# INITIAL MODEL maestro.model_file = "kepler_new_6.25e8.hybrid.hse.320" maestro.perturb_model = true maestro.drdxfac = 5 #maestro.ppm_type = 1 # PROBLEM SIZE geometry.prob_lo = 0.0 0.0 0.0 geometry.prob_hi = 5.e8 5.e8 5.e8 # BOUNDARY CONDITIONS # 0 = Interior 3 = Symmetry # 1 = Inflow 4 = Slipwall # 2 = Outflow 5 = NoSlipWall maestro.lo_bc = 2 2 2 maestro.hi_bc = 2 2 2 geometry.is_periodic = 0 0 0 # VERBOSITY maestro.maestro_verbose = 1 # verbosity # DEBUG FOR NAN amrex.fpe_trap_invalid = 1 # floating point exception # GRIDDING AND REFINEMENT amr.n_cell = 64 64 64 amr.max_grid_size = 32 amr.max_level = 1 # maximum level number allowed maestro.regrid_int = 2 # how often to regrid amr.ref_ratio = 2 2 2 2 2 2 # refinement ratio amr.blocking_factor = 8 # block factor in grid generation amr.refine_grid_layout = 0 # chop grids up into smaller grids if nprocs > ngrids # TIME STEPPING maestro.max_step = 3 maestro.stop_time = 30000. maestro.cfl = 0.7 # cfl number for hyperbolic system # In this test problem, the velocity is # time-dependent. We could use 0.9 in # the 3D test, but need to use 0.7 in 2D # to satisfy CFL condition. # ALGORITHMIC OPTIONS maestro.spherical = 1 maestro.evolve_base_state = true maestro.do_initial_projection = true maestro.init_divu_iter = 3 maestro.init_iter = 1 maestro.grav_const = -1.5e10 maestro.anelastic_cutoff_density = 1.e6 maestro.base_cutoff_density = 1.e5 maestro.do_sponge = 1 maestro.sponge_center_density = 3.e6 maestro.sponge_start_factor = 3.333e0 maestro.sponge_kappa = 10.e0 maestro.init_shrink = 0.1e0 maestro.use_soundspeed_firstdt = true maestro.use_divu_firstdt = true maestro.use_tfromp = true maestro.use_delta_gamma1_term = false # PLOTFILES maestro.plot_base_name = wdconvect_plt # root name of plot file maestro.plot_int = 1 # number of timesteps between plot files maestro.plot_deltat = 10.0e0 # CHECKPOINT maestro.check_base_name = wdconvect_chk maestro.chk_int = -1 # tolerances for the initial projection maestro.eps_init_proj_cart = 1.e-12 maestro.eps_init_proj_sph = 1.e-10 # tolerances for the divu iterations maestro.eps_divu_cart = 1.e-12 maestro.eps_divu_sph = 1.e-10 maestro.divu_iter_factor = 100. maestro.divu_level_factor = 10. # tolerances for the MAC projection maestro.eps_mac = 1.e-10 maestro.eps_mac_max = 1.e-8 maestro.mac_level_factor = 10. maestro.eps_mac_bottom = 1.e-3 # tolerances for the nodal projection maestro.eps_hg = 1.e-11 maestro.eps_hg_max = 1.e-10 maestro.hg_level_factor = 10. maestro.eps_hg_bottom = 1.e-4 # OMP settings amrex.regtest_reduction = 1 # GPU parameters maestro.deterministic_nodal_solve = true # override the default values of the probin namelist values here problem.velpert_amplitude = 1.e5 problem.velpert_radius = 2.e7 problem.velpert_scale = 1.e7 problem.velpert_steep = 1.e5 problem.tag_density_1 = 5.e7 problem.tag_density_2 = 1.e8 problem.tag_density_3 = 1.e8 problem.particle_temp_cutoff = 6.e8 problem.particle_tpert_threshold = 2.e7 # Note that some of the parameters in this # namelist are specific to the default EOS, # network, and/or integrator used in the # makefile. If you try a different set of # microphysics routines be sure to check that # the parameters in here are consistent. eos.use_eos_coulomb = 1