Atmos. Chem. Phys. Discuss., 11, 16185-16206, 2011
www.atmos-chem-phys-discuss.net/11/16185/2011/
doi:10.5194/acpd-11-16185-2011
© Author(s) 2011. This work is distributed
under the Creative Commons Attribution 3.0 License.
Review Status
This discussion paper has been under review for the journal Atmospheric Chemistry and Physics (ACP). Please refer to the corresponding final paper in ACP.
Observation of a mesospheric front in a dual duct over King George Island, Antarctica
J. V. Bageston1, C. M. Wrasse2, P. P. Batista1, R. E. Hibbins3, D. C. Fritts4, D. Gobbi1, and V. F. Andrioli1
1Instituto Nacional de Pesquisas Espaciais (INPE), São José dos Campos, Brazil
2Vale Soluções em Energia (VSE), São José dos Campos, Brazil
3British Antarctic Survey (BAS), Cambridge, UK, and Norwegian University of Science and Technology (NTNU), Trondheim, Norway
4Colorado Research Associates (CoRA), Boulder, USA

Abstract. A mesospheric bore was observed with an all-sky airglow imager on the night of 9–10 July 2007 at Ferraz Station (62° S, 58° W), located on King George island on the Antarctic Peninsula. The observed bore propagated from southwest to northeast with a well defined wave front and a series of crests behind the main front. There was no evidence of dissipation during its propagation within the field of view. The wave parameters were obtained via a 2-D Fourier transform of the imager data providing a horizontal wavelength of 33 km, an observed period of 6 min, and a horizontal phase speed of 92 m s−1. Simultaneous mesospheric winds were measured with a medium frequency (MF) radar at Rothera Station (68° S, 68° W) and temperature profiles were obtained from the SABER instrument on the TIMED satellite. These wind and temperature profiles were used to estimate the propagation environment of the bore. A wavelet technique was applied to the wind in the plane of bore propagation at the OH emission height spanning three days centered on the bore event to define the dominant periodicities. Results revealed a dominance of near-inertial periods, and semi-diurnal and terdiurnal tides suggesting that the ducting structure enabling bore propagation occurred on large spatial scales. The observed tidal motions were used to reconstruct the winds employing a least-squares method, which were then compared to the observed ducting environment. Results suggest an important contribution of large-scale winds to the ducting structure, but with buoyancy frequency variations in the vertical also expected to be important. These results allow us to conclude that the bore was supported by a duct including contributions from both winds and temperature (or stability). A co-located airglow temperature imager operated simultaneously with the all-sky imager confirmed that the bore event was the dominant small-scale wave event during the analysis interval.

Citation: Bageston, J. V., Wrasse, C. M., Batista, P. P., Hibbins, R. E., Fritts, D. C., Gobbi, D., and Andrioli, V. F.: Observation of a mesospheric front in a dual duct over King George Island, Antarctica, Atmos. Chem. Phys. Discuss., 11, 16185-16206, doi:10.5194/acpd-11-16185-2011, 2011.
 
Search ACPD
Discussion Paper
XML
Citation
Final Revised Paper
Share