Theoretical non-Maxwellian particle velocity distribution functions for spherically symmetric solar wind-like plasma systems and consequences
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 8 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Skewness and kurtosis of solar wind proton distribution functions: The normal inverse-Gaussian model and its implications;Astronomy & Astrophysics;2024-01-31
2. Multiscale views of an Alfvénic slow solar wind: 3D velocity distribution functions observed by the Proton-Alpha Sensor of Solar Orbiter;Astronomy & Astrophysics;2021-12
3. A Generalized Model for the Proton Expansion in Astrophysical Winds. I. The Velocity Distribution Function Representation;The Astrophysical Journal;1997-07
4. The Excitation Equilibrium in the Solar Corona and Non-Maxwellian Electron Distributions;International Astronomical Union Colloquium;1994
5. The ionization balance of the Fe in the solar corona for a non-Maxwellian electron distribution function;Solar Physics;1992-08
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