JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 101,NO. D14, PAGES 18,961-18,977,AUGUST 27, 1996 Microphysical and electrical evolution of a Florida thunderstorm 1. Observations JeffreyR. French, • JohnH. Helsdon,AndrewG. Detxvilcr,andPaulL. Smith Instituteof Atmospheric Sciences, SouthDakotaSchoolof MinesandTcchnology• RapidCity Abstract. This studydealswith the microphysical and electricalevolutionof a thunderstorm that occurredon August9, 1991,duringthe Convection andPrecipitationf Electrification(CAPE) Experimentin easternFlorida. During its approximately1-hourlifetime,the stormwaspenetratedseveraltimesby the Instituteof AtmosphericSciences' T-28 aircraftat midlevels. It was alsopenetratedat low andmiddle-levels by a NationalOceanographic and AtmosphericAdministration(NOAA) P-3 and scanned by threeradars,oneof whichhad multiparameter capabilities,operatedby the NationalCenterfor Atmospheric Research.Two stagesof the storm's evolutionare analyzedhereinduringwhichthe stormgrewto produceprecipitationandlightning. The first stage,sampledduringthefirst T-28 penetrationat 5.25 km (-3øC) andthe P-3 at 6.4km(-10øC),wascharacterized bya 2- to3-kinwideupdraft (maximum 14m s'•) withcloud liquidwatercontents upto4 g m-3,lowconcentrations ofgraupel at-10øC,andsmalltomedium raindrops in concentrations oflessthan200m-3at-3øC. A downdraft region alsoexisted that wasdevoidof cloudliquid water,but containedgraupelup to 2 mm. Radardata(Zr)•) are consistent with a coalescence-dominated precipitationgenerationmechanismfollowedby transportof dropsin theupdraftto heightswith temperatures colderthan-7øC, wherefreezingformedgraupel that continuedto growby riming. Electrificationduringthis stageremainedweak. The secondstage,sampledduringthe secondandthird T-28 penetrations andthe secondP-3 penetration, wascharacterized at midlevelsby a narrowerupdraftanda morediffuse,broaddowndraft separated by a 1- to 2-km wide transitionzone. The updraftcontinuedto showsignificantcloud liquidwater(•2 g m-3)withfewprecipitation particles, whilethedowndraft hadverylittlecloud liquidwithgraupel in concentrations >1 e-•. Thetransition zoneshared bothupdraft anddowndraft characteristics.The increasein ice concentration wasaccompanied by a rapid increasein theelectrification ofthecloudwithpeakelectric fieldsreaching-20 kV m-• atT-28altitude and thedetection of lightningby ground-based sensors andpilotreport. As timeprogressed, precipitationparticleconcentrations reachedseveralper liter at midlevelsin bothupdraftsand downdrafts. The observations areconsistent with electrification througha precipitation-based mechanisminvolvingthe development of the ice phase. 1. Introduction and large-scale separation togravitational sorting oftheparticles. Questions dealing withtheelectrical natureof thtmderclouds Thistheory hasbeenexplored tbrvirtually all typesofhydromehavebeenpuzzling atmospheric scientists forcenturies, yetmost teorcollisions [e.g.,LathamandMason,1962;Attfdetynattr and majoradvances in thefieldhavecomein onlythelastfewdec- Johnson, 1972;Brooks andSaunders, 1994].Thenoninductive ades.Despite these advances, manyquestions concerning chargehypothesis hasbeendeveloped through a setof laboratory exstructure, mechanisms for charge separation, andelectrical el- periments datingbackto Reynolds et al. [1957]. It hasbeen fectsona thunderstorm's microphysical evolution remainlargely shown[e.g.,Reynolds et al., 1957;Church,1966;Takahashi, um'esolved. 1978a;Jayaratneet al., 1983'Saunders et al., 1991]thatcharge It is unclear at thistimeexactly whichmechanisms arepri- will betransferred during rebounding collisions between graupel marilyresponsible fortheelectrification of thunderstorms. The andsmallerice crystals in thepresence of supercooled water. convective hypothesis, firstproposed byGrenet [1947]andlater Large-scale chargeseparation thenresultsfromgravitational byVonnegut [1953], attributes charge separation tothemotion of separation ofthetwodifferent-sized hydrometeor species. A recharged cloud particles andsmall ions inthecloud updraft andin viewofthese theories along withtheirstrengths andwealo•esses thedowndraft atitsedges. Theinductive hypothesis, originallyinexplaining observed electrical characteristics ofthunderstorms proposed byElsterandGeltel[1913]forraindrop/cloud dropletisgiven bySaunders [1993,1995]. Recently,severalfield investigations involvingboth remote collisions,attributeschargetransferto the interactionof polarand in situ measurements have been mounted to characterize the ized hydrometeorsin the presenceof an ambientelectric field microphysical and electricalstateof convectivecloudsin orderto •Now at Department of Atmospheric Sciences, University of Wyoming, Laramie. Copyright1996 by the .tunerican Geophysical Union. cal stormssuchas occuralongthe eastcoastof Florida. Studies of subtropical stormshaveinvolvedradaranalysisandgroundbased electric field data to infer the interior electrical structure of Papernumber96JD01625. 0148-0227/96/96JD-01625 shedlightonthequestion of chargeseparation. It is noteworthy thatrelativelyfew of theseinvestigations havestudiedsubtropi- $09.00 the thunderstorms [e.g., ,lacobsonand Krider, 1976; Krehbiel, 18,961 18,962 FRENCH ET AL.' OBSERVATIONS OF EVOI.UTION OF A THUNDERSTORM 1981, 1986; Krider, 1989; Lhet•itte and Williams, 1985; 34aier and Krider, 1986;3•lurphyet al., 1996]. The resultshavecharacterizedthe electricalstructureof thesestorms(basicallytri-polar) without characterizingthe accompanying microphysics to aid in identifyingthe electrificationprocesses. Somestudieshave obtainedin situ electricaland microphysical datafromsubtropical andtropicalclouds. Talcahashi [1978b] made balloon-borne,large-hydrometeor chargemeasurements in two maritime thunderstom•s near Penape,Micronesia. They exhibited different degreesof electrificationcorrelatedwith lightningproduction.One storm,sampledprior to the initiation detennineboththe microphysical and electricalevolutionof the storm. In section2 we discussthe collectionandanalysisof the datafrom the August9 storm. Section3 coversthe resultsof the data analysis. Section4 summarizesthe observations, and sec- tion 5 discusses how our restiltsshedlight on the questions raisedearlierin comparison with otherstudies. A companion paperdealswith the numericalsimulationsof this storm. 2. Data Set Two main data setswere usedin the analysisof this storm. Data collectedby radarsconstitutethe first set. The secondset of lightning, hadcharges ofbothsigns at levelsfroin0 to-60øC comprises in situmeasurements madeusinga varietyof probes with a slightexcessof positivechargeat warmertemperatures on boardinstrumented aircraft. The majorityof the in situ data and net negative charge at colder temperatures,reachinga was collectedby the SouthDakota Schoolof Mines and Technolmaximum aroundthe -40øC level. The secondstorm was al- ogy T-28. Data collectedby the National Oceanicand Atmosreadyproducinglightningat the time it was sampled.This storm phericAdministration's (NOAA) P-3 werealsoanalyzed.Since had a more distinct tri-polar structurewith the net negative ourviewof theevolutionof thisstormis highlydependent onthe charge peaking at around-20øC.Takahashi inferred fromthese interpretation of thesedata,we t•cl it necessary to discuss the data that the tipper positivechargewas carriedby ice crystals measurement devicesusedandhowmeasurements madeby each and the main negativechargewas carriedon graupel,whichhe devicewere interpreted. foundto be consistent with thenoninductive rimingmechanism. 2.1. Radar Measurements Takahashi[1990] flexva balloon-borneparticleimagingsystem, correlatinglow lightningfrequencyxvithlow graupelconThe stormonAugust9 wascontinually scanned by threeNacentrationsbelow the -30øC level, and highergraupelconcen- tionalCenterfor Atmospheric Research(NCAR) radars,CP-2, trations,but lack of liquid water above the -30øC level. This CP-3, and CP-4. Figure 1 showsthe locationof the stormin relack of collocatedgraupeland liquid water wouldproduceweak lation to the radar installations, Cape Canaveral,and the Melelectrificationvia a noninductive rimingprocess. bourneAirport. Boththe CP-3andCP-4DopplerradarsoperGoodmanet al. [1989] useda polarization-diversity radar in atedin the C band,at wavelengths of 5.45 cm and 5.49 cm, reAlabamato examinecloudsthat were maritimein nature. They spectively.During the August9 storm,the antennafrom CP4 foundthatlightningoccurred onlyaftersignificant concentrationshad elevationcontrolproblems.Becauseof this, the radardata of ice were intbrredto have formedbasedon multiparameterra- discussed in the followingsections comefromeitherthe CP-3 or dar signatures. Willis et al. [1994] obtainedobservations l¾om the CP-2 radar. aircraftpassesthrougha thunderstormduringCAPE. Electrified regionsat the-7 ø to-10øC level within this storm contained graupel,relatively little cloud water, and either downdraftor a :..Atlantic • • • ' I CP-2 relative minimumwithin an updraft. The synthesisof theseob. ';:'•Ocean . servationssuggestthat ice formationis a precursorto significant :--:;:..::':.:'!:::i":"." ":' electrificationin subtropicalmaritimestorms. In a studysimilar to the one describedbelow,Ramacha•drcm et al. [1996] examinedtwo stormson the sameday duringCaPE usingaircraftand multiparameterradar data. Both stormswere in closeproximityspatiallyand temporallyand both exhibiteda multicellularcharacter.Both stormsshoweddevelopment of icephaseprecipitationthroughthe freezingof supercooled raindrops and the growthof electric fieldsto tensof kV in'• at the6 kin (-6øC) level subsequent to the initiation of ice. While the aircraft-measuredelectric fields were of coinparablemagnitudein bothstorms,onlythe moredynamicallyvigorotiscellsin the secCP-4 Melbourne ond stormproducedlightning. In each of thesecells, the time betweenthe first freezingof rain and first lightningwas between 10 and 12 min. They concludedthat the observations were consistentwith a chargingmechanisminvolvingcollisionsof cloud and precipitationparticlesin regionswith modestamountsof cloudwater abovethe 6-kin level. Electrifichtionto the stageof lightningwas dependentuponthe vigor of the updraftsand the maximumdepthof the cloud. In this anda companion paper,xvetry to shedadditionallight Figure 1. Locationof August9 CaPE stormin relationto radar on the relation betweenthe microphysics and electrificationof sitesandMelbourneAirport(baseR)rT-28). The stipplingindisubtropicalstormsthroughthe analysisof both observational cateswater. To the far right (east) is the Atlantic Ocean. The data and an associatedmodelingstudy. In this paper, xvedeal outer banks (Cape Canaveral)are separatedfrom mainland specificallyxviththe analysisof in situ and remotelysensedob- Florida by the Bananaand Indian Rivers. The scanarea indiservationaldata from a thunderstonnthat occurredon August9, catesthe regionin whichthe radarswere scanningfor this par1991, duringCAPE. The datawere analyzedin detail in orderto ticularstorm.ModifiedfromFoote[ 1991]. CP-3 FRENCH ET AL.: OBSERVATIONS OF EVOLUTION OF A THUNDERSTOILM The CP-2 was a dual-wavelengthradar with multiparameter capabilities.It operatedsimultaneously in boththe S bandand the X band,corresponding to wavelengths of 10.68 cm and 3.20 cm, respectively.Both bandswere able to providereflectivity andDopplerdata. In addition,the S bandchannelprovideddifferentialreflectivity,ZD}•,and the X bandprovidedlinear depo- 18,963 with respectto the Earth's surfaceand the componentthat is perpendicularto the plane'sheadingand horizontalwith respect to the Earth's surface. Willis et al. [1994] describethe method used to calculate the electric field based on measurements from the field meterson boardthe P-3. Contraryto the sign convention used by Willis et al., in this discussiona positive vertical electricfield (z component)rel•rs to net negativechargeabove larizationratio (LDR). ReflectivitydatacollectedfromCP-2 were comparedto those the aircraft,and a positivehorizontalelectricfield (y component) collectedfrom CP-3, andthe two datasetscomparedwell in both refersto net negativechargeto the rightof the aircraft'sflight distructureand value even thoughthe CP-3 data usedare raxvre- rection. This sign conventioncorresponds to a right-handedcoflectivity data, while the CP-2 data are griddedand smoothed. ordinatesystemin which the positivex direction(a component Bothreflectivityfieldswerethereforeusedin tile analysisof this not resolvedin the electricfield calculations)pointsout of the storm. In addition,we analyzedtile difl•rential rellectivityfield tail of the aircraft. The T-28 madesevenpenetrations at 5.25 'Ion(-3øC,ambient) recordedby CP-2. Analysisof ZDRplayeda vital role in determiningthe microphysical characteristics of this storm. Differen- throughoutthe stonn'slifetime. The first penetration(1835:15) tial reflectivityis a measureof the differencein backscattered beganat about 11 rain after detectionof first echo,and penetrapowerfroma wavebothtransmitted andreceivedpolarizedhori- tions continueduntil the stormwas well illto its decayingstage. zontallyas opposedto onepolarizedvertically. Mathematically, The T-28 madeits last penetration(1920:00) about55 rain after ZDR is defined as first echo. Hereill we discussdata collectedduringthe first three T-28 penetrations,corresponding to times up to about 25 after first echo (about 9 rain after first lightning). The R)urth penetrationwas madeconsiderably southof the main reflectivity Zvv core. The remainingpenetrationswere made while the storm was in its decayingstage,after collapseof the "ZD• column," whereZHHrepresents the reflectivityfactordue to horizontally indicatingat this stagethe lack of sufficientupdraftto maintain polarizedtransmittedand receivedwavesandZvv represents the supercooled raindropsaloft. reflectivityfactordue to verticallypolarizedtransmittedand reMeasurmnents of cloudliquid water concentrations (CLWC) ceived waves. from the T-28 were made usinga Jolmson-Williams(JW) probe. Our interpretations of ZDRmeasurements were basedon the The accuracyof this deviceis not as great as that of the King conclusions reachedby Herzeghand Jameson[1992]. Basedon Probe. Tile JW respondsmainly to liquid water ill the form of analysesof Alabama thunderstorms, they concludedthat from dropletsless than 30 to 50 •tm ill diameter. Recent intercomZDRmeasurements one could clearly delineateregionsof ice parisonsbetweenthis JW and a King Probe flown simultaneprecipitation (ZDR'4)dB) fromregionsof significantrain precipiouslyon the T-28 showthat this JW tendsto give readings---1/2 tation(ZDP,>2dB). Further,it •vasnotedthat in convectivesysthoseof the King Probeill wann-basedcloudswith broadercloud tems, ZDRcan providethe informationnecessaryto detectthe dropletspectra. presenceof supercooled rain (liquid water dropsabovethe 0øC The vertical wind estimates(l¾omthe T-28) were based on isotherm).We refer the readerto Bri,gi and Hendty [1990] for changesin aircraftpressurealtitude,pitch,andverticalacceleraflirtherdiscussions on the topicof difl•rential reflectivityand its tion,usinga methoddescribed by Kopp[1985]. The noiselevel usefulnessin radar meteorology. for thesecalculationsis about2-3 m s'• Tile verticalwind calculationmaybe biasedby up to a few metersper second,positively or negatively,dependingon the trim of the airplane. The base2.2. In Situ Measurements line zerovalueshouldbe takenas tile valuecomputedin straightData collected frmn two instnnnented aircraft were used in and-levelflightjust prior to cloudentry. Data from two probeson the T-28 were used in analyzing the analysisof this storm. The P-3 made two penetrationsinto the storm,oneat 6.4 km meansealevel (MSL) (-10øC, ambient) particlesizesand types:a PMS 2D-P imagingprobeand a foil of the phases(wateror about 2 rain after first echo (•-1825:00 UTC) and anotherat impactor.In this analysis,detemfination was consideredvery important. Since 4.1 km MSL (+3øC, ambient),20 rain after first echo(all alti- ice) of the hydrometeors tudesreferredto henceforthwill be with respectto mean sea the determinationof water phaseis somewhatsubjective,we dislevel, and all times will be with respectto universaltime con- cuss how this was done. The PMS 2D-OAP probesare imagingprobesdesignedto revention). image(or shadow)of eachsampledparData collectedby the P-3 and used in this analysisinclude corda two-dimensional ilparticle imagesfrom both the ParticleMeasuringSystemsInc. ticle. Each probeconsistsof a linear arrayof 32 photodiodes (PMS) two-dimensional imagingprecipitationprobe(2D-P) and luminatedby a laserbeam. The diodearrayis scannedrepeatcloudprobe(2D-C). Operationof theseprobesis discussed fi•r- edly as particlespassthroughthe beam, yielding a two-dimenther, below. Also usedwere vertical wind calculationsbasedon sional shadowimage. The opticsand opticalpathsdiffer beinertial navigation data, true air speed, and angle of attack tween the 2D-P and 2D-C models, giving different effective (describedby Willis et al. [1994]). Liquid water concentrations resolutions.For the 2D-P probeson both the T-28 and P-3, the were derivedfrom measurements made by the King Liquid Waeffectivediodespacingis ---200[tm, while for the 2D-C probeon the P-3 tile spacingis 50 [tm. ter Probe[King et al., 1985]. Last, we analyzedthe two components of the ambientelectric Basedon the shapeof tile particle image, one can oftell defield derivedfrom measurements madeby four electricfield me- terminethe phaseof the hydrometeor.Water dropswith diameters on the aircratl. Tile two resolvablecomponents of the elec- ters greaterthan-600 [tm tend to cant(elongationalongan axis tric field measuredby the P-3 are the componentthat is vertical of---45ø) in the flow field aroundtile probe[Blackand Hallet, ZDR =10log ZHH (1) 18,964 FRENCH ET AL.: OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM 1986]. Graupelparticles,on tile other hand, do not cant, and thereforetend to result in less regularly orientedimages. Becauseof resolutionlimitationsimposedby the 2D-P probe,it is difficult to determinephasefor hydrometeors.For this reason we analyzeddatacollectedby the foil impactorto help discriminate the phase of hydrometeorsin regionspenetratedby the T-28. The foil impactorconsistsof a thin movingstripof aluminuln (-7.5 cm wide and---0.003 cm thick) that passesover a ridged drum behindan openwindow (with dimensionsof 3.75 by 3.75 cm). As particlesstrike the foil, they leave ridgedimpressions. The ridgesare spacedat 0.25 iron, which definesthe resolution of the instrument;the minimulndetectablesize is approximately 0.5 mm. The foil is exposedandtransported onlywhenthepilot- probesalongwith tintinginformationencodedinto tile image data. In regionswith highparticleconcentrations, theseprobes are oftenlimited by memoryand data transferrate constraints to obtainingimagesfor only a portionof the total time in-cloud. However,the disadvantages of this intermittentsamplingare mitigatedby the abilityto ignorefor countingpurposes thoseim- agesthat are obviousartifacts,andto compute an appropriate size-dependent samplevoltimefor largerparticles onlypartially imaged. DatafromtheP-3, withboth2D-C and2D-Pprobes,suggest thatthe latterseriously underconnts particles sosmalltheytrip the probebut are not imaged,i.e. smallerthan-43.4min. For largersizeswe believeour computed concentrations are representativeof actualparticleconcentrations.One additionalconactivated"in-cloud" switch is on. At other times, the tbil is not siderationin the concentrations computedfroin the T-28 2D-P moving,and a metal shuttercoversthe foil at the windowposi- probein this studyis that the imagesin the first halvesof each tion. Each time the in-cloud switch is turned off, the shutter 4 kilobytebufferwereoftencorrupted.Thisrequiredconcentracloses,anda punchmark is madein the foil. The foil movesat a tionsto be estimated basedonjust half (the "good"half) of the constant speed (-3.4 cms'l) duringa penetration, punchmarks totalnumberof recordedimages. denotethe boundariesbetweenpenetrations,and the times assoDetermination of the electrical evolution of this storm relied ciatedwith thesepunchmarksare recordedon the data system. heavilyon measurements madeby four electricfield lnetersoil Thusonecandeterminethe locationill the cloudthat eachpartitheT-28. Thesefourfieldmetersareableto resolvetwocompocle struckthe foil with an nncertaintyof about 100 ill (the nominents of the ambient electric field, vertical and trailsverseto the nal accuracyof the globalpositioningsystemreceiveroil the airdirection of motion(thesameasthoseresolved by theP-3). The craft). field metersare modelE-100, rotating-shutter type instruments The method used to determinethe phasesof hydrometeors described by Wim•[ 1993]. that left impressions oil the foil is basedoil the shapesof the iln(Ey) prints. Water dropsare assumedto leave circularimpressions, The two field metersusedto determinethe horizontal while ice or ice-liquid combinationparticlesare asstunedto componentof the electric field are locatedoil the end of each leave "splatter"marks. This is basedoil a reportpreparedby wingtip. Thetwoothermeters(locatedonthebottomandtopof the vertical(E•) component Miller et al. [1967]. Laboratory experimentsdiscussedby the fuselage)are usedto determine of the electric field. Details are presented by Ramachandran et Knight et al. [1977] producedsimilar restilts,but also demonstratedthat water-dropand ice-sphereimpressions were indistin- al. [1996]. A brief summaryis givenhere. guishablefor particleslessthan-3 mm in diameter. As the lbil impressionswere analyzedonly for their character,and not detailed concentration and size statistics,overlappingimpressionsin regionsof high precipitationparticle concentration did not hinderthe analysis. We carefi•llyconsideredboth setsof particledata (2D-P and foil impactor)beforeconcludingwhat typesof particlesexisted in a given region in cloud. Using thesetwo setsof data, we coulddiscriminatebetweenwater and ice regionsin cloud for particleswith diametersgreaterthana few nm•with a reasonable degreeof certainty. In this work the primaryemphasisis on precipitationparticle The four electricfield metersin the four differentpositions responddifferentlyto a unit-magnitude field component normal to their faces, due to differences in curvature and local surface featuresat eachmounting location.The readings of the individual metersrespondingto the samefield magnitudeare scaled relativeto eachotherusingself-charging testsin negligible ambient fields and roll maneuvers in constant ambient fields with negligibleself-charging. Eachof the ambientfield components is thencomputed by calculating the scaleddifferences fromeach pair of oppositely facingfield metersandcorrecting for the roll andpitch(usingsimpletrigonometry).Overallenhancement of theambientelectricfieldaround theaircraftis accounted forby measurements. Particle concentrations are estimated in two multiplyingthe measurements by an enhancement factordeterwith the New Mexico ways. A rough estimateof precipitationparticle concentration minedthroughin-flightintercomparisons of MiningandTectmology's (NMIMT) SpecialPurpose canbe obtainedby dividingthe PMS probeshadow/orcount(the Institute Research(SPTVAR) as docutotal number of particlescountedper second)by tile optical Test Vehicle for Atmospheric sampling volume sweptoutby theprobe(-0.15 m3 s'•, forex- mentedby Giori andNanevicz[1992].The electricfield meters in ambient fieldsof approximately +200kV m'• ample,for the T-28 2D-P probe).This concentration includesall saturate sizesof particles,fromthosejust big enoughto activatetheprobe Whentheaircraftis highlycharged, asit oftenis duringthunpenetrations dueto precipitation particleimpacts,variwhile not leavingan image(-0.2 mm, for the 2D-P) to thoseso derstorm largethat they couldnot be entirelycontainedwithin the sample ouslocations ontheairframeandpropellerwill discharge plumes volume. It alsoincludesartilhctsdue to water streaming off of ions. Theseplumesdistorttile electricfield sensedby the probetips, foggedoptics,and otherphenomena.The precipitation particle concentration can be estimatedsimilarly froln the foil impactorby dividingthe numberof valid impressions within an areaof foil, by that foil areamultipliedby the distancemoved duringthe time of expostire(roughly90 ill per secondof expo- meterson the fuselageandwingtipsand may introduceartifacts in estimatesof mnbientfield components [e.g., doneset al., 1993]. Experiencewith the T-28 has shown that when the magnitude of the ambientfield is greaterthanthe fieldowingto chargeon the aircraft(computed froin scaledsumsof readings sure). from the wingtip pair of meters,usingthe sameoverallenA more rigorousestimateof precipitationparticleconcentra- hancement factor)signsof distortions like thosedescribed by tion can be obtainedusingthe imagedata recordedby the PMS doneset al. [1993] are infrequent. FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A TI-IUNDERSTO• 18,965 We feel that T-28 measurements are accurate within about a this stormis somexvhat atypicalof otherCaPE tlnmderstonns defactorof 2, basedon clear-airformationflight intercomparisons scribedin the literature. Althoughmostof the incastiredparameetc.) were comparable madeduringCaPEwith theNCAR SailplaneandKingAir, and ters (i.e., CLWC, particleconcentrations, throughcontinuity of spatialstructure in electricfield estimates to those measured in other storms, the overall structure seemed madeduringsuccessive penetrations madeby theT-28,P-3, and different. In particular,mostof the other stormsin CaPE develNCARKingAir in anotherstonnonthissameday(V.N. Bringi opeda distinctmulticellularstructurewith the individualcells et al., Evolutionof a Floridathunderstonn duringthe Convecton relatively easyto distinguishon radar plots. This stormdid not andPrecipitation/Electrification Experiment: Tile caseof 9 August 1991, submittedto Monthly kVeather Review,1995), and by share that characteristic. Figure 3 presentsa seriesof ConstantAltitude Plan Position Indicators(CAPPIs) constructedfroin CP-3 data at four times aircraftchargingappearto be minimalin the electricfield data duringthe observingperiod(1830, 1835, 1842, and 1849), from discussed below, exceptpossiblyduringtile final P-3 penetra- 5 min after first echountil tile end of the third T-28 penetration. tion. Duringthis penetration, aircraftchargingxvashigh;how- The different heightsapproximatetile +3, -3, -10, and -20øC ever,the variationacrossthe cloudof the ambientelectricfield levelsin the cloud,respectively.During tile first threetime periods,the cloudwas essentiallystationaryand wc believe characcomponents still looksreasonable. terizedby a singleupdraft. This conjectureis supportedby the presenceof a singleZr• columnduringthis period(as discussed below). Tile presenceof two distinctmaximain tile reflectivity 3. Analysisof ObservationalData at 1842 in the 6 km and 5 'kmCAPPIsis likely to be precipitation 3.1. Environmental Conditions cascadingoff the top of the nearlyverticaltipdraft. There is an indicationof the developmentof a secondupdraftregion in tile The stormon August9 waslocatedoverthe westernedgeof northeastquadrantby 1849, whichis supported by tile spreading CapeCanaveral,abovethe field mill networkoperated by the of the stormin that directionin the 1849 columnof Figtire 3. KennedySpaceCenter. The stormformedalonga convergence While there is evidencefor the developmentof a secondcell boundary [Bringiet at., 1993]. Figure2 showsa sounding from a radiosondethat was launchedat 1810:00, 15 min before detec- within this cloud, it seemsto occurafter tile original cell had evolvedelectricallyto tile pointof producinglightningat or betion of first echo. The sonde was launched froill a mobile CrossChainLORAN AtmosphericSoundingSystem(CLASS) facility fore 1842. So, we believethat xvhatis describedin tile lbllowing approximately 3 'kmsouthof wheretile stormtBrmed.It showsa discussionis the microphysicaland electricalevolutionof a sinconditionallyunstableatmosphere (lifted index -3.5, K index gle thunderstormcell. 3.2.1. P-3 penetration 1. At about 1827:00, tile P-3 pene36.8) thatis relativelymoistthroughout its depth. Tile shearis 16.1m s'• through thelowest6 l•n, whiletileconvective avail- trated this cloud at 6.4 'km (-10øC, ambient) flying from the the T-28 and P-3 in tile stonn described belo•v. Tile effects of northwest to the southeast. Tile cloud at this time and altitude able potentialenergy(CAPE) for this soundingis 1872 J/kg. The CAPE value is characteristicof illany subtropicalthunder- was only 2-3 Ion in diameter,with a peak reflectivityof 15 dBz vertical winds at stormenvironments both over land and over ocean[Lucaset at., near the penetrationlevel. Aircraft-measured thislevelwereall positive 0naximum •-14m s'•). TheKing 1994].The bulk Richardson numberis 15. Probeindicated a peakCLWCvalueof4 g in'3.Table1 indicates that the 2D-C and 2D-P probesencountered a few small precipitation-sizeparticles,nonelargerthan 1 min. Electricfields(both When comparingdata from this stormwith data froin other horizontaland vertical) encounteredby tile P-3 were less than stormsobservedduringCAPE,we cameto the conclusionthat 2 kV m'• andmayhavebeeninfluenced bya mature stonnlo- 3.2. Storm Evolution cated a few kilometers to tile southeast. These measured electric fields were smaller than the uncertaintyof tile measurements [Willis et al., 1994]. 3.2.2. T-28 penetration 1. The maximtimreflectivityin the cloudreached20 dBz by 1830:00,and 45 dBz by 1835:00.The T-28 beganmakingits first penetration8 rain after the P-3, enteringcloudat 1835:15. Flying from the southeast to the northwest, the aircraft penetratedat an altitude of 5.25 'km (-3øC, ambient). Figure 4 showsa CAPPI of reflectivityat 5.25 km. ThesedatawerecollectedfroinCP-2 nearandduringthetime of the first penetration;the CP-2 site is tile originfor the coordinate systemused. In the southeastern half of the cloud,the T-28 flew throughan area of relativelyhigh reflectivity(in excessof 40 dBz). In the northwesternhalf, the refiectivitieswere much lower, between 20 and 40 dBz. The lower panelin Figure5a showsa verticalcrosssectionof CP-2 reflectivityalongthe flight path of the T-28. The ordinate is altitudeaboveground,andthe abscissa is plottedin time units but can be thoughtof as a spatialvariable. Sincethe T-28 was flyingat approximately 90 m s'l (although the trueair speed varies between 80 and 105 m s'•), each 10 s represents 4).9 kin Figure 2. Plot of a sounding(temperatureand dew point) launchedby mobileCLASS at 1810:00on August9. The soilde of data. Tile two graphsabovethe reflectivitycrosssectionshow the 2D-P shadow/orcount,whichrepresents the numberof times wasreleasedapproximately 3 kin southof the stonn'slocation. 18,966 FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A TH-UNDERSTORM E --• E E E --- c5oi• "•0 0 •,--, r.,0 0 ,4.., 0 " .,.., FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A TIIUNDERS'FORM 18,967 Table 1. MicrophysicalCharacteristics of tile Different CloudRegionsDiscussedin the Text Begin P-3 1826:57 T-28 End Pen 1 Alt, km T, øC 6.4 -10 5.2 -3 1827:06 Pen 1 Max CWC VW Total 4 up 220 >400 mm > lmm >2mm >3 mm Max D, mm 0.95 35 1835:15 1835:21 dn 2400 370 16 1835:27 1835:27 dn 2700 690 100 16 Phase ice 1.6 ice 2.4 ice 1835:28 1835:40 dn 2600 790 260 80 37 7.5 ice 1835:40 1835:44 dn 2000 430 21 9 6 7.4 mixed 2 up 2900 160 32 6 3 3.4 liquid 2 up 1200 300 64 10 10 5.6 liquid 1835:50 T-28 1836:24 Pen 2 5.2 -3 1840:48 1840:51 1840:51 1840:59 2 up 1300 200 29 12 1841:00 1841:09 1.5 tr 2900 420 74 19 1841:10 1841:20 tr 3800 680 72 10 1841:20 1841:48 dn 4800 1700 690 110 dn 850 530 190 35 5 7.2 ice 5 9.5 mixed 0.8 ice 2.4 Ice P-3 Pen 2 1845:10 1845:40 1845:40 1846:16 T-28 Pen 3 4.1 liquid 6.6 mixed 6 6.8 mixed 41 7.2 ice 9 3 3 5.2 2.6 up 1100 460 110 15 -3 1847:51 1847:54 dn 4800 280 1847:55 1848:00 dn 4000 340 34 1848:00 1848:18 dn 3800 1000 320 120 41 6.6 ice 1848:18 1848:30 tr 5900 1800 620 250 160 6.3 mixed up 2100 730 350 200 130 7.6 m•xed 5.6 m•xed 1848:30 1848:40 0.8 1848:43 1849:00 0.3 dn/up 3400 1000 370 120 36 "Begin"and"end"columnsdelimitthetime intervalwhentile aircraftpassed throughtheregion,Air istheaveragegeopotential altitude,T istheaveragetemperature, Max CWC isthemaximumcloudwaterconcentration encountered duringtheperiod,VW characterizes theregionasupdraft(up), downdraft(dn), or a transition(tr) betweenthetwo.Total is thetotalparticleconcentration of particleslargerthan200 l•tm(estimated from2D-P probe observations exceptfor tile firstP-3 penetration. wheretheestimateis basedona 2D-C probe)whilethesucceeding columnsdenotethenumberlargerthan or equalto the indicatedsize.In thefinal column.Phasenotesthepredominant phaseof thehydrometeors encountered duringthe period. per secondthe 2D-P probewas 'lripped"(top), and the vertical electric field component(bottom) as computedl¾omT-28 field meters. Figtire 5b showsa corresponding crosssectionof differential reflectivity along the flight path of the T-28. The two graphsabovethis panel show the CLWC measuredby the JW probe(top) and the verticalwind (bottom). Referringto Figures5a and 5b, it is apparentthat as the T-28 flew ttu'oughthe southeastern half of the cloud (1835:15 to 1835:50)it encountered a doxvndraft with verticalvelocitiesbe- drops. In the updraftportion,where the reflectivitywas rather weak, Zi:)• valuesas greatas 3.5 dB were measuredat the level of the T-28. Tile 'lligh Z•)• column"(1.5dB contour)was lbund to extendup to a heightof 7 km (-15øC, ambient). This is indicative of an area in which relatively low concentrations of largerliquid water dropsare present. Also, CLWCs in the up- draftwererelatively high(maxinmm of -1.7 g m-3asmeasured by the JW probe),while tile doxvndrafi was virtually devoidof anycloudliquid water. tween-5 and-10 m s-•. Asmentioned earlier,thereflectivity A sampleof particle imagesdetectedby the 2D-P probedurvalueswere highestin this portionof the cloud. Also, as one ing the downdraftin tile first penetration is shoxvn in Figtire6a. would expect,the 2D-P shadow/orcounts,proportionalto pre- Particle concentration statisticsare given in Table 1. This cipitationparticle concentration, were relativelyhigh in this por- downdraftregionis far frombeinghomogeneous in particlesize, tion. In the northwesternhalf of the cloud (1835:50 to 1836:30) habit(shape),andconcentration. In the southeastenunost portion the T-28 encountered moderateupdrallswith verticalwinds be- of the downdraft(tlu'ough1835:21),tile 2D-P probedetecteda tween 5 and 15 m s'•. The reflectivitiesand shadow/orcounts relatively lowconcentration (-10 m'3)of graupel particles, all in here were generally lower, except for one local peak in the 1- to 2-ram sizerange. For the next 7 s (-630 m) tile T-28 shadow/orcountsnear 1836:20, on the northwestedge of the flew througha regionof predominantlysmallerparticles(less strongestupdraft, where the highestconcentrations of the pene- than 1 mm in diameter)with a muchgreaterconcentration.From tration were encountered. These concentrationsare relatively 1835:28until 1835:40,the 2D-P probedetecteda considerably low(---300 m'3)compared tothose thateventually develop in the broadersize distributionwith hydrometeors up to 7 mm in distorm. ameter. Both tile 2D-P and the foil impactordata indicatedthat up to this pointwere in tile In the downdraftportion(1835:15to 1835:50),Zr• values(at all of the particlesin the doxvndraft the level of the T-28) were low, lessthan 1 dB. This is indica- ice phase;this is consistentxviththe concurrentlow valuesof tive of an area made up mostly of ice particlesor small water Zi•}•. i8,968 CP-2 FRENCH ET AL.: OBSERVATIONSOF EVOLUTION OF A THUNDERSTOI•,'M and T28 Altitude= 5 25 183500-183700 UTC 9 August 1991 km 55 As the T-28 flew tlu-oughthe northwesternmost kilometerof the downdraft(1835:40 to 1835:50) ZD}:increasedfrom 0 to about1.5 dB. In this region,the 2D-P probedetectedan average concentration of 9 m'• of particles with diameters 2 nun or -18 greater. Both the 2D-P and foil impactordata indicatedthat someof the particleswere in the ice phase(graupel)and some - were in the water phase(raindrops). The T-28 enteredthe updraft at 1835:50. The entire 4-'•n -20 :::::::.:::::::: -22 ß width of the updraft(at 5.25 l•n) was characterized by high Zo:: (•eater than 1.5 dB), relativelyhighCLWC, andlow concentrationsof precipitation-size particles.Duringthe first 2 s that the aircraftwas in the tipdraft(---180m), the 2D-P probedetecteda ... :::..:. '.:.. localconcentration of morethan40 particles m-3xvithdiameters -24 greaterthan 1 1ran(Figure6b). The 2D-P imagesand foil imprintsindicatethat all of thesehydrometeors were water drops. Ttu-oughout the remainderof the updraft,neitherthe 2D-P probe nor the foil impactordetectedanyparticlesgreaterthan 1.5 mm in diameter. During this 2.9 km of tile updraftpenetration,tile ..... ...:.:::.. -26 -28 2D-Pprobe andtbiliinpactor each xvould havesampled 4.6m3of -30 15 3 5 7 9 11 13 15 dBZ X DISTANCEFROM CP-2 (km) cloud. The reflectivityin this regionmusthavebeendominated by large dropsin concentrations too low to be detectedby the T-28 probes[cf. Illi,gm,orth,1988]. Toxvardthe middle of the updraft,a large numberof very sillall (d < 0.4 mln) particles were detected. The phase(water or ice) of thesedrizzle-drop sizehydrometeors couldnot be determinedbecauseof the reso- Figure 4. A CAPPI displayat 5.25 kin constructed froIllgriddcd lution limit of the instn,nents; however, in an tipdraft at the and smoothedCP-2 data between 1835:00 and 1837:00 during of-3øC, one Wotlldexpectthem to be thefirstT-28 penetration. The solidline indicatesthe flightpath penetrationtemperature of the T-28 (SE to NW). The origin Ibr this figureis the CP-2 liquid. The 2D-P probe also imaged a large number of (long, thin imagescausedby water flowingoff the radarsite. Reflectivitiesare plottedfrom 15 to 55 dBz in incre- 'Sstreakers" probetips), which are indicativeof relativelyhigher CLWCs. mentsof 10 dB as indicatedby the scaleoil the right. B CP-2 and T28 183500-183700 UTC CP-2 9 August 1991 and T28 183500-183700 UTC 9 August 1991 3 JWCLWC (g/ms) •saa IaDe-Sh/or (#/•) 55 10•0 4.5 2 20 3½ VERTICALELECTRICFlED (kV/m) ....... :::::::::::::: • -30 z -10 • •2 3 GHz Zn I 1.5 3 GHz Zrm 8 o 25 o < 4 4 ß .::..':;:::' :::::::'.::::.i::":" :.'::::.. ::::::::::::::::::::::::::::::::::::::::::::::: ......... '.... -1.5 15 dB dBZ o 183500 FLIGHTTIME (UTC) 1837013 SE --) NW 83500 FLIGHTTIME (UTC) • 83700 SE --) NW Figure5. (a) Thelowerpallelshows a rcflcctivity cross section alongtileflighttrackof theT-28duringits firstpenetration. 'Ille upperpallelsindicate theverticalelectric fieldderived frointhethselage millsandthe shadow/or countderivedfrointhe2D-P probe. (b) The lowerpanelshoxvs a ZD• crosssectionalongtheT-28 flightpath. Theupperpanelsindicate theverticalwindcalculated from%28 measurements andthecloud liquidwaterconcentration (CLWC)derivedt¾om theJW probe.Eachtic on theabscissa indicates 10 s of flighttime,or about0.9 •n of aircrafttravel. FRENCH ET AL.' OBSERVATIONS OF EVOLUTION 18,969 20- A Buffer 316 OF A TItUNDERSTORM 2D-P Stad Time = 183521.65 Duration = 0.88 sees iiillllllllUIIIIIIIIl•llltllilN l.F-7•- 1I-I •--•--•UI••im••t•[•1••[[• iig•i•i•i•1•i•H•lU•i•i'•i•i•Fri•U•i•i•i•'•H•Hi•ri•i•i•F•ii[i•L•[•i•L•$• Buffer 322 2D-P Start Time = 163530.70 Duration = 1 26 secs Vet' L teal Hop tzon Lal •[•k•L•i•"•illilL•L•-i•L•t•[•i•i•r•LB•L•r•!•-•IFIlIFILl•i•i•IH•i Buffer 324 2D-P Slart Time -- 183533.35 Duration = 0.68 secs •U•i•i•il•t•i•iiH•H•F•i•FH•i•i•E•'•L•Ell'•P•U•i•P•L• Buffer 326 2D-P Slart Time = 183535.35 •L•"L••i•i•iH•'H•CL•-•[•i• Buffer 328 2D-P Slart Time = 183537.35 blh Duration = 0.21 sees Duration •11111tlllli IIIlLI_LIIIHlt--L.I-kt--IFI = 0.66 secs •i••L•r•'b•i•-f.•H•FF•LB•b.[•1•H•iL•P•n•rf•F•H•r•iL•F Buffer 330 2D-P Start Time = 183539 35 Duration = 0.36 secs o B Buffer333 2D-P Slart Time = 183544.00 Duration= 7.77 secs -IIIBl'•ItiEIIUtI--HIIilIfi•It-1111!-11•11111• •i•i•i••i••i•[I•|•ig Buffer334 2D-P StartTime= 183551.95 Duralion= 2.80 sec.s -2e II I 183• [ [ [ ] 836 [ l 1837 T I H E .ILiHI IIIIt[ll LliliiSillblliiib,Llil,lililJEILilt_tllt ILl •11•1 [i1__lI-'-IFil-I-[IIIIit•ilIIIIBII I Buffer336 2D-P Start Time = 183557.40 Duration= 1.05 secs -Ll'-tl_llL_-L - Ill-L_=-I11-t1'-'-'-1--I_l_ll-II[ I1__ LLLI_ I--I--I-tM- Figure7. Ambientelectricfield(kV nf]) derivedfromT-28 Buffer338 2D-P Slarl Time = 183559.85 Duration= 1.84 secs duringthe firstpenetration.The solidline repre-- IIIII-I-1111111-M----I--I•l ___i._l--!i-kLl-!--llllilH_•-• LIIIbl-I-- measurements Buffer340 2D-P S!art Time = 1836O5.75 Duration: 2.77 •ecs sentsthe vertical(z) component, andthe dashedline represents _ill t-IIII•IIiIt--ilHt iilLI--iLI__ILiI'I•IILII-llI--k_lLI-ilLliki-tt-IilLtLI thehorizontal(y) component.Seetext lbr signconvention. Buffer342 2D-P Start Time = 183609.70 Burnlion= 3.21 secs ----I-.-tHt-l--fil-il-[tlJI •t--ilI-II•11-}_I71tLI-IIILIIIIIII[IILIi li--P--ilillilil• Buffer344 2D-P Start Time = 183614.45 Duration= 2.82 secs -II il -- -i•lil_LllllLJllllHl-::•il-lillllililllIFFi[11l__l[[l-i_l-I--iliillli Buffer346 2D-P Staff Time = 183618.45 Duration= 0.77 sees this time the stormwas approximately 9 km longand 5.5 •i•i•i•i•ii•i•i•i•i•i•i[•iiil.---••i•i•i•i•iii•i•i• wide, still arrangedalonga northwestto southeast axis. The BUffer348 2D-P Slart Time = 183620.55 Duration= 1.05 secs high-reflectivity core (greater than 50 dBz) •vas located slightly -iillllllllllil __11111il•111iltlllllUlll IUlI_•!I -----------FIl--It-IBuffer350 2D-P Slart Time = 183623.15 Duration= 126 secs -- northwest of the stormecho'scenter. Throughout muchof the Hllll•111111•111111-!!llll!lt -Iilllii•1111111•lffililliilliElliiilllilillillillilil_l--t--H-I_ penetrationthe T-28 was in an area with refiectivities between Figure 6. A sampleof particlei]nagesrecordedby tile 2D-P probefrom the (a) downdraftand (b) updraftduringthe first penetration. Vertical bars representthe 6.4-ram vddth of the probeaperture.Eachline corresponds to one buffer(4 kbytesof data). Tile buflL-rheadingsshow tile bul'l•zrnumber, tile start 30 and 50 dBz, with greaterreflectivitiesencountered earlier in the penetration. Figure8 showsa 5.25-kmCAPPIwith the T-28 flighttrack superimposed, andFigtire9a showsa crosssection of reflectivity time of each bufi•2r(lbnnat is 183533.35 = 1800 hours, 35 ]nin, 33.35 s, for example)and the duration,or total elapsedtime duringxvhichimageswere recorded,in decimalseconds.It takes a finite time tbr the datato be dumpedto the datarecordingsystem; duringthis time, no datafire recordedby the probe. ]'herefore this recordrepresentsa noncontinuous set oœparticleimages. Only selectedbufibrsare shoxvn. CP-2 and T28 Altitude= -18 5.25 184000-184200 UTC 9 August 1991 km - Tile existenceof thesestreakerimagesin tile PMS data supports themeasurements oftiptonearly 2 g m-3o1' CLWCmade bythe '•JWprobe.TheT-28 exitedthecloudat 1836:30. • -22 The electric fields (both the vertical and horizontalcompo- & nents)measuredby the %28 during the first penetrationwere • weak(Figure 7). Bothcomponents werenegative throughout the p,-24 entirepenetration, andthemagnitudes wereonlya fewkV m'• • near what isbelieved tobethetillcertainty ofthemeasurements. • -26 Also, there was no correlation betxveenelectric field measure- a 25 ments andupdraft/dovmdraft structure orparticle clusters. These b measurenmnts and earlier ones made by the P-3 indicate that electrification up to thispointwasrelativelyweak,at leastin the vicinityof the penetrations. 3.2.3. T-28 penetration2. The secondpenetration madeby the T-28 beganat 1840:30, 15 rnin after the initial radar echo. The aircraftenteredthe cloudon the northwestside,flew directly -28 -302 15 4 6 8 113 12 14 dBZ X DISTANCEFROMCP-2 (km) through thehighZDRcolumn andthehigh-reflectivity core,and Figure8. As in Figtire4, exceptfor tilesecond penetration, exitedthroughthe southeasten• edgeof the cloudat 1842:00. At 1840:00-1842:00. 18,970 CP-2 FRENCH ET AL.: OBSERVATIONS OF EVOLUTION' OF A THUNDERSTORM and T28 184000-184200 UTC 9 August 1991 CP-2 and T28 •sea 2DP-Sh/or (#/s) 50• 184000-184200 UTC 9 August 1991 3I JW CLWC 4.5 •• 30 v•x•ca• •L•CTmC •'Im) (•V/m) ....... :i:i:i:i:i:i: o -10 .:.:.:.:.:.:. ............. -30 J • ....... ....... 3 GHz Z• 1.5 3 GHz ZDR 8 .o........... =========================== :.:.y.:.:.:.::..'..'.::::::iiii•i•iiiiiiiiiiii!iiiii:i:•:i: ...;.:-:.:.:.:.:.:4 -1.5 dBZ 84000 1842•0 FLIGHTTIME (UTC) NW-) dB 184000 FLIGHT TIME (UTC) NW-) SE 184200 SE Figure 9. As in Figtire5, exceptIbr the secondpenetration. alongthe flight pathof the T-28, alongxvithtile verticalelectric field and the 2D-P shadow/orcount. Figtire 9b shoxvsthe ZDR crosssectionalongthe flight pathalongwith the JW CLWC and the verticalwind. In the northxvestenunost portionof the cloud (1840:48 to 1841:00) the T-28 encountereda narrow,moderate updraft withvertical speeds between 10and16m s-•. Afterexit- Imagesrecordedby the 2D-P probewhile the T-28 xvasin the updraft(1840:48 to 1841:00) are shownin Figure 10a. Concentration and size statisticsare indicatedin Table 1. The updraft was characterizedby a numberof streakerimages. In the very begilmingof the updraft(northwcstcnunost edge)a clusteringof 11 particlesrangingfrom0.5 to 1 mrn in diameterwasdetected ingtheupdraft,theaircraftflew througha 2-kin-wide"transition in a regiononly 100m across;thiscruxesponds to a localconcen- zone,"wherevertical velocities variedbetween -2 and+4 m s'•. tration ofnearly70in'3oftheselarger particles. Thelbili•npac- h• this region, reflectivity values along the flight track were tor also detectedthis clustering,and the characterof the impresgreatest(in excessof 50 dBz). In the downdraftregion(1841:20 sionsindicatedthat theseparticleswere all liquid drops. About to 1841:48), vertical velocities werebetxveen -1 and-7 m s'• 2 s (---180m) later, the 2D-P probedetecteda very large liquid and reflectivities were ---40 dBz. Shadow/or counts were much waterdropwith a diameterof 5.5 min. This is a significantfind, higherin the downdraftthantheywerein the updraftandtransi- in that the T-28 was locatedin a regionof very high Zm (-3.5 tion zones. dB) with reflectivityof 43 dBz. This indicatesthat a relatively Similarto the firstT-28 penetration,the updrafthadrelatively low concentrationof large liquid-waterdrops can return high highCLWC(JWreadings between 1.5and2 g m4) andwas valuesof Zm togetherwith moderatereflectivity. The foil imcollocatedwith a highZm column. Throughoutthe tipdraft,Zm pactor,despitesamplinga similar voltime,did not detectany rangedfrom 1.5 to 3.5 dB. The 1.5-dB contourextendedtip to dropsof this sizein the tipdraft. Sevenotherdropsof diameter1 about6.5 km (-12øC) in this region,again indicatingthe pres- to 2 mm were detectedby both the 2D-P probeand the foil imence of supercooled raindrops. In the transitionzone, xvhich pactorthroughoutthe remainderof the tipdraft. The total volume sharedcharacteristics of boththe tipdraftand the douq•drafi,the sweptout by the 2D-P probeand foil impactor,each,in the tip- CLWCvariedbetween 0.5 and1.5g ma andZD•ranged l¾om draftwasapproximately 2.4 m3 (although 2D-Pimages were 0.5 up to 2 dB. The presenceof substantialliquid water,the absenceof significantupdraft,the moderatelyhigh reflectivity,the increasingprecipitationparticle concentration, and the particle imagesdiscussed belowindicatethat this regionreflectsthe decayof a portionof the originaltipdraft,probablydue to precipitationloading. Note that the tipdrafthasnarrmvedconsiderably in Figure 9b comparedto Figtire 5b, althoughthe locationremainsthe samexvithrespectto the cloudstn•cture.In the downdraft,whichagainxvasvirtuallydevoidof anycloudliquidwater, measured values for Zm were between-0.5 and 0.5 dB. This collectedfor onlya fractionof thistime). Data from the 2D-P probe and foil impactorindicatedthe presenceof both liquid water and ice particlesin the transition zone. Figtire 10b shows2D-P imagescollectedxvhiletile T-28 was in the transitionportion of the storm. The presenceof streakerimages(fewer than in the updraft)indicatesthe continued presenceof cloudliquid water; This agreeswith measurementsmade by the JW probe. h• the northwesternhalf of the transitionzone(1841:00to 1841:10;---1kin) the 2D-P probedetectedat least four particleswith diametersgreaterthan 2.5 mm volume of---1.4 m3. Thetxvolargest ones, -7 nundiindicatesthat this portionof the stormwas madeup of graupel in a sample particles,which xvill be sho•vnto be consistentwith measure- ameter,appearedto be ice. Data from the foil impactoras well as the 2D-P imagesindicatedthat someof theseparticleswere mentsmadeby the T-28 2D-P probe. FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM 18,971 A Buffer 375 2D-P Slam Time = 184120 85 Duration = 1 33 secs Stad Time = !LllllIIIIItlIIIIIIItI!!.!_•.-I!I!I•llI•L tl-Utl-_t--l-•IilIIIIIIIIIltLllIIILI[•IIL[MItI!IIIIitlI•III•IIIIIIIIIItI[llm Buffer 376 2D-P Slam T•me = 184122 35 Duration = 1 27 secs Buffer 353 2D*P Buffer 354 2D P Sram Time = 184O51 35 Duration = 1 48 secs - IIIII•111•FIIIIIItlIIlUlIIII•ItllIIIIffilII•III[HtlIIIIIIr•!H-111-11111111•I,,,11IL..IIIIfilLIII•H•11I$1__ I•'[11•1IltlllllH-i -H Buffer 355 Buffer 377 2D-P Slam Time = 184123 8O Duration = 0 59 secs lhllb•lL il II- FILMIII-I-IMLI•Illi 2D-P Slad Time = 184O53 • Durallon = 0 90 secs FFIl•lll[•r-[Lllllllllttlllllmmlllll-JiJai-ll•,itllllllilllllHil•llltllllllllr HIH-H[! • I-IItF[II!IilIffiH•ililIMI Buffer 378 2D-P Slam T•me = 184124 80 Duration = 0 54 secs 111llllllllllllllllllllllllt!l!!l!l! •!•B•-`•t•B••••HF•`•H•H•M•Hr•H• Buffer 379 2D-P Slam Time = 184125 80 Duration = 0 37 secs "i:'ii[tiEYiFit[?......... ']mtll1111LIlIILILIIItIFIrLIIIltt:-IF 111111rlllll•-H H--LII tllllllitfllll.1111111_!!!!ll!!!.!!!!.. !!!Hi_!!!!!lllllllHrtil'tlll-till LIIiI-IIItItlIItIILHrH. IIlIIItlIlIlIt!IItltlIMII•111i Buffer380 2D-P SlamTime = 184126 80 Duration= 0 43 secs -II III-111LI-! fi IllHItIHH-[I u•e• 359 2D-P Sla• T,me =lg4057 75 Duration =113 sees I._ I•1•1I•1-•]11[•1111LH••I--IIIII2LI•I Buffer 360 2D-P •1 • T 1•4059 05 D ! 3 9d It]milli,[FlfilUililll',t-. UlilBIlllmfi[lllllll m4r'llIIfiII['IILLIlli Illl/1111Ulllltlltllllltrf'llill![tllllllllfi •--•-•i-•-L-Ill.•i••.•-•L-!j•tH•r•[•L•I••r-•m•.•L• Buffer383 2D-P StartTime = 18412980 Duration= 0 27 secs !111r&l•ll•lfir-tLLIIfiI•t•T!IPiItlIIiiH-ii, H!ilttMitliiiHii[!iiiiiiiiiiittlii. itlitliiilmHHi Buffer384 2D-P SlamTime = 18413O8O Durallon= 0 2Osecs Buffer382 2D-P StartT•me = 184128 80 Duration= 0 16 secs Buffer385 2D-P SlamTime = 184131 8O Duration= 0 22 secs Fl•llll.lLll-rlll.i1,11 •KllltlLI II!ttfll,tMPl[tfillrM!l•!l_[tHillLiLl. lltH.-lllHi-----i-illl[lll. l.iHlfirlrll Buffer386 2D-P SlamT•me= 18413280 Duration= 0 32 secs B •.t••Li•r•..ur!••i•••H•.•tL•E•.•H•r•it•-•H• .Fl.Ih Buffer387 2D-P SlamT,me = 18413380 Durallon= 0 24 secs UFIbll----I-L•LLII[H-II'IIIIII•I-ILIH_111LI• •1•1--III ll•••J!I_II'LI!_•L!! L•r•H•H•LH•H•f•H•L•L•L•H`•r•B• Buffer388 2D-P SlamTime = 18413480 Duration= 0 30 secs Iit%-Ii,i,-iiiii,iliiiF %ii i-iih-t[l•f1• IELI•I•WI•IIFI•IrIWIII.[l!_I-!!_ rt•III[rtI•IHItIIlltllII[MIIIIIrlHWtlIIIHIHIII[fIIIIIIILrl iltllllllltH Buffer389 2D-P SlamT•me= 18413580 Duration= 0 35 secs II IIIII I1HII!11l--IIIHII II1'11[I •11111 III1•1111• IIIIIltlr bll•l[ IIIII-Hl•tlttlI, I[1111111,1tt•I-IIIIlIIIII IIIIIIII] IIIIilt II'rUllll!Lrtll,lllllLtltllltlrl •H•••t•M••[•.•r•t•t•W`••M• Buffer390 2D-P SlamTime = 18413680 Durahon= 0 36 secs [I. I[I[11LII'IH •[•t•[L•[•Hr•i•[•F•[•H•F•tr•L•HHI[[B•r•H•[W•[•L•t•H•i•L•B•L[• Buffer391 2D-P SlamTime = 184137 8O Duration= 0 28 secs •L!•.•!t•r•a•L!.HJ•[•rtH•L11114••r••i•r•Lp•i•f•r•rFt•ii•p• Buffer392 2D-P SlamT•me= 18413880 Duration= 0 27 secs -fiIIIII[-ILi_HlI-LI Buff ......D-. StaM T.... .- Hii;[,iiiki u,,it ,[r[, ,m[ u]H,[uu[[ [[lIIIIIIlilLIII-IIIIUHIlUIIIIIIBuffer IF I_L!'_ !!KLr![!l,__lr!![ rr!, __1!,!.lr •1_ !!!!1!rf!!!wr_!,!'_ !.!_[l,!!_Ll.! !!._HI'111.11' I,,ILIIIL IfIllr tl'• Ill111m 11,HlIHlILIIitrHIIIIII!l lll.11'Ltllrri 393 2D-P SlamTime = 184139 80 Duration= 0 36 secs iiiiiiifiil•lifi•lli•lii•l•il•ii•il•'Jli•ll•!•lHtlllllllllltll IIIIIIIIH IIIII III illllll Illlltllll 1III IllU Illtlllllllilt Ifillit tU ]llllill.1111.111rlrlU I--t'l,1111.ltrlrl •-•.•`•U•1M`r•`•B•L•MH•.M•`•`•LLt•HH•r•L•r•Ht•r Buffer 361 2D-P Sram Time = 184103 15 Duration = 2 O0 secs Buffer 363 2D-P Slam Time = 1841O6 50 Durahon = 0 42 secs Buffer 364 2D-P Sram Tlrne= . = Buffer 36B 2D-P 1841O7 5O Duration = 1 34 secs 84111 10 D Slam Time -- 184113.10 I Durallon o59 Buffer 394 2D-P Slam Time = 184140 80 Duration = 0 23 secs = 0.55 secs IIIIIIII. tHlIIIIlIIILIIH-I II_lllHI IllllHlillllllllllll[ IllllllllHllllltllHIt IHIHIIlllllllllll IIIllil!llUlllltllllllflllltllllllllH[llHIIIlfifillllllll [.llll-dlllllll 'lH•tl.[b!,_r tr!trlt! •m•_!-!!t•!.!•t•iLB.tllll. iltrIILLMLIHrrIHlII['tIItI/WlIIIfIII-IIII. LIIIItIlltLtItlHtt •i•ii•i•i•i•i•i]i•i•i•i•i•i•ii•]•i•ii•i•i•ii•ii•ii• IIIIItlllltnllt Illllll Iilllllllllt_lllltlllUllltlll. IIIIFI I%lilø111il•il)11•½illit•i•ili-i ......•tiii.,.o. ½631•1111111 ILI!--III I[[1111-I-I I1-t-FIIt-HIIIFI I-IllII •lr!!t!!lll Ir.!!L !r!.!!!!!_!ILI, Lt!!I_!I!LILP!I_!!!!,!L!'!!,. l!Mtllaltllllll, LIIrlI. I,II'LIrI. rHIIIIII. FHIIIfflIIIIFIHII•I"IIIIItIIIfM[D,I _. -_ i•116 - 8•....ira,[o•[• - i - -L_u--un Buf•eiFlEtit•T,•e .111lll•!l•Hl.lflllllll•11.llt HtMtll•.111tl illrllrll.•rl.ll.lfll tlI'11tlI. IIIIIrttlWI[IIHIIIIILLttrtilI!'I•Irl[ItllltHLrtlIIllI. IIIIlill Buffer 396 2D-P Slam T,me = 184142 80 Duration = 0 17 secs Buffer 397 2D-P Slam Time = 184143 80 Duration = 0 21 secs ' Buffer 398 2D-P Bullet 373 2D*P Slam Time = 184118 85 Duration = 0 41 secs '111.[IJ IIIII41ZqlL_-•HL!---HF•!!L[1-tllHq- Slam Time = 184144 8O Duration = 0 19 secs •u•tk!m!;•i•-•mi•ur•m•t•Lt•rH•r•Pk•Mr•I•L•L•L.H•t•r• LII•!I-LLIIt-LI-II Buffer 374 2D P Sram Time = 184119 85 Duration = 0 33 secs Buffer 4OO 2D-P Slam Time = 184146 8O Duration = 0 18 secs :L!11111/I[111111LI LLLI-I-I-III-t[11111111111il/illlillll tllllBIlitlllllth -[-_F__!!III-L•!/.._!,I_L!' # I !•L•!•m•.•I•[•b•HrI•[•r•-•H••.•La•• Figure 10. As in Figure.6, exceptduringthe (a) updral•.,(b) transitionzone,and(c) doxvndrafi in the second penetration.In this sample,all bul'Ik2rs are shoxxqi. probablywater drops,while somewere probablygraupcl. During the last 10 s (southeasten•hall) that the T-28 was in the transitionzone, both devicesdetecteda larger concentrationof smallerparticles,with only a few particlesgreaterthan 3 mm in diameter. Foil impactordata indicatedthat most, if not all, of the particleswere ice. Particleimagesfrom the first 0.5 km (1841:20 to 1841:25) of the downdraft(Figure 10c) indicatedyet higherconcentrations of smallparticles,and a relativelyhigh numberof particlesgreater than 3 mm in diameter.Those2D-P imagesof a•fficient size, andthe foil impactordata,indicatedthat the particlesdetectedin this region,as well as the rest of the downdraft,were ice. As the T-28 flew farther throughthe doxvndrafi,both devicesindicated that rest of the do•vndrafiwas fairly homogeneous in particle sizes and concentrations, with someM•atfewer very small and verylargeparticles. The magnitudesof the electric field componentsmeasured duringthe secondT-28 penetration(Figure 11) were significantly largerthanthosemeasuredduringthe first penetration.The vertical componentof the electric field was near zero as the T-28 enteredthe cloud from the northwest(1840:30). It increasedal- 20- _ 1•- _ _ _ _ _ Ver' LLcol Hør' LzønL71_••.z_. .,Z /-II _½-10 -1• -20 1 B40 1841 T T 1842 H F mostlinearlyto about7 kV m'• at theilaredgeof thetransition Figure 11. As in Figure7, exccpttbr the sccondpenetration. 18,972 FRENCH ET AL.: OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM zone(1841:20). The T-28 then experienceda relativelystrong, of tipdraftswith relativelyhigherCLWC (King Probereadingsto positive, verticalcomponent (up to 14 kV m-l) overa spanof 3 g m'3)andupdrafts of 10to 14m s'•. 10 s (4).9 km flight path) as it enteredthe downdraft. Figure 9 showsthat the 2D-P probe particle detectionrate (shadow/or count) increaseddramaticallyin this region, while Figtire 10c showsthis to be a regionwith a mixtureof small and largeprecipitationparticles,predominantlyice. The verticalcomponent The particleprobeson the P-3 detectedmainlygraupelin the dom•draftregion,with a mixtureof graupelandrain in the up- of the electric field relaxed to zero as the T-28 flew on toward draft region. Particleconcentrations were generallylower than foundby the T-28 4 rain earlierand 1.1 km above,with generally similarpeak sizes(cf. Table 1). The electricfield measuredby theP-3 wasconsistent (in sign) with that measuredby the T-28 during its secondpenetration. The P-3 encountered positiveverticalelectricfields tlu'oughout the southeastern edge of the cloud,througha region of higher concentrations of smallgraupel. (thepeakvalueof 4 kV m'• occurred in the The horizontalcomponent of the electricfield (Figure 11) was the penetration smallerin magnitude,but its variationwas similarin structureto downdraftregion), indicatingnet negativechargeabovethe airthe vertical component. The horizontalcolnponentincreased craft. The magnitudeof the vertical componentwas relatively linearly fromzero(at 1840:30) to about 4.5 kV m'xat 1841:20. smallerthanthat measuredby the T-28 1.1 km above. This can This, coupledwith the positiveverticalcomponent, indicatedthe be interpretedas consistentwith a region of negative charge presenceof negativechargeaboveandto the right (south)of the above the T-28 altitude with the P-3 flirther removed from it and aircraft at this location. At the same location where the vertical thus measuringa lower field magnitude. An inductionring incomponentincreasedsharply,the horizontalcomponentbecame stmmenton the P-3 measuredparticle chargesof both signsin negative (-5 kV in'X).Thisisindicative ofa localized region of the downdraftregion,xvithan excessof negativeparticlesover negativechargeslightlyaboveand to the left (north)of the T-28 positiveones[Brooks,1993]. No particlechargedeterminations position. The horizontal componentthen recoveredback to could be made in the updraft region due to signal interference 3 kV in'• and decreasedto zero as the T-28 exited the cloud. fromwatersheddingfromthe inductionring. The electric field measurements tlu-oughout this penetration 3.2.5. T-28 penetration 3. The T-28 beganmakingits third at 1847:30, some22 min afreflectedsomecorrelationwith microphysical variables. In par- penetrationfrom the east-southeast passticular, the dominantpeak in both resolvedcomponents of the ter the initial echo. The planeflew to the west-northwest, electric field was encountered in the transition zone and northing tlu'oughthe southernhalf of the highestreflectivitiesas westportionof the downdraft,in a regioncoincidentxvitha rela- shownin Figure 12. It passedabout2 km southof the high Zm portion tive maximtimin the concentration of large graupel,as seenin column,whichwas then locatedin the northwesternmost of the storm. The T-28 wasoutof cloudby 1849:30. Figtire 10b. A reflectivitycrosssectionalong the flight path of the T-28 The T-28 pilot reportedlightningduringthis penetrationnear 1441:22,just beforethe peakin measuredverticalandhorizontal (Figtire 13a) revealsthat the high-reflectivitycorewas locatedin field components abruptlyended. Closeexaminationof the in- the easternhalf of the storm(beghminghalf of the penetration). dividual T-28 field mill recordsindicatesa small field change The T-28 just penetratedthe top of the regionof highestreflec(œ1kV m'l) at thistime.Examination ofdatal¾om several indi- tivities,whichwere between55 and60 dBz. The easternportion vidual field mills in the Kem•edy Space Center ground-based of this corewas locatedin a weak to moderatedowndraftregion networkshowsindicationsof an intmclouddischargeat this time but a more restrictiveanalysis[M. Murphy, personalcommuniCP-2 and T28 184730-184930 UTC 9 August 1991 cation, 1995) indicatesthe first resolvableintracloudlighming Altitude= 5.25 km occurredat 1842:31,just afterthis penetrationended. 55 At 1845:00,while the T-28 was turningin preparationfor a thirdpenetration,the stormshowedslowmovementto the north, -18 whereasit had beenprimarilystationaryuntil this time (cf. Figtire 3). The highestreflectivitiesat 5 km (over 60 dBz) were found in the centerof the storm.This time corresponded to the -2O highestreflectivitydetectedat the 5-hn level duringthe entire life of the storm.At this level, the stormhad a diameterof ap- proximately10 kin. The high Zm column•vaslocatedin the northwesternportion of the highestreflectivitiesat 5 km; the •.• -22 ::::::::::::::.: 1.5-dB contourextendedup to about6 kin. The 1.5-dB contour wasforrodat a heightof about4 .l•nthroughout the remainderof • -24 the high-reflectivitycore, indicatinggraupeldescending below the freezinglevel andmelting. • -26 3.2.4. P-3 penetration2. The P-3 beganmakingits second and final penetrationat about1845:00. It flew from the south-28 eastto the northwestat an altitudeof •4.1 .l•n(+3øC, ambient). The aircraft flew directlytlu'oughthe centerof the stormand penetrated the high-reflectivity core(-60 dBz at thislevel). -30 The horizontalprofile of verticalwindsmeasuredby the P-3 4 was consistentwith that of the T-28 in its secondpenetration.In 25 6 8 10 12 14 16 15 dBZ X DISTANCEFROMCP-2 (km) the center of the storm and to the southeast,dox•n•draflsof about 2 to4 m s'• in magnitude •vereencountered. Thenorthwestern Figure 12. As in Figure 4, exceptfor the third penetration, sideof the storm(corresponding to theZm column)wasmadeup 1847:30-1849:30. FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM 18,973 A CP-2 and T28 184730-184930 UTC 9 August 1991 CP-2 and T28 15002DP-Sh/or 184730-184930 UTC 9 Augus[ 1991 3•-JW CLWC (g/m •) 55 2- 4.5 _ 500 1 i i 30 VERTICAL ELECTRIC FIELD (kV/m) 0 t • : 20 VERTICAL VELOCITY (rn•s) ii!ii!!!iiiii ; I :i:i:•:i:i:i: 3 .:.:.:.:.:.:. ...... -30 ' 12[ i:i:!:i:i:i:i ß.'.'.'.'.'.'. i:i:i:i:i:!:i: 3 GHz ZH • : f :•.•: .. ::::::::::::: ...... -, 0 .':' ß 3GHz Z•R .... --- ß ... .'i': ß ß 8 8 ß....... " : -..:':.....-.... ß : 25 15 184730 -1.5 dBZ o FLIGHT TIME (UTC) ES E -) WNW 184930 dB 184730 FLIGHTTIME(UTC) 184930 ESE -) WNW Figure 13. As in Figtire5, exceptfor the thirdpenctratiol]. of larger (1847:50to 1848:18)xvitha maximumnegativeverticalvelocity (Figure14bandTable 1) revealedhigherconcentrations of-7 m s-•andmoderate shadow/or counts.Thewesten] portion graupelparticlescomparedto the dovmdraft.The largenumber of the core was in the transition zone (1848:18 to 1848:30), of "splatter"imagesevident in the PMS recordshouldnot be where vertical winds between-5 and 5 m s'• were encountered. confused with streakerimages.Thesesplatterimagesare the reIn this regionthe shadow/orcountpeakedat over 1000 particles sult of mixed-phaseprecipitationparticleshitting one of the s'•, corresponding tototal2D-Pparticle concentrations ontheor- probetips and thereforethere is no correlationbetweenthese derof6000Ill'3. Theupdraft (nlaxiilltln] ---10111 S'i) was½ncotlll-imagesandhighCLWC. During the first 10 s (-0.9 kin) of the updraft, 1848:32tered on the northxvestemlnost edgeand just outsideof the reflectivitycore. The shadow/orcountwas significantlylower ill 1848:42, tile T-28 flew throughan area with a concentrationof large particlessimilar to that in the transitionzone (Table 1). this region. to the highestreflectivitiesand The ZDRprofileis shownill Figtire 13b. Throughlnuchof the This 1-km regioncorresponded penetration, the 1.5-dBcontourremainedbelmvthe flight level ZDRthat were measuredin the tipdrafton this pelletration. Relaof the aircraft. Yet, in the centerof the tipdraft,the 1.5-dBcoil- tively fewer small particles(0.4 mm < d <1 mm) were detected tour did extendup to 5.25 kin. This is alsothe regionin xvhich in the updraft comparedto the transitionzone. Data from both maximum CLWCwasencountered (-0.7 g in'3). Northof the the2D-P probe(Figure14c)andfoil impactorwere in agreement T-28 track, on the northwestemlnost sideof the reflectivitycore, thatthe vastmajorityof the particlesdetectedwere ice (gmupel), the 1.5-dB contourdid extend above 6 kin. The strongestup- althoughsomeraindropswere present. Someof what appearto be streakerimagesare actuallydue to a stuckbit in the probe drafts•vereprobablylocatedin this regionat this tilne. Particle data revealed fewer difl%rences betxveen the various and do not representreal images(a stuckbit is generallyrepreportionsof the stormcomparedwith earlierpenetrations.hi the sentedby a perfectly"straight"image,that is, only one pixel, that folloxved,and southeastern portionof the dmvndrafi(1847:51 to 1847:54)the 0.2 nm] wide). Durillg a narrow dox•qldraft 2D-P probedetectedrelativelylow concentrations of sinallgrau- the remainderof the tipdraft(endingat 1849:00),both devices than pel particles,up to-0.8 mm in diameter(Figtire 14a and Table revealeda broadsizedistributionwith higherconcentrations 1). For the next 0.5 kin, the probemeasuredpredominantlyvery in the main updraftportionof the penetration.Many of the parsmallparticles,but with maximumsizessteadilyincreasing with ticles detectedin this regionappearedto be liquid, and splatter particlesam alsoevident. time to 2.2 nun at 1848:00.At this point, the T-28 enteredan imagesindicativeof mixed-phase The peak magnitudeof the vertical electric field component areaof greaterreflectivity(50 to 55 dBz). Throughout therestof the downdraftregion,data•¾o111 boththe 2D-P probeand foil im- during the third penetrationwas not much different than that pactor indicatedhigher concentrations of particlesin all size duringthe secondpenetration,but the horizontalcomponentwas categories,up to 6.6 mm in diameter. All of the particlesde- much larger than that measuredduringthe secondpenetration (Figure 15). The vertical componentof the electric field was tectedin the downdraftappearedto be graupel. There was no distinctboundary,at leastin tile particletypes, positivethroughthe first 40 s (-3.6 Ion) of the penetration. betweenfile downdraftregionand the transitionzone. The 2D-P Fromthis point,the field decreased dramatically overa 10-speimagesand statisticsfrom the transitionzone, 1848:18-1848:31 riod (---0.9 km) andwent througha nfinilnumof approximately 1-8,974 A FRENCH ET AL.' OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM of the aircraftat this time. The horizontalcomponentrecovered to about-7 kV m'• and then decreasedas the T-28 crossedthe •[•IF•[•BF•rH•HkL•rLr•H•r•L•[r•LH•I••r•r•i•I•L•r• Buffer 447 2D-P Start Time = 184757 80 Duration = 1 10 secs fringeof the updraftand approached the northwestern edgeof the •l•l•a•B•••l•••• IIIIIIIIIIIIIIIIlI!11111•11111111111111llllll cloud. Buffer 444 2D-P Start Time = 184750 85 Duration = 3 49 secs Buffer 450 2D-P Start Time = 1848O1.55 Duration = 0 82 secs [I.ILItlII•IiI'I.I[LILlII'I•IJlHI•IIFLLlI[IIILIIIIrUrlIII t1_ 11L'tl•MllrII'I•IlIrI•III'LI-----IIIII. II-LI'1111 ILIIFIIIrLlll. Much morevariationin the electricfield wasmeasuredby the T-28 duringthis penetrationthan in the two earlierpenetrations. •LI--!•IrFI_-HIIIIl!!!ltH-•II'III•111111111BIII II-IIIIIIIIIIII. IilII. I•!111tlIIIIItlilIII!rLIHIIIIIII'11•I' When the vertical componentreachedits most negativevalue HILLI'LI!IH--q--11I---•--.....!1•!.......II_!11tllLllllllll'rllLIPL•lli'lLrlr•tlltllrllll•l!llliHr'llbLl[ (1848:18), the T-28 was in the mostsignificantdowndraftmeasBuffer 460 2D-P Start Time = 184811 55 Duration -- 0 45 $ecs I'B•.1111111-•!!!!!!H•!!! !!!!!!!_rrluI.JHHrltllLl'111,1111-111111lll I-LI-HIII_11IIItlI, IIII. IIIIit Illl[11HIirlllll ured duringthat penetration.Yet, the particlephases,sizes,and Buffer 462 2D-P Start Time = 184813 55 Duration -- 0 71 secs duringthis time were similarto thosesampledbelllelIL[LIItI-tl-.-I_ LIIIPllJll!l!!lailllll[tlJl-lllllll•llrHlllllrlllll IIIIIIBIIBtlilIII,,,1111It[MII-I-11111114111Iilll Ilfitll concentrations Buffer464 2D-P Start Time = 184815 55 Duration = 0 08 secs fore and after this downdraftwas encountered.One interpretaLltitlI!I!-IIIFI!ilI'IIiI!II•I!!!!!•!IILIIJI!Ir!tlIItLIILIIIIIItlII-IIFrlIi•I - - i-IFFI IlL tion of these observations is that the T-28 was close in altitude to Buffer 453 2D-P Start Time = 184804 55 Duration = 0 25 secs Bufter 466 2D-P Slart Time = 184817 55 Dural•on = 0 58 $ec$ •!11111-11•1111BII.I.IILI•KL[IBItle•IIIiI'IIItlrlItl tHrl-II F' ritli[11LI - ttl•l•l-I, lallt the centerof a negativec!•argelayer, and that the centeraltitude of this regionwasbelowthe aircraftin the downdraftand above it elsewhere. Buffer467 2D-P Start Time = 184818 55 Duration-- 0 30 secs i•;•111'tJJlllellrJllJ. l'_l-•...._IF'• ._11-_•-!-!4!•!--lkllllltllllllf• ;'c;"-IIL:II-IIt[ILplILlII/[IrI'I, Buffer 469 2D-P Start Time = 184820 55 Duration= 0 22 secs 4. Summary of Observations tI.1111elI,•LP!I,UL! I-'---! l!F-•! IlllIII, IIt[IIL•IIllI-II•tlLI-LIItlII"ILIdlilI'PI[ILIt-[ Buffer 471 2D-P Start Time = 184822 55 Duration= 0 19 secs IIIilIIliL_I411H_F-!bl Itt---t I• III, IIIII1'II The early electricalevolutionof this stormwas stronglycouBuffer472 2D-P Slart Time = 184823 55 Duralion = 0 41 secs pled with the evolutionof the stonn's microphysics.For this I•11tllllll•LiiillrlttlHllllalllrl•1itllltll Hltl--ILdlIIIllIIII!I"'I-HI[III•IIIHIIIII!1111ttl--IIIII1•111'1"11-1 Buffer473 2D-P Start Time = 184824.55 Duration = 0 02 secs :llll•L•r••-•F•:•-•`•f••F•-•p•`--. -----•'-•F -- reason, we sununarizehere the evolution of the storm as a whole and do not breakit into electricalandnonelectricalcomponents. The P-3 penetratedthe storm near the time and level of the Buffer477 2D-P $1artTime = 184828 55 Duralion= 0 10 secs first radar echo. It detecteda t•w small precipitation-size ice ._ - I-IL!IL•ILAI•HI-_I------It-IFI Buffer 479 2D-P Slad Time = 184830 55 Duration = 0 14 sees particlesat the -10øC level, but no significantelectric fields. ---•"-*,•- --•.....-_--:.=•4•-•.•--:•---•l--iil[ltl•11•11tltllllllllll'111Ill•1111•11111 FI Eight minuteslater, the T-28 penetratedat the -3øC level. It detectedsignificantconcentrations of precipitation-size particles in the dmvndraft(mostlyice) and only a fexvprecipitation-size Buffer 481 2D-P Start Time ,= 184832 55 Duration = 0 38 secs up to this l-N]IaI'LLIEL.,PlttlIH !!!11"[[I,I[t[IIt-LI[IL I-[1tMI-LIFIIIIIIIIII'-LIII-r[Hparticles(mostlyliquid) in the updraft. Electrification pointhadremainedrelativelyxveak. Buffer 483 2D-P Start Time =184834 55 Duiitlon =085 secs !! _l-t!' l[IJ.-i . ...__!!!!!-LI-l_ _l•tk_!-I!!11_ _1-1•11•!-IL-IIFIIlalLI•__I_IiI-LLll Five minutesafter the T-28's first penetration,it again flew Buffer 485 2D-P Start Time = 184837 05 Duration = 0 74 secs -IIIII1-1II I-tlI•111LLIilIilI!.IlIIIIII-PH.I-LllIFIY•ILLJJLII-I PI---ILItPIHII,l!-[PI tttk-!IIIIIIIllI•ILFI. tlu'oughthe stormat the-3øC level. It encountered significant concentrations of precipitation-size particles. Moderate updrafts __11lPtLI,,I•h were encountered,which containedthe lowest concentrationof Buffer 493 2D-P Start Time = 184847 30 Duration = 2 01 secs precipitation-size particles. The observations are consistent with -t-I!rI[IiltI[LLII-H 11tlIIlt--11LI-••:•.•IItll•l•LIIIIIllatllllltltll !11rli i'111t•rlErlli'11 ilel liquid particlesin the updraft growingby collision/coalescence Buffer 497 2D-P Stad Time = 184852 75 Duration -- 0 34 secs & IIIJlfi!llqllillillllllL Ilrl•ltlrllllLItlll!lll!llUll l--71tllllr-iiiii I-Ill,IlL IIt--IlllE•L IlLIII, I1.• 1 I'LIIHIIIIIIIIIand then beingcarriedupward,where they would freezeat temperaturesbetween-5 ø and -10øC. This interpretationis sup-11tl--rL[11-•__ i1_P1111 •1•-•t•-•L•.•'•L••bP•H•L•P•'• Buffer 501 2D-P Slart Time = '184856 75 Duralion = 044secs portedby the ZD• profile. Also, high concentrations of ice partiIIIIItlIILI'I!IH LHIl-•ll"tllfl!,llll. lflTItl!111111111J"lltllllll II-II,IllIllIII[11,[tI-IIIIILiltlIHIIIItllIIIIiilIII[tttlIIIILirl [1•11 cles (graupel)were detectedin the douq•draft. These particles Buffer475 2D-P Slad Time = 184826 55 .Duration= 0 28 secs Le!IIIlllILF! •ll•l[!Frr!_!!•!,_ •!•.•1•L•r-•e•i••[••H•.k•L•r•-•I•h Buffer 499 2D-P Start Time = 184854 75 Duration = 0 44 secs Figure 14. As in Figure6, exceptlbr duringthe (a) doxvndraft, (b) transitionzone,and(c) updratlin thethirdpenetration. 2O Ver' t Lco I Hor- tzon tal .... -10 kV m'• attheedgeofthedowndraft region at 1848:18.The vertical componentof the electric field then recovered to 13 kV m'• and then decreasedto zero as the T-28 crossedthe fringe of the updraft region and approachedthe northwestern edgeof the cloud. The measuredhorizontalcomponentof the electricfield was oppositein signfrom that measuredduringthe secondpenetration. This is consistentxviththe secondpenetration,sincethe T-28 was flying in the oppositedirection. The horizontalcomponentdecreased fromzeroat the southeastern edgeof the cloud to a minimum of-20 kV m'• about40 s intothepenetration, coincident with the n•aximum in the vertical componentin the downdraftregion. The T-28 then passedthroughan area at 1848:30 where the horizontalcomponentwas a relative maxi- mum(0 kVm'•). Thislocation corresponded to theboundary betweenthe transitionregionandthe updraft,anda shiftin sign of the verticalcomponent,indicatinga localizedregionof relatively high positivechargedensityaboveand to the left (south), or negativechargebelowandto the riglit(north),of theposition E 1• ....... 0 -•5 •"x /1 \ •• \ \ (- x •_• -10 20 x i , , / i i i i I i i 18•7.5 T ]- P1E Figure 15. As in Figure7, exceptfor the third penetration. FRENCHET AL.:OBSERVATIONS OFEVOLUTIONOFA THUNDERSTORM 18,975 thattileaircraft wasnotontilemainelectrical didnotmeltuntiltheywere•vellbelowthelevelof theaircraft, large,indicating of lightning andof a second as wasevidentfromsubsequent P-3 observations about1 km axiseither.Withthedevelopment convective region(or themovement andreinvigoration of the lower in altitude. one)thedistribution ofcharge withinthestorm hasbeThe electricalcharacter of the stormhadchanged significantly original duringthe5-raininterval betxveen thetimesof the firsttwo comemorecomplexby thistime. penetrations. Such rapiddevelopment ofelectrification hasbeen notedin studiesof otherCaPE storms[e.g., l¾illiset al., 1994; Ramachandran et al., 1996]andill similarstudies of thunderstorms elsewhere [e.g.,Dyeetal. 1986,1988].Duringthesec- 5. Discussion The evolution of this storm can be divided into two main priorto anyindications of ondpenetration, vertical electric fieldsof theorderof several parts. Firstis the earlyevolution kVm 4 were measuredat the level of the T-28. From these measurements andonesmadeduringearlierpenetrations, it is obvious thattherewasa definitelagbetween theinitiation of electrification, includingthe time t¾omfirst echotN-oughthe next12to 15min. Thefirstpenetrations of boththeP-3andthe T-28 were madeduringthis time. The secondpart of this precipitation-size particles andtherapidbuildup oftheelectric storm'sevolutionconsistsof the following10 to 15 rain of its field. Thisdelayis notsuq, rising;it hasbeendocumented sev- lifetime. Duringthisperiod,the T-28 madetwo penetrations, andelectricalactivitybecame eraltimes[e.g.,Reynolds andBrook,1956;Dyeetal., 1986].h• theP-3 madeits lastpenetration, bothof theseearlierstudies thedelaywasof theorderof 8 to 10 evident. After this second"evolution period"the stormbeganto stage(microphysically anddynamically). We min,whilewefound a delayof 11to 17min. Whether thisdif- enterits decaying ference is significant is opento debate, butonepossible expla- didnotanalyzethisfinaltimeperiodin detail,above. nationis thatill the earlierstudies, precipitation wasinitiated ttu-ough iceprocesses. In ourcase, precipitation wasinitiated at higher temperatures through collision/coalescence. If iceplays a 5.1. First Stage significant rolein tileelectrification of thunderstorms (assugThe first 12 to 15 min in the evolutionof this stormwas chargested by precipitation-based electrification hypotheses), we acterized bybroad updralls reaching 14m s'• andcontaining would expect a longer delayincoalescence-dominated clouds. CLWCranging uptoatleast 4 gin-3initially (asmeasured bythe Aninteresting feature found in theelectric fieldprofileduring P-3 KingProbe;theT-28 JW readings laterin thisperiodare thesecond T-28 penetration is thattilemaximumseems to occur probably anunderestimate ofthetrueCLWC).Concentrations of between thetransition anddox•q•draft regions andis nearlycoin- mediumto smallraindrops (0.4 < d _<1.5 ram)rangedtip to alcident withtheregionof highest reflectivity. Thistoohasbeen most1000m-3. Downdrafts duringthisperiodxverebroadand documented in earlierstudies [Dyeet al., 1986,1988;IFilliset ranged to-10 m s-1. Thedovmdrall region wasdevoid ofcloud al.,1994]. Thisfinding supports tileideaofa precipitation-based liquidwater.Them•jorityoftheparticles in thisregion •vereice charging mechanism active in thiscloud.It is ill thetransition(d _<2 nm•)yeta fewraindrops •veredetected in thetransition zonewhereonewouldexpect to findthegreatest number of dif- zonenearthe edgeof thedox•q•draft withina kilometerof the ferent particle types (graupel, snow, cloud ice,etc.).Also,inthis updraftregion. region, CLWCwouldbelargeenough to allowtimingof tile Ouranalysis is consistent witha coalescence-dominated congraupel particles (averyimportant requirement lbrnon-inductive vectivestormin whichraindrops tbnnandgrowin an updraft charging totakeplace).Without measurements ofactual particle regionthatis richin cloudliquidwater. Theseraindrops are charge at thisandotherlevelsin thisstorm, it is impossible to carriedvia thetipdrafts to levelsabovethe0øCisotherm.The determine towhatextentcharge separation mayhavebeentaking Zm column(collocated withthetipdraftandindicative of larger placein thetransition zone.However, theideaof charging in raindrops) extended toabout 6 kmthroughout thisportion ofthe thisregionis consistent •vithourmeasurements. stonn'sevolution.Thisheightcorresponds to approximately The P-3 madeits second penetration about3 rain aftertile -10øC. At thislevel,eventhe smallerraindrops wouldbeginto T-28 exitedthecloudl¾om its second pass.TheP-3 flewsignili- freezeandthenewlyformedgraupcl,withdiameters of 3 nunor cantly lowerthanintheearlier penetration (4.1kin,•-3øC).The less,wouldcontinue to growthrough accretion of cloudandrain water. electricfield profilemeasured by tile P-3 wasconsiderably smaller in magnitude butconsistent in signwiththatmeasured It is alsoprobable thatcloudicewouldbcIonnedthrough the Hallet-Mossop process [Hailerand•1ossop, 1974]nearthislevel bytheT-28duringits second penetration. Thesemeasurements are consistent with a largeregionof negativechargelocated in theupdraft, giventhetemperature, highCLWC,broadcloud abovetheflightlevelof tileT-28. Tilegreater distance betxveendroplet sizedistribution characteristic of warm-base clouds, and theP-3andthecharge region, andpossible rearrangement of tile the existence of graupel. Thesecrystalswouldgrow l•airly charge distribution dueto tilelightning discharge, couldaccount quicklythrough deposition, sincethe enviromnent shouldbe fortheweakerfieldsobserved bytheP-3. It is alsopossible that highlysupersaturated •vithrespect to ice. Aggregation of these should alsoleadtotheproduction of snowthatcould someof theredtiction in tile strength of tile electricfield (with icecrystals anothersource of graupel. decreasing altitude) •vasduetoa region of weakpositive charge thenrimeandrepresent At higherlevels,someoftherecently lbnnedgraupel beganto located between thetwoflightlevels(4.1 and5.25kin, +3ø and intothedo•ldraft. Loading of thetipdraft -3øC);however, it is ilnpossiblc to tollif thisis thecasel¾om falloutofthetipdraft, the data. mayin facthavehelped to produce theupper-level downdraft at the Thethirdpenetration madeby theT-28beganabout2 rain aboutthe sametimerainbegallto freeze.As Illis occurred, portion of theupdraft regionpropagated northxvestward aftertheP-3'ssecond penetration. Again,theT-28 flewat 5.25 leading regionwas km. Thispenetration wasoffset œrom themostactive convectionat lowerlevels.Muchof tilegraupelin tiledoxvndraft withinthestorm(south of tilehighZD•column).Themeasuredless than 2 nnn in diameter. Particle concentrationsin this regionweremuchhigherthanin theupdraft, withthe horizontal component of tile electricfieldwasalsorelatively downdraft 18,976 FRENCH ET AL.: OBSERVATIONS OF EVOLUTION OF A THUNDERSTORM highest concentrations (nearly1000m'3)foundin thatportion of the downdraftnearestthe updraft. This, coupledwith the low concentrations in the tipdraft, explainsthe patternof moderate reflectivitythroughoutmuch of the downdraft•vith the highest refiectivities in the transition zone, between the updraft and downdraft,on the edgeof the ZDRcolunto. The weakestrefiectivities were collocatedwith the updraftandthe ZDRcohmm. Electrification,throughoutthis early stagein the storm'sevolution, was extremelyweak. This is to be expectedif charge transferandseparation were basedon sometypeof precipitation mechanisminvolvingice-phaseparticles. Throughoutthis period, concentrations of ice particlesremainedrelatively low. Also, it was not until the end of this periodthat significantrefiectivities, implying higher concentrations of graupel, were found to exist at temperaturesof-20øC. Significantcharge transfervia a noninductivemechanis•nrequiresreasonablyhigh concentrations of graupelandsnowand/orcloudice in the-20øC region[e.g.,Takahashi,1978a;Satmde•'s, 1993]. If the concentrationsare not high enough,there will be too tkw collisions betweenthese particlesto lead to strongelectrification. Althoughsomechargetransfermayhavetakenplaceat and around -10øC with graupeland cloudice (tbnnedthroughthe HalletMossopmechanism), it is not clear from the observations what effectthismayhavehadon the large-scale electrification of this storm. This questionwill be addressed fitrtherin the companion modelingpaper. 5.2. Second Stage The nextportionof tile stonn'sevolutionwascharacterized by a narrowerupdraftanda morebroad,diffilse,doxxqldraft. The regionswereseparated by a 1- to 2-kin-widetransitionzonev,'hich hadweak to moderatetipdraftsanddo,aqldrafis.The tipdraftwas During this portionof the stonn'sevolution,it went througha rapidincreasein electrification,as evidencedby the observedincreasein electricfield strengthat the aircraftpenetrationlevels. This is consistentwith a precipitation-based mechanismbeing responsible for the electrification.As graupelandcloudice both beganto appearin significantconcentrations at low temperatures (-20øC), appreciablechargetransferand separationwould be expectedto occuraccordingto the noninductivecharge-transfer processes studiedin the laboratory[Takahashi,1978a;Saunders et al., 1991]. When particles (graupel/cloudice and/or graupel/snow)collidein regionsof this temperatureand in the presenceof cloudliquid xvater,the graupelacquiresnegativecharge and cloudice and/or snowacquirespositivecharge. If theseinteractionswere taking place in the transitionregion(where all the necessary components were present),we wouldexpectgraupel to be chargednegativelyand snoxvand cloud ice to be chargedpositively. As the graupelparticlest•qllout, the negativechargesare carried dovmxvard, away t¾omthe regionof production.This leads to large-scalechargeseparation. We envisionthis processcontinuing,leadingto a regionof negativechargeabovethe aircraft penetrationlevels, and positivechargeat even higher altitudes. This processcontinuesand electricfields build tip to the point, near 1842:00,when lighmingwasdetected. Furtherincreasesin electricfield strength,as measuredby the T-28, mostlikely are the restilt of two phenomena. First, as chargecontinuesto be separatedwell abovethe 0øC level, electric fields will continue to increase.Second,sincethe negativechargeis associated with graupeldescending in tile doxxqldrafi, we might expecttile lnain negative charge region to descendwith time. Although the magnitudeof tile chargein this regionmaynot be increasing, the electric fields at the level of the T-28 would continue to increase as the descendingcenter of mass of the chargedgraupel ap- richin cloudliquidwater(peakJWreadings of2 gnf3)butwas proachedthe aircraftaltitude t¾omabove. As the centerof this relatively freeofprecipitation-size particles (hundreds m'3).The charge layer passesthroughthe aircraft penetrationlevels in downdraftwascharacterized by verylittle cloudliquid waterand downdraftregions,the sign of the vertical field componentre- highconcentrations (many thousand m'3)ofgraupel. Thetransi- verses. tion zone sharedcharacteristics of both the updraft and dmvn- draft.In thisregion, CLWCwasmoderate (-1 g nf3)andprecipitationparticleconcentrations xverealsomoderate(manyhun- dredto a fewthousand m-3).Someparticles detected in thisre- ConcludingRemarks Althoughwe cannotbe sureof all of the elementsenvisioned gionwere ice, while othersxveremixedphaseor liquid. in this discussion of tile evolutionof tile August9 storm,we have Measurementsmade duringthis portionof the stonn's life- presenteda "story" that is consistentwith the measurements. time seeinto presenta consistent view of howthe stormevolved We alsoquantitativelydescribedhow the stormevolvedbothmimicrophysically from being dominatedby liquid coalescence crophysically and electrically. In a companionpaper,we attempt processes to beingdominated by ice-phase processes. Raindrops to capturethisevolutionin a numericalsimulationusingthe txvowould form and grow in the updraftregionand be carriedto dimensionalStormElectrificationModel (2-D SEM) and quantihigherregionsin the storm,wherethey wouldfreezeforming tativelycomparethe simulatedto the observed storm. graupel.Also,duringthisstage,significant mnounts of cloudice weremostlikely beingproduced throughheterogeneous l¾cczing Acknowledgments. We wish to thank V. N. Bringi and J. of clouddropletsat higherlevelsin the storm(althoughxvcob- Turk for radaranalysissoftwareusedin generatingseveralof the tainedno in situ observations at theselevelsto vcril}' this conjec- figures; K. Hartman for generating the particle images; D. ture). Ice crystalsproducedthroughthis and othermechanisms Priegnitzfor help in creatingsomeof the radarfigures;andC. P. would grow by diffilsionand aggregateto lbrm snow,which R. Saunders,I. Brooks, and R. Black for providingthe NOAA couldthen serveas graupclembryos,althoughraindropt?eezing P-3 data. This researchwas supportedby the National Science is probablythe primary graupelproductionmechanism. We Foundationunder grantsATM-9104474, ATM-9401117, ATMwouldexpectthe graupelto continueto growby accretion in the 9022846, ATM-9509810, and ATM-9200698. updraftandtransitionzoneuntil theseparticlesbecamepart of a downdraft. Microphysically,this is the same processas de- References scribedfor the early portionof the stormevolution. The main Aufdermaur,A. N., and D. A. Johnson,Chargeseparationdueto riming in differenceis that, in the maturephase,the processtakes place an electricfield, Q. d. R. Meteorol. Soc.,98, 369-382, 1972. over a largerdepthand thereforemoreand largerparticlesare Black, R. A., and J. Hallet, Observationsof the distributionof ice in hu•Ticanes,d. Atmos. Set., 43, 802-822, 1986. produced. 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