16 - 21 June 2024
Yokohama, Japan
Conference 13093 > Paper 13093-42
Paper 13093-42

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

18 June 2024 • 13:20 - 13:40 Japan Standard Time | Room G414/415, North - 4F

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.

Presenter

INAF - Osservatorio Astronomico di Brera (Italy)
Application tracks: Astrophotonics
Presenter/Author
INAF - Osservatorio Astronomico di Brera (Italy)
Author
INAF - Osservatorio Astronomico di Brera (Italy)
Author
INAF - Istituto di Astrofisica Spaziale e Fisica cosmica Milano (Italy)
Author
INAF - Osservatorio Astronomico di Brera (Italy)
Author
Salvatore Incorvaia
INAF - Istituto di Astrofisica Spaziale e Fisica cosmica Milano (Italy)
Author
Luigi Lessio
INAF - Osservatorio Astronomico di Padova (Italy)
Author
INAF - Osservatorio Astronomico di Brera (Italy)
Author
INAF - Osservatorio Astronomico di Brera (Italy)
Author
INAF - Istituto di Astrofisica Spaziale e Fisica cosmica Milano (Italy)
Author
Gabriele Vecchi
INAF - Osservatorio Astronomico di Brera (Italy)