Stallard, A., Ikei, H. and Masuda, T. 2002. Quicktime movies of 3D spiral inclusion trail development. In: Bobyarchick, A. 2002. Visualisation, Teaching and Learning in Structural Geology. Journal of the Virtual Explorer, 9, 17-30.
Quicktime movies of 3D spiral inclusion trail development

 

Results

Results of the simulations are presented in Figs. 3-6. Figure 3 shows the 3D development of the central inclusion surface during spiral formation, while Fig. 4 shows 2D movies of spiral development in the XZ, XY and YZ planes. The XZ plane is perpendicular to both the shear plane and axis of relative rotation between sphere and matrix, while the XY plane is parallel to the shear plane, and the YZ plane is perpendicular to the shear plane and parallel to the axis of relative rotation between sphere and matrix. Figure 5 compares the final rotation and non-rotation simulation geometries, and Fig. 6 shows 2D movies of serial slices through the spirals parallel to the XZ, XY and YZ planes. Results of both the rotation and non-rotation simulations are presented in these figures.

Figure 3. 3D movies showing the progressive development of spiral inclusion trails according to both the non-rotation (a) and rotation (b) models of spiral formation. For maximum clarity, the movies show the development of the central inclusion surface only. A green marker has been added to the sphere margin to provide a visual trace of sphere rotation during the simulation. Note, this marker has been positioned on the sphere margin in all frames of the movie, and does not represent equivalent marker points within the simulation at different stages of spiral development. In the non-rotation movie, arrows indicate the sense of matrix shear. The long axes of the arrows are parallel to the orientation of the shear plane, and parallel to the orientation of the theoretically developing matrix foliation.

3D spiral development, non-rotation simulation

In the non-rotation simulation, the matrix wraps around the irrotational growing sphere, and it is this shape, in combination with the rotation of the matrix foliation about the sphere, that defines the 3D geometry of the spiral (Figs. 3a, 4d-f). Further from the sphere, the matrix is unaffected by the flow perturbation about the sphere and maintains a sub-planar geometry during the course of the simulation. The maximum perturbation of the matrix occurs in the plane through the centre of the sphere, perpendicular to the axis of relative rotation between the sphere and matrix. The perturbation decreases to zero along the axis of relative rotation as we move away from the centre of the sphere, resulting in a strongly non-cylindrical spiral geometry.

From the centre to the rim of the sphere, the central inclusion plane develops with intervals of relatively gentle curvature separated by intervals of relatively tight curvature. The reason for this is related to the repeated cycles of foliation development in the matrix. At the initiation of each new foliation, the matrix foliation is oriented at approximately 90° to the new shear plane, and is thus quickly rotated toward the shear plane. The rate of rotation slows once the matrix foliation is oriented close to the shear plane. Thus the spiral development is marked by periods of relatively rapid rotation of the foliation about the sphere, coinciding with the development of a new foliation, and periods of relatively slower rotation as the new foliation matures and is reoriented closer to the shear plane.

Figure 4. Movies showing the progressive development of spiral inclusion trails according to both the rotation and non-rotation models of spiral formation. Spiral development is shown in sections oriented parallel to the XZ, XY, and YZ planes. Equivalent colours represent equivalent surfaces in different sections of each simulation. Subplots show the orientation of the 2D sections with respect to the spiral. In all figures, the sphere is represented by a dashed black line.

3D spiral development, rotation simulation

As with the non-rotation simulation, the non-cylindrical spiral geometry reflects the wrapping of the matrix foliation around the growing porphyroblast, although in the rotation simulation, it is the rotation of the sphere, rather than the matrix, that is the driving force behind spiral formation. Once captured within the sphere, the foliation is progressively rotated away from the equivalent foliation in the matrix, thus forming the spiral geometry. The central inclusion surface forms a doubly curving non-cylindrical geometry, whose development can be visualised as a symmetrical pair of sheath folds. Once formed, the sheath fold is progressively rotated and stretched about the axis of relative rotation between the porphyroblast and matrix (Fig. 3b). The central surface develops relatively smoothly compared to the non-rotation simulation. The development of foliation surfaces that were originally oriented off-centre with respect to the sphere can be visualised as the progressive rotation and elongation of a single sheath fold (Fig. 4a). The part of the spiral further from the ‘sheath fold’ tip has a more open geometry due to the wrapping of the matrix foliation about the growing sphere.

 

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