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Six years of hydroxyl airglow rotational temperatures at Davis station (68.6S,78.0E), Antarctica. PSMOS (Planetary Scale Mesopause Observing System) 2000 Workshop. University of Toronto, Canada, 23-26 May, 2000., 2000 (Ref: 9228)
Category 3: Abstract

An overview of the Davis station hydroxyl airglow temperature program will be given. Seasonal structure, planetary scale periodicities and inter-year variability determined from six years of hydroxyl airglow rotational temperatures will be presented. Solar cycle influences will be examined.

Antarctic noctilucent clouds: the upper atmosphere exposed to view. The Physicist, 2000 (Ref: 9361)
Category 3: Article

Noctilucent ("night shining") clouds can be a beautiful, awe-inspiring sight but they are viewed by some scientists as harbingers of mans impact on his environment. We use a rare sighting of a noctilucent cloud at Davis station (68.6S, 78.0E)…

Tidal periodicities in observations of the OH(6-2) emission from eastern Antarctica ANARE Reports, 2001 (Ref: 10036)
Category 1: Peer-reviewed literature

High-resolution Fabry-Perot spectrometer observations of the OH(62) Q1(1) line, l834.46 nm, were made at Mawson, 67.6ºS 62.9ºE, and Davis, 68.6ºS 78.0ºE, Antarctica, in 1997. The observing program resulted in three sets of continuous OH observations suitable for tidal analysis: July 25…

A large Vertical Wind in the thermosphere at the Auroral Oval/Polar Cap Boundary seen simultaneously from Mawson and Davis, Antarctica. Journal of Atmospheric and Solar-Terrestial Physics, 1999 (Ref: 8819)
Category 1: Peer-reviewed literature

Ground-based Fabry-Perot spectrometer observations from the Australian Antarctic stations of Davis and Mawson show an upward wind ~100 m s-1 in the thermosphere at ~240 km altitude on the night of Day of Year 159 in 1997.

Thermospheric wind field over Mawson and Davis, Antarctica; simultaneous observations by two Fabry-Perot spectrometers of l630 nm emission. Journal of Atmospheric and Solar-Terrestrial Physics., 1999 (Ref: 8818)
Category 1: Peer-reviewed literature

The thermopheric oxygen l630 nm emission has been observed using high-resolution Fabry-Perot spectrometers at Mawson (67.6°S, 62.9°E) and Davis (68.6°S, 78.0°E), Antarctica. A new technique, combining the results from the two instruments, is used to derive vector wind fields.

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