Improving the SWS Spectrum of Titan. Correcting for the reset pulse aftermath.

Details Improving the SWS Spectrum of Titan. Correcting for the reset pulse aftermath. Improving the SWS Spectrum of Titan. Correcting for the reset pulse aftermath.

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..275k&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Mathematics

Sws Processing

Scientific paper

The SWS observation of Titan is chosen to demonstrate the benefits of correcting properly for the reset pulse aftermath in SWS detectors. The reset pulse aftermath is responsible for a certain non-linearity in the slopes which in turn might mask the presence of small glitches. And due to its changing character it is also responsible for jumps in the zero level of the detectors. Correcting for these effects we obtain straighter slopes, less affected by undetected glitches. Also most of the detector jumps disappear, not all though. The method presented here is the best which can be done within reasonable CPU limits. As such it is not fit for bulk processing. For pipeline version 9.4 and up we have implemented a different method which grabs most of the effects and which can be done in bulk.

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