ASYMMETRIC SOLAR WIND ELECTRON DISTRIBUTIONS
Abstract
The present paper provides a possible explanation for the solar wind electron velocity distribution functions possessing asymmetric energetic tails. By numerically solving the electrostatic weak turbulence equations that involve nonlinear interactions among electrons, Langmuir waves, and ion-sound waves, it is shown that different ratios of ion-to-electron temperatures lead to the generation of varying degrees of asymmetric tails. The present finding may be applicable to observations in the solar wind near 1 AU and in other regions of the heliosphere and interplanetary space.
- Authors:
-
- School of Space Research, Kyung Hee University, Yongin-Si, Gyeonggi-Do 446-701 (Korea, Republic of)
- Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon 305-701 (Korea, Republic of)
- Publication Date:
- OSTI Identifier:
- 22039092
- Resource Type:
- Journal Article
- Journal Name:
- Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 755; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ASTRONOMY; ASTROPHYSICS; ASYMMETRY; DISTRIBUTION; DISTRIBUTION FUNCTIONS; ELECTRON EMISSION; ELECTRON TEMPERATURE; HELIOSPHERE; INTERPLANETARY SPACE; IONS; NONLINEAR PROBLEMS; SOLAR CORONA; SOLAR ELECTRONS; SOLAR WIND; SOUND WAVES; SUN; TURBULENCE
Citation Formats
Yoon, Peter H, Kim, Sunjung, Lee, Junggi, Lee, Junhyun, Park, Jongsun, Park, Kyungsun, Seough, Jungjoon, and Hong, Jinhy. ASYMMETRIC SOLAR WIND ELECTRON DISTRIBUTIONS. United States: N. p., 2012.
Web. doi:10.1088/0004-637X/755/2/112.
Yoon, Peter H, Kim, Sunjung, Lee, Junggi, Lee, Junhyun, Park, Jongsun, Park, Kyungsun, Seough, Jungjoon, & Hong, Jinhy. ASYMMETRIC SOLAR WIND ELECTRON DISTRIBUTIONS. United States. https://doi.org/10.1088/0004-637X/755/2/112
Yoon, Peter H, Kim, Sunjung, Lee, Junggi, Lee, Junhyun, Park, Jongsun, Park, Kyungsun, Seough, Jungjoon, and Hong, Jinhy. 2012.
"ASYMMETRIC SOLAR WIND ELECTRON DISTRIBUTIONS". United States. https://doi.org/10.1088/0004-637X/755/2/112.
@article{osti_22039092,
title = {ASYMMETRIC SOLAR WIND ELECTRON DISTRIBUTIONS},
author = {Yoon, Peter H and Kim, Sunjung and Lee, Junggi and Lee, Junhyun and Park, Jongsun and Park, Kyungsun and Seough, Jungjoon and Hong, Jinhy},
abstractNote = {The present paper provides a possible explanation for the solar wind electron velocity distribution functions possessing asymmetric energetic tails. By numerically solving the electrostatic weak turbulence equations that involve nonlinear interactions among electrons, Langmuir waves, and ion-sound waves, it is shown that different ratios of ion-to-electron temperatures lead to the generation of varying degrees of asymmetric tails. The present finding may be applicable to observations in the solar wind near 1 AU and in other regions of the heliosphere and interplanetary space.},
doi = {10.1088/0004-637X/755/2/112},
url = {https://www.osti.gov/biblio/22039092},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 755,
place = {United States},
year = {Mon Aug 20 00:00:00 EDT 2012},
month = {Mon Aug 20 00:00:00 EDT 2012}
}
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