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CCPP Scientific Documentation
v5.0.0
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CCPP Scientific Documentation
v5.0.0
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| subroutine module_bl_mynn::dmp_mf | ( | integer, intent(in) | kts, |
| integer, intent(in) | kte, | ||
| real, intent(in) | dt, | ||
| real, dimension(kts:kte+1), intent(in) | zw, | ||
| real, dimension(kts:kte), intent(in) | dz, | ||
| real, dimension(kts:kte), intent(in) | p, | ||
| integer, intent(in) | momentum_opt, | ||
| integer, intent(in) | tke_opt, | ||
| integer, intent(in) | scalar_opt, | ||
| real, dimension(kts:kte), intent(in) | u, | ||
| real, dimension(kts:kte), intent(in) | v, | ||
| real, dimension(kts:kte), intent(in) | w, | ||
| real, dimension(kts:kte), intent(in) | th, | ||
| real, dimension(kts:kte), intent(in) | thl, | ||
| real, dimension(kts:kte), intent(in) | thv, | ||
| real, dimension(kts:kte), intent(in) | tk, | ||
| real, dimension(kts:kte), intent(in) | qt, | ||
| real, dimension(kts:kte), intent(in) | qv, | ||
| real, dimension(kts:kte), intent(in) | qc, | ||
| real, dimension(kts:kte), intent(in) | qke, | ||
| real, dimension(kts:kte), intent(in) | qnc, | ||
| real, dimension(kts:kte), intent(in) | qni, | ||
| real, dimension(kts:kte), intent(in) | qnwfa, | ||
| real, dimension(kts:kte), intent(in) | qnifa, | ||
| real, dimension(kts:kte), intent(in) | exner, | ||
| real, dimension(kts:kte), intent(inout) | vt, | ||
| real, dimension(kts:kte), intent(inout) | vq, | ||
| real, dimension(kts:kte), intent(inout) | sgm, | ||
| real, intent(in) | ust, | ||
| real, intent(in) | flt, | ||
| real, intent(in) | flq, | ||
| real, intent(in) | flqv, | ||
| real, intent(in) | flqc, | ||
| real, intent(in) | pblh, | ||
| integer, intent(in) | kpbl, | ||
| real, intent(in) | DX, | ||
| real, intent(in) | landsea, | ||
| real, intent(in) | ts | ||
| ) |
dmp_mf() calculates the nonlocal turbulent transport from the dynamic multiplume mass-flux scheme as well as the shallow-cumulus component of the subgrid clouds. Note that this mass-flux scheme is called when the namelist paramter bl_mynn_edmf is set to 1 (recommended).
Much thanks to Kay Suslj of NASA-JPL for contributing the original version of this mass-flux scheme. Considerable changes have been made from it's original form. Some additions include:
This scheme remains under development, so consider it experimental code.
References bl_mynn_mixchem, condensation_edmf(), debug_code, env_subs, ep_3, esat_blend(), gtr, onethird, p1000mb, qsat_blend(), svp1, tv0, xl_blend(), and xlvcp.
Referenced by mynn_bl_driver().
1.8.11