Stereographic Projection of Probabilistic Frequency-Domain Uncertainty
Anton Nystrom, Venkatraman Renganathan, Michael Cantoni
TL;DR
The paper addresses probabilistic uncertainty in SISO LTI systems by projecting Nyquist plots onto the Riemann sphere via stereographic projection and measuring distances with the chordal metric $\kappa$. It derives an explicit expression for the CDF $\mathbb{F}_{\mathsf{K}}(d)$ of the point-wise chordal distance $K=\kappa(\bar{P},P)$ at a fixed frequency, showing that $K=\frac{\sqrt{Q}}{c}$ with $Q=z/w$ and $c=\sqrt{1+|\bar{P}|^2}$, and expressing the result through the joint density $f_{zw}$ and the corresponding $f_{xy}$. A numerical example with Gaussian uncertainty around $\bar{P}=1+j$ validates the monotonic CDF $\mathbb{F}_{\mathsf{K}}(d)$ and demonstrates the method. The work lays a foundation for probabilistic robust control by linking distributions over complex Nyquist values to distributional statements about stability-related distances, and it outlines future extensions to the $\nu$-gap and MIMO settings. The approach enables quantifiable probabilistic guarantees for closed-loop performance under model uncertainty.
Abstract
This paper investigates the stereographic projection of points along the Nyquist plots of single input single output (SISO) linear time invariant (LTI) systems subject to probabilistic uncertainty. At each frequency, there corresponds a complex-valued random variable with given probability distribution in the complex plane. The chordal distance between the stereographic projections of this complex value and the corresponding value for a nominal model, as per the well-known Nu-Gap metric of Vinnicombe, is also a random quantity. The main result provides the cumulative density function (CDF) of the chordal distance at a given frequency. Such a stochastic distance framework opens up a fresh and a fertile research direction on probabilistic robust control theory.
