Hostname: page-component-848d4c4894-pftt2 Total loading time: 0 Render date: 2024-05-16T22:34:11.914Z Has data issue: false hasContentIssue false
  • English
  • Français

Formation of electron clouds during particle acceleration in a 3D current sheet

Published online by Cambridge University Press:  08 June 2011

Valentina V. Zharkova  and
Taras Siversky
Valentina V. Zharkova
Affiliation:
Department of Mathematics, University of Bradford, Bradford BD7 1DP, UK email: v.v.zharkova@brad.ac.uk
Taras Siversky
Affiliation:
Department of Mathematics, University of Bradford, Bradford BD7 1DP, UK email: v.v.zharkova@brad.ac.uk
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.

Acceleration of protons and electrons in a reconnecting current sheet (RCS) is investigated with the test particle and particle-in-cell (PIC) approaches in the 3D magnetic configuration including the guiding field. PIC simulations confirm a spatial separation of electrons and protons towards the midplane and reveal that this separation occur as long as protons are getting accelerated. During this time electrons are ejected into their semispace of the current sheet moving away from the midplane to distances up to a factor of 103 – 104 of the RCS thickness and returning back to the RCS. This process of electron circulation around the current sheet midplane creates a cloud of high energy electrons around the current sheet which exists as long as protons are accelerated. Only after protons gain sufficient energy to break from the magnetic field of the RCS, they are ejected to the opposite semispace dragging accelerated electrons with them. These clouds can be the reason of hard X-ray emission in coronal sources observed by RHESSI.

Keywords

Sun: flaresplasmasacceleration of particlesmagnetic field
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 453 - 457
Copyright
Copyright © International Astronomical Union 2011

References

Birn, J., Drake, J. F., Shay, M. A., et al. . 2001, Journal of Geophysics Research, 106, 3715CrossRefGoogle Scholar
Drake, J. F., Swisdak, M., Che, H., & Shay, M. A. 2006, Nature, 443, 553CrossRefGoogle Scholar
Priest, E. & Forbes, T. 2000, Magnetic Reconnection (Magnetic Reconnection, by Priest, Eric and Forbes, Terry, pp. 612. ISBN 0521481791. Cambridge, UK: Cambridge University Press, June 2000.)CrossRefGoogle Scholar
Siversky, T. V. & Zharkova, V. V. 2009, Journal of Plasma Physics, 75, 619CrossRefGoogle Scholar
Sui, L. & Holman, G. D. 2003, Astrophysical Journal, Letters, 596, L251Google Scholar
Tsiklauri, D. & Haruki, T. 2007, Physics of Plasmas, 14, 2905CrossRefGoogle Scholar
Wood, P. & Neukirch, T. 2005, Solar Physics, 226, 73CrossRefGoogle Scholar
Zharkova, V. V. & Agapitov, O. V. 2009, Journal of Plasma Physics, 75, 159Google Scholar
Zharkova, V. V. & Gordovskyy, M. 2004, Astrophysical Journal, 604, 884CrossRefGoogle Scholar
Zharkova, V. V. & Gordovskyy, M. 2005 a, Monthly Notices of the Royal Astronomical Society, 356, 1107CrossRefGoogle Scholar
Zharkova, V. V. & Gordovskyy, M. 2005 b, Space Science Reviews, 121, 165CrossRefGoogle Scholar