MHD simulation data for manuscript "A new tool for understanding solar wind-Venus interaction: 3D multi-fluid MHD model"

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.

本数据集对应学术论文《用于理解太阳风与金星相互作用的新工具：三维多流体磁流体力学（Magnetohydrodynamics, MHD）模型》的磁流体力学模拟工作，包含基于该三维多流体磁流体力学模型生成的模拟数据。1）三个压缩文件分别对应论文中的三组模拟工况：太阳活动极大期、太阳活动极小期以及金星快车（VEX）对照工况；2）数据中的MATLAB格式数据文件（.mat）内，“eq”与“xz”分别代表X-Y平面与X-Z平面的数据变量；变量名后缀的数字代表离子种类：无数字时对应整体等离子体流体，1为氢离子H+，2为氧离子O+，3为O₂+离子，4为CO₂+离子；(Vx, Vy, Vz)为等离子体速度的三个分量，(Bx, By, Bz)为磁场的三个分量，P代表热压强，D代表密度。