Articles | Volume 42, issue 1
https://doi.org/10.5194/angeo-42-1-2024
https://doi.org/10.5194/angeo-42-1-2024
Regular paper
 | 
02 Feb 2024
Regular paper |  | 02 Feb 2024

High-time-resolution analysis of meridional tides in the upper mesosphere and lower thermosphere at mid-latitudes measured by the Falkland Islands SuperDARN radar

Gareth Chisham, Andrew J. Kavanagh, Neil Cobbett, Paul Breen, and Tim Barnes

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Electrodynamic Reconfiguration of the Polar Ionosphere During the 2021 Antarctic Solar Eclipse
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EGUsphere, https://doi.org/10.5194/egusphere-2026-5257,https://doi.org/10.5194/egusphere-2026-5257, 2026
This preprint is open for discussion and under review for Annales Geophysicae (ANGEO).
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Cited articles

Azeem, I., Walterscheid, R. L., Crowley, G., Bishop, R. L., and Christensen, A. B.: Observations of the migrating semidiurnal and quaddiurnal tides from the RAIDS/NIRS instrument, J. Geophys. Res., 121, 4626–4637, 2016. a, b, c
Bristow, W. A., Yee, J.-H., Zhu, X., and Greenwald, R. A.: Simultaneous observations of the July 1996 2-day wave event using the Super Dual Auroral Radar Network and the High Resolution Doppler Imager, J. Geophys. Res., 104, 12715–12721, 1999. a, b, c
Ceplecha, Z., Borovicka, J., Elford, W. G., Revelle, P. O., Hawkes, R. L., Porubcan, V., and Simek, M.: Meteor phenomena and bodies, Space Sci. Rev., 84, 327–471, 1998. a
Chapman, S., and Lindzen, R.S.: Atmospheric tides: thermal and gravitational, Springer Science and Business Media, ISBN: 978-9401034012, 2011. a, b
Chisham, G.: Calibrating SuperDARN interferometers using meteor backscatter, Radio Sci., 53, 761–774, https://doi.org/10.1029/2017RS006492, 2018. a, b, c
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Short summary
Solar tides in the atmosphere are driven by solar heating on the dayside of the Earth. They result in large-scale periodic motion of the upper atmosphere. This motion can be measured by ground-based radars. This paper shows that making measurements at a higher time resolution than the standard operation provides a better description of higher-frequency tidal variations. This will improve the inputs to empirical atmospheric models and the benefits of data assimilation.
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