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Flat Field and Imaging Gratings

Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 67.4 nm/mm
Wavelength Range: 1600 – 2200 nm
Spectrum Length: 8.9 mm
F/Number: 2
Groove Density: 130 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 15.5 nm/mm
Wavelength Range: 340 – 800 nm
Spectrum Length: 29.6 mm
F/Number: 2.2
Groove Density: 785 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 15.6 nm/mm
Wavelength Range: 800 – 1000 nm
Spectrum Length: 12.8 mm
F/Number: 2.2
Groove Density: 595 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 16 nm/mm
Wavelength Range: 340 – 690 nm
Spectrum Length: 24 mm
F/Number: 3.3
Groove Density: 430 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 15.8 nm/mm
Wavelength Range: 340 – 830 nm
Spectrum Length: 31 mm
F/Number: 3.3
Groove Density: 372 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 16 nm/mm
Wavelength Range: 380 – 780 nm
Spectrum Length: 25 mm
F/Number: 2.8
Groove Density: 457 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 23 nm/mm
Wavelength Range: 340 – 800 nm
Spectrum Length: 19.7 mm
F/Number: 2.8
Groove Density: 440 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 24 nm/mm
Wavelength Range: 190 – 800 nm
Spectrum Length: 25 mm
F/Number: 2.8
Groove Density: 298 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 25.1 nm/mm
Wavelength Range: 1600 – 2200 nm
Spectrum Length: 23.9 mm
F/Number: 3.7
Groove Density: 267 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 25.5 nm/mm
Wavelength Range: 190 – 800 nm
Spectrum Length: 24.6 mm
F/Number: 2
Groove Density: 340 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 27 nm/mm
Wavelength Range: 400 – 950 nm
Spectrum Length: 20 mm
F/Number: 1.8
Groove Density: 217 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 29 nm/mm
Wavelength Range: 320 – 710 nm
Spectrum Length: 13.4 mm
F/Number: 2
Groove Density: 310 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 32 nm/mm
Wavelength Range: 300 – 1100 nm
Spectrum Length: 25 mm
F/Number: 2.8
Groove Density: 227 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 40 nm/mm
Wavelength Range: 330 – 780 nm
Spectrum Length: 11.3 mm
F/Number: 3.5
Groove Density: 250 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 53 nm/mm
Wavelength Range: 190 – 870 nm
Spectrum Length: 12.6 mm
F/Number: 2
Groove Density: 185 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 67 nm/mm
Wavelength Range: 380 – 720 nm
Spectrum Length: 5 mm
F/Number: 1.5
Groove Density: 320 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 67 nm/mm
Wavelength Range: 380 – 820 nm
Spectrum Length: 6.6 mm
F/Number: 1.8
Groove Density: 143 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 9 nm/mm
Wavelength Range: 175 – 400 nm
Spectrum Length: 25.1 mm
F/Number: 4
Groove Density: 580 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 10 nm/mm
Wavelength Range: 370 – 760 nm
Spectrum Length: 37.1 mm
F/Number: 3
Groove Density: 950 l/mm
Type IV aberration corrected flat field and imaging gratings are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors. These gratings are produced with grooves that are neither equispaced nor parallel, and are computer optimized to form near-perfect images of the entrance ...

Specifications

Dispersion: 1 nm/mm
Wavelength Range: 250 – 450 nm
Spectrum Length: 203 mm
F/Number: 5.1
Groove Density: 1800 l/mm

Flat-Field and Imaging Diffraction Gratings: Enhancing Spectral Imaging Precision

Flat-field and imaging diffraction gratings are specialized optical components designed to disperse light while correcting for optical aberrations, enabling the capture of sharp, undistorted spectra across a broad wavelength range. These gratings are integral to modern spectroscopic instruments, particularly those employing array detectors like charge-coupled devices (CCDs) and photodiode arrays (PDAs).

Key Features and Advantages

Aberration Correction for Flat Imaging Planes
Unlike traditional gratings, flat-field gratings are engineered to minimize optical aberrations such as astigmatism and coma. This design ensures that dispersed spectra focus onto a flat plane, aligning seamlessly with planar detectors and eliminating the need for additional corrective optics. 

Concave Holographic Design
Many flat-field gratings utilize a concave holographic structure, combining dispersion and focusing capabilities within a single element. This integration simplifies optical systems, reduces component count, and enhances throughput by minimizing light losses .

High Spectral Resolution and Efficiency
These gratings are capable of delivering high spectral resolution across ultraviolet (UV), visible, and near-infrared (NIR) regions. Their design allows for efficient light dispersion, making them suitable for applications requiring precise wavelength discrimination .

Applications Across Industries

Spectroscopy and Analytical Instruments
Flat-field gratings are widely used in spectrometers and monochromators for chemical analysis, environmental monitoring, and material characterization. Their ability to produce undistorted spectra enhances the accuracy of quantitative measurements .

Hyperspectral and Raman Imaging
In hyperspectral imaging systems, these gratings facilitate the acquisition of spatial and spectral information simultaneously. Similarly, in Raman spectroscopy, they enable the detection of subtle spectral features, aiding in the identification of molecular compositions .

Compact and Portable Devices
The integration of dispersion and focusing functions allows for the development of compact spectroscopic devices, including miniature spectrometers and portable analytical tools. This compactness is particularly beneficial for field applications and point-of-care diagnostics .

Considerations and Limitations

While flat-field gratings offer numerous advantages, certain considerations must be addressed:

  • Customization Requirements: Designing gratings for specific applications may necessitate custom groove patterns and blaze angles, potentially increasing manufacturing complexity and cost.

  • Spectral Range Limitations: The efficiency of a grating is often optimized for a particular spectral region; thus, selecting the appropriate grating for the desired wavelength range is crucial.

  • Detector Compatibility: Ensuring that the grating's flat-field correction aligns with the detector's geometry is essential to achieve optimal performance.

Conclusion

Flat-field and imaging diffraction gratings are pivotal in advancing spectroscopic technologies, offering enhanced spectral resolution, reduced optical aberrations, and compact system integration. Their versatility and precision make them indispensable in various scientific and industrial applications, from environmental analysis to biomedical diagnostics. By understanding their features and aligning them with specific application requirements, users can leverage these gratings to achieve superior optical performance.

Did You know?

Flat field and imaging gratings are aberration-reduced concave gratings. The spectral images of the entrance slit are focused on a flat plane, so a flat detector array can detect the spectral intensity information simultaneously. This type of gratings is introduced by the holographic reading techniques. They have the important advantage of near stigmatic imaging, and hence are able to achieve maximum resolution and high photometric efficiency. Today, holographic reading is the most common solution for flat-field imaging. This is because classically ruled gratings are not capable of good imaging outside Rowland circle, and ruling of specially curved grooves by computer controlled engines or electron beams are much more expensive. Additionally improvement could be from delicate substrate design, and by having two different radii of curvature in the vertical and horizontal plane, astigmatism can be significantly reduced.