Shock Drift Acceleration and Type II Solar Radio Bursts

Author:

Street Arthur G.,Ball Lewis,Melrose D. B.

Abstract

AbstractShock drift acceleration of the electrons which produce herringbone structure in type II bursts is considered. A non-coplanar component of the magnetic field within the shock front and an electric field across the shock are taken into account. A quantitative difficulty with shock drift acceleration is identified, and possible ways of overcoming the difficulty are outlined.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Generation of interplanetary type II radio emission;Astronomy & Astrophysics;2021-10

2. Evolution of the Alfvén Mach number associated with a coronal mass ejection shock;Astronomy & Astrophysics;2020-01

3. Type II radio bursts: 1. New entirely analytic formalism for the electron beams, Langmuir waves, and radio emission;Journal of Geophysical Research: Space Physics;2012-04

4. Theory of type II radio emission from the foreshock of an interplanetary shock;Journal of Geophysical Research: Space Physics;2001-11-01

5. Shock Drift Acceleration of Electrons;Publications of the Astronomical Society of Australia;2001

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