Eruptive Instability of the Magnetic-Flux Rope: Gravitational Force and Mass-Unloading
Based on the Kuperus–Raadu filament model, we analyze the vertical stability of a magnetic-flux rope as a whole, taking into account the gravitational force and mass-unloading. We use the small-perturbation method to determine conditions of the eruptive instability caused by vertical displacements. It has been shown that the upper limit of the magnetic-field decay index describing the flux-rope stability increases with an increase of its mass. The decrease of the flux-rope mass leads to activation and subsequent eruption of the filament. Possible mechanisms of the solar-filament destabilization are discussed.
KeywordsSun: magnetic fields Sun: oscillations Sun: photosphere
We would like to thank the anonymous referees for very useful comments, which we found to be very constructive and helpful to improve our manuscript. Yu. T. Tsap and Yu. G. Kopylova were partially supported by the Russian Foundation for Basic Research (project No. 18-02-00856), and RAS Program of Basic Research 12 “Problems of Origin and Evolution of the Universe”.
Disclosure of Potential Conflicts of Interest
The authors declare that they have no conflicts of interest.
- Bommier, V., Landi Degl’Innocenti, E., Leroy, J.-L., Sahal-Brechot, S.: 1994, Complete determination of the magnetic field vector and of the electron density in 14 prominences from linear polarization measurements in the HeI D3 and H-alpha lines. Solar Phys. 154, 231. DOI. ADS. ADSCrossRefGoogle Scholar
- Filippov, B.P.: 2007, Eruptive Processes on the Sun, Fizmatlit, Moscow. (In Russian). Google Scholar