INSOLATION

'Insolation' is a measure of solar radiation incident on a surface. It is the amount of solar energy received over a given area in a given time. It is commonly expressed in kilowatt-hours per square meter per day (kW•h/m²/day) or watts per square meter (W/m²).
The surface may be a planet or a terrestrial object inside the atmosphere, or any object exposed to solar rays including spacecraft. Some of the solar radiation will be absorbed, causing radiant heating of the object, and the remainder will be reflected. The proportion of radiation reflected or absorbed depends on the object's reflectivity or albedo.

Contents

Projection effect

Earth's insolation

Applications

See also

References

External links

Projection effect

The insolation into a surface is largest when the surface directly faces the Sun. As the angle increases between the direction normal to the surface and the direction of the rays of Sunlight, the insolation is reduced in proportion to the cosine of the angle. This is known in optics as ''Lambert's cosine law''. This 'projection effect' is the main reason why the polar regions are much colder than equatorial regions on Earth. On an annual average the poles receive less insolation than does the equator, because at the poles the Earth's surface is angled away from the Sun.

Earth's insolation

Direct insolation is the solar radiation that is transmitted directly through the atmosphere to the earth's surface without interacting with atmospheric components. Diffuse insolation is the solar radiation that is scattered or reflected by atmospheric components.
Over the course of a year the average solar radiation arriving at the top of the Earth's atmosphere is 1366 watts per square meter^[1] (see solar constant). The radiant power is distributed across the entire electromagnetic spectrum, although most of the power is in the visible light portion of the spectrum. The Sun's rays are attenuated as they pass though the atmosphere, thus reducing the insolation at the Earth's surface to approximately 1000 watts per square meter for a surface perpendicular to the Sun's rays at sea level on a clear day.
The actual figure varies with the Sun angle at different times of year, according to the distance the sunlight travels through the air, and depending on the extent of atmospheric haze and cloud cover. Ignoring clouds, the average insolation for the Earth is approximately 250 watts per square meter (= 6 kW•h/m²/day), taking into account the lower radiation intensity in early morning and evening, and its near-absence at night.

Applications

In spacecraft design and planetology, it is the primary variable affecting equilibrium temperature and global climate.
In construction, insolation is an important consideration when designing a building for a particular climate. It is one of the most important climate variables for human comfort and building energy efficiency.^[2]
The projection effect can be used in architecture to design buildings that are cool in summer and warm in winter, by providing large vertical windows on the equator-facing side of the building (the south face, in the northern hemisphere): this maximizes insolation in the winter months when the Sun is low in the sky, and minimizes it in the summer when the noonday Sun is high in the sky. (The Sun's north/south path through the sky spans 47 degrees through the year).
Insolation figures are used as an input to worksheets to size solar power systems for the location where they will be installed.^[3] The figures can be obtained from an insolation map or by city or region from insolation tables that were generated with historical data over the last 30-50 years.
In the fields of civil engineering and hydrology, numerical models of snowmelt runoff use observations of insolation. This permits estimation of the rate at water is released from a melting snowpack. Field measurement is accomplished using a pyranometer.

See also

★ Albedo

★ Flux

★ Power density

★ Sun chart

References

1. Construction of a Composite Total Solar Irradiance (TSI) Time Series from 1978 to present
2. Looking across the water: Climate-adaptive buildings in the United States & Europe
3. Determining your solar power requirements and planning the number of components.

External links

★ Global Insolation Map

★ National Science Digital Library - Insolation

★ Yesterday‘s Australian Solar Radiation Map