A high resolution large x-ray mission based on thin glass: optomechanical design

The technology of X-ray optics based on very thin glass sheets curved on mandrels figured to an optical quality have been quickly developed in these last years, as the on flight NUSTAR or the glass solutions for the IXO mission have demonstrated. Different possibilities to freeze the correct shape can be chosen and the constrains to the glass can widely affect the response in term of strength and quality. This study shows the opto-mechanical performances of the design based on the hot slumped glass sheets stiffed with reinforcing ribs. With this concept a glass stack can be integrated into a mechanical structure in order to form a module that can be assembled in a large structure. The considered input data and requirements are those specified for the proposed Athena mission. Different types of materials are considered following the latest progress in the slumping and the availability of alternative tougher glass. Static and dynamic FE analyses coupled with ray-tracing are performed in order to reach a high resolution (less than 5 arcsec). Also an optimization of the ribs distribution is implemented in function of the radius of curvature.

[1]  Paolo Conconi,et al.  Accurate integration of segmented x-ray optics using interfacing ribs , 2013 .

[2]  Marcos Bavdaz,et al.  Design, fabrication, and characterization of silicon pore optics for ATHENA/IXO , 2011, Optical Engineering + Applications.

[3]  Paolo Conconi,et al.  Hot slumping glass technology for the grazing incidence optics of future missions with particular reference to IXO , 2010, Astronomical Telescopes + Instrumentation.

[4]  Marcos Bavdaz,et al.  In focus measurements of IXO type optics using the new PANTER x-ray test facility extension , 2013, Optics & Photonics - Optical Engineering + Applications.

[5]  Kazuhiko Ohno,et al.  NT-SiC (new-technology silicon carbide) : Φ 650mm optical space mirror substrate of high-strength reaction-sintered silicon carbide , 2005, SPIE Optics + Photonics.

[6]  M. Ghigo,et al.  Evaluation of the surface strength of glass plates shaped by hot slumping process , 2013, Optics & Photonics - Optical Engineering + Applications.

[7]  P. Gondoin,et al.  XMM-Newton observatory. I. The spacecraft and operations , 2001 .

[8]  Joseph L. Robichaud,et al.  Silicon carbide optics for space and ground based astronomical telescopes , 2012, Other Conferences.

[9]  Joern Wilms,et al.  The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission , 2013 .

[10]  Giovanni Pareschi,et al.  Production of thin glass mirrors by hot slumping for x-ray telescopes: present process and ongoing development , 2014, Astronomical Telescopes and Instrumentation.

[11]  Paolo Conconi,et al.  Design of the IXO optics based on thin glass plates connected by reinforcing ribs , 2011, Optical Engineering + Applications.

[12]  Haruyoshi Katayama,et al.  Manufacturing and optical testing of 800 mm lightweight all C/SiC optics , 2013, Optics & Photonics - Optical Engineering + Applications.

[13]  Paolo Conconi,et al.  Development of high angular resolution x-ray telescopes based on slumped glass foils , 2012, Other Conferences.

[14]  Marcos Bavdaz,et al.  Direct hot slumping and accurate integration process to manufacture prototypal x-ray optical units made of glass , 2013, Optics & Photonics - Optical Engineering + Applications.

[15]  Peter Mao,et al.  The Nuclear Spectroscopic Telescope Array (NuSTAR) , 2010, Astronomical Telescopes + Instrumentation.