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Ground-Based Observations of Near Ecliptic Zodiacal Light Brightness

Published online by Cambridge University Press:  12 April 2016

Nebil Y. Misconi  and
J.L. Weinberg
Nebil Y. Misconi
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, USA
J.L. Weinberg
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, USA

Abstract

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Ground-based observations of the evening zodiacal light taken by Weinberg and Mann from Mt. Haleakala, Hawaii, during March 1966 are used to derive a table of zodiacal light brightnesses at high spatial resolution (as little as 0.5° in differential ecliptic longitude λ−λ⊙ and 1.0° in ecliptic latitude β) over the region 29. 5°< λ−λ⊙ < 56°, −30°< β <30°. Significant differences are found in the brightness distributions above and below the ecliptic plane.

Type
I. Zodiacal Light and F-Corona: Observations
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 11 - 15
Copyright
Copyright © Reidel 1985

References

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Weinberg, J.L. and Mann, H.M., in Proc., Symp. on the Zodiacal Light and the Interplanetary Medium, NASA SP-150, ed. Weinberg, J.L., p. 3, 1967.Google Scholar