Article 1: The Beginner's Guide to Solar Energy
Solar Industry Growth and Affordability
Solar is playing an increasingly important role
in the transition to a world powered by renewable energy. Over the past decade,
the number of solar installations has grown at an accelerating rate and with
increasing affordability.
Figure 1 illustrates the correlation of the
increasing number of installations with the decreasing costs. It shows that the
price of a solar installation is now less than a third of what it was in 2009,
while annual installations have grown more than tenfold during the same period
of time.
SEIA states that the solar industry is a
powerful engine for economic growth. The solar industry currently employs
over 200,000 people, twice as many as in 2010 and now employs more people than
the coal, or the oil and gas industries. As installed capacity continues to
increase, SEIA predicts that the solar workforce will expand to 420,000 by
2020.
Solar
Energy, Power, and Irradiance
Solar panels convert the energy of photons, or
light particles, from the sun into electricity. Photovoltaic devices, such as
solar panels, permit the incoming photons to transfer their energy to
electrons. These energized electrons begin to flow, creating an electric
current. We use the terms irradiance or insolation to refer to the power
density of sunlight on a surface.
We typically measure energy in kilowatt-hours
(kWh), and power (the rate at which energy is produced) in kilowatts (kW).
In solar, we usually define the size of a solar
installation in terms of its power (in kW).
Irradiance is typically reported in units of
kilowatt-hours per meter squared per day (kWh/m2-d). The amount of
irradiance hitting the surface of the earth is often quoted in terms of the
number of hours of “full-sun” of solar energy. A "full-sun" is
defined as 1 kW/m2.
Quantity
|
Units
|
Definition
|
Power
|
kW
|
Rate of energy production/output
|
Energy
|
kWh
|
Capacity to do work
|
Irradiance
|
kWh/m2-d
|
Hours of full-sun for a square meter each day
|
Solar Resource of a Rooftop
We can estimate the solar potential of a
rooftop using its area and the local irradiance. NREL, the National Renewable
Energy Laboratory, publishes irradiance data in its report Solar
Radiation Data Manual for Flat-Plate and Concentrating Collectors.
It is fairly straight forward to calculate
rooftop solar potential of a rooftop using this data. For example, a
south-facing roof plane of a home (Figure 4) receives an
average irradiance of approximately 1,900 kWh/m2/year. Dividing the
annual irradiance value by the number of days in a year yields the average
daily irradiance.
To calculate the amount of solar energy
available on a roof face, multiply its area by the average irradiance value.
If the rooftop has an area of approximately 150m2, the solar energy
available on the rooftop is as follows.
Besides the solar irradiance, Figure 4 also
displays information on three additional quantities related to the solar
resource: Solar Access, TOF, and TSRF:
Solar Access: This is the ratio
of the actual solar energy available — taking into account shading cast by
objects in the environment — to the solar energy that would be available in the
absence of shading. You can learn more about the effects of shading on PV
systems here.
TOF (Tilt and
Orientation Factor): This is the ratio of the amount of solar energy a
location receives to the amount it would receive if the orientation of the roof
were optimal.
and orientation
TSRF (Total Solar
Resource Factor): This is the percentage of the available solar
resource that a location receives as compared to what it would receive with
optimal orientation and without shading. TSRF is equivalent to the Solar Access
multiplied by the Tilt and Orientation Factor.
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