Beck, C.; Fabbian, D.; Rezaei, R.; Puschmann, K. G.: The Polarization Signature of Photospheric Magnetic Fields in 3D MHD Simulations and Observations at Disk Center. Astrophysical Journal 842 (1), 37 (2017)
Fabbian, D.; Simoniello, R.; Collet, R.; Criscuoli, S.; Korhonen, H.; Krivova, N. A.; Olah, K.; Jouve, L.; Solanki, S. K.; Alvarado-Gomez, J. D.et al.; Booth, R.; Garcia, R. A.; Lehtinen, J.; See, V.: The variability of magnetic activity in solar-type stars. Astron. Nachrichten 338 (7), pp. 753 - 772 (2017)
Beck, C.; Rezaei, R.; Puschmann, K. G.; Fabbian, D.: Spectroscopy at the Solar Limb: II. Are Spicules Heated to Coronal Temperatures? Solar Physics 291 (8), pp. 2281 - 2328 (2016)
Doerr, H.-P.; Vitas, N.; Fabbian, D.: How different are the Liège and Hamburg atlases of the solar spectrum? Astronomy and Astrophysics 590, A118 (2016)
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.