J. H. Guo
Also known as: Jin-Han Guo, 郭金涵
Harbin Institute of Technology, Nanjing University, KU Leuven
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Magnetic confinement fusion research · Stellar, planetary, and galactic studies
0000-0002-4205-5566
About
Jinhan’s research focuses on solar and heliospheric physics. He studies solar activities (e.g., coronal mass ejections, flares, and filaments) and interplanetary transients (e.g., magnetic clouds) by combining magnetohydrodynamic (MHD) modeling with observations. His main interests include: (1) Data-driven MHD modeling of CMEs in the heliosphere, covering their precursors, initiation, and propagation through interplanetary space; (2) Formation, fine structure, and dynamics of solar filaments; and (3) Numerical development and implementation of operational space-weather forecasting tools.
Employment
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Harbin Institute of Technology Associate Professor2026 - Present
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Nanjing University Postdoc2024 - 2026
Education
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KU Leuven Ph.D in Mathmatics2022 - 2024
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Nanjing University Ph.D in Astronomy2019 - 2024
Projects & Funding
Projects & funding information is unavailable.
Publications (56)
- Volume Dependence of Helicity-based Eruption Diagnostics in Recurrent Coronal Jets Save
- Observations and Magnetohydrodynamic Simulation of External Reconnection Resulting in a Failed Filament Eruption Save
- Data-based MHD simulation of the origin of a coronal mass ejection: onset mechanism and twist buildup Save
- Radiation Synthesis Tools: Arbitrary Perspective Multiwavelength Radiation Synthesis for Solar Magnetohydrodynamic Simulations Save
- Constraints and observational manifestations of failed solar eruptions in a toroidal magnetic cage Save
- Dynamics of An Erupting Filament and a Coronal Loop during Their Interaction Save
- Preferential Appearance of Hα Moreton Waves along Photospheric Magnetic Network Boundaries Save
- Multiple Extreme-ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare Save
- Observations of a Two-sided Loop Jet and Magnetic Reconnection Involving a Medium-scale Filament Eruption Save
- Rotation of a Solar Jet Driven by Plasma Flow along Helical Magnetic Fields in an Active Region Save
- Elongation of a Solar Filament and its Three-dimensional Numerical Reconstruction for Magnetic Structures Save
- Data-driven magnetohydrodynamic simulation of the initiation of a coronal mass ejection with multiple stages Save
- Data-constrained Magnetohydrodynamic Simulation of the Global Solar Corona Including Solar Wind Effects within 2.5 R ⊙ Save
- Two-stage Primary Acceleration in Filament Initial Eruption under a Fan–Spine Magnetic Configuration Save
- SIP-IFVM: An Observation-based Magnetohydrodynamic Model of a Coronal Mass Ejection Save
- Fast Reconstruction of Solar Wind Magnetohydrodynamic Parameters at 0.1 au with Machine Learning Save
- Simulating the Ring-shaped Line-of-sight Flows in Prominence-cavity Systems Save
- A Unified Model of Solar Prominence Formation with Self-consistent Heating Save
- High-resolution Observations of a Flare Associated with a Partial Filament Eruption on 2023 April 21 Save
- Responses of a Coronal Hole to a Fast Flare-driven Coronal Wave Save