First Observations of a Geomagnetic Superstorm With a Sub‐L1 Monitor

First Observations of a Geomagnetic Superstorm With a Sub‐L1 Monitor

Abstract Forecasting the geomagnetic effects of solar coronal mass ejections (CMEs) is currently an unsolved problem. CMEs, responsible for the largest values of the north‐south component of the interplanetary magnetic field, are the key driver of intense and extreme geomagnetic activity. Observatio...

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Main Authors: E. Weiler, C. Möstl, E. E. Davies, A. M. Veronig, U. V. Amerstorfer, T. Amerstorfer, J. Le Louëdec, M. Bauer, N. Lugaz, V. Haberle, H. T. Rüdisser, S. Majumdar, M. Reiss
Format: Article
Language:English
Published: Wiley 2025-03-01
Series:Space Weather
Subjects:
space weather forecasting
geomagnetic storms
solar coronal mass ejections
solar wind
heliosphere
dynamical evolution
Online Access:https://doi.org/10.1029/2024SW004260
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https://doi.org/10.1029/2024SW004260

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