World's Best Scientists 2026 revealed!
Pascal Démoulin

Pascal Démoulin

D-Index & Metrics

Physics

D-Index
85
Citations
22694
World Ranking
2621
National Ranking
110

Pascal Démoulin publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Pascal Démoulin sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 453 publications — 48th percentile

48% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Pascal Démoulin D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Pascal Démoulin sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 85 D-Index — 31st percentile

31% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

Pascal Démoulin is affiliated with Université Paris Cité in France and has contributed extensively to research in physics and astronomy, with a particular focus on solar and space plasma dynamics.

The scientist's research spans several interrelated fields and subfields:

  • Physics and Astronomy
  • Astronomy and Astrophysics
  • Molecular Biology
  • Artificial Intelligence
  • Oceanography
  • Aerospace Engineering

Main research topics include:

  • Solar and Space Plasma Dynamics
  • Astro and Planetary Science
  • Ionosphere and Magnetosphere Dynamics
  • Stellar, Planetary, and Galactic Studies
  • Geomagnetism and Paleomagnetism Studies
  • Solar Radiation and Photovoltaics
  • Geophysics and Gravity Measurements

Frequent collaborators in Pascal Démoulin's work include Miho Janvier, B. Schmieder, G. Valori, David M. Long, and C. H. Mandrini. These coauthors have contributed significantly to various publications with Démoulin.

Scientific articles by Pascal Démoulin have appeared predominantly in journals and venues recognized in the field, such as:

  • arXiv (Cornell University)
  • Astronomy and Astrophysics
  • The Astrophysical Journal
  • Solar Physics
  • Springer Link (Chiba Institute of Technology)

Notable recent papers by Pascal Démoulin include:

  • Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au and Their Semiempirical Isopoly Fluid Modeling (2022, The Astrophysical Journal)
  • Alfvénic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma in the Corona (2021, The Astrophysical Journal)
  • Comparing the Properties of ICME-Induced Forbush Decreases at Earth and Mars (2020, Journal of Geophysical Research Space Physics)
  • Observational Evidence of S-web Source of the Slow Solar Wind (2023, The Astrophysical Journal)
  • Magnetic twist profile inside magnetic clouds derived with a superposed epoch analysis (2020, Astronomy and Astrophysics)

This body of work indicates a focus on solar wind dynamics, space plasma phenomena, and magnetic structures in space environments, contributing data and modeling efforts across solar and planetary science disciplines.

Best Publications

  • Basic topology of twisted magnetic configurations in solar flares

    V. S. Titov;P. Demoulin

  • Formation of Torus-Unstable Flux Ropes and Electric Currents in Erupting Sigmoids

    G. Aulanier;T. Török;P. Démoulin;E. E. DeLuca

  • Three-dimensional magnetic reconnection without null points: 1. Basic theory of magnetic flipping

    E. R. Priest;P. Démoulin

  • Theory of magnetic connectivity in the solar corona

    Vyacheslav S. Titov;Gunnar Hornig;Pascal Démoulin

  • 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

  • Quasi-Separatrix layers in solar flares. I. Method.

    P. Demoulin;J. C. Henoux;E. R. Priest;C. H. Mandrini

  • CRITERIA FOR FLUX ROPE ERUPTION: NON-EQUILIBRIUM VERSUS TORUS INSTABILITY

    P. Démoulin;G. Aulanier

  • 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

  • QUASI-SEPARATRIX LAYERS IN SOLAR FLARES. II. OBSERVED MAGNETIC CONFIGURATIONS

    P. Demoulin;L. G. Bagala;C. H. Mandrini;J. C. Henoux

  • 3-D magnetic configurations supporting prominences I. The natural presence of lateral feet

    G. Aulanier;P. Demoulin

  • Eruption of a Kink-Unstable Filament in Active Region NOAA 10696

    D. R. Williams;T. Toeroek;P. Demoulin;L. van Driel-Gesztelyi

  • Slip-Running Reconnection in Quasi-Separatrix Layers

    G. Aulanier;E. Pariat;P. Démoulin;C. R. Devore

  • Coronal ``Wave'': Magnetic Footprint of a Coronal Mass Ejection?

    Gemma D. R. Attrill;Louise K. Harra;Lidia van Driel-Gesztelyi;Lidia van Driel-Gesztelyi;Lidia van Driel-Gesztelyi;Pascal Démoulin

  • MAGNETIC ENERGY AND HELICITY FLUXES AT THE PHOTOSPHERIC LEVEL

    P. Démoulin;M.A. Berger

  • Magnetic Field and Plasma Scaling Laws: Their Implications for Coronal Heating Models

    Cristina Hemilse Mandrini;Pascal Démoulin;James Klimchuk

  • Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes

    G. Aulanier;E. Pariat;P. Démoulin

  • What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978

    P. Démoulin;C. H. Mandrini;C. H. Mandrini;L. van Driel-Gesztelyi;B. J. Thompson

  • Three‐dimensional magnetic reconnection without null points: 2. Application to twisted flux tubes

    P. Démoulin;E. R. Priest;D. P. Lonie

  • Electric current in flares ribbons: observations and 3D standard model

    V. Bommier;G. Aulanier;Miho Janvier;P Démoulin

  • Conditions for the appearance of "bald patches" at the solar surface

    V. S. Titov;E. R. Priest;P. Demoulin

Frequent Co-Authors

Sergio Dasso
Sergio Dasso University of Buenos Aires
Eric Priest
Eric Priest University of St Andrews
Daniel N. Baker
Daniel N. Baker University of Colorado Boulder
Benoit Lavraud
Benoit Lavraud Federal University of Toulouse Midi-Pyrénées
Angelos Vourlidas
Angelos Vourlidas Johns Hopkins University Applied Physics Laboratory
Charles J. Farrugia
Charles J. Farrugia University of New Hampshire
Bruce W. Lites
Bruce W. Lites National Center for Atmospheric Research
Janet G. Luhmann
Janet G. Luhmann University of California, Berkeley
Stephane Regnier
Stephane Regnier Northumbria University

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