Numerical MHD simulations of post-flare loop formation on the sun: Allowing for thermal-conductivity anisotropy
作者： A. I. Podgorny , I. M. Podgorny
DOI: 10.1134/1.1436206
关键词: Magnetic field 、 Plasma 、 Anisotropy 、 Loop (topology) 、 Flare 、 Classical mechanics 、 Physics 、 Mechanics 、 Magnetohydrodynamics 、 Flux tube 、 Thermal conductivity
摘要: The process of post-flare loop formation, including the heating flux tubes by hot chromospheric sources and their filling with plasma, is demonstrated simulations in an MHD approximation. additionally heated at its apex interaction oppositely directed plasma streams. Local coronal over also possible due to magnetic-field-line reconnection. A new version PERESVET code that can take into account anisotropy thermal conductivity a magnetic field was used for computations.
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