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Cited article:

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Turbulent Heating of Solar Wind Plasma Downstream of Magnetohydrodynamic Shocks

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Recent Developments in Particle Acceleration at Shocks: Theory and Observations

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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

Matina Gkioulidou, M. Opher, M. Kornbleuth, K. Dialynas, J. Giacalone, J. D. Richardson, G. P. Zank, S. A. Fuselier, D. G. Mitchell, S. M. Krimigis, E. Roussos and I. Baliukin
The Astrophysical Journal Letters 931 (2) L21 (2022)
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Boundary Conditions at the Heliospheric Termination Shock with Pickup Ions

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The Astrophysical Journal 916 (1) 57 (2021)
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Warm protons at comet 67P/Churyumov–Gerasimenko – implications for the infant bow shock

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A computational study of the properties of the quasi-perpendicular fast forward shock event during solar maximum

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Evolution of Entropy and Mediation of the Solar Wind by Turbulence

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Concerning pressure and entropy of shock-accelerated heliosheath electrons

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Temperature of electrons downstream of the solar wind termination shock

S V Chalov
Monthly Notices of the Royal Astronomical Society 485 (4) 5207 (2019)
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Neutralized solar wind ahead of the Earth's magnetopause as contribution to non-thermal exospheric hydrogen

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Rankine‐Hugoniot Relations in Multispecies Plasma With Gyrotropic Anisotropic Downstream Ion Distributions

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Journal of Geophysical Research: Space Physics 122 (12) (2017)
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On the evolution of the κ distribution of protons in the inner heliosheath

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Journal of Geophysical Research: Space Physics 121 (9) 8203 (2016)
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GENERALIZED MULTI-POLYTROPIC RANKINE–HUGONIOT RELATIONS AND THE ENTROPY CONDITION

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Testing the H-wave Hypothesis for the Origin of the IBEX Ribbon

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The electron distribution function downstream of the solar-wind termination shock: Where are the hot electrons?

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Astronomy & Astrophysics 579 A18 (2015)
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