Spectrum of short-wave emission for aeronomical calculations for different levels of solar activity

Details Spectrum of short-wave emission for aeronomical calculations for different levels of solar activity Spectrum of short-wave emission for aeronomical calculations for different levels of solar activity

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..581b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, July-Aug. 1984, p. 581-585. In Russian.

Astronomy and Astrophysics

Astronomy

6

Aeronomy, Line Spectra, Short Wave Radiation, Solar Activity Effects, Solar Radio Emission, Solar Spectra, Ultraviolet Astronomy

Scientific paper

A two-component model of short-wave (10-105 nm) solar emission shows that the intensity ratios of individual spectral lines depend only slightly on the activity level. Formulas are obtained which make it possible to calculate the spectrum and total flux of short-wave emission for any level of solar activity on the basis of flux measurements in the 58.4 nm line or measurements of radio emission at 10.7 cm. The results can be used for the simulation of processes in the earth's ionosphere and upper atmosphere.

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