Dependence of the intensity of lines of short-wave solar emission on the activity level

Details Dependence of the intensity of lines of short-wave solar emission on the activity level Dependence of the intensity of lines of short-wave solar emission on the activity level

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..529n&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, July-Aug. 1984, p. 529-536. In Russian.

Astronomy and Astrophysics

Astronomy

3

Line Spectra, Short Wave Radiation, Solar Radio Emission, Solar Spectra, Astronomical Spectroscopy, Background Radiation, Regression Analysis, Stellar Models

Scientific paper

Consideration is given to a two-component model for solar radio and short-wave (10-105 nm) emission from the undisturbed surface (background) and from active regions. Nonlinear regression relationships between the short-wave emission and radio emission are obtained, and regression coefficients are determined for a number of lines. An allowance for variations of background emission makes possible a significant improvement (up to 3-5 percent) in the accuracy with which fluxes of short-wave emission can be calculated, which opens the possibility of improving the accuracy of ionospheric predictions.

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