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ALPMON FINAL REPORT - ARC systems research

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

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

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

especially in 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 />

as proposed by Sandmeier and Itten (1997), is strongly recommended. Unfortunately, no such<br />

software is available to the public up to now.<br />

In summary, one can say that from visual interpretation application of the described atmospheric<br />

correction algorithms in general cannot be recommended (also compare section 3.4.2).<br />

3.3.6 Data preparation<br />

3.3.6.1 Data merging<br />

Current remote sensors offer a wide variety of image data with different characteristics in terms of<br />

temporal, geometric, radiometric and spectral resolution. Although the information content of these<br />

images might be partially overlapping, the complementary aspects represent a valuable improvement<br />

for information extraction. To exploit the entire content of multi-sensor image data, appropriate<br />

techniques for image fusion are indispensable. The adaptive image fusion (AIF) method allows the<br />

fusion of geometric (spatial) and thematic (spectral) features from multi-source raster data using<br />

adaptive filter algorithms. If applied to multi-resolution image data, it will sharpen the low spatial<br />

resolution image according to object edges found in the higher spatial resolution image. In contrast to<br />

substitution methods, such as Intensity-Hue-Saturation or Principal-Component Merging, AIF<br />

preserves the spectral characteristics of the original low resolution image.<br />

A major prerequisite for successful data fusion is the geometric and temporal accordance of the input<br />

images. A geometric displacement will lead to undesired artefacts, independent from the fusion<br />

method applied. Differences in the time of data acquisition are another source of artefacts because of<br />

changes that might occur between the two dates. However, these changes are less critical when<br />

applying AIF, as long as they only reflect changes in the spectral characteristic but not in the size of<br />

objects.<br />

Assuming no geometric or temporal variations between the images the quality of the fusion process<br />

depends on the information content of the images. Low quality of the panchromatic data might lead to<br />

poor results because the fusion algorithm will not be able to detect the features necessary for the<br />

merging procedure. However, applying substitution techniques to such a low quality image will not<br />

significantly improve the results either. The major limitation of AIF lies in the loss of local texture that is<br />

present in the panchromatic image. This local variation of grey values cannot be reconstructed in the<br />

multi-spectral image without distorting its spectral characteristic. Only edges that appear clearly in both<br />

images will be sharpened.<br />

The conclusions drawn from the application during the project are manifold. The AIF is considered<br />

useful for areas, that are dominated by objects larger than the low resolution pixel size. Taking the<br />

average pixel size of today’s multi-spectral sensors (20 – 30m) this prerequisite is only true for certain<br />

types of image objects. Due to the size and heterogeneity of the single objects, this does not hold for<br />

forest areas. There the AIF leads to a loss of details caused by averaging the multi-spectral pixels,<br />

which is due to missing information in panchromatic image. However, for the segmentation of forest<br />

and non forest areas the approach is considered valuable. One suggestion might be to use the fusion<br />

JR, RSDE, ALU, LMU, Seibersdorf, WSL 77

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