Dynamic Model of Magnetic Flux Ropes
- Authors: Zaitsev V.V.1, Stepanov A.V.2,3, Melnikov A.V.2
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Affiliations:
- Institute of Applied Physics
- Central Astronomical Observatory at Pulkovo
- Ioffe Institute, Russian Academy of Sciences
- Issue: Vol 59, No 7 (2019)
- Pages: 806-809
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157794
- DOI: https://doi.org/10.1134/S0016793219070272
- ID: 157794
Cite item
Abstract
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.
About the authors
V. V. Zaitsev
Institute of Applied Physics
Author for correspondence.
Email: za130@appl.sci-nnov.ru
Russian Federation, Nizhny Novgorod, 603600
A. V. Stepanov
Central Astronomical Observatory at Pulkovo; Ioffe Institute, Russian Academy of Sciences
Author for correspondence.
Email: stepanov@gaoran.ru
Russian Federation, St. Petersburg, 196140; St. Petersburg, 194021
A. V. Melnikov
Central Astronomical Observatory at Pulkovo
Email: stepanov@gaoran.ru
Russian Federation, St. Petersburg, 196140
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