Collisional relaxation of bi-Maxwellian plasma temperatures in magnetized plasmas-Reference-Cited by-同舟云学术

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Collisional relaxation of bi-Maxwellian plasma temperatures in magnetized plasmas

Published:2016-07 Issue:7 Volume:23 Page:072114
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Yoon Peter H.¹^ORCID

Affiliation:

1. University of Maryland, College Park, Maryland 20742, USA

Funder

GFT Foundation

Directorate for Geosciences (GEO)

National Research Foundation of Korea (NRF)

Ruhr-Universität Bochum (RUB)

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/am-pdf/10.1063/1.4958813

Reference30 articles.

1. Dynamics of the Interplanetary Gas and Magnetic Fields.

2. Interplanetary Gas. III. a Hydrodynamic Model of the Corona.

3. Kinetic models of the solar wind

4. Basics of the Solar Wind

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1. Expanding-box Quasilinear Model of the Solar Wind;The Astrophysical Journal;2023-07-28

2. Collision term for uniformly magnetized plasmas;Reviews of Modern Plasma Physics;2023-04-23

3. Quasilinear theory of general electromagnetic fluctuations including discrete particle effects for magnetized plasmas: General analysis;Physics of Plasmas;2022-09

4. Strong Magnetic Field Effects on the Collision Term and Electron-Ion Temperature Relaxation;Journal of Fusion Energy;2020-12

5. Solar Wind Temperature Isotropy;Physical Review Letters;2019-10-03

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