Computer Science – Sound
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsa33a0266k&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SA33A-0266
Computer Science
Sound
0560 Numerical Solutions (4255), 2427 Ionosphere/Atmosphere Interactions (0335), 2447 Modeling And Forecasting, 2471 Plasma Waves And Instabilities (2772), 4564 Tsunamis And Storm Surges
Scientific paper
Internal-gravity waves (IGWs) produced during the tsunami's propagation are known to produce identifiable signature in the overlying ionosphere. Notwithstanding several observations and one case of successful modellings, an heterogenic directivity in the ionospheric IGW propagation has been put in evidence recently using total electron content (TEC) measured by GPS receivers. To explicit the link between the anomalous propagation observed by ionospheric sounding, and the IGW propagation in the neutral atmosphere, we explore the role of magnetic field in the neutral-plasma coupling. A 3D numerical solution of closed set of non-linear hydro-magnetic equations in physical and chemical realistic hypothesis, is used, here, to reproduce the complete response of ionosphere to neutral motion. Vertical and horizontal scale of the modelled perturbed ionosphere corroborates the total electron content (TEC) observations and confirms the effective role of magnetic field in the ionospheric signature of tsunamis.
Kherani Alam E.
Lognonné Philippe
Occhipinti Giovani
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