Particle Acceleration and Transport in Solar Flares

Modeling Electron Acceleration and Transport in the Early Impulsive Phase of the 2017 September 10th Solar Flare. Two cases with different Lundquist numbers are shown here. (Li et al., 2022)

Solar flares are among the most remarkable phenomenon of energy release and particle acceleration in our solar system. A large amount of magnetic energy in the solar corona can be released and converted into non-thermal particles within a few minutes. These high-energy particles produce impulsive non-thermal emissions that are commonly observed, and they can be released into interplanetary space and produce impulsive solar energetic particle events. The non-thermal emissions provide critical diagnostics of the non-thermal particles. Modeling particle acceleration during solar flares is particularly challenging due to the enormous scale separation (kinetic scales < m and global scales >1E8 m) in solar flares.

A framework to bridge simulations and observations.

We have been building a framework for studying particle acceleration during solar flares. Besides the kinetic studies, we are actively working on

  • building a numerical model solving the energetic particle transport equations
  • studying electron acceleration in the whole flare region (e.g., reconnection and termination shocks)
  • producing hard X-ray and microwave emissions from the MHD simulations and the energetic electron maps generated from the model and comparing them with the flare observations
  • studying the large-scale transport of energetic electrons in the whole solar eruption regions (SEPs project)

Publications

2024

  1. ApJ
    Compression Acceleration of Protons and Heavier Ions at the Heliospheric Current Sheet
    Giulia Murtas, Xiaocan Li, and Fan Guo
    The Astrophysical Journal, Oct 2024
  2. ApJ
    Energetic Electrons Accelerated and Trapped in a Magnetic Bottle above a Solar Flare Arcade
    Bin Chen, Xiangliang Kong, Sijie Yu, and 6 more authors
    The Astrophysical Journal, Aug 2024
  3. arXiv
    A New Computational Method for Energetic Particle Acceleration and Transport with its Feedback
    Jeongbhin Seo, Fan Guo, Xiaocan Li, and 1 more author
    arXiv e-prints, Apr 2024

2023

  1. Whitepaper
    Particle acceleration in solar flares with imaging-spectroscopy in soft X-rays
    Mitsuo Oka, Amir Caspi, Bin Chen, and 15 more authors
    In Bulletin of the American Astronomical Society, Jul 2023
  2. Whitepaper
    Quantifying Energy Release in Solar Flares and Solar Eruptive Events: New Frontiers with a Next-Generation Solar Radio Facility
    Bin Chen, Dale Gary, Sijie Yu, and 38 more authors
    In Bulletin of the American Astronomical Society, Jul 2023
  3. Whitepaper
    Advancing Theory and Modeling Efforts in Heliophysics
    Fan Guo, Spiro Antiochos, Paul Cassak, and 15 more authors
    In Bulletin of the American Astronomical Society, Jul 2023

2022

  1. ApJL
    Numerical Modeling of Energetic Electron Acceleration, Transport, and Emission in Solar Flares: Connecting Loop-top and Footpoint Hard X-Ray Sources
    Xiangliang Kong, Bin Chen, Fan Guo, and 8 more authors
    The Astrophysical Journal Letters, Dec 2022
  2. ApJ
    A Model of Double Coronal Hard X-Ray Sources in Solar Flares
    Xiangliang Kong, Jing Ye, Bin Chen, and 6 more authors
    The Astrophysical Journal, Jul 2022
  3. ApJ
    Modeling Electron Acceleration and Transport in the Early Impulsive Phase of the 2017 September 10th Solar Flare
    Xiaocan Li, Fan Guo, Bin Chen, and 2 more authors
    The Astrophysical Journal, Jun 2022

2021

  1. PhPl
    The relation between the energy conversion rate and reconnection rate in Petschek-type reconnection—Implications for solar flares
    Matthew Goodbred, Yi-Hsin Liu, Bin Chen, and 1 more author
    Physics of Plasmas, Aug 2021

2018

  1. ApJ
    Large-scale Compression Acceleration during Magnetic Reconnection in a Low-\ensuremathβ Plasma
    Xiaocan Li, Fan Guo, Hui Li, and 1 more author
    The Astrophysical Journal, Oct 2018

2014

  1. ASR
    Energization of charged particle in a time-dependent chaotic magnetic field with an implication of the production of seed particles in solar energetic particle events
    Xiaocan Li, Brahmananda Dasgupta, and Gang Li
    Advances in Space Research, Apr 2014