Observation of solar Type II bursts at low radio frequencies

Details Observation of solar Type II bursts at low radio frequencies Observation of solar Type II bursts at low radio frequencies

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..117g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, Jan.-Feb. 1977, p. 117-124. In Russian.

Astronomy and Astrophysics

Astronomy

Radio Astronomy, Satellite-Borne Instruments, Shock Wave Propagation, Solar Corona, Type 2 Bursts, Astronomical Models, Distribution Functions, Electron Density (Concentration), Electron Distribution, Propagation Velocity, Solar Activity Effects

Scientific paper

Observations of Type II bursts on board the satellites Prognoz 1 and 2 at frequencies between 70 and 750 kHz are discussed. The mean rate of shock wave propagation is estimated for each individual observations during the period from May through August 1972. These estimates are obtained for two models of the electron concentration distribution in the solar corona.

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