Search Results - "Michaels, T. I."
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Significant vertical water transport by mountain-induced circulations on Mars
Published in Geophysical research letters (01-08-2006)“…Using a 3‐D, non‐hydrostatic mesoscale Mars atmospheric model with detailed aerosol/cloud microphysics, we show that the formation of discrete afternoon clouds…”
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Meteorological predictions for 2003 Mars Exploration Rover high-priority landing sites
Published in Journal of Geophysical Research - Planets (01-12-2003)“…The Mars Regional Atmospheric Modeling System is used to predict meteorological conditions that are likely to be encountered by the Mars Exploration Rovers at…”
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Meteorological predictions for candidate 2007 Phoenix Mars Lander sites using the Mars Regional Atmospheric Modeling System (MRAMS)
Published in Journal of Geophysical Research - Planets (01-03-2008)“…The 2007 Phoenix Mars lander will land in the late afternoon at a high northern latitude in the late northern hemisphere spring season. Various types of Mars…”
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Field measurements of horizontal forward motion velocities of terrestrial dust devils: Towards a proxy for ambient winds on Mars and Earth
Published in Icarus (New York, N.Y. 1962) (01-11-2012)“…► We measured the speed dust devils (DDs) move across the ground on Earth. ► Long baseline stereo imaging allowed ground motion of >100 DDs to be measured. ►…”
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Numerical modeling of Mars dust devils: Albedo track generation
Published in Geophysical research letters (01-10-2006)“…Dust devil tracks are abundant on Mars, and can significantly change the regional surface albedo, possibly altering regional‐scale atmospheric circulations…”
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Analysis of atmospheric mesoscale models for entry, descent, and landing
Published in Journal of Geophysical Research - Planets (01-12-2003)“…Each Mars Exploration Rover (MER) is sensitive to the Martian winds encountered near the surface during the entry, descent, and landing (EDL) process. These…”
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Crater Mound Formation by Wind Erosion on Mars
Published in Journal of geophysical research. Planets (01-01-2018)“…Most of Mars' ancient sedimentary rocks by volume are in wind‐eroded sedimentary mounds within impact craters and canyons, but the connections between mound…”
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Investigating the Role of Amazonian Mesoscale Wind Patterns and Strength on the Spatial Distribution of Martian Bedrock Exposures
Published in Journal of geophysical research. Planets (01-11-2022)“…The Martian highlands contain Noachian‐aged areally‐extensive (>225 km2) bedrock exposures that have been mapped using thermal and visible imaging datasets…”
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Large‐eddy simulation of atmospheric convection on Mars
Published in Quarterly journal of the Royal Meteorological Society (01-04-2004)“…Large‐eddy simulations are performed using the Mars Regional Atmospheric Modeling System (a nonhydrostatic, mesoscale model) in order to obtain a detailed,…”
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Simulation of the atmospheric thermal circulation of a martian volcano using a mesoscale numerical model
Published in Nature (London) (17-10-2002)“…Mesoscale (<100 km) atmospheric phenomena are ubiquitous on Mars, as revealed by Mars Orbiter Camera images. Numerical models provide an important means of…”
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Wind-related features in Gusev crater, Mars
Published in Journal of Geophysical Research - Planets (01-12-2003)“…Gusev crater has a complex history beginning with its formation by an impact in the Noachian Period and subsequent evolution, including erosion and deposition…”
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Comprehensive observations and geostatistics of slope streaks within the Olympus Mons aureole
Published in Icarus (New York, N.Y. 1962) (01-06-2024)“…Slope streaks (SS) are enigmatic linear features characterized by relatively low-albedo features that appear and fade on high-albedo slopes on Mars. Despite…”
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Meteorological predictions for the Beagle 2 mission to Mars
Published in Geophysical research letters (01-01-2004)“…A general circulation and mesoscale model are used to predict the weather at the Beagle 2 landing site. The afternoon high temperature predicted by the general…”
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Investigating the hysteretic behavior of Mars-relevant chlorides
Published in Icarus (New York, N.Y. 1962) (15-05-2020)“…Liquid solution stability has been a highly studied topic in the Martian community since the detection of perchlorate (ClO4−) at the Phoenix landing site and…”
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Interpretation of the complex dune morphology on Mars: dune activity, modelling and a terrestrial analogue
Published in Earth surface processes and landforms (01-10-2012)“…ABSTRACT In this work we analyze a dark erg on Mars that could be considered a mega‐dune (draa) where secondary dunes of different morphology are superposed…”
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Meteorological predictions for candidate 2007 Phoenix Mars Lander sites using the Mars Regional Atmospheric Modeling System (MRAMS) : The phoenix mission: Landing site characterization experiments, mission overviews, and expected science
Published in Journal of geophysical research (2009)Get full text
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Aeolian bedforms, yardangs, and indurated surfaces in the Tharsis Montes as seen by the HiRISE Camera: Evidence for dust aggregates
Published in Icarus (New York, N.Y. 1962) (2010)“…HiRISE images of Mars with ground sampling down to 25 cm/pixel show that the dust-rich mantle covering the surfaces of the Tharsis Montes is organized into…”
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The Mars Regional Atmospheric Modeling System: Model Description and Selected Simulations
Published in Icarus (New York, N.Y. 1962) (01-06-2001)“…The Mars regional atmospheric modeling system (MRAMS) is introduced, and selected model results are presented and compared with landed meteorological data when…”
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