Dynamic Model of Magnetic Flux Ropes


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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.

Sobre autores

V. Zaitsev

Institute of Applied Physics

Autor responsável pela correspondência
Email: za130@appl.sci-nnov.ru
Rússia, Nizhny Novgorod, 603600

A. Stepanov

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

Autor responsável pela correspondência
Email: stepanov@gaoran.ru
Rússia, St. Petersburg, 196140; St. Petersburg, 194021

A. Melnikov

Central Astronomical Observatory at Pulkovo

Email: stepanov@gaoran.ru
Rússia, St. Petersburg, 196140

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Declaração de direitos autorais © Pleiades Publishing, Ltd., 2019