Abstract
Abstract. In the last decades, mesospheric tides have been intensively investigated
with observations from both ground-based radars and satellites. Single-site
radar observations provide continuous measurements at fixed locations without
horizontal information, whereas single-spacecraft missions typically provide
global coverage with limited temporal coverage at a given location. In this
work, by combining 8 years (2009–2016) of mesospheric winds collected by
five specular meteor radars from three different longitudinal sectors at
boreal midlatitudes (49±8.5∘ N), we develop an approach to
investigate the most intense global-scale oscillation, namely at the period
T=12±0.5 h. Six waves are resolved: the semidiurnal westward-traveling
tidal modes with zonal wave numbers 1, 2, and 3 (SW1, SW2, SW3), the lunar
semidiurnal tide M2, and the upper and lower sidebands (USB and LSB) of the
16 d wave nonlinear modulation on SW2. The temporal variations of the waves
are studied statistically with a special focus on their responses to sudden
stratospheric warming events (SSWs) and on their climatological seasonal
variations. In response to SSWs, USB, LSB, and M2 enhance, while SW2
decreases. However, SW1 and SW3 do not respond noticeably to SSWs, contrary
to the broadly reported enhancements in the literature. The USB, LSB, and SW2
responses could be explained in terms of energy exchange through the
nonlinear modulation, while LSB and USB might previously have been
misinterpreted as SW1 and SW3, respectively. Besides, we find that LSB and M2
enhancements depend on the SSW classification with respect to the associated
split or displacement of the polar vortex. In the case of seasonal
variations, our results are qualitatively consistent with previous studies
and show a moderate correlation with an empirical tidal model derived from
satellite observations.
Funder
Leibniz-Gemeinschaft
Deutsche Forschungsgemeinschaft
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