Inferring Fundamental Properties of the Flare Current Sheet Using Flare Ribbons: Oscillations in the Reconnection Flux Rates

Inferring Fundamental Properties of the Flare Current Sheet Using Flare Ribbons: Oscillations in the Reconnection Flux Rates

Magnetic reconnection is understood to be the main physical process that facilitates the transformation of magnetic energy into heat, motion, and particle acceleration during solar eruptions. Yet, observational constraints on reconnection region properties and dynamics are limited due to a lack of h...

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Bibliographic Details
Main Authors: Marcel F. Corchado Albelo, Maria D. Kazachenko, Benjamin J. Lynch
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar flares
Solar x-ray flares
Solar magnetic reconnection
Solar magnetic fields
Solar physics
Solar active region magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/ad25f4

Internet

https://doi.org/10.3847/1538-4357/ad25f4

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