@InProceedings{KheraniLognPaulRoll:2013:HySiIo,
author = "Kherani, Esfhan Alam and Lognonne, Philippe Henri and Paula,
Eurico Rodrigues de and Rolland, Lucie M.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Institute
de Physique du Globe de Paris} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Observatoire de La Cote d’Azur}",
title = "Hydromagnetic simulation of the ionospheric disturbances generated
by the 2011 Tohoku-oki tsunami and associated acoustic-gravity
waves",
booktitle = "Abstracts...",
year = "2013",
organization = "AGU Meeting of the Americas.",
keywords = "Ionosphere atmosphere interactions.",
abstract = "Owing to the natural disturbances such as Earth quake/tsunami and
tropospheric convection, Acosutic gravity waves (AGWs) are excited
in the troposphere. These AGWs propagates upward to the
thermosphere, attain large amplitude therein and subsequently
dissipate, leading to the excitation of secondary AGWs which
mainly propagate horizontally. Both primary and secondary AGWs
significantly modify the ionosphere, leading to the Total electron
Content disturances, current and magnetic disturbances. Focus of
the present work is the recent Japan tsunami that occurred on 11
March 2011 over Tohoku-Oki and caused enormous damage in terms of
human life and infrastructures. Moreover, it triggered nuclear
catastrophe that makes it a global disaster and much more
alarming. The growing concern is towards failure of short-term
forecasting of this event in spite that the Japan is densely
populated with the various ground based seismic instrument as well
with the GPS receivers that may detect the activities in the space
related to the tsunami. However, owing to these dense networks,
this event is examined much more thoroughly than other big events
in the past, leading to the knowledge of various interesting
aspects that may be helpful in the future for the short-term
forecasting of such event. One such aspect is that the effects of
the seismic activities occurring deep into the ocean, are detected
much more efficiently and in varieties in space (in the overlying
atmosphere and ionosphere) than over the ocean or Earth's surface.
In the present work, hydrodynamic and hydromagnetic simulations of
the atmospheric and ionospheric anomalies are performed for the
Tohoku-Oki tsunami (11 March 2011). The
Tsunami-Atmosphere-Ionosphere (TAI) coupling mechanism via AGWs is
explored theoretically using the TAI coupled model. In this
mechanism, tsunami in the ocean excites the AGWs in the atmosphere
owing to the vertical uplift which subsequently interact with the
ionosphere to gives rise density, electric and magnetic field
disturbances or anomalies. For the modeled tsunami wave as an
input, the coupled model simulates the wind, density and
temperature disturbances or anomalies in the atmosphere and
electron density/magnetic anomalies in the F region of the
ionosphere. Also presented are the GPS-TEC and ground-based
magnetometer measurements during first hour of tsunami and good
agreements are found between modeled and observed anomalies. The
high frequency component \$\sim\$10 minutes of the simulated
wind, TEC and magnetic anomalies in the F region develops within
6-7 minutes after the initiation of the tsunami, suggesting the
importance of monitoring the high-frequency
atmospheric/ionospheric anomalies for the early warning. These
anomalies are found to maximize across the epicenter in the
direction opposite to the tsunami propagation suggesting that the
large atmospheric/ionospheric disturbances are excited in the
region where tsunami does not travel.",
conference-location = "Cancun, Mexico",
conference-year = "14-17 Maio",
label = "self-archiving-INPE-MCTI-GOV-BR",
language = "en",
targetfile = "abstract_congresso.pdf",
urlaccessdate = "17 jan. 2021"
}