Generation of coronal and interplanetary shock waves during the solar flares of 2-13 August 1972

Details Generation of coronal and interplanetary shock waves during the solar flares of 2-13 August 1972 Generation of coronal and interplanetary shock waves during the solar flares of 2-13 August 1972

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977izssr..41.1849p&link_type=abstract

(Mezhdunarodnyi Seminar po Aktivnym Protsessam na Solntse i Probleme Solnechnykh Neitrino, 8th, Leningrad, USSR, Sept. 25-27, 19

Mathematics

2

Interplanetary Medium, Shock Wave Propagation, Solar Corona, Solar Flares, Deceleration, Pioneer 9 Space Probe, Satellite Observation, Solar Spectra, Time Lag, Type 2 Bursts

Scientific paper

Data on Type II bursts for the flare-active period of August 1972 were interpreted to determine whether shock waves observed to be propagating in the interplanetary medium are of coronal origin. The acceleration and time lag dynamics of four shock waves generated in the Mc Math 11 976 region were analyzed using Pioneer 9 and the earth as detectors. The most significant result was that a linear time lag was found for only one of the waves. Consideration was also given to the amount of mechanical energy freed in each of the four flares.

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