5:15 PM - 6:30 PM
[PEM05-P02] Radiation Magnetohydrodynamic Simulations of Solar Chromospheric Jets
Keywords:Plasma Jets, Solar Chromosphere, Magnetohydrodynamics
In this presentation, we will show our recent results of the numerical simulations by our radiation magnetohydrodynamic code for the comprehensive modeling of the solar atmosphere. The code contains the gravity, the radiative cooling, the thermal conduction, and the thermodynamic effect of partial ionization. The numerical domain includes the convective unstable layer that drives the motion in the simulated chromosphere. Many chromospheric jets with the maximum height greater than 6 Mm are reproduced in the simulations. The typical formation process and the statistical behavior of simulated jets are investigated. We will discuss the comparison between the two-dimensional and three-dimensional simulations and the relation to the observational signatures.