<pre class="moz-quote-pre">Recent studies have shown that the effects of three dimensional
radiative transfer may impact cloud formation and precipitation.
While one-dimensional solvers are favoured due to their computational
simplicity, they do however neglect any horizontal energy transport.
In particular, the 1D approximation neglects 3D effects such as cloud side illumination
and the displacement of the cloud's shadow at the surface which are
relevant whenever the sun is not in the zenith.
This has a detrimental effect on the results of high resolution simulations.
3D radiative transfer has the potential to considerably change the
boundary layer dynamics, the evolution of clouds, their lifetime and
precipitation onset.
To this date, studies that investigate the influence of 3D effects on
realistic NWP settings are rare,
primarily because there haven't been 3D radiative transfer solvers
around that were fast enough to be run interactively in a forecast
simulation.
For that purpose we adapted the TenStream solver (parallel 3D radiative
transfer solver for LES) to unstructured meshes and coupled it to ICON-LEM.
We will present the new solver in the context of ICON-LEM simulations,
the methodologies used and its characteristics.</pre>