Jove
Visualize
联系我们
JoVE
x logofacebook logolinkedin logoyoutube logo
关于 JoVE
概览领导团队博客JoVE 帮助中心
作者
出版流程编辑委员会范围与政策同行评审常见问题投稿
图书馆员
用户评价订阅访问资源图书馆顾问委员会常见问题
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experiments存档
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教师资源中心教师网站
使用条款与条件
隐私政策
政策

相关概念视频

Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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...
Molecular Spectroscopy: Absorption and Emission01:14

Molecular Spectroscopy: Absorption and Emission

Molecules possess discrete energy levels called quantum states. Unlike atoms, which have simpler energy levels, molecules possess additional rotational and vibrational energy levels. Each energy level is separated by an energy gap, with the gaps between adjacent electronic, vibrational, and rotational levels varying significantly. The three types of energy levels in a diatomic molecule are shown in Figure 1.
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...
Mass Spectrum: Interpretation01:24

Mass Spectrum: Interpretation

An unknown compound can be established by identifying the molecular ion peak in the mass spectrum. The molecular ion peak is often weak or absent due to the predominance of fragmentation in high-energy electron beams. In such cases, a soft-energy electron beam can be used to scan the spectrum to enhance the intensity of the molecular ion peak. Additionally, chemical ionization, field ionization, and desorption ionization spectra are used to obtain a relatively intense molecular ion peak.To...

您也可能阅读

相关文章

通过共同作者、期刊和引用图与本文相关的文章。

排序
Same author

Blue carbon sinks in South Africa and the need for restoration to enhance carbon sequestration.

The Science of the total environment·2022
Same author

Barcoding of estuarine macrophytes and phylogenetic diversity of estuaries along the South African coastline.

Genome·2019
Same author

The outpatient total hip arthroplasty : a paradigm change.

The bone & joint journal·2018
Same author

Natural nutrient enrichment and algal responses in near pristine micro-estuaries and micro-outlets.

The Science of the total environment·2017
Same author

Distribution of phyllosilicates on the surface of Ceres.

Science (New York, N.Y.)·2016
Same author

Dawn arrives at Ceres: Exploration of a small, volatile-rich world.

Science (New York, N.Y.)·2016
Same journal

Erratum for the Research Article "Detecting supramolecular organic nanoparticles during heat wave".

Science (New York, N.Y.)·2026
Same journal

Local signals, systemic decline.

Science (New York, N.Y.)·2026
Same journal

The mechanics of liver regeneration.

Science (New York, N.Y.)·2026
Same journal

Computing in a memory with physics.

Science (New York, N.Y.)·2026
Same journal

Retraction.

Science (New York, N.Y.)·2026
Same journal

Making time.

Science (New York, N.Y.)·2026
查看所有相关文章

相关实验视频

Updated: Jun 24, 2026

Measuring Spatially- and Directionally-varying Light Scattering from Biological Material
11:57

Measuring Spatially- and Directionally-varying Light Scattering from Biological Material

Published on: May 20, 2013

小行星背心:光谱反射和组成影响.

T B McCord, J B Adams, T V Johnson

    Science (New York, N.Y.)
    |June 19, 1970
    PubMed
    概括
    此摘要是机器生成的。

    这项研究介绍了对小行星Vesta,Pallas和Ceres的第一个光谱反射度测量. 维斯塔呈现出独特的吸收带,这表明其表面成分类似于玄武岩 achondrites.

    更多相关视频

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures
    08:01

    Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures

    Published on: November 21, 2019

    相关实验视频

    Last Updated: Jun 24, 2026

    Measuring Spatially- and Directionally-varying Light Scattering from Biological Material
    11:57

    Measuring Spatially- and Directionally-varying Light Scattering from Biological Material

    Published on: May 20, 2013

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures
    08:01

    Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures

    Published on: November 21, 2019

    科学领域:

    • 行星科学 行星科学
    • 频谱学是一种光谱学.
    • 矿物学是什么?矿物学是什么?

    背景情况:

    • 小行星表面的组成为我们提供了关于太阳系早期的见解.
    • 以前的小行星光谱数据有限,特别是在0.30至1.10微米范围内.

    研究的目的:

    • 首次测量了小行星维斯塔,帕拉斯和塞雷斯的光谱反射率.
    • 识别特征性吸收带并将其与已知的矿物学成分进行比较.

    主要方法:

    • 在紫外线到近红外光谱 (0.30至1.10微米) 中进行了光谱反射度测量.
    • 小行星光谱与石和阿波罗月球样本的实验室测量进行比较.

    主要成果:

    • 维斯塔在0.9微米处显示出强烈的吸收带,在0.5-0.6微米处显示出较弱的吸收带,在紫外线中反射率降低.
    • 帕拉斯和可能的塞雷斯缺乏突出的0.9微米吸收带.
    • 维斯塔的吸收带是任何固体太阳系物体中观察到的最强的吸收带,归因于 pyroxene 中的铁.

    结论:

    • 维斯塔的表面构成与特定的玄武岩石石石非常相似.
    • 维斯塔的独特光谱特征提供了关于其地质历史和起源的重要线索.
    • 比较光谱学是了解小行星矿物学的强大工具.