Kilometer‐scale roughness of Mars: Results from MOLA data analysis

By M. Kreslavsky, James W. Head III. 2000

330 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/74b6e1062e9c9446b9ff8b394ea3f41aa95f7fc8

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

Icelandic analogs to Martian flood lavas (2004, background): “In fact, the average slope across the Cerberus plains is only 0.02–0.04% [ Kreslavsky and Head, 2000; Plescia, 2003; Lanagan and McEwen, 2004].”
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.”
Oceans on Mars: An assessment of the observational evidence and possible fate (2002, background): “…data have confirmed the presence of a geologically young, latitude-dependent, probably ice-and dust-rich mantle layer that is superposed on the Vastitas Borealis Formation and other units [e.g., Kreslavsky and Head, 2000; Mustard et al., 2001; Malin and Edgett, 2001; Kreslavsky and Head, 2002b].”
The timing of martian valley network activity : Constraints from buffered crater counting (2008, background): “Valleys outside the region from −30◦ to 30◦ N latitude were generally not included in order to avoid the complicating effects of recent mantling material (Soderblom et al., 1973; Kreslavsky and Head, 2000; Mustard et al., 2001) and terrain softening (Squyres and Carr, 1986).”
Multiscale Analysis of Topographic Surface Roughness in the Midland Valley, Scotland (2011, background): “…and Carver (2009), satellite imagery Beyer et al. (2003); Cord et al. (2007), bathymetric data Dartnell and Gardner (2004); Valentine et al. (2004); Lundblad et al. (2006); Wilson et al. (2007) or elevation profiles Van Der Veen et al. (1998); Kreslavsky and Head (2000); Shepard et al. (2001).”
Transverse Aeolian Ridges (TARs) on Mars (2008, background): “, 2003) is partly responsible for topographic smoothing at subkilometer scale at latitudes N30° in both hemispheres (Kreslavsky and Head, 2000).”
Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario (2009, background): “They are revealed in MOLA data by a latitudinal trend of roughness and concavity at 0.6 km baseline (Kreslavsky and Head, 2000, 2002), and in MOC images by various latitude-dependent geomorphologies (Mustard et al., 2001; Milliken et al., 2003).”
The High Resolution Imaging Science Experiment (HiRISE) during MRO’s Primary Science Phase (PSP) (2010, background): “Their occurrences sometimes include craters and inverted channel deposits within valley networks as seen in PSP_009318_1465, suggestive of water ponding and subsequent evaporation leading to their formation.”
Initial observations from the Lunar Orbiter Laser Altimeter (LOLA) (2010, methodology): “As for Mars [Aharonson et al., 2001; Kreslavsky and Head, 2000], different geologic units have distinct slope and roughness properties.”
Global surface slopes and roughness of the Moon from the Lunar Orbiter Laser Altimeter (2011, methodology): “[11] The median differential slope is a measure introduced by Kreslavsky and Head [2000] to disentangle small‐ and large‐scale contributions to surface roughness.”
Mars: Nature and evolution of young latitude‐dependent water‐ice‐rich mantle (2002, background): “Over much of the northern high latitudes, the mantle overlies the Late Hesperian Vastitas Borealis Formation (VBF), a unit with a distinctive roughness characteristic [Kreslavsky and Head, 2000].”
Recent ice ages on Mars (2003, methodology): “MGS observations The subkilometre-scale roughness derived from global Mars Orbiter Laser Altimeter (MOLA) data revealed smoothing at subkilometre scales above about 30° latitude in both hemisphere”