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Related Concept Videos

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...
Spectrophotometry: Introduction01:16

Spectrophotometry: Introduction

Spectrophotometry is the quantitative measurement of the absorption, reflection, diffraction, or transmission of electromagnetic radiation through a material as a function of the intensity and wavelength of the radiation. A spectrophotometer is a device used to measure the change in the radiation intensity caused by its interaction with the material.
The essential components of a spectrophotometer include a source of electromagnetic radiation, a slot for placing a material to be analyzed, and a...
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...
Atomic Spectroscopy: Absorption, Emission, and Fluorescence01:23

Atomic Spectroscopy: Absorption, Emission, and Fluorescence

Atomic spectroscopy is a vital tool in elemental analysis, both qualitatively and quantitatively. It can be broadly divided into optical spectroscopy, mass spectroscopy, and X-ray spectroscopy methods. The optical spectroscopic methods are atomic absorption spectroscopy (AAS), atomic emission spectroscopy (AES), and atomic fluorescence spectroscopy (AFS). The first step in all three methods is atomization, where the solid, liquid, or solution-phase samples are converted into gas-phase atoms and...
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.
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.

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Updated: Jun 15, 2026

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

Efficiency of spectrometers.

B Carli, V Natale

    Applied Optics
    |March 11, 2010
    PubMed
    Summary
    This summary is machine-generated.

    A new formula helps calculate the signal-to-noise ratio (SNR) in spectroscopic measurements. It identifies essential and avoidable signal losses, aiding in method comparison and optimization.

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    Area of Science:

    • Spectroscopy
    • Analytical Chemistry
    • Physical Chemistry

    Background:

    • Signal-to-noise ratio (SNR) is a critical parameter in spectroscopic measurements, directly impacting data quality and reliability.
    • Understanding factors influencing SNR is essential for optimizing experimental design and data interpretation.
    • Existing methods for SNR assessment may not comprehensively address all sources of signal loss.

    Purpose of the Study:

    • To derive a general formula for calculating the signal-to-noise ratio (SNR) in spectroscopic measurements.
    • To identify and categorize factors contributing to signal loss, distinguishing between inherent and avoidable losses.
    • To provide a tool for comparing the performance of different spectroscopic techniques.

    Main Methods:

    • Derivation of a general mathematical formula for SNR calculation based on fundamental spectroscopic principles.
    • Analysis of various components contributing to signal attenuation and noise generation within spectroscopic systems.
    • Systematic evaluation of signal loss factors, including instrumental, environmental, and sample-related contributions.

    Main Results:

    • A comprehensive formula for SNR calculation applicable to diverse spectroscopic methods has been established.
    • Key factors causing signal loss have been identified, with a clear distinction between unavoidable and reducible sources.
    • The derived formula facilitates quantitative comparison of SNR across different spectroscopic techniques.

    Conclusions:

    • The developed SNR formula offers a standardized approach for evaluating spectroscopic measurement quality.
    • Identifying and minimizing avoidable signal losses can significantly enhance SNR, leading to improved analytical sensitivity.
    • This work provides a valuable framework for selecting and optimizing spectroscopic methods for specific applications.