Jacob Bleacher |
Herb Frey |
Noah Petro |
Paul Lowman |
Scott Mest (NRC) |
Jim Roark (ADNET) |
Mike Purucker (RITTS) |
David Rubincam |
Terry Sabaka |
Braulio Sanchez |
Patrick Taylor |
Coerte Voorhies |
Interest in future lunar exploration has led to renewed study of the lunar crust (P. Lowman). |
Interior crater deposits on Mars from a variety of sources provide information on surface processes (S. Mest). |
Interactive graphics software was developed for analysis of MOLA data (J. Roark). |
Buried impact basins found in MOLA data show that the Mars lowlands are very much older than we first thought (H. Frey). |
High quality planetary topography facilitates planetary comparison in the form of plastic models of Earth and Mars surface features, used in classroom and other outreach efforts (J. Roark). |
Tidal deformation models helps explain the complex landscape on Europa (T. Hurford). |
Mars crustal magnetic anomalies are studied on a global sacale (P. Taylor). |
Mars crustal magnetic anomalies are studied on an individual feature basis (M. Purucker). |
Magnetic anomaly spectra are very different for Earth and Mars and show the lack of a Mars core field (from Voorhies, Sabaka, Purucker, J. Geophys. Res.) |