Hostname: page-component-f554764f5-rj9fg Total loading time: 0 Render date: 2025-04-12T08:29:52.818Z Has data issue: false hasContentIssue false
  • English
  • Français

Electron Acceleration by Strong DC Electric Fields in Extragalactic Jets

Published online by Cambridge University Press:  25 May 2016

Y. E. Litvinenko
Y. E. Litvinenko*
Affiliation:
Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH 03824-3525, U.S.A.

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.

Fast magnetic reconnection in extragalactic jets leads to electron acceleration by the DC electric field in the reconnecting current sheet. The maximum electron energy (γ > 106) and the acceleration time (< 106 s) are determined by the magnetic field dynamics in the sheet.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 311 - 312
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Eilek, J. A., & Hughes, P. A. 1991, in Beams and Jets in Astrophysics, ed. Hughes, P. A. (Cambridge: Cambridge Univ. Press), 428.Google Scholar
Hill, T. W. 1975, J. Geophys. Res., 80, 4689.CrossRefGoogle Scholar
Litvinenko, Y. E. 1996, ApJ, 462, 997.Google Scholar
Litvinenko, Y. E. 1999, A&A, 349, 685.Google Scholar