Dual titanium nitride layers for solar control

Information

  • Patent Grant
  • 6188512
  • Patent Number
    6,188,512
  • Date Filed
    Monday, November 2, 1998
    26 years ago
  • Date Issued
    Tuesday, February 13, 2001
    23 years ago
Abstract
A solar control member utilizes a combination of layers that include spaced apart titanium nitride layers to selectively transmit a higher percentage of visible light than near infrared energy, with a low visible light reflection. The titanium nitride layers are spaced apart by a distance that promotes optical decoupling with respect to occurrence of constructive and destructive interference of visible light propagating between the two titanium nitride layers. In one embodiment, the titanium nitride layers are spaced apart by a laminating adhesive layer. In another embodiment, the titanium nitride layers are formed on opposite sides of a substrate. The ratio of transmission at the wavelength of 550 nm to transmission at the wavelength of 1500 is at least 1.25. Each titanium nitride layer is sputter deposited. Care is taken to ensure that each layer does not become too metallic and to ensure that excessive oxygen is not incorporated into the layer. Thus, the nitrogen flow rate and the linespeed are controlled. Sputtering occurs at a fast rate using high powers and a minimum acceptable nitrogen flow, while minimizing background contamination.
Description




TECHNICAL FIELD




The invention relates generally to solar control members for coating windows and the like, and relates more specifically to applied window film members which provide solar rejection and low visible reflection.




BACKGROUND ART




Various films have been applied to windows to reduce glare and to obtain solar screening for an interior of a structure, such as a home, building or car. For example, a plastic film may be dyed to provide desired optical properties or may be coated with a number of layers to acquire the optical properties. A film that provides solar screening is one that has a low transmission in both the visible range (400 to 700 nm) and the near infrared range (700 to 2100 nm). To reduce glare, the transmission of visible light (T


VIS


) must be controlled.




Primarily through absorption, dyed films can be fabricated to provide a wide range of T


VIS


values. However, dyed films generally do not block near infrared solar energy and, consequently, are not completely effective as solar control films. Another shortcoming of dyed films is that they often fade with solar exposure. When the films are colored with multiple dyes, the dyes often fade at different rates, causing unwanted color changes over the life of the film.




Other known window films are fabricated using vacuum-deposited grey metals, such as stainless steel, inconel, monel, chrome or nichrome alloys. The deposited grey metal films offer about the same degrees of transmission in the visible and near infrared portions of the solar spectrum. As a result, the grey metal films are an improvement over dyed films with regard to solar control. The grey metal films are relatively stable when exposed to light, oxygen and moisture, and in those cases in which the transmission of the coatings increases due to oxidation, color changes are generally not detectable. After application to clear float glass, grey metals block light transmission by approximately equal amounts of solar reflection and solar absorption.




Vacuum-deposited layers such as silver, aluminum and copper control solar radiation primarily by reflection. Because of the high reflection in the visible spectrum (i.e., high R


VIS


), films having these vacuum-deposited layers are useful in only a limited number of applications. A modest degree of selectivity of transmission in the visible spectrum over transmission in the near infrared spectrum is afforded by certain reflective materials, such as copper and silver.




Traditionally, the best glare reducing coatings have been sputtered grey metals, such as stainless steel, chrome and nickel. The graph of

FIG. 1

is a transmission spectrum


10


for a sputtered nichrome coating that is designed to transmit approximately 50% of the light at the center of the visible light spectrum (i.e., T


VIS


=50%). The nichrome is affixed to a 3.2 mm-thick plate of float glass. As can be seen, the transmission of energy is controlled in both the visible and near infrared portions of the solar spectrum. A slight degree of wavelength selectivity is observed due to the iron oxide in the glass.




In the graph of

FIG. 2

, the visible reflectivities of single and double layer nichrome films of various thicknesses are shown as a function of the corresponding visible light transmissions. (Here, double nichrome films refer to a construct in which two optically isolated sputtered coatings are employed, with the films being separated from each other by a relatively thick (22 micrometers) layer, such as a laminating adhesive.) While not shown in

FIG. 2

, the nichrome layer thicknesses decrease from left to right. As can be seen, the R


VIS


value decreases and the T


VIS


value increases as the nichrome layers become thinner. The comparison between the single and double layer nichrome films evidences that the double layer of nichrome has a substantially reduced R


VIS


value for the same T


VIS


value. For example, at a T


VIS


value of 20%, the single nichrome coating has an R


VIS


value of 24%, while the double nichrome coating has an R


VIS


value of 13%. As the nichrome layers become thinner, the R


VIS


values of the two films converge.




The percentages of solar rejection achieved by films with single and double layers of nichrome are compared in the graph of FIG.


3


. Solar rejection is defined as:






solar rejection=solar reflection+(0.73×solar absorption).






Within the art, solar rejection is often calculated using solar energy distributions as given in the ASTM E 891 method. The slightly better solar rejection noted for the low transmission single nichrome coatings relative to the twin nichrome equivalents is due to solar reflection differences.




A low visible light transmission and low visible light reflection film utilizing double layers of nichrome is disclosed in U.S. Pat. No. 5,513,040 to Yang. The patent discloses a solar control film having two or more transparent substrates, each bearing a thin, transparent and discontinuous film of metal having low R


VIS


and a degree of visible light blocking capacity. The substrates are arranged and laminated into a composite, such that the visible light blocking capacities of the metal films are effectively combined to provide a composite having low visible light transmittance, i.e., a low T


VIS


. The discontinuous films of nichrome are attached using an adhesive layer.




The possibility of using metal nitride films in window-energy applications was discussed by C. Ribbing and A. Roos in an article entitled, “Transition Metal Nitride Films for Optical Applications,” which was presented at SPIE's International Symposium on Optical Science, Engineering and Instrumentation, San Diego, July/August 1997. Single layers of TiN, ZrN and HfN were specifically identified. The article discusses the use of the materials in low emissivity coatings to replace noble metals, such as silver and gold. It is noted that the low emissivity coatings will not reach as high a selectivity as the current noble metal-based multi-layers, but may find use in aggressive environments, because of their excellent stability.




What is needed is a solar control member for application to a window or the like in order to achieve a high selectivity of visible transmission to near infrared transmission, with a controlled visible reflection and with age stability. What is further needed is a repeatable method of fabricating such a solar control member.




SUMMARY OF THE INVENTION




A solar control member utilizes a combination of layers that include spaced apart titanium nitride layers in order to achieve a desired combination of optical characteristics, including characteristics relating to visible transmission (T


VIS


), near infrared transmission (T


NIR


) and visible reflection (R


VIS


). Adjacent titanium nitride layers are spaced apart by a distance that promotes optical decoupling with respect to constructive and destructive interference of visible light propagating between the two titanium nitride layers. In the preferred embodiment, each titanium nitride layer is formed on a separate substrate, such as a PET substrate, with first and second titanium nitride layers then being joined by a laminating adhesive having a thickness greater than the wavelengths associated with visible light (i.e., greater than 700 nm). It is recommended that the distance between the titanium nitride layers be at least 1000 nm, with 3000 nm being more preferred. In another embodiment, the first and second titanium nitride layers are formed on opposite sides of a substrate, such as PET, so that the substrate provides the recommended spacing between the two layers.




The thickness of each titanium nitride layer depends upon the desired optical properties. Preferably, the titanium nitride layers are sputter deposited in a manner that facilitates reproducibility, but allows an adaptation for varying the T


VIS


value within a range of 20 to 70% and more preferably within the range of 30 to 60%. The T


VIS


value is achieved while the R


VIS


value remains below 20%. Moreover, the ratio of transmission at the wavelength of 550 nm (T


550


) to transmission at the wavelength of 1500 nm (T


1500


) is at least 1.25. That is, the selectivity as defined by T


550


/T


1500


exceeds 1.25.




In most applications, two sputtered titanium nitride layers are sufficient. Individual T


VIS


values for the films should be within the range of 45 to 70%, so that the dual film laminate structure has an R


VIS


close to 10%. However, to obtain a composite visible transmission of less than 40% while maintaining the individual film visible transmissions within the range of 45 to 70%, a third sputtered titanium nitride layer may be necessary. More than three sputtered layers may be required to obtain a composite visible transmission of 20%.




Greater wavelength selectivity is obtained if the titanium nitride layers are combined with transparent oxides (e.g., oxides of tin, indium, zinc, titanium, niobium, bismuth, zirconium, or hafnium) or nitrides (e.g., silicon or aluminum nitride) having a refractive index at least as great as that of the substrate material (the refractive index of PET is 1.7). The transparent oxides or nitrides can be placed on one or both sides of the titanium nitride. The thickness would range between 10 and 60 nm, depending upon color, reflectivity, or cost requirements. A transparent nitride, such as silicon nitride, is preferred over an oxide, since during the deposition process “crosstalk” between the titanium and silicon processes is less likely to introduce excessive oxygen into the titanium nitride layer.




In all practical vacuum web coaters, some incorporation of oxygen will occur, so that in practice what is deposited is actually titanium oxynitride. However, if excessive oxygen is incorporated into the titanium nitride coating, the wavelength selectivity and electrical conductivity will be lost. It is believed that the oxygen-to-nitrogen partial pressure ratio during the sputtering process should be less than 0.5. To ensure that wavelength selectivity and electrical conductivity are achieved, the stoichiometry of each titanium nitride layer must be controlled. Two of the concerns with regard to adversely affecting the titanium nitride performance are (1) ensuring that each layer does not become too metallic and (2) ensuring that excessive oxygen is not incorporated into the layers. In either case, the wavelength selectivity will be lost if the sputtering process is not properly performed. A titanium nitride layer will become too metallic if it is nitrogen depleted, as will occur if nitrogen flow during the process is inadequate. The exact nitrogen flow to achieve a suitable titanium nitride layer varies from coater to coater. However, the most preferred flow generally corresponds to minima in sheet resistance and absorption at 1500 nm. As the nitrogen flow is being adjusted, if a T


1500


value is to be maintained with an increase in nitrogen flow, the linespeed of the deposition process should be reduced. This is largely due to a decrease in the deposition rate of the titanium nitride.




Regarding excessive oxygen, the extra oxygen typically comes from background water and oxygen contaminants present in the sputtering system. The problem is enhanced if other oxygen-requiring processes (e.g., plasma pretreatments or reactive sputtering) are conducted in the vacuum chamber while the titanium nitride deposition process is being conducted. To reduce the likelihood that contamination will occur, the following steps may be taken (1) sputter as fast as possible using high powers and the minimum acceptable nitrogen flow, since excessive nitrogen “poisons” the titanium target and reduces the deposition rate; (2) minimize background contamination by controlling “crosstalk” between neighboring processes, by minimizing the water content in the substrate (for example by preheating or separate outgassing steps), by eliminating any water leaks in the vacuum chamber, and by adequately pumping down the vacuum system prior to beginning the deposition; and (3) sputter through a mask, so that the outer perimeter of the titanium nitride plasma (which deposits on a mask, rather than the substrate) acts as an “oxygen getter.”




Optionally, the surface that is exposed when the solar control member is attached to a window is protected by a hardcoat layer. Hardcoat layers are known to provide resistance against abrasion. Another optional layer is a low surface energy layer on the hardcoat. The low surface energy layer acts as an antisoiling layer for resisting smudges and the like and as a lubrication layer for improving the resistance to mechanical abrasion.











BRIEF DESCRIPTION OF THE DRAWINGS





FIG. 1

is a graph of a transmission spectrum for a single layer nichrome film that is designed to transmit approximately 50% of the light at the center of the visible light spectrum.





FIG. 2

is a graph of visible reflection versus visible light trans- mission as a function of film thickness for a single layer nichrome film and a double layer nichrome film on 3.2 mm glass.





FIG. 3

is a graph of the percentage of solar rejection versus visible light transmission as a function of film thickness of a single layer nichrome film and a double layer nichrome film on 3.2 mm glass.





FIG. 4

is a side sectional view of a portion of a solar control member in accordance with the invention.





FIG. 5

is a side sectional view of the solar control member of 15

FIG. 4

shown in a window energy application.





FIG. 6

is a side sectional view of another embodiment of a window energy application in accordance with the invention.





FIG. 7

is a side sectional view of a third embodiment of a solar control member in accordance with the invention.





FIGS. 8-11

are plots of values from Table 1 that is to follow.





FIG. 12

is a comparison of performances of three laminates having single and double layer titanium nitride film and a double layer nichrome film.











BEST MODE FOR CARRYING OUT THE INVENTION




With reference to

FIG. 4

, a solar control member


11


is shown as including first and second substrates


12


and


14


, with each substrate having a layer of titanium nitride


16


and


18


, respectively. The titanium nitride layers are bonded together using a laminating adhesive layer


20


.




Preferably, the substrates


12


and


14


are flexible members that allow the titanium nitride layers


16


and


18


to be sputter deposited using web processing techniques. The substrates may be PET films, but other materials may be substituted. The substrates must be substantially transparent, since the objectives in forming the solar control member


11


include providing an R


VIS


value in the range of 5 to 20%, a T


VIS


value in the range of 20 to 70% (and more preferably within the range of 30 to 60%), and an NIR transmission (i.e., from 700 to 2100 nm) that is lower than the T


VIS


value. With regard to the wavelength selectivity, the ratio of transmission at the wavelength of 550 nm to transmission at the wavelength of 1500 nm should be at least 1.25 (i.e., T


550


/T


1500


≧1.25).




A standard thickness of the substrates


12


and


14


is between 1 and 2 mils, but the thickness is not critical to the invention. The thicknesses of the titanium nitride layers


16


and


18


are selected based upon the desired optical properties of the solar control member


11


. A thicker titanium nitride layer will block a greater percentage of energy, but will also increase reflection and decrease transmission within the visible range. Preferably, the individual film transmissions are within the range of 45 to 70% at the visible range. This is the preferred range of individual film transmissions, even if more than two layers of titanium nitride are used. While the layers


16


and


18


are described as titanium nitride layers, in practice it is difficult to avoid some incorporation of oxygen into the layers, so that the titanium nitride layers are actually titanium oxynitride layers (TiN


x


O


y


). However, if the amount of oxygen in the layers becomes excessive, wavelength selectivity and electrical conductivity are lost. It is believed that the ratio of oxygen to nitrogen partial pressures during the sputtering process should be less than 0.5. Measurements of various TiN


x


samples indicate the highest wavelength selectivity is obtained when the oxygen content of TiN


x


O


y


coatings is less than 20 atomic percent or most preferably less than 10 atomic percent. The sheet resistance of each titanium nitride layer should be less than 500 ohms/square.




The laminating adhesive layer


20


is an optically massive layer. That is, the thickness of the adhesive layer should be such that the two titanium nitride layers


16


and


18


are sufficiently spaced apart to avoid constructive and destructive interference of visible light propagating between the two titanium nitride layers. To ensure that the spacing between the two layers is greater than the wavelengths associated with visible light, the adhesive layer should have a thickness of at least 700 nm. In a more preferred embodiment, the thickness is at least 1 micron (i.e., 1000 nm), with at least three microns being most preferred.




In another embodiment, the spacing between the two titanium nitride layers


16


and


18


is achieved by forming the two layers on opposite sides of a single substrate, such as a PET film. Thus, the laminating adhesive layer


20


would not be required. In other embodiments, the spacing between the two titanium nitride layers


16


and


18


may be provided by more than one layer. However, the layers should not adversely affect the above-identified optical objectives of the solar control member


11


. While not shown in

FIG. 4

, there is often a hardcoat layer on one PET surface opposite to the titanium nitride coated side. Hardcoat layers improve the durability of the flexible substrate during processing and particularly during use of the end product. The hardcoat layers can be any one of a variety of known hardcoat materials, such as silica-based hardcoats, siloxane hardcoats, melamine hardcoats, and acrylic hardcoats. An acceptable thickness range is 1 μm to 20 μm. The use of hardcoat layers is not critical to the invention.




Other optional layers include primer layers between the adhesive layer


20


or the substrate layers


12


and


14


and each of the titanium layers


16


and


18


. The primer layers may be used to improve adhesion between the titanium nitride layers and the adhesive or substrate. The primer layer may be a metal that undergoes oxidation or nitridation in situ during processing, so as to yield a substantially transparent, substantially colorless inorganic metal oxide. Examples of useful primer materials include silicon, titanium, chromium, nickel and alloys. The primer layer should be sufficiently thin to minimize disruption of the desired optical properties of the solar control member


11


. Preferably, the primer layer has a thickness of less than 30 angstroms.




The laminating adhesive layer


20


may be an adhesive such as Morton's Adcote 1130 adhesive. This and other such adhesives are well known in the industry. For fabricating prototype samples, MacTac transfer adhesive #IP2704 may be used.




Typically, the two substrates


12


and


14


will be from separate webs, since it is more practical. However, the substrates may be different portions from a single web. That is, following the web processing operation of depositing titanium nitride onto a continuous web of PET, the PET film is divided into sections that may be combined as shown in FIG.


4


. This is possible when the two titanium nitride layers


16


and


18


are to have the same thickness. However, in some applications, there may be advantages to having titanium layers of different thicknesses. In such applications, it is typically more economical to sputter the titanium nitride layers on different substrates.




Referring now to

FIG. 5

, the solar control member of

FIG. 4

is shown attached to float glass


22


by means of a second adhesive layer


24


. The float glass may be a windshield of a vehicle or may be a window of a home or building. The solar control member provides solar screening to the interior of the vehicle, home or building. It should be noted that the titanium nitride layers


16


and


18


are not specifically designed to provide low heat emissivity. Although titanium nitride layers are electrically conductive, and therefore have relatively low heat emissivity and relatively high heat reflection, in the construct of

FIG. 5

, the titanium nitride layers do not directly contact air and are “buried” within infrared opaque wet coatings and substrates. This renders them relatively ineffective at blocking long wave (IR) heat transfer. As noted above, PET films typically are provided with a hardcoat layer. Thus, the exposed surface of the substrate


14


will be protected by the hardcoat layer. As will be explained more fully with reference to

FIG. 6

, another optional layer is a low surface energy (anti smudge) layer that resists mechanical damage and soiling to the solar control member.




With reference to

FIG. 6

, a second embodiment of a solar control member is shown. For simplicity, reference numerals of

FIG. 5

are used for comparable elements of FIG.


6


. Thus, the solar control member is attached to float glass


22


by means of adhesive layer


24


. The solar control member includes first and second titanium nitride layers


16


and


18


that were previously sputter deposited onto substrates


12


and


14


and adhered to one another by means of a laminating adhesive layer


20


. The solar control member includes a third titanium nitride layer


26


on the side of the substrate


14


opposite to the second titanium nitride layer


18


. While not critical, the third titanium nitride layer may have a thickness identical to the thicknesses of the first and second titanium nitride layers. As previously noted, the individual film transmission should be within the range of 45 to 70% with respect to visible light. In many applications, a third titanium nitride layer is not necessary in order to achieve the target T


VIS


value for the composite solar control member. However, if the target T


VIS


value is in the range of 20 to 40%, the third layer may be required in order to keep the R


VIS


value within the targeted range (e.g., approximately 10%). In fact, there may be applications in which more than three sputtered titanium nitride layers are necessary.




The solar control member of

FIG. 6

is shown as including the hardcoat layer


28


described above. The hardcoat layer is an abrasion-resistant coating that enhances durability of the solar control member. An acceptable thickness is within the range of 1 μm to 20 μm.




An anti smudge layer


30


coats the hardcoat layer


28


. The anti smudge layer reduces the susceptibility of the solar control member to scratches and other damage caused by contact with the outermost surface of the member. A desirable anti smudge layer is achieved by providing an adhesion promotion lower film of silane material and an upper film of a fluorocarbon with a low surface energy and with anti friction properties that facilitate cleaning and provide scratch resistance. The low surface energy layer may be a fluorocarbon sold by 3M Company under the federally registered trademark FLUORAD. In a more preferred embodiment, the material is FLUORAD FC722, which is sold diluted in 2% solution of a fluorinated solvent. The silane that is used as the adhesion promotion film may be N-(2-aminoethyl)-3-propyltrimethoxysilane in isopropyl alcohol (2-propanol). However, other silanes may be used, and in fact a silane may not be required in some applications.




Referring now to

FIG. 7

, a third embodiment of a solar control member


32


includes first and second substrates


34


and


36


, first and second titanium nitride layers


38


and


40


, an adhesive layer


42


, and first and second silicon nitride layers


44


and


46


. The only significant difference between the embodiments of

FIGS. 4 and 7

is the inclusion of the silicon nitride layers


44


and


46


. Greater wavelength selectivity can be obtained if the titanium nitride layers are combined with transparent oxides or nitrides with a refractive index that exceeds the refractive index of the substrates


34


and


36


. Thus, if a PET film is used to form the substrates, the additional layers


44


and


46


should have a refractive index of 1.7 or greater. An acceptable transparent oxide is an oxide of tin, indium, zinc, titanium, niobium, bismuth, zirconium, or hafnium. Acceptable nitrides are silicon and aluminum nitride. However, the silicon nitride is preferred, since the nitride layers are likely to introduce excessive oxygen into the titanium nitride layers


38


and


40


. While each titanium nitride layer is shown as having only one adjacent silicon nitride layer, silicon nitride may be formed on both sides of each titanium nitride layer. The thickness of the silicon nitride layers should be within the range of 10 and 60 nm, depending upon color, reflectivity, or cost requirements. While greater wavelength selectivity is achieved by including the silicon nitride layers, the solar control member


32


of

FIG. 7

is less cost-effective than the member


11


of FIG.


4


.




DEPOSITION CONDITIONS FOR TiN


x






Each of the solar control members of

FIGS. 4-7

includes at least two layers of titanium nitride that cooperate to provide the desired wavelength selectivity with the low R


VIS


value. In particular, the transmission of visible wavelengths is significantly higher than the transmission of wavelengths in the near infrared. The ratio of T


550


to T


1500


should be at least 1.25. To ensure that the target selectivity is achieved, the stoichiometry of the titanium nitride must be controlled during the sputtering process. Two concerns regarding adversely affecting the titanium nitride performance are (1) ensuring that the titanium nitride does not become too metallic and (2) ensuring that excessive oxygen is not incorporated into the titanium nitride. If a titanium nitride layer becomes too metallic (i.e., nitrogen is depleted, as would happen if the nitrogen flow to the process were inadequate), wavelength selectivity will be less desirable. If excessive oxygen is incorporated into a titanium nitride layer (i.e., more than 10 to 20 percent), the selectivity will be adversely affected. Sources of extra oxygen are background water and oxygen contaminants present within the sputtering system. The difficulties are enhanced if other oxygen-requiring processes are conducted in the vacuum chamber while the titanium nitride deposition process is being conducted. For this reason, the silicon or aluminum nitride layers


44


and


46


of

FIG. 7

are preferred over the formation of oxide layers.




To minimize contamination from oxygen sources, several steps can be taken. The sputtering process for depositing the titanium nitride should be performed as quickly as possible using high powers and a minimal amount of nitrogen, while still retaining the desired stoichiometry. Excessive nitrogen “poisons” the titanium target and reduces the deposition rate. A second step is to minimize background contamination. This can be accomplished by controlling “crosstalk” between neighboring processes, by minimizing the water content in the substrates (e.g., by preheating or outgassing), by ensuring that there are no water leaks in the vacuum chamber, and by adequately pumping down the vacuum system prior to the start of the deposition process. As a third step, the sputtering may occur through a mask, so that the outer perimeter of the titanium nitride plasma deposits on the mask, rather than on the substrate. Thus, the mask acts as an “oxygen getter.”




A number of experiments were conducted in view of these concerns and corrective steps. Results are shown in Table 1. The legends are defined as follows:




“Linespeed”—Rate at which the film is moved through the coating zone of the system;




“N


2


flow”—Gas flow to the titanium source;




“R


SHEET


”—Sheet resistance of TiN


x


coated film measured in the vacuum coater (i.e., in situ);




“T1550”—Transmission of coated film at a wavelength of 1550 nm, measured in situ;




“T


max


”—The transmission at the wavelength in the range 400 to 700 nm at which a maxima is observed;




“T


max


/T


1550


”—A first wavelength selectivity ratio;




“R


1550


”—The reflectivity at 1550 nm;




“T


VIS


”—The integrated visible transmission weighted for wavelength variations in illuminant (i.e., C) intensity and eye sensitivity (assuming a standard 20 observer);




“T


VIS


/T


1550


”—A second wavelength selectivity ratio.












TABLE 1











OPTIMIZATION OF THE TIN


x


PROCESS






OPTICAL PARAMETERS ARE FOR FILMS ONLY


















Experiment




No. 1




No. 2




No. 3




No. 4




No. 5




No. 6




Units









Linespeed




7.90




10.15




13.27




15.76




18.05




20.0




mm/s






N


2


Flow




45.0




40.0




35.0




32.5




30.0




27.5




sccm






R


SHEET






103




86




75




75




80




115




Ω/□






T


1550






15.3




14.9




14.8




15.1




15.0




14.9




% at 1550 nm






T


max






38.9




40.4




42.4




43.4




42.5









%






T


max


/T


1550






2.54




2.71




2.86




2.87




2.83
















R


1550






50.6




52.4




53.6




53.7




53.3




49.6




%






T


VIS






37.6




38.5




39.4




39.5




37.4




26.7




%






T


VIS


/T


1550






2.46




2.58




2.66




2.62




2.49




1.79



















In these experiments, the titanium power was maintained at 5.7 kW and an argon flow was set at 110 sccms, as required to obtain a 3 milliTorr pressure. As the nitrogen flow was varied between 27.5 and 45 sccms, the linespeed was adjusted as required to maintain a T


1500


value of approximately 15%. The dimensions of the titanium target were 397.88 mm by 82.55 mm. As can be seen in Table 1, as the nitrogen flow varied, so did the spectral properties of the titanium nitride layers that were formed during the experiments.




In order to obtain a simple measure of the selectivity at various nitrogen flow rates, two factors were considered, (1) T


max


/T


1550


and (2) T


VIS


/T


1550


. T


max


is the maximum transmission at any wavelength in the visible spectrum and T


VIS


is the weighted visible light transmission. These two factors from Table 1 are shown as being plotted in FIG.


8


. Clearly, the preferred coatings were formed with a nitrogen flow rate of 32.5 to 35 sccms. However, acceptable values were achieved with a nitrogen flow rate within the range of 30 to 35 sccms. It is interesting, as shown in the plots of

FIGS. 9 and 10

, that these preferred flows correspond to the minima and sheet resistance and absorption at 1550 nm (because the transmission was held relatively constant at 1550 nm, a minimum absorption at that wavelength corresponds to a maximum reflection). The “poisoning” effect of nitrogen on the titanium deposition rate is shown in FIG.


11


. As the nitrogen flow increased, the linespeed had to be reduced substantially in order to maintain the same value of T


1500


. This is largely due to the decrease in the deposition rate of the titanium nitride as the nitrogen flow rate was increased.




Table 2 shows the details of the measured deposition parameters for forming seven samples of titanium nitride on a PET substrate. In each case, the titanium nitride layers were electrically conductive (i.e., less than 300 ohms per square). Of course, as the films were made thinner in order to achieve higher visible light transmission, the electrical resistance increased. In Table 2, the sheet resistivity was measured in the vacuum chamber immediately after the coating was deposited. These samples (as distinguished by the sample numbers given in Table 2) were used to fabricate various window laminate structures (as given in Tables 4 and 5) for performance comparisons.












TABLE 2











DETAILS OF DEPOSITION PARAMETERS FOR TiN


x


SAMPLES



















Measured




Units




82-2




83-1




83-2




83-3




83-4




84-1




84-2









Glow Current




Amps




100




100




100




100




100




50




50






Glow Voltage




Volts




1500




1500




1500




1500




1500




1500




1500






Glow O


2


Flow




sccm




13.3




13.6




14.1




14.0




13.9




11.5




11.5






Glow Pressure




microns




10




10




10




9




10




7




8






Titanium Power




kWatt




4.5




5.7




5.7




5.7




5.7




5.7




5.7






Titanium Volts




Volts




460




465




457




454




458




446




446






Titanium Current




Amps




9.8




12.26




12.4




12.5




12.4




12.76




12.78






Titanium Ar Flow




sccm




105.5




105.5




105.5




104




104




105




105






Titanium N


2


Flow




sccm




26.2




33.5




32.5




32.5




32.5




32.5




32.5






Titanium Pressure




microns




3.61




3.71




3.72




3.67




3.7




3.67




3.65






Linespeed




mm/sec




10.1




8.8




16.7




12.45




7.45




6.05




4.18






Resistance (in situ)




ohm/sq




185




109




278




194




123




68




43.5






T


VIS


(in situ)




%




55




47




63




60




47




36




26














Benefits of Using Double TiN


x


Layers




In order to determine whether window structures with double titanium nitride layers provided better results than those containing a single titanium nitride layer and/or double nichrome layers, a number of samples were fabricated, with the results being shown in Tables 3-5. The samples listed in Table 3 were dual TiN


x


laminates. The laminates listed in Table 4 had a single layer of titanium nitride. The laminates listed in Table 5 included dual layers of a nonselective metal alloy, nichrome. In each table, when a reflection measurement is listed, it is followed by (PET) or (GLASS). This refers to the side on which the laminated window structure reflection measurement was made.












TABLE 3











TiN


x


DATA SUMMARY






OPTICAL PROPERTIES FOR WINDOW FILM LAMINATES






CONTAINING TWO (I.E., DUAL) SPUTTERED TiN


x


FILMS
















Sample No.




82-2




83-1




83-2











Lamination Type




Dual




Dual




Dual







T


VIS


: in situ - film only




55




47




63







T


VIS


: film only




59.47




51.34




67.35







T


VIS






43.55




33.49




53.98







R


VIS


(Glass)




10.64




12.29




9.93







R


VIS (PET)






10.97




12.8




10.21







T


SOL






30.85




21.55




41.7







R


SOL


(Glass)




12.14




15.67




10.01







R


SOL


(PET)




13.74




18.76




11.1







Ta*




−3.32




−3.98




−2.73







Tb*




1.55




0.23




3.92







Ra* (Glass)




1.2




2.13




0.15







Rb* (Glass)




−0.35




1.9




−2.05







Ra* (PET)




1.64




2.88




0.6







Rb* (PET)




−0.23




2.47




−1.9







Sol Rej (Glass)




53.8




61.5




45.3























TABLE 4











TiN


x


DATA SUMMARY






OPTICAL PROPERTIES FOR WINDOW FILM LAMINATES






CONTAINING A SINGLE SPUTTERED TiN


x


COATED FILM















Sample No.




83-3




83-4




84-1




84-2









Lamination Type




Single




Single




Single




Single






T


VIS


: in situ - film only




57




47




36




26






T


VIS


: film only




61.25




51.1




39.51




28.82






T


VIS






62.74




54.9




42.88




33.41






R


VIS


(Glass)




10.04




10.8




14.81




19.38






R


VIS


(PET)




12.15




13.4




18.26




22.86






TSOL




50.41




41.42




29.79




21.79






R


SOL


(Glass)




10.7




13.5




20.28




26.54






R


SOL


(PET)




14.47




18.55




27.45




34.78






Ta*




−2.32




−2.8




−3.2




−3.43






Tb*




1.75




0.81




−2.34




−4.62






Ra* (Glass)




0.54




1.55




2.52




2.98






Rb* (Glass)




−1.04




0.94




6.78




11.05






Ra* (PET)




1.04




2.23




3.16




3.71






Rb* (PET)




−1.7




−0.46




5.58




9.27






Sol Rej (Glass)




39.1




46.4




56.7




64.3






















TABLE 5











NiCr DATA SUMMARY






OPTICAL PARAMETERS FOR WINDOW FILM LAMINATES






CONTAINING TWO (I.E., DUAL) SPUTTERED NiCr FILMS
















Sample No.




R1-Q1




R1-Q2




R1-Q3











Lamination Type




Dual




Dual




Dual







T


VIS


: film only




40.06




52.39




65.43







T


VIS






22.03




35.2




51.49







R


VIS


(Glass)




14.61




11.39




9.84







R


VIS


(PET)




15.35




11.51




9.8







T


SOL






18.18




30.25




46.75







R


SOL


(Glass)




13.98




10.59




8.87







R


SOL


(PET)




15.96




12.02




9.54







Ta*




−0.95




−1.14




−1.12







Tb*




−2.99




−0.97




1.4







Ra* (Glass)




−0.85




−0.48




−0.56







Rb* (Glass)




1.36




−0.18




−1.14







Ra* (PET)




−0.084




−0.015




−0.17







Rb* (PET)




1.9




0.43




−0.42







Sol Rej (Glass)




63.5




53.8




41.3















Within the single sputtered films of titanium nitride of Table 4, thicker titanium nitride layers were required in order to obtain lower transmissions. After lamination to glass, the resulting composites had visible transmissions ranging from approximately 33% to approximately 63%. The dual titanium nitride layers provided a visible transmission range of 33% to 54%. Regarding visible reflection from the glass side of applied window film laminates containing various single and double titanium nitride films, at lower transmissions (e.g., approximately 55%), significantly lower reflections are obtained if two separate sputtered titanium nitride layers are used instead of one thicker titanium nitride layer. The same trend applies with regard to reflection from the PET side.




One concern with using dual layers is that for a given visible transmission, the solar rejection might be significantly lower than that observed for coatings containing a single sputtered layer. Measurements of solar rejection are obtained using the following equation for monolithic glazing:






solar rejection=solar reflection+(0.73×solar absorption)






where






solar absorption=100%−solar reflection−solar transmission.






Here, integrated solar properties are determined using wavelength specific weighting factors as specified in ASTM E 891. From Tables 3-5 and

FIG. 12

, it can be seen that the solar rejection for single titanium nitride layers is only two or three percentage points greater than the double layers. This is a relatively small sacrifice in order to receive the benefit of the large decrease in visible reflection.





FIG. 12

also illustrates the benefits of the present invention over the prior art of dual nonselective metals. Clearly, for a given visible transmission the dual TiN


x


window construct provides significantly higher solar rejection than the dual nichrome constructs.




In Tables 3-5, transmitted and reflected a* b* colors (from both sides of the glass/film composite) are indicated. It is noted that +a* means red, −a* means green, while +b* means yellow and −b* means blue. The primary difference between the two structures is in Rb*. The single film structures become more yellowish (gold or brass-like) at lower transmissions when viewed from either side of the composite. The dual film structures remain more color neutral.



Claims
  • 1. A solar control member comprising:a substantially transparent substrate; a first titanium nitride layer having a fixed position relative to said substrate; and a second titanium nitride layer having a fixed position relative to said first titanium nitride layer and being on a same side of said substrate as said first titanium nitride layer, said first and second titanium nitride layers being spaced apart by a distance of at least 700 nm to provide optical decoupling with respect to constructive and destructive interference of visible light propagating therebetween; wherein said first and second titanium nitride layers cooperate to provide a higher transmission of visible light than near infrared light.
  • 2. The solar control member of claim 1 further comprising a second substrate, said second titanium nitride layer being formed on said second substrate, said first titanium nitride layer being formed on said transparent substrate, said second substrate and said transparent substrate being on opposite sides of a combination of said first and second titanium nitride layers, said first titanium nitride layer being spaced apart from said second titanium nitride layer by an optically massive layer.
  • 3. The solar control member of claim 1 further comprising an optically massive layer which contacts each of said first and second titanium layers and has a thickness greater than 1000 nm, thereby providing said optical decoupling.
  • 4. The solar control member of claim 3 wherein said optically massive layer is a laminating adhesive having a thickness of at least 3000 nm.
  • 5. The solar control member of claim 2 wherein each of said transparent substrate and said second substrate is formed of a flexible transparent polymeric material.
  • 6. The solar control member of claim 1 wherein each of said first and second titanium nitride layers is a continuous layer, said distance between said first and second titanium nitride layers being at least 1000 nm.
  • 7. The solar control member of claim 1 further comprising a third titanium nitride layer spaced apart from each of said first and second titanium nitride layers by a distance that provides optical decoupling with respect to constructive and destructive interference of visible light.
  • 8. The solar control member of claim 1 wherein at least one surface of each of said first and second titanium nitride layers is coated with one of a transparent oxide and a transparent nitride such that said coating has a high selectivity ratio of visible light transmission to infrared light transmission.
  • 9. The solar control member of claim 1 further comprising a hardcoat layer and a low surface energy layer.
  • 10. The solar control member of claim 1 wherein said transparent substrate is fixed to a glass substrate.
  • 11. The solar control member of claim 1 wherein said titanium nitride layers contain less than 20 atomic percent of oxygen.
  • 12. The solar control member of claim 1 wherein said titanium nitride layers contain less than 10 atomic percent of oxygen.
  • 13. A solar control member comprising:a first transparent substrate; a first layer of titanium nitride on said first substrate; a second transparent substrate; a second layer of titanium nitride on said second substrate; and an optically massive bonding layer joining said first and second layers, thereby forming an assembly in which said first and second layers are sandwiched between said first and second substrates, said first and second layers being spaced apart by a distance that provides optical decoupling with respect to constructive and destructive interference of visible light propagating therebetween, said first and second layers being cooperative to provide a higher transmission of visible light than near infrared light.
  • 14. The solar control member of claim 13 wherein said bonding layer is an adhesive having a thickness greater than 700 nm.
  • 15. The solar control member of claim 14 further comprising a third layer of titanium nitride on a side of said second layer opposite to said first layer, said third layer being spaced apart from said second layer by a distance greater than 700 nm.
  • 16. The solar control member of claim 13 wherein said assembly has a ratio of transmission at 550 nm to transmission at 1550 nm is at least 1.25.
  • 17. The solar control member of claim 13 wherein each of said first and second layers is a sputtered layer having a sheet resistance of less than 500 ohms/square.
  • 18. A solar control member comprising:a substantially transparent substrate, said substrate being a flexible member having a first side for attachment to a transparent member through which solar protection is of interest; a first titanium nitride layer formed on said first side of said substrate; a second titanium nitride layer formed on a second side of said substrate, said first and second titanium nitride layers being spaced apart by a distance that provides optical decoupling with respect to constructive and destructive interference of visible light propagating therebetween; and a hardcoat layer and a low surface energy layer at said second side of said substrate and opposite to said second titanium nitride layer to provide protection for an exposed surface when said substrate is attached to said transparent member through which solar protection is of interest; wherein said first and second titanium nitride layers cooperate to provide a higher transmission of visible light than near infrared light.
US Referenced Citations (6)
Number Name Date Kind
4226910 Dahlen et al. Oct 1980
4799745 Meyer et al. Jan 1989
5091244 Biornard Feb 1992
5111329 Gajewski et al. May 1992
5216542 Szczyrbowski et al. Jun 1993
5513040 Yang Apr 1996