Neogene remagnetization of normal polarity in the Late Jurassic black shales from the southern Subalpine Chains (French Alps). Evidence for late anticlockwise rotations

Citation
C. Aubourg et C. Chabert-pelline, Neogene remagnetization of normal polarity in the Late Jurassic black shales from the southern Subalpine Chains (French Alps). Evidence for late anticlockwise rotations, TECTONOPHYS, 308(4), 1999, pp. 473-486
Citations number
34
Categorie Soggetti
Earth Sciences
Journal title
TECTONOPHYSICS
ISSN journal
00401951 → ACNP
Volume
308
Issue
4
Year of publication
1999
Pages
473 - 486
Database
ISI
SICI code
0040-1951(19990730)308:4<473:NRONPI>2.0.ZU;2-6
Abstract
This study presents paleomagnetic investigations of 23 sites from the Late Jurassic black shales, the so-called Terres Noires, that outcrop in the sou thern Subalpine Chains (SSC). Six sites are located in the Diois, six sites in the Trieves and Devoluy, and eleven sites in the Digne nappe. The magne tizations are weak and are carried by titanomagnetites. We found generally one component per site within the medium range of temperature (200 degrees to 500 degrees C). All magnetizations are characterized by the lack of reve rse polarity. The directions of magnetization are generally better grouped in geographic coordinates in the Trieves, the Devoluy and the Digne nappe. Fold testing at one site from the Trieves demonstrated a late synfolding ac quisition of magnetization. In contrast, pre-tilting magnetizations are sug gested in the Diois and locally, in the Digne nappe. Given an average incli nation close to late Tertiary expected inclinations in geographic coordinat es, we propose that these magnetizations are Neogene overprints. Our result s point to two major results. (1) The lack of reverse polarity which is puz zling during the Neogene where 50% of the magnetic field is reverse. (2) Th e discovery of quite systematic anticlockwise rotations. These anticlockwis e rotations do not occur in the Diois and are larger in the southern part o f the Digne nappe. We presume that these rotations were active during the l ate stage of Alpine folds emplacement and are still active today. (C) 1999 Elsevier Science B.V. All rights reserved.