Solar Power - For Your
Home
How Solar Power
Works
Solar power,
particularly when it's used to provide home electricity needs,
may seem like a relatively recent invention. And it's true
that large, cost-effective panels that form the core of most
systems have only been in use for about that past 30 years.
But the underlying method they employ goes back to 1839, when
it was discovered by Becquerel. He found that shining sunlight
on an electrolytic cell would produce a current.
Other scientists built on that work. In fact,
while Albert Einstein is most well known for the Theory of
Relativity, he received his 1921 Nobel Prize for something quite
different. According to the Nobel organization it was 'for his
services to Theoretical Physics, and especially for his discovery
of the law of the photoelectric effect'. His paper on the subject
was written in 1905.
The photoelectric effect is essentially similar
to what solar power enthusiasts and workers know as the
photovoltaic effect, the principle Becquerel first found. When
light, in this case from the sun, strikes certain materials it
knocks loose electrons from their associated atoms. Those moving
electrons create a current that can flow through the material to
provide electrical power.
Those materials today are typically some type of
doped silicon. 'Doping' is another way of saying that other
elements are deliberately introduced. In other applications, those
impurities would be undesirable. In solar power, they're essential.
Pure silicon has its uses, but it's not a good conductor of
electricity. Adding phosphorus in just the right way, for example,
turns them into semiconductors.
Certain specialized applications use
gallium-arsenide or other materials, instead of silicon. But
because of their relative rarity the cost is much higher. Silicon
is a major component of ordinary sand and hence plentiful.
The silicon-phosphorus compound is arranged in
layers, then connected to a grid to enhance the flow of
electricity. It reduces the resistance losses. Then terminals are
installed to allow for the electricity to flow into the home
electrical system. The whole assembly is covered with glass to
protect it and forms what's known as a PV (photovoltaic) cell.
Those cells are then arrayed into a module. Modules can then be
connected together into a complete system.
Those modules comes in various sizes that
determine how much electricity they generate. All other things
being equal, the larger the area, the more power they can produce.
Naturally, the larger panels tend to cost more.
Though the solar energy reaching the surface (at
the equator) is about 1,000 watts per square meter, not all of it
is usable energy. A square meter is a square whose sides are a
little larger than three feet - it's about 10.7 square feet. Apart
from losses due to latitude, atmosphere, dust and other natural
factors, the modules themselves only convert with about 10-15%
efficiency.
The growth of solar power as a practical energy
production method depends heavily on increasing that efficiency and
lowering the costs of production. To a degree, that efficiency is
bound by certain difficult-to-get-around physical constraints, so
most of the research efforts involve attempts to lower the
manufacturing costs.
When or if that happens, solar power
applications may well become even more commonplace in homes and
businesses than they are today.
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