MOPA laser apparatus with two master oscillators for generating ultraviolet radiation

Abstract

Laser apparatus including two different, pulsed MOPAs, one having a fundamental wavelength of 1064 nm and the other having a fundamental wavelength of 2114 nm, provide trains of optical pulses. The 1064-nm pulses are frequency-quintupled to a wavelength of 213 nm. The 2114-nm pulses are mixed with the 213-nm pulses to provide pulses having a wavelength of 193 nm. Each MOPA includes a fiber-laser and a bulk amplifier.

Description

BRIEF DESCRIPTION OF THE DRAWINGS

The accompanying drawings, which are incorporated in and constitute a part of the specification, schematically illustrate a preferred embodiment of the present invention, and together with the general description given above and the detailed description of the preferred embodiment given below, serve to explain the principles of the present invention.

FIG. 1 schematically illustrates one preferred embodiment of apparatus in accordance with the present invention including first and second optical fiber, master-oscillator power-amplifiers (MOPAs) generating laser radiation pulses at respectively first and second fundamental wavelengths, the MOPAs being slaved to a master clock via a phase shifter, and the apparatus further including four optically nonlinear crystals, a first and second of the optically nonlinear crystals generating the fourth-harmonic of the first fundamental wavelength, a third of the optically nonlinear crystals mixing the fourth harmonic of the first fundamental wavelength with the second fundamental wavelength to provide an intermediate UV wavelength and residual second-fundamental-wavelength radiation, and a fourth of the optically nonlinear crystals mixing the intermediate UV wavelength with the residual second-fundamental-wavelength radiation to provide output pulses of UV radiation having a wavelength less than 200 nm.

FIG. 2 schematically illustrates another preferred embodiment of apparatus in accordance with the present invention, similar to the apparatus of FIG. 1, wherein the first MOPA has an output wavelength of 1064 nm, the second MOPA has an output wavelength of 1547 nm, and the UV output pulses have a wavelength of about 198 nm.

FIG. 3 is a block diagram schematically illustrating computed power of intermediate wavelengths after each conversion stage, and power of 198-nm output radiation in one example of the apparatus of FIG. 2.

FIG. 4 is a contour graph schematically illustrating computed output radiation power as a function of average fundamental power of the first and second MOPAs in the example of FIG. 2.

FIG. 5 is a contour graph schematically illustrating computed output radiation power as a function of average fundamental power in a prior-art arrangement for generating 198-nm radiation for 1064-nm radiation and 1568-nm radiation.

FIG. 6 is a graph schematically illustrating computed conversion efficiency as a function of 198-nm average output power in one example of the apparatus of FIG. 2.

FIG. 7 schematically illustrates yet another preferred embodiment of apparatus in accordance with the present invention, similar to the apparatus of FIG. 1, but wherein the first MOPA has an output wavelength of 1031 nm, the second MOPA has an output wavelength of 1547 nm, and the UV output pulses have a wavelength of about 193 nm.

FIG. 8 is a block diagram schematically illustrating computed average power of intermediate wavelengths after each conversion stage, and power of 193-nm output radiation in one example of the apparatus of FIG. 7.

FIG. 9 is a contour graph showing computed average output radiation power as a function of average fundamental power of the first and second MOPAs in the example of FIG. 8.

FIG. 10 schematically illustrates details of one preferred example of the first MOPA in the apparatus of FIG. 2.

FIG. 11 schematically illustrates details of one preferred example of an amplified fiber laser suitable for use as the second MOPA in the apparatus of FIG. 2 or the apparatus of FIG. 7.

FIG. 12 schematically illustrates still another preferred embodiment of apparatus in accordance with the present invention, similar to the apparatus of FIG. 2, but wherein the first, second and third optically nonlinear crystals generate the fifth-harmonic of the first fundamental wavelength, the second MOPA has an output wavelength of 2114 nm, and UV output pulses are created by mixing the fifth harmonic of the first fundamental wavelength with the second fundamental wavelength and have a wavelength of about 193 nm.

DETAILED DESCRIPTION OF THE INVENTION

Referring now to the drawings, wherein like components are designated by like reference numerals, FIG. 1 schematically illustrates one preferred embodiment 20 of laser apparatus in accordance with the present invention. In the drawing, optical beam paths are depicted by fine lines, with open arrowheads indicating propagation direction. Electrical or electronic connections are depicted in bold line, with the communication direction indicated by closed arrowheads.

Apparatus 20 includes generic fiber laser MOPAs 22 and 28. MOPA 22 includes a fiber master oscillator 24 (seed-laser) providing fundamental radiation at a wavelength between about 1000 and 1099 nm (designated in FIG. 1 and referred to hereinafter as 10XX nm radiation). This wavelength range is the most common range of operation in ytterbium-doped and neodymium-doped fiber amplifiers. This range can, however, extend to about 1150 nm for a long wavelength limit and to about 975 nm for a short wavelength limit.

The oscillator is preferably operated in a continuous-wave (CW) mode with the CW output being modulated, preferably by a modulator such as an integrated Mach-Zehnder (MZ) modulator. At the 10XX nm wavelength, it may be found advantageous to employ two such modulators in series to ensure an acceptable contrast ratio. Laser 24 can also be a fiber laser, distributed feedback (DFB) or distributed Bragg reflector (DBR) diode laser, an extended cavity diode laser (with a wavelength stabilizing fiber Bragg grating in close proximity to the diode), or a solid-state laser. For most of the above-mentioned lasers a wavelength locking mechanism is provided by an integrated grating structure in the cavity. If a precise control of a central wavelength is required then an external wavelength locker (38) can be used. In that case, a portion of the CW radiation is directed to a wavelength locker 38 that maintains a predetermined operating wavelength of the laser. Pulses output by the modulated fiber laser are amplified by a bulk (solid-state) amplifier 26. Laser 24 may also be provided with a fiber pre-amplification stage. This is discussed in detail further hereinbelow. As fiber lasers, fiber amplifiers, wavelength lockers and MZ modulators are well known in the art to which the present invention pertains, and a detailed description thereof is not necessary for understanding principles of the present invention, such a detailed description is not presented herein.

MOPA 28 is arranged similar to MOPA 22. A fiber laser 30 of MOPA 28 includes an Er-doped gain fiber. Laser 30 is operated in the same manner as laser 24 of MOPA 22 and, in this example, provides laser pulses having a wavelength between about 1500 nm and 1599 nm (designated in FIG. 1 and referred to hereinafter as 15XX nm radiation) to an optical fiber amplifier 32, such as a large mode area (LMA) erbium and ytterbium-doped (Er:Yb:LMA) fiber amplifier. Laser 30 is preferably a single-frequency fiber laser. However, laser 30 may also be a DFB or DBR diode-laser, an extended-cavity diode-laser, or a solid-state laser. Single-frequency diode-lasers emitting in the range between about 1510 nm and about 1599 nm are available at any predetermined wavelength close to a standard grid of telecommunication wavelengths. If a precise control of a central wavelength is required, an external wavelength locker 40 and tuner 42 can be used. In that case, a portion of the CW radiation is directed to a wavelength locker 40, which maintains a predetermined operating wavelength of the laser. A tuner 42 provides that the locked wavelength is adjustable within the tuning range of the Er-doped gain fiber. As several tuning schemes for Er-doped fiber lasers are well-known in the art, and as a knowledge of such schemes is not necessary for understanding principles of the present invention, a detailed description of any one of the schemes is not presented herein.

Pulse delivery by MOPAs 22 and 28 is controlled by a controller 37 cooperative with a 5-MHz oscillator 34, a phase shifter 36, and the integral MZ modulators (not explicitly shown) of the master oscillators. A radio frequency (RF), here, 5 MHz, signal voltage from oscillator 34 is delivered to one electrode of the MZ modulator (or modulators) of master oscillator 24 and via phase shifter 36 to one electrode of the MZ modulator of master oscillator 30. Controller 37 provides digital signals to another electrode of the MZ modulators of the master oscillators for keying the MZ modulators. Each master oscillator delivers a train of pulses at a pulse repetition frequency (PRF) that is determined by the frequency of oscillator 34, and with a pulse duration that is determined by the keying signals applied to the MZ modulators. The phase difference between the two pulse trains is controlled by controller 37, in cooperation with phase shifter 34, using standard phase-shift-keying (PSK) techniques. MOPAs as described here will deliver pulses at a PRF in the megahertz range with pulse durations of less than 5 ns and even less than 1 ns.

It should be noted, here, that while the above described modulation scheme is a preferred modulation scheme, other modulation schemes may be employed without departing from the spirit and scope of the present invention. By way of example, master oscillators 24 and 30 may be directly modulated by modulating the optical pump source of the lasers. Whatever modulation scheme is employed, however, there must be some provision for adjusting the relative phase of pulse trains emitted by the lasers.

Provision of phase control is important in apparatus 20, as frequency-converted pulses from each MOPA are required to be further frequency converted by at least one optically nonlinear crystal, common to both. The fiber length in each MOPA amplifier will almost certainly be different. Beam paths followed delivery of pulses from each MOPA to a common crystal will also almost certainly be different. This being the case, and given that a 1-ns pulse has an optical path length in air of only about 30 centimeters (cm), phase control between the pulse trains generated by the MOPAs must be provided to ensure that the corresponding frequency converted pulses arrive simultaneously (temporally overlapping) at the common optically nonlinear crystal, thereby allowing further frequency conversion to take place. Phase control can be automatically implemented by detecting the mixing product output of any common optically nonlinear crystal, and communicating this output to controller 37. Controller 37 can then command phase shifter 36 to adjust the relative phase of the MOPAs until the detected mixing product is maximized. This phase control also enables a method of either digitally modulating or amplitude modulating UV output pulses of the apparatus.

Continuing with reference to FIG. 1, in a preferred frequency-conversion architecture for pulses delivered by MOPAs 22 and 28, amplified 10XX-nm pulses from fiber amplifier 26 follow a path B₁ to an optically nonlinear crystal 44, which is arranged to generate the second harmonic (2HG) of the pulse wavelength. In this preferred conversion architecture, crystal 44 is a lithium borate (LBO) crystal, preferably between about 10 millimeters (mm) and 20 mm long, and arranged for non-critical phase matching. 2H-radiation pulses generated by crystal 44 and having a wavelength of about 5XX nm (half the 10XX wavelength) are again frequency doubled in another optically nonlinear crystal 46 to generate fourth-harmonic (4H) pulses having a wavelength of about 2XX nm (half the 5XX wavelength). Crystal 46 is preferably a cesium lithium borate (CLBO) crystal preferably between about 5 mm and 15 mm long, and also arranged for non-critical phase matching.

Amplified 15XX-nm pulses from fiber amplifier 32 follow a path B₂. The 2XX-nm pulses from crystal 46 proceed along path B₁ and are incident on a face 52A of an optically nonlinear crystal 52. Crystal 52 is preferably a CLBO crystal between about 10 mm and about 15 mm long, and is cut and arranged such that the 2XX-nm radiation is incident at Brewster's angle for the crystal material at that wavelength. Path B₂ is folded by mirrors 54 and 56 such that 15XX-nm pulses traveling therealong are incident on face 52A of crystal 52 at an angle close to Brewster's angle for the crystal material at the 15XX-nm wavelength, such that the 15XX-nm radiation propagates substantially collinear with the 2XX-nm radiation within crystal 52. This means, for a CLBO crystal, that there will be an angle of about 1.6 degrees between paths B₁ and B₂ at face 52A of the crystal. Crystal 52, in this example is arranged for Type-I phase-matching for the 2XX-nm and 15XX-nm wavelengths and generates radiation pulses having a wavelength of about 2YY-nm (where 2YY is less than 2XX) by sum-frequency mixing, provided, of course, the above-described phase control between the MOPAs is adjusted such that the 2XX-nm and 15XX-nm radiation arrive simultaneously at crystal 52.

The 2YY-nm radiation pulses exit crystal 52 via face 52B thereof along a path B₄. A beam sampler 72, for example, a tilted, uncoated calcium fluoride (CaF₂) plate, directs a portion (for example, less than 1%) of the output of crystal 52 to a high speed UV photodiode 74. The output of photodiode 74 is transmitted to controller 37 for phase control implementation as discussed above. The remaining portion of the 2YY-nm pulses are incident on a face 58A of an optically nonlinear crystal 58. Crystal 58 is also preferably a CLBO crystal, about 15 mm long, and cut and arranged for Type-I phase matching for the 2YY-nm wavelength and residual 15XX radiation. Path B₂, along which residual 15XX-nm radiation pulses are propagating, is folded by mirrors 60 and 62 such that the 15XX-nm radiation pulses are incident on face 58A of crystal 58 at an angle close to Brewster's angle for the crystal material at the 1064-nm wavelength, such that the 2YY-nm radiation propagates substantially collinear with the 15XX-nm radiation inside crystal 58. For a CLBO crystal, there will be an angle of about 4.5 degrees between paths B₃ and B₄ at face 58A of crystal 58. Crystal 58 generates 19X-nm radiation (output) pulses by sum-frequency mixing the 2YY-nm and residual 15XX-nm input pulses. Care must be taken to match the optical length of paths B₂ and B₄ between crystal 52 and crystal 58 such that the desired phase relationship of the 15XX-nm and 2YY-nm pulses is maintained at crystal 58. The 19X-nm output pulses exit crystal 58 via face 58B thereof along a beam path B₅. Any residual (longer) wavelength pulses exiting crystal 58 will be propagating at some angle to path B₅ and can be separated from the 19X-nm pulses by spatial filtering.

It is important that output pulses from MOPA 22 have about the same temporal pulse width as output pulses from MOPA 28. This is because sum-frequency mixing can only occur when both radiations are co-propagating in the optically nonlinear crystals in which the mixing is taking place. In apparatus 20, the MZ modulator arrangement in MOPAs provides a means of accurately selecting and controlling temporal pulse widths.

It should be noted here that while CLBO is a particularly preferred crystal material for crystal 58, there is another crystal material, potassium aluminum borate (KABO) that may also be more or less useful, depending on the particular wavelengths that are to be finally mixed. The material has a phase-matching limit that extends to shorter fundamental wavelengths than that of CLBO, has a transparency comparable to CLBO and has a nonlinear coefficient that is between about 0.2 pM/V and 0.45 pM/V. This material, however, has not yet been commercially developed. Other possible crystal materials are potassium beryllium barium fluoride (KBBF), and yttrium aluminum borate (YAB), which also in the early stages of commercial development.

Those skilled in the art will recognize without further illustration that instead of using residual 15XX-nm radiation for the sum frequency mixing in crystal 58, it is possible to divide the 15XX radiation output of MOPA 28 two portions using a beamsplitter or the like, then use one portion for sum frequency mixing in crystal 52 and the other portion for sum frequency mixing in crystal 58. This, is not as efficient however as the sum frequency mixing arrangement using residual 15XX radiation described above with reference to FIG. 1.

It should be noted here that a major shortcoming of 15xx-nm Er:Yb-doped fiber amplifiers is a low conversion efficiency (of pump power to output power), for example, between about 25% and 35%. By way of comparison Yb-doped fiber amplifiers for 10XX-nm amplification have a conversion efficiency between about 50% and 80%. Because of this, an increase of output power from an Er:Yb fiber amplifier by a factor of two will require at least between about 2 and 3 times more pump power than would be required to provide the same increase in a Yb-doped fiber amplifier. Further, existing bulk amplifiers at 1510-1590 nm, wherein gain media are typically Er:Yb glasses, have poor thermal properties and power scaling compared to those of bulk amplifiers for 10xx-nm, which typically employ crystal gain media. Accordingly, power up-scaling at 15xx-nm, while preserving a narrow linewidth of optical radiation, is more difficult and expensive power up-scaling at 10XX nm.

Apparatus 20 has certain advantages over prior-art apparatus in that by employing two lasers, the power required to be produced by the 15XX-nm laser is reduced compared with above discussed schemes in which only an Er-doped fiber laser is employed. In the inventive scheme, each laser is operating at a wavelength close to a peak-gain wavelength. The total number of frequency conversion (sum-frequency mixing or harmonic generating) stages for the apparatus is only four. An advantage of the apparatus relating to the frequency conversion architecture thereof is that combining beam paths B₁ and B₂ and beam paths B₂ and B₄ by Brewster's angle incidence at the corresponding crystal faces eliminates a requirement for dichroic mirrors to provide such beam-path combination. At wavelengths less than about 400 nm, even the best commercially available such mirrors are lossy to some extent, and become increasingly lossy the shorter the wavelength. Such mirrors are also subject to degradation by short-wavelength UV radiation.

FIG. 2 schematically illustrates another preferred embodiment 20A of apparatus in accordance with the present invention. Apparatus 20A is similar to above discussed apparatus 20 of FIG. 1 with exceptions as follows. In apparatus 20A, MOPA 22A includes a quasi-CW modulated ytterbium-doped (Yb-doped) amplified fiber laser 102, pulses of which are amplified by a bulk (solid-state) amplifier 27 having a gain-medium of neodymium-doped yttrium vanadate Nd:YVO₄. The term “quasi-CW” here refers to a laser source having a pulsed output at a pulse-repetition frequency (PRF) of about 0.2 MHz or greater. By way of example source, 102 is exemplified in above described apparatus 20A as having a PRF of 5.0 MHz, slaved to master clock 34. MOPA 22A has an output wavelength of 1064 nm. MOPA 28A includes an amplified Er-doped fiber laser 104, pulses of which are amplified by a large mode area (LMA) erbium and ytterbium-doped (Er:Yb:LMA) fiber amplifier 32 as discussed above. MOPA 28A has an output wavelength of 1547 nm. Preferred examples of each of these MOPA arrangements are described in detail further hereinbelow.

FIG. 3 is a block diagram, schematically depicting the computed power of frequency-converted wavelength components at each frequency-conversion stage in an example of the apparatus of FIG. 2 in which the MOPAs are assumed to deliver pulses having a duration of about 1.0 ns at a PRF of 5.0 MHz. MOPA 22A is assumed to have a 1064-nm average power output of 13.5 W. MOPA 28A is assumed to have a 1547-nm average power output of 13.5 W. 198 nm average output power is about 1.03 W. A beam diameter in each crystal of about 80.0 micrometers (μm) is assumed. The crystals are represented by bold-outlined blocks and designated by the same reference numerals as the crystals in FIG. 2.

While FIG. 3 is essentially self explanatory, it is worthwhile to note that relatively little of the 1547-nm power is consumed by the two sum-frequency mixing or sum-frequency generation (SFG) stages. Further, the UV power is reduced by a relatively small percentage on being converted from 266 nm to 198 nm in the SFG stages. This would suggest that scaling output power could be achieved primarily by increasing the 1064-nm power, with correspondingly little increase of 1547-nm power being required. This is confirmed in the graph of FIG. 4, which schematically depicts, in contour graph form, computed 198-nm output power (the contours) as a function of average fundamental power delivered by MOPAs 22A and 28A for pulses having a duration of 1 ns delivered at a frequency of 5.0 MHz. In computing the output power contours, the same assumptions are made that are made in the computations of FIG. 3.

Dashed line E_MAX in the graph of FIG. 4 indicates the combination of 1064-nm power and 1547-nm power that would provide maximum conversion efficiency of total fundamental power at the various power levels. The graph contours indicate that 198-nm output pulses can have 1.0 W of average power for an average 1064-nm power of about 13.3 W, and an average 1547-nm power of about 9.2 W. Similarly, the contours indicate that the 198-nm output pulses can have 10.0 W of average power for an average 1064-nm power of about 39.2 W and an average 1547-nm power of about 15.5 W. This indicates that scaling output power in apparatus of FIG. 2 is achieved primarily by scaling the output power of the 1064 nm laser. By way of comparison, FIG. 5 schematically illustrates computed contour plots for 198 nm output pulses generated from 1064-nm and 1547-nm radiation in one example of prior-art art apparatus described in the above-discussed application Ser. No. 11/387,400. Here, it can be seen that increasing output power requires about equal contributions from each power source.

FIG. 6 is a graph schematically illustrating computed conversion efficiency of total fundamental power as a function of output power, derived from the computations of FIG. 4. Here, the graph indicates that 10 W of 198-nm average output power may be achieved at an efficiency of conversion of the total fundamental output power of the two lasers of about 18% (0.18).

FIG. 7 schematically illustrates another preferred embodiment 20B of apparatus in accordance with the present invention. Apparatus 20B is similar to above discussed apparatus 20 of FIG. 1 with exceptions as follows. In apparatus 20B, MOPA 22B includes a modulated ytterbium-doped (Yb-doped) amplified fiber laser 103 pulses of which are amplified by a bulk (solid-state) amplifier 29, preferably having a gain-medium of ytterbium-doped potassium yttrium tungstate (KY(WO₄)₂ or simply KYW). MOPA 22B has an output wavelength of 1031 nm. MOPA 28B includes an Er-doped fiber laser 104 pulses of which are amplified by a large mode area (LMA) erbium and ytterbium-doped (Er:Yb:LMA) fiber amplifier 32. MOPA 28B has an output wavelength of 1547 nm.

FIG. 8 is a block diagram, schematically depicting the computed power of frequency converted wavelength components at each frequency conversion stage in an example of the apparatus of FIG. 7 in which the MOPAs are assumed to deliver pulses having a duration of about 1.0 ns at a PRF of 5.0 MHz. MOPA 22B is assumed to have a 1031-nm average power output of 13.5 W. MOPA 28B is assumed to have a 1547-nm average power output of 10.0 W. 198-nm average output power is about 1.05 W. A beam diameter in each crystal of about 80.0 micrometers (μm) is assumed. The crystals are represented by bold-outlined blocks and designated by the same reference numerals as the crystals of FIG. 7.

FIG. 9, schematically depicts, in contour graph form, computed 193-nm output power as a function of average fundamental power delivered by MOPAs 22B and 28B for pulses having a duration of 1 ns delivered at a frequency of 5.0 MHz. In computing the output power the same assumptions are made that are made in the computations of FIG. 8.

Dashed line E_MAX in the graph of FIG. 9 indicates the combination of 1031-nm power and 1547-nm power that would provide maximum conversion efficiency of total power at the various power levels. Here again it can be seen that increasing UV output power is optimally achieved primarily by increasing the power of the shorter wavelength MOPA, i.e., the MOPA, the output of which is frequency quadrupled prior to being mixed with the fundamental wavelength of the longer wavelength MOPA.

The efficiencies calculated by the graphs of FIGS. 4 and 9 are based on a beam size of 80 μm in all of the crystals. With this beam size, particularly at the higher powers the lifetime of CLBO crystals may be limited to a duration that is less than commercially attractive. It is believed that, all else being equal, increasing the beam size to about 260 μm could extend the crystal lifetime to at least about 1000 hours, this, however, would reduce the efficiency for 1.0 W output to about 2%. Methods have been suggested in prior-art documents for preventing deterioration of CLBO by UV radiation. These suggested methods include using certain coatings on crystal faces; locating the crystals in vacuum or hermetically-sealed enclosures; raising the temperature of the crystals; and ion-beam etching surfaces of the crystals to remove embedded polishing compounds. In developing the inventive frequency conversion architecture, no attempt has been made to evaluate the effectiveness of any of these suggested lifetime-extending methods. Further, as the frequency-conversion architecture of the present invention is not limited to CLBO, either in frequency-quadrupling stages or SHG stages, it is also possible that extended operating lifetime of the inventive apparatus can be achieved simply by substituting another crystal type such as the above-mentioned KABO, KABF, or YAB.

It is emphasized, here, that the present invention is not limited to using two pulsed lasers (or MOPAs) of any particular type. Preferably, however, any laser used as one of the two lasers in the inventive apparatus should provide a fundamental wavelength between about 800 nm and 1700 nm. Any two lasers used in the inventive apparatus preferably either inherently deliver, or can be controlled to deliver, pulses of about the same duration. Any two lasers used in the inventive apparatus must also be capable of being synchronized such that frequency multiplied (harmonic) pulses generated from the shorter-wavelength laser can be delivered simultaneously to an optically nonlinear crystal arranged to sum-frequency mix the harmonic pulses, with pulses of fundamental-wavelength radiation from the longer-wavelength laser.

It is emphasized again that the frequency-converted-output modulation scheme described above is not limited to use with the optical fiber MOPAs of FIG. 7. By way of example, the fiber MOPAs could be replaced by Q-switched, diode-pumped solid-state lasers such as Nd:YAG or Nd:YVO₄ lasers each of which can provide pulsed fundamental radiation at the 1064 nm wavelength. PRF of such lasers can be controlled by operating the Q-switches synchronously with the 5 MHz (or some other frequency) RF signal of oscillator 34 via an appropriate phase-shifter.

FIG. 10 schematically illustrates a preferred example of quasi-CW 1064-nm source 102 for use in the apparatus 22A of FIG. 2. A single-mode diode-laser 106 driven by a pulsed power supply 108 serves as a master oscillator (MO), and provides pulsed output at a frequency (here 5 MHz) slaved to master clock 34 of apparatus 22A (see FIG. 2). Pulse duration is controlled by signals delivered to power supply 108 from controller 37 of apparatus 22A. Output from diode-laser 106 is directed by an optical arrangement (not shown) into a first optical fiber amplifier stage 112. Amplifier stage 112 includes an ytterbium-doped gain-fiber 116 optically pumped by a plurality (here, four) of diode-lasers 118 emitting CW radiation at a wavelength of 980 nm.

The output of each diode-laser 118 is coupled into cladding of the gain-fiber by a fiber 120 fused into the cladding of the gain fiber. An isolator 114 prevents feedback from amplifier stage 112 into the diode-laser. Amplified (pre-amplified) pulses are delivered from first amplifier stage 112 into a second fiber-amplifier stage 122, here, configured similarly to the first amplifier stage. Further pre-amplified pulses from amplifier stage 122 are delivered via an optical arrangement (not shown) to solid-state Nd:YVO₄ amplifier 27 of laser apparatus 22A (see FIG. 2) for final amplification. This arrangement is also suitable for use in MOPA 22B of the apparatus of FIG. 7, but with the Yb-doped fiber laser and fiber amplifier arranged to provide seed pulses at a wavelength of 1031 nm. Lasers (MOPAs) amplified by bulk amplifiers are capable of providing an average power output of up to 50 W for 1.0 ns pulses delivered at 5.0 MHz.

FIG. 11 schematically illustrates a preferred example of a 1547 nm source 104 suitable for apparatus 22A of FIG. 2 or for apparatus 22B of FIG. 7. A distributed feedback (DFB) single-mode diode-laser 130 delivers CW output at a wavelength of 1547 nm and serves as a master oscillator. Output of diode-laser 130 is fiber coupled to MZ modulator 132. MZ modulator converts the CW output to a train of pulses at a pulse repetition frequency (PRF) that is determined by the frequency of oscillator or master clock 34 of apparatus 22A (see FIG. 2). Pulse duration is controlled by keying-signals delivered to the MZ modulator from controller 37 of apparatus 22A. The train of pulses is directed by a circulator 134 into a first optical fiber amplifier stage 136.

Amplifier 136 is a double-pass amplifier including an erbium-doped gain-fiber 138 having a fiber Bragg grating (FBG) 140 at a distal end thereof and written into the core of the gain-fiber. FBG 140 is strongly reflective at a wavelength of 1547 nm and has a reflection bandwidth of about 1 nm or less. The distal end of the gain fiber is connected to a first port 143 of a wavelength division multiplexer (WDM) 142. Gain fiber 138 is optically pumped by CW radiation delivered by a diode-laser 144 and having a wavelength of 980 nm. The radiation from diode-laser 144 is coupled into gain-fiber 138 via a second port 146 of WDM 142. The FBG 140 reflects pulses amplified on a first pass through gain-fiber back through the gain fiber for amplification in a return pass. Most of any amplified spontaneous emission (ASE) generated in the first (forward) pass direction in the gain-fiber is transmitted by FBG 144, enters port 143 of the WDM, and exits the WDM via a third port 148 thereof.

Pulses that are pre-amplified in double-pass fiber amplifier 136 return to circulator 134 and are directed by the circulator into a second optical fiber amplifier stage 150 for further pre-amplification. Amplifier stage 150 includes an ytterbium-sensitized erbium-doped gain-fiber 152, optically pumped by a plurality (here, two) of diode-lasers 154, emitting CW radiation at a wavelength of 980 nm. The output of each diode-laser 154 is coupled into cladding of the gain-fiber by a fiber 156 fused into the cladding of the gain fiber. Amplified pulses from amplifier stage 150 are delivered via an optical arrangement (not shown) to Er:Yb:LMA fiber amplifier 32 as discussed above. Lasers (MOPAs) amplified by Er:Yb:LMA fiber amplifiers are capable of providing an average power output of up to 15 W for 1.0 ns pulses delivered at 5.0 MHz. This, as can be seen from the graphs of FIG. 4 and FIG. 9, is sufficient to provide UV output power up to 10W.

FIG. 12 schematically illustrates still another preferred embodiment 20C of apparatus in accordance with the present invention. Apparatus 20C is similar to above discussed apparatus 20A of FIG. 2 with exceptions as follows. In apparatus 20C, a laser source 28C replaces laser source 28A of apparatus 20A. Laser source 28C includes a holmium-doped fiber (Ho:Fiber) laser 114 amplified by a holmium-doped bulk amplifier 116. Laser 28C is tuned to a wavelength of 2114 nm. Fiber laser 114 may be a thulium (Tm) holmium co-doped fiber laser pumped by 785 nm radiation from a diode-laser, a ytterbium holmium co-doped fiber laser pumped by 970 nm radiation from a diode-laser, a holmium-doped fiber laser pumped by 1100 nm radiation from a ytterbium (Yb) doped fiber laser or by 2-micrometer radiation from a thulium-doped fiber laser. A suitable bulk amplifier material is thulium and holmium co-doped YAG.

In apparatus 20C, the 1064 nm output of bulk-amplified laser source 22A is frequency-converted to radiation having a wavelength of about 213 nm by fifth-harmonic generation (5HG). Second-harmonic (532 nm) radiation is generated in an optically nonlinear crystal 44, preferably of LBO, by frequency doubling (2HG). The second-harmonic radiation is converted to fourth-harmonic (266 nm) radiation in an optically nonlinear crystal 46, preferably of CLBO, by frequency-doubling. The fourth-harmonic radiation is mixed with residual (fundamental) 1064 nm radiation in an optically nonlinear crystal 148 to generate the fifth-harmonic radiation. Crystal 148 is also preferably a CLBO crystal. A dichroic beamsplitter 130 directs unconverted second-harmonic (2H) radiation out of the apparatus. A dichroic beamsplitter 132 directs unconverted fourth-harmonic (4H) and 1064 nm fundamental radiation (F) out of the apparatus.

Turning mirrors 54 and 56 direct the 2114 nm fundamental radiation from laser source 20C along path B₂ onto entrance face 152A of an optically nonlinear crystal 152. Fifth-harmonic 213 nm radiation follows path B₁ to entrance face 152A. Paths B₁ and B₂ are incident on the entrance face at an angle α₃ to each other, and each at about the Brewster angle for the corresponding radiation wavelength, such that the 231 nm radiation and the 2114 nm radiation follow a common path through the crystal and are sum-frequency mixed therein. Sum-frequency radiation having a wavelength of 193 nm exits exit face 152B of crystal 152 as output radiation of apparatus 20C.

It should be noted here that the 2114 nm fundamental wavelength of laser source 28C of apparatus 20C should not be construed as limiting this particular embodiment of the inventive apparatus. Ho:fiber lasers may have other fundamental wavelengths, for example in a range between about 2090 nm and about 2150 nm. The longest of these wavelengths will still provide a UV output of the apparatus. A thulium (Tm) doped fiber laser (optionally amplified) may also be substituted for laser 28C in apparatus 20C. Such a laser may be tuned to provide an output (fundamental) wavelength in a range between about 1930 nm and about 2080 nm.

It should be noted here that bulk amplifiers are particularly preferred as final amplification stages in laser apparatus in accordance with the present invention. This is because at high average output power, nonlinear effects in fiber amplifiers cause broadening of the output radiation wavelength. This, in turn, causes broadening of the UV output radiation of the apparatus. Several applications of the UV output radiation are sensitive to the out radiation are sensitive to the radiation bandwidth.

In summary, the present invention is described above in terms of a preferred and other embodiments. The invention is not limited, however, to the embodiments described and depicted. Rather, the invention is limited only by the claims appended hereto.

Claims

1. A method of generating optical pulses, comprising the steps of: generating radiation having a first fundamental wavelength from a first laser, the first fundamental wavelength being between about 975 nm and 1150 nm;generating radiation having a second fundamental wavelength from a second laser, the second fundamental wavelength being between about 1500 nm and about 2150 nm;frequency-multiplying the first-wavelength radiation to provide radiation having a wavelength which is a harmonic-wavelength of the first fundamental wavelength; andin a first sum-frequency mixing step, sum-frequency mixing the harmonic-wavelength radiation with the second-fundamental-wavelength radiation to provide radiation having a first frequency-converted wavelength that is less than the harmonic-wavelength.

2. The method of claim 1, wherein the harmonic wavelength of the first fundamental wavelength is the fifth harmonic, and wherein the first frequency converted wavelength is less than about 200 nm.

3. The method of claim 2, wherein the second fundamental wavelength is between about 1930 nm and about 2150 nm.

4. The method of claim 3, wherein the second fundamental wavelength is between about 1930 nm and 2080 nm.

5. The method of claim 3, wherein the second fundamental wavelength is between about 2090 nm and about 2150 nm.

6. The method of claim 4, wherein the first fundamental wavelength is about 1064 nm, the second fundamental wavelength is about 2114 nm and the first-frequency converted wavelength is about 193 nm.

7. The method of claim 1, further including, in a second sum-frequency mixing step, sum-frequency mixing the first frequency-converted-wavelength radiation with the second-fundamental-wavelength radiation to provide frequency-converted radiation having a second frequency-converted wavelength, the second frequency-converted wavelength being less than the first frequency-converted wavelength.

8. The method of claim 7, wherein the first fundamental wavelength is between about 1000 nanometers and 1099 nanometers and the second fundamental wavelength is between about 1510 nanometers and 1599 nanometers.

9. The method of claim 8, wherein the first fundamental wavelength is about 1064 nm and the second fundamental wavelength is about 1547 nm.

10. The method of claim 8, wherein the first fundamental wavelength is about 1031 nm and the second fundamental wavelength is about 1547 nm.

11. The method of claim 7, wherein the second frequency-converted wavelength is less than about 200 nm.

12. The method of claim 7, wherein the harmonic-wavelength of the first fundamental wavelength is the fourth-harmonic wavelength.

13. The method of claim 12, wherein the first fundamental wavelength is about 1064 nm, the second fundamental wavelength is about 1547 nm, and the second frequency-converted wavelength is about 198 nm.

14. The method of claim 12, wherein the first fundamental wavelength is about 1031 nm, the second fundamental wavelength is about 1547 nm, and the second frequency-converted wavelength is about 193 nm.

15. The method of claim 7, wherein following the first sum-frequency mixing step there is a residual portion of the second-fundamental-wavelength radiation, and, in the second sum-frequency mixing step, the second-fundamental-wavelength radiation that is mixed with the first frequency-converted-wavelength radiation is the residual portion of the second-fundamental-wavelength radiation from the first sum-frequency mixing step.

16. Apparatus for generating pulses of optical radiation, comprising: a first laser apparatus arranged to generate pulses of radiation having a first fundamental wavelength between about 975 nm and 1150 nm;first, second and third optically nonlinear crystals arranged to generate pulses having the fifth-harmonic wavelength of the first fundamental wavelength, from the first-fundamental-wavelength pulses;a second laser apparatus arranged to generate pulses of radiation having a first fundamental wavelength between about 1930 nm and about 2150 nm; anda fourth optically nonlinear crystal arranged to sum-frequency mix the fifth-harmonic radiation pulses with the second-fundamental-wavelength pulses to provide pulses having frequency-converted wavelength less than the fifth-harmonic wavelength.

17. The apparatus of claim 16, wherein the first-fundamental-wavelength pulses have a wavelength of about 1064 nm, the second wavelength pulses have a wavelength of about 2114 nm, and the frequency-converted wavelength pulses have a wavelength of about 193 nm.

18. Apparatus for generating pulses of optical radiation, comprising: a first laser apparatus arranged to generate radiation having a first fundamental wavelength;at least two optically nonlinear crystals arranged to generate radiation having a harmonic wavelength of the first fundamental wavelength, from the first-fundamental-wavelength radiation;a second laser apparatus arranged to generate radiation having a second fundamental wavelength;at least one optically nonlinear crystal arranged to sum-frequency mix the harmonic-radiation with the second-fundamental-wavelength radiation to provide pulses having frequency-converted wavelength less than harmonic wavelength; andwherein the first laser apparatus and the second laser apparatus each include a fiber-laser source and a bulk amplifier.

19. The apparatus of claim 18, wherein at least one of the fiber laser sources includes a fiber amplifier, and output of the fiber amplifier is amplified by the bulk amplifier.

20. The apparatus of claim 18, wherein the first laser apparatus includes a Yb-doped fiber laser and a Nd-doped YVO4 bulk amplifier.

21. The apparatus of claim 20, wherein the second laser apparatus includes a Ho-doped fiber laser and a Ho-doped YAG bulk amplifier.

22. The apparatus of claim 20, wherein the second laser apparatus includes a Er-doped fiber laser and a Er-doped LMA fiber amplifier.