相关实验视频
Updated: Jun 29, 2025

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
10.3K
概括
通过球体散射部分连贯光,表明极化和连贯性显著影响结果,导致脱极化和独特的极化奇点.
科学领域:
- 电磁理论 电磁理论
- 光学是什么?光学是什么?光学是什么?
- 散射理论是一种散射理论.
背景情况:
- 微散射描述了光与同质球体的相互作用.
- 光的极化和连贯性影响散射现象.
- 了解这些效应对于光学传感和成像至关重要.
研究的目的:
- 为了调查落灯的部分连贯性和偏振如何影响Mie散射.
- 分析斯托克斯参数和远场极化程度.
- 为了探索极化奇点和脱极化效应.
主要方法:
- 电磁波散射的理论分析.
- 用米散射理论应用于同质球体.
- 对散射场的斯托克斯参数和极化程度的计算.
主要成果:
- 远区域偏振和斯托克斯参数对发生束的连贯性和偏振非常敏感.
- 部分空间连贯性导致显著的去极化效应.
- 在分散场中观察到极化奇点的出现.
结论:
- 落下的光的连贯性和极化状态从根本上改变了Mie散射结果.
- 脱极化和极化奇点是部分连贯性产生的关键特征.
- 散射场的对称性质受到这些落射束特征的影响.
相关概念视频
Electric Field of a Non Uniformly Charged Sphere
1.5K
Gauss's law states that the electric flux through any closed surface equals the net charge enclosed within the surface. This law is beneficial for determining the expressions for the electric field for a particular charge distribution if the electric flux is known.
Consider a non-uniformly charged sphere, for which the density of charge depends only on the distance from a point in space and not on the direction. Such a sphere has a spherically symmetrical charge distribution. Here, the electric...
Consider a non-uniformly charged sphere, for which the density of charge depends only on the distance from a point in space and not on the direction. Such a sphere has a spherically symmetrical charge distribution. Here, the electric...
1.5K
Generating Electromagnetic Radiations
2.9K
The German physicist Heinrich Hertz (1857–1894) was the first to generate and detect certain types of electromagnetic waves in the laboratory. Starting in 1887, he performed a series of experiments that confirmed the existence of electromagnetic waves and verified that they travel at the speed of light. Hertz used an alternating-current RLC (resistor-inductor-capacitor) circuit that resonated at a known frequency and connected it to a loop of wire. High voltages induced across the gap in...
2.9K
Electromagnetic Waves in Matter
3.0K
Electromagnetic waves can travel in the vacuum as well as in matter. For example light, which is an electromagnetic wave, can travel through air, water, or glass.
Consider the electromagnetic wave passing through a dielectric medium. In such a case, Maxwell's equations get modified. In Ampere's law, ε0 , the dielectric permittivity of free space is replaced with ε, the permittivity of dielectric. Also, the vacuum permeability μ0 is replaced by the permeability of the...
Consider the electromagnetic wave passing through a dielectric medium. In such a case, Maxwell's equations get modified. In Ampere's law, ε0 , the dielectric permittivity of free space is replaced with ε, the permittivity of dielectric. Also, the vacuum permeability μ0 is replaced by the permeability of the...
3.0K
Electromagnetic Fields
2.1K
Electric fields generated by static charges, often referred to as electrostatic fields, are characteristically different from electric fields created by time-varying magnetic fields. While the former is a conservative field, implying that no net work is done on a test charge if it goes around in a complete loop in the field, the latter is, by definition, not a conservative field; net work is done, and it is proportional to the rate of change of magnetic flux.
However, the observation of...
However, the observation of...
2.1K
Gauss's Law: Spherical Symmetry
7.5K
A charge distribution has spherical symmetry if the density of charge depends only on the distance from a point in space and not on the direction. In other words, if the system is rotated, it doesn't look different. For instance, if a sphere of radius R is uniformly charged with charge density ρ0, then the distribution has spherical symmetry. On the other hand, if a sphere of radius R is charged so that the top half of the sphere has a uniform charge density ρ1 and the bottom half...
7.5K
The de Broglie Wavelength
25.9K
In the macroscopic world, objects that are large enough to be seen by the naked eye follow the rules of classical physics. A billiard ball moving on a table will behave like a particle; it will continue traveling in a straight line unless it collides with another ball, or it is acted on by some other force, such as friction. The ball has a well-defined position and velocity or well-defined momentum, p = mv, which is defined by mass m and velocity v at any given moment. This is the typical...
25.9K

