Changeset 1747


Ignore:
Timestamp:
Jul 24, 2017, 5:10:39 PM (7 years ago)
Author:
aslmd
Message:

Amended previous commit. Committed more files than I wanted to.

Location:
trunk
Files:
1 deleted
6 edited

Legend:

Unmodified
Added
Removed

  • trunk/LMDZ.GENERIC/DOC/main.aux

    r1746 r1747  
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    30 \@writefile{lof}{\contentsline {figure}{\numberline {2.2}{\ignorespaces Dynamical and physical grids for a 6 $\times $ 7 horizontal resolution. In the dynamics (but not in the physics) winds u and v are on specific staggered grids. Other dynamical variables are on the dynamical ``scalar'' grid. The physics uses the same ``scalar'' grid for all the variables, except that nodes are indexed in a single vector containing NGRID=2+(JM-1)$\times $IM points when counting from the north pole. N.B.: In the Fortran program, the following variables are used: {\tt  iim=IM , iip1=IM+1, jjm=JM , jjp1=JM+1}.}}{5}}
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    39 \@writefile{lof}{\contentsline {figure}{\numberline {2.4}{\ignorespaces Vertical grid description of the {\tt  llm (or nlayer)} atmospheric layers in the programming code ({\tt  llm} is the variable used in the dynamical part, and {\tt  nlayer} is used in the physical part). Variables {\tt  ap, bp} and {\tt  aps, bps} indicate the hybrid levels at the interlayer levels and at middle of the layers respectively. Pressure at the interlayer is $Plev(l)=ap(l)+bp(l) \times Ps$ and pressure in the middle of the layer is defined by $Play(l)=aps(l)+bps(l) \times Ps$, (where $Ps$ is surface pressure). Sigma coordinates are merely a specific case of hybrid coordinates such that $aps=0$ and $bps=P/Ps$. Note that for the hybrid coordinates, $bps=0$ above $\sim 50$~km, leading to purely pressure levels. The user can choose whether to run the model using hybrid coordinates or not by setting variable {\tt  hybrid} in run.def to True or False.}}{7}}
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    42 \@writefile{toc}{\contentsline {subsection}{\numberline {2.4.3}Tracers}{8}}
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     37\@writefile{lof}{\contentsline {figure}{\numberline {2.4}{\ignorespaces Vertical grid description of the {\tt  llm (or nlayer)} atmospheric layers in the programming code ({\tt  llm} is the variable used in the dynamical part, and {\tt  nlayer} is used in the physical part). Variables {\tt  ap, bp} and {\tt  aps, bps} indicate the hybrid levels at the interlayer levels and at middle of the layers respectively. Pressure at the interlayer is $Plev(l)=ap(l)+bp(l) \times Ps$ and pressure in the middle of the layer is defined by $Play(l)=aps(l)+bps(l) \times Ps$, (where $Ps$ is surface pressure). Sigma coordinates are merely a specific case of hybrid coordinates such that $aps=0$ and $bps=P/Ps$. Note that for the hybrid coordinates, $bps=0$ above $\sim 50$~km, leading to purely pressure levels. The user can choose whether to run the model using hybrid coordinates or not by setting variable {\tt  hybrid} in run.def to True or False.}}{8}}
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    4343\citation{Holt:79}
    4444\citation{LeVa:89}
    4545\citation{Arak:77}
    46 \@writefile{toc}{\contentsline {chapter}{\numberline {3}3D Dynamical Code}{9}}
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    51 \@writefile{lof}{\contentsline {figure}{\numberline {3.1}{\ignorespaces Grille obtenue avec 96 points en longitude et 73 en latitude et un zoom d'un facteur 3 centr\'e sur la m\'edit\'erann\'ee (grille utilis\'ee au laboratoire par Ali Harzallah)}}{9}}
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    55 \@writefile{toc}{\contentsline {paragraph}{la pression extensive:}{10}}
    56 \@writefile{toc}{\contentsline {paragraph}{les trois composantes du flux de masse:}{10}}
    57 \@writefile{toc}{\contentsline {paragraph}{le facteur de Coriolis multipli\'e par l'aire de la maille:}{10}}
    58 \@writefile{toc}{\contentsline {paragraph}{la vorticit\'e potentielle absolue:}{10}}
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     56\@writefile{toc}{\contentsline {paragraph}{les trois composantes du flux de masse:}{13}}
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    7272\citation{Forg:99}
    7373\citation{Forg:99}
    7474\citation{Lewi:99}
    75 \@writefile{toc}{\contentsline {chapter}{\numberline {4}Physical parameterizations of the generic model: some references}{13}}
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    78 \newlabel{sc:phystd}{{4}{13}}
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    80 \@writefile{toc}{\contentsline {paragraph}{General references:}{13}}
    81 \@writefile{toc}{\contentsline {section}{\numberline {4.2}Radiative transfer}{13}}
    82 \@writefile{toc}{\contentsline {subsection}{\numberline {4.2.1}\bf  Absorption/emission and diffusion by dust:}{13}}
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    8383\citation{Toon:89}
    8484\citation{Forg:98grl}
    … …  
    9090\citation{Hour:99}
    9191\citation{Mont:04jgr}
    92 \@writefile{toc}{\contentsline {section}{\numberline {4.3}Subgrid atmospheric dynamical processes}{14}}
    93 \@writefile{toc}{\contentsline {subsection}{\numberline {4.3.1}Turbulent diffusion in the upper layer}{14}}
    94 \@writefile{toc}{\contentsline {subsection}{\numberline {4.3.2}Convection}{14}}
    95 \@writefile{toc}{\contentsline {section}{\numberline {4.4}Surface thermal conduction}{14}}
    96 \@writefile{toc}{\contentsline {section}{\numberline {4.5}CO$_2$ Condensation}{14}}
    97 \@writefile{toc}{\contentsline {section}{\numberline {4.6}Tracer transport and sources}{14}}
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    … …  
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    160 \@writefile{toc}{\contentsline {paragraph}{The ``control'' array}{42}}
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    165 \@writefile{toc}{\contentsline {chapter}{\numberline {8}Water Cycle Simulation}{50}}
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     179\@writefile{toc}{\contentsline {section}{\numberline {10.2}Making a zoomed initial state}{57}}
     180\@writefile{toc}{\contentsline {section}{\numberline {10.3}Running a zoomed simulation and stability issue}{58}}
     181\@writefile{toc}{\contentsline {chapter}{\numberline {11}Changing the radiative transfer properties}{59}}
    184182\@writefile{lof}{\addvspace {10\p@ }}
    185183\@writefile{lot}{\addvspace {10\p@ }}
    186 \newlabel{sc:kspectrum}{{11}{58}}
    187 \@writefile{toc}{\contentsline {section}{\numberline {11.1}Producing the high-resolution data}{58}}
    188 \@writefile{toc}{\contentsline {section}{\numberline {11.2}Performing the correlated-k conversion}{59}}
     184\newlabel{sc:kspectrum}{{11}{59}}
     185\@writefile{toc}{\contentsline {section}{\numberline {11.1}Producing the high-resolution data}{59}}
     186\@writefile{toc}{\contentsline {section}{\numberline {11.2}Performing the correlated-k conversion}{60}}
    189187\bibdata{newfred.bib}
    190 \@writefile{toc}{\contentsline {section}{\numberline {11.3}Implementing the absorption data in the GCM}{60}}
     188\@writefile{toc}{\contentsline {section}{\numberline {11.3}Implementing the absorption data in the GCM}{61}}
    191189\bibstyle{plain}

  • trunk/LMDZ.MARS/libf/dynphy_lonlat/phymars/callphysiq_mod.F90

    r1746 r1747  
    7777              zplev_omp,      & ! pplev
    7878              zplay_omp,      & ! pplay
    79 
    8079              zphi_omp,       & ! pphi
    81 
    82 
    8380              zufi_omp,       & ! pu
    8481              zvfi_omp,       & ! pv

  • trunk/MESOSCALE/LMD_MM_MARS/SIMU/RUN/vert_level_python/levspe.py

    r1746 r1747  
    1414#psurf=92.e5 # Venus
    1515psurf=1.212862e6
    16 
    17 hache = 10.
    18 psurf = 610.
    19 
    20 
    2116print hache, psurf
    2217#read paramlevspe
    23 
    24 
    25 
    26 
    2718param=np.loadtxt('paramlevspe')
    2819nlev=param[0]
    … …  
    6152#print ptop
    6253etas=(pressions-ptop)/(psurf-ptop)
    63 etas[int(nlev)-1]=0.
     54etas[nlev-1]=0.
    6455#print etas
    6556press=etas*(psurf-ptop)+ptop
    … …  
    7768np.savetxt('levels',etas)
    7869
    79 plt.figure(figsize=(12, 6))
     70plt.figure(figsize=(15, 15))
    8071plt.subplot(221)
    81 plt.plot(x, etas, 'b.')
     72plt.plot(x, etas)
    8273plt.xlabel('levels')
    8374plt.ylabel('etas')
    … …  
    8576#plt.title('a) NINO3 Sea Surface Temperature (seasonal)')
    8677#plt.hold(False)
    87 axes = plt.gca()
    88 axes.set_ylim([0,1])
    8978
    9079plt.subplot(222)
    91 plt.plot(x, pseudo, 'b.')
     80plt.plot(x, pseudo)
    9281plt.xlabel('levels')
    9382plt.grid()
    9483plt.ylabel('pseudo-altitude (km)')
    95 plt.semilogy()
    96 axes = plt.gca()
    97 axes.set_ylim([0,60])
    98 
    9984
    10085plt3 = plt.subplot(223)
    101 plt.semilogy(x, press, 'b.')
     86plt.semilogy(x, press)
    10287plt.xlabel('levels')
    10388plt.grid()
    104 plt.ylabel('pressure (Pa)')
     89plt.ylabel('pression (Pa)')
    10590
    10691plt4 = plt.subplot(224)
    107 plt.plot(x, res, 'b.')
     92plt.plot(x, res)
    10893plt.xlabel('levels')
    10994plt.grid()

  • trunk/MESOSCALE/LMD_MM_MARS/SIMU/RUN/vert_level_python/paramlevspe

    r1746 r1747  
    33#epsilon augmentation totale en pourcentage de l'ecart max (modifie inflexion). epsilon = 0   : point d'inflexion parfaitement plat. epsilon = 100 : pas de point d'inflexion
    44#elong_cos plus petit rapproche l'inflexion du sol ;; 2/3 parfait pour un nlev divisible par 3
    5 61
    6 60.
    7 100
    8 1.75
     5201
     6280.
     70
     80.000000044

  • trunk/MESOSCALE/LMD_MM_MARS/SIMU/namelist.input_full

    r1746 r1747  
    8888 h_sca_adv_order = 5,        !! (*d) Horizontal scalar advection order
    8989 v_sca_adv_order = 3,        !! (*d) Vertical scalar advection order
    90  khdif = 10.,      !! ** direct diffusion for tests (km_opt=1). horizontal diffusion constant (m^2/s)
    91  kvdif = 10.,      !! ** direct diffusion for tests (km_opt=1). vertical diffusion constant (m^2/s)
    9290 /
    9391

  • trunk/UTIL/SPECTRA/makefile

    r1746 r1747  
    1 netcdfpath=/home/aymeric/Science/NETCDF/netcdf64-4.0.1_gfortran
    2 spherepackpath=./spherepack3.2
    3 FC=gfortran
     1netcdfpath=/planeto/milmd/library/netcdf/netcdf-4.0.1_levan_pgf90
     2spherepackpath=/planeto/milmd/library/spherepack/spherepack3.2_levan_pgf90
     3FC=pgf90
    44
    55
    66FFLAGS=-I${netcdfpath}/include -I${spherepackpath}/lib
    7 #LDFLAGS=-L${netcdfpath}/lib -lnetcdf -L${spherepackpath}/lib -lspherepack
    8 LDFLAGS=-L${netcdfpath}/lib -lnetcdf -lnetcdff -L${spherepackpath}/lib -lspherepack
     7LDFLAGS=-L${netcdfpath}/lib -lnetcdf -L${spherepackpath}/lib -lspherepack
    98
    109SRCS= $(wildcard *.f90)
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