The SAC and SMAUG codes are based on the Versatile Advection Code we heard from one of the authors of the code about MPI-AMRVAC. This code is an advance on VAC, the parallel scaling of the code exhibits weak scaling up to 30000 processors allowing to exploit modern peta-scale infrastructure. In particular the code has been developed to allow adaptive refinements of the computational mesh.
The discussion focussed on solar physical applications modeled by the magnetohydrodynamic module of MPI-AMRVAC. The spatial discretizations available cover standard shock capturing finite volume algorithms, there are extensions to conservative high order finite difference schemes, employing many flavors of limited reconstruction strategies. Multi-step explicit time stepping includes strong stability preserving high order Runge-Kutta steppers to obtain stable evolutions in multidimensional applications realizing up to fourth order accuracy in space and time.
Solar physics applications target the formation of flux rope topologies through
boundary driven shearing of magnetic arcades, following the in situ
condensation of prominences in radiatively controlled evolutions of arcades and
flux ropes, and the enigmatic phenomenon of coronal rain, where small-scale
condensations repeatedly form and rain down in thermodynamically structured
References`MPI-AMRVAC for solar and astrophysics', O. Porth, C. Xia, T. Hendrix, S.P. Moschou, & R. Keppens, 2014, ApJS 214, 4 (26pp) Full paper, doi:10.1088/0067-0049/214/1/4 )
`Parallel, grid-adaptive approaches for relativistic hydro and magnetohydrodynamics', R. Keppens, Z. Meliani, A.J. van Marle, P. Delmont, A. Vlasis, & B. van der Holst, 2012, JCP 231, 718-744. Full paper, doi:10.1016/j.jcp.2011.01.020. Accepted for special topical issue, with R. Keppens as Associate Editor. See also the Editorial Preface: Computational Plasma Physics.
`Three-dimensional prominence-hosting magnetic configurations: creating a helical magnetic flux rope', C. Xia, R. Keppens, & Y. Guo, 2014, ApJ 780, 130 (11pp) Full paper, doi:10.1088/0004-637X/780/2/130
`Simulating the in situ condensation process of solar prominences', C. Xia, R. Keppens, P. Antolin, & O. Porth, 2014, ApJ Letters 792, L38 (6pp) Full paper, doi:10.1088/2041-8205/792/2/L38