Wilhelm, K.; Cosmovici, C. B.; Delamere, W. A.; Huebner, W. F.; Keller, H. U.; Reitsema, H.; Schmidt, H. U.; Whipple, F. L.: A three-dimensional model of the nucleus of Comet Halley. In: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet, pp. 367 - 369 (Eds. Battrick, B.; Rolfe, E. J.; Reinhard, R.). ESA Publ. Div., Noordwijk (1986)
Wilhelm, K.: Quantitative Spectroscopy of the Solar Atmosphere. Dynamic Sun: I. MHD Waves and Confined Transients in the Magnetised Atmosphere, Varanasi, India (2016)
Wilhelm, K.: Bhola N. Dwivedi - 25 Years of Cooperation with SUMER. Dynamic Sun: I. MHD Waves and Confined Transients in the Magnetised Atmosphere, Varanasi, India (2016)
Rao, Y. K.; Kayshap, P.; Srivastava, A. K.; Wilhelm, K.; Dwivedi, B. N.: Multi-line Spectroscopic Analyses of the Dynamical Cool Loops Using Interface Region Imaging Spectrometer (IRIS) Observations. IAU Symposia 340: Long-term datasets for the understanding of solar and stellar magnetic cycles, Jaipur, India (2018)
Wilhelm, K.; Marsch, E.; Dwivedi, B.; Feldman, U.: Observations of the Sun at vacuumu-ultravioletwavelengths form space. Part II: Results and interpretations. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (2007)
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.