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Latent Heating Evaluation

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Latent Heating Evaluation Yukari N. Takayabu CCSR/Univ. of Tokyo with S. Shige, Osaka Prefecture University, W.-K. Tao, C.-L. Shie, GSFC/NASA, and Y. Kodama, Hirosaki ... – PowerPoint PPT presentation

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Title: Latent Heating Evaluation


1
Latent Heating Evaluation
  • Yukari N. Takayabu
  • CCSR/Univ. of Tokyo
  • with
  • S. Shige, Osaka Prefecture University,
  • W.-K. Tao, C.-L. Shie, GSFC/NASA,
  • and Y. Kodama, Hirosaki University

2
TRMM Spectral Latent Heating (SLH) Estimate
  • SLH utilizes precipitation-top-heights and
    precipitation rate at melting level and at
    surface obtained from TRMM PR for the LH
    estimates.
  • With the aid of a 2D Cloud Resolving Model
    (GCEM) simulations forced by field experiment
    data, SLH constructs a set of precipitation-LH
    tables for convective rain and stratiform rain,
    separately. (Shige et al.
    2004, JAM)

3
Spectral Latent Heating (SLH) Algorithm
Field Experiments
COARE
SCSMEX
GATE
2D CRM simulation (GCEM)
Lookup Tables Conv / Strat
Simulated rain
PR2a25 Rain
Retrieval
GV
Diagnosed Q1R
Simulated Q1R
Reconstructed Q1R
Estimated Q1R
4
GV for LH
Apparent Heat Source Apparent Moisture Sink
diagnozed from upper-air network observations
(Yanai et al. 1973)
? Large-scale network observation, such as GATE,
COARE, SCSME, KWAJEX.
Q1RQ1-QR
? Large-scale network observation
5
Field Experiments
6
Q1R with COARE-TABLE-SLH vs. GCE-simulated
GATE Reconstructed Q1R is higher than simulated
(forced)
(b) SCSMEX 2-9 Jun 1998
SCSMEX Reconstructed Q1R is lower than
simulated (forced)
7
For the same storm height, precipitation
profiles, therefore Q1R profiles, differ among
experiments.
8
COARE LH look-up tables
Pf Additional usage of precipitation rate 1km
above the melting level for the convective
rain We also adjusted the melting level of the
table to the observed melting level.
9
Heating from diagnostic calculations (Johnson and
Ciesielski 2002) and SLH algorithm for SCSMEX (15
May 20 June 1998).
Budget Q1
SLHQ1RGCE QR
10
Possibility of utilizing wind profiler w-wind
data for evaluating Q1
Kodama (2005)
11
GPM ERA
Precipitating Phenomena in the Midlatitude with a
significant role of LH
  • Explosive developments of the extratropical
    cyclones (ex. QEII Storm in 1978)
  • Mesoscale (meso-alpha, beta) systems in the
    Baiu front
  • Winter disturbances over the Japan Sea

12
GPM ERA
Precipitating Phenomena in the Midlatitude with a
significant role of LH
  • Explosive developments of the extratropical
    cyclones (ex. QEII Storm in 1978)
  • Mesoscale (meso-alpha, beta) systems in the
    Baiu front
  • Winter disturbances over the Japan Sea

13
GPM ERA
Precipitating Phenomena in the Midlatitude with a
significant role of LH
  • Explosive developments of the extratropical
    cyclones (ex. QEII Storm in 1978)
  • Mesoscale (meso-alpha, beta) systems in the
    Baiu front
  • Winter disturbances over the Japan Sea

14
The role of the Latent Heating on the explosive
development of Extratropical Cyclone (Queen
Elizabeth II Storm)
QEII
Omega for different LH peaks
Difference of Psfc and winds between with and
without LH
300hPa
500hPa
700hPa
Pressure drop
Anthes et al. 1983
Gyakum 1983
Time ?
15
Mesoscale Precipitation Systems on the Baiu Front
X-BAIU-99
Moteki et al. 2004
Three-dimensional dynamical structure determines
the precipitation characteristics which feed back
to the dynamical fields.
Baiu front
continental moist air
oceanic moist air
Water vapor front
16
Winter Disturbances over the Japan Sea (Yoshizaki
et al. 2004)
WMO-01
GMS
5km-NHM
JPCZ is well simulated
QuickSCAT
Sfc flux contributes largely to ltQ1gt ltQ1-QR-Q2gt
SLE
17
www.ecmwf.int
From Dr. M. Ishihara (JMA)s presentation
18
GPM ERA
Precipitating Phenomena in the Midlatitude with a
significant role of LH
  • Interaction with dynamical three-dimensional
    structures of phenomena becomes more important.
  • Various network observations and other satellite
    data (winds, clouds) will be available.
  • Larger computer resources will be available.

19
Latent Heating Estimates and GV in GPM ERA
  • With these background,
  • GPM precipitation More satellites to observe
    winds, and clouds
  • Wind Profiler Networks
  • Radar Networks (NEXRAD, R-AMeDAS)
  • Non-hydrostatic Numerical Models with larger
    computer resources
  • We should collaborate for ? 4DVar data
    assimilation
  • (In collaboration with operational
    organizations)
  • Field experiments to verify the analysis data
  • Especially, validation for model cloud
    microphysics will be very important

20
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