This invention relates to a fight assembly having an integrated test facility, in particular, this invention relates to a photo detector integrated with the light assembly that can be used to measure the quantity of the light flux distributed through a fight output aperture of the light assembly.

Information about the quantity of the light flux distributed through the light output aperture of the light assembly is a critical safety parameter in many applications including, but not limited to, automotive signalling and position light assemblies and/or airborne signalling and position light assemblies and/or marine signalling and position fight assemblies and/or submarine signalling and position light assemblies. The quantity of the light flux required for the specific application distributed through the light output aperture of the light assembly can be compromised during operational conditions, for a number of reasons.

The light flux distributed through the fight output aperture can fluctuate as a result of changes in light source properties and/or a result of changes in optical properties of the light output aperture itself. Visual checking of the light assembly optical properties such as light beam geometry and/or intensity can be difficult to obtain and is often inaccurate. An unexpected accumulation of dust, ice or water vapour on the light output aperture and/or mechanical damage to the light output aperture can also decrease the lamp light flux without the lamp operators' awareness, and can lead to a catastrophic failure of the device containing such a light assembly,

In order to address these problems, various pieces of remote test equipment which use photo detectors have been developed to check and record the intensity, direction and angular distribution of the light assembly similar to that known in the automotive industry. It is an object of the present invention to provide a light assembly that includes an Integrated test facility which can be used to provide monitoring of the Sight flux passing the light output aperture to indicate when the light output aperture s damaged or dirty, and/or the light source starts to degrade and may need replacement or repair, it is a further object of the present invention to provide a measurement of the light flux distributed through the light output aperture emitted from sources of light within the assembly in the presence of dynamically changing ambient light.

According to the present invention there is provided a light assembly, comprising:

a base;

at least one electromagnetic radiation source mounted on the base;

a cover located over the base, the cover being transparent to the electromagnetic radiation produced by the electromagnetic radiation source; and

at least one photo detector, optically isolated from the at least one electromagnetic radiation source, the at least one photo detector being configured to receive electromagnetic radiation conveyed by the cover.

By optically isolating the at least one photo detector from the at least one electromagnetic radiation source, the at least one photo detector is advantageously configured to receive electromagnetic radiation conveyed by the cover. An advantage of using the present invention for delecting the electromagnetic radiation emitted from the at least one electromagnetic radiation source Is that an operator is quickiy able to diagnose that the electromagnetic radiation source is failing, or is about to fail, or that the cover surrounding the electromagnetic radiation source is dirty or damaged. It is to be understood that term "optically isolated" is intended to define arrangements where the electromagnetic radiation produced by the electromagnetic radiation source is not directly detected by at least one photo detector, Preferably, the light assembly comprises a plurality of electromagnetic radiation sources.

Further preferably, the light assembly comprises a pluraiity of electromagnetic radiation sources disposed in a matrix.

In use, the or each electromagnetic radiation source may comprise an LED.

Preferably, the at least one photo detector comprises a photodiode,

Further preferably, the light assembly comprises an optical waveguide coupled between the cover and the at least one photo detector.

In use, the optical waveguide may comprise a light pipe.

Preferably, the light pipe is configured as a solid transparent structure that contains the electromagnetic radiation by total internal reflection.

Further preferabiy, the light pipe is configured as a hollow structure having a generally circular cross-section that contains the electromagnetic radiation within a reflective lining.

In use, the light pipe may have a first end optically coupled to the cover, and an opposite second end which is optically coupled to the at least one photo detector. Preferably, the light pipe is an extruded or moulded part of the cover. In use, the cover may further comprise shielding means adjacent to the first end of the light pipe to prevent ambient electromagnetic radiation directly from entering the light pipe, Preferably, the shielding means is an internally mirrored diaphragm.

Further preferably, the shielding means is a metaiised foil or opaque window. In use, the at least one photo detector may be disposed in the base.

Preferably, the electromagnetic radiation produced by the electromagnetic radiation source is visible light.

Further preferably, the electromagnetic radiation produced by the electromagnetic radiation source Is selected from the group of X~rays ₍ ultraviolet, infrared and microwaves,

In use, the at least one photo detector may detect the scattered light S ^* which is distributed through the cover, the scattered light S' being the sum of the forward light produced by the at least one electromagnetic radiation source F and the ambient light falling on the cover A.

Preferably, the scattered light from ambient light S'A is measured during a first period when the at least one electromagnetic radiation source is turned off. Further preferably, the light assembly comprises a processing means for controlling the at least one electromagnetic radiation source and the at least one photo detector. In use, an estimation of the scattered light from the forward light (ST) may be obtained from the equation, S'{F÷A) - S'A, where the scattered light from ambient Sight S'A Is measured during a first period when the at least one electromagnetic radiation source is turned off.

Preferably, the processing means synchronises the measurement of the scattered light as the at least one electromagnetic radiation source is pulse width modulated on and off.

Further preferably, the output of the at least one photo detector is connected to a eurrent- to-volfage converter implemented on an operational amplifier, the output of which is inputted to the processing means.

In use, the light assembly may further comprise two photo detectors connected in antiphase to each other.

Preferably, the light assembly may further comprise a band pass filter coupled between the optical waveguide and the at least one photo detector, the band pass filter having a central wavelength that is matched to the wavelength of the at least one electromagnetic radiation source.

Also according to the present invention there is provided a method of measuring the electromagnetic radiation distributed within the cover of a light assembly of the first aspect of the invention, the method comprising the steps of;

turning on the at least one electromagnetic radiation source and measuring the electromagnetic radiation which is distributed through the cover using at least one photo detector optically isolated from the at least one electromagnetic radiation source; turning off the at least one electromagnetic radiation source and measuring the radiation failing on the at least one photo detector; and

subtracting the measured ambient electromagnetic radiation from the measured electromagnetic radiation to give an estimation of the total electromagnetic radiation flux emitted from the at least one electromagnetic radiation source.

Preferably, the method further comprising the step of:

matching the wavelength of the at least one electromagnetic radiation source to the at least one photo detector using a band pass filter,

Further preferably, the method further comprising the step of:

turning on the at least one electromagnetic radiation source and measuring the forward light which is distributed through the cover using two photo detectors connected in anti-phase.

In use, the steps of turning on the at feast one electromagnetic radiation source and measuring the forward light which is distributed through the cover and turning off the at least one electromagnetic radiation source and measuring the ambient light falling on the at least one photo detector may be achieved by pulse width modulating the at least one electromagnetic radiation source on and off under the control of the processing means.

Further according to the present invention there is provided a computer program product for measuring the electromagnetic radiation distributed within the cover of a light assembly of the first aspect of the invention, comprising:

computer program product means for turning on the at least one electromagnetic radiation source and measuring the forward electromagnetic radiation which is distributed through the cover using at least one photo detector optically Isolated from the at least one electromagnetic radiation source;

computer program product means for turning off the at least one electromagnetic radiation source and measuring the ambient electromagnetic radiation falling on the at ieast one photo detector; and

computer program product means for subtracting the measured ambient electromagnetic radiation from the measured forward electromagnetic radiation to give an estimation of the total electromagnetic radiation flux emitted from the at Ieast one electromagnetic radiation source.

It is believed that a light assembly that includes an integrated test facility at Ieast addresses the problems outlined above. The advantages of the present invention are that an operator of the light assembly is able to diagnose the optical properties of the light source incorporated into the light assembly continuously during light assembl ^" operation and in real time. The present invention also provides information on the protective cover surrounding the light assembly such as whether it is dirty, damaged or otherwise advising that the cover needs cleaning.

It will be obvious to those skilled in the art that variations of the present invention are possible and it is intended that the present invention may be used other than as specifically described herein.

Specific non-limiting embodiments of the invention will now be described by way of example only and with reference to the accompanying drawings, in which:

Figure 1 is a cross sectional view of a first embodiment of a light assembly according to the present invention; Rgure 2 shows a method of measuring the light flux distributed through the fight cover of a light assembly according to the present invention; Rgure 3 is a plan view from above of a second embodiment of the fight assembl according to the invention, where a differentia! measurement of the light fluxes is made at points PA and PB;

Rgure 4 is a schematic diagram showing how the present invention can be implemented under the control of a microprocessor.

Referring now to the drawings, the light assembly 100 comprises a light source mounting base 101 having a generally planar non-transparent upper surface 103 and a hemispherical transparent plastics domed light cover 108 mounted sealingly to the surface 103 (e.g. by means of adhesive), A light source 104 is mounted on the upper surface 103 of the base 101 and, when actuated, projects light into and through the domed light cover 108. This fight flux, which is transmitted through the domed light cover 108, is shown for illustration purposes only by fight ray F in Figure 1. In the embodiment shown in Figure 1 , the light source 104 is a semiconductor light emitting diode.

Figure 1 also shows that an optical waveguide 108 extends between the domed light cover 108 and the interior of the base 101. The optical waveguide 108 is used for transporting the scattered light that is distributed throughout the hemispherical cover 106 to a photo detector 105 embedded in the light assembly 100. The photo detector 105 embedded in the light assembly 100 is optically shielded from stray light by optical shield 105A. Figure 1 shows that the photo detector 105 and the fight source 104 are connected to a processing means 102 situated in the fight assembly 100. The photo detector 105 is understood to be a device able to convert light flux to eiectrica! quantities, The optical waveguide 108 comprises a first portion 18A which extends perpendicularly from the inner surface of the hemispherical cover 106 and a second portion 188, optically continuous with the first portion 18A, which passes perpendicularly through the planar upper surface 103 of the base 102. The walls of the optical waveguide 108, between the cover 106 and upper surface 103 of the case are coated by non-transparent light means 108C, which prevents any stray light from entering the optical waveguide 108 from the side walls 108C,

Figure 1 also shows that, at the position where the first portion 108A of the optical waveguide 108 extends perpendicularly from the inner surface of the hemispherical transparent light cover 108, the outer surface of the light cover 108 Is covered by an infernally mirrored diaphragm 109 which prevents ambient or stray light from entering the optical waveguide 108 directly. The annular periphery of the domed lens 16, which abuts the surface 13 of the base 12, is also internally mirrored (shown at 28) for reflecting the scattered light distributed through the front protection fens 18.

It is important to note that the photo detector 105 is optically isolated from the light source 104 and never directly senses the light flux F from the light source 104 and/or the ambient light flux A that which is also distributed through the light cover 108. The ambient light flux, which is distributed through the fight cover 108, is shown for illustration purposes only by line A in Figure 1. The photo detector 105 detects the scattered light S'(F ) which is distributed through the hemispherical transparent light cover 108. An estimation of the scattered forward light S'F is a computation result S'(F÷A) - S'A, where the scattered ambient light S'A is measured during a period when the light source 104 is turned off.

The skilled person will appreciate that if the ambient light A is reduced to zero by, for example, covering the light cover 108, then the output of the photo detector 105 Is equal to the scattered forward light S'F only, and gives an estimation of the total light flux of he light source 104. By recording this value over successive measurements the present invention permits the quantification and recognition of degradation of the light source 104 before the risk of a cri!Ica! failure.

Equaliy, by measuring the output of the photo detector 105 when the light source 104 is turned off, which can be achieved by synchronising the measurement to the pulse width modulated control signal, an estimation of the scattered ambient light S'A can be obtained. The measured scattered ambient light S'A therefore provides information on the domed light cover 106.

The photo detector 105 is therefore capable of measuring and diagnosing the light flux in the following conditions: total light flux in a wide range of offset light (ambient/background light);

ii) light flux degradation due to aging or fault of the light source 104 within the light assembly 100;

iii) hemispherical light cover 108 degradation due to accumulation of ice, dust and water vapour;

iv) hemispherical light cover 108 degradation due to mechanical damage; and v) degradation ofjhe light beam geometry due to mechanical damage.

Figure 2 shows the method of measuring the tight flux distributed through the light cover 106 of the light assembly 100 by measuring the output of the photo detector 105 when the fight source 104 is turned on and off, which can be achieved by synchronising the measurement to pulse width modulated control signals.

As shown in Figure 2, each measurement N essentially comprises three steps, numbered as steps S__1 , S__2 and 5_3. The first step S__1 of the measurement procedure involves turning on the light source 104 incorporated into tight assembly 100 and measuring the scattered light from the total light flux distributed through the light cover 108 and recording the result as S'(F+A). The second step S_ 2 involves turning off the light source 104, previously energised in S__1 ₁ and measuring the scattered light from the total light flux distributed through the cover 108 and recording as a result S'A, The final and final step S_3 is to estimate the scattered light flux from the light source 104 energised in S_1 by subtracting the S'F~ S'(F+A) - S'A.

Whilst the embodiment shown in Figure 1 shows how the present Invention operates with a single photo detector 105 to measure the total ambient light and measure total light flux, in a further embodiment of the invention, as illustrated in Figure 3, two or more photo detectors 305A and 305B located at points PA and PB„ respectively, are able to perform a differential mode light measurement, as follows.

Figure 3 shows schematically the principle of differential light measurement, The light assembly 300 of Figure 3 is identical to that of the first embodiment, but a plurality of light sources LS are mounted on its planar upper surface, The light assembly of Figure 3 is also provided with a hemispherical light cover 106, as in Figure 1 , which is not illustrated in Figure 3. However, two optical waveguides (not shown), identical to the optical waveguide 108 of Figure 1 , are provided, each conveying fight to a respective one of two photo detectors 3Q5A and 305B located at points PA and PS, identical to the photo detector 105 of Figure 1,

Measurements obtained using two differentially-connected photo detectors 305A and 3058 respectively at points PA and PB gives better noise to signal ratio of processed signals because it measures the offset between light flux, at points PA and PB, which operate at the similar common mode signal level, as described above in relation to the embodiment of Figure 1.

Figure 3 shows that fauity Sight sources, respectively LS{n) and LS(n*1), incorporated into the light assembly 300 and/or damage to the light assembly 300 geometry and/or damage to the light output aperture of respectively L5(n) and LS(n*1) will cause changes in the distributed light flux Φ(ΡΑ_Α), 0(PA_LSn), t>(PA_LSn+1) and/or Φ(ΡΒ _„ Α}, <t>(PBJ-Sn), P{PBJ_Sn 1) _t respectively, and will change the light flux offset respectively Δ Ρ, ΔΦΡ' between points PA and PB, which will be outputted as an imbalanced signal. The light flux offset respectively ΔΦΡ» ΔΦΡ' between points PA and PB are therefore constant in uniform ambient Sight A as Song as the magnitudes of distributed Sight flux from the Sight sources respectively LS{n) and LS(n*1) incorporated into the light assembly 300 stay unchanged and/or properties of light distribution path within the light assembly 300 stay unchanged.

In use, the differentially-connected photo detectors light flux measurement is particularly usefuf in an application where light sources LS incorporated into the light assembly 300 are connected in a matrix, such as LEDs to produce a high intensity output light flux and/or output light flux of specific geometry. In the left hand figure of Figure 3, the total brightness of the two differentially-connected photo detectors 30SA and 305B located at points PA or PB and each receiving iighi from a respective optical waveguide, is a sum of the brightness contributed by the plurality of light sources LS and the ambient Sight measurement A.

The brightness offset between points PA and PB is therefore constant in uniform ambient fight A as long as the distributed light fluxes from the light sources LS and the assembly geometry stays unchanged, and the output from the differentially-connected photo detectors 305A and 305B is therefore equal and opposite.

A faulty light source (in the example shown in the right hand of Figure 3, light source LS{n 1 ) 6 starts to degrade) or damage to the assembly geometry will cause changes in the distributed fight fluxes, and will change the brightness offset between points PA and PB which will be outputted from the differentially-connected photo detectors positioned at points PA or PB as an imbalance signal.

The differential mode of operation is particularly useful in LED aviation applications where the high intensity output of the light assembly 300 makes it difficult to recognise and detect degradation from a common mode measurement. For example, a high power LED landing light might contain 19 LEDs disposed in matrix producing a peak intensity 400,000cd. A measurement obtained using the "common mode" technique described in relation to Figure 1 would give us information about the total light flux and front cover 106. Measurements obtained using two differentially-connected photo detectors 305A and 305B gives better resolution because it measures the brightness offset between points PA and PB which helps to more accurately detect light flux degradation due to aging or failure of the LEDs disposed within the light assembly 300. Figure 4 is a schematic diagram showing how the common mode and differential measurement techniques of the present invention can be implemented using a microprocessor-controlled electronic detection circuit.

Figure 4 shows a schematic diagram of an electronic circuit which is to monitor a number photo detectors 405A, 405Bn, 405Bn÷1. This detection circuit is realised using a processing means 402 such as a microprocessor. The skilled person will appreciate that, in operation, a set of instructions or algorithm written in software in the processing means continually monitors the output of a current-to-voitage converter implemented on an operational amplifier 412 which has a number photo detectors 405A, 405Bn ₍ 4G5Bn+1 connected at its input, The skilled person will also appreciate that for purposes of clarity many of the analogue signals being inputted to the processing means 402 are first converted to digital form by any suitable type of analogue-to-digital (ADC) conversion. This ADC conversion is not shown in Figure 4. Other circuit functions such as, for example, bus interfaces and memory are also not expressly shown in Figure 4.

Figure 4 shows that in a common mode of operation, photo detectors 405Bn and 4G5Bn÷1 are disabled and the output of a single photo detector 405A positioned at point PA in the light assembly is processed by the current-to-voltage converter implemented on the operational amplifier 412. In common mode operation, the output of the current-to- voitage converter is proportional to the scattered light S'{F÷A) which ss distributed through the hemispherical cover 108. In the differential mode of operation, the photo detector 405A at point PA is used as a reference signal source to differentially connect one~at~a~tsme, photo detectors respectively 405Bn, 4GSBn-M positioned in the detector matrix. In differential mode of operation, the imbalance in scattered light between the reference point PA and a given measurement point PB or PBn-M iif force an imba!anced signal on the output of current-to-voltage converter. Figure 4 also shows that the present invention can include a self-test built-in light source 415 optically connected to the photo detector 405A _S which can be used to validate the photo detector 405A response to the optical stimulus.

The estimation of scattered light from the light source forward light (S'F) is a computation result S'{F÷A)-S'A, where the scattered light S'A from ambient is measured during the period when the light sources are off. This can be achieved by synchronising the measurements as the light sources are pulse width modulated on and off under the control of the processing means 50, By implementing the present invention in software, the photo detector's 405A, 405Bn, 405Bn÷1 optical parameters, including QE and dark current, are subject to temperature shift and can be compensated for by software, It is also possible, in software, to compensate for the light source temperature to give better measurement discrimination. Figure 4 also shows that optical input aperture of the photo detectors respectively 405A, 405Bn, 4G5Bn÷1 are each covered by absorptive neutral density and band pass optical filters OF.

Various alterations and modifications may be made to the present invention without departing from the scope of the invention. For example, although particular embodiments refer to a light assembly with sources of light understood to be a source of electromagnetic radiation whose significant part of the power radiated spectrum is infrared IR and/or visible spectrum VIS and/or ultraviolet IN, this can include, but not limited to, light emitting semiconducior devices and/or filament bulbs and/or incandescent bulbs.

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