Articles | Volume 7, issue 6
https://doi.org/10.5194/gmd-7-2859-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/gmd-7-2859-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Evaluation of the ECHAM family radiation codes performance in the representation of the solar signal
T. Sukhodolov
CORRESPONDING AUTHOR
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center, Davos, Switzerland
Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland
E. Rozanov
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center, Davos, Switzerland
Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland
A. I. Shapiro
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center, Davos, Switzerland
Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland
C. Cagnazzo
Institute of Atmospheric Sciences and Climate of the Italian National Research Council, Rome, Italy
T. Peter
Institute for Atmospheric and Climate Science, ETH Zurich, Zurich, Switzerland
W. Schmutz
Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center, Davos, Switzerland
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Short summary
The performance of the main generations of the ECHAM shortwave radiation schemes is analysed in terms of the representation of the solar signal in the heating rates. The way to correct missing or underrepresented spectral intervals in the solar signal in the heating rates is suggested using the example of ECHAM6 and six-band ECHAM5 schemes. The suggested method is computationally fast and suitable for any other radiation scheme.
The performance of the main generations of the ECHAM shortwave radiation schemes is analysed in...