Qualification Type: | PhD |
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Location: | Reading |
Funding for: | UK Students, EU Students, International Students |
Funding amount: | £19,237 - please see advert |
Hours: | Full Time |
Placed On: | 13th March 2024 |
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Closes: | 17th April 2024 |
Supervisors: Prof Mathew Owens and Dr. Luke Barnard
Project overview: The solar wind is a continuous outflow of charged particles and magnetic field from the Sun’s upper atmosphere. Variability in the solar wind conditions leads to space weather, which can adversely affect technological infrastructures, such as power grids and telecommunications networks, as well as the health of humans in space and on high-altitude flights.
The most severe space weather is driven by coronal mass ejections (CMEs) which propagate through the solar wind to reach Earth. The physics and dynamics of CMEs between the Sun and Earth are still poorly understood, mainly due to limited observations of any one event. This project will combine observations and models to determine the importance of different physical processes.
Informal enquiries to Prof. Mathew Owens
Eligibility:
This project would be suitable for students with at least a 2:1 degree in physics, mathematics or a closely related environmental or physical science. Experience with the python programming language would be advantageous, but not essential.
Funding details:
How to apply:
To apply click Apply for a Programme and create your account, and use the link sent by email to start the application process. During the application process please select the PhD in space physics, Department of Meteorology
*Important notes*
Application deadline: 17th April 2024
Further enquiries: Mathew Owens
Please note that, where a candidate is successful in being awarded funding, this will be confirmed via a formal studentship award letter; this will be provided separately from any Offer of Admission and will be subject to standard checks for eligibility and other criteria.
For further details please contact m.j.owens@reading.ac.uk
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