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astro-ph.SR2024
Modeling Time-Variable Elemental Abundances in Coronal Loop Simulations
Jeffrey W. Reep, John Unverferth, Will T. Barnes +1
Numerous recent X-ray observations of coronal loops in both active regions (ARs) and solar flares have shown clearly that elemental abundances vary with time. Over the course of a…
astro-ph.SR2024
Determining the nanoflare heating frequency of an X-ray Bright Point observed by MaGIXS
Biswajit Mondal, P. S. Athiray, Amy R. Winebarger +18
Nanoflares are thought to be one of the prime candidates that can heat the solar corona to its multi-million kelvin temperature. Individual nanoflares are difficult to detect with…