Solar radiation is the full spectrum of light given off by the sun. It includes visible light and all other frequencies of radiation on the electromagnetic spectrum. Compared to familiar energy sources on Earth, the sun emits a tremendous amount of energy into space. The type of radiation given off by the sun is a product of its high temperature, which is caused by nuclear fusion inside the sun’s core. Solar radiation is studied by scientists for its effects on phenomena on Earth, such as weather, and for the science of astronomy.
The sun was formed about 4.5 billion years ago when a cloud of gas collapsed upon itself. Gravity caused the large amount of matter, which was primarily hydrogen, to pull itself together tightly; a very high pressure resulted in the sun’s core. This pressure became so great that hydrogen atoms began to fuse together, a process that releases much heat energy. The temperature of any collection of matter, including the sun, is what gives rise to emitted radiation.
Only a small fraction of solar radiation ever reaches Earth; the majority is radiated into empty space. Even the fraction that does reach Earth, however, is much larger than the amount of energy that is consumed on Earth by sources such as fossil fuels. The average power consumed by humans during 2008 was about 1.5 x 1013 watts. By comparison, the average power than reaches Earth via sunlight is more than 10,000 times larger. The tremendous amount of power radiated by the sun can be attributed to its large mass and high temperature.
Sunlight is measured in different ways. One instrument that measures sunlight from a full 180 degree field of view is called a pyranometer. A pyrheliometer is a device that is pointed directly at the sun for radiation measurements. Solar radiation is measured in a quantity called irradiance, which has standard units of watts per square meter. The average solar irradiance at the Earth’s distance from the sun is about 1,366 watts per square meter.
Measurements of solar radiation tend to fluctuate somewhat over time. Part of the reason for this fluctuation is that Earth’s orbit is not perfectly circular, and Earth-based observers are constantly changing their distance from the sun. Actual variations in solar radiation also give rise to fluctuations in measurements, but these amounts are usually small. Some of these variations have been observed to follow an 11-year cycle. Periodic fluctuations like these have been measured to affect levels of solar irradiance by 0.1%
