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Hernandez et al. 1990
Hernandez, G., Clark, K.C., Smith, R.W., Roble, R.G. and Gress, J. (1990). Thermospheric dynamics at the South Pole. Geophysical Research Letters 17: doi: 10.1029/90GL01256. issn: 0094-8276.

A self-aligning Fabry--Perot spectrometer has been installed at Amundsen-Scott Station, Antarctica (Geographic South Pole) and has been used to determine neutral upper thermosphere winds and temperatures, obtained from the measurement of the Doppler shift and Doppler width of the line profiles of the [OI> 15,867 K (630 nm) line emission, during the austral winter of 1989 (April 1989 to September 1989). These first ground-based measurements of F-region neutral dynamics at the South Pole, show a rich variety of dynamic phenomena and strong couplings with the ionospheric plasma. Data for two contrasting days in April 1989 are presented here. The data of April 23 UT illustrate the diurnal variations of winds and temperatures during geomagnetic quiet-to-moderate conditions, while the data of April 27 UT illustrate diurnal variations during geomagnetically disturbed periods. These data are compared with the average pattern obtained at a similar geomagnetic latitude and conditions, but in the Northern Hemishpere (Longyearbyen, Spitsbergen) and with predictions of the average dynamics in the South Pole region made by the NCAR thermosphere-ionosphere general circulation model (TIGCM). The measured winds at the South Pole have a stronger prevailing westward component in its diurnal cycle than is either observed at Longyearbyen (in the Northern Hemisphere) or predicted at South Pole by the TIGCM. ¿ American Geophysical Union 1990

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Abstract

Keywords
Atmospheric Composition and Structure, Thermosphere—composition and chemistry
Journal
Geophysical Research Letters
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Publisher
American Geophysical Union
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