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Picardi G, Plaut JJ, Biccari D, et al. Radar soundings of the subsurface of Mars. Science. 2005;310(5756):1925-8doi: 10.1126/science.1122165.
Picardi, G., Plaut, J. J., Biccari, D., Bombaci, O., Calabrese, D., Cartacci, M., Cicchetti, A., Clifford, S. M., Edenhofer, P., Farrell, W. M., Federico, C., Frigeri, A., Gurnett, D. A., Hagfors, T., Heggy, E., Herique, A., Huff, R. L., Ivanov, A. B., Johnson, W. T., Jordan, R. L., Kirchner, D. L., Kofman, W., Leuschen, C. J., Nielsen, E., Orosei, R., Pettinelli, E., Phillips, R. J., Plettemeier, D., Safaeinili, A., Seu, R., Stofan, E. R., Vannaroni, G., Watters, T. R., & Zampolini, E. (2005). Radar soundings of the subsurface of Mars. Science (New York, N.Y.), 310(5756), 1925-8. https://doi.org/10.1126/science.1122165
Picardi, Giovanni, et al. "Radar soundings of the subsurface of Mars." Science (New York, N.Y.) vol. 310,5756 (2005): 1925-8. doi: https://doi.org/10.1126/science.1122165
Picardi G, Plaut JJ, Biccari D, Bombaci O, Calabrese D, Cartacci M, Cicchetti A, Clifford SM, Edenhofer P, Farrell WM, Federico C, Frigeri A, Gurnett DA, Hagfors T, Heggy E, Herique A, Huff RL, Ivanov AB, Johnson WT, Jordan RL, Kirchner DL, Kofman W, Leuschen CJ, Nielsen E, Orosei R, Pettinelli E, Phillips RJ, Plettemeier D, Safaeinili A, Seu R, Stofan ER, Vannaroni G, Watters TR, Zampolini E. Radar soundings of the subsurface of Mars. Science. 2005 Dec 23;310(5756):1925-8. doi: 10.1126/science.1122165. Epub 2005 Nov 30. PMID: 16319122.
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Science. 2005 Dec 23;310(5756):1925-8. doi: 10.1126/science.1122165. Epub 2005 Nov 30.

Radar soundings of the subsurface of Mars.

Science (New York, N.Y.)

Giovanni Picardi, Jeffrey J Plaut, Daniela Biccari, Ornella Bombaci, Diego Calabrese, Marco Cartacci, Andrea Cicchetti, Stephen M Clifford, Peter Edenhofer, William M Farrell, Costanzo Federico, Alessandro Frigeri, Donald A Gurnett, Tor Hagfors, Essam Heggy, Alain Herique, Richard L Huff, Anton B Ivanov, William T K Johnson, Rolando L Jordan, Donald L Kirchner, Wlodek Kofman, Carlton J Leuschen, Erling Nielsen, Roberto Orosei, Elena Pettinelli, Roger J Phillips, Dirk Plettemeier, Ali Safaeinili, Roberto Seu, Ellen R Stofan, Giuliano Vannaroni, Thomas R Watters, Enrico Zampolini

Affiliations

  1. Infocom Department, "La Sapienza" University of Rome, 00184 Rome, Italy.

PMID: 16319122 DOI: 10.1126/science.1122165

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.

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