000006976 001__ 6976
000006976 005__ 20240416144859.0
000006976 037__ $$aPOSTER-2024-0068
000006976 100__ $$aKatsiyannis, A. C.
000006976 245__ $$aSolar wind electron temperature estimation from low corona to 1 au derived by the DYN model
000006976 260__ $$c2023
000006976 269__ $$c2023-11-20
000006976 520__ $$aThe 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.
000006976 594__ $$aSTCE
000006976 6531_ $$aCorona
000006976 6531_ $$aSolar Wind
000006976 6531_ $$aElectron Density
000006976 6531_ $$aElectron Temperature
000006976 700__ $$aLemaire, J.
000006976 773__ $$tEuropean Space Weather Week, Toulouse, France
000006976 8560_ $$fthanassis.katsiyannis@ksb-orb.be
000006976 85642 $$ahttps://esww2023.org/
000006976 980__ $$aCPOSTER