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Stellar physics itself is benefiting greatly from solar discoveries, but, in tum, our understanding of many solar phenomena (such as sunspots, sunspot cycles, the corona and the solar wind) will undoubtedly increase in the future due to their observation under different conditions in other stars.
In three lectures on magnetohydrodynamics, on kinetic plasma physics and on particle acceleration, leading experts describe the physical basis of their subjects and extend the discussion to several applications in modern problems of astrophysics.
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