CHARACTERIZATION DEVICE, SYSTEM AND METHOD FOR CHARACTERIZING REFLECTIVE ELEMENTS FROM THE LIGHT BEAMS REFLECTED THEREIN

Abstract

A characterization device, system, and method for characterizing reflective elements from the light beams reflected in it. The device has two variable-gain detectors on a common structure, which can be portable or fixed, and for capturing light beams reflected by a reflective element, and from at least one processor characterizing the quality of the reflected light beams and evaluating the quality of the reflective element from its reflective capacity. Each detector has a lens for increasing the signal-to-noise ratio of the reflected beam or beams, a light sensor on which the beam or beams captured by the lens are focused, an automatic gain selection system associated with the optical sensor, and a data communication device associated with the device itself. A characterization system and a characterization method for characterizing reflective elements from the quality of the light beams reflected in at least one reflective element or heliostat.

Claims

1.-16. (canceled)

17. Characterization device for characterizing the shape and deformations of the surface of reflective elements (30) through the combination of light beams (40) reflected by the surface and images of the surface, characterized in that it comprises at least two variable-gain detectors (50), for capturing the reflected beams (40), and at least one pin-hole camera (60), for taking images of the reflective elements (30), located on a structure (10) for receiving the light beam reflected by at least one reflective element (30), so that by said combination of the reflected beams (40) with the images of the surface the orientation of all the points of said surface and the deviation with respect to the design shape of said surface is determined, and each detector (50) comprising: a lens (51), with an aperture angle (56) smaller than 15°, for increasing the signal-to-noise ratio of the beam (40), at least one optical sensor (52) on which the beam (40) captured by the lens (51) is focused, an automatic gain selection system (53), associated with the optical sensor (52), with a data capture and processing unit (55), to select or adjust the gain of the detector (50), in an automated manner, as a result of the processing unit associated with each detector (50) and therefore with each sensor (52), with respect to the incident radiation reflected by the reflective element (30), and data communication means associated with the detector (50).

18. The device according to claim 17, characterized in that the structure (10) comprises the detectors (50) aligned forming an array (11).

19. The device according to claim 17, characterized in that the structure (10) comprises the vertically aligned detectors (50).

20. The device according to claim 17, characterized in that the structure (10) comprises the horizontally aligned detectors (50).

21. The device according to claim 17, characterized in that the automatic gain selection system (53) comprises variable-gain electronics for selecting the gain of a sensor (52) most suited to the light intensity of the beam (40) received by said sensor (52).

22. The device according to claim 17, characterized in that the automatic gain selection system (53) comprises fixed-gain electronics for selecting a sensor (52), from at least two sensors (52), with the gain most suited to the light intensity of the beam (40) received by the sensors (52).

23. The device according to claim 17, characterized in that the automatic gain selection system (53) comprises logarithmic-gain electronics.

24. The device according to claim 21, characterized in that the optical sensor (52) is a silicon photodiode and/or a thermopile.

25. The device according to claim 22, characterized in that the optical sensors (52) are at least two photodiodes and/or at least two thermopiles and/or at least one photodiode and at least one thermopile.

26. The device according to claim 17, characterized in that it comprises an automatic detector orientation system, such that either the structure support of the device moves, preferably rotating and changing the orientation of all the detectors at the same time, or each detector moves or rotates independently with respect to the structure of the device.

27. A characterization system for characterizing the shape of the reflective elements (30), characterized in that it comprises: At least one device according to claim 17, and At least one reflective element (30) whose reflected light is incident on the detectors (50) of the device with a given angle of view.

28. The system according to claim 27, characterized in that it comprises a processor and calculation means (12) for determining the complete reflector shape through the image reflected by the reflective element which is generated by means of the scanning of the aligned sensors of the device as a result of the movement of the sun, and the images captured by the pin-hole camera.

29. The system according to claim 27, characterized in that said at least one device is located at the top of a tower of a solar plant with reflective elements for simultaneously characterizing as many reflective elements as devices are arranged in the tower.

30. The system according to claim 27, characterized in that said at least one device is located in any location of a field of reflective elements with the detectors aligned with at least one reflective element such that the aperture angle allows the characterization of said at least one reflective element.

31. A characterization method for characterizing the shape and deformations of the surface of a reflective elements by the quality of the light reflected, characterized in that it comprises the following steps: a) Arranging a device according to claim 17 in a field of reflective elements comprising at least two reflective elements, b) Keeping the reflective element immobile, in a fixed position, during the time required by the movement of the sun so that the beam reflected by the reflective element sweeps across the detectors in the characterizing device, c) Selecting the gain of each of the detectors of the device for reducing the noise signal as a function of intensity of the light beam reflected by the reflective element and received by each of said detectors with a given angle, d) Capturing and measuring, by the detectors of the device, the light reflected by the reflective element that remains in a immobile, fixed, position, and taking, by the pin-hole camera images continuously and simultaneously with respect to the capture of the reflected light e) Normalizing the measurements taken by the detectors of the device for the estimation of the radiant energy on the device, and f) Processing said taken measurements, reconstructing the beam reflected by the at least one reflective element, determining the orientation of the reflector over its entire surface, and obtaining the exact shape and deformations with respect to the design shape.

Description

DESCRIPTION OF THE DRAWINGS

[0059] The following figures showing a preferred embodiment of the invention in an illustrative and non-limiting manner are attached to the present description:

[0060] FIG. 1 shows a basic diagram of a system according to the invention with the characterization device for characterizing heliostats claimed.

[0061] FIG. 2A shows a basic diagram of the movement of the sun and of the beam.

[0062] FIG. 2B shows a series of measurements during the movement of the reflected beam and the reconstruction of a reflected beam.

[0063] FIG. 3 shows a diagram of the components of a detector installed in a device object of the invention.

[0064] FIG. 4 shows a block diagram of the gain adjustment method performed by the detectors forming the device object of the invention.

[0065] FIG. 5 shows a basic diagram of an embodiment of a system object of the invention.

[0066] FIG. 6 shows the aperture angle of a detector of the device and how, as a result of it, capturing the rays coming directly from the sun is avoided.

[0067] FIGS. 7 and 8 show FIGS. 1 and 2A with a pin-hole camera system.

PREFERRED EMBODIMENT

[0068] FIG. 1 shows a system according to the present invention in which there can be observed an array or set of detectors 11, preferably up to 25 optical power detectors, which are preferably equidistantly placed in a device with a vertical structure or column 10 of, preferably, 15 meters in height. Optionally, as shown in FIG. 7, a pin-hole camera system 60 is incorporated in the device at the halfway point of the column, contiguous to the detectors and secured to said column. This pin-hole camera system preferably incorporates at least one pin-hole camera 60 (only one camera shown), although in alternative embodiments, the system can be made up of digital cameras, which are distributed in a vertical array contiguous to the detectors.

[0069] The light 40 reflected by the heliostat 30 to be characterized is detected by the detectors 50 for determining the pattern of the beam reflected by it. By using the movement of the beam 40 reflected by the heliostat 30 due to the continuous and known movement of the sun 20 and keeping the heliostat 30 immobile, the tracing of the distribution of the beam 40 reflected by the heliostat 30 that is obtained is horizontal. Simultaneously to the measurements taken, if the device comprises a pin-hole camera system, the at least one pin-hole camera 60 takes images in which the part of the heliostat that reflects the sun 20 or part of it is illustrated. In these images, the part of the heliostat that is correctly oriented is shown illuminated, as it is reflecting the sun 20, whereas the part that is poorly oriented remains dark.

[0070] In cases where the vertical dimension of the reflected beam 40 is greater than the height of the measurement column of the device, the beam 40 reflected by the vertical measurement column 1 is traced as many times as necessary. Assuming that it needs to be traced twice, the first trace is for measuring the lower part of the reflected beam 40, and subsequently a second trace (after having reoriented the heliostat 30 downwards and rendering it immobile to take the measurement) is for the upper part of the reflected beam 40.

[0071] The measurements taken by each detector 50 are captured and processed in real time (order of milliseconds) by the local processor or local processing and capture unit in each detector 55. The measurements taken can be sent to a global processor of the device 12 with a global control, capture, and processing unit located, preferably at the base of the column 10.

[0072] The horizontal sweeping of the beam across the array of detectors 11 due to the movement of the sun 20 (d-20) is described in a basic manner in FIG. 2A. As the sun 20 moves, the beam 40 reflected by the heliostat 30 passes over the characterization device, and the vertical distribution of the band of the beam 40 that is projected onto the detectors 50 each sampling time (FIG. 2B) is obtained. This figure shows, in the upper part, a series of measurements during the movement of the reflected beam and, in the lower part, a reconstruction of said reflected beam. Given that the movement and position of the sun 20 is known, by means of suitable calculation is outlined the complete shape of the beam 40 that will be formed by the vertical bands individually measured when the beam (d-40) passes over the array of detectors 11. The measurement time is determined by the size of the beam 40 and the traveling speed of the sun 20 (about 4.4 mrad per minute). For a measurement capacity below one second, the beam measurement formed by the set of measured vertical bands can be considered continuous. The complete shape of the beam is thereby reconstructed, as shown in FIG. 2B, and by means of analysis, the heliostat 30 can be characterized, which means preferably obtaining the global optical quality of the reflector.

[0073] FIG. 8 shows an equivalent to FIG. 2A in which the device comprises a pin-hole camera system with at least one camera 60, such that by combining the reconstructed beam with the images taken by the pin-hole camera system, the orientation of all the points of the surface of the reflector and the deviation with respect to the design shape can be determined, achieving a more precise and detailed characterization.

[0074] The characterization device included in the preceding system is formed by detectors 50 which capture the optical power (I) of the beam reflected in the heliostat which is incident on each of them. Each detector 50 is formed by an electronic detection part or automatic gain system 53, an optical detection part 51, and a data communication part 54. A basic diagram of the detector 50, including the local processor or local processing and capture unit 55 of the detector 50, is shown in FIG. 3.

[0075] The detection of each detector is preferably performed by means of an optical sensor 52 arranged in each detector 50. Said optical sensors 52 are preferably silicon photodiodes with a large surface area, although there may be sensors of another type that allow adjusting the gain, such as thermopiles, for example. The detection electronics or automatic gain system 53 takes the measurement of the continuous signal captured by the optical sensor 52 and includes a digital gain potentiometer which allows adjusting the gain (G) level of each detector 50 to the power level received by each detector 50 each sampling time. This is because beam power densities will vary greatly between the central area of the beam and its outer area (see FIG. 2). The adjustment of the gain (G) of each detector 50 to the level of signal received will determine the final measurement time of each vertical band. It is foreseeable that, given that the changes in power density will be slow, in the order of seconds, the gain adjustment algorithm will allow optimizing the signals of all the detectors in a time below one second, so there will be a measurement of each vertical band of the beam in times in the order of one second. A basic diagram of the measurement method of each detector, including the automatic gain adjustment, is reflected in FIG. 4.

[0076] After the optical sensor 52 detect the intensity (I) of the light beam, said automatic gain selection method comprises converting said intensity (I) to electric current (C) so as to measure the gain in the automatic gain system 53 the electric signal (S) of which is transmitted to the processor 55 of the detector 50. If said signal (S) is greater than a pre-established maximum threshold (Umax), an order to decrease the gain (G) is sent to the gain system 53, and if said signal (S) is less than a pre-established minimum threshold (Umin), an order to increase the gain (G) is sent to the automatic gain system 53. Once the gain (G) is adjusted, the electric signal (S) is saved (S.sub.s).

[0077] In the preceding embodiment, the automatic gain selection system 53 of each detector 50 with a single optical sensor 52, preferably a photodiode or a thermopile, has variable-gain electronics selecting or adjusting in said sensor 52 the gain most suited to the light intensity (I) of the beam received by said sensor 52 or detector 50.

[0078] In an alternative embodiment of a detector with an automatic variable-gain system, the detector comprises several sensors, at least two, with each one being associated with a fixed gain, such that by means of the different sensors the dynamic measurement range required for the correct characterization of the heliostats is covered. In this case, the automatic gain system selects, from the at least two sensors, that sensor with the fixed gain most suited to the light intensity of the beam received by the sensors, i.e., the variable-gain of the system is determined by the arrangement of at least two fixed-gain sensors from which the electronics selects the most suitable sensor, allowing adaptations to different circumstances.

[0079] The other time of interest is the time of capture of the signals of all the detectors 50, which will be in the order of milliseconds in any situation. That is, once all the detectors 50 have selected or adjusted their gains (below one second) the signals of each detector 50 will be captured and measured in the time of milliseconds.

[0080] The optical part of the detector 51 is made up of a lens with an aperture angle 56 preferably less than 15°, which allows reducing the background level captured due to scattered light, eliminating unwanted contributions, such as those from other heliostats, or that of the sun (for example, in heliostats located to the south). This situation is shown in FIG. 6, which depicts a plant in the northern hemisphere, where the heliostat 30, positioned to the south of the tower 31, reflects a sunray 33 on the characterization device 11 with an incidence angle (+) on it which is less than half the aperture angle (=) of the detector 50, whereas the ray 21 coming directly from the sun 20, without being reflected in the heliostat 30, is also incident on the detectors 50, forming an angle (α) with the optical axis of the detector 50 greater than half the aperture angle (γ) of the detector 50, so it is not captured by the sensor 52, thus preventing the occurrence of said light as noise in the measurement. In the methods and systems of the state of the art, this direct radiation of the sun cannot be avoided, making it impossible to correctly characterize the heliostat 30. At the same time, the optics of the detector 51 allows multiplying the detected optical power factor for increasing the useful detected signal level. With all this, the signal-to-background ratio is multiplied by a factor of 50-100 with respect to direct detection, such as one that may be carried out, for example, by a signal capture system by means of camera. So being able to also characterize heliostats 30 located far away, even more than 800 m away, is thus assured.

[0081] Lastly, the data communication electronics 54 allows acquiring the signals measured by each detector 50 and sending them to the global processor or global capture and global processing unit of the device 12, preferably located in the device, although it can be situated far from it, which is in charge of normalizing said measurements for the estimation of the radiant energy on the device or devices, in order to subsequently process the measurements and reconstruct the beam reflected by each heliostat.

[0082] As mentioned, the set 11 of detectors 50 will report the measured signals to the global processor of the device 12 preferably arranged in the actual structure of the device 10. Given that this global processor of the device 12 must work outdoors, it will be suitably conditioned for that purpose. As mentioned, the acquired signals may also be sent to a central data processing system which will be preferably a computer located in a comfortable area. The data will be treated by a suitable signal processing software, and the shape of the spatial distribution of the characterized beam will be graphically depicted, FIG. 2B, by means of the same or another suitable software having the interface functions necessary for the capture, saving, and editing thereof.

[0083] The column of detectors 11 will preferably have a mechanical securing system 10 preferably based on aluminum sections which allows stably reaching the same height as the distribution of detectors, for example 15 m. Said distance corresponds with the approximate diameter of the beam reflected by a heliostat at a distance of 800 m, for greater distances the beam will be gradually increased, making it necessary to make as many passes as necessary. Evidently, the size of the beam 40 as a function of distance is approximate and depends on the optical quality of the heliostat 30. In this system, the detection elements 50 and the feed and communication wiring for said elements will be arranged equally spaced from one another. The mechanical system 10 that is initially considered will allow collapsing or raising the measurement column 11. Therefore, during the times or days of activity, the measurement column 11 will be vertical and erected, secured by means of ropes conveniently anchored to the ground for withstanding the actions of the wind. Furthermore, during the times or days when testing is not performed, the measurement column 11 will be collapsed on the ground, laying in horizontal position on it and covered, for example, by a tarp, to prevent wearing or fouling of the column. Thus, the assembly of the column 10, its setting up, and maintenance or cleaning tasks can be performed comfortably working at ground level, without the need to work at heights. This will also allow performing the system calibration process in a simpler manner. The actions of erecting and collapsing the measurement column 11 would be performed by means of using a motor with a towrope suited to the weight and torque of the structure 10. The manner of assembling the vertical column and the wiring associated with the column will be such that it can be disassembled in several sections of length suitable for being transferred to and assembled in other locations. With the device 11 collapsed on the ground, a suitable optical system will allow a calibration process for the set of detectors 50 that is simple to perform.

[0084] Alternatively, FIG. 5 describes the preferred application of the device object of the invention located in the tower 31 of a tower solar plant. Thus, several devices 11, 11″ coexist and characterize heliostats 30, 30″ simultaneously through reflected beams 40, 40″ in the same manner described above. As a result of the use of lenses in the detectors 50, the beams of the heliostats 30, 30″ aimed at contiguous systems, do not affect one another or damage the measurements.

[0085] According to the systems described above, the characterization method for characterizing the quality of the beam reflected by a heliostat comprises the following steps:

[0086] a) Arranging a characterization device as described above,

[0087] b) Keeping the reflective element being characterized immobile and in standby for a given time sufficient for the beam to pass over the device as a result of the movement of the sun,

[0088] c) Automatically and continuously selecting the gain of each of the detectors of the device for the optimization of the noise signal as a function of intensity of the light beam reflected by the heliostat and received by each of said detectors,

[0089] d) The device capturing discrete measurements of the light reflected by the heliostat, which is in standby, over a given period of time as the beam sweeps across the device, in all those scans that are necessary,

[0090] e) Normalizing the measurements of the detectors of the device for the estimation of the radiant energy on the device, and

[0091] f) Processing the measurements taken and reconstructing the reflected beam, obtaining the complete shape thereof, the analysis and post-processing of which characterizes the heliostat, preferably its focal distance and optical quality.

[0092] As mentioned throughout the description and in step b), during the mentioned characterization method the heliostat is kept immobile and in standby the time necessary for the movement of the sun to cause the beam to be swept across the device. Prior to immobilizing the reflective element, the latter must be situated for the purpose of allowing the positioning of the reflected beam adjoined to the measurement device on the side and in the position favoring the beam to be swept across the entire measurement device as a consequence of the movement of the sun. Likewise, step d) can be repeated the times that are necessary until the beam reflected by the heliostat passes over the entire device. Additionally, after said step d), which is repeated as many times as is necessary, and before the step e), the method could be repeated from step b) in the event that several scans are necessary for completely characterizing the entire expanse of the beam.