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Sun-as-a-star Spectroscopic Observations of the Line-of-sight Velocity of a Solar Eruption on 2021 October 28

The propagation direction and true velocity of a solar coronal mass ejection, which are among the most decisive factors for its geo-effectiveness, are difficult to determine through single-perspective imaging observations. Here we show that Sun-as-a-star spectroscopic observations, together with ima...

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Bibliografski detalji
Glavni autori: Yu Xu, Hui Tian, Zhenyong Hou, Zihao Yang, Yuhang Gao, Xianyong Bai
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2022-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/ac69d5
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