Relaxation of electron fluxes generating type III bursts

Details Relaxation of electron fluxes generating type III bursts Relaxation of electron fluxes generating type III bursts

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..323l&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Radio Bursts, Relaxation Processes, Electrons

Scientific paper

A one-dimensional analysis of the quasilinear relaxation process is made of the electron fluxes produced as a result of fast local heating. The initial stage of the process is investigated by the perturbation method. The subsequent relaxation process is investigated by numerical simulation. It is shown that the main effect determining the flux relaxation is the kinematic effect of the spreading of electrons in the space due to their different velocities. Quasilinear diffusion under the influence of plasma turbulence gives rise a local "plateau" on the top of the distribution function at each point of space without an essential growth in velocity spread. Results obtained are compared with type III solar radio bursts observations.

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