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Multilayer simulations for accurate geological interpretations of SHARAD radargrams
Authors:MG Spagnuolo  F Grings  P Perna  M Franco  H Karszenbaum  VA Ramos
Institution:1. Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, United States;2. Department of Earth and Space Sciences, University of Washington, Seattle, WA 98195, United States;3. SETI Institute, 189 N. Bernardo Ave, Mountain View, CA, United States;1. Department of Geography, Dawson College, Montreal, H3Z 1A4, Canada;2. Department of Physical Sciences, Open University, Milton Keynes, MK7 6AA, United Kingdom;3. Laboratoire de Planétologie et Géodynamique - UMR CNRS 6112, 2 rue de la Houssinière - BP 92208, Nantes, 44322 CEDEX 3, France;4. UCD School of Geography, University College, Belfield, Dublin 4, Ireland;5. UCD Earth Institute, University College, Belfield, Dublin 4, Ireland;6. The University Museum, The University of Tokyo, Hongo 7-3-1, Bunkyo-ku, Tokyo 113-0033, Japan
Abstract:SHARAD (SHAllow RADar) is a nadir-looking Synthetic Aperture Ground Penetrating Radar on board NASA's 2005 Mars Reconnaissance Orbiter. There are three main characteristics that define the performance of this instrument: ground penetration (due to the operational frequency, the observed echoes can be related to reflections from surface or subsurface), spaceborne operation (the first reflection does not necessarily correspond to the nadir reflection), and nadir looking SAR (there will always be left/right ambiguities). All this implies that there will be surface/subsurface range ambiguity and the geological interpretation of the radargrams cannot be straightforward. In order to avoid data misinterpretation, a simulator of SHARAD’s expected response for a given observation geometry and topography is needed. Simulations can take into account all surface/subsurface reflections in order to identify common families of ambiguities and facilitate the interpretation. In this work we present SHARSIM (SHARAD Radargram SIMulator), a software tool designed to simulate SHARAD radargrams taking as inputs Mars surface information and hypothetical subsurface structure. Its performance is analyzed by investigating typical artifacts and by a direct comparison with real radargrams. We show that SHARSIM simulations can help to discern between artifacts and real subsurface features in order to make accurate geological interpretations.
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