- Project plans
- Project activities
- Legislation and standards
- Industry context
- Specialist wikis
Last edited 21 Jan 2021
Radiation is a heat transfer mechanism, along with conduction, convection, phase change and mass transfer. All bodies which are hotter than 0°K emit thermal radiation. They also absorb thermal radiation emitted by their surroundings. The difference in the total amount of radiation emitted and absorbed by a body at any given moment may result in a net heat transfer which will produce a change in the temperature of that body.
Thermal radiation includes all those wavelengths of the electromagnetic spectrum which will heat a body when absorbed by it, ranging from about 100nm to 100,000nm. In general, the higher the temperature of a body, the lower the average wavelength of the radiation it emits.
The range of terrestrial temperatures experienced within the built environment is relatively small, and relative to the temperature of the sun this range is ‘cold’ and so radiating at a ‘long’ wavelength compared to the sun. This anomaly allows us to categorise thermal radiation as short-wave solar radiation and terrestrial or long wave infra-red radiation.
Solar radiation may be considered to include the ultra violet, visible and near or short wave infra-red wavebands. Around 97% of the solar radiation incident upon the earth's surface is within the range 300 to 2,300nm. Its spectral profile is roughly analogous to that of a black body at 5762°K, and as terrestrial temperatures are unlikely to reach anything like this temperature, solar radiation reaching the earth may be treated as a pure thermal gain.
Most 'terrestrial' radiation occurs within the far or long wave infra-red wavebands. The wavelength of terrestrial radiation varies with temperature, however at room temperature approximately 97% of the radiation emanating from a perfect emitter will be within the range 3,000nm to 50,000nm.
The atmosphere is relatively transparent to solar radiation, this means it allows sunlight to enter the atmosphere and heat the Earth’s surface. These surfaces then re-radiate that heat as long-wave infra-red radiation, which greenhouse gases tend to absorb rather than transmit. The result is that the long-wave infra-red radiation is ‘trapped’ and heat accumulates in the atmosphere causing a warming process.
The way in which thermal radiation affects different materials is determined by their transmittance, reflectance and absorptance. These properties change for different wavelengths of radiation and for different angles of incidence.
 Related articles on Designing Buildings Wiki
- Climate change science.
- Heat transfer.
- Low-e glass.
- Phosphorescent building materials.
- Radiant heating.
- Shading coefficient.
- Solar gain.
- Solar heat gain coefficient.
- Solar thermal panels.
- Tempering heating.
- Thermal bridge.
- Thermal optical properties
- U value.
- Visible light.
Featured articles and news
Her development as a thinker and writer. Book review.
Smart motorway strategies.
Actuate UK urges change of deadline to at least December 2022.
Study shows harmful impact of late payments on SME personnel.
Upcoming changes to the commercial supply and purchase of chemicals.
CLC introduces card for learners.
CIOB members recognised for public procurement.
Experts discuss the complex issues damaging the supply chain.
The co-founder of Get Kids into Survey discusses career paths for kids.
Report examines lack of detail in the Government's vision.
Look up construction terms on any website direct from your browser.
The revival of the public sphere in Toronto.
The story behind the copycat architecture craze.
Insight into construction materials supply and demand issues.