Chen, Y.; Peter, H.; Przybylski, D.; Tian, H.; Zhang, J.: Doppler shifts of spectral lines formed in the solar transition region and corona. Astronomy and Astrophysics 661, p. A94 (2022)
Chen, Y.; Przybylski, D.; Peter, H.; Tian, H.; Auchère, F.; Berghmans, D.: Transient small-scale brightenings in the quiet solar corona: A model for campfires observed with Solar Orbiter. Astronomy and Astrophysics 656, L7 (2021)
Rempel, M.; Przybylski, D.: Efficient Numerical Treatment of Ambipolar and Hall Drift as Hyperbolic System. The Astrophysical Journal 923, p. 79 (2021)
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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.