source: trunk/LMDZ.MARS/libf/phymars/yomlw_h.F90 @ 3026

Last change on this file since 3026 was 2578, checked in by romain.vande, 3 years ago

First stage of implementing Open_MP in the physic.
So far it can initialyse physic and run with all routines at .FALSE.

File size: 3.3 KB
RevLine 
[1047]1module yomlw_h
2! Coefficients for the longwave radiation subroutines
3use dimradmars_mod, only: nir, nabsmx, npademx
4implicit none
5
6  real,save :: at(2,2)
7  real,save :: bt(2,2)
8  real,save :: tref= 200.0 ! tref: temperature dependence of the absorption
9  real,save :: xp(6,nir)
10  real,save :: tstand = 200.0 ! reference temperature for the Planck function
11  real,save :: ga(npademx,nabsmx)
12  real,save :: gb(npademx,nabsmx)
13  real,save :: cst_voigt(2,nabsmx)
14  real,save :: gcp ! = g/cpp (set in callradite)
15
[2578]16!$OMP THREADPRIVATE(at,bt,tref,xp,tstand,ga,gb,cst_voigt,gcp)
17
[1047]18! Number of layers on which LTE calculations (in lw and sw) are performed
19! (Computed in nlthermeq) :
20  integer,save :: nlaylte
21
22  real,save,allocatable :: xi(:,:,:,:)
23  real,save,allocatable :: xi_ground(:,:)
24  real,save,allocatable :: xi_emis(:,:,:)
25
[2578]26!$OMP THREADPRIVATE(nlaylte,xi,xi_ground,xi_emis)
27
[1047]28contains
29
[1224]30! Allocate array (subroutine ini_yomlw_h is called by phys_state_var_init)
[1047]31  subroutine ini_yomlw_h(ngrid)
32   
33    use dimradmars_mod, only: nuco2,nflev
34    implicit none
35   
36    integer,intent(in) :: ngrid ! number of atmospheric columns
37   
38    allocate(xi(ngrid,nuco2,0:nflev+1,0:nflev+1))
39    allocate(xi_ground(ngrid,nuco2))
40    allocate(xi_emis(ngrid,nuco2,nflev-1))
[1772]41   
42    xi (:,:,:,:)=0. ! initialisation previously done in lwmain at firstcall
43 
[1047]44    ! initialize xp(),at(),bt(),ga(),gb(),cst_voigt()
45
46    ! What follows was taken from old "sulw.F" routine (by Jean-Jacques
47    ! Morcrette, ECMWF, further simplified by F. Forget 01/2000),
48    ! adapted to F90
49   
50    ! ROOTS AND WEIGHTS FOR THE 2-POINT GAUSSIAN QUADRATURE
51!     DATA (RT1(IG1),IG1=1,2) / -0.577350269, +0.577350269 /
52!     DATA (WG1(IG1),IG1=1,2) /  1.0        ,  1.0         /
53    ! COEFFICIENTS OF THE POLYNOMIALS GIVING THE PLANCK FUNCTIONS
54    xp = reshape ( (/ &
55           0.63849788E+01, 0.30969419E+02, 0.44790835E+02, &
56           0.52651048E+01,-0.18799237E+02, 0.92836181E+01, &
57           0.26166790E+02, 0.12348011E+03, 0.17868306E+03, &
58           0.33657659E+02,-0.66869343E+02, 0.21017507E+02, &
59           0.11101254E+02, 0.86037325E+02, 0.25892695E+03, &
60           0.35582991E+03, 0.16958020E+03,-0.41311413E+02, &
61           0.47045285E+02, 0.12234377E+03, 0.61873275E+02, &
62           -0.31971883E+02, 0.59168472E+01, 0.91927407E+01 &
63                    /) , (/ 6,nir /) )
64
65    ! temperature dependency of absorber amounts:
66    at = reshape( (/ &
67           0.694E-03, 0.272E-02, 0.275E-02, 0.178E-01  &
68                   /) , (/ 2,2 /) )
69    bt = reshape( (/ &
70           0.328E-05, 0.298E-05,-0.705E-04,-0.163E-04  &
71                   /) , (/ 2,2 /) )
72
73    ga(1:4,1) = (/ 0.288231E-04, 0.170794E-01,-0.339714E-01, 0.000000E+00 /)
74    gb(1:4,1) = (/ 0.288231E-04, 0.145426E-01, 0.543812E+00, 0.100000E+01 /)
75   
76    ga(1:4,2) = (/ 0.289299E-01, 0.190634E+01, 0.384061E+01, 0.000000E+00 /)
77    gb(1:4,2) = (/ 0.289299E-01, 0.189485E+01, 0.600363E+01, 0.100000E+01 /)
78   
79    cst_voigt = reshape( (/ &
80                  0.500E-02, 0.100E-01, 0.150E-01, 0.100E+00  &
81                         /) , (/ 2,2 /) )
82 
83  end subroutine ini_yomlw_h
[1772]84   
85  subroutine end_yomlw_h
86
87    implicit none
88
89    if (allocated(xi)) deallocate(xi)
90    if (allocated(xi_ground)) deallocate(xi_ground)
91    if (allocated(xi_emis)) deallocate(xi_emis)
92
93  end subroutine end_yomlw_h
94 
[1047]95end module yomlw_h
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