MOC observations of the 2001 Mars planet-encircling dust storm

By B. Cantor. 2007

233 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Earth-Surface Processes

View Paper: https://www.semanticscholar.org/paper/580407affd1b4821a0b47b00613a7f487e2f2984

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In Astronomy and Astrophysics

In Earth-Surface Processes

Citations in the corpus

Context Camera Investigation on board the Mars Reconnaissance Orbiter (2007, background): “[27] Dust storms, as with dust devils, come in a variety of sizes and commonly occur at predictable times and pass through the same regions year after year [Cantor et al., 2001; Cantor, 2003, 2007].”
Selection of the InSight Landing Site (2017, methodology): “116, doi:10.1029/2011je003857. C.S. Edwards, K.J. Nowicki, P.R. Christensen, J. Hill, N. Gorelick, K. Murray (2011b) Mosaicking of global planetary image datasets: 1.”
Spacecraft Observations of the Martian Atmosphere (2008, methodology): “He also thanks Bruce Cantor for images of dust storms from the MGS MOC camera, Paul Withers for temperature profiles obtained by the MER Spirit and Opportunity rovers during their descent through the atmosphere, and John Wilson for Viking IRTM temperatures.”
Mars Science Laboratory Observations of the 2018/Mars Year 34 Global Dust Storm (2018, background): “…1979; Newman et al., 2002; Wilson, 1997; Zurek, 1982), change surface albedo patterns (e.g., Cantor, 2007; Szwast et al., 2006; Vincendon et al., 2015), and modify subsequent transport and deposition of water and CO 2 at the poles (Benson & James, 2005; Cantor, 2007; Strausberg et al., 2005).”
Dust aerosol, clouds, and the atmospheric optical depth record over 5 Mars years of the Mars Exploration Rover mission (2014, background): “The earliest was the most extensive of these dust events, observed as the MGS spacecraft came out of contingency mode on 27 December 2004, LS = 135 (Cantor, 2007).”
An overview of the 1985-2006 Mars Orbiter Camera science investigation (2010, background): “Cantor (2007) noted that most storms were observed to develop in close proximity to the seasonal and residual polar cap margins (e.g., Figure 33).”
Eight-year climatology of dust optical depth on Mars (2014, background): “Because dust storms on Mars have a wide range of spatial and temporal scales (Cantor, 2007; Wang et al., 2003, 2005), these discrete observations can affect the space–time representation of dust storm activity.”