Abstract
The physics of flares on the Sun now becomes ‘an étalon’ for contemporary astrophysics, in particular for gamma and X-ray astronomy. In contrast to flares on other stars and to many analogous phenomena in the Universe, solar flares are accessible to a broad variety of observational methods to see and investigate the magnetic reconnection process in high-temperature strongly-magnetized plasma of the corona as well as in low-temperature weakly-ionized plasma in the photosphere.
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© 2006 Springer Science+Business Media, LLC
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(2006). Evidence of Reconnection in Solar Flares. In: Plasma Astrophysics. Astrophysics and Space Science Library, vol 341. Springer, New York, NY. https://doi.org/10.1007/978-0-387-68894-7_25
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DOI: https://doi.org/10.1007/978-0-387-68894-7_25
Publisher Name: Springer, New York, NY
Print ISBN: 978-0-387-34948-0
Online ISBN: 978-0-387-68894-7
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