Gaussian input uncertainty at a clipped acquisition-time threshold
ID: gaussian-input-uncertainty-at-a-clipped-acquisition-time-threshold
Gaussian input uncertainty at a clipped acquisition-time threshold produces a mixed output distribution rather than an ordinary Gaussian error bar. Hold the decay time fixed and assume the logarithmic input ratio has distribution , with . The required extension isThe directional derivative of a clipped logarithmic acquisition time explains the kink; here the full input distribution is propagated through it.
Writing and for the standard normal cumulative distribution function and density, respectively,For the continuous part has density . It integrates to less than one because the remaining probability is an atom at zero. Treating this density alone as the entire distribution loses that atom.
At the nominal threshold , half the outcomes are zero and the conditional positive part has a half-normal distribution. Direct integration of the normal density givesFor an original example, and logarithmic standard deviation give mean extension about and standard deviation , although inserting the nominal input into the clipped formula gives zero. The probability of an extension above is .
The quantiles of a clipped Gaussian acquisition duration must likewise include the zero atom. A symmetric interval around the nominal zero duration cannot represent these probabilities. NIST's uncertainty discussion stresses the need to know and combine input distributions when assigning an interval probability.[ref]
This is a stated uncertainty model for a conditional recording requirement, not a worst-case optical-energy guarantee. Uncertain decay time, correlation among the original envelope parameters or a non-Gaussian logarithmic ratio requires the corresponding joint propagation instead. Establishing the optical envelope remains a separate experimental task.
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