Proton and He 2+ Temperature Anisotropies in the Solar Wind Driven by Ion Cyclotron Waves
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/1009-9271/5/2/009/pdf
Reference32 articles.
1. Ion Cyclotron Wave Dissipation in the Solar Corona: The Summed Effect of More than 2000 Ion Species
2. Ion cyclotron diffusion of velocity distributions in the extended solar corona
3. Interpenetrating solar wind streams
4. The ion cyclotron anisotropy instability and the inverse correlation between proton anisotropy and proton beta
5. Proton temperature anisotropy constraint in the solar wind: ACE observations
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3. Two-dimensional hybrid models of H+ -He++ expanding solar wind plasma heating;Journal of Geophysical Research: Space Physics;2014-06
4. Instantaneous frequency and wave mode identification in a magnetosheath using few spatial points;Chinese Physics B;2013-08
5. The Effects of Relative Drift Velocities Between Proton and He2+on the Magnetic Spectral Signatures in the Plasma Depletion Layer;Plasma Science and Technology;2011-10
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