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A Rocket Payload Using Cassegrain-Echelle Optics with Image Intensification for High Resolution Ultraviolet Stellar Spectroscopy

Published online by Cambridge University Press:  14 August 2015

W. M. Burton
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berkshire, England
N. K. Reay
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berkshire, England
D. B. Shenton
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berkshire, England
R. Wilson
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berkshire, England

Abstract

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A description is given of a rocket payload designed to record high resolution ultraviolet stellar spectra using the star-stabilised ‘Skylark’ rocket vehicle. The system consists of a 35 cm aperture f/12 Cassegrain telescope and a spectrometer in which the high spectral dispersion of an echelle grating is crossed with that of a plane grating to separate the echelle orders. The spectrum is focussed onto an electrostatic image intensifier tube, the fibre optic faceplate of which is coated with sodium salicylate to give ultraviolet sensitivity. Photographic film is used to record the two dimensional spectrum array with a resolving power λ/dλ ≃ 104 between 1200 Å and 3000 Å. Efficiency measurements of components indicate that the photometric efficiency of the entire system will allow spectra to be recorded for early-type stars which are brighter than mr ≃ 5.

Type
Part III: UV Astronomy
Copyright
Copyright © Reidel 1971 

References

Burton, W. M. and Reay, N. K.: 1970, Appl. Opt. 9, 1227.Google Scholar
Macchetto, F. M. F.: 1970, (private communication).Google Scholar
Walker, I. F. M. and Abbot, J. K.: 1970 ‘A Star-Pointing attitude Control System for the Skylark Sounding Rocket’. Paper to be presented at the ‘Sounding Rocket Vehicle Technology Specialist Conference’, Williamsburg, Virginia, U.S.A., December 1970.Google Scholar