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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書誌詳細

主要な著者:	Elizabeth A. Jensen, W. B. Manchester IV, J. E. Kooi, T. Nieves-Chinchilla, L. K. Jian, D. B. Wexler, S. F. Fung, N. Gopalswamy
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2025-01-01
シリーズ:	The Astrophysical Journal
主題:	Radio astronomy Solar corona Solar coronal mass ejections Solar physics Solar wind Heliosphere
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/add1c3
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