Pascal Démoulin spends much of his time researching Astrophysics, Coronal mass ejection, Solar flare, Magnetohydrodynamics and Magnetic flux. His work on Flare as part of general Astrophysics research is frequently linked to Rope, thereby connecting diverse disciplines of science. His work in Coronal mass ejection tackles topics such as Solar minimum which are related to areas like Solar maximum.
His Magnetohydrodynamics study integrates concerns from other disciplines, such as Interplanetary medium and Mechanics, Instability. Pascal Démoulin combines subjects such as Computational physics, Kink instability and Magnetic helicity with his study of Magnetic flux. His Field line course of study focuses on Magnetic reconnection and Solar wind, Solar physics, Geophysics and Invariant.
His primary scientific interests are in Astrophysics, Coronal mass ejection, Magnetic flux, Magnetic reconnection and Astronomy. The Astrophysics study combines topics in areas such as Photosphere, Field line and Magnetic helicity. His Coronal mass ejection research is multidisciplinary, incorporating perspectives in Interplanetary medium, Interplanetary spaceflight and Space weather.
His Magnetic flux study incorporates themes from Twist, Computational physics, Geophysics and Classical mechanics. His Magnetic reconnection study frequently draws connections between related disciplines such as Nanoflares. His Solar flare research incorporates elements of Magnetohydrodynamics, Current sheet and Magnetic energy.
Pascal Démoulin mainly focuses on Astrophysics, Coronal mass ejection, Magnetic flux, Interplanetary spaceflight and Photosphere. His research in Astrophysics intersects with topics in Field line, Plasma and Chromosphere. His work deals with themes such as Astronomy and Space weather, which intersect with Coronal mass ejection.
His study in Magnetic flux is interdisciplinary in nature, drawing from both Dispersion, Twist, Computational physics and Order of magnitude. His research integrates issues of Corona and Stellar atmosphere in his study of Photosphere. His Flare study also includes fields such as
Pascal Démoulin focuses on Astrophysics, Magnetic flux, Photosphere, Solar flare and Coronal mass ejection. Pascal Démoulin integrates many fields in his works, including Astrophysics and Rope. His studies in Magnetic flux integrate themes in fields like Solar cycle, Order of magnitude and Plasma.
His Photosphere study combines topics in areas such as Twist, Stellar atmosphere, Field line, Northern Hemisphere and Solar cycle 23. Pascal Démoulin has researched Solar flare in several fields, including Meteorology, Flare and Chromosphere. Pascal Démoulin interconnects Parameter space and Computational physics in the investigation of issues within Coronal mass ejection.
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Basic topology of twisted magnetic configurations in solar flares
V. S. Titov;P. Demoulin.
Astronomy and Astrophysics (1999)
Formation of Torus-Unstable Flux Ropes and Electric Currents in Erupting Sigmoids
G. Aulanier;T. Török;P. Démoulin;E. E. DeLuca.
The Astrophysical Journal (2010)
Three-dimensional magnetic reconnection without null points: 1. Basic theory of magnetic flipping
E. R. Priest;P. Démoulin.
Journal of Geophysical Research (1995)
Theory of magnetic connectivity in the solar corona
Vyacheslav S. Titov;Gunnar Hornig;Pascal Démoulin.
Journal of Geophysical Research (2002)
Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection
C.J. Schrijver;M.L. DeRosa;T. Metcalf;G. Barnes.
arXiv: Astrophysics (2007)
Quasi-Separatrix layers in solar flares. I. Method.
P. Demoulin;J. C. Henoux;E. R. Priest;C. H. Mandrini.
Astronomy and Astrophysics (1996)
QUASI-SEPARATRIX LAYERS IN SOLAR FLARES. II. OBSERVED MAGNETIC CONFIGURATIONS
P. Demoulin;L. G. Bagala;C. H. Mandrini;J. C. Henoux.
Astronomy and Astrophysics (1997)
3-D magnetic configurations supporting prominences I. The natural presence of lateral feet
G. Aulanier;P. Demoulin.
Astronomy and Astrophysics (1998)
Nonlinear Force‐free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection
Carolus Schrijver;Marc DeRosa;Thomas Metcalf;Graham Barnes.
The Astrophysical Journal (2008)
CRITERIA FOR FLUX ROPE ERUPTION: NON-EQUILIBRIUM VERSUS TORUS INSTABILITY
P. Démoulin;G. Aulanier.
The Astrophysical Journal (2010)
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