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

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266 F. Jacob et al.ird-00392669, version 1 - 9 Jun 2009with the SEVIRI f<strong>in</strong>est temporal sampl<strong>in</strong>g, <strong>and</strong> with observations near daily temperatureextrema [187, 215]. TISIE is a two step approach for <strong>in</strong>vert<strong>in</strong>g Eq. 10.7 <strong>over</strong>TIR <strong>and</strong> MIR daytime/nighttime observations. Rais<strong>in</strong>g emissivity ratios to specificpower yields relative variations free from radiometric temperature. Assum<strong>in</strong>g TISIEare stable between consecutive observations, MIR r-emissivities can be retrieved,<strong>and</strong> next TIR ones. Various TISIE versions were designed for AVHRR, MODIS,SEVIRI [12, 186, 188, 218]. Day Night Pair is a one step approach for <strong>in</strong>vert<strong>in</strong>gboth Eqs. 10.6 <strong>and</strong> 10.7 <strong>over</strong> TIR <strong>and</strong> MIR daytime/nighttime observations. Thesystem of 2N equations with N + 2 unknowns can be solved with k additional unknowns,as long as k ≤ N − 2. Thus, the 7 MODIS channels allow rec<strong>over</strong><strong>in</strong>g fiveunknowns about atmospheric <strong>and</strong> surface effects [216].The accuracies reported for these methods range from 0.5 to 2.5 K, <strong>and</strong> areslightly worse for TTM. They correspond to sensitivity studies for TTM <strong>and</strong> TISIE[186–188], to validation exercises <strong>over</strong> various study sites for Day Night Pair(Fig. 10.6) [181, 182], <strong>and</strong> to <strong>in</strong>tercomparisons aga<strong>in</strong>st ASTER/TES retrievals forTISIE [158].10.6.2.5 Partial ConclusionsRadiometric temperature is derived by <strong>in</strong>directly <strong>in</strong>vert<strong>in</strong>g simulation modelsthrough differenc<strong>in</strong>g equations (Eq. 10.9), or directly <strong>in</strong>vert<strong>in</strong>g simple radiativetransfer equations (Eqs. 10.6 <strong>and</strong> 10.7). Solv<strong>in</strong>g the ill-posed problem depends onEmissivity10.950.90.850.80.750.70.65s<strong>and</strong>1s<strong>and</strong>2s<strong>and</strong>3s<strong>and</strong>4sahara_em20sahara_em22sahara_em23sahara_em29sahara_em31sahara_em320.63 4 5 6 7 8 9 10 11 12 13 14 15Wavelength (um)(a)Uncorrected ProofFig. 10.6 Validation, aga<strong>in</strong>st sample-based laboratory spectra (l<strong>in</strong>es), of Day Night Pair-basedMODIS retrievals <strong>over</strong> the Sahara Desert (po<strong>in</strong>ts). (From [182].)

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