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Research Paper | Astronomy Science | Volume 3 Issue 8, August 2014 | Pages: 820 - 828 | India
Solar Irradiance Modelling
Abstract: CTSI is the solar energy received on outer layer of earth (at 1AU distance from sun) in form of heat flux ( in various wavelength bands) measured in w/m^2. SSA is the area of vissible sunspot on photosphere of sun. B is the daily averged solar global magnetic field. The CTSI & SSA shows delay9 with respect to each other.27day running averaged values of CTSI, SSA, B for delayed events are suitably combined in solar irradiance modelling. Using solar data for cycles 21, 22, 23 about 6 modelling equations are developed for solar irradiance. The modelled equations very well predict solar irradiance (RAWCTSI) within an error limit of +/- 0.12 w/m^2.
Keywords: Sun, CTSI, SSA, Average solar magnetic field B, Delay
How to Cite?: V S Rohini, "Solar Irradiance Modelling", Volume 3 Issue 8, August 2014, International Journal of Science and Research (IJSR), Pages: 820-828, https://www.ijsr.net/getabstract.php?paperid=2015448, DOI: https://dx.doi.org/10.21275/2015448