Improvements to the FLASH code for Simulating HEDP Experiments

POSTER

Abstract

FLASH is an open source, compressible spatially adaptive radiation magnetohydrodynamics code that incorporates capabilities for a broad range of physical processes, performs well on a wide range of existing advanced computer architectures, and has a broad user base. Capabilities have been incorporated into the FLASH code to enable simulations of laser-driven HEDP experiments. We summarize recent improvements to the HEDP capabilities of the FLASH code and present results from several collaborations that use FLASH to simulate HEDP experiments. The ray trace that package models laser energy deposition has been substantially improved. Methods have been added for smoothing laser deposition and a ``3D-in-2D'' ray trace has been added for improved accuracy in 2D cylindrical simulations. Numerous improvements have been made to the FLASH MHD solver, including support for 2D cylindrical geometry and magnetic resistivity. Post-processing scripts have been generated that enables the SPECT3D simulated diagnostic software to operate on FLASH output. The results of several verification tests will also be presented.

*This work was supported in part at the University of Chicago by the DOE NNSA ASC through the Argonne Institute for Computing in Science under field work proposal 57789; and the NSF under grant PHY-0903997.

Authors

  • Milad Fatenejad

    • The Flash Center for Computational Science, University of Chicago
    • University of Chicago
  • John Bachan

    • University of Chicago
  • Sean Couch

    • University of Chicago
  • Chris Daley

    • University of Chicago
  • Anshu Dubey

    • University of Chicago
  • Norbert Flocke

    • University of Chicago
  • Carlo Graziani

    • University of Chicago
  • Don Lamb

    • University of Chicago
  • Dongwook Lee

    • University of Chicago
  • Anthony Scopatz

    • University of Chicago
  • Petros Tzeferacos

    • University of Chicago
  • Klaus Weide

    • University of Chicago