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Meteorological optics is "that part of atmospheric optics concerned with the study of patterns observable with the naked eye". [2] Nevertheless, the two terms are sometimes used interchangeably. Meteorological optical phenomena, as described in this article, are concerned with how the optical properties of Earth's atmosphere cause a wide range ...
Atmospheric Optics site graphical user interface. It creates simulations by accurately tracing up to several million light rays through mathematical models of ice crystals. 2010 Halopoint2 Jukka Ruoskanen webpage graphical user interface. Ray-tracing code for various ice crystals with graphical user interface 2008 HALOSKY [5] Stanley David ...
Atmospheric optical phenomena include: Afterglow; Airglow; Alexander's band, the dark region between the two bows of a double rainbow. Alpenglow; Anthelion; Anticrepuscular rays; Aurora (northern and southern lights, aurora borealis and aurora australis) Belt of Venus; Brocken Spectre; Circumhorizontal arc; Circumzenithal arc; Cloud iridescence ...
Optical phenomena encompass a broad range of events, including those caused by atmospheric optical properties, other natural occurrences, man-made effects, and interactions involving human vision (entoptic phenomena).
Atmospheric optical phenomena are often due to the interaction of light from the sun or moon with the atmosphere, clouds, water, or dust and other particulates. Subcategories This category has the following 6 subcategories, out of 6 total.
Lunar corona A solar corona up Beinn Mhòr (South Uist). In meteorology, a corona (plural coronae) is an optical phenomenon produced by the diffraction of sunlight or moonlight (or, occasionally, bright starlight or planetlight) [1] by individual small water droplets and sometimes tiny ice crystals of a cloud or on a foggy glass surface.
In the 1960s, Fried published a series of papers on the optical effects of atmospheric turbulence that provided much of the analytic foundations for the development of adaptive optics systems, and that resulted in the definition of the quantity now known as Fried’s parameter. In addition, his 1966 paper, "Limiting Resolution Looking Down ...
Multiple-scattering effects of light scattering by particles are treated by radiative transfer techniques (see, e.g. atmospheric radiative transfer codes). The relative size of a scattering particle is defined by its size parameter x, which is the ratio of its characteristic dimension to its wavelength: