The blast wave propagating in a variable density medium with ring-magnetic field

Details The blast wave propagating in a variable density medium with ring-magnetic field The blast wave propagating in a variable density medium with ring-magnetic field

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...3..135w&link_type=abstract

Chinese Journal of Space Science, vol. 3, April 1983, p. 135-145. In Chinese, with abstract in English.

Physics

1

Interplanetary Space, Magnetic Field Configurations, Shock Wave Propagation, Solar Flares, Magnetic Disturbances, Solar Terrestrial Interactions, Space Density

Scientific paper

The propagation of solar flare shock waves is discussed based on analytical solutions for blast waves propagating in a variable density medium with a ring magnetic field. When the flare shock waves propagate into interplanetary space, the configuration of the magnetic field appears to be of the U type and occurs mainly in part of the shock wave head. The flare shock waves must have higher energy than the magnetic cutoff energy. The ring-closed region of the magnetic field offers a stronger constraint to the propagation of the shock wave.

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