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Evidence for Hot Plasma after CME events from Remote and In Situ ObservationsWe present here evidence for highly ionized Fe observed both in the corona, in the aftermath of a CME, and, after propagation, {\it in situ}. The apparent source temperature is $>$6 MK. To our knowledge, this is the first time that such an unambiguous identification has been made. This detection complements studies correlating other properties of plasma observed {\it in situ} to the same properties of the same plasma remotely observed at its source in the corona.
Document ID
20040085900
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Poletto, G.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Suess, S. T.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Bemporad, A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Schwadron, N.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Elliott, H. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Zurbuchen, T.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ko, Y.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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