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.
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Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
Statistical analysis of solar events shows type II radio burst starting frequencies vary by source region and anti-correlate with proton spectral indices, constraining SEP acceleration mechanisms.
citing papers explorer
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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.
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Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
Statistical multipoint observations indicate ICME shock acceleration efficiency increases with heliocentric distance up to 0.7 AU before decreasing.
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Solar Energetic Particle Events and Associated Type II Radio Bursts from Different Source Regions
Statistical analysis of solar events shows type II radio burst starting frequencies vary by source region and anti-correlate with proton spectral indices, constraining SEP acceleration mechanisms.