Sample records for incentive nova scotia

  1. Capital Investment Incentive (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    The Capital Investment Incentive (CII) is part of the Productivity Investment Program as outlined in the economic growth plan for Nova Scotia, jobsHere.

  2. Nova Scotia Jobs Fund (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    The Nova Scotia Jobs Fund pursues investment opportunities for assisting communities in transition, supporting industry sectors, offering regional support, assisting small businesses programs, and...

  3. Nova Scotia Business Development Program (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    The Nova Scotia Business Development Program helps small business get started and existing businesses expand. This program encourages business start-ups and provides help through qualified...

  4. Environmental Assessment (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    Nova Scotia Environment conducts environmental assessments on projects and developments to ensure they adhere to the laws and regulations of the province. Developments required to undergo an...

  5. Air Quality (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    Nova Scotia Environment is responsible for monitoring the air quality in the province, as well as administering fines and permits relating to air quality. The Air Quality Regulations state...

  6. Renewable Energy Standard (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    On February 1, 2007, Nova Scotia's new Renewable Energy Standards took effect. By 2013, Nova Scotia will generate at least 18.5% of the Province's electricity through renewable energy -- wind,...

  7. Scotia Energy Electricity- Net Metering Program (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    Nova Scotia Power Inc. Net Metering allows residential and commercial customers to connect small, renewable energy generating units to the provincial power grid.

  8. Solid Waste Regulations (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    Nova Scotia Environment administers waste management for the province. Regulations include specific rules and standards for landfills, establish a Resource Recovery Fund, and guidelines for...

  9. Efficiency Nova Scotia Releases Energy Efficiency Mobile App...

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

    Efficiency Nova Scotia Releases Energy Efficiency Mobile App Efficiency Nova Scotia Releases Energy Efficiency Mobile App Graphic of the inside of a house, with table and chairs,...

  10. Energy Security in Nova Scotia Larry Hughes

    E-Print Network [OSTI]

    Hughes, Larry

    to maintain energy security #12;Mr. Harper and his energy superpower · "...an ocean of oil soaked sand liesERG/200706 Energy Security in Nova Scotia Larry Hughes Energy Research Group Electrical to Café Canada, Mahone Bay 30 November 2007 #12;Energy security in Nova Scotia Larry Hughes, PhD Energy

  11. Qualifying RPS Market States (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    This entry lists the states with RPS policies that accept generation located in Nova Scotia, Canada as eligible sources towards their Renewable Portfolio Standard targets or goals. For specific...

  12. Climate Action Plan (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    Nova Scotia's Climate Change Action Plan has two main goals: reducing the province's contribution to climate change by reducing greenhouse gas (GHG) emissions and preparing for changes to the...

  13. Nova Scotia: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere I Geothermal Pwer PlantMunhall,Missouri: EnergyExcellence Seed LLCShores,Activity on Low RiskNova Scotia:

  14. area nova scotia: Topics by E-print Network

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

    Renewed Energy Strategy and Climate Change Action Plan Larry Halifax, Nova Scotia, Canada larry.hughes@dal.ca http:lh.ece.dal.caenen 19 December 2007 Hughes, Larry 4 Foreign...

  15. Community Feed-in Tariff (Nova Scotia, Canada)

    Broader source: Energy.gov [DOE]

    The Community Feed-In Tariff Program (COMFIT) is designed to increase local ownership of small-scale energy projects in Nova Scotia. The program provides an opportunity for community-based power...

  16. Dendrochronological dating of coal mine workings at the Joggins Fossil Cliffs, Nova Scotia, Canada

    E-Print Network [OSTI]

    Walters, Bradley B.

    Dendrochronological dating of coal mine workings at the Joggins Fossil Cliffs, Nova Scotia, Canada,NovaScotia,wasoneofthefirstplacesinNorthAmericawherecoalwasmined.Dendrochronologicalmeth- ods were employed to date timber pit props preserved within relic coal mine workings on the closely with archival records of mining activity. Analysis of the 14 openings al- lows differentiation of two phases

  17. CCCG 2014, Halifax, Nova Scotia, August 1113, 2014 An improved method for generating triangle-mesh models of images

    E-Print Network [OSTI]

    Adams, Michael D.

    CCCG 2014, Halifax, Nova Scotia, August 11­13, 2014 An improved method for generating triangle of Victoria, Victoria, BC, Canada, {xiaom,mdadams}@ece.uvic.ca triangulated were chosen. Since

  18. Mineralogical characterization of arsenic in gold mine tailings from three sites in Nova Scotia

    SciTech Connect (OSTI)

    M Corriveau; H Jamieson; M Parsons; G Hall

    2011-12-31T23:59:59.000Z

    Chronic exposure to high concentrations of arsenic (As) in windblown and vehicle-raised dust from tailings sites in Nova Scotia poses a potential health risk to recreational users of these areas and to nearby residents. The exposure may involve inhalation of dust, as well as oral ingestion of particles. It is important to understand the mineralogy and morphology of As-bearing dust particles in order to evaluate the risk posed by near-surface particulates in As-bearing tailings fields, as this will influence the stability and toxicity of As in the wastes. Optical mineralogy, scanning electron microscopy, electron microprobe, X-ray diffraction, synchrotron-based micro-X-ray diffraction ({mu}XRD) and micro-X-ray absorption near edge structure ({mu}XANES), and sequential leach extractions were applied to tailings samples from three sites in eastern Nova Scotia. Arsenic occurs naturally in these gold deposits mainly in arsenopyrite (FeAsS). In the near-surface material of the tailings fields, sulphide minerals have almost completely oxidized to secondary minerals such as scorodite (FeAsO{sub 4}{center_dot}2H{sub 2}O) and Ca-Fe arsenates. Iron oxyhydroxides contain variable amounts of As{sub 2}O{sub 5} from trace to 30 wt.% and CaO up to 8 wt.%. The presence of multiple As-hosting solid phases, including relatively soluble Ca-Fe arsenates and Fe oxyhydroxides with adsorbed As has important implications for human health risk assessment and remediation design.

  19. NOVA SCOTIA UTILITY AND REVIEW BOARD IN THE MATTER OF: The Public Utilities Act, R.S.N.S. 1989, c.380 as

    E-Print Network [OSTI]

    Hughes, Larry

    in the United Kingdom.7 I teach undergraduate courses in Computer Engineering and graduate courses in energy8 of the Nova Scotia Wind Energy Project, a $400,000 project1 designed to educate Nova Scotians about the benefits of wind energy. The first phase of2 the project collected wind data from various sites around

  20. Petrology, geochemistry, and palynology of Joggins Formation (Westphalian A) coals, Cumberland basin, Nova Scotia

    SciTech Connect (OSTI)

    Hower, J.C. [Univ. of Kentucky Center for Applied Energy Research, Lexington, KY (United States); Calder, J.H. [Nova Scotia Dept. of Natural Resources, Halifax (Canada); Cortland, F.E. [Kentucky Geological Survey, Lexington, KY (United States)] [and others

    1996-09-01T23:59:59.000Z

    Five Westphalian A coals were collected from the Joggins Formation section exposed along Chignecto Bay at Joggins, Nova Scotia. Several of the coal beds along the bay were mined beginning in the early 17th century. There has been little detailed investigation of the coal beds of this classic section. The lowermost coal, the Upper Coal 29 (Fundy), is a high-vitrinite coal with a spore assemblage dominated by arboreous lycopod spores with tree ferns subdominant. The upper portions of the coal bed have the highest ratio of well-preserved to poorly-preserved telinite of any of the coals investigated. Coal 19 (Forty Brine) has 88% total vitrinite but, unlike the Fundy coal bed, the telinite has a poor preservation ratio and half of the total vitrinite population comprises gelocollinite and vitrodetrinite. The latter coal bed is directly overlain by a basin-wide limestone bed. The Lower Kimberly (Coal 15) shows good preservation of vitrinite with relatively abundant telinite among the total vitrinite. The Upper Kimberly, which underlies the tetrapod-bearing lycopsid trees found by Lyell and Dawson in 1852, exhibits an upward decrease in arboreous lycopod spores and an increase in the tree fern spore Punctatisporites minutus. The megaspore record is similarly dominated by Lagenicularugosa paralycopodites and tree fern spores. Telinite preservation increases upwards in the Upper Kimberly but overall is well below the preservation ratio of the Fundy coal bed. The coals are all high sulfur, up to 13.7% total sulfur for the lower lithotype of the Fundy coal bed. The Kimberly coals are not only high in total and pyritic sulfur, but also have high concentrations of chalcophile elements.

  1. An investigation of cathodoluminescence in albite from the A-type Georgeville granite, Nova Scotia

    SciTech Connect (OSTI)

    Dalby, Kim N.; Anderson, Alan J.; Mariano, Anthony N.; Gordon, Robert A.; Mayanovic, Robert A.; Wirth, Richard (Missouri SU); (SFX); (Simon); (GFZ)

    2009-12-15T23:59:59.000Z

    Cathodoluminescence (CL) reveals red and blue colors within single, non-turbid albite (Ab{sub 98-99}) grains from the Georgeville granite, Nova Scotia. A 720 nm X-ray excited optical luminescence (XEOL) peak characterizes red CL regions, while a 280 nm XEOL feature dominates blue CL regions. Synchrotron X-ray fluorescence results indicate that red CL and the 720 nm XEOL peak intensities relate to total Fe concentrations. The relationship between red CL and Fe content is confirmed by electron microprobe (EMPA) and laser ablation-inductively coupled mass spectrometry (LA-ICP-MS). The XEOL technique is used to exclude the Fe K-edge as the cause of red CL. X-ray absorption spectroscopy results indicate that Fe in both the red and blue CL regions is Fe{sup 3+}, and that red CL activation may relate to the Si-Al order of the feldspar and to the distribution of Fe on tetrahedral sites. The CL textures, combined with EMPA and LA-ICPMS analyses, indicate that blue CL albite (Ab98) regions contain higher concentrations of Ca, Ti, Pb and rare earth elements, and were replaced, in part, by a more Fe-rich, trace element depleted albite (Ab99) which displays red CL. Complex diffraction contrasts and amorphous deposits identified in transmission electron microscope images suggest that aqueous fluids have reacted with both red and blue CL regions. Fluid inclusion homogenization temperatures of up to 430 C provide a lower estimate of the fluid temperature.

  2. Space Heating Trends in Prince Edward Island and Nova Scotia1 Mandeep Dhaliwal and Larry Hughes

    E-Print Network [OSTI]

    Hughes, Larry

    . Household income and shelter costs 4. Size and condition of the house 5. Fuel prices 6. Administration Hughes Energy Research Group Department of Electrical and Computer Engineering Dalhousie University Scotia have about the same fuel mix, although there are some differences in the use of electricity

  3. Arsenic Mineralogy of Near-surface Tailings and Soils: Influences on Arsenic Mobility and Bioaccessibility in the Nova Scotia Mining Districts

    SciTech Connect (OSTI)

    Walker, S.; Parsons, M; Jamieson, H; Lanzirotti, A

    2009-01-01T23:59:59.000Z

    The mineral form, grain size and texture of As-bearing particles are important factors influencing the risk to human health associated with exposure to As-contaminated soils, sediments and mine wastes. Mining of arsenopyrite-bearing gold ores in Nova Scotia in the late 1800s and early 1900s has left a legacy of weathered, As-rich tailings deposits in more than 60 gold districts across the province. Fourteen samples of near-surface tailings and one of soil from several former gold mines frequented by the public were sieved to <150 {mu}m and characterized using conventional mineralogical techniques (XRD, microscopy and EPMA) and synchrotron micro-analysis ({mu}-X-ray diffraction, {mu}-X-ray fluorescence and {mu}-X-ray absorption spectroscopy). This study is part of a broader coordinated effort by a multi-department federal and provincial advisory committee formed to coordinate the study of ecosystem and human health risks associated with historical gold mine sites in Nova Scotia. Our study shows that (i) the mineralogy of As in weathered tailings is highly variable, with aggregates of more than one As-bearing phase common in a given sample, and (ii) major differences in As mineralogy in the tailings are mainly controlled by factors that influence the weathering history (e.g., presence or absence of mill concentrates, degree of water saturation, and abundance of relict carbonate minerals). The variable solubility of these primary and secondary As-bearing minerals influences both the environmental mobility and the bioaccessibility of As in near-surface tailings and soil samples.

  4. Effects of Soil Composition and Mineralogy on the Bioaccessibility of Arsenic from Tailings and Soil in Gold Mine Districts of Nova Scotia

    SciTech Connect (OSTI)

    Meunier, Louise; Walker, Stephen R.; Wragg, Joanna; Parsons, Michael B.; Koch, Iris; Jamieson, Heather E.; Reimer, Kenneth J. (Queens); (Brit. Geo.); (Royal); (NRC)

    2010-10-20T23:59:59.000Z

    Bioaccessibility tests and mineralogical analyses were performed on arsenic-contaminated tailings and soils from gold mine districts of Nova Scotia, Canada, to examine the links between soil composition, mineralogy, and arsenic bioaccessibility. Arsenic bioaccessibility ranges from 0.1% to 49%. A weak correlation was observed between total and bioaccessible arsenic concentrations, and the arsenic bioaccessibility was not correlated with other elements. Bulk X-ray absorption near-edge structure analysis shows arsenic in these near-surface samples is mainly in the pentavalent form, indicating that most of the arsenopyrite (As{sup 1-}) originally present in the tailings and soils has been oxidized during weathering reactions. Detailed mineralogical analyses of individual samples have identified up to seven arsenic species, the relative proportions of which appear to affect arsenic bioaccessibility. The highest arsenic bioaccessibility (up to 49%) is associated with the presence of calcium-iron arsenate. Samples containing arsenic predominantly as arsenopyrite or scorodite have the lowest bioaccessibility (<1%). Other arsenic species identified (predominantly amorphous iron arsenates and arsenic-bearing iron(oxy)hydroxides) are associated with intermediate bioaccessibility (1 to 10%). The presence of a more soluble arsenic phase, even at low concentrations, results in increased arsenic bioaccessibility from the mixed arsenic phases associated with tailings and mine-impacted soils.

  5. The alteration of metamict zircon and its role in the remobilization of high-field strength elements in the Georgeville granite, Nova Scotia

    SciTech Connect (OSTI)

    Anderson, A.J.; Wirth, R.; Thomas, R. (SFX); (GFZ)

    2008-10-02T23:59:59.000Z

    The structure and composition of metamict zircon from the Georgeville epizonal A-type granite in the Antigonish Highlands, Nova Scotia, were determined using EMPA, SXRF, LA-ICP-MS, Raman microspectroscopy and TEM data. Individual crystals of zircon are variably altered and consist of four domains distinguished on the basis of texture and composition. Domain A consists of zircon and zirconium oxide nanocrystals in an amorphous matrix and is trace-element-enriched. Replacement of domain A in proximity to microfractures produced a porous and relatively trace-element-poor zircon (domain B) with disseminated Th-U- and Y-enriched inclusions (domain C). Domain D consists of amorphous zirconium silicate that is depleted in trace elements but enriched in Hf. It is found in fractures, together with minor amounts of thorite and thorianite. It Domain D is anhydrous and free of inclusions and pore spaces and has a composition similar to highly crystalline zircon. Micro- and nanoscale element-distribution maps indicate that high-field-strength trace elements in metamict zircon were redistributed during alteration by diffusion and by dissolution-and-reprecipitation processes near microfractures and other fluid channelways. The anomalous chondrite-normalized rare-earth-element patterns and Nd isotopic signature of the granite is attributed largely to the preferential transport and deposition of rare-earth elements during subsolidus re-equilibration of metamict zircon. Hydrothermally deposited zirconium silicate (domain D) has a composition similar to that of highly crystalline Hf-rich zircon but is completely amorphous. This observation emphasizes the need to verify the structural integrity and aqueous durability of hydrothermally deposited zircon before it is used to reconstruct hydrothermal processes.

  6. Energy Security in Nova Scotia Larry Hughes

    E-Print Network [OSTI]

    Hughes, Larry

    on the rest of Canada for its energy needs: all major energy corridors for natural gas and petroleum products

  7. Radiological Scoping Survey of the Scotia Depot, Scotia, NY

    SciTech Connect (OSTI)

    Bailey, E. N.

    2008-02-25T23:59:59.000Z

    The objectives of the radiological scoping survey were to collect adequate field data for use in evaluating the radiological condition of Scotia Depot land areas, warehouses, and support buildings.

  8. Application to Export Electric Energy OE Docket No. EA-355 Scotia...

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

    Scotia Capital Energyto export electric energy to Canada Application to Export Electric Energy OE Docket No EA-355 Scotia Capital Energy More Documents & Publications EA-355 Scotia...

  9. On the Weddell-Scotia Confluence and the Scotia Front

    E-Print Network [OSTI]

    Smith, Stephen Gregory

    1989-01-01T23:59:59.000Z

    of the ACC is separated from that oi' the Weddell Gyre by the Weddell-Scotia, Confluence. The 4 0 CO at I o o o o t 'cu o o d\\ 0 0 IA 0 o ' o c;- j d I o. . O dp Og 'Ig 0 pg Xgpg ' ' ~ ~ ', ' 'Od Ott a! co M ut OO Ch 0 0 cd... of the continental SAP PFZ PF AAZ C)NB CZ 26 27 28 29 (30 32 34 36 38 )40 42 43 44 45 46 4 48 49 0 0 l. s (m) /' / / I. O 05 ( / / I ~ I (m) 57 S 59 61' 62 0 IOO 200 300 400 500 600 700 800 km Figure 3. Vertical section of potential temperature ('C...

  10. Nova Scotia Topographic Database 1:10000 Received: April 2009

    E-Print Network [OSTI]

    Brownstone, Rob

    Topographic Database Data Compilation Specifications Common Name Actual Name Description Building_Point BL_POINT Buildings too small to be represented as polygons. These include homes and small public buildings. There are codes to indicate usage Building_Poly BL_POLY Larger buildings. There are codes to indicate usage. Some

  11. I; Dalhousie University Department of Earth Sciences Hjliijv Nova Scotia

    E-Print Network [OSTI]

    Beaumont, Christopher

    and Analytical Methods 29 Figure 4.1 Iron conglomerate (red circle) found in the abandoned slate quarry, used Arnold #12;Chapter 5: Results 39 A) -~c B) Figure 5.2 Halifax slate whole rock thin section (JAS00403 B crystals (Po) from Halifax slate sample JAS00403 B size fraction. The anhedral grain has a garnet (Gnt) rim

  12. Does Nova Scotia have an electric future? Response to

    E-Print Network [OSTI]

    Hughes, Larry

    of a jurisdiction. If supplies of refined petroleum products such as gasoline or home heating fuel become difficult in renewables such as wind will make limited impact on coal consumption. Figure 2: NSPI's supply mix

  13. 24 November 2004 Nova Scotia Utility and Review Board

    E-Print Network [OSTI]

    Hughes, Larry

    ) This letter and its accompanying report discusses NSPI's proposed Domestic Service Tariff price increase and Review Board (UARB) for increases in all its rate classes. In the Domestic Service Tariff, NSPI has Tariff NSPI's Domestic Service Tariff applies to about 418,900 residential customers. An analysis of NSPI

  14. Efficiency Nova Scotia Releases Energy Efficiency Mobile App | Department

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742Energy Chinaof EnergyImpactOn July 2, 2014 in theGroup Report |ofMTechnologicalNonprofitof

  15. STEP Request For Incentives

    Broader source: Energy.gov [DOE]

    STEP Request For Incentives, from the Tool Kit Framework: Small Town University Energy Program (STEP).

  16. Nonprice incentives and energy conservation.

    E-Print Network [OSTI]

    Asensio, OI; Delmas, MA

    2015-01-01T23:59:59.000Z

    challenging. Traditional economic incentives for householdbeen an important economic incentive for household energycant change in existing economic incentives advances our un-

  17. Sustaining Cost-Effective Incentives

    Broader source: Energy.gov [DOE]

    Presents how understanding the way in which customers' minds process incentives can help energy efficiency programs structure effective incentives.

  18. Incentives for Energy Independence

    Broader source: Energy.gov [DOE]

    In August 2007 Kentucky established the ''Incentives for Energy Independence Act'' to promote the development of renewable energy and alternative fuel facilities, energy efficient buildings,...

  19. Small Commercial Refrigeration Incentive

    Broader source: Energy.gov [DOE]

    Efficiency Vermont offers financial incentives to cover the incremental costs of energy efficient refrigeration for commercial, industrial, agricultural and institutional buildings. To receive the...

  20. Enterprise Zone Incentives (Florida)

    Broader source: Energy.gov [DOE]

    Enterprise Zone Incentives encourage business growth within certain geographic areas targeted for economic revitalization. Businesses which create jobs within a designated zone are eligible for...

  1. Effective Incentive Structures

    Broader source: Energy.gov [DOE]

    Presents an in-depth look at effective incentive structures, how to clarify your program goals, and tips to plan for the long term.

  2. Local Incentives (Massachusetts)

    Broader source: Energy.gov [DOE]

    The Massachusetts Office of Business Development helps companies to identify communities interested in offering locally-negotiated incentives, such as Tax Increment Financing (TIF), Special Tax...

  3. PV Incentive Program

    Broader source: Energy.gov [DOE]

    The New York State Energy Research and Development Authority (NYSERDA) provides an incentive eligible installers for the installation of approved, grid-connected photovoltaic (PV) systems. The base...

  4. Renewable Energy Incentive Program

    Broader source: Energy.gov [DOE]

    In February 2009, the District Department of the Environment (DDOE) introduced the Renewable Energy Incentive Program (REIP), a rebate for solar photovoltaic (PV) systems. In April 2012, solar...

  5. State and Local Incentives

    Broader source: Energy.gov [DOE]

    To help you make energy efficiency improvements in your commercial building, your state and/or local community might offer incentives or have special programs.

  6. New Homes Incentive Program

    Broader source: Energy.gov [DOE]

    Energy Trust's New Homes Program offers builders cash incentives for energy efficient measures included in new homes, where the measures exceed the building code. Lighting upgrades, whole home...

  7. Freezing in the dark: Energy security and heating emergencies in Nova Scotia

    E-Print Network [OSTI]

    Hughes, Larry

    ) supply of energy at an affordable price. A "regular supply" requires: Supply Infrastructure Why coal 10PJImported coal 69PJ Natural gas 5PJ Hydro 3PJ Biomass 17PJ 0 10 20 30 40 50 60 70 80 90 100 0% Biomass Electricity Fuel Oil 60% Fuel Oil 85% Natural gas 62% Natural gas 90% Percentageofafter

  8. Assessing Success in Aquaculture from the Farmer Perspective: The Case of Nova Scotia, Canada

    E-Print Network [OSTI]

    Charles, Anthony

    Canada). Available at: http://husky1.smu.ca/~charles/ Abstract This paper explores, from the farmer industry worth $28 million (DFO, * Address correspondence to A. Charles (t.charles@smu.ca) #12

  9. MHK Projects/OpenHydro Bay of Fundy Nova Scotia CA | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere I Geothermal Pwer Plant Jump to:LandownersLuther, Oklahoma:Energy Information Basin Bay

  10. Soil Profile CO2 concentrations in forested and clear cut sites in Nova Scotia, Canada

    E-Print Network [OSTI]

    Beltrami, Hugo

    concentration; Forest management; Soil temperature; Soil moisture; Soil texture 1. Introduction Subsurface2 production and transport caused by the complex interactions between biotic and environmental content, and soil physical characteristics (transport factors) mainly determine the variability

  11. NOvA Groundbreaking

    SciTech Connect (OSTI)

    2009-05-07T23:59:59.000Z

    May 1, 2009, marked the groundbreaking for the NOvA neutrino experiment located in Ash River, Minnesota.

  12. Exploration Incentive Tax Credit (Montana)

    Broader source: Energy.gov [DOE]

    The Mineral and Coal Exploration Incentive Tax Credit provides tax incentives to entities conducting exploration for minerals and coal. Expenditures related to the following activities are eligible...

  13. Economic Development Incentive Program (Massachusetts)

    Broader source: Energy.gov [DOE]

    The Economic Development Incentive Program (EDIP) is a tax incentive program designed to foster job creation and stimulate business growth throughout the Commonwealth. Participating companies may...

  14. Aligning Incentives With Program Goals

    Broader source: Energy.gov [DOE]

    Presents techniques used by Michigan Saves to increase participation and provide greater incentives.

  15. LADWP- Solar Incentive Program

    Broader source: Energy.gov [DOE]

    '''''Note: LADWP reached its budget limit for non-residential solar incentive applications in Augugst 2012. Applicants who have not received a confirmation as of August 22, 2012, have had their...

  16. Solar Thermal Incentive Program

    Broader source: Energy.gov [DOE]

    The New York State Energy Research and Development Authority (NYSERDA) offers incentives for the installation of solar water heating systems to residential and non-residential customers of the...

  17. Biomass Energy Production Incentive

    Broader source: Energy.gov [DOE]

    In 2007 South Carolina enacted the ''Energy Freedom and Rural Development Act'', which provides production incentives for certain biomass-energy facilities. Eligible systems earn $0.01 per kilowatt...

  18. Renewable Energy Incentives

    Broader source: Energy.gov [DOE]

    '''''Note: The Public Service Commission of Wisconsin (PSC) issued an order in September 2013 which suspends incentives for Solar Thermal and Solar Photovoltaic (PV) systems for the remainder of...

  19. JEA- Solar Incentive Program

    Broader source: Energy.gov [DOE]

    The JEA Solar Incentive Program provides rebates to JEA's residential customers who install new and retrofit solar hot water heaters on their homes. The rebate is worth $800 for new solar thermal...

  20. EA-355 Scotia Capital Energy, Inc. | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny:Revised Finding of No53197EFindingEA-257-CEA-296-B2244 TwinEA-355 Scotia Capital

  1. Ameren Illinois (Gas)- Business Efficiency Incentives

    Broader source: Energy.gov [DOE]

    The Specialty Equipment Application offers incentives on steamers, griddles, fryers, and other commercial kitchen equipment. The Steam Trap /Process Steam Incentive Program offers incentives on s...

  2. CPS Energy- New Residential Construction Incentives

    Broader source: Energy.gov [DOE]

    CPS Energy offers incentives for new residential construction that is at least 15% more efficient than required by the [http://dsireusa.org/incentives/incentive.cfm?Incentive_Code=TX29R&re=1...

  3. High Performance Incentive Program (Kansas)

    Broader source: Energy.gov [DOE]

    High Performance Incentive Program provides tax incentives to eligible employers that pay above-average wages and have a strong commitment to skills development for their workers. A substantial...

  4. Self-Generation Incentive Program

    Broader source: Energy.gov [DOE]

    Initiated in 2001, the Self-Generation Incentive Program (SGIP) offers incentives to customers who produce electricity with wind turbines, fuel cells, various forms of combined heat and power (CHP)...

  5. Solar Water Heating Incentive Program

    Broader source: Energy.gov [DOE]

    Beginning in the fall of 2003, Energy Trust of Oregon's Solar Water Heating (SWH) Incentive Program offers incentives to customers of Pacific Power, PGE, NW Natural Gas and Cascade Natural Gas who...

  6. City of Bloomington - Sustainable Development Incentives | Department...

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

    Bloomington - Sustainable Development Incentives City of Bloomington - Sustainable Development Incentives < Back Eligibility Commercial Construction Industrial Residential Savings...

  7. Performance Incentives for Transmission

    E-Print Network [OSTI]

    Oren, Shmuel S.

    ) establishes a framework for markets based on locational marginal pricing (LMP). The NOPR envisions a critical role for congestion rev- enue rights (CRRs), which entitle holders to streams of nodal price, because the extent and location of congestion in LMP-based markets is transparent. Incentive regulation

  8. MONITORING STRATIFICATION AND CURRENTS AT THE CONTINENTAL SLOPE OF THE SCOTIA SEA, ANTARCTICA

    E-Print Network [OSTI]

    Thornton, Melanie 1989-

    2011-05-02T23:59:59.000Z

    fulfillment of the requirements for the designation as UNDERGRADUATE RESEARCH SCHOLAR A Senior Scholars Thesis by MELANIE R. THORNTON MONITORING STRATIFICATION AND CURRENTS AT THE CONTINENTAL SLOPE OF THE SCOTIA SEA, ANTARCTICA Approved by... of the requirements for the designation as UNDERGRADUATE RESEARCH SCHOLAR A Senior Scholars Thesis by MELANIE R. THORNTON iii ABSTRACT Monitoring Stratification and Currents at the Continental Slope of the Scotia Sea, Antarctica. (April 2011...

  9. Saskatchewan Petroleum Research Incentive (SPRI)

    Broader source: Energy.gov [DOE]

    The Saskatchewan Petroleum Research Incentive is intended to encourage research, development and demonstration of new technologies that facilitate the expanded production of Saskatchewan's oil and...

  10. GMP- Biomass Electricity Production Incentive

    Broader source: Energy.gov [DOE]

    Green Mountain Power Corporation (GMP), Vermont's largest electric utility, offers a production incentive to farmers who own systems utilizing anaerobic digestion of agricultural products,...

  11. Advanced Technology Vehicles Manufacturing Incentive Program...

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

    Advanced Technology Vehicles Manufacturing Incentive Program Advanced Technology Vehicles Manufacturing Incentive Program This is an interim final rule that establishes the...

  12. Voluntary Initiative on Incentives: Toolkit Training Webinar...

    Energy Savers [EERE]

    Voluntary Initiative on Incentives: Toolkit Training Webinar Voluntary Initiative on Incentives: Toolkit Training Webinar March 26, 2015 12:30PM to 2:0...

  13. Quantitative Financial Analysis of Alternative Energy Efficiency Shareholder Incentive Mechanisms

    E-Print Network [OSTI]

    Cappers, Peter

    2010-01-01T23:59:59.000Z

    of DSR program incentive regulation. Introduction Recentin developing an incentive regulation approach for demand-

  14. This project was funded by Nova Scotia Power. The views and opinions expressed in the report are those of the Do Electric Vehicles Make Carbon-Sense in Nova Scotia?

    E-Print Network [OSTI]

    Hughes, Larry

    the EPRI report, Environmental Assessment of Plug-In Hybrid Electric Vehicles, Volume 1: Nationwide Greenhouse Gas Emissions (EPRI, 2007), which determines annual emissions based on the vehicle's Utility Factor (UF), the distance driven electrically and non-electrically (i.e., with gasoline). In the EPRI

  15. Funding for the food miles project was provided through Agriculture and Agri-Food Canada's Advancing Canadian Agriculture and Agri-Food (ACAAF) Program. In Nova Scotia the program is delivered by Agri-Futures Nova Scotia.

    E-Print Network [OSTI]

    Peak, Derek

    Funding for the food miles project was provided through Agriculture and Agri-Food Canada.................................................................... 7 Energy .................................................................................. 9 Self grown? With these two questions at the fore, combing through various statistics and reports

  16. Projected impacts of climate change on species distribution in the Acadian Forest region of eastern Nova Scotia

    E-Print Network [OSTI]

    .e., hydrological cycle and earth- sun geometry. Growing degree days and mean air temperature are basedProjected impacts of climate change on species distribution in the Acadian Forest region of eastern on processing remote sensing data, mean air temperatures serves as one of several inputs to model calculation

  17. Commercial Scale Wind Incentive Program

    Broader source: Energy.gov [DOE]

    Energy Trust of Oregons Commercial Scale Wind offering provides resources and cash incentives to help communities, businesses land owners, and government entities install wind turbine systems up...

  18. Wind Energy Manufacturing Tax Incentive

    Broader source: Energy.gov [DOE]

    With the passage of [http://www.arkansasenergy.org/media/261385/act736.pdf HB 2230 (2009)] in April 2009, the Arkansas Legislature expanded a tax incentive for manufacturers of windmill blades or...

  19. Vermont Employment Growth Incentive (Vermont)

    Broader source: Energy.gov [DOE]

    The purpose of the Employment Growth Incentive (VEGI) is to encourage job creation in Vermont by a Vermont company, a Vermont division of a company that plans to grow and expand in Vermont, a...

  20. Employment Incentive Credit (New York)

    Broader source: Energy.gov [DOE]

    The Employment Incentive Credit is through the New York State Department of Taxation and Finance based on the same qualifying investment for the ITC. The credit is equal to 1.5% to 2.5% of...

  1. Xcel Energy- Solar Production Incentive

    Broader source: Energy.gov [DOE]

    Beginning in 2014, Xcel must offer a solar production incentive for systems 20 kW-DC or less. The customer's system capacity may not be more than 120% of the customer's on-site annual energy...

  2. SCE- California Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    Southern California Edison offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new...

  3. Profit incentives and technological change

    E-Print Network [OSTI]

    Linn, Joshua

    2005-01-01T23:59:59.000Z

    This thesis is a collection of three empirical essays on the effect of profit incentives on innovation and technology adoption. Chapter 1, written with Daron Acemoglu, investigates the effect of (potential) market size on ...

  4. Renewable Energy Business Tax Incentives

    Broader source: Energy.gov [DOE]

    [http://www.azleg.gov/legtext/49leg/1r/bills/sb1403s.pdf SB 1403], signed in July of 2009, created tax incentives intended to draw renewable energy product manufacturers to Arizona. Specifically,...

  5. NOvA First Blast

    SciTech Connect (OSTI)

    2009-07-22T23:59:59.000Z

    Blasting began at the future site of the NOvA detector facility near Ash River, Minnesota, on Monday, July 20.

  6. Economic Incentives to Promote Innovation in Healthcare Delivery

    E-Print Network [OSTI]

    Luft, Harold S.

    2009-01-01T23:59:59.000Z

    U E S IN ORTHOPAEDIC SURGERY Economic Incentives to Promoteservice offers no economic incentives for clinicians to ef?10, October 2009 Economic Incentives Promoting Innovation

  7. Better Buildings: Financing and Incentives: Spotlight on Michigan...

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

    Michigan: Experiment to Find the Right Mix of Incentives Better Buildings: Financing and Incentives: Spotlight on Michigan: Experiment to Find the Right Mix of Incentives Better...

  8. NY-Sun Commerical/ Industrial Incentive Program

    Broader source: Energy.gov [DOE]

    New York State Energy Research and Development Authority (NYSERDA) through NY-Sun Commercial/Industrial Incentive Program (PON 3082) provides incentives for installation of non-residential new grid...

  9. Clean Energy Manufacturing Incentive Program (Virginia)

    Broader source: Energy.gov [DOE]

    In April 2011, Virginia created the Clean Energy Manufacturing Incentive Grant Program. The program is meant to replace the [http://en.openei.org/wiki/Solar_Manufacturing_Incentive_Grant_%28SMIG%29...

  10. Business Employment Incentive Program (BEIP) (New Jersey)

    Broader source: Energy.gov [DOE]

    Economically viable expanding or relocating businesses that create jobs in New Jersey are eligible to secure annual incentive grants via the Business Employment Incentive Program (BEIP) of up to 80...

  11. Puerto Rico- Economic Development Incentives for Renewables

    Broader source: Energy.gov [DOE]

    The 2008 Economic Incentives for the Development of Puerto Rico Act (EIA) provides a wide array of tax incentives and credits that enable local and foreign companies dedicated to certain business...

  12. Federal Incentives for Wind Power (Fact Sheet)

    SciTech Connect (OSTI)

    Not Available

    2013-05-01T23:59:59.000Z

    This fact sheet describes the federal incentives available as of April 2013 that encourage increased development and deployment of wind energy technologies, including research grants, tax incentives, and loan programs.

  13. International Microgrid Assessment: Governance, INcentives, and Experience (IMAGINE)

    E-Print Network [OSTI]

    Marnay, Chris

    2014-01-01T23:59:59.000Z

    DSIRE (Database of State Incentives for Renewables andSource: Database of State Incentives for Renewables and

  14. Federal Incentives for Water Power (Fact Sheet)

    SciTech Connect (OSTI)

    Not Available

    2013-05-01T23:59:59.000Z

    This fact sheet describes the federal incentives available as of April 2013 for the development of water power technologies.

  15. Nova Era | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca AgricolaNovaNova

  16. Economic Incentives for Protecting Digital Rights Online

    E-Print Network [OSTI]

    Wright , Matthew

    Economic Incentives for Protecting Digital Rights Online N. Boris Margolina, , Brian Neil Levineb propose the use of economic incentives to both limit and detect unautho- rized sharing. This approach has using direct economic incentives to discourage illegitimate shar- ing and to detect it when it occurs

  17. Forging the Link: Linking the Economic Incentives

    E-Print Network [OSTI]

    Forging the Link: Linking the Economic Incentives of Low Impact Development with Community on the economic incentives of LID to address the local decisional realities of community watershed protection in nature but details the economic incentives to LID. It is best suited for audiences seeking to understand

  18. Overview of State Programs, Incentives & Tax Credits for Business

    E-Print Network [OSTI]

    manufacturer classification (or R&D company) from DOR Web site: www.mass.gov/dor #12;Tax Incentives Economic Development Incentive Program The Economic Development Incentive Program (EDIP) is the primary economic-100) of added value Tax Incentives #12;Tax Incentives Economic Development Incentive Program Negotiated

  19. Argonne's Vilas Pol on NOVA!

    ScienceCinema (OSTI)

    None

    2013-04-19T23:59:59.000Z

    Can innovations in materials science help clean up our world? Argonne's material scientist Vilas Pol guest starred on NOVA's "Making Stuff: Cleaner," where David Pogue explored the rapidly-developing science and business of clean energy.

  20. american energy strategy: Topics by E-print Network

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

    Department of Energy's Consultation Paper Nova Scotia's Renewed Energy Strategy and Climate Change Action Plan Larry Halifax, Nova Scotia, Canada larry.hughes@dal.ca http:...

  1. Dover Public Utilities- Green Energy Program Incentives

    Broader source: Energy.gov [DOE]

    Delaware's municipal utilities provide incentives for solar photovoltaic (PV), solar thermal, wind, geothermal, and fuel cell systems installed by their electric customers. Eligibility is limited...

  2. Solar Manufacturing Incentive Grant (SMIG) Program

    Broader source: Energy.gov [DOE]

    Created in 1995 and administered jointly by the Virginia Department of Mines, Minerals and Energy, and the Virginia Economic Development Partnership, the Solar Manufacturing Incentive Grant (SMIG)...

  3. Clean and Green Property Tax Incentives

    Broader source: Energy.gov [DOE]

    In 2007, the Legislature passed House Bill 3 (May special session) that established property tax incentives to encourage energy projects with less environmental impact than conventional facilities....

  4. Industrial and Process Efficiency Performance Incentives

    Broader source: Energy.gov [DOE]

    The New York State Energy Research and Development Authority (NYSERDA) offers the Industrial and Process Efficiency (IPE) Program to provide performance-based incentives to manufacturers and data...

  5. Small-Scale Renewable Energy Incentive Program

    Broader source: Energy.gov [DOE]

    Vermont's Small Scale Renewable Energy Incentive Program (SSREIP), initiated in June 2003, provides funding for new solar water heating, solar electric (photovoltaic), modern wood pellet heating,...

  6. Delmarva- Commissioning and Operations Incentive Programs

    Broader source: Energy.gov [DOE]

    Delmarva's Enhanced Commissioning Program offers building design and commissioning incentives to commercial, industrial, governmental and institutional customers planning large new buildings....

  7. Alternative Fuel Production Facility Incentives (Kentucky) |...

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

    or biomass as a feedstock. Beginning Aug. 1, 2010, tax incentives are also available for energy-efficient alternative fuel production facilities and up to five alternative fuel...

  8. Virginia Economic Development Incentive Grant (Virginia)

    Broader source: Energy.gov [DOE]

    The Virginia Economic Development Incentive Grant is a discretionary cash grant, designed to assist and encourage companies to invest and create new employment opportunities by locating significant...

  9. Catawba County- Green Construction Permitting Incentive Program

    Broader source: Energy.gov [DOE]

    Catawba County is providing incentives to encourage the construction of sustainably built homes and commercial buildings. Rebates on permit fees and plan reviews are available for certain...

  10. Indianapolis Power & Light- Business Energy Incentives Program

    Broader source: Energy.gov [DOE]

    The Indiana Power and Light Business (IPL) Energy Incentives Program assists commercial and industrial customers with reducing energy consumption through three common types of equipment: lighting,...

  11. Fuel Cell Rebate and Performance Incentive

    Broader source: Energy.gov [DOE]

    Under PON 2157 The New York State Energy Research and Development Authority (NYSERDA) offers incentives for the purchase, installation, and operation of customer sited tier (CST, also called ...

  12. Renewable Energy Cost Recovery Incentive Payment

    Broader source: Energy.gov [DOE]

    In May 2005, Washington enacted Senate Bill 5101, establishing production incentives for individuals, businesses, and local governments that generate electricity from solar power, wind power or...

  13. Mohave Electric Cooperative- Renewable Energy Incentive Program

    Broader source: Energy.gov [DOE]

    Mohave Electric Cooperative provides incentives for its customers to install renewable energy systems on their homes and businesses. Mohave Electric Cooperative will provide rebates for...

  14. EXP Job Creation Incentive Program (Connecticut)

    Broader source: Energy.gov [DOE]

    The EXP Job Creation Incentive Program provides loans towards expenditures related to training, marketing, working capital, or other Connecticut Department of Economic and Community Development...

  15. PEPCO- Commissioning and Operations Incentive Programs

    Broader source: Energy.gov [DOE]

    Pepco's Enhanced Commissioning Program offers building design and commissioning incentives to commercial, industrial, governmental and institutional customers planning large new buildings....

  16. Energy Incentive Programs, Florida | Department of Energy

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

    for State Incentives for Renewables and Efficiency (DSIRE) site. What load managementdemand response options are available to me? TECO offers several load management programs:...

  17. NOvA Experiment - The Local Community

    ScienceCinema (OSTI)

    Deb Wieber

    2010-01-08T23:59:59.000Z

    Local proprietors Steve and Deb Wieber discuss the impact of the NOvA experiment on their community.

  18. NOvA Experiment - The Local Community

    SciTech Connect (OSTI)

    Deb Wieber

    2009-05-14T23:59:59.000Z

    Local proprietors Steve and Deb Wieber discuss the impact of the NOvA experiment on their community.

  19. Lesson learned from (some) recurrent novae

    E-Print Network [OSTI]

    Mason, Elena

    2013-01-01T23:59:59.000Z

    In this talk we present early decline and nebular spectra of the recurrent novae YY Dor and nova LMC 2009. These and a few other recurrent novae of the same type, share similar spectral characteristics and evolution. We will critically discuss those common features suggesting same white dwarf progenitor and post outburst phases for all of them.

  20. Vicerreitora de Calidade e Novas Tecnoloxas

    E-Print Network [OSTI]

    Fraguela, Basilio B.

    #12;#12;#12;Vicerreitora de Calidade e Novas Tecnoloxas CENTRO/DPTO./I.U./CENTRO DE GASTO.: Data: RESOLUCIN DA VICERREITORA DE CALIDADE E NOVAS TECNOLOXAS Conforme Data: Aplicacin.: Vicerreitor de Calidade e Novas Tecnoloxas A Corua, ___de ___________ de _______ SOLICITUDE DE ADQUISICIN

  1. Strategies to Address Split Incentives in Multifamily Buildings...

    Office of Environmental Management (EM)

    Strategies to Address Split Incentives in Multifamily Buildings Strategies to Address Split Incentives in Multifamily Buildings Better Buildings Neighborhood Program Multifamily ...

  2. NIPSCO Custom Commercial and Industrial Gas and Electric Incentive Program

    Broader source: Energy.gov [DOE]

    NIPSCOs Commercial and Industrial Custom Electric and Natural Gas Incentive Program offers financial incentives to qualifying large commercial, industrial, non-profit, governmental and...

  3. Better Buildings: Financing and Incentives: Spotlight on Maine...

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

    to a Sustainable Level of Incentives More Documents & Publications Spotlight on Maine: Transition to a Sustainable Level of Incentives Better Buildings: Workforce, Spotlight on...

  4. Avista Utilities (Electric)- Commercial Energy Efficiency Incentives Program

    Broader source: Energy.gov [DOE]

    Avista Utilities offers numerous incentives to commercial and industrial customers to increase the energy efficiency of customer facilities or equipment. Incentive options are available for heating...

  5. Federal Fuel Cell Tax Incentives: An Investment in Clean and...

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

    Fuel Cell Tax Incentives: An Investment in Clean and Efficient Technologies Federal Fuel Cell Tax Incentives: An Investment in Clean and Efficient Technologies A brief created by...

  6. APS - Renewable Energy Incentive Program | Department of Energy

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

    program. Performance-based incentives, which had previously been available for larger renewable energy systems have been terminated. Only upfront incentives for smaller systems...

  7. Financial Incentives Available for Facilities Affected by the...

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

    discussed. This paper provides an overview of incentives for which larger boilers and CHP systems qualify; Federal incentive programs are discussed and state, utility and...

  8. Miami-Dade County- Targeted Jobs Incentive Fund

    Broader source: Energy.gov [DOE]

    The Targeted Jobs Incentive Fund (TJIF) provides financial incentives for select industries, including solar thermal and photovoltaic manufacturing, installation and repair companies that are...

  9. National Grid (Electric) Residential EnergyWise Incentive Program

    Broader source: Energy.gov [DOE]

    National Grid offers a variety of energy efficiency incentives for residential customers. Incentives are provided for purchasing and implementing insulation upgrades, HVAC equipment, appliances,...

  10. Cascade Natural Gas- Conservation Incentives for New Homes

    Broader source: Energy.gov [DOE]

    Cascade Natural Gas offers a variety of incentives to residential customers for including energy efficiency measures in new homes in Washington and Oregon. Incentives are available directly from...

  11. Incentive Games and Mechanisms for Risk Management

    E-Print Network [OSTI]

    Alpcan, Tansu

    2010-01-01T23:59:59.000Z

    Incentives play an important role in (security and IT) risk management of a large-scale organization with multiple autonomous divisions. This paper presents an incentive mechanism design framework for risk management based on a game-theoretic approach. The risk manager acts as a mechanism designer providing rules and incentive factors such as assistance or subsidies to divisions or units, which are modeled as selfish players of a strategic (noncooperative) game. Based on this model, incentive mechanisms with various objectives are developed that satisfy efficiency, preference-compatibility, and strategy-proofness criteria. In addition, iterative and distributed algorithms are presented, which can be implemented under information limitations such as the risk manager not knowing the individual units' preferences. An example scenario illustrates the framework and results numerically. The incentive mechanism design approach presented is useful for not only deriving guidelines but also developing computer-assistan...

  12. AT Cnc: A SECOND DWARF NOVA WITH A CLASSICAL NOVA SHELL

    SciTech Connect (OSTI)

    Shara, Michael M.; Mizusawa, Trisha; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024-5192 (United States); Wehinger, Peter [Steward Observatory, the University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Martin, Christopher D.; Neill, James D.; Forster, Karl [Department of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Mail Code 405-47, Pasadena, CA 91125 (United States); Seibert, Mark [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

    2012-10-20T23:59:59.000Z

    We are systematically surveying all known and suspected Z Cam-type dwarf novae for classical nova shells. This survey is motivated by the discovery of the largest known classical nova shell, which surrounds the archetypal dwarf nova Z Camelopardalis. The Z Cam shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts, in accord with the hibernation scenario of cataclysmic binaries. Here we report the detection of a fragmented 'shell', 3 arcmin in diameter, surrounding the dwarf nova AT Cancri. This second discovery demonstrates that nova shells surrounding Z Cam-type dwarf novae cannot be very rare. The shell geometry is suggestive of bipolar, conical ejection seen nearly pole-on. A spectrum of the brightest AT Cnc shell knot is similar to that of the ejecta of the classical nova GK Per, and of Z Cam, dominated by [N II] emission. Galaxy Evolution Explorer FUV imagery reveals a similar-sized, FUV-emitting shell. We determine a distance of 460 pc to AT Cnc, and an upper limit to its ejecta mass of {approx}5 Multiplication-Sign 10{sup -5} M {sub Sun }, typical of classical novae.

  13. Radiation from Dwarf Nova Discs

    E-Print Network [OSTI]

    Irit Idan; Jean-Pierre Lasota; Jean-Marie Hameury; Giora Shaviv

    1998-06-04T23:59:59.000Z

    We use the Shaviv and Wehrse (1991) code to model the vertical structure and the emission properties of quiescent dwarf nova discs. We find that in the case of HT Cas the quiescent disc must be optically thin, in contradiction with the requirements of the standard disc instability model. We find a viscosity parameter alpha > 1. Although this is much less than values (~ 100) obtained in isothermal slab models it is not consistent with the accretion disc model assumptions.

  14. NUCLEAR THERMOMETERS FOR CLASSICAL NOVAE

    SciTech Connect (OSTI)

    Downen, Lori N.; Iliadis, Christian [Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255 (United States)] [Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255 (United States); Jose, Jordi [Departament de Fisica i Enginyeria Nuclear, EUETIB, Universitat Politecnica de Catalunya, E-08036 Barcelona (Spain)] [Departament de Fisica i Enginyeria Nuclear, EUETIB, Universitat Politecnica de Catalunya, E-08036 Barcelona (Spain); Starrfield, Sumner [School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-1404 (United States)] [School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-1404 (United States)

    2013-01-10T23:59:59.000Z

    Classical novae are stellar explosions occurring in binary systems, consisting of a white dwarf and a main-sequence companion. Thermonuclear runaways on the surface of massive white dwarfs, consisting of oxygen and neon, are believed to reach peak temperatures of several hundred million kelvin. These temperatures are strongly correlated with the underlying white dwarf mass. The observational counterparts of such models are likely associated with outbursts that show strong spectral lines of neon in their shells (neon novae). The goals of this work are to investigate how useful elemental abundances are for constraining the peak temperatures achieved during these outbursts and determine how robust 'nova thermometers' are with respect to uncertain nuclear physics input. We present updated observed abundances in neon novae and perform a series of hydrodynamic simulations for several white dwarf masses. We find that the most useful thermometers, N/O, N/Al, O/S, S/Al, O/Na, Na/Al, O/P, and P/Al, are those with the steepest monotonic dependence on peak temperature. The sensitivity of these thermometers to thermonuclear reaction rate variations is explored using post-processing nucleosynthesis simulations. The ratios N/O, N/Al, O/Na, and Na/Al are robust, meaning they are minimally affected by uncertain rates. However, their dependence on peak temperature is relatively weak. The ratios O/S, S/Al, O/P, and P/Al reveal strong dependences on temperature and the poorly known {sup 30}P(p, {gamma}){sup 31}S rate. We compare our model predictions to neon nova observations and obtain the following estimates for the underlying white dwarf masses: 1.34-1.35 M {sub Sun} (V838 Her), 1.18-1.21 M {sub Sun} (V382 Vel), {<=}1.3 M {sub Sun} (V693 CrA), {<=}1.2 M {sub Sun} (LMC 1990 no. 1), and {<=}1.2 M {sub Sun} (QU Vul).

  15. An Incentive Compatible Mechanism for Distributed Resource Planning

    E-Print Network [OSTI]

    Wu, David

    process and their economic incentives. If agents are not provided with proper incentives, they mayAn Incentive Compatible Mechanism for Distributed Resource Planning Erhan Kutanoglu Department is that without proper incentives, agents may not reveal this information trufully and they may not behave

  16. NOVA Making Stuff Season 2

    SciTech Connect (OSTI)

    Leombruni, Lisa; Paulsen, Christine Andrews

    2014-12-12T23:59:59.000Z

    Over the course of four weeks in fall 2013, 11.7 million Americans tuned in to PBS to follow host David Pogue as he led them in search of engineering and scientific breakthroughs poised to change our world. Levitating trains, quantum computers, robotic bees, and bomb-detecting plantsthese were just a few of the cutting-edge innovations brought into the living rooms of families across the country in NOVAs four-part series, Making Stuff: Faster, Wilder, Colder, and Safer. Each of the four one-hour programs gave viewers a behind-the-scenes look at novel technologies poised to change our worldshowing them how basic research and scientific discovery can hold the keys to transforming how we live. Making Stuff Season 2 (MS2) combined true entertainment with educational value, creating a popular and engaging series that brought accessible science into the homes of millions. NOVAs goal to engage the public with such technological innovation and basic research extended beyond the broadcast series, including a variety of online, educational, and promotional activities: original online science reporting, web-only short-form videos, a new online quiz-game, social media engagement and promotion, an educational outreach toolkit for science educators to create their own makerspaces, an online community of practice, a series of nationwide Innovation Cafs, educator professional development, a suite of teacher resources, an Idealab, participation in national conferences, and specialized station relation and marketing. A summative evaluation of the MS2 project indicates that overall, these activities helped make a significant impact on the viewers, users, and participants that NOVA reached. The final evaluation conducted by Concord Evaluation Group (CEG) confidently concluded that the broadcast, website, and outreach activities were successful at achieving the projects intended impacts. CEG reported that the MS2 series and website content were successful in raising awareness and sparking interest in innovation, and increased public awareness that basic research leads to technological innovation; this interest was also sustained over a six month period. Efforts to create an online community of practice were also successful: the quality of collaboration increased, and community members felt supported while using Maker pedagogy. These findings provide clear evidence that large-scale science media projects like MS2 are an effective means of moving the needle on attitudes about and excitement for science. NOVAs broadcast audience and ratings have always indicated that a large portion of the population is interested in and engages with educational science media on a weekly basis. Yet these evaluation results provide the empirical evidence that beyond being capable of attracting, maintaining, and growing a dedicated group of citizens interested in science, these showswith their diverse content provided on a variety of media channelsare capable of sparking new interest in science, raising public awareness of the importance of science, and maintaining and growing that interest over time. In a country where approximately a quarter of the population doesnt know the earth rotates around the sun,1 roughly half still dont accept evolution,2 and about 20% dont think climate change is happening,3 the importance of these findings cannot be overstated. The success of MS2 suggests that large-scale media projects dedicated to and linked by coverage of scientific big ideas are an effective means of shifting public opinion onand improving understanding ofscience. REFERENCES 1, 2 National Science Foundation, Science and Engineering Indicators (2014). Chapter 7: Science and Technology: Public Attitudes and Understanding. 3 Leiserowitz, A., Maibach, E., Roser-Renouf, C., Feinberg, G., & Rosenthal, S. (2014) Climate change in the American mind: April, 2014. Yale University and George Mason University. New Haven, CT: Yale Project on Climate Change Communication.

  17. CPS Energy- New Commercial Construction Incentives

    Broader source: Energy.gov [DOE]

    CPS Energy offers incentives for new commercial construction that is at least 15% more efficient than required by the City of San Antonio Building Code (based on IECC 2009). The building code and...

  18. Alternative Energy Development Incentive (Corporate) (Utah)

    Broader source: Energy.gov [DOE]

    The Alternative Energy Development Incentive (AEDI) is a post-performance non-refundable tax credit for 75% of new state tax revenues (including, state, corporate, sales and withholding taxes) over...

  19. Commonwealth Wind Incentive Program Micro Wind Initiative

    Broader source: Energy.gov [DOE]

    Through the Commonwealth Wind Incentive Program Micro Wind Initiative the Massachusetts Clean Energy Center (MassCEC) offers rebates of up to $4/W with a maximum of $130,000 for design and...

  20. San Bernardino County- Green Building Incentive

    Broader source: Energy.gov [DOE]

    San Bernardino's Board of Supervisors launched Green County San Bernardino in August 2007. The program includes a number of incentives to encourage residents, builders, and businesses to adopt more...

  1. SMUD- Non-Residential PV Incentive Program

    Broader source: Energy.gov [DOE]

    SMUD offers cash incentives to commercial, industrial, and non-profit customers who install solar photovoltaic (PV) systems. Customers have the option of taking a one-time, up-front payment through...

  2. Austin Energy- Commercial PV Incentive Program

    Broader source: Energy.gov [DOE]

    Austin Energy, a municipal utility, offers a production incentive to its commercial and multi-family residential customers for electricity generated by qualifying photovoltaic (PV) systems of up to...

  3. SCE- New Construction Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    Southern California Edison offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new...

  4. Process Integration- What is the Incentive?

    E-Print Network [OSTI]

    Declercq, D.; Kaibel, G.

    PROCESS INTEGRATION - WHAT IS THE INCENTIVE? D. Declercq and G. Kaibel BASF Aktiengesellschaft? Ludwigshafen, West Germany ABSTRACT I. The optimization process The very fi rst flow sheet for a new plant arises when a number of unit operations...

  5. Arlington County- Green Building Incentive Program

    Broader source: Energy.gov [DOE]

    In October 1999, the County Board of Arlington adopted a Pilot Green Building Incentive Program using the standards established by the U. S. Green Building Councils Leadership in Energy and...

  6. PG&E- California Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    Pacific Gas and Electric (PG&E) offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new...

  7. Alternative Energy Development Incentive (Personal) (Utah)

    Broader source: Energy.gov [DOE]

    The Alternative Energy Development Incentive (AEDI) is a post-performance non-refundable tax credit for 75% of new state tax revenues (including, state, corporate, sales and withholding taxes) over...

  8. Clean Coal Incentive Tax Credit (Kentucky)

    Broader source: Energy.gov [DOE]

    Clean Coal Incentive Tax Credit provides for a property tax credit for new clean coal facilities constructed at a cost exceeding $150 million and used for the purposes of generating electricity....

  9. SDG&E- California Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    SDG&E offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new construction projects. A...

  10. Solar Volumetric Incentive and Payments Program

    Broader source: Energy.gov [DOE]

    '''''NOTE: Portland General Electric, PacifiCorp, and Idaho Power are now accepting applications for the volumetric incentive program. Subsequent re-openings will take place every six months until...

  11. Renewable Energy Tax Incentive Program (Texas)

    Broader source: Energy.gov [DOE]

    The Renewable Energy Tax Incentive Program provides various tax exemptions to businesses that either use or manufacture or install solar or wind energy. They can receive franchise tax deductions...

  12. Avista Utilities (Gas)- Prescriptive Commercial Incentive Program

    Broader source: Energy.gov [DOE]

    Avista Utilities offers Natural Gas saving incentives to commercial customers on rate schedule 420 and 424. This program provides rebates for a variety of equipment and appliances including cooking...

  13. Nova Biosource Fuels formerly Nova Energy Holding Inc | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca Agricola

  14. NOVA Portal: Submit VASP Jobs to Carver via the Web

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

    NOVA Portal: Submit VASP Jobs to Carver via the Web NOVA Portal: Submit VASP Jobs to Carver via the Web May 11, 2012 by Francesca Verdier (0 Comments) NOVA is an experimental web...

  15. Nova Produtiva | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca

  16. A Global Review of Incentive Programs to Accelerate Energy-Efficient Appliances and Equipment

    E-Print Network [OSTI]

    de la Rue du Can, Stephane

    2014-01-01T23:59:59.000Z

    DSIRE (Database of State Incentives for Renewable Energy).DSIRE (Database of State Incentives for Renewable Energy).2013. Database of State Incentives for Renewable Energy.

  17. Designing PV Incentive Programs to Promote System Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2006-01-01T23:59:59.000Z

    Washington Renewable Energy Production Incentives Cash BackSupport for Renewable Energy October 2006 Incentive-basedSupport for Renewable Energy October 2006 Incentive Hold-

  18. Dalhousie Medical School Cancer Researcher Seeks Biomarkers of Treatment Success HALIFAX,NOVA SCOTIA | CANADA B3H 4H7 | +1 (902) 494-2756

    E-Print Network [OSTI]

    Dellaire, Graham

    Dalhousie Medical School Cancer Researcher Seeks Biomarkers of Treatment Success HALIFAX for monitoring the effectiveness of cancer treatments. "Structures in the nucleus of every cell - known as PML. Their response to cancer therapies could tell us if treatment is working - within 24 hours, instead of weeks," he

  19. Text and slides of presentation originally presented to the Nova Scotia Utility and Review Board regarding the province's Demand Side Management program,19 April 2010.

    E-Print Network [OSTI]

    Hughes, Larry

    that affordable and available oil is becoming harder to obtain (Figure 2). Figure 2: World oil demand and prices); even offshore Newfoundland and Labrador (which meets about 26% of Atlantic Canada's crude oil demand As fuel oil prices rise, one can expect to see additional demand being put on the electrical system

  20. EIS-0339: Presidential Permit Application, GenPower 500 kV Submarine Electric Transmission Cable from Nova Scotia to New York

    Broader source: Energy.gov [DOE]

    The Department of Energy (DOE) announced its intent to prepare an Environmental Impact Statement (EIS) in accordance with the National Environmental Policy Act of 1969 (NEPA) for GenPower New York, L.L.C.s (GenPower) request for a Presidential permit for a proposed international electric transmission line.

  1. A 1600-year history of the Labrador Current off Nova Scotia Received: 11 June 2002 / Accepted: 3 January 2003 / Published online: 8 April 2003

    E-Print Network [OSTI]

    Sachs, Julian P.

    is one of the two main sources for the Labrador Current, warming and melting of ice caps in that region may have affected Labrador Current properties. Before this recent warming, sea surface temperature

  2. The NOvA Technical Design Report

    SciTech Connect (OSTI)

    Ayres, D.S.; Drake, G.R.; Goodman, M.C.; Grudzinski, J.J.; Guarino, V.J.; Talaga, R.L.; Zhao, A.; /Argonne; Stamoulis, P.; Stiliaris, E.; Tzanakos, G.; Zois, M.; /Athens U. /Caltech /UCLA /Fermilab /College de France /Harvard U. /Indiana U. /Lebedev Inst. /Michigan State U. /Minnesota U., Duluth /Minnesota U.

    2007-10-08T23:59:59.000Z

    Technical Design Report (TDR) describes the preliminary design of the NOvA accelerator upgrades, NOvA detectors, detector halls and detector sites. Compared to the March 2006 and November 2006 NOvA Conceptual Design Reports (CDR), critical value engineering studies have been completed and the alternatives still active in the CDR have been narrowed to achieve a preliminary technical design ready for a Critical Decision 2 review. Many aspects of NOvA described this TDR are complete to a level far beyond a preliminary design. In particular, the access road to the NOvA Far Detector site in Minnesota has an advanced technical design at a level appropriate for a Critical Decision 3a review. Several components of the accelerator upgrade and new neutrino detectors also have advanced technical designs appropriate for a Critical Decision 3a review. Chapter 1 is an Executive Summary with a short description of the NOvA project. Chapter 2 describes how the Fermilab NuMI beam will provide a narrow band beam of neutrinos for NOvA. Chapter 3 gives an updated overview of the scientific basis for the NOvA experiment, focusing on the primary goal to extend the search for {nu}{sub {mu}} {yields} {nu}{sub e} oscillations and measure the sin{sup 2}(2{theta}{sub 13}) parameter. This parameter has not been measured in any previous experiment and NOvA would extend the search by about an order of magnitude beyond the current limit. A secondary goal is to measure the dominant mode oscillation parameters, sin{sup 2}(2{theta}{sub 23}) and {Delta}m{sub 32}{sup 2} to a more precise level than previous experiments. Additional physics goals for NOvA are also discussed. Chapter 4 describes the Scientific Design Criteria which the Fermilab accelerator complex, NOvA detectors and NOvA detector sites must satisfy to meet the physics goals discussed in Chapter 3. Chapter 5 is an overview of the NOvA project. The changes in the design relative to the NOvA CDR are discussed. Chapter 6 summarizes the NOvA design performance relative to the Design Criteria set out in Chapter 4. Chapter 7 presents the Work Breakdown Structure dictionary at Level 3 and the Milestone dictionary. Chapters 8 through 17 then take each Level 2 WBS element of the NOvA project and present each part of the design in more detail than the overview given in Chapter 5. Specific technical design criteria are delineated for each part of the project in addition to the scientific design criteria outlined in Chapter 4. Changes in the design since the NOvA CDR are discussed in detail. The work remaining to bring each part of this preliminary design to a final design is outlined. Appendix A is a guide to other NOvA Project documentation with links to those documents.

  3. Question of the Week: Do Energy-Related Financial Incentives...

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

    Do Energy-Related Financial Incentives Prompt You to Be More Energy Efficient? Question of the Week: Do Energy-Related Financial Incentives Prompt You to Be More Energy Efficient?...

  4. The impact of financial incentives on firm behavior

    E-Print Network [OSTI]

    Matsa, David

    2006-01-01T23:59:59.000Z

    This dissertation analyzes the impact of various financial incentives on firm behavior. The first two chapters examine product-market and input-market effects of a firm's capital structure and the incentives they create. ...

  5. Incentive competitions as a policy tool for technological innovation

    E-Print Network [OSTI]

    Campbell, Georgina A. (Georgina Amy)

    2011-01-01T23:59:59.000Z

    Large incentive competitions are becoming increasingly popular amongst policymakers and philanthropists as a mission-orientated tool for inducing innovation, particularly in areas of national priority where market incentives ...

  6. Quantitative Financial Analysis of Alternative Energy Efficiency Shareholder Incentive Mechanisms

    E-Print Network [OSTI]

    Cappers, Peter

    2010-01-01T23:59:59.000Z

    Analysis of Alternative Energy Efficiency ShareholderAnalysis of Alternative Energy Efficiency Shareholderof alternative shareholder incentive mechanisms for energy

  7. Alternative fuel information: State alternative fuel laws and incentives

    SciTech Connect (OSTI)

    Not Available

    1994-06-01T23:59:59.000Z

    Laws and incentives related to the use of alternative fuels in automobiles are listed for most states of USA.

  8. Program Evaluation and Incentives for Administrators of Energy-Efficiency Programs: Can Evaluation Solve the Principal/Agent Problem?

    E-Print Network [OSTI]

    Blumstein, Carl

    2009-01-01T23:59:59.000Z

    Schmalensee, Incentive regulation for electric utilities. are proponents of incentive regulation, are nonetheless wary

  9. WORKING PAPER N 2010 -04 Senior activity rate, retirement incentives

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    Blake Marc Sangnier JEL Codes: Z10, J14, J22 Keywords: Early retirement incentives, labor relations trust. JEL Codes: Z10, J14, J22 Keywords: Early retirement incentives, labor relations, seniors activityWORKING PAPER N 2010 - 04 Senior activity rate, retirement incentives and labor relations Hlne

  10. Agricultural Research for Development Innovations & Incentives

    E-Print Network [OSTI]

    Agricultural Research for Development Innovations & Incentives The Swedish research network Agricultural Research for Development (Agri4D) organises an annual multi/inter-disciplinary and multi-stakeholder conference on agriculture, livestock and forest research in an international development context. Since

  11. Economic Development Incentive Programs: Some Best Practices

    E-Print Network [OSTI]

    Noble, James S.

    Economic Development Incentive Programs: Some Best Practices Judith I. Stallmann and Thomas G to be concerned about their ability to generate good returns to public investments. First, firms receiving. Johnson is Frank Miller Professor of Agricultural and Applied Economics, and Professor of Public Affairs

  12. Harvested Wood Products -an Incentive for Deforestation?

    E-Print Network [OSTI]

    Fischlin, Andreas

    1 Harvested Wood Products - an Incentive for Deforestation? Andreas Fischlin1 Abstract Mitigation for deforestation is real. To curb the disadvantages of HWP, some debiting of non-sustainable forest management activities are implemented that provide true disincentives to deforestation, HWP may continue to create some

  13. The database of state incentives for renewable energy: Utility programs and incentives report

    SciTech Connect (OSTI)

    Rogers, H.H. II; Shirley, L.E.; Reed, A.; Larsen, E.C.

    1999-07-01T23:59:59.000Z

    The past three decades saw the rapid development of renewable energy technologies and the concurrent evolution of state and federal financial and regulatory incentives, programs and policies to augment that development. Within the past two years, utility companies have created new incentives and programs that promote the use of renewable energy. Many of these incentives are in response to electric utility restructuring, while others are part of a broader corporate perspective that seeks to diversify into renewable energy generation, manage demand-side growth, or reap environmental benefits. This paper will present the current status of available utility incentives and programs throughout the united States as collected and databased by the Interstate Renewable Energy Council's (IREC) Database of State Incentives for Renewable Energy (DSIRE) project. Discussion will focus on putting the status of utility incentives programs into the context of the current restructuring movement, as well as how the DSIRE project can assist local, state, and national policy makers; industry, businesses and consumers; environmental and consumer advocates; and energy policy researchers.

  14. Energy Incentive Programs | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: Alternative FuelsNovember 13,Statement | DepartmentBlog2013Deployment ofEnergy ExchangeIncentive

  15. Incentives for demand-side management

    SciTech Connect (OSTI)

    Reid, M.W.; Brown, J.B. (Barakat and Chamberlin, Inc., Oakland, CA (United States))

    1992-01-01T23:59:59.000Z

    This report is the first product of an ongoing project to monitor the efforts of states to remove regulatory barriers to, and provide financial incentives for, utility investment in demand-side management (DSM) resources. The project was commissioned by the National Association of Regulatory Utility Commissioners (NARUC) in response to growing interest among regulators for a comprehensive survey of developments in this area. Each state report beings with an overview of the state's progress toward removing regulatory barriers and providing incentives for DSM. Information is organized under five headings: status; IRP regulations and practice; current treatment of DSM, directions and trends; commission contact person. Where applicable, each overview is followed by one or more sections that report on specific incentive proposals or mechanisms within the state. Information on each proposal or mechanism is organized under eight headings. A notation on each page identifies the utility or other group associated with the proposal or mechanism. The eight headings are as follows: status; background; treatment of cost recovery; treatment of lost revenues/decoupling; treatment of profitability; other features; issues, and additional observations.

  16. Incentives for demand-side management

    SciTech Connect (OSTI)

    Reid, M.W.; Brown, J.B. [Barakat and Chamberlin, Inc., Oakland, CA (United States)] [Barakat and Chamberlin, Inc., Oakland, CA (United States)

    1992-01-01T23:59:59.000Z

    This report is the first product of an ongoing project to monitor the efforts of states to remove regulatory barriers to, and provide financial incentives for, utility investment in demand-side management (DSM) resources. The project was commissioned by the National Association of Regulatory Utility Commissioners (NARUC) in response to growing interest among regulators for a comprehensive survey of developments in this area. Each state report beings with an overview of the state`s progress toward removing regulatory barriers and providing incentives for DSM. Information is organized under five headings: status; IRP regulations and practice; current treatment of DSM, directions and trends; commission contact person. Where applicable, each overview is followed by one or more sections that report on specific incentive proposals or mechanisms within the state. Information on each proposal or mechanism is organized under eight headings. A notation on each page identifies the utility or other group associated with the proposal or mechanism. The eight headings are as follows: status; background; treatment of cost recovery; treatment of lost revenues/decoupling; treatment of profitability; other features; issues, and additional observations.

  17. State Clean Energy Policies Analysis (SCEPA): State Tax Incentives

    SciTech Connect (OSTI)

    Lantz, E.; Doris, E.

    2009-10-01T23:59:59.000Z

    As a policy tool, state tax incentives can be structured to help states meet clean energy goals. Policymakers often use state tax incentives in concert with state and federal policies to support renewable energy deployment or reduce market barriers. This analysis used case studies of four states to assess the contributions of state tax incentives to the development of renewable energy markets. State tax incentives that are appropriately paired with complementary state and federal policies generally provide viable mechanisms to support renewable energy deployment. However, challenges to successful implementation of state tax incentives include serving project owners with limited state tax liability, assessing appropriate incentive levels, and differentiating levels of incentives for technologies with different costs. Additionally, state tax incentives may result in moderately higher federal tax burdens. These challenges notwithstanding, state tax incentives that consider certain policy design characteristics can support renewable energy markets and state clean energy goals.The scale of their impact though is directly related to the degree to which they support the renewable energy markets for targeted sectors and technologies. This report highlights important policy design considerations for policymakers using state tax incentives to meet clean energy goals.

  18. The Expanding Fireball of Nova Delphini 2013

    E-Print Network [OSTI]

    Schaefer, G H; Gies, D R; Farrington, C D; Kloppenborg, B; Chesneau, O; Monnier, J D; Ridgway, S T; Scott, N; Tallon-Bosc, I; McAlister, H A; Boyajian, T; Maestro, V; Mourard, D; Meilland, A; Nardetto, N; Stee, P; Sturmann, J; Vargas, N; Baron, F; Ireland, M; Baines, E K; Che, X; Jones, J; Richardson, N D; Roettenbacher, R M; Sturmann, L; Turner, N H; Tuthill, P; van Belle, G; von Braun, K; Zavala, R T; Banerjee, D P K; Ashok, N M; Joshi, V; Becker, J; Muirhead, P S

    2015-01-01T23:59:59.000Z

    A classical nova occurs when material accreting onto the surface of a white dwarf in a close binary system ignites in a thermonuclear runaway. Complex structures observed in the ejecta at late stages could result from interactions with the companion during the common envelope phase. Alternatively, the explosion could be intrinsically bipolar, resulting from a localized ignition on the surface of the white dwarf or as a consequence of rotational distortion. Studying the structure of novae during the earliest phases is challenging because of the high spatial resolution needed to measure their small sizes. Here we report near-infrared interferometric measurements of the angular size of Nova Delphini 2013, starting from one day after the explosion and continuing with extensive time coverage during the first 43 days. Changes in the apparent expansion rate can be explained by an explosion model consisting of an optically thick core surrounded by a diffuse envelope. The optical depth of the ejected material changes ...

  19. NUCLEAR MIXING METERS FOR CLASSICAL NOVAE

    SciTech Connect (OSTI)

    Kelly, Keegan J.; Iliadis, Christian; Downen, Lori; Champagne, Art [Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255 (United States); Jos, Jordi [Departament de Fsica i Enginyeria Nuclear, EUETIB, Universitat Politcnica de Catalunya, E-08036 Barcelona (Spain)

    2013-11-10T23:59:59.000Z

    Classical novae are caused by mass transfer episodes from a main-sequence star onto a white dwarf via Roche lobe overflow. This material possesses angular momentum and forms an accretion disk around the white dwarf. Ultimately, a fraction of this material spirals in and piles up on the white dwarf surface under electron-degenerate conditions. The subsequently occurring thermonuclear runaway reaches hundreds of megakelvin and explosively ejects matter into the interstellar medium. The exact peak temperature strongly depends on the underlying white dwarf mass, the accreted mass and metallicity, and the initial white dwarf luminosity. Observations of elemental abundance enrichments in these classical nova events imply that the ejected matter consists not only of processed solar material from the main-sequence partner but also of material from the outer layers of the underlying white dwarf. This indicates that white dwarf and accreted matter mix prior to the thermonuclear runaway. The processes by which this mixing occurs require further investigation to be understood. In this work, we analyze elemental abundances ejected from hydrodynamic nova models in search of elemental abundance ratios that are useful indicators of the total amount of mixing. We identify the abundance ratios ?CNO/H, Ne/H, Mg/H, Al/H, and Si/H as useful mixing meters in ONe novae. The impact of thermonuclear reaction rate uncertainties on the mixing meters is investigated using Monte Carlo post-processing network calculations with temperature-density evolutions of all mass zones computed by the hydrodynamic models. We find that the current uncertainties in the {sup 30}P(p, ?){sup 31}S rate influence the Si/H abundance ratio, but overall the mixing meters found here are robust against nuclear physics uncertainties. A comparison of our results with observations of ONe novae provides strong constraints for classical nova models.

  20. AN EXTENDED GRID OF NOVA MODELS. III. VERY LUMINOUS, RED NOVAE

    SciTech Connect (OSTI)

    Shara, Michael M.; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024-5192 (United States); Yaron, Ofer; Prialnik, Dina; Kovetz, Attay [Department of Geophysics and Planetary Sciences, Sackler Faculty of Exact Sciences, Tel Aviv University, Ramat Aviv 69978 (Israel)

    2010-12-10T23:59:59.000Z

    Extremely luminous, red eruptive variables like RV in M31 are being suggested as exemplars of a new class of astrophysical objects. Our greatly extended series of nova simulations shows that classical nova models can produce very red, luminous eruptions. In a poorly studied corner of three-dimensional nova parameter space (very cold, low-mass white dwarfs, accreting at very low rates) we find bona fide classical novae that are very luminous and red because they eject very slowly moving, massive envelopes. A crucial prediction of these nova models-in contrast to the predictions of merging star ('mergeburst') models-is that a hot remnant, the underlying white dwarf, will emerge after the massive ejected envelope has expanded enough to become optically thin. This blue remnant must fade on a timescale of decades-much faster than a 'mergeburst', which must fade on timescales of millennia or longer. Furthermore, the cooling nova white dwarf and its expanding ejecta must become redder in the years after eruption, while a contracting mergeburst must become hotter and bluer. We predict that red novae will always brighten to L {approx} 1000 L{sub sun} for about one year before rising to the maximum luminosity at L {approx} 10{sup 6}-10{sup 7} L{sub sun}. The maximum luminosity attainable by a nova is likely to be L {approx} 10{sup 7} L{sub sun}, corresponding to M {approx} -12. In an accompanying paper, we describe a fading, luminous blue candidate for the remnant of M31-RV; it is observed with the Hubble Space Telescope to be compatible only with the nova model.

  1. NoVaS Transformations: Flexible Inference for Volatility Forecasting

    E-Print Network [OSTI]

    Politis, Dimitris N; Thomakos, Dimitrios D

    2008-01-01T23:59:59.000Z

    NoVaS Transformations: Flexible Inference for VolatilityNoVaS Transformations: Flexible Inference for Volatility

  2. Applying Psychology to Economic Policy Design: Using Incentive Preserving Rebates to Increase Acceptance of Critical Peak Electricity Pricing

    E-Print Network [OSTI]

    Letzler, Robert

    2007-01-01T23:59:59.000Z

    by im- proving economic incentives. This project adds thatproblems by improving economic incentives. Insights abouta way to present good economic incentives that is IP rebates

  3. An Analysis of the Costs, Benefits, and Implications of Different Approaches to Capturing the Value of Renewable Energy Tax Incentives

    E-Print Network [OSTI]

    Bolinger, Mark

    2014-01-01T23:59:59.000Z

    the Value of Renewable Energy Tax Incentives Mark Bolingerthe value of renewable energy tax incentives in threegovernment incentives for renewable energy deployment. It

  4. Central Lincoln People's Utility District- Renewable Energy Incentive Program

    Broader source: Energy.gov [DOE]

    Central Lincoln People's Utility District provides financial incentives for its commercial and residential customers to install photovoltaic (PV), solar water heating, wind, and hydro electric...

  5. Federal Tax Incentives Encourage Alternative Fuel Use; Clean...

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

    on the Incentives and Laws section of the Alternative Fuels and Vehicles Data Center Web site at www.eere.energy.govafdcprogsfedsummaryphpafdcUS0. Please refer to this...

  6. Local Incentive-Based Policy for Vegetable-Agroforestry: alocally...

    Open Energy Info (EERE)

    Incentive-Based Policy for Vegetable-Agroforestry: a locally-appropriate adaptation and mitigation action (LAAMA) to climate change Jump to: navigation, search Tool Summary LAUNCH...

  7. Federal Tax Incentives for PV: Potential Implications for Program Design

    E-Print Network [OSTI]

    Wiser, Ryan; Bolinger, Mark

    2006-01-01T23:59:59.000Z

    Forthcoming. EPAct 2005s PV Tax Credits: What Are TheyAssumptions Installed PV system costs exhibit economies ofFederal Tax Incentives for PV Potential Implications for

  8. Structuring Rebate and Incentive Programs for Sustainable Demand...

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

    Peer Exchange Call: Structuring Rebate and Incentive Programs for Sustainable Demand, call slides and discussion summary, August 18, 2011. Call Slides and Discussion Summary More...

  9. Motivate Homeowner Action With Updated DOE Incentives Database...

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

    database includes a search tool that filters incentives and policies by type, state, technology, implementing sector, and eligible sector. DSIRE's latest improvements include:...

  10. NV Energy (Northern Nevada)- Solar Hot Water Incentive Program

    Broader source: Energy.gov [DOE]

    NV Energy is providing an incentive for its residential customers, small commercial, nonprofit, school and other public customers to install solar water heaters on their homes and facilities. ...

  11. Better Buildings: Financing and Incentives: Spotlight on Maine...

    Energy Savers [EERE]

    betterbuildings.energy.govneighborhoods 1 June 2012 Financing and Incentives Key Takeaways Maintain a base level of demand in the absence of rebates by providing mul-...

  12. New Generation Cooperative Incentive Tax Credit Program (Missouri)

    Broader source: Energy.gov [DOE]

    The Missouri Agricultural and Small Business Development Authority provides New Generation Cooperative Incentive Tax Credits to induce producer member investment into new generation processing...

  13. Central Lincoln People's Utility District- Renewable Energy Incentive Program (Oregon)

    Broader source: Energy.gov [DOE]

    Central Lincoln People's Utility District provides financial incentives for its commercial and residential customers to install photovoltaic (PV), solar water heating, wind, and hydro electric...

  14. Delmarva Power- Home Performance with Energy Star Incentive Program

    Broader source: Energy.gov [DOE]

    Delmarva Power and Light Company offers the Home Performance with Energy Star Program, which provides incentives for residential customers who have audits performed by participating contractors....

  15. Better Buildings: Financing and Incentives: Spotlight on Michigan...

    Energy Savers [EERE]

    betterbuildings.energy.govneighborhoods 1 Spotlight on Michigan: Experiment to Find the Right Mix of Incentives With support from the U.S. Energy Department's Better Buildings...

  16. Xcel Energy- Agriculture, Schools and Government Incentive Program

    Broader source: Energy.gov [DOE]

    Xcel Energy offers financial incentives toward energy efficient equipment installations including: Lighting, HVAC, Compressed Air, Refrigeration, VFDs, Information Systems and Renewables.

  17. Aligning Utility Incentives with Investment in Energy Efficiency...

    Open Energy Info (EERE)

    Aligning Utility Incentives with Investment in Energy Efficiency: A Resource of the National Action Plan for Energy Efficiency (United States) Jump to: navigation, search Tool...

  18. Cascade Natural Gas- Conservation Incentives for Existing Homes

    Broader source: Energy.gov [DOE]

    Cascade Natural Gas offers a variety of incentives to residential customers for making energy efficiency improvements to existing homes. Eligible equipment includes furnaces, water heaters,...

  19. City of San Francisco- Solar Energy Incentive Program

    Broader source: Energy.gov [DOE]

    The City and County of San Francisco, through the San Francisco Public Utilities Commission (SFPUC), are providing incentives to residents and businesses who install photovoltaic (PV) systems on...

  20. Ameren Illinois (Gas)- Cooking and Heating Business Efficiency Incentives

    Broader source: Energy.gov [DOE]

    Ameren Illinois offers several incentive programs that include efficient natural gas technologies. The programs are available only to non-residential customers that receive natural gas service from...

  1. PEPCO- Home Performance with Energy Star Incentive Program

    Broader source: Energy.gov [DOE]

    The Potomac Electric Power Company (PEPCO) offers the Home Performance with Energy Star Program which provides incentives for residential customers who have audits performed by participating...

  2. NOvA: Exploring Neutrino Mysteries

    SciTech Connect (OSTI)

    Vahle, Tricia; Messier, Mark

    2012-09-06T23:59:59.000Z

    Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers.

  3. NOvA: Exploring Neutrino Mysteries

    ScienceCinema (OSTI)

    Vahle, Tricia; Messier, Mark

    2014-08-12T23:59:59.000Z

    Neutrinos are a mystery to physicists. They exist in three different flavors and mass states and may be able to give hints about the origins of the matter-dominated universe. A new long-baseline experiment led by Fermilab called NOvA may provide some answers.

  4. CIRCUMSTELLAR SHELL FORMATION IN SYMBIOTIC RECURRENT NOVAE

    SciTech Connect (OSTI)

    Moore, Kevin; Bildsten, Lars [Department of Physics, Broida Hall, University of California, Santa Barbara, CA 93106 (United States)

    2012-12-20T23:59:59.000Z

    We present models of spherically symmetric recurrent nova shells interacting with circumstellar material (CSM) in a symbiotic system composed of a red giant (RG) expelling a wind and a white dwarf accreting from this material. Recurrent nova eruptions periodically eject material at high velocities ({approx}> 10{sup 3} km s{sup -1}) into the RG wind profile, creating a decelerating shock wave as CSM is swept up. High CSM densities cause the shocked wind and ejecta to have very short cooling times of days to weeks. Thus, the late-time evolution of the shell is determined by momentum conservation instead of energy conservation. We compute and show evolutionary tracks of shell deceleration, as well as post-shock structure. After sweeping up all the RG wind, the shell coasts at a velocity {approx}100 km s{sup -1}, depending on system parameters. These velocities are similar to those measured in blueshifted CSM from the symbiotic nova RS Oph, as well as a few Type Ia supernovae that show evidence of CSM, such as 2006X, 2007le, and PTF 11kx. Supernovae occurring in such systems may not show CSM interaction until the inner nova shell gets hit by the supernova ejecta, days to months after the explosion.

  5. Employee training, incentives boost conservation programs

    SciTech Connect (OSTI)

    Alejandro, C.

    1982-10-04T23:59:59.000Z

    Hotel energy managers are finding that a cooperative and trained staff is a major factor in the success of conservation projects. Some managers go beyond training to offer cash bonus and other incentives. Training must be continuous because of the high turnover in personnel. Most of the training is geared to increasing employee awareness of conservation basics, such as turning off lights, heat, and air conditioning. It is as important for employees to take a personal interest in the size of the utility bill as it is for them to understand the sophisticated control devices. (DCK)

  6. Energy Incentive Programs, Colorado | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFact SheetColorado Energy Incentive

  7. Energy Incentive Programs, Iowa | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowa Energy Incentive Programs,

  8. Energy Incentive Programs, Kansas | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowa Energy Incentive

  9. Energy Incentive Programs, Kentucky | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowa Energy IncentiveKentucky

  10. Energy Incentive Programs, Maine | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowa EnergyMaine Energy Incentive

  11. Energy Incentive Programs, Montana | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowaMontana Energy Incentive

  12. Energy Incentive Programs, Texas | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated June 2015 What

  13. Energy Incentive Programs, Utah | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated June 2015 WhatUtah

  14. Energy Incentive Programs, Vermont | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated June 2015

  15. Energy Incentive Programs, Virginia | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated June 2015Virginia

  16. Energy Incentive Programs, Washington | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated JuneWashington Energy

  17. Energy Incentive Programs, Wisconsin | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated

  18. Energy Incentive Programs, Wyoming | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas UpdatedWyoming Energy

  19. SES Awards and Incentives | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOrigin ofEnergy atLLC - FE DKT. 10-160-LNG - ORDER 2913 |DepartmentEECBGAwards and Incentives

  20. Washington/Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTri GlobalJump to: navigation, search Contents 1 Financial Incentive

  1. List of Boilers Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOf Kilauea Volcano,LakefrontLighthouse SolarI JumpListBoilers Incentives

  2. Montana/Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOfRose BendMiasole IncMinutemanVista Capital LLCMontana/Incentives <

  3. Tennessee/Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-f <Maintained ByManagement IncDrillbe nice ifTennessee/Incentives <

  4. Incentives and Policies | OpenEI Community

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup | OpenHunan Runhua New EnergyIT PowerImagine Energy IncInIncentives and

  5. Decentralization and Economic Incentives to Manage Groundwater Withdrawals for Irrigation: from Theory to

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    1 Decentralization and Economic Incentives to Manage Groundwater Withdrawals for Irrigation: from water management scenarios relying on four levers: economic incentives, transparency, negotiation, joint, in particular in the agricultural sector. This paper looks at possible institutional arrangements and incentive

  6. Ownership Change, Incentives and Plant Efficiency: The Divestiture of U.S. Electric Generation Plants

    E-Print Network [OSTI]

    Bushnell, James B.; Wolfram, Catherine

    2005-01-01T23:59:59.000Z

    that were subject to incentive regulation also saw fuel e?a strong form of incentive regulation. This suggests thata speci?c focus on incentive regulation. from the generation

  7. Ameren Illinois (Electric & Gas)- Multi-Family Properties Energy Efficiency Incentives

    Broader source: Energy.gov [DOE]

    The shell measure segment offers incentives for air sealing the shell of multifamily buildings. Incentives will be paid based on the total CFM reduction. Insulation incentives will be based on sq...

  8. Helping New Hampshire Achieve Its 25 x 25 Goal Renewable Energy Incentives, Energy Metering, and

    E-Print Network [OSTI]

    Lotko, William

    Helping New Hampshire Achieve Its 25 x 25 Goal Renewable Energy Incentives, Energy Metering................................................................................................................. 7 2. RENEWABLE ENERGY: FINANCING INCENTIVES......................................... 8 2.1 LOANS............................................................ 12 3. RENEWABLE ENERGY: PRODUCTION INCENTIVES................................... 14 3.1 NET METERING

  9. OGLE Atlas of Classical Novae I. Galactic Bulge Objects

    E-Print Network [OSTI]

    Mroz, P; Poleski, R; Soszynski, I; Szymanski, M K; Pietrzynski, G; Wyrzykowski, L; Ulaczyk, K; Kozlowski, S; Pietrukowicz, P; Skowron, J

    2015-01-01T23:59:59.000Z

    Classical novae eruptions are possible sources of lithium formation and gamma-rays emission. The remnant systems of novae eruptions can also become Type Ia supernovae. The contribution of novae to these phenomena depends on nova rates that are not well established for the Galaxy. Here, we directly measure the Galactic bulge nova rate of $13.9 \\pm 2.6$ yr$^{-1}$. This measurement is much more accurate than any previous measurement of this kind thanks to multiple years of bulge monitoring by the OGLE survey. Our sample consists of 39 novae eruptions, $\\sim$1/3 of which are OGLE-based discoveries. The long-term monitoring allows us to not only measure the nova rate but also to study in detail the light curves of 39 eruptions and over 80 post-nova candidates. We measured orbital periods for 9 post-novae and 9 novae, in 14 cases we procured the first estimates. The OGLE survey is very sensitive to the frequently erupting recurrent novae. We did not found any object similar to M31 2008-12a, which erupts once a year...

  10. In this issue: New Tax Incentives for Land in Conservation

    E-Print Network [OSTI]

    Watson, Craig A.

    In this issue: New Tax Incentives for Land in Conservation Florida's Outstanding Tree Farmers Quantifies Economic Impact of Private, Working Forests New Longleaf Book for Landowners and Foresters Get Landowners and Resource Professionals Volume 16, No. 4 Spring 2010 New Tax Incentives for Land

  11. ANIMAL TRACING: BENEFITS IN CATTLE INDUSTRY AND PRIVATE INCENTIVES

    E-Print Network [OSTI]

    McCarl, Bruce A.

    AND PRIVATE INCENTIVES The economic implications of foreign animal diseases and their mitigation options haveANIMAL TRACING: BENEFITS IN CATTLE INDUSTRY AND PRIVATE INCENTIVES LEVAN ELBAKIDZE Assistant Research Professor Department of Agricultural Economics Texas A&M University College Station, TX, 77843

  12. Economic changes and afforestation incentives in rural China Sylvie Dmurger

    E-Print Network [OSTI]

    Boyer, Edmond

    1 Economic changes and afforestation incentives in rural China Sylvie Dmurger HIEBS of this paper is to examine the forces that shape the afforestation incentives of rural economic agents and Economics (Beijing) Corresponding author: Sylvie Dmurger HK Institute of Economics & Business Strategy

  13. Mortality transition and differential incentives for early retirement

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    Mortality transition and differential incentives for early retirement Hippolyte d'Albis Sau for early retirement; years- to-consume effect; lifetime human wealth effect We are grateful to Robert. In this article, we continue this line of inquiry by studying the differential incentives for early retirement

  14. Designing PV Incentive Programs to Promote System Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2006-01-01T23:59:59.000Z

    Dan. 2006. Best Practices in PV Rebate Programs: Helpingprogram staff. Designing PV Incentive Programs to PromoteGroup), Mike Taylor Designing PV Incentive Programs to

  15. Country Review of Energy-Efficiency Financial Incentives in the Residential Sector

    E-Print Network [OSTI]

    Can, Stephane de la Rue du

    2011-01-01T23:59:59.000Z

    Financial Incentives in the Residential Sector Stephane deFinancial Incentives in the Residential Sector Stephane desavings achieved in the residential sector. In contrast,

  16. Microsoft PowerPoint - Wayne_Shirley_Overview_of_Incentives2008...

    Office of Environmental Management (EM)

    Utility Incentives Presentation to the Kansas Corporation Commission E Effi i I i W k h Energy Efficiency Incentives Workshop August 26, 2008 Presented by The Regulatory Assistance...

  17. Financial Analysis of Incentive Mechanisms to Promote Energy Efficiency: Case Study of a Prototypical Southwest Utility

    E-Print Network [OSTI]

    Cappers, Peter

    2009-01-01T23:59:59.000Z

    costs. Energy Efficiency Incentives Analysis risks of under-Shareholder Risk/Reward Incentive Mechanism for Energyof the energy efficiency effort and the risk to the utility

  18. Very high energy gamma-ray follow-up observations of novae and dwarf novae with the MAGIC telescopes

    E-Print Network [OSTI]

    Sitarek, J; Lopez-Coto, R; Wilhelmi, E de Ona; Desiante, R; Longo, F; Hays, E

    2015-01-01T23:59:59.000Z

    In the last few years the Fermi -LAT instrument has detected GeV gamma-ray emission from a few novae. Such GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. It is expected that hadrons can be accelerated in the same conditions, but reaching much higher energies. They can produce a second component in the gamma-ray spectrum at TeV energies. We performed follow-up observations of selected novae and dwarf novae in a search of the second component in the gamma-ray spectrum. This can shed light on the acceleration process of leptons and hadrons in nova explosions. We have performed observations with the MAGIC telescopes of 3 sources, a symbiotic nova YY Her, a dwarf nova ASASSN-13ax and a classical nova V339 Del shortly after their outbursts.

  19. Program Evaluation and Incentives for Administrators of Energy-Efficiency Programs: Can Evaluation Solve the Principal/Agent Problem?

    E-Print Network [OSTI]

    Blumstein, Carl

    2009-01-01T23:59:59.000Z

    the Commissions Energy Efficiency Risk/Reward IncentiveShareholder Risk/Reward Incentive Mechanism for Energy

  20. SALT observations of southern post-novae

    E-Print Network [OSTI]

    Tomov, T; Mikolajewski, M; Ilkiewicz, K

    2015-01-01T23:59:59.000Z

    We report on recent optical observations of the stellar and the nebular remnants of 22 southern post-novae. In this study, for each of our targets, we obtained and analysed long-slit spectra in the spectral range 3500-6600 A and in H$\\alpha$+NII narrow-band images. The changes in the emission lines' equivalent widths with the time since the outburst agree with earlier published results of other authors. We estimated an average value $\\alpha$=2.37 for the exponent of the power law fitted to the post-novae continua. Our observations clearly show the two-component structure of the V842 Cen expanding nebulae, owing to the different velocities of the ejected matter. We discovered an expanding shell around V382 Vel with an outer diameter of about 12 arcsec.

  1. Hubble Space Telescope Observations of Novae in M49

    E-Print Network [OSTI]

    Laura Ferrarese; Patrick Cote; Andres Jordan

    2003-09-30T23:59:59.000Z

    A search for novae in M49 (NGC 4472) has been undertaken with the Hubble Space Telescope. A 55-day observing campaign in F555W (19 epochs) and F814W (five epochs) has led to the discovery of nine novae. We find that M49 may be under-abundant in slow, faint novae relative to the Milky Way and M31. Instead, the decline rates of the M49 novae are remarkably similar to those of novae in the LMC. This fact argues against a simple classification of novae in "bulge" and "disk" sub-classes. We examine the Maximum-Magnitude versus Rate of Decline (MMRD) relation for novae in M49, finding only marginal agreement with the Galactic and M31 MMRD relations. A recalibration of the Buscombe-de Vaucouleurs relation gives an absolute magnitude 15 days past maximum of M_{V,15} = -6.36+/-0.19, which is substantially brighter than previous calibrations based on Galactic novae. Monte Carlo simulations yield a global nova rate for M49 of 100{+35}{-30} per year, and a luminosity-specific nova rate in the range \

  2. The SuperNova Early Warning System

    E-Print Network [OSTI]

    K. Scholberg

    2008-03-04T23:59:59.000Z

    A core collapse in the Milky Way will produce an enormous burst of neutrinos in detectors world-wide. Such a burst has the potential to provide an early warning of a supernova's appearance. I will describe the nature of the signal, the sensitivity of current detectors, and SNEWS, the SuperNova Early Warning System, a network designed to alert astronomers as soon as possible after the detected neutrino signal.

  3. The SuperNova Early Warning System

    E-Print Network [OSTI]

    Scholberg, K

    2008-01-01T23:59:59.000Z

    A core collapse in the Milky Way will produce an enormous burst of neutrinos in detectors world-wide. Such a burst has the potential to provide an early warning of a supernova's appearance. I will describe the nature of the signal, the sensitivity of current detectors, and SNEWS, the SuperNova Early Warning System, a network designed to alert astronomers as soon as possible after the detected neutrino signal.

  4. Nova power systems: status and operating experience

    SciTech Connect (OSTI)

    Whitham, K.; Merritt, B.T.; Gritton, D.G.; Smart, A.J.; Holloway, R.W.; Oicles, J.A.

    1983-11-28T23:59:59.000Z

    This paper describes the pulse power systems that are used in these lasers; the status and the operating experiences. The pulsed power system for the Nova Laser is comprised of several distinct technology areas. The large capacitor banks for driving flashlamps that excite the laser glass is one area, the fast pulsers that drive pockels cell shutters is another area, and the contol system for the pulsed power is a third. This paper discusses the capacitor banks and control systems.

  5. Novas Descobertas sobre o Sistema Solar

    E-Print Network [OSTI]

    dos Santos, C.A.

    Novas Descobertas sobre o Sistema Solar FIS 2009 Explorando o Universo: dos Quarks aos Quasares da temperatura da Terra A forma do espectro solar (máximo de emissão no visível) também é muito energia para a Terra, a Terra está em equilíbrio radioactivo com o Sol, este é um dos fatores

  6. Pumped profiles of ammonium and chlorophyll fluorescence from the upper 120 meters of the western Gulf of Mexico and the southwest Scotia Sea

    E-Print Network [OSTI]

    Johnson, Mark Andrew

    1981-01-01T23:59:59.000Z

    the depth of the 15 isotherm and approximate centers of anticyclonic feature (Station Alpha) and cyclonic feature (Station Bravo), denoted by H and L, respectively. Stars mark deployment of the parachute drogued surface buoys tracked for diel pumped...) and chlorophyll (lower trace) and region of 50 kHz. acoustic scattering. 25 Cumulative vertical structure index for Scotia Sea pumped profile 474. 27 FI GURE PAGE 10. Temperature fine structure during pumped vertical profiles, Station Alpha, Western Gulf...

  7. Getting to know Classical Novae with Swift

    E-Print Network [OSTI]

    Osborne, Julian P

    2015-01-01T23:59:59.000Z

    Novae have been reported as transients for more than two thousand years. Their bright optical outbursts are the result of explosive nuclear burning of gas accreted from a binary companion onto a white dwarf. Novae containing a white dwarf close to the Chandrasekhar mass limit and accreting at a high rate are potentially the unknown progenitors of the type Ia supernovae used to measure the acceleration of the Universe. Swift X-ray observations have radically transformed our view of novae by providing dense monitoring throughout the outburst, revealing new phenomena in the super-soft X-rays from the still-burning white dwarf such as early extreme variability and half- to one-minute timescale quasi-periodic oscillations. The distinct evolution of this emission from the harder X-ray emission due to ejecta shocks has been clearly delineated. Soft X-ray observations allow the mass of the white dwarf, the mass burned and the mass ejected to be estimated. In combination with observations at other wavelengths, includi...

  8. Tax Credits, Rebates & Savings | Department of Energy

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

    Community Feed-in Tariff (Nova Scotia, Canada) The Community Feed-In Tariff Program (COMFIT) is designed to increase local ownership of small-scale energy projects in Nova Scotia....

  9. The national database of state incentives for renewable energy

    SciTech Connect (OSTI)

    Rogers, H.H. II; Shirley, L.E. [North Carolina State Univ., Raleigh, NC (United States). North Carolina Solar Center

    1996-11-01T23:59:59.000Z

    In late 1995, the US Department of Energy initiated a new program through the Interstate Renewable Energy Council to survey each of the 50 states for available information on financial and regulatory incentives that are designed to promote the application of renewable energy technologies. This information is being developed into a database, reports prepared and printed which detail the incentives on a state-by-state basis, and access provided to much of the database via the Internet. By providing this information on a wide basis, it will be much easier for other states to get the information needed to analyze and replicate successful incentives in their own states.

  10. On the definition of stochastic -transducers1 Stavros Konstantinidis2

    E-Print Network [OSTI]

    and Computing Science Saint Mary's University Halifax, Nova Scotia B3H 3C3, Canada s.konstantinidis@smu

  11. ccpi-petra nova | netl.doe.gov

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

    ccpi-petra nova Industrial Carbon Capture and Storage Clean Coal Power Initiative Power Plant Improvement Initiative Clean Coal Technology Demonstration Program FutureGen Petra...

  12. Cutting Residential, Commercial, and Industrial Energy Use: Tools and Incentives that Work

    Broader source: Energy.gov [DOE]

    Cutting Residential, Commercial, and Industrial Energy Use: Tools and Incentives that Work Presentation

  13. Designing Effective Incentives to Drive Residential Retrofit Program Participation (Text Version)

    Broader source: Energy.gov [DOE]

    Transcript of the webinar, "Designing Effective Incentives to Drive Residential Retrofit Program Participation."

  14. Wireless Network Coding: Analysis, Control Mechanisms, and Incentive Design

    E-Print Network [OSTI]

    Hsu, Yu-Pin

    2014-05-08T23:59:59.000Z

    by developing novel network controllers, packet schedulers, and incentive mechanisms that would encourage the clients to collaborate and contribute resources to the information transfer. Our contributions can be broadly divided into three research thrusts: (1...

  15. Fact #788: July 15, 2013 State and Private Consumer Incentives...

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

    for Residents with a Separate Meter for PEV Charging AK, AL, AZ, CA, GA, HI, IN, KY, MI, MN, NV, TX, VA Charging EquipmentInstallation Incentive AZ, CA, CO, IL, IN, MD, MI, TN,...

  16. City of Phoenix- Energize Phoenix Commercial Incentives (Arizona)

    Broader source: Energy.gov [DOE]

    Through a partnership with Arizona State University and Arizona Public Service (APS), the City of Phoenix is providing incentives for businesses located along a 10-mile stretch of the Metro light...

  17. The Role of Incentives in Promoting CHP Development

    E-Print Network [OSTI]

    Kaufman, N.; Elliot, R. N.

    2010-01-01T23:59:59.000Z

    Conventional wisdom suggests that financial incentives should be sufficient to spur the installation of combined heat and power (CHP) systems. However, the states with the most CHP development are often not the states with the most generous...

  18. ConEd (Gas)- Residential Energy Efficiency Incentives Program

    Broader source: Energy.gov [DOE]

    Con Edison is offering the Residential HVAC Gas Rebate Program. Through this program, incentives are offered on energy efficient heating and cooling equipment for residences in the eligible service...

  19. Impact of Direct Financial Incentives in the Emerging Battery...

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

    2013 Percent of Registered BEVs Through 2013 Nissan Leaf December 2010 38,841 56 Tesla Model S June 2012 19,275 28 Source: R.L. Polk data 4 Project Scope Incentives offered...

  20. LADWP- Non-Residential Energy Efficiency Incentive Program

    Broader source: Energy.gov [DOE]

    Los Angeles Department of Water and Power offers prescriptive and custom incentives to non-residential customers for the installation of energy saving measures, equipment, or systems that exceed...

  1. Home Performance with Energy Star High Efficiency Measure Incentive (HEMI)

    Broader source: Energy.gov [DOE]

    The New York State Research and Development Authority (NYSERDA) offers an incentive for homeowners of 1-4 homes that participate in the Home Performance with Energy Star program. The program...

  2. NV Energy (Southern Nevada)- Solar Hot Water Incentive Program

    Broader source: Energy.gov [DOE]

    NV Energy is providing an incentive for its residential customers to install solar water heaters on their homes. As of July 26, 2013, NV Energy electric customers in Southern Nevada who own their...

  3. U.S. Department of Defense's Rebates and Incentives Regulations

    Broader source: Energy.gov [DOE]

    Presentationgiven at the Spring 2009 Federal Utility Partnership Working Group (FUPWG) meetingcovers the U.S. Department of Defense's (DoD's) statuatory authority and financial management regulation for rebates and incentives.

  4. INCENTIVES FOR ACCURACY IN ANALYST RESEARCH Patricia CRIFO

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    and ethical concerns. The recent scandals in Wall Street research that followed the bursting of the dot-com bubble has led to an examination of the perverse role of analysts incentives in providing biased research

  5. Oklahoma Local Development and Enterprise Zone Incentive Leverage Act (Oklahoma)

    Broader source: Energy.gov [DOE]

    The Oklahoma Local Development and Enterprise Zone Incentive Leverage Act provides funding for local units of government to match local tax revenue dedicated to support a project located in an...

  6. Short & long run transmission incentives for generation location

    E-Print Network [OSTI]

    Turvey, Ralph

    2006-01-01T23:59:59.000Z

    This paper is about one aspect of Britain's electricity trading system, its advantages and its weaknesses concerning the incentives it provides or fails to provide for the location of generation. (Similar considerations ...

  7. Small Employer Quality Jobs 7-Year Cash Incentive (Oklahoma)

    Broader source: Energy.gov [DOE]

    This program provides incentive payments to a qualifying small employer (90 employees or less). The payments may reach as high as 5% of new taxable payroll and last for up to seven years. Annual...

  8. Cost Bases for Incentive Rates Applicable to Industrial Loads

    E-Print Network [OSTI]

    Stover, C. N.

    1987-01-01T23:59:59.000Z

    Incentive rates applicable to industrial customers are presently receiving a great deal of attention and increased acceptance. This represents a substantial change in attitude, particularly on the part of the ...

  9. Alliant Energy Interstate Power and Light- New Home Construction Incentives

    Broader source: Energy.gov [DOE]

    Interstate Power and Light's New Home Program gives incentives to builders and contractors who build energy efficient homes. A base rebate is available to those customers that make the minimum...

  10. SoCalGas- New Construction Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    SoCalGas offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new construction projects. A...

  11. SDG&E- New Construction Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    SDG&E offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new construction projects. A...

  12. Incentive Cost Recovery Rule for Nuclear Power Generation (Louisiana)

    Broader source: Energy.gov [DOE]

    The Incentive Cost Recovery Rule for Nuclear Power Generation establishes guidelines for any utility seeking to develop a nuclear power plant in Louisiana. The rule clarifies, as well as...

  13. Letting Down the Team? Social Effects of Team Incentives

    E-Print Network [OSTI]

    Babcock, Philip; Bedard, Kelly; Charness, Gary; Hartman, John; Royer, Heather

    2012-01-01T23:59:59.000Z

    incentives with a much larger bonus payment contingent onincentive, the awarding of the bonus was dependent on bothdefaults, no one earns the bonus. 7 While this may seem less

  14. Small Scale CHP and Fuel Cell Incentive Program (New Jersey)

    Broader source: Energy.gov [DOE]

    The New Jersey Clean Energy Program (NJCEP) offers incentives for several types of small combined heat and power (CHP) and fuel cell systems that have a generating capacity of 1 MW or less and are...

  15. Innovation incentives and competition in the hard disk drive industry

    E-Print Network [OSTI]

    Wu, Xiaohua Sherry

    2011-01-01T23:59:59.000Z

    Firms in the hard disk drive industry are continually engaging in R & D and improving the quality of their products. We explore various determinants of the product innovation incentives for firms concerned with both their ...

  16. Sales Tax Incentives for Energy-Efficient Manufactured Homes

    Broader source: Energy.gov [DOE]

    In July 2008, [http://www.scstatehouse.gov/sess117_2007-2008/bills/1141.htm SB 1141] (known as the ''Energy-Efficient Manufactured Homes Incentive Program'') was enacted, which amended the sales...

  17. Lincoln County- LEED-Certified Building Incentive Program (North Carolina)

    Broader source: Energy.gov [DOE]

    Lincoln county is providing an incentive for the construction of certified green buildings in the commercial and industrial sector. Only newly constructed buildings are eligible, and they must have...

  18. Performance based incentive for Combined Heat and Power Program

    Broader source: Energy.gov [DOE]

    CHP technologies are eligible for either a grant, loan or power purchase incentive under the initial round of solicitations for new renewable energy generating equipment up to five megawatts at ...

  19. SoCalGas- California Advanced Homes Incentives

    Broader source: Energy.gov [DOE]

    SoCalGas offers an incentive for home builders to build homes which exceed 2008 Title 24 standards by 15%. The program is open to all single-family and multi-family new construction projects. A...

  20. Incentive zoning and environmental quality in Boston's Fenway neighborhood

    E-Print Network [OSTI]

    DeFlorio, Joshua (Joshua C.)

    2007-01-01T23:59:59.000Z

    A density bonus, also called incentive zoning, is a conditional liberalization of zoning regulations, allowing a real estate development to exceed as-of-right density limits in exchange for the in-kind provision or purchase ...

  1. NW Natural (Gas)- New Homes Stand Alone Incentive Program

    Broader source: Energy.gov [DOE]

    Builders with new construction projects in NW Naturals Washington gas service territory are eligible to receive cash incentives from Energy Trust of Oregon for gas heated homes that receive Energy...

  2. SRP- EarthWise Solar Energy Incentive Program

    Broader source: Energy.gov [DOE]

    '''''NOTE: SRP reopened its incentive programs effective May 1, 2013. SRP has funding available for 12 MW of residential photovoltaic (PV) systems, 4 MW of small commercial PV systems, 5 MW of...

  3. Hopkins Ultraviolet Telescope Observations of Nova Circini 1995 and Nova Aquilae 1995

    E-Print Network [OSTI]

    companion star undergoes a thermonuclear runaway. Accurate abundance information is important as a diagnostic of this thermonuclear runaway, and of the initial conditions which produce the runaway. Enhanced carbon, nitrogen, and oxygen (CNO) abundances are necessary in fast novae for thermonuclear runaway

  4. Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)

    E-Print Network [OSTI]

    Tajitsu, Akito; Naito, Hiroyuki; Arai, Akir; Aoki, Wako

    2015-01-01T23:59:59.000Z

    The origin of lithium (Li) and its production process have long been an unsettled question in cosmology and astrophysics. Candidates environments of Li production events or sites suggested by previous studies include big bang nucleosynthesis, interactions of energetic cosmic rays with interstellar matter, evolved low mass stars, novae, and supernova explosions. Chemical evolution models and observed stellar Li abundances suggest that at least half of the present Li abundance may have been produced in red giants, asymptotic giant branch (AGB) stars, and novae. However, no direct evidence for the supply of Li from stellar objects to the Galactic medium has yet been found. Here we report on the detection of highly blue-shifted resonance lines of the singly ionized radioactive isotope of beryllium, $^{7}$Be, in the near ultraviolet (UV) spectra of the classical nova V339 Del (Nova Delphini 2013). Spectra were obtained 38 to 48 days after the explosion. $^{7}$Be decays to form $^{7}$Li within a short time (half-li...

  5. Cost Bases for Incentive Rates Applicable to Industrial Loads

    E-Print Network [OSTI]

    Stover, C. N.

    great deal of attention and increased acceptance. This represents a substantial change in attitude, particularly on the part of the regulatory commissions; a few years ago any proposal related to an incentive type rate would not have been... in rate discrimination as between customer classes. Over the last few years many utilities have experienced changes that have resulted in increased interest in incentive rates by the utility, by its customer, and by the regulatory commission. In most...

  6. Some electric myths Larry Hughes

    E-Print Network [OSTI]

    Hughes, Larry

    . Two of these illustrate some of the common misconceptions regarding Nova Scotia Power's use of coal for Nova Scotia Power's decline in coal consumption. Nova Scotia Power's demand for coal started to decline. Since the start of this century, government regulations to reduce various coal-related emissions

  7. Some electric myths Larry Hughes

    E-Print Network [OSTI]

    Hughes, Larry

    is responsible for Nova Scotia Power's decline in coal consumption. Nova Scotia Power's demand for coal started. Since the start of this century, government regulations to reduce various coal-related emissions Power's declining demand for coal. For example, in 2007, Nova Scotia Power produced 9,561 GWh (gigawatt

  8. Spectra Nova Technologies Inc | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt LtdShawangunk,Southeast Colorado PowerSouthwesternCompaniesSES JumpSpectra Nova

  9. Api Nova Energia Srl | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof EnergyInnovation in Carbon Capture and SequestrationAnemoiAnokaApi Nova Energia Srl

  10. Incentive Pass-through for Residential Solar Systems in California

    Broader source: Energy.gov [DOE]

    The deployment of solar photovoltaic (PV) systems has grown rapidly over the last decade, partly because of various government incentives. In the United States, those established in California are among the largest and longest-running incentives. Building on past research, this report addresses the still-unanswered question: to what degree have the direct PV incentives in California been passed along from installers to consumers? This report addresses this question by carefully examining the residential PV market in California and applying both a structural-modeling approach and a reduced-form regression analysis to estimate the incentive pass-through rate. The results suggest an average pass-through rate of direct incentives of nearly 100%, but with regional differences among California counties. While these results could have multiple explanations, they suggest a relatively competitive market and well-functioning subsidy program. Further analysis is required to determine whether similar results broadly apply to other states, to other customer segments, to all third-party-owned PV systems, or to all forms of financial incentives for solar.

  11. Quantitative Financial Analysis of Alternative Energy Efficiency Shareholder Incentive Mechanisms

    SciTech Connect (OSTI)

    Cappers, Peter; Goldman, Charles; Chait, Michele; Edgar, George; Schlegel, Jeff; Shirley, Wayne

    2008-08-03T23:59:59.000Z

    Rising energy prices and climate change are central issues in the debate about our nation's energy policy. Many are demanding increased energy efficiency as a way to help reduce greenhouse gas emissions and lower the total cost of electricity and energy services for consumers and businesses. Yet, as the National Action Plan on Energy Efficiency (NAPEE) pointed out, many utilities continue to shy away from seriously expanding their energy efficiency program offerings because they claim there is insufficient profit-motivation, or even a financial disincentive, when compared to supply-side investments. With the recent introduction of Duke Energy's Save-a-Watt incentive mechanism and ongoing discussions about decoupling, regulators and policymakers are now faced with an expanded and diverse landscape of financial incentive mechanisms, Determining the 'right' way forward to promote deep and sustainable demand side resource programs is challenging. Due to the renaissance that energy efficiency is currently experiencing, many want to better understand the tradeoffs in stakeholder benefits between these alternative incentive structures before aggressively embarking on a path for which course corrections can be time-consuming and costly. Using a prototypical Southwest utility and a publicly available financial model, we show how various stakeholders (e.g. shareholders, ratepayers, etc.) are affected by these different types of shareholder incentive mechanisms under varying assumptions about program portfolios. This quantitative analysis compares the financial consequences associated with a wide range of alternative incentive structures. The results will help regulators and policymakers better understand the financial implications of DSR program incentive regulation.

  12. Database of State Incentives for Renewable Energy (DSIRE) Program

    SciTech Connect (OSTI)

    Jane M. Weissman, Executive Director

    2002-11-14T23:59:59.000Z

    OAK - B135 Advancement in the use of renewable energy over the past decade is due, in part, to progress in coordinating renewable energy policies, programs and initiatives across all governmental levels and all sectors of business. Through recent efforts by IREC?s DSIRE project, information on existing federal, state, local, and utility programs and incentives has been easier for the general public and government agencies to access and, as a result, use of these programs is beginning to increase. Increasing awareness of incentives can directly and positively impact the use of renewable energy. The DSIRE project?s primary objective, therefore, is to provide a single resource for all available incentive programs. Information produced by DSIRE is of increasing value to an audience of: State and local energy offices and regulatory agencies that may be considering new programs or initiatives, or extensions and expansions of past programs; State regulatory agencies or utility commissions that have approval or influence over the creation of regulatory incentives; Utility companies who may be considering the creation of new programs and incentives for renewable energy; Consumers, businesses, and renewable energy industries that need timely information on such incentives for purchasing and business planning; Schools and youth activity organizations seeking exciting and innovative applications of science and technology; and Renewable energy, environmental and consumer organizations actively promoting the utilization of renewable energy technologies.

  13. Petra Nova Project Breaks Ground on World's Largest Post-Combustion...

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

    Petra Nova Project Breaks Ground on World's Largest Post-Combustion Carbon Capture Project Petra Nova Project Breaks Ground on World's Largest Post-Combustion Carbon Capture...

  14. New findings show some Type Ia supernovae linked to novae | EurekAlert! Science News

    E-Print Network [OSTI]

    ... findings show some Type Ia supernovae linked to novae ... least some thermonuclear (Type Ia) supernovae come from a recurrent nova ... originators of other Type Ia supernovae . ...

  15. Cimpor inventa nova frmula para reduzir pegada de CO2

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    Cimpor inventa nova frmula para reduzir pegada de CO2 CIMENTO. A Cimpor descobriu uma nova frmula para produzir ci- mento que lhe permitir reduzir a pegada de CO 2 em 25%. Segundo as contas da as fbricas do grupo, seriam emitidos menos quatro milhes de toneladas de CO 2 por ano, o que permitiria uma

  16. Quark Nova Model for Fast Radio Bursts

    E-Print Network [OSTI]

    Zachary Shand; Amir Ouyed; Nico Koning; Rachid Ouyed

    2015-05-29T23:59:59.000Z

    FRBs are puzzling, millisecond, energetic radio transients with no discernible source; observations show no counterparts in other frequency bands. The birth of a quark star from a parent neutron star experiencing a quark nova - previously thought undetectable when born in isolation - provides a natural explanation for the emission characteristics of FRBs. The generation of unstable r-process elements in the quark nova ejecta provides millisecond exponential injection of electrons into the surrounding strong magnetic field at the parent neutron star's light cylinder via $\\beta$-decay. This radio synchrotron emission has a total duration of hundreds of milliseconds and matches the observed spectrum while reducing the inferred dispersion measure by approximately 200 cm$^{-3}$ pc. The model allows indirect measurement of neutron star magnetic fields and periods in addition to providing astronomical measurements of $\\beta$-decay chains of unstable neutron rich nuclei. Using this model, we can calculate expected FRB average energies ($\\sim$ 10$^{41}$ ergs), spectra shapes and provide a theoretical framework for determining distances.

  17. Analysis of federal incentives used to stimulate energy consumption

    SciTech Connect (OSTI)

    Cole, R.J.; Cone, B.W.; Emery, J.C.; Huelshoff, M.; Lenerz, D.E.; Marcus, A.; Morris, F.A.; Sheppard, W.J.; Sommers, P.

    1981-08-01T23:59:59.000Z

    The purpose of the analysis is to identify and quantify Federal incentives that have increased the consumption of coal, oil, natural gas, and electricity. The introductory chapter is intended as a device for presenting the policy questions about the incentives that can be used to stimulate desired levels of energy development. In the theoretical chapter federal incentives were identified for the consumption of energy as Federal government actions whose major intent or result is to stimulate energy consumption. The stimulus comes through changing values of variables included in energy demand functions, thereby inducing energy consumers to move along the function in the direction of greater quantity of energy demanded, or through inducing a shift of the function to a position where more energy will be demanded at a given price. The demand variables fall into one of six categories: price of the energy form, price of complements, price of substitutes, preferences, income, and technology. The government can provide such incentives using six different policy instruments: taxation, disbursements, requirements, nontraditional services, traditional services, and market activity. The four major energy forms were examined. Six energy-consuming sectors were examined: residential, commercial, industrial, agricultural, transportation, and public. Two types of analyses of incentive actions are presented in this volume. The generic chapter focused on actions taken in 1978 across all energy forms. The subsequent chapters traced the patterns of incentive actions, energy form by energy form, from the beginning of the 20th century, to the present. The summary chapter includes the results of the previous chapters presented by energy form, incentive type, and user group. Finally, the implications of these results for solar policy are presented in the last chapter. (MCW)

  18. Near-Infrared and Optical Studies of the fast nova V4643 Sgr (Nova Sagittarii 2001)

    E-Print Network [OSTI]

    N. M. Ashok; D. P. K. Banerjee; W. P. Varricatt; U. S. Kamath

    2006-02-07T23:59:59.000Z

    V4643 Sagittarii or Nova Sagittarii 2001 was discovered in outburst at 7.7 mag. on 2001 February 24. Here, we present near-infrared results of this fast classical nova obtained in the early decline phase in 2001 March followed by optical observations about one month later. Subsequently we also present near-infrared spectra taken later in the nova's evolution, about four months after the outburst, when V4643 Sgr had entered the coronal phase. The spectra in the early decline phase are dominated by emission lines of the HI Brackett series and also the Paschen beta and gamma lines. We study the cause of the excitation of the the OI line at 1.128 micron and discuss the variation in its strength with time after outburst. We discuss the role of optical depth effects on the observed strengths of the hydrogen Brackett and Paschen lines and discuss possible reasons for the puzzling behavior of the Br gamma line strength and whether it is correlated with the OI 1.128 micron line behavior. An optical spectrum is presented which shows that HeII lines are the most prominent features - after HI - to be seen in early 2001 April. We present and also discuss spectra taken in 2001 June and August which prominently show coronal lines of [Si VI] and [Si VII] at 1.9641 micron and 2.4807 micron respectively.

  19. State financial and regulatory incentives: Return of the power?

    SciTech Connect (OSTI)

    Rogers, H.H. II; Shirley, L.E. [North Carolina State Univ., Raleigh, NC (United States). North Carolina Solar Center

    1997-12-31T23:59:59.000Z

    The National Database of State Incentives for Renewable Energy (DSIRE) is an ongoing project of the Interstate Renewable Energy Council (IREC), and is managed by the North Carolina Solar Center with funding from the Office of Utility Technologies, US Department of Energy. This database serves as the nation`s one-stop source of information on the status of regulatory and financial incentives for renewable energy that are provided by state governments in the states and territories. Information on existing incentives is provided to industry, government officials, utilities, regulatory officials and the public through written reports, a world wide web site, and a database application on computer diskette. For additional information on DSIRE, contact the N.C. Solar Center: (919) 515-3480; fax: (919) 515-5778; email: ncsun{at}ncsu.edu; or http://www/ncsc.ncsu.edu/dsire.htm.

  20. A primer on incentive regulation for electric utilities

    SciTech Connect (OSTI)

    Hill, L.J.

    1995-10-01T23:59:59.000Z

    In contemplating a regulatory approach, the challenge for regulators is to develop a model that provides incentives for utilities to engage in socially desirable behavior. In this primer, we provide guidance on this process by discussing (1) various models of economic regulation, (2) problems implementing these models, and (3) the types of incentives that various models of regulation provide electric utilities. We address five regulatory models in depth. They include cost-of-service regulation in which prudently incurred costs are reflected dollar-for-dollar in rates and four performance-based models: (1) price-cap regulation, in which ceilings are placed on the average price that a utility can charge its customers; (2) revenue-cap regulation, in which a ceiling is placed on revenues; (3) rate-of-return bandwidth regulation, in which a utility`s rates are adjusted if earnings fall outside a {open_quotes}band{close_quotes} around equity returns; and (4) targeted incentives, in which a utility is given incentives to improve specific components of its operations. The primary difference between cost-of-service and performance-based approaches is the latter sever the tie between costs and prices. A sixth, {open_quotes}mixed approach{close_quotes} combines two or more of the five basic ones. In the recent past, a common mixed approach has been to combine targeted incentives with cost-of-service regulation. A common example is utilities that are subject to cost-of-service regulation are given added incentives to increase the efficiency of troubled electric-generating units.

  1. Distributed computer control system in the Nova Laser Fusion Test Facility

    SciTech Connect (OSTI)

    Not Available

    1985-09-01T23:59:59.000Z

    The EE Technical Review has two purposes - to inform readers of various activities within the Electronics Engineering Department and to promote the exchange of ideas. The articles, by design, are brief summaries of EE work. The articles included in this report are as follows: Overview - Nova Control System; Centralized Computer-Based Controls for the Nova Laser Facility; Nova Pulse-Power Control System; Nova Laser Alignment Control System; Nova Beam Diagnostic System; Nova Target-Diagnostics Control System; and Nova Shot Scheduler. The 7 papers are individually abstracted.

  2. Analysis of federal incentives used to stimulate energy production: an executive summary

    SciTech Connect (OSTI)

    Cone, B. W.; Brenchley, D. L.; Brix, V. L.; Brown, M. L.; Cochran, K. E.; Cohn, P. D.; Cole, R.J.; Curry, M. G.; R. Davidson, Easter1ing, J; Emery, J. C.; Fassbender, A. G.; Fattorini, Jr. J.S.; Gordon, B.; Harty, H.; Mazzucchi, R.; McClain, C; Morre, D. D.; Sheppard, E. J.; Solomon, S

    1980-02-01T23:59:59.000Z

    The purpose of this research was to analyze past and present federal incentives to production of various energy sources and thereby assist the Division of Conservation and Solar Applications, Department of Energy, in the study and recommendation of federal incentives for the development of solar energy. The research was divided into five parts: a survey of current thought about incentives for solar energy production; the theoretical approach to analyzing and characterizing incentives; a generic view of the energy incentive creating landscape for 1978; analysis of the major energy sources (nuclear, hydro, coal, electricity, oil, and gas) along their trajectories from exploration to waste management, including their costs in 1978 dollars; and insights into potential incentives for solar policy. Economic, political, organizational, and legal viewpoints were considered in formulating the typology of incentives. Eight types of incentives were identified.

  3. Relational Capital and Appropriate Incentives: A Recipe for Human Resource Sustainability?1

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    economic literature on incentives, experimental economics and research in cognitive psychology can provideRelational Capital and Appropriate Incentives: A Recipe for Human Resource Sustainability?1 Agns Festr University of Picardie Jules Verne, France Faculty of Economics Agnes

  4. Incentive Regulation in Theory and Practice: Electricity Distribution and Transmission Networks

    E-Print Network [OSTI]

    Joskow, Paul

    2006-03-14T23:59:59.000Z

    Modern theoretical principles to govern the design of incentive regulation mechanisms are reviewed and discussed. General issues associated with applying these principles in practice are identified. Examples of the actual application of incentive...

  5. Incentive Regulation of Electricity Distribution Networks: Lessons of Experience from Britain

    E-Print Network [OSTI]

    Jamasb, Tooraj; Pollitt, Michael G.

    This paper reviews the recent experience of the UK electricity distribution sector under incentive regulation. The UK has a significant and transparent history in implementing incentive regulation in the period since 1990. We demonstrate...

  6. Fermilab | Web Cams | NOvA Far Detector

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

    Follow us on: Facebook Twitter NOvA Far Detector Live Webcam Detector Hall Looking Downstream This text will be replaced View this full feed on Twitter @NOvANuz Twitter Feed...

  7. SNEWS: The SuperNova Early Warning System

    E-Print Network [OSTI]

    Antonioli, P

    2004-01-01T23:59:59.000Z

    This paper provides a technical description of the SuperNova Early Warning System (SNEWS), an international network of experiments with the goal of providing an early warning of a galactic supernova.

  8. SNEWS: The SuperNova Early Warning System

    E-Print Network [OSTI]

    P. Antonioli

    2004-07-30T23:59:59.000Z

    This paper provides a technical description of the SuperNova Early Warning System (SNEWS), an international network of experiments with the goal of providing an early warning of a galactic supernova.

  9. Federal Register Notice EPAct 2005 Section 242 Hydroelectric Incentive Program: January 2015

    Broader source: Energy.gov [DOE]

    Federal Register Notice for the EPAct 2005 Section 242 Hydroelectric Incentive Program application period announcement: January, 2015.

  10. Evaluating the Economic Impact of Film Production Incentives in South Carolina

    E-Print Network [OSTI]

    Almor, Amit

    Evaluating the Economic Impact of Film Production Incentives in South Carolina Prepared by Division (2008) February 2008 #12;Evaluating the Economic Impact of Film Production Incentives in South Carolina. #12;Evaluating the Economic Impact of Film Production Incentives in South Carolina, 2 This model

  11. Economic Incentives of Providing Network Security Services Journal of Information Technology Management 1

    E-Print Network [OSTI]

    Sadeh, Norman M.

    Economic Incentives of Providing Network Security Services Journal of Information Technology Management 1 THE ECONOMIC INCENTIVES OF PROVIDING NETWORK SECURITY SERVICES ON THE INTERNET INFRASTRUCTURE Li in the economic incentives inherent in providing the defenses as well as uncertainty in current defenses. We

  12. Managing Cellular Congestion Using Incentives Jagadeesh M. Dyaberi, Ben Parsons, Karthik Kannan, Vijay S. Pai,

    E-Print Network [OSTI]

    Greenberg, Albert

    . Our results indicate a high level of compliance with economic incentives and disincentives. Detailed/or punishments to help reduce network congestion. We found a high level of compliance with economic incentives several stud- ies on using economic incentives to help shape consumer behaviors towards more efficient use

  13. Optimum Inverter Sizing in Consideration of Irradiance Pattern and PV Incentives

    E-Print Network [OSTI]

    Lehman, Brad

    Optimum Inverter Sizing in Consideration of Irradiance Pattern and PV Incentives Song Chen* Peng Li for a PV system. The method evaluates effects of PV incentive policies, inverter efficiency curves, different scenarios of PV incentives are discussed and compared to show that the optimal inverter size

  14. City of Anaheim This page outlines solar PV incentives, financing mechanisms, permitting process, and

    E-Print Network [OSTI]

    a contract. Back to Top Financing Information Federal Solar Incentives o Residential Renewable Energy TaxCity of Anaheim This page outlines solar PV incentives, financing mechanisms, permitting process | Incentives | Permitting | Interconnection Contact Information City of Anaheim Building Division 200 S

  15. City of Los Angeles This page outlines solar PV incentives, financing mechanisms, permitting process, and

    E-Print Network [OSTI]

    Incentives o Residential Renewable Energy Tax Credit · A taxpayer may claim a credit of 30% of qualifiedCity of Los Angeles This page outlines solar PV incentives, financing mechanisms, permitting these hyperlinks: Find an Installer | Financing | Incentives | Permitting | Interconnection Contact Information

  16. COMPARING ALASKA'S OIL PRODUCTION TAXES: INCENTIVES AND ASSUMPTIONS1

    E-Print Network [OSTI]

    Pantaleone, Jim

    context of Alaska oil production taxes, comparing MAPA and ACES to the original petroleum profits tax (PPT1 COMPARING ALASKA'S OIL PRODUCTION TAXES: INCENTIVES AND ASSUMPTIONS1 Matthew Berman In a recent analysis comparing the current oil production tax, More Alaska Production Act (MAPA, also known as SB 21

  17. Location-Based Tax Incentives: Evidence From India Ritam Chaurey

    E-Print Network [OSTI]

    Bandyopadhyay, Antar

    in India. Specifically, I examine the federally financed New Industrial Policy for the statesLocation-Based Tax Incentives: Evidence From India Ritam Chaurey Department of Economics, State University of New York, Binghamton August 24, 2014 Abstract While policies targeting particular geographic

  18. Fuel Cell Tax Incentives: How Monetization Lowers the

    E-Print Network [OSTI]

    for electricity produced and sold by a qualified facility for a 5- or 10-year period. o Currently 2.1 cent or 1Fuel Cell Tax Incentives: How Monetization Lowers the Government Outlay By: Lee J. Peterson, Esq.48-9(a)(1). 5R G Building Business Value February 19, 2009 #12;How Do Tax Credits Minimize Government

  19. CSEM WP 140 Ownership Change, Incentives and Plant Efficiency

    E-Print Network [OSTI]

    Kammen, Daniel M.

    CSEM WP 140 Ownership Change, Incentives and Plant Efficiency: The Divestiture of U.S. Electric and Plant Efficiency: The Divestiture of U.S. Electric Generation Plants James B. Bushnell and Catherine efficiency from the Environmental Protection Agency's Continuous Emissions Monitoring System (CEMS

  20. Bringing Up Incentives: A Look at the Determinants of Poverty

    E-Print Network [OSTI]

    New Hampshire, University of

    Bringing Up Incentives: A Look at the Determinants of Poverty Alice Sheehan #12;Outline presentation What's going on out there? Growth, Human Development indicators, Poverty rates, etc. A look at determinants of poverty on three different levels: Immediate, Community, and Regional/National An example

  1. Hawaii Bioenergy Master Plan Financial Incentives And Barriers; And

    E-Print Network [OSTI]

    at levels sufficient to contribute a significant renewable energy resource to the State of HawaiHawaii Bioenergy Master Plan Financial Incentives And Barriers; And Other Funding Sources Prepared for: Hawai`i Natural Energy Institute University of Hawai`i at Manoa 1680 East West Road, POST 109

  2. Analysis of the results of Federal incentives used to stimulate energy production

    SciTech Connect (OSTI)

    Cone, B.W.; Emery, J.C.; Fassbender, A.G.

    1980-06-01T23:59:59.000Z

    The research program analyzed the Federal incentives used to stimulate nuclear, hydro, coal, gas, oil, and electricity production in order to supply what was learned to the selection of an incentives strategy to induce new energy production from renewable resources. Following the introductory chapter, Chapter 2 examines the problem of estimating effects from a theoretical perspective. Methods of quantifying and identifying the many interactive effects of government actions are discussed. Chapter 3 presents a generic analysis of the result of Federal incentives. Chapters 4 through 9 deal with incentives to energy forms - nuclear, hydro, coal, oil, gas, and electricity. Chapter 10 summarizes the estimated results of the incentives, which are presented in terms of their quantity and price impacts. The incentive costs per million Btu of induced energy production is also discussed. Chapter 11 discusses the parity issue, that is an equivalence between Federal incentives to renewable resources and to traditional energy resources. Any analysis of incentives for solar needs will profit from an analysis of the costs of solar incentives per million Btu compared with those for traditional energy forms. Chapter 12 concludes the analysis, discussing the history of traditional energy incentives as a guide to solar-energy incentives. 216 references, 38 figures, 91 tables.

  3. Acknowledgements: The author would like to thank his colleagues and associates for their assistance with this report.

    E-Print Network [OSTI]

    Hughes, Larry

    . All three replacement energy sources being promoted by the province face significant challenges: wind shortages and unstable energy prices. The purpose of the 2009 Energy Strategy was to help Nova Scotia meet with this report. ERG/200904 Nova Scotia's energy strategy: Energy security for Nova Scotians Response to The Nova

  4. Nova Bio Fuels Pvt Ltd | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca Agricola eNova

  5. Nova Chemicals Reliance Industries JV | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca AgricolaNova

  6. NOvA: Building a Next Generation Neutrino Experiment

    ScienceCinema (OSTI)

    Perko, John; Williams, Ron; Miller, Bill;

    2014-05-30T23:59:59.000Z

    The NOvA neutrino experiment is searching for the answers to some of the most fundamental questions of the universe. This video documents how collaboration between government research institutions like Fermilab, academia and industry can create one of the largest neutrino detectors in the world.

  7. Gamma-ray spectroscopy measurements for nuclear reactions in novae

    E-Print Network [OSTI]

    Lotay, Gavin James

    2009-01-01T23:59:59.000Z

    The 23Mg(p?)24Al and 26Al(p?)27Si astrophysical reactions are expected to be of considerable importance in the nucleosynthesis of A?20 nuclei in classical novae. Previous studies have indicated that both reactions are ...

  8. Incentive Thresholds, Risk-Taking, and Performance. Evidence from Hedge Funds

    E-Print Network [OSTI]

    Shelef, Orie

    2012-01-01T23:59:59.000Z

    term incentive plans. 2Taking Stock: Are Employee Optionspercentile of managers. 8Taking Stock: Are Employee OptionsCEO stock options on company risk-taking and performance.

  9. Designing PV Incentive Programs to Promote Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2007-01-01T23:59:59.000Z

    DESIGNING PV INCENTIVE PROGRAMS TO PROMOTE SYSTEMcustomer-sited photovoltaic (PV) systems, provided throughface to ensuring that their PV systems perform well, and the

  10. Alliant Energy Interstate Power and Light (Gas and Electric)- Farm Equipment Energy Efficiency Incentives

    Broader source: Energy.gov [DOE]

    Interstate Power and Light (Alliant Energy) offers prescriptive rebates for a variety of energy efficient products for agricultural customers. In addition to these incentives, IPL offers a Farm...

  11. Energy Smart Federal Partnership: Partnering to Provide Technical Assistance, Financial Incentives, and More

    Broader source: Energy.gov [DOE]

    Presentation covers technical and financial incentives for the Energy Smart Federal Partnership and is given at the Spring 2011 Federal Utility Partnership Working Group (FUPWG) meeting.

  12. Designing PV Incentive Programs to Promote System Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2006-01-01T23:59:59.000Z

    communication with New York State Energy Research andSolar Pioneer Program New York Energy $mart PV IncentivePower Authority (LIPA) New York State Energy Research and

  13. FirstEnergy (Mon Power & Potomac Edison)- Business Lighting Incentive Program

    Broader source: Energy.gov [DOE]

    FirstEnergy's commercial, industrial, and governmental customers are eligible to participate in the Business Lighting Incentive Program. This program provides a performance-based rebate for energ...

  14. Incentive drilling contracts; A logical approach for enhancement of drilling efficiency

    SciTech Connect (OSTI)

    Moomjian, C.A. Jr. (Santa Fe Drilling Co. (US))

    1992-03-01T23:59:59.000Z

    Incentive drilling contracts historically have been based on the footage and turnkey concepts. Because these concepts have not been used widely in the international and offshore arenas, this paper discusses other innovative approaches to incentive contracts. Case studies of recently completed or current international and offshore contracts are presented to describe incentive projects based on a performance bonus (Case 1), lump sum per well (Case 2), target time and cap for a specified hole section (Case 3), and per-well target time (Case 4). This paper concludes with a review and comparison of the case studies and a general discussion of factors that produce successful innovative incentive programs that enhance drilling efficiency.

  15. Incentives to stimulate solar energy use- a proceedings of the second Seattle workshop

    SciTech Connect (OSTI)

    Cole, R.J.; Cone, B.W.; Sheppard, W.J.; Sommers, P.; Marcus, A.; Lenerz, D.

    1981-06-01T23:59:59.000Z

    Nineteen papers are included. A separate abstract was prepared for each one. Summaries of workshop discussions on types of incentives are also included. (MHR)

  16. PHOTOMETRIC AND SPECTROSCOPIC PROPERTIES OF NOVAE IN THE LARGE MAGELLANIC CLOUD

    SciTech Connect (OSTI)

    Shafter, A. W. [Department of Astronomy, San Diego State University, San Diego, CA 92182 (United States)

    2013-05-15T23:59:59.000Z

    The photometric and spectroscopic properties of the 43 known LMC nova candidates are summarized and reviewed. Of these, photometric data sufficient to establish decline rates are available for 29 novae, while spectroscopic data sufficient to establish the spectroscopic classes are available for 18 systems. Half of the 18 novae belong to the Fe II class, with the remaining nine belonging to either the He/N or the Fe IIb classes. As seen in previous nova studies of M31 and M33, the He/N and Fe IIb novae have on average faster photometric developments than do their Fe II counterparts. Overall, the available photometry confirms earlier studies, and shows conclusively that LMC novae have faster rates of decline than do novae in the Galaxy and M31. It appears that the increased fraction of faster, He/N and Fe IIb novae observed in the LMC compared with M31 is almost certainly the result of differences in the underlying stellar population between the two galaxies. We propose that the younger population seen in the LMC compared with M31's bulge (where most of the novae are found), produces progenitor binaries with higher average white dwarf masses. The higher mean white dwarf mass not only produces a larger fraction of fast, He/N novae compared with M31, but also results in a relatively large recurrent nova population.

  17. Energy Incentive Programs, New York | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 Federal RegisterHydrogenDistributionFactIowaMontanaYork Energy Incentive

  18. Energy Incentive Programs, Washington DC | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated June

  19. Energy Incentive Programs, West Virginia | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube|6721 FederalTexas Energy Incentive Programs, Texas Updated JuneWashington

  20. List of Evaporative Coolers Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOf Kilauea Volcano,LakefrontLighthouseEvaporative Coolers Incentives Jump

  1. List of Food Service Equipment Incentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOf Kilauea Volcano,LakefrontLighthouseEvaporative Coolers Incentives

  2. List of Other Alternative Fuel Vehicles Incentives | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOf KilaueaInformation Other Alternative Fuel Vehicles Incentives Jump

  3. List of Other Distributed Generation Technologies Incentives | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOf KilaueaInformation Other Alternative Fuel Vehicles Incentives

  4. Buildings Energy Data Book: 7.2 Federal Tax Incentives

    Buildings Energy Data Book [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: Alternative Fuels Data Center HomeIdle Reduction WeightRebate -5 20054 Share of6351 Tax Incentives

  5. Alternative Fuels Data Center: Federal and State Laws and Incentives

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItem NotEnergy,ARMForms About BecomeTechnologies | BlandineNaturalEmergingIncentives

  6. Property:NumberOfIncentives | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere I Geothermal PwerPerkins County, Nebraska:PrecourtOidNumberOfCompanies Jump to: navigation,NumberOfIncentives

  7. Incentive program for energy efficient design of state buildings

    SciTech Connect (OSTI)

    Case, M.E.; Wingerden, J. [and others

    1998-07-01T23:59:59.000Z

    In 1996, the State of Utah instigated a pilot program intended to improve the energy efficiency of newly designed State buildings. The goal of the program was to show that buildings could be designed to be more energy efficient than the State's energy code, ASHRAE/IES 90.1, without adding to the construction costs. Four of the eight buildings beat the code by at least 50%; one by 40% and one by only 22%. One project is still in design. This paper summarizes the program's design, implementation and results through May 3, 1998. It presents an informal evaluation and discusses program highlights - both positive and negative. The difficulties--both technical and political--in using the ASHRAE Standard for Energy Efficient Design of New Buildings (ASHRAE/IES 90.1) in an incentive-based program are discussed. Possible solutions to specific problems are presented. The impact of incentives on the design teams, their methods and the resulting design are also discussed.

  8. Eliminating Software Task Overestimation Using Economic Game Theory to Create a Competitive Incentive System

    E-Print Network [OSTI]

    McGaughey, Alan

    Eliminating Software Task Overestimation Using Economic Game Theory to Create a Competitive Incentive System T.J. Glazier It is common for software engineers to overestimate the time to successfully is an organizational behavior that is the product of tangible penalties for being late and no incentives for being

  9. Not Just a TRIP! Two Cases of Business Strategy and Economic Incentives to Patent in Beijing

    E-Print Network [OSTI]

    Sadoulet, Elisabeth

    Not Just a TRIP! Two Cases of Business Strategy and Economic Incentives to Patent in Beijing Senior Honors Thesis by Shelley Jingyi Jiang Undergraduate Department of Economics University of California! Corporate Strategies and National Incentives to Patent in Beijing ABSTRACT In order to explore

  10. Trust and Exclusion in Vehicular Ad Hoc Networks: An Economic Incentive Model based Approach

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    Trust and Exclusion in Vehicular Ad Hoc Networks: An Economic Incentive Model based Approach Nadia, and lowers the overall data reception ratio in the network. To tackle this, we propose a new incentive model with exclusion for malicious nodes called VIME. VIME is inspired from the signaling theory from economics

  11. Dandelion: Cooperative Content Distribution with Robust Incentives Michael Sirivianos Xiaowei Yang Stanislaw Jarecki

    E-Print Network [OSTI]

    Pris, Jehan-Franois

    Dandelion: Cooperative Content Distribution with Robust Incentives Michael Sirivianos Xiaowei Yang in coopera- tive content distribution. First, it provides robust incentives for clients who possess content- Web [13,24, 30, 36] lack a viable economic model to scale. This work explores a cost

  12. Dandelion: Cooperative Content Distribution with Robust Incentives Michael Sirivianos Xiaowei Yang Stanislaw Jarecski

    E-Print Network [OSTI]

    Yang, Xiaowei

    Dandelion: Cooperative Content Distribution with Robust Incentives Michael Sirivianos Xiaowei Yang- tive content distribution. First, it provides robust incentives for clients who possess content- Web [11,20, 26, 31] lack a viable economic model to scale. This work explores a cost

  13. Benchmarking and incentive regulation of quality of service: an application to the UK electricity distribution utilities

    E-Print Network [OSTI]

    Giannakis, D; Jamasb, Tooraj; Pollitt, Michael G.

    2004-06-16T23:59:59.000Z

    Cambridge Working Papers in Economics CWPE 0408 Benchmarking and Incentive Regulation of Quality of Service: an Application to the UK Electricity Distribution Utilities D. Giannakis, T. Jamasb, and M. Pollitt... and Environmental Policy Research CMI Working Paper Series UNIVERSITY OF CAMBRIDGE Department of Applied Economics BENCHMARKING AND INCENTIVE REGULATION OF QUALITY OF SERVICE: AN APPLICATION TO THE UK ELECTRICITY DISTRIBUTION UTILITIES Dimitrios Giannakis...

  14. Health-Insurer Bargaining Power and Firms' Incentives to Manage Earnings Francesco Bova

    E-Print Network [OSTI]

    Tipple, Brett

    Health-Insurer Bargaining Power and Firms' Incentives to Manage Earnings Francesco Bova Rotman Power and Firms' Incentives to Manage Earnings 1. Introduction The United States relies primarily School of Management University of Toronto Francesco.Bova@rotman.utoronto.ca Yiwei Dou Stern School

  15. Managerial Incentive Horizons and the Quality of Firms' Information Environments Jianxin (Daniel) Chi

    E-Print Network [OSTI]

    in the short-term speculative component of the stock price. Current shareholders benefit from the option` information environments. When a firm`s managerial incentive horizon is short, it is more likely to report are consistent with the hypothesis that short incentive horizons induce managers to adopt strategies that reduce

  16. The incentives and disincentives of innovation prizes : a survey of the dropout teams from Progressive Insurance Automotive X PRIZE

    E-Print Network [OSTI]

    Bhushan, Bharat, S.M. Massachusetts Institute of Technology

    2010-01-01T23:59:59.000Z

    Technological innovation is driven by incentives. However, our understanding of how incentives actually work "on the ground" to change the level of activity of innovators or to shape the direction of their innovation is ...

  17. Designing PV Incentive Programs to Promote Performance: A Review of Current Practice in the U.S.

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2008-01-01T23:59:59.000Z

    Washington Renewable Energy Production Incentives Cash Backincentives for customer- sited PV: Non-Residential Renewable Energy (Renewable Energy Program SolarGenerations Solar Pioneer Program New York Energy $mart PV Incentive

  18. The recurrent nova U Scorpii - an evolutionary considerations

    E-Print Network [OSTI]

    Marek J. Sarna; Ene Ergma; Jelena Greskevits

    2005-11-30T23:59:59.000Z

    We perform evolutionary calculations of binary stars to find progenitors of systems with parameters similar to the recurrent nova U Sco. We show that a U Sco-type system may be formed starting with an initial binary system which has a low-mass carbon-oxygen white dwarf as an accretor. Since the evolutionary stage of the secondary is not well known, we calculate sequences with hydrogen-rich and helium-rich secondaries. The evolution of the binary may be divided into several observable stages as: classical nova, supersoft X-ray source with stable hydrogen shell burning, or strong wind phase. It culminates in the formation of a massive white dwarf near the Chandrasekhar mass limit. We follow the chemical evolution of the secondary as well as of the matter lost from the system, and we show that observed $^{12}$C/$^{13}$C and N/C ratios may give some information about the nature of the binary.

  19. VERITAS OBSERVATIONS OF THE NOVA IN V407 CYGNI

    SciTech Connect (OSTI)

    Aliu, E. [Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States); Archambault, S. [Physics Department, McGill University, Montreal, QC H3A 2T8 (Canada); Arlen, T. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Aune, T.; Bouvier, A. [Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064 (United States); Beilicke, M.; Buckley, J. H.; Bugaev, V.; Dickherber, R. [Department of Physics, Washington University, St. Louis, MO 63130 (United States); Benbow, W. [Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645 (United States); Bradbury, S. M. [School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT (United Kingdom); Byrum, K. [Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 (United States); Cannon, A.; Collins-Hughes, E. [School of Physics, University College Dublin, Belfield, Dublin 4 (Ireland); Cesarini, A.; Connolly, M. P. [School of Physics, National University of Ireland Galway, University Road, Galway (Ireland); Ciupik, L. [Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States); Cui, W. [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Decerprit, G. [DESY, Platanenallee 6, 15738 Zeuthen (Germany); Duke, C., E-mail: daniel-d-gall@uiowa.edu, E-mail: kazuma-tsurusaki@uiowa.edu [Department of Physics, Grinnell College, Grinnell, IA 50112-1690 (United States); and others

    2012-07-20T23:59:59.000Z

    We report on very high energy (E > 100 GeV) gamma-ray observations of V407 Cygni, a symbiotic binary that underwent a nova outburst producing 0.1-10 GeV gamma rays during 2010 March 10-26. Observations were made with the Very Energetic Radiation Imaging Telescope Array System during 2010 March 19-26 at relatively large zenith angles due to the position of V407 Cyg. An improved reconstruction technique for large zenith angle observations is presented and used to analyze the data. We do not detect V407 Cygni and place a differential upper limit on the flux at 1.6 TeV of 2.3 Multiplication-Sign 10{sup -12} erg cm{sup -2} s{sup -1} (at the 95% confidence level). When considered jointly with data from Fermi-LAT, this result places limits on the acceleration of very high energy particles in the nova.

  20. Summary of control and data acquisition systems for Nova experiments

    SciTech Connect (OSTI)

    McCauley, E.W.; Campbell, E.M.; Auerbach, J.M.; Montgomery, D.S.; Martin, V.A.; Randolph, J.E.; Shaw, J.G.; Stewart, B.L.; Stone, G.F.

    1986-04-01T23:59:59.000Z

    The Nova Laser has completed its first year of operation. During this period, emphasis has been placed on activation of the facility and of the numerous target and beam diagnostics. Two separate target chambers are in use. Nova operation is separated into two broad functions: Laser Operations and Experiments. The Operations Group provides the laser system control, operation and data acquisition and the Experiments Group provides experiment definition, diagnostic instrumentation and overall data processing. On the Operations side, VAX 11/780 computers are used to set up diagnostic operating parameters and collect data recorded by the CAMAC and CCD modules. These data are delivered in files by electronic link to the Laser Experiments and Analysis Facility (LEAF) VAX 11/785 of the Experiments Group for processing. Film data are digitized at LEAF and the film data files are also processed on the LEAF VAX.

  1. Case Studies on the Effectiveness of State Financial Incentives for Renewable Energy

    SciTech Connect (OSTI)

    Gouchoe, S.; Everette, V.; Haynes, R.

    2002-09-01T23:59:59.000Z

    The North Carolina Solar Center at NC State University, in collaboration with the National Renewable Energy Laboratory, examined 10 state financial-incentive programs in six states using a case-study approach in order to clarify the key factors-both internal and external to the program-that influence their effectiveness at stimulating deployment of renewable energy technologies. While existing information resources such as the National Database of State Incentives for Renewable Energy (DSIRE, www.dsireusa.org) have documented what incentive programs are available, the effectiveness of such programs is not well understood. Understanding the impact of current financial incentives on the deployment of renewables and the factors that influence their effectiveness is critical to a variety of stakeholders, particularly in states considering new incentives or interested in improving or discarding existing ones.

  2. SWIFT X-RAY OBSERVATIONS OF CLASSICAL NOVAE. II. THE SUPER SOFT SOURCE SAMPLE

    SciTech Connect (OSTI)

    Schwarz, Greg J. [American Astronomical Society, 2000 Florida Avenue, NW, Suite 400, Washington, DC 20009-1231 (United States); Ness, Jan-Uwe [XMM-Newton Science Operations Centre, ESAC, Apartado 78, 28691 Villanueva de la Canada, Madrid (Spain); Osborne, J. P.; Page, K. L.; Evans, P. A.; Beardmore, A. P. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Walter, Frederick M. [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800 (United States); Andrew Helton, L. [SOFIA Science Center, USRA, NASA Ames Research Center, M.S. N211-3, Moffett Field, CA 94035 (United States); Woodward, Charles E. [Minnesota Institute of Astrophysics, 116 Church Street S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Bode, Mike [Astrophysics Research Institute, Liverpool John Moores University, Birkenhead CH41 1LD (United Kingdom); Starrfield, Sumner [School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404 (United States); Drake, Jeremy J., E-mail: Greg.Schwarz@aas.org [Smithsonian Astrophysical Observatory, 60 Garden Street, MS 3, Cambridge, MA 02138 (United States)

    2011-12-01T23:59:59.000Z

    The Swift gamma-ray burst satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the X-Ray Telescope (0.3-10 keV) instrument count rates and the UltraViolet and Optical Telescope (1700-8000 A) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with Super Soft X-ray emission, 19 from Swift observations. The data set shows that the faster novae have an early hard X-ray phase that is usually missing in slower novae. The Super Soft X-ray phase occurs earlier and does not last as long in fast novae compared to slower novae. All the Swift novae with sufficient observations show that novae are highly variable with rapid variability and different periodicities. In the majority of cases, nuclear burning ceases less than three years after the outburst begins. Previous relationships, such as the nuclear burning duration versus t{sub 2} or the expansion velocity of the eject and nuclear burning duration versus the orbital period, are shown to be poorly correlated with the full sample indicating that additional factors beyond the white dwarf mass and binary separation play important roles in the evolution of a nova outburst. Finally, we confirm two optical phenomena that are correlated with strong, soft X-ray emission which can be used to further increase the efficiency of X-ray campaigns.

  3. Expriences de laboratoire en conomie et incitations montaires Experimenting in the Lab in Economics and Monetary Incentives

    E-Print Network [OSTI]

    Paris-Sud XI, Universit de

    in Economics and Monetary Incentives Nathalie Etchart-Vincent CNRS, CIRED* Rsum : La mise en place d the introduction of monetary incentives in economic laboratory experiments. Still, the empirical impact pertes Abstract: A strong positive relation is generally assumed between monetary incentives and effort

  4. Expriences de laboratoire en conomie et incitations montaires Experimenting in the Lab in Economics and Monetary Incentives

    E-Print Network [OSTI]

    Boyer, Edmond

    in Economics and Monetary Incentives Nathalie Etchart-Vincent CIRED, CNRS/EHESS/ENPC/ENGREF* Rsum : La mise legitimates the introduction of monetary incentives in economic laboratory experiments. Still, the empirical monetary incentives and effort on the one hand, and between effort and performance on the other hand, which

  5. Institutions and Incentives for R&D: Implications for L.A.C. Economies Walter G. Park,

    E-Print Network [OSTI]

    Lansky, Joshua

    Survey) 3.2 Fiscal Incentives A. Conceptual Issues B. Index of Fiscal Incentives C. Economic EffectsInstitutions and Incentives for R&D: Implications for L.A.C. Economies Walter G. Park, Associate Professor, Department of Economics, American University, Washington, D.C. 20016 August 2002 Abstract

  6. THE INTER-ERUPTION TIMESCALE OF CLASSICAL NOVAE FROM EXPANSION OF THE Z CAMELOPARDALIS SHELL

    SciTech Connect (OSTI)

    Shara, Michael M.; Mizusawa, Trisha; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024-5192 (United States); Martin, Christopher D.; Neill, James D. [Department of Physics, Math and Astronomy, California Institute of Technology, 1200 East California Boulevard, Mail Code 405-47, Pasadena, CA 91125 (United States); Seibert, Mark [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

    2012-09-10T23:59:59.000Z

    The dwarf nova Z Camelopardalis is surrounded by the largest known classical nova shell. This shell demonstrates that at least some dwarf novae must have undergone classical nova eruptions in the past, and that at least some classical novae become dwarf novae long after their nova thermonuclear outbursts. The current size of the shell, its known distance, and the largest observed nova ejection velocity set a lower limit to the time since Z Cam's last outburst of 220 years. The radius of the brightest part of Z Cam's shell is currently {approx}880 arcsec. No expansion of the radius of the brightest part of the ejecta was detected, with an upper limit of {<=}0.17 arcsec yr{sup -1}. This suggests that the last Z Cam eruption occurred {>=}5000 years ago. However, including the important effect of deceleration as the ejecta sweeps up interstellar matter in its snowplow phase reduces the lower limit to 1300 years. This is the first strong test of the prediction of nova thermonuclear runaway theory that the interoutburst times of classical novae are longer than 1000 years. The intriguing suggestion that Z Cam was a bright nova, recorded by Chinese imperial astrologers in October-November 77 B.C.E., is consistent with our measurements. If Z Cam was indeed the nova of 77 B.C.E. we predict that its ejecta are currently expanding at 85 km s{sup -1}, or 0.11 arcsec yr{sup -1}. Detection and measurement of this rate of expansion should be possible in just a few years.

  7. Thermonuclear Runaways on Accreting White Dwarfs: Models of Classical Novae Explosions

    E-Print Network [OSTI]

    Margarita Hernanz; Jordi Jose

    2000-01-11T23:59:59.000Z

    The mechanism of classical novae explosions is explained, together with some of their observational properties. The scarce but not null impact of novae in the chemical evolution of the Milky Way is analyzed, as well as their relevance for the radioactivity in the Galaxy. A special emphasis is given to the predicted gamma-ray emission from novae and its relationship with the thermonuclear model itself and its related nucleosynthesis.

  8. Understanding the Complexities of Subnational Incentives in Supporting a National Market for Distributed Photovoltaics

    SciTech Connect (OSTI)

    Bush, B.; Doris, E.; Getman, D.

    2014-09-01T23:59:59.000Z

    Subnational policies pertaining to photovoltaic (PV) systems have increased in volume in recent years and federal incentives are set to be phased out over the next few. Understanding how subnational policies function within and across jurisdictions, thereby impacting PV market development, informs policy decision making. This report was developed for subnational policy-makers and researchers in order to aid the analysis on the function of PV system incentives within the emerging PV deployment market. The analysis presented is based on a 'logic engine,' a database tool using existing state, utility, and local incentives allowing users to see the interrelationships between PV system incentives and parameters, such as geographic location, technology specifications, and financial factors. Depending on how it is queried, the database can yield insights into which combinations of incentives are available and most advantageous to the PV system owner or developer under particular circumstances. This is useful both for individual system developers to identify the most advantageous incentive packages that they qualify for as well as for researchers and policymakers to better understand the patch work of incentives nationwide as well as how they drive the market.

  9. Distributed Solar Incentive Programs: Recent Experience and Best Practices for Design and Implementation

    SciTech Connect (OSTI)

    Bird, L.; Reger, A.; Heeter, J.

    2012-12-01T23:59:59.000Z

    Based on lessons from recent program experience, this report explores best practices for designing and implementing incentives for small and mid-sized residential and commercial distributed solar energy projects. The findings of this paper are relevant to both new incentive programs as well as those undergoing modifications. The report covers factors to consider in setting and modifying incentive levels over time, differentiating incentives to encourage various market segments, administrative issues such as providing equitable access to incentives and customer protection. It also explores how incentive programs can be designed to respond to changing market conditions while attempting to provide a longer-term and stable environment for the solar industry. The findings are based on interviews with program administrators, regulators, and industry representatives as well as data from numerous incentive programs nationally, particularly the largest and longest-running programs. These best practices consider the perspectives of various stakeholders and the broad objectives of reducing solar costs, encouraging long-term market viability, minimizing ratepayer costs, and protecting consumers.

  10. altered granitic rock: Topics by E-print Network

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

    22 Everglades National Park Groundwater wells Surface water monitoring locations Rock mining locations 12 Demers, Nora Egan 211 Nova Scotia Rock Garden Club Membership...

  11. GREENHOUSE GAS (GHG) INVENTORY REPORT 20102011 Dalhousie Office of Sustainability

    E-Print Network [OSTI]

    Brownstone, Rob

    Caption. LSC Solar thermal panels installed 20102011. #12;Page | 1 TableofContents Table ......................................................................................... 35 Appendix I: Nova Scotia Power Emission Factors ......

  12. f-Words and Binary Solid Codes1 Stavros Konstantinidis

    E-Print Network [OSTI]

    and Computing Science Saint Mary's University Halifax, Nova Scotia, B3H 3C3 Canada s.konstantinidis@smu.ca, jyo

  13. DISCUSSION PAPER 11 TOWARD SUSTAINABLE AND RESILIENT FISHERIES

    E-Print Network [OSTI]

    Charles, Anthony

    Mary's University, Halifax, Nova Scotia B3H3C3 Canada, t.charles@smu.ca. #12;222 limited usefulness, so

  14. ICES CM 2008/O:05 Theme Session: Governmental

    E-Print Network [OSTI]

    Charles, Anthony

    's University Halifax, Nova Scotia, Canada B3H3C3 Tel: 1-902-420-5732 tony.charles@smu.ca Not to be cited

  15. Determining exponential density and maximal encoding capabilities of a regular language

    E-Print Network [OSTI]

    , Halifax, Nova Scotia, B3H 3C3 Canada, s.konstantinidis@smu.ca, nic.santean@smu.ca Abstract. The density

  16. FORMAL DESCRIPTIONS OF CODE PROPERTIES: DECIDABILITY, COMPLEXITY, IMPLEMENTATION1

    E-Print Network [OSTI]

    's University, Halifax, Nova Scotia, B3H 3C3 Canada krystian dudzinski@hotmail.com, s.konstantinidis@smu

  17. What is a Maximal Error-Detecting Capability of a Formal Language?

    E-Print Network [OSTI]

    Department of Mathematics and Computing Science Saint Mary's University Halifax, Nova Scotia B3H 3C3 CANADA s.konstantinidis@smu

  18. Interactive Learning of Alert Signatures in High Performance Cluster System Logs

    E-Print Network [OSTI]

    Milios, Evangelos E.

    , Nova Scotia, Canada. B3H 1W5. +1-902-494-2093 {makanju, zincir, eem}@cs.dal.ca Abstract--The ability

  19. Matching and Retrieval of Distorted and Occluded Shapes Using Dynamic Programming

    E-Print Network [OSTI]

    Petrakis, Euripides G.M.

    , Dalhousie University, Halifax, Nova Scotia, Canada B3H 1W5. E-mail: eem@cs.dal.ca, URL: http://www.cs.dal.ca/~eem

  20. LABORATORY ANALYSIS OF PRESOLAR SILICATE STARDUST FROM A NOVA

    SciTech Connect (OSTI)

    Leitner, J.; Kodolanyi, J.; Hoppe, P. [Max Planck Institute for Chemistry, Particle Chemistry Department, Hahn-Meitner-Weg 1, D-55128 Mainz (Germany); Floss, C., E-mail: jan.leitner@mpic.de [Laboratory for Space Sciences and Physics Department, Washington University, One Brookings Drive, St. Louis, MO 63130 (United States)

    2012-08-01T23:59:59.000Z

    We report the major element as well as the oxygen, magnesium, and silicon isotope composition of a unique presolar silicate grain found in the fine-grained fraction of the Antarctic CR2 chondrite Graves Nunataks 95229. The grain is characterized by an extremely high {sup 17}O/{sup 16}O ratio (6.3 {+-} 0.2 Multiplication-Sign 10{sup -3}) relative to solar values, whereas its {sup 18}O/{sup 16}O ratio is solar within measurement uncertainty. It also shows enrichments in {sup 25,26}Mg and a significant excess in {sup 30}Si relative to solar system compositions, with {delta}{sup 25}Mg = 79 {+-} 21 per mille , {delta}{sup 26}Mg = 70 {+-} 20 per mille , and {delta}{sup 30}Si = 379 {+-} 92 per mille . This isotopic composition is consistent with an origin in the ejecta of a {approx}1.3-1.4 M{sub Sun} ONe nova with large contributions of material from a main-sequence companion star of roughly solar metallicity. However, many details of the stellar source remain undetermined, owing to the uncertainties of current nova nucleosynthesis models. Auger electron spectroscopic analyses identify O, Mg, Si, and Fe as the grain's major constituents. Its (Mg+Fe)/Si atomic ratios are lower than that of olivine and correspond on average to Fe-Mg-pyroxene. A complex texture and heterogeneous major element distribution within the grain attest to condensation under non-equilibrium conditions, which is consistent with the proposed nova origin.

  1. NOVA Portal: Submit VASP Jobs to Carver via the Web

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Saleshttp://www.fnal.gov/directorate/nalcal/nalcal02_07_05_files/nalcal.gif Directorate1,Stewardship now661NONLINEARRPSEA~ ~ . _NOVA

  2. Nova Alinca Agricola e Comercial | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpenNorth AmericaNorthwest Rural PubNova Alinca Agricola e

  3. HelioNova S L | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup | Open Energy InformationHebei QindaoHeilongjiangHeishuiHelioNova S

  4. Create PDF files without this message by purchasing novaPDF printer (http://www.novapdf.com) Create PDF files without this message by purchasing novaPDF printer (http://www.novapdf.com)

    E-Print Network [OSTI]

    Barthelat, Francois

    Create PDF files without this message by purchasing novaPDF printer (http://www.novapdf.com) #12; Create PDF files without this message without this message by purchasing novaPDF printer (http://www.novapdf.com) #12

  5. Designing PV Incentive Programs to Promote Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2007-01-01T23:59:59.000Z

    Sustainable Development Fund (SDF) and CCEF require a fullor hybrid incentive structure. SDFs Solar Grant program andEntity receiving the PBI payment. SDF splits the PBI payment

  6. Cost trends and government incentives in the California photovoltaics market, 2007-2008

    E-Print Network [OSTI]

    Wang Yan, S.B. Massachusetts Institute of Technology

    2009-01-01T23:59:59.000Z

    The focus of this thesis is to analyze cost trends and government incentives in the California PV market during 2007-2008. The data show that pre-rebate system costs increased in California during this time period and that ...

  7. FirstEnergy (Mon Power and Potomac Edison)- Business Lighting Incentive Program (West Virginia)

    Broader source: Energy.gov [DOE]

    FirstEnergy's West Virginias utilities (Mon Power and Potomac Edison) offer the Business Lighting Incentive Program in accordance with the December 30, 2011, order issued by the Public Service...

  8. Agency and incentive contract in private investment of transport project : an exploration of fundamental relationships

    E-Print Network [OSTI]

    Chiang, Risharng

    2002-01-01T23:59:59.000Z

    This thesis codifies and relates critical incentive-design and financial-contracting issue to the unique principal-agent circumstances generated from private investment of transport infrastructure and provides a framework ...

  9. Fact #789: July 22, 2013 Comparison of State Incentives for Plug...

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

    addition to a Federal government tax credit up to 7,500, consumers who purchase plug-in electric vehicles (PEVs) may also receive state government incentives which are different...

  10. ConEd (Gas)- Multi-family Energy Efficiency Incentives Program

    Broader source: Energy.gov [DOE]

    Con Edison is offering a Multifamily Natural Gas Heating Rebate Program. Through this program, incentives are offered on energy efficient heating equipment for 5-75 unit buildings in the eligible...

  11. Incentive-based approaches for mitigating greenhouse gas emissions : issues and prospects for India

    E-Print Network [OSTI]

    Gupta, Shreekant.

    As a consequence of the flexibility mechanisms incorporated in the Kyoto Protocol, incentive-based policies such as emissions trading and the clean development mechanism are being widely discussed in the context of greenhouse ...

  12. Incentive regulation in theory and practice : electricity distribution and transmission networks

    E-Print Network [OSTI]

    Joskow, Paul L.

    2005-01-01T23:59:59.000Z

    Modern theoretical principles to govern the design of incentive regulation mechanisms are reviewed and discussed. General issues associated with applying these principles in practice are identified. Examples of the actual ...

  13. Efficiency of incentives to jointly increase carbon sequestration and species conservation

    E-Print Network [OSTI]

    Weiblen, George D

    Efficiency of incentives to jointly increase carbon sequestration and species conservation the provision of carbon sequestration and species conservation across heterogeneous landscapes. Using data from the Willamette Basin, Oregon, we compare the provision of carbon sequestration and species conservation under

  14. Investment and Efficiency under Incentive Regulation: The Case of the Norwegian Electricity Distribution Networks

    E-Print Network [OSTI]

    Poudineh, Rahmatallah; Jamasb, Tooraj

    2013-04-01T23:59:59.000Z

    Following the liberalisation of the electricity industry since the early 1990s, many sector regulators have recognised the potential for cost efficiency improvement in the networks through incentive regulation aided by benchmarking and productivity...

  15. Planning for sustainable communities: Regional incentives and local policy under SB375

    E-Print Network [OSTI]

    California at Davis, University of

    Planning for sustainable communities: Regional incentives and local policy under SB375 Gian Institute Policy for Energy, Environment and the Economy University of California, Davis March 19, 2014 impacts access density alternatives sustainability #12;Sustainable Communities Strategy (SCS) San Diego

  16. Designing PV Incentive Programs to Promote Performance: A Review of Current Practice

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2007-01-01T23:59:59.000Z

    manufacturers of PV modules and inverters are to establishPV modules, and UL- 1741 is the analogous standard for inverters andPV incentive programs surveyed for this paper, most require that inverters

  17. Reducing emissions from deforestation--The ``combined incentives'' mechanism and empirical simulations

    E-Print Network [OSTI]

    Vermont, University of

    Reducing emissions from deforestation--The ``combined incentives'' mechanism and empirical throughout a century of climate-change (Gullison et al., 2007). The financial rationale for deforestation be sufficient to greatly reduce deforestation (Stern, 2007). For political and methodological reasons

  18. Memphis Light, Gas and Water (Electric)- Commercial Efficiency Advice and Incentives Program

    Broader source: Energy.gov [DOE]

    Memphis Light, Gas and Water (MLGW), in partnership with the Tennessee Valley Authority (TVA), offers a variety of energy efficient incentives to non-residential customers. The program provides...

  19. Utility and state industrial EMS incentives programs: Experience and success factors

    SciTech Connect (OSTI)

    Roop, J.M.; Stucky, D.J.

    1993-03-01T23:59:59.000Z

    This paper summarizes the results of a survey of utility and state demand-side management (DSM) programs that address efficient motor systems. The paper discusses the incentive structures in place at both the state and utility levels to encourage efficient motor systems, and the market barriers associated with implementation of efficient motor equipment. The paper also assesses how the current incentives might address the market barriers to the implementation of efficient motor systems.

  20. Direct measurement of the $^{18}F(p,\\alpha)^{15}O$ reaction for application to nova gamma-ray emission

    E-Print Network [OSTI]

    De Srville, N; Leleux, P; Coc, A; Kiener, J; Lefebvre-Schuhl, A; Tatischeff, V; Descouvemont, P; Figuera, P; Hammache, F; Achouri, L; Orr, N; Stefan, I; Casarejos, E; Davinson, T; Robertson, D; Laird, A M; Fox, S P; Mumby-Croft, P; Vaughan, K

    2006-01-01T23:59:59.000Z

    Direct measurement of the $^{18}F(p,\\alpha)^{15}O$ reaction for application to nova gamma-ray emission

  1. Incentive mechanisms as a strategic option for acid rain compliance

    SciTech Connect (OSTI)

    South, D.W.; Bailey, K.A.; McDermott, K.A.

    1991-01-01T23:59:59.000Z

    Title IV of the Clean Air Act Amendments (CAAA) of 1990 (P.L. 101--549) establishes the use of flexible emission compliance strategies for electric utilities to reduce the emissions of add precursors (SO[sub 2], NO[sub 2]). To control SO[sub 2] emissions, tradeable emission allowances will be used; NO[sub 2] emissions will be controlled by an emission standard, but a utility is permitted to average NO[sub 2] emissions systemwide to meet the standard. Both of these policies promote flexibility and cost savings for the utility while achieving the prescribed emission reduction goals of P.L. 101--549. The use of SO[sub 2] emission allowances has two notable benefits: A utility has the choice of a wide range of compliance methods allowing it to minimize compliance costs and second; the use of transferable emission allowances promote technological innovation with respect to emissions reduction/control. This report discusses the use of regulatory incentives towards the achievement of a Title IV goal of cost reduction of SO[sub 2] emissions.

  2. Incentive mechanisms as a strategic option for acid rain compliance

    SciTech Connect (OSTI)

    South, D.W.; Bailey, K.A.; McDermott, K.A.

    1991-12-31T23:59:59.000Z

    Title IV of the Clean Air Act Amendments (CAAA) of 1990 (P.L. 101--549) establishes the use of flexible emission compliance strategies for electric utilities to reduce the emissions of add precursors (SO{sub 2}, NO{sub 2}). To control SO{sub 2} emissions, tradeable emission allowances will be used; NO{sub 2} emissions will be controlled by an emission standard, but a utility is permitted to average NO{sub 2} emissions systemwide to meet the standard. Both of these policies promote flexibility and cost savings for the utility while achieving the prescribed emission reduction goals of P.L. 101--549. The use of SO{sub 2} emission allowances has two notable benefits: A utility has the choice of a wide range of compliance methods allowing it to minimize compliance costs and second; the use of transferable emission allowances promote technological innovation with respect to emissions reduction/control. This report discusses the use of regulatory incentives towards the achievement of a Title IV goal of cost reduction of SO{sub 2} emissions.

  3. United States/Mexico electricity exchanges. [History, incentives, and constraints

    SciTech Connect (OSTI)

    None,

    1980-05-01T23:59:59.000Z

    As a result of the agreement between the respective presidents, a joint study was undertaken to analyze the possibilities of increasing the international electricity exchange between the two countries. Responsibility for this undertaking was assigned to the United States Department of Energy (DOE) and to the Direccion de Energia de Mexico (DEM) through the Comision Federal de Electricidad (CFE). Representatives from Mexico and the US were chosen from the regional utilities along the border between the two countries and made up working groups that particiated in the study. With the support of both governments, and a high degree of cooperation between the two countries, work on the study was completed within fourteen months The completion of the study has been a major step in broadening the base of bilateral energy relations. the study highlights the opportunities for increased electricity exchanges, which could increase cooperation along the common border. Expansion of electricity interchange could offer substantial economic benefit to both countries, both directly and indirectly. Direct benefits include increased reliability of electric power and cost savings through economies of scale and diversity of peak demand patterns. Indirect benefits include improved economic and employment opportunities, especially in the border areas of both countries. This report provides background on the history of past exchanges and the characteristics of the US and Mexico electric systems, a summary of opportunities and incentives, and suggestions for procedures to remove obstacles and constraints.

  4. A search for radioactive 26Al in the nova-like variable V4332 Sagittarii

    E-Print Network [OSTI]

    D. P. K. Banerjee; N. M. Ashok; O. Launila; C. J. Davis; W. P. Varricatt

    2004-06-21T23:59:59.000Z

    We have searched for the important radioactive isotope 26Al in the nova-like source V4332 Sgr. Recent results from gamma ray astronomy show that there is pervasive emission of the 1.809 MeV gamma ray photon, arising from the decay of 26Al to 26Mg, from all over the galactic plane. Though the sites from where this emission originates are not clearly established, novae are believed to be an important contributing source. In this context, V4332 Sgr presented a rare opportunity to observationally investigate whether novae or novae-like sources synthesize 26Al and to what extent. Strong AlO bands in the near-IR have been reported in this object recently. As molecular bands of different isotopic compositions are readily resolved spectroscopically (e.g. 12CO and 13CO), it was thought that the components of AlO associated with 26Al and stable 27Al could be detected as separate bands. Our spectra indicate that there is no strong presence of 26Al in V4332 Sgr. A reliable upper limit of 0.10 for the 26Al/27Al ratio is determined which constitutes the first observational constraint for this ratio in a potential 26Al producing source. While V4332 Sgr is not a typical nova, its outburst amplitude and light-curve behaviour bear close similarity to that of novae. Hence, although the results from V4332 Sgr cannot be directly extended to novae in general, the limit on the observed 26Al/27Al ratio could be a useful input in constraining rather uncertain nucleosynthesis models for the production of 26Al in novae/novae-like sources. By comparing the observed 26Al/27Al ratio in V4332 Sgr with that expected in classical novae it appears unlikely that the progenitor of V4332 Sgr is an Oxygen-Neon-Magnesium white dwarf.

  5. Reducing Electrical Power Use with a Performance Based Incentive

    SciTech Connect (OSTI)

    M. Kathleen Nell

    2004-07-01T23:59:59.000Z

    This Departmental Energy Management Program (DEMP) funded Model Program Study developed out of a potential DOE-ID Performance Based Incentive for the Idaho National Engineering and Environmental Laboratory (INEEL), lasting from October 2001 through May 2002, which stressed reductions in electrical usage. An analysis of demand usage obtained from monthly INEEL Power Management electric reports revealed reductions in demand from a majority of the site areas. The purpose of this Model Program study was to determine the methods and activities that were used at these site areas to achieve the reductions in demand and to develop these demand reduction methods and activities into a Model Program that could be shared throughout the INEEL and DOE complex-wide for additional demand savings. INEEL Energy Management personnel interviewed contacts from the eight areas which had achieved a consistent reduction in demand during the study period, namely, Idaho Nuclear Technology and Engineering Center (INTEC), Test Area North (TAN), Power Burst Facility (PBF), Test Reactor Area (TRA) including Advanced Test Reactor ATR), Engineering Test Reactor (ETR), and Materials Test Reactor (MTR) areas, Central Facilities Area (CFA), Specific Manufacturing Capability (SMC), Radioactive Waste Management Complex (RWMC), and Argonne National Laboratory-West (ANLW). The information that resulted from the interviews indicated that more than direct demand and energy reduction actions were responsible for the recorded reductions in demand. INEEL Energy Management identified five categories of actions or conditions that contributed to the demand reduction. These categories are Decontamination and Decommissioning (D&D), employee actions, improvements, inactivation for maintenance, and processes. The following information details the findings from the study.

  6. NOvA (Fermilab E929) Official Plots and Figures

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    The NOvA collaboration, consisting of 180 researchers across 28 institutions and managed by the Fermi National Accelerator Laboratory (FNAL), is developing instruments for a neutrino-focused experiment that will attempt to answer three fundamental questions in neutrino physics: 1) Can we observe the oscillation of muon neutrinos to electron neutrinos; 2) What is the ordering of the neutrino masses; and 3) What is the symmetry between matter and antimatter? The collaboration makes various data plots and figures available. These are grouped under five headings, with brief descriptions included for each individual figure: Neutrino Spectra, Detector Overview, Theta12 Mass Hierarchy CP phase, Theta 23 Delta Msqr23, and NuSterile.

  7. NOVA-NREL Optimal Vehicle Acquisition Analysis (Brochure)

    SciTech Connect (OSTI)

    Blakley, H.

    2011-03-01T23:59:59.000Z

    Federal fleet managers face unique challenges in accomplishing their mission - meeting agency transportation needs while complying with Federal goals and mandates. Included in these challenges are a variety of statutory requirements, executive orders, and internal goals and objectives that typically focus on petroleum consumption and greenhouse gas (GHG) emissions reductions, alternative fuel vehicle (AFV) acquisitions, and alternative fuel use increases. Given the large number of mandates affecting Federal fleets and the challenges faced by all fleet managers in executing day-to-day operations, a primary challenge for agencies and other organizations is ensuring that they are as efficient as possible in using constrained fleet budgets. An NREL Optimal Vehicle Acquisition (NOVA) analysis makes use of a mathematical model with a variety of fleet-related data to create an optimal vehicle acquisition strategy for a given goal, such as petroleum or GHG reduction. The analysis can helps fleets develop a vehicle acquisition strategy that maximizes petroleum and greenhouse gas reductions.

  8. Nova DAQ, System Architecture, Data Combiner and Timing System

    SciTech Connect (OSTI)

    Biery, K.A.; Cooper, R.G.; Foulkes, S.C.; Guglielmo, G.M.; Haynes, B.W.; Kwarciany, R.; Pavlicek, F.V.; Piccoli, L.P.; Votava, M.E.V.; /Fermilab

    2007-04-01T23:59:59.000Z

    NOvA (E929) is a long baseline experiment that will search for neutrino oscillations. There will be one detector near the beam source at Fermilab, and one detector in northern Minnesota. The DAQ system for the far detector collects over-threshold hits from over 450,000 channels of scintillator readouts, sorts the time-stamped data packets and archives selected time periods of data for transmission and processing. While a simple point-to-point protocol is used for the first level of data collection, Ethernet was chosen as the fabric for the rest of the DAQ. The packet time-stamp and overall system synchronization is based on two common-view GPS trained clock oscillators, one at each site. The present design cost-effectively satisfies the experiment's moderate speed and data volume requirements.

  9. Near Infrared Observations of the novae V2491 Cygni and V597 Puppis

    E-Print Network [OSTI]

    Sachindra Naik; D. P. K. Banerjee; N. M. Ashok

    2008-12-22T23:59:59.000Z

    We present results obtained from near-infrared JHK spectroscopic observations of novae V2491 Cyg and V597 Pup in the early declining phases of their 2007 and 2008 outbursts respectively. In both objects, the spectra displayed emission lines of HI, OI, HeI and NI. In V597 Pup, the HeI lines were found to strengthen rapidly with time. Based on the observed spectral characteristics, both objects are classified as He/N novae. We have investigated the possibility of V2491 Cyg being a recurrent nova as has been suggested. By studying the temporal evolution of the line widths in V2491 Cyg it appears unlikely that the binary companion is a giant star with heavy wind as in recurrent novae of the RS Oph type. Significant deviations from that of recombination case B conditions are observed in the strengths of the HI lines. This indicates that the HI lines, in both novae, are optically thick during the span of our observations. The slope of the continuum spectra in both cases was found to have a \\lambda^-(3-3.5) dependence which deviates from a Rayleigh-Jeans spectral distribution. Both novae were detected in the post-outburst super-soft X-ray phase; V2491 Cyg being very bright in X-rays has been the target of several observations. We discuss and correlate our infrared observations with the observed X-ray properties of these novae.

  10. The {sup 30}P(p, ?){sup 31}S reaction in classical novae: progress and prospects

    SciTech Connect (OSTI)

    Wrede, C., E-mail: wrede@nscl.msu.edu [Department of Physics and Astronomy and National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824 (United States)

    2014-04-15T23:59:59.000Z

    The unknown thermonuclear rate of the {sup 30}P(p, ?){sup 31}S reaction at classical-nova temperatures currently prohibits the accurate modeling of nova nucleosynthesis in the A ? 30 region. This is hindering the calibration of nova thermometers based on observed O/S, S/Al, O/P, and P/Al abundance ratios in nova ejecta, the calibration of a meter to probe mixing at the core-envelope interface in novae based on the observed Si/H abundance ratio, and the identification of candidate pre-solar nova grains found in primitive meteorites based on laboratory measurements of their {sup 30}Si/{sup 28}Si isotopic ratios. Each of these diagnostics could address key questions in our understanding of classical novae if the {sup 30}P(p, ?){sup 31}S rate were known. We review progress on the determination of the {sup 30}P(p, ?){sup 31}S rate leading to a critical assessment of current interpretations of published data and prospects for future work.

  11. An analysis of cost effective incentives for initial commercial deployment of advanced clean coal technologies

    SciTech Connect (OSTI)

    Spencer, D.F. [SIMTECHE, Half Moon Bay, CA (United States)

    1997-12-31T23:59:59.000Z

    This analysis evaluates the incentives necessary to introduce commercial scale Advanced Clean Coal Technologies, specifically Integrated Coal Gasification Combined Cycle (ICGCC) and Pressurized Fluidized Bed Combustion (PFBC) powerplants. The incentives required to support the initial introduction of these systems are based on competitive busbar electricity costs with natural gas fired combined cycle powerplants, in baseload service. A federal government price guarantee program for up to 10 Advanced Clean Coal Technology powerplants, 5 each ICGCC and PFBC systems is recommended in order to establish the commercial viability of these systems by 2010. By utilizing a decreasing incentives approach as the technologies mature (plants 1--5 of each type), and considering the additional federal government benefits of these plants versus natural gas fired combined cycle powerplants, federal government net financial exposure is minimized. Annual net incentive outlays of approximately 150 million annually over a 20 year period could be necessary. Based on increased demand for Advanced Clean Coal Technologies beyond 2010, the federal government would be revenue neutral within 10 years of the incentives program completion.

  12. Inverter Eligibility Listing Procedure for Solar Electric Incentive Programs Updated 6/2/14 Senate Bill 1 (SB1) defines the solar incentive programs for California, and inverters must be listed on

    E-Print Network [OSTI]

    (Maximum Continuous Output Power, Conversion Efficiency, and Tare Losses) and weighted inverter efficiencyInverter Eligibility Listing Procedure for Solar Electric Incentive Programs Updated 6/2/14 Senate Bill 1 (SB1) defines the solar incentive programs for California, and inverters must be listed

  13. Designing PV Incentive Programs to Promote Performance: A Review of Current Practice in the U.S.

    E-Print Network [OSTI]

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2008-01-01T23:59:59.000Z

    Solar Program Solar Electric Rebate Program Customer Onsitecustomer- sited PV: Non-Residential Renewable Energy (NOFA 07-02), Residential Renewable Energy (NOFA 07-03), and New Solarsolar resource. Incentive-based approaches provide a direct monetary incentive to program participants (typically the customer

  14. Proposed Program: Voluntary Retirement Incentive Program for Staff Proposed by: University of Tennessee Institute of Agriculture (UTIA)

    E-Print Network [OSTI]

    Tennessee, University of

    : 1. Eligible for federal retirement benefits under a Voluntary Early Retirement Authority (VERA)2#12;#12;Proposed Program: Voluntary Retirement Incentive Program for Staff Proposed by: University of Tennessee Institute of Agriculture (UTIA) Purpose: The UTIA Voluntary Retirement Incentive Program for Staff

  15. Pulsed power supply for Nova Upgrade. Final report, August 1, 1991 to March 31, 1992

    SciTech Connect (OSTI)

    Bacon, J.L.; Kajs, J.P.; Walls, A.; Weldon, W.F.; Zowarka, R.C. [Univ. of Texas, Austin, TX (US). Center for Electromechanics] [Univ. of Texas, Austin, TX (US). Center for Electromechanics

    1992-12-31T23:59:59.000Z

    This report describes work carried out at the Center for Electromechanics at The University of Texas at Austin (CEM-UT). A baseline design of the Nova Upgrade has been completed by Lawrence Livermore National Laboratory. The Nova Upgrade is an 18 beamline Nd: glass laser design utilizing fully relayed 4x4 30 cm aperture segmented optical components. The laser thus consists of 288 independent beamlets nominally producing 1.5 to 2.0 MJ of 0.35 {mu}m light in a 3 to 5 ns pulse. The laser design is extremely flexible and will allow a wide range of pulses to irradiate ICF targets. This facility will demonstrate ignition/gain and the scientific feasibility of ICF for energy and defense applications. The pulsed power requirements for the Nova Upgrade are given. CEM-UT was contracted to study and develop a design for a homopolar generator/inductor (HPG/inductor) opening switch system which would satisfy the pulsed power supply requirements of the Nova Upgrade. The Nd:glass laser amplifiers used in the Nova Upgrade will be powered by light from xenon flashlamps. The pulsed power supply for the Nova Upgrade powers the xenon flashlamps. This design and study was for a power supply to drive flashlamps.

  16. UNBC Executive Compensation Disclosure -April 1/08 -March 31/09 Name and Principal Position (b) Salary (c) Bonus (d) Incentive Plan Comp (e) Pension1

    E-Print Network [OSTI]

    Northern British Columbia, University of

    ) Salary (c) Bonus (d) Incentive Plan Comp (e) Pension1 (f) All Other Comp2 (g) Total (h) Previous year Position (b) Salary (c) Bonus (d) Incentive Plan Comp (e) Pension11 (f) All Other Comp12 (g) Total (h

  17. SWIFT X-RAY AND ULTRAVIOLET MONITORING OF THE CLASSICAL NOVA V458 VUL (NOVA VUL 2007)

    SciTech Connect (OSTI)

    Ness, J.-U. [European Space Astronomy Centre, P.O. Box 78, 28691 Villanueva de la Canada, Madrid (Spain); Drake, J. J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Beardmore, A. P.; Evans, P. A.; Osborne, J. P.; Page, K. L. [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Boyd, D. [BAA VSS, 5 Silver Lane, West Challow, Wantage, OX12 9TX (United Kingdom); Bode, M. F. [Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD (United Kingdom); Brady, S. [AAVSO, 5 Melba Drive, Hudson, NH 03051 (United States); Gaensicke, B. T.; Steeghs, D. [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); Kitamoto, S.; Takei, D. [Department of Physics, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501 (Japan); Knigge, C. [School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom); Miller, I. [BAA VSS, Furzehill House, Ilston, Swansea SA2 7LE (United Kingdom); Rodriguez-Gil, P. [Isaac Newton Group, PO Ap. de Correos 321, 38700 Sta. Cruz de la Palma (Spain); Schwarz, G. [Department of Geology and Astronomy, West Chester University, West Chester, PA 19383 (United States); Staels, B. [CBA Flanders, Alan Guth Observatory, Koningshofbaan 51, Hofstade, Aalst (Belgium); Tsujimoto, M. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Wesson, R. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom)], E-mail: juness@sciops.esa.int (and others)

    2009-05-15T23:59:59.000Z

    We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vul became a variable hard X-ray source due to optically thin thermal emission at kT = 0.64 keV with an X-ray band unabsorbed luminosity of 2.3 x 10{sup 34} erg s{sup -1} during days 71-140. The X-ray spectrum at this time requires a low Fe abundance (0.2{sup +0.3} {sub -0.1} solar), consistent with a Suzaku measurement around the same time. On day 315 we find a new X-ray spectral component which can be described by a blackbody with temperature of kT = 23{sup +9} {sub -5} eV, while the previous hard X-ray component has declined by a factor of 3.8. The spectrum of this soft X-ray component resembles those typically seen in the class of supersoft sources (SSS) which suggests that the nova ejecta were starting to clear and/or that the white dwarf photosphere is shrinking to the point at which its thermal emission reaches into the X-ray band. We find a high degree of variability in the soft component with a flare rising by an order of magnitude in count rate in 0.2 days. In the following observations on days 342.4-383.6, the soft component was not seen, only to emerge again on day 397. The hard component continued to evolve, and we found an anticorrelation between the hard X-ray emission and the UV emission, yielding a Spearman rank probability of 97%. After day 397, the hard component was still present, was variable, and continued to fade at an extremely slow rate but could not be analyzed owing to pile-up contamination from the bright SSS component.

  18. [1] D. Alderson and K. S. Hoo. The role of economic incentives in securing cyberspace. Technical report, CISAC, Stanford University, November 2004. [ bib | .pdf

    E-Print Network [OSTI]

    Briesemeister, Linda

    [1] D. Alderson and K. S. Hoo. The role of economic incentives in securing cyberspace. Technical of a failure by public policy to recognize and to address those incentives and the technological, economic of coherent policy in which the interaction of economic incentives among stakeholders is explicitly considered

  19. The Effect of Monetary Incentives on Sales of Advanced Clean Cars

    E-Print Network [OSTI]

    California at Davis, University of

    electric vehicle (HEV) sales, with a number of studies already available for the case of PEVs. Examples (PEVs). The same study estimated that the public and private benefits resulting from the large- scale the strategies referenced earlier is to offer monetary incentives. Studies find that reducing the relative cost

  20. EIS-0016: Cumulative Production/Consumption Effects of the Crude Oil Price Incentive Rulemakings, Programmatic

    Broader source: Energy.gov [DOE]

    The U.S. Department of Energy prepared this Final Statement to FEA-FES-77-7 to assess the environmental and socioeconomic implications of a rulemaking on crude oil pricing incentives as pertains to the full range of oil production technologies (present as well as anticipated.)

  1. Assessing the Feasibility of An Energy Savings Incentive Program for Williams College

    E-Print Network [OSTI]

    Aalberts, Daniel P.

    budgets have been cut 15% campus wide,2 behavioral changes require only modest investment.3 Up until $5,838,229 on utilities (electricity, natural gas, #2 fuel oil, water).4 If utility use could incentive program) would require some investment. However, the electric and steam meters are already

  2. Country Review of Energy-Efficiency Financial Incentives in the Residential Sector

    SciTech Connect (OSTI)

    Can, Stephane de la Rue du; Shah, Nihar; Phadke, Amol

    2011-07-13T23:59:59.000Z

    A large variety of energy-efficiency policy measures exist. Some are mandatory, some are informative, and some use financial incentives to promote diffusion of efficient equipment. From country to country, financial incentives vary considerably in scope and form, the type of framework used to implement them, and the actors that administer them. They range from rebate programs administered by utilities under an Energy-Efficiency Resource Standards (EERS) regulatory framework (California, USA) to the distribution of Eco-points rewarding customers for buying highly efficient appliances (Japan). All have the primary objective of transforming the current market to accelerate the diffusion of efficient technologies by addressing up-front cost barriers faced by consumers; in most instances, efficient technologies require a greater initial investment than conventional technologies. In this paper, we review the different market transformation measures involving the use of financial incentives in the countries belonging to the Major Economies Forum. We characterize the main types of measures, discuss their mechanisms, and provide information on program impacts to the extent that ex-ante or ex-post evaluations have been conducted. Finally, we identify best practices in financial incentive programs and opportunities for coordination between Major Economies Forum countries as envisioned under the Super Efficient Appliance Deployment (SEAD) initiative.

  3. Designing PV Incentive Programs to Promote Performance: A Reviewof Current Practice in the U.S.

    SciTech Connect (OSTI)

    Barbose, Galen; Wiser, Ryan; Bolinger, Mark

    2006-10-06T23:59:59.000Z

    In the U.S., the increasing financial support for customer-sited photovoltaic (PV) systems provided through publicly-funded incentive programs has heightened concerns about the long-term performance of these systems. Given the barriers that customers face to ensuring that their PV systems perform well, and the responsibility that PV incentive programs bear to ensure that public funds are prudently spent, these programs should, and often do, play a critical role in addressing PV system performance. To provide a point of reference for assessing the current state of the art, and to inform program design efforts going forward, we examine the approaches to encouraging PV system performance used by 32 prominent PV incentive programs in the U.S. We identify eight general strategies or groups of related strategies that these programs have used to address factors that affect performance, and describe key implementation details. Based on this review, we then offer recommendations for how PV incentive programs can be effectively designed to mitigate potential performance issues.

  4. Competition Law Enforcement: the "Free-Riding" Plaintiff and Incentives for the Revelation of Private

    E-Print Network [OSTI]

    Feigon, Brooke

    -on.1 With a de novo case, a plaintiff initiates a private action based on an alleged breach of Private Information by Michael Harker and Morten Hviid ESRC Centre for Competition Policy and Norwich Law of firms and individuals to use private enforcement suggests that there are limited incentives for self

  5. Signaling environmental quality to green consumers and the incentive to invest in cleaner technology: Eect of

    E-Print Network [OSTI]

    Edwards, Paul N.

    to environmentally conscious consumers that are not informed about the environmental damage caused by ...rms to pay more for goods pro- duced with lower environmental damage1, and the market incentives it generates speci...c kinds of environmental damage and remains signi...cantly limited relative to the environmental

  6. Near-Infrared Studies of V1280 Sco (Nova Scorpii 2007)

    E-Print Network [OSTI]

    Ramkrishna Das; Dipankar Banerjee; Nagarhalli Ashok; Olivier Chesneau

    2008-09-26T23:59:59.000Z

    We present spectroscopic and photometric results of Nova V1280 Sco which was discovered in outburst in early 2007 February. The large number of spectra obtained of the object leads to one of the most extensive, near-infrared spectral studies of a classical nova. The spectra evolve from a P-Cygni phase to an emission-line phase and at a later stage is dominated by emission from the dust that formed in this nova. A detailed model is computed to identify and study characteristics of the spectral lines. Inferences from the model address the vexing question of which novae have the ability to form dust. It is demonstrated, and strikingly corroborated with observations, that the presence of lines in the early spectra of low-ionization species like Na and Mg - indicative of low temperature conditions - appear to be reliable indicators that dust will form in the ejecta. It is theoretically expected that mass loss during a nova outburst is a sustained process. Spectroscopic evidence for such a sustained mass loss, obtained by tracing the evolution of a P-Cygni feature in the Brackett gamma line, is presented here allowing a lower limit of 25-27 days to be set for the mass-loss duration. Photometric data recording the nova's extended 12 day climb to peak brightness after discovery is used to establish an early fireball expansion and also show that the ejection began well before maximum brightness. The JHK light curves indicate the nova had a fairly strong second outburst around 100 days after the first.

  7. Isotopic 32S/33S ratio as a diagnostic of presolar grains from novae

    E-Print Network [OSTI]

    A. Parikh; K. Wimmer; T. Faestermann; R. Hertenberger; J. Jose; H. -F. Wirth; C. Hinke; R. Krucken; D. Seiler; K. Steiger; K. Straub

    2014-09-01T23:59:59.000Z

    Measurements of sulphur isotopes in presolar grains can help to identify the astrophysical sites in which these grains were formed. A more precise thermonuclear rate of the 33S(p,gamma)34Cl reaction is required, however, to assess the diagnostic ability of sulphur isotopic ratios. We have studied the 33S(3He,d)34Cl proton-transfer reaction at 25 MeV using a high-resolution quadrupole-dipole-dipole-dipole magnetic spectrograph. Deuteron spectra were measured at ten scattering angles between 10 and 55 degrees. Twenty-four levels in 34Cl over Ex = 4.6 - 5.9 MeV were observed, including three levels for the first time. Proton spectroscopic factors were extracted for the first time for levels above the 33S+p threshold, spanning the energy range required for calculations of the thermonuclear 33S(p,gamma)34Cl rate in classical nova explosions. We have determined a new 33S(p,gamma)34Cl rate using a Monte Carlo method and have performed new hydrodynamic nova simulations to determine the impact on nova nucleosynthesis of remaining nuclear physics uncertainties in the reaction rate. We find that these uncertainties lead to a factor of less than 5 variation in the 33S(p,gamma)34Cl rate over typical nova peak temperatures, and variation in the ejected nova yields of S--Ca isotopes by less than 20%. In particular, the predicted 32S/33S ratio is 110 - 130 for the nova model considered, compared to 110 - 440 with previous rate uncertainties. As recent type II supernova models predict ratios of 130 - 200, the 32S/33S ratio may be used to distinguish between grains of nova and supernova origin.

  8. Economic incentives for hazardous-waste management: Deposit-refunded systems and used lubricating oil

    SciTech Connect (OSTI)

    Belzer, R.B.

    1989-01-01T23:59:59.000Z

    Economic incentives have been widely advocated for controlling environmental externalities. There has been increasing interest in devising such incentives to reduce the generation of hazardous waste. It is demonstrated that since firms comply with existing disposal rules, there is no efficiency basis for additional incentives. In contrast, incentives may be appropriate for firms that do not comply with existing rules. A range of regulatory instruments is compared, including taxes on inputs and waste generation, and subsidies for safe disposal and waste minimization. Each instrument has undesirable properties. Waste-end taxes encourage illegal disposal; safe-disposal subsides stimulate waste generation; and waste-minimization subsidies cannot be effectively targeted. The economic incentive instrument proposed is a combination of input taxes and safe-disposal subsidies, sometime manifest in the deposit-refund system. This instrument is efficiency-enhancing under plausible real-world conditions. The theoretical results are applied to the case of used lubricating oil, a large-volume waste stream that has vexed regulators for many years. An empirical model is developed that enables the simulation of prices, quantities, and net social benefits resulting from the establishment of a tax-subsidy or deposit-refund system. This model accounts for variations in: price-responsiveness; residual external damage from disposal; ex ante rates of regulatory compliance; and the level of transactions costs implied by the program. The instrument offers positive net social benefits, but only under a narrow range of conditions. The model is modified to apply to a generic hazardous waste problem that emphasizes illegal dumping. The existence of positive net social benefits depends on differences in risk across disposal options, the ex ante level of regulatory compliance, and the magnitude of unit transactions costs.

  9. A Global Review of Incentive Programs to Accelerate Energy-Efficient Appliances and Equipment

    SciTech Connect (OSTI)

    de la Rue du Can, Stephane; Phadke, Amol; Leventis, Greg; Gopal, Anand

    2013-08-01T23:59:59.000Z

    Incentive programs are an essential policy tool to move the market toward energy-efficient products. They offer a favorable complement to mandatory standards and labeling policies by accelerating the market penetration of energy-efficient products above equipment standard requirements and by preparing the market for increased future mandatory requirements. They sway purchase decisions and in some cases production decisions and retail stocking decisions toward energy-efficient products. Incentive programs are structured according to their regulatory environment, the way they are financed, by how the incentive is targeted, and by who administers them. This report categorizes the main elements of incentive programs, using case studies from the Major Economies Forum to illustrate their characteristics. To inform future policy and program design, it seeks to recognize design advantages and disadvantages through a qualitative overview of the variety of programs in use around the globe. Examples range from rebate programs administered by utilities under an Energy-Efficiency Resource Standards (EERS) regulatory framework (California, USA) to the distribution of Eco-Points that reward customers for buying efficient appliances under a government recovery program (Japan). We found that evaluations have demonstrated that financial incentives programs have greater impact when they target highly efficient technologies that have a small market share. We also found that the benefits and drawbacks of different program design aspects depend on the market barriers addressed, the target equipment, and the local market context and that no program design surpasses the others. The key to successful program design and implementation is a thorough understanding of the market and effective identification of the most important local factors hindering the penetration of energy-efficient technologies.

  10. White Dwarf Heating and Subsequent Cooling in Dwarf Nova Outbursts

    E-Print Network [OSTI]

    Anthony L. Piro; Phil Arras; Lars Bildsten

    2005-03-30T23:59:59.000Z

    We follow the time dependent thermal evolution of a white dwarf (WD) undergoing sudden accretion in a dwarf nova outburst, using both simulations and analytic estimates. The post-outburst lightcurve clearly separates into early times when the WD flux is high, and late times when the flux is near the quiescent level. The break between these two regimes, occurring at a time of order the outburst duration, corresponds to a thermal diffusion wave reaching the base of the freshly accreted layer. Our principal result is that long after the outburst, the fractional flux perturbation about the quiescent flux decays as a power law with time (and {\\it not} as an exponential). We use this result to construct a simple fitting formula that yields estimates for both the quiescent flux and the accreted column, i.e. the total accreted mass divided by WD surface area. The WD mass is not well constrained by the late time lightcurve alone, but it can be inferred if the accreted mass is known from observations. We compare our work with the well-studied outburst of WZ Sge, finding that the cooling is well described by our model, giving an effective temperature $T_{\\rm eff}=14,500 {\\rm K}$ and accreted column $\\Delta y\\approx10^6 {\\rm g cm^{-2}}$, in agreement with the modeling of Godon et al. To reconcile this accreted column with the accreted mass inferred from the bolometric accretion luminosity, a large WD mass $\\gtrsim1.1M_\\odot$ is needed. Our power law result is a valuable tool for making quick estimates of the outburst properties. We show that fitting the late time lightcurve with this formula yields a predicted column within 20% of that estimated from our full numerical calculations.

  11. Classical Novae as a Probe of the Cataclysmic Variable Population

    E-Print Network [OSTI]

    Dean M. Townsley; Lars Bildsten

    2005-03-24T23:59:59.000Z

    Classical Novae (CNe) are the brightest manifestation of mass transfer onto a white dwarf in a cataclysmic variable (CV). As such, they are probes of the mass transfer rate, Mdot, and WD mass, Mwd, in these interacting binaries. Our calculations of the dependence of the CN ignition mass, Mign, on Mdot and Mwd yields the recurrence times of these explosions. We show that the observed CNe orbital period distribution is consistent with the interrupted magnetic braking evolutionary scenario, where at orbital periods Porb > 3 hr mass transfer is driven by angular momentum loss via a wind from the companion star and at Porb < 3 hr by gravitational radiation. About 50% of CNe occur in binaries accreting at Mdot ~= 10^{-9} Msun/yr with Porb = 3-4 hr, with the remaining 50% split evenly between Porb longer (higher Mdot) and shorter (lower Mdot) than this. This resolution of the relative contribution to the CN rate from different CVs tells us that 3(9)x10^5 CVs with WD mass 1.0(0.6)Msun are needed to produce one CN per year. Using the K-band specific CN rate measured in external galaxies, we find a CV birthrate of 2(4)x10^{-4}/yr per 10^{10}Lsun,K, very similar to the luminosity specific Type Ia supernova rate in elliptical galaxies. Likewise, we predict that there should be 60-180 CVs for every 10^6Lsun,K in an old stellar population, similar to the number of X-ray identified CVs in the globular cluster 47 Tuc, showing no overabundance relative to the field. Using a two-component steady state model of CV evolution we show that the fraction of CVs which are magnetic (22%) implies a birthrate of 8% relative to non-magnetic CVs, similar to the fraction of strongly magnetic field WDs. (abridged)

  12. X-ray Study of Rekindled Accretion in the Classical Nova V2491 Cygni

    E-Print Network [OSTI]

    Takei, D; Tsujimoto, M; Kitamoto, S; Drake, J J; Osborne, J P; Takahashi, H; Kinugasa, K

    2011-01-01T23:59:59.000Z

    We conducted an X-ray spectroscopic study of the classical nova V2491 Cygni using our target-of-opportunity observation data with the Suzaku and XMM-Newton satellites as well as archived data with the Swift satellite. Medium-resolution (R~10-50) spectra were obtained using the X-ray CCD spectrometers at several post-nova epochs on days 9, 29, 40, 50, and 60-150 in addition to a pre-nova interval between days -322 and -100 all relative to the time when the classical nova was spotted. We found remarkable changes in the time series of the spectra: (a) In the pre-nova phase and on day 9, the 6.7 keV emission line from Fe XXV was significantly detected. (b) On day 29, no such emission line was found. (c) On day 40, the 6.7 keV emission line emerged again. (d) On days 50 and 60-150, three emission lines at 6.4, 6.7, and 7.0 keV respectively from quasi-neutral Fe, Fe XXV, and Fe XXVI were found. Statistically significant changes of the Fe K line intensities were confirmed between day 29 and 50. Based on these phenom...

  13. The Effects of Thermonuclear Reaction Rate Variations on Nova Nucleosynthesis: A Sensitivity Study

    E-Print Network [OSTI]

    Christian Iliadis; Art Champagne; Jordi Jose; Sumner Starrfield; Paul Tupper

    2002-06-03T23:59:59.000Z

    We investigate the effects of thermonuclear reaction rate uncertainties on nova nucleosynthesis. One-zone nucleosynthesis calculations have been performed by adopting temperature-density-time profiles of the hottest hydrogen-burning zone (i.e., the region in which most of the nucleosynthesis takes place). We obtain our profiles from 7 different, recently published, hydrodynamic nova simulations covering peak temperatures in the range from Tpeak=0.145-0.418 GK. For each of these profiles, we individually varied the rates of 175 reactions within their associated errors and analyzed the resulting abundance changes of 142 isotopes in the mass range below A=40. In total, we performed 7350 nuclear reaction network calculations. We use the most recent thermonuclear reaction rate evaluations for the mass ranges A=1-20 and A=20-40. For the theoretical astrophysicist, our results indicate the extent to which nova nucleosynthesis calculations depend on presently uncertain nuclear physics input, while for the experimental nuclear physicist our results represent at least a qualitative guide for future measurements at stable and radioactive ion beam facilities. We find that present reaction rate estimates are reliable for predictions of Li, Be, C and N abundances in nova nucleosynthesis. However, rate uncertainties of several reactions have to be reduced significantly in order to predict more reliable O, F, Ne, Na, Mg, Al, Si, S, Cl and Ar abundances. Results are presented in tabular form for each adopted nova simulation.

  14. Incentives to Accelerate the Penetration of Electricity in the Industrial Sector by Promoting New Technologies: A French Experiment

    E-Print Network [OSTI]

    Bouchet, J.; Froehlich, R.

    1983-01-01T23:59:59.000Z

    be effectively associated with them in particular in the form of dual energy installations. EXISTING INCENTIVES Some incentives have been provided by the State, others by E.D.F. State incentives are basically intended to promote energy savings. With a few... Several new approaches designed, tested and imple mented by E.D.F. and its partners, are supported by the Public Authorities. Their aim is to accelerate the design, availability to users and the widespread introduction of elec trical or dual-energy...

  15. Construction of AC Motor Controllers for NOvA Experiment Upgrades

    SciTech Connect (OSTI)

    Cooley, Patrick; /Fermilab; ,

    2011-08-04T23:59:59.000Z

    I have been constructing Alternating Current (AC) motor controllers for manipulation of particle beam detectors. The capability and reliability of these motor controllers are essential to the Laboratory's mission of accurate analysis of the particle beam's position. The device is moved in and out of the beam's path by the motor controller followed by the Neutrinos at the Main Injector Off-Axis {nu}{sub e} Appearance (NOvA) Experiment further down the beam pipe. In total, I built and tested ten ac motor controllers for new beam operations in the NOvA experiment. These units will prove to be durable and provide extremely accurate beam placement for NOvA Experiment far into the future.

  16. The Impact of Nuclear Reaction Rate Uncertainties on Evolutionary Studies of the Nova Outburst

    E-Print Network [OSTI]

    W. Raphael Hix; Michael S. Smith; Anthony Mezzacappa; Sumner Starrfield; Donald L. Smith

    2000-01-27T23:59:59.000Z

    The observable consequences of a nova outburst depend sensitively on the details of the thermonuclear runaway which initiates the outburst. One of the more important sources of uncertainty is the nuclear reaction data used as input for the evolutionary calculations. A recent paper by Starrfield, Truran, Wiescher, & Sparks (1998) has demonstrated that changes in the reaction rate library used within a nova simulation have significant effects, not just on the production of individual isotopes (which can change by an order of magnitude), but on global observables such as the peak luminosity and the amount of mass ejected. We present preliminary results of systematic analyses of the impact of reaction rate uncertainties on nova nucleosynthesis.

  17. Do Generation Firms in Restructured Electricity Markets Have Incentives to Support Social-Welfare-Improving Transmission Investments? *

    E-Print Network [OSTI]

    Oren, Shmuel S.

    electricity markets in the US, relies on locational marginal prices for energy to price and manage congestion of the incentive structures proposed in the literature have been broadly adopted. 1 While locational m

  18. Reference Models and Incentive Regulation of Electricity Distribution Networks: An Evaluation of Swedens Network Performance Assessment Model (NPAM)

    E-Print Network [OSTI]

    Jamasb, Tooraj; Pollitt, Michael G.

    The world-wide electricity sector reforms have led to a search for alternative and innovative approaches to regulation to promote efficiency improvement in the natural monopoly electricity networks. A number of countries have used incentive...

  19. Can historic neighborhoods compete? Analysis of and recommendations for local incentives for owner-occupied historic housing

    E-Print Network [OSTI]

    Rowe, Rebecca Elizabeth

    2005-02-17T23:59:59.000Z

    have been surveyed to discover what programs are being utilized and which might be successful in Texas cities. Also surveyed were prospective homebuyers to determine what incentives and maintenance assistance could induce them to purchase...

  20. Optical and Near-Infrared spectroscopy of Nova V1494 Aquilae 1999 #2

    E-Print Network [OSTI]

    Kamath, U S; Ashok, N M; Mayya, Y D; Sahu, D K

    2005-01-01T23:59:59.000Z

    Optical and near-infrared spectroscopic observations of the fast nova V1494 Aquilae 1999 #2 covering various phases -- early decline, transition and nebular -- during the first eighteen months of its post-outburst evolution are presented in this paper. During this period, the nova evolved in the P_fe P_fe^o C_o spectral sequence. The transition from an optically thick wind to a polar blob - equatorial ring geometry is seen in the evolution of the spectral line profiles. There is evidence of density and temperature stratification in the ejecta. Physical conditions in the ejecta have been estimated based on our observations.

  1. Optical and Near-Infrared spectroscopy of Nova V1494 Aquilae 1999 #2

    E-Print Network [OSTI]

    U. S. Kamath; G. C. Anupama; N. M. Ashok; Y. D. Mayya; D. K. Sahu

    2005-06-27T23:59:59.000Z

    Optical and near-infrared spectroscopic observations of the fast nova V1494 Aquilae 1999 #2 covering various phases -- early decline, transition and nebular -- during the first eighteen months of its post-outburst evolution are presented in this paper. During this period, the nova evolved in the P_fe P_fe^o C_o spectral sequence. The transition from an optically thick wind to a polar blob - equatorial ring geometry is seen in the evolution of the spectral line profiles. There is evidence of density and temperature stratification in the ejecta. Physical conditions in the ejecta have been estimated based on our observations.

  2. Analysis of how changed federal regulations and economic incentives affect financing of geothermal projects

    SciTech Connect (OSTI)

    Meyers, D.; Wiseman, E.; Bennett, V.

    1980-11-04T23:59:59.000Z

    The effects of various financial incentives on potential developers of geothermal electric energy are studied and the impact of timing of plant construction costs on geothermal electricity costs is assessed. The effect of the geothermal loan guarantee program on decisions by investor-owned utilities to build geothermal electric power plants was examined. The usefulness of additional investment tax credits was studied as a method for encouraging utilities to invest in geothermal energy. The independent firms which specialize in geothermal resource development are described. The role of municipal and cooperative utilities in geothermal resource development was assessed in detail. Busbar capital costs were calculated for geothermal energy under a variety of ownerships with several assumptions about financial incentives. (MHR)

  3. Making solar laws work: a study of state solar energy incentives

    SciTech Connect (OSTI)

    Roessner, J.D.

    1980-11-01T23:59:59.000Z

    The results of a research investigation of solar financial and research, demonstration, and development (RD and D) incentive programs in 18 states are summarized. The investigation focuses upon implementation - the organization and administrative processes required to convert a law into a viable program. Eleven financial and 12 RD and D programs were investigated. Results indicate that four conditions are common to successful implementation of both types of incentive programs: the opportunity to use solar energy as a heating source; characteristics of the agency selected to complement the law; involvement of outside groups in program implementation; and the specificity of guidance given to those responsible for implementation. Other conditions specific to the implementation of each type of program are discussed as well as the implications of these findings for state and federal policy makers.

  4. The Cost Reduction Incentive Program at the Savannah River Site. Audit report

    SciTech Connect (OSTI)

    NONE

    1998-05-01T23:59:59.000Z

    The Department of Energy (Department) established a Cost-Reduction Incentive Program (CRIP) at Westinghouse Savannah River Company (Westinghouse) in October 1992. In 1997, the Department performed a comprehensive review of Westinghouse`s performance-based incentives and cost-reduction incentives, and concluded that most of the savings identified through the CRIP occurred through greater management focus on reducing costs, working smart, or the results of budget constraints, as opposed to innovative changes in work methods and processes. The Assessment Team recommended that the Savannah River Operations Office (Operations Office) re-evaluate the effectiveness of the CRIP and consider either modifying the program to provide for payment only for innovative ideas, or cancel the program and utilize performance-based incentives to reward cost savings over some pre-established threshold. The objective of this audit was to determine whether the Operations Office took appropriate action in response to the Department`s internal assessment of the CRIP. The Operations Office did not take appropriate action in response to the internal assessment. The Operations Office stated that Westinghouse did not agree to the modification or cancellation of the CRIP, and the Department could not unilaterally modify or cancel the program because it was incorporated into the contract. However, the Operations Office could have substantially reduced its CRIP payments to Westinghouse without amending the contract by (1) enforcing the contract terms that required Westinghouse to use best commercial practices and industry standards in contract performance, and (2) requiring Westinghouse to comply with its internal procedures which required that cost-reduction proposals be innovative.

  5. Disability Insurance and the Dynamics of the Incentive-Insurance Tradeoff

    E-Print Network [OSTI]

    Low, Hamish; Pistaferri, Luigi

    2015-01-01T23:59:59.000Z

    Disability Insurance and the Dynamics of the Incentive-Insurance Tradeo#3; Hamish Low University of Cambridge Luigi Pistaferri Stanford University March 10, 2015 Abstract We provide a lifecycle framework for comparing the insurance value and the in... or work limitation shock which reduces the ability to work (distinguishing between severe and moderate shocks), a permanent productivity shock unrelated to health (such as a decline in the price of skills), and labor market frictions. Individuals dier ex...

  6. Inspection of the cost reduction incentive program at the Department of Energy`s Idaho Operations Office

    SciTech Connect (OSTI)

    Not Available

    1994-07-07T23:59:59.000Z

    The purpose of this inspection was to review the economy and efficiency of Idaho`s Fiscal Year 1992 Cost Reduction Incentive Program, as well as to provide information to Departmental officials regarding any difficulties in administering these types of programs. The report is of the findings and recommendations. According to Idaho officials, their Cost Reduction Incentive Program was designed to motivate and provide incentives to management and operating contractors which would result in cost savings to the Department while increasing the efficiency and effectiveness of the contractors` operations. Idaho officials reported that over $22.5 million in costs were saved as a result of the Fiscal Year 1992 Cost Reduction Incentive Program. It was found that: (1) Idaho officials acknowledged that they did not attempt a full accounting records validation of the contractor`s submitted cost savings; (2) cost reduction incentive programs may result in conflicts of interest--contractors may defer work in order to receive an incentive fee; (3) the Department lacks written Department-wide policies and procedures--senior Procurement officials stated that the 1985 memorandum from the then-Assistant Secretary for Management and Administration was not the current policy of the Department; and (4) the Department already has the management and operating contract award fee provisions and value engineering program that can be used to provide financial rewards for contractors that operate cost effectively and efficiently.

  7. Simulations of the symbiotic recurrent nova V407 Cyg. I. Accretion and shock evolutions

    E-Print Network [OSTI]

    Pan, Kuo-Chuan; Taam, Ronald E

    2015-01-01T23:59:59.000Z

    The shock interaction and evolution of nova ejecta with a wind from a red giant star in a symbiotic binary system are investigated via three-dimensional hydrodynamics simulations. We specifically model the March 2010 outburst of the symbiotic recurrent nova V407~Cygni from the quiescent phase to its eruption phase. The circumstellar density enhancement due to wind-white dwarf interaction is studied in detail. It is found that the density-enhancement efficiency depends on the ratio of the orbital speed to the red giant wind speed. Unlike another recurrent nova, RS~Ophiuchi, we do not observe a strong disk-like density enhancement, but instead observe an aspherical density distribution with $\\sim 20\\%$ higher density in the equatorial plane than at the poles. To model the 2010 outburst, we consider several physical parameters, including the red giant mass loss rate, nova eruption energy, and ejecta mass. A detailed study of the shock interaction and evolution reveals that the interaction of shocks with the red ...

  8. Quark-Novae, cosmic reionization, and early r-process element production

    E-Print Network [OSTI]

    R. Ouyed; R. E. Pudritz; P. Jaikumar

    2009-06-30T23:59:59.000Z

    We examine the case for Quark-Novae (QNe) as possible sources for the reionization and early metal enrichment of the universe. Quark-Novae are predicted to arise from the explosive collapse (and conversion) of sufficiently massive neutron stars into quark stars. A Quark-Nova (QN) can occur over a range of time scales following the supernova event. For QNe that arise days to weeks after the supernovae, we show that dual-shock that arises as the QN ejecta encounter the supernova ejecta can produce enough photons to reionize hydrogen in most of the Inter-Galactic medium (IGM) by z ~ 6. Such events can explain the large optical depth tau_e ~ 0.1 as measured by WMAP, if the clumping factor, C, of the material being ionized is smaller than 10. We suggest a way in which a normal initial mass function (IMF) for the oldest stars can be reconciled with a large optical depth as well as the mean metallicity of the early IGM post reionization. We find that QN also make a contribution to r-process element abundances for atomic numbers A > 130. We predict that the main cosmological signatures of Quark-Novae are the gamma-ray bursts that announce their birth. These will be clustered at redshifts in the range z ~ 7-8 in our model.

  9. The mass of the white dwarf in the old nova BT Mon

    E-Print Network [OSTI]

    D. A. Smith; V. S. Dhillon; T. R. Marsh

    1997-09-22T23:59:59.000Z

    We present spectrophotometry of the eclipsing old nova BT Mon (Nova Mon 1939). By detecting weak absorption features from the secondary star, we find its radial velocity semi-amplitude to be K_R = 205+/-5 km/s and its rotational velocity to be vsin i = 138+/-5 km/s. We also measure the radial velocity semi-amplitude of the primary star to be K_R = 170+/-10 km/s. From these parameters we obtain a mass of 1.04+/-0.06 M_sun for the white dwarf primary star and a mass of 0.87+/-0.06 M_sun for the G8V secondary star. The inclination of the system is found to be 82.2+/-3.2 deg and we estimate that the system lies at a distance of 1700+/-300pc. The high mass of the white dwarf and our finding that BT Mon was probably a fast nova together constitute a new piece of evidence in favour of the thermonuclear runaway model of classical nova outbursts. The emission lines are single peaked throughout the orbital cycle, showing absorption around phase 0.5, high velocity S-wave components and large phase offsets in their radial velocity curves. In each of these respects, BT Mon is similar to the SW Sex stars. We also find quasi-periodic flaring in the trailed spectra, which makes BT Mon a candidate intermediate polar.

  10. Engineering design of the Nova Laser Facility for inertial-confinement fusion

    SciTech Connect (OSTI)

    Simmons, W W; Godwin, R O; Hurley, C A; Wallerstein, E. P.; Whitham, K.; Murray, J. E.; Bliss, E. S.; Ozarski, R. G.; Summers, M. A.; Rienecker, F.; Gritton, D. G.; Holloway, F. W.; Suski, G. J.; Severyn, J. R.

    1982-01-25T23:59:59.000Z

    The design of the Nova Laser Facility for inertial confinement fusion experiments at Lawrence Livermore National Laboratory is presented from an engineering perspective. Emphasis is placed upon design-to-performance requirements as they impact the various subsystems that comprise this complex experimental facility.

  11. Design and implementation of a financial planning and tracking system for the Nova Project

    SciTech Connect (OSTI)

    Holcomb, F.

    1982-01-01T23:59:59.000Z

    The Nova project is a 185 million dollar DOE funded project to build an experimental facility to demonstrate the thermonuclear ignition of laser fusion targets. This paper describes the design and implementation considerations for the project's computerized performance measurement financial planning and tracking system and critiques its actual operation.

  12. Financial Analysis of Incentive Mechanisms to Promote Energy Efficiency: Case Study of a Prototypical Southwest Utility

    SciTech Connect (OSTI)

    Cappers, Peter; Goldman, Charles; Chait, Michele; Edgar, George; Schlegel, Jeff; Shirley, Wayne

    2009-03-04T23:59:59.000Z

    Many state regulatory commissions and policymakers want utilities to aggressively pursue energy efficiency as a strategy to mitigate demand and energy growth, diversify the resource mix, and provide an alternative to building new, costly generation. However, as the National Action Plan for Energy Efficiency (NAPEE 2007) points out, many utilities continue to shy away from aggressively expanding their energy efficiency efforts when their shareholder's fundamental financial interests are placed at risk by doing so. Thus, there is increased interest in developing effective ratemaking and policy approaches that address utility disincentives to pursue energy efficiency or lack of incentives for more aggressive energy efficiency efforts. New regulatory initiatives to promote increased utility energy efficiency efforts also affect the interests of consumers. Ratepayers and their advocates are concerned with issues of fairness, impacts on rates, and total consumer costs. From the perspective of energy efficiency advocates, the quid pro quo for utility shareholder incentives is the obligation to acquire all, or nearly all, achievable cost-effective energy efficiency. A key issue for state regulators and policymakers is how to maximize the cost-effective energy efficiency savings attained while achieving an equitable sharing of benefits, costs and risks among the various stakeholders. In this study, we modeled a prototypical vertically-integrated electric investor-owned utility in the southwestern US that is considering implementing several energy efficiency portfolios. We analyze the impact of these energy efficiency portfolios on utility shareholders and ratepayers as well as the incremental effect on each party when lost fixed cost recovery and/or utility shareholder incentive mechanisms are implemented. A primary goal of our quantitative modeling is to provide regulators and policymakers with an analytic framework and tools that assess the financial impacts of alternative incentive approaches on utility shareholders and customers if energy efficiency is implemented under various utility operating, cost, and supply conditions.We used and adapted a spreadsheet-based financial model (the Benefits Calculator) which was developed originally as a tool to support the National Action Plan for Energy Efficiency (NAPEE). The major steps in our analysis are displayed graphically in Figure ES- 1. Two main inputs are required: (1) characterization of the utility which includes its initial financial and physical market position, a forecast of the utility?s future sales, peak demand, and resource strategy to meet projected growth; and (2) characterization of the Demand-Side Resource (DSR) portfolio ? projected electricity and demand savings, costs and economic lifetime of a portfolio of energy efficiency (and/or demand response) programs that the utility is planning or considering implementing during the analysis period. The Benefits Calculator also estimates total resource costs and benefits of the DSR portfolio using a forecast of avoided capacity and energy costs. The Benefits Calculator then uses inputs provided in the Utility Characterization to produce a ?business-as usual? base case as well as alternative scenarios that include energy efficiency resources, including the corresponding utility financial budgets required in each case. If a decoupling and/or a shareholder incentive mechanism are instituted, the Benefits Calculator model readjusts the utility?s revenue requirement and retail rates accordingly. Finally, for each scenario, the Benefits Calculator produces several metrics that provides insights on how energy efficiency resources, decoupling and/or a shareholder incentive mechanism impacts utility shareholders (e.g. overall earnings, return on equity), ratepayers (e.g., average customer bills and rates) and society (e.g. net resource benefits).

  13. Underground study of the 17 O(p,? )18F reaction at Gamow energies for classical novae

    E-Print Network [OSTI]

    Scott, David Andrew

    2014-11-27T23:59:59.000Z

    Classical novae are explained as thermonuclear explosions on the surface of white dwarf stars accreting hydrogen-rich material from less evolved companions in binary star systems. These events occur frequently within our ...

  14. Renewable Energy Cost Modeling: A Toolkit for Establishing Cost-Based Incentives in the United States; March 2010 -- March 2011

    SciTech Connect (OSTI)

    Gifford, J. S.; Grace, R. C.; Rickerson, W. H.

    2011-05-01T23:59:59.000Z

    This report is intended to serve as a resource for policymakers who wish to learn more about establishing cost-based incentives. The report will identify key renewable energy cost modeling options, highlight the policy implications of choosing one approach over the other, and present recommendations on the optimal characteristics of a model to calculate rates for cost-based incentives, feed-in tariffs (FITs), or similar policies. These recommendations will be utilized in designing the Cost of Renewable Energy Spreadsheet Tool (CREST). Three CREST models will be publicly available and capable of analyzing the cost of energy associated with solar, wind, and geothermal electricity generators. The CREST models will be developed for use by state policymakers, regulators, utilities, developers, and other stakeholders to assist them in current and future rate-setting processes for both FIT and other renewable energy incentive payment structures and policy analyses.

  15. Tax Incentives

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

    of 1992, allows owners of qualified over a 10-year period. Qualified wind wind turbines (indexed for inflation). - The federal Renewable Electricity Production Tax Credit...

  16. Tax Incentives

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently AskedEnergyIssues DOE'sSummaryDepartmentEnergyonWIPPDepartmentBlueTax

  17. incentive2

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently20,000 Russian Nuclearand Characterization of aShiprock)Report

  18. Gamma Ray Bursts within the Quark-Nova scenario: Precursor, prompt and afterglow phases

    E-Print Network [OSTI]

    Ouyed, Rachid; Niebergal, Brian; Staff, Jan

    2007-01-01T23:59:59.000Z

    By exploring the dynamical and thermal evolution of the iron-rich ejecta in a Quark-Nova explosion we find that the ejecta breaks up into multiple subjets. If the quark-nova occurs inside a collapsar, the interaction between these subjets and collapsar envelope, in the case of a failed and successful supernova, leads to features indicative of those observed in Gamma Ray Bursts. These features include: (i) precursor activity (optical, X-ray, gamma-ray), (ii) prompt gamma-ray emission, and (iii) afterglow emission. We discuss SN-less long duration GRBs, short hard GRBs (including association and non-association with star forming regions), dark GRBs, as well as the energetic X-ray flares detected in Swift GRBs in our model.

  19. Genetic and environmental factors affecting growth and reproduction characters of Morada Nova sheep in Northeastern Brazil

    E-Print Network [OSTI]

    Fernandes, Antonio Amaury Oria

    1985-01-01T23:59:59.000Z

    sheep was raised at the Fazenda Iracema-Sertao Central Research Unit which belongs to the "Empresa de Pesquisa Agropecuaria do Ceara" (EPACE). The Fazenda Iracema is located at Quixada, Ceara, Brazil situ- Table 3 Summary of the Experimental Morada... collected over a 6-year period (1979-1984) from the Morada Nova sheep flock (Figure 2) maintained by the Experimental Research Unit of the "Empresa de Pesquisa Agropecuaria do Ceara" (EPACE) at the Experimental Iracema Farm, Quixada, Ceara, Brazil...

  20. The enigmatic outburst of V445 Puppis - a possible Helium nova?

    E-Print Network [OSTI]

    N. M. Ashok; D. P. K. Banerjee

    2003-07-16T23:59:59.000Z

    JHK spectroscopic and photometric observations are reported for the enigmatic, nova-like, variable V445 Puppis which erupted at the end of 2000. The near-IR spectra are hydrogen-deficient and unusually rich in CI lines. The important CI lines are found to be positioned at 1.133, 1.166, 1.175, 1.189, 1.26 and 1.689 microns. Model calculations for the CI lines are done to make the identification of the lines secure. Photometric data, taken on January 2.90 UT, 2001 shortly after the outburst, show the formation of an optically thin dust shell around V445 Puppis. The temperature and upper limit for the mass of the dust shell are estimated to be 1800K and M(dust) ~ 1oe-9 M(sun) respectively . A subsequent episode of massive dust formation - indicated by the observed, deep visual dimming - is also seen in JHK images of early November 2001. V445 Puppis has shown two unusual properties for a nova i) the hydrogen-deficiency and He/C enrichment of the object as seen from optical and IR data and ii) synchrotron radio emission which was detected nearly a year after it's outburst by other workers. The strange nature of the object is discussed and it is shown that it is difficult to place it in the known categories of eruptive variables viz. novae (classical, recurrent or symbiotic); born-again AGB stars; the new class of eruptive variables like V838 Mon; and RCB/HdC stars. Tentative evidence for an accretion disk and binarity of the V445 Puppis system is presented. It is debated whether V445 Puppis is a rare Helium nova or an unique object.

  1. Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst

    E-Print Network [OSTI]

    Jeremy Shears; Roger Pickard; Tom Krajci; Gary Poyner

    2007-05-31T23:59:59.000Z

    During 2006 November an outburst of the dwarf nova AW Sge was observed using CCD photometry. This revealed 0.25 magnitude superhumps confirming it to be a superoutburst, possibly only the second confirmed such outburst of this star. The superhumps were observed for 4 days and had a stable period Psh = 0.0745(2)d, a value which is consistent with Psh measured during the 2000 superoutburst.

  2. Nova Virgem :b the story of a nineteenth-century Brazilian slave smuggler

    E-Print Network [OSTI]

    Miller, Mason Daniel

    2001-01-01T23:59:59.000Z

    HISTORICAL BACKGROUND . Thc Eighteenth Century Slave frade and British Domestic Abolition A "Judicious Mixture of Bullying 'md Bribery' Brazilian Independence and the Abolition of the Slave Trade III LEGALITIES OF ILLEGALITY British Presence on thc... , . . . 27 . . . . . 29 . . . . . 33 . . . . . 36 CHAPTER Page IV THE NOVA VIRGFM . . . 41 Background: The Pre-Ninetccnth Century Slaver. . . The Illegal Era Slave Ship Arqucacgo or Lotaqao: How Big Was this Ship? . . . . Thc Hull of the Nr...

  3. Incentive Compatible Online Scheduling of Malleable Parallel Jobs with Individual Deadlines

    SciTech Connect (OSTI)

    Carroll, Thomas E.; Grosu, Daniel

    2010-09-13T23:59:59.000Z

    We consider the online scheduling of malleable jobs on parallel systems, such as clusters, symmetric multiprocessing computers, and multi-core processor computers. Malleable jobs is a model of parallel processing in which jobs adapt to the number of processors assigned to them. This model permits the scheduler and resource manager to make more ef?cient use of the available resources. Each malleable job is characterized by arrival time, deadline, and value. If the job completes by its deadline, the user earns the payoff indicated by the value; otherwise, she earns a payoff of zero. The scheduling objective is to maximize the sum of the values of the jobs that complete by their associated deadlines. Complicating the matter is that users in the real world are rational and they will attempt to manipulate the scheduler by misreporting their jobs parameters if it bene?ts them to do so. To mitigate this behavior, we design an incentive compatible online scheduling mechanism. Incentive compatibility assures us that the users will obtain the maximum payoff only if they truthfully report their jobs parameters to the scheduler. Finally, we simulate and study the mechanism to show the effects of misreports on the cheaters and on the system.

  4. Thermal radio emission from novae & symbiotics with the Square Kilometre Array

    E-Print Network [OSTI]

    O'Brien, Tim; Chomiuk, Laura; Ribeiro, Valerio; Bode, Michael; Sokoloski, Jennifer; Woudt, Patrick

    2015-01-01T23:59:59.000Z

    The thermal radio emission of novae during outburst enables us to derive fundamental quantities such as the ejected mass, kinetic energy, and density profile of the ejecta. Recent observations with newly-upgraded facilities such as the VLA and e-MERLIN are just beginning to reveal the incredibly complex processes of mass ejection in novae (ejections appear to often proceed in multiple phases and over prolonged timescales). Symbiotic stars can also exhibit outbursts, which are sometimes accompanied by the expulsion of material in jets. However, unlike novae, the long-term thermal radio emission of symbiotics originates in the wind of the giant secondary star, which is irradiated by the hot white dwarf. The effect of the white dwarf on the giant's wind is strongly time variable, and the physical mechanism driving these variations remains a mystery (possibilities include accretion instabilities and time-variable nuclear burning on the white dwarf's surface). The exquisite sensitivity of SKA1 will enable us to su...

  5. DYNAMICAL FRAGMENTATION OF THE T PYXIDIS NOVA SHELL DURING RECURRENT ERUPTIONS

    SciTech Connect (OSTI)

    Toraskar, Jayashree; Mac Low, Mordecai-Mark; Shara, Michael M.; Zurek, David R., E-mail: toraskar@amnh.org, E-mail: mordecai@amnh.org, E-mail: mshara@amnh.org, E-mail: dzurek@amnh.org [Department of Astrophysics, American Museum of Natural History, 79th Street at Central Park West, New York, NY 10024-5192 (United States)

    2013-05-01T23:59:59.000Z

    Hubble Space Telescope images of the ejecta surrounding the nova T Pyxidis resolve the emission into more than 2000 bright knots. We simulate the dynamical evolution of the ejecta from T Pyxidis during its multiple eruptions over the last 150 years using the adaptive mesh refinement code Ramses. We demonstrate that the observed knots are the result of Richtmyer-Meshkov gas dynamical instabilities (the equivalent of Rayleigh-Taylor instabilities in an accelerated medium). These instabilities are caused by the overrunning of the ejecta from the classical nova of 1866 by fast-moving ejecta from the six subsequent recurrent nova outbursts. Magnetic fields may play a role in determining knot scale and preventing their conductive evaporation. The model correctly predicts the observed expansion and dimming of the T Pyx ejecta as well as the knotty morphology. The model also predicts that deeper, high-resolution imagery will show filamentary structure connecting the knots. We show reprocessed Hubble Space Telescope imagery that shows the first hints of such a structure.

  6. Gamma-ray novae as probes of relativistic particle acceleration at non-relativistic shocks

    E-Print Network [OSTI]

    Metzger, Brian D; Vurm, Indrek; Hascoet, Romain; Beloborodov, Andrei M; Chomiuk, Laura

    2015-01-01T23:59:59.000Z

    The Fermi LAT discovery that classical novae produce >100 MeV gamma-rays establishes that shocks and relativistic particle acceleration are key features of these events. These shocks are likely to be radiative due to the high densities of the nova ejecta at early times coincident with the gamma-ray emission. Thermal X-rays radiated behind the shock are absorbed by neutral gas and reprocessed into optical emission, similar to Type IIn (interacting) supernovae. The ratio of gamma-ray and optical luminosities, L_gam/L_opt, thus sets a lower limit on the fraction of the shock power used to accelerate relativistic particles, e_nth. The measured values of L_gam/L_opt for two classical novae, V1324 Sco and V339 Del, constrains e_nth > 1e-2 and > 1e-3, respectively. Inverse Compton models for the gamma-ray emission are disfavored given the low electron acceleration efficiency, e_nth ~ 1e-4-1e-3, inferred from observations of Galactic cosmic rays and particle-in-cell (PIC) numerical simulations. Recent hybrid PIC simu...

  7. Beacons In the Dark: Using Novae and Supernovae to Detect Dwarf Galaxies in the Local Universe

    E-Print Network [OSTI]

    Conroy, Charlie

    2015-01-01T23:59:59.000Z

    We propose that luminous transients, including novae and supernovae, can be used to detect the faintest galaxies in the universe. Beyond a few Mpc, dwarf galaxies with stellar masses $<10^6 M_{\\odot}$ will likely be too faint and/or too low in surface brightness to be directly detected in upcoming large area ground-based photometric surveys. However, single epoch LSST photometry will be able to detect novae to distances of $\\sim30$ Mpc and SNe to Gpc-scale distances. Depending on the form of the stellar mass-halo mass relation and the underlying star formation histories of low mass dwarfs, the expected nova rates will be a few to $\\sim100$ yr$^{-1}$ and the expected SN rates (including both type Ia and core-collapse) will be $\\sim10^2-10^4$ within the observable ($4\\pi$ sr) volume. The transient rate associated with intrahalo stars will be comparably large, but these transients will be located close to bright galaxies, in contrast to the dwarfs, which should trace the underlying large scale structure of th...

  8. Welcome to the new digital College of Medicine research incentive award nomination process! The digital system has been initiated in order to ensure accuracy of documentation and to

    E-Print Network [OSTI]

    Wu, Shin-Tson

    Welcome to the new digital College of Medicine research incentive award nomination process the committee review process. The following checklist can be used to track your application progress. Once you for the grants funded during the 5 year review period College of Medicine Research Incentive Awards 2013 2014

  9. Consolidating N.J.'s clean-tech resources into database for Online center a one-stop center for incentives, assistance programs

    E-Print Network [OSTI]

    Delgado, Mauricio

    -stop center for incentives, assistance programs By J. Kaltwasser, www.NJBIZ.com 4/16/12 The Garden State-to-use database bringing together information about incentives and business assistance programs at the state president for economic development at Rutgers, said the site is critical because it promotes the state

  10. EMPLOYEE STOCK OPTIONS INCENTIVE EFFECTS: A CPT-BASED MODEL Hamza BAHAJI, DRM Finance,Universit de Paris Dauphine, France

    E-Print Network [OSTI]

    Boyer, Edmond

    employee behaviour in terms of risk taking. Most of the theoretical literature on stock options relies to predict stock options as part of the compensation contract. Several quantitative studies taking placeEMPLOYEE STOCK OPTIONS INCENTIVE EFFECTS: A CPT-BASED MODEL Hamza BAHAJI, DRM Finance,Université de

  11. A deciso judicial apoiada na Nova Economia Institucional: Acertos e erros dos magistrados brasileiros no caso de reviso dos contratos de arrendamento mercantil de automveis indexados ao dlar

    E-Print Network [OSTI]

    Bertran, Maria Paula

    2007-01-01T23:59:59.000Z

    judicial apoiada na Nova Economia Institucional: Acertos ede S. Paulo FD/USP. - Graduanda em Economia pelaFaculdade de Economia, Administrao e Contabilidade da

  12. FY 1996 performance evaluation and incentive fee agreement for the Pacific Northwest National Laboratory

    SciTech Connect (OSTI)

    NONE

    1996-01-08T23:59:59.000Z

    The document describes the critical outcomes, objectives, performance indicators, expected levels of performance, specific detail on incentive fee, and agreements concerning the evaluation of the Pacific Northwest National Laboratory`s FY 1996 Self-Assessment. This information will be the basis for the evaluation of the Laboratory`s performance as required by Articles H-24 and H-25 of the Contract. For the period October 1, 1995 through September 30, 1996, the Parties have agreed to measure and evaluate the individual areas of Laboratory activities identified herein. This reflects the fact that the Contractor will be evaluated on two dimensions, namely (1) accomplishment of critical outcomes and (2) the effectiveness of the Contractor`s self-assessment program. Each area will receive its own evaluation rating and they will be combined to determined an overall rating with the first area weighted at 75% and the second area weighted at 25%.

  13. Report on inspection of the performance based incentive program at the Richland Operations Office

    SciTech Connect (OSTI)

    NONE

    1997-03-10T23:59:59.000Z

    The Fiscal Year (FY) 1995 Performance Based Incentive (PBI) Program at the Department of Energy`s (DOE) Richland Operations Office (Richland) was initiated by Richland as one part of the broader DOE Contract Reform Initiative being implemented at the Hanford Site in FY 1995. This program was identified as an area of concern by the Office of Inspections as a result of previous inspection work. Specifically, during a limited review of the construction of an Effluent Treatment Facility at the Hanford Site, we were unable to identify any written policies describing PBI program controls or implementation procedures. We were told that Richland Operations Office Program Management personnel were not directly involved in the selection of the Effluent Treatment Facility project for the PBI Program, or in the determination that this particular PBI would be established with a potential fee of $1 million.

  14. Financing alternatives and incentives for solar-thermal central-receiver systems

    SciTech Connect (OSTI)

    Bos, P.B.

    1982-07-01T23:59:59.000Z

    As a result of various recently enacted incentive and regulatory legislation combined with the new administration policy and budgetary guidelines, the commercialization of solar thermal central receiver systems will involve financing alternatives other than conventional utility financing. This study was conducted to identify these potential financing alternatives and the associated requirements and impacts on the Department of Energy program. Based upon this analysis, it is concluded that the current alternative financing window is extremely short (through 1985), and that an extension or at the least a gradual phasing out, of the solar tax credits is necessary for the successful transfer of the central receiver technology to the private sector. Furthermore, throughout this time period, continued government support of the R and D activities is necessary to provide the necessary confidence in this technology for the private (financial) sector to underwrite this technology transfer. Consequently, even though the central receiver technology shows high promise for replacing a significant fraction of the oil/gas-fired utility industry peaking and intermediate generation, the current readiness status of this technology still requires further direct and indirect government support for a successful technology transfer. The direct government research and development support will provide the basis for a technological readiness and confidence, whereas the indirect tax incentive support serves to underwrite the extraordinary risks associated with the technology transfer. These support requirements need only be limited to and decreasing during this technology transfer phase, since as the systems approach successful full-scale commercialization, the extraordinary risks will be gradually eliminated. At the time of commercialization the system's value should be on a par with the installed system's cost.

  15. Economic Incentives for Cybersecurity: Using Economics to Design Technologies Ready for Deployment

    SciTech Connect (OSTI)

    Vishik, Claire [Intel Corporation] [Intel Corporation; Sheldon, Frederick T [ORNL] [ORNL; Ott, David [Intel Corporation] [Intel Corporation

    2013-01-01T23:59:59.000Z

    Cybersecurity practice lags behind cyber technology achievements. Solutions designed to address many problems may and do exist but frequently cannot be broadly deployed due to economic constraints. Whereas security economics focuses on the cost/benefit analysis and supply/demand, we believe that more sophisticated theoretical approaches, such as economic modeling, rarely utilized, would derive greater societal benefits. Unfortunately, today technologists pursuing interesting and elegant solutions have little knowledge of the feasibility for broad deployment of their results and cannot anticipate the influences of other technologies, existing infrastructure, and technology evolution, nor bring the solutions lifecycle into the equation. Additionally, potentially viable solutions are not adopted because the risk perceptions by potential providers and users far outweighs the economic incentives to support introduction/adoption of new best practices and technologies that are not well enough defined. In some cases, there is no alignment with redominant and future business models as well as regulatory and policy requirements. This paper provides an overview of the economics of security, reviewing work that helped to define economic models for the Internet economy from the 1990s. We bring forward examples of potential use of theoretical economics in defining metrics for emerging technology areas, positioning infrastructure investment, and building real-time response capability as part of software development. These diverse examples help us understand the gaps in current research. Filling these gaps will be instrumental for defining viable economic incentives, economic policies, regulations as well as early-stage technology development approaches, that can speed up commercialization and deployment of new technologies in cybersecurity.

  16. Earth System History Announcements

    E-Print Network [OSTI]

    Mojzsis, Stephen J.

    Earth System History GEOL 1020 [35] Announcements The demise of the Paleozoic (extinction, Nova Scotia. #12;The Carboniferous was marked by the progressive formation of the supercontinent Pangea, there is evidence of significant cooling and drying in the sedimentologi

  17. Preparing for the peak: Energy security and Atlantic Canada

    E-Print Network [OSTI]

    Hughes, Larry

    Hydroelectricity Uranium Canada is not "energy homogenous" #12;Atlantic Canada Older housing stock Declining-Mobil) No exploration >90% exported Some coal Government and Nova Scotia Power: Yes: FERC 888/889 Slow: RPS Slower

  18. International Conference on Ocean Energy | Department of Energy

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

    on Ocean Energy International Conference on Ocean Energy November 4, 2014 1:00PM EST to November 6, 2014 10:00PM EST Halifax, Nova Scotia, Canada http:www.icoe2014canada.org...

  19. Quantifying atmospheric pollution across north america from boreal forest fires: a combined analysis of atmospheric modelling and ground-based remote sensing

    E-Print Network [OSTI]

    Trigwell, Robert

    2011-11-24T23:59:59.000Z

    This paper describes the interpretation of the 2010 summer LIDAR observations from Dal- housie University, Nova Scotia. The GEOS-Chem global 3D chemistry transport model was used to identify the chemical and optical ...

  20. Aircraft-protection radar for use with atmospheric lidars Thomas J. Duck, Bernard Firanski, Frank D. Lind, and Dwight Sipler

    E-Print Network [OSTI]

    Duck, Thomas J.

    . Lind, and Dwight Sipler A modified X-band radar system designed to detect aircraft during atmospheric, Dalhousie Univer- sity, Halifax, Nova Scotia, Canada B3H 3J5. F. D. Lind and D. Sipler are with Haystack

  1. THE BIG PICTURE: A "FISHERY SYSTEM APPROACH"

    E-Print Network [OSTI]

    Charles, Anthony

    , and its lengthy history combined with its rather narrow definition have had a negative impact in limiting Charles Management Science / Environmental Studies Saint Mary's University Halifax, Nova Scotia B3H3C3

  2. 3, 32673299, 2003 Relative humidity and

    E-Print Network [OSTI]

    Deutsches Zentrum fur Luft- und Raumfahrt (DLR), Institut fur Physik der Atmosphare (IPA, Sweden 3 Dalhousie University, Department of Physics and Atmospheric Science, Halifax, Nova Scotia

  3. Notices

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

    a Canadian company incorporated pursuant to the laws of Nova Scotia, and that Bear Head (USA) is a Delaware limited liability company. Both have their principal place of business...

  4. Green University Planning Committee Friday, January 18, 2013

    E-Print Network [OSTI]

    Northern British Columbia, University of

    Solar PV proposal differs significantly from initial proposal - Motion: Solar PV Proposal to be included Cooperative, Small-scale wind (Nova Scotia), Data server farm - To be discussed with Energy Subcommittee B

  5. Teaching Humanities in Medicine: The University of Massachusetts Family Medicine Residency Program Experience

    E-Print Network [OSTI]

    Silk, Hugh; Shields, Sara

    2012-01-01T23:59:59.000Z

    Charon R. Narrative and medicine. N Eng J Med 2004;350:862-California, Irvine, College of Medicine. Acad Med. 2003;78:University Faculty of Medicine, Nova Scotia, Canada, 1992

  6. The OGLE-II event sc5_2859 a Classical Nova outburst?

    E-Print Network [OSTI]

    Afonso, C; Andersen, J; Ansari, R; Aubourg, E; Bareyre, P; Beaulieu, J P; Blanc, G; CSmith, M; Charlot, X; Coutures, C; De Kat, J; Ferlet, R; Fouqu, P; Glicenstein, J F; Goldman, B; Gould, A; Graff, D; Gros, M; Hamadache, C; Hassinski, J; Le Guillou, Laurent; Lesquoy, E; Loup, C; Magneville, C; Marquette, J B; Maurice, E; Maury, A; Milsztajn, A; Moniez, M; Palanque-Delabrouille, Nathalie; Perdereau, O; Prvt, L; Rahal, Y R; Rich, J; Spiro, M; Tisserand, P; Vidal-Madjar, A; Vigroux, L; Wagner, R M; Zylberajch, S

    2006-01-01T23:59:59.000Z

    The OGLE-II event sc5_2859 was previously identified as the third longest microlensing event ever observed. Additional photometric observations from the EROS (Experience de Recherche d'Objets Sombres) survey and spectroscopic observations of the candidate star are used to test the microlensing hypothesis.The combined OGLE and EROS data provide a high quality coverage of the light curve. The colour of the sc5_2859 event is seen to change with time. A spectrum taken in 2003 exhibits a strong Halpha emission line. The additionnal data show that the OGLE-II sc5_2859 event is actually a classical nova outburst.

  7. Classical novae and type I X-ray bursts: Challenges for the 21st century

    SciTech Connect (OSTI)

    Parikh, A., E-mail: anuj.r.parikh@upc.edu; Jos, J., E-mail: jordi.jose@upc.edu; Sala, G., E-mail: gloria.sala@upc.edu [Departament de Fsica i Enginyeria Nuclear, Universitat Politcnica de Catalunya (EUETIB), E-08036 Barcelona (Spain); Institut dEstudis Espacials de Catalunya (IEEC), E-08034 Barcelona (Spain)

    2014-04-15T23:59:59.000Z

    Classical nova explosions and type I X-ray bursts are the most frequent types of thermonuclear stellar explosions in the Galaxy. Both phenomena arise from thermonuclear ignition in the envelopes of accreting compact objects in close binary star systems. Detailed observations of these events have stimulated numerous studies in theoretical astrophysics and experimental nuclear physics. We discuss observational features of these phenomena and theoretical efforts to better understand the energy production and nucleosynthesis in these explosions. We also examine and summarize studies directed at identifying nuclear physics quantities with uncertainties that significantly affect model predictions.

  8. X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku

    E-Print Network [OSTI]

    Masahiro Tsujimoto; Dai Takei; Jeremy J. Drake; Jan-Uwe Ness; Shunji Kitamoto

    2008-10-17T23:59:59.000Z

    We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 days after the explosion using the Suzaku satellite. With a 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows K lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single temperature (0.64 keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ~3e21/cm2, a flux of ~1e-12 erg/s/cm2, and a luminosity of ~6e34 erg/s in the 0.3-3.0 keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova.

  9. X-Ray Spectroscopy of the Classical Nova V458 Vulpeculae with Suzaku

    E-Print Network [OSTI]

    Tsujimoto, Masahiro; Drake, Jeremy J; Ness, Jan-Uwe; Kitamoto, Shunji

    2008-01-01T23:59:59.000Z

    We conducted a target of opportunity X-ray observation of the classical nova V458 Vulpeculae 88 days after the explosion using the Suzaku satellite. With a 20 ks exposure, the X-ray Imaging Spectrometer detected X-ray emission significantly harder than typical super-soft source emission. The X-ray spectrum shows K lines from N, Ne, Mg, Si, and S, and L-series emission from Fe in highly ionized states. The spectrum can be described by a single temperature (0.64 keV) thin thermal plasma model in collisional equilibrium with a hydrogen-equivalent extinction column density of ~3e21/cm2, a flux of ~1e-12 erg/s/cm2, and a luminosity of ~6e34 erg/s in the 0.3-3.0 keV band at an assumed distance of 13 kpc. We found a hint of an enhancement of N and deficiencies of O and Fe relative to other metals. The observed X-ray properties can be interpreted as the emission arising from shocks of ejecta from an ONe-type nova.

  10. Surface studies and implanted helium measurements following NOVA high-yield DT experiments

    SciTech Connect (OSTI)

    Stoyer, M.A.; Hudson, G.B.

    1997-02-18T23:59:59.000Z

    This paper presents the results of three March 6, 1996 direct-drive high-yield DT NOVA experiments and provides `proof-of-principal` results for the quantitative measurement of energetic He ions. Semiconductor quality Si wafers and an amorphous carbon wafer were exposed to NOVA high-yield implosions. Surface damage was sub-micron in general, although the surface ablation was slightly greater for the carbon wafer than for the Si wafers. Melting of a thin ({approx} 0.1{mu}) layer of Si was evident from microscopic investigation. Electron microscopy indicated melted blobs of many different metals (e.g. Al, Au, Ta, Fe alloys, Cu and even Cd) on the surfaces. The yield measured by determining the numbers of atoms of implanted {sup 4}He and {sup 3}He indicate the number of DT fusions to be 9.1({plus_minus}2.3) X 10{sup 12} and DD fusions to be 4.8({plus_minus}1.0) x 10{sup 10}, respectively. The helium DT fusion yield is slightly lower than that of the Cu activation measurement, which was 1.3({plus_minus}0.l) x 10{sup 13} DT fusions.

  11. Quasi-Coherent Oscillations in the Extreme Ultraviolet Flux of the Dwarf Nova SS Cygni

    E-Print Network [OSTI]

    Christopher W. Mauche

    1996-03-18T23:59:59.000Z

    Quasi-coherent oscillations have been detected in the extreme ultraviolet flux of the dwarf nova SS Cygni during observations with the Extreme Ultraviolet Explorer satellite of the rise and plateau phases of an anomalous outburst in 1993 August and a normal outburst in 1994 June/July. On both occasions, the oscillation turned on during the rise to outburst and persisted throughout the observation. During the 1993 outburst, the period of the oscillation fell from 9.3 s to 7.5 s over an interval of 4.4 days; during the 1994 outburst, the period fell from 8.9 s to 7.19 s (the shortest period ever observed in SS Cyg, or any other dwarf nova) within less than a day, and then rose to 8.0 s over an interval of 8.0 days. For both outbursts, the period $P$ of the oscillation was observed to correlate with the 75--120 \\AA \\ count rate $I_{\\rm EUV}$ according to $P\\propto I_{\\rm EUV}^{-0.094}$. A magnetospheric model is considered to reproduce this variation. It is found that an effective high-order multipole field is required, and that the field strength at the surface of the white dwarf is 0.1--1 MG. Such a field strength is at the lower extreme of those measured or inferred for bona fide magnetic cataclysmic variables.

  12. A near-infrared shock wave in the 2006 outburst of recurrent nova RS Ophiuchi

    E-Print Network [OSTI]

    Ramkrishna Das; Dipankar P. K. Banerjee; Nagarhalli M. Ashok

    2006-11-08T23:59:59.000Z

    Near-infrared spectra are presented for the recent 2006 outburst of the recurrent nova RS Ophiuchi (RS Oph).We report the rare detection of an infrared shock wave as the nova ejecta plows into the pre-existing wind of the secondary in the RS Oph system consisting of a white dwarf (WD) primary and a red giant secondary. The evolution of the shock is traced through a free expansion stage to a decelerative phase. The behavior of the shock velocity with time is found to be broadly consistent with current shock models. The present observations also imply that the WD in the RS Oph system has a high mass indicating that it could be a potential SNIa candidate. We also discuss the results from a recent study showing that the near-IR continuum from the recent RS Oph eruption does not originate in an expanding fireball. However, the present work shows that the IR line emission does have an origin in an expanding shock wave.

  13. Photoionization Heating of Nova Ejecta by the Post-Outburst Supersoft Source

    E-Print Network [OSTI]

    Cunningham, Timothy; Bildsten, Lars

    2015-01-01T23:59:59.000Z

    The expanding ejecta from a classical nova remains hot enough ($\\sim10^{4}\\, {\\rm K}$) to be detected in thermal radio emission for up to years after the cessation of mass loss triggered by a thermonuclear instability on the underlying white dwarf (WD). Nebular spectroscopy of nova remnants confirms the hot temperatures observed in radio observations. During this same period, the unstable thermonuclear burning transitions to a prolonged period of stable burning of the remnant hydrogen-rich envelope, causing the WD to become, temporarily, a super-soft X-ray source. We show that photoionization heating of the expanding ejecta by the hot WD maintains the observed nearly constant temperature of $(1-4)\\times10^4\\mathrm{~K}$ for up to a year before an eventual decline in temperature due to either the cessation of the supersoft phase or the onset of a predominantly adiabatic expansion. We simulate the expanding ejecta using a one-zone model as well as the Cloudy spectral synthesis code, both incorporating the time-d...

  14. Minara Nova

    E-Print Network [OSTI]

    Multiple Contributors

    1982-01-01T23:59:59.000Z

    .) -- Colp. Toys in the Attic -- Citadel What is Rain (Children's Album) --Decca World of Susie Wong -- RCA Victor You Can't Run Away from It (Decca) The Man with Bogart's Face Then Came Bronson -- Capitol Records Television includes: Alcoa-Goodyear...

  15. 50-Plus Ways to Be Water Smart 1. If your local water utility offers water-saving incentives or in-home water audits, take advantage

    E-Print Network [OSTI]

    50-Plus Ways to Be Water Smart BEHAVIORS 1. If your local water utility offers water-saving incentives or in-home water audits, take advantage of these programs. 2. Don't let water run while brushing

  16. A Case Study of NGO-Government Collaboration in Vietnam: Partnership Dynamics Explained through Contexts, Incentives, and Barriers

    E-Print Network [OSTI]

    Nguyen, Anh Thuc

    2012-10-19T23:59:59.000Z

    and barriers to partnerships are shaped first by their contexts, the framework acknowledged the role of the conditioning factors that influence partnership development, particularly their agenda of engagement (Teamey, 2007; Lewis & Opuku- Mensah, 2006..., barriers, and feedback loop. Conditioning factors shape incentives and barriers for partnerships, the former leading to agenda of engagement while the latter to a renegotiation of agenda. The feedback loop channels updates from conditioning factors...

  17. Incentives and recent proposals for partitioning and transmutation in the United States

    SciTech Connect (OSTI)

    Donovan, T.J.

    1995-05-01T23:59:59.000Z

    Partitioning and transmutation (P-T) is perhaps the most elegant means of high level waste disposal. Currently, the cost of fuel obtained from reprocessing spent fuel exceeds the cost of fuel obtained by mining. This has resulted in the once through fuel cycle dominating the US nuclear industry. Despite this fact P-T continues to be examined and debated by the US as well as abroad. The US first seriously considered P-T between approximately 1976 and 1982 but rejected the concept in favor of reprocessing. More recently, since about 1989, as a result of the once through fuel cycle and the growing problems of waste disposal, studies concerning P-T have resumed. This essay will seek to outline the incentives and goals of partitioning and transmutation as it would apply to the disposal of spent fuel in the US. Recent proposals by various US national laboratories for implementing partitioning and transmutation as a high level waste management and disposal device will also be discussed. The review will seek to examine the technical concepts utilized in each of the proposals and their feasibility. The major focus of this essay will be the transmutation methods themselves, while the partitioning methods will be discussed only briefly. This is because of the fact that partitioning methods fall under reprocessing as an already fairly well established and accepted technology while feasible methods for transmutation are still being advanced.

  18. Re-thinking incentives and penalties: Economic aspects of waste management in Italy

    SciTech Connect (OSTI)

    Cossu, R. [IMAGE, Department of Hydraulic, Maritime, Environmental and Geotechnical Engineering, University of Padua, Via Loredan, 35131 Padua (Italy); Masi, S., E-mail: salvatore.masi@unibas.it [DIFA, Department of Environmental Engineering and Physics, University of Basilicata, Via dellAteneo 10, 85100 Potenza (Italy)

    2013-11-15T23:59:59.000Z

    Highlights: We focused on the dynamics the formation of operational costs of waste management. We provide the basic elements to compose a picture of economic management. We present a reflection on the last hidden costs associated with the consumption of goods and packaging. Reduction of waste production. - Abstract: This paper focuses on the dynamics the formation of operational costs of waste management in Italy and the effect of economic measures. Currently incentives and penalties have been internalized by the system no differently from other cost items and revenues. This has greatly influenced the system directing it towards solutions that are often distant from the real environmental objectives. Based on an analysis of disaggregated costs of collection treatment and recovery, we provide the basic elements to compose a picture of economic management in various technicalorganizational scenarios. In the light of the considerations contained in the paper it is proposed, e.g. for controlled landfills, that the ecotax, currently based on weight, could be replaced by one based on the volume consumption. Likewise, for tax reduction on disposal system, instead a pre-treatment might ask an environmental balance of the overall system. The article presents a reflection on the last hidden costs associated with the consumption of goods and packaging, and how to reduce waste production is the necessary path to be followed in ecological and economic perspectives.

  19. INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE

    SciTech Connect (OSTI)

    Hinkle, Kenneth H.; Joyce, Richard R. [National Optical Astronomy Observatories, P.O. Box 26732, Tucson, AZ 85726 (United States); Fekel, Francis C. [Center of Excellence in Information Systems, Tennessee State University, 3500 John A. Merritt Blvd., Box 9501, Nashville, TN 37209 (United States); Wood, Peter, E-mail: hinkle@noao.edu, E-mail: joyce@noao.edu, E-mail: fekel@evans.tsuniv.edu, E-mail: wood@mso.anu.edu.au [Research School of Astronomy and Astrophysics, Australian National University, Private Bag, Canberra, ACT 2611 (Australia)

    2013-06-10T23:59:59.000Z

    Time-series spectra of the near-infrared 1.6 {mu}m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. No orbital motion is detected in agreement with previous estimates of orbital periods {approx}>100 yr and semimajor axes {approx}50 AU. The 1-5 {mu}m spectra of the Miras show line weakening during dust obscuration events. This results from scattering and continuum emission by 1000 K dust. In the heavily obscured HM Sge system the 4.6 {mu}m CO spectrum formed in 1000 K gas is seen in emission against an optically thick dust continuum. Spectral features that are typically produced in either the cool molecular region or the expanding circumstellar region of late-type stars cannot be detected in the D-symbiotic novae. This is in accord with the colliding wind model for interaction between the white dwarf and Mira. Arguments are presented that the 1000 K gas and dust are not Mira circumstellar material but are in the wind interaction region of the colliding winds. CO is the first molecule detected in this region. We suggest that dust condensing in the intershock region is the origin of the dust obscuration. This model explains variations in the obscuration. Toward the highly obscured Mira in HM Sge the dust zone is estimated to be {approx}0.1 AU thick. The intershock wind interaction zone appears thinnest in the most active systems. Drawing on multiple arguments masses are estimated for the system components. The Miras in most D-symbiotic novae have descended from intermediate mass progenitors. The large amount of mass lost from the Mira combined with the massive white dwarf companion suggests that these systems are supernova candidates. However, timescales and the number of objects make these rare events.

  20. PHASE-RESOLVED INFRARED SPECTROSCOPY AND PHOTOMETRY OF V1500 CYGNI, AND A SEARCH FOR SIMILAR OLD CLASSICAL NOVAE

    SciTech Connect (OSTI)

    Harrison, Thomas E. [Department of Astronomy, New Mexico State University, Box 30001, MSC 4500, Las Cruces, NM 88003-8001 (United States); Campbell, Randy D.; Lyke, James E., E-mail: tharriso@nmsu.edu, E-mail: jlyke@keck.hawaii.edu, E-mail: randyc@keck.hawaii.edu [W. M. Keck Observatory, 65-1120 Mamalahoa Hwy., Kamuela, HI 96743 (United States)

    2013-08-01T23:59:59.000Z

    We present phase-resolved near-infrared photometry and spectroscopy of the classical nova (CN) V1500 Cyg to explore whether cyclotron emission is present in this system. While the spectroscopy do not indicate the presence of discrete cyclotron harmonic emission, the light curves suggest that a sizable fraction of its near-infrared fluxes are due to this component. The light curves of V1500 Cyg appear to remain dominated by emission from the heated face of the secondary star in this system. We have used infrared spectroscopy and photometry to search for other potential magnetic systems among old CNe. We have found that the infrared light curves of V1974 Cyg superficially resemble those of V1500 Cyg, suggesting a highly irradiated companion. The old novae V446 Her and QV Vul have light curves with large amplitude variations like those seen in polars, suggesting they might have magnetic primaries. We extract photometry for 79 old novae from the Two Micron All Sky Survey Point Source Catalog and use those data to derive the mean, un-reddened infrared colors of quiescent novae. We also extract WISE data for these objects and find that 45 of them were detected. Surprisingly, a number of these systems were detected in the WISE 22 {mu}m band. While two of those objects produced significant dust shells (V705 Cas and V445 Pup), the others did not. It appears that line emission from their ionized ejected shells is the most likely explanation for those detections.