Uncertainties in the heliosheath ion temperatures
The Voyager plasma observations show that the physics of the heliosheath is rather complex and that the temperature derived from observation particularly differs from expectations. To explain this fact, the temperature in the heliosheath should be based on <i>κ</i> distributions inste...
Main Authors: | K. Scherer, H. J. Fahr, H. Fichtner, A. Sylla, J. D. Richardson, M. Lazar |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2018-01-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/36/37/2018/angeo-36-37-2018.pdf |
Similar Items
-
The charge-exchange induced coupling between plasma-gas counterflows in the heliosheath
by: H. J. Fahr
Published: (2003-06-01) -
VARIABILITY OF PLASMA IN THE HELIOSHEATH
by: Richardson, John D.
Published: (2015) -
Unexpected sites of efficient stochastic acceleration in the inner heliosheath
by: S. V. Chalov, et al.
Published: (2007-03-01) -
The "step feature" of suprathermal ion distributions: a discriminator between acceleration processes?
by: H. J. Fahr, et al.
Published: (2012-09-01) -
Plasma flows in the heliosheath
by: Richardson, John D., et al.
Published: (2010)