Zobrazeno 1 - 10
of 271
pro vyhledávání: '"YIJUN HOU"'
Autor:
Shoude Guan, Fei-Fei Jin, Jiwei Tian, I-I Lin, Iam-Fei Pun, Wei Zhao, John Huthnance, Zhao Xu, Wenju Cai, Zhao Jing, Lei Zhou, Ping Liu, Yihan Zhang, Zhiwei Zhang, Chun Zhou, Qingxuan Yang, Xiaodong Huang, Yijun Hou, Jinbao Song
Publikováno v:
Nature Communications, Vol 15, Iss 1, Pp 1-12 (2024)
Abstract Tropical Cyclones (TCs) are devastating natural disasters. Analyzing four decades of global TC data, here we find that among all global TC-active basins, the South China Sea (SCS) stands out as particularly difficult ocean for TCs to intensi
Externí odkaz:
https://doaj.org/article/4a534af3e6c847b2b93dbcf1fc598783
Publikováno v:
The Astrophysical Journal Letters, Vol 965, Iss 2, p L28 (2024)
Solar prominences, intricate structures on the Sun’s limb, have been a subject of fascination owing to their threadlike features and dynamic behaviors. Utilizing data from the New Vacuum Solar Telescope, Chinese H α Solar Explorer, and Solar Dynam
Externí odkaz:
https://doaj.org/article/af367dfbff2b44e08abf4a43ef97327f
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 69 (2024)
White-light flares (WLFs) are energetic activity in the stellar atmosphere. However, observed solar WLFs are relatively rare compared to stellar WLFs or solar flares observed at other wavelengths, which limits our further understanding of solar/stell
Externí odkaz:
https://doaj.org/article/8b67e66fa2634bdf9c08b1e1dbed431b
Autor:
Shuhong Yang, Jie Jiang, Zifan Wang, Yijun Hou, Chunlan Jin, Qiao Song, Yukun Luo, Ting Li, Jun Zhang, Yuzong Zhang, Guiping Zhou, Yuanyong Deng, Jingxiu Wang
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 2, p 183 (2024)
As a large-scale motion on the Sun, the meridional flow plays an important role in determining magnetic structure and strength and solar cycle. However, the meridional flow near the solar poles is still unclear. The Hinode observations show that the
Externí odkaz:
https://doaj.org/article/ff9da7f9f63f41188cf3932c9726c34a
Autor:
Yilin Guo, Yijun Hou, Ting Li, Yuandeng Shen, Jincheng Wang, Jun Zhang, Jianchuan Zheng, Dong Wang, Lin Mei
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 2, p 110 (2024)
Prominence bubbles, the dark arch-shaped voids below quiescent prominences, are generally believed to be caused by the interaction between the prominences and the slowly emerging or quasi-stable underlying magnetic loops. However, this scenario could
Externí odkaz:
https://doaj.org/article/e5f7a59786d44c3eb1ef5784d5cc7975
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 2, p 159 (2024)
Until now, how the magnetic fields in M/X-class flaring active regions (ARs) differ from C-class flaring ARs remains unclear. Here, we calculate the key magnetic field parameters within the area of high photospheric free energy density (HED region) f
Externí odkaz:
https://doaj.org/article/98aa1c2e84004b1dbcb8b946fe737908
Publikováno v:
Journal of Marine Science and Engineering, Vol 11, Iss 9, p 1759 (2023)
Storm surge and concomitant waves induced by extreme weather systems can significantly modulate the marine dynamic environment. In this study, we used the Advanced Circulation-Simulating Waves Nearshore (ADCIRC-SWAN) coupled model to analyze spatiote
Externí odkaz:
https://doaj.org/article/4f1145ff3b724b058afaf21100de4b7f
Publikováno v:
Frontiers in Marine Science, Vol 9 (2022)
Storm surge inundation can induce great disasters in coastal regions, and Laizhou Bay (LZB), located in the Bohai Sea, is a bay that frequently experiences coastal storm flooding. In this study, we perform a numerical study of the effects of wind and
Externí odkaz:
https://doaj.org/article/7f0f494dc7ee47928fe3c5378b409b59
Autor:
Jun Zhang, Yijun Hou, Yue Fang, Feng Chen, Ting Li, Xiaoli Yan, Tao Ding, Zhiping Song, Yongyuan Xiang, Zhong Liu
Publikováno v:
The Astrophysical Journal Letters, Vol 942, Iss 1, p L2 (2022)
The question of what heats the solar chromosphere and corona remains one of the most important puzzles in solar physics and astrophysics. Up to now, two mechanisms are considered to work in heating the chromosphere and corona: magnetic reconnection a
Externí odkaz:
https://doaj.org/article/501137a1e1774751be7d05c1ff5cbad4
Autor:
Yijun Hou, Chuan Li, Ting Li, Jiangtao Su, Ye Qiu, Shuhong Yang, Liheng Yang, Leping Li, Yilin Guo, Zhengyong Hou, Qiao Song, Xianyong Bai, Guiping Zhou, Mingde Ding, Weiqun Gan, Yuanyong Deng
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 2, p 69 (2023)
Partial eruptions of solar filaments are the typical representatives of solar eruptive behavior diversity. Here we investigate a typical filament partial eruption event and present integrated evidence for the configuration of the pre-eruption filamen
Externí odkaz:
https://doaj.org/article/3be2c0650f054e51bea38c8ed2fd537b