This short report documents the changes in the COSMO-Model versions 4.15 (implemented into the VCS on 2010-11-19) and 4.16 (implemented into the VCS on 2010-12-07). Version 4.16 is running operational at DWD since 2010-12-15. Version 4.16 only was a small technical update. The modifications are marked below.
A new option for 3rd order implicit vertical advection has been implemented in the Runge-Kutta scheme. At the same time the namelist control of vertical advection has been changed (in the group /DYNCTL/
New subroutines have been implemented for the new scheme in src_runge_kutta.f90 (calc_wcon_sqrtg), in src_slow_tendencies.f90 (complete_tend_uvwtpp_CN3Crow) and in numeric_utilities.f90 (solve_5banddiag, bandec, banbks).
A new subroutine weighting_factors_full2half has been implemented in fast_waves_rk.f90 to summarize the calculation of weighting coefficients for vertical interpolation.
The value of the /TUNING/ Namelist variable securi has been limited. According to numerical stability tests, the range from 0 to 1 is too big. The default value and the allowed range therefore have been reduced:
Default: securi_d = 0.5 and the range: 0 <= securi <= 0.5
This will change the results, if a value greater than 0.5 has been chosen before with limpltkediff=.FALSE. For limpltkediff=.TRUE., this security value has no effect any more.
There were bug fixes in src_lheat_nudge to correct bugs when applying bright band detection. This also includes a tuning of the parameter used for the detection. These fixes will change the results for LHN analysis.
The default value of namelist parameter nradar has been changed to 33 to consider the additional radar station "MEM" which will be operational soon.
Group | Name | Meaning | Default |
---|---|---|---|
/NUDGING/ | mqcorr92 | switch for bias correction for Vaisala RS92
|
0 |
There were the following changes for the Namelist variables:
Group | Name | Meaning | Default |
---|---|---|---|
/DYNCTL/ | lva_impl_dyn | eliminated | - |
y_vert_adv_dyn | string to specify the vertical advection scheme in the Runge-Kutta dynamics:
|
'impl2' | |
/NUDGING/ | mqcorr92 | switch for bias correction for Vaisala RS92
|
1 |
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Due to the bug fixes in the latent heat nudging the result will change for LHN analysis
(for COSMO-DE).
The bias correction also causes a change in results. The analysis will become
wetter during day time and drier during night time (if mqcorr92 set to 2).
In case of mqcorr92=0 results do not change.
6. Changes of Results