Zhang, J.; Zhang, B.; Li, T.; Yang, S.; Zhang, Y.; Li, L.; Chen, F.; Peter, H.: Coronal Heating By the Interaction between Emerging Active Regions and the Quiet Sun Observed By the Solar Dynamics Observatory. Astrophysical Journal 799, L27 (2015)
Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: A model for the formation of the active region corona driven by magnetic flux emergence. Astronomy and Astrophysics 564, A12 (2014)
Li, L. P.; Peter, H.; Chen, F.; Zhang, J.: Conversion from mutual helicity to self-helicity observed with IRIS. Astronomy and Astrophysics 570, A93 (2014)
Tian, H.; DeLuca, E. E.; Cranmer, S. R.; De Pontieu, B.; Peter, H.; Martinez-Sykora, J.; Golub, L.; McKillop, S.; Reeves, K. K.; Miralles, M. P.et al.; McCauley, P.; Saar, S.; Testa, P.; Weber, M.; Murphy, N.; Lemen, J.; Title, A.; Boerner, P.; Hurlburt, N.; Tarbell, T. D.; Wuelser, J. P.; Kleint, L.; Kankelborg, C.; Jaeggli, S.; Carlsson, M.; Hansteen, V.; McIntosh, S. W.: Prevalence of small-scale jets from the networks of the solar transition region and chromosphere. Science 346 (6207), 1255711 (2014)
Tian, H.; Kleint, L.; Peter, H.; Weber, M.; Testa, P.; DeLuca, E.; Golub, L.; Schanche, N.: Observations of Subarcsecond Bright Dots in the Transition Region above Sunspots with the Interface Region Imaging Spectrograph. Astrophysical Journal 790 (2), L29 (2014)
Bourdin, P.-A.; Bingert, S.; Peter, H.: Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region. Astronomy and Astrophysics 555, A123 (2013)
Peter, H.; Bingert, S.; Klimchuk, J. A.; de Forest, C.; Cirtain, J. W.; Golub, L.; Winebarger, A. R.; Kobayashi, K.; Korreck, K. E.: Structure of solar coronal loops: from miniature to large-scale. Astronomy and Astrophysics 556, A104 (2013)
van Wettum, T.; Bingert, S.; Peter, H.: Parameterisation of coronal heating: spatial distribution and observable consequences. Astronomy and Astrophysics 554, A39 (2013)
Wang, X.; McIntosh, S. W.; Curdt, W.; Tian, H.; Peter, H.; Xia, L.-D.: Temperature dependence of ultraviolet line parameters in network and internetwork regions of the quiet Sun and coronal holes. Astronomy and Astrophysics 557, A126 (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)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
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).