The Development of a New Model of Solar EUV Irradiance Variability

Details The Development of a New Model of Solar EUV Irradiance Variability The Development of a New Model of Solar EUV Irradiance Variability

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0243799w&link_type=abstract

Technical Report, Smithsonian Astrophysical Observatory Cambridge, MA United States

Astronomy and Astrophysics

Astrophysics

Extreme Ultraviolet Radiation, Solar Radiation, Variability, Models, Irradiance, Sun, Coronal Holes, Atmospheric Radiation

Scientific paper

The goal of this research project is the development of a new model of solar EUV (Extreme Ultraviolet) irradiance variability. The model is based on combining differential emission measure distributions derived from spatially and spectrally resolved observations of active regions, coronal holes, and the quiet Sun with full-disk solar images. An initial version of this model was developed with earlier funding from NASA. The new version of the model developed with this research grant will incorporate observations from SoHO as well as updated compilations of atomic data. These improvements will make the model calculations much more accurate.

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