\chapter{Finite-radius distances without an artificial noise floor} \section{From a normal vector to an actual point} A scalar normal echo is a tangent-space quantity. To connect it with a Riemannian distance, fix $x$ in the soul and use the normal exponential map. In the global coordinates of Chapter~2, \[ \exp_x(tu)=(x,tu),\qquad \exp_x(tHu)=(x,tHu). \] Define the normalized squared-distance signal \begin{equation}\label{eq:radiusdef} \mathcal D_t(u,H)= \frac{d_{M_\lambda}((x,tu),(x,tHu))^2}{2t^2},\qquad t>0. \end{equation} For a general smooth metric one expects its limit to be $1-u^{\mathsf T}Hu$. The explicit quotient family permits a multiplicative bound, uniform even when this echo deficit is very small. \section{The normal fibers are totally geodesic} Recall the metric \[ g_\lambda=Q+ h_v(\mathrm dv+\lambda\theta v, \mathrm dv+\lambda\theta v), \qquad h_v(W,W)=\ip W{B_v^{-1}W}. \] The fiber metric $h$ is invariant under the standard $\SO(d)$ action. The horizontal flow of the connection acts on the fiber by such rotations and therefore preserves its metric. \begin{lemma}[Totally geodesic fibers]\label{lem:geodesicfibers} Every fiber $\{x\}\times\R^d$ is totally geodesic in $M_\lambda$. \end{lemma} \begin{proof} Take vertical vector fields $V,W$ and a horizontal field $X$. The Koszul formula expresses $2g(\nabla_VW,X)$ as the negative horizontal derivative of $g(V,W)$ plus the two correction terms involving the vertical parts of $[X,V]$ and $[X,W]$. Their sum is the negative Lie derivative of the fiber metric along the horizontal flow. That derivative is zero because the flow is a fiber isometry. The other Koszul terms vanish by horizontal--vertical orthogonality and because $[V,W]$ is vertical. Hence the horizontal part of $\nabla_VW$ is zero. This is exactly the vanishing of the second fundamental form of the fiber. \end{proof} Total geodesy alone does not say that arbitrary distant fiber points are joined by ambient minimizing geodesics staying in the fiber. We use it only inside a sufficiently small common convex neighborhood of the zero section. For such points the fiber geodesic is an ambient geodesic and, by local uniqueness, is the ambient minimizer. \section{Uniform local distance comparison} In polar fiber coordinates, \[ h=\mathrm dr^2+\frac{r^2}{1+\coup r^2}\,g_{\mathbb S^{d-1}}. \] Consequently, on the Euclidean fiber ball $|v|\le t$, \begin{equation}\label{eq:fibercomparison} \frac1{1+\coup t^2}g_{\rm Eucl}\le h\le g_{\rm Eucl}. \end{equation} The function $r^2$ is geodesically convex for this fiber metric. For example, the radial Hessian is positive and the angular Hessian has the sign of $f'(r)$ for $f(r)=r/\sqrt{1+\coup r^2}$; here $f'(r)>0$. Thus a minimizing fiber segment with endpoints of radius $t$ remains in that ball. \begin{theorem}[Multiplicative finite-radius calibration]\label{thm:radius} There is a radius $t_0(d)>0$ such that, for $0