Ion-rich Acceleration during an Eruptive Flux Rope Event in a Multiple Null-point Configuration

Ion-rich Acceleration during an Eruptive Flux Rope Event in a Multiple Null-point Configuration

We report on the γ -ray emission above 100 MeV from the GOES M3.3 flare SOL2012-06-03. The hard X-ray (HXR) and microwave emissions have typical time profiles with a fast rise to a well-defined peak followed by a slower decay. The >100 MeV emission during the prompt phase displayed a double-peake...

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Bibliographic Details
Main Authors: Melissa Pesce-Rollins, Alexander MacKinnon, Karl-Ludwig Klein, Alexander J. B. Russell, Hugh Hudson, Alexander Warmuth, Thomas Wiegelmann, Sophie Masson, Clare Parnell, Nariaki V. Nitta, Nicola Omodei
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar flares
Gamma-rays
Solar coronal waves
Online Access:https://doi.org/10.3847/1538-4357/adeb7f
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https://doi.org/10.3847/1538-4357/adeb7f

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