2023518 — For example, sunlight falls on an apple, and all the colours falling on it get absorbed except the colour red. Red colour then gets reflected ...

This thus leads to the question: When is stray light significant in a measurement? Unfortunately, there is no general answer to this question. It depends on the application and the corresponding measurement requirements. Below are two guidelines that can be adhered to:

This article focuses on giving an overview of the causes of stray light, its effects on the measurement accuracy of spectroradiometers, and the different methods of stray light suppression. It provides a detailed description of the different stray light suppression requirements for different applications.

Note: In most cases, the responsivity of a pure VIS device is not ideal for the UV range which increases the measurement uncertainty. With the BTS2048-VL-TEC or BTS2048-UVVISNIR and mathematical stray light correction, Gigahertz-Optik offers a good universal device that is characterized by high responsivity and high stray light suppression, even in the UV range. This is perfectly supplemented by the BTS2048-UV, BTS2048-UV-2 and the BTS2048-UV-S for high-quality UV measurements.

The reason an extra signal level is shown in addition to the LED peak in the LED measurement is not just because of the stray light but also due to the spectrometer’s noise. Here, a noise count of 1 for a 16 bit ADC means a 1:65536 dynamic range which corresponds to 6E-4. For a spectroradiometer, the basic measurement dynamic range achievable is limited by the resolution of the ADC and the signal-to-noise ratio. Ideally, the stray light level should be less than the ADC resolution.

The requirements for stray light suppression vary for different applications. As explained in the previous chapter, good stray light suppression may introduce some complexity and cost. These should therefore be well matched to the specific application requirements. This chapter provides guidance several typical application areas.

With the SDF data and the measurement data from the light source being measured, mathematical correction methods according to (Zong et al., 2006) or (Nevas et al., 2012) can be used for the different applications. Here, the mathematical correction must be performed for every measurement, so a good software implementation is crucial. In addition, the manufacturer must have an OPO in order to perform the measurements precisely without excessive extrapolation and model assumptions. The spectroradiometer must also be stable (over time) for the stray light matrix to be valid over useful periods of time. If this is the case, the quality of the mathematical stray light correction can be described as follows. The level of stray light can be reduced by about 1 or 2 orders of magnitude as shown in the example below:

In short, the effect that stray light has on the measurement uncertainty cannot be ignored. The method used for stray light suppression should be selected based on the respective application and its requirements. For instance, measurements in the UV range typically require more extensive suppression methods than in the VIS range. The extent of the stray light effect is a device specification and must be characterized by the manufacturer. In addition, the amount of stray light also depends on the spectral distribution of the light source being measured.

An innovative way to optimize stray light suppression, particularly in the critical UV range, is combining a spectroradiometer with several optical longpass filters and bandpass filters within the device. Bandpass filters basically allow the approximation of a single array spectroradiometer to a double monochromator since the bandpass filter is significantly reducing the radiation entering the spectroradiometer and thus the potential for stray light generation. With the use of long pass filters the above described method can be applied during calibration and at each measurement.

For measurements of the sun and daylight, it is important to determine which parts of the solar spectrum are to be measured. If you only need information from VIS and NIR, the arguments from section 4.1 must be taken into account. However, if the UV range is of interest in particular, high- quality spectroradiometers that are optimized for the UV range are needed for UV index, erythema, and ozone measurements among others. In such applications, VIS universal devices quickly reveal their limits in terms of stray light suppression. This was confirmed by the publication by (Egli et al., 2016) among others. In addition, the devices must be temperature-stabilized and weather-proof since long measurement sequences are often required.

LED lighting by CCS is the key to success for machine vision applications,CCS is the leading company of LED industrial inspection lighting.

S-polarized light (from the German word senkrecht) is perpendicular to the plane of incidence. Depiction of a linearly polarized wave (left) and standard ...

Stray lightwikipedia

Nevas S, Wübbeler G, Sperling A, Elster C and Teuber A 2012 Simultaneous correction of bandpass and stray-light effects in array spectroradiometer data Metrologia 49 S43

The same arguments as those described in section 4.4 apply to this type of measurements. Sufficient stray light suppression is required to prevent any stray results, especially for erythema and ICNIPR measurements or evaluations regarding e.g. artificial optical radiation Directive 2006/25/EC or DIN EN 62471 photo biological safety.

Stray light leads to measurement uncertainty and must be considered in thecalculation of measurement uncertainty as specified in CIE S025 or CIE 198. Since the amount of stray light is dependent on the spectral distribution being measured and the design of the spectrometer, the calculation must be performed for each particular spectroradiometer and measurement application.

Note: With this technology, Gigahertz-Optik GmbH developed one of the best optimized UV spectroradiometers for stray light suppression and that almost works as a perfect double monochromator – the BTS2048-UV-S.

Besides the design, the choice of the optical components is also crucial. The quality of the mirror coating determines the proportion of diffusely reflected radiation and the resulting amount of stray light. Similarly, the quality of the optical grating is also crucial in minimizing stray light.

Note: Gigahertz-Optik has many years of experience in the development of spectrometers and optimizes its spectrometer units using ZEMAX. In addition, every unit must go through a long and thorough development and qualification process where all its optical elements and properties are tested and optimized.

A well-known method of stray light correction in the UV range is based on long-pass filters such as Schott GG435. The GG435 is used to perform an additional measurement during calibration where the amount of OoR stray light is directly determined. This signal can then be subtracted from the raw data and thus applied to the resulting calibration data. This method enables calibrations with reduced stray light influences but the subsequent measurement of other light sources may still have a different stray light influence.

Note: The BTS2048-UV-S-WP, BTS2048-VL-TEC-WP and BTS2048-IR-WP from Gigahertz-Optik are devices that guarantee high-quality measurements for a wide spectral range – from deep UV up to NIR.

Find Light Through Prism stock images in HD and millions of other royalty-free stock photos, illustrations and vectors in the Shutterstock collection.

Figure 8: Comparison of the BTS2048-UV-S with a double monochromator. The sun edge can be resolved by up to 10E- 5 at a measurement time of 3 s (comparison with 90 s of the double monochromator).

Our annual Christmas light show transforms Stockeld Park into a dazzling, twinkling Winter Wonderland! Book your ticket now and enjoy our spectacular Christmas ...

Thanks to tunable lasers OPO optical parametric oscillator), spectrometers can be analyzed and characterized at any wavelength. Thus, LSFs (line spread functions) can be determined at each wavelength, which together form an SDF (signal distribution function) characterization matrix of the spectrometer. This means that the data collected from the measurements can be used to characterize the device and its stray light properties based onwavelength.

This means that the level of stray light also depends on the spectral distribution of the measurement light source being measured.

However, this method has a limitation – the LSFs must be measured for the entire spectral range of the detector for optimal stray light suppression (i.e. the spectroradiometer should also cover this range). For silicon based detectors, this ranges from 200 nm to 1100 nm. If all functions are not measured, only part of the stray light will be corrected!

Stray lightexamples

You can add products to the watchlist and compare them with one another or send us an inquiry. There are watchlist symbols on product pages and product tables for this purpose.

Stray lighttest in UV calibration

Note: The term spectroradiometer is used regularly in the article. A spectroradiometer is a radiometrically calibrated spectrometer and its function is based on relative measurements.

Note: The (Nevas et al., 2012) method also performs an optical bandwidth correction. Alternatively, the (Zong et al., 2006) method can also be used and combined with the CIE 214 optical bandwidth correction. Gigahertz-Optik offers both methods.

What causesstray lightin spectrophotometer

Ideally, different filters must be used if a large spectral range is to be covered in order to ensure optimal stray light suppression. Implementing this requires an integrated fast filter wheel, extensive know-how about filter technology and powerful software since several individual measurement steps have to be intelligently combined to produce one final measurement. A user-friendly system requires that all these be implemented automatically by software.

In comparison, Figure 3 shows measurement data for a similar scenario (an OG515 filter is used instead of GG475) but using a measurement device that is less optimized for stray light suppression. It can be seen that the amount of stray light is significantly higher, even though there is actually less potential for stray light in this case since the OG515 filter is more effective than the GG475. This poorer stray light suppression has a negative effect on the measurement accuracy for this type of measurement including, for example, chromaticity values.

Illumination from this 300 watt Xenon Light Source is to be used for observation of body cavities, hollow organs, and other surgical sites. This device is also ...

If you are interested in our products, pls feel free to contact led strip light factory.

The figure below shows a halogen lamp measurement with and without a Schott GG475 edge filter using a spectroradiometer.

How doesstray lightaffect absorbance

What isstray lightin spectrophotometer

A prerequisite is a properly designed spectrometer unit. Optical simulations are often used to optimize modern spectroradiometers since the complexity of optical beam paths has to be carefully considered. Through such simulations, spectroradiometers can be optimized to meet the highest demands. For instance, the image sharpness must be optimized, the 0th order blocked, and higher orders removed diligently from the beam path towards the detector.

However, if you compare these data with the measurement of a red LED (same spectroradiometer), you will see that in the measurement of the red LED, the stray light level below 475 nm (the red LED does not have a signal with this wavelength) is significantly lower (2E-5 for the LED compared to 6E-4 for the halogen lamp):

Stray lightin UV VIS spectrophotometer

Egli L, Gröbner J, Hülsen G, Bachmann L, Blumthaler M, Dubard J, Khazova M, Kift R, Hoogendijk K, Serrano A, Smedley A and Vilaplana J M 2016 Quality assessment of solar UV irradiance measured with array spectroradiometers Atmos. Meas. Tech. 9 1553-67

Blockout & Light Control Films · 2 mil white vinyl diffuser films · Provides 37% or 65% light transmission · Pressure sensitive, permanent adhesive · Adheres to ...

Vision Light Tech supplies a broad range of solutions in light, lenses and filters for the industrial machine vision worldwide. VLT is renowned for their ...

This means that in this measurement the strong broadband signal from the halogen lamp, at wavelengths above 475 nm, produced little stray light below 475 nm. The signal detected in this wavelength therefore consists of the stray light and noise.

Zong Y, Brown S W, Johnson B C, Lykke K R and Ohno Y 2006 Simple spectral stray light correction method for array spectroradiometers Appl. Opt. 45 1111-9

The same arguments as mentioned in section 4.1 apply to laboratory and production measurements. However, handheld measurement devices demand different measures. The need to keep these devices compact poses an extra challenge for the optical design in terms of stray light suppression. The very small size of “mini-spectrometers”, is not well suited for suppressing stray light and therefore can result in instruments that are unsuitable for precise color measurements.. However, they are ideal for fast, onsite test measurements, where the requirements are quite different. High- quality handheld devices have fully-fledged spectrometer units which match up well to laboratory instruments and provide accurate, onsite measurement result. These high-quality handheld devices should also be temperature-corrected and provide reproducible and stable measurement results!

Note: These calculations require several specification and characterizations of the spectroradiometer. In addition, models for calculating the measurement uncertainty in spectroradiometry are arbitrarily complex. Gigahertz-Optik GmbH is a reliable partner who offers you an ideal, quick solution fitting your requirements.

Stray lightphotography

I have read the data privacy declaration. I consent to my details and data being collected and stored electronically for the purpose of responding. Note: You can revoke your consent at any time for the future.

For most applications in which the measurement of monochromatic LEDs is necessary in the visible (VIS) range, standard stray light suppression using a high-quality spectroradiometer with good optical is enough. This can also be sufficient for the measurement of white LEDs if e.g. an accuracy of ±0.0020 of CIE1931 chromaticity coordinates (x,y) is sufficient. Measurements of white LEDs with and without mathematical stray light correction show that this accuracy of the color location can be improved by about 0.0005 through the correction. This means that in cases where precision is needed, mathematical stray light correction can be a good option.

Stray light discussed here, also known as “false” light, is signal that is detected during a spectrometer measurement additional to the measurement signal dedicated for the selected wavelength ranges. These signals cannot be separated and thus the stray light considerably distorts the measurement result. The amount of stray light in a measurement strongly depends on the light source and the spectrometer itself. Inside a spectrometer unit, stray light can originate from:

For LED measurements spectroradiometers that are optimized for the visible spectral range are often used. Thus, their stray light suppression in the UV range is usually insufficient which results in large measurement uncertainties. However, the results of such measurements and the required stray light suppression depend on the intended application and the available boundary conditions. In a dark room or integrating sphere where just the UV LED is present the stray light influence might be less significant. However if there is ambient light present a sufficient stray light suppression is essential. This should especially be considered when measuring white LED with a non-negligible UV content. It is therefore recommended to use at least one of the stray light correction methods available for UV/VIS spectroradiometers. If applicable, a spectroradiometer that was specifically developed for the UV range should be used.

For users, a partner with comprehensive expertise, competent advice, and a coherent product portfolio with appropriate measurement technology e.g., tunable lasers (OPO) and an accredited calibration laboratory are essential.

Note: Gigahertz-Optik offers stray light matrices for its high-end spectrometers from the BTS2048 Series as standard options. The mathematical application is completely integrated in the S-BTS2048 software as well as the S-SDK-BTS2048. The characterization and calibration data for the stray light correction are saved on the device for easy access by the user. No extra measures are required from the user.

Since the GG475 filters out the signal in the short-wave spectral range below 475 nm, one can conclude that the signal detected below the edge is caused by stray light + noise. Since this is difficult to identify using a linear scale, the logarithmic view is recommended. The ideal filter function is shown in green.

Note: Gigahertz-Optik offers the corrected MSC15 mini-spectrometer, which perfectly meets all the requirements of a low-budget device. In addition, the BTS256-EF high-quality devices perfectly round off the portfolio of our handheld devices. These guarantee sufficient stray light suppression and support many extra features such as Wi-Fi and flicker measurements.

2008729 — The mercury vaporises, and it is this vapour that is responsible for producing light. Mercury atoms absorb energy from the electric current that ...

Figure 3: Halogen lamp measurement filtered with the OG515 (logarithmic view), spectroradiometer not ideal for stray light suppression