Zobrazeno 1 - 10
of 1 700
pro vyhledávání: '"QIU Ye"'
Publikováno v:
Taiyuan Ligong Daxue xuebao, Vol 55, Iss 5, Pp 905-911 (2024)
Purposes This research has been carried out to investigate the wind load characteristics of dual-slope solar panels. Methods Wind tunnel tests with rigid models were conducted to investigate the effects of wind direction, inclination angle, and panel
Externí odkaz:
https://doaj.org/article/faecaa61d86a48bd8904e03bcbed46ad
Publikováno v:
Shuitu Baochi Xuebao, Vol 38, Iss 3, Pp 12-18 (2024)
[Objective] This study was aimed to elucidate wind-induced rill erosion characteristics on the windward slope. [Methods] Artificial simulated wind-driven rain experiments were conducted. The study investigated changes in water and sediment processes
Externí odkaz:
https://doaj.org/article/223edb76f9ec44fca5201bdb7b4d7002
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:
Qiu Ye, Ji Junyuan
Publikováno v:
E3S Web of Conferences, Vol 406, p 01019 (2023)
The effects of oxytetracycline on anaerobic ammonium oxidation (ANAMMOX) were analyzed in this study. Meanwhile, the change of specific ANAMMOX activity (SAA) and the content of heme c were also revealed. The performance of ANAMMOX reactor decreased
Externí odkaz:
https://doaj.org/article/3ea2637662b1496e94db55b08a88c7fa
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
Solar prominences observed close to the limb commonly include a bright feature that, from the perspective of the observer, runs along the interface between itself and the underlying chromosphere. Despite several idealised models being proposed to exp
Externí odkaz:
http://arxiv.org/abs/2403.09931
Publikováno v:
The Astrophysical Journal Letters, 961 (2024), 2, L30
The eruption of solar filaments, also known as prominences appearing off-limb, is a common phenomenon in the solar atmosphere. It ejects massive plasma and high-energy particles into interplanetary space, disturbing the solar-terrestrial environment.
Externí odkaz:
http://arxiv.org/abs/2401.16730
Autor:
Hou, Yijun, Li, Chuan, Li, Ting, Su, Jiangtao, Qiu, Ye, Yang, Shuhong, Yang, Liheng, Li, Leping, Guo, Yilin, Hou, Zhengyong, Song, Qiao, Bai, Xianyong, Zhou, Guiping, Ding, Mingde, Gan, Weiqun, Deng, Yuanyong
Partial eruptions of solar filaments are the typical representative of solar eruptive behavior diversity. Here we investigate a typical filament partial eruption event and present integrated evidence for configuration of the pre-eruption filament and
Externí odkaz:
http://arxiv.org/abs/2311.00456
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
Autor:
Wei, Hengyuan, Huang, Zhenghua, Li, Chuan, Hou, Zhenyong, Qiu, Ye, Fu, Hui, Bai, Xianyong, Xia, Lidong
Filaments are one of the most common features in the solar atmosphere, and are of significance in solar, stellar and laboratory plasma physics. Using data from the Chinese H$\alpha$ Solar Explorer, the Solar Upper Transition Region Imager and the Sol
Externí odkaz:
http://arxiv.org/abs/2308.15747