PV 2012/2013. Radiation from the Sun Atmospheric effects Insolation maps Tracking the Sun PV in urban environment

Similar documents
Solar resource. Radiation from the Sun Atmospheric effects Insolation maps Tracking the Sun PV in urban environment

Exercise 6. Solar Panel Orientation EXERCISE OBJECTIVE DISCUSSION OUTLINE. Introduction to the importance of solar panel orientation DISCUSSION

Solar Radiation Measurements and Model Calculations at Inclined Surfaces

Photovoltaic potential in a Lisbon suburb using LiDAR data

Uncertainties in solar electricity yield prediction from fluctuation of solar radiation

ME 476 Solar Energy UNIT THREE SOLAR RADIATION

Chapter 1 Solar Radiation

Motion of the Sun. View Comments

Calculating equation coefficients

Photovoltaic Systems Solar Radiation

1. SOLAR GEOMETRY, EXTRATERRESTRIAL IRRADIANCE & INCIDENCE ANGLES

FLATE Hillsborough Community College - Brandon (813)

Sunlight and its Properties Part I. EE 446/646 Y. Baghzouz

PHOTOVOLTAIC SOLAR ENERGY TRAINER DL SOLAR-D1 Manual

Chapter 2 Available Solar Radiation

Solutions Manual to Exercises for Weather & Climate, 8th ed. Appendix A Dimensions and Units 60 Appendix B Earth Measures 62 Appendix C GeoClock 63

Mr Riaan Meyer On behalf of Centre for Renewable and Sustainable Energy Studies University of Stellenbosch

Lecture 3: Global Energy Cycle

COMPUTER PROGRAM FOR THE ANGLES DESCRIBING THE SUN S APPARENT MOVEMENT IN THE SKY

ME 430 Fundamentals of Solar Energy Conversion for heating and Cooling Applications

Chapter Seven. Solar Energy

Which Earth latitude receives the greatest intensity of insolation when Earth is at the position shown in the diagram? A) 0 B) 23 N C) 55 N D) 90 N

Chapter 3. Multiple Choice Questions

Lecture #03. January 20, 2010, Wednesday

4. Solar radiation on tilted surfaces

MAPH & & & & & & 02 LECTURE

Seasonal & Daily Temperatures

1/55. Solar energy. solar radiation definitions incident solar energy

EE Properties of Sunlight. Y. Baghzouz Professor of Electrical Engineering

Introduction to Photovoltaics

STANDARD. S6E1 d. Explain the motion of objects in the day/night sky in terms of relative position.

HEATING THE ATMOSPHERE

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

THE SOLAR RESOURCE: PART I MINES ParisTech Center Observation, Impacts, Energy (Tel.: +33 (0) )

Direct Normal Radiation from Global Radiation for Indian Stations

The Celestial Sphere. Chapter 1. Constellations. Models and Science. Constellations. Diurnal vs. Annular Motion 9/16/2010

L.O: EARTH'S 23.5 DEGREE TILT ON ITS AXIS GIVES EARTH ITS SEASONS March 21 (SPRING), June 21(SUMMER), Sept 22 (AUTUMN) & Dec 21(WINTER)

Earth s Orbit. Sun Earth Relationships Ridha Hamidi, Ph.D. ESCI-61 Introduction to Photovoltaic Technology

Earth-Sun Relationships. The Reasons for the Seasons

Insolation and Temperature variation. The Sun & Insolation. The Sun (cont.) The Sun

Observer-Sun Angles. ), Solar altitude angle (α s. ) and solar azimuth angle (γ s )). θ z. = 90 o α s

Basic information about developed Calculator for solar / wind hybrid power supply

OPTIMIZATION OF GLOBAL SOLAR RADIATION OF TILT ANGLE FOR SOLAR PANELS, LOCATION: OUARGLA, ALGERIA

1/71 AES-LECTURE 1. Solar energy. solar radiation definitions incident solar energy

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

The Atmosphere. Importance of our. 4 Layers of the Atmosphere. Introduction to atmosphere, weather, and climate. What makes up the atmosphere?

XI. DIFFUSE GLOBAL CORRELATIONS: SEASONAL VARIATIONS

C) the seasonal changes in constellations viewed in the night sky D) The duration of insolation will increase and the temperature will increase.

Time Series Model of Photovoltaic Generation for Distribution Planning Analysis. Jorge Valenzuela

Solar Insolation and Earth Radiation Budget Measurements

Seasonal & Diurnal Temp Variations. Earth-Sun Distance. Eccentricity 2/2/2010. ATS351 Lecture 3

CLASSICS. Handbook of Solar Radiation Data for India

Bi-annual Sun Tracking for Solar PV Module Support Structure: Study and Implementation

38 B Our Environment. Ederlinda Viñuales Gavín Marco Nicolini. Sun Exposition &

2.626 Fundamentals of Photovoltaics

Sunlight and its Properties II. EE 446/646 Y. Baghzouz

Solar Radiation in Thailand:

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D)

Integrating the Solar Spectrum

Characterization of the solar irradiation field for the Trentino region in the Alps

C) wavelength C) eastern horizon B) the angle of insolation is high B) increases, only D) thermosphere D) receive low-angle insolation

C2: NĂNG LƯỢNG ĐIỆN MẶT TRỜI

Celestial Sphere & Solar Motion Lab (Norton s Star Atlas pages 1-4)

Purdue University Bifacial Module Calculator (PUB)

atmospheric influences on insolation & the fate of solar radiation interaction of terrestrial radiation with atmospheric gases

AVAILABLE SOLAR RADIATION THEORETICAL BACKGROUND

Basic human requirements

THE AVERAGE TOTAL DAYLIGHT FACTOR

Meteorology Practice Test

What is Climate? Understanding and predicting climatic changes are the basic goals of climatology.

Data and formulas at the end. Exam would be Weds. May 8, 2008

CONSTRUCTION AND CALIBRATION OF A LOCAL PYRANOMETER AND ITS USE IN THE MEASUREMENT OF INTENSITY OF SOLAR RADIATION

Determination of Optimum Fixed and Adjustable Tilt Angles for Solar Collectors by Using Typical Meteorological Year data for Turkey

Which table correctly shows the dates on which the apparent paths of the Sun were observed? A) B) C) D)

Practice Questions: Seasons #1

BMM4753 RENEWABLE ENERGY RESOURCES

Global Solar Dataset for PV Prospecting. Gwendalyn Bender Vaisala, Solar Offering Manager for 3TIER Assessment Services

1. Weather and climate.

Chapter 11 Lecture Outline. Heating the Atmosphere

SURFACE ORIENTATIONS AND ENERGY POLICY FOR SOLAR MODULE APPLICATIONS IN DHAKA, BANGLADESH

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

The Sky Perceptions of the Sky

Why the Earth has seasons. Why the Earth has seasons 1/20/11

Online data and tools for estimation of solar electricity in Africa: the PVGIS approach

P1.34 MULTISEASONALVALIDATION OF GOES-BASED INSOLATION ESTIMATES. Jason A. Otkin*, Martha C. Anderson*, and John R. Mecikalski #

CCMR Educational Programs

Fundamentals of Satellite technology

The Atmosphere: Structure and Temperature

Solar Time, Angles, and Irradiance Calculator: User Manual

9/1/14. Chapter 2: Heating Earth s Surface and Atmosphere. The Atmosphere: An Introduction to Meteorology, 12 th. Lutgens Tarbuck

Lecture 2: Global Energy Cycle

ATMOSPHERIC CIRCULATION AND WIND

PHYS 4400, Principles and Varieties of Solar Energy Instructor: Randy J. Ellingson The University of Toledo

LESSON PLAN - Optimum Orientation of Solar Panels Using Soltrex Data

A New Angle on Energy Optimization of a microfit PV System

Earth is tilted (oblique) on its Axis!

Earth s Motion. Lesson Outline LESSON 1. A. Earth and the Sun 1. The diameter is more than 100 times greater than

Evaluation of long-term global radiation measurements in Denmark and Sweden

November 20, NOTES ES Rotation, Rev, Tilt.notebook. vertically. night. night. counterclockwise. counterclockwise. East. Foucault.

SEASONAL AND DAILY TEMPERATURES

Transcription:

SOLAR RESOURCE Radiation from the Sun Atmospheric effects Insolation maps Tracking the Sun PV in urban environment 1

is immense Human energy use: 4.0x10 14 kwh/year on Earth s surface: 5.5x10 17 kwh/year is immense Human energy use: 4.0x10 14 kwh/year on Earth s surface: 5.5x10 17 kwh/year ia.org/wiki/file:solar_land_area.png http://en.wikiped Local solar irradiance averaged over three years from 1991 to 1993 (24 hours a day) taking into account the cloud coverage available from weather satellites Solar power systems covering the areas defined by the dark disks could provide more than the world's total primary energy demand (assuming a conversion efficiency of 8%). 2

is immense Human energy use: 4.0x10 14 kwh/year on Earth s surface: 5.5x10 17 kwh/year is global and democratic is relatively constant but depends on atmospheric effects, including absorption and scattering local variations in the atmosphere, such as water vapour, clouds, and pollution latitude of the location the season of the year and the time of day P 0 T 4 2 4 Rsun Total radiative power (Stefan Boltzman) T=5762K Surface area of sun Power radiated per unit area 5.96x10 7 W/m 2 3

P 0 T 4 2 4 Rsun Ratio of surface areas of the 2 spheres Solar constant average energy flux incident at the Earth s orbit: 1366 W/m 2 4 R S 4 D 2 sun 2 P 0 Distance Sun-Earth P 0 T 4 2 4 Rsun R sun D avg R Earth 6.96x10 5 km 1.5x10 8 km 6.35x10 3 km Energy incident on Earth Total area of Earth 4 R S 4 D S R 2 4 R 2 Earth Earth 2 sun 2 P 0 S 4 Average energy incident per unit area of surface of Earth: 342 W/m 2 4

Earth-Sun motion 23.7 º Polar axis 365 days and 6 hours H 360n 2 1 0.033cos S 365 H(W/m2) is radiant power density outside the atmosphere; S is solar constant; n is day of the year Earth-Sun motion Solar declination: angle between line joining centres of Earth and Sun and the equatorial plane Polar axis 0º +23º 27 5

Earth-Sun motion Solar declination: angle between line joining centres of Earth and Sun and the equatorial plane Polar axis 0º +23º 27 Autumnal equinox Earth-Sun motion Solar declination: angle between line joining centres of Earth and Sun and the equatorial plane Polar axis 0º +23º 27 Autumnal equinox -23º 27 6

Earth-Sun motion Solar declination: angle between line joining centres of Earth and Sun and the equatorial plane Polar axis +23º 27 0º Vernal and automnal equinox -23º 27 Earth-Sun motion Solar declination: angle between line joining centres of Earth and Sun and the equatorial plane the equatorial plane 23.45 284 n sin2 180 365 Declination in radians; n is the number of the day (Jan 1st = 1) 7

Earth-Sun motion sin sin sin cos cos sin sin sin cos cos cos 0º solar azimuth S 0º solar elevation 90º O N E -90º Optimum orientation: facing south (north in the southern hemisphere) Optimum inclination: local latitude but not quite 8

Atmospheric effects Atmospheric effects on solar radiation at the Earth's surface: a reduction in the power of the solar radiation due to absorption, scattering and reflection in the atmosphere; scattering and reflection in the atmosphere; a change in the spectral content of the solar radiation due to greater absorption or scattering of some wavelengths; the introduction of a diffuse or indirect component into the solar radiation; and local variations in the atmosphere (such as water vapour, clouds and pollution) which have additional effects on the incident power, spectrum and directionality. 9

Air Mass is a measure of the reduction in the power of light as it passes through the atmosphere and is absorbed by air and dust AM 1 cos 2.5 2.0 AM0 - Extraterrestrial Wm -2 nm -1 1.5 1.0 AM1.5 - Global AM1.5D - Direct 0.5 0.0 0 200 400 600 800 1000 1200 1400 1600 1800 2000 Wavelength (nm) 10

Wm -2 nm -1 2.5 2.0 1.5 1.0 0.5 Photon flux [photons/s/m 2 ] Power density H[W/m 2 ] Spectal irradiance F [W/m 2 /m] is the power density at a given (m) H F photons 2 m s hc 1.24 E m d F W hc H 2 m W hc F 2 2 m m 0 i0 0.0 0 200 400 600 800 1000 1200 1400 1600 1800 2000 Wavelength (nm) 11

Insolation: Incoming Solar Radiation Typical units: kwh/m 2 /day Affected by latitude, local weather patterns, Šúri M., Huld T.A., Dunlop E.D. Ossenbrink H.A., 2007. Potential of solar electricity generation in the European Union member states and candidate countries. Solar Energy, 81, 1295 1305, http://re.jrc.ec.europa.eu/pvgis/. 12

Yearly sum of global irradiation on vertical surface (kwh/m 2 ) period 1981-1990 13

Yearly sum of global irradiation on horizontal surface (kwh/m 2 ) period 1981-1990 Yearly sum of global irradiation on optimally-inclined surface (kwh/m 2 ) period 1981-1990 14

Yearly sum of global irradiation on 2-axis tracking surface (kwh/m 2 ) period 1981-1990 15

Coastal areas and higher mountains face wider variations (up to 10%) Winter is much more variable (up to x6) than summer months Šúri M., Huld T., Dunlop E.D., Albuisson M., Lefèvre M., Wald L., 2007. Uncertainties in photovoltaic electricity yield prediction from fluctuation of solar radiation. Proceedings of the 22nd European Photovoltaic Solar Energy Conference, Milano, Italy 3-7.9.2007 16

PV 2012/2013 Solar tracking Compared to PV with modules fixed at optimum angle: Changing inclination twice a year contributes only marginally Comparison of electricity yield from fixed and suntracking PV systems in Europe [JRC, 2008] Solar tracking Comparison of electricity yield from fixed and suntracking PV systems in Europe [JRC, 2008] 17

Solar tracking Comparison of electricity yield from fixed and suntracking PV systems in Europe [JRC, 2008] Solar tracking Compared to PV with modules fixed at optimum angle: Changing inclination twice a year contributes only marginally (2-4%) 1-axis tracking PV with vertical or South-inclined axis generates only 1-4% less than 2-axis tracking system 1-axis tracking PV with horizontal axis oriented E-W typically performs only slightly better than fixed mounting systems Comparison of electricity yield from fixed and suntracking PV systems in Europe [JRC, 2008] 18

180 360 Solar tracking 1.5x10-4 Hourly energy produced by PV system with 2-axes tracking [kwh/wp] 0 110º Incidence angle on fixed panel with optimum inclination 100% Ratio between energy produced using system with 2-axes tracking and fixed panel with optimum inclination. 0 12 24 Gaspar et al, Exploring One-Axis Tracking Configurations For CPV Application, CPV7, Las Vegas 2011 Configuration Tracking angle Incidente angle on PV receptor Energy produced compared with 2-axis tracking S N 0 180 360 0 12 24 90º -90º During the summer, in the North- South horizontal axis, the misalignment between module and the position of the sun reaches 40º. S N In a North-South inclined axis, the position of the module is perfect twice a year, in spring and autumn, and misalignment never exceeds 30º. E W Horizontal East-West axis is particularly suitable for midday hours, when insolation is at a maximum, but misses early and late hours. In a vertical axis with inclined panel, the misalignment will be lowest when the insolation is highest. Gaspar et al, Exploring One-Axis Tracking Configurations For CPV Application, CPV7, Las Vegas 2011 19

Solar tracking kwh/wp/year 2000 1500 1000 1635 1577 1537 1436 1269 1177 An inclined axis tracking system orientated in the north-south direction is able to closely follow the Sun 500 throughout the year, and have a relatively high acceptance for CPV applications. 0 The vertical 2-axes tracking, NS inclined with Vertical optimum NS horinclination, EW features Fixed a similar performance that an inclined axis tracking system orientated in the north-south direction. Gaspar et al, Exploring One-Axis Tracking Configurations For CPV Application, CPV7, Las Vegas 2011 Solar tracking 20

Solar tracking of blobal irradiation kwh/m2 350 300 250 200 150 Solar tracking PVGIS exercise: Lisbon Fixed angle 0º Fixed angle 33º Vertical axis 33º Inclined axis 33º 2-axis tracking Average sum of blobal irradiation kwh/m2 A 200% 150% 100% 50% 0% Fixed Fixed Vertical Inclined 2-axis angle 0º angle 33º axis 33º axis 33º tracking Average sum 100 50 0 1 2 3 4 5 6 7 8 9 10 11 12 Month 21

Solar tracking Shadowing effect Ground cover ratio = PV area / total area Inclined tracking 2-axis tracking Horizontal tracking GCR = PV density 1 /GCR E. Narvarte et al, Tracking and Ground Cover Ratio, Prog. Photovolt: Res. Appl. 2008; 16:703 714 PV in urban environment Carnaxide (38.43 N, 9.8 W) N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy 22

PV in urban environment N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy PV in urban environment N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy 23

PV in urban environment N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy PV in urban envir http://www.fcsh.unl.pt/e-geo/energiasolar/ 24

PV in urban envir http://www.fcsh.unl.pt/e-geo/energiasolar/ PV in urban envir http://www.lisboaenova.org/pt/cartasolarlisboa 25

PV in urban envir http://www.lisboaenova.org/pt/cartasolarlisboa PV in urban environment NW N 20% 15% NE Orientation distribution of roof area (black line). Irradiation distribution as a function of roof orientation (red line). 10% 5% W 0% E SW SE S Roof area Irradiation 100% 80% 93% 60% 58% Distribution of footprint area (dark boxes) and estimated population (white boxes) according to building typology. 40% 20% 0% 28% 14% 7% 0% House Flats Uninhabited N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy 26

PV in urban environment 100% 80% % available energy 60% 40% 24% 57% 20% 13% 0% 0% 20% 40% 60% 80% 100% % available area Fraction of available irradiation as a function of occupied roof area, for the SDM (black line) and TDM (red line). N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy PV in urban environment 115% 110% SDM/TDM 105% 102% 100% 95% 0% 20% 40% 60% 80% 100% % available area Ratio of cumulative irradiation for SDM and TDM as a function of occupied area (solid line). Red line indicates overall ratio (assuming 100% roof coverage) and dashed line indicates 100% for easier reading. N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy 27

PV in urban environment 2.0 1.8 16 1.6 1.64 1.4 MWh/m2/year 1.2 1.0 0.8 0.6 0.4 0.2 31% 0.0 0% 20% 40% 60% 80% 100% % available area Annual irradiation per unit area as a function of roof area. Dotted line indicates annual irradiation per unit area on a horizontal surface for the same location. N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy PV in urban environment Procedure for estimating the PV potential of an urban region using LiDAR data based on the Solar Analyst extension for ArcGIS. PV potential of the 538 buildings to be around 11.5 GWh/year for an installed capacity of 7MW, which corresponds to 48 % of the local electricity demand. For low PV penetration (about 10% of total roof area) the PV potential is well estimated by considering no shade and the local optimum inclination andorientation. For high PV penetration (i.e. covering close to all roof area) the PV potential is well estimated by considering a horizontal surface with the footprint area of the buildings. N. Gomes et al, PV potential in urban environment using LIDAR data, 2010, Solar Energy 28

PV in urban environment Each point of the DSM will cast a shadow along the line opposite to the position of the sun at that particular time. This shadow line is interrupted when a DSM cell along that line features a Z value higher that the shadow line at that position. P. Redweik et al, PV potential estimation using 3D local scale solar radiation model based on urban LIDAR data, PVSEC 2011 PV in urban environment Combining the shadow height for the façades with the shadow map for the ground. North is upwards. Shadows on January 1 st, at 9:00am. P. Redweik et al, PV potential estimation using 3D local scale solar radiation model based on urban LIDAR data, PVSEC 2011 29

PV in urban environment Monthly radiation (kwh/m 2 ) for all months of the year (January top left to December bottom right). Colour code is the same for all maps. P. Redweik et al, PV potential estimation using 3D local scale solar radiation model based on urban LIDAR data, PVSEC 2011 PV in urban environment 30

Next class Further reading M. Šúri,et al, Potential of solar electricity generation in the European Union member states and candidate countries. Solar Energy, 81 (2007) 1295 1305 M. Šúri et al, Uncertainties in photovoltaic electricity yield prediction from fluctuation of solar radiation. Proc. 22nd European Photovoltaic Solar Energy Conference, Milano, Italy 2007 T. Huld et al, Comparison of Potential Solar Electricity Output from Fixed- Inclined and Two-Axis Tracking Photovoltaic Modules in Europe, Prog. Photovolt: Res. Appl. 2008; 16:47 59 E. Narvarte et al, Tracking and Ground Cover Ratio, Prog. Photovolt: Res. Appl. 2008; 16:703 714 31