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Active and passive microwave remote sensing of precipitation at high latitudes R. Bennartz - M. Kulie - C. O’Dell (1) S. Pinori – A. Mugnai (2) (1) University of Wisconsin – AOS – Madison,WI - USA (2) Institute of Atmospheric Science and Climate, National Research Council, Rome, Italy
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Introduction High latitudes and why study light rain snow Modeling Strategy Light snow/rain validation database Case study Light snowfall event from radar Satellite-model comparison UW-NMS mesoscale model comparison Sensitivity of the MW frequencies to perturbation in the IWC Outlook Towards GPM IPWG Outline
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SNOW AT MID-TO-HIGH LATITUDES (Figures from P. Yoe, J. Koistinen) At mid-to-high latitudes, snowfall represents a substantial portion of the precipitation. Snow to Total Precipitation Ratio Snowfall Accumulation From higher latitudes at least 90% of the precipitation occurs at rates less than 3 mm/hr and 60 % at less than 1 mm/h
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What we can observe Radar reflectivity (vertically resolved) Passive MW brightness temperatures (vertical integral)
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What we can NOT observe: Drop size distribution Ice particle density Index of refraction...
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What we can NOT observe: Drop size distribution Ice particle density Index of refraction... We need models to relate the microphysics to microwave optical properties
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What we can NOT observe: Drop size distribution Ice particle density Index of refraction... We need models to relate the microphysics to microwave optical properties And those models have to agree with all available information
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How can we trust our modeling assumptions?
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Precip microphysics model Radar reflectivites Environmental data Observed TBs Radiative transfer model Simulated TBs Compare Change microphysics How can we trust our modeling assumptions?
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X = 1X = 2 Frozen Liquid X = 0.5 Adjustable parameters: Ice density Size of ice relative to liquid particles Consistent description of Radar Refl/ Fall Speed/ Particle number concentration One Microphysics Model (Bennartz & Petty 2001)
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High latitude light snow/rain database (2002-ongoing) Radar data BALTRAD radar composites BALTRAD gauge adjustments Gotland radar volume scans Satellite data NOAA 15,16,17 AMSU-A/B AQUA AMSR-E SSMIS (if/when available) Global/regional model data: global NCEP/GFS data UW-NMS model (for selected cases)
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CASE STUDY Light snowfall over the Baltic Sea the 12-13 January, 2003. Comparing different ground- based, satellite and modelling data MODIS 15 March 2003
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2003-01-12 0130 UTC Gotland radar reflectivity (lowest scan)
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2003-01-12 0130 UTC
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Radar composite (gauge adjusted surface rain rate)
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2003-01-12 0130 UTC AMSU 89 GHz and 150 GHz NOAA-17 0107 UTC
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2003-01-12 0130 UTC AMSU 89 - 150 GHz NOAA-17 0107 UTC
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2003-01-12 0130 UTC AMSR 89 GHz AQUA 01:31 UTC
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RT : Reverse 3D Monte-Carlo with Henyey-Greenstein Phase Function, on a 2 km x 2 km x 1 km grid with 10 vertical levels. FASTEM-2 Ocean emissivity model, everywhere. 89 GHz (a) channel, at 36 GHz resolution 89 GHz (a) channel, at radar resolution
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Model vs. Observation Comparison: Little bias, reasonably good correlation. Only areas where there is precip
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3 two-way nested grids 18 hr simulation: from 12 UTC 11 January to 06 UTC 12 January 2003 3rd grid: 6 hours from 00UTC 12 Jan 6 category bulk microphysics: Cloud droplets, Rain, Pristine crystals, Snow (rimed crystals/low density graupel), Aggregated crystals, High density graupel Mixing ratios of total water and 5 hydrometeors categories are predicted: rain, graupel, snow, pristine crystals, and aggregates. Cloud water is diagnosed UW-NMS MODEL SETUP [Tripoli 1992]
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Selected two areas of similar environmental parameters (LWP,WVP). Take into account the radar beam width at ~100 km from the radar site RADAR-MODEL COMPARISON dBZ
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Relation between scattering index and 89 GHz brightness temperature for model (blue) and AMSR (red) for x=1; Relation between scattering index and 89 GHz brightness temperature for radar (red) and AMSR (black) for x=1. SCATTERING INDEX FOR PRECIPITATING AREA Red: radar Black:satellite Radar and model datasets are in good agreement, with the scattering index ranging from -5 and 20 K.
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AMSU–MODEL COMPARISON Relation between TB89-TB150 and the surface precipitation for different size ratio x for observed AMSU-B data (red) and simulated data (blue). X=1
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Where are we? Microphysics model agrees with radar observations Microphysics model agrees with passive mw observation at various scattering frequencies Surface rain rates are comparable to gauge- adjusted radar
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Channel definition for new sensors The Jacobian is defined as the partial derivative of a function: The increase the IWC of ε allow us to see the sensitivity of TBs to perturbations in hydrometeor contents.
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150 GHz is more sensitive to the IWC perturbation than the 89GHz especially in the upper levels. 89 GHz 150 GHz K / (g/m 3 )
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Potential of the O 2 -sounding channels for frozen precipitation detection 118±8.5 GHz 118±4.2 GHz 118±2.3 GHz K / (g/m 3 )
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Conclusions/Outlook Use all observable Tb dBZ to ensure consistency of microphysical assumptions in observation space Need for coordination of different groups working towards snowfall/high lat precip. using different microphysics schemes (intercomparison) -> IPWG
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Conclusions/Outlook Use all observable Tb dBZ to ensure consistency of microphysical assumptions in observation space Need for coordination of different groups working towards snowfall/high lat precip. using different microphysics schemes (intercomparison) -> IPWG Dedicated experiments necessary to better understand cloud microphysics
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Conclusions/Outlook Use all observable Tb dBZ to ensure consistency of microphysical assumptions in observation space Need for coordination of different groups working towards snowfall/high lat precip. using different microphysics schemes (intercomparison) -> IPWG Dedicated experiments necessary to better understand cloud microphysics BUT on a global scale we have to go with simple solutions for retrieval algorithms etc…
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Two more things for high latitudes We need channels that are surface blind We need GPM like radars
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Thanks
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