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Radar map

Harmon J. K. and Slade M. A. (1992) Radar mapping of Mercury fuU-disk images and polar anomahes. Science 258, 640-642. [Pg.482]

May 20, 1978 Pioneer Venus 1, orbiter Orbit insertion Dec. 4, 1978, first radar mapping of another planetary surface, Venus atm. entry Aug. 1992... [Pg.486]

May 4, 1989 Magellan, orbiter Orhit insertion Aug. 10, 1990, radar mapping, altimetry, emissivity data for surface radio occultation expts. atm. science, end of mission and loss of orhiter Oct. 12/13, 1994 see J. Geophys. Res. 97, Aug. 25 Oct. 25, 1992. [Pg.486]

Two different interferometric radar slope monitoring systems are available. These are Synthetic Aperture Radar (GB-SAR) and Real Aperture Radar (RAR). To be useful, a radar map must have adequate resolution for its intended. A radar system that obtains a low resolution image will not adequately capture displacements leading up... [Pg.1138]

FIGURE 16 Arecibo delay-Doppler OC radar map of Maxwell Montes on Venus. (Courtesy of D. B. Campbell.)... [Pg.232]

With the Arecibo radar mapping also the search for ice on the lunar poles was performed (Stacy, Campbell and Ford, 1997 [323]). [Pg.100]

Stacy, N.J.S., Campbell, D.B., Ford, P.G. Arecibo radar mapping of the lunar poles a search for ice deposits. Science 276, 1527-1530 (1997)... [Pg.227]


See other pages where Radar map is mentioned: [Pg.163]    [Pg.44]    [Pg.50]    [Pg.104]    [Pg.104]    [Pg.164]    [Pg.1319]    [Pg.44]    [Pg.85]    [Pg.822]    [Pg.839]    [Pg.1141]    [Pg.353]    [Pg.226]    [Pg.226]    [Pg.227]    [Pg.228]    [Pg.229]    [Pg.233]    [Pg.235]    [Pg.243]    [Pg.244]   
See also in sourсe #XX -- [ Pg.104 ]




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RADAR

Radar Mapping of Spherical Targets

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