Solar and Magnetospheric MHD Theory Group

Welcome to the WWW pages of the Solar and Magnetospheric MHD Theory Group. We are one of the Applied Mathematics research groups in the School of Mathematics and Statistics at the University of St Andrews in Scotland.

We are a large group of applied mathematicians, who study the Sun using mathematical modelling techniques and observational data from satellites such as SoHO, Yohkoh and TRACE, or ground based observatories such as Kitt Peak and Big Bear. We also have close collaborations with the Solar Group at Glasgow University and will be actively involved with the new space missions that are soon to be launched, namely, Stereo, SolarB and Solar Dynamics Observatory (on which we are a Co-Investigators).

The Group is currently investigating several fundamental MHD and plasma processes such as magnetic reconnection, magnetic equilibria, MHD waves, MHD instabilities and particle acceleration. By using these processes we model a wide range of solar phenomena, including coronal heating, solar flares, prominences, the Sun's global magnetic field, coronal loop structure and topology, coronal oscillations, coronal seismology, emerging flux, the magnetic carpet and flux cancellation.

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