Observations of bursts of long-wavelength radio emission during large chromospheric events.

Details Observations of bursts of long-wavelength radio emission during large chromospheric events. Observations of bursts of long-wavelength radio emission during large chromospheric events.

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cosre..26..781g&link_type=abstract

Cosmic Res., Vol. 26, No. 6, p. 781 - 789

Physics

Solar Radio Bursts

Scientific paper

The authors present the results of their analysis of bursts of long-wavelength radio emission in the frequency range from 540 to 2160 kHz. The data were recorded in April - May 1981 by the Prognoz-2 satellite, and they refer to events which are associated with the development of large chromospheric flares on the Sun. Judging from the time delay between the bursts of long-wavelength radio emission and the explosive phase of the flares, all of the observed events can be divided into three major groups: (1) events in which type III bursts coincide with the explosive phase of the flare; (2) events with bursts belonging to the shock accelerated (SA) type, with delays of up to several minutes relative to the explosive phase; and (3) events which are characterized by the presence of large chromospheric flares but there are no bursts of long-wavelength radio emission.

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