Fine structure of a local solar radio source

Details Fine structure of a local solar radio source Fine structure of a local solar radio source

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..467b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Sept.-Oct. 1978, p. 467-470.) Soviet Astronomy Letters, vol. 4, Sept.-Oct. 1978, p.

Astronomy and Astrophysics

Astronomy

1

Fine Structure, Radio Observation, Radio Sources (Astronomy), Solar Radio Emission, Sunspots, Brightness Temperature, High Resolution, Polarized Radiation, Radio Telescopes, Solar Eclipses

Scientific paper

Radio observations of the eclipsed sun at 8 arcsec resolution have
revealed that the local source of a complex sunspot group consisted of
several separate features. In the intervening gaps the radio emission
was not enhanced. During the growth of an active region the brightness
temperature above the spots may reach 7.6 million K.

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