source: trunk/LMDZ.GENERIC/libf/phystd/radinc_h.F90 @ 1974

Last change on this file since 1974 was 1529, checked in by emillour, 9 years ago

Generic GCM: Towards a cleaner separation between physics and dynamics

  • Got rid of references to "dimensions.h" from physics packages: use nbp_lon (=iim), nbp_lat (=jjp1) and nbp_lev from module mod_grid_phy_lmdz (in phy_common) instead.
  • Removed module "comhdiff_mod.F90", as it is only used by module surf_heat_transp_mod.F90, moved module variables there.
  • Addedin "surf_heat_transp_mod" local versions of some arrays and routines (from dyn3d) required to compute gradient, divergence, etc. on the global dynamics grid. As before, the slab ocean only works in serial.

EM

File size: 3.9 KB
Line 
1module radinc_h
2
3  implicit none
4
5  include "bands.h"
6  include "scatterers.h"
7
8!======================================================================
9!
10!     RADINC.H
11!
12!     Includes for the radiation code; RADIATION LAYERS, LEVELS,
13!     number of spectral intervals. . .
14!
15!======================================================================
16
17!     RADIATION parameters
18
19!     In radiation code, layer 1 corresponds to the stratosphere.  Level
20!     1 is the top of the stratosphere.  The dummy layer is at the same
21!     temperature as the (vertically isothermal) stratosphere, and
22!     any time it is explicitly needed, the appropriate quantities will
23!     be dealt with (aka "top". . .)
24
25!     L_NLEVRAD corresponds to the surface - i.e., the GCM Level that
26!     is at the surface.  PLEV(L_NLEVRAD) = P(J,I)+PTROP,
27!     PLEV(2) = PTROP, PLEV(1) = ptop
28
29!     L_NLAYRAD is the number of radiation code layers
30!     L_NLEVRAD is the number of radiation code levels.  Level N is the
31!               top of layer N.
32!
33!     L_NSPECTI is the number of IR spectral intervals
34!     L_NSPECTV is the number of Visual(or Solar) spectral intervals
35!     L_NGAUSS  is the number of Gauss points for K-coefficients
36!               GAUSS POINT 17 (aka the last one) is the special case
37!
38!     L_NPREF   is the number of reference pressures that the
39!               k-coefficients are calculated on
40!     L_PINT    is the number of Lagrange interpolated reference
41!               pressures for the gas k-coefficients - now for a
42!               smaller p-grid than before
43!     L_NTREF   is the number of reference temperatures for the
44!               k-coefficients
45!     L_TAUMAX  is the largest optical depth - larger ones are set
46!               to this value
47!
48!     L_REFVAR  The number of different mixing ratio values for
49!               the k-coefficients. Variable component of the mixture
50!               can in princple be anything: currently it's H2O.
51!
52!     NAERKIND  The number of radiatively active aerosol types
53!
54!     NSIZEMAX  The maximum number of aerosol particle sizes
55!
56!----------------------------------------------------------------------
57
58      integer,save :: L_NLAYRAD  ! = nbp_lev ! set by ini_radinc_h
59      integer,save :: L_LEVELS   ! = 2*(nbp_lev-1)+3 ! set by ini_radinc_h
60      integer,save :: L_NLEVRAD  ! = nbp_lev+1 ! set by ini_radinc_h
61!$OMP THREADPRIVATE(L_NLAYRAD,L_LEVELS,L_NLEVRAD)
62
63      ! These are set in sugas_corrk
64      ! [uses allocatable arrays] -- AS 12/2011
65      integer :: L_NPREF, L_NTREF, L_REFVAR, L_PINT   !L_NPREF, L_NTREF, L_REFVAR, L_PINT read by master in sugas_corrk
66
67      integer, parameter :: L_NGAUSS  = 17
68
69      integer, parameter :: L_NSPECTI = NBinfrared
70      integer, parameter :: L_NSPECTV = NBvisible
71
72!      integer, parameter :: NAERKIND  = 2 ! set in scatterers.h
73      real,    parameter :: L_TAUMAX  = 35
74
75      ! For Planck function integration:
76      ! equivalent temperatures are 1/NTfac of these values
77      integer, parameter :: NTstar = 500
78      integer, parameter :: NTstop = 15000 ! new default for all non hot Jupiter runs
79      real*8, parameter :: NTfac = 1.0D+1 
80      !integer, parameter :: NTstar = 1000
81      !integer, parameter :: NTstop = 25000
82      !real*8,parameter :: NTfac = 5.0D+1   
83      !integer, parameter :: NTstar = 2000
84      !integer, parameter :: NTstop = 50000
85      !real*8,parameter :: NTfac = 1.0D+2   
86
87      ! Maximum number of grain size classes for aerosol convolution:
88      ! This must correspond to size of largest dataset used for aerosol
89      ! optical properties in datagcm folder.
90      integer, parameter :: nsizemax = 60
91
92      character(len=100),save :: corrkdir
93!$OMP THREADPRIVATE(corrkdir)
94
95      character(len=100),save :: banddir
96!$OMP THREADPRIVATE(banddir)
97
98contains
99
100  subroutine ini_radinc_h(nbp_lev)
101  ! Initialize module variables
102  implicit none
103  integer,intent(in) :: nbp_lev
104 
105  L_NLAYRAD = nbp_lev
106  L_LEVELS = 2*(nbp_lev-1)+3
107  L_NLEVRAD = nbp_lev+1
108 
109  end subroutine
110
111end module radinc_h
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