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Volume 9, issue 4 | Copyright
Geosci. Model Dev., 9, 1413-1422, 2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.

Model description paper 15 Apr 2016

Model description paper | 15 Apr 2016

3-D radiative transfer in large-eddy simulations – experiences coupling the TenStream solver to the UCLA-LES

Fabian Jakub and Bernhard Mayer
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Cited articles
Di Giuseppe, F. and Tompkins, A.: Three-dimensional radiative transfer in tropical deep convective clouds, J. Geophys. Res.-Atmos., 108, 4741,, 2003.
Evans, K. F.: The spherical harmonics discrete ordinate method for three-dimensional atmospheric radiative transfer, J. Atmos. Sci., 55, 429–446,<0429:TSHDOM>2.0.CO;2, 1998.
Frame, J. W., Petters, J. L., Markowski, P. M., and Harrington, J. Y.: An application of the tilted independent pixel approximation to cumulonimbus environments, Atmos. Res., 91, 127–136,, 2009.
Fu, Q. and Liou, K.: On the correlated k-distribution method for radiative transfer in nonhomogeneous atmospheres, J. Atmos. Sci., 49, 2139–2156,<2139:OTCDMF>2.0.CO;2, 1992.
Publications Copernicus
Short summary
Radiative heating or cooling plays a vital role in the evolution and lifecycle of clouds. Due to the immense computational cost of 3-D radiative transfer, today's atmospheric models usually employ crude 1-D approximations which neglect any horizontal energy transport whatsoever and may introduce non-negligible errors. This paper documents the implementation and runtime characteristics of the new TenStream solver that enables us to study 3-D effects on large domains and extended periods of time.
Radiative heating or cooling plays a vital role in the evolution and lifecycle of clouds. Due to...