Dual-spacecraft observations of a November 2021 CME confirm that the CAAP method reliably estimates instantaneous expansion speed from single-point data while revealing unexpected evolution in shock strength and magnetic flux.
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Aspect ratio of fast and slow Earth-directed CMEs shows a systematic three-phase evolution from corona to 1 AU with reduced radial expansion efficiency at larger distances.
A spatiotemporal agent-based model simulates satellite responses to extreme space weather and provides real-time maneuver guidance with 92% accuracy using 41,644 satellite records and 5 historical events.
Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.
The C-SWIM model estimates $5.2 billion in capital losses to the US satellite fleet and daily economic impacts ranging from $70 million to $1.3 billion under a 1-in-100-year solar energetic particle event.
citing papers explorer
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Validating a Non-conventional Method for Expansion of Coronal Mass Ejections (CMEs) and Investigating the Evolution of a CME Substructures Using Solar Orbiter and Wind Observations
Dual-spacecraft observations of a November 2021 CME confirm that the CAAP method reliably estimates instantaneous expansion speed from single-point data while revealing unexpected evolution in shock strength and magnetic flux.
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Three-Phase Evolution of Aspect Ratio in Fast and Slow CMEs from the Sun to 1 AU
Aspect ratio of fast and slow Earth-directed CMEs shows a systematic three-phase evolution from corona to 1 AU with reduced radial expansion efficiency at larger distances.
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Preparing for the Next Carrington: Spatiotemporal Agent-Based Modeling for Safeguarding Satellite Infrastructure Under Extreme Space Weather Disturbances
A spatiotemporal agent-based model simulates satellite responses to extreme space weather and provides real-time maneuver guidance with 92% accuracy using 41,644 satellite records and 5 historical events.
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Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool
Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.
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C-SWIM: A Coupled Space Weather Impact Model for Satellite Fleet Vulnerability and Economic Loss Under a 1-in-100-Year Solar Energetic Particle Event
The C-SWIM model estimates $5.2 billion in capital losses to the US satellite fleet and daily economic impacts ranging from $70 million to $1.3 billion under a 1-in-100-year solar energetic particle event.