NASA’s Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) was launched 10 years ago on 5 Feb 2002. Its unprecedented view of the high energy X-ray and γ-ray emission from solar flares has provided many insights into these explosive phenomena. The Glasgow A&A group are heavily involved with analysing and interpreting the data from RHESSI, with these results recently reviewed by group members in the RHESSI monograph.
- Dr. Ryan Milligan stars in his own space TV show [06-Dec-2017]
- Award from China arrived to Hamish Reid and Heather Ratcliffe [13-Nov-2017]
- Congratulations to Dr Motorina [01-Nov-2017]
- Nicolina Chrysaphi made intriguing solar observations operating UK LOFAR [17-Oct-2017]
- Visiting Professor Gordon Emslie explains to Physics Central the role of turbulence in solar flares [21-Sep-2017]