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Section 3.3 Direction Cosines and Angular Velocity

If the orientation of referential \(\cB\) relative to \(\cA\) is defined in terms of the direction cosines \(c_{ij} = \bha_i \cdot \bhb_j\) between basis \((\bha_1 , \bha_2 , \bha_3 )\) of \(\cA\) and basis \((\bhb_1 , \bhb_2 , \bhb_3 )\) of \(\cB\text{,}\) then it should be possible to relate the components of angular velocity \(\bom_{\cB / \cA}\) on either basis to the time-derivatives of these quantities.
First we resolve \(\bom_{\cB / \cA}\) on the bases of \(\cA\) and \(\cB\) in the following way
\begin{equation*} \bom_{\cB / \cA} = \Omega_1 \bha_1 + \Omega_2 \bha_2 + \Omega_3 \bha_3 = \omega_1 \bhb_1 + \omega_2 \bhb_2 + \omega_3 \bhb_3 \end{equation*}
We then determine \(\dot{c}_{ij}\) by differentiating \(\bha_i \cdot \bhb_j\) relative to referential \(\cA\text{:}\)
\begin{align*} \dot{c}_{ij} \amp = \bha_i \cdot\left({d \bhb_j \over dt} \right)_{\cA} \\ \amp = (c_{i1} \bhb_1 + c_{i2} \bhb_2 + c_{i3} \bhb_3) \cdot (\bom_{\cB / \cA} \times \bhb_j) \\ \amp = \bom_{\cB / \cA} \cdot \left(c_{i1} \bhb_j\times \bhb_1 + c_{i2} \bhb_j \times \bhb_2 + c_{i3} \bhb_j \times \bhb_3 \right) \end{align*}
where we have used the property \(({\bf u} \times {\bf v})\cdot {\bf w} = {\bf u} \cdot ( {\bf v} \times {\bf w})\) of the triple scalar product (see Definition A.1.10). Then letting \(j=1,2,3\) we find:
Alternatively, we can express \(\dot{c}_{ij}\) in terms of the components \((\Om_1 , \Om_2 , \Om_3)\text{:}\)
\begin{equation} \begin{array}{l} \dot{c}_{1j} = c_{3j} \Omega_2 - c_{2j} \Omega_3 \\ \dot{c}_{2j} = c_{1j} \Omega_3 - c_{3j} \Omega_1 \\ \dot{c}_{3j} = c_{2j} \Omega_1 - c_{1j} \Omega_2 \end{array} \qquad (j=1,2,3)\tag{3.3.2} \end{equation}
In practical applications such as spacecraft attitude dynamics, the time evolution of \(\bom_{\cB/\cA}\) is obtained as a vector resolved into the “body basis”, that is, in terms of components \((\om_1 , \om_2 , \om_3)\text{:}\) the orientation of \(\cB\) relative to \(\cA\) is then obtained by integration of the system of equations (3.3.1).