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

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https://doi.org/10.1007/978-3-0348-0169-0ndard atmospheres, summarizing the results of studies of structure and composition, give densities, pressures, temperatures, molecular weights, and other structural parameters up to very high altitudes for a great variety of geophysical conditions: time of day, season, solar cycle, etc. Other atmosp

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Partialbruchzerlegung und Residuumkalkül early period of twilight, when ζ. > 6–7°, when the primary twilight segment is not yet detached from the horizon on the antisolar vertical circle or is at a negligible distance from it [2]. If it is assumed that during bright twilight the degree of higher-order polarization is negligible or entirel

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Normale Familien von meromorphen Funktionenes when the image quality satisfies the observer. Underlying this method is the assumption, which was made long ago by Donjon and Kude, that at some instant it is likely that the atmosphere will quiet down on the line of sight from the telescope objective to the star [3]. The work of Platt, who in 1

Malaise

Funktionen von mehreren Ver?nderlichenspheric scattering of sunlight. To obtain the true scattering indicatrix, we must eliminate from the brightness indicatrix this multiply scattered light. This is one of the central problems of atmospheric optics. I proposed a method for this that is apparently simpler than all of the others [1]. Obv

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敲竹杠

Measuring Limb Vibrations of Solar Images,uctuations in the lowest atmospheric layer or whether an important role is played by localized high-altitude layers with a wavy refractive-index structure. Similar disagreements arise in explanations of ultralong UHF propagation. Some researchers attribute it to incoherent scattering by turbulent fl

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Eliminating Multiple Scattering and Reflection of Light from the Underlying Surface from the Scattespheric scattering of sunlight. To obtain the true scattering indicatrix, we must eliminate from the brightness indicatrix this multiply scattered light. This is one of the central problems of atmospheric optics. I proposed a method for this that is apparently simpler than all of the others [1]. Obv