activity
19992026
most citedFormation of current sheets and sigmoidal structure by the kink instability of a magnetic loop

188 citations · 431 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2026

On the 3D Magnetic Structure of Coronal Mass Ejections Through the Solar Corona

Erika Palmerio, Michal Ben-Nun, Tibor Török +2

The magnetic fields that make up the internal structure of coronal mass ejections (CMEs) are thought to be organised in a flux rope configuration, consisting of twisted magnetic fi…

astro-ph.SR2026

Tracking Magnetic Topological Change in a Time-Dependent Coronal Model

Emily I. Mason, Cooper Downs, Roberto Lionello +2

We apply the slip-back mapping method of Titov et al. 2009 and Lionello et al. 2020 to a thermodynamic MHD simulation to track topological changes in the magnetic field at a range…

astro-ph.SR2023

CORHEL-CME: An Interactive Tool For Modeling Solar Eruptions

Jon Linker, Tibor Torok, Cooper Downs +5

Coronal Mass Ejections (CMEs) are immense eruptions of plasma and magnetic fields that are propelled outward from the Sun, sometimes with velocities greater than 2000 km/s. They ar…

astro-ph.SR2023

Deflection of Coronal Mass Ejections in Unipolar Ambient Magnetic Fields

Michal Ben-Nun, Tibor Török, Erika Palmerio +5

The trajectories of coronal mass ejections (CMEs) are often seen to substantially deviate from a purely radial propagation direction. Such deviations occur predominantly in the cor…

astro-ph.SR2015★ 1 cited

Modeling Jets in the Corona and Solar Wind

T. Torok, R. Lionello, V. S. Titov +4

Coronal jets are transient, collimated eruptions that occur in regions of predominantly open magnetic field in the solar corona. Our understanding of these events has greatly evolv…

astro-ph.SR2014★ 102 cited

Distribution of Electric Currents in Solar Active Regions

Tibor Török, James E. Leake, Viacheslav S. Titov +6

There has been a long-lasting debate on the question of whether or not electric currents in solar active regions are neutralized. That is, whether or not the main (or direct) coron…

astro-ph.SR2010★ 69 cited

Testing magnetofrictional extrapolation with the Titov-Démoulin model of solar active regions

G. Valori, B. Kliem, T. Török +1

We examine the nonlinear magnetofrictional extrapolation scheme using the solar active region model by Titov and Démoulin as test field. This model consists of an arched, line-tied…