About the role
As a research associate in space plasma physics in the Physics Department you will work on data from the Solar Orbiter and Parker Solar Probe missions, studying the global evolution of the Sun's magnetic field and large scale structure of the solar wind through the solar cycle. You will also have the chance to work on data from IMAP and other spacecraft at L1 to investigate the 3D structure of the solar wind and its effect on space weather at the Earth.
What you would be doing
You will be analysing spacecraft data, including measurements from the magnetic field instruments on Solar Orbiter and IMAP which were built at Imperial. The particular focus of this work is on using the novel out of ecliptic orbit of Solar Orbiter to characterise the global structure of the heliospheric magnetic field and link this to the evolution of the Sun's internal field as it evolves from solar maximum to minimum over the next few years. Combined with other measurements such as those from Parker Solar Probe, you will also study the spatial and temporal evolution of flows from coronal holes and other solar regions. With the launch of IMAP later in 2025, there is also the opportunity to work with multi-point data from L1, where you will investigate which methods are most useful in determining the 3D field structure, building on work done with Cluster and MMS data. This work has direct application for real-time space weather forecasting as well as the study of plasma dynamics and turbulence.
What we are looking for
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