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Results: 1-16 |
Results: 16

Authors: Heinzel, P Anzer, U
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

Authors: Heinzel, P Schmieder, B Tziotziou, K
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: Tziotziou, K Heinzel, P Mein, P Mein, N
Citation: K. Tziotziou et al., Non-LTE inversion of chromospheric CaII cloud-like features, ASTRON ASTR, 366(2), 2001, pp. 686-698

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: Anzer, U Heinzel, P
Citation: U. Anzer et P. Heinzel, Energy considerations for solar prominences with mass inflow, ASTRON ASTR, 358(3), 2000, pp. L75-L78

Authors: Mein, P Briand, C Heinzel, P Mein, N
Citation: P. Mein et al., Solar arch filaments observed with THEMIS, ASTRON ASTR, 355(3), 2000, pp. 1146-1151

Authors: Varady, M Fludra, A Heinzel, P
Citation: M. Varady et al., Decaying post-flare loops system observed by SOHO/CDS and Yohkoh/SXT, ASTRON ASTR, 355(2), 2000, pp. 769-780

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

Authors: Heinzel, P Anzer, U
Citation: P. Heinzel et U. Anzer, Magnetic dips in prominences, SOLAR PHYS, 184(1), 1999, pp. 103-111

Authors: Anzer, U Heinzel, P
Citation: U. Anzer et P. Heinzel, The energy balance in solar prominences, ASTRON ASTR, 349(3), 1999, pp. 974-984

Authors: Marsch, E Tu, CY Heinzel, P Wilhelm, K Curdt, W
Citation: E. Marsch et al., Proton and hydrogen temperatures at the base of the solar polar corona, ASTRON ASTR, 347(2), 1999, pp. 676-683

Authors: Heinzel, P Mein, N Mein, P
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

Authors: Molowny-Horas, R Heinzel, P Mein, P Mein, N
Citation: R. Molowny-horas et al., A non-LTE inversion procedure for chromospheric cloud-like features, ASTRON ASTR, 345(2), 1999, pp. 618-628

Authors: Curdt, W Heinzel, P
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
Risultati: 1-16 |