| 41. | The first extra term is the Coriolis force, the second the centrifugal force, and the third the Euler force.
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| 42. | The concept was originally introduced by a French physicist Jacques Babinet in 1859 using mathematical deduction and Coriolis force.
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| 43. | Where matter moves relative to the co-rotating frame it will seem to be acted upon by a Coriolis force.
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| 44. | The force of spin, called the Coriolis Force, is a maximum at the poles and zero at the Equator.
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| 45. | The centripetal centrifugal force may be dispensed with, but we still have to take the Coriolis force into account.
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| 46. | It can be seen that for any object, the coriolis force over it is proportional to its momentum vector.
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| 47. | In application to the HRG shell, Coriolis forces cause a precession of vibration patterns around the axis of rotation.
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| 48. | In this case the Coriolis force is twice the magnitude of the centrifugal force, and it points in centripetal direction.
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| 49. | The deviations are caused by the Coriolis force and conservation of potential vorticity which leads to changes of relative vorticity.
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| 50. | The force of spin, called the Coriolis force, is at a maximum at the poles and is zero at the equator.
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