Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Nanbin Xiang"'
Autor:
Fuyu Li, Changhui Rao, Huaning Wang, Xinhua Zhao, Nanbin Xiang, Linhua Deng, Haitang Li, Yu Liu
Publikováno v:
The Astrophysical Journal Letters, Vol 976, Iss 1, p L2 (2024)
Solar active regions (ARs) provide the required magnetic energy and the topology configuration for flares. Apart from conventional static magnetic parameters, the evolution of AR magnetic flux systems should have nonnegligible effects on magnetic ene
Externí odkaz:
https://doaj.org/article/34a9c1d32c9544cabac348bb7f171361
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 2, p 235 (2024)
Coronal mass ejection (CME) is a powerful solar phenomenon that can lead to severe space weather events. Forecasting whether and when the corresponding interplanetary coronal mass ejection (ICME) will reach the Earth is very important in space weathe
Externí odkaz:
https://doaj.org/article/7b38614154e8415a9bb9c5eb57631bd6
Autor:
Fuyu Li, Changhui Rao, Xinhua Zhao, Yang Guo, Xiaoying Gong, Yuhao Chen, Nanbin Xiang, Huaning Wang
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 271, Iss 1, p 34 (2024)
The formation mechanism of light bridges (LBs) is strongly related to the dynamic evolution of solar active regions (ARs). To study the relationship between LB formation and AR evolution phases, we employ 109 LB samples from 69 ARs in 2014 using obse
Externí odkaz:
https://doaj.org/article/45e7a5dff6f246fdad8d7b69ebd15d3c
Autor:
Ran Li, Xinhua Zhao, Jingye Yan, Lin Wu, Yang Yang, Xuning Lv, Shiwei Feng, Mengsi Ruan, Nanbin Xiang, Yidan Liang
Publikováno v:
The Astrophysical Journal, Vol 962, Iss 2, p 178 (2024)
Since fast head-on coronal mass ejections and their associated shocks represent potential hazards to the space environment of the Earth and even other planets, forecasting the arrival time of the corresponding interplanetary shock is a priority in sp
Externí odkaz:
https://doaj.org/article/8f4076ec977741ae83ffda6f916478e8
Publikováno v:
Universe, Vol 8, Iss 1, p 30 (2022)
As an important index of solar activity, the 10.7-cm solar radio flux (F10.7) can indicate changes in the solar EUV radiation, which plays an important role in the relationship between the Sun and the Earth. Therefore, it is valuable to study and for
Externí odkaz:
https://doaj.org/article/7680036a9d494016be405c2d5f378d77
Publikováno v:
Quaternary International. 613:39-45
Based on the latest database, we analyze the characteristics of the changing trends of sunspot number (SSN) and temperatures of the global mean surface (GMST) as well as six latitude bands during the Holocene, aiming to explore the long-term response
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d02b273aa18ef6c0d477e5bfaf77d8d2
https://doi.org/10.1016/j.quaint.2021.09.006
https://doi.org/10.1016/j.quaint.2021.09.006
Publikováno v:
Publications of the Astronomical Society of Japan. 66:28
At mid and low heliographic latitudes, filament activity shifts equatorward starting from the beginning of the solar cycle. At high latitudes, it migrates poleward. Solar filaments exhibit the "rush to the poles" close to solar maximum, when the sola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6e88fafa44c4ae2de931ea6b6edde8d
https://doi.org/10.1093/pasj/pst029
https://doi.org/10.1093/pasj/pst029
Autor:
Li, Fuyu, Rao, Changhui, Wang, Huaning, Zhao, Xinhua, Xiang, Nanbin, Deng, Linhua, Li, Haitang, Liu, Yu
Publikováno v:
Astrophysical Journal Letters; 11/20/2024, Vol. 976 Issue 1, p1-6, 6p
Autor:
Zhang, Wanting1,2 wtzhang@spaceweather.ac.cn, Zhao, Xinhua1,3,4 fengx@spaceweather.ac.cn, Feng, Xueshang1 luwei181@mails.ucas.ac.cn, Liu, Cheng'ao5 liuchengao@cetc.com.cn, Xiang, Nanbin6 nanbin@ynao.ac.cn, Li, Zheng7 zli@nuist.edu.cn, Lu, Wei1,2
Publikováno v:
Universe (2218-1997). Jan2022, Vol. 8 Issue 1, p30-30. 1p.
Publikováno v:
Publications of the Astronomical Society of Japan; Apr2014, Vol. 66 Issue 1, p1-8, 8p