2 November 1998 Super-X: a soft x-ray telescope for Solar-B
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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 Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Loren W. Acton, Jay A. Bookbinder, Marilyn E. Bruner, Leon Golub, James R. Lemen, "Super-X: a soft x-ray telescope for Solar-B", Proc. SPIE 3442, Missions to the Sun II, (2 November 1998); doi: 10.1117/12.330250; https://doi.org/10.1117/12.330250


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