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Laser propagation measurements in long-scale-length underdense plasmas relevant to magnetized liner inertial fusion

Journal Article · · Physical Review E
 [1];  [1];  [2];  [1];  [3];  [2];  [4];  [4];  [1];  [5]
  1. Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
  2. General Atomics, San Diego, CA (United States)
  3. Univ. of Rochester, NY (United States). Lab. for Laser Energetics
  4. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  5. Naval Research Lab. (NRL), Washington, DC (United States)
Here, we report experimental results and simulations showing efficient laser energy coupling into plasmas at conditions relevant to the magnetized liner inertial fusion (MagLIF) concept. In MagLIF, to limit convergence and increase the hydrodynamic stability of the implosion, the fuel must be efficiently preheated. To determine the efficiency and physics of preheating by a laser, an Ar plasma with n e / n c r i t ~ 0.04 is irradiated by a multi-ns, multi-kJ, 0.35-μm, phase-plate-smoothed laser at spot-averaged intensities ranging from 1.0 × 10 14 to 2.5 × 10 14 W / c m 2 and pulse widths from 2 to 10 ns. Time-resolved x-ray images of the laser-heated plasma are compared to two-dimensional radiation-hydrodynamic simulations that show agreement with the propagating emission front, a comparison that constrains laser energy deposition to the plasma. The experiments show that long-pulse, modest-intensity ( I = 1.5 × 10 14 W / c m 2 ) beams can efficiently couple energy ( ~ 82 % of the incident energy) to MagLIF-relevant long-length (9.5 mm) underdense plasmas. The heating efficiency we demonstrate is significantly higher than it was thought to have been achieved in early integrated MagLIF experiments [A. B. Sefkow et al., Phys. Plasmas 21, 072711 (2014)].
Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Sandia National Laboratories (SNL-NM), Albuquerque, NM (United States)
Sponsoring Organization:
USDOE; USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC04-94AL85000; AC52-07NA27344
OSTI ID:
1338676
Alternate ID(s):
OSTI ID: 1330738
OSTI ID: 1438716
Report Number(s):
LLNL-JRNL--740586; SAND2016--11073J; 648803
Journal Information:
Physical Review E, Journal Name: Physical Review E Journal Issue: 5 Vol. 94; ISSN PLEEE8; ISSN 2470-0045
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

References (10)

Advances in NLTE modeling for integrated simulations journal January 2010
Experiments and multiscale simulations of laser propagation through ignition-scale plasmas journal September 2007
Three-dimensional HYDRA simulations of National Ignition Facility targets journal May 2001
Hydrodynamics simulations of 2ω laser propagation in underdense gasbag plasmas journal December 2004
Pulsed-power-driven cylindrical liner implosions of laser preheated fuel magnetized with an axial field journal May 2010
Design of magnetized liner inertial fusion experiments using the Z facility journal July 2014
Diagnosing laser-preheated magnetized plasmas relevant to magnetized liner inertial fusion journal December 2015
Laser ionization and heating of gas targets for long‐scale‐length instability experiments journal June 1994
Experimental Demonstration of Fusion-Relevant Conditions in Magnetized Liner Inertial Fusion journal October 2014
Ideal Laser-Beam Propagation through High-Temperature Ignition Hohlraum Plasmas journal February 2007

Cited By (5)

Laser entrance window transmission and reflection measurements for preheating in magnetized liner inertial fusion journal June 2018
One dimensional imager of neutrons on the Z machine journal October 2018
Magnetised thermal self-focusing and filamentation of long-pulse lasers in plasmas relevant to magnetised ICF experiments journal September 2018
Diagnosing and mitigating laser preheat induced mix in MagLIF journal November 2018
Enhancing performance of magnetized liner inertial fusion at the Z facility journal November 2018

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