Sub-Surface Radar for the EJSM mission: discussion on environmental noise limiting performance

Details Sub-Surface Radar for the EJSM mission: discussion on environmental noise limiting performance Sub-Surface Radar for the EJSM mission: discussion on environmental noise limiting performance

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1797a&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1797

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The Europa Jupiter System Mission (EJSM) is one of the major European Space Agency (ESA) missions in the Solar System currently under study. It is aimed at exploring Jupiter and its icy moon Ganymede. The Sub-Surface Radar (SSR) instrument is a radar sounder system at low frequency (HF/VHF band) designed to penetrate the surface of Ganymede icy moon of Jupiter for performing a subsurface analysis with a relatively high range resolution. The paper addresses the main sources of environmental noises that can limit the overall performance of the radar: the presence of a relevant Jupiter radio emission and the clutter caused by characteristics of planet's surface.

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