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The Cloud Population of the Madden-Julian Oscillation 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. Weckwerth, J. Vivekanandan, J. Hubbert, W.-C. Lee Early Results from DYNAMO

The Cloud Population of the Madden-Julian Oscillation

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The Cloud Population of the Madden-Julian Oscillation. Early Results from DYNAMO. R. Houze and 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. - PowerPoint PPT Presentation

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Page 1: The Cloud Population of the Madden-Julian Oscillation

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 DYNAMO

Page 2: The Cloud Population of the Madden-Julian Oscillation

IndianOcean 1

2

3

4

5

6

7

8

Wheeler and Hendon 2004

The MJO

DYNAMO

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7N

Equator

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S

Ka

NCAR S-PolKaRadar

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Satellite

Global models

Soundings

Other island radars

Ship data

Ship radarsAircraft data

S-PolKaradar

NCARradarprocessor

UW server UW workstations

Daily Science Summaries

NCAR field catalog

Project Data Flow

LIghtning

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Radar experiment goal

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

Addu Atoll

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Supp. Supp. Supp.ActiveActive ActiveLull

Rain over area scanned by S-PolKa

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Suppressed conditionechoes

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Supp. Supp. Supp.ActiveActive ActiveLull

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Suppressed phases:

Lines of non-precipitating

clouds

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Suppressed phases: The “worm echo”

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Slightly active moist layer

Clouds building at cold pool boundaries

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Slightly active moist layer

Clouds building at cold pool boundaries

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Cold pool boundaries seen

in differential reflectivity

(ZDR)

Birds?Dragonflies?

???

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Birds caught on camera

Page 20: The Cloud Population of the Madden-Julian Oscillation

graupel

small ice large non-melting ice

heavyrain

meltingice

Moderate cumulonimbus begin to grow upscale

Doppler velocity

Hydrometeor type

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Supp. Supp. Supp.ActiveActive ActiveLull

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October 16

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Refl. Rain

Conv.

Strat.

October 16

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5 km

10 km

Intense melting layer

melting snow

graupel

50 dBZ!

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Active phase few days later

Convection feeding into a large MCS

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Biggest MCS of first active phase: weak unidirectional shear

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Supp. Supp. Supp.ActiveActive ActiveLull

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Giant Rings of Convection

Larger than mesoscale

organization of deep

convection

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Squall line in late active phase westerlies

Doppler velocity

Hydrometeor type

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Supp. Supp. Supp.ActiveActive ActiveLull

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Suppressed condition clouds

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Supp. Supp. Supp.ActiveActive ActiveLull

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Supp. Supp. Supp.ActiveActive ActiveLull

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Westerly Surges

November

October

Larger than mesoscale

organization of deep

convection

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Supp. Supp. Supp.ActiveActive ActiveLull

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Long arc line

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Long arc linesegment on

radar

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Squall linein the strong westerlies

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Weak stratiform in the strong westerlies

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Stra

tifor

m R

ain

Frac

tion

S-PolKa S-band Stratiform Rain Fraction

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Supp. Supp. Supp.ActiveActive ActiveLull

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The most robust squall line in the

strong westerlies…

…only moderate stratiform

…robust momentum transport

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Supp. Supp. Supp.ActiveActive ActiveLull

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

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End

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