Fragmented Energy Release in Sun and Stars
The Interface between MHD and Plasma Physics
Samenvatting
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 gamma-ray emission often directly results from magnetic `flares',  implying that these processes are spatially fragmented and of an  impulsive nature. A true understanding of these processes requires a  combined magnetohydrodynamical and plasma physical approach.  Fragmented Energy Release in Sun and Stars: the Interface  between MHD and Plasma Physics provides a comprehensive,  interdisciplinary summary of magnetic energy release in the Sun and  stars, in accretion disks, in pulsar magnetospheres and in laboratory  plasmas. These proceedings include papers on both theoretical and  observational aspects. 
  Fragmented Energy Release in Sun and Stars: the Interface between  MHD and Plasma Physics is for researchers in the fields of  solar physics, stellar astrophysics and (laboratory) plasma physics  and is a useful resource book for graduate level astrophysics courses.
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