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)
Tian, H.; McIntosh, S. W.; Wang, T.; Ofman, L.; De Pontieu, B.; Innes, D. E.; Peter, H.: Persistent Doppler Shift Oscillations Observed with Hinode/EIS in the Solar Corona: Spectroscopic Signatures of Alfvénic Waves and Recurring Upflows. Astrophysical Journal 759, 144 (2012)
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.