Nonevolutionary MHD shocks in the solar wind and interstellar medium interaction

Details Nonevolutionary MHD shocks in the solar wind and interstellar medium interaction Nonevolutionary MHD shocks in the solar wind and interstellar medium interaction

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...354..697p&link_type=abstract

Astronomy and Astrophysics, v.354, p.697-702 (2000)

Astronomy and Astrophysics

Astrophysics

23

Magnetohydrodynamics (Mhd), Shock Waves, Sun: Solar Wind, Ism: Kinematics And Dynamics

Scientific paper

We present the study of the solar wind interaction with the super-Alfvénic magnetized interstellar medium in the controversial case when fast magnetosonic shocks are nonevolutionary, while admissible switch-on shocks cannot exist due to geometrical reasons. The flow behaviour and the accompanying shock configuration are investigated both in the two-dimensional axisymmetric and 2.5-dimensional, that is, permitting rotation around the symmetry axis, statements. General questions of the origin of nonevolutionary MHD shocks are discussed.

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