›IAU Symposium 327: Fine Structure and Dynamics of the Solar Atmosphere
The scientific goal of this symposium is to discuss recent results on the processes shaping the structure of the solar atmosphere and driving plasma eruptions and explosive events. Activity of the solar atmosphere entails numerous multi-scale processes. State-of-the-art solar instrumentation is revealing the dynamics of the Sun with unprecedented temporal and spatial resolutions. Together with advanced numerical simulations these investigations are making new steps in our understanding of the complex dynamical structure of the solar atmosphere.
The understanding of the fine structure and dynamics of the solar atmosphere requires a considerable coordinated effort of observers, theorists and experts in realistic numerical simulations. The proposed symposium is very timely and important. It will make an important step in the big international effort for our understanding of the solar atmosphere with large telescopes and detailed modelling. The Symposium will provide a forum for discussion of the recent advances, and a platform for developing new coordinated observing and theoretical programs. This Symposium will be of great interest also for the IAU Divisions studying stellar atmospheres, starspots, exoplanetary systems, and developing advanced observational techniques and theoretical models.
We are looking forward to seeing you in Cartagena de Indias!
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