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<title>Weak palaeointensity results over a Pliocene volcanic sequence from Lesser Caucasus (Georgia): transitional record or time averaged field?</title>
<creator>Sánchez Moreno, Elisa María</creator>
<creator>Calvo Rathert, Manuel</creator>
<creator>Goguitchaichvili, Avto</creator>
<creator>Tauxe, Lisa .</creator>
<creator>Vashakidze, George T.</creator>
<creator>Lebedev, Vladimir A.</creator>
<subject>Palaeointensity</subject>
<subject>Magnetic field variations through time</subject>
<subject>Palaeomagnetism</subject>
<description>A palaeointensity study has been carried out on a Pliocene sequence of 20 consecutive lava&#xd;
flows where previous directional results seem to reflect anomalous behaviour of the Earth’s&#xd;
magnetic field (EMF), which can be explained by a polarity transition record or non-averaged&#xd;
palaeosecular variation or both. Here, we perform a total of 55 palaeointensity determinations&#xd;
using the original Thellier–Thellier (TT) method and 100 with the IZZI method.We assess the&#xd;
performance of our selection criteria using a set of strict threshold values applied to a set of&#xd;
test data whose TRMs were acquired in known fields. Absolute palaeointensity determinations&#xd;
that passed our selection criteria were obtained on four specimens with the TT method and on&#xd;
41 specimens with the IZZI method. Application of reliability criteria at a site level yielded&#xd;
palaeointensity results in 8 of 20 studied lava flows. We obtained median values of VADM&#xd;
between 28.9 and 45.6 ZAm2 for the reverse polarity lower Apnia section, while the normal&#xd;
polarity upper section displayed a single value of 54.6 ZAm2. The low palaeointensity values&#xd;
before a transitional direction lava flow and the higher value after it, suggest the common&#xd;
behaviour at the start of a polarity reversal and the recovery after it. However, an isolated&#xd;
record of a stable EMF, where the intensity is lower than the current for the same location&#xd;
(83.7 ZAm2), cannot be discarded. Consequently, this interpretation would support a weak&#xd;
time-averaged field.</description>
<date>2021-11-05</date>
<date>2021-11-05</date>
<date>2020-03</date>
<type>info:eu-repo/semantics/article</type>
<identifier>1365-246X</identifier>
<identifier>http://hdl.handle.net/10259/6108</identifier>
<identifier>10.1093/gji/ggz533</identifier>
<language>eng</language>
<relation>Geophysical Journal International. V. 220, n. 3, p. 1604–1618</relation>
<relation>https://doi.org/10.1093/gji/ggz533</relation>
<relation>info:eu-repo/grantAgreement/MINECO//CGL2012-32149/ES/VARIACION DE LA PALEOINTENSIDAD ABSOLUTA DEL CAMPO MAGNETICO TERRESTRE REGISTRADA EN ROCAS VOLCANICAS: MOMENTO DIPOLAR, TRANSICIONES DE POLARIDAD Y SUPERCRONES</relation>
<relation>info:eu-repo/grantAgreement/Junta de Castilla y León//BU066U16//Estudio arqueomagnéticos y de propiedades magnéticas en registros de fuegos antrópicos prehistóricos. Aplicaciones a la arqueología</relation>
<relation>info:eu-repo/grantAgreement/MINECO//BES-2013-064060</relation>
<relation>info:eu-repo/grantAgreement/NSF//EAR1345003</relation>
<rights>info:eu-repo/semantics/openAccess</rights>
<publisher>Oxford University Press</publisher>
</thesis></metadata></record></GetRecord></OAI-PMH>