The Intermediate Complexity Atmospheric Research model (ICAR)
A computationally efficient atmospheric model for downscaling.
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This is the complete list of members for module_bl_ysu, including all inherited members.
tridin(cl, cm, cu, r1, r2, au, f1, f2, its, ite, kts, kte, nt) | module_bl_ysu | |
ysu(u3d, v3d, th3d, t3d, qv3d, qc3d, qi3d, p3d, p3di, pi3d,rublten, rvblten, rthblten,rqvblten, rqcblten, rqiblten, flag_qi,cp, g, rovcp, rd, rovg,dz8w, z, xlv, rv, psfc,znu, znw, mut, p_top,znt, ust, zol, hol, hpbl, psim, psih,xland, hfx, qfx, tsk, gz1oz0, wspd, br,dt, dtmin, kpbl2d,svp1, svp2, svp3, svpt0, ep1, ep2, karman, eomeg, stbolt,exch_h,u10, v10,ids, ide, jds, jde, kds, kde,ims, ime, jms, jme, kms, kme,its, ite, jts, jte, kts, kte, | module_bl_ysu | |
ysu2d(j, ux, vx, tx, qx, qcx, qix, p2d, p2di, pi2d,utnp, vtnp, ttnp,qtnp, qctnp, qitnp,cp, g, rovcp, rd, rovg,dz8w2d, z2d, xlv, rv, psfcpa,znt, ust, zol, hol, hpbl, psim, psih,xland, hfx, qfx, tsk, gz1oz0, wspd, br,dt, dtmin, kpbl1d,svp1, svp2, svp3, svpt0, ep1, ep2, karman, eomeg, stbolt,exch_hx,u10, v10,ids, ide, jds, jde, kds, kde,ims, ime, jms, jme, kms, kme,its, ite, jts, jte, kts, kte, | module_bl_ysu | |
ysuinit(rublten, rvblten, rthblten, rqvblten, rqcblten, rqiblten, p_qi, p_first_scalar, restart, allowed_to_read, ids, ide, jds, jde, kds, kde, ims, ime, jms, jme, kms, kme, its, ite, jts, jte, kts, kte) | module_bl_ysu |