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![Page 1: Click to add Text © Crown copyright Met Office Statistical Analysis of UK Convection and its representation in high resolution NWP Models Humphrey Lean,](https://reader035.fdocuments.in/reader035/viewer/2022062518/56649ece5503460f94bdb794/html5/thumbnails/1.jpg)
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© Crown copyright Met Office
Statistical Analysis of UK Convection and its representation in high resolution NWP ModelsHumphrey Lean, Kirsty Hanley, Carol Halliwell
MetOffice@Reading, Reading, UK
Robin Hogan, Thorwald Stein, Bob Plant, Peter Clark
University of Reading, Reading, UK
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Introduction
• “Convection permitting models” (i.e. those with explicit convection) have provided a step change in our ability to forecast on smaller scales.
• Here describe work to improve our understanding of representation of convection in these models.
• Not a trivial question. Just running at higher resolution is not necessarily a panacea. Although there is no convection scheme we have to think about the representation of other subgrid processes.
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Model resolution
• Current highest resolution operational UK configuration 1.5km (UKV model)
•For research we are running higher resolution versions of the Unified Model down to 100m (55m for London)
• Helps understanding of convection permitting versions of model to look as function of gridlength.
• Also looking to future. Higher resolution very expensive but also interest in high res models of small areas (e.g. Weymouth 333m for Olympics, London 333m).
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Heathrow downscaler from UKV
300 x 200
333m resolution
70L
10 second timestep
Run twice a day at 03Z and 09Z
Run to T+36
Clive Wilson, Anke Finnenkoetter
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“UKV” 1.5km UK Model convection1.5km model Radar
15 UTC 12th April 2012
•Convective cells too large and too intense. •Not enough light rain.
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Average cell diameter (km)(averaged over 22 convective cases)
Threshold (mm/hr)
Radar 1.5km UKV
0.125 7.81 16.04
0.25 6.32 13.21
0.5 5.58 11.71
1.0 4.42 9.93
2.0 3.28 7.95
4.0 2.57 5.96
16.0 2.13 3.37
6
UKV Under-resolvedCurrently investigating shallow scheme rather thantrying to resolve smaller showers.
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Gridscale structure in 750 hPa w13UTC 12/05/2010 – case of light scattered showers
4km 1.5km 500mEmilie Carter
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100m UM versions
• Cold pooling in valleys COLPEX (Clark, Vosper, Carter)
• London (Lean)
• Convection (Carter, Halliwell, Hanley)
•Tornadoes (Hanley)
• StCu (Boutle)
• Fog inc nesting in ensemble (Porson)
• (Also 333m Weymouth model for Olympic sailing and 333m London model (fog)).
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Comparison with observations
Temp RH
Wind speed Wind dir
Emilie Carter
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COPE IOP 2 July 5 2013 sea breeze convergence
Different scale!
Vertical velocity at 500m amsl
Below 500m starting to resolve BL turbulence
K Hanley
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DYMECS project
• DYnamical and Microphysical Evolution of Convective Storms (DYMECS).
• Statistical analysis of convective cells with Chilbolton Radar over a number of cases.
• Compare to UM configurations between 1.5km and 100m
• R Hogan, Plant, Stein, Nicol, Clark University of Reading
• Lean, Halliwell, Hanley MetOffice@Reading
Also in summer 2013 had field phase of COPE (COnvective Precipitation Experiment) which will be used for similar analysis and model comparisons.
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The DYMECS approach: beyond case studies
Met Office 1km rainfall composite
Track storms in real time
and automatically
scan Chilbolton
radar
Derive properties of hundreds of storms on ~40 days:Vertical velocity3D structureRain & hailIce water contentTKE & dissipation rate
Evaluate these properties in model varying:Resolution (down to 100m)Microphysics schemeSub-grid turbulence parametrization
25m diameter S-band (3 GHz)Steerable (2 degrees per second)
0 dBZ out to 150 km
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Model Differences
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2.2km 1.5km
200m 100m 1km RADAR
500m4km
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Convective cell life cycle
Thorwald Stein
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20 April 2012 25 Aug 2012
100m model best
500m model best
1.5km model best
11 UTC - radar 15 UTC - radar
Surface rainrate statistics
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Cloud widths for different reflectivity thresholds.
Radar Distance (km) 1.5km 500m
200m 100m
Thorwald Stein
Median width of deep storms25th Aug 2012
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25 Aug 2012
Cutaway: reflectivity Surface: rainrateShading: extent of cloud
Robin Hogan
3D visualisation of data
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Reflectivity
Actual model vertical velocity
Estimated vertical velocity
Observations UKV 1500m Updraft Updraft retrievalretrieval
10 km height
20 km width
40 dBZ
+10 m/s
-10 m/sEstimate vertical velocity from vertical profiles of radial velocity, assuming zero divergence across plane.
Quantify errors due to 2D flow assumption
John Nicol
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Vertical distribution of vertical velocity and reflectivity
Observations
1500m
500m
200m
100m
John Nicol
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Vertical distribution of vertical velocity and reflectivity
John Nicol
Vertical velocity and reflectivity distributions as function of radius from centre of updrafts. Set to zero where: w<1m/s, Z<20dBZ.
1200-1600UTC 25/08/12. Black traces - mean widths for 1m/s and 20dBZ.
N.B. higher values of Z than before - rain
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Vertical distribution of vertical velocity and reflectivity
John Nicol
Vertical velocity and reflectivity distributions as function of radius from centre of updrafts. Set to zero where: w<1m/s, Z<20dBZ AND where values start increasing again.“primary profile”
1200-1600UTC 25/08/12. Black traces - mean widths for 1m/s and 20dBZ.
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Vertical velocity and reflectivity as a function of gridlength.
John Nicol
Observations
1500m
500m
200m
100m
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Vertical velocity and reflectivity as a function of gridlength.
John Nicol
Observations
1500m
500m
200m
100m
Updrafts fit best at about 200m – definitely too narrow at 100m
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Vertical velocity and reflectivity as a function of gridlength.
John Nicol
Observations
1500m
500m
200m
100m
Primary (monotonic) cloud widths proxy for updraft width
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Vertical velocity and reflectivity as a function of gridlength.
John Nicol
Observations
1500m
500m
200m
100m
Non monotonic profiles of Z too narrow in 100m and 200m (tallies with cloud and rain data).
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Vertical velocity and reflectivity as a function of gridlength.
John Nicol
Observations
1500m
500m
200m
100m
Obs show bigger increase from dropping the monotonic condition than any model. Fits with cloud not correctly filling in between updrafts.
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25 Aug 2012
Cutaway: reflectivity Surface: rainrateShading: extent of cloud
Robin Hogan
3D visualisation of data
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Mixing length dependence
John Nicol
radar
200m l=300m
200m l=100m
200m l=40m
Smaller mixing length lower vertical velocity (but more cells)
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• Can we make the 200m model produce larger storms on 25th Aug 2012 by changing the mixing length?
• Need to reduce the timestep to 3s to avoid hitting stability limit.
• Can produce larger storms but at the expense of the smaller storms.
• Increasing the mixing with height may be a solution i.e. make Smagorinsky scheme dependent on Δz.
Varying the mixing length
l=300m – 2491 stormsl=100m – 3583 stormsl=40m – 4359 storms
200m
Kirsty Hanley
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Variation with microphysics
John Nicol
Observations
aggregates
graupel
default
Melting level at 2.6km.
Hypothesise differencedue to fall speed.
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Conclusions• UKV clearly under-resolves many small showers in UK
• High res models (~100m) improve some aspects but also some problems.
• Models below 500m tend to produce too narrow showers (measured by surface rain or cloud) in cases where showers are large (for small showers 200m or 100m fits well). Cloud widths roughly the same in 200m and 100m.
• Updraft widths good in 200m model but too narrow at 100m.
• Above two together imply there may be an issue about how the model fills in cloud between updraft cores.
• Representation very sensitive to mixing. Also sensitivity to microphysics (fall speed).
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Future work
• What can be done to understand lack of convergence and too narrow updrafts/clouds in 100m/200m models?
• Suspect problem is turbulence “grey zone”. Would better resolution of turbulence solve these problems at higher resolution? Try higher vertical/horizontal resolution and see if updrafts/clouds get wider (or stop collapsing). Work with LES community.
• Can we improve models with more appropriate subgrid mixing schemes?
• Effect of microphysics?
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DYMECS References
Hanley, K. E., Plant, R. S., Stein, T. H. M., Hogan, R. J., Nicol, J. C., Lean, H. W., Halliwell, C. and Clark, P. A. (2014), Mixing-length controls on high-resolution simulations of convective storms. Q.J.R. Meteorol. Soc.. doi: 10.1002/qj.2356
Stein, Thorwald H. M., Hogan, Robin J., Hanley, Kirsty E., Nicol, John C., Lean, Humphrey W., Plant, Robert S., Clark, Peter A., Halliwell, Carol E. (2014), The three-dimensional morphology of simulated and observed convective storms over southern England. Mon. Wea. Rev.. doi: 10.1175/MWR-D-13-00372.1
Stein, Thorwald H. M., Hogan, Robin J., Clark, Peter A., Halliwell, Carol E., Hanley, Kirsty E., Lean, Humphrey W., Nicol, John C., Plant, Robert S., (2014), The DYMECS project: A statistical approach for the evaluation of convective storms in high-resolution NWP models. (submitted to Bull. Amer. Meteorol. Soc.).
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Thank you for listening.Any questions?