A New Method Linking the Solar Wind Speed to the Coronal Magnetic Field

The release and acceleration of the solar wind is still an outstanding question. There are several aspects related to this phenomenon that still need to be investigated, and one of these is the identification of the region within the inner corona where the larger fraction of acceleration occurs. To...

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Veröffentlicht in:	The Astrophysical journal Jg. 949; H. 2; S. 42 - 53
Hauptverfasser:	Casti, Marta, Arge, Charles N., Bemporad, Alessandro, Pinto, Rui F., Henney, Carl J.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 01.06.2023 IOP Publishing American Astronomical Society
Schlagworte:	Acceleration Astrophysics Charged particles Corona Coronal magnetic fields Dimming Magnetic field configurations Magnetic fields Photosphere Photospheric magnetic fields Physics Solar and Stellar Astrophysics Solar corona Solar magnetic field Solar magnetic fields Solar wind Solar wind speed Solar wind velocity Velocity Velocity distribution Wind speed Wind velocities
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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