Modeling VIRGO Spectral and Bolometric Irradiances with MDI Data

Details Modeling VIRGO Spectral and Bolometric Irradiances with MDI Data Modeling VIRGO Spectral and Bolometric Irradiances with MDI Data

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..259..283s&link_type=abstract

The Dynamic Sun, Proceedings of the Summerschool and Workshop held at the Solar Observatory Kanzelhöhe, Kärnten, Austria, August

Astronomy and Astrophysics

Astrophysics

Scientific paper

The last solar activity minimum in 1996 was characterized by several periods without any sunspots or faculae visible on the solar disk. Between these extremely quiet intervals, from time to time a single active region emerged and developed. The passage of these individual active regions across the visible solar hemisphere was accompanied by a pronounced variation in the solar irradiance as observed by VIRGO onboard SOHO. Making use of photometric full-disk observations of the Sun obtained by MDI we try to reconstruct the temporal behaviour of the three spectral and the total irradiance channels measured by VIRGO by applying starspot modeling techniques. In this paper we mainly discuss possible error sources.

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