Data of "Thermodynamic Modulation of the Venusian Ionosphere and Induced Magnetosphere by Neutral Atmospheric Temperature"

This dataset comprises the simulation data used in the paper titled “Thermodynamic Modulation of the Venusian Ionosphere and Induced Magnetosphere by Neutral Atmospheric Temperature”. The data files are described as follows: “Case1_xz_0150.mat”: Simulation results for Case 1 at t=15.0 min. This file includes the three components of the magnetic field and electric current in the x-z plane, as well as the thermal pressure, density, and velocity for various particle species. These data are used to generate Figures 2, 3, 4, 5, and 7 in the manuscript. “Case2_xz_0150.mat”: Simulation results for Case 2 at t=15.0 min. These data are used to generate Figures 2, 3, 4, 5, and 7 in the manuscript. “Case3_xz_0150.mat”: Simulation results for Case 3 1 at t=15.0 min. These data are used to generate Figure 7 in the manuscript. “Case4_xz_0150.mat”: Simulation results for Case 4 2 at t=15.0 min. These data are used to generate Figure 7 in the manuscript. Folder “data_KH”: Contains simulation results for Case 2 at t=15.9,16.0,16.1, and 16.2 min, illustrating an example of a Kelvin-Helmholtz (KH) vortex structure. It also includes the power spectra derived from a Fast Fourier Transform (FFT) of the By component in the x-z plane for both Case 1 and Case 2 over the time interval from 15.0 to 30.0 min, used for calculating the integrated power of the KH instability. These data are used to generate Figure 5 in the manuscript. Folder “data_Oesp”: Contains calculations of the global O+ escape rate for Case 1 and Case 2 over the time interval from 0.0 to 20.0 min. These data are used to generate Figure 6 in the manuscript.