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Turbulent Heating of Solar Wind Plasma Downstream of Magnetohydrodynamic Shocks

Interplanetary (IP) shocks are believed to play a significant role in both amplifying the background level of turbulent fluctuations and in heating the bulk solar wind (SW). This study investigates the thermodynamic properties downstream of IP shocks. We examine the temperature, density, and specifi...

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Principais autores: Alexander Pitňa, Jana Šafránková, Zdeněk Němeček, Gilbert Pi, Gary Zank, Lingling Zhao, Laxman Adhikari, Masaru Nakanotani
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2024-01-01
Serier:The Astrophysical Journal
Fag:
Interplanetary shocks
Interplanetary turbulence
Solar wind
Online adgang:https://doi.org/10.3847/1538-4357/ad1c64
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