Paper
1 January 1992 Narrow-band solar images in the soft x-ray regime with multilayer optics
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Abstract
High quality multilayers with 2d spacings as short as about 44 A have been used successfully for astronomical observations. Observation of both the sun and cosmic X-ray sources (for which radiation longward of the carbon edge at about 44 A is strongly attenuated by interstellar matter) are possible at wavelengths shorter than 40 A with current multilayer technology, if mirrors are used at nonnormal angles of incidence. We discuss several configurations which are suitable for high resolution solar imaging observations in the wavelength interval between 0.5 and 50 A. We also describe the design and anticipated performance of a multilayer optical system we are currently developing for a rocketborne solar observatory.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Arthur B. C. Walker II, Charles C. Kankelborg, Richard B. Hoover, Troy W. Barbee Jr., and Phillip C. Baker "Narrow-band solar images in the soft x-ray regime with multilayer optics", Proc. SPIE 1546, Multilayer and Grazing Incidence X-Ray/EUV Optics, (1 January 1992); https://doi.org/10.1117/12.51253
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KEYWORDS
Mirrors

Multilayers

Telescopes

Iron

X-ray optics

Image resolution

X-rays

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