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Toward the fabrication of a 5 μm resolution Wolter microscope for the National Ignition FacilityAdvancements in computer-controlled polishing, metrology, and replication have led to a x-ray mirror fabrication
process that is capable of producing high-resolution Wolter microscopes. The mirror is a nickel-cobalt
replicated full-shell mirror that was electroformed from a finely figured and polished mandrel. This mandrel
was designed and fabricated for a 8 m source-to-detector distance microscope, with 10× magnification. A
computer controlled polishing process corrected the low-frequency mandrel figure to < 2.0 nm RMS error.
The mandrel design was optimized to reduce shell distortions that occur mainly < 20 mm from the shell ends.
This design, in combination with improved replication tooling design and refined bath parameters informed
by a detailed COMSOL model, have led to reductions in replication errors in the mirror shell. X-ray tests
performed on a pair of mirror shells replicated from the mandrel have demonstrated < 10 μm FWHM source
plane imaging resolution. Here we discuss the development process, highlight results from metrology and
x-ray testing, and define a path for achieving 5 μm FWHM resolution.
Document ID
20220008583
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Patrick R Champey
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Jeffery Kolodziejczak
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Bernard Kozioziemski
(Lawrence Livermore National Laboratory Livermore, California, United States)
Jackie Davis
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Charles Griffith
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Tom Kester
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Kiranmayee Kilaru
(Universities Space Research Association Columbia, Maryland, United States)
Amy Meekham
(Jacobs Space Exploration Group)
Joe Menapace
(Lawrence Livermore National Laboratory Livermore, California, United States)
Brian Ramsey
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Oliver J Roberts
(Universities Space Research Association Columbia, Maryland, United States)
Javier Sanchez
(Jacobs Space Exploration Group Livermore, California, United States)
Panini Singam
(Oak Ridge Associated Universities Oak Ridge, Tennessee, United States)
W Scott Smith
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Chet Speegle
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Mark Stahl
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Tayyab Suratwala
(Lawrence Livermore National Laboratory Livermore, California, United States)
Nick Thomas
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Mark Young
(Jacobs Space Exploration Group)
Julia K Vogel
(Lawrence Livermore National Laboratory Livermore, California, United States)
Date Acquired
May 31, 2022
Subject Category
Astrophysics
Meeting Information
Meeting: High Temperature Plasma Diagnostics Conference 2022
Location: Rochester, NY
Country: US
Start Date: May 16, 2022
End Date: May 19, 2022
Sponsors: University of Rochester
Funding Number(s)
WBS: 199008.02.08.11.ST4F.20
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
Grazing Incidence, Wolter Microscope, X-ray Optics
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