The Prompt ElastoGravity Signals (PEGS) : Detection capabilities and limitations of very broadband seismometers
Martin Vallée  1@  , Kévin Juhel  2, 1  , Jean-Paul Ampuero  3  , Pascal Bernard  4  , Jean-Paul Montagner  5  , Matteo Barsuglia  6  , Team Geoscope@
1 : Institut de physique du globe de Paris
IPG PARIS
2 : AstroParticule et Cosmologie
Université Paris Diderot - Paris 7
3 : Géoazur
Université Côte d’Azur, IRD, CNRS, Observatoire de la Côte d’Azur, Géoazur
4 : Institut de Physique du Globe de Paris  (IPGP)  -  Site web
IPG PARIS
IPGP, 1 rue Jussieu, 75238 Paris cedex 05 -  France
5 : Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Seismology Group, CNRS UMR 7154, Paris, France,
CNRS : UMR7154
6 : AstroParticule et Cosmologie  (APC - UMR 7164)  -  Site web
CEA, Université Paris VII - Paris Diderot, Observatoire de Paris, IN2P3, CNRS : UMR7164
APC - UMR 7164, Université Paris Diderot, 10 rue Alice Domon et Léonie Duquet, case postale 7020, F-75205 Paris Cedex 13 -  France

Prompt ElastoGravity Signals (PEGS) originate from the gravitational perturbations associated with the mass redistribution carried by elastic waves. As such, they are the earliest deformation signals observable after an earthquake. Today, PEGS were clearly observed with (very) broadband seismometers for 6 large magnitude earthquakes (Mw >7.8), and can be accurately modeled by several approaches. After summarizing these main observational results of the last two years, we will then concretely illustrate when detection can or cannot be achieved with seismometers, based on the characteristics of the lowest-noise very-broadband stations (Geoscope, Global Seismic Network, FNET).



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