# Magnetic field gradient effects on the magnetorotational instability

## TL;DR

This paper explores how azimuthal magnetic field gradients influence the magnetorotational instability, revealing new unstable regions and altered growth rates, which could impact understanding of turbulence in accretion discs.

## Contribution

It introduces the effect of azimuthal magnetic field gradients into MRI analysis, showing their impact on instability growth rates and unstable wavenumber ranges.

## Key findings

- Azimuthal magnetic field gradient creates new unstable regions.
- Higher gradients increase growth rates and unstable wavenumber range.
- Implications for MRI in T Tauri discs with misaligned stellar magnetic fields.

## Abstract

The magnetorotational instability (MRI), also known as the Balbus -- Hawley instability, is thought to have an important role on the initiation of turbulence and angular momentum transport in accretion discs. In this work, we investigate the effect of the magnetic field gradient in the azimuthal direction on MRI. We solve the magnetohydrodynamic equations by including the azimuthal component of the field gradient. We find the dispersion relation and calculate the growth rates of the instability numerically. The inclusion of the azimuthal magnetic field gradient produces a new unstable region on wavenumber space. It also modifies the growth rate and the wavelength range of the unstable mode: the higher the magnitude of the field gradient, the greater the growth rate and the wider the unstable wavenumber range. Such a gradient in the magnetic field may be important in T Tauri discs where the stellar magnetic field has an axis which is misaligned with respect to the rotation axis of the disc.