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arxiv: 2605.22576 · v1 · pith:WN6KX7PCnew · submitted 2026-05-21 · ⚛️ physics.space-ph

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

Pith reviewed 2026-05-22 01:21 UTC · model grok-4.3

classification ⚛️ physics.space-ph
keywords solar energetic particlessatellite fleet vulnerabilityeconomic impactspace weatherSEP eventradiation dosefailure probabilityorbital regimes
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The pith

A 1-in-100-year solar energetic particle event could produce $5.2 billion in capital losses across the U.S. satellite fleet, with roughly 100 satellites at critical risk.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper constructs an integrated model that traces solar energetic particle events through geomagnetic shielding, radiation dose accumulation, and satellite failure probabilities to overall economic impacts on the U.S. fleet. It draws on 27 years of event data to size a once-in-a-century storm and finds that one percent of the 10,650 operational satellites fall into the highest-risk category while most others remain effectively unaffected under standard hardening assumptions. The resulting expected fleet loss reaches $5.2 billion, with daily service disruptions ranging from $70 million to $1.3 billion depending on how many satellites are assumed to fail. Readers should care because satellites support Earth observation, military communications, and other daily infrastructure whose sudden loss would be felt immediately in the economy.

Core claim

The C-SWIM model links extreme-value statistics from 160 SEP events to orbital-regime shielding, total ionizing dose transport, and failure-probability estimation. Under the 1-in-100-year event it places about 100 satellites (1.0 percent of the fleet) in the Critical risk class, concentrated in high-altitude LEO and HEO, while MEO and GEO satellites register Negligible risk (P_fail < 10^-9). This yields an expected capital loss of $5.2 billion from the $254 billion fleet. Three nested failure scenarios produce daily economic impacts of approximately $70 million, $270 million, and $1.3 billion, with Earth observation suffering up to 95.6 percent capacity loss and military services facing 16.1

What carries the argument

The C-SWIM coupled framework, which chains SEP hazard characterization, dynamic geomagnetic cutoff modeling, radiation dose transport, and fleet-wide failure probability estimation into macroeconomic loss calculations.

If this is right

  • Earth observation capacity could drop by as much as 95.6 percent in the broadest failure scenario.
  • Military services would experience 16.1 to 20.4 percent disruption across the three scenarios.
  • Expected capital losses are first-order estimates because only total ionizing dose is modeled.
  • Daily economic figures represent upper bounds since recovery and operator mitigation are omitted.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Insurance and risk models for commercial space assets could incorporate these orbital-specific probabilities for extreme events.
  • The same coupled approach could be applied to other space-weather-sensitive systems such as power grids or aviation to produce comparable loss estimates.
  • Hardening priorities might shift toward high-altitude LEO and HEO platforms given their disproportionate contribution to the critical-risk count.

Load-bearing premise

The assessment assumes satellites carry radiation-hardened components and that failure risk can be estimated from total ionizing dose modeling alone, without other particle damage mechanisms or operator responses.

What would settle it

Direct comparison of the model's predicted failure counts and orbital-class distributions against observed satellite anomalies during any future SEP event whose intensity matches the modeled 1-in-100-year threshold.

Figures

Figures reproduced from arXiv: 2605.22576 by D. Bor, E. J. Oughton, M. J. Wiltberger, R. Linares, R. S. Weigel, R. Yang, T. Clower.

Figure 1
Figure 1. Figure 1: Integrated C-SWIM framework for SEP-driven satellite vulnerability [PITH_FULL_IMAGE:figures/full_fig_p008_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Complementary cumulative distribution functions for SEP peak flux. [PITH_FULL_IMAGE:figures/full_fig_p011_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: Flux profiles of three major historical solar energetic proton events. The Bastille Day 2000 event (panel a) serves as the baseline template, with the 1-in-100-year return-level scenarios overlaid in red, showing the scaled flux amplitude derived from generalized Pareto distribution extrapolation. Horizontal lines indicate NOAA Solar Radiation Storm thresholds (NOAA, 2026). S1 (10 pfu) marks the onset of a… view at source ↗
Figure 4
Figure 4. Figure 4: Distribution of US active payload satellites by orbital regime and inclination. Left panel: 2D histogram showing satellite count as a function of inclination for each regime. Right panel: marginal counts per regime (log scale). LEO dominates the population with strong clus￾tering at sun-synchronous (97◦ ) and constellation-specific inclinations (53◦ , 52◦ ). 3.3 Geomagnetic cutoff rigidity modeling Having … view at source ↗
Figure 5
Figure 5. Figure 5: SEP vulnerability assessment of the operational satellite fleet. [PITH_FULL_IMAGE:figures/full_fig_p024_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: Fleet value and expected loss assessment. [PITH_FULL_IMAGE:figures/full_fig_p026_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: Economic impact under three failure scenarios. [PITH_FULL_IMAGE:figures/full_fig_p028_7.png] view at source ↗
read the original abstract

Modern economies depend critically on satellite infrastructure, yet the aggregate economic consequences of extreme solar energetic particle (SEP) events have not been rigorously assessed. This study develops an integrated framework linking SEP hazard characterization, dynamic geomagnetic cutoff rigidity modeling, radiation dose transport, and fleet-wide failure probability estimation to macroeconomic impact analysis. Using extreme-value analysis of 160 SEP events over 27.4 years (1996-2025), failure probability is estimated for ~10,650 US operational satellites under orbital regime-dependent shielding assumptions. The assessment reveals that ~100 satellites (1.0%) are at Critical risk, concentrated in high-altitude low Earth orbit and highly elliptical orbit, while medium Earth orbit and geosynchronous orbit satellites fall in the Negligible class (P_fail < 10^-9) under the assumed radiation-hardened components and shielding. The expected capital loss across the ~$254B fleet totals ~$5.2B. Three failure scenarios, expanding from Critical satellites only (P_fail > 10^-2), to Critical and Elevated (P_fail > 10^-3), and to all satellites with non-negligible risk (P_fail > 10^-6), yield daily economic impacts of ~$70M, ~$270M, and ~$1.3B, respectively. Earth observation suffers up to 95.6% capacity loss in the worst case, while military services experience 16.1-20.4% disruption across scenarios. Results are first-order estimates: hardware failure counts are conservative because only total ionizing dose is modeled, and daily economic impacts represent upper bounds because operator response and recovery are not included.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The paper introduces the C-SWIM model, a coupled framework that integrates SEP hazard characterization from extreme-value analysis of 160 events, dynamic geomagnetic cutoff rigidity modeling, radiation dose transport, and orbital regime-dependent failure probability estimation to evaluate the vulnerability and economic losses of the US satellite fleet (~10,650 satellites valued at ~$254B) under a 1-in-100-year SEP event. It reports that approximately 100 satellites (1.0%) are at Critical risk, primarily in high-altitude LEO and HEO, with MEO and GEO in Negligible risk class under assumed radiation-hardened components. The expected capital loss is ~$5.2B, and three failure scenarios yield daily economic impacts of ~$70M, ~$270M, and ~$1.3B, with notable disruptions in Earth observation (up to 95.6% capacity loss) and military services (16.1-20.4% disruption). Results are presented as first-order estimates with conservative failure counts and upper-bound impacts.

Significance. If the modeling assumptions hold, this study offers a significant contribution by providing a quantitative, integrated assessment of the aggregate economic risks posed by extreme solar energetic particle events to satellite-dependent economies. The use of a substantial dataset for extreme-value analysis and the mapping to sector-specific impacts (e.g., Earth observation and military) strengthens its relevance for space weather risk management and policy. The explicit acknowledgment of limitations, such as modeling only total ionizing dose and excluding recovery, enhances transparency. This type of work bridges space physics with economic impact analysis, which is valuable for highlighting infrastructure vulnerabilities.

major comments (2)
  1. [§3.2] §3.2: The orbital regime-dependent shielding assumptions and radiation-hardened component premise are load-bearing for the failure probability classifications. The abstract indicates that MEO and GEO satellites are classified as Negligible (P_fail < 10^-9) based on these, but no sensitivity analysis or validation against measured shielding data is provided. Thinner actual shielding or use of commercial-grade components would increase the dose, potentially reclassifying these satellites and substantially increasing the number of Critical and Elevated risk satellites beyond the reported ~100, thereby affecting the $5.2B loss estimate.
  2. [§2.1] §2.1: The extreme-value analysis of 160 SEP events over 27.4 years underpins the 1-in-100-year flux level, yet the manuscript does not report confidence intervals, error propagation, or cross-validation with other SEP datasets. This uncertainty directly impacts the downstream dose calculations and economic loss figures.
minor comments (2)
  1. The abstract would benefit from explicitly stating the total satellite count (~10,650) and fleet value (~$254B) in the opening sentence for better context.
  2. [Abstract] Clarify the definition of the three failure scenarios (Critical only, Critical+Elevated, all non-negligible) with their exact P_fail thresholds in a single location.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their constructive comments, which help clarify the robustness of our modeling assumptions. We respond to each major comment below and indicate planned revisions to the manuscript.

read point-by-point responses
  1. Referee: [§3.2] §3.2: The orbital regime-dependent shielding assumptions and radiation-hardened component premise are load-bearing for the failure probability classifications. The abstract indicates that MEO and GEO satellites are classified as Negligible (P_fail < 10^-9) based on these, but no sensitivity analysis or validation against measured shielding data is provided. Thinner actual shielding or use of commercial-grade components would increase the dose, potentially reclassifying these satellites and substantially increasing the number of Critical and Elevated risk satellites beyond the reported ~100, thereby affecting the $5.2B loss estimate.

    Authors: We agree that the shielding thickness and radiation-hardened component assumptions are central to the Negligible risk classification for MEO and GEO satellites. These assumptions reflect standard design practices for operational satellites in those regimes, as documented in the methods. However, we acknowledge that the absence of a formal sensitivity analysis limits the ability to quantify how deviations (e.g., thinner shielding or commercial off-the-shelf components) would propagate to the fleet-wide loss estimate. In the revised manuscript we will add a dedicated sensitivity analysis section that varies shielding areal density and component tolerance thresholds, reporting the resulting changes in risk classifications and the $5.2B capital-loss figure. revision: yes

  2. Referee: [§2.1] §2.1: The extreme-value analysis of 160 SEP events over 27.4 years underpins the 1-in-100-year flux level, yet the manuscript does not report confidence intervals, error propagation, or cross-validation with other SEP datasets. This uncertainty directly impacts the downstream dose calculations and economic loss figures.

    Authors: The 1-in-100-year flux is obtained via peaks-over-threshold extreme-value analysis applied to the 160-event catalog spanning 27.4 years. While the manuscript presents the central estimate, we recognize that reporting uncertainty measures would strengthen the downstream propagation to dose and economic impacts. In the revision we will include bootstrap-derived 95% confidence intervals on the return-level flux, propagate these intervals through the dose-transport step, and add a brief discussion of consistency with independent SEP event catalogs (e.g., from GOES and other instruments). revision: yes

Circularity Check

0 steps flagged

No significant circularity; derivation relies on external SEP data and standard modeling steps

full rationale

The paper constructs its estimates by applying extreme-value analysis to an external catalog of 160 observed SEP events (1996-2025), then chaining established physical models for geomagnetic cutoff rigidity, dose transport, and regime-dependent shielding to compute per-satellite failure probabilities. These steps remain independent of the target outputs; the failure thresholds (e.g., Critical >10^-2) and shielding assumptions are explicit modeling choices, not self-definitions or fitted parameters renamed as predictions. No load-bearing self-citations, uniqueness theorems, or ansatzes imported from prior author work are required for the central claims. The framework is therefore self-contained against external benchmarks and falsifiable outside its own fitted values.

Axiom & Free-Parameter Ledger

2 free parameters · 1 axioms · 0 invented entities

The model rests on several domain assumptions about satellite shielding and failure modes that are introduced to enable the calculations but lack independent verification details in the provided abstract.

free parameters (2)
  • orbital regime-dependent shielding assumptions
    Used to assign failure probabilities across different orbits for the ~10,650 satellites.
  • failure probability thresholds
    Critical (P_fail > 10^-2), Elevated (> 10^-3), and non-negligible (> 10^-6) classes defined to generate the three economic impact scenarios.
axioms (1)
  • domain assumption Extreme-value analysis of 160 SEP events over 27.4 years suffices to characterize a 1-in-100-year event
    Invoked to define the hazard level for the vulnerability assessment.

pith-pipeline@v0.9.0 · 5879 in / 1403 out tokens · 49897 ms · 2026-05-22T01:21:03.739271+00:00 · methodology

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Reference graph

Works this paper leans on

12 extracted references · 12 canonical work pages

  1. [1]

    (2017).Social and Economic Impacts of Space Weather in the United States(Tech

    Abt-Associates. (2017).Social and Economic Impacts of Space Weather in the United States(Tech. Rep.). Retrieved fromhttps://www.weather.gov/ media/news/SpaceWeatherEconomicImpactsReportOct-2017.pdf Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogo- molov, E. A., . . . Zampa, N. (2016). PAMELA’s measurements of geomagnetic ...

  2. [2]

    doi: 10.1186/s40623-020-01288-x Baker, D. N. (2001). Satellite Anomalies due to Space Storms. In I. A. Daglis (Ed.), Space Storms and Space Weather Hazards(pp. 285–311). Dordrecht: Springer Netherlands. doi: 10.1007/978-94-010-0983-6 11 Baker, D. N., & Kanekal, S. G. (2008). Solar cycle changes, geomagnetic varia- tions, and energetic particle properties ...

  3. [3]

    Retrieved fromhttps://doi.org/10 .1007/s41116-016-0002-5doi: 10.1007/s41116-016-0002-5 Dietzenbacher, E. (1997). In vindication of the Ghosh model: A reinterpretation as a price model.Journal of Regional Science,37(4), 629–651. doi: 10.1111/0022 -4146.00073 Eastwood, J. P., Biffis, E., Hapgood, M. A., Green, L., Bisi, M. M., Bentley, R. D., . . . Burnett,...

  4. [4]

    doi: 10.3847/1538-4357/ad7462 Hands, A. D. P., Ryden, K. A., Meredith, N. P., Glauert, S. A., & Horne, R. B. (2018). Radiation Effects on Satellites During Extreme Space Weather Events. Space Weather,16(9), 1216–1226. doi: 10.1029/2018SW001913 Hansen, D. L., Manich, T., & Zavatkay, I. (2024). A Review of Single-Event Upset- Rate Calculation Methods.IEEE T...

  5. [5]

    N., Kravtsova, M

    doi: 10.1186/s40623-021-01420-5 Kichigin, G. N., Kravtsova, M. V., & Sdobnov, V. E. (2018). Variations in the Geomagnetic Cutoff Rigidity during the Magnetic Storm in March 2015.Phys. Atom. Nuclei,81(3), 396–400. doi: 10.1134/S1063778818030122 Koga, R., & Kolasinski, W. (2007). Effects of heavy ions on microcircuits in space: Recently investigated upset m...

  6. [6]

    E., & Blair, P

    doi: 10.3390/electronics13101822 Miller, R. E., & Blair, P. D. (2009).Input-output analysis: Foundations and ex- tensions(2nd ed.). Cambridge: Cambridge University Press. doi: 10.1017/ CBO9780511626982 Montenbruck, O., & Gill, E. (2000).Satellite Orbits. Berlin, Heidelberg: Springer. doi: 10.1007/978-3-642-58351-3 NASA/GSFC. (2024).SPDF - OMNIWeb Service....

  7. [7]

    (2025a).Goes-15 sem energetic particle flux.Retrieved 2026- 04-20, fromhttps://www.ncei.noaa.gov/data/goes-space-environment -monitor/access/avg/ NOAA NCEI

    NOAA NCEI. (2025a).Goes-15 sem energetic particle flux.Retrieved 2026- 04-20, fromhttps://www.ncei.noaa.gov/data/goes-space-environment -monitor/access/avg/ NOAA NCEI. (2025b).Goes-16 sgps level 2 proton flux.Retrieved 2026-04-20, fromhttps://data.ngdc.noaa.gov/platforms/solar-space-observing -satellites/goes/goes16/l2/data/sgps-l2-avg5m/ NRC. (2009).Seve...

  8. [8]

    doi: 10.2514/1.A36164 Petersen, E. (2007). Radiation induced soft fails in space electronics.IEEE Transac- tions on Nuclear Science,30(2), 1638–1641. Petersen, E. L. (1998). The SEU figure of merit and proton upset rate calcula- tions.IEEE Transactions on Nuclear Science,45(6), 2550–2562. doi: 10.1109/ 23.736497 Physics Today Staff. (2012, August). Costs ...

  9. [9]

    doi: 10.3390/universe10100391 Pulkkinen, T. (2007). Space Weather: Terrestrial Perspective.Living Rev. Sol. Phys.,4(1),

  10. [10]

    doi: 10.12942/lrsp-2007-1 Reames, D. V. (1995). Solar energetic particles: A paradigm shift.Reviews of Geo- physics,33, 585–589. Retrieved fromhttps://onlinelibrary.wiley.com/ doi/abs/10.1029/95RG00188doi: 10.1029/95RG00188 Robinson, R., & Behnke, R. (2001). The us national space weather program: a ret- rospective.Geophysical Monograph Series,125, 1–10. R...

  11. [11]

    doi: 10.12942/lrsp-2006-2 Seltzer, S. M. (1994).Updated calculations for routine space-shielding radiation dose estimates: Shieldose-2(Tech. Rep.). Gaithersburg, MD: National Institute of –42– manuscript submitted toSpace Weather Standards and Technology. Sierawski, B. D., Pellish, J. A., Reed, R. A., Schrimpf, R. D., Warren, K. M., Weller, R. A., . . . S...

  12. [12]

    doi: 10.1029/2001JA000219 U.S

    Mathematical structure.Journal of Geophysical Research: Space Physics,107(A8), SMP 12-1–SMP 12-15. doi: 10.1029/2001JA000219 U.S. Bureau of Economic Analysis. (2023).Input-output accounts data.Retrieved 2024-03-04, fromhttps://www.bea.gov/industry/input-output-accounts -data U.S. Department of Defense. (2020).Global positioning system standard positioning...