Characteristic analysis of the solar radio burst event on November 2, 1992.

Details Characteristic analysis of the solar radio burst event on November 2, 1992. Characteristic analysis of the solar radio burst event on November 2, 1992.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ppmto..14..104x&link_type=abstract

Publ. Purple Mt. Obs., Vol. 14, No. 2, p. 104 - 109

Computer Science

Solar Radio Bursts: Solar Protons, Flux Densities: Solar Protons

Scientific paper

The characteristics of the solar radio outburst occurring at 0233 UT Nov 2, 1992 have been analysed in detail. The spectrum of the event is U type and an accompaning proton event with great proton flux is observed. During the period of burst there are fast pulsations superimposed on the background of the event at 9.4 GHz. The mean flux density of the event is nearly proportional to the corresponding number of fast pulsations per second.

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