Modelling solar irradiance variations: separate models for the network and active region faculae

Details Modelling solar irradiance variations: separate models for the network and active region faculae Modelling solar irradiance variations: separate models for the network and active region faculae

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..231w&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

Physics

2

Solar Activity, Irradiance Variations, Faculae, Network, Solar Activity, Irradiance Variations, Faculae, Network

Scientific paper

In order to determine to what extent solar surface magnetism affects solar irradiance we need to reconstruct the irradiance from magnetograms. This process requires the use of model atmospheres. Here we present two model atmospheres describing faculae in active regions and the network. The models have been constructed such that they reproduce various data sets simultaneously.

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