Fragmented energy release in Sun and stars. The interface between MHD and plasma physics. Proceedings. Workshop on the occasion of the 350th anniversary of the Astronomical Institute Utrecht, Utrecht (Netherlands), 18 - 21 Oct 1993.

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Magnetohydrodynamics: Sun, Accretion Disks: Stars, Accretion Disks: Black Holes, Accretion Disks: Pulsar Magnetospheres

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Magnetic energy release plays an important role in a wide variety of cosmic objects such as the Sun, stellar coronae, stellar and galactic accretion disks and pulsars. The observed radio, X-ray and γ-ray emission often directly results from magnetic 'flares', implying that these processes are spatially fragmented and of an impulsive nature. These proceedings provide a comprehensive, interdisciplinary summary of magnetic energy release in the Sun and stars, in accretion disks, in pulsar magnetospheres and in laboratory plasmas. Included are papers on both theoretical and observational aspects.

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