Citation: P. Heinzel et U. Anzer, Prominence fine structures in a magnetic equilibrium: Two-dimensional models with multilevel radiative transfer, ASTRON ASTR, 375(3), 2001, pp. 1082-1090
Citation: P. Heinzel et al., Why are solar filaments more extended in extreme-ultraviolet lines than inH alpha?, ASTROPHYS J, 561(2), 2001, pp. L223-L227
Authors:
Mein, N
Schmieder, B
DeLuca, EE
Heinzel, P
Mein, P
Malherbe, JM
Staiger, J
Citation: N. Mein et al., A study of hydrogen density in emerging flux loops from a coordinated Transition Region and Coronal Explorer and Canary Islands observation campaign, ASTROPHYS J, 556(1), 2001, pp. 438-451
Authors:
Heinzel, P
Schmieder, B
Vial, JC
Kotrc, P
Citation: P. Heinzel et al., SOHO/SUMER observations and analysis of the hydrogen Lyman spectrum in solar prominences, ASTRON ASTR, 370(1), 2001, pp. 281-297
Authors:
Plunkett, SP
Vourlidas, A
Simberova, S
Karlicky, M
Kotrc, P
Heinzel, P
Kupryakov, YA
Guo, WP
Wu, ST
Citation: Sp. Plunkett et al., Simultaneous SOHO and ground-based observations of a large eruptive prominence and coronal mass ejection, SOLAR PHYS, 194(2), 2000, pp. 371-391
Authors:
Schmieder, B
Heinzel, P
Vial, JC
Rudawy, P
Citation: B. Schmieder et al., SOHO/SUMER observations and analysis of hydrogen Lyman lines in a quiescent prominence, SOLAR PHYS, 189(1), 1999, pp. 109-127
Citation: P. Heinzel et al., Cloud model with variable source function for solar H alpha structures II.Dynamical models, ASTRON ASTR, 346(1), 1999, pp. 322-328
Citation: W. Curdt et P. Heinzel, Dynamic behavior of the upper solar atmosphere: SUMER/SOHO observations ofhydrogen Lyman lines, ASTROPHYS J, 503(1), 1998, pp. L95-L100