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Radial Transport of Radiation Belt Electrons Due to Stormtime Pc5 Waves : Volume 27, Issue 5 (13/05/2009)

By Ukhorskiy, A. Y.

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Book Id: WPLBN0003977400
Format Type: PDF Article :
File Size: Pages 9
Reproduction Date: 2015

Title: Radial Transport of Radiation Belt Electrons Due to Stormtime Pc5 Waves : Volume 27, Issue 5 (13/05/2009)  
Author: Ukhorskiy, A. Y.
Volume: Vol. 27, Issue 5
Language: English
Subject: Science, Annales, Geophysicae
Collections: Periodicals: Journal and Magazine Collection, Copernicus GmbH
Historic
Publication Date:
2009
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Sitnov, M. I., Anderson, B. J., Takahashi, K., & Ukhorskiy, A. Y. (2009). Radial Transport of Radiation Belt Electrons Due to Stormtime Pc5 Waves : Volume 27, Issue 5 (13/05/2009). Retrieved from http://ebook.worldlibrary.net/


Description
Description: The Johns Hopkins University, Applied Physics Laboratory, Johns Hopkins Road, Laurel, MD, USA. During geomagnetic storms relativistic electron fluxes in the outer radiation belt exhibit dynamic variability over multiple orders of magnitude. This requires radial transport of electrons across their drift shells and implies violation of their third adiabatic invariant. Radial transport is induced by the interaction of the electron drift motion with electric and magnetic field fluctuations in the ULF frequency range. It was previously shown that solar-wind driven ULF waves have long azimuthal wave lengths and thus can violate the third invariant of trapped electrons in the process of resonant interaction with their gradient-curvature motion. However, the amplitude of solar-wind driven ULF waves rapidly decreases with decreasing L. It is therefore not clear what mechanisms are responsible for fast transport rates observed inside the geosynchronous orbit. In this paper we investigate wether stormtime Pc5 waves can contribute to this process. Stormtime Pc5s have short azimuthal wave lengths and therefore cannot exhibit resonance with the the electron drift motion. However we show that stormtime Pc5s can cause localized random scattering of electron drift motion that violates the third invariant. According to our results electron interaction with stormtime Pc5s can produce rapid radial transport even as low as L≃4. Numerical simulations show that electron transport can exhibit large deviations from radial diffusion. The diffusion approximation is not valid for individual storms but only applies to the statistically averaged response of the outer belt to stormtime Pc5 waves.

Summary
Radial transport of radiation belt electrons due to stormtime Pc5 waves

Excerpt
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