Brought to you by:

Evidence for the Same Hot Plasma after Coronal Mass Ejection Events, in Both Remote and In Situ Observations

, , , , , , and

Published 2004 September 2 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation G. Poletto et al 2004 ApJ 613 L173 DOI 10.1086/425136

1538-4357/613/2/L173

Abstract

We present here evidence for highly ionized Fe observed both in the corona, in the aftermath of a coronal mass ejection, and, after propagation, in situ. The apparent source temperature is greater than 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 in situ to the same properties of the same plasma remotely observed at its source in the corona.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/425136