Dynamic Model of Magnetic Flux Ropes


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

Developing ideas of the paper Zaitsev and Stepanov (2018) with regards to activation of a current-carrying filament with an increase in electric current, in which the Ampère force is opposed by gravity and medium viscosity, we take into account the influence of an external magnetic field. It is shown that, depending on mutual directions of the external magnetic field and electric current in the flux rope, the additional Ampère force can lead to the deceleration or to additional eruption of the flux rope. A phase diagram describing the peculiarities of flux rope dynamics has been constructed. The maximum height and velocity of the flare loop are determined for the event on March 30, 2001.

作者简介

V. Zaitsev

Institute of Applied Physics

编辑信件的主要联系方式.
Email: za130@appl.sci-nnov.ru
俄罗斯联邦, Nizhny Novgorod, 603600

A. Stepanov

Central Astronomical Observatory at Pulkovo; Ioffe Institute, Russian Academy of Sciences

编辑信件的主要联系方式.
Email: stepanov@gaoran.ru
俄罗斯联邦, St. Petersburg, 196140; St. Petersburg, 194021

A. Melnikov

Central Astronomical Observatory at Pulkovo

Email: stepanov@gaoran.ru
俄罗斯联邦, St. Petersburg, 196140

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2019