Statistics – Applications
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.8243t&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 95, June 1, 1990, p. 8243-8251.
Statistics
Applications
63
Electromagnetic Radiation, Extreme Ultraviolet Radiation, Solar Flux, Solar Terrestrial Interactions, Solar X-Rays, Lyman Alpha Radiation, Upper Atmosphere
Scientific paper
A full-disk solar EUV and soft X-ray flux model has been developed for the period of late 1981 into 1989. This corresponds to the declining and minimum phase of solar cycle 21 and the rising to maximum phase of solar cycle 22. The model calculates 39 wavelength intervals or prominent discrete lines between 1.9 and 105.0 nm in both magnitude and relative temporal variation. The model wavelength equations are based on two 13-day smoothed solar indices, SME Lyman-alpha and Ottawa F(10.7), which are used with tabulated coefficients and spectral weighting functions to produce both chromospheric and transition region-coronal energy fluxes. The principal use of this model is for aeronomical applications to calculate the EUV and soft X-ray energy flux at the top of the atmosphere.
Barth Charles A.
Kent Tobiska W.
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