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• W2510874180 endingPage "199" @default.
• W2510874180 startingPage "162" @default.
• W2510874180 abstract "We conclude our radar imaging survey of Mars, which maps spatial variations in depolarized radar reflectivity using Arecibo S-band (λ12.6 cm) observations from 2005–2012. Whereas our earlier paper (Harmon et al., 2012, Arecibo radar imagery of Mars: the major volcanic provinces. Icarus 220, 990–1030) covered the volcanic regions of Tharsis, Elysium, and Amazonis, this paper includes non-volcanic regions where hydrologic and impact processes can be the dominant resurfacing agents affecting radar backscatter. Many of the more prominent and interesting radar-bright features outside the major volcanic provinces are located in and around Chryse Planitia and Xanthe Terra. These features are identified with: a basin in northeast Lunae Planum containing the combined deposits from Maja Vallis and Ganges Catena outflows; channel outwash plains in western and southern Chryse basin; plateaus bordering chasma/chaos zones, where surface modification may have resulted from hydrologic action associated with incipient chaos formation; and some bright-ejecta craters in Chryse basin, of a type otherwise rare on Mars. Dark-halo craters have also been identified in Chryse and elsewhere that are similar to those seen in the volcanic provinces. Although the cratered highlands are relatively radar-bland, they do exhibit some bright depolarized features; these include eroded crater rims, several unusual ejecta flows and impact melts, and terrain-softened plains. The rims of large impact basins (Hellas, Argyre, Isidis) show a variety of radar-bright features provisionally identified with massif slopes, erosion sediments, eroded pyroclastics, impact melts, and glacial deposits. The interiors of these basins are largely radar-dark, which is consistent with coverage by rock-free sediments. Tempe Terra and Acheron Fossae show bright features possibly associated with rift volcanism or eroded tectonic structures, and northwest Tempe Terra shows one very bright feature associated with glacial or other ice processes in the dichotomy boundary region. The first delay-Doppler images of the radar-bright features from the north and south polar icecaps are presented. Both poles show the circular polarization inversion and high reflectivity characteristic of coherent volume backscatter from relatively clean ice. The south polar feature is primarily backscatter from the residual CO2 icecap (with a lesser contribution from the polar layered deposits), whose finite optical depth probably accounts for the feature's strong S/X-band wavelength dependence. Conversely, the north polar radar feature appears to be mostly backscatter from the H2O-ice-rich polar layered deposits rather than from the thin residual H2O cap. The north polar region shows additional radar-bright features from Korolev Crater and a few other outlying circumpolar ice deposits." @default.
• W2510874180 created "2016-09-16" @default.
• W2510874180 creator A5074966227 @default.
• W2510874180 creator A5086818248 @default.
• W2510874180 date "2017-01-01" @default.
• W2510874180 modified "2023-10-18" @default.
• W2510874180 title "Arecibo radar imagery of Mars: II. Chryse–Xanthe, polar caps, and other regions" @default.
• W2510874180 cites W1508461208 @default.
• W2510874180 cites W1603808383 @default.
• W2510874180 cites W1641745919 @default.
• W2510874180 cites W1881492471 @default.
• W2510874180 cites W1920766701 @default.
• W2510874180 cites W1932544194 @default.
• W2510874180 cites W1966238033 @default.
• W2510874180 cites W1967517928 @default.
• W2510874180 cites W1967739508 @default.
• W2510874180 cites W1968255829 @default.
• W2510874180 cites W1969665288 @default.
• W2510874180 cites W1969736911 @default.
• W2510874180 cites W1970218536 @default.
• W2510874180 cites W1971648362 @default.
• W2510874180 cites W1972753949 @default.
• W2510874180 cites W1978395515 @default.
• W2510874180 cites W1978896237 @default.
• W2510874180 cites W1979154559 @default.
• W2510874180 cites W1980658479 @default.
• W2510874180 cites W1980711571 @default.
• W2510874180 cites W1981559436 @default.
• W2510874180 cites W1981614797 @default.
• W2510874180 cites W1982160969 @default.
• W2510874180 cites W1985206187 @default.
• W2510874180 cites W1986449672 @default.
• W2510874180 cites W1988940157 @default.
• W2510874180 cites W1993154150 @default.
• W2510874180 cites W1993652213 @default.
• W2510874180 cites W1993939648 @default.
• W2510874180 cites W1995176891 @default.
• W2510874180 cites W1996228581 @default.
• W2510874180 cites W1997889228 @default.
• W2510874180 cites W1999318757 @default.
• W2510874180 cites W1999777813 @default.
• W2510874180 cites W2001102643 @default.
• W2510874180 cites W2001659855 @default.
• W2510874180 cites W2002607051 @default.
• W2510874180 cites W2002839023 @default.
• W2510874180 cites W2003023356 @default.
• W2510874180 cites W2005784391 @default.
• W2510874180 cites W2006936345 @default.
• W2510874180 cites W2007228294 @default.
• W2510874180 cites W2010020196 @default.
• W2510874180 cites W2011568504 @default.
• W2510874180 cites W2013629336 @default.
• W2510874180 cites W2013647460 @default.
• W2510874180 cites W2015271082 @default.
• W2510874180 cites W2017024114 @default.
• W2510874180 cites W2019613873 @default.
• W2510874180 cites W2019672678 @default.
• W2510874180 cites W2021115878 @default.
• W2510874180 cites W2021722013 @default.
• W2510874180 cites W2023102361 @default.
• W2510874180 cites W2028134116 @default.
• W2510874180 cites W2030139975 @default.
• W2510874180 cites W2037541159 @default.
• W2510874180 cites W2040336061 @default.
• W2510874180 cites W2044637732 @default.
• W2510874180 cites W2045287665 @default.
• W2510874180 cites W2047305551 @default.
• W2510874180 cites W2048104778 @default.
• W2510874180 cites W2048961523 @default.
• W2510874180 cites W2055776664 @default.
• W2510874180 cites W2056036768 @default.
• W2510874180 cites W2056216751 @default.
• W2510874180 cites W2056404015 @default.
• W2510874180 cites W2056999183 @default.
• W2510874180 cites W2057276801 @default.
• W2510874180 cites W2057806072 @default.
• W2510874180 cites W2058457013 @default.
• W2510874180 cites W2060402141 @default.
• W2510874180 cites W2061694321 @default.
• W2510874180 cites W2063530398 @default.
• W2510874180 cites W2064215472 @default.
• W2510874180 cites W2067007275 @default.
• W2510874180 cites W2067353794 @default.
• W2510874180 cites W2069937230 @default.
• W2510874180 cites W2070157361 @default.
• W2510874180 cites W2070870769 @default.
• W2510874180 cites W2075752194 @default.
• W2510874180 cites W2076092888 @default.
• W2510874180 cites W2076121333 @default.
• W2510874180 cites W2077234953 @default.
• W2510874180 cites W2078938542 @default.
• W2510874180 cites W2079759482 @default.
• W2510874180 cites W2080508464 @default.
• W2510874180 cites W2082197764 @default.
• W2510874180 cites W2082231146 @default.
• W2510874180 cites W2086231674 @default.
• W2510874180 cites W2086277408 @default.
• W2510874180 cites W2088496656 @default.

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