Michael C. Rushford
Lawrence Livermore National Laboratory
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Featured researches published by Michael C. Rushford.
Nuclear Fusion | 2004
C. P. J. Barty; M.H. Key; J.A. Britten; R. Beach; G. Beer; C. Brown; S. Bryan; John A. Caird; T. Carlson; John K. Crane; Jay W. Dawson; Alvin C. Erlandson; D. N. Fittinghoff; Mark Hermann; C. Hoaglan; A. Iyer; L. Jones; Igor Jovanovic; Aleksey M. Komashko; O. L. Landen; Zhi M. Liao; William A. Molander; S. Mitchell; E. I. Moses; Norman D. Nielsen; H.-H. Nguyen; J. Nissen; Stephen A. Payne; Deanna M. Pennington; L. Risinger
The technical challenges and motivations for high-energy, short-pulse generation with the National Ignition Facility (NIF) and possibly other large-scale Nd : glass lasers are reviewed. High-energy short-pulse generation (multi-kilojoule, picosecond pulses) will be possible via the adaptation of chirped pulse amplification laser techniques on NIF. Development of metre-scale, high-efficiency, high-damage-threshold final optics is a key technical challenge. In addition, deployment of high energy petawatt (HEPW) pulses on NIF is constrained by existing laser infrastructure and requires new, compact compressor designs and short-pulse, fibre-based, seed-laser systems. The key motivations for HEPW pulses on NIF is briefly outlined and includes high-energy, x-ray radiography, proton beam radiography, proton isochoric heating and tests of the fast ignitor concept for inertial confinement fusion.
Applied Optics | 2001
Ian M. Barton; Jerald A. Britten; S. Dixit; Leslie J. Summers; Ian M. Thomas; Michael C. Rushford; Katy Lu; Roderick A. Hyde; Michael D. Perry
We describe the advantages of using diffractive (Fresnel) lenses on thin membranes over conventional optics for, among others, future space telescope projects. Fabrication methods are presented for lenses on two types of freestanding membrane up to 50 cm in size. The first is a Fresnel lens etched into a thin (380-microm) glass sheet, and the second is an approximately 50-microm-thick polymer membrane containing a Fresnel lens made by replication process from a specially made fused-silica master. We show optical performance analysis of all the lenses that are fabricated, including a diffraction-limited Airy spot from a 20-m- focal-length membrane lens in a diffractive telescope system.
Optics Letters | 2010
H. Habara; Guang Xu; Takahisa Jitsuno; R. Kodama; Kenji Suzuki; K. Sawai; K. Kondo; Noriaki Miyanaga; K. Tanaka; Kunioki Mima; Michael C. Rushford; Jerald A. Britten; C. P. J. Barty
Segmented (tiled) grating arrays are being intensively investigated for petawatt-scale pulse compression due to the expense and technical challenges of fabricating monolithic diffraction gratings with apertures of over 1m. However, the considerable freedom of motion among grating segments complicates compression and laser focusing. We constructed a real compressor system using a segmented grating for an 18cm aperture laser beam of the Gekko MII 100TW laser system at Osaka University. To produce clean pulse shapes and single focal spots tolerant of misalignment and groove density difference of grating tiles, we applied a new compressor scheme with image rotation in which each beam segment samples each grating segment but from opposite sides. In high-energy shots of up to 50J, we demonstrated nearly Fourier-transform-limited pulse compression (0.5ps) with an almost diffraction-limited spot size (20microm).
Journal of Physics: Conference Series | 2010
John K. Crane; G Tietbohl; P Arnold; E S Bliss; C Boley; G Britten; G Brunton; W Clark; Jay W. Dawson; S Fochs; R Hackel; C. Haefner; J Halpin; John E. Heebner; M Henesian; Mark Hermann; J Hernandez; V Kanz; B McHale; J B McLeod; H Nguyen; H Phan; Michael C. Rushford; B Shaw; M Shverdin; R Sigurdsson; R Speck; C Stolz; D Trummer; J Wolfe
We are converting a quad of NIF beamlines into eight, short-pulse (1–50 ps), petawatt-class beams for advanced radiography and fast ignition experiments. This paper describes progress toward completing this project.
Astronomical Telescopes and Instrumentation | 2002
Roderick A. Hyde; S. Dixit; Andrew H. Weisberg; Michael C. Rushford
Eyeglass is a very large aperture (25 - 100 meter) space telescope consisting of two distinct spacecraft, separated in space by several kilometers. A diffractive lens provides the telescopes large aperture, and a separate, much smaller, space telescope serves as its mobile eyepiece. Use of a transmissive diffractive lens solves two basic problems associated with very large aperture space telescopes; it is inherently fieldable (lightweight and flat, hence packagable and deployable) and virtually eliminates the traditional, very tight, surface shape tolerances faced by reflecting apertures. The potential drawback to use of a diffractive primary (very narrow spectral bandwidth) is eliminated by corrective optics in the telescopes eyepiece. The Eyeglass can provide diffraction-limited imaging with either single-band, multiband, or continuous spectral coverage. Broadband diffractive telescopes have been built at LLNL and have demonstrated diffraction-limited performance over a 40% spectral bandwidth (0.48 - 0.72 μm). As one approach to package a large aperture for launch, a foldable lens has been built and demonstrated. A 75 cm aperture diffractive lens was constructed from 6 panels of 1 mm thick silica; it achieved diffraction-limited performance both before and after folding. This multiple panel, folding lens, approach is currently being scaled-up at LLNL. We are building a 5 meter aperture foldable lens, involving 72 panels of 700 μm thick glass sheets, diffractively patterned to operate as coherent f/50 lens.
Optics Letters | 2008
Michael C. Rushford; Jerald A. Britten; C. P. J. Barty; Takahisa Jitsuno; K. Kondo; Noriaki Miyanaga; K. Tanaka; R. Kodama; Guang Xu
We introduce a four-pass laser pulse compressor design based on two grating apertures with two gratings per aperture that is tolerant to some alignment errors and, importantly, to grating-to-grating period variations. Each half-beam samples each grating in a diamond-shaped compressor that is symmetric about a central bisecting plane. For any given grating, the two half-beams impinge on opposite sides of its surface normal. It is shown that the two split beams have no pointing difference from paired gratings with different periods. Furthermore, no phase shift between half-beams is incurred as long as the planes containing a grating line and the surface normal for each grating of the pair are parallel. For grating pairs satisfying this condition, gratings surfaces need not be on the same plane, as changes in the gap between the two can compensate to bring the beams back in phase.
Journal of the Optical Society of America | 1978
L. A. Hackel; Michael C. Rushford
We have refined and extended an existing technique for determining an atomic transition probability by carefully measuring the transition branching ratio (BR) and excited-state lifetime (τ), with particular attention paid to systematic errors. The technique was applied to the red region of the 238U i spectrum where little accurate data is presently available. In particular, we find for the 6395.42 A transition the following values: τ = 607 ± 20 ns, BR = 0.586 ± 0.05, and g2A = 1.45 × 107 ± 1.25 × 106.
Proceedings of SPIE | 2015
J. M. Di Nicola; Steven T. Yang; C. D. Boley; John K. Crane; John E. Heebner; T. Spinka; P. A. Arnold; C. P. J. Barty; M. W. Bowers; Tracy Budge; Kim Christensen; Jay W. Dawson; Gaylen V. Erbert; Eyal Feigenbaum; Gabe Guss; C. Haefner; Mark Hermann; Doug Homoelle; J. Jarboe; Janice K. Lawson; Roger Lowe-Webb; K. P. McCandless; Brent McHale; L. J. Pelz; P. P. Pham; Matthew A. Prantil; M. Rehak; Matthew Rever; Michael C. Rushford; Richard A. Sacks
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.
Journal of the Optical Society of America | 1979
L. A. Hackel; C. F. Bender; M. A. Johnson; Michael C. Rushford
A technique for precisely measuring hyperfine structure of any level of neutral uranium which can be excited by a single or multistep transition from the ground or a low-lying-metastable state has been developed. Numerous spectra were measured and fit to obtain precise hyperfine splitting constants. In particular, measurements on the 31 869-cm−1 odd level have determined the following: J = 6, magnetic dipole constant A = −47.2 ± 0.6 MHz and electric quadrupole constant B = 1892 ± 26 MHz. Structure of serveral excited states of known configuration were measured including the 15 632-cm−1f2d2s2(5L7) and the 16 930-cm−1f3dsp (7K5) levels.
Physics of Plasmas | 2017
H. Chen; Mark Hermann; D. H. Kalantar; D. Martinez; P. Di Nicola; R. Tommasini; O. L. Landen; D. Alessi; M. W. Bowers; D. Browning; G. Brunton; Tracy Budge; John K. Crane; J. M. Di Nicola; T. Döppner; S. Dixit; Gaylen V. Erbert; B. Fishler; J. Halpin; M. Hamamoto; John E. Heebner; Vincent J. Hernandez; M. Hohenberger; Doug Homoelle; J. Honig; W. W. Hsing; N. Izumi; S. F. Khan; K. N. LaFortune; Janice K. Lawson
The Advanced Radiographic Capability (ARC) laser system at the National Ignition Facility (NIF) is designed to ultimately provide eight beamlets with a pulse duration adjustable from 1 to 30 ps, and energies up to 1.5 kJ per beamlet. Currently, four beamlets have been commissioned. In the first set of 6 commissioning target experiments, the individual beamlets were fired onto gold foil targets with energy up to 1 kJ per beamlet at 20–30 ps pulse length. The x-ray energy distribution and pulse duration were measured, yielding energy conversion efficiencies of 4–9 × 10−4 for x-rays with energies greater than 70 keV. With greater than 3 J of such x-rays, ARC provides a high-precision x-ray backlighting capability for upcoming inertial confinement fusion and high-energy-density physics experiments on NIF.