[AMR] Small remarks

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2026-08-09 14:26:36 +02:00
parent df428322e8
commit 3de83b61dc
3 changed files with 7 additions and 3 deletions
@@ -6,7 +6,7 @@
\item \textit{Turning} Wheel axis must intersect the \bi{Instant Centre of Rotation} (ICR) of vehicle,
speeds: $v_i \div R_i = \Omega$ ($R_i$ = dist. wheel-ICR; $\Omega$: vehicle rotation rate (around ICR))
\end{itemize}
To compute ICR, use $v_i \div R_i = \Omega$ and similarity.
To compute ICR, use $v_i \div R_i = \Omega$ and similarity (see \ref{sec:classic-stereo}.
Below: $\alpha$, $l$ pos in frame, $\beta$ rot at that pos ($z$-ax).
To compute $\vec{c}$ in $\vec{c} \cdot {_B}\vec{v}_{WB} = \omega$
@@ -7,10 +7,14 @@ Typ. derive D.M. with sensor dir param (as vec line eq)
\subsubsection{Classic Stereo}
Both images: same plane, focal length $f$, centre, $x$-axis. Given corresponding pixels $[u_l, v]$ and $[u_r, v]$: disparity (pixel offset) $d = u_r - u_l$;
\label{sec:classic-stereo}
Both images: same plane, focal length $f$, centre, $x$-axis. Given corresponding pixels $[u_l, v]$ and $[u_r, v]$: \bi{disparity} (pixel offset) $d = u_r - u_l$;
$z = \frac{b \cdot f}{d}$, then projected into left (right) cam, $u_l = f\cdot \frac{x}{z} + c_u$ or $u_r = f \cdot \frac{x - b}{z} + c_u$, $b$ distance between cameras.
Then often apply pinhole camera projection (to e.g. get 3D point coords, comp ${_C}\vec{r}$, then point $z \cdot {_C}\vec{r}$).
Uncertainty introduced with 1.-order error propag. $\Delta z = \pardiff{d}z \Delta d$, with $\Delta d$ error of $d$
Uncertainty introduced with 1.-order error propag. $\Delta z = \pardiff{d}z \Delta d$, with $\Delta d$ error of $d$.
Too large $b$ disables depth estimations, too small increases error
\shorttheorem[Intercept] $f \div Z = u_l \div X$, with $Z$ and $X$ the $z$ and $x$ coordinates of tracked object
\subsubsection{Time of Flight, Projection}