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相关概念视频

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...
Mutations01:35

Mutations

Mutations are changes in the sequence of DNA. These changes can occur spontaneously or they can be induced by exposure to environmental factors. Mutations can be characterized in a number of different ways: whether and how they alter the amino acid sequence of the protein, whether they occur over a small or large area of DNA, and whether they occur in somatic cells or germline cells.
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Radiation: Applications01:17

Radiation: Applications

The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
Absorption of Radiation01:05

Absorption of Radiation

The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
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...

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相关实验视频

Updated: Jul 12, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

月球样本中的太阳辐射效应.

B W Hapke, A J Cohen, W A Cassidy

    Science (New York, N.Y.)
    |January 30, 1970
    PubMed
    概括

    粉碎的阿波罗11号水晶岩石显示了与月球土壤不同的光学特性. 辐射和加热改变了这些特性,导致土壤白度和光谱与预期值的显著偏差.

    科学领域:

    • 地质地质地质地质地质地
    • 行星科学 行星科学
    • 材料科学 材料科学 材料科学

    背景情况:

    • 月球正规岩的光学特性对于理解表面过程至关重要.
    • 阿波罗11号的样本提供了关于月球地质和物质进化的见解.

    研究的目的:

    • 为了研究破碎的阿波罗11号水晶岩石的光学特性.
    • 为了确定环境因素对这些光学属性的影响.
    • 为了比较岩石和土壤的光学特征.

    主要方法:

    • 分析结晶岩石粉末的光学特性 (白度,光谱).
    • 样品暴露于紫外线和X射线辐射.
    • 热处理 (加热) 的应用.
    • 与自然的月球土壤特性进行比较.

    主要成果:

    • 与月球土壤相比,粉碎的晶体岩石具有独特的光学特性.
    • 辐射和加热显著改变了样品的光学特征.
    • 观察到的处理土壤的白度和光谱值明显偏离了预测.

    结论:

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    Scattering And Absorption of Light in Planetary Regoliths
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  • 辐射和热量等环境因素可以改变月球岩石的光学特性.
  • 这些修改解释了预期和观察到的月球土壤光学行为之间的差异.
  • 了解这些变化对于准确的遥感和表面解释至关重要.