High-frequency Coronal Alfvénic Waves Observed with DKIST/Cryo-NIRSP

The presence and nature of low-frequency (0.1–10 mHz) Alfvénic waves in the corona have been established over the past decade, with many of these results coming from coronagraphic observations of the infrared Fe xiii line. The Cryo-NIRSP instrument situated at DKIST has recently begun acquiring scie...

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Bibliographic Details
Main Authors: Richard J. Morton, Momchil Molnar, Steven R. Cranmer, Thomas A. Schad
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/adb8df
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