Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/187222
Title: Refining geomagnetic field intensity changes in Europe between 200 CE and 1800 CE. New data from the Mediterranean region
Author: Rivero Montero, M.
Gómez Paccard, M.
Pavón Carrasco, F. J.
Cau Ontiveros, Miguel Ángel
Fantuzzi, Leandro
Martín Hernández, F.
Palencia Ortas, A.
Aidona, E.
Tema, E.
Kondopoulou, D.
Mas Florit, Catalina
Ramon Torres, J.
Keywords: Arqueologia
Arqueometria
Archaeology
Archaeometry
Issue Date: 2021
Publisher: Elsevier B.V.
Abstract: Absolute past geomagnetic intensity values can mainly be recovered by fired archaeological materials and volcanic rocks. Here, we present 10 new archeointensities from the Mediterranean region that help to better constrain geomagnetic field intensity changes in Europe over the last two millennia. The new archeointensity results were obtained from the Thellier classical method including thermoremanent magnetization (pTRM) checks and both the TRM anisotropy and cooling rate corrections and were derived from at least three specimens. The new data presented, together with a selection of previous archeointensities satisfying a set of quality criteria, confirm the presence of several intensity maxima in Europe over the last 2000 years. In particular, the new archeointensities allow to better define the starting point of the double-oscillation feature that occurred in Europe during the second half of the first millennium CE, and reinforce the existence of a relative maximum at the end of the 14th century - beginning of the 15th century in Western Europe. From selected European archeointensities two new paleosecular variation curves are constructed for Western and Eastern Europe using temporal cubic b-splines in a bootstrap approach. The obtained curves suggest that the occurrence of the intensity maxima is characterized by a period of about 300 ± 50 years. In addition, our results suggest that the maxima do not occur simultaneously in Western and Eastern Europe, pointing out an intensity eastward drift with a mean lag-time of about 100 years.
Note: Versió postprint del document publicat a: https://doi.org/10.1016/j.pepi.2021.106749
It is part of: Physics of the Earth and Planetary Interiors, 2021, vol. 317, p. 1-14
URI: http://hdl.handle.net/2445/187222
Related resource: https://doi.org/10.1016/j.pepi.2021.106749
ISSN: 0031-9201
Appears in Collections:Articles publicats en revistes (Història i Arqueologia)
Articles publicats en revistes (Institut d’Arqueologia de la Universitat de Barcelona (IAUB))

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