Detection of the solar chromospheric network at centimeter wavelengths

Details Detection of the solar chromospheric network at centimeter wavelengths Detection of the solar chromospheric network at centimeter wavelengths

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sval....1..205b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 1, Oct. 1975, p. 25-27.) Soviet Astronomy Letters, vol. 1, Sept.-Oct. 1975, p. 205. Tra

Astronomy and Astrophysics

Astronomy

1

Chromosphere, Microwave Emission, Radio Astronomy, Solar Granulation, Solar Radio Emission, Radio Telescopes, Solar Atmosphere, Solar Flux Density

Scientific paper

Results are reported for radio telescopic observations of small-scale brightness fluctuations at wavelengths of 2 to 4 cm in the chromosphere of the quiet sun. These fluctuations are found to have characteristic dimensions of about 12 sec and a flux density corresponding to 0.00001 of the total solar flux. Data analysis shows that the fluctuations are most likely associated with a radio-range chromospheric mesh (supergranulation, spicules, spicule clusters).

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