First-authored, refereed papers of Pascal Demoulin, ordered by citations

A list of first-authored, refereed publications of Pascal Demoulin, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations.

Orcid ID: 0000-0001-8215-6532

416	Quasi-Separatrix layers in solar flares. I. Method. Demoulin, P., Henoux, J. C., Priest, E. R. & Mandrini, C. H., 1996, A&A, 308, 643
295	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	Criteria for Flux Rope Eruption: Non-equilibrium Versus Torus Instability Démoulin, P. & Aulanier, G., 2010, ApJ, 718, 1388
215	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
213	Magnetic Energy and Helicity Fluxes at the Photospheric Level Démoulin, P. & Berger, M. A., 2003, Solar Physics, 215, 203
201	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
143	Causes and consequences of magnetic cloud expansion Démoulin, P. & Dasso, S., 2009, A&A, 498, 551
124	Extending the concept of separatrices to QSLs for magnetic reconnection Démoulin, P., 2006, Advances in Space Research, 37, 1269
107	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
102	Modelling and observations of photospheric magnetic helicity Démoulin, P. & Pariat, E., 2009, Advances in Space Research, 43, 1013
94	Are magnetic null points important in solar flares ? Demoulin, P., Henoux, J. C. & Mandrini, C. H., 1994, A&A, 285, 1023
92	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	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
80	Recent theoretical and observational developments in magnetic helicity studies Démoulin, P., 2007, Advances in Space Research, 39, 1674
70	A review of the quantitative links between CMEs and magnetic clouds Démoulin, P., 2008, Annales Geophysicae, 26, 3113
69	Development of a Topological Model for Solar Flares Demoulin, P., Henoux, J. C. & Mandrini, C. H., 1992, Solar Physics, 139, 105
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
57	Basic Properties of Mutual Magnetic Helicity Demoulin, P., Pariat, E. & Berger, M. A., 2006, Solar Physics, 233, 3
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
47	Magnetic cloud models with bent and oblate cross-section boundaries Démoulin, P. & Dasso, S., 2009, A&A, 507, 969
45	Instability of a prominence supported in a linear force-free field Demoulin, P. & Priest, E. R., 1988, A&A, 206, 336
44	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
39	Where will efficient energy release occur in 3-D magnetic configurations? Démoulin, P., 2007, Advances in Space Research, 39, 1367
39	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	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	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
38	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	The Importance of Photospheric Intense Flux Tubes for Coronal Heating Démoulin, P. & Priest, E. R., 1997, Solar Physics, 175, 123
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	Does spacecraft trajectory strongly affect detection of magnetic clouds? Démoulin, P., Dasso, S. & Janvier, M., 2013, A&A, 550, A3
30	The properties of sources and sinks of a linear force-free field Demoulin, P. & Priest, E. R., 1992, A&A, 258, 535
27	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
26	Magnetic Flux and Helicity of Magnetic Clouds Démoulin, P., Janvier, M. & Dasso, S., 2016, Solar Physics, 291, 531
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
23	A three-dimensional model for solar prominences Demoulin, P., Priest, E. R. & Anzer, U., 1989, A&A, 221, 326
20	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
18	Structural Characteristics of Eruptive Prominences Demoulin, P. & Vial, J. C., 1992, Solar Physics, 141, 289
17	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
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
15	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	Weighted Current Sheets Supported in Normal and Inverse Configurations: A Model for Prominence Observations Demoulin, P. & Forbes, T. G., 1992, ApJ, 387, 394
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
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
12	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
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
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
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
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	Helical Structures around Quiescent Solar Prominences Computed from Observable Magnetic Fields Demoulin, P. & Raadu, M. A., 1992, Solar Physics, 142, 291
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
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
1	How to Form a Dip in a Magnetic Field Before the Formation of a Solar Prominence Démoulin, P. & Priest, E. R., 1990, IAU Colloquium 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.269
1	Solar magnetic topologies and reconnection Démoulin, P., 1997, Geophysical Monograph Series, 99, 91
0	A Three-Dimensional Model for Solar Prominences Demoulin, P., Priest, E. R. & Anzer, U., 1989, Hvar Observatory Bulletin, 13, 253
0	A three-dimensional model for solar prominences Démoulin, P., Priest, E. R. & Anzer, U., 1990, IAU Colloquium 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.268
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