https://www.asiaoceania.org/aogs2022/public.asp?page=submit_abstracts.asp

Small-scale eruptions are ubiquitous on the Sun. Based on their different sizes, dominant temperatures, and wavelengths they are observed, they have been given different names including spicules, macro-spicules, micro-jets, jets, bright-points, camp-fire etc.. These small-scale eruptions have often been found to be accompanied or associated with different solar magnetic field phenomena.

Since the first modern observations of these small-scale eruptions in the solar atmosphere, the understanding of those eruptions has been many advanced. Thanks for the development of MHD and plasma-astrophysics theories, the improvement of computational powers, and the realization of a number of state-of-the-arts observational facilities with high spatial and spectral resolution and temporal cadence.

We welcome presentations about small-scale eruptions. We encourage contributions to a variety of research methodologies, including the application of techniques drawn from other disciplines. We hope to see submissions ranging from observations and theory to numerical, statistical, and machine learning modelling, in order to foster collaborations across communities.