Pascal Demoulin

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Cristina H. MandriniInstituto de Astronomia y Fisica del EspacioVerificeret mail på iafe.uba.ar
Lidia van Driel-GesztelyiProfessor of Pysics, University College LondonVerificeret mail på obspm.fr
Sergio DassoDepartamento de Física, FCEN (UBA) - Instituto de Astronomía y Física del Espacio (UBA-CONICET)Verificeret mail på df.uba.ar
Guillaume AulanierLPP (Observatoire de Paris-PSL) & RoCS (Universitet i Oslo)Verificeret mail på lpp.polytechnique.fr
Gherardo ValoriMax Planck Institute for Solar System ResearchVerificeret mail på mps.mpg.de
E R PriestApplied Mathematics Professor, St Andrews UniversityVerificeret mail på st-andrews.ac.uk
Tibor TorokResearch Scientist, Predictive Science Inc.Verificeret mail på predsci.com
David M LongMullard Space Science Laboratory, University College LondonVerificeret mail på ucl.ac.uk
Viacheslav TitovSenior Scientist, Predictive Science Inc.Verificeret mail på predsci.com
David H. BrooksGeorge Mason UniversityVerificeret mail på ssd5.nrl.navy.mil
Barbara J. ThompsonNASA GSFCVerificeret mail på nasa.gov
James KlimchukAstrophysicist, NASA Goddard Spaceflight CenterVerificeret mail på nasa.gov
M A BergerUniversity of ExeterVerificeret mail på exeter.ac.uk
Charles FarrugiaUniversity of New HampshireVerificeret mail på unh.edu
Yang GuoNanjing University, Nanjing 210023, ChinaVerificeret mail på nju.edu.cn
Kévin DalmasseIRAP / OMPVerificeret mail på irap.omp.eu
Sarah A MatthewsUCLVerificeret mail på ucl.ac.uk
Benoit LavraudLaboratoire d'Astrophysique de Bordeaux, FranceVerificeret mail på u-bordeaux.fr
Marcos E. MachadoCONAEVerificeret mail på conae.gov.ar
Janet G LuhmannSpace Sciences Laboratory of the University of California, BerkeleyVerificeret mail på berkeley.edu

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Pascal Demoulin

LESIA, Observatoire de Paris, section of Meudon; Laboratoire Cogitamus

Verificeret mail på obspm.fr - Startside

Solar & interplanetary physics


Titel Sortér efter henvisninger Sortér efter årstal Sortér efter titel	Citeret af Citeret af	År
Basic topology of twisted magnetic configurations in solar flares VS Titov, P Démoulin Astronomy and Astrophysics, v. 351, p. 707-720 (1999) 351, 707-720, 1999	741	1999
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	534	2009
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	508	1995
Quasi-Separatrix layers in solar flares. I. Method. P Demoulin, JC Henoux, ER Priest, CH Mandrini Astronomy and Astrophysics, v. 308, p. 643-655 308, 643-655, 1996	474	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	467	2002
Quasi-separatrix layers in solar flares. II. Observed magnetic configurations. P Demoulin, LG Bagala, CH Mandrini, JC Henoux, MG Rovira Astronomy and Astrophysics, v. 325, p. 305-317 325, 305-317, 1997	340	1997
3-D magnetic configurations supporting prominences. I. The natural presence of lateral feet G Aulanier, P Démoulin Astronomy and Astrophysics, v. 329, p. 1125-1137 (1998) 329, 1125-1137, 1998	332	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	328	2008
Criteria for flux rope eruption: non-equilibrium versus torus instability P Démoulin, G Aulanier The Astrophysical Journal 718 (2), 1388, 2010	285	2010
Coronal “wave”: magnetic footprint of a coronal mass ejection? GDR Attrill, LK Harra, L van Driel-Gesztelyi, P Démoulin The Astrophysical Journal 656 (2), L101, 2007	263	2007
Slip-running reconnection in quasi-separatrix layers G Aulanier, E Pariat, P Demoulin, CR DeVore Solar Physics 238, 347-376, 2006	262	2006
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	262	2002
Magnetic energy and helicity fluxes at the photospheric level P Démoulin, MA Berger Solar Physics 215, 203-215, 2003	256	2003
Magnetic Field and Plasma Scaling Laws: Their Implications for CoronalHeating Models CH Mandrini, P Démoulin, JA Klimchuk The Astrophysical Journal 530 (2), 999, 2000	252	2000
Conditions for the appearance of" bald patches" at the solar surface VS Titov, ER Priest, P Demoulin Astronomy and Astrophysics, Vol. 276, p. 564 (1993) 276, 564, 1993	249	1993
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	239	1996
Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes G Aulanier, E Pariat, P Démoulin Astronomy & Astrophysics 444 (3), 961-976, 2005	236	2005
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	226	1998
A new model-independent method to compute magnetic helicity in magnetic clouds S Dasso, CH Mandrini, P Démoulin, ML Luoni Astronomy & Astrophysics 455 (1), 349-359, 2006	223	2006
The standard flare model in three dimensions-III. Slip-running reconnection properties M Janvier, G Aulanier, E Pariat, P Démoulin Astronomy & Astrophysics 555, A77, 2013	210	2013

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