We present the first comparison of profiles of H et He resonance lines
observed by SUMER with theoretical profiles computed with our non-LTE radiative
transfer code. We use the H I Lyman-beta, H I Lyman-epsilon, and He I 584 A
lines. Our code allows us to obtain the plasma parameters in prominences in
conjunction with a multi-line, multi-element set of observations. The plasma
temperature in the prominence core is ~ 8600 K and the pressure is 0.03
dyn/cm^2. The Ly-beta line is formed in a higher temperature region (more than
11000 K).Comment: 2 pages, 2 color figures. Proceedings of SF2A, Semaine de
l'Astrophysique Francaise, Journees de la SF2A 2006, Pari
