The IAU Symposium 410 New Look at Solar and Stellar Coronae will address some of the most pressing open questions in coronal physics, capitalising on the rapid expansion of high-resolution solar and stellar observations and the growing synergy between the solar and stellar research communities.
Scheduled for 29 November – 4 December 2026 (please note the change of dates) in Shenzhen, China, the symposium coincides with the arrival of major new facilities and missions, as well as significant theoretical advances, making it an ideal moment to reassess the fundamental physical processes operating across the Sun and cool stars.
The scientific programme spans impulsive phenomena, including solar and stellar flares and CMEs, coronal heating and winds, solar and stellar radio physics, coronal seismology, atmospheric connectivity, and novel approaches to data analysis and diagnostics, laying the groundwork for effective exploitation of the solar–stellar analogy.
Registration is now open via the IAUS410 website: https://www.shenzhen-astronomy.org.cn/iaus410