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Ruled Plane Gratings

Reflective ruled diffraction grating is a kind of optical glass substrate composed of dense, equidistant parallel lines, and the surface is coated with aluminized, multi-layer dielectric or other reflective film, which can separate white light into various components through diffraction effect or combine several different spectral ...

Specifications

Substrate Material: NBK7, Fused Silica, Custom
Dimension: Custom
Groove Density: up to 2400l/mm
Blaze Wavelength: 250-3400nm optional
Diffraction Efficiency: up to 99%@1065±20nm
Fused Silica Gratings customized for your application

Specifications

Groove Density: 800 l/mm
Blaze Wavelength: 1840 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Fused Silica Gratings

Specifications

Groove Density: 1000 l/mm
Blaze Wavelength: 1550 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Fused Silica Gratings

Specifications

Groove Density: 800 l/mm
Blaze Wavelength: 1550 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Gratings customized for your application

Specifications

Groove Density: 800 l/mm
Blaze Wavelength: 1150 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Fused Silica Gratings

Specifications

Groove Density: 1000 l/mm
Blaze Wavelength: 1064 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Gratings for Pulse Compression

Specifications

Groove Density: 1000 l/mm
Blaze Wavelength: 1030 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Fused Silica Gratings

Specifications

Groove Density: 1200.5 l/mm
Blaze Wavelength: 975 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Gratings for Pulse Compression

Specifications

Groove Density: 1200.5 l/mm
Blaze Wavelength: 800 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
Fused Silica Gratings customized for your application

Specifications

Groove Density: 1000 l/mm
Blaze Wavelength: 810 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
High-Efficiency Gratings customized for your application

Specifications

Groove Density: 1379.3 l/mm
Blaze Wavelength: 450 nm
Substrate Material: Fused Silica
Dimension (Length): 137 mm
Dimension (Height): 56 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 30 l/mm
Blaze Wavelength: 30000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 90 mm
Dimension (Height): 90 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 20 l/mm
Blaze Wavelength: 45000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 76 mm
Dimension (Height): 76 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 1800 l/mm
Blaze Wavelength: 330 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 90 mm
Dimension (Height): 90 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 40 l/mm
Blaze Wavelength: 25000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 90 mm
Dimension (Height): 90 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 50 l/mm
Blaze Wavelength: 12000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 110 mm
Dimension (Height): 110 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 60 l/mm
Blaze Wavelength: 10000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 90 mm
Dimension (Height): 90 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 75 l/mm
Blaze Wavelength: 4000 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 110 mm
Dimension (Height): 110 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 100 l/mm
Blaze Wavelength: 450 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 110 mm
Dimension (Height): 110 mm
HORIBA Jobin Yvon has produced a wide range of ruled master gratings from which we manufacture high precision replicas. Dimensions of our high-precision replica gratings typically range from 25x25 mm up to 120x140 mm.

Specifications

Groove Density: 120 l/mm
Blaze Wavelength: 2500 nm
Substrate Material: Custom, Metallic, ULE, Zerodur, Fused Silica, NBK7, Pyrex
Dimension (Length): 110 mm
Dimension (Height): 110 mm

Ruled Plane Diffraction Gratings: Precision Tools for Spectral Analysis

Ruled plane diffraction gratings are fundamental optical components that disperse light into its constituent wavelengths. These gratings are created by mechanically etching a series of parallel grooves onto a flat substrate, typically using a diamond-tipped tool. The precise spacing and depth of these grooves determine the grating's ability to diffract light at specific angles, making them essential in various scientific and industrial applications.

Key Features and Advantages

High Diffraction Efficiency
One of the primary advantages of ruled plane gratings is their high diffraction efficiency, especially when designed with a specific blaze angle. The blaze angle is tailored to direct the maximum amount of diffracted light into a desired order at a particular wavelength, enhancing the grating's performance in targeted spectral regions. This makes them particularly suitable for applications requiring efficient light dispersion within narrow wavelength bands.

Customization and Versatility
The mechanical ruling process allows for a high degree of customization. Manufacturers can produce gratings with varying groove densities, blaze angles, and substrate materials to meet specific application requirements. This versatility ensures that ruled plane gratings can be optimized for tasks ranging from ultraviolet to infrared spectroscopy.

Robustness and Durability
Ruled gratings are known for their mechanical robustness. The physical grooves etched into the substrate provide a durable structure that can withstand various environmental conditions, making them suitable for both laboratory and field applications.

Applications Across Industries

Spectroscopy and Analytical Instruments
Ruled plane gratings are integral components in spectrometers and monochromators, where they disperse light into its spectral components for analysis. Their high efficiency and customizable parameters make them ideal for detecting and measuring specific wavelengths in chemical analysis, environmental monitoring, and material characterization.

Astronomy and Astrophysics
In astronomical instruments, such as telescopes and spectrographs, ruled gratings are used to analyze the light from celestial bodies. They help in determining the composition, temperature, and motion of stars and galaxies by dispersing their light into spectra.

Laser Systems and Telecommunications
Ruled gratings play a role in laser tuning and wavelength selection, ensuring that lasers emit at precise wavelengths necessary for various applications. In telecommunications, they assist in managing different wavelength channels in fiber-optic networks, enabling efficient data transmission.

Educational and Research Laboratories
Due to their relatively straightforward design and operation, ruled plane gratings are commonly used in educational settings to demonstrate the principles of light diffraction and interference. They also serve as essential tools in research laboratories for various optical experiments.

Considerations and Limitations

While ruled plane gratings offer numerous advantages, they are not without limitations. The mechanical ruling process can introduce imperfections, leading to increased stray light and reduced spectral purity compared to holographic gratings. Additionally, their efficiency can be polarization-dependent, which may affect performance in certain applications. Careful selection and alignment are necessary to mitigate these issues and achieve optimal results.

Conclusion

Ruled plane diffraction gratings are indispensable tools in the field of optics, offering high efficiency, customization, and durability. Their ability to disperse light with precision makes them valuable in a wide range of applications, from scientific research to industrial processes. By understanding their features and appropriate use cases, users can effectively harness the capabilities of ruled plane gratings to meet their specific optical needs.

Did You know?

Ruled plane diffraction gratings are produced by physically forming grooves on a reflective surface with a ruling engine. The distance between adjacent grooves and the angle they form with the substrate affect both the dispersion and efficiency of the grating. The first diffraction gratings made for commercial use were mechanically ruled. It was manufactured by burnishing grooves individually with a diamond tool against a thin coating of evaporated metal applied to a plane or concave surface. Today, several types of ruling engines are applied to produce gratings with low Rowland ghosts, high resolving power, and high efficiency uniformity. Ruled gratings can be blazed for specific wave lengths and are generally desired because of their high efficiency. They are often used in systems requiring high resolution, and comprise the majority of diffraction gratings used in spectroscopic instrumentation.