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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.
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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...
IR Spectroscopy: Molecular Vibration Overview
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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...
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Related Experiment Video
Updated: Jun 16, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
Moderate Resolution VUV Rocket Spectrograph.
Applied Optics
|February 4, 2010
Summary
A new rocket spectrograph captures vacuum ultraviolet (VUV) spectra from 1050-2000 A. This instrument, utilizing a Carruthers electronographic camera, analyzes atmospheric sources and provides detailed CO spectra.
Area of Science:
- Atmospheric Science
- Spectroscopy
- Astrophysics
Background:
- Vacuum ultraviolet (VUV) spectroscopy is crucial for analyzing atmospheric composition and stellar emissions.
- Moderate resolution instruments are needed for detailed spectral analysis in the VUV range.
Purpose of the Study:
- To describe a novel moderate-resolution rocket spectrograph for VUV spectral measurements.
- To demonstrate the spectrograph's capability in analyzing atmospheric sources and molecular bands.
Main Methods:
- Development and deployment of a rocket-borne spectrograph.
- Incorporation of a Carruthers electronographic camera, a plane grating, and focusing optics.
- Acquisition of spectral data in the 1050 A to 2000 A range.
Main Results:
- The spectrograph provides a well-defined field of view for extended atmospheric sources.
- Sample spectra of the fourth positive band of carbon monoxide (CO) were successfully obtained between 1200 A and 1800 A.
- The instrument demonstrates effective performance in the VUV spectral region.
Conclusions:
- The described rocket spectrograph is a capable instrument for VUV atmospheric and astrophysical observations.
- The obtained CO spectra validate the spectrograph's performance and utility for molecular analysis.

