Publications of Pascal Demoulin ordered by citations

A list of publications authored or co-authored by Pascal Demoulin, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations. Publications above the horizontal line count towards the h-index.

Orcid ID: 0000-0001-8215-6532

595	Basic topology of twisted magnetic configurations in solar flares Titov, V. S. & Démoulin, P., 1999, A&A, 351, 707
476	Formation of Torus-Unstable Flux Ropes and Electric Currents in Erupting Sigmoids Aulanier, G., Török, T., Démoulin, P. & DeLuca, E. E., 2010, ApJ, 708, 314
412	Three-dimensional magnetic reconnection without null points. 1. Basic theory of magnetic flipping Priest, E. R. & Démoulin, P., 1995, Journal of Geophysical Research, 100, 23443
390	Quasi-Separatrix layers in solar flares. I. Method. Demoulin, P., Henoux, J. C., Priest, E. R. & Mandrini, C. H., 1996, A&A, 308, 643
362	Theory of magnetic connectivity in the solar corona Titov, Vyacheslav S., Hornig, Gunnar & Démoulin, Pascal, 2002, Journal of Geophysical Research (Space Physics), 107, 1164
284	Quasi-separatrix layers in solar flares. II. Observed magnetic configurations. Demoulin, P., Bagala, L. G., Mandrini, C. H., Henoux, J. C. & Rovira, M. G., 1997, A&A, 325, 305
276	3-D magnetic configurations supporting prominences. I. The natural presence of lateral feet Aulanier, G. & Demoulin, P., 1998, A&A, 329, 1125
266	Nonlinear Force-free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection Schrijver, C. J., DeRosa, M. L., Metcalf, T., Barnes, G., Lites, B., Tarbell, T., McTiernan, J., Valori, G., Wiegelmann, T., Wheatland, M. S., Amari, T., Aulanier, G., Démoulin, P., Fuhrmann, M., Kusano, K., Régnier, S. & Thalmann, J. K., 2008, ApJ, 675, 1637
259	Criteria for Flux Rope Eruption: Non-equilibrium Versus Torus Instability Démoulin, P. & Aulanier, G., 2010, ApJ, 718, 1388
215	Slip-Running Reconnection in Quasi-Separatrix Layers Aulanier, G., Pariat, E., Démoulin, P. & Devore, C. R., 2006, Solar Physics, 238, 347
213	Coronal ``Wave'': Magnetic Footprint of a Coronal Mass Ejection? Attrill, Gemma D. R., Harra, Louise K., van Driel-Gesztelyi, Lidia & Démoulin, Pascal, 2007, ApJ, 656, L101
210	Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes Aulanier, G., Pariat, E. & Démoulin, P., 2005, A&A, 444, 961
206	Magnetic Energy and Helicity Fluxes at the Photospheric Level Démoulin, P. & Berger, M. A., 2003, Solar Physics, 215, 203
199	Three-dimensional magnetic reconnection without null points 2. Application to twisted flux tubes Démoulin, P., Priest, E. R. & Lonie, D. P., 1996, Journal of Geophysical Research, 101, 7631
197	What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978 Démoulin, P., Mandrini, C. H., van Driel-Gesztelyi, L., Thompson, B. J., Plunkett, S., Kovári, Zs., Aulanier, G. & Young, A., 2002, A&A, 382, 650
193	A new model-independent method to compute magnetic helicity in magnetic clouds Dasso, S., Mandrini, C. H., Démoulin, P. & Luoni, M. L., 2006, A&A, 455, 349
190	The standard flare model in three dimensions. III. Slip-running reconnection properties Janvier, M., Aulanier, G., Pariat, E. & Démoulin, P., 2013, A&A, 555, A77
190	Eruption of a Kink-unstable Filament in NOAA Active Region 10696 Williams, David R., Török, Tibor, Démoulin, Pascal, van Driel-Gesztelyi, Lidia & Kliem, Bernhard, 2005, ApJ, 628, L163
183	Magnetic Field and Plasma Scaling Laws: Their Implications for Coronal Heating Models Mandrini, C. H., Démoulin, P. & Klimchuk, J. A., 2000, ApJ, 530, 999
179	Conditions for the appearance of "bald patches" at the solar surface Titov, V. S., Priest, E. R. & Demoulin, P., 1993, A&A, 276, 564
173	The Effect of Curvature on Flux-Rope Models of Coronal Mass Ejections Lin, J., Forbes, T. G., Isenberg, P. A. & Démoulin, P., 1998, ApJ, 504, 1006
166	Electric Currents in Flare Ribbons: Observations and Three-dimensional Standard Model Janvier, M., Aulanier, G., Bommier, V., Schmieder, B., Démoulin, P. & Pariat, E., 2014, ApJ, 788, 60
165	The standard flare model in three dimensions. II. Upper limit on solar flare energy Aulanier, G., Démoulin, P., Schrijver, C. J., Janvier, M., Pariat, E. & Schmieder, B., 2013, A&A, 549, A66
161	The Magnetic Helicity Budget of a cme-Prolific Active Region Green, L. M., López fuentes, M. C., Mandrini, C. H., Démoulin, P., Van Driel-Gesztelyi, L. & Culhane, J. L., 2002, Solar Physics, 208, 43
160	Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars Möstl, Christian, Rollett, Tanja, Frahm, Rudy A., Liu, Ying D., Long, David M., Colaninno, Robin C., Reiss, Martin A., Temmer, Manuela, Farrugia, Charles J., Posner, Arik, Dumbović, Mateja, Janvier, Miho, Démoulin, Pascal, Boakes, Peter, Devos, Andy, Kraaikamp, Emil, Mays, Mona L. & Vršnak, Bojan, 2015, Nature Communications, 6, 7135
157	Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation Ruffenach, A., Lavraud, B., Owens, M. J., Sauvaud, J. -A., Savani, N. P., Rouillard, A. P., Démoulin, P., Foullon, C., Opitz, A., Fedorov, A., Jacquey, C. J., Génot, V., Louarn, P., Luhmann, J. G., Russell, C. T., Farrugia, C. J. & Galvin, A. B., 2012, Journal of Geophysical Research (Space Physics), 117, A09101
152	Catastrophic Evolution of a Force-free Flux Rope: A Model for Eruptive Flares Isenberg, P. A., Forbes, T. G. & Demoulin, P., 1993, ApJ, 417, 368
150	Photospheric flux density of magnetic helicity Pariat, E., Démoulin, P. & Berger, M. A., 2005, A&A, 439, 1191
148	Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed Mandrini, C. H., Pohjolainen, S., Dasso, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Copperwheat, C. & Foley, C., 2005, A&A, 434, 725
146	Coexisting Flux Rope and Dipped Arcade Sections Along One Solar Filament Guo, Y., Schmieder, B., Démoulin, P., Wiegelmann, T., Aulanier, G., Török, T. & Bommier, V., 2010, ApJ, 714, 343
145	Progressive Transformation of a Flux Rope to an ICME. Comparative Analysis Using the Direct and Fitted Expansion Methods Dasso, S., Nakwacki, M. S., Démoulin, P. & Mandrini, C. H., 2007, Solar Physics, 244, 115
144	Solar filament eruptions and their physical role in triggering coronal mass ejections Schmieder, B., Démoulin, P. & Aulanier, G., 2013, Advances in Space Research, 51, 1967
129	Causes and consequences of magnetic cloud expansion Démoulin, P. & Dasso, S., 2009, A&A, 498, 551
128	Evidence for Large-Scale Solar Magnetic Reconnection from Radio and X-Ray Measurements Manoharan, P. K., van Driel-Gesztelyi, L., Pick, M. & Demoulin, P., 1996, ApJ, 468, L73
126	Statistical study of magnetic cloud erosion by magnetic reconnection Ruffenach, A., Lavraud, B., Farrugia, C. J., Démoulin, P., Dasso, S., Owens, M. J., Sauvaud, J. -A., Rouillard, A. P., Lynnyk, A., Foullon, C., Savani, N. P., Luhmann, J. G. & Galvin, A. B., 2015, Journal of Geophysical Research (Space Physics), 120, 43
126	Observational Consequences of a Magnetic Flux Rope Emerging into the Corona Gibson, S. E., Fan, Y., Mandrini, C., Fisher, G. & Demoulin, P., 2004, ApJ, 617, 600
125	From Coronal Observations to MHD Simulations, the Building Blocks for 3D Models of Solar Flares (Invited Review) Janvier, M., Aulanier, G. & Démoulin, P., 2015, Solar Physics, 290, 3425
124	Evidence for the interaction of large scale magnetic structures in solar flares. Mandrini, C. H., Demoulin, P., Henoux, J. C. & Machado, M. E., 1991, A&A, 250, 541
123	The Structure and Evolution of a Sigmoidal Active Region Gibson, S. E., Fletcher, L., Del Zanna, G., Pike, C. D., Mason, H. E., Mandrini, C. H., Démoulin, P., Gilbert, H., Burkepile, J., Holzer, T., Alexander, D., Liu, Y., Nitta, N., Qiu, J., Schmieder, B. & Thompson, B. J., 2002, ApJ, 574, 1021
119	Extending the concept of separatrices to QSLs for magnetic reconnection Démoulin, P., 2006, Advances in Space Research, 37, 1269
115	Magnetic Reconnection along Quasi-separatrix Layers as a Driver of Ubiquitous Active Region Outflows Baker, D., van Driel-Gesztelyi, L., Mandrini, C. H., Démoulin, P. & Murray, M. J., 2009, ApJ, 705, 926
110	Global and local expansion of magnetic clouds in the inner heliosphere Gulisano, A. M., Démoulin, P., Dasso, S., Ruiz, M. E. & Marsch, E., 2010, A&A, 509, A39
110	Equilibrium and observational properties of line-tied twisted flux tubes Aulanier, G., Démoulin, P. & Grappin, R., 2005, A&A, 430, 1067
110	3-D magnetic configurations supporting prominences. II. The lateral feet as a perturbation of a twisted flux-tube Aulanier, G., Demoulin, P., van Driel-Gesztelyi, L., Mein, P. & Deforest, C., 1998, A&A, 335, 309
108	The Counterkink Rotation of a Non-Hale Active Region López Fuentes, M. C., Demoulin, P., Mandrini, C. H. & van Driel-Gesztelyi, L., 2000, ApJ, 544, 540
105	Evidence for magnetic reconnection in solar flares Demoulin, P., van Driel-Gesztelyi, L., Schmieder, B., Hemoux, J. C., Csepura, G. & Hagyard, M. J., 1993, A&A, 271, 292
101	Twisted Flux Tube Emergence Evidenced in Longitudinal Magnetograms: Magnetic Tongues Luoni, M. L., Démoulin, P., Mandrini, C. H. & van Driel-Gesztelyi, L., 2011, Solar Physics, 270, 45
97	Modelling and observations of photospheric magnetic helicity Démoulin, P. & Pariat, E., 2009, Advances in Space Research, 43, 1013
95	Magnetic twist and writhe of active regions. On the origin of deformed flux tubes López Fuentes, M. C., Démoulin, P., Mandrini, C. H., Pevtsov, A. A. & van Driel-Gesztelyi, L., 2003, A&A, 397, 305
94	Differential Magnetic Field Shear in an Active Region Schmieder, B., Demoulin, P., Aulanier, G. & Golub, L., 1996, ApJ, 467, 881
92	Are magnetic null points important in solar flares ? Demoulin, P., Henoux, J. C. & Mandrini, C. H., 1994, A&A, 285, 1023
91	Estimation of the squashing degree within a three-dimensional domain Pariat, E. & Démoulin, P., 2012, A&A, 541, A78
91	3D Magnetic Reconnection at an X-Ray Bright Point Mandrini, C. H., Démoulin, P., Van Driel-Gesztelyi, L., Schmieder, B., Cauzzi, G. & Hofmann, A., 1996, Solar Physics, 168, 115
91	The Magnetic Helicity Injected by Shearing Motions Démoulin, P., Mandrini, C. H., Van Driel-Gesztelyi, L., Lopez Fuentes, M. C. & Aulanier, G., 2002, Solar Physics, 207, 87
91	3-D magnetic configurations supporting prominences. III. Evolution of fine structures observed in a filament channel Aulanier, G., Démoulin, P., Mein, N., van Driel-Gesztelyi, L., Mein, P. & Schmieder, B., 1999, A&A, 342, 867
87	Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections Démoulin, P., Nakwacki, M. S., Dasso, S. & Mandrini, C. H., 2008, Solar Physics, 250, 347
82	Are CME-Related Dimmings Always a Simple Signature of Interplanetary Magnetic Cloud Footpoints? Mandrini, C. H., Nakwacki, M. S., Attrill, G., van Driel-Gesztelyi, L., Démoulin, P., Dasso, S. & Elliott, H., 2007, Solar Physics, 244, 25
80	Homologous Flares and Magnetic Field Topology in Active Region NOAA 10501 on 20 November 2003 Chandra, R., Schmieder, B., Mandrini, C. H., Démoulin, P., Pariat, E., Török, T. & Uddin, W., 2011, Solar Physics, 269, 83
79	Large scale MHD properties of interplanetary magnetic clouds Dasso, S., Mandrini, C. H., Démoulin, P., Luoni, M. L. & Gulisano, A. M., 2005, Advances in Space Research, 35, 711
78	Relationship between magnetic field evolution and flaring sites in AR 6659 in June 1991 Schmieder, B., Hagyard, M. J., Guoxiang, Ai, Hongqi, Zhang, Kalman, B., Gyori, L., Rompolt, B., Demoulin, P. & Machado, M. E., 1994, Solar Physics, 150, 199
77	The Magnetic Structure of Coronal Loops Observed by TRACE López Fuentes, M. C., Klimchuk, J. A. & Démoulin, P., 2006, ApJ, 639, 459
75	Magnetic reconnection driven by emergence of sheared magnetic field. Schmieder, B., Aulanier, G., Demoulin, P., van Driel-Gesztelyi, L., Roudier, T., Nitta, N. & Cauzzi, G., 1997, A&A, 325, 1213
75	Recent theoretical and observational developments in magnetic helicity studies Démoulin, P., 2007, Advances in Space Research, 39, 1674
75	Emerging Flux and the Heating of Coronal Loops Schmieder, B., Rust, D. M., Georgoulis, M. K., Démoulin, P. & Bernasconi, P. N., 2004, ApJ, 601, 530
74	Generic Magnetic Field Intensity Profiles of Interplanetary Coronal Mass Ejections at Mercury, Venus, and Earth From Superposed Epoch Analyses Janvier, Miho, Winslow, Reka M., Good, Simon, Bonhomme, Elise, Démoulin, Pascal, Dasso, Sergio, Möstl, Christian, Lugaz, Noé, Amerstorfer, Tanja, Soubrié, Elie & Boakes, Peter D., 2019, Journal of Geophysical Research (Space Physics), 124, 812
71	Comparing Values of the Relative Magnetic Helicity in Finite Volumes Valori, G., Démoulin, P. & Pariat, E., 2012, Solar Physics, 278, 347
71	Recurrent coronal jets induced by repetitively accumulated electric currents Guo, Y., Démoulin, P., Schmieder, B., Ding, M. D., Vargas Domínguez, S. & Liu, Y., 2013, A&A, 555, A19
69	Interpretation of multiwavelength observations of November 5, 1980 solar flares by the magnetic topology of AR 2766 Demoulin, P., Mandrini, C. H., Rovira, M. G., Henoux, J. C. & Machado, M. E., 1994, Solar Physics, 150, 221
68	Nonlinear Force-Free Extrapolation of Emerging Flux with a Global Twist and Serpentine Fine Structures Valori, G., Green, L. M., Démoulin, P., Vargas Domínguez, S., van Driel-Gesztelyi, L., Wallace, A., Baker, D. & Fuhrmann, M., 2012, Solar Physics, 278, 73
68	Development of a Topological Model for Solar Flares Demoulin, P., Henoux, J. C. & Mandrini, C. H., 1992, Solar Physics, 139, 105
68	A review of the quantitative links between CMEs and magnetic clouds Démoulin, P., 2008, Annales Geophysicae, 26, 3113
67	Companion Event and Precursor of the X17 Flare on 28 October 2003 Mandrini, C. H., Demoulin, P., Schmieder, B., Deluca, E. E., Pariat, E. & Uddin, W., 2006, Solar Physics, 238, 293
66	Superposed epoch study of ICME sub-structures near Earth and their effects on Galactic cosmic rays Masías-Meza, J. J., Dasso, S., Démoulin, P., Rodriguez, L. & Janvier, M., 2016, A&A, 592, A118
66	Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind van Driel-Gesztelyi, L., Culhane, J. L., Baker, D., Démoulin, P., Mandrini, C. H., DeRosa, M. L., Rouillard, A. P., Opitz, A., Stenborg, G., Vourlidas, A. & Brooks, D. H., 2012, Solar Physics, 281, 237
65	Linking two consecutive nonmerging magnetic clouds with their solar sources Dasso, S., Mandrini, C. H., Schmieder, B., Cremades, H., Cid, C., Cerrato, Y., Saiz, E., Démoulin, P., Zhukov, A. N., Rodriguez, L., Aran, A., Menvielle, M. & Poedts, S., 2009, Journal of Geophysical Research (Space Physics), 114, A02109
65	Quasi-Separatrix Layers in a Reduced Magnetohydrodynamic Model of a Coronal Loop Milano, Leonardo J., Dmitruk, Pablo, Mandrini, Cristina H., Gómez, Daniel O. & Démoulin, Pascal, 1999, ApJ, 521, 889
64	Evidence of Magnetic Reconnection from Hα, Soft X-Ray and Photospheric Magnetic Field Observations Mandrini, C. H., DÉmoulin, P., BagalÁ, L. G., Van Driel-Gesztelyi, L., HÉnoux, J. C., Schmieder, B. & Rovira, M. G., 1997, Solar Physics, 174, 229
62	How are Emerging Flux, Flares and CMEs Related to Magnetic Polarity Imbalance in Midi Data? Green, L. M., Démoulin, P., Mandrini, C. H. & Van Driel-Gesztelyi, L., 2003, Solar Physics, 215, 307
61	Magnetic helicity analysis of an interplanetary twisted flux tube Dasso, S., Mandrini, C. H., DéMoulin, P. & Farrugia, C. J., 2003, Journal of Geophysical Research (Space Physics), 108, 1362
61	Testing magnetic helicity conservation in a solar-like active event Pariat, E., Valori, G., Démoulin, P. & Dalmasse, K., 2015, A&A, 580, A128
60	Evidence for magnetic reconnection in large-scale magnetic structures in solar flares Mandrini, C. H., Rovira, M. G., Demoulin, P., Henoux, J. C., Machado, M. E. & Wilkinson, L. K., 1993, A&A, 272, 609
60	Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events Mandrini, C. H., Schmieder, B., Démoulin, P., Guo, Y. & Cristiani, G. D., 2014, Solar Physics, 289, 2041
57	Constraints on flare models set by the active region magnetic topology Magnetic topology of AR 6233. Mandrini, C. H., Demoulin, P., Rovira, M. G., de La Beaujardiere, J. -F. & Henoux, J. C., 1995, A&A, 303, 927
57	Coronal Magnetic Reconnection Driven by CME Expansion—the 2011 June 7 Event van Driel-Gesztelyi, L., Baker, D., Török, T., Pariat, E., Green, L. M., Williams, D. R., Carlyle, J., Valori, G., Démoulin, P., Kliem, B., Long, D. M., Matthews, S. A. & Malherbe, J. -M., 2014, ApJ, 788, 85
55	Dynamical evolution of a magnetic cloud from the Sun to 5.4 AU Nakwacki, M. S., Dasso, S., Démoulin, P., Mandrini, C. H. & Gulisano, A. M., 2011, A&A, 535, A52
55	Basic Properties of Mutual Magnetic Helicity Demoulin, P., Pariat, E. & Berger, M. A., 2006, Solar Physics, 233, 3
53	Plasma Composition in a Sigmoidal Anemone Active Region Baker, D., Brooks, D. H., Démoulin, P., van Driel-Gesztelyi, L., Green, L. M., Steed, K. & Carlyle, J., 2013, ApJ, 778, 69
52	What is the spatial distribution of magnetic helicity injected in a solar active region? Pariat, E., Nindos, A., Démoulin, P. & Berger, M. A., 2006, A&A, 452, 623
52	The role of magnetic bald patches in surges and arch filament systems Mandrini, C. H., Démoulin, P., Schmieder, B., Deng, Y. Y. & Rudawy, P., 2002, A&A, 391, 317
52	Accuracy of magnetic energy computations Valori, G., Démoulin, P., Pariat, E. & Masson, S., 2013, A&A, 553, A38
51	Expansion of magnetic clouds in the outer heliosphere Gulisano, A. M., Démoulin, P., Dasso, S. & Rodriguez, L., 2012, A&A, 543, A107
51	A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence Demoulin, P. & Priest, E. R., 1989, A&A, 214, 360
51	Magnetohydrostatic Model of a Bald-Patch Flare Aulanier, G., Démoulin, P., Schmieder, B., Fang, C. & Tang, Y. H., 1998, Solar Physics, 183, 369
50	Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation Janvier, M., Démoulin, P. & Dasso, S., 2013, A&A, 556, A50
50	Filament Interaction Modeled by Flux Rope Reconnection Török, T., Chandra, R., Pariat, E., Démoulin, P., Schmieder, B., Aulanier, G., Linton, M. G. & Mandrini, C. H., 2011, ApJ, 728, 65
48	Are There Different Populations of Flux Ropes in the Solar Wind? Janvier, M., Démoulin, P. & Dasso, S., 2014, Solar Physics, 289, 2633
48	Radio and X-Ray Signatures of Magnetic Reconnection behind an Ejected Flux Rope Pick, M., Démoulin, P., Krucker, S., Malandraki, O. & Maia, D., 2005, ApJ, 625, 1019
48	Amplitude and orientation of prominence magnetic fields from constant-alpha magnetohydrostatic models Aulanier, G. & Démoulin, P., 2003, A&A, 402, 769
46	Magnetic cloud models with bent and oblate cross-section boundaries Démoulin, P. & Dasso, S., 2009, A&A, 507, 969
46	Reduction, Analysis, and Properties of Electric Current Systems in Solar Active Regions Gary, G. Allen & Demoulin, Pascal, 1995, ApJ, 445, 982
44	The Long-Term Evolution of AR 7978: The Scalings of the Coronal Plasma Parameters with the Mean Photospheric Magnetic Field van Driel-Gesztelyi, L., Démoulin, P., Mandrini, C. H., Harra, L. & Klimchuk, J. A., 2003, ApJ, 586, 579
44	Relationship between electric currents, photospheric motions, chromospheric activity, and magnetic field topology van Driel-Gesztelyi, L., Hofmann, A., Demoulin, P., Schmieder, B. & Csepura, G., 1994, Solar Physics, 149, 309
44	Instability of a prominence supported in a linear force-free field Demoulin, P. & Priest, E. R., 1988, A&A, 206, 336
43	Coronal ``wave'': A signature of the mechanism making CMEs large-scale in the low corona? Attrill, G. D. R., Harra, L. K., van Driel-Gesztelyi, L., Démoulin, P. & Wülser, J. -P., 2007, Astronomische Nachrichten, 328, 760
43	Magnetic reconnection: a common origin for flares and AR interconnecting arcs Bagalá, L. G., Mandrini, C. H., Rovira, M. G. & Démoulin, P., 2000, A&A, 363, 779
42	Estimation of the bias of the Minimum Variance technique in the determination of magnetic clouds global quantities and orientation Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., 2007, Advances in Space Research, 40, 1881
42	Tracking Solar Active Region Outflow Plasma from Its Source to the Near-Earth Environment Culhane, J. L., Brooks, D. H., van Driel-Gesztelyi, L., Démoulin, P., Baker, D., DeRosa, M. L., Mandrini, C. H., Zhao, L. & Zurbuchen, T. H., 2014, Solar Physics, 289, 3799
42	A Topological Approach to Understand a Multiple-Loop Solar Flare Bagalá, L. G., Mandrini, C. H., Rovira, M. G., Démoulin, P. & Hénoux, J. C., 1995, Solar Physics, 161, 103
41	Magnetic clouds: A statistical study of magnetic helicity Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., 2005, Journal of Atmospheric and Solar-Terrestrial Physics, 67, 1761
41	FIP Bias Evolution in a Decaying Active Region Baker, D., Brooks, D. H., Démoulin, P., Yardley, S. L., van Driel-Gesztelyi, L., Long, D. M. & Green, L. M., 2015, ApJ, 802, 104
40	A Relationship Between Transition Region Brightenings, Abundances, and Magnetic Topology Fletcher, Lyndsay, López Fuentes, Marcelo C., Mandrini, Cristina H., Schmieder, Brigitte, Démoulin, Pascal, Mason, Helen E., Young, Peter R. & Nitta, Nariaki, 2001, Solar Physics, 203, 255
40	The Origin of Net Electric Currents in Solar Active Regions Dalmasse, K., Aulanier, G., Démoulin, P., Kliem, B., Török, T. & Pariat, E., 2015, ApJ, 810, 17
39	Understanding Coronal Mass Ejections and Associated Shocks in the Solar Corona by Merging Multiwavelength Observations Zucca, P., Pick, M., Démoulin, P., Kerdraon, A., Lecacheux, A. & Gallagher, P. T., 2014, ApJ, 795, 68
39	Where will efficient energy release occur in 3-D magnetic configurations? Démoulin, P., 2007, Advances in Space Research, 39, 1367
38	Determination of force-free magnetic fields above the photosphere using three-component boundary conditions. II - Analysis and minimization of scale-related growing modes and of computational induced singularities Demoulin, P., Cuperman, S. & Semel, M., 1992, A&A, 263, 351
38	Can we Extrapolate a Magnetic Field when its Topology is Complex? DÉmoulin, P., HÉnoux, J. C., Mandrini, C. H. & Priest, E. R., 1997, Solar Physics, 174, 73
38	The interplanetary magnetic structure that guides solar relativistic particles Masson, S., Démoulin, P., Dasso, S. & Klein, K. -L., 2012, A&A, 538, A32
37	Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU Rodriguez, L., Masías-Meza, J. J., Dasso, S., Démoulin, P., Zhukov, A. N., Gulisano, A. M., Mierla, M., Kilpua, E., West, M., Lacatus, D., Paraschiv, A. & Janvier, M., 2016, Solar Physics, 291, 2145
37	Interactions between nested sunspots. II. A confined X1 flare in a delta-type sunspot Gaizauskas, V., Mandrini, C. H., Demoulin, P., Luoni, M. L. & Rovira, M. G., 1998, A&A, 332, 353
36	Initiation and Development of the White-light and Radio Coronal Mass Ejection on 2001 April 15 Démoulin, P., Vourlidas, A., Pick, M. & Bouteille, A., 2012, ApJ, 750, 147
36	Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections? Démoulin, P., 2009, Solar Physics, 257, 169
36	A Model for an Inverse Polarity Prominence Supported in a Dip of a Quadrupolar Region Demoulin, P. & Priest, E. R., 1993, Solar Physics, 144, 283
36	The Long-Term Evolution of AR 7978: Testing Coronal Heating Models Démoulin, P., van Driel-Gesztelyi, L., Mandrini, C. H., Klimchuk, J. A. & Harra, L., 2003, ApJ, 586, 592
35	Magnetic Activity Associated With Radio Noise Storms Bentley, R. D., Klein, K. -L., van Driel-Gesztelyi, L., Démoulin, P., Trottet, G., Tassetto, P. & Marty, G., 2000, Solar Physics, 193, 227
35	The Recovery of CME-Related Dimmings and the ICME's Enduring Magnetic Connection to the Sun Attrill, G. D. R., van Driel-Gesztelyi, L., Démoulin, P., Zhukov, A. N., Steed, K., Harra, L. K., Mandrini, C. H. & Linker, J., 2008, Solar Physics, 252, 349
35	Flows in the solar atmosphere due to the eruptions on the 15th July, 2002 Harra, L. K., Démoulin, P., Mandrini, C. H., Matthews, S. A., van Driel-Gesztelyi, L., Culhane, J. L. & Fletcher, L., 2005, A&A, 438, 1099
35	Dynamics of solar filaments. VI - Center-to-limb study of H-alpha and C IV velocities in a quiescent filament Simon, G., Schmieder, B., Demoulin, P. & Poland, A. I., 1986, A&A, 166, 319
34	The Importance of Photospheric Intense Flux Tubes for Coronal Heating Démoulin, P. & Priest, E. R., 1997, Solar Physics, 175, 123
33	Does spacecraft trajectory strongly affect detection of magnetic clouds? Démoulin, P., Dasso, S. & Janvier, M., 2013, A&A, 550, A3
33	Implications of Non-cylindrical Flux Ropes for Magnetic Cloud Reconstruction Techniques and the Interpretation of Double Flux Rope Events Owens, M. J., Démoulin, P., Savani, N. P., Lavraud, B. & Ruffenach, A., 2012, Solar Physics, 278, 435
33	In situ properties of small and large flux ropes in the solar wind Janvier, M., Démoulin, P. & Dasso, S., 2014, Journal of Geophysical Research (Space Physics), 119, 7088
33	Tracing magnetic helicity from the solar corona to the interplanetary space Luoni, M. L., Mandrini, C. H., Dasso, Sergio, van Driel-Gesztelyi, L. & Démoulin, P., 2005, Journal of Atmospheric and Solar-Terrestrial Physics, 67, 1734
32	Parallel Evolution of Quasi-separatrix Layers and Active Region Upflows Mandrini, C. H., Baker, D., Démoulin, P., Cristiani, G. D., van Driel-Gesztelyi, L., Vargas Domínguez, S., Nuevo, F. A., Vásquez, A. M. & Pick, M., 2015, ApJ, 809, 73
32	CFHT eclipse observation of the very fine-scale solar corona Koutchmy, S., Belmahdi, M., Coulter, R. L., Demoulin, P., Gaizauskas, V., MacQueen, R. M., Monnet, G., Mouette, J., Noens, J. C. & November, L. J., 1994, A&A, 281, 249
32	Why Are Flare Ribbons Associated with the Spines of Magnetic Null Points Generically Elongated? Pontin, David, Galsgaard, Klaus & Démoulin, Pascal, 2016, Solar Physics, 291, 1739
32	Evolution of Hard X-Ray Sources and Ultraviolet Solar Flare Ribbons for a Confined Eruption of a Magnetic Flux Rope Guo, Y., Ding, M. D., Schmieder, B., Démoulin, P. & Li, H., 2012, ApJ, 746, 17
32	Are Constant Loop Widths an Artifact of the Background and the Spatial Resolution? López Fuentes, M. C., Démoulin, P. & Klimchuk, J. A., 2008, ApJ, 673, 586
32	The creation of the magnetic environment for prominence formation in a coronal arcade Amari, T., Démoulin, P., Browning, P., Hood, A. & Priest, E., 1991, A&A, 241, 604
32	Magnetic Helicity Budget of Solar-Active Regions from the Photosphere to Magnetic Clouds Mandrini, C. H., Démoulin, P., Van Driel-Gesztelyi, L., Van Driel-Gesztelyi, L., Van Driel-Gesztelyi, L., Van Driel-Gesztelyi, L. L. M. & Fuentes, M. C. López, 2004, Astrophysics and Space Science, 290, 319
31	Comparing generic models for interplanetary shocks and magnetic clouds axis configurations at 1 AU Janvier, M., Dasso, S., Démoulin, P., Masías-Meza, J. J. & Lugaz, N., 2015, Journal of Geophysical Research (Space Physics), 120, 3328
31	Observations of magnetic helicity van Driel-Gesztelyi, L., Démoulin, P. & Mandrini, C. H., 2003, Advances in Space Research, 32, 1855
30	Mean shape of interplanetary shocks deduced from in situ observations and its relation with interplanetary CMEs Janvier, M., Démoulin, P. & Dasso, S., 2014, A&A, 565, A99
30	The properties of sources and sinks of a linear force-free field Demoulin, P. & Priest, E. R., 1992, A&A, 258, 535
30	Emergence of a U-loop - sub-photospheric link between solar active regions van Driel-Gesztelyi, L., Malherbe, J. -M. & Démoulin, P., 2000, A&A, 364, 845
30	Transient Inverse-FIP Plasma Composition Evolution within a Solar Flare Baker, Deborah, van Driel-Gesztelyi, Lidia, Brooks, David H., Valori, Gherardo, James, Alexander W., Laming, J. Martin, Long, David M., Démoulin, Pascal, Green, Lucie M., Matthews, Sarah A., Oláh, Katalin & Kővári, Zsolt, 2019, ApJ, 875, 35
29	Signatures of interchange reconnection: STEREO, ACE and Hinode observations combined Baker, D., Rouillard, A. P., van Driel-Gesztelyi, L., Démoulin, P., Harra, L. K., Lavraud, B., Davies, J. A., Opitz, A., Luhmann, J. G., Sauvaud, J. -A. & Galvin, A. B., 2009, Annales Geophysicae, 27, 3883
29	Initiation of CMEs: the role of magnetic twist van Driel-Gesztelyi, L., Manoharan, P. K., Démoulin, P., Aulanier, G., Mandrini, C. H., Lopez-Fuentes, M., Schmieder, B., Orlando, S., Thompson, B. & Plunkett, S., 2000, Journal of Atmospheric and Solar-Terrestrial Physics, 62, 1437
28	Evidence of Twisted Flux-Tube Emergence in Active Regions Poisson, M., Mandrini, C. H., Démoulin, P. & López Fuentes, M., 2015, Solar Physics, 290, 727
28	Photospheric Injection of Magnetic Helicity: Connectivity-Based Flux Density Method Dalmasse, K., Pariat, E., Démoulin, P. & Aulanier, G., 2014, Solar Physics, 289, 107
28	Modeling the Effect of Mass-draining on Prominence Eruptions Jenkins, Jack M., Hopwood, Matthew, Démoulin, Pascal, Valori, Gherardo, Aulanier, Guillaume, Long, David M. & van Driel-Gesztelyi, Lidia, 2019, ApJ, 873, 49
28	First observational application of a connectivity-based helicity flux density Dalmasse, K., Pariat, E., Valori, G., Démoulin, P. & Green, L. M., 2013, A&A, 555, L6
28	The magnetic field topology associated with two M flares Luoni, M. L., Mandrini, C. H., Cristiani, G. D. & Démoulin, P., 2007, Advances in Space Research, 39, 1382
27	Successive injection of opposite magnetic helicity in solar active region NOAA 11928 Vemareddy, P. & Démoulin, P., 2017, A&A, 597, A104
26	Fine structures in solar filaments. I - Observations and thermal stability Demoulin, P., Malherbe, J. M., Schmieder, B. & Raadu, M. A., 1987, A&A, 183, 142
26	Why are CMEs large-scale coronal events: nature or nurture? van Driel-Gesztelyi, L., Attrill, G. D. R., Démoulin, P., Mandrini, C. H. & Harra, L. K., 2008, Annales Geophysicae, 26, 3077
26	Analysis of large scale MHD quantities in expanding magnetic clouds Nakwacki, María Soledad, Dasso, Sergio, Mandrini, Cristina Hemilse & Démoulin, Pascal, 2008, Journal of Atmospheric and Solar-Terrestrial Physics, 70, 1318
26	Coronal Elemental Abundances in Solar Emerging Flux Regions Baker, Deborah, Brooks, David H., van Driel-Gesztelyi, Lidia, James, Alexander W., Démoulin, Pascal, Long, David M., Warren, Harry P. & Williams, David R., 2018, ApJ, 856, 71
25	Dynamics of solar magnetic arches in the photosphere and the chromosphere. Mein, P., Demoulin, P., Mein, N., Engvold, O., Molowny-Horas, R., Heinzel, P. & Gontikakis, C., 1996, A&A, 305, 343
25	A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME Goff, C. P., van Driel-Gesztelyi, L., Démoulin, P., Culhane, J. L., Matthews, S. A., Harra, L. K., Mandrini, C. H., Klein, K. L. & Kurokawa, H., 2007, Solar Physics, 240, 283
25	How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer? Mandrini, C. H., Nuevo, F. A., Vásquez, A. M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., Culhane, J. L., Cristiani, G. D. & Pick, M., 2014, Solar Physics, 289, 4151
24	The 3D Geometry of Active Region Upflows Deduced from Their Limb-to-Limb Evolution Démoulin, P., Baker, D., Mandrini, C. H. & van Driel-Gesztelyi, L., 2013, Solar Physics, 283, 341
24	Sequential Eruptions Triggered by Flux Emergence: Observations and Modeling Dacie, S., Török, T., Démoulin, P., Linton, M. G., Downs, C., van Driel-Gesztelyi, L., Long, D. M. & Leake, J. E., 2018, ApJ, 862, 117
24	Magnetic Flux and Helicity of Magnetic Clouds Démoulin, P., Janvier, M. & Dasso, S., 2016, Solar Physics, 291, 531
24	Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au and Their Semiempirical Isopoly Fluid Modeling Dakeyo, Jean-Baptiste, Maksimovic, Milan, Démoulin, Pascal, Halekas, Jasper & Stevens, Michael L., 2022, ApJ, 940, 130
24	Alfvénic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma in the Corona Baker, Deborah, Stangalini, Marco, Valori, Gherardo, Brooks, David H., To, Andy S. H., van Driel-Gesztelyi, Lidia, Démoulin, Pascal, Stansby, David, Jess, David B. & Jafarzadeh, Shahin, 2021, ApJ, 907, 16
23	Removal of singularities in the Cauchy problem for the extrapolation of solar force-free magnetic fields Cuperman, S., Demoulin, P. & Semel, M., 1991, A&A, 245, 285
23	Vortex and Sink Flows in Eruptive Flares as a Model for Coronal Implosions Zuccarello, F. P., Aulanier, G., Dudík, J., Démoulin, P., Schmieder, B. & Gilchrist, S. A., 2017, ApJ, 837, 115
23	Investigating the observational signatures of magnetic cloud substructure Steed, K., Owen, C. J., Démoulin, P. & Dasso, S., 2011, Journal of Geophysical Research (Space Physics), 116, A01106
23	Initiation and Early Development of the 2008 April 26 Coronal Mass Ejection Huang, J., Démoulin, P., Pick, M., Auchère, F., Yan, Y. H. & Bouteille, A., 2011, ApJ, 729, 107
22	A three-dimensional model for solar prominences Demoulin, P., Priest, E. R. & Anzer, U., 1989, A&A, 221, 326
22	Interaction of ICMEs with the Solar Wind Démoulin, Pascal, 2010, Twelfth International Solar Wind Conference (Editors: Maksimovic, M., Issautier, K., Meyer-Vernet, N., Moncuquet, M. & Pantellini, F.), American Institute of Physics Conference Series, 1216, p. 329
21	Hα and Soft X-Ray Brightening Events Caused by Emerging Flux Tang, Y. H., Li, Y. N., Fang, C., Aulanier, G., Schmieder, B., Demoulin, P. & Sakurai, T., 2000, ApJ, 534, 482
21	Relationships between CME's and prominences Schmieder, B., van Driel-Gesztelyi, L., Aulanier, G., Démoulin, P., Thompson, B., De Forest, C., Wiik, J. E., Saint Cyr, C. & Vial, J. C., 2002, Advances in Space Research, 29, 1451
20	Distribution of Electric Currents in Sunspots from Photosphere to Corona Gosain, Sanjay, Démoulin, Pascal & López Fuentes, Marcelo, 2014, ApJ, 793, 15
19	Properties of Magnetic Tongues over a Solar Cycle Poisson, Mariano, Démoulin, Pascal, López Fuentes, Marcelo & Mandrini, Cristina H., 2016, Solar Physics, 291, 1625
19	Model-independent large-scale magnetohydrodynamic quantities in magnetic clouds Dasso, S., Gulisano, A. M., Mandrini, C. H. & Démoulin, P., 2005, Advances in Space Research, 35, 2172
18	Structural Characteristics of Eruptive Prominences Demoulin, P. & Vial, J. C., 1992, Solar Physics, 141, 289
18	Magnetic reconfiguration before the X 17 Solar flare of October 28 2003 Schmieder, B., Mandrini, C. H., Démoulin, P., Pariat, E., Berlicki, A. & Deluca, E., 2006, Advances in Space Research, 37, 1313
17	Some dynamical aspects of a quiescent filament Schmieder, B., Demoulin, P., Poland, A. & Thompson, B., 1988, A&A, 197, 281
17	How to improve the maps of magnetic helicity injection in active regions? Pariat, Etienne, Démoulin, Pascal & Nindos, Alexander, 2007, Advances in Space Research, 39, 1706
17	The evolution of writhe in kink-unstable flux ropes and erupting filaments Török, T., Kliem, B., Berger, M. A., Linton, M. G., Démoulin, P. & van Driel-Gesztelyi, L., 2014, Plasma Physics and Controlled Fusion, 56, 064012
17	What is the role of magnetic null points in large flares? Schmieder, B., Mandrini, C. H., Démoulin, P., Aulanier, G., Li, H. & Berlicki, A., 2007, Advances in Space Research, 39, 1840
16	The magnetic field around quiescent solar prominences computed from observational boundary conditions Demoulin, P., Malherbe, J. M. & Priest, E. R., 1989, A&A, 211, 428
16	Expanding and Contracting Coronal Loops as Evidence of Vortex Flows Induced by Solar Eruptions Dudík, J., Zuccarello, F. P., Aulanier, G., Schmieder, B. & Démoulin, P., 2017, ApJ, 844, 54
15	Quantitative model for the generic 3D shape of ICMEs at 1 AU Démoulin, P., Janvier, M., Masías-Meza, J. J. & Dasso, S., 2016, A&A, 595, A19
15	Observational Evidence of S-web Source of the Slow Solar Wind Baker, D., Démoulin, P., Yardley, S. L., Mihailescu, T., van Driel-Gesztelyi, L., D'Amicis, R., Long, D. M., To, A. S. H., Owen, C. J., Horbury, T. S., Brooks, D. H., Perrone, D., French, R. J., James, A. W., Janvier, M., Matthews, S., Stangalini, M., Valori, G., Smith, P., Cuadrado, R. Aznar, Peter, H., Schuehle, U., Harra, L., Barczynski, K., Berghmans, D., Zhukov, A. N., Rodriguez, L. & Verbeeck, C., 2023, ApJ, 950, 65
14	Weighted Current Sheets Supported in Normal and Inverse Configurations: A Model for Prominence Observations Demoulin, P. & Forbes, T. G., 1992, ApJ, 387, 394
14	Dynamics of a filament at the boundary of a SPOT region with magnetic shear Schmiedler, B., Demoulin, P., Raadu, M. A. & Dere, K. P., 1989, A&A, 213, 402
14	Apparent and Intrinsic Evolution of Active Region Upflows Baker, Deborah, Janvier, Miho, Démoulin, Pascal & Mandrini, Cristina H., 2017, Solar Physics, 292, 46
14	Contribution of the ageing effect to the observed asymmetry of interplanetary magnetic clouds Démoulin, P., Dasso, S., Lanabere, V. & Janvier, M., 2020, A&A, 639, A6
14	Structuring of the Solar Plasma by the Magnetic Field Demoulin, Pascal & Klein, Karl-Ludwig, 2000, Transport and Energy Conversion in the Heliosphere (Editors: Rozelot, J. P., Klein, L. & Vial, J. -C.), p.99
14	Can Subphotospheric Magnetic Reconnection Change the Elemental Composition in the Solar Corona? Baker, Deborah, van Driel-Gesztelyi, Lidia, Brooks, David H., Démoulin, Pascal, Valori, Gherardo, Long, David M., Laming, J. Martin, To, Andy S. H. & James, Alexander W., 2020, ApJ, 894, 35
14	The Two-step Forbush Decrease: A Tale of Two Substructures Modulating Galactic Cosmic Rays within Coronal Mass Ejections Janvier, Miho, Démoulin, Pascal, Guo, Jingnan, Dasso, Sergio, Regnault, Florian, Topsi-Moutesidou, Sofia, Gutierrez, Christian & Perri, Barbara, 2021, ApJ, 922, 216
14	Measurement of coronal magnetic twists during loop emergence of NOAA 8069 Portier-Fozzani, F., Aschwanden, M., Démoulin, P., Neupert, W., EIT Team & Delaboudinière, J. -P., 2001, Solar Physics, 203, 289
13	Physical Processes Involved in the EUV "Surge" Event of 9 May 2012 López Fuentes, Marcelo, Mandrini, Cristina H., Poisson, Mariano, Démoulin, Pascal, Cristiani, Germán, López, Fernando M. & Luoni, Maria Luisa, 2018, Solar Physics, 293, 166
13	Actors of the main activity in large complex centres during the 23 solar cycle maximum Schmieder, B., Démoulin, P., Pariat, E., Török, T., Molodij, G., Mandrini, C. H., Dasso, S., Chandra, R., Uddin, W., Kumar, P., Manoharan, P. K., Venkatakrishnan, P. & Srivastava, N., 2011, Advances in Space Research, 47, 2081
13	Decametric N Burst: A Consequence of the Interaction of Two Coronal Mass Ejections Démoulin, P., Klein, K. -L., Goff, C. P., van Driel-Gesztelyi, L., Culhane, J. L., Mandrini, C. H., Matthews, S. A. & Harra, L. K., 2007, Solar Physics, 240, 301
13	Study of Three-dimensional Magnetic Structure and the Successive Eruptive Nature of Active Region 12371 Vemareddy, P. & Demóulin, P., 2018, ApJ, 857, 90
12	Active-Region Twist Derived from Magnetic Tongues and Linear Force-Free Extrapolations Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H. & Démoulin, Pascal, 2015, Solar Physics, 290, 3279
12	Instability of a prominence supported in a linear force-free field. II - Effect of twist or flux conservation Demoulin, P., Ferreira, J. & Priest, E. R., 1991, A&A, 245, 289
11	Exploring the biases of a new method based on minimum variance for interplanetary magnetic clouds Démoulin, P., Dasso, S. & Janvier, M., 2018, A&A, 619, A139
11	The smallest source region of an interplanetary magnetic cloud: A mini-sigmoid Mandrini, C. H., Pohjolainen, S., Dasso, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Foley, C. & Copperwheat, C., 2005, Advances in Space Research, 36, 1579
11	Common Evolution of Adjacent Sunspot Groups van Driel-Gesztelyi, L., Csepura, G., Nagy, I., Gerlei, O., Schmieder, B., Rayrole, J. & Demoulin, P., 1993, Solar Physics, 145, 77
11	Studying the Transfer of Magnetic Helicity in Solar Active Regions with the Connectivity-based Helicity Flux Density Method Dalmasse, K., Pariat, É., Valori, G., Jing, J. & Démoulin, P., 2018, ApJ, 852, 141
11	The Magnetic Environment of a Stealth Coronal Mass Ejection O'Kane, Jennifer, Mac Cormack, Cecilia, Mandrini, Cristina H., Démoulin, Pascal, Green, Lucie M., Long, David M. & Valori, Gherardo, 2021, ApJ, 908, 89
10	Homologous Solar Events on 2011 January 27: Build-up and Propagation in a Complex Coronal Environment Pick, M., Stenborg, G., Démoulin, P., Zucca, P. & Lecacheux, A., 2016, ApJ, 823, 5
10	Magnetic clouds along the solar cycle: expansion and magnetic helicity Dasso, Sergio, Démoulin, Pascal & Gulisano, Adriana M., 2012, Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars (Editors: Mandrini, Cristina H. & Webb, David F.), IAU Symposium, 286, p. 139
10	Multi-scale reconnections in a complex CME van Driel-Gesztelyi, L., Goff, C. P., Démoulin, P., Culhane, J. L., Matthews, S. A., Harra, L. K., Mandrini, C. H., Klein, K. -L. & Kurokawa, H., 2008, Advances in Space Research, 42, 858
9	A study of the long term evolution in active region upflows Harra, Louise K., Ugarte-Urra, Ignacio, De Rosa, Marc, Mandrini, Cristina, van Driel-Gesztelyi, Lidia, Baker, Deborah, Culhane, J. Leonard & Démoulin, Pascal, 2017, Publications of the Astronomical Society of Japan, 69, 47
9	Evolution of Plasma Composition in an Eruptive Flux Rope Baker, D., Green, L. M., Brooks, D. H., Démoulin, P., van Driel-Gesztelyi, L., Mihailescu, T., To, A. S. H., Long, D. M., Yardley, S. L., Janvier, M. & Valori, G., 2022, ApJ, 924, 17
9	Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption Joshi, Reetika, Mandrini, Cristina H., Chandra, Ramesh, Schmieder, Brigitte, Cristiani, Germán D., Mac Cormack, Cecilia, Démoulin, Pascal & Cremades, Hebe, 2022, Solar Physics, 297, 81
9	Do Current and Magnetic Helicities Have the Same Sign? Russell, A. J. B., Demoulin, P., Hornig, G., Pontin, D. I. & Candelaresi, S., 2019, ApJ, 884, 55
9	The evolution from birth to decay of a short-lived active region Deng, Yuan Yong, Schmieder, Brigitte, Mandrini, Cristina H., Khan, Josef I., Démoulin, Pascal & Rudawy, Pawel, 1999, A&A, 349, 927
9	Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage Yardley, Stephanie L., Owen, Christopher J., Long, David M., Baker, Deborah, Brooks, David H., Polito, Vanessa, Green, Lucie M., Matthews, Sarah, Owens, Mathew, Lockwood, Mike, Stansby, David, James, Alexander W., Valori, Gherardo, Giunta, Alessandra, Janvier, Miho, Ngampoopun, Nawin, Mihailescu, Teodora, To, Andy S. H., van Driel-Gesztelyi, Lidia, Démoulin, Pascal, D'Amicis, Raffaella, French, Ryan J., Suen, Gabriel H. H., Rouillard, Alexis P., Pinto, Rui F., Réville, Victor, Watson, Christopher J., Walsh, Andrew P., De Groof, Anik, Williams, David R., Zouganelis, Ioannis, Müller, Daniel, Berghmans, David, Auchère, Frédéric, Harra, Louise, Schuehle, Udo, Barczynski, Krysztof, Buchlin, Éric, Cuadrado, Regina Aznar, Kraaikamp, Emil, Mandal, Sudip, Parenti, Susanna, Peter, Hardi, Rodriguez, Luciano, Schwanitz, Conrad, Smith, Phil, Teriaca, Luca, Verbeeck, Cis, Zhukov, Andrei N., De Pontieu, Bart, Horbury, Tim, Solanki, Sami K., del Toro Iniesta, Jose Carlos, Woch, Joachim, Gandorfer, Achim, Hirzberger, Johann, Súarez, David Orozco, Appourchaux, Thierry, Calchetti, Daniele, Sinjan, Jonas, Kahil, Fatima, Albert, Kinga, Volkmer, Reiner, Carlsson, Mats, Fludra, Andrzej, Hassler, Don, Caldwell, Martin, Fredvik, Terje, Grundy, Tim, Guest, Steve, Haberreiter, Margit, Leeks, Sarah, Pelouze, Gabriel, Plowman, Joseph, Schmutz, Werner, Sidher, Sunil, Thompson, William T., Louarn, Philippe & Federov, Andrei, 2023, ApJS, 267, 11
9	A solar flare driven by thermal conduction observed in mid-infrared López, Fernando M., Giménez de Castro, Carlos Guillermo, Mandrini, Cristina H., Simões, Paulo J. A., Cristiani, Germán D., Gary, Dale E., Francile, Carlos & Démoulin, Pascal, 2022, A&A, 657, A51
8	Filament Eruption Driving EUV Loop Contraction and Then Expansion above a Stable Filament Chandra, Ramesh, Démoulin, Pascal, Devi, Pooja, Joshi, Reetika & Schmieder, Brigitte, 2021, ApJ, 922, 227
8	Re-analysis of Lepping's Fitting Method for Magnetic Clouds: Lundquist Fit Reloaded Démoulin, Pascal, Dasso, Sergio, Janvier, Miho & Lanabere, Vanina, 2019, Solar Physics, 294, 172
8	Stationary subalfvenic and low-β MHD flows in solar coronal loops and arcades. Surlantzis, G., Demoulin, P., Heyvaerts, J. & Sauty, C., 1994, A&A, 284, 985
7	Evolution of the magnetic field distribution of active regions Dacie, S., Démoulin, P., van Driel-Gesztelyi, L., Long, D. M., Baker, D., Janvier, M., Yardley, S. L. & Pérez-Suárez, D., 2016, A&A, 596, A69
7	Radial evolution of the accuracy of ballistic solar wind backmapping Dakeyo, J. -B., Badman, S. T., Rouillard, A. P., Réville, V., Verscharen, D., Démoulin, P. & Maksimovic, M., 2024, A&A, 686, A12
7	Study of magnetic flux emergence and related activity in active region NOAA 10314 Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H., Démoulin, Pascal & Pariat, Etienne, 2013, Advances in Space Research, 51, 1834
7	Linear force-free magnetic field around quiescent solar prominences computed from observable boundary conditions Demoulin, P., Raadu, M. A. & Malherbe, J. M., 1992, A&A, 257, 278
7	On Asymmetry of Magnetic Helicity in Emerging Active Regions: High-resolution Observations Tian, Lirong, Démoulin, Pascal, Alexander, David & Zhu, Chunming, 2011, ApJ, 727, 28
6	Reorganization of the solar corona following a C4.7 flare van Driel-Gesztelyi, L., Manoharan, P. K., Pick, M. & Démoulin, P. P., 1997, Advances in Space Research, 19, 1883
6	Active-region Tilt Angles from White-light Images and Magnetograms: The Role of Magnetic Tongues Poisson, Mariano, Démoulin, Pascal, Mandrini, Cristina H. & López Fuentes, Marcelo C., 2020, ApJ, 894, 131
6	Multi-source connectivity as the driver of solar wind variability in the heliosphere Yardley, Stephanie L., Brooks, David H., D'Amicis, Raffaella, Owen, Christopher J., Long, David M., Baker, Deb, Démoulin, Pascal, Owens, Mathew J., Lockwood, Mike, Mihailescu, Teodora, Coburn, Jesse T., Dewey, Ryan M., Müller, Daniel, Suen, Gabriel H. H., Ngampoopun, Nawin, Louarn, Philippe, Livi, Stefano, Lepri, Sue, Fludra, Andrzej, Haberreiter, Margit & Schühle, Udo, 2024, Nature Astronomy, 8, 953
6	Locating the solar source of 13 April 2006 magnetic cloud Steed, K., Owen, C. J., Harra, L. K., Green, L. M., Dasso, S., Walsh, A. P., Démoulin, P. & van Driel-Gesztelyi, L., 2008, Annales Geophysicae, 26, 3159
5	Bright Points and Subflares in Ultraviolet Lines and X-Rays Rovira, M., Schmieder, B., Démoulin, P., Simnett, G. M., Hagyard, M. J., Reichmann, E. & Tandberg-Hanssen, E., 1999, ApJ, 510, 474
5	How to Form a Dip in a Magnetic Field Before the Formation of a Solar Prominence Demoulin, P. & Priest, E. R., 1989, Hvar Observatory Bulletin, 13, 261
5	Relationship between a spot and a filament observed during spacelab 2 mission Schmieder, B., Dere, K. P., Raadu, M. A., Démoulin, P. & Alissandrakis, C. E., 1990, Advances in Space Research, 10, 195
5	Eruption of the EUV Hot Channel from the Solar Limb and Associated Moving Type IV Radio Burst Vemareddy, P., Démoulin, P., Sasikumar Raja, K., Zhang, J., Gopalswamy, N. & Vasantharaju, N., 2022, ApJ, 927, 108
5	Helical Structures around Quiescent Solar Prominences Computed from Observable Magnetic Fields Demoulin, P. & Raadu, M. A., 1992, Solar Physics, 142, 291
5	Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope Baker, Deborah, Mihailescu, Teodora, Démoulin, Pascal, Green, Lucie M., van Driel-Gesztelyi, Lidia, Valori, Gherardo, Brooks, David H., Long, David M. & Janvier, Miho, 2021, Solar Physics, 296, 103
4	3-D Magnetic Configurations for Filaments and Flares: The Role of ``Magnetic Dips'' and ``Bald Patches'' Aulanier, G., Schmieder, B., van Driel-Gesztelyi, L., Kucera, T., Démoulin, P., Fang, C., Mein, N., Vial, J. -C., Mein, P., Tang, Y. H. & Deforest, C., 2000, Advances in Space Research, 26, 485
4	Recurrent filament eruptions and associated CMEs Schmieder, Brigitte, Cremades, Hebe, Mandrini, Cristina, Démoulin, Pascal & Guo, Yang, 2014, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 489
4	Filament formation Démoulin, P., 1993, Advances in Space Research, 13, 95
4	Results on 3-D solar magnetic field, observations and models Démoulin, P., 1999, Journal of Atmospheric and Solar-Terrestrial Physics, 61, 101
3	Evolution of magnetic clouds in the inner heliosphere Gulisano, Adriana Maria, Démoulin, Pascal, Dasso, Sergio, Ruiz, Maria Emilia & Marsch, Eckart, 2010, Twelfth International Solar Wind Conference (Editors: Maksimovic, M., Issautier, K., Meyer-Vernet, N., Moncuquet, M. & Pantellini, F.), American Institute of Physics Conference Series, 1216, p. 391
3	Identification of a Peculiar Radio Source in the Aftermath of Large Coronal Mass Ejection Events Vourlidas, Angelos, Pick, Monique, Hoang, Sang & Démoulin, Pascal, 2007, ApJ, 656, L105
3	Evolution of interplanetary coronal mass ejections and magnetic clouds in the heliosphere Démoulin, Pascal, 2014, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 245
3	A filament supported by different magnetic field configurations Guo, Y., Schmieder, B., Démoulin, P., Wiegelmann, T., Aulanier, G., Török, T. & Bommier, V., 2011, Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 328
2	Relationship between magnetic field evolution and flaring sites in AR 6659 on June 1991 Schmieder, B., Démoulin, P., Hagyard, M., Machado, M. E., Guo, Xiang Ai, Zhang, Hongqi, Fu, Qijun, Zhi, Kai Li, Luan, Ti, Kalman, B. & Györi, L., 1993, Advances in Space Research, 13, 123
2	Observational support of reconnection in solar flares Démoulin, P., Hénoux, J. C., Schmieder, B., Mandrini, C. H., Rovira, M. G. & Somov, B., 1994, Space Science Reviews, 68, 129
2	The control of the corona by the convective zone magnetic fields Démoulin, P., 1994, Advances in Solar Physics (Editors: Belvedere, G., Rodono, M. & Simnett, G. M.), p.121
2	Linking coronal observations of a `mini´active region with its interplanetary manifestation Dasso, S., Mandrini, C. H., Pohjolainen, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Foley, C. & Copperwheat, C., 2004, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 18
2	FIP bias in a sigmoidal active region Baker, D., Brooks, D. H., Démoulin, P., van Driel-Gesztelyi, Lidia, Green, L. M., Steed, K. & Carlyle, J., 2014, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 222
2	Magnetic reconnection driven by filament eruption in the 7 June 2011 event van Driel-Gesztelyi, L., Baker, D., Török, T., Pariat, E., Green, L. M., Williams, D. R., Carlyle, J., Valori, G., Démoulin, P., Matthews, S. A., Kliem, B. & Malherbe, J. -M., 2014, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 502
2	Active region helicity evolution and related coronal mass ejection activity Green, L. M., López Fuentes, M. C., Mandrini, C. H., van Driel-Gesztelyi, L. & Démoulin, P., 2003, Advances in Space Research, 32, 1959
1	Coronal loops, flare ribbons and aurora during slip-running Schmieder, Brigitte, Aulanier, Guillaume, Démoulin, Pascal & Pariat, Etienne, 2009, Earth, Planets and Space, 61, 565
1	Solar magnetic topologies and reconnection Démoulin, P., 1997, Geophysical Monograph Series, 99, 91
1	Solar activity due to magnetic complexity of active regions Schmieder, Brigitte, Mandrini, Cristina, Chandra, Ramesh, Démoulin, Pascal, Török, Tibor, Pariat, Etienne & Uddin, Wahab, 2011, Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 164
1	Identification of a single plasma parcel during a radial alignment of the Parker Solar Probe and Solar Orbiter Berriot, Etienne, Démoulin, Pascal, Alexandrova, Olga, Zaslavsky, Arnaud & Maksimovic, Milan, 2024, A&A, 686, A114
1	Multi-spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth Baratashvili, T., Grison, B., Schmieder, B., Démoulin, P. & Poedts, S., 2024, A&A, 689, A98
1	Searching for Evidence of Subchromospheric Magnetic Reconnection on the Sun Baker, D., van Driel-Gesztelyi, L., James, A. W., Démoulin, P., To, A. S. H., Murabito, M., Long, D. M., Brooks, D. H., McKevitt, J., Laming, J. M., Green, L. M., Yardley, S. L., Valori, G., Mihailescu, T., Matthews, S. A. & Kuniyoshi, H., 2024, ApJ, 970, 39
1	Sites of flares and filaments in solar active regions Schmieder, B., van-Driel, L., Hofmann, A., Démoulin, P., Hénoux, J. C. & Hagyard, M., 1993, Advances in Space Research, 13, 119
1	Twist and writhe of δ-island active regions López Fuentes, M. C., Mandrini, C. H. & Démoulin, P., 2011, Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 153
1	Field distribution of magnetograms from simulations of active region formation Dacie, S., van Driel-Gesztelyi, L., Démoulin, P., Linton, M. G., Leake, J. E., MacTaggart, D. & Cheung, M. C. M., 2017, A&A, 606, A34
1	Magnetic topology analysis of an M6.7 solar flare Luoni, M. L., Mandrini, C. H. & Démoulin, P., 2005, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 84
1	Magnetic clouds orientations using minimum variance analysis Gulisano, A. M., Dasso, S., Mandrini, C. H. & D'Emoulin, P., 2006, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 34
1	Homologous flares in AR 10486 on 27 October 2003 Luoni, M. L., Mandrini, C. H., Cristiani, G. & D'Emoulin, P., 2006, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 42
1	From The Photosphere to the Interplanetary Medium: The Magnetic Helicity Sign from Observations Luoni, M. L., Mandrini, C. H., Dasso, S., Démoulin, P. & Van Driel-Gesztelyi, L., 2007, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 50, 43
1	Evolution of a very complex active region during the decay phase of Cycle 23 Poisson, Mariano, Fuentes, Marcelo López, Mandrini, Cristina H., Démoulin, Pascal & Pariat, Etienne, 2012, Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars (Editors: Mandrini, Cristina H. & Webb, David F.), IAU Symposium, 286, p. 246
1	Magnetic tongues properties in solar active regions Poisson, M., López Fuentes, M., Mandrini, C. H. & Démoulin, P., 2012, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 55, 147
1	Can we determine the magnetic helicity sign of the solar active regions? Luoni, M. L., Mandrini, C. H., Démoulin, P., van Diel-Gesztelyi, L. & Kövári, Zs., 2004, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 14
1	How to Form a Dip in a Magnetic Field Before the Formation of a Solar Prominence Démoulin, P. & Priest, E. R., 1990, IAU Colloq. 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.269
0	Interaction of Largescale Magnetic Structures in Solar Flares Mandrini, C. H., Demoulin, P. & Henoux, J. C., 1992, IAU Colloq. 133: Eruptive Solar Flares (Editors: Svestka, Zdenek, Jackson, Bernard V. & Machado, Marcos E.), p.54
0	The solar corona's magnetism. Amari, T. & Démoulin, P., 1993, La Recherche, 24, 258
0	A three-dimensional model for solar prominences Démoulin, P., Priest, E. R. & Anzer, U., 1990, IAU Colloq. 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.268
0	3-D reconnection related to new emerging flux Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J. M., van Driel-Gesztelyi, L., Mandrini, C. H., Roudier, T., Nitta, N. & Harra-Murnion, L. K., 1997, Advances in Space Research, 19, 1871
0	Formation of a Filament around a Magnetic Region Schmieder, B., Démoulin, P., Ferreira, J. & Alissandrakis, C. E., 1990, IAU Colloq. 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.232
0	Flux rope axis geometry of magnetic clouds deduced from in situ data Janvier, Miho, Démoulin, Pascal & Dasso, Sergio, 2014, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 265
0	Brightening Event in Hα and Soft X-Ray on May 18, 1994 Tang, Y. H., Li, Y. N., Schmieder, B., Aulanier, G., Demoulin, P., Fang, C. & Sakurai, T., 2000, Advances in Space Research, 25, 1829
0	Energetics of the 18 May 1994 brightening event Tang, Y. H., Li, Y. N., Fang, C., Schmieder, B., Aulanier, G. & Demoulin, P., 2002, Advances in Space Research, 30, 557
0	A Three-Dimensional Model for Solar Prominences Demoulin, P., Priest, E. R. & Anzer, U., 1989, Hvar Observatory Bulletin, 13, 253
0	Helicity loading and dissipation: The helicity budget of ar 7978 from the cradle to the grave Driel-Gesztelyi, L. van, Démoulin, P., Mandrini, C. H., Plunkett, S., Thompson, B., Kővári, Zs., Aulanier, G., Young, A., López Fuentes, M. & Poedts, S., 2002, Cospar, 13, 143
0	Formation of a Filament around a Magnetic Region Schmieder, B., Demoulin, P., Ferreira, J. & Alissandrakis, C. E., 1989, Hvar Observatory Bulletin, 13, 1
0	Definition of the Spatial Propagator and Implications for Magnetic Field Properties Edmondson, Justin K. & Démoulin, Pascal, 2019, Solar Physics, 294, 76
0	Magnetohydrodinamic properties of solar origin magnetic clouds: an statistical study Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., 2004, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 28
0	Analysis of 20 magnetic clouds at 1 AU during a solar minimum Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., 2005, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 79
0	Study of an expanding magnetic cloud Nakwacki, M. S., Dasso, S., Mandrini, C. H. & Démoulin, P., 2005, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 93
0	On the origin of the 28 October 2003 X17 event and its companion event Mandrini, C. H., Demoulin, P., Schmieder, B., de Luca, E. E., Pariat, E. & Uddin, W., 2006, Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 109
0	Modeling Global Magnetic-Flux Emergence in Bipolar Solar-Active Regions Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H., Démoulin, Pascal & Grings, Francisco, 2024, Solar Physics, 299, 56
0	Impact of the Solar Activity on the Propagation of ICMEs: Simulations of Hydro, Magnetic and Median ICMEs at the Minimum and Maximum of Activity Perri, Barbara, Schmieder, Brigitte, Démoulin, Pascal, Poedts, Stefaan & Regnault, Florian, 2023, ApJ, 955, 50
0	Why proton temperature and velocity are correlated in the SW and not in ICMEs? Démoulin, Pascal, 2010, Twelfth International Solar Wind Conference (Editors: Maksimovic, M., Issautier, K., Meyer-Vernet, N., Moncuquet, M. & Pantellini, F.), American Institute of Physics Conference Series, 1216, p. 231
0	Embedded Coherent Structures from Magnetohydrodynamics to Sub-ion Scales in Turbulent Solar Wind at 0.17 au Vinogradov, Alexander, Alexandrova, Olga, Démoulin, Pascal, Artemyev, Anton, Maksimovic, Milan, Mangeney, André, Vasiliev, Alexei, Petrukovich, Anatoli A. & Bale, Stuart, 2024, ApJ, 971, 88
0	Reorganization of solar magnetic field by a flare event Manoharan, P. K., van Driel-Gesztelyi, L., Pick, M. & Démoulin, P., 1998, Bulletin of the Astronomical Society of India, 26, 319