How Turbulent is the Magnetically Closed Corona?

We argue that the magnetically closed corona evolves primarily quasi-statically, punctuated by many localized bursts of activity associated with magnetic reconnection at a myriad of small current sheets. The sheets form by various processes that do not involve a traditional turbulent cascade whereby...

Full description

Bibliographic Details
Main Authors: James A. Klimchuk, Spiro K. Antiochos
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-05-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2021.662861/full