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ALPMON FINAL REPORT - ARC systems research

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Contract ENV4-CT96-0359 <strong>ALPMON</strong><br />

Geometric displacements between the image and the DEM is another potential source of wrong<br />

corrections. The model performs the correction according to the DEM. If the image is slightly shifted<br />

the transition between illuminated and shadow areas will not any more correspond to the topography.<br />

This leads to systematic errors on ridges and in valleys resulting in extreme over- or under-correction<br />

of areas in the magnitude of the displacement.<br />

The optimum result in topographic correction could be obtained if the entire area was covered by one<br />

cover type, which is indicated by a specific Minnaert constant. Then it could be assumed that a<br />

particular value of the Minnaert constant is valid for the entire area. In reality this scenario is rather<br />

rare, in particular in the alpine area. In order to optimise the model a priori information on the<br />

distribution of major cover types is helpful. This idea was considered in the implementation of the<br />

model by separating vegetated and non-vegetated areas applying an NDVI. The more cover types are<br />

separated the better the correction performs. On the other hand the recognition of these cover types is<br />

the major motivation for performing the topographic correction. So it was useful to apply the correction<br />

and subsequent classification in an iterative way.<br />

Nevertheless, by applying different topographic normalisation procedures in the different test sites, the<br />

satellite image quality could be significantly improved with respect to the subsequent classification of<br />

the images.<br />

2.2.4.2 Atmospheric Correction (WP7)<br />

There has been continual discussion on the meaning and quality of divers atmospheric correction<br />

algorithms within the project team. On one hand, atmospheric correction seems to be important for<br />

accurate quantitative image interpretation. On the other hand, it has been stated that none of the<br />

currently available atmospheric correction models is suitable for alpine areas. Several problems reduce<br />

the applicability of atmospheric correction especially in alpine terrain:<br />

� Methods not relying on local atmospheric measurements, are too inaccurate. For example, the<br />

Point Spread method seems to be ineffective at all. Applied on the satellite data the procedure only<br />

sharpened image features.<br />

� Applying the method of Lavreau, quantitative analysis of the corrected scenes has to be handled<br />

with care due to dramatic changes in the histograms of some spectral bands. A problem that may<br />

occur by using the Tasseled Cap method is, that the simple linear combination of LANDSAT-TM<br />

bands may not produce in every case the desired new band which is higher correlated to dust. It is<br />

not clear to what extent the coefficients, which were derived from agricultural areas in Michigan in<br />

June are valid for other areas and seasons. Also it should be kept in mind, that haze does not only<br />

change digital numbers in a spectral band but also causes a loss of information.<br />

� Other available atmospheric correction algorithms, like MODTRAN or LOWTRAN, implemented in<br />

ATCOR, strongly rely on information about the atmospheric conditions at acquisition time of the<br />

respective satellite image. This becomes a major disadvantage taking into account the poor<br />

information usually available about the atmosphere. Having different measures of the horizontal<br />

visibility within the <strong>research</strong> area at a time before or after satellite image acquisition makes<br />

estimation of a mean value necessary. The result is not very accurate and may cause overcorrection<br />

or under-correction. Over-correction, additionally, results in critical loss of information in<br />

dark areas of the image.<br />

Thus, the result of atmospheric correction is to be seen as very critical. Resulting changes appear to<br />

be not due to real correction but to errors in the correction models. The shortcomings of the available<br />

atmospheric correction algorithms are in our opinion according to the dramatic height differences in all<br />

test sites. These are not considered properly in the correction models. In this direction efforts have to<br />

be addressed to the scientific community dealing with atmospheric effects on satellite data especially in<br />

alpine terrain.<br />

Further discussion concerned the order of performing atmospheric correction before or after<br />

topographic normalisation. In general, atmospheric correction is performed on original data, followed<br />

by topographic normalisation. As atmospheric correction may cause information loss mainly within the<br />

lower grey value ranges this becomes a problem for topographic normalisation. This is due to the fact<br />

that diffuse illumination is important for atmospheric correction as well as for topographic<br />

normalisation. Therefore, the opposite order was tested as well. Not being able to solve this problem<br />

by performing the correction in two separate steps, an integrated approach for both correction tasks,<br />

JR, RSDE, ALU, LMU, Seibersdorf, WSL 20

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