He Fei
hefei@mail.iggcas.ac.cn
Chinese, English
Beijing
University of Chinese Academy of Sciences
Earth sciences
  • 2006-09--2011-06 Doctor of Science: Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences
  • 2002-09--2006-06 Bachelor of Science: Southwest University
  • 2021-01~Present, Institute of Geology and Geophysics, Chinese Academy of Sciences, Researcher
  • 2017-02~2020-12, Institute of Geology and Geophysics, Chinese Academy of Sciences, Associate Researcher
  • 2013-09~2017-02, Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Associate Researcher
  • 2011-07~2013-09, Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Assistant Researcher
  • Fu Chengyi Youth Science and Technology Award, National, 2023
  • International Union of Radio Science Young Scientist Award, Other, 2019
Plasma layer dynamics
Ionospheric dynamics in the auroral region
Ionosphere-plasma layer coupling
Planetary optical remote sensing
Magnetospheric optical detection technology
Magnetospheric optical detection inversion technology
Space weather
  • Sawtooth and dune auroras simultaneously driven by waves around the plasmapause, He Fei, 2023
  • Progress in Planetary Optical Observations at Lenghu, He Fei, 2023
  • The 50BiN Telescope of CWNU and Open Clusters Studies, He Fei, 2023
  • The orbit schemes to monitor Martian dust storms: Benefits to China’s future Mars missions, He Fei, 2023
  • Evidence for lunar tide effects in Earth's plasmasphere, He Fei, 2023
  • The impact of dust storms on Mars surface rovers: Review and prospect, He Fei, 2023
  • Monitoring methods for Martian dust storms, He Fei, 2023
  • A New Method for Predicting Non-Recurrent Geomagnetic Storms, He Fei, 2023
  • Martian Proton Aurora Brightening Reveals Atmospheric Ion Loss Intensifying, He Fei, 2023
  • The 8‐Year Solar Cycle During the Maunder Minimum, He Fei, 2023
  • A Simplified Pointing Model for Alt-Az Telescopes, He Fei, 2023
  • A Radial Standing Pc5-6 Wave and Its Energy Coupling With Field Line Resonance Within the Dusk-Sector Magnetosphere, He Fei, 2023
  • Banana Current in the Inner Magnetosphere Observed by Van Allen Probes, He Fei, 2023
  • Survival of the magnetotactic bacterium Magnetospirillum gryphiswaldense exposed to Earth's lower near space, He Fei, 2022
  • Comparison of upstream solar wind plasma characteristics observed by Tianwen-1, Mars Express, and MAVEN satellites, He Fei, 2022
  • Lenghu Astronomical Observing Site and Dark Sky Protection, He Fei, 2022
  • Preliminary predictions of the dust storm activity at the landing site of China's Zhurong Mars rover in 2022, He Fei, 2022
  • The orbit schemes to monitor Martian dust storms, He Fei, 2022
  • A Statistical Model of Inner Magnetospheric Electron Density: Van Allen Probes Observations, He Fei, 2022
  • Correlations Between Giant Undulations and Plasmapause Configurations, He Fei, 2022
  • Three-dimensional Configuration of Induced Magnetic Fields around Mars, He Fei, 2022
  • The solar wind plasma upstream of Mars observed by Tianwen-1: Comparison with Mars Express and MAVEN, He Fei, 2022
  • The Frequency-Domain Characterization of Cosmic Ray Intensity Variations Before Forbush Decreases Associated With Geomagnetic Storms, He Fei, 2022
  • Astrobiology at altitude in Earth's near space, He Fei, 2022
  • The impact of dust storms on Mars surface rovers: Review and prospect, He Fei, 2022
  • Monitoring methods for Martian dust storms, He Fei, 2022
  • Ancient equatorial aurora reveals evolution of the west Pacific anomaly, He Fei, 2022
  • Far-ultraviolet airglow remote sensing measurements on Feng Yun 3-D meteorological satellite, He Fei, 2022
  • Solar X-ray and EUV imager on board the FY-3E satellite, He Fei, 2022
  • Long-term variations in precipitable water vapor and temperature at Lenghu Site, He Fei, 2022
  • Statistical Characteristics of Giant Undulations During Geomagnetic Storms, He Fei, 2021
  • Evaluation of the 900-Year European Auroral Records With Extreme Value Theory, He Fei, 2021
  • Ancient Auroral Records Compiled From Korean Historical Books, He Fei, 2021
  • Automatic Scheduling Tool for Balloon-Borne Planetary Optical Remote Sensing, He Fei, 2021
  • Lenghu on the Tibetan Plateau as an astronomical observing site, He Fei, 2021
  • Longitudinal Dependence of Ionospheric Poynting Flux in the Northern Hemisphere During Quite Times, He Fei, 2021
  • Development and prospect of planetary optical remote sensing at Lenghu, He Fei, 2021
  • Equatorial auroral records reveal dynamics of the paleo-West Pacific geomagnetic anomaly, He Fei, 2021
  • A statistical analysis of the electron number density fluctuations near the plasmapause based on Van Allen Probes observations, He Fei, 2020
  • Equatorial aurora: the aurora-like airglow in the negative magnetic anomaly, He Fei, 2020
  • Implantation of Earth's Atmospheric Ions Into the Nearside and Farside Lunar Soil: Implications to Geodynamo Evolution, He Fei, 2020
  • Plasmapause surface wave oscillates the magnetosphere and diffuse aurora, He Fei, 2020
  • A method to derive global O/N2 ratios from SSUSI/DMSP based on Re-AURIC algorithm, He Fei, 2020
  • Remote sensing of planetary space environment, He Fei, 2020
  • Prediction of the geomagnetic disturbances in high-latitude region with Weimer model, He Fei, 2020
  • The Magnetic Local Time Distribution of Storm Geomagnetic Field Disturbance Under Different Conditions of solar Wind and interplanetary Magnetic Field, He Fei, 2019
  • Tilt of the ring current during the main phases of intense geomagnetic storms, He Fei, 2019
  • Wide-field auroral imager onboard the Fengyun satellite, He Fei, 2019
  • Evolution of the subauroral polarization stream oscillation during the severe geomagnetic storm on 20 november 2003, He Fei, 2019
  • Status and Prospect for Chinese Planetary Physics, He Fei, 2019
  • Development of a 3-D Plasmapause Model With a Back-Propagation Neural Network, He Fei, 2019
  • The Magnetospheric Driving Source of Double-P
Plasma Dynamics Auroral Ionosphere Coupling Remote Sensing Optical Technology Inversion Technology Space Weather Magnetosphere Detection Planetary Science

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