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The Cloud Population of the Madden-Julian Oscillation The Cloud Population of the Madden-Julian Oscillation

The Cloud Population of the Madden-Julian Oscillation - PowerPoint Presentation

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The Cloud Population of the Madden-Julian Oscillation - PPT Presentation

Atmos Sci Colloquium Seattle 6 April 2012 R Houze and D Hence S Brodzik K Rasmussen S Powell H Barnes B Dolan K Chakravarty C Burleyson Z Li S Ellis T ID: 489199

supp active stratiform lull active supp lull stratiform convection westerlies squall suppressed rain line population lines clouds ice cold

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Slide1

The Cloud Population of the Madden-Julian Oscillation

Atmos. Sci. Colloquium, Seattle, 6 April 2012

R. Houzeand D. Hence, S. Brodzik, K. Rasmussen, S. Powell, H. Barnes, B. Dolan, K. Chakravarty, C. Burleyson, Z. Li, S. Ellis, T. Weckwerth, J. Vivekanandan, J. Hubbert, W.-C. Lee

Early Results

from DYNAMOSlide2

Indian

Ocean12

345678

Wheeler and Hendon 2004The MJODYNAMOSlide3
Slide4

7N

EquatorSlide5
Slide6

S

KaNCAR S-PolKa

RadarSlide7
Slide8

SatelliteGlobal models

SoundingsOther island radarsShip dataShip radarsAircraft dataS-PolKaradarNCARradar

processorUW serverUW workstationsDaily Science SummariesNCAR field catalog

Project Data FlowLIghtningSlide9
Slide10

Radar experiment goal

 Characteristics and evolution of the MJO cloud population in the region where the disturbance builds up

Addu AtollSlide11

Supp.

Supp.

Supp.

ActiveActive

Active

Lull

Rain over area scanned by S-PolKaSlide12

Suppressed condition

echoesSlide13

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide14

Suppressed phases:

Lines of non-precipitating cloudsSlide15

Suppressed

phases: The “worm echo”Slide16

Slightly active moist layer

Clouds building at cold pool boundariesSlide17

Slightly active moist layer

Clouds building at cold pool boundariesSlide18

Cold

pool boundaries seen in differential reflectivity (ZDR)Birds?Dragonflies????Slide19

Birds caught on cameraSlide20

graupel

small ice

large non-melting ice

heavyrain

m

elting

ice

Moderate cumulonimbus begin to grow upscale

Doppler velocity

Hydrometeor typeSlide21

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide22

October 16Slide23

Refl.

RainConv.Strat.October 16Slide24

5 km

10 km

Intense

melting layermelting snow

graupel

50 dBZ!Slide25

Active phase few days later

Convection

feeding into a large MCS Slide26

Biggest MCS of first active phase:

weak unidirectional shearSlide27

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide28

Giant Rings of Convection

Larger than mesoscale organization of deep convection Slide29
Slide30
Slide31

Squall line in late active phase westerlies

Doppler velocity

Hydrometeor typeSlide32

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide33

Suppressed condition cloudsSlide34

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide35
Slide36
Slide37

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide38
Slide39

Westerly Surges

November

October

Larger than mesoscale organization of deep convection Slide40

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide41
Slide42

Long arc lineSlide43

Long arc linesegment on radarSlide44

Squall linein the strong westerliesSlide45

Weak stratiform in the strong westerlies Slide46

Stratiform Rain Fraction

S-PolKa S-band Stratiform Rain FractionSlide47

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide48
Slide49

The most robust squall line in the strong westerlies…

…only moderate stratiform…robust momentum transportSlide50

Supp.

Supp.

Supp.

ActiveActive

Active

LullSlide51
Slide52
Slide53

Summary of MJO cloud population characteristics & evolution seen by the S-PolKa radar

Humidity gradient layers monitored & measuredCloud lines dominate in highly suppressed periodCold pools are first stage of convective population

Graupel & other ice lofted & input into stratiform regionsConvection enhanced inside stratiform regionsMCS development strongest in weak shearShear inhibits stratiform region formation Westerlies organize convection on larger than mesoscaleSquall lines form in westerlies at back of active zoneSquall lines transport momemtum downwardSlide54

End

This research is supported by NSF grant ATM AGS-1059611, DOE grant DE-SC0001164/ER-64752, and NASA grants NNX10AM28G and NNX10AH70G