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| United States Patent | 3987780 |
| Link to this page | http://www.wikipatents.com/3987780.html |
| Inventor(s) | Nozik; Arthur Jack (Westport, CT);
Haacke; Gottfried (Stamford, CT) |
| Abstract | Cadmium stannate has been found to be useful as a window for solar heat
absorbing systems in which advantage is taken of the unique optical
properties of cadmium stannate. When cadmium stannate is in an
electrically conductive state, having a conductivity of greater than
10.sup.3 ohm.sup.-.sup.1 cm.sup.-.sup.1, it becomes transparent to solar
radiation and reflective of thermal infrared radiation. This enables the
cadmium stannate to function as a window which allows passage of solar
radiation through it and incident onto a black body, and at the same time
serve as a reflector of thermal infrared radiation emitted from said body.
This results in more efficient solar heat transfer to the solar heat
collector provided with such a window. |
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Title Information  |
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Drawing from US Patent 3987780 |
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Greenhouse window for solar heat absorbing systems derived from Cd.sub.2
SnO.sub.4 |
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| Publication Date |
October 26, 1976 |
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| Filing Date |
March 3, 1975 |
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Title Information  |
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Description  |
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BACKGROUND OF THE INVENTION
Realization that the fossil fuel supply of the United States is finite and
may be rapidly depleted if the projected growth rate of national energy
consumption continues has led to a search for substitute energy sources.
Among a number of yet unexploited resources, those which have the least
adverse environmental impact and are independent of foreign supplied
deserve the most attention. Utilization of solar radiation is one of the
possibilities for satisfying part of the nation's need for clean and
reliable energy.
The direct conversion of sunlight into electricity by photovoltaic cells or
its collection by heat collectors are proven techniques of solar energy
utilization. They are now used in specialized applications where cost is
not of importance. To be useful on a large scale, in competition with
existing energy sources, the development of technology is needed to enable
the economic production of efficient photovoltaic cells and solar heat
collectors.
The combination of high optical transparency and high electrical
conductivity exhibited by cadmium stannate (Cd.sub.2 SnO.sub.4) can be
exploited for use as transparent electrodes in photovoltaic cells. This is
fully discussed in a copending United States Patent Application, Ser. No.
181,916 and in a paper published in Physical Review, Vol. 6, No. 2, pp
453-59 dated July 15, 1972, entitled: "Optical and Electrical Properties
of Cd.sub.2 SnO.sub.4 : A Defect Semiconductor," by A. J. Nozik.
Utilization of solar energy for space heating or air conditioning
(absorption refrigeration) by collecting solar radiation in heat
collectors has been suggested in a number of publications, including:
Physics Today, Vol. 25, pp 44-49 of February 1972; Natural Resources J.
Vol. 10, 268-326 (1970); Solar Energy, Vol. 13, pp 395-401 (1972); and,
Technical Report AFML-TR-70- 294, pp 21-44 of January 1971. In the
referenced Physics Today article, it has also been proposed to use solar
heat collectors in large-scale solar "farms" and to operate conventional
central power stations with the collected heat.
Two types of solar heat collectors are under consideration, flat-plate
collectors and pipe collectors. In flat-plate collectors, unconcentrated
solar energy is absorbed by flat plates; pipe collectors absorb sunlight
which has been concentrated by suitable lenses and mirrors. The light
absorbing element in both devices is a coating with a large optical
absorption coefficient, .alpha., over most of the solar spectrum. The
collection efficiency depends on .alpha. and on heat losses, which consist
of convection, conduction and radiation losses. Convection and conduction
losses can be eliminated by placing the collecting surface in a vacuum.
Radiation losses consist of infrared radiation and are temperature
dependent, becoming more severe with increasing operating temperature of
the collecting surface. These losses can be minimized by using selective
absorber surfaces which have a large .alpha. for sunlight but a small
emissivity, .epsilon., for heat radiation. Such surfaces are feasible, and
in fact have been prepared since the solar spectrum and the heat radiation
spectrum (up to at least 600.degree. C.) have little overlap -- See J.
Opt. soc. Am. 46, 31 (1956) and Technical Rept. AFML-TR-65-317 (October
1965 ).
Further reduction of radiation losses can be achieved by a greenhouse
window coating deposited adjacent to the solar heat absorbing surface. The
requirements for this coating are high transmittance for the incident
solar radiation and high reflectance for heat radiation escaping from the
absorber surface. These requirements are met by electrically conductive
films of Cd.sub.2 SnO.sub.4 having a conductivity greater than 10.sup.3
ohm.sup.-.sup.1 cm.sup.-.sup.1. These films can be readily formed by the
radio-frequency sputtering technique described in a copending U.S. Pat.
Application, Ser. No. 181,916, filed Sept. 20, 1971, now U.S. Pat. No.
3,811,953 or by chemical spraying methods wherein a solution of cadmium
and tin bromides in the presence of H.sub.2 O.sub.2 and O.sub.2 is sprayed
onto hot substrates at 400.degree. to 1000.degree. C.
The available heat flux from solar heat collectors, consisting of black
body absorbers and greenhouse windows or of selective absorbers and
greenhouse windows, is a function of solar concentration and absorber
temperature. For high solar concentrations (> 10) and absorber
temperatures below 500.degree. C., it has been shown in Technical Report
AFML-TR-70-294 that a greenhouse window does not add to the available heat
flux. However, for lower solar concentrations, the addition of a
greenhouse window contributes significantly to the available heat flux.
Obviously, these investigations show that the highest heat flux
contribution of a greenhouse window coating can be realized in flat-plate
collectors and in pipe collectors which work at high operating
temperatures.
Unfortunately, the solar heat collectors as presently known do not provide
for highly efficient heat collection. This lack of efficiency relates
primarily to the re-radiating of substantial amounts of infrared thermal
energy by the heat collecting surface.
It is an object of this invention to provide a solar heat collector of
improved efficiency.
It is a further object of this invention to provide a solar heat collector
having a greenhouse window which increases the heat flux available to the
heat collecting system of a solar energy converter.
Other objects and attendant advantages of the present invention will be
apparent from the description thereof taken in connection with the
accompanying drawings. The invention is capable of a variety of mechanical
expressions, two of which are illustrated in the accompanying drawings.
Therefore, it is to be expressly understood that the drawings are for the
purpose of illustration only, and are not intended to present the full
scope of the invention which is defined by the appended claims.
SUMMARY OF THE INVENTION
In accordance with the present invention, there is provided an article
comprising cadmium stannate films having the properties of high solar
transmissivity, electrical conductivity and thermal infrared reflectivity
positioned adjacent to a body having a high absorptivity for solar
radiation, said body having heat transfer means attached thereto whereby
thermal energy in said body is dissipated therefrom as useful energy. In
preferred embodiments there are provided heat collectors in two types of
structures. In one the cadmium stannate is contiguous with said body; and
is directly supported by it. In another type the cadmium stannate is
separated from said body by a barrier to thermal conduction and
convection, for example, an evacuated space and is supported on a second
substrate, said substrate itself having high solar transmittance.
In accordance with the present invention the cadmium stannate layer has a
thickness of from 300A to three microns, an electrical conductivity
greater than 10.sup.3 ohm.sup.-.sup.1 cm.sup.-.sup.1, and is preferably of
crystalline phase. It also has a reflectivity greater than 50% for
radiation with wavelengths greater than 3 microns, and preferably a
reflectivity of greater than 90% for radiation with wavelengths in excess
of 2 microns.
The transmissitivity of the Cd.sub.2 SnO.sub.4 layer is at least 50% for
radiation with wavelengths between 0.45 and 1.0 microns, and is preferably
95% for radiation with wavelengths between 0.45 and 1.0 microns. The
average transmissivity of the Cd.sub.2 SnO.sub.4 layer over the wavelength
region 1.0 to 1.5 micron is greater than 25%, and is preferably about 80%.
Control of the transmissivity is achieved by controlling the thickness of
the Cd.sub.2 SnO.sub.4 layer.
BRIEF DESCRIPTION OF THE DRAWINGS
In the accompanying drawings, wherein like characters designate
corresponding parts throughout the several figures:
FIG. 1 is a schematic cross-sectional representation of a solar energy
collecting element adapted for use in a pipe-type heat collector.
FIG. 2 is a schematic cross-sectional representation of a planar heat
collecting element adapted for use in a flat panel type heat collector.
DESCRIPTION OF THE INVENTION
In FIG. 1, the heat transfer fluid 11 is flowing through a steel pipe 12
which is covered on its outer surface with a black coating 13 having a
high absorptivity for solar radiation. The steel pipe 12 is located within
an evacuated glass pipe 14 which has a coating of cadmium stannate 15 on
its inner surface. The glass pipe 14 is positioned such that the inner
steel pipe 12 is located at the focal point of a parabolic reflecting
trough 16. Sunlight 17 impenging on the glass pipe and/or reflecting
trough is absorbed by the black coating 13, and the solar thermal energy
is thus transferred to the fluid 11. Infrared radiation 18 emitted by the
hot surface 13 is reflected back into the system, resulting in more
efficient solar heat transfer.
In FIG. 2, heat transfer fluid 21 is flowing through internal channels 22
located inside flat aluminum panels 23. A black coating 24 having a high
absorptivity for solar radiation is painted on top of the aluminum panel
23. A glass panel 25 having a coating of cadmium stannate 26 on its inner
surface is separated from the aluminum panel 23 by an air gap 27. The
cadmium stannate layer 26 has a high transmittance for solar energy 28 and
a high reflectance for thermal infrared radiation 29, so that the thermal
energy 28 is effectively trapped in the black coating 24 and transferred
to the fluid 21.
EXAMPLE I
A 40% (wt. basis) aqueous solution of SnBr.sub.4 is mixed with a 30% (wt.
basis) aqueous solution CdBr.sub.2 such that the final solution contains
Cd and Sn in the molar ratio of 2:1. A 30% solution of hydrogen peroxide
is then added in an amount equal to one-half of the volume of the mixed
Cd-Sn solution. The resulting solution is then immediately sprayed as a
fine mist onto a quartz substrate maintained at 950.degree. C., using an
oxygen atomizing spray nozzle. A crystalline film of cadmium stannate is
formed on the substrate and it exhibits high transmittance for solar
radiation and high reflectance for thermal infrared radiation. These
optical properties are further enhanced by placing the cadmium stannate
coated quartz in a H.sub.2 atmosphere at 280.degree. C. for 10 minutes.
EXAMPLE II
The same procedure is followed as is described in Example I, except that
glass is used as the substrate and the substrate temperature is maintained
at 600.degree. C. The resulting cadmium stannate film is amorphous rather
than crystalline.
EXAMPLE III
A glass pipe is coated on the inner surface with a 3 micron film of
Cd.sub.2 SnO.sub.4 by the procedure described in Example II. A steel pipe
is coated on its outer surface with a highly absorbing black paint and
then located within the glass pipe. The glass pipe is evacuated and sealed
to maintain a pressure of about 10.sup.-.sup.6 torr. The glass pipe is
then positioned in a parabolic reflecting trough such that the inner steel
pipe is located at the focal point of the parabolic mirror. A
heat-transfer fluid is pumped through the steel pipe. Irradiation of the
ensemble with sunlight results in efficient transfer of solar thermal
energy to the heat-transfer fluid.
EXAMPLE IV
Same as Example II except that the Cd.sub.2 SnO.sub.4 film is deposited
directly on the coated steel pipe.
EXAMPLE V
An aluminum panel with internal channels interconnected to provide a
torturous path for the flow of a heat-transfer fluid is coated on its
outer surface with highly absorbing black paint. A flat panel of glass is
coated with a 0.3 micron film of cadmium stannate by the method described
in Example I, and placed adjacent to the aluminum panel, but separated by
an air gap. Irradiation of the ensemble with sunlight results in highly
efficient transfer of solar thermal energy to the heat-transfer fluid
flowing through the channels of the aluminum panel.
EXAMPLE VI
Same as Example IV, except that the air gap is evacuated to a pressure of
about 10.sup.-.sup.6 torr., and the system sealed to maintain the vacuum.
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Description  |
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