The Variable Structure of Convection at Low Latitudes

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Presentation transcript:

The Variable Structure of Convection at Low Latitudes Robert A. Houze, Jr. TRMM Celebration, Baltimore, 13 July 2015

TRMM Instruments Important! Radar measures 3D structure of radar echoes PR: Precipitation Radar λ = 2 cm λ= 2 cm > Recall TRMM PR samples a 3D volume. We can plot a histogram showing frequency of occurrence of reflectivity values at each altitude. Kummerow et al, 1998

Re-map and interpolate the PR reflectivity field Satellite Geolocate Interpolate

Use remapped interpolated data to: View PR data in visualization software Objectively identify 3D echo objects indicative of convective lifecycle stage

TRMM algorithm subdivisions Convective Stratiform Other TRMM algorithm subdivisions

Convective cores land echo core Type Threshold Width Height 3D convective echo bounded by threshold dBZ Type Threshold Width Height Shallow-isolated 17 dBZ 2 pixels < 5 km Deep-strong 40 dBZ >10 km Deep-moderate 30 dBZ > 8 km Wide-strong >1000 km2 Wide-moderate >800 km2 First we will look at echoes identified as “convective” byTRMM. To do this—identify 3D echo “cores” that are EMBEDDED in larger echoes Deep cores—associated with young, extremely vigorous convection Wide cores—indicate where intense convection is aggregating and growing upscale into mesoscale systems Two categories—we find strong categories are better indicators of processes over land, moderate better over oceans Shallow isolated—are generally warm rain showers or small cumulonimbus clouds—fall into the category of “congestus”

Shallow-isolated and Strong-deep in DJF Sample of results Because of time limitation—showing only DJF Shallow isolated echoes—are an oceanic phenomenon Deepest, most intense, embedded cores--continental

Deep and Wide in DJF As noted…wide cores are those growing upscale This shows Mesoscale development much more widespread than the occurrence of extremely deep/intense convective core occurrence Close correspondence of moderate deep conv. cores and mesoscale development The rainiest regions—Amazon, MC, & Gulf coast—have mesoscale development from mostly moderately deep & intense convection

Broad stratiform regions Look for ones that are broad and contiguous Stratiform echo volume land First we will look at convective echo structure in the TRMM data. To do this— identify 3D echo “cores” Type Width Strong > 50,000 km2 Moderate > 30,000 km2

Wide Convective and Broad Stratiform in DJF Broad stratiform regions Manifest in regions of wide convective cores, i.e. where mesoscale aggregation & organization occur—globally Manifests more strongly over oceans—wherever mesoscale organization is happening Over land regions where the most intense deep & wide convective systems occur, stratiform development is not especially strong. Over semi-oceanic regions—Amazon, MC, and Gulf, BRSs manifest more strongly than regions where mesoscale conv. aggregation manifests most strongly

Regions of Frequent Broad Stratiform Looking at BSRs in both winter & summer in both hemispheres— Several regimes: warm pool, monsoonal ITCZ, frontal, plum

Visualization software views of broad stratiform region echoes West Pacific Km Visualization software views of broad stratiform region echoes Bay of Bengal 12 Height (km) 8 4 Km Frontal system Km

Lifecycle stages of convection seen by TRMM Convective cores Shallow isolated echoes—oceanic Deep intense cores—continental Upscale growth of convection (“aggregation,” “organization”) Associated with less deep & intense conv. Cores Stratiform development Wherever mesoscale aggregation occurs Mostly oceanic and semi-oceanic Less strong over land regions—where convection is strongest Stratiform structure Mesoscale system type—over open tropical oceans Weak cellular form—in ITCZ and monsoonal coastal regions Frontal—over subtropical oceans

trmm. atmos.washington.edu For more details, see: Houze, Rasmussen, Zuluaga, and Brodzik (2015, Reviews of Geophysics, in minor revision) And our new web portal: trmm. atmos.washington.edu

This research is supported by: NASA grant NNX13AG71G END This research is supported by: NASA grant NNX13AG71G