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Development of a Slitless Spectrograph for X-Ray Astronomy

Published online by Cambridge University Press:  06 March 2019

T. Zehnpfennig*
Affiliation:
American Science and Engineering Cambridge, Massachusetts 02142
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Abstract

The soft x - ray slitless spectrograph is described, and its usefulness in making rapid surveys of wide spectral regions is discussed Fabrication of the 1μ thick gold-shadowed transmission gratings used in the instrument is described. Spectra taken in the laboratory and during a solar sounding rocket flight are presented. Because a simple absorbing strip model is inadequate to explain the distribution of intensities among the spectral orders, a phase-grating model must be adopted.

Type
Research Article
Copyright
Copyright © International Centre for Diffraction Data 1969

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References

1. Gursky, H. and Zehnpfennig, T., “An Image-Forming Slitless Spectrometer for Soft X-Ray Astronomy,” Appl, Opt. 5:875876, (1966).Google Scholar
2. Zehnpfennig, T., “A Functioning Model of the Soft X-Ray Slitless Spectrometer,” Appl. Opt. 5:18551856, (1966).Google Scholar
3. Vaiana, G. S., Reidy, W. P., Zehnpfennig, T., Van Speybroeck, L., and Giacconi, R., “X-Ray Structures of the Sun during the Importance IN Flare of 8 June 1968,Science 161:564567, (1968).Google Scholar
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7. Electron microscope pictures of the gratings were supplied by Jeolco (U.S.A.) Inc., Medford, Massachusetts.Google Scholar
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