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The Change in Near-Ecliptic Zodiacal Light Brightness with Heliocentric Distance

Published online by Cambridge University Press:  12 April 2016

G.N. Toller
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.
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Abstract

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Background starlight observed by the Pioneer 10 Imaging Photopolarimeter from beyond the asteroid belt is used to isolate zodiacal light in Pioneer observations at heliocentric distances R between 1 and 3 AU. Near-ecliptic zodiacal light brightness data in the range 65° to 180° elongation ε are used to depict changes in the shape of the zodiacal light with ε and R and are compared to the corresponding views seen from the Earth and from the Helios 1 and 2 spacecraft.

Type
I. Zodiacal Light and F-Corona: Observations
Copyright
Copyright © Reidel 1985

References

Hanner, M.S., Sparrow, J.G., Weinberg, J.L., Beeson, D.E.: 1916, in Lecture Notes in Physics, No. 48, 29 (Springer-Verlag).Google Scholar
Hanner, M.S., Weinberg, J.L., DeShields, L.M., Green, B.A., Toller, G.N: 1974, J. Geophys. Res., 79, 3671.CrossRefGoogle Scholar
Leinert, C., Richter, I., Pitz, E., Planck, B.: 1981, Astron. Astrophys., 103, 177.Google Scholar
Levasseur-Regourd, A.C., Dumont, R.: 1980, Astron. Astrophys., 84, 277.Google Scholar
Link, H., Leinert, C., Pitz, E., Salm, N.: 1976, in Lecture Notes in Physics, No. 48, 24 (Springer-Verlag).Google Scholar
Schuerman, D.W., Weinberg, J.L., Beeson, D.E.: 1977, B.A.A.S., 2, 313.Google Scholar
Toller, G.N: 1981, Dissertation, State Univ. of N.Y. at Stony Brook.Google Scholar
Weinberg, J.L., Hanner, M.S., Mann, H.M., Hutchison, P.B., Fimmel, R.: 1973, Space Res. XIII, 1187.Google Scholar
Weinberg, J.L., Hanner, M.S., Beeson, D.E., DeShields, L.M., Green, B.A: 1974, J. Geophys. Res. 739, 3665.CrossRefGoogle Scholar
Weinberg, J.L., Sparrow, J.G: 1978, in Cosmic Dust, 75 (Wiley- Interscience).Google Scholar
Weinberg, J.L: 1981, Skt and Tel. 61, 114.Google Scholar
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