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A VSH-Chebyshev vector transform with two "fast directions" is also developed and briefly presented.
Fig. 5. Rose diagrams showing the distribution of shear-wave-splitting fast directions determined using the cross-correlation method.
The anisotropy in the region is relatively simple, with a high amplitude and fast directions parallel to the Red River Shear Zone in the western part.
However, at periods of 16 s, the fast directions of the anisotropy are almost parallel to the RRSZ (Figure 11b) in the western part of the model.
At the jump point, the fast directions of the flow take over, which causes the formation of a small spike as the orbit segment leaves S; see also Figure 5c.
Nakajima et al. (2006) examined the fast directions of shear-wave splitting near the plate junction of the southwestern part of the Kurile arc and the northeastern Japan arc.
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In region c, the fast direction of Pn anisotropy is generally the same as the SKS splitting fast direction.
The black trajectories on (S^{a}) move towards F and then jump in the fast direction.
The fast direction of the P n velocity appears to be perpendicular to the lin-eation of magnetic anomalies.
Around 93°E, the fast Pn direction is different from the SKS splitting fast direction, which might be caused by the eastward movement of the lithosphere due to the push from the collision and decoupling with the deep upper mantle.
The first is an extended version of the normal form of a folded node [34, 47], where a fast variable with a stable fast direction is added.
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