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AGU: Journal of Geophysical Research, Planets

 

Index Terms

  • Planetary Sciences: Solid Surface Planets: Ices
  • Planetary Sciences: Solid Surface Planets: Polar regions
  • Planetary Sciences: Solid Surface Planets: Remote sensing
  • Planetary Sciences: Solid Surface Planets: Instruments and techniques
  • Planetary Sciences: Solar System Objects: Mars
  • Radio Science: Radio wave propagation
Abstract
Cited By (8)
 

Abstract

SHARAD sounding radar on the Mars Reconnaissance Orbiter

Roberto Seu

INFOCOM, Universitàdi Roma “La Sapienza,” Rome, Italy

Roger J. Phillips

Department of Earth and Planetary Sciences, Washington University, St. Louis, Missouri, USA

Daniela Biccari

INFOCOM, Universitàdi Roma “La Sapienza,” Rome, Italy

Roberto Orosei

Istituto di Astrofisica Spaziale e Fisica Cosmica, Rome, Italy

Arturo Masdea

INFOCOM, Universitàdi Roma “La Sapienza,” Rome, Italy

Giovanni Picardi

INFOCOM, Universitàdi Roma “La Sapienza,” Rome, Italy

Ali Safaeinili

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Bruce A. Campbell

Center for Earth and Planetary Studies, Smithsonian Institution, Washington, D. C., USA

Jeffrey J. Plaut

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Lucia Marinangeli

IRSPS, UniversitàG. d'Annunzio, Pescara, Italy

Suzanne E. Smrekar

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Daniel C. Nunes

Lunar and Planetary Institute, Houston, Texas, USA

SHARAD (SHAllow RADar) is a sounding radar provided by Agenzia Spaziale Italiana (ASI) as a Facility Instrument on the Mars Reconnaissance Orbiter mission. Its 20-MHz center frequency and 10-MHz bandwidth complement the lower-frequency, relatively narrower bandwidth capability of the MARSIS sounding radar. A joint Italian-U.S. team has guided the experiment development and is responsible for data analysis and interpretation. The radar transmits signals at a 700 Hz pulse repetition frequency (PRF) and collects reflections from both the surface and near subsurface of Mars. Vertical and horizontal resolutions are, respectively, 15 m (free-space) and 3–6 km (cross-track) by 0.3–1 km (along-track). The scientific objective of SHARAD is to map, in selected locales, dielectric interfaces to at least several hundred meters depth in the Martian subsurface and to interpret these results in terms of the occurrence and distribution of expected materials, including competent rock, soil, water, and ice. A signal-to-noise ratio of ∼50 dB (for a specular surface return) is achieved with 10 W of radiated power by using range and azimuth focusing in ground data processing. Preprocessed data as well as range- and azimuth-focused data will be formatted according to Planetary Data System (PDS) standards and be made available from the ASI Science Data Center (ASDC) and from the Geosciences Node of the Planetary Data System (PDS). Important targets for SHARAD include the polar layered deposits, sedimentary stacks (especially in Terra Meridiani), buried channel systems, buried impact craters, volcanic complexes, and shallow ice deposits in equilibrium with the atmosphere.

Received 7 May 2006; accepted 19 October 2006; published 18 May 2007.

Citation: Seu, R., et al. (2007), SHARAD sounding radar on the Mars Reconnaissance Orbiter, J. Geophys. Res., 112, E05S05, doi:10.1029/2006JE002745.

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