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0593_C11_fm  Page 361  Monday, May 6, 2002  2:59 PM





                       Generalized Dynamics: Kinematics and Kinetics                               361


                        Let B be a part of a mechanical system S which has n degrees of freedom represented
                       by  n generalized coordinates  q  (r = 1,…,  n). Specifically, let the movement of  B in an
                                                   r
                       inertial reference frame R be determined by the coordinates q  and time t. Then, if c is
                                                                               r
                       fixed in B, the derivative of c in R is:

                                                      R         n
                                                       dc  =  c ∂  + ∑  c ∂  q ˙
                                                       dt   t ∂     q ∂  r                     (11.4.10)
                                                                r=1  r
                       By following the exact same procedure as in Section 4.5 in the development of Eq. (11.4.8)
                       we can readily show that the partial derivatives ∂c/∂t and ∂c/∂q  may be expressed as:
                                                                                 r
                                               ∂∂ = ωω  × c and  ∂∂q  = ωω  × c                (11.4.11)
                                                   t
                                                c
                                                                 c
                                                       t             r   q r ˙
                       where ωω ωω  and  ωω  ˙ q r  are defined as:
                              t
                                                 ∂n        ∂n        ∂n   
                                           ωω =   t ∂  2  ⋅n 3  n 1  +    t ∂  3  ⋅nn  2  +    t ∂  1  ⋅n 2  n  3  (11.4.12)
                                                                  
                                                      
                                                                               
                                                                  
                                            t
                                                                  1
                                                 ∂n        ∂n         ∂n  
                                              =   2  ⋅n  n  +  3  ⋅nn  +   1  ⋅n  n            (11.4.13)
                                          ωω ˙ q r     q ∂  r  3    1     q ∂  r  1    2     q ∂  r  2    3
                       where, as in Eq. (11.4.9) n , n , and n  are mutually perpendicular unit vectors fixed in B,
                                                2
                                                       3
                                             1
                       and the partial derivatives are all computed in R. Then, by substituting from Eq. (11.4.11)
                       into (11.4.10),  dc/dt becomes:
                                   R
                                                                 r )
                                          R            n                n      
                                           dc  = ωω  × c + ∑ ( ωω  ×  c ˙ q = ωω t ∑ ω  q ×
                                                                       +
                                                                              ˙
                                          dt    t          q r ˙           q r ˙  r   c    (11.4.14)
                                                      r=1                r=1
                       Recalling that c is an arbitrary vector fixed in B and by comparing Eqs. (11.4.8) and (11.4.14)
                       we see that the angular velocity of B in R may be expressed as:
                                                               n
                                                         =
                                                       ωωωω + ∑  ωω q ˙                        (11.4.15)
                                                            t      q r ˙  r
                                                               r =1
                        The vectors ω  and  ωω  ˙ q r  are called partial angular velocity vectors of B in R. As with the
                                     t
                       partial velocity vectors of Eq. (11.4.3), the partial angular velocity vectors may be thought
                       of as being base vectors for the movement of B in the n-dimensional space of the q .
                                                                                                 r
                        Partial velocity and partial angular velocity vectors are remarkably easy to evaluate:
                       from Eqs. (11.4.5) and (11.4.15) we see that the partial velocity and partial angular velocity
                       vectors  v   and  ωω   are simply the coefficients of the  ˙ q  . Specifically, we see from Eq.
                                ˙ q r   ˙ q r                             r
                       (11.4.15) that analogous to Eq. (11.4.4):

                                                                 ∂
                                                         ωω =∂ ωω ˙ q                          (11.4.16)
                                                           ˙ q r   r
                        To illustrate the ease of evaluation of these vectors, consider first the motion of a particle
                       P in a three-dimensional inertia frame R as in Figure 11.4.1. Let p locate P relative to a
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