SOLAR WIND MODEL ASSESSMENT IN PREDICTING INNER HELIOSPHERIC CONDITIONS DURING 1994-2024

This scheme employs a three-dimensional numerical magnetohydrodynamic (MHD) model to reconstruct the solar wind parameters from 20 Rs to 1 AU, with inner boundary conditions constrained by observations. We perform a quantitative study by comparing the modeled results with OMNI observations using various assessment methods.

Particularly, the distance D and the Dynamic Time Warping (DTW) algorithm are presented to evaluate the similarity between time series data. The polarity of the interplanetary magnetic field (IMF) and stream interaction regions (SIRs) are also assessed.