Radiometer retrievals of LWP

11
Radiometer retrievals of LWP Nicolas GAUSSIAT

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Radiometer retrievals of LWP. Nicolas GAUSSIAT. Statistical/physical retrieval. Physical retrieval : k l , k v,  d are estimated using GCM model vertical information, then with - PowerPoint PPT Presentation

Transcript of Radiometer retrievals of LWP

Page 1: Radiometer retrievals of LWP

Radiometer retrievals of LWP

Nicolas GAUSSIAT

Page 2: Radiometer retrievals of LWP

Statistical/physical retrieval

SOME BASICS:Radiometers measure Tb at 22.2 GHz end 28.8 GHz

with

bm

skym

TT

TTlog

Physical retrieval : kl, kv, d are estimated using GCM model vertical information, then with

Statistical retrieval : a22, a28 and b are assumed to be constant and directly deduced from observations of Tb and LWP

28,28,28,28

22,22,22,22

dvl

dvl

VWPkLWPk

VWPkLWPk

bTaTaLWP bb 28,2822,22

),,,,,(,, 28,22,28,22,28,22,2822 ddvvll kkkkfbaa

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Model data /radiosondes4 years of radiosondes2 years of model data

LWP

VWP

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Physical retrieval (Kl22, kv22, d22), (Kl28, kv28, d28) are estimated using GCM model (ECMWF)

for each profiles, and a22, a28 and b are deduced.

Kl22, Kl28

Kv22, Kv28

d22, d28

a22

a28

b

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Statistical retrieval

a22

(kg/m2xm)

a28

(kg/m2xm)

b (kg/m2xm)

RMS errorg/m2

Using (m)LWP<500 g/m2 -1.9962 6.8043 -0.1530 17 g/m2

0.0017 cm

Using Tb instead of LWP<500 g/m2

-0.009 0.029 -0.197 20 g/m2

0.0017 cm

Using Tb instead of Simpson et Al.

-0.008 0.025 -0.126 18 g/m2

0.0018 cm

Use of a bi-linear regression to work out a22, a28 and b directly

We assume that LWPi depends linearly on the optical depths 22i and 28i

Ideally, we want to find a22, a28, b for all the N measurements : a22 22i + a28 28i + b =LWPi

But the best we can do is to minimize the sum : R2 = (a22 22i + a28 28i + b - LWPi)2

In matrices notations A=[…(22i 28i 1) ;…(22N 28N 1) ] X=[a22 ; a28 ; b] Y=[… LWPi ;… LWPN]

X = (AtA)-1 AtY

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Lidar identify liquid-cloud-free regions (LWP should be 0)

Results can look good but …

statisticalphysicalclear sky

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when it comes to the details…

minutes

Fluctuations must be due to a calibration problem…

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Cunning technique…In clear sky conditions LWP=0 so we have :

then (1)

A second constrain is found by minimizing the cost fct J,

then (2)

So, from (1) and (2), we work out C22 , C28 in the clear sky regions and interpolate values in between

28,

2828,28

22,

2222,22

v

d

v

d

k

C

k

C

28,28,28

22,22,22

dv

dv

VWPk

VWPk

228

222 CCJ

2822,

28,22 C

k

kC

v

v

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…cunning results(1)Chilbolton offset (lens ?) … solved

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Palaiseau calibration problem… not a problem.

…cunning results(2)

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Further improvement Lidar measure cloud-base and using model temperature a better estimate of Kv is obtained.