Development of solar flares and features of the fine structure of solar radio emission


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The reason for the occurrence of different elements of the fine structure of solar radio bursts in the decimeter and centimeter wavelength ranges has been determined based on all available data from terrestrial and satellite observations. In some phenomena, fast pulsations, a zebra structre, fiber bursts, and spikes have been observed almost simultaneously. Two phenomena have been selected to show that the pulsations of radio emission are caused by particles accelerated in the magnetic reconnection region and that the zebra structure is excited in a source, such as a magnetic trap for fast particles. The complex combination of unusual fiber bursts, zebra structure, and spikes in the phenomenon on December 1, 2004, is associated with a single source, a magnetic island formed after a coronal mass ejection.

作者简介

G. Chernov

Huairou Solar Observing Station; Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

编辑信件的主要联系方式.
Email: gchernov@izmiran.ru
中国, Beijing; Moscow

V. Fomichev

Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: gchernov@izmiran.ru
俄罗斯联邦, Moscow

Y. Yan

Huairou Solar Observing Station

Email: gchernov@izmiran.ru
中国, Beijing

B. Tan

Huairou Solar Observing Station

Email: gchernov@izmiran.ru
中国, Beijing

Ch. Tan

Huairou Solar Observing Station

Email: gchernov@izmiran.ru
中国, Beijing

Q. Fu

Huairou Solar Observing Station

Email: gchernov@izmiran.ru
中国, Beijing

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2017