants with double thermal storage system and subdivided solar field  

Science Journals Connector (OSTI)

In the paper, two systems for solar thermal power plants (STPPs) are devised for improving the overall performance of the plant. Each one attempts to reduce losses coming from two respective sources. The systems are simulated and compared to a reference STPP. They consists on: (a) a double thermal energy storage (DTS) with different functionalities for each storage and (b) the subdivision of the solar collector field (SSF) into specialised sectors, so that each sector is designed to meet a thermal requirement, usually through an intermediate heat exchanger. This subdivision reduces the losses in the solar field by means of a decrease of the temperature of the heat transfer fluid (HTF). Double thermal energy storage is intended for keeping the plant working at nominal level for many hours a day, including post-sunset hours. One of the storages gathers a fluid which is heated up to temperatures above the nominal one. In order to make it work, the solar field must be able to overheat the fluid at peak hours. The second storage is the classical one. The combination of both allows the manager of the plant to keep the nominal of the plant for longer periods than in the case of classical thermal energy storage. To the authors knowledge, it is the first time that both configurations are presented and simulated for the case of parabolic through STPP with HTF technology. The results show that, if compared to the reference STPP, both configurations may raise the annual electricity generation (up to 1.7% for the DTS case and 3.9% for the SSF case).

Antonio Rovira; Mara Jos Montes; Manuel Valdes; Jos Mara Martnez-Val

2011-01-01T23:59:59.000Z

34

On characterization and measurement of average solar field mirror reflectance in utility-scale concentrating solar power plants  

Science Journals Connector (OSTI)

Abstract Due to the emerging need for the development of acceptance test codes for commercial concentrating solar power (CSP) plants, an effort is made here to develop a mirror reflectance model suitable for CSP applications as well as a general procedure to measure the average mirror reflectance of a solar field. Typically, a utility-scale solar field includes hundreds of thousands of mirror panels (if not more), and their reflectance is subject to many factors, such as weather and planned washing schedule. The newly developed mirror reflectance model can be used to characterize different types of mirror materials and can be directly used to perform optical performance evaluation of solar collectors. The newly proposed procedure for average solar field reflectance measurements includes a baseline comprehensive measurement and an individual factor measurement: the former allows a comprehensive survey of mirror reflectance across the whole solar field, and the latter can provide correcting factors for selected individual factors to further improve the accuracy of the baseline measurements. A detailed test case implementing the general procedure is applied to a state-of-the-art commercial parabolic trough plant and validates the proposed mirror reflectance model and average reflectance measurement procedure. In the test case, the plant-wide reflectance measurements at a commercial utility-scale solar plant were conducted and can shed light on relevant analysis of CSP applications. The work can also be naturally applied to other types of solar plants, such as power towers and linear Fresnel plants.

Guangdong Zhu; David Kearney; Mark Mehos

2014-01-01T23:59:59.000Z

35

A Solar Re-Skin at FedEx Field | Department of Energy  

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

A Solar Re-Skin at FedEx Field A Solar Re-Skin at FedEx Field A Solar Re-Skin at FedEx Field August 2, 2011 - 10:40am Addthis Ramamoorthy Ramesh Former Director, SunShot Initiative & Solar Energy Technologies Program What does this mean for me? Investments by major companies like the Redskins show the growing market demand for solar technology, as the SunShot Initiative works to accelerate this growth to make solar energy cheaper. If solar power could score a touchdown, then this week's news would definitely count. On Wednesday, the Washington Redskins announced they are working with NRG Energy, one of America's largest energy companies, to bring renewable energy to the football franchise. This means more than just a few panels on the roof. Through the partnership, NRG will install 8,000 translucent solar panels to

36

A Solar Re-Skin at FedEx Field | Department of Energy  

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

A Solar Re-Skin at FedEx Field A Solar Re-Skin at FedEx Field A Solar Re-Skin at FedEx Field August 2, 2011 - 10:40am Addthis Ramamoorthy Ramesh Former Director, SunShot Initiative & Solar Energy Technologies Program What does this mean for me? Investments by major companies like the Redskins show the growing market demand for solar technology, as the SunShot Initiative works to accelerate this growth to make solar energy cheaper. If solar power could score a touchdown, then this week's news would definitely count. On Wednesday, the Washington Redskins announced they are working with NRG Energy, one of America's largest energy companies, to bring renewable energy to the football franchise. This means more than just a few panels on the roof. Through the partnership, NRG will install 8,000 translucent solar panels to

37

A strong, highly-tilted interstellar magnetic field near the Solar System  

Science Journals Connector (OSTI)

... hydrogen was not taken into account. Here we report measurements of the deflection of the solar wind plasma flows in the heliosheath to determine the magnetic field strength and orientation in ... We conclude that the interstellar medium field is turbulent or has a distortion in the solar vicinity. The local interstellar medium magnetic field (BISM) is one of the key ...

M. Opher; F. Alouani Bibi; G. Toth; J. D. Richardson; V. V. Izmodenov; T. I. Gombosi

2009-12-24T23:59:59.000Z

38

Electromagnetic field optimization for enhancing photovoltaic efficiency of organic solar cells  

Science Journals Connector (OSTI)

The electromagnetic field distribution inside multilayer organic solar cells composed of interpenetrated networks of conjugated polymers is calculated. By enhancing the...

Simon, Jean-Jacques; Torchio, Philippe; Escoubas, Ludovic; Cathelinaud, Michel; Alem, Salima; Nunzi, Jean-Michel

39

RDI Development: Wisdom Way Solar Village, Greenfield, Massachusetts Field Test Report  

SciTech Connect (OSTI)

NREL, Mountain Energy Partnership, and the Consortium of Advanced Residential Buildings conducted field tests on a house in Wisdom Way Solar Village to verify energy efficiency.

Fang, X.; Hancock, E.

2009-05-01T23:59:59.000Z

40

Discrepancies in the Prediction of Solar Wind using Potential Field Source Surface Model: An  

E-Print Network [OSTI]

expansion near the Sun and the solar wind speed observed at earth was first noted by Levine, AltschulerDiscrepancies in the Prediction of Solar Wind using Potential Field Source Surface Model between the magnetic flux tube expansion factor (FTE) at the source surface and the solar wind speed

Zhao, Xuepu

Note: This page contains sample records for the topic "usa solar fields" 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

Particle acceleration and radiation by direct electric fields in flaring complex solar active regions  

E-Print Network [OSTI]

to connect the energy re- lease process with the acceleration of electrons in solar flares, using a CA modelParticle acceleration and radiation by direct electric fields in flaring complex solar active-Meudon, 92195 Meudon Cedex, FRANCE Abstract The acceleration and radiation of solar energetic particles

Anastasiadis, Anastasios

42

Three-dimensional multispecies MHD studies of the solar wind interaction with Mars in the presence of crustal fields  

E-Print Network [OSTI]

Three-dimensional multispecies MHD studies of the solar wind interaction with Mars in the presence of Michigan, Ann Arbor, Michigan, USA K. G. Powell Aerospace Engineering Department, University of Michigan, Ann Arbor, Michigan, USA Received 30 January 2002; revised 5 April 2002; accepted 13 May 2002

De Zeeuw, Darren L.

43

Investigation of the fluid temperature field inside a flat-plate solar collector  

Science Journals Connector (OSTI)

An experimental study was conducted to investigate fluid temperature fields inside a flat-plate solar collector tube. The results show the highest fluid ... tube, whereas, the temperature field in the horizontal ...

Gurveer Sandhu; Kamran Siddiqui

2014-11-01T23:59:59.000Z

44

Solar Energy Education. Industrial arts: student activities. Field test edition  

SciTech Connect (OSTI)

In this teaching manual several activities are presented to introduce students to information on solar energy through classroom instruction. Wind power is also included. Instructions for constructing demonstration models for passive solar systems, photovoltaic cells, solar collectors and water heaters, and a bicycle wheel wind turbine are provided. (BCS)

Not Available

1981-02-01T23:59:59.000Z

45

A COMPARISON BETWEEN GLOBAL SOLAR MAGNETOHYDRODYNAMIC AND POTENTIAL FIELD SOURCE SURFACE MODEL RESULTS  

E-Print Network [OSTI]

ABSTRACT The large-scale, steady-state magnetic field configuration of the solar corona is typicallyA COMPARISON BETWEEN GLOBAL SOLAR MAGNETOHYDRODYNAMIC AND POTENTIAL FIELD SOURCE SURFACE MODEL computer resources, and can resolve structure on scales beyond those that can be handled by current MHD

California at Berkeley, University of

46

SOLARCAP: Super Capacitor Buffering of Solar Energy for Self-Sustainable Field Systems  

E-Print Network [OSTI]

SOLARCAP: Super Capacitor Buffering of Solar Energy for Self-Sustainable Field Systems Amal Fahad of the conventional battery-based energy storage, this paper argues that the super capacitor buffering of solar energy (SOLARCAP) has the advantages of precise energy lifetime awareness, low maintenance, and operational

Shen, Kai

47

Performance Enhancement of a Graphene-Zinc Phosphide Solar Cell Using the Electric Field-Effect  

E-Print Network [OSTI]

Performance Enhancement of a Graphene-Zinc Phosphide Solar Cell Using the Electric Field, University of California, Berkeley, California 94720, United States Material Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States § Department of Applied Physics

Javey, Ali

48

Observations of Unresolved Photospheric Magnetic Fields in Solar Flares Using Fe i and Cr i Lines  

Science Journals Connector (OSTI)

The structure of the photospheric magnetic field during solar flares is examined using echelle spectropolarimetric observations. The study is based on several Fei and Cri lines observed at locations correspondi...

M. Gordovskyy; V. G. Lozitsky

2014-10-01T23:59:59.000Z

49

Thermal and Hydraulic Design of a Solar Collector Field for a Primary School Pool  

Science Journals Connector (OSTI)

Abstract The methodology and results of the thermal and hydraulic design for a solar heating field of an elementary school's semi-olympic pool is presented. Improved flat solar collectors with copper tube and aluminum fins were used. From own experiences, many Mexican solar fields do not operate correctly because of their poor flow balance (irrigation), may be due to lack of attention given to this aspect. That's why the research of this work focuses on studying the behavior of the pressure drop in a hydraulic arrangement, particularly of this facility, in which all collector batteries are connected in parallel. Previously two solar collectors were sent to a specialized laboratory for certification tests, obtaining the optimum water flow value for maximum thermal efficiency. The results show an optimum range between 4 and 11 L/min. On the other hand, the development of a thermal model based on a temporal energy balance, allowed us to determine that the optimum solar heating area is around 338 m2, using 195 flat-coated solar collectors, with copper tube and aluminum fin. For this heating system a water volume/solar collection area relation, called REVA, of 1.45m3/m2 was obtained. Referred to the hydraulic design and using the program EPANET 2.0 it was found that in the proposed arrangement, 192 solar collectors were irrigated with the optimal range and only 2 solar collectors were below the lower range at 3 L/min.

Rubn Dorantes; Georgina Garca; Carlos Salazar; Heber Oviedo; Humberto Gonzlez; Ral Alanis; Edgar Salazar; Ignacio R. Martn-Dominguez

2014-01-01T23:59:59.000Z

50

Large-scale solar cycle features of solar photospheric magnetic field  

E-Print Network [OSTI]

It is well accepted that the solar cycle originates from a magnetohydrodynamics dynamo deep inside the Sun. Many dynamo models have long been proposed based on a lot of observational constraints. In this paper, using 342 NSO/Kitt Peak solar synoptic charts we study the solar cycle phases in different solar latitudinal zones to set further constraints. Our results can be summarized as follows. (1) The variability of solar polar regions' area has a correlation with total unsigned magnetic flux in advance of 5 years. (2) The high-latitude region mainly appears unipolar in the whole solar cycle and its flux peak time lags sunspot cycle for 3 years. (3) For the activity belt, it is not surprised that its phase be the same as sunspot's. (4) The flux peak time of the low-latitude region shifts forward with an average gradient of 32.2 $day/deg$. These typical characteristics may provide some hints for constructing an actual solar dynamo.

W. B. Song

2007-05-14T23:59:59.000Z

51

Field studies of engineered barriers for closure of low level radioactive waste landfills at Los Alamos, New Mexico, USA  

SciTech Connect (OSTI)

The Los Alamos National Laboratory examined water balance relationships for four different landfill cover designs containing engineered barriers. These field experiments were performed at Los Alamos, New Mexico, USA, in 1.0- by 10.0-m plots with downhill slopes of 5, 10, 15, and 25%. Field measurements of seepage, precipitation, interflow, runoff, and soil water content were collected in each of the 16 plots representing four slopes each with four cover designs: Conventional, EPA, Loam Capillary Barrier and Clay Loam Capillary Barrier. A seepage collection system was installed beneath each cover design to evaluate the influence of slope length on seepage using a series of four metal pans filled with medium gravel that were placed end-to-end in the bottom of each field plot. An automated water flow data logging system was used to collect hourly seepage, interflow and runoff data and consisted of 100 100-liter tanks, each of which was equipped with an ultrasonic liquid-level sensor and a motor-operated ball valve used to drain the tank. Soil water content was routinely monitored every six hours at each of 212 locations throughout the 16 plots with time domain reflectrometry (TDR) techniques using an automated and multiplexed measurement system. Field data is presented to show the effects of slope and slope length on the performance of each landfill cover design for the first 15 months of this field experiment.

Nyhan, J.W.; Langhorst, G.J.; Martin, C.E.; Martinez, J.L.; Schofield, T.G.

1993-05-01T23:59:59.000Z

52

MAGNETOHYDRODYNAMIC SIMULATION-DRIVEN KINEMATIC MEAN FIELD MODEL OF THE SOLAR CYCLE  

SciTech Connect (OSTI)

We construct a series of kinematic axisymmetric mean-field dynamo models operating in the {alpha}{Omega}, {alpha}{sup 2}{Omega} and {alpha}{sup 2} regimes, all using the full {alpha}-tensor extracted from a global magnetohydrodynamical simulation of solar convection producing large-scale magnetic fields undergoing solar-like cyclic polarity reversals. We also include an internal differential rotation profile produced in a purely hydrodynamical parent simulation of solar convection, and a simple meridional flow profile described by a single cell per meridional quadrant. An {alpha}{sup 2}{Omega} mean-field model, presumably closest to the mode of dynamo action characterizing the MHD simulation, produces a spatiotemporal evolution of magnetic fields that share some striking similarities with the zonally-averaged toroidal component extracted from the simulation. Comparison with {alpha}{sup 2} and {alpha}{Omega} mean-field models operating in the same parameter regimes indicates that much of the complexity observed in the spatiotemporal evolution of the large-scale magnetic field in the simulation can be traced to the turbulent electromotive force. Oscillating {alpha}{sup 2} solutions are readily produced, and show some similarities with the observed solar cycle, including a deep-seated toroidal component concentrated at low latitudes and migrating equatorward in the course of the solar cycle. Various numerical experiments performed using the mean-field models reveal that turbulent pumping plays an important role in setting the global characteristics of the magnetic cycles.

Simard, Corinne; Charbonneau, Paul [Departement de Physique, Universite de Montreal, C.P. 6128 Succ. Centre-ville, Montreal, Qc H3C 3J7 (Canada); Bouchat, Amelie, E-mail: corinne@astro.umontreal.ca, E-mail: paulchar@astro.umontreal.ca, E-mail: amelie.bouchat@mail.mcgill.ca [Department of Atmospheric and Oceanic Sciences, McGill University, 805 Sherbrooke West, Montreal, Quebec H3A 2K6 (Canada)

2013-05-01T23:59:59.000Z

53

Solar  

Science Journals Connector (OSTI)

With sharp drop in costs for photovoltaic and solar thermal processes, solar energy has become more attractive alternative ... Almost half the total was earmarked for PV and solar thermal projects. ...

WARD WORTHY

1991-06-17T23:59:59.000Z

54

LONG EXPOSURE POINT SPREAD FUNCTION ESTIMATION FROM SOLAR ADAPTIVE OPTICS LOOP DATA  

E-Print Network [OSTI]

Astronomer, National Solar Observatory, New Mexico, USA Dr. Haimin Wang, Dissertation Co-Advisor DateABSTRACT LONG EXPOSURE POINT SPREAD FUNCTION ESTIMATION FROM SOLAR ADAPTIVE OPTICS LOOP DATA during solar observations due to the lack of point sources in the field-of-view. Moreover, the highly

55

Current Helicity and Twist as Two Indicators of The Mirror Asymmetry of solar Magnetic Fields  

E-Print Network [OSTI]

A comparison between the two tracers of magnetic field mirror asymmetry in solar active regions, twist and current helicity, is presented. It is shown that for individual active regions these tracers do not possess visible similarity while averaging by time over the solar cycle, or by latitude, reveals similarities in their behaviour. The main property of the dataset is anti-symmetry over the solar equator. Considering the evolution of helical properties over the solar cycle we find signatures of a possible sign change at the beginning of the cycle, though more systematic observational data are required for a definite confirmation. We discuss the role of both tracers in the context of the solar dynamo theory.

D. D. Sokoloff; H. Zhang; K. Kuzanyan; V. N. Obridko; D. N. Tomin; V. N. Tutubalin

2008-02-25T23:59:59.000Z

56

Effect of internal electric field on InAs/GaAs quantum dot solar cells  

SciTech Connect (OSTI)

We studied time-resolved carrier recombination in InAs/GaAs quantum dot (QD) solar cells. The electric field in a p-i-n diode structure spatially separates photoexcited carriers in QDs, strongly affecting the conversion efficiency of intermediate-band solar cells. The radiative decay lifetime is dramatically reduced in a strong electric field (193?kV/cm) by efficient recombination due to strong carrier localization in each QD and significant tunneling-assisted electron escape. Conversely, an electric field of the order of 10?kV/cm maintains electronic coupling in the stacked QDs and diminishes tunneling-assisted electron escape.

Kasamatsu, Naofumi; Kada, Tomoyuki; Hasegawa, Aiko; Harada, Yukihiro; Kita, Takashi [Department of Electrical and Electronic Engineering, Graduate School of Engineering, Kobe University, 1-1 Rokkodai, Nada, Kobe 657-8501 (Japan)

2014-02-28T23:59:59.000Z

57

Spectro-polarimetric Imaging Reveals Helical Magnetic Fields in Solar Prominence Feet  

E-Print Network [OSTI]

Solar prominences are clouds of cool plasma levitating above the solar surface and insulated from the million-degree corona by magnetic fields. They form in regions of complex magnetic topology, characterized by non-potential fields, which can evolve abruptly, disintegrating the prominence and ejecting magnetized material into the heliosphere. However, their physics is not yet fully understood because mapping such complex magnetic configurations and their evolution is extremely challenging, and must often be guessed by proxy from photometric observations.Using state-of-the-art spectro-polarimetric data, we reconstruct the structure of the magnetic field in a prominence. We find that prominence feet harbor helical magnetic fields connecting the prominence to the solar surface below.

Gonzalez, M J Martinez; Ramos, A Asensio; Beck, C; Rodriguez, J de la Cruz; Diaz, A J

2015-01-01T23:59:59.000Z

58

Solar axions as an energy source and modulator of the Earth magnetic field  

E-Print Network [OSTI]

We show existence of strong negative correlation between the temporal variations of magnetic field toroidal component of the solar tachocline (the bottom of convective zone) and the Earth magnetic field (Y-component). The possibility that hypothetical solar axions, which can transform into photons in external electric or magnetic fields (the inverse Primakoff effect), can be the instrument by which the magnetic field of convective zone of the Sun modulates the magnetic field of the Earth is considered. We propose the axion mechanism of "solar dynamo-geodynamo" connection, where an energy of axions, which form in the Sun core, is modulated at first by the magnetic field of the solar tachocline zone (due to the inverse coherent Primakoff effect) and after that is absorbed in the liquid core of the Earth under influence of the terrestrial magnetic field, thereby playing the role of an energy source and a modulator of the Earth magnetic field. Within the framework of this mechanism new estimations of the strength of an axion coupling to a photon (ga_gamma about 5*10^-9 GeV^-1) and the axion mass (ma ~ 30 eV) have been obtained.

V. D. Rusov; E. P. Linnik; K. Kudela; S. Cht. Mavrodiev; T. N. Zelentsova; V. P. Smolyar; K. K. Merkotan

2010-08-16T23:59:59.000Z

59

Neutrino transition magnetic moments and the solar magnetic field on the light of the Kamland evidence  

E-Print Network [OSTI]

We present here a recopilation of recent results about the possibility of detecting solar electron antineutrinos produced by solar core and convective magnetic fields. These antineutrinos are predicted by spin-flavor oscillations at a significant rate even if this mechanism is not the leading solution to the SNP. Using the recent Kamland results and assuming a concrete model for antineutrino production by spin-flavor precession in the convective zone based on chaotic magnetic fields,we obtain bounds on the flux of solar antineutrinos, on the average conversion neutrino-antineutrino probability and on intrinsic neutrino magnetic moment. In the most conservative case, $\\mu\\lsim 2.5\\times 10^{-11} \\mu_B$ (95% CL). When studying the effects of a core magnetic field, we find in the weak limit a scaling of the antineutrino probability with respect to the magnetic field profile in the sense that the same probability function can be reproduced by any profile with a suitable peak field value. In this way the solar electron antineutrino spectrum can be unambiguosly predicted. We use this scaling and the negative results indicated by the KamLAND experiment to obtain upper bounds on the solar electron antineutrino flux. We find that, for a wide family of magnetic field profiles in the sun interior, the antineutrino appearance probability is largely determined by the magnetic field intensity but not by its shape. Explicit limits on neutrino transition moments are also obtained consistent with the convective case. These limits are therefore largerly independent of the detailed structure of the magnetic field in the solar interior.

V. Antonelli; B. C. Chauhan; J. Pulido; E. Torrente-Lujan

2003-10-29T23:59:59.000Z

60

Tracking Solar Energy Conersion Unit Adapted For Field Assembly  

DOE Patents [OSTI]

A modular solar energy collector having elongated V-shaped side walls formed by a pair of coplanar panels for each side wall. The upper panels, occupying most of the wall area are diffusely reflective, but the lower panels are specularly reflective. A Fresnel lens, having a snap fit relation to the side walls focuses some light on the lower specularly reflective panels which direct light to the solar cells at the base of the V-shaped walls. A heat sink provides support for the two panels with two opposed, upwardly extending wings terminating in opposed linear clips located near the lengthwise seam of the coplanar panels, each clip holding two coplanar panels in parallel alignment. The clips not only provide support for the panels, but also transfer heat to the remainder of the heat sink. The clips are shaped so that edges of the panels engage each clip by a snap fit, outside of the clip in one embodiment and inside of the clip in another embodiment. End caps are also formed with structures which snap to the wall panels. Since all junctions of components snap together, the collector of the present invention is easily assembled without specialized tools. Using side walls which are only partly specularly reflective permits a large angle of acceptance, yet provides an economical wall design because the entire wall need not be specularly reflective.

Kaminar, Neil R. (Boulder Creek, CA); Ross, III, James G. (Bothell, WA); Carrie, Peter J. (Toronto, CA)

2000-02-01T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Real-Time Frame Selector and its Application to Observations of the Horizontal Velocity Field in the Solar Photosphere  

Science Journals Connector (OSTI)

......RTFS at the Domeless Solar Telescope (DST) of...rapid development of PC technology, our system can evaluate...applied our RTFS to obtain solar granulation im- ages...ture is located in a SG cell boundary (figure 6a...Velocity Field in the Solar Photosphere 519 G - b......

Reizaburo Kitai; Yasuhiro Funakoshi; Satoru Ueno; Shusaku Sano; Kiyoshi Ichimoto

1997-08-01T23:59:59.000Z

62

Electron heat flow in the solar corona: Implications of non-Maxwellian velocity distributions, the solar gravitational  

E-Print Network [OSTI]

Electron heat flow in the solar corona: Implications of non-Maxwellian velocity distributions, the solar gravitational field, and Coulomb collisions John C. Dorelli Space and Atmospheric Science Group, Los Alamos National Laboratory, Los Alamos, New Mexico, USA Jack D. Scudder Department of Physics

Scudder, Jack

63

Solar nebula magnetic fields recorded in the Semarkona meteorite  

E-Print Network [OSTI]

Magnetic fields are proposed to have played a critical role in some of the most enigmatic processes of planetary formation by mediating the rapid accretion of disk material onto the central star and the formation of the ...

Fu, Roger Rennan

64

Nonlinear force-free modeling of the solar coronal magnetic field  

E-Print Network [OSTI]

The coronal magnetic field is an important quantity because the magnetic field dominates the structure of the solar corona. Unfortunately direct measurements of coronal magnetic fields are usually not available. The photospheric magnetic field is measured routinely with vector magnetographs. These photospheric measurements are extrapolated into the solar corona. The extrapolated coronal magnetic field depends on assumptions regarding the coronal plasma, e.g. force-freeness. Force-free means that all non-magnetic forces like pressure gradients and gravity are neglected. This approach is well justified in the solar corona due to the low plasma beta. One has to take care, however, about ambiguities, noise and non-magnetic forces in the photosphere, where the magnetic field vector is measured. Here we review different numerical methods for a nonlinear force-free coronal magnetic field extrapolation: Grad-Rubin codes, upward integration method, MHD-relaxation, optimization and the boundary element approach. We briefly discuss the main features of the different methods and concentrate mainly on recently developed new codes.

T. Wiegelmann

2008-01-18T23:59:59.000Z

65

The Solar Magnetic Field as a Coronal Hole Extension Forms: Effects of Magnetic Helicity and Boundary Conditions  

Science Journals Connector (OSTI)

An analytical solution is presented for linear force fields within a spherical shell, representing the solar corona. Allowing for a global magnetic helicity, we find magnetic fields over the entire corona with...

J. R. Clegg; B. J. I. Bromage; P. K. Browning

66

Simulation Study of Solar Plasma Eruptions Caused by Interactions between Emerging Flux and Coronal Arcade Fields  

E-Print Network [OSTI]

We investigate the triggering mechanisms of plasma eruptions in the solar atmosphere due to interactions between emerging flux and coronal arcade fields by using two-dimensional MHD simulations. We perform parameter surveys with respect to arcade field height, magnetic field strength, and emerging flux location. Our results show that two possible mechanisms exist, and which mechanism is dominant depends mostly on emerging flux location. One mechanism appears when the location of emerging flux is close to the polarity inversion line (PIL) of an arcade field. This mechanism requires reconnection between the emerging flux and the arcade field, as pointed out by previous studies. The other mechanism appears when the location of emerging flux is around the edge of an arcade field. This mechanism does not require reconnection between the emerging flux and the arcade field but does demand reconnection in the arcade field above the PIL. Furthermore, we found that the eruptive condition for this mechanism can be repre...

Kaneko, T

2014-01-01T23:59:59.000Z

67

Recovery of 3D Solar Magnetic Field Model Parameter Using Image Structure Matching  

Science Journals Connector (OSTI)

An approach to recover a 3D solar magnetic field model parameter using intensity images of the Sun's corona is introduced. The approach is a quantitative approach in which the 3D model parameter is determined via an image structure matching scheme. The ... Keywords: 3D Parameter Recovery, Image-based Modeling, Structure Matching

Jong Kwan Lee; G. Allen Gary

2009-05-01T23:59:59.000Z

68

MAGNETIC POWER SPECTRA DERIVED FROM GROUND AND SPACE MEASUREMENTS OF THE SOLAR MAGNETIC FIELDS  

E-Print Network [OSTI]

of gas about in the photosphere, and will evidently act in the same way upon a magnetic line of force motion is by investigating the nature of the photospheric magnetic fields in terms Solar Physics 201: 225 with an energy cascade of turbulent motions. In the turbulent fluid motion, the kinetic energy cascades from

69

Supporting Information for Screening-engineered Field-effect Solar Cells  

E-Print Network [OSTI]

Supporting Information for Screening-engineered Field-effect Solar Cells William Regan1,2, , Steven of efficiency and Voc as a function of finger separation s Figure S2. Simulated IV curves (AM1.5 illumination includes: Supporting Methods: I.A: Simulation methods for type A cells I.B: Simulation methods for type B

Zettl, Alex

70

SOLAR WIND ELECTRIC FIELDS IN THE ION CYCLOTRON FREQUENCY RANGE P. J. Kellogg,1  

E-Print Network [OSTI]

SOLAR WIND ELECTRIC FIELDS IN THE ION CYCLOTRON FREQUENCY RANGE P. J. Kellogg,1 S. D. Bale,2 F. S wind in the region near the ion cyclotron frequency of protons, larger than the force due to magnetic fluctuations. They provide sufficient velocity- space diffusion or heating to counteract conservation

California at Berkeley, University of

71

A model study of the impact of magnetic field structure on atmospheric composition during solar proton events  

E-Print Network [OSTI]

A model study of the impact of magnetic field structure on atmospheric composition during solar is possible into regions that are at the moment effectively shielded by the Earth's magnetic field. A two (process, timescale, magnetostratigraphy); 1650 Global Change: Solar variability; 2716 Magnetospheric

Steinhoff, Heinz-Jürgen

72

Exoplanet-Induced Chromospheric Activity: Realistic Light Curves from Solar-type Magnetic Fields  

E-Print Network [OSTI]

There is growing observational evidence for some kind of interaction between stars and close-in extrasolar giant planets. Shkolnik et al. reported variability in the chromospheric Ca H and K lines of HD 179949 and upsilon And that seemed to be phased with the planet's orbital period, instead of the stellar rotational period. However, the observations also indicate that the chromospheric light curves do not repeat exactly, which may be expected for a planet plowing through a variable stellar magnetic field. Using the complex solar magnetic field (modeled with the Potential Field Source Surface technique) as a guide, we simulate the shapes of light curves that would arise from planet-star interactions that are channeled along magnetic field lines. We also study the orbit-to-orbit variability of these light curves and how they vary from solar minimum (i.e., a more or less axisymmetric stretched dipole) to solar maximum (a superposition of many higher multipole moments) fields. Considering more complex magnetic fields introduces new difficulties in the interpretation of observations, but it may also lead to valuable new diagnostics of exoplanet magnetospheres.

Steven R. Cranmer; Steven H. Saar

2007-02-20T23:59:59.000Z

73

Uncertainty Analysis of Heliostat Alignment at the Sandia Solar Field  

Science Journals Connector (OSTI)

Abstract Low-cost heliostats with open-loop tracking systems require careful calibration in order to track the sun accurately. This calibration can be done by mechanical adjustment, which increases the cost of both the components and commissioning, or it can be done automatically, using software, by learning the various forms of misalignment present in a particular heliostat, and adjusting the pointing directions in order to cancel out the effect of those misalignments. A large set of training data will allow these corrections to be determined to quite high accuracy, and several of low-cost heliostat concepts have already been developed which make use of some form of this principle to reduce overall CSP system cost, though the methods used have not been thoroughly described in open literature. The current study builds upon earlier work by Baheti and Scott (1980), Khalsa et al (2011) and Pye and Zhang (2012), to analyze the process of automated misalignment correction with the introduction of an uncertainty analysis applied to an experimental training data set. The accuracy of correction process from this experimental data is quantified, allowing a criterion to be applied to determine whether or not sufficient training has been completed for each heliostat to mean overall field accuracy requirements. To investigate the potential improvements from extended training, a synthetic data set is generated, and used to investigate preferred times of year and times of data for training specific heliostats in the field. Summer data is shown to be best, but the additional of some winter data is helpful. Time-of-day is also important, especially for the sides of the heliostat field; middle-of- the-day training and spring or autumn training are seen to be less effective. A training programme for the entire heliostat field is presented and discussed: each heliostat is trained daily in summer for two minutes, and daily in winter for one minute in the morning and evening, resulting in 95% certainty that all heliostats will have their focal spot within 1.5 m of the target for the entire year, by an entirely automated process.

Rachel Hogan; John Pye; Clifford Ho; Edward Smith

2014-01-01T23:59:59.000Z

74

Field-effect BaTiO{sub 3}-Si solar cells  

SciTech Connect (OSTI)

Conventional solar cells make use of the spatial variation in electronic environment due to junctions for charge separation. We investigated field-effect BaTiO{sub 3}-Si solar cells that utilize the bound surface charges of BaTiO{sub 3} to separate charge carriers in silicon. Rectifying behavior and photovoltaic effect were observed on cells with forward polarization. Theoretical simulation indicated that the induced electric field due to BaTiO{sub 3} polarization could extend into the silicon layer, which is consistent with experimental observations. In addition, adjusting relevant parameters may optimize the electric field distribution. The cells are promising in terms of material selection, device design, and fabrication.

Wang, Wentao; Liu, Fude, E-mail: fordliu@hku.hk; Man Lau, Chor; Wang, Lei; Yang, Guandong; Zheng, Dawei [Department of Mechanical Engineering, The University of Hong Kong, Pokfulam Road, Hong Kong (China); Li, Zhigang [Department of Mechanical and Aerospace Engineering, The Hong Kong University of Science and Technology, Hong Kong (China)

2014-03-24T23:59:59.000Z

75

DECLINE AND RECOVERY OF THE INTERPLANETARY MAGNETIC FIELD DURING THE PROTRACTED SOLAR MINIMUM  

SciTech Connect (OSTI)

The interplanetary magnetic field (IMF) is determined by the amount of solar magnetic flux that passes through the top of the solar corona into the heliosphere, and by the dynamical evolution of that flux. Recently, it has been argued that the total flux of the IMF evolves over the solar cycle due to a combination of flux that extends well outside of 1 AU and is associated with the solar wind, and additionally, transient flux associated with coronal mass ejections (CMEs). In addition to the CME eruption rate, there are three fundamental processes involving conversion of magnetic flux (from transient to wind-associated), disconnection, and interchange reconnection that control the levels of each form of magnetic flux in the interplanetary medium. This is distinct from some earlier models in which the wind-associated component remains steady across the solar cycle. We apply the model of Schwadron et al. that quantifies the sources, interchange, and losses of magnetic flux to 50 yr of interplanetary data as represented by the Omni2 data set using the sunspot number as a proxy for the CME eruption rate. We do justify the use of that proxy substitution. We find very good agreement between the predicted and observed interplanetary magnetic flux. In the absence of sufficient CME eruptions, the IMF falls on the timescale of ?6 yr. A key result is that rising toroidal flux resulting from CME eruption predates the increase in wind-associated IMF.

Smith, Charles W.; Schwadron, Nathan A. [Physics Department, Space Science Center, University of New Hampshire, Durham, New Hampshire (United States); DeForest, Craig E., E-mail: Charles.Smith@unh.edu, E-mail: N.Schwadron@unh.edu, E-mail: DeForest@Boulder.SwRI.edu [Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, Colorado (United States)

2013-09-20T23:59:59.000Z

76

MAGNETIC RECONNECTION IN THE SOLAR WIND AT CURRENT SHEETS ASSOCIATED WITH EXTREMELY SMALL FIELD SHEAR ANGLES  

SciTech Connect (OSTI)

Using Wind 3 s plasma and magnetic field data, we have identified nine reconnection exhausts within a solar wind disturbance on 1998 October 18-20 driven by a moderately fast interplanetary coronal mass ejection (ICME). Three of the exhausts within the ICME were associated with current sheets having local field shear angles, {theta}, ranging from 4 Degree-Sign to 9 Degree-Sign , the smallest reported values of {theta} yet associated with reconnection exhausts in a space plasma. They were observed in plasma characterized by extremely low (0.02-0.04) plasma {beta}, and very high (281-383 km s{sup -1}) Alfven speed, V{sub A}. Low {beta} allows reconnection to occur at small {theta} and high V{sub A} leads to exhaust jets that are fast enough relative to the surrounding solar wind to be readily identified. Very small-{theta} current sheets are common in the solar wind at 1 AU, but typically are not associated with particularly low plasma {beta} or high V{sub A}. On the other hand, small-{theta} current sheets should be common in the lower solar corona, a plasma regime of extremely low {beta} and extremely high V{sub A}. Our observations lend credence to models that predict that reconnection at small-{theta} current sheets is primarily responsible for coronal heating.

Gosling, J. T. [Laboratory for Atmospheric and Space Physics, University of Colorado, 3665 Discovery Drive, Boulder, CO 80303 (United States); Phan, T. D., E-mail: jack.gosling@lasp.colorado.edu [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States)

2013-02-01T23:59:59.000Z

77

Solar Physics DOI: 10.1007/----  

E-Print Network [OSTI]

University of Cambridge SOLA: eve_Doppler.tex; 7 May 2011; 17:19; p. 1 #12;Hudson et al. Much of this energy: photosphere 1. Introduction The directly radiated energy of a solar flare represents a substantial fraction of the total energy released from the magnetic field (e.g., Emslie et al., 2005). 1SSL, UC Berkeley, CA, USA

Hudson, Hugh

78

Optical performance of vertical heliostat fields integrated in building faades for concentrating solar energy uses  

Science Journals Connector (OSTI)

Abstract One way for integrating concentrating solar energy systems based on central receiver technology in metropolitan areas consists of using building faades as frame for installing a heliostat reflector field that reflects radiation coming from the sun towards a common area where receiver is located. This work analyzes the optical performance of vertical solar field concept. It provides the effect of several geometric parameters such as receiver height, separation between heliostat edges, and different building typologies on the hourly and annual optical efficiency along the year including the contribution of different optical efficiency factors such as shadowing, blocking, cosine, and spillage. The optical efficiency of a vertical heliostat field was found to be mainly controlled by shadowing, cosine and spillage factors. The field reaches the maximum overall optical efficiency during spring and winter at noon time and the minimum ones during the summer season mainly due to shadowing factor. Results obtained for best configurations are comparable to those ones reached by traditional horizontal field arrangements, what supports the feasibility of the vertical heliostats field concept as a CSP building integrated facility.

Aurelio Gonzlez-Pardo; Sara Cesar Chapa; Jos Gonzalez-Aguilar; Manuel Romero

2013-01-01T23:59:59.000Z

79

Correlated solar wind speed, density, and magnetic field changes at J. D. Richardson and C. Wang1  

E-Print Network [OSTI]

Correlated solar wind speed, density, and magnetic field changes at Voyager 2 J. D. Richardson and C. Wang1 Center for Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts December 2003. [1] The character of the solar wind plasma data observed by Voyager 2 recently changed

Richardson, John

80

Dependence of Solar-Wind Power Spectra on the Direction of the Local Mean Magnetic Field  

Science Journals Connector (OSTI)

Wavelet analysis can be used to measure the power spectrum of solar-wind fluctuations along a line in any direction (?, ) with respect to the local mean magnetic field B 0. This technique is applied to study solar-wind turbulence in high-speed streams in the ecliptic plane near solar minimum using magnetic field measurements with a cadence of eight vectors per second. The analysis of nine high-speed streams shows that the reduced spectrum of magnetic field fluctuations (trace power) is approximately azimuthally symmetric about B 0 in both the inertial range and dissipation range; in the inertial range the spectra are characterized by a power-law exponent that changes continuously from 1.6 0.1 in the direction perpendicular to the mean field to 2.0 0.1 in the direction parallel to the mean field. The large uncertainties suggest that the perpendicular power-law indices 3/2 and 5/3 are both consistent with the data. The results are similar to those found by Horbury et al. at high heliographic latitudes. Comparisons between solar-wind observations and the theories of strong incompressible MHD turbulence developed by Goldreich & Sridhar and Boldyrev are not rigorously justified because these theories only apply to turbulence with vanishing cross-helicity although the normalized cross-helicity of solar-wind turbulence is not negligible. Assuming these theories can be generalized in such a way that the three-dimensional wavevector spectra have similar functional forms when the cross-helicity is nonzero, then for the interval of Ulysses data analyzed by Horbury et al. the ratio of the spectra perpendicular and parallel to B 0 is more consistent with the Goldreich & Sridhar scaling P ?/P ? ? ?1/3 than with the Boldyrev scaling ?1/2. The analysis of high-speed streams in the ecliptic plane does not yield a reliable measurement of this scaling law. The transition from a turbulent MHD-scale energy cascade to a kinetic Alfvn wave (KAW) cascade occurs when k ?? i 1, which coincides with the spectral break. At slightly higher wavenumbers, in the dissipation range, there is a peak in the power ratio with P ?/P ? 1. The decay of this peak may be caused by the damping of KAWs, which is predicted to occur near k ?? i 4.

J. J. Podesta

2009-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta  

E-Print Network [OSTI]

field occurs at the day side mag- netopause and this reconnection transports energy from the solar wind interplanetary ejecta Vasyl Yurchyshyn Big Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314, USA Crimean Astrophysical

Yurchyshyn, Vasyl

82

On the GCR intensity and the inversion of the heliospheric magnetic field during the periods of the high solar activity  

E-Print Network [OSTI]

We consider the long-term behavior of the solar and heliospheric parameters and the GCR intensity in the periods of high solar activity and the inversions of heliospheric magnetic field (HMF). The classification of the HMF polarity structures and the meaning of the HMF inversion are discussed. The procedure is considered how to use the known HMF polarity distribution for the GCR intensity modeling during the periods of high solar activity. We also briefly discuss the development and the nearest future of the sunspot activity and the GCR intensity in the current unusual solar cycle 24.

Krainev, M B

2014-01-01T23:59:59.000Z

83

Automated Technique For Comparison Of Magnetic Field Inversion Lines With Filament Skeletons From The Solar Feature Catalogue  

Science Journals Connector (OSTI)

We present an automated technique for comparison of magnetic field inversion-line maps from SOHO/MDI magnetograms with solar ... component labelling are used to identify nearest inversion lines to filament skelet...

S. S. Ipson; V. V. Zharkova; S. Zharkov; A. K. Benkhalil; J. Aboudarham

2005-05-01T23:59:59.000Z

84

ENERGETIC PARTICLE CROSS-FIELD PROPAGATION EARLY IN A SOLAR EVENT  

SciTech Connect (OSTI)

Solar energetic particles (SEPs) have been observed to easily spread across heliographic longitudes, and the mechanisms responsible for this behavior remain unclear. We use full-orbit simulations of a 10 MeV proton beam in a turbulent magnetic field to study to what extent the spread across the mean field can be described as diffusion early in a particle event. We compare the full-orbit code results to solutions of a Fokker-Planck equation including spatial and pitch angle diffusion, and of one including also propagation of the particles along random-walking magnetic field lines. We find that propagation of the particles along meandering field lines is the key process determining their cross-field spread at 1 AU at the beginning of the simulated event. The mean square displacement of the particles an hour after injection is an order of magnitude larger than that given by the diffusion model, indicating that models employing spatial cross-field diffusion cannot be used to describe early evolution of an SEP event. On the other hand, the diffusion of the particles from their initial field lines is negligible during the first 5 hr, which is consistent with the observations of SEP intensity dropouts. We conclude that modeling SEP events must take into account the particle propagation along meandering field lines for the first 20 hr of the event.

Laitinen, T.; Dalla, S.; Marsh, M. S. [Jeremiah Horrocks Institute, University of Central Lancashire, PR1 2HE Preston (United Kingdom)

2013-08-20T23:59:59.000Z

85

TWIST AND CONNECTIVITY OF MAGNETIC FIELD LINES IN THE SOLAR ACTIVE REGION NOAA 10930  

SciTech Connect (OSTI)

Twist and connectivity of magnetic field lines in the flare-productive active region NOAA 10930 are investigated in terms of the vector magnetograms observed by the Solar Optical Telescope on board the Hinode satellite and the nonlinear force-free field (NLFFF) extrapolation. First, we show that the footpoints of magnetic field lines reconstructed by the NLFFF correspond well to the conjugate pair of highly sheared flare ribbons on the Ca II images, which were observed by Hinode as an X3.4 class flare on 2006 December 13. This demonstrates that the NLFFF extrapolation may be used to analyze the magnetic field connectivity. Second, we find that the twist of magnetic field lines anchored on the flare ribbons increased as the ribbons moved away from the magnetic polarity inversion line in the early phase of the flare. This suggests that magnetic reconnection might commence from a region located below the most strongly twisted field. Third, we reveal that the magnetic flux twisted more than a half turn and gradually increased during the last one day prior to the onset of the flare, and that it quickly decreased for two hours after the flare. This is consistent with the store-and-release scenario of magnetic helicity. However, within this active region, only a small fraction of the flux was twisted by more than one full turn and the field lines that reconnected first were twisted less than one turn. These results imply that the kink mode instability could hardly occur, at least before the onset of flare. Based on our results, we discuss the trigger process of solar flares.

Inoue, S. [National Institute of Information and Communications Technology (NICT), 4-2-1, Nukui-Kitamachi, koganei, Tokyo 184-8795 (Japan); Kusano, K.; Yamamoto, T. T. [Solar-Terrestrial Environment Laboratory, Nagoya University Furo-cho, Chikusa-ku, Nagoya, 464-8601 (Japan); Magara, T. [Department of Astronomy and Space Science, School of Space Research, Kyung Hee University, 1, Seocheon-dong, Giheung-gu, Yongin, Gyeonggi-do, 446-701 (Korea, Republic of); Shiota, D., E-mail: inosato@nict.go.jp [Advanced Science Institute, RIKEN - Institute of Physics and Chemical Research, Wako, Saitama 351-0198 (Japan)

2011-09-10T23:59:59.000Z

86

The Astrophysical Journal, 701:19111921, 2009 August 20 doi:10.1088/0004-637X/701/2/1911 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

the convection zone is a central process of solar physics. The intense magnetic fields that constitute active. The American Astronomical Society. All rights reserved. Printed in the U.S.A. CURRENT BUILDUP IN EMERGING; accepted 2009 July 6; published 2009 August 6 ABSTRACT The increase of magnetic flux in the solar

Demoulin, Pascal

87

SOLAR WAVE-FIELD SIMULATION FOR TESTING PROSPECTS OF HELIOSEISMIC MEASUREMENTS OF DEEP MERIDIONAL FLOWS  

SciTech Connect (OSTI)

The meridional flow in the Sun is an axisymmetric flow that is generally directed poleward at the surface, and is presumed to be of fundamental importance in the generation and transport of magnetic fields. Its true shape and strength, however, are debated. We present a numerical simulation of helioseismic wave propagation in the whole solar interior in the presence of a prescribed, stationary, single-cell, deep meridional circulation serving as synthetic data for helioseismic measurement techniques. A deep-focusing time-distance helioseismology technique is applied to the synthetic data, showing that it can in fact be used to measure the effects of the meridional flow very deep in the solar convection zone. It is shown that the ray approximation that is commonly used for interpretation of helioseismology measurements remains a reasonable approximation even for very long distances between 12 Degree-Sign and 42 Degree-Sign corresponding to depths between 52 and 195 Mm. From the measurement noise, we extrapolate that time-resolved observations on the order of a full solar cycle may be needed to probe the flow all the way to the base of the convection zone.

Hartlep, T.; Zhao, J.; Kosovichev, A. G. [W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA (United States)] [W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA (United States); Mansour, N. N. [NASA Ames Research Center, Moffett Field, CA (United States)] [NASA Ames Research Center, Moffett Field, CA (United States)

2013-01-10T23:59:59.000Z

88

A bibliographic analysis of recent solar energy literatures: The expansion and evolution of a research field  

Science Journals Connector (OSTI)

Abstract This paper characterizes the solar energy literature from 1992 to 2011 using bibliometric techniques based on databases of the Science Citation Index and the Social Science Citation Index. Journal articles were the most frequently used document type representing 86.4% (6670) of the records. The pace of publishing in this field increased exponentially over these two decades, with the US accounting for the highest h-index (87) and the most publications (1273), followed by China and India. The US also plays a central role in the collaboration network among the 20 most productive countries, while China and India do not because of their more limited cross-national authorships. The Indian Institute of Technology was the organization with the most records (126), but it has few multinational co-authored articles. In contrast, the Paul Scherrer Institute in Switzerland is central to the collaboration network. The largest number of retrieved journal articles was in the area of energy applications (1059 articles) followed by light absorbing materials (983) and solar cells (420). Energy applications mainly address hydrogen, desalination, air conditioning, drying, heat pumps, biomass, and water splitting, while the light absorbing material mainly cover nano materials, TiO2, semiconductors, thin films, phase change material and so on. This analysis not only identifies global hotspots in solar energy research, but may also influence researchers' selection of future studies and publications.

Huibin Du; Na Li; Marilyn A. Brown; Yuenuan Peng; Yong Shuai

2014-01-01T23:59:59.000Z

89

University of Tennessee, USA Georgia State University, USA Johns Hopkins Medicine Institute, USA University of Virginia, USA  

E-Print Network [OSTI]

#12; : University of Tennessee, USA Georgia State University, USA Johns Hopkins Medicine Institute, USA University of Virginia, USA Columbia University, USA Queen's University, Canada University of Akron, USA

Wang, Jianbo

90

On fibrils and field lines: The nature of H$\\alpha$ fibrils in the solar chromosphere  

E-Print Network [OSTI]

Observations of the solar chromosphere in the line-core of the \\Halpha\\ line show dark elongated structures called fibrils that show swaying motion. We performed a 3D radiation-MHD simulation of a network region, and computed synthetic \\Halpha\\ images from this simulation to investigate the relation between fibrils and the magnetic field lines in the chromosphere. The periods, amplitudes and phase-speeds of the synthetic fibrils are consistent with those observed. We analyse the relation between the synthetic fibrils and the field lines threading through them, and find that some fibrils trace out the same field line along the fibril's length, but there are also fibrils that sample different field lines at different locations along their length. Fibrils sample the same field lines on a time scale of $\\sim200$~s. This is shorter than their own lifetime. We analysed the evolution of the atmosphere along a number of field lines that thread through fibrils and find that they carry slow-mode waves that load mass in...

Leenaarts, Jorrit; van der Voort, Luc Rouppe

2015-01-01T23:59:59.000Z

91

Hanle effect in the solar Ba II D2 line: a diagnostic tool for chromospheric weak magnetic fields  

E-Print Network [OSTI]

The physics of the solar chromosphere depends in a crucial way on its magnetic structure. However there are presently very few direct magnetic field diagnostics available for this region. Here we investigate the diagnostic potential of the Hanle effect on the Ba II D2 line resonance polarization for the determination of weak chromospheric turbulent magnetic fields......

M. Faurobert; M. Derouich; V. Bommier; J. Arnaud

2008-11-07T23:59:59.000Z

92

Ferroelectric field effect of the bulk heterojunction in polymer solar cells  

SciTech Connect (OSTI)

A ferroelectric field effect in the bulk heterojunction was found when an external electric field (EEF) was applied on the active layer of polymer solar cells (PSCs) during the annealing process of the active layer spin-coated with poly(3-hexylthiophene):[6,6]-phenyl-C{sub 61} butyric acid methyl ester. For one direction field, the short circuit current density of PSCs was improved from 7.2 to 8.0?mA/cm{sup 2}, the power conversion efficiency increased from 2.4% to 2.8%, and the incident photon-to-current conversion efficiency increased from 42% to 49% corresponding to the different EEF magnitude. For an opposite direction field, the applied EEF brought a minus effect on the performance mentioned above. EEF treatment can orientate molecular ordering of the polymer, and change the morphology of the active layer. The authors suggest a explanation that the ferroelectric field has been built in the active layer, and therefore it plays a key role in PSCs system. A needle-like surface morphology of the active film was also discussed.

Li, Meng; Ma, Heng, E-mail: hengma@henannu.edu.cn; Liu, Hairui; Jiang, Yurong [College of Physics and Electronic Engineering, Henan Normal University, Xinxiang 453007 (China); Henan Key Laboratory of Photovoltaic Materials, Xinxiang 453007 (China); Niu, Heying; Amat, Adil [College of Physics and Electronic Engineering, Henan Normal University, Xinxiang 453007 (China)

2014-06-23T23:59:59.000Z

93

PROPAGATING WAVES TRANSVERSE TO THE MAGNETIC FIELD IN A SOLAR PROMINENCE  

SciTech Connect (OSTI)

We report an unusual set of observations of waves in a large prominence pillar that consist of pulses propagating perpendicular to the prominence magnetic field. We observe a huge quiescent prominence with the Solar Dynamics Observatory Atmospheric Imaging Assembly in EUV on 2012 October 10 and only a part of it, the pillar, which is a foot or barb of the prominence, with the Hinode Solar Optical Telescope (SOT; in Ca II and H? lines), Sac Peak (in H?, H?, and Na-D lines), and THEMIS ({sup T}lescope Hliographique pour l' Etude du Magntisme et des Instabilits Solaires{sup )} with the MTR (MulTi-Raies) spectropolarimeter (in He D{sub 3} line). The THEMIS/MTR data indicates that the magnetic field in the pillar is essentially horizontal and the observations in the optical domain show a large number of horizontally aligned features on a much smaller scale than the pillar as a whole. The data are consistent with a model of cool prominence plasma trapped in the dips of horizontal field lines. The SOT and Sac Peak data over the four hour observing period show vertical oscillations appearing as wave pulses. These pulses, which include a Doppler signature, move vertically, perpendicular to the field direction, along thin quasi-vertical columns in the much broader pillar. The pulses have a velocity of propagation of about 10 km s{sup 1}, a period of about 300 s, and a wavelength around 2000 km. We interpret these waves in terms of fast magnetosonic waves and discuss possible wave drivers.

Schmieder, B. [Observatoire de Paris, LESIA, UMR 8109 (CNRS), F-92195 Meudon (France); Kucera, T. A.; Knizhnik, K. [Code 671, NASA's GSFC, Greenbelt, MD 20771 (United States); Luna, M. [Instituto de Astrofsica de Canarias, E-38200 La Laguna, Tenerife (Spain); Lopez-Ariste, A. [THEMIS, CNRS-UPS853, E-38205 La Laguna (Spain); Toot, D. [Alfred University, Alfred, NY 14802 (United States)

2013-11-10T23:59:59.000Z

94

Numerical simulations for high efficiency HIT solar cells using microcrystalline silicon as emitter and back surface field (BSF) layers  

Science Journals Connector (OSTI)

Abstract In present article the influence of thickness and band gap of microcrystalline silicon emitter layer, amorphous silicon front and back intrinsic layers and p-type crystalline silicon (c-Si) wafer thickness on the performance of TCO/?c-Si:H(n)/a-Si:H(i)/c-Si(p)/a-Si:H(i)/?c-Si:H(p+)/Ag Heterojunction with thin intrinsic layer (HIT) solar cell along with other structural possibilities were investigated through computer simulations using AFORS-HET software. These simulations revealed the importance of inclusion of intrinsic a-Si:H thin layer in improving the performance of solar cell with the help of interface passivation. Also microcrystalline BSF can raise the conversion efficiency more than 4% compared to HIT solar cell having no BSF layer. Highest stable efficiency of 24.12% for p-type substrate based HITBSF (HIT with back surface field) solar cells was observed. Furthermore the effect of textured transparent conductive oxide (TCO) on solar cells was investigated where the enhanced light trapping was observed with the use of textured TCO surface which raised the performance of solar cells. These optimizations may help in fabricating ?c-Si emitter and BSF based HIT solar cells with stable efficiencies compared to possibly degraded efficiencies as in case of a-Si:H based HIT solar cell structures studied so far.

Arti Rawat; Mansi Sharma; Deepika Chaudhary; S. Sudhakar; Sushil Kumar

2014-01-01T23:59:59.000Z

95

Solar Blog  

Office of Environmental Management (EM)

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Using solar energy at home can help you save...

96

Solar Physics A Journal for Solar and Solar-  

E-Print Network [OSTI]

. With society's increased dependence on space-based technology, much of which is at risk due to solar activity1 23 Solar Physics A Journal for Solar and Solar- Stellar Research and the Study of Solar-010-9653- x Solar Polar Fields During Cycles 21??? 23: Correlation with Meridional Flows #12;1 23 Your article

Padmanabhan, Janardhan

97

A new method for the design of the heliostat field layout for solar tower power plant  

Science Journals Connector (OSTI)

A new method for the design of the heliostat field layout for solar tower power plant is proposed. In the new method, the heliostat boundary is constrained by the receiver geometrical aperture and the efficiency factor which is the product of the annual cosine efficiency and the annual atmospheric transmission efficiency of heliostat. With the new method, the annual interception efficiency does not need to be calculated when places the heliostats, therefore the total time of design and optimization is saved significantly. Based on the new method, a new code for heliostat field layout design (HFLD) has been developed and a new heliostat field layout for the PS10 plant at the PS10 location has been designed by using the new code. Compared with current PS10 layout, the new designed heliostats have the same optical efficiency but with a faster response speed. In addition, to evaluate the feasibility of crops growth on the field land under heliostats, a new calculation method for the annual sunshine duration on the land surface is proposed as well.

Xiudong Wei; Zhenwu Lu; Zhifeng Wang; Weixing Yu; Hongxing Zhang; Zhihao Yao

2010-01-01T23:59:59.000Z

98

On Polar Magnetic Field Reversal and Surface Flux Transport During Solar Cycle 24  

E-Print Network [OSTI]

As each solar cycle progresses, remnant magnetic flux from active regions (ARs) migrates poleward to cancel the old-cycle polar field. We describe this polarity reversal process during Cycle 24 using four years (2010.33--2014.33) of line-of-sight magnetic field measurements from the Helioseismic and Magnetic Imager. The total flux associated with ARs reached maximum in the north in 2011, more than two years earlier than the south; the maximum is significantly weaker than Cycle 23. The process of polar field reversal is relatively slow, north-south asymmetric, and episodic. We estimate that the global axial dipole changed sign in October 2013; the northern and southern polar fields (mean above 60$^\\circ$ latitude) reversed in November 2012 and March 2014, respectively, about 16 months apart. Notably, the poleward surges of flux in each hemisphere alternated in polarity, giving rise to multiple reversals in the north. We show that the surges of the trailing sunspot polarity tend to correspond to normal mean AR ...

Sun, Xudong; Liu, Yang; Zhao, Junwei

2014-01-01T23:59:59.000Z

99

THE EFFECTS OF MAGNETIC-FIELD GEOMETRY ON LONGITUDINAL OSCILLATIONS OF SOLAR PROMINENCES  

SciTech Connect (OSTI)

We investigate the influence of the geometry of the solar filament magnetic structure on the large-amplitude longitudinal oscillations. A representative filament flux tube is modeled as composed of a cool thread centered in a dipped part with hot coronal regions on either side. We have found the normal modes of the system and establish that the observed longitudinal oscillations are well described with the fundamental mode. For small and intermediate curvature radii and moderate to large density contrast between the prominence and the corona, the main restoring force is the solar gravity. In this full wave description of the oscillation a simple expression for the oscillation frequencies is derived in which the pressure-driven term introduces a small correction. We have also found that the normal modes are almost independent of the geometry of the hot regions of the tube. We conclude that observed large-amplitude longitudinal oscillations are driven by the projected gravity along the flux tubes and are strongly influenced by the curvature of the dips of the magnetic field in which the threads reside.

Luna, M. [CRESST and Space Weather Laboratory NASA/GSFC, Greenbelt, MD 20771 (United States); Diaz, A. J. [Instituto de Astrofisica de Canarias, E-38200 La Laguna, Tenerife (Spain); Karpen, J. [NASA/GSFC, Greenbelt, MD 20771 (United States)

2012-09-20T23:59:59.000Z

100

OBSERVATIONS AND MAGNETIC FIELD MODELING OF A SOLAR POLAR CROWN PROMINENCE  

SciTech Connect (OSTI)

We present observations and magnetic field modeling of the large polar crown prominence that erupted on 2010 December 6. Combination of Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) and STEREO{sub B}ehind/EUVI allows us to see the fine structures of this prominence both at the limb and on the disk. We focus on the structures and dynamics of this prominence before the eruption. This prominence contains two parts: an active region part containing mainly horizontal threads and a quiet-Sun part containing mainly vertical threads. On the northern side of the prominence channel, both AIA and EUVI observe bright features which appear to be the lower legs of loops that go above then join in the filament. Filament materials are observed to frequently eject horizontally from the active region part to the quiet-Sun part. This ejection results in the formation of a dense-column structure (concentration of dark vertical threads) near the border between the active region and the quiet Sun. Using the flux rope insertion method, we create nonlinear force-free field models based on SDO/Helioseismic and Magnetic Imager line-of-sight magnetograms. A key feature of these models is that the flux rope has connections with the surroundings photosphere, so its axial flux varies along the filament path. The height and location of the dips of field lines in our models roughly replicate those of the observed prominence. Comparison between model and observations suggests that the bright features on the northern side of the channel are the lower legs of the field lines that turn into the flux rope. We suggest that plasma may be injected into the prominence along these field lines. Although the models fit the observations quiet well, there are also some interesting differences. For example, the models do not reproduce the observed vertical threads and cannot explain the formation of the dense-column structure.

Su Yingna; Van Ballegooijen, Adriaan, E-mail: ynsu@head.cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States)

2012-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Equations of State for Collisionless Guide-Field Reconnection J. Egedal,1  

E-Print Network [OSTI]

. Fox,1 and N. Katz1 1 Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA 2 Los, including solar flares, coronal mass ejections, magnetic storms in the Earth's magnetosphere, and sawtooth] and by spacecraft in Earth's magnetotail and the far solar wind [2,3]. In guide-field reconnection, the parallel

Egedal, Jan

102

Biological solar energy  

Science Journals Connector (OSTI)

...over the same time period, solar energy incident on our planet...represents energy conversion from solar of 0.1 to 1.0% efficiency...in some parts of the USA and Canada, as well as in India and the...require the biomass crops to have solar energy conversion efficiencies...

2007-01-01T23:59:59.000Z

103

Photoelectrochemical solar cells  

Science Journals Connector (OSTI)

Photoelectrochemical solar cells ... Plastic Solar Cells: A Multidisciplinary Field To Construct Chemical Concepts from Current Research ... Plastic Solar Cells: A Multidisciplinary Field To Construct Chemical Concepts from Current Research ...

John T. McDevitt

1984-01-01T23:59:59.000Z

104

Magnetic connections of solar formations inside magneto-isolated complexes based on observations of arch structures and calculations of magnetic field lines  

Science Journals Connector (OSTI)

The magnetic connections of solar formations inside magneto-isolated ... corona, as well as from calculations of magnetic field lines. It was found that 65% of the constructed field lines are closed within comple...

V. G. Fainshtein; V. M. Malashchuk

2013-06-01T23:59:59.000Z

105

Solar Energy Education. Home economics: teacher's guide. Field test edition. [Includes glossary  

SciTech Connect (OSTI)

An instructional aid is provided for home economics teachers who wish to integrate the subject of solar energy into their classroom activities. This teacher's guide was produced along with the student activities book for home economics by the US Department of Energy Solar Energy Education. A glossary of solar energy terms is included. (BCS)

Not Available

1981-06-01T23:59:59.000Z

106

Solar Energy Education. Industrial arts: teacher's guide. Field test edition. [Includes glossary  

SciTech Connect (OSTI)

An instructional aid is presented which integrates the subject of solar energy into the classroom study of industrial arts. This guide for teachers was produced in addition to the student activities book for industrial arts by the USDOE Solar Energy Education. A glossary of solar energy terms is included. (BCS)

Not Available

1981-05-01T23:59:59.000Z

107

Solar Energy Education. Social studies: activities and teacher's guide. Field test edition  

SciTech Connect (OSTI)

Solar energy information is made available to students through classroom instruction by way of the Solar Energy Education teaching manuals. In this manual solar energy, as well as other energy sources like wind power, is introduced by performing school activities in the area of social studies. A glossary of energy related terms is included. (BCS)

Not Available

1982-01-01T23:59:59.000Z

108

RFID TECHNOLOGY FOR AVI: FIELD DEMONSTRATION OF A WIRELESS SOLAR POWERED E-ZPASS1  

E-Print Network [OSTI]

mark of the Port Authority of New York and New Jersey #12;- 2 - ROADWAY SIDE MOUNT SOLAR PANEL OUTPUT Bluetooth GROUND/POLE-MOUNT CABINET CHARGER BATTERY ARRAY MGATE I READER OVERHEAD SOLAR PANEL (POLE MOUNTGateTM tag reader, antenna, solar panel, batteries and charger, enclosure and a pocket PC (PPC). A schematic

Mitchell, John E.

109

CORONAL MAGNETIC FIELD MEASUREMENT FROM EUV IMAGES MADE BY THE SOLAR DYNAMICS OBSERVATORY  

SciTech Connect (OSTI)

By measuring the geometrical properties of the coronal mass ejection (CME) flux rope and the leading shock observed on 2010 June 13 by the Solar Dynamics Observatory (SDO) mission's Atmospheric Imaging Assembly we determine the Alfven speed and the magnetic field strength in the inner corona at a heliocentric distance of {approx}1.4 Rs. The basic measurements are the shock standoff distance ({Delta}R) ahead of the CME flux rope, the radius of curvature of the flux rope (R{sub c}), and the shock speed. We first derive the Alfvenic Mach number (M) using the relationship, {Delta}R/R{sub c} = 0.81[({gamma}-1) M{sup 2} + 2]/[({gamma}+1)(M{sup 2} - 1)], where {gamma} is the only parameter that needed to be assumed. For {gamma} = 4/3, the Mach number declined from 3.7 to 1.5 indicating shock weakening within the field of view of the imager. The shock formation coincided with the appearance of a type II radio burst at a frequency of {approx}300 MHz (harmonic component), providing an independent confirmation of the shock. The shock compression ratio derived from the radio dynamic spectrum was found to be consistent with that derived from the theory of fast-mode MHD shocks. From the measured shock speed and the derived Mach number, we found the Alfven speed to increase from {approx}140 km s{sup -1} to 460 km s{sup -1} over the distance range 1.2-1.5 Rs. By deriving the upstream plasma density from the emission frequency of the associated type II radio burst, we determined the coronal magnetic field to be in the range 1.3-1.5 G. The derived magnetic field values are consistent with other estimates in a similar distance range. This work demonstrates that the EUV imagers, in the presence of radio dynamic spectra, can be used as coronal magnetometers.

Gopalswamy, Nat; Akiyama, Sachiko; Maekelae, Pertti; Yashiro, Seiji [NASA Goddard Space Flight Center, Greenbelt, MD 20771-0001 (United States); Nitta, Nariaki [Lockheed-Martin Solar and Astrophysics Laboratory, Palo Alto, CA 94304 (United States)

2012-01-01T23:59:59.000Z

110

ORGANIZATION Aarti Gupta (NEC, USA)  

E-Print Network [OSTI]

ORGANIZATION CHAIRS Aarti Gupta (NEC, USA) Panagiotis Manolios (Georgia Tech, USA) LOCAL ARRANGEMENTS Jeremy Levitt (Mentor Graphics, USA) Vigyan Singhal (Oski, USA) PANELS Andreas Kuehlmann (Cadence, USA) TUTORIALS Leonardo de Moura (SRI, USA) WEBMASTERS Sudarshan Srinivasan (Georgia Tech, USA) Daron

Manolios, Panagiotis "Pete"

111

The field test and optimization of a solar assisted heat pump system for space heating in extremely cold area  

Science Journals Connector (OSTI)

Abstract As a kind of sustainable energy source, solar energy is becoming highly valued. Especially in extremely cold areas, the amount of energy consumed for space heating is huge, and the conventional coal heating has polluted the environment seriously, therefore solar heating is significant on both energy and environment conservation. In this study, a solar assisted heat pump (SAHP) system was investigated for space heating under extremely cold climatic condition. The system principle and operation modes was presented, and then the project profile and design procedure were introduced, and finally the system performance was evaluated by field test on typical winter days and modeling via TRNSYS simulation environment. The results show that the solar collector efficiency was 51%, and the solar fraction can reach 66% in December. Economic analysis was also performed and the heating expenses for the present SAHP system was 18RMB/m2. Finally, the temperatures of solar energy for both direct heating and storage and only for direct heating (T1A and T1B) were simulated and optimized, which have important significance on the operation time of different operation modes.

Huifang Liu; Yiqiang Jiang; Yang Yao

2014-01-01T23:59:59.000Z

112

Coronal Magnetic Field Measurement from EUV Images made by the Solar Dynamics Observatory  

E-Print Network [OSTI]

By measuring the geometrical properties of the coronal mass ejection (CME) flux rope and the leading shock observed on 2010 June 13 by the Solar Dynamics Observatory (SDO) mission's Atmospheric Imaging Assembly (AIA) we determine the Alfv\\'en speed and the magnetic field strength in the inner corona at a heliocentric distance of ~ 1.4 Rs. The basic measurements are the shock standoff distance (deltaR) ahead of the CME flux rope, the radius of curvature of the flux rope (Rc), and the shock speed. We first derive the Alfv\\'enic Mach number (M) using the relationship, deltaR/Rc = 0.81[(gamma-1) M^2 + 2]/[(gamma+1)(M^2-1)], where gamma is the only parameter that needed to be assumed. For gamma =4/3, the Mach number declined from 3.7 to 1.5 indicating shock weakening within the field of view of the imager. The shock formation coincided with the appearance of a type II radio burst at a frequency of ~300 MHz (harmonic component), providing an independent confirmation of the shock. The shock compression ratio derived...

Gopalswamy, Nat; Akiyama, Sachiko; Mkel, Pertti; Yashiro, Seiji

2011-01-01T23:59:59.000Z

113

Geothermal Energy Production Coupled with CCS: a Field Demonstration at the SECARB Cranfield Site, Cranfield, Mississippi, USA  

Science Journals Connector (OSTI)

Abstract A major global research and development effort is underway to commercialize carbon capture and storage (CCS) as a method to mitigate climate change. Recent studies have shown the potential to couple CCS with geothermal energy extraction using supercritical CO2 (ScCO2) as the working fluid. In a geothermal reservoir, the working fluid produces electricity as a byproduct of the CCS process by mining heat out of a reservoir as it is circulated between injector and producer wells. While ScCO2 has lower heat capacity than water, its lower viscosity more than compensates by providing for greater fluid mobility. Furthermore, CO2 exhibits high expansivity and compressibility, which can both help reduce parasitic loads in fluid cycling. Given the high capital costs for developing the deep well infrastructure for geologic storage of CO2, the potential to simultaneously produce geothermal energy is an attractive method to offset some of the costs and added energy requirements for separating and transporting the waste CO2 stream. We present here the preliminary design and reservoir engineering associated with the development of direct-fired turbomachinery for pilot-scale deployment at the SECARB Cranfield Phase III CO2 Storage Project, in Cranfield, Mississippi, U.S.A. The pilot-scale deployment leverages the prior investment in the Cranfield Phase III research site, providing the first ever opportunity to acquire combined CO2 storage/geothermal energy extraction data necessary to address the uncertainties involved in this novel technique. At the SECARB Cranfield Site, our target reservoir, the Tuscaloosa Formation, lies at a depth of 3.0km, and an initial temperature of 127C. A CO2 injector well and two existing observation wells are ideally suited for establishing a CO2 thermosiphon and monitoring the thermal and pressure evolution of the well-pair on a timescale that can help validate coupled models. It is hoped that this initial demonstration on a pre-commercial scale can accelerate commercialization of combined CCS/geothermal energy extraction by removing uncertainties in system modeling.

Barry Freifeld; Steven Zakim; Lehua Pan; Bruce Cutright; Ming Sheu; Christine Doughty; Timothy Held

2013-01-01T23:59:59.000Z

114

Report on the analysis of field data relating to the reliability of solar hot water systems.  

SciTech Connect (OSTI)

Utilities are overseeing the installations of thousand of solar hot water (SHW) systems. Utility planners have begun to ask for quantitative measures of the expected lifetimes of these systems so that they can properly forecast their loads. This report, which augments a 2009 reliability analysis effort by Sandia National Laboratories (SNL), addresses this need. Additional reliability data have been collected, added to the existing database, and analyzed. The results are presented. Additionally, formal reliability theory is described, including the bathtub curve, which is the most common model to characterize the lifetime reliability character of systems, and for predicting failures in the field. Reliability theory is used to assess the SNL reliability database. This assessment shows that the database is heavily weighted with data that describe the reliability of SHW systems early in their lives, during the warranty period. But it contains few measured data to describe the ends of SHW systems lives. End-of-life data are the most critical ones to define sufficiently the reliability of SHW systems in order to answer the questions that the utilities pose. Several ideas are presented for collecting the required data, including photometric analysis of aerial photographs of installed collectors, statistical and neural network analysis of energy bills from solar homes, and the development of simple algorithms to allow conventional SHW controllers to announce system failures and record the details of the event, similar to how aircraft black box recorders perform. Some information is also presented about public expectations for the longevity of a SHW system, information that is useful in developing reliability goals.

Menicucci, David F. (Building Specialists, Inc., Albuquerque, NM)

2011-07-01T23:59:59.000Z

115

Investigation of Force-Freeness of Solar Emerging Magnetic Field via Application of the Virial Theorem to MHD Simulations  

E-Print Network [OSTI]

Force-freeness of a solar magnetic field is a key to reconstructing invisible coronal magnetic structure of an emerging flux region on the Sun where active phenomena such as flares and coronal mass ejections frequently occur. We have performed magnetohydrodynamic (MHD) simulations which are adjusted to investigate force-freeness of an emerging magnetic field by using the virial theorem. Our focus is on how the force-free range of an emerging flux region develops and how it depends on the twist of a pre-emerged magnetic field. As an emerging flux region evolves, the upper limit of the force-free range continuously increases while the lower limit is asymptotically reduced to the order of a photospheric pressure scale height above the solar surface. As the twist becomes small the lower limit increases and then seems to be saturated. We also discuss the applicability of the virial theorem to an evolving magnetic structure on the Sun.

Kang, Jihye

2014-01-01T23:59:59.000Z

116

The Astrophysical Journal, 629:L65L68, 2005 August 10 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.  

E-Print Network [OSTI]

), although no naturally occurring radiation had been confirmed as TR. In an astrophysical context, TR must. All rights reserved. Printed in U.S.A. SPATIAL EVIDENCE FOR TRANSITION RADIATION IN A SOLAR RADIO and electric and magnetic fields, is of great interest in astrophysical plasmas, but occurs on spatial scales

117

Solar News  

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

news Office of Energy Efficiency & Renewable news Office of Energy Efficiency & Renewable Energy Forrestal Building 1000 Independence Avenue, SW Washington, DC 20585 en Energy Department Announces $19 Million to Drive Down Solar Soft Costs, Increase Hardware Efficiency http://energy.gov/eere/articles/energy-department-announces-19-million-drive-down-solar-soft-costs-increase-hardware solar-soft-costs-increase-hardware" class="title-link">Energy Department Announces $19 Million to Drive Down Solar Soft Costs, Increase Hardware Efficiency

118

Field lines twisting in a noisy corona: implications for energy storage and release, and initiation of solar eruptions  

E-Print Network [OSTI]

We present simulations modeling closed regions of the solar corona threaded by a strong magnetic field where localized photospheric vortical motions twist the coronal field lines. The linear and nonlinear dynamics are investigated in the reduced magnetohydrodynamic regime in Cartesian geometry. Initially the magnetic field lines get twisted and the system becomes unstable to the internal kink mode, confirming and extending previous results. As typical in this kind of investigations, where initial conditions implement smooth fields and flux-tubes, we have neglected fluctuations and the fields are laminar until the instability sets in. But previous investigations indicate that fluctuations, excited by photospheric motions and coronal dynamics, are naturally present at all scales in the coronal fields. Thus, in order to understand the effect of a photospheric vortex on a more realistic corona, we continue the simulations after kink instability sets in, when turbulent fluctuations have already developed in the co...

Rappazzo, A F; Einaudi, G

2013-01-01T23:59:59.000Z

119

Field synergy principle analysis for reducing natural convection heat loss of a solar cavity receiver  

Science Journals Connector (OSTI)

Abstract Due to the operating temperature from 900K to 1300K produced by the concentrating ratio over 2000 in solar parabolic dish-engine system, the natural convection heat loss driven by the buoyancy force of air contributes an important role in the energy loss of cavity receiver. 3-D numerical simulations were performed and the results are analyzed from the novel viewpoint of field synergy principle (FSP) in order to study the heat transfer and fluid flow characteristics in natural convection heat loss of cavity receiver. The effects of geometric parameters, including the inclination angle, aperture size, aperture position and cavity geometric shape on the natural convection heat loss of cavity receiver were examined. The FSP analysis on the simulation results demonstrates that FSP can well explain the reduction mechanism for natural convection heat loss of cavity receiver because the smaller inner production of velocity vector and temperature gradient always corresponds to the lower Nusselt number occurred in the cases with lager inclination angle, smaller aperture size, lower aperture position and frustum-cylinder cavity, respectively. Therefore, the reducing natural convection heat loss attributes to the weakening synergy between velocity vector and temperature gradient. In addition, the local heat transfer performance is studied by the presented distributions of heat transferred via fluid motion, where more interesting natural convection heat loss characteristics of cavity receiver and the detailed explanations were provided. The results of this work offer benefits for the development of theory and technique about reducing natural convection heat loss of cavity receiver.

Yuqiang Li; Gang Liu; Zhenghua Rao; Shengming Liao

2015-01-01T23:59:59.000Z

120

Determination of Topology Skeleton of Magnetic Fields in a Solar Active Region  

E-Print Network [OSTI]

The knowledge of magnetic topology is the key to understand magnetic energy release in astrophysics. Based on observed vector magnetograms, we have determined threedimensional (3D) topology skeleton of the magnetic fields in active region NOAA 10720. The skeleton consists of six 3D magnetic nulls and a network of corresponding spines, fans, and null-null lines. For the first time, we have identified a spiral magnetic null in Sun's corona. The magnetic lines of force twisted around the spine of the null, forming a 'magnetic wreath' with excess of free magnetic energy and resembling observed brightening structures at extraultraviolet (EUV) wavebands. We found clear evidence of topology eruptions which are referred to as the catastrophic changes of topology skeleton associated with a coronal mass ejection (CME) and an explosive X-ray flare. These results shed new lights in exploring the structural complexity and its role in explosive magnetic activity. In solar astrophysics and space science, the concept of flux rope has been widely used in modelling explosive magnetic activity, although their observational identity is obscure or, at least, lacking of necessary details. The current work suggests that the magnetic wreath associated with the 3D spiral null is likely an important class of the physical entity of flux ropes.

Hui Zhao; Jing-Xiu Wang; Jun Zhang; Chi-Jie Xiao; Hai-Min Wang

2007-12-20T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Statistical Characteristics of the Heliospheric Plasma and Magnetic Field at the Earth's Orbit during Four Solar Cycles 20-23  

E-Print Network [OSTI]

The review presents analysis and physical interpretation of available statistical data about solar wind plasma and interplanetary magnetic field (IMF) properties as measured in-situ at 1 A.U. by numerous space experiments during time period from 1964 to 2007. The experimental information have been collected in the OMNI Web/NSSDC data set of hourly averaged heliospheric parameters for last four solar cycles from 20th to 23rd. We studied statistical characteristics of such key heliospheric parameters as solar wind proton number density, temperature, bulk velocity, and IMF vector as well as dimensionless parameters. From harmonic analysis of the variations of key parameters we found basic periods of 13.5 days, 27 days, 1 year, and ~11 years, which correspond to rotation of the Sun, Earth and to the solar cycle. We also revealed other periodicities such as specific five-year plasma density and temperature variations, which origin is a subject of discussion. We have found that the distribution of solar wind proton...

Dmitriev, A V; Veselovsky, I S

2013-01-01T23:59:59.000Z

122

Solar Wind Sources in the Late Declining Phase ofCycle23: Effects of the Weak Solar Polar Field onHighSpeed Streams  

E-Print Network [OSTI]

P. , Arge, C.N. : 2008, Solar Phys. Lee, C.O. , Luhmann,De Pater, I. , et al. : 2009, Solar Phys. in press. Li, Y. ,G.W. , Kopp, R.A. : 1971, Solar Phys. 18, 258. Schatten,

2009-01-01T23:59:59.000Z

123

Solar Energy Education. Humanities: activities and teacher's guide. Field test edition  

SciTech Connect (OSTI)

Activities are outlined to introduce students to information on solar energy while performing ordinary classroom work. In this teaching manual solar energy is integrated with the humanities. The activities include such things as stories, newspapers, writing assignments, and art and musical presentations all filled with energy related terms. An energy glossary is provided. (BCS)

Not Available

1982-01-01T23:59:59.000Z

124

Solar Energy Materials & Solar Cells 78 (2003) 567595 Low-mobility solar cells: a device physics primer  

E-Print Network [OSTI]

Solar Energy Materials & Solar Cells 78 (2003) 567­595 Low-mobility solar cells: a device physics, Syracuse, New York 13244-1130, USA Abstract The properties of pin solar cells based on photogeneration for the solar conversion efficiency of amorphous silicon-based cells that are limited by valence bandtail

Schiff, Eric A.

125

Increasing the efficiency of organic solar cells by photonic and electrostatic-field enhancements  

SciTech Connect (OSTI)

Organic photovoltaic (OPV) technology is an attractive solar-electric conversion paradigm due to the promise of low cost roll-to-roll production and amenability to flexible substrates. Power conversion efficiency (PCE) exceeding 7% has recently been achieved. OPV cells suffer from low charge carrier mobilities of polymers, leading to recombination losses, higher series resistances and lower fill-factors. Thus, it is imperative to develop fabrication methodologies that can enable efficient optical absorption in films thinner than optical absorption length. Active layers conformally deposited on light-trapping, microscale textured, grating-type surfaces is one possible approach to achieve this objective. In this study, 40% theoretical increase in photonic absorption over flat OPVs is shown for devices with textured geometry by the simulation results. For verifying this theoretical result and improving the efficiency of OPVs by light trapping, OPVs were fabricated on grating-type textured substrates possessing t pitch and -coat PV active-layer on these textured substrates led to over filling of the valleys and shunts at the crest, which severely affected the performance of the resultant PV devices. Thus, it is established that although the optical design is important for OPV performance but the potential of light trapping can only be effectively tapped if the textures are amenable for realizing a conformal active layer. It is discovered that if the height of the underlying topographical features is reduced to sub-micron regime (e.g. 300 nm) and the pitch is increased to more than a micron (e.g. 2 ?m), the textured surface becomes amenable to coating a conformal PV active-layer. The resultant PV cells showed 100% increase in average light absorption near the band edge due to trapping of higher wavelength photons, and 20% improvement in power conversion efficiency as compared with the flat PV cell. Another factor that severely limits the performance of OPVs is recombination of charge carriers. Thus it becomes imperative to understand the effect of processing conditions such as spin coating speed and drying rate on defect density and hence induced carrier recombination mechanism. In this study, It is shown that slow growth (longer drying time) of the active-layer leads to reduction of sub-bandgap traps by an order of magnitude as compared to fast grown active-layer. By coupling the experimental results with simulations, it is demonstrated that at one sun condition, slow grown device has bimolecular recombination as the major loss mechanism while in the fast grown device with high trap density, the trap assisted recombination dominates. It has been estimated that non-radiative recombination accounts nearly 50% of efficiency loss in modern OPVs. Generally, an external bias (electric field) is required to collect all the photogenerated charges and thus prevent their recombination. The motivation is to induce additional electric field in otherwise low mobility conjugated polymer based active layer by incorporating ferroelectric dipoles. This is expected to facilitate singlet exciton dissociation in polymer matrix and impede charge transfer exciton (CTE) recombination at polymer:fullerene interface. For the first time, it is shown that the addition of ferroelectric dipoles to modern bulk heterojunction (BHJ) can significantly improve exciton dissociation, resulting in a ~50% enhancement of overall solar cell efficiency. The devices also exhibit the unique ferroelectric-photovoltaic effect with polarization-controlled power conversion efficiency.

Nalwa, Kanwar

2012-11-03T23:59:59.000Z

126

Design of a telescope pointing and tracking subsystem for the Big Bear Solar Observatory New Solar Telescope  

E-Print Network [OSTI]

, California, U.S.A.; bNew Jersey Institute of Technology, Newark, New Jersey, U.S.A. ABSTRACT The New SolarDesign of a telescope pointing and tracking subsystem for the Big Bear Solar Observatory New Solar Telescope J. R. Varsika and G.Yangb aBig Bear Solar Observatory, 40386 North Shore Lane, Big Bear City

127

EXTRAPOLATION OF THE SOLAR CORONAL MAGNETIC FIELD FROM SDO/HMI MAGNETOGRAM BY A CESE-MHD-NLFFF CODE  

SciTech Connect (OSTI)

Due to the absence of direct measurement, the magnetic field in the solar corona is usually extrapolated from the photosphere in a numerical way. At the moment, the nonlinear force-free field (NLFFF) model dominates the physical models for field extrapolation in the low corona. Recently, we have developed a new NLFFF model with MHD relaxation to reconstruct the coronal magnetic field. This method is based on CESE-MHD model with the conservation-element/solution-element (CESE) spacetime scheme. In this paper, we report the application of the CESE-MHD-NLFFF code to Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) data with magnetograms sampled for two active regions (ARs), NOAA AR 11158 and 11283, both of which were very non-potential, producing X-class flares and eruptions. The raw magnetograms are preprocessed to remove the force and then inputted into the extrapolation code. Qualitative comparison of the results with the SDO/AIA images shows that our code can reconstruct magnetic field lines resembling the EUV-observed coronal loops. Most important structures of the ARs are reproduced excellently, like the highly sheared field lines that suspend filaments in AR 11158 and twisted flux rope which corresponds to a sigmoid in AR 11283. Quantitative assessment of the results shows that the force-free constraint is fulfilled very well in the strong-field regions but apparently not that well in the weak-field regions because of data noise and numerical errors in the small currents.

Jiang Chaowei; Feng Xueshang, E-mail: cwjiang@spaceweather.ac.cn, E-mail: fengx@spaceweather.ac.cn [SIGMA Weather Group, State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190 (China)

2013-06-01T23:59:59.000Z

128

Dynamics and optimal control of flexible solar updraft towers  

Science Journals Connector (OSTI)

...control of flexible solar updraft towers...University of New Mexico, , Albuquerque...USA The use of solar chimneys for energy production was...a) Potential energy as a function of...University of New Mexico solar chimney prototype...

2015-01-01T23:59:59.000Z

129

Field Lines Twisting in a Noisy Corona: Implications for Energy Storage and Release, and Initiation of Solar Eruptions  

Science Journals Connector (OSTI)

We present simulations modeling closed regions of the solar corona threaded by a strong magnetic field where localized photospheric vortical motions twist the coronal field lines. The linear and nonlinear dynamics are investigated in the reduced magnetohydrodynamic regime in Cartesian geometry. Initially the magnetic field lines get twisted and the system becomes unstable to the internal kink mode, confirming and extending previous results. As typical in this kind of investigations, where initial conditions implement smooth fields and flux-tubes, we have neglected fluctuations and the fields are laminar until the instability sets in. However, previous investigations indicate that fluctuations, excited by photospheric motions and coronal dynamics, are naturally present at all scales in the coronal fields. Thus, in order to understand the effect of a photospheric vortex on a more realistic corona, we continue the simulations after kink instability sets in, when turbulent fluctuations have already developed in the corona. In the nonlinear stage the system never returns to the simple initial state with ordered twisted field lines, and kink instability does not occur again. Nevertheless, field lines get twisted, although in a disordered way, and energy accumulates at large scales through an inverse cascade. This energy can subsequently be released in micro-flares or larger flares, when interaction with neighboring structures occurs or via other mechanisms. The impact on coronal dynamics and coronal mass ejections initiation is discussed.

A. F. Rappazzo; M. Velli; G. Einaudi

2013-01-01T23:59:59.000Z

130

FIELD LINES TWISTING IN A NOISY CORONA: IMPLICATIONS FOR ENERGY STORAGE AND RELEASE, AND INITIATION OF SOLAR ERUPTIONS  

SciTech Connect (OSTI)

We present simulations modeling closed regions of the solar corona threaded by a strong magnetic field where localized photospheric vortical motions twist the coronal field lines. The linear and nonlinear dynamics are investigated in the reduced magnetohydrodynamic regime in Cartesian geometry. Initially the magnetic field lines get twisted and the system becomes unstable to the internal kink mode, confirming and extending previous results. As typical in this kind of investigations, where initial conditions implement smooth fields and flux-tubes, we have neglected fluctuations and the fields are laminar until the instability sets in. However, previous investigations indicate that fluctuations, excited by photospheric motions and coronal dynamics, are naturally present at all scales in the coronal fields. Thus, in order to understand the effect of a photospheric vortex on a more realistic corona, we continue the simulations after kink instability sets in, when turbulent fluctuations have already developed in the corona. In the nonlinear stage the system never returns to the simple initial state with ordered twisted field lines, and kink instability does not occur again. Nevertheless, field lines get twisted, although in a disordered way, and energy accumulates at large scales through an inverse cascade. This energy can subsequently be released in micro-flares or larger flares, when interaction with neighboring structures occurs or via other mechanisms. The impact on coronal dynamics and coronal mass ejections initiation is discussed.

Rappazzo, A. F. [Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, DE 19716 (United States); Velli, M. [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Einaudi, G., E-mail: rappazzo@udel.edu [Berkeley Research Associates, Inc., 6537 Mid Cities Avenue, Beltsville, MD 20705 (United States)

2013-07-10T23:59:59.000Z

131

Offshore Wind Power USA  

Broader source: Energy.gov [DOE]

The Offshore Wind Power USA conference provides the latest offshore wind market updates and forecasts.

132

Monograph Series, No. 4: 10 MWe Solar Thermal Central Receiver Pilot Plant heliostat field aimpoint improvements  

SciTech Connect (OSTI)

New early morning and late afternoon heliostat aimpoints have been developed for the 10 MWe Solar Thermal Central Receiver Pilot Plant. These new heliostat aimpoints increase the fraction of the total receiver incident solar energy on selected panels to reduce the early morning start-up time and extend the late afternoon operating time, compared to those in current use at the Pilot Plant. Preliminary results from tests using the new morning start-up aimpoint file indicates that the winter start-up time was reduced by 30 to 45 minutes.

Baker, A.F.; Atwood, D.L.

1986-01-01T23:59:59.000Z

133

The Astrophysical Journal, 692:15431560, 2009 February 20 doi:10.1088/0004-637X/692/2/1543 c 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

. The American Astronomical Society. All rights reserved. Printed in the U.S.A. VECTOR MAGNETIC FIELDS using the Imaging Vector Magnetograph (IVM) at Mees Solar Observatory. Two IVM effects are newly discussed and taken into account: (1) the central wavelength of the Fabry­P´erot is found to drift with time

Li, Jing

134

The Astrophysical Journal, 702:3949, 2009 September 1 doi:10.1088/0004-637X/702/1/39 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

. The American Astronomical Society. All rights reserved. Printed in the U.S.A. SHOCK-GENERATED VORTICITY fields of astrophysics. The form of the IMF plays a central role in subjects as diverse as galactic at low stellar masses with a power-law tail at masses exceeding a solar mass (e.g., Chabrier 2003

Kevlahan, Nicholas

135

OTB USA Inc | Open Energy Information  

Open Energy Info (EERE)

OTB USA Inc OTB USA Inc Jump to: navigation, search Name OTB USA Inc Address 1871 Suffolk Rd. Place Columbus, Ohio Zip 43221 Sector Solar Product Other:Capital Equipment Phone number 614-481-6701 Website http://www.otb-solar.com Coordinates 40.002562°, -83.0592999° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.002562,"lon":-83.0592999,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

136

Cleaning strategies for parabolic-trough solar-collector fields; guidelines for decisions  

SciTech Connect (OSTI)

This report is intended to assist the owner or operator of a parabolic trough solar collector system to decide on a cleaning strategy (equipment, materials, procedures, and schedules). The guidelines are based on information obtained in past research studies, as well as interviews with vendors and users of cleaning and water treatment equipment. The basic procedure recommended utilizes high pressure portable washing equipment. However, since the cleaning problem is so site-specific, no single, detailed approach can be specified. A systematic procedure for evaluating the particular requirements of a site is therefore given. This will allow the solar energy system operator to develop a cleaning strategy which is cost-effective because it is suited to local conditions.

Bergeron, K.D.; Freese, J.M.

1981-06-01T23:59:59.000Z

137

Solar aided power generation of a 300MW lignite fired power plant combined with line-focus parabolic trough collectors field  

Science Journals Connector (OSTI)

Abstract Nowadays, conventional coal or gas fired power plants are the dominant way to generate electricity in the world. In recent years there is a growth in the field of renewable energy sources in order to avoid the threat of climate change from fossil fuel combustion. Solar energy, as an environmental friendly energy source, may be the answer to the reduction of global CO2 emissions. This paper presents the concept of Solar Aided Power Generation (SAPG), a combination of renewable and conventional energy sources technologies. The operation of the 300MW lignite fired power plant of Ptolemais integrated with a solar field of parabolic trough collectors was simulated using TRNSYS software in both power boosting and fuel saving modes. The power plant performance, power output variation, fuel consumption and CO2 emissions were calculated. Furthermore, an economic analysis was carried out for both power boosting and fuel saving modes of operation and optimum solar contribution was estimated.

G.C. Bakos; Ch. Tsechelidou

2013-01-01T23:59:59.000Z

138

Final Environmental Impact Statement for the Quartzsite Solar Energy Project and Proposed Yuma Field Office Resource Management Plan Amendment  

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

Final Environmental Impact Statement for the Quartzsite Solar Energy Project and Proposed Yuma Field Office Resource Management Plan Amendment DOE/EIS - 0440 Lead Federal Agency: U.S. Department of Energy, Western Area Power Administration Cooperating Agencies: U.S. Department of the Interior, Bureau of Land Management, Yuma Field Office U.S. Army Corps of Engineers U.S. Army Garrison Yuma Proving Ground Arizona Department of Environmental Quality Arizona Game and Fish Department December 2012 COVER SHEET Lead Federal Agency: U.S. Department of Energy, Western Area Power Administration Cooperating Agencies: U.S. Department of the Interior, Bureau of Land Management U.S. Army Corps of Engineers U.S. Army Garrison-Yuma Proving Ground Arizona Department of Environmental Quality

139

Solar Permitting & Inspection Webinar Series  

Office of Energy Efficiency and Renewable Energy (EERE)

ICLEI Local Governments for Sustainability U.S.A. and the Interstate Renewable Energy Council, Inc. (IREC) present a series of three webinars on Solar Permitting & Inspection. As part of the U...

140

Ion kinetic energy conservation and magnetic field strength constancy in multi-fluid solar wind Alfv\\'enic turbulence  

E-Print Network [OSTI]

We investigate properties of the plasma fluid motion in the large amplitude low frequency fluctuations of highly Alfv\\'enic fast solar wind. We show that protons locally conserve total kinetic energy when observed from an effective frame of reference comoving with the fluctuations. For typical properties of the fast wind, this frame can be reasonably identified by alpha particles, which, owing to their drift with respect to protons at about the Alfv\\'en speed along the magnetic field, do not partake in the fluid low frequency fluctuations. Using their velocity to transform proton velocity into the frame of Alfv\\'enic turbulence, we demonstrate that the resulting plasma motion is characterized by a constant absolute value of the velocity, zero electric fields, and aligned velocity and magnetic field vectors as expected for unidirectional Alfv\\'enic fluctuations in equilibrium. We propose that this constraint, via the correlation between velocity and magnetic field in Alfv\\'enic turbulence, is at the origin of ...

Matteini, L; Pantellini, F; Velli, M; Schwartz, S J

2015-01-01T23:59:59.000Z

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


141

Fracture characterization and fluid flow simulation with geomechanical constraints for a CO2EOR and sequestration project Teapot Dome Oil Field, Wyoming, USA  

Science Journals Connector (OSTI)

Mature oil and gas reservoirs are attractive targets for geological sequestration of CO2 because of their potential storage capacities and the possible cost offsets from enhanced oil recovery (EOR). In this work, we analyze the fracture system of the Tensleep Formation to develop a geomechanically-constrained 3D reservoir fluid flow simulation at Teapot Dome Oil Field, WY, USA. Teapot Dome is the site of a proposed CO2-EOR and sequestration pilot project. The objective of this work is to model the migration of the injected CO2 in the fracture reservoir, as well as to obtain limits on the rates and volumes of CO2 that can be injected, without compromising seal integrity. Furthermore we want to establish the framework to design injection experiments that will provide insight into the fracture network of the reservoir, in particular of fracture permeability and connectivity. Teapot Dome is an elongated asymmetrical, basement-cored anticline with a north-northeast axis. The Tensleep Fm. in this area is highly fractured, and consists of an intercalation of eolian-dune sandstones and inter-dune deposits. The dune sandstones are permeable and porous intervals with different levels of cementation that affects their porosity, permeability, and fracture intensity. The inter-dune deposits consist of thin sabkha carbonates, minor evaporates, and thin but widespread extensive beds of very low-permeability dolomicrites. The average permeability is 30mD, ranging from 10100mD. The average reservoir thickness is 50 ft. The caprock for the Tensleep Fm. consists of the Opeche Shale member, and the anhydrite of the Minnekhata member. The reservoir has strong aquifer drive. In the area under study, the Tensleep Fm. has its structural crest at 1675m. It presents a 2-way closure trap against a NE-SW fault to the north and possibly the main thrust to the west. The CO2-EOR and sequestration project will consist of the injection of 1 million cubic feet of supercritical CO2 for six weeks. A previous geomechanical analysis suggested that the trapping faults do not appear to be at risk of reactivation and it was estimated that caprock integrity is not a risk by the buoyancy pressure of the maximum CO2 column height that the formation can hold. However, in the present study we established the presence of critically stressed minor faults and fractures in the reservoir and caprock, which if reactivated, could not only enhance the permeability of the reservoir, but potentially compromise the top seal capacity. The results of the preliminary fluid flow simulations indicate that the injected CO2 will rapidly rise to the top layers, above the main producing interval, and will accumulate in the fractures, where almost none will get into the matrix.

Laura Chiaramonte; Mark Zoback; Julio Friedmann; Vicki Stamp; Chris Zahm

2011-01-01T23:59:59.000Z

142

Solar Sail Technology for Nanosatellites Michael D. Souder  

E-Print Network [OSTI]

Solar Sail Technology for Nanosatellites Michael D. Souder Stanford University, Stanford, CA, 94305, USA Matthew West University of Illinois, Urbana, IL, 61801, USA Solar sailing is an attractive means. This allows a solar sail spacecraft to accomplish new classes of missions that would otherwise require

West, Matthew

143

Nanotechnology in Solar and Biofuels  

Science Journals Connector (OSTI)

Nanotechnology in Solar and Biofuels ... This paper reviews selected recent advances in the development of nanotechnology in the emerging solar energy and biofuel fields. ...

Hema Ramsurn; Ram B. Gupta

2013-05-22T23:59:59.000Z

144

Innovation Conditions in the Case of Solar Power Generation  

Science Journals Connector (OSTI)

In 1954 Bell Laboratories (USA) unveiled the first silicon solar cell the USA is thus known as ... result of the costs involved, the new technology was primarily used in space travel in ... satellite (Vanguard ...

Prof. Dr. Elke Bruns; Dr. Drte Ohlhorst

2011-01-01T23:59:59.000Z

145

Modern Solar Facilities Advanced Solar Science, 18 F. Kneer, K. G. Puschmann, A. D. Wittmann (eds.)  

E-Print Network [OSTI]

States. The 4-meter aperture Advanced Technology Solar Telescope (ATST) under the stewardshipModern Solar Facilities ­ Advanced Solar Science, 1­8 F. Kneer, K. G. Puschmann, A. D. Wittmann (eds.) c Universit¨atsverlag G¨ottingen 2007 Ground-Based Solar Facilities in the U.S.A. Carsten Denker

146

A general relativistic model for the light propagation in the gravitational field of the Solar System: the dynamical case  

E-Print Network [OSTI]

Modern astrometry is based on angular measurements at the micro-arcsecond level. At this accuracy a fully general relativistic treatment of the data reduction is required. This paper concludes a series of articles dedicated to the problem of relativistic light propagation, presenting the final microarcsecond version of a relativistic astrometric model which enable us to trace back the light path to its emitting source throughout the non-stationary gravity field of the moving bodies in the Solar System. The previous model is used as test-bed for numerical comparisons to the present one. Here we also test different versions of the computer code implementing the model at different levels of complexity to start exploring the best trade-off between numerical efficiency and the micro-arcsecond accuracy needed to be reached.

Fernando de Felice; Alberto Vecchiato; Maria Teresa Crosta; Mario G. Lattanzi; Beatrice Bucciarelli

2006-09-04T23:59:59.000Z

147

Generation of polarized shear Alfvn waves by a rotating magnetic field source  

E-Print Network [OSTI]

Department of Physics and Astronomy, University of California, Los Angeles, California 90095-1696, USA 2 in the Large Plasma Device at the University of California, Los Angeles to study the propagation of field in a variety of astrophysical settings such as the solar corona,2 near other planets such as Jupiter,3

California at Los Angles, University of

148

Microwave Mapping As a Possible New Diagnostic Tool for LargeScale Solar Magnetic Fields  

E-Print Network [OSTI]

, they are able to give a general impression of the nature and order of magnitude of the expected effects (where the field values used for the construction of synoptic charts are measured) this component with the synoptic magnetic charts and in terms of quantitative details they still have some deficiencies

Petrovay, Kristóf

149

The origin of the helicity hemispheric sign rule reversals in the mean-field solar-type dynamo  

Science Journals Connector (OSTI)

......cancellation of magnetic energy in the chromosphere and corona, the impact of the solar wind etc., so we leave...it has been shown that solar-type dynamos can be...was chosen to tune the solar cycle period. VP, DS...support of the Integration Project of SB RAS N 34, and......

V. V. Pipin; H. Zhang; D. D. Sokoloff; K. M. Kuzanyan; Y. Gao

2013-01-01T23:59:59.000Z

150

Electrochemical Investigation of a Microbial Solar Cell Reveals a Nonphotosynthetic Biocathode Catalyst  

Science Journals Connector (OSTI)

...Electrochemical Investigation of a Microbial Solar Cell Reveals a Nonphotosynthetic Biocathode...Jose, California, USA c Microbial solar cells (MSCs) are microbial fuel cells...been hypothesized that microbial solar cells (MSCs) can continuously generate...

Sarah M. Strycharz-Glaven; Richard H. Glaven; Zheng Wang; Jing Zhou; Gary J. Vora; Leonard M. Tender

2013-04-19T23:59:59.000Z

151

Solar powered induction motor-driven water pump operating on a desert well, simulation and field tests  

Science Journals Connector (OSTI)

A photovoltaic-powered water pumping system, employing an induction motor pump, capable of supplying a daily average of 50m3 at 37-m head has been developed. The system was installed on a desert well in Jordan, where: the average solar radiation amount to 5.5kWh/m3/day, to provide the Bedouins living in the well area with drinking water. A mathematical model to enable testing the system performance by computer simulation was developed. This model allows the representation of motor torque in function of speed (and slip) at different supply frequencies, as well as the flow rate and efficiency of the system in function of supply frequency and pumping head. Prior to its installation on the desert well, the system performance, in accordance with frequency and head, was thoroughly tested in the laboratory. As illustrated in this paper, simulation and laboratory testing results are well matched. At constant pumping head, the flow rate is proportional to the supply frequency of the motor. At constant flow rate, the pumping head is proportional to the supply frequency squared only in the range below the peak efficiency of the pump. For higher flow rate values, a special algorithm based on the experimental results could be developed. Higher system efficiency is achievable at higher frequency. It is advisable to operate the motor pump at the nominal frequency, flow rate and head corresponding to maximum efficiency. Long-term field testing of the system shows that it is reliable and has an overall efficiency exceeding 3%, which is comparable to the highest efficiencies reported elsewhere for solar powered pumps.

Abdel-Karim Daud; Marwan M. Mahmoud

2005-01-01T23:59:59.000Z

152

Bruce R. Kowalski (USA) Barry M Wise (USA)  

E-Print Network [OSTI]

Bruce R. Kowalski (USA) Barry M Wise (USA) Paul Geladi (SE) Alex Freitas (UK) Lutgarde Buydens (NL) Jose Cardoso de Menezes (PT) Paul J. Gemperline (USA) Rasmus Bro (DK) Roma Tauler (ES) Steven D. Brown (USA) Beata Walczak (PL) Klaas Faber (NL) Patricia Heussen (UNILEVER, NL) Peter de B. Harrington (USA

Ferreira, Márcia M. C.

153

Variations in the Solar Neutrino Flux  

DOE R&D Accomplishments [OSTI]

Observations are reported from the chlorine solar neutrino detector in the Homestake Gold Mine, South Dakota, USA. They extend from 1970 to 1985 and yield an average neutrino capture rate of 2.1 +- 0.3 SNU. The results from 1977 to 1985 show an anti-correlation with the solar activity cycle, and an apparent increased rate during large solar flares.

Davis, R. Jr.; Cleveland, B. T.; Rowley, J. K.

1987-08-02T23:59:59.000Z

154

Dolomite in Permian Paleosols of the Bravo Dome CO2 Field, U.S.A.: Permian Reflux Followed by Late Recrystallization at Elevated Temperature  

Science Journals Connector (OSTI)

...of Petroleum Geology, Atlas of Oil and Gas Fields...1999, Palaeogeographic Atlas: University of Texas-Arlington...Gabal Ataqu, northwest Gulf of Suez, Egypt: Sedimentary Geology...Sandstone Member United States wind transport Yeso Formation...

Katherine A. Hartig; Gerilyn S. Soreghan; Robert H. Goldstein; Michael H. Engel

155

Vestas USA | Open Energy Information  

Open Energy Info (EERE)

Vestas USA Jump to: navigation, search Name: Vestas USA Place: Rolling Meadows, Illinois Zip: IL 60008-4030 Sector: Wind energy Product: Vestas Wind Systems American arm....

156

Orion Registrar, Inc., USA  

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

Registrar, Inc., USA Registrar, Inc., USA Certificate of Registration This is to certify the Environmental Management System of: National Renewable Energy Laboratory 15013 Denver West Parkway Golden, Colorado 80401 USA Has been assessed by Orion Registrar and found to be in compliance with the following Environmental Management Standard: ISO 14001:2004 The Environmental Management System is applicable to: Research, Development, Commercialization and Deployment of Renewable Energy and Energy Efficiency Technologies This Scope is Applicable to All Sites The Registration period is from February 18, 2013 to August 23, 2014. This registration is subject to the company maintaining its system to the required standard, and applicable exceptions, which will be monitored by Orion.

157

Flexible Assembly Solar Technology  

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

field and secured on steel pylons. PROJECT DESCRIPTION The research team is applying automation processes to the design of a Flexible Assembly Solar Technology (FAST). FAST is an...

158

HOUSEHOLD SOLAR POWER SYSTEM.  

E-Print Network [OSTI]

?? Photovoltaic power has become one of the most popular research area in new energy field. In this report, the case of household solar power (more)

Jiang, He

2014-01-01T23:59:59.000Z

159

X-RAY EMISSION FROM PLANETS AND COMETS: RELATIONSHIP WITH SOLAR X-RAYS AND SOLAR WIND  

E-Print Network [OSTI]

with the occurrence of solar X-ray flare, when light travel time delay is accounted, suggesting that X-rays fromX-RAY EMISSION FROM PLANETS AND COMETS: RELATIONSHIP WITH SOLAR X-RAYS AND SOLAR WIND ANIL BHARDWAJ Flight center, Greenbelt, MD 20771, USA Scattering of solar X-ray radiation mainly produces the non

?stgaard, Nikolai

160

Solar Circuitry  

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

Solar Circuitry" with the Solar Powered Energy Kit Curriculum: Solar Power- (lightelectromagnetic radiation, electricity, circuitry, efficiency, energy transformation, subatomic...

Note: This page contains sample records for the topic "usa solar fields" 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

Overview of BNL's Solar Energy Research Plans  

E-Print Network [OSTI]

Overview of BNL's Solar Energy Research Plans March 2011 #12;2 Why Solar Energy Research at BNL BNL's capabilities can advance solar energy In the Northeast #12;North Array Field South Array Field Variability and Non-Dispatchability · Solar energy varies · Solar generation cannot be dispatched when needed

Homes, Christopher C.

162

The solar dynamo  

Science Journals Connector (OSTI)

...science compiled by J. M. T. Thompson The solar dynamo S. M. Tobias Department of Applied...this article I review the fundamentals of solar-dynamo theory. I describe both historical and contemporary observations of the solar magnetic field before outlining why it...

2002-01-01T23:59:59.000Z

163

Development of a %22Solar Patch%22 calculator to evaluate heliostat-field irradiance as a boundary condition in CFD models.  

SciTech Connect (OSTI)

A rigorous computational fluid dynamics (CFD) approach to calculating temperature distributions, radiative and convective losses, and flow fields in a cavity receiver irradiated by a heliostat field is typically limited to the receiver domain alone for computational reasons. A CFD simulation cannot realistically yield a precise solution that includes the details within the vast domain of an entire heliostat field in addition to the detailed processes and features within a cavity receiver. Instead, the incoming field irradiance can be represented as a boundary condition on the receiver domain. This paper describes a program, the Solar Patch Calculator, written in Microsoft Excel VBA to characterize multiple beams emanating from a 'solar patch' located at the aperture of a cavity receiver, in order to represent the incoming irradiance from any field of heliostats as a boundary condition on the receiver domain. This program accounts for cosine losses; receiver location; heliostat reflectivity, areas and locations; field location; time of day and day of year. This paper also describes the implementation of the boundary conditions calculated by this program into a Discrete Ordinates radiation model using Ansys{reg_sign} FLUENT (www.fluent.com), and compares the results to experimental data and to results generated by the code DELSOL.

Khalsa, Siri Sahib S. (Sandia Staffing Alliance); Ho, Clifford Kuofei

2010-05-01T23:59:59.000Z

164

Development of a %22solar patch%22 calculator to evaluate heliostat-field irradiance as a boundary condition in CFD models.  

SciTech Connect (OSTI)

A rigorous computational fluid dynamics (CFD) approach to calculating temperature distributions, radiative and convective losses, and flow fields in a cavity receiver irradiated by a heliostat field is typically limited to the receiver domain alone for computational reasons. A CFD simulation cannot realistically yield a precise solution that includes the details within the vast domain of an entire heliostat field in addition to the detailed processes and features within a cavity receiver. Instead, the incoming field irradiance can be represented as a boundary condition on the receiver domain. This paper describes a program, the Solar Patch Calculator, written in Microsoft Excel VBA to characterize multiple beams emanating from a 'solar patch' located at the aperture of a cavity receiver, in order to represent the incoming irradiance from any field of heliostats as a boundary condition on the receiver domain. This program accounts for cosine losses; receiver location; heliostat reflectivity, areas and locations; field location; time of day and day of year. This paper also describes the implementation of the boundary conditions calculated by this program into a Discrete Ordinates radiation model using Ansys{reg_sign} FLUENT (www.fluent.com), and compares the results to experimental data and to results generated by the code DELSOL.

Khalsa, Siri Sahib; Ho, Clifford Kuofei

2010-04-01T23:59:59.000Z

165

Investigation of the Electric Field in TiO2/FTO Junctions Used in Dye-Sensitized Solar Cells by Photocurrent Transients  

Science Journals Connector (OSTI)

Investigation of the Electric Field in TiO2/FTO Junctions Used in Dye-Sensitized Solar Cells by Photocurrent Transients ... The input resistance of the scope was 50 ? (dc mode), and each transient was averaged 10 times (repetition rate, 1 Hz) to get a stabilized signal. ... The elementary charge is denoted as q, n, and p are the electron and hole densities, while the respective mobilities are given by ?n and ?p. ...

Sven Rhle; Thomas Dittrich

2005-04-22T23:59:59.000Z

166

DOE SunShot Webinar: Solar for All- A Community Solar Webinar  

Broader source: Energy.gov [DOE]

This DOE SunShot Outreach Partnership webinar, presented in partnership with ICLEI Local Governments for Sustainability USA, will focus on solar programs that are complimentary to ICLEI's Renewables Division as part of the DOE's SunShot Initiative. The webinar will feature the city of Beaverton, Oregon's Solar on Reservoirs project, and Tompkins County, New York's Solarize Program.

167

Statistics of counter-streaming solar wind suprathermal electrons at solar minimum: STEREO observations  

E-Print Network [OSTI]

1 Statistics of counter-streaming solar wind suprathermal electrons at solar minimum: STEREO, University of New Brunswick, Fredericton, Canada 6 Space Sciences Laboratory, University of California University of New Hampshire, Durham, USA Abstract. Previous work has shown that solar wind suprathermal

Paris-Sud XI, Université de

168

Development and testing of a photometric method to identify non-operating solar hot water systems in field settings.  

SciTech Connect (OSTI)

This report presents the results of experimental tests of a concept for using infrared (IR) photos to identify non-operational systems based on their glazing temperatures; operating systems have lower glazing temperatures than those in stagnation. In recent years thousands of new solar hot water (SHW) systems have been installed in some utility districts. As these numbers increase, concern is growing about the systems dependability because installation rebates are often based on the assumption that all of the SHW systems will perform flawlessly for a 20-year period. If SHW systems routinely fail prematurely, then the utilities will have overpaid for grid-energy reduction performance that is unrealized. Moreover, utilities are responsible for replacing energy for loads that failed SHW system were supplying. Thus, utilities are seeking data to quantify the reliability of SHW systems. The work described herein is intended to help meet this need. The details of the experiment are presented, including a description of the SHW collectors that were examined, the testbed that was used to control the system and record data, the IR camera that was employed, and the conditions in which testing was completed. The details of the associated analysis are presented, including direct examination of the video records of operational and stagnant collectors, as well as the development of a model to predict glazing temperatures and an analysis of temporal intermittency of the images, both of which are critical to properly adjusting the IR camera for optimal performance. Many IR images and a video are presented to show the contrast between operating and stagnant collectors. The major conclusion is that the technique has potential to be applied by using an aircraft fitted with an IR camera that can fly over an area with installed SHW systems, thus recording the images. Subsequent analysis of the images can determine the operational condition of the fielded collectors. Specific recommendations are presented relative to the application of the technique, including ways to mitigate and manage potential sources of error.

He, Hongbo (University of New Mexico, Albuquerque, NM); Vorobieff, Peter V. (University of New Mexico, Albuquerque, NM); Menicucci, David (University of New Mexico, Albuquerque, NM); Mammoli, Andrea A. (University of New Mexico, Albuquerque, NM); Carlson, Jeffrey J.

2012-06-01T23:59:59.000Z

169

Western Michigan University, Kalamazoo, USA  

E-Print Network [OSTI]

Western Michigan University, Kalamazoo, USA Michael Backer Auslandssemester USA:WMU, Fall 20101 #12, Unterkunft Auslandssemester USA:WMU, Fall 20102 #12;Bewerbung Schriftliche Bewerbung Notenspiegel in beiden Sprachen Auslandssemester USA:WMU, Fall 20103 #12;Bewerbung Auswahlgespräch mit Domik und Blömer

Hellebrand, Sybille

170

Power spectrum analysis of the annual rainfall series for Massachusetts (NE, U.S.A.)  

Science Journals Connector (OSTI)

Maximum Entropy Spectral Analysis of the annual rainfall series for 18871976 (90 years) for Massachusetts (northeastern USA.) shows T...= 17.8 (very near the 18.6 year luni-solar signal) as the most prominent pe...

R. P. Kane; N. R. Teixeira

1991-01-01T23:59:59.000Z

171

A survey on control schemes for distributed solar collector fields. Part I: Modeling and basic control approaches  

Science Journals Connector (OSTI)

This article presents a survey of the different automatic control techniques that have been applied to control the outlet temperature of solar plants with distributed collectors during the last 25 years. Different aspects of the control problem involved in this kind of plants are treated, from modeling and simulation approaches to the different basic control schemes developed and successfully applied in real solar plants. A classification of the modeling and control approaches is used to explain the main features of each strategy.

E.F. Camacho; F.R. Rubio; M. Berenguel; L. Valenzuela

2007-01-01T23:59:59.000Z

172

Category:Solar | Open Energy Information  

Open Energy Info (EERE)

RAPIDSolarWater Use RAPIDSolarWell Field S Solar Decathlon Retrieved from "http:en.openei.orgwindex.php?titleCategory:Solar&oldid374814" Category: Renewable Energy...

173

Sandia National Laboratories: National Solar Thermal Testing...  

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

Beam Profiling On November 2, 2012, in Concentrating Solar Power, News, Renewable Energy, Solar On Thursday, June 7, we began beam profiling the NSTTF field heliostat beam....

174

Solar Power for Deployment in Populated Areas.  

E-Print Network [OSTI]

??The thesis presents background on solar thermal energy and addresses the structural challenges associated with the deployment of concentrating solar power fields in urban areas. (more)

Hicks, Nathan Andrew

2009-01-01T23:59:59.000Z

175

Polyhedral Specular Reflector Design for Ultra-High Spectrum Splitting Solar Module Efficiencies (>50%)  

E-Print Network [OSTI]

Polyhedral Specular Reflector Design for Ultra-High Spectrum Splitting Solar Module Efficiencies., Pasadena, CA, USA 95555-0345 ABSTRACT One pathway to achieving ultra-high solar efficiencies (>50, multijunction solar cell, solar concentrator 1. INTRODUCTION Solar cell efficiency is increased through

Atwater, Harry

176

Meridian Energy USA | Open Energy Information  

Open Energy Info (EERE)

Logo: Meridian Energy USA Name Meridian Energy USA Address 6200 Stoneridge Mall Road, Suite 300 Place Pleasanton, California Zip 94588 Sector Solar Product PV power developer Website http://meridianenergyusa.com/ Coordinates 37.696133°, -121.92419° 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":37.696133,"lon":-121.92419,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

177

GREEN ENERGY AND ELECTRIC VEHICLES. BMW GROUP TECHNOLOGYOFFICE USA.  

E-Print Network [OSTI]

GREEN ENERGY AND ELECTRIC VEHICLES. BMW GROUP TECHNOLOGYOFFICE USA. LT-Z-Z, OCTOBER 2012 #12;GREEN E, LT-Z-Z,OCT 2012 Page 2 BACKGROUND. Markets for green energy and electric vehicles can accelerate each other. Nearly 40% of MINI E customers invested in residential solar. Adding Green-E options

California at Davis, University of

178

Mitsubishi Electric and Electronics USA Inc | Open Energy Information  

Open Energy Info (EERE)

Electric and Electronics USA Inc Electric and Electronics USA Inc Jump to: navigation, search Name Mitsubishi Electric and Electronics USA Inc Place Cypress, California Zip 90630 Sector Solar Product Markets and supports consumer, commercial and industrial electronic products in US, including solar powered. Coordinates 29.975226°, -95.680206° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.975226,"lon":-95.680206,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

179

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">

180

A Continuous Solar Thermochemical Hydrogen Production Plant Design  

E-Print Network [OSTI]

change thermal-storage systems, and solar fields. Chapter 3Storage System . 21 2.5 Solarchange thermal-storage system and the solar field were not

Luc, Wesley Wai

Note: This page contains sample records for the topic "usa solar fields" 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

usa | OpenEI  

Open Energy Info (EERE)

usa usa Dataset Summary Description Estimates for each of the 50 states and the entire United States show Source Wind Powering America Date Released February 04th, 2010 (4 years ago) Date Updated April 13th, 2011 (3 years ago) Keywords annual generation installed capacity usa wind Data application/vnd.ms-excel icon Wind potential data (xls, 102.4 KiB) Quality Metrics Level of Review Some Review Comment Temporal and Spatial Coverage Frequency Time Period License License Other or unspecified, see optional comment below Comment Work of the U.S. Federal Government. Rate this dataset Usefulness of the metadata Average vote Your vote Usefulness of the dataset Average vote Your vote Ease of access Average vote Your vote Overall rating Average vote Your vote Comments Login or register to post comments

182

SOURCE REGIONS OF THE INTERPLANETARY MAGNETIC FIELD AND VARIABILITY IN HEAVY-ION ELEMENTAL COMPOSITION IN GRADUAL SOLAR ENERGETIC PARTICLE EVENTS  

SciTech Connect (OSTI)

Gradual solar energetic particle (SEP) events are those in which ions are accelerated to their observed energies by interactions with a shock driven by a fast coronal mass ejection (CME). Previous studies have shown that much of the observed event-to-event variability can be understood in terms of shock speed and evolution in the shock-normal angle. However, an equally important factor, particularly for the elemental composition, is the origin of the suprathermal seed particles upon which the shock acts. To tackle this issue, we (1) use observed solar-wind speed, magnetograms, and the potential-field source-surface model to map the Sun-L1 interplanetary magnetic field (IMF) line back to its source region on the Sun at the time of the SEP observations and (2) then look for a correlation between SEP composition (as measured by Wind and Advanced Composition Explorer at ?2-30 MeV nucleon{sup 1}) and characteristics of the identified IMF source regions. The study is based on 24 SEP events, identified as a statistically significant increase in ?20 MeV protons and occurring in 1998 and 2003-2006, when the rate of newly emergent solar magnetic flux and CMEs was lower than in solar-maximum years, and the field-line tracing is therefore more likely to be successful. We find that the gradual SEP Fe/O is correlated with the field strength at the IMF source, with the largest enhancements occurring when the footpoint field is strong due to the nearby presence of an active region (AR). In these cases, other elemental ratios show a strong charge-to-mass (q/M) ordering (at least on average), similar to that found in impulsive events. Such results lead us to suggest that magnetic reconnection in footpoint regions near ARs bias the heavy-ion composition of suprathermal seed ions by processes qualitatively similar to those that produce larger heavy-ion enhancements in impulsive SEP events. To address potential technical concerns about our analysis, we also discuss efforts to exclude impulsive SEP events from our event sample.

Ko, Yuan-Kuen; Wang, Yi-Ming [Space Science Division, Naval Research Laboratory, Code 7680, Washington, DC 20375 (United States); Tylka, Allan J. [NASA Goddard Space Flight Center, Code 672, Greenbelt, MD 20771 (United States); Ng, Chee K. [College of Science, George Mason University, Fairfax, VA 22030 (United States); Dietrich, William F., E-mail: yko@ssd5.nrl.navy.mil [Praxis, Inc., Alexandria, VA 22303 (United States)

2013-10-20T23:59:59.000Z

183

ORGANIZATION Panagiotis Manolios (GeorgiaTech, USA)  

E-Print Network [OSTI]

ORGANIZATION CHAIRS Panagiotis Manolios (GeorgiaTech, USA) Matthew Wilding (Rockwell Collins, USA) PUBLICATIONS Ruben Gamboa (U. Wyoming, USA) WEBMASTERS Sudarshan Srinivasan (Georgia Tech, USA) Daron Vroon (Georgia Tech, USA) PROGRAM COMMITTEE Ruben Gamboa (U. Wyoming, USA) David Greve (Rockwell Collins, USA

Manolios, Panagiotis "Pete"

184

Evaluating Solar Radiation Attenuation Models to Assess the Effects of Climate and Geographical Location on the Heliostat Field Efficiency in Brazil  

Science Journals Connector (OSTI)

Abstract Most of the solar power plants using a central receiver which are currently in operation are installed in the Sun Belt region, specifically above the Tropic of Cancer. These plants are located in regions characterized by a dry summers and a yearly sum of Direct Normal Irradiation (DNI) of over 2300 kWh/m2. These regions include the Mojave Desert (semi-arid climate) and Andaluca in southern Spain (Mediterranean and semi-arid climate). Potential locations for installing such plants in Brazil, identified in previous studies, are the So Francisco river basin and the Sobradinho area in the Northeast Region of the country. These locations are characterized by high humidity levels and yearly DNI values ranging from 1800 to 2300 kWh/m2, which is in clear contrast with the dry and desert climates where the solar tower projects currently in operation are located. Besides the combined effects of climate and the inter-tropicalization of the site, based on the solar angles and atmospheric attenuation, the potential locations in Brazil provide a small variation between the monthly averages DNI values. In this paper, the effects of these particularities on the performance of a heliostat field are assessed. For instance, the effects of the atmospheric water vapor and aerosol concentration on the optical performance of the heliostat field are analyzed. The results suggest that, for the same DNI level, the heliostat field in Brazil should be 4% larger due to the effect of the water vapor concentration in the atmosphere. This is an important finding, which shows that the current models for calculating the attenuation between the heliostat and the receiver need to be reviewed and compared with experimental observations and validated for the conditions prevailing at potential locations in Brazil.

JM Cardemil; AR Starke; VK Scariot; IL. Grams; S Colle

2014-01-01T23:59:59.000Z

185

Field zero-age main-sequence stars in the solar neighbourhood: where have they come from?  

Science Journals Connector (OSTI)

......G-type stars in the solar vicinity we estimate...sense of equipartition of energy) will not lead to an...on average half of the energy gained by perturbations is in potential energy. Therefore the shape...D-0236(A)]. This project has been supported by......

R. Wichmann; J. H. M. M. Schmitt

2003-07-11T23:59:59.000Z

186

Meridian Energy USA | Open Energy Information  

Open Energy Info (EERE)

Energy USA (Redirected from Cleantech America) Jump to: navigation, search Logo: Meridian Energy USA Name: Meridian Energy USA Address: 6200 Stoneridge Mall Road, Suite 300 Place:...

187

Barloworld Supply Chain Software USA  

E-Print Network [OSTI]

Barloworld Supply Chain Software USA Supply Chain Consultant / Inventory Analyst Position November 2011 #12;Barloworld SCS USA ­ Supply Chain / Inventory Analyst Aug 2011 Page 2 of 4 INTRODUCTION Barloworld Supply Chain Software (SCS) USA would like to invite you to apply for a Supply Chain

Heller, Barbara

188

Solar-radiation-maintained glacier recession on Kilimanjaro drawn from combined ice-radiation geometry modeling  

E-Print Network [OSTI]

Solar-radiation-maintained glacier recession on Kilimanjaro drawn from combined ice of Massachusetts, Amherst, Massachusetts, USA Georg Kaser Tropical Glaciology Group, Department of Geography retreat during the twentieth century. To evaluate the role of solar radiation in maintaining glacier

Massachusetts at Amherst, University of

189

Sol-Up USA, LLC | Open Energy Information  

Open Energy Info (EERE)

Sol-Up USA, LLC Sol-Up USA, LLC Jump to: navigation, search Logo: Sol-Up USA, LLC Name Sol-Up USA, LLC Address 3355 West Spring Mountain Road, Suite 3 Place Las Vegas, NV Zip 89102 Sector Solar Product PV, Solar Thermal, Solar Cooling Year founded 2009 Number of employees 1-10 Phone number +1 (702) 586-9800 Website http://www.sol-up.com Coordinates 36.125853°, -115.184757° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":36.125853,"lon":-115.184757,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

190

Early Solar System Chronology K.D. McKeegan  

E-Print Network [OSTI]

, and to a first approximation can be thought of as ``hand samples'' of the condensable portion of the solar nebula1.16 Early Solar System Chronology K.D. McKeegan University of California, Los Angeles, CA, USA Meteorites as Probes of Early Solar System Evolution 2 1.16.1.2 Short-Lived Radioactivity at the Origin

Reiners, Peter W.

191

MORPHOLOGY DEPENDENT SHORT CIRCUIT CURRENT IN BULK HETEROJUNCTION SOLAR CELL  

E-Print Network [OSTI]

a relatively inexpensive option for the future solar cell technology, provided its efficiency increases beyondMORPHOLOGY DEPENDENT SHORT CIRCUIT CURRENT IN BULK HETEROJUNCTION SOLAR CELL Biswajit Ray, Pradeep, West Lafayette, Indiana, USA ABSTRACT Polymer based bulk heterostructure (BH) solar cell offers

Alam, Muhammad A.

192

Repetitive substorms caused by Alfvenic waves of the interplanetary magnetic field during high-speed solar wind streams  

E-Print Network [OSTI]

, but they may be locally generated from stream-stream interaction effects or amplified Alfve´n waves originating-speed solar wind streams D.-Y. Lee,1 L. R. Lyons,2 K. C. Kim,1 J.-H. Baek,3 K.-H. Kim,3 H.-J. Kim,1 J. Weygand wind streams, J. Geophys. Res., 111, A12214, doi:10.1029/2006JA011685. 1. Introduction [2] During

Lyons, Larry

193

Energy Optimizers USA | Open Energy Information  

Open Energy Info (EERE)

Optimizers USA Optimizers USA Jump to: navigation, search Name Energy Optimizers USA Address 6 S. 3rd Street Place Tipp City, Ohio Zip 45371 Sector Biomass, Carbon, Geothermal energy, Services, Solar, Wind energy Product Business and legal services;Consulting;Energy audits/weatherization; Engineering/architectural/design;Installation;Investment/finances; Trainining and education Phone number 937-877-1919 Website http://www.energyoptimizersusa Coordinates 39.9610217°, -84.1712945° 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":39.9610217,"lon":-84.1712945,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

194

MAGNETIC HELICITY SPECTRUM OF SOLAR WIND FLUCTUATIONS AS A FUNCTION OF THE ANGLE WITH RESPECT TO THE LOCAL MEAN MAGNETIC FIELD  

SciTech Connect (OSTI)

Magnetic field data acquired by the Ulysses spacecraft in high-speed streams over the poles of the Sun are used to investigate the normalized magnetic helicity spectrum {sigma}{sub m} as a function of the angle {theta} between the local mean magnetic field and the flow direction of the solar wind. This spectrum provides important information about the constituent modes at the transition to kinetic scales that occurs near the spectral break separating the inertial range from the dissipation range. The energetically dominant signal at scales near the thermal proton gyroradius k{sub perpendicular{rho}i} {approx} 1 often covers a wide band of propagation angles centered about the perpendicular direction, {theta} {approx_equal} 90{sup 0} {+-} 30{sup 0}. This signal is consistent with a spectrum of obliquely propagating kinetic Alfven waves with k{sub perpendicular} >> k{sub ||} in which there is more energy in waves propagating away from the Sun and along the direction of the local mean magnetic field than toward the Sun. Moreover, this signal is principally responsible for the reduced magnetic helicity spectrum measured using Fourier transform techniques. The observations also reveal a subdominant population of nearly parallel propagating electromagnetic waves near the proton inertial scale k{sub ||} c/{omega}{sub pi} {approx} 1 that often exhibit high magnetic helicity |{sigma}{sub m}| {approx_equal} 1. These waves are believed to be caused by proton pressure anisotropy instabilities that regulate distribution functions in the collisionless solar wind. Because of the existence of a drift of alpha particles with respect to the protons, the proton temperature anisotropy instability that operates when T{sub pperpendicular}/T{sub p||} > 1 preferentially generates outward propagating ion-cyclotron waves and the fire-hose instability that operates when T{sub pperpendicular}/T{sub p||} < 1 preferentially generates inward propagating whistler waves. These kinetic processes provide a natural explanation for the magnetic field observations.

Podesta, J. J.; Gary, S. P., E-mail: jpodesta@solar.stanford.edu [Los Alamos National Laboratory, Los Alamos, NM 87545 (United States)

2011-06-10T23:59:59.000Z

195

PNE WIND USA II  

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

PNE WIND USA II PNE WIND USA II 1 PNE Wind USA Tribal Energy Partnerships Cherokee & Chilocco Wind Parks Buchholz wind farm, Germany André De Rosa Managing Director Andre.DeRosa@PNEWind.com p. (312) 919-8042 Hot Springs NP M is s i s s i ppi M iss is s i pp i Mis si ss ip p i M ississippi M iss iss ippi M i ss i ss i pp i M is s issippi Missis sip pi M i s s is s ip p i Bonny State Park Bonny State Park Buffalo River State Park Buffalo River State Park Caprock Caprock Canyons Canyons State Park State Park Robbers Cave State Park Robbers Cave State Park Clinton State Park Clinton State Park Hillsdale State Park Hillsdale State Park Indian Cave State Park Indian Cave State Park Lake Murray State Park Lake Murray State Park Lake of Lake of the Ozarks the Ozarks St Park St Park Little River State Park Little River State Park Palo Duro

196

Solar Radiation and Pyranometry Studies for Solar Energy Applications: an Overview of IEA Task IX  

Science Journals Connector (OSTI)

With increased activity in the field of solar energy research and application, there is a need for accurate solar radiation and meteorological data to aid in resource assessment, solar system design evaluation, a...

D. C. McKay

1984-01-01T23:59:59.000Z

197

Ammonia at Blodgett Forest, Sierra Nevada, USA  

E-Print Network [OSTI]

Forest, Sierra Nevada, USA Marc L. Fischer and DavidRd. , Berkeley CA, 94720, USA Corresponding author address:

Fischer, Marc L.; Littlejohn, David

2007-01-01T23:59:59.000Z

198

The role of solar absorption in climate and climate change  

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

role of solar absorption in climate and role of solar absorption in climate and climate change William Collins UC Berkeley and Lawrence Berkeley Lab with Andrew Conley, David Fillmore, and Phil Rasch National Center for Atmospheric Research Boulder, Colorado, USA 2 Prior Research on Absorption and Climate Field Experiments: * Central Equatorial Pacific Experiment * Indian Ocean Experiment Modeling studies of clouds: * The color of the planet * Climate with enhanced cloud absorption Synthesis of models and aerosol observations: * Development of aerosol assimilation * Application to aerosol/climate interactions 3 Natural and anthropogenic aerosols India, March 2000 California, October 2003 Africa, March 2003 4 Historical and projected sulfate emissions * Emissions from India have tripled in last 20 years of 20 th century..

199

Solar Policy Environment: Seattle  

Broader source: Energy.gov [DOE]

The objective of the Emerald City Solar Initiative is to overcome the barriers to widespread deployment of solar energy technology, dramatically increasing residential, commercial, City-owned, and community-scale solar energy use. The City has assembled a strong team of partners that have proven track records in the fields of public planning, renewable energy resource mapping, financial analysis, site analysis, education and outreach, policy analysis and advocacy, community organizing and renewable energy project development.

200

Photoelectrochemical solar energy conversion  

Science Journals Connector (OSTI)

In the present paper the progress in the field of solar energy conversion for the production of electricity and storable ... critically analyzed in view of their stability and conversion efficiency. A number of factors

Rdiger Memming

1988-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Predicting solar cycle 24 with a solar dynamo model  

E-Print Network [OSTI]

Whether the upcoming cycle 24 of solar activity will be strong or not is being hotly debated. The solar cycle is produced by a complex dynamo mechanism. We model the last few solar cycles by `feeding' observational data of the Sun's polar magnetic field into our solar dynamo model. Our results fit the observed sunspot numbers of cycles 21-23 extremely well and predict that cycle~24 will be about 35% weaker than cycle~23.

Arnab Rai Choudhuri; Piyali Chatterjee; Jie Jiang

2007-01-18T23:59:59.000Z

202

Solar startup to manufacture in Milwaukee | Department of Energy  

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

Solar startup to manufacture in Milwaukee Solar startup to manufacture in Milwaukee Solar startup to manufacture in Milwaukee August 10, 2010 - 10:00am Addthis Helios USA will build photovoltaic modules such as these this fall. | File photo Helios USA will build photovoltaic modules such as these this fall. | File photo Joshua DeLung $1 million loan through Wisconsin funded by Recovery Act to Helios USA Loan helps cover upfront costs of 40,000-square-foot factory 20 employees to be hired this year, more than 100 within five years Helios USA, a startup solar energy company based in Wisconsin, will begin manufacturing photovoltaic modules in Milwaukee this fall. The firm is the first in the state to do so. Helios, founded in February 2009, received a $1 million loan from the state in May 2010, funded by the American Recovery

203

SciTech Connect: Solar Energy Education. Home economics: student...  

Office of Scientific and Technical Information (OSTI)

Solar Energy Education. Home economics: student activities. Field test edition Citation Details In-Document Search Title: Solar Energy Education. Home economics: student...

204

National Laboratory Concentrating Solar Power Research and Development  

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

and performance improvements across all major concentrating solar power (CSP) subsystems-solar fields, power plants, receivers, and thermal storage-are necessary to achieve the...

205

A Continuous Solar Thermochemical Hydrogen Production Plant Design  

E-Print Network [OSTI]

16, 2013 [22] Solar Central Power Towers. Web. 22 AprilA diagram of the solar field, the receiver tower, the NaCl

Luc, Wesley Wai

206

FIELD DEPENDENT ADAPTIVE OPTICS CORRECTION DERIVED WITH THE SPECTRAL RATIO TECHNIQUE  

E-Print Network [OSTI]

for Solar-Terrestrial Research, 323 Martin Luther King Blvd, Newark, NJ 07102, U.S.A. 2 National Solar Bear Solar Observatory (BBSO) in 2005 and with the Dunn Solar Telescope (DST) at the National Solar atmosphere dominated seeing, as well as different FOVs of the wavefront sensors. In addition, we find

207

The Astrophysical Journal, 495:L27L30, 1998 March 1 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.  

E-Print Network [OSTI]

were made at the Vacuum Tower Telescope of the National Solar Observatory in Sunspot, New Mexico. All rights reserved. Printed in U.S.A. ON THE ORIGIN OF SOLAR OSCILLATIONS Philip R. Goode,1,2 Louis H and relate them to theories of the excitation of solar oscillations. We also discuss the local seismic

208

Solar Easements  

Broader source: Energy.gov [DOE]

New Jersey law provides for the creation of solar easements to ensure that proper sunlight is available to those who operate solar-energy systems. The term "solar energy device" is not defined by...

209

Solar Easements  

Broader source: Energy.gov [DOE]

Virginia's solar easement law is similar to those in effect in other states. The Virginia Solar Easements Act of 1978 allows property owners to create binding solar easements for the purpose of...

210

Literature Survay in the Field of Primary and Secondary Concentrating Solar Energy Systems Concerning the Choice and Manufacturing Process of Suitable Materials  

Science Journals Connector (OSTI)

The following report summarizes the actual knowledge concerning aspects of solar energy, that had been specified in the convocation.

A. Grychta; J. Kaufmann; P. Lippert; G. Lensch

1987-01-01T23:59:59.000Z

211

, Effect Publishing, New York, USA, 1991 , Hermitage Publishing, New Jersey, USA, 1995  

E-Print Network [OSTI]

1 . «», Effect Publishing, New York, USA, 1991 « », Hermitage Publishing, New Jersey, USA and hints at manifestations of the metaphysical." ("World Literature Today" , Automn, 1995, USA, USA) « . , , , , , "" , » (, 10, 2004) «"" . -- , , -- , ». ( , 69, 2004

Karpovsky, Mark

212

The solar interior - radial structure, rotation, solar activity cycle  

E-Print Network [OSTI]

Some basic properties of the solar convection zone are considered and the use of helioseismology as an observational tool to determine its depth and internal angular velocity is discussed. Aspects of solar magnetism are described and explained in the framework of dynamo theory. The main focus is on mean field theories for the Sun's magnetic field and its differential rotation.

Axel Brandenburg

2007-03-28T23:59:59.000Z

213

Solar collector  

DOE Patents [OSTI]

The field of this invention is solar collectors, and more particularly, the invention pertains to a flat plate collector that employs high performance thin films. The solar collector of this invention overcomes several problems in this field, such as excessive hardware, cost and reliability, and other prior art drawbacks outlined in the specification. In the preferred form, the apparatus features a substantially rigid planar frame (14). A thin film window (42) is bonded to one planar side of the frame. An absorber (24) of laminate construction is comprised of two thin film layers (24a, 24b) that are sealed perimetrically. The layers (24a, 24b) define a fluid-tight planar envelope (24c) of large surface area to volume through which a heat transfer fluid flows. Absorber (24) is bonded to the other planar side of the frame. The thin film construction of the absorber assures substantially full envelope wetting and thus good efficiency. The window and absorber films stress the frame adding to the overall strength of the collector.

Wilhelm, William G. (Cutchogue, NY)

1982-01-01T23:59:59.000Z

214

Undocumented Migration in the USA and Germany  

E-Print Network [OSTI]

Undocumented Migration in the USA and Germany: An AnalysisUndocumented Migration in the USA and Germany. An Analysismore restricted than in the USA. To my knowledge, there is

Stobbe, Holk

2000-01-01T23:59:59.000Z

215

Teaching-Assistantships in England/USA  

E-Print Network [OSTI]

Teaching-Assistantships in England/USA Anglistik University Atlanta/ U.S.A. (August 2014 ­ Mai 2015), Stipendium") oder in der Sprechstunde von Christoph Singer. #12;Studienplatz USA Anglistik

Noé, Reinhold

216

NPP Grassland: Konza Prairie, U.S.A. [Kansas]  

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

Konza Prairie, U.S.A., 1984-1990 Konza Prairie, U.S.A., 1984-1990 Data Citation Cite this data set as follows: Knapp, A. K., and D. Ojima. 1996. NPP Grassland: Konza Prairie, U.S.A., 1984-1990. Data set. Available on-line [http://www.daac.ornl.gov] from Oak Ridge National Laboratory Distributed Active Archive Center, Oak Ridge, Tennessee, U.S.A. Description Productivity of a humid temperate tall-grass prairie was determined at the Konza Prairie Natural Research Area from 1975 to the present. Monthly dynamics of above-ground plant biomass have been monitored since 1984, and estimates of above-ground plant production have been made since 1975. The Konza Prairie was the site of the First ISLSCP (International Satellite Land Surface Climatology Project) Field Experiment (FIFE), an intensive

217

Community Shared Solar with Solarize  

Broader source: Energy.gov [DOE]

An overview of the concept behind The Solarize Guidebook, which offers neighborhoods a plan for getting volume discounts when making group purchases of rooftop solar energy systems.

218

AREA USA LLC | Open Energy Information  

Open Energy Info (EERE)

AREA USA LLC Jump to: navigation, search Name: AREA USA LLC Place: Washington, DC Zip: 20004 Sector: Services Product: Washington, D.C.-based division of Fabiani & Company...

219

Energy Pro USA | Open Energy Information  

Open Energy Info (EERE)

Pro USA Jump to: navigation, search Name: Energy Pro USA Place: Chesterfield, Missouri Zip: MO 63017 Product: Energy Pro funds and implements demand side energy savings programs to...

220

Windkraft Nord USA | Open Energy Information  

Open Energy Info (EERE)

Windkraft Nord USA Jump to: navigation, search Name: Windkraft Nord USA Place: San Diego, California Zip: 92122 Product: Subsidiary of WKN AG based in North America. References:...

Note: This page contains sample records for the topic "usa solar fields" 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

Overview of BNL's Solar Energy Research Plansgy  

E-Print Network [OSTI]

Overview of BNL's Solar Energy Research Plansgy March 8, 2011, #12;Outline O i f th LISF S l PV P j Field LIPA Substation South Array Field LIPA Substation #12;#12;#12;BNL is developing a solar energy, February 2009 � EERE Renewable Systems interconnection Study, February 2008 � EERE Solar Energy Technology

Homes, Christopher C.

222

Manuscript Submitted to Solar Energy 4/2002 A NEW OPERATIONAL SATELLITE-TO-IRRADIANCE MODEL DESCRIPTION AND VALIDATION  

E-Print Network [OSTI]

Manuscript Submitted to Solar Energy 4/2002 A NEW OPERATIONAL SATELLITE-TO-IRRADIANCE MODEL, OR, USA #12;Manuscript Submitted to Solar Energy 4/2002 ABSTRACT We present a new simple model zenith angle to account for first order solar #12;Manuscript Submitted to Solar Energy 4/2002 geometry

Perez, Richard R.

223

A model and observations of the multifractal spectrum of the heliospheric magnetic field strength fluctuations near 40 AU  

E-Print Network [OSTI]

, Greenbelt, Maryland, USA C. Wang Center for Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA Laboratory for Space Weather, Chinese Academy of Sciences, Beijing, China N. F. Ness Bartol phases of the solar cycle (the decli- ning phase, solar minimum, and the rising phase approach- ing solar

Richardson, John

224

Philadelphia, Pennsylvania: Solar in Action (Brochure), Solar...  

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

(Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Boston Massachusetts: Solar in Action (Brochure), Solar America Cities, Energy Efficiency &...

225

OpenEI - solar thermal  

Open Energy Info (EERE)

Summary World Solar Summary World Solar Energy Data (from World on the Edge) http://en.openei.org/datasets/node/460 This dataset presents summary information related to world solar energy. It is part of a supporting dataset for the book World On the Edge: How to Prevent Environmental and Economic Collapse by Lester R.

License
field field-type-text field-field-license-type"> Type of License:  Open Data Commons Attribution License - Attribution for

226

Alternative Application of Solar Sail Technology  

Science Journals Connector (OSTI)

The development of Gossamer sail structures for solar sails contributes to a large field of future space applications like thin film solar generators, membrane antennas and drag sails. ... the development of a dr...

Nino Wolff; Patric Seefeldt; Wolfgang Bauer

2014-01-01T23:59:59.000Z

227

The Solar System in the next millennium  

Science Journals Connector (OSTI)

...non-magnetic interactions with the solar wind (adapted from Kivelson & Russell 1995). The two panels on the right illustrate the bow shocks...of Saturn but it is sometimes in the solar wind, and field line draping seems...

1999-01-01T23:59:59.000Z

228

Solar Keymark Testing of Solar Thermal Products  

Science Journals Connector (OSTI)

The Solar Keymark is the official CEN certification scheme for thermal solar collectors and factory made thermal solar systems. The Solar Keymark requires that the products fulfil the...

Harald Drck; Stephan Fischer

2009-01-01T23:59:59.000Z

229

Simulation Research Group, LBNL, USA  

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

* T. Hong () Simulation Research Group, LBNL, USA e-mail: thong@lbl.gov Building Energy Benchmarking between the United States and China: Methods and Challenges Tianzhen Hong 1,* , Le Yang 2 , Jianjun Xia 2 , Wei Feng 1 1 Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA 2 Tsinghua University, Beijing 100084, China Abstract. Currently, buildings in the U.S. account for more than 40% of total primary energy. In China the

230

Scattering Solar Thermal Concentrators  

Broader source: Energy.gov [DOE]

"This fact sheet describes a scattering solar thermal concentrators project awarded under the DOE's 2012 SunShot Concentrating Solar Power R&D award program. The team, led by the Pennsylvania State University, is working to demonstrate a new, scattering-based approach to concentrating sunlight that aims to improve the overall performance and reliability of the collector field. The research team aims to show that scattering solar thermal collectors are capable of achieving optical performance equal to state-of-the-art parabolic trough systems, but with the added benefits of immunity to wind-load tracking error, more efficient land use, and utilization of stationary receivers."

231

Multi-objective optimization of solar tower power plants  

E-Print Network [OSTI]

Multi-objective optimization of solar tower power plants Pascal Richter Center for Computational · Optimization of solar tower power plants 1/20 #12;Introduction ­ Solar tower power plants Solar tower PS10 (11 MW) in Andalusia, Spain · Solar tower with receiver · Heliostat field with self-aligning mirrors

Ábrahám, Erika

232

Mirror Mode Structures in the Solar Wind: STEREO Observations  

E-Print Network [OSTI]

Mirror Mode Structures in the Solar Wind: STEREO Observations O. Enríquez-Rivera1 , X. Blanco-Cano1 Autónoma de México, Coyoacán, D.F., 04510, MEXICO 2. Institute of Geophysics and Planetary Physics of California, Berkeley, CA 94720, USA Abstract. Mirror mode structures occur in the solar wind either

California at Berkeley, University of

233

Controlling access to pervasive information in the "Solar" system  

E-Print Network [OSTI]

Controlling access to pervasive information in the "Solar" system Kazuhiro Minami and David Kotz Dept. of Computer Science, Dartmouth College Hanover, NH, USA 03755 {minami, dfk}@cs.dartmouth.edu http://www.cs.dartmouth.edu/~solar and enforced in a decentralized, distributed system with no central administrator or central policy maker

234

Next-Generation Solar Collectors for CSP  

Broader source: Energy.gov [DOE]

This fact sheet on Next-Generation Collectors for CSP highlights a solar energy program awarded through the 2012 SunShot Concentrating Solar Power R&D awards. The team is developing new solar collector base technologies for next-generation heliostats used in power tower systems. If successful, this project will result in a 50% reduction in solar field equipment cost and a 30% reduction in field installation cost compared to existing heliostat designs.

235

Scientific Committee Gina Ahlstrom, FHWA, USA  

E-Print Network [OSTI]

Scientific Committee Gina Ahlstrom, FHWA, USA Enrico Benetto, PRC Tudor, Luxembourg Youcef State University/ISCP, USA Laëtitia D'Aloïa, CERTU, France Hervé Di Benedetto, ENTPE, France Heather Dylla, National Asphalt Pavement Association, USA Jon Epps, Texas A&M, USA Adélaïde Feraille

California at Davis, University of

236

20-. , -USAS (UCREL semantic analysis system) 2.  

E-Print Network [OSTI]

. . - , - . , - , ( - ) - . 20- . , - , - ­ - USAS (UCREL semantic analysis system) 2. WordNet3, EuroWordNet4 USAS - Wmatrix http://www.comp.lancs.ac.uk/ucrel/wmatrix/. 3 Fellbaum C. (ed), Word. 73-89. 5 http://www.keenage.com #12;2 () . - USAS - . , , , c USAS

Rayson, Paul

237

University of Tennessee, USA Pacific Northwest National Laboratory,  

E-Print Network [OSTI]

#12; : University of Tennessee, USA Pacific Northwest National Laboratory, USA Georgia State University, USA University of Virginia, USA The Ohio State University, USA National Institute for Materials Science, Japan

Wang, Zhong L.

238

Sharp Electronics Corporation USA | Open Energy Information  

Open Energy Info (EERE)

USA USA Jump to: navigation, search Name Sharp Electronics Corporation (USA) Place Huntington Beach, California Zip 92647 Product North American division of Japanese electronics company References Sharp Electronics Corporation (USA)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Sharp Electronics Corporation (USA) is a company located in Huntington Beach, California . References ↑ "Sharp Electronics Corporation (USA)" Retrieved from "http://en.openei.org/w/index.php?title=Sharp_Electronics_Corporation_USA&oldid=350899" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version

239

Alternative Fuels Data Center: Clean Construction USA  

Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

Construction USA Construction USA to someone by E-mail Share Alternative Fuels Data Center: Clean Construction USA on Facebook Tweet about Alternative Fuels Data Center: Clean Construction USA on Twitter Bookmark Alternative Fuels Data Center: Clean Construction USA on Google Bookmark Alternative Fuels Data Center: Clean Construction USA on Delicious Rank Alternative Fuels Data Center: Clean Construction USA on Digg Find More places to share Alternative Fuels Data Center: Clean Construction USA on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Clean Construction USA Clean Construction USA is a voluntary program that promotes the reduction of diesel exhaust emissions from construction equipment and vehicles by encouraging proper operations and maintenance, use of emissions-reducing

240

Alternative Fuels Data Center: Clean Agriculture USA  

Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

Clean Agriculture USA Clean Agriculture USA to someone by E-mail Share Alternative Fuels Data Center: Clean Agriculture USA on Facebook Tweet about Alternative Fuels Data Center: Clean Agriculture USA on Twitter Bookmark Alternative Fuels Data Center: Clean Agriculture USA on Google Bookmark Alternative Fuels Data Center: Clean Agriculture USA on Delicious Rank Alternative Fuels Data Center: Clean Agriculture USA on Digg Find More places to share Alternative Fuels Data Center: Clean Agriculture USA on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Clean Agriculture USA Clean Agriculture USA is a voluntary program that promotes the reduction of diesel exhaust emissions from agricultural equipment and vehicles by encouraging proper operations and maintenance by farmers, ranchers, and

Note: This page contains sample records for the topic "usa solar fields" 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

Alternative Fuels Data Center: Clean Ports USA  

Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

Ports USA to Ports USA to someone by E-mail Share Alternative Fuels Data Center: Clean Ports USA on Facebook Tweet about Alternative Fuels Data Center: Clean Ports USA on Twitter Bookmark Alternative Fuels Data Center: Clean Ports USA on Google Bookmark Alternative Fuels Data Center: Clean Ports USA on Delicious Rank Alternative Fuels Data Center: Clean Ports USA on Digg Find More places to share Alternative Fuels Data Center: Clean Ports USA on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Clean Ports USA Clean Ports USA is an incentive-based program designed to reduce emissions by encouraging port authorities and terminal operators to retrofit and replace older diesel engines with new technologies and use cleaner fuels.

242

A brief history of the solar oblateness. J.P. Rozelot,a  

E-Print Network [OSTI]

A brief history of the solar oblateness. A review. J.P. Rozelot,a , C. Damianib , S. Lefebvrec , A-4085, (USA) Abstract We hereby present a review on solar oblateness measurements. By emphasizing historical theories. We stress out the need to get accurate data from space to enhance our knowledge of the solar core

Boyer, Edmond

243

Department of Solar Energy & Environmental Physics Conference presentations, 2006-2007.  

E-Print Network [OSTI]

Department of Solar Energy & Environmental Physics Conference presentations, 2006-2007. Albu, (eds.) Proceedings of the 22nd European Photovoltaic Solar Energy Conference. Milan, Italy, pp. 132: L. Vayssieres (ed.) Solar Hydrogen and Nanotechnology - Proceedings of SPIE, San Diego, USA. Albu

Prigozhin, Leonid

244

New Astronomy Reviews 42 (1998) 489492 Site tests for CLEAR by solar scintillometry  

E-Print Network [OSTI]

Mexico) because the Big the boundary layer, which for day-time solar observ- Bear measurements indicatedNew Astronomy Reviews 42 (1998) 489­492 Site tests for CLEAR by solar scintillometry a b Jacques M. Beckers , Robert J. Rutten a 1 National Solar Observatory/NOAO, P.O. Box 26732, Tucson, AZ 85726, USA b

Rutten, Rob

245

Cloud Formation in the Plumes of Solar Chimney Power Generation Facilities: A Modeling Study  

E-Print Network [OSTI]

1 Cloud Formation in the Plumes of Solar Chimney Power Generation Facilities: A Modeling Study Institute of Technology, 311 Ferst Drive, Atlanta , Georgia 30332-0340, USA Abstract The solar chimney power the potential impacts on plant capacity resulting from cloud formation within or downwind of the solar chimney

Nenes, Athanasios

246

Solar MagnetoConvection David J. Bercik  

E-Print Network [OSTI]

Solar Magneto­Convection David J. Bercik Dept. of Physics and Astronomy, Michigan State University, Michigan State University, East Lansing, MI 48824, U.S.A. š Ake Nordlund Theoretical Astrophysics Center, ?ster Voldgade 3, 1350 Copenhagen K, Denmark Robert F. Stein Dept. of Physics and Astronomy, Michigan

Stein, Robert

247

Solar Energy  

Science Journals Connector (OSTI)

There are major advantages to using solar energy for a variety of energy needs including electrical generation and space heating. The availability of solar radiation is extremely high in some localities of the...

Charles E. Brown Ph.D.

2002-01-01T23:59:59.000Z

248

Solar Easements  

Broader source: Energy.gov [DOE]

Idahos solar easement provisions allow for the access rights to sunlight for a solar energy device. The easement is transferred with the property title. Only a few Idaho communities have passed...

249

Solar Easements  

Broader source: Energy.gov [DOE]

Alaska's solar easement provisions are similar to those in many other states. They do not create an automatic right to sunlight. Rather, they allow parties to voluntarily enter into solar...

250

Solar Easements  

Broader source: Energy.gov [DOE]

Rhode Island allows property owners to establish solar easements in the same manner and with the same effect as a conveyance of an interest in real property. Solar easements must be created in...

251

Solar Easements  

Broader source: Energy.gov [DOE]

Ohio's solar-easement provisions are similar to those in effect in other states. Ohio law allows property owners to create binding solar easements for the purpose of protecting and maintaining...

252

Solar Easements  

Broader source: Energy.gov [DOE]

In determining that the use of solar energy "can help reduce the nation's reliance upon imported fuels," Georgia encourages the development of solar-energy systems. Accordingly, under Georgia's...

253

An Introduction of Richard Heinberg New College of California, Santa Rosa, CA, USA  

E-Print Network [OSTI]

An Introduction of Richard Heinberg New College of California, Santa Rosa, CA, USA Seminar;. . #12;Why exactly does a Society or an Economy depend upon Energy? Thermodynamics · Energy: capacity (corn) 1.3 today 10 Ethanol (corn residues) 0.7­1.8 Coal Methanol (wood) 2.6 1950s 80 Solar space heat

Keeling, Stephen L.

254

Solar energy  

Science Journals Connector (OSTI)

... good book and certainly can be recommended as an introductory text for a course on solar ...solarenergy ...

D.O. Hall

1980-02-28T23:59:59.000Z

255

Total Solar Irradiance Variability and the Solar Activity Cycle  

E-Print Network [OSTI]

It is suggested that the solar variability is due to the perturbed nature of the solar core and this variability is provided by the variability of the solar neutrino flux from the solar neutrino detectors i.e., Homestake, Superkamiokande, SAGE and GALLEX-GNO. The solar neutrino flux in the standard solar model (SSM) was calculated on the assumption of L_nu (neutrino luminosity) = L_gamma (optical luminosity) which implies that if there is a change in optical luminosity then solar neutrino flux data will also be changed. An internal dynamo due to the cyclic variation of nuclear energy generation inside the core of the sun is responsible for the solar activity cycle was suggested and thus the internal magnetic field is also variable. Again the changes in the nuclear energy generation induce structural changes that result in variations of the global solar parameters i.e., luminosity, radius and temperatures etc. From the analysis of total solar irradiance (TSI) data during the year from 1970 to 2003 we have found five phases within the solar activity cycle. The first phase (I) starts before two years from the sunspot minimum. The second phase (II) starts at the time of sunspot minimum and phase (III) starts before 2/3 years from sunspot maximum whereas phase (IV) starts at sunspot maximum and fifth phase (V) starts at after 2-3 years from sunspot maximum.

Probhas Raychaudhuri

2006-05-06T23:59:59.000Z

256

De'Longhi USA, Inc.  

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

De'Longhi USA, Inc. De'Longhi USA, Inc. (Dehumidifiers) BEFORE THE U.S. DEPARTMENT OF ENERGY Washington, D.C. 20585 ) 1 ) Case Number: 20 10-CE-2114 ) ) NOTICE OF PROPOSED CIVIL PENALTY Date issued: September 8,2010 Number of alleged violations: 13 Maximum possible assessment: $741,820 Proposed civil penalty: $94,900 The Office of the General Counsel of the U.S. Department of Energy (DOE) alleges that De'Longhi USA, Inc. (DeyLonghi) violated certain provisions of the Energy Policy and Conservation Act, 42 U.S.C. $ 6201 et seq., 10 C.F.R. Part 430, or both. Specifically, DOE alleges: 1. DeyLonghi manufactures or privately labels a variety of dehumidifiers, including, models DD40P, DD45, DD45P, DDSOP, DE400, DE400P, DE500, DESOOP, DE650P, DENSOOP, DG50, and DW30M.

257

Solar DEM Models : A solar image in color band b, mn pixels,  

E-Print Network [OSTI]

Solar DEM Models : A solar image in color band b, m?n pixels, containing a particular solar feature, for t = 1, 2, . . . , T. btM sianFieldRandomGaus I M I I bbb T t bbtt bbb bb 2 1 2 )( #12;Solar DEM.bI : the measure error of the ith row and jth column pixel of the certain image in color band b. ijbe #12;Solar DEM

Wolfe, Patrick J.

258

THE POLARITY DISTRIBUTION OF INTRANETWORK AND NETWORK FIELDS  

E-Print Network [OSTI]

Solar Observatory, New Jersey Institute of Technology, U.S.A. (E- mail: zjun obtained at Big Bear Solar Observatory (BBSO) and Huairou Solar Observation Station (HSOS). We found 80 network cells and measured the polarities of intranetwork and network magnetic flux within each cell

259

A simulation study of the solar wind including the solar rotation effect  

Science Journals Connector (OSTI)

An axisymmetric solar wind structure including the solar rotation effect is studied by the method of MHD computer simulation. For the case of the radial magnetic field configuration, the simulation result is fair...

H. Washimi; T. Sakurai

1993-01-01T23:59:59.000Z

260

Solar Power  

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

Solar Power Solar Power Project Opportunities Abound in the Region The WIPP site is receives abundant solar energy with 6-7 kWh/sq meter power production potential As the accompanying map of New Mexico shows, the WIPP site enjoys abundant year-round sunshine. With an average solar power production potential of 6-7 kWh/sq meter per day, one exciting project being studied for location at WIPP is a 30-50 MW Solar Power Tower: The American Solar Energy Society (ASES) is is a national trade association promoting solar energy as a clean source of electricity, and provides a comprehensive resource for additional information. DOE's Office of Energy Efficiency and Renewable Energy is also a comprehensive resource for more information on renewable energy.

Note: This page contains sample records for the topic "usa solar fields" 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

Optical Optimization of Organic Solar Cells  

Science Journals Connector (OSTI)

The electromagnetic field distribution inside multilayer organic solar cells is simulated and optimized. The relative importance of optical, electrical and morphological properties...

Monestier, Florent; Simon, Jean-Jacques; Torchio, Philippe; Escoubas, Ludovic; Flory, Franois; El Amrani, Aumeur; Moliton, Andr; Ratier, Bernard; Cathelinaud, Michel; Defranoux, Christophe

262

Solar Phys (2009) 256: 285305 DOI 10.1007/s11207-009-9354-5  

E-Print Network [OSTI]

Solar Phys (2009) 256: 285­305 DOI 10.1007/s11207-009-9354-5 STEREO SCIENCE RESULTS AT SOLAR MINIMUM Solar Wind Sources in the Late Declining Phase of Cycle 23: Effects of the Weak Solar Polar Field.com Abstract The declining phases of solar cycles are known for their high speed solar wind streams

California at Berkeley, University of

263

Slow magnetohydrodynamic waves in the solar atmosphere  

Science Journals Connector (OSTI)

...waves and oscillations in the solar plasma organized by Robert Erdelyi...waves at a magnetic interface. Solar Phys. 69, 1981a 27-38...Cram1981bpp. 369-383. Eds. New Mexico:Sunspot, Sacramento Peak...Magnetohydrodynamic waves. In Solar system magnetic fields E.R...

2006-01-01T23:59:59.000Z

264

Magnetic coupling in the solar system  

Science Journals Connector (OSTI)

......Bewsher Chris Davis Head of Solar and Stellar Physics at...sam@mssl.ac.uk . Solar physicist working with...Appleton Laboratory. Project Scientist for the STEREO...the complexities of the solar magnetic field, informed...own) and their moons. Energy from within the convection......

Sarah Matthews; Danielle Bewsher; Chris Davis

2009-04-01T23:59:59.000Z

265

Abengoa Solar, Inc. (Mojave Solar) | Department of Energy  

Energy Savers [EERE]

Solar, Inc. (Mojave Solar) Abengoa Solar, Inc. (Mojave Solar) Abengoa Solar, Inc. (Mojave Solar) Location: San Bernardino County, CA Eligibility: 1705 Snapshot In September 2011,...

266

Computerization and Competitiveness: National Information Infrastructure in the USA  

E-Print Network [OSTI]

stay 'fairly intense,' USA Today, August 1994. Clinton,INFRASTRUCTURE IN THE USA Kenneth L. Kraemer Professor ofINFRASTRUCTURE IN THE USA INTRODUCTION The production and

Kraemer, Kenneth L.

1994-01-01T23:59:59.000Z

267

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

Estimating Unmeasured Solar Radiation Quantities . . . . . .Weather Data . . . . . , . , . . . . . . . . . .Solar DataB. l'he Solar Constant. . . . . . C. Solar Time and Standard

Berdahl, P.

2010-01-01T23:59:59.000Z

268

Euro Chef USA: Order (2014-CE-23004)  

Broader source: Energy.gov [DOE]

DOE ordered Euro Chef USA Inc. to pay a $8,000 civil penalty after finding Euro Chef USA had failed to certify that certain models of cooking products comply with the applicable energy conservation standards.

269

Absolute Energy USA | Open Energy Information  

Open Energy Info (EERE)

USA Jump to: navigation, search Name: Absolute Energy (USA) Place: St. Ansgar, Iowa Zip: 50472 Product: Absolute Energy has built a 100 million gallon per year ethanol plant on the...

270

Hisense USA: Order (2010-CE-1211)  

Broader source: Energy.gov [DOE]

DOE issued an Order after entering into a Compromise Agreement with Hisense USA Corp. after finding Hisense USA had failed to certify that certain models of residential refrigerators, refrigerator-freezers, and freezers comply with the applicable energy conservation standards.

271

Sandia National Laboratories: Solar Tower  

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

Solar Thermal Test Facility * NSTTF * Renewable Energy * SAND2012-8086W * solar * Solar Energy * solar power * Solar Research * Solar Tower Comments are closed. Renewable...

272

DOE Solar Decathlon: 2007 Juries  

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

Two jurors holding notebooks listen intently as a young member of the Lawrence Technological Team explains the home's environmental features and sustainable materials during the 2007 Solar Decathlon. Between them is a desk and chair made from sustainable wood. Two jurors holding notebooks listen intently as a young member of the Lawrence Technological Team explains the home's environmental features and sustainable materials during the 2007 Solar Decathlon. Between them is a desk and chair made from sustainable wood. A Lawrence Technological University student explains to architectural jurors that the team's environmental ethic is reflected in the choice of materials used in their home during the 2007 Solar Decathlon. Solar Decathlon 2007 Juries The following panel of jurors assembled to judge the 2007 Solar Decathlon. The panels are composed of individuals at the top of their respective professions, who bring academic excellence and practical, in-the-field experience to the 10 contests. Using objective and subjective measures to evaluate the teams' solar

273

SciTech Connect: Solar Energy Education. Humanities: activities...  

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

and teacher's guide. Field test edition Citation Details In-Document Search Title: Solar Energy Education. Humanities: activities and teacher's guide. Field test edition ...

274

SciTech Connect: Solar Energy Education. Home economics: teacher...  

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

guide. Field test edition. Includes glossary Citation Details In-Document Search Title: Solar Energy Education. Home economics: teacher's guide. Field test edition. Includes...

275

SciTech Connect: Solar Energy Education. Industrial arts: teacher...  

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

guide. Field test edition. Includes glossary Citation Details In-Document Search Title: Solar Energy Education. Industrial arts: teacher's guide. Field test edition. Includes...

276

Dagan Solar Energy | Open Energy Information  

Open Energy Info (EERE)

Dagan Solar Energy Dagan Solar Energy Jump to: navigation, search Name Dagan Solar Energy Place Israel Zip 36052 Sector Solar Product Develops and implements technologies in the field of solar thermal energy. References Dagan Solar Energy[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Dagan Solar Energy is a company located in Israel . References ↑ "Dagan Solar Energy" Retrieved from "http://en.openei.org/w/index.php?title=Dagan_Solar_Energy&oldid=344034" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link Browse properties 429 Throttled (bot load) Error 429 Throttled (bot load)

277

Orion Registrar, Inc., USA Certificate of Registration  

E-Print Network [OSTI]

Orion Registrar, Inc., USA Certificate of Registration D'fus Js lo cerl!fy !he Occupalional Golden, Colorado 80401 USA J fas been assessedby Orion !l?egislrar and}Oundlobe 1i2 compliance mi-456-6681 To authenticate this certificate please visit www.orion4value.com #12;Orion Registrar, Inc., USA Certificate

278

Electrodialysis, powered by solar panels, could provide drinking water for villages in India  

Science Journals Connector (OSTI)

Off-grid communities in India with salty groundwater could obtain potable water by using electrodialysis, powered by solar panels, shows a study conducted by researchers in the USA at Massachusetts Institute of Technology.

2014-01-01T23:59:59.000Z

279

Solar cooling in Madrid: Available solar energy  

SciTech Connect (OSTI)

This paper analyzes the behaviour of an absorption chiller lithium bromide installation fed by a field of flat-plate solar collectors and condensed by swimming pool water. A method of calculation in a variable regime is developed in terms of the obtained experimental results. Starting from the meteorological variables of a clear summer day and from the project data (collector normalization curve, collector and installation mass), the minimum solar radiation level necessary to initiate the process, I[sub min], and the instantaneous available solar energy, Q[sub u] + W[sub 1] is determined. The solar radiation threshold, I[sub min], necessary to obtain the process temperature, t[sub ave], in each instant, is obtained by adding to the corrected Klein radiation threshold, I[sub k,c], the heat capacity effects of the collector, HCE[sub CO], and of the installation, HCE[sub ins], as well as the losses of heat of the pipes to the surroundings, Q[sub 1]. The instantaneous available solar energy, available useful heat, in addition to the wind collector losses to the surroundings, Q[sub u] + W[sub 1], is the difference, in each instant, between the radiation, I[sub g1T], and the radiation threshold, I[sub min].The integration during the day of the instantaneous available solar energy allows us to calculate the daily available function, H[sub T]. The value of H[sub T], measured in the swimming-pool water condensation installation reached 6.92 MJ/(m[sup 2] day ). The calculated values of H[sub T] for a conventional installation condensed by tower water, or air, have been 6.35 and 0.56 MJ/(m[sup 2] day). respectively.

Izquierdo, M.; Hernandez, F.; Martin, E. (Instituto de Ciencias de la Construccion Eduardo Torroja, Madrid (Spain))

1994-11-01T23:59:59.000Z

280

Solar Decathlon  

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

U.S. Department of Energy U.S. Department of Energy Solar Decathlon Sara Farrar-Nagy National Renewable Energy Laboratory sara.farrar-nagy@nrel.gov, 303-384-7514 April 3, 2013 Solar Decathlon 2009 Solar Decathlon 2011 Solar Decathlon 2013 & XPO Washington, D.C. Washington, D.C. Irvine, California 2 | Building Technologies Office eere.energy.gov Purpose & Objectives Problem Statement: How to provide workforce training, improve building science instruction, foster innovation in whole-building design, and

Note: This page contains sample records for the topic "usa solar fields" 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

Solar Energy.  

E-Print Network [OSTI]

??This thesis is about Photovoltaic (PV) cells and its stresses in various directions by calculating the power generated using solar cells under different conditions to (more)

Bafana, Ramzi

2014-01-01T23:59:59.000Z

282

Solar Mapper  

Broader source: Energy.gov [DOE]

Interactive, online mapping tool providing access to spatial data related to siting utility-scale solar facilities in the southwestern United States.

283

Solar startup to manufacture in Milwaukee | Department of Energy  

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

startup to manufacture in Milwaukee startup to manufacture in Milwaukee Solar startup to manufacture in Milwaukee August 10, 2010 - 10:00am Addthis Helios USA will build photovoltaic modules such as these this fall. | File photo Helios USA will build photovoltaic modules such as these this fall. | File photo Joshua DeLung $1 million loan through Wisconsin funded by Recovery Act to Helios USA Loan helps cover upfront costs of 40,000-square-foot factory 20 employees to be hired this year, more than 100 within five years Helios USA, a startup solar energy company based in Wisconsin, will begin manufacturing photovoltaic modules in Milwaukee this fall. The firm is the first in the state to do so. Helios, founded in February 2009, received a $1 million loan from the state in May 2010, funded by the American Recovery

284

Application of Machine Learning in Solar Physics Frank Y. Shih, Ju Jing, Ming Qu, and Haimin Wang  

E-Print Network [OSTI]

Center for Solar-Terrestrial Research, New Jersey Institute of Technology Newark, NJ 07102, U.S.A. and Big Bear Solar Observatory, New Jersey Institute of Technology, 40386 North Shore Lane, Big Bear CityApplication of Machine Learning in Solar Physics Frank Y. Shih¹, Ju Jing², Ming Qu¹, and Haimin

285

A PARALLEL ADAPTIVE 3D MHD SCHEME FOR MODELING CORONAL AND SOLAR WIND PLASMA FLOWS  

E-Print Network [OSTI]

A PARALLEL ADAPTIVE 3D MHD SCHEME FOR MODELING CORONAL AND SOLAR WIND PLASMA FLOWS C. P. T. GROTH, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109­2143, USA K. G. POWELL Department of Aerospace Engineering, University of Michigan, Ann Arbor, MI 48109­2118, USA Abstract. A parallel adaptive

De Zeeuw, Darren L.

286

DOE Solar Decathlon: Solar Decathlon Videos  

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

Consumer Workshops Consumer Workshops Building Industry Workshops Technical Resources Sponsors Where Are the Houses Now? Quick Links Solar Decathlon Home Solar Decathlon 2011 Solar Decathlon 2009 Solar Decathlon 2007 Solar Decathlon 2005 Solar Decathlon 2002 Solar Decathlon 2011 Solar Decathlon Videos For video of the U.S. Department of Energy Solar Decathlon 2011, see the collections listed below or visit the U.S. Department of Energy Solar Decathlon YouTube Channel. General Solar Decathlon Videos Watch these videos to learn about the Solar Decathlon competition and event. Solar Decathlon House Video Tours Learn about each of the U.S. Department of Energy Solar Decathlon teams and their houses in these video tours. Solar Decathlon Team-Produced Videos Watch videos produced by the teams themselves for the Solar Decathlon

287

Solar Power  

Science Journals Connector (OSTI)

...of desert solar energy farm with 30 percent conversion...85 percent of the solar farm energy now reflected back...Washington, D.C. 20550. Wind Power Martin Wolf (19...counting the cost of the offshore platforms, would thus...15 billion. If these wind generators were placed...

Paul E. Damon

1974-08-09T23:59:59.000Z

288

Plenary Speakers Weng Cho Chew (Hongkong/USA)  

E-Print Network [OSTI]

Plenary Speakers Weng Cho Chew (Hongkong/USA) Vladimir G. Maz ya (UK/Sweden) Jean-Claude Nédélec (France) Wolfgang L. Wendland (Germany) Invited Speakers Thomas S. Angell (USA) Giles Auchmuty (USA) Constantin Bacuta (USA) Yassine Boubendir (USA) Alexey Chernov (Germany) David Colton (USA) Martin Costabel

Gilbert, Robert P.

289

The Solar Wind-Magnetosphere-Ionosphere System  

Science Journals Connector (OSTI)

...Earth's magnetic field acts as the wires to transmit the solar wind energy to the ionosphere, where the energy is dissipated...Earth's magnetic field acts as the wires to transmit the solar wind energy to the ionosphere, where the energy is dissipated...

John G. Lyon

2000-06-16T23:59:59.000Z

290

DOE Solar Decathlon: Contests  

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

Solar Decathlon Contests Solar Decathlon Contests Like the Olympic decathlon, the U.S. Department of Energy Solar Decathlon consists of 10 contests. These contests are designed to gauge how well the houses perform and how livable and affordable they are. Each contest is worth a maximum of 100 points, for a competition total of 1,000 points. Teams can earn points three ways: Task completion Teams complete household tasks such as cooking, washing dishes, and doing laundry. Monitored performance Team houses perform to specified criteria, such as maintaining a comfortable (71°-76°F) indoor temperature range. Jury evaluation Jurors who are experts in their field (such as architecture, engineering, and communications) award points for features that cannot be measured (such as aesthetics and design inspiration).

291

Detection of solar events  

DOE Patents [OSTI]

A flux detection apparatus can include a radioactive sample having a decay rate capable of changing in response to interaction with a first particle or a field, and a detector associated with the radioactive sample. The detector is responsive to a second particle or radiation formed by decay of the radioactive sample. The rate of decay of the radioactive sample can be correlated to flux of the first particle or the field. Detection of the first particle or the field can provide an early warning for an impending solar event.

Fischbach, Ephraim; Jenkins, Jere

2013-08-27T23:59:59.000Z

292

GroSolar formerly Global Resource Options Inc | Open Energy Information  

Open Energy Info (EERE)

GroSolar formerly Global Resource Options Inc GroSolar formerly Global Resource Options Inc Jump to: navigation, search Name groSolar (formerly Global Resource Options Inc) Place Vermont Zip VT 05001 Sector Solar Product A solar integration firm that designs, distributes, and installs solar electric, hot water and air systems in the USA. References groSolar (formerly Global Resource Options Inc)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. groSolar (formerly Global Resource Options Inc) is a company located in Vermont . References ↑ "groSolar (formerly Global Resource Options Inc)" Retrieved from "http://en.openei.org/w/index.php?title=GroSolar_formerly_Global_Resource_Options_Inc&oldid=346141

293

CORONAL MAGNETIC FIELD MEASUREMENTS THROUGH GYRORESONANCE EMISSION  

E-Print Network [OSTI]

Chapter 5 CORONAL MAGNETIC FIELD MEASUREMENTS THROUGH GYRORESONANCE EMISSION Stephen M. White This article reviews the use of gyroresonance emission at radio wavelengths to measure coronal magnetic fields. Keywords: Sun, solar corona, solar magnetic fields, solar radio emission Introduction Since the realization

White, Stephen

294

Method for processing silicon solar cells  

DOE Patents [OSTI]

The instant invention teaches a novel method for fabricating silicon solar cells utilizing concentrated solar radiation. The solar radiation is concentrated by use of a solar furnace which is used to form a front surface junction and back-surface field in one processing step. The present invention also provides a method of making multicrystalline silicon from amorphous silicon. The invention also teaches a method of texturing the surface of a wafer by forming a porous silicon layer on the surface of a silicon substrate and a method of gettering impurities. Also contemplated by the invention are methods of surface passivation, forming novel solar cell structures, and hydrogen passivation. 2 figs.

Tsuo, Y.S.; Landry, M.D.; Pitts, J.R.

1997-05-06T23:59:59.000Z

295

The Astrophysical Journal, 734:31 (11pp), 2011 June 10 doi:10.1088/0004-637X/734/1/31 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125, USA 7 Department California Institute of Technology, Department of Astrophysics, MC 249-17, Pasadena, CA 91125, USA 10 ESO, a transition between the much lower interstellar value and the higher value observed in solar system comets

Adolphs, Ralph

296

The Astronomical Journal, 144:14 (9pp), 2012 July doi:10.1088/0004-6256/144/1/14 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

.c.roberts@jpl.nasa.gov 2 American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024, USA 3. The American Astronomical Society. All rights reserved. Printed in the U.S.A. SPECTRAL TYPING OF LATE solar- type stars. Five of these stars are known binary stars and we detected the late-type secondaries

297

Solar Energy  

Science Journals Connector (OSTI)

The sun is the main source of all alternative energies on the earths surface. Wind energy, bioenergy, ocean energy, and hydro energy are derived from the sun. However,...solar energy refers to the energy that is...

Tushar K. Ghosh; Mark A. Prelas

2011-01-01T23:59:59.000Z

298

Solar collector  

SciTech Connect (OSTI)

A solar collector is disclosed which is tiltable about a horizontal axis so as to vary the angle at which solar radiation is received by the collector. The solar collector, which uses air as the heat transfer medium, has connected to it a pair of fixed, well-insulated air transfer passages which penetrate through into the interior of the collector at the lateral sides thereof aligned with the horizontal axis about which the collector is pivoted. The air transfer passages are insulated and are gasketed to the sides of the collector so as to improve the efficiency of the solar energy system by avoiding losses of heat from the heat transfer fluid during transfer of the fluid from the collector to the space being heated.

Stevenson, S.

1981-06-30T23:59:59.000Z

299

Solar energy  

Science Journals Connector (OSTI)

Even in European latitudes, solar energy can contribute towards the saving of a considerable amount of energy steming fron exhaustible sources. In the domestic sector (heating and cooling) there is even some p...

1977-01-01T23:59:59.000Z

300

Solar Easements  

Broader source: Energy.gov [DOE]

Maine allows for the creation of easements to ensure access to direct sunlight. Instruments creating a solar easement may include, but are not limited to, a description of the space affected by the...

Note: This page contains sample records for the topic "usa solar fields" 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

Solar Easements  

Broader source: Energy.gov [DOE]

Tennessee law allows for the creation of easements for the purpose of ensuring access to direct sunlight for solar energy systems. This statute also states that the "encouragement and protection of...

302

Solar Easements  

Broader source: Energy.gov [DOE]

In Kentucky, solar easements may be obtained for the purpose of ensuring access to direct sunlight. Easements must be expressed in writing and will become an interest in real property that may be...

303

DOE Solar Decathlon: 2009 Juries  

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

Communications jurors listening and taking pictures as two University of Louisiana at Lafayette team members speak. In front of the group is a wooden bench with integrated signs. Communications jurors listening and taking pictures as two University of Louisiana at Lafayette team members speak. In front of the group is a wooden bench with integrated signs. The Solar Decathlon 2009 Communications Jury inspects exterior signage on a visit to the University of Louisiana at Lafayette house. Solar Decathlon 2009 Juries The panel of judges and jurors assembled to evaluate the 20 U.S. Department of Energy Solar Decathlon 2009 teams and their houses is composed of individuals at the top of their professions. Renowned in their fields of study, they bring academic excellence and practical, in-the-field expertise to each of the 10 contests. Their involvement in the Solar Decathlon will help advance energy efficiency and renewable energy throughout the world.

304

SJ Solar | Open Energy Information  

Open Energy Info (EERE)

SJ Solar Jump to: navigation, search Name: SJ Solar Place: San Jose, California Zip: 95131 Sector: Solar Product: Cell design firm for concentrated solar References: SJ Solar1...

305

Sandia National Laboratories: Solar Research  

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

Solar Energy On February 3, 2011, in Solar Programs Photovoltaics Concentrating Solar Power Sunshine to Petrol Solar Publications Recent Solar Highlights Photovoltaics (PV)...

306

Sandia National Laboratories: Solar Furnace  

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

Test Facility * NSTTF * Parabolic Dish * Renewable Energy * SAND 2011-4654W * solar * Solar Energy * Solar Furnace * solar power * Solar Research Comments are closed. Renewable...

307

Solar Sail Propulsion: An Enabling Technology for Fundamental Physics Missions  

Science Journals Connector (OSTI)

Solar sails enable a wide range of high- ... system. They are also an enabling propulsion technology for two types of deep-space missions ... and the large-scale gravitational field of the solar system: the first...

Bernd Dachwald; Wolfgang Seboldt; Claus Lammerzahl

2008-01-01T23:59:59.000Z

308

Augmentation of thermal power stations with solar energy  

Science Journals Connector (OSTI)

A new concept of integration of a solar concentrator field with a modern thermal power station is proposed. Such a configuration ... and infrastructure as a base load facility and solar energy to reduce the fuel ...

BR Pai

1991-06-01T23:59:59.000Z

309

Simulation Calculation on Solar Chimney Power Plant System  

Science Journals Connector (OSTI)

It is unpractical to establish a Solar Chimney Power Plant System (SCPPS) used to ... flow field of the SCPPS which caused by solar radiation intensity have been analyzed. The calculated ... as well as the differ...

HuiLan Huang; Hua Zhang; Yi Huang; Feng Lu

2007-01-01T23:59:59.000Z

310

Dayside Aurora as an Indicator of Asymmetric Solar Wind-  

E-Print Network [OSTI]

magnetosphere responds directly to incident interplanetary magnetic field (IMF) and solar wind energy Changes the magnetosphere-ionosphere system responds to IMF and solar wind energy input #12;Introduction (part 2) Focus

Fillingim, Matthew

311

Solar News  

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

field-type-text-with-summary field-label-hidden">

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U.S. Deputy Secretary of Energy Daniel...

312

DOE Analysis Related to H2USA  

Broader source: Energy.gov [DOE]

Presentation slides from the DOE Fuel Cell Technologies Office webinar, DOE Analysis Related to H2USA, held on July 24, 2013.

313

USA PATRIOT ACT and civil liberties.  

E-Print Network [OSTI]

??In the wake of terrorist attacks in New York and Washington on September 11, 2001, the United States government hurriedly passed the USA PATRIOT Act. (more)

Bergstrom, M. Ann.

2005-01-01T23:59:59.000Z

314

Team China Solar Decathlon 2011 Project Manual  

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

China China TongjiUniversity 1 Project Manual Team China 20110715 Project Name: Y container, Solar Decathlon 2011 USA. Team Name: Team China, Tongji University Primary Student: HuaGuodong Faculty Advisor: Prof.TanHongwei Contact: , jellyhua@gmail.com,tong_team@yahoo.com Address: 1239 Siping Rd, Shanghai, China 200092 Tel: +86 65987788-8074 Team China TongjiUniversity 2 Table of contents Table of contents ................................................................................................................................................................. 2 1. Summary of Changes ...................................................................................................................................................... 6

315

Department of Solar Energy & Environmental Physics Scientific Publications, 2006-2007.  

E-Print Network [OSTI]

Department of Solar Energy & Environmental Physics Scientific Publications, 2006-2007. Albu:185-198. Faiman, D., Raviv, D. and Rosenstreich, R. (2007), Using solar energy to arrest the increasing rate of fossil-fuel consumption: The southwestern states of the USA as case studies. Energy Policy, 35

Prigozhin, Leonid

316

Low-energy particle response to CMEs during the Ulysses solar maximum northern polar passage  

E-Print Network [OSTI]

Low-energy particle response to CMEs during the Ulysses solar maximum northern polar passage D. Reisenfeld, and T. R. Sanderson (2004), Low-energy particle response to CMEs during the Ulysses solar maximum, New Mexico, USA T. R. Sanderson Research and Scientific Support Department of European Space Agency

Sanahuja, Blai

317

E-Print Network 3.0 - area solar neutron Sample Search Results  

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

Printed in the U.S.A. Summary: OF PROTONS AND ELECTRONS FROM THE DECAY OF LOW-ENERGY SOLAR FLARE NEUTRONS Neus Agueda1,2 , Sam Krucker1... decay of low-energy (1-10 MeV) solar...

318

Ten-percent solar-to-fuel conversion with nonprecious materials  

Science Journals Connector (OSTI)

...Mechanical Engineering, Massachusetts Institute of Technology...Mechanical Engineering, Massachusetts Institute of Technology...Cambridge, MA 02139 Direct solar-to-fuels conversion...Information for 10% solar-to-fuel conversion...University, Cambridge, Massachusetts 02138, USA. bMassachusetts...

Casandra R. Cox; Jungwoo Z. Lee; Daniel G. Nocera; Tonio Buonassisi

2014-01-01T23:59:59.000Z

319

Design and global optimization of high-efficiency solar thermal systems  

E-Print Network [OSTI]

, Massachusetts 02139, USA bermel@mit.edu Abstract: Solar thermal, thermoelectric, and thermophotovoltaic (TPVDesign and global optimization of high-efficiency solar thermal systems with tungsten cermets DavidDepartment of Physics, Massachusetts Institute of Technology, 77 Massachusetts Ave., Cambridge, Massachusetts

Soljaèiæ, Marin

320

The radial temperature profile of the solar wind John D. Richardson  

E-Print Network [OSTI]

The radial temperature profile of the solar wind John D. Richardson Center for Space Research, Massachusetts Institute of Technology, Cambridge, Massachusetts, USA Charles W. Smith Bartol Research Institute but do not account for the smaller scale (few AU) temperature variations. At 1 AU, the solar wind

Richardson, John

Note: This page contains sample records for the topic "usa solar fields" 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

Relationship between magnetic power spectrum and flare productivity in solar active regions  

E-Print Network [OSTI]

; Politano et al. 1989) energy spectrum of solar wind plasma is close to k-5/3 . In the MHD case, Alfven.I. Abramenko Big Bear Solar Observatory, 40386 N. Shore Lane, Big Bear City, CA 92314, USA ABSTRACT Power turbulent regime with constant rate of energy transfer along the spectrum is holding. Due to an equilibrium

322

NREL: Innovation Impact - Solar  

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

Solar Energy Menu Home Home Solar Solar Wind Wind Analysis Analysis Bioenergy Bioenergy Buildings Buildings Transportation Transportation Manufacturing Manufacturing Energy Systems...

323

SOLAR MARKET POWERS SILICON  

Science Journals Connector (OSTI)

SOLAR MARKET POWERS SILICON ... Polysilicon shortages are boon to manufacturers, bane of solar energy industry ... Solar energy is a relatively new market for polysilicon manufacturers. ...

JEAN-FRA&CCEDIL;NOIS TREMBLAY

2006-10-02T23:59:59.000Z

324

Solar forecasting review  

E-Print Network [OSTI]

2.1.2 European Solar Radiation Atlas (ESRA)2.4 Evaluation of Solar Forecasting . . . . . . . . .2.4.1 Solar Variability . . . . . . . . . . . . .

Inman, Richard Headen

2012-01-01T23:59:59.000Z

325

Residential Solar Valuation Rates  

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

Residential Solar Valuation Rates Karl R. Rbago Rbago Energy LLC 1 The Ideal Residential Solar Tariff Fair to the utility and non-solar customers Fair compensation to...

326

Solar Deployment and Policy  

Gasoline and Diesel Fuel Update (EIA)

Solar Deployment and Policy Justin Baca Director of Research Solar Energy Industries Association About SEIA * Founded in 1974 * U.S. National Trade Association for Solar Energy *...

327

Sandia National Laboratories: solar  

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

Solar Thermal Testing Facility Beam Profiling On November 2, 2012, in Concentrating Solar Power, News, Renewable Energy, Solar On Thursday, June 7, we began beam profiling...

328

Sandia National Laboratories: solar  

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

heat can also be efficiently and cheaply stored to produce electricity when the sun ... Solar Energy On February 3, 2011, in Solar Programs Photovoltaics Concentrating Solar...

329

Sandia National Laboratories: solar  

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

in Concentrating Solar Power, Customers & Partners, Energy, News, Partnership, Renewable Energy, Solar Areva Solar is collaborating with Sandia National Laboratories on a new...

330

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

cycle air conditioning. Solar assisted heat pumps. Systemsheat source. COP for solar assisted heat pump (heat pumpcycle air conditioners, solar-assisted heat pumps, and some

Berdahl, P.

2010-01-01T23:59:59.000Z

331

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

conditioning. Solar assisted heat pumps. Systems with someheat source. COP for solar assisted heat pump (heat pumpconditioners, solar-assisted heat pumps, and some passive

Berdahl, P.

2010-01-01T23:59:59.000Z

332

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

room )I I( I I ,i I CALIFORNIA SOLAR DATA MANUAL I. ! I ienergy resource. The California Solar Data Manual describestowards fulfilling California's solar data needs is the

Berdahl, P.

2010-01-01T23:59:59.000Z

333

Sandia National Laboratories: Solar  

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

for Download On March 13, 2014, in Energy, News, News & Events, Photovoltaic, Renewable Energy, Solar, Solar Newsletter Sandia developed the Solar Glare Hazard Analysis Tool...

334

Solar powered desalination system  

E-Print Network [OSTI]

As a clean energy source, solar power is inexhaustible,renewables for energy sources, including solar power. Also,Requirements Energy Source Natural Gas Nuclear Solar Wind

Mateo, Tiffany Alisa

2011-01-01T23:59:59.000Z

335

Analysis of field-test data from domestic solar-water heaters in the southern United States, period through September 1982  

SciTech Connect (OSTI)

The monitored performance data used here was gathered from 137 solar water heaters. All but 51 are located in Florida. The gathered data accumulated from weekly mailers consists of the following measurements: total gallons of hot water consumed; total kWh of electricity used; total hours the circulating pump operated; hot and cold water temperatures at the top; number of household members at home since last reading; tank thermostat setting and any changes to it; total number of hours that the tank's backup heating element had power available; and problems or comments concerning system operational status or component reliability and maintenance. The data analysis is described and results are presented. (MHR)

Jones, W.M.; Fenner, M.F.

1983-01-01T23:59:59.000Z

336

Oecologia (Berl.) 44, 159-163 (1980) Oecologia9 by Springer-Verlag 1980 Solar Tracking Response to Drought in a Desert Annual  

E-Print Network [OSTI]

on possible adaptive benefits that might be conferred by solar tracking movements. Two species have beenOecologia (Berl.) 44, 159-163 (1980) Oecologia9 by Springer-Verlag 1980 Solar Tracking Response Lake City, UT, 84112, USA Summary. The responses to drought of the solar tracking winter annual Lupinus

Ehleringer, Jim

337

HELIUM VARIATION IN THE SOLAR WIND John D. Richardson1, Ian G. Richardson2, Justin C. Kasper1, Hilary V. Cane2, Nancy U.  

E-Print Network [OSTI]

, Boston, Massachusetts, USA ABSTRACT Solar wind parameters show strong solar cycle varia- tions in plasma1 HELIUM VARIATION IN THE SOLAR WIND John D. Richardson1, Ian G. Richardson2, Justin C. Kasper1, Hilary V. Cane2, Nancy U. Crooker3, and Alan J. Lazarus1 1Massachusetts Institute of Technology

Richardson, John

338

Solar Electric Light Fund | Open Energy Information  

Open Energy Info (EERE)

Solar Electric Light Fund Solar Electric Light Fund Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Solar Electric Light Fund Agency/Company /Organization: Solar Electric Light Fund Sector: Energy Focus Area: Solar Phase: Create Early Successes Resource Type: Publications, Training materials Website: www.self.org/ Locality: US, Africa, Asia, Latin America Cost: Free The mission of the Solar Electric Light Fund (SELF) is to empower people in developing countries to rise from poverty using energy from the sun. What We Do The Solar Electric Light Fund (SELF) has been working in the field of renewable energy, household energy and decentralized rural electrification for over 18 years. We have a proven track record of managing complex, multi-disciplinary international projects and have worked on renewable

339

DOE Solar Decathlon: 2009 Daily Journals  

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

Richard King next to a deck and planter boxes. Decathlete Way and the U.S. Capitol are in the background. Richard King next to a deck and planter boxes. Decathlete Way and the U.S. Capitol are in the background. Solar Decathlon Director Richard King takes a break from the competition along Decathlete Way. Solar Decathlon 2009 Daily Journals The daily journals highlighted the events of the U.S. Department of Energy Solar Decathlon 2009. Each day, Richard King, Solar Decathlon director, covered the latest on the teams, their standings, and the events going on in the solar village. October 19, 2009 I personally believe one of the greatest discoveries in the field of energy from the 20th century is our ability to generate electricity from sunlight using photovoltaic solar cells. Read more. October 17, 2009 Solar Decathlon 2009 was intriguing and suspenseful to the very end. None

340

French population exposure to 50 Hz magnetic fields : first results in Ile-de-France and Rhne-Alpes regions  

E-Print Network [OSTI]

randomly taken from telephone lists. Each one has worn an EMDEX II (Enertech, USA) recording magnetic field

Paris-Sud XI, Université de

Note: This page contains sample records for the topic "usa solar fields" 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

Plasmonic nanoparticle enhanced photocurrent in GaN/InGaN/GaN quantum well solar cells  

E-Print Network [OSTI]

Plasmonic nanoparticle enhanced photocurrent in GaN/InGaN/GaN quantum well solar cells Imogen M of Applied Physics, California Institute of Technology, Pasadena, California 91125, USA 2 Semiconductor Nanoscience Institute, California Institute of Technology, Pasadena, California 91125, USA Received 26

Atwater, Harry

342

Journal of Atmospheric and Solar-Terrestrial Physics 62 (2000) 15151525 www.elsevier.nl/locate/jastp  

E-Print Network [OSTI]

Journal of Atmospheric and Solar-Terrestrial Physics 62 (2000) 1515­1525 wwwDepartment of Atmospheric, Oceanic and Space Sciences, The University of Michigan, Ann Arbor, MI 48109, USA bDepartment ofAerospace Engineering, The University of Michigan, Ann Arbor, MI 48109, USA cDepartment of Electrical Engineering

Stout, Quentin F.

343

Solar Neutrinos  

DOE R&D Accomplishments [OSTI]

The prospect of studying the solar energy generation process directly by observing the solar neutrino radiation has been discussed for many years. The main difficulty with this approach is that the sun emits predominantly low energy neutrinos, and detectors for observing low fluxes of low energy neutrinos have not been developed. However, experimental techniques have been developed for observing neutrinos, and one can foresee that in the near future these techniques will be improved sufficiently in sensitivity to observe solar neutrinos. At the present several experiments are being designed and hopefully will be operating in the next year or so. We will discuss an experiment based upon a neutrino capture reaction that is the inverse of the electron-capture radioactive decay of argon-37. The method depends upon exposing a large volume of a chlorine compound, removing the radioactive argon-37 and observing the characteristic decay in a small low-level counter.

Davis, R. Jr.; Harmer, D. S.

1964-12-00T23:59:59.000Z

344

President Obama Discusses Solar Power in Nevada | Department of Energy  

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

Discusses Solar Power in Nevada Discusses Solar Power in Nevada President Obama Discusses Solar Power in Nevada March 22, 2012 - 10:26am Addthis President Barack Obama delivers remarks on energy after a tour of a solar panel field at the Copper Mountain Solar 1 Facility, the largest photovoltaic plant operating in the country with nearly one million solar panels powering 17,000 homes, in Boulder City, Nevada, March 21, 2012. | Official White House Photo by Lawrence Jackson. President Barack Obama delivers remarks on energy after a tour of a solar panel field at the Copper Mountain Solar 1 Facility, the largest photovoltaic plant operating in the country with nearly one million solar panels powering 17,000 homes, in Boulder City, Nevada, March 21, 2012. | Official White House Photo by Lawrence Jackson.

345

Solar ADEPT: Efficient Solar Energy Systems  

SciTech Connect (OSTI)

Solar ADEPT Project: The 7 projects that make up ARPA-E's Solar ADEPT program, short for 'Solar Agile Delivery of Electrical Power Technology,' aim to improve the performance of photovoltaic (PV) solar energy systems, which convert the sun's rays into electricity. Solar ADEPT projects are integrating advanced electrical components into PV systems to make the process of converting solar energy to electricity more efficient.

None

2011-01-01T23:59:59.000Z

346

Solar system  

SciTech Connect (OSTI)

An improved solar heat collecting system is described comprising: a collecting means having upper and lower end caps; means for supporting the collecting means in a position generally perpendicular to ambit solar radiation and to permit periodic adjustment thereof; the support means including a base, a first support bar pivotally secured to the base and extending parallel to the ground, and a first support member extending perpendicular from the first support bar to the lower end cap. The support means also includes a second support bar pivotally secured to the base and extending generally parallel to the first support bar, a support leg having a lower portion that extends perpendicularly from the second support bar, an intermediate leg portion slidingly mounted on the lower leg portion and an upper leg portion pivotally secured to the intermediate leg portion, and a second support member extending perpendicularly from the upper leg portion to the upper end cap; lens means disposed above the collecting means for concentrating solar radiation on the collecting means; a pair of reflector means mounted below and on opposite sides of the radiation shadow of the lens means for concentrating solar radiation on the collecting means; mounting means for mounting the lens means and the reflector means. The mounting means includes first and second bracket means rotatively mounted respectively to the first and second support members. A pair of radially extending U-shaped reflector mounts have opposite ends secured to respective bracket means, and a pair of radially extending lens supports secured to respective bracket means; and means for rotating the mounting means and associated lens mean and reflector means to track the source of solar radiation whereby an improved, highly efficient solar heat collecting system is provided.

Gregory, S.T.

1987-02-24T23:59:59.000Z

347

Calorimetry and solar energy  

Science Journals Connector (OSTI)

Calorimetry and solar energy ... An experiment is described that helps students relate concepts of calorimetry to solar energy. ...

R. B. Shiflett

1978-01-01T23:59:59.000Z

348

Solar Energy Technologies Program: Solar Multimedia  

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

Energy Efficiency and Renewable Energy Energy Efficiency and Renewable Energy EERE Home Programs & Offices Consumer Information Solar Multimedia search Home EERE » SunShot Initiative » Solar Multimedia Printable Version Bookmark and Share Feature Photo of 3 solar dishes, which have reflective, square-shaped material that creates a mirror image of the sky and clouds. Each dish is anchored to the ground by a vertical pole. Solar Dish - Albuquerque, New Mexico Credit: Sandia National Laboratories/Randy Montoya Solar Technologies Photovoltaics Photovoltaics Concentrating Solar Power Concentrating Solar Power Solar Applications Residential Residential Commercial Commercial Large Installations Large Installations City and County City and County Federal Federal Manufacturing Manufacturing Development and Testing

349

Excitonic Solar Cells  

Science Journals Connector (OSTI)

Excitonic Solar Cells ... Existing types of solar cells may be divided into two distinct classes:? conventional solar cells, such as silicon p?n junctions, and excitonic solar cells, XSCs. ... Most organic-based solar cells, including dye-sensitized solar cells, DSSCs, fall into the category of XSCs. ...

Brian A. Gregg

2003-05-01T23:59:59.000Z

350

CUTTING SOLAR RED TAPECUTTING SOLAR RED TAPE Evergreen State Solar PartnershipEvergreen State Solar Partnership  

E-Print Network [OSTI]

CUTTING SOLAR RED TAPECUTTING SOLAR RED TAPE Evergreen State Solar PartnershipEvergreen State Solar Partnership Rooftop Solar Challenge 1 Sunshot #12;WASHINGTON PV CONTEXTWASHINGTON PV CONTEXT 285 cities, 39 Installations happen where process is easier #12;EVERGREEN STATE SOLAR PARTNERSHIP Commerce NWSEEDEdmonds

351

Reply to 'Influence of cosmic ray variability on the monsoon rainfall and temperature': a false-positive in the field of solar-terrestrial research  

E-Print Network [OSTI]

A litany of research has been published claiming strong solar influences on the Earth's weather and climate. Much of this work includes documented errors and false-positives, yet is still frequently used to substantiate arguments of global warming denial. This manuscript reports on a recent study by Badruddin & Aslam (2014), hereafter BA14, which claimed a highly significant ($p=1.4\\times10^{-5}$) relationship between extremes in the intensity of the Indian monsoon and the cosmic ray flux. They further speculated that the relationship they observed may apply across the entire tropical and sub-tropical belt, and be of global importance. However, their statistical analysis---and consequently their conclusions---were wrong. Specifically, their error resulted from an assumption that their data's underlying distribution was Gaussian. But, as demonstrated in this work, their data closely follow an ergodic chaotic distribution biased towards extreme values. From a probability density function, calculated using a...

Laken, Benjamin A

2015-01-01T23:59:59.000Z

352

Worldwide Energy and Manufacturing USA Inc formerly Worldwide Manufacturing  

Open Energy Info (EERE)

Manufacturing USA Inc formerly Worldwide Manufacturing Manufacturing USA Inc formerly Worldwide Manufacturing USA Jump to: navigation, search Name Worldwide Energy and Manufacturing USA Inc (formerly Worldwide Manufacturing USA) Place San Bruno, California Zip 94066 Product Worldwide Manufacturing USA is an engineering company based in San Bruno, California. References Worldwide Energy and Manufacturing USA Inc (formerly Worldwide Manufacturing USA)[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Worldwide Energy and Manufacturing USA Inc (formerly Worldwide Manufacturing USA) is a company located in San Bruno, California . References ↑ "Worldwide Energy and Manufacturing USA Inc (formerly Worldwide Manufacturing USA)"

353

Late Cretaceous chimaeroids (Chondrichthyes: Holocephali) from Alabama, USA  

E-Print Network [OSTI]

Holocephali) from Alabama, USA. Paleo- Bios 31(2). ucmp_Williston Basin, North Dakota, USA. Palaeontology 48:709Holocephali) from Alabama, USA DAVID J. CICIMURRI 1 * and

Cicimurri, David J.; Ebersole, Jun A.

2014-01-01T23:59:59.000Z

354

September 6th , 2008, Kimmel Center, New York, USA.  

E-Print Network [OSTI]

MFCA'08 September 6th , 2008, Kimmel Center, New York, USA. http of Utah, USA) Mathematical Foundations of Computational Anatomy Geometrical and Statistical Methods, University of Utah, USA) Program Committee Rachid Deriche (INRIA, France) Ian L. Dryden (University

Paris-Sud XI, Université de

355

Designing Sustainability at BMW Group: The Designworks/USA Experience  

E-Print Network [OSTI]

Table 1. The Designworks/USA creative process Element 1.will be disseminated to many of Designworks/USAs clients.acknowledge those Designworks/USA employees who provided

McElhaney, Kellie A; Toffel, Michael W.; Hill, Natalie

2002-01-01T23:59:59.000Z

356

Relationship between Solar Wind and Coronal Heating: Scaling Laws from Solar X-Rays  

Science Journals Connector (OSTI)

Pevtsov et al. recently showed that the luminosity of solar and stellar X-rays from closed magnetic structures scales nearly linearly with magnetic flux over 12 decades. We show here that the total power available to accelerate the solar wind also scales linearly with magnetic flux, provided that its sources inject a roughly constant energy per particle prior to losses from heat conducted by electrons into radiation. Using a recently developed model of the solar wind energy source and particle source, we calculate the available solar wind power and convert it into an equivalent X-ray luminosity to explore whether the same process that drives solar wind may also power coronal heating. The quantitative results agree remarkably well with the Pevtsov et al. X-ray observations and with GOES X-ray observations over almost two solar cycles from 1985 to 2004. The model for the solar wind energy and particle source relies on the continual reconfiguration of the supergranular network through the emergence of small bipolar or more complex closed magnetic fields. This naturally leads to an energy flux proportional to field strength on large-scale field structures with field strengths larger than the emerging flux. We conclude that the sources of energy for the solar wind and coronal heating are linked, likely through the emergence of new magnetic flux that continually reconfigures large-scale solar magnetic fields and powers and heats the corona.

N. A. Schwadron; D. J. McComas; C. DeForest

2006-01-01T23:59:59.000Z

357

The Astrophysical Journal, 707:15331540, 2009 December 20 doi:10.1088/0004-637X/707/2/1533 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

. The American Astronomical Society. All rights reserved. Printed in the U.S.A. EVOLUTION OF THE BINARY FRACTION that the hard binary fraction in the core tends to increase with time over a range of initial cluster central dynamics is unimportant, such as the solar neighbor- hood, yield a binary fraction of 50% among solar

Rasio, Frederic A.

358

The Astrophysical Journal, 770:42 (15pp), 2013 June 10 doi:10.1088/0004-637X/770/1/42 C 2013. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

of their central stars. The physical regime of hot Jupiters differs substantially from those of solar-system gi. The American Astronomical Society. All rights reserved. Printed in the U.S.A. ATMOSPHERIC CIRCULATION OF HOT solar system. These differences have motivated a flourishing research program focused on elucidating

359

Solar Energy  

Science Journals Connector (OSTI)

...Arizona) noted results achieved with the Puerto Penasco Solar Desalination Plant, Sonora, Mexico. This plant, operated in cooperation...State Univ., Jniversity Park) 22-25. American Home Economics As-oc., 56th annual, Atlantic City, N.J. (Mrs...

Peter E. Glaser

1965-05-21T23:59:59.000Z

360

SOLAR ENERGY FOR ACADEMIC INSTITUTIONS Solar Suitability Assessment  

E-Print Network [OSTI]

SOLAR ENERGY FOR ACADEMIC INSTITUTIONS Solar Suitability Assessment of Dalhousie University.................................................................................................. 2 2.2 Solar Radiation Data for Calculating Solar Energy Resource .................... 3 3 Campus.1 Evaluation of Suitability for Solar Energy Generation................................ 12 4.2 Solar

Brownstone, Rob

Note: This page contains sample records for the topic "usa solar fields" 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

Towards a model for the solar dynamo  

Science Journals Connector (OSTI)

......to give a plausible butterfly diagram. For small Prandtl numbers...solar dynamo. magnetic fields|MHD|Sun: activity|Sun: magnetic...exhibit the well-known butterfly diagram- i.e. the main region of...simultaneously a realistic butterfly diagram and an approximately solar rotation......

David Moss; John Brooke

2000-07-01T23:59:59.000Z

362

Prospects for the use of amorphous semiconductors in solar energy conversion  

Science Journals Connector (OSTI)

... this article, we review some potential applications of amorphous Si in the field of solar energy ...energyconversion ...

J. I. B. Wilson; D. Weaire

1978-09-14T23:59:59.000Z

363

USA Science and Engineering Festival: Inspiring and Educating...  

Energy Savers [EERE]

USA Science and Engineering Festival: Inspiring and Educating the Clean Energy Workforce of Tomorrow USA Science and Engineering Festival: Inspiring and Educating the Clean Energy...

364

MOU signed between CIAE and Jefferson National Lab, USA. (China...  

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

https:www.jlab.orgnewsarticlesmou-signed-between-ciae-and-jefferson-national-lab-usa-china-nuclear-industry-news-ge... MOU signed between CIAE and Jefferson National Lab, USA....

365

Results from the investigations on leaking electricity in the USA  

E-Print Network [OSTI]

on leaking electricity in the USA Alan Meier, Wolfgang Huber120 million VCRs in the USA. Data were collected for 69

Meier, Alan; Huber, Wolfgang

1997-01-01T23:59:59.000Z

366

NEUTRAL BEAM INJECTOR RESEARCH AND DEVELOPMENT WORK IN THE USA  

E-Print Network [OSTI]

AND DEVELOPMENT WORK IN THE USA A* S R. V. Pyle, ' W. R.AND DEVELOPMENT WORK IN THE USA* -I- LBL ' R. V. Pyle, W. R.

Pyle, R.V.

2011-01-01T23:59:59.000Z

367

Central solar energy receiver  

DOE Patents [OSTI]

An improved tower-mounted central solar energy receiver for heating air drawn through the receiver by an induced draft fan. A number of vertically oriented, energy absorbing, fin-shaped slats are radially arranged in a number of concentric cylindrical arrays on top of the tower coaxially surrounding a pipe having air holes through which the fan draws air which is heated by the slats which receive the solar radiation from a heliostat field. A number of vertically oriented and wedge-shaped columns are radially arranged in a number of concentric cylindrical clusters surrounding the slat arrays. The columns have two mirror-reflecting sides to reflect radiation into the slat arrays and one energy absorbing side to reduce reradiation and reflection from the slat arrays.

Drost, M. Kevin (Richland, WA)

1983-01-01T23:59:59.000Z

368

Solar electric systems  

SciTech Connect (OSTI)

Electricity from solar sources is the subject. The state-of-the-art of photovoltaics, wind energy and solar thermal electric systems is presented and also a broad range of solar energy activities throughout the Arab world is covered. Contents, abridged: Solar radiation fundamentals. Basic theory solar cells. Solar thermal power plants. Solar energy activities at the scientific research council in Iraq. Solar energy program at Kuwait Institute for Scientific Research. Prospects of solar energy for Egypt. Non-conventional energy in Syria. Wind and solar energies in Sudan. Index.

Warfield, G.

1984-01-01T23:59:59.000Z

369

San Diego, California: Solar in Action (Brochure), Solar America...  

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

San Diego, California: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) San Diego, California: Solar in Action (Brochure), Solar...

370

Milwaukee, Wisconsin: Solar in Action (Brochure), Solar America...  

Energy Savers [EERE]

Milwaukee, Wisconsin: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Milwaukee, Wisconsin: Solar in Action (Brochure), Solar America...

371

Denver, Colorado: Solar in Action (Brochure), Solar America Cities...  

Energy Savers [EERE]

Denver, Colorado: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Denver, Colorado: Solar in Action (Brochure), Solar America Cities,...

372

Berkeley, California: Solar in Action (Brochure), Solar America...  

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

Berkeley, California: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Berkeley, California: Solar in Action (Brochure), Solar America...

373

Concentrating Solar Power Facilities and Solar Potential | Department...  

Office of Environmental Management (EM)

Facilities and Solar Potential Concentrating Solar Power Facilities and Solar Potential Concentrating Solar Power Facilities and CSP Energy Potential Gradient Click icons to filter...

374

China Glass Solar aka CG Solar formerly Weihai Bluestar Terra...  

Open Energy Info (EERE)

Solar aka CG Solar formerly Weihai Bluestar Terra Photovoltaic Co Ltd Jump to: navigation, search Name: China Glass Solar (aka CG Solar, formerly Weihai Bluestar Terra Photovoltaic...

375

Tucson, Arizona: Solar in Action (Brochure), Solar America Cities...  

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

Tucson, Arizona: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Tucson, Arizona: Solar in Action (Brochure), Solar America Cities,...

376

Austin, Texas: Solar in Action (Brochure), Solar America Cities...  

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

Austin, Texas: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Austin, Texas: Solar in Action (Brochure), Solar America Cities, Energy...

377

Pittsburgh, Pennsylvania: Solar in Action (Brochure), Solar America...  

Energy Savers [EERE]

Pittsburgh, Pennsylvania: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Pittsburgh, Pennsylvania: Solar in Action (Brochure), Solar...

378

Seattle, Washington: Solar in Action (Brochure), Solar America...  

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

Seattle, Washington: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Seattle, Washington: Solar in Action (Brochure), Solar America...

379

Knoxville, Tennessee: Solar in Action (Brochure), Solar America...  

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

Knoxville, Tennessee: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Knoxville, Tennessee: Solar in Action (Brochure), Solar America...

380

Boston Massachusetts: Solar in Action (Brochure), Solar America...  

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

Boston Massachusetts: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) Boston Massachusetts: Solar in Action (Brochure), Solar America...

Note: This page contains sample records for the topic "usa solar fields" 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

Passive Solar Building Design and Solar Thermal Space Heating...  

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

Passive Solar Building Design and Solar Thermal Space Heating Webinar Passive Solar Building Design and Solar Thermal Space Heating Webinar Watch a recording of National Renewable...

382

San Antonio, Texas: Solar in Action (Brochure), Solar America...  

Energy Savers [EERE]

San Antonio, Texas: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) San Antonio, Texas: Solar in Action (Brochure), Solar America...

383

Petrovay: Solar physics Helioseismology SOLAR OSCILLATIONS: INTRODUCTION  

E-Print Network [OSTI]

: Solar oscillations first observed by both Doppler and intensity method (Leighton, Noyes & Simon 1962: ApPetrovay: Solar physics Helioseismology SOLAR OSCILLATIONS: INTRODUCTION Small departures from hydrostatic equilibrium caused by ­ turbulent convection ­ localized events related to solar activity (e

Petrovay, Kristóf

384

Solar Impulse's Solar-Powered Plane  

SciTech Connect (OSTI)

Solar Impulse lands in Washington, DC at Washington Dulles International Airport as part of its journey across the United States. Secretary Ernest Moniz speaks about how advancements like those at the Department of Energy are leading the way for innovations like the solar-powered plane. Footage of the solar-powered plane courtesy of Solar Impulse.

Moniz, Ernest; Piccard, Bertrand; Reicher, Dan

2013-07-08T23:59:59.000Z

385

Solar Impulse's Solar-Powered Plane  

ScienceCinema (OSTI)

Solar Impulse lands in Washington, DC at Washington Dulles International Airport as part of its journey across the United States. Secretary Ernest Moniz speaks about how advancements like those at the Department of Energy are leading the way for innovations like the solar-powered plane. Footage of the solar-powered plane courtesy of Solar Impulse.

Moniz, Ernest; Piccard, Bertrand; Reicher, Dan

2014-01-07T23:59:59.000Z

386

Solar Neutrinos and Solar Oscillations  

Science Journals Connector (OSTI)

...solar core, it is not out of the question that they induce motion that influences substantially the rates of the various thermonuclear reactions that emit the neutrinos. The basic processes of seismic inference will be discussed briefly, followed by a summary...

1994-01-01T23:59:59.000Z

387

Solar Lakes and Solar Energy  

Science Journals Connector (OSTI)

... It is worth estimating the magnitude of the energy that can be extracted from the stable layer of such a lake. Por presented ... the depth of 125 cm as the top of that layer. Now the fraction of solar radiation which penetrates unabsorbed below a water layer 125 cm thick2 is about 30 per ...

J. NEUMANN

1968-08-24T23:59:59.000Z

388

Solar Kit Lessons  

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

Solar Kit Lessons Middle School Curriculum Created by Northeast Sustainable Energy Association (NESEA) Click on the links below to take you to the Chapter heading: Solar Cell Inquiry Sunshine Timer Parts of a Solar Panel Part 1 Parts of a Solar Panel Part 2 Build a Simple Ammeter Solar-Powered Battery Charger Positioning Solar Panels 1 Positioning Solar Panels 2 Properties of Solar Radiation: Reflection, Transmission, and Absorption Properties of Solar Radiation: Direct and Diffuse Light Power Maximum: An Electrical Determination Calibration Curve for a Radiation Meter Solarize a Toy Solar Cells as Control Devices Solar-Powered Electrolysis of Water and the Hydrogen Economy Solar Kit Lesson #1 Solar Cell Inquiry TEACHER INFORMATION LEARNING OUTCOME

389

Bisfuel links - Solar energy news  

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

Solar energy news ASU Lightworks ScienceDaily: Solar Energy News Solar Power From Renewable Energy World...

390

2008 Solar Technologies Market Report  

E-Print Network [OSTI]

Extending Federal Solar Tax Credits. Prepared for the Solar2008). The Solar Investment Tax Credit Frequently Askedtax credit .

Price, S.

2010-01-01T23:59:59.000Z

391

Performance of Civil Aviation Receivers during Maximum Solar Activity Events  

E-Print Network [OSTI]

Performance of Civil Aviation Receivers during Maximum Solar Activity Events Lina DEAMBROGIO on the fields of ionosphere scintillations, solar energetic particles and on the implementation of operational the upcoming period of high solar activity. Emilien ROBERT got his PhD in 2005 and started to work on behalf

Boyer, Edmond

392

Proton corebeam system in the expanding solar wind: Hybrid simulations  

E-Print Network [OSTI]

Proton corebeam system in the expanding solar wind: Hybrid simulations Petr Hellinger1,2 and Pavel. Trávnícek (2011), Proton corebeam system in the expanding solar wind: Hybrid simulations, J. Geophys. Res beamcore system in the solar wind are presented. The expansion with a strictly radial magnetic field leads

California at Berkeley, University of

393

Alfv'en Wave Solitons and Solar Intermediate Drift Bursts  

E-Print Network [OSTI]

propagate at velocities of the order of the Alfv'en velocity in a direction inclined to the magnetic field to be magnetized, as e.g. the solar atmosphere, the solar and stellar coronae, the solar wind, accretion disks'en speed v A , a fundamental plasma parameter depending on the gas and the magnetic pressures. It has been

Guedel, Manuel

394

Deceleration of Alpha Particles in the Solar Wind by Instabilities and the Rotational Force: Implications for Heating, Azimuthal Flow, and the Parker Spiral Magnetic Field  

E-Print Network [OSTI]

Protons and alpha particles in the fast solar wind are only weakly collisional and exhibit a number of non-equilibrium features, including relative drifts between particle species. Two non-collisional mechanisms have been proposed for limiting differential flow between alpha particles and protons: plasma instabilities and the rotational force. Both mechanisms decelerate the alpha particles. In this paper, we derive an analytic expression for the rate $Q_{\\mathrm{flow}}$ at which energy is released by alpha-particle deceleration, accounting for azimuthal flow and conservation of total momentum. We find that $Q_{\\mathrm{flow}} > 0 $ at $r r_{\\mathrm{crit}}$. We compare the value of $Q_{\\mathrm{flow}}$ at $r< r_{\\mathrm{crit}}$ with empirical heating rates for protons and alpha particles, denoted $Q_{\\mathrm{p}}$ and $Q_{\\alpha}$, deduced from in-situ measurements of fast-wind streams from the Helios and Ulysses spacecraft. We find that $Q_{\\mathrm{flow}}$ exceeds $Q_{\\alpha}$ at $r < 1\\,\\mathrm{AU}$, $Q_{...

Verscharen, Daniel; Bourouaine, Sofiane; Hollweg, Joseph V

2014-01-01T23:59:59.000Z

395

NREL: Concentrating Solar Power Research - News  

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

News News Below are news stories related to NREL Concentrating Solar Power research. Subscribe to the RSS feed RSS . Learn about RSS. November 5, 2013 Solar Working Group Releases Standard Contracts A working group representing solar industry stakeholders has developed standard contracts that should help lower transaction costs and make it easier to access low-cost financing for residential and commercial solar power projects. October 24, 2013 NREL Researcher Honored with Hispanic STEM Award A national organization devoted to getting more Hispanics into the fields of science, technology, engineering, and math (STEM), has honored a scientist at the Energy Department's National Renewable Energy Laboratory (NREL) with its annual Outstanding Technical Achievement Award.

396

High Field Magnet R&D in the USA  

E-Print Network [OSTI]

aI. , "Status of High Temperature Superconductor Magnet R&Dmention High Temperature Superconductor (I-ITS). Though

Gourlay, S.A.

2011-01-01T23:59:59.000Z

397

NPP Grassland: Dickinson, U.S.A.  

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

Dickinson, U.S.A., 1970 Dickinson, U.S.A., 1970 [PHOTOGRAPH] Photograph: Washing root samples at the Dickinson site (click on the photo to view a series of images from this site). Data Citation Cite this data set as follows: Whitman, W., and W. K. Lauenroth. 1998. NPP Grassland: Dickinson, U.S.A., 1970. Data set. Available on-line [http://www.daac.ornl.gov] from Oak Ridge National Laboratory Distributed Active Archive Center, Oak Ridge, Tennessee, U.S.A. Description Productivity of a northern mixed prairie grassland was monitored at the Dickinson study site during 1970. Dynamics of above-ground plant biomass were monitored at roughly 2-week intervals during the growing season. Data on above-ground live biomass, standing dead matter and litter are available, for two replications of a grazed and an "ungrazed" (relatively

398

H2USA | Department of Energy  

Energy Savers [EERE]

similar to the public-private partnerships in other countries focused on hydrogen, particularly Germany, Japan, and the UK. H2USA currently consists of more than 30 participants....

399

Solar Neutrinos  

E-Print Network [OSTI]

Experimental work with solar neutrinos has illuminated the properties of neutrinos and tested models of how the sun produces its energy. Three experiments continue to take data, and at least seven are in various stages of planning or construction. In this review, the current experimental status is summarized, and future directions explored with a focus on the effects of a non-zero theta-13 and the interesting possibility of directly testing the luminosity constraint. Such a confrontation at the few-percent level would provide a prediction of the solar irradiance tens of thousands of years in the future for comparison with the present-day irradiance. A model-independent analysis of existing low-energy data shows good agreement between the neutrino and electromagnetic luminosities at the +/- 20 % level.

R. G. H. Robertson

2006-02-05T23:59:59.000Z

400

Declination Solar | Open Energy Information  

Open Energy Info (EERE)

Declination Solar Jump to: navigation, search Name: Declination Solar Place: San Francisco, California Sector: Solar Product: San Francisco solar installation firm acquired by...

Note: This page contains sample records for the topic "usa solar fields" 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

Aztec Solar | Open Energy Information  

Open Energy Info (EERE)

Solar Jump to: navigation, search Name: Aztec Solar Place: Rancho Cordova, California Zip: 95742 Sector: Solar Product: Installer of solar hot water and pool heating systems....

402

Solar Energy | Department of Energy  

Office of Environmental Management (EM)

Solar Energy Solar Energy Below are resources for Tribes on solar energy technologies. A Guide to Community Solar: Utility, Private, and Nonprofit Project Development A resource...

403

Solar2 | Open Energy Information  

Open Energy Info (EERE)

Solar2 Jump to: navigation, search Name: Solar2 Place: Cuxhaven, Germany Zip: 27472 Sector: Solar Product: Sells and installs PV, solar thermal and wood pellet powered heating...

404

Solar Wind | Open Energy Information  

Open Energy Info (EERE)

Place: Krasnodar, Romania Zip: 350000 Sector: Solar, Wind energy Product: Russia-based PV product manufacturer. Solar Wind manufactures solar modules and cells. References: Solar...

405

Apex Solar | Open Energy Information  

Open Energy Info (EERE)

Name: Apex Solar Place: Sofia, Bulgaria Zip: 1616 Sector: Solar Product: Bulgarian PV and solar thermal project developer and installer. References: Apex Solar1 This article is a...

406

Khmer Solar | Open Energy Information  

Open Energy Info (EERE)

Khmer Solar Jump to: navigation, search Name: Khmer Solar Place: Phnom Penh, Cambodia Sector: Solar, Wind energy Product: Specializes in solar and wind systems for off-grid...

407

Solar collector  

SciTech Connect (OSTI)

The disclosure is a solar collector consisting of glass rods enclosed in a housing and mounted vertically on a roof or other elevated place to gather solar rays. The collector is fixed, with no tracking device or other moving parts. The glass rods are 6 mm or smaller in diameter, and there can be several thousand, depending on the sizes of the rods and collector. The upper ends of the rods are inclined at an angle of thirty degrees from horizontal, with the inclined surfaces occupying a plane which faces south so as to obtain maximum exposure to the winter sun. Solar rays striking the inclined ends of the rods are refracted into the rods. The rays travel down through the rods, with a predominantly parallel path of propagation being established by repeated reflections off the inside walls of the rods. The rays are emitted from the lower perpendicular ends of the rods as parallel rays of incoherent light which are directed into beam concentrators.

Clegg, J.E.

1985-01-08T23:59:59.000Z

408

Sandia National Laboratories: Concentrating Solar Power  

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

Concentrating Solar Power Solar Energy On February 3, 2011, in Solar Programs Photovoltaics Concentrating Solar Power Sunshine to Petrol Solar Publications Recent Solar Highlights...

409

Observation of the Decay Dynamics and Instabilities of Megagauss Field Structures in Laser-Produced Plasmas  

E-Print Network [OSTI]

Center, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA R. P. J. Town, P. A, be it a simple oscillator, spin-polarized [1] matter, or a solar flare [2]. Here we report, for the first time

410

arXiv:1203.3907v1[astro-ph.SR]17Mar2012 Solar Physics  

E-Print Network [OSTI]

energy in the attendant seismic emission, suggesting that Lorentz forces can contribute significantly Associates, CORA Division, Boulder, CO USA; email: clindsey@cora.nwra.com SOLA: SP_Alvarado_et_al_2011.tex, driven by solar flares. Sunquakes carry energy and momentum into the solar photosphere and interior from

California at Berkeley, University of

411

Light-Beam-Induced-Current Characterization of CdTe Solar Cells Russell M. Geisthardt and James R. Sites  

E-Print Network [OSTI]

Light-Beam-Induced-Current Characterization of CdTe Solar Cells Russell M. Geisthardt and James RTe solar cells. II. EXPERIMENTAL The LBIC system at CSU has been described in [1] and [2]. The light. Sites Colorado State University, Fort Collins, CO, 80523, USA Abstract--In this work, light

Sites, James R.

412

Did geomagnetic activity challenge electric power reliability during solar cycle 23? Evidence from the PJM regional transmission  

E-Print Network [OSTI]

Did geomagnetic activity challenge electric power reliability during solar cycle 23? Evidence from of America, Washington, DC, 20064 USA Chris.StCyr@nasa.gov #12;Abstract During Solar Cycle 22, a very intense geomagnetic storm on 13 March 1989 contributed to the collapse of the Hydro-Quebec power system in Canada

Schrijver, Karel

413

Petascale Simulations of Inhomogeneous Alfven Turbulence in the Solar Wind  

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

A snapshot of turbulent magnetic field lines (red) inside a coronal hole that expands from a small patch on the solar surface to 5 solar radii A snapshot of turbulent magnetic field lines (red) inside a coronal hole that expands from a small patch on the solar surface to 5 solar radii A snapshot of turbulent magnetic field lines (red) inside a coronal hole that expands from a small patch on the solar surface to 5 solar radii. Alfven waves (AW), launched by convective motions on the photosphere, propagate in the inhomogeneous Solar atmosphere producing primary reflected waves that interact non-linearly with the outward waves, driving a turbulent cascade. This cascade continues with secondary reflections in a very complex interplay between wave reflections and nonlinear interactions. Selected slices across the simulation domain show contours of plasma current, indicating the generation of small scale structures where the

414

Development of an analytical method and its quick algorithm to calculate the solar energy collected by a heliostat field in a year  

Science Journals Connector (OSTI)

Abstract In this paper, we firstly propose an analytical equation to calculate the energy collected by the heliostat field. A ray tracing method is developed based on the analytical equation. Then we introduce three approximations to reduce computation spending, and estimate the errors caused by these approximations. A fast and accurate algorithm is developed with the three approximations to calculate the energy collected by the heliostat field over a year. It was compared with the ray tracing results, which shows good consistency with them. With the method, the energy collected and efficiency of each heliostat in a year can be computed exactly and rapidly, the difference between the method and ray tracing method is less than 0.1% for the energy collected by a heliostat over a day. It needs only about 0.1% computation time used by ray tracing method to calculate the intercept factor of a heliostat at a moment, and 2.67h to compute the annual collected energy of PS10 heliostat field by using one CPU of i3 processor when the time span for integration is 5min and each heliostat is calculated.

Weidong Huang; Qian Xu

2014-01-01T23:59:59.000Z

415

Breakthrough Cutting Technology Promises to Reduce Solar Costs | Department  

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

Breakthrough Cutting Technology Promises to Reduce Solar Costs Breakthrough Cutting Technology Promises to Reduce Solar Costs Breakthrough Cutting Technology Promises to Reduce Solar Costs March 1, 2010 - 4:34am Addthis Using SiGen's new cutting process, less material is wasted in creating solar products like this, a breakthrough that is expected to help make solar power more affordable. | Photo courtesy SiGen Using SiGen's new cutting process, less material is wasted in creating solar products like this, a breakthrough that is expected to help make solar power more affordable. | Photo courtesy SiGen Joshua DeLung Silicon Genesis is a San Jose, Calif., company that is advancing the field of solar energy by developing a process that will virtually eliminate all waste when cutting materials needed to implement solar technology.

416

Solar Innovator | Alta Devices  

SciTech Connect (OSTI)

Selected to participate in the Energy Department's SunShot Initiative, Alta Devices produces solar cells that convert sunlight into electricity at world record-breaking levels of efficiency. Through its innovative solar technology Alta is helping bring down the cost of solar. Learn more about the Energy Department's efforts to advance solar technology at energy.gov/solar .

Mattos, Laila; Le, Minh

2012-01-01T23:59:59.000Z

417

Journal ofAtmospheric and Solar-Terrertrrol Physrcr, Vol. 60, No. 3. pp. 349-357, 1998 SC 1998 Elsevier Scmce Ltd  

E-Print Network [OSTI]

Pergamon Journal ofAtmospheric and Solar-Terrertrrol Physrcr, Vol. 60, No. 3. pp. 349-357, 1998 SC, Massachusetts Institute of Technology, Room 54-1823, Cambridge, Massachusetts 02139, U.S.A. serve

Cho, John Y. N.

418

Solar neutrinos and the solar composition problem  

E-Print Network [OSTI]

Standard solar models (SSM) are facing nowadays a new puzzle: the solar composition problem. New determinations of solar metal abundances lead SSM calculations to conflict with helioseismological measurements, showing discrepancies that extend from the convection zone to the solar core and can not be easily assigned to deficiencies in the modelling of the solar convection zone. We present updated solar neutrino fluxes and uncertainties for two SSM with high (old) and low (new) solar metallicity determinations. The uncertainties in iron and carbon abundances are the largest contribution to the uncertainties of the solar neutrino fluxes. The uncertainty on the ^14N+p -> ^15O+g rate is the largest of the non-composition uncertainties to the CNO neutrino fluxes. We propose an independent method to help identify which SSM is the correct one. Present neutrino data can not distinguish the solar neutrino predictions of both models but ongoing measurements can help to solve the puzzle.

Carlos Pena-Garay; Aldo Serenelli

2008-11-16T23:59:59.000Z

419

Alternative Fuels Data Center: Clean School Bus USA  

Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

School Bus USA School Bus USA to someone by E-mail Share Alternative Fuels Data Center: Clean School Bus USA on Facebook Tweet about Alternative Fuels Data Center: Clean School Bus USA on Twitter Bookmark Alternative Fuels Data Center: Clean School Bus USA on Google Bookmark Alternative Fuels Data Center: Clean School Bus USA on Delicious Rank Alternative Fuels Data Center: Clean School Bus USA on Digg Find More places to share Alternative Fuels Data Center: Clean School Bus USA on AddThis.com... More in this section... Federal State Advanced Search All Laws & Incentives Sorted by Type Clean School Bus USA Clean School Bus USA is a public-private partnership that focuses on reducing children's exposure to harmful diesel exhaust by limiting school bus idling, implementing pollution reduction technologies, improving route

420

Solar Concentration in Space  

Science Journals Connector (OSTI)

Solar concentrators go space. Lens and mirror-based solar concentrators have recently begun to boost photovoltaic power supplies for satellites in space. In 1998, the first mission carrying solar concentrators...

Dr. Ralf Leutz; Dr. Akio Suzuki

2001-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "usa solar fields" 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

Solar Energy Entrepreneurs  

E-Print Network [OSTI]

Solar Energy Entrepreneurs Meeting MD, DC, DE, VA Region May 31, 2012 #12;Solar Energy Entrepreneurs Meeting MD, DC, DE, VA Region Meeting Objectives should attend if you.... · ... work in the solar energy market

Rubloff, Gary W.

422

Solar Heating Contractor Licensing  

Broader source: Energy.gov [DOE]

Michigan offers a solar heating contractor specialty license to individuals who have at least three years of experience installing solar equipment under the direction of a licensed solar contractor...

423

Solar forecasting review  

E-Print Network [OSTI]

to solar thermal power pants energy production planning,to solar ther- mal power plants energy production planning [solar resource, seasonal deviations in production and load profiles, the high cost of energy

Inman, Richard Headen

2012-01-01T23:59:59.000Z

424

Nanocrystal Solar Cells  

E-Print Network [OSTI]

Nov, 2005). Chapter 4 Hybrid solar cells with 3-dimensional5 All-inorganic nanocrystal solar cells 5.1 Introduction Inoperation of organic based solar cells and distinguish them

Gur, Ilan

2006-01-01T23:59:59.000Z

425

Nanocrystal Solar Cells  

E-Print Network [OSTI]

inorganic nanocrystal solar cells 5.1 Introduction In recentoperation of organic based solar cells and distinguish themThe organic donor-acceptor solar cell relies on a type II

Gur, Ilan

2006-01-01T23:59:59.000Z

426

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

and William A. Beckman, Solar Energy Thermal Processes (JohnWiley, Inc" New York. Solar Energy Thermal Processes. John1977): SOLCOST, Solar Energy Design Program for Non-Thermal

Berdahl, P.

2010-01-01T23:59:59.000Z

427

Solar forecasting review  

E-Print Network [OSTI]

P(t) and the boring solar sensor. Denoting the bulk veloci equipped with solar irradiance sensors, see Figure 10.3.f that utilizes the low solar cost sensor network deployment

Inman, Richard Headen

2012-01-01T23:59:59.000Z

428

Solar Thermal Processes  

Science Journals Connector (OSTI)

The use of solar energy for desalination purposes was one of ... The process is based on the use of solar thermal energy to evaporate water, thus separating pure ... brine. In this chapter an overview of solar thermal

M.T. Chaibi; Ali M. El-Nashar

2009-01-01T23:59:59.000Z

429

Energy-based Control of a Distributed Solar Collector Tor A. Johansena  

E-Print Network [OSTI]

Energy-based Control of a Distributed Solar Collector Field Tor A. Johansena Camilla Storaaa that the primary energy source, solar radiation, cannot be manipulated. The distributed solar collector eld may, Norway. Model-based control of the outlet temperature of a distributed solar col- lector eld is studied

Johansen, Tor Arne

430

Solar Phys (2009) 256: 345363 DOI 10.1007/s11207-009-9345-6  

E-Print Network [OSTI]

Solar Phys (2009) 256: 345­363 DOI 10.1007/s11207-009-9345-6 STEREO SCIENCE RESULTS AT SOLAR MINIMUM Effects of the Weak Polar Fields of Solar Cycle 23: Investigation Using OMNI for the STEREO(s) 2009. This article is published with open access at Springerlink.com Abstract The current solar cycle

California at Berkeley, University of

431

Solar cycle changes in coronal holes and space weather cycles J. G. Luhmann,1  

E-Print Network [OSTI]

Solar cycle changes in coronal holes and space weather cycles J. G. Luhmann,1 Y. Li,1 C. N. Arge,2-heliolatitude solar wind over approximately the last three solar cycles. Related key parameters like interplanetary explain solar magnetic field control of long-term interplanetary variations. In particular, the enduring

California at Berkeley, University of

432

Long-Period Solar Variability  

SciTech Connect (OSTI)

Terrestrial climate records and historical observations of the Sun suggest that the Sun undergoes aperiodic oscillations in radiative output and size over time periods of centuries and millenia. Such behavior can be explained by the solar convective zone acting as a nonlinear oscillator, forced at the sunspot-cycle frequency by variations in heliomagnetic field strength. A forced variant of the Lorenz equations can generate a time series with the same characteristics as the solar and climate records. The timescales and magnitudes of oscillations that could be caused by this mechanism are consistent with what is known about the Sun and terrestrial climate.

GAUTHIER,JOHN H.

2000-07-20T23:59:59.000Z

433

GaInP/GaAs dual junction solar cells on Ge/Si epitaxial templates Melissa J. Archer,1,a  

E-Print Network [OSTI]

GaInP/GaAs dual junction solar cells on Ge/Si epitaxial templates Melissa J. Archer,1,a Daniel C Richard R. King,2 and Harry A. Atwater1 1 California Institute of Technology, Pasadena, California 91125, USA 2 Spectrolab, Inc., Sylmar, California 91342, USA 3 Aonex Technologies, Pasadena, California 91106

Atwater, Harry

434

FIRST DEMONSTRATION OF MONOLITHIC InP-BASED InAlAs/InGaAsP/InGaAs TRIPLE JUNCTION SOLAR CELLS  

E-Print Network [OSTI]

FIRST DEMONSTRATION OF MONOLITHIC InP-BASED InAlAs/InGaAsP/InGaAs TRIPLE JUNCTION SOLAR CELLS Robyn C. Law 1 1 Spectrolab, Inc., A Boeing Company, Sylmar, California 91342, USA 2 California Institute of Technology, Pasadena, California 91125, USA ABSTRACT Spectrolab has demonstrated the first lattice matched In

Atwater, Harry

435

Shunda SolarE Technologies | Open Energy Information  

Open Energy Info (EERE)

Shunda SolarE Technologies Jump to: navigation, search Name: Shunda-SolarE Technologies Sector: Solar Product: US-based JV with vertically integrated operations in the solar...

436

First Solar AVSR Solar Ranch Technical Eligibility Re-Evaluation...  

Energy Savers [EERE]

First Solar AVSR Solar Ranch Technical Eligibility Re-Evaluation Memo First Solar AVSR Solar Ranch Technical Eligibility Re-Evaluation Memo FirstSolarAVSRSolarRanchOneTechnic...

437

Solar energy: Hydrogen and oxygen  

Science Journals Connector (OSTI)

Solar energy: Hydrogen and oxygen ... Demonstrating the electrolysis of water with solar energy. ...

John J. Farrell

1982-01-01T23:59:59.000Z

438

Solar in Cold, Cloudy Climates  

Broader source: Energy.gov [DOE]

Presentation delivered by Chuck Marken during the 2009 Northeastern Solar Cities Conference Solar Survey session.

439

Application of solar energy.  

E-Print Network [OSTI]

??The purpose of the project is to learn the principle and application of solar energy and to know the situation of solar energy in China (more)

Li, Jingcheng

2010-01-01T23:59:59.000Z

440

Solar | Department of Energy  

Office of Environmental Management (EM)

Science & Innovation Energy Sources Renewable Energy Solar Solar The Energy Department's 2014 SunShot Grand Challenge Summit is in full swing -- bringing together...

Note: This page contains sample records for the topic "usa solar fields" 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

Sandia National Laboratories: Solar  

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

Center in Vermont Achieves Milestone Installation On September 23, 2014, in Concentrating Solar Power, Energy, Facilities, National Solar Thermal Test Facility, News, News &...

442

NREL: Solar STAT Blog -  

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

Outreach Policy Basics Publications Request Assistance Technical Assistance Project Map Solar STAT Blog The Solar STAT blog discusses the most recent NREL and DOE SunShot...

443

Solar heating in Colombia.  

E-Print Network [OSTI]

?? This report describes the process of a thesis implemented in Colombia concerning solar energy. The project was to install a self-circulating solar heating system, (more)

Skytt, Johanna

2012-01-01T23:59:59.000Z

444

Solar Energy Technologies Office  

Broader source: Energy.gov [DOE]

In 2011, the Energy Department's Solar Energy Technologies Office (SETO) became the SunShot Initiative, a collaborative national effort that aggressively drives innovation to make solar energy...

445

Solar Thermoelectric Energy Conversion  

Broader source: Energy.gov [DOE]

Efficiencies of different types of solar thermoelectric generators were predicted using theoretical modeling and validated with measurements using constructed prototypes under different solar intensities

446

Your Solar Home  

Broader source: Energy.gov [DOE]

Solar Schoolhouse Education supplement for the Sacramento Bee to introduce solar to elementary school children and introduce the design and AD contest for local students.

447

Solar | Department of Energy  

Energy Savers [EERE]

Energy Sources Renewable Energy Solar Solar The Energy Department's 2014 SunShot Grand Challenge Summit is in full swing -- bringing together government, industry, national...

448

Making a Solar Oven  

Broader source: Energy.gov [DOE]

Students make solar ovens. Student background information is provided. The expected outcome is that students will learn about solar energy transfer.

449

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

Total Radiation in Canada. Solar Energy ~, p.153. Threlkeld,Solar Energy Society Joint Conference, Vol. 4, p.281, Winnipeg, Canada.

Berdahl, P.

2010-01-01T23:59:59.000Z

450

Subsidizing Global Solar Power.  

E-Print Network [OSTI]

?? With national cuts on solar PV subsidies and the current oversupply of panels, the global solar market is clearly threatened by a contraction. Yet, (more)

Arnesson, Daniel

2013-01-01T23:59:59.000Z

451

Solar power satellites.  

E-Print Network [OSTI]

??During energy crisis at the end of the Sixties, a new idea to exploit solar energy arose: Solar Power Satellites. These satellites need a huge (more)

Palmas, Alessandro

2013-01-01T23:59:59.000Z

452

Solar skylight  

DOE Patents [OSTI]

A reflective shutter rotates within a skylight housing in such a fashion as to control solar energy thereby providing a combination of heating, lighting, and ventilation. The skylight housing has three faces: a glazed southern face, a glazed northern face, and an open downwardly oriented face to the interior of the structure. Counter-weighted pivot arms support the shutter at either end causing the center of rotation to pass through the center of gravity. The shutter has three basic positions: In the first position, during the winter day, the shutter closes off the northern face, allowing solar energy to enter directly into the supporting structure providing heat gain and daylighting. In the second position, during the winter night, the shutter closes off the open face to the interior, providing insulation between the structure and the skylight housing. In the third position, during the non-heating season, the shutter closes off the southern face blocking unwanted heat gain but allowing diffuse northern light to penetrate for daylighting. In this last position, a means is provided for ventilating by natural convection. The apparatus can be operated either manually or by motor.

Adamson, James C. (Osprey La., Rumson, NJ 07760)

1984-01-01T23:59:59.000Z

453

The Astrophysical Journal, 501:L213L216, 1998 July 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.  

E-Print Network [OSTI]

. All rights reserved. Printed in U.S.A. ENERGY DISTRIBUTION OF HEATING PROCESSES IN THE QUIET SOLAR of the Sun. The emission measure is found to vary significantly in at least 85% of all the pixels within 42 the observed increases in emission measure and the derived temperature. Heating events have been found

454

You are here: OUP USA Home > U.S. General Catalog > Atmospheric Science > Climatology Radiation and Cloud Processes in the Atmosphere  

E-Print Network [OSTI]

You are here: OUP USA Home > U.S. General Catalog > Atmospheric Science > Climatology Radiation and long-range levels. The author here offers a systematic discussion of the transfer of solar and thermal important topics in atmospheric radiation, cloud physics, and thermal equilibrium. Aspects

Liou, K. N.

455

Forecasting Solar Wind Speeds  

E-Print Network [OSTI]

By explicitly taking into account effects of Alfven waves, I derive from a simple energetics argument a fundamental relation which predicts solar wind (SW) speeds in the vicinity of the earth from physical properties on the sun. Kojima et al. recently found from their observations that a ratio of surface magnetic field strength to an expansion factor of open magnetic flux tubes is a good indicator of the SW speed. I show by using the derived relation that this nice correlation is an evidence of the Alfven wave which accelerates SW in expanding flux tubes. The observations further require that fluctuation amplitudes of magnetic field lines at the surface should be almost universal in different coronal holes, which needs to be tested by future observations.

Takeru K. Suzuki

2006-02-03T23:59:59.000Z

456

Solar Fuels and Chemicals, Solar Hydrogen  

Science Journals Connector (OSTI)

The term solar power plant commonly refers to electricity production by photothermal or photovoltaic conversion. Within this book, these main conversion techniques are called the solar thermoelectric path and the...

M. Fischer; R. Tamme

1991-01-01T23:59:59.000Z

457

Solar Blog  

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

blog Office of Energy Efficiency & Renewable blog Office of Energy Efficiency & Renewable Energy Forrestal Building 1000 Independence Avenue, SW Washington, DC 20585 en From Mind to Marketplace: SunShot Incubator's Latest Protégés Get to Work http://energy.gov/eere/articles/mind-marketplace-sunshot-incubator-s-latest-prot-g-s-get-work From Mind to Marketplace: SunShot Incubator's Latest Protégés Get to Work

458

Magnetic Relaxation in the Solar Corona Kenneth Miller1  

E-Print Network [OSTI]

Magnetic Relaxation in the Solar Corona Kenneth Miller1 , Bengt Fornberg2 , Natasha Flyer3 , & B. C- duced in the tenuous solar corona by the turbulent, resistive relaxation of a magnetic field under interact with its surrounding fields. A boundary-value problem is posed for a two dimensional model

Fornberg, Bengt

459

Sandia National Laboratories: Solar Resource Assessment  

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

Tagged with: Energy * photovoltaic * Photovoltaics * PV * Renewable Energy * solar * Solar Energy * Solar Research * Solar Resource Assessment Comments are closed. Renewable...

460

Coaltec Energy USA Inc | Open Energy Information  

Open Energy Info (EERE)

Coaltec Energy USA Inc Coaltec Energy USA Inc Jump to: navigation, search Name Coaltec Energy USA, Inc. Place Carterville, Illinois Zip 62918 Sector Biomass Product Coaltec Energy provides energy systems for businesses that have large quantities of waste, biomass, or other fuel source available. Coordinates 37.149025°, -94.433657° 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":37.149025,"lon":-94.433657,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "usa solar fields" 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

DOE Solar Decathlon: Sponsors  

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

Dow Corning Lowe's M.C. Dean Pepco Schneider Electric Supporting Sponsors Contributing Sponsors Where Are the Houses Now? Quick Links Solar Decathlon Home Solar Decathlon 2011 Solar Decathlon 2009 Solar Decathlon 2007 Solar Decathlon 2005 Solar Decathlon 2002 Solar Decathlon 2011 Sponsors The U.S. Department of Energy (DOE) Solar Decathlon is organized by the National Renewable Energy Laboratory, which works in partnership with sponsors at all levels to make this student solar housing competition and event a reality. 2011 Sustaining Sponsors These sponsors made significant contributions-including financial support, materials, volunteers, outreach, and awards-to the success of Solar Decathlon 2011. Learn more about each sponsor and its role in Solar Decathlon 2011. Dow Corning

462

Assessing occupational and domestic elf magnetic field exposure in the uk adult brain tumour study: results of a feasibility study  

Science Journals Connector (OSTI)

......investigation. Data collection Emdex II magnetic field meters (Enertech Consultants Ltd, California, USA) were used to record data...investigation. Data collection Emdex II magnetic eld meters (Enertech Consultants Ltd, California, USA) were used to record data......

Martie van Tongeren; Terry Mee; Pamela Whatmough; Lisa Broad; Myron Maslanyj; Stuart Allen; Ken Muir; Patricia McKinney

2004-02-01T23:59:59.000Z

463

Flows and Non-thermal Velocities in Solar Active Regions Observed with the Extreme-ultraviolet Imaging Spectrometer on Hinode: A Tracer of Active Region Sources of Heliospheric Magnetic Fields?  

E-Print Network [OSTI]

From Doppler velocity maps of active regions constructed from spectra obtained by the Extreme-ultraviolet Imaging Spectrometer (EIS) on the Hinode spacecraft we observe large areas of outflow (20-50 km/s) that can persist for at least a day. These outflows occur in areas of active regions that are faint in coronal spectral lines formed at typical quiet Sun and active region temperatures. The outflows are positively correlated with non-thermal velocities in coronal plasmas. The bulk mass motions and non-thermal velocities are derived from spectral line centroids and line widths, mostly from a strong line of Fe XII at 195.12 Angstroms. The electron temperature of the outflow regions estimated from an Fe XIII to Fe XII line intensity ratio is about 1.2-1.4 MK. The electron density of the outflow regions derived from a density sensitive intensity ratio of Fe XII lines is rather low for an active region. Most regions average around 7E10+8 cm(-3), but there are variations on pixel spatial scales of about a factor of 4. We discuss results in detail for two active regions observed by EIS. Images of active regions in line intensity, line width, and line centroid are obtained by rastering the regions. We also discuss data from the active regions obtained from other orbiting spacecraft that support the conclusions obtained from analysis of the EIS spectra. The locations of the flows in the active regions with respect to the longitudinal photospheric magnetic fields suggest that these regions might be tracers of long loops and/or open magnetic fields that extend into the heliosphere, and thus the flows could possibly contribute significantly to the solar wind.

G. A. Doschek; H. P. Warren; J. T. Mariska; K. Muglach; J. L. Culhane; H. Hara; T Watanabe

2008-07-17T23:59:59.000Z

464

Sunshot Rooftop Solar Challenge | Department of Energy  

Energy Savers [EERE]

Sunshot Rooftop Solar Challenge Sunshot Rooftop Solar Challenge Sunshot Rooftop Solar Challenge View All Maps Addthis...

465

Solar collector  

SciTech Connect (OSTI)

A solar energy water heating unit is provided which heats water from a swimming pool by passing the water through a series of spiral hoses mounted on a supporting surface. The supporting surface is mounted on a platform raised from the ground and is cone-shaped to allow for at least a portion of each hose line to be exposed to the sun at all times of the day. The spiral hose lines are mounted in spiral grooves provided on the supporting surface. A pump pumps the water from the swimming pool to the inlet of the hose lines, which inlet is adjacent the lowermost edge of the supporting surface so that the water is always pumped upwardly to the outlet end of the hose lines adjacent the apex of the supporting surface.

Miller, R.L.

1983-05-31T23:59:59.000Z

466

BNL | NSERC, the Northeast Solar Energy Research Center  

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

Northeast Solar Energy Research Center Northeast Solar Energy Research Center A multi-purpose research facility on the BNL campus Home Map of the Research Array Project Updates solar array NSERC, a multi-purpose research facility on the Brookhaven campus Brookhaven National Laboratory is developing a new Northeast Solar Energy Research Center (NSERC) on its campus that will serve as a solar energy research and test facility for the solar industry. The NSERC will include laboratories for standardized testing in accordance with industry standards, along with a solar PV research array for field testing existing or innovative new technologies under actual northeastern weather conditions. The NSERC will also include access to unique high-resolution data sets from the 32MW Long Island Solar Farm located at Brookhaven. Our vision is to

467

CALIFORNIA SOLAR DATA MANUAL  

E-Print Network [OSTI]

horizontal. Knowing this quantity is important since most solar applications that employ flat-plate collectors

Berdahl, P.

2010-01-01T23:59:59.000Z

468

Solar Policy Environment: Sacramento  

Broader source: Energy.gov [DOE]

The City of Sacramento and the greater Sacramento region is the home of a long standing history of commitment to solar. Sacramento Solar Access seeks to further widespread adoption of solar energy by addressing current market barriers and preparing, through design guidelines and education, the infrastructure that will optimize solar production in the future.

469

Solar Policy Environment: Houston  

Broader source: Energy.gov [DOE]

The City of Houston is committed to achieving a sustainable solar infrastructure through strategic partnerships that address market barriers for solar energy through the Houston Solar Initiative. The initiative is dedicated to this long-term goal while focusing on near- and mid-term results that go beyond demonstration solar projects.

470

The solar dynamo  

Science Journals Connector (OSTI)

...compiled and edited by Clare E. Parnell The solar dynamo Mark S. Miesch * * miesch@ucar...Astrophysical processes on the Sun . The origins of solar magnetism lie below the visible surface...recent insights into the operation of the solar dynamo obtained from solar and stellar...

2012-01-01T23:59:59.000Z

471

Can solar power deliver?  

Science Journals Connector (OSTI)

...Articles 1002 117 Discussion Meeting Issue Can solar power deliver? organized and edited by...S. Roberto Amendolia and Can Li Can solar power deliver? Jenny Nelson 1 2 Christopher...of 15 to a Discussion Meeting Issue Can solar power deliver? . Solar power represents...

2013-01-01T23:59:59.000Z

472

Solar Policy Environment: Boston  

Broader source: Energy.gov [DOE]

City of Bostons objective in creating Solar Boston is to maximize solar technologys role in the Citys sustainable development, educational and emergency preparedness policies. Solar Bostons objective is the installation of solar technology on all feasible and appropriate locations throughout Boston.

473

DOE Solar Decathlon: About Solar Decathlon  

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

About Solar Decathlon About Solar Decathlon The U.S. Department of Energy Solar Decathlon is an award-winning program that challenges collegiate teams to design, build, and operate solar-powered houses that are cost-effective, energy-efficient, and attractive. The winner of the competition is the team that best blends affordability, consumer appeal, and design excellence with optimal energy production and maximum efficiency. The first Solar Decathlon was held in 2002; the competition has since occurred biennially in 2005, 2007, 2009, 2011, and 2013. The next event will take place in 2015. Open to the public free of charge, the Solar Decathlon gives visitors the opportunity to tour solar-powered houses, gather ideas to use in their own homes, and learn how energy-saving features can help them save money today.

474

Concentrating Solar Power Basics | Department of Energy  

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

Basics Basics Concentrating Solar Power Basics August 20, 2013 - 4:38pm Addthis Text Version This solar concentrator has a fixed-focus faceted dish with a concentration of about 250 suns. This system can be used for large fields connected to the utility grid, hydrogen generation, or water pumping. Credit: Science Applications International Corporation / PIX 13464 Concentrating solar power (CSP) technologies use mirrors to reflect and concentrate sunlight onto receivers that collect solar energy and convert it to heat. This thermal energy can then be used to produce electricity via a steam turbine or heat engine that drives a generator. Concentrating solar power offers a utility-scale, firm, dispatchable renewable energy option that can help meet our nation's demand for

475

Titan interaction with the supersonic solar wind  

E-Print Network [OSTI]

After 9 years in the Saturn system, the Cassini spacecraft finally observed Titan in the supersonic solar wind. These unique observations reveal that Titan interaction with the solar wind is in many ways similar to un-magnetized planets Mars and Venus in spite of the differences in the properties of the solar plasma in the outer solar system. In particular, Cassini detected a collisionless, supercritical bow shock and a well-defined induced magnetosphere filled with mass-loaded interplanetary magnetic field lines, which drape around Titan ionosphere. Although the flyby altitude may not allow the detection of an ionopause, Cassini reports enhancements of plasma density compatible with plasma clouds or streamers in the flanks of its induced magnetosphere or due to an expansion of the induced magnetosphere. Because of the upstream conditions, these observations are also relevant for unmagnetized bodies in the outer solar system such as Pluto, where kinetic processes are expected to dominate.

Bertucci, C; Kurth, W S; Hospodarsky, G; Mitchell, D; Sergis, N; Edberg, N J T; Dougherty, M K

2014-01-01T23:59:59.000Z

476

The Solar Wind Power from Magnetic Flux  

Science Journals Connector (OSTI)

Observations of the fast, high-latitude solar wind throughout Ulysses' three orbits show that solar wind power correlates remarkably well with the Sun's total open magnetic flux. These observations support a recent model of the solar wind energy and particle sources, where magnetic flux emergence naturally leads to an energy flux proportional to the strength of the large-scale magnetic field. This model has also been shown to be consistent with X-ray observations of the Sun and a variety of other stars over 12 decades of magnetic flux. The observations reported here show that the Sun delivers ~600 kW Wb?1 to power the solar wind, and that this power to magnetic flux relation has been extremely stable over the last 15 years. Thus, the same law that governs energy released in the corona and from other stars also applies to the total energy in the solar wind.

N. A. Schwadron; D. J. McComas

2008-01-01T23:59:59.000Z

477

Solar | Department of Energy  

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

Solar Solar Solar Learn how a fourth grade classroom solar project is contributing to the clean energy revolution. | Photo courtesy of Aaron Sebens. Learn how a fourth grade classroom solar project is contributing to the clean energy revolution. | Photo courtesy of Aaron Sebens. The tremendous growth in the U.S. solar industry is helping to pave the way to a cleaner, more sustainable energy future. Over the past few years, the cost of a solar energy system has dropped significantly -- helping to give more American families and business access to affordable, clean energy. Through a portfolio of R&D efforts, including the SunShot Initiative, the

478

Ocean Thermal Energy Conversion Mostly about USA  

E-Print Network [OSTI]

Ocean Thermal Energy Conversion History Mostly about USA 1980's to 1990's and bias towards Vega or other energy carriers to be delivered to shore... 13luisvega@hawaii.edu #12;US Federal Government OTEC period estimated at 3 to 4 years. #12;luisvega@hawaii.edu 20 Energy Carriers · OTEC energy could

479

Solar for All: A Community Solar Webinar  

Office of Energy Efficiency and Renewable Energy (EERE)

ICLEI Local Governments for Sustainability U.S.A. presents the second part of the Members Webinar Series highlighting best practices and innovative local solutions from the ICLEI member network....

480

Solar Policy Environment: Pittsburgh  

Broader source: Energy.gov [DOE]

In this project, Pittsburgh plans to build on its reputation as a national leader in green practices. Its Solar America Cities project will develop a distributed approach to adoption of solar energy technologies. Pittsburghs partnership includes universities, non-profit organizations, and business, labor and foundation communities. The city plans to transform the solar energy market and stimulate early adoption of solar technology, to show that solar technology works in a northern city.

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


481

Geothermal, Energy Efficiency, and Solar PV Opportunities at Nissan USE  

E-Print Network [OSTI]

Geothermal, Energy Efficiency, and Solar PV Opportunities at Nissan USA May 21st, 2014 Robinson Ford Justin Ong Jake Reeder Vikram Sridar Rica Zhang ESL-IE-14-05-04 Proceedings of the Thrity-Sixth Industrial Energy Technology Conference New... Orleans, LA. May 20-23, 2014 Carbon Goal is Driving Innovation ESL-IE-14-05-04 Proceedings of the Thrity-Sixth Industrial Energy Technology Conference New Orleans, LA. May 20-23, 2014 Research Areas Geothermal Solar Photovoltaics EE Verification ESL...

Ford, R.; Ong, J.; Reeder, J.; Sridar, V.; Zhang, R.

2014-01-01T23:59:59.000Z

482

Substance use by adolescents of the USA national longitudinal lesbian family study  

E-Print Network [OSTI]

use by adolescents of the USA national longitudinal lesbianuse by adolescents of the USA National Longitudinal LesbianUCLA School of Law, USA of Amsterdam, The Netherlands 3

Goldberg, Naomi G.; Bos, Henny M.W.; Gartrell, Nanette K.

2011-01-01T23:59:59.000Z

483

First report of the Asian seaweed Sargassum filicinum Harvey (Fucales) in California, USA  

E-Print Network [OSTI]

for cox3 sequences. Country USA Site Intake Pipes, SantaFucales) in California, USA Kathy Ann Miller 1 , John M.Berkeley, California, USA Marine Science Institute,

Miller, Kathy Ann; Engle, John M.; Uwai, Shinya; Kawai, Hiroshi

2007-01-01T23:59:59.000Z

484

Building a Balance: Housing Affordability and Environmental Protection in the USA  

E-Print Network [OSTI]

University, Ithaca, NY 14853, USA. TEL: 607-225-2145.and Environmental Protection in the USA Joseph LaquatraCornell University, USA and Gregory L. Potter Independent

Laquatra, Joseph; Potter, Gregory L.

2000-01-01T23:59:59.000Z

485

Levels of metals from salt marsh plants from Southern California, USA  

E-Print Network [OSTI]

in San Diego Bay (California, USA). Chemosphere, 63(5), 818-Diego Bay region, California, USA. Environmental Toxicologymarsh sediment in California, USA. Part 2: Occurrence and

Hoyt, Kimberly Ann

2009-01-01T23:59:59.000Z

486

Hindawi Publishing Corporation 410 Park Avenue,15th Floor,#287 pmb,New York,NY 10022,USA  

E-Print Network [OSTI]

Corporation 410 Park Avenue,15th Floor,#287 pmb,New York,NY 10022,USA http. Bona USA J. R. Cannon USA S.-N. Chow USA B. S. Dandapat India E. DiBenedetto USA R. Finn USA R. L. Fosdick USA J. Frehse Germany A. Friedman USA R. Grimshaw UK J. Malek Czech Republic J. T. Oden USA R

Shen, Xuemin "Sherman"

487

San Francisco, California: Solar in Action (Brochure), Solar...  

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

San Francisco, California: Solar in Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) San Francisco, California: Solar in Action (Brochure),...

488

Portland, Oregon: Solar in Action (Brochure), Solar America Cities...  

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

Action (Brochure), Solar America Cities, Energy Efficiency & Renewable Energy (EERE) San Francisco, California: Solar in Action (Brochure), Solar America Cities, Energy Efficiency...

489

NREL: Technology Deployment - Portland, Oregon Grassroots Solarize...  

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

30% News Watch a video on the Solarize movement Pallets of PV: Communities Purchase Solar and Drive Down Costs Together Solarize Portland Solarize New York Solarize...

490

Krnvapennedrustning i USA och Sovjetunionen; Nuclear disarmament: USA and the Soviet Union.  

E-Print Network [OSTI]

?? AbstractIII-essay in political science by Christoffer Harnell, autumn -08. Supervisor: Malin Stegman-McCallion. Nuclear Disarmament - USA and the Soviet Union 1960-2002 This essay is (more)

Harnell, Christoffer

2009-01-01T23:59:59.000Z

491

Photovoltaic solar concentrator module  

SciTech Connect (OSTI)

This invention consists of a planar photovoltaic concentrator module for producing an electrical signal from incident solar radiation which includes an electrically insulating housing having a front wall, an opposing back wall and a hollow interior. A solar cell having electrical terminals is positioned within the interior of the housing. A planar conductor is connected with a terminal of the solar cell of the same polarity. A lens forming the front wall of the housing is operable to direct solar radiation incident to the lens into the interior of the housing. A refractive optical element in contact with the solar cell and facing the lens receives the solar radiation directed into the interior of the housing by the lens and directs the solar radiation to the solar cell to cause the solar cell to generate an electrical signal. An electrically conductive planar member is positioned in the housing to rest on the housing back wall in supporting relation with the solar cell terminal of opposite polarity. The planar member is operable to dissipate heat radiated by the solar cell as the solar cell generates an electrical signal and further forms a solar cell conductor connected with the solar cell terminal to permit the electrical signal generated by the solar cell to be measured between the planar member and the conductor.

Chiang, C.J.

1991-05-16T23:59:59.000Z

492

Evaluation on penetration rate of cloud for incoming solar radiation using geostationary satellite data  

Science Journals Connector (OSTI)

Solar surface insolation (SSI) represents how much solar radiance reaches the Earths surface in a specified area and is an important parameter in various fields such as surface energy research, meteorology, a...

Jong-Min Yeom; Kyung-Soo Han; Jae-Jin Kim

2012-05-01T23:59:59.000Z

493

Improving the reliability and accuracy of a multipyranometer array measuring solar radiation  

E-Print Network [OSTI]

The measurement of solar radiation is crucial for the use of solar energy in fields including power generation, agriculture and meteorology. In the building sciences, It is essential for daylighting studies, energy use calculations, and thermal...

Klima, Peter Miloslaw

2012-06-07T23:59:59.000Z

494

Smeg USA: Order (2011-CE-14/1909)  

Broader source: Energy.gov [DOE]

DOE ordered Smeg USA, Inc. to pay a $6,000 civil penalty after finding Smeg USA had failed to certify that certain models of dishwashers and refrigerators comply with the applicable energy conservation standards.

495

DuraLamp USA: Order (2010-CE-0912)  

Broader source: Energy.gov [DOE]

DOE ordered DuraLamp USA, Inc. to pay a $2,500 civil penalty after finding DuraLamp USA had failed to certify that model PAR 30, an incandescent reflector lamp, complies with the applicable energy conservation standards.

496

Recent developments for realistic solar models  

SciTech Connect (OSTI)

The 'solar abundance problem' has triggered a renewed interest in revising the concept of SSM from different perspectives: 1) constituent microphysics: equation of state, nuclear rates, radiative opacities; 2) constituent macrophysics: the physical processes impact the evolution of the Sun and its present-day structure, e.g. dynamical processes induced by rotation, presence of magnetic fields; 3) challenge the hypothesis that the young Sun was chemically homogeneous: the possible interaction of the young Sun with its protoplanetary disk. Here, I briefly review and then present a (personal) view on recent advances and developments on solar modeling, part of them carried out as attempts to solve the solar abundance problem.

Serenelli, Aldo M. [Institute of Space Sciences (CSIC-IEEC), Campus UAB, Bellaterra, 08193 (Spain)

2014-05-02T23:59:59.000Z

497

The Sun's interior structure and dynamics, and the solar cycle  

E-Print Network [OSTI]

The Sun's internal structure and dynamics can be studied with helioseismology, which uses the Sun's natural acoustic oscillations to build up a profile of the solar interior. We discuss how solar acoustic oscillations are affected by the Sun's magnetic field. Careful observations of these effects can be inverted to determine the variations in the structure and dynamics of the Sun's interior as the solar cycle progresses. Observed variations in the structure and dynamics can then be used to inform models of the solar dynamo, which are crucial to our understanding of how the Sun's magnetic field is generated and maintained.

Broomhall, A -M; Howe, R; Norton, A A; Thompson, M J

2014-01-01T23:59:59.000Z

498

QUANTIFICATION OF LOSSES IN THIN-FILM CdS/CdTe SOLAR CELLS S.H. Demtsu and J.R. Sites  

E-Print Network [OSTI]

QUANTIFICATION OF LOSSES IN THIN-FILM CdS/CdTe SOLAR CELLS S.H. Demtsu and J.R. Sites Department of Physics, Colorado State University, Fort Collins, CO 80523, USA ABSTRACT Quantification of solar cell Thin-film CdS/CdTe devices have been studied extensively, but some basic underlying properties

Sites, James R.

499

Evolution Solar | Open Energy Information  

Open Energy Info (EERE)

Town Tortola, United Kingdom Sector: Solar Product: British Virgin Islands-based solar energy company dedicated to establishing solar panel factories in the Middle East and...

500

2008 Solar Technologies Market Report  

E-Print Network [OSTI]

Department of Energy. Solar Technologies Program and LoanRenewable Energy 2008 SOLAR TECHNOLOGIES MARKET REPORTinvestments by solar technology 108 Figure 5.4.

Price, S.

2010-01-01T23:59:59.000Z