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https://doi.org/10.5194/egusphere-2025-3102
https://doi.org/10.5194/egusphere-2025-3102
07 Jul 2025
 | 07 Jul 2025
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Ground-based observations of periodic temperature fluctuations in the mesopause region with periods larger than 2 days

Christoph Kalicinsky, Robert Reisch, and Peter Knieling

Abstract. We analysed more than 30 years (1988–2021) of OH(3,1) rotational temperatures observed from Wuppertal, Germany, with respect to periodic fluctuations (2 to 60 d) using the Lomb-Scargle periodogram. The main type of fluctuation observed in the last decades shows a period of about 28 d and is most likely a Rossby wave (1,4) mode. Other periods which are frequently found in the observations lie in the period ranges 5 to 6 d, 8 to 12 d, and around 15 d and can likely be assigned to the quasi-5-day, the quasi-10-day , and the quasi-16-day wave, respectively. According to theory, these observations are the Rossby wave (1,1) mode, the (1,2) mode, and the (1,3) mode, respectively.

The wave activity is typically larger in winter time than in summer time because of the different wave filtering in summer and winter. This winter to summer difference holds for waves with larger periods, but it breaks off in the case of smaller periods below about 20 d. The occurrence frequency of these waves exhibit two smaller maxima around the equinoxes.

The long-term behaviour of the wave activity shows a quasi-bidecadal oscillation. A further analysis suggests that the yearly mean amplitude of the significant events shows this oscillation not the number of days with significant events in one year. This means, that in certain years not more events but events with larger amplitudes are expected, whereas in other years the mean amplitude of the events is smaller.

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Christoph Kalicinsky, Robert Reisch, and Peter Knieling

Status: open (until 10 Sep 2025)

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Christoph Kalicinsky, Robert Reisch, and Peter Knieling
Christoph Kalicinsky, Robert Reisch, and Peter Knieling

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Short summary
Planetary waves are important for driving large scale circulations. We observed planetary waves in a ground-based data set spanning more than 30 years. The waves can be assigned to expected waves due to their periods. The wave activity is strongest in winter for waves with periods greater than 20 days and shows maxima around equinoxes for periods below 20 days. The long-term behaviour shows a quasi-20 year oscillation of the wave activity with respect to the magnitude of the wave amplitudes.
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