UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Monitoring aeolian bedform migration rates on Mars

Boazman, Sarah Jane; (2022) Monitoring aeolian bedform migration rates on Mars. Doctoral thesis (Ph.D), UCL (University College London). Green open access

[thumbnail of SN17115067_Sarah_Jane_Boazman_Monitoring Aeolian Bedform Migration Rates on Mars.pdf]
Preview
Text
SN17115067_Sarah_Jane_Boazman_Monitoring Aeolian Bedform Migration Rates on Mars.pdf

Download (28MB) | Preview

Abstract

In recent years aeolian bedforms across the surface of Mars have been monitored, however, the boundary conditions that control bedform migration rates in different topographical and environmental settings are yet to be explored. Especially the effect of local conditions (topography, CO2 ice presence, and if bedforms are located on plains or within a crater) on bedform migration, in comparison to regional conditions. In this thesis I measured dune migration rates in three different environments, using images from the ConTeXt (CTX) and High Resolution Imaging Science Experiment (HiRISE) cameras on board the Mars Reconnaissance Orbiter (MRO), with software Co-Registration of Optically Sensed Images and Correlation (COSI-Corr) method. In Valles Marineris the topography of the valley caused fast slope winds, which converged with winds flowing through the valley allowing migration of 0.3m/EY of some of the tallest dunes (up to 180 m in height) on Mars. Near Scandia Cavi, near the north pole of Mars, CO2 ice stabilized linear dunes during the martian winter and lateral migration of the dunes occurred only in ice free seasons, of up to 2 m/EY. Fast circumpolar winds, combined with local topographic winds likely caused the fast migration rates. In the region surrounding landing sites of NASA’s Mars 2020 and ExoMars 2022 missions, I demonstrated craters can act as sediment traps by investigating three dune fields within craters near each landing site and measured migration rates varying from 0.5 m/EY to 5.6 m/EY. These three studies demonstrate that the local boundary conditions dominantly control the wind regimes present which can be complex, which in turn, control the bedform migration rates. Investigating the boundary conditions at future Mars landing sites would prove valuable by showing possible areas of aeolian erosion exposing fresh outcrops for sampling, which would further the understanding of the geomorphology and geology of Mars.

Type: Thesis (Doctoral)
Qualification: Ph.D
Title: Monitoring aeolian bedform migration rates on Mars
Event: UCL
Open access status: An open access version is available from UCL Discovery
Language: English
Additional information: Copyright © The Author 2022. Original content in this thesis is licensed under the terms of the Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0) Licence (https://creativecommons.org/licenses/by-nc/4.0/). Any third-party copyright material present remains the property of its respective owner(s) and is licensed under its existing terms. Access may initially be restricted at the author’s request.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Earth Sciences
URI: https://discovery.ucl.ac.uk/id/eprint/10142280
Downloads since deposit
191Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item