Two‐dimensional structure of the solar wind near the Sun
Two‐dimensional structure of the solar wind near the Sun
复制标题
太阳附近太阳风的二维结构
DOI：
10.1029/gl014i005p00487
复制
发表时间：
1987
影响因子：
5.2
通讯作者：
T. Ogino
中科院分区：
文献类型：
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作者：
H. Washimi;Yutaka Yoshino;T. Ogino
用MHD模拟方法分析了太阳附近太阳风的二维结构。在封闭区域和开放区域之间具有清晰边界的头盔-流光配置已被复制。由于薄片中的压力驱动电流，在光球处具有偶极配置的磁场被发现在距离太阳很远的地方表现为R−2。
The two-dimensional structure of the solar wind near the sun is analyzed by the method of MHD simulation. The helmet-streamer configuration with a sharp boundary between the closed and open field regions has been reproduced. Due to the pressure-driven current in the sheet, the magnetic field, which has a dipole configuration at the photosphere, is found to behave like R−2 at a large distance, R, from the sun.
影响因子：
--
作者：
T. Ogino
通讯作者：
T. Ogino