1 code implementation • 29 Sep 2016 • T. Stolker, C. Dominik, M. Min, A. Garufi, G. D. Mulders, H. Avenhaus
This allows us to map physical quantities (scattering radius and scattering angle) onto scattered light images and retrieve stellar irradiation corrected (r^2-scaled) images and dust phase functions.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
