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About Enhanced MHD Transport in Astrophysical Accretion Flows:: Turbulence, Winds and Jets
This document discusses MHD (magnetohydrodynamic) accretion theory and simulations. It summarizes that while MHD turbulence enhances angular momentum transport compared to viscosity alone, it is still inefficient. A generalized MHD accretion model is proposed where large-scale MHD torques primarily drive vertical angular momentum transport and accretion, while radial transport is secondary. Resistive and radiative MHD simulations are needed to better understand magnetic field evolution and compare modeled accretion disk spectra to observations.
Detailed Information
| Author: | ['Pogz1995'] |
|---|---|
| Publication Year: | 2012 |
| Pages: | 17 |
| Language: | English |
| Format: | |
| Price: | FREE |
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