Solar Energy Types of Generators Irradiance Insolation How Solar Cells work.

Slides:



Advertisements
Similar presentations
SOLAR ENERGY ISRAEL TODAY.. TOMORROW? Jerusalem College Of Technology Prof. Claude Oiknine 05/03/2013.
Advertisements

EE580 – Solar Cells Todd J. Kaiser Lecture 03 Nature of Sunlight 1Montana State University: Solar Cells Lecture 3: Nature of Sunlight.
Solar Energy Presented By: Isah Adamu Bazuwa (099271) Sani khalil (118312)
Exploring Solar Energy. Review: Atomic Structure  Three particles  Nucleus  Electrostatic Force  Strong nuclear force © The NEED Project.
1 Part B6: Concentrating collectors. 2 B6.1Concentrating collectors Used to increase outlet temperature Increase in temperature due to reduction in collector.
Solar Power. Before the bell rings get out your notes and begin answering the following based on your row… Row 1- (closest to the front!)- What are the.
Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction) From London and Upton.
CPSC 641 Computer Graphics: Radiometry and Illumination Jinxiang Chai Many slides from Pat Haranhan.
The NEED Project: 30 Years of Energy Education1 Solar Energy.
Energy Budget of the Earth-Atmosphere System
SEASONS, ENERGY FLOW AND THE SUN
Energy Budget of the Earth- Atmosphere System. Energy Transfer Conduction -- direct molecular transfer Convection -- fluids; air or water –Sensible heat.
Solar Energy Robert Kinzler
Sun-Earth relationships Array Orientation Solar Radiation Data Sheets
Solar Energy. Radiant Energy Solar Radiation Average Daily Solar Insolation Per Month.
Solar Power By: Christina Nahar. Solar Energy Potential The amount of solar energy that reaches the Earth’s surface every hour is greater than human kind’s.
Solar Power: Types, Capacities, Potential What is solar power? R. Todd Gabbard, LEED-AP, Assoc. AIA Asst. professor, Dept of Architecture, KSU
Solar Energy
ENGR101 © Copyright, 2005, TAMU ENGR 101 Prof. Maria A. Barrufet Petroleum Engineering Renewable Energy - Solar.
Energy from the Sun Workshop Introduction to Solar Energy.
Lighting calculations
CS348B Lecture 4Pat Hanrahan, 2005 Light Visible electromagnetic radiation Power spectrum Polarization Photon (quantum effects) Wave (interference, diffraction)
Solar Energy. What is solar energy? Solar energy is light or heat (radiant energy) that comes from the sun. Although solar energy is the most abundant.
The sunlight falling on the earth per day delivers energy which is 50,000 times (fifty thousand times) the total energy used all over the world in one.
Solar Energy. Radiant Energy 19% energy absorbed by vapor, ozone, dust, etc. 8% energy dispersed in the atmosphere 17 % energy reflected by clouds 4%
Solar Photovoltaics. Solar Photovoltaics (PVs) Make electricity directly from sunlight without pollution, moving parts, or on site noise Sun covers the.
Solar Power.
Solar Radiation 1367 W/m2 this is called the solar constant
Environmental Science Environmental Science Solar Energy Lecture Notes.

Photovoltaic (fo-to-vol-ta-ik) systems are solar systems that produce electricity directly from sunlight. The term "photo" comes from the Greek "phos,"
Renewable Energy Sources
Solar Energy. Solar energy has been an under-achiever Source: U.S. Department of Energy.
Solar Energy Part 1: Resource San Jose State University FX Rongère January 2009.
BY: RALIAT O. ALABI SOLAR ENERGY. HOW TO STORE THE ENERGY Through the use of a technique used in thermal plants Water is in one thermotank while molten.
By, N Venkata Srinath, MS Power Systems.. Introduction Solar energy is a very large, inexhaustible source of energy. The power from the sun intercepted.
Solar Thermal Plants. Thermal Energy: Reliable source Reliable source Could potentially supply 10% U.S. energy demand Could potentially supply 10% U.S.
Solar Hot Water Heater. Flat Plate Collector Problem A flat plate solar collector is used as a solar hot water heater. The collector area equals 20 square.
Solar Thermal Energy: Heating our homes while cooling our planet Chris Mayor and Stephen Mizera.
Chap 16-1 Light Fundamentals. What is Light? A transverse electromagnetic wave.
Power Generation from Renewable Energy Sources Fall 2013 Instructor: Xiaodong Chu : Office Tel.:
Describe how electromagnetic energy is transferred through space as electromagnetic waves of varying wavelength and frequency.
Solar energy Passive solar utilizes building design an placement to maximize heat in the winter and minimize heat in the summer. It is only building, not.
Do Now: Baltimore Polytechnic Institute receives an average of 150 W/m 2 every day during the month of January. How many kW of solar energy land on our.
Power Plant Construction and QA/QC Section 1.6– Solar Energy Engineering Technology Division.
Do Now: Baltimore Polytechnic Institute receives an average of 150 W/m 2 every day during the month of January. How many kW of solar energy land on our.
Solar Energy. Major Uses of Solar Energy  Daylight  Drying Agricultural Products  Space Heating  Water Heating  Generating Electrical Power  Concentrating.
EM Plane Wave: z Wave propagates along k, magnitude = 2p/l
S OLAR R ADIATION. R ADIATION Sun is a sphere of hot gaseous matter with a diameter of 1.39*10^9m. Due to its temperature, sun emits energy in the form.
Ali Saffar Shamshirgar
INSOLATION Incoming Solar Radiation Portion of sun’s output of electromagnetic radiation that is received by earth.
 Solar energy is radiant light and heat from the sun harnessed using a range of ever- evolving technologies such as solar heating, solar photovoltaics,
Solar Energy Samara Angel, Emilie Harold, Elyssa Hofgard, Jules Pierce, Joyce Xu.
Light. The nature of Light Spherical and plane waves.
Solar power (direct) -- the “greenest” of all energy sources, a one that dwarfs all other available energy sources combined (including those who are “transformed”
30/09/2016 Irradiance and Inverse square law. Read Summary Notes, page 65, “Irradiance and Inverse square law.” The irradiance of light, I, is defined.
Solar Power.
PHYSICS.
Date of download: 10/16/2017 Copyright © ASME. All rights reserved.
Date of download: 10/16/2017 Copyright © ASME. All rights reserved.
Module 1/7: Solar Technology Basics
P PT 1 Solar power Describe how electricity can be generated
SOLAR Energy Manisha Goel, Lecturer, EE Deptt
Inverse Square Law In Light.
Exploring solar energy
Do Now: Baltimore Polytechnic Institute receives an average of 150 W/m2 every day during the month of January. How many kW of solar energy land on our.
Warm - Up 1) What is the speed of light?
Light and Illumination
The Properties of Light
Presentation transcript:

Solar Energy Types of Generators Irradiance Insolation How Solar Cells work

Topics Part 1  Types of Solar Power Generators  Irradiance  Inverse Square Law Part 2  Path of Sun: Seasonal and daily  Effective cross section  Insolation Rate Part 3  How Solar Cells work  Power & IV Curves  Maximum Power Point  Efficiency

Part 1: Types of Solar Power Generators Passive Solar heat collectors  Rooftop solar water heaters Solar heat collectors – Steam Turbines  Parabolic Troughs  Thermal Towers  Other Solar Concentrators Photovoltaic Panels  Silicon, crystalline, thin film, organic dyes

Solar Water Heaters

Solar-Steam Generators

Parabolic Trough Ausra: 177 MW Carizzo Plain

Thermal Tower Mojave

Other Solar Concentrators

Photovoltaics PG&E Carizzo Plain Topaz 550 MW & High Plains Ranch 250 MW CalExpo Solar Park

Irradiance Visible light only F V = luminous flux of the source (lumens) E V = Illuminance of an object illuminated by F V at a distance d ( lm/m 2 = lux) E V = F V / 4  d 2 ex: 800 lumen bulb at 2 meters distance E V = (800 lm / 4  (2m) 2 = 16 lx All electromagnetic radiation: Visible efficacy of an Incandescent light:  =17 lm / W F R = Radiant Flux of the source ( W ) F R = F V /  E R = Irradiance of an object illuminated by F R at a distance d ( W/m 2 ) E R = F V / (4  d 2  ) = E V /  Example: An 800 lumen bulb at 2 meter distance E R = E V /  = 16 lx / 17 lm/W = 0.94 W/m 2

Inverse Square Law Irradiance (E) is inversely proportional to the square of the distance (d) from the source

Part 2 Path of Sun: Seasonal & Daily

Effective Area

Insolation Rate Top of the atmosphere: Solar constant =1366 W/m 2 Peak Surface Insolation: Clear sky, summer, noon =1000 W/m 2 Average Surface Insolation: Clear sky, year round, all day = 250 W/m 2 Typical Insolation: Paso Robles, Average weather, all day avg Summer: 6 kWh / m 2 / day Winter: 3 kWh / m 2 / day

Part 3: Photovoltaics How Solar Cells work

Power & IV Curves

Maximum Power Point

Efficiency