1993•Unpublished venueOpen access

Magnetic Fabric Studies of Samples from Hole 808C, Nankai Trough

William H. Owens

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Abstract

Measurements of magnetic susceptibility anisotropy, orientated using stable remanences, are presented for Hole 808C, over the depth range 300 to 1050 meters below seafloor.Within the accretionary prism, magnetic fabric directions are remarkably consistent, the maximum susceptibility axes lying horizontal and at right angles to the direction of underthrusting, with minimum susceptibility axes generally close to vertical.Steeper inclinations of the minimum susceptibility axes are observed in the fold below the frontal thrust and in a disturbed zone just above the décollement.Anisotropy parameters are scattered, possibly reflecting local inhomogeneity of deformation, but the broad pattern is consistent with the model for magnetic fabric modification put forward by Graham (1966).Below the décollement the magnetic fabric is strongly oblate, with no preferred azimuthal orientation.There is evidence of deformation of remanence in the zone immediately below the frontal thrust.

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Measurements of magnetic susceptibility anisotropy, orientated using stable remanences, are presented for Hole 808C, over the depth range 300 to 1050 meters below seafloor.Within the accretionary prism, magnetic fabric directions are remarkably consistent, the maximum susceptibility axes lying horizontal and at right angles to the direction of underthrusting, with minimum susceptibility axes generally close to vertical.Steeper inclinations of the minimum susceptibility axes are observed in the fold below the frontal thrust and in a disturbed zone just above the décollement.Anisotropy parameters are scattered, possibly reflecting local inhomogeneity of deformation, but the broad pattern is consistent with the model for magnetic fabric modification put forward by Graham (1966).Below the décollement the magnetic fabric is strongly oblate, with no preferred azimuthal orientation.There is evidence of deformation of remanence in the zone immediately below the frontal thrust.

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Available abstract

Measurements of magnetic susceptibility anisotropy, orientated using stable remanences, are presented for Hole 808C, over the depth range 300 to 1050 meters below seafloor.Within the accretionary prism, magnetic fabric directions are remarkably consistent, the maximum susceptibility axes lying horizontal and at right angles to the direction of underthrusting, with minimum susceptibility axes generally close to vertical.Steeper inclinations of the minimum susceptibility axes are observed in the fold below the frontal thrust and in a disturbed zone just above the décollement.Anisotropy parameters are scattered, possibly reflecting local inhomogeneity of deformation, but the broad pattern is consistent with the model for magnetic fabric modification put forward by Graham (1966).Below the décollement the magnetic fabric is strongly oblate, with no preferred azimuthal orientation.There is evidence of deformation of remanence in the zone immediately below the frontal thrust.

Key concepts: Geology, Remanence, Décollement, Accretionary wedge, Anisotropy, Magnetic anomaly, Deformation (meteorology), Lineation

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