Documentation of the Changes in the COSMO-Model
Version 4.27

13.03.2013

This version again is a consolidation version. There are more adaptations for the new fast waves solver and several technical changes. Two bugs have been fixed in the Runge-Kutta advection schemes and, as a bigger technical change, the interface for the MESSy system have been implemented with ifdefs.

Contents:

  1. Adaptations for the new Fast Waves Solver
  2. Advection in the Runge-Kutta scheme
  3. Bug Fix in the Microphysics
  4. More Adaptations in the Nudging Code to the 14-digit date format
  5. Implementation of MESSy Interfaces
  6. Problems with conditional compilation
  7. Bug Fixes and Technical Changes
  8. Changing default values for several Namelist Variables
  9. Changes to the Namelists
  10. Changes of Results


1. Adaptations for the new fast waves solver

(by Michael Baldauf)

Again, there has been some consolidation work in the new fast-waves solver. The changes are:

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2. Advection in the Runge-Kutta scheme

(by Michael Baldauf, Andreas Will)

There have been two corrections in the Runge-Kutta advection scheme (in module src_advection_rk.f90), which do change the results:

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3. Bug Fix in the Microphysics

(by Felix Rieper)

In the microphysics, several physical coefficients have been modified, which were wrongly initialized:

Also, the values of variables zcsdep, zsamel have been adapted to lately modified diffusion coefficient zdv in the cloud ice scheme hydci_pp

These changes affect the results of COSMO_EU and COSMO_DE.

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4. More Adaptations in the Nudging Code to the 14-digit date format

(by Christoph Schraff)

Several places still had to be adapted to the use of the 14-digit date format. This includes the fact that the new version now writes VOF Version 4:
Affected modules are:

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5. Implementation of MESSy Interfaces

(by Astrid Kerkweg, et al., University of Mainz)

Interfaces have been implemented to use the COSMO within the "Modular Earth Sub-System" (MESSy). Especially, the use within this system requires a special treatment of tracers. All changes have been introduced using conditional compilation with the pragma -DMESSY.

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6. Problems with conditional compilation

(by Uli Schättler)

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7. Bug Fixes and Technical Changes

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8. Changing default values for several Namelist Variables

The defaults of some Namelist parameters have been modified, mainly to reflect now the usage of the Runge-Kutty dynamical scheme with the new fast-waves solver as standard. If values are different depending on the horizontal resolution, most values now reflect the settings of COSMO-EU application (with 7 km) at DWD.

Group Parameter New Default Old Default
/TUNING/ v0snow 25.0 20.0
wichfakt 0.0 0.15
tkhmin 0.4 1.0
tkmmin 0.4 1.0
/DYNCTL/ l2tls .TRUE. .FALSE.
iadv_order 3 5
itype_fast_waves 2 1
itype_bbc_w 114 1
l_diff_Smag .TRUE. .FALSE.
y_scalar_advect BOTT2_STRANG SL3_MF
lexpl_lbc .TRUE. .FALSE.
rlwidth 85000.0 50000.0
nrdtau 5 10
ldiabf_lh .TRUE. .FALSE.
hd_corr_u_in 0.25 1.0
hd_corr_u_bd 0.25 1.0
hd_corr_t_in 0.0 0.75
hd_corr_t_bd 0.0 0.75
hd_corr_p_in 0.0 0.75
hd_corr_p_bd 0.0 0.75
hd_corr_trcr_in 0.0 0.5
hd_corr_trcr_bd 0.0 0.5
/PHYCTL/ limpltkediff .TRUE. .FALSE.
lsso .TRUE. .FALSE.
lseaice .TRUE. .FALSE.
lexpcor .FALSE. .TRUE.
nincconv 4 10

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9. Changes to the Namelists

There were no changes to the Namelists.

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10. Changes of Results

The results of COSMO_EU and COSMO_DE are influenced by the following modifications:

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