Wiegelmann, T.; Xia, L. D.; Marsch, E.: Links between magnetic fields and plasma flows in a coronal hole. Astronomy and Astrophysics 432, pp. 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, pp. 629 - 645 (2004)
Wiegelmann, T.; Solanki, S. K.: Similarities and differences between coronal holes and the quiet sun: are loop statistics the key? Solar Physics 225, pp. 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, pp. 29 - 40 (2003)
Wiegelmann, T.; Inhester, B.: Magnetic modelling and tomography: First steps towards a consistent reconstruction of the solar corona. Solar Physics 214, pp. 287 - 312 (2003)
Wiegelmann, T.; Büchner, J.: Evolution of magnetic helicity under kinetic magnetic reconnection 2. B ≠ 0 reconnection. Nonlinear Processes in Geophysics 9 (2), pp. 139 - 147 (2002)
Wiegelmann, T.; Neukirch, T.: Including stereoscopic information in the reconstruction of coronal magnetic fields. Solar Physics 208, pp. 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), pp. 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, pp. 141 - 150 (2000)
Wiegelmann, T.; Schindler, K.; Neukirch, T.: Helmet Streamers with Triple Structures: Simulations of resistive dynamics. Solar Physics 191 (2), pp. 391 - 407 (2000)
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, pp. 58 - 61 (Eds. Büchner, J.; Dum, C.; Scholer, M.). Copernicus Gesellschaft 2001 (2001)
Koumtzis, A.; Wiegelmann, T.; Madjarska, M. S.: Computing the global coronal magnetic field during activity maximum and minimum with a newly developed nonlinear force-free Yin-Yang code. In: EGU General Assembly Conference Abstracts, pp. EGU - 17168. EGU General Assembly Conference Abstracts, Vienna, Austria, 2023. (2023)
Lagg, A.; Ishikawa, R.; Merenda, L.; Wiegelmann, T.; Tsuneta, S.; Solanki, S. K.: Internetwork Horizontal Magnetic Fields in the Quiet Sun Chromoshpere: Results from a Joint Hinode/VTT Study. In: The Second Hinode Science Meeting: Beyond Discovery - Torward Understanding, 327 (Eds. B., L.; M., C.; T., M.; J., M.; K., R.). (2009)
Raouafi, N.-E.; Solanki, S. K.; Wiegelmann, T.: Hanle Effect Diagnostics of the Coronal Magnetic Field: A Test Using Realistic Magnetic Field Configurations. In: Solar Polarization 5: In Honor of Jan Stenflo, pp. 429 - 434 (Eds. Berdyugina, S. V.; Nagendra, K. N.; Ramelli, R.). (2009)
Teriaca, L.; Wiegelmann, T.; Lagg, A.; Solanki, S. K.; Curdt, W.; Sekii, T.; the Team, H.: Loop morphology and flows and their relation to the magnetic field. In: First Results from Hinode, p. 196 (Eds. Matthews, S.; Davis, J. M.; Harra, L. K.). (2008)
Madjarska, M. S.; Wiegelmann, T.: Evolution of coronal hole boundaries seen in EIT 195 Å and TRACE 171 Å images. In: Modern Solar Facilities - Advanced Solar Science, pp. 249 - 252 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätverlag Göttingen (2007)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)
IMPRS alumn Yuto Bekki is given a honourable mention by the IAU Division E Sun and Heliosphere for his PhD thesis “Theory of solar oscillations in the inertial frequency range”