Magnetorotational transport and magnetic-flux dependence
Research context
research method · conditional · As of 2026-10-10
Weak well-coupled magnetic fields can destabilize outwardly decreasing differential rotation and drive angular-momentum transport.
Key knowledge
Weak well-coupled magnetic fields can destabilize outwardly decreasing differential rotation and drive angular-momentum transport. Reynolds and Maxwell stresses diagnose transport in a specified simulation; an effective alpha varies with flux, stratification, boundaries and dissipation.
Values and equations
T_rφ=ρ δv_r δv_φ-B_r B_φ/μ0; α=average(T_rφ)/average(P)
- T_rφ
- Radial azimuthal momentum flux Pa
- ρ
- Mass density kg m^-3
- δv_r,δv_φ
- Fluctuating velocities m s^-1
- B_r,B_φ
- Field components T
- μ0
- Magnetic permeability H m^-1
- P
- Declared pressure normalization Pa
- α
- Effective transport parameter 1
Conditions and scope
- The cited global model omits vertical stratification; its reported stress cannot be a universal disk or jet efficiency.
- Nonideal conductivity and kinetic-scale physics can alter instability and saturation.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Turbulence and angular momentum transport in a global accretion disk simulation: Sections 1–3: conducting-disk instability, stress diagnostics and unstratified-model limitations (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
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- research-earth-mri-stress
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference