Modelling Short-Term Spectral Irradiance Variations

Details Modelling Short-Term Spectral Irradiance Variations Modelling Short-Term Spectral Irradiance Variations

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ssrv...94..139f&link_type=abstract

Space Science Reviews, v. 94, Issue 1/2, p. 139-144 (2000).

Computer Science

7

Scientific paper

On time-scales of the solar rotation most of the solar irradiance variations are caused by the changing distribution of solar surface magnetic features. We model these short-term irradiance variations using calculations of sunspot and facular contrasts as a function of wavelength and limb angle on the Sun. The position of active regions on the solar disc is derived from the MDI magnetograms. The reconstructed irradiance variations are compared with total and spectral irradiance measurements obtained by the VIRGO experiment on SOHO.

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