Lunar tidal winds in the upper atmosphere over Collm |
| |
Authors: | R. J. Stening C. Jacobi |
| |
Affiliation: | (1) School of Physics, University of New South Wales, UNSW SYDNEY NSW 2052, Australia;(2) Institute for Meteorology, University of Leipzig, Stephanstr. 3, 04103 Leipzig, Germany |
| |
Abstract: | 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. |
| |
Keywords: | Meteorology and atmospheric dynamics (middle atmosphere dynamics waves and tides) |
本文献已被 SpringerLink 等数据库收录! |
|