#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
Times are listed in
the US/Central time zone.
Add Time Zone
Poster Session: Martian Aeolian Processes
Thursday, March 16, 2023, 6:30 PM
Town Center Exhibit Hall
Kim L. D.*
Lewis K. W.
Mapping Ventifact Orientations as Wind Indicators with the Curiosity Rover at Gale Crater, Mars
[#2733]
Using data from the Curiosity rover, we mapped ventifacts on Mars that indicated the presence of winds originating in the northeast within Gale Crater.
Using data from the Curiosity rover, we mapped ventifacts on Mars that indicated the presence of winds originating in the northeast within Gale Crater.
Kozakiewicz J.*
Dluzewski M.
Rotnicka-Dluzewska J.
Sobucki M.
Michaels T.
et al.
Typology of Coarse-Grained Ripples on Meridiani Planum, Mars
[#1616]
A developed classification of aeolian ripples on Mars based on three factors: the size of ripples, the ripple sand PSD, and the ripple formation context.
A developed classification of aeolian ripples on Mars based on three factors: the size of ripples, the ripple sand PSD, and the ripple formation context.
Widmer J. M.*
Day M.
Martian Rover Track Monitoring — A Helpful Tool to Understand Aeolian Activity
[#1272]
MER track duration / Across different terrains / Tells windy story.
MER track duration / Across different terrains / Tells windy story.
Bohacek E. V.*
Barrett A. M.
Favaro E. A.
Balme M. R.
Sefton-Nash E.
et al.
Automated Aeolian Bedform Orientation Measurements in HiRISE Images — Determining Wind Regimes on Mars
[#2966]
Sand organises / Itself into ripples when / Wind blows fast enough.
Sand organises / Itself into ripples when / Wind blows fast enough.
Barrett A. M.*
Favaro E. A.
Balme M. R.
Detecting and Measuring Transverse Aeolian Ridges (TARs) on Mars Using Deep Learning
[#1534]
We train a supervised deep learning system to segment transverse aeolian ridges on Mars and automate the computation of formative wind direction statistics.
We train a supervised deep learning system to segment transverse aeolian ridges on Mars and automate the computation of formative wind direction statistics.
Silvestro S.*
Chojnacki M.
Vaz D. A.
Botteon A.
Characterizing the Mobility of Megaripples on Mars
[#1582]
Moving and static megaripples (MRs) are found together in McLaughlin and Ganges. Fluxes for MRs and dunes are computed and topographic effects are evaluated.
Moving and static megaripples (MRs) are found together in McLaughlin and Ganges. Fluxes for MRs and dunes are computed and topographic effects are evaluated.
Martin D. N.*
Ewing R. C.
Young B. W.
Bishop M. P.
Soto A.
et al.
Classification of the Aeolian Sedimentary Systems at Herschel Crater, Mars
[#2836]
Using a grid overlain on CTX images we classified aeolian features across Herschel crater to explore the primary controls on type and distribution of sediment.
Using a grid overlain on CTX images we classified aeolian features across Herschel crater to explore the primary controls on type and distribution of sediment.
Ju M.*
Seelos K. D.
Effect of Wind Regime on Geomorphology of Russell Crater Floor on Mars
[#2681]
Russell dust and dunes / In opposite directions / An old wind regime?
Russell dust and dunes / In opposite directions / An old wind regime?
*presenter