Importing Rayfiles of LEDs from OSRAM Opto Semiconductors Application Note
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1 Importing Rayfiles of LEDs from OSRAM Opto Semiconductors Application Note Introduction Optical simulation software typically propagates light through an optical system by ray tracing. Light sources can be defined which emit rays from their surfaces or volumes. Many software packages accept rayfiles, which are virtual sources created from measured or calculated sources. Each ray in the file has a starting point, a direction, and associated power. Some optical design software packages can additionally use wavelength information for the individual rays or consider an overall spectrum. OSRAM Opto Semiconductors provides rayfiles in several software formats. The properties of those rayfiles are described in this application note. Rayfile Generation by Near Field Measurement For the generation of rayfiles by measurement, a near field goniometer is used. Basic principle of this method is a Luminance camera on a moving arm, looking at the LED sample. The camera scans the upper hemisphere typically in a polar angular range of ~+/- 100 and a typical resolution <1 in polar as well as in azimuthal direction. At each position of the camera a Luminance picture is taken. A software algorithm evaluates the picture and generates rays according to the grabbed spatial Luminance and the angular position of the camera. Rayfile Import Process Rayfiles can be found on the homepage ( of OSRAM Opto Semiconductors under Application Support in the section Application. Selecting the link Optical Simulation / Rayfiles forwards you to the page labeled Optical Simulation with the two subfolders IR and LED and also to the Disclaimer and User Agreement file. The subfolders list the different product types of the respective application area. After selecting the group of interest discrete LED names are shown, which are in parallel the links to the individual rayfiles. There are several formats available. Click on the desired link, read and agree to the disclaimer, then Save the file to your computer. (These are large files and can take some time to download. Since the time to Open or Save is roughly the same, Save is recommended). Each *.zip file contains: Rayfiles A file depicting the orientation of the rayfiles vs. the LED package CAD files (for mechanical package study only) spectrum files When you open the *.zip file, you will see ray files of three different sizes: 100,000 (100k), 500,000 (500k), and 5,000,000 (5M) rays. If larger ray numbers are needed, contact your OSRAM Opto Semiconductors representative. Next, refer to the file depicting the orientation of the rayfiles (named *_info.pdf). You will see a mechanical drawing of the LED, with an (x,y,z) axis system February, 2013 Page 1 of 5
2 superimposed. This shows the orientation and location of the LED with respect to original coordinate system. Before using the rayfiles in your software, consider the following: If an optic needs to be designed around the LED, the best focus location has to be calculated. The procedure for doing this depends on the software package. The source lumens for most rayfiles are set to 1 lumen (the exception are rayfiles in SPEOS format). The OSRAM Opto Semiconductors rayfiles are made such that the starting points of the rays in the rayfile must be in air. The rayfile packages provided for Zemax and Lighttools contain a sample file / library element, which includes all necessary settings to start an optical simulation. The documentation file contains also an info about the virtual focus of the specific rayfile. For OSRAM Opto Semiconductors rayfiles this virtual focus is defined as the point, where all rays of the rayset have closest distance in 3D space. For the calculation of the coordinates given, all rays are used. Additional Considerations for White LED Rayfiles The spectra of OSRAM Opto Semiconductors white LEDs have two local maxima due to the specific generation of white light. The peak in the blue wavelength range has narrow width and a peak wavelength around 460nm; the peak in the yellow wavelength range has a wide distribution with a peak wavelength around nm, depending on the LED type. Figure 1: Typical radiometric spectrum for a white OSRAM LED. February, 2013 Page 2 of 5
3 Figure 2: Typical photometric spectrum for a white OSRAM LED. Due to the different angular characteristics of rays in the blue and yellow parts of the spectrum, a separation of the ray model into two parts is done. Therefore, two rayfiles are delivered with each white LED, one rayfile for the blue and one rayfile for the yellow part of the spectrum. Both rayfiles have the same global coordinate origin and must be placed in the simulation software at exactly the same (x,y,z) coordinates. To use the rayfiles in a simulation the user has to consider the following points: "blue" and "yellow" rayfiles must be placed at the same (x,y,z) coordinates simulation should run simultaneously for the two rayfiles, like for two overlapping sources luminous flux contributions of both rayfiles must be set appropriately The luminous flux ratio between yellow and blue depends on the type of conversion material used for the specific LED. In addition, the ratio varies slightly for different color bins. Recommended luminous flux ratios are given in the *info.pdf. To enable the user to make optical simulations for different color bins, ratios for some representative bins are given. Besides the flux ratio, the user has to import the related color spectra. Spectrum files are provided also in the rayfile *.zip packages. It should be emphasized, that there exists no bidirectional relationship between a color spectrum and a certain color point, e.g. in terms of CIE chromaticity coordinates Cx/Cy. A certain color point can be generated with different color spectra. Therefore, the provided color spectrum files are only exemplary and do not guarantee, that a LED delivered for a color bin has exactly the spectrum shown in the rayfile package. February, 2013 Page 3 of 5
4 Spectral Data Spectrum files are provided in all rayfile packages as ASCII files. For white LEDs the spectrum is split up in a blue and yellow part, so two files are given in that case. For the SPEOS format the spectrum is already included in the rayset. Some optical design software packages do not support the simulation of the complete color spectrum, but only single wavelengths. In that case, it is recommended to use the peak wavelength. For a white LED, the peak wavelength of the blue part of the spectrum should be used for the blue rayfile, and the peak wavelength of the yellow part of the spectrum should be used with the yellow rayfile. Please have a look at the related spectrum file to identify the peak wavelength of the specific LED. Import Procedure Summary 1. Download *zip file with rayfiles and supporting documentation from OSRAM website. 2. Confirm the origin and orientation of the rayfiles from the orientation file. 3. Import the appropriate rayfiles into your optical software. (If using a white LED, import a blue and a yellow file with the same number of rays). For Zemax and Lighttools it is recommended to use the provided sample / library files. 4. Set the source lumens to desired value. (If using a white LED, set the lumen ratio of yellow to blue). 5. Enter appropriate spectral information. Figure 3: Sharp division of the radiometric spectrum for a white OSRAM LED into blue and yellow parts. February, 2013 Page 4 of 5
5 Authors: Christopher Eichelberger, Ulrich Streppel, Andreas Stich About OSRAM Opto Semiconductors OSRAM AG (Munich, Germany) is a wholly-owned subsidiary of Siemens AG and one of the two leading light manufacturers in the world. Its subsidiary, OSRAM Opto Semiconductors GmbH in Regensburg (Germany), offers its customers solutions based on semiconductor technology for lighting, sensor and visualization applications. OSRAM Opto Semiconductors has production sites in Regensburg (Germany) and Penang (Malaysia). Its headquarters for North America is in Sunnyvale (USA), and for Asia in Hong Kong. OSRAM Opto Semiconductors also has sales offices throughout the world. For more information go to DISCLAIMER PLEASE CAREFULLY READ THE BELOW TERMS AND CONDITIONS BEFORE USING THE INFORMATION. IF YOU DO NOT AGREE WITH ANY OF THESE TERMS AND CONDITIONS, DO NOT USE THE INFORMATION. The Information shown in this document was produced with due care, but is provided by OSRAM Opto Semiconductors GmbH as is and without OSRAM Opto Semiconductors GmbH assuming, express or implied, any warranty or liability whatsoever, including, but not limited to the warranties of correctness, completeness, merchantability, fitness for a particular purpose, title or non-infringement. In no event shall OSRAM Opto Semiconductors GmbH be liable - regardless of the legal theory - for any direct, indirect, special, incidental, exemplary, consequential, or punitive damages related to the use of the Information. This limitation shall apply even if OSRAM Opto Semiconductors GmbH has been advised of possible damages. As some jurisdictions do not allow exclusion of certain warranties or limitations of liability, the above limitations or exclusions may not apply. The liability of OSRAM Opto Semiconductors GmbH would in such case be limited to the greatest extent permitted by law. OSRAM Opto Semiconductors GmbH may change the Information at anytime without notice to user and is not obligated to provide any maintenance or support related to the Information. The Information is based on specific Conditions and, therefore, alterations to the Information cannot be excluded. Any rights not expressly granted herein are reserved. Except for the right to use the Information included in this document, no other rights are granted nor shall any obligation be implied requiring the grant of further rights. Any and all rights or licenses to patents or patent applications are expressly excluded. Reproduction, transfer, distribution or storage of part or all of the contents of this document in any form without the prior written permission of OSRAM Opto Semiconductors GmbH is prohibited except in accordance with applicable mandatory law. February, 2013 page 5 of 5
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