Hostname: page-component-cd9895bd7-p9bg8 Total loading time: 0 Render date: 2024-12-12T12:53:39.612Z Has data issue: false hasContentIssue false
  • English
  • Français

Spatially Varying Optical Properties of the Zodiacal Dust

Published online by Cambridge University Press:  14 August 2015

S. S. Hong  and
S. M. Kwon
S. S. Hong
Affiliation:
Department of Astronomy, Seoul National University, Korea
S. M. Kwon
Affiliation:
Space Astronomy Laboratory, University of Florida, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Analyses of both the zodiacal light in the visible and the zodiacal emission in the infrared have provided us with ample evidence to claim that the interplanetary dust particles are mixtures or coagulations of more than one constituents and their mixing ratios vary with the distance from the sun.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 267 - 272
Copyright
Copyright © Kluwer 1989

References

Dumont, R. and Levasseur-Regourd, A.-C. 1988, Astr. Ap., 191, 154.Google Scholar
Giese, R. H. and Dziembowski, C.V. 1969, Planet. Space Sci., 17, 949.CrossRefGoogle Scholar
Hauser, M. G. et al 1984, Ap.J., 278, L15.Google Scholar
Hauser, M. G. and Vrtilek, J. M. 1988, a paper presented to the commission 21 meeting of the 20th IAU.Google Scholar
Hong, S. S. 1985, Astr. Ap., 146, 67.Google Scholar
Hong, S. S. and Um, I. K. 1987, Ap.J., 320, 928.Google Scholar
Leinert, C., Richter, I., Pitz, E., and Planck, B. 1981, Astr. Ap., 103, 177.Google Scholar
Murdock, T. L. and Price, S. D. 1985, A. J., 90., 375.Google Scholar
Weinberg, J. L. and Sparrow, J. G. 1978, in Cosmic Dust ed. by McDonell, J. A. M. (New York: Wiley), p.75.Google Scholar