Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session BP11: Poster Session I: HEDP; General Stellarator; Wendelstein 7-X; Heating, Current Drive, and Energetic Ions (9:30am-12:30pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.BP11.4
Abstract: BP11.00004 : Improvements to the VISAR and Streaked Optical Pyrometer at the Omega Laser Facility*
Presenter:
Mary Kate Ginnane
(Laboratory for Laser Energetics, U. of Rochester)
Authors:
Mary Kate Ginnane
(Laboratory for Laser Energetics, U. of Rochester)
Andrew Sorce
(Laboratory for Laser Energetics, U. of Rochester)
Joshua Kendrick
(Laboratory for Laser Energetics, U. of Rochester)
Robert Boni
(Laboratory for Laser Energetics, U. of Rochester)
Benjamin Saltzman
(Laboratory for Laser Energetics, U. of Rochester)
David Weiner
(Laboratory for Laser Energetics, U. of Rochester)
Mohamed Zaghoo
(Laboratory for Laser Energetics, U. of Rochester)
Danae N Polsin
(Laboratory for Laser Energetics, U. of Rochester)
Brian Henderson
(Laboratory for Laser Energetics, U. of Rochester)
Jun Zou
(Laboratory for Laser Energetics, U. of Rochester)
Michael Couch
(Laboratory for Laser Energetics, U. of Rochester)
Michelle C Gregor
(Lawrence Livermore Natl Lab)
Craig Rogoff
(Laboratory for Laser Energetics, U. of Rochester)
Thomas Boehly
(Laboratory for Laser Energetics, U. of Rochester)
James R Rygg
(Laboratory for Laser Energetics, U. of Rochester)
Gilbert W Collins
(Laboratory for Laser Energetics, U. of Rochester)
VISAR and optical pyrometry measurements are mainstay of high-energy-density physics experiments. These systems on OMEGA share an optical telescope to relay probe beam and optical signals to their respective detectors. The telescope, originally optimized for 532 nm, was redesigned to provide better performance for 600 to 900 nm and include a baffle system that reduces signal from outside the field of view. This poster provide an overview of these refinements and an update on recent calibrations.
*This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE‑NA0001944.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.4
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