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[期刊论文] 作者:WeiXing Wan, 来源:地球与行星物理:英文版 年份:2017
[期刊论文] 作者:LiBo Liu,WeiXing Wan, 来源:地球与行星物理:英文版 年份:2018
After the release of the previous report to the Committee on Space Research(COSPAR)on progress achieved by Chinese scientists in ionospheric researches(Liu LB a...
[期刊论文] 作者:LiBo Liu,WeiXing Wan, 来源:地球与行星物理:英文版 年份:2020
Since the release of the 2018 National Report of China on ionospheric research(Liu LB and Wan WX,2018)to the Committee on Space Research(COSPAR),scientists from...
[期刊论文] 作者:Libo Liu,Weixing Wan,, 来源:Science Bulletin 年份:2016
在中国的大陆, ionospheric 研究组的数字是超过 10。与 ionospheric 物理有关的约 110 篇文章在 2014-2015 期间被出版了。在空间研究(COSPAR ) 上的委员会的这份年度国家报...
[期刊论文] 作者:ZhiPeng Ren,WeiXing Wan,JianGa, 来源:地球与行星物理:英文版 年份:2020
Through respectively adding June tide and December tide at the low boundary of the GCITEM-IGGCAS model (Global CoupledIonosphere–Thermosphere–Electrodynamics...
[期刊论文] 作者:XinAn Yue,WeiXing Wan,Han Xiao, 来源:地球与行星物理:英文版 年份:2020
In the past decades,the Incoherent Scatter Radar(ISR)has been demonstrated to be one of the most powerful instruments for ionosphere monitoring.The Institute of...
[期刊论文] 作者:WeiXing Wan,Chi Wang,ChunLai L, 来源:地球与行星物理:英文版 年份:2020
Mars is not only our nearby but also the most Earth-like planetary neighbor.Scientific exploration of Mars is thus of crucial value to our understanding of the...
[期刊论文] 作者:Xing Li,WeiXing Wan,JinBin Cao, 来源:地球与行星物理:英文版 年份:2020
The wavenumber spectral components WN4 at the mesosphere and low thermosphere(MLT)altitudes(70–10 km)and in the latitude range between±45°are obtaine...
[期刊论文] 作者:Xing Li,WeiXing Wan,JinBin Cao, 来源:地球与行星物理:英文版 年份:2020
With the method of Hough mode decomposition(HMD),the tidal sources of the three main tidal components,namely,the migrating components DW1(diurnal westward propa...
[期刊论文] 作者:Fei He,Yong Wei,Weixing Wan, 来源:国家科学评论(英文版) 年份:2020
The most fantastic optical phenomena in the Earth’s upper atmosphere are the auroras.They are highly informative indicators of solar activity,geomagnetic activ...
[期刊论文] 作者:JunYi Wang,XinAn Yue,Yong Wei,WeiXing Wan, 来源:黑龙江科技信息 年份:2018
本文通过对荣华二采区10...
[期刊论文] 作者:WeiXing Wan,Chi Wang,ChunLai Li,Yong Wei,JianJun Liu,, 来源:Earth and Planetary Physics 年份:2020
Mars is not only our nearby but also the most Earth-like planetary neighbor. Scientific exploration of Mars is thus of crucial value to our understanding of the solar system. The existence of abundant...
[会议论文] 作者:Xiuhong Han,Eduard Dubinin,Yong Wei,Markus Fraenz,David Andrew,Weixing Wan,Stas Barabash, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
[会议论文] 作者:Xin Yao,Biqiang Zhao,Bo Xiong,Tao Yu,Weixing Wan,Jin Wen,Jie Zhu, 来源:2014年中国地球科学联合学术年会 年份:2014
In the present work we investigate variations of ionospheric total electron content (TEC) with applying empirical orthogonal functions (EOF) to the dataset from the global ionospheric maps (GIMs) prod...
[期刊论文] 作者:XinZhou Li,ZhaoJin Rong,JiaWei Gao,Yong Wei,Zhen Shi,Tao Yu,WeiXing Wan,, 来源:Earth and Planetary Physics 年份:2020
Unlike Earth, Mars lacks a global dipolar magnetic field but is dominated by patches of a remnant crustal magnetic field. In2021, the Chinese Mars Rover will land on the surface of Mars and measure th...
[会议论文] 作者:Xiuhong Han,Markus Fraenz,David Andrew,Yong Wei,Eduard Dubinin,Weixing Wan,Stas Barabash, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
The Martian ionosphere directly interacts with solar wind due to lack of a significant intrinsic magnetic field,however,the interaction is significantly influenced by the crustal field and induced fie...
[期刊论文] 作者:QianQian Han,Markus Fraenz,Yong Wei,Eduard Dubinin,Jun Cui,LiHui Chai,ZhaoJin Rong,WeiXing Wan,Yoshifumi, 来源:地球与行星物理(英文) 年份:2020
The Venusian dayside ionosphere, similar to other planetary ionospheres, is produced primarily by ionization of its neutralupper atmosphere due to solar extreme...
[会议论文] 作者:Chai Lihui,Weixing Wan,Markus Fraenz,Tielong Zhang,Yong Wei,Eduard Dubinin,Zhaojin Rong,Jun Zhong,Xiuhong, 来源:The Fourteenth International Solar Wind Conference (第十四届国际太阳 年份:2015
The interplanetary magnetic field(IMF) frozen in the solar wind,together with the solar EUV radiation,can significantly affect the location of Venusian bow shock....
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