The May 2024 Storm: The Cusps and Dayside Magnetopause in Simulated Soft X‐Rays

Abstract The coronal mass ejection (CME) arriving at Earth on 10 May 2024 caused the most intense geomagnetic storm in the last two decades, resulting in highly unusual cusp and magnetopause dynamics. We simulate soft X‐Ray emission due to solar wind charge exchange with exospheric neutrals to image the global dayside dynamics, focusing on the impact of a dense CME current sheet during the storm main phase. The magnetopause moves inward to , and the cusps manifest as nearly parallel emission ridges in X‐Ray. As the interplanetary magnetic field reverses, the cusp ridges move apart to higher latitudes for minutes after the reversal, addressing the open question of how the cusps evolve during and after northward turning of the IMF. Our work highlights soft X‐ray imaging enabling simultaneous observations of extreme solar‐wind impacts across multiple magnetospheric regions.

Authors

Institutions

Publication Details

Journal
Geophysical Research Letters
Published
2026-10-24
DOI
https://doi.org/10.1029/2025gl120479
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

The May 2024 Storm: The Cusps and Dayside Magnetopause in Simulated Soft X‐Rays

Brandon Lee Burkholder, B. L. Alterman, J. W. Bonnell, David Gary Sibeck et al.
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

The May 2024 Storm: The Cusps and Dayside Magnetopause in Simulated Soft X‐Rays

Brandon Lee Burkholder, B. L. Alterman, J. W. Bonnell, David Gary Sibeck, S. M. Petrinec, V. G. Merkin, Ying Zou, Jonathan Ng, Hyunju Kim Connor, Li‐Jen Chen, Gonzalo Cucho‐Padin, Kevin H Pham, Frederick Scott Porter
article en

Abstract

Abstract The coronal mass ejection (CME) arriving at Earth on 10 May 2024 caused the most intense geomagnetic storm in the last two decades, resulting in highly unusual cusp and magnetopause dynamics. We simulate soft X‐Ray emission due to solar wind charge exchange with exospheric neutrals to image the global dayside dynamics, focusing on the impact of a dense CME current sheet during the storm main phase. The magnetopause moves inward to , and the cusps manifest as nearly parallel emission ridges in X‐Ray. As the interplanetary magnetic field reverses, the cusp ridges move apart to higher latitudes for minutes after the reversal, addressing the open question of how the cusps evolve during and after northward turning of the IMF. Our work highlights soft X‐ray imaging enabling simultaneous observations of extreme solar‐wind impacts across multiple magnetospheric regions.

Geophysical Research LettersVol. 53(20)
NSF National Center for Atmospheric Research (US), NSF NCAR High Altitude Observatory (US), University of Maryland, Baltimore (US), Goddard Space Flight Center (US), Johns Hopkins University (US), Johns Hopkins University Applied Physics Laboratory (US), Space Sciences Laboratory (US), University of Maryland, College Park (US), University of California, Berkeley (US)
Openalex Percentile: Top 14%
Ionosphere and magnetosphere dynamics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon