Physics
Scientific paper
Jun 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..617d&link_type=abstract
The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 617-620 (1999).
Physics
Particle Acceleration
Scientific paper
We applied our model of space plasma consisting from two types of particle scatters moving with different speeds to the situation in the Heliosphere. We consider: 1-solar wind plasma as background plasma moving with some velocity u with frozen in magnetic inhomogeneties, and 2-magnetic clouds, high speed streams, shock waves (considered only as scatters) moving with some average velocity U. We suppose that u and U contain regular and fluctuating parts: u=uo+u1 and U=Uo+U1. From the collisional Boltzmann equation we derive the diffusion approximation describing the propagation and acceleration of charged particles. This diffusion approximation consists with usually used at uo=Uo. It is shown that when uo≠Uo, we obtain particle acceleration and convection, additional to well known acceleration and convection processes.
Dorman Lev I.
Shogenov Kh. V.
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