Flux ropes in SANE disks
Fuente:
arXiv
Guardado en:
| Autores principales: | , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2020
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866911858343018496 |
|---|---|
| author | Čemeljić, Miljenko Yuan, Feng Yang, Hai |
| author_facet | Čemeljić, Miljenko Yuan, Feng Yang, Hai |
| contents | Three-dimensional numerical simulations of a hot accretion flow around a supermassive black hole are performed using the general relativity magneto-hydrodynamic (GRMHD) code Athena++. We focus on the case of SANE, with the initial magnetic field consisting of multiple loops with oppositely directed poloidal magnetic field in the torus. Using the simulation data, we investigate the formation of flux ropes, follow the forming of flux ropes atop the disk, and their release into corona. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2012_00916 |
| institution | arXiv |
| publishDate | 2020 |
| record_format | arxiv |
| spellingShingle | Flux ropes in SANE disks Čemeljić, Miljenko Yuan, Feng Yang, Hai High Energy Astrophysical Phenomena Three-dimensional numerical simulations of a hot accretion flow around a supermassive black hole are performed using the general relativity magneto-hydrodynamic (GRMHD) code Athena++. We focus on the case of SANE, with the initial magnetic field consisting of multiple loops with oppositely directed poloidal magnetic field in the torus. Using the simulation data, we investigate the formation of flux ropes, follow the forming of flux ropes atop the disk, and their release into corona. |
| title | Flux ropes in SANE disks |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2012.00916 |