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Method for the Determination of Density and Phase Functions of Interplanetary Dust

Published online by Cambridge University Press:  14 August 2015

A. Mujica ,
G. Lôpez  and
F. Sánchez
A. Mujica
Affiliation:
Instituto de Astrofísica de Canarias. C.S.I.C. Universidad de La Laguna. España
G. Lôpez
Affiliation:
Instituto de Astrofísica de Canarias. C.S.I.C. Universidad de La Laguna. España
F. Sánchez
Affiliation:
Instituto de Astrofísica de Canarias. C.S.I.C. Universidad de La Laguna. España

Summary

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A method of determination of the scattered light intensity, , by a unit-volume of interplanetary space is presented. From ground base Zodiacal Light measurements and the experimental results of Pioneer X the density, ρ(r), and phase, σ(θ), functions are obtained without any previous assumptions about them.

Type
I: Zodiacal Light - Measurements and Models
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 55 - 60
Copyright
Copyright © Reidel 1980 

References

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