Plasmas flows

Aims: Understand the dynamics and evolution of the solar atmosphere

Harra, L.K., Démoulin, P., Mandrini, C.H., Matthews, S.A.,
                 van Driel-Gesztelyi, L., Culhane, J.L., Fletcher, L.,
                 Flows in the solar atmosphere due to the eruptions on the 15th July, 2002
         2005, A&A,  438, 1099       PDF
 Mein, P., Démoulin, P., Mein, N., Engvold, O.,  Molowny-Horas, R., Heinzel, P., Gontikakis, C.,
                 Dynamics of solar magnetic arches in photosphere and chromosphere,
         1996, A&A 305, 343
 Surlantzis, G., Démoulin, P., Heyvaerts, J., Sauty, C.,
                 Stationnary subalfvenic and low beta MHD flows in solar coronal loops and arcades.,
         1994, A&A 284, 985, (Erratum: 1996, A&A310, 351)
 Schmieder, B., Raadu, M.A., Démoulin, P., Dere, K.P.,
                Dynamics of a filament at the boundary of a spot region with magnetic shear.,
         1989, A&A 213, 402
 Schmieder, B., Poland, A., Thompson, B., Démoulin. P.,
                 Some dynamical aspects of a quiescent filament.,
         1988, A&A 197, 281
  Simon, G., Schmieder, B., Démoulin, P., Poland, A.I.,
                 Center-to-limb study of Halpha and CIV velocities  in a quiescent filament.,
         1986, A&A 166, 319