Jitter (optics)


title: "Jitter (optics)" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["image-defects"] topic_path: "general/image-defects" source: "https://en.wikipedia.org/wiki/Jitter_(optics)" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

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 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^{-\frac {1} {2} k^2\sigma^2} where k is the spatial frequency and \sigma is the amplitude of the jitter. Note that this frequency is in radians of phase per cycle. The equivalent expression in Hz is :MTF_{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.

References

References

  1. {{Google books. rcrGlrguj1YC. Encyclopedia of optical engineering
  2. Johnson, Jerris F.. (10 November 1993). "Modeling imager deterministic and statistical modulation transfer functions". Applied Optics.

::callout[type=info title="Wikipedia Source"] This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page. ::

image-defects