If I understand your question correctly, you want to know how to calculate the angle and position of a laser beam downstream of two steering mirrors (which happen to be actuated electrically). I would recommend using ray matrix methods. Since you want to ask a question about the optical axis and not the size and shape of the beam, you will need to use 4x4 (or 3x3) ray matrix techniques.
For more in depth info see section 15.4 of Anthony Siegman's textbook "Lasers" and the review article on matrix methods in decentered systems by Wang Shaomin. Siegman uses the less clear 3x3 matrices, but has explanations which are easier to follow; Shaomin uses 4x4 matrices and has an appendix with all useful matrices already calculated, but the exposition is highly mathematical.
Working in the 4x4 case the quantity of interest is a 4x1 vector whose first two components describe the position and angle of a ray within the beam, with respect to the optical axis, and whose second two components describe the position and angle of the optical axis itself. The 4x4 matrices describe how this 4x1 vector transforms under interaction with an optical system. For your case you only need the two most basic matrices, the translation operator and flat mirror reflection operator, given by
$$
T(d)=
\begin{bmatrix}
1 & d & 0 & 0\\
0 & 1 & 0 & 0\\
0 & 0 & 1 & 0\\
0 & 0 & 0 & 1
\end{bmatrix}
\qquad
M(\epsilon)=
\begin{bmatrix}
1 & 0 & 0 & 0 \\
0 & 1 & 0 & -2\epsilon\\
0 & 0 & 1 & 0\\
0 & 0 & 0 & 1
\end{bmatrix},
$$
where $d$ is the distance of propagation and $\epsilon$ is the misalignment of the mirror in units of slope.
In your case you know the position and angle of the optical axis at the start, and you want to run the beam through a system with three translations and two reflections. Recall that matrix multiplication is not commutative so the final matrix is given by
$$
T(d_3)M(\epsilon_2)T(d_2)M(\epsilon_1)T(d_1)=
\begin{bmatrix}
1 & d_1+d_2+d_3 & 0 & -2(d_2\epsilon_1+d_3(\epsilon_1+\epsilon_2))\\
0 & 1 & 0 & -2(\epsilon_1+\epsilon_2)\\
0 & 0 & 1 & 0\\
0 & 0 & 0 & 1
\end{bmatrix}.
$$
The two terms in the upper right of the matrix describe how the position and angle of the optical axis changes with respect to the original. One final piece of information; all of this takes place within the paraxial approximation so be careful when dealing with large misalignments.
So, the final result is that the angle and position of the optical axis will be given at a distance $d_3$ downstream of the second mirror by
$$
x=-2(d_2\epsilon_1+d_3(\epsilon_1+\epsilon_2))
\qquad
\theta=-2(\epsilon_1+\epsilon_2).
$$
In this relatively simple example we could have figured this out with straightforward geometry; the position change caused by the first mirror is $-2(d_2+d_3)\epsilon_1$ and the position change caused by the second mirror is $-2d_3\epsilon_2$. The change in angle of the beam is simply the sum of the two angles of the mirrors. The minus signs are due simply to an arbitrary definition of which way the mirror turns when $\epsilon$ is positive.
