Zobrazeno 1 - 10
of 162
pro vyhledávání: '"Su, Yingna"'
Autor:
Xue, Jianchao, Feng, Li, Li, Hui, Zhang, Ping, Chen, Jun, Shi, Guanglu, Ji, Kaifan, Qiu, Ye, Li, Chuan, Lu, Lei, Ying, Beili, Li, Ying, Huang, Yu, Li, Youping, Li, Jingwei, Zhao, Jie, Song, Dechao, Li, Shuting, Tian, Zhengyuan, Su, Yingna, Zhang, Qingmin, Ge, Yunyi, Shan, Jiahui, Li, Qiao, Li, Gen, Zhou, Yue, Tian, Jun, Liu, Xiaofeng, Jing, Zhichen, Chen, Bo, Song, Kefei, He, Lingping, Lei, Shijun, Gan, Weiqun
Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here we present two failed prominence eruptions on 26 October 2022 and explore their connections. Using stereos
Externí odkaz:
http://arxiv.org/abs/2406.11602
Autor:
Teng, Weilin, Su, Yingna, Liu, Rui, Chen, Jialin, Liu, Yanjie, Dai, Jun, Cao, Wenda, Shen, Jinhua, Ji, Haisheng
Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by
Externí odkaz:
http://arxiv.org/abs/2405.17303
Autor:
Li, Qiao, Li, Ying, Su, Yang, Song, Dechao, Li, Hui, Feng, Li, Huang, Yu, Li, Youping, Li, Jingwei, Zhao, Jie, Lu, Lei, Ying, Beili, Xue, Jianchao, Zhang, Ping, Tian, Jun, Liu, Xiaofeng, Li, Gen, Jing, Zhichen, Li, Shuting, Shi, Guanglu, Tian, Zhengyuan, Chen, Wei, Su, Yingna, Zhang, Qingmin, Li, Dong, Ge, Yunyi, Shan, Jiahui, Zhou, Yue, Lei, Shijun, Gan, Weiqun
Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (say X- and M-class flares). Here we report a small C2.3 white-light flare (SOL2022-12-20T04:10) observed by the \emph{Advanced Spac
Externí odkaz:
http://arxiv.org/abs/2405.01308
Autor:
Hashim, Parida, Xu, Fangyu, Wang, Ya, Men, Weijie, Shen, Jinhua, Su, Yingna, Li, Jianping, Jin, Zhenyu, Ji, Haisheng
In this paper, with a set of high-resolution He I 10830 \AA\ filtergrams, we select an area in a plage, very likely an EUV moss area, as an interface layer to follow the clues of coronal heating channels down to the photosphere. The filtergrams are o
Externí odkaz:
http://arxiv.org/abs/2402.18077
Autor:
Dai, Jun, Zhang, Qingmin, Qiu, Ye, Li, Chuan, Li, Zhentong, Li, Shuting, Su, Yingna, Ji, Haisheng
In this paper, we present the imaging and spectroscopic observations of the simultaneous horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an EUV wave on 2022 October 02. Particularly, the filament oscillation i
Externí odkaz:
http://arxiv.org/abs/2310.19228
We investigate the formation and eruption of hot channels associated with the M6.5 class flare (SOL2015-06-22T18:23) occurring in NOAA AR 12371 on 2015 June 22. Two flare precursors are observed before the flare main phase. Observations in 94 {\AA} a
Externí odkaz:
http://arxiv.org/abs/2211.06060
The separation of a filament and sigmoid is observed during an X1.4 flare on July 12, 2012 in solar active region 11520, but the corresponding magnetic field change is not clear. We construct a data-constrained magnetohydrodynamic simulation of the f
Externí odkaz:
http://arxiv.org/abs/2211.02354
Autor:
Wang, Yuming, Bai, Xianyong, Chen, Changyong, Chen, Linjie, Cheng, Xin, Deng, Lei, Deng, Linhua, Deng, Yuanyong, Feng, Li, Gou, Tingyu, Guo, Jingnan, Guo, Yang, Hao, Xinjun, He, Jiansen, Hou, Junfeng, Jiangjiang, Huang, Huang, Zhenghua, Ji, Haisheng, Jiang, Chaowei, Jiang, Jie, Jin, Chunlan, Li, Xiaolei, Li, Yiren, Liu, Jiajia, Liu, Kai, Liu, Liu, Liu, Rui, Qiu, Chengbo, Shen, Chenglong, Shen, Fang, Shen, Yuandeng, Shi, Xiangjun, Su, Jiangtao, Su, Yang, Su, Yingna, Sun, Mingzhe, Tan, Baolin, Tian, Hui, Wang, Yamin, Xia, Lidong, Xie, Jinglan, Xiong, Ming, Xu, Mengjiao, Yan, Xiaoli, Yan, Yihua, Yang, Shangbin, Yang, Shuhong, Zhang, Shenyi, Zhang, Quanhao, Zhang, Yonghe, Zhao, Jinsong, Zhou, Guiping, Zou, Hong
Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360{\deg} perspective in the ecliptic plane. It will deploy three 120{\deg}-separated spacecraft on the 1-AU orbit. The first spacecra
Externí odkaz:
http://arxiv.org/abs/2210.10402
Autor:
Dai, Jun, Li, Zhentong, Wang, Ya, Xu, Zhe, Zhang, Yanjie, Li, Leping, Zhang, Qingmin, Su, Yingna, Ji, Haisheng
We present an investigation of partial filament eruption on 2012 June 17 in the active region NOAA 11504. For the first time, we observed the vertical splitting process during the partial eruption with high resolution narrow band images at 10830 . Th
Externí odkaz:
http://arxiv.org/abs/2201.11314
We investigate the failed partial eruption of a filament system in NOAA AR 12104 on 2014 July 5, using multiwavelength EUV, magnetogram, and H$\alpha$ observations, as well as magnetic field modeling. The filament system consists of two almost co-spa
Externí odkaz:
http://arxiv.org/abs/2111.13174