Turbulence in a Coronal Loop Excited by Photospheric Motions

Turbulence in a Coronal Loop Excited by Photospheric Motions

Photospheric motions are believed to be the source of coronal heating and of velocity fluctuations detected in the solar corona. A numerical model, based on the shell technique applied on reduced magnetohydrodynamics equations, is used to represent energy injection due to footpoint motions, storage...

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Bibliographic Details
Main Authors: Giuseppina Nigro, Francesco Malara, Antonio Vecchio, Leonardo Primavera, Francesca Di Mare, Vincenzo Carbone, Pierluigi Veltri
Format: Article
Language:English
Published: MDPI AG 2020-04-01
Series:Atmosphere
Subjects:
solar corona
turbulence
numerical modeling
Online Access:https://www.mdpi.com/2073-4433/11/4/409

Internet

https://www.mdpi.com/2073-4433/11/4/409

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