Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pasj...55l..35s&link_type=abstract
Publications of the Astronomical Society of Japan, Vol.55, No.3, pp. L35-L39
Astronomy and Astrophysics
Astronomy
7
Conduction, Mhd, Shock Waves, Sun: Corona
Scientific paper
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.
Chen Peng-Fei
Isobe Hiroaki
Sakajiri Takuma
Shibata Kazunari
Shiota Daikou
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