Diffusion coefficient with displacement variance of energetic particles with adiabatic focusing
arXiv:1909.11547 · doi:10.3847/1538-4357/ab505e
Abstract
The equation (hereafter DCDV) is a well-known formula of energetic particles describing the relation of parallel diffusion coefficient with the parallel displacement variance . In this study, we find that DCDV is only applicable to two kinds of transport equations of isotropic distribution function, one is without cross terms, the other is without 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 as a function of is obtained. We find that DCDV is the special case of the new equation. In addition, another equation of as a function of corresponding to the telegraph equation is also investigated preliminarily.
References in corpus (8)
- Analytical description of stochastic field-line wandering in magnetic turbulence
- The Diffusion Approximation vs. the Telegraph Equation for Modeling Solar Energetic Particle Transport with Adiabatic Focusing. I. Isotropic Pitch-angle Scattering
- The Modification of the Nonlinear Guiding Center Theory
- Cosmic Ray Transport with Magnetic Focusing and the "Telegraph" model
- An Exact Solution of the Fokker-Planck Equation for Isotropic Scattering
- Parallel and perpendicular diffusion coefficients of energetic charged particles with adiabatic focusing
- Perpendicular diffusion coefficient of cosmic rays in the presence of weak adiabatic focusing
- Magnetic field line random walk in two-dimensional dynamical turbulence
Cited by in corpus (4)
- Turbulent diffusion of streaming cosmic rays in compressible, partially ionised plasma
- Diffusion of cosmic-ray electrons in M 51 observed with LOFAR at 54 MHz
- The invariance of the diffusion coefficient with the iterative operations of charged particles' transport equation
- Study of momentum diffusion with the effect of adiabatic focusing