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2019ApJ...886...89W - Astrophys. J., 886, 89-89 (2019/December-1)

The diffusion coefficient with displacement variance of energetic particles caused by adiabatic focusing.

WANG J.F. and QIN G.

Abstract (from CDS):

The equation κzz = dσ2/(2dt) describing the relation of the parallel diffusion coefficient κzz with the displacement variance σ2 (hereafter DCDV) is a well-known formula. In this study, we find that DCDV is only applicable to two kinds of transport equations of the isotropic distribution function, one without cross-terms and the other without a convection term. Here, by employing the more general transport equation, i.e., the variable coefficient differential equation derived from the Fokker-Planck equation, a new equation of κzz as a function of σ2 is obtained. We find that DCDV is the special case of the new equation. In addition, another equation of κzz as a function of σ2 corresponding to the telegraph equation is also investigated preliminarily.

Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.

Journal keyword(s): Interplanetary turbulence - Magnetic fields - Solar energetic particles

Simbad objects: 0

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