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    Response of OH airglow temperatures to neutral air dynamics at 78oN, 16oE during the anomalous 2003-2004 winter


    Dyrland, M.E. and Mulligan, F.J. and Hall, C.M. and Sigernes, F. and Tsutsumi, M. and Deehr, C.S. (2010) Response of OH airglow temperatures to neutral air dynamics at 78oN, 16oE during the anomalous 2003-2004 winter. Journal of Geophysical Research, 115 (D7). pp. 1-11. ISSN 0148-0227

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    Abstract

    Hydroxyl (OH) brightness temperatures from the mesopause region derived from temperature profiles from the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics (TIMED) satellite are compared with OH(6-2) rotational temperatures measured by spectrometer from Longyearbyen, Norway (780N, 16"E), during the winter 2003-2004. The two series correspond well, although the satellite measurements are higher by an average of 5.6 K * 4.4 K. Reasons for this apparent bias are discussed. The two series give a near-continuous temperature record from this winter, making it possible to study the response of the temperatures to neutral air dynamics observed from meteor radar measurements of meridional and zonal wind. Vertical profiles of 1.6 pm OH volume emission rates from SABER reveal that the unusually high temperatures observed during January and February 2004 (240-250 K) correspond to a very low and bright OH layer. Significant linear correlations are found between meridional wind, OH temperature, and peak altitude. These data support the theory that the high temperatures result from an anomalously strong upper stratospheric vortex that confined air to the polar regions, coupled with meridional transport, which led to a strong downwelling of atomic oxygen-rich air, thereby lowering the altitude of the OH layer. The SABER data reveal that the re-formation of the OH layer at approximately 78 km altitude accounted for an increase in temperature of approximately 15 K, while the remaining temperature increase (20-35 K) is attributed to adiabatic heating and chemical heating from the exothermic reactions involved in producing the vibrationally excited OH.

    Item Type: Article
    Additional Information: An edited version of this paper was published by AGU. Copyright (2010) American Geophysical Union. Acknowledgments: We are very grateful to the entire NASA TlMED/SABER team for making the SABER data freely avaiIable. We also thank the three anonymous reviewers for their constructive comments and suggestions, which helped improve the paper.
    Keywords: Atmospheric Processes; Middle atmosphere dynamics (0341, 0342); Atmospheric Composition and Structure; Airglow and aurora; Atmospheric Processes; Climate change and variability (1616, 1635, 3309, 4215, 4513); Planetary Sciences; Solid Surface Planets; Polar regions;
    Academic Unit: Faculty of Science and Engineering > Experimental Physics
    Item ID: 822
    Identification Number: https://doi.org/10.1029/2009JD012726
    Depositing User: Dr. Frank Mulligan
    Date Deposited: 08 Sep 2011 08:16
    Journal or Publication Title: Journal of Geophysical Research
    Publisher: American Geophysical Union (AGU)
    Refereed: Yes
    URI:

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