results of the esa-due uhi project · meteorological and climate models, to facilitate preventing...
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13/12/2011
Results of the ESA-DUE UHI project
Bino Maiheu ([email protected]), on behalf of the UHI project
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13/12/2011 2© 2011, VITO NV
Outline
» Urban heat island problem
» The ESA-DUE urban heat island project
» UHI air temperature modeling approach
» TIR user requirements analysis
» Requirements for UHI modeling
» Importance of synergetic observations for studying UHI
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13/12/2011 3© 2011, VITO NV
The urban heat island
» Discomfort : thermal stress & deaths
» Energy Consumption, airconditioning
» Atmospheric chemistry (O3, emissions from energyconsumption)
» Local meteorology e.g. encreased rainfall downwind of cities
» Increased mixing heights, urban plume
» Higher temperature run-off water temperature stressesecosystems
New Orleans,Tailor & Muñoz, 1997
London
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13/12/2011 4© 2011, VITO NV
Thermal remote sensing and UHI
» Urban heat mitigation initiatives in many cities in Europe
» Clear added value of TIR remote sensing : LST retrievals !
» Optimize emergency response, reduce risk, asses mitigation measures
» Study building energy efficiency (airborne thermography)
» Aid in improving forecast, integration in urban climate modeling tools
» J.A. Voogt, T.R. Oke, Thermal remote sensing of urban climates (2003), Remote Sensing of Environment 86 (2003) 370–384
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13/12/2011 5© 2011, VITO NV
Multi-scale analysis
Oke, 1997
AVHRR
(1km)
Airborne
(10m)
IR CAM
(10cm)
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» Project financed by ESA in framework of DUE program, started end 2008.
» Quite ambitious goals :
» Build archive of 10 years worth of LST retrievals for various sensors for 10 European cities : Madrid, Lisbon, Athens, Brussels, Budapest, Sevilla, Paris, London, Bari, Thessaloniki
» Integration / assimilation of satellite remote sensing observations : Land Surface Temperature and ground weather stations data into urban meteorological and climate models, to facilitate preventing the impact of UHI and to reduce the risk of a heat wave
» Study user requirements for new TIR satellite sensor from the UHI perspective
» IEG : J. Sobrino, Benedicte Dousset, Kostas Kourtidis
The UHI project
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13/12/2011 7© 2011, VITO NV
www.urbanheatislands.info
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13/12/2011 8© 2011, VITO NV
Data sources UHI project
Sensor TIR Spatial
Resolution
Night/Day Revisiting # TIR
bands
MSG-Seviri3km
(5km)ND
Geostat.,
15min5
NOAA AVHRR 1.1 km ND [12hr] 2
MODIS (Terra
AM, Aqua PM)1 km ND Daily 10
Envisat-AATSR 1 km ND Daily 2
Landsat
(TM/ETM+)
120 m /
60 mD, [N] 16 days 1
ASTER 90 m D 16 days 4
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13/12/2011 9© 2011, VITO NV
Air temperature modeling approach
H
LEA
07/01 07/02 07/03 07/04 07/05 07/06 07/07 07/08 07/09 07/10 07/11
280
300
320
Surf
ace T
em
p [
K]
07/01 07/02 07/03 07/04 07/05 07/06 07/07 07/08 07/09 07/10 07/112
3
4
5
Ensem
ble
Std
ev
Ts Model
LST
Ens STD
Ens STD
Ensemble data assimilation technique
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13/12/2011 10© 2011, VITO NV
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13/12/2011 11© 2011, VITO NV
Validation over Paris 2003
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13/12/2011 12© 2011, VITO NV
The UHI project of ESACities and User communities involved
» TIR requirements analysis (contribution to the mission requirements for a high resolution TIR (Thermal Infra Red) satellite sensor ('Reorientation of the Fuegosat Consolidation Phase')
10 European Municipalities
Belgium: Brussels
France: Paris,
Greece (2): Athens, Thessaloniki
Italy: Bari
Spain (2): Madrid, Seville
Portugal: Lisbon
UK: London
Hungary: Budapest
Urban planning
Urban environmental quality
Meteorological services
Health prevention, emergencies
management and risk analysis
Energy efficiency (including winter
thermography)
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13/12/2011 13© 2011, VITO NV
Spatial resolution vs. revisit time gaps
Source: INDRA
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Spatial resolution
10 m 50 m 100 m
500 m 1 km
Madrid, Retiro park
2008 (DESIREX)
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TIR Requirements synthesis (INDRA)
Meteorological services / Emergencies / Urban Environment al Quality
Observation timeThe time of observation shall be at least of 2 images per day with a
minimum amplitude of 6 hours, and ideally 3 images per day
Spatial resolution The spatial resolution should be < 500 m
Revisit time The revisit time should be < Daily
Spectral Sampling At least two bands centred on 9 µm and 12 µm. Desirable: 4
Timeliness The delivery shall be NRT
Energy Efficiency and Urban Planning
Observation timeThe time of observation should be ideally 2 images per day with a
large amplitude (minimum amplitude of 6 hours)
Spatial resolution The spatial resolution should be between 1m and max
Spectral Sampling 4 TIR Bands
Revisit Time The revisit time should be weekly or more
Source: INDRA
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13/12/2011 16© 2011, VITO NV
LST in urban climate modeling
» MSG-SEVIRI too coarse, but still useful for UHI dynamics over large metropolitan areas, e.g. estimate kB-1
» De Ridder, K., C. Bertrand, G. Casanova, W. Lefebvre, and S. Mekaoui, 2011. Estimating urban thermophysical properties using thermal infared geostationary remote sensing. In preparation
» Revisit time of 1 km sensors, capturing the daily amplitude, night & day !
» Uncertainty of urban surface emissivity
» Temperature Emissivity Separation (TES) algorithms best suited
» Multiple TIR bands needed…
» Anisotropy, directional effects in TIR radiance : nadir view vs. off nadir view
» Make use of it / correct for it ?
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13/12/2011 17© 2011, VITO NV
Directional effects
» J-P Lagouarde (Remote Sensing of Env. 93 (2004) 443-462) : airborne
» Directional effects of -5 +7 K !!!
» Low res instruments (AVHRR, AATSR) can have incidence angles up to 60 °
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13/12/2011 18© 2011, VITO NV
Importance of other synergetic observations
» FVC, Albedo, urban surface characterization
» Atmospheric Composition
» Aerosol extinction & effect on UHI ?
» Effects on long wave radiation loss (greenhouse effect)
» Photo-chemistry : T dependence of O3 NO2
» Urban plume… profile measurements
Other important parameters for UHI modeling / studies
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13/12/2011 19© 2011, VITO NV