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Proceedings Paper

Design and development of thin quartz glass WFXT polynomial mirror shells by direct polishing
Author(s): L. Proserpio; S. Campana; O. Citterio; M. Civitani; H. Combrinck; P. Conconi; V. Cotroneo; R. Freeman; P. Langstrof; E. Mattaini; R. Morton; B. Oberle; G. Pareschi; G. Parodi; C. Pels; C. Schenk; R. Stock; G. Tagliaferri
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Paper Abstract

The Wide Field X-ray Telescope (WFXT) is a medium class mission for X-ray surveys of the sky with an unprecedented area and sensitivity. In order to meet the effective area requirement, the design of the optical system is based on very thin mirror shells, with thicknesses in the 1-2 mm range. In order to get the desired angular resolution (10 arcsec requirement, 5 arcsec goal) across the entire 1x1 degree FOV (Field Of View), the design of the optical system is based on nested modified grazing incidence Wolter-I mirrors realized with polynomial profiles, focal plane curvature and plate scale corrections. This design guarantees an increased angular resolution at large off-axis angle with respect to the normally used Wolter I configuration, making WFXT ideal for survey purposes. The WFXT X-ray Telescope Assembly is composed by three identical mirror modules of 78 nested shells each, with diameter up to 1.1 m. The epoxy replication process with SiC shells has already been proved to be a valuable technology to meet the angular resolution requirement of 10 arcsec. To further mature the telescope manufacturing technology and to achieve the goal of 5 arcsec, a deterministic direct polishing method is under investigation. The direct polishing method has already been used for past missions (as Einstein, Rosat, Chandra): the technological challenge now is to apply it for almost ten times thinner shells. Under investigation is quartz glass (fused silica), a well-known material with good thermo-mechanical and polishability characteristics that could meet our goal in terms of mass and stiffness, with significant cost and time saving with respect to SiC. Our approach is based on two main steps: first quartz glass tubes available on the market are grinded to conical profiles, and second the obtained shells are polished to the required polynomial profiles by CNC (Computer Numerical Control) polishing machine. In this paper, the first results of the direct grinding and polishing of prototypes shells made by quartz glass with low thickness, representative of the WFXT optical design, are presented.

Paper Details

Date Published: 29 July 2010
PDF: 14 pages
Proc. SPIE 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 77320D (29 July 2010); doi: 10.1117/12.857418
Show Author Affiliations
L. Proserpio, Osservatorio Astronomico di Brera (Italy)
Insubria Univ. (Italy)
S. Campana, Osservatorio Astronomico di Brera (Italy)
O. Citterio, Osservatorio Astronomico di Brera (Italy)
M. Civitani, Osservatorio Astronomico di Brera (Italy)
Insubria Univ. (Italy)
H. Combrinck, Zeeko Ltd. (United Kingdom)
P. Conconi, Osservatorio Astronomico di Brera (Italy)
V. Cotroneo, Osservatorio Astronomico di Brera (Italy)
R. Freeman, Zeeko Ltd. (United Kingdom)
P. Langstrof, Heraeus Quarzglas GmbH & Co. KG (Germany)
E. Mattaini, INAF - IASF Milano (Italy)
R. Morton, Zeeko Ltd. (United Kingdom)
B. Oberle, Heraeus Quarzglas GmbH & Co. KG (Germany)
G. Pareschi, Osservatorio Astronomico di Brera (Italy)
G. Parodi, BCV Progetti S.r.l. (Italy)
C. Pels, Heraeus Quarzglas GmbH & Co. KG (Germany)
C. Schenk, Heraeus Quarzglas GmbH & Co. KG (Germany)
R. Stock, Heraeus Quarzglas GmbH & Co. KG (Germany)
G. Tagliaferri, Osservatorio Astronomico di Brera (Italy)


Published in SPIE Proceedings Vol. 7732:
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
Monique Arnaud; Stephen S. Murray; Tadayuki Takahashi, Editor(s)

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