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Magnetic reconnection is a fundamental physical process in many laboratory,space, and astrophysical plasma contexts. Solar flares serve as an outstandinglaboratory to study the magnetic reconnection and the associated energy releaseand conversion processes under plasma conditions difficult to reproduce in thelaboratory, and with considerable spatiotemporal details not possible elsewherein astrophysics. Here we emphasize the unique power of remote-sensingobservations of solar flares at radio wavelengths. In particular, we discussthe transformative technique of broadband radio dynamic imaging spectroscopy inmaking significant contributions to addressing several outstanding challengesin magnetic reconnection, including the capability of pinpointing magneticreconnection sites, measuring the time-evolving reconnecting magnetic fields,and deriving the spatially and temporally resolved distribution function offlare-accelerated electrons.

Astro2020 Science White Paper: Probing Magnetic Reconnection in Solar Flares - New Perspectives from Radio Dynamic Imaging Spectroscopy