Observations of a quasi-90-day oscillation in the MLT winds and tides over an equatorial station using meteor radar winds |
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Authors: | A Guharay PP Batista RA Buriti |
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Institution: | 1. Space and Atmospheric Sciences Division, Physical Research Laboratory, Ahmedabad, GJ, India;2. Heliophysics, Planetary Sciences and Aeronomy Division, National Institute for Space Research, INPE, São José dos Campos, SP, Brazil;3. Department of Physics, Federal University of Campina Grande, Campina Grande, PB, Brazil |
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Abstract: | An evident signature of a least studied quasi-90-day oscillation is found in the winds and tides in the MLT from an equatorial station, São João do Cariri (7.4°S, 36.5°W). The oscillation is found to appear mainly in certain intervals with small but appreciable seasonal (fourth harmonic of annual oscillation) contribution. The maximum amplitude of the oscillation is found to be around 10 m/s in the zonal wind. The enhancement peak of the oscillation exhibits downward movement indicating a plausible role of upward moving waves/tides in carrying its imprint from below to the MLT. Similar oscillation feature in the tropospheric zonal wind and ozone may imply its lower atmospheric origin as a component of the intraseasonal oscillation (ISO) that moves upward by modulating the tides. Subsequently, the propagating tides (mainly semidiurnal) are enhanced by the ozone in the stratosphere through absorption of solar UV radiation and finally manifest the oscillation in the MLT. Consistency of the present findings with the past investigations are observed in some aspects of the oscillation, whereas existing mismatches in others are believed to be due to geophysical variability depending on space and time among various locations on the globe. |
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Keywords: | Quasi-90-day oscillation MLT dynamics Meteor radar winds |
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