Kappa Distributions: Theory and Applications in Space Plasmas |
| |
Authors: | V Pierrard M Lazar |
| |
Institution: | 1.Belgian Institute for Space Aeronomy, Space Physics,Brussels,Belgium;2.Center for Space Radiations, Institute of Research in Mathematics and Physics,Université Catholique de Louvain,Louvain-La-Neuve,Belgium;3.Research Department – Plasmas with Complex Interactions,Ruhr-Universit?t Bochum,Bochum,Germany;4.Center for Plasma Astrophysics,Leuven,Belgium |
| |
Abstract: | The plasma particle velocity distributions observed in the solar wind generally show enhanced (non-Maxwellian) suprathermal
tails, decreasing as a power law of the velocity and well described by the family of Kappa distribution functions. The presence
of non-thermal populations at different altitudes in space plasmas suggests a universal mechanism for their creation and important
consequences concerning plasma fluctuations, the resonant and nonresonant wave – particle acceleration and plasma heating.
These effects are well described by the kinetic approaches where no closure requires the distributions to be nearly Maxwellian.
This paper summarizes and analyzes the various theories proposed for the Kappa distributions and their valuable applications
in coronal and space plasmas. |
| |
Keywords: | |
本文献已被 SpringerLink 等数据库收录! |
|