Comparative analysis of two episodes of strongly geoeffective CME events in November and December 2023

Abstract

In autumn 2023, a series of closely timed eruptive events were observed remotely and measured in situ. We studied analogous solar events, where several CMEs were launched partly from the same (active) regions near a CH. These events occurred in two episodes, separated by a full solar rotation, covering October 31-November 3 and November 27-28, 2023. Both episodes are linked to strong geomagnetic storms on November 4-5 and December 1-2, 2023. We aim to understand the complexity of these events and how the global magnetic field, solar wind conditions, and structural interactions relate to the observed geomagnetic effects. Using the GCS 3D reconstruction method, we derived each CME's motion direction and speed. These results were input into the DBM with enhanced latitudinal information (3D DBM), aiding in connecting in-situ measurements with solar surface structures for integrated interpretation. The first episode caused SAR arcs, with a three-step Dst index drop to -163 nT on November 5, 2023. Two CME-related shocks arrived close in time, separated by a SBC, followed by a short-duration flux rope-like structure. The second episode saw auroral lights and a two-step Dst index drop to -108 nT on December 1, 2023. A shock from one CME interacted with the magnetic structure of a preceding CME, again combined with an SBC. A clear flux rope structure from the shock-producing CME was detected. Both events showed distinct magnetic field 'ripples' and fluctuations in density and temperature following the SBC. This study compares two episodes of multiple eruptive events in November and December 2023. Interacting CME structures and SBC-related magnetic modulations contributed to the stronger geomagnetic impacts, particularly in the November 4-5, 2023 event. The highly tilted heliospheric current sheet may have further influenced the CMEs' impact at Earth.

arXiv commentAccepted for publication in A&A

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