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Elsevier, Advances in Space Research, 3(26), p. 511-520

DOI: 10.1016/s0273-1177(99)01081-9

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MHD simulations of magnetic reconnection in solar flares and jets

Journal article published in 2000 by T. Yokoyama ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

Yohkoh observed many dynamic phenomena in the solar corona, such as flares, microflares, plasma ejections, and jets. These can be explained by the magnetic reconnection model. The review summarizes some results obtained from our magnetohydrodynamic (MHD) simulations of the microflares triggered by emerging flux (Shibata et al. 1992), X-ray jets (Yokoyama and Shibata 1995), plasma ejections (Magara et al. 1996), and solar flares (Yokoyama and Shibata 1998) based on the magnetic reconnection models.