Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-25T05:55:05.878Z Has data issue: false hasContentIssue false
  • English
  • Français

The Possible Sources of the Relativistic Electrons in the Magnetosphere

Published online by Cambridge University Press:  03 June 2005

L. Xie ,
Z.Y. Pu  and
Y. Lu
L. Xie
Affiliation:
Department of Geophysics, Peking University, Beijing, 100871, China email: [email protected] Present address: Peking University, Beijing, China.
Z.Y. Pu
Affiliation:
Department of Geophysics, Peking University, Beijing, 100871, China email: [email protected]
Y. Lu
Affiliation:
Department of Geophysics, Peking University, Beijing, 100871, China email: [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.

Using data from ACE and low-altitude polar orbit satellite of NOAA, we investigate the possible sources of the enhancements of relativistic electrons in the magnetosphere. The observations from NOAA for the different geomagnetic activity periods show that substorms injections provide seed electrons for MeV electron enhancement associated with geomagnetic storms and the energetic electrons in the solar wind provide an alternative source for the relativistic electrons in the magnetosphere during the SEP events.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)particle emissionsolar-terrestrial relationssolar wind
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 458 - 463
Copyright
© 2005 International Astronomical Union