A combined optical and radio study of the solar ejection of 1982 January 22

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Solar Flares, Solar Radio Bursts, Stellar Mass Ejection, H Alpha Line, Radiant Flux Density, Radio Spectra, Solar Magnetic Field, Type 2 Bursts, Type 3 Bursts, Type 5 Bursts

Scientific paper

The west-limb ejection event of 0423 UT on January 22, 1982, is characterized on the basis of H-alpha observations obtained with the chromosphere telescope at Beijing Observatory; Culgoora radio dynamic spectra, 80-MHz images, and 80-MHz and 160-MHz total fluxes; total fluxes at 1.415, 2.695, 4.995, 8.800, and 15.400 GHz from Western Australia Radio Station; and geomagnetic data from Beijing Geomagnetic Observatory. Consideration is given to the Type III + IV burst, the Type II burst, a weak Type IV(mu) burst, and the flux-rate/time curve of the bursts in cm and dm wavelengths; and the main H-alpha mass ejection is examined in detail. Parameters estimated for this ejection include magnetic field 12 G, mass 10 to the 38th electrons (or about 100 Tg), and energy 8 x 10 to the 29th erg (of the total event energy 2 x 10 to the 30th erg). The fact that this clump did not disperse immediately is attributed to the magnetic field, inertia, and the ram pressure on the surrounding medium.

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