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Transverse Oscillation of a Filament Triggered by an Extreme Ultraviolet Wave
Xue ZK(薛志科); Yan XL(闫晓理); Qu ZQ(屈中权); Zhao L(赵丽)
2014-10
会议名称7th Solar Polarization Workshop (SPW7)
会议日期2013-09-09
会议地点Kunming, PEOPLES R CHINA
卷号489
页码53-58
通讯作者Xue, ZK (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming, Yunnan, Peoples R China.
英文摘要We analyze a case of transverse oscillation of a filament triggered by an extreme ultraviolet (EUV) wave on 2011 September 7 observed by the Atmospheric Imaging Assembly (AIA) and the Helioseismic and Magnetic Imager (HMI) aboard the Solar Dynamics Observatory (SDO). The EUV wave first appeared at 22:35 UT after a filament (F1) eruption in the NOAA active region 11283 and then propagated toward the northwest with a speed of 690 km s-1. When the EUV wave propagated through another filament (F2), it caused F2 to oscillate transversely. The oscillation period and damping time are calculated by a damped cosine function, and they are around 1140 s and 5920 s respectively. Based on coronal seismology, we estimate the average values of magnetic fields inside and outside the oscillating filament, about 17.6 G and 7.4 G respectively. 
收录类别CPCI
产权排序第一完成单位
会议网址http://aspbooks.org/custom/publications/paper/489-0053.html
会议录Astronomical Society of the Pacific (ASP) Conference Series - SOLAR POLARIZATION 7
会议录出版者Astronomical Society of the Pacific
会议录出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
学科主题Astronomy & Astrophysics
语种英语
ISBN号978-1-58381-863-3; 978-1-58381-862-6
WOS记录号WOS:000370308600004
内容类型会议论文
源URL[http://ir.ynao.ac.cn/handle/114a53/9659]  
专题云南天文台_抚仙湖太阳观测站
作者单位Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, China
推荐引用方式
GB/T 7714
Xue ZK,Yan XL,Qu ZQ,et al. Transverse Oscillation of a Filament Triggered by an Extreme Ultraviolet Wave[C]. 见:7th Solar Polarization Workshop (SPW7). Kunming, PEOPLES R CHINA. 2013-09-09.http://aspbooks.org/custom/publications/paper/489-0053.html.
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