Changeset 2037 for LMDZ5/trunk/libf/dyn3dpar/calfis_p.F

Timestamp:

May 6, 2014, 4:56:20 PM (10 years ago)

Author:

lguez

Message:

PVteta computed by PVtheta was not used. Also there were a couple of
problems with PVtheta:

-- PVtheta calls tetalevel in phylmd, and interpolates at

Earth-specific values of potential temperature.

-- PVtheta calls tourabs, and the computation of rot in tourabs should

be modified (it is not correct when there is a zoom).

-- Even when there is no zoom, the computation of rot in tourabs

should probably be modified: directly combine vcov and ucov, as in
tourpot, instead of dividing by cv and cu.

File:

• LMDZ5/trunk/libf/dyn3dpar/calfis_p.F (modified) (4 diffs)

LMDZ5/trunk/libf/dyn3dpar/calfis_p.F

@@ -217 +217 @@
       REAL unskap, pksurcp
 c
-cIM diagnostique PVteta, Amip2
-      INTEGER,PARAMETER :: ntetaSTD=3
-      REAL,SAVE :: rtetaSTD(ntetaSTD)=(/350.,380.,405./) ! Earth-specific, beware !!
-      REAL PVteta(klon,ntetaSTD)
-      
       REAL SSUM
 
@@ -249 +244 @@
       klon=klon_mpi
       
-      PVteta(:,:)=0.
-            
 c
       IF ( firstcal )  THEN
@@ -484 +477 @@
       endif
 
-
-      IF (is_sequential.and.(planet_type=="earth")) THEN
-#ifdef CPP_PHYS
-! PVtheta calls tetalevel, which is in the physics
-cIM calcul PV a teta=350, 380, 405K
-        CALL PVtheta(ngridmx,llm,pucov,pvcov,pteta,
-     $           ztfi,zplay,zplev,
-     $           ntetaSTD,rtetaSTD,PVteta)
-c
-#endif
-      ENDIF
-
 c On change de grille, dynamique vers physiq, pour le flux de masse verticale
       CALL gr_dyn_fi_p(llm,iip1,jjp1,klon,flxw,flxwfi)
@@ -668 +649 @@
      .             zdqfi_omp,
      .             zdpsrf_omp,
-cIM diagnostique PVteta, Amip2          
-     .             pducov,
-     .             PVteta)
+     .             pducov)
 
       else if ( planet_type=="generic" ) then