Research Fellow in Solar Physics (2 vacancies) – Northumbria University, UK

June 10, 2020, from Richard Morton

Applications are invited for two separate four-year (53 month) postdoctoral research fellow positions in the area of Solar Physics; to be hosted at Northumbria University, UK.

The successful candidates will conduct research relevant to understanding how Alfvénic waves transfer energy through the Sun’s atmosphere, with a particular focus on the corona and the connection with the solar wind. These positions are funded by a Future Leader grant from UKRI (the RiPSAW project, MR/T019891/1) and you will work primarily with Dr Richard Morton (PI). RiPSAW focuses on both the observation of the Alfvénic waves and modelling of their turbulent cascade. You will initiate, develop and conduct high-quality research in support of the project. Research fellow positions are expected to begin on the 1st October 2020

The first of the available positions will be related to the analysis of EUV data from the Solar Dynamics Observatory and infrared data from the Coronal Multi-Channel Polarimeter, along with data coming from DKIST, PSP and SolO. The position will require experience with data from remote sensing instrumentation, and a good knowledge of standard methodology required for typical data analysis tasks. The ideal candidate will also have a good knowledge of statistical data analysis, with some experience in the analysis of MHD waves and/or machine learning. Competence in IDL, Python or R is essential. Experience in numerical modelling of MHD waves would also be beneficial but not essential. This aspect of the project will involve working closely with collaborators at HAO, NCAR and include the opportunity for extended visits.

The second of the available positions will be related to the analysis of infrared data from the Coronal Multi-Channel Polarimeter and DKIST, along with numerical and forward modelling of MHD waves in the corona. The position will require experience with data analysis and/or numerical simulations of MHD waves. The ideal candidate will have experience in both of these domains, with knowledge of either MHD wave simulations or Alfvénic Turbulence modelling. A working knowledge of IDL, Python or R is also desirable. This aspect of the project will involve working closely with collaborators at Smithsonian Center for Astrophysics, Harvard, and include the opportunity for extended visits.

The two positions offer the opportunity for regular travel to international conferences and collaborators. There will also be a strong focus on the professional and personal development of the appointed staff, with substantial resources available for training of the successful candidates (including attending workshops, courses, etc).

Both fellows would also be expected to contribute to the general development of the research group, supporting each other’s research and mentoring PhD, Masters, undergraduate and summer students. The positions also require engagement with the project’s public outreach and communication activities.

For informal enquiries about this post please contact Dr Richard Morton, UKRI Future Leader Fellow, at richard.morton@northumbria.ac.uk .

Further details on how to apply are available here: https://www.northumbria.ac.uk/work-for-us/job-vacancies/academic-3188-research-fellow-in-solar-physics

Deadline for applications is the 5th July 2020.


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