2026-10-13T00:24:47Z https://www.scidb.cn/oai

10.57760/sciencedb.o00009.00353 2022-11-14T14:09:28Z

2022-11-14 MHD simulation data for manuscript "A new tool for understanding solar wind-Venus interaction: 3D multi-fluid MHD model" doi:10.57760/sciencedb.o00009.00353 en Data from the MHD simulation for manuscript " A new tool for understanding solar wind-Venus interaction: 3D multi-fluid MHD model".This dataset includes simulation data based on a 3D multifluid MHD simulation model. 1) Three compressed files refer to the three simulation cases in the manuscript: solar maximum, solar minimum, and VEX-comparison. 2) For the mat file in the data, “eq” and “xz” denote the X-Y plane and X-Z plane, respectively. The numbers represent the ion species (no number->bulk; 1->H+; 2->O+; 3->O2+; 4->CO2+). (Vx, Vy, Vz) are the three components of plasma velocity. (Bx, By, Bz) are the three components of magnetic field. P is the thermal pressure and D is the density. Unmagnetized planets; Magnetohydrodynamics; Multifluid MHD model; Solar wind-Venus Tong Dang PUBLIC https://creativecommons.org/licenses/by/4.0/ dataset Science Data Bank