Localized Heating and Dynamics of the Solar Corona due to a Symbiosis of Waves and Reconnection

Localized Heating and Dynamics of the Solar Corona due to a Symbiosis of Waves and Reconnection

The Sun’s outer atmosphere, the corona, is maintained at mega-Kelvin temperatures and fills the heliosphere with a supersonic outflowing wind. The dissipation of magnetic waves and direct electric currents are likely to be the most significant processes for heating the corona, but a lively debate ex...

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Bibliographic Details
Main Authors: A. K. Srivastava, Sripan Mondal, Eric R. Priest, Sudheer K. Mishra, David I. Pontin, R.Y. Kwon, Ding Yuan, K. Murawski, Ayumi Asai
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar corona
Active solar corona
Solar magnetic reconnection
Solar coronal waves
Magnetohydrodynamics
Online Access:https://doi.org/10.3847/1538-4357/adc379
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https://doi.org/10.3847/1538-4357/adc379

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