Modeling solar irradiance variations through PSPT images and semiempirical models

Details Modeling solar irradiance variations through PSPT images and semiempirical models Modeling solar irradiance variations through PSPT images and semiempirical models

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..299p&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Computer Science

8

Solar Irradiance: Variations

Scientific paper

We try to reconstruct the variations of the disk integrated spectrum, both in the spectral ranges of VIRGO (blue at 403 nm, green at 501 nm and red at 863 nm) and in the bolometric flux, using semiempirical models (FAL models, Fontenla et al. 1999), built to reproduce different features in the solar atmosphere. Each computed spectrum is weighted with the disk coverage factor of the corresponding feature provided by the PSPT observations carried out at the Rome Observatory. We present the results obtained reconstructing the variations measured by VIRGO bolometers during periods of about one solar rotation and of the entire ascending phase of Solar Cycle 23.

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