共找到5條詞條名為王繼業的結果 展開
- 副主任醫師
- 溫縣黃庄鎮黨委書記
- 中央民族大學教授
- 桂林市第二人民醫院工作者
- 2022年北京冬奧會火炬手
王繼業
中央民族大學教授
王繼業,男,碩士,中央民族大學信息工程學院教授,北京市電子線路研究會理事,中國電子學會電子線路研究會理事。
1995年畢業后長時間就職於北大青鳥公司,2001年離開青鳥公司到中央民族大學任教。
2007年起任電子信息工程系主任,現已卸任
北京市電子線路研究會理事,中國電子學會電子線路研究會理事。
研究領域
文章
1. Zhang Ling Qian, Liu Zhen Xing, Ma Zhi Wei, Pu Zhu Yin, Wang Ji Ye, Shen Chao. The continuous tailward flow in the near-Earth magnetotail explored by TC-1. Chin Sci Bulletin., 2007, 52(1), 1-6 張靈倩,劉振興,馬志為等,TC-1衛星在近地磁尾觀測到的持續尾向流事件,中國科學通報,52卷4期,p432-437,2007
2. Zhang Ling Qian, Liu Zhen Xing, Wang Ji Ye, Ma Zhi Wei, Pu Zhu Yin, Shen Chao, Guo Jiu Ling. The distribution characteristics of the near-Earth plasma flow explored by TC-1. Chin Sci Bulletin., 2007, 53(7): 843-847 張靈倩,劉振興,王繼業,馬志為等,地球磁層內近地磁尾流場的分佈特性,中國科學通報,52卷7期,p843-847,2007
3. Liu Zhen Xing, Zhang Ling Qian, Ma Zhi Wei, Wang Ji Ye, Pu Zhu Yin, Shen Chao, Guo Jiu Ling. The statistical characteristics of the tailward flows in the near-Earth region explored by TC-1. Chinese J. Geophys. (in Chinese), 2007, 50(3): 655-661 劉振興,張靈倩,馬志為等,探測一號衛星在近地磁尾觀測到的尾向流統計特性,地球物理學報,50卷3期,p654-661,2007
4. Zhang Ling Qian, Liu Zhen Xing, Wang Ji Ye, Pu ZhuYin, Ma ZhiWei, Shen Chao. Effect of tailward flows from the ionosphere on the near-Earth magnetic field. Chin. J. Space Sci., (in Chinese) 2007, 27(3): 192-197 張靈倩,劉振興,王繼業,濮祖蔭,馬志為,沈超。來自電離層的尾向流對近地磁場位形的影響,空間科學學報, 27卷3期,p192-197,2007
5. Wang JiYe, Zhang ling qian. Polynomial Fit Of The Magnetic Field In The Near-Earth Magnetotail Around The Equator Region., Journal of The Central University for Nationalities (in Chinese), 2007
6. ZHANG LingQian, LIU ZhenXing, MA ZhiWei, W. Baumjohann, J. Wu, M.W. Dunlop, L. Lu, J.Y. Wang. A New Processing Method for the AE Index, Sci in China, 2008, 51, 1713-1720
7. Wang ji-ye,ZHANG ling-qian,LIU zhen-xing,MA zhi-wei,Shi jian-kui,Guo jiu-ling. The ULF Wave In the Pile-up and Dipolarization Process. Chinese J. Geophys.(In Chinese), 2008, 51(5): 1285-1295 (通量堆積和偶極化過程中的超低頻波動)
8. Zhang, L. Q., Z. X. Liu, W. Baumjohann, Z. W. Ma, Z. Y. Pu, M. W. Dunlop, L. Lu, J. K. Shi, C. Carr, H. Rème, and J. Y. Wang (2009), Convective bursty flows in the near-Earth magnetotail inside 13 RE, J. Geophys. Res., 114, A02202, doi:10.1029/2008JA013125.
9. Wang Jiye, Zhang Lingqian, et al. (2009), Tailward Flow, Plasma Sheet Thinning and Dipolarization Observed by TC-1 Satellite. (In Chinese), Progress in Geophys, 2009, 24 (4): 1183~1188, 王繼業,張靈倩,劉振興,馬志為,史建魁,郭九苓(2009)TC-1衛星在近地磁尾觀測到的持續尾向流、等離子體片變薄和偶極化過程, 地球物理進展2009 24 (4): 1183~1188
10. Zhang, L. Q., Z. X. Liu, Z. W. Ma, W. Baumjohann, Z. Y. Pu, M. W. Dunlop, H. Rème, and J. Y. Wang (2010), X line distribution determined from earthward and tailward convective bursty flows in the central plasma sheet, J. Geophys. Res., 115, A06218, doi:10.1029/2009JA014429.
11. Zhang, L. Q. et al., Earthward convective bursty flows in the center plasma sheet, Chin. J. Space Sci., 2011, 31(1): 20-26 張靈倩,王繼業,劉振興,史建魁。中心等離子體片的地向對流型高速流,空間科學學報, 31卷1期,p20-26,2011
12. 基於超像素和SVM的互動式聯合分割演演算法研究,喬琪瓏,王繼業,楊舒,電視技術,2015年22期,85頁。
13. Zhang, L. Q., Lui, A. T. Y., Baumjohann, W., Wang, J. Y (2015), Probabilities of magnetic reconnection encounter at different activity levels in the Earth’s magnetotail, Advances in Space research, doi:10.1016/ja.asr.2015,05.001
14. Zhang, L. Q., J. Y. Wang, W. Baumjohann, H. Rème, and M. W. Dunlop (2015), Earthward and tailward flows in the plasma sheet, J. Geophys. Res. Space Physics, 120, 4487–4495, doi:10.1002/2015JA021154.
15. Zhang, L. Q., W. Baumjohann, J. Y. Wang, H. Rème, and M. W. Dunlop, T. Chen (2015), Statistical characteristics of slow earthward and tailward flows in the plasma sheet, J. Geophys. Res. Space Physics, 120, doi: 10.1002/2015JA021354.
16. Zhang, L. Q., J. Y. Wang, W. Baumjohann, H. Rème, L. Dai, M. W. Dunlop, T. Chen, and Y. Huang (2015), X-lines in the magnetotail for southward and northward IMF conditions, J. Geophys. Res. Space Physics, doi:10.1002/2015JA021503.
17. Zhang, L. Q., C. Wang, J. Y. Wang, Lui, A. T. Y. (2019), Statistical properties of the IMF clock angle in the solar wind with northward and southward interplanetary magnetic field based on ACE observation from 1998 to 2009: dependence on the temporal scale of the solar wind, Advances in Space research, doi:10.1016/ja.asr.2018,14.094