The sunlight is sending us radiation over a wide range of wavelength at differing intensities. The electro-magnetic solar radiation impinging top top the top edge that the environment is dubbed extra-terrestrial radiation. The mean integral for the finish spectrum is 1,367 W/m² (the Solar Constant).

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The regular measurement the the wavelength of solar and also atmospheric radiation is the nanometer (nm, 10-9 m) and for infrared radiation is the micrometer (µm, 10-6 m). The range is presented in listed below table. In astronomy and older books you may see wavelengths in Ångström (Å, 10-10 m).

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The meteorologically far-ranging spectral range extends indigenous 300nm come 3000nm (short-wave radiation). About 96% that the complete extra-terrestrial radiation is located within this spectral range. The preferably radiation soot of the solar spectrum wake up at 500 nm, towards the blue end of the visible range.

The complete spectrum comprises the ultraviolet (UV), visible (Vis) and infrared (IR) wavelengths. However, this wavelength ranges need to be sub-divided depending on the individual applications fields. Best known are the prismatic color of visible light, the color of the rainbow. IR is separation into close to infrared (NIR) and also far infrared (FIR).

UV is typically sub-divided right into UV-A, UV-B and also UV-C radiation. About 6% that the full solar radiation fall on the planet is ultraviolet. Much shorter wavelengths (higher frequency) have greater energy, for this reason increasing the result on biological and chemical systems.

The attenuation of solar radiation passing through our environment is as result of the adhering to processes:

ultraviolet rangeScattering by molecules and aerosol particles and absorption by Ozone, Sulphur Dioxide, Nitrogen Dioxide and trace gases.

visible rangeScattering by molecules and aerosol particles, tiny absorption by aerosol particles, Ozone and other map gases.

infrared rangeAbsorption through water vapour and also aerosol corpuscle but small scattering.

Molecular Ozone in the top layers of our environment functions as a filter for ultraviolet radiation and also the effect increases with shorter wavelengths. Whereas almost all UV-A radiation get the floor surface, almost 90% the the UV-B radiation is soaked up by the Ozone, and all of the UV-C. Throughout this process, brand-new Ozone (O³) is additionally produced indigenous atmospheric Oxygen and this reinforces the process.

Changes of the atmospheric Ozone content will certainly especially affect the lot of UV-B. Raising Ozone great concentration way decreasing UV-B radiation and a to decrease Ozone layer method increasing UV-B radiation reaching the surface.

Solar radiation is the driver for plenty of chemical, biological and physical phenomena in the atmosphere, on the ground and in the seas.

A major effect the solar radiation reaching the earth’s surface ar is the it is warming the up, which is an important for our existence. 30% the the extra-terrestrial radiation solar radiation (yellow in Illustration below) is reflected earlier into space but approximately 51% is took in by land and water and another 19% is took in by the clouds and atmosphere.

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Long-wave far infrared radiation (FIR) is presented in red and is greatly transformed short-wave energy that is re-radiated indigenous the land, water, clouds and also atmosphere. Just a little amount the the complete energy stays on the earth but this is sufficient to preserve all the biological processes on our planet and also to drive the weather systems.

Variations in the reflected and also re-radiated power do, of course, influence the energy balance between ground and also atmosphere. This energy balance, in turn, impacts meteorological conditions and other processes, for example the growth of plants.

Rising concern for the survival of our atmosphere and means of life, along with the desire for greater crop yields, provides it necessary to have available an accurate information top top incoming and reflected radiation. In this respect the distribution of the radiation soot at different wavelengths can be of the utmost importance.

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Nowadays, measure up solar radiation is extremely essential in plenty of different areas of application, such as climatology, meteorology, hydrology, contamination forecasting, solar energy, agriculture and product testing.