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Nowcasting convection velocity in the high-latitude ionosphere using statistical models. Journal of Atmospheric and Solar-Terrestrial Physics, 1999 (Ref: 8763)
Category 1: Peer-reviewed literature

The Weimer and IZMEM statistical convection models are driven with a time series of interplanetary magnetic field (IMF) measurements made onboard the Wind spacecraft. The model outputs are used to infer convection velocity at Casey, Antarctica (80.8°S geomagnetic latitude)…

Signatures of the ionospheric cusp in digital ionosonde measurements of plasma drift above Casey, Antarctica Journal of Geophysical Research, 1999 (Ref: 8752)
Category 1: Peer-reviewed literature

Signatures of the ionospheric cusp in HF digital ionosonde measurements of plasma drift made at the polar cap station Casey, Antarctica (-80.8° geomagnetic latitude) are investigated. Measurements recorded during the campaign interval February 13-17…

Application of the Dopplionogram to Doppler-sorted interferometry measurements of ionospheric drift velocity Radio Science, 1999 (Ref: 8715)
Category 1: Peer-reviewed literature

The Dopplionogram was developed as a method of displaying Doppler shifts along the frequency axis of ionograms recorded using B-mode soundings of the Dynasonde, an early type of HF digital ionosonde.

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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