Since many years it is assumed and in scientific  journals intensively discussed that turbulence, that is ubiquituous in  all types of clouds more or less in clouds, has an impact on collisions  between cloud droplets. For investigation of this effect scientists of  the Aerodynamisches Institut (AIA) of   RWTH Aachen  , the Institut für Meteorologie und Klimatologie (IMUK), Hannover,
, the Institut für Meteorologie und Klimatologie (IMUK), Hannover,  and IMK-TRO have gathered as part of the  priority program 1276 ‘Metstroem’ (meteorology and fluid dynamics) of  the German Research Foundation. In detail it is investigated which  influence of the local turbulence (in clouds) exists on the collision  efficiency of small cloud droplets and thus on the coagulation function  the latter of which is important to the physical effect of precipitation  evolution. In particular it should be clarified how the precipitation  process is altered if turbulence effects are taken into account.  Applications of the new results will be an improved (or adapted) version  of a parameterization of the coagulation function to be used in 2D  cloud model (IMUK) and in the 3D simulation of deep convective clouds by  the operational NWP model COSMO of the German Weather Service. Starting  point of the investigations which are performed mainly at AIA is a  program package that has been developed by AIA since many years and  which has successfully used for situations with technical background.  This package works with a (fluid) solver of the RANS equations  considering Cartesian hierarchically refined grids with the help of a  finite volume method. Large a number of droplets (more than 107) are  introduced in an isotropic-turbulent fluid field as passive tracers. The  turbulent flow (with certain predefined characteristics at the entrance  plane) decays on its further way. The trajectories of the droplets and  their mutual collisions are then calculated. The number of resolved  numerical cells is approximately 50 million, the time step is about less  than 10-4 s.  The drop radii considered vary between 5 and 95 microns.   First results show, relative to other independent calculations as from  Franklin et al. (2007) and Ayala et al. (2008), mostly a good agreement  for the polydisperse case. For monodisperse particles which are not  important for cloud microphysical problems a larger discrepancy appears  relative to the other investigations mentioned previously.
 and IMK-TRO have gathered as part of the  priority program 1276 ‘Metstroem’ (meteorology and fluid dynamics) of  the German Research Foundation. In detail it is investigated which  influence of the local turbulence (in clouds) exists on the collision  efficiency of small cloud droplets and thus on the coagulation function  the latter of which is important to the physical effect of precipitation  evolution. In particular it should be clarified how the precipitation  process is altered if turbulence effects are taken into account.  Applications of the new results will be an improved (or adapted) version  of a parameterization of the coagulation function to be used in 2D  cloud model (IMUK) and in the 3D simulation of deep convective clouds by  the operational NWP model COSMO of the German Weather Service. Starting  point of the investigations which are performed mainly at AIA is a  program package that has been developed by AIA since many years and  which has successfully used for situations with technical background.  This package works with a (fluid) solver of the RANS equations  considering Cartesian hierarchically refined grids with the help of a  finite volume method. Large a number of droplets (more than 107) are  introduced in an isotropic-turbulent fluid field as passive tracers. The  turbulent flow (with certain predefined characteristics at the entrance  plane) decays on its further way. The trajectories of the droplets and  their mutual collisions are then calculated. The number of resolved  numerical cells is approximately 50 million, the time step is about less  than 10-4 s.  The drop radii considered vary between 5 and 95 microns.   First results show, relative to other independent calculations as from  Franklin et al. (2007) and Ayala et al. (2008), mostly a good agreement  for the polydisperse case. For monodisperse particles which are not  important for cloud microphysical problems a larger discrepancy appears  relative to the other investigations mentioned previously.
Literature:
Kunnen, R.P.J., Siewert, C., Meinke, M., Schröder, W., Beheng, K.D., 2012: 
Numerically determined geometric collision kernels in spatially evolving isotropic turbulence relevant for droplets in clouds. 
Atmos. Res. (submitted)
 
