3D Views on Cool Stellar Atmospheres3D Views on Cool Stellar AtmospheresTheory meets observationTheory meets observation

Three-dimensional, time-dependent radiation-magneto-hydrodynamic simulations constitute a rapidly evolving branch in the field of modeling cool stellar atmospheres.

This meeting will bring together observers and theoreticians to discuss the perspectives for applications and future developments of 3D stellar atmospheres.

Scientific Organizing Committee: Carlos Allende Prieto (UK), Martin Asplund (Germany), Mats Carlsson (Norway), Márcio Catelan (Chile), Kwing Lam Chan (China), Dainis Dravins (Sweden), Hans-G. Ludwig (France, chair), K.N. Nagendra (India),

Åke Nordlund (Denmark), Natalia Shchukina (Ukraine), T. Sivarani (USA), Matthias Steffen (Germany)

Joint Discussion 10, IAU General Assembly, Rio de Janeiro, August 10-11, 2009

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