Spectrometers & Spectroscopy Equipment | Edmund
Explore optical spectrometers, systems, and components for spectroscopy, detection, and analysis. Ideal
In spectroscopy, spectral lines are specific wavelengths of light emitted or absorbed by atoms or molecules, serving as unique "fingerprints" for identifying substances . A spectrometer measures these lines by dispersing light into its component wavelengths using elements like diffraction gratings or prisms and detecting the intensity at each wavelength . An external line often comes from a calibration source outside the spectrometer, such as a low-pressure mercury lamp or a xenon lamp, which emits well-defined emission lines . These lines are used to calibrate the wavelength scale of the spectrometer, ensuring accurate measurement of unknown samples. For example, mercury lamps provide sharp lines at 254 nm, 365 nm, 436 nm, and 546 nm, which are commonly used for UV-visible spectrophotometer calibration .

Explore optical spectrometers, systems, and components for spectroscopy, detection, and analysis. Ideal
Rotational spectroscopy is sometimes referred to as pure rotational spectroscopy to distinguish it from rotational-vibrational
While external standard calibration mitigates the need to consider response factors and does
ctrometer measurements to be triggered by an external source. To fulfill this need, Avantes ofers. an external trigger source, known
To synchronize data acquisition with external events, other modes of acquiring data are available. Each mode involves connecting
Spectrometers for Elemental Spectrochemical Analysis, Part I: The Basic Spectrometer An overview of the
Spectroscopy, primarily in the electromagnetic spectrum, is a fundamental exploratory tool in the fields of astronomy, chemistry,
13.1 INTRODUCTION As analytical and bioanalytical methods must be validated before using them for routine sample analysis and
A spectrometer is used in spectroscopy for producing spectral lines and measuring their wavelengths and intensities. Spectrometers
External Triggering with Ocean FX The triggering functions for the Ocean FX provide accurate timing and synchronization between
external event and spectral acquisition. An event outside the measurement system (such as pulse) increases or decreases the
Line broadening refers to the phenomenon where spectral emission lines become wider due to various mechanisms, including
The most important figure for our spectroscopy users is Spectral Resolution. This is a
OverviewExternal linksSpectroscopesSpectrographsSee alsoBibliography
• Spectrograph for astronomical Spectra• Photographs of spectrographs used in the Lick Observatory from the Lick Observatory Records Digital Archive, UC Santa Cruz Library''s Digital Collections Archived 2019-04-25 at the Wayback Machine
2 Line Arrays for Miniaturized Spectrometers The line array of a spectrometer is, besides the grating, the main parameter
Narrow-linewidth lasers are required for applications such as fiber-optic sensors, laser spectroscopy
Instruments in our AvaSpec NIRLine are high-performance, near-infrared spectrometers that are optimized for the demands of
A spectrophotometer uses the mercury emission lines to calibrate the displayed wavelength values. The
External Fields Broadening Magnetic or Electrical external fields cause the Zeeman effect or the Stark effect with the
OverviewTypes of line spectraNomenclatureLine broadening and shiftSpectral lines of chemical elementsSee alsoFurther reading
Spectral lines are the result of interaction between a quantum system (usually atoms, but sometimes molecules or atomic nuclei) and a single photon. When a photon has about the right amount of energy (which is connected to its frequency) to allow a change in the energy state of the system (in the case of an atom this is usually an electron changing orbitals), the photon is absorbed. Then the energy will be spontane
Ultraviolet–visible spectroscopy is an example. These spectrometers utilize the phenomenon of optical dispersion. The light from a
A comprehensive guide to line broadening in atomic spectroscopy, covering its principles, types, and applications in
Observed spectral lines are always broadened, partly due to the finite resolution of the spectrometer and partly due to intrinsic
With external triggering enabled, click OK and begin measurements. You will notice that the measure-ment counter will not increase
2. Types of Light Source Many light sources meet some of the requirements above but no light source is able to meet them all. Many
Avantes Mini Spectrometer – AvaSpec-Mini SensLine The AvaSpec SensLine family of products is
A flat-field extreme ultraviolet (EUV) spectrometer working in the 20-500 Å wavelength range with fast time response
The output socket has an SMA-905 connector and optical fibres direct the light directly to the spectrometer or to the
On-line gas detection during the thermal runaway of Li-ion cells by coupling ARC with a mass spectrometer and
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