Filaments
 Prominences

 Aims:    - Understand how plasma hundred times denser and cooler than the coronal plasma can exist in the corona
                    - Get important informations on the coronal magnetic field (e.g. what is its magnetic topology ?)
 

Aulanier, G., Démoulin, P.,
                Amplitude and orientation of prominence magnetic fields
                    from constant-alpha magnetohydrostatic models,
         2003, A&A, 402, 769     PDF
Aulanier G., Démoulin P., Mein N., van Driel-Gesztelyi L.,  Mein P., Schmieder B.,
                3-D magnetic configuration supporting a prominence
                         III. Evolution of fine structures observed in a filament  channel,
         1999, A&A 342, 867   PS gzip
Aulanier G., Démoulin P., van Driel-Gesztelyi L., Mein P.,  DeForest C.,
                3-D magnetic configuration supporting a prominence
                         II. The lateral feet as a perturbation  of a twisted flux-tube,
         1998, A&A 335, 309   PS gzip
Aulanier G., Démoulin P.,
                3-D magnetic configuration supporting a prominence
                          I. The natural presence of lateral feet,
         1998, A&A 329, 1125  PS gzip
Démoulin, P., Priest, E.R.,
               A Model for an Inverse-polarity prominence supported
                          in a dip of a quadrupolar region.,
         1993, Solar Physics 144, 283
Démoulin, P., Raadu, M.A.,
              Helical structures around quiescent solar prominences
                          computed from observable magnetic field.,
         1992, Solar Physics 142, 291
Démoulin, P., Forbes, T.G.,
              Weighted current sheets supported in Normal and Inverse
                          configurations: a model for prominence observations.,
         1992, ApJ 387, 394
 Démoulin, P.,  Raadu, M.A., Malherbe, J.M.,
              Linear force-free magnetic field around quiescent solar
                          prominences computed from observable boundary conditions.,
         1992, A&A 257, 278
 Amari, T., Démoulin, P., Browning, P., Hood, A.W., Priest, E.R.,
              The creation of the magnetic environment for
                          prominence formation in a coronal arcade.,
         1991, A&A 241, 604
 Démoulin, P.,  Malherbe, J.M.,  Priest, E.R.,
              The magnetic field around quiescent solar prominences
                          computed from  observationnal boundary conditions.,
         1989, A&A 211, 428
 Démoulin, P.,  Priest, E.R.,
               A twisted flux model for solar prominences.,
         1989, A&A 214, 360
 Démoulin, P.,  Priest, E.R., Anzer, U.,
               A three dimensionnal model for solar prominences.,
        1989, A&A 221, 326
 Démoulin, P., Raadu, M.A., Malherbe, J.M., Schmieder, B.,
               Fine structures in solar filaments.,
        1987, A&A 183, 142