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The winds pull surface water with them, creating currents. As these currents flow westward, the Coriolis effect—a force that results from the rotation of the Earth—deflects them. The currents then bend to the right, heading north.
The Coriolis effect describes the pattern of deflection experienced by objects that are not firmly attached to the ground as they travel long distances around the Earth. Many large-scale weather patterns are caused by the Coriolis effect.
The rotation of the Earth is crucial to the Coriolis effect. The Earth, in particular, rotates faster at the Equator than at the poles. Because the Earth is wider at the Equator, equatorial regions must travel nearly 1,600 kilometers (1,000 miles) per hour to complete a 24-hour rotation. The Earth rotates at a slow 0.00008 kilometers (0.00005 miles) per hour near the poles.
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