Abstract
WINDS in the upper atmosphere have been measured at Adelaide, South Australia (35°S) by radio observations of drifting meteor trails, using a combined continuous wave and pulse technique1. The systematic features of the winds can be described in terms of a prevailing component and 24-, 12- and 8-h periodic components. Here we are concerned primarily with the behaviour of the prevailing component in the height range 75–105 km for the six years from June 1966 to June 1972.
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References
Weiss, A. A., and Elford, W. G., Proc. Instn Radio Engnrs. Aust., 24, 197 (1963).
Groves, G. V., J. atmos. terr. Phys., 16, 344 (1959).
Belmont, A. D., Dartt, D. G., and Nastrom, G. D., Q. Jl R. met. Soc., 100, 203 (1974).
Green, J. S. A., Phil. Trans. R. Soc., A 271, 577 (1972).
Ebel, A. Tellus, 26, 325 (1974).
Gilman, P. A., Tellus, 16, 160 (1964).
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ELFORD, W. Prevailing winds in lower thermosphere. Nature 261, 123–124 (1976). https://doi.org/10.1038/261123a0
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DOI: https://doi.org/10.1038/261123a0
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