从而求得普遍的大气动力学方程。
Then general dynamic equations of the atmosphere are obtained.
第一节叙述太阳大气动力学过程的光谱特征及其诊断原理。
The first section describes the spectral features of the dynamical processes in the solar atmosphere and the principles of their diagnostics.
探讨了大气的熵概念，研究了熵理论在大气动力学中的应用。
The paper presents an approach to a concept of atmospheric entropy, and discussed the application of the entropy theory in atmospheric dynamics.
色球压缩区是耀斑大气动力学过程的一个基本特征，是产生色球谱线红不对称性的基础。
The chromospheric condensation is a basic property of the flare dynamical process and the cause of the red asymmetry of chromospheric lines.
阿承诺学校教师，教授Fovell教授，包括大气动力学，热力学，主题课程，天气预测和预报，和云动力。
A committed classroom teacher, Professor Fovell teaches courses on topics including atmospheric dynamics, thermodynamics, weather prediction and forecasting, and cloud dynamics.
具体课程包括：大气化学和物理学，大气动力学，气候和气候变化，气候模拟，气象预报，气候模拟和数学理论。
Specific subjects include: atmospheric chemistry and physics, atmospheric dynamics, climatology and climate change, weather simulation, weather forecasting, climate modeling and mathematical theory;
在大气动力学领域，主要介绍了非绝热波和大气低频动力学、湍流的频散效应和大气非线性波动等方向的研究进展。
First, in the field of atmospheric dynamics the developments in dynamics of diabatic waves and low frequency waves, the dispersive effects of turbulence and nonlinear atmospheric waves are reviewed.
采用理想磁流体力学方程组(MHD)作为太阳大气动力学过程的控制方程组，定性数值模拟日冕物质抛射(CME)现象。
The ideal Magnetohydrodynamic equations (MHD), the governing equations of the solar atmosphere dynamical process, are taken to numerically simulate Coronal Mass Ejection (CME) phenomena.
采用理想磁流体力学方程组(MHD)作为太阳大气动力学过程的控制方程组，定性数值模拟日冕物质抛射(CME)现象。
The ideal Magnetohydrodynamic equations (MHD), the governing equations of the solar atmosphere dynamical process, are taken to numerically simulate Coronal Mass Ejection (CME) phenomena.
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