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Solar radiation
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Earth's axis and sunlight A flowchart diagram shows the average exchange of energy between Earth's surface, atmosphere, and space as percentages of incoming solar radiation, with arrows and labeled percentages illustrating how solar energy is absorbed, reflected, scattered, or emitted by clouds, the atmosphere, and the surface. Color-coded circles and boxes represent different forms of energy transfer, including solar radiation, longwave radiation, and non-radiative exchanges, highlighting the complexity of Earth's clima
See how differing amounts of solar radiation at the poles and Equator affect Earth's climate and atmosphere
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Nicolaus Copernicus. Nicolas Copernicus (1473-1543) Polish astronomer. In 1543 he published, forward proof of a Heliocentric (sun centered) universe. Coloured stipple engraving published London 1802. De revolutionibus orbium coelestium libri vi.
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Solar radiation

astronomy
Written by
Harold Zirin
Professor of Astrophysics, Emeritus; Director and Builder, Big Bear Solar Observatory, California Institute of Technology, Pasadena. Author of Astrophysics of the Sun and others.
Harold Zirin
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Solar radiation, electromagnetic radiation, including X-rays, ultraviolet and infrared radiation, and radio emissions, as well as visible light, emanating from the Sun. Of the 3.8 × 1033 ergs emitted by the Sun every second, about 1 part in 120 million is received by its attendant planets and their satellites. The small part of this energy intercepted by Earth (the solar constant, on average 1.4 kilowatts per square metre) is of enormous importance to life and to the maintenance of natural processes on Earth’s surface (see also sunlight). The energy output of the Sun has its peak at a wavelength of 0.47 micrometre (0.000019 inch; a micrometre is 10−6 metre), and the Sun radiates about 8 kilowatts per square cm of its surface.

Harold Zirin