Optical window

Rough plot of Earth's atmospheric transmittance (or opacity) to various wavelengths of electromagnetic radiation, including visible light.

The optical window is the portion of the optical spectrum that is not blocked by the Earth's atmosphere. The window runs from around 300 nanometers (ultraviolet-B) up into the range the human eye can detect, roughly 400–700 nm and continues up to approximately 2 μm.[1][2] Sunlight mostly reaches the ground through the optical atmospheric window;[3][4] the Sun is particularly active in most of this range (44% of the radiation emitted by the Sun falls within the visible spectrum and 49% falls within the infrared spectrum).[5]

  1. ^ Dwivedi, Ravi Shankar (2017). Remote Sensing of Soils. Springer. p. 13. ISBN 978-3-662-53740-4. OCLC 959595730.
  2. ^ Thorne, Anne P. (2012). Spectrophysics. Springer Science & Business Media. p. 3. ISBN 978-94-009-1193-2. OCLC 906664124.
  3. ^ Fluorocarbons, Environmental and Health Implications: Environmental Impact Statement. Food and Drug Administration. 1978. p. 79. OCLC 4611045.
  4. ^ Stergis, Christos G. (1966). Rayleigh Scattering in the Upper Atmosphere. Air Force Cambridge Research Laboratories, Office of Aerospace Research, United States Air Force. p. 273. OCLC 1037802615.
  5. ^ "Climate Science Investigations South Florida - Energy: The Driver of Climate". www.ces.fau.edu. Retrieved 2021-12-26.

From Wikipedia, the free encyclopedia · View on Wikipedia

Developed by Nelliwinne