Category Archives: L

Lighting system

Professional scanners should have a lighting system that provides uniform and gentle illumination and can adapt variably to a wide variety of originals, depending on the specific requirements. In addition, the light sources should be glare-free as well as UV/IR-free, so that there is no radiation exposure for the user in accordance with EN60825-1.

LED lighting unit: Less is more!

All our book2net scanners are therefore equipped with a LED lighting system as standard, which provides a stable color temperature during the scanning process and thus guarantees true color reproduction. When using conventional LED light bands, different luminous intensities also occur in due to the different light paths on the surface, depending on the position of the light source. Therefore, we use only Fresnel lenses, which compensate for this process and provide uniform illumination of the entire scan area.

Thanks to the CMOS sensor technology we use and innovative process optimization, our scanners operate with an extremely reduced illumination time of 0.6 sec. This guarantees particularly gentle recording of originals with the lowest light requirement to avoid irretrievable damage to paper, ink and colors that can be caused by excessive light intensity.

In addition, we have optimized the design of our devices to ensure the best possible illumination and to assure constant scan quality:

The elegant black design of our scanners prevents annoying back reflections.

The rear-mounted lighting system and optimized housing curvature provide the optimum angle of light incidence to avoid uncontrolled reflections into the optics caused by the curvature of the side.

All of our lighting units are customized for specific applications as fixed components of our high-quality systems.

 

Additional lighting: optimal illumination for large formats and precious old books

Large formats and particularly valuable old books with waved surfaces, special inks, gold grounds and gildings require more than standard illumination.

To meet these special requirements, we have developed auxiliary lighting for our Ultra, Flash, Mosquito, Hornet and Cobra production scanners that can be integrated, mounted or controlled externally as required. The additional lighting can be easily synchronized with the integrated scanner lighting via a light control module. This ensures optimum shadow- and reflection-free illumination.

 

Sided light: individual illumination for special requirementsn

Some of our devices such as our reprographic systems and book2net Archive Pro scanners also feature individually controllable back and side lighting units to enable application-specific lighting scenarios.

Lighting scenarios with book2net reprographic system to highlight different features on a coin.

Advantages of the book2net lighting system:

Modern, LED lighting concept (UV/IR and ozone free, according to EN60825-1)

Glare- and flicker-free light (no flash effects)

Low energy consumption < 100 W

Stable color temperature of 5500 Kelvin

Lowest light intensity; controllable from 1000 to 3500 lux

LED lighting units individually adjustable and controllable according to special requirements

Unique Fresnel lens concept for uniform illumination of originals

Continuous regulation of the light emission angle

Additional illumination (optional)

Extremely long service life (10,000 working hours)

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LED

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Fresnel lens

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Exposure time

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Image sensor / CMOS versus CCD

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Luminance

Luminance is a photometric measure of the luminous intensity (brightness) per unit area of light travelling in a given direction. It describes the amount of light that passes through, is emitted from, or is reflected from a particular area, and falls within a given solid angle. The standard unit of luminance is candela per square meter (cd/m2).

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Candela

Candela (cd) is an internationally standardized physical unit of measurement for [...]

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Luminous intensity distribution curve

The luminous intensity distribution curve (LID) or light distribution curve is a graphical representation of the measured luminous intensity of a luminaire. In a LID, the luminous intensity in candela (cd) as well as the beam angle can be read.

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Candela

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Luminous efficacy

The luminous efficacy of a light source is its efficiency or energy efficiency, which is the quotient of luminous flux (lumen) and absorbed electrical power (watt). Thus, a 100 W light bulb that delivers a luminous flux of 1500 lm has a luminous efficacy of 15 lm/W. This means that only part of the electrical power absorbed by a light bulb is converted into visible light radiation. The remaining power is mainly emitted in the infrared range and is thus detectable as thermal radiation.

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Lumen

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Lumen

Lumen (lm) is the internationally standardized unit of measurement for the luminous flux of a light source and thus allows conclusions to be drawn about the brightness of the illuminant. Colloquially, one also speaks of the light output of a lamp.

The luminous flux indicates the amount of light generated per unit of time; the unit of time is quasi = 0 due to the speed of light of 300,000 km/second, since the speed of light forms our perceptual limit.

Lumen is not to be confused with the unit for illuminance lux, which indicates how much light per unit of time is incident on a unit of area, i.e. the amount of brightness on/at an illuminated surface.

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Candela

Candela (cd) is an internationally standardized physical unit of measurement [...]

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Lux

Lux (lx) is the internationally standardized physical unit of measurement [...]

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Luminous efficacy

The luminous efficacy of a light source is its efficiency [...]

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Lux

Lux (lx) is the internationally standardized physical unit of measurement for the illuminance of a light source. The name is derived from the Latin word for light.

The unit lux is calculated from the luminous flux incident on a given surface, i.e. the number of lumens per m². Thus, the illuminance of one lux corresponds to the uniform illumination of a 1 m² surface with a luminous flux of one lumen (1 lux is 1 lumen/m²). Alternatively, 1 lux can be defined as the illuminance at 1 meter from a point light source of luminous intensity 1 candela (1 cd).

Thus, the lux number depends on the distance between the light source and the surface: The greater the distance, the lower the number of lux.

Unlike lumen and candela, which are transmit quantities, lux is a receive quantity.

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Candela

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Lumen

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LPI

LPI is an abbreviation for „lines per inch“.

Similar to DPI or PPI, LPI Lines per inch (LPI) is a measurement of printing resolution. A line consists of halftones built up by physical ink dots made by the printer device to create different tones. Specifically LPI is a measure of how close together the lines in a halftone grid are. The quality of printer device or screen determines how high the LPI will be. High LPI indicates greater detail and sharpness.

Conversion of the LPI to DPI can be done by simple multiplication: z.B. 150 LPI x 16 = 2400 DPI

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DPI

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PPI

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Light spectrum

The light spectrum is the visible range of the electromagnetic spectrum that can be perceived by the eye. The spectral range visible to humans is between 380 and 780 nanometers, corresponding to a frequency range of about 4·1014 to 7.5·10 14 Hz.

Each wavelength produces a different color, for example green has a wavelength of about 540nm and blue is between 450 and 500nm. If all visible wavelengths are displayed next to each other, a rainbow-like color gradient appears. In addition, there are wavelength ranges that the human eye cannot see or perceive because there is no trigger for a pulse. These ranges are called ultra-violet (10-380nm) and infrared radiation (>780nm). The shorter a wavelength is, the more energy it has. This is also the reason why ultraviolet light is so harmful for our skin and our eyes, because in the long run it stimulates molecules to change their spatial structure and to split off single atoms.

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Multispectral Imaging System at The National Archives

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Line sensor

Line sensors are light or radiation sensitive detectors (mostly semiconductor detectors), which consists of one or sometimes several rows of pixels (lines) to capture information. The counterpart to the line sensor is the area sensor, which has a rectangular arrangement (matrix) of pixels.

Line sensors are based on the original development for data storage from 1969 and have not changed significantly to this day. The light-sensitive sensors are very suitable for scanning documents in order to capture an image. The detector runs close to the original, scans the document line by line and combines the information from the individual scan lines to form an overall image. Sometimes only one line is used; sometimes a separate line is used for each color channel (red, green, blue).
This technology is still employed today in scanners, fax machines and copiers because it is very cheap and available in large quantities.

A major disadvantage of using this type of sensor in scanners is that the image capturing takes a comparatively long time due to the sequential scanning and that mechanical wear always takes place due to the movement of the components. This can lead to premature wear, especially with production scanners that have to digitize large quantities of documents in continuous operation.

In addition, the depth of field of line sensors is very small and covers only a few millimeters. Particularly in the case of books with a deep book fold or wavy pages that are not completely flat, this leads to blurring or even loss of information in the digitized material.

At book2net, we therefore only use image area sensors in our scanning systems.

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Bayer Matrix (Bayer Sensor)

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Image sensor / area sensor

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Image sensor / CMOS versus CCD

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Depth of field

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Lens

Every camera needs a lens to project the object or the image to be captured onto the sensor. Lenses come in a variety of designs for a wide range of applications: Macro, back-magnification, telephoto, wide-angle, zoom or tilt-shift lens. Basically, lenses can be adjusted in two ways: focal length and aperture. The focal length determines how close or how far away objects must be to be in focus. This is also referred to as focusing. The aperture controls how much light falls through the optics onto the sensor. If the aperture is wide open, a lot of light falls on the sensor and the depth of field is basically shallow. If you close the aperture, the image becomes darker, but the depth of field increases.

In our systems we use a special lens, which was designed for the digitization of documents and books. Here we pay a lot of attention to a distortion-free image in order to avoid deformations of the documents. This ensures that the documents are also scanned and displayed at right angles and true to scale. In addition, the lens we use differs from other commercially available lenses in that it is apochromatic corrected and has extremely high sharpness even in the peripheral areas. This is because unlike in photography, when digitizing, the important image information is not only in the center of the image, but also, or especially, in the peripheral areas.

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Focus

In physics, the focus describes the point in an optical system [...]

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Depth of field

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Margin area

When digitizing with reflected light scanners, the margin area of the [...]

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Autofocus

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Motorized focus

Our systems work with a fixed focal length as standard. This [...]

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Image sensor / CMOS versus CCD

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Bayer Matrix (Bayer Sensor)

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