Bučík, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R.: Long-lasting 3He-rich solar energetic particle sources. STEREO SEP meeting, Laurel, Maryland, USA (2014)
Bučík, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E.: Observations of a blast EUV wave in 3He-rich solar energetic particle sources. 14th Annual International Astrophysics Conference, Tampa, USA (2015)
Park, J.; Innes, D. E.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: Study of solar energetic particle associations with extreme-ultraviolet waves. The 3rd Asia-Pacific Solar Physics Meeting, Seoul, Rep. of Korea (2015)
Chen, N.-H.; Bučík, R.; Innes, D. E.; Mason, G. M.: The relation between solar jets and 3He-rich solar energetic particle events at 1 AU. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Park, J.; Innes, D.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: The study of solar energetic protons associated with EUV waves. 224th AAS Meeting, Boston, MA, USA (2014)
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.