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contributor authorHanel, R. A.
contributor authorBandeen, W. R.
contributor authorConrath, B. J.
date accessioned2017-06-09T14:12:59Z
date available2017-06-09T14:12:59Z
date copyright1963/03/01
date issued1963
identifier issn0022-4928
identifier otherams-14887.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150497
description abstractHorizon sensors are essential elements in the orientation systems of many space vehicles and satellites. Their design and an evaluation of their capabilities and limitations requires a knowledge of the spectral radiance emitted by the Earth. This report investigates the discontinuity between the surface, the atmosphere, and outer space for various latitudinal, seasonal, climatic, and meteorological conditions. Calculations are carried out for the following five spectral intervals?the water vapor band from 6.33 to 6.85 microns, the ozone band from 8.9 to 10.1 microns, the atmospheric window from 10.75 to 11.75 microns, the carbon dioxide band from 14 to 16 microns, and finally the rotational water vapor band from 21 to 125 microns. The superior properties of the carbon dioxide band and the rotational water vapor region for horizon sensor purposes are shown.
publisherAmerican Meteorological Society
titleThe Infrared Horizon of the Planet Earth
typeJournal Paper
journal volume20
journal issue2
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1963)020<0073:TIHOTP>2.0.CO;2
journal fristpage73
journal lastpage86
treeJournal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 002
contenttypeFulltext


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