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| Les deux révisions précédentesRévision précédenteProchaine révision | Révision précédente | ||
| animation:workshops:2013:plasma [2013/04/19 12:06] – [Shocks, Reconnection, and Particle Acceleration in Plasma-fluids] sbarends | animation:workshops:2013:plasma [2013/04/26 13:52] (Version actuelle) – [Shocks, Reconnection, and Particle Acceleration in Plasma-fluids] sbarends | ||
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| - | Location: Salle de réunion LR6 C 023, Centre Blaise Pascal, ENS-Lyon, France | + | Centre Blaise Pascal, ENS-Lyon, France |
| - | June 20-21, 2013 \\ | + | June 20-21, 2013 \\ |
| [[http:// | [[http:// | ||
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| Organizing committee: | Organizing committee: | ||
| * **Rolf Walder**, CRAL, École normale supérieure de Lyon | * **Rolf Walder**, CRAL, École normale supérieure de Lyon | ||
| - | * **Christophe Winisdoerffer**, | + | |
| + | * **Andrei Bykov**, Ioffe Institute, Russian Academy of Sciences, St. Petersburg, Russia | ||
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| + | * **Mickaël Melzani**, CRAL, École normale supérieure de Lyon, France | ||
| Administrative coordination: | Administrative coordination: | ||
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| The workshop is supported by: | The workshop is supported by: | ||
| - | * Centre Blaise Pascal | + | * **CBP** - Centre Blaise Pascal, Lyon, France |
| - | * FLMSN | + | |
| - | * CRAL | + | |
| + | * **ENSL** - École normale supérieure de Lyon | ||
| + | * **Université de Lyon** | ||
| + | * **CNRS** - Centre National de la Recherche Scientifique | ||
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| + | ===== Summary ===== | ||
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| + | The acceleration of non-thermal particles in large scale flows is of prime importance in astrophysics and beyond. Cosmic accelerators can energize particles up to 10²⁰ eV. The flux of high-energy cosmic rays has a strong impact on Earth, on its climate and weather. | ||
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| + | However, accelerators embedded in large scale MHD flows within astrophysical objects still remain enigmatic in various ways. The aim of the workshop is to bring together people of different communities and approaches: modelers of large scale flows, scientists scrutinizing fundamental processes, people who are deriving observable signatures, and numerical specialists. We also aim at bringing together the French with the European community and strengthen the collaboration between them, specially emphasizing the Rhône-Alpes region. | ||
| - | ===== Program ===== | + | The first day concentrates on theoretical questions of plasma physics, particle acceleration, |
| - | The acceleration | + | The second day presents results |