application brief AB20-5 replaces AN1149-5 Secondary Optics Design Considerations for SuperFlux LEDs Secondary optics are those optics which exist outside of the LED package, such as reflector cavities, Fresnel lenses, and pillow lenses. Secondary optics are used to create the desired appearance and beam pattern of the LED signal lamp. The following section details the optical characteristics and optical model creation for Lumileds SuperFlux LEDs. In addition, simple techniques to aid in the design of collimating reflectors, collimating lenses, and pillow lenses are discussed. Table of Contents Optical Characteristics of SuperFlux LEDs LED Light Output SuperFlux LED Radiation Patterns Optical Modeling of SuperFlux LEDs Point Source Optical Model Detailed Optical Models Secondary Optics Pillow Lens Design Design Case—Pillow Design for an LED CHMSL Non-symmetric Pillow Lenses Selecting the Size of the Pillow Optic Recommended Pillow Lens Prescriptions Other Diverging Optics Reflector Design Design Case—Reflector for a CHMSL Application Reflector Cavities with Linear Profiles Reflector Cavities with Square and Rectangular Exit Apertures Other Reflector Design Techniques Collimating Lens Design Fresnel Lens Design Design Case—Collimator Lens Other Lens Design Options Appendix 5A 2 2 2 3 3 4 5 9 9 11 11 12 13 14 14 15 15 16 17 18 19 19 21 Optical Characteristics of SuperFlux LEDs LED Light Output The light output of an LED is typically described Solid angle is used to describe the amount of by two photometric measurements, flux and angular space subtended. Angular space is intensity. described in terms of area on a sphere. If a solid angle ω, with its apex at the center of a sphere of In simple terms, flux describes the rate at which radius r, subtends an area A on the surface of light energy is emitted from the LED. Total flux that sphere, then ω = A/r2. The units for solid from an LED is the sum of the flux radiated in all angle are steradians (sr). directions. If the LED is placed at the center of a sphere, the total flux can be described as the To put some of these concepts into perspective, sum of the light incident over the entire inside consider the simple example of a candle. A surface of the sphere. The symbol for candle has an intensity of approximately one photometric for flux is Φv, and the unit of candela. A candle placed in the center of a measurement is the lumen (lm). sphere radiates light in a fairly uniform manner over the entire inner surface (ω = A/ r2 = 4π r2/ r2 = In simple terms, intensity describes the flux 4π steradians). With this information, the flux from density at a position in space. Intensity is the a candle can be calculated as shown below: flux per unit solid angle radiating from the LED source. The symbol for photometric intensity is Iv, and the unit of measurement is the candela (cd). SuperFlux LED Radiation Patterns The radiation pattern of an LED describes intensity, the radiation pattern becomes a how the flux is distributed in space. This is description of how the flux is distributed, accomplished by defining the intensity of the independent of the amount of flux produced. LED as a function of angle from the optical axis. Figure 5.1 shows a graph of the radiation pattern for an HPWA-Mx00 LED. Since the radiation pattern of most LEDs is rotationally symmetric about the optical axis, it An attribute of the radiation pattern that is of can be described by a simple, two-axis graph of common interest is known as the full-width, half- intensity versus angle from the optical axis. max, or 2θ1/2. This attribute describes the full Intensity is normalized in order to describe the angular width of the radiation pattern at the half relative intensity at any angle. By normalizing power, or half maximum intensity point. Looking at Figure 5.1, the 2θ1/2 of the HPWA-Mx00 LED Looking at Figure 5.2, the total included angle is is approximately 90°. approximately 95°. This implies that 90% of the flux produced by an HPWA-Mx00 LED is emitted Another attribute that is of common interest is within a 95° cone centered on the optical axis. the total included angle, or θv 0.9. This attribute describes the cone angle within which 90% of the total flux is radiated. Using Figure 5.1, the percent of total flux versus included angle can be calculated and graphed. (The derivation of this graph is shown in Appendix 5A.) This graph is included in the data sheet of SuperFlux LEDs and is shown in Figure 5.2 for the HPWA-Mx00 Figure 5.1 Graph of the radiation pattern for an HPWA-MxOO LED. LED. Optical Modeling of SuperFlux LEDs An optical model of the LED is useful when unacceptable when lenses or reflectors are designing secondary optic elements such as placed within 25 mm of the SuperFlux LED. A reflector cavities and pillow lenses. The optical more accurate technique involves using an output of an LED can be approximated as a optical model, which takes into account the point source of light passing through an extended source size of the LED. aperture, but modeling errors may be Point Source Optical Model The internal structure of a SuperFlux LED is shown in Figure 5.3. Light is produced in the LED chip. A portion of this light goes directly from the chip and is refracted by the epoxy dome (refracted-only light). The remainder of the light is reflected by the reflector cup and then refracted by the epoxy dome (reflectedrefracted light). Figure 5.2 Percent total flux vs. included angle for an HPWA-MxOO LED. The light that is refracted appears to come from and is not a point source, the refracted-only light a certain location within the LED, while the light does not appear to come from a single location, which is reflected and refracted appears to but a range of locations or a focal smear. This is come from a different location. In addition, true for the reflected-refracted light as well. because the LED chip itself has physical size 3 These focal smears overlap, creating an points source; and the aperture size should be elongated focal smear as shown in Figure 5.4. equal to that of the epoxy dome at its base as shown in Figure 5.5. To create the best approximation using a point source model, the center point of the focal The optimal position of the point source for each smears should be chosen as the location of the SuperFlux LED is shown in Table 5.1. Figure 5.3 Internal structure of a SuperFlux LED. Figure 5.4 Focal smear produced by reflected and reflected-refracted light. Detailed Optical Models Detailed optical models of LEDs include all surface, and the epoxy encapsulant must be the internal optical structures within the LED known. The process usually involves a tedious including the chip, the reflector, and the dome. trial and error technique of changing parameters In order to accurately construct such a model, in the model until empirical measurements are detailed information about the chip, the reflector matched. Table 5.1 Position of Point Source for SuperFlux LEDs SuperFlux LED Position of Point Source Part Number “Z” (mm) HPWA-MxOO HPWA-Dx00 HPWT-Mx00 HPWT-DxOO 1.03 1.13 0.99 1.17 Due to the complexity of this process, Lumileds can be used by many optical-modeling software Lighting provides customers with rayset files for packages. Contact your local Lumileds SuperFlux LEDs. The raysets contain spacial Applications Engineer for more information and and angular information on a set of rays exiting copies of the raysets. the device at the dome surface. These raysets 4 Secondary Optics This section contains practical design tools for optics), and those that gather the incoming light secondary optic design. More accurate and into a collimated beam (collimating optics). sophisticated techniques exist which are beyond the scope of this application note. The design The most common type of diverging optic used methods discussed here are proven, but no in automotive signal lamp applications is the analytical technique can completely replace pillow lens. The pillow lens spreads the incoming empirical testing. Designs should always be light into a more divergent beam pattern, and it prototyped and tested as early in the design breaks up the appearance of the source process as possible. resulting in a more uniform appearance. A cross section of an LED signal lamp with a pillow lens Secondary optics are used to modify the output is shown in Figure 5.6. beam of the LED such that the output beam of the finished signal lamp will efficiently meet the desired photometric specification. In addition, secondary optics serve an aesthetic purpose by determining the lit and unlit appearance of the signal lamp. The primary optic is included in the LED package, and the secondary optics are part of the finished signal lamp. There are two primary categories of secondary optics used, those that spread the incoming light (diverging Figure 5.5 Point source model of a SuperFlux LED. Figure 5.6 Cross section of an LED signal lamp with a pillow lens. Figure 5.7 Cross section of an LED signal lamp with a reflector cavity and pillow lens. 5 Figure 5.8 Cross section of an LED signal lamp with Fresnel and pillow lenses. As the spacing between the pillow and the LED signal lamp with a Fresnel lens and a pillow LEDs is increased, each LED will illuminate a lens is shown in Figure 5.8. larger area of the pillow lens. As the spot illuminated by each LED grows and as the In general, designs that use collimating adjacent spots begin to overlap, the lens will secondary optics are more efficient, and produce appear more evenly illuminated. The trade-off a more uniform lit appearance than designs between lamp depth and lit uniformity is a utilizing only pillow or other non-collimating common consideration in LED design, where optics. Fresnel lenses are a good choice for thin both unique appearance and space-saving lamp designs and produce a very uniform lit packages are desired. appearance. Reflectors are a good choice for thicker lamp designs and are more efficient than Collimating optics come in two main varieties: Fresnel lenses at illuminating non-circular areas. reflecting and refracting. Reflecting elements are This is because reflectors gather all of the light, typically metalized cavities with a straight or which is emitted as a circular pattern for most parabolic profile. A cross section of an LED SuperFlux LEDs, and redirect it into the desired signal lamp with a reflector cavity and a pillow shape. In addition, reflectors can be used to lens is shown in Figure 5.7. create a unique, “jeweled” appearance in both the on and off states. Refracting, collimating optics typically used in LED signal lamp applications include plano- The dependency of reflector height on reflector convex, dualconvex, and collapsed plano- efficiency will be covered later in this section. convex (Fresnel) lenses. A cross section of an Figure 5.9 Half-angle subtended by an individual pillow (A) for convex (upper) and concave (lower) pillow lenses. 6 Figure 5.10 Half-angle divergence of the input beam (B). Figure 5.11 Ideal radiation pattern produced by a pillow optic where A(n-1) > B. Figure 5.12 Ideal radiation pattern produced by a pillow optic where A(n-1) < B. Figure 5.13 Ideal input beam with halfangle divergence B. 7 Figure 5.14 Common form of the input beam with half-angle divergence B. Figure 5.15 Ideal vs. actual radiation patterns from a pillow lens. Table 5.2 CHMSL INTENSITY SPECIFICATION Vertical Test Points (degrees) 10 U 5U H 5D Horizontal Test Points (degrees) Minimum Luminous Intensity (cd) 8 16 8 16 25 25 25 16 16 25 25 25 16 16 25 25 25 16 10 L 8 5L V 5R 10 R Pillow Lens Design Consider a pillow lens where the half-angle The ideal radiation patterns shown in Figures subtended by and individual pillow is A as 5.11 and 5.12 assume that the input beam has shown in Figure 5.9, and the input beam has a box-like radiation pattern as shown in Figure a half-angle divergence B as shown in Figure 5.13. 5.10. However, in actual cases the input beam will The ideal radiation pattern generated would be have the characteristics of the Cosine form of as shown in Figure 5.11, where n is the index of the Lambertian as shown in Figure 5.14. refraction of the pillow lens material. It should be noted that Figure 5.11 is applicable when B is The differences between the ideal, box-like input smaller than A(n-1). This assumption is true for beam, and the more common Lambertian input most LED applications using a collimating beam result in changes to the final radiation secondary optic. pattern as shown in Figure 5.15. The magnitude of this deviation in the radiation pattern can be In cases where B is larger than A(n-1), which is estimated by evaluating the magnitude of the often the case when the LED is used without a input beam’s deviation from the ideal. This collimating optic, the ideal radiation pattern deviation from the ideal should be considered would be as shown in Figure 5.12. in the design of the pillow lens. Design Case—Pillow Design for an LED CHMSL Consider the case where a collimating secondary optic is used producing a beam divergence of B = 5° (B < A(n-1)) and similar to that shown in Figure 5.14. The pillow lens material is Polycarbonate which has an index of refraction of 1.59 (n = 1.59). The ideal CHMSL radiation pattern is shown in Figure 5.17 such that all the extreme points of the specification are satisfied. Figure 5.17 shows the predicted actual radiation pattern. Using a Center High Mounted Stop Lamp (CHMSL) as an example, we can see how the design techniques discussed previously can be used to determine an optimum value of A. The minimum intensity values for a CHMSL are shown in Table 5.2. As a conservative estimate, we can treat this pattern as symmetric about the most extreme points. The extreme points are those with the highest specified intensity values at the largest angular displacements from the center of the pattern. These points are shown in italics in Table 5.2. The angular displacement of a point from the center is found by taking the square root of the sum of the squares of the angular displacements in the vertical and horizontal directions. A point at 10R and 5U would have an angular displacement from the center of: From Figure 5.17, we can see that A(n-1)-B = 8°?and A(n-1)+B = 18°; therefore, A = 22°. The value of A selected will determine how much spread the pillow optic adds to the input beam. These points are charted on an intensity versus angle plot in Figure 5.16. 9 Figure 5.16 Extreme points on the CHMSL specification. Figure 5.17 Ideal and actual radiation patterns satisfying the extreme points of the CHMSL specifications. Figure 5.18 Toroidal pillow geometry. 10 Figure 5.19 Radiation pattern produced by a toroidal pillow (determine AV < Ah) Non-symmetric Pillow Lenses performance, provided the individual pillows are In our previous example, the CHMSL radiation small relative to the area illuminated by the light pattern was treated as if it were symmetric source. For incandescent designs, this is not an about its center. In this case, the radii of the issue and aesthetic considerations dictate the pillow were the same along the horizontal and pillow size. However, for LED designs, the light vertical axes, resulting in a spherical pillow. source is an array of individual LEDs. The pillow lens pitch must be small relative to the area In some signal lamps, the desired output beam illuminated by a single LED or the pillow will not is much wider along the horizontal axis than behave as designed. For this reason, pillows along the vertical axis. In these cases, the designed for LED applications typically have a optimum value of A will be larger for the pitch of 1 to 5 mm; where those designed for horizontal axis (Ah) than the vertical axis (Av). incandescents can be as large as 10 mm. The resulting geometry would be that of a circular toroid, which can be visualized as a Figure 5.20 shows a top view of a single pillow rectangular piece cut from a doughnut as with the pitches along both the horizontal, Ph , shown in Figure 5.18. and vertical, Pv, axes. In addition, the crosssection geometry through the center of the For non-symmetric pillow designs, an exercise primary axes is shown. similar to that performed for the CHMSL example must be performed for both the After Ah and Av have been calculated, and the vertical and horizontal axes in order to pitch has been chosen along one axis; the radii, determine Av and Ah. The resulting isocandela R, and pitch along the other axis can be plot of the radiation pattern will appear as determined by using the following equations: shown in Figure 5.19. (Note: Ph was chosen as a known value for this example.) Selecting the Size of the Pillow Optic After determining A for both axes, the next step is to determine the size, or pitch of the pillows. The pitch of the pillow typically does not effect 11 Recommended Pillow Lens Prescriptions case of the CHMSL, the desired output beam is Table 5.3 lists recommended pillow the same in the vertical and horizontal. In prescriptions (Ah & Av) for different signal lamp addition, for applications where no collimating applications. The pitch can be changed to suit secondary optic is used, the function of the by varying R as described in the previous pillow is to break up the appearance of the section. sources rather than spread the output beam. In these cases, a weak, symmetric prescription Examining Table 5.3, we observe that for pillow was chosen. CHMSL designs, a symmetric pillow prescription was chosen (Ah = Av). However, for The technique described above provides some the rear combination lamp/front turn signal practical tools for designing pillow lenses. If (RCL/FTS) application utilizing a collimating optical modeling software is available, along with optic, a non-symmetric pillow prescription was an accurate model of the LED source, these used (Ah > Av). The desired output beam pattern tools should be utilized to aid in the design for the RCL/FTS applications is twice as wide in process and provide more accurate models of the horizontal than in the vertical; whereas in the the final output beam. Table 5.3 RECOMMENDED PILLOW LENS PRESCRIPTIONS Application CHMSL LED Type HPWA-MHOO CHMSL HPWT-DHOO RCL/FTS HPWT-MxOO RCL/FTS HPWT-MxOO Collimating Optic Ah (deg) Av (deg) Rh (mm) Ph (mm) Rv (mm) Pv (mm) Fresnel Lens (B = 5°) None (B = 20°) Fresnel Lens (B = 7°) Reflector Cavity (B = 20°) 22 22 5.3 4 5.3 4 5 5 17 3 17 3 30 20 4.0 4 8.9 5.7 5 5 17 3 17 3 Figure 5.20 Geometry of a single pillow. 12 Figure 5.21 Cross-section geometry of a desired reflector cavity. Other Diverging Optics Pillow lenses are the most popular diverging example, diffuse lenses produce a uniform lit optic used in automotive signal lamps, however, appearance and a cloudy unlit appearance. Pillow other types exist which produce similar effects lenses can be diffused by bead-blasting the pillow but have different appearances. Alternate types lens surface on the mold tool resulting in a less of diverging optics include: diffuse lenses, efficient optic, but one that is more uniform in faceted lenses, rod lenses, and many others appearance when lit. including combinations of the above. For Figure 5.22 Geometry of a parabola. Figure 5.23 LED position relative to the parabola. Figure 5.24 Design of parabolic reflector with f = 0.66 mm. 13 Reflector Design Reflector cavities serve two main purposes: to the reflector. Once the parabola has been redirect the light from the LED into a useful designed, a cavity with a profile comprised of beam pattern, and to provide a unique multiple linear sections that closely approximates appearance for the finished lamp. Often the look the form of the parabola may be used depending sought after is not achievable by the most on the look desired. optically efficient design. As a result, there is a trade-off required between optical efficiency In order to accommodate the SuperFlux LED and lit appearance to arrive at an acceptable dome, the bottom aperture of the reflector must design. be greater than three-millimeters in diameter. Considering the tolerances of the molded As discussed in the previous section Point reflector, the LED, the LED alignment to the PCB, Source Optical Model, a parabola is designed and the alignment of the reflector to the PCB, the to collimate the light from the point source. For bottom reflector aperture should be a minimum of the design technique discussed here, the LED is 3.5 mm in diameter. The focal length of the treated as a point source. This treatment is very reflector must be greater than 0.5 mm to produce accurate for larger parabolas where the size of a bottom aperture of greater than 3.5 mm. the dome is small relative to the exit aperture of Design Case—Reflector for a CHMSL Application Consider the case where a reflector cavity will be used to collimate the light from an HPWT-MH00 source, and a pillow optic cover lens will be used to form the final radiation pattern. Vacuum-metalized ABS plastic will be used as the reflector material. The reflector cavity can be a maximum of 20 mm in height and should have a minimum opening for the LED dome of diameter 3.75mm to accommodate piecepart misalignment and tolerances. The LED spacing is 15 mm, and each cell must illuminate a 15 mm x 15 mm patch on the pillow lens. Figure 5.21 shows a cross-section of the lamp described above. The geometry of a parabola, in polar coordinates, is described by the following equation: Table 5.4 describes the profiles of three different parabolas (f = 0.9 mm, 0.7 mm, 0.66 mm). An efficient, practical collimator design for a CHMSL application should collimate all the light beyond 20°?from on axis (φ ≤ 20°). More efficient reflectors can be designed which collimate more of the light, but they are typically too deep to be of practical value. The ideal reflector for this application will have the following characteristics: Height constraint: 0.99 ≤ z ≤ 20 mm Figure 5.22 shows how the terms in this equation are applied. From Table 5.1, we find that the optimum point source location for the HPWT-MH00 LED is at Z = 0.99 mm. Placing the point source of the LED at the focus of the parabola will result in an LED position as shown in Figure 5.23. Fit of LED dome into bottom aperture:x (z = 0.99 mm) ≥?1.875 mm 15 mm pitch: x (Φ = 20°) ≅?7.5 mm Looking at Table 5.4, we find that the parabola with f = 0.66 mm most closely meets these requirements. Figure 5.24 gives the geometry of the parabolic reflector chosen. Since the base of the LED dome is above the location of the parabola’s focus, this implies that 2f < 1/2 base aperture = 3.75 mm/2 = 1.875 mm (f < 0.94 mm). This information will give us a starting point to begin searching for the optimum parabola. 14 Figure 5.25 shows the profiles of several practical reflector geometries (f = 0.5 to 1.0 Reflector Cavities with Square mm). It should be noted that in order to and Rectangular Exit Apertures produce a reflector with a cutoff angle less than The previous sections dealt with reflector cavities 20°, the height must increase radically. For this that are rotationally symmetric about the optical reason, reflectors with a high degree of axis, which result in round entrance and exit collimation (<20°) are often impractical. apertures. In some designs, it may be desirable to Therefore, Fresnel lenses are the preferred have a square or rectangular exit aperture in order method to produce highly collimated beams. In to more evenly illuminate a square or rectangular addition, it can be seen that reflectors with section of the cover lens. In this type of design, smaller focal lengths can produce a greater each axis of the reflector cavity must be analyzed degree of collimation in a shorter height, separately, using the techniques described in the however, the exit aperture also becomes previous section. smaller. It should be noted that these reflector cavities will Reflector Cavities with Linear Profiles produce beam patterns that are similar in shape After designing the appropriate parabolic to their exit aperture. Figure 5.27 compares the reflector, this form can be closely approximated beam patterns of the rotationally-symmetric by a few linear sections. Reflectors with linear parabolic reflector designed in the previous profiles require simpler mold tools and are example Design Case—Reflector for a CHMSL easier to measure and verify the accuracy of the Application to that of a reflector cavity with a form. Usually two linear sections are sufficient square exit aperture having the same wall profile. depending on the efficiency needed and the In this case, each side of the square exit aperture appearance that is sought. Figure 5.26 shows is equal in length to the diameter of the circular an approximation of the parabolic reflector from exit aperture of the parabolic design. the previous section, designed by a best fit of two linear sections. _ Figure 5.25 Comparison of Practical Parabolic Reflector Profiles. 15 Other Reflector Design Techniques rotationally symmetric reflectors by mapping the Many other methods exist to design reflectors flux contained within the source beam into the for LED sources. desired output beam. This method breaks the input beam into angular sections, each containing Nonimaging techniques focus on extracting light a known percentage of the total flux. It is then from the LED source and redirecting it such that determined at what angle each of these flux the exit beam has the desired divergence. The packets should be reflected to produce the most common form of a Nonimaging reflector desired output beam. The profile of the final used for LED applications is a truncated, reflector will consist of a series of straight compound parabolic collector (CPC). Several sections. As the number of flux packets publications explaining the principles of considered is increased, the number of steps in Nonimaging optics exist. One such text is High the reflector increases, until a smooth curve is Collection Nonimaging Optics by Welford & approximated. Winston, 1989. Detailed information on the reflector design Other reflector design techniques have been principles developed by William Elmer can be developed by William B. Elmer. One concept of found in The Optical Design of Reflectors by particular interest is a method for designing William Elmer, 1989. Figure 5.27 Isocandela plots of a circular vs. square reflector design. Figure 5.26 Linear profile approximation of a parabolic reflector (f = 0.66 mm). 16 Table 5.4 PROFILE GEOMETRY OF PARABOLAS (f = 0.9 mm, 0.7 mm, 0.66mm) f (mm) 0.9 0.70 0.66 Φ (deg.) Φ (rad.) r (mm) x (mm) (mm) 20 22 25 30 35 40 45 50 55 60 65 70 20 22 25 30 35 40 45 50 55 60 65 70 20 22 25 30 35 40 45 50 55 60 65 70 0.35 0.38 0.44 0.52 0.61 0.70 0.79 0.87 0.96 1.05 1.13 1.22 0.35 0.38 0.44 0.52 0.61 0.70 0.79 0.87 0.96 1.05 1.13 1.22 0.35 0.38 0.44 0.52 0.61 0.70 0.79 0.87 0.96 1.05 1.13 1.22 29.85 24.72 19.21 13.44 9.95 7.69 6.15 5.04 4.22 3.60 3.12 2.74 23.21 19.23 14.94 10.45 7.74 5.98 4.78 3.92 3.28 2.80 2.42 2.13 21.89 18.13 14.09 9.85 7.30 5.64 4.51 3.70 3.10 2.64 2.29 2.01 10.21 9.26 8.12 6.72 5.71 4.95 4.35 3.86 3.46 3.12 2.83 2.57 7.94 7.20 6.31 5.22 4.44 3.85 3.38 3.00 2.69 2.42 2.20 2.00 7.49 6.79 5.95 4.93 4.19 3.63 3.19 2.83 2.54 2.29 2.07 1.89 28.05 22.92 17.41 11.64 8.15 5.89 4.35 3.24 2.42 1.80 1.32 0.94 21.81 17.83 13.54 9.05 6.34 4.58 3.38 2.52 1.88 1.40 1.02 0.73 20.57 16.81 12.77 8.53 5.98 4.32 3.19 2.38 1.78 1.32 0.97 0.69 z Collimating Lens Design In this section we will deal with spherical lenses Where: and geometrical optics design techniques, f = focal length of the lens treating the LED as a point source of light. More n = index of refraction of the lens material sophisticated and accurate methods exist, but R1= radius of lens surface nearest the LED are beyond the scope of this application note. R2= radius of other lens surface T = thickness of the lens An LED signal lamp with a dual-convex, collimator lens is shown in Figure 5.28. The If T is less than one sixth of the diameter of the “lensmaker’s” formula for this arrangement lens, then this equation simplifies to: is shown below: 17 For thin lenses, it is a good approximation to A cross-section through the center of a plano- measure f from the center of the lens. convex lens, and its Fresnel counterpart are shown in Figure 5.32. For thin, plano-convex lenses (R1 = ∞), the equation further simplifies to: The thickness of the Fresnel lens is reduced as the number of steps is increased. Typically Fresnel lenses are designed with the minimum number of The above equations assume all rays arrive at steps needed to achieve the desired thickness, shallow angles with respect to the optical axis because additional light losses may occur at the (paraxial assumption). However, for SuperFlux internal faces and joining vertices. However, for LED applications, where much of the flux is plastic lenses, a thin design is desirable where contained at angles far from the optical axis, excessive lens thickness will result in sink this is not the case. As a result, rays which are distortions. Therefore, the performance and not close to the optical axis will be bent at too moldability of a lens are traded-off when choosing great an angle, a condition known as spherical the optimal number of steps. aberration. A correction factor, C, can be added to the above equations to compensate for this effect as shown below: For most LED collimator designs, a correction factor of C ≅ 1.35 will produce the best results. The value of f chosen can be checked by tracing a ray from the source to the outer edge of the collimator lens (edge ray). If the edge ray is under collimated, the value of C used is too Figure 5.28 Cross-section of an LED signal lamp using a dual-convex, collimator lens. large. If the edge ray is over collimated, the value of C used is too small. Figure 5.29 graphically depicts the edge ray method for checking f. Fresnel Lens Design A Fresnel lens can be visualized as a thick convex lens which has been collapsed about a series of circular, stepped setbacks. This type of lens takes on the properties of a much thicker lens and eliminates the difficulties involved with the manufacture of thick lenses. Figure 5.29 Edge ray method for checking f. 18 Design Case—Collimator Lens Consider the case where a lens will be used to collimate the light from an HPWT-DH00 source, and a pillow optic cover lens will be used to form the final radiation pattern. Clear PMMA (n = 1.49) will be used as the lens material. The LED spacing is 20 mm and the spacing from the top of the PCB to the top surface of the lens must be less than 25 mm. The total included angle of the HPWT-DH00 is 70°, therefore, to capture 90% of the light from the LED, the lens must span 35°?from the optical axis, and fill a 20 mm X 20 mm area. The combination of included angle, lamp depth, and LED spacing define the necessary items to determine f. Figure 5.30 shows a cross-section of the lamp described above. Examining the geometry shown in Figure 5.30, the desired focal length, f, is approximately 15.3mm. A lens of this power will be a dual-convex, and R1 and R2 can now be calculated using the following equation: To optimize collection efficiency, R1 must be greater than R2. By placing the flatter surface closer to the LED, the ray bending is more equally shared between the two lens surfaces. However, if R2 becomes too small, the lens will be too thick and difficult to manufacture. A good compromise between these two competing factors is R1 = 24 mm, and R2 = 18 mm. Figure 5.31 shows a cross-section of an LED signal lamp with this dual-convex lens design. Consider a case with a plano-convex lens (R = efficient than spherical forms. However, the 19mm) where an aperture diameter of 25 mm design of these types of lenses is more complex is desired for use as a collimating lens. This lens and generally requires optical modeling software will be too thick to properly injection mold and accurate optical models of the LED. (greater than 6 mm), so a Fresnel design will be used with a maximum height of 4 mm. The Another class of lens exists which couple the resulting design will have three steps, as shown principles of refraction and total internal reflection in Figure 5.32. (TIR). These lenses are commonly referred to as reflective/refractive, or catadioptric lenses. Lenses Convex-Fresnel lenses can be designed in designed by Fresnel over 100 years ago for light which a large radius (low curvature) lens is used houses contained such TIR faces for improved on the LED side, and a Fresnel-type lens with a efficiency. An example of a catadioptric lens is smaller radius (more curvature) is used on the shown in Figure 5.34. other side as shown in Figure 5.33. This type of lens is useful when refractive lens Other Lens Design Options designs cannot efficiently bend the light rays at In this section we have discussed only spherical the required angle. By combining reflection and lens designs. Spherical lenses are easily refraction into a single optical element, a very designed, specified, and checked; but may not powerful and efficient lens can be designed. TIR be the most efficient collimator due to spherical is most efficient when incident rays are nearly aberrations. Other lens designs, such as tangential, where as refraction is most efficient hyperbolic-planar, sphero-elliptic, and free-form when the rays are close to the normal. lenses can be designed which may be more 19 Figure 5.30 Cross-section of the desired LED lamp configuration. Figure 5.31 Cross-section of an LED signal lamp with a dual convex lens (R1 = 24mm, R2 = 18mm). Figure 5.32 Cross-section of a planoconvex lens and its Fresnel equivalent. Figure 5.33 Convex-Fresnel lens used as an LED collimator. Figure 5.34 Cross-section of a catadioptric lens used as an LED collimator. 20 Appendix 5A Flux Integration of Rotationally Symetric Radiation Patterns The cummulative flux as a function of angle Substituting Iv(θ) into (6) we get: from the optical axis (Figure 5.2) can be Φv(θ) calculated from the radiation pattern (Figure 5.1). This calculation is simple for rotationally ∫ = 2 π cosθ sinθ dθ = π sin2 θ (7) symetric radiation patterns and is shown below: Intensity is defined as the flux per unit solid angle, or This equation can be rearranged to solve for flux. Φv = Iv ω Φ v= (2) ∫ Iv d ω (3) Figure 5A.1 Graphic explanation of flux integration technique. Solid angle, ω, as a function of θ can be determined with the aid of Figure 5A.1. dω(θ) = 2 πτ sinθ dθ (4) Assigning a value of r=1, this equation becomes dω(θ) = 2 π sinθ dθ (4) and substituting (5) into (3) we can solve for Φv(θ). Φv(θ) = 2 π ∫ Iv (θ)sinθ dθ (6) Figure 5A.2 Rotationally symmetric, lambertian radiation pattern. Consider the case where the LED has a rotationally symetric, lambertian radiation pattern as shown in the Figure 5A.2. 21 The plot for equation (7) is shown in Figure 5A.3. By normalizing the Y-axis to 100% at 90°, this graph becomes that which is typically shown in the LED data sheets (Figure 5A.4). It should be noted that the data sheet refers to the X-axis as “Total Included Angle” which is equal to 2θ (see Figure 5A.1). Figure 5A.4 Percent cummulative flux vs. total included angle. For rotationally symetric radiation patterns that cannot be easily represented with functions, Simpson’s rule can be applied to approximate the integral. For example, the HPWT-MH00 radiation pattern cannot be easily described by a function. In such a case, the radiation pattern can be divided into a finite number of elements each with an angular width, dθ, as shown in Figure 5A.5. The smaller the dθ chosen, the larger n will become and the more accurate the approximation of the integral becomes. Applying Simpsons rule, we can approximate (6) by the following summation Figure 5A.5 Approximation of the HPWT-MH00 radiation pattern. As before, (8) can be plotted as shown in Figure 5A.6. Figure 5A.3 Graphic representation of Equation (7). Figure 5A.6 Graphic representation of equation (8). 22 Company Information Lumileds is a world-class supplier of Light Emitting Diodes (LEDs) producing billions of LEDs annually. Lumileds is a fully integrated supplier, producing core LED material in all three base colors (Red, Green, Blue) and White. Lumileds has R&D development centers in San Jose, California and Best, The Netherlands. Production capabilities in San Jose, California and Malaysia. Lumileds is pioneering the high-flux LED technology and bridging the gap between solid state LED technology and the lighting world. Lumileds is absolutely dedicated to bringing the best and brightest LED technology to enable new applications and markets in the Lighting world. LUMILEDS www.luxeon.com www.lumileds.com For technical assistance or the location of your nearest Lumileds sales office, call: Worldwide: +1 408-435-6044 US Toll free: 877-298-9455 Europe: +31 499 339 439 Fax: 408-435-6855 Email us at [email protected] 2002 Lumileds Lighting. All rights reserved. Lumileds Lighting is a joint venture between Agilent Technologies and Philips Lighting. Luxeon is a trademark of Lumileds Lighting, Inc. Product specifications are subject to change without notice. Publication No. AB20-5 (Sept2002) 23 Lumileds Lighting, LLC 370 West Trimble Road San Jose, CA 95131