Solar Coronal Heating by Kinetic Alfvén Waves

The utilization of the Cairns distribution serves as a vital tool for characterizing the nonthermal attributes commonly observed in space plasmas. In these intricate plasma environments, extensive measurements have been conducted to monitor the fluctuations inherent in the perturbed electromagnetic...

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Vydané v:	The Astrophysical journal Ročník 970; číslo 2; s. 140 - 151
Hlavní autori:	Ayaz, Syed, Li, Gang, Khan, Imran A.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Philadelphia The American Astronomical Society 01.08.2024 IOP Publishing
Predmet:	Alfven waves Corona Coronal heating Distribution functions Fluctuations Heating Kinetic theory Magnetic fields Magnetohydrodynamic waves Solar atmosphere Solar corona Solar coronal heating Solar magnetic field Space plasmas
ISSN:	0004-637X, 1538-4357
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