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contributor authorCraig, Richard A.
contributor authorGille, John C.
date accessioned2017-06-09T14:14:47Z
date available2017-06-09T14:14:47Z
date copyright1969/03/01
date issued1969
identifier issn0022-4928
identifier otherams-15571.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151258
description abstractA detailed numerical integration of the equation of radiative transfer over the 62 µ line of atomic oxygen is described. The results show that the cooling rate h in the lower thermosphere is appreciably lower than the value (hB) given by Bates? approximate expression, and may even be negative near the mesopause. For the CIRA atmosphere, hhB = 0.02, 0.21 and 0.50 at altitudes 100, 110 and 120 km, respectively, and reaches 0.88 above 200 km. In relating cooling rates to temperature changes, a calculation of cp is performed which includes the effects of dissociation and accessibility of vibrational levels. The latter leads to an increase of the same order as the former.
publisherAmerican Meteorological Society
titleCooling of the Thermosphere by Atomic Oxygen
typeJournal Paper
journal volume26
journal issue2
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1969)026<0205:COTTBA>2.0.CO;2
journal fristpage205
journal lastpage209
treeJournal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 002
contenttypeFulltext


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