© crown copyright met office electromagnetic and light scattering by atmospheric particulates: how...

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© Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony Baran, Met Office, Exeter, UK. LMS NAMP, Durham, July 2010

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Page 1: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

© Crown copyright Met Office

Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation?Anthony Baran, Met Office, Exeter, UK.

LMS NAMP, Durham, July 2010

Page 2: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

© Crown copyright Met Office

ContentsThis presentation covers the following areas

• Why are atmospheric particulates important to the climate system

• Challenges posed by the new remote sensing era

• Observed sizes & shapes of atmospheric particles: Which model geometries?

• The single-scattering properties & Solutions

• Using measurements to constrain theory

• An application to the Met Office Unified Model: Cirrus

• Summary & Future Measurements

Page 3: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Why ice crystals & dust ?

Page 4: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Midlatitudes 20-30%

Tropics 50% - 60%

Hydrological cycle

Radiative (reflection, transmission, emission)

Uncertainties

Ice Mass ± 50%

SW flux ~± 30 Wm-2

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Wind blown mineral dust aerosol

Uncertainties

SW flux ~± 46 Wm-2

Page 6: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Volcanic Eruptions

Icelandic Volcano, April 2010

Page 7: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Challenges posed by the new remote sensing era

Page 8: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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The new remote sensing problem: The A-Train Constellation

Lidar

94 GHz cloud-profiling radar

Solar reflection & Infrared transmission

Total & polarized solar reflection

Page 9: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Observed shapes & sizes of atmospheric particulates: Which model geometries ?

Page 10: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Tropical Example, A. Heymsfield

Fresh Anvils, Um and McFarquhar 2008.University of Manchester

Page 11: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Dm 10 µm

Dm ~ 4000 µm

X ~50 – 23000 !

At ~ 0.55 µm

Page 12: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Mineral dust aerosol

Dm 1 µm

~ < 100 µm

X 5 ~ 500

Page 13: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Volcanic Dust (Iceland Volcano)

Dm 1 µm

~ several hundred µm X 5 ~ 500

Page 14: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Macke et al., 1996 Yang and Liou 1998

Labonnote et al.

2000

Baran and Labonnote 2006.

Traditional single models

Yang et al. 2003

Nousiainen 2004

McFarquhar 2002

Asano 1980

Page 15: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Consider an ensemble of ice crystals

Try to model what is observed

Ack: P Yang, B Baum and G Hong

Page 16: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Consider an ensemble of ice crystals

Number Concen

Ice crystal maximum dimension

Baran & Labonnote (2007)

Page 17: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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The single-scattering properties & Solutions

Page 18: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Iinc, Qinc, Uinc, Vinc

Isca, Qsca, Usca, Vsca

V inc

U inc

Qinc

I inc

PP

PP

PP

PP

r

V sca

U sca

Qsca

I sca

4443

3433

2221

1211

2sca

00

00

00

00

4c

111

1

1( )sin 1

2P d

P12/P11 describes the degree of linear polarization (DLP)

-

Page 19: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Total Optical Properties1

111

(cos ) (cos )cosd P g = <cos>=

g=1 g=0 g= - 1

q)dqn()qS())q(Q)q((QK asext

0=ksca/(Ksca + Kabs)

Page 20: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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X

n

X ~ 50

Electromagnetic

T-matrix

DDA

FDTD

Physical Optics

X ~ 200

Modified geometric optics

Geometric optics

X >> 200

Ray Tracing

0

~2.0

Page 21: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Scattering parameters: Geometric Optics

Page 22: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Using Measurements to constrain theory

Page 23: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Sun

Aerosol/cloudlayer

Surface

Measure transmitted radiances thro’ cloud/aerosol layer

Page 24: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Traditional single ice crystal models do not predict the measured transmitted intensity

The best fits are obtained with phase functions representing an ensemble of ice crystals

Cirrus layer =0.55 µm only

Page 25: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Mineral dust =0.55 m only

max surface

mean surface

aer= 1.0

Fails at more absorbing

wavelengths

+

Page 26: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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What do space-based satellites show ?

Satellite Sampling

Page 27: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Tests against PARASOL total & polarized reflectance (up to 14 scattering angles)

Randomised Ensemble

Are the observations ‘truth’ ???

Need polarization measurements < 60o

Inappropriate phase function

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What do single-particle levitation experiments show ?

J. Ulanowski, Univ Herts

Estimated g=0.79

Used to test fundamental scattering theory

Page 29: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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An application to the Met Office Unified Model: Cirrus

Page 30: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Consider an ensemble of ice crystalsNumber Concen

Dm

Geometric Optics

0, g, ext

Directly Related to GCM IWC & Tc

Page 31: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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0 and g in IWC-TC space

z=a+bTc+cqi

Page 32: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Ensemble (qi, Tc) - old qi/De scheme (Short-wave TOA): NO tuning

Diagnostic

Wm-2

Page 33: © Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony

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Outstanding issues

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•Theory: Can we predict the observed scattered intensity using one single scattering theory ? (Holy grail)

•Can we develop a model ensemble that is consistent across the electromagnetic spectrum – one theory – one model ?

•Can we predict the ensemble from first principles -> Aggregation, hollowness & surface roughness

•What is the role of electric fields ? Orientation ? Does it matter ?

• GCM & remote sensing in terms of optical properties related to the GCM variables IWC & Tc

•To further constrain theoretical ice crystal models high-resolution simultaneous measurements from across the electromagnetic spectrum are required (visible – far ir : sub-mm – radar)

•High-resolution scattering angle measurements (250) of polarization & intensity from the forthcoming GLORY mission (November 2010) will be fundamental in further constraining ice crystal ensemble models

• Further cirrus aircraft measurement campaigns are require to measure ice crystal or dust shapes down to < 50 µm, hollowness & surface roughness ?

•The particle size distribution not yet fully characterized; refractive indices of dust from optical to sub-mm frequencies