| 1 | !================================================================================
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| 2 | ! AstroBEAR physics.data file.
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| 3 | ! Input data describing built-in physics-related parameters of the code.
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| 4 | ! Created for problem: Template
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| 5 | ! Default values for variables in [brackets]
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| 6 | !================================================================================
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| 7 |
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| 8 | &EOSData
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| 9 | !================================================================================
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| 10 | ! Equation of State stuff
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| 11 | !================================================================================
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| 12 | iEOS = 0, ! Equation of State [0]-ideal gas, 1-MultiSpecies gas, 3-Van der Waals gas, 4-Isothermal, 5-Marshak Radiation Test
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| 13 | gamma = 1.667, ! Adiabatic index used for ideal gas and Van der Waals gas [1.66666666667]
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| 14 | IsoTemp = 10d0 ! Isothermal temperature for Isothermal EOS
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| 15 | CriticalDens = 30.693677103 ! maximum density in Van der Waals EOS
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| 16 | AttractionParam = 1.38d6 ! attraction pram in Van der Waals EOS
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| 17 | Marshak_epsilon = .5 ! Ratio of Equilibrium Radiation energy density to thermal energy density
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| 18 | /
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| 19 |
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| 20 | &AbundanceData
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| 21 | !================================================================================
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| 22 | ! Abundance information
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| 23 | ! Define Xmu or set it to zero and it will be calculated from everything else.
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| 24 | !================================================================================
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| 25 | HeFrac = .084d0 ! Ratio of Helium Nuclei to Hydrogen Nuclei
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| 26 | xH = .01d0 ! Ionization fraction of Hydrogenn
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| 27 | xHe = 0d0 ! Ionization fraction of Helium (singly ionized)
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| 28 | xHeII = 0d0 ! Ionization fraction of Helium (doubly ionized)
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| 29 | ZFrac = .00126d0 ! Ratio of Metal Nuclei to Hydrogen Nuclei
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| 30 | xZ = .001d0 ! Ionization fraction of metals
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| 31 | Zmu = 16d0 ! Mean atomic mass of metals - (including electrons from ionized metals)
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| 32 | Xmu = 1, ! Mean atomic mass of everything - (including all free electrons and nuclei)
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| 33 | /
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| 34 |
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| 35 | &PhysicsData
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| 36 | !================================================================================
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| 37 | ! Field based refinement control
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| 38 | !================================================================================
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| 39 | InterpOpts = 1,1,1,1,1,1,1,1,1 ! [0]-constant, 1-minmod, 2-superbee, 3-vanLeer, 4-mc, 5-Parabolic (not conservative), 6-Linear (not limited). It is recommended to use constant interpolation for any fields in q that correspond to aux fields (iBx, iBy, iBz, etc...)
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| 40 | refineVariableFactor = 1d0,0d0,0d0,0d0,0d0,0d0,0d0,0d0,0d0,0d0,0d0 ! weight factors for each field used in triggering refinement. Combined with qtolerance for that level. [1d0]
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| 41 |
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| 42 | !================================================================================
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| 43 | ! Global source term switches
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| 44 | !================================================================================
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| 45 | iSelfGravity = 1 ! [0]-No Self Gravity, 1-Momentumn Conserving SelfGravity, 2-Non momentum conserving self-gravity
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| 46 | iSinkParticles = 0 ! [0]-Sink Particles OFF [1]-Sink Particles ON (default value/recommended for use with self-gravity)
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| 47 | DefaultAccretionRoutine = 2 ! 0-No accretion, [1]-Federrath Accretion, [2]-Krumholz Accretion
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| 48 | UniformGravity = 0d0 ! Gravitational acceleration in the -y direction [0d0]
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| 49 | OmegaRot = 0d0 ! Shifts to a rotating reference frame (enables coriolis and centripetal force terms)
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| 50 | iCylindrical = 0 ! [0]-No cylindrical geometry, 1-Cylindrical with no angular momentum, 2-Cylindrical with angular momentum
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| 51 | iCooling = 7 ! Cooling module [NoCool=0, AnalyticCool=1, DMCool=2, IICool=3, ZCool=4, AlCool=5, NKCool=6, NeutrinoCool=7]
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| 52 | FloorTemp = 1d-10 ! Temperature at which to shut of cooling source terms
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| 53 | SrcPrecision = 1d-3 ! Relative precision desired for source terms. [1d-3]
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| 54 | lTrackHydrogen = .false. ! Track Hydrogen ionization and recombination (Currently only works with iEOS=1 (MultiSpecies)
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| 55 | lTrackHelium = .false. ! Track Helium ionization and recombination (Currently only works with iEOS=1 (MultiSpecies)
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| 56 | iLineTransfer = 0 ! Turn on photo-ionizing line transfer from left by setting to 1.
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| 57 | LineTransferFlux = 0 ! Incoming flux at left boundary in units of cm^-2 s^-1 used if iLineTransfer=1
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| 58 |
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| 59 | !================================================================================
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| 60 | ! Density Protection Options
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| 61 | !================================================================================
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| 62 | lRestartOnDensityProtections = .false. ! Do density protections trigger restarts? [.false.]
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| 63 | lTrackDensityProtections = .false. ! Track density protections [.false.]
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| 64 | iDensityProtect = 2 ! 0-Set to MinDensity, 1-Set to minimum nearby density, [2]-Average nearby densities
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| 65 | iMomentumProtect = 2 ! 0-Conserve momentum, 1-Set to zero, [2]-Average nearby velocities
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| 66 | MinDensity = 1e-8 ! Minimum computational density before protection is triggered [1d-10]
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| 67 |
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| 68 | !================================================================================
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| 69 | ! Pressure Protection Options
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| 70 | !================================================================================
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| 71 | lRestartOnPressureProtections = .false. ! Do pressure protections trigger restarts? [.false.]
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| 72 | lTrackPressureProtections = .false. ! Track pressure protections [.false.]
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| 73 | iPressureProtect = 4 ! 0-Set to MinTemp, 1-Set to minimim nearby pressure, [2]-Set to average nearby pressure, 3-Set to minimum nearby temperature, 4-Set to average nearby temperature
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| 74 | MinTemp = 1e-8, ! [1d-10] minimum allowed temperature for the system in Kelvin before protection is triggered
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| 75 |
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| 76 | !================================================================================
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| 77 | ! Other Protection Options
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| 78 | !================================================================================
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| 79 | lRestartOnHypreMaxIters = T ! Restart steps if hypre does not converge
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| 80 |
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| 81 | !================================================================================
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| 82 | ! Description of various scaling parameters
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| 83 | ! Define lScale and one of [nScale, rScale], and one of [TimeScale, TempScale, or pScale]. Other combinations are possible - as long as the scales are consistent with each other.
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| 84 | !================================================================================
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| 85 | nScale = 0.0, ! number density scale parameter [particles/cc]
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| 86 | rScale = 6.41d9, ! density scale [g/cc]
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| 87 | TimeScale = 0d0, ! time scale [s] (day=8.64d4, yr=3.1556926d7
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| 88 | TempScale = 0d0, ! temperature scale parameter [Kelvin]
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| 89 | pScale = 4.99e27, ! pressure scale [dynes/cm^2]
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| 90 | lScale = 7.26e9 ! length scale parameter [cm] (AU=1.49598e13, pc=3.08568025e18, R_sun=6.955e10
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| 91 |
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| 92 | !================================================================================
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| 93 | ! MHD related section
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| 94 | !================================================================================
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| 95 | lMHD = F, ! Magnetic Fields present? [.false.]
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| 96 | lCheckDivergence = .false. ! Turn on divergence checking [.false.]
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| 97 |
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| 98 | !================================================================================
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| 99 | ! Resistivity switches
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| 100 | !================================================================================
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| 101 | lResistive = .false. ! Turns on resistivity [.false.]
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| 102 | ResType = 2 ! Resistivity type. 1-constant, 2-user defined distribution, 3-Spitzer. [1]
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| 103 | resistivity = 1.2d-1 ! resistivity value [0d0]
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| 104 |
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| 105 | !================================================================================
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| 106 | ! Explicit Conductivity switches
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| 107 | !================================================================================
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| 108 | lConductive = .false. ! Turns on mhd heat conduction [.false.]
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| 109 | ConType = 1 ! Conduction type. 1-constant, 2-Spitzer. [1]
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| 110 | conductivity = 8d-2 ! conductivity value [0d0]
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| 111 | lThermalFluxLimiter = .false. ! Turns on saturation heat flux. (only works for ConType==2). [.false.]
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| 112 | lIsoDiff = .false. ! Turns on isotropic heat conduction. Allows isotropicity to be in the range (0,1). [.false.]
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| 113 |
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| 114 | !================================================================================
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| 115 | ! Implicit Thermal Diffusion switches
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| 116 | !================================================================================
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| 117 | iDiffusion = 0 ! [0]-No diffusion, [1]-Thermal diffusion
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| 118 | kappa1 = 1d0 ! Heat diffusion coefficient
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| 119 | flb = 0d0 ! boundary flux
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| 120 | ndiff = 2.5 ! Temperature power
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| 121 | diffcfl = .01 ! Relative Temperature change allowed per subcycle
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| 122 |
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| 123 | !================================================================================
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| 124 | ! Viscosity switches
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| 125 | !================================================================================
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| 126 | lViscous = .false. ! Turns on viscosity (2D only) [.false.]
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| 127 | VisType = 1 ! viscosity type. 1-classic, 2-Braginskii [1]
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| 128 | bviscosity = 0d0 ! viscosity value [0d0]
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| 129 |
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| 130 | !================================================================================
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| 131 | ! Radiation Transfer switches
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| 132 | !================================================================================
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| 133 | iRadiation = 0 ! [0]-No radiation, 1-Diffusion and energy exchange only, 2-Radiation Advection terms included as well
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| 134 | RadLimiter = 1 ! [0]-LP_FLUX_LIMITER, 1-Diffusion limit, 2-Free streaming limit
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| 135 | PlanckOpacityType = 0 ! [0]-Constant Specific Opacity (k=A*d), [1]-Power Law Opacity (k=A*d^B*T^C)
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| 136 | RoselandOpacityType = 0 ! [0]-Constant Specific Opacity (k=A*d), [1]-Power Law Opacity (k=A*d^B*T^C)
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| 137 | PlanckSpecificOpacity = 1d0 ! Specific Planck Opacity [1d0] (A)
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| 138 | RoselandSpecificOpacity = 1d0 ! Specific Roseland Opacity [1d0] (A)
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| 139 | Roseland_dpow = 1d0 ! Density Power for Roseland Opacity [1d0] (B)
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| 140 | Roseland_tpow = 0d0 ! Temperature Power for Roseland Opacity [0d0] (C)
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| 141 | Planck_dpow = 1d0 ! Density Power for Planck Opacity [1d0] (B)
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| 142 | Planck_tpow = 0d0 ! Temperature Power for Planck Opacity [0d0] (C)
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| 143 | /
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