spectrometers

Author: the photonics expert (RP)

Definition: devices for separating spectral components

More general term: optical metrology instruments

More specific terms: spectrographs, spectrophotometers

Categories: general optics, light detection and characterization, optical metrology

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DOI: 10.61835/ev5   Cite the article: BibTex plain textHTML   Link to this page!   LinkedIn

Contents

Generally, an optical spectrometer is an instrument which can be used for investigating wavelength-dependent properties of light, substances or objects; the term is rather broad:

• An spectrometer may be an instrument which can spatially separate spectral components of light, so that they can be separately analyzed – e.g. with a photographic plate or an external photodetector. The used polychromator is usually either a diffraction grating or a prism.
• A spectrometer often also contains some photodetector(s) for analyzing the intensities. A spectrograph, containing a large detector array, can be used for recording the optical spectrum of a light source without scanning e.g. a grating orientation. When equipped with intensity calibration, such devices are more specifically called spectroradiometers.
• Other optical spectrometers are made for analyzing substances or objects in terms of spectroscopic properties, for example wavelength-dependent transmittance or reflectance. They are more specifically called spectrophotometers, and find applications in fields like chemistry, for example. Particularly high spectral resolutions in combination with high sensitivity are obtained with laser spectrometers, containing some narrow-linewidth tunable laser(s). However, these can often cover only quite limited spectral regions.

Also many kinds of spectrometers outside the area of optics and photonics – for example, devices for measuring particle velocity or particle size distributions. This article, however, focuses entirely on spectrometers for spectrally analyzing light; see the article on spectrophotometers when the analysis of substances or objects is of interest.

Measurements with spectrometers typically deliver the optical power spectral density (PSD) as a function of the wavelength or optical frequency. Not all spectrometers deliver calibrated PSDs; often, the intensity readings are uncalibrated, possibly with a substantial wavelength dependence of the (unknown) calibration factor (responsivity).

There are also methods of spectral phase interferometry, which can measure not only the power spectral density but also the spectral phase.

There are spectrometers which also have imaging capabilities, and are called imaging spectrometers. See the articles on hyperspectral imaging and multispectral imaging.

If only the spectral linewidth of a laser beam needs to be measured, but not the detailed spectral shape, one can use other methods, e.g. perform a self-heterodyne linewidth measurement. With such methods, one can measure very small linewidths which are far below the typical resolution of a spectrometer.

Applications of Spectrometers

Spectrometers find applications in a wide range of fields. Some typical examples:

• In optical technology and fundamental physics, spectrometers are applied for characterizing various kinds of light sources and optical components.
• Astronomy with optical telescopes often uses the spectrometers to acquire additional information on galaxies, stars and planets, for example.
• In chemistry, spectrometers can be used for identifying substances or measuring concentrations of multiple substances, for example in liquid solutions or in gases. See the article on spectrophotometers for more details. In the context of LIDAR, spectral analysis can be used for environmental monitoring.
• There are industrial process spectrometers, used for monitoring and automatically controlling chemical processes in production lines or power stations.

See also the article on spectroscopy for more applications.

Depending on the application, the requirements concerning the covered wavelength region, the performance (e.g. resolution, sensitivity, speed, etc.) and the cost can be extremely different. Therefore, a wide range of spectrometers is available commercially, and specialized versions are developed for special applications, e.g. in astronomy.

Types of Spectrometers

Spectrometers Based on Diffraction Gratings or Prisms

Most spectrometers are based on some kind of polychromator, i.e., a device which can spatially separate different wavelength components of light. Usually, they exploit either wavelength-dependent diffraction on one or several diffraction gratings or the wavelength-dependent refraction at one or several prisms.

Typically, an incident beam is collimated (made parallel) before being sent to a grating or prism. After that dispersive element, different wavelength components propagate in slightly different directions. The light may then go through some additional optics and finally get to a photodetector.

For obtaining a spectrograph (a non-scanning spectrometer), the photodetector may be a photodiode array, CCD array or similar, recording intensities over some spatial range, which correspond to a certain spectral interval. One does directly obtain a spectrum by mapping the detector pixels to wavelengths. The data acquisition is then relatively fast because all wavelength components can be measured simultaneously. The resolution is then typically limited by the density of detector pixels, or possibly by the optical setup. Spectral peak positions may be determined with an accuracy better than according to the pixel spacing by using interpolation.

In a scanning spectrometer, the detector can be a single photodiode or a photomultiplier, placed after a narrow optical slit, so that only one narrow interval of wavelengths can get to the detector at one time. The slit position or the angular orientation of the grating or prism may then be moved such that a certain wavelength range can be scanned, assuming that the PSD of the input remains constant during that time. The setup then functions as a tunable monochromator. Figure 1 shows the common design of the Czerny–Turner grating monochromator. The acquisition time for a full spectrum can be long if a wide spectral range is scanned with high resolution and if the detector cannot be very fast, e.g. because the low optical power enforces a substantial average time. Long acquisition times may not only be inconvenient, but a real problem if the properties of the light source are not constant.

Light passing the entrance slit is collimated with a curved mirror, experiences a wavelength-dependent deflection at the diffraction grating and is then focused again with another curved mirror. For one orientation of the diffraction grating, only light in a narrow wavelength band can pass the exit slit. (The shown rays apply for a wavelength in that interval.) The whole setup is placed in a box, containing additional apertures and black shields to minimize effects of stray light.

There are also modified designs, e.g. the crossed Czerny–Turner spectrometer, allowing for more compact designs than the unfolded version. Another version is based on a concave holographic grating, not involving additional curved mirrors.

Some grating spectrometers are extremely compact, with a width of only a few centimeters. However, the highest performance – in particular in terms of resolution and sensitivity – is obtained with much larger instruments. Typical wavelength resolutions reached with such spectrometers are about 0.01 nm to 0.1 nm.

Depending on the type of spectrometer used (e.g. a grating spectrometer), various details have to be observed:

• The input light often has to be sent onto an entrance slit of variable width. For highest spectral resolution, the slit should be made narrow, but that reduces the transmitted power and may therefore lead to increased noise or longer acquisition times, particularly for sources with low brightness. Some spectrometers have a fiber input, either with multimode fiber or single-mode fiber. Multimode fibers make it easier to collect light, while single-mode fibers allow for highest spectrometer performance.
• Diffraction gratings are often used with the first diffraction order, but sometimes with higher diffraction orders to obtain a better performance. In any case, there can be problems with artifacts related to light being diffracted on other orders. If one finds spectral features which are hard to explain, one may check whether they could be such artifacts.
• The response of a spectrometer may depend on the polarization because the diffraction efficiency of a grating or the reflection loss on a prism arrangement is polarization-dependent.
• Some spectrometers have to be calibrated by the user. For wavelength calibration, one may use certain discharge lamps, emitting line spectra with precisely defined wavelength components. Calibration of the responsivity for the whole wavelength interval is often more difficult. One possibility is to use an incandescent lamp with a known filament temperature or calibrated spectrum.

Interferometric Spectrometers

A high spectral resolution, but only in a very limited spectral range, is obtained with various types of interferometric spectrometers:

• Some instruments are based on a Fabry–Pérot interferometer, where the mirror spacing is mechanically scanned, e.g. via a piezo actuator, while the transmitted optical power is registered. The usable spectral interval is the so-called free spectral range, determined by the mirror distance; this is typically of the order of 0.1 GHz to 10 GHz, i.e., very small in terms of nanometers. The resolution bandwidth is the free spectral range divided by the finesse, the latter being determined essentially by the mirror reflectivities. A large distances between the mirrors allows for a higher performance, but also leads to a narrow free spectral range.
• Fourier-transform spectrometers can contain a Michelson interferometer, where one arm length can be mechanically scanned over a long distance (millimeters, centimeters or even more). The detector signal versus time, recorded during a full arm length scan, has to be Fourier-transformed to obtain the optical spectrum. Advantages are the potentially high spectral resolution and that one requires only a single-element photodetector.
• A simplified version is the wavemeter, specialized on precisely measuring only the wavelength of a laser source, rather than recording full spectra.
• Arrayed waveguide gratings are sometimes used for very compact spectrometers. They are based on interference effects in a small waveguide device.

Dispersive Spectral Analysis Based on Propagation Times

A totally different principle of operation can be realized for the spectral analysis of broadband ultrashort pulses. One may simply send such pulses through a long fiber, which introduces substantial chromatic dispersion. The latter then results in substantially different arrival times of different spectral components after the fiber: a pulse with an original pulse duration of far below 100 fs may then be spread over several nanoseconds, for example. By analyzing that light with a fast photodiode and oscilloscope, one can obtain information on the spectrum. Of course, one should make sure that optical nonlinearities are not invalidating the results; in fibers, this strongly limits the allowable peak power.

A very attractive property of that method is the high speed with which a spectrum can be recorded. A single ultrashort pulse is sufficient for that purpose, whereas a conventional scanning spectrometer, for example, may require many seconds for that and would average the spectrum over many pulses of a pulse train.

Spectrometers for Extreme Spectral Regions

Traditional spectrometers work in the visible spectral range and/or with near-infrared, or possibly with near-ultraviolet light. However, there are also spectrometers for operation in extreme spectral regions.

Some devices work with short wavelengths, i.e., in the extreme ultraviolet (EUV) or even the X-ray region, with wavelengths of only a few nanometers. Such devices may be based on diffraction gratings with very small line spacings, or in the X-ray region even on single crystals, exploiting the periodicity on the atomic scale. As photodetectors, one may use special X-ray CCD cameras or multichannel plate (MCP) detectors (→ photomultipliers).

Other spectrometers are suitable for the mid-infrared spectral region (→ mid-infrared spectrometers). They require special infrared optics and also suitable detectors. Long-wavelength photodetectors are available, but with limited performance in terms of detection noise and bandwidth. Substantial improvements are possible by upconversion of the infrared light into the visible or near-IR, using sum frequency generation with a laser, to utilize the more powerful visible or near-IR photodetectors. That aspect is particularly important for spectrographs, where one requires a multi-channel detector. Such devices are mostly available in silicon technology, which is suitable only for wavelengths below ≈1 μm.

More to Learn

Suppliers

The RP Photonics Buyer's Guide contains 129 suppliers for spectrometers. Among them:

HighFinesse

The grating-based HighFinesse/ Ångstrom’ spectrometers offer the capability for a very accurate simultaneous measurement of both wavelength and linewidth of laser sources. With a resolving power up to 40000 and a measurement speed up to 500 MHz, the product series covers the range from 192 nm to 11000 nm, allowing measurements of both pulsed and cw lasers. The grating based technology enables the analysis of laser sources over a large linewidth range. Connected to the PC via USB, after a simple software installation the spectrometers are ready for use.

GWU-Lasertechnik

GWU's portfolio of CCD-based spectrometers provides a great variety of features to fulfill nearly any requirement of versatile applications. The detection range covers the UV to near-infrared spectrum and even reaches out to the mid-infrared at 2.6 µm. Models with tiny footprint, e.g. for wavelength monitoring in OEM applications, as well as thermo-electric (TE) cooled devices with high resolution, high sensitivity and ultra-low noise for weak-light applications, such as fluorescence sensing or Raman analysis, are offered.

UltraFast Innovations

EVEREST, by UltraFast Innovations (UFI®), is a soft X-ray/XUV/VUV spectrograph that features aberration-corrected flat-field imaging and is available with three gratings covering the spectral ranges 1–17 nm (1240–73 eV), 5–80 nm (248–15.5 eV) and 24–200 nm (51.7–6.2 eV). In order to maximize light collection, the spectrometer can be used without an entrance slit over a variety of source distances, with 3–17 nm, 10–80 nm and 24–200 nm spectral coverage. Its modular design is able to match different experimental geometries and configurations. It features an integrated slit holder, gate valve, and filter insertion unit, as well as a 3-axis motorized grating positioning.

Edmund Optics

Edmund Optics offers a wide variety of spectrometers, including spectrometers that have been optimized for Raman or fluorescence spectroscopy. Raman spectrometers are ideal for Raman applications in the visible to the near infrared. The fluorescence spectrometers are ideal for use in low light fluorescence applications where the ability to detect weak signals is crucial for proper measurement. Additionally, fluorescence spectrometers feature broadband spectral response ranges for detecting wide wavelength bands along with a wide slit width for increased throughput.

Femto Easy

The MISS (Mini Imaging Spatial Spectrometer) is an innovative imaging spectrometer for ultrashort pulse characterization. It provides optical spectra with spatial resolution in one direction of a laser beam, thus allowing for vertical and horizontal spatial chirp measurements. Both free-space and fiber input versions are available.

APE

The waveScan spectrometer by APE is a compact and cost-efficient optical spectrometer for characterizing light sources, e.g. ultrafast as well as cw laser systems. The waveScan device family cover the spectral range from 200 nm to 6300 nm and allows also the characterization of low-repetition rate lasers down to 100 Hz. The rotating grating technology achieves high resolution measurements at a 5 Hz spectral measurement rates. This makes waveScan an ideal real-time alignment tool for laser systems.

Light Conversion

The HARPIA spectroscopy systems perform a variety of sophisticated time-resolved measurements in a compact footprint. The HARPIA-TA is a transient absorption spectroscopy system extendable with time-resolved fluorescence, microscopy, and other modules. The HARPIA-TG is a novel transient grating system for carrier diffusion and lifetime measurements. For a single-supplier solution, the HARPIA systems are combined with a PHAROS or a CARBIDE laser together with ORPHEUS series or I-OPA series of OPAs.

NLIR

The S2050 2–5 µm fiber spectrometer has a unique combination of a super-fast full spectra acquisition rate of up to 130 kHz, an ultra-sensitive minimum detection power of 5 pW/nm and a resolution of 6 cm⁻¹.

Our spectrometer is based upon a new measuring paradigm where mid-infrared light is converted into near-visible light and then measured with conventional near-visible grating spectrometer technology.

LightMachinery

LightMachinery's spectrometers are setting the new standard for range, resolution, cost and size. The HyperFine HF series spectrometer is designed for LIBS or simultaneous Brillouin and Raman spectroscopy. With 1 pm resolution in a small package size it offers an affordable approach to advanced spectroscopic applications. The Hyperfine HN Series spectrometer is a smaller version with about 25-pm resolution anywhere in the UV, visible and NIR wavelength ranges. The Hyperfine HN is ideal for characterizing light sources such as laser spectra in real time.

CNI Laser

CNI offers fiber-optic spectrometers, multi-channel spectrometers and some spectroscopy systems like a LIBS system, Raman spectrum systems and others which are widely used in spectroscopy applications.

Holographix

We can design and manufacture custom spectrometers incorporating original or replicated gratings. Industry leading hyperspectral-imaging systems utilize our own designed and produced components and assemblies, so you can be assured of the very highest quality.

Thorlabs

Thorlabs spectrometer development and manufacturing capabilities cover a wide range of wavelengths and applications. The compact grating-based Czerny–Turner spectrometers are fiber compatible and available for three different wavelength ranges. For applications that require higher spectral resolution, our optical spectrum analyzers employ a Michelson interferometric design compatible with fiber-coupled and free-space light sources that can be used in spectrometer or even wavelength meter mode. They are complemented by Fabry–Pérot interferometers that allow users to examine the fine spectral characteristics of e.g., CW lasers. In contrast, our holographic grating spectrometer is designed for integration into OCT systems and provides high measurement speed. For our unique Raman spectrograph, we use a coded aperture technology with exceptionally large étendue.

Hamamatsu Photonics

Hamamatsu Photonics offers a range of spectrometers and spectrum sensors, including mini-spectrometers, FTIR engines, MEMS-FPI spectrum sensors, and Raman spectroscopic modules.

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