太阳爆发的能量积累机制研究
序号 | 标题 | 类型 | 作者 |
---|---|---|---|
1 | WHY DOES THE APPARENT MASS OF A CORONAL MASS EJECTION INCREASE? | 期刊论文 | Chenglong Shen|Bernd Inhester|Lei Lu|Weiqun Gan| |
2 | HOOKED FLARE RIBBONS AND FLUX-ROPE-RELATED QSL FOOTPRINTS | 期刊论文 | Guillaume Aulanier|Brigitte Schmieder|Etienne Pariat|Hui Li| |
3 | The Lyman-α Solar Telescope (LST) for the ASO-S Mission | 期刊论文 | Hui Li| |
4 | Observational Evidence of Magnetic Reconnection for Brightenings and Transition Region Arcades in IRIS observations | 期刊论文 | Etienne Pariat|Xioashuai Zhu|Li Feng|Michalina Grubecka| |
5 | Study of a solar flare on 2005 August 22 observed in hard X-rays and microwaves | 期刊论文 | Zhong-Yin Liu|You-Ping Li|Wei-Qun Gan|Kazi A Firoz| |
6 | RADIAL FLOW PATTERN OF A SLOW CORONAL MASS EJECTION | 期刊论文 | Li Feng|Bernd Inhester|Weiqun Gan| |
7 | TEMPORAL EVOLUTION OF THE MAGNETIC TOPOLOGY OF THE NOAA ACTIVE REGION 11158 | 期刊论文 | Etienne Pariat|Brigitte Schmieder|Yang Guo|Thomas Wiegelmman| |