Pulse timing jitter describes variation of pulse arrival times relative to a stated timing reference. Choose a reproducible pulse feature and reference instants ; define errors . One measure is their standard deviation . Edge-time error relative to an ideal reference differs from variation of successive periods or cycle-to-cycle differences; the primary timing guide distinguishes these measurements.[ref]
Digital Design Debugging Guide by Tektronix. Picking out Jitter, Diagram5 and statistical discussion, printedpp.12–14
For an original distribution, let each error equal , where is equally likely to be or . The mean delay is and . The root mean square error about zero is instead . A fixed delay changes the mean without increasing the spread. None of these numbers is the individual pulse's duration.
A fast photodetector, reference timing signal and oscilloscope can measure a selected arrival feature. A fixed electrical threshold can also turn amplitude/readout noise into an apparent time change, producing threshold timing noise from amplitude noise. Specify the reference, feature, observation duration and measurement response. A fitted or recovered reference can absorb some timing variation, changing the reported residual.
Timing variation can become gated-energy variation even at constant full pulse energy. The Gaussian gate centring error provides one quantitative model, distinct from pulse-to-pulse energy fluctuation of complete pulses.
Threshold timing noise from amplitude noise occurs when voltage fluctuations move the apparent time at which a pulse crosses a fixed threshold. Let a clean electrical trace cross at with nonzero slope . For small additive noise , linearizing givesThe result concerns a selected measurement feature. It is not automatically the source's physical arrival-time spread. The timing primer distinguishes reference-edge error from other jitter statistics.[ref]
Digital Design Debugging Guide by Tektronix. Picking out Jitter, Diagrams5–6
For an original readout example, use noise standard deviation and crossing slope . The linear estimate is . At half that slope it becomes , even with the same noise amplitude. Both units and the local slope matter.
A pulse generator, receiver and oscilloscope can compare crossing times while the threshold position or signal slope changes. Small-noise linearization presumes a unique nearby crossing; ringing, large noise or multiple crossings require a fuller model. The relevant noise bandwidth must match the recorded trace.
A changing pulse scale can also shift a fixed threshold time even without additive noise. That amplitude-dependent time walk is a different effect from the random perturbation derived above. Pulse timing jitter describes the resulting timing observable, while the original optical arrival and detector readout contributions must be distinguished.
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