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Lithosphere-Atmosphere-Ionosphere Coupling (LAIC)
The
LAIC phenomenon consists of the coupling of three geo-levels of the
Earth, the lithosphere, the atmosphere and the ionosphere, so that
phenomena occurring in the lithosphere can propagate into the
atmosphere and affect higher layers reaching the ionosphere. From a
seismological point of view, understanding the underlying physical
processes that take place during the seismic preparation phase of
high-energy events can be challenging, especially at the fault level.
An alternative approach is to study whether during this preparation
phase the lithosphere interacts with the atmosphere and ionosphere
assuming a LAIC-type coupling.
Three main coupling mechanisms have been proposed. The first is related
to the presence of p-holes (positive vacancies) that are generated
during the preparation phase of an earthquake by stresses along the
fault. These charged particles could alter the electrical circuit in
the atmosphere, ionising it and creating instabilities in the
mesosphere, eventually reaching the ionosphere (Freund, 2011).
Another hypothesis is related to the migration of fluids along the
fault and the release of radon gas that seems to be detected during the
preparation phase of the most energetic seismic events. This release
would affect the atmosphere, which would eventually propagate and
generate disturbances in the ionosphere (Pulinets & Ouzounov, 2011).
Finally, the third mechanism is based on the generation of acoustic
gravity waves that would be generated before or a few minutes after an
earthquake and would propagate to higher levels, affecting the
ionosphere (Yeh & Liu, 1974).
All these observed disturbances at the three geo-levels
have normally been observed through the detection of anomalies measured
by ground stations. However, in recent years, with the launch of
satellite missions such as DEMETER, Swarm
or CSES, electromagnetic anomalies associated with seismic activity
have been detected from space. This is a major step forward in the
understanding of the preparation phase of the most energetic seismic
events and highlights the need to use multi-parametric analyses to
study this type of complex phenomena by combining not only
seismological but also atmospheric and ionospheric information.
Adapted from De Santis et al. (2015)
Within the Paleomagnetism group, some of its members have participated
in several European projects focused on this study, as well as in the
development of several works in collaboration with the Istituto
Nazionale di Geofisica e Vulganologia (INGV). Some examples are:
D. Marchetti, A. De Santis, J., Shuanggen, S.A. Campuzano, G.
Cianchini, A. Piscini (2020), Co-Seismic Magnetic Field Perturbations
Detected by Swarm Three-Satellite Constelallation. Remote Sens.
Environ. 12(7), 1166. DOI:10.3390/rs12071166.
D. Marchetti, A. De Santis, X. Shen, S.A. Campuzano, L. Perrone, A.
Piscinini, R. Di Giovambattista, S. Jin, A. Ippolito, G. Cianchini, C.
Cesaroni, D. Sabbagh, L. Spogli, Z. Zhima, J. Huang (2020) Possible
Litosphere-Atmosphere-Ionosphere Coupling effects prior to the 2018 Mw
= 7.5 Indonesia earthquake from seismic, atmospheric and ionospheric
data. Journal of Asian Earth Sciences, 188, 104097. DOI:
10.1016/j.jseaes.2019.104097.
A. De Santis, G. Balasis, F.J. Pavón-Carrasco,
G. Cianchini, M. Mandea (2017). Potential earthquake precursory pattern
from space: the 2015 Nepal event as seen by magnetic Swarm satellites.
Earth and Planetary Science Letters, 421, 119 - 126. DOI: 10.1016/j.epsl.2016.12.037.
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