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contributor authorBallif, Jae R.
contributor authorVenkateswaran, S. V.
date accessioned2017-06-09T14:12:58Z
date available2017-06-09T14:12:58Z
date copyright1963/01/01
date issued1963
identifier issn0022-4928
identifier otherams-14879.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150488
description abstractThe hydroxyl bands in the glow emanating from the earth's upper atmosphere are chemically excited. The two possible precursor reactions are O3+H?OH*+O2 and O2*+H?OH*+O. Arguments are advanced in this paper to show that the night-time variations of the emission intensifies stimulated by these two reactions might be characteristically different. The relative importance of the reactions can therefore be judged by a systematic observational study of the intensity variations.
publisherAmerican Meteorological Society
titleOn the Temporal Variations of the OH Nightglow
typeJournal Paper
journal volume20
journal issue1
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1963)020<0001:OTTVOT>2.0.CO;2
journal fristpage1
journal lastpage4
treeJournal of the Atmospheric Sciences:;1963:;Volume( 020 ):;issue: 001
contenttypeFulltext


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