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Contents

   



(Top)
 


1 Optical systems  



1.1  Monochromatic light  





1.2  Astronomy  







2 Sources  





3 Design tools  





4 See also  





5 References  














Stray light







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From Wikipedia, the free encyclopedia
 


Stray lightislight in an optical system which was not intended in the design. The light may be from the intended source, but follow paths other than intended, or it may be from a source other than that intended. This light will often set a working limit on the dynamic range of the system; it limits the signal-to-noise ratioorcontrast ratio, by limiting how dark the system can be.[1] Ocular straylight is stray light in the human eye.

Optical systems

[edit]

Monochromatic light

[edit]

Optical measuring instruments that work with monochromatic light, such as spectrophotometers, define stray light as light in the system at wavelengths (colors) other than the one intended. The stray light level is one of the most critical specifications of an instrument.[2] For instance, intense, narrow absorption bands can easily appear to have a peak absorption less than the true absorption of the sample because the ability of the instrument to measure light transmission through the sample is limited by the stray light level. One method to reduce stray light in these systems is the use of double monochromators. The ratio of transmitted stray light to signal is reduced to the product of the ratio for each monochromator, so combining two monochromators in series with 10−3 stray light each produces a system with a stray light ratio of 10−6, allowing a much larger dynamic range for measurements.

Methods have also been invented to measure and compensate for stray light in spectrophotometers.[3] ASTM standard E387 describes methods of estimating stray light in spectrophotometers.[4] The terms used are stray radiant power (SRP) and stray radiant power ratio (SRPR).

There are also commercial sources of reference materials to help in testing the stray light level in spectrophotometers.[5]

Astronomy

[edit]

Inoptical astronomy, stray light from sky glow can limit the ability to detect faint objects. In this sense stray light is light from other sources that is focused to the same place as the faint object.

Stray light is a major issue in the design of a coronagraph, used for observing the Sun's corona.

Sources

[edit]

There are many sources of stray light.[6] For example:

Design tools

[edit]

A number of optical design programs can model stray light in an optical system, for instance:

Such models can be used to predict and minimize stray light in the final system.

See also

[edit]

References

[edit]
  1. ^ "Section 4: Optical Signal-to-Noise Ratio and Stray Light". Retrieved Feb 6, 2009.
  • ^ "Stray Light and Performance Verification". Mettler Toledo. Retrieved Aug 14, 2018.
  • ^ "Stray light measurement and compensation – Patent 4526470". Retrieved Feb 6, 2009.
  • ^ "ASTM E387 -04 Standard Test Method for Estimating Stray Radiant Power Ratio of..." Retrieved Feb 6, 2009.
  • ^ "Stray Light Reference Materials". Retrieved Feb 6, 2009.
  • ^ a b "Stray light and ghost images – analyzed and reduced using simulation software" (PDF). Retrieved Feb 6, 2009.
  • ^ Lau, A. S. (1977). Lytle, John D.; Morrow, Howard E. (eds.). "The Narcissus effect in infrared optical scanning systems". Stray-Light Problems in Optical Systems. Stray Light Problems in Optical Systems. 107: 57. Bibcode:1977SPIE..107...57L. doi:10.1117/12.964596. S2CID 122030149.

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=Stray_light&oldid=1205255112"

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