6976 20240416144859.0 POSTER-2024-0068 Katsiyannis, A. C. Solar wind electron temperature estimation from low corona to 1 au derived by the DYN model 2023 2023-11-20 The DYN model is an analytical solution of Parker's hydrodynamical equation that describes the solar wind corona. It requires a radial electron density distribution and produces various physical quantities as output. In this contribution we use an equatorial electron density distribution created from many decades of eclipse observations to derive an electron temperature radial distribution. It is the compared to recently published in situ satellite measurements to validate the DYN model. STCE Corona Solar Wind Electron Density Electron Temperature Lemaire, J. European Space Weather Week, Toulouse, France thanassis.katsiyannis@ksb-orb.be https://esww2023.org/ CPOSTER