Zobrazeno 1 - 10
of 206
pro vyhledávání: '"Xia, LiDong"'
Autor:
Shi, Xinzheng, Fu, Hui, Huang, Zhenghua, Yan, Limei, Ma, Chi, Huangfu, Chenxi, Song, Hongqiang, Xia, Lidong
The dependence of the sources and properties of the near-Earth solar wind on solar cycle activity is an important issue in solar and space physics. We use the improved two-step mapping procedure that takes into account the initial acceleration proces
Externí odkaz:
http://arxiv.org/abs/2407.00915
Autor:
Liang, Shiyu, Wang, Ziyuan, Huang, Zhenghua, Wei, Hengyuan, Fu, Hui, Xiong, Ming, Xia, Lidong
Loops are fundamental structures in the magnetized atmosphere of the sun. Their physical properties are crucial for understanding the nature of the solar atmosphere. Transition region loops are relatively dynamic and their physical properties have no
Externí odkaz:
http://arxiv.org/abs/2404.09805
Autor:
Li, Haiyi, Huang, Zhenghua, Deng, Kaiwen, Fu, Hui, Xia, Lidong, Song, Hongqiang, Xiong, Ming, Wei, Hengyuan, Qi, Youqian, Zhang, Chao
Context. Propagating streamer blobs could be an important source of disturbances in the solar wind. Direct observations on formation of streamer blobs could be a proxy for understanding the formation of small-scale structures and disturbances in the
Externí odkaz:
http://arxiv.org/abs/2402.02375
The studies on the origination and generation mechanisms of ICME materials are crucial for understanding the connection between CMEs and flares. The materials inside ICMEs can be classified into three types, coming from corona directly (corona-materi
Externí odkaz:
http://arxiv.org/abs/2309.09434
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
The Structure of Coronal Mass Ejections Recorded by the K-Coronagraph at Mauna Loa Solar Observatory
Previous survey studies reported that coronal mass ejections (CMEs) can exhibit various structures in white-light coronagraphs, and $\sim$30\% of them have the typical three-part feature in the high corona (e.g., 2--6 $R_\odot$), which has been taken
Externí odkaz:
http://arxiv.org/abs/2307.01398
The origination and generation mechanisms of small magnetic flux ropes (SFRs), which are important structures in solar wind, are not clearly known. In present study, 1993 SFRs immersed in coronal holes, active regions, and quiet Sun solar wind are an
Externí odkaz:
http://arxiv.org/abs/2304.11802
Autor:
Song, Hongqiang, Zhang, Jie, Li, Leping, Yang, Zihao, Xia, Lidong, Zheng, Ruisheng, Chen, Yao
Coronal mass ejections (CMEs) result from eruptions of magnetic flux ropes (MFRs) and can possess a three-part structure in white-light coronagraphs, including a bright front, dark cavity and bright core. In the traditional opinion, the bright front
Externí odkaz:
http://arxiv.org/abs/2212.04013
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:
Wei, Hengyuan, Huang, Zhenghua, Fu, Hui, Xiong, Ming, Xia, Lidong, Zhang, Chao, Deng, Kaiwen, Li, Haiyi
Jets are one of the most common eruptive events in the solar atmosphere, and they are believed to be important in the context of coronal heating and solar wind acceleration. We present an observational study on a sequence of jets with the data acquir
Externí odkaz:
http://arxiv.org/abs/2208.00112