Examples of magnetosphere

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The third plot shows the field lines when the filament almost reaches its maximum depth into the magnetosphere.
To understand oblique penetration, in this paper we investigate the dynamics of the filament and the magnetic field after a filament penetrates into the magnetosphere.
It is shown that within the framework of this model of the magnetosphere, plasma at each magnetic shell moves with a constant angular velocity.
The second significant non-thermal feature of observed velocity distributions is related to the loss-cone effects inherent in any mirror configuration as the planetary magnetospheres.
In nearequatorial regions of the outer magnetosphere the geomagnetic field is most likely to be a force field.
The central problem with such investigations is that currently there is no suitable self-consistent dipole (or dipole-like) model of the magnetosphere with traveling plasma.
Such results may be of relevance to the magnetosphere of pulsars.
We can call it the magnetopause of the artificial magnetosphere.
If a satellite orbiting in the magnetosphere crosses both of these surfaces, it must detect a double plasmapause.
Wave-particle interactions also have diver se applications in other planetary magnetospheres, and in other space and cosmic plasmas.
First, a filament with excess flow velocity is found to be capable of penetrating into the magnetosphere.
The simulations presented in this paper are useful only to gain a qualitative understanding of the real interaction between solar-wind filaments and the magnetosphere.
When the angle is small, the filament will penetrate deeply into the magnetosphere before it is repelled back.
The filament has penetrated deeply into the magnetosphere before it is repelled back toward the magnetopause.
This book presents an excellent, thorough description of plasma physics tools for describing large-scale plasma activity in the terrestrial magnetosphere and solar atmosphere.
These regions are also associated with energetic electrons accelerated within the planetary magnetospheres and beamed along the magnetic field to form the aurora.

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