Eolian erosion and deposition on earth was studied in order to interpret the eolian land forms of Mars. Emphasis of the wind tunnel studies was on the flow field around models of eolian forms. Areas of the wind tunnel studies include: simulation of the atmospheric boundary layer; velocity profile measurements around different models in the desert boundary layer, and estimating shear stress distributions on the model surfaces; flow visualization techniques; streamline mapping using tuft photographs; and roughness contrasts
Wind blowing over sand on Earth produces decimeter-wavelength ripples and hundred-meter– to kilomete...
To study the eolian mechanics of saltating particles, both an experimental investigation of the flow...
Wind is one of the major drivers of geomorphic change on terrestrial bodies throughout our solar sys...
The physics and geological relationships of particles driven by the wind under near Martian conditio...
Global and regional patterns on Mars were inferred from surface aeolian features, such as wind strea...
Aeolian processes are important in modifying the surface of Mars at present, and appear to have been...
The objective of the research was to assess the significance of aeolian (windblown) processes in the...
Wind is currently the dominant geological agent acting on the surface of Mars. A study of Martian ae...
Preliminary results are reported of an investigation which involves wind tunnel simulations, geologi...
The martian surface is a natural laboratory for testing our understanding of the physics of aeolian ...
Kutzbach reports wind profiles over a series of roughness elements on a frozen lake and how the wind...
The characteristics of aerolian (wind) activity as a surface modifying process on Earth, Mars, Venus...
Emphasis was placed on the morphology and patterns of streaks in the Uweinat region, the relationshi...
Aeolian activity was predicted for Mars from earth based observations of changing surface patterns t...
The landscape seen by the Mars Exploration Rover (MER) Opportunity at Meridiani Planum is dominated ...
Wind blowing over sand on Earth produces decimeter-wavelength ripples and hundred-meter– to kilomete...
To study the eolian mechanics of saltating particles, both an experimental investigation of the flow...
Wind is one of the major drivers of geomorphic change on terrestrial bodies throughout our solar sys...
The physics and geological relationships of particles driven by the wind under near Martian conditio...
Global and regional patterns on Mars were inferred from surface aeolian features, such as wind strea...
Aeolian processes are important in modifying the surface of Mars at present, and appear to have been...
The objective of the research was to assess the significance of aeolian (windblown) processes in the...
Wind is currently the dominant geological agent acting on the surface of Mars. A study of Martian ae...
Preliminary results are reported of an investigation which involves wind tunnel simulations, geologi...
The martian surface is a natural laboratory for testing our understanding of the physics of aeolian ...
Kutzbach reports wind profiles over a series of roughness elements on a frozen lake and how the wind...
The characteristics of aerolian (wind) activity as a surface modifying process on Earth, Mars, Venus...
Emphasis was placed on the morphology and patterns of streaks in the Uweinat region, the relationshi...
Aeolian activity was predicted for Mars from earth based observations of changing surface patterns t...
The landscape seen by the Mars Exploration Rover (MER) Opportunity at Meridiani Planum is dominated ...
Wind blowing over sand on Earth produces decimeter-wavelength ripples and hundred-meter– to kilomete...
To study the eolian mechanics of saltating particles, both an experimental investigation of the flow...
Wind is one of the major drivers of geomorphic change on terrestrial bodies throughout our solar sys...