Transport equations for low-energy solar particles in evolving interplanetary magnetic fields

Details Transport equations for low-energy solar particles in evolving interplanetary magnetic fields Transport equations for low-energy solar particles in evolving interplanetary magnetic fields

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..114..165n&link_type=abstract

Solar Physics, Volume 114, Issue 1, pp.165-179

Physics

Scientific paper

Two new forms of a simplified Fokker-Planck equation are derived for the transport of low-energy solar energetic particles in an evolving interplanetary magnetic field, carried by a variable radial solar wind. An idealised solution suggests that the ‘invariant’ anisotropy direction reported by Allum et al. (1974) may be explained within the conventional theoretical framework. The equations may be used to relate studies of solar particle propagation to solar wind transients, and vice versa.

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