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Th`ese Marouan BOUALI - Sites personnels de TELECOM ParisTech

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114 5. Application : Restoration of Aqua MODIS Band 6<br />

missing data over vegetation, clouds, <strong>de</strong>sert or oceanic surfaces require further refinement<br />

to distinguish surface cover types. In addition, it is assumed that the polynomial relation<br />

established on Terra data is transposable to Aqua. This assumption is all the more sensitive<br />

to unknown calibration differences between Terra and Aqua MODIS, and the striping<br />

noise <strong>de</strong>scribed in the previous chapters. Furthermore, the analytical relation is <strong>de</strong>rived<br />

without prior pre-processing of bands 7 and 6 for stripe noise removal.<br />

5.2.2 Local interpolation<br />

More recently, Rakwatin2009 proposed a restoration procedure for Aqua MODIS band<br />

6 that consists in three step :1) the <strong>de</strong>termination of non functioning <strong>de</strong>tectors ; 2) the<br />

correction of periodic stripes for functioning <strong>de</strong>tectors using histogram matching ; 3) the<br />

estimation of missing pixels via local cubic polynomial regression between band 6 and band<br />

7. Similarly to the approach proposed in [L. L. Wang and Nianzeng], the high correlation<br />

between band 6 and 7 reflectances is quantified using polynomial regression. However, the<br />

fitting is computed locally to account for land cover types. The restoring algorithm can<br />

be summarized with the following :<br />

1) For a <strong>de</strong>ad pixel x in band 6, a initial rectangular window of size 15 × 3 is centered<br />

at x. The minimum and maximum values of the window in band 7, respectively ρ min<br />

7<br />

and ρ max<br />

7 and their location x min , x max are <strong>de</strong>termined.<br />

2) If ρ min<br />

7 ≤ ρ 7 (x) ≤ ρ max<br />

7 , a local cubic polynomial function is calculated from the<br />

values ρ 7 (x min ), ρ 7 (x max ), ρ 6 (x min ) and ρ 6 (x max ) and used to estimated the values of<br />

ρ 6 (x)<br />

3) If ρ 7 (x) < ρ min<br />

7 , ρ 7 (x) > ρ max<br />

7 or if pixels x min or x max in band 6 are also <strong>de</strong>ad,<br />

the size of the analizing window is increased until these criteria are met.<br />

4) Step 1, 2 and 3 are repeated for every <strong>de</strong>ad pixel of band 6<br />

This local cubic interpolation procedure is illustrateed in figure 5.3.<br />

5.3 Proposed approach<br />

We propose here a simple methodology to estimate the value of Aqua MODIS band 6<br />

missing pixels. The approach is based on a concept wi<strong>de</strong>ly used in the field of hyperspectral<br />

image classification, spectral similarity. Data collected from MODIS can be perceived as a<br />

cube, where the third dimension represents the signal’s wavelenght and can also be used to<br />

extract useful information. In hyperspectral remote sensing, the <strong>de</strong>termination of surface<br />

composition requires the analysis of its reflectance spectrum and comparison with known<br />

field spectra via spectral matching techniques [Kruse et al.]. Although conditionned by the<br />

number of available spectral bands, this reasoning also applies to multispectral imagery.

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