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Solar Storms in a Time of War

Published online by Cambridge University Press:  02 October 2026

Freddy Moreno-Cárdenas*
Affiliation:
Centro de Estudios Astrofísicos, Gimnasio Campestre, Bogotá, Colombia
Santiago Vargas-Domínguez
Affiliation:
Observatorio Astronómico Nacional, Universidad Nacional de Colombia, Carrera 45, Bogotá, 111321, Colombia
Juan Camilo Buitrago-Casas
Affiliation:
Space Sciences Laboratory, University of California Berkeley 7 Gauss Way, 94720, Berkeley, USA
Claire Gasque
Affiliation:
Space Sciences Laboratory, University of California Berkeley 7 Gauss Way, 94720, Berkeley, USA
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Abstract

This work revisits the possible influence of solar activity on unexplained terrestrial events during the early years of World War II. By comparing records of major geomagnetic storms with contemporary news archives, we identified several explosions and communication failures that occurred between 1938 and 1941. Among these, the geomagnetic superstorm of September 17–19, 1941, stands out as an exceptional case: triggered by a large sunspot group and intense solar flare activity, it produced global magnetic disturbances (K-index 9) and widespread auroras visible as far south as New Mexico. Several unexplained detonations in Europe and North America were reported within hours of the storm’s peak, suggesting a possible physical link between solar-induced electrical currents and accidental explosions in sensitive wartime materials. While causality cannot be conclusively demonstrated, the temporal correspondence and physical plausibility support the hypothesis that space weather may have influenced certain wartime incidents traditionally attributed to sabotage. This historical analysis underscores the importance of integrating solar and geophysical research to better understand how extreme space weather can affect technological systems, both past and present.

Information

Type
Contributed Paper
Copyright
© The Author(s), 2026. Published by Cambridge University Press on behalf of The International Astronomical Union
Figure 0

Figure 1. Figure 1 long description.Magnetic field data: Declination (D), Vertical (Z) and Horizontal (H) component, recorded by the Kakioka Geomagnetic Observatory in September 1941. The vertical lines mark dates where unexplained explosion events were identified in this research.