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Relevant bibliographies by topics / Standard solar models

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Academic literature on the topic 'Standard solar models'

Author: Grafiati

Published: 4 June 2021

Last updated: 3 February 2022

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Journal articles on the topic "Standard solar models"

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Bahcall, John N. "Standard solar models." Nuclear Physics B - Proceedings Supplements 77, no. 1-3 (May 1999): 64–72. http://dx.doi.org/10.1016/s0920-5632(99)00399-0.

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Ciacio, F., S. Degl'Innocenti, and B. Ricci. "Updating standard solar models." Astronomy and Astrophysics Supplement Series 123, no. 3 (June 1997): 449–54. http://dx.doi.org/10.1051/aas:1997168.

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Castellani, V., S. Degl'Innocenti, G. Fiorentini, M. Lissia, and B. Ricci. "Solar neutrinos: beyond standard solar models." Physics Reports 281, no. 5-6 (March 1997): 309–98. http://dx.doi.org/10.1016/s0370-1573(96)00032-4.

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Degl'Innoccenti, S., W. A. Dziembowski, G. Fiorentini, and B. Ricci. "Helioseismology and standard solar models." Astroparticle Physics 7, no. 1-2 (June 1997): 77–95. http://dx.doi.org/10.1016/s0927-6505(97)00004-2.

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Vinyoles, N., A. Serenelli, and F. L. Villante. "The B16 Standard Solar Models." Journal of Physics: Conference Series 1056 (July 2018): 012058. http://dx.doi.org/10.1088/1742-6596/1056/1/012058.

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Bahcall, John N., M. H. Pinsonneault, Sarbani Basu, and J. Christensen-Dalsgaard. "Are Standard Solar Models Reliable?" Physical Review Letters 78, no. 2 (January 13, 1997): 171–74. http://dx.doi.org/10.1103/physrevlett.78.171.

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Serenelli, Aldo M. "New results on standard solar models." Astrophysics and Space Science 328, no. 1-2 (November 3, 2009): 13–21. http://dx.doi.org/10.1007/s10509-009-0174-8.

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Bahcall, John N. "Recent work on standard solar models." Nuclear Physics B - Proceedings Supplements 31 (April 1993): 125–28. http://dx.doi.org/10.1016/0920-5632(93)90123-n.

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Maeder, André. "A Look on Non-Standard Solar Models." International Astronomical Union Colloquium 121 (1990): 133–44. http://dx.doi.org/10.1017/s0252921100067889.

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AbstractA short review of some of the non–standard models proposed in these last two decades is presented. Their main physical assumptions are shown, as well as the way they meet or do not meet the various observational constraints.

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Vinyoles, Núria, Aldo M. Serenelli, Francesco L. Villante, Sarbani Basu, Johannes Bergström, M. C. Gonzalez-Garcia, Michele Maltoni, Carlos Peña-Garay, and Ningqiang Song. "A New Generation of Standard Solar Models." Astrophysical Journal 835, no. 2 (January 31, 2017): 202. http://dx.doi.org/10.3847/1538-4357/835/2/202.

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Dissertations / Theses on the topic "Standard solar models"

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Lay, Michael David. "Creation and detection of Cerenkov light in the Sudbury Neutrino Observatory." Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.239323.

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Daniel, John Edward. "Development of enhanced multiport network analyzer calibrations using non-ideal standards." [Tampa, Fla.] : University of South Florida, 2005. http://purl.fcla.edu/fcla/etd/SFE0001392.

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Dalnoki-Veress, Ferenc J. R. Carleton University Dissertation Physics. "Investigation of the triggered source technique for the calibration of SNO." Ottawa, 1996.

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Books on the topic "Standard solar models"

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Pavlov, Sergey. Astronomy. ru: INFRA-M Academic Publishing LLC., 2021. http://dx.doi.org/10.12737/1148996.

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The textbook presents almost all sections of modern astronomy: a historical overview, the basics of practical astronomy, the laws of motion of celestial bodies, the structure of the Solar system, methods of astronomical research, basic information about the Sun, stars, planets, galaxies and the Universe as a whole. To work with the textbook, you need knowledge of the main sections of mathematics, physics and chemistry in the volume of the high school course. At the end of the paragraphs, there is a list of questions for better assimilation of the material, as well as tasks focused on preparing for the Unified State Exam in physics. Meets the requirements of the federal state educational standards of secondary vocational education of the latest generation. For students of the 11th grade, students of secondary special educational institutions and anyone interested in the problems of modern astronomy.

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1942-, Klapdor-Kleingrothaus H. V., ed. Sixty years of double beta decay: From nuclear physics to beyond standard model particle physics. Singapore: World Scientific, 2001.

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Goswami, B. N., and Soumi Chakravorty. Dynamics of the Indian Summer Monsoon Climate. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190228620.013.613.

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Lifeline for about one-sixth of the world’s population in the subcontinent, the Indian summer monsoon (ISM) is an integral part of the annual cycle of the winds (reversal of winds with seasons), coupled with a strong annual cycle of precipitation (wet summer and dry winter). For over a century, high socioeconomic impacts of ISM rainfall (ISMR) in the region have driven scientists to attempt to predict the year-to-year variations of ISM rainfall. A remarkably stable phenomenon, making its appearance every year without fail, the ISM climate exhibits a rather small year-to-year variation (the standard deviation of the seasonal mean being 10% of the long-term mean), but it has proven to be an extremely challenging system to predict. Even the most skillful, sophisticated models are barely useful with skill significantly below the potential limit on predictability. Understanding what drives the mean ISM climate and its variability on different timescales is, therefore, critical to advancing skills in predicting the monsoon. A conceptual ISM model helps explain what maintains not only the mean ISM but also its variability on interannual and longer timescales.The annual ISM precipitation cycle can be described as a manifestation of the seasonal migration of the intertropical convergence zone (ITCZ) or the zonally oriented cloud (rain) band characterized by a sudden “onset.” The other important feature of ISM is the deep overturning meridional (regional Hadley circulation) that is associated with it, driven primarily by the latent heat release associated with the ISM (ITCZ) precipitation. The dynamics of the monsoon climate, therefore, is an extension of the dynamics of the ITCZ. The classical land–sea surface temperature gradient model of ISM may explain the seasonal reversal of the surface winds, but it fails to explain the onset and the deep vertical structure of the ISM circulation. While the surface temperature over land cools after the onset, reversing the north–south surface temperature gradient and making it inadequate to sustain the monsoon after onset, it is the tropospheric temperature gradient that becomes positive at the time of onset and remains strongly positive thereafter, maintaining the monsoon. The change in sign of the tropospheric temperature (TT) gradient is dynamically responsible for a symmetric instability, leading to the onset and subsequent northward progression of the ITCZ. The unified ISM model in terms of the TT gradient provides a platform to understand the drivers of ISM variability by identifying processes that affect TT in the north and the south and influence the gradient.The predictability of the seasonal mean ISM is limited by interactions of the annual cycle and higher frequency monsoon variability within the season. The monsoon intraseasonal oscillation (MISO) has a seminal role in influencing the seasonal mean and its interannual variability. While ISM climate on long timescales (e.g., multimillennium) largely follows the solar forcing, on shorter timescales the ISM variability is governed by the internal dynamics arising from ocean–atmosphere–land interactions, regional as well as remote, together with teleconnections with other climate modes. Also important is the role of anthropogenic forcing, such as the greenhouse gases and aerosols versus the natural multidecadal variability in the context of the recent six-decade long decreasing trend of ISM rainfall.

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Book chapters on the topic "Standard solar models"

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Serenelli, Aldo M. "New results on standard solar models." In Synergies between Solar and Stellar Modelling, 11–19. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-90-481-9198-7_2.

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Maeder, André. "A Look on Non-Standard Solar Models." In Inside the Sun, 133–44. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0541-2_12.

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Turcotte, S., and J. Christensen-Dalsgaard. "Solar Models with Non-Standard Chemical Composition." In Solar Composition and its Evolution — from Core to Corona, 133–40. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4820-7_13.

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Bahcall, J. N., and M. Cribier. "The Standard Solar Model." In Inside the Sun, 21–41. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0541-2_3.

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Dziembowski, W. A. "Shortcomings of the Standard Solar Model." In Solar Composition and its Evolution — from Core to Corona, 37–48. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4820-7_3.

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Baker, D. N., S. G. Kanekal, M. D. Looper, J. B. Blake, and R. A. Mewaldt. "Jovian, Solar, and other Possible Sources of Radiation Belt Particles." In Radiation Belts: Models and Standards, 49–55. Washington, D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm097p0049.

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Serenelli, Aldo. "Standard Solar Models." In Neutrinos in Particle Physics, Astrophysics and Cosmology, 119–45. CRC Press, 2008. http://dx.doi.org/10.1201/9781420082401.ch5.

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Berthomieu, G., J. Provost, P. Morel, and Y. Lebreton. "Standard solar models with CESAM code." In Solar Neutrinos, 62. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-25.

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Bancall, John N., Walter F. Huebner, Stephen H. Lubow, Peter D. Parker, and Roger K. Ulrich. "Standard solar models and the uncertainties in predicted capture rates of solar neutrinos." In Solar Neutrinos, 57. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-20.

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Bahcall, J. N., and M. H. Pinsonneault. "Standard solar models, with and without helium diffusion, and the solor neutrino problem." In Solar Neutrinos, 60. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-23.

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Conference papers on the topic "Standard solar models"

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BAHCALL, JOHN N. "SOLAR MODELS: AN HISTORICAL OVERVIEW." In Neutrinos and Implications for Physics Beyond the Standard Model - The Conference. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704207_0004.

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Myers, Daryl R., Keith Emery, and C. Gueymard. "Revising and Validating Spectral Irradiance Reference Standards for Photovoltaic Performance Evaluation." In ASME Solar 2002: International Solar Energy Conference. ASMEDC, 2002. http://dx.doi.org/10.1115/sed2002-1074.

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In 1982, the American Society for Testing and Materials (ASTM) adopted consensus standard direct-normal and global-tilted solar terrestrial spectra (ASTM E891/E892). These standard spectra were intended to evaluate photovoltaic (PV) device performance and other solar-related applications. The International Standards Organization (ISO) and International Electrotechnical Commission (IEC) adopted these spectra as spectral standards ISO 9845-1 and IEC 60904-3. Additional information and more accurately representative spectra are needed by today’s PV community. Modern terrestrial spectral radiation models, knowledge of atmospheric physics, and measured radiometric quantities are applied to develop new reference spectra for consideration by ASTM.

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Bergquam, James B., and Joseph M. Brezner. "Solar Fired, Compressor Assisted Absorption Chillers." In ASME Solar 2002: International Solar Energy Conference. ASMEDC, 2002. http://dx.doi.org/10.1115/sed2002-1041.

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This paper presents the results of a thermodynamic and heat transfer analysis of solar fired, compressor assisted absorption chillers. The objectives are to determine and evaluate the feasibility of using vapor compressors to lower the operating temperature of the primary generator, simplify the maintenance and reduce the cost of solar/waste heat powered absorption HVAC systems. The nominal generator temperature in a single effect absorption chiller is 88°C and the coefficient of performance is approximately 0.8. A standard double effect chiller requires the high temperature generator to operate at about 150°C. The nominal COP of a double effect cycle is 1.2 to 1.4. Various modifications have been proposed to lower the operating temperature of the primary generator. One such modification is to add a vapor compressor to the basic cycle. Computer models that simulate the effect of vapor compressors at selected locations in single and double effect LiBr/H2O absorption chillers have been developed. Two locations were modeled for single effect chillers and three locations for double effect chillers. The best results were obtained for a double effect chiller with the compressor located between the high and low temperature generators.

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Canada, Scott, Doug A. Brosseau, and Henry Price. "Design and Construction of the APS 1-MWe Parabolic Trough Power Plant." In ASME 2006 International Solar Energy Conference. ASMEDC, 2006. http://dx.doi.org/10.1115/isec2006-99139.

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Arizona Public Service (APS) is currently installing and operating new power facilities to generate a portion of its electricity from solar resources that will satisfy its obligation under the Arizona Environmental Portfolio Standard. During FY04, APS began construction on a 1-MWe parabolic trough concentrating solar power plant. Site preparation and construction activities continued throughout FY05 and early FY06. Construction was completed and initial startup occurred by the end of December 2005. Full power production and initial performance monitoring and evaluation will occur early in 2006. This project is the first commercial deployment of parabolic trough collector technology developed by Solargenix Energy, Inc. of Raleigh, North Carolina. The plant, located near Red Rock, Arizona, uses an organic Rankine cycle power plant by Ormat, which is much simpler than conventional steam Rankine cycles and allows unattended operation of the facility. APS has teamed with the National Renewable Energy Laboratory and Sandia National Laboratories (collectively called SunLab), along with Nexant, Inc. to support design and startup activities and performance assessment. SunLab has developed TRNSYS models of the plant and will utilize initial performance baseline data to validate the models. Eventually, those models will be used to determine whether a proposed thermocline energy storage system designed by Nexant, Inc. is technically and economically feasible for this plant. SunLab has also assisted APS with development of an O&M database using the Maximo system to track solar plant costs and component failure modes.

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Lyakhov, Andrey, Stanislav Kozlov, Tatiana Losseva, Susanna Bekker, Julia Korsunskaya, Boris Gavrilov, Valerij Kudryavtsev, and Egor Goncharov. "The comparison of standard and swarm D-layer ionosphere models on the simulation of the x-ray solar flare response." In XXV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, edited by Gennadii G. Matvienko and Oleg A. Romanovskii. SPIE, 2019. http://dx.doi.org/10.1117/12.2540423.

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Litardo, Jaqueline, José Macías, Rubén Hidalgo-León, Maria Gabriela Cando, and Guillermo Soriano. "Measuring the Effect of Local Commercial Roofing Samples on the Thermal Behavior of a Social Interest Dwelling Located in Different Climates in Ecuador." In ASME 2019 International Mechanical Engineering Congress and Exposition. American Society of Mechanical Engineers, 2019. http://dx.doi.org/10.1115/imece2019-11472.

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Abstract This paper presents an assessment of the effect of the solar reflectance of roofing assemblies on the thermal behavior of a social interest dwelling model located in six representative cities in Ecuador. The model house complies the Ecuadorian building standard. The solar reflectances of 23 local commercial roofing samples were measured following the E1918A Procedure. The thermal behavior of the dwelling was simulated in EnergyPlus. The models use input data, such as: loads and schedules, provided by previous studies on social dwellings. The hours of thermal discomfort based on ASHRAE Standard 55-2013 adaptive model were obtained for each case by varying the experimental solar reflectance of the roofing sample and meteorological data for each hourly time step calculation. Results indicated that the 1808001-50 sample provided between 3240 to 5524 discomfort hours in all cases, being the most suitable roofing assembly for all studied cities due to its higher solar reflectance.

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Barigozzi, G., G. Bonetti, G. Franchini, A. Perdichizzi, and S. Ravelli. "Solar Hybrid Combined Cycle Performance Prediction: Influence of GT Model and Spool Arrangement." In ASME Turbo Expo 2012: Turbine Technical Conference and Exposition. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/gt2012-68881.

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A modeling procedure was developed to simulate design and off-design operation of Hybrid Solar Gas Turbines in a combined cycle (CC) configuration. The system includes an heliostat field, a receiver and a commercial gas turbine interfaced with a conventional steam Rankine cycle. Solar power input is integrated in the GT combustor by natural gas. Advanced commercial software tools were combined together to get design and off-design performance prediction: TRNSYS® was used to model the solar field and the receiver while the gas turbine and steam cycle simulations were performed by means of Thermoflex®. Three GT models were considered, in the 35–45 MWe range: a single shaft engine (Siemens SGT800) and two two-shaft engines (the heavy-duty GT Siemens SGT750 and the aero derivative GE LM6000 PF). This in order to assess the influence of different GT spool arrangements and control strategies on GT solarization. The simulation method provided an accurate modeling of the daily solar hybrid CC behavior to be compared against the standard CC. The effects of solarization were estimated in terms of electric power and efficiency reduction, fossil fuel saving and solar energy to electricity conversion efficiency.

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Fumo, N., V. Bortone, and J. C. Zambrano. "Comparative Analysis of Solar Thermal Cooling and Solar Photovoltaic Cooling Systems." In ASME 2011 5th International Conference on Energy Sustainability. ASMEDC, 2011. http://dx.doi.org/10.1115/es2011-54162.

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The Energy Information Administration of the United States Department of Energy projects that more than 80% of the energy consumption of the U.S. by 2035 will come from fossil fuels. This projection should be the fuel to promote projects related to renewable energy in order to reduce energy consumption from fossil fuels to avoid their undesirable consequences such as carbon dioxide emissions. Since solar radiation match pretty well building cooling demands, solar cooling systems will be an important factor in the next decades to meet or exceed the green gases reduction that will be demanded by the society and regulations in order to mitigate environmental consequences such as global warming. Solar energy can be used as source of energy to produce cooling through different technologies. Solar thermal energy applies to technology such as absorption chillers and desiccant cooling, while electricity from solar photovoltaic can be used to drive vapor compression electric chillers. This study focuses on the comparison of a Solar Thermal Cooling System that uses an absorption chiller driven by solar thermal energy, and a Solar Photovoltaic Cooling System that uses a vapor compression system (electric chiller) driven by solar electricity (solar photovoltaic system). Both solar cooling systems are compared against a standard air cooled cooling system that uses electricity from the grid. The models used in the simulations to obtain the results are described in the paper along with the parameters (inputs) used. Results are presented in two figures. Each figure has one curve for the Solar Thermal Cooling System and one for the Solar Photovoltaic Cooling System. One figure allows estimation of savings calculated based the net present value of energy consumption cost. The other figure allows estimating primary energy consumption reduction and emissions reduction. Both figures presents the result per ton of refrigeration and as a function of area of solar collectors or/and area of photovoltaic modules. This approach to present the result of the simulations of the systems makes these figures quite general. This means that the results can be used to compare both solar cooling systems independently of the cooling demand (capacity of the system), as well as allow the analysis for different sizes of the solar system used to harvest the solar energy (collectors or photovoltaic modules).

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Loong, Lim Yaw, Norhasliza Yusof, Hasan Abu Kassim, H. B. Senin, G. Carini, J. B. Abdullah, and D. A. Bradley. "Standard Solar Model." In CURRENT ISSUES OF PHYSICS IN MALAYSIA: National Physics Conference 2007 - PERFIK 2007. AIP, 2008. http://dx.doi.org/10.1063/1.2940667.

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Letexier, Blaise, Olivier Marc, Jean-Philippe Praene, and Franck Lucas. "Sensitivity Analysis of a Solar Cooling System." In ASME 2012 11th Biennial Conference on Engineering Systems Design and Analysis. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/esda2012-82785.

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The aim of this paper is the optimization of Solar Absorption Cooling (SAC) system’s performances. Over the past decade the electricity consumption has significantly increased in Reunion Island during the summer months, which is mainly due to the use of standard air conditioning systems. SAC systems present a good alternative for reducing this consumption. Solar cooling systems are environmentally friendly as they use water and lithium bromide solution as the working fluid. The purpose of this work is to undertake a sensitivity analysis to identify parameters which have a significant influence on the SAC systems performances. The sensitivity analysis has been carried out on numerical models developed at the PIMENT laboratory and validated using RAFSOL experimental data (experimental plant is set up at the IUT in St-Pierre). The results of the sensitivity analysis are used to establish the design and create the control rules to allow for the optimization and ensure the performance of future SAC systems. Firstly, this paper presents the modelization of the SAC system and the sensitivity analysis method used. Secondly, it displays the results from the sensitivity analysis that has been applied to all main components of the plant separately (solar collector field, solar loop and absorption chiller) and to the entire system. Finally, the results are analyzed and discussed. Two types of influential parameters have been distinguished: variables factors and geometrical properties of the plant. This study highlights that the compactness of the installation, the quality of the solar collector, and the control of the temperature at the output of the distribution loop are essential.

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Reports on the topic "Standard solar models"

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Bahcall, J. N., C. A. Barnes, J. Christensen-Dalsgaard, B. T. Cleveland, S. Degl'Innocenti, B. W. Filippone, A. Glasner, et al. Has a standard model solution to the solar neutrino problem been found? Office of Scientific and Technical Information (OSTI), August 1994. http://dx.doi.org/10.2172/10176840.

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