What Is Stray Light?

Definition of Stray Light

Stray light is any electromagnetic radiation that is unwanted and interferes with the performance of an optical system’s intended functions. Unwanted stray light can occur in either imaging or projection systems, although it is usually more critical to control the former. Stray light can originate from the object the optical system is capturing, from unintended external emitters, or, in the case of infrared-sensitive systems, it can originate from elements of the system itself emitting light due to their own heat.

Examples of stray light include:

  • Light reflections off mechanical mounting surfaces inside the optical system
  • Light leaking through a gap in the system enclosure
  • Light scattering off dust and other imperfections on the system’s optical surfaces
  • Sky glow, which is caused by the reflection of municipal lights from the atmosphere and affects ground-based astronomy
  • The sun, Earth, and moon, which can affect orbiting telescopes

Two Types of Stray Light

Stray light can be characterized in two distinct types: ghosts and flare or veiling glare.

Ghosts occur in imaging systems when light from a source in the image field undergoes two or more unwanted reflections and then falls on the imaging device, creating an unwanted ghost image. For digital cameras, one of the most common sources of ghost images is light that reflects off the imaging device back into the optical system and then reflects off a lens surface back to form a secondary image.

Flare, or veiling glare, generally occurs when light scatters inside the optical system either off imperfections in the optical surfaces, or off mechanical elements in the system. Veiling glare can also be caused by atmospheric reflection of light such as with haze or sky glow.

Ghosts:
  • Arise from unintended reflections between imaging surfaces
  • Result from higher or unblocked diffractive orders generated by gratings
  • Form through secondary imaging of bright scattering surfaces

Flare or veiling glare:

  • Enter the image from sources outside the optical system’s field
  • Originate from bright sources within the field of view or from thermal emission by warm surfaces
  • Occur when light scatters within the optical system
Photo taken with a cell phone camera that shows three sharply focused ghost images of candle flames and one extended ghost image.

Figure 1. Ghost example: Photo taken with a cell phone camera that clearly shows three sharply focused ghost images of the candle flames. There is also a fourth, extended ghost image centered on the middle sharp ghost image.

Why Is It Important to Find Stray Light in a Design?

Stray light can reduce the contrast of an image by adding unwanted light to the image. For example, stray light can:

  • Reduce the sensitivity of detection systems.
  • Create unappealing images in commercial imaging systems.
  • Cause unwanted bright spots in the beam pattern of light projection systems.

How Does Software Help Find Stray Light?

Stray light can reduce the contrast of an image by adding unwanted light to the image. For example, stray light can:

  • Reduce the sensitivity of detection systems.
  • Create unappealing images in commercial imaging systems.
  • Cause unwanted bright spots in the beam pattern of light projection systems.
A sequential ray trace of a single ghost image path.

Figure 2. Ghost example: A sequential ray trace of a single ghost image path. The light from an object in the field of view passes through the lens and forms an image on the detector at right. Some of the light is then reflected by the detector back into the lens. One of the lens surfaces then reflects the light back to the detector at a different location. This ghost image is of interest because the ghost light is nearly focused on the detector, which will lead to a much brighter ghost image than if the light were spread out over a larger area.

Flare can enter the optical system through many and often unexpected optical paths. You can use Monte Carlo software to investigate the contributions. Brute-force methods will randomly generate many rays and analyze how the energy is distributed through the model. Variance reduction methods can efficiently find contributions coming from paths that include low probability events such as high-angle scattering.

Unintended light example: Light from an object scatters off the lens mount and then is reflected to the detector.

Figure 3. Unintended light example: Light from an object in the field of view scatters off the lens mount and then is reflected by a lens surface to the detector.

Computational Approaches to Simulating Stray Light

The analysis and control of stray light, composed of ghost images and flare, is an important but complex task for the design of imaging systems. Ghost images arise from multiple reflections from surfaces in the primary optical path. Ghost images that impinge on the image plane at or near a focus are of specific concern ⁠— flare can arise from light reflecting off lens mounts, nonoptical surfaces of the lenses (such as flats and edges), and the detector itself reimaged back onto the detector. Diffraction from the microstructure of the detector can also complicate the process of modeling light reflected from the detector.

Stray Light Workflow

Here is a typical workflow for using Keysight software to analyze stray light in a camera system:

Typical workflow for using Keysight software to analyze stray light in a camera system.

Model and Analyze Stray Light with Keysight

Our optical design engineering portfolio offers several software options for modeling and analyzing stray light. Choosing the right software depends on your application, and our products allow for cosimulations.

Closeup of face with a screen reflecting off curved glass

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