Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST

Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST

We present the highest-resolution H α observations of a solar flare to date, collected during the decay phase of an X1.3-class flare on 2024 August 8 at 20:12 UT. Observations with the Visible Broadband Imager at the National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) reveal dark...

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Bibliographic Details
Main Authors: Cole A. Tamburri, Maria D. Kazachenko, Gianna Cauzzi, Adam F. Kowalski, Ryan French, Rahul Yadav, Caroline L. Evans, Yuta Notsu, Marcel F. Corchado-Albelo, Kevin P. Reardon, Alexandra Tritschler
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar flares
Solar corona
Solar coronal loops
Solar active regions
Solar X-ray flares
Online Access:https://doi.org/10.3847/2041-8213/adf95e
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https://doi.org/10.3847/2041-8213/adf95e

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