Flare evolution and polarization changes in fine structures of solar radio emission in the 2013 April 11 event-Reference-Cited by-同舟云学术

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Flare evolution and polarization changes in fine structures of solar radio emission in the 2013 April 11 event

Published:2016-02 Issue:2 Volume:16 Page:008
ISSN:1674-4527
Container-title:Research in Astronomy and Astrophysics
language:
Short-container-title:Res. Astron. Astrophys.

Author:

Chernov Gennady,Sych Robert,Tan Bao-Lin,Yan Yi-Hua,Tan Cheng-Ming,Fu Qi-Jun,Karlický Marian,Fomichev Valery

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1674-4527/16/i=2/a=008/pdf

Reference35 articles.

1. On the origin of microwave zebra pattern

2. Whistlers in the solar corona and their relevance to fine structures of type IV radio emission

3. Delay between the circularly polarized components in fine structures during solar type IV events

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. Development of solar flares and features of the fine structure of solar radio emission;Geomagnetism and Aeronomy;2017-11

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