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相关概念视频

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...
Atomic Emission Spectroscopy: Instrumentation01:22

Atomic Emission Spectroscopy: Instrumentation

The instrumentation of atomic emission spectrometry (AES) involves various components, including atomization devices that convert samples into gas-phase atoms and ions. There are two main types of atomization devices: continuous and discrete atomizers.  Continuous atomizers, like plasmas and flames, introduce samples in a constant stream, while discrete atomizers inject individual samples using syringes or autosamplers. The most common discrete atomizer is the electrothermal atomizer.
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...
Atomic Emission Spectroscopy: Lab01:29

Atomic Emission Spectroscopy: Lab

AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...
Flame Photometry: Lab01:16

Flame Photometry: Lab

In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
IR Spectrometers01:25

IR Spectrometers

There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...

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相关实验视频

Updated: Jul 11, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

阿波罗16号远紫外相机/光谱仪:地球观测结果

G R Carruthers, T Page

    Science (New York, N.Y.)
    |September 1, 1972
    PubMed
    概括

    阿波罗16号航天飞船的任务是

    科学领域:

    • 行星科学 行星科学
    • 大气科学 大气科学
    • 空间物理 空间物理

    背景情况:

    • 地球的地质冠和上层大气层发射紫外线.
    • 了解这些排放提供了对大气组成和动态的洞察.

    研究的目的:

    • 分析来自地球大气和地球冠状病毒的远紫外辐射.
    • 确定各种原子和分子物种的空间分布和强度.

    主要方法:

    • 在阿波罗16号任务期间,在月球表面运行远紫外相机/光谱仪.
    • 获取1600安格斯特罗姆以下的光谱和成像数据.

    主要成果:

    • 获得了地球大气层和地质冠状的图像和光谱.
    • 映射了原子,原子氧和分子排放的空间分布和相对强度.
    • 在光谱上首次观察到某些物种的排放.

    结论:

    • 阿波罗16号任务提供了关于地球上层大气和地球冠状的宝贵远紫外线数据.
    • 该实验成功地描述了主要大气成分的排放.
    • 这些发现有助于我们了解大气组成和遥感能力.

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    Last Updated: Jul 11, 2026

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    Published on: February 12, 2013

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    Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

    Published on: May 10, 2020

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    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

    Published on: July 30, 2020