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International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056
Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072
© 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 463
A review on Design and construction of a one-axis sun-tracking system
Mr. P. R. Mistri1, Mr. S. S. Patel2
1,2 Asst. Prof, Dept of Smt. S. R. Patel engineering College, Gujarat, India
---------------------------------------------------------------------***---------------------------------------------------------------------
Abstract - This paper explains a tracking system which can
be used with single-axis solar concentrating systems. The
position and "status" of the Sun are detected by three light-
dependent resistors (LDRs), one of which detects whether the
collector is focused, whilst a second resistordeterminesifthere
is cloud cover, and the third senses whether it is day or night.
The resultant signals are passed to an electronic control
system which operates a low-speed 12-V d.c. motor which
rotates the collector with the help of a speed-reduction
gearbox. The tracking system accuracy depends on the
magnitude of the solar radiation. The deviation from zero is
0.3 and 0.06 ° with solar radiation of 95and 550 W m-2,
respectively. Both values instruct that the mechanism can be
used comfortably for parabolic trough collectorsofmediumto
high concentration ratios.
Key Words: tracking, solar radiation, concentratingratio,
etc
Introduction
Concentrating solar collectors can provide considerable
advantages over the usual flat plate collectors especially for
medium- to high-temperature applications,althoughtheSun
must be very accurately tracked to ensure good thermal
performance. Variousformsoftrackingmechanisms,varying
from complex to very simple, have been proposed. They can
be divided into two broad categories, namely mechanical
and electrical/electronic systems. The electronic systems
generally exhibit improved reliabilityandtrackingprecision.
These can be further subdivided into:
(1) Mechanisms employing motorscontrolledelectronically
through sensors which detect the magnitude of the solar
illumination
(2) Mechanisms using computer-controlled motors with
feedback control provided from sensorsmeasuringthesolar
flux on the receiver
Although these latter systems employing computer control
are more costly. Due to the fact that the Sun alwaysmovesin
single direction, it is believed that the refinement of the
feedback control does not justify the supplementary cost.
The Tracking System
A tracking mechanism must be reliable and capable to
follow the Sun with a some degree of accuracy, return the
collector to its original position at the end of the day or
during the night, and alsotrackduringperiodsofintermittent
cloud cover. The required accuracy of the tracking
mechanism depends on the collector acceptance angle. This
angle is defined as the range of solar incidence angles,
measured relative to the normal to the tracking axis, over
which the efficiency varies by less than 3% from that
associated with normal incidence (ASHRAE, 1987). The
results of tests, carried out on the parabolic trough collector
model constructed aspart of a research work , are presented
in Fig. 1.
Fig 1: Collector acceptance angle.
The acceptance angle of this collector is approximately 1.6 °
(Kalogirou, 1994). It thus appears that it is sufficient for the
presentmechanism to track the Sunwith an accuracy of 0.7°
(The employed mode of tracking is the E-W horizontal, i.e.,
the parabolic trough collector axis is orientated in a N-S
direction and the collector tracksthe Sunin anE-W direction
and styled.
System Description
The final system, which was designed to operate with the
required tracking accuracy, consists of a small direct current
(d.c.)motor which rotatesthe collector via aspeed-reduction
gearbox.A control systemis used todetect the Sun'sposition
and operate the motor.
A diagram of the system, to gather with a table showing the
functions of the control system, are presented in Fig. 2. The
system employs three sensors of which A is installed on the
east side of the collector shaded by the frame, whereas the
other two (B and C) are installed on the collector frame.
Sensor A acts as the "focus" sensor, i.e., it will only receive
direct sunlight.
International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056
Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072
© 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 464
Fig 2. Tracking mechanism-system diagram.
when the collector is focused. As the Sun moves, sensor A
becomes shaded and the motor turns "ON". Sensor B is the
"cloud" sensor and cloud cover isassumedwhenillumination
falls below a certain level. Sensor C is the "daylight" sensor.
The condition when all three sensors approach sunlight is
translated via control system as daytime with no cloud
passing over the Sun and the collector being in a absolutely
focused position. The functions shown in the table of Fig. 2
are followed provided that sensor C is"ON", i.e., itis daytime.
The control system
When the preliminary stages of the design of the control
system a number of sensor types were considered including
photocells, bimetallic strips, fluid-mechanical devices and
light dependent resistors (LDRs).
These all have few merits, e.g., the performance of sensors
which depend upon heat differences are affected by other
ambient conditions such aswindandtemperature.Photocells
were rejected because they require a large area in order to
supply the power required for the operation of the relays.
The principle of operation of the system is demonstrated in
the controldiagram presented in Fig. 3.The presentLDRsare
type ORP 13 (RS, 1991). Their resistances normally 310Ω in
the shade and15 Ω in direct sunlight.
Fig 3. Tracking mechanism- control diagram
Asmentioned previously, the motor ofthesystemisswitched
on when any of the three LDRs is shaded. Which sensor is
activated depends on the amount of shading determined by
the value set on the adjustable resistor, i.e.,thresholdvalueof
radiation required to trigger the relays. The logic with which
each sensor behaves is shown by the flow charts presented
in Fig. 4 Irjet template sample paragraph, Irjet template
sample paragraph .Irjet template sample paragraph. Irjet
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Sensor A is alwayspartially shaded. Asthe shadingincreases,
due to the movement of the Sun, a value is reached which
triggers the forward relay which switches the motor on
(connection not shown in Fig. 5), to turn the collector and
therefore re-exposes sensor A.
The system also accommodatescloud cover, i.e.,whensensor
B is not receiving direct sunlight, determined by the value of
another adjustable resistor, a timer is automatically
connected to the system and this powers the motor every 2
min for about 8s (see Fig. 4). As a result the collector usually
follows the Sun's path, and when the Sun reappears the
collector is re-focused by the function of sensor A
The system alsoincorporatestwo limit switches,thefunction
of which is to stop the motor from going beyond the
rotational limits. These are installed on two stops, which
restrict the overallrotationof the collectorinbothdirections,
east and west. The collector tracks to the west as long as it is
daytime. When the Sun goes down and sensor C determines
that it is night, power is connected to a reverse relay (see Fig.
4) which changes the motor's polarity and rotates the
collectoruntilitsmotion is restricted by the east limitswitch.
If there is no Sun during the following morning, the timer is
used to follow the Sun's path as under normal cloudy
conditions. Figure 5 is a block diagram of the control system
showing the three sensors together with the timer chip,
forward and reverse relays, and limit switches (denoted as
east and west L/S). The control systemusesa combinationof
inverters and "nand" gates in order to "translate" the
resistance of the LDRs into a signal which triggers the relays.
Nand gates give a logic high "1" signal when any of the input
signals is logic zero "0." They give logic zero "0" signal when
all input signals are logic high "1". Light-emitting diodes
(LEDs) are employed to show the condition of the sensors
and motor.
Fig 4. Sensor function flow charts.
International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056
Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072
© 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 465
Performance of the tracking Mechanism
The Sun "travels" at a constant speed of 0.27 ° min -1, so that
tracking accuracy (i.e., the out of focus angle required to
initialize the system), can be determined by measuring the
period between successive operations of
the motor.
The tracking mechanism proved to be very Reliable and
durable during the testing period of about 3.5 years. All the
functions of the control system as described previously
performed reliably. The function which allowed the
mechanism to follow the approximate path of the Sun when
shaded behind a cloud was very effective as less than 25 s
were needed to re-focus the collector after the Sun
reappeared. Extensive testing of the solar collector
established that the tracking mechanism was very effective
and accurate. The accuracy of the system depends on the
intensity of the Sun's illumination. In the worst case, with
radiation of the order of 95 W m -2, the accuracy of the
position mechanism was 0.3°.This variation was reduced to
0.05 ° with radiation levels of about 550 W m - 2. Thus the
mechanism performed satisfactorily throughout the year in
the present parabolic trough collector application. The
accuracy was much greater than the suggested 0.7° which
was derived by the collector acceptance angle test (Fig, 1).
The accuracy of the tracking mechanism can be increasedby
changing the value of the adjustable resistor connected in
series with sensor A.
Conclusion
The electronic trackingmechanism, which wasdesignedand
constructed,has proved to be nearly accurate forthe present
solar energy utilization . The accuracy is such that the
mechanism can be used for"tracking" solar parabolic trough
collectors ofmedium to high concentration ratios, under any
weather conditions.
The mechanism may also find application in other systems
which are required to follow the path of the Sun, e.g.,
equipment used for measuring solar beam radiation, In this
case the pointing error must be smaller than the
instrument's angular field of view, which is typically 8°, and
the instrument is usually mounted on a platform which
tracks the Sun. The accuracy obtained from the proposed
tracking mechanism is well within safe limits.
Tracking in the altitude direction could be achieved by
manual periodic adjustment.Beamradiationmeasurementis
also required in cloudy conditions so that the ability of the
present mechanism to follow the Sun in these conditions is
particularly important for computerized data collection.
References
1. ASHRAE Standard 94 (1986) Method of Testing to
Determine the Thermal Performance of Solar Collectors.
Boultinghouse K. D. (1982) Development of a Solar-Flux
Tracker for Parabolic-Trough Collectors. Sandia National
Laboratories.
2. Hession P. J. and BonwickW. J. (1985) Experience with a
sun tracker system. Solar Energy 32, 3-11
3. Kupta K. C., Mirakhur P. K. and Sathe A. P. (1979) A simple
solar tracking system, SUN. Proceedingsof the International
Solar Energy Society. Pergamon, New Delhi, India
4. Zogbi R. and Laplaze D. (1985) Design and construction of
a sun tracker. Solar Energy 33, 369 372.

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IRJET- A Review on Design and Construction of a One-Axis Sun-Tracking System

  • 1. International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072 © 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 463 A review on Design and construction of a one-axis sun-tracking system Mr. P. R. Mistri1, Mr. S. S. Patel2 1,2 Asst. Prof, Dept of Smt. S. R. Patel engineering College, Gujarat, India ---------------------------------------------------------------------***--------------------------------------------------------------------- Abstract - This paper explains a tracking system which can be used with single-axis solar concentrating systems. The position and "status" of the Sun are detected by three light- dependent resistors (LDRs), one of which detects whether the collector is focused, whilst a second resistordeterminesifthere is cloud cover, and the third senses whether it is day or night. The resultant signals are passed to an electronic control system which operates a low-speed 12-V d.c. motor which rotates the collector with the help of a speed-reduction gearbox. The tracking system accuracy depends on the magnitude of the solar radiation. The deviation from zero is 0.3 and 0.06 ° with solar radiation of 95and 550 W m-2, respectively. Both values instruct that the mechanism can be used comfortably for parabolic trough collectorsofmediumto high concentration ratios. Key Words: tracking, solar radiation, concentratingratio, etc Introduction Concentrating solar collectors can provide considerable advantages over the usual flat plate collectors especially for medium- to high-temperature applications,althoughtheSun must be very accurately tracked to ensure good thermal performance. Variousformsoftrackingmechanisms,varying from complex to very simple, have been proposed. They can be divided into two broad categories, namely mechanical and electrical/electronic systems. The electronic systems generally exhibit improved reliabilityandtrackingprecision. These can be further subdivided into: (1) Mechanisms employing motorscontrolledelectronically through sensors which detect the magnitude of the solar illumination (2) Mechanisms using computer-controlled motors with feedback control provided from sensorsmeasuringthesolar flux on the receiver Although these latter systems employing computer control are more costly. Due to the fact that the Sun alwaysmovesin single direction, it is believed that the refinement of the feedback control does not justify the supplementary cost. The Tracking System A tracking mechanism must be reliable and capable to follow the Sun with a some degree of accuracy, return the collector to its original position at the end of the day or during the night, and alsotrackduringperiodsofintermittent cloud cover. The required accuracy of the tracking mechanism depends on the collector acceptance angle. This angle is defined as the range of solar incidence angles, measured relative to the normal to the tracking axis, over which the efficiency varies by less than 3% from that associated with normal incidence (ASHRAE, 1987). The results of tests, carried out on the parabolic trough collector model constructed aspart of a research work , are presented in Fig. 1. Fig 1: Collector acceptance angle. The acceptance angle of this collector is approximately 1.6 ° (Kalogirou, 1994). It thus appears that it is sufficient for the presentmechanism to track the Sunwith an accuracy of 0.7° (The employed mode of tracking is the E-W horizontal, i.e., the parabolic trough collector axis is orientated in a N-S direction and the collector tracksthe Sunin anE-W direction and styled. System Description The final system, which was designed to operate with the required tracking accuracy, consists of a small direct current (d.c.)motor which rotatesthe collector via aspeed-reduction gearbox.A control systemis used todetect the Sun'sposition and operate the motor. A diagram of the system, to gather with a table showing the functions of the control system, are presented in Fig. 2. The system employs three sensors of which A is installed on the east side of the collector shaded by the frame, whereas the other two (B and C) are installed on the collector frame. Sensor A acts as the "focus" sensor, i.e., it will only receive direct sunlight.
  • 2. International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072 © 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 464 Fig 2. Tracking mechanism-system diagram. when the collector is focused. As the Sun moves, sensor A becomes shaded and the motor turns "ON". Sensor B is the "cloud" sensor and cloud cover isassumedwhenillumination falls below a certain level. Sensor C is the "daylight" sensor. The condition when all three sensors approach sunlight is translated via control system as daytime with no cloud passing over the Sun and the collector being in a absolutely focused position. The functions shown in the table of Fig. 2 are followed provided that sensor C is"ON", i.e., itis daytime. The control system When the preliminary stages of the design of the control system a number of sensor types were considered including photocells, bimetallic strips, fluid-mechanical devices and light dependent resistors (LDRs). These all have few merits, e.g., the performance of sensors which depend upon heat differences are affected by other ambient conditions such aswindandtemperature.Photocells were rejected because they require a large area in order to supply the power required for the operation of the relays. The principle of operation of the system is demonstrated in the controldiagram presented in Fig. 3.The presentLDRsare type ORP 13 (RS, 1991). Their resistances normally 310Ω in the shade and15 Ω in direct sunlight. Fig 3. Tracking mechanism- control diagram Asmentioned previously, the motor ofthesystemisswitched on when any of the three LDRs is shaded. Which sensor is activated depends on the amount of shading determined by the value set on the adjustable resistor, i.e.,thresholdvalueof radiation required to trigger the relays. The logic with which each sensor behaves is shown by the flow charts presented in Fig. 4 Irjet template sample paragraph, Irjet template sample paragraph .Irjet template sample paragraph. Irjet template sample paragraph Sensor A is alwayspartially shaded. Asthe shadingincreases, due to the movement of the Sun, a value is reached which triggers the forward relay which switches the motor on (connection not shown in Fig. 5), to turn the collector and therefore re-exposes sensor A. The system also accommodatescloud cover, i.e.,whensensor B is not receiving direct sunlight, determined by the value of another adjustable resistor, a timer is automatically connected to the system and this powers the motor every 2 min for about 8s (see Fig. 4). As a result the collector usually follows the Sun's path, and when the Sun reappears the collector is re-focused by the function of sensor A The system alsoincorporatestwo limit switches,thefunction of which is to stop the motor from going beyond the rotational limits. These are installed on two stops, which restrict the overallrotationof the collectorinbothdirections, east and west. The collector tracks to the west as long as it is daytime. When the Sun goes down and sensor C determines that it is night, power is connected to a reverse relay (see Fig. 4) which changes the motor's polarity and rotates the collectoruntilitsmotion is restricted by the east limitswitch. If there is no Sun during the following morning, the timer is used to follow the Sun's path as under normal cloudy conditions. Figure 5 is a block diagram of the control system showing the three sensors together with the timer chip, forward and reverse relays, and limit switches (denoted as east and west L/S). The control systemusesa combinationof inverters and "nand" gates in order to "translate" the resistance of the LDRs into a signal which triggers the relays. Nand gates give a logic high "1" signal when any of the input signals is logic zero "0." They give logic zero "0" signal when all input signals are logic high "1". Light-emitting diodes (LEDs) are employed to show the condition of the sensors and motor. Fig 4. Sensor function flow charts.
  • 3. International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 05 Issue: 03 | Mar-2018 www.irjet.net p-ISSN: 2395-0072 © 2018, IRJET | Impact Factor value: 6.171 | ISO 9001:2008 Certified Journal | Page 465 Performance of the tracking Mechanism The Sun "travels" at a constant speed of 0.27 ° min -1, so that tracking accuracy (i.e., the out of focus angle required to initialize the system), can be determined by measuring the period between successive operations of the motor. The tracking mechanism proved to be very Reliable and durable during the testing period of about 3.5 years. All the functions of the control system as described previously performed reliably. The function which allowed the mechanism to follow the approximate path of the Sun when shaded behind a cloud was very effective as less than 25 s were needed to re-focus the collector after the Sun reappeared. Extensive testing of the solar collector established that the tracking mechanism was very effective and accurate. The accuracy of the system depends on the intensity of the Sun's illumination. In the worst case, with radiation of the order of 95 W m -2, the accuracy of the position mechanism was 0.3°.This variation was reduced to 0.05 ° with radiation levels of about 550 W m - 2. Thus the mechanism performed satisfactorily throughout the year in the present parabolic trough collector application. The accuracy was much greater than the suggested 0.7° which was derived by the collector acceptance angle test (Fig, 1). The accuracy of the tracking mechanism can be increasedby changing the value of the adjustable resistor connected in series with sensor A. Conclusion The electronic trackingmechanism, which wasdesignedand constructed,has proved to be nearly accurate forthe present solar energy utilization . The accuracy is such that the mechanism can be used for"tracking" solar parabolic trough collectors ofmedium to high concentration ratios, under any weather conditions. The mechanism may also find application in other systems which are required to follow the path of the Sun, e.g., equipment used for measuring solar beam radiation, In this case the pointing error must be smaller than the instrument's angular field of view, which is typically 8°, and the instrument is usually mounted on a platform which tracks the Sun. The accuracy obtained from the proposed tracking mechanism is well within safe limits. Tracking in the altitude direction could be achieved by manual periodic adjustment.Beamradiationmeasurementis also required in cloudy conditions so that the ability of the present mechanism to follow the Sun in these conditions is particularly important for computerized data collection. References 1. ASHRAE Standard 94 (1986) Method of Testing to Determine the Thermal Performance of Solar Collectors. Boultinghouse K. D. (1982) Development of a Solar-Flux Tracker for Parabolic-Trough Collectors. Sandia National Laboratories. 2. Hession P. J. and BonwickW. J. (1985) Experience with a sun tracker system. Solar Energy 32, 3-11 3. Kupta K. C., Mirakhur P. K. and Sathe A. P. (1979) A simple solar tracking system, SUN. Proceedingsof the International Solar Energy Society. Pergamon, New Delhi, India 4. Zogbi R. and Laplaze D. (1985) Design and construction of a sun tracker. Solar Energy 33, 369 372.