Coupling of small- and large-scale filament eruptions

来源 :天文和天体物理学研究:英文版 | 被引量 : 0次 | 上传用户:wlfzjut
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
We present observations of the eruption of a large-scale quiescent filament(LF) that is associated with the formation and eruption of a miniature filament(MF). As a result of convergence and subsequent cancelation of opposite-polarity magnetic flux, MF wa
其他文献
This is a memorial report on the biography and scientific heritage of M.A.Svechnikov-an outstanding scientist and teacher,the founder of the Ural school of clos
The Plastic Scintillator Detector(PSD) onboard the DArk Matter Particle Explorer(DAMPE)is designed to measure cosmic ray charge(Z) and to act as a veto detector
The first generation solar adaptive optics(AO) system, which consists of a fine tracking loop with a tip-tilt mirror(TTM) and a correlation tracker, and a high-
Blazars are characterized by large intensity and spectral variations across the electromagnetic spectrum It is believed that jets emerging from them are almost
期刊
We performed a multiwavelength study towards the infrared dark cloud(IRDC) G31.23+0.05 with new CO observations from Purple Mountain Observatory and archival da
The neutrino burst detected during supernova SN 1987A is explained in a strangeon star model, in which it is proposed that a pulsar-like compact object is compo
预定数组工程的脉冲星的主要目标是检测极端低频率的重力的波浪。脉冲星数据集合被众多的噪音过程包括在星际的媒介并且从太阳的风改变散延期影响。太阳的风能导致用存在望远
有大数组(VLA ) 的成像研究揭示了嗨与扩大 circumstellar 联系的排放红轰炸巨人。我们分析光谱在 Y CVn 上获得的地图, Asymptotic 巨人上的一颗 J 类型碳星分叉。HI 线侧面