A solar radiation model for photovoltaic and solar thermal

Slides:



Advertisements
Similar presentations
Solar Energy Forecasting Using Numerical Weather Prediction (NWP) Models Patrick Mathiesen, Sanyo Fellow, UCSD Jan Kleissl, UCSD.
Advertisements

The solar spectrum compared to a black body. Sun ~6000K Sun radiates a lot more energy that the Earth! Earth ~290K Blackbody radiation curves typical.
GLOBAL CLIMATES & BIOMES
Measurement of Radiation - Solar radiation - Long wave radiation - Net radiation - Exposure of radiation sensors.
Chapter 2 Solar Heating. (Variations in) Solar Heating Power Weather Important Global and Seasonal Variations: Low latitudes receive more solar heating.
Power Generation from Renewable Energy Sources
1 Part B5: System design/performance prediction. 2 B5.1System design Irradiance: Variables Latitude at the point of observation Orientation of the surface.
Atmospheric effect in the solar spectrum
Radiation: Processes and Properties - Environmental Radiation - Chapter 12 Section 12.8.
Atmospheric scatterers
Climate. Ozone Hole over Antarctica Ban on fluorocarbons began 1979.
Elements of Weather & Climate
To compute the solar radiation flux density at the surface we need to know effects of atmosphere in filtering and depleting the beam from the top of the.
Our atmosphere is perilously thin. Yet it provides important solar protection as well as oxygen.
Sun-Earth relationships Array Orientation Solar Radiation Data Sheets
MET 61 1 MET 61 Introduction to Meteorology MET 61 Introduction to Meteorology - Lecture 8 “Radiative Transfer” Dr. Eugene Cordero San Jose State University.
GY205 Weather and Climate Lecture 2 (Please turn in homework on the table.)
WIND ENSEMBLE FORECASTING USING AN ADAPTIVE MASS-CONSISTENT MODEL A. Oliver, E. Rodríguez, G. Montero.
Chapter 17 Notes: The Atmosphere. What is the Atmosphere? The atmosphere can be defined as the portion of planet earth that contains gas. Weather can.
 Weather Weather is over a short period of time Constantly changing, current condition of the atmosphere  Climate Climate is over a long period of.
Southern Taiwan University Department of Electrical engineering
University Institute of Intelligent Systems and Numerical Applications in Engineering CMN June 29 – July 2, 2015, Lisbon, Portugal.
Ch 17 - The Atmosphere Vocab Charts (Example) WordDefinitionPicture Weather the state of the atmosphere at a given time and place.
Solar Energy Part 1: Resource San Jose State University FX Rongère January 2009.
Meteorology Ch 3 Jeopardy
Copyright © 2013 Pearson Education, Inc. The Atmosphere: An Introduction to Meteorology, 12 th By: Lutgens and Tarbuck Lectures by: Heather Gallacher,
Power Generation from Renewable Energy Sources Fall 2012 Instructor: Xiaodong Chu : Office Tel.:
Extraterrestrial Solar Radiation The amount of solar energy per unit time, at the mean distance of the earth from the sun, received on a unit area of a.
Model Construction: interpolation techniques 1392.
Climate and Terrestrial Biodiversity Chapter What Factors Influence Climate?  Concept 7-1 An area's climate is determined mostly by solar radiation,
AOSC Lesson 2. Temperature Scales Temperature scales are defined by upper and lower calibration points (fixed points) In the Fahrenheit temperature scale.
Lecture Objectives: Define Solar Radiation Components Introduce Internal Surface Energy Balance.
Desarrollo de un método ensemble para la predicción del viento a escala local usando elementos finitos MINECO PROGRAMA.
Power Generation from Renewable Energy Sources Fall 2013 Instructor: Xiaodong Chu : Office Tel.:
Ensemble Wind Forecasting Based on the HARMONIE Model and Adaptive Finite Elements in Complex Orography.
Meteorology Lecture 1 Weather and Climate Review.
1 MET 12 Global Climate Change - Lecture 4 Clouds and global climate Shaun Tanner San Jose State University  By the end of this chapter you should: Understand.
Earth’s Energy Balance
Factors That Affect Climate
Lecture Objectives: Summarize heat transfer review
Atmosphere. Atmosphere structure Tropopause Troposphere 20 km 40 km 10 mi 20 mi 30 mi Weather zone Water Vapor Dry Ozone Stratosphere Stratopause Mesosphere.
INCIDENCE ANGLE, θ The solar incidence angle, θ, is the angle between the sun’s rays and the normal on a surface. For a horizontal plane, the incidence.
Meteorologisches Institut Theresienstr. 37 D –80333 Munich Dependence of UV radiation on altitude and aerosol optical.
1. The atmosphere 2 © Zanichelli editore 2015 Characteristics of the atmosphere 3 © Zanichelli editore 2015.
Reflectance Function Estimation and Shape Recovery from Image Sequence of a Rotating object Jiping Lu, Jim Little UBC Computer Science ICCV ’ 95.
Power Generation from Renewable Energy Sources Fall 2013 Instructor: Xiaodong Chu : Office Tel.:
Earth and Space Science TEK 14 a 14) Fluid Earth. The student knows that Earth’s global ocean stores solar energy and is a major driving force for weather.
Planck’s law  Very early in the twentieth century, Max Karl Ernest Ludwig Planck put forth the idea of the quantum theory of radiation.  It basically.
Solar Radiation Characteristics
TEM – Lecture 5 Radiative Heat Flow. Radiation Radiation intensity increases with temperature! Every surface above zero K Radiates!
Unit 4: Climate Change Earth’s Climate System. Introduction Atmosphere: layer of gases that surrounds a planet or moon Without the atmosphere, days would.
HCB-3 Chap 4: Solar Radiation1 Chapter 4: SOLAR RADIATION Agami Reddy (July 2016) 1.Effect of earth’s tilt and rotation about the sun 2.Basic solar angles:
Climate vs Weather.
Climate and Terrestrial Biodiversity
Wind Ensemble Forecasting Using Differential Evolution
Technology on the Cutting Edge of Weather Research and Forecasting
EASC 11 Chapters 14-18: The Atmosphere
Atmosphere & Weather Review
Explain the significance of Earth’s Atmosphere
TEM – Lecture 5 Radiative Heat Flow.
The application of an atmospheric boundary layer to evaluate truck aerodynamics in CFD “A solution for a real-world engineering problem” Ir. Niek van.
Zhang Hailong, Xin Xiaozhou, Liu Qinhuo
Chapter 4B: SOLAR IRRADIATION CALCULATION
AOSC Lesson 4.
Climate Change.
Can you think of any temperature patterns on Earth?
Solar Energy.
Three-Dimensional Finite Element Modeling of Stack Pollutant Emissions
Local Scale Finite Element Modelling of Stack Pollutant Emissions
Presentation transcript:

A solar radiation model for photovoltaic and solar thermal power exploitation F. Díaz, G. Montero, J.M. Escobar, E. Rodríguez, R. Montenegro

Contents 1. Introduction 2. Terrain surface mesh and detection of shadows 3. Solar radiation modelling -Solar radiation equations for clear sky Beam radiation Diffuse radiation Reflected radiation -Solar radiation for real sky -Typical meteorological year (TMY) 4. Results 5. Conclusions

Introduction Solar power is one of the most appreciate renewable energies in the world Three groups of factors determine the interaction of solar radiation with the earth’s atmosphere and surface a. Earth’s geometry, revolution and rotation (declination, latitude, solar hour angle) b. Terrain (elevation, albedo, surface inclination/orientation, shadows) c. Atmospheric attenuation (scattering, absorption) by c.1. Gases (air molecules, ozone, CO2 and O2) c.2. Solid and liquid particles (aerosols, including non-condensed water) c.3. Clouds (condensed water) Correct estimation needs an accurate definition of the terrain surface and the produced shadows. Previous works. A typical meteorological year (TMY) for each available measurement stations has been developed.

Introduction Topography Shadows Albedo Beam Radiation Diffuse Radiation Reflected Radiation Global Radiation Clear Sky Experimental Data Real sky

Terrain surface mesh and shadows Build a sequence of nested meshes from a regular triangulation of the rectangular region, such that the level j is obtained by a global refinement of the previous level j−1 with the 4-T Rivara’s algorithm The number of levels m of the sequence is determined by the degree of discretization of the terrain, Define a new sequence until level m’ ≤ m applying a derefinement algorithm Two derefinement parameters εh and εa are introduced and they determine the accuracy of the approximation to terrain surface and albedo, respectively.

Terrain surface mesh and shadows Day angle Hour angle Sun declination Solar altitude and Solar azimuth Solar beam direction

Terrain surface mesh and shadows Construct a reference system x’, y’ and z’, with z’ in the direction of the beam radiation, and the mesh is projected on the plane x’y’ The incidence solar angle δexp is then computed for each triangle Check for each triangle Δ of the mesh, if there exists another Δ’ that intersects Δ and is in front of it, i.e., the z’ coordinates of the intersection points with Δ’ are greater than those of Δ.

Terrain surface mesh and shadows 12:00 hours 14:00 hours 14:00 hours 12:00 hours 16:00 hours 18:00 hours 16:00 hours 18:00 hurs

Solar radiation modelling General aspects: Use of adaptive meshes for surface discretization and a new method for detecting the shadows over each triangle of the surface. This solar radiation model is based on the work of Šúri and Hofierka Calculations flow: We first calculate the solar radiation under the assumption of clear sky for all the triangles of the mesh. Typical Meteorological Year (TMY) is evaluated for all the involved measurement stations. Solar radiation values are corrected for a real sky by using the TMY from the available data of the measurement stations in each time step along an episode. Steps 1 and 3 are repeated for each time step and finally, the total solar radiation is obtained integrating all the instantaneous values in each triangle.

Solar radiation modelling Solar radiation equations for clear sky Solar radiation types Beam Diffuse Reflected

Solar radiation modelling Solar radiation equations for clear sky Solar constant Beam radiation Extraterrestrial irradiance G0 normal to the solar beam Correction factor Linke atmospheric turbidity factor Beam irradiance normal to the solar beam Gb0c = G0 exp{−0.8662TLKmδR(m)} Relative optical air mass Beam irradiance on a horizontal surface h0: the solar altitude angle Lf: the lighting factor Gbc(0) = Gb0c Lf sin h0 Beam irradiance on an inclined surface δexp: the incidence solar angle Gbc(b) = Gb0cLf sin δexp

Solar radiation modelling Solar radiation equations for clear sky Diffuse radiation Diffuse transmission Diffuse radiation on horizontal surfaces Diffuse radiation on inclined surfaces Function depending on the solar altitude Sunlit surfaces ho ≥ 0.1 ho < 0.1 Shadowed surfaces

Solar radiation modelling Solar radiation equations for clear sky Reflected radiation Mean ground albedo

Solar radiation modelling Solar radiation under real-sky Values of global irradiation on a horizontal surface for real sky conditions G(0) are calculated as a correction of those of clear sky Gc(0) with the clear sky index kc If some measures of global radiation Gs(0) are available at different measurement stations, the value of the clear sky index at those points may be computed as Then kc may be interpolated in the whole studied zone

Solar radiation modelling Typical meteorological year (TMY) To obtain accurate real sky values of global irradiation, the evaluation of a TMY is needed to avoid results based on a particular year weather conditions We compute the daily typical meteorological year of maximums, means, medians, variance and percentiles of 90% and 75% series of values using weight means to smooth the irregular data. TMY series were fitted to third grade Fourier series

Solar radiation modelling Typical meteorological year (TMY) Means Medians

Results The studied case corresponds to Gran Canaria, one of the Canary Islands in the Atlantic Ocean at 28.06 latitude and −15.25 longitude. The UTM coordinates (metres) that define the corners of the considered rectangular domain including the island are (417025, 3061825) and (466475, 3117475), respectively. TMY (1998 – 2008) for all the stations in Gran Canaria Island were obtained for every month. The average global radiation (real sky), varies from: 10.6 MJ/m2 per day in December 25.6 MJ/m2 per day in June

Geolocation of different stations on Results Geolocation of different stations on Gran Canaria Island Elevation map of Gran Canaria

Results Albedo map of Gran Canaria Macaronesic laurisilva 0.05 Salt mine 0.6 Albedo map of Gran Canaria

Results Intermediate mesh 5866 nodes 11683 triangles Triangular mesh adapted to topography and albedo

Beam radiation map (J/m2) Results EXAMPLE 82 − 87% of the mean global irradiation Beam radiation map (J/m2) December 2006

Diffuse radiation map (J/m2) Results EXAMPLE 13 − 18% of the mean global irradiation Diffuse radiation map (J/m2) December 2006

Reflected radiation map (J/m2) Results EXAMPLE 0 − 0.5% of the mean global irradiation Reflected radiation map (J/m2) December 2006

Results Clear sky global radiation map (J/m2) December 2006 Real sky global radiation map (J/m2) December 2006

Results Annual evolution of the computed monthly average per day (TMY) for both, clear sky and real sky global radiation DE DE

Percentage decrease from the computed radiation: Real sky to clear sky Results Percentage decrease from the computed radiation: Real sky to clear sky TRADE WINDS Months

Influence of the trade winds: Annual Wind Rose for Canary Islands Results Influence of the trade winds: Annual Wind Rose for Canary Islands Frequency (%)

Influence of the trade winds: Results Influence of the trade winds:

Monthly average Real Sky radiation Results SIMULATIONS: Monthly average Real Sky radiation January April

Monthly average Real Sky radiation Results SIMULATIONS: Monthly average Real Sky radiation July October

Solar Power Generation: Photovoltaic and Solar Thermal Results Solar Power Generation: Photovoltaic and Solar Thermal Hourly Clear Sky radiation calculation for all days Numerical Integration Clear Sky Index and Interpolation Irradiation and Energy for Real Sky conditions Clear Sky Irradiance Real Sky Irradiance Solar PV Model Solar Thermal Electric Power Generation

Conclusions The adaptive triangulation related to the topography and albedo is essential in order to obtain accurate results of shadow distribution and solar radiation Adaptive meshes lead to a minimum computational cost, since the number of triangles to be used is optimum. Statistical treatment of data is necessary to reach accurate conclusions about the possible behaviour of the radiation distribution values Typical meteorological year (TMY) is the departure point to estimate the real sky radiation values The model allows to choose the most suitable zone in the island for a solar power station Rectangular collectors can be included in the model as composed by two triangles in the same plane

Future research Improve the interpolation procedure used for processing such data Calculate the optimal orientation and inclination of solar collectors for each location Optimal selection of the warning points for detecting the shadows Determinate the shadow boundary using ref/deref and mesh adaption by moving nodes Define an error indicator to ref/deref the mesh attending to daily real global radiation Fully parallelise the calculations

A solar radiation model for photovoltaic and solar thermal power exploitation F. Díaz, G. Montero, J.M. Escobar, E. Rodríguez, R. Montenegro