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  • 1
    Publication Date: 2017-04-04
    Description: Dati di paleovariazioni secolari (PSV) del campo geomagnetico sono stati ottenuti negli ultimi 25.000 anni da diverse carote recuperate nel Golfo di Salerno (Mar Tirreno orientale). Le curve composte di PSV, sono comparate con le “ PSV Master Curves” britanniche e francesi. La comparazione fornisce uno strumento cronologico per determinare un trend di accrescimento del tasso di sedimentazione nell’ Olocene superiore e di variazione ad intervalli di circa 1000 anni nell’ Olocene medio della piattaforma. Inoltre durante i due principali episodi caldi del Mediterraneo a circa 3.3 e tra 6-9 ka sia la piattaforma che la scarpata superiore registrano un aumento con successiva diminuzione del tasso di sedimentazione, mentre ulteriori diminuzioni si registrano, in scarpata superiore, durante l’ ultimo picco Glaciale (LGM) e l’interstadio Bølling-Allerød, suggerendo cosi un’ influenza climatica sui processi di accumulo dei sedimenti del margine del Golfo di Salerno.
    Description: Published
    Description: 173-176
    Description: 3.8. Geofisica per l'ambiente
    Description: open
    Keywords: Paleomagnetic secular variation ; Tyrrhenian Sea ; sedimentation ; climatic changes ; 04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetism
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: book chapter
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  • 2
    Publication Date: 2017-04-04
    Description: 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.
    Description: Published
    Description: 798-812
    Description: 1A. Geomagnetismo e Paleomagnetismo
    Description: JCR Journal
    Description: restricted
    Keywords: Palaeomagnetic secular variation; Rapid time variations; Reversals: process, time scale, magnetostratigraphy; Rock and mineral magnetism ; 04. Solid Earth::04.05. Geomagnetism::04.05.06. Paleomagnetism
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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