Using energetic electrons to probe the topology of the October 18-20, 1995 magnetic cloud

Computer Science – Sound

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Magnetic Clouds, Energetic Particles, Plasma Diagnostics, Solar Wind, Satellite-Borne Instruments, Coronal Mass Ejection, Solar Electrons, Satellite Sounding

Scientific paper

This study uses 0.1-100-keV electron observations from the WIND 3D Plasma and Energetic Particles experiment to elucidate the magnetic structure and topology of clouds. The WIND electron observations are used to trace the October 18-20, 1995 cloud magnetic field back to a specific solar active region, and it is shown that the cloud field line lengths vary in a way that is consistent with a twisted flux tube. Evidence that much of the cloud may already be magnetically disconnected from the sun in a patchy way is also presented.

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