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関連する概念動画

Infrared (IR) Spectroscopy: Overview01:09

Infrared (IR) Spectroscopy: Overview

When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
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...
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...
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 Spectrum01:19

IR Spectrum

When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0% (complete...
IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...

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関連する実験動画

Updated: Jul 12, 2026

The Use of High-resolution Infrared Thermography (HRIT) for the Study of Ice Nucleation and Ice Propagation in Plants
09:36

The Use of High-resolution Infrared Thermography (HRIT) for the Study of Ice Nucleation and Ice Propagation in Plants

Published on: May 8, 2015

マリナー9号の赤外線放射測定実験

S C Chase, H Hatzenbeler, H H Kieffer

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

    マリナー9号の赤外線放射計の測定は,火星における有意な違いを示しています.

    科学分野:

    • 惑星科学は惑星科学である.
    • 赤外線スペクトロスコーピーは,赤外線スペクトロスコーピーを用います.
    • 大気科学 大気科学

    背景:

    • マリナーズ6号と7号からの以前の赤外線放射計データは,火星の熱放射測定基準を示した.
    • 火星の大気組成と熱的性質を理解することは,惑星探査にとって極めて重要です.

    研究 の 目的:

    • マリナー9号によって測定された赤外線光の温度における差異を,以前のマリナー号ミッションと比較して分析する.
    • 火星の熱放出における大気中の塵の役割を調査する.

    主な方法:

    • マリナー9号宇宙船からの赤外線放射計データを活用した.
    • 10および20マイクロメートルの明るさの温度を分析した.
    • マリナー9号のデータと,マリナー6号と7号のデータを比較した.

    主要な成果:

    • マリナー9号と以前のミッション間の明るさ温度における実質的な違いが観察されました.
    • 大気中の塵が熱放射に有意な緯度依存の貢献を特定した.
    • 火星の赤外線スペクトルシグネチャーに塵の影響を定量化しました.

    結論:

    さらに関連する動画

    Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
    07:00

    Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite

    Published on: March 11, 2020

    In Situ SIMS and IR Spectroscopy of Well-defined Surfaces Prepared by Soft Landing of Mass-selected Ions
    10:22

    In Situ SIMS and IR Spectroscopy of Well-defined Surfaces Prepared by Soft Landing of Mass-selected Ions

    Published on: June 16, 2014

    関連する実験動画

    Last Updated: Jul 12, 2026

    The Use of High-resolution Infrared Thermography (HRIT) for the Study of Ice Nucleation and Ice Propagation in Plants
    09:36

    The Use of High-resolution Infrared Thermography (HRIT) for the Study of Ice Nucleation and Ice Propagation in Plants

    Published on: May 8, 2015

    Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite
    07:00

    Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite

    Published on: March 11, 2020

    In Situ SIMS and IR Spectroscopy of Well-defined Surfaces Prepared by Soft Landing of Mass-selected Ions
    10:22

    In Situ SIMS and IR Spectroscopy of Well-defined Surfaces Prepared by Soft Landing of Mass-selected Ions

    Published on: June 16, 2014

    • 大気中の塵は,火星の観測された熱放出に大きく影響する.
    • 緯度に依存する塵の分布は,熱の変化の重要な要因である.
    • マリナー9号のデータは,これまで理解していたよりも複雑な熱プロフィールを明らかにしています.