EGU25-3941, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-3941
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 29 Apr, 10:45–12:30 (CEST), Display time Tuesday, 29 Apr, 08:30–12:30
 
Hall X4, X4.62
MHD simulations of linear and nonlinear resistive tearing-mode instability in Harris sheet equilibrium
Chun-Kai Chang1 and Lin-Ni Hau1,2
Chun-Kai Chang and Lin-Ni Hau
  • 1National Central University, Department of Space Science and Engineering, Taiwan (chunkai13@gmail.com)
  • 2National Central University, Department of Physics, Taiwan

The tearing mode instability may develop in Harris type current sheets with antiparallel magnetic field. In this study, we study the tearing mode instability in the Harris sheet equilibrium using two-dimensional, linear and nonlinear resistive magnetohydrodynamic (MHD) models with isotropic pressure. We calculate the linear growth rates and eigenmode structures based on the linear MHD model which are used as initial perturbations in the MHD simulations for the full evolution of nonlinear tearing mode instability. Our primary focus is on the effects of various background density profiles on the linear growth rate and nonlinear evolution and saturation of the tearing mode instability. Additionally, we examine the effects of thermodynamic conditions on the tearing mode instability.

How to cite: Chang, C.-K. and Hau, L.-N.: MHD simulations of linear and nonlinear resistive tearing-mode instability in Harris sheet equilibrium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3941, https://doi.org/10.5194/egusphere-egu25-3941, 2025.