This paper investigates the performance of a parallel Newton, first-order system least-squares (FOSLS) finite-element method with local adaptive refinement and algebraic multigrid (AMG) applied to incompressible, resistive magnetohydrodynamics. In particular, an island coalescence test problem is studied that models magnetic reconnection using a reduced two-dimensional (2D) model of a tokamak fusion reactor. The results show that, using an appropriate temporal and spatial resolution, these methods are capable of resolving the physical instabilities accurately at small computational cost. The time-dependent, nonlinear system of PDEs is solved using work equivalent to about 50-60 simple relaxation sweeps (Gauss-Seidel iterations) per time step. Experiments show that, unless the time step is sufficiently small, nonphysical numerical instabilities may occur. Further, decreasing the time step size does not proportionally increase the cost of the computation, because AMG convergence is improved. In addition, an effective implementation of the methods in parallel keeps load balancing issues to a minimum. Various quantities, such as the reconnection rate and the "sloshing" effect of the plasma instability, are measured to confirm that the correct physics is reproduced.
Introduction.The island coalescence problem for studying fast magnetic reconnection in a plasma has been studied extensively (e.g., in [9,11,34,41,42,45,52]). Many numerical algorithms have been implemented to simulate this problem using various types of physical and mathematical models [1,15,22,24,25,35,37,38,41,43,44,46,47,49,50]. The aim of this paper is to extend the results of [2, 3, 4] and show that by using the first-order system least-squares (FOSLS) finite-element method along with nested iteration (NI), algebraic multigrid (AMG), and an efficiency-based adaptive local refinement scheme (ACE) in parallel, the relevant physics of the reconnection is modeled with a low amount of computational cost. Preliminary results are obtained in [2,3,4] using an incompressible resistive magnetohydrodynamics (MHD) model with the above methods. However, limitations with the computational resources used exposed several deficiencies in the method. Namely, at high Lundquist numbers (low resistivity), time integration was not resolving the magnetic instabilities, resulting in numerical oscillations in the current density peak. These, in turn, affected the performance of the solvers and the convergence of the discrete methods. With an efficient implementation of the method on computers with a distributed