Radio observation at the wavelength of 3 CM during the solar eclipse of September 22, 1968

Details Radio observation at the wavelength of 3 CM during the solar eclipse of September 22, 1968 Radio observation at the wavelength of 3 CM during the solar eclipse of September 22, 1968

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975acasn..16..200.&link_type=abstract

Acta Astronomica Sinica, vol. 16, Dec. 1975, p. 200-209. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Radio Observation, Radio Sources (Astronomy), Solar Eclipses, Solar Radio Emission, Brightness Temperature, Data Processing, Radiant Flux Density, Radio Astronomy, Radio Telescopes, Solar Corona, Solar Instruments, Solar Physics, Sunspots

Scientific paper

Radio intensity measurements were performed with two radio telescopes at 3 cm wavelength during the eclipse of September 22, 1968. The data processing and the identification of S-component sources were described. The following parameters have been obtained: angular size (along the direction of the motion of the moon's center on the sun's disk), flux density, average brightness temperature and height of the S-component sources associated with sunspots, plages and coronal condensations during the eclipse.

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