Constraining the Physical Properties of Stellar Coronal Mass Ejections with Coronal Dimming: Application to Far-ultraviolet Data of ϵ Eridani

Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather and might have impacted the Sun’s early angular momentum evolution. A signal diagnostic of CMEs on the Sun is coronal dimming: a drop in coronal emission, tied to the mass of the CME, that is the direct result of...

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Veröffentlicht in:	The Astrophysical journal 2022-09, Vol.936 (2), p.170
Hauptverfasser:	Loyd, R. O. Parke, Mason, James Paul, Jin, Meng, Shkolnik, Evgenya L., France, Kevin, Youngblood, Allison, Villadsen, Jackie, Schneider, Christian, Schneider, Adam C., Llama, Joe, Ramiaramanantsoa, Tahina, Richey-Yowell, Tyler
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Astrophysics Corona Coronal mass ejection Dimming Emission Hubble Space Telescope Physical properties Plasma Solar coronal mass ejections Solar system Space telescopes Space weather Stellar coronal mass ejections Stellar coronas Stellar flares Stellar mass loss Ultraviolet astronomy Weather
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