[38] | 1 | # |
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| 2 | #----------------------------------------------------------------------- |
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[1949] | 3 | #GCM run control parameters: |
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| 4 | #--------------------------- |
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[38] | 5 | |
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[1949] | 6 | # planet type |
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| 7 | planet_type=mars |
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| 8 | |
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| 9 | # Number of days to run model for |
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[38] | 10 | nday=9999 |
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| 11 | |
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[1949] | 12 | # Number of dynamical steps per day (must be a multiple of iperiod) |
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[38] | 13 | day_step = 960 |
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| 14 | |
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[1949] | 15 | # Apply a Matsuno step every iperiod dynamical step |
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[38] | 16 | iperiod=5 |
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| 17 | |
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[1949] | 18 | # Control output information in the dynamics every iconser dynamical steps |
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[38] | 19 | iconser=120 |
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| 20 | |
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[1949] | 21 | # Apply dissipation every idissip dynamical steps |
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[1970] | 22 | idissip=1 |
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[38] | 23 | |
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[1949] | 24 | # dissipation operator to use (star or non-star) |
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[38] | 25 | lstardis=.true. |
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| 26 | |
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[1949] | 27 | # use hybrid vertical coordinate (else will use sigma levels) |
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[38] | 28 | hybrid=.true. |
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| 29 | |
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[1949] | 30 | # use hybrid vertical coordinate (else will use sigma levels) |
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[38] | 31 | nitergdiv=1 |
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| 32 | |
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[1949] | 33 | # iterate lateral dissipation operator nxgradrot nitergrot times |
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[38] | 34 | nitergrot=2 |
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| 35 | |
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[1949] | 36 | # iterate lateral dissipation operator divgrad niterh times |
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[38] | 37 | niterh=2 |
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| 38 | |
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[1949] | 39 | # time scale (s) for shortest wavelengths for u,v (gradiv) |
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[2637] | 40 | tetagdiv= 2500. |
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[38] | 41 | |
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[1949] | 42 | # time scale (s) for shortest wavelengths for u,v (nxgradrot) |
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[38] | 43 | tetagrot=5000. |
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| 44 | |
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[1949] | 45 | # time scale (s) for shortest wavelengths for h (divgrad) |
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[38] | 46 | tetatemp=5000. |
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| 47 | |
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[2637] | 48 | # multiplicative constants for dissipation with altitude: |
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| 49 | # coefficient for middle atmosphere (~20-70km) |
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| 50 | dissip_fac_mid = 2 |
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| 51 | # coefficient for upper atmosphere (~100km+) |
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| 52 | dissip_fac_up = 10 |
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| 53 | |
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[1949] | 54 | # coefficient for gamdissip |
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[38] | 55 | coefdis=0. |
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| 56 | |
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[1949] | 57 | # time marching scheme (Matsuno if purmats is true, else Matsuno-Leapfrog) |
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[38] | 58 | purmats=.false. |
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| 59 | |
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[1949] | 60 | # run with (true) or without (false) physics |
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[38] | 61 | physic=.true. |
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| 62 | |
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[1949] | 63 | # call physics every iphysiq dynamical steps |
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| 64 | iphysiq=10 |
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[38] | 65 | |
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[1949] | 66 | # Use a regular grid |
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[38] | 67 | grireg=.true. |
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| 68 | |
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[1949] | 69 | # Output in diagfi file every ecritphy dynamical steps |
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[38] | 70 | ecritphy=240 |
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| 71 | |
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[1949] | 72 | # longitude (degrees) of zoom center |
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[38] | 73 | clon=63. |
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| 74 | |
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[1949] | 75 | # latitude (degrees) of zoom center |
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[38] | 76 | clat=0. |
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| 77 | |
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[1949] | 78 | # enhancement factor of zoom, along longitudes |
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[38] | 79 | grossismx=1. |
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| 80 | |
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[1949] | 81 | # enhancement factor of zoom, along latitudes |
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[38] | 82 | grossismy=1. |
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| 83 | |
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[1949] | 84 | # Use an hyperbolic function f(y) if .true., else use a sine |
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[38] | 85 | fxyhypb=.false. |
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| 86 | |
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[1949] | 87 | # extention along longitudes of zoom region (fraction of global domain) |
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[38] | 88 | dzoomx= 0. |
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| 89 | |
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[1949] | 90 | # extention along latitudes of zoom region (fraction of global domain) |
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[38] | 91 | dzoomy=0. |
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| 92 | |
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[1949] | 93 | # zoom stiffness along longitudes |
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[38] | 94 | taux=2. |
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| 95 | |
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[1949] | 96 | # zoom stiffness along latitudes |
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[38] | 97 | tauy=2. |
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| 98 | |
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[1949] | 99 | # Fonction f(y) as y = Sin(latitude) if = .true. , else y = latitude |
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[38] | 100 | ysinus= .false. |
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| 101 | |
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[1949] | 102 | # Use a sponge layer |
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[38] | 103 | callsponge = .true. |
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| 104 | |
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[2637] | 105 | # Sponge layer extends over topmost nsponge layers (default =3) |
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[1949] | 106 | nsponge = 3 |
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| 107 | |
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[2637] | 108 | # Sponge: mode0(h=hmoy,u=v=0), mode1(h=hmoy,u=umoy,v=0), mode2(h=hmoy,u=umoy,v=vmoy) |
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| 109 | mode_sponge= 2 |
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[38] | 110 | |
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[1949] | 111 | # Sponge layer time scale (s): tetasponge |
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[575] | 112 | tetasponge = 30000 |
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[38] | 113 | |
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| 114 | # some definitions for the physics, in file 'callphys.def' |
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| 115 | INCLUDEDEF=callphys.def |
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