Shock waves generated by the intense solar flare of 1972, August 7, 15:00 UT

Details Shock waves generated by the intense solar flare of 1972, August 7, 15:00 UT Shock waves generated by the intense solar flare of 1972, August 7, 15:00 UT

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...37..437m&link_type=abstract

Solar Physics, vol. 37, Aug. 1974, p. 437-442.

Physics

4

Microwave Emission, Shock Wave Propagation, Solar Flares, Solar Radio Bursts, Explorer 43 Satellite, Interplanetary Gas, Piston Theory, Solar Wind Velocity, Type 2 Bursts, Type 4 Bursts

Scientific paper

The dynamic radio spectrum of the class 3B solar flare of 1972, August 7, 15:00 UT, over the band 10 to 2000 MHz is examined. Type II and type IV bursts in the spectrum are interpreted in terms of a piston-driven shock, which appeared to be traveling at a velocity of about 1500 km per sec and which generated pulsations in the band 100 to 200 MHz as it passed through the corona. The progress of the shock through the interplanetary plasma was subsequently monitored by Malitson et al. with radio equipment covering the band 0.03 to 2.6 MHz on the IMP-6 satellite.

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