A unified approach to cirrus microphysics, remote sensing ...ucahdhe/Workshop_Talks/01_Baran.pdf ·...
Transcript of A unified approach to cirrus microphysics, remote sensing ...ucahdhe/Workshop_Talks/01_Baran.pdf ·...
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A unified approach to cirrus microphysics, remote sensing and climate prediction, and its impact in a climate model
Anthony Baran & Paul Field, Met Office, Exeter, UK.
Oxford Conference, March 2014
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Acknowledgements !
Peter Hill (Met Office)
Kalli Furtado (Met office)
Jerome Vidot (Centre de Météorologie Spatiale, DP/Météo-
France, Lannion, France)
Ping Yang and Bi Lei (Texas A & M)
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Wavelength range of importance to the energetics of the
Earth’s atmosphere: Solar and terrestrial Planck
emission spectrum
Wavelength m
kL~1000s kL<<1
250 K
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Complex refractive index of ice (Warren and Brandt 2007)
Scattering properties weighted by solar and terrestrial irradiances over
wavelength bands in a climate model
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A myriad of ice crystal size and shape
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Some observations: Laboratory (Bailey and Hallet 2009)
100
110
120
130
140
150
160
RHi%
Fresh Anvils, Um and McFarquhar 2008.
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Range of the size spectrum in a climate model
KL~30
KL~5700
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Ze =
Moment estimation parameterization, Field et al. (2007)
A(n) exp[B(n)Tc] M2C(n)
M2=aDb=2
PSDs in climate model
cloud microphysics
scheme same as radiation
scheme & mass-D
relationship same in both
Links PSD to ice mass (climate
model prediction) and Tc.
Moments are used to predict
cloud evolution
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Idealized Habit mixture models and their consistency with observation
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Generalise
Number Concen
Ice crystal maximum dimension
Baran & Labonnote (2007)
An example image
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Microphysical Consistency
Observed area Relationships: Area ratio:
A(D)/Ac(D)
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Asymmetry parameter, g
Extinction, ext
Single Scattering albedo, 0
Z
-1 g 1
0 0 1
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Scattering methods applied to compute the single-scattering properties
T-matrix (Havemann & Baran 2001)
& Mischenko & Travis (1997)
Physical Optics (Macke et al. 1996)
Cext=2<G>
½ < 0 <1
gtotal= 1/2(gdiff+grt) for 0=1
kL~120
Fresnel,snells law,Fraunhoffer
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Relative error in physical optics in the transition region between
the two methods at a distinct ice crystal size
Measurement uncertainty in Cext
50%
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0 and g in IWC-TC space: =1.65 µm
The IWC and cloud temperature were obtained from a number of field
campaigns including CAESAR (UK), CEPEX (Tropics), FRAMZY (Europe)
A total number of 20662 PSDs were generated & randomly generated
K(,IWC)ext(sca)=aIWC : g(,IWC)=bIWCc()
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The effect on the climate model of fixing PSD and varying habit mixture model
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Ensemble area ratios compared against in situ
measurements
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Varying the transmission properties of ice cloud
observation
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Broader PSD
Same PSD but weighted towards
more aggregated members
Temperature measurements-Observations
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Fix the PSD to best observational evidence but vary the weights to determine which weights are best to satisfy radiometric measurement
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Combine radar and lidar to obtain cloud profiles
IIR centred at 8, 11 and 12 µm
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cloud profiles of IWC
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N=26791
Global distribution of cirrus cases
0.03 < <4 Semi-transparent cirrus
Altitudes high troposphere to stratosphere
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Results
Measurement - Simulation
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What effect does this solution have in the next version of the Met Office global model?
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SW reflected flux and LW – Measurements at TOA
Likely MO/HC global model-inconsistent consistent
Climate model - Measurement
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Effect on temperature averaged over JJA, DJF
Unified-consistent Likely MO/HC global model-inconsistent
Temperature measurements-Observations
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Discussion
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Specific Research Goals
Raleigh regime GO regime
FDTD/PSTD, DDA, T-matrix … Geometric Optics Method (GOM)
Increasing Size Parameter
Fast & accurate
electromagnetic
method
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NEED ELECTROMAGNETIC SOLUTIONS TO COVER SMALL TO GEOMETRIC OPTICS REGIONS BECAUSE
Non-absorptive or weak-absorptive particles. The asymmetry factor has a valley at some resonant sizes. This is impossible for physical optics
Particles with strong absorption. The absorption efficiency factor may be larger than unity. However, the physical optics results are always smaller than unity.
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Invariant Imbedding T-matrix Method (II–TM)
Bi , L., and P. Yang, 2014: Accurate simulation of the optical properties of atmospheric ice crystals with invariant imbedding T-matrix method. J. Quant. Spectrosc. Radiat. Transfer, 138,36–49.
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KD=65
Comparison
33
T-matrix
DDA
m=1.3078+i1.67x10-8
In the Discrete-dipole-approximation(DDA )simulation, 1056 orientations with 128
scattering planes are set to achieve the randomness. Data from Bi and Yang (2014)
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Comparison between IGOM and II–TM
Bi , L., and P. Yang, 2014: Accurate simulation of the optical properties of atmospheric ice crystals with invariant imbedding T-matrix method. J. Quant. Spectrosc. Radiat. Transfer, 138,36–49.
Simulations were carried out at the EOS cluster at Texas A&M University; each single node contains 8 64-bit 2.8Ghz processors. The computational time of the II-TM increases quickly as the size parameter increases. The computational wall time (8 processors) is about 21 hours at the size parameter of 100.
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•Current models contrived – designed to re-produce observations in the form of m-D and A-D relationships
•Predict PSD and ice crystals given an initial atmospheric state?
•How does the PSD and ice crystals evolve as a function of distance from cloud-top?
•How is ice crystal complexity related to atmospheric state?
•Relate the two problems to electromagnetic theory – synergy between ice crystal growth and electromagnetic theory via Boundary Element Methods?
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Ii
Is
=0
=
Is M Ii
Is=P11()Ii
Qs=P12()Ii
1dsin)(P2
1
0
11
dsincos)(P2
1cosg
0
11
Wsca=CscaIi
Wabs=CabsIi
Wext=(Csca+ Cabs)Ii
)CC(
C
scaabs
sca
0
D
D >>
Csca=Cext=Geometrical+Diffraction=2<G>
Qext=2
D <<
Csca mass2/4
r
The single-scattering properties
-Z
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Brightness Temperature histograms – 1 month data -Inconsistent
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Brightness Temperature histograms – 1 month data : Consistent
microphysics & radiation
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Analytic Baran et al. (2001)
Ensemble distortion only Ensemble distortion and inclusions
Fully randomized
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Tests against PARASOL total reflectance (up to 14 scattering angles 60o-180o)
Fully Randomised Ensemble Inappropriate: Pristine ensemble
Is the scattering phase function
really featureless??
8 ’s 0.443 – 0.910 µm; 434000 scattering angles sampled
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Ze =
Lille Methodology: Optimal estimation (Rodgers,1976)
Minimization of the cost function
J(x) = (x-x0)T B-1 (x-x0) + (y-y(x))T R-1 (y-y(x))
x is the state vector (log10(IWC), liquid water cloud ,mid-level cloud ,water
re, mid-level re) (x0 is the a-priori)
y is the measurement vector
(IIR 8.65, 10.60 12.05 um and MODIS 0.86 and 2.13 µm)
y(x) is forward model (ensemble optical properties plus fully randomized ensemble phase function; single-homogeneous cirrus, full multiple scattering radiative transfer solar+thermal)
B is the background error covariance matrix
R is the observations+model error covariance matrix
log10((,IWC,Tc)) = a1() + b1()Tc + c1()log10(IWC)
0(,IWC,Tc) = a2() + b2()Tc + c2() log10(IWC)
g(,IWC,Tc) = a3() + b3() Tc + c3()log10(IWC)
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Cloudy Case Study (2nd March 2010) Assuming Ensemble: Single-scattering
properties in IWC-TC space
MODIS Image 1114Z
Aircraft location & lidar
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In-situ
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A note on Shattering
Assume to be artefacts of
shattered ice crystals
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Impact of Shattering on volume extinction coefficient
For the same IWC
ext=0.0021 m-1 assuming no shattering F07
ext=0.004 m-1 assuming shattering F07 with
modelled small mode
For the same IWC Assume Hex cols
ext=7.86e-04 m-1 assuming no shattering
F07
ext=0.002 m-1 assuming shattering F07 with
modelled small mode !
Error cancellation particle geometry
compensates exaggerated small mode.