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Proceedings Article

Super-X: a soft x-ray telescope for Solar-B

[+] Author Affiliations
Loren W. Acton

Montana State Univ. (USA)

Jay A. Bookbinder, Leon Golub

Harvard-Smithsonian Ctr. for Astrophysics (USA)

Marilyn E. Bruner, James R. Lemen

Lockheed Martin Palo Alto Advanced Technology Ctr. (USA)

Proc. SPIE 3442, Missions to the Sun II, 140 (November 2, 1998); doi:10.1117/12.330250
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From Conference Volume 3442

  • Missions to the Sun II
  • Clarence M. Korendyke
  • San Diego, CA | July 19, 1998


This paper describes the conceptual design of a soft x-ray telescope, super-x, which we will propose for the Japan/US/UK Solar-B mission. Super-X will break new ground in both angular resolution and solar coronal temperature discrimination. The telescope design is based upon the successful transition region and coronal explorer instrument. It features four XUV spectral channels spanning the 0.3 to 20 MK temperature range with an angular resolution of approximately 0.27 seconds of arc. We will describe considerations affecting spectral line selection and some details of the characteristics of the instrument.

© (1998) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.

Loren W. Acton ; Jay A. Bookbinder ; Marilyn E. Bruner ; Leon Golub and James R. Lemen
"Super-X: a soft x-ray telescope for Solar-B", Proc. SPIE 3442, Missions to the Sun II, 140 (November 2, 1998); doi:10.1117/12.330250; http://dx.doi.org/10.1117/12.330250

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