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関連する概念動画

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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関連する実験動画

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

アポロ16号の遠紫外線カメラ/スペクトログラフ:地球の観測

G R Carruthers, T Page

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

    アポロ16号はアポロ16号でした.

    科学分野:

    • 惑星科学は惑星科学である.
    • 大気科学 大気科学
    • 宇宙物理学 宇宙物理学

    背景:

    • 地球のジオコロナと上層大気圏は紫外線を放射します.
    • これらの排出量を理解することで,大気の組成と動態に関する洞察が得られます.

    研究 の 目的:

    • 地球の大気と地球コロナからの遠紫外線放射を分析する.
    • 様々な原子・分子種の空間的分布と強度を決定する.

    主な方法:

    • アポロ16号ミッションの月の表面での遠紫外線カメラ/スペクトログラフの操作.
    • 1600アングストロム以下でスペクトルおよび画像データの取得.

    主要な成果:

    • 地球の大気とジオコロナの画像とスペクトルを取得しました.
    • 原子水素,原子酸素,分子窒素からの排出量の空間的分布と相対的強度をマッピングした.
    • 特定の種の放射能が初めてスペクトログラフィーで観測されました.

    結論:

    • アポロ16号ミッションは,地球の上層大気とジオコロナに関する貴重な遠紫外線データを提供した.

    さらに関連する動画

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

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    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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    Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

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    関連する実験動画

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    Bringing the Visible Universe into Focus with Robo-AO

    Published on: February 12, 2013

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

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    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

  • この実験では,大気の重要な構成要素からの排出を成功裏に特徴づけました.
  • この発見は,大気組成と遠隔感知能力の理解に寄与する.