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C$Header: $ |
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C$Name: $ |
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|
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#include "OPPS_OPTIONS.h" |
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|
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CBOP |
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C !ROUTINE: OPPS_CALC |
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|
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C !INTERFACE: ====================================================== |
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subroutine OPPS_CALC( |
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U tracerEnv, |
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I wVel, |
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I kMax, nTracer, nTracerInuse, |
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I I, J, bi, bj, myTime, myIter, myThid ) |
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|
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C !DESCRIPTION: \bv |
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C /=====================================================================\ |
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C | SUBROUTINE OPPS_CALC | |
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C | o Compute all OPPS fields defined in OPPS.h | |
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C |=====================================================================| |
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C | This subroutine is based on the routine 3dconvection.F | |
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C | by E. Skyllingstad (?) | |
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C | plenty of modifications to make it work: | |
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C | - removed many unused parameters and variables | |
25 |
C | - turned everything (back) into 1D code | |
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C | - pass variables, that are orginially in common blocks: | |
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C | maxDepth | |
28 |
C | - pass vertical velocity, set in OPPS_INTERFACE | |
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C | - do not use convadj for now (whatever that is) | |
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C | - changed two .LT. 0 to .LE. 0 statements (because of possible | |
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C | division) | |
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C | - replaced statement function state1 by call to a real function | |
33 |
C | - removed range check, actually moved it up to OPPS_INTERFACE | |
34 |
C | - avoid division by zero: if (Wd.EQ.0) dt = ...1/Wd | |
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C | - cleaned-up debugging | |
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C | - replaced local dz and GridThickness by global drF | |
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C | - replaced 1/dz by 1*recip_drF | |
38 |
C | - replaced 9.81 with gravity (=9.81) | |
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C | - added a lot of comments that relate code to equation in paper | |
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C | (Paluszkiewicz+Romea, 1997, Dynamics of Atmospheres and Oceans, | |
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C | 26, pp. 95-130) | |
42 |
C | - included passive tracer support. This is the main change and may | |
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C | not improve the readability of the code because of the joint | |
44 |
C | treatment of active (theta, salt) and passive tracers. The array | |
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C | tracerEnv(Nr,2+PTRACERS_num) contains | |
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C | theta = tracerEnv(:,1), | |
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C | salt = tracerEnv(:,2), and | |
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C | ptracers = tracerEnv(:,3:PTRACERS_num+2). | |
49 |
C | All related array names have been changed accordingly, so that | |
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C | instead of Sd(Nr) and Td(Nr) (plume salinity and temperature), we | |
51 |
C | have Pd(Nr,nTracer) (tracer in plume), with Sd(:) = Pd(:,2), | |
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C | Td(:) = Pd(:,1), etc. | |
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C | o TODO: | |
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C | clean up the logic of the vertical loops and get rid off the | |
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C | GOTO statements | |
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C \=====================================================================/ |
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IMPLICIT NONE |
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C |
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C-------------------------------------------------------------------- |
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|
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C \ev |
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|
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C !USES: ============================================================ |
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#include "SIZE.h" |
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#include "EEPARAMS.h" |
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#include "PARAMS.h" |
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#include "OPPS.h" |
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#include "FFIELDS.h" |
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#include "GRID.h" |
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|
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EXTERNAL DIFFERENT_MULTIPLE |
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LOGICAL DIFFERENT_MULTIPLE |
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|
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C !INPUT PARAMETERS: =================================================== |
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c Routine arguments |
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c bi, bj - array indices on which to apply calculations |
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c myTime - Current time in simulation |
78 |
|
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INTEGER I, J, bi, bj, KMax, nTracer, nTracerInUse |
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INTEGER myThid, myIter |
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_RL myTime |
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_RL tracerEnv(Nr,nTracer),wVel(Nr) |
83 |
|
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#ifdef ALLOW_OPPS |
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C !LOCAL VARIABLES: ==================================================== |
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c Local constants |
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C imin, imax, jmin, jmax - array computation indices |
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C msgBuf - Informational/error meesage buffer |
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CHARACTER*(MAX_LEN_MBUF) msgBuf |
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INTEGER K, K2, K2m1, K2p1, ktr |
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INTEGER ntime,nn,kmx,ic |
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INTEGER maxDepth |
93 |
|
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_RL wsqr,oldflux,newflux,entrainrate |
95 |
_RL pmix |
96 |
_RL D1,D2,state1 |
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_RL dz1,dz2 |
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_RL radius,StartingFlux |
99 |
_RL dtts,dt |
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C Arrays |
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_RL Paa(Nr,nTracer) |
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_RL wda(Nr), mda(Nr), pda(Nr,nTracer) |
103 |
C |
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C Pd, Wd - tracers, vertical velocity in plume |
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C Md - plume mass flux (?) |
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C Ad - fractional area covered by plume |
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C Dd - density in plume |
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C De - density of environment |
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C PlumeEntrainment - |
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_RL Ad(Nr),Wd(Nr),Dd(Nr),Md(Nr) |
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_RL De(Nr) |
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_RL PlumeEntrainment(Nr) |
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_RL Pd(Nr,nTracer) |
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CEOP |
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|
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|
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C-- Check to see if should convect now |
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C IF ( DIFFERENT_MULTIPLE(cAdjFreq,myTime,myTime-deltaTClock) ) THEN |
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IF ( .true. ) THEN |
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C local initialization |
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|
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C Copy some arrays |
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dtts = deltaTtracer |
124 |
C |
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C start k-loop |
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C |
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|
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DO k=1,KMax-1 |
129 |
c |
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c initialize the plume T,S,density, and w velocity |
131 |
c |
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DO ktr=1,nTracerInUse |
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Pd(k,ktr) = tracerEnv(k,ktr) |
134 |
ENDDO |
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Dd(k)=state1(Pd(k,2),Pd(k,1),i,j,k,bi,bj,myThid) |
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De(k)=Dd(k) |
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CML print *, 'ml-opps:', i,j,k,tracerEnv(k,2),tracerEnv(k,1), |
138 |
CML & Dd(k),Pd(k,1),Pd(k,2) |
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CML compute vertical velocity at cell centers from GCM velocity |
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Wd(k)= - .5*(wVel(K)+wVel(K+1)) |
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CML( |
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CML avoid division by zero |
143 |
CML IF (Wd(K) .EQ. 0.D0) Wd(K) = 2.23e-16 |
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CML) |
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c |
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c guess at initial top grid cell vertical velocity |
147 |
c |
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CML Wd(k) = 0.03 |
149 |
c |
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c these estimates of initial plume velocity based on plume size and |
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c top grid cell water mass |
152 |
c |
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c Wd(k) = 0.5*drF(k)/(dtts*FRACTIONAL_AREA) |
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c Wd(k) = 0.5*drF(k)/dtts |
155 |
c |
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wsqr=Wd(k)*Wd(k) |
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PlumeEntrainment(k) = 0.0 |
158 |
c |
159 |
c |
160 |
c |
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#ifdef ALLOW_OPPS_DEBUG |
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IF ( OPPSdebugLevel.GE.debLevB ) THEN |
163 |
WRITE(msgBuf,'(A,I3)') |
164 |
& 'S/R OPPS_CALC: doing old lowerparcel', k |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
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ENDIF |
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#endif /* ALLOW_OPPS_DEBUG */ |
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radius=PlumeRadius |
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StartingFlux=radius*radius*Wd(k)*Dd(k) |
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oldflux=StartingFlux |
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|
173 |
dz2=DrF(k) |
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DO k2=k,KMax-1 |
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D1=state1( Pd(k2,2), Pd(k2,1),i,j,k2+1,bi,bj,myThid) |
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D2=state1( tracerEnv(k2+1,2), tracerEnv(k2+1,1), |
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& i,j,k2+1,bi,bj,myThid) |
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De(k2+1)=D2 |
179 |
c |
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c To start downward, parcel has to initially be heavier than environment |
181 |
c but after it has started moving, we continue plume until plume tke or |
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c flux goes negative |
183 |
c |
184 |
CML & _hFacC(i,j,k-1,bi,bj) |
185 |
CML & *_hFacC(i,j,k,bi,bj) .GT. 0. |
186 |
CML & .AND. |
187 |
IF (D2-D1 .LT. STABILITY_THRESHOLD.or.k2.ne.k) THEN |
188 |
dz1=dz2 |
189 |
dz2=DrF(k2+1) |
190 |
c |
191 |
C find mass flux according to eq.(3) from paper by vertical integration |
192 |
c |
193 |
newflux=oldflux+e2*radius*Wd(k2)*Dd(k2)* |
194 |
& .5*(dz1+dz2) |
195 |
CML print *, 'ml-opps:', i,j,k,oldflux,newflux,e2,radius, |
196 |
CML & Wd(k2),Dd(k2),Pd(k2,1),Pd(k2,2),dz1,dz2 |
197 |
c |
198 |
PlumeEntrainment(k2+1) = newflux/StartingFlux |
199 |
c |
200 |
IF(newflux.LE.0.0) then |
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#ifdef ALLOW_OPPS_DEBUG |
202 |
IF ( OPPSdebugLevel.GE.debLevA ) THEN |
203 |
WRITE(msgBuf,'(A,I3)') |
204 |
& 'S/R OPPS_CALC: Plume entrained to zero at level ', k2 |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
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ENDIF |
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#endif /* ALLOW_OPPS_DEBUG */ |
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maxdepth = k2 |
210 |
if(maxdepth.eq.k) goto 1000 |
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goto 1 |
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endif |
213 |
c |
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c entrainment rate is basically a scaled mass flux dM/M |
215 |
c |
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entrainrate = (newflux - oldflux)/newflux |
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oldflux = newflux |
218 |
c |
219 |
c |
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c mix var's are the average environmental values over the two grid levels |
221 |
c |
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DO ktr=1,nTracerInUse |
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pmix=(dz1*tracerEnv(k2,ktr)+dz2*tracerEnv(k2+1,ktr)) |
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& /(dz1+dz2) |
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Pd(k2+1,ktr)=Pd(k2,ktr) |
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& - entrainrate*(pmix - Pd(k2,ktr)) |
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ENDDO |
228 |
c |
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c compute the density at this level for the buoyancy term in the |
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c vertical k.e. equation |
231 |
c |
232 |
Dd(k2+1)=state1(Pd(k2+1,2),Pd(k2+1,1),i,j,k2+1,bi,bj,myThid) |
233 |
c |
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c next, solve for the vertical velocity k.e. using combined eq. (4) |
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c and eq (5) from the paper |
236 |
c |
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#ifdef ALLOW_OPPS_DEBUG |
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IF ( OPPSdebugLevel.GE.debLevA ) THEN |
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WRITE(msgBuf,'(A,3E12.4,I3)') |
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& 'S/R OPPS_CALC: Dd,De,entr,k ',Dd(k2),De(k2),entrainrate,k2 |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
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ENDIF |
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#endif /* ALLOW_OPPS_DEBUG */ |
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CML insert Eq. (4) into Eq. (5) to get something like this for wp^2 |
246 |
wsqr = wsqr - wsqr*abs(entrainrate)+ gravity* |
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& (dz1*(Dd(k2)-De(k2))/De(k2) |
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& +dz2*(Dd(k2+1)-De(k2+1))/De(k2+1)) |
249 |
c |
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c if negative k.e. then plume has reached max depth, get out of loop |
251 |
c |
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IF(wsqr.LE.0.0)then |
253 |
maxdepth = k2 |
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#ifdef ALLOW_OPPS_DEBUG |
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IF ( OPPSdebugLevel.GE.debLevA ) THEN |
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WRITE(msgBuf,'(A,I3)') |
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& 'S/R OPPS_CALC: Plume velocity went to zero at level ', k2 |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
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WRITE(msgBuf,'(A,4A14)') |
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& 'S/R OPPS_CALC: ', 'wsqr', 'entrainrate', |
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& '(Dd-De)/De up', '(Dd-De)/De do' |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
265 |
WRITE(msgBuf,'(A,4E14.6)') |
266 |
& 'S/R OPPS_CALC: ', wsqr, entrainrate, |
267 |
& (Dd(k2)-De(k2))/De(k2), (Dd(k2+1)-De(k2+1))/De(k2+1) |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
269 |
& SQUEEZE_RIGHT , 1) |
270 |
ENDIF |
271 |
#endif /* ALLOW_OPPS_DEBUG */ |
272 |
if(maxdepth.eq.k) goto 1000 |
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goto 1 |
274 |
endif |
275 |
Wd(k2+1)=sqrt(wsqr) |
276 |
C |
277 |
C compute a new radius based on the new mass flux at this grid level |
278 |
C from Eq. (4) |
279 |
C |
280 |
radius=sqrt(newflux/(Wd(k2)*Dd(k2))) |
281 |
ELSE |
282 |
maxdepth=k2 |
283 |
if(maxdepth.eq.k) goto 1000 |
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GOTO 1 |
285 |
ENDIF |
286 |
ENDDO |
287 |
c |
288 |
c plume has reached the bottom |
289 |
c |
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MaxDepth=kMax |
291 |
c |
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1 CONTINUE |
293 |
c |
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Ad(k)=FRACTIONAL_AREA |
295 |
IC=0 |
296 |
c |
297 |
c start iteration on fractional area, not used in OGCM implementation |
298 |
c |
299 |
c |
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DO IC=1,Max_ABE_Iterations |
301 |
c |
302 |
c |
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c next compute the mass flux beteen each grid box using the entrainment |
304 |
c |
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Md(k)=Wd(k)*Ad(k) |
306 |
c |
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DO k2=k+1,maxDepth |
308 |
Md(k2)=Md(k)*PlumeEntrainment(k2) |
309 |
#ifdef ALLOW_OPPS_DEBUG |
310 |
IF ( OPPSdebugLevel.GE.debLevA ) THEN |
311 |
WRITE(msgBuf,'(A,2E12.4,I3)') |
312 |
& 'S/R OPPS_CALC: Md, Wd, and k are ',Md(k2),Wd(k2),k2 |
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CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
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& SQUEEZE_RIGHT , 1) |
315 |
ENDIF |
316 |
#endif /* ALLOW_OPPS_DEBUG */ |
317 |
ENDDO |
318 |
c |
319 |
c Now move on to calculate new temperature using flux from |
320 |
c Td, Sd, Wd, ta, sa, and we. Values for these variables are at |
321 |
c center of grid cell, use weighted average to get boundary values |
322 |
c |
323 |
c use a timestep limited by the GCM model timestep and the maximum plume |
324 |
c velocity (CFL criteria) |
325 |
c |
326 |
c |
327 |
c calculate the weighted wd, td, and sd |
328 |
c |
329 |
dt = dtts |
330 |
do k2=k,maxDepth-1 |
331 |
IF ( Wd(K2) .NE. 0. _d 0 ) dt = min(dt,drF(k2)/Wd(k2)) |
332 |
c |
333 |
c time integration will be integer number of steps to get one |
334 |
c gcm time step |
335 |
c |
336 |
ntime = nint(0.5*int(dtts/dt)) |
337 |
if(ntime.eq.0) then |
338 |
ntime = 1 |
339 |
endif |
340 |
c |
341 |
c make sure area weighted vertical velocities match; in other words |
342 |
c make sure mass in equals mass out at the intersection of each grid |
343 |
c cell. Eq. (20) |
344 |
c |
345 |
mda(k2) = (md(k2)*drF(k2)+md(k2+1)*drF(k2+1))/ |
346 |
* (drF(k2)+drF(k2+1)) |
347 |
c |
348 |
wda(k2) = (wd(k2)*drF(k2)+wd(k2+1)*drF(k2+1))/ |
349 |
* (drF(k2)+drF(k2+1)) |
350 |
c |
351 |
DO ktr = 1, nTracerInUse |
352 |
Pda(k2,ktr) = Pd(k2,ktr) |
353 |
Paa(k2,ktr) = tracerEnv(k2+1,ktr) |
354 |
ENDDO |
355 |
c |
356 |
enddo |
357 |
dt = min(dt,dtts) |
358 |
#ifdef ALLOW_OPPS_DEBUG |
359 |
IF ( OPPSdebugLevel.GE.debLevA ) THEN |
360 |
WRITE(msgBuf,'(A,F14.4)') |
361 |
& 'S/R OPPS_CALC: time step = ', dt |
362 |
CALL PRINT_MESSAGE( msgBuf, standardMessageUnit, |
363 |
& SQUEEZE_RIGHT , 1) |
364 |
ENDIF |
365 |
#endif /* ALLOW_OPPS_DEBUG */ |
366 |
DO ktr=1,nTracerInUse |
367 |
Pda(maxdepth,ktr) = Pd(maxdepth,ktr) |
368 |
ENDDO |
369 |
C |
370 |
kmx = maxdepth-1 |
371 |
do nn=1,ntime |
372 |
C |
373 |
C top point |
374 |
C |
375 |
DO ktr = 1,nTracerInUse |
376 |
tracerEnv(k,ktr) = tracerEnv(k,ktr)- |
377 |
& (mda(k)*(Pda(k,ktr)-Paa(k,ktr)))*dt*recip_drF(k) |
378 |
ENDDO |
379 |
c |
380 |
c now do inner points if there are any |
381 |
c |
382 |
CML if(Maxdepth-k.gt.1) then |
383 |
CML This if statement is superfluous |
384 |
CML IF ( k .LT. Maxdepth-1 ) THEN |
385 |
CML DO k2=k+1,Maxdepth-1 |
386 |
CML mda(maxDepth) = 0. |
387 |
DO k2=k+1,kmx |
388 |
k2m1 = max(k,k2-1) |
389 |
k2p1 = max(k2+1,maxDepth) |
390 |
c |
391 |
DO ktr = 1,nTracerInUse |
392 |
tracerEnv(k2,ktr) = tracerEnv(k2,ktr) + |
393 |
& (mda(k2m1)*(Pda(k2m1,ktr)-Paa(k2m1,ktr)) |
394 |
& -mda(k2) *(Pda(k2,ktr) -Paa(k2,ktr)) ) |
395 |
& *dt*recip_drF(k2) |
396 |
ENDDO |
397 |
ENDDO |
398 |
CML This if statement is superfluous |
399 |
CML ENDIF |
400 |
C |
401 |
C bottom point |
402 |
C |
403 |
DO ktr=1,nTracerInUse |
404 |
tracerEnv(kmx+1,ktr) = tracerEnv(kmx+1,ktr)+ |
405 |
& mda(kmx)*(Pda(kmx,ktr)-Paa(kmx,ktr))*dt*recip_drF(kmx+1) |
406 |
ENDDO |
407 |
c |
408 |
c set the environmental temp and salinity to equal new fields |
409 |
c |
410 |
DO ktr=1,nTracerInUse |
411 |
DO k2=1,kmx |
412 |
paa(k2,ktr) = tracerEnv(k2+1,ktr) |
413 |
ENDDO |
414 |
ENDDO |
415 |
c |
416 |
c end loop on number of time integration steps |
417 |
c |
418 |
enddo |
419 |
ENDDO |
420 |
999 continue |
421 |
C |
422 |
C count convection event in this grid cell |
423 |
C |
424 |
OPPSconvectCount(I,J,K,bi,bj) = |
425 |
& OPPSconvectCount(I,J,K,bi,bj) + 1. _d 0 |
426 |
C |
427 |
C jump here if k = maxdepth or if level not unstable, go to next |
428 |
C profile point |
429 |
C |
430 |
1000 continue |
431 |
c |
432 |
C |
433 |
C end of k-loop |
434 |
C |
435 |
ENDDO |
436 |
|
437 |
C-- End IF (DIFFERENT_MULTIPLE) |
438 |
ENDIF |
439 |
|
440 |
RETURN |
441 |
END |
442 |
_RL FUNCTION STATE1(sLoc,tLoc,I,J,KREF,bi,bj,mythid) |
443 |
C !DESCRIPTION: \bv |
444 |
C *===============================================================* |
445 |
C | o SUBROUTINE STATE1 |
446 |
C | Calculates rho(S,T,p) |
447 |
C | It is absolutely necessary to compute |
448 |
C | the full rho and not sigma=rho-rhoConst, because |
449 |
C | density is used as a scale factor for fluxes and velocities |
450 |
C *===============================================================* |
451 |
C \ev |
452 |
|
453 |
C !USES: |
454 |
IMPLICIT NONE |
455 |
C == Global variables == |
456 |
#include "SIZE.h" |
457 |
#include "EEPARAMS.h" |
458 |
#include "PARAMS.h" |
459 |
#include "EOS.h" |
460 |
#include "GRID.h" |
461 |
#include "DYNVARS.h" |
462 |
|
463 |
C !INPUT/OUTPUT PARAMETERS: |
464 |
C == Routine arguments == |
465 |
INTEGER I,J,kRef,bi,bj,myThid |
466 |
_RL tLoc,sLoc |
467 |
|
468 |
C !LOCAL VARIABLES: |
469 |
C == Local variables == |
470 |
_RL rhoLoc, dRho |
471 |
_RL pLoc |
472 |
_RL t1, t2, t3, t4, s1, s3o2, p1, p2, sp5, p1t1 |
473 |
_RL rfresh, rsalt, rhoP0 |
474 |
_RL bMfresh, bMsalt, bMpres, BulkMod |
475 |
_RL rhoNum, rhoDen, den, epsln |
476 |
PARAMETER ( epsln = 0.D0 ) |
477 |
|
478 |
character*(max_len_mbuf) msgbuf |
479 |
|
480 |
CMLC estimate pressure from depth at cell centers |
481 |
CML mtoSI = gravity*rhoConst |
482 |
CML pLoc = ABS(rC(kRef))*mtoSI |
483 |
|
484 |
IF ( buoyancyRelation .EQ. 'OCEANIC' ) THEN |
485 |
C in Z coordinates the pressure is rho0 * (hydrostatic) Potential |
486 |
IF ( useDynP_inEos_Zc ) THEN |
487 |
C---------- |
488 |
C NOTE: For now, totPhiHyd only contains the Potential anomaly |
489 |
C since PhiRef is not available for Atmos and has not (yet) |
490 |
C been added in S/R DIAGS_PHI_HYD |
491 |
C---------- |
492 |
pLoc = rhoConst*( totPhiHyd(i,j,kRef,bi,bj) |
493 |
& -rC(kRef)*gravity |
494 |
& )*maskC(i,j,kRef,bi,bj) |
495 |
ELSE |
496 |
pLoc = -rhoConst*rC(kRef)*gravity*maskC(i,j,kRef,bi,bj) |
497 |
ENDIF |
498 |
ELSEIF ( buoyancyRelation .EQ. 'OCEANICP' ) THEN |
499 |
C in P coordinates the pressure is just the coordinate of |
500 |
C the tracer point |
501 |
pLoc = rC(kRef)* maskC(i,j,kRef,bi,bj) |
502 |
ENDIF |
503 |
|
504 |
rhoLoc = 0. _d 0 |
505 |
rhoP0 = 0. _d 0 |
506 |
bulkMod = 0. _d 0 |
507 |
rfresh = 0. _d 0 |
508 |
rsalt = 0. _d 0 |
509 |
bMfresh = 0. _d 0 |
510 |
bMsalt = 0. _d 0 |
511 |
bMpres = 0. _d 0 |
512 |
rhoNum = 0. _d 0 |
513 |
rhoDen = 0. _d 0 |
514 |
den = 0. _d 0 |
515 |
|
516 |
t1 = tLoc |
517 |
t2 = t1*t1 |
518 |
t3 = t2*t1 |
519 |
t4 = t3*t1 |
520 |
|
521 |
s1 = sLoc |
522 |
|
523 |
IF ( equationOfState .EQ. 'LINEAR' ) THEN |
524 |
|
525 |
dRho = rhoNil-rhoConst |
526 |
rhoLoc=rhoNil* ( |
527 |
& sBeta *(sLoc-sRef(kRef)) |
528 |
& - tAlpha*(tLoc-tRef(KREF)) ) + dRho |
529 |
|
530 |
ELSEIF (equationOfState.EQ.'POLY3') THEN |
531 |
|
532 |
C this is not correct, there is a field eosSig0 which should be use here |
533 |
C but I DO not intent to include the reference level in this routine |
534 |
WRITE(*,'(a)') |
535 |
& ' FIND_RHO_SCALAR: for POLY3, the density is not' |
536 |
WRITE(*,'(a)') |
537 |
& ' computed correctly in this routine' |
538 |
rhoLoc = 0. _d 0 |
539 |
|
540 |
ELSEIF ( equationOfState(1:5).EQ.'JMD95' |
541 |
& .OR. equationOfState.EQ.'UNESCO' ) THEN |
542 |
C nonlinear equation of state in pressure coordinates |
543 |
|
544 |
s3o2 = s1*SQRT(s1) |
545 |
|
546 |
p1 = pLoc*SItoBar |
547 |
p2 = p1*p1 |
548 |
|
549 |
C density of freshwater at the surface |
550 |
rfresh = |
551 |
& eosJMDCFw(1) |
552 |
& + eosJMDCFw(2)*t1 |
553 |
& + eosJMDCFw(3)*t2 |
554 |
& + eosJMDCFw(4)*t3 |
555 |
& + eosJMDCFw(5)*t4 |
556 |
& + eosJMDCFw(6)*t4*t1 |
557 |
C density of sea water at the surface |
558 |
rsalt = |
559 |
& s1*( |
560 |
& eosJMDCSw(1) |
561 |
& + eosJMDCSw(2)*t1 |
562 |
& + eosJMDCSw(3)*t2 |
563 |
& + eosJMDCSw(4)*t3 |
564 |
& + eosJMDCSw(5)*t4 |
565 |
& ) |
566 |
& + s3o2*( |
567 |
& eosJMDCSw(6) |
568 |
& + eosJMDCSw(7)*t1 |
569 |
& + eosJMDCSw(8)*t2 |
570 |
& ) |
571 |
& + eosJMDCSw(9)*s1*s1 |
572 |
|
573 |
rhoP0 = rfresh + rsalt |
574 |
|
575 |
C secant bulk modulus of fresh water at the surface |
576 |
bMfresh = |
577 |
& eosJMDCKFw(1) |
578 |
& + eosJMDCKFw(2)*t1 |
579 |
& + eosJMDCKFw(3)*t2 |
580 |
& + eosJMDCKFw(4)*t3 |
581 |
& + eosJMDCKFw(5)*t4 |
582 |
C secant bulk modulus of sea water at the surface |
583 |
bMsalt = |
584 |
& s1*( eosJMDCKSw(1) |
585 |
& + eosJMDCKSw(2)*t1 |
586 |
& + eosJMDCKSw(3)*t2 |
587 |
& + eosJMDCKSw(4)*t3 |
588 |
& ) |
589 |
& + s3o2*( eosJMDCKSw(5) |
590 |
& + eosJMDCKSw(6)*t1 |
591 |
& + eosJMDCKSw(7)*t2 |
592 |
& ) |
593 |
C secant bulk modulus of sea water at pressure p |
594 |
bMpres = |
595 |
& p1*( eosJMDCKP(1) |
596 |
& + eosJMDCKP(2)*t1 |
597 |
& + eosJMDCKP(3)*t2 |
598 |
& + eosJMDCKP(4)*t3 |
599 |
& ) |
600 |
& + p1*s1*( eosJMDCKP(5) |
601 |
& + eosJMDCKP(6)*t1 |
602 |
& + eosJMDCKP(7)*t2 |
603 |
& ) |
604 |
& + p1*s3o2*eosJMDCKP(8) |
605 |
& + p2*( eosJMDCKP(9) |
606 |
& + eosJMDCKP(10)*t1 |
607 |
& + eosJMDCKP(11)*t2 |
608 |
& ) |
609 |
& + p2*s1*( eosJMDCKP(12) |
610 |
& + eosJMDCKP(13)*t1 |
611 |
& + eosJMDCKP(14)*t2 |
612 |
& ) |
613 |
|
614 |
bulkMod = bMfresh + bMsalt + bMpres |
615 |
|
616 |
C density of sea water at pressure p |
617 |
rhoLoc = rhoP0/(1. _d 0 - p1/bulkMod) - rhoConst |
618 |
|
619 |
ELSEIF ( equationOfState.EQ.'MDJWF' ) THEN |
620 |
|
621 |
sp5 = SQRT(s1) |
622 |
|
623 |
p1 = pLoc*SItodBar |
624 |
p1t1 = p1*t1 |
625 |
|
626 |
rhoNum = eosMDJWFnum(0) |
627 |
& + t1*(eosMDJWFnum(1) |
628 |
& + t1*(eosMDJWFnum(2) + eosMDJWFnum(3)*t1) ) |
629 |
& + s1*(eosMDJWFnum(4) |
630 |
& + eosMDJWFnum(5)*t1 + eosMDJWFnum(6)*s1) |
631 |
& + p1*(eosMDJWFnum(7) + eosMDJWFnum(8)*t2 |
632 |
& + eosMDJWFnum(9)*s1 |
633 |
& + p1*(eosMDJWFnum(10) + eosMDJWFnum(11)*t2) ) |
634 |
|
635 |
|
636 |
den = eosMDJWFden(0) |
637 |
& + t1*(eosMDJWFden(1) |
638 |
& + t1*(eosMDJWFden(2) |
639 |
& + t1*(eosMDJWFden(3) + t1*eosMDJWFden(4) ) ) ) |
640 |
& + s1*(eosMDJWFden(5) |
641 |
& + t1*(eosMDJWFden(6) |
642 |
& + eosMDJWFden(7)*t2) |
643 |
& + sp5*(eosMDJWFden(8) + eosMDJWFden(9)*t2) ) |
644 |
& + p1*(eosMDJWFden(10) |
645 |
& + p1t1*(eosMDJWFden(11)*t2 + eosMDJWFden(12)*p1) ) |
646 |
|
647 |
rhoDen = 1.0/(epsln+den) |
648 |
|
649 |
rhoLoc = rhoNum*rhoDen - rhoConst |
650 |
|
651 |
ELSEIF( equationOfState .EQ. 'IDEALG' ) THEN |
652 |
C |
653 |
ELSE |
654 |
WRITE(msgbuf,'(3A)') |
655 |
& ' STATE1 : equationOfState = "', |
656 |
& equationOfState,'"' |
657 |
CALL PRINT_ERROR( msgbuf, mythid ) |
658 |
STOP 'ABNORMAL END: S/R STATE1 in OPPS_CALC' |
659 |
ENDIF |
660 |
|
661 |
state1 = rhoLoc + rhoConst |
662 |
|
663 |
#endif /* ALLOW_OPPS */ |
664 |
RETURN |
665 |
END |
666 |
|
667 |
|
668 |
#undef OPPS_ORGCODE |
669 |
#ifdef OPPS_ORGCODE |
670 |
c Listed below is the subroutine for use in parallel 3-d circulation code. |
671 |
c It has been used in the parallel semtner-chervin code and is now being used |
672 |
c In the POP code. The subroutine is called nlopps (long story to explain why). |
673 |
|
674 |
c I've attached the version of lopps that we've been using in the simulations. |
675 |
c There is one common block that is different from the standard model commons |
676 |
c (countc) and it is not needed if the array convadj is not used. The routine |
677 |
c does need "kmp" which is why the boundc common is included. For massively |
678 |
c parallel codes (like POP) we think this will work well when converted from a |
679 |
c "slab" (i=is,ie) to a column, which just means removing the "do i=is,ie" loop. c There are differences between this |
680 |
c code and the 1-d code and the earlier scheme implemented in 3-d models. These c differences are described below. |
681 |
|
682 |
|
683 |
subroutine nlopps(j,is,ie,ta,sa,gcmdz) |
684 |
c |
685 |
parameter (imt = 361 , jmt = 301 , km = 30 ) |
686 |
c |
687 |
c Nlopps: E. Skyllingstad and T. Paluszkiewicz |
688 |
c |
689 |
c Version: December 11, 1996 |
690 |
c |
691 |
c Nlopps: This version of lopps is significantly different from |
692 |
c the original code developed by R. Romea and T. Paluskiewicz. The |
693 |
c code uses a flux constraint to control the change in T and S at |
694 |
c each grid level. First, a plume profile of T,S, and W are |
695 |
c determined using the standard plume model, but with a detraining |
696 |
c mass instead of entraining. Thus, the T and S plume |
697 |
c characteristics still change, but the plume contracts in size |
698 |
c rather than expanding ala classical entraining plumes. This |
699 |
c is heuristically more in line with large eddy simulation results. |
700 |
c At each grid level, the convergence of plume velocity determines |
701 |
c the flux of T and S, which is conserved by using an upstream |
702 |
c advection. The vertical velocity is balanced so that the area |
703 |
c weighted upward velocity equals the area weighted downdraft |
704 |
c velocity, ensuring mass conservation. The present implementation |
705 |
c adjusts the plume for a time period equal to the time for 1/2 of |
706 |
c the mass of the fastest moving level to move downward. As a |
707 |
c consequence, the model does not completely adjust the profile at |
708 |
c each model time step, but provides a smooth adjustment over time. |
709 |
c |
710 |
c |
711 |
|
712 |
|
713 |
c |
714 |
|
715 |
c include "params.h" |
716 |
c include "plume_fast_inc.h" |
717 |
c include "plume_fast.h" |
718 |
c #include "loppsd.h" |
719 |
|
720 |
real ta(imt,km),sa(imt,km),gcmdz(km),dz(km) |
721 |
real pdensity,wsqr,oldflux,newflux,entrainrate,adtemp |
722 |
REAL Del,D,dza1,dza2,kd,kd1,Smix,Thmix,PlumeS,PlumeT,PlumeD |
723 |
c |
724 |
c |
725 |
|
726 |
INTEGER i,j,k |
727 |
clfh |
728 |
integer is,ie,k2 |
729 |
clfh |
730 |
REAL D1,D2,state1,Density |
731 |
REAL dz1,dz2 |
732 |
REAL radius,StartingFlux |
733 |
real ttemp(km),stemp(km),taa(km),saa(km) |
734 |
real wda(km),tda(km),sda(km),mda(km) |
735 |
real dtts,dt,sumo,sumn |
736 |
integer ntime,nn,kmx,ic |
737 |
c |
738 |
c |
739 |
LOGICAL debug,done |
740 |
INTEGER MAX_ABE_ITERATIONS |
741 |
PARAMETER(MAX_ABE_ITERATIONS=1) |
742 |
REAL PlumeRadius |
743 |
REAL STABILITY_THRESHOLD |
744 |
REAL FRACTIONAL_AREA |
745 |
REAL MAX_FRACTIONAL_AREA |
746 |
REAL VERTICAL_VELOCITY |
747 |
REAL ENTRAINMENT_RATE |
748 |
REAL e2 |
749 |
PARAMETER ( PlumeRadius = 100.D0 ) |
750 |
PARAMETER ( STABILITY_THRESHOLD = -1.E-4 ) |
751 |
PARAMETER ( FRACTIONAL_AREA = .1E0 ) |
752 |
PARAMETER ( MAX_FRACTIONAL_AREA = .8E0 ) |
753 |
PARAMETER ( VERTICAL_VELOCITY = .02E0 ) |
754 |
PARAMETER ( ENTRAINMENT_RATE = -.05E0 ) |
755 |
PARAMETER ( e2 = 2.E0*ENTRAINMENT_RATE ) |
756 |
! Arrays. |
757 |
REAL Ad(km),Sd(km),Td(km),Wd(km),Dd(km),Md(km) |
758 |
REAL Se(km),Te(km),We(km),De(km) |
759 |
REAL PlumeEntrainment(km) |
760 |
REAL GridThickness(km) |
761 |
|
762 |
c |
763 |
c input kmp through a common block |
764 |
c |
765 |
common / boundc / wsx(imt,jmt),wsy(imt,jmt),hfs(imt,jmt), |
766 |
1 ple(imt,jmt),kmp(imt,jmt),kmq(imt,jmt) |
767 |
cwmseas |
768 |
& ,wsx1(imt,jmt),wsy1(imt,jmt) |
769 |
1 ,wsx2(imt,jmt),wsy2(imt,jmt) |
770 |
c |
771 |
c input the variables through a common |
772 |
c |
773 |
logical problem |
774 |
common /countc/ convadj(imt,jmt,km),ics,depth(km),problem |
775 |
|
776 |
|
777 |
c-----may want to setup an option to get this only on first call |
778 |
c otherwise it is repetive |
779 |
c griddz is initialize by call to setupgrid |
780 |
c |
781 |
c |
782 |
|
783 |
dtts = 2400 |
784 |
c |
785 |
do k=1,km |
786 |
dz(k) = 0.01*gcmdz(k) |
787 |
enddo |
788 |
c |
789 |
do k=1,km |
790 |
GridThickness(k) = dz(k) |
791 |
enddo |
792 |
c |
793 |
c modified to loop over slab |
794 |
c |
795 |
DO i=is,ie |
796 |
|
797 |
numgridpoints=kmp(i,j) |
798 |
c |
799 |
c go to next column if only 1 grid point or on land |
800 |
c |
801 |
if(numgridpoints.le.1) goto 1100 |
802 |
c |
803 |
c loop over depth |
804 |
c |
805 |
c |
806 |
debug = .false. |
807 |
c |
808 |
c first save copy of initial profile |
809 |
c |
810 |
DO k=1,NumGridPoints |
811 |
stemp(k)=sa(i,k) |
812 |
ttemp(k)=ta(i,k) |
813 |
c |
814 |
c do a check of t and s range, if out of bounds set flag |
815 |
c |
816 |
if(problem) then |
817 |
write(0,*)"Code in trouble before this nlopps call" |
818 |
return |
819 |
endif |
820 |
c |
821 |
if(sa(i,k).gt.40..or.ta(i,k).lt.-4.0) then |
822 |
problem = .true. |
823 |
write(0,*)"t out of range at j ",j |
824 |
debug = .true. |
825 |
return |
826 |
endif |
827 |
ENDDO |
828 |
|
829 |
if(debug) then |
830 |
write(*,*)"T and S Profile at ",i,j |
831 |
write(*,*)(ta(i,k),sa(i,k),k=1,NumGridPoints) |
832 |
endif |
833 |
|
834 |
DO k=1,NumGridPoints-1 |
835 |
c |
836 |
c initialize the plume T,S,density, and w velocity |
837 |
c |
838 |
Sd(k)=stemp(k) |
839 |
Td(k)=ttemp(k) |
840 |
Dd(k)=state1(stemp(k),ttemp(k),k) |
841 |
De(k)=Dd(k) |
842 |
c Wd(k)=VERTICAL_VELOCITY |
843 |
c |
844 |
c guess at initial top grid cell vertical velocity |
845 |
c |
846 |
Wd(k) = 0.03 |
847 |
c |
848 |
c these estimates of initial plume velocity based on plume size and |
849 |
c top grid cell water mass |
850 |
c |
851 |
c Wd(k) = 0.5*dz(k)/(dtts*FRACTIONAL_AREA) |
852 |
c Wd(k) = 0.5*dz(k)/dtts |
853 |
c |
854 |
wsqr=Wd(k)*Wd(k) |
855 |
PlumeEntrainment(k) = 0.0 |
856 |
c |
857 |
c |
858 |
c |
859 |
if(debug) write(0,*) 'Doing old lowerparcel' |
860 |
radius=PlumeRadius |
861 |
StartingFlux=radius*radius*Wd(k)*Dd(k) |
862 |
oldflux=StartingFlux |
863 |
|
864 |
dz2=GridThickness(k) |
865 |
DO k2=k,NumGridPoints-1 |
866 |
D1=state1(Sd(k2),Td(k2),k2+1) |
867 |
D2=state1(stemp(k2+1),ttemp(k2+1),k2+1) |
868 |
De(k2+1)=D2 |
869 |
c |
870 |
c To start downward, parcel has to initially be heavier than environment |
871 |
c but after it has started moving, we continue plume until plume tke or |
872 |
c flux goes negative |
873 |
c |
874 |
IF (D2-D1 .LT. STABILITY_THRESHOLD.or.k2.ne.k) THEN |
875 |
dz1=dz2 |
876 |
dz2=GridThickness(k2+1) |
877 |
c |
878 |
c define mass flux according to eq. 4 from paper |
879 |
c |
880 |
newflux=oldflux+e2*radius*Wd(k2)*Dd(k2)*0.50* |
881 |
. (dz1+dz2) |
882 |
c |
883 |
PlumeEntrainment(k2+1) = newflux/StartingFlux |
884 |
c |
885 |
IF(newflux.LT.0.0) then |
886 |
if(debug) then |
887 |
write(0,*)"Plume entrained to zero at ",k2 |
888 |
endif |
889 |
maxdepth = k2 |
890 |
if(maxdepth.eq.k) goto 1000 |
891 |
goto 1 |
892 |
endif |
893 |
c |
894 |
c entrainment rate is basically a scaled mass flux dM/M |
895 |
c |
896 |
entrainrate = (newflux - oldflux)/newflux |
897 |
oldflux = newflux |
898 |
c |
899 |
c |
900 |
c mix var's are the average environmental values over the two grid levels |
901 |
c |
902 |
smix=(dz1*stemp(k2)+dz2*stemp(k2+1))/(dz1+dz2) |
903 |
thmix=(dz1*ttemp(k2)+dz2*ttemp(k2+1))/(dz1+dz2) |
904 |
c |
905 |
c first compute the new salinity and temperature for this level |
906 |
c using equations 3.6 and 3.7 from the paper |
907 |
c |
908 |
c |
909 |
c |
910 |
sd(k2+1)=sd(k2) - entrainrate*(smix - sd(k2)) |
911 |
td(k2+1)=td(k2) - entrainrate*(thmix - td(k2)) |
912 |
c |
913 |
c |
914 |
c compute the density at this level for the buoyancy term in the |
915 |
c vertical k.e. equation |
916 |
c |
917 |
Dd(k2+1)=state1(Sd(k2+1),Td(k2+1),k2+1) |
918 |
c |
919 |
c next, solve for the vertical velocity k.e. using combined eq. 4 |
920 |
c and eq 5 from the paper |
921 |
c |
922 |
if(debug) then |
923 |
write(0,*)"Dd,De,entr,k ",Dd(k2),De(k2),entrainrate,k2 |
924 |
endif |
925 |
c |
926 |
wsqr = wsqr - wsqr*abs(entrainrate)+ 9.81* |
927 |
. (dz1*(Dd(k2)-De(k2))/De(k2) |
928 |
. +dz2*(Dd(k2+1)-De(k2+1))/De(k2+1)) |
929 |
c |
930 |
c if negative k.e. then plume has reached max depth, get out of loop |
931 |
c |
932 |
IF(wsqr.LT.0.0)then |
933 |
maxdepth = k2 |
934 |
if(debug) then |
935 |
write(0,*)"Plume velocity went to zero at ",k2 |
936 |
endif |
937 |
if(maxdepth.eq.k) goto 1000 |
938 |
goto 1 |
939 |
endif |
940 |
Wd(k2+1)=sqrt(wsqr) |
941 |
c |
942 |
c compute a new radius based on the new mass flux at this grid level |
943 |
c |
944 |
radius=sqrt(newflux/(Wd(k2)*Dd(k2))) |
945 |
ELSE |
946 |
maxdepth=k2 |
947 |
if(maxdepth.eq.k) goto 1000 |
948 |
GOTO 1 |
949 |
ENDIF |
950 |
ENDDO |
951 |
c |
952 |
c plume has reached the bottom |
953 |
c |
954 |
MaxDepth=NumGridPoints |
955 |
c |
956 |
1 continue |
957 |
c |
958 |
Ad(k)=FRACTIONAL_AREA |
959 |
IC=0 |
960 |
c |
961 |
c start iteration on fractional area, not used in OGCM implementation |
962 |
c |
963 |
c |
964 |
DO IC=1,Max_ABE_Iterations |
965 |
c |
966 |
c |
967 |
c next compute the mass flux beteen each grid box using the entrainment |
968 |
c |
969 |
92 continue |
970 |
Md(k)=Wd(k)*Ad(k) |
971 |
c |
972 |
DO k2=k+1,MaxDepth |
973 |
Md(k2)=Md(k)*PlumeEntrainment(k2) |
974 |
if(debug) then |
975 |
write(0,*)"Md, Wd, and k are ",Md(k2),Wd(k2),k2 |
976 |
endif |
977 |
ENDDO |
978 |
c |
979 |
c Now move on to calculate new temperature using flux from |
980 |
c Td, Sd, Wd, ta, sa, and we. Values for these variables are at |
981 |
c center of grid cell, use weighted average to get boundary values |
982 |
c |
983 |
c use a timestep limited by the GCM model timestep and the maximum plume |
984 |
c velocity (CFL criteria) |
985 |
c |
986 |
c |
987 |
c calculate the weighted wd, td, and sd |
988 |
c |
989 |
dt = dtts |
990 |
do k2=k,maxdepth-1 |
991 |
dt = min(dt,dz(k2)/wd(k2)) |
992 |
c |
993 |
c time integration will be integer number of steps to get one |
994 |
c gcm time step |
995 |
c |
996 |
ntime = nint(0.5*int(dtts/dt)) |
997 |
if(ntime.eq.0) then |
998 |
ntime = 1 |
999 |
endif |
1000 |
c |
1001 |
c make sure area weighted vertical velocities match; in other words |
1002 |
c make sure mass in equals mass out at the intersection of each grid |
1003 |
c cell. |
1004 |
c |
1005 |
mda(k2) = (md(k2)*dz(k2)+md(k2+1)*dz(k2+1))/ |
1006 |
* (dz(k2)+dz(k2+1)) |
1007 |
c |
1008 |
wda(k2) = (wd(k2)*dz(k2)+wd(k2+1)*dz(k2+1))/ |
1009 |
* (dz(k2)+dz(k2+1)) |
1010 |
c |
1011 |
tda(k2) = td(k2) |
1012 |
sda(k2) = sd(k2) |
1013 |
c |
1014 |
taa(k2) = ttemp(k2+1) |
1015 |
saa(k2) = stemp(k2+1) |
1016 |
c |
1017 |
enddo |
1018 |
dt = min(dt,dtts) |
1019 |
if(debug) then |
1020 |
write(0,*)"Time step is ", dt |
1021 |
endif |
1022 |
tda(maxdepth) = td(maxdepth) |
1023 |
sda(maxdepth) = sd(maxdepth) |
1024 |
c |
1025 |
c do top and bottom points first |
1026 |
c |
1027 |
kmx = maxdepth-1 |
1028 |
do nn=1,ntime |
1029 |
|
1030 |
ttemp(k) = ttemp(k)- |
1031 |
* (mda(k)*(tda(k)-taa(k)))*dt*recip_drF(k) |
1032 |
c |
1033 |
stemp(k) = stemp(k)- |
1034 |
* (mda(k)*(sda(k)-saa(k)))*dt*recip_drF(k) |
1035 |
c |
1036 |
c |
1037 |
c now do inner points if there are any |
1038 |
c |
1039 |
if(Maxdepth-k.gt.1) then |
1040 |
do k2=k+1,Maxdepth-1 |
1041 |
c |
1042 |
ttemp(k2) = ttemp(k2) + |
1043 |
* (mda(k2-1)*(tda(k2-1)-taa(k2-1))- |
1044 |
* mda(k2)*(tda(k2)-taa(k2))) |
1045 |
* *dt*recip_drF(k2) |
1046 |
|
1047 |
c |
1048 |
stemp(k2) = stemp(k2) + |
1049 |
* (mda(k2-1)*(sda(k2-1)-saa(k2-1))- |
1050 |
* mda(k2)*(sda(k2)-saa(k2))) |
1051 |
* *dt*recip_drF(k2) |
1052 |
|
1053 |
c |
1054 |
enddo |
1055 |
endif |
1056 |
ttemp(kmx+1) = ttemp(kmx+1)+ |
1057 |
* (mda(kmx)*(tda(kmx)-taa(kmx)))* |
1058 |
* dt*recip_drF(kmx+1) |
1059 |
c |
1060 |
stemp(kmx+1) = stemp(kmx+1)+ |
1061 |
* (mda(kmx)*(sda(kmx)-saa(kmx)))* |
1062 |
* dt*recip_drF(kmx+1) |
1063 |
c |
1064 |
c set the environmental temp and salinity to equal new fields |
1065 |
c |
1066 |
do k2=1,maxdepth-1 |
1067 |
taa(k2) = ttemp(k2+1) |
1068 |
saa(k2) = stemp(k2+1) |
1069 |
enddo |
1070 |
c |
1071 |
c end loop on number of time integration steps |
1072 |
c |
1073 |
enddo |
1074 |
ENDDO |
1075 |
999 continue |
1076 |
c |
1077 |
c assume that it converged, so update the ta and sa with new fields |
1078 |
c |
1079 |
c if(i.gt.180.and.j.gt.200.and.i.lt.240) then |
1080 |
c write(*,*)"Converged ",i,j,k,maxdepth,ttemp(k+1),ta(i,k+1) |
1081 |
c endif |
1082 |
do k2=k,maxdepth |
1083 |
convadj(i,j,k2) = convadj(i,j,k2) + (ttemp(k2)- |
1084 |
* ta(i,k2)) |
1085 |
sa(i,k2) = stemp(k2) |
1086 |
ta(i,k2) = ttemp(k2) |
1087 |
c if(i.gt.180.and.j.gt.200.and.i.lt.240) then |
1088 |
c write(*,*)"convadj ",convadj(i,j,k2) |
1089 |
c endif |
1090 |
c |
1091 |
c see if nlopps messed up |
1092 |
c |
1093 |
if(sa(i,k).gt.40..or.ta(i,k).lt.-4.0) then |
1094 |
problem = .true. |
1095 |
write(0,*)"t out of range at j after adjust",j |
1096 |
debug = .true. |
1097 |
endif |
1098 |
c |
1099 |
enddo |
1100 |
c |
1101 |
c jump here if k = maxdepth or if level not unstable, go to next |
1102 |
c profile point |
1103 |
c |
1104 |
1000 continue |
1105 |
c |
1106 |
c |
1107 |
c end loop on k, move on to next possible plume |
1108 |
c |
1109 |
ENDDO |
1110 |
1100 continue |
1111 |
c |
1112 |
c i loop |
1113 |
c |
1114 |
ENDDO |
1115 |
END |
1116 |
|
1117 |
#endif /* OPPS_ORGCODE |