Airglow imaging observations of small‐scale structures driven by convective instability in the upper mesosphere over Tirunelveli (8.7°N)

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dc.contributor.author Narayanan, V. Lakshmi
dc.contributor.author Gurubaran, S.
dc.contributor.author Emperumal, K.
dc.date.accessioned 2015-10-13T10:39:47Z
dc.date.accessioned 2021-02-12T09:35:34Z
dc.date.available 2015-10-13T10:39:47Z
dc.date.available 2021-02-12T09:35:34Z
dc.date.issued 2010
dc.identifier.citation JGR, 115, D19119, doi:10.1029/2009JD012937, 2010 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/571
dc.description.abstract Airglow imaging observations of broadband OH Meinel band emissions made on the night of 20 January 2007 from the tropical Indian site Tirunelveli (8.7°N, 77.8°E) reveal large‐ and small‐scale wave features that are aligned perpendicular to each other and that are associated with gravity wave dynamics. The large‐scale waves were the signatures of propagating quasi‐monochromatic (QM) waves, whereas the small‐scale features were identified to be ripples generated by convective instability in the mesosphere‐lower thermosphere (MLT) region. The QM waves showed consistent propagation toward the northwest direction throughout the observation period of ∼4.5 hr, whereas the ripples that manifested as short‐lived patches in the airglow images were transient and did not show any prominent phase propagation. In addition to these well‐resolved structures in images, we infer the presence of waves with relatively longer observed time periods (compared with the observed time period of QM waves) from the spectrum of the time series generated with zenith intensity values derived from the images. From the complementary wind and temperature data obtained with co‐located MF radar and Sounding of Atmosphere with Broad band Emission Radiometry on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics mission, an attempt is made to understand the dynamic processes occurring in the vicinity of the mesopause during the night of 20 January 2007. The uniqueness of the present observations is that there were short‐lived ripple patches seen in various parts of the sky during the entire observation period of 4.5 hr. The precipitation rates obtained by the Tropical Rainfall Measuring Mission satellite mission suggest that the deep convective activity occurring over the equatorial eastern Indian Ocean provided a plausible source mechanism for sustained generation of the waves observed over Tirunelveli during this night. en_US
dc.language.iso en en_US
dc.subject Airglow imaginh en_US
dc.subject Upper Mesosphere en_US
dc.subject Mesosphere en_US
dc.subject Tirunelveli en_US
dc.subject Tropical Area en_US
dc.subject OH Meinel band en_US
dc.subject Quasi-monochromatic waves en_US
dc.subject MLT region en_US
dc.title Airglow imaging observations of small‐scale structures driven by convective instability in the upper mesosphere over Tirunelveli (8.7°N) en_US
dc.type Article en_US
dc.identifier.accession 091117


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