This glossary contains the definition of common lighting fundamental terms used in the lighting profession. The IES Lighting Library has a large glossary as well as RP-16 which define common terms for the industry.

Absorption - The total amount of light that is absorbed on or in a material. The light that is not reflected or transmitted through a material is absorbed.

Accent Lighting - Directional lighting used to emphasize a particular object or area to direct attention to that field of view.

Ambient Lighting - Lighting throughout an area which produces general illumination.

Azimuthal Angle - The horizontal angular distance between a fixed reference direction and a position contained within a circle in the horizontal plane. Often referenced as the horizontal angles of a candela distribution. In Photopia’s photometric coordinate system, the azimuthal angle is measured in the world XY plane in the counter clockwise direction, with 0 deg. aligned with the +Y axis.

Baffle - A single opaque or translucent element to shield a source from direct view of an observer at certain angles or to absorb unwanted light.

Ballast - A device used with an electric-discharge lamp to obtain the necessary circuit conditions for starting and operating.

Ballast Factor - The fractional flux of a lamp(s) operated on a ballast as compared to the flux when operated on the reference ballast used when the initial lamp lumens were determined.

BRDF / BTDF / BSDF - Bidirectional Reflectance Distribution Function / Bidirectional Transmittance Distribution Function / Bidirectional Scatter Distribution Function. These functions represent the ratio of luminance / illuminance (L/E) of a material as viewed from a given direction and illuminated from a given direction. The absolute values are a function of the specific geometric conditions under which they are measured. These values are generally used to quantify how light scatters upon reflection or transmission through a surface.

Brightness - The subjective term associated with the luminous magnitude of a surface using qualities such as bright, light, brilliant, dim or dark. The brightness of a surface is directly related to the surface Luminance via Steven’s Law, which states that the brightness ratio between 2 luminous surfaces is proportional to the cube root of the luminance ratio between the 2 surfaces. So this relationship means that it takes an 8:1 luminance ratio in order to produce the perception of a surface being twice as bright (2:1) as another since the cube root of 8 is 2.

Bulb - The glass or quartz shell enclosing the luminous element of a lamp.

Candela - The International System (SI) unit of luminous intensity (candlepower). One candela is one lumen per steradian. Steradians are the units of Solid Angle. Candelas are often incorrectly interchanged with the term candlepower. Candelas are the units of candlepower, like feet is a unit for distance.

Candlepower - Equivalent to luminous intensity. The units for luminous intensity, and thus candlepower, are candelas.

Candlepower Distribution Curve - A curve, generally polar, which represents the luminous intensity of a lamp or luminaire at measured horizontal and vertical angles.

Cavity Ratio - A number indicating cavity proportions from length, width, and height. This value used in the coefficient of utilization calculation for a given luminaire in a space with specified room reflectances and dimensions.

Coefficient of Utilization (CU) - For a given luminaire, it is the ratio of the total luminous flux (lumens) received on the work-plane to the total luminous flux emitted by the luminaire’s lamps alone

Compact Fluorescent Lamp (CFL) - A small fluorescent lamp generally made from a series of folded or twisted tubes so that the lamp can be used in much smaller luminaires than standard linear fluorescent lamps.

Diffuse - The characteristic of a surface to scatter reflected or transmitted light. Strictly speaking, a diffuse surface exhibits a constant luminance from all viewing directions. However, the term is used for surfaces which only approach this ideal. A white wall is an example of a diffuse surface. Perfectly diffuse surfaces are also sometimes called Lambertian.

Diffuser - A device to redirect or scatter the light from a source. A translucent white plastic sheet is an example of a diffuser

Direct Component - That portion of the light from a luminaire which arrives at the work- plane without being reflected by room surfaces.

Discomfort Glare - Glare producing discomfort.

Downlight - A small direct luminaire which directs the light downward.

Downward Component - The portion of the light from the luminaire emitted into the lower hemisphere.

Efficacy - Typically the output lumens per watt of input electrical power. Also, see the various Luminous Efficacy definitions.

Efficiency - Typically the output lumens / input lumens, represented as a %. See Luminaire Efficiency for more details.

Equipment Operating Factor - It is commonly assumed that a ballast operated at its rated input voltage delivers rated wattage to a lamp and that a lamp operated at its rated wattage delivers its rated lumen output. This is a factor to adjust to the specific combination of luminaire, lamp type, and ballast used in a system.

Exitance - See Luminous Exitance.

Exitance Coefficient - A coefficient similar to the coefficient of utilization used to determine wall and ceiling exitances.

Filter - A coefficient similar to the coefficient of utilization used to determine wall and ceiling exitances.

Fixture - A coefficient similar to the coefficient of utilization used to determine wall and ceiling exitances.

Fluorescent Lamp - A coefficient similar to the coefficient of utilization used to determine wall and ceiling exitances.

Flux - See Luminous Flux

Foodcandle (fc) - The Imperial unit of illuminance (lumens incident onto a surface per ft2).

Foodlambert (FL) - The Imperial unit of illuminance (lumens incident onto a surface per ft2).

General Diffuse Light - The Imperial unit of illuminance (lumens incident onto a surface per ft2).

General Lighting - Lighting designed to provide a substantially uniform level of illumination throughout an area, exclusive of any provision for special local requirements.

Glare - The sensation produced by luminance within the visual field that is sufficiently greater than the luminance to which the eyes are adapted to cause annoyance, discomfort, or loss in visual performance and visibility.

Goniophotometer - A device on which a luminaire or lamp is mounted such that a photocell can be rotated around it at precise angles to obtain the luminous intensity distribution. Photometric laboratories use goniophotometers to measure the light distributions of luminaires and lamps.

High Intensity Discharge Lamp - An electric discharge lamp, including groups of lamps known as mercury vapor, metal halide, high pressure sodium, and low pressure sodium.

High Pressure Sodium - High intensity discharge (HID) lamp in which light is produced by radiation from sodium vapor operating at a partial pressure of about 1.33 x 104 Pa (100 torr). Includes clear and diffuse coating.

Illuminance (E) - The density of the luminous flux incident on a surface; lumens per unit area onto a surface. The units are footcandles (lumens/ft2) or lux (lumens/m2).

Illumination - The act of illuminating or state of being illuminated.

Incandescent - A lamp in which light is produced by a filament heated to incandescence by an electric current.

Indirect Component - The portion of the luminous flux from a luminaire arriving at the work-plane after being reflected by room surfaces.

Intensity (I) - A shortening of the term luminous intensity.

Inverse Square Cosine Law - The equation for determining the illuminance at a point given a luminaire position and candela distribution. The equation assumes the luminaire is a point source. Where: E: Illuminance I(,): Luminous intensity at a given horizontal and vertical angle in the candela distribution. : The incidence angle of the light directed onto the point being illuminated. D: The distance between the center of the luminaire and the point being illuminated.

Isofootcandle Line - A line plotted on any appropriate set of coordinates to show all points on a surface where the illuminance is constant. A series of such lines for various illuminance values is called an isofootcandle plot.

Lambert (L) - A unit of measurement of luminance equal to 1 candela per square centimeter.

Lamp - A generic term used for a man-made source of light. The lamp includes a base, filament (or arc tube) and a bulb. By extension, the term is also used to denote sources that radiate in regions of the visible spectrum.

Lamp Burnout Factor - While a specific lamp’s burn-out is impossible to predict, a group of lamps will fail predictably.

Lamp Position(titl) Factor - This factor accounts for the fact that lamps will generate a reduced output in some orientations, most prevalent in HID sources.

Lamp Lumen Depreciation Factor - The multiplier to be used in illumination calculation to elate the initial rated output of light sources to the anticipated depreciation of the lamp lumens when used over an extended period of time.

LED - See Light Emitting Diode.

Lens - A glass or plastic element used in luminaires to change the direction and control the distribution of the light.

Light - Radiant energy that is capable of exciting the retina and producing a visual sensation. The visible portion of the electromagnetic spectrum (light) extends from about 380 to 780 nm.

Light Emitting Diode - A light source based on a small die or chip made from semiconductor materials. The light generated is incoherent and in a narrow spectrum, with the wavelength determined by the specific composition and condition of the semiconducting material. LED’s are capable of generating radiant flux in the visible, infrared and near-ultraviolet range. White LED’s are based on chips that emit light in the blue wavelengths combined with one or more phosphors that add yellow and red wavelengths to the total distribution. LED’s are supplied in many forms, many of which are embedded within packages that include lenses to control the pattern of emitted light.

Light Loss Factor - A factor used in calculating illuminances after a given period of time and under specified conditions. It takes into account the dirt accumulation on luminaires and room surfaces, lamp depreciation, maintenance procedures and atmosphere conditions.

Louver - A series of baffles used to shield a source from view at certain angles or to absorb unwanted light.

Low Pressure Mercury Lamp - A discharge lamp (with or without phosphor coating) in which the partial pressure of the mercury vapor during operation does not exceed 100 Pa.

Low Pressure Sodium lamp - A discharges lamp in which light is produced by radiation from sodium vapor operating at a partial pressure of about .1 to 1.5 Pa.

Lumen (lm) - International System (SI) unit of luminous flux. Lumens fundamentally quantify the total amount of light produced by a luminous source. Lumens are determined by integrating the total radiant watts over the visible spectrum while weighting each wavelength according to its ability to stimulate the human visual system. The equation to determine lumens is as follows: Where: : wavelength in nanometers (nm). SPDF(): Spectral Power Distribution Function of the source, which is the amount of radiant watts the source produces at each wavelength. V(): The Photometric Luminous Efficiency Function, which is a normalized function that represents the human eye’s relative sensitivity to each wavelength over the visible spectrum. All other lighting metrics result from various geometrical conditions under which lumens are constrained. For example, measuring the number of lumens directed into a particular region of space is the luminous intensity and measuring the number of lumens falling onto a surface over a given area is the illuminance.

Lumen Method - A lighting design procedure used for predetermining the relation between the number and types of lamps or luminaires, the room characteristics, and the average illuminance on the work-plane. It takes into account both direct and reflected flux.

Luminaire - A complete assembly consisting of a lamp or lamps together with other parts intended to help distribute the light, position and protect the lamps and connect the lamp to the power supply. A luminaire is sometimes called a lighting fixture or a fitting.

Luminaire Dirt Depreciation Factor - The multiplier to be used in illuminance calculations to relate the initial illuminance provided by a clean, new luminaires to the reduced illuminance due to dirt collection.

Luminaire Spacing Criterion (SC) - A term defined by the IESNA that is intended to indicate the largest ratio of the luminaire spacing to the mounting height (Spacing / Mounting Height) that can be achieved while maintaining even illumination underneath an array of luminaires. This value is generally reported in directions along and across the lamp axes. Thus, values are generally reported for horizontal angles of 0 and 90 degrees, and sometimes beyond depending on the symmetry of the luminaire. The S.C. is determined by finding the lateral distance away from the luminaire at which the illuminance on a horizontal surface is ½ the value directly underneath. If the next luminaire is located at twice this distance away, then the contribution from each luminaire directly in between will equal the illuminance directly underneath the luminaire. Note that this method does not guaranty perfect uniformity of light on the work plane, just that the points directly under and directly in between the luminaires are equal.

Luminaire Surface Depreciation Factor - The ratio of luminous flux (lumens) emitted by a luminaire to that emitted by the lamp or lamps used therein.

Luminaire Efficiency - The ratio of luminous flux (lumens) emitted by a luminaire to that emitted by the lamp or lamps used therein.

Luminance (L) - The flux emitted from a surface in a given viewing direction. Can also be thought of as the light emitting power of a surface. Luminance is related to the visual sensation of brightness via Steven’s Law (see definition for Brightness). Luminance is measured in candelas/ ft2 or candelas/m2 .

Luminous Efficacy of a Source of Light - The IESNA defines this to be the quotient of the total luminous flux, measured in lumens, divided by the total electrical watts consumed by the source. It is expressed in lumens per watt. In the architectural lighting industry, this term is generally referred to as simply the Efficacy. In other industries, this term has been referred to as the Luminous Efficiency.

Luminous Efficacy of Radiant Flux - The International System unit of illuminance. One lux is one lumen/m2 .

Luminous Exitance (M) - The International System unit of illuminance. One lux is one lumen/m2 .

Luminous Flux - The International System unit of illuminance. One lux is one lumen/m2 .

Luminous Intensity (I) - The International System unit of illuminance. One lux is one lumen/m2 .

Lux (lx) - The International System unit of illuminance. One lux is one lumen/m2 .

Mercury Vapor - A high intensity discharge (HID) lamp in which the major portion of the light is produced by radiation from mercury operating at a partial pressure in excess of 105 Pa (approximately 1 atmosphere). Includes clear, phosphor-coated (mercury- fluorescent), and self-ballasted lamps.

Metal Halide - A high intensity discharge (HID) lamp in which the major portion of the light is produced by radiation of metal halides and their products of dissociation- possibly in combination with metallic vapors such as mercury. Includes clear and phosphor coated lamps.

Photometric Luminous Efficiency Function (V(lambda)) - A high intensity discharge (HID) lamp in which the major portion of the light is produced by radiation of metal halides and their products of dissociation- possibly in combination with metallic vapors such as mercury. Includes clear and phosphor coated lamps.

Photometry - Light-measurement; the measurement of quantities associated with light.

Photopia - Light-vision; vision under bright light conditions.

Photopic Vision - Vision under bright light viewing conditions involving the use of the cones in the human visual system.

Point Method - A lighting design procedure for predetermining the illuminance at various points in lighting installations, by use of luminaire photometric data and the application of the Inverse Square Cosine Law.

Point Source - A source of radiation the dimensions of which are small enough, compared with the distance between the source and the irradiated surface, for them to be neglected in calculations and measurements.

Preheat Fluorescent Lamp - A fluorescent lamp designed for operation in a circuit requiring a manual or automatic starting switch to preheat the electrodes in order to start the arc.

Quantity of Light - The product of the luminous flux and the time over which it is maintained. It is the time integral of luminous flux. Quantified in terms of footcandle-hours or lux-hours, this is important to lighting analyses for plant life.

Quartz Halogen - A gas filled tungsten incandescent lamp containing a proportion of halogens in an inert gas whose pressure exceeds three atmospheres. The halogen gases combine with tungsten particles and redeposit them on the filament when contact is made. This halogen cycle takes place at a high temperature (brighter filament) and increases the life of the lamp.

Rapid Start Fluorescent Lamp - A fluorescent lamp designed for operation with a ballast that provides a low-voltage winding for preheating the electrodes and initiating the arc without a starting switch or the application of high voltage.

Reflectance - See Total Integrated Reflectance.

Room Surface Depreciation Factor - The reduction of the reflectance capabilities of room surfaces due to the dirt that accumulates on these surfaces. This is dependent on the cleaning interval and the type of atmospheric conditions.

Scotopic Vision - Vision under dim light viewing conditions involving the use of the rods in the human visual system.

Shielding Angle of a Luminatire - Vision under dim light viewing conditions involving the use of the rods in the human visual system.

Solid Angle (w) - A measure of spatial extent. It can be thought of as the 3D equivalent to a 2D angle. A way of quantifying the size of a cone or other arbitrarily shaped regions of space. It is expressed in units of steradians. The total solid angle of a sphere is 4pi.

Spotlight - A type of luminaire with a relatively narrow beam angle designed to illuminate a specifically defined area.

Steradian (sr) - The units of solid angle.

Target Efficiency - The number of lumens reaching a given "target area" divided by the total lamp lumens in the luminaire.

Task Lighting - Lighting directed to a specific surface or area that provides illumination for visual tasks.

Temperature Factor - This represents the thermal factor of the installation that compensates for the light losses or gains due to luminaire temperatures which differ from test conditions.

Total Integrated Reflectance - The fraction of incident light that is reflected from a surface into all directions. This value is also referred to as simply the reflectance. The reflectance is generally not constant for all incidence angles of light directed onto a surface. This value is measured in an integrating sphere device.

Total Integrated Transmittance - The fraction of incident light that is transmitted from a surface into all directions. This value is also referred to as simply the transmittance. The transmittance is generally not constant for all incidence angles of light directed onto a surface. This value is measured in an integrating sphere device.

Transmission - A general term for the process by which incident flux is passed through a surface.

Transmittance - A recessed luminaire installed with the opening flush with the ceiling.

Troffer - A recessed luminaire installed with the opening flush with the ceiling.

Upward Component - The portion of the light form a luminaire emitted at angles above the horizontal.

Visual Task - Conventionally designates those details and objects that must be seen for the performance of a given activity, and includes the immediate background of the details or objects.

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Lamps

Photopia Lamp Modeling

Background

Photopia comes with a large library of lamp models for use in optical designs. Sometimes a lamp you may want to use is not in the library. In these cases, you can either construct a lamp model yourself using information in the Photopia User's Guide Appendix B, or have us construct the model for you.

Components in a Lamp Model

Lamp models in the Photopia Library contain 3 basic components: a CAD model, an IES formatted bare lamp photometric file, and luminance information for the source.

The geometry is described in an AutoCAD 2000 formatted DXF file. The model includes all of the physical geometry as well as non-physical geometry such as arc shapes. Materials are assigned to each part of the lamp model, so that the correct interactions occur wen light comes back into contact with the lamp.

The output of the lamp is described in a bare lamp photometric file. This file is created by a lab measurement of the candela distribution and lumen output of each lamp.

The final part of a lamp model is a description of the luminance properties of the source. For HPS and Metal Halide lamps this means determining the shape and luminance variation of the arc. The image below shows a sample 1500W Metal Halide arc tube with the arc inside, along with the Photopia model of the arc. For fluorescent sources this involves the luminance variation across the surface.

Creating your own Lamp Model

If you are looking for a lamp in the Library and don't find it, you can make your own lamp model. There are instructions for creating lamp models in Appendix B of the Photopia User's Guide, which is available by selecting Help > Documentation in Photopia.

Using an IES file for a lamp

If your luminaire uses LEDs with off the shelf secondary optics from companies such as Ledil, Carclo, Fraen, etc. and if those optics do not interact with other lenses or reflectors in close proximity, then they can be represented using a special set of lamp models in Photopia's library. The special lamp models consist of planar geometry and will emit light in a distribution driven by the IES file you assign to it. The light will be emitted uniformly from the front surface of the lamp geometry. We have created a range of models that can be used for various sized optics. You will see them in the lamp list with names that begin with "LEDLENS..." The rest of the name indicates the geometry of the source, with a single number indicating a diameter. Some of these lamp models also include several copies so you can work with multiple lens types in the same luminaire. In this case, the extra copies have numbers at the end of their name. Some of these models include:

• LEDLENS20MM (This has a round emission area)
• LEDLENS50MM (This has a round emission area)
• LEDLENS75MM (This has a round emission area)
• LEDLENS19x95MM (This has a rectangular emission area for symmetric beams. It is sized for the Ledil Florence product line.)
• LEDLENS95x19MM (This has a rectangular emission area for asymmetric beams where the main throw is perpendicular to the long axis of the lens. It is sized for the Ledil Florence product line.)

To set the lamp model's IES file, just rename your IES file to match the model name you want to use and put it into the following folder: C:\ProgramData\LTI Optics\Library\Lamps

Note that this folder is sometimes hidden by Windows, so if you don't see it in Windows Explorer then change your Folder Options to display all hidden folders and files.

Once you load the lamp into your Photopia project, then you will set its lumens, LED watts and driver watts in the Edit > Design Properties > Lamp screen to define the values appropriate for your LED, its running current, temperature and lens efficiency.

Getting a new lamp in the Library

If you are looking for a lamp in the Library and can't find it, let us know and we'll try to get it in the Library. Lamp manufacturers can have their new products included in the Photopia Library. This is a very beneficial service as your products will be seen by all of our users. You can see more information about adding a new lamp to the Library on this order form.

Raysets

LED Modeling Using Raysets

Overview

Producing accurate simulations of LED based optical systems requires accurate source models. This means the source models must not only produce the correct distribution of light in a far field measurement, they must also produce the correct near field behavior since secondary LED optics are often employed in very close proximity to the LED. Accurate simulations are vital to the design process especially with lens optics commonly used on LEDs given the high cost and long lead times for lens tooling. The data presented in the case studies below is a direct result of the lessons learned by one manufacturer about the importance of simulation accuracy.

What Are Raysets?

Raysets have become a convenient way to model light source behavior, and are commonly provided by LED vendors. A rayset is simply a collection of rays (vectors) that describe the initial emanation of light from a source. Each ray consists of a start point, direction, and magnitude (in lumens). Rayset files are ususally provided in multiple formats for compatability with most optical simulation software.

What Are Raysets Missing?

Raysets are missing one key componenet of a lamp model, geometry. Raysets only describe the exiting light and do not contain any geometric data about the light source. Since there is no geometric information, there is nothing for the light to interact with if it comes back towards the light source. Some vendors provide 3D cad models as a supplement to their raysets, but this relies on the users to assign appropriate materials to each part of the LED. Additionally, many of these CAD models don't contain enough detail but only describe the bounding volume of the package. This lack of geometry also causes an issue with accurate ray emanation points. Since there is no geometry, the ray emanation points are not coming from geometric locations, but just points in space. The process of combining the 2D images to create raysets does not seem to provide an accurate way to determine correct ray emanation points.

The images below show a cross section of the CREE XR-E LED. The image on the left shows the light field for a rayset based model. The geometry is included only as a reference since the rayset based model doesn't contain any geometric information. The image on the right shows a Photopia lamp model, with the associated geometry. The light field for the Photopia model looks more coherent and seems to match the geometry better than the rayset based model, which seems to indicate light coming directly behind the LED, through the package, which is a physical impossibility.

Using Raysets in Photopia

Since the original beta release, Photopia v3.0 has supported the use of raysets. You can see how to use these in Appendix B of the v3 User's Guide. Photopia uses raysets that end in a .rir extension. Radiant Imaging's ProSource software exports this format natively, and other lamp manufacturers are working on providing this format of their raysets. Our format is identical to the TracePro Binary format, so if you see this format (which ends in a .ray extension) you can use these in Photopia simply by changing the extension to .rir. When you have a .rir rayset, you'll simpy import a simple lamp model from the Photopia lamp library, and then in the Property control, choose the rayset by browsing to it. You'll also need to set the appropriate lumen value for the source model.

Rayset Accuracy

Raysets seem to have a good potential of capturing near field photometric data, however, they do have some significant limitations. Their lack of CAD geometry puts the responsibility on the user of the software to import and assign materials in order to achieve an accurate output. Additionally, because the data is compiled from a series of 2D images, raysets often don't contain accurate 3D emanation points. Of the two aspects of lamp modeling, where is the light going and where is it coming from, raysets only accurately adddress where the light is going. Without proper material assignments to the 3D geometry as well as the proper emanation points, photometric simuations can be very inaccurate. Appendix B of the Photopia User's Guide illustrates some of these issues.

In conjunction with Ruud Lighting, we've also done a series of studies that compared simulations with raysets and simulations with Photopia lamp models to measured photometry. We consistently saw very strong correlation between the Photopia lamp models and measured photometry. The match between raysets based models and measured photometry was less consistent. In any application where secondary optics will be placed close to an LED, the Photopia lamp model provides the best correlation. Since these raysets are typically generated from 2D images, they have no way to accurately determine the 3D ray emanation points, which are critical when an optic is placed close to or directly on the LED. Additionally, if an index matching gel is used to join the LED and the optic, raysets provide no way to account for this surface interaction. Case studes are included below as well as in the following papers:

LED Source Modeling Method Evaluations in the November/December 2008 issue of LED Professional Review and LED Source Models in the January/February 2009 issue of LED Journal both cover this study of physical measurements.

These case studies use data collected by BetaLEDTM during the development of their NanoOpticTM LED outdoor area lighting lens optics. The data includes measured luminous intensity distributions along with simulations using both Type 1 and Type 3 source models in Photopia. The optics were measured at Independent Testing Laboratories, Inc. (ITL) in Boulder, Colorado, USA. The simulations used lens geometry that was scanned from the physical as-built parts. This is important since the as-built parts did not always perfectly match the intended design, which removes a potential source of difference between measured and simulated performance.

Case 1: Roadway Type 5 Lens with Index Matching Gel between LED and Lens

The image on the left shows the measured (blue) versus rayset predicted (red) candela plot. The image on the right shows the measured (blue) versus Photopia model predicted (red) candela plot. The rayset based models are called Type 1, the Photopia models are called Type 3 based on the terminology in this paper on lamp modeling.

The Photopia (Type 3) model on the right predicts the beam more closely than the rayset (Type 1) model on the left. The image on the right shows that the predicted and measured candela plots trace each other more closely, especially at the higher vertical angles, which are critical in a roadway application. If the simulations are underpredicting these values, then the optimization of the optic will be misdirected. The rayset model on the left shows very significant deviations between the high angle light, the angle at which the peak intensity occurs, and the nadir intensity, all of which are main design criteria in a roadway optic.

Case 2: Roadway Type 5 Lens without Index Matching Gel

The differences between the rayset and Photopia model performance are not as great as in Case 1, but the left images below do show an upward shift in the beam angle and significantly more light directly below the luminaire. Accurately predicting the peak vertical angle in the intensity distribution is another critical issue in this type of lens. The right images below show a more accurate overall beam shape and peak beam angles.

Case 3: Medium Beam Lens with Index Matching Gel

This case illustrates how the differences between the 2 model types remains significant when a gel is used between the LED and lens even in a much narrower beam distribution. The higher intensities seen in the central part of the beam using the Type 1 model on the left result from the extra lumens that were not directed to the higher angles in the distribution where they belonged. The Type 3 model results shown on the right reveal a much closer beam shape at the full range of angles in this distribution.

Summary

The 3 cases presented illustrate that there are significant differences in simulated results depending on the source modeling method used. These results show that a Type 3 model more closely matches the measured performance than the Type 1 model for both wide and medium beam lenses. The differences are greatest when an index matching gel is used between the LED and lens. The main reasons for this are that in addition to the challenge Type 1 models have in creating accurate 3D ray emanation points, all of their digital images showing the luminous view of the source are measured in air. When a gel is used between the LED and the lens, light never exits from the LED primary lens into air so the measurements are inappropriate. Since Type 3 models include the lens geometry, the material can simply be changed to account for the glass / gel interface instead of glass / air.

The 2nd set of data shows that the Type 1 model fairs better when there is no gel, yet it does not outperform the Type 3 model. Wider beam optics are more sensitive than narrower beam optics to exactly how much light is directed onto each part of the lens. As the beam gets narrower, more light is directed to the same angles in the beam and differences in the amount of light sent to each part of the lens between the simulation and physical reality become less important. It should also be noted that other 3D ray emanation point geometry mapping options were tested such as mapping the points to a sphere and the results did not vary significantly from those presented here.

Given a choice between Type 1 and Type 3 source models for the same LED, a Type 3 model will likely produce more accurate results, especially as the beam gets wider. If gels are used between the LED and lens, then Type 1 models should not be used since the measurements on which they are based is not appropriate for this situation.

The simulation data in these case studies was provided by Kurt Wilcox and Chris Strom at Ruud Lighting. ITL in Boulder, Colorado provided the physical measured data for comparison.

Materials

Photopia Materials Library

Background

Our customers rely on Photopia to produce accurate predictive photometry. Having accurate material models is necessary to have accurate output. Photopia includes a library with over 1440 measured materials from most of the major vendors that the lighting industry uses.

Our Measurement Process

LTI Optics uses a custom-built BRDF/BTDF measurement device to accurately characterize the real reflecting/transmitting properties of various materials such as semi-specular aluminum, hammertone, prismatic lenses, perforated diffusers, and many others. The measurements are collected for a wide range of light incidence angles to capture the true scattering nature of real materials (see image below). Photopia uses the measured data in lookup table format and therefore does not attempt to "curve fit" the data into standardized equations that do not model the wide range of scattering effects observed in real materials. The library of measured data also eliminates the need for the user to "guess" at the scattering properties of materials. Customers can also submit proprietary materials for measurement, ensuring the most accurate data possible for their analyses. To create an accurate material model we perform two types of measurements: integrated reflectance/transmittance, and material scattering.

Adding a Material to the Library

If you're looking for a material that you don't find in the Library, please let us know and we'll work on adding it. Often, you may use a custom material that isn't generally available. We can add this material to a custom library for your company. For information on getting a material in the Library, please see this order form.

Modifying a Material in the Library

You are able to modify the integrated reflectance of reflective materials, the integrated reflectance and transmittance of transmissive materials, and the index of refraction and extinction coefficient of refractive materials. The integrated reflectance and transmittance values can be changed as a function of incidence angle. You can also change the ratio of the light reflected in a specular manner to that scattered by a material and the ratio of the light transmitted in a straight-through manner to that scattered by the material. You cannot change the distribution of the scattered light from materials, however, as this data is measured in our BRDF/BTDF device and stored in binary format. Following are descriptions of the material files:

Reflective Material Files:

Filename.rfl - ASCII file of integrated reflectance values at each incidence angle. Files can contain an arbitrary angle set, so long as 0, 90 and 180 degrees are included. Valid reflectance values range from 0.0 to 1.0.

Filename.brd - Binary file of the BRDF data for a material. This file cannot be modified. A .brd file only 2 bytes in size indicates the material is specular.

Filename.rsc - ASCII file specifying the ratio of the reflected light that is reflected in a specular manner. Note that these are not the specular reflectance values, but the fraction of the reflected light that is specular at each angle. To derive specular reflectance from these values, multiply these values by the reflectance at each incidence angle. Valid values range from 0.0 to 1.0. This file may or may not be associated with a material. A data byte indicating whether or not the material has a specular reflectance component is contained in the .brd file.

Transmissive Material Files (includes reflective files above, plus the following):

Filename.trn - ASCII file of integrated transmittance values at each incidence angle. Files can contain an arbitrary angle set, so long as 0, 90 and 180 degrees are included. Valid transmittance values range from 0.0 to 1.0.

Filename.btd - Binary file of the BTDF data for a material. This file cannot be modified. A .btd file only 2 bytes in size indicates the material is clear or image-preserving.

Filename.tsc - ASCII file specifying the ratio of the transmitted light that is transmitted in a straight-through manner. Note that these are not the straight-through transmittance values, but the fraction of the transmitted light that passes through un-scattered at each angle. To derive straight-through transmittance from these values, multiply these values by the transmittance at each incidence angle. Valid values range from 0.0 to 1.0. This file may or may not be associated with a material. A data byte indicating whether or not the material has a straight-through transmittance component is contained in the .btd file.

Refractor Materials Files:

Filename.rfc - ASCII file containing 3 values: the index of refraction of the outside medium (usually assumed to be air at 1.0), the index of refraction of the material averaged over the visible spectrum, and the extinction coefficient in units of inches. Note that the extinction coefficient is applied in the equation: Trans = e^(k*L), where e is the exponential (2.71Ö), k is the extinction coefficient, and L is the distance the ray travels in the material in inches. Thus, k is a value per inch.

To Modify Material Files:

You can modify any of the ASCII files described above with a text editor such as Notepad. If you want to create a new version of a file without changing the original copy, then follow the specific instructions below:

Differences Between Refractive and Transmissive Materials

Transmissive surfaces are modeled as infinitely thin surfaces in the CAD model and all optical properties of the physical material are assigned to this surface. When a ray strikes a transmissive surface all of the effects of the thick material are accounted for at this single ray/surface interface. The amount of reflected, transmitted and absorbed light is dictated by the material's .RFL and .TRN files which list the reflectance and transmittance as a function of incidence angle, respectively. The scattering properties for the reflected and transmitted light are dictated by the BRDF and BTDF data, respectively. The "front" side of the material always has reflectance and transmittance properties and the "back" side has data on only some of the materials in the library. Examples of transmissive materials are clear glass and plastics, white translucent materials, isotropic* prismatic lenses and isotropic perforated materials.

Refractive surfaces model the entire volume of a lens including the inside, outside and side surfaces. When a ray strikes a refractor surface from the "outside" (from the air, for example), it is partially reflected and refracted according to Fresnel's Equations and Snell's Law of Refraction, respectively. Light is also absorbed within the material according to the path length within the material and the material's extinction coefficient. Once rays have entered into a refractor material such as glass, Photopia searches for intersections with other refractor surfaces on all refractor layers in the model. Once an intersection is found, the ray is either partially internally reflected and partially refracted out or it is Totally Internally Reflected (TIR) back into the material, depending on the incidence angle.

Clear lenses can be modeled with either Transmissive or Refractive surfaces. Transmissive surfaces will result in a faster analysis. If the lens is curved, then only the inside surface of the true lens shape should be modeled if making it a Transmissive surface. If the curvature and thickness of the clear lens are such that there might be some refractive effects, then it should be modeled as a Refractor using its true geometry and thickness.

*Isotropic materials are those for which their orientation within the plane of the material is not important. For example, a flat sheet of translucent white plastic can be rotated within the plane of the material and the scattering of the incident light will be unaffected. If a material such as a plastic lens with extruded linear prisms was rotated there would be a significant difference between the scattered light patterns. The effects of the prisms on the light are different depending on whether the light strikes the prisms from within a plane that is parallel, perpendicular or some other orientation to them. Such materials are referred to as anisotropic. A perforated material is isotropic if it has round holes in a regular pattern, but it would be anisotropic of it contained linear slots.

When to Use the Solid Model Versions of Transmissive Materials

Transmissive materials use BRDF & BTDF files to characterize how light reflects and transmits when it is incident upon the material. When a ray strikes a transmissive surface in Photopia, the appropriate reaction is applied to the ray using the BRDF & BTDF data. The important point to note is that the measured BRDF & BTDF data takes into account the effects of the full material thickness. So when a ray in Photopia strikes an infinitely thin polygon with a transmissive material assigned to it, the full reaction of the physical material (with a thickness) is accounted for at this single ray/polygon interface.

When a CAD model is constructed as a solid, every part has a thickness. Thus, if a prismatic lens or white diffuser material is drawn as a solid, it will be constructed with the thickness of the physical part. When this model is exported to Photopia via a STL file it imports as a mesh of polygons that cover the surface of the original solid model. If a transmissive material is assigned to the mesh that models this lens, then a ray will encounter 2 surfaces when passing through the material model. Since the full effect of the material is accounted for at the first ray/surface interaction, it will then be accounted for twice if the ray then strikes a second surface of the lens.

To avoid this problem, we have made special versions of the transmissive materials where the second surface is ignored in such a case. These are the Solid Model versions of the transmissive materials and they should be used when the CAD model was constructed as a solid model. Note however, that the Solid Model versions of the materials only produce the proper effect if all of the surfaces of the lens model are oriented so that their "front" side is facing to the outside of the part. Thus, if the part is on a layer with a color of white, then the part should be rendered as white from all points of view when viewed in the Show Surface Orientation model in Photopia. This is important because the way that the Solid Model materials work is to have the reaction on the "back" side of the material be perfectly transmissive. So when the ray encounters the second surface of a lens model, it strikes the "back" side and is allowed to pass directly through with no losses or scattering.

One significant consequence of this is that it prohibits (or at least limits) the use of materials with different properties on each side. Materials that have a textured surface on one side and a smooth finish on the another, for example, can be properly modeled with a single, infinitely thin surface in Photopia since we can assign unique BRDF & BTDF data to each side of the material. But in the case of Solid Model materials, the "back" side must be set to be perfectly clear, so this flexibility is lost. This is why all of the Solid Model materials in the library are for materials that are the same (or mostly the same) on both sides. If you have a need for another material to be made into a Solid Model material, then contact us about making a new material for you. It is possible to make Solid Model materials for materials that are different on each side as long as light is only incident onto one side of the lens in the luminaire model.

Volumetric Scattering

Background

Beginning with Photopia 2017, Photopia and Photopia for SOLIDWORKS support volumetric scattering refractive materials. This is for materials which scatter light within their volume, usually via pigment or diffusion particles. These are a special class of Refractive materials, and as such require the General Refractor Module or Photopia Premium. Volumetric scattering can also be used along with spectral material properties to model phosphor particles suspended in a clear material.

Description

Photopia uses a specific XML formatted file for defining the material properties. For Volumetric Scattering, the scattering is described by the Beer-Lambert Law. Photopia accounts for the extinction coefficient within the clear base material, the scattering coefficient (likelihood to scatter), the absorption of the scatter reaction, as well as the distribution and energy conversion of the scatter reaction.

Full details are provided in this Volumetric Scattering Documentation.

Spectral Materials

Background

With Photopia 2015, we introduced the ability to set spectral properties for materials. For spectral materials to function, a raytrace must be set as an SPD raytrace. You must also have appropriate .material, .spdrfc, .spdrfl, .spdtrn, and .spdmatrix files.

.material file

Each spectral material must have a .material file. This is an XML based file that tells Photopia what files contain the data for the given material.

• the label “id” must have “matlname (matl type)
• depending on the material type, lines for the brd,btd,rfl,trn,rfc,spdrfc,spdrfl,spdtrn can be included
• for refractive materials, if brd/btd/rfl/trn files are included then the material will refract but use the scattering data (no more flags in the rfc file)
• the individual file names do not matter, however their extensions must be appropriate

.spdrfc file

A .spdrfc file is used for refractors where either the index of refraction or the absorption coefficient or both vary with wavelength.

• name does not need to match .matlname, but must be referenced in the .material file
• 1st row: start wavelength, end wavelength, wavelength increment in nm
• additional rows: outside index of refraction (typically air), inside index of refraction, extinction coefficient

.spdrfl file

The .spdrfl file is the spectral reflectance. The file lists a scale value and then the name of an spdmatrix file for each incident angle.

• name does not need to match matlname, just spdrfl in the .material file
• incidence angle, scale value, spdmatrix filename
• scale value is applied to each value in the matrix

.spdtrn file

The .spdtrn file is the spectral transmittance. The file lists a scale value and then the name of an spdmatrix file for each incident angle.

• name does not need to match matlname, just spdtrn in the .material file
• incidence angle, scale value, spdmatrix filename
• scale value is applied to each value in the matrix

.spdmatrix file

The .spdmatrix file is the spectral material operator file. The format is the same for reflective or transmissive materials. This file can describe something as simple as a paint color or color filter, or it can describe the complex behavior of a phosphor or other wavelength conversion material.

• name does not need to match matlname
• 1st row: start wavelength, end wavelength, wavelength increment in nm
• additional rows: square matrix of wavelength conversion data
• rows are the input nm, columns are the output nm
• for a material that does not convert energy, the matrix will only have values on the diagonal, with zeros in all other locations
• the sum of each row of the matrix must be less than 1 to satisfy conservation of energy

Suggested Raytrace Settings

Since Photopia is a probabilistic based raytracing program, the results get more accurate as more rays are traced. The number of rays that are required to obtain accurate results depends on the level of "resolution" you have specified, in other words, the level of detail in the results. You can view the results such as the candela polar plot and the illuminance plane shaded plot and watch as they vary around their final values with each update as the raytrace proceeds. The default update frequency is 10%, so you see results at 10%, 20% and so on until the raytrace is finished. The least detailed result is the luminaire efficiency (LOR). This is a single number that represents how many lumens exit the luminaire compared to how many lumens were generated by the lamps. The exact direction of the exiting lumens is not critical when determining the efficiency. Thus, you can see that the efficiency changes very little after the first update of the results during the raytrace. The candela distribution requires much more detail to be resolved since Photopia needs to determine exactly how many lumens belong in all of the angular zones of the distribution. The more angles that are specified in the distribution, the smaller the angular zones and thus the more rays it takes to determine the correct proportions of lumens in all zones. The most level of detail is generally required for the illuminance planes. Whereas the angular zones in the candela distribution might be separated by 2.5 or 5 degrees, the small patches in a high-resolution illuminance plane might be separated by fractions of a degree in angular spread. With this general understanding, we make the following recommendations for the Raytrace and Photometric Output settings. Keep in mind that these are only general recommendations and you can vary these values as long as you understand the consequences.

Raytrace & Photometric Output Setting Recommendations

Applications	Photometry Type	# of Rays - Initial Evaluation	# of Rays - Final Evaluation	# of Reflections - No Lens	# of Reflections - With Lens	Vertical Angle Increment	Horizontal Angle Increment
Wide Beam	C	500,000	5,000,000	15	25	5	15
Narrow Beam	C	500,000	5,000,000	15	25	2.5	15
Very Narrow Beam	C	500,000	5,000,000	15	25	1	15
Roadway or Area Light	C	2,500,000	10,000,000	15	25	5	5 or 10
Wide Beam Floodlight	B	2,500,000	10,000,000	15	25	5	5
Very Narrow Beam	B	2,500,000	10,000,000	15	25	2.5	2.5

*Note: When using CFL lamps, we recommend that you turn ON the Lamp Shadow Check option. This options can be left off for most other lamp types. All other raytrace settings can generally be left at their default values.

Energy Units

Photopia 2015 introduced the ability so set the output units to lumens, radiant watts, μmol photons / sec and μmol photons / sec in the 400-700nm range (PAR). This allows the use of Photopia for a wide range of applications from general lighting to agriculture and radiant heating.

Under Setting > Project Settings there is a setting for "Lamp Flux Energy Units". Set this to the units you wish to see for your input and output. You can update your lamp energy values under Edit > Design Properties.

IESX Files

The IESX file contains color/spectral data for each angle in the intensity distribution. This is an XML format file, using a pre-release version of a future IES file format that has been expanded to support luminaire color data. The data in this file can most easily be viewed by opening it in Excel, using a reference style sheet file that tells Excel how to format the data. The style sheet file is named "iesxToText.xslt" and is installed in the following folder on your computer:

C:\Users\Public\Documents\LTI Optics\Photopia\Utilities

Put a copy of this file in the same folder as your IESX file. Then open the IESX file in Excel. At the "Import XML..." pop-up dialog, choose the 2nd option:

"Open the file with the following stylesheet applied (select one):"

It will default to iesxToText.xslt, so keep that option.

Then choose "Delimited" on the Text Import Wizard dialog, then click Next and then choose Comma as the delimiter.

Then click Finish.

The first row in the spreadsheet will include the column labels. If you chose the "Power distribution raytrace" option in Photopia, then the full spectral values will be listed for each angle in the beam at the nm resolution you specified.

Conventions

Having the correct Photometric Settings is critical to obtaining accurate results from Photopia. When you send a product for testing, the laboratory often determines the correct photometric angles, but when you are running Photopia it is something you must always be aware of. The angle sets are often broken down to vertical and horizontal angles, described below.

Vertical Angles

Vertical photometric angles go from directly below the fixture at 0 degrees to directly above at 180 degrees. The vertical angles that you choose are governed by the vertical distribution of your product. See the table below for information on the correct choice of vertical angles.

	Direct	Indirect	Direct/Indirect
Distribution	Light Directed Downward	Light Directed Upward	Light Directed Upward and Downward
Orientation	Beam in -z direction	Beam in +z direction	Beam in -z direction
Vertical Angles	0-90 degrees	90-180 degrees	0-180 degrees

Horizontal Angles

The horizontal photometric angles that you will choose depend on the horizontal symmetric of your product. Fixtures can have four types of symmetry, as outlined in the table below. In Photopia it is important to choose the correct angle set based on the fixture symmetry because otherwise the output can become incorrect. Photopia always has data for the full 0-360 degrees, but averages down to the angle set that you choose. In the extreme case all 360 degrees are averaged together when you choose a horizontal angle of "0" only.

	Axially Symmetric	Quadrilaterally Symmetric	Bilaterally Symmetric	Completely Asymmetric
Examples	Revolved Downlights	Louvered Fluorescent	"Asymmetric" Fluorescent Wallwash, Roadway	Directional Tunnel Lighting
Lamp Orientation		Along y axis
Outside U.S.		Along x axis
Beam Direction			Along +y axis
Horizontal Angles	0 degrees only	0-90 degrees	0-180 degrees	0-360 degrees

Distribution

As Photopia has come to be more widely used in the architectural lighting industry, an increasing number of Photopia generated photometric files are being distributed by lighting manufacturers to their customers. By photometric files, we are referring to IES files in North America and TM-14 or EULUMDAT in other regions of the world.

The original intent of Photopia was to allow manufacturers to develop new designs more quickly and more cost effectively by evaluating their design ideas on their computer instead of building and testing each and every design alternative. Once the predicted design performance met the desired criteria, a prototype was built and physically tested. If the physical test did not meet the design requirements, then modifications would be made until the requirements were met. In many cases, this involved troubleshooting the design to ensure it was built to specifications, so that it matched what was modeled in Photopia.

Photopia is no longer only used in the development of new standard products. It is also used to model the performance of custom luminaires where the time from concept to installation does not allow for the classic product development cycle. Additionally, it is being used to model some existing products for which photometric testing was never before required. In these cases and others, some manufactures will distribute photometric files generated by Photopia.

Whenever a photometric file generated by Photopia is distributed to a customer, the data should be as accurate as possible. The consequences of the photometric data not being accurate can be very costly if you are called out to fix an installed job. The distribution of inaccurate data also hurts Photopia's reputation and therefore its overall value. So it is in everyone's interest to ensure photometric data generated by Photopia is as accurate as possible.

While Photopia's accuracy has been confirmed by our own experience as well as that of our customers, the accuracy is dependent upon several critical factors, including but not limited to the following:

You need to build exactly what you have modeled. If you compromise and choose a similar lamp or materials to the ones you will actually use, then you can expect differences between the predicted and measured photometry.

You need to understand your manufacturing tolerances for all of the parts in your design. You can create a range of Photopia models for the expected range of part configurations to gain a better understanding of the expected range of photometric performance.

You need to understand how to use Photopia well enough to properly setup your analysis so you get accurate results. This means properly orienting your luminaire, using the proper angle set in the candela distribution, using the proper number of reflections and the proper number of rays. See this link for more information about photometric standards.

Some issues such as thermal effects are completely ignored by Photopia, so if you have thermally sensitive lamps then you know that there will be differences between the simulated and measured efficiencies.

Anisotropic materials are only supported in Version 3.0. So if you use a material with a significant grained texture such as Alanod Miro 5, then the anisotropic properties need to be accurately modeled within Version 3.0.

For more information about the factors that affect the accuracy, see Appendix C of the User's Guide.

Guidelines for Distributing Photometric Files:

If you do distribute IES files generated by Photopia, then please follow this advice:

Leave the [TESTLAB] keyword in the IES file exactly how Photopia has defined it. This will ensure that your customers know that the file is the result of a simulation and not a physical test.

Remove all lines with the [OTHER] keyword. This information is useful to the optical designer, but not necessarily to your customers. This data could invite questions from your customers about details of the analysis that are not important. You can edit the IES file in Notepad.

You should review the total luminaire watts as defined in the IES file. This value is set according to the default lamp and assumed ballast wattage for the Photopia lamp model. If you have more accurate information about the total luminaire watts, then use it. See the end of Appendix B of the User's Guide for the IES file format.

Be sure to let your customers know that the data is simulated when you distribute the files either in your e-mail or on your website so that there is no misunderstanding about this issue later on.

Thank you for your attention to this issue.

The Photopia Product Support Team

Labs

While Photopia is excellent for simulating photometry, there are often times when you must use a physical lab. These may include:

Confirmation of Photopia results

Significant thermal effects

Lamps or materials not available in Photopia Library

Physical testing required by code or specifying engineer

There are many labs available for photometric testing. We would recommend the following labs:

LightLab International - Phoenix, Arizona & Brisbane, Australia

LightLab Allentown - Allentown, Pennsylvania

IES - LM-63

This standard format maintained by the IES contains the intensity distribution of a product in photometric units (lumens & candelas) and cannot contain any color or spectral information.

The IES photometric file is an ASCII file with the format shown below. Items inside the {{ }} brackets are brief data descriptions. Items surrounded by [ ] brackets are keywords that must be present. Multiple data on the same line shall be separated by either a comma or at least one space. The {{ }} brackets themselves should not be present in the file. Full details of the file format are defined in the IES LM-63-2002 standard document, avaliable for purchase.

IESNA:LM-63-1995
[TEST] ...
[MANUFAC] ...
[keyword 3]
...
[Keyword n]
TILT=tilt file name -or- INCLUDE -or- NONE {{ Most common }}
{{ number of lamps }} {{ lumens per lamp }} {{ candela multiplier }} {{ number of vertical angles }} {{ number of horizontal angles }} {{ photometric type (1,2 or 3) }} {{ units (1 or 2) }} {{ width }} {{ length }} {{ height }}
{{ ballast factor }} {{ ballast lamp factor }} {{ input watts }}
{{ vertical angles }}
{{ horizontal angles }}
{{ candela values for all vertical angles at first horizontal angle }}
{{ candela values for all vertical angles at second horizontal angle }}
.
.
{{ candela values for all vertical angles at last horizontal angle }}

IESX - TM-33

This standard format maintained by the IES contains the intensity distribution of a product in photometric units (lumens & candelas), but can also contain this in radiometric or spectral units, as well as other data like integrating sphere results.

LDT - Eulumdat

Although widely used, the Eulumdat file (LDT) is not defined or maintained by a standard body. The Eulumdat file is widely used outside of North America. It contains the intensity distribution of a product in photometric units (lumens & candelas) and cannot contain any color or spectral information.