Spatial structure of the 12-hour wave in the Antarctic as observed by radar

Riggin, D.M.; Fritts, D.C.; Jarvis, M.J.; Jones, G.O.L.. 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar. Earth, Planets and Space, 51 (7-8). 621-628. 10.1186/BF03353220

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Text (Open Access) Copyright © The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. BF03353220.pdf - Published Version Download (5MB) | Preview

Abstract/Summary

We present radar measurements of the 12-hour wave, a zonal wavenumber 1 westward propagating wave that exists in the southern polar mesopause region winds (Hernandez et al, 1993; Forbes et al, 1995). MF radar measurements of the horizontal winds at McMurdo (77.8° S, 166.67° E) show that the 12-hour wave is highly seasonal, occurring during the austral summer solstice. During these seasonal occurrences, the wave is highly intermittent with amplitude peaks of 30 m s-1. The burst-like occurrences of large 12-hour wave amplitudes are highly correlated between the zonal and meridional direction. The diurnal tide over McMurdo has a more constant amplitude, but it is also an almost exclusively summertime phenomenon. Inertia-gravity wave activity is evident at periods less than 12 hr during the austral winter months. The weakening of gravity wave activity during the summer is probably due to critical layer filtering by the zonal mean wind, 12-hour wave and diurnal tide which are all strong during this season. The 12-hour wave is confined in height to the vicinity of the zero crossing in the zonal winds above the westward jet. Extreme distortion is observed in the vertical phase fronts of the 12-hour wave which could signify either refraction or in situ forcing. The distortion in the phase fronts and localization of the 12-hour wave in time and height is apparently responsible for departures in period from the nominal 12 hours. We do not find the wave period to be systematically different from 12 hours. The association of the 12-hour wave events with shear in the mean wind suggests that refractive effects could conceivably cause a dilation in wave amplitude. However, the shear is of the opposite sign to cause this dilation unless the wave originates at higher altitudes and propagates downward into the mesosphere. Investigations are made of the zonal structure of the 12-hour wave by comparing phases of the 12-hour wind component between McMurdo and the dynasonde at Halley (75.8° S, 26.4° W). The phase is found to be stable and consistent with a westward propagating zonal wavenumber 2 structure during seasons when the 12-hour wave is weak. The migrating semidiurnal tide evidently dominates during these times of the year. During seasons when the 12-hour wave amplitude is large, the zonal structure is highly unstable and there is not an obvious dominant zonal wavenumber.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.1186/BF03353220
Programmes:	BAS Programmes > Pre 2000 programme
ISSN:	1343-8832
Date made live:	11 Nov 2013 15:29 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/503766

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