Beamlines at the National Ignition Facility (NIF) use large neodymium-doped glass slabs for amplification of pulsed beams with various temporal shapes and transverse dimensions _40 cm _ 40 cm. Currently, the Virtual Beam Line (VBL) simulator1 computes saturable amplification according to the approach of Frantz and Nodvik, modified to include drain of the lasing transition's lower level. Linearly chirped pulses are amplified by gain media parameterized by an emission cross section value referenced to the instantaneous beam wavelength. Expanding the capabilities of VBL to a family of waveforms that is more diverse in terms of spectral amplitude and phase calls for the adoption of an approach that is fundamentally dispersive. In this work, we describe an approach to computing broadband amplification in the time domain according to coupled equations that describe evolution of the population inversion and the associated resonant polarization. Considering the diversity of glass species with respect to various gain inhomogeneities, we explore various model extensions for capturing the non-Lorentzian emission cross section in the small-signal regime and how the underlying resonant susceptibility is deformed by gain saturation. The polarization envelope acts as transverse-spatial sources to (3+1)D spectral envelope propagation that fully accounts for linear-optical diffraction and dispersion in the host glass, and includes the usual instantaneous non-resonant third-order electronic response (optical Kerr effect).
Design, activation, and operation of large laser systems rely on accurate, efficient, user-friendly simulation of laser performance. At the Lawrence Livermore National Laboratory, the principle tool for this simulation over the past ten years has been the VBL, an outgrowth of the Prop code that uses the same text-file input grammar and is closely integrated with the Laser Performance Operations Model (LPOM). Here, we describe the physics capabilities of this code, its user interface, and our plans for near-term future developments.
The National Ignition Facility (NIF) at Lawrence Livermore National Laboratory is the first of a kind megajoule-class laser with 192 beams capable of delivering over 1.8 MJ and 500TW of 351nm light [1], [2]. It has been commissioned and operated since 2009 to support a wide range of missions including the study of inertial confinement fusion, high energy density physics, material science, and laboratory astrophysics. In order to advance our understanding, and enable short-pulse multi-frame radiographic experiments of dense cores of cold material, the generation of very hard x-rays above 50 keV is necessary. X-rays with such characteristics can be efficiently generated with high intensity laser pulses above 1017 W/cm² [3]. The Advanced Radiographic Capability (ARC) [4] which is currently being commissioned on the NIF will provide eight, 1 ps to 50 ps, adjustable pulses with up to 1.7 kJ each to create x-ray point sources enabling dynamic, multi-frame x-ray backlighting. This paper will provide an overview of the ARC system and report on the laser performance tests conducted with a stretched-pulse up to the main laser output and their comparison with the results of our laser propagation codes.
Wade Williams, Jerome Auerbach, Mark Henesian, Kenneth Jancaitis, Kenneth Manes, Naresh Mehta, Charles Orth, Richard Sacks, Michael Shaw, Clifford Widmayer
Optical propagation modeling of the National Ignition Facility has been utilized extensively from conceptual design several years ago through to early operations today. In practice we routinely (for every shot) model beam propagation starting from the waveform generator through to the target. This includes the regenerative amplifier, the 4-pass rod amplifier, and the large slab amplifiers. Such models have been improved over time to include details such as distances between components, gain profiles in the laser slabs and rods, transient optical distortions due to the flashlamp heating of laser slabs, measured transmitted and reflected wavefronts for all large optics, the adaptive optic feedback loop, and the frequency converter. These calculations allow nearfield and farfield predictions in good agreement with measurements.
KEYWORDS: Wavefronts, National Ignition Facility, Control systems, Actuators, Sensors, Mirrors, High power lasers, Computing systems, Coating, Deformable mirrors
The use of lasers as the driver for inertial confinement fusion and weapons physics experiments is based on their ability to produce high-energy short pulses in a beam with low divergence. Indeed, the focusability of high quality laser beams far exceeds alternate technologies and is a major factor in the rationale for building high power lasers for such applications. The National Ignition Facility (NIF) is a large, 192-beam, high-power laser facility under construction at the Lawrence Livermore National Laboratory for fusion and weapons physics experiments. Its uncorrected minimum focal spot size is limited by laser system aberrations. The NIF includes a Wavefront Control System to correct these aberrations to yield a focal spot small enough for its applications. Sources of aberrations to be corrected include prompt pump-induced distortions in the laser amplifiers, previous-shot thermal distortions, beam off-axis effects, and gravity, mounting, and coating-induced optic distortions. Aberrations from gas density variations and optic-manufacturing figure errors are also partially corrected. This paper provides an overview of the NIF Wavefront Control System and describes the target spot size performance improvement it affords. It describes provisions made to accommodate the NIF's high fluence (laser beam and flashlamp), large wavefront correction range, wavefront temporal bandwidth, temperature and humidity variations, cleanliness requirements, and exception handling requirements (e.g. wavefront out-of-limits conditions).
The National Ignition Facility (NIF) laser will use a 192- beam multi-pass architecture capable of delivering several MJ of UV energy in temporal phase formats varying from sub- ns square to 20 ns precisely-defined high-contrast shapes. Each beam wavefront will be subjected to effects of optics inhomogeneities, figuring errors, mounting distortions, prompt and slow thermal effects from flashlamps, driven and passive air-path turbulence, and gravity-driven deformations. A 39-actuator intra-cavity deformable mirror, controlled by data from a 77-lenslet Hartman sensor will be used to correct these wavefront aberrations and thus to assure that stringent farfield spot requirements are met. We have developed numerical models for the expected distortions, the operation of the adaptive optics systems, and the anticipated effects on beam propagation, component damage, frequency conversion, and target-plane energy distribution. These models have been extensively validated against data from LLNL's Beamlet, and Amplab lasers. We review the expected beam wavefront aberrations and their potential for adverse effects on the laser performance, describe our model of the corrective system operation, and display our predictions for corrected-beam operation of the NIF laser.
KEYWORDS: Wavefronts, National Ignition Facility, Control systems, Sensors, Actuators, Deformable mirrors, Mirrors, Wavefront sensors, Control systems design, Near field optics
A wavefront control system will be employed on NIF to correct beam aberrations that otherwise would limit the minimum target focal spot size. For most applications, NIF requires a focal spot that is a few times the diffraction limit. Sources of aberrations that must be corrected include prompt pump-induced distortions in the laser slabs, thermal distortions in the laser slabs from previous shots, manufacturing figure errors in the optics, beam off-axis effects, gas density variations, and gravity, mounting, and coating-induced optic distortions.
The performance of the National Ignition Facility (NIF), especially in terms of laser focusability, will be determined by several key factors. One of these key factors is the optical specification of the thousands of large aperture optics that will comprise the 192 beamlines. We have previously reported on the importance of the specification of the power spectral density (PSD) on NIF performance. Recently, we have been studying the importance of long spatial wavelength phase errors on focusability. We have concluded that the preferred metric for determining the impact of these long spatial wavelength phase errors is the rms phase gradient. In this paper, we outline the overall approach to NIF optical specifications, detail the impact of the rms phase gradient on NIF focusability, discuss its trade-off with the PSD in determining the spot size, and review measurements of optics similar to those to be manufactured for NIF.
KEYWORDS: Wavefronts, National Ignition Facility, Control systems, Wavefront sensors, Control systems design, Laser applications, Optics manufacturing, Computing systems, Sensors, Interferometers
The use of lasers as the driver for inertial confinement fusion experiments and weapons physics applications is based on their ability to produce high-energy short pulses in a beam with low divergence. Indeed, the focusability of high quality laser beams far exceeds alternate technologies and is a major factor in the rationale for building lasers for such applications The National Ignition Facility (NIF) is a large 192-beam laser facility now under construction at the Lawrence Livermore National Laboratory for fusion and weapons physics experiments. Its uncorrected focal spot minimum size is limited by wavefront aberrations in the laser system. NIF is designed with a wavefront control system to correct these aberrations to yield a focal spot that is small enough for NIF' s intended applications. Sources of aberrations to be corrected include prompt pump-induced distortions in the laser amplifiers, thermal distortions in the amplifiers from previous shots, beam off-axis effects, and gravity, mounting, and coating-induced optic distortions. Aberrations from gas density variations and manufacturing figure errors in the optics are also partially corrected by the wavefront control system. The NIF wavefront control system consists of five subsystems for each of the 192 beams: 1) a deformable mirror, 2) a wavefront sensor, 3) a computer controller, 4) a wavefront reference system, and 5) a rapid reconfiguration system to allow the wavefront control system to operate to within one second of the laser shot. The system includes the capability for in situ calibrations and operates in closed loop prior to the shot. Shot wavefront data is recorded. This paper describes the function, realization, and performance of each wavefront control subsystem. Subsystem performance will be characterized by computer models and by test results. The focal spot improvement in the NIF laser system effected by the wavefront control system will be characterized through computer models. The sensitivity of the target focal spot to various aberration sources will be presented. Analyses to optimize the wavefront control system will also be presented.
KEYWORDS: Adaptive optics, National Ignition Facility, Modulation, Frequency conversion, Near field optics, Near field, Nano opto mechanical systems, Turbulence, Spatial filters, Phase shift keying
The predicted focal spot size of the National Ignition Facility laser is parameterized against the finish quality of the optics in the system. Results are reported from simulations which include static optics aberrations, as well as pump-induced distortions, beam self-focusing, and the effect of an adaptive optic. The simulations do not include contributions from optics mounting errors, residual thermal noise in laser slabs from previous shots, air turbulence, a kinoform phase plate, or smoothing by spectral dispersion. Consequently, these results represent `first shot of the day', without-SSD, predictions.
We present the energy, propagation, and thermal modeling for a diode-pumped solid-state laser called Mercury being designed and built at LLNL using Yb:S-FAP [i.e., Yb3+-doped Sr5(PO4)3F crystals] for the gain medium. This laser is intended to produce 100 J pulses at 1 to 10 ns at 10 Hz with an electrical efficiency of approximately 10%. Our modeling indicates that the laser will be able to meet its performance goals.
We discuss the partitioning of effects on the fundamental focal irradiance distribution from whole beam self-focusing, and PSDs of the optical components in the laser chain, and the resulting third harmonic focal distribution. Beamlet and NIF simulation results are discussed.
Design optimization of the 1 .8 MJ, 500 TW National Ignition Facility (NIF) laser has proceeded with the use of a suite of new computational models. Cost-effectiveness of alternative fundamental architectures was considered using CHAINOP. A very fast, lumped-element energetics code, CHA1NOP includes an extensive cost database, a runtime choice of optimization algorithm, and a set of heuristic rules for diffraction and nonlinear effects and for operational constraints. Its ability to flexibly consider many alternative configurations at a few seconds per chain made it the ideal "first-cut" tool for narrowing the investigation to the switched, multi-pass cavity architecture that was chosen.
The effect of a change in the system parameters upon the one micron laser's power, energy and beam quality will be discussed. The parameters varied in the study were the optical losses, the gain and gain profile of the amplifiers. Additionally, the effect upon power, energy and beam quality as a function of slab count and position will be presented.
We discuss the partitioning of effects on the fundamental focal irradiance distribution from whole beam self-focusing, and PSDs of the optical components in the laser chain. Beamlet and NIF simulation results are discussed.
KEYWORDS: National Ignition Facility, Data modeling, Optimization (mathematics), Optical amplifiers, Switches, Amplifiers, Frequency conversion, Parallel processing, Data conversion, Thermography
The design of the National Ignition Facility (NIF) is the result of optimization studies that maximized laser performance and reliability within a restricted cost budget. We modeled the laser using a suite of tools that included a 1D propagation code, a frequency conversion code, a 2D ray trace code for calculating the gain profile, thermo- mechanical codes for calculating the pump-induced distortions in the slabs, a database giving estimates of optics bulk/finish quality, and costing models of the laser/building. By exploiting parallel processing, we were able to consider approximately 750 possible designs per hour using a cluster of 28 workstations. For our optimization studies, we used a temporally shaped (ICF indirect drive) pulse producing at least 2.2 MJ and 600 TW in a 600 micron diameter hole at the target entrance plane. We varied as many as 20 design variables (e.g., slab counts, slab thickness, Nd concentration, amplifier pulse length) and applied as many as 40 constants (e.g., flashlamp voltage and fluence damage/filamentation at various points in the chain). We did not vary the number of beamlets (fixed at 192 or the aperture (fixed at 40 cm). We used three different optimization approaches: a variable metric algorithm, an exhaustive grid search of more than 50,000 candidate designs, and a parabolic interpolation scheme. All three approaches gave similar results. Moreover, a graphical analysis of the parameter scan data (analogous to sorting and pruning designs using a spreadsheet) has allowed us to understand why the optimizers eliminated alternate designs. The most inexpensive main-switch-boot slab configuration meeting the mission requirements and satisfying all constraints was 9-5-3. The cost of this configuration is approximately $DOL10M less than the 9-5-5 conceptual design. However, the NIF Project has chosen a slightly more expensive 11-0-7 configuration for continued Title I engineering because of its similarity to the Beamlet 11-0-5 design and a lower B-integral.
P. Renard, C. Clay Widmayer, Jerome Auerbach, Scott Haney, Mark Henesian, John Hunt, Janice Lawson, Kenneth Manes, David Milam, Charles Orth, Richard Sacks, David Speck, John Trenholme, Wade Williams
The near field irradiance parameters at the interface between the one micron laser, the UV generation, and transport subsystem will be discussed. The test results obtained from the Beamlet and Nova lasers used to validate the mathematical models will be presented.
Mark Henesian, P. Renard, Jerome Auerbach, John Caird, B. Ehrlich, Steven Haney, John Hunt, Janice Lawson, Kenneth Manes, David Milam, Richard Sacks, Lynn Seppala, I. Smith, David Speck, Calvin Thompson, Bruno Van Wonterghem, Paul Wegner, Timothy Weiland, C. Clay Widmayer, Wade Williams, John Trenholme
An exhaustive set of Beamlet and Nova laser system simulations were performed over a wide range of power levels in order to gain understanding about the statistical trends in Nova and Beamlet's experimental data sets, and to provide critical validation of propagation tools and design `rules' applied to the 192-arm National Ignition Facility at Lawrence Livermore National Laboratory.
Optical components of large-aperture, high irradiance and high fluence lasers can experience significant levels of stimulated scattering along their transverse dimensions. We have observed transverse stimulated Raman scattering in large aperture KDP crystals, and have measured the stimulated gain coefficient.
Detailed modeling of beam propagation in Beamlet has been made to predict system performance. New software allows extensive use of optical component characteristics. This inclusion of real optical component characteristics has resulted in close agreement between calculated and measured beam distributions.
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