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Global magnetic fields in planets, in the Sun and other stars, in spiral galaxies and galaxy clusters are believed to be generated and maintained by a hydromagnetic dynamo, a process that converts turbulent kinetic energy into magnetic energy. These dynamo processes operate on drastically different scales, but are associated with common physical mechanisms, involving a complex interaction of rotation, turbulence and instabilities. The goal of IAU Symposium 294 was to discuss the most important results of recent studies of ...

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Solar and Astrophysical Dynamos and Magnetic Activity (IAU S294) 2013, Cambridge University Press, Cambridge

ISBN-13: 9781107033832

Hardcover