Solar atmosphere and magnetic field:
 Démoulin P., Klein K.L.
              Structuring of the solar plasma by the magnetic field
         2000, in ``Transport and Energy Conversion in the Heliosphere'',
                            3eme  Ecole d'Astrophysique d'Oléron,
                           eds. J.P. Rozelot, L. Klein and J.C. Vial, Lecture Notes in Physics,
                            Springer Verlag, p. 99   PS gzip
 Démoulin, P.,
              The control of the corona by the convective zone  magnetic fields
         1994, in "Advances in Solar Physics", eds. G. Belvedere,
                       M. Rodono and G.M. Simnett, Springer-Verlag,  p.121

Long-term Evolution of Active Regions:
 Démoulin P.,
      The long-term evolution of active regions - multi-wavelength
                flux and heating study: Observations and theory
         2004, IAU Symposium 223, ``Multi-Wavelength Investigations of Solar Activity'',
               Eds.: A.V. Stepanov, E.E. Benevolenskaya, A.G. Kosovichev, p. 13 PDF

 Démoulin, P.,
              Results of 3-D solar magnetic  field observations and modeling
         1999, JASTP, 61, 101
 Démoulin, P., Hénoux, J.C., Mandrini, C.H.,  Priest, E.R.,
              Can we extrapolate a magnetic field when its topology is complex ?
         1997, Solar Physics, 174, 73
 Amari, T., Démoulin, P.,
              Le magnétisme de la couronne solaire
         1993, La Recherche, 24, 62
 Amari, T., Démoulin, P.
              Extrapolation of the photospheric magnetic field:  necessity, methods and  constraints
         1992, Proceedings of  workshop "Méthodes de détermination des champs magnétiques solaires et
                       stellaires", Observatoire de Paris, 187

Magnetic Helicity:
 Démoulin, P., Pariat, E.,
              Modelling and observations of photospheric magnetic helicity   
       2009, Advances in Space Research
,  43, 1013  PDF
 Démoulin, P.,
               Recent theoretical and observational developments in magnetic helicity studies 
       2007, Advances in Space Research, 39, 1674      PDF
 Démoulin, P., Pariat, E.,
              Computing magnetic energy and helicity fluxes from series of magnetograms  
       2007, Mem. S. A. It., 78, 136                             PDF
 Mandrini C.H., Démoulin P., van Driel-Gesztelyi L., Green L.M.,  Lòpez Fuentes M.,

       Magnetic helicity budget of solar-active regions from
                    the photosphere to magnetic clouds
         2004, Astrophysics and Space Science, 290, 319   PDF
 van Driel-Gesztelyi, L., Démoulin, P., Mandrini, C.H.,
              Observations of magnetic helicity,
         2003, Adv. Space Research, 32, 10, 1855    PDF

Confined flares & magnetic reconnection:
 Démoulin, P.,
              Where will efficient energy release occur in 3D magnetic configurations?   
         2007, Advances in Space Research, 39, 1367        PDF
 Démoulin, P.,
      Extending the concept of separatrices to QSLs for magnetic reconnection
         2006,  Advances in Space Research, 37, 7, 1269   PDF
 Démoulin, P.,
      Magnetic topologies: where will reconnection occur ?
         2005,  ESA SP-596, ``Chromospheric and coronal magnetic fields'',
                   D.E. Innes, A. Lagg & S. K. Solanki (eds.), s2_11   PDF
 Démoulin, P., Hénoux, J.C., Schmieder, B.,
              3-D structures of flaring active regions
         2001,  Eds. C. Fang, J.C. Hénoux, and M.D. Ding, International Academic
                     Publishers & World Publishing Corporation, p. 57
 Démoulin, P.,
              Solar Flares, 3-D magnetic field modelling
         1997, IAU Reports on Astronomy, Transaction of the
                  International Astronomical Union
 Hénoux, J.C., Démoulin, P., Mandrini, C.H., Rovira, M.G.,
               Observational evidence for magnetic reconnection in solar flares
         1993, ASP Conf. Ser. 46, IAU Colloq. 141,
                  The Magnetic and Velocity Fields of Solar Active Regions, 333

Coronal Mass Ejections & eruptions & Magnetic Clouds:
  Démoulin, P.,
              Interaction of ICMEs with the Solar Wind         
         2009, proceedings of SW12, in press               PDF
 Dasso, S., Mandrini, C.H., Démoulin, P., Luoni, M.L., Gulisano, A.M.,
      Large scale MHD properties of interplanetary magnetic clouds
         2005, Advances in Space Research, 35, 711   PDF
 Schmieder B,  Van Driel-Gesztelyi, L., Aulanier, G., Démoulin, P., Mein, P.,  et al.
              CMEs and Prominences Observed in Halpha and with SOHO and Yohkoh
         2000, Nagoya COSPAR, Adv. Space Research, in press
 Pick M., Démoulin P., Maia D., Plunckett S.,
              Coronal mass ejections
         1999, European meeting on Solar Physics ``Magnetic Fields and
                        Solar Processes''     ESA SP-448 p. 915
 Démoulin, P.,
              Solar Topologies and Reconnection
         1997, in AGU Monograph on Coronal Mass Ejections,
                  ed. N. Crooker, J.A. Joselyn, and J. Feynman, p. 91

Filaments & prominences:
 Démoulin, P.,
              Magnetic Fields in Filaments
         1998, IAU colloquim 167, eds. D. Webb, D. Rust and B.  Schmieder,
                  A.S.P. Conf. Ser., 150, 78        PDF
 Démoulin, P.,
              Filament formation
         1993, Advances in Space Research, 13, 9, 119
 Démoulin P., Vial, J.C.,
              Structural Characteristics of Eruptive Prominences
         1992, Solar Physics 141, 289
 Démoulin P.,
             Solar prominences
         1991, Advances in Solar System MHD (eds. E.R. Priest,  A.W. Hood),
                  Cambridge Univ. Press., 281