Advancing towards a swift, deterministic, and reliable process for high-resolution thin monolithic shells

The traditional approach for creating very large X-ray mirror modules (with diameters exceeding 1 meter) involves dividing the optics into azimuthal and radial modules, similar to the Silicon Pore Optics used in Athena. While this method addresses the initial challenges of procuring and handling very large substrates, it introduces complexities in the later stages, particularly when thousands of segments must be assembled without compromising their optical performance. In contrast, a simpler design for large mirror modules could involve fewer than a few hundred thin monolithic shells (2-4 mm for mirror shells ranging from 0.4 to 3 meters in diameter). This configuration offers the dual benefits of design simplicity and high-resolution capability, achieved through direct polishing. Additionally, it significantly reduces the polishing time. In Italy, a technology development roadmap for this approach is being funded by ASI and led by INAF-OABrera. In this paper, we present the advancements made in the various phases of this process and in the procurement of new substrates.

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Published
2024-08-21
DOI
https://doi.org/10.1117/12.3019155
Primary Topic
Manufacturing Process and Optimization
Type
article
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article

Advancing towards a swift, deterministic, and reliable process for high-resolution thin monolithic shells

G. Vecchi, M. Civitani, Giorgio Toso, Giovanni Pareschi et al.
Manufacturing Process and Optimization
article

Advancing towards a swift, deterministic, and reliable process for high-resolution thin monolithic shells

G. Vecchi, M. Civitani, Giorgio Toso, Giovanni Pareschi, Stefano Basso, Salvatore Incorvaia, M. Ghigo, M. Fiorini, Daniele Spiga, Luigi Lessio
article en

Abstract

The traditional approach for creating very large X-ray mirror modules (with diameters exceeding 1 meter) involves dividing the optics into azimuthal and radial modules, similar to the Silicon Pore Optics used in Athena. While this method addresses the initial challenges of procuring and handling very large substrates, it introduces complexities in the later stages, particularly when thousands of segments must be assembled without compromising their optical performance. In contrast, a simpler design for large mirror modules could involve fewer than a few hundred thin monolithic shells (2-4 mm for mirror shells ranging from 0.4 to 3 meters in diameter). This configuration offers the dual benefits of design simplicity and high-resolution capability, achieved through direct polishing. Additionally, it significantly reduces the polishing time. In Italy, a technology development roadmap for this approach is being funded by ASI and led by INAF-OABrera. In this paper, we present the advancements made in the various phases of this process and in the procurement of new substrates.

Brera Astronomical Observatory (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano (IT), Osservatorio Astronomico di Padova (IT)
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