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DynaSun: Dynamics of the solar corona in the era of data intensive observations

The solar atmosphere is a dynamic system with phenomena including solar flares, coronal mass ejections, magnetohydrodynamic (MHD) waves, plasma oscillations and time-dependent heating. In Solar Physics, we are now living in the era of data intensive observations and so, with the right techniques and understanding, we can start to address fundamental questions around the physical scenarios of energy releases and plasma heating.

The European Commission has recognised this challenge (and scientific opportunity) and so has created the DynaSun Network: Dynamics of the solar corona in the era of data intensive observations. This international network discusses key challenges in solar physics, including understanding of mechanisms for plasma heating, and energetics and physical scenarios of energy releases such as flares and coronal mass ejections. 

Scientific Organising Committee:

• Regina Aznar Cuadrado  (Max Planck Institute, Germany)

• Miroslav Bárta (Astronomical Institute, Academy of Sciences, Czech Republic)

• Mariana Cécere (National Scientific & Technical Research Council of Argentina)

• Andrea Costa (National Scientific & Technical Research Council of Argentina)

• Hebe Cremades (National Scientific & Technical Research Council of Argentina)

• Petr Jelínek (University of South Bohemia, Czech Republic)

• James McLaughlin (Northumbria University, UK)

• Valery Nakariakov (Warwick University, UK)

• Tom Van Doorsselaere (KU Leuven, Belgium)

• Santiago Vargas Dominguez (National University of Colombia)

• Astrid Veronig (University of Graz, Austria)

Registration & Abstract Submission