During relativistic magnetic reconnection, antiparallel magnetic fields undergo a rapid change in topology, releasing a large amount of energy in the form of non-thermal particle acceleration. This work explores the application of mesh refinement to 2D reconnection simulations to efficiently model the ineherent disparity in length-scales. We have systematically investigated the effects of mesh refinement and determined necessary modifications to the algorithm required to mitigate non-physical artifacts at the coarse-fine interface. We have used the ultrahigh-order Pseudo-Spectral Analytical Time-Domain (PSATD) Maxwell solver to analyze how its use can mitigate the numerical dispersion that occurs with the finite-difference time-domain (FDTD) (or ``Yee'') method. Absorbing layers are introduced at the coarse-fine interface to eliminate spurious effects that occur with mesh refinement. We also study how damping the electromagnetic fields and current density in the absorbing layer can help prevent the non-physical accumulation of charge and current density at the coarse-fine interface. Using a mesh refinement ratio of 8 for two-dimensional magnetic reconnection simulations, we obtained good agreement with the high resolution baseline simulation, using only 36% of the macroparticles and 71% of the node-hours needed for the baseline. The methods presented here are especially applicable to 3D systems where higher memory savings are expected than in 2D, enabling comprehensive, computationally efficient 3D reconnection studies in the future.
foap4: Adaptive mesh refinement with OpenACC/OpenMP, MPI, and p4est
Centrum Wiskunde & Informatica (CWI)(荷兰数学与计算机科学中心);Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven(荷语鲁汶大学数学系数学等离子体天体物理中心);Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications (CIDMA)(阿威罗大学数学系及数学与应用研发中心);Netherlands eScience Center(荷兰电子科学中心);School of Astronomy and Space Science and Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University(南京大学天文与空间科学学院现代天体物理学重点实验室)
Field conserving adaptive mesh refinement (AMR) scheme on massively parallel adaptive octree meshes
Iowa State University(爱荷华州立大学);Stanford University(斯坦福大学);University of Utah(犹他大学);Tufts University(塔夫茨大学);RIKEN Center for Computational Science(理化学研究所计算科学中心)
A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies