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Journal ArticleDOI

The Torus instability

Bernhard Kliem, +1 more
- 24 May 2006 - 
- Vol. 96, pp 255002
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TLDR
In this paper, the expansion instability of a toroidal current ring in low-beta magnetized plasma is investigated, and the results are verified with experiments on spheromak expansion and with essential properties of solar coronal mass ejections.
Abstract
The expansion instability of a toroidal current ring in low-beta magnetized plasma is investigated. Qualitative agreement is obtained with experiments on spheromak expansion and with essential properties of solar coronal mass ejections, unifying the two apparently disparate classes of fast and slow coronal mass ejections.

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Journal ArticleDOI

Electric Current Evolution at the Footpoints of Solar Eruptions

TL;DR: In this paper, the authors analyzed the only 9 eruptive X-class flares for which clear ribbon-hooks were identifiable, and showed a decrease of the electric current in the area surrounded by the ribbon hooks during and after the eruption.
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A new trigger mechanism for coronal mass ejections: The role of confined flares and photospheric motions in the formation of hot flux ropes

TL;DR: In this article, extreme-ultraviolet observations were used to identify five pre-eruptive hot flux ropes in the solar corona and study how they evolved, and they were used as indicators of episodic bursts of magnetic reconnection by which each flux rope formed.
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Magnetic energy release: flares and coronal mass ejections

TL;DR: In this article, the authors describe key observational signatures of flares and CMEs on the Sun, their magnetic field topology, and discuss how the combined analysis of solar and interplanetary observations can be used to constrain the flare/CME ejection mechanism.
Journal ArticleDOI

Eruptions from coronal bright points: A spectroscopic view by IRIS of a mini-filament eruption, QSL reconnection, and reconnection-driven outflows

TL;DR: In this paper , the authors investigated a mini-lament eruption associated with cancelling magnetic fluxes in the coronal bright point (CBP) and showed that the mini-eruption is manifested via the ejection of hot (cBP loops) and cool (mini-filament) plasma recorded in both imaging and spectroscopic data.
Journal ArticleDOI

Height of a solar filament before eruption

TL;DR: The relationship between the height of a solar filament observed above the photosphere before the eruption on October 21, 2010, and the critical height of the stable equilibrium of magnetic flux ropes in the coronal magnetic field is analyzed in this paper.
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