SlideShare a Scribd company logo
Solar Resource Lab
Learning Goal
• Students will be able to understand sources of
variation in insolation, construct insolation
forecasting models, validate these models with solar
radiation measurements, and gain an appreciation
for solar forecasting as an intriguing challenge for the
design of renewable energy systems.
Learning Outcome
• Forecast seasonal and daily variation in insolation on
a collector surface using clear-sky insolation theory.
• Estimate model error using pyrheliometer and
pyranometer measurements.
• Propose plausible sources of error in model and
derive optimal parameter estimates.
• Predict the quantity and timing of insolation losses
due to obstructions using site maps and sun-path
diagrams.
P1) The component of insolation that
has the most insolation during clear-
sky conditions is
1. Diffuse
2. Direct-beam
3. Reflected
P2) Solar altitude angle is
1. The angle between the incoming direct sunlight and
a plane normal to the earth’s surface.
2. The angle between the incoming direct sunlight and
the equator.
3. The angle between due south and the location of an
obstruction to a solar collector.
P3) Applying clear-sky insolation
theory during cloudy conditions
1. may underestimate optical depth and result in an
overestimate of direct insolation.
2. may underestimate the sky diffuse factor and result
in an underestimate of diffuse insolation.
3. may overestimate the air mass ratio and result in
an underestimate of direct insolation.
4. Both 1 and 2.
P4) The pyrheliometer measurements (blue line)
represent what component(s) of insolation ?
1. Direct
2. Diffuse
3. Direct + Diffuse + Reflected
Clear-Sky Insolation Theory
PyranometerPyrheliometer
PyranometerPyrheliometer
kW/m2
Lat/Lon = 37.414319/-122.057944
http://maps.google.com/?ie=UTF8&ll=37.414319,-122.057944&spn=0.000392,0.000603&t=h&z=21
Tools and Data
• Clear-sky insolation theory (Masters, 2004)
• Google maps : 37.414319,-122.0579 Lat / Lon
http://maps.google.com/?ie=UTF8&ll=37.414319,-122.057944&spn=0.000392,0.000603&t=h&z=21
• Sun path diagram (Appendix B)
• UCSC Tracker
– Online tracker controller (Use from my computer)
– Archived daily insolation (10/15/10, 10/17/10)
1. Compare the archived insolation data on 10/15/2010 with your
prediction based on clear-sky insolation calculations. Complete the
table below (each team pick a different time) and discuss the
differences.
2. Discuss which parameters could be adjusted to improve the fit of the
model. Adjust these parameters in your model for solar noon to
improve fit to the data and report the optimal adjustment.
3. Compare the observations and calculations from #1 with expected
values based on insolation data in the appendix of Masters (2004).
Quantity Symbol
Day Number n
Latitude, deg. L
Collector azimuth, deg φc
Collector tilt Σ
Solar time, 24 hr ST
Hour angle H
Declination,deg δ
Altitude angle β
Solar azimuth φs
Air mass ratio m
Appar.ET fluxW/m2 A
Optical depth k
Beam radiation, W/m2 IB
Incidence angle cos(θ)
Beam on collector, W/m2 IBC
Sky diffuse factor C
Diffuse rad on collector, W/m2 IDC
Adding Reflected
Reflectance ρ
Reflec. Rad on collector W/m2 IRC
Total I (IBC+IDC+IRC) W/m2 IC
4. Use Google maps and a sun-path diagram to estimate the timing of
obstructions in the afternoon.
5. Does your sun-path diagram analysis agree with the measured data?
6. What percent of the potentially collected energy is lost during January,
June and October in the afternoon?
1. Compare the archived insolation data on 10/15/2010 with what insolation
values you would predict from calculations by completing the following
table.
Measured vs. Predicted
• Total insolation is similar between measurements and predictions
• However the model does a poor job of predicting the partitioning to direct and
diffuse insolation
0
200
400
600
800
1000
6 7 8 9 10 11 12 13 14 15 16 17 18
Appendix
Simulated Direct
Simulated Total
Class - Total
Class - Direct
2. Comment on the reason for the difference and on what parameter
adjustments might be required to obtain a better match.
1. Larger optical depth (k) to get less direct.
2. Larger sky diffuse factor (C) to get more diffuse
0
200
400
600
800
1000
1200
Measured Model (k = 0.171, C = 0.092) Model (k = 0.45, C = 0.75)
Insolation(W/m^2)
Total
Direct
Diffuse
3. Compare the observations and calculations from #1 with expected values
based on Appendix of your text book. 996 kW/m2 (Appendix C: Hourly
clear-sky Insolation Tables).
0
200
400
600
800
1000
6 7 8 9 10 11 12 13 14 15 16 17 18
Appendix
Simulated Direct
Simulated Total
4. Use Google maps and a sun-path diagram to estimate the timing of
obstructions in the afternoon.
Azimuth of obstruction (φ): Altitude angle of obstruction (β):
φ = -tan-1(Y/X) = -58°
φX
Y
Z
Height (H) roughly 9 meters
β = tan-1(H/Z) = 72°
4. Use Google maps and a sun-path diagram to estimate the timing of
obstructions in the afternoon.
5. Does your sun-path diagram analysis agree with the measured data?
6. What percent of the potentially collected energy is lost during October
and June due to obstructions in the afternoon?
October: 10% loss in daily energy due to afternoon obstructions
June: 45% loss in daily energy due to afternoon obstructions
The component of insolation that has
the most insolation during clear-sky
conditions is
1. Diffuse
2. Direct-beam
3. Reflected
Solar altitude angle is
1. The angle between the incoming direct sunlight and
a plane normal to the earth’s surface.
2. The angle between the incoming direct sunlight and
the equator.
3. The angle between due south and the location of an
obstruction to a solar collector.
Applying clear-sky insolation theory
during cloudy conditions
1. may underestimate optical depth and result in an
overestimate of direct insolation.
2. may underestimate the sky diffuse factor and result
in an underestimate of diffuse insolation.
3. may overestimate the air mass ratio and result in
an underestimate of direct insolation.
4. Both 1 and 2.
The pyrheliometer measurements (blue line)
represent what component(s) of insolation ?
1. Direct
2. Diffuse
3. Direct + Diffuse + Reflected
Anonymous Survey
http://www.surveymonkey.com/s/R6WT33Z

More Related Content

What's hot

Welcome to International Journal of Engineering Research and Development (IJERD)
Welcome to International Journal of Engineering Research and Development (IJERD)Welcome to International Journal of Engineering Research and Development (IJERD)
Welcome to International Journal of Engineering Research and Development (IJERD)IJERD Editor
 
Fractional approaches in dielectric broadband spectroscopy
Fractional approaches in dielectric broadband spectroscopyFractional approaches in dielectric broadband spectroscopy
Fractional approaches in dielectric broadband spectroscopySimon Candelaresi
 
Deep Impact Poster Revised
Deep Impact Poster RevisedDeep Impact Poster Revised
Deep Impact Poster RevisedAlejandro Cota
 
A Study on the Development of High Accuracy Solar Tracking Systems
A Study on the Development of High Accuracy Solar Tracking SystemsA Study on the Development of High Accuracy Solar Tracking Systems
A Study on the Development of High Accuracy Solar Tracking Systemsiskandaruz
 
Michael_Tierney_INAM_SURE_2
Michael_Tierney_INAM_SURE_2Michael_Tierney_INAM_SURE_2
Michael_Tierney_INAM_SURE_2Michael Tierney
 
Estimating natural illumination from a single outdoor scene final
Estimating natural illumination from a single outdoor scene   finalEstimating natural illumination from a single outdoor scene   final
Estimating natural illumination from a single outdoor scene finalDebaleena Chattopadhyay
 
Magnetic Field Line Tangling and Topological Entropy
Magnetic Field Line Tangling and Topological EntropyMagnetic Field Line Tangling and Topological Entropy
Magnetic Field Line Tangling and Topological EntropySimon Candelaresi
 
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...IAEME Publication
 
Satellite Mapping
Satellite MappingSatellite Mapping
Satellite MappingPinus57
 
TH3.TO4.3.ppt
TH3.TO4.3.pptTH3.TO4.3.ppt
TH3.TO4.3.pptgrssieee
 
3D Cloud Visualizations
3D Cloud Visualizations3D Cloud Visualizations
3D Cloud VisualizationsJohn Pham
 
Adjoint Radiosity Borel Earsel09 2 11 09 White
Adjoint Radiosity Borel Earsel09 2 11 09 WhiteAdjoint Radiosity Borel Earsel09 2 11 09 White
Adjoint Radiosity Borel Earsel09 2 11 09 Whiteguest0030172
 
Measuring and colouring M87
Measuring and colouring M87Measuring and colouring M87
Measuring and colouring M87Nelson Correia
 

What's hot (20)

Welcome to International Journal of Engineering Research and Development (IJERD)
Welcome to International Journal of Engineering Research and Development (IJERD)Welcome to International Journal of Engineering Research and Development (IJERD)
Welcome to International Journal of Engineering Research and Development (IJERD)
 
Fractional approaches in dielectric broadband spectroscopy
Fractional approaches in dielectric broadband spectroscopyFractional approaches in dielectric broadband spectroscopy
Fractional approaches in dielectric broadband spectroscopy
 
Deep Impact Poster Revised
Deep Impact Poster RevisedDeep Impact Poster Revised
Deep Impact Poster Revised
 
A Study on the Development of High Accuracy Solar Tracking Systems
A Study on the Development of High Accuracy Solar Tracking SystemsA Study on the Development of High Accuracy Solar Tracking Systems
A Study on the Development of High Accuracy Solar Tracking Systems
 
Michael_Tierney_INAM_SURE_2
Michael_Tierney_INAM_SURE_2Michael_Tierney_INAM_SURE_2
Michael_Tierney_INAM_SURE_2
 
Estimating natural illumination from a single outdoor scene final
Estimating natural illumination from a single outdoor scene   finalEstimating natural illumination from a single outdoor scene   final
Estimating natural illumination from a single outdoor scene final
 
Magnetic Field Line Tangling and Topological Entropy
Magnetic Field Line Tangling and Topological EntropyMagnetic Field Line Tangling and Topological Entropy
Magnetic Field Line Tangling and Topological Entropy
 
IJET-V3I1P5
IJET-V3I1P5IJET-V3I1P5
IJET-V3I1P5
 
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...
EMPLOYING MULTI CORE ARCHITECTURE TO OPTIMIZE ON PERFORMANCE, FOR APPROACH IN...
 
Satellite Mapping
Satellite MappingSatellite Mapping
Satellite Mapping
 
12 3-2014 atsoa.ppt
12 3-2014 atsoa.ppt12 3-2014 atsoa.ppt
12 3-2014 atsoa.ppt
 
TH3.TO4.3.ppt
TH3.TO4.3.pptTH3.TO4.3.ppt
TH3.TO4.3.ppt
 
Ge3111891192
Ge3111891192Ge3111891192
Ge3111891192
 
AAS_Poster
AAS_PosterAAS_Poster
AAS_Poster
 
UST_inquiry_Poster
UST_inquiry_PosterUST_inquiry_Poster
UST_inquiry_Poster
 
3D Cloud Visualizations
3D Cloud Visualizations3D Cloud Visualizations
3D Cloud Visualizations
 
Adjoint Radiosity Borel Earsel09 2 11 09 White
Adjoint Radiosity Borel Earsel09 2 11 09 WhiteAdjoint Radiosity Borel Earsel09 2 11 09 White
Adjoint Radiosity Borel Earsel09 2 11 09 White
 
GRL99
GRL99GRL99
GRL99
 
D04722440
D04722440D04722440
D04722440
 
Measuring and colouring M87
Measuring and colouring M87Measuring and colouring M87
Measuring and colouring M87
 

Viewers also liked

Introduction to nanoscience and nanotechnology
Introduction to nanoscience and nanotechnologyIntroduction to nanoscience and nanotechnology
Introduction to nanoscience and nanotechnologyMazhar Laliwala
 
Nanotech presentation
Nanotech presentationNanotech presentation
Nanotech presentationjayly03
 
Nanotechnology: Basic introduction to the nanotechnology.
Nanotechnology: Basic introduction to the nanotechnology.Nanotechnology: Basic introduction to the nanotechnology.
Nanotechnology: Basic introduction to the nanotechnology.Sathya Sujani
 
Nano Technology
Nano TechnologyNano Technology
Nano TechnologyZeusAce
 
Solar Energy Presentation
Solar Energy PresentationSolar Energy Presentation
Solar Energy PresentationKurt Kublbeck
 
Nanotechnology
NanotechnologyNanotechnology
NanotechnologyKANNAN
 
Solar energy power point presentation
Solar energy power point presentation Solar energy power point presentation
Solar energy power point presentation Shrijeet Modi
 
Solar panel Technology ppt
Solar panel Technology pptSolar panel Technology ppt
Solar panel Technology pptGourav Kumar
 
NANOTECHNOLOGY AND IT'S APPLICATIONS
NANOTECHNOLOGY AND IT'S APPLICATIONSNANOTECHNOLOGY AND IT'S APPLICATIONS
NANOTECHNOLOGY AND IT'S APPLICATIONSCHINMOY PAUL
 
Solar energy ppt
Solar energy pptSolar energy ppt
Solar energy pptshubhajit_b
 
Presentation on solar cell
Presentation on solar cellPresentation on solar cell
Presentation on solar cellOmar SYED
 

Viewers also liked (14)

Introduction to nanoscience and nanotechnology
Introduction to nanoscience and nanotechnologyIntroduction to nanoscience and nanotechnology
Introduction to nanoscience and nanotechnology
 
Nanotech presentation
Nanotech presentationNanotech presentation
Nanotech presentation
 
Nanotechnology: Basic introduction to the nanotechnology.
Nanotechnology: Basic introduction to the nanotechnology.Nanotechnology: Basic introduction to the nanotechnology.
Nanotechnology: Basic introduction to the nanotechnology.
 
Nano technology
Nano technologyNano technology
Nano technology
 
Nano Technology
Nano TechnologyNano Technology
Nano Technology
 
Solar Energy Presentation
Solar Energy PresentationSolar Energy Presentation
Solar Energy Presentation
 
Nanotechnology
NanotechnologyNanotechnology
Nanotechnology
 
Solar energy power point presentation
Solar energy power point presentation Solar energy power point presentation
Solar energy power point presentation
 
Nanotechnology ppt
Nanotechnology pptNanotechnology ppt
Nanotechnology ppt
 
Solar panel Technology ppt
Solar panel Technology pptSolar panel Technology ppt
Solar panel Technology ppt
 
NANOTECHNOLOGY AND IT'S APPLICATIONS
NANOTECHNOLOGY AND IT'S APPLICATIONSNANOTECHNOLOGY AND IT'S APPLICATIONS
NANOTECHNOLOGY AND IT'S APPLICATIONS
 
Solar energy ppt
Solar energy pptSolar energy ppt
Solar energy ppt
 
Solar Energy
Solar EnergySolar Energy
Solar Energy
 
Presentation on solar cell
Presentation on solar cellPresentation on solar cell
Presentation on solar cell
 

Similar to Solar trackersolution

Irsolav Methodology 2013
Irsolav Methodology 2013Irsolav Methodology 2013
Irsolav Methodology 2013IrSOLaV Pomares
 
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES  A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES Roberto Valer
 
Remote sensing in space krishna
Remote sensing in space krishnaRemote sensing in space krishna
Remote sensing in space krishnaKrishna Gaihre
 
Coulter_JPL_Poster_Final
Coulter_JPL_Poster_FinalCoulter_JPL_Poster_Final
Coulter_JPL_Poster_FinalDave Coulter
 
Estimation of diffuse solar radiation in the south of cameroon
Estimation of diffuse solar radiation in the south of cameroonEstimation of diffuse solar radiation in the south of cameroon
Estimation of diffuse solar radiation in the south of cameroonAlexander Decker
 
46 optimization paper id 0017 edit septian
46 optimization paper id 0017 edit septian46 optimization paper id 0017 edit septian
46 optimization paper id 0017 edit septianIAESIJEECS
 
Use of satellite imageries in weather forecasting
Use of satellite imageries in weather forecastingUse of satellite imageries in weather forecasting
Use of satellite imageries in weather forecastingDK27497
 
System testing for the fresnel lens-based optical
System testing for the fresnel lens-based opticalSystem testing for the fresnel lens-based optical
System testing for the fresnel lens-based opticalJuan Milton Garduno Rubio
 
MC2016_Lazaridou_Konstantina
MC2016_Lazaridou_KonstantinaMC2016_Lazaridou_Konstantina
MC2016_Lazaridou_KonstantinaNadia Lazaridou
 
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...Sérgio Sacani
 
Computational Physics Final Report (MATLAB)
Computational Physics Final Report (MATLAB)Computational Physics Final Report (MATLAB)
Computational Physics Final Report (MATLAB)Ricardo Fritzke
 
420 16-meshram (1)
420 16-meshram (1)420 16-meshram (1)
420 16-meshram (1)Ahson Khan
 
Design and performance evaluation of a solar tracking panel of single axis in...
Design and performance evaluation of a solar tracking panel of single axis in...Design and performance evaluation of a solar tracking panel of single axis in...
Design and performance evaluation of a solar tracking panel of single axis in...IJECEIAES
 
VHR_preliminary-system_study_issue2
VHR_preliminary-system_study_issue2VHR_preliminary-system_study_issue2
VHR_preliminary-system_study_issue2Stefano Coltellacci
 

Similar to Solar trackersolution (20)

Aee036
Aee036Aee036
Aee036
 
Irsolav Methodology 2013
Irsolav Methodology 2013Irsolav Methodology 2013
Irsolav Methodology 2013
 
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES  A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES
A PHYSICAL METHOD TO COMPUTE SURFACE RADIATION FROM GEOSTATIONARY SATELLITES
 
AIAA Paper dlt228
AIAA Paper dlt228AIAA Paper dlt228
AIAA Paper dlt228
 
Remote sensing in space krishna
Remote sensing in space krishnaRemote sensing in space krishna
Remote sensing in space krishna
 
Coulter_JPL_Poster_Final
Coulter_JPL_Poster_FinalCoulter_JPL_Poster_Final
Coulter_JPL_Poster_Final
 
Thermal2
Thermal2Thermal2
Thermal2
 
43 hendrik holst_modelling_of_the_expected_yearly_power_yield_on_building_fac...
43 hendrik holst_modelling_of_the_expected_yearly_power_yield_on_building_fac...43 hendrik holst_modelling_of_the_expected_yearly_power_yield_on_building_fac...
43 hendrik holst_modelling_of_the_expected_yearly_power_yield_on_building_fac...
 
Estimation of diffuse solar radiation in the south of cameroon
Estimation of diffuse solar radiation in the south of cameroonEstimation of diffuse solar radiation in the south of cameroon
Estimation of diffuse solar radiation in the south of cameroon
 
46 optimization paper id 0017 edit septian
46 optimization paper id 0017 edit septian46 optimization paper id 0017 edit septian
46 optimization paper id 0017 edit septian
 
Use of satellite imageries in weather forecasting
Use of satellite imageries in weather forecastingUse of satellite imageries in weather forecasting
Use of satellite imageries in weather forecasting
 
System testing for the fresnel lens-based optical
System testing for the fresnel lens-based opticalSystem testing for the fresnel lens-based optical
System testing for the fresnel lens-based optical
 
MC2016_Lazaridou_Konstantina
MC2016_Lazaridou_KonstantinaMC2016_Lazaridou_Konstantina
MC2016_Lazaridou_Konstantina
 
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...
New Post-DART Collision Period for the Didymos System: Evidence for Anomalous...
 
Solar Irradiance
Solar IrradianceSolar Irradiance
Solar Irradiance
 
Computational Physics Final Report (MATLAB)
Computational Physics Final Report (MATLAB)Computational Physics Final Report (MATLAB)
Computational Physics Final Report (MATLAB)
 
09 huld presentation_61853_4_a
09 huld presentation_61853_4_a09 huld presentation_61853_4_a
09 huld presentation_61853_4_a
 
420 16-meshram (1)
420 16-meshram (1)420 16-meshram (1)
420 16-meshram (1)
 
Design and performance evaluation of a solar tracking panel of single axis in...
Design and performance evaluation of a solar tracking panel of single axis in...Design and performance evaluation of a solar tracking panel of single axis in...
Design and performance evaluation of a solar tracking panel of single axis in...
 
VHR_preliminary-system_study_issue2
VHR_preliminary-system_study_issue2VHR_preliminary-system_study_issue2
VHR_preliminary-system_study_issue2
 

Solar trackersolution

  • 1. Solar Resource Lab Learning Goal • Students will be able to understand sources of variation in insolation, construct insolation forecasting models, validate these models with solar radiation measurements, and gain an appreciation for solar forecasting as an intriguing challenge for the design of renewable energy systems. Learning Outcome • Forecast seasonal and daily variation in insolation on a collector surface using clear-sky insolation theory. • Estimate model error using pyrheliometer and pyranometer measurements. • Propose plausible sources of error in model and derive optimal parameter estimates. • Predict the quantity and timing of insolation losses due to obstructions using site maps and sun-path diagrams.
  • 2. P1) The component of insolation that has the most insolation during clear- sky conditions is 1. Diffuse 2. Direct-beam 3. Reflected
  • 3. P2) Solar altitude angle is 1. The angle between the incoming direct sunlight and a plane normal to the earth’s surface. 2. The angle between the incoming direct sunlight and the equator. 3. The angle between due south and the location of an obstruction to a solar collector.
  • 4. P3) Applying clear-sky insolation theory during cloudy conditions 1. may underestimate optical depth and result in an overestimate of direct insolation. 2. may underestimate the sky diffuse factor and result in an underestimate of diffuse insolation. 3. may overestimate the air mass ratio and result in an underestimate of direct insolation. 4. Both 1 and 2.
  • 5. P4) The pyrheliometer measurements (blue line) represent what component(s) of insolation ? 1. Direct 2. Diffuse 3. Direct + Diffuse + Reflected
  • 7.
  • 8.
  • 11.
  • 12.
  • 14. Tools and Data • Clear-sky insolation theory (Masters, 2004) • Google maps : 37.414319,-122.0579 Lat / Lon http://maps.google.com/?ie=UTF8&ll=37.414319,-122.057944&spn=0.000392,0.000603&t=h&z=21 • Sun path diagram (Appendix B) • UCSC Tracker – Online tracker controller (Use from my computer) – Archived daily insolation (10/15/10, 10/17/10)
  • 15. 1. Compare the archived insolation data on 10/15/2010 with your prediction based on clear-sky insolation calculations. Complete the table below (each team pick a different time) and discuss the differences. 2. Discuss which parameters could be adjusted to improve the fit of the model. Adjust these parameters in your model for solar noon to improve fit to the data and report the optimal adjustment. 3. Compare the observations and calculations from #1 with expected values based on insolation data in the appendix of Masters (2004). Quantity Symbol Day Number n Latitude, deg. L Collector azimuth, deg φc Collector tilt Σ Solar time, 24 hr ST Hour angle H Declination,deg δ Altitude angle β Solar azimuth φs Air mass ratio m Appar.ET fluxW/m2 A Optical depth k Beam radiation, W/m2 IB Incidence angle cos(θ) Beam on collector, W/m2 IBC Sky diffuse factor C Diffuse rad on collector, W/m2 IDC Adding Reflected Reflectance ρ Reflec. Rad on collector W/m2 IRC Total I (IBC+IDC+IRC) W/m2 IC
  • 16. 4. Use Google maps and a sun-path diagram to estimate the timing of obstructions in the afternoon. 5. Does your sun-path diagram analysis agree with the measured data? 6. What percent of the potentially collected energy is lost during January, June and October in the afternoon?
  • 17. 1. Compare the archived insolation data on 10/15/2010 with what insolation values you would predict from calculations by completing the following table.
  • 18. Measured vs. Predicted • Total insolation is similar between measurements and predictions • However the model does a poor job of predicting the partitioning to direct and diffuse insolation 0 200 400 600 800 1000 6 7 8 9 10 11 12 13 14 15 16 17 18 Appendix Simulated Direct Simulated Total Class - Total Class - Direct
  • 19. 2. Comment on the reason for the difference and on what parameter adjustments might be required to obtain a better match. 1. Larger optical depth (k) to get less direct. 2. Larger sky diffuse factor (C) to get more diffuse 0 200 400 600 800 1000 1200 Measured Model (k = 0.171, C = 0.092) Model (k = 0.45, C = 0.75) Insolation(W/m^2) Total Direct Diffuse
  • 20. 3. Compare the observations and calculations from #1 with expected values based on Appendix of your text book. 996 kW/m2 (Appendix C: Hourly clear-sky Insolation Tables). 0 200 400 600 800 1000 6 7 8 9 10 11 12 13 14 15 16 17 18 Appendix Simulated Direct Simulated Total
  • 21. 4. Use Google maps and a sun-path diagram to estimate the timing of obstructions in the afternoon. Azimuth of obstruction (φ): Altitude angle of obstruction (β): φ = -tan-1(Y/X) = -58° φX Y Z Height (H) roughly 9 meters β = tan-1(H/Z) = 72°
  • 22. 4. Use Google maps and a sun-path diagram to estimate the timing of obstructions in the afternoon. 5. Does your sun-path diagram analysis agree with the measured data?
  • 23. 6. What percent of the potentially collected energy is lost during October and June due to obstructions in the afternoon? October: 10% loss in daily energy due to afternoon obstructions June: 45% loss in daily energy due to afternoon obstructions
  • 24. The component of insolation that has the most insolation during clear-sky conditions is 1. Diffuse 2. Direct-beam 3. Reflected
  • 25. Solar altitude angle is 1. The angle between the incoming direct sunlight and a plane normal to the earth’s surface. 2. The angle between the incoming direct sunlight and the equator. 3. The angle between due south and the location of an obstruction to a solar collector.
  • 26. Applying clear-sky insolation theory during cloudy conditions 1. may underestimate optical depth and result in an overestimate of direct insolation. 2. may underestimate the sky diffuse factor and result in an underestimate of diffuse insolation. 3. may overestimate the air mass ratio and result in an underestimate of direct insolation. 4. Both 1 and 2.
  • 27. The pyrheliometer measurements (blue line) represent what component(s) of insolation ? 1. Direct 2. Diffuse 3. Direct + Diffuse + Reflected

Editor's Notes

  1. Remind students of motivation. Urgently need to develop models for forecasting solar insolation as a critical component of designing renewable energy systems. Forecasting models are required at multiple temporal scales (second, hours, days, years, decades) to design and operate renewable energy systems. While this class focuses on clear-sky insolation theory we have also discussed more complex models that are being developed at the frontiers of sustainable energy research.
  2. Julie Shattuck is conducting assessment
  3. Total insolation stays constant but the fraction of diffuse and of direct are highly variable
  4. Note different scales on y-axis
  5. Real-time data*Image: what does the sky look like? A little cloudy.*Azimuth (φS)is 153… but civil time is 10:33. Does this seem correct? *ask them def of solar azimuth *but in REEPS it is defined as degrees away from due south with degrees in east direction as positive and degrees in west direction as negative *so based on REEPS def what would you expect the solar azimuth to be at 10:33 in mountain view, California… 20 degrees … this doesn’t agree with 153. *reason is that alternative definition is angle from due north in clockwise direction. *If the north/clockwise definition is used for 153 then what angle would that be with our south definition? 153-180 = -27; UCSC-180 = REEPS*Altitude: altitude angle (β). *Currently is two-axis tracker but can adjust the orientation by enter new values in the boxes.*PSP: Pyranometer measurements in W/m^2 . Psp stands for precision spectral pyranometer. Thermopile sensor. What does this measure? Total radiation on the collector surface (direct + diffuse + reflected)*NIP: Pyrheliometer in W/m^2. NIP stands for Normal Incidence Pyrheliometer. Thermopile sensor. What does it measure? Direct sunlight. *IV Curve is something we cover in the next section of course.
  6. Make a table on the board that has: solar time, collector azimuth, collector title, altitude angle, solar azimuth, air mass ratio, direct normal, direct collector, diffuse collectorWhen walking around the room have the students check their calculator with the sample data provided in 7.15 which is one of their HW questionsWrite students results on this plot
  7. Small between calculations and appendix due to slightly different latitude and date from appendix.
  8. Check the beta calc… in class we found tree is 48 ft and z = 43 ft and beta of 48 deg
  9. Should agree… we see obstruction around 3:30 until sunset in sun path and 3pm in measurements. If we had used the edge of the tree instead of the center of the tree then probably would have much closer agreement.Draw the box on the sun-path diagram
  10. Discuss the 30min gap between blockage of diffuse and blockage of total.