Physics
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..750i&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 21, July-Aug. 1981, p. 750-752. In Russian.
Physics
1
Interplanetary Medium, Shock Wave Interaction, Solar Flares, Wave Attenuation, Collision Parameters, Propagation Velocity, Refracted Waves
Scientific paper
Arguments are presented in support of the proposal that series of solar flares produce in interplanetary space ensembles of highly oblate shock waves which experience strong cancellation due to mutual collisions. An analytical solution is obtained for the head-on collision of symmetrical perpendicular shock waves, resulting in expressions for the values of the amplitude of the refracted wave, the density difference across the reflected wave, the pressure, magnetic field and density behind the refracted wave front, and the velocity of the refracted wave. The solution is then applied to demonstrate the theoretical possibility of strong cancellation in the flanking interaction of interplanetary shock waves from two successive strong solar flares.
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