Reversals of Toroidal Magnetic Field in Local Shearing Box Simulations of Accretion Disk with a Hot Corona
The presence of a hot corona above the accretion disk can have important consequences for the evolution of magnetic fields and the Shakura–Sunyaev viscosity parameter α in such a strongly coupled system. In this work, we have performed three-dimensional magnetohydrodynamical shearing-box numerical s...
Saved in:
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adbf02 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|