LWS observations of Mars - a search for rotational variability

Details LWS observations of Mars - a search for rotational variability LWS observations of Mars - a search for rotational variability

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..189s&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 189

Physics

5

Solar System, Mars

Scientific paper

A total of ten observations covering the full LWS wavelength were carefully reduced and analysed using pipeline 7 software and the LWS Interactive Analysis tools. The observed variability in the LWS wavelength range is consistent with a rotational modulation and compares favourably with the predictions of a thermophysical model of the Martian surface. The implications of this work on the role of Uranus as the LWS prime flux calibrator are also discussed.

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