Dependence of great geomagnetic storm intensity ($\Delta$SYM-H$\le$-200 nT) on associated solar wind parameters
Ming-Xian Zhao, Gui-Ming Le, Qi Li, Gui-Ang Liu, Tian Mao

TL;DR
This study investigates how solar wind parameters, especially the combined effect of electric field and dynamic pressure, influence the intensity of great geomagnetic storms, providing insights into predicting such extreme space weather events.
Contribution
It identifies the solar wind dynamic pressure combined with the electric field as the primary factor influencing the strength of great geomagnetic storms, based on correlation analysis.
Findings
Q parameter has the highest correlation with storm intensity (CC=0.94)
B$_s$ influence is less significant than Q during main phase
11 great storms analyzed during solar cycle 23
Abstract
We use SYM-H to capture the variation in the SYM-H index during the main phase of a geomagnetic storm. We define great geomagnetic storms as those with SYM-H -200 nT. After analyzing the data that were not obscured by solar winds, we determined that 11 such storms occurred during solar cycle 23. We calculated time integrals for the southward interplanetary magnetic field component I(B), the solar wind electric field I(E), and a combination of E and the solar wind dynamic pressure I(Q) during the main phase of a great geomagnetic storm. The strength of the correlation coefficient (CC) between SYM-H and each of the three integrals I(B) (CC = 0.74), I(E) (CC = 0.85), and I(Q) (CC = 0.94) suggests that Q, which encompasses both the solar wind electric field and the solar wind dynamic pressure, is the main driving factor that determines the…
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