The effect of uncertainties in reproducing the ambient solar wind at Earth on forecasting CME arrival times
Syed Raza, Talwinder Singh, Nikolai Pogorelov

TL;DR
This paper explores how uncertainties in modeling the solar wind affect CME arrival time predictions and uses machine learning to improve forecast accuracy by correcting model errors.
Contribution
It introduces ML-based correction methods for CME arrival time forecasts, reducing errors by up to 45 minutes using data from NASA's CCMC database.
Findings
ML models improved CME arrival time predictions by up to 45 minutes
Support vector machine and linear regression outperformed simpler models
Error correction significantly enhances space weather forecasting accuracy
Abstract
Coronal Mass Ejections (CMEs) are the major drivers of Space Weather (SWx), so predicting their arrival at Earth is a major aspect of SWx forecasting. Despite increasingly complex models proposed over the past decades, the mean absolute error (MAE) for predictions of CME arrival still surpasses 10 hours. In this study, we use machine learning (ML) techniques trained on the discrepancies between observed and modeled solar wind (SW) at the L1 point, upstream of CMEs, to quantify and ''correct'' the errors in CME Time of Arrival (TOA) associated with these discrepancies. We use CME data from the Database Of Notifications, Knowledge, Information (DONKI) developed by the NASA Community Coordinated Modeling Center (CCMC) for our investigation. The WSA-ENLIL-Cone (WEC) model inputs and outputs are available on DONKI for each CME, along with the associated forecast errors. The dataset consists…
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