A flashtube ( flashlamp) produces an electrostatic discharge with an extremely intense, incoherent, full-spectrum white light for a very short time. A flashtube is a glass tube with an electrode at each end and is filled with a gas that, when triggered, ionizes and conducts a high-voltage pulse to make light. Flashtubes are used most in photography; they also are used in science, medicine, industry, and entertainment.
The power level of the lamps is rated in watts/area, total electrical input power divided by the lamp's inner wall surface. Cooling of the electrodes and the lamp envelope is of high importance at high power levels. Air cooling is sufficient for lower average power levels. High power lamps are cooled with a liquid, typically by flowing deionized water through a tube in which the lamp is encased. Water-cooled lamps will generally have the glass shrunk around the electrodes, to provide a direct thermal conductor between them and the cooling water. The cooling medium should flow also across the entire length of the lamp and electrodes. High average power or continuous-wave arc lamps must have the water flow across the ends of the lamp, and across the exposed ends of the electrodes as well, so the deionized water is used to prevent a short circuit. Above 15 W/cm2 forced air cooling is required; liquid cooling if in a confined space. Liquid cooling is generally necessary above 30 W/cm2.
Thinner walls can survive higher average-power loads due to lower mechanical strain across the thickness of the material, which is caused by a temperature gradient between the hot plasma and cooling water, (e.g. 1 mm thick doped quartz has a limit of 160 W/cm2, a 0.5 mm thick one has a limit of 320 W/cm2). For this reason, thinner glass is often used for continuous-wave arc-lamps. Thicker materials can generally handle more impact energy from the shock wave that a short-pulsed arc can generate, so quartz as much as 1 mm thick is often used in the construction of flashtubes. The material of the envelope provides another limit for the output power; 1 mm thick fused quartz has a limit of 200 W/cm2, synthetic quartz of same thickness can run up to 240 W/cm2. Other glasses such as borosilicate generally have less than half the power loading capacity of quartz. Aging lamps require some derating, due to increased energy absorption in the glass due to solarization and sputtered deposits.
For low electrode wear the electrodes are usually made of tungsten, which has the highest melting point of any metal, to handle the thermionic emission of electrons. are often made from porous tungsten filled with a barium compound, which gives low work function; the structure of cathode has to be tailored for the application. are usually made from pure tungsten, or, when good machinability is required, lanthanum-alloyed tungsten, and are often machined to provide extra surface area to cope with power loading. DC arc lamps often have a cathode with a sharp tip, to help keep the Electric arc away from the glass and to control temperature. Flashtubes usually have a cathode with a flattened radius, to reduce the incidence of hot spots and decrease sputter caused by peak currents, which may be in excess of 1000 amperes. Electrode design is also influenced by the average power. At high levels of average power, care has to be taken to achieve sufficient cooling of the electrodes. While anode temperature is of lower importance, overheating the cathode can greatly reduce the lamp's life expectancy.
Ablative flashtubes need to be refilled and vacuumed to the proper pressure for each flash. Therefore, they cannot be used for very high-repetition applications. Also, this usually precludes the use of very expensive gases like krypton or xenon. The most common gas used in an ablative flashtube is air, although sometimes cheap argon is also used. The flash usually must be very short to prevent too much heat from transferring to the glass. However, because nearly all the plasma is concentrated at the surface, the lamps have very low inductance and flashes can often be shorter than a normal lamp of comparative size. The flash from a single ablative flashtube can also be more intense than multiple lamps. For these reasons, the most common use for the lamps is for the pumping of dye lasers. Photochemistry by D. Bryce-Smith -- The Chemical Society 1979 Page 93--94
Ko is used to calculate the amount of input voltage and capacitance needed to emit a desired spectrum, by controlling the current density. Ko is determined by the internal diameter, arc length, and gas type of the lamp and, to a lesser extent, by fill pressure. The resistance in flashtubes is not constant, but quickly drops as current density increases. In 1965, John H. Goncz showed that the plasma resistivity in flashtubes is inversely proportional to the square root of current density. As the arc develops, the lamp experiences a period of negative resistance, causing both the resistance and voltage to decrease as the current increases. This occurs until the plasma comes into contact with the inner wall. When this happens, the voltage becomes proportional to the square root of current, and the resistance in the plasma becomes stable for the remainder of the flash. It is this value which is defined as Ko. However, as the arc develops the gas expands, and calculations for Ko do not take into account the dead volume, which leads to a lower pressure increase. Therefore, any calculation of Ko is merely an approximation of lamp impedance.
The spectrum emitted by flashtubes is far more dependent on current density than on the fill pressure or gas type. Low current-densities produce narrow spectral-line emission, against a faint background of continuous radiation. Xenon has many spectral lines in the UV, blue, green, red, and IR portions of the spectrum. Low current densities produce a greenish-blue flash, indicating the absence of significant yellow or orange lines. At low current-densities, most of xenon's output will be directed into the invisible IR spectral lines around 820, 900, and 1000 nm. Low current-densities for flashtubes are generally less than 1000 A/cm2.
Higher current-densities begin to produce continuum emission. Spectral lines broaden and become less dominant as light is produced across the spectrum, usually peaking, or "centered", on a certain wavelength. Optimum output-efficiency in the visual range is obtained at a density that favors "greybody radiation" (an arc that produces mostly continuum emission, but is still mostly translucent to its own light; an effect similar to sunlight when it passes through a cloud). For xenon, greybody radiation is centered near green, and produces the right combination for white light. Greybody radiation is produced at densities above 2400 A/cm2.
Current densities that are very high, approaching 4000 A/cm2, tend to favor black-body radiation. Spectral lines all but disappear as the continuum radiation dominates, and output center shifts toward the ultraviolet. As current densities become even higher, visually, xenon's output spectrum will begin to settle on that of a blackbody radiator with a color temperature of 9800 kelvins (a rather sky-blue shade of white). Except in cases where intense UV light is needed, such as water decontamination, blackbody radiation is usually not desired because the arc becomes opaque, and much of the radiation from within the arc can be absorbed before reaching the surface, impairing output efficiency.
Due to its high-efficiency, white output, xenon is used extensively for photographic applications, despite its great expense. In lasers, spectral-line emission is usually favored, as these lines tend to better match absorption lines of the lasing media. Krypton is also occasionally used. At low current-densities, krypton's spectral-line output in the near-IR range is better matched to the absorption profile of neodymium-based laser media than xenon emission, and very closely matches the narrow absorption-profile of Nd:YAG. None of xenon's spectral lines match Nd:YAG's absorption lines so, when pumping Nd:YAG with xenon, the continuum radiation must be used. Solid-state lasers: a graduate text By Walter Koechner, Michael Bass – Springer-Verlag 2003 Page 190
Heavier gases exhibit higher resistance, and therefore, have a higher value for Ko. Impedance, being defined as the resistance required to change energy into work, is higher for heavier gases, and as such, the heavier gases are much more efficient than the lighter ones. Helium and neon are far too light to produce an efficient flash. Krypton can be as good as 40% efficient, but requires up to a 70% increase in pressure over xenon to achieve this. Argon can be up to 30% efficient, but requires an even greater pressure-increase. At such high pressures, the voltage drop between the electrodes, formed by the spark streamer, may be greater than the capacitor voltage. These lamps often need a "boost voltage" during the trigger phase, to overcome the extremely high trigger-impedance.
Nitrogen, in the form of air, has been used in flashtubes in home made dye lasers, but the nitrogen and oxygen present form chemical reactions with the electrodes, and themselves, causing premature wear and the need to adjust the pressure for each flash.
Some research has been done on mixing gases to alter the spectral output. The effect on the output spectrum is negligible, but the effect on efficiency is great. Adding a lighter gas will only reduce the efficiency of the heavier one.
Within the plasma, positive ions accelerate toward the cathode while electrons accelerate toward the anode. Neutral atoms move toward the anode at a slower rate, filling some localized pressure differential created by the ions. At normal pressures this motion is in very short distances, because the particles interact and bump into each other, and, exchanging electrons, they reverse direction. Thus, during the pulse neutral atoms are constantly ionizing and recombining, emitting a photon each time, relaying electrons from the cathode to the anode. The greater the number of ion transitions for each electron; the better the conversion efficiency will be, so longer tubes or higher pressures both help increase the efficiency of the lamp. During the pulse, skin effect causes free electrons to gather near the inner wall, creating an electron sheath around the plasma. This makes the area electro-negative and helps to keep it cool. The skin effect also increases inductance by inducing in the central plasma.
Bound-bound transitions occur when the ions and neutral atoms collide, transferring an electron from the atom to the ion. This method predominates at low current-densities, and is responsible for producing the spectral-line emission. Free-bound transitions happen when an ion captures a free electron. This method produces the continuum emission, and is more prominent at higher current-densities. Some of the continuum is also produced when an electron accelerates toward an ion, called free-free transitions, producing bremsstrahlung radiation. Bremsstrahlung radiation increases with increasing energy density, and causes a shift toward the blue and ultraviolet end of the spectrum.
In contrast, changes in the input voltage or capacitance have no effect on discharge time, although they do have an effect on current density. As flash duration decreases, the electrical energy becomes concentrated into shorter pulses, so the current density will increase. Compensating for this usually requires lowering the capacitance as pulse duration decreases, and then raising the voltage proportionately in order to maintain a high enough energy-level. However, as pulse duration decreases, so does the "explosion energy" rating of the lamp, so the energy level must also be decreased to avoid destroying the lamp.
The amount of power loading the glass can handle is the major mechanical limit. Even if the amount of energy (joules) that is used remains constant, electrical power (wattage) will increase in inverse proportion to a decrease in discharge time. Therefore, energy must be decreased along with the pulse duration, to keep the pulsed power levels from rising too high. Quartz glass (1 millimeter thick per 1 second discharge) can usually withstand a maximum of 160 watts per square centimeter of internal surface-area. Other glasses have a much lower threshold. Extremely fast systems, with inductance below critical damping (0.8 microhenries), usually require a shunt diode across the capacitor, to prevent current reversal (ringing) from destroying the lamp. If the pulse is allowed to ring through the lamp it will lengthen the flash, so the diode traps the ringing, allowing the lamp to shut down at the correct time.
The limits to long pulse durations are the number of transferred electrons to the anode, sputter caused by ion bombardment at the cathode, and the temperature gradients of the glass. Pulses that are too long can vaporize large amounts of metal from the cathode, while overheating the glass will cause it to crack lengthwise. For continuous operation the cooling is the limit. Discharge durations for common flashtubes range from 0.1 microsecond to tens of , and can have repetition rates of hundreds of hertz. Flash duration can be carefully controlled with the use of an inductor.
The flash that emanates from a xenon flashtube may be so intense that it can ignite flammable materials within a short distance of the tube. Carbon nanotubes are particularly susceptible to this spontaneous ignition when exposed to the light from a flashtube. Similar effects may be exploited for use in aesthetic or medical procedures known as intense pulsed light (IPL) treatments. IPL can be used for treatments such as hair removal and destroying or moles.
Failure from heat is usually caused by excessively long pulse-durations, high average-power levels, or inadequate electrode-size. The longer the pulse; the more of its intense heat will be transferred to the glass. When the inner wall of the tube gets too hot while the outer wall is still cold, this temperature gradient can cause the lamp to crack. Similarly, if the electrodes are not of a sufficient diameter to handle the peak currents they may produce too much resistance, rapidly heating up and thermally expanding. If the electrodes heat much faster than the glass, the lamp may crack or even shatter at the ends.
Sputter occurs when the energy level is very low, below 15% of the explosion energy, or when the pulse duration is very long. Sputter is the vaporization of metal from the cathode, which is redeposited on the walls of the lamp, blocking the light output. Because the cathode is more emissive than the anode, the flashtube is polarized, and connecting the lamp to the power source incorrectly will quickly ruin it. However, even if connected properly, the degree of sputter may vary considerably from lamp to lamp. Therefore, it is impossible to predict the lifetime accurately at low energy-levels.
At higher energy-levels, wall ablation becomes the main process of wear. The electrical arc slowly erodes the inner wall of the tube, forming microscopic cracks that give the glass a frosted appearance. The ablation releases oxygen from the glass, increasing the pressure beyond an operable level. This causes triggering problems, known as "jitter." Above 30%, the ablation may cause enough wear to rupture the lamp. However, at energy levels greater than 15%, the lifetime can be calculated with a fair degree of accuracy.
When operated below 30% of the explosion energy, flashtube lifetime is generally between a few million to tens of millions of flashes.
In dentistry it is used in "light box" devices to light-activate the hardening of various restorative and auxiliary light-curing resins (for example: Megaflash mini, Uni XS and other devices).
Due to their high intensity and relative brightness at short (extending into the ultraviolet) and short pulse widths, flashtubes are also ideally suited as light sources for laser pumping atoms in a laser to where they can be stimulated to emit coherent, monochromatic light. Proper selection of both the filler gas and current density is crucial, so that the maximum radiated output-energy is concentrated in the bands that are the best absorbed by the lasing medium; e.g. krypton flashtubes are more suitable than xenon flashtubes for pumping , as krypton emission in near infrared is better matched to the absorption spectrum of Nd:YAG.
Xenon flashtubes have been used to produce an intense flash of white light, some of which is absorbed by that produces the laser power for inertial confinement fusion. In total about 1 to 1.5% of the electrical power fed into the flashtubes is turned into useful laser light for this application.
Pulsed light (PL) is a technique to decontaminate surfaces by killing microorganisms using pulses of an intense broad spectrum, rich in UV-C light. UV-C is the portion of the electromagnetic spectrum corresponding to the band between 200 and 280 Nanometer. Pulsed light works with xenon lamps that can produce flashes several times per second. Disinfection robots use pulsed UV light.
A recent application of flashlamps is photonic curing.
Because electrical arcs could be made that were much faster than mechanical-shutter speeds, early high-speed photographs were taken with an open-air, electrical-arc discharge, called spark photography, helping to remove blur from moving objects. This was typically done with the shutter locked open while in a dark or dimly lit room, to avoid overexposing the film, and a method of timing the flash to the event to be photographed. The earliest known use of spark photography began with Henry Fox Talbot around 1850. In 1886, Ernst Mach used an open-air spark to photograph a speeding bullet, revealing the shockwaves it produced at supersonic speeds. Ernst Mach; his work, life, and influence By John T. Blackmore - University of California Press 1972 Page x Open-air spark systems were fairly easy to build, but were bulky, very limited in light output, and produced loud noises comparable to that of a gunshot.
In 1927, Harold Edgerton built his first flash unit while at the Massachusetts Institute of Technology. Wanting to photograph the motion of a motor in vivid detail, without blur, Edgerton decided to improve the process of spark photography by using a mercury-arc rectifier, instead of an open-air discharge, to produce the light. He was able to achieve a flash duration of 10 microseconds, and was able to photograph the moving motor as if "frozen in time."
His colleague's interest in the new flash apparatus soon provoked Edgerton to improve upon the design. The mercury lamp's efficiency was limited by the coolest part of the lamp, causing them to perform better when very hot but poorly when cold. Edgerton decided to try a noble gas instead, feeling that it would not be as temperature dependent as mercury, and, in 1930, he employed the General Electric company to construct some lamps using argon instead. The argon tubes were much more efficient, were much smaller, and could be mounted near a reflector, concentrating their output. Slowly, camera designers began to take notice of the new technology and began to accept it. Edgerton received his first major order for the strobes from the Kodak company in 1940. Afterward, he discovered that xenon was the most efficient of the noble gases, producing a spectrum very close to that of daylight, and xenon flashtubes became standard in most large photography sets. It was not until the 1970s that strobe units became portable enough to use in common cameras.
In 1960, after Theodore Maiman invented the ruby laser, a new demand for flashtubes began for use in lasers, and new interest was taken in the study of the lamps.
Flashtubes operate at high pressures and are known to explode, producing violent shockwaves. The "explosion energy" of a flashtube (the amount of energy that will destroy it in just a few flashes) is well defined, and to avoid catastrophic failure, it is recommended that no more than 30% of the explosion energy be used. Flashtubes should be shielded behind glass or in a reflector cavity. If not, eye and ear protection should be worn.
Flashtubes produce very intense flashes, often faster than the eye can register, and may not appear as bright as they are. Quartz glass will transmit nearly all of the long and short wave UV, including the germicidal wavelengths, and can be a serious hazard to eyes and skin. This ultraviolet radiation can also produce large amounts of ozone, which can be harmful to people, animals, and equipment.
Many compact cameras charge the flash capacitor immediately after power-up, and some even just by inserting the batteries. Merely inserting the battery into the camera can prime the capacitor to become dangerous or at least unpleasant for up to several days. The energy involved is also fairly significant; a 330 microfarad capacitor charged to 300 volts (common ballpark values found in cameras) stores almost 15 joules of energy.
Frame 2: The trigger pulse ionizes the gas, glowing with a faint, blue light. Spark streamers form from each electrode, moving toward each other along the inner surface of the glass tube.
Frame 3: Spark streamers connect and move away from the glass, and a plasma tunnel forms allowing current to surge.
Frame 4: Capacitor current begins to run away, heating the surrounding xenon.
Frame 5: As resistance decreases voltage drops and current fills the tube, heating the xenon to a plasma state.
Frame 6: Fully heated, resistance and voltage stabilize into an arc and the full current load rushes through the tube, causing the xenon to emit a burst of light.
Electrodes and seals
Gases and fill pressure
Operation
External triggering
Series triggering
Simmer-voltage triggering
Prepulse techniques
Ablative flashtubes
Variable pulse width control
Electrical requirements
Output spectrum
Xenon
Krypton and other gases
Light production
Intensity and duration of flash
Lifetime
Catastrophic failure
Gradual failure
Applications
History
Safety
Popular culture
Animation
See also
External links
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