Viscous flow features on the surface of Mars: Observations from high‐resolution Mars Orbiter Camera (MOC) images

By Ralph E. Milliken, J. F. Mustard, D. Goldsby. 2003

285 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/a822f14644d2294b948e101be2f294ac33b57ec3

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Citations in the corpus

The Polar Deposits of Mars (2009, background): “…flow features (Milliken et al. 2003), lobate debris aprons (Pierce & Crown 2003), a dissected mantle deposit (Mustard et al. 2001), latitude-dependent topographic statistics (Kreslavsky & Head 2000, 2002), and recently formed gullies (Malin & Edgett 2000, Milliken et al. 2003) in 548 Byrne A nn u.”
Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario (2009, background): “6 km baseline (Kreslavsky and Head, 2000, 2002), and in MOC images by various latitude-dependent geomorphologies (Mustard et al., 2001; Milliken et al., 2003).”
Context Camera Investigation on board the Mars Reconnaissance Orbiter (2007, background): “…at least speculated to be related to, the presence or former presence of ice, including lobate flows on some midlatitude crater walls [Baker, 2003; Milliken et al., 2003]; arcuate ridges at the base of slopes (often associated with gullies) and pitted crater floors [Berman et al., 2005]; and…”
Impact crater formation in icy layered terrains on Mars (2006, background): “To explain the observed km-scale thickness of viscous layers of material, Milliken et al. (2003) suggest that a portion of a glacial deposit (protected by a lag deposit) may remain stable between glacial cycles, building up thicker ice-rich layers over time.”
Tropical mountain glaciers on Mars: Altitude-dependence of ice accumulation, accumulation conditions, formation times, glacier dynamics, and implications for planetary spin-axis/orbital history (2007, background): “An important advantage of ice-sheet modeling on Mars is that the theory of glacier flow is well characterized (Goldsby and Kohlsdedt , 2001; see discussion in Milliken et al., 2003).”
Thermal contraction crack polygons on Mars: Classification, distribution, and climate implications from HiRISE observations (2009, background): “…is consistent with the extent of the Martian latitude-dependent mantle: a unit interpreted to originate from the deposition and modification of tens of meters of atmospherically emplaced ice and sediments [Mustard et al., 2001; Kreslavsky and Head, 2002; Head et al., 2003; Milliken et al., 2003].”
Geologic history of Mars (2010, background): “If thick enough such mantling deposits could flow to form glaciers (Milliken et al., 2003).”