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Radial Variations in Solar Type III Radio Bursts

Type III radio bursts are generated by electron beams accelerated at reconnection sites in the corona. This study, utilizing data from the Parker Solar Probe’s first 17 encounters, closely examines these bursts down to 13 solar radii. A focal point of our analysis is the near-radial alignment (withi...

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Wedi'i Gadw mewn:
Prif Awduron: Vratislav Krupar, Oksana Kruparova, Adam Szabo, Lynn B. Wilson III, Frantisek Nemec, Ondrej Santolik, Marc Pulupa, Karine Issautier, Stuart D. Bale, Milan Maksimovic
Fformat: Artigo
Iaith:Inglês
Cyhoeddwyd: IOP Publishing 2024-01-01
Cyfres:The Astrophysical Journal Letters
Pynciau:
Radio astronomy
Radio bursts
Mynediad Ar-lein:https://doi.org/10.3847/2041-8213/ad4be7
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