对流层上层的斜压波、高空槽对天气的变化有重要的影响。
Baroclinic waves in upper? Troposphere, upper troughs and surface cyclones associated with wave packets are important systems for weather change and prediction.
利用理论结果的计算表明，对流层的湍动对流完全有可能激发足够的波能去补充日冕中等离子体对流和辐射造成的能量损失。
Evaluation results show that the turbulence in convection zone is capable of generating enough wave energy to supply coronal energy lose due to convection and radiation.
大气波导的影响是对流层电磁波传播研究的热点和难点问题之一。
Atmospheric duct is one of the hot-topics and difficult problems in the propagation of electromagnetic waves in troposphere.
模式在对流层成功地模拟了行星波的年际变化形势，而对平流层的模拟并不理想。
In the troposphere, the interannual variation is well simulated by AGCM, but in the stratosphere the simulation is not successful.
当然，这些增温并非是由臭氧损耗的辐射效应直接造成的，而是通过波-流相互作用以及平流层-对流层相互作用等动力学过程实现的。
The warming is not due to direct radiative effect of ozone depletion, instead, it is throughout dynamic processes, such as wave-mean flow and stratosphere-troposphere interactions.
这与对流层中激发的行星尺度波在冬季易于垂直向上传播的理论是定性上一致的。
Theory of vertical propagation of planetary stationary waves was used to explain the observations.
这就证实了一些人认为的对流层机械波并不是一个对色球和日冕的有效加热机制的说法。
This confirms the idea that the mechanical waves generated from the convection zone are not very effective in heating the chromosphere and corona.
这就证实了一些人认为的对流层机械波并不是一个对色球和日冕的有效加热机制的说法。
This confirms the idea that the mechanical waves generated from the convection zone are not very effective in heating the chromosphere and corona.
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