Data simulated with the HLL generalizedd Riemann solver on steady-state coronal structures of CR2218
收藏科学数据银行2023-06-20 更新2026-04-23 收录
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资源简介：
This data shows the simulated radial speed, number density, and 2D magnetic field lines from 1Rs to 20Rs. The left column is from HLL-GRP model and the right column is from RK2 model. The figure also displays the helmet streamers stretched by the solar wind and the thin current sheets between different magnetic polarities. The typical structures of the solar wind during the solar minimum are presented by simulated results.
提供机构：
SIGMA Weather Group, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences; College of Earth and Planetary Sciences, University of Chinese Academy of Sciences; Mengqing Liu; Xiaojing Liu
创建时间：
2022-11-03
