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Wavelength Dependent Models of the Zodiacal Light

Published online by Cambridge University Press:  14 August 2015

H. J. Staude  and
S. Röser
H. J. Staude
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg-Königstuhl
S. Röser
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg

Extract

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We discuss the significance of our zodiacal light models, which are based on Mie theory and refractive indices measured in the range 0.15 μm ≤ λ ≤ 100 μm. The models include scattering and thermal emission. They are absolute, since particle number density at 1 AU, size distribution and radial density gradient in the Ecliptic are fixed by lunar microcrater counts and by Helios and Pioneer results. The only free parameter is the chemical composition of the dust.

Type
II: Meteors and Meteorites
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 81 - 84
Copyright
Copyright © Reidel 1980 

References

Briotta, D.A.: 1976, , Google Scholar
Giese, R.H., Grün, E.: 1976, Proc. IAU Coll. No. 31, “Interplanetary Dust and Zodiacal Light”, Eds. Elsässer, H. and Fechtig, H., pp. 135–139 CrossRefGoogle Scholar
Leinert, C.: 1975, Space Sci. Rev. 18, pp. 281–339 CrossRefGoogle Scholar
Röser, S., Staude, H.J.: 1978, Astron. Astrophys. 67, pp. 381–394 Google Scholar
Röser, S., Staude, H.J.: 1979, Astron. Astrophys. 71, p. 269 Google Scholar