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Magnetic storm effects on the occurrence and characteristics of plasma bubbles

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Zenodo2023-10-08 更新2026-05-26 收录
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This supporting information provides two datasets that contain information about all the storms that occurred from 2008 to 2014, as well as storms with available PRE (Pre-Reversal Enhancement) and plasma bubble occurrence data during those years. The datasets include the start and end times of the initial, main, and recovery phases (both first and second half) of the detected storms. Additionally, the datasets contain the minimum and maximum SYM-H index attained during each storm, the intensity of the storms classified as follows: (1) Intense (SYM-H<sub>min</sub> &lt; -100 nT), (2) Moderate (-100 ≤ SYM-H<sub>min </sub>&lt; -50 nT), and (3) Weak (-50 ≤ SYM-H<sub>min</sub> &lt; -30 nT), and the overall duration of the storm, among other relevant parameters.This supporting information provides two datasets that contain information about all the storms that occurred from 2008 to 2014, as well as storms with available PRE (Pre-Reversal Enhancement) and plasma bubble occurrence data during those years. The datasets include the start and end times of the initial, main, and recovery phases (both first and second half) of the detected storms. Additionally, the datasets contain the minimum and maximum SYM-H index attained during each storm, the intensity of the storms classified as follows: (1) Intense (SYM-H<sub>min</sub> &lt; -100 nT), (2) Moderate (-100 ≤ SYM-H<sub>min </sub>&lt; -50 nT), and (3) Weak (-50 ≤ SYM-H<sub>min</sub> &lt; -30 nT), and the overall duration of the storm, among other relevant parameters.

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2023-10-08
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