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Timestamp:
Aug 6, 2024, 6:39:29 PM (19 months ago)
Author:
llange
Message:

Mars PCM
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Correction of the computation of the water vapor flux from the subsurface ice when thin frost is at the surface: When the frost was too thin (thickness < tol_frost), the flux from the subsurface ice to the surface/atmosphere was not computed. It is now corrected, assuming that the frost is too thin to prevent exchange between subsurface ice and the atmosphere
cleaning testphys1d (unused comments)
LL, who should be writing his PhD dissertation

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1 edited

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  • trunk/LMDZ.MARS/libf/phymars/dyn1d/testphys1d.F90

    r3369 r3400  
    207207            endif
    208208        endif
    209     !EV profile
    210 !            IF(atm_wat_profile.eq.2) THEN
    211 !             DO ilayer=1,16
    212 !              q(1,ilayer,igcm_h2o_vap)=min(zqsat(ilayer),6e-5)
    213 !             ENDDO! ilayer=1,16
    214 !             DO ilayer=17,22
    215 !              q(1,ilayer,igcm_h2o_vap)=min(zqsat(ilayer),3e-5)
    216 !             ENDDO! ilayer=17,22
    217 !             DO ilayer=23,nlayer
    218 !              q(1,ilayer,igcm_h2o_vap)=0
    219 !             ENDDO! ilayer=23,nlayer
    220 !             endif
    221209     endif
    222210
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