SOLAR WIND MODEL ASSESSMENT IN PREDICTING INNER HELIOSPHERIC CONDITIONS DURING 1994-2024
收藏科学数据银行2025-09-30 更新2026-04-23 收录
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资源简介：
We systematically simulate the solar wind over the past thirty years based on a well-established scheme. 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.
提供机构：
张嫚
创建时间：
2025-09-30
