Paper
16 September 1992 Structural mechanics of the solar-A Soft X-ray Telescope
Bruce K. Jurcevich, Marilyn E. Bruner, K. F. Gowen
Author Affiliations +
Abstract
The Soft X-ray Telescope (SXT) is one of four major instruments that constitute the payload of the NASA-Japanese mission YOHKOH (formerly known as Solar-A), scheduled to be launched in August, 1991. This paper describes the design of the SXT, the key system requirements, and the SXT optical and structural systems. Particular attention is given to the design considerations for stiffness and dimensional stability, temperature compensation, and moisture sensitivyty control. Consideration is also given to the X-ray mirror, the aspect telescope, the entrance filters, the mechanical structure design, the aft support plate and mount, the SXT finite element model, and other subsystems.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bruce K. Jurcevich, Marilyn E. Bruner, and K. F. Gowen "Structural mechanics of the solar-A Soft X-ray Telescope", Proc. SPIE 1690, Design of Optical Instruments, (16 September 1992); https://doi.org/10.1117/12.138014
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Optical instrument design

X-rays

Optical components

Space telescopes

X-ray telescopes

Objectives

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