Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Ni, Yiwei"'
Autor:
Guo, Yang, Guo, Jinhan, Ni, Yiwei, Ding, M. D., Chen, P. F., Xia, Chun, Keppens, Rony, Yang, Kai E.
Solar eruptive activities could occur in weak magnetic field environments and over large spatial scales, especially relevant to eruptions involving intermediate or quiescent solar filaments. To handle the large scales, we implement and apply a flux r
Externí odkaz:
http://arxiv.org/abs/2309.01325
Autor:
Guo, Jinhan, Qiu, Ye, Ni, Yiwei, Guo, Yang, Li, Chuan, Gao, Yuhang, Schmieder, Brigitte, Poedts, Stefaan, Chen, Pengfei
Solar filaments often exhibit rotation and deflection during eruptions, which would significantly affect the geoeffectiveness of the corresponding coronal mass ejections (CMEs). Therefore, understanding the mechanisms that lead to such rotation and l
Externí odkaz:
http://arxiv.org/abs/2308.08831
In this Letter, we perform a detailed analysis of the M5.5-class eruptive flare occurring in active region 12929 on 2022 January 20. The eruption of a hot channel generates a fast coronal mass ejection (CME) and a dome-shaped extreme-ultraviolet (EUV
Externí odkaz:
http://arxiv.org/abs/2209.00194
Autor:
Qiu, Ye, Rao, ShiHao, Li, Chuan, Fang, Cheng, Ding, MingDe, Li, Zhen, Ni, YiWei, Wang, WenBo, Hong, Jie, Hao, Qi, Dai, Yu, Chen, PengFei, Wan, XiaoSheng, Xu, Zhi, You, Wei, Yuan, Yuan, Tao, HongJiang, Li, XianSheng, He, YuKun, Liu, Qiang
Publikováno v:
Sci. China-Phys. Mech. Astron. 65, 289603 (2022)
The H{\alpha} line is an important optical line in solar observations containing the information from the photosphere to the chromosphere. To study the mechanisms of solar eruptions and the plasma dynamics in the lower atmosphere, the Chinese H{\alph
Externí odkaz:
http://arxiv.org/abs/2205.06075
Autor:
Li, Chuan, Fang, Cheng, Li, Zhen, Ding, MingDe, Chen, PengFei, Qiu, Ye, You, Wei, Yuan, Yuan, An, MinJie, Tao, HongJiang, Li, XianSheng, Chen, Zhe, Liu, Qiang, Mei, Gui, Yang, Liang, Zhang, Wei, Cheng, WeiQiang, Chen, JianXin, Chen, ChangYa, Gu, Qiang, Huang, QingLong, Liu, MingXing, Han, ChengShan, Xin, HongWei, Chen, ChangZheng, Ni, YiWei, Wang, WenBo, Rao, ShiHao, Li, HaiTang, Lu, Xi, Wang, Wei, Lin, Jun, Jiang, YiXian, Meng, LingJie, Zhao, Jian
Publikováno v:
Sci. China-Phys. Mech. Astron. 65, 289602 (2022)
The Chinese H{\alpha} Solar Explorer (CHASE), dubbed "Xihe" - Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a newly developed
Externí odkaz:
http://arxiv.org/abs/2205.05962
As one of the main formation mechanisms of solar filament formation, the chromospheric evaporation-coronal condensation model has been confirmed by numerical simulations to explain the formation of filament threads very well in flux tubes with single
Externí odkaz:
http://arxiv.org/abs/2107.12181
Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associated with coronal sheared and twisted magnetic field lines. However, the
Externí odkaz:
http://arxiv.org/abs/2107.02580
Publikováno v:
Journal of Physics: Conference Series; 2024, Vol. 2876 Issue 1, p1-7, 7p
Autor:
Guo, Yang, Guo, Jinhan, Ni, Yiwei, Xia, Chun, Zhong, Ze, Ding, Mingde, Chen, Pengfei, Keppens, Rony
Publikováno v:
Reviews of Modern Plasma Physics; 9/5/2024, Vol. 8 Issue 1, p1-40, 40p
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