Dan Naylor

PhD student

Research Overview

Soft X-rays are generated within planetary magnetosheaths due to the interaction between magnetospheric neutrals and highly charged solar wind ions. Imaging of these soft X-rays is an emerging technology that can allow for a dynamic, global diagnostic view of the magnetosheath region to be built and exploration of the solar wind driving of planetary magnetospheres. I am modelling the magnetosheath of Uranus, a highly complex and interesting system, to investigate soft X-ray emission from the region and ultimately aim to test the viability of sending an SXI along with the planned flagship mission to the Uranian system.

Can We Detect Soft X-Ray Emission from Uranus's Magnetosheath?
Oral presentation

FST Celebration of Science
Participation in conference - Academic

Autumn MIST (Birmingham 2024)
Participation in conference - Academic

STFC Introductory Course in Solar and Solar-Terrestrial Physics 2024
Participation in workshop, seminar, course

Charge Exchange X-Ray Universe 2024
Participation in conference - Academic

  • Space and Planetary Physics