Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311...99u&link_type=abstract
In ESA, Plasma Astrophysics p 99-101 (SEE N91-15046 06-90)
Astronomy and Astrophysics
Astrophysics
1
Magnetic Storms, Magnetohydrodynamic Waves, Shock Wave Attenuation, Solar Flares, Wave Equations, Approximation, Magnetoacoustics, Mathematical Models, Shock Waves, Solar Wind
Scientific paper
The calculation of parameters of flare shock waves arriving at Earth with moderate or small intensity by the approximation of nonlinear magnetic acoustics of a moving medium is addressed. Relationships of explosion magnetohydrodynamic shock wave damping in this approximation were previously obtained. The solution starts from the model of an undisturbed solar wind and the importance and position of the flare on the solar disk. The explosion shock parameters are calculated along ray tubes corrected by taking into account the nonlinear factor of ray displacement. Results of the calculations are detailed.
Uralova S. V.
Urolov A. M.
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