The expected imprint of flux rope geometry on suprathermal electrons in magnetic clouds

Magnetic clouds are a subset of interplanetary coronal mass ejections characterized by a smooth rotation in the magnetic field direction, which is interpreted as a signature of a magnetic flux rope. Suprathermal electron observations indicate that one or both ends of a magnetic cloud typically r...

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Bibliographic Details
Main Authors: M. J. Owens, N. U. Crooker, T. S. Horbury
Format: Article
Language:English
Published: Copernicus Publications 2009-10-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/27/4057/2009/angeo-27-4057-2009.pdf