Abstract:
A numerical method to calculate “subsonic” regions of the flow to the stationary problems,
when supersonic and superaflven gas stream with infinite electrical conductivity carrying
frozen-in magnetic field flows past conducting bodies, is considered within the framework
of the ideal 3-D magnetohydrodynamic (MHD) model. Test examples on calculation of gas
dynamical and MHD flows and an example of the 3-D solar wind flow past the earth's
magnetopause are presented.
Fulltext:
PDF file (1777 kB)