1 | ## $Header$ |
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2 | # |
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3 | ## Planet: |
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4 | planet_type=venus |
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5 | # |
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6 | ## Number of dynamical steps per day (must be a multiple of iperiod) |
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7 | day_step=240000 |
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8 | ## Apply a Matsuno step every iperiod dynamical step |
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9 | iperiod=5 |
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10 | ## dissipation is applied every dissip_period dynamical steps |
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11 | ## DEFAULT: dissip_period=0 , meaning dissip_period is automatically computed |
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12 | ## (in practice it is =>25 in recent runs) |
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13 | dissip_period=5 |
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14 | ## dissipation operator to use (star or non-star) |
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15 | lstardis=y |
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16 | ## iterate lateral dissipation operator gradiv nitergdiv times |
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17 | nitergdiv=1 |
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18 | ## iterate lateral dissipation operator nxgradrot nitergrot times |
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19 | nitergrot=2 |
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20 | ## iterate lateral dissipation operator divgrad niterh times |
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21 | niterh=2 |
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22 | ## dissipation time scale (s) for shortest wavelengths for u,v (gradiv) |
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23 | tetagdiv=1.e4 |
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24 | ## dissipation time scale (s) for shortest wavelengths for u,v (nxgradrot) |
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25 | tetagrot=1.e4 |
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26 | ## dissipation time scale (s) for shortest wavelengths for u,v (divgrad) |
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27 | tetatemp=1.e4 |
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28 | ## coefficient for gamdissip |
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29 | coefdis=0. |
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30 | ## time marching scheme (Matsuno if purmats is y, else Matsuno-Leapfrog) |
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31 | purmats=n |
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32 | # run with (true) or without (false) physics |
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33 | physic=y |
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34 | ## Physics package type |
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35 | ## 0: no physics (e.g. Shallow Water mode) |
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36 | ## 1: with physics (e.g. phyvenus physics package) |
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37 | ## 2: with a netwonian relaxation scheme in the dynamics |
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38 | iflag_phys=1 |
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39 | ## run with or without initial condition files (start.nc, startphy.nc) ? |
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40 | ## (in the without case, initialization of fields is done via the iniacademic |
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41 | ## routine in the dynamics => not available for Venus |
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42 | read_start=y |
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43 | ## call physics every iphysiq dynamical steps |
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44 | iphysiq=5 |
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45 | ## runwith or without tracers |
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46 | iflag_trac=1 |
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47 | ## run with or without stratosphere // i.e. a sponge layer and secondary |
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48 | ## higher altitude level of horizontal dissipation |
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49 | ok_strato=y |
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50 | ## Horizontal dissipation multipliers along the vertical |
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51 | dissip_fac_mid=2. |
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52 | dissip_fac_up=50. |
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53 | # deltaz et hdelta in km |
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54 | dissip_deltaz=30. |
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55 | dissip_hdelta=5. |
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56 | # pupstart in Pa |
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57 | dissip_pupstart=1.e4 |
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58 | ## Sponge layer |
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59 | # 1: over the topmost 4 levels |
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60 | # 2: over layers at pressures down to 100 times below the topmost layer pressure |
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61 | iflag_top_bound=1 |
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62 | ## Sponge layer mode |
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63 | # mode = 0 : no sponge |
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64 | # mode = 1 : u et v -> 0 |
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65 | # mode = 2 : u et v -> zonal average |
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66 | # mode = 3 : u, v et h -> zonale average |
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67 | mode_top_bound=1 |
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68 | # Coefficient for the sponge layer (value in topmost layer) |
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69 | au_top_bound=1.e-4 |
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70 | # |
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71 | ############################################### |
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72 | ### Zoom parameters |
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73 | ############################################### |
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74 | ## longitude (degrees) of zoom center |
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75 | clon=0. |
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76 | ## latitude (degrees) of zoom center |
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77 | clat=0. |
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78 | ## enhancement factor of zoom, along longitudes |
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79 | grossismx=1.0 |
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80 | ## enhancement factor of zoom, along latitudes |
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81 | grossismy=1.0 |
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82 | ## Use an hyperbolic function f(y) if .true., else use a sine |
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83 | fxyhypb=y |
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84 | ## extention along longitudes of zoom region (fraction of global domain) |
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85 | dzoomx=0.0 |
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86 | ## extention along latitudes of zoom region (fraction of global domain) |
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87 | dzoomy=0.0 |
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88 | ## zoom stiffness along longitudes |
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89 | taux=3. |
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90 | ## zoom stiffness along latitudes |
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91 | tauy=3. |
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92 | ## Fonction f(y) as y = Sin(latitude) if = .true. , else y = latitude |
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93 | ysinus=y |
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