Operational Modeling of Heliospheric Space Weather for the Parker Solar Probe

The interpretation of multi-spacecraft heliospheric observations and three-dimensional reconstruction of the structured and evolving solar wind with propagating and interacting coronal mass ejections (CMEs) is a challenging task. Numerical simulations can provide global context and suggest what may...

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Veröffentlicht in:	The Astrophysical journal. Supplement series 2020-02, Vol.246 (2), p.73
Hauptverfasser:	Odstrcil, Dusan, Mays, M. Leila, Hess, Phillip, Jones, Shaela I., Henney, Carl J., Arge, Charles N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Charged particles Computer simulation Coronal mass ejection Ejecta In situ measurement Magnetohydrodynamical simulations Missions Numerical simulations Perihelions Solar corona Solar coronal mass ejections Solar probes Solar wind Space weather Spacecraft Weather White light
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