Structure and activation of solar prominences based on radio and optical observations

Details Structure and activation of solar prominences based on radio and optical observations Structure and activation of solar prominences based on radio and optical observations

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..162a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Jan.-Feb. 1986, p. 162-165) Soviet Astronomy (ISSN 0038-5301), vol. 30, Jan.-Feb. 1986, p. 9

Astronomy and Astrophysics

Astronomy

Activation, Radio Spectra, Solar Activity Effects, Solar Prominences, Spectral Energy Distribution, Visible Spectrum, Brightness Distribution, Brightness Temperature, Optical Thickness, Solar Flares

Scientific paper

Prominences in eclipse radio observations have bright dense knots and 'holes'. The activation of a prominence by a flare, according to radio observations, takes place from the bottom up, with the disturbance evidently propagating along low-lying magnetic arches of a single activity complex. A comparison of the distribution of radio brightness with the distribution in UV shows considerable similarity.

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