Common origin for UV and radio fluctuations

Details Common origin for UV and radio fluctuations Common origin for UV and radio fluctuations

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...66..323p&link_type=abstract

Solar Physics, vol. 66, June 1980, p. 323-332.

Astronomy and Astrophysics

Astronomy

1

Brightness Temperature, Plasma Oscillations, Shock Heating, Solar Atmosphere, Solar Radiation, Solar Radio Emission, Ultraviolet Spectra, Atmospheric Heating, Atmospheric Temperature, Perturbation Theory, Radio Astronomy, Shock Wave Propagation, Solar Spectra

Scientific paper

Brightness temperature fluctuations induced by a shock wave transit through the solar transition region are computed at several decimetric wavelengths. A simplified method previously used to reproduce the observed UV line intensity fluctuations is shown to give oscillation amplitudes which are consistent with experimental results. The detectability of shock-induced radio fluctuations is briefly discussed, to check the possibility of a common origin for the observed UV and radio phenomena.

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