Abstract
Yohkoh observed many dynamic phenomena in the solar corona, such as flares, microflares, plasma ejections, and jets. These phenomena can be explained by a magnetic reconnection model. This paper is a review of the results of our magnetohydrodynamic (MHD) simulations of magnetic reconnection in the solar corona and flares.
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Yokoyama, T. (1998). MHD Simulations of Magnetic Reconnection in the Solar Corona and Flares. In: Watanabe, T., Kosugi, T., Sterling, A.C. (eds) Observational Plasma Astrophysics: Five Years of Yohkoh and Beyond. Astrophysics and Space Science Library, vol 229. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5220-4_26
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DOI: https://doi.org/10.1007/978-94-011-5220-4_26
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6198-8
Online ISBN: 978-94-011-5220-4
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