Abstract
As Professor Holton has reminded us (q.v., this Proceedings), the terrestrial quasibiennial oscillation or QBO is a remarkably persistent phenomenon. It has been clearly seen in tropical meteorological radiosonde data since the early 1950s, and there is indirect but persuasive evidence that it has been present in varying degrees since at least the 1880s (e.g. Hamilton 1983; Hamilton and Garcia 1984,6; Hagan et al. 1993; Teitelbaum et al. 1994). I suggest we postpone the interesting question of the possible modulation of solar-terrestrial effects by the terrestrial QBO until after the presentation by Professor Labitzke. I thought, however, that it might be interesting to consider one or two very fundamental points about the fluid dynamics of the terrestrial QBO and its robustnesses and sensitivities, and then to consider briefly the possibility that some aspects of solar variability - some of the many aspects that we have been hearing about - might be related to partially similar mechanisms in the Sun’s interior.
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McIntyre, M.E. (1994). The Quasi-Biennial Oscillation (QBO): Some Points about the Terrestrial QBO and the Possibility of Related Phenomena in the Solar Interior. In: Nesme-Ribes, E. (eds) The Solar Engine and Its Influence on Terrestrial Atmosphere and Climate. NATO ASI Series, vol 25. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-79257-1_18
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