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Magnetic Cloud as a Dual-Polarity Flux Rope
Published online by Cambridge University Press: 13 May 2016
Abstract
The magnetic cloud of November 17-18, 1975 is analyzed and it is shown that measurements of magnetic field and solar wind plasma are consistent with the interpretation that this magnetic cloud is a dual-polarity flux rope which consists of a core and an annular region. The core has a strong magnetic field; the annular region has a higher plasma density and opposite magnetic polarity.
- Type
- Session VI: The Solar Wind and Heliosphere
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- Copyright
- Copyright © Astronomical Society of the Pacific 2001