Replication Data for: High-order solar migrating tides quench at SSW onsets

Solar tides are the most predictably-occurring waves in the upper atmosphere. Although the dynamical theory can be dated back to Laplace in the 16th century, upper atmospheric tides were rarely studied observationally until satellites and ground-based radars became common. To date, observational studies have mainly dealt with low-order solar-day harmonics. Here, we combine mesospheric wind observations from three longitudinal sectors to investigate high-order harmonics. Results illustrate that the first six harmonics appear in early 201