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Near-IR Ruled Reflective Diffraction Gratings


  • Gratings with 750 nm to 1600 nm Blaze Wavelengths
  • Higher Efficiencies than Holographic Gratings

GR50-0310

50 mm x 50 mm
1000 nm Blaze
Wavelength

GR25-0608

25 mm x 25 mm
750 nm Blaze
Wavelength

GR13-0616

12.7 mm x 12.7 mm
1600 nm Blaze
Wavelength

See the Gratings Tutorial Tab Below for Definitions and Equations

Related Items


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Selection Guide
Reflective Gratings
Ruled UV
Visible
Near IR
Mid IR
Holographic
Echelle
Transmission Gratings
UV
Visible
Near IR

Features

  • Blaze Wavelengths from 750 to 1600 nm
  • High Grating Efficiency of 60 to 80% at Blaze Wavelength
  • Low Ghosting, <0.5% of Parent Line
  • Aluminum Reflective Coating
  • Soda Lime Glass Substrate with 300 to 1200 Grooves/mm
  • Produced from Ruled Original

Thorlabs offers ruled diffraction gratings for use in the near-IR region. These gratings will have a relatively sharp efficiency peak about their blaze wavelength and are produced from ruled originals. They are offered with different blaze angles to suit a variety of applications in spectroscopy and analysis where high efficiency is of primary concern. For more information, please click on the Gratings Tutorial tab above. We also offer holographic gratings, which do not produce ghosting effects at the expense of efficiency. For information regarding the differences between grating types, please click on the Gratings Guide tab above.

Please note that these gratings are bare aluminum and do not contain an overcoat. However, custom MgFor gold coatings are available to protect the aluminum surface of the gratings. The gold coating offers high performance in the IR, while the MgFcoating offers the best protection; contact Tech Support for further details.


Click to Enlarge

Ruled Diffraction Grating Used in
Littrow Configuration (θi=γ)
(Note: 1st Order Beam is Collinear and Antiparallel to Incident Beam)

Mounts and Adapters

Thorlabs offers a variety of mounts and adapters for precise and stable mounting and aligning square optics. All of Thorlabs' gratings can be mounted directly into the KM100C Right-Handed or KM100CL Left-Handed Kinematic Rectangular Optic Mount. Gratings can also be mounted in one of three Kinematic Grating Mount Adapters which can be used with any of Thorlabs' Ø1" Mirror Mounts, including the POLARIS-K1 Ultra-Stable Kinematic Mirror Mount.

Warning

Optical gratings can be easily damaged by moisture, fingerprints, aerosols, or the slightest contact with any abrasive material. Gratings should only be handled when necessary and always held by the sides. Latex gloves or a similar protective covering should be worn to prevent oil from fingers from reaching the grating surface. No attempt should be made to clean a grating other than blowing off dust with clean, dry air or nitrogen. Solvents will likely damage the grating's surface.

Thorlabs uses a clean room facility for assembly of gratings into mechanical setups. If your application requires integrating the grating into a sub-assembly or a setup please contact Tech Support to learn more about our assembly capabilities.

Diffraction Gratings Tutorial

Diffraction gratings, either transmissive or reflective, can separate different wavelengths of light using a repetitive structure embedded within the grating. The structure affects the amplitude and/or phase of the incident wave, causing interference in the output wave. In the transmissive case, the repetitive structure can be thought of as many tightly spaced, thin slits. Solving for the irradiance as a function wavelength and position of this multi-slit situation, we get a general expression that can be applied to all diffractive gratings when = 0°,

Grating Equation 1

(1)

known as the grating equation. The equation states that a grating with spacing a will deflect light at discrete angles (theta sub m), dependent upon the value λ, where  is the order of principal maxima. The diffracted angle, theta sub m, is the output angle as measured from the surface normal of the grating. It is easily observed from Eq. 1 that for a given order m, different wavelengths of light will exit the grating at different angles. For white light sources, this corresponds to a continuous, angle-dependent spectrum.

 

Transmission Grating
Figure 1. Transmission Grating

Transmission Gratings

One popular style of grating is the transmission grating. This type of grating is created by scratching or etching a transparent substrate with a repetitive, parallel structure. This structure creates areas where light can scatter. A sample transmission grating is shown in Figure 1.

The transmission grating, shown in Figure 1, is comprised of a repetitive series of narrow-width grooves separated by distance a. The incident light impinges on the grating at an angle theta sub i, as measured from the surface normal. The light of order m exiting the grating leaves at an angle of theta sub m, relative to the surface normal. Utilizing some geometric conversions and the general grating expression (Eq. 1) an expression for the transmissive diffraction grating can be found:

Grating Equation 2

(2)

where both  and  are positive if the incident and diffracted beams are on opposite sides of the grating surface normal, as illustrated in the example in Figure 1. If they are on the same side of the grating normal,  must then be considered negative.

 

Reflective Grating
Figure 2. Reflective Grating

Reflective Gratings

Another very common diffractive optic is the reflective grating. A reflective grating is traditionally made by depositing a metallic coating on an optic and ruling parallel grooves in the surface. Reflective gratings can also be made of epoxy and/or plastic imprints from a master copy. In all cases, light is reflected off of the ruled surface at different angles corresponding to different orders and wavelengths. An example of a reflective grating is shown in Figure 2. Using a similar geometric setup as above, the grating equation for reflective gratings can be found:

Grating Equation 3

(3)

where is positive and is negative if the incident and diffracted beams are on opposite sides of the grating surface normal, as illustrated in the example in Figure 2. If the beams are on the same side of the grating normal, then both angles are considered positive.

Both the reflective and transmission gratings suffer from the fact that the zeroth order mode contains no diffraction pattern and appears as a surface reflection or transmission, respectively. Solving Eq. 2 for this condition, theta sub i = theta sub m, we find the only solution to be m=0, independent of wavelength or gratings spacing. At this condition, no wavelength-dependent information can be obtained, and all the light is lost to surface reflection or transmission.

This issue can be resolved by creating a repeating surface pattern, which produces a different surface reflection geometry. Gratings of this type are commonly referred to as blazed (or ruled) gratings. An example of this repeating surface structure is shown in Figure 3.

 

Blazed (Ruled) Gratings

Blazed Grating
Figure 4. Blazed Grating, 0th Order Reflection
Blazed Grating
Figure 3. Blazed Grating Geometry

The blazed grating, also known as the echelette grating, is a specific form of reflective or transmission diffraction grating designed to produce the maximum grating efficiency in a specific diffraction order. This means that the majority of the optical power will be in the designed diffraction order while minimizing power lost to other orders (particularly the zeroth). Due to this design, a blazed grating operates at a specific wavelength, known as the blaze wavelength.

The blaze wavelength is one of the three main characteristics of the blazed grating. The other two, shown in Figure 3, are a, the groove or facet spacing, and gamma, the blaze angle. The blaze angle gamma is the angle between the surface structure and the surface parallel. It is also the angle between the surface normal and the facet normal.

The blazed grating features geometries similar to the transmission and reflection gratings discussed thus far; the incident angle () and th order reflection angles () are determined from the surface normal of the grating. However, the significant difference is the specular reflection geometry is dependent on the blaze angle, gamma, and NOT the grating surface normal. This results in the ability to change the diffraction efficiency by only changing the blaze angle of the grating.

The 0th order reflection from a blazed grating is shown in Figure 4. The incident light at angle theta sub i is reflected at theta sub m for m = 0. From Eq. 3, the only solution is theta sub i = –theta sub m. This is analogous to specular reflection from a flat surface.

Blazed Grating
Figure 6. Blazed Grating, Incident Light Normal to Grating Surface
Blazed Grating
Figure 5. Blazed Grating, Specular Reflection from Facet

The specular reflection from the blazed grating is different from the flat surface due to the surface structure, as shown in Figure 5. The specular reflection, theta sub r, from a blazed grating occurs at the blaze angle geometry. This angle is defined as being negative if it is on the same side of the grating surface normal as theta sub i. Performing some simple geometric conversions, one finds that

Grating Equation 2

(4)

Figure 6 illustrates the specific case where theta sub i= 0°, hence the incident light beam is perpendicular to the grating surface. In this case, the 0th order reflection also lies at 0°. Utilizing Eqs. 3 and 4, we can find the grating equation at twice the blaze angle:

Grating Equation 2

(5)

Littrow Configuration

The Littrow configuration refers to a specific geometry for blazed gratings and plays an important role in monochromators and spectrometers. It is the angle  at which the grating efficiency is the highest. In this configuration, the angle of incidence of the incoming and diffracted light are the same, theta sub i = theta sub m, and m > 0 so

Grating Equation 2

(6)

Blazed Grating
Figure 7. Littrow Configuration

The Littrow configuration angle, Theta sub L, is dependent on the most intense order (m = 1), the design wavelength, lambda sub D, and the grating spacing a. It is easily shown that the Littrow configuration angle, Theta sub L, is equal to the blaze angle, gamma, at the design wavelength. The Littrow / blaze angles for all Thorlabs' Blazed Gratings can be found in the grating specs tables.

Grating Equation 2

(7)

It is easily observed that the wavelength dependent angular separation increases as the diffracted order increases for light of normal incidence (for theta sub i= 0°, theta sub m increases as m increases). There are two main drawbacks for using a higher order diffraction pattern over a low order one: (1) a decrease in efficiency at higher orders and (2) a decrease in the free spectral range, Free Spectral Range, defined as:

Grating Equation 2

(8)

 

where lambda is the central wavelength, and m is the order.

The first issue with using higher order diffraction patterns is solved by using an Echelle grating, which is a special type of ruled diffraction grating with an extremely high blaze angle and relatively low groove density. The high blaze angle is well suited for concentrating the energy in the higher order diffraction modes. The second issue is solved by using another optical element: grating, dispersive prism, or other dispersive optic, to sort the wavelengths/orders after the Echelle grating.

 

Holographic Gratings
Figure 8. Holographic Grating

Holographic Surface Gratings

While blazed gratings offer extremely high efficiencies at the design wavelength, they suffer from periodic errors, such as ghosting, and relatively high amounts of scattered light, which could negatively affect sensitive measurements. Holographic gratings are designed specially to reduce or eliminate these errors. The drawback of holographic gratings compared to blazed gratings is reduced efficiency.

Holographic gratings are made from master gratings by similar processes to the ruled grating. The master holographic gratings are typically made by exposing photosensitive material to two interfering laser beams. The interference pattern is exposed in a periodic pattern on the surface, which can then be physically or chemically treated to expose a sinusoidal surface pattern. An example of a holographic grating is shown in Figure 8.

Please note that dispersion is based solely on the number of grooves per mm and not the shape of the grooves. Hence, the same grating equation can be used to calculate angles for holographic as well as ruled blazed gratings.

Thorlabs offers 4 types of Diffraction Gratings:

PhotoTypeDescription
Reflective Gratings
Ruled UV Ruled gratings can achieve higher efficiencies than holographic gratings due to their blaze angles. They are ideal for applications centered near the blaze wavelength. Thorlabs offers replicated ruled diffraction gratings in a variety of sizes and blaze angles.
Visible
Near IR
Mid IR
Holographic Holographic gratings have a low occurrence of periodic errors, which results in limited ghosting, unlike ruled gratings. The low stray light of these gratings makes them ideal for applications where the signal-to-noise ratio is critical, such as Raman Spectroscopy.
Echelle Echelle gratings are low period gratings designed for use in high diffraction orders. They are generally used with a second grating or prism to separate overlapping diffracted orders. They are ideal for applications such as high-resolution spectroscopy.
Transmission Gratings
UV Thorlabs' transmission gratings disperse incident light on the opposite side of the grating at a fixed angle. They are ruled and blazed for optimum efficiency in their respective wavelength range, are relatively polarization insensitive, and have an efficiency comparable to that of a reflection grating optimized for the same wavelength. They are ideal for applications that require fixed gratings such as spectrographs.
Visible
Near IR

Selecting a grating requires consideration of a number of factors, some of which are listed below:

Efficiency:
Ruled gratings generally have a higher efficiency than holographic gratings. However, holographic gratings tend to have less efficiency variation across their surface due to how the grooves are made. The efficiency of ruled gratings may be desirable in applications such as fluorescence excitation and other radiation-induced reactions.

Blaze Wavelength:
Ruled gratings have a sawtooth groove profile created by sequentially etching the surface of the grating substrate. As a result, they have a sharp peak around their blaze wavelength. Holographic gratings are harder to blaze, and tend to have a sinusoidal groove profile resulting in a less intense peak around the design wavelength. Applications centered around a narrow wavelength range could benefit from a ruled grating blazed at that wavelength.

Wavelength Range:
Groove spacing determines the optimum spectral range a grating covers and is the same for ruled and holographic gratings having the same grating constant. As a rule of thumb, the first order efficiency of a grating decreases by 50% at 0.66λB and 1.5λB, where λB is the blaze wavelength. Note: No grating can diffract a wavelength greater than 2 times the groove period.

Stray Light:
Due to a difference in how the grooves are made, holographic gratings have less stray light than ruled gratings. The grooves on a ruled grating are machined one at a time which results in a higher frequency of errors. Holographic grooves are made all at once which results in a grating that is virtually free of errors. Applications such as Raman spectroscopy, where signal-to-noise is critical, can benefit from the limited stray light of the holographic grating.

Resolving Power:
The resolving power of a grating is a measure of its ability to spatially separate two wavelengths. It is determined by applying the Rayleigh criteria to the diffraction maxima; two wavelengths are resolvable when the maxima of one wavelength coincides with the minima of the second wavelength. The chromatic resolving power (R) is defined by R = λ/Δλ = n*N, where Δλ is the resolvable wavelength difference, n is the diffraction order, and N is the number of grooves illuminated.

For further information about gratings and selecting the grating right for your application, please visit our Gratings Tutorial.

Caution:

The surface of a diffraction grating can be easily damaged by fingerprints, aerosols, moisture or the slightest contact with any abrasive material. Gratings should only be handled when necessary and always held by the sides. Latex gloves or a similar protective covering should be worn to prevent oil from fingers from reaching the grating surface. Solvents will likely damage the grating's surface. No attempt should be made to clean a grating other than blowing off dust with clean, dry air or nitrogen. Scratches or other minor cosmetic imperfections on the surface of a grating do not usually affect performance and are not considered defects.


Posted Comments:
liyonghong6  (posted 2017-08-16 11:28:23.113)
can you offer the reflective grating which polarization independent
tfrisch  (posted 2017-09-07 09:24:46.0)
Hello, thank you for contacting Thorlabs. Metal coatings will always have a difference in performance between the S and P polarization states. I will reach out to you directly about the needs of your application.

750 nm Blaze Wavelength Reflective Diffraction Gratings

Item # Dimensions (W x H x D) Blaze
Wavelength
Grooves/mm Blaze Angle Dispersion Efficiency
Curvesa,b
GR13-0608 12.7 mm x 12.7 mm x 6 mm 750 nm 600 13° 0' 1.62 nm/mrad Efficiency Plot
GR25-0608 25 mm x 25 mm x 6 mm
GR50-0608 50 mm x 50 mm x 9.5 mm
GR13-1208 12.7 mm x 12.7 mm x 6 mm 1200 26° 44' 0.74 nm/mrad Efficiency Plot
GR25-1208 25 mm x 25 mm x 6 mm
GR50-1208 50 mm x 50 mm x 9.5 mm
  • All gratings utilize an aluminum reflective coating. The efficiency data is measured in the Littrow mounting configuration and provided for reference only. Actual grating efficiency is 60 to 80% at the blaze wavelength.
  • For diffraction gratings, parallel and perpendicular polarization are defined with respect to the lines of the grating.
Based on your currency / country selection, your order will ship from Newton, New Jersey  
+1 Qty Docs Part Number - Universal Price Available / Ships
GR13-0608 Support Documentation
GR13-0608Ruled Reflective Diffraction Grating, 600/mm, 750 nm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-0608 Support Documentation
GR25-0608Ruled Reflective Diffraction Grating, 600/mm, 750 nm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-0608 Support Documentation
GR50-0608Ruled Reflective Diffraction Grating, 600/mm, 750 nm Blaze, 50 x 50 x 9.5 mm
$192.78
Today
GR13-1208 Support Documentation
GR13-1208Ruled Reflective Diffraction Grating, 1200/mm, 750 nm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-1208 Support Documentation
GR25-1208Ruled Reflective Diffraction Grating, 1200/mm, 750 nm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-1208 Support Documentation
GR50-1208Ruled Reflective Diffraction Grating, 1200/mm, 750 nm Blaze, 50 x 50 x 9.5 mm
$192.78
Today

1 µm Blaze Wavelength Reflective Diffraction Gratings

Item # Dimensions (W x H x D) Blaze
Wavelength
Grooves/mm Blaze Angle Dispersion Efficiency
Curvesa,b
GR13-0310 12.7 mm x 12.7 mm x 6 mm 1 µm 300 8° 36' 3.30 nm/mrad Efficiency Plot
GR25-0310 25 mm x 25 mm x 6 mm
GR50-0310 50 mm x 50 mm x 9.5 mm
GR13-0610 12.7 mm x 12.7 mm x 6 mm 600 17° 27' 1.59 nm/mrad Efficiency Plot
GR25-0610 25 mm x 25 mm x 6 mm
GR50-0610 50 mm x 50 mm x 9.5 mm
GR13-1210 12.7 mm x 12.7 mm x 6 mm 1200 36° 52' 0.67 nm/mrad Efficiency Plot
GR25-1210 25 mm x 25 mm x 6 mm
GR50-1210 50 mm x 50 mm x 9.5 mm
  • All gratings utilize an aluminum reflective coating. The efficiency data is measured in the Littrow mounting configuration and provided for reference only. Actual grating efficiency is 60 to 80% at the blaze wavelength.
  • For diffraction gratings, parallel and perpendicular polarization are defined with respect to the lines of the grating.
Based on your currency / country selection, your order will ship from Newton, New Jersey  
+1 Qty Docs Part Number - Universal Price Available / Ships
GR13-0310 Support Documentation
GR13-0310Ruled Reflective Diffraction Grating, 300/mm, 1 µm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-0310 Support Documentation
GR25-0310Ruled Reflective Diffraction Grating, 300/mm, 1 µm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-0310 Support Documentation
GR50-0310Ruled Reflective Diffraction Grating, 300/mm, 1 µm Blaze, 50 x 50 x 9.5 mm
$192.78
Today
GR13-0610 Support Documentation
GR13-0610Ruled Reflective Diffraction Grating, 600/mm, 1 µm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-0610 Support Documentation
GR25-0610Ruled Reflective Diffraction Grating, 600/mm, 1 µm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-0610 Support Documentation
GR50-0610Ruled Reflective Diffraction Grating, 600/mm, 1 µm Blaze, 50 x 50 x 9.5 mm
$192.78
Today
GR13-1210 Support Documentation
GR13-1210Ruled Reflective Diffraction Grating, 1200/mm, 1 µm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-1210 Support Documentation
GR25-1210Ruled Reflective Diffraction Grating, 1200/mm, 1 µm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-1210 Support Documentation
GR50-1210Ruled Reflective Diffraction Grating, 1200/mm, 1 µm Blaze, 50 x 50 x 9.5 mm
$192.78
Today

1.25 µm Blaze Wavelength Reflective Diffraction Gratings

Item # Dimensions (W x H x D) Blaze
Wavelength
Grooves/mm Blaze Angle Dispersion Efficiency
Curvesa,b
GR25-0613 25 mm x 25 mm x 6 mm 1.25 µm 600 22° 1' 1.55 nm/mrad Efficiency Plot
GR50-0613 50 mm x 50 mm x 9.5 mm
  • All gratings utilize an aluminum reflective coating. The efficiency data is measured in the Littrow mounting configuration and provided for reference only. Actual grating efficiency is 60 to 80% at the blaze wavelength.
  • For diffraction gratings, parallel and perpendicular polarization are defined with respect to the lines of the grating.
Based on your currency / country selection, your order will ship from Newton, New Jersey  
+1 Qty Docs Part Number - Universal Price Available / Ships
GR25-0613 Support Documentation
GR25-0613Ruled Reflective Diffraction Grating, 600/mm, 1.25 µm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-0613 Support Documentation
GR50-0613Ruled Reflective Diffraction Grating, 600/mm, 1.25 µm Blaze, 50 x 50 x 9.5 mm
$192.78
Today

1.6 µm Blaze Wavelength Reflective Diffraction Gratings

Item # Dimensions (W x H x D) Blaze
Wavelength
Grooves/mm Blaze Angle Dispersion Efficiency
Curvesa,b
GR13-0616 12.7 mm x 12.7 mm x 6 mm 1.6 µm 600 28° 41' 1.46 nm/mrad Efficiency Plot
GR25-0616 25 mm x 25 mm x 6 mm
GR50-0616 50 mm x 50 mm x 9.5 mm
  • All gratings utilize an aluminum reflective coating. The efficiency data is measured in the Littrow mounting configuration and provided for reference only. Actual grating efficiency is 60 to 80% at the blaze wavelength.
  • For diffraction gratings, parallel and perpendicular polarization are defined with respect to the lines of the grating.
Based on your currency / country selection, your order will ship from Newton, New Jersey  
+1 Qty Docs Part Number - Universal Price Available / Ships
GR13-0616 Support Documentation
GR13-0616Ruled Reflective Diffraction Grating, 600/mm, 1.6 µm Blaze, 12.7 x 12.7 x 6 mm
$67.07
Today
GR25-0616 Support Documentation
GR25-0616Ruled Reflective Diffraction Grating, 600/mm, 1.6 µm Blaze, 25 x 25 x 6 mm
$110.16
Today
GR50-0616 Support Documentation
GR50-0616Ruled Reflective Diffraction Grating, 600/mm, 1.6 µm Blaze, 50 x 50 x 9.5 mm
$192.78
Today
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