First-authored, refereed papers of Pascal Demoulin

A list of first-authored, refereed publications of Pascal Demoulin, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0001-8215-6532

List of publications ordered by citations
Number of papers: 58
No. of citations: 3522

2020

  1. Contribution of the ageing effect to the observed asymmetry of interplanetary magnetic clouds [15]
    Démoulin, P., Dasso, S., Lanabere, V. & Janvier, M., A&A, 639, A6

2019

  1. Re-analysis of Lepping's Fitting Method for Magnetic Clouds: Lundquist Fit Reloaded [8]
    Démoulin, Pascal, Dasso, Sergio, Janvier, Miho & Lanabere, Vanina, Solar Physics, 294, 172

2018

  1. Exploring the biases of a new method based on minimum variance for interplanetary magnetic clouds [12]
    Démoulin, P., Dasso, S. & Janvier, M., A&A, 619, A139

2016

  1. Magnetic Flux and Helicity of Magnetic Clouds [26]
    Démoulin, P., Janvier, M. & Dasso, S., Solar Physics, 291, 531
  2. Quantitative model for the generic 3D shape of ICMEs at 1 AU [17]
    Démoulin, P., Janvier, M., Masías-Meza, J. J. & Dasso, S., A&A, 595, A19

2013

  1. The 3D Geometry of Active Region Upflows Deduced from Their Limb-to-Limb Evolution [27]
    Démoulin, P., Baker, D., Mandrini, C. H. & van Driel-Gesztelyi, L., Solar Physics, 283, 341
  2. Does spacecraft trajectory strongly affect detection of magnetic clouds? [35]
    Démoulin, P., Dasso, S. & Janvier, M., A&A, 550, A3

2012

  1. Initiation and Development of the White-light and Radio Coronal Mass Ejection on 2001 April 15 [38]
    Démoulin, P., Vourlidas, A., Pick, M. & Bouteille, A., ApJ, 750, 147

2010

  1. Criteria for Flux Rope Eruption: Non-equilibrium Versus Torus Instability [276]
    Démoulin, P. & Aulanier, G., ApJ, 718, 1388
  2. Interaction of ICMEs with the Solar Wind [20]
    Démoulin, Pascal, 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
  3. Why proton temperature and velocity are correlated in the SW and not in ICMEs? [0]
    Démoulin, Pascal, 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

2009

  1. Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections? [44]
    Démoulin, P., Solar Physics, 257, 169
  2. Modelling and observations of photospheric magnetic helicity [102]
    Démoulin, P. & Pariat, E., Advances in Space Research, 43, 1013
  3. Magnetic cloud models with bent and oblate cross-section boundaries [47]
    Démoulin, P. & Dasso, S., A&A, 507, 969
  4. Causes and consequences of magnetic cloud expansion [143]
    Démoulin, P. & Dasso, S., A&A, 498, 551

2008

  1. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections [91]
    Démoulin, P., Nakwacki, M. S., Dasso, S. & Mandrini, C. H., Solar Physics, 250, 347
  2. A review of the quantitative links between CMEs and magnetic clouds [70]
    Démoulin, P., Annales Geophysicae, 26, 3113

2007

  1. Decametric N Burst: A Consequence of the Interaction of Two Coronal Mass Ejections [13]
    Démoulin, P., Klein, K.-L., Goff, C. P., van Driel-Gesztelyi, L., Culhane, J. L., Mandrini, C. H., Matthews, S. A. & Harra, L. K., Solar Physics, 240, 301
  2. Recent theoretical and observational developments in magnetic helicity studies [80]
    Démoulin, P., Advances in Space Research, 39, 1674
  3. Where will efficient energy release occur in 3-D magnetic configurations? [39]
    Démoulin, P., Advances in Space Research, 39, 1367

2006

  1. Basic Properties of Mutual Magnetic Helicity [57]
    Demoulin, P., Pariat, E. & Berger, M. A., Solar Physics, 233, 3
  2. Extending the concept of separatrices to QSLs for magnetic reconnection [124]
    Démoulin, P., Advances in Space Research, 37, 1269

2003

  1. Magnetic Energy and Helicity Fluxes at the Photospheric Level [213]
    Démoulin, P. & Berger, M. A., Solar Physics, 215, 203
  2. The Long-Term Evolution of AR 7978: Testing Coronal Heating Models [36]
    Démoulin, P., van Driel-Gesztelyi, L., Mandrini, C. H., Klimchuk, J. A. & Harra, L., ApJ, 586, 592

2002

  1. The Magnetic Helicity Injected by Shearing Motions [92]
    Démoulin, P., Mandrini, C. H., Van Driel-Gesztelyi, L., Lopez Fuentes, M. C. & Aulanier, G., Solar Physics, 207, 87
  2. What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978 [201]
    Démoulin, P., Mandrini, C. H., van Driel-Gesztelyi, L., Thompson, B. J., Plunkett, S., Kovári, Zs., Aulanier, G. & Young, A., A&A, 382, 650

2000

  1. Structuring of the Solar Plasma by the Magnetic Field [14]
    Demoulin, Pascal & Klein, Karl-Ludwig, Transport and Energy Conversion in the Heliosphere (Editors: Rozelot, J. P., Klein, L. & Vial, J.-C.), p.99

1999

  1. Results on 3-D solar magnetic field, observations and models [4]
    Démoulin, P., Journal of Atmospheric and Solar-Terrestrial Physics, 61, 101

1997

  1. Quasi-separatrix layers in solar flares. II. Observed magnetic configurations. [295]
    Demoulin, P., Bagala, L. G., Mandrini, C. H., Henoux, J. C. & Rovira, M. G., A&A, 325, 305
  2. Can we Extrapolate a Magnetic Field when its Topology is Complex? [39]
    DÉmoulin, P., HÉnoux, J. C., Mandrini, C. H. & Priest, E. R., Solar Physics, 174, 73
  3. The Importance of Photospheric Intense Flux Tubes for Coronal Heating [36]
    Démoulin, P. & Priest, E. R., Solar Physics, 175, 123
  4. Solar magnetic topologies and reconnection [1]
    Démoulin, P., Geophysical Monograph Series, 99, 91

1996

  1. Quasi-Separatrix layers in solar flares. I. Method. [416]
    Demoulin, P., Henoux, J. C., Priest, E. R. & Mandrini, C. H., A&A, 308, 643
  2. Three-dimensional magnetic reconnection without null points 2. Application to twisted flux tubes [215]
    Démoulin, P., Priest, E. R. & Lonie, D. P., Journal of Geophysical Research, 101, 7631

1994

  1. Interpretation of multiwavelength observations of November 5, 1980 solar flares by the magnetic topology of AR 2766 [69]
    Demoulin, P., Mandrini, C. H., Rovira, M. G., Henoux, J. C. & Machado, M. E., Solar Physics, 150, 221
  2. Are magnetic null points important in solar flares ? [94]
    Demoulin, P., Henoux, J. C. & Mandrini, C. H., A&A, 285, 1023
  3. Observational support of reconnection in solar flares [2]
    Démoulin, P., Hénoux, J. C., Schmieder, B., Mandrini, C. H., Rovira, M. G. & Somov, B., Space Science Reviews, 68, 129
  4. The control of the corona by the convective zone magnetic fields [2]
    Démoulin, P., Advances in Solar Physics (Editors: Belvedere, G., Rodono, M. & Simnett, G. M.), p.121

1993

  1. A Model for an Inverse Polarity Prominence Supported in a Dip of a Quadrupolar Region [38]
    Demoulin, P. & Priest, E. R., Solar Physics, 144, 283
  2. Evidence for magnetic reconnection in solar flares [107]
    Demoulin, P., van Driel-Gesztelyi, L., Schmieder, B., Hemoux, J. C., Csepura, G. & Hagyard, M. J., A&A, 271, 292
  3. Filament formation [4]
    Démoulin, P., Advances in Space Research, 13, 95

1992

  1. Helical Structures around Quiescent Solar Prominences Computed from Observable Magnetic Fields [5]
    Demoulin, P. & Raadu, M. A., Solar Physics, 142, 291
  2. Structural Characteristics of Eruptive Prominences [18]
    Demoulin, P. & Vial, J. C., Solar Physics, 141, 289
  3. Development of a Topological Model for Solar Flares [69]
    Demoulin, P., Henoux, J. C. & Mandrini, C. H., Solar Physics, 139, 105
  4. Weighted Current Sheets Supported in Normal and Inverse Configurations: A Model for Prominence Observations [14]
    Demoulin, P. & Forbes, T. G., ApJ, 387, 394
  5. 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 [38]
    Demoulin, P., Cuperman, S. & Semel, M., A&A, 263, 351
  6. The properties of sources and sinks of a linear force-free field [30]
    Demoulin, P. & Priest, E. R., A&A, 258, 535
  7. Linear force-free magnetic field around quiescent solar prominences computed from observable boundary conditions [7]
    Demoulin, P., Raadu, M. A. & Malherbe, J. M., A&A, 257, 278

1991

  1. Instability of a prominence supported in a linear force-free field. II - Effect of twist or flux conservation [12]
    Demoulin, P., Ferreira, J. & Priest, E. R., A&A, 245, 289

1990

  1. How to Form a Dip in a Magnetic Field Before the Formation of a Solar Prominence [1]
    Démoulin, P. & Priest, E. R., IAU Colloquium 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.269
  2. A three-dimensional model for solar prominences [0]
    Démoulin, P., Priest, E. R. & Anzer, U., IAU Colloquium 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.268

1989

  1. How to Form a Dip in a Magnetic Field Before the Formation of a Solar Prominence [5]
    Demoulin, P. & Priest, E. R., Hvar Observatory Bulletin, 13, 261
  2. A Three-Dimensional Model for Solar Prominences [0]
    Demoulin, P., Priest, E. R. & Anzer, U., Hvar Observatory Bulletin, 13, 253
  3. A three-dimensional model for solar prominences [23]
    Demoulin, P., Priest, E. R. & Anzer, U., A&A, 221, 326
  4. A twisted flux model for solar prominences. II - Formation of a dip in a magnetic structure before the formation of a solar prominence [51]
    Demoulin, P. & Priest, E. R., A&A, 214, 360
  5. The magnetic field around quiescent solar prominences computed from observational boundary conditions [16]
    Demoulin, P., Malherbe, J. M. & Priest, E. R., A&A, 211, 428

1988

  1. Instability of a prominence supported in a linear force-free field [45]
    Demoulin, P. & Priest, E. R., A&A, 206, 336

1987

  1. Fine structures in solar filaments. I - Observations and thermal stability [26]
    Demoulin, P., Malherbe, J. M., Schmieder, B. & Raadu, M. A., A&A, 183, 142

Created on Mon Jun 8 04:27:20 2026.