Annales Geophysicae

, Volume 18, Issue 12, pp 1645–1650 | Cite as

Lunar tidal winds in the upper atmosphere over Collm

  • R. J. SteningEmail author
  • C. Jacobi
Original articles


The lunar semidiurnal tide in winds measured at around 90 km altitude has been isolated with amplitudes observed up to 4 m s−1. There is a marked amplitude maximum in October and also a considerable phase variation with season. The average variation of phase with height indicated a vertical wavelength of more than 80 km but this, and other results, needs to be viewed in the light of the considerable averaging required to obtain statistical significance. Large year-to-year variations in both amplitude and phase were also found. Some phase comparisons with the GSWM model gave reasonable agreement but the model amplitudes above a height of 100 km were much larger than those measured. An attempt to make a comparison with the lunar geomagnetic tide did not yield a statistically significant result.

Key words

Meteorology and atmospheric dynamics (middle atmosphere dynamics; waves and tides) 


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Copyright information

© EGS – Springer-Verlag 2001

Authors and Affiliations

  1. 1.School of PhysicsUniversity of New South WalesAustralia

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