HR: 1400h
AN: SA33B-05    [Abstracts]
TI: Searching for Dominant Oscillation Modes and Phase Synchronization in Ionospheric, Solar and Geomagnetic Time Series
AU: * Šauli, P
EM: pkn@ufa.cas.cz
AF: Institute of Atmospheric Physics ASCR, Boční II/1401, Prague 4, 14131, Czech Republic
AU: Novotná, D
EM: nov@ufa.cas.cz
AF: Institute of Atmospheric Physics ASCR, Boční II/1401, Prague 4, 14131, Czech Republic
AU: Paluš, M
EM: mp@cs.cas.cz
AF: Institute of Computer Science ASCR, Pod vodárenskou&vcaron;ězí 2 , Prague 8, 182 07, Czech Republic
AU: Mošna, Z
EM: zbn@ufa.cas.cz
AF: Institute of Atmospheric Physics ASCR, Boční II/1401, Prague 4, 14131, Czech Republic
AB: Enhanced Monte Carlo Singular Space and Wavelet based methods are used to detect possible oscillatory modes in long-term time series describing state of ionosphere, neutral atmosphere, solar activity and geomagnetic activity. These modes are extracted from raw data, their instantaneous phases are computed and their relations are studied using the tools of synchronization and coherence.
DE: 2427 Ionosphere/atmosphere interactions (0335)
DE: 2437 Ionospheric dynamics
DE: 2443 Midlatitude ionosphere
SC: SPA-Aeronomy [SA]
MN: 2007 Joint Assembly