High- and mid-latitude quasi-2-day waves observed simultaneously by four meteor radars during summer 2000
Merzlyakov, E., Pancheva, D., Mitchell, N., Forbes, J. M., Portnyagin, Y. I., Palo, S., Makarov, N. and Muller, H. G., 2004. High- and mid-latitude quasi-2-day waves observed simultaneously by four meteor radars during summer 2000. Annales Geophysicae, 22 (3), pp. 773-788.
Related documents:This repository does not currently have the full-text of this item.
You may be able to access a copy if URLs are provided below.
Results from the analysis of MLT wind measurements at Dixon (73.5degreesN, 80degreesE), Esrange (68degreesN, 21degreesE), Castle Eaton (UK) (53degreesN, 2degreesW), and Obninsk (55degreesN, 37degreesE) during summer 2000 are presented in this paper. Using S-transform or wavelet analysis, quasi-two-day waves (QTDWs) are shown to appear simultaneously at high- and mid-latitudes and reveal themselves as several bursts of wave activity. At first this activity is preceded by a 51-53 h wave with S=3 observed mainly at mid-latitudes. After a short recess (or quiet time interval for about 10 days near day 205), we observe a regular sequence of three bursts, the strongest of them corresponding to a QTDW with a period of 47-48 h and S=4 at mid-altitudes. We hypothesize that these three bursts may be the result of constructive and destructive interference between several spectral components: a 47-48 h component with S=4; a 60-h component with S=3; and a 80-h component with S=2. The magnitudes of the lower (higher) zonal wave-number components increase (decrease) with increasing latitude. The S-transform or wavelet analysis indicates when these spectral components create the wave activity bursts and gives a range of zonal wave numbers for observed bursts from about 4 to about 2 for mid- and high-latitudes. The main spectral component at Dixon and Esrange latitudes is the 60-h oscillation with S=3. The zonal wave numbers and frequencies of the observed spectral components hint at the possible occurrence of the nonlinear interaction between the primary QTDWs and other planetary waves. Using a simple 3-D nonlinear numerical model, we attempt to simulate some of the observed features and to explain them as a consequence of the nonlinear interaction between the primary 47-48 h and the 9-10 day waves, and the resulting linear superposition of primary and secondary waves. In addition to the QTDW bursts, we also infer forcing of the 4-day wave with S=2 and the 6-7 day wave with S=1, possibly arising from nonlinear decoupling of the 60-h wave with S=3. The starting mechanism for this decoupling is the Rossby wave instability (e.g. Baines, 1976). This result is consistent with the day-to-day wind variability during the observed QTDW events. An interesting feature of the final stage of the observed QTDW activity in summer 2000 is the occurrence of strong 4-5 day waves with S=3.
|Creators||Merzlyakov, E., Pancheva, D., Mitchell, N., Forbes, J. M., Portnyagin, Y. I., Palo, S., Makarov, N. and Muller, H. G.|
|Departments||Faculty of Engineering & Design > Electronic & Electrical Engineering|
|Additional Information||ID number: ISI:000220762200007|
Actions (login required)