Concerning pressure and entropy of shock-accelerated heliosheath electrons
Author:
Affiliation:
1. Argelander-Institut für Astronomie der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/484/3/3537/27714923/stz182.pdf
Reference21 articles.
1. The role of solar wind electrons at the solar wind termination shock
2. Unexpected sites of efficient stochastic acceleration in the inner heliosheath
3. Revisiting the theory of the evolution of pick-up ion distributions: magnetic or adiabatic cooling?
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1. The Role of Electrons and Helium Atoms in Global Modeling of the Heliosphere;The Astrophysical Journal;2023-04-01
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3. On ‘Isobaric and Isentropic’ Distribution Functions of Plasma Particles in the Heliosheath;Kappa Distributions;2021
4. Probing the thermodynamic conditions of the heliosheath plasma by shock wave propagation;Astronomy & Astrophysics;2020-10
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