Precursory worldwide signatures of earthquake occurrences on Swarm satellite data.


Journal

Scientific reports
ISSN: 2045-2322
Titre abrégé: Sci Rep
Pays: England
ID NLM: 101563288

Informations de publication

Date de publication:
30 Dec 2019
Historique:
received: 10 07 2019
accepted: 25 11 2019
entrez: 1 1 2020
pubmed: 1 1 2020
medline: 1 1 2020
Statut: epublish

Résumé

The study of the preparation phase of large earthquakes is essential to understand the physical processes involved, and potentially useful also to develop a future reliable short-term warning system. Here we analyse electron density and magnetic field data measured by Swarm three-satellite constellation for 4.7 years, to look for possible in-situ ionospheric precursors of large earthquakes to study the interactions between the lithosphere and the above atmosphere and ionosphere, in what is called the Lithosphere-Atmosphere-Ionosphere Coupling (LAIC). We define these anomalies statistically in the whole space-time interval of interest and use a Worldwide Statistical Correlation (WSC) analysis through a superposed epoch approach to study the possible relation with the earthquakes. We find some clear concentrations of electron density and magnetic anomalies from more than two months to some days before the earthquake occurrences. Such anomaly clustering is, in general, statistically significant with respect to homogeneous random simulations, supporting a LAIC during the preparation phase of earthquakes. By investigating different earthquake magnitude ranges, not only do we confirm the well-known Rikitake empirical law between ionospheric anomaly precursor time and earthquake magnitude, but we also give more reliability to the seismic source origin for many of the identified anomalies.

Identifiants

pubmed: 31889060
doi: 10.1038/s41598-019-56599-1
pii: 10.1038/s41598-019-56599-1
pmc: PMC6937265
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

20287

Subventions

Organisme : European Space Agency (ESA)
ID : 4000113862/15/NL/MP

Références

Nature. 2007 May 3;447(7140):76-9
pubmed: 17476265
Sensors (Basel). 2017 Jan 26;17(2):
pubmed: 28134755
Entropy (Basel). 2019 Apr 18;21(4):
pubmed: 33267126

Auteurs

A De Santis (A)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy. angelo.desantis@ingv.it.

D Marchetti (D)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.
Now at School of Remote Sensing and Geomatics Engineering NUIST, Nanjing University of Information Science and Technology, Nanjing, China.

F J Pavón-Carrasco (FJ)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.
Now at Univ. Complutense de Madrid, Facultad CC. Físicas, Avd. Complutense, s/n - Madrid 28040, Spain & Geoscience Institute IGEO (CSIC - UCM), Madrid, 28040, Spain.

G Cianchini (G)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

L Perrone (L)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

C Abbattista (C)

Planetek Italia srl, via Massaua 12, Bari, 70132, Italy.

L Alfonsi (L)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

L Amoruso (L)

Planetek Italia srl, via Massaua 12, Bari, 70132, Italy.

S A Campuzano (SA)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

M Carbone (M)

Planetek Italia srl, via Massaua 12, Bari, 70132, Italy.

C Cesaroni (C)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

G De Franceschi (G)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

Anna De Santis (A)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

R Di Giovambattista (R)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

A Ippolito (A)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.
Now at ASI, Via del Politecnico snc, Roma, 00133, Italy.

A Piscini (A)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

D Sabbagh (D)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

M Soldani (M)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.

F Santoro (F)

Planetek Italia srl, via Massaua 12, Bari, 70132, Italy.

L Spogli (L)

Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, Roma, 00143, Italy.
SpacEarth Technology, Via di Vigna Murata 605, Roma, 00143, Italy.

R Haagmans (R)

European Space Agency, ESTEC, Keplerlaan 1, NL-2201 AZ, Noordwijk, The Netherlands.

Classifications MeSH