Pascal Demoulin
Pascal Demoulin
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Cited by
Cited by
Basic topology of twisted magnetic configurations in solar flares
VS Titov, P Démoulin
Astronomy and Astrophysics 351, 707-720, 1999
Three‐dimensional magnetic reconnection without null points: 1. Basic theory of magnetic flipping
ER Priest, P Démoulin
Journal of Geophysical Research: Space Physics 100 (A12), 23443-23463, 1995
Formation of torus-unstable flux ropes and electric currents in erupting sigmoids
G Aulanier, T Török, P Démoulin, EE DeLuca
The Astrophysical Journal 708 (1), 314, 2009
Quasi-Separatrix layers in solar flares. I. Method.
P Demoulin, JC Henoux, ER Priest, CH Mandrini
Astronomy and Astrophysics 308, 643-655, 1996
Theory of magnetic connectivity in the solar corona
VS Titov, G Hornig, P Démoulin
Journal of Geophysical Research: Space Physics 107 (A8), SSH 3-1-SSH 3-13, 2002
Quasi-separatrix layers in solar flares. II. Observed magnetic configurations.
P Demoulin, LG Bagala, CH Mandrini, JC Henoux, MG Rovira
Astronomy and Astrophysics 325, 305-317, 1997
3-D magnetic configurations supporting prominences. I. The natural presence of lateral feet
G Aulanier, P Démoulin
Astronomy and Astrophysics 329, 1125-1137, 1998
Nonlinear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection
CJ Schrijver, ML DeRosa, T Metcalf, G Barnes, B Lites, T Tarbell, ...
The Astrophysical Journal 675 (2), 1637, 2008
Coronal “wave”: magnetic footprint of a coronal mass ejection?
GDR Attrill, LK Harra, L van Driel-Gesztelyi, P Demoulin
The Astrophysical Journal Letters 656 (2), L101, 2007
What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978
P Démoulin, CH Mandrini, L van Driel-Gesztelyi, BJ Thompson, S Plunkett, ...
Astronomy & Astrophysics 382 (2), 650-665, 2002
Magnetic energy and helicity fluxes at the photospheric level
P Démoulin, MA Berger
Solar Physics 215 (2), 203-215, 2003
Conditions for the appearance of" bald patches" at the solar surface
VS Titov, ER Priest, P Demoulin
Astronomy and Astrophysics 276, 564, 1993
Magnetic field and plasma scaling laws: their implications for coronal heating models
CH Mandrini, P Démoulin, JA Klimchuk
The Astrophysical Journal 530 (2), 999, 2000
Slip-running reconnection in quasi-separatrix layers
G Aulanier, E Pariat, P Demoulin, CR DeVore
Solar Physics 238 (2), 347-376, 2006
The effect of curvature on flux-rope models of coronal mass ejections
J Lin, TG Forbes, PA Isenberg, P Démoulin
The Astrophysical Journal 504 (2), 1006, 1998
Criteria for flux rope eruption: non-equilibrium versus torus instability
P Démoulin, G Aulanier
The Astrophysical Journal 718 (2), 1388, 2010
Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes
G Aulanier, E Pariat, P Démoulin
Astronomy & Astrophysics 444 (3), 961-976, 2005
Eruption of a kink-unstable filament in NOAA active region 10696
DR Williams, T Török, P Démoulin, L van Driel-Gesztelyi, B Kliem
The Astrophysical Journal Letters 628 (2), L163, 2005
Three‐dimensional magnetic reconnection without null points: 2. Application to twisted flux tubes
P Démoulin, ER Priest, DP Lonie
Journal of Geophysical Research: Space Physics 101 (A4), 7631-7646, 1996
Evidence for the interaction of large scale magnetic structures in solar flares
CH Mandrini, P Démoulin, JC Hénoux, ME Machado
Astronomy and Astrophysics 250, 541-547, 1991
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