Gang Li

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    A[Gang Li]
    AC["Associated Concepts (25)"]
    AW["Authored Works (17)"]
    CA["Linked Co-Authors (28)"]
    CI["Linked Collaborating Institutions (26)"]
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    click AW "#authored-works"
    click CA "#co-authors"
    click CI "#collaborating-institutions"

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ORCiD

https://orcid.org/0000-0003-4695-8866

OpenAlex ID

https://openalex.org/A5081233545 (API record)

Associated Concepts [?]

• Physics
• Quantum mechanics
• Nuclear physics
• Magnetic field
• Plasma
• Solar wind
• Astrophysics
• Astronomy
• Coronal mass ejection
• Electron
• Computational physics
• Classical mechanics
• Engineering
• Acceleration
• Aerospace engineering
• Medicine
• Solar energetic particles
• Particle acceleration
• Thermodynamics
• Radiology
• Internal medicine
• Shock (circulatory)
• Geology
• Biology
• Mechanics

Authored Works

sorted by decreasing year, and then by display-name

• The Role of Intermittency in Anisotropic Plasma Velocity Distributions
• On the seed population of solar energetic particles in the inner heliosphere
• Interplanetary Mesoscale Observatory (InterMeso): A mission to untangle dynamic mesoscale structures throughout the heliosphere
• ESP Heavy Ion Property Variations in Solar Cycles 23 and 24
• Constrain the Diffusive Transport of SEPs for Simulations with PSP Observations in the Inner Heliosphere.
• The meandering nature of solar Wind magnetic field and constraining it using multiple spacecraft observation
• Stochastic Parker Spirals in the Solar Wind: Role of the Radial Field Fluctuations and Switchbacks
• Investigating the Relationship Between the Solar Wind Turbulence Spectral Break at Dissipation Scales with Upstream Spectral Bumps near Planetary Bow Shocks
• Extreme Energetic Particle Events by Superflare Associated CMEs from Planet Hosting Stars
• Dependence of Energetic Storm Particle Heavy Ion Peak Intensities and Spectra on CME Source Longitude and Speed
• Constraining the underlying acceleration mechanism from various observational features in Large Solar Energetic Particle Events
• Particle acceleration and transport at a 2D CME-driven shock using the HAFv3 and PATH Code
• Modeling the transport of protons and heavy ions in SEP events
• Pre-existing turbulence and large gradual SEP events
• FLAREs, CMEs and Stereo Mission
• Acceleration and transport of heavy ions at CME-driven shocks
• On Modeling the April 21, 2002 SEP event

Linked Co-Authors

• B. J. Anderson
• Bennett A. Maruca
• C. M. S. Cohen
• Charles W. Smith
• D. Lario
• D. Malaspina
• Daniel Verscharen
• Frederic Effenberger
• G. C. Ho
• G. P. Zank
• J. M. Raines
• Joseph E. Borovsky
• L. K. Jian
• M. I. Desai
• Meng Jin
• Nicolas Wijsen
• Noé Lugaz
• Parisa Mostafavi
• R. C. Allen
• R. Chhiber
• R. W. Ebert
• Rachael Filwett
• Robert F. Wimmer‐Schweingruber
• S. K. Vines
• S. Livi
• S. T. Lepri
• Stefaan Poedts
• Zheyi Ding

Linked Collaborating Institutions

• Aerospace Corporation, California
• Bay Area Environmental Research Institute, California
• California Institute of Technology, Division of Physics, Mathematics and Astronomy
• Christian Albrechts University of Kiel, Germany
• Goddard Space Flight Center, Astrophysics Division
• Johns Hopkins University, Applied Physics Laboratory
• Katholieke University of Leuven, Belgium
• NASA Goddard Space Flight Center, Maryland
• SETI Institute, California
• Saint Andrews University, School of Physics and Astronomy
• Southwest Research Institute, Texas
• University College London, UK
• University of Alabama, Huntsville
• University of Alabama, Huntsville, Department of Physics
• University of Applied Sciences Northwestern Switzerland
• University of California, Berkeley, Space Sciences Laboratory
• University of California, Riverside, Department of Earth Sciences
• University of Central Lancashire, UK
• University of Colorado, Boulder
• University of Delaware
• University of Glasgow, UK
• University of Iowa
• University of Maryland, Department of Physics
• University of Michigan
• University of New Hampshire
• University of Texas, San Antonio

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