Solar Wind In Situ Parameters Propagated from the Earth to Saturn

These data sets are the simulation outputs of solar wind parameters observed near the Earth (from several inputs) and propagated to Saturn using a 1-dimensional 2-component (radial and azimuthal) magnetohydrodynamic (MHD) model. The model code is based on the Coordinated Astronomical Numerical Software (CANS) available at http://www.astro.phys.s.chiba-u.ac.jp/netlab/pub/haifu-CANS-e.html. Model details, validation with observation data, and limitations are described in Tao et al. 2005, J. Geophys. Res., 110, A11208, https://doi.org/10.1029/2004JA010959

本数据集为基于多组输入的近地太阳风参数观测数据，经一维双分量（径向与方位角向）磁流体动力学（magnetohydrodynamic, MHD）模型传播至土星后的模拟输出结果。该模型代码基于协调天文数值软件（Coordinated Astronomical Numerical Software, CANS）开发，相关软件可通过链接 http://www.astro.phys.s.chiba-u.ac.jp/netlab/pub/haifu-CANS-e.html 获取。该模型的细节、观测数据验证方法及局限性已在Tao等人2005年发表于《地球物理研究杂志（Journal of Geophysical Research, J. Geophys. Res.）》的论文中详述，论文卷号为110，文章编号为A11208，DOI为10.1029/2004JA010959。