VPH gratings can be reliably generated with higher line densities than ruled gratings, delivering high quality gratings with low ghosting and scatter at line densities ranging from 150 to near 5000 lines/mm, serving applications as diverse as broadband NIR hyperspectral imaging and high resolution atomic spectroscopy. The flexibility of our manufacturing process allows us to easily customize the line density and wavelength of operation for your needs.
Surface relief reflection gratings typically offer much lower efficiency for p-polarization than s-polarization, often with very different efficiency response between the two states. This is particularly evident as the line frequency of the grating increases. VPH gratings are far less sensitive to polarization, with the added benefit that the polarization response is both smoothly varying and well understood. We offer several design solutions, including our patented Dickson and HD gratings, which allow us to minimize and/or optimize polarization response specifically for your application.
A transmission grating is a very simple way to make an optical design more compact, as transmission gratings can be designed to work in the Littrow configuration (Ɵd = Ɵi). In general, transmission gratings offer the optical engineer more geometry options, whether designing a pulse compression system or a spectrometer. The net result is that a system designed around a Wasatch Photonics VPH grating is likely to be smaller, lighter and less expensive than one designed around a conventional reflection grating, in addition to being easier to align.
A grating sandwiched between two prisms is called a grism. This compound optic separates light into its components while canceling out the beam deviations caused by each element. Grisms can be used to either create a straight pass dispersive optic or an optic with dispersion higher than is possible with a grating alone. They are convenient for use in imaging, astronomy, spectrally encoded confocal microscopy, and other applications. Learn more about grisms.
VPH transmission gratings diffract light using stacked layers of sinusoidally varying index. This stack creates a resonant structure that can be tuned in center wavelength simply by varying the angle of incidence (AOI) by up to ~10°. This allows a single grating to be angle-tuned to study spectral features of interest in different ranges, a common technique in astronomy. In fact, several very large gratings on rotating stages may be used in a single large scale telescope to cover the visible through near infrared continuously.
Ruled gratings are prone to “ghosts”, a term used to describe light artefacts which appear in the dispersion plane due to periodic ruling errors. VPH gratings can be designed to eliminate ghosting. They also have 90% less stray light than ruled gratings, excellent spatial uniformity, and very low transmitted wavefront error. These factors are all important contributors to the excellent 1st order diffraction efficiency of VPH gratings.
The optically active portion of a VPH grating is sealed between 2 substrates, creating a very robust component that offers excellent thermal stability and environmental performance. Many of our gratings have been in service for 10+ years with no signs of degradation, while others have been deployed at near cryogenic temperatures. This allows our gratings to be used in a wide range of applications, from laser pulse compression, spectroscopy, and biomedical devices to astronomy.
Everyone knows never to touch a ruled, reflective grating, as they cannot be cleaned – every speck of dust or fingerprint must remain, as the scratching that would occur from “cleaning” would be worse than the contamination itself! In contrast, our encapsulated VPH gratings can be handled and cleaned like any other glass optical component, making them much more manufacturing-friendly and reducing cost at every stage, from build through long-term use.
Size & Substrates – Big & Small
VPH gratings can be made much larger than one might expect – in fact, we routinely manufacture custom gratings up to 300 mm in size for astronomical spectrographs (larger sizes upon request). They can also be cut to as small as 8 mm across for volume OEM applications. Many different types of glass materials may be used for manufacture, the most common substrates being N-BK7 or equivalent, B270i, and fused silica (UV optional).
We stand behind the quality of our optics with advanced interferometric measurement capabilities for critical applications like laser pulse compression, optical coherence tomography, and astronomy. Our metrology lab sports a new state of the art Zygo Verifire™ capable of measuring up to 4” optics!
When the founders of Wasatch Photonics began writing volume phase gratings in dichromated gelatin over 40 years ago, it was because they knew VPH grating technology had the performance, flexibility, and ability to scale from prototype to volume for a wide range of applications. Since then, we’ve worked hard to offer the quality and consistency you should expect from an experienced volume gratings supplier. Contact us to discuss your unique needs today!
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Wavelengths: 300-2500 nm | Bandwidth: 5-800 nm | Frequency: 150-5000 lines/mm