Every optical system for sunlight concentration requires following the sun in its movement. The sun tracking method is essentially chosen on the base of collection geometry and optical system configuration. A simple, useful, and original technique to realise sun tracking is proposed. It is based on a double guiding system using two complementary procedures. A passive tracking device performs a preliminary collector orientation. Then an active tracking system realises its fine positioning and adjustments exploiting an optical pointing sensor. The core of this active tracking device is the sun finder. Pointing sensors for fibre-coupled, CPV (Concentrating Photo voltaic), and linear collectors are presented, illustrating in detail the working principle and practical use. All sensors were optically characterised in laboratory, under controlled and reproducible conditions. Some field tests completed the experimentation evaluating the sensors performance in outdoor working conditions.
Tracking the movement of the sun is a strategy to enhance the performance of solar photovoltaic plants. Using plane Photo voltaic (PV) panels, the required pointing precision is of the order of few angular degrees; hence it is sufficient to drive the motors dedicated to orient the PV panels, using a software taking into account sun’s ephemerides during the arc of the year [
In Concentrating PhotoVoltaic (CPV) plants that, on the contrary, can work only with direct sunlight, it is necessary to employ an optical pointing system. In these devices, the central optical component typically is a Fresnel lens or a parabolic concentrator and some secondary optical elements could be added to improve pointing precision and plant collection efficiency.
Maintaining aligned the optical system with the sun’s position requires an angular precision higher than the tenth of degree. This accuracy is not realisable using a passive driving device due to problems connected to the plant orientation, difficulties in keeping a high mechanical stability, wind action, and the precision required by the type of concentrator in use. For these reasons, it is not sufficient to use only the alignment technique based on the
These devices, used to furnish the error signal to the control electronics, are commonly called “sun finders”. In general, the optoelectronic device utilises couples of photodetectors that, in conditions of alignment in the sun’s direction, supply the same response because they detect the same amount of light. The simplest device is composed of an opaque sector, which separates two photodiodes [
However, an enhanced pointing accuracy can be obtained employing an optical system with a focal length
The movement of the sun with respect to a determined site on the Earth surface seems very complicated. The sun’s altitude over the horizon depends on the site Latitude and it varies during the year and during the day. Figure
Altitude of sun over the horizon for Firenze (Italy).
The movement of the sun can be subdivided in two components. These two movements correspond to the sun tracking for a linear collector in the North-South and East-West placements. Then the bidirectional tracking system combines the two movement components to follow the sun’s displacement during the day and for each day of the year.
If the linear collector axis is parallel to the North-South direction, the tracking system must follow the sun in its daily excursion and the sun’s altitude over the horizon depends on Latitude and day of the year. With this layout, the solar rays impinge on the collector with an inclination dictated by Latitude and hour of the day.
If the linear collector axis is parallel to the East-West direction, the sun should not be tracked in its daily excursion. However, the tracking system must follow the displacements in sun’s altitude occurring every day of the year. In this layout only at noontime sun’s rays are perpendicular to the entrance aperture of the solar trough.
Linear tracking is obviously employed for sunlight collecting systems working in one direction, like solar troughs or linear lenses. Linear mirrors of troughs are typically combined to linear metal pipes for thermal or cooling applications, but the absorber can also be constituted by an array of PV cells. Linear lenses concentrators are mostly made of Fresnel lenses and they can either be used in thermal or low concentration CPV applications.
The bidirectional tracking is applied to solar collectors working on two axes, like point focus systems or dish systems. These collection systems are mostly coupled to PV cells of various size, shape, and features, which sometime require the introduction of a secondary optics. However, these solar concentrators could also be coupled to optical fibres, exploiting the same tracking techniques. In the bidirectional tracking, the optical collectors are oriented in the sun’s direction using an equatorial structure with two movements on the
The accurate placement of the sunlight collection device is the essential requirement for the efficacy of any tracking technique. The movements, the necessary precision level and the orientation actuation are facilitated by a precise solar plant positioning. However, placement errors can be compensated modifying the angle of tracking system rotation. This angular correction corresponds to the daily sun tracking. The values of correction angle are experimentally determined maximising the light received by the absorber. For example, for thermal linear collectors a misalignment error in North-South placement can be recovered up to 15°, typically with negligible energy losses [
This practical compensation could also mitigate the effects of mechanical misalignments or tracking errors or external agents (atmospheric or environmental). However, its efficacy basically depends on collection system and on orientation errors amount: only after examining the specific case, it can be assessed how much the correction method is able to compensate the orientation errors. Finally the compensation effectiveness also depends on sun’s altitude
The proposed tracking methodology consists in using two complementary tracking techniques, which are integrated to keep the optical collector oriented in the sun’s direction. Hence the device for collector movement is provided with a double guiding system. The first one is of passive type and it drives the motors in order to correctly orient the collector every day of the year, while the second one is of dynamic type and it exploits an optical sun finder. The two tracking techniques are complementary since the first one provides the preliminary orientation, then the second one realises the fine positioning and adjustments. The passive preliminary orientation is necessary to track the sun position when the solar light does not reach the sun finder (in case of could passage or sun absence). In this way when the sun illuminates again the sun finder, the active system can take the control of the tracking.
The advantage of the double-driving technique is to confer flexibility to the tracking system, which automatically follows every weather variation in all environmental conditions. To achieve and maintain the sun tracking, the double guiding system must fulfil several requirements. The time axis of the device should to be oriented in the North-South direction; nevertheless, the device should correctly work even in case of an approximate placement. During the starting phase, the optical system must reach the correct orientation in the sun’s direction, even in cloudy sky conditions. The speed of motors ought to be synchronised with the sun’s velocity. Therefore, the value of set speed should consider geographic position, collector inclination, and day of the year. When the cloudy sky comes back to a clear sky condition, the sun’s image will be aligned with the photodetector only if the motor speed is appropriate and the initial positioning operation is correctly carried out. On the contrary (the more frequent case), the control is taken by the sun finder.
The sun finder is the optical device constituting the active guiding system of the tracking methodology. To improve the pointing precision, we suggest the use of a device including two sections, with different Field Of View apertures (FOV), corresponding to different accuracies. The low-precision section allows the reorientation of the collector within a suitably large FOV, while the high-precision section has a smaller FOV. The two sections of the sun finder are used in sequence, improving the accuracy. The FOVs are determined by the solar application and usually the larger FOV exceeds 30°, while the smaller FOV is lower than 10°.
Two examples of realised sun finders are shown in Figures
Example of sun finder with 1 section.
(a) A sun finder with 2 sections. (b) Scheme of the pointer in (a).
Figure
In the last decade, Concentrating Photovoltaics (CPV systems) have improved their diffusion and the related electronics, and optical components have experienced great technological and scientific developments. Photovoltaic cells of the last generation require concentrations that can exceed 700 suns. Consequently, the associated optical systems must have a quite high value of posterior numerical aperture and a very tiny Field Of View. These requirements impose a very high angular precision to the systems for sun tracking. For tracking sensors that guide high concentration systems, the typical required resolution is at least 0.1°.
Sun tracking has been studied and experimented in our laboratory since 1997, developing mechanics, electronics, and software to realise prototypes [
All sensors were tested in laboratory under controlled and reproducible conditions. This laboratory experimentation includes a deep analysis of angular resolution and Field Of View of the sensors. The purpose of these tests is to provide an optical characterisation of the devices. Finally the sensors were tested under operative conditions in an outdoor installation.
The Pinhole Sensor works as a pinhole camera without lenses. Figure
Pinhole sensor.
The distance
The FOV aperture can be obtained as
The Slit Sensor is analogous to the Pinhole Sensor, with a slit replacing the pinhole. Consequently, the four-quadrant detector works as a two-quadrant photodetector and it can be substituted by a
Slit sensor.
In general the Slit Sensor is applied to solar trough collectors and linear Fresnel lenses because its sensitivity is only on one axis. Solar troughs are linear collectors employed in solar plant and they are usually placed parallel to the ground. These systems are provided with a unique motor that performs the sun tracking during the whole day.
The employed sensors of position should be able to work for the entire daytime. Hence they should be sensitive only to the daily movement of the sun and their functioning should not be dependent on the sun’s monthly position.
The Slit Sensor developed in our laboratory is based on the projection of a light line produced by a slit. As Figure
Ray incidence on slit sensor.
The fine displacements of the sun are assessed, analogously to the case of Pinhole Sensor, from the transversal position of the light line over the photodetector.
The electronic system controlling the motor guide is of digital type. It employs an Input/Output DAQ device NI USB-6009 supplied by National Instrument. The I/O card is linked to a personal computer through a connection of USB type. The analogical inputs of the card are used to manage the photodetector with 2 or 4 quadrants of the sun finder. The digital outputs are employed to guide the drivers of electric motors, which move the concentrators or the collectors’ supports.
The programme, which assesses the solar
Figure
Scheme of the electronics.
In case of Pinhole Sensor, Figure
4
The spot misalignment is expressed by the coordinates of point
The misalignment of sun’s image barycentre is provided by the following algorithm:
The elaboration procedure is analogous for the case of Slit Sensor, but considering only
The laboratory setup to test Pinhole Sensor and Slit Sensor is described in Figure
Test setup for the laboratory tests of the sensors.
Figures
(a) Results for Pinhole Sensor. (b) Results for Slit Sensor.
Finally Figure
Results of laboratory tests.
In conclusion, laboratory tests have assessed that the angular resolution is at least 0.1°, for Pinhole and Slit Sensors. As evidenced by Figure
The sun tracking sensors were experimented in operative conditions with direct exposition to the sun. The aim of these field tests was to verify if the sensor characteristics measured in laboratory are applicable also in real conditions.
The tracking system for outdoor tests was placed with the axis aligned to the North-South direction, with a fixed orientation towards the sun, as shown in Figure
Scheme of field tests of the sensors.
Figures
(a) Output signals for Slit Sensor. (b) Misalignment for Slit Sensor.
Then the time axis can be converted into angular coordinate, to have more useful graphics and to check the correspondence with the laboratory characterisation of Figures
For the Slit Sensor, Figure
Lab and filed tests for Slit Sensor.
Laboratory and field measurements for Pinhole Sensor are reported in Figure
Lab and field tests for pinhole sensor.
The curve measured with direct exposition to the sun is in agreement with the laboratory measurements for all sensors. However, the match is particularly good for the case of Slit Sensor. It is interesting to note that there is perfect coincidence between the two curves in the central zone of Figure
In conclusion, Figure
Laboratory and field tests for both sensors.
The field tests were performed placing the sun pointer towards the sun and acquiring, every 0.5 second, while the sun moved over the pointer. Consequently, applying the time-to-angular coordinate transformation, this temporal sampling corresponded to an angular sampling of 0.002°. From these field tests, the angular resolution results better than 0.01° for Slit Sensor and Pinhole Sensor. However the Pinhole Sensor remains the most precise one.
In case of long acquisition time, the field test curve can show some disturbs caused by cloud transit. Nevertheless, these isolated perturbations do not affect the sensor functionality.
The results of the experimentation performed in laboratory and with direct exposition to the sun were finally compared to the corresponding theoretical data. The Pinhole sensor was reproduced in a Zemax-EE optical simulation and the output signal was compared to the signal measured in the laboratory and filed tests. Therefore, the research was completed validating the experimental results by a comparison with the simulated data.
Figure
Simulated and measured data for pinhole sensor.
An innovative methodology for sun tracking was developed and experimented both in laboratory and in real working conditions. This tracking procedure is based on an optical pointing system exploiting one or two sensors. The optical tracking system was applied to different testing devices for sunlight collection. This experimentation examined solar concentrators coupled to photovoltaic cells, optical fibres, or linear metal pipes.
The proposed tracking technique consists in a double guiding system: the first one provides the preliminary orientation, then the second one realises the fine positioning and adjustments. The first directing system is of passive type and it drives the motors to correctly orient the collector every day of the year. The second driving system is of dynamic type and it employs an optical sun finder.
The heart of the active tracking system is the sun finder, which is a camera without lenses composed of a Pinhole Sensor (or a Slit Sensor) mounted over a four-quadrant detector. For safety the sun finder usually contains two sections with different Field of Views. The two sections are used in sequence, improving the precision, from the wide-angle section to the narrow-angle section.
The distance from the pinhole to the four-quadrant detector determines the sensor FOV aperture. The described optical system can track the sun’s position with an angular precision up to 0.01°, but usually the required precision is 0.1°. This angular resolution was experimentally determined for every sensor; moreover, the field tests evidenced that the Pinhole Sensor is more precise than the Slit Sensor.
The tracking system is simple, reliable, and adaptable to all weather conditions and environmental variations. Even in case of sun shading or temporary sun absence, the system provides a realignment of the collector in few seconds. The system is able to compensate possible errors in the placement of the device, which should be correctly aligned to the Earth axis. Figure
The sun finder with 2 sections mounted with the covering glass.
Two exemplificative pointing sensors were realised and experimented: Pinhole Sensor and Slit Sensor. The Pinhole Sensor contains a photodetector coupled to a pinhole, while in the Slit Sensor it is coupled to a slit. Suitable mechanics and electronics were realised for the prototypes of both sensors to obtain their optical characterisation. All devices were analysed in laboratory, under controlled and reproducible conditions. Then the sun tracking sensors were experimented in operating conditions, with direct exposition to the sun.
The Pinhole Sensor is the most precise one and it performs sun tracking in two perpendicular directions achieving a very high sensitivity. It is indicated for solar optical systems requiring high pointing precision, like concentrators coupled to small PV cells or optical fibres. The Slit Sensor reaches the same precision of the Pinhole Sensor but only in one direction. Hence it can be applied to linear collectors for solar thermal plants or low concentration CPV systems.