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JamesEdgeley authored Apr 25, 2024
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* [Execution](#execution)
* [Parameters](#parameters)
* [Examples](#examples)
*[Unsteady Ring](#unsteady-ring)
* [Unsteady Ring](#unsteady-ring)
* [MAST-U](#mast-u)
* [References](#references)
* [License](#license)

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Shown below is the system at a later stage
![System at an evolved state](/readme/evolved.png)

### MAST-U
The second example is a poloidal section through the MAST-U device, using the magnetic field given in the file `B.pts`. The heat diffusion is again isotropic, favouring the magnetic field direction.

For the boundary conditions, the core region is held at a high temperature `TCore`, and the outer region at a low temperature (300 and 0 respectively for these images). Currently the domain does not have axial symmetry, so does not completely represent the true scenario.

Shown below is the system at an early stage
![System at an early state](/readme/mast-early.png)

Shown below is the system at a later stage
![System at an evolved state](/readme/mast-evolved.png)

## References

<a name="cantwell-et-al-2015"></a>\[1\] Cantwell et al, *Nektar++: An open-source spectral/hp element framework.*, JCP, 2015 [[DOI](https://doi.org/10.1016/j.cpc.2015.02.008)]
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