ICON‐A, The Atmosphere Component of the ICON Earth System Model: II. Model Evaluation. (21st July 2018)

• Record Type: Journal Article
• Authors: Crueger, T.; Giorgetta, M. A.; Brokopf, R.; Esch, M.; Fiedler, S.; Hohenegger, C.; Kornblueh, L.; Mauritsen, T.; Nam, C.; Naumann, A. K.; Peters, K.; Rast, S.; Roeckner, E.; Sakradzija, M.; Schmidt, H.; Vial, J.; Vogel, R.; Stevens, B.
• Is Part Of: Journal of advances in modeling earth systems. Volume 10:Number 7(2018)
• Page Start: 1638
• Page End: 1662
• Publication Date: 2018-07-21
• Subjects: general circulation model; Geological modeling -- Periodicals; Climatology -- Periodicals; Geochemical modeling -- Periodicals; 551.5011
• DOI: 10.1029/2017MS001233
• Languages: English
• ISSNs: 1942-2466

Abstract

Abstract: We evaluate the new icosahedral nonhydrostatic atmospheric (ICON‐A) general circulation model of the Max Planck Institute for Meteorology that is flexible to be run at grid spacings from a few tens of meters to hundreds of kilometers. A simulation with ICON‐A at a low resolution (160 km) is compared to a not‐tuned fourfold higher‐resolution simulation (40 km). Simulations using the last release of the ECHAM climate model (ECHAM6.3) are also presented at two different resolutions. The ICON‐A simulations provide a compelling representation of the climate and its variability. The climate of the low‐resolution ICON‐A is even slightly better than that of ECHAM6.3. Improvements are obtained in aspects that are sensitive to the representation of orography, including the representation of cloud fields over eastern‐boundary currents, the latitudinal distribution of cloud top heights, and the spatial distribution of convection over the Indian Ocean and the Maritime Continent. Precipitation over land is enhanced, in particular at high‐resolution ICON‐A. The response of precipitation to El Niño sea surface temperature variability is close to observations, particularly over the eastern Indian Ocean. Some parameterization changes lead to improvements, for example, with respect to rain intensities and the representation of equatorial waves, but also imply a warmer troposphere, which we suggest leads to an unrealistic poleward mass shift. Many biases familiar to ECHAM6.3 are also evident in ICON‐A, namely, a too zonal SPCZ, an inadequate representation of north hemispheric blocking, and a relatively poor representation of tropical intraseasonal variability. Key Points: Article presents evaluation of atmosphere component of new ICON Earth system model The new MPI atmospheric ICON‐A model partly outperforms ECHAM6.3 ICON‐A is flexible to be run at grid spacings from a few tens of meters to hundreds of kilometers