Publications of Pascal Demoulin

A list of publications authored or co-authored by 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: 294 (refereed: 283)
No. of citations: 16798
First author papers: 59 (refereed: 58)

2026

  1. Elongation of a Solar Filament and its Three-dimensional Numerical Reconstruction for Magnetic Structures [0]
    Karki, Garima, Guo, Jinhan, Schmieder, Brigitte, Chandra, Ramesh, Démoulin, Pascal, Poedts, Stefaan & Gelly, Bernard, ApJ, 999, 148

2025

  1. Kinetic collisionless model of the solar transition region and corona with spatially intermittent heating [0]
    Barbieri, Luca & Démoulin, Pascal, A&A, 704, A84
  2. Radial Evolution of a Density Structure within a Solar Wind Magnetic Sector Boundary [0]
    Berriot, Etienne, Démoulin, Pascal, Alexandrova, Olga, Zaslavsky, Arnaud, Maksimovic, Milan & Nicolaou, Georgios, ApJ, 981, 140
  3. On Alfvénic turbulence of solar wind streams observed by Solar Orbiter during March 2022 perihelion and their source regions [9]
    D'Amicis, R., Velli, M., Panasenco, O., Sorriso-Valvo, L., Perrone, D., Benella, S., De Marco, R., Bruno, R., Wang, Y.-M., Réville, V., Baker, D., Matteini, L., Yardley, S., Settino, A., Sioulas, N., Alterman, B., Tenerani, A., Raines, J., Holmes, J., Buchlin, E., Verdini, A., Demoulin, P., van Driel-Gesztelyi, L., Telloni, D., Consolini, G., Marcucci, M. F., Stangalini, M., Marino, R., Fortunato, V., Mele, G., Monti, F., Owen, C. J., Louarn, P. & Livi, S., A&A, 693, A243
  4. Generalized Two Thermal Regime Approach: Bipoly Fluid Modeling [1]
    Dakeyo, Jean-Baptiste, Démoulin, Pascal, Rouillard, Alexis, Maksimovic, Milan, Chapiron, Alice & Bale, Stuart, ApJ, 986, 157
  5. Partial Null-Point Reconnection of an Eruptive Filament [0]
    Devi, Pooja, Mandrini, Cristina H., Chandra, Ramesh, Cristiani, Germán D., Démoulin, Pascal, Mac Cormack, Cecilia & Lloveras, Diego G., Solar Physics, 300, 163
  6. Counter-Streaming Velocities in a Quiescent Filament [2]
    Karki, Garima, Schmieder, Brigitte, Démoulin, Pascal, Devi, Pooja, Chandra, Ramesh & Joshi, Reetika, Solar Physics, 300, 98
  7. Bayesian Modeling of Emerging Bipolar Active Regions from Solar Cycle 23 [0]
    Poisson, Mariano, Démoulin, Pascal, López Fuentes, Marcelo & Mandrini, Cristina H., Solar Physics, 300, 106

2024

  1. Searching for Evidence of Subchromospheric Magnetic Reconnection on the Sun [6]
    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., ApJ, 970, 39
  2. Multi-spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth [3]
    Baratashvili, T., Grison, B., Schmieder, B., Démoulin, P. & Poedts, S., A&A, 689, A98
  3. Identification of a single plasma parcel during a radial alignment of the Parker Solar Probe and Solar Orbiter [9]
    Berriot, Etienne, Démoulin, Pascal, Alexandrova, Olga, Zaslavsky, Arnaud & Maksimovic, Milan, A&A, 686, A114
  4. Radial evolution of the accuracy of ballistic solar wind backmapping [17]
    Dakeyo, J.-B., Badman, S. T., Rouillard, A. P., Réville, V., Verscharen, D., Démoulin, P. & Maksimovic, M., A&A, 686, A12
  5. Modeling Global Magnetic-Flux Emergence in Bipolar Solar-Active Regions [2]
    Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H., Démoulin, Pascal & Grings, Francisco, Solar Physics, 299, 56
  6. Embedded Coherent Structures from Magnetohydrodynamics to Sub-ion Scales in Turbulent Solar Wind at 0.17 au [8]
    Vinogradov, Alexander, Alexandrova, Olga, Démoulin, Pascal, Artemyev, Anton, Maksimovic, Milan, Mangeney, André, Vasiliev, Alexei, Petrukovich, Anatoli A. & Bale, Stuart, ApJ, 971, 88
  7. Multi-source connectivity as the driver of solar wind variability in the heliosphere [30]
    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, Nature Astronomy, 8, 953

2023

  1. Observational Evidence of S-web Source of the Slow Solar Wind [27]
    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., ApJ, 950, 65
  2. Impact of the Solar Activity on the Propagation of ICMEs: Simulations of Hydro, Magnetic and Median ICMEs at the Minimum and Maximum of Activity [0]
    Perri, Barbara, Schmieder, Brigitte, Démoulin, Pascal, Poedts, Stefaan & Regnault, Florian, ApJ, 955, 50
  3. Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage [15]
    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, ApJS, 267, 11

2022

  1. Evolution of Plasma Composition in an Eruptive Flux Rope [12]
    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., ApJ, 924, 17
  2. Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au and Their Semiempirical Isopoly Fluid Modeling [45]
    Dakeyo, Jean-Baptiste, Maksimovic, Milan, Démoulin, Pascal, Halekas, Jasper & Stevens, Michael L., ApJ, 940, 130
  3. Analysis of the Evolution of a Multi-Ribbon Flare and Failed Filament Eruption [14]
    Joshi, Reetika, Mandrini, Cristina H., Chandra, Ramesh, Schmieder, Brigitte, Cristiani, Germán D., Mac Cormack, Cecilia, Démoulin, Pascal & Cremades, Hebe, Solar Physics, 297, 81
  4. A solar flare driven by thermal conduction observed in mid-infrared [11]
    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, A&A, 657, A51
  5. Eruption of the EUV Hot Channel from the Solar Limb and Associated Moving Type IV Radio Burst [9]
    Vemareddy, P., Démoulin, P., Sasikumar Raja, K., Zhang, J., Gopalswamy, N. & Vasantharaju, N., ApJ, 927, 108

2021

  1. Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope [6]
    Baker, Deborah, Mihailescu, Teodora, Démoulin, Pascal, Green, Lucie M., van Driel-Gesztelyi, Lidia, Valori, Gherardo, Brooks, David H., Long, David M. & Janvier, Miho, Solar Physics, 296, 103
  2. Alfvénic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma in the Corona [31]
    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, ApJ, 907, 16
  3. Filament Eruption Driving EUV Loop Contraction and Then Expansion above a Stable Filament [11]
    Chandra, Ramesh, Démoulin, Pascal, Devi, Pooja, Joshi, Reetika & Schmieder, Brigitte, ApJ, 922, 227
  4. The Two-step Forbush Decrease: A Tale of Two Substructures Modulating Galactic Cosmic Rays within Coronal Mass Ejections [19]
    Janvier, Miho, Démoulin, Pascal, Guo, Jingnan, Dasso, Sergio, Regnault, Florian, Topsi-Moutesidou, Sofia, Gutierrez, Christian & Perri, Barbara, ApJ, 922, 216
  5. The Magnetic Environment of a Stealth Coronal Mass Ejection [12]
    O'Kane, Jennifer, Mac Cormack, Cecilia, Mandrini, Cristina H., Démoulin, Pascal, Green, Lucie M., Long, David M. & Valori, Gherardo, ApJ, 908, 89

2020

  1. Can Subphotospheric Magnetic Reconnection Change the Elemental Composition in the Solar Corona? [20]
    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., ApJ, 894, 35
  2. 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
  3. Active-region Tilt Angles from White-light Images and Magnetograms: The Role of Magnetic Tongues [10]
    Poisson, Mariano, Démoulin, Pascal, Mandrini, Cristina H. & López Fuentes, Marcelo C., ApJ, 894, 131

2019

  1. Transient Inverse-FIP Plasma Composition Evolution within a Solar Flare [39]
    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, ApJ, 875, 35
  2. 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
  3. Definition of the Spatial Propagator and Implications for Magnetic Field Properties [0]
    Edmondson, Justin K. & Démoulin, Pascal, Solar Physics, 294, 76
  4. Generic Magnetic Field Intensity Profiles of Interplanetary Coronal Mass Ejections at Mercury, Venus, and Earth From Superposed Epoch Analyses [79]
    Janvier, Miho, Winslow, Reka M., Good, Simon, Bonhomme, Elise, Démoulin, Pascal, Dasso, Sergio, Möstl, Christian, Lugaz, Noé, Amerstorfer, Tanja, Soubrié, Elie & Boakes, Peter D., Journal of Geophysical Research (Space Physics), 124, 812
  5. Modeling the Effect of Mass-draining on Prominence Eruptions [35]
    Jenkins, Jack M., Hopwood, Matthew, Démoulin, Pascal, Valori, Gherardo, Aulanier, Guillaume, Long, David M. & van Driel-Gesztelyi, Lidia, ApJ, 873, 49
  6. Do Current and Magnetic Helicities Have the Same Sign? [12]
    Russell, A. J. B., Demoulin, P., Hornig, G., Pontin, D. I. & Candelaresi, S., ApJ, 884, 55

2018

  1. Coronal Elemental Abundances in Solar Emerging Flux Regions [35]
    Baker, Deborah, Brooks, David H., van Driel-Gesztelyi, Lidia, James, Alexander W., Démoulin, Pascal, Long, David M., Warren, Harry P. & Williams, David R., ApJ, 856, 71
  2. Sequential Eruptions Triggered by Flux Emergence: Observations and Modeling [26]
    Dacie, S., Török, T., Démoulin, P., Linton, M. G., Downs, C., van Driel-Gesztelyi, L., Long, D. M. & Leake, J. E., ApJ, 862, 117
  3. Studying the Transfer of Magnetic Helicity in Solar Active Regions with the Connectivity-based Helicity Flux Density Method [11]
    Dalmasse, K., Pariat, É., Valori, G., Jing, J. & Démoulin, P., ApJ, 852, 141
  4. 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
  5. Physical Processes Involved in the EUV "Surge" Event of 9 May 2012 [14]
    López Fuentes, Marcelo, Mandrini, Cristina H., Poisson, Mariano, Démoulin, Pascal, Cristiani, Germán, López, Fernando M. & Luoni, Maria Luisa, Solar Physics, 293, 166
  6. Study of Three-dimensional Magnetic Structure and the Successive Eruptive Nature of Active Region 12371 [14]
    Vemareddy, P. & Demóulin, P., ApJ, 857, 90

2017

  1. Apparent and Intrinsic Evolution of Active Region Upflows [15]
    Baker, Deborah, Janvier, Miho, Démoulin, Pascal & Mandrini, Cristina H., Solar Physics, 292, 46
  2. Field distribution of magnetograms from simulations of active region formation [2]
    Dacie, S., van Driel-Gesztelyi, L., Démoulin, P., Linton, M. G., Leake, J. E., MacTaggart, D. & Cheung, M. C. M., A&A, 606, A34
  3. Expanding and Contracting Coronal Loops as Evidence of Vortex Flows Induced by Solar Eruptions [19]
    Dudík, J., Zuccarello, F. P., Aulanier, G., Schmieder, B. & Démoulin, P., ApJ, 844, 54
  4. A study of the long term evolution in active region upflows [12]
    Harra, Louise K., Ugarte-Urra, Ignacio, De Rosa, Marc, Mandrini, Cristina, van Driel-Gesztelyi, Lidia, Baker, Deborah, Culhane, J. Leonard & Démoulin, Pascal, Publications of the Astronomical Society of Japan, 69, 47
  5. Successive injection of opposite magnetic helicity in solar active region NOAA 11928 [28]
    Vemareddy, P. & Démoulin, P., A&A, 597, A104
  6. Vortex and Sink Flows in Eruptive Flares as a Model for Coronal Implosions [26]
    Zuccarello, F. P., Aulanier, G., Dudík, J., Démoulin, P., Schmieder, B. & Gilchrist, S. A., ApJ, 837, 115

2016

  1. Evolution of the magnetic field distribution of active regions [9]
    Dacie, S., Démoulin, P., van Driel-Gesztelyi, L., Long, D. M., Baker, D., Janvier, M., Yardley, S. L. & Pérez-Suárez, D., A&A, 596, A69
  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
  3. Magnetic Flux and Helicity of Magnetic Clouds [26]
    Démoulin, P., Janvier, M. & Dasso, S., Solar Physics, 291, 531
  4. Superposed epoch study of ICME sub-structures near Earth and their effects on Galactic cosmic rays [73]
    Masías-Meza, J. J., Dasso, S., Démoulin, P., Rodriguez, L. & Janvier, M., A&A, 592, A118
  5. Homologous Solar Events on 2011 January 27: Build-up and Propagation in a Complex Coronal Environment [11]
    Pick, M., Stenborg, G., Démoulin, P., Zucca, P. & Lecacheux, A., ApJ, 823, 5
  6. Properties of Magnetic Tongues over a Solar Cycle [21]
    Poisson, Mariano, Démoulin, Pascal, López Fuentes, Marcelo & Mandrini, Cristina H., Solar Physics, 291, 1625
  7. Why Are Flare Ribbons Associated with the Spines of Magnetic Null Points Generically Elongated? [37]
    Pontin, David, Galsgaard, Klaus & Démoulin, Pascal, Solar Physics, 291, 1739
  8. Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU [39]
    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., Solar Physics, 291, 2145

2015

  1. FIP Bias Evolution in a Decaying Active Region [47]
    Baker, D., Brooks, D. H., Démoulin, P., Yardley, S. L., van Driel-Gesztelyi, L., Long, D. M. & Green, L. M., ApJ, 802, 104
  2. The Origin of Net Electric Currents in Solar Active Regions [44]
    Dalmasse, K., Aulanier, G., Démoulin, P., Kliem, B., Török, T. & Pariat, E., ApJ, 810, 17
  3. From Coronal Observations to MHD Simulations, the Building Blocks for 3D Models of Solar Flares (Invited Review) [139]
    Janvier, M., Aulanier, G. & Démoulin, P., Solar Physics, 290, 3425
  4. Comparing generic models for interplanetary shocks and magnetic clouds axis configurations at 1 AU [33]
    Janvier, M., Dasso, S., Démoulin, P., Masías-Meza, J. J. & Lugaz, N., Journal of Geophysical Research (Space Physics), 120, 3328
  5. Parallel Evolution of Quasi-separatrix Layers and Active Region Upflows [33]
    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., ApJ, 809, 73
  6. Strong coronal channelling and interplanetary evolution of a solar storm up to Earth and Mars [183]
    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, Nature Communications, 6, 7135
  7. Testing magnetic helicity conservation in a solar-like active event [63]
    Pariat, E., Valori, G., Démoulin, P. & Dalmasse, K., A&A, 580, A128
  8. Evidence of Twisted Flux-Tube Emergence in Active Regions [29]
    Poisson, M., Mandrini, C. H., Démoulin, P. & López Fuentes, M., Solar Physics, 290, 727
  9. Active-Region Twist Derived from Magnetic Tongues and Linear Force-Free Extrapolations [12]
    Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H. & Démoulin, Pascal, Solar Physics, 290, 3279
  10. Statistical study of magnetic cloud erosion by magnetic reconnection [138]
    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., Journal of Geophysical Research (Space Physics), 120, 43

2014

  1. FIP bias in a sigmoidal active region [2]
    Baker, D., Brooks, D. H., Démoulin, P., van Driel-Gesztelyi, Lidia, Green, L. M., Steed, K. & Carlyle, J., Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 222
  2. Tracking Solar Active Region Outflow Plasma from Its Source to the Near-Earth Environment [46]
    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., Solar Physics, 289, 3799
  3. Photospheric Injection of Magnetic Helicity: Connectivity-Based Flux Density Method [29]
    Dalmasse, K., Pariat, E., Démoulin, P. & Aulanier, G., Solar Physics, 289, 107
  4. Evolution of interplanetary coronal mass ejections and magnetic clouds in the heliosphere [3]
    Démoulin, Pascal, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 245
  5. Distribution of Electric Currents in Sunspots from Photosphere to Corona [20]
    Gosain, Sanjay, Démoulin, Pascal & López Fuentes, Marcelo, ApJ, 793, 15
  6. Mean shape of interplanetary shocks deduced from in situ observations and its relation with interplanetary CMEs [31]
    Janvier, M., Démoulin, P. & Dasso, S., A&A, 565, A99
  7. Are There Different Populations of Flux Ropes in the Solar Wind? [49]
    Janvier, M., Démoulin, P. & Dasso, S., Solar Physics, 289, 2633
  8. In situ properties of small and large flux ropes in the solar wind [33]
    Janvier, M., Démoulin, P. & Dasso, S., Journal of Geophysical Research (Space Physics), 119, 7088
  9. Electric Currents in Flare Ribbons: Observations and Three-dimensional Standard Model [200]
    Janvier, M., Aulanier, G., Bommier, V., Schmieder, B., Démoulin, P. & Pariat, E., ApJ, 788, 60
  10. Flux rope axis geometry of magnetic clouds deduced from in situ data [0]
    Janvier, Miho, Démoulin, Pascal & Dasso, Sergio, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 265
  11. How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer? [26]
    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., Solar Physics, 289, 4151
  12. Topological Analysis of Emerging Bipole Clusters Producing Violent Solar Events [64]
    Mandrini, C. H., Schmieder, B., Démoulin, P., Guo, Y. & Cristiani, G. D., Solar Physics, 289, 2041
  13. Recurrent filament eruptions and associated CMEs [3]
    Schmieder, Brigitte, Cremades, Hebe, Mandrini, Cristina, Démoulin, Pascal & Guo, Yang, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 489
  14. The evolution of writhe in kink-unstable flux ropes and erupting filaments [19]
    Török, T., Kliem, B., Berger, M. A., Linton, M. G., Démoulin, P. & van Driel-Gesztelyi, L., Plasma Physics and Controlled Fusion, 56, 064012
  15. Understanding Coronal Mass Ejections and Associated Shocks in the Solar Corona by Merging Multiwavelength Observations [44]
    Zucca, P., Pick, M., Démoulin, P., Kerdraon, A., Lecacheux, A. & Gallagher, P. T., ApJ, 795, 68
  16. Coronal Magnetic Reconnection Driven by CME Expansion—the 2011 June 7 Event [61]
    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., ApJ, 788, 85
  17. Magnetic reconnection driven by filament eruption in the 7 June 2011 event [2]
    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., Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 502

2013

  1. The standard flare model in three dimensions. II. Upper limit on solar flare energy [194]
    Aulanier, G., Démoulin, P., Schrijver, C. J., Janvier, M., Pariat, E. & Schmieder, B., A&A, 549, A66
  2. Plasma Composition in a Sigmoidal Anemone Active Region [69]
    Baker, D., Brooks, D. H., Démoulin, P., van Driel-Gesztelyi, L., Green, L. M., Steed, K. & Carlyle, J., ApJ, 778, 69
  3. First observational application of a connectivity-based helicity flux density [27]
    Dalmasse, K., Pariat, E., Valori, G., Démoulin, P. & Green, L. M., A&A, 555, L6
  4. Does spacecraft trajectory strongly affect detection of magnetic clouds? [35]
    Démoulin, P., Dasso, S. & Janvier, M., A&A, 550, A3
  5. 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
  6. Recurrent coronal jets induced by repetitively accumulated electric currents [76]
    Guo, Y., Démoulin, P., Schmieder, B., Ding, M. D., Vargas Domínguez, S. & Liu, Y., A&A, 555, A19
  7. Global axis shape of magnetic clouds deduced from the distribution of their local axis orientation [52]
    Janvier, M., Démoulin, P. & Dasso, S., A&A, 556, A50
  8. The standard flare model in three dimensions. III. Slip-running reconnection properties [210]
    Janvier, M., Aulanier, G., Pariat, E. & Démoulin, P., A&A, 555, A77
  9. Study of magnetic flux emergence and related activity in active region NOAA 10314 [7]
    Poisson, Mariano, López Fuentes, Marcelo, Mandrini, Cristina H., Démoulin, Pascal & Pariat, Etienne, Advances in Space Research, 51, 1834
  10. Solar filament eruptions and their physical role in triggering coronal mass ejections [155]
    Schmieder, B., Démoulin, P. & Aulanier, G., Advances in Space Research, 51, 1967
  11. Accuracy of magnetic energy computations [56]
    Valori, G., Démoulin, P., Pariat, E. & Masson, S., A&A, 553, A38

2012

  1. Magnetic clouds along the solar cycle: expansion and magnetic helicity [8]
    Dasso, Sergio, Démoulin, Pascal & Gulisano, Adriana M., Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars (Editors: Mandrini, Cristina H. & Webb, David F.), IAU Symposium, 286, p. 139
  2. 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
  3. Expansion of magnetic clouds in the outer heliosphere [51]
    Gulisano, A. M., Démoulin, P., Dasso, S. & Rodriguez, L., A&A, 543, A107
  4. Evolution of Hard X-Ray Sources and Ultraviolet Solar Flare Ribbons for a Confined Eruption of a Magnetic Flux Rope [32]
    Guo, Y., Ding, M. D., Schmieder, B., Démoulin, P. & Li, H., ApJ, 746, 17
  5. The interplanetary magnetic structure that guides solar relativistic particles [41]
    Masson, S., Démoulin, P., Dasso, S. & Klein, K.-L., A&A, 538, A32
  6. Implications of Non-cylindrical Flux Ropes for Magnetic Cloud Reconstruction Techniques and the Interpretation of Double Flux Rope Events [33]
    Owens, M. J., Démoulin, P., Savani, N. P., Lavraud, B. & Ruffenach, A., Solar Physics, 278, 435
  7. Estimation of the squashing degree within a three-dimensional domain [97]
    Pariat, E. & Démoulin, P., A&A, 541, A78
  8. Magnetic tongues properties in solar active regions [1]
    Poisson, M., López Fuentes, M., Mandrini, C. H. & Démoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 55, 147
  9. Evolution of a very complex active region during the decay phase of Cycle 23 [0]
    Poisson, Mariano, Fuentes, Marcelo López, Mandrini, Cristina H., Démoulin, Pascal & Pariat, Etienne, Comparative Magnetic Minima: Characterizing Quiet Times in the Sun and Stars (Editors: Mandrini, Cristina H. & Webb, David F.), IAU Symposium, 286, p. 246
  10. Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation [163]
    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., Journal of Geophysical Research (Space Physics), 117, A09101
  11. Comparing Values of the Relative Magnetic Helicity in Finite Volumes [74]
    Valori, G., Démoulin, P. & Pariat, E., Solar Physics, 278, 347
  12. Nonlinear Force-Free Extrapolation of Emerging Flux with a Global Twist and Serpentine Fine Structures [69]
    Valori, G., Green, L. M., Démoulin, P., Vargas Domínguez, S., van Driel-Gesztelyi, L., Wallace, A., Baker, D. & Fuhrmann, M., Solar Physics, 278, 73
  13. Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind [69]
    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., Solar Physics, 281, 237

2011

  1. Homologous Flares and Magnetic Field Topology in Active Region NOAA 10501 on 20 November 2003 [85]
    Chandra, R., Schmieder, B., Mandrini, C. H., Démoulin, P., Pariat, E., Török, T. & Uddin, W., Solar Physics, 269, 83
  2. A filament supported by different magnetic field configurations [2]
    Guo, Y., Schmieder, B., Démoulin, P., Wiegelmann, T., Aulanier, G., Török, T. & Bommier, V., Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 328
  3. Initiation and Early Development of the 2008 April 26 Coronal Mass Ejection [23]
    Huang, J., Démoulin, P., Pick, M., Auchère, F., Yan, Y. H. & Bouteille, A., ApJ, 729, 107
  4. Twisted Flux Tube Emergence Evidenced in Longitudinal Magnetograms: Magnetic Tongues [106]
    Luoni, M. L., Démoulin, P., Mandrini, C. H. & van Driel-Gesztelyi, L., Solar Physics, 270, 45
  5. Twist and writhe of δ-island active regions [1]
    López Fuentes, M. C., Mandrini, C. H. & Démoulin, P., Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 153
  6. Dynamical evolution of a magnetic cloud from the Sun to 5.4 AU [56]
    Nakwacki, M. S., Dasso, S., Démoulin, P., Mandrini, C. H. & Gulisano, A. M., A&A, 535, A52
  7. Actors of the main activity in large complex centres during the 23 solar cycle maximum [14]
    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., Advances in Space Research, 47, 2081
  8. Solar activity due to magnetic complexity of active regions [1]
    Schmieder, Brigitte, Mandrini, Cristina, Chandra, Ramesh, Démoulin, Pascal, Török, Tibor, Pariat, Etienne & Uddin, Wahab, Physics of Sun and Star Spots (Editors: Prasad Choudhary, Debi & Strassmeier, Klaus G.), IAU Symposium, 273, p. 164
  9. Investigating the observational signatures of magnetic cloud substructure [23]
    Steed, K., Owen, C. J., Démoulin, P. & Dasso, S., Journal of Geophysical Research (Space Physics), 116, A01106
  10. On Asymmetry of Magnetic Helicity in Emerging Active Regions: High-resolution Observations [7]
    Tian, Lirong, Démoulin, Pascal, Alexander, David & Zhu, Chunming, ApJ, 727, 28
  11. Filament Interaction Modeled by Flux Rope Reconnection [53]
    Török, T., Chandra, R., Pariat, E., Démoulin, P., Schmieder, B., Aulanier, G., Linton, M. G. & Mandrini, C. H., ApJ, 728, 65

2010

  1. Formation of Torus-Unstable Flux Ropes and Electric Currents in Erupting Sigmoids [528]
    Aulanier, G., Török, T., Démoulin, P. & DeLuca, E. E., ApJ, 708, 314
  2. Criteria for Flux Rope Eruption: Non-equilibrium Versus Torus Instability [274]
    Démoulin, P. & Aulanier, G., ApJ, 718, 1388
  3. 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
  4. 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
  5. Global and local expansion of magnetic clouds in the inner heliosphere [121]
    Gulisano, A. M., Démoulin, P., Dasso, S., Ruiz, M. E. & Marsch, E., A&A, 509, A39
  6. Evolution of magnetic clouds in the inner heliosphere [3]
    Gulisano, Adriana Maria, Démoulin, Pascal, Dasso, Sergio, Ruiz, Maria Emilia & Marsch, Eckart, 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
  7. Coexisting Flux Rope and Dipped Arcade Sections Along One Solar Filament [164]
    Guo, Y., Schmieder, B., Démoulin, P., Wiegelmann, T., Aulanier, G., Török, T. & Bommier, V., ApJ, 714, 343

2009

  1. Magnetic Reconnection along Quasi-separatrix Layers as a Driver of Ubiquitous Active Region Outflows [122]
    Baker, D., van Driel-Gesztelyi, L., Mandrini, C. H., Démoulin, P. & Murray, M. J., ApJ, 705, 926
  2. Signatures of interchange reconnection: STEREO, ACE and Hinode observations combined [30]
    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., Annales Geophysicae, 27, 3883
  3. Linking two consecutive nonmerging magnetic clouds with their solar sources [67]
    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., Journal of Geophysical Research (Space Physics), 114, A02109
  4. Causes and consequences of magnetic cloud expansion [140]
    Démoulin, P. & Dasso, S., A&A, 498, 551
  5. Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections? [42]
    Démoulin, P., Solar Physics, 257, 169
  6. Modelling and observations of photospheric magnetic helicity [102]
    Démoulin, P. & Pariat, E., Advances in Space Research, 43, 1013
  7. Magnetic cloud models with bent and oblate cross-section boundaries [47]
    Démoulin, P. & Dasso, S., A&A, 507, 969
  8. Coronal loops, flare ribbons and aurora during slip-running [1]
    Schmieder, Brigitte, Aulanier, Guillaume, Démoulin, Pascal & Pariat, Etienne, Earth, Planets and Space, 61, 565

2008

  1. The Recovery of CME-Related Dimmings and the ICME's Enduring Magnetic Connection to the Sun [39]
    Attrill, G. D. R., van Driel-Gesztelyi, L., Démoulin, P., Zhukov, A. N., Steed, K., Harra, L. K., Mandrini, C. H. & Linker, J., Solar Physics, 252, 349
  2. Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections [90]
    Démoulin, P., Nakwacki, M. S., Dasso, S. & Mandrini, C. H., Solar Physics, 250, 347
  3. A review of the quantitative links between CMEs and magnetic clouds [70]
    Démoulin, P., Annales Geophysicae, 26, 3113
  4. Are Constant Loop Widths an Artifact of the Background and the Spatial Resolution? [33]
    López Fuentes, M. C., Démoulin, P. & Klimchuk, J. A., ApJ, 673, 586
  5. Analysis of large scale MHD quantities in expanding magnetic clouds [26]
    Nakwacki, María Soledad, Dasso, Sergio, Mandrini, Cristina Hemilse & Démoulin, Pascal, Journal of Atmospheric and Solar-Terrestrial Physics, 70, 1318
  6. Nonlinear Force-free Field Modeling of a Solar Active Region around the Time of a Major Flare and Coronal Mass Ejection [280]
    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., ApJ, 675, 1637
  7. Locating the solar source of 13 April 2006 magnetic cloud [6]
    Steed, K., Owen, C. J., Harra, L. K., Green, L. M., Dasso, S., Walsh, A. P., Démoulin, P. & van Driel-Gesztelyi, L., Annales Geophysicae, 26, 3159
  8. Why are CMEs large-scale coronal events: nature or nurture? [29]
    van Driel-Gesztelyi, L., Attrill, G. D. R., Démoulin, P., Mandrini, C. H. & Harra, L. K., Annales Geophysicae, 26, 3077
  9. Multi-scale reconnections in a complex CME [12]
    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., Advances in Space Research, 42, 858

2007

  1. Coronal ``wave'': A signature of the mechanism making CMEs large-scale in the low corona? [44]
    Attrill, G. D. R., Harra, L. K., van Driel-Gesztelyi, L., Démoulin, P. & Wülser, J.-P., Astronomische Nachrichten, 328, 760
  2. Coronal ``Wave'': Magnetic Footprint of a Coronal Mass Ejection? [220]
    Attrill, Gemma D. R., Harra, Louise K., van Driel-Gesztelyi, Lidia & Démoulin, Pascal, ApJ, 656, L101
  3. Progressive Transformation of a Flux Rope to an ICME. Comparative Analysis Using the Direct and Fitted Expansion Methods [152]
    Dasso, S., Nakwacki, M. S., Démoulin, P. & Mandrini, C. H., Solar Physics, 244, 115
  4. Recent theoretical and observational developments in magnetic helicity studies [80]
    Démoulin, P., Advances in Space Research, 39, 1674
  5. 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
  6. Where will efficient energy release occur in 3-D magnetic configurations? [39]
    Démoulin, P., Advances in Space Research, 39, 1367
  7. A Multiple Flare Scenario where the Classic Long-Duration Flare Was Not the Source of a CME [27]
    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., Solar Physics, 240, 283
  8. Estimation of the bias of the Minimum Variance technique in the determination of magnetic clouds global quantities and orientation [45]
    Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., Advances in Space Research, 40, 1881
  9. From The Photosphere to the Interplanetary Medium: The Magnetic Helicity Sign from Observations [1]
    Luoni, M. L., Mandrini, C. H., Dasso, S., Démoulin, P. & Van Driel-Gesztelyi, L., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 50, 43
  10. The magnetic field topology associated with two M flares [29]
    Luoni, M. L., Mandrini, C. H., Cristiani, G. D. & Démoulin, P., Advances in Space Research, 39, 1382
  11. Are CME-Related Dimmings Always a Simple Signature of Interplanetary Magnetic Cloud Footpoints? [87]
    Mandrini, C. H., Nakwacki, M. S., Attrill, G., van Driel-Gesztelyi, L., Démoulin, P., Dasso, S. & Elliott, H., Solar Physics, 244, 25
  12. How to improve the maps of magnetic helicity injection in active regions? [17]
    Pariat, Etienne, Démoulin, Pascal & Nindos, Alexander, Advances in Space Research, 39, 1706
  13. What is the role of magnetic null points in large flares? [18]
    Schmieder, B., Mandrini, C. H., Démoulin, P., Aulanier, G., Li, H. & Berlicki, A., Advances in Space Research, 39, 1840
  14. Identification of a Peculiar Radio Source in the Aftermath of Large Coronal Mass Ejection Events [3]
    Vourlidas, Angelos, Pick, Monique, Hoang, Sang & Démoulin, Pascal, ApJ, 656, L105

2006

  1. Slip-Running Reconnection in Quasi-Separatrix Layers [235]
    Aulanier, G., Pariat, E., Démoulin, P. & Devore, C. R., Solar Physics, 238, 347
  2. A new model-independent method to compute magnetic helicity in magnetic clouds [208]
    Dasso, S., Mandrini, C. H., Démoulin, P. & Luoni, M. L., A&A, 455, 349
  3. Basic Properties of Mutual Magnetic Helicity [57]
    Demoulin, P., Pariat, E. & Berger, M. A., Solar Physics, 233, 3
  4. Extending the concept of separatrices to QSLs for magnetic reconnection [123]
    Démoulin, P., Advances in Space Research, 37, 1269
  5. Magnetic clouds orientations using minimum variance analysis [1]
    Gulisano, A. M., Dasso, S., Mandrini, C. H. & D'Emoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 34
  6. Homologous flares in AR 10486 on 27 October 2003 [1]
    Luoni, M. L., Mandrini, C. H., Cristiani, G. & D'Emoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 42
  7. The Magnetic Structure of Coronal Loops Observed by TRACE [79]
    López Fuentes, M. C., Klimchuk, J. A. & Démoulin, P., ApJ, 639, 459
  8. On the origin of the 28 October 2003 X17 event and its companion event [0]
    Mandrini, C. H., Demoulin, P., Schmieder, B., de Luca, E. E., Pariat, E. & Uddin, W., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 49, 109
  9. Companion Event and Precursor of the X17 Flare on 28 October 2003 [68]
    Mandrini, C. H., Demoulin, P., Schmieder, B., Deluca, E. E., Pariat, E. & Uddin, W., Solar Physics, 238, 293
  10. What is the spatial distribution of magnetic helicity injected in a solar active region? [52]
    Pariat, E., Nindos, A., Démoulin, P. & Berger, M. A., A&A, 452, 623
  11. Magnetic reconfiguration before the X 17 Solar flare of October 28 2003 [19]
    Schmieder, B., Mandrini, C. H., Démoulin, P., Pariat, E., Berlicki, A. & Deluca, E., Advances in Space Research, 37, 1313

2005

  1. Equilibrium and observational properties of line-tied twisted flux tubes [115]
    Aulanier, G., Démoulin, P. & Grappin, R., A&A, 430, 1067
  2. Current sheet formation in quasi-separatrix layers and hyperbolic flux tubes [223]
    Aulanier, G., Pariat, E. & Démoulin, P., A&A, 444, 961
  3. Model-independent large-scale magnetohydrodynamic quantities in magnetic clouds [19]
    Dasso, S., Gulisano, A. M., Mandrini, C. H. & Démoulin, P., Advances in Space Research, 35, 2172
  4. Large scale MHD properties of interplanetary magnetic clouds [83]
    Dasso, S., Mandrini, C. H., Démoulin, P., Luoni, M. L. & Gulisano, A. M., Advances in Space Research, 35, 711
  5. Magnetic clouds: A statistical study of magnetic helicity [41]
    Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., Journal of Atmospheric and Solar-Terrestrial Physics, 67, 1761
  6. Analysis of 20 magnetic clouds at 1 AU during a solar minimum [0]
    Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 79
  7. Flows in the solar atmosphere due to the eruptions on the 15th July, 2002 [35]
    Harra, L. K., Démoulin, P., Mandrini, C. H., Matthews, S. A., van Driel-Gesztelyi, L., Culhane, J. L. & Fletcher, L., A&A, 438, 1099
  8. Tracing magnetic helicity from the solar corona to the interplanetary space [33]
    Luoni, M. L., Mandrini, C. H., Dasso, Sergio, van Driel-Gesztelyi, L. & Démoulin, P., Journal of Atmospheric and Solar-Terrestrial Physics, 67, 1734
  9. Magnetic topology analysis of an M6.7 solar flare [1]
    Luoni, M. L., Mandrini, C. H. & Démoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 84
  10. The smallest source region of an interplanetary magnetic cloud: A mini-sigmoid [11]
    Mandrini, C. H., Pohjolainen, S., Dasso, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Foley, C. & Copperwheat, C., Advances in Space Research, 36, 1579
  11. Interplanetary flux rope ejected from an X-ray bright point. The smallest magnetic cloud source-region ever observed [149]
    Mandrini, C. H., Pohjolainen, S., Dasso, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Copperwheat, C. & Foley, C., A&A, 434, 725
  12. Study of an expanding magnetic cloud [0]
    Nakwacki, M. S., Dasso, S., Mandrini, C. H. & Démoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 48, 93
  13. Photospheric flux density of magnetic helicity [156]
    Pariat, E., Démoulin, P. & Berger, M. A., A&A, 439, 1191
  14. Radio and X-Ray Signatures of Magnetic Reconnection behind an Ejected Flux Rope [48]
    Pick, M., Démoulin, P., Krucker, S., Malandraki, O. & Maia, D., ApJ, 625, 1019
  15. Eruption of a Kink-unstable Filament in NOAA Active Region 10696 [198]
    Williams, David R., Török, Tibor, Démoulin, Pascal, van Driel-Gesztelyi, Lidia & Kliem, Bernhard, ApJ, 628, L163

2004

  1. Linking coronal observations of a `miniẤactive region with its interplanetary manifestation [2]
    Dasso, S., Mandrini, C. H., Pohjolainen, S., Green, L. M., Démoulin, P., van Driel-Gesztelyi, L., Foley, C. & Copperwheat, C., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 18
  2. Observational Consequences of a Magnetic Flux Rope Emerging into the Corona [133]
    Gibson, S. E., Fan, Y., Mandrini, C., Fisher, G. & Demoulin, P., ApJ, 617, 600
  3. Magnetohydrodinamic properties of solar origin magnetic clouds: an statistical study [1]
    Gulisano, A. M., Dasso, S., Mandrini, C. H. & Démoulin, P., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 28
  4. Can we determine the magnetic helicity sign of the solar active regions? [1]
    Luoni, M. L., Mandrini, C. H., Démoulin, P., van Diel-Gesztelyi, L. & Kövári, Zs., Boletin de la Asociacion Argentina de Astronomia La Plata Argentina, 47, 14
  5. Magnetic Helicity Budget of Solar-Active Regions from the Photosphere to Magnetic Clouds [33]
    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, Astrophysics and Space Science, 290, 319
  6. Emerging Flux and the Heating of Coronal Loops [76]
    Schmieder, B., Rust, D. M., Georgoulis, M. K., Démoulin, P. & Bernasconi, P. N., ApJ, 601, 530

2003

  1. Amplitude and orientation of prominence magnetic fields from constant-alpha magnetohydrostatic models [49]
    Aulanier, G. & Démoulin, P., A&A, 402, 769
  2. Magnetic helicity analysis of an interplanetary twisted flux tube [60]
    Dasso, S., Mandrini, C. H., DéMoulin, P. & Farrugia, C. J., Journal of Geophysical Research (Space Physics), 108, 1362
  3. Magnetic Energy and Helicity Fluxes at the Photospheric Level [213]
    Démoulin, P. & Berger, M. A., Solar Physics, 215, 203
  4. 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
  5. How are Emerging Flux, Flares and CMEs Related to Magnetic Polarity Imbalance in Midi Data? [64]
    Green, L. M., Démoulin, P., Mandrini, C. H. & Van Driel-Gesztelyi, L., Solar Physics, 215, 307
  6. Active region helicity evolution and related coronal mass ejection activity [2]
    Green, L. M., López Fuentes, M. C., Mandrini, C. H., van Driel-Gesztelyi, L. & Démoulin, P., Advances in Space Research, 32, 1959
  7. Magnetic twist and writhe of active regions. On the origin of deformed flux tubes [97]
    López Fuentes, M. C., Démoulin, P., Mandrini, C. H., Pevtsov, A. A. & van Driel-Gesztelyi, L., A&A, 397, 305
  8. Observations of magnetic helicity [33]
    van Driel-Gesztelyi, L., Démoulin, P. & Mandrini, C. H., Advances in Space Research, 32, 1855
  9. The Long-Term Evolution of AR 7978: The Scalings of the Coronal Plasma Parameters with the Mean Photospheric Magnetic Field [47]
    van Driel-Gesztelyi, L., Démoulin, P., Mandrini, C. H., Harra, L. & Klimchuk, J. A., ApJ, 586, 579

2002

  1. Helicity loading and dissipation: The helicity budget of ar 7978 from the cradle to the grave [0]
    Driel-Gesztelyi, L. van, Démoulin, P., Mandrini, C. H., Plunkett, S., Thompson, B., Kővári, Zs., Aulanier, G., Young, A., López Fuentes, M. & Poedts, S., Cospar, 13, 143
  2. 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
  3. What is the source of the magnetic helicity shed by CMEs? The long-term helicity budget of AR 7978 [200]
    Démoulin, P., Mandrini, C. H., van Driel-Gesztelyi, L., Thompson, B. J., Plunkett, S., Kovári, Zs., Aulanier, G. & Young, A., A&A, 382, 650
  4. The Structure and Evolution of a Sigmoidal Active Region [126]
    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., ApJ, 574, 1021
  5. The Magnetic Helicity Budget of a cme-Prolific Active Region [164]
    Green, L. M., López fuentes, M. C., Mandrini, C. H., Démoulin, P., Van Driel-Gesztelyi, L. & Culhane, J. L., Solar Physics, 208, 43
  6. The role of magnetic bald patches in surges and arch filament systems [54]
    Mandrini, C. H., Démoulin, P., Schmieder, B., Deng, Y. Y. & Rudawy, P., A&A, 391, 317
  7. Relationships between CME's and prominences [22]
    Schmieder, B., van Driel-Gesztelyi, L., Aulanier, G., Démoulin, P., Thompson, B., De Forest, C., Wiik, J. E., Saint Cyr, C. & Vial, J. C., Advances in Space Research, 29, 1451
  8. Energetics of the 18 May 1994 brightening event [0]
    Tang, Y. H., Li, Y. N., Fang, C., Schmieder, B., Aulanier, G. & Demoulin, P., Advances in Space Research, 30, 557
  9. Theory of magnetic connectivity in the solar corona [400]
    Titov, Vyacheslav S., Hornig, Gunnar & Démoulin, Pascal, Journal of Geophysical Research (Space Physics), 107, 1164

2001

  1. A Relationship Between Transition Region Brightenings, Abundances, and Magnetic Topology [41]
    Fletcher, Lyndsay, López Fuentes, Marcelo C., Mandrini, Cristina H., Schmieder, Brigitte, Démoulin, Pascal, Mason, Helen E., Young, Peter R. & Nitta, Nariaki, Solar Physics, 203, 255
  2. Measurement of coronal magnetic twists during loop emergence of NOAA 8069 [14]
    Portier-Fozzani, F., Aschwanden, M., Démoulin, P., Neupert, W., EIT Team & Delaboudinière, J.-P., Solar Physics, 203, 289

2000

  1. 3-D Magnetic Configurations for Filaments and Flares: The Role of ``Magnetic Dips'' and ``Bald Patches'' [5]
    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., Advances in Space Research, 26, 485
  2. Magnetic reconnection: a common origin for flares and AR interconnecting arcs [47]
    Bagalá, L. G., Mandrini, C. H., Rovira, M. G. & Démoulin, P., A&A, 363, 779
  3. Magnetic Activity Associated With Radio Noise Storms [37]
    Bentley, R. D., Klein, K.-L., van Driel-Gesztelyi, L., Démoulin, P., Trottet, G., Tassetto, P. & Marty, G., Solar Physics, 193, 227
  4. 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
  5. The Counterkink Rotation of a Non-Hale Active Region [113]
    López Fuentes, M. C., Demoulin, P., Mandrini, C. H. & van Driel-Gesztelyi, L., ApJ, 544, 540
  6. Magnetic Field and Plasma Scaling Laws: Their Implications for Coronal Heating Models [199]
    Mandrini, C. H., Démoulin, P. & Klimchuk, J. A., ApJ, 530, 999
  7. Hα and Soft X-Ray Brightening Events Caused by Emerging Flux [22]
    Tang, Y. H., Li, Y. N., Fang, C., Aulanier, G., Schmieder, B., Demoulin, P. & Sakurai, T., ApJ, 534, 482
  8. Brightening Event in Hα and Soft X-Ray on May 18, 1994 [0]
    Tang, Y. H., Li, Y. N., Schmieder, B., Aulanier, G., Demoulin, P., Fang, C. & Sakurai, T., Advances in Space Research, 25, 1829
  9. Initiation of CMEs: the role of magnetic twist [31]
    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., Journal of Atmospheric and Solar-Terrestrial Physics, 62, 1437
  10. Emergence of a U-loop - sub-photospheric link between solar active regions [32]
    van Driel-Gesztelyi, L., Malherbe, J.-M. & Démoulin, P., A&A, 364, 845

1999

  1. 3-D magnetic configurations supporting prominences. III. Evolution of fine structures observed in a filament channel [97]
    Aulanier, G., Démoulin, P., Mein, N., van Driel-Gesztelyi, L., Mein, P. & Schmieder, B., A&A, 342, 867
  2. The evolution from birth to decay of a short-lived active region [9]
    Deng, Yuan Yong, Schmieder, Brigitte, Mandrini, Cristina H., Khan, Josef I., Démoulin, Pascal & Rudawy, Pawel, A&A, 349, 927
  3. Results on 3-D solar magnetic field, observations and models [4]
    Démoulin, P., Journal of Atmospheric and Solar-Terrestrial Physics, 61, 101
  4. Quasi-Separatrix Layers in a Reduced Magnetohydrodynamic Model of a Coronal Loop [66]
    Milano, Leonardo J., Dmitruk, Pablo, Mandrini, Cristina H., Gómez, Daniel O. & Démoulin, Pascal, ApJ, 521, 889
  5. Bright Points and Subflares in Ultraviolet Lines and X-Rays [5]
    Rovira, M., Schmieder, B., Démoulin, P., Simnett, G. M., Hagyard, M. J., Reichmann, E. & Tandberg-Hanssen, E., ApJ, 510, 474
  6. Basic topology of twisted magnetic configurations in solar flares [629]
    Titov, V. S. & Démoulin, P., A&A, 351, 707

1998

  1. Magnetohydrostatic Model of a Bald-Patch Flare [57]
    Aulanier, G., Démoulin, P., Schmieder, B., Fang, C. & Tang, Y. H., Solar Physics, 183, 369
  2. 3-D magnetic configurations supporting prominences. II. The lateral feet as a perturbation of a twisted flux-tube [115]
    Aulanier, G., Demoulin, P., van Driel-Gesztelyi, L., Mein, P. & Deforest, C., A&A, 335, 309
  3. 3-D magnetic configurations supporting prominences. I. The natural presence of lateral feet [289]
    Aulanier, G. & Demoulin, P., A&A, 329, 1125
  4. Interactions between nested sunspots. II. A confined X1 flare in a delta-type sunspot [38]
    Gaizauskas, V., Mandrini, C. H., Demoulin, P., Luoni, M. L. & Rovira, M. G., A&A, 332, 353
  5. The Effect of Curvature on Flux-Rope Models of Coronal Mass Ejections [177]
    Lin, J., Forbes, T. G., Isenberg, P. A. & Démoulin, P., ApJ, 504, 1006
  6. Reorganization of solar magnetic field by a flare event [0]
    Manoharan, P. K., van Driel-Gesztelyi, L., Pick, M. & Démoulin, P., Bulletin of the Astronomical Society of India, 26, 319

1997

  1. Quasi-separatrix layers in solar flares. II. Observed magnetic configurations. [294]
    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
  5. Evidence of Magnetic Reconnection from Hα, Soft X-Ray and Photospheric Magnetic Field Observations [65]
    Mandrini, C. H., DÉmoulin, P., BagalÁ, L. G., Van Driel-Gesztelyi, L., HÉnoux, J. C., Schmieder, B. & Rovira, M. G., Solar Physics, 174, 229
  6. 3-D reconnection related to new emerging flux [0]
    Schmeider, B., Démoulin, P., Aulanier, G., Malherbe, J. M., van Driel-Gesztelyi, L., Mandrini, C. H., Roudier, T., Nitta, N. & Harra-Murnion, L. K., Advances in Space Research, 19, 1871
  7. Magnetic reconnection driven by emergence of sheared magnetic field. [78]
    Schmieder, B., Aulanier, G., Demoulin, P., van Driel-Gesztelyi, L., Roudier, T., Nitta, N. & Cauzzi, G., A&A, 325, 1213
  8. Reorganization of the solar corona following a C4.7 flare [5]
    van Driel-Gesztelyi, L., Manoharan, P. K., Pick, M. & Démoulin, P. P., Advances in Space Research, 19, 1883

1996

  1. Quasi-Separatrix layers in solar flares. I. Method. [415]
    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
  3. 3D Magnetic Reconnection at an X-Ray Bright Point [94]
    Mandrini, C. H., Démoulin, P., Van Driel-Gesztelyi, L., Schmieder, B., Cauzzi, G. & Hofmann, A., Solar Physics, 168, 115
  4. Evidence for Large-Scale Solar Magnetic Reconnection from Radio and X-Ray Measurements [129]
    Manoharan, P. K., van Driel-Gesztelyi, L., Pick, M. & Demoulin, P., ApJ, 468, L73
  5. Dynamics of solar magnetic arches in the photosphere and the chromosphere. [25]
    Mein, P., Demoulin, P., Mein, N., Engvold, O., Molowny-Horas, R., Heinzel, P. & Gontikakis, C., A&A, 305, 343
  6. Differential Magnetic Field Shear in an Active Region [97]
    Schmieder, B., Demoulin, P., Aulanier, G. & Golub, L., ApJ, 467, 881

1995

  1. A Topological Approach to Understand a Multiple-Loop Solar Flare [42]
    Bagalá, L. G., Mandrini, C. H., Rovira, M. G., Démoulin, P. & Hénoux, J. C., Solar Physics, 161, 103
  2. Reduction, Analysis, and Properties of Electric Current Systems in Solar Active Regions [47]
    Gary, G. Allen & Demoulin, Pascal, ApJ, 445, 982
  3. Constraints on flare models set by the active region magnetic topology Magnetic topology of AR 6233. [57]
    Mandrini, C. H., Demoulin, P., Rovira, M. G., de La Beaujardiere, J.-F. & Henoux, J. C., A&A, 303, 927
  4. Three-dimensional magnetic reconnection without null points. 1. Basic theory of magnetic flipping [448]
    Priest, E. R. & Démoulin, P., Journal of Geophysical Research, 100, 23443

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. 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
  4. 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
  5. CFHT eclipse observation of the very fine-scale solar corona [32]
    Koutchmy, S., Belmahdi, M., Coulter, R. L., Demoulin, P., Gaizauskas, V., MacQueen, R. M., Monnet, G., Mouette, J., Noens, J. C. & November, L. J., A&A, 281, 249
  6. Relationship between magnetic field evolution and flaring sites in AR 6659 in June 1991 [80]
    Schmieder, B., Hagyard, M. J., Guoxiang, Ai, Hongqi, Zhang, Kalman, B., Gyori, L., Rompolt, B., Demoulin, P. & Machado, M. E., Solar Physics, 150, 199
  7. Stationary subalfvenic and low-β MHD flows in solar coronal loops and arcades. [8]
    Surlantzis, G., Demoulin, P., Heyvaerts, J. & Sauty, C., A&A, 284, 985
  8. Relationship between electric currents, photospheric motions, chromospheric activity, and magnetic field topology [44]
    van Driel-Gesztelyi, L., Hofmann, A., Demoulin, P., Schmieder, B. & Csepura, G., Solar Physics, 149, 309

1993

  1. The solar corona's magnetism. [0]
    Amari, T. & Démoulin, P., La Recherche, 24, 258
  2. 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
  3. 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
  4. Filament formation [4]
    Démoulin, P., Advances in Space Research, 13, 95
  5. Catastrophic Evolution of a Force-free Flux Rope: A Model for Eruptive Flares [159]
    Isenberg, P. A., Forbes, T. G. & Demoulin, P., ApJ, 417, 368
  6. Evidence for magnetic reconnection in large-scale magnetic structures in solar flares [62]
    Mandrini, C. H., Rovira, M. G., Demoulin, P., Henoux, J. C., Machado, M. E. & Wilkinson, L. K., A&A, 272, 609
  7. Sites of flares and filaments in solar active regions [1]
    Schmieder, B., van-Driel, L., Hofmann, A., Démoulin, P., Hénoux, J. C. & Hagyard, M., Advances in Space Research, 13, 119
  8. Relationship between magnetic field evolution and flaring sites in AR 6659 on June 1991 [2]
    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., Advances in Space Research, 13, 123
  9. Conditions for the appearance of "bald patches" at the solar surface [190]
    Titov, V. S., Priest, E. R. & Demoulin, P., A&A, 276, 564
  10. Common Evolution of Adjacent Sunspot Groups [11]
    van Driel-Gesztelyi, L., Csepura, G., Nagy, I., Gerlei, O., Schmieder, B., Rayrole, J. & Demoulin, P., Solar Physics, 145, 77

1992

  1. 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
  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. Helical Structures around Quiescent Solar Prominences Computed from Observable Magnetic Fields [5]
    Demoulin, P. & Raadu, M. A., Solar Physics, 142, 291
  5. Weighted Current Sheets Supported in Normal and Inverse Configurations: A Model for Prominence Observations [14]
    Demoulin, P. & Forbes, T. G., ApJ, 387, 394
  6. 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
  7. The properties of sources and sinks of a linear force-free field [30]
    Demoulin, P. & Priest, E. R., A&A, 258, 535
  8. Interaction of Largescale Magnetic Structures in Solar Flares [0]
    Mandrini, C. H., Demoulin, P. & Henoux, J. C., IAU Colloquium 133: Eruptive Solar Flares (Editors: Svestka, Zdenek, Jackson, Bernard V. & Machado, Marcos E.), p.54

1991

  1. The creation of the magnetic environment for prominence formation in a coronal arcade [32]
    Amari, T., Démoulin, P., Browning, P., Hood, A. & Priest, E., A&A, 241, 604
  2. Removal of singularities in the Cauchy problem for the extrapolation of solar force-free magnetic fields [23]
    Cuperman, S., Demoulin, P. & Semel, M., A&A, 245, 285
  3. 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
  4. Evidence for the interaction of large scale magnetic structures in solar flares. [126]
    Mandrini, C. H., Demoulin, P., Henoux, J. C. & Machado, M. E., A&A, 250, 541

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
  3. Formation of a Filament around a Magnetic Region [0]
    Schmieder, B., Démoulin, P., Ferreira, J. & Alissandrakis, C. E., IAU Colloquium 117: Dynamics of Quiescent Prominences (Editors: Ruzdjak, Vladimir & Tandberg-Hanssen, Einar), p.232
  4. Relationship between a spot and a filament observed during spacelab 2 mission [5]
    Schmieder, B., Dere, K. P., Raadu, M. A., Démoulin, P. & Alissandrakis, C. E., Advances in Space Research, 10, 195

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
  6. Formation of a Filament around a Magnetic Region [0]
    Schmieder, B., Demoulin, P., Ferreira, J. & Alissandrakis, C. E., Hvar Observatory Bulletin, 13, 1
  7. Dynamics of a filament at the boundary of a SPOT region with magnetic shear [14]
    Schmiedler, B., Demoulin, P., Raadu, M. A. & Dere, K. P., A&A, 213, 402

1988

  1. Instability of a prominence supported in a linear force-free field [45]
    Demoulin, P. & Priest, E. R., A&A, 206, 336
  2. Some dynamical aspects of a quiescent filament [17]
    Schmieder, B., Demoulin, P., Poland, A. & Thompson, B., A&A, 197, 281

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

1986

  1. Dynamics of solar filaments. VI - Center-to-limb study of H-alpha and C IV velocities in a quiescent filament [35]
    Simon, G., Schmieder, B., Demoulin, P. & Poland, A. I., A&A, 166, 319

Created on Wed Apr 8 04:28:15 2026.