Zobrazeno 1 - 10
of 227
pro vyhledávání: '"Liu, Xianyu"'
Autor:
Xu, Yu, Alvarado-Gómez, Julián D., Tian, Hui, Poppenhäger, Katja, Guerrero, Gustavo, Liu, Xianyu
Coronal mass ejections (CMEs) on stars can change the stars' magnetic field configurations and mass loss rates during the eruption and propagation and therefore, may affect the stars' rotation properties on long time-scales. The dynamics of stellar C
Externí odkaz:
http://arxiv.org/abs/2406.08194
Autor:
Chan, Lami, Tian, Hui, Liu, Xianyu, Török, Tibor, Bai, Xianyong, Feng, Yufei, Banerjee, Dipankar
Publikováno v:
ApJ 967 162 (2024)
Full-disk spectroscopic observations of the solar corona are highly desired to forecast solar eruptions and their impact on planets and to uncover the origin of solar wind. In this paper, we introduce a new multi-slit design (5 slits) to obtain extre
Externí odkaz:
http://arxiv.org/abs/2404.13120
Measurements of the stellar coronal magnetic field are of great importance in understanding the stellar magnetic activity, yet the measurements have been extremely difficult. Recent studies proposed a new method of magnetic field measurements based o
Externí odkaz:
http://arxiv.org/abs/2209.08755
Publikováno v:
In Journal of Chromatography A 16 August 2024 1730
Publikováno v:
In Journal of Energy Storage 1 June 2024 89
Publikováno v:
In International Journal of Pressure Vessels and Piping June 2024 209
Publikováno v:
In Fuel 1 June 2024 365
Autor:
Zhu, Hongxia, Gong, Li, Jiang, Ling, Liu, Xianyu, Hu, Laigang, Wu, Wenhao, Lin, Daohui, Yang, Kun
Publikováno v:
In Science of the Total Environment 10 October 2024 946
Autor:
Chen, Yajie, Liu, Xianyu, Tian, Hui, Bai, Xianyong, Jin, Meng, Li, Wenxian, Yang, Yang, Yang, Zihao, Deng, Yuanyong
Measurements of the magnetic field in the stellar coronae are extremely difficult. Recently, it was proposed that the magnetic-field-induced transition (MIT) of the Fe X 257 {\AA} line can be used to measure the coronal magnetic field of the Sun. We
Externí odkaz:
http://arxiv.org/abs/2108.08155
Autor:
Chen, Yajie, Li, Wenxian, Tian, Hui, Chen, Feng, Bai, Xianyong, Yang, Yang, Yang, Zihao, Liu, Xianyu, Deng, Yuanyong
It was recently proposed that the intensity ratios of several extreme ultraviolet spectral lines from the Fe X ion can be used to measure the solar coronal magnetic field based on the magnetic-field-inducedtransition (MIT) theory. To verify the suita
Externí odkaz:
http://arxiv.org/abs/2107.11783