Airglow measurements of gravity wave propagation and damping over Kolhapur (16.5°N, 74.2°E)

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dc.contributor.author Ghodpage, R.N.
dc.contributor.author Taori, A.
dc.contributor.author Patil, P.T.
dc.contributor.author Gurubaran, S.
dc.contributor.author Sharma, A.K.
dc.contributor.author Nikte, S.
dc.contributor.author Nade, D.
dc.date.accessioned 2015-12-08T06:12:13Z
dc.date.accessioned 2021-02-12T09:39:02Z
dc.date.available 2015-12-08T06:12:13Z
dc.date.available 2021-02-12T09:39:02Z
dc.date.issued 2014
dc.identifier.citation International Journal of Geophysics, v.2014, ID 514937, 2014, doi: 10.1155/2014/514937 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/793
dc.description.abstract Simultaneous mesospheric OH and O  (1S) night airglow intensity measurements from Kolhapur (16.8°N, 74.2°E) reveal unambiguous gravity wave signatures with periods varying from 01 hr to 9 hr with upward propagation. The amplitudes growth of these waves is found to vary from 0.4 to 2.2 while propagating from the OH layer (~87 km) to the O (1S) layer (~97 km). We find that vertical wavelength of the observed waves increases with the wave period. The damping factors calculated for the observed waves show large variations and that most of these waves were damped while traveling from the OH emission layer to the O (1S) emission layer. The damping factors for the waves show a positive correlation at vertical wavelengths shorter than 40 km, while a negative correlation at higher vertical wavelengths. We note that the damping factors have stronger positive correlation with meridional wind shears compared to the zonal wind shears. en_US
dc.language.iso en en_US
dc.subject Gravity wave en_US
dc.subject Night airglow en_US
dc.subject Kolhapur en_US
dc.title Airglow measurements of gravity wave propagation and damping over Kolhapur (16.5°N, 74.2°E) en_US
dc.type Article en_US
dc.identifier.accession 091457


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