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An Observational Search for the Schuerman Dust Arcs

Published online by Cambridge University Press:  12 April 2016

F. Giovane ,
J.L. Weinberg ,
H.M. Mann  and
J.P. Oliver
F. Giovane
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, U.S.A.
J.L. Weinberg
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, U.S.A.
H.M. Mann
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, U.S.A.
J.P. Oliver
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, U.S.A.

Abstract

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Large-scale interplanetary dust arcs were predicted by Schuerman (1980) to be associated with the planets. An arc, if one exists, would produce asymmetries on opposite sides of the Gegenschein during the Earth’s two passages through the arc each year. A brief description is given of Gegenschein/arc observing constraints, of future viewing opportunities, and of the results of a test program conducted from Mt. Haleakala, Hawaii, in Jan/Feb 1984 when the Earth encountered the arc associated with Saturn.

Type
I. Zodiacal Light and F-Corona: Observations
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 39 - 42
Copyright
Copyright © Reidel 1985

References

Misconi, N.Y.: 1977, Astron. Astrophys., 6l, 497.Google Scholar
Schuerman, D.W.: 1980, Ap. J., 238, 337.Google Scholar
Schwehm, G.H., Giese, R.H., Giovane, F., Schuerman, D.W., and Weinberg, J.L.: 1981, in Adv. Space Res., &1, 121.Google Scholar