Observational Features of Large-Scale Structures as Revealed by the Catastrophe Model of Solar Erupt

• 作 者: Jun Lin
• 机 构: NationalAstronomicalObservatories/YunnanObservatory,Harvard-SmithsonianCenterforAstrophysics
• 出 处: 中国天文和天体物理学报：英文版
• 发表日期: 2007年4期
• 关键词: 太阳系 太阳活动 磁场 内部结构 Sun： large-scale magnetic structures - Sun： eruptive processes
• 基金项目: Supported by the National Natural Science Foundation of China.Acknowledgements This work was supported by the Ministry of Science and Technology of China under the 973 Program grant 2006CB806303, and

Large-scale magnetic structures are the main carrier of major eruptions in the solar atmosphere. These structures are rooted in the photosphere and are driven by the unceas-ing motion of the photospheric material through a series of equilibrium configurat