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Planned Observations of the Diffuse Sky Radiation During Shuttle Mission STS-4

Published online by Cambridge University Press:  14 August 2015

J. L. Weinberg ,
R. C. Hahn ,
F. Giovane  and
D. W. Schuerman
J. L. Weinberg
Affiliation:
Space Astronomy Laboratory, State University of N. Y. at Albany, Albany, N. Y. 12203
R. C. Hahn
Affiliation:
Space Astronomy Laboratory, State University of N. Y. at Albany, Albany, N. Y. 12203
F. Giovane
Affiliation:
Space Astronomy Laboratory, State University of N. Y. at Albany, Albany, N. Y. 12203
D. W. Schuerman
Affiliation:
Space Astronomy Laboratory, State University of N. Y. at Albany, Albany, N. Y. 12203

Abstract

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The Skylab flight spare 10-color photopolarimeter (Weinberg, et al., 1975; Sparrow, et al., 1977) is being refurbished for use in Space Shuttle mission STS-4, a test flight currently scheduled for October 1980. Observations will be made of zodiacal light, background starlight, and the Shuttle-induced atmosphere (spacecraft corona), with emphasis on regions of sky closer than 90° to the sun.

Type
I: Zodiacal Light - Measurements and Models
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 25 - 28
Copyright
Copyright © Reidel 1980 

References

Henize, K.G. and Weinberg, J.L.: 1973, Sky Telesc. 45, pp. 2–6.Google Scholar
Sparrow, J.G., Weinberg, J.L., and Hahn, R.C.: 1977, Applied Optics 16, pp. 978–982.CrossRefGoogle Scholar
Weinberg, J.L., Sparrow, J.G., and Hahn, R.C.: 1975, Space Sci. Instr. 1, pp. 407–418.Google Scholar