Abstract
We performed magnetohydrodynamic (MHD) simulations of a giant arcade formation with a model of magnetic reconnection coupled with heat conduction, to investigate the dynamical structure of slow and fast MHD shocks associated with reconnection. Based on the numerical results, theoretical soft X-ray images were calculated and compared with the Yohkoh soft X-ray observations of a giant arcade on 1992 January 24. The Y-shaped structure observed in the event was identified to correspond to the slow and fast shocks associated with the magnetic reconnection.
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CITATION STYLE
Shiota, D., Yamamoto, T. T., Sakajiri, T., Isobe, H., Chen, P. F., & Shibata, K. (2003). Slow and fast MHD shocks associated with a giant cusp-shaped arcade on 1992 January 24. Publications of the Astronomical Society of Japan, 55(3). https://doi.org/10.1093/pasj/55.3.L35
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