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Particle Acceleration at Reconnecting X points in Solar Flares by Electrostatic Waves

Published online by Cambridge University Press:  01 November 2006

Wang De-Yu ,
Lu Quan-Ming  and
Huang Guang-Li
Wang De-Yu
Affiliation:
Purple Mountain Observatory, Nanjing, 210008, China, email: dy_wang@jlonline.com; glhuang@pmo.ac.cn Present address: 2nd, West-Beijing Road, Nanjing, 210008, China
Lu Quan-Ming
Affiliation:
School of Earth and Space Sciences, University of Sciences and Technology of China, Hefei, 230026, China, email: qmlu@ustc.edu.cn
Huang Guang-Li
Affiliation:
Purple Mountain Observatory, Nanjing, 210008, China, email: dy_wang@jlonline.com; glhuang@pmo.ac.cn
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Abstract

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In the impulsive phase of solar flares, the electrostatic waves can be excited during magnetic reconnection. The proton and electron at reconnecting X points can be accelerated by perpendicular propagating electrostatic waves.

Keywords

sun:flaresmagnetic reconnectionacceleration of particleswaves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 77 - 78
Copyright
© 2006 International Astronomical Union