Persistence of the planetary wave type oscillations in foF2 over Europe

• Published in: Annales geophysicae (1988) Vol. 21; no. 7; pp. 1543 - 1552
• Main Authors: LASTOVICKA, J, KRIZAN, P, SAULI, P, NOVOTNA, D
• Format: Journal Article
• Language: English
• Published: Katlenburg-Lindau European Geophysical Society 01.07.2003; European Geosciences Union; Copernicus Publications
• Subjects: Earth Sciences; Earth, ocean, space; Exact sciences and technology; External geophysics; General circulation. Atmospheric waves; Marine; Meteorology; Ocean, Atmosphere; Physics of the high neutral atmosphere; Sciences of the Universe; Tides, waves, convection, winds, turbulence; Europe; Mid latitude; Troposphere; Ionosphere (ionosphere-atmosphere interaction, mid-latitude ionosphere, ionospheric disturbances); Persistence; Meteorology and atmospheric dynamics (waves and tides); Atmospheric dynamics; Wavelet transformation; Predictability; Oscillation; Ionospheric disturbance; Planetary wave; Solar cycle; Ionospheric F2 layer; Wave number; Atmospheric wave
• ISSN: 0992-7689; 1432-0576; 1432-0576
• DOI: 10.5194/angeo-21-1543-2003

Planetary waves are oscillations of very predominantly tropospheric origin with typical periods of about 2-30 days. Their dominant zonal wave numbers are 1, 2 and 3, i.e. the waves are of large-scale (global) character. The planetary wave type oscillations have been observed in the lower and middle atmosphere but also in the ionosphere, including the ionospheric F2-layer. Here, we deal only with the oscillations analyzed for four European stations over a solar cycle with the use of the Meyer and Morlet wavelet transforms. Waves with periods near 5, 10 and 16 days are studied. Only events with a duration of three wave-cycles and more are considered. The 5-day period wave events display a typical duration of 4 cycles, while 10- and 16-day wave events are less persistent, with a typical duration of about 3.5 cycles and 3 cycles, respectively. The persistence pattern in terms of number of cycles and in terms of number of days is different. In terms of number of cycles, the typical persistence of oscillations decreases with increasing period. On the other hand, in terms of number of days the typical persistence evidently increases with increasing period. The spectral distribution of event duration is too broad to allow for a reasonable prediction of event duration. Thus, the predictability of the planetary wave type oscillations in foF2 seems to be very questionable.