Kinematics of General Spatial Mechanical Systems. M. Kemal Ozgoren
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1 (b) Extraction of the 1‐2‐3 Euler Angles
If the RFB 1‐2‐3 sequence is used,
Similarly as done above for the 3‐2‐3 Euler angles, the following five scalar equations can be derived from Eq. (3.140) by picking up the appropriate elements of
From Eq. (3.141), cosφ2 and φ2 can be found as follows with an arbitrary sign variable σ:
(3.146)
(3.147)
In Eq. (3.148), σ2 is different from σ. It is defined as follows if c13 ≠ 0.
(3.149)
If cosφ2 ≠ 0, i.e. if d13 > 0, φ1 and φ3 can be found as follows, respectively, from Eq. Pairs 3.142,3.143,3.144,3.145 and (3.144)–(3.145) consistently with σ, without introducing any additional sign variable.
(3.150)
(3.151)
(3.152)
(3.153)
(3.154)
(3.155)
1 Selection of the Sign Variable
Based on the solution obtained above for d13 > 0, the following analysis can be made concerning the sign variable σ.
If σ = + 1 leads to
(3.156)
Here, σ2 = sgn(φ2) as introduced before. As for