Ignore:
Timestamp:
Apr 7, 2011, 4:15:05 PM (14 years ago)
Author:
Ehouarn Millour
Message:

Added possibility to have the base of the atmosphere heated (to mimic a constant uniform heat flux from below), set in .def file (parameter ihf = ... , in W/m2); only active if in "Newtonian mode" (iflag_phys=2) and if planet_type=="giant".
EM

File:
1 edited

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  • LMDZ5/trunk/libf/dyn3dpar/iniacademic.F90

    r1492 r1505  
    178178           tetajl(j,l)=teta0-delt_y*ddsin*ddsin+eps*ddsin &
    179179                -delt_z*(1.-ddsin*ddsin)*log(zsig)
     180           if (planet_type=="giant") then
     181             tetajl(j,l)=teta0+(delt_y*                   &
     182                ((sin(rlatu(j)*3.14159*eps+0.0001))**2)   &
     183                / ((rlatu(j)*3.14159*eps+0.0001)**2))     &
     184                -delt_z*log(zsig)
     185           endif
    180186           ! Profil stratospherique isotherme (+vortex)
    181187           w_pv=(1.-tanh((rlatu(j)-phi_pv)/dphi_pv))/2.
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