Jing, J.; Yuan, Y.; Wiegelmann, T.; Xu, Y.; Liu, R.; Wang, H.: Nonlinear Force-free Modeling of Magnetic Fields in a Solar Filament. Astrophysical Journal 719, pp. L56 - L59 (2010)
Lim, E.-K.; Chae, J.; Jing, J.; Wang, H.; Wiegelmann, T.: The Formation of a Magnetic Channel by the Emergence of Current-carrying Magnetic Fields. Astrophysical Journal 719, pp. 403 - 414 (2010)
Nickeler, D. H.; Wiegelmann, T.: Thin current sheets caused by plasma flow gradients in space and astrophysical plasma. Annales Geophysicae 28, pp. 1523 - 1532 (2010)
Wiegelmann, T.; Inhester, B.: How to deal with measurement errors and lacking data in nonlinear force-free coronal magnetic field modelling? Astronomy and Astrophysics 516, A107 (2010)
Wiegelmann, T.; Solanki, S. K.; Borrero, J. M.; Martínez Pillet, V.; del Toro Iniesta, J. C.; Domingo, V.; Bonet, J. A.; Barthol, P.; Gandorfer, A.; Knölker, M.et al.; Schmidt, W.; Title, A. M.: Magnetic Loops in the Quiet Sun. Astrophysical Journal 723, pp. L185 - L189 (2010)
DeRosa, M. L.; Schrijver, C. J.; Barnes, G.; Leka, K. D.; Lites, B. W.; Aschwanden, M. J.; Amari, T.; Canou, A.; McTiernan, J. M.; Régnier, S.et al.; Thalmann, J. K.; Valori, G.; Wheatland, M. S.; Wiegelmann, T.; Cheung, M. C. M.; Conlon, P. A.; Fuhrmann, M.; Inhester, B.; Tadesse, T.: A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953. Astrophysical Journal 696, pp. 1780 - 1791 (2009)
Guo, Y.; Ding, M. D.; Jin, M.; Wiegelmann, T.: Formation Heights of Extreme Ultraviolet Lines in an Active Region Derived by Correlation of Doppler Velocity and Magnetic Field. Astrophysical Journal 696, pp. 1526 - 1532 (2009)
Jing, J.; Chen, P. F.; Wiegelmann, T.; Xu, Y.; Park, S.-H.; Wang, H.: Temporal Evolution of Free Magnetic Energy Associated with Four X-Class Flares. Astrophysical Journal 696, pp. 84 - 90 (2009)
Madjarska, M. S.; Wiegelmann, T.: Coronal hole boundary evolution at small scales. I. EIT 195 Å and TRACE 171 Å view. Astronomy and Astrophysics 503, pp. 991 - 997 (2009)
Srivastava, N.; Mathew, S. K.; Louis, R. E.; Wiegelmann, T.: Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23. Journal Geophysical Research 114, A03107 (2009)
Tadesse, T.; Wiegelmann, T.; Inhester, B.: Nonlinear force-free coronal magnetic field modelling and preprocessing of vector magnetograms in spherical geometry. Astronomy and Astrophysics 508, pp. 421 - 432 (2009)
Wiegelmann, T.; Inhester, B.; Feng, L.: Solar stereoscopy where are we and what developments do we require to progress? Annales Geophysicae 27, pp. 2925 - 2936 (2009)
Aschwanden, M. J.; Burlaga, L. F.; Kaiser, M. L.; Ng, C. K.; Reames, D. V.; Reiner, M. J.; Gombosi, T. I.; Lugaz, N.; Manchester, W.; Roussev, I. I.et al.; Zurbuchen, T. H.; Farrugia, C. J.; Galvin, A. B.; Lee, M. A.; Linker, J. A.; Mikić, Z.; Riley, P.; Alexander, D.; Sandman, A. W.; Cook, J. W.; Howard, R. A.; Odstrčil, D.; Pizzo, V. J.; Kóta, J.; Liewer, P. C.; Luhmann, J. G.; Inhester, B.; Schwenn, R. W.; Solanki, S. K.; Vasyliūnas, V. M.; Wiegelmann, T.; Blush, L.; Bochsler, P.; Cairns, I. H.; Robinson, P. A.; Bothmer, V.; Kecskemety, K.; Llebaria, A.; Maksimovic, M.; Scholer, M.; Wimmer-Schweingruber, R. F.: Theoretical Modeling for the Stereo Mission. Space Science Reviews 136, pp. 565 - 604 (2008)
Guo, Y.; Ding, M. D.; Wiegelmann, T.; Li, H.: 3D Magnetic Field Configuration of the 2006 December 13 Flare Extrapolated with the Optimization Method. Astrophysical Journal 679, pp. 1629 - 1635 (2008)
Jing, J.; Wiegelmann, T.; Suematsu, Y.; Kubo, M.; Wang, H.: Changes of Magnetic Structure in Three Dimensions Associated with the X3.4 Flare of 2006 December 13. Astrophysical Journal 676, pp. L81 - L84 (2008)
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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...