Pitch-angle scattering of energetic particles with adiabatic focusing
arXiv:1408.6947 · doi:10.1088/0004-637X/794/2/138
Abstract
Understanding turbulent transport of charged particles in magnetized plasmas often requires a model for the description of random variations in the particle's pitch angle. The Fokker-Planck coefficient of pitch-angle scattering, which is used to describe scattering parallel to the mean magnetic field, is therefore of central importance. Whereas quasi-linear theory assumes a homogeneous mean magnetic field, such a condition is often not fulfilled, especially for high-energy particles. Here, a new derivation of the quasi-linear approach is given that is based on the unperturbed orbit found for an adiabatically focused mean magnetic field. The results show that, depending on the ratio of the focusing length and the particle's Larmor radius, the Fokker-Planck coefficient is significantly modified but agrees with the classical expression in the limit of a homogeneous mean magnetic field.
arXiv comment10 pages, 6 figures, accepted for publication in ApJ
References in corpus (6)
- Global Dynamical Evolution of the ISM in Star Forming Galaxies - I. High Resolution 3D HD and MHD Simulations: Effect of the Magnetic Field
- Particle Transport in intense small scale magnetic turbulence with a mean field
- A Generalized Diffusion Tensor for Fully Anisotropic Diffusion of Energetic Particles in the Heliospheric Magnetic Field
- Tomography of plasma flows in the upper solar convection zone using time--distance inversion combining ridge and phase-speed filtering
- Pitch-angle scattering in magnetostatic turbulence. I. Test-particle simulations and the validity of analytical results
- Pitch-angle scattering in magnetostatic turbulence. II. Analytical considerations and pitch-angle isotropization
Cited by in corpus (6)
- An empirical modification of the force field approach to describe the modulation of galactic cosmic rays close to Earth in a broad range of rigidities
- Explaining TeV Cosmic-Ray Anisotropies with Non-Diffusive Cosmic-Ray Propagation
- Perpendicular Diffusion in the Transport of Solar Energetic Particles from Unconnected Sources: The Counter-streaming Particle Beams Revisited
- Parallel and perpendicular diffusion coefficients of energetic charged particles with adiabatic focusing
- Propagation of Solar Energetic Particles in the Outer Heliosphere: Interplay between Scattering and Adiabatic Focusing
- An Evaluation of Different Numerical Methods to Calculate the Pitch-angle Diffusion Coefficient from Full-orbit Simulations: disentangling a rope of sand