Probing Coronal Mass Ejection Inclination Effects with EUHFORIA

Coronal mass ejections (CMEs) are complex magnetized plasma structures in which the magnetic field spirals around a central axis, forming what is known as a flux rope (FR). The central FR axis can be oriented at any angle with respect to the ecliptic. Throughout its journey, a CME will encounter int...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	The Astrophysical journal 2024-10, Vol.974 (2), p.203
Hauptverfasser:	Martinić, Karmen, Asvestari, Eleanna, Dumbović, Mateja, Rindlisbacher, Tobias, Temmer, Manuela, Vršnak, Bojan
Format:	Artikel
Sprache:	eng
Schlagworte:	Coronal mass ejection Drag Ecliptic Heliosphere Inclination Interplanetary magnetic field Magnetic fields Magnetic flux Magnetic properties Magnetohydrodynamical simulations Orientation effects Parameters Sheaths Solar coronal mass ejections Solar magnetic field Solar physics Solar wind Spacecraft
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!