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相关概念视频

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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相关实验视频

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

在Mariner 9上进行红外放射测量实验.

S C Chase, H Hatzenbeler, H H Kieffer

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

    马里纳9号红外辐射仪的测量显示,火星上存在显著差异.

    科学领域:

    • 行星科学 行星科学
    • 红外光谱学 红外光谱学
    • 大气科学 大气科学

    背景情况:

    • 之前来自Mariners 6和7的红外辐射仪数据为火星提供了基线热辐射测量.
    • 了解火星大气组成和热特性对于行星探索至关重要.

    研究的目的:

    • 为了分析与以前的Mariner任务相比,Mariner 9任务测量的红外亮度温度的差异.
    • 为了研究大气尘埃在火星的热辐射中的作用.

    主要方法:

    • 利用来自Mariner 9航天器的红外辐射仪数据.
    • 分析了10和20微米的亮度温度.
    • 他将Mariner 9的数据与Mariner 6和7的数据进行了比较.

    主要成果:

    • 在Mariner 9和之前的任务之间观察到明亮度温度的实质差异.
    • 确定了大气尘埃对热辐射的显著依赖于度的贡献.
    • 量化了尘埃对火星红外光谱特征的影响.

    结论:

    • 大气中的尘埃显著影响火星观测到的热辐射.

    更多相关视频

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    Thermocapillary Convection Space Experiment on the SJ-10 Recoverable Satellite

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    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

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    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

  • 取决于度的尘埃分布是热变化的关键因素.
  • 马里纳9号的数据揭示了比以前理解的更复杂的热谱.