Name: Martin Haynes
Magnetic reconnection as a fundamental plasma process and its effects in the solar corona.
3D MHD simulations of confined flares and their observational signatures.
Emergence of flux tubes from the convection zone to the corona including a partially ionized layer.
"Block Adaptive Mesh refinement for a Lagrangian Remap Code"
I converted an already existing Lagrangian remap MHD code to contain block adaptive mesh refinement. This is a technique which allows the fluid simulation to place more points in regions of interest thus better allocating the available resources.
 Arber, T.D. & Haynes, M., "A generalized Petschek magnetic reconnection rate", Phys. Plas., 13, 112105, 2006
 Haynes, M. & Arber, T.D., "Observational properties of a kink unstable loop", A&A, 467,327-333, 2007
 Arber, T.D., Haynes, M. & Leake, J.E., "Emergence of a flux tube through a partially ionized solar atmosphere", ApJ, 666, 541-546, 2007
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+44 (0) 24 765 23672