source: LMDZ6/branches/Amaury_dev/libf/phylmd/macv2sp.F90 @ 5136

Last change on this file since 5136 was 5111, checked in by abarral, 4 months ago

Put abort_physic into a module
Remove -g option from makelmdz_fcm, since that option is linked to a header file that isn't included anywhere.
(lint) light lint on traversed files

File size: 7.3 KB
Line 
1SUBROUTINE MACv2SP(pphis, pplay, paprs, xlon, xlat, tau_allaer, piz_allaer, cg_allaer)
2
3  !--routine to read the MACv2SP plume and compute optical properties
4  !--requires flag_aerosol = 7
5  !--feeds into aerosol optical properties and newmicro cloud droplet size if ok_cdnc activated
6  !--for this one needs to feed natural (pre-industrial) aerosols twice for nat and 1980 files
7  !--pre-ind aerosols (index=1) are not changed, present-day aerosols (index=2) are incremented
8  !--uses model year so year_cur needs to be correct in the model simulation
9
10  !--aod_prof = AOD per layer
11  !--ssa_prof = SSA
12  !--asy_prof = asymetry parameter
13  !--dNovrN   = enhancement factor for CDNC
14
15  USE mo_simple_plumes, ONLY: sp_aop_profile
16  USE phys_cal_mod, ONLY: year_cur, day_cur, year_len
17  USE dimphy
18  USE aero_mod
19  USE phys_local_var_mod, ONLY: t_seri, od443aer, od550aer, od865aer, ec550aer, dryod550aer, od550lt1aer, dNovrN
20  !!USE YOMCST, ONLY: RD, RG
21  USE lmdz_abort_physic, ONLY: abort_physic
22  IMPLICIT NONE
23
24  include "YOMCST.h"
25
26  REAL, DIMENSION(klon), INTENT(IN) :: pphis   ! Geopotentiel de surface
27  REAL, DIMENSION(klon, klev), INTENT(IN) :: pplay   ! pression pour le mileu de chaque couche (en Pa)
28  REAL, DIMENSION(klon, klev + 1), INTENT(IN) :: paprs   ! pression pour les interfaces de chaque couche (en Pa)
29  REAL, DIMENSION(klon), INTENT(IN) :: xlat    ! latitudes pour chaque point
30  REAL, DIMENSION(klon), INTENT(IN) :: xlon    ! longitudes pour chaque point
31
32  REAL, DIMENSION(klon, klev, 2, nbands_sw_rrtm), INTENT(OUT) :: tau_allaer !  epaisseur optique aerosol
33  REAL, DIMENSION(klon, klev, 2, nbands_sw_rrtm), INTENT(OUT) :: piz_allaer !  single scattering albedo aerosol
34  REAL, DIMENSION(klon, klev, 2, nbands_sw_rrtm), INTENT(OUT) :: cg_allaer  !  asymmetry parameter aerosol
35
36  REAL, DIMENSION(klon, klev) :: aod_prof, ssa_prof, asy_prof
37  REAL, DIMENSION(klon, klev) :: z, dz
38  REAL, DIMENSION(klon) :: oro, zrho, zt
39
40  INTEGER, PARAMETER :: nmon = 12
41
42  REAL, PARAMETER :: l443 = 443.0, l550 = 550.0, l865 = 865.0 !--wavelengths in nm
43
44  INTEGER, PARAMETER :: Nwvmax = 25
45  REAL, DIMENSION(0:Nwvmax), PARAMETER :: lambda = (/ 240.0, &  !--this one is for band 1
46          280.0, 300.0, 330.0, 360.0, 400.0, &  !--these are bounds of Streamer bands
47          440.0, 480.0, 520.0, 570.0, 640.0, &
48          690.0, 750.0, 780.0, 870.0, 1000.0, &
49          1100.0, 1190.0, 1280.0, 1530.0, 1640.0, &
50          2130.0, 2380.0, 2910.0, 3420.0, 4000.0   /)
51
52  REAL, DIMENSION(1:Nwvmax - 1), PARAMETER :: weight = (/    &   !--and the weights to be given to the bands
53          0.01, 4.05, 9.51, 15.99, 26.07, 33.10, &   !--corresponding to a typical solar spectrum
54                  33.07, 39.91, 52.67, 27.89, 43.60, 13.67, &
55                  42.22, 40.12, 32.70, 14.44, 19.48, 14.23, &
56                  13.43, 16.42, 8.33, 0.95, 0.65, 2.76  /)
57
58  REAL :: zlambda, zweight
59  REAL :: year_fr
60
61  INTEGER band, i, k, Nwv
62
63  ! define the height and dheight arrays
64
65  oro(:) = pphis(:) / RG                             ! surface height in m
66
67  DO k = 1, klev
68    zrho(:) = pplay(:, k) / t_seri(:, k) / RD                         ! air density in kg/m3
69    dz(:, k) = (paprs(:, k) - paprs(:, k + 1)) / zrho(:) / RG              ! layer thickness in m
70    IF (k==1) THEN
71      z(:, 1) = oro(:) + (paprs(:, 1) - pplay(:, 1)) / zrho(:) / RG     ! altitude middle of first layer in m
72      zt(:) = oro(:) + dz(:, 1)                                ! altitude top of first layer in m
73    ELSE
74      z(:, k) = zt(:) + (paprs(:, k) - pplay(:, k)) / zrho(:) / RG       ! altitude middle of layer k in m
75      zt(:) = zt(:) + dz(:, k)                                  ! altitude top of layer k in m
76    ENDIF
77  ENDDO
78
79  !--fractional year
80
81  year_fr = FLOAT(year_cur) + (FLOAT(day_cur) - 0.5) / FLOAT(year_len)
82  IF (year_fr<1850.0.OR.year_fr>=2017.0) THEN
83    CALL abort_physic ('macv2sp', 'year not supported by plume model', 1)
84  ENDIF
85
86  !--CALL to sp routine -- 443 nm
87
88  CALL sp_aop_profile                                    (&
89          klev, klon, l443, oro, xlon, xlat, &
90          year_fr, z, dz, dNovrN, aod_prof, ssa_prof, &
91          asy_prof)
92
93  !--AOD calculations for diagnostics
94  od443aer(:) = od443aer(:) + SUM(aod_prof(:, :), dim = 2)
95
96  !--CALL to sp routine -- 550 nm
97
98  CALL sp_aop_profile                                    (&
99          klev, klon, l550, oro, xlon, xlat, &
100          year_fr, z, dz, dNovrN, aod_prof, ssa_prof, &
101          asy_prof)
102
103  !--AOD calculations for diagnostics
104  od550aer(:) = od550aer(:) + SUM(aod_prof(:, :), dim = 2)
105
106  !--dry AOD calculation for diagnostics
107  dryod550aer(:) = dryod550aer(:) + od550aer(:)
108
109  !--fine-mode AOD calculation for diagnostics
110  od550lt1aer(:) = od550lt1aer(:) + od550aer(:)
111
112  !--extinction coefficient for diagnostic
113  ec550aer(:, :) = ec550aer(:, :) + aod_prof(:, :) / dz(:, :)
114
115  !--CALL to sp routine -- 865 nm
116
117  CALL sp_aop_profile                                    (&
118          klev, klon, l865, oro, xlon, xlat, &
119          year_fr, z, dz, dNovrN, aod_prof, ssa_prof, &
120          asy_prof)
121
122  !--AOD calculations for diagnostics
123  od865aer(:) = od865aer(:) + SUM(aod_prof(:, :), dim = 2)
124
125  !--re-weighting of piz and cg arrays before adding the anthropogenic aerosols
126  !--index 2 = all natural + anthropogenic aerosols
127  piz_allaer(:, :, 2, :) = piz_allaer(:, :, 2, :) * tau_allaer(:, :, 2, :)
128  cg_allaer(:, :, 2, :) = cg_allaer(:, :, 2, :) * piz_allaer(:, :, 2, :)
129
130  !--now computing the same at many wavelengths to fill the model bands
131
132  DO Nwv = 0, Nwvmax - 1
133
134    IF (Nwv==0) THEN          !--RRTM spectral band 1
135      zlambda = lambda(Nwv)
136      zweight = 1.0
137      band = 1
138    ELSEIF (Nwv<=5) THEN      !--RRTM spectral band 2
139      zlambda = 0.5 * (lambda(Nwv) + lambda(Nwv + 1))
140      zweight = weight(Nwv) / SUM(weight(1:5))
141      band = 2
142    ELSEIF (Nwv<=10) THEN     !--RRTM spectral band 3
143      zlambda = 0.5 * (lambda(Nwv) + lambda(Nwv + 1))
144      zweight = weight(Nwv) / SUM(weight(6:10))
145      band = 3
146    ELSEIF (Nwv<=16) THEN     !--RRTM spectral band 4
147      zlambda = 0.5 * (lambda(Nwv) + lambda(Nwv + 1))
148      zweight = weight(Nwv) / SUM(weight(11:16))
149      band = 4
150    ELSEIF (Nwv<=21) THEN     !--RRTM spectral band 5
151      zlambda = 0.5 * (lambda(Nwv) + lambda(Nwv + 1))
152      zweight = weight(Nwv) / SUM(weight(17:21))
153      band = 5
154    ELSE                        !--RRTM spectral band 6
155      zlambda = 0.5 * (lambda(Nwv) + lambda(Nwv + 1))
156      zweight = weight(Nwv) / SUM(weight(22:Nwvmax - 1))
157      band = 6
158    ENDIF
159
160    CALL sp_aop_profile                                       (&
161            klev, klon, zlambda, oro, xlon, xlat, &
162            year_fr, z, dz, dNovrN, aod_prof, ssa_prof, &
163            asy_prof)
164
165    !--adding up the quantities tau, piz*tau and cg*piz*tau
166    tau_allaer(:, :, 2, band) = tau_allaer(:, :, 2, band) + zweight * MAX(aod_prof(:, :), 1.e-15)
167    piz_allaer(:, :, 2, band) = piz_allaer(:, :, 2, band) + zweight * MAX(aod_prof(:, :), 1.e-15) * ssa_prof(:, :)
168    cg_allaer(:, :, 2, band) = cg_allaer(:, :, 2, band) + zweight * MAX(aod_prof(:, :), 1.e-15) * ssa_prof(:, :) * asy_prof(:, :)
169
170  ENDDO
171
172  !--renpomalizing cg and piz now that MACv2SP increments have been added
173  cg_allaer(:, :, 2, :) = cg_allaer(:, :, 2, :) / piz_allaer(:, :, 2, :)
174  piz_allaer(:, :, 2, :) = piz_allaer(:, :, 2, :) / tau_allaer(:, :, 2, :)
175
176END SUBROUTINE MACv2SP
Note: See TracBrowser for help on using the repository browser.