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相关概念视频

Momentum And Radiation Pressure01:20

Momentum And Radiation Pressure

An object absorbing an electromagnetic wave would experience a force in the direction of propagation of the wave. This force occurs because electromagnetic waves contain and transport momentum. The force accounts for the wave's radiation pressure exerted on the object. Maxwell's prediction was confirmed in 1903 by Nichols and Hull by precisely measuring radiation pressures with a torsion balance. The measuring instrument had mirrors suspended from a fiber kept inside a glass container. Nichols...
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Scanning Electron Microscopy01:07

Scanning Electron Microscopy

A scanning electron microscope (SEM) is used to study the surface features of a sample by using an electron beam that scans the sample surface in a two-dimensional manner. Typically, areas between ~1 centimeter to 5 micrometers in width can be imaged. SEM can be used to image bacteria, viruses, tissues as well as larger samples like insects. Conventional SEM gives a magnification ranging from 20X to 30,000X and spatial resolution of 50 to 100 nanometers.
Fundamental Principles
Accelerated...
Atomic Emission Spectroscopy: Interference01:30

Atomic Emission Spectroscopy: Interference

In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
Interference and Diffraction02:18

Interference and Diffraction

Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.
Interaction of EM Radiation with Matter: Spectroscopy01:12

Interaction of EM Radiation with Matter: Spectroscopy

Electromagnetic (EM) radiation can be considered an oscillating electric and magnetic field propagating through a medium that can interact with matter in its path. The electric field in the radiation can interact with electrical charges in the atoms or molecules in the matter. On the other hand, the magnetic field can interact with the magnetic field in the atomic nucleus. The study of the interaction between electromagnetic radiation and matter is termed spectroscopy. Spectroscopy is the study...

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相关实验视频

Updated: Jul 11, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

西彗星和彗星尘埃的散射功能.

E P Ney, K M Merrill

    Science (New York, N.Y.)
    |December 3, 1976
    PubMed
    概括

    研究人员使用红外观测研究了西彗星的尘埃特性. 尘埃颗粒很可能是1微米的介电粒,前向散射特性表明它们的尺寸和组成.

    科学领域:

    • 彗星科学 彗星科学
    • 尘埃物理 尘埃物理
    • 红外天文学 红外天文学

    背景情况:

    • 彗星尘埃在了解太阳系形成方面发挥着至关重要的作用.
    • 以前的研究已经描述了彗星尘埃的组成和尺寸分布.
    • 西彗星 (1975n) 提供了一个独特的机会来研究尘埃的特性.

    研究的目的:

    • 为了确定西彗星中的尘埃的散射相位函数.
    • 为了推断彗星尘埃颗粒的大小和组成.
    • 为了将尘埃行为与彗星碎片事件相关联.

    主要方法:

    • 在0.5至18微米的波长中对西彗星进行红外观测.
    • 来自彗星昏迷的散射光和热辐射的分析.
    • 基于观测数据的散射相函数的建模.

    主要成果:

    • 西彗星尘埃的散射相函数在向前方向强烈达到峰值.
    • 尘埃颗粒被确定为介电粒,半径约为1微米.
    • 昏迷的亮度突然增加与预测的彗星碎片化时间相关.

    结论:

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    • 西彗星中的彗星尘埃颗粒具有与1微米介电粒相一致的向前散射特性.
    • 观察到的亮度变化表明碎片事件影响了尘埃释放和昏迷特性.
    • 这项研究提高了我们对彗星尘埃动态和演变的理解.