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 First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, India, August 27 - September 7, 2007 Astrophysics and Space Science Proceedings

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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes
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Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes - First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, India, August 27 - September 7, 2007
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It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops , jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time
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