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http://www.iaeme.com/IJMET/index.asp 27 editor@iaeme.com
International Journal of Mechanical Engineering and Technology (IJMET)
Volume 8, Issue 2, February 2017, pp. 27–33, Article ID: IJMET_08_02_004
Available online at http://www.iaeme.com/ijmet/issues.asp?JType=IJMET&VType=8&IType=2
ISSN Print: 0976-6340 and ISSN Online: 0976-6359
© IAEME Publication
SIMULATION OF SOLAR THERMAL CENTRAL
RECEIVER POWER PLANT AND EFFECT OF
WEATHER CONDITIONS ON THERMAL POWER
GENERATION
Sandhya Jadhav
Research Scholar, Bharati Vidyapeeth Deemed
University College of Engineering, Pune, India
Dr. V. Venkat Raj
Former Director, Health Safety and Environment Group,
Bhabha Atomic Research Centre, Mumbai, India
ABSTRACT
Mathematical model is presented for prediction of thermal losses from central receiver solar
thermal power plant. Results obtained are verified with evidence from solar experiments. Code is
developed for studying the effect of variation of weather conditions i.e. variation of incident solar
radiation, wind speed and ambient temperature during the entire year on the thermal performance
of receiver. Thermal losses have its effect on efficiency of the receiver and hence the overall cost of
solar thermal to electric power. Radiation and convection losses are the major components of
thermal losses. Simulation is done for weather data of Jaipur city of India.
Key words: Central receiver solar plant, external receiver, thermal losses, simulation.
Cite this Article: Sandhya Jadhav and Dr. V. Venkat Raj. Simulation of Solar Thermal Central
Receiver Power Plant and Effect of Weather Conditions on Thermal Power Generation.
International Journal of Mechanical Engineering and Technology, 8(2), 2017, pp. 27–33.
http://www.iaeme.com/ijmet/issues.asp?JType=IJMET&VType=8&IType=2
1. INTRODUCTION
In central receiver solar thermal power plant (CRSTPP), the incident solar rays from the sun are
concentrated and reflected by heliostat field onto a receiver mounted at the top of a tower. Heat transport
fluid flowing through the receiver tubes gets heated up by absorbing the incident energy on the receiver
and is used to produce steam which drives the turbine. The CRSTPP requires a large space for installation
and the components are costly. To carry out experimentation, it becomes costly and time consuming.
Therefore experimental work has shown the necessity to master user friendly modeling tools and
simulation to reduce the effort and time required. Tools can be of great help in predicting the performance
of components of plant and also plant as a whole. It also helps in plant optimization.
Several codes have been developed since 1970s. According to different specifications and needs of
power plants, these softwares can be modified and adopted for simulation. In the literature, some software
for energy balance and performance analysis of entire power plant are available. DELSOL developed by
Sandhya Jadhav and Dr. V. Venkat Raj
http://www.iaeme.com/IJMET/index.asp 28 editor@iaeme.com
Kristler in 1986 is a performance and design optimization software developed by using FORTRAN 77.
Although receiver radiation and convection losses are also calculated, the detail is probably insufficient for
use in receiver evaluation, thus only flux density calculation capabilities are used for receiver analysis.
SOLERGY developed in 1987 used FORTRAN 77 for simulation of the plant.
Code is developed using Visual Basic for studying the thermal performance of the central receiver
solar thermal power plant for different amount of solar radiation received during the entire year. The code
developed simulates the operation and annual power output of a solar central receiver power plant using an
actual simulated weather data recorded at time intervals of 1 hour. It calculates the net electrical energy
output including parasitic power requirements over 24 hrs a day. It has subroutine for each major plant
system, receiver, thermal energy storage and turbine. Annual plant performance is found by adding the
performance at every considered time step.
For each time step, the heliostat field concentrates the incident solar radiation and directs it on to the
receiver placed on the top of the tower. On receiving the adequate amount of solar radiation from the
heliostat field, the receiver starts working. The operation of the receiver depends upon the power received
from the heliostat field and the previous receiver status. The lower receiver power limit is set by the
minimum flow rate that the receiver flow valves can handle. If the power to the receiver is greater than the
receiver thermal rating, the input is decreased to the thermal rating, by heliostat defocusing. All thermal
power from the receiver is delivered to thermal storage tank, provided that storage tank can accept it (i.e.
until storage tank is full). The turbine operates, after a specific level in thermal storage is achieved.
2. THERMAL LOSSES IN THE RECEIVER
In Solar thermal power plants, heat loss can significantly reduce the efficiency and consequently the cost
effectiveness of the system. It is therefore vital to fully understand the nature of these heat loss
mechanisms. The magnitude of the thermal losses varies and it depends on the receiver type, geometry
and size. Apart from receiver configurations weather conditions also play a significant role in thermal
losses of receiver. Therefore it becomes important to study the effect of incident solar flux, ambient
temperature and wind speed. Thermal losses in receiver are due to conduction, convection and radiation
processes. Experimental works have shown that conduction losses are very small. Therefore neglecting
thermal power loss due to conduction, the total thermal power lost by the receiver is the summation of loss
due to radiation by the receiver and loss due to convection by the receiver. These losses account for most
of the receiver thermal losses resulting from calculation. They are evaluated in the receiver simulation
model.
3. EFFECT OF VARIATION IN WEATHER CONDITIONS
Variation of incident flux, wind speed and ambient temperature affects the performance of receiver and
hence thermal losses from receiver. Therefore, effect of variation in incident flux, wind speed and ambient
temp is studied.
3.1. Variation of Incident Solar Radiation
Figure 1 Monthly average incident flux in W/m2
for Jaipur.
0
200
400
600
800
Jan March May July Sept Nov
IncidentFluxinW/m2
Month
Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on
Thermal Power Generation
http://www.iaeme.com/IJMET/index.asp 29 editor@iaeme.com
The total solar incident flux obtained in year 2007 in Jaipur is shown in Fig.1. It is observed that most
of the sunny days of the year the incident flux received is 900 W/m2
as. On rainy seasons and cloudy days
it is zero. Therefore the effect of variation of incident flux is studied for the values ranging from 0 to 900
W/m2
. As most of the days in the year, wind speed is observed to be 4m/s and the ambient temperature to
be 300
C, therefore these values are considered for simulation.
Figure 2 (a) Variation in thermal losses due to radiation with increase in incident flux
Figure 2 (b) Variation in thermal losses due to convection with increase in incident flux
Figure 2 (c) Variation in thermal power with increase in incident flux
Increase in solar radiation increases the receiver temperature and hence the loss due to radiation also
increases. It can be observed from Fig.2a that the radiation loss increases considerably, almost 4 times
when incident solar radiation increases from 100 W/m2
to 900 W/m2
. Thermal loss due to convection on
the other hand increases by only a small amount i.e. only by 0.6 MWth as shown in Fig 2b. Due to the
increase in thermal losses, the total loss in the receiver increases with increase in flux intensity as shown in
Fig 2c. As the flux intensity increases, the net power absorbed by the receiver increases but as there is
increase in losses, net power generated and the overall efficiency of the receiver is almost constant and is
within a range of 78% to 82%.
0.00
4.00
8.00
12.00
16.00
20.00
0 200 400 600 800 1000
Thermalpowerlossdue
toradiationinMWth
Incident flux in W/m2
2.20
2.30
2.40
2.50
2.60
2.70
2.80
2.90
0 200 400 600 800 1000
Thermalpowerlossdueto
ConvectioninMWth
Incident flux in W/m2
0.00
100.00
200.00
0 100 200 300 400 500 600 700 800 900
ThermalPowerinMWth
Incident flux in W/m2
power absorbed net power Power loss
Sandhya Jadhav and Dr. V. Venkat Raj
http://www.iaeme.com/IJMET/index.asp 30 editor@iaeme.com
3.2. Variation in Wind Speed
It is observed that the average value of wind speed is more than 1.5 m/s in all the months as shown in Fig
3. Hourly data of weather however shows that on many hours of the day, there is no wind i.e. wind velocity
is zero m/s. The maximum value of wind speed is observed to be 15.4 m/s. Therefore for simulation, wind
velocity is varied from 0 m/s to 20 m/s. As most of the days in the year, solar incident flux is observed to
be 700 W/m2
and the ambient temperature is 300
C, therefore the solar incident radiation is taken to be 700
W/m2
and ambient temperature is assumed to be 300
C for simulation.
Figure 3 Monthly average wind speed in m/s for Jaipur.
With input values stated earlier, the performance of receiver is studied under varying values of wind
velocity from 0 m/s to 20 m/s. Power loss due to radiation (PR) remains constant as it is independent of
wind speed and is 11.46 MW and variation in heat loss due to convection is observed, thus affecting the
total power loss and net power generated from receiver along with the efficiency of the receiver.
Figure 4 (a) Variation of heat transfer coefficient Figure 4 (b) Power loss due to convection
with variation of speed with variation of wind speed
Figure 4 (c) Variation in net power generated Figure 4 (d) Variation of efficiency of receiver
with variation of wind speed with variation of wind speed
0
1
2
3
4
5
Jan March May July Sept Nov
Windspeedinm/s
Month
0
10
20
30
40
0 5 10 15 20 25
Heattransfer
CoefficientinW/m2K
Velocity of wind in m/s
0
2
4
6
8
10
0 5 10 15 20 25
PowerLossdueto
ConvectioninMWth
Velocity of Wind in m/s
74
76
78
80
82
84
0 5 10 15 20 25
Netpowergeneratedin
MW
Velocity of wind in m/s
0.72
0.74
0.76
0.78
0.80
0.82
0 5 10 15 20 25
EfficiencyofReceiver
Velocity of Wind in m/s
Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on
Thermal Power Generation
http://www.iaeme.com/IJMET/index.asp 31 editor@iaeme.com
The results obtained are plotted to visualize the impact of wind speed. Fig No 4a shows that the heat
transfer coefficient increases with the increase in wind speed and the thermal power loss due to convection
also increases with wind speed as shown in Fig 4b. It can be seen that after wind speed of 5m/s, power loss
due to convection increases sharply. It is observed, at 0 m/s wind velocity, the net thermal power generated
in the receiver decreases with increase of wind speed. This shows that there is 8.9% of reduction in net
thermal power for increase of wind speed from 0m/s to 20m/s as shown in Fig No.4c. Decrease in receiver
efficiency due to increase in heat loss is also observed from 81.35% to 74.1% as shown in Fig No.4d.
3.3. Variation of Ambient Temperature
Figure 5 Monthly average ambient temperature in 0
C for Jaipur.
Fig No.5 shows the average ambient temperature for all the months of the year 2007 for Jaipur city. It
is observed that the average value of ambient temperature is more than 180
C in all the months, above 350
C
on sunny days and as low as 20
C on winter days. The highest temperature is observed as 450
C. Therefore
for simulation, ambient temperature is varied from 00
C to 450
C. The solar incident radiation is taken to be
700 W/m2
and wind speed is assumed to be 4m/s. The values of thermal losses obtained after simulation
show that with increase in ambient temperature, convection loss increases very slowly and radiation loss
decreases. Thus net power decreases as well as the efficiency also decreases by a very small amount. In
general, there is little impact of ambient temperature on the thermal performance of the receiver. Thermal
power loss due to radiation decreases by very small amount as shown in Fig No.6a. This happens due to
large difference between the receiver temperature and ambient temperature. Small increase in ambient
temperature affects the radiation loss by negligible amount. Thermal power loss due to convection
decreases sharply for the increase in ambient temperature from 00
C to 450
C as shown in Fig.No.6b. The
decrease in loss due to convection is 0.2MWth. Since there is decrease in thermal power loss due to both,
convection and radiation, the net thermal power of receiver increases as shown in Fig.No.6c. Same pattern
is observed for increase in efficiency of the receiver as shown in FigNo.6d. The efficiency of the receiver
increases as net thermal power of the receiver increases.
0
5
10
15
20
25
30
35
40
AmbientTemperaturein0C
Month
Sandhya Jadhav and Dr. V. Venkat Raj
http://www.iaeme.com/IJMET/index.asp 32 editor@iaeme.com
1.70
1.75
1.80
1.85
1.90
1.95
0 5 10 15 20 25 30 35 40 45 50
Powerlossduetoconvection
inMWth
Ambient temperature in deg Celcius
11.56
11.58
11.60
11.62
11.64
11.66
11.68
0 10 20 30 40 50
Powerlossduetoradiationin
MWth
Ambient temperature in deg Celcius
74.55
74.60
74.65
74.70
74.75
74.80
74.85
0 10 20 30 40 50
Efficiencyofreceiver
Ambient temperature in deg Celcius
79.70
79.75
79.80
79.85
79.90
79.95
80.00
80.05
0 10 20 30 40 50
NetthermalpowerinMWth
Ambient temperature in deg Celcius
Figure 6 (a) Power loss due to radiation with Figure 6 (b) Power loss due to convection with
variation of ambient temperature variation of ambient temperature
Figure 6 (c) Variation in net power generated with Figure 6 (d) Variation of efficiency of receiver
variation of ambient temperature with variation of ambient temperature
4. CONCLUSION
It is observed that, the thermal losses due to radiation increases considerably with the increase in incident
flux. It is seen that due to variation in flux intensity the receiver temperature varies and hence the mean
temperature which results in variation of the working fluid properties. The net thermal power generated in
the receiver decreases with increase of wind speed. There is 8.9% of reduction in net thermal power for
increase of wind speed from 0m/s to 20m/s. The efficiency of the receiver increases as net thermal power
of the receiver increases with increase in ambient temperature. Out of these three weather parameters;
incident solar radiation is the most affecting parameter for thermal losses and hence generation of thermal
power.
REFERENCES
[1] A. Sobin & W. Wagner. Central collector solar energy receivers. Solar Energy , Vol.18, pp-21-30,1976.
[2] Clifford K. Ho, Software and codes for Analysis of Concentrating Solar Power Technologies, Sandia
Report, December 2008.
[3] James E. Calogeras and Larry H. Gordon, Storage Systems for Solar Thermal Power, in Proceedings of
Thirteenth Intersociety Energy Conversion Engineering Conference San Diego, California, August 20-
25, 1978.
Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on
Thermal Power Generation
http://www.iaeme.com/IJMET/index.asp 33 editor@iaeme.com
[4] L.J.Yebra, M. Berenguel, S. Dorando and M. Romero, Modelling and Simulation of Central Receiver
Solar Thermal Power Plants in Proceedings of the 44th IEEE Conference on Decision and Control and
the European Control Conference, Spain Dec 12-15, 2005.
[5] M. Castro, J. L. Presa, J. Diaz, J. Peire, A. F. Baker, S. E. Faas, L. G. Radosevich & A. C. Skinrood.
Central receiver & storage systems evaluation. Solar Energy Vol. 47, No3, pp-197-207, Printed in
U.S.A,1991
[6] Magal, B. S., Solar Power Engineering, Tata McGraw – Hill Publishing Company Limited, Second
Print. 1994.
[7] Ortega, J., J. Burgaleta, M. Tellez, Central Receiver System (CRS) Solar power plant using molten
SALT as heat transfer fluid, Journal of Solar Energy Engineering (Transactions of the ASME), Vol. 130,
No. 2, , pp. 024501 (6 pg), May 2008.
[8] Robert Z. Litwin, Receiver System: Lessons Learned from Solar Two, The Boeing Company, Canoga
park, CA, SANDIA National Laboratories, March 2002.
[9] Romero, M., R. Buck, J. Pacheco, An Update on Solar Central Receiver Systems, Projects, and
Technologies. ASME Journal of Solar Energy Engineering Vol.124, pp. 98-108, May 2002.
[10] S. P. Sukhatame, Solar thermal power generation, in Proc. Indian Acad Sci (Chem Sci.), Vol. 109, No.
6, pp 521-531. Dec 1997.
[11] Winter, C. J., R. L. Sizmann, L. L. Vant, - Hull (Eds.), Solar Power Plants – Fundamentals, Technology,
Systems, Economics (New York: Springer – Verlag) 2005
[12] Zhihao Yao, Zhiheng Wang, Zhenwu Lu & Xiudong Wei, Modeling and simulation of the pioneer 1
MW solar thermal central receiver system in China, Renewable Energy Vol. 34, 2009, pp. 2437-2446.
[13] Alo Mikola, Teet-Andrus Kõiv and Mikk Maivel. Production of Domestic Hot Water with Solar
Thermal Collectors in North-European Apartment Buildings. International Journal of Mechanical
Engineering and Technology, 7 (1), 2016, pp. 58-66.
[14] Jadhav Sandhya Dilip and Dr. V. Venkatraj, Thermal Losses in Solar Central Receiver, International
Journal of Mechanical Engineering and Technology, 4(6), 2013, pp. 84–90.

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SIMULATION OF SOLAR THERMAL CENTRAL RECEIVER POWER PLANT AND EFFECT OF WEATHER CONDITIONS ON THERMAL POWER GENERATION

  • 1. http://www.iaeme.com/IJMET/index.asp 27 editor@iaeme.com International Journal of Mechanical Engineering and Technology (IJMET) Volume 8, Issue 2, February 2017, pp. 27–33, Article ID: IJMET_08_02_004 Available online at http://www.iaeme.com/ijmet/issues.asp?JType=IJMET&VType=8&IType=2 ISSN Print: 0976-6340 and ISSN Online: 0976-6359 © IAEME Publication SIMULATION OF SOLAR THERMAL CENTRAL RECEIVER POWER PLANT AND EFFECT OF WEATHER CONDITIONS ON THERMAL POWER GENERATION Sandhya Jadhav Research Scholar, Bharati Vidyapeeth Deemed University College of Engineering, Pune, India Dr. V. Venkat Raj Former Director, Health Safety and Environment Group, Bhabha Atomic Research Centre, Mumbai, India ABSTRACT Mathematical model is presented for prediction of thermal losses from central receiver solar thermal power plant. Results obtained are verified with evidence from solar experiments. Code is developed for studying the effect of variation of weather conditions i.e. variation of incident solar radiation, wind speed and ambient temperature during the entire year on the thermal performance of receiver. Thermal losses have its effect on efficiency of the receiver and hence the overall cost of solar thermal to electric power. Radiation and convection losses are the major components of thermal losses. Simulation is done for weather data of Jaipur city of India. Key words: Central receiver solar plant, external receiver, thermal losses, simulation. Cite this Article: Sandhya Jadhav and Dr. V. Venkat Raj. Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on Thermal Power Generation. International Journal of Mechanical Engineering and Technology, 8(2), 2017, pp. 27–33. http://www.iaeme.com/ijmet/issues.asp?JType=IJMET&VType=8&IType=2 1. INTRODUCTION In central receiver solar thermal power plant (CRSTPP), the incident solar rays from the sun are concentrated and reflected by heliostat field onto a receiver mounted at the top of a tower. Heat transport fluid flowing through the receiver tubes gets heated up by absorbing the incident energy on the receiver and is used to produce steam which drives the turbine. The CRSTPP requires a large space for installation and the components are costly. To carry out experimentation, it becomes costly and time consuming. Therefore experimental work has shown the necessity to master user friendly modeling tools and simulation to reduce the effort and time required. Tools can be of great help in predicting the performance of components of plant and also plant as a whole. It also helps in plant optimization. Several codes have been developed since 1970s. According to different specifications and needs of power plants, these softwares can be modified and adopted for simulation. In the literature, some software for energy balance and performance analysis of entire power plant are available. DELSOL developed by
  • 2. Sandhya Jadhav and Dr. V. Venkat Raj http://www.iaeme.com/IJMET/index.asp 28 editor@iaeme.com Kristler in 1986 is a performance and design optimization software developed by using FORTRAN 77. Although receiver radiation and convection losses are also calculated, the detail is probably insufficient for use in receiver evaluation, thus only flux density calculation capabilities are used for receiver analysis. SOLERGY developed in 1987 used FORTRAN 77 for simulation of the plant. Code is developed using Visual Basic for studying the thermal performance of the central receiver solar thermal power plant for different amount of solar radiation received during the entire year. The code developed simulates the operation and annual power output of a solar central receiver power plant using an actual simulated weather data recorded at time intervals of 1 hour. It calculates the net electrical energy output including parasitic power requirements over 24 hrs a day. It has subroutine for each major plant system, receiver, thermal energy storage and turbine. Annual plant performance is found by adding the performance at every considered time step. For each time step, the heliostat field concentrates the incident solar radiation and directs it on to the receiver placed on the top of the tower. On receiving the adequate amount of solar radiation from the heliostat field, the receiver starts working. The operation of the receiver depends upon the power received from the heliostat field and the previous receiver status. The lower receiver power limit is set by the minimum flow rate that the receiver flow valves can handle. If the power to the receiver is greater than the receiver thermal rating, the input is decreased to the thermal rating, by heliostat defocusing. All thermal power from the receiver is delivered to thermal storage tank, provided that storage tank can accept it (i.e. until storage tank is full). The turbine operates, after a specific level in thermal storage is achieved. 2. THERMAL LOSSES IN THE RECEIVER In Solar thermal power plants, heat loss can significantly reduce the efficiency and consequently the cost effectiveness of the system. It is therefore vital to fully understand the nature of these heat loss mechanisms. The magnitude of the thermal losses varies and it depends on the receiver type, geometry and size. Apart from receiver configurations weather conditions also play a significant role in thermal losses of receiver. Therefore it becomes important to study the effect of incident solar flux, ambient temperature and wind speed. Thermal losses in receiver are due to conduction, convection and radiation processes. Experimental works have shown that conduction losses are very small. Therefore neglecting thermal power loss due to conduction, the total thermal power lost by the receiver is the summation of loss due to radiation by the receiver and loss due to convection by the receiver. These losses account for most of the receiver thermal losses resulting from calculation. They are evaluated in the receiver simulation model. 3. EFFECT OF VARIATION IN WEATHER CONDITIONS Variation of incident flux, wind speed and ambient temperature affects the performance of receiver and hence thermal losses from receiver. Therefore, effect of variation in incident flux, wind speed and ambient temp is studied. 3.1. Variation of Incident Solar Radiation Figure 1 Monthly average incident flux in W/m2 for Jaipur. 0 200 400 600 800 Jan March May July Sept Nov IncidentFluxinW/m2 Month
  • 3. Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on Thermal Power Generation http://www.iaeme.com/IJMET/index.asp 29 editor@iaeme.com The total solar incident flux obtained in year 2007 in Jaipur is shown in Fig.1. It is observed that most of the sunny days of the year the incident flux received is 900 W/m2 as. On rainy seasons and cloudy days it is zero. Therefore the effect of variation of incident flux is studied for the values ranging from 0 to 900 W/m2 . As most of the days in the year, wind speed is observed to be 4m/s and the ambient temperature to be 300 C, therefore these values are considered for simulation. Figure 2 (a) Variation in thermal losses due to radiation with increase in incident flux Figure 2 (b) Variation in thermal losses due to convection with increase in incident flux Figure 2 (c) Variation in thermal power with increase in incident flux Increase in solar radiation increases the receiver temperature and hence the loss due to radiation also increases. It can be observed from Fig.2a that the radiation loss increases considerably, almost 4 times when incident solar radiation increases from 100 W/m2 to 900 W/m2 . Thermal loss due to convection on the other hand increases by only a small amount i.e. only by 0.6 MWth as shown in Fig 2b. Due to the increase in thermal losses, the total loss in the receiver increases with increase in flux intensity as shown in Fig 2c. As the flux intensity increases, the net power absorbed by the receiver increases but as there is increase in losses, net power generated and the overall efficiency of the receiver is almost constant and is within a range of 78% to 82%. 0.00 4.00 8.00 12.00 16.00 20.00 0 200 400 600 800 1000 Thermalpowerlossdue toradiationinMWth Incident flux in W/m2 2.20 2.30 2.40 2.50 2.60 2.70 2.80 2.90 0 200 400 600 800 1000 Thermalpowerlossdueto ConvectioninMWth Incident flux in W/m2 0.00 100.00 200.00 0 100 200 300 400 500 600 700 800 900 ThermalPowerinMWth Incident flux in W/m2 power absorbed net power Power loss
  • 4. Sandhya Jadhav and Dr. V. Venkat Raj http://www.iaeme.com/IJMET/index.asp 30 editor@iaeme.com 3.2. Variation in Wind Speed It is observed that the average value of wind speed is more than 1.5 m/s in all the months as shown in Fig 3. Hourly data of weather however shows that on many hours of the day, there is no wind i.e. wind velocity is zero m/s. The maximum value of wind speed is observed to be 15.4 m/s. Therefore for simulation, wind velocity is varied from 0 m/s to 20 m/s. As most of the days in the year, solar incident flux is observed to be 700 W/m2 and the ambient temperature is 300 C, therefore the solar incident radiation is taken to be 700 W/m2 and ambient temperature is assumed to be 300 C for simulation. Figure 3 Monthly average wind speed in m/s for Jaipur. With input values stated earlier, the performance of receiver is studied under varying values of wind velocity from 0 m/s to 20 m/s. Power loss due to radiation (PR) remains constant as it is independent of wind speed and is 11.46 MW and variation in heat loss due to convection is observed, thus affecting the total power loss and net power generated from receiver along with the efficiency of the receiver. Figure 4 (a) Variation of heat transfer coefficient Figure 4 (b) Power loss due to convection with variation of speed with variation of wind speed Figure 4 (c) Variation in net power generated Figure 4 (d) Variation of efficiency of receiver with variation of wind speed with variation of wind speed 0 1 2 3 4 5 Jan March May July Sept Nov Windspeedinm/s Month 0 10 20 30 40 0 5 10 15 20 25 Heattransfer CoefficientinW/m2K Velocity of wind in m/s 0 2 4 6 8 10 0 5 10 15 20 25 PowerLossdueto ConvectioninMWth Velocity of Wind in m/s 74 76 78 80 82 84 0 5 10 15 20 25 Netpowergeneratedin MW Velocity of wind in m/s 0.72 0.74 0.76 0.78 0.80 0.82 0 5 10 15 20 25 EfficiencyofReceiver Velocity of Wind in m/s
  • 5. Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on Thermal Power Generation http://www.iaeme.com/IJMET/index.asp 31 editor@iaeme.com The results obtained are plotted to visualize the impact of wind speed. Fig No 4a shows that the heat transfer coefficient increases with the increase in wind speed and the thermal power loss due to convection also increases with wind speed as shown in Fig 4b. It can be seen that after wind speed of 5m/s, power loss due to convection increases sharply. It is observed, at 0 m/s wind velocity, the net thermal power generated in the receiver decreases with increase of wind speed. This shows that there is 8.9% of reduction in net thermal power for increase of wind speed from 0m/s to 20m/s as shown in Fig No.4c. Decrease in receiver efficiency due to increase in heat loss is also observed from 81.35% to 74.1% as shown in Fig No.4d. 3.3. Variation of Ambient Temperature Figure 5 Monthly average ambient temperature in 0 C for Jaipur. Fig No.5 shows the average ambient temperature for all the months of the year 2007 for Jaipur city. It is observed that the average value of ambient temperature is more than 180 C in all the months, above 350 C on sunny days and as low as 20 C on winter days. The highest temperature is observed as 450 C. Therefore for simulation, ambient temperature is varied from 00 C to 450 C. The solar incident radiation is taken to be 700 W/m2 and wind speed is assumed to be 4m/s. The values of thermal losses obtained after simulation show that with increase in ambient temperature, convection loss increases very slowly and radiation loss decreases. Thus net power decreases as well as the efficiency also decreases by a very small amount. In general, there is little impact of ambient temperature on the thermal performance of the receiver. Thermal power loss due to radiation decreases by very small amount as shown in Fig No.6a. This happens due to large difference between the receiver temperature and ambient temperature. Small increase in ambient temperature affects the radiation loss by negligible amount. Thermal power loss due to convection decreases sharply for the increase in ambient temperature from 00 C to 450 C as shown in Fig.No.6b. The decrease in loss due to convection is 0.2MWth. Since there is decrease in thermal power loss due to both, convection and radiation, the net thermal power of receiver increases as shown in Fig.No.6c. Same pattern is observed for increase in efficiency of the receiver as shown in FigNo.6d. The efficiency of the receiver increases as net thermal power of the receiver increases. 0 5 10 15 20 25 30 35 40 AmbientTemperaturein0C Month
  • 6. Sandhya Jadhav and Dr. V. Venkat Raj http://www.iaeme.com/IJMET/index.asp 32 editor@iaeme.com 1.70 1.75 1.80 1.85 1.90 1.95 0 5 10 15 20 25 30 35 40 45 50 Powerlossduetoconvection inMWth Ambient temperature in deg Celcius 11.56 11.58 11.60 11.62 11.64 11.66 11.68 0 10 20 30 40 50 Powerlossduetoradiationin MWth Ambient temperature in deg Celcius 74.55 74.60 74.65 74.70 74.75 74.80 74.85 0 10 20 30 40 50 Efficiencyofreceiver Ambient temperature in deg Celcius 79.70 79.75 79.80 79.85 79.90 79.95 80.00 80.05 0 10 20 30 40 50 NetthermalpowerinMWth Ambient temperature in deg Celcius Figure 6 (a) Power loss due to radiation with Figure 6 (b) Power loss due to convection with variation of ambient temperature variation of ambient temperature Figure 6 (c) Variation in net power generated with Figure 6 (d) Variation of efficiency of receiver variation of ambient temperature with variation of ambient temperature 4. CONCLUSION It is observed that, the thermal losses due to radiation increases considerably with the increase in incident flux. It is seen that due to variation in flux intensity the receiver temperature varies and hence the mean temperature which results in variation of the working fluid properties. The net thermal power generated in the receiver decreases with increase of wind speed. There is 8.9% of reduction in net thermal power for increase of wind speed from 0m/s to 20m/s. The efficiency of the receiver increases as net thermal power of the receiver increases with increase in ambient temperature. Out of these three weather parameters; incident solar radiation is the most affecting parameter for thermal losses and hence generation of thermal power. REFERENCES [1] A. Sobin & W. Wagner. Central collector solar energy receivers. Solar Energy , Vol.18, pp-21-30,1976. [2] Clifford K. Ho, Software and codes for Analysis of Concentrating Solar Power Technologies, Sandia Report, December 2008. [3] James E. Calogeras and Larry H. Gordon, Storage Systems for Solar Thermal Power, in Proceedings of Thirteenth Intersociety Energy Conversion Engineering Conference San Diego, California, August 20- 25, 1978.
  • 7. Simulation of Solar Thermal Central Receiver Power Plant and Effect of Weather Conditions on Thermal Power Generation http://www.iaeme.com/IJMET/index.asp 33 editor@iaeme.com [4] L.J.Yebra, M. Berenguel, S. Dorando and M. Romero, Modelling and Simulation of Central Receiver Solar Thermal Power Plants in Proceedings of the 44th IEEE Conference on Decision and Control and the European Control Conference, Spain Dec 12-15, 2005. [5] M. Castro, J. L. Presa, J. Diaz, J. Peire, A. F. Baker, S. E. Faas, L. G. Radosevich & A. C. Skinrood. Central receiver & storage systems evaluation. Solar Energy Vol. 47, No3, pp-197-207, Printed in U.S.A,1991 [6] Magal, B. S., Solar Power Engineering, Tata McGraw – Hill Publishing Company Limited, Second Print. 1994. [7] Ortega, J., J. Burgaleta, M. Tellez, Central Receiver System (CRS) Solar power plant using molten SALT as heat transfer fluid, Journal of Solar Energy Engineering (Transactions of the ASME), Vol. 130, No. 2, , pp. 024501 (6 pg), May 2008. [8] Robert Z. Litwin, Receiver System: Lessons Learned from Solar Two, The Boeing Company, Canoga park, CA, SANDIA National Laboratories, March 2002. [9] Romero, M., R. Buck, J. Pacheco, An Update on Solar Central Receiver Systems, Projects, and Technologies. ASME Journal of Solar Energy Engineering Vol.124, pp. 98-108, May 2002. [10] S. P. Sukhatame, Solar thermal power generation, in Proc. Indian Acad Sci (Chem Sci.), Vol. 109, No. 6, pp 521-531. Dec 1997. [11] Winter, C. J., R. L. Sizmann, L. L. Vant, - Hull (Eds.), Solar Power Plants – Fundamentals, Technology, Systems, Economics (New York: Springer – Verlag) 2005 [12] Zhihao Yao, Zhiheng Wang, Zhenwu Lu & Xiudong Wei, Modeling and simulation of the pioneer 1 MW solar thermal central receiver system in China, Renewable Energy Vol. 34, 2009, pp. 2437-2446. [13] Alo Mikola, Teet-Andrus Kõiv and Mikk Maivel. Production of Domestic Hot Water with Solar Thermal Collectors in North-European Apartment Buildings. International Journal of Mechanical Engineering and Technology, 7 (1), 2016, pp. 58-66. [14] Jadhav Sandhya Dilip and Dr. V. Venkatraj, Thermal Losses in Solar Central Receiver, International Journal of Mechanical Engineering and Technology, 4(6), 2013, pp. 84–90.