Kinematic Alignment and Bonding of Silicon Mirrors for High-Resolution Astronomical X-Ray Optics
Optics for the next generation's high-resolution, high throughput x-ray telescope requires fabrication of well-formed lightweight mirror segments and their integration at arc-second precision. Recent advances in the fabrication of silicon mirrors developed at NASA/Goddard prompted us to develop...
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| creator | Chan, Kai-Wing Mazzarella, James R. Saha, Timo T. Zhang, William W. Mcclelland, Ryan S. Biskack, Michael P. Riveros, Raul E. Allgood, Kim D. Kearney, John D. Sharpe, Marton V. Hlink, Michal Numata, Ai |
| description | Optics for the next generation's high-resolution, high throughput x-ray telescope requires fabrication of well-formed lightweight mirror segments and their integration at arc-second precision. Recent advances in the fabrication of silicon mirrors developed at NASA/Goddard prompted us to develop a new method of mirror alignment and integration. In this method, stiff silicon mirrors are aligned quasi-kinematically and are bonded in an interlocking fashion to produce a "meta-shell" with large collective area. We address issues of aligning and bonding mirrors with this method and show a recent result of 4 seconds-of-arc for a single pair of mirrors tested at soft x-rays. |
| format | Conference Proceeding |
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| language | eng |
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| subjects | Astronomy Nonmetallic Materials Optics |
| title | Kinematic Alignment and Bonding of Silicon Mirrors for High-Resolution Astronomical X-Ray Optics |
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