今年AGU中关于 三维湍流磁重联 为数不多的几个报告(Oral+Poster, observation+simulation)之一。 Application of HPIC-LBM in large temporal-spatial scale 3D turbulent magnetic reconnection Eposter 下载链接： https://agu.confex.com/agu/fm18/meetingapp.cgi/Paper/393523
计算太阳物理(2.5D/3D大时空尺度湍流磁重联)中用到的等离子体温度、热松弛时间等等.......基本参数，下面两本书介绍的比较准确。 Physics of the Solar Corona and Transition Region: Proceedings of the Monterey Workshop 全文链接：https://pan.cstcloud.cn/s/4b7CV5PaQt8 Physics of the Solar Corona and ...
During the smallest bubble coalesce with each other and form bigger plasmoid bubble process, the new magnetic reconnection will happen around the adjacent bubble collision and coalescence process in vertical direction. AVI Formate file: http://ddl.escience.cn/f/y91h AVI Format ...
一篇写的非常详细的综述文章，值得认真读几遍！PDF下载地址：http://ddl.escience.cn/f/yHs0 详细介绍了从large-global-scale to small-local scale 过程中 MHD, Test particle, PIC方法各自的特点、优势及局限性，只可惜没涉及LBM。 Recent Advances in Understanding Particle Acceleration Process in Solar Fl ...
What behind in the fractal current sheet region? 磁湍流精细拓扑结构演化不仅是随尺度降低拓扑结构满足分形规律这样简单——电流片主x点附近，等离子体运动将不再稳定流动。 e.g 扰动-湍流发育-湍流充分过程算例 1. Gif format file for macro-global scale turbulent magnetic topological structure evolut ...
三流体磁重联模型-云图(contour)磁力线(streamtrace line)磁力线值(Follow) Original Figure: http://ddl.escience.cn/f/yso9 Gif format file http://ddl.escience.cn/f/ysoT Gif format file http://ddl.escience.cn/f/ysoV Gif format file http://ddl.escience ...
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