行星际介质
- 网络interplanetary medium
行星际介质-
应用电子计算机计算了太阳宇宙线在均匀并无限的行星际介质中传播的各向异性扩散对流方程的量纲分析解。
Computer calculations have been made on the dimensional solution to the anisotropic diffusion convection equation for solar cosmic rays propagating in an uniform and unbounded interplanetary medium .
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电离层与日一地系统的其它区域，包括太阳、行星际介质、磁层、热层和中层之间存在着强烈地耦合相互作用。
The ionosphere is strongly coupled with the other regions in the solar-terrestrial system , including the sun , the interplanetary medium , the magnetosphere , the thermosphere , and the mesosphere .