We discuss methods and lessons learned during the integration and testing of five individual kW-class fiber amplifiers seeded with pseudorandom phase-modulated light, using a 1x5 Diffractive Optical Element (DOE). Each amplifier is capable of producing approximately 1.2 kW of near diffraction-limited output power (M2 <1.1). Low power samples from each amplifier are used for active polarization control. Phase control of each amplifier was accomplished using a low power combined beam sample and AFRL’s Locking of Optical Coherent via Single-detector Electronic-frequency Tagging (LOCSET) control system. Approximately 5 kW of signal output was achieved with a combined efficiency of 82%. Losses in the system arise from DOE efficiency limitations, Amplified Spontaneous Emission (ASE), polarization errors, uncorrelated wavefront errors, optical path length mismatches, and beam misalignments. We discuss the impact of recent amplifier developments and how these developments impact this beam combining method.
Recent years have seen silica emerge as a viable material for optical refrigeration with potential applications in directed energy, integrated photonics, and precision metrology. Proper characterization of potential composition profiles is vital for optimization. Here, static photoluminescence spectroscopy of a Yb, Al co-doped silica sample over the temperature range 80 K to 300 K reveals the emission lineshape is dependent on the excitation wavelength. The impact this has on extracted laser cooling parameters is discussed.
Record laser cooling of Yb-doped silica by 18.4 K and 6.3 K was observed in vacuum and atmospheric pressure conditions, respectively. We present a detailed investigation into the optical refrigeration of ytterbium doped silica glass for both in-air and in-vacuum conditions using various pump powers. Temperature measurements were made relative to the room temperature using thermal camera imaging and differential luminescence thermometry. Through analysis of the temporal behavior of the temperature differential at the start of the in-vacuum experiments, we find the cooling efficiency of the studied silicates to be 0.66 ± 0.07%.
Recent advances in thulium doped fibers have significantly improved the optical conversion efficiencies, indicating their potential utility for a variety of applications. Recently, kilowatt-class fiber amplifiers have been demonstrated with narrow linewidth operation. However, their limitations in scaling to higher powers aren’t well understood. While thermal mode instability (TMI) is a well-known limitation in ytterbium doped fiber amplifiers, no experimental data exists for CW thulium doped fiber amplifiers. As such, it’s difficult to quantify or predict when this limitation is expected to impact TDFA’s. Here, we report on the first measurements of TMI in CW thulium doped fiber amplifiers. We characterize the TMI threshold of both 20μm and 25μm fibers by measuring the beam quality, relative intensity noise (RIN), and polarization extinction ratio (PER). In particular, a strong dependence on the TMI threshold with the fiber length is noted. Counter intuitively, measurements show that short fibers have significantly higher TMI thresholds than longer fiber lengths; indeed doubling the fiber length can reduce the TMI threshold by almost 50%. By optimizing the fiber length, a 20/400μm thulium doped fiber amplifier is scaled to 905W, with 57% optical conversion efficiency and a linewidth 5 GHz.
Record laser cooling of Yb-doped silica by 18.4 K was recently observed in vacuum. There is a strong indication pointing to even stronger laser-cooling of Yb-doped silica. In light of these results, a radiation-balanced fiber laser in which cooling from spontaneous emission offsets waste heat generation appears more feasible than before. We will discuss the possibility of a radiation-balanced fiber laser, the similarities and differences with the conventional fiber lasers, and performance issues.
KEYWORDS: Space telescopes, Telescopes, James Webb Space Telescope, Mirrors, Optical instrument design, Astronomy, Space operations, Cryogenics, Aerospace engineering, Cryocoolers
The Origins Space Telescope will trace the history of our origins from the time dust and heavy elements permanently altered the cosmic landscape to present-day life. How did galaxies evolve from the earliest galactic systems to those found in the universe today? How do habitable planets form? How common are life-bearing worlds? We describe how Origins was designed to answer these alluring questions. We discuss the key decisions taken by the Origins mission concept study team, the rationale for those choices, and how they led through an exploratory design process to the Origins baseline mission concept. To understand the concept solution space, we studied two distinct mission concepts and descoped the second concept, aiming to maximize science per dollar and hit a self-imposed cost target. We report on the study approach and describe the concept evolution. The resulting baseline design includes a 5.9-m diameter telescope cryocooled to 4.5 K and equipped with three scientific instruments. The chosen architecture is similar to that of the Spitzer Space Telescope and requires very few deployments after launch. The cryo-thermal system design leverages James Webb Space Telescope technology and experience.
A 1.1 kW CW fiber amplifier emitting at 1.95µm and phase modulated at 5 GHz, with 51% optical conversion efficiency and near diffraction limited beam quality (M2<1.1) is demonstrated. The fiber amplifier consists of 9m of active 20/400um thulium doped fiber, and 2m of passive delivery fiber. Several limiting nonlinearities critical to maintaining coherence were analyzed, including stimulated Brillouin Scattering and modulation instability. To our knowledge, this is the first kw-class thulium doped fiber amplifier operating with narrow linewidth.
Stimulated Brillouin scattering (SBS) is typically the lowest order nonlinearity encountered in ytterbium doped fiber amplifiers (YDFA), and the simplest means of suppressing it is though linewidth broadening from phase modulation. However, to maintain compatibility with beam combining techniques critical to scaling to high output powers, narrow linewidths are needed, and bandwidth efficient means of suppressing SBS are key to scaling to high powers. Here, the scalability of novel phase modulation techniques in combination with laser gain competition are explored. Ultimately, LGC is shown to improve the TMI threshold by 15%, and reduce the linewidth by a factor of 2.1. A 1.8 kW fiber amplifier with 7 Ghz linewidth is demonstrated.
KEYWORDS: Silica, Glasses, Luminescence, High power lasers, Optical fibers, Optical amplifiers, High power fiber amplifiers, Absorption, High power fiber lasers, Fiber lasers
Anti-Stokes fluorescence cooling of a Yb-doped silica glass optical fiber preform is achieved using a high-power laser in a double-pass configuration. The coherent laser beam illuminates the silica glass preform in the red tail of its absorption spectrum, and the heat is carried out by anti-Stokes fluorescence of the blue-shifted photons. The high-purity Yb-doped silica glass preform has low parasitic absorption and is codoped with modifiers to mitigate the quenching-induced non-radiative decay for sufficiently high concentrations of Yb ions in silica glass. Therefore, sufficiently large laser absorption could be achieved to observe cooling while maintaining a near-unity external quantum efficiency.
In this paper we report the generation of flat top optical spectrum using an arbitrary waveform generator to increase the SBS threshold in high power optical fiber amplifiers. The optical spectrum consists of a number of discrete spectral lines, ranging from 16 to 380, within the bandwidth of 2GHz, corresponding to line spacing between 133 MHz and 5 MHz. These discrete spectral lines correspond to a PRBS pattern of n = 4 to n = 8. The SBS threshold and coherence properties of the flat top spectrum are measured and compared to that of the filtered PRBS in a kilowatt class fiber amplifier. It is experimentally demonstrated that for large frequency line spacing, the flat top spectrum significantly outperforms the corresponding filtered PRBS, but as the line spacing is decreased to less than the Brillouin bandwidth, the two modulation waveforms have similar enhancement factors in the SBS threshold due to the enhanced crosstalk between neighboring frequency components.
We report efficient coherent beam combining of five kW-class fiber amplifiers seeded with pseudorandom phase-modulated light, using a 1×5 diffractive optical element (DOE). Each fiber amplifier channel was path length matched, actively polarized, and provided approximately 1.2 kW of near diffraction-limited output power (M2<1.1). A low-power sample of the combined beam after the DOE provided an error signal for active phase stabilization. After phase stabilization, the beams were coherently combined via the DOE. Notably, a total output power of ∼5 kW was achieved with 82% combining efficiency and excellent beam quality (M2<1.1). The intrinsic DOE splitter loss was 5%. Additional losses due in part to nonideal polarization, amplified spontaneous emission content, uncorrelated wavefront errors, and fractional beam misalignments contributed to the efficiency reduction. Overall, multi-kW beam combining of pseudorandom-modulated fiber amplifiers was demonstrated for the first time.
We report efficient coherent beam combining of five kilowatt-class fiber amplifiers with a diffractive optical element (DOE). Based on a master oscillator power amplifier (MOPA) configuration, the amplifiers were seeded with pseudo random phase modulated light. Each non-polarization maintaining fiber amplifier was optically path length matched and provides approximately 1.2 kW of near diffraction-limited output power (measured M2<1.1). Consequently, a low power sample of each laser was utilized for active linear polarization control. A low power sample of the combined beam after the DOE provided an error signal for active phase locking which was performed via Locking of Optical Coherence by Single-Detector Electronic-Frequency Tagging (LOCSET). After phase stabilization, the beams were coherently combined via the 1x5 DOE. A total combined output power of 4.9 kW was achieved with 82% combining efficiency and excellent beam quality (M2<1.1). The intrinsic DOE splitter loss was 5%. Similarly, losses due in part to non-ideal polarization, ASE content, uncorrelated wavefront errors, and misalignment errors contributed to the efficiency reduction.
Power scaling investigation of a narrow-linewidth, Ytterbium-doped all-fiber amplifier operating at 1034 nm is presented. Nonlinear stimulated Brillouin scattering (SBS) effects were suppressed through the utilization of an external phase modulation technique. Here, the power amplifier was seeded with a spectrally broadened master oscillator and the results were compared using both pseudo-random bit sequence (PRBS) and white noise source (WNS) phase modulation formats. By utilizing an optical band pass filter as well as optimizing the length of fiber used in the pre-amplifier stages, we were able to appreciably suppress unwanted amplified spontaneous emission (ASE). Notably, through PRBS phase modulation, greater than two-fold enhancement in threshold power was achieved when compared to the WNS modulated case. Consequently, by further optimizing both the power amplifier length and PRBS pattern at a clock rate of 3.5 GHz, we demonstrated 1 kilowatt of power with a slope efficiency of 81% and an overall ASE content of less than 1%. Beam quality measurements at 1 kilowatt provided near diffraction-limited operation (M2 < 1.2) with no sign of modal instability. To the best of our knowledge, the power scaling results achieved in this work represent the highest power reported for a spectrally narrow all-fiber amplifier operating at < 1040 nm in Yb-doped silica-based fiber.
We report results from two ~1.5 kW Yb-doped fiber amplifiers with comparable optical to optical efficiencies and linewidths. One amplifier utilized a fiber with a core diameter of 25 μm while the core diameter of the fiber utilized in the other amplifier was 20 μm. Stimulated Brillouin scattering (SBS) suppression in both cases was achieved through pseudo-random bit sequence (PRBS) phase modulation. While the power generated in the larger core fiber was modal instability (MI) limited, no sign of MI was observed in the smaller core fiber. This may allow us to utilize the higher MI threshold fiber to scale further while maintaining sufficiently narrow linewidth for beam combining. Furthermore, in a demonstration of the utility of applying a thermal gradient in conjunction with phase modulation to suppress SBS further, we report on a 1 kW amplifier driven at a PRBS clock rate of 2 GHz. Finally, we compare the coherent beam combining properties of amplifiers seeded with PRBS phase modulated sources to those seeded with white noise sources.
Laser gain competition was used in conjunction with external phase modulation techniques in order to investigate power scaling of narrow-linewidth monolithic Ytterbium-doped fiber amplifiers. In this study, both pseudo-random bit sequence (PRBS) and filtered white noise source (WNS) modulation techniques were separately utilized to drive the external phase modulator for linewidth broadening. The final-stage amplifier was then seeded with the phase modulated narrow-linewidth 1064 nm signal along with a spectrally broader 1038 nm source. Consequently, integration of laser gain competition in conjunction with PRBS phase modulation yields a factor of ∼15 dB in stimulated Brillouin scattering (SBS) threshold enhancement at a clock rate of 2.5 GHz; leading to 1 kilowatt of output power with 85% optical efficiency at 1064 nm. Notably, the combination of PRBS phase modulation with laser gain competition provided superior enhancement in SBS threshold power when compared to the WNS modulated case. The beam quality at maximum power was near the diffraction limit (M2 <1.2) with no sign of modal instability. Overall, the power scaling results represent a significant reduction in spectral linewidth compared to that of commercially available narrowlinewidth Ytterbium-doped fiber amplifiers.
White noise phase modulation (WNS) and pseudo-random binary sequence phase modulation (PRBS) are effective
techniques for mitigation of nonlinear effects such as stimulated Brillouin scattering (SBS); thereby paving the way for
higher power narrow linewidth fiber amplifiers. However, detailed studies comparing both coherent beam combination
and the SBS suppression of these phase modulation schemes have not been reported. In this study an active fiber cutback
experiment is performed comparing the enhancement factor of a PRBS and WNS broadened seed as a function of
linewidth and fiber length. Furthermore, two WNS and PRBS modulated fiber lasers are coherently combined to measure
and compare the fringe visibility and coherence length as a function of optical path length difference. Notably, the
discrete frequency comb of PRBS modulation provides a beam combining re-coherence effect where the lasers
periodically come back into phase. Significantly, this may reduce path length matching complexity in coherently
combined fiber laser systems.
White noise phase modulation is an effective technique capable of increasing the SBS threshold in high power fiber amplifiers. Theoretical models predict the enhancement factor as a function of linewidth and fiber length, but have yet to be experimentally verified over wide ranges of these variables. We present results on a cut-back experiment performed on a passive fiber with a white-noise broadened laser, measuring the SBS enhancement factor as a function of fiber length and bandwidth. In addition, the experimental results will be compared to phase modulation models of the SBS process in optical fibers.
We present experimental results of SBS suppression in high power, monolithic, Yb-doped fiber amplifiers via phase modulated laser gain competition. To narrow the linewidth, two-tone laser gain competition between broad (1036 nm) and narrow linewidth (1064 nm) laser signals is investigated in conjunction with phase modulation and yields pump limited output powers of 600 W. Here integration of both two-tone and pseudo random bit sequence (PRBS) phase modulation concepts, generated SBS enhancement factors of greater than 17x at a modulation frequency of 500 MHz, without reaching the SBS threshold. Significantly, the results represent a near order of magnitude reduction in linewidth over current high-power, monolithic, Yb-doped fiber amplifiers.
We present experimental and theoretical studies on the stimulated Brillouin scattering (SBS) threshold in fiber amplifiers seeded with a spectrally broadened single-frequency laser source. An electro-optic phase modulator is driven with various pseudo-random binary sequence (PRBS) patterns to highlight the unique characteristics of this linewidth broadening technique and its facility in SBS mitigation. Theoretical predictions show a variation in SBS suppression based on PRBS pattern and modulation frequency. These predictions are experimentally investigated in a kilowatt level monolithic fiber amplifier operating with near diffraction-limited beam quality. We also show Rayleigh scattering and other sources of back reflected light in phase modulated signals can seed the SBS process and significantly reduce the nonlinear threshold.
We present a detailed study of power scaling in polarization-maintaining Raman fiber amplifiers operating at 1178 nm since this wavelength can be frequency doubled into 589 nm for sodium guide star applications. We confirm experimentally that the optimized output signal at SBS threshold scales linearly with the pump power. We also present results from numerical and experimental studies investigating the scalability of Raman fiber amplifiers with seed power. Both co-pumped and counter pumped two-stage amplifiers utilizing acoustically tailored fiber for SBS suppression were constructed and studied. For the former configuration spectral broadening was observed, while the latter configuration provided 22 W of single-frequency output. Finally, we show results of a phase-modulated amplifier generating multiple spectral lines separated by 886 MHz, which corresponds to the spectral separation of the sodium D2a, and D2b lines after frequency doubling in a nonlinear cavity.
We present an experimental study on active coherent combining of five Yb (Ytterbium)-doped fiber laser amplifiers that
employs multiplexed volume Bragg gratings (MVBGs), reporting a combining efficiency of 82% and near-diffraction
limited beam quality at a combined input power of 380 W, and 70% combining efficiency with equal beam quality at
670 W input power.
We present detailed studies of the effect of sinusoidal phase modulation on stimulated Brillouin scattering (SBS) in
ytterbium-doped fiber amplifiers. Based on a time-dependent SBS model, SBS enhancement factor versus pump
linewidth for different modulation depths ranging from 0 to π , and modulation frequencies ranging from 30 MHz to
500 MHz were analyzed. In addition, experimental validation of SBS suppression via sinusoidal phase modulation is
presented with experimental results agreeing well with the model and simulations. Furthermore, narrow linewidth
coherent beam combining (CBC) of 5 sinusoidal phase modulated lasers is demonstrated via LOCSET.
We report on various single and multimode channel waveguide structures fabricated via microtransfer molding and
microfluidic techniques. These soft lithographic fabrication techniques can result in an inexpensive and rapid turnover of
various types of channel waveguide structures and general integrated optic devices. It may be particularly useful for
production of waveguides on user-desired surface substrates including those of a curved or distorted nature. Microscopic
cross-sectional images for both single and multimode waveguides are obtained and compared between the two
fabrication methods. The novel microfluidic technique results in superior waveguide formation and improved
propagation loss performance.
An infrared imaging lens that produces beams with long focal depth while preserving the entire aperture for full light capturing and high transverse resolution is presented. Based on the conjugate-gradient algorithm, a diffractive optical lens with four times depth of focus improvement at the 10.6-µm wavelength has been designed and fabricated. ZEMAX simulation has confirmed the designed lens performance showing legible images over an extended image range. Through laser direct-write photoresist patterning and subsequent reactive ion etching on a germanium substrate, we have realized a diffractive lens with four times depth of focus improvement over a conventional infrared lens of the same numerical aperture. The extended depth of focus lens should yield a variety of applications in focus-free imaging without reducing lens aperture.
An infrared imaging lens that produces beams with long focal depth whilst preserving the entire aperture for full light capturing and high transverse resolution is presented. It is a diffractive optical element that generates a long range of pseudo-non-diffractive rays. The design technique is based on the conjugate-gradient algorithm. The surface relief pattern was generated on a thick film photoresist and then the pattern was transferred to germanium substrate. Preliminary experimental results demonstrated four times improvement in depth of focus at 10.6 μm wavelength.
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