This application claims the benefit of priority under 35 U.S.C. §365 of International Patent Application Serial No. PCT/GB2007/000136 filed on Jan. 18, 2007, designating the United States of America, which in turn claims the benefit of priority under 35 U.S.C. §119 of United Kingdom Patent Application Serial No. GB 0601154.8, filed on Jan. 20, 2006.
The invention relates to a high power short optical pulse source.
There are many existing and emerging applications of high power lasers in industrial, medical and scientific processes. Conventionally, solid state and gas lasers, with bulk-optical cavities, are used in these applications, and the outputs of these lasers are generally free space, collimated beams. In most cases, the laser source can be very large, and often constitutes the largest single element of an instrument or machine. In using laser systems in industrial applications, it is often difficult to position the large laser very close to the intended target of the laser beam and therefore bulk-optic beam steering is required. Such beam steering includes specially designed, low loss, high reflective and high-damage threshold mirrors, mounted and positioned with precision and on a heavy and vibration-isolated surface to enable a robust, reliable performance. In many applications such as semiconductor inspection, the inspection tool is just one of many instruments and machines used within the semiconductor manufacturing process, and space on the manufacturing floor—very often being in an expensive, clean-room environment—costs a premium. Therefore, reduction of the instrumentation footprint is highly beneficial. In other industrial applications, such as laser materials processing, the application environment can very often be noisy, dirty and a challenge to the operation of a laser source. In this application additional measures are often required to protect the laser and beam steering optics from the hostile working environment.
Fibre delivery of the laser beam is a clear and interesting option, enabling the laser source to be positioned remotely from the target space and enabling a compact optical beam delivery head (optical head) to be installed within the instrument, with the large laser source being positioned, along with any power supplies and cooling systems, outside an instrument and clean room environment. With conventional bulk lasers, fibre delivery involves launching of the laser output beam into an optical fibre. This is very difficult to achieve, especially in high-power laser applications. Most applications require a good beam quality of the laser, which requires a single mode fibre to deliver the beam. In reality, a single mode fibre has a core diameter of less than 15 μm, very often less than 10 μm, and efficient and stable launching of a beam into this aperture is difficult to achieve. Furthermore, in high-power applications, launching of such high intensities into a fibre will damage the fibre facet.
In addition, applications of UV fibre lasers cannot use a conventional optical fibre to deliver the beam since the UV is absorbed by the fibre. One option that has been considered is to use Hollow Core Photonic Crystal Fibres (HCPCF's) in which the light is mostly guided within an air-core of the fibre. The use of HCPCF's does not solve the problem of launching the light into the fibre and avoiding facet damage at high powers. However, HCPCF's have two benefits—they enable the propagation of UV radiation with relatively low loss and also reduced fibre nonlinearity by a factor of approximately 1000 in comparison to conventional glass-guided optical fibres.
Fibre lasers clearly have a significant advantage over conventional bulk lasers, since the optical beam is already within the fibre and no launching optics are required. Most high-power fibre lasers, particularly in the pulsed lasers, use a Master Oscillator Power Amplifier (MOPA) configuration, in which the output of a low-power fibre oscillator is amplified in a series of high-power fibre amplifiers. In principle, the output of a fibre laser or fibre amplifier can be delivered directly to the intended target through an output fibre. However, in short pulse applications the nonlinear effects of the fibre and amplifier prevent this. Short optical pulses are generally defined (and defined herein) as pulses having a duration of less than 10 ns (10−8 seconds). Reduction of fibre nonlinearity is a major challenge in any fibre-based system, particularly when short pulses are required at relatively high peak intensities.
In cw and long pulse applications, there is little issue with the use of additional lengths of fibre at the amplifier output, since nonlinear effects can often be neglected owing to relatively low peak powers. However, for short-pulse fibre delivery, the nonlinear effects within an optical fibre prevent the delivery of high power pulses due to degradation of the pulses' temporal and spectral characteristics due to high order nonlinear effects such as self-phase modulation, which causes spectral broadening, and Raman scattering, which causes both spectral and temporal broadening.
HCPCF's and conventional optical fibres with larger core sizes (referred to as large-mode-area (LMA) fibres) have been used to reduce fibre nonlinearity. HCPCF's reduce the nonlinearity by several orders of magnitude, where LMA fibres reduce the nonlinearity, scaling with the area of the core. However, the use of LMA fibres for beam delivery in high-power pulsed applications is not a solution since even the largest single-mode core fibre (of 15-20 μm), results in significant nonlinear effects when high-peak power pulses are delivered.
The importance of reducing nonlinear effects can be illustrated by considering UV to generation from a short-pulse source. The use of short pulses to generate visible and UV radiation is a common approach, since the high peak powers attainable from short pulses provide efficient frequency conversion in nonlinear materials such as lithium triborate (LBO) and β-barium borate (BBO). However, efficient conversion within conventional nonlinear media often requires that the spectral bandwidth of the pulse is as narrow as possible—preferably with the pulses transform limited. Any high order nonlinearity within a delivery fibre or a fibre amplifier will result in spectral broadening; a relatively low nonlinearity will double the spectral bandwidth of a pulse and hence significantly reduce the conversion efficiency of that pulse. It is therefore important in all stages of amplification of the pulse to avoid or reduce fibre nonlinear effects.
For amplifying short optical pulses, it is possible to use Chirped Pulse Amplification (CPA), a technique developed for bulk-laser systems, in which a short pulse from an oscillator is stretched in a fibre or bulk optic stretcher, amplified and then compressed. In this instance, the amplified, long pulses can also be delivered by an optical fibre to a remote probe where they are subsequently re-compressed, as described in U.S. Pat. No. 6,249,630.
One of the main problems with the CPA approach is that, in order to amplify pulses without significant nonlinear distortion, the pulse must be stretched to a duration of typically greater than 10 ns. Therefore, to compress the stretched amplified pulse, a fairly long and complex compressor is required. Furthermore, in stretching and compressing the pulse, bulk optic components are typically required, preventing an all-fibre approach. This is difficult to make robust and involves significant loss which necessitates another stage of amplification in the MOPA. Furthermore, after amplification and fibre delivery, the compression stage also involves significant optical loss and, due to the relatively long pulse duration, the compressor itself is very large, meaning that the optical head itself has a large footprint. In general, the approach of CPA is not ideal and is also difficult to maintain in a compact, robust and lightweight form especially in a harsh operating environment.
According to an aspect of the present invention there is provided a high power short optical pulse source comprising:
The optical signal source preferably comprises a master oscillator optically coupled to an optical fibre preamplifier, comprising a preamplifier amplifier optical fibre and one or more preamplifier optical pump sources. The preamplifier amplifier optical fibre preferably comprises a rare-earth doped optical fibre. The optical signal source is preferably provided at the first location. Alternatively, the master oscillator and the preamplifier amplifier optical fibre may be provided at a third location, intermediate the first and second locations, with the or each preamplifier optical pump source being provided at the first location and being coupled to the preamplifier amplifier optical fibre via a corresponding one or more preamplifier pump delivery fibres.
A plurality of optical pump light sources may be provided at the first location and a corresponding plurality of pump light delivery fibres.
The high power optical fibre amplifier means preferably comprises an amplifier optical fibre and one or more pump signal combiners. The amplifier optical fibre preferably comprises a rare-earth doped optical fibre, and is most preferably of the same type of rare-earth doped optical fibre as the preamplifier amplifier optical fibre.
The high power short optical pulse source may comprise a plurality of high power optical fibre amplifier means optically coupled in series, at least the optical output of the final high power optical fibre amplifier means being located within the optical head.
The or each amplifier optical fibre is preferably located within the optical head. The or each pump signal combiner may be located within the optical head. The or each pump signal combiner may alternatively be located at the first location, with the high power optical fibre amplifier means additionally comprising a pump signal delivery fibre optically coupled between the or each pump signal combiner and the or each amplifier optical fibre. The or each pump signal delivery fibre is preferably a double-clad optical fibre and is most preferably a polarisation maintaining optical fibre.
Alternatively, the amplifier optical fibre may be arranged to extend from the first location to the optical head. The amplifier optical fibre preferably comprises a double-clad amplifier optical fibre. The or a pump signal combiner may be provided at the first location, arranged to couple optical pulses and pump light into one end of the amplifier optical fibre. Alternatively or additionally, the or a pump signal combiner may be provided within the optical head, arranged to couple pump light into the signal output end of the amplifier optical fibre.
The optical head preferably further comprises an optical isolator and optical collimator assembly optically coupled to the output of the high power optical fibre amplifier means.
The high power optical fibre amplifier means may further comprise a bulk optic amplifier element, most preferably a rod amplifier, optically coupled to the output end of the or the final amplifier optical fibre, said amplifier optical fibre being under-length such that a proportion of any pump light coupled into said amplifier optical fibre is unabsorbed by it, and serves to pump the bulk optic amplifier element.
The high power short optical pulse source may further comprise nonlinear optical frequency conversion means optically coupled to the output of the or the final high power optical fibre amplifier means. The nonlinear optical frequency conversion means preferably comprises a nonlinear optical crystal. The nonlinear optical frequency conversion means may comprise a plurality of nonlinear optical crystals arranged optically in series. The nonlinear optical frequency conversion means may alternatively comprise a nonlinear optical fibre.
The high power short optical pulse source may alternatively or additionally comprise an optical pulse compressor optically coupled to the output of the or the final high power optical fibre amplifier means or the nonlinear optical frequency conversion means. The optical pulse compressor may comprise a transmission grating pair or photonic crystal fibre having anomalous dispersion at the signal wavelength.
The high power short optical pulse source may further comprise a pulse picker operable to reduce the optical pulse frequency. The pulse picker preferably comprises an optical gate, such as an acousto-optic modulator, driven at a synchronised gating frequency lower than the optical pulse frequency output from the optical signal source.
The high power short optical pulse source may further comprise optical monitoring means within the optical head.
The optical head may be movably mounted to enable accurate direction of generated high power short optical pulses onto a target or specimen under test. The optical head is preferably mounted on a translation stage or a mechanical manipulator, such as a robotic arm.
Embodiments of the invention will now be described in detail, by way of example only, with reference to the accompanying drawings, in which:
First Embodiment
Referring to
The master oscillator 12 comprises a modelocked fibre oscillator operable to output 10 ps pulses at a pulse frequency of 200 MHz. The preamplifier 14 amplifies the pulse average power to approximately 100 mW.
In this example, the master oscillator 12, preamplifier 14, and pump laser 16, together with their associated drive and control electronics, and cooling systems (not shown), are provided within a first enclosure 28 at a first location. Additional optical isolators 30, 32 are provided after the master oscillator 12 and the preamplifier 14 to protect them from back reflections.
The high power fibre amplifier means 20 comprises a 1 m long single-mode, polarisation maintaining, large mode area Ytterbium doped amplifier fibre and a pump signal combiner having a large mode area signal fibre. The high power fibre amplifier means 20 and the high power optical isolator 26 are provided within the optical head 18, which is located at a second location, remote from the first location.
The short, relatively low power optical pulses output from the preamplifier 14 are delivered to the pump signal combiner of the high power fibre amplifier means 20 via the optical signal delivery fibre 22, which comprises a 5 m long polarisation maintaining, single-mode optical fibre; the use of polarisation maintaining fibre prevents any environmental effects disturbing the signal.
The pump light source 16 comprises a fibre pig-tailed multi-emitter pump source operable to generate cw pump light at a wavelength of 915 nm, and an optical power of between 20 W and 40 W.
The pump light is delivered to the pump signal combiner of the high power optical fibre amplifier means 20 through the pump delivery fibre 24, which in this example is a 5 m length of optical fibre having a 105 μm diameter core and a numerical aperture of 0.22. The pump delivery fibre 24 is not sensitive to environmental effects but can, along with signal delivery fibre, be protected within an armoured jacket for industrial applications.
The high power optical fibre amplifier means 20 amplifies the received optical pulses to an average power of approximately 20 W, resulting in a pulse peak power of approximately 10 kW. The overall low nonlinearity of the high power optical pulse source 10 ensures that spectral broadening of the optical pulses is minimised, and the pulses have a final spectral bandwidth of less than 0.5 nm.
The optical head 18, containing the high power optical fibre amplifier means 20 and the isolator 26, has a small footprint and can be positioned at the intended target of the optical pulses. The large, noisy elements of the high power short optical pulse source 10 are thereby provided away from the application site of the pulses, and only the smaller optical head need be located near the intended target.
Second Embodiment
In this embodiment, a second pump light source 42 is provided at the first location, within the first enclosure. A second pump light delivery fibre 44 is also provided and delivers pump light from the second pump light source 42 to the pump signal combiner of the high power optical fibre amplifier means 20.
It will be appreciated that the high power optical fibre amplifier means 20 may alternatively comprise a two-stage amplifier having a series of two amplifier fibres and pump signal combiners, with an isolator provided between amplifier stages as necessary. Each pump signal source 16, 42 would then pump a separate amplifier stage, the amplifier stages being cascaded to provide increasing signal with balanced gain throughout the cascade.
In most applications, the high power optical fibre amplifier means 20 will only require a single amplifier fibre. However, the number of amplifier fibres (and thus the number of pump light sources) will at least in part be determined by the power of the optical pulses output from the preamplifier 14, the length of signal delivery fibre 22, and the permitted amount of nonlinear effects as determined by the application of the high power short optical pulse source 10.
Third Embodiment
A high power short optical pulse source 50 according to a third embodiment of the invention is shown in
In this embodiment, the pump signal combiner 52 of the high power optical fibre amplifier means 20 is provided at the first location, within the first enclosure 28. The pump delivery fibres 24, 44 and the signal delivery fibre 22 are also wholly contained within the first enclosure 28.
The high power optical fibre amplifier means 20 of this embodiment further comprises a pump signal delivery fibre 54, which comprises the output fibre of the pump signal combiner 52. The pump signal delivery fibre 54 is a polarisation maintaining double clad optical fibre which has a signal-guiding core region and an inner cladding which guides the pump light from the pump sources 16, 42.
The pump signal delivery fibre 54 extends from the pump signal combiner 52, within the first enclosure 28, to the amplifier fibre 56, within the optical head 18. The amplifier fibre 56 is therefore pumped in the co-propagating regime.
Fourth Embodiment
In this embodiment, the amplifier fibre 62 comprises a polarisation maintaining double clad amplifier fibre and extends between the pump signal combiner 52 and the optical head 18. The input end of the amplifier fibre 62 is coupled to the output of the pump signal combiner 52 and the output end of the amplifier fibre 62 is located in the optical head 18, where it is coupled to an optical isolator and collimating optics 64. The amplifier fibre 62 therefore provides the dual functions of pulse amplification and pulse delivery to the optical head 18.
Since fibre amplifiers are not 100% efficient (typically 50 to 75% efficiency is achievable), the amplifier fibre 62 will get warm during use. Heat dissipation may be achieved by using an armoured cable to protect the amplifier fibre 62; the void around the amplifier fibre 62 being filled with a suitable heat transfer fluid or paste to ensure good thermal contact between the amplifier fibre 62 and the cable inner surface.
Fifth Embodiment
A high power short optical pulse source 70 according to a fifth embodiment of the invention is shown in
In this example, the pump signal combiner 52 is provided in the optical head 18, so that a counter-propagating pump regime is used. The pump delivery fibres 24, 44 extend from the pump sources 16, 42 in the first enclosure to the pump signal combiner 52 in the optical head 18.
Sixth Embodiment
A high power short optical pulse source 80 according to a sixth embodiment of the invention is shown in
In this example, the amplifier fibre 62 is made to be “under-length”, such that quite a large portion of the pump light delivered to the amplifier fibre is not absorbed within the amplifier fibre, but propagates through to the fibre output, along with the signal pulses. The high power optical fibre amplifier means 20 further comprises a rod amplifier 82, in the form of a Yttrium Aluminium Garnet (YAG) crystal rod, optically coupled to the output of the amplifier fibre 62, to form a hybrid amplifier device. The YAG crystal rod 82 performs a second stage of amplification of the short optical pulses, in a very short piece of material, using the unabsorbed pump light to pump the YAG crystal rod 82. The YAG crystal rod 82 can provide an additional gain of a few dB's while providing very little nonlinear distortion to the signal pulses. The gain of the YAG crystal rod 82 is determined by the efficiency of the crystal, the divergence of pump light and the signal pulses, and the overlap of the pump light and the signal pulses through the YAG crystal rod 82.
In order to prevent optical feedback from the YAG crystal 82 into the amplifier fibre 62, both the output end of the amplifier fibre 62 and the YAG crystal rod 82 are coated with anti-reflection coatings. Alternatively, the amplifier fibre 62 and the YAG crystal rod can be fused together.
It will be appreciated that a rod amplifier such as the YAG crystal rod 82 may also be used with any of the embodiments described above.
Seventh Embodiment
In this example the high power short optical pulse source 90 further comprises nonlinear optical frequency conversion means 92, optically coupled to the output of the high power optical fibre amplifier means 20 and located within the optical head 18.
The nonlinear optical frequency conversion means 92 comprises (optically coupled in series) a set of phase plates 94, a first nonlinear crystal 96, which in this example is a Type I LBO crystal, a second nonlinear crystal 98, which in this example is a Type I BBO crystal, and a harmonic separator 100.
The output optical pulses from the high power optical fibre amplifier means 20, having a wavelength of 1064 nm and an average power of approximately 20 W, pass through the phase plates 94, to set the optimum state of polarisation for the nonlinear frequency conversion. The pulses are then launched, using conventional collimation and focusing optics, into the LBO crystal 96, to convert the wavelength of the pulses to their second harmonic of 532 nm, at an average power of 12 W.
The frequency converted pulses output from the LBO crystal 96 are then launched into the BBO crystal 98, where the wavelength is converted to their fourth harmonic wavelength of 266 nm, at an average power of 1.2 W. The output from the BBO crystal 98 is then passed through the harmonic separator 100, which transmits only the desired wavelength, in this case 266 nm, as the output of the high power short optical pulse source 90 to the intended target.
The LBO and BBO crystals 96, 98 are respectively mounted within ovens, controlled by a temperature controller 102. Electrical power for the ovens and the temperature controller 102, and to a cooling fan (not shown) for the high power optical fibre amplifier means 20 is delivered to the optical head 18 through a power cable 104.
It will be appreciated that the nonlinear optical frequency conversion means 92 could alternatively use other combinations of crystals to generate 3.sup.rd, 4.sup.th or higher harmonics, for example periodically poled nonlinear crystals such as periodically poled lithium niobate (PPLN) or periodically poled potassium titanyl phosphate (PPKTP), or could use other combinations of conventional crystals such as LBO, BBO, BiB3O6(BIBO), cesium lithium borate (CLBO), and potassium titanyl phosphate (KTP).
For efficient frequency conversion the spectral bandwidth of the pulses must be maintained as narrow as possible. By transmitting the optical pulses through the greatest length of fibre before amplifying the pulses close to the nonlinear optical conversion means 92, the high power short optical pulse source 90 ensures that spectral distortion of the pulses is minimised and nonlinear optical conversion efficiency is thereby maximised.
The high power short optical pulse source 90 can therefore deliver UV light directly to an intended target whilst remotely positioning the bulky elements of the source 90 away from the intended target.
It will be appreciated that the nonlinear optical frequency conversion means 92 may be is included in any of the high power short optical pulse sources according to the previously described embodiments.
Eighth Embodiment
A high power short optical pulse source 110 according to an eighth embodiment of the invention is shown in
The optical pulse source 110 further comprises a pulse compressor 112 provided within the optical head 18 and optically coupled to the output of the high power optical fibre amplifier means 20.
In this example the pulse compressor takes the form of a transmission grating pair 112 having a grating separation of less than 10 cm. The pulse compressor 112 could alternatively comprise a fibre pulse compressor based on Photonic Crystal Fibre with anomalous dispersion at the signal wavelength.
The master oscillator 12 generates optical pulses having a duration of approximately 10 ps at a pulse frequency of 10 MHz. The pulses are then amplified by the optical fibre preamplifier 14 to an optical power of approximately 50 mW. The signal pulses and 20 W 975 nm pump light from the pump light source 16 single are delivered over the signal delivery fibre 22 and the pump delivery fibre 24 respectively, each of which are 2 m long in this example, to large mode area, polarisation maintaining, single-mode Ytterbium doped amplifier fibre within the high power optical fibre amplifier means 20. The high power optical fibre amplifier means 20 amplifies the average pulse power to approximately 12 W, resulting in a pulse energy of greater than 1 μJ.
During amplification within the high power optical fibre amplifier means, the pulses (which enter the high power optical fibre amplifier means with a duration of approximately 10 ps) becomes linearly chirped due to the combination of positive fibre dispersion and self-phase modulation.
The amplified pulses are then passed through the transmission grating pair 112, which acts to compress the pulses to less than 500 femtoseconds duration, with an efficiency of greater than 80%, to produce pulses having an energy of approximately 10 and peak powers of 2 MW. The high power ultrashort pulses can then be delivered from the head 18 which can be positioned directly at the intended target without the need for complex beam steering optics.
It will be appreciated that a pulse compressor 112 may be incorporated into any of the above described high power short optical pulse sources in order to generate ultrashort, femtosecond pulses.
Ninth Embodiment
In this embodiment the pump light sources 16, 42 are provided within the first enclosure 28, at the first location, together with the pump sources 122, 124 for the preamplifier 14, and their associated electrical drive circuitry, cooling and heat dissipation elements (not shown). The high power optical fibre amplifier means 20 and the optical isolator 26 are provided within the optical head 18, at a second location, remote from the first location.
The master oscillator 12 and the amplifier fibre and pump signal combiner of the optical fibre preamplifier 14, together with their associated isolators 30, 32, are provided within a second enclosure 126, at a third location intermediate the first and second locations, 126. The outputs of the preamplifier pump sources 122, 124 are delivered to the amplifier fibre of the optical fibre preamplifier 14 respectively via preamplifier pump delivery fibres 128, 130.
The master oscillator 12, preamplifier 14, and high power optical fibre amplifier means 20 can thus be enclosed in one or more separate enclosures positioned close to the application target area thus avoiding the need for beam steering optics.
It will be appreciated that this arrangement can also be applied to any of the previously described embodiments, including those with nonlinear frequency conversion and pulse compression.
Tenth Embodiment
The pulse source 140 further comprises a pulse picker 142 operable to reduce the optical pulse frequency. In this example the pulse picker 142 comprises an acousto-optic modulator driven at a synchronised gating frequency lower than the optical pulse frequency output from the master oscillator 12. The pulse picker 142 is provided after the preamplifier 14, within the first enclosure 28. The pulse picker 142 is located at a position within the pulse source 140 where the optical pulses have a low pulse energy. This is because the optical insertion loss into the acousto-optical modulator pulse picker 142 is high, so it is preferable for the pulses to be transmitted through the pulse picker 142 prior to amplifying them to their final high power. The provision of a pulse picker also enables higher pulse energies to be achieved for a given average output power.
It will be appreciated that a pulse picker 142 may be provided within any of the above described pulse sources, and that where the pulse source comprises high power optical fibre amplifier means having two or more amplifier stages the pulse picker may be provided after any one of the amplifier stages between the master oscillator the final high power amplifier stage.
Eleventh Embodiment
A high power short optical pulse source 50 according to an eleventh embodiment of the invention is shown in
It will be appreciated that the optical heads 18 of any of the previously described embodiments may be similarly movably mounted.
Various modifications may be made to the described embodiments without departing from the scope of the invention.
It will be appreciated that the master oscillator could alternatively comprise any optical source operable to generate short optical pulses, such as a solid-state modelocked laser, for example a Neodynium Vanadate laser, or a gain-switched laser diode. The amplifier fibres of the preamplifier and the high power optical fibre amplifier means may alternatively be doped with a different rare-earth dopant, such as Erbium, Thulium, or Neodynium.
In most applications, the pump source/s will be a multi-mode pump source operating at a suitable wavelength to pump the rare-earth-doped amplifier fibre (eg 808 nm, 915 nm or 975 nm). For example, a single fibre-pigtailed laser diode, diode bar or multi-emitter pump source such as the PUMA source commercially supplied by Fianium Ltd, which delivers between 20 and 40 W within a single, 105 μm core, 0.22 NA pump delivery fibre.
Where multi-mode pump delivery fibres are used, the pump signal combiner will typically include a conventional tapered bundle, such as those commercially available from OFS or Sifam Fibre Optics. Alternatively, the pump signal combiner may be a tapered coupler, a side-pumping fibre configuration, or a distributed pump coupling fibre configuration such as that proposed in U.S. Pat. No. 6,826,335. In the multi-mode pumping regime, the amplifier fibre typically comprises a double-clad fibre structure where the signal pulses are guided within a signal core and the pump light is guided within the fibre cladding.
Alternatively, the pump source/s can be a single mode pump source such as a fibre-pigtailed laser diode or a fibre laser. The fibre laser can be a Raman fibre laser or could be a cladding pumped fibre laser generating cw or pulsed radiation at the wavelength required to pump the rare-earth-doped amplifier fibre. In the single-mode pump regime, the signal pulses and pump light from the one or more pump sources are combined using conventional wavelength-division multiplexing (WDM) components such as fused WDM couplers or thin-film WDM couplers.
In the single-mode pump regime, the amplifier fibre has a conventional single clad geometry, where both the signal pulses and the pump light propagate within the core of the amplifier fibre. This has benefits in increasing the pump absorption and thus reducing amplifier length and hence nonlinearity.
The optical head of any of the high power short optical pulse sources described may also include a heat sink and integrated fan within the high power optical fibre amplifier means, to provide forced-air cooling of the amplifier fibre. Optical monitoring means may also be provided within the optical head, with both electrical and optical communication to the first enclosure to monitor feedback and power levels, enabling interlocks and automatic fault detection.
The described embodiments provide various advantages, as follows.
The high power short optical pulse sources enable a short-length fibre amplifier system and post processing optics to be remotely located from the bulky, noisy heat producing elements of the pulse source, and thereby enable optical head to be very compact. The optical head can therefore be positioned close to the application space, taking up minimal space and avoiding the need for complex and expensive beam steering optics.
The high power short optical pulse sources enable the delivery of ultrashort (femtosecond) optical pulses with high energy and narrow spectral bandwidth, without the use of complex chirped pulse amplification (CPA) methods. In short optical pulse amplifier systems which don't incorporate CPA methods, it is essential that all fibre lengths which deliver or amplify pulses to high peak powers, are kept as short as physically possible; the structure and configuration of the high power short optical pulse sources ensures that this is achieved.
The high power short optical pulse sources incorporating a pulse compressor eliminate the need for CPA in fibre-delivered laser sources. Providing a high power ultrashort pulse source which is more robust, lower cost and easier to maintain and assemble than known ultrashort pulse sources using CPA pulse compression.
The high power short optical pulse sources further enable the delivery of UV optical pulses, efficiently generated within the optical head.
The high power short optical pulse sources also provide the advantage of beam delivery directly to the target without the use of complex beam steering optics. The high power short optical pulse sources therefore offer improved mechanical robustness, reduced cost and weight, and ease of maintenance over known high power optical pulse sources.
The high power short optical pulse sources also allow for scalability in power because they can incorporate multiple pump light sources in the remote pump enclosure and the pump delivered over long lengths with very low loss to the amplifier system which is remotely located whether within or close to the output optical head.
It will be apparent to those skilled in the art that various modifications and variations can be made to the present invention without departing from the spirit and scope of the invention. Thus, it is intended that the present invention cover the modifications and variations of this invention provided they come within the scope of the appended claims and their equivalents.
Number | Date | Country | Kind |
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0601154.8 | Jan 2006 | GB | national |
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PCT/GB2007/000136 | 1/18/2007 | WO | 00 | 1/16/2009 |
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WO2007/083110 | 7/26/2007 | WO | A |
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Communication from the EPO examination division: Communication Pursuant to Article 94(3) EPC 07 700 401.8-2216, (EP1979997) Aug. 6, 2010 (2 pages). |
Annex to the communication from the EPO examination division, Communication Pursuant to Article 94(3) EPC 07 700 401.8-2216, (EP1979997) Aug. 6, 2010 (2 pages). |
Reply to EPO Communication Pursuant to Article 94(3) EPC 07 700 401.8-2216, (EP1979997) Aug. 6, 2010 (5 pages). |
Amended claims with annotations submitted with Reply to EPO communication Pursuant to Article 94(3) EPC 07 700 401.8-2216, (EP1979997) Aug. 6, 2010 (4 pages). |
Amended specification submitted with Reply to EPO communication Pursuant to Article 94(3) EPC 07 700 401.8-2216, (EP1979997) Aug. 6, 2010 (1 page). |
Communication from the EPO examination division: Communication Pursuant to Article 94(3) EPC 07 700 401.8-2217, (EP1979997) dated Feb. 22, 2012 (6 pages). |
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20100157419 A1 | Jun 2010 | US |