Lesson: Solar Angles and Tracking SystemsContributed by: Integrated Teaching and Learning Program, College of Engineering and Applied Science, University of Colorado at Boulder
Educational Standards :
Learning Objectives (Return to Contents)
After this lesson, students should be able to:
Introduction/Motivation (Return to Contents)
(In advance, make copies of the attached Fundamentals Article, which contains basic photovoltaic efficiency information and facts that are used throughout this unit [including this lesson], one per student or one per small group.)
Where is the sun in the sky? From our perspective on Earth, the sun is always changing its position in the sky. It is pretty obvious that every day the sun moves from the east to the west between sunrise and sunset, but did you know that it also moves from north to south throughout the course of the year? If you were to measure the position of the sun every day at solar noon (or the time of day when the sun is the highest in the sky) it would be at a different angle every day. The exact location of the sun in the sky depends on where you live, the day of the year, and, of course, the time of day. This effects the design decisions engineers make when they are installing photovoltaic (PV) panels.
What are photovoltaic (PV) panels? "Photo" means light and "voltaic" means voltage. Thus, a photovoltaic panel is a device that turns light into electric potential. Commonly, these devices are referred to simply as "solar panels" because the light source in many applications is the sun. Yet the term "solar panel" can also refer to other devices that capture the sun's heat but do not produce electricity. Photovoltaic panels use layers of special materials to create a voltage and current when sunlight is absorbed.
It is important for engineers to know where the sun will be throughout the year so they can install PV panels at the ideal angle to absorb the maximum amount of sunlight during the course of a year. To improve the efficiency of PV panels, engineers also design creative ways so more sunlight hits the surface of the panel. Can you think of ways to improve the efficiency of PV panels that relates to the angle of the sun? (Have students brainstorm ideas as a class.) Let's do some reading to find out more.
(Have the students read the Fundamentals Article, and record 10 important facts, then conduct the post-introduction assessment described in the Assessment section.)
Lesson Background & Concepts for Teachers (Return to Contents)
Using Solar Angles to Predict the Sun's Location
On one day every year, called the equinox, the sun is positioned directly above our planet's equator. On this day, the angle between a line that points to the sun and a line that points straight up (vertical) exactly matches the latitude of the place you are standing. If you live on the equator, then in the very middle of the day (solar noon) the sun will be directly above you, or at 0º from the vertical. If you live in Boulder, CO, which is in the northern hemisphere at the latitude of 40º, then on the equinox the sun will be 40º to the south from the vertical (see Figure 2). The sun's position on the equinox is the average location of the sun throughout the year and is a great reference to use when designing a solar system for a specific location.
But keep in mind, the sun is always moving. In the summer, the sun appears higher in the sky, which increases the duration of sunlight seen in a day, and in the winter it appears lower, which decreases the length of sunlight in a day. The sun is highest in the sky on the summer solstice. To be more exact, it is 23.45º higher than on the equinox, or at 40 - 23.45 = 16.55º to the south of vertical.
The winter solstice is the day when the sun appears lowest in the sky. On this day, the sun is 23.45º lower than on the equinox, or at 40 + 23.45 = 63.45º to the south of vertical in Boulder. So, if you live in the northern hemisphere at latitude higher than 23.45º, then the sun will never shine from the north. This means the north side of your house would be a bad place for a solar panel (or a garden).
Summary of Solar Angles
Below is an overview of the angles involved in calculating the amount of solar radiation that a PV panel receives at any given time (also see Figure 3). The angle at which the sun hits a PV panel is the basis for understanding how to design the most efficient PV array for a specific location. This is one of the first topics presented in solar engineering textbooks.
Zenith Angle, Θz: This is the angle between the line that points to the sun and the vertical — basically, this is just where the sun is in the sky. At sunrise and sunset this angle is 90º.
Solar Altitude Angle, αs: This is the angle between the line that points to the sun and the horizontal. It is the complement of the zenith angle. At sunrise and sunset this angle is 0º.
Solar Azimuth Angle, γs: This is the angle between the line that points to the sun and south. Angles to the east are negative. Angles to the west are positive. This angle is 0º at solar noon. It is probably close to -90º at sunrise and 90º at sunset, depending on the season. This angle is only measured in the horizontal plane; in other words, it neglects the height of the sun.
Angle of Incidence, θ: This is the angle between the line that points to the sun and the angle that points straight out of a PV panel (this is also called the line that is normal to the surface of the panel). This is the most important angle. Solar panels are the most efficient when pointing at the sun, so engineers want to minimize this angle at all times. To know this angle, you must know all of the angles listed and described next.
Hour Angle, ω: This is based on the sun's angular displacement, east or west, of the local meridian (the line the local time zone is based on). The earth rotates 15º per hour so at 11am, the hour angle is -15º and at 1pm it is 15º.
Surface Azimuth Angle, γ: This is the angle between the line that points straight out of a PV panel and south. It is only measured in the horizontal plane. Again, east is negative and west is positive. If a panel pointed directly south, this angle would be 0º.
Collector Slope, β: This is the angle between the plane of the solar collector and the horizontal. If a panel is lying flat, then it is 0º. As you tip it up, this angle increases. It does not matter which direction the panel faces.
Declination, δ: This is the angle between the line that points to the sun from the equator and the line that points straight out from the equator (at solar noon). North is positive and south is negative. This angle varies from 23.45 to -23.45 throughout the year, which is related to why we have seasons.
Latitude, φ: This is the angle between a line that points from the center of the Earth to a location on the Earth's surface and a line that points from the center of the Earth to the equator. This can be easily found on a map.
Solar Tracking Systems
Now let's talk about how to apply all of this information. Figure 1 shows a small portion of North America's largest solar PV power plant (as of 2010). The 14-megawatt power plant is located at Nellis Air Force Base in Nevada and is expected to provide more than 30 million kilowatt-hours of electricity each year. A typical compact fluorescent lamp (CFL) uses 15 watts, so when the sun is shining, this plant could power almost a million CFLs. At this site, 72,000 PV panels are placed across 140 acres of land. This power plant has more than just PV panels. Look at Figure 1 to see if you notice anything else that might affect the efficiency of the panels.
It might not be obvious at first, but look closely at the bases supporting the panels. They are designed to move! SunPower Corporation, a German company that specializes in PV power systems, designed this PV power plant with an east-west single-axis tracking system. That means that the panels rotate from east to west throughout the day to follow the sun and optimize panel efficiency. Because of this tracking system, these panels produce 30% more power than they would if they were fixed facing south.
Further panel efficiency can be obtained by tracking the sun not only along a single axis, but on two perpendicular axes. Figure 4 shows one of the most efficient PV panels in the world (more than 40% conversion efficiency) created by Spectrolab. These PV panels are extremely expensive so this module uses very small panels and less expensive mirrors to reflect sunlight from a larger area onto the small PV panel. The process of concentrating the sunlight for photovoltaic power production is explained in more detail in the Concentrated Solar Panel lesson. For this high-tech system, it is important to track the sun's location exactly throughout the day to provide the maximum amount of sunlight for the module at all times. To do that, this module has a double-axis tracking system that moves from east to west and an adjustable collector slope, β, to follow the height of the sun in the sky throughout the year.
Vocabulary/Definitions (Return to Contents)
Associated Activities (Return to Contents)
Lesson Closure (Return to Contents)
The energy output of a photovoltaic (PV) panel changes based on the angle between the PV panel and the sun. The angle at which the sun hits a PV panel determines its efficiency and is what engineers use in the design of an efficient PV array for a specific location.
Solar tracking systems designed by engineers help optimize the amount of sunlight that hits a photovoltaic panel over time (day, month, year). One example is SunPower Corporation — a German company that creates photovoltaic power systems — that designed a PV power plant with an east-west single-axis tracking system. That means that the panels rotate from east to west throughout the day to follow the sun and optimize panel efficiency. Because of this tracking system, these panels produce 30% more power than they would if they were fixed facing south.
Whether a panel is fixed in one direction or integrated with a single- or double-axis tracking system, it is important to know the location of the sun throughout the year and the effect that the angle of sunlight hitting the panel has on its overall efficiency.
Attachments (Return to Contents)
Assessment (Return to Contents)
Discussion Questions: Ask a few discussion questions to get students to think about the upcoming lesson. After soliciting answers, explain that these questions will be answered during the lesson.
Brainstorming: As a class, have students engage in open discussion. Remind them that in brainstorming, no idea or suggestion is "silly." All ideas should be respectfully heard. Encourage wild ideas and discourage criticism of ideas. Have students raise their hands to respond. Write answers on the board. Ask the students:
Class Discussion: Have students read the Fundamentals Article, which contains basic facts that are used throughout this unit (including this lesson). As they read, have students each write 10 facts from the article on a sheet of paper. Engage the class in a discussion of what they have read. Ask each student or student group to record on the board one fact about PV panels that they have learned from the reading.
Lesson Summary Assessment
Writing/Reflection: Have students think about solar panels and panel tracking systems, and compose a journal entry on their thoughts. How would they explain the importance of designing a solar panel to track the sun to someone who did not know a lot about solar panels? Have them list and describe any of the solar angles that were discussed in class.
Lesson Extension Activities (Return to Contents)
Human Solar Tracker Activity: Have every student in the class hold up a book. Tell them that the front of the classroom is south. Give them the time of the year, and hour of the day, and ask them to position their books as though they are solar panels seeking to receive the maximum amount of sunlight. Guide them through each aspect of the sun's positions and help them think through the solar angles.
Long-Term Classroom Tracking: To make more tangible the annual cycle of the sun's angle, designate an area in the classroom or school that receives direct sunlight at which to have students make a daily mark to record how far sunlight reaches into the classroom at solar noon. Do this for a month or longer. For the daily mark, place of piece of (removable) masking tape on the floor, wall or tabletop, and write the date on the tape.
Additional Multimedia Support (Return to Contents)
Interactive Seasons: Have students explore this interactive astronomy website to see the how the angle of the sun changes throughout the year. Students can view what would happen if our planet had a different tilt angle. See: http://highered.mcgraw-hill.com/sites/007299181x/student_view0/chapter2/seasons_interactive.html
References (Return to Contents)
High-Performance Photovoltaics. Last updated July 25, 2008. Photovoltaic Research, National Renewable Energy Laboratory (NREL). Accessed February 4, 2010. http://www.nrel.gov/pv/high_performance_pv.html
Solar Energies Technology Program. Last updated January 18, 2010. Energy Efficiency & Renewable Energy, US Department of Energy. Accessed February 4, 2010. http://www1.eere.energy.gov/solar/
Photovoltaic cell. The American Heritage® Dictionary of the English Language, Fourth Edition. Houghton Mifflin Company, 2004, via Dictionary.com. Accessed February 11, 2010. http://dictionary.reference.com/browse/photovoltaic+cell
ContributorsWilliam Surles, Abby Watrous, Eszter Horanyi, Malinda Schaefer Zarske (This high school curriculum was originally created as a class project by engineering students in a Building Systems Program course at CU-Boulder.)
Copyright© 2009 by Regents of the University of Colorado
The contents of these digital library curricula were developed by the Integrated Teaching and Learning Program under National Science Foundation GK-12 grant no. 0338326. However, these contents do not necessarily represent the policies of the National Science Foundation, and you should not assume endorsement by the federal government.
Supporting Program (Return to Contents)Integrated Teaching and Learning Program, College of Engineering and Applied Science, University of Colorado at Boulder
Last Modified: March 1, 2013