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.
Space Weather: Terrestrial Perspective
3 Pith papers cite this work, alongside 346 external citations. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
No bursty planet-induced radio emission detected from five inactive M dwarfs; upper limits constrain GJ 367 b magnetosphere to <0.8 G under assumed stellar wind conditions.
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.
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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Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs
No bursty planet-induced radio emission detected from five inactive M dwarfs; upper limits constrain GJ 367 b magnetosphere to <0.8 G under assumed stellar wind conditions.
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A robust empirical relationship between speed and turbulence energy in the near-Earth solar wind
Long-term near-Earth solar wind observations establish a robust empirical connection between flow speed and magnetohydrodynamic turbulence energy.