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High-Resolution, Lightweight, and Low-cost X-Ray Optics for the Lynx Observatory

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TLDR
An approach to build an x-ray mirror assembly that can meet Lynx’s requirements of high-angular resolution, large effective area, light weight, short production schedule, and low-production cost is described.
Abstract
We describe an approach to build an x-ray mirror assembly that can meet Lynx’s requirements of high-angular resolution, large effective area, light weight, short production schedule, and low-production cost. Adopting a modular hierarchy, the assembly is composed of 37,492 mirror segments, each of which measures ∼100  mm  ×  100  mm  ×  0.5  mm. These segments are integrated into 611 modules, which are individually tested and qualified to meet both science performance and spaceflight environment requirements before they in turn are integrated into 12 metashells. The 12 metashells are then integrated to form the mirror assembly. This approach combines the latest precision polishing technology and the monocrystalline silicon material to fabricate the thin and lightweight mirror segments. Because of the use of commercially available equipment and material and because of its highly modular and hierarchical building-up process, this approach is highly amenable to automation and mass production to maximize production throughput and to minimize production schedule and cost. As of fall 2018, the basic elements of this approach, including substrate fabrication, coating, alignment, and bonding, have been validated by the successful building and testing of single-pair mirror modules. In the next few years, the many steps of the approach will be refined and perfected by repeatedly building and testing mirror modules containing progressively more mirror segments to fully meet science performance, spaceflight environments, as well as programmatic requirements of the Lynx mission and other proposed missions, such as AXIS.

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Next Generation X-Ray Optics: High-Resolution, Light-Weight, and Low-Cost

TL;DR: In this article, the authors describe a comprehensive program to advance the technology for x-ray telescopes well beyond the state of the art represented by the three currently operating missions: Chandra, XMM-Newton, and Suzaku.
Proceedings ArticleDOI

Progress in x-ray critical-angle transmission grating technology development

TL;DR: In this article, the critical-angle transmission (CAT) grating technology has been proposed for soft x-ray spectroscopy, which combines the advantages of traditional transmission gratings and blazed reflection gratings (high diffraction efficiency, high resolving power R due to blazing into high orders).
Journal ArticleDOI

Design and Fabrication Technology of Metal Mirrors Based on Additive Manufacturing: A Review

TL;DR: In this paper, a review of AM technologies and powder materials for metal mirrors, recent advances in optomechanical design methods for AM metal mirror, challenges faced by AM metal mirrors in fabricating, and future trends in AM metal metal mirrors.
References
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Journal ArticleDOI

A “telescope” for soft X‐ray astronomy

TL;DR: In this article, the authors describe the design of an X-ray "telescope" and analyze some of its characteristics, including the characteristics of the parabolic mirror, which can be used to observe soft X rays from extraterrestrial sources.
Journal ArticleDOI

Design, construction, and performance of the ROSAT high-resolution x-ray mirror assembly

Bernd Aschenbach
- 15 Apr 1988 - 
TL;DR: A grazing incidence telescope has been developed for the x-ray astronomy satellite ROSAT including a verification model and a flight model that indicates an even better performance.
Proceedings ArticleDOI

Performance expectation versus reality

TL;DR: The AXAF high resolution mirror assembly (HRMA) is complete and has been tested at the NASA Marshall Space Flight Center (MSFC) X-ray Calibration Facility (XRCF) as mentioned in this paper.
Proceedings ArticleDOI

Fabrication of the NuSTAR flight optics

TL;DR: The NuSTAR flight optics modules are glass-graphite-epoxy-composite structures to be employed for the first time in space-based X-ray optics by NuSTAR, a NASA Small Penetrator Space Explorer schedule for launch in February 2012.
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