2021•Quarterly Journal of the Royal Meteorological SocietyRequires access

Elucidating the causes of errors in 2.2 km Met Office Unified Model simulations of a convective case over the US Great Plains

Kirsty E. Hanley, Humphrey W. Lean

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Abstract

Abstract Convective‐scale ensemble simulations with perturbed initial and lateral boundary conditions have been performed to investigate the role of compensating errors in the model representation of a US Great Plains severe convective event. The convective‐scale ensembles were generated by nesting a 2.2 km grid‐length domain within the Met Office global ensemble. Within the ensemble framework, two different science configurations (i.e. parametrization set‐ups) were trialled in the 2.2 km model. The variability due to the use of a different driving global ensemble member was significant with differences in the pre‐convective thermodynamic environment and the initiation time of convection. The science changes also influence initiation time as well as the details in the convective structure. Comparison with observed soundings showed that most of the 2.2 km simulations had too little convective inhibition (CIN). The CIN was found to be independent of the science configuration, implying it is determined by the global model, which was also found to have less CIN than the observed soundings. In both 2.2 km ensembles, the member that produced one of the best simulations of the supercells that developed on this day had more CIN than the other members. However, comparisons with surface station data found that this member had a pre‐convective environment that was too cool and too dry. This suggests there are compensating errors in the factors controlling initiation in these models which comparisons with observations can help elucidate.

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Abstract Convective‐scale ensemble simulations with perturbed initial and lateral boundary conditions have been performed to investigate the role of compensating errors in the model representation of a US Great Plains severe convective event. The convective‐scale ensembles were generated by nesting a 2.2 km grid‐length domain within the Met Office global ensemble. Within the ensemble framework, two different science configurations (i.e. parametrization set‐ups) were trialled in the 2.2 km model. The variability due to the use of a different driving global ensemble member was significant with differences in the pre‐convective thermodynamic environment and the initiation time of convection. The science changes also influence initiation time as well as the details in the convective structure. Comparison with observed soundings showed that most of the 2.2 km simulations had too little convective inhibition (CIN). The CIN was found to be independent of the science configuration, implying it is determined by the global model, which was also found to have less CIN than the observed soundings. In both 2.2 km ensembles, the member that produced one of the best simulations of the supercells that developed on this day had more CIN than the other members. However, comparisons with surface station data found that this member had a pre‐convective environment that was too cool and too dry. This suggests there are compensating errors in the factors controlling initiation in these models which comparisons with observations can help elucidate.

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Available abstract

Abstract Convective‐scale ensemble simulations with perturbed initial and lateral boundary conditions have been performed to investigate the role of compensating errors in the model representation of a US Great Plains severe convective event. The convective‐scale ensembles were generated by nesting a 2.2 km grid‐length domain within the Met Office global ensemble. Within the ensemble framework, two different science configurations (i.e. parametrization set‐ups) were trialled in the 2.2 km model. The variability due to the use of a different driving global ensemble member was significant with differences in the pre‐convective thermodynamic environment and the initiation time of convection. The science changes also influence initiation time as well as the details in the convective structure. Comparison with observed soundings showed that most of the 2.2 km simulations had too little convective inhibition (CIN). The CIN was found to be independent of the science configuration, implying it is determined by the global model, which was also found to have less CIN than the observed soundings. In both 2.2 km ensembles, the member that produced one of the best simulations of the supercells that developed on this day had more CIN than the other members. However, comparisons with surface station data found that this member had a pre‐convective environment that was too cool and too dry. This suggests there are compensating errors in the factors controlling initiation in these models which comparisons with observations can help elucidate.

Key concepts: Parametrization (atmospheric modeling), Convection, Ensemble forecasting, Convective available potential energy, Meteorology, Scale (ratio), Environmental science, Convective inhibition

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