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Solar Radiation

The Sun • Solar Radiation •

Sun-Earth Relationships • Array

Orientation • Solar Radiation Data

Sets • Estimating Array Performance

The Sun • Solar Radiation •

Sun-Earth Relationships • Array

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 A false color image

of the sun enhances the turbulent nature of the sun’s

photosphere,

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 Even over the vast distance, an enormous

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 Solar irradiance is

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 The inverse square law states that irradiance is

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 Solar irradiation

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 The electromagnetic

spectrum is the

range of all types of electromagnetic

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 The wavelength

distribution of extraterrestrial solar radiation forms a spectral

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 Solar radiation

entering Earth’s

atmosphere consists of direct, diffuse,

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 Air mass is a

representation of the amount of

atmosphere

radiation that must pass through to

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 Peak sun hours is an

equivalent measure of total solar irradiation in a day.

 For example, a day with an

average irradiance of 600 W/m2 over 8 hr may only

reach peak sun condition for an hour or less around noon. However, the total irradiation of 4800 Wh/m2

(600 W/m2 × 8 hr = 4800

Wh/m2) is equivalent to 4.8

peak sun hours (4800 Wh/ m2 ÷ 1000 W/m2 = 4.8

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 Insolation (solar

irradiation received over a period of time, kWh/m2/day) maps

rate locations by their average daily peak

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 The atmosphere

absorbs

extraterrestrial

radiation at certain wavelengths,

resulting in an altered spectral distribution for

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 A pyranometer

measures total global solar

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 Diffuse solar

irradiance can be measured by

adding a shadowing device to a

pyranometer, which blocks the direct

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 Handheld

pyranometers use less precise sensors than precision

pyranometers but

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 A pyrheliometer

measures the

direct component of solar irradiance, which is important when installing

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 The ecliptic plane is formed by Earth’s elliptical orbit around the sun.  In one year, Earth makes a slightly elliptical orbit around the sun.

Perihelion is the point in Earth’s orbit when it is closest to the sun.

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 The equatorial plane is tipped 23.5° from the

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 The summer solstice

occurs when the Northern

Hemisphere is tipped towards the sun. The winter solstice

occurs when the Northern

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 The fall and spring

equinoxes occur when the sun is

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Two angles are used to define the sun’s

position, relative to an observer on Earth:

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 Array orientation can be described using

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 Energy production at certain times of the year

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 The average

seasonal declinations define the optimal

References

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