偏振角

The polarization state of reflected light of water and the relationship of incidence angle and degree of water polarization were deduced.

理论上证明了以非布儒斯特角入射时偏振消除太阳耀光的可能性，计算了从各个角度入射到纯净水体表面太阳耀光剥离的程度，实验验证了结论。

In addition, it also can be applied to the measurement of the cell thickness and twist angle of single polarizer reflected liquid crystal cell.

另外，此方法也可以应用到单偏振片反射式液晶盒盒厚和扭曲角的测量。

The obtained mass spectra of methyl iodide was different from others when coulomb explosion happened. We didn...

分析了碳和碘的各价离子的角分布，比较了激光在水平和垂直偏振时各种离子强度的变化。

The experimental results indicated that the light-induced MR molecular reorientation effect, the so-called twisted angle, caused by the adsorbed MR, decreased with increasing ellipticity of the elliptically polarized green light. Notably, zero pre-tilt angle of LC alignment was achieved in this experiment.

再利用不同光强度的圆偏振绿光雷射激发MR，观察并探讨MR吸附的结果，实验结果显示在圆偏振光各方向能量均等的情况之下，不会有扭转角跟倾角产生，且在吸附面上有不均匀的成核现象发生。

By computer simulation, we analyze the influence of the incidence plane, incidence angle and thickness of air gap on transmittance, and the dependence of the transmittance on wavelength is given in the spectral range which is required by the instrument system using Sellmeier dispersion equation. The transmittance of Grand-Taylor prism is tested in experiment, and the results are in good agreement with the theoretical results, so the correctness of the theory is verified.

论述了自行设计研制的偏振干涉成像光谱仪的工作原理，分析了其核心部件格兰-泰勒棱镜的分光机理；运用光线追迹方法，推导出了格兰-泰勒棱镜全视场角透过率计算公式；通过计算机模拟分析了入射面、入射角和空气隙厚度对该棱镜透过率的影响，并利用方解石Sellmeier色散方程，给出了该棱镜在仪器系统要求的光谱范围内透过率与波长的关系曲线；实验测试结果与理论计算公式相符，验证了理论公式的正确性。

The uniformity of the beam polarization plane of rotation angles are be tter than ±3°.

测量结果表明：在法拉第旋光器的有效通光面内，光偏振面旋转角的径向分布均匀性优于±3°。

The relationship between the thermal emission polarization and viewing angles in metal targets is studied by using this thermal imaging polarimeter.

利用该系统，研究了金属板热红外偏振度和观测角之间的关系。

In this paper, assuming that pulsar magnetic field is rotating vacuum dipole, which is derived from retarded potential, the PA curve is reinvestigated.

文章采用从推迟势导出的旋转真空磁偶极场，研究了在脉冲星磁场为旋转磁偶极场位形下的线偏振位置角曲线。

For larger inclination and impact angles, or inner field lines close to magnetic pole, the rotating dipole PA curves show more significant distortion comparing with the results of rotating vector model.

相比旋转矢量模型的结果，旋转磁偶极场偏振位置角曲线在大磁倾角、碰撞角，或靠近磁轴的内层磁力线上有显著的变形。

When scattering angle is in the range from 0.025π to 0.997 π radian, the scattering phase function varies obviously.

同时比较了偏振状态下多粒子和单粒子散射相位函数随散射角和极化角的分布。

The split between the two groups can hardly be papered over.

这两个团体间的分歧难以掩饰。

This approach not only encourages a greater number of responses, but minimizes the likelihood of stale groupthink.

这种做法不仅鼓励了更多的反应，而且减少跟风的可能性。