دورية أكاديمية
Vertical structure of cloud radiative heating in the tropics: confronting the EC-Earth v3.3.1/3P model with satellite observations
العنوان: | Vertical structure of cloud radiative heating in the tropics: confronting the EC-Earth v3.3.1/3P model with satellite observations |
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المؤلفون: | E. Johansson, A. Devasthale, M. Tjernström, A. M. L. Ekman, K. Wyser, T. L'Ecuyer |
المصدر: | Geoscientific Model Development, Vol 14, Pp 4087-4101 (2021) |
بيانات النشر: | Copernicus Publications, 2021. |
سنة النشر: | 2021 |
المجموعة: | LCC:Geology |
مصطلحات موضوعية: | Geology, QE1-996.5 |
الوصف: | Understanding the coupling of clouds to large-scale circulation is one of the grand challenges for the global climate research community. In this context, realistically modelling the vertical structure of cloud radiative heating (CRH) and/or cooling in Earth system models is a key premise to understand this coupling. Here, we evaluate CRH in two versions of the European Community Earth System Model (EC-Earth) using retrievals derived from the combined radar and lidar data from the CloudSat and Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) satellites. One model version is also used with two different horizontal resolutions. Our study evaluates large-scale intraseasonal variability in the vertical structure of CRH and cloud properties and investigates the changes in CRH during different phases of the El Niño–Southern Oscillation (ENSO), a process that dominates the interannual climate variability in the tropics. EC-Earth generally captures both the intraseasonal and meridional pattern of variability in CRH over the convectively active and stratocumulus regions and the CRH during the positive and negative phases of ENSO. However, two key differences between model simulations and satellite retrievals emerge. First, the magnitude of CRH, in the upper troposphere, over the convectively active zones is up to twice as large in the models compared to the satellite data. Further dissection of net CRH into its shortwave and longwave components reveals noticeable differences in their vertical structure. The shortwave component of the radiative heating is overestimated by all model versions in the lowermost troposphere and underestimated in the middle troposphere. These over- and underestimates of shortwave heating are partly compensated by an overestimate of longwave cooling in the lowermost troposphere and heating in the middle troposphere. The biases in CRH can be traced back to disagreement in cloud amount and cloud water content. There is no noticeable improvement of CRH by increasing the horizontal resolution in the model alone. Our findings highlight the importance of evaluating models with satellite observations that resolve the vertical structure of clouds and cloud properties. |
نوع الوثيقة: | article |
وصف الملف: | electronic resource |
اللغة: | English |
تدمد: | 1991-959X 1991-9603 |
Relation: | https://gmd.copernicus.org/articles/14/4087/2021/gmd-14-4087-2021.pdf; https://doaj.org/toc/1991-959X; https://doaj.org/toc/1991-9603 |
DOI: | 10.5194/gmd-14-4087-2021 |
URL الوصول: | https://doaj.org/article/b84c70392788409fbbb963a0ccdd121b |
رقم الأكسشن: | edsdoj.b84c70392788409fbbb963a0ccdd121b |
قاعدة البيانات: | Directory of Open Access Journals |
تدمد: | 1991959X 19919603 |
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DOI: | 10.5194/gmd-14-4087-2021 |