期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
卷 55, 期 3, 页码 L35-L39出版社
OXFORD UNIV PRESS
DOI: 10.1093/pasj/55.3.L35
关键词
conduction; MHD; shock waves; Sun; corona
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 cot-respond to the slow and fast shocks associated with the magnetic reconnection.
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