On coupling between magnetic field and plasma flow in the solar wind.
Abstract
A steady state model of the solar wind flow in the equatorial plane is solved for both the radial and azimuthal motions for the case of neglecting the effect of magnetic field on the particles temperatures in solar wind, making use of the results of two known two-fluid solar wind models.
- Publication:
-
Acta Geophys. Sinica
- Pub Date:
- 1988
- Bibcode:
- 1988AcGSn..31..622C
- Keywords:
-
- Magnetic Fields:Solar Wind;
- Plasma:Solar Wind;
- Solar Wind:Magnetic Fields;
- Solar Wind:Plasma