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)
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.; Inhester, B.; Mierla, M.: Comparisons of CME Morphological Characteristics Derived from Five 3D Reconstruction Methods. Solar Physics 282 (1), pp. 221 - 238 (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)
Kramar, M.; Inhester, B.; Lin, H.; Davila, J.: Vector Tomography for the Coronal Magnetic Field. II. Hanle Effect Measurements. Astrophysical Journal 775 (1), 25 (2013)
Kumar, P.; Innes, D. E.; Inhester, B.: Solar Dynamics Observatory/Atmospheric Imaging Assembly Observations of a Reflecting Longitudinal Wave in a Coronal Loop. Astrophysical Journal 779 (1), L7 (2013)
Mierla, M.; Seaton, D. B.; Berghmans, D.; Chifu, I.; De Groof, A.; Inhester, B.; Rodriguez, L.; Stenborg, G.; Zhukov, A. N.: Study of a Prominence Eruption using PROBA2/SWAP and STEREO/EUVI Data. Solar Physics 286, pp. 241 - 253 (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)
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)
Feng, L.; Inhester, B.; Wei, Y.; Gan, W. Q.; Zhang, T. L.; Wang, M. Y.: Morphological Evolution of a Three-Dimensional Coronal Mass Ejection Cloud Reconstructed from Three Viewpoints. Astrophysical Journal 751 (1), 18 (2012)
Innes, D. E.; Cameron, R. H.; Fletcher, L.; Inhester, B.; Solanki, S. K.: Break up of returning plasma after the 7 June 2011 filament eruption by Rayleigh-Taylor instabilities. Astronomy and Astrophysics 540, L10 (2012)
Tadesse, T.; Wiegelmann, T.; Inhester, B.; Pevtsov, A.: Magnetic Connectivity Between Active Regions 10987, 10988, and 10989 by Means of Nonlinear Force-Free Field Extrapolation. Solar Physics 277, pp. 119 - 130 (2012)
Tadesse, T.; Wiegelmann, T.; Inhester, B.; Pevtsov, A.: Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and Its Surroundings. Solar Physics 281, pp. 53 - 65 (2012)
Wiegelmann, T.; Thalmann, J. K.; Inhester, B.; Tadesse, T.; Sun, X.; Hoeksema, J. T.: How Should One Optimize Nonlinear Force-Free Coronal Magnetic Field Extrapolations from SDO/HMI Vector Magnetograms? Solar Physics 281, pp. 37 - 51 (2012)
Mierla, M.; Chifu, I.; Inhester, B.; Rodriguez, L.; Zhukov, A.: Low polarised emission from the core of coronal mass ejections. Astronomy and Astrophysics 530, L1 (2011)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.