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Modeling and Inversion in Thermal Infrared Remote Sensing over ...

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10 <strong>Model<strong>in</strong>g</strong> <strong>and</strong> <strong>Inversion</strong> <strong>in</strong> <strong>Thermal</strong> <strong>Infrared</strong> <strong>Remote</strong> Sens<strong>in</strong>g 24910.3.2 Spectral <strong>and</strong> Directional Capabilitiesird-00392669, version 1 - 9 Jun 2009The spectral dimension corresponds to the number <strong>and</strong> location of sensor waveb<strong>and</strong>swith<strong>in</strong> the TIR <strong>and</strong> optionally the MIR doma<strong>in</strong>s. The directional dimensioncorresponds to the number <strong>and</strong> angular distribution of view<strong>in</strong>g directions. Both dimensionsare used for rec<strong>over</strong><strong>in</strong>g emissivities <strong>and</strong> temperatures via model<strong>in</strong>g tools.The basic spectral configuration corresponds to TM <strong>and</strong> ETM, with 1 channel.Richer <strong>in</strong>formation is provided via two channels with GOES Imager, AVHRR <strong>and</strong>the ATSR suite; three channels with MODIS <strong>and</strong> GLI; <strong>and</strong> five channels with SE-VIRI <strong>and</strong> ASTER. Additional MIR <strong>in</strong>formation can be comb<strong>in</strong>ed with TIR <strong>in</strong>formation,to be used with cont<strong>in</strong>uous observations from geostationary sensors (SEVIRI,GOES Imager), or day night observations from sunsynchronous sensors (AVHRR,MODIS).The basic directional configuration corresponds to SEVIRI, GOES Imager, TM,ETM, <strong>and</strong> ASTER; with a s<strong>in</strong>gle view<strong>in</strong>g direction. Richer <strong>in</strong>formation is collectedfrom across track view<strong>in</strong>g with AVHRR, MODIS, GLI; <strong>and</strong> along track view<strong>in</strong>gwith the ATSR suite. Across track view<strong>in</strong>g allows a daily monitor<strong>in</strong>g, while sampl<strong>in</strong>gthe angular dynamic with<strong>in</strong> a given temporal w<strong>in</strong>dow (16 days for MODIS).This is of <strong>in</strong>terest for stable surface properties such as emissivity. For surface temperaturewhich fluctuates, captur<strong>in</strong>g the angular dynamic requires almost simultaneousobservations. This is possible with ATSR along track bi-angular observationsonly, which is limited.Future spaceborne missions will pursue current ones for long-term records: theGOES suite [100], NPOESS/VIIRS follow<strong>in</strong>g AVHRR <strong>and</strong> MODIS [101]. MTIprovides orig<strong>in</strong>al <strong>in</strong>formation: 2 MIR/3 TIR b<strong>and</strong>s, 0 ◦ <strong>and</strong> 50 ◦ along track. Atthe airborne level, the spectral dimension has been <strong>in</strong>vestigated with multispectral(TIMS, DAIS, MAS & MASTER) <strong>and</strong> hyperspectral (SEBASS [102]) sensors, <strong>and</strong>the directional dimension has been assessed with video cameras (see [103] with theReSeDA program). At the ground level, the spectral dimension has been exploredwith hyperspectral sensors (FTIR BOMEM [104]), or with broadb<strong>and</strong> radiometers[105–107], <strong>and</strong> the directional dimension has been exam<strong>in</strong>ed with goniometric systems[58, 108, 109].In the context of monitor<strong>in</strong>g l<strong>and</strong> processes, the various types of <strong>in</strong>formationpresented here are valuable for rec<strong>over</strong><strong>in</strong>g l<strong>and</strong> surface emissivity <strong>and</strong> temperature.Us<strong>in</strong>g this <strong>in</strong>formation requires design<strong>in</strong>g model<strong>in</strong>g tools <strong>and</strong> <strong>in</strong>version methods,either under development for prospective studies or with operational capabilities.10.4 Develop<strong>in</strong>g <strong>Model<strong>in</strong>g</strong> Tools <strong>and</strong> <strong>Inversion</strong> Methods<strong>Model<strong>in</strong>g</strong> tools aim at forwardly simulat<strong>in</strong>g, with different complexities, measuredbrightness temperature from emissivities <strong>and</strong> temperatures of <strong>in</strong>terest. Table 10.2provides an <strong>over</strong>view of the model<strong>in</strong>g tools currently used. Based on TIR fundamentals(Section 10.4.1), simple radiative transfer equations directly l<strong>in</strong>k measurementsUncorrected Proof

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