The distributions of. temperature T, density N and velocity V are given using the equations coupling the MHD waves with the coronal atmosphere.
本文利用MHD波与日冕大气耦合的磁流体动力学方程组，计算得到冕洞内的日冕大气的温度T、密度N和流速V的分布。
The later period ocean-atmosphere variation conforms to the second coupling field of the sea temperature and atmosphere.
后期海、气关键区变化与第二耦合场相符。
应用推荐