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A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results Peter M.K. Yau and Badrinath Nagarajan McGill University

A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

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A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results. Peter M.K. Yau and Badrinath Nagarajan McGill University. Outline. Motivation & Objectives Case Overview Modeling Strategy Results & Conclusions Future work. Motivation. - PowerPoint PPT Presentation

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Page 1: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

A Numerical Study of a TOGA COARE Super Cloud Cluster –

Preliminary results

Peter M.K. Yau and Badrinath Nagarajan

McGill University

Page 2: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Outline

•Motivation & Objectives•Case Overview•Modeling Strategy•Results & Conclusions•Future work

Page 3: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Motivation• MJO associated with supercloud clusters.

Processes organizing warm-pool convection a “zeroth-order problem” (Webster & Lucas 1992)

• Organizing mechanisms (OM) particularely at meso-and synoptic scale not well understood (Yanai et al 2000, Gabrowksi 2003).

• Improved understanding of OM on various scales should lead to:– better representation of convection in models– reduced forecast errors at the medium range – better representation and understanding of the

role of convection on water vapor distribution in the vertical

Page 4: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Objective Use a real data multi-grid (15-5-1 km)

numerical modeling approach to• simulate supercloud clusters (SCCs)

over TOGA COARE• diagnose the processes that:

– organize MCSs,– cause clustering of MCSs, and

• study the impact of convection on water vapor distribution in the vertical

Page 5: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Case Overview – IOP of TOGA COARE

Yanai et al (2000)

OLR (W m-2)•Once a day•Averaged 5S - 5N

•OLR < 215 W m-2

Shaded

•Focus of this study on SCC A

1Nov 92

28 Feb 93

1Dec 92

1Jan 93

1Feb 93

Page 6: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

IFA

Longitude

Tim

e

Time cluster

MCSs

Time cluster:•Lifetime > 24 h

MCS:•Lifetime < 24 h

The 6 DEC. 92 – 6 JAN. 93 SUPER CLOUDCLUSTER

Data Used:•Hourly GMS Infrared data•0-10S average

•Areas < 235 K precipitating (GATE/COARE convection)

Page 7: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

EVOLUTION of IFA time cluster (11-13 DEC 92)

Data Used:•Precipitation retrieved from SSM/I, VIS/IR satellite data Sheu et al (1996), Curry et al (1999)•3 hourly/ 30 km resolution

mm h-1

Page 8: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

mm/h

Data Used:•Precipitation retrieved from SSM/I, VIS/IR satellite data Sheu et al (1996), Curry et al (1999)•3 hourly/ 30 km resolution

EVOLUTION of IFA time cluster (11-13 DEC 92)

Page 9: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Madden & Julian (1994)

Schematics of Nakazawa (1988)

Page 10: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

IFA

Longitude

Tim

e

1

2

3 4

5

6

7

89

1011

12 13

14

15

16

Time cluster:•Lifetime > 24 h

Westwardpropagating

Eastwardpropagating

Propagation of Time Clusters

Page 11: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

IFA

Longitude

Tim

e

1

2

3 4

5

6

7

89 1

011

12

1314

15

16

Westward propagating Eastward propagating

IFA

200 hPaPROPAGATION OF TIME CLUSTERS

Page 12: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Time Evolution of Domain Average Brightness Temperature

Early morning minimum

Afternoon minimum(land)

Afternoon minimum(ocean)

Page 13: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

• Brightness temperature minimum occurs: –Early morning for 8 time clusters,

–Afternoon for 4 time clusters • Suggests that most of the time

clusters are indeed MCSs

Page 14: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Organizing Mechanisms

• Large scale flow features (e.g., 2-day waves)

• Vertical wind shear (Le Mone et al 1999)

• Mid-level mesovortices (Nagarajan et al 2004) – Dec. 15, 1992

• Mapes gravity-wave mechanism

Page 15: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Longitude

Tim

e

1

2

3 4

5

6

7

89

1011

12 13

14

15

16

Westward propagating Eastward propagating

IFA

TIME CLUSTERS & 2-DAY PERIODICITY

K

1-4, 7-9, 11-13associated with2-day wave (Chen et. al 1996,Takayabu et. al 1996)

Page 16: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

TIME CLUSTERS & VERTICAL SHEAR* (wind speed)

DATE 1000-850 hPa

800-400 hPa

6 – 19 Dec. 9228 - 31 Dec. 921, 4-6 Jan. 93

< 3.0 m s-1 < 5.0 m s-1

20 - 28 Dec. 92

> 3.0 m s-1 > 5.0 m s-1

27 Dec. 922-3 Jan. 93

< 3.0 m s-1 > 5.0 m s-1

*Areal & Temporal AveragesTemporal average: Duration of the time clusterAreal average: 0-10S, longitudinal extent of time cluster

Page 17: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

SummaryDuring the lifetime of the SCC (6Dec-

6Jan):• Identified 16 time clusters consisting

of eastward & westward propagating cloud clusters.

• Convection generally associated with 2-day wave activity

• Convection occurred in a weak vertical wind shear environment except between 20-28 Dec 1992.

Page 18: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

The Model

• Canadian mc2 model (Benoit et al. 1997)

• Fully compressible equations• Semi-Lagrangian, semi-implicit

numerics• One-way nesting of lateral boundary

conditions• RPN1 physics package

1 Recherche en Prevision du Numerique

Page 19: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

1-month long time series

00 UTC/6 Dec. 92

03UTC/7 Dec. 92

00 UTC/7 Dec. 92 03 UTC/8 Dec. 92

00 UTC/6 Jan. 93

Time series based on last 24 h of each 27h long simulation.

•00 UTC chosen because of high availability of rainfall data for assimilation •Time integration strategy follows guichard et al. (2003)

Page 20: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

3900 km

3900 km

130E 160E 190E

10N

EQ

10S

MC2 MODEL DOMAIN

Grid Size: 549 x 279 x 40, Horizontal grid length: 15 kmModel Top: 26 km

IFA

Page 21: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Modeling Strategy• Model Parameters:

– KF CPS (deep convection), BM CPS (shallow convection), Kong and Yau (1997) explicit bulk 2-ice microphysics, time step(90 s)

• Initial Conditions:– ECMWF operational analysis (0.5 o)

enhanced:• radiosonde data (Cieleski et al 2003), • temperature & moisture profiles modified

by 1D-VAR rainfall rate assimilation scheme (Nagarajan et al. 2006) and

• ABL moistening due to diurnal SST warming (Nagarajan et al 2001, 2004).

• 6-hourly lateral boundary conditions

Page 22: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

IFA averaged surface precipitation rate

Missing data

Page 23: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

IFA averaged surface sensible and latent heat flux

Page 24: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Horizontal size distribution of clouds (Model Domain)

Wielicki & Welch (1986)

Missing data

Page 25: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Domain-averaged surface precipitation rate (140-180E, 0-10S)

Missing data

Page 26: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

RH

(h)

Heig

ht

(km

)IFA Av. RH

Page 27: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

• The IFA-mean and temporal variability of:– surface fluxes of latent and sensible heat,

surface precipitation reasonable

• Large scale :– Simulated surface precipitation overpredicted– Horizontal size of cloud clusters are reasonably

simulated.

• Month long mesoscale simulation captures reasonably the life cycle of the super cloud cluster.

Conclusions

Page 28: A Numerical Study of a TOGA COARE Super Cloud Cluster – Preliminary results

Future Work• Nesting to higher resolutions (5 km

and 1 km) with new three-moment 4 - ice microphysics (Milbrandt and Yau 2005a,b)

• Diagnose mechanisms that organized the super cloud cluster

• Diagnose processes for water vapor and temperature distributions