[1758] - Modelling convectively induced secondary circulations in the terra incognita with TerrSysMP

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Citation
Poll, S., Shrestha, P., Simmer, C., 2017. Modelling convectively induced secondary circulations in the terra incognita with TerrSysMP. QJRMS, 1 - 10. DOI: DOI:10.1002/qj.3088.
Identification
Title(s):Main Title: Modelling convectively induced secondary circulations in the terra incognita with TerrSysMP
Description(s):Abstract: Advances in high-performance computing have led to kilometre and even sub-kilometre scale regional simulations with numerical weather prediction models. This range of grid resolution – also termed ‘terra incognita’ – approaches the length-scale of the most energetic eddies of the convective atmospheric boundary layer (ABL), which accordingly can only be inadequately resolved. This dilemma becomes particularly obvious when simulating convectively induced secondary circulations (CISCs) in the terra incognita, because the modelled CISC-like circulations – also termed M-CISCs – are poorly resolved and exhibit a grid-resolution dependence. Previous studies have pointed out this problem using different modelling platforms and also suggested options for attenuating poorly resolved M-CISCs with methods specific to the applied ABL schemes. This study examines M-CISCs at horizontal grid resolutions of O(1km), using the Terrestrial Systems Modelling Platform (TerrSysMP) for idealized and real case studies. The analysis of simulations using different surface heterogeneity and grid resolutions of O(1 km) shows that the presence of a superadiabatic layer near the surface and the increase of the horizontal grid resolution allow the critical Rayleigh number to be exceeded, generating poorly resolved M-CISCs, whose amplitudes are strongly dependent on the horizontal grid resolution. We show that the asymptotic turbulent mixing length-scale in the used ABL scheme can be tuned in a way that M-CISCs are attenuated while the non-resolved turbulence dealt with by the ABL scheme effectively propagates the surface fluxes into the ABL and sustains reasonable ABL profiles.
Identifier(s):DOI: DOI:10.1002/qj.3088
Citation Advice:Poll, S., Shrestha, P., & Simmer, C., (2017) Modelling Convectively Induced Secondary Circulations in the Terra Incognita with TerrSysMP. Quarterly Journal of the Royal Meteorological Society.
Responsible Party
Creator(s):Author: Stefan Poll
Author: Prabhakar Shrestha
Author: Clemens Simmer
Publisher:WILEY
Topic
TR32 Topic:Atmosphere
Related Sub-project(s):Z4
Subject(s):CRC/TR32 Keywords: Modelling
File Details
File Name:Poll_etal_2017_RMetS.pdf
Data Type:Text
File Size:12185 kB (11.899 MB)
Date(s):Date Accepted: 2017-07-23
Mime Type:application/pdf
Language:English
Status:Completed
Constraints
Download Permission:Free
General Access and Use Conditions:According to the TR32DB data policy agreement.
Access Limitations:According to the TR32DB data policy agreement.
Geographic
North:50.8874086
East:6.5296204
South:50.5395844
West:5.980304
Measurement Region:NorthRhine-Westphalia
Measurement Location:--NorthRhine-Westphalia--
Specific Informations - Publication
Status:Published
Review:PeerReview
Year:2017
Type:Article
Article Type:Journal
Source:QJRMS
Page Range:1 - 10
Metadata Details
Metadata Creator:Prabhakar Shrestha
Metadata Created:2018-01-16
Metadata Last Updated:2018-01-16
Subproject:Z4
Funding Phase:3
Metadata Language:English
Metadata Version:V42
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