Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator I. Magnetic Rayleigh-Taylor Instability at the Top of Emerging Flux as the Origin of Filamentary Structure
Three-Dimensional Simulation of Solar Emerging Flux Using the Earth Simulator I. Magnetic Rayleigh-Taylor Instability at the Top of Emerging Flux as the Origin of Filamentary Structure
复制标题
地球模拟器对太阳新兴通量的三维模拟 一、新兴通量顶部磁瑞利-泰勒不稳定性作为丝状结构的起源
DOI：
--
复制
发表时间：
2006
期刊：
影响因子：
--
通讯作者：
T.
中科院分区：
文献类型：
--
作者：
Isobe;H.;Miyagoshi;T.;Shibata K.;Yokoyama;T.
