On fluctuations of radio emission of the quiet atmosphere of the Sun.

Details On fluctuations of radio emission of the quiet atmosphere of the Sun. On fluctuations of radio emission of the quiet atmosphere of the Sun.

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990bsold...7...88a&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 7/90, p. 88 - 92

Physics

Solar Radio Radiation: Fluctuations

Scientific paper

Fluctuations of radio emission of solar quiet regions are studied with the aim of detection of a number of parameters of wave processes, occurring in these regions. The observations were made at λ = 5.2 and 8.1 cm with the radio telescope THA-1500 in July - August 1963. Using the obtained data the crosscorrelation function and its spectrum have been calculated. Time spectra of power density are approximated by the function f-α, where α is in the interval 1.6 - 2.1 at λ = 5.2 cm and 1 - 1.7 at λ = 8.1 cm. Time delays of fluctuations have not been found at different wavelengths. A supposition is made that fluctuations of radio emission in the quiet atmosphere of the Sun are due to density disturbances in optical regions.

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