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:	arXiv.org 2020-02
Hauptverfasser:	Rouillard, Alexis P, Poirier, Nicolas, Lavarra, Michael, Bourdelle, Antony, 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 simulation Coronal mass ejection Evolution Image acquisition Magnetic fields Morphology Physics - Solar and Stellar Astrophysics Physics - Space Physics Poloidal flux Solar probes Solar wind Two dimensional models
Online-Zugang:	Volltext
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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:	2331-8422
DOI:	10.48550/arxiv.2002.08756