AGE-DEPENDENT 3-DIMENSIONAL MAGNETIC MODELING OF THE NORTH-PACIFIC AND NORTH-ATLANTIC OCEANIC-CRUST AT INTERMEDIATE WAVELENGTHS

Citation
Ga. Yanez et Jl. Labrecque, AGE-DEPENDENT 3-DIMENSIONAL MAGNETIC MODELING OF THE NORTH-PACIFIC AND NORTH-ATLANTIC OCEANIC-CRUST AT INTERMEDIATE WAVELENGTHS, J GEO R-SOL, 102(B4), 1997, pp. 7947-7961
Citations number
69
Categorie Soggetti
Geochemitry & Geophysics
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH
ISSN journal
21699313 → ACNP
Volume
102
Issue
B4
Year of publication
1997
Pages
7947 - 7961
Database
ISI
SICI code
2169-9313(1997)102:B4<7947:A3MMOT>2.0.ZU;2-9
Abstract
Three-dimensional magnetic modeling of the North Atlantic and northeas t Pacific is performed at intermediate wavelengths using three models for the acquisition of a natural remanent magnetization. It is shown t hat a remanent magnetization which is dependent on the crustal age is the dominant source for the intermediate-wavelength pattern in both ba sins. However, a pure thermoremanent magnetization of layer 2 alone is insufficient to model the intensity and shape of the observed magneti c anomalies at satellite altitude. We conclude that the best fitting m agnetization model for both basins is a combination of a chemical rema nent magnetization in the altered upper crust and a thermoviscous rema nent magnetization of the slowly cooling lower crust and upper mantle. The North Pacific requires a bulk magnetization which is 50% higher t han that of the North Atlantic in order to fit the Magsat field. Geolo gical processes associated with a faster spreading rate such as a fast er hydrothermal alteration and the growth of a thicker gabbro layer at the expense of a weakly magnetized sheeted dike layer are plausible e xplanations for the higher North Pacific magnetization. The lineated p ositive magnetic anomaly observed over the North Atlantic spreading ce nter is not well reproduced by our models. This anomaly is likely due to a highly magnetized body along or in the vicinity of the spreading center. This highly magnetic body could be an unstable serpentinized l ens of crustal material younger than 20 m.y. which develops within the zone cooled by hydrothermal circulation.