Directory: | ./ |
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File: | phys/thermcell_alim.f90 |
Date: | 2022-01-11 19:19:34 |
Exec | Total | Coverage | |
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Lines: | 18 | 50 | 36.0% |
Branches: | 19 | 60 | 31.7% |
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1 | ! | ||
2 | ! $Id: thermcell_plume.F90 2311 2015-06-25 07:45:24Z emillour $ | ||
3 | ! | ||
4 | 480 | SUBROUTINE thermcell_alim(flag,ngrid,klev,ztv,d_temp,zlev,alim_star,lalim) | |
5 | IMPLICIT NONE | ||
6 | |||
7 | !-------------------------------------------------------------------------- | ||
8 | ! FH : 2015/11/06 | ||
9 | ! thermcell_alim: calcule la distribution verticale de l'alimentation | ||
10 | ! laterale a la base des panaches thermiques | ||
11 | !-------------------------------------------------------------------------- | ||
12 | |||
13 | ! | ||
14 | ! $Header$ | ||
15 | ! | ||
16 | ! ATTENTION!!!!: ce fichier include est compatible format fixe/format libre | ||
17 | ! veillez � n'utiliser que des ! pour les commentaires | ||
18 | ! et � bien positionner les & des lignes de continuation | ||
19 | ! (les placer en colonne 6 et en colonne 73) | ||
20 | ! | ||
21 | ! | ||
22 | ! A1.0 Fundamental constants | ||
23 | REAL RPI,RCLUM,RHPLA,RKBOL,RNAVO | ||
24 | ! A1.1 Astronomical constants | ||
25 | REAL RDAY,REA,REPSM,RSIYEA,RSIDAY,ROMEGA | ||
26 | ! A1.1.bis Constantes concernant l'orbite de la Terre: | ||
27 | REAL R_ecc, R_peri, R_incl | ||
28 | ! A1.2 Geoide | ||
29 | REAL RA,RG,R1SA | ||
30 | ! A1.3 Radiation | ||
31 | ! REAL RSIGMA,RI0 | ||
32 | REAL RSIGMA | ||
33 | ! A1.4 Thermodynamic gas phase | ||
34 | REAL RMO3,RMCO2,RMC,RMCH4,RMN2O,RMCFC11,RMCFC12 | ||
35 | REAL R,RMD,RMV,RD,RV,RCPD,RCPV,RCVD,RCVV | ||
36 | REAL RKAPPA,RETV, eps_w | ||
37 | ! A1.5,6 Thermodynamic liquid,solid phases | ||
38 | REAL RCW,RCS | ||
39 | ! A1.7 Thermodynamic transition of phase | ||
40 | REAL RLVTT,RLSTT,RLMLT,RTT,RATM | ||
41 | ! A1.8 Curve of saturation | ||
42 | REAL RESTT,RALPW,RBETW,RGAMW,RALPS,RBETS,RGAMS | ||
43 | REAL RALPD,RBETD,RGAMD | ||
44 | ! | ||
45 | COMMON/YOMCST/RPI ,RCLUM ,RHPLA ,RKBOL ,RNAVO & | ||
46 | & ,RDAY ,REA ,REPSM ,RSIYEA,RSIDAY,ROMEGA & | ||
47 | & ,R_ecc, R_peri, R_incl & | ||
48 | & ,RA ,RG ,R1SA & | ||
49 | & ,RSIGMA & | ||
50 | & ,R ,RMD ,RMV ,RD ,RV ,RCPD & | ||
51 | & ,RMO3 ,RMCO2 ,RMC ,RMCH4 ,RMN2O ,RMCFC11 ,RMCFC12 & | ||
52 | & ,RCPV ,RCVD ,RCVV ,RKAPPA,RETV, eps_w & | ||
53 | & ,RCW ,RCS & | ||
54 | & ,RLVTT ,RLSTT ,RLMLT ,RTT ,RATM & | ||
55 | & ,RESTT ,RALPW ,RBETW ,RGAMW ,RALPS ,RBETS ,RGAMS & | ||
56 | & ,RALPD ,RBETD ,RGAMD | ||
57 | ! ------------------------------------------------------------------ | ||
58 | !$OMP THREADPRIVATE(/YOMCST/) | ||
59 | ! | ||
60 | ! $Id: YOETHF.h 2799 2017-02-24 18:50:33Z jyg $ | ||
61 | ! | ||
62 | ! ATTENTION!!!!: ce fichier include est compatible format fixe/format libre | ||
63 | ! veillez n'utiliser que des ! pour les commentaires | ||
64 | ! et bien positionner les & des lignes de continuation | ||
65 | ! (les placer en colonne 6 et en colonne 73) | ||
66 | ! | ||
67 | !* COMMON *YOETHF* DERIVED CONSTANTS SPECIFIC TO ECMWF THERMODYNAMICS | ||
68 | ! | ||
69 | ! *R__ES* *CONSTANTS USED FOR COMPUTATION OF SATURATION | ||
70 | ! MIXING RATIO OVER LIQUID WATER(*R_LES*) OR | ||
71 | ! ICE(*R_IES*). | ||
72 | ! *RVTMP2* *RVTMP2=RCPV/RCPD-1. | ||
73 | ! *RHOH2O* *DENSITY OF LIQUID WATER. (RATM/100.) | ||
74 | ! | ||
75 | REAL R2ES, R3LES, R3IES, R4LES, R4IES, R5LES, R5IES | ||
76 | REAL RVTMP2, RHOH2O | ||
77 | REAL R5ALVCP,R5ALSCP,RALVDCP,RALSDCP,RALFDCP,RTWAT,RTBER,RTBERCU | ||
78 | REAL RTICE,RTICECU,RTWAT_RTICE_R,RTWAT_RTICECU_R,RKOOP1,RKOOP2 | ||
79 | LOGICAL OK_BAD_ECMWF_THERMO ! If TRUE, then variables set by rrtm/suphec.F90 | ||
80 | ! If FALSE, then variables set by suphel.F90 | ||
81 | COMMON /YOETHF/R2ES, R3LES, R3IES, R4LES, R4IES, R5LES, R5IES, & | ||
82 | & RVTMP2, RHOH2O, & | ||
83 | & R5ALVCP,R5ALSCP,RALVDCP,RALSDCP, & | ||
84 | & RALFDCP,RTWAT,RTBER,RTBERCU, & | ||
85 | & RTICE,RTICECU,RTWAT_RTICE_R,RTWAT_RTICECU_R,RKOOP1,& | ||
86 | & RKOOP2, & | ||
87 | & OK_BAD_ECMWF_THERMO | ||
88 | |||
89 | !$OMP THREADPRIVATE(/YOETHF/) | ||
90 | ! | ||
91 | ! $Header$ | ||
92 | ! | ||
93 | ! | ||
94 | ! ATTENTION!!!!: ce fichier include est compatible format fixe/format libre | ||
95 | ! veillez n'utiliser que des ! pour les commentaires | ||
96 | ! et bien positionner les & des lignes de continuation | ||
97 | ! (les placer en colonne 6 et en colonne 73) | ||
98 | ! | ||
99 | ! ------------------------------------------------------------------ | ||
100 | ! This COMDECK includes the Thermodynamical functions for the cy39 | ||
101 | ! ECMWF Physics package. | ||
102 | ! Consistent with YOMCST Basic physics constants, assuming the | ||
103 | ! partial pressure of water vapour is given by a first order | ||
104 | ! Taylor expansion of Qs(T) w.r.t. to Temperature, using constants | ||
105 | ! in YOETHF | ||
106 | ! ------------------------------------------------------------------ | ||
107 | REAL PTARG, PDELARG, P5ARG, PQSARG, PCOARG | ||
108 | REAL FOEEW, FOEDE, qsats, qsatl, dqsats, dqsatl | ||
109 | LOGICAL thermcep | ||
110 | PARAMETER (thermcep=.TRUE.) | ||
111 | ! | ||
112 | FOEEW ( PTARG,PDELARG ) = EXP ( & | ||
113 | & (R3LES*(1.-PDELARG)+R3IES*PDELARG) * (PTARG-RTT) & | ||
114 | & / (PTARG-(R4LES*(1.-PDELARG)+R4IES*PDELARG)) ) | ||
115 | ! | ||
116 | FOEDE ( PTARG,PDELARG,P5ARG,PQSARG,PCOARG ) = PQSARG*PCOARG*P5ARG & | ||
117 | & / (PTARG-(R4LES*(1.-PDELARG)+R4IES*PDELARG))**2 | ||
118 | ! | ||
119 | qsats(ptarg) = 100.0 * 0.622 * 10.0 & | ||
120 | & ** (2.07023 - 0.00320991 * ptarg & | ||
121 | & - 2484.896 / ptarg + 3.56654 * LOG10(ptarg)) | ||
122 | qsatl(ptarg) = 100.0 * 0.622 * 10.0 & | ||
123 | & ** (23.8319 - 2948.964 / ptarg & | ||
124 | & - 5.028 * LOG10(ptarg) & | ||
125 | & - 29810.16 * EXP( - 0.0699382 * ptarg) & | ||
126 | & + 25.21935 * EXP( - 2999.924 / ptarg)) | ||
127 | ! | ||
128 | dqsats(ptarg,pqsarg) = RLVTT/RCPD*pqsarg * (3.56654/ptarg & | ||
129 | & +2484.896*LOG(10.)/ptarg**2 & | ||
130 | & -0.00320991*LOG(10.)) | ||
131 | dqsatl(ptarg,pqsarg) = RLVTT/RCPD*pqsarg*LOG(10.)* & | ||
132 | & (2948.964/ptarg**2-5.028/LOG(10.)/ptarg & | ||
133 | & +25.21935*2999.924/ptarg**2*EXP(-2999.924/ptarg) & | ||
134 | & +29810.16*0.0699382*EXP(-0.0699382*ptarg)) | ||
135 | integer :: iflag_thermals,nsplit_thermals | ||
136 | |||
137 | !!! nrlmd le 10/04/2012 | ||
138 | integer :: iflag_trig_bl,iflag_clos_bl | ||
139 | integer :: tau_trig_shallow,tau_trig_deep | ||
140 | real :: s_trig | ||
141 | !!! fin nrlmd le 10/04/2012 | ||
142 | |||
143 | real,parameter :: r_aspect_thermals=2.,l_mix_thermals=30. | ||
144 | real :: alp_bl_k | ||
145 | real :: tau_thermals,fact_thermals_ed_dz | ||
146 | integer,parameter :: w2di_thermals=0 | ||
147 | integer :: isplit | ||
148 | |||
149 | integer :: iflag_coupl,iflag_clos,iflag_wake | ||
150 | integer :: iflag_thermals_ed,iflag_thermals_optflux,iflag_thermals_closure | ||
151 | |||
152 | common/ctherm1/iflag_thermals,nsplit_thermals,iflag_thermals_closure | ||
153 | common/ctherm2/tau_thermals,alp_bl_k,fact_thermals_ed_dz | ||
154 | common/ctherm4/iflag_coupl,iflag_clos,iflag_wake | ||
155 | common/ctherm5/iflag_thermals_ed,iflag_thermals_optflux | ||
156 | |||
157 | !!! nrlmd le 10/04/2012 | ||
158 | common/ctherm6/iflag_trig_bl,iflag_clos_bl | ||
159 | common/ctherm7/tau_trig_shallow,tau_trig_deep | ||
160 | common/ctherm8/s_trig | ||
161 | !!! fin nrlmd le 10/04/2012 | ||
162 | |||
163 | !$OMP THREADPRIVATE(/ctherm1/,/ctherm2/,/ctherm4/,/ctherm5/) | ||
164 | !$OMP THREADPRIVATE(/ctherm6/,/ctherm7/,/ctherm8/) | ||
165 | |||
166 | ! fort(10) ptimestep,ztv,zthl,po,zl,rhobarz,zlev,pplev,pphi,zpspsk,f0 | ||
167 | INTEGER, INTENT(IN) :: ngrid,klev | ||
168 | REAL, INTENT(IN) :: ztv(ngrid,klev) | ||
169 | REAL, INTENT(IN) :: d_temp(ngrid) | ||
170 | REAL, INTENT(IN) :: zlev(ngrid,klev+1) | ||
171 | REAL, INTENT(OUT) :: alim_star(ngrid,klev) | ||
172 | INTEGER, INTENT(OUT) :: lalim(ngrid) | ||
173 | INTEGER, INTENT(IN) :: flag | ||
174 | |||
175 | 960 | REAL :: alim_star_tot(ngrid),zi(ngrid),zh(ngrid) | |
176 | 480 | REAL :: zlay(ngrid,klev) | |
177 | REAL ztv_parcel | ||
178 | |||
179 | INTEGER ig,l | ||
180 | |||
181 | REAL h,z,falim | ||
182 | falim(h,z)=0.2*((z-h)**5+h**5) | ||
183 | |||
184 | |||
185 | !=================================================================== | ||
186 | |||
187 |
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477600 | lalim(:)=1 |
188 |
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477600 | alim_star_tot(:)=0. |
189 | |||
190 | !------------------------------------------------------------------------- | ||
191 | ! Definition de l'alimentation a l'origine dans thermcell_init | ||
192 | !------------------------------------------------------------------------- | ||
193 |
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480 | IF (flag==0) THEN ! CMIP5 version |
194 |
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18720 | do l=1,klev-1 |
195 |
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18149280 | do ig=1,ngrid |
196 |
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18148800 | if (ztv(ig,l)> ztv(ig,l+1) .and. ztv(ig,1)>=ztv(ig,l) ) then |
197 | alim_star(ig,l)=MAX((ztv(ig,l)-ztv(ig,l+1)),0.) & | ||
198 | 606965 | & *sqrt(zlev(ig,l+1)) | |
199 | 606965 | lalim(ig)=l+1 | |
200 | 606965 | alim_star_tot(ig)=alim_star_tot(ig)+alim_star(ig,l) | |
201 | endif | ||
202 | enddo | ||
203 | enddo | ||
204 |
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19200 | do l=1,klev |
205 |
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18626400 | if (alim_star_tot(ig) > 1.e-10 ) then |
207 | 9688770 | alim_star(ig,l)=alim_star(ig,l)/alim_star_tot(ig) | |
208 | endif | ||
209 | enddo | ||
210 | enddo | ||
211 | 480 | alim_star_tot(:)=1. | |
212 | |||
213 | !------------------------------------------------------------------------- | ||
214 | ! Nouvelle definition avec possibilite d'introduire un DT en surface | ||
215 | ! On suppose que la forme du profile d'alimentation scale avec la hauteur | ||
216 | ! d'inversion calculée avec une particule partant de la premieere couche | ||
217 | |||
218 | ! Fonction f(z) = z ( h - z ) , avec h = zi/3 | ||
219 | ! On utilise l'integralle | ||
220 | ! Int_0^z f(z') dz' = z^2 ( h/2 - z/3 ) = falim(h,z) | ||
221 | ! Pour calculer l'alimentation des couches | ||
222 | !------------------------------------------------------------------------- | ||
223 | ELSE | ||
224 | ! Computing inversion height zi and zh=zi/3. | ||
225 | ✗ | zi(:)=0. | |
226 | ! Il faut recalculer zlay qui n'est pas dispo dans thermcell_plume | ||
227 | ! A changer eventuellement. | ||
228 | ✗ | do l=1,klev | |
229 | ✗ | zlay(:,l)=0.5*(zlev(:,l)+zlev(:,l+1)) | |
230 | enddo | ||
231 | |||
232 | ✗ | do l=klev-1,1,-1 | |
233 | ✗ | do ig=1,ngrid | |
234 | ✗ | ztv_parcel=ztv(ig,1)+d_temp(ig) | |
235 | ✗ | if (ztv_parcel<ztv(ig,l+1)) lalim(ig)=l | |
236 | enddo | ||
237 | enddo | ||
238 | |||
239 | ✗ | do ig=1,ngrid | |
240 | ✗ | l=lalim(ig) | |
241 | ✗ | IF (l==1) THEN | |
242 | ✗ | zi(ig)=0. | |
243 | ELSE | ||
244 | ✗ | ztv_parcel=ztv(ig,1)+d_temp(ig) | |
245 | ✗ | zi(ig)=zlay(ig,l)+(zlay(ig,l+1)-zlay(ig,l))/(ztv(ig,l+1)-ztv(ig,l))*(ztv_parcel-ztv(ig,l)) | |
246 | ENDIF | ||
247 | enddo | ||
248 | |||
249 | ✗ | zh(:)=zi(:)/2. | |
250 | ✗ | alim_star_tot(:)=0. | |
251 | ✗ | alim_star(:,:)=0. | |
252 | ✗ | lalim(:)=0 | |
253 | ✗ | do l=1,klev-1 | |
254 | ✗ | do ig=1,ngrid | |
255 | ✗ | IF (zh(ig)==0.) THEN | |
256 | ✗ | alim_star(ig,l)=0. | |
257 | ✗ | lalim(ig)=1 | |
258 | ✗ | ELSE IF (zlev(ig,l+1)<=zh(ig)) THEN | |
259 | ✗ | alim_star(ig,l)=(falim(zh(ig),zlev(ig,l+1))-falim(zh(ig),zlev(ig,l)))/falim(zh(ig),zh(ig)) | |
260 | ✗ | lalim(ig)=l | |
261 | ✗ | ELSE IF (zlev(ig,l)<=zh(ig)) THEN | |
262 | ✗ | alim_star(ig,l)=(falim(zh(ig),zh(ig))-falim(zh(ig),zlev(ig,l)))/falim(zh(ig),zh(ig)) | |
263 | ✗ | lalim(ig)=l | |
264 | ELSE | ||
265 | ✗ | alim_star(ig,l)=0. | |
266 | ENDIF | ||
267 | ENDDO | ||
268 | ✗ | alim_star_tot(:)=alim_star_tot(:)+alim_star(:,l) | |
269 | ENDDO | ||
270 | ✗ | IF (ngrid==1) print*,'NEW ALIM CALCUL DE ZI ',alim_star_tot,lalim,zi,zh | |
271 | ✗ | alim_star_tot(:)=1. | |
272 | |||
273 | ENDIF | ||
274 | |||
275 | |||
276 | 480 | RETURN | |
277 | END | ||
278 |