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UV–Vis Spectrometers01:14

UV–Vis Spectrometers

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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.
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Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

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Inductively coupled plasma (ICP) is the common plasma source used in atomic emission spectroscopy (AES), a technique that detects and analyzes various elements in a sample. This method is often called inductively coupled plasma atomic emission spectroscopy (ICP-AES).
There are three main types of inductively coupled plasma atomic emission spectroscopy  (ICP-AES) instruments: sequential, simultaneous multichannel, and Fourier transform instruments, with the latter being less commonly used....
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Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

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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...
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IR Spectrometers01:25

IR Spectrometers

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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...
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Atomic Fluorescence Spectroscopy01:29

Atomic Fluorescence Spectroscopy

1.1K
Atomic fluorescence spectroscopy (AFS) is an analytical technique that involves the electronic transitions of atoms in a flame, furnace, or plasma being excited by electromagnetic (EM) radiation. When these atoms absorb energy, they become excited and subsequently release energy as they return to their original state. This emitted light, or "fluorescence," is observed at a right angle to the incident beam. Both absorption and emission processes transpire at distinct wavelengths, which...
1.1K
Infrared (IR) Spectroscopy: Overview01:09

Infrared (IR) Spectroscopy: Overview

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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...
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Related Experiment Video

Updated: May 3, 2026

Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−
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Anamorphic integral field spectrometer for diffuse ultraviolet astronomy.

Timothy Cook

    Applied Optics
    |February 12, 2014
    PubMed
    Summary
    This summary is machine-generated.

    We designed a new anamorphic integral field spectrometer to study faint ultraviolet light from diffuse astronomical sources. This instrument offers a large field of view and high spectral resolution, improving our ability to analyze cosmic emissions.

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    Area of Science:

    • Astronomy and Astrophysics
    • Spectroscopy
    • Ultraviolet Astronomy

    Background:

    • Diffuse astrophysical sources emit faint ultraviolet light.
    • Studying these sources requires instruments with high spectral resolution and large fields of view.
    • Current spectroscopic systems have limitations in etendue (AΩ) and resolving power (R).

    Purpose of the Study:

    • To present the design of a novel anamorphic integral field spectrometer.
    • To enable the measurement of faint diffuse astrophysical sources across a large field.
    • To achieve an exceptional area, field of view, resolving power (AΩR) product.

    Main Methods:

    • Utilizes a standard focal plane image slicer.
    • Incorporates an anamorphic relay mirror and spectrometer.
    • Optimizes the system for a high area, field of view, resolving power (AΩR) product.

    Main Results:

    • A typical design achieves a spectral resolving power (R) of approximately 1000.
    • The system demonstrates an effective etendue (AΩ) of 1.5×10(-4) cm² sr.
    • The design facilitates the study of line emission from extended or diffuse sources.

    Conclusions:

    • The novel anamorphic integral field spectrometer design significantly enhances capabilities for diffuse ultraviolet astronomy.
    • The system's high AΩR product is crucial for detecting faint, extended cosmic emissions.
    • This instrument will advance the study of diffuse astrophysical phenomena in the ultraviolet spectrum.