White Light Sources

The following properties of white light sources are often particularly important for applications:

• For applications like lighting, the color temperature of a white light source, indicating its color tone, is an important parameter.
• The color rendering index (CRI) is a measure for how well colors can be judged when objects are illuminated with that light.
• Concerning energy efficiency, the luminous efficacy is an important parameter. Note that the effectively achieved energy efficiency can also substantially depend on how directional the light emission is. For example, the energy-saving qualities of LED-based solutions often come to a substantial degree from their directed emission, making it easier to send the light where it is needed.
• The temporal coherence of any white light source is necessarily low as a consequence of its broad optical bandwidth.
• Many white light sources also have a low spatial coherence, making it difficult to tightly focus the light, and a correspondingly low radiance. For example, that applies to long-arc lamps, having a large light-emitting volume. A low radiance is usually no problem for applications like lighting, but is not acceptable for applications like projection displays. Higher radiance can be achieved with short-arc lamps, which are operated with high power densities (high intensity discharge lamps).
• Most white light sources operate continuously, some others are made for pulsed emission – in particular, flash lamps.

Our properties of interest may be the operation lifetime, the ability of rapid switching, the constancy of the radiant flux (low intensity noise, weak aging, weak temperature dependence), the constancy of the spectral shape and color tone, and the absence of possibly disturbing ultraviolet light.

Many white light sources are required for various lighting applications (indoor and outdoor), where one often needs to generate a substantial luminous flux over extended times. The energy efficiency, largely determined by the luminous efficacy, is then particularly important.

There are various other applications in the context of illumination, often in a more or less localized manner – for example, reading lights, projection displays, machine vision and microscope illumination.

Pulsed white light sources can be used for photography, for stroboscopes and in some scientific applications.

Further, there are special applications of white light sources in scientific and technical areas such as spectroscopy, colorimetry, forensic investigations and solar cell testing.

In some cases, the term white light sources is used for sources which do not really produce a white color impression, but just produce light with a broad optical bandwidth. Some of them do not even emit in the visible spectral range, while others cover a range from somewhere in the infrared to the ultraviolet. Certain applications such as white light interferometry do not really need a white color impression, but just the large bandwidth. Other examples for applications are the characterization of optical components and spectroscopy.

While most white light sources have a poor spatial coherence, there are broadband sources with a high spatial coherence, sometimes even with the whole optical power delivered in a single spatial mode e.g. of an optical fiber. This allows focusing of the radiation to very small spots. Such sources can be different types of superluminescent sources, e.g. superluminescent diodes or ASE sources based on rare-earth-doped fibers.

For particularly high bandwidths, sometimes even more than octave-spanning, one may employ supercontinuum sources, based on strongly nonlinear interactions e.g. in an optical fiber. Most widely used for those are photonic crystal fibers. The input light can be supplied in the form ultrashort pulses, nanosecond pulses, or continuously.

For some applications, the optical bandwidth specified as a full-width half-maximum value is important, whereas weak tails in the spectrum are not relevant. In other cases, it is only important to have at least some moderate level of power spectral density over a broad range, even if the spectral flux varies a lot within that range.

Your question or comment:

Spam check:

  (Please enter the sum of thirteen and three in the form of digits!)

By submitting the information, you give your consent to the potential publication of your inputs on our website according to our rules. (If you later retract your consent, we will delete those inputs.) As your inputs are first reviewed by the author, they may be published with some delay.