Su, J. T.; Jing, J.; Wang, S.; Wiegelmann, T.; Wang, H. M.: Statistical Study of Free Magnetic Energy and Flare Productivity of Solar Active Regions. Astrophysical Journal 788 (2), 150 (2014)
Tadesse, T.; Pevtsov, A. A.; Wiegelmann, T.; MacNeice, P. J.; Gosain, S.: Global Solar Free Magnetic Energy and Electric Current Density Distribution of Carrington Rotation 2124. Solar Physics 289, pp. 4031 - 4045 (2014)
Tadesse, T.; Wiegelmann, T.; Gosain, S.; MacNeice, P.; Pevtsov, A. A.: First use of synoptic vector magnetograms for global nonlinear, force-free coronal magnetic field models. Astronomy and Astrophysics 562, A105 (2014)
Tadesse, T.; Wiegelmann, T.; MacNeice, P. J.; Inhester, B.; Olson, K.; Pevtsov, A.: A Comparison Between Nonlinear Force-Free Field and Potential Field Models Using Full-Disk SDO/HMI Magnetogram. Solar Physics 289 (3), pp. 831 - 845 (2014)
Thalmann, J. K.; Tiwari, S. K.; Wiegelmann, T.: Force-free Field Modeling of Twist and Braiding-induced Magnetic Energy in an Active-region Corona. Astrophysical Journal 780 (1), 102 (2014)
Vemareddy, P.; Wiegelmann, T.: Quasi-static Three-dimensional Magnetic Field Evolution in Solar Active Region NOAA 11166 Associated with an X1.5 Flare. Astrophysical Journal 792 (10), 40 (2014)
Zhao, J.; Li, H.; Pariat, E.; Schmieder, B.; Guo, Y.; Wiegelmann, T.: Temporal Evolution of the Magnetic Topology of the NOAA Active Region 11158. Astrophysical Journal 787 (1), 88 (2014)
de Patoul, J.; Inhester, B.; Feng, L.; Wiegelmann, T.: 2D and 3D Polar Plume Analysis from the Three Vantage Positions of STEREO/EUVI A, B, and SOHO/EIT. Solar Physics 283, pp. 207 - 225 (2013)
Feng, L.; Wiegelmann, T.; Su, Y.; Inhester, B.; Li, Y. P.; Sun, X. D.; Gan, W. Q.: Magnetic Energy Partition between the Coronal Mass Ejection and Flare from AR 11283. Astrophysical Journal 765, 37 (2013)
Liu, C.; Deng, N.; Lee, J.; Wiegelmann, T.; Moore, R. L.; Wang, H.: Evidence for Solar Tether-Cutting Magnetic Reconnection from Coronal Field Extrapolations. Astrophysical Journal 778 (2), L36 (2013)
Nickeler, D. H.; Karlicky, M.; Wiegelmann, T.; Kraus, M.: Fragmentation of electric currents in the solar corona by plasma flows. Astronomy and Astrophysics 556, A61 (2013)
Shen, J.; Ji, H.; Wiegelmann, T.; Inhester, B.: Double Power-law Distribution of Magnetic Energy in the Solar Corona over an Active Region. Astrophysical Journal 764, 86 (2013)
Tadesse, T.; Wiegelmann, T.; MacNeice, P. J.; Olson, K.: Modeling coronal magnetic field using spherical geometry: cases with several active regions. Astrophysics and Space Science 347 (1), pp. 21 - 27 (2013)
Thalmann, J. K.; Tiwari, S. K.; Wiegelmann, T.: Comparison of force-free coronal magnetic field modeling using vector fields from Hinode and Solar Dynamics Observatory. Astrophysical Journal 769, pp. 59 - 68 (2013)
Wiegelmann, T.; Solanki, S. K.; Borrero, J. M.; Peter, H.; Barthol, P.; Gandorfer, A.; Martínez Pillet, V.; Schmidt, W.; Knölker, M.: Evolution of the Fine Structure of Magnetic Fields in the Quiet Sun: Observations from Sunrise/IMaX and Extrapolations. Solar Physics 283, pp. 253 - 272 (2013)
Chifu, I.; Inhester, B.; Mierla, M.; Chifu, V.; Wiegelmann, T.: First 4D Reconstruction of an Eruptive Prominence Using Three Simultaneous View Directions. Solar Physics 281, pp. 121 - 135 (2012)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.