A numerical study of the propagation of flare-induced shock waves

Details A numerical study of the propagation of flare-induced shock waves A numerical study of the propagation of flare-induced shock waves

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..242h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 2, p. 242-248.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using a one-dimensional MHD model and the shock fitting method (SFM) we discuss the propagation of flare-induced shocks and the associated wave structure downstream. It is shown that in the downstream region a rarefaction wave system forms, consisting of a fast rarefaction wave pair and a reverse slow rarefaction wave and an entropy wave-like structure sandwiched in between. It is also shown that the alternative method, the shock capturing method (SCM) cannot provide an acceptable description of the propagation in the interplanetary space.

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