This invention relates generally to a solar collector. In particular, the present invention is directed to a light-weight, highly-stable solar collector that incorporates cables and a compression element to support and stabilize solar elements.
Solar collector systems are generally characterized by having large surface areas to collect solar radiation. The large collecting surface area is usually made up of a group of sub-components connected together and supported to create the larger surface area. Collector systems are designed to either directly collect the sun's electromagnetic energy, such as photovoltaic array systems, or to reflect the energy to a receiving element, such as with heliostats or parabolic concentrators. To improve the efficiency of these systems, many solar collectors track with the sun. These systems either directly track to the sun, such as a solar parabolic dish concentrator which must face the sun, or these systems follow a different path in order to reflect the electromagnetic radiation to a particular location, such as a heliostat. Tracking usually requires the collector system have two rotational degrees of freedom, e.g. altitude and azimuth.
From a design perspective, one of the most critical features of solar collector systems is to have a large surface area for the collector. However, when exposed to environmental elements, these large surface areas create many design problems. Of particular importance are the loads imposed upon the structure due to extreme weather, primarily high winds. To accommodate these high-wind loads, large and heavy structures are incorporated into the design to support the solar elements. A common design for a prior art solar collector system 15 is shown in
While this prior art has been around for decades, to date these systems have been very heavy and expensive to manufacture and install. Their cost and bulkiness has limited their widespread use and acceptance for solar collector systems. The first problem is that these systems contain heavy structural elements to support and stabilize the system in high winds, which contributes to the overall initial high cost of implementing a system. The second problem is that the drive system and other auxiliary components must also be large and powerful to effectively deal with the weight and inertia of the bulky system. The associated large and powerful motors make it difficult to provide fine positional control and motion of the entire structure.
Accordingly, there remains a continuing need to provide solar collector systems which are light weight, stable, easy to manufacture, simple to assemble, inexpensive and can withstand high winds.
One aspect of the present invention is directed to a solar collector comprising solar elements connected to form an array for intercepting the sun's radiation, a compression element positioned substantially perpendicular to the array, and pairs of cables running from opposite sides of the array to the compression element to stabilize the solar elements.
Another aspect is directed to a solar collector comprising solar elements, means for connecting the solar elements to form an array; a compression element positioned substantially perpendicular to the array, and means for stabilizing each solar element with cables running between the array and the compression element.
Yet another aspect is directed to a solar collector comprising solar elements, means for connecting the solar element to form a substantially parabolic array, a compression element positioned along the single axis of symmetry of the parabolic array, and means for stabilizing each solar element with cables running between the parabolic array and the compression element.
Still another aspect is directed to a solar collector comprising a solar element, a compression element positioned substantially perpendicular to the solar element, and a pair of cables connected to opposite sides of the solar element, wherein the pair of cables further connect to the compression element to strengthen the solar element.
The foregoing and other aspects and advantages of the invention will be apparent from the following detailed description of the invention, as illustrated in the accompanying drawings, in which:
a is a side perspective view of a solar collector according to the present invention put under the forces of a high wind;
b is a side perspective view the solar collector in
a is a plan view of a first type of connector according to the present invention;
b is a plan view of a second type of connector according to the present invention;
c is a plan view of a third type of connector according to the present invention;
a is a side perspective view of a solar element according to one embodiment of this invention incorporating cables, a frame and compression elements for strengthening and stabilizing the solar element; and
b is a side perspective view of a solar element according to another embodiment of this invention incorporating cables, corner frames and a compression element for strengthening and stabilizing the solar element.
The size and shape of each collector 20 is dictated by the size, shape and number of solar elements 22 used to build array 30. Typically solar elements 22, such as mirrors and photovoltaic cells, are manufactured as flat panels. The shape of these panels can be any shape, i.e., rectangular, square, hexagonal, etc. The exact size and number of panels used to build array 30 depend on the application of solar collector 20. For the embodiment illustrated in
The overall surface shape of each array 30 is dictated by the orientation of each solar element within array 30. If solar collector 20 comprises photovoltaic elements, then a flat surface array is the preferred shape. However, if solar collector 20 comprises reflector elements for focusing the sun's energy to a specific location, then a substantially parabolic array is required. It is noted that for small arcs, spherical arrays can approximate parabolic arrays. For a parabolic array 30, compression element 28 is positioned along the single axis of reflective symmetry of the parabolic array. Adjustment of the focus of each solar element 22 is accomplished by moving tension elements (a.k.a. cables) along the length of compression element 28. When cables 26 from the outer portions of array 30 are moved closer to the end of compression element 28, they tilt the reflective surface of mirrors towards the compression element and shorten the focus of these mirrors.
The use of cables and connectors to support solar elements 22 results in only a modest decrease in the active area of array 30. Cables 26 are thin and connectors 24 cover just a small portion of the edges of each element 22. The resulting decrease in solar radiation imparted to solar elements 22 is only about 1-2% of their total surface area.
A support structure 34 is used to secure array 30 relative to a fixed structure such as the ground or a building. As shown in
Together compression element 28 and cables 26 form a tension compression system. Each cable 26 may be fitted with a tension adjuster 32 that allows for independent adjustment of the tension within each cable as shown in
Solar collector 20 may be modified to provide it with the capability of furling under high winds as shown in
Although the basic structure and principles behind operation of solar collector 20 are defined above, variations can be made to various components without deviating from the scope of the invention. For instance, several different types of connectors can be used as shown in
Each solar element 22 may itself be strengthened and stabilized through the use of cables 26′ and compression elements 28′ to produce a solar element assembly 22′ that can be used in place of solar elements 22 described above. The strengthening and stabilizing process may be further used to affect the curvature of each element 22.
If solar elements 22 are photovoltaic elements, then array 30 can act as the complete collector system. However if solar elements 22 are reflectors, then a solar receiving element (e.g., solar receiving element 62 as shown in
The key aspects of solar collector 20 defined in this application are the versatility and performance of the system. First, the basic design can be scaled from an array with a surface area of a few square meters to an array having a couple hundred square meters, the only modification being the size of individual components and the number of components used. Second, the invention provides a way to reduce the amount of structural materials required to support solar elements 22. This considerably reduces the weight and cost of the structure. Reducing the weight and cost of the structure to support the solar elements also results in reducing the size and cost of the drive mechanism and auxiliary components needed due to the lower weight and inertia of the system. Third, the invention provides a structure that is inexpensive to ship in disassembled form and that is easy to assemble at the point of installation. Fourth, the structure can be easily mass produced thereby further lowering the cost of the system. Fifth, the invention provides an easy way to change the focal length of the system either during manufacture or at the point of installation. And lastly, the invention provides a system that allows for easy maintenance and replacement of critical components.
The solar collection system defined by the present invention can be extended for use over the complete electromagnetic radiation (EMR) spectra. This may include ultraviolet, optical, infrared, microwaves, radio waves and other astronomic applications. It may also be used to collect EMR from man made sources. Depending on the wavelength of EMR, solar elements 20 may include EMR elements that collect or reflect radiation at any given wavelength. For example, at radio-wave wavelengths wire mesh grids make good reflectors. Solar system 20 works for any application where a large area is required for intercepting and collecting the electromagnetic radiation.
The invention is not limited to the embodiments represented and described above but includes all variants notably those concerning the types of solar elements used to form the solar collector, the manner in which individual solar elements are strengthened, the manner in which individual solar elements are connected and the types of materials used to construct the apparatus. Nothing in the above specification is intended to limit the invention more narrowly than the appended claims. The examples given are intended only to be illustrative rather than exclusive.
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20090107542 A1 | Apr 2009 | US |