I would like to draw your attention to an AGU Fall Meeting (15-19 Dec 2025) session relevant to high-energy solar physics. While the meeting is still six months away, the abstracts are due 30th July 2025. Hope to see you in New Orleans!
SH028. Solar Flares in the High-Resolution, High-Cadence Era: Observations, Modelling and Future Prospects
“Solar flares are fundamentally multi-scale phenomena that result from the dramatic and dynamic evolution of the Sun’s atmosphere and magnetic field, from photosphere through corona. Flares are now being observed with unprecedented spatial resolution at very high cadence, and sometimes from multiple viewpoints, providing remarkable new insights into flare energetics and evolution. Recent exciting observations include those from Solar Orbiter’s coordinated major flare campaigns, from IRIS’ high-cadence campaigns, and from ground-based observatories such as DKIST, SST and BBSO. These observations are challenging longstanding views of the flare energy release, transport and dissipation process, and have further revealed the significant sub-structure appearing within flare sources. Equal advancements in flare modeling are required to interpret the observations, and to demonstrate what future observations are required. We seek abstracts covering fine-scale flare structures, rapid temporal evolution, and future prospects for flare-optimized observations. Observational, modeling, instrumentation, and theoretical studies are all applicable and welcomed.”
Best,
Graham Kerr, Andrew Inglis, Gianna Cauzzi and Hannah Collier