Jove
Visualize
联系我们

相关概念视频

UV–Vis Spectrometers01:14

UV–Vis Spectrometers

The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for electronic transitions. As a result...
UV–Vis Spectrum01:30

UV–Vis Spectrum

When light passes through a substance, a portion of the light is absorbed while the remaining light is reflected or transmitted. If the molecule absorbs light between the wavelengths of 180–400 nm range, the UV spectrum is obtained, and if it absorbs light in the 400–780 nm wavelength range, the visible spectrum is obtained.     
The UV–Vis spectrum of a molecule is the plot of its absorbance versus wavelength. The plot is drawn by taking molar absorptivity (ε) or log ε on the y-axis (ordinate)...
UV–Vis Spectroscopy: Beer–Lambert Law01:09

UV–Vis Spectroscopy: Beer–Lambert Law

The Beer-Lambert law describes the relationship between absorbance and concentration, which combines the principles established by scientists Johann Heinrich Lambert and August Beer. Lambert's law states that when light passes through a medium, the loss in intensity is directly proportional to the original intensity and the path length of the light. Beer's law proposed that the transmittance of a solution remains constant if the product of concentration and path length is constant. The modern...
UV–Vis Spectroscopy: Molecular Electronic Transitions01:16

UV–Vis Spectroscopy: Molecular Electronic Transitions

In Ultraviolet–Visible (UV–Vis) spectroscopy, the absorption of electromagnetic radiation is used to probe the electronic structure of molecules. This technique provides insights into molecular electronic transitions, particularly the movement of electrons between different molecular orbitals. Radiation is absorbed if the energy of the electromagnetic radiation passing through the molecule is precisely equal to the energy difference between the excited and ground states. During this process,...
UV–Vis Spectroscopy of Conjugated Systems01:32

UV–Vis Spectroscopy of Conjugated Systems

Organic compounds with conjugated double bonds show strong absorption features in the UV–visible region of the electromagnetic spectrum attributed to π → π* electronic excitations. Generally, a UV–vis absorption spectrum is recorded as a plot of absorbance vs wavelength. The wavelength of maximum absorbance, which manifests as a peak in the absorption spectrum, is denoted as λmax.
One of the factors influencing λmax is the extent of conjugation in the...

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

Simple ultraviolet calibration source with reference spectra and its use with the Galileo orbiter ultraviolet spectrometer.

Applied optics·2010
Same author

Rocket-borne instrument with a high-resolution microchannel plate detector for planetary UV spectroscopy.

Applied optics·2010
Same author

Mariner 6 and 7 ultraviolet spectrometers.

Applied optics·2010
Same author

Planetary ultraviolet spectroscopy.

Applied optics·2010
Same author

Atmospheric scattering of the solar flux in the middle ultraviolet.

Applied optics·2010
Same author

Structure and vibrational dynamics of model compounds of the [FeFe]-hydrogenase enzyme system via ultrafast two-dimensional infrared spectroscopy.

The journal of physical chemistry. B·2008
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

相关实验视频

Updated: Jul 12, 2026

Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
09:53

Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation

Published on: October 30, 2012

马里纳9号紫外线光谱仪实验:初步结果

C A Barth, C W Hord, A I Stewart

    Science (New York, N.Y.)
    |January 21, 1972
    PubMed
    概括

    火星上的紫外线空气发光显示了与太阳活动相关的一氧化碳波段的变化. 始终观察到原子氧和排放,而火星尘埃显著影响大气反射率.

    科学领域:

    • 行星科学 行星科学
    • 大气物理学 大气物理学
    • 频谱学是一种光谱学.

    背景情况:

    • 了解火星大气的组成和动态对于行星探索至关重要.
    • 之前的任务提供了关于紫外线空气发光和大气散射的有限数据.

    研究的目的:

    • 测量火星的紫外线空气发光光谱.
    • 调查大气排放和反射率的变化.
    • 为了模拟尘埃在火星大气中的作用.

    主要方法:

    • 轨道航天器在1971年30天内进行的测量.
    • 对一氧化碳 (CO) 排放率的分析卡梅伦和第四正波段.
    • 测量原子氧 (1304 Å) 和原子 (1216 Å) 的气光线作为高度的函数.
    • 低大气层反射率的光谱测量测量.

    主要成果:

    • 观察到CO卡梅伦带空气发光的尺度高度的显著变化与太阳活动相关.
    • 在整个观察期间,一直检测到原子氧和气发光线.
    • 火星大气反射率约为1969年测量的50%,表明粒子散射.
    • 以紫外线吸收和光学深度> 1的尘埃为模型的反射率变化.

    更多相关视频

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media
    05:16

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media

    Published on: October 25, 2021

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna
    06:41

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna

    Published on: September 14, 2016

    相关实验视频

    Last Updated: Jul 12, 2026

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
    09:53

    Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation

    Published on: October 30, 2012

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media
    05:16

    UV-Vis Spectroscopic Characterization of Nanomaterials in Aqueous Media

    Published on: October 25, 2021

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna
    06:41

    Assays to Detect UV-reflecting Structures and Determine their Importance in Mate Preference using the Sailfin Molly Poecilia latipinna

    Published on: September 14, 2016

  • 发现火星极地上的大气层比其他地区清晰.
  • 结论:

    • 太阳活动影响火星上一氧化碳空气发光的尺度高度.
    • 原子氧和是火星上层大气的持续组成部分.
    • 火星尘埃是大气散射的一个重要因素,特别是在紫外线光谱中.
    • 大气清晰度因地区而异,极地地区较少被尘埃遮蔽.