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nitoring polar climate change from spa Thorsten Markus NASA Goddard Space Flight Center Greenbelt, MD 20771
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Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Dec 31, 2015

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Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center Greenbelt, MD 20771. February 1996 September 1996. February 1996 September 1996. Space-borne Capabilities: - PowerPoint PPT Presentation
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Page 1: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Monitoring polar climate change from space

Thorsten MarkusNASA Goddard Space Flight Center

Greenbelt, MD 20771

Page 2: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

February 1996 September 1996

Page 3: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

February 1996 September 1996

Page 4: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

QuickTime™ and aMicrosoft Video 1 decompressorare needed to see this picture.

Page 5: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

QuickTime™ and aMicrosoft Video 1 decompressorare needed to see this picture.

Page 6: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

QuickTime™ and aMicrosoft Video 1 decompressorare needed to see this picture.

Page 7: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Space-borne Capabilities:

- Visible (Passive: Photography; Active: Laser backscattering)

- Thermal infrared (Passive: Temperature)

- Microwave (Passive: Emission; Active: Radar backscattering)

Page 8: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Space-borne Capabilities:

- Visible (Passive: Photography; Active: Laser backscattering- Very high spatial resolution (up to 15 m (Landsat))- No measurements during night or under cloudy conditions

- Thermal infrared (Passive: Temperature)- Very high spatial resolution- No measurements under cloudy conditions

- Microwave (Passive: Emission; Active: Radar backscattering)- Passive: Coarse spatial resolution (6.25 - 50 km)- Active: High spatial resolution (30 m SAR)- No dependence on solar illumination- Penetration through clouds (“more or less”)- Passive: Daily to twice-daily global coverage- Capability to retrieve sub-surface information

Page 9: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Space-borne Capabilities:

- Visible (Passive: Photography; Active: Laser backscattering- Very high spatial resolution (up to 15 m (Landsat))- No measurements during night or under cloudy conditions

- Thermal infrared (Passive: Temperature)- Very high spatial resolution- No measurements under cloudy conditions

- Microwave (Passive: Emission; Active: Radar backscattering)- Passive: Coarse spatial resolution (6.25 - 50 km)- Active: High spatial resolution (30 m SAR)- No dependence on solar illumination- Penetration through clouds (“more or less”)- Passive: Daily to twice-daily global coverage- Capability to retrieve sub-surface information`

The length of microwave observations and their continuous coverage make them the primary data source for climate studies

of sea ice

Page 10: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Some microwave fundamentals:

Every body (and everybody) is emitting radiation at a frequency spectrum depending on its temperature (blackbody radiation)

- Sun (T = 6000 K): peak in visible range- Earth (T=280 K): peak in infrared range

Microwave range is in far end of the spectrum

Most objects are not perfect emitters (blackbodies)Emissivity (between 0 and 1)

Page 11: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center
Page 12: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Microwave spectrum

Page 13: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

For example: Sea ice

Page 14: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

For example: Sea ice

These differences in emissivity enable us toderive sea ice concentration, i.e. the sea ice cover

fraction within a pixel

Page 15: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Snow depth on sea ice• Idea:

– Radiation from the ground is scattered by the snow cover.

– The more snow the more scattering.

– Scattering efficiency is frequency dependent.

– hs = c (T37GHz-T19GHz)

• Difficulties:- Different terrain forms - Scattering varies with

snow physical properties (e.g., grain size, density, wetness)

(From C.L. Parkinson, Earth from above,1997)

Page 16: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Multiyear ice

Melt/freeze, Wx

Summer melt

Snow depth product10/2004 - 9/2005

Land

Open ocean

New mulityear ice mask for AMSR-E snow depthNew mulityear ice mask for AMSR-E snow depth

Page 17: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Other variables derivable from passive microwave data:

- Sea ice type- Ice temperature- Melt onset and end- Sea ice drift

Page 18: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

hs

hi

hf

i

s

w

ICESat (laser altimeter)

Cryosat2 (radar altimeter, 2009)

hs = snow depthhi = ice thickness hf = freeboard

What is missing? The 3rd dimension!

Page 19: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Importance of sea ice (1): Global energy balance; Ice/snow albedo feedback

Ocean

Forest

Snow/ice

Page 20: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Importance of sea ice (2): Ocean circulation

What makes the ocean move?1) Wind-driven surface currents 2) Thermohaline circulation

Page 21: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Importance of sea ice (3): Ecology, e.g. polar bears

Page 22: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center
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Change in temperature 30 years after collapse of the thermohaline circulation

Michael Vellinga, Hadley Centre

Page 25: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center
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From Gordon and Comiso, 1988

Moisture flux

Albedo

Ice drift

PrecipitationProcesses:

Page 28: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Warmer temperatures

More moisture

More precipitation

More freshwater input into ocean

More stable Southern Ocean

Less entrainment of WDW

Antarctic sea ice increase with global warming?

More sea ice production

Page 29: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Warmer temperatures

More moisture

More precipitation

More freshwater input into ocean

More stable Southern Ocean

Less entrainment of WDW

Antarctic sea ice increase with global warming?

More sea ice production

Thicker snowon sea ice

More snow-to-ice conversion

More thermal insulation

Less basal freezing

Page 30: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Change in sea ice volume as a function of precipitation(Balance between thermal insulation and snow-to-ice conversion)

Page 31: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

??

Page 32: Monitoring polar climate change from space Thorsten Markus NASA Goddard Space Flight Center

Past Present Future

Observations

Data analysis; process studies

Modeling

Validation; enhancement

Extrapolation;trends; cycles

Assimilation