Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-28T18:33:31.017Z Has data issue: false hasContentIssue false
  • English
  • Français

Energetic Particle Tracing of Interplanetary CMEs: ULYSSES/HI-SCALE and ACE/EPAM Results

Published online by Cambridge University Press:  03 June 2005

Olga E. Malandraki ,
D. Lario ,
T.E. Sarris ,
N. Tsaggas  and
E.T. Sarris
Olga E. Malandraki
Affiliation:
Democritus University of Thrace, Space Research Laboratory, Xanthi, 67100 Greece, email: [email protected], [email protected]
D. Lario
Affiliation:
Applied Physics Laboratory, the Johns Hopkins University, Laurel, Maryland, USA email: [email protected]
T.E. Sarris
Affiliation:
Democritus University of Thrace, Space Research Laboratory, Xanthi, 67100 Greece, email: [email protected], [email protected]
N. Tsaggas
Affiliation:
Democritus University of Thrace, Space Research Laboratory, Xanthi, 67100 Greece, email: [email protected], [email protected]
E.T. Sarris
Affiliation:
Democritus University of Thrace, Space Research Laboratory, Xanthi, 67100 Greece, email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Solar energetic particle (SEP) fluxes measured by the ULYSSES (ULS)/HI-SCALE experiment during its second polar orbit as well as by the identical ACE/EPAM experiment at 1 AU are utilized as diagnostics of the large-scale structure and topology of the Interplanetary Magnetic Field (IMF) embedded within Interplanetary Coronal Mass Ejections (ICMEs). Survey results are also reported.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)interplanetary mediummagnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 361 - 366
Copyright
© 2005 International Astronomical Union