The present invention relates to the field of photometric test systems for measuring luminous flux characteristics of a light emitting source.
The integrating sphere is the standard instrument for measuring total flux, spectral flux and color of light sources. The fundamental characteristics of integrating spheres are their spherical geometry and the white diffusive coating on their interiors to maximize reflections. In order to achieve acceptable accuracy of measurement, it is required that an integrating sphere be at least 3 times larger than the Device Under Test (DUT). With the size of LED lighting products, such as LED luminaires, ranging from several inches to several feet, the required integrating sphere diameter often reaches 6-10 feet (2-3 meters). Additionally, due to the many reflections within the sphere and from the sphere to the DUT, the effect of the DUT's absorption on the measurement, which is known as self-absorption, is significant and must be calibrated. This calibration must be performed separately for each DUT and depends on the size, type and reflectivity of the DUT.
There are some prior art photometric test systems that are not integrating spheres, but rather boxlike structures with photo-detective solar panels on the walls facing the Device Under Test (DUT). In U.S. Pat. No. 7,804,589 to I-S. Tseng et al, entitled “System and Method for Testing Light Emitting Devices”, there is described a method for testing light-emitting devices batch-wise, associated with a system for the same purpose, using a moving carrier unit. In U.S. Pat. No. 8,773,655 to H-T. Cheng et al, entitled Total Luminous Flux Measurement System and Total Luminous Flux Measuring Method”, there is described a total luminous flux measurement system and a method thereof for measuring a total luminous flux of a light emitting component. However, due to the non-insignificant level of reflectivity of the solar panels in such systems, there is also a non-insignificant level of reflection off the DUT and back onto the solar panels that affects the measurement. Therefore, like integrating spheres, such systems must be calibrated differently for each type of DUT. This level of solar panel reflectivity and the constant need for recalibration decrease both the accuracy and the efficiency of such systems.
There therefore exists a need for a more compact, efficient and accurate photometric test system which overcomes at least some of the disadvantages of prior art systems and methods.
The disclosures of each of the publications mentioned in this section and in other sections of the specification, are hereby incorporated by reference, each in its entirety.
The present application describes new exemplary systems for measuring the spectral flux and total luminous flux of a light emitting source. Such systems may be absolutely calibrated for self-absorption effects arising from the nonzero reflection of incident light from photo-detection panels and again from the Device Under Test. Consequently, such systems are suitable for multiple sizes and types of DUTs, increasing the efficiency and accuracy of measurement over prior art systems. Furthermore, such systems need not be larger than the DUT, spherical geometry is not required, and the measurements provided by the system are not affected by the geometry of the DUT or by the incidence angle of light emitted from the DUT.
Such an exemplary system may comprise an enclosure with one or more walls adapted to receive light from a light-emitting source (DUT). The walls of the enclosure have a light absorbing layer, a diffusing layer, and a photo-detective layer over at least most of their areas. The light absorbing layer is the closest layer to the light-emitting source and is a low-transmission and low-reflection layer that absorbs most of the light incident on it from the light emitting source. According to one implementation, the light absorbing layer has a plurality of pinholes that provide penetration of luminous flux of light through this absorbing layer to ultimately reach the photo-detective layer. The photo-detective layer receives this portion of light from the light emitting source and emits a signal corresponding to a measurement of light impinging on its light receiving surface. The diffusive layer is positioned in between the light absorbing layer and the photo-detective layer and receives light through the pinholes of the light absorbing layer. The diffusive layer then diffuses the light it receives from each pinhole in a predetermined angular distribution onto the photo-detective layer such that the angle of light incident on the diffusive layer does not affect the signal, and thus the measurement, provided by the photo-detective layer.
The light absorbing layer absorbs the majority of light (i) incident thereon from the light-emitting source and (ii) incident thereon from light reflected from the photo-detective layer. This approach essentially eliminates reflections inside the enclosure and between the enclosure and the DUT. Thus, light reflected from the walls of the enclosure and from the photo-detective layer towards the interior of the enclosure and the DUT is minimal such that it does not detract from the accuracy of measurement. It is known with good accuracy how much light is absorbed by the light absorbing layer, and since the vast majority of light from the light-emitting source will be either absorbed in the absorbing layer (the majority of the light) or received and measured by the photo-detectors (a minority of the light), almost all light emitted from the light-emitting source is thus taken into account in the measurement of the incident light and in the calculation of the flux density. This arrangement, wherein most of the light from the DUT is absorbed in the light absorbing layer, is made possible because of the high level of sensitivity of the photo-detective layer, relative to the levels of illumination available from typically measured DUTs. This allows the small amounts of light impinging on the photo-detective layer after attenuation by the light absorbing layer, to be detected and measured with a high level of accuracy. This is in contrast to prior art systems that have multiple reflections that cannot always be accurately predicted or measured, and in which some of the light becomes “lost” from the measurement. The above described light absorbing approach of the presently disclosed systems also provides an advantage over prior art systems that do not intentionally use multiple reflections but that have a significant level of solar panel reflectivity, for example, prior art systems in which light reflects off solar panels and back towards the DUT or out of the enclosure, and thus interferes with the accuracy of measurement.
As an alternative to having an absorbing layer with pinholes, it is possible to use a non-perforated layer that absorbs over the whole of its area, having optical properties that allow a small percentage of the incident light to be transmitted to the photo-detective layer while maintaining very low reflection back to the DUT. Such a layer thus acts in the same way as the pinhole array, limiting reflections from the DUT back into the volume of the enclosure, and limiting reflections from the photo-detective layer back towards the volume of the enclosure and the DUT.
As an alternative implementation, the device may comprise photodiodes disposed within apertures in an absorbing layer. Since the majority of light from the DUT is absorbed by the absorbing layer, there is very little light reflected back from the measurement surface towards the DUT, from which reflections could interfere with the accuracy of the measurement. The spatially sampled portion of light that is collected by the photodiodes passes through a diffusing element disposed on the light impingement surface of each photodiode, such that angular dependent effects are mitigated.
Such exemplary systems of this disclosure further comprise a spectrometer and a flicker sensor. The spectrometer provides measurements used to determine spectral flux and color quality parameters such as CCT (Correlated Color Temperature), CRI (Color Rendering Index), and chromaticity.
There is thus provided in accordance with an exemplary implementation of the devices described in this disclosure, a system for measuring the total luminous flux of a light emitting source, comprising:
a measurement volume, comprising one or more walls adapted to receive light from the light-emitting source, at least a substantial part of at least one of the walls comprising:
In such a system, the light absorbing layer should have an absorption for wavelengths of light emitted by the light emitting source greater than the transmission of the wavelengths through the light absorbing layer. Additionally, according to one implementation of such systems, the reflection from the light absorbing layer may be less than 6%, or it may even be less than 3%.
Yet further implementations of such systems may comprise an optical diffusing layer disposed between the photo-detective layer and the light absorbing layer. In any of such systems, the light absorbing layer may have diffusing properties to light passing therethrough. In such a case, the light absorbing layer may comprise at least one of:
(i) a uniform thickness of diffusive black ink,
(ii) a surface having texturing, and
(iii) scattering particles embedded in the light absorbing layer,
such that the light absorbing layer diffuses the light passing through it.
According to an alternative implementation, the light absorbing layer may be essentially opaque except for a plurality of pinholes providing the transmission of the light therethrough onto the photo-detective layer. In such a case, the density and size of the pinholes are such that the absorption by the absorbing layer of the light emitted by the light emitting source is substantially greater than the transmission of the light therethrough. In any embodiment incorporating pinholes, the plurality of pinholes may be configured to provide access of a spatially sampled portion of light from the light emitting source onto the photo-detective layer. Such a pinhole absorbing layer may further comprise variable density filters disposed in proximity to the light receiving surface of the photo-detective layer opposite the pinholes, such that the attenuation of light passing through the variable density filters is dependent upon the angle of incidence of the light on the pinholes. In any of these cases, the light absorbing layer comprising the pinhole array may be applied using (i) screen printing (ii) digital printing or (iii) a sticker having a printed pattern of pinholes, applied directly to the photo-detective layer.
In accordance with yet other implementations of such systems, as an alternative to the implementations using pinholes, the light absorbing layer may have uniform transmittance. Furthermore, any light absorbing layer may be a separate layer of material. Alternatively, the light absorbing layer may comprise black matte paint.
Yet other implementations may involve a system wherein the level of the absorption of the light absorbing layer is such that the light absorbing layer absorbs more than 94 percent of light incident thereon from the light-emitting source, and more than 94 percent of light incident thereon from light reflected from the photo-detective layer.
In any of the above described systems, the photo-detective layer may be comprised of at least one solar panel, which can be a rigid panel or a flexible solar panel deposited on a thin polymer layer.
Different implementations of the measurement volume may include a closed rectangular box with at least a substantial part of at least one of the walls comprising a transparent plate, and the light emitting source mounted on or suspended from the transparent plate, or a mirror on at least one wall of the measurement volume configured to reflect light to at least one of the walls adapted to receive light from the light-emitting source.
Yet other embodiments of such systems may comprising a photo-sensor, the photo-sensor providing a signal for inputting to a flicker measurement module. Additionally, such systems may further comprise a fiber optic sensor, the fiber optic sensor being configured to deliver light incident on it to a spectrometer. Such a spectrometer may provide information relating to the spectral properties of light emitted from the light-emitting source. The fiber optic sensor may be multi-furcated, such that the fiber optic sensor collects light at least two points from within the measurement volume. The system may also comprise an integrated temperature sensor.
Still other example implementations involve a system for measuring the total luminous flux of a light emitting source, comprising a measurement volume comprising one or more walls adapted to receive light from the light-emitting source, at least a substantial part of at least one of the walls comprising:
In such a system, the level of the absorption of the light absorbing layer may be such that it absorbs the majority of light incident thereon from the light-emitting source. In either of these systems, the density of the array of apertures and the size of the apertures are such that the absorption by the light absorbing layer of the light emitted by the light-emitting source is substantially greater than the transmission of the light therethrough. The light absorbing layer may be screen printed or digital printed, or it alternatively may comprise black matte paint. In all such cases, the level of the absorption of the light absorbing layer may be such that the light absorbing layer absorbs more than 94 percent of light incident thereon from the light-emitting source. In any event, the light absorbing layer should have an absorption for wavelengths of light emitted by the light emitting source greater than the transmission of those wavelengths through the light absorbing layer.
The present invention will be understood and appreciated more fully from the following detailed description, taken in conjunction with the drawings in which:
Reference is first made to
The photo-detective layer 5 may be comprised of photo-detectors, photo-diodes or solar cells, for detecting light and converting it into a measurable electrical signal. The relationship between the intensity of the light reaching the detection surface and the intensity of the electrical signal produced, otherwise referred to as the responsivity, is known for any given wavelength of light. The uniformity of solar panel responsivity is high. For example, when illuminated with white, red, green and blue LEDs, the uniformity of the photocurrent of the solar panels for all of these LED types may generally be better than ±0.3%. The system is used in 2π geometry with the light emitting source positioned over the opening and facing the enclosure walls; thus, the system measures light that is emitted from the light emitting source into a solid angle of 2π steradians.
The system may have a controller (not shown in Figures) that generally includes a microprocessor incorporating software programs for automating various aspects of the measurement operations.
The light emitting source 2 projects light rays 3 towards the wall of the enclosure 6. The light absorbing layer 4 is shown to be the innermost layer of the enclosure, and is the first layer to receive light 3 from the light emitting source 2. The light absorbing layer 4 may be painted with an opaque, high-absorption black matte paint such that most of its surface is absorptive. Due to the low reflectance level of the black matte paint, only a small percentage of the light emitted by the light emitting source 2 is reflected back into the volume of the system. The light absorbing layer 4 absorbs the majority of light incident thereon, both light incident thereon from the light-emitting source 2, and also light reflected from the photo-detective layer 5 that falls on the opposite side of the absorbing layer 4 to that of the light source 2. Such a majority of light absorbed by the absorbing layer 4 from both sides may be for example, 90%, 95% or 98%, or even more, of the light incident thereon.
The light absorbing layer 4 may comprise a dense array of pinholes 9 through which a minority of light 3 may pass to the diffusive layer 20 and ultimately to the photo-detective layer, where it is measured. Light incident on the panel 6 of the enclosure 1 is therefore spatially sampled by this dense pinhole array 9.
A diffusive layer, or diffusing plate 20, is shown in between the light absorbing layer 4 and the photo-detective layer 5, whose function is described more fully in accordance with
In yet another alternative implementation of the present disclosure, the pinhole array is applied directly on the solar cells or solar panels using screen printing or digital printing, or a sticker having a printed pattern of pinholes applied to the panels. A diffusing layer is not needed in this implementation because the apertures of the pinhole array are cosine corrected, provided that the absorbing layer with the pinhole array is sufficiently thin.
In yet another implementation of the present disclosure, instead of a pinhole array, a uniform absorbing layer, such as black ink, is applied to the photo-detective layer. The thickness of the layer of ink is controlled, for example to be 30 μm thick over the entire area of the photo-detective layer, and the ink is selected to have a limited predetermined reflectivity, and high absorptivity. Thus, this uniform layer has a predefined and uniform transmittance with a good cosine corrected response. The uniform transmittance allows light to pass through to the photodetectors. Such a layer may be very thin, for example 30 μm, or it may have a surface relief, such as of cone shapes, or it may have scattering particles impregnated in the layer giving the layer diffusive properties without the need for a separate diffusing layer.
In any of the above implementations of the present disclosure, the photo-detective layer may be realized by using flexible solar panels such as amorphous silicon solar panels deposited on a thin polymer layer, such as PET (polyethylene terephthalate). This will allow for creation of a variety of measurement cavities with different shapes.
While it is understood that the most common embodiment is to have the absorbing layer, diffusive layer, and photo-detective layer on all the walls of the enclosure, alternative implementations may have these layers only on a substantial portion of one of the walls of the enclosure. For example, the system can be built with a single absorbing plate, such as at the bottom of the measurement enclosure that may be positioned close to and opposite the DUT. This arrangement makes this implementation of the system very simple, small and lightweight. Alternatively, the system can be built as a box with a single absorbing plate on one wall, and mirrors that reflect light from the DUT to the absorbing plate. For example, one efficient arrangement of this disclosure positions the single absorbing plate on the bottom of the enclosure, and the mirrors on the side walls of the enclosure.
The following section now presents the mathematical derivation of the spectral flux and total flux measurement, using inputs from one of the exemplary systems described above. For clarity, it is assumed that the detection surface responsivity is spatially uniform and is not sensitive to illumination angle. It is further assumed a spectrometer is used to sample the spectrum of the DUT and that the spectral content of the DUT is uniform in all directions. A more realistic analysis is brought in the next section.
The total current, I, produced by the photo-detective layer is given by:
I=∫R(λ)Φe(λ) (1)
where R(λ) is the responsivity of the photo-detective layer in [A/W], and Φe(k) is the spectral flux of the DUT in [W/nm]. The spectrometer measures the normalized spectrum S(λ) given by:
where Φe is the total flux of the DUT in [W]. The normalization is achieved by scaling S(λ) such that ∫S(λ)dλ=1.
Having measured S(λ) with the spectrometer, color quality parameters such as CCT, CRI, and chromaticity can be calculated directly since they depend only on the spectral profile.
Substituting (2) into (1) and rearranging yields
Substituting again into (2) yields the spectral flux in [W/nm]
Having obtained the spectral flux Φe(λ), the total luminous flux in lumens is calculated using:
where V(λ) is the human visual sensitivity function or photopic function.
As mentioned previously, the angular dependence of the photo-detective layer's responsivity on illumination angle is low with use of the diffusing plate, increasing the accuracy of measurement.
In this model, the LED luminaire 60 is positioned over the enclosure opening. The luminaire surface is divided into area elements dAS, and the detection surfaces are divided into area elements dAR. For every dAS and dAR, the flux element dΦ, incident on dAR is calculated, based on the subtended solid angle dΩ and the luminance, L of the luminaire. The total incident flux on the photo-detective layer is given by:
Φv=∫∫A
and the total detected flux of the photo-detective layer is given by:
Φ′v=∫∫A
The difference in the ratio between Φv and Φ′v for different luminaire sizes and illumination beam angles is the uncertainty contribution of the nonideal K(θ). As the luminaire size and beam angle increase, more rays hit the panels at high slant angles (greater angles of incidence) and the effect of K(θ) is more noticeable. Thus, it is desirable to use a diffusing plate that keeps K(θ) as close to 1 as possible. As shown previously in
Referenced is now made to Table 1 below, which shows that the error due to the sensitivity to illumination angle, K(θ), of the presently disclosed system ranges between −1.2%, for a small and narrow beam DUT, and −6.3%, for a large and wide beam DUT. If the system is calibrated using a calibration standard with a beam angle of 80° FWHM, the error will be shifted to ±2.6%.
Below is a table showing the reduced photocurrent due to angular response of an exemplary solar panel for different luminaire sizes and beam angles using an enclosure of 640 mm (length)×480 mm (width)×160 mm (height):
Furthermore, since this is a systematic and predictable error, in a novel method of the present disclosure, a correction factor can be applied based on the size and beam angle of the luminaire being measured. An example of this correction is shown in table 1 below, which shows the reduced photocurrent due to angular response of the solar panel for different luminaire sizes and beam angles. For example, for a luminaire size of 70×50 mm and a FWHM angle of 20 degrees, a correction factor of −1.2% should be applied to the calculation of total flux. By measuring the current of individual solar cells or photodiodes in the absorber array, information on the angular distribution of light from the DUT can be obtained. By modeling the system's response to various DUT sizes and beam angles, as shown for instance in the table below, correction factors can be applied. There may be software controlling the system that applies these correction factors automatically, upon receiving the DUT size and beam angle.
In addition to the photo-detective layer 5, which may be covered by an absorbing layer on the inner walls of the enclosure, the implementation shown in
To illustrate this implementation, a ray of light 30 having a certain luminous flux, passing through the pinhole 9 normally without the variable density filter would have a predefined luminous flux density on the surface of the photodetector 5. On the other hand, a ray of light 31, having the same luminous flux as ray 30, incident at an angle 61 to the normal (approximately 35 degrees in
As an alternative to the implementation of the single fiber optic sensor 50 in
In most prior art integrating sphere systems, self-absorption of the DUT has a large effect on the measurement. This is because the DUT changes the average reflectivity of the sphere which, in turn, greatly affects the sphere's throughput. Calculating this effect is not practical due to the infinite number of reflections that occur inside the sphere, and it must be calibrated for every DUT.
In contrast, in the presently disclosed system, the reflectivity of the black pinhole array seen in
Furthermore, in an exemplary method of the present disclosure, LEDs may be placed at different positions on the enclosure walls, allowing the effect of the DUT to be measured. The LEDs point outward and a measurement is taken with these LEDs serving as the light source with the DUT removed, and then with the DUT placed on the system, with the DUT is off during both of these measurements. The difference between the two measurements is due to the reflection of the DUT and can be used to calculate the effect of the reflectivity of the DUT on the system measurement.
The following correction methods of the present disclosure can be applied to mitigate this small reflectivity of the light absorbing layer and its effects:
(a) A fixed 2% may be added to the initial calibration to shift the error from 0%-4% to ±2%.
(b) A phenomenological correction may be applied based on the size and tone of the luminaire surface.
(c) A light source may be added to the system for automatic reflection correction. The light source may be activated with and without the DUT present. The measured signal in these two cases can be used to determine the reflection from the DUT and be used to correct the measurement of the DUT. For example, a LED on the bottom of the enclosure may flash to measure the reflectance of the DUT right before the measurement is made.
The uncertainties discussed in the previous sub sections are summarized in Table 2 below. Table 2 shows uncertainty contributors and the percentage of uncertainty of each contributor, with and without correction factors, and including total percentages. The uncertainty, and the corrected uncertainty is shown for each uncertainty contributor. Since there are systematic errors, they are summed arithmetically and not geometrically (rms). The resulting total uncertainty is, for example, 7.8%. However, by applying various correction factors as described earlier, a low total uncertainty, for example, of 4.3%, can be reached.
The initial total flux calibration is an absolute calibration, such as for NIST standards. It is known that the optical output of light sources changes as the source heats up, until it reaches thermal equilibrium. Waiting until the DUT reaches thermal equilibrium to perform optical measurements may be inefficient in terms of the time taken to perform the measurement. It is therefore advantageous to be able to perform optical measurement shortly after the DUT is turned on, and, based on that measurement, to confidently predict the optical output after the DUT will have reached thermal equilibrium. In a novel exemplary method of the present disclosure, the system software performs measurements over long periods of time, for example hours or days, and based on the information gathered, the software automatically determines the optimal timing for measurement, shortly after the DUT is turned on, the relationship between the measurement and the optical output after the DUT has reached thermal equilibrium, and the confidence level of this prediction. A fast photodiode incorporated in the presently disclosed systems can be used to automatically detect when the DUT is turned on and thus to apply the required delay before the measurement in a precise and controlled fashion, for example, to commence the measurement automatically and at a controlled time delay following the turning on of the DUT.
Although it is understood that the most common implementation of the enclosure is a rectangular box as shown in
It is appreciated by persons skilled in the art that the present invention is not limited by what has been particularly shown and described hereinabove. Rather the scope of the present invention includes both combinations and subcombinations of various features described hereinabove as well as variations and modifications thereto which would occur to a person of skill in the art upon reading the above description and which are not in the prior art.
Filing Document | Filing Date | Country | Kind |
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PCT/IL2017/050862 | 8/3/2017 | WO | 00 |
Number | Date | Country | |
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62370791 | Aug 2016 | US |