Some features of solar magnetic flares. I - Magnetic field oscillations of spots in an active region

Details Some features of solar magnetic flares. I - Magnetic field oscillations of spots in an active region Some features of solar magnetic flares. I - Magnetic field oscillations of spots in an active region

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976avest..10...61c&link_type=abstract

(Astronomicheskii Vestnik, vol. 10, Jan.-Mar. 1976, p. 61-67.) Solar System Research, vol. 10, no. 1, July 1976, p. 47-51. Tran

Astronomy and Astrophysics

Astronomy

Magnetic Flux, Magnetic Variations, Solar Flares, Solar Magnetic Field, Sunspots, Chromosphere

Scientific paper

A method and results of observations of the intensity H of sunspot magnetic fields is given. During periods of flare lull on the sun, the values of H for the spots remain relatively constant for 4-6 h. After a chromospheric flare or an increase in the brightness of the floculli near the spots in the same active region, a short-term increase (pulsation) of H called a magnetic flare is observed. Chromospheric and magnetic flares appear to be parallel processes in time. A magnetic flare is not a consequence of a chromospheric flare.

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