2.5D Magnetohydrodynamic Simulation of the Formation and Evolution of Plasmoids in Coronal Current Sheets

2.5D Magnetohydrodynamic Simulation of the Formation and Evolution of Plasmoids in Coronal Current Sheets

In the present paper, using MPI-AMRVAC , we perform a 2.5D numerical magnetohydrodynamic simulation of the dynamics and associated thermodynamical evolution of an initially force-free Harris current sheet subjected to an external velocity perturbation under the condition of uniform resistivity. The...

Full description

Bibliographic Details
Main Authors: Sripan Mondal, Abhishek K. Srivastava, David I. Pontin, Ding Yuan, Eric R. Priest
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar atmosphere
Solar corona
Magnetohydrodynamics
Magnetic fields
Solar magnetic reconnection
Online Access:https://doi.org/10.3847/1538-4357/ad2079

Internet

https://doi.org/10.3847/1538-4357/ad2079

Similar Items