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  5. How fast was the Matuyama-Brunhes geomagnetic reversal? A new subcentennial record from the Sulmona Basin, central Italy
 
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How fast was the Matuyama-Brunhes geomagnetic reversal? A new subcentennial record from the Sulmona Basin, central Italy

Author(s)
Sagnotti, L.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia  
Giaccio, B.  
IGAG, CNR  
Liddicoat, J. C.  
Barnard College, Columbia University, USA  
Nomade, S.  
IPSL, CEA/CNRS/UVSQ et Universit´e Paris–Saclay, France  
Renne, P. R.  
Berkeley Geochronology Center, Berkeley, USA  
Scardia, G.  
Universidade Estadual Paulista, Brazil  
Sprain, C. J.  
Language
English
Obiettivo Specifico
1A. Geomagnetismo e Paleomagnetismo
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Geophysical Journal International  
Issue/vol(year)
/204(2016)
ISSN
0956-540X
Electronic ISSN
1365-246X
Publisher
Wiley-Blackwell
Pages (printed)
798-812
Date Issued
February 2, 2016
DOI
10.1093/gji/ggv486
Alternative Location
http://gji.oxfordjournals.org/content/204/2/798.full.pdf+html
URI
https://www.earth-prints.org/handle/2122/10193
Subjects
04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetism  
Subjects

Palaeomagnetic secula...

Abstract
A recent study of the Matuyama–Brunhes (M-B) geomagnetic field reversal recorded in
exposed lacustrine sediments from the Sulmona Basin (Italy) provided a continuous, highresolution
record indicating that the reversal of the field direction at the terminus of the M-B
boundary (MBB) occurred in less than a century, about 786 ka ago. In the sediment, thin
(4–6 cm) remagnetized horizons were recognized above two distinct tephra layers—SUL2-
19 and SUL2-20—that occur ∼25 and ∼35 cm below the MBB, respectively. Also, a faint,
millimetre-thick tephra (SUL2-18) occurs 2–3 cm above the MBB.With the aim of improving
the temporal resolution of the previous Sulmona MBB record and understanding the possible
influence of cryptotephra on the M-B record in the Sulmona Basin,we performed more detailed
sampling and analyses of overlapping standard and smaller samples from a 50 cm-long block
that spans the MBB. The new data indicate that (i) the MBB is even sharper than previously
reported and occurs ∼2.5 cm below tephra SUL2-18, in agreement with the previous study;
(ii) the MBB coincides with the rise of an intensity peak of the natural remanent magnetization
(NRM) intensity, which extends across SUL2-18; (iii) except for a 2-cm-thick interval just
above tephra SUL2-18, the rock magnetic parameters (k, ARM, Mr, Ms, Bc, Bcr) indicate
exactly the same magnetic mineralogy throughout the sampled sequence. We conclude that
either SUL2-18 resulted in the remagnetization of an interval of about 6 cm (i.e. during the
NRM intensity peak spanning ∼260 ± 110 yr, according to the estimated local sedimentation
rate), and thus the detailed MBB record is lost because it is overprinted, or the MBB is well
recorded, occurred abruptly about 2.5 cm below SUL2-18 and lasted less than 13 ± 6 yr. Both
hypotheses challenge our understanding of the geomagnetic field behaviour during a polarity
transition and/or of the NRM acquisition process in the Sulmona lacustrine sediment.
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