Available student project - Modelling a solar fare by MRXMHD

Research fields

  • Astrophysics
  • Fusion and Plasma Confinement

Project details

The structure and dynamics of the solar corona is dominated by the magnetic field. In most areas in the corona magnetic forces are so dominant that all non-magnetic forces like plasma pressure gradient and gravity can be neglected in the lowest order. This model assumption is called the force-free field assumption, as the Lorentz force vanishes.

A common assumption in modelling coronal solar flares is to assume the field is force-free, and adjust the field pitch to match local measurements of the photosphere field footprint. Such fields are called nonlinear force free fields.

In this project, we apply multiple-region relaxed MHD model, designed to describe the fractal fix of chaotic field lines, magentic islands, and flux surfaces in toroidal magnetic confinement, to describe a solar flare.

Required background

Electrodynamics. A knowledge of plasma physics is desirable, but not essential,

Project suitability

This research project can be tailored to suit students of the following type(s)
  • 3rd year special project
  • PhB (2nd or 3rd year)
  • Vacation scholar

Contact supervisor

Hole, Matthew profile
Senior Fellow
57606

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