2024年5月30日(木) 10:15 〜 10:30 201B (幕張メッセ国際会議場)

Solar Cycle 25 is steadily increasing its activity and is expected to reach maximum within the next few years. While the cutting-edge observations are being produced by ground-based observatories such as DKIST, a new space-borne solar observing network is also being established, including the Solar Orbiter and Parker Solar Probe explorers, as well as the recently launched CHASE, ASO-S, and Adytia-L1 missions. Progress is also being made in state-of-the-art numerical modeling that is essential for disentangling the complex observables and for gaining fresh insights into the highly dynamic nature of solar magnetism and dynamics. To share and discuss recent advancements in solar physics and related fields, we invite contributions from solar researchers, and also from researchers in heliospheric, planetary, and stellar physics, covering results from their latest observation, numerical modeling, and experimental investigations.