Published October 7, 2023 | Version v1

Magnetic storm effects on the occurrence and characteristics of plasma bubbles

Authors/Creators

  • 1. University of South Alabama

Description

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-Hmin < -100 nT), (2) Moderate (-100 ≤ SYM-Hmin < -50 nT), and (3) Weak (-50 ≤ SYM-Hmin < -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-Hmin < -100 nT), (2) Moderate (-100 ≤ SYM-Hmin < -50 nT), and (3) Weak (-50 ≤ SYM-Hmin < -30 nT), and the overall duration of the storm, among other relevant parameters.

Files

Supporting Dataset S1.csv

Files (190.7 kB)

Name Size Download all
md5:9538a0dd77ae16306eb9de3ee91a6cf6
94.3 kB Preview Download
md5:9618548d5785da900449b3b8a312500a
96.4 kB Preview Download