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ICE-POP WORKSOP Sep 5-9 2016, Korea
FOG FORMATION, DEVELOPMENT AND DISSIPATION: MEASUREMENTS AND VARIABILITY Ismail Gultepe Cloud Physics and Severe Weather Research Section, Science and Tech Branch, Environment Canada, Toronto, Ontario, M3H5T4 ICE-POP WORKSOP Sep , Korea
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Objectives Classify fog types Evaluate instruments for Vis
Emphasize variability, scale issues
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VIS reduction due to fog particles
Vis=f(Vrh;Vmix;Vliquidfog;Vicefog; Vdrizzle;Vrain;Vsnow;Vblows)
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Vis versus Nd
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Vis versus LWC
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VIS VERSUS f(LWC;Nd)
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Vis parameterization RUC Vis Fixed LWC
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FOG MICROPHYSICAL PARAMETERIZATION MATERHORN 2015 JAN
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Ice crystal shapes Jan 28 2010 Jan 28 2010 March 7 2010 March 4 2010
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Fog Formation Saturation wrt water or ice CCN and IN nuclei
Nd=f(CCN;Sw) Ni-f(IN, Si)
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Fog Development When air parcel has enough CCN(IN) and RH~100% or >100%, droplets (ice crystals) form. Development or fog intensity increases with increasing Nd(Ni) or LWC(IWC) It happens when a cooling processes occurs and IN or CCN increases Cooling occurs due to advection, radiation, subsidence, mixing, precipitation, upslope etc.
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Fog Dissipation Dissipation of fog happens due to =precipitation,
=mixing with warm and dry air, and =heating processes such as SW heating and warm air advection.
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MATERHORN 2015 ICE FOG DISSIPATION
MATERHORN: Mountain Terrain Atmospheric Modeling and Observations Project
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Visibility Instruments Based on extinction of visible light using forward and backscattering techniques
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VIS FOR ICE FOG CONDITIONS
1.7 KM 0.3 KM 0.5 KM
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Microphysical sensors
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Variability in Measurements
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Comparisons of Vis for snow conditions
FD12P SENTRY
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Comparisons of snow PR
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SWE SENSOR amount water in snow layer
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Variability/Uncertainty in Model Predictions
SCALE ISSUES MICROPHYSICAL SCHEMES VISIBILITY PARAMETERIZATIONS UNCERTAINITY IN THE BOUNDARY CONDITIONS
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MODEL VIS-SCALE ISSUES
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LWC comparisons at various
forecast hours
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Vis versus RHw 5% accuracy of RHw measurements is needed.
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VIS-PRrain
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CONCLUSIONS Multiple sensor approach (MSA) is needed to measure same physical parameter (e.g. precip rate, extinction…) Multiple model runs/ensemble simulations at different initialization times are needed because of variability in the predicted microphysical parameters. Microphysical parameterizations are needed to be improved Observational based nowcasting schemes are needed.
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