Variations of the sun's integral radio emission at wavelengths of 6.3 and 8.6 MM

Details Variations of the sun's integral radio emission at wavelengths of 6.3 and 8.6 MM Variations of the sun's integral radio emission at wavelengths of 6.3 and 8.6 MM

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..377p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Mar.-Apr. 1985, p. 377-379) Soviet Astronomy (ISSN 0038-5301), vol. 29, Mar.-Apr. 1985, p. 2

Astronomy and Astrophysics

Astronomy

Millimeter Waves, Periodic Variations, Solar Activity, Solar Cycles, Solar Radio Emission, Brightness Distribution, High Resolution

Scientific paper

On the basis of data of high-resolution measurements of the solar disk
brightness distribution made synchronously at the wavelengths 6.3 and
8.6 mm the variations of the S-component of the solar integral radio
emission during the period of maximum of the 11-year activity cycle of
the sun are estimated.

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