Microwave observations of compact radio sources during solar eclipses on RT-22

Details Microwave observations of compact radio sources during solar eclipses on RT-22 Microwave observations of compact radio sources during solar eclipses on RT-22

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011astl...37...55t&link_type=abstract

Astronomy Letters, Volume 37, Issue 1, pp.55-60

Astronomy and Astrophysics

Astronomy

Sun, Coronal Bright Points, Microwave Emission, Compact Radio Sources

Scientific paper

Based on the observations of solar eclipses performed on the RT-22 radio telescope at CrAO in the wavelength range 2.0-3.5 cm, we consider the fine spatial structure of the microwave emission from the quiet Sun. We have established that the positions of compact radio sources with a typical size of about 7″.0 and coronal bright points coincide. The mean radio flux exceeds the level of the quiet Sun by 0.28 sfu. The brightness temperatures increase with wavelength and lie within the range 0.3-2.7 MK. Evidence for a nonthermal nature of the emission from compact radio sources has been obtained.

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