F. Javier Pavón-Carrasco

Dr. F. Javier Pavón-Carrasco

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Research Focus & Metrics

Academic Career Length

19Years (2008-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 February 2014 in Earth and Planetary Science Letters
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Journal Article
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FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
MOMaría Luisa Osete
María Luisa Osete
JTJ. Miquel Torta
J. Miquel Torta
ASAngelo De Santis
Angelo De Santis

1 February 2011 in Journal of Archaeological Science
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Journal Article
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FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
JRJuan Rodríguez-González
Juan Rodríguez-González
MOMaria Luisa Osete
Maria Luisa Osete
JTJ. Miquel Torta
J. Miquel Torta

1 March 2017 in Earth and Planetary Science Letters
Verified
Journal Article
Closed access
ASA. De Santis
A. De Santis
Georgios BalasisGeorgios Balasis
Georgios Balasis
FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
GCG. Cianchini
G. Cianchini
MMM. Mandea
M. Mandea

20 April 2016 in Frontiers in Earth Science
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Journal Article
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FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
ASAngelo De Santis
Angelo De Santis
The South Atlantic Anomaly is nowadays one of the most important features of the Earth’s magnetic field. Its extent area at the Earth’s surface is continuously growing since the intensity instrumental measurements are available covering part of the Southern Hemisphere and centred in South America. Several studies associate this anomaly as an indicator of an upcoming geomagnetic transition, such an excursion or reversal. In this paper we carry out a detailed study about this issue using the most recent models that also include data from the last ESA mission Swarm. Our results reveal that one of the reversed polarity patch located under the South Atlantic Ocean is growing with a pronounced rate of -2.54•105 nT per century and with western drift. In addition, we demonstrate that the quadrupole field mainly controls this reversal patch at the CMB along with the rapid decay of the dipolar field. The presence of the reversal patches at the CMB seems to be characteristic during the preparation phase of a geomagnetic transition. However, the present value of the dipolar moment (7.7 1022A•m2) is not so low when compared with recent paleomagnetic data for the Holocene (last 12ka) and for the entire Brunhes geomagnetic normal polarity (last 0.8 Ma), although the rate of decay is similar of the previous documented geomagnetic reversals or excursions.

25 March 2009 in Geochemistry, Geophysics, Geosystems
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FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
MOMaria Luisa Osete
Maria Luisa Osete
JTJ. Miquel Torta
J. Miquel Torta
LGLuis R. Gaya‐Piqué
Luis R. Gaya‐Piqué

30 December 2019 in Scientific Reports
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Journal Article
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Dedalo MarchettiDedalo Marchetti
Dedalo Marchetti
FPF. Javier Pavón-Carrasco
F. Javier Pavón-Carrasco
GCG. Cianchini
G. Cianchini
LPL. Perrone
L. Perrone
CAC. Abbattista
C. Abbattista
RHR. Haagmans
R. Haagmans
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.