Paper
27 November 1989 Stanford/Msfc Rocket X-Ray Spectroheliograph
Richard B. Hoover, Arthur B. C. Walker Jr., Joakim F. Lindblom, Troy W. Barbee Jr., Richard A VanPatten, John P. Gill, Forbes Powell, Gordon Steele
Author Affiliations +
Abstract
The first high resolution soft X-ray/EUV images of the Sun with normal incidence multilayer optics were obtained by the Stanford/MSFC Rocket X-Ray Spectroheliograph on October 23, 1987. Numerous images at selected wavelengths from 8 Å to 256 Å were obtained simultaneously by a diverse array of telescopes onboard. These telescopes included single reflection normal incidence multilayer systems (Herschelian), double reflection multilayer systems (Cassegrain), a grazing incidence mirror system (Wolter Schwarzschild), and Spectral Slicing systems using normal incidence multilayer optics in conjunction with the grazing incidence primary (Wolter-Cassegrain). Filters comprised of 1640 - 1720 Å aluminum supported on a nickel mesh were used to transmit the soft X-Ray/EUV radiation while preventing the intense visible light emission of the Sun from fogging the sensitive experimental T-grain photographic emulsions. These systems yielded high resolution soft x-ray/EUV images of the solar corona and transition region, which reveal magnetically confined loops of hot solar plasma, coronal plumes, polar coronal holes, supergranulation, and features associated with overlying cool prominences.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard B. Hoover, Arthur B. C. Walker Jr., Joakim F. Lindblom, Troy W. Barbee Jr., Richard A VanPatten, John P. Gill, Forbes Powell, and Gordon Steele "Stanford/Msfc Rocket X-Ray Spectroheliograph", Proc. SPIE 1140, X-Ray Instrumentation in Medicine and Biology, Plasma Physics, Astrophysics, and Synchrotron Radiation, (27 November 1989); https://doi.org/10.1117/12.961811
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KEYWORDS
Multilayers

Mirrors

Telescopes

Iron

Optical filters

Sun

X-rays

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