The evolution and structure of the flare-active region HR 16 631 (February 1980) based on RATAN-600 observations

Details The evolution and structure of the flare-active region HR 16 631 (February 1980) based on RATAN-600 observations The evolution and structure of the flare-active region HR 16 631 (February 1980) based on RATAN-600 observations

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...63b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Jan.-Feb. 1989, p. 63-67. In Russian.

Physics

3

Radio Telescopes, Solar Flares, Solar Radio Emission, Sunspots, Magnetic Flux, Photosphere, Polarized Radiation, Solar Magnetic Field, Solar X-Rays

Scientific paper

The evolution of a local radio source associated with the flare-active solar region HR 16 631 (February 1980) is studied. RATAN-600 observations at five wavelengths in the 2-4 cm range are used. It is shown that, during the period of increased flare activity of the sunspot group, a peculiar source situated above the region of the maximum magnetic field gradient appears and dominates in the local radio source structure. This peculiar source is associated with the region of the emerging new magnetic flux.

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