FS
Fang Shen
National Space Science Center Chinese Academy of Sciences, Peking University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0002-4935-6679
Employment
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National Space Science Center Chinese Academy of Sciences Professor2013 - Present
Education
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Peking University Ph. D1999 - 2004
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Peking University Bachelor of Science1995 - 1999
Projects & Funding
Projects & funding information is unavailable.
Publications (86)
- Data Coverage Dependence of Interplanetary Scintillation Tomography: Insights from Carrington Rotation 2075 Save
- A numerical study of the interplanetary propagation of solar energetic particles with a three-dimensional heliospheric current sheet Save
- A Nonspherical Source Surface Model for the Solar Coronal Magnetic Field Save
- Self-consistent Numerical Model for Solar Wind Suprathermal Electrons: Coupling of MHD Turbulence and Electron Kinetics Save
- Optimization Algorithm for Determining the Source Surface Radius Based on Parker Solar Probe In Situ Measurements From Encounters 1 to 19 Save
- Variability in the Propagation Characteristics of Small Transients in the Near-Sun Solar Wind Identified by the CORAR Technique Save
- PASSIT-CME: A Pixel-annotation-free System for Automatic Segmentation, Inpainting, and Tracking of Coronal Mass Ejections Save
- Identification of Coronal Mass Ejection–Driven Shocks Based on Numerical Simulation and Deep Learning Save
- Influence of Solar Polar Magnetic Fields on the Propagation of Coronal Mass Ejections Save
- Automatic Identification of Interplanetary Shocks Based on Machine Learning Save
- Automatic Segmentation, Inpainting, and Tracking of CMEs By A Pixel-Annotation-Free System Save
- Modelling Solar Energetic particle (SEP) Transport Related with Stream Interaction Regions and CME Events Save
- Interaction of Four Homologous Coronal Mass Ejections near the Sun Save
- Non-Radial Propagation and Magnetic Field Evolution of Large-scale Magnetized Plasmoid from the Sun to Mars Save
- Simulation of the 2010 September 9 Solar Energetic Particle Event by Using a Data-constrained Transport Model Save
- Backmapping of the High- and Low-latitude Solar Wind under Multiple Heliospheric and Coronal Magnetic Field Configurations Save
- Fast Reconstruction of Solar Wind Magnetohydrodynamic Parameters at 0.1 au with Machine Learning Save
- MMS Observations of an Active Flux Rope During Asymmetric Magnetic Reconnection Save
- Automatic 3D Reconstruction of Coronal Mass Ejections Based on Dual-viewpoint Observations and Machine Learning Save
- A 2D Fourth-Order CESE Scheme for Solving the Ideal MHD Equations Save