Publikationen von Thomas Wiegelmann
Alle Typen
Zeitschriftenartikel (143)
121.
Zeitschriftenartikel
240, S. 227 - 239 (2007)
Computing Nonlinear Force-Free Coronal Magnetic Fields in Spherical Geometry. Solar Physics 122.
Zeitschriftenartikel
475, S. 701 - 706 (2007)
Optimization approach for the computation of magnetohydrostatic coronal equilibria in spherical geometry. Astronomy and Astrophysics 123.
Zeitschriftenartikel
235, S. 201 - 221 (2006)
Nonlinear force-free magnetic field extrapolations: comparisonof the Grad-Rubin and Wheatland-Sturrock-Roumeliotis algorithm. Solar Physics 124.
Zeitschriftenartikel
235, S. 161 - 190 (2006)
Nonlinear force-free modeling of coronal magnetic fields Part I: A quantitative comparison of methods. Solar Physics 125.
Zeitschriftenartikel
236, S. 25 - 40 (2006)
Magnetic Stereoscopy. Solar Physics 126.
Zeitschriftenartikel
453, S. 737 - 741 (2006)
Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Démoulin equilibrium. Astronomy and Astrophysics 127.
Zeitschriftenartikel
233, S. 215 - 232 (2006)
Preprocessing of vector magnetograph data for a nonlinear force-free magnetic field reconstruction. Solar Physics 128.
Zeitschriftenartikel
457, S. 1053 - 1058 (2006)
An optimization principle for the computation of MHD equilibria in the solar corona. Astronomy and Astrophysics 129.
Zeitschriftenartikel
228, S. 67 - 78 (2005)
How to use magnetic field information for coronal loop identification. Solar Physics 130.
Zeitschriftenartikel
433, S. 701 - 705 (2005)
Comparing magnetic field extrapolations with measurements of magnetic loops. Astronomy and Astrophysics 131.
Zeitschriftenartikel
432, S. L1 - L4 (2005)
Links between magnetic fields and plasma flows in a coronal hole. Astronomy and Astrophysics 132.
Zeitschriftenartikel
428, S. 629 - 645 (2004)
Coronal plasma flows and magnetic fields in solar active regions Combined observations from SOHO and NSO/Kitt Peak. Astronomy and Astrophysics 133.
Zeitschriftenartikel
219, S. 87 - 108 (2004)
Optimization code with weighting function for the reconstruction of coronal magnetic fields. Solar Physics 134.
Zeitschriftenartikel
225, S. 227 - 247 (2004)
Similarities and differences between coronal holes and the quiet sun: are loop statistics the key? Solar Physics 135.
Zeitschriftenartikel
218, S. 29 - 40 (2003)
A quantitative method to optimise magnetic field line fitting of observed coronal loops. Solar Physics 136.
Zeitschriftenartikel
214, S. 287 - 312 (2003)
Magnetic modelling and tomography: First steps towards a consistent reconstruction of the solar corona. Solar Physics 137.
Zeitschriftenartikel
10, S. 313 - 322 (2003)
Computing nonlinear force free coronal magnetic fields. Nonlinear Processes in Geophysics 138.
Zeitschriftenartikel
9 (2), S. 139 - 147 (2002)
Evolution of magnetic helicity under kinetic magnetic reconnection 2. B ≠ 0 reconnection. Nonlinear Processes in Geophysics 139.
Zeitschriftenartikel
208, S. 233 - 251 (2002)
Including stereoscopic information in the reconstruction of coronal magnetic fields. Solar Physics 140.
Zeitschriftenartikel
8 (3), S. 127 - 140 (2001)
Evolution of magnetic helicity in the course of kinetic magnetic reconnection 1. B=0 reconnection. Nonlinear Processes in Geophysics