Radiation pattern of solar microwave bursts

Details Radiation pattern of solar microwave bursts Radiation pattern of solar microwave bursts

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977dossr.236q1331b&link_type=abstract

Akademiia Nauk SSSR, Doklady, vol. 236, Oct. 21, 1977, p. 1331-1333. In Russian.

Physics

Microwave Emission, Radiation Distribution, Solar Radio Bursts, Distribution Functions, Longitude, Microwave Attenuation, Solar Magnetic Field

Scientific paper

The solar-longitude dependence of the intensity of microwave bursts was studied at frequencies of 1415, 2695, 4995, and 8800 MHz. For each of six solar-longitude ranges, distribution functions of the number of bursts with an intensity greater than a specified intensity are obtained. Microwave attenuation studied as a function of longitude shows an east-west asymmetry of the burst radiation pattern. The results of the analysis are used to construct a microwave-burst radiation pattern averaged with respect to all possible orientations of the magnetic field in the source regions.

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