Performances of the Data Compression and Binning Algorithms adopted on the VIRTIS-M Spectrometer onboard Rosetta

Computer Science – Performance

Scientific paper

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Scientific paper

This paper describes the analysis of the consequences on the retrieval of reflectance spectra of using several levels of data compression algorithms and of degrading the instrument resolution by means of spectral/spatial binning. These are software algorithms available on the spectrometer VIRTIS-M onboard the ESA's Rosetta spacecraft. An accurate knowledge of the compression algorithms performances and of the spectral/spatial binning performances will be very useful when Rosetta will arrive to its main target (comet 67P/Churyumov-Gerasimenko) in order to define the limits of operability of VIRTIS-M and therefore to plan a set of observation types which can be adapted to various phases and to various scientific objectives. This analysis has used observations performed during Earth swing-by#1 and Earth swing-by#3 which have been planned explicitly for this purpose.

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