Thermodynamic Evolution of Flaring Loops with Nonlocal Thermal Transport

Hot solar coronal loops, such as flaring loops, reach temperatures where the thermal transport becomes nonlocal. This occurs when the mean-free-path of electrons can no longer be assumed to be small. Using a modified version of the Lare2d code, we study the evolution of flare-heated coronal loops un...

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Bibliographic Details
Main Authors: S. Belov, T. Parmenter, T. Arber, D. Kolotkov, F. Reale, T. Goffrey
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/ade542
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