Radio imagery of the sun at wavelengths of 3.5, 2.8, 2.25 and 1.95 CM during the period preceding the solar eclipse on July 11, 1991

Details Radio imagery of the sun at wavelengths of 3.5, 2.8, 2.25 and 1.95 CM during the period preceding the solar eclipse on July 11, 1991 Radio imagery of the sun at wavelengths of 3.5, 2.8, 2.25 and 1.95 CM during the period preceding the solar eclipse on July 11, 1991

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..188b&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 188; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 5, May 1992, p. 467-

Astronomy and Astrophysics

Astronomy

Brightness Distribution, Radio Astronomy, Solar Eclipses, Radio Emission, Solar Activity, Sunspots, Wavelengths

Scientific paper

Solar emission observations conducted on July 10-11, 1991 with the
Crimean Astrophysical Observatory 22-m radio telescope using the
four-wavelength polarimeter are reported. Radio sources are compared
with optical formations on the sun. Some estimates of physical
parameters in regions of increased radio brightness are presented.

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