Weak palaeointensity results over a Pliocene volcanic sequence from Lesser Caucasus (Georgia): transitional record or time averaged field?

Author:

Sánchez-Moreno Elisa M1ORCID,Calvo-Rathert Manuel12,Goguitchaichvili Avto3,Tauxe Lisa4,Vashakidze George T5,Lebedev Vladimir A6

Affiliation:

1. Departamento de Física, EPS Campus Rio Vena – Universidad de Burgos, Av. Cantabria, s/n, 09006 Burgos, Spain

2. Hawaii Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, University of Hawaii at Manoa, Honolulu, HI 96822, USA

3. Laboratorio Interinstitucional de Magnetismo Natural, Instituto de Geofísica Unidad Michoacán, UNAM – Campus Morelia, 58990 Morelia, México

4. Scripps Institution of Oceanography, University of California - San Diego, La Jolla, CA 92093-0220, USA

5. Alexandre Janelidze Institute of Geology – Ivane Javakhishvili Tbilisi State University, 1/9 M. Alexidze str., 0171 Tbilisi, Georgia

6. Institute of Geology of Ore Deposits, Petrography, Mineralogy and Geochemistry – Russian Academy of Sciences (IGEM RAS), Staromonetny per., 35, 119017 Moscow, Russia

Abstract

SUMMARY A palaeointensity study has been carried out on a Pliocene sequence of 20 consecutive lava flows where previous directional results seem to reflect anomalous behaviour of the Earth's magnetic field (EMF), which can be explained by a polarity transition record or non-averaged palaeosecular variation or both. Here, we perform a total of 55 palaeointensity determinations using the original Thellier–Thellier (TT) method and 100 with the IZZI method. We assess the performance of our selection criteria using a set of strict threshold values applied to a set of test data whose TRMs were acquired in known fields. Absolute palaeointensity determinations that passed our selection criteria were obtained on four specimens with the TT method and on 41 specimens with the IZZI method. Application of reliability criteria at a site level yielded palaeointensity results in 8 of 20 studied lava flows. We obtained median values of VADM between 28.9 and 45.6 ZAm2 for the reverse polarity lower Apnia section, while the normal polarity upper section displayed a single value of 54.6 ZAm2. The low palaeointensity values before a transitional direction lava flow and the higher value after it, suggest the common behaviour at the start of a polarity reversal and the recovery after it. However, an isolated record of a stable EMF, where the intensity is lower than the current for the same location (83.7 ZAm2), cannot be discarded. Consequently, this interpretation would support a weak time-averaged field.

Funder

Ministerio de Economía y Competitividad

Junta de Castilla y León, Spain

National Science Foundation

DGAPA-PAPIIT

Publisher

Oxford University Press (OUP)

Subject

Geochemistry and Petrology,Geophysics

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