Articles | Volume 26, issue 4
https://doi.org/10.5194/acp-26-2531-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/acp-26-2531-2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Ground-based observations of periodic temperature fluctuations in the mesopause region with periods longer than 2 d
Christoph Kalicinsky
CORRESPONDING AUTHOR
Institute for Atmospheric and Environmental Research, University of Wuppertal, Wuppertal, Germany
Robert Reisch
Institute for Atmospheric and Environmental Research, University of Wuppertal, Wuppertal, Germany
Institute of Climate and Energy Systems: Stratophere (ICE-4), Research Center Jülich, Jülich, Germany
Peter Knieling
Institute for Atmospheric and Environmental Research, University of Wuppertal, Wuppertal, Germany
Related authors
Dirk Offermann, Christoph Kalicinsky, Ralf Koppmann, and Johannes Wintel
Atmos. Chem. Phys., 23, 3267–3278, https://doi.org/10.5194/acp-23-3267-2023, https://doi.org/10.5194/acp-23-3267-2023, 2023
Short summary
Short summary
Atmospheric oscillations with periods between 5 and more than 200 years are believed to be self-excited (internal) in the atmosphere, i.e. non-anthropogenic. They are found at all altitudes up to 110 km and at four very different geographical locations (75° N, 70° E; 75° N, 280° E; 50° N, 7° E; 50° S, 7° E). Therefore, they hint at a global-oscillation mode. Their amplitudes are on the order of present-day climate trends, and it is therefore difficult to disentangle them.
Christoph Kalicinsky, Sabine Griessbach, and Reinhold Spang
Atmos. Meas. Tech., 14, 1893–1915, https://doi.org/10.5194/amt-14-1893-2021, https://doi.org/10.5194/amt-14-1893-2021, 2021
Short summary
Short summary
For an airborne viewing geometry, radiative transfer simulations of infrared limb emission spectra in the presence of polar stratospheric clouds – nitric acid trihydrate (NAT), supercooled ternary solution, ice, and mixtures – were used to develop a size-sensitive NAT detection algorithm. Characteristic size-dependent spectral features in the 810–820 cm−1 region were exploited to subgroup the NAT into three size regimes: small NAT (≤ 1.0 μm), medium NAT (1.5–4.0 μm), and large NAT (≥ 3.5 μm).
Dirk Offermann, Christoph Kalicinsky, Ralf Koppmann, and Johannes Wintel
Atmos. Chem. Phys., 23, 3267–3278, https://doi.org/10.5194/acp-23-3267-2023, https://doi.org/10.5194/acp-23-3267-2023, 2023
Short summary
Short summary
Atmospheric oscillations with periods between 5 and more than 200 years are believed to be self-excited (internal) in the atmosphere, i.e. non-anthropogenic. They are found at all altitudes up to 110 km and at four very different geographical locations (75° N, 70° E; 75° N, 280° E; 50° N, 7° E; 50° S, 7° E). Therefore, they hint at a global-oscillation mode. Their amplitudes are on the order of present-day climate trends, and it is therefore difficult to disentangle them.
Christoph Kalicinsky, Sabine Griessbach, and Reinhold Spang
Atmos. Meas. Tech., 14, 1893–1915, https://doi.org/10.5194/amt-14-1893-2021, https://doi.org/10.5194/amt-14-1893-2021, 2021
Short summary
Short summary
For an airborne viewing geometry, radiative transfer simulations of infrared limb emission spectra in the presence of polar stratospheric clouds – nitric acid trihydrate (NAT), supercooled ternary solution, ice, and mixtures – were used to develop a size-sensitive NAT detection algorithm. Characteristic size-dependent spectral features in the 810–820 cm−1 region were exploited to subgroup the NAT into three size regimes: small NAT (≤ 1.0 μm), medium NAT (1.5–4.0 μm), and large NAT (≥ 3.5 μm).
Cited articles
Andrews, D., Holton, J., and Leovy, C.: Middle atmosphere dynamics, Academic Press, London, ISBN 0-12-058575-8, 1987. a
Beig, G., Scheer, J., Mlynczak, M. G., and Keckhut, P.: Overview of the temperature response in the mesosphere and lower thermosphere to solar activity, Rev. Geophys., 46, RG3002, https://doi.org/10.1029/2007RG000236, 2008. a
Bittner, M., Offermann, D., Graef, H. H., Donner, M., and Hamilton, K.: An 18-year time series of OH* rotational temperatures and middle atmosphere decadal variations, J. Atmos. Sol. Terr. Phy., 64, 1147–1166, https://doi.org/10.1016/S1364-6826(02)00065-2, 2002. a
Buriti, R. A., Takahashi, H., Lima, L. M., and Medeiros, A. F.: Equatorial planetary waves in the mesosphere observed by airglow periodic oscillations, Adv. Space Res., 35, 2031-2036, https://doi.org/10.1016/j.asr.2005.07.012, 2005. a
Charney, J. G. and Drazin, P. G.: Propagation of planetary-scale disturbances from lower into the upper atmosphere, J. Geophys. Res., 66, 83–109, 1961. a
Cumming, A., Marcy, G. W., and Butler, R. P.: The lick planet search: detectability and mass thresholds, Astrophys. J., 526, 890–915, https://doi.org/10.1086/308020, 1999. a, b
Day, K. A. and Mitchell, N. J.: The 16-day wave in the Arctic and Antarctic mesosphere and lower thermosphere, Atmos. Chem. Phys., 10, 1461–1472, https://doi.org/10.5194/acp-10-1461-2010, 2010b. a, b, c, d
Egito, F., Buriti, R. A., Fragoso Medeiros, A., and Takahashi, H.: Ultrafast Kelvin waves in the MLT airglow and wind, and their interaction with the atmospheric tides, Ann. Geophys., 36, 231–241, https://doi.org/10.5194/angeo-36-231-2018, 2018. a, b
Ern, M., Preusse, P., Kalisch, S., Kaufmann, M., and Riese, M.: Role of gravity waves in the forcing of quasi two-day waves in the mesosphere: An observational study, J. Geophys. Res.-Atmos., 118, 3467–3485, https://doi.org/10.1029/2012JD018208, 2013. a
Espy, P. J., Hibbins, R. E., Riggin, D. M., and Fritts, D. C.: Mesospheric planetary waves over Antarctica during 2002, Geophys. Res. Lett., 32, L21804, https://doi.org/10.1029/2005GL023886, 2005. a, b, c
Forbes, J. M. and Zhang, X.: Quasi-10-day wave in the atmosphere, J. Geophys. Res.-Atmos., 120, 11079–11089, https://doi.org/10.1002/2015JD023327, 2015. a, b
French, W. J. R., Burns, G. B., and Espy, P. J.: Anomalous winter hydroxyl temperatures at 69° S during 2002 in a multiyear context, Geophys. Res. Lett., 32, L12818, https://doi.org/10.1002/2015JD023327, 2005. a, b, c
French, W. J. R., Klekociuk, A. R., and Mulligan, F. J.: Analysis of 24 years of mesopause region OH rotational temperature observations at Davis, Antarctica – Part 2: Evidence of a quasi-quadrennial oscillation (QQO) in the polar mesosphere, Atmos. Chem. Phys., 20, 8691–8708, https://doi.org/10.5194/acp-20-8691-2020, 2020. a, b
Hecht, J. H., Walterscheid, R. L., Gelinas, L. J., Vincent, R. A., Reid, I. M., and Woithe, J. M.: Observations of the phase-locked 2 day wave over the Australian sector using medium-frequency radar and airglow data, J. Geophys. Res., 115, D16115, https://doi.org/10.1029/2009JD013772, 2010. a, b, c
Holton, J. R.: The Generation of Mesospheric Planetary Waves by Zonally Asymmetric Gravity Wave Breaking, J. Atmos. Sci., 41, 3427–3430, https://doi.org/10.1175/1520-0469(1984)041<3427:TGOMPW>2.0.CO;2, 1984. a
Kalicinsky, C. and Koppmann, R.: Multi-decadal oscillations of surface temperatures and the impact on temperature increases, Sci. Rep., 12, 19895, https://doi.org/10.1038/s41598-022-24448-3, 2022. a
Kalicinsky, C., Knieling, P., Koppmann, R., Offermann, D., Steinbrecht, W., and Wintel, J.: Long-term dynamics of OH∗ temperatures over central Europe: trends and solar correlations, Atmos. Chem. Phys., 16, 15033–15047, https://doi.org/10.5194/acp-16-15033-2016, 2016. a, b
Kalicinsky, C., Reisch, R., Knieling, P., and Koppmann, R.: Determination of time-varying periodicities in unequally spaced time series of OH* temperatures using a moving Lomb-Scargle periodogram and a fast calculation of the false alarm probabilities, Atmos. Meas. Tech., 13, 467–477, https://doi.org/10.5194/amt-13-467-2020, 2020. a, b, c, d, e, f, g, h, i, j, k, l, m
Kalicinsky, C., Kirchhoff, S., Knieling, P., and Zlotos, L. O.: Long-term variations in the mesopause region derived from OH*(3,1) rotational temperature observations at Wuppertal, Germany, from 1988–2022, Adv. Space Res., 73, 3398–3407, https://doi.org/10.1016/j.asr.2023.08.045, 2024. a, b, c, d, e, f
Kasahara, A.: Effect of zonal flows on the free oscillations of a barotropic atmosphere, J. Atmos. Sci., 37, 917–929, https://doi.org/10.1175/1520-0469(1980)037<0917:EOZFOT>2.0.CO;2, 1980. a, b, c, d
Kishore, P., Namboothiri, S. P., Igarashi, K., Gurubaran, S., Sridharan, S., Rajaram, R., and Venkat Ratnam, M.: MF radar observations of 6.5-day wave in the equatorial mesosphere and lower thermosphere, J. Atmos. Sol.-Terr. Phy., 66, https://doi.org/10.1016/j.jastp.2004.01.026, 2004. a, b
Laštovička, J.: Observations of tides and planetary waves in the atmosphere-ionosphere system, Adv. Space Res., 20, 1209–1222, https://doi.org/10.1016/S0273-1177(97)00774-6, 1997. a
Lomb, N. R.: Least-squares frequency analysis of unequally spaced data, Astrophys. Space Sci., 39, 447–462, 1976. a
López-González, M. J., Rodríguez, E., García-Comas, M., Costa, V., Shepherd, M. G., Shepherd, G. G., Aushev, V. M., and Sargoytchev, S.: Climatology of planetary wave type oscillations with periods of 2–20 days derived from O2 atmospheric and OH(6-2) airglow observations at mid-latitude with SATI, Ann. Geophys., 27, 3645–3662, https://doi.org/10.5194/angeo-27-3645-2009, 2009. a, b, c, d, e, f
Noll, S., Kausch, W., Kimeswenger, S., Unterguggenberger, S., and Jones, A. M.: OH populations and temperatures from simultaneous spectroscopic observations of 25 bands, Atmos. Chem. Phys., 15, 3647–3669, https://doi.org/10.5194/acp-15-3647-2015, 2015. a
Oberheide, J., Offermann, D., Russell III, J. M., and Mlynczak, M. G.: Intercomparison of kinetic temperature from 15 µm CO2 limb emissions and OH*(3,1) rotational temperature in nearly coincident air masses: SABER, GRIPS, Geophys. Res. Lett., 33, L14811, https://doi.org/10.1029/2006GL026439, 2006. a, b, c
Offermann, D., Hoffmann, P., Knieling, P., Koppmann, R., Oberheide, J., and Steinbrecht, W.: Long-term trend and solar cycle variations of mesospheric temperature and dynamics, J. Geophys. Res., 115, D18127, https://doi.org/10.1029/2009JD013363, 2010. a, b, c
Riggin, D. M., Liu, H.-L., Lieberman, R. S., Roble, R. G., Russell III, J. M., Mertens, C. J., Mlynczak, M. G., Pancheva, D., Franke, S. J., Murayama, Y., Manson, A. H., Meek, C. E., and Vincent, R. A.: Observations of the 5-day wave in the mesosphere and lower thermosphere, J. Atmos. Sol.-Terr. Phy., 68, 323–339, https://doi.org/10.1016/j.jastp.2005.05.010, 2006. a, b
Rong, P., von Savigny, C., Zhang, C., Hoffmann, C. G., and Schwartz, M. J.: Response of middle atmospheric temperature to the 27 d solar cycle: an analysis of 13 years of microwave limb sounder data, Atmos. Chem. Phys., 20, 1737–1755, https://doi.org/10.5194/acp-20-1737-2020, 2020. a
Salby, M.: Survey of planetary-scale travelling waves: the state of theory and observation, Rev. Geophys. Space Phys., 22, 209–236, 1984. a
Salby, M. L.: Rossby Normal Modes in Nonuniform Background Configurations. Part I: Simple fields, J. Atmos. Sci., 38, 1803–1826, 1981a. a
Sassi, F., Garcia, R. R., and Hoppel, K. W.: Large‐scale Rossby normal modes during some recent Northern Hemisphere winters, J. Atmos. Scien., 69, 820–839, https://doi.org/10-1175/JAS-D-11-0103.1, 2012. a, b
Scargle, J. D.: Studies in astronomical time series analysis. II. Statistical aspects of spectral analysis of unevenly spaced data, Astrophys. J., 263, 835–853, 1982. a
Smith, A. K.: The Origin of Stationary Planetary Waves in the Upper Mesosphere, J. Atmos. Sci., 60, 3033 – 3041, https://doi.org/10.1175/1520-0469(2003)060<3033:TOOSPW>2.0.CO;2, 2003. a
Stockwell, R. G., Riggin, D. M., French, W. J. R., Burns, G. B., and Murphy, D. J.: Planetary waves and intraseasonal oscillations at Davis, Antarctica, from undersampled time series, J. Geophys. Res., 112, D21107, https://doi.org/10.1029/2006JD008034, 2007. a, b, c, d
Takahashi, H., Buriti, R. A., Gobbi, D., and Batista, P. P.: Equatorial planetary wave signatures observed in mesospheric airglow emissions, J. Atmos. Sol.-Terr. Phy., 64, 1263–1272, https://doi.org/10.1016/S1364-6826(02)00040-8, 2002. a
Takahashi, H., Lima, L. M., Wrasse, C. M., Abdu, M. A., Batista, I. S., Gobbi, D., Buriti, R. A., and Batista, P. P.: Evidence on 2–4 day oscillations of the equatorial ionosphere h′F and mesospheric airglow emissions, Geophys. Res. Lett., 32, L12102, https://doi.org/10.1029/2004GL022318, 2005. a, b, c
Takahashi, H., Shiokawa, K., Egito, F., Murayama, Y., Kawamura, S., and Wrasse, C. M.: Planetary wave induced wind and airglow oscillations in the middle latitude MLT region, J. Atmos. Sol.-Terr. Phy., 98, 97–104, https://doi.org/10.1016/j.jastp.2013.03.014, 2013. a, b, c, d
Thomas, G. E., Thurairajah, B., Hervig, M. E., and von Savigny, C.: Solar‐induced 27‐day variations of mesospheric temperature and water vapor from the AIM SOFIE experiment: Drivers of polar mesospheric cloud variability, J. Atmos. Sol.‐Terr. Phy., 134, 56–68, https://doi.org/10.1016/j.jastp.2015.09.015, 2015. a
Volland, H.: Atmospheric Tidal and Planetary Waves, Kluwer Academic Publishers, Boston, ISBN-13 918-94-010-7787-3, 1988. a
von Savigny, C., Eichmann, K.-U., Robert, C. E., Burrows, J. P., and Weber, M.: Sensitivity of equatorial mesopause temperatures to the 27-day solar cycle, Geophys. Res. Lett., 39, L21804, https://doi.org/10.1029/2012GL053563, 2012. a
Wu, D. L., Hays, P. B., Skinner, W. R., Marshall, A. R., Burrage, M. D., Lieberman, R. S., and Ortland, D. A.: Observations of the quasi 2-day wave from the High Resolution Doppler Imager on Uars, Geophys. Res. Lett., 20, 2853–2856, https://doi.org/10.1029/93GL03008, 1993. a, b
Wu, D. L., Hays, P. B., and Skinner, W. R.: Observations of the 5-day wave in the mesosphere and lower thermosphere, Geophys Res. Lett., 21, 2733–2736, https://doi.org/10.1029/94GL02660, 1994. a, b
Yamazaki, Y. and Matthias, V.: Large-amplitude quasi-10-day waves in the middle atmosphere during final warmings, J. Geophys. Res.-Atmos., 124, 9874–9892, https://doi.org/10.1029/2019JD030634, 2019. a
Yoshida, S., Tsuda, T., Shimizu, A., and Nakamura, T.: Seasonal variations of 3.0∼3.8-day ultra-fast Kelvin waves observed with a meteor wind radar and radiosonde in Indonesia, Earth Planet Space, 51, 675–684, https://doi.org/10.1186/BF03353225, 1999. a, b
Yue, J., Liu, H.-L., and Chang, L. C.: Numerical investigation of the quasi 2 day wave in the mesosphere and lower thermosphere, J. Geophys. Res., 117, D05111, https://doi.org/10.1029/2011JD016574, 2012. a, b
Zechmeister, M. and Kürster, M.: The generalised Lomb-Scargle periodogram – A new formalism for the floating-mean and Keplerian periodograms, Astron. Astrophys., 496, 577–584, https://doi.org/10.1051/0004-6361:200811296, 2009. a
Zhao, Y., Taylor, M. J., Pautet, P.‐D., Moffat‐Griffin, T., Hervig, M. E., Murphy, D. J., French, W. J. R., Liu, H. L., Pendleton Jr., W. R., and Russell III, J. M.: Investigating an unusually large 28‐day oscillation in mesospheric temperature over Antarctica using ground‐based and satellite measurements. J. Geophys. Res.-Atmos., 124, 8576–8593, https://doi.org/10.1029/2019JD030286, 2019. a, b, c, d, e
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 longer than 20 days and shows maxima around equinoxes for periods below 20 d. The long-term behaviour shows a quasi-20 year oscillation of the wave activity with respect to the magnitude of the wave amplitudes.
Planetary waves are important for driving large scale circulations. We observed planetary waves...
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