Short-wavelength plasma turbulence and temperature anisotropy instabilities: Recent computational progress
Abstract
Plasma turbulence consists of an ensemble of enhanced, broadband electromagnetic fluctuations, typically driven by multi-wave interactions which transfer energy in wavevector space via non- linear cascade processes. In addition, temperature anisotropy instabilities in collisionless plasmas are driven by quasi-linear wave–particle interactions which transfer particle kinetic energy to field fluctuation energy; the resulting enhanced fluctuations are typically narrowband in wavevector magnitude and direction. Whatever their sources, short-wavelength fluctuations are those at which charged particle kinetic, that is, velocity-space, properties are important; these are generally wavelengths of the order of or shorter than the ion inertial length or the thermal ion gyroradius. The purpose of this review is to summarize and interpret recent computational results concerning short-wavelength plasma turbulence, short-wavelength temperature anisotropy instabilities and relationships between the two phenomena.
- Authors:
-
- Space Science Institute, Boulder, CO (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- National Science Foundation (NSF)
- OSTI Identifier:
- 1159569
- Report Number(s):
- LA-UR-14-27994
Journal ID: ISSN 1364-503X
- Grant/Contract Number:
- AC52-06NA25396
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Philosophical Transactions of the Royal Society. A, Mathematical, Physical and Engineering Sciences
- Additional Journal Information:
- Journal Volume: 373; Journal Issue: 2041; Journal ID: ISSN 1364-503X
- Publisher:
- Royal Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 70 PLASMA PHYSICS AND FUSION TECHNOLOGY; heliospheric and magnetospheric physics; plasma turbulence; plasma instabilities
Citation Formats
Gary, S. Peter. Short-wavelength plasma turbulence and temperature anisotropy instabilities: Recent computational progress. United States: N. p., 2015.
Web. doi:10.1098/rsta.2014.0149.
Gary, S. Peter. Short-wavelength plasma turbulence and temperature anisotropy instabilities: Recent computational progress. United States. https://doi.org/10.1098/rsta.2014.0149
Gary, S. Peter. Mon .
"Short-wavelength plasma turbulence and temperature anisotropy instabilities: Recent computational progress". United States. https://doi.org/10.1098/rsta.2014.0149. https://www.osti.gov/servlets/purl/1159569.
@article{osti_1159569,
title = {Short-wavelength plasma turbulence and temperature anisotropy instabilities: Recent computational progress},
author = {Gary, S. Peter},
abstractNote = {Plasma turbulence consists of an ensemble of enhanced, broadband electromagnetic fluctuations, typically driven by multi-wave interactions which transfer energy in wavevector space via non- linear cascade processes. In addition, temperature anisotropy instabilities in collisionless plasmas are driven by quasi-linear wave–particle interactions which transfer particle kinetic energy to field fluctuation energy; the resulting enhanced fluctuations are typically narrowband in wavevector magnitude and direction. Whatever their sources, short-wavelength fluctuations are those at which charged particle kinetic, that is, velocity-space, properties are important; these are generally wavelengths of the order of or shorter than the ion inertial length or the thermal ion gyroradius. The purpose of this review is to summarize and interpret recent computational results concerning short-wavelength plasma turbulence, short-wavelength temperature anisotropy instabilities and relationships between the two phenomena.},
doi = {10.1098/rsta.2014.0149},
journal = {Philosophical Transactions of the Royal Society. A, Mathematical, Physical and Engineering Sciences},
number = 2041,
volume = 373,
place = {United States},
year = {Mon Apr 06 00:00:00 EDT 2015},
month = {Mon Apr 06 00:00:00 EDT 2015}
}
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Statistical Study of Whistler Waves in the Solar Wind at 1 au
journal, June 2019
- Tong, Yuguang; Vasko, Ivan Y.; Artemyev, Anton V.
- The Astrophysical Journal, Vol. 878, Issue 1
Effects of Alpha–Proton Differential Flow on Proton Temperature Anisotropy Instabilities in the Solar Wind: Wind Observations
journal, October 2019
- Zhao, G. Q.; Li, H.; Feng, H. Q.
- The Astrophysical Journal, Vol. 884, Issue 1
On the generation mechanism of electromagnetic cyclotron waves in the solar wind: statistical results from Wind observations
preprint, January 2018
- Zhao, G. Q.; Feng, H. Q.; Wu, D. J.
- arXiv
Statistical Study of Whistler Waves in the Solar Wind at 1 AU
text, January 2019
- Tong, Yuguang; Vasko, Ivan Y.; Artemyev, Anton V.
- arXiv
Effects of alpha-proton differential flow on proton temperature anisotropy instabilities in the solar wind: Wind observations
text, January 2019
- Zhao, G. Q.; Li, H.; Feng, H. Q.
- arXiv