Yi‐Hsin Liu
- ORCiD
- https://orcid.org/0000-0001-5880-2645
- OpenAlex ID
- https://openalex.org/A5052691102 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Nuclear physics
- Magnetic field
- Plasma
- Magnetic reconnection
- Mathematics
- Thermodynamics
- Chemistry
- Mechanics
- Classical mechanics
- Engineering
- Geology
- Computer science
- Computational physics
- Biology
- Electron
- Geography
- Organic chemistry
Authored Works
sorted by decreasing year, and then by display-name
- Three-dimensional magnetic reconnection spreading using particle-in-cell (PIC) simulations
- Revisiting the Electron Diffusion Region in Asymmetric Guide-Field Reconnection
- Reconnection Signatures within the Kelvin-Helmholtz Vortex-Induced Lower-Hybrid Waves at Earth's Magnetopause
- On the Effect of Driving Turbulence on Magnetic Reconnection: A Particle-In-Cell Simulation Study
- Multi-Scale and Cross-Process Character of the Kelvin-Helmholtz Instability during Southward Interplanetary Magnetic Field Conditions
- Kinetic Origin of Bulk Energy Conversion in the Electron Diffusion Region of Magnetopause Reconnection: MMS Observations and PIC Simulations
- Extended active magnetic reconnection X-lines in three-dimensional kinetic turbulence
- Three-dimensional Turbulent Magnetic Reconnection and Its Particle Energization
- The relation between the energy conversion rate and reconnection rate in Petschek-type reconnectionImplications for solar flares
- The acceleration of charged particles in nonrelativistic magnetic reconnection
- The Azimuthal Extension of Reconnection x-line in the Magnetotail Geometry
- Multi-Scale Observations of the Magnetopause Kelvin-Helmholtz Waves During Southward IMF
- Magnetic reconnection for low-density inflow conditions
- Identifying active magnetic reconnection in simulations and in situ observations of plasma turbulence using magnetic flux transport
- Exploring Kelvin Helmholtz instability in the magnetopause and relativistic regime
- Evidence for extended active magnetic reconnection X-lines in three-dimensional plasma turbulence
- Connecting X-line heating efficiency to the reconnection rate problem
Linked Co-Authors
- A. S. Afshari
- A. S. Sharma
- Adriana Settino
- B. L. Giles
- C. T. Russell
- Cecilia Norgren
- Chen Bin
- D. J. Gershman
- D. Payne
- E. V. Panov
- F. D. Wilder
- Ferdinand Plaschke
- Harsha Gurram
- Hiroshi Hasegawa
- J. C. Holmes
- J. Dorelli
- J. E. Stawarz
- J. L. Burch
- J. R. Shuster
- J. Webster
- Jonathan Ng
- K. A. Blasl
- K. J. Genestreti
- L. A. Avanov
- Li‐Jen Chen
- M. Hesse
- M. R. Argall
- M. Volwerk
- Martin Hosner
- Naoki Bessho
- Owen Roberts
- P. A. Cassak
- Patrick Kilian
- R. B. Torbert
- R. E. Denton
- R. Nakamura
- S. Wang
- Senbei Du
- Susanne Flø Spinnangr
- Tak Chu Li
- Yi Qi
- Z. Vörös
Linked Collaborating Institutions
- Austrian Academy of Sciences
- Austrian Institute of Space Science Research
- Catholic University, Washington DC
- Dartmouth College, New Hampshire
- Imperial College, London
- JAXA Japan Aerospace Exploration Agency
- Karl Franzens University of Graz, Austria
- Los Alamos National Laboratory, New Mexico
- Massachusetts Institute of Technology
- NASA Ames Research Center
- NASA Goddard Space Flight Center, Maryland
- New Jersey Institute of Technology
- Princeton University, New Jersey
- Southwest Research Institute, Texas
- Technical University of Braunschweig, Germany
- University of Bergen, Norway
- University of California, Los Angeles
- University of Colorado, Boulder
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Iowa
- University of Maryland, College Park
- University of New Hampshire
- University of Texas, Arlington
- University of Wisconsin, Madison
- West Virginia University
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