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atmospheric optics

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Weather balloons, atmospheric effects, optical illusions.
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The unique optical properties of the atmosphere cause a wide range of spectacular optical phenomena.
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This optical atmospheric effect had fooled Peary, and now they had committed time, energy, and resources to explore something that was not real.
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Also aboard will be a 20-inch [50 cm] optical window to study atmospheric gases, coral-reef bleaching, hurricanes, and other natural phenomena on earth.
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This illusion so confounded Ptolemy that he incorrectly attributed it to atmospheric refraction when he described it in his treatise, Optics.
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Techniques known as adaptive optics have been used to eliminate the atmospheric disruption of images and achieve results that approach the diffraction limit.
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Abū ‘Alī al-Ḥasan ibn al-Haytham (Alhazen) of Basra (10th-11th century), mathematician and physicist; made significant contributions to the theory of optics, including refraction, reflection, binocular vision, and atmospheric refraction; first to explain correctly vision as the effect of light coming from an object to the eye.
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Common optical phenomena are often due to the interaction of light from the sun or moon with the atmosphere, clouds, water, dust, and other particulates.
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The most common seeing measurement is the full width at half maximum (FWHM) of the optical intensity across the seeing disc (the point spread function for imaging through the atmosphere).
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Keck II was able to pick up the eruption thanks to its adaptive optics, which “flex fast enough to compensate for the blurring caused by turbulence in Earth’s atmosphere,” says Science News.
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The company develops, manufactures and markets advanced atmospheric sensors using optical,
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The main focus is aerosols, clouds and reactive gases in the atmosphere, and their physical, optical and chemical properties.
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A halo (ἅλως; also known as a nimbus, icebow or gloriole) is an optical phenomenon produced by the interaction of light from the sun or moon with ice crystals in the atmosphere, resulting in colored or white arcs, rings or spots in the sky.
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During 1847, he got his doctorate from the University of Halle on optical effects in the Earth's atmosphere.
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b) If the atmospheric forcing is strengthened, for instance by increasing the optical depth to surface IR radiation through a rising atmospheric content of GHGs, the Earth’s surface will warm INdirectly.
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The FWHM of the point spread function (loosely called seeing disc diameter or "seeing") is the best possible angular resolution that can be achieved by an optical telescope in a long-exposure image, and corresponds to the FWHM of the fuzzy blob seen when observing a point-like source (such as a star) through the atmosphere.
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AO technology improves the performance of optical systems by reducing the effect of atmospheric distortion.
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It is used in astronomical telescopes[1] and laser communication systems to remove the effects of atmospheric distortion, in microscopy,[2] optical fabrication[3] and in retinal imaging systems[4] to reduce optical aberrations.
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It is used in astronomical telescopes[1] and laser communication systems to remove the effects of atmospheric distortion, in microscopy,[2] optical fabrication[3] and in retinal imaging systems[4] to reduce optical aberrations.
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The telescope has an innovative five-mirror design that includes advanced adaptive optics to correct for the turbulent atmosphere, giving exceptional image quality.
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The instrument uses advanced adaptive optics to remove atmospheric distortion, a coronagraph to block most of the light from the central star and a combination of differential imaging and polarimetry to isolate the light from features in the disc.
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[3] The telescope optics also include correction for dispersion by the Earth’s atmosphere.
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The effects of the atmosphere can be compensated for in some modern telescopes by the adaptive optics technique.
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It is commonly used on astronomical telescopes to remove the effects of atmospheric distortion, or astronomical seeing. Adaptive optics works by measuring the distortion and rapidly compensating for it either using deformable mirrors or material with variable refractive properties.
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NILU conducts research on a range of topics related to the geophysical climate system, such as soil moisture, atmospheric water transport and circulation, meteorology and cloud optical properties. Page content:
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