Alan Hood

Alan Hood is a Professor in Applied Mathematics at the School of Mathematics and Statistics, University of St Andrews, UK. He holds a Ph.D. and B.Sc. from the same institution and is a leading researcher in solar physics and magnetohydrodynamics (MHD). His work focuses on the stability and energy release mechanisms in solar coronal loops, employing advanced numerical modeling techniques.

• Education: Ph.D., University of St Andrews; B.Sc., University of St Andrews
• Professional Affiliation: Fellow of the Royal Society of Edinburgh (2004)

Alan Hood's research centers on solar physics, particularly the modeling of solar phenomena using magnetohydrodynamics. His work investigates how magnetic fields in the solar atmosphere become unstable and release energy through processes like nanoflares and MHD avalanches. He explores the coupling of magnetic and thermal effects, including thermal conduction and radiation, to understand the dynamics of coronal heating. His research has direct implications for space weather and solar flare prediction.

Recent publications highlight his focus on multi-threaded coronal loops, MHD avalanches, and the thermodynamic response of heating at magnetic null points. His work combines 3D numerical simulations with observational modeling, especially in extreme ultraviolet (EUV) spectroscopy, to predict signatures detectable by missions like MUSE. The research outputs consistently emphasize MHD instabilities, energy dissipation, and fine-scale plasma structures.

Scientific Awards and Recognition:

• Fellow of the Royal Society of Edinburgh (2004)
• Group Achievement Award for Geophysics (2013, 2015)
• Head of School, School of Mathematics and Statistics, University of St Andrews (2004)
• Lord Kelvin Medal (2020)

Hood is actively involved in the academic community through research grants, supervision, and editorial roles. He has served as an external examiner for PhD theses at multiple institutions, including Manchester University, UCL, and City University London. He has also chaired scientific conferences such as the UKMHD/BAMC in 2018. His leadership extends to directing major research projects funded by the Science & Technology Facilities Council and the European Research Council, including the WholeSun ERC Synergy Project.

He leads the Solar and Magnetospheric MHD Theory Group, which develops theoretical models to explain solar and space plasma phenomena. The group produces open-access datasets and software, supporting reproducibility and collaboration in solar physics research.