Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions

We develop a general description of how information propagates through a magnetohydrodynamic (MHD) system based on the method of characteristics and use that to formulate numerical boundary conditions that are intrinsically consistent with the MHD equations. Our formulation includes two major advanc...

Descrizione completa

Dettagli Bibliografici

Autori principali:	Lucas A. Tarr, N. Dylan Kee, Mark G. Linton, Peter W. Schuck, James E. Leake
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2024-01-01
Serie:	The Astrophysical Journal Supplement Series
Soggetti:	Solar physics Solar magnetic fields Magnetohydrodynamical simulations Solar photosphere Solar corona Solar chromosphere
Accesso online:	https://doi.org/10.3847/1538-4365/ad0e0c
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!