| 1 |
! |
module diagphy_m |
| 2 |
! $Header: /home/cvsroot/LMDZ4/libf/phylmd/diagphy.F,v 1.1.1.1 2004/05/19 12:53:08 lmdzadmin Exp $ |
|
| 3 |
! |
implicit none |
| 4 |
SUBROUTINE diagphy(airephy,tit,iprt |
|
| 5 |
$ , tops, topl, sols, soll, sens |
contains |
| 6 |
$ , evap, rain_fall, snow_fall, ts |
|
| 7 |
$ , d_etp_tot, d_qt_tot, d_ec_tot |
SUBROUTINE diagphy(airephy, tit, iprt, tops, topl, sols, soll, sens, evap, & |
| 8 |
$ , fs_bound, fq_bound) |
rain_fall, snow_fall, ts, d_etp_tot, d_qt_tot, d_ec_tot) |
| 9 |
C====================================================================== |
|
| 10 |
C |
! From LMDZ4/libf/phylmd/diagphy.F, version 1.1.1.1 2004/05/19 12:53:08 |
| 11 |
C Purpose: |
|
| 12 |
C Compute the thermal flux and the watter mass flux at the atmosphere |
! Purpose: compute the thermal flux and the water mass flux at |
| 13 |
c boundaries. Print them and also the atmospheric enthalpy change and |
! the atmospheric boundaries. Print them and print the atmospheric |
| 14 |
C the atmospheric mass change. |
! enthalpy change and the atmospheric mass change. |
| 15 |
C |
|
| 16 |
C Arguments: |
! J.-L. Dufresne, July 2002 |
| 17 |
C airephy-------input-R- grid area |
|
| 18 |
C tit---------input-A15- Comment to be added in PRINT (CHARACTER*15) |
USE dimphy, ONLY: klon |
| 19 |
C iprt--------input-I- PRINT level ( <=0 : no PRINT) |
USE suphec_m, ONLY: rcpd, rcpv, rcs, rcw, rlstt, rlvtt |
| 20 |
C tops(klon)--input-R- SW rad. at TOA (W/m2), positive up. |
|
| 21 |
C topl(klon)--input-R- LW rad. at TOA (W/m2), positive down |
! Arguments: |
| 22 |
C sols(klon)--input-R- Net SW flux above surface (W/m2), positive up |
|
| 23 |
C (i.e. -1 * flux absorbed by the surface) |
! Input variables |
| 24 |
C soll(klon)--input-R- Net LW flux above surface (W/m2), positive up |
real, intent(in):: airephy(klon) ! grid area |
| 25 |
C (i.e. flux emited - flux absorbed by the surface) |
CHARACTER(len=15), intent(in):: tit ! comment to be added in PRINT |
| 26 |
C sens(klon)--input-R- Sensible Flux at surface (W/m2), positive down |
INTEGER, intent(in):: iprt ! PRINT level (<=0 : no PRINT) |
| 27 |
C evap(klon)--input-R- Evaporation + sublimation watter vapour mass flux |
real, intent(in):: tops(klon) ! SW rad. at TOA (W/m2), positive up |
| 28 |
C (kg/m2/s), positive up |
real, intent(in):: topl(klon) ! LW rad. at TOA (W/m2), positive down |
| 29 |
C rain_fall(klon) |
|
| 30 |
C --input-R- Liquid watter mass flux (kg/m2/s), positive down |
real, intent(in):: sols(klon) |
| 31 |
C snow_fall(klon) |
! net SW flux above surface (W/m2), positive up (i.e. -1 * flux |
| 32 |
C --input-R- Solid watter mass flux (kg/m2/s), positive down |
! absorbed by the surface) |
| 33 |
C ts(klon)----input-R- Surface temperature (K) |
|
| 34 |
C d_etp_tot---input-R- Heat flux equivalent to atmospheric enthalpy |
real, intent(in):: soll(klon) |
| 35 |
C change (W/m2) |
! net longwave flux above surface (W/m2), positive up (i. e. flux |
| 36 |
C d_qt_tot----input-R- Mass flux equivalent to atmospheric watter mass |
! emited - flux absorbed by the surface) |
| 37 |
C change (kg/m2/s) |
|
| 38 |
C d_ec_tot----input-R- Flux equivalent to atmospheric cinetic energy |
real, intent(in):: sens(klon) |
| 39 |
C change (W/m2) |
! sensible Flux at surface (W/m2), positive down |
| 40 |
C |
|
| 41 |
C fs_bound---output-R- Thermal flux at the atmosphere boundaries (W/m2) |
real, intent(in):: evap(klon) |
| 42 |
C fq_bound---output-R- Watter mass flux at the atmosphere boundaries (kg/m2/s) |
! evaporation + sublimation water vapour mass flux (kg/m2/s), |
| 43 |
C |
! positive up |
| 44 |
C J.L. Dufresne, July 2002 |
|
| 45 |
C====================================================================== |
real, intent(in):: rain_fall(klon) |
| 46 |
C |
! liquid water mass flux (kg/m2/s), positive down |
| 47 |
use dimens_m |
|
| 48 |
use dimphy |
real, intent(in):: snow_fall(klon) |
| 49 |
use YOMCST |
! solid water mass flux (kg/m2/s), positive down |
| 50 |
use yoethf |
|
| 51 |
implicit none |
REAL, intent(in):: ts(klon) ! surface temperature (K) |
| 52 |
|
|
| 53 |
C |
REAL, intent(in):: d_etp_tot |
| 54 |
C Input variables |
! heat flux equivalent to atmospheric enthalpy change (W/m2) |
| 55 |
real airephy(klon) |
|
| 56 |
CHARACTER*15 tit |
REAL, intent(in):: d_qt_tot |
| 57 |
INTEGER iprt |
! Mass flux equivalent to atmospheric water mass change (kg/m2/s) |
| 58 |
real tops(klon),topl(klon),sols(klon),soll(klon) |
|
| 59 |
real sens(klon),evap(klon),rain_fall(klon),snow_fall(klon) |
REAL, intent(in):: d_ec_tot |
| 60 |
REAL ts(klon) |
! flux equivalent to atmospheric cinetic energy change (W/m2) |
| 61 |
REAL d_etp_tot, d_qt_tot, d_ec_tot |
|
| 62 |
c Output variables |
! Local: |
| 63 |
REAL fs_bound, fq_bound |
REAL fs_bound ! thermal flux at the atmosphere boundaries (W/m2) |
| 64 |
C |
real fq_bound ! water mass flux at the atmosphere boundaries (kg/m2/s) |
| 65 |
C Local variables |
real stops, stopl, ssols, ssoll |
| 66 |
real stops,stopl,ssols,ssoll |
real ssens, sfront, slat |
| 67 |
real ssens,sfront,slat |
real airetot, zcpvap, zcwat, zcice |
| 68 |
real airetot, zcpvap, zcwat, zcice |
REAL rain_fall_tot, snow_fall_tot, evap_tot |
| 69 |
REAL rain_fall_tot, snow_fall_tot, evap_tot |
integer i |
| 70 |
C |
integer:: pas = 0 |
| 71 |
integer i |
|
| 72 |
C |
!------------------------------------------------------------------ |
| 73 |
integer pas |
|
| 74 |
save pas |
IF (iprt >= 1) then |
| 75 |
data pas/0/ |
pas=pas+1 |
| 76 |
C |
stops=0. |
| 77 |
pas=pas+1 |
stopl=0. |
| 78 |
stops=0. |
ssols=0. |
| 79 |
stopl=0. |
ssoll=0. |
| 80 |
ssols=0. |
ssens=0. |
| 81 |
ssoll=0. |
sfront = 0. |
| 82 |
ssens=0. |
evap_tot = 0. |
| 83 |
sfront = 0. |
rain_fall_tot = 0. |
| 84 |
evap_tot = 0. |
snow_fall_tot = 0. |
| 85 |
rain_fall_tot = 0. |
airetot=0. |
| 86 |
snow_fall_tot = 0. |
|
| 87 |
airetot=0. |
! Pour les chaleurs spécifiques de la vapeur d'eau, de l'eau et de |
| 88 |
C |
! la glace, on travaille par différence à la chaleur spécifique de |
| 89 |
C Pour les chaleur specifiques de la vapeur d'eau, de l'eau et de |
! l'air sec. En effet, comme on travaille à niveau de pression |
| 90 |
C la glace, on travaille par difference a la chaleur specifique de l' |
! donné, toute variation de la masse d'un constituant est |
| 91 |
c air sec. En effet, comme on travaille a niveau de pression donne, |
! totalement compensée par une variation de masse d'air. |
| 92 |
C toute variation de la masse d'un constituant est totalement |
|
| 93 |
c compense par une variation de masse d'air. |
zcpvap=RCPV-RCPD |
| 94 |
C |
zcwat=RCW-RCPD |
| 95 |
zcpvap=RCPV-RCPD |
zcice=RCS-RCPD |
| 96 |
zcwat=RCW-RCPD |
|
| 97 |
zcice=RCS-RCPD |
do i=1, klon |
| 98 |
C |
stops=stops+tops(i)*airephy(i) |
| 99 |
do i=1,klon |
stopl=stopl+topl(i)*airephy(i) |
| 100 |
stops=stops+tops(i)*airephy(i) |
ssols=ssols+sols(i)*airephy(i) |
| 101 |
stopl=stopl+topl(i)*airephy(i) |
ssoll=ssoll+soll(i)*airephy(i) |
| 102 |
ssols=ssols+sols(i)*airephy(i) |
ssens=ssens+sens(i)*airephy(i) |
| 103 |
ssoll=ssoll+soll(i)*airephy(i) |
sfront = sfront + (evap(i) * zcpvap - rain_fall(i) * zcwat & |
| 104 |
ssens=ssens+sens(i)*airephy(i) |
- snow_fall(i) * zcice) * ts(i) * airephy(i) |
| 105 |
sfront = sfront |
evap_tot = evap_tot + evap(i)*airephy(i) |
| 106 |
$ + ( evap(i)*zcpvap-rain_fall(i)*zcwat-snow_fall(i)*zcice |
rain_fall_tot = rain_fall_tot + rain_fall(i)*airephy(i) |
| 107 |
$ ) *ts(i) *airephy(i) |
snow_fall_tot = snow_fall_tot + snow_fall(i)*airephy(i) |
| 108 |
evap_tot = evap_tot + evap(i)*airephy(i) |
airetot=airetot+airephy(i) |
| 109 |
rain_fall_tot = rain_fall_tot + rain_fall(i)*airephy(i) |
enddo |
| 110 |
snow_fall_tot = snow_fall_tot + snow_fall(i)*airephy(i) |
stops=stops/airetot |
| 111 |
airetot=airetot+airephy(i) |
stopl=stopl/airetot |
| 112 |
enddo |
ssols=ssols/airetot |
| 113 |
stops=stops/airetot |
ssoll=ssoll/airetot |
| 114 |
stopl=stopl/airetot |
ssens=ssens/airetot |
| 115 |
ssols=ssols/airetot |
sfront = sfront/airetot |
| 116 |
ssoll=ssoll/airetot |
evap_tot = evap_tot /airetot |
| 117 |
ssens=ssens/airetot |
rain_fall_tot = rain_fall_tot/airetot |
| 118 |
sfront = sfront/airetot |
snow_fall_tot = snow_fall_tot/airetot |
| 119 |
evap_tot = evap_tot /airetot |
|
| 120 |
rain_fall_tot = rain_fall_tot/airetot |
slat = RLVTT * rain_fall_tot + RLSTT * snow_fall_tot |
| 121 |
snow_fall_tot = snow_fall_tot/airetot |
fs_bound = stops-stopl - (ssols+ssoll)+ssens+sfront + slat |
| 122 |
C |
fq_bound = evap_tot - rain_fall_tot -snow_fall_tot |
| 123 |
slat = RLVTT * rain_fall_tot + RLSTT * snow_fall_tot |
|
| 124 |
C Heat flux at atm. boundaries |
print 6666, tit, pas, fs_bound, d_etp_tot, fq_bound, d_qt_tot |
| 125 |
fs_bound = stops-stopl - (ssols+ssoll)+ssens+sfront |
print 6668, tit, pas, d_etp_tot+d_ec_tot-fs_bound, d_qt_tot - fq_bound |
| 126 |
$ + slat |
|
| 127 |
C Watter flux at atm. boundaries |
IF (iprt >= 2) print 6667, tit, pas, stops, stopl, ssols, ssoll, ssens, & |
| 128 |
fq_bound = evap_tot - rain_fall_tot -snow_fall_tot |
slat, evap_tot, rain_fall_tot + snow_fall_tot |
| 129 |
C |
end IF |
| 130 |
IF (iprt.ge.1) write(6,6666) |
|
| 131 |
$ tit, pas, fs_bound, d_etp_tot, fq_bound, d_qt_tot |
6666 format('Physics flux budget ', a15, 1i6, 2f8.2, 2(1pE13.5)) |
| 132 |
C |
6667 format('Physics boundary flux ', a15, 1i6, 6f8.2, 2(1pE13.5)) |
| 133 |
IF (iprt.ge.1) write(6,6668) |
6668 format('Physics total budget ', a15, 1i6, f8.2, 2(1pE13.5)) |
| 134 |
$ tit, pas, d_etp_tot+d_ec_tot-fs_bound, d_qt_tot-fq_bound |
|
| 135 |
C |
end SUBROUTINE diagphy |
| 136 |
IF (iprt.ge.2) write(6,6667) |
|
| 137 |
$ tit, pas, stops,stopl,ssols,ssoll,ssens,slat,evap_tot |
end module diagphy_m |
|
$ ,rain_fall_tot+snow_fall_tot |
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return |
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6666 format('Phys. Flux Budget ',a15,1i6,2f8.2,2(1pE13.5)) |
|
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6667 format('Phys. Boundary Flux ',a15,1i6,6f8.2,2(1pE13.5)) |
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6668 format('Phys. Total Budget ',a15,1i6,f8.2,2(1pE13.5)) |
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end |
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C====================================================================== |
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SUBROUTINE diagetpq(airephy,tit,iprt,idiag,idiag2,dtime |
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e ,t,q,ql,qs,u,v,paprs,pplay |
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s , d_h_vcol, d_qt, d_qw, d_ql, d_qs, d_ec) |
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C====================================================================== |
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C |
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C Purpose: |
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C Calcul la difference d'enthalpie et de masse d'eau entre 2 appels, |
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C et calcul le flux de chaleur et le flux d'eau necessaire a ces |
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C changements. Ces valeurs sont moyennees sur la surface de tout |
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C le globe et sont exprime en W/2 et kg/s/m2 |
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C Outil pour diagnostiquer la conservation de l'energie |
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C et de la masse dans la physique. Suppose que les niveau de |
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c pression entre couche ne varie pas entre 2 appels. |
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C |
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C Plusieurs de ces diagnostics peuvent etre fait en parallele: les |
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c bilans sont sauvegardes dans des tableaux indices. On parlera |
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C "d'indice de diagnostic" |
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c |
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C |
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c====================================================================== |
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C Arguments: |
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C airephy-------input-R- grid area |
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C tit-----imput-A15- Comment added in PRINT (CHARACTER*15) |
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C iprt----input-I- PRINT level ( <=1 : no PRINT) |
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C idiag---input-I- indice dans lequel sera range les nouveaux |
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C bilans d' entalpie et de masse |
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C idiag2--input-I-les nouveaux bilans d'entalpie et de masse |
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C sont compare au bilan de d'enthalpie de masse de |
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C l'indice numero idiag2 |
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C Cas parriculier : si idiag2=0, pas de comparaison, on |
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c sort directement les bilans d'enthalpie et de masse |
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C dtime----input-R- time step (s) |
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c t--------input-R- temperature (K) |
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c q--------input-R- vapeur d'eau (kg/kg) |
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c ql-------input-R- liquid watter (kg/kg) |
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c qs-------input-R- solid watter (kg/kg) |
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c u--------input-R- vitesse u |
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c v--------input-R- vitesse v |
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c paprs----input-R- pression a intercouche (Pa) |
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c pplay----input-R- pression au milieu de couche (Pa) |
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c |
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C the following total value are computed by UNIT of earth surface |
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C |
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C d_h_vcol--output-R- Heat flux (W/m2) define as the Enthalpy |
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c change (J/m2) during one time step (dtime) for the whole |
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C atmosphere (air, watter vapour, liquid and solid) |
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C d_qt------output-R- total water mass flux (kg/m2/s) defined as the |
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C total watter (kg/m2) change during one time step (dtime), |
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C d_qw------output-R- same, for the watter vapour only (kg/m2/s) |
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C d_ql------output-R- same, for the liquid watter only (kg/m2/s) |
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C d_qs------output-R- same, for the solid watter only (kg/m2/s) |
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C d_ec------output-R- Cinetic Energy Budget (W/m2) for vertical air column |
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C |
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C other (COMMON...) |
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C RCPD, RCPV, .... |
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C |
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C J.L. Dufresne, July 2002 |
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c====================================================================== |
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use dimens_m |
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use dimphy |
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use YOMCST |
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use yoethf |
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IMPLICIT NONE |
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C |
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C |
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c Input variables |
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real airephy(klon) |
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CHARACTER*15 tit |
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INTEGER iprt,idiag, idiag2 |
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REAL, intent(in):: dtime |
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REAL t(klon,klev), q(klon,klev), ql(klon,klev), qs(klon,klev) |
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REAL u(klon,klev), v(klon,klev) |
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REAL, intent(in):: paprs(klon,klev+1) |
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real pplay(klon,klev) |
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c Output variables |
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REAL d_h_vcol, d_qt, d_qw, d_ql, d_qs, d_ec |
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C |
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C Local variables |
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c |
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REAL h_vcol_tot, h_dair_tot, h_qw_tot, h_ql_tot |
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. , h_qs_tot, qw_tot, ql_tot, qs_tot , ec_tot |
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c h_vcol_tot-- total enthalpy of vertical air column |
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C (air with watter vapour, liquid and solid) (J/m2) |
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c h_dair_tot-- total enthalpy of dry air (J/m2) |
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c h_qw_tot---- total enthalpy of watter vapour (J/m2) |
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c h_ql_tot---- total enthalpy of liquid watter (J/m2) |
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c h_qs_tot---- total enthalpy of solid watter (J/m2) |
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c qw_tot------ total mass of watter vapour (kg/m2) |
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c ql_tot------ total mass of liquid watter (kg/m2) |
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c qs_tot------ total mass of solid watter (kg/m2) |
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c ec_tot------ total cinetic energy (kg/m2) |
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C |
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REAL zairm(klon,klev) ! layer air mass (kg/m2) |
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REAL zqw_col(klon) |
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REAL zql_col(klon) |
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REAL zqs_col(klon) |
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REAL zec_col(klon) |
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REAL zh_dair_col(klon) |
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REAL zh_qw_col(klon), zh_ql_col(klon), zh_qs_col(klon) |
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C |
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REAL d_h_dair, d_h_qw, d_h_ql, d_h_qs |
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C |
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REAL airetot, zcpvap, zcwat, zcice |
|
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C |
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INTEGER i, k |
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C |
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INTEGER ndiag ! max number of diagnostic in parallel |
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PARAMETER (ndiag=10) |
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integer pas(ndiag) |
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save pas |
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data pas/ndiag*0/ |
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C |
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REAL h_vcol_pre(ndiag), h_dair_pre(ndiag), h_qw_pre(ndiag) |
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$ , h_ql_pre(ndiag), h_qs_pre(ndiag), qw_pre(ndiag) |
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$ , ql_pre(ndiag), qs_pre(ndiag) , ec_pre(ndiag) |
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SAVE h_vcol_pre, h_dair_pre, h_qw_pre, h_ql_pre |
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$ , h_qs_pre, qw_pre, ql_pre, qs_pre , ec_pre |
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c====================================================================== |
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C |
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DO k = 1, klev |
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DO i = 1, klon |
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C layer air mass |
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zairm(i,k) = (paprs(i,k)-paprs(i,k+1))/RG |
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ENDDO |
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END DO |
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C |
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C Reset variables |
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DO i = 1, klon |
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zqw_col(i)=0. |
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zql_col(i)=0. |
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zqs_col(i)=0. |
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zec_col(i) = 0. |
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zh_dair_col(i) = 0. |
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zh_qw_col(i) = 0. |
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zh_ql_col(i) = 0. |
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zh_qs_col(i) = 0. |
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ENDDO |
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C |
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zcpvap=RCPV |
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zcwat=RCW |
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zcice=RCS |
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C |
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C Compute vertical sum for each atmospheric column |
|
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C ================================================ |
|
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DO k = 1, klev |
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DO i = 1, klon |
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C Watter mass |
|
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zqw_col(i) = zqw_col(i) + q(i,k)*zairm(i,k) |
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zql_col(i) = zql_col(i) + ql(i,k)*zairm(i,k) |
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zqs_col(i) = zqs_col(i) + qs(i,k)*zairm(i,k) |
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C Cinetic Energy |
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zec_col(i) = zec_col(i) |
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$ +0.5*(u(i,k)**2+v(i,k)**2)*zairm(i,k) |
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C Air enthalpy |
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zh_dair_col(i) = zh_dair_col(i) |
|
|
$ + RCPD*(1.-q(i,k)-ql(i,k)-qs(i,k))*zairm(i,k)*t(i,k) |
|
|
zh_qw_col(i) = zh_qw_col(i) |
|
|
$ + zcpvap*q(i,k)*zairm(i,k)*t(i,k) |
|
|
zh_ql_col(i) = zh_ql_col(i) |
|
|
$ + zcwat*ql(i,k)*zairm(i,k)*t(i,k) |
|
|
$ - RLVTT*ql(i,k)*zairm(i,k) |
|
|
zh_qs_col(i) = zh_qs_col(i) |
|
|
$ + zcice*qs(i,k)*zairm(i,k)*t(i,k) |
|
|
$ - RLSTT*qs(i,k)*zairm(i,k) |
|
|
|
|
|
END DO |
|
|
ENDDO |
|
|
C |
|
|
C Mean over the planete surface |
|
|
C ============================= |
|
|
qw_tot = 0. |
|
|
ql_tot = 0. |
|
|
qs_tot = 0. |
|
|
ec_tot = 0. |
|
|
h_vcol_tot = 0. |
|
|
h_dair_tot = 0. |
|
|
h_qw_tot = 0. |
|
|
h_ql_tot = 0. |
|
|
h_qs_tot = 0. |
|
|
airetot=0. |
|
|
C |
|
|
do i=1,klon |
|
|
qw_tot = qw_tot + zqw_col(i)*airephy(i) |
|
|
ql_tot = ql_tot + zql_col(i)*airephy(i) |
|
|
qs_tot = qs_tot + zqs_col(i)*airephy(i) |
|
|
ec_tot = ec_tot + zec_col(i)*airephy(i) |
|
|
h_dair_tot = h_dair_tot + zh_dair_col(i)*airephy(i) |
|
|
h_qw_tot = h_qw_tot + zh_qw_col(i)*airephy(i) |
|
|
h_ql_tot = h_ql_tot + zh_ql_col(i)*airephy(i) |
|
|
h_qs_tot = h_qs_tot + zh_qs_col(i)*airephy(i) |
|
|
airetot=airetot+airephy(i) |
|
|
END DO |
|
|
C |
|
|
qw_tot = qw_tot/airetot |
|
|
ql_tot = ql_tot/airetot |
|
|
qs_tot = qs_tot/airetot |
|
|
ec_tot = ec_tot/airetot |
|
|
h_dair_tot = h_dair_tot/airetot |
|
|
h_qw_tot = h_qw_tot/airetot |
|
|
h_ql_tot = h_ql_tot/airetot |
|
|
h_qs_tot = h_qs_tot/airetot |
|
|
C |
|
|
h_vcol_tot = h_dair_tot+h_qw_tot+h_ql_tot+h_qs_tot |
|
|
C |
|
|
C Compute the change of the atmospheric state compare to the one |
|
|
C stored in "idiag2", and convert it in flux. THis computation |
|
|
C is performed IF idiag2 /= 0 and IF it is not the first CALL |
|
|
c for "idiag" |
|
|
C =================================== |
|
|
C |
|
|
IF ( (idiag2.gt.0) .and. (pas(idiag2) .ne. 0) ) THEN |
|
|
d_h_vcol = (h_vcol_tot - h_vcol_pre(idiag2) )/dtime |
|
|
d_h_dair = (h_dair_tot- h_dair_pre(idiag2))/dtime |
|
|
d_h_qw = (h_qw_tot - h_qw_pre(idiag2) )/dtime |
|
|
d_h_ql = (h_ql_tot - h_ql_pre(idiag2) )/dtime |
|
|
d_h_qs = (h_qs_tot - h_qs_pre(idiag2) )/dtime |
|
|
d_qw = (qw_tot - qw_pre(idiag2) )/dtime |
|
|
d_ql = (ql_tot - ql_pre(idiag2) )/dtime |
|
|
d_qs = (qs_tot - qs_pre(idiag2) )/dtime |
|
|
d_ec = (ec_tot - ec_pre(idiag2) )/dtime |
|
|
d_qt = d_qw + d_ql + d_qs |
|
|
ELSE |
|
|
d_h_vcol = 0. |
|
|
d_h_dair = 0. |
|
|
d_h_qw = 0. |
|
|
d_h_ql = 0. |
|
|
d_h_qs = 0. |
|
|
d_qw = 0. |
|
|
d_ql = 0. |
|
|
d_qs = 0. |
|
|
d_ec = 0. |
|
|
d_qt = 0. |
|
|
ENDIF |
|
|
C |
|
|
IF (iprt.ge.2) THEN |
|
|
WRITE(6,9000) tit,pas(idiag),d_qt,d_qw,d_ql,d_qs |
|
|
9000 format('Phys. Watter Mass Budget (kg/m2/s)',A15 |
|
|
$ ,1i6,10(1pE14.6)) |
|
|
WRITE(6,9001) tit,pas(idiag), d_h_vcol |
|
|
9001 format('Phys. Enthalpy Budget (W/m2) ',A15,1i6,10(F8.2)) |
|
|
WRITE(6,9002) tit,pas(idiag), d_ec |
|
|
9002 format('Phys. Cinetic Energy Budget (W/m2) ',A15,1i6,10(F8.2)) |
|
|
END IF |
|
|
C |
|
|
C Store the new atmospheric state in "idiag" |
|
|
C |
|
|
pas(idiag)=pas(idiag)+1 |
|
|
h_vcol_pre(idiag) = h_vcol_tot |
|
|
h_dair_pre(idiag) = h_dair_tot |
|
|
h_qw_pre(idiag) = h_qw_tot |
|
|
h_ql_pre(idiag) = h_ql_tot |
|
|
h_qs_pre(idiag) = h_qs_tot |
|
|
qw_pre(idiag) = qw_tot |
|
|
ql_pre(idiag) = ql_tot |
|
|
qs_pre(idiag) = qs_tot |
|
|
ec_pre (idiag) = ec_tot |
|
|
C |
|
|
RETURN |
|
|
END |
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