Wet, dry, and stabilized dune systems
Aeolian systems exist as a dynamic continuum that, for convenience, are assigned dry, wet, and stabilized end members. Aeolian dunes […]
Aeolian systems exist as a dynamic continuum that, for convenience, are assigned dry, wet, and stabilized end members. Aeolian dunes […]
Bounding surfaces are an integral part of aeolian dune stratigraphy. Aeolian dune stratification is characterized by crossbedding. Crossbeds occur in
A series introducing aeolian processes and deposition, comparing the conditions on Earth and Mars. Key words: sand dunes, ripples, crossbeds,
A series introducing aeolian processes and deposition, comparing the conditions on Earth and Mars. Key words: Curiosity rover, Namib dune,
An Introduction to aeolian processes and deposition, comparing the conditions on Earth and Mars. Key words: Mars, Hadley cell, barchan
An Introduction to wind-blown, aeolian deposition, comparing the conditions on Earth, Mars, Venus, and Titan. Modern sand dunes cover extensive
The experiment at the Experimental EarthScape facility focused on evaluating sequence stratigraphic discordances in a scale-independent sedimentary basin model. Key findings included significant stratigraphic surfaces like downlap and onlap, generated during base level changes. The results align well with natural stratigraphic systems, showcasing the importance of base level dynamics in sedimentary processes.
This post discusses an experimental stratigraphic modeling process conducted at Minnesota University’s Experimental EarthScape facility. It highlights the methods, boundary conditions, and variable base levels used to analyze sedimentary systems and stratigraphic responses, building on previous research by Martin et al. and emphasizing the importance of controlling various factors.
This post is part of a series on Mars geology that focuses on sedimentary processes and systems. Why focus on
The rocky planets – Mercury, Venus, Earth (its Moon), and Mars Our knowledge and understanding of the Solar System and