Dynamic Model of Magnetic Flux Ropes
- 作者: Zaitsev V.V.1, Stepanov A.V.2,3, Melnikov A.V.2
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隶属关系:
- Institute of Applied Physics
- Central Astronomical Observatory at Pulkovo
- Ioffe Institute, Russian Academy of Sciences
- 期: 卷 59, 编号 7 (2019)
- 页面: 806-809
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157794
- DOI: https://doi.org/10.1134/S0016793219070272
- ID: 157794
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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
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