3D state of the inner heliosphere from 0.1 AU to Earth
The inner boundary conditions is based on an empricial model of the wind speed, density and magnetic field obtained from white light observations.
The solution is propagated using the PLUTO code up to 1AU.
The inner boundary is computed at the beginning of the interval at -3 days and the forecasting is obtained considering Earth motion in the steady heliosphere to +7 days. The movie shows a comparison with data over a month.