The electron distribution function downstream of the solar-wind termination shock: Where are the hot electrons?
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Title
The electron distribution function downstream of the solar-wind termination shock: Where are the hot electrons?
Authors
Keywords
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Journal
ASTRONOMY & ASTROPHYSICS
Volume 579, Issue -, Pages A18
Publisher
EDP Sciences
Online
2015-05-22
DOI
10.1051/0004-6361/201525710
References
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Related references
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- ON QUIET-TIME SOLAR WIND ELECTRON DISTRIBUTIONS IN DYNAMICAL EQUILIBRIUM WITH LANGMUIR TURBULENCE
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- On Solar-Wind Electron Heating at Large Solar Distances
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- Phasespace transport of a quasi-neutral multi-fluid plasma over the solar wind MHD termination shock
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- Asymptotic equilibrium between Langmuir turbulence and suprathermal electrons in three dimensions
- (2012) Peter H. Yoon PHYSICS OF PLASMAS
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- Upstream ions converting into downstream pick-up ions: the effect of shock-decelerated frozen-in fields
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- MICROSTRUCTURE OF THE HELIOSPHERIC TERMINATION SHOCK: IMPLICATIONS FOR ENERGETIC NEUTRAL ATOM OBSERVATIONS
- (2009) G. P. Zank et al. ASTROPHYSICAL JOURNAL
- The Effects of a κ‐Distribution in the Heliosheath on the Global Heliosphere and ENA Flux at 1 AU
- (2008) J. Heerikhuisen et al. ASTROPHYSICAL JOURNAL
- Mediation of the solar wind termination shock by non-thermal ions
- (2008) R. B. Decker et al. NATURE
- Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock
- (2008) John D. Richardson et al. NATURE
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