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Energetic solar particle behaviour in the magnetosphere (1979)

Scholer, M.

In: CASI

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Publication Date: 2006-01-16

Description: The behavior of energetic solar flare particles in the magnetosphere is discussed. In the absence of magnetospheric motion, the problem of particle transport can be treated as simple propagation of charged particles in a stationary magnetic field configuration using, for instance, trajectory calculations in model fields. This single particle approach is the basis for the determination of intensity and anisotropy structures over the polar caps and in the geomagnetic tail from different interplanetary conditions. Particle transport on closed field lines is in addition strongly affected by resonant interaction processes as pitch angle scattering and radial diffusion.

Keywords: GEOPHYSICS

Type: NASA. Marshall Space Flight Center Solar-Terrest. Predictions Proc., Vol. 2; p 446-463

Format: text

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