DEVICE FOR HEATING WITH SOLAR ENERGY

Abstract: Device for heating with solar energy, which device contains at least one mirror construction (1) which is mounted on a frame (3) in a movable manner and which be directed towards the sun, and at least one collector (4) extending parallel to the mirror construction (1) in order to collect the solar radiation reflected by the mirror construction (1), characterized in that the mirror construction (1) contains a number of almost flat mirror strips (2) extending next to one another in the longitudinal direction of the collector (4) and which are each provided on the frame (3) such that they can rotate around their longitudinal direction, whereas the collector (4) is stationary in relation to the frame (3), whereby the mirror strips (2) are situated in an almost horizontal plane with their axes of rotation, whereby the device contains means (16) to rotate the mirror strips (2) and the mirroring surface of the mirror strips (2) such that the solar rays coming in on said surface can be reflected towards the collector (4).

Description: Device for heating with solar energy. The present invention concerns a device for heating with solar energy, which device contains at least one mirror construction which is mounted on a frame in a moveable manner and which can be directed towards the sun, and at least one collector extending parallel to the mirror construction in order to collect the solar radiation reflected by the mirror construction either directly or via a second mirror construction. In known devices of this kind, the mirror construction is a rotatable, longitudinal mirror with a parabolic section, whereas the collector is a tube coated with a heat-absorbing material situated on the focal line of the mirror. Such a device is also described in Belgian patent No. 888.400. The mirror construction is a large, longitudinal mirror which is bent according to a semi- parabola and it is mounted on a frame such that it can rotate as a whole and reflects the solar radiation by means of a convex mirror erected on its focal line through a slot in an insulated space in which the collector is situated. In all these known devices, the mirror, which is constantly directed towards the sun, has very large dimensions and is for example 30 m long. As it is bent, its construction is relatively complex. Moreover, the large mirror surface can be exposed to a lot of wind, so that it has to be built relatively heavy and so that the device usually cannot be used when there is a lot of wind. Also the frame for this large and relatively heavy mirror must have a very strong and heavy construction. It is clear that the rotatable mounting on the frame of this rather large mirror is not easy either. Heavy hinges are required, and also the means for rotating this relatively heavy mirror, which may be subject to wind load, so as to direct it constantly towards the sun have to be very strong. The result of all this is that these known devices are relatively expensive. The present invention aims a device for heating with solar energy which does not have the above-mentioned and other disadvantages, which is thus relatively economical and whose construction and mounting are relatively simple, without having any negative effect on its efficiency. This aim is reached according to the invention in that the mirror construction contains a number of almost flat mirror strips extending next to one another in the longitudinal direction of the collector and which are each provided on the frame such that they can rotate around their longitudinal direction, whereas the collector is stationary in relation to the frame, whereby the mirror strips are situated in an almost horizontal plane with their axes of rotation, whereby the device contains means to rotate the mirror strips and the mirroring surface of the mirror strips such that the solar rays coming in on said surface can be reflected towards the collector. The first mirror construction can be seen as a segmented parabola or a part thereof whose segments have been flattened and placed in a horizontal plane. Each segment is flat and has a simple construction. It can be made relatively light. It can be rotated rather easily. The first mirror construction as a whole has little height and thus does not catch much wind. Since the movement of the sun is known, the simultaneous movement of all the mirror strips can be programmed and can be carried out automatically. This movement may also be controlled by a system which observes the position of the sun, also called a tracking system. The mirror strips can be directed eastward/westward in the longitudinal direction. In this case they only have to take into account the inclination of the earth in relation to the sun, which changes depending on the season as the earth rotates around the sun. The mirror strips are thus rotated around their longitudinal direction over a total angle of about 46° in one year. Even when the sun is low on a certain day, one mirror strip will not cast any shadows on a neighbouring strip. However, the mirror strips can also be directed northward/southward in the longitudinal direction and follow the movement of the sun during one day, and thus be directed towards the east in the morning and towards the west in the evening . If, in the latter case, the mirror strips are directed with their mirroring surface towards a single collector which is then situated in the middle above the first mirror construction, the angle between the incident solar rays and the rays reflected towards the collector will be larger than 90° for a number of the mirror strips, except when the sun is in its highest position above the mirror construction. The moment at which this angle becomes an acute angle coincides with different positions of the sun for these mirror strips and thus takes place at different points in time. Mirror strips whose above-mentioned angle is larger than 90° make the efficiency of the device decrease. In order to avoid this, the device preferably contains at least three collectors, namely a middle collector and collectors situated eastward and westward respectively at equal distances in relation thereto, whereby the inclinations of the almost flat mirror strips are such in their cross directions that a first series of mirror strips situated between the middle collector and the collector situated to the east thereof reflect towards this latter collector, whereas a second series of mirror strips situated between the middle collector and the collector situated to the west thereof reflect towards the middle collector and, after having rotated over a certain angle when the sun is at its highest point during the day, i.e. in the afternoon, the first series of mirror strips will reflect towards the middle collector and the second series will reflect towards the collector situated to the west thereof. In fact, the mirror construction can be regarded as two segmented, semi-parabolic mirrors which extend parallel to one another and whose segments have been flattened and 5 have been brought in a horizontal plane. The first mirror construction can be further extended with one or several additional series of mirror strips and with an extra collector for every series. The means for rotating the mirror strips can be means to rotate at least a number of the mirror strips, for example all the mirror strips situated between two collectors or all the mirror strips together, simultaneously and to the same extent. The means may then have a wheel, for example a sprocket wheel or a toothed wheel on at least one end of each of the mirror strips, an endless element, for example a chain or toothed belt, working in conjunction with all these wheels, and drive means for driving this element. The collector preferably contains at least one heat- absorbing pipe and at least one reflector, preferably consisting of two parabolic bent mirrors, directed towards the pipe situated in between and which is erected above the pipe like a cap for collecting the solar rays reflected by the mirror construction and for reflecting them to the pipe . This pipe preferably is a double-walled glass tube whose inner wall is coated with a heat-absorbing material on the outside and with a vacuum between both walls. Through this pipe may extend a metal tube, whereas the space between this metal tube and the pipe may be filled with a heat-transferring material such as steel wool. In order to better explain the characteristics of the invention, the following two preferred embodiments of a device for heating with solar energy according to the invention are described as an example only without being limitative in any way, with reference to the accompanying drawings, in which: figure 1 shows a very schematic view in perspective of a first embodiment of the device according to the invention; figure 2 schematically shows a front view of the device from figure 1 ; figure 3 shows a section according to line III-III in figure 1, to a larger scale; figure 4 shows a view in perspective with the collector of the device according to figures 1 to 3 being partially cut out; figure 5 schematically shows a longitudinal section of the collector from figure 4 ; figure 6 schematically shows a front view analogous to that in figure 2, but with reference to another embodiment of the invention; figures 7, 8 and 9 represent schematic front views analogous to those in figure 6, but with reference to two other situations of the device; figure 10 shows the detail which is indicated by F10 in figure 5 to a larger scale; figure 11 shows a section according to line XI-XI in figure 10. In its simplest embodiment, as represented in figures 1 and 2, the device for heating with solar energy according to the invention mainly consists of a mirror construction 1 which is formed of a number of flat mirror strips 2 situated next to one another which are mounted on a frame 3 in a rotating manner according to their longitudinal 7 direction or parallel to their longitudinal axis, and a collector 4 erected on top of it which is fixed stationary on the above-mentioned frame 3. The mirror strips 2 are flat and parallel to one another with their longitudinal direction. They are for example made of glass with a mirroring coat on the top side and preferably a coat which can resist sandstorms on the bottom side, such as a coat on the basis of rubber or plastic. They have a width of for example almost 50 cm, a length of about 3 m and a thickness of 3 mm. The mirror construction 1 is in fact a longitudinal parabolic mirror which has been divided into segments and whose segments have been flattened and put down in the same horizontal plane. Instead of rotating the parabola as a function of the position of the sun, one only has to make the segments rotate, i.e. the mirror strips 2, which is simpler. To this end, every mirror strip 2 can rotate. As is represented in detail in figure 2, every mirror strip 2 is hooked on a frame 6 made of aluminium profiles by means of clamps 5, which frame is in turn fixed on a tube 8 by means of clamping brackets 7, which tube is mounted in a bearing 9 every three metres which is fixed on a horizontal cross-latch 10 which is part of the frame 3. All these cross-latches 10 are fixed with their ends to the rest of the frame 3, namely to standing profiles 11 or 12, at a height of about 1.5 m above the ground, but adjustable in height. Between two profiles 12 in a longitudinal side are erected three shorter profiles 11, for example one shorter profile 11 every three metres. The profiles 11 extend up to a distance above the mirror construction 1 and their top ends are connected to one another and to the profiles 12 by means of longitudinal profiles 13 in the longitudinal sides. The standing profiles 12 are considerably higher than the profiles 11 and their top ends are connected to one another by means of horizontal cross- sectional profiles 14. The standing profiles 11 and 12 are fixed to a concrete foundation 15. Over the two longitudinal profiles 13 may possibly ride a trolley which is not represented in the figures for maintaining, washing or repairing the mirror construction 1. Means 16 are provided to rotate the mirror strips 2 as a function of the position of the sun, either during the day if the mirror strips are directed with their longitudinal direction northward/southward, or spread over a year if they are directed with their longitudinal direction eastward/westward. These means 16, which are only represented in figure 2 for clarity's sake, contain a sprocket wheel 17 on one end of every tube 8 which is connected to a sprocket wheel 19 via a chain 18 which is driven by a drive consisting of a stepping motor 20. For clarity's sake, only the outer stepping motors 20 are represented. These means 16 further contain an electronic control 21 which controls this stepping motor 20 as a function of the position of the sun, such that the mirror strips 2 can follow the sun. In principle, the length of the device in the longitudinal direction of the mirror strips 2 is unlimited, and this length may amount to one kilometre. It is clear that the mirror strips 2 erected in the north/south direction must have different mutual inclinations for each position of the sun in their cross direction in order to reflect the collected solar rays to the only collector 4 which is hung in the middle above the mirror construction 1 on cross-sectional profiles 14. Figure 2 schematically represents the position of the mirror strips 2 at the time the sun is at its highest point. For a number of the mirror strips 2, the direction of the incident solar rays and the axis of a number of reflected beams are represented, and also the bisectors standing at right angles on the mirroring surface of the mirror strip 2 between the above-mentioned devices are represented. According to a variant, the chain 18 extends around all the sprocket wheels 17 and the means 16 only have a single stepping motor 20 which drives all the sprocket wheels 17 via a sprocket wheel 19 and the chain 18, and thus rotates all the mirror strips 2 simultaneously and to the same extent . This variant is appropriate when the mirror strips 2 are directed with their longitudinal direction 10 eastward/westward. They all have to be directed in the same direction at any time, and thus they can all be simultaneously directed to the same extent. The collector 4 is situated at a height above the mirror construction 1 which is for example half of the width of the mirror construction, for example at a height of twelve metres. However, the height can also be less and amount to for example six metres. This collector 4 extends in the longitudinal direction of the mirror strips 2 above the middle of the mirror construction 1. As is represented in detail in figures 4 and 5, this collector 4 contains a metal, preferably a steel tube 22 of for example 6 inches (about 15 cm) long which is surrounded by double-walled glass tubes 23-24. As opposed to steel tubes, glass tubes are not permeable to hydrogen, they are less expensive and they can have a smaller diameter. The outer tube-shaped wall 23 of the tubes 23-24 is translucent, but the inner tube-shaped wall 24 is coated with a black, heat-absorbing layer on the outside which has for example been sputtered onto it . On the ends, the walls 23 and 24 are closed, and there is a vacuum between these walls 23 and 24 which are for example situated at a distance of about 1 mm from one another. This double-walled tube 23-24 is made of heat-resistant glass, for example glass which is known under the 11 brandname Pyrex. The inner, black wall 24 can be heated up to temperatures of 300 to 500°C. The outer wall 23, however, remains relatively cold. This tube 23-24 is up to 4 metres long, and in order to make it possible for the inner wall 24 to expand, expansion bellows 25 are provided at one end of the outer wall 23, preferably made of tempered glass which has been fused to the rest of the glass wall 23. In order to prevent the inner wall 24 from buckling when it exerts some force on the expansion bellows 25 as a result of the expansion, glass rings 26 are clasped around said inner wall 24 , for example by providing them over the wall 24 when they are hot and by making them shrink by cooling them, which make contact with the outer wall 23 only locally so as to limit the heat transfer. The space between the inner wall 24 and the steel pipe 22, which has an atmospheric pressure, is filled with a medium 27 which transfers heat, for example steel wool surrounded by a thin aluminium sheet having a thickness of for example 0.3 mm, which is closely connected to the tube 22 and the wall 24. Moreover, the double-walled tube 23-24 rests on the steel tube 22 through the agency of said medium 27. The tube 22 extends over the entire length of the mirror strips 2 , but it can also extent over several series of 12 mirror strips 2 or mirror constructions 1 and even have a length of 1 kilometre. The double-walled tube 23-24, however, only has a length of about 3 m, and several tubes 23-24 are provided one after the other around the steel tube 22 in the collector 4. On the ends of the device and between two successive double-walled glass tubes 23-24, the steel tube 22 is suspended to a trolley 29 by means of a suspension 28 rolling over a I-profile 30 of the frame 3, as is schematically represented in figure 5, and into more detail in figures 10 and 11. This I-profile 30, which extends over the entire length of the collector 4, but which is provided with an expansion joint 31 at regular distances, is suspended to horizontal cross-sectional profiles 14. The trolley 29 is a U-profile whose two legs carry two small wheels 32 on their sides turned to one another. As is represented in figure 10, the front and rear wheels 32 are not placed on one and the same axis, but they are shifted in relation to one another in the driving direction, such that only one wheel 32 at a time rides over an expansion joint 31 while the trolley 29 is still resting with three wheels 32 on the I-profile 30. Thus, the trolley 29 is prevented from swinging as it rides over an expansion joint 31. As is represented in detail in figures 10 and 11, the suspension 28 may consist of a first bar 33 which is screwed in a bush 34 which is welded on the steel tube 22 13 and which is surrounded by insulating material 35 between the ends of two neighbouring tubes 23-24 on the one hand, and which is screwed in a sleeve 36 on the other hand, and of a second bar 37 which is welded onto the trolley 29 and which is also screwed in the above-mentioned sleeve 36, such that, as the sleeve 36 turns, the bars 33 and 37 are drawn towards one another or are moved away from one another. The screw thread is directed in one and the same direction on both ends of the bar 33, but the screw threads on both ends screwed in the sleeve 36 are directed in the opposite sense. The collector 4 further contains a number of reflectors 38 which each consist of two longitudinal mirrors which are fixed to one another in the length above the glass tube 23-24 and which form a cap over the heat-absorbing pipe formed by the wall 24. The cross section of each mirror is a part, for example half, of a parabola. The reflectors 38 are suspended on a cross -sectional profile 40 by means of bars 39 which is fixed to the bottom side of the I-profile 30. Each reflector 38 is directed with its mirroring side on this wall 24 which is practically situated on the focal line of the two parabolic halves of this reflector 38. The reflector 38 has a length which is almost equal to the length of a double-walled glass tube 23-24, and the collector 4 has several of those reflectors 38 which are situated in line above the mirror construction 1. The opening at the bottom of the reflector 38 is calculated such that the solar rays which are reflected 14 by all the mirror strips 2 of the mirror construction 1 fall in it and are thus reflected towards the inner wall 24 of the glass tube 23-24, insofar as they did not fall directly on this wall 24. If the height of the collector 4 above the mirror construction 1 is about half of the width of the latter, this opening is such that it can collect an angle of rays of 90°, and it is for example about 72 cm. When the collector 4 is positioned lower, the angle can be larger, for example up to 135°. For practical reasons, the length of the mirror strips 2 is limited to for example 3 m, but several mirror constructions 1 can be put one after the other in the longitudinal direction, whereby the tubes 8 of a number of mirror strips 2 or even all the mirror strips 2 situated in line can form an uninterrupted whole, so that a single stepping motor 20 can simultaneously rotate a number of these mirror strips 2 which are coupled to one another, or all of them at once. Also the frame 3 and among others the longitudinal profiles 13 and the I-profile 30, abstracting from the expansion joints 31, may continue uninterruptedly over several series of mirror constructions 1. This also goes for the collector 4 suspended on the I- profile 30 which may have a length of up to one kilometre. Moreover, several individual mirror constructions or mirror constructions situated one after the other in the longitudinal direction may also be situated next to one 15 another in the cross direction. By making use of flat mirror strips 2 instead of a single parabolic mirror, the construction is relatively simple. Its maintenance is relatively easy, especially thanks to a trolley riding over the longitudinal profiles 13. In case of for example a sandstorm, the mirror strips can be rotated against the direction of the wind with their protected back side. The device has a large efficiency. Only for a very short period in the early morning or late in the evening, the mirror strips may cast a shadow on a neighbouring mirror strip. During the rest of the day, little solar energy is lost due to shadows . The device can be made even simpler if all the mirror strips 2 of a mirror construction 1 can be rotated all together and to the same extent as they follow the sun. Figures 6 to 9 represent an embodiment where this is the case and in which the mirror strips 2 are directed with their longitudinal direction in the north/south direction. This embodiment mainly differs from the above-described embodiment in that, above the mirror-construction 1, three above-described collectors 4 are suspended to a I- profile 30, in that the mirror strips 2 have a different inclination in their cross direction and in that they are all driven by one and the same stepping motor 20 as in the above-mentioned variant of the embodiment according to figures 1 to 5. 16 One of the three collectors 4 is erected in the middle, as in the above-mentioned embodiment, whereas the other two are situated above the longitudinal edges, to the east and to the west respectively of this middle collector 4. The mirror strips 2 are inclined such that they coincide with two longitudinal semi-parabolas which have been divided into segments and whereby the segments have been flattened and lowered in one and the same horizontal plane, and whereby the two semi-parabolas are practically parallel to one another. The mirror strips 2 which coincide with the one se i- parabola reflect towards one collector 4, whereas those coinciding with the other semi-parabola reflect towards another collector 4, whereby, when the sun has reached its highest point, all the mirror strips 2 are rotated together over an angle, so that they each reflect towards another collector 4. This angle is 22.5° when the width of the mirror construction 1 is equal to twice the height at which the collectors 4 are situated, and the distance between the collectors 4 is thus equal to this height. In figure 6, the mirror strips 2 are represented at the time the sun stands on the horizon in the east. The first series or half of the mirror strips 2 situated on the side of the sun reflect the collected solar rays towards the collector 4 situated eastward. The other series or half of the mirror strips 2 reflect towards the middle collector 4. It is clear that in the farthest position represented in figure 6, the reflection is rather theoretical, since the 17 mirror strips are situated in each other's shadow when the position of the sun is this low. The mirror strips 2 are all continuously rotated by the means 16, but they keep reflecting towards the above- mentioned collectors 4 as the sun rises until they take the position in which they are represented in figure 7, when the sun is at its highest point. Before noon, they are rotated over 45° in total. At noon, i.e. when the sun has reached its highest point, all mirror strips 2 are rotated, in the given example over 22.5°, into the position represented in figure 8. The mirror strips 2 of the first series now reflect towards the middle collector 4 and the other mirror strips 2 towards the collector 4 situated westward. In the course of the afternoon, all the mirror strips 2 are further simultaneously rotated by the means 16 over a total angle of 45° until the sun goes down in the west. The mirror strips 2 are then situated in the position represented in figure 9 and thus form the mirrored image of the situation before the rotation. At any time, the angle between the incident solar rays and the solar rays reflected to a collector 4, which is represented for some mirror strips 2 in figures 6 to 9 , is smaller than 90°, so that the efficiency of the device is excellent. As all the mirror strips 2 are always rotated together and to the same extent, the means 16 have a simple construction and the tracking of the sun is rather easy. 18 It is clear that on both sides of the above-described mirror construction 1, additional mirror strips 2 can be provided as is represented by means of a dashed line in figures 6 to 9, in particular one or several series of mirror strips 2 which coincide with a segmented semi- parabola, but for every series also one additional collector 4. The additional series of mirror strips 2 situated eastward will reflect towards the collector 4 of the above-described mirror construction 1 situated the most eastward in the afternoon. In an analogous manner, an additional series situated westward will reflect towards the collector 4 of the above-described mirror construction 1 situated the most westward before noon. As the mirror construction is divided in mirror strips 2, it is possible, especially when these mirror strips 2 are directed eastward/westward, to put one or several mirror strips 2 entirely or partly off-duty, for example by tilting them separately so that they are no longer directed towards the sun, so as to thus adjust the total amount of solar energy which is collected by the device. The present invention is by no means restricted to the embodiments described above and represented in the accompanying drawings; on the contrary, such a device for heating with solar energy can be made in all sorts of variants while still remaining within the scope of the invention.

Claims: 19 Claims . 1. Device for heating with solar energy, which device contains at least one mirror construction (1) which is mounted on a frame (3) in a moveable manner and which can be directed towards the sun, and at least one collector (4) extending parallel to the mirror construction (1) in order to collect the solar radiation reflected by the mirror construction (1) , characterized in that the mirror construction (1) contains a number of almost flat mirror strips (2) extending next to one another in the longitudinal direction of the collector (4) and which are each provided on the .frame (3) such that they can rotate around their longitudinal direction, whereas the collector (4) is stationary in relation to the frame (3) , whereby the mirror strips (2) are situated in an almost horizontal plane with their axes of rotation, whereby the device contains means (16) to rotate the mirror strips (2) and the mirroring surface of the mirror strips (2) such that the solar rays coming in on said surface can be reflected towards the collector (4) . 2. Device according to claim 1, characterized in that the mirror construction (1) is a segmented parabola or a part thereof whose segments have been flattened and placed in a horizontal field. 3. Device according to claim 1, characterized in that the mirror strips (2) are directed with their longitudinal direction northward/southward, and in that the device contains at least three collectors (4), namely a middle collector (4) and a collector (4) situated eastward and 20 westward respectively at equal distances in relation thereto, whereby the inclinations of the almost flat mirror strips (2) are such in their cross directions that a first series of mirror strips (2) situated between the middle collector (4) and the collector (4) situated to the east thereof reflect towards this latter collector (4) , whereas a second series of mirror strips (2) situated between the middle collector (4) and the collector (4) situated to the west thereof reflect towards the middle collector (4) and, after having rotated over a certain angle when the sun is at its highest point during the day, i.e. in the afternoon, the first series of mirror strips (2) will reflect towards the middle collector (4) and the second series will reflect towards the collector (4) situated to the west thereof . 4. Device according to claim 3 , characterized in that the mirror construction (1) consists of two segmented, semi- parabolic mirrors which extend parallel to one another and whose segments have been flattened and have been placed in a horizontal plane. 5. Device according to claim 3 or 4 , characterized in that the mirror construction (1) is further extended with at least one additional series of mirror strips (2) and with an extra collector (4) per series. 6. Device according to any of the preceding claims, characterized in that the means (16) to rotate the mirror strips (2) are means to rotate at least a number of the mirror strips (2) or all the mirror strips (2) together, simultaneously and to the same extent. 21 7. Device according to claims 3 and 6, characterized in that the means (16) to rotate the mirror strips (2) are means to rotate at least all the mirror strips (2) which are situated between two collectors (4) . 8. Device according to claim 6 or 7 , characterized in that the means (16) to rotate at least a number of mirror strips (2) simultaneously have a wheel, for example a sprocket wheel (17) or a toothed wheel on at least one end of each of these mirror strips (2) , an endless element, for example a chain (18) or toothed belt, working in conjunction with all these wheels, and drive means (20) for driving this element. 9. Device according to any of the preceding claims, characterized in that the collector (4) contains at least one heat-absorbing tube (23-24) and at least one reflector (36) , directed towards the tube (23-24) situated in between and which is erected above the tube (23-24) like a cap for collecting the solar rays reflected by the mirror construction (1) and for reflecting them to the tube (23-24) . 10. Device according to claim 9, characterized in that the reflector (38) consists of two parabolic bent mirrors . 11. Device according to claim 9 or 10, characterized in that the tube (23-24) is a double-walled glass tube whose inner tube-shaped wall (24) is coated with a heat- absorbing material on the outside and whose outer tube- shaped wall is translucent, and with a vacuum between both walls (23 and 24) . 22 12. Device according to claim 13 , characterized in that a metal tube' (22) extends through the tube (23-24), whereas the space between this metal tube (22) and the tube (23-24) is filled with a heat-transferring medium (27) such as steel wool. 13. Device according to claim 11 or 12, characterized in that expansion bellows (25) are provided in the inner wall (24) . 14. Device according to claim 13, characterized in that rings (26) are provided between the two walls (23 and 24) of the tube which preferably make contact with the outer wall (23) only locally. 15. Device according to any of claims 13 to 14, characterized in that above the mirror construction (1) , several tubes (23-24) are provided one after the other around a single metal tube (22) , and in that these tubes (23-24) are carried by this metal tube (22) . 16. Device according to any of the preceding claims, characterized in that the collector (4) contains a metal tube (22) for fluid to be heated, suspended at regular distances on a longitudinal profile (30) which is part of the frame (3) by means of a trolley (29) which can ride over this longitudinal profile. 17. Device according to claim 16, characterized in that the longitudinal profile (30) is provided with expansion joints (31) and in that the trolley (29) contains two front and two back wheels (32) which are not placed on the same axis, but which are shifted in relation to one another in the driving direction. 23 18. Device according to claim 16 or 17, characterized in that the metal tube (30) is suspended by means of a suspension containing two bars (33 and 37) which are screwed together in a sleeve (36) , so that they can be adjusted in relation to one another by turning the sleeve.

Inventors: SUREDA MICHEL, VEN LIVIEN DOMIEN, SUREDA, MICHEL, VEN, LIVIEN, DOMIEN
Applicants: SUREDA MICHEL, SURIA HOLDINGS SARL, VEN LIVIEN DOMIEN, SUREDA, MICHEL, SURIA HOLDINGS, SOCIETE A RESPONSABILITE LIMITEE, VEN, LIVIEN, DOMIEN
Application year: 1999
Main classification: F24J2
IPC codes: F24J2