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Spatial Relationship of Signatures of Interplanetary Coronal Mass EjectionsInterplanetary coronal mass ejections (ICMEs) are characterized by a number of signatures. In particular, we examine the relationship between Fe charge states and other signatures during ICMEs in solar cycle 23. Though enhanced Fe charge states characterize many ICMEs, average charge states vary from event to event, are more likely to be enhanced in faster or flare-related ICMEs, and do not appear to depend on whether the ICME is a magnetic cloud.
Document ID
20040031460
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Richardson, I. G. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Cane, H. V. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lepri, S. T. (Michigan Univ. Ann Arbor, MI, United States)
Zurbuchen, T. H. (Michigan Univ. Ann Arbor, MI, United States)
Gosling, J. T. (Los Alamos National Lab. NM, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Subject Category
Solar Physics
Meeting Information
Meeting: Solar Wind Ten
Location: Pisa
Country: Italy
Start Date: June 1, 2002
Distribution Limits
Public
Copyright
Public Use Permitted.
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