Efficiency of electron acceleration by shock waves in the solar corona according to observational data on the fine structure of type II radio bursts-Reference-Cited by-同舟云学术

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Efficiency of electron acceleration by shock waves in the solar corona according to observational data on the fine structure of type II radio bursts

Published:1998-02 Issue:2 Volume:41 Page:107-114
ISSN:0033-8443
Container-title:Radiophysics and Quantum Electronics
language:en
Short-container-title:Radiophys Quantum Electron

Author:

Zaitsev V. V.,Zlotnik E. Y.,Mann G.,Aurass H.,Klassen A.

Publisher

Springer Science and Business Media LLC

Subject

Electrical and Electronic Engineering,Astronomy and Astrophysics,Nuclear and High Energy Physics,Statistical and Nonlinear Physics,Electronic, Optical and Magnetic Materials

Link

http://link.springer.com/content/pdf/10.1007/BF02679627.pdf

Reference16 articles.

1. J. A. Roberts,Austral. J. Phys.,12, 322 (1959).

2. I. N. Cairns and R. D. Robinson,Solar Phys.,111, 365 (1987).

3. G. Mann and S. Klose, in: AGU 1995 Fall Meeting, Suppl. EOJ7, F455 (1995).

4. S. A. Kaplan and V. N. Tsytovich,Plasma Astrophysics [in Russian], Nauka, Moscow (1972).

5. V. V. Zaitsev and A. V. Stepanov,Izv. Vyssh. Uchebn. Zaved., Radiofiz.,17, 1229 (1974).

Cited by 1 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. Fine and Superfine Structure of the Decameter–Hectometer Type II Burst on 7 June 2011;Solar Physics;2015-06-30

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