Paper
9 August 1979 Paraboloidal X-Ray Telescope Mirror For Solar Coronal Spectroscopy
W. A. Brown, E. C. Bruner Jr., L. W. Acton, A. Franks, M. Stedman, R. J. Speer
Author Affiliations +
Proceedings Volume 0184, Space Optics Imaging X-Ray Optics Workshop; (1979) https://doi.org/10.1117/12.957462
Event: 1979 Huntsville Technical Symposium, 1979, Huntsville, United States
Abstract
The telescope mirror for the X-Ray Spectrograph Spectrometer Telescope System is a sixty degree sector of an extreme off-axis paraboloid of revolution. It was designed fo focus a coronal region 1 by 10 arc seconds in size on the entrance slit of the spectrometer after reflection from the gold surface at a glancing angle of about 2.9 degrees. This paper discusses the design, manufacture, and metrology of the mirror, the methods of precision mechanical metrology used to focus the system, the mounting system which serves to locate the mirror and has proven itself through several vibration tests, and the results of reflection efficiency measurements at 8 and 44 Angstroms, and alignment tolerances and ray trace analysis of the effects of misalignment. The mirror was developed under NASA Contract NAS2-9181.
© (1979) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
W. A. Brown, E. C. Bruner Jr., L. W. Acton, A. Franks, M. Stedman, and R. J. Speer "Paraboloidal X-Ray Telescope Mirror For Solar Coronal Spectroscopy", Proc. SPIE 0184, Space Optics Imaging X-Ray Optics Workshop, (9 August 1979); https://doi.org/10.1117/12.957462
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Spectroscopy

X-ray telescopes

Metrology

Optical alignment

Space telescopes

X-ray optics

Back to Top