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About Infrared Spectrometers

Infrared (IR) spectrometers measure the wavelength and intensity of the absorption of infrared light by a sample. Infrared light lies between the visible and microwave portions of the electromagnetic spectrum and has a range of wavelengths. Near infrared light is closest in wavelength to visible light. By contrast, far infrared light is closest to the microwave region. Mid-infrared light is energetic enough to excite molecular vibrations to higher energy levels. These vibrations, which are caused by changes to a molecule’s dipole moment, occur only at those frequencies where the molecule absorbs infrared light. Because the wavelengths of infrared absorption bands are characteristic of specific types of chemical bonds, infrared spectrometers are often used to identify organic and organometallic molecules. 

There are two basic types of infrared spectrometers. Fourier transform infrared (FTIR) spectrometers are single-beam instruments that use an interferometer to spread a sample with infrared light and measure the intensity of the infrared light not absorbed by the sample. The application of a Fourier transform converts the resulting time domain digital signal into a frequency domain digital signal. Dispersive infrared spectrometers use visible lasers, a grating, and charged coupled devices (CCDs) to collect data. The laser acts as a light source and irradiates the sample. Most of the radiation scatters elastically at the same energy as the incoming laser radiation. A small amount, approximately one photon in a million (0.00001%), scatters from the sample at a wavelength shifted slightly from the original wavelength.

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Products & Services Related to Infrared Spectrometers

Atomic Absorption Spectrometers
Atomic absorption spectrometers (AA) use the absorption of light to measure the concentration of gas-phase atoms.
Atomic Absorption Spectrometers
Atomic absorption spectrometers (AA) use the absorption of light to measure the concentration of gas-phase atoms.
Atomic Emission and Optical Emission Spectrometers
Atomic emission and optical emission spectrometers determine analyte concentration via a quantitative measurement of the optical emission from excited atoms.
Atomic Emission and Optical Emission Spectrometers
Atomic emission and optical emission spectrometers determine analyte concentration via a quantitative measurement of the optical emission from excited atoms.
Fluorometers
Fluorometers measure the amount of fluorescent radiation produced by a sample exposed to monochromatic radiation.
X-ray Fluorescence Spectrometers
X-ray fluorescence spectrometers (XRFs) use a spectroscopic technique that is commonly used with solids, in which X-rays are used to excite a sample and generate secondary X-rays. 
X-ray Fluorescence Spectrometers
X-ray fluorescence spectrometers (XRFs) use a spectroscopic technique that is commonly used with solids, in which X-rays are used to excite a sample and generate secondary X-rays. 

Other Topics You Might Be Interested In

  • Deuterated Triglycine Sulfate (DTGS)
    Deuterated triglycine sulfate (DTGS) is a very sensitive detector type for infrared spectrometers that take measurements in the mid-infrared (mid IR) range. Most scanning instruments incorporate a...
    (read more)
  • Dispersive Raman Spectrometers
    Dispersive Raman spectrometers measure the wavelength and intensity of inelastically-scattered light. They use visible lasers, a grating, and charged-coupled detectors (CCD) to collect data. In most...
    (read more)
  • Interferometers
    Interferometers are illuminated by a source of infrared energy. In the interferometer, the infrared energy is split in to two beams, and then optically recombined. In this way, the two beams interfere...
    (read more)

Engineering Web: Infrared Spectrometers

Pages: 1 - 3 of 380

Infrared Spectroscopy in Astronomy
Spectrometers onboard infrared missions like the Kuiper Airborne Observatory (KAO), and the Infrared Space Observatory (ISO), as well as
UCLA Infrared Laboratory
Eric Becklin and I initiated the Infrared Laboratory from scratch, with the specific intention of supporting infrared astronomy in the "era of the
Infrared Spectroscopy
Infrared spectrometers, similar in principle to the UV-Visible spectrometer described elsewhere, permit chemists to obtain absorption spectra of
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