Emphasis was placed on the morphology and patterns of streaks in the Uweinat region, the relationship of topography to streak patterns, and correlation of field and laboratory studies of the desert surface sediments with color and tonal variations seen from orbit. The research objectives were to provide the necessary groundtruth information on terrestrial eolian features in order to properly interpret the orbital data and to use the interpretations as a basis for investigation of Martian eolian features
The Mars Science Laboratory (MSL) Curiosity rover landed at Gale crater in August 2012 with the goal...
Comparison of Martian tectonic and topographic features with earth and moon based on Mariner 6 and 7...
The landscape seen by the Mars Exploration Rover (MER) Opportunity at Meridiani Planum is dominated ...
Geologic interpretations of The Gilf Kebir-Uweinat of Apollo-Soyuz photographs were verified. The ph...
Global and regional patterns on Mars were inferred from surface aeolian features, such as wind strea...
Asymmetrical crater shadings and diffuse light and dark streaks visible on the photography returned ...
Eolian erosion and deposition on earth was studied in order to interpret the eolian land forms of Ma...
High spatial resolution (1.5 to 12 m/pixel) Mars Global Surveyor Mars Orbiter Camera images obtained...
High resolution images of planetary surfaces, such as of Mars from the High Resolution Imaging Scien...
Results of analysis of spectral variation of sand dunes in El Ghorabi, Bahariya, Egypt; Tombouctou/A...
Abstracts of papers regarding the Martian Channels, variable surface and atmospheric features on Mar...
Martian sedimentation is primarily aeolian with the principal source areas being the cratered highla...
Preliminary results are reported of an investigation which involves wind tunnel simulations, geologi...
The author has identified the following significant results. Recent acquisition of generally high qu...
Viking Orbiter images of intracrater dunefields in the Noachis Terra region were examined in order t...
The Mars Science Laboratory (MSL) Curiosity rover landed at Gale crater in August 2012 with the goal...
Comparison of Martian tectonic and topographic features with earth and moon based on Mariner 6 and 7...
The landscape seen by the Mars Exploration Rover (MER) Opportunity at Meridiani Planum is dominated ...
Geologic interpretations of The Gilf Kebir-Uweinat of Apollo-Soyuz photographs were verified. The ph...
Global and regional patterns on Mars were inferred from surface aeolian features, such as wind strea...
Asymmetrical crater shadings and diffuse light and dark streaks visible on the photography returned ...
Eolian erosion and deposition on earth was studied in order to interpret the eolian land forms of Ma...
High spatial resolution (1.5 to 12 m/pixel) Mars Global Surveyor Mars Orbiter Camera images obtained...
High resolution images of planetary surfaces, such as of Mars from the High Resolution Imaging Scien...
Results of analysis of spectral variation of sand dunes in El Ghorabi, Bahariya, Egypt; Tombouctou/A...
Abstracts of papers regarding the Martian Channels, variable surface and atmospheric features on Mar...
Martian sedimentation is primarily aeolian with the principal source areas being the cratered highla...
Preliminary results are reported of an investigation which involves wind tunnel simulations, geologi...
The author has identified the following significant results. Recent acquisition of generally high qu...
Viking Orbiter images of intracrater dunefields in the Noachis Terra region were examined in order t...
The Mars Science Laboratory (MSL) Curiosity rover landed at Gale crater in August 2012 with the goal...
Comparison of Martian tectonic and topographic features with earth and moon based on Mariner 6 and 7...
The landscape seen by the Mars Exploration Rover (MER) Opportunity at Meridiani Planum is dominated ...