Supersonic solar wind ion flows downstream of the termination shock explained by a two-fluid shock model
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:200810679/pdf
Reference29 articles.
1. Coupled quasi-linear wave damping and stochastic acceleration of pickup ions in the solar wind
2. Magnetic fields at the solar wind termination shock
3. Reflection of pre-accelerated pick-up ions at the solar wind termination shock: The seed for anomalous cosmic rays
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2. On the Energization of Pickup Ions Downstream of the Heliospheric Termination Shock by Comparing 0.52–55 keV Observed Energetic Neutral Atom Spectra to Ones Inferred from Proton Hybrid Simulations;The Astrophysical Journal Letters;2022-05-30
3. Interstellar Neutrals, Pickup Ions, and Energetic Neutral Atoms Throughout the Heliosphere: Present Theory and Modeling Overview;Space Science Reviews;2022-04
4. Boundary Conditions at the Heliospheric Termination Shock with Pickup Ions;The Astrophysical Journal;2021-07-01
5. Interaction of interplanetary shock wave with the solar wind;Journal of Atmospheric and Solar-Terrestrial Physics;2020-10
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