Speaker
Description
A Coronal Mass Ejection (CME) is a large-scale eruption of plasma and magnetic fields from the Sun into interplanetary space. In coronagraph observations, around one-third of CMEs exhibit a characteristic three-part structure consisting of a bright inner core, an outer leading edge, and a darker cavity in the middle. However, observations of the inner corona suggest this three-part structure is more common than previously thought. The traditional view that prominence material forms the bright inner core and that the cavity represents a low-density magnetic flux rope has recently been questioned. Some studies propose that the bright core may instead result from the geometric projection of a twisted flux rope. In contrast, more recent observations from the Solar Orbiter in the He II 304 Å passband of the EUI/Full Sun Imager have detected prominence material as far as six solar radii. To reassess the association between prominence material and the bright inner core of CMEs, we analyzed data from GONG H
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Theme | Energetic Phenomena |