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

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Spectral Brightness of the Sky,le results, for example, [1–3], were obtained only for a small set of parameters using visual and photoelectric photometers with wideband filters. In a number of cases, transmittance was not determined [2], and the results were given in relative units (readings from various points in the sky were tied to the zenith).
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The Height of the Twilight Ray, When observations are made in direction BM, the height of the twilight layer in this direction is the difference h = OM −R, i.e., the height above the earth’s surface of the point of intersection of the line of sight BM and the twilight ray SM.
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Erstes Kapitel Stetige Konvergenz at 25 frames/sec. It was also necessary to create, if only rather approximately, a method of determining a quality criterion for an astronomical (in this case, a point) image and, thereby, to be able to compare quantitatively the changes in the structure of the image caused by scintillation.
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Some Statistical Determinations of the Instability of Television Images of Stars, at 25 frames/sec. It was also necessary to create, if only rather approximately, a method of determining a quality criterion for an astronomical (in this case, a point) image and, thereby, to be able to compare quantitatively the changes in the structure of the image caused by scintillation.
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