The Impact of Alfvénic Shear Flow on Magnetic Reconnection and Turbulence

Magnetic reconnection is a fundamental and omnipresent energy conversion process in plasma physics. Novel observations of fields and particles from Parker Solar Probe (PSP) have shown the absence of reconnection in a large number of current sheets in the near-Sun solar wind. Using near-Sun observati...

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Hlavní autoři:	Tamar Ervin, Alfred Mallet, Stefan Eriksson, M. Swisdak, James Juno, Orlando M. Romeo, Tai Phan, Trevor A. Bowen, Roberto Livi, Phyllis L. Whittlesey, Davin E. Larson, Stuart D. Bale
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2025-01-01
Edice:	The Astrophysical Journal Letters
Témata:	Solar magnetic reconnection Solar wind Slow solar wind
On-line přístup:	https://doi.org/10.3847/2041-8213/ae0b56
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