Energy and
Power
Solar radiation or
insolation
- Solar radiation is energy transmitted from the
sun to the earth in the form of electromagnetic
waves. These waves transmit energy at a certain rate and density.
The solar flux defines
the rate and density in which the energy is transmitted.
- Solar flux is typically measured in W/m2.
- It is important to note that solar energy is more
than the light humans can see with their eyes. "About half of the
radiation is in the visible
short-wave part of the electromagnetic
spectrum [light you can see]. The other half is mostly in the near-infrared part,
with some in the ultraviolet
part of the spectrum" (http://www.grida.no/climate/ipcc_tar/wg1/041.htm).
- Direct solar radiation is the solar radiation in the
form of a collimated
beam with a known orientation.
- Diffuse solar radiation is solar radiation in an
uncollimated form. Diffuse radiation becomes uncollimated due to
scattering in the atmosphere and reflection off of objects on the
earth's surface (ground, buildings, etc.).
- Total solar radiation is the sum of the direct and
diffuse solar radiation.
- For more information see http://en.wikipedia.org/wiki/Solar_radiation
and http://en.wikipedia.org/wiki/Insolation
Sun Position
- Although the earth actually revolves around the sun,
for the sake of solar energy analysis, in the reference frame of the
earth we can consider the sun to be moving about the earth. For
example, the sun rises in the east and sets in the west.
- The position of the sun is defined using spherical
coordinates.
- Azimuth and altitude angles are a function of
geographic location and time.
- The azimuth and altitude angles are defined
assuming that the earth is effectively flat.
- Azimuth angle: The angle of the sun about the plane
of the earth's surface (the same direction that a compass would measure
measure).
- Altitude angle: The angle of the sun formed
between the earths surface and the sun (i.e. how high the sun is in
the sky when facing the sun).
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