Page 166 - Biomedical Engineering and Design Handbook Volume 1, Fundamentals
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BIOMECHANICS OF HUMAN MOVEMENT  143

                          Euler angles described here are commonly reported in biomechanical studies (e.g., Grood and
                          Suntay, 1983) because the rotations take place about clinically meaningful axes corresponding
                          to joint flexion-extension (Z), abduction-adduction (Y′), and internal-external rotation ( ′′ ). The
                                                                                           X
                           , ′
                          ZY X′′  sequence of rotations is expressed using matrix notation in Eq. (6.32), with the elements
                             ,
                          of the individual matrices shown in Eq. (6.33).
                                                       R = [R z ][R  ' y  ][R x '' ]         (6.32)
                                                          s
                                 ⎡1  0      0  ⎤       ⎡  cosθ  0  sinθ ⎤   ⎡ cosφ − sinφ 0⎤
                                                                                        0
                                 ⎢             ⎥       ⎢            ⎥       ⎢            ⎥
                            R = 0   cosψ  − sinψ ⎥  R =  ⎢  0  1  0  ⎥  R z  = sinφ  cosφ  0 ⎥  (6.33)
                                                                            ⎢
                                 ⎢
                             x''
                                                    y'
                                 ⎢0  sinψ  cosψ  ⎥ ⎦   ⎣ − ⎢  sinθ 0  cosθ ⎦ ⎥  ⎢ ⎣  0  0  1 ⎦ ⎥
                                 ⎣
                          where φ, θ, and ϕ are the Euler angles about the ZY X, ′ , ′′  axes, respectively. Expanding Eq. (6.33)
                          using the matrices from Eq. (6.33) leads to the rotation matrix R in Eq. (6.34).
                                                       ψ
                               ⎡ cos( )cos( ) cos( )sin( )sin( ) − sin( )cos(ψψ) cos( φ)sin( cos( ψ) sin( φ)sin( ψ)⎤
                                                                                    +
                                        θ
                                                  θ
                                                             φ
                                              φ
                                   φ
                                                                             θ)
                               ⎢                                                              ⎥
                                                       ψ
                                                  θ
                                                                                    −
                                                                                 ψ
                                                                                            ψ
                                                                                        φ
                                                                             θ
                                                             φ
                                                         +
                                                                        φ
                                                                  ψ
                                        θ
                                              φ
                                   φ)
                            R = sin( cos( )  sin( )sin( )sin( ) cos( )cos( ) sin( )sinn( )cos( ) cos( )sin( ) ⎥
                                       (
                               ⎢
                               ⎢ ⎣  − sin( )       cos( )sin( )              c cos( )cos( )   ⎥ ⎦
                                                                                θ
                                                                                     ψ
                                                          ψ
                                      θ
                                                      θ
                                                                                             (6.34)
                            It is easy to show that a different sequence of rotations can be used to move the ACS shank  from its
                          initially aligned position to its final orientation relative to the ACS thigh . Because matrix multiplica-
                          tion is not commutative in general, the terms of R in Eq. (6.34) will differ depending on the sequence
                          of rotations selected. Equations (6.35) through (6.37) can be used to determine the Euler angles for
                          this particular sequence of rotations:
                                                               ⎛ r  ⎞
                                                        φ= arctan ⎜  21 ⎟                    (6.35)
                                                               ⎝ r 11  ⎠
                                                            ⎛   −r   ⎞
                                                     θ= arctan ⎜  31  ⎟                      (6.36)
                                                            ⎜   2   2  ⎟
                                                            ⎝ r 11  + r 21  ⎠
                                                               ⎛ r  ⎞
                                                        ψ= arctan ⎜  32 ⎟                    (6.37)
                                                               ⎝ r 33 ⎠
                          where r is the element in the ith row and jth column of matrix R.
                               ij
                            The methods outlined above can also be used to calculate segmental kinematics. For example,
                          rather than calculating the relative orientation between the shank and thigh at time 1, we can use
                          Euler angles to determine the relative orientation between the ACS  at times 1 and 2.
                                                                          shank
              6.4.4 Body Segment Parameters
                          Reexamining Eqs. (6.17) and (6.18), we see that estimates for mass (m) and the inertia tensor (I ) for
                          each segment are required to determine the right-hand side of the equations. Several other terms,
                          including the location of the center of mass and the distances from the distal and proximal joint
                          centers to the COM, are embedded in the left-hand side of Eq. (6.18). The term body segment
                          parameters (BSP) is used to describe this collection of anthropometric information.
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