Solar Wind In Situ Parameters Propagated from the Earth to Jupiter
收藏DataCite Commons2026-05-05 更新2024-07-13 收录
下载链接：
https://cdpp.sedoo.fr/cdpp-products?uuid=1068bfe1-bbae-45a4-aa4a-e552f2a2b38a
下载链接
链接失效反馈官方服务：
资源简介：
These data sets are the simulation outputs of solar wind parameters observed near the Earth (from several inputs) and propagated to Jupiter 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
提供机构：
OVGSO
创建时间：
2021-11-26
