Publication Date:
2016-06-07
Description:
The interaction of a nonstationary plasma flow with a model ionosphere is studied. On the basis of a numerical simulation, the calculation yields results of the distribution of the plasma concentration and magnetic field in the transition region.
Keywords:
ASTROPHYSICS
Type:
NASA. Goddard Space Flight Center Solar-Wind Interaction with the Planets Mercury, Venus, and Mars; p 151-158
Format:
application/pdf