High-resolution imaging of warm x-ray sources with a Wolter optic on the Z Machine

POSTER

Abstract

We have developed a Wolter optic$^{\mathrm{\thinspace }}$to image warm (\textgreater 15 keV) x-ray sources on the Z Machine, the first-ever instrument of its kind specifically designed and fabricated for HED applications. Adapted from observational astronomy for Z, the optic uses curved x-ray mirrors to form an energy band-limited 2D image of a source with 5-mm FOV and better than measured 100-$\mu $m resolution on-axis. The first images obtained by the instrument of Mo wire array z-pinches on the Z Machine demonstrate unprecedented spatial resolution and signal-to-noise compared to pinhole imaging, revealing small-scale structures not previously observed in these sources.

Authors

  • Jeffrey R. Fein

    SNL, Sandia National Laboratories

  • David Ampleford

    SNL

  • Julia Vogel

    LLNL

  • Bernie Kozioziemski

    LLNL

  • Chris Walton

    LLNL

  • Ming Wu

    SNL

  • Jay Ayers

    Lawrence Livermore National Laboratory, LLNL

  • Chris Ball

    SNL, Sandia National Laboratory

  • Suzanne Romaine

    Harvard-Smithsonian Center for Astrophysics

  • Perry Bell

    LLNL

  • Chris Bourdon

    SNL

  • D. K. Bradley

    LLNL, Lawrence Livermore Natl Lab

  • Ricardo Bruni

    Harvard-Smithsonian Center for Astrophysics

  • Paul Gard

    SNL

  • Clark Highstrete

    Sandia National Laboratories, SNL

  • Kiranmayee Kilaru

    Universities Space Research Association

  • Pat Lake

    SNL, Sandia National Laboratory

  • Andrew Maurer

    SNL

  • L. A. Pickworth

    LLNL, Lawrence Livermore National Lab

  • Michael Pivovaroff

    LLNL

  • Brian Ramsey

    NASA Marshall Space Flight Center