Patent Grant
9404676
The present invention relates to a vacuum solar thermal panel with pipe housing for a solar absorber pipe.
As it is well known, vacuum solar thermal panels comprise at least a flat vacuum tight envelope with a glass plate transparent to visible solar radiation. Inside the vacuum envelope are disposed heat absorbers and a pipe entering and exiting the envelope connected to the heat absorbers.
The solar radiation thus enters the vacuum envelope through the glass plate, is absorbed by the heat absorbers and converted into heat. The converted heat is transferred to the pipe and to a heat transfer fluid flowing in the pipe.
Vacuum is kept inside the envelope enclosing the heat absorbers and part of the pipe connected to them, in order to prevent heat from escaping to the external environment by means of convection.
A vacuum solar thermal panel of the known type is described for instance in the PCT application published under No. WO 2010/003653 in the name of the same Applicant.
It is known that vacuum solar thermal panels require a support structure for the glass plate which is also used for firmly holding in place the solar absorber.
It is also known that the efficiency of a vacuum solar thermal panel is limited by thermal losses and that, when the internal pressure is low enough to suppress convection, only conduction and radiation losses remain. Conduction losses are thus caused by the inevitable contact points between the solar absorber pipe and its support frame.
According to the prior art solutions, conduction losses are limited by reducing the number of contact points between the solar absorber pipe and its support frame and by providing long thermal paths from these points to the vacuum envelope, which is at ambient temperature during panel operation.
Existing thermal panels essentially comprise a frame equipped with spacers, which cross one another and support the glass plate against a metallic panel bottom. The network-like path defined by the spacers creates a plurality of areas wherein the heat absorbers are housed.
Typical low conduction loss pipe housings, being normally shaped like a fork with protruding edges to accommodate the pipe, are used in vacuum solar thermal panels.
A known type of this low conduction loss pipe housing is described for instance in the PCT application published under No. WO 2010/023074 in the name of the same Applicant. According to this application, as shown in its
In this way, the pipe (and therefore the solar absorber) is centred horizontally into the structure and will not be able to move apart. The major drawback of this latter solution is the freedom of vertical movement left to the pipe-absorber structure.
It is known that vacuum solar thermal panels can reach very high temperatures in case of stagnation, i.e. when panel is exposed to maximum solar irradiance and the heat transfer fluid does not flow inside the pipe. Therefore the solar absorber, composed by a selective metal sheet welded to a metal pipe, tends to elongate and/or bend the pipe.
In particular, a pipe of copper, typically 1.5 meters long and welded to a selective copper sheet of same length as usually employed in solar thermal panels, when heated at a temperature of 400° C. will expand by 10 mm.
The known solutions, while allowing for pipe elongation, do not allow for pipe retention in the vertical direction and this may cause the solar absorber to eventually contact the glass plate adding additional conduction losses. This conduction path from the solar absorber to the ambient temperature will dramatically reduce the efficiency of the solar thermal panel
This is of particular relevance in the case of vacuum solar thermal panel of reduced thickness, where the distance between the selective metal sheet of the solar absorber and the facing glass plate is less than 10 mm.
The technical problem underlying the present invention is that of providing a vacuum solar thermal panel with low conduction loss pipe housing providing self-retention of the pipe in the vertical direction, in this way overcoming the limits which still affect the housings realised according to the prior art.
The solution idea underlying the present invention is that of providing a retention mechanism which prevents a pipe from moving in the vertical direction when housed in a low conduction loss pipe housing, while allowing its thermal expansion in the longitudinal direction and an easy insertion or mounting of the pipe itself during the assembly or manufacturing of the vacuum solar thermal panel.
On the basis of such solution idea the technical problem is solved by a vacuum solar thermal panel with pipe housing for a solar absorber pipe of the type comprising at least a base portion and a retention element for said pipe, characterized in that said retention element is in the form of a fork and has an elastic behaviour when forced by said pipe.
This retention element comprises a first and a second tine both protruding from said base portion and being mirrored one another, and defining an open housing space therebetween having different widths starting from said base portion up to an opening inlet for said pipe, said open housing space where said pipe is housed being wider than a diameter of said pipe.
Moreover, the retention element comprises a first portion having an increasing opening width from a first opening width to a second opening width that is greater than said first opening width, and a second portion having a decreasing opening width from said second opening width to a third opening width.
The tines of said retention element comprise retaining edges at their tips and define said opening inlet which has a fourth opening width that is smaller than said second opening width.
Advantageously, the second opening width has a value in range of 110%-150% of a diameter of said pipe.
The fourth opening width has a value in range of 90-97% of the diameter of said pipe.
Advantageously, the retention element is made of stainless steel.
The base portion and the retention element with its tines have a same and substantially constant thickness. In particular, they are realized by moulding or by sheet cutting.
The thickness of the base portion and of the tines is substantially constant, being realized by moulding or by sheet cutting.
Moreover, advantageously according to the invention, the vacuum solar thermal panel with pipe housing further comprises spacers disposed in a transverse direction with respect to the base portions of the retention elements and provided with uprights support elements which abut against the glass plate of the vacuum solar thermal panel.
Furthermore, the vacuum solar thermal panel with pipe housing further comprises a continuous solar absorber provided with holes for allowing the uprights support elements of the spacers to cross the continuous solar absorber and abut against the glass plate of the vacuum solar thermal panel.
The characteristics and advantages of the vacuum solar thermal panel with pipe housing according to the invention will be apparent from the following description.
In the drawings:
With reference to such figures, and in particular to
More in particular, the pipe housing 1 comprises a base portion 2 and at least a retention element 3, in the form of a fork.
Advantageously according to an embodiment of the invention, the retention element 3 comprises a first tine 4a and a second tine 4b both protruding from the base portion 2 and being mirrored one another, and defining an open housing space 5 therebetween having different widths starting from the base portion 2 up to an opening inlet 6. The open housing space 5 will properly house a pipe 10 of the vacuum solar thermal panel comprising the pipe housing 1.
In particular, the tines 4a and 4b are substantially C shaped and the retention element 3 thus comprises a first portion A having an increasing opening width from a first opening width W1 to a second opening width W2, being greater than the first opening width W1, and a second portion B having a decreasing opening width from the second opening width W2 to a third opening width W3, preferably equal to the first opening width W1. Advantageously according to an embodiment of the invention, the tines of the retention element 3 comprise retaining edges 7 at their tips, thus defining the opening inlet 6 which has a fourth opening width W4, which is smaller than the second opening width W2.
For instance, for a pipe having an external diameter equal to 10 mm, the first opening width W1 and the third opening width W3 may be 11 mm, the second opening width W2 may be 14.5 mm and the fourth opening width W4 may be 9.5 mm. In this way, the retention element 3 provides for a self-retention of the pipe being housed into it, in particular in the vertical direction considering the local reference system of
In particular, the second opening width W2 is bigger than the pipe diameter while the fourth opening width W4 is smaller than the pipe diameter. Suitable values for the second opening width W2 are among 110-150% of the pipe diameter, while suitable values for the fourth opening width W4 are among 90-97% of the pipe diameter.
In a preferred embodiment, the retention element 3 is made of stainless steel and has a thickness of 2 mm having both elastic behaviour and strength to insert and then retain the pipe.
The mechanism of self-retention is enabled by the elastic behaviour of retention element 3 in the form of a fork, having appropriate thicknesses of its tines, 4a and 4b, and the two retaining edges 7 at its tip. In particular, the thicknesses of the tines, 4a and 4b, of the 3 should be chosen in such a way that the retention element 3 shows an elastic behaviour when forced by a solar absorber pipe 10 as shown in
More in particular, once the solar absorber pipe 10 is pressed against the retention element 3 in correspondence with its opening inlet 6, it widens because of it elasticity to let the pipe 10 go inside the open housing space 5. Then it closes back to its original width preventing the pipe 10 to move upward by means of the retaining edges 7 at its tip, as shown in
Moreover, advantageously according to the invention, the spacers 9 comprises uprights support elements 8 which abut against the glass plate of the vacuum solar thermal panel, traversing the selective metal sheet of the solar absorber provided with suitable holes.
It is to be remarked that the pipe housing 1 of the vacuum solar thermal panel according to the invention avoids the risk of a vertical movement of the pipe and then of the solar absorber associate to the pipe 10 while allowing an easy insertion or mounting of the pipe itself during the assembly or manufacturing of the vacuum solar thermal panel.
In fact, the tines 4a and 4b of the retention element 3 provide a self-retention of the solar absorber pipe in the vertical direction. However, it should be underlined that the retention element 3 has a long thermal path because the housing space 5 where the pipe 10 is accommodated is wider than the pipe diameter and the pipe can thus expand and move freely in the longitudinal direction within the retention element 3 without being allowed move upward or downward thanks to the retaining edges 7.
Moreover, the pipe housing 1 of the vacuum solar thermal panel according to the invention, comprising the spacers 9 and the uprights support elements 8 traversing the solar absorber 11 provided with suitable holes 8A, allows to further elongate the thermal path between the solar absorber and the glass plate, as well to use a continuous solar absorber 11.
In fact, the continuous solar absorber 11 of the vacuum solar thermal panel according to the present invention has an increased active area than the solar absorbers of the known solutions, for instance the one described in the PCT application published under No. WO 2009/149753, which comprises a plurality of absorbing elements, each connected to a cooling pipe, the longitudinal spacers inside the solar panel having their whole upper edge in contact with the glass plate. In particular, the spacers according to this known solution can shade part of the absorbing elements reducing their respective active area.
On the contrary, advantageously according to the present invention, only small holes 8A for the uprights support elements 8 of the spacers 9 are to be provided in a single continuous solar absorber 11 thus maximising its surface as well as minimising any shading caused by the spacers 9.
In this way, a vacuum solar thermal panel with a low conduction loss pipe housing, which allows for pipe self-retention in the vertical direction, is obtained.
Obviously, a technician of the field, aiming at meeting incidental and specific needs, will bring several modifications to the above described vacuum solar thermal panel with pipe housing, all within the scope of protection of the invention as defined by the following claims.
| Number | Date | Country | Kind |
|---|---|---|---|
| 10197369 | Dec 2010 | EP | regional |
| Number | Name | Date | Kind |
|---|---|---|---|
| 1334545 | Londelius, Jr. | Mar 1920 | A |
| 2038912 | Summers | Apr 1936 | A |
| 2819858 | Mittendorf | Jan 1958 | A |
| 2896887 | Beltz | Jul 1959 | A |
| 3233852 | Azar | Feb 1966 | A |
| 3627300 | Caveney et al. | Dec 1971 | A |
| 3924676 | Bennett | Dec 1975 | A |
| 3952725 | Edmondson | Apr 1976 | A |
| 3961619 | Estes et al. | Jun 1976 | A |
| 4080957 | Bennett | Mar 1978 | A |
| 4122829 | Lowe et al. | Oct 1978 | A |
| 4131258 | Okuda et al. | Dec 1978 | A |
| 4164935 | Marles et al. | Aug 1979 | A |
| 4164975 | Bottum | Aug 1979 | A |
| 4213640 | Miles | Jul 1980 | A |
| 4289113 | Whittemore | Sep 1981 | A |
| 4332241 | Dalstein et al. | Jun 1982 | A |
| 4338994 | Hewing et al. | Jul 1982 | A |
| 4577435 | Springer et al. | Mar 1986 | A |
| 4616486 | Ohashi | Oct 1986 | A |
| 4657069 | Easton | Apr 1987 | A |
| 4681288 | Nakamura | Jul 1987 | A |
| D292554 | Yagi | Nov 1987 | S |
| D293205 | Nakano | Dec 1987 | S |
| D293207 | Nakano | Dec 1987 | S |
| 4709556 | Hupfer | Dec 1987 | A |
| D302938 | Fujioka | Aug 1989 | S |
| 4876810 | Piana et al. | Oct 1989 | A |
| 4881521 | Kellner | Nov 1989 | A |
| 5074282 | Reed | Dec 1991 | A |
| 5327737 | Eggemar | Jul 1994 | A |
| 5454428 | Pickard et al. | Oct 1995 | A |
| 5467948 | Gillespie | Nov 1995 | A |
| 5588857 | Feldmeier et al. | Dec 1996 | A |
| 5743330 | Bilotta et al. | Apr 1998 | A |
| 6216987 | Fukuo | Apr 2001 | B1 |
| 6557317 | Sorkin | May 2003 | B2 |
| 6955168 | Nakauchi | Oct 2005 | B2 |
| 6969832 | Daughtry, Sr. | Nov 2005 | B1 |
| 7364321 | Chen et al. | Apr 2008 | B2 |
| 7523898 | Barry et al. | Apr 2009 | B1 |
| 7556225 | Riedy et al. | Jul 2009 | B2 |
| 7810491 | Benvenuti | Oct 2010 | B2 |
| D654600 | Devine et al. | Feb 2012 | S |
| 8499823 | Shaw et al. | Aug 2013 | B1 |
| 20050028966 | Pickard | Feb 2005 | A1 |
| 20050173597 | Farrell et al. | Aug 2005 | A1 |
| 20070039611 | Benvenuti | Feb 2007 | A1 |
| 20080011289 | Sichanugrist et al. | Jan 2008 | A1 |
| 20100108825 | Brock | May 2010 | A1 |
| 20110146667 | Benvenuti | Jun 2011 | A1 |
| Number | Date | Country |
|---|---|---|
| 7834 | Sep 2005 | AT |
| 4430106 | Feb 1996 | DE |
| EP 1538403 | Jun 2005 | DE |
| 1496320 | Jan 2005 | EP |
| 2211079 | Jul 2010 | EP |
| 2009149753 | Dec 2009 | WO |
| Number | Date | Country | |
|---|---|---|---|
| 20120186578 A1 | Jul 2012 | US |
