The extreme solar storm of May 1921: observations and a complex topological model

The extreme solar storm of May 1921: observations and a complex topological model

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A complex solid torus model was developed in order to be able to study an extreme solar storm, the so-called "Great Storm" or "New York Railroad Storm" of May Bike Parts - Tubes 1921, when neither high spatial and time resolution magnetic field measurements, solar flare nor coronal mass ejection observations were available.We ORG HIMALAYAN SUNSHIN suggest that a topological change happened in connection with the occurrence of the extreme solar storm.The solar storm caused one of the most severe space weather effects ever.