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.
Details are available at https://www.imperial.ac.uk/jobs/search-jobs/description/index.php?jobId=24943&jobTitle=Research+Associate+in+space+plasma+physics
The closing date for applications is 22 August 2025. If you have questions, please contact Tim Horbury, t.horbury@imperial.ac.uk