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

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Transport equations for low-energy solar particles in evolving interplanetary magnetic fields does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Transport equations for low-energy solar particles in evolving interplanetary magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transport equations for low-energy solar particles in evolving interplanetary magnetic fields will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1693049

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.