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Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK); Thomas Lachlan Cope and John King (British Antarctic Survey). Daniel Grosvenor, T. Choularton, M. Gallagher, K. Bower, J. Crosier (University of Manchester, UK); Thomas Lachlan Cope and Russell Ladkin (British Antarctic Survey). In-cloud aircraft observations over the Antarctic Peninsula

Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

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In-cloud aircraft observations over the Antarctic Peninsula. Daniel Grosvenor, T. Choularton, M. Gallagher, K. Bower, J. Crosier (University of Manchester, UK); Thomas Lachlan Cope and Russell Ladkin (British Antarctic Survey). - PowerPoint PPT Presentation

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Page 1: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Thomas Lachlan Cope and John King (British Antarctic Survey).

Daniel Grosvenor, T. Choularton, M. Gallagher, K. Bower, J. Crosier (University of Manchester, UK);

Thomas Lachlan Cope and Russell Ladkin (British Antarctic Survey).

In-cloud aircraft observations over the Antarctic Peninsula

Page 2: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

•ContentsContents•Antarctic cloudsAntarctic clouds•Flight 102 – In situ observations of Flight 102 – In situ observations of lenticular cloudslenticular clouds

•Ice number observations – can Ice number observations – can they give an estimate of Ice Nuclei they give an estimate of Ice Nuclei concentrations?concentrations?•How do they compare to current How do they compare to current ice parameterisations (based on ice parameterisations (based on non-Antarctic clouds)?non-Antarctic clouds)?•Are Antarctic clouds different?Are Antarctic clouds different?

•Flight 104Flight 104•Ice observations at colder Ice observations at colder temperaturestemperatures•Ice formed by the Hallet Mossop Ice formed by the Hallet Mossop process.process.

Page 3: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

The BAS cloud instruments

•The CAPS instrument•Consists of 3 instruments

CAS (Cloud Aerosol Spectrometer)Size distributions of particles 0.61-50 μm in diameter

CIP (Cloud Imaging Probe)Takes images of particles 25-1550 μm in diameter (mainly ice)Can calculate size distributions from these

Hotwire probeMeasures the liquid water content

•How do Antarctic clouds differ from mid-latitude ones?Cloud Condensation Nuclei (CCN) concentrations?Ice Nuclei (IN) concentrations?Different CCN/IN sources – e.g. Bio IN?

Knowing these is important as they determine cloud reflectivity

Page 4: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

The Antarctic Peninsula region

Larsen B

Larsen C

Wilkins

1540 km

1750

km

Topography

Scale comparisonScale comparison

•Consists of a long ridge of high mountains (up to ~2000 m high).

•Have 14 flights worth of cloud data

= Rothera BAS base

Page 5: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Case study – lenticular clouds in Marguerite bay

200 250 300 350 400 450 500 550200

250

300

350

400

450

500

550

X (km)

Y (

km)

Altitude (m) from 19.6861 to 22.0281 UTC

-7

2

-70

-70

-68

-68

-66

-66

-64

-69.5

-69

-68.5

-68.5

-68

-68

-68

-67.5

-67.5

-67

-67

-66.5

-66.5

-66

500

1000

1500

2000

2500

3000

Approx wind direction

Approx wind direction

Altitude (m)Altitude (m)

Deep low in the North Weddell Sea.

Led to a strong cross Peninsula flow (east to west).

Large stacks of lenticulars were developing over the mountains.

But flew through bands of lenticulars developing out into Marguerite Bay.

Clouds most likely formed on the crests of lee waves.

= Rothera BAS base

Page 6: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Flow over mountain sets off vertical motions

Stable air on downwind side allows vertical oscillations

Lee wave clouds

•Since such clouds are likely to have been recently formed and are not likely to be deep they are quite simple•May therefore be useful to look at ice nucleation

Droplet evaporation

Droplet formation

Aerosol (CCN/IN) processing through successive clouds?

Page 7: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

The overall picture

Approx wind direction

Approx wind direction

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Page 8: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Flight segment20:20-20:40 UTC

Approx wind direction

Approx wind direction

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Page 9: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Examining the lee waves

• Gravity waves of temperature amplitude 2-5 oC.

• Horizontal wavelengths of 9-10 km.

• Predominately liquid formed at the crests of the gravity waves.

• But some ice too

• Ice present on the downward part of the waves – likely sedimentation from above

• RHi > RH at these temperatures – so would be supersaturated w.r.t. ice if are forming liquid

Page 10: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 11: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Not many observed ice crystals to base the statistics on.

Page 12: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

3500 m

3000 m

2500 m

2000 m

1500 m

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Page 13: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 14: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Distance along flight track (km)

Ice

ma

ss (

mg

m-3

)

Ice mass (mg m-3) for flight 102 on

160 170 180 190 200 210 220 2300

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1Total ice mass

Page 15: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 16: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Ice Nuclei concentration parameterisations

Heterogeneous Ice Nuclei (IN)Heterogeneous Ice Nuclei (IN)

Heterogeneous IN number cocentration (L-1)

Te

mp

era

ture

(oC

)

Ice nuclei concentations

0 0.5 1 1.5 2 2.5

-20

-15

-10

-5

WRF (Coooper)Fletcher

These include deposition IN (direct nucleation from vapour phase) and condensation IN (liquid droplet nucleated first, which then freezes)

Numbers of up to ~0.15-0.35 per litre predicted for the temperature range of the lenticulars for the WRF scheme

These include deposition IN (direct nucleation from vapour phase) and condensation IN (liquid droplet nucleated first, which then freezes)

Numbers of up to ~0.15-0.35 per litre predicted for the temperature range of the lenticulars for the WRF scheme

Actual ice concentrations of 0.1-0.45 per litre observed. Thus IN parameterisation seem to be of the right magnitude.

Actual ice concentrations of 0.1-0.45 per litre observed. Thus IN parameterisation seem to be of the right magnitude.

Page 17: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Ice number production rate (L-1 s-1)

Te

mp

era

ture

(oC

)

Ice number formation rates for P=650 mb, QC=0.1 g m-3

0 1 2 3

x 10-4

-15

-14

-13

-12

-11

-10

-9

-8

-7

-6

-5

WRF BiggsContact freezingBiggs + contact freezing

Immersion and contact INImmersion and contact IN

Ice Nuclei concentration parameterisations

•Bigg’s (immersion IN) - IN already contained within droplets•Contact IN – when droplets collide with airborne IN and freeze

Gives a rate of freezing – need to estimate a period of nucleation to get a concentration

•Bigg’s (immersion IN) - IN already contained within droplets•Contact IN – when droplets collide with airborne IN and freeze

Gives a rate of freezing – need to estimate a period of nucleation to get a concentration

Page 18: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Estimation of ice duration of formation

•Icy regions at gravity wave crests are ~5 km wide.•Wind speeds of ~20 m/s. Gives an ice forming time of ~250 s.

Gives an ice concentration of ~0.015-0.040 per litre for -11 to -14 oC.For higher LWC of 0.2 g m-3 get 0.015-0.080 per litre.

•Icy regions at gravity wave crests are ~5 km wide.•Wind speeds of ~20 m/s. Gives an ice forming time of ~250 s.

Gives an ice concentration of ~0.015-0.040 per litre for -11 to -14 oC.For higher LWC of 0.2 g m-3 get 0.015-0.080 per litre.

Actual ice concentrations of 0.1-0.45 per litre observed. Thus immersion ice parameterisations are on the low side of the observed ice concentrations.Heterogeneous IN likely slightly dominant over Biggs and contact freezing, according to parameterisations.

Overall, observed ice concentrations similar to predicted IN concentrations

Actual ice concentrations of 0.1-0.45 per litre observed. Thus immersion ice parameterisations are on the low side of the observed ice concentrations.Heterogeneous IN likely slightly dominant over Biggs and contact freezing, according to parameterisations.

Overall, observed ice concentrations similar to predicted IN concentrations

Page 19: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

Blue - indicates small particles, probably droplets

Green – large particles, probably ice

Grey - both.

3500 m

3000 m

2500 m

2000 m

1500 m

Page 20: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 21: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 22: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 23: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 24: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 25: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 26: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);
Page 27: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Summary of another flight

300 350 400 450 500 550 600 650200

250

300

350

400

450

500

550

X (km)

Y (

km)

Altitude (m) from 18.6612 to 21.9909 UTC

-70

-68

-68

-66

-66

-66

-64

-64

-62

-69

-68.5

-68

-68

-67.5

-67.5

-67

-67

-67

-66.5

-66.5

-66

-66

-65.5

-65

500

1000

1500

2000

2500

3000

3500

4000

0 1 2 3 4 5

-25

-20

-15

-10

-5

0

5

10

Ice number (L-1)

Tem

pera

ture

(o C)

Ice mass (colours; mg m-3) and number for flight 104 for 18:39:41 to 21:59:27

0

0.5

1

1.5

2

2.5

3

3.5

4

Cold temperatures of cloud over the mountain.Fairly low concentrations and large ice particles:-

Cold temperatures of cloud over the mountain.Fairly low concentrations and large ice particles:-

Ice mass (mg m-3)Ice mass (mg m-3)

Ice numberIce number

Page 28: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

0 1 2 3 4 5

-25

-20

-15

-10

-5

0

5

10

Ice number (L-1)

Tem

pera

ture

(o C)

Ice mass (colours; mg m-3) and number for flight 104 for 18:39:41 to 21:59:27

0

0.5

1

1.5

2

2.5

3

3.5

4

Hallet Mossop splinter production zonePlenty of liquid water available.Lots of ice splinter columns observed:-

Hallet Mossop splinter production zonePlenty of liquid water available.Lots of ice splinter columns observed:-

Ice numberIce number

Liquid waterLiquid water

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

-25

-20

-15

-10

-5

0

5

Hotwire LWC (g m-3)

Tem

pera

ture

(o C)

LWC&altitude (colours; m) for flight 104 for 18:40:12 to 21:58:25

500

1000

1500

2000

2500

3000

3500

4000

Ice mass (mg m-3)Ice mass (mg m-3)

Cold temperatures of cloud over the mountain.Fairly low concentrations and large ice particles:-

Cold temperatures of cloud over the mountain.Fairly low concentrations and large ice particles:-

Page 29: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Ice Nuclei parameterisation comparison

Observed ice generally < 1 per litreSuggests possible overestimation of parameterisations?

Observed ice generally < 1 per litreSuggests possible overestimation of parameterisations?

Heterogeneous IN parameterisations estimate ~2.25 L-1 at T= -20 oC Biggs freezing (immersion IN) of up to ~0.02 L-1 s-1

predicted for T= -20 oC and LWC=0.3 g m-3.

Wind speeds of 18 m/s at T=-20 oC. Ice present over distances of ~25 km.Gives estimate of ~>20 per litre at coldest temperatures.

Heterogeneous IN parameterisations estimate ~2.25 L-1 at T= -20 oC Biggs freezing (immersion IN) of up to ~0.02 L-1 s-1

predicted for T= -20 oC and LWC=0.3 g m-3.

Wind speeds of 18 m/s at T=-20 oC. Ice present over distances of ~25 km.Gives estimate of ~>20 per litre at coldest temperatures.

Heterogeneous IN number cocentration (L-1)

Te

mp

era

ture

(oC

)

Ice nuclei concentations

0 0.5 1 1.5 2 2.5

-20

-15

-10

-5

WRF (Coooper)Fletcher

Page 30: Daniel Grosvenor, Thomas Choularton, Martin Gallagher (University of Manchester, UK);

Conclusions

• Lee wave (lenticular clouds) likely provide a good “natural laboratory” to look at Ice Nuclei numbers.

• Mostly liquid formed in the gravity wave crests, but some ice was observed in the crests and in the troughs (where was likely precipitated from above).

• Ice numbers were consistent with IN parameterisations for the -11 to -14 oC temperature range.

• Parameterisations suggested that deposition/condensation IN likely the biggest source of ice.

• Likely seeding of ice from aircraft exhaust – caution required in data interpretation and flight track planning.

• For the colder clouds at -20 oC the parameterisation numbers were considerably higher than those observed (factor of 20 or so).

• In the -3 to -8 oC temperature range the Hallet Mossop process was observed producing more ice particles – concentrations up to 3.5 per litre.

• This process is likely to be important for glaciating Antarctic clouds given the likely low IN concentrations.