Observation of the 22 September, 1968 solar eclipse at wavelength 11.1 CM

Details Observation of the 22 September, 1968 solar eclipse at wavelength 11.1 CM Observation of the 22 September, 1968 solar eclipse at wavelength 11.1 CM

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974acasn..15..113.&link_type=abstract

Acta Astronomica Sinica, vol. 15, Oct. 1974, p. 113-122. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Brightness Temperature, Radiant Flux Density, Radio Sources (Astronomy), Solar Eclipses, Solar Radio Emission, Data Processing, Solar Instruments, Solar Observatories, Sunspots

Scientific paper

Measurements were made of the 22 September, 1968 solar eclipse by Purple Mountain Observatory in Kashih, Sinkiang at wavelength of 11.1 cm. The association of radio sources with the optical active regions was examined. Source flux densities, associated one-dimensional source sizes, heights and brightness temperatures for these regions are given. The measure of emission from the halo above plage was calculated to be about 1.4 times 10 to the 28th electron squared per cm to the fifth power.

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