Proton temperature relaxation in the solar wind by combined collective and collisional processes
Author:
Affiliation:
1. Institute for Physical Science and Technology University of Maryland College Park Maryland USA
2. Also at School of Space Research Kyung Hee University Yongin Korea
Funder
National Science Foundation
National Research Foundation of Korea
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023044
Reference44 articles.
1. Magnetized plasma kinetic theory. II. Derivation of Rosenbluth potentials for a uniform magnetized plasma
2. Magnetic Fluctuation Power Near Proton Temperature Anisotropy Instability Thresholds in the Solar Wind
3. LIMITS ON ALPHA PARTICLE TEMPERATURE ANISOTROPY AND DIFFERENTIAL FLOW FROM KINETIC INSTABILITIES: SOLAR WIND OBSERVATIONS
4. INCORPORATING KINETIC PHYSICS INTO A TWO-FLUID SOLAR-WIND MODEL WITH TEMPERATURE ANISOTROPY AND LOW-FREQUENCY ALFVÉN-WAVE TURBULENCE
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1. Boundary of the Distribution of Solar Wind Proton Beta versus Temperature Anisotropy;The Astrophysical Journal;2024-07-01
2. Expanding-box Quasilinear Model of the Solar Wind;The Astrophysical Journal;2023-07-28
3. The multi-scale nature of the solar wind;Living Reviews in Solar Physics;2019-12
4. Solar Wind Temperature Isotropy;Physical Review Letters;2019-10-03
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