T
Tibor Torok
Researcher at Paris Diderot University
Publications - 120
Citations - 9796
Tibor Torok is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Coronal mass ejection & Magnetohydrodynamics. The author has an hindex of 49, co-authored 118 publications receiving 8718 citations. Previous affiliations of Tibor Torok include University College London & University of St Andrews.
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Journal ArticleDOI
Sun-to-Earth MHD Simulation of the 14 July 2000 "Bastille Day" Eruption
Tibor Torok,Cooper Downs,Jon A. Linker,Roberto Lionello,Viacheslav S. Titov,Zoran Mikic,Pete Riley,Ron Caplan,Janvier Wijaya +8 more
TL;DR: In this paper, a magnetohydrodynamic (MHD) simulation of the 14 July 2000 Bastille Day eruption was presented, which produced a very strong geomagnetic storm.
Journal ArticleDOI
Initiation of Coronal Mass Ejections by Sunspot Rotation
Tibor Torok,Manuela Temmer,Manuela Temmer,Gherardo Valori,Astrid Veronig,L. van Driel-Gesztelyi,L. van Driel-Gesztelyi,L. van Driel-Gesztelyi,Bojan Vršnak +8 more
TL;DR: In this paper, the authors studied the effect of twisting the initially potential field overlying a pre-existing flux-rope, using three-dimensional zero-β MHD simulations.
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A method for embedding circular force-free flux ropes in potential magnetic fields
TL;DR: In this paper, the authors propose a method for constructing approximate force-free equilibria in pre-eruptive configurations in which a thin force free flux rope is embedded into a locally bipolar-type potential magnetic field.
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Homologous Flares and Magnetic Field Topology in Active Region NOAA 10501 on 20 November 2003
Ramesh Chandra,Brigitte Schmieder,Cristina Hemilse Mandrini,Pascal Démoulin,Etienne Pariat,Tibor Torok,Wahab Uddin +6 more
TL;DR: In this paper, the location of quasiseparatrix layers (QSLs) was calculated to understand the connectivity between the flare ribbons in order to understand how different magnetic connectivity domains of the quadrupolar configuration become unstable during each flare, so that magnetic reconnection proceeds differently in both events.
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Magnetohydrodynamic Simulations of Interplanetary Coronal Mass Ejections
TL;DR: In this paper, a new MHD model for the propagation of interplanetary coronal mass ejections (ICMEs) in the solar wind is described, which solves the MHD equations in spherical coordinates from a lower boundary above the critical point to Earth and beyond.