Radial diffusion revisited

Details Radial diffusion revisited Radial diffusion revisited

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995em%26p...71...33r&link_type=abstract

Earth, Moon, and Planets, Volume 71, Issue 1-2, pp. 33-41

Physics

Scientific paper

The radial diffusion of equatorially mirroring particles (J = 0) is considered for Jupiter. A steady-state phase-space density distribution is obtained for (i) source-loss-free diffusion; (ii) diffusion with synchrotron radiation losses only and (iii) diffusion with synchrotron radiation plus the resonant wave-particle interaction losses. The resonant wave-particle interaction is assumed to occur when particles are in phase with a wave propagating across the magnetic field. The interaction of particles which go through a ∇B drift with electrostatic plasma waves is shown to alter the phase-space density which is observed byPioneer 10 and 11 flybys.

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