| 11. | Then the Euler momentum equation in the steady incompressible case becomes:
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| 12. | This is similar to the extrinsic rotation equivalence for Euler angles.
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| 13. | A demonstration model illustrating the different " Euler " buckling modes.
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| 14. | This leads to the general vector form of Euler's equations
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| 15. | Nevertheless, Euler's problem has a second constant of motion
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| 16. | The equation reduced in this form is called the Euler equation.
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| 17. | Otherwise, the order is 2 divided by the Euler characteristic.
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| 18. | It performs well when solving the Euler equations, see below.
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| 19. | You can also use Euler's formula and its corollaries.
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| 20. | Early results are due to Euler, Gauss, and Cauchy.
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