Abstract
In an attempt to advance the understanding of the Earth's weather and climate by representing deep convection explicitly, we present a global, four-month simulation (November 2018 to February 2019) with ECMWF's hydrostatic Integrated Forecasting System (IFS) at an average grid spacing of 1.4 km. The impact of explicitly simulating deep convection on the atmospheric circulation and its variability is assessed by comparing the 1.4 km simulation to the equivalent well-tested and calibrated global simulations at 9 km grid spacing with and without parametrized deep convection. The explicit simulation of deep convection at 1.4 km results in a realistic large-scale circulation, better representation of convective storm activity, and stronger convective gravity wave activity when compared to the 9 km simulation with parametrized deep convection. Comparison of the 1.4 km simulation to the 9 km simulation without parametrized deep convection shows that switching off deep convection parametrization at a too coarse resolution (i.e., 9 km) generates too strong convective gravity waves. Based on the limited statistics available, improvements to the Madden-Julian Oscillation or tropical precipitation are not observed at 1.4 km, suggesting that other Earth system model components and/or their interaction are important for an accurate representation of these processes and may well need adjusting at deep convection resolving resolutions. Overall, the good agreement of the 1.4 km simulation with the 9 km simulation with parametrized deep convection is remarkable, despite one of the most fundamental parametrizations being turned off at 1.4 km resolution and despite no adjustments being made to the remaining parametrizations.
Original language | English |
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Article number | e2020MS002192 |
Journal | Journal of Advances in Modeling Earth Systems |
Volume | 12 |
Issue number | 11 |
DOIs | |
State | Published - Nov 2020 |
Funding
This research used resources of the Oak Ridge Leadership Computing Facility (OLCF), which is a DOE Office of Science User Facility supported under Contract DE‐AC05‐00OR22725. Access to the simulation output can be requested by contacting OLCF Help Desk via email to [email protected] and referring to Project CLI900. This paper benefited from the close collaboration between high‐resolution simulation model benchmarking and advanced methodologies presently being developed for heterogeneous high‐performance computing platforms at ECMWF in the ESCAPE‐2 (No. 800897), MAESTRO (No. 801101), EuroEXA (No. 754337), and ESiWACE‐2 (No. 823988) projects funded by the European Union's Horizon 2020 future and emerging technologies and the research and innovation programmes. The authors thank the three anonymous reviewers for their comments, which have significantly improved this manuscript. This research used resources of the Oak Ridge Leadership Computing Facility (OLCF), which is a DOE Office of Science User Facility supported under Contract DE-AC05-00OR22725. Access to the simulation output can be requested by contacting OLCF Help Desk via email to [email protected] and referring to Project CLI900. This paper benefited from the close collaboration between high-resolution simulation model benchmarking and advanced methodologies presently being developed for heterogeneous high-performance computing platforms at ECMWF in the ESCAPE-2 (No. 800897), MAESTRO (No. 801101), EuroEXA (No. 754337), and ESiWACE-2 (No. 823988) projects funded by the European Union's Horizon 2020 future and emerging technologies and the research and innovation programmes. The authors thank the three anonymous reviewers for their comments, which have significantly improved this manuscript.
Funders | Funder number |
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ECMWF | |
EuroEXA | ESiWACE‐2, 823988, 754337 |
MAESTRO | 801101 |
Office of Science | 800897, DE‐AC05‐00OR22725, CLI900 |
European Commission | |
Horizon 2020 |
Keywords
- MJO
- atmosphere
- explicitly simulated convection
- high performance computing
- stratosphere
- winter season
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