The blast wave propagating in a moving medium with variable density

Details The blast wave propagating in a moving medium with variable density The blast wave propagating in a moving medium with variable density

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982chjss...2...63w&link_type=abstract

Chinese Journal oF Space Sciences, vol. 2, Jan. 1982, p. 63-72. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

4

Detonation Waves, Plasma Density, Shock Wave Propagation, Solar Flares, Solar Wind Velocity, Spaceborne Astronomy, Deceleration, Interplanetary Space, Pioneer 10 Space Probe, Pioneer 11 Space Probe, Propagation Velocity

Scientific paper

On the basis of analytical solutions obtained for a blast wave propagating from a point source in a moving medium with variable density, a discussion is undertaken of important characteristics of flare-generated shock waves propagating in the solar wind. The 1 AU region is found to be a transitional one encompassing several important effects on the shock waves. The equivalent power of shock wave deceleration is a function of solar wind velocity, shock wave energy, shock propagation distance, and convective effects of the solar wind. Attention is given to Pioneer 10 and 11 observations.

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