Ying, B.; Feng, L.; Inhester, B.; Mierla, M.; Gan, W.; Lu, L.; Li, S.: Three-dimensional analyses of an aspherical coronal mass ejection and its driven shock. Astronomy and Astrophysics 660, p. A23 (2022)
Zhang, Q. M.; Ning, Z. J.; Guo, Y.; Zhou, T. H.; Cheng, X.; Ji, H. S.; Feng, L.; Wiegelmann, T.: Multiwavelength Observations of a Partially Eruptive Filament on 2011 September 8. Astrophysical Journal 805, 4, pp. 1 - 18 (2015)
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)
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)
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)
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)
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, ...