ACE/EPAM energetic particle signatures during the October/November 2003 interplanetary coronal mass ejection events

Authors

O. E. Malandraki, ESTEC - European Space Research and Technology Centre
D. Lario, Johns Hopkins University Applied Physics Laboratory
L. J. Lanzerotti, New Jersey Institute of Technology
E. T. Sarris, National and Kapodistrian University of Athens
A. Geranios, Democritus University of Thrace

Document Type

Conference Proceeding

Publication Date

12-1-2006

Abstract

Solar energetic particles are utilized as diagnostic tracers of the large-scale structure and topology of the Interplanetary Magnetic Field embedded within two Interplanetary Coronal Mass Ejections detected in late October and early November 2003 at 1 AU by the ACE spacecraft. Two candidate scenarios to account for the observations in terms of open and closed magnetic field configurations are examined. We also use ACE/EPAM observations to reassess the boundaries of the ICMEs with respect to those previously proposed. © 2006 American Institute of Physics.

Identifier

33846473082 (Scopus)

ISBN

[0735403430, 9780735403437]

Publication Title

Aip Conference Proceedings

External Full Text Location

https://doi.org/10.1063/1.2347975

e-ISSN

15517616

ISSN

0094243X

First Page

176

Last Page

183

Volume

848

Recommended Citation

Malandraki, O. E.; Lario, D.; Lanzerotti, L. J.; Sarris, E. T.; and Geranios, A., "ACE/EPAM energetic particle signatures during the October/November 2003 interplanetary coronal mass ejection events" (2006). Faculty Publications. 18715.
https://digitalcommons.njit.edu/fac_pubs/18715