Jitter (optics) explained

In optics, jitter is used to refer to motion that has high temporal frequency relative to the integration/exposure time. This may result from vibration in an assembly or from the unstable hand of a photographer. Jitter is typically differentiated from smear, which has a lower frequency relative to the integration time. Whereas smear refers to a relatively constant rate during the integration/exposure time, jitter refers to a relatively sinusoidal motion during the integration/exposure time.

The equation for the optical Modulation transfer function associated with jitter is

MTF _{jitter} (k) = e ^{- (1)/(k ^{2\sigma} ^{2} 2)} where k is the spatial frequency and \sigma is the amplitude of the jitter.^[1] Note that this frequency is in radians of phase per cycle. The equivalent expression in Hz isMTF _{jitter} (u) = e ^{-2 \pi ^{2} u ^{2\sigma} ^{2}} where u is the spatial frequency and \sigma is again the amplitude of the jitter (note that as the jitter approaches infinity, the value of the function tends towards zero).

For spacecraft, operation in a vacuum often means low mechanical damping. Meanwhile, spacecraft are compact and rigid, to withstand high launch loads. Jitter, then, is transmitted easily and often a limiting factor for high-resolution optics.

Notes and References

1. Johnson. Jerris F.. Modeling imager deterministic and statistical modulation transfer functions. Applied Optics. 10 November 1993. 32. 32. 6503–13. 10.1364/AO.32.006503. 20856491.