%0 Journal Article %1 GiovanniPicardi12232005 %A Picardi, Giovanni %A Plaut, Jeffrey J. %A Biccari, Daniela %A Bombaci, Ornella %A Calabrese, Diego %A Cartacci, Marco %A Cicchetti, Andrea %A Clifford, Stephen M. %A Edenhofer, Peter %A Farrell, William M. %A Federico, Costanzo %A Frigeri, Alessandro %A Gurnett, Donald A. %A Hagfors, Tor %A Heggy, Essam %A Herique, Alain %A Huff, Richard L. %A Ivanov, Anton B. %A Johnson, William T. K. %A Jordan, Rolando L. %A Kirchner, Donald L. %A Kofman, Wlodek %A Leuschen, Carlton J. %A Nielsen, Erling %A Orosei, Roberto %A Pettinelli, Elena %A Phillips, Roger J. %A Plettemeier, Dirk %A Safaeinili, Ali %A Seu, Roberto %A Stofan, Ellen R. %A Vannaroni, Giuliano %A Watters, Thomas R. %A Zampolini, Enrico %D 2005 %J Science %K mars perugia ciro geomorphology radar geophysics subsurface imported topography %N 5756 %P 1925-1928 %R 10.1126/science.1122165 %T Radar Soundings of the Subsurface of Mars %U http://www.sciencemag.org/cgi/content/abstract/310/5756/1925 %V 310 %X The martian subsurface has been probed to kilometer depths by the Mars Advanced Radar for Subsurface and Ionospheric Sounding instrument aboard the Mars Express orbiter. Signals penetrate the polar layered deposits, probably imaging the base of the deposits. Data from the northern lowlands of Chryse Planitia have revealed a shallowly buried quasi-circular structure about 250 kilometers in diameter that is interpreted to be an impact basin. In addition, a planar reflector associated with the basin structure may indicate the presence of a low-loss deposit that is more than 1 kilometer thick.

@article{GiovanniPicardi12232005, abstract = {The martian subsurface has been probed to kilometer depths by the Mars Advanced Radar for Subsurface and Ionospheric Sounding instrument aboard the Mars Express orbiter. Signals penetrate the polar layered deposits, probably imaging the base of the deposits. Data from the northern lowlands of Chryse Planitia have revealed a shallowly buried quasi-circular structure about 250 kilometers in diameter that is interpreted to be an impact basin. In addition, a planar reflector associated with the basin structure may indicate the presence of a low-loss deposit that is more than 1 kilometer thick. }, added-at = {2007-02-27T20:40:57.000+0100}, author = {Picardi, Giovanni and Plaut, Jeffrey J. and Biccari, Daniela and Bombaci, Ornella and Calabrese, Diego and Cartacci, Marco and Cicchetti, Andrea and Clifford, Stephen M. and Edenhofer, Peter and Farrell, William M. and Federico, Costanzo and Frigeri, Alessandro and Gurnett, Donald A. and Hagfors, Tor and Heggy, Essam and Herique, Alain and Huff, Richard L. and Ivanov, Anton B. and Johnson, William T. K. and Jordan, Rolando L. and Kirchner, Donald L. and Kofman, Wlodek and Leuschen, Carlton J. and Nielsen, Erling and Orosei, Roberto and Pettinelli, Elena and Phillips, Roger J. and Plettemeier, Dirk and Safaeinili, Ali and Seu, Roberto and Stofan, Ellen R. and Vannaroni, Giuliano and Watters, Thomas R. and Zampolini, Enrico}, biburl = {https://www.bibsonomy.org/bibtex/29814f8515c2acd745862f883f6c8774f/andreab}, doi = {10.1126/science.1122165}, eprint = {http://www.sciencemag.org/cgi/reprint/310/5756/1925.pdf}, interhash = {4dc79cec1fd02e495b03fcf949357b5c}, intrahash = {9814f8515c2acd745862f883f6c8774f}, journal = {Science}, keywords = {mars perugia ciro geomorphology radar geophysics subsurface imported topography}, number = 5756, pages = {1925-1928}, timestamp = {2007-02-27T20:40:57.000+0100}, title = {{Radar Soundings of the Subsurface of Mars}}, url = {http://www.sciencemag.org/cgi/content/abstract/310/5756/1925}, volume = 310, year = 2005 }