Mapping the Topography of Maxwell Montes Using Ground-based Radar Interferometry

Details Mapping the Topography of Maxwell Montes Using Ground-based Radar Interferometry Mapping the Topography of Maxwell Montes Using Ground-based Radar Interferometry

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2261c&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2261

Physics

Scientific paper

We use ground-based radar interferometry to map the topography of
Maxwell Montes at a higher spatial resolution than Magellan. The data
have a spatial resolution of ~2 km and can be used to study the
relationship between emissivity and altitude on a more localized scale
than was previously possible.

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