Chen Shi
Department of Physics
Assistant Professor

Research Areas: Space Plasma Physics

Office: Leach Science Center 2130

Address: 380 Duncan Drive
Auburn, AL 36849

Phone: (334) 844-4264

Email: chenshi@auburn.edu

Website


Education
University of California, Los Angeles; Ph.D., Geophysics and Space Physics
2020
Peking University; B.S. Space Science and Technology
2015


Professional Employment
Assistant Professor, Department of Physics, Auburn University
2025-present
Assistant Researcher, Department of Earth, Planetary, and Space Sciences, UCLA
2023-2025
Postdoctoral Researcher, Department of Earth, Planetary, and Space Sciences, UCLA
2020-2023


Honors and Awards
NASA Group Achievement Award to Parker Solar Probe Team
2023
Physics of Plasmas Early Career Collection
2022
Vincenzo Ferraro Award for Best PhD thesis
2021


Research and Teaching Interests

My research focuses on space plasma physics and solar physics, with particular emphasis on solar wind turbulence, magnetic reconnection, and the origin of solar wind. My recent work focuses on three areas: (1) analyzing satellite observations from missions such as Parker Solar Probe, WIND, and MMS to investigate dynamic processes in the solar wind; (2) developing high-performance magnetohydrodynamic (MHD) simulation codes to study plasma turbulence, magnetic reconnection, and solar wind dynamics; and (3) advancing fundamental theories on current sheet instabilities, solar wind generation, and MHD turbulence. In addition, I am interested in applying machine learning techniques to predict space weather from remote-sensing observations of the Sun.



Selected Publications

  1. Evolution of Magnetohydrodynamic turbulence in the expanding solar wind: residual energy and intermittency, Chen Shi, Nikos Sioulas, Zesen Huang, et al., 2025, The Astrophysical Journal,https://iopscience.iop.org/article/10.3847/1538-4357/ad9f38/meta
  2. LAPS: An MPI-parallelized 3D pseudo-spectral Hall-MHD simulation code incorporating the expanding box model, Chen Shi, Anna Tenerani, Antonio Franco Rappazzo, Marco Velli, 2024, Frontiers in Astronomy and Space Sciences,https://www.frontiersin.org/journals/astronomy-and-space-sciences/articles/10.3389/fspas.2024.1412905/full
  3. Analytic model and MHD simulations of three-dimensional magnetic switchbacks, Chen Shi, Marco Velli, Gabor Toth, et al., 2024, The Astrophysical Journal Letters,https://iopscience.iop.org/article/10.3847/2041-8213/ad335a
  4. Proton and electron temperatures in the solar wind and their correlations with the solar wind speed, Chen Shi, Marco Velli, Roberto Lionello, et al., 2023, The Astrophysical Journal,https://iopscience.iop.org/article/10.3847/1538-4357/acb341
  5. Acceleration of polytropic solar wind: Parker Solar Probe observation and one-dimensional model, Chen Shi, Marco Velli, Stuart Bale, et al., 2022, Physics of Plasma,https://aip.scitation.org/doi/full/10.1063/5.0124703
  6. Patches of Magnetic Switchbacks and Their Origins, Chen Shi, Olga Panasenco, Marco Velli, et al., 2022, The Astrophysical Journal,https://iopscience.iop.org/article/10.3847/1538-4357/ac7c11
  7. Instabilities in a current sheet with plasma jet, Chen Shi, 2022, Journal of Plasma Physics,https://www.doi.org/10.1017/S0022377822000575
  8. Influence of the heliospheric current sheet on the evolution of solar wind turbulence, Chen Shi, Marco Velli, Anna Tenerani, et al., 2022, The Astrophysical Journal,https://iopscience.iop.org/article/10.3847/1538-4357/ac558b
  9. Alfvénic versus non-Alfvénic turbulence in the inner heliosphere as observed by Parker Solar Probe, Chen Shi, Marco Velli, Olga Panasenco, et al., 2021, Astronomy and Astrophysics,https://www.aanda.org/articles/aa/abs/2021/06/aa39818-20/aa39818-20.html
  10. Oblique Tearing Mode Instability: Guide Field and Hall Effect, Chen Shi, Marco Velli, Fulvia Pucci, Anna Tenerani, Maria Elena Innocenti, 2020, The Astrophysical Journal,https://doi.org/10.3847/1538-4357/abb6fa






Last updated: 09/10/2025