Simulating Compressive Stream Interaction Regions during Parker Solar Probe’s First Perihelion Using Stream-aligned Magnetohydrodynamics

Simulating Compressive Stream Interaction Regions during Parker Solar Probe’s First Perihelion Using Stream-aligned Magnetohydrodynamics

We used the stream-aligned magnetohydrodynamics (SA-MHD) model to simulate Carrington rotation 2210, which contains Parker Solar Probe’s (PSP) first perihelion at 36.5 R _⊙ on 2018 November 6, to provide context to the in situ PSP observations by FIELDS and SWEAP. The SA-MHD model aligns the magneti...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: E. M. Wraback, A. P. Hoffmann, W. B. Manchester IV, I. V. Sokolov, B. van der Holst, D. Carpenter
Aineistotyyppi: Artikkeli
Kieli:English
Julkaistu: IOP Publishing 2024-01-01
Sarja:The Astrophysical Journal
Aiheet:
Solar corona
Hydrodynamical simulations
Solar wind
Linkit:https://doi.org/10.3847/1538-4357/ad21fd

Internet

https://doi.org/10.3847/1538-4357/ad21fd

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