Objectives:
Wind-driven processes dominate the present day surface environment on Mars. Understanding landform and bedform evolution by wind action helps determine Mars’ evolutionary history. Aeolian (windblown) accumulations now dominate the planet’s surface in the form of extensive dune fields and within these a distinct bedform type known as Transverse Aeolian Ridges (TARs) are common. These enigmatic landforms are distributed semi-globally and are closely associated with local climate and wind regimes, however, present day winds may not necessarily be representative of original formative processes or mechanisms of TARs. Ambiguity therefore exists on their origin, genesis and dynamics, however, recent high-resolution remote sensing imagery (HiRISE) has revealed much more detail on their 3D form and extent.
TARs have simple ripple-like form and are often far bigger (up to tens of metres across) than similar bedforms on Earth such as megaripples. Few in-situ measurements of TARs have been made on Mars, as Rovers have tended to avoid accumulations of sand for reasons of safety. Therefore, many questions remain, including “why are TARS so much bigger than ripples on Earth?”, and “When and how rapidly do they form?”. Terrestrial analogue studies can help answer these questions. The use of Terrestrial analogues allows us to study geological processes observed on other planets such as Mars. Some examples of bedforms similar to TARs do occur on Earth, and provide an excellent opportunity to explore in situ (instrumented) localised airflow around these features as well as any associated sediment flux patterns. Using findings from Earth analogues (Iceland) this project will explore similarly scaled TARs found in Martian settings to directly compare their behaviour between both environments and shed new light on their origins on Mars. A range of sites on Mars will be selected to expand our investigations of TARs to examine their evolutionary patterns and also the winds that would have been/are transport capable and therefore responsible for the genesis and/or the movement.
The project will use the mesoscale climate model MarsWRF (Richard et al., 2007) to help supply high resolution 3D computational Fluid Dynamic modelling of airflow both on Earth (Jackson et al., 2011, 2020) and Mars (Jackson et al., 2015) to investigate spatial patterns of surface wind forcing over and around TARs. Instrumented field experiments at sites in Iceland will make use of a suite of monitoring equipment including terrestrial laser scanning, drones, high frequency 3D sonic anemometry and load cell sediment flux traps.
Candidates will be expected to have a background in geological/earth sciences and/or physical sciences (physics, astronomy, astrophysics).
References will be requested for shortlisted candidates.
Applicants should hold, or expect to obtain, a First or Upper Second Class Honours Degree in a subject relevant to the proposed area of study.
We may also consider applications from those who hold equivalent qualifications, for example, a Lower Second Class Honours Degree plus a Master’s Degree with Distinction.
In exceptional circumstances, the University may consider a portfolio of evidence from applicants who have appropriate professional experience which is equivalent to the learning outcomes of an Honours degree in lieu of academic qualifications.
The University offers the following levels of support:
The following scholarship options are available to applicants worldwide:
These scholarships will cover full-time PhD tuition fees for three years (subject to satisfactory academic performance) and will provide a £900 per annum research training support grant (RTSG) to help support the PhD researcher.
Applicants who already hold a doctoral degree or who have been registered on a programme of research leading to the award of a doctoral degree on a full-time basis for more than one year (or part-time equivalent) are NOT eligible to apply for an award.
Please note: you will automatically be entered into the competition for the Full Award, unless you state otherwise in your application.
The scholarship will cover tuition fees at the Home rate and a maintenance allowance of £19,000 (tbc) per annum for three years (subject to satisfactory academic performance).
This scholarship also comes with £900 per annum for three years as a research training support grant (RTSG) allocation to help support the PhD researcher.
Due consideration should be given to financing your studies. Further information on cost of living
Balme, M., Berman, D.C., Bourke, M.C., Zimbelman, J., 2008. Transverse aeolian ridges (TARs) on Mars. Geomorphology 101 (4), 703–720.
Foroutan, M. and Zimelman, J.R. 2020 Evaluation of large data sets for Transverse Aeolian Ridges on Erth and Mars. Planetary and Space Science, 189, 104966.
Jackson, D.W.T., Beyers, J.H.M., Lynch, K., Cooper, J.A.G., Baas, A.C.W. and Delgado-Fernandez, I. 2011. Investigation of three dimensional wind flow behaviour over coastal dune morphology under offshore winds using Computational Fluid Dynamics (CFD) and ultrasonic anemometry. Earth Surface Processes and Landforms, 36 (8), 1113–1124.
Jackson, D.W.T., Bourke, M.C. and Smyth, T.A.G. 2015. The dune effect on sand-transporting winds on Mars. Nature Communications, 6:8796.
Jackson, D.W.T., Cooper, J.A.G., Green, A., Beyers, M., GuisadoPintado, E., Wiles, E., Benallack K., Balme, M. 2020. Reversing transverse dunes: modelling of airflow switching using 3D Computational Fluid Dynamics. Earth and Planetary Science Letters, 544, 116363.
Richardson, M. I., Toigo, A. D., & Newman, C. E. 2007. PlanetWRF: A general purpose, local to global numerical model for planetary atmospheric and climate dynamics. Journal of Geophysical Research, Planets, 112, E09001
Submission deadline
Friday 5 February 2021
12:00AM
Interview Date
Week Commencing 22 March 2021
Preferred student start date
Mid-September 2021
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