Microsphere-Based Coatings for Radioactive Cooling Under Direct Sunlight

Abstract

The present prevention provides a surface coating for cooling a surface by light scattering comprising a plurality of successive layers, each of the layers may be comprised of a plurality of spheres arranged to form a structure comprised of packed spheres. Each layer may have a different arrangement of packed spheres to create to a different light scattering property in each of the layers. The coating of the structures may also be formed by randomly packed spheres and the spheres may have a uniform diameter.

Claims

1-39. (cancelled)

40. A film for cooling a surface of a substrate by light scattering comprising: a plurality of layers in said film, each of said layers comprised of a plurality of spheres arranged to form a structure comprised of randomly packed spheres; and said spheres have a uniform diameter.

41. The film of claim 40 wherein said uniform diameter of said spheres is greater than 0.4 microns.

42. The film of claim 40 wherein said uniform diameter of said spheres is less than 3 microns.

43. The film of claim 40 wherein said uniform diameter of said spheres is 0.4-3 microns.

44. The film of claim 40 wherein said uniform diameter of said spheres is 1-3 microns.

45. The film of claim 44 wherein said spheres are hollow.

46. The film of claim 46 wherein said hollow spheres have a shell thickness of 1-100 nanometers.

47. The film of claim 46 wherein said hollow spheres have a shell thickness greater than 1 nanometer.

48. The film of claim 40 wherein said film has an average light emissivity of greater than 80% in a range of 8-13 microns.

49. The film of claim 46 wherein said film also has an average light emissivity of greater than 80% in a range of 18-30 microns.

50. The film of claim 40 wherein each of said layers has a different degree of randomness.

51. A film for cooling a surface of a substrate by light scattering comprising: a plurality of spheres arranged to form a structure comprised of randomly packed spheres; and said spheres have a uniform diameter.

52. The film of claim 51 wherein said uniform diameter of said spheres is greater than 0.4 microns.

53. The film of claim 51 wherein said uniform diameter of said spheres is less than 3 microns.

54. The film of claim 51 wherein said uniform diameter of said spheres is 0.4-3 microns.

55. The film of claim 51 wherein said uniform diameter of said spheres is 1-3 microns.

56. The film of claim 54 wherein said spheres are hollow.

57. The film of claim 56 wherein said hollow spheres have a shell thickness of 1-100 nanometers.

58. The film of claim 56 wherein said hollow spheres have a shell thickness greater than 1 nanometer.

59. The film of claim 51 wherein said film has an average light emissivity of greater than 80% in a range of 8-13 microns.

60. The film of claim 51 wherein said film also has an average light emissivity of greater than 80% in a range of 18-30 microns.

61. A film for cooling a surface of a substrate by light scattering comprising: a plurality of successive layers in said film; each of said layers comprised of a plurality randomly packed spheres; each structure of each layer has a different arrangement of said randomly packed spheres to create to a different light scattering property in each of said layers; said layers are comprised of lateral periodic structures and non-periodic structures; and said periodic layers are ordered structures and said non-periodic structures are random structures.

62. The film of claim 61 wherein each of said layers is made of a monolayer of microspheres with a predetermined degree of randomness.

63. The film of claim 61 wherein each of said layers has a sphere filling fraction of less than 55%.

64. The film of claim 61 wherein each of said layers has a sphere filling fraction between 20-45% and said spheres have a diameter between 0.4 and 1 micron.

65. The film of claim 61 wherein each of said layers has spheres joined into fibrillar networks and said fibrillar networks of each layer have different periodicities and orientations.

Description

BRIEF DESCRIPTION OF THE SEVERAL VIEWS OF THE DRAWINGS

[0032] In the drawings, which are not necessarily drawn to scale, like numerals may describe substantially similar components throughout the several views. Like numerals having different letter suffixes may represent different instances of substantially similar components. The drawings illustrate generally, by way of example, but not by way of limitation, a detailed description of certain embodiments discussed in the present document.

[0033] FIGS. 1A and 1B illustrate diffuse intensity distribution in the two tiers of randomly packed SiO.sub.2 spheres on Si (FIG. 1A) when the first and second tiers have l*=3 m and 30 m, respectively and (FIG. 1B) when the two tiers are interchanged. Light is incident on z=0 plane as shown in insets.

[0034] FIG. 2 illustrates intensity spectra of solar radiation and atmospheric radiation. Each is normalized to its maximum intensity.

[0035] FIG. 3 is a Mid-IR emissivity spectrum of solid silica film and silica microsphere packing of 55%. The thickness of both films is 100 m and normal direction of emission is considered.

[0036] FIG. 4 are SEM images and G parameter values (boxed numbers) in microns for various combinations of the pulling speed and the surface pressure for Langmuir-Blodgett (LB) assembled monolayers.

[0037] FIGS. 5A and 5B illustrate the optimal pulling speed and the optimal surface pressure for (FIG. 5A) a monolayer and (FIG. 5B) an additional layer assembly. The black square dots show the experimental points where the G value is the greatest and the lines are model predictions.

[0038] FIG. 6A is an SEM image of disordered microspheres.

[0039] FIG. 6B shows an autocorrelation function obtained from FIG. 6A.

[0040] FIG. 7A illustrates a complete assembly of spray-coating apparatus.

[0041] FIG. 7B is a top view of heated stage where the substrate can be placed on the metal platform.

[0042] FIG. 7C is a cross-sectional view of the heated, movable stage showing the linear motor.

[0043] FIG. 7D is an SEM image of microsphere coating with 1 stage cycle.

[0044] FIG. 7E is an SEM image of microsphere coating with 3 stage cycles.

[0045] FIG. 8 illustrates a fabrication process for creating fibrillar network structures by microsphere self-assembly.

[0046] FIG. 9 is an illustrates an SEM image of microspheres coated on c-Si grooves by LB technique.

[0047] FIGS. 10A shows a schematic illustration of order-disorder mixing in fibrillar network structures with separate ordered layers (bold circles) and disordered (circles) layers.

[0048] FIG. 10B shows intermediate mixing of layers.

[0049] FIG. 10C shows random mixing of the original ordered and disordered layers.

[0050] FIG. 11A illustrates a straight sphere chain depending on the groove width.

[0051] FIG. 11B illustrates a non-straight sphere chain depending on the groove width.

[0052] FIG. 12 illustrates calculated solar absorptivity of randomly packed SiO.sub.2 spheres on an absorbing material as a function of the sphere coating thickness at the interface reflectance of 0 and 0.96.

[0053] FIG. 13 illustrates cooling power as a function of the temperature of various materials when the ambient temperature is 27 C. The black body and the ideal emissivity refer to mid-IR spectrum only. The solar absorptivity of the materials is 0.034, the same value as the SiO.sub.2 coating.

[0054] FIGS. 14A and 14B illustrates absorptivity in semi-infinite Si substrate with a perfect antireflection coating due to diffuse light and to both diffuse and ballistic light when SiO2 microspheres are placed on top. (FIG. 14A) l*=3 m and (FIG. 14B) l*=200 m.

[0055] FIG. 15 is a comparison of experimental results and CPA prediction of l* for randomly packed SiO.sub.2 microspheres of a 0.9 m diameter. Predictions are given for two extreme values of filling fraction 0.55 and 0.64 for randomly packed single size spheres.

[0056] FIG. 16 illustrates l* spectra at various sphere diameters d when the filling fraction is 55%.

[0057] FIG. 17 is a CPA prediction of l* as a function of SiO.sub.2 microsphere filling fraction in random packing at selected light wavelengths in the solar spectrum.

[0058] FIG. 18 illustrates dependence of the sunblock power, 1/<l*>, on the diameter and filling fraction of randomly packed SiO.sub.2 microspheres.

[0059] FIGS. 19A and 19B are schematic illustrations of sphere polydispersity effect on filling fraction.

[0060] FIG. 20 illustrates dependence of the sunblock power, 1/<l*>, on the diameter and filling fraction of randomly packed TiO.sub.2 microspheres in a medium of refractive index 1.54.

DETAILED DESCRIPTION OF THE INVENTION

[0061] Detailed embodiments of the present invention are disclosed herein; however, it is to be understood that the disclosed embodiments are merely exemplary of the invention, which may be embodied in various forms. Therefore, specific structural and functional details disclosed herein are not to be interpreted as limiting, but merely as a representative basis for teaching one skilled in the art to variously employ the present invention in virtually any appropriately detailed method, structure or system. Further, the terms and phrases used herein are not intended to be limiting, but rather to provide an understandable description of the invention.

[0062] In one embodiment of the present invention, control of light scattering is obtained by using tiered structures where each tier has its own predetermined characteristic scattering properties. For example, FIG. 1 shows diffuse intensity distribution in the two tiers of l*=3 m and 30 m on Si. In FIG. 1, U.sub.d is the diffuse component of the intensity inside the tiers and U.sub.0 is the intensity of incident light. When the two tiers are interchanged, the diffuse intensity distribution is drastically modified. This permits the fabrication of a plurality of tiers of varying degrees of randomness as well as versatile control of scattering properties.

[0063] The diffusion model gives the steady state diffusion equation for light propagation in a slab in the z-direction that is normal to the slab surface as

[00001]$\begin{array}{cc}\frac{d^2.Math.U_d}{d.Math.z^2}=-\frac{3}{l^2}.Math.U_0.Math.e^{-z/1}.& \left(1\right)\end{array}$

[0064] The ballistic component of the intensity in the media is given by

U.sub.b=U.sub.0e.sup.z/l. (2)

[0065] When the thickness of the slab, L, is much larger than l*, the solution to Eq. (1) with appropriate boundary conditions gives transmittance

[00002]$\begin{array}{cc}T\frac{1+z_e}{L/l^{*}+2.Math.z_e},& \left(3\right)\end{array}$

[0066] where z.sub.e is the extrapolation length normalized by l* and the extrapolation length is the distance outside the slab over which the diffuse intensity vanishes. When the internal reflectance at the boundaries is R, the extrapolation length ratio is given by

[00003]$\begin{array}{cc}{z}_e=\frac{2}{3}.Math.\frac{1+R}{1-R}.& \left(4\right)\end{array}$

[0067] Equation (3) shows that, roughly, transmittance in a thick slab is inversely proportional to the thickness. With transmittance measurement at various thicknesses, l* and z.sub.e can be experimentally determined using Eq. (3). The 1 can be determined from the ballistic transmittance of, desirably, thin samples. Therefore, the scattering parameters of each tier in a multi-tiered stack can be obtained from the measurement on the uniform slabs of the same scattering properties as each tier.

[0068] The scattering properties of the multi-tiered stack may be predicted by solving the diffusion equation with the obtained parameters. Angle-dependent internal reflectance in the equation may also be considered because it can account for the change in the diffuse transmission and reflection when the tier distribution in multi-tiered structures is modified. In solving the diffusion equation, z.sub.e would be close to for the boundaries between the tiers according to Eq. (4) because the internal reflection at the boundaries would be small.

[0069] In other applications, the embodiments of the present invention may be used with solar energy in heating and cooling applications. For example, solar collectors concentrate sunlight in a small area covered with solar selective surfaces. These selective surfaces, that are housed in a vacuum, absorb sunlight strongly while minimizing thermal radiation loss in mid-infrared (mid-IR). Compared to heating, the possibility of cooling by preventing sunlight absorption and maximizing thermal radiation is much less recognized. However, it has been demonstrated that radiative cooling by a purely passive way can achieve temperatures lying almost 40 C. below the ambient temperature at night. Moreover, studies have shown that, even under direct sunlight, materials can be radiatively cooled to temperatures that are 5 C. below the ambient temperature. The remarkable radiative cooling performance shows that the passive cooling technology of the embodiments of the present invention have great potential for widespread use in buildings. The inexpensive radiation cooling technology of the present invention may save electrical energy consumption in residential buildings substantially because 87% of U.S. households are equipped with air conditioners. In addition to air conditioning in residential buildings, the potential applications of radiative cooling of the present invention has application in various interior/exterior automotive parts, outdoor non-residential construction walls, chemical container tanks, electronic devices with hot spots, and so on.

[0070] The cooling power of a material under sunlight is defined by

P.sub.cool(T)=P.sub.rad(T)P.sub.atm(T.sub.amb)P.sub.sumP.sub.other, (5)

[0071] where P.sub.rad is the power radiated by the material, P.sub.atm, is the power absorbed by the material from the atmospheric radiation, P.sub.sum is the power absorbed by the material from the solar radiation, P.sub.other is the power transferred to the material from other sources typically by conduction and convection, T is the material temperature, and T.sub.amb is the ambient temperature. T is lowered as the cooling process proceeds and reaches a final value when the cooling power becomes zero. The cooling power is calculated using the standard solar spectrum such as AM1.5G for P.sub.sun and the mid-IR atmospheric radiation spectra for P.sub.atm. The solar and atmospheric radiation spectra are shown in FIG. 2 where each spectrum is normalized by its maximum intensity. These two spectra have little overlap with each other so that each can be controlled separately. The black body radiation power at 25 C. is 450 W/m.sup.2 which is comparable to the solar power that is 1000 W/m.sup.2. Therefore, the control of both solar absorptivity and mid-IR emissivity of a material has substantial effect on the cooling power.

[0072] In the mid-IR, P.sub.rad , and P.sub.atm have opposite effects on cooling. If atmospheric radiation were a black body spectrum, these two would be the same at the same temperature. This is because of the Kirchhoff's law which states that absorptivity is the same as emissivity at equilibrium. Thus, if the atmosphere were a black body, the power radiated from the material would be the same as the absorbed power by the material. However, the atmospheric radiation spectrum in FIG. 2 exhibits a wavelength interval 813m where the radiation is minimal. Thus, if the material radiates into this window strongly while the radiation is suppressed in the other spectral regions, the heat exchange between the material and the atmosphere would be minimized so that the cooling is facilitated. It has long been recognized that the ideal emissivity consists of 1 within the atmospheric window and 0 otherwise. However, actual experiment has revealed negligible difference in the sample temperature between a material close to the ideal emissivity and another close to a black body.

[0073] For certain embodiments of the present invention, it has been found that the cooling power of a mid-IR black body is actually larger than that of an ideal emissivity material. Therefore, for maximum cooling, the material should exhibit high emissivity in the broad mid-IR range and low absorptivity in the solar spectrum.

[0074] For high emissivity in the mid-IR, many polar materials may be used such as SiO.sub.2, SiO, SiC, TiO.sub.2, HfO.sub.2, Al.sub.2O.sub.3, ZnO, etc. These materials exhibit resonances in the mid-IR due to atomic vibrations. The resonances are manifest as a strong dispersion in the dielectric function. This dispersion typically involves not only high absorption peaks but also high reflection. For maximum cooling, the reflection should be minimized. In certain embodiments, the present invention reduces the reflection loss due to increase emission using microsphere-based structures. In the mid-IR, the photon wavelength (10 m) is much greater than the size of the microspheres (1 m). In this case, mid-IR light does not see the detailed structures and responds roughly to an average of the dielectric function. Based on the effective medium theory, which finds the average dielectric function, reflection decreases as the filling fraction of the microspheres decreases. For example, FIG. 3 compares the calculated mid-IR emissivity spectrum of a solid SiO.sub.2 film and a film of SiO.sub.2 microspheres of 55% filling fraction. The calculation is based on Maxwell-Garnett effective medium theory and the films are thick (100 m). The SiO.sub.2 microspheres show high emissivity in the mid-IR and the emissivity is enhanced compared to a solid SiO.sub.2 film. Therefore, the cooling power can be enhanced by decreasing the microsphere filling fraction in the structures for thick films.

[0075] In certain embodiments, the present invention concerns radiative cooler coatings adapted for use with sunlight which consist of multilayer stacks with photonic band gaps to reduce sunlight absorption. In other embodiments, fabrication of the structures involves layer-by-layer deposition processes with a precise control of the thickness of each layer. Moreover, for efficient suppression of the broad solar absorption, a large number of layers with several different periodicities are required in the multilayer stack. For example, a previous study used 30 layers to achieve a 3.5% solar absorptivity. When many layers are used, the fabrication cost and time would not be within the practical bounds. The embodiments of the present invention overcome this known problem and achieve similar or even better cooling performance using random arrangements of microspheres. The coatings of the present invention allow for inexpensive manufacturing without requiring precision control. The microsphere-based coatings of the present invention can scatter incident light back to the atmosphere so that solar absorption is reduced. Even when the coating needs to be thick, the thickness does not matter much in terms of the manufacturing and material cost.

[0076] The radiative cooling is expected to be most effective in regions of dry atmosphere such as the State of New Mexico (NM). This is because the moisture in the atmosphere is a strong absorber of certain bands in the mid-IR. In particular, the atmospheric transparent window 813m is significantly affected by the water vapor absorption. Thus, as the atmosphere becomes more humid, the atmospheric radiation becomes closer to the black body radiation and the radiative cooling effect decreases. Because of the low relative humidity in NM, the radiative cooling technology of the microsphere-based coatings of certain embodiments of the present invention would be greatly beneficial. Moreover, the effective sunlight scattering of the coatings would prevent solar heating in regions of strong sunshine. For example, in the city of Albuquerque in NM, average 278 days per year are sunny or partly sunny days.

[0077] Light trapping is important in various optoelectronic applications. For example, for solar photovoltaics, light trapping inside photoactive layers enhances energy conversion efficiency. It has also been demonstrated that photonic nanostructures that are highly efficient in light trapping in silicon solar cells. The structures diffract light into the underneath film and light is trapped in the film through resonances. An alternative strategy for light trapping is to randomly corrugate the film surface. For the present invention, when the film is much thicker than the light wavelength, the light trapping reaches the thermodynamic limit known as the Lambertian limit. The Lambertian light trapping is approximately realized in silicon solar cells by randomly corrugating the silicon surface. While this strategy is already used in commercial silicon cells, its usefulness in thin-film photovoltaics is highly questioned because a significant part of the expensive photoactive layer is lost by texturing. In contrast, additive techniques can also be used. For example, random metallic particles can be added on thin solar cells for light trapping. However, the plasmonic resonances in the particles involve significant optical loss. Thus, this technique is not commonly used for high efficiency solar cells such as GaAs or CIGS based cells. In certain embodiments of the present invention, a different approach that relies on random packing of microspheres to realize the Lambertian light trapping is used.

[0078] The microsphere-based coatings of the present invention control randomness to minimize reflection loss, while randomizing the light path. The degree of randomness is an important parameter that determines the level of light trapping. When the coating scatters light too strongly, a significant fraction of the incident light will be back-scattered as optical loss. If the scattering is too weak, the light path randomization will be difficult. Thus, embodiments of the present invention adjust the randomness in the microsphere-based coating to realize the Lambertian light trapping with minimal reflection loss.

[0079] It has long been noted that the efficiency of solar cells deteriorates as they are heated under sunlight. The typical temperature difference between a solar cell and the atmosphere is 50-60 C. at the solar irradiance of 1000 W/m.sup.2. For silicon solar cells that exhibit 25% efficiency at 25 C., the efficiency drops to 21% when the cell temperature reaches 55 C. The heating problem in solar cells becomes even more serious when they operate with sunlight concentration. To prevent heating of solar cells, various heat removal systems based on convection and conduction have been considered. More recently, it was demonstrated that radiative cooling will also be effective in increasing solar cell efficiency. For radiative cooling, a promising experimental study used periodic SiO.sub.2 structures on silicon cells. These structures reduced the temperature of a silicon solar cell by 13 C. However, the light trapping effect of the structures was only slight. Moreover, the structures raise practical fabrication issues. For example, the deposition of 500-m-thick SiO.sub.2 films (the study used a SiO.sub.2 plate and an index matching liquid, which would still not be very practical) and the reactive ion etching of a 10-m-depth on the film would be time consuming and expensive. In comparison, the microsphere-based coatings of the present invention enable much simpler processing. Further, the mid-IR emissivity of the coatings is very high as shown in FIG. 3. Certain embodiments of the present invention have achieved 94.3% emissivity averaged over the mid-IR emission spectrum and angle. Therefore, the microsphere-based coatings of certain embodiments of the present invention are very effective in removing heat in solar cells and efficient light trapping is realized with the coatings without decreasing the high mid-IR emissivity.

[0080] Langmuir-Blodgett (LB) technique is commonly used to self-assemble monolayers on a substrate. In this technique, a monolayer of hexagonally close-packed structures is formed on a liquid surface is then transferred onto a substrate that is vertically pulled out of the liquid. By repeating the process, multilayer sphere arrays may be fabricated. In this case, the degree of randomness typically increases as each layer is added. Thus, structures with graded randomness can be fabricated. Moreover, the degree of disorder in each layer can be controlled.

[0081] In one preferred embodiment of the present invention, the degree of randomness will be controlled in each layer in the LB assembly. The disorder may be characterized by image analysis after adding each layer. Light scattering may be characterized by measuring transmission and reflection for SiO.sub.2 and TiO.sub.2 microspheres.

[0082] The assembled SiO.sub.2 sphere monolayers made in accordance with an embodiment of the present invention were characterized by laser diffraction. The average crystalline domain size, G, was obtained from the laser diffraction pattern. FIG. 4 shows scanning electron micrograph (SEM) images of the SiO.sub.2 sphere monolayers with the G values in microns for various combinations of the pulling speed and the surface pressure. The results show that the structural order can be controlled by the latter parameters in the LB process. Moreover, the results agree with model predictions very well. The comparison between the two is given in FIG. 5 where black dots are experimental points at the largest crystalline domain size and the lines are model predictions. At moderate pulling speeds, the required surface pressure increases for the second layer (b) compared to the first layer (a).

[0083] In other embodiments, the present invention may vary the pulling speed and surface pressure in each layer in the LB process to control the degree of randomness. The randomness of a layer depends not only on the two parameters but also on the randomness of the previous layer. Sample preparations may be categorized as follows: (1) the two parameters are set to the maximum G condition throughout the multilayers, (2) the parameters are gradually detuned from the condition as the layers are added, and (3) the parameters are initially detuned and are closer to the maximum G condition as the layers are added. Following these methods, the variation of the randomness in the film thickness direction may be controlled.

[0084] Sedimentation of colloidal microspheres is known to induce f. c.c. crystals of a long range order with a (111) plane at the film surface. The sedimentation process may be accelerated using a centrifuge without affecting the order. In the sedimentation process, it is difficult to introduce a controlled degree of randomness into the crystals. However, it is possible to create almost completely random arrangement of microspheres by inducing colloidal instability. Colloidal microspheres in suspensions are often charged and the interaction between the spheres becomes repulsive. When the repulsive force dominates the van der Waals attraction force, the colloid is stable. However, when an electrolyte is added to the solution, the repulsive potential barrier is lowered. As a result, the microspheres coagulate when the electrolyte concentration exceeds a limit known as the critical coagulation concentration. This coagulation process leads to random structures. Thus, layers having structures of alternating tiers of order and disorder may be created using the sedimentation process above and below the critical coagulation concentration alternately. A previous study on template directed colloidal self-assembly showed that, when sphere layers are grown on a structure with a lattice plane different than (111), the structure transitions into the (111) plane through the gradual introduction of defects. Based on this, the sedimentation of stable colloids on random structures may result in ordered layers after addition of some number of layers. In this case, an ordered tier may be deposited on a disordered tier using the sedimentation method. Therefore, the present invention advantageously uses this to obtain structures of alternating ordered and disordered tiers using the sedimentation process.

[0085] Alternating tiers of ordered and disorders structures may be fabricated using the sedimentation method of the present invention. The scattering properties of the multi- tiered structures based on SiO.sub.2 and TiO.sub.2 microspheres may be characterized by transmission and reflection measurement.

[0086] KCl salt solution was added to stable SiO.sub.2 microsphere colloids to induce instability. After the solvent was removed, a film of randomly packed microspheres was obtained. FIG. 6A shows an SEM image of the resulting structures. The randomness of the structures was characterized by autocorrelation function as shown in FIG. 6B. The autocorrelation function was obtained by analyzing the image contrast in FIG. 6A over an arbitrarily selected line. The function shows the clear signature of the random structures. Sedimentation without inducing colloidal instability results in well-ordered structures.

[0087] In other embodiments, the present invention provides multi-tiered structures of alternating order and disorder using a sedimentation method. For these embodiments of the present invention, the deposition of an ordered film on disordered structures is provided. This may be accomplished by using sediment stable colloids on random structures with different film thicknesses and sedimentation conditions. Ordered SiO.sub.2 or TiO.sub.2 sphere films may be grown on randomly packed polystyrene spheres. Subsequent selective removal of the polystyrene spheres will result in a film of the ordered SiO.sub.2 or TiO.sub.2 spheres. The scattering properties of the ordered SiO.sub.2 or TiO.sub.2 film can be measured to extract the diffusion parameters. The diffusion parameters of the disordered structures can be determined separately with similar measurement on uniform disordered films. The diffusion problem described above may be solved for multi-tiers of alternating order and disorder using the obtained scattering parameters.

[0088] Light propagation in well-ordered tiers depends on the photonic band structure. Thus, the actual interaction between the ordered and the disordered tiers will be more complicated than the prediction by the diffusion equation that ignores the spectral dependence of scattering parameters. However, for low index microspheres, the modification of photonic band structure by the structure periodicity will be weak. In this case, the diffusion approximation may be plausible.

[0089] In a preferred embodiment, as shown in FIGS. 7A-7E, the microsphere suspension can be directly spray-coated onto a substrate with an airbrush pistol to achieve random structures. FIG. 7A shows an apparatus consisting of a gravity-fed airbrush 100 (Badger gravity feed series, Model 100G), an air compressor 102 (Badger, TC910 Aspire Pro), and a custom-built, linear-motion, heated stage 104. Spray deposition can be performed multiple times over the substrate as the stage moves back and forth on a metal platform 106 over heater 108, and the heating dries the fine droplets on the surface in a controlled fashion. The stage temperature and speed of motor 110 are controlled up to 150 C. and 3.6 mm/s, respectively.

[0090] The spray process involves a number of parameters such as stage/scan speed, distance of airbrush from the substrate, flow rate, nozzle outlet pressure, and substrate temperature. Substrate temperature is important for the drying dynamics of droplets, in which higher substrate temperatures allow for faster drying of the droplets and prevent coalescence into larger droplet before drying. Stage operating temperatures may be in the range of 130 C. This temperature is high enough to allow for fast evaporation.

[0091] Nozzle outlet pressure and distance from the substrate are other parameters in the deposition process. Increasing pressure results in increasing pressure drop across the nozzle and subsequently increasing fluid velocity through the airbrush. With increasing pressure, liquid dispersion breaks into smaller/finer ligaments and droplets. While nozzle pressure affects the mass flow rate of microsphere suspension, the nozzle distance controls the surface coverage of microspheres deposited onto the substrate. It was determined for a preferred embodiment of the present invention that the nozzle pressure and distance of 20 psi and 10 cm, respectively, allow for fast droplet drying and relatively uniform coats of microspheres after a few stage cycles. See FIGS. 7D-E.

[0092] Light scattering in random structures and photonic band gap in periodic structures may have relations to each other. For example, as the refractive index of a constituent material increases, in general, the scattering strength increases in random media and the photonic band gap widens in photonic crystals. For 3D structures, the realization of a complete photonic band gap has proved challenging but a few structures exhibit such a band gap. A well-known example of 3D photonic band gap structures is the woodpile structures of a diamond lattice. The structures consist of layers of 1D rod arrays with the rod direction of a layer rotated by 90 at the next layer. When the periodicity of the structures is destroyed, a random fibrillar network would result. Interestingly, this random structure is recently found in white beetle scales which exhibit the smallest transport mean free path among known random media of low refractive index. The inverse woodpile structures exhibit even a larger photonic band gap than the woodpile structures. Interestingly, the inverse structures of random fibrillar network, namely the random networks of nanopores, achieved the highest light scattering efficiency when first introduced in 1999. While the photonic band gap in the woodpiles or the inverse woodpiles is partly due to the diamond lattice, the strong scattering properties that result when the lattice is disturbed might derive from the network structures. Fibrillar networks resulting from the disturbance of diamond-bonding networks can even exhibit a photonic band gap without the periodicity requirement. While the band gap can be explained by the bonding and antibonding photonic states, it would also indicate extremely strong light scattering of fibrillar networks. However, the origin of such light scattering strength manifested by the small transport mean free paths in the network structures is still largely unknown.

[0093] Toward the understanding of the strong light scattering in fibrillar networks, it is important to establish the relationship between the structure and the optical properties. In particular, the transition of the optical properties from periodic to random structures may reveal important physics that relates between the two. The physics may provide insight on how to realize optical Anderson localization in 3D structures with hints from the research in photonic band gap materials. The realization of the Anderson localization has been quite challenging: only a few reports so far claimed success and these reports are still inconclusive because of the complications such as optical absorption. The establishment of the structure-property relationship will also be important in the realization of extremely thin white films using fibrillar networks which would enable paper-thin displays, solar heat management in buildings and space vehicles, etc.

[0094] In other aspects, the present invention provides a method based on self-assembly of SiO.sub.2 or TiO.sub.2 microspheres to fabricate fibrillar network nanostructures. The method is designed to enable the precise control of the structures. FIG. 8 illustrates the following fabrication process: (step a) periodic grooves 200-203 are patterned on a surface which may be a c-Si surface 204, (step b) microspheres may be deposited on the surface inside the grooves as monolayer chains by template directed self-assembly, (step c) the sphere chain arrays 210-212 may be transferred onto an organic tape 220, (step d) samples of various periodicities may be fabricated and stacked with controlled orientations, and (step e) after burning out the tape, the sphere chain arrays will collapse down and form a disordered network 230 of sphere chains forming a multilayer coating. As shown in FIG. 8E, a coating having 3 layers is formed but other numbers of layers may be used as well. Because the developed method provides precise control on structures, a relationship between the optical properties and the structures may be established.

[0095] For one particular embodiment, the present invention patterned c-Si surfaces using interference lithography and deposited spheres on the grooves using the LB method as shown in FIG. 9. A simpler spin coating can also be used. After the sphere chains were prepared on c-Si surfaces, the tape was burned out.

[0096] To obtain l*, l, and R for various combinations of the periodicity distribution, the sphere filling fraction, and the sphere chain orientation may be used. The sphere filling fraction was fixed using monodisperse spheres. The distribution of the in-plane periodicity may be varied in the thickness direction with isotropy to achieve almost completely random scattering. Once the periodicity distribution is determined, a structure that consists of a periodic stack and a random stack was fabricated. FIG. 10A illustrates the structure schematically with ordered layers 300-305 and disordered layers 310-315. This structure will be compared to a uniform scattering structure in FIG. 10C that consists of the same in-plane layers with a different distribution in the thickness direction. The uniform structure in FIG. 10C represents the complete mixing of the periodic stack and the random stack. The intermediate mixing of the two stacks may be realized by a number of different distributions of the same in-plane layers. An example of the intermediate mixing is shown in FIG. 10B. Assuming that the resulting structure can be regarded as a uniform diffusive medium, the mean free paths will be obtained to show how the mean free paths depend on the distribution of the in-plane periodicities. This will reveal how the mean free paths increase as a random structure is diluted by mixing with a periodic structure. Based on the results the dilution path that gives the slowest and the fastest increase of the mean free paths may be determined. To use the results as a means to finding extremely strong scattering structures, the original undiluted random structure shown in FIG. 10A may be viewed as a structure that is diluted from unknown more concentrated structures. This view is similar to treating the FIG. 10B structure as one that is diluted from the FIG. 10A structure. In this case, the layers with the average periodicity in the original random structure can be identified as a periodic solvent.

[0097] In yet other embodiments, the present invention concerns ways in which the transport mean free path, l*, may be changed or altered as desired. For example, the l* for layers 310-315 in FIG. 10A is smaller than the r for layers 310-315 in FIG. 10B as a result of adding ordered layers in 312 and 313. In turn, the l* for layers 310-315 in FIG. 10C is even greater than the l* for layers 310-315 in FIG. 10B as a result of adding even more ordered layers in 311, 312 and 314.

[0098] As is also shown, an ordered layer as shown in FIG. 9 may be used to create an ordered layer in a tier such as layer 305 for example. Layer 305 in FIG. 10A may be created by exfoliating or otherwise transferring the layer shown in FIG. 9 to the tier.

[0099] The same steps may be used with different sphere filling fractions. For each filling fraction, the structures of the least transport mean free paths may be determined. These will determine the filling fraction dependence of the mean free paths. They will also determine the optimum filling fraction for the smallest mean free paths for both SiO.sub.2 and TiO.sub.2 microspheres.

[0100] In other embodiments of the present invention, the anisotropy of the optimum structures may also be determined to minimize the mean free paths as suggested by the structures in white beetle scales.

[0101] In still further embodiments, the present invention provides scattering material that can be made to scatter light even more strongly than know before. Conversely, in other embodiments, the present invention shows how to mitigate the scattering strength of a material in a highly controlled fashion based on the relation between the order-disorder mixing and the scattering properties and the ability to control the scattering properties of materials precisely.

[0102] The structures based on microsphere chains can model the actual morphology of fiber or pore networks that are found to provide extremely strong scattering. Such morphologies include, but are not limited to, curved sphere chains with non-uniform cross-sections. As illustrated in FIGS. 11A and 11B, when grooves are wider than the sphere size, self-assembly will result in non-straight chains (FIG. 11B) as the spheres are connected by capillary forces.

[0103] The kinked chain of FIG. 11B has a higher degree of randomness than the linear chain shown in FIG. 11A. As a result, where desired, kinked chains may be used or introduced to lower the transport mean free path, l*.

[0104] Moreover, using microspheres with polydispersity, randomly non-uniform cross-sections in the fibrils was realized for certain embodiments of the present invention. These concepts may also be applied to the linear-chain structures that are found to exhibit very small transport mean free paths.

[0105] In one embodiment of the present invention, the primary materials for the microspheres may be SiO.sub.2 and TiO.sub.2, which have refractive indices of 1.45 and 2.5 (anatase), respectively. However, the dependence of the refractive index on the scattering properties will not be limited to these two indices. Once the solid structures are fabricated, the structures may be infiltrated with a liquid with a known refractive index to control the refractive index contrast. The refractive index of the liquid may be controlled by mixing low and high index liquids in varied ratios. Without liquid infiltration, it is possible that the structures made of TiO.sub.2 microspheres exhibit Anderson localization because of the high refractive index.

[0106] In radiative cooling under sunlight applications, scattering is generally desired to reduce sunlight absorption by the material underlying the scattering coating. For cooling, it is important to achieve high emissivity in the mid-IR. The high emissivity is not affected much by the structures because the sphere size is much smaller than the wavelength of mid-IR radiation. Rather, the emissivity will be determined mostly by the sphere filling fraction and the sphere materials. In principle, the sphere filling fraction can be controlled by various methods such as the one that fabricates fibrillar networks described above. However, in real applications, manufacturability of the structures should be considered. In this respect, the fabrication methods based on colloidal instability or spray coating would be more suitable. Because the sphere filling fraction of the structures obtained by these methods would have a quite limited range, the emissivity control will not be easy in real applications. In fact, the embodiments of the present invention have achieved a very high emissivity.

[0107] In one embodiment, the present invention deposits uniform random structures of microspheres on materials mostly using the techniques of colloidal instability and spray coating. The solar absorptivity and mid-IR emissivity of the samples may be measured at various random structure coating thicknesses, sphere materials, and coating conditions.

[0108] Solving the diffusion problem described above, the solar absorptivity for random SiO.sub.2 microspheres on absorbing materials was calculated. For initial estimation, an expected transport mean free path of l*=3 m and filling fraction of 55% was used. For the front surface, the proper internal reflectance was taken into account. For the internal reflectance at the interface between the microsphere coating and the absorbing material, R.sub.s, two extreme values of 0 and 0.96, which represent an ideal black body and a good metal, respectively were selected. The actual internal reflectance for a good metal would not reach as high as 0.96 because of the excitation of surface plasmon polaritons. The calculated solar absorptivity as a function of the coating thickness is shown in FIG. 12. In general, absorptivity decreases as the coating thickness increases because of the light scattering in the coating. The effect of the interface reflectance on the absorptivity diminishes as the coating becomes thicker. FIG. 12 shows that absorptivity for a sphere-coated black body is only 3.4% when the coating thickness is 200 m. With TiO.sub.2 microspheres, the absorptivity would be even less because of the stronger scattering.

[0109] In yet another embodiment of the present invention, uniform random SiO.sub.2 spheres of a diameter 900 nm were coated on a Ag film using the method of colloidal instability and measured absorptivity using an integrating sphere. Absorptivity increases as the wavelength increases. The spectral dependence of absorptivity suggests that the addition of more layers of larger spheres may be more efficient in reducing absorptivity in the near-IR. The measured absorptivity (0.15) is larger than the value (0.05) calculated with R.sub.s=0.96 partly due to the excitation of surface plasmon polaritons. However, it was found that the measurement had an error of 0.1 in reflectance and transmittance. A recent study reported a similar level of error for the similar measurement system. While the error was attributed to the light lost in the sample holder in the past study, the analysis indicates that the scattered light was not completely collected by the integrating sphere.

[0110] The mid-IR emissivity of a SiO.sub.2 spheres on a Ag film may be measured. The measurement gives an average emissivity with the room temperature black body radiation spectrum as a weighting function. The emissivity is also averaged over the hemispherical solid angle. The measurement gave an emissivity of 0.943 which is already very high

[0111] Based on the measured emissivity (0.943) and the predicted absorptivity (0.034), the cooling power in Eq. (5) for a random SiO.sub.2 sphere coating on a black body (black over the solar spectrum) was calculated. The use of the constant mid-IR emissivity may introduce errors in the cooling power and the spectral measurement of emissivity will correct the errors. For the convection and conduction term, the heat transfer relation P.sub.other=(T.sub.ambT) was used where =2.5 W/(m.sup.2K) is the measured value for a device in a past study. The predicted cooling power when the coating thickness is 200 m and the ambient temperature is 27 C. is given as the middle line in FIG. 13. The cooling power of the coating is slightly below a mid-IR black body and significantly higher than an ideal emissivity discussed above. While the cooling power decreases most slowly in the case of the ideal emissivity as temperature decreases, its magnitude is less than a mid-IR black body. The lower cooling power of the ideal emissivity is due to the fact that the low mid-IR emissivity of the atmosphere is not limited to 813m as seen in FIG. 2. At steady state, the temperature of the material will reach a point where the cooling power becomes zero. FIG. 14 shows that, under direct sunlight, the material with the coating will reach the temperature of 10 C., which is 37 C. below the ambient temperature. When the material is not a black body (black over the solar spectrum), its temperature will be even lower than 10 C. When the emissivity spectrum predicted from effective medium theory as in FIG. 3 is used instead of a constant 0.943, the predicted material temperature is 9.4 C. which is very close to 10 C. For simple processing, the colloidal instability method and spray coating to deposit the sphere layer was used. The coating may be a uniform random structure.

[0112] As in the previous section, the mid-IR emissivity of the solar cell coatings are mostly determined by the sphere materials and the sphere filling fraction. When absorption is too small, the efficiency will be low. In the opposite case, however, it is not clear if the maximum absorption will achieve the highest efficiency because of the increase in the cell temperature. The temperature dependence and the absorption dependence of the photovoltaic efficiency will be different for different cells. To maximize absorption, the microspheres will radiatively cool the cells, which is always an advantage while the optimum absorption is not clear. To determine the desired distribution of randomness in the tiered coatings for efficient light trapping, the diffusion equation may be used by a microsphere-based coating of a uniform randomness on a semi-infinite Si substrate with a perfect antireflection coating. The diffusion problem was solved for this structure to obtain absorptivity as a function of the coating thickness. The results are displayed in FIG. 14 for (a) l*=3 m and (b) l*=200 m. Here, absorption by diffuse light is shown by the lower line and total absorption is shown by the upper line. In both cases, total absorption decreases as the coating becomes thicker and the diffuse absorption exhibits a maximum. When the coating is thick enough, absorption is mostly due to diffuse light. For thin Si films, diffuse absorption should be maximized for efficient light trapping. FIG. 14 shows that the maximum diffuse absorption is only 0.67 for the strong scattering (a) but is as large as 0.94 for the weak scattering (b). The required coating thickness for the two cases is 2.2 m and 5.2 m, respectively. The results indicate that, for efficient light trapping, weak-scattering thick structures are desired rather than strong-scattering thin structures.

[0113] For a flat Si surface, the diffuse light is not completely randomized inside the Si layer. Instead, due to Snell's law, the direction of the diffuse light inside Si is confined within a cone defined by =sin.sup.1(1/ n) where is the angle from the surface normal and n is the index contrast between Si and the coating. Thus, for efficient light trapping, the effective index of the coating should be high. However, typical non-absorbing materials for microspheres exhibit a refractive index lower than Si and is less than 90. For the Lambertian light trapping, the Si surface should be corrugated. Because the coating generates diffuse light, the corrugation does not have to be deep. When the corrugation is only shallow, the loss of expensive photoactive layer by corrugation will be minimal. Therefore, efficient light trapping in semiconductor-based solar cells requires weak-scattering thick coatings on slightly corrugated surfaces with an antireflection coating.

[0114] The example of l*=200 m in FIG. 14B represents highly ordered structures. The desired structures of tiered randomness will maximize diffusive intensity at the semiconductor interface while minimizing reflection loss. Semiconductor surfaces may be slightly corrugate to maximize light trapping. For the corrugation, periodic structures with controlled depths of corrugation may be used. In other embodiments, the surface of working solar cells will be corrugated, an antireflection coating will be applied on the surface, and the microspheres will be coated on top.

[0115] In yet other embodiments, coatings are provided that effectively and efficiently scatter sunlight. The scattering strength may be characterized by the so-called transport mean free paths (l*). The transport mean free path is the length over which light loses its memory of original direction while traveling in a scattering medium. Approximately, solar absorption is linearly proportional to r in thick coatings. l* depends on both the particle diameter d and the filling fraction f For randomly packed single size spheres, f ranges between 0.55 and 0.64. A powerful method to determine l* is coherent potential approximation (CPA), which is known to be highly accurate for any f. The calculated l* for the two extreme values off in randomly packed SiO.sub.2 spheres of 0.9 m in diameter d is compared in FIG. 15. The results should be between the two predicted values and is closer to the prediction for f=0.64. The CPA predictions of l* agree remarkably well reproducing even the detailed spectral features. Because l* increases as the light wavelength increases in this case, absorption will also exhibit the same trend when the microsphere-based coating is placed on an absorbing material. For example, when a microsphere coating of a thickness L=700 m is on a black body, absorption A2l*/L is expected to be 0.7% and 11% at =0.4 m and 2.5 m, respectively. Therefore, with the d=0.9 m microspheres, solar absorption in the near IR is significant and this increases the temperature of a material underneath the coating. Commercial paints also suffer from IR absorption by materials underneath the paints in even higher degrees.

[0116] The near IR absorption can be reduced by using different size spheres. FIG. 16 shows calculated l* in the solar spectrum at various sphere diameters. It is revealed that l*, hence solar absorption, is minimized when the sphere size is d=4 m. In general, l* decreases as d increases up to 4 m with the effect being most pronounced in the long wavelengths. When d is larger than 4 m, l* increases as d increases primarily in the short wavelengths. When d is much larger than , l* can be estimated based on the theory developed by Kubelka-Munk and Brewster-Tien. The estimation gives

[00004]$l^{*}\frac{d}{3.Math.f}.$

Thus, l* is linearly proportional to d for large spheres.

[0117] For example, when d=50 m, l* is estimated to be 30.3m. Popular low refractive index pigments used in commercial solar reflective paints are of a shape of hollow spherical shells of d=20150. Therefore, the sphere size of popular commercial paints based on low refractive index pigments leads to much weaker light scattering than the coatings of the present invention.

[0118] Brewster-Tien criterion says that, when spheres are large enough, the filling fraction of spheres does not significantly affect the scattering efficiency of each particle. However, for small size spheres, it has been reported that light scattering strength is maximized at a sphere volume fraction of roughly around f=0.2..sup.0 Because the filling fraction in random packing is larger than this value, the dependence of l* on f for random packing was analyzed. FIG. 17 shows this dependence at selected wavelengths in the solar spectrum when the diameter of SiO.sub.2 spheres is 4 m. The region off >0.64 corresponds to the case where microspheres are sintered. Overall, l* increases as f increases, while an opposite behavior is observed at short wavelengths. The spectral average of l* is minimum at f=0.55. Thus, for maximum scattering of sunlight, it is desired to minimize the sphere volume fraction in random packing.

[0119] The cooling effect of white coatings can be characterized by l* averaged with a solar spectrum as a weighting factor. This average <l*> is approximately proportional to the solar power absorbed by the material underneath a coating, p.sub.sun, because

[00005]$P_{\mathrm{sun}}=A\left(\right).Math.I\left(\right).Math.d\frac{2.Math.l^{*}\left(\right)}{L}.Math.I\left(\right).Math.d.Math.=\frac{2}{L}<l^{*}>I\left(\right).Math.d.Math..Math.,$

[0120] where I() is the sunlight spectrum and <l*> is defined by

[00006]$<l^{*}>\frac{l^{*}\left(\right).Math.I\left(\right).Math.d.Math..Math.}{I\left(\right).Math.d.Math..Math.}$

[0121] FIG. 18 shows 1/<l*>, which is a measure of sunblock performance, as a function of d and f for SiO.sub.2 microspheres. The maximum sunblock performance is obtained when d=4m and f=0.55. The optimum f corresponds to the minimum achievable value for random sphere packing. It is known that, as the sphere size distribution becomes wider, the sphere fraction decreases. This is schematically illustrated in FIG. 19. In FIG. 19, the sphere filling fraction is low when monodisperse spheres are randomly packed (left) and is high when polydisperse spheres are packed (right). Thus, it is desired that the spheres are monodisperse to maximize the sunblock power of the coatings. Current commercial paints based on pigments of a low refractive index consist of highly polydisperse particles ranging from 20 to 150 m in size. At these large sizes, polydispersity is desirable for light scattering because, based on the relation

[00007]$l^{*}\frac{d}{3.Math.f},$

increase in f results in decrease in l*. However, for sphere sizes near the optimum for sunblock, monodisperse spheres are desired.

[0122] TiO.sub.2-based paints exhibit optical characteristics that are different from SiO.sub.2 microspheres because of the high refractive index of the pigments. Paints based on rutile TiO.sub.2 particles typically include binders and fillers. The refractive indices of the medium materials and the rutile TiO.sub.2 particles are approximately 1.5 and 2.8, respectively. Commercial solar reflective TiO.sub.2 paints use particles of 200-250 nm in size to maximize scattering in the visible wavelengths. However, solar spectrum includes more than a half of the power in the near IR spectrum >700 nm and the TiO.sub.2 particles of the size range are not efficient in blocking IR sunlight.

[0123] FIG. 20 shows the dependence of 1/<l*> on the TiO.sub.2 sphere diameter and filling fraction. The refractive indices of the medium material and the TiO.sub.2 particles are set to 1.54 and 2.74, respectively. Sunblock performance is maximized when the particle diameter is 1 m and the filling fraction is 26%. Current commercial paints with a TiO.sub.2 particle diameter of 200-250 nm show much smaller sunblock performance for all filling fractions between 0.2 and 0.6. To verify the results, the temperature of a silicon wafer when coated with a commercial TiO.sub.2-based paint was measured. Electron micrographs of the paint confirmed that the particle size is 200-250 nm. For comparison, a silicon wafer is coated with randomly packed SiO.sub.2 spheres of d=0.9m. The two samples had a similar coating thickness and were exposed to direct sunlight. To minimize convective heat transfer, the samples were housed in a box made of a transparent film. The sample with a commercial TiO.sub.2-based paint was 8 C. higher than the one coated with SiO.sub.2 spheres. Calculated l* was 45 m and 19 for the TiO.sub.2 commercial paint and the SiO.sub.2 sphere packing, respectively. Therefore, the calculation is consistent and when a paint with TiO.sub.2 particles of d=1m is used, l* is only 2 m which is more than 20 times smaller than that of the commercial paint.

[0124] In yet other embodiments, for efficient light scattering, the present invention uses hollow microspheres that consist of nanoshells. These hollow microspheres are directly mixed with binders that are typically used for paints. In a preferred embodiment, the binders are polymeric materials. The contrast in refractive index between the binder and the air inside the hollow microspheres is used for efficient light scattering. In this case, the size range of the hollow microspheres is 1-3 microns and the nanoshell thickness is on the order of 1-10 nm.

[0125] In yet other embodiments, rather than have the coatings described above being cooled by radiating thermal energy in the mid-IR spectrum, the present invention may be comprised of a substrate that may be in the form of a sheet that is transparent in the mid-IR spectrum and efficiently scatters sunlight. In this embodiment, the object under the sheet is cooled under sunlight, rather than the substrate itself. The substrate functions both as a sunlight blocker and a mid-IR window for the object. In operation, the object will lose heat by thermal radiation that passes through the substrate into the space in the universe, while not being heated by sunlight. The substrate of this embodiment may be made of polyethylene that is transparent to the mid-IR spectrum.

[0126] In yet other embodiments, the fabrication of a polyethylene substrate can be accomplished by the use of fiber spinning, the deposition of polyethylene microspheres, or the formation of microbubbles within a polyethylene sheet/substrate. In yet other embodiments, the present invention may co-deposit polyethylene with other materials that are subsequently etched away. For example, polyethylene and another polymer is co-deposited by using fiber spinning and the polymer is selectively etched. Similarly, polyethylene microspheres are mixed with the microspheres of other materials. After the microsphere mixture is deposited by spraying or colloidal methods, the microspheres of other materials are selectively etched. For microbubble formation, similar techniques can be used.

[0127] In still further embodiments, thermochromic pigments may be used in the microsphere coatings of the present invention. These coatings are configured to become dark when the atmosphere is cold and bright when warm. For these embodiments, the coating will cool down in summer and warm-up in winter.

[0128] While the foregoing written description enables one of ordinary skill to make and use what is considered presently to be the best mode thereof, those of ordinary skill will understand and appreciate the existence of variations, combinations, and equivalents of the specific embodiment, method, and examples herein. The disclosure should therefore not be limited by the above described embodiments, methods, and examples, but by all embodiments and methods within the scope and spirit of the disclosure.