Numerical MHD models of stream interaction regions (SIRs) and corotating interaction regions (CIRs) using sunRunner3D: comparison with observations.
In: Monthly Notices of the Royal Astronomical Society, Jg. 529 (2024-04-01), Heft 2, S. 1250-1257
Online
academicJournal
Zugriff:
Titel: |
Numerical MHD models of stream interaction regions (SIRs) and corotating interaction regions (CIRs) using sunRunner3D: comparison with observations.
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Autor/in / Beteiligte Person: | Aguilar-Rodriguez, E ; González-Avilés, J J ; Riley, P ; Ben-Nun, M ; Rodriguez-Martinez, M ; González, R F ; Perez-Rivera, M A ; Raga-Rasmussen, A C |
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Zeitschrift: | Monthly Notices of the Royal Astronomical Society, Jg. 529 (2024-04-01), Heft 2, S. 1250-1257 |
Veröffentlichung: | 2024 |
Medientyp: | academicJournal |
ISSN: | 0035-8711 (print) |
DOI: | 10.1093/mnras/stae640 |
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