SETA: An Imaging Spectrometer for Marco Polo Mission

Details SETA: An Imaging Spectrometer for Marco Polo Mission SETA: An Imaging Spectrometer for Marco Polo Mission

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1203d&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1203

Computer Science

Scientific paper

The aim of the SETA experiment is to perform imaging spectroscopy in the
spectral range 400-3300 nm for a complete mapping of the Marco
Polo target with a spectral sampling of at least 20 nm and a spatial
resolution on the order of meters.

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