Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T23:34:59.713Z Has data issue: false hasContentIssue false
  • English
  • Français

Balance of energetic electrons in zebra pattern solar radio sources

Published online by Cambridge University Press:  14 March 2005

E.Ya. Zlotnik ,
V.V. Zaitsev ,
H. Aurass  and
G. Mann
E.Ya. Zlotnik
Affiliation:
IAP RAS, 46 Uljanov St., N. Novgorod 603950 Russia, email: [email protected]
V.V. Zaitsev
Affiliation:
IAP RAS, 46 Uljanov St., N. Novgorod 603950 Russia, email: [email protected]
H. Aurass
Affiliation:
Astrophysicsl Institute Potsdam, Germany, email: [email protected]
G. Mann
Affiliation:
Astrophysicsl Institute Potsdam, Germany, 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.

An aestimate of a typical life time of zebra pattern associated with escaping of fast particles from the trap into the loss-cone, is given. Besides, we estimate a number of fast electrons that is necessary to be injected into the trap in order to provide the observed brightness temperature of zebra stripes.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 495 - 496
Copyright
© 2004 International Astronomical Union