HR: 0830h
AN: GP11D-0288 [PDF]
TI: Magnetic versus Crystallographic Fabrics in Basaltic Lava Flows
AU: Bascou, J
EM: bascou@dstu.univ-montp2.fr
AF: Laboratoire de Tectonophysique, CNRS and ISTEEM, Universit\'{e}
Montpellier 2, cc049,Pl. E. Bataillon, Montpellier, 34095
France
AU: Camps, P C
EM: camps@dstu.univ-montp2.fr
AF: Laboratoire de Tectonophysique, CNRS and ISTEEM, Universit\'{e}
Montpellier 2, cc049,Pl. E. Bataillon, Montpellier, 34095
France
AU: * Plenier, G
EM: plenier@cerege.fr
AF: CEREGE, Universit\'{e} Aix Marseille III, BP 80, Europ\^{o}le
m\'{e}diterran\'{e}en de l'Arbois, Aix en Provence, 13545
France
AU: Dautria, J
EM: dautria@dstu.univ-montp2.fr
AF: Laboratoire de Tectonophysique, CNRS and ISTEEM, Universit\'{e}
Montpellier 2, cc049,Pl. E. Bataillon, Montpellier, 34095
France
AB:
Indicators of flow direction and sense in lava flows are often
difficult
to observe. To
overcome this difficulty, anisotropy of magnetic susceptibility (AMS)
can be used.
However, a major issue is to know how consistently the axes of magnetic
susceptibility
(K1, K2 and K3) correlate with the flow direction.\\
We carried out a systematically sampling of the base, the middle part
and the top of
lava flow for which the flowing directions are well known. These
quaternary flows,
located in the area of P\'{e}zenas (southern France), are pluri -
kilometric
long, between 2
and 10 m thick, rather narrow ($<$ 500 m) and characterized by a weak
slope ($<$10$^\circ$).
Oriented cores offer an opportunity to investigate the relationships
between flow
direction, principal susceptibilities and crystallographic preferred
orientations (shape
and lattice orientations) of rock-forming minerals.\\
In thin-section, the opaque grains observed in reflected light are
abundant (about 5
percent) and the largest in size (15-20 $\mu$m) are sub-automorphous.
Microsonde analyses
and thermomagnetic curves measured in the range 80 - 900 K indicate
that
titano
magnetite ($x = 0.6$) is the dominant oxide mineral. FORC diagrams
reveal that the
magnetic grain sizes are both PSD-MD and PSD-SD assemblages. AMS
measurements from 180
specimens reveal a tight clustering of the K3 axes close to the
vertical
and a weaker
degree of clustering of K1, K2 axes. A significant enhancing of the
magnetic fabric is
observed after demagnetization by thermal treatment. Lattice Preferred
Orientation (LPO)
measurements of titano magnetite and plagioclase were performed using
the electron
backscattered diffraction (EBSD) technique. The highest fabric strength
is observed from
plagioclase measurements and the LPO of this mineral are correlated to
the flow dynamic.
For the samples collected from near the flow base a good correlation is
observed between
the AMS ellipsoid axes and the LPO of plagioclase: the K1 axis is close
to the maximum
concentration of the [001] axes, the K2 axis is close to the maximum
concentration of
[100] axes and the K3 axis is close to the preferential orientation of
the (010) poles.
The angle between the K3 axes and the vertical plane define a
significant flow related
imbrication of the magnetic foliation that can be used to infer the
flow
direction.
Determination of relationships between the AMS axes and the flow
related
LPO of the
plagioclase may represent a valuable constraints to interpret the ASM
signature in lava
flows.
DE: 1518 Magnetic fabrics and anisotropy
DE: 1519 Magnetic mineralogy and petrology
DE: 1540 Rock and mineral magnetism
SC: Geomagnetism and Paleomagnetism [GP]
MN: 2003 Fall Meeting