AAS 199th meeting, Washington, DC, January 2002
Session 118. Galaxies II
Oral, Wednesday, January 9, 2002, 2:00-3:30pm, Jefferson East

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[118.03] Gradient Particle Magnetohydrodynamics, the next generation SPH algorithm.

J. L. Maron, G. G. Howes (Imperial College, London)

We introduce Gradient Particle Magnetohydrodynamics (GPM), a new Lagrangian method for magnetohydrodynamics based on gradients corrected for the locally disordered particle distribution. The development of a numerical code for MHD simulation using the GPM algorithm is outlined. Validation tests simulating linear and nonlinear sound waves, linear MHD waves, advection of magnetic fields in a magnetized vortex, hydrodynamical shocks, and three-dimensional collapse are presented, demonstrating the viability of an MHD code using GPM. The characteristics of a GPM code are discussed and possible avenues for further development and refinement are mentioned. We conclude with a view of how GPM may complement other methods currently in development for the next generation of computational astrophysics.


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