Infrared Application of the Month #1: Drying Screen Printing on Auto Glass
A manufacturer of automotive glass sought a more efficient method for drying of screen printing onto the glass. The previous method resulted in a low line speed and left the glass hot after drying. Fitting the process with carbon emitters from Heraeus Noblelight doubled power density, nearly tripled line speed and reduced glass temperature by more than 15°C.
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Infrared Application of the Month #2: Textile Printing with Thermosetting Ink
A textile manufacturer had been using ceramic heaters to dry thermosetting ink. the low efficiency of that method resulted in high energy consumption, arequired an oven with a large footprint, and the short lamp life necessitated frequent lamp replacement. A mediumwave infrared solution from Heraeus Noblelight corrected all of these problems.
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Tech Center Spotlight: Mediumwave IR Heaters
Stable and efficient, fast response medium wave heaters can transfer high power over long lengths. The high absorption by surface layers and films makes them particularly applicable to thin materials, while the fact that they also have a penetrative effect fits them for use in plastics processing. The heaters can be switched on and off in seconds and are consequently best suited for processes with short cycle times.
Because infrared heaters can be individually matched to a particular application, heating and drying processes can be seamlessly integrated within finishing operations – and with minimum disruption to existing manufacturing lines.
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Special Designs: Hybrid Carbon/Shortwave Heaters
Heraeus Noblelight's hybrid Carbon/Shortwave heater offers all of the benefits of Carbon and Shortwave heaters using Heraeus' proven twin-tube design. This infrared heater combines a carbon heater and a short wave infrared heater in the proven quartz glass twin tube.
For more on Hybrid Heaters, click HERE.
A wide assortment of other special design heaters is available from Heraeus. Click HERE for details.
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Engineering Aspects of Radiation Theory
continued from last month's issue
Wien's Law
The relationship between the absolute temperature T of a heat emitting body and the peak wavelength of emission, λ m , is
given by Wien's displacement law:
λ m T = constant
If λ m is expressed in microns
Then T λ m = 2898
An important aspect of this effect is that as the temperature of an emitter is changed, for example, by varying the supply
voltage, the peak wavelength of emission changes in inverse ratio. Therefore, as the temperature increases the peak
wavelength decreases and vice versa.
For example, an emitter operating at a typical temperature of 2200 °C (2473K) would have a radiation peak at 2898/2473
= 1.17 microns, whereas an emitter operating at 650 °C (923K) would have a radiation peak at 2898/923 = 3.14 microns.
We therefore have a means of selecting an emitter whose emission spectrum is best matched to the absorption spectrum
of a receiving body wherever this is a critical factor in optimizing the rate of heat transfer. It should be remembered,
however, that in the infrared process heating field the transmission and absorption wavebands are usually sufficiently
broad to utilize the side-bands of the emitted radiation in addition to the peak wavelength. The basic types of emitters
which have become established over many years in industrial process applications are designed to operate within defined
limits of temperature determined by their construction and materials.
Reflectivity
This is defined as the fraction of the incident radiation which is reflected by a surface. It therefore makes no immediate
contribution to the heating at the surface. The property of reflection is however used extensively in infrared heating both to
orientate the energy and to provide enclosures in which the radiant energy can also take indirect paths to the surface
requiring to be heated.
Transmissivity
This is defined as the fraction of the incident radiation which is transmitted through the receiving surface. Many
substances, particularly those in the liquid and gaseous state, transmit infrared. Thickness of the layer is an important
factor. As illustrated by the greenhouse effect, transmission of visible and short wave energy does not necessarily extend
to the longer wavelengths.
Accounting for Total Radiation
lnfrared radiation striking a body is dispersed in three ways: by reflection, absorption and transmission. The summation of
these three quantities is equal to the value of the incident radiation, but it is normally the aim in infrared process heating to
make the value of the absorbed radiation as high as possible.
Lambert's Cosine Law
This is one of the basic laws of photometry which states that the intensity of radiation falling onto a flat surface from a
small radiant source is a maximum when the receiving surface is normal to the source. However, if the receiving surface
is turned away from the normal by an angle X, the intensity of the radiation received is proportional to the cosine of the
angle X between the normal to the receiving surface at that point and the direction of the radiation.
This law applies only to a small source radiating over a relatively large distance, for example in illumination engineering.
In infrared engineering the sources usually occupy substantial areas, sometimes larger than the individual receiving
surfaces of the workpieces and the distances between the source and receiver are usually comparatively small. The
cosine law is therefore not universally valid in the process heating field, but it does underline the need to arrange for the
radiation to strike the receiver at right angles for the best efficiency of heat transfer. Conversely, if a thin metal panel, for
example, is placed with its edge towards the source of radiation (that is, when Cos X = 0) it would not, in theory, receive
any heat. However, this directional effect does not present a problem in a well designed infrared oven, and in certain
cases it can even be put to good use.
The Inverse Square Law
This law is also based on the concept of a point source of radiation and is more appropriate to illumination engineering. It
states that the radiant intensity at a receiving surface varies inversely as the square of its distance from the point source
of radiation. On the other hand, radiation between two infinitely large parallel plates is independent of the distance between
them. Another example not conforming to the Inverse Square Law is that of radiation to a sphere from a Iarger spherical
shell surrounding it. For comparatively large radiant source areas such as those commonly employed in infrared ovens
the surface-to-surface relationship between distance and intensity is found not to conform to the inverse square law. In
practice the intensity can be almost independent of distance over very small distances of the order of a few centimeters,
increasing to an almost linear relationship at greater distances.
Tungsten Halogen High Intensity Emitters
As with the basic short wave emitters , the tungsten halogen units
comprise a linear coiled tungsten filament surrounded by a clear quartz
glass tube.
However, with the basic type the tungsten slowly evaporates from the
filament when the emitter is in use. This causes progressive blackening of
the inner walls of the tube causing a steady loss of short wave output. The
addition of a halogen such as iodine or bromine to the gas -filled tube
prevents this blackening by combining with the tungsten particles to form a tungsten halide. This would normally
condense on the inner wall of the tube, but if the wall is maintained above 300 °C it will not condense, but will be returned
to the vicinity of the filament. The high temperature of the filament causes the tungsten halide to break down into tungsten
and halogen. The tungsten being deposited on to the filament, and the halogen released to repeat the cycle.
The filament temperature of tungsten halogen tubes is around 2700 °C, equivalent to a peak wavelength of 1 micron. The
color temperature is therefore similar to an incandescent lamp bulb. Ratings up to 20 kW per tube are available, with a
heated length up to 670 mm.
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That's it for this month's issue of Application Notes for IR Heating. Feel free to encourage your colleagues to subscribe. Just click HERE to send them an invitation to subscribe. It's quick, easy, FREE, and no-obligation.
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