Equilateral Dispersive Prisms
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Our Dispersive Equilateral Prisms, which are fabricated from N-SF11, F2, CaF2, ZnSe, or Ge, are available in sizes ranging from 10 mm to 50 mm. These prisms create less stray light than diffraction gratings, thereby eliminating the higher order problems typically associated with gratings. Dispersive prisms are typically used at the minimum angle of deviation. This is the angle for which the wavelength of interest will travel parallel to the base of the prism, and the angle of incidence is equal to the angle of refraction when measured with respect to the normal of the prism face at the respective interface (see the Equilateral Tutorial tab for more information). At the minimum angle of deviation, a maximum clear aperture is achieved and reflective loss of P-polarized light is reduced since the angle of incidence is nearly Brewster's angle. For S-polarization, a custom antireflective coating can be used to minimize surface reflections. Please refer to the Prism Guide tab above for assistance in selecting the appropriate prism for your application, or to view Thorlabs' extensive line of prisms, please click here.
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| General Specifications |
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| Material | F2 | N-SF11 | CaF2 | ZnSe | Germanium |
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| Clear Aperture | 70% | | Surface Quality (Scratch-Dig) | 40-20 | 60-40 | | Angular Tolerance | ±5 arcmin | ±3 arcmin | ±10 arcmin | ±10 arcmin | | Number of Polished Faces | 2 (one face and the bases are fine ground) |
| Item # | A=B=C=H (mm) | Material | Minimum Angle of Deviation | Vd** | Surface Flattness @ 633 nm |
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| PS850 | 10 ± 0.15 | F2 | 47.9° @ 633 nm | 36.37 | λ/10 | | PS856 | 15 ± 0.1 | | PS858 | 20 ± 0.1 | | PS852 | 25 ± 0.1 | | PS854 | 50 ± 0.1 | | PS851 | 10 ± 0.15 | N-SF11* | 65.6° @ 633 nm | 25.76 | λ/10 | | PS857 | 15 ± 0.1 | | PS859 | 20 ± 0.1 | | PS853 | 25 ± 0.1 | | PS855 | 40 ± 0.1 | | PS862 | 10 +0.0/-0.3 | CaF2 | 31.6° @ 633 nm | 95.00 | λ/2 | | PS863 | 25 +0.0/-0.3 | | PS860 | 10 +0.0/-0.3 | ZnSe | N/A | N/A | λ/2 | | PS861 | 25 +0.0/-0.3 | | PS864 | 10 +0.0/-0.3 | Ge | N/A | N/A | λ/2 |
*N-SF11 stains easily. Clean off fingerprints quickly. **The Abbe number, Vd, is calculated by: Vd= (nd - 1) / (nF - nC), where nd, nF, and nC are the indices of refraction for the helium D-line (587.6 nm), the hydrogen F-line (486.1 nm), and the hydrogen C-line (656.3 nm). A lower Abbe number indicates more dispersion.  Click to Enlarge
Click Here to Download Index of Refraction Data
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| Material | Wavelength Range | Index of Refraction | Abbe Number |
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| F2 | 385 nm - 2 µm | 1.617 @ 633 nm | 36.37 | | N-SF11 | 420 nm - 2.3 µm | 1.779 @ 633 nm | 25.76 | | CaF2 | 180 nm - 8 µm | 1.433 @ 633 nm | 95.00 | | ZnSe | 600 nm - 16 µm | 2.403 @ 10.6 µm | N/A* | | Germanium | 2 - 16 µm | 4.004 @ 10.6 µm | N/A* |
| *Germanium and ZnSe are opaque at some or all visible wavelengths, and thus the Abbe number is undefined. |
N-SF11 and F2 Both N-SF11 and F2 both offer excellent performance in the visible range. When compared to each other, F2, which is a flint glass, has superior chemical resistance and better transmission than N-SF11. For instance, at 420 nm the theoretical internal transmittance of a 10 mm thick piece of F2 is 0.995, whereas for the same thickness of N-SF11, the internal transmittance is 0.910. If the glass is increased to a thickness of 25 mm, these internal transmission values decrease to 0.987 and 0.790, respectively. With high indices of refraction and low Abbe Numbers Vd, both N-SF11 and F2 provide maximum dispersive power. Calcium Flouride CaF2 is commonly used for applications requiring high transmission in the infrared and ultraviolet spectral ranges. The material exhibits a low refractive index, varying from 1.35 to 1.51 within its usage range of 180 nm to 8.0 µm, as well as an extremely high laser damage threshold. Calcium fluoride is also fairly chemically inert and offers superior hardness compared to its barium fluoride, magnesium fluoride, and lithium fluoride cousins. Zine Selenide Zinc Selenide is ideal fo use in the 600 nm 16 µm range. It features low absorption (including in the red visible wavelength range) and high resistance to thermal shock. ZnSe is ideal for use in CO2 laser systems operating at 10.6 µm, including those with HeNe alignment lasers. Please note that, due to its low hardness, care should be taken when handling ZnSe optics. Germanium Due to its broad transmission range (2 - 16 µm) and opacity in the visible portion of the spectrum, Germanium is well suited for IR applications. Germanium has a refractive index of over 4 in the 2 - 16 µm range (see the Index of Refraction tab for details). It is also inert to air, water, alkalis, and acids (except nitric acid). Germanium's transmission properties are highly temperature sensitive. Germanium is nearly opaque at 100 °C and completely non-transmissive at 200 °C.
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The index of refraction of various materials can be calculated via Sellmeier equations. Each material is empirically assigned a set of coefficients, through which the index of refraction can be calculated at any wavelength*. Sellmeier Equation 1:  Sellmeier Equation 4:  | Material** | K1 | L1 | K2 | L2 | K3 | L3 | λmin* (µm) | λmax* (µm) | Plot |
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| F2 | 1.345 | 9.977 x 10-3 | 2.091 x 10-1 | 4.705 x 10-2 | 9.374 x 10-1 | 1.119 x 102 | 0.32 | 2.5 |  | | N-SF11 | 1.737 | 1.319 x 10-2 | 3.137 x 10-1 | 6.231 x 10-2 | 1.899 | 1.552 x 102 | 0.37 | 2.5 |  | | CaF2 | 5.676 x 10-1 | 2.526 x 10-3 | 4.711 x 10-1 | 1.008 x 10-2 | 3.848 | 1.201 x 103 | 0.23 | 9.7 |  | | ZnSe | 4.298 | 3.689 x 10-2 | 6.278 x 10-1 | 1.435 x 10-1 | 2.896 | 2.208 x 103 | 0.55 | 18.0 |  |
| Material** | A | B | C | D | E | λmin* (µm) | λmax* (µm) | Plot |
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| Ge | 9.281 | 6.730 | 4.418 x 10-1 | 2.131 x 10-1 | 3.870 x 103 | 2.0 | 15.0 |  |
*The Sellmeier equation is only accurate within the wavelength range specified by λmin and λmax. **F2, N-SF11, CaF2, and ZnSe indices should be calculated using Sellmeier equation1, while the index of Ge should be calculated using sellmeier equation 4. Click Here to Download Index of Refraction Data
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Angle of Minimum Deviation Through a PrismIf one were to use ray tracing techniques to determine the light propagation path due to the presence of the equilateral prism shown to the right, you would find that for most incidence angles, the angle of deviation of the transmitted ray (denoted by γ in the figure to the right) is roughly the same, regardless of the angle of incidence considered. However, although the angle of deviation is largely unchanged, there is a minimum value that is obtainable. This angle is known as the minimum angle of deviation; it occurs when the light ray passing through the prism is parallel to the prism's base (as shown to the right), and therefore, = β (i.e., the angle of the light ray entering the prism is identical to that of the light ray exiting the prism). To illustrate the relationship between the incident, exit, and deviation angles in the triangle to the right, consider the equilateral triangle shown below, which is identical to the one shown to the right but has several more angles labeled. Using the geometric relationships that exist for vertical angles, it becomes apparant that A = - θ1 and C = β - θ2. Since the angles A, B, and C define a triangle, we know that A + B + C = 180o, and thus, B = 180o - (A + C) = 180o - [( - θ1) + (β - θ2)]. Finally, B + γ = 180o, so γ = 180o - B = [( - θ1) + (β - θ2)]. Now, consider the triangle outlined in green in the figure below. Here, (90 - θ1) + (90 - θ2) + 60o = 180o. Thus, θ1 + θ2 = 60o. Substituting this relationship into the end result derived in the previous paragraph, yields γ = + β - (θ1 + θ2) = + β - 60o. For the angle of minimum deviation, = β, so there is a simple relationship between the angle of incidence and the angle of minimum deviation: γ = + β - 60o = 2 - 60o By applying Snell's Law to the interfaces of prism and using a little calculus, a general equation for the relationship between the index of refraction of the equilateral prism n and the angle of minimum deviation γ can be obtained: 
At the design wavelength (633 nm), the indices of refraction for N-SF11 and F2 are 1.779 and 1.617, respectively. Solving for γ in the equation above yields 65.6o for N-SF11 and 47.9o for F2.
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Selection Guide for PrismsThorlabs offers a wide variety of prisms, which can be used to reflect, invert, rotate, disperse, steer, and collimate light. Prisms are available in N-BK7, UV Fused Silica, F2, N-SF11, α-BBO, N-KZFS8, Ge, and CaF2. For prisms and substrates not listed below, please contact tech support. Beam Steering Prisms| Prism | Material | Deviation | Invert | Reverse or Rotate | Illustration | Applications |
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| Right Angle Prisms | N-BK7, UV Fused Silica, Germanium, or Calcium Fluoride | 90° | 90° | No |  | 90° reflector, independent of entrance beam angle. Used in optical systems such as telescopes and periscopes. | | 180° | 180° | No |  | 180° reflector, independent of entrance beam angle. Acts as a non-reversing mirror and can be used in binocular configurations. | Retroreflectors and Mounted Retroreflectors | N-BK7 | 180° | 180° | No |  | 180° reflector, independent of entrance beam angle. Beam alignment and beam delivery. Substitute for mirror in applications where orientation is difficult to control. | Penta Prisms and Mounted Penta Prisms | N-BK7 | 90° | No | No |  | 90° reflector, without inversion or reversal of the beam profile. Can be used for alignment and optical tooling. | | Roof Prisms | N-BK7 | 90° | 90° | 180o Rotation |  | 90° reflector, inverted and rotated (deflected left to right and top to bottom). Can be used for alignment and optical tooling. | Dove Prisms and Mounted Dove Prisms | N-BK7 | No | 180° | 2x Prism Rotation |  | Dove prisms may invert, reverse, or rotate an image based on which face the light is incident on. Prism in a beam rotator orientation. | | 180° | 180° | No |  | Prism acts as a non-reversing mirror. Same properties as a retro-reflector or right angle (180° orientation) prism in an optical setup. | | Wedge Prisms | N-BK7 | Models Available from 2° to 10° | No | No |  | Beam steering applications. By rotating one wedged prism, light can be steered to trace the circle defined by 2 times the specified deviation angle. | | No | No |  | Variable beam steering applications. When both wedges are rotated, the beam can be moved anywhere within the circle defined by 4 times the specified deviation angle. | | Coupling Prisms | Rutile (TiO2) or GGG | Variable* | No | No |  | High index of refraction substrate used to couple light into films. Rutile used for nfilm > 1.8 GGG used for nfilm < 1.8 |
* Depends on angle of incidence and index of refraction Dispersive Prisms
| Prism | Material | Deviation | Invert | Reverse or Rotate | Illustration | Applications |
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| Equilateral Prisms | F2, N-SF11, Germanium, or Calcium Flouride | Variable* | No | No |  | Dispersion prisms are a substitute for diffraction gratings. Use to separate white light into visible spectrum. | | Pellin Broca Prisms | N-BK7, UV Fused Silica, or CaF2 | 90° | 90° | No |  | Ideal for wavelength separation of a beam of light, output at 90°. Used to separate harmonics of a laser or compensate for group velocity dispersion. | | Dispersion Compensating Prism Pairs | Fused Silica, CaF2, SF10, or N-SF14 | Variable Vertical Offset | No | No |  | Compensate for pulse broadening effects in ultrafast laser systems. Can be used as an optical filter, for wavelength tuning, or dispersion compensation. |
* Depends on angle of incidence and index of refraction Beam Manipulating Prisms| Prism | Material | Deviation | Invert | Reverse or Rotate | Illustration | Applications |
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| Anamorphic Prism Pairs | N-KZFS8 or N-SF11 | Variable Vertical Offset | No | No |  | Variable magnification along one axis. Collimating elliptical beams (e.g., laser diodes) Converts an elliptical beam into a circular beam by magnifying or contracting the input beam in one axis. |
Polarization Altering Prisms| Prism | Material | Deviation | Invert | Reverse or Rotate | Illustration | Applications |
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| Glan-Taylor, Glan-Laser, and α-BBO Glan-Laser Polarizers | Glan-Taylor: Calcite Glan-Laser: α-BBO or Calcite | p-pol. - 0° s-pol. - 112°* | No | No |  | Double prism configuration and birefringent calcite produce extremely pure linearly polarized light. Total Internal Reflection of s-pol. at the gap between the prism while p-pol. is transmitted. | | Rutile Polarizers | Rutile (TiO2) | s-pol. - 0° p-pol. absorbed by housing | No | No |  | Double prism configuration and birefringent rutile (TiO2) produce extremely pure linearly polarized light. Total Internal Reflection of p-pol. at the gap between the prisms while s-pol. is transmitted. | | Double Glan-Taylor Polarizers | Calcite | p-pol. - 0° s-pol. absorbed by housing | No | No |  | Triple prism configuration and birefringent calcite produce maximum polarized field over a large half angle. Total Internal Reflection of s-pol. at the gap between the prism while p-pol. is transmitted. | | Glan Thompson Polarizers | Calcite | p-pol. - 0° s-pol. absorbed by housing | No | No |  | Double prism configuration and birefringent calcite produce a polarizer with the widest field of view while maintaining a high extinction ratio. Total Internal Reflection of s-pol. at the gap between the prism while p-pol. is transmitted. | Wollaston Prisms Wollaston Polarizers | Calcite | Symmetric p-pol. and s-pol. deviation angle | No | No |  | Double prism configuration and birefringent calcite produce the widest deviation angle of beam displacing polarizers. s-pol. and p-pol. deviate symmetrically from the prism. Wollaston prisms are used in spectrometers and polarization analyzers. | | Beam Displacing Prisms | Calcite | 2.7 or 4.0 mm Beam Displacement | No | No |  | Single prism configuration and birefringent calcite separate an input beam into two orthogonally polarized output beams. s-pol. and p-pol. are displaced by 2.7 or 4.0 mm. Beam displacing prisms can be used as polarizing beamsplitters where 90o separation is not possible. | | Fresnel Rhomb Retarders | N-BK7 | Linear to circularly polarization Vertical Offset | No | No |  | λ/4 Fresnel Rhomb Retarder turns a linear input into circularly polarized output. Uniform λ/4 retardance over a wider wavelength range compared to birefringent wave plates. | | Rotates linearly polarized light 90° | No | No |  | λ/2 Fresnel Rhomb Retarder rotates linearly polarized light 90°. Uniform λ/2 retardance over a wider wavelength range compared to birefringent wave plates. |
* s-polarized light is not pure and contains some p-polarized reflections. Beamsplitter Prisms
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