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Modeling Polarized Radio Sounding Observations of a Coronal Mass Ejection

Coronal mass ejections (CMEs) evolve significantly as they propagate from the Sun to the Earth, so remote observations of their changes in speed, strength of the magnetic field, density, and overall structure are critical for predicting their arrival time and geoeffectiveness. Radio line-of-sight ob...

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Principais autores: Elizabeth A. Jensen, W. B. Manchester IV, J. E. Kooi, T. Nieves-Chinchilla, L. K. Jian, D. B. Wexler, S. F. Fung, N. Gopalswamy
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/add1c3
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