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Detailed Reference Information |
Plagmann, M., Marsh, S.H., Baggaley, W.J., Bennett, R.G.T., Deutsch, K.A., Fraser, G.J., Hernandez, G., Lawrence, B.N., Plank, G.E. and Smith, R.W. (1998). Annual variation of airglow heights derived from wind measurements. Geophysical Research Letters 25: doi: 10.1029/1998GL900212. issn: 0094-8276. |
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Three independent techniques for measuring wind in the mesosphere and lower thermosphere region were compared using simultaneous measurements during the period May 1997 to April 1998. The three instruments used, a Fabry-Perot spectrometer, a medium frequency radar, and a meteor radar, are located on New Zealand's South Island. The results obtained during this investigation show reasonable agreement amongst the three methods, in particular between the Fabry-Perot and the meteor radar. Correlation analysis of the meteor radar height-resolved winds and the Fabry-Perot spectrometer winds provides a valuable method for determining airglow heights. The results from the height determinations show a yearly variation of the OH emission layer, with its lowest height during summer, while the OI emission layer is found to remain at a relatively constant height. ¿ 1998 American Geophysical Union |
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Abstract |
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Keywords
Atmospheric Composition and Structure, Airglow and aurora, Atmospheric Composition and Structure, Instruments and techniques |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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