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 Regulators dynamics are limited due to a lack of high-cadence and high-spatial-resolution