This invention relates to the field of general illumination, and more specifically, to illumination devices using semiconductor based lighting elements such as light emitting diodes (LEDs).
The use of light emitting diodes in general lighting is still limited due to limitations in light output level or flux generated by the illumination devices. Limits in flux are due to the limited maximum temperature of the LED chip, and the life time requirements, which are strongly related to the temperature of the LED chip. The temperature of the LED chip is determined by the cooling capacity in the system, and the power efficiency of the device (optical power produced by the LEDs and LED system, versus the electrical power going in). Illumination devices that use LEDs also typically suffer from poor color quality characterized by color point instability. The color point instability varies over time as well as from part to part. Poor color quality is also characterized by poor color rendering, which is due to the spectrum produced by the LED light sources having bands with no or little power. Further, illumination devices that use LEDs typically have spatial and/or angular variations in the color. Additionally, illumination devices that use LEDs are expensive due to, among other things, the necessity of required color control electronics and/or sensors to maintain the color point of the light source or using only a small selection of produced LEDs that meet the color and/or flux requirements for the application.
Consequently, improvements to illumination device that uses light emitting diodes as the light source are desired.
A light emitting diode module is produced using at least one light emitting diode (LED) and at least two selectable components that are a part of a light mixing chamber that surrounds the LEDs and includes an output port. A first selectable component has a first type of wavelength converting material with a first wavelength converting characteristic and a second selectable component has a second type of wavelength converting material with a different wavelength converting characteristic. The first and second wavelength converting characteristics alter the spectral power distribution of the light produced by the LED to produce light through the output port that has a color point that is a predetermined tolerance from a predetermined color point. Moreover, a set of LED modules may be produced such that each LED module has the same color point within a predetermined tolerance. The LED module may be produced by pre-measuring the wavelength converting characteristics of the different components selecting components with wavelength converting characteristics that convert the spectral power distribution of the LED to a color point that is a predetermined tolerance from a predetermined color point.
The LED module 100 includes a base 110 and a top section 120, which may be manufactured from highly thermally conductive material, such as an aluminum based material. The base 110 includes a board 112 with a plurality of LEDs 114 that may be symmetrically arranged. In one embodiment, the LEDs 114 are packaged LEDs, such as the Luxeon Rebel manufactured by Philips Lumileds Lighting. Other types of packaged LEDs may also be used, such as those manufactured by OSRAM (Ostar package), Luminus Devices (USA), or Tridonic (Austria). As defined herein, a packaged LED is an assembly of one or more LED die that contains electrical connections, such as wire bond connections or stud bumps, and possibly includes an optical element and thermal, mechanical, and electrical interfaces. The LEDs 114 may include a lens over the LED die. Alternatively, LEDs without a lens may be used. The board 112 provides electrical and thermal contact with the LEDs 114. The board 112 is also in thermal contact with the base 110, which acts as a heat sink. The board may be an FR4 board, e.g., that is 0.5 mm thick, with relatively thick copper layers, e.g., 30 μm to 100 μm, that serve as thermal contact areas. Alternatively, the board 104 may be a metal core printed circuit board (PCB) or a ceramic submount with appropriate electrical connections. Other types of boards may be used, such as those made of alumina (aluminum oxide in ceramic form), or aluminum nitride (also in ceramic form). The board 112 may include a reflective top surface or a reflective plate 113 may be mounted over the top surface of the board 112. The reflective plate 113 may be made manufactured from a material with high thermal conductivity, such as an aluminum based material that is processed to make the material highly reflective and durable. By way of example, a material referred to as Miro®, type Miro 27 Silver, manufactured by Alanod, a German company, may be used.
If desired, the base 110 may be produced from multiple pieces. For example, the base 110 may include a lower section 116 through which electrical connection to the board 112 is made and an upper section 118 that is attached to the lower section 116, e.g., by screws 117 (shown in
The top section 120 includes a center aperture 122 that extends through the top section 120. The top section 120 is attached to the base 110 by screws 124, bolts, or other appropriate attachment mechanism. For example, the top section 120 may be screwed onto the base 110 if desired. An output port is defined by the center aperture 122 and is covered with a window 130 that is mounted to the upper surface of the top section 120, e.g., by epoxy, silicone or other appropriate attachment mechanism. The window 130 may be transparent or translucent to scatter the light as it exits. The window 130 may be manufactured from an acrylic material that includes scattering particles, e.g., made from TiO2, ZnO, or BaSO4, or other materials that have low absorption over the full visible spectrum. In another embodiment, the window 130 may be a transparent or translucent plate with a microstructure on one or both sides. By way of example, the microstructure may be a lenslet array, or a holographic microstructure. Alternatively, the window 130 may be manufactured from AlO2, either in crystalline form (Sapphire) or on ceramic form (Alumina), which is advantageous because of its hardness (scratch resistance), and high thermal conductivity. The thickness of the window may be between e.g., 0.5 and 1.5 mm. If desired, the window may have diffusing properties. Ground sapphire disks have good optical diffusing properties and do not require polishing. Alternatively, the diffuse window may be sand or bead blasted windows or plastic diffusers, which are made diffusing by dispersing scattering particles into the material during molding, or by surface texturing the molds.
A sidewall insert 126 may be positioned within the center aperture 122 of the top section 120 to define the sidewalls. Alternatively, the sidewalls may be defined by the walls of the aperture 122 itself. The sidewall insert 126 may be, e.g., manufactured from a material referred to as Miro®, type Miro 27 Silver, manufactured by Alanod, a German company. The sidewall insert 126 may be produced as a strip of material that is bent to form a ring shape. When assembled, a light mixing chamber 101 is defined by the sidewalls of the center aperture 122 of the top section 120, e.g., the sidewall insert 126, along with the window 130 and the reflective bottom surface, e.g., the reflective plate 113 on the board 112 of the base 110, which are, therefore, sometimes collectively referred to as components of the chamber 101.
The light mixing chamber 101 of the LED module 100 may be formed from different or additional components. For example, as illustrated in cross-sectional view in
At least two of the components of the chamber 101 are coated or impregnated with different wavelength converting materials, and are sometimes referred to herein as wavelength converting components. The different types of wavelength converting materials on the wavelength converting components have different wavelength converting characteristics. By way of example, the window 130 may be coated with a first type of wavelength converting materials 132 that, e.g., converts blue light to yellow light, while the sidewall insert 126 may be coated with second type of wavelength converting material 128 that, e.g., converts blue light to red light. In one embodiment, the sidewall insert 126 is not used and the sidewalls of the center aperture 122 are coated with a wavelength converting material. If desired, the reflective plate 113 may be coated with wavelength converting material that may be the same or differ from the other wavelength converting materials on other wavelength converting components. If desired, the top and bottom sidewall inserts 126, 127 and/or windows 130, 131 (
The wavelength converting materials may be phosphor or luminescent dyes, which will be generally referred to herein as phosphor for the sake of simplicity. By way of example, the phosphors used as the wavelength converting materials may be chosen from the set denoted by the following chemical formulas: Y3Al5O12:Ce, (also known as YAG:Ce, or simply YAG), Lu3Al5O12 (also known as LuAG:Ce, or simply LuAG), (Y,Gd)3Al5O12:Ce, CaS:Eu, SrS:Eu, SrGa2S4:Eu, Ca3(Sc,Mg)2Si3O12:Ce, Ca3Sc2Si3O12:Ce, Ca3Sc2O4:Ce, Ba3Si6O12N2:Eu, (Sr,Ca)AlSiN3:Eu, CaAlSiN3:Eu. The phosphor or combination of phosphors may be mixed as a dispersion in a binder for application to a surface by spray painting, screen printing, stenciling, or doctor blading techniques. These techniques are useful to deposit small dots of phosphor, stripes of phosphor, or to uniformly coat the surface. Alternatively, the phosphor or combination of phosphors may also be mixed in powder form with small pellets of binding material for application to a surface, e.g., by spraying or by application of an electric field, as part of a powder coating process. The small pellets have a low melting point and uniformly coat the surface when heated to the melting point of the binder.
With the two or more of wavelength converting components of the light mixing chamber 101 each with different wavelength converting properties, the LED module 100 may produce a predetermined or target color point with a high degree of accuracy.
An LED is typically binned after a production run based on a variety of characteristics derived from their spectral power distribution. The cost of the LEDs is determined by the size (distribution) of the bin. For example, a particular LED may be binned based on the value of its peak wavelength. The peak wavelength of an LED is the wavelength where the magnitude of its spectral power distribution is maximal. Peak wavelength is a common metric to characterize the color aspect of the spectral power distribution of blue LEDs. Many other metrics are commonly used to bin LEDs based on their spectral power distribution (e.g. dominant wavelength, xy color point, uv color point, etc.). It is common for blue LEDs to be separated for sale into bins with a range of peak wavelength of five nanometers.
As discussed above, LED module 100 includes a board 112 with a plurality of LEDs LEDs 114. The plurality of LEDs 114 populating board 112 are operable to produce light with a particular spectral power distribution. The color aspect of this spectral power distribution may be characterized by its centroid wavelength. A centroid wavelength is the wavelength at which half of the area of the spectral power distribution is based on contributions from wavelengths less than the centroid wavelength and the other half of the area of the spectral power distribution is based on contributions from wavelengths greater than the centroid wavelength. In some production examples, the centroid wavelengths for a plurality of boards each having a number of LEDs, e.g., eight LEDs, will differ by 1 nm or more. Where the boards are populated with LEDs carefully selected for their close to matching spectral power distribution or with LEDs from a small bin, the centroid wavelengths will differ by 0.5 nm or more. Of course, costs increase significantly by producing boards with a closely matched centroid wavelengths.
The LED module 100 can accommodate LEDs with a wide spectral power distribution while still achieving a target color point within a predetermined tolerance. Moreover, multiple LED modules 100 may be produced, each with one or more LEDs having different spectral power distributions, e.g., a deviation in centroid wavelengths of 0.5 nm to 1.0 nm or more, while still achieving closely matched color points from one LED module 100 to the next and, where the matching color points of the LED modules 100. Moreover, the color points from the LED modules 100 may also be within a predetermined tolerance from a target color point. Thus, less expensive LEDs may be used. By using the two or more selectable wavelength converting components of the light mixing chamber 101, the color point of the light emitted by the LED module 100 may be accurately controlled. For example, during assembly of the LED module 100, the two or more wavelength converting components may be selected based on their wavelength converting characteristics and the spectral power distribution of the light produced by the LEDs 114 so that the resulting light that is transmitted through the window 130 has a color point that is within a predetermined tolerance of a predetermined target color point. The wavelength converting components of the LED module 100 may be selected to produce a desired degree of departure Δu′v′ of between 0.009 and 0.0035 and smaller if desired, such as 0.002. For example, LED modules 100 having light sources with centroid wavelengths that differ by more than 1.0 nm may be produced using selected wavelength converting components to produce a degree of departure of Δu′v′ of 0.007 or less, such as 0.0035. Where LED modules 100 have light sources with centroid wavelengths that differ by more than 0.5 nm, the wavelength converting components may be selected to produce a degree of departure of Δu′v′ of 0.0035 or less.
The CIE 1960 UCS color space has generally been superseded by the CIE 1976 UCS as an expression of uniform chromaticity space. However, the CIE 1960 UCS color space is still useful as an expression of chromaticity because the isothermal lines of correlated color temperature (CCT) are lines aligned perpendicular to the Planckian locus. Producing a target color point is desirable for light sources in general. For example, when used for purposes of general illumination, it is desirable that the LED module 100 produce white light with a particular correlated color temperature (CCT). CCT relates to the temperature of a black-body radiator and temperatures between 2700K and 6000K are typically useful for general illumination purposes. Higher color temperatures are considered “cool” as they are bluish in color, while lower temperatures are considered “warm” as they contain more yellow-red colors. By way of example, CCTs of 2700K, 3000K, 3500K, 4000K, 4200K, 5000K, 6500K on the black body curve or a CCT in illuminant series D are often desirable. In the context of the CIE 1960 UCS diagram, the degree of departure is the distance between the color point of the light produced by the light source and the Planckian locus along a line of constant CCT. In the context of the CIE 1960 UCS diagram, the degree of departure is referred to in units of Δuv. Thus, the color point of a white light source may be described as a CCT value and a Δuv value, i.e., the degree of departure from the black-body curve as measured in the CIE 1960 color space. It follows that the specification for color of light output by LED module 100 can be expressed as a CCT value within a predetermined tolerance and a Δuv value within a predetermined tolerance.
The wavelength converting characteristics of the plurality of the wavelength converting components are measured (306 and 308). The wavelength converting components are placed on a test fixture, which includes a light source, e.g., a board 112 with LEDs 114, that produces light with a known spectral power distribution and color point. The wavelength converting components are separately placed on the test fixture and the color point shift is measured using, e.g., a spectrometer and an integrating sphere. If desired, an intensity measurement using a dichroic filter can be done as well as or instead of the integrating sphere measurement, or a colorimeter such as produced by Konica-Minolta (CL-200 colorimeter) can be used. The measured wavelength converting characteristics for each component is stored. A self referencing measurement may be used for the wavelength converting characteristics of the components. For example, color point produced by the full spectral power distribution of the LEDs 114 and the measured component may be compared to the color point produced by the spectral power distribution that excludes the wavelength converted light to produce a self referencing Δuv value.
The color point shift of the wavelength converting components is illustrated in the CIE 1976 diagram of
The color point produced by, e.g., the wavelength converting material on or within the window 130, is illustrated as point 230 which corresponds with a dominant wavelength of, e.g., 570 nm. The color point shift produced by a window 130 with the test light source is along the dotted line 232 depending on the thickness and/or concentration of the wavelength converting material 132 on the window 130. By way of example, the measured color point produced by one of the windows 130 with the test light source is illustrated by point 234 and the shift Δnu′v′ from the color point produced by the test light source without the window 130 (e.g., point 210) is illustrated by line 236. If desired, different formulations of the wavelength converting materials on a wavelength converting component may also be used, which would alter the color point produced by the wavelength converting materials (as illustrated by arrow 240), and thus, the slope of the color point shift.
Typically, there is a difference in spectral power distribution from one LED to the next. For example, LEDs that are supposed to produce blue light at 452 nm will typically produce light that may range between 450 nm and 455 nm or more. In another example, LEDs that are supposed to produce blue light may produce light that ranges between 440 nm and 475 nm. In this example, the spectral power distribution from one LED to another may be as much as 8%. Accordingly, during the assembly process, the spectral power distribution and/or color point of the LEDs 114 in the base 110 may be measured for each LED module 100 (310 in
The diagram illustrates two color lines centered on the 3000K CCT for reference purposes. One color line 402 corresponds to the color point shift produced by a first wavelength converting material. In the present example, color line 402 is a yellow phosphor coating on the window 130. Color line 404 corresponds to the color point shift produced by a second wavelength converting material. In the present example, color line 404 is a red phosphor coating on the sidewall insert 126. Color line 402 indicates the direction of a shift in color point of light produced by the yellow phosphor. Color line 404 indicates the direction of shift in color point produced by the red phosphor. The first wavelength converting material and the second wavelength converting material are selected such that their respective directions of shift in color point are not parallel. Because the direction of shift of the yellow phosphor and the red phosphor are not parallel, the direction of the color point shift of light emitted by LED module 100 can be arbitrarily designated. This may be achieved by selecting the proper thickness and/or concentration of each phosphor as discussed above. By way of example, the small spots, 412, 414, 416, and 418 graphically illustrate the color points produced by one LED module 100 using different wavelength converting components. For example, spot 412 illustrates the color point for the LED module 100 with one set of wavelength converting components. By selecting a different window 130, the color point shifted for the LED module 100 to spot 414. As can be seen, the difference in the color points from spot 412 to 414 is parallel with the color line 402. A different sidewall insert 126 is then selected to produce a color point illustrated by spot 416. The difference in the color points from spot 414 to 416 is parallel with the color line 404. While this is within the 3000K target, an attempt to improve the color point by replacing the window 130 resulted in a color point illustrated by spot 418, where the shift between spot 416 and 418 is parallel with the color line 402. By again replacing the window 130 a color point of the LED module 100 shifted along line 402 to produce a color point illustrated by large spot 420, which is well within the predetermined tolerance from the target color point of 3000K on the black-body curve.
The above example illustrates a trial and error approach to selecting the appropriate wavelength converting components for a particular set of LEDs 114 to produce an LED module 100 with a desired color point. With a trial and error approach, it is unnecessary to measure the spectral power distribution of the light produced by the LEDs 114 before selecting the wavelength converting components. For example, a set of wavelength converting components may be selected and combined with the LEDs 114 and the resulting color point measured. Adjustments of the wavelength converting components may then be made based on the measured color point. However, in large scale production, it would be desirable to eliminate the trial and error approach. To eliminate the trial and error approach, the spectral power distribution and/or color point of the LEDs 114 would be measured and the wavelength converting components may then be appropriately selected to produce the target color point within a predetermined tolerance. The selection may be made based on, e.g., a database generated from previous trials or based on mathematical calculations. It may be desirable to measure the light output after the LEDs 114 are combined with the selected wavelength converting components to ensure the light is within the predetermined tolerance of the target color point, where one or both wavelength converting components may be changed if the light output is out of tolerance. For this purpose it is beneficial to label each module with a unique serial number, for example in the form of a barcode which can easily be scanned in the production process. It is beneficial to store in the database the spectral power densities of the board, and the final assembly, together with the types of wavelength converting components used. This data is then used by an algorithm to suggest the wavelength components to be used to achieve the desired performance of the modules.
With the two or more wavelength converting components selected, the LED module 100 can then be assembled (314). As discussed above, the assembly may include permanently attaching the base 110 with the reflective plate 113, the top section 120 with sidewall insert 126 and the window 130, e.g., with bolts, screws, clamps, epoxy, silicon, or other appropriate attachment mechanisms. By repeating this process multiple times, a plurality of LED modules 100 may be produced with nearly identical color points, e.g., each LED module 100 may produce a color point that differs from another by a predetermined tolerance, e.g., a Δuv of less than 0.001.
Thus, the LED module 100 includes a means for converting the spectral power distribution of the light emitting diodes to produce light from the light mixing chamber 101 with a color point within a degree of departure Δu′v′ of 0.009 or smaller from a target color point in a CIE 1976 u′v′ diagram. The means for converting the spectral power distribution includes a first means for converting the light produced by the light emitting diodes to produce a color point shift of a first magnitude along a first direction in the CIE 1976 u′v′ diagram and a second means for converting the light produced by the light emitting diodes to produce a color point shift of a second magnitude along a second direction in the CIE 1976 u′v′ diagram as illustrated in
Additionally, if desired, different wavelength LEDs 114 may be used in an LED module to improve the color rendering index (CRI). When all the LEDs 114 in the LED module 100 have substantially the same peak wavelengths, e.g., all the LEDs 114 are from the same bin having a bin size of 5 nm (for example a bin that includes 450 nm to 455 nm), a CRI value between, e.g., 75-85 may be achieved for an LED module 100 with CCTs of 2700K, 3000K, and 4000K, when a yellow (YAG) phosphor is used on the window 130 and red phosphor with a peak wavelength of 630 nm is used on the sidewall insert 126. However, by replacing one or more of the LEDs 114 with LEDs from a different bin so that the peak wavelength differs from the peak wavelength of LEDs 114 by 10 nm or more, a higher CRI may be achieved.
Additionally, phosphors may be used to produce high CRI values. A number of these phosphors are typically not used with LEDs due to the sensitivity of their respective emission properties to heat. However, the phosphors on the wavelength converting components, particularly the window 130 and the sidewall insert 126, are physically distant from the heat producing LEDs 114. In addition, the top section 120 of the LED module 100 is thermally coupled to the wavelength converting components and acts as a heat sink. Thus, the phosphors can be maintained at a relatively low temperature. For example, phosphors deposited directly on an LED source may reach temperatures in excess of 150 degrees centigrade, whereas the phosphors deposited on window 130 and sidewall insert 126 typically reach temperatures of approximately 70 to 90 degrees centigrade. As a result of the use of thermally sensitive phosphors LED module 100 may be tailored to produce a desired CRI value. For example, phosphors such as La3Si6N11:Ce,LaSi3N5,(Sr,Ca)AlSiN3:Eu,CaAlSiN3:Eu2+, (Sr,Ca)AlSiN3:Eu2+,Ca3(Sc,Mg)2,Si3O12:Ce,Sr0.8Ca0.2AlSiN3:Eu,CaSc2O4:Ce,(Sr,Ba)2SiO4:Eu2+, SrGa2S4:Eu2+,SrSi2N2O2:Eu2+,Ca3Sc2Si3O12:Ce3+, Y3−xAl2Al3O12:Cex+ and Lu3−xAl2Al3A12:Cex+, can be used on wavelength converting components to produce CRI values of 80 and higher, or even 95 and higher.
Although the present invention is illustrated in connection with specific embodiments for instructional purposes, the present invention is not limited thereto. It should be understood that the embodiments described herein may use any desired wavelength converting materials, including dyes, and are not limited to the use of phosphors. Various adaptations and modifications may be made without departing from the scope of the invention. Therefore, the spirit and scope of the appended claims should not be limited to the foregoing description.
This application is a continuation of U.S. application Ser. No. 13/956,007, filed Jul. 31, 2013, which, in turn, is a continuation of U.S. application Ser. No. 13/744,274, filed Jan. 17, 2013, now U.S. Pat. No. 8,500,297, issued Aug. 6, 2013, which, in turn, is a divisional of U.S. application Ser. No. 13/534,661, filed Jun. 27, 2012, now U.S. Pat. No. 8,382,335, issued Feb. 26, 2013, which, in turn, is a divisional of U.S. application Ser. No. 12/617,668, filed Nov. 12, 2009, now U.S. Pat. No. 8,220,971, issued Jul. 17, 2012, which, in turn, claims the benefit of U.S. Provisional Application No. 61/117,060, filed Nov. 21, 2008, all of which are incorporated by reference herein in their entireties.
Number | Name | Date | Kind |
---|---|---|---|
3593055 | Geusic et al. | Jul 1971 | A |
5959316 | Lowery | Sep 1999 | A |
5962971 | Chen | Oct 1999 | A |
5966393 | Hide et al. | Oct 1999 | A |
5982092 | Chen | Nov 1999 | A |
5998925 | Shimizu et al. | Dec 1999 | A |
6066861 | Hohn et al. | May 2000 | A |
6068383 | Robertson et al. | May 2000 | A |
6220725 | Arnold | Apr 2001 | B1 |
6234648 | Borner et al. | May 2001 | B1 |
6340824 | Komoto et al. | Jan 2002 | B1 |
6351069 | Lowery et al. | Feb 2002 | B1 |
6357889 | Duggal et al. | Mar 2002 | B1 |
6469322 | Srivastava et al. | Oct 2002 | B1 |
6504301 | Lowery | Jan 2003 | B1 |
6576930 | Reeh et al. | Jun 2003 | B2 |
6577073 | Shimizu et al. | Jun 2003 | B2 |
6586882 | Harbers | Jul 2003 | B1 |
6600175 | Baretz et al. | Jul 2003 | B1 |
6621211 | Srivastava et al. | Sep 2003 | B1 |
6649946 | Bogner et al. | Nov 2003 | B2 |
6680569 | Mueller-Mach et al. | Jan 2004 | B2 |
6724142 | Ellens et al. | Apr 2004 | B2 |
6765237 | Doxsee et al. | Jul 2004 | B1 |
6791259 | Stokes et al. | Sep 2004 | B1 |
6809342 | Harada | Oct 2004 | B2 |
6812500 | Reeh et al. | Nov 2004 | B2 |
6850002 | Danielson et al. | Feb 2005 | B2 |
7005679 | Tarsa et al. | Feb 2006 | B2 |
7083302 | Chen et al. | Aug 2006 | B2 |
7126162 | Reeh et al. | Oct 2006 | B2 |
7250715 | Mueller et al. | Jul 2007 | B2 |
7331697 | Hulse | Feb 2008 | B1 |
7344952 | Chandra | Mar 2008 | B2 |
7404652 | Ng et al. | Jul 2008 | B2 |
7479662 | Soules et al. | Jan 2009 | B2 |
7494246 | Harbers | Feb 2009 | B2 |
7534002 | Yamaguchi et al. | May 2009 | B2 |
7564180 | Brandes | Jul 2009 | B2 |
7614759 | Negley | Nov 2009 | B2 |
7629621 | Reeh et al. | Dec 2009 | B2 |
7682850 | Harbers et al. | Mar 2010 | B2 |
7768192 | Van De Ven et al. | Aug 2010 | B2 |
7942556 | Harbers et al. | May 2011 | B2 |
7984999 | Harbers et al. | Jul 2011 | B2 |
8035287 | Schmidt et al. | Oct 2011 | B2 |
8220971 | Harbers et al. | Jul 2012 | B2 |
8382335 | Harbers et al. | Feb 2013 | B2 |
8500297 | Harbers et al. | Aug 2013 | B2 |
8746922 | Harbers et al. | Jun 2014 | B2 |
8888329 | Harbers et al. | Nov 2014 | B2 |
20020043926 | Takahashi et al. | Apr 2002 | A1 |
20050057145 | Shieh et al. | Mar 2005 | A1 |
20060076882 | Chan et al. | Apr 2006 | A1 |
20060087487 | Ota | Apr 2006 | A1 |
20060125923 | Israel et al. | Jun 2006 | A1 |
20060152140 | Brandes | Jul 2006 | A1 |
20070081336 | Bierhuizen et al. | Apr 2007 | A1 |
20070115665 | Mueller et al. | May 2007 | A1 |
20070147032 | Furukawa et al. | Jun 2007 | A1 |
20070215890 | Harbers et al. | Sep 2007 | A1 |
20070223219 | Medendorp, Jr. et al. | Sep 2007 | A1 |
20070263393 | Van De Ven | Nov 2007 | A1 |
20080128735 | Yoo et al. | Jun 2008 | A1 |
20080142816 | Bierhuizen et al. | Jun 2008 | A1 |
20080169480 | Weng et al. | Jul 2008 | A1 |
20080211751 | Kim | Sep 2008 | A1 |
20080310152 | Verbrugh et al. | Dec 2008 | A1 |
20080310158 | Harbers et al. | Dec 2008 | A1 |
20090008655 | Peeters et al. | Jan 2009 | A1 |
20090086475 | Caruso et al. | Apr 2009 | A1 |
20090103293 | Harbers et al. | Apr 2009 | A1 |
20100067214 | Hoelen et al. | Mar 2010 | A1 |
20100127282 | Harbers et al. | May 2010 | A1 |
20100327306 | Van Der Burgt et al. | Dec 2010 | A1 |
20110026257 | Holten et al. | Feb 2011 | A1 |
20120051045 | Harbers et al. | Mar 2012 | A1 |
20120224177 | Harbers et al. | Sep 2012 | A1 |
20120267653 | Harbers et al. | Oct 2012 | A1 |
Number | Date | Country |
---|---|---|
0 890 996 | Jan 1999 | EP |
1 548 851 | Jun 2005 | EP |
1 780 592 | May 2007 | EP |
2 117 055 | Nov 2009 | EP |
1 081 771 | Jun 2011 | EP |
2005-093896 | Apr 2005 | JP |
2006-032726 | Feb 2006 | JP |
2008-159707 | Jul 2008 | JP |
I283078 | Jun 2007 | TW |
I296448 | May 2008 | TW |
WO 2007002234 | Jan 2007 | WO |
WO 2007130536 | Nov 2007 | WO |
WO 2008047290 | Apr 2008 | WO |
WO 2008126038 | Oct 2008 | WO |
WO 2008142638 | Nov 2008 | WO |
WO 2008149250 | Dec 2008 | WO |
WO 2008157080 | Dec 2008 | WO |
WO 2008157080 | Dec 2008 | WO |
WO 2009052099 | Apr 2009 | WO |
WO 2009052099 | Apr 2009 | WO |
WO 2009093163 | Jul 2009 | WO |
Entry |
---|
International Search Report mailed on Feb. 23, 2010 for PCT Application No. PCT/US2009/064492 filed on Nov. 14, 2009, 16 pages. |
International Preliminary Report on Patentability mailed on May 24, 2011 for PCT Application No. PCT/US2009/064492 filed on Nov. 14, 2009, 9 pages. |
International Search Report mailed on Dec. 15, 2011 for PCT Application No. PCT/US2011/049017 filed on Aug. 24, 2011 by Xicato, Inc., 11 pages. |
English Abstract of JP2008159707 (A) published on Jul. 10, 2008 visited at <http://worldwide.espacenet.com> on Sep. 18, 2012, 2 pages. |
English Abstract of JP2005093896 (A) published on Apr. 7, 2005 visited at <http://worldwide.espacenet.com> on Sep. 18, 2012, 2 pages. |
English Abstract of TWI296448 (B) published on May 1, 2008 visited at <http://worldwide.espacenet.com> on Sep. 18, 2012, 2 pages. |
English Abstract of TWI283078 (B) published on Jun. 21, 2007 visited at <http://worldwide.espacenet.com> on Sep. 18, 2012, 2 pages. |
Harbers et al. (Jun. 2007). “Performance of High Power Light Emitting Diodes in Display Illumination Applications,” Journal of Display Technology vol. 3, No. 2, pp. 98-109. |
Hoelen et al. (Sep. 12, 2008). “Remote Phosphor LED Modules for General Illumination Towards 200 1m/W General Lighting LED Light Sources,” SPIE vol. 7058, pp. 1-10. |
Notice of Allowance mailed on Sep. 6, 2013 for U.S. Appl. No. 13/956,007, filed Jul. 31, 2013 by Xicato, Inc., 10 pages. |
Request for Continued Examination mailed on Dec. 6, 2013 for U.S. Appl. No. 13/956,007, filed Jul. 31, 2013 by Xicato, Inc., 12 pages. |
Office Action mailed on Feb. 4, 2014 for U.S. Appl. No. 13/956,007, filed Jul. 31, 2013 by Xicato, Inc., 12 pages. |
Response to Office Action mailed on Apr. 29, 2014 for U.S. Appl. No. 13/956,007, filed Jul. 31, 2013 by Xicato, Inc., 12 pages. |
Notice of Allowance by mailed on Jun. 6, 2014 for U.S. Appl. No. 13/956,007, filed Jul. 31, 2013 by Xicato, Inc., 11 pages. |
Machine translation in English of Abstract of JP 2006-032726-A visited at www.espacenet.com on Sep. 16, 2015, 2 pages. |
Number | Date | Country | |
---|---|---|---|
20150070888 A1 | Mar 2015 | US |
Number | Date | Country | |
---|---|---|---|
61117060 | Nov 2008 | US |
Number | Date | Country | |
---|---|---|---|
Parent | 13534661 | Jun 2012 | US |
Child | 13744274 | US | |
Parent | 12617668 | Nov 2009 | US |
Child | 13534661 | US |
Number | Date | Country | |
---|---|---|---|
Parent | 13956007 | Jul 2013 | US |
Child | 14542413 | US | |
Parent | 13744274 | Jan 2013 | US |
Child | 13956007 | US |