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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