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A Method for Deriving the Mean Volume Scattering Phase Function for Zodiacal Dust

Published online by Cambridge University Press:  12 April 2016

S.S. Hong
S.S. Hong*
Affiliation:
Space Astronomy Laboratory, University of Florida, 1810 NW 6th Street Gainesville, Florida 32609, USA

Abstract

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A linear combination of 3 Henyey-Greenstein phase functions is substituted for the mean volume scattering phase function in the zodiacal light brightness integral. Results of the integral are then compared with the observed brightness to form residuals. Minimization of the residuals provides us with the best combination of Henyey-Greenstein functions for the scattering phase function of zodiacal dust particles.

Type
IV. Optical Studies of Dust
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 215 - 218
Copyright
Copyright © Reidel 1985

References

Dumont, R., Sánchez, F.: 1975, Astron. Astrophys. 38, 405.Google Scholar
Dumont, R.: 1976, in Interplanetary Dust and Zodiacal Light, Lecture Notes in Physics 48, ed. by Elsasser, H. and Fechtig, H., p. 115.Google Scholar
Leinert, C., Link, H., Pitz, E., Giese, R.H.: 1976, Astron, Astrophys. 47, 221.Google Scholar