Riemann solvers and Alfven waves in black hole magnetospheres

In the magnetosphere of a rotating black hole, an inner Alfven critical surface (IACS) must be crossed by inflowing plasma. Inside the IACS, Alfven waves are inward directed toward the black hole. The majority of the proper volume of the active region of spacetime (the ergosphere) is inside of the I...

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Detalles Bibliográficos
Autores principales: Punsly, Brian, Balsara, Dinshaw, Kim, Jinho, Garain, Sudip
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2016
Materias:
Research
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6511996/
https://www.ncbi.nlm.nih.gov/pubmed/31149560
http://dx.doi.org/10.1186/s40668-016-0018-1

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6511996/
https://www.ncbi.nlm.nih.gov/pubmed/31149560
http://dx.doi.org/10.1186/s40668-016-0018-1

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