Meter wavelength characteristics of a solar active region in August 1972

Details Meter wavelength characteristics of a solar active region in August 1972 Meter wavelength characteristics of a solar active region in August 1972

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976acasn..17...81y&link_type=abstract

Acta Astronomica Sinica, vol. 17, June 1976, p. 81-92. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Microwave Emission, Millimeter Waves, Solar Activity, Solar Protons, Solar Radio Bursts, Electron Clouds, Solar Magnetic Field, Sunspots, Superhigh Frequencies, Time Lag, Wavelengths

Scientific paper

Observations, at 146 MHz of radio bursts during the period in which the active region moved across the solar disk are described and analyzed. The data are compared with the associated S-components at centimeter wavelengths. It is found that the daily variations of the type I source are correlated with those of the S-components with a two-day time delay. This relation could be the result of the emergence of nonpotential magnetic fields imbedded in slowly moving electron plasma clouds. Strengths of the background magnetic fields are estimated from measurements of the angular size of the type I source.

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