Suchergebnisse

Wiegelmann, T.; Inhester, B.: Magnetic Stereoscopy. Solar Physics 236, S. 25 - 40 (2006)

Wiegelmann, T.; Inhester, B.; Kliem, B.; Valori, G.; Neukirch, T.: Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Démoulin equilibrium. Astronomy and Astrophysics 453, S. 737 - 741 (2006)

Wiegelmann, T.; Inhester, B.; Sakurai, T.: Preprocessing of vector magnetograph data for a nonlinear force-free magnetic field reconstruction. Solar Physics 233, S. 215 - 232 (2006)

Wiegelmann, T.; Neukirch, T.: An optimization principle for the computation of MHD equilibria in the solar corona. Astronomy and Astrophysics 457, S. 1053 - 1058 (2006)

Wiegelmann, T.; Inhester, B.; Lagg, A.; Solanki, S. K.: How to use magnetic field information for coronal loop identification. Solar Physics 228, S. 67 - 78 (2005)

Wiegelmann, T.; Lagg, A.; Solanki, S. K.; Inhester, B.; Woch, J.: Comparing magnetic field extrapolations with measurements of magnetic loops. Astronomy and Astrophysics 433, S. 701 - 705 (2005)

Wiegelmann, T.; Xia, L. D.; Marsch, E.: Links between magnetic fields and plasma flows in a coronal hole. Astronomy and Astrophysics 432, S. L1 - L4 (2005)

Marsch, E.; Wiegelmann, T.; Xia, L. D.: Coronal plasma flows and magnetic fields in solar active regions Combined observations from SOHO and NSO/Kitt Peak. Astronomy and Astrophysics 428, S. 629 - 645 (2004)

Wiegelmann, T.: Optimization code with weighting function for the reconstruction of coronal magnetic fields. Solar Physics 219, S. 87 - 108 (2004)

Wiegelmann, T.; Solanki, S. K.: Similarities and differences between coronal holes and the quiet sun: are loop statistics the key? Solar Physics 225, S. 227 - 247 (2004)

Carcedo, L.; Brown, D. S.; Hood, A. W.; Neukirch, T.; Wiegelmann, T.: A quantitative method to optimise magnetic field line fitting of observed coronal loops. Solar Physics 218, S. 29 - 40 (2003)

Wiegelmann, T.; Inhester, B.: Magnetic modelling and tomography: First steps towards a consistent reconstruction of the solar corona. Solar Physics 214, S. 287 - 312 (2003)

Wiegelmann, T.; Neukirch, T.: Computing nonlinear force free coronal magnetic fields. Nonlinear Processes in Geophysics 10, S. 313 - 322 (2003)

Wiegelmann, T.; Büchner, J.: Evolution of magnetic helicity under kinetic magnetic reconnection 2. B ≠ 0 reconnection. Nonlinear Processes in Geophysics 9 (2), S. 139 - 147 (2002)

Wiegelmann, T.; Neukirch, T.: Including stereoscopic information in the reconstruction of coronal magnetic fields. Solar Physics 208, S. 233 - 251 (2002)

Wiegelmann, T.; Büchner, J.: Evolution of magnetic helicity in the course of kinetic magnetic reconnection 1. B=0 reconnection. Nonlinear Processes in Geophysics 8 (3), S. 127 - 140 (2001)

Wiegelmann, T.; Büchner, J.: Kinetic simultations of the coupling between current instabilities and reconnection in thin current sheets. Nonlinear Processes in Geophysics 7, S. 141 - 150 (2000)

Wiegelmann, T.; Schindler, K.; Neukirch, T.: Helmet Streamers with Triple Structures: Simulations of resistive dynamics. Solar Physics 191 (2), S. 391 - 407 (2000)

Wiegelmann, T.: Solar magnetic fields: Triple arcade structures. Physica Scripta T74, S. 77 - 81 (1998)

Wiegelmann, T.; Neukirch, T.; Büchner, J.: Particle code simulation - Tests and limits of Vlasov code simulations and its application to null-helicity and co-helicity reconnection. In: Space Plasma Simulation, S. 58 - 61 (Hg. Büchner, J.; Dum, C.; Scholer, M.). Copernicus Gesellschaft 2001 (2001)