This invention refers to a device which provides an improvement in solar energy collection and conservation, in thermal solar collectors. The device is formed by using conventional components, which allows guaranteeing a better efficiency and a reduction in manufacturing cost.
This invention is directly related with flat solar collectors, which are used to absorb solar energy and transferring it to a fluid. Moreover, it is linked with flat vacuum solar collectors which provide vacuum between a collection plate and a glass closure to obtain a better performance.
Since time ago it is known that flat vacuum solar collectors are the most reliable of its kind, due to simplicity in their structure and low operating temperatures. These low operating temperatures do not damage the commercial materials being used in their manufacturing. However, collectors which are able to transfer a higher amount of energy to a fluid have been demanded in recent times, and a number of promising technologies have been achieved.
A reason why flat solar collectors do not reach high temperatures is mainly due to the convection effect. In these collectors, the main energy loss is due to the produced convection since the collecting plate is at a different temperature than the glass plate (collector closure). A number of different methods have been proved with the passage of time to prevent this effect, such as plate panels (hexagonal shape surfaces), by assembling a double glass plate, and creating a vacuum between the collector plate and the glass plate. This last method is the most commonly used, but requires a more rough structure than the conventional flat collector to support the vacuum caused stresses. In order to provide the required structural support to withstand these efforts, the collector structure has been modified, but a device is not yet available to reach the desired temperature without requiring costly, specialized materials and a troublesome manufacturing process.
In order to get an outlet temperature in the collector higher than 200° C. using commercial parts and simple manufacturing processes, the present device has been developed. Said device comprises high transmittance in solar spectrum tubes (TATES) closed in the end sides by a pair of heads attached to small vacuum chambers. The only TATES which are not closed by the vacuum chambers, are those with working fluid inlet and outlet. Within these TATES conducting tubes (TUCS) made of any thermal conducting material are located, attached to collector plates and closed with a selective surface in the solar spectrum to absorb the largest possible amount of energy. These TUCS are arranged over low thermal conduction supports, preferably ceramics, in order to lose the least possible amount of energy by conduction. By means of a vacuum pump coupling, a vacuum is created within the high transmittance in solar spectrum tubes and the vacuum chambers, which allows reaching temperatures higher than 200° C. The present invention is different from previously designed devices due to several factors, most relevant of them disclosed below. The first difference is that flat vacuum solar collectors in the past (U.S. Pat. No. 4,038,965-Lyon, U.S. Pat. No. 4,281,642-Steinberg, U.S. Pat. No. 4,289,113-Whittemore, U.S. Pat. No. 5,653,222-Newman) were designed in such a way that they all have a base, and a glass plate which closes the collector at all. These have a severe technical problem, since stresses created by a pressure difference within the collector and the atmospheric pressure, distort the structure and make it to fail, which causes a loss in vacuum within the collector. Lyon and Whittemore use linear supports which are attached along the collector so that they prevent distortion of the collector containing box. Steinberg designed a complex support which is located within the box. This support is a series of semicircles, which provide support to the glass closure on one side, while providing box support on the other side. Finally, Newman proponed a less complex solution, which uses a glass closure for the top of collector but the bottom thereof is comprised of semicircles, the semicircle peaks serve as a support for the top portion. In present invention the problem of pressure difference is solved by using high transmittance in solar spectrum tubes, which provide a smoothly spread stress distribution between said tubes. Another important problem having the above mentioned collectors is that glass thermal expansion and that from the base is different, which causes vacuum losses. The expansion of one piece depends on both the thermal expansion coefficient and the piece size. This is not a problem under present invention, since the only expansion which produces significant differences is the one occurring along the high transmittance in solar spectrum tubes and the conducting tubes, but because of the collector assembly form, said expansion does not cause any vacuum losses since having enough space for conducting tube differential expansion. Newman proposes in his design that tempered glass is used on top closure and then a series of treatment is provided to improve the glass optical properties, while under present invention commercial tubes showing better optical and thermal properties are used without any need to subject them to any additional treatment.
a is rear view of one of the heads.
b is a top view of one of the heads.
c is a front view of one of the heads.
The present invention represented in
Within each TATES and longitudinally arranged is a conducting tube (TUCS) (9) with a lower diameter than TATE, which transport the working fluid, TUCS are composed of any thermal conducting material, and each TUCS has attached along its length, a collecting plate (8) covered with a selective surface in solar spectrum to absorb the most possible amount of solar energy. These TUCS are arranged on low thermal conduction supports, preferably ceramics (10) to minimize the energy losses by conduction.
Each TATES end is closed by a head (1); the heads are preferably rectangular, having small punctures aligned along the head, this punctures have a larger diameter than TUCS to allow passing them therein. The number of circular punctures coincides with the number of TUCS, and the head side which is attached to TATES is named front side and the opposite one, rear side; being through this side where these vacuum chambers are joined (3), being of an area such that covers the cross-sectional area of 2 TATES. Vacuum chambers cover and are grouping in pairs the head circular punctures, where TUCS (9) are introduced. TUCS are located in parallel and they are joined each other, within the vacuum chamber by 90° or 180° elbows. The only circular punctures which are not covered by vacuum chambers are the first circular puncture or inlet puncture (6) and the last circular puncture or outlet puncture (7) from conducting tubes (TUCS) (9) which carry the working fluid. These are the only two contact points, no matter what the amount of TUCS comprising the solar collector is, with the feature that in this and last circular puncture the thermal expansion coefficient is different from the remaining.
For vacuum control and generation, at least on vacuum generation pump (4), and a pressure level meter (5) are connected to one of the vacuum chambers (3), which allows to generate the vacuum within the TATES and vacuum chambers, that is, in case that the vacuum within the system is lost, it is possible to recover it without requiring a system replacement and allowing additionally to control vacuum levels to keep a determined temperature thus preventing a modification in fluid temperature and flow. Because of that, the vacuum level in turn allows that TUCS reach temperatures higher than 200° C.
It may be noted from
Heads (1) are more detailed shown in
In
One of the most important elements of this invention are the high transmittance in solar spectrum tubes (TATES), which shall be preferably of borosilicate glass, since these tubes show high optical, thermal and mechanical properties beneficial for collector performance. For example a common borosilicate glass tube will transmit more than 92% of the energy received from the sun and would reflect a negligible percentage (a common glass cannot reach these properties unless subjected to several additional treatments after manufacturing). Another important property is that its thermal expansion coefficient is so low that allows a wide material selection for head manufacturing (1). These TATES (2) shall be preferably of an outer diameter higher than 50 mm to adjust internally the conducting tubes (TUCS) with its respective collecting plate, as well as the support means. TATES are an ideal element since their circular cross-sectional surface show a smooth stress distribution in vacuum and therefore a need to add additional supports is nonexistent. Another element is the vacuum chambers (3); which serve as head closures (1), these are preferably built of glass tubes with a depth larger than 5 mm, although the cross section of these chambers may be circular, elliptic and polygonal, provided that fulfills the function of covering with one of their cross-sectional ends two adjacent TUCS. The use of glass is recommended since in this way takes advantage of the joint and elbow collecting surface which connect among them the TUCS. These vacuum chambers (3) may be of regular or borosilicate glass. It is worth to mention that some of these chambers carry a coupling to connect a vacuum pump (4) in the opposite end to the one on contact with the head, which allows to generate an initial vacuum or to recover the vacuum in case that due to any event a loss may exist. It is advisable that in another one of the vacuum chambers (3), preferably in the opposite side of a vacuum chamber (3) with vacuum pump (4), a pressure indicator (5) is installed, with which the existing vacuum level may be measured and the type of leakage if any. Another important feature which may be noticed in
In
In
Collector plates (8) are made of a thermal conducting material (preferably copper). These collector plates (8) shall be of a thickness not larger than 0.2 mm and their length shall be shorter than each TATES (2) on each end depending on the circular slot (11) depth. Their width shall be also a minimum of 95% from TATES (2) diameter, and the maximum dimension of these plates shall be only determined by the collector plate material thermal expansion (8), since in any time these will not touch the TATES (2) because that would cause heat losses by contact. Another important feature of collector plates (8) is that these are coated by a solar spectrum selective surface on both sides. Together with these collector plates (8) the TUCS (9) are located which carry the working fluid. The joint between these components is carried out by using any additive which allows a maximum possible heat transmission, such as silver welding. The TUCS (9) are also coated with a selective surface, preferably black chromium. This selective surface shall have a high solar spectrum monochromatic absorptivity and a low solar spectrum monochromatic emittance to be a candidate for use in a collector. All the thermal conducting material angles of this selective surface are coated since in special cases concentrators may be arranged together to the collector and directing their light beam to the concentrator bottom, since being the TATES (2) bottom would pass the same energy passing in the top portion (more than 92%). TUCS and collector plate assembly stands on support means (10) made of a thermal insulating material (e.g. ceramics) so that the largest possible amount of energy is transferred to the working fluid. These supports (10) may be substituted by designs having a lower contact surface with the TUCS (9) or with the TATES (2). In the vacuum chamber ends (3) is where the TUCS attachment is made. Materials within the vacuum chambers (3) generally form 180° elbows which are also coated with a solar spectrum selective surface, in order to take advantage as much as possible from solar energy.
A flat vacuum solar collector with chamber type heads is possible to operate by fulfilling with all previous disclosure, which may raise the working fluid temperature higher than 200° C. since vacuum prevents that convection is present, then conduction losses are only present. These losses are very small since the contact is with insulating materials. In addition, a 100% of the piping for solar energy absorption may be used since everything is enclosed within containers with high solar spectrum transmittance.
Number | Date | Country | Kind |
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NL/A/2006/000045 | Jul 2006 | MX | national |
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/MX07/00087 | 7/23/2007 | WO | 00 | 9/19/2008 |