Titlebook: Atmospheric Optics; Nikolai B. Divari (Chairman) Book 1970 Consultants Bureau, New York 1970 optics

perpetual

Erstes Kapitel Stetige Konvergenzpheric layers that cause this phenomenon. Since the vibrations were estimated visually with the eyepiece grid, we dealt with near-maximum amplitudes. It was shown that the upper limit of atmospheric heterogeneities that were capable of causing displacement as a unit of large sections of an image of

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Congeal

Funktionen von mehreren Veränderlichenx. The former value characterizes the total light attenuation in the atmosphere while the latter describes the attenuation due only to scattering and gives information about the luminous fluxes scattered in different directions. While optical thickness can be determined directly, for example, by mea

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https://doi.org/10.1007/978-3-8348-2340-3 of applied problems. In twilight studies, for example, in order to take into account the influence of the troposphere, the brightness of the daytime clear sky must be known in absolute units for a large set of parameters. Experimental data on the brightness distribution make it possible to judge ho

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Differentialrechnung im Komplexen,rious directions by almucantar measurements of the polarization of light scattered by the atmosphere. The almucantar measurements were made visually with a Martens polarimeter without filters and, therefore, had the following shortcomings: the results depended upon the sensitivity of the observer’s

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Der Riemannsche Abbildungssatz,on of the sinking of the sun. This was first demonstrated by V. G. Fesenkov [1] and later examined in detail by N. M. Shtaude [2]. The thickness of the layer that determines the main flow of scattered radiation is not great, so in the first approximation the layer is often replaced by a single ray (