Computer Science
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sers.conf...20a&link_type=abstract
Proceedings of the Workshop on The Solar Electromagnetic Radiation Study for Solar Cycle 22, p. 20.
Computer Science
6
Sun, Solar Atmosphere, Irradiance
Scientific paper
Solar atmospheric models can be used to calculate the spectra from various quiet and active regions on the solar disk. One-dimensional models for such regions are adequate because vertical changes occur over very short distances compared with the horizontal size of most observed features. Several quiet-Sun component models and a plage-facula model are discussed. The computed spectra can be used to interrelate the intensities at different wavelengths, so that the irradiance at UV wavelengths, for example, can be calculated given the distribution of quiet and active regions observed at visible wavelengths. Intensity and irradiance calculations based on solar atmospheric models can be used to normalize and interpolate between available observations at various wavelengths obtained at different times during the solar activity cycle.
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