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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Bibliographic Details

Published in:	The Astrophysical journal Vol. 970; no. 2; pp. 140 - 151
Main Authors:	Ayaz, Syed, Li, Gang, Khan, Imran A.
Format:	Journal Article
Language:	English
Published:	Philadelphia The American Astronomical Society 01.08.2024 IOP Publishing
Subjects:	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
Online Access:	Get full text
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