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Related Concept Videos

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation01:26

Inductively Coupled Plasma Atomic Emission Spectroscopy: Instrumentation

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.
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...
Tandem Mass Spectrometry01:21

Tandem Mass Spectrometry

Tandem mass spectrometry is a technique that uses multiple mass analyzers in series to obtain a higher selectivity and reduce chemical noise during analyte detection. Instruments with multiple analyzers separated by an interaction cell enable secondary fragmentation and selected study of the fragment ions.Secondary fragmentations occur in the interaction cell and can be induced by various factors. Fragmentation induced by collision with inert gases, such as N2, Ar, He, etc., is called...
Atomic Emission Spectroscopy: Instrumentation01:22

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.
UV–Vis Spectrometers01:14

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...
Atomic Absorption Spectroscopy: Instrumentation01:22

Atomic Absorption Spectroscopy: Instrumentation

An atomic absorption spectrophotometer (AAS) comprises several components: a radiation source, an atomizer, a monochromator, and a detector. The radiation source can be a hollow-cathode lamp (HCL) or an electrodeless-discharge lamp (EDL), both of which provide a narrow emission line of the required wavelength. However, some instruments use continuum sources and high-resolution monochromators to achieve a narrow range of radiation.
The atomizer used in AAS can be either a flame atomizer or an...

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High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis
13:31

High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis

Published on: December 22, 2015

Parabolic telescope and spectrometer combination.

G Schmidtke, P Henneberg, K H Hager

    Applied Optics
    |March 12, 2010
    PubMed
    Summary
    This summary is machine-generated.

    This study details a nonfocusing parabolic telescope

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    Area of Science:

    • Optical astronomy and instrumentation.
    • Telescope design and performance analysis.

    Background:

    • Nonfocusing parabolic telescopes offer unique optical properties.
    • Understanding aberrations is crucial for telescope performance.

    Purpose of the Study:

    • To thoroughly investigate the optical characteristics of a nonfocusing collimating parabolic telescope.
    • To assess its performance with different spectrometer types for high-resolution spectroscopy.

    Main Methods:

    • Detailed ray-tracing analysis to evaluate optical quality.
    • Calculation of optimal optical performance for on-axis rays.
    • Discussion of diffraction effects and aperture implications.

    Main Results:

    • Optimal optical quality is achieved for rays near the optical axis, with aberrations affecting field borders.
    • The parabolic telescope demonstrates excellent compatibility with echelle, Wadsworth, and Ebert-Fastie spectrometers.
    • Spot diagrams visually represent the optical performance in specific scenarios.

    Conclusions:

    • The nonfocusing parabolic telescope, when combined with suitable spectrometers, enables very high spectral resolution.
    • Aberrations necessitate careful consideration for applications requiring sharp field edges.
    • Diffraction effects are an important factor in the overall performance analysis.