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姓名 何飞 性别:
职称 研究员 学位 博士
电话 010-82998310 传真: 010-62010846
Email: hefei[a]mail.iggcas.ac.cn 邮编: 100029
地址 北京朝阳区北土城西路19号,中科院地质与地球物理研究所
更多信息:
English地球与行星物理院重点实验室 行星物理学学科组
 
简历:

  何飞,博士,研究员。1984年11月生于四川省汉源县。2006年毕业于西南大学物理学系获学士学位。2011年毕业于中国科学院长春光学精密机械与物理研究所,获博士学位。从事地球与行星空间环境光学探测方法研究、空间光学遥感器总体设计、空间光学探测数据反演与科学应用、地球与磁层耦合动力学研究。在Nature Communications、National Science Review、GRL和JGR等国际重要期刊发表论文50多篇。多次担任JGR,GRL,中国科学和地球物理学报等杂志审稿人。 

  • 2002.09-2006.07 西南大学物理学系,理学学士 
  • 2006.09-2011.07 中国科学院长春光学精密机械与物理研究所,理学博士 
  • 2011.07-2013.09 中国科学院长春光学精密机械与物理研究所,助理研究员 
  • 2013.09-2017.02 中国科学院长春光学精密机械与物理研究所,副研究员 
  • 2017.02-2020.12,中国科学院地质与地球物理研究所,副研究员
  • 2021.01-至今,中国科学院地质与地球物理研究所,研究员
ORCiD: 0000-0003-0542-2686
 
学科类别:
行星物理学、空间物理学
 
研究方向:
  1. 地球与行星空间环境光学探测方法研究
  2. 空间光学探测数据反演与应用研究
  3. 地球与行星极光物理研究
  4. 地球与行星磁层动力学研究
 
职务:
 
社会任职:
 
承担科研项目情况:

主持 

  1. 中国科学院战略性先导科技专项课题
  2. 国家自然科学基金青年基金(批准号:41204102,2013-2015) 
  3. 国家自然科学基金面上项目(批准号:41674155,2017-2020) 

参与 

  1. 973项目子课题 
  2. 嫦娥工程、风云卫星工程
 
获奖及荣誉:
  1. 中国科学院青年创新促进会会员 
  2. 科技部遥感青年科技创新人才 
  3. 第三届全球华人空间天气科学大会优秀青年论文奖
 
代表论著:

2020: 

  1. He, F., R.-L. Guo, W. R. Dunn, Z. Yao, H.-S. Zhang, Y.-X. Hao, Q.-Q. Shi, Z.-J. Rong, J. Liu, A.-M. Tian, X.-X. Zhang*, Y. Wei*, Y.-L. Zhang, Q.-G. Zong, Z.-Y. Pu, W. Wan (2020). Plasmapause surface wave oscillates the magnetosphere and diffuse aurora. Nature Communications, 11, 1668, https://doi.org/10.1038/s41467-020-15506-3
  2. He, F., Y. Wei*, W. Wan* (2020). Equatorial aurora: aurora-like airglow in the negative magnetic anomaly. National Science Review, 7, 1606–1615, https://doi.org/10.1093/nsr/nwaa083
  3. Wang Y. Q., Chen, S., Xu, K. H., Yan L. M., Yue X., He, F.*, Wei, Y.* (2020). Ancient auroral records compiled from Korean historical books, J. Geophys. Res. Space Physics, in press.
  4. 何飞 (2020). 行星空间环境光学遥感. 科学通报, 65, 1305-1319, https://doi.org/10.1360/TB-2019-0804. 

2019: 

  1. He, F., Zhang, X.-X.*, Wang, W., Pu, Z.-Y., Zong, Q.-G., Yao, Z., et al. (2019). Evolution of the subauroral polarization stream oscillations during the severe geomagnetic storm on 20 November 2003. Geophys. Res. Lett., 46, 599–607. https://doi.org/10.1029/2018GL081446.
  2. Zhang, X.-X.#*, Chen, B.#, He, F.# (共同第一作者), et al. (2019). Wide-field auroral imager onboard Fengyun satellite. Light: Science & Applications, 8, 47. https://doi.org/10.1038/s41377-019-0157-7
  3. Zheng, Z., Lei, J., Yue, X., Zhang, X., & He, F.* (2019), Development of a 3-D plasmapause model with a back-propagation neural network. Space Weather, 17, 1689–1703.

2018: 

  1. He, F., Zhang, X.-X.*, Wang, W., Liu, L., Ren, Z.-P., Yue, X., et al. (2018). Large-scale structure of subauroral polarization streams during the main phase of a severe geomagnetic storm. J. Geophys. Res. Space Physics, 123, 2964–2973. https://doi.org/10.1002/2018JA025234.

2017: 

  1. F. He, X. X. Zhang*, W. B. Wang, W. X. Wan (2017), Different evolution patterns of subauroral polarization streams (SAPS) during intense storms and quiet-time substorms, Geophys. Res. Lett., 44, doi:10.1002/2017GL075449.
  2. He, F., X. X. Zhang, R. L. Lin, M.-C. Fok, R. M. Katus, M. W. Liemohn, D. L. Gallagher, and S. Nakano (2017), A new solar wind driven global dynamic plasmapause model: 2. Model and Validation, J. Geophys. Res. Space Physics, 122, 7153–7171, doi:10.1002/2017JA023913.  
  3. X. X. Zhang, F. He*, R. L. Lin, M.-C. Fok, R. M. Katus, M. W. Liemohn, D. L. Gallagher, and S. Nakano (2017), A new solar wind driven global dynamic plasmapause model: 1. Database and Statistics, J. Geophys. Res. Space Physics, 122, 7153–7171, doi:10.1002/2017JA023912
  4. Ding, G. X., F. He*, X. X. Zhang, and B. Chen (2017), A new auroral boundary determination algorithm based on observations from TIMED/GUVI and DMSP/SSUSI, J. Geophys. Res. Space Physics, 122, doi:10.1002/2016JA023295. 

2016: 

  1. He, F., X. X. Zhang, B. Chen, M.-C. Fok, and S. Nakano (2016), Determination of the Earth’s plasmapause location from the CE-3 EUVC images, J. Geophys. Res. Space Physics, 121, 296–304, doi:10.1002/2015JA021863. 
  2. He, F., X.-X. Zhang, W. Wang, and B. Chen (2016), Double-peak subauroral ion drifts (DSAIDs), Geophys. Res. Lett., 43, 5554–5562, doi:10.1002/2016GL069133. 
  3. Yan, Y., H. N. Wang, H. He, F. He, B. Chen, J. Q. Feng, J. S. Ping, C. Shen, R. L. Xu, and X. X. Zhang (2016), Analysis of observational data from extreme ultraviolet camera onboard Chang’E-3 mission, Astrophys. Space Sci., 361:76, doi:10.1007/s10509-016-2650-2. 
  4. He, H., C. Shen, H. N. Wang, X. X. Zhang, B. Chen, J. Yan, Y. L. Zou, A. M. Jorgensen, F. He, Y. Yan, X. S. Zhu, Y. Huang, and R. L. Xu (2016), Response of plasmaspheric configuration to substorms revealed by Chang’E-3, Sci. Rep., 6: 32362, doi:10.1038/srep32362. 

2015: 

  1. He, F., X.-X. Zhang, X.-Y. Wang, and B. Chen (2015), EUV emissions from solar wind charge exchange in the Earth’s magnetosheath: Three-dimensional global hybrid simulation, J. Geophys. Res. Space Physics, 120, 138-156, doi: 10.1002/2014JA020521. 
  2. Niu, Y. Y., X. X. Zhang, F. He, and Y. Jiang (2015), Statistical characteristics of the equatorial boundary of the nightside auroral particle precipitation, Sci. China Earth Sci., 58: 1602–1608, doi: 10.1007/s11430-015-5090-x. 
  3. Zhang, X. X., F. He*, W. B. Wang, B. Chen (2015), Hemispheric asymmetry of subauroral ion drifts: Statistical results, J. Geophys. Res. Space Physics, 120, 4544-4554, doi: 10.1002/2015JA021016. 
  4. Lv, J. T., X. X. Zhang, R. L. Lin, F. He, and Y. Jiang (2015), Dynamic distribution features of energetic proton in South Atlantic anomaly based on the observation of SAMPEX (in Chinese), Chin. J. Space Sci., 35(2), 192-202, doi: 10.11728/cjss2015.02.192. 

2014: 

  1. He, F., X.-X. Zhang, and B. Chen (2014), Solar cycle, seasonal, and diurnal variations of subauroral ion drifts: Statistical results, J. Geophys. Res. Space Physics, 119, 1-11, doi: 10.1002/2014JA019807.  
  2. Zhang, Y. C., He, F.,* X. X. Zhang, and B. Chen (2014), A method to calculate the ionospheric LBH dayglow emissions for the large field of view, Chinese J. Geophys., 57(2), 354?363, doi: 10.6038/cjg20140202. (in Chinese). 
  3. Zhang, Y. C., X. X. Zhang, F. He, and B. Chen (2014), Retrieving O/N2 technique from ionospheric FUV dayglow emissions, Opt. Precision Eng., 22(5), 1120-1128, doi: 10.3788/OPE.20142205.1120 (in Chinese).  
  4. Li, Y. P., H. J. Zhang, H. F. Wang, F. He, X. D. Wang, Y. Liu, S. L. Han, X. Zheng, X. D. Wang, B. Chen, H. B. Li, B. Chen, and J. L. Cao (2014), Thermal and stress studies of the 30.4 nm Mo/Si multilayer mirror for the moon-based EUV camera, Applied Surface Science, 317, 902-907.  
  5. Chen, B., K. F. Song, Z. H. Li, Q. W. Wu, Q. L. Ni, X. D. Wang, J. J. Xie, S. J. Liu, L. P. He, F. He, X. G. Wang, B. Chen, H. J. Zhang, X. D. Wang, H. F. Wang, X. Zheng, S. L. E, Y. C. Wang, T. Yu, L. Sun, J. L. Wang, Z. Wang, L. Yang, Q. L. Hu, K. Qiao, Z. S. Wang, X. W. Yang, H. M. Bao, W. G. Liu, Z. Li, Y. Chen, Y. Gao, H. Sun, W. C. Chen (2014), Investigation and calibration of the Moon-based EUV camera for Chang’E-3, Res. Astron. Astrophys., 14(12), 1654-1663, doi: 10.1088/1674–4527/14/12/013. 
  6. Feng, J. Q., J. J. Liu, F. He, W. Yan, X. Ren, X. Tan, L. P. He, B. Chen, W. Zuo, W. B. Win, Y. Su, Y. L. Zou, C. L. Li (2014), Data processing and initial results from the CE-3 Extreme Ultraviolet Camera, Res. Astron. Astrophys., 14(12), 1664-1673, doi: 10.1088/1674-4527/14/12/014. 
  7. Yang, H. B., L. H. Chen, Y. Li, H. W. Liu, F. He (2014), Thermal design and verification of transmission filter for wide angle auroral imager, Opt. Precision Eng., 22(11), 3019-3027, doi: 10.3788/OPE.20142211.3019 (in Chinese).  
  8. Li, Y. P., B. Chen, F. He, H. B. Yang, X. D. Wang, X. Zheng, X. D. Wang, H. J. Zhang, H. F. Wang, J. L. Cao (2014), In-situ and real time stress of 30.4 nm Mo/Si multilayer mirror for the moon-based EUV camera, Proc. SPIE, 9295, doi: 10.1117/12.2073023.  

2013:  

  1. He, F., X.-X. Zhang, B. Chen, M.-C. Fok, and Y.-L. Zou (2013), Moon-based EUV imaging of the Earth’s plasmasphere: Model simulations, J. Geophys. Res. Space Physics, 118, 1-19, doi: 10.1002/2013JA018962. 
  2. Yang, J. M., W. Q. Liu, W. Z. Lv, D. L. Zhang, F. He, Z. L. Wei, and Y. S. Kang (2013), Method of achieving a wide field-of-view head-mounted display with small distortion, Optics Lett., 38(12), 2035-2037, doi: 10.1364/OL.38.002035. 
  3. Li, X., F. He, and B. Chen (2012), Measuring system for diffraction efficiency of transmission grating in soft X-ray, J. Jilin Univ. (Eng. and Tech. Ed.), 43(4), 1011-1026, doi: 10.7964/jdxbgxb201304027 (in Chinese).  

2012:  

  1. He, F., X. X. Zhang, B. Chen, and M.-C. Fok (2012), Inversion of the Earth’s plasmaspheric density distribution from EUV images with genetic algorithm, Chinese J. Geophys., 55(1), 29?35, doi: 10.6038/j.issn.0001-5733.2012.01.003 (in Chinese).  
  2. He F., X. X. Zhang, B. Chen, and M.-C. Fok (2012), Plasmaspheric trough evolution under different conditions of subauroral ion drift, Sci. China. Tech. Sci., 55(5): 1?8, doi: 10.1007/s11431-012-4781-1. 
  3. Li, X., F. He, D. Li, and B. Chen (2012), Influence of structural defect of square-hole micro channel plate on imaging quality, Acta Optica Sinica, 32(10), 1-10, doi: 10.3788/AOS.201232.1011001 (in Chinese).  
  4. Li, X., F. He, and B. Chen (2012), Transmission grating measuring system in X-ray wavelength, J. Changchun Univ. Sci. and Tech. (Nat. Sci. Ed.), 35(3), 50-53 (in Chinese).  

2011:  

  1. He, F., X. X. Zhang, B. Chen, and M.-C. Fok (2011), Reconstruction of the plasmasphere from Moon-based EUV images, J. Geophys. Res., 116, A11203, doi: 10.1029/2010JA016364.  
  2. Chen, B., and F. He (2011), Optical design of moon-based earth’s plasmaspheric extreme ultraviolet imager, Opt. Precision Eng., 19(9), 2057-2062, doi: 10.3788/OPE.20111909.2057 (in Chinese).  

2010:  

  1. He, F., X. X. Zhang, B. Chen, and M.-C. Fok (2010), Calculation of the extreme ultraviolet radiation of the earth’s plasmasphere, Sci. China. Tech. Sci., 53(1), 200?205, doi: 10.1007/s11431-009-0311-1. 
  2. He, F., B. Chen, X. X. Zhang (2010), Moon-based imaging of the Earth’s plasmaspheric extreme ultraviolet radiation, Opt. Precision Eng., 18(12), 2564-2573, doi: 10.3788/OPE.20101812.2562 (in Chinese).  
 

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