Predicting the magnetic vectors within coronal mass ejections arriving at Earth: 1. Initial Architecture
N. P. Savani, A. Vourlidas, A. Szabo, M. L. Mays, I. G. Richardson, B., J. Thompson, A. Pulkkinen, R. Evans, T. Nieves-Chinchilla

TL;DR
This paper introduces an initial architecture combining a helicity rule and flux rope topology to predict magnetic vectors in Earth-directed CMEs, aiming to improve space weather forecasting accuracy.
Contribution
It presents a novel proof-of-concept model that predicts CME magnetic vectors by integrating solar origin helicity with flux rope topology, tested on multiple events.
Findings
Angular rotation in predictions matches in situ data
Early CME evolution impacts forecasting accuracy
Time-varying magnetic field estimates enable Kp index prediction
Abstract
The process by which the Sun affects the terrestrial environment on short timescales is predominately driven by the amount of magnetic reconnection between the solar wind and Earth's magnetosphere. Reconnection occurs most efficiently when the solar wind magnetic field has a southward component. The most severe impacts are during the arrival of a coronal mass ejection (CME) when the magnetosphere is both compressed and magnetically connected to the heliospheric environment. Unfortunately, forecasting magnetic vectors within coronal mass ejections remains elusive. Here we report how, by combining a statistically robust helicity rule for a CME's solar origin with a simplified flux rope topology the magnetic vectors within the Earth-directed segment of a CME can be predicted. In order to test the validity of this proof-of-concept architecture for estimating the magnetic vectors within…
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