Modeling the Early Evolution of a Slow Coronal Mass Ejection Imaged by the Parker Solar Probe

Modeling the Early Evolution of a Slow Coronal Mass Ejection Imaged by the Parker Solar Probe

During its first solar encounter, the Parker Solar Probe (PSP) acquired unprecedented up-close imaging of a small coronal mass ejection (CME) propagating in the forming slow solar wind. The CME originated as a cavity imaged in extreme ultraviolet that moved very slowly (

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Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal. Supplement series 2020-02, Vol.246 (2), p.72
Hauptverfasser: Rouillard, Alexis P., Poirier, Nicolas, Lavarra, Michael, Bourdelle, Anthony, Dalmasse, Kévin, Kouloumvakos, Athanasios, Vourlidas, Angelos, Kunkel, Valbona, Hess, Phillip, Howard, Russ A., Stenborg, Guillermo, Raouafi, Nour E.
Format: Artikel
Sprache:eng
Schlagworte:
Acceleration
Computer Science
Computer simulation
Corona
Coronal mass ejection
Engineering Sciences
Evolution
Image acquisition
Magnetic fields
Magnetic reconnection
Mathematics
Morphology
Physics
Poloidal flux
Slow solar wind
Solar coronal streamers
Solar coronal transients
Solar probes
Solar wind
Two dimensional models
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Beschreibung
Zusammenfassung:During its first solar encounter, the Parker Solar Probe (PSP) acquired unprecedented up-close imaging of a small coronal mass ejection (CME) propagating in the forming slow solar wind. The CME originated as a cavity imaged in extreme ultraviolet that moved very slowly (
ISSN:0067-0049
1538-4365
DOI:10.3847/1538-4365/ab6610