Abstract
Anisotropy of magnetic susceptibility (AMS) and anisotropy of magnetic
remanence (AARM and AIRM) are efficient and versatile techniques to
indirectly determine rock fabrics. Yet, deciphering the source of a
magnetic fabric remains a crucial and challenging step, notably in the
presence of ferrimagnetic phases. Here we use X-ray micro-computed
tomography to directly compare mineral shape-preferred orientation and
spatial distribution fabrics to AMS, AARM and AIRM fabrics from five
hypabyssal trachyandesite samples. Magnetite grains in the
trachyandesite are euhedral with a mean aspect ratio of 1.44 (0.24 s.d.,
long/short axis), and > 50% of the magnetite grains occur in
clusters, and they are therefore prone to interact magnetically.
Amphibole grains are prolate with magnetite in breakdown rims. We
identified three components of the petrofabric that influence the AMS of
the analyzed samples: the magnetite and the amphibole shape fabrics and
the magnetite spatial distribution. Depending on their relative
strength, orientation and shape, these three components interfere either
constructively or destructively to produce the AMS fabric. If the three
components are coaxial, the result is a relatively strongly anisotropic
AMS fabric (P’ = 1.079). If shape fabrics and/or magnetite distribution are non-coaxial, the resulting AMS is weakly anisotropic (P’
= 1.012). This study thus reports quantitative petrofabric data that
show the effect of magnetite distribution anisotropy on magnetic fabrics
in igneous rocks, which has so far only been predicted by experimental
and theoretical models. Our results have first-order implications for
the interpretation of petrofabrics using magnetic methods.
Original language | English |
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Article number | e2021JB021895 |
Number of pages | 23 |
Journal | Journal of Geophysical Research: Solid Earth |
Volume | 126 |
Issue number | 6 |
DOIs | |
Publication status | Published - 9 Jun 2021 |
Keywords
- AMS
- MicroXCT
- Distribution Anisotropy
- AARM