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Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview01:13

Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview

Attenuated total reflectance (ATR) infrared spectroscopy is a powerful analytical technique used to study the composition of materials. It is widely employed in chemistry, materials science, forensic science, and other fields where sample characterization is required. ATR has several advantages over traditional transmission IR spectroscopy, including the requirement of little to no sample preparation and the ability to analyze a wide range of samples.
The ATR process begins by directing a beam...
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,...
Atomic Emission Spectroscopy: Overview01:20

Atomic Emission Spectroscopy: Overview

Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
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...
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.
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.

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関連する実験動画

Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

星の隠蔽による地球の大気組成

P B Hays, R G Roble, A N Shah

    Science (New York, N.Y.)
    |May 19, 1972
    PubMed
    まとめ
    この要約は機械生成です。

    軌道上の天文観測所-2 (OAO-2) の衛星データは,夜間の分子酸素とオゾンプロフィールを明らかにした. 恒星の紫外線光度計は,大気吸収を測定し,地球の上層大気の重要な密度データを提供しました.

    さらに関連する動画

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
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    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

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

    Published on: May 10, 2020

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    Last Updated: Jul 12, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
    06:27

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

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

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    科学分野:

    • 大気科学 大気科学
    • 天体物理学 天体物理学
    • リモートセンシング (リモートセンサー)

    背景:

    • 地球の上層大気は,恒星の紫外線 (UV) を吸収する.
    • オゾンと分子酸素は,大気中の紫外線を主に吸収します.

    研究 の 目的:

    • 分子酸素とオゾンの夜間垂直数密度プロフィールを決定する.
    • 大気組成分析のための恒星隠蔽データを活用する.

    主な方法:

    • 軌道上の天文観測所-2 (OAO-2) 衛星に搭載された星の紫外線光度計が利用されました.
    • 地球の大気隠蔽の間に恒星の強度の変化を測定した.
    • 大気密度プロフィールを導き出すために,隠蔽データを分析した.

    主要な成果:

    • 分子酸素の夜間垂直数密度プロファイル (120~200kmの高さ) を取得した.
    • オゾン (60~100kmの高さ) の夜間垂直数密度プロファイルを取得しました.

    結論:

    • 恒星隠蔽は,大気成分をプロファイリングするための効果的な方法です.
    • この研究は,上層大気圏における夜間オゾンと分子酸素の分布に関する貴重なデータを提供します.