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The IMF spectrometric reference lab makes substantial contributions to databases for monitoring atmospheric trace gases. Due to the high number of spectral bands and ambitious accuracy requirements, this task is particularly challenging in the domain of atmospheric sounding. Preconditions are both precise understanding of the measuring equipment and constant monitoring of the instrument’s characteristics over the entire mission duration. The know-how obtained here benefits the conception and operation of hyper-spectrometers such as HySpex, ROSIS or EnMap.
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