In this study, the three-dimensional time-dependent Ginzburg-Landau equations were numerically solved to visualize the motion of the flux lines in a superconductor under a transverse magnetic field. Pins were inserted into a superconducting rectangular parallelepiped, and the magnetic field dependence of the normalized critical current density Jc was calculated. Anisotropy y<sub>Z</sub> of different magnitudes was introduced along the direction of the magnetic field (z-axis). Different pin shapes and orientations were also considered: columnar pins aligned parallel to the direction of either the magnetic field or the current flow, spherical pins, and a planar pin in the field-current plane. For the columnar pins aligned parallel to the field (along the flux lines), J c showed almost no dependence on y<sub>Z</sub>. Additionally, a peak in the Jc -B c urve for this pin geometry was observed at normalized magnetic field, B= 0.4 for all considered y<sub>z</sub>. In contrast, J c was dependent on y<sub>Z</sub> for the columnar pins aligned parallel to the current flow (perpendicular to the flux lines) and the spherical pins. At low magnetic fields (B= 0.1), J c increased with increasing y<sub>Z</sub> in both these cases. In the case of the planar pin, J c showed no dependence on y<sub>Z</sub>. In conclusion, when a pin was inserted parallel to the normalized magnetic field B, Jc did not decrease even when the z-axis anisotropy y<sub>Z</sub> was large.
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