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.
Development and technical paper
| 
03 Dec 2014
Development and technical paper |
| 03 Dec 2014
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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- The SOLAR-HRS New High-Resolution Solar Spectra for Disk-Integrated, Disk-Center, and Intermediate Cases M. Meftah et al. 10.3390/rs15143560
- Future Climate Under CMIP6 Solar Activity Scenarios J. Sedlacek et al. 10.1029/2022EA002783
- The representation of solar cycle signals in stratospheric ozone – Part 2: Analysis of global models A. Maycock et al. 10.5194/acp-18-11323-2018
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- The role of methane in projections of 21st century stratospheric water vapour L. Revell et al. 10.5194/acp-16-13067-2016
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Latest update: 23 Nov 2024
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...
