Marsch, E.; Tian, H.; Sun, J.; Curdt, W.; Wiegelmann, T.: Plasma flows guided by strong magnetic fields in the solar corona. Astrophysical Journal 685, pp. 1262 - 1269 (2008)
Metcalf, T.; Derosa, M.; Schrijver, C.; Barnes, G.; van Ballegooijen, A.; Wiegelmann, T.; Wheatland, M.; Valori, G.; McTiernan, J.: Nonlinear Force-Free Modeling of Coronal Magnetic Fields. II. Modeling a Filament Arcade and Simulated Chromospheric and Photospheric Vector Fields. Solar Physics 247, pp. 269 - 299 (2008)
Ruan, P.; Wiegelmann, T.; Inhester, B.; Neukirch, T.; Solanki, S. K.; Feng, L.: A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum. Astronomy and Astrophysics 481, pp. 827 - 834 (2008)
Schrijver, C. J.; Derosa, M. L.; Barnes, G.; Lites, B.; Tarbell, T.; McTiernan, J.; Valori, G.; Wiegelmann, T.; Wheatland, M. S.; Amari, T.et al.; Demoulin, P.; Fuhrmann, M.; Kusano, K.; Regnier, S.; Thalmann, J. K.: Nonlinear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection. Astrophysical Journal 675, pp. 1637 - 1644 (2008)
Thalmann, J. K.; Wiegelmann, T.: Evolution of the flaring active region NOAA 10540 as a sequence of nonlinear force-free field extrapolations. Astronomy and Astrophysics 484, pp. 495 - 502 (2008)
Thalmann, J. K.; Wiegelmann, T.; Raouafi, N.-E.: First nonlinear force-free field extrapolations of SOLIS/VSM data. Astronomy and Astrophysics 488, pp. L71 - L74 (2008)
Wang, H.; Jing, J.; Tan, C.; Wiegelmann, T.; Kubo, M. K.: Study of Magnetic Channel Structure in Active Region 10930. Astrophysical Journal 687, pp. 658 - 667 (2008)
Wiegelmann, T.; Thalmann, J. K.; Schrijver, C. J.; DeRosa, M. L.; Metcalf, T. R.: Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations? Solar Physics 247, pp. 249 - 267 (2008)
Wiegelmann, T.; Neukirch, T.; Ruan, P.; Inhester, B.: Optimization approach for the computation of magnetohydrostatic coronal equilibria in spherical geometry. Astronomy and Astrophysics 475, pp. 701 - 706 (2007)
Inhester, B.; Wiegelmann, T.: Nonlinear force-free magnetic field extrapolations: comparisonof the Grad-Rubin and Wheatland-Sturrock-Roumeliotis algorithm. Solar Physics 235, pp. 201 - 221 (2006)
Schrijver, C. J.; DeRosaand, M. L.; Metcalf, T. R.; Liu, Y.; McTiernan, J.; Regnier, S.; Valori, G.; Wheatland, M. S.; Wiegelmann, T.: Nonlinear force-free modeling of coronal magnetic fields Part I: A quantitative comparison of methods. Solar Physics 235, pp. 161 - 190 (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, pp. 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, pp. 215 - 232 (2006)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.