Numerical Modeling of Electron Transport in Solar Wind: Effects of Whistler Turbulence and Coulomb Collisions
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
http://stacks.iop.org/1742-6596/1100/i=1/a=012025/pdf
Reference20 articles.
1. Radial evolution of nonthermal electron populations in the low-latitude solar wind: Helios, Cluster, and Ulysses Observations
2. Electron Properties and Coulomb Collisions in the Solar Wind at 1 AU:WindObservations
3. Self-Similar Theory of Thermal Conduction and Application to the Solar Wind
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1. Suprathermal Electron Transport in the Solar Wind: Effects of Coulomb Collisions and Whistler Turbulence;The Astrophysical Journal;2024-03-29
2. Stability of superthermal strahl electrons in the solar wind;Monthly Notices of the Royal Astronomical Society;2021-08-02
3. Exploring the Properties of the Electron Strahl at 1 AU as an Indicator of the Quality of the Magnetic Connection Between the Earth and the Sun;Frontiers in Astronomy and Space Sciences;2021-03-05
4. The Interplay Between Ambipolar Electric Field and Coulomb Collisions in the Solar Wind Acceleration Region;Journal of Geophysical Research: Space Physics;2021-03
5. Collisionless Heat Flux Regulation via the Electron Firehose Instability in the Presence of a Core and Suprathermal Population in the Expanding Solar Wind;The Astrophysical Journal;2020-07-30
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