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Zodiacal Light - Scattered Fraunhofer Line Profiles
Published online by Cambridge University Press: 27 February 2018
Abstract
The scattering function of Hong's successful model for the brightness variation with elongation, B(ε), of the Zodiacal Light has been used to calculate profiles of Doppler shifted Fraunhofer lines. Substantial line shape changes with ε are predicted with an indication of a bifurcation at ε < 30°, so offering an explanation for reported F corona observations.
- Type
- IX. Zodiacal Light and Thermal Emission
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- Copyright © Astronomical Society of the Pacific 1996
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