Solar Energy
Solar Energy
This section covers the fundamentals of solar energy. From this we can determine how much energy is available over an area to be used for heat or electricity.
Motivation
To use the sun effectively as a source of energy, we have to know how it moves through the sky and what energy is available. From this knowledge we can place photovoltaic panels, building windows, or heat collectors correctly.
References
Renewable and Efficient, Gil Masters
Questions we will be able to answer
Where is the sun at any time?
How much radiation does it produce?
Where do I put solar panels or windows?
Will my solar devices be blocked by trees or homes?
Which direction should they face?
How much will they produce now? this month? this year?
Solar Fundamentals
This section covers the sun, the solar system, and the atmosphere in order to understand the radiation striking the earth.
The journey of a photon
Created in the core of the sun
Millions of years to bounce out to surface of sun
Zips to earth in about 8 minutes
Passes through the atmosphere
Strikes a solar panel and dislodges an electron in the PV panel
Electron is collected and delivered to the grid
Electromagnetic Spectrum
Blackbody Spectrum
Solar Spectrum
The Solar System
Radiation units
Atmospheric depth
Atmospheric absorption
Air mass ratio
Air mass ratio
Air mass ratio
There are some standard air mass ratios we use
AM0 is "in space"
AM1 is for noon-day sun
AM1.5 is the standard test condition that resembles year round
insolation
Earth sun distance
Is this close to circular?
Theory vs Practice
I'll demonstrate mathematical expressions for solar radiation
In practice you will use tables or software applications that
calculate these values
I want you to be able to go back in 10 years, pick up this book, and
figure it out again.
Summary of Angles
Box 4.1 of REEPS
Solar Irradiation
Solar Constant
Peak sun hours
Radiation Basics
Power per unit area
Spectral intensity
Mass Glazing Ratio
Extraterrestrial solar radiation
Sunlight striking the top of the atmosphere
Where
Software Implementation
You can see an example of these equations implemented in a software library at these locations
Solar Measurements
Pyranometers
Shading Measurements
Path Finder
Historical radiation data
Radiation measurements
We've seen how to calculate radiation
How do we measure it?
Measuring solar radiation
Typical meteorological year
Hourly solar and weather estimates for typical conditions
Based on historical data
Typical meteorological year
TMY Station Locations
TMY quantities
Global Horizontal Irradiance (GHI)
Direct Normal Irradiance (DNI)
Diffuse Horizontal Irradiance (DHI)
Components of solar radiation
Direct
Reflected
Diffuse
Direct, reflected, diffuse
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