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Synthetic Maps of the Brightness and Polarization of the F-Corona

Published online by Cambridge University Press:  12 April 2016

Y. Fang ,
P.L. Lamy  and
A. Llebaria
Y. Fang
Affiliation:
Laboratoire d’Astronomie Spatiale Les Trois Lues 13012 Marseille, France
P.L. Lamy
Affiliation:
Laboratoire d’Astronomie Spatiale Les Trois Lues 13012 Marseille, France
A. Llebaria
Affiliation:
Laboratoire d’Astronomie Spatiale Les Trois Lues 13012 Marseille, France

Abstract

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The Wide-Field Light and Spectrometric Coronograph (LASCO) to be flown on SOHO in 1995 is designed to perform accurate photopolarimetric observations of the solar corona. For simulation purpose but also to have a two-dimensional model of the F-corona, we have realized synthetic maps of its brightness and polarization

Type
Interplanetary Dust: Zodiacal Light and Optical Studies
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 195 - 198
Copyright
Copyright © Kluwer 1991

References

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