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Cited article:

Potential Flow Theory Formulation of Parker’s Unsteady Solar Wind Model and Nonlinear Stability of Parker’s Steady Solar Wind Solution

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The Astrophysical Journal 985 (1) 3 (2025)
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Thermodynamics of Alfvénic slow solar wind produced by Alfvénic turbulence

Hwanhee Lee, Jungjoon Seough, Bo Li, Yeon-Han Kim and Kyung-Suk Cho
Monthly Notices of the Royal Astronomical Society 532 (3) 3268 (2024)
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What is the Solar Wind Frame of Reference?

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The Astrophysical Journal 889 (2) 163 (2020)
https://doi.org/10.3847/1538-4357/ab65f7

MULTI-FLUID APPROACH TO HIGH-FREQUENCY WAVES IN PLASMAS. I. SMALL-AMPLITUDE REGIME IN FULLY IONIZED MEDIUM

David Martínez-Gómez, Roberto Soler and Jaume Terradas
The Astrophysical Journal 832 (2) 101 (2016)
https://doi.org/10.3847/0004-637X/832/2/101

Turbulent heating and acceleration of He++ ions by spectra of Alfvén-cyclotron waves in the expanding solar wind: 1.5-D hybrid simulations

Y. G. Maneva, A. F. Viñas and L. Ofman
Journal of Geophysical Research: Space Physics 118 (6) 2842 (2013)
https://doi.org/10.1002/jgra.50363

Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision

Ming Xiong, Huinan Zheng and Shui Wang
Journal of Geophysical Research: Space Physics 114 (A11) (2009)
https://doi.org/10.1029/2009JA014079