Zobrazeno 1 - 10
of 847
pro vyhledávání: '"TAN, Song"'
A solar jet can often cause coronal mass ejections (CMEs) with different morphologies in the high corona, for example, jet-like CMEs, bubble-like CMEs, and so-called twin CMEs that include a pair of simultaneous jet-like and bubble-like CMEs. However
Externí odkaz:
http://arxiv.org/abs/2404.19179
Autor:
Zhou, Xinping, Shen, Yuandeng, Yan, Yihua, Yu, Ke, Qu, Zhining, Ibrahim, Ahmed Ahmed, Tang, Zehao, Zhou, Chengrui, Tan, Song, Qiu, Ye, Liang, Hongfei
This paper presents three distinct wave trains that occurred on 2023 April 21: a broad quasi-periodic fast-propagating (QFP) wave train and a bi-directional narrow QFP wave train. The broad QFP wave train expands outward in a circular wavefront, whil
Externí odkaz:
http://arxiv.org/abs/2404.18391
Autor:
Shen, Yuandeng, Liu, Dongxu, Yao, Surui, Zhou, Chengrui, Tang, Zehao, Qu, Zhining, Zhou, Xinping, Duan, Yadan, Tan, Song, Ibrahim, Ahmed Ahmed
Double-decker filaments and their eruptions have been widely observed in recent years, but their physical formation mechanism is still unclear. Using high spatiotemporal resolution, multi-wavelength observations taken by the New Vacuum Solar Telescop
Externí odkaz:
http://arxiv.org/abs/2401.11080
Autor:
Tan, Song, Shen, Yuandeng, Zhou, Xinping, Tang, Zehao, Zhou, Chengrui, Duan, Yadan, Yao, Surui
We report the first observations of simultaneous large-amplitude longitudinal and transverse oscillations of a quiescent filament trigged by a two-sided-loop jet formed by the magnetic reconnection between the filament and an emerging loop in the fil
Externí odkaz:
http://arxiv.org/abs/2301.07989
Autor:
Ying Gao, Pengjie Wang, Bin Liu, Shirui Xu, Shiyou Chen, Yinren Shou, Jianbo Liu, Zhusong Mei, Zhengxuan Cao, Tianqi Xu, Zhipeng Liu, Zhuo Pan, Defeng Kong, Ziyang Peng, Yulan Liang, Tan Song, Xun Chen, Qingfan Wu, Yujia Zhang, Jiarui Zhao, Wei Qi, Zhigang Deng, Yanying Zhao, Fuyuan Wu, Matt Zepf, Rafael Ramis, Paul R. Bolton, Xueqing Yan, Wenjun Ma, Jörg Schreiber
Publikováno v:
Physical Review Research, Vol 6, Iss 4, p L042031 (2024)
We demonstrate an all-optical method that online produces “microstructured” targets by manipulating a Laguerre-Gaussian (LG) prepulse. Besides the enhancement of the proton number, the cutoff energy is nearly doubled. Such transient “microstruc
Externí odkaz:
https://doaj.org/article/10801618300f4bf18cfa771a93e09a6b
Autor:
Xiao, Xiao1,2 (AUTHOR) xiaoxiao1@cib.ac.cn, Tan, Song1 (AUTHOR) tansong@cib.ac.cn, He, Kehu3 (AUTHOR) hekehu2024@126.com, Chen, Ying1,2 (AUTHOR) chenying@cib.ac.cn, Cui, Lin1,2 (AUTHOR) cuilin@cib.ac.cn, Zhu, Bicheng1 (AUTHOR) zhubc@cib.ac.cn, Qiu, Xia4 (AUTHOR) qiu999@cjlu.edu.cn, Qi, Yin1 (AUTHOR) qiyin@cib.ac.cn, Yang, Weizhao1 (AUTHOR) qiyin@cib.ac.cn
Publikováno v:
Animals (2076-2615). Oct2024, Vol. 14 Issue 20, p2923. 13p.
Autor:
Duan, Yadan, Shen, Yuandeng, Chen, Hechao, Tang, Zehao, Zhou, Chenrui, Zhou, Xinping, Tan, Song
Solar macrospicules are beam-like cool plasma ejections of size in-between spicules and coronal jets, which can elucidate potential connections between plasma jetting activity at different scales. With high-resolution observations from the {\em New V
Externí odkaz:
http://arxiv.org/abs/2212.03425
Autor:
Zhou, Xinping, Shen, Yuandeng, Liang, Hongfei, Qu, Zhining, Duan, Yadan, Tang, Zehao, Zhou, Chengrui, Tan, Song
About the driven mechanisms of the quasi-periodic fast-propagating (QFP) wave trains, there exist two dominant competing physical explanations: associated with the flaring energy release or attributed to the waveguide dispersion. Employing Solar Dyna
Externí odkaz:
http://arxiv.org/abs/2211.14488
Autor:
Shen, Yuandeng, Yao, Surui, Tang, Zehao, Zhou, Xinping, Qu, Zhining, Duan, Yadan, Zhou, Chengrui, Tan, Song
Publikováno v:
A&A 665, A51 (2022)
Quasi-periodic fast-propagating (QFP) magnetosonic wave trains are commonly observed in the low corona at extreme ultraviolet wavelength bands. Here, we report the first white-light imaging observation of a QFP wave train propagating outwardly in the
Externí odkaz:
http://arxiv.org/abs/2207.08110
Autor:
Tan, Song, Shen, Yuandeng, Zhou, Xinping, Duan, Yadan, Tang, Zehao, Zhou, Chengrui, Yao, Surui
The fine magnetic structure is vitally important to understanding the formation, stabilization and eruption of solar filaments, but so far, it is still an open question yet to be resolved. Using stereoscopic observations taken by the Solar Dynamics O
Externí odkaz:
http://arxiv.org/abs/2206.13827