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• W220104696 abstract "A study of the middle atmosphere structure and the amplitude of its response to periodic heating of the middle atmosphere caused by ozone and having strong longitudinal variations is carried out on the basis of the numerical two-dimensional model of planetary waves and analysis of the data on the global ozone distribution (the TOMS data) and variations of the solar ultraviolet radiation (the data of the SUSIM instrument on board the UARS satellite). The analysis of the total ozone content shows that in some years the longitudinal irregularity amplitude may be as high as 100 Dobson units (DU). The corresponding variations of the stratosphere heating may reach 1 K per day. The calculations show that the solar ultraviolet radiation variations (according to the SUSIM instrument data they are about 1% with the period of 25-27 days corresponding to the solar rotation) lead to an selective (resonant) response of the middle atmosphere with the period of 25-27 days in the form of a propagating planetary wave. The amplitudes of such waves are a few geopotential meters for a geopotential disturbance and up to 1 K for temperature variations in the upper stratosphere." @default.
• W220104696 created "2016-06-24" @default.
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• W220104696 date "2003-01-01" @default.
• W220104696 modified "2023-09-23" @default.
• W220104696 title "Generation of wave motions in the middle atmosphere induced by variations of the solar ultraviolet radiation flux (based on the UARS satellite data)" @default.
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• W220104696 hasPublicationYear "2003" @default.
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