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Conversion between quaternions and Euler angles
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Conversion between quaternions and Euler angles : ウィキペディア英語版
Conversion between quaternions and Euler angles
Spatial rotations in three dimensions can be parametrized using both Euler angles and unit quaternions. This article explains how to convert between the two representations. Actually this simple use of "quaternions" was first presented by Euler some seventy years earlier than Hamilton to solve the problem of magic squares. For this reason the dynamics community commonly refers to quaternions in this application as "Euler parameters".
==Definition==
A unit quaternion can be described as:
:\mathbf = \begin q_0 & q_1 & q_2 & q_3 \end^T
:|\mathbf|^2 = q_0^2 + q_1^2 + q_2^2 + q_3^2 = 1
We can associate a quaternion with a rotation around an axis by the following expression
:\mathbf_0 = \cos(\alpha/2)
:\mathbf_1 = \sin(\alpha/2)\cos(\beta_x)
:\mathbf_2 = \sin(\alpha/2)\cos(\beta_y)
:\mathbf_3 = \sin(\alpha/2)\cos(\beta_z)
where α is a simple rotation angle (the value in radians of the angle of rotation) and cos(β''x''), cos(β''y'') and cos(β''z'') are the "direction cosines" locating the axis of rotation (Euler's Theorem).

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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