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Synthetic Maps of the Brightness and Polarization of the F-Corona
Published online by Cambridge University Press: 12 April 2016
Abstract
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