LfV

Propagation of Alfven waves in multi-layer solar atmosphere model

多层太阳大气模式中Alfvén波的传播

And the change of local density in belt has little effect on both RFV and LFV.

径向力及侧向力基本不受带束层局部密度变化的影响。

A new model for auroral particle acceleration produced by shear Alfven waves is put forward.

提出一个剪切Alfven波加速极光粒子的新模式。

Many kinds of popular specific models, like supersymmetry, technicolor, and little Higgs models, indicate the possibility of large LFV.

很多新物理模型如超对称理论，人工色理论，小Higgs理论等都预言了LFV过程的存在。

After above analytical theories, we combine the two part of work into an integrated model of coronal heating. In this thesis, we investigate the role of Alfven wave in the coronal heating process.

在完成了本论文的理论工作后，我们将这两个部分的理论结合起来，就得到了一个相对完整的日冕加热模型，包含了Alfven波的波源和耗散机制。

Interaction of the Alfven waves and the slow mode shocks

Alfvèn波与慢激波的相互作用

The model is used to analyze the effect of the gage, lateral deviation and local density in belt on the radial force variation ( RFV) and lateral force variation ( LFV).

分析在静态条件下子午线轮胎带束层厚度变化、左右偏移量以及局部密度变化对轮胎径向力波动和侧向力波动的影响。

Solitary kinetic Alfven waves in inertial limit region with low-β plasma

惯性区低-β等离子体中的动力学Alfvén孤波