Cometary brightness flares and solar corpuscular activity

Details Cometary brightness flares and solar corpuscular activity Cometary brightness flares and solar corpuscular activity

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57.1310a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 57, Nov.-Dec. 1980, p. 1310-1316.) Soviet Astronomy, vol. 24, Nov.-Dec. 1980, p. 754-757. Trans

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Comets, Solar Corpuscular Radiation, Solar Cycles, Amplitudes, Brightness, Flares, Magnetohydrodynamic Flow, Schwassmann-Wachmann Comet

Scientific paper

On the basis of an analysis of a catalog of flares of cometary brightness, evidence is given for their connection with solar corpuscular radiation. It is shown that cometary flare activity depends on the phase of the 11-year solar activity cycle: the maxima correspond to periods of rise and fall. Active phenomena in comets correlate not only with the appearance of high-velocity streams of solar plasma but also with many geophysical phenomena generated as a result of the action of the solar plasma on the earth's magnetosphere and atmosphere.

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