Bučík, R.; Innes, D.E.; Mason, G.M.; Wiedenbeck, M.E.; Gómez-Herrero, R.; Nitta, N.V.: Evidence for Alfvén Waves in Source Flares of Impulsive Solar Energetic Particle Events. AGU Fall Meeting, New Orleans, LA, USA (2017)
Chen, N.-H.; Bučík, R.; Kim, R. S.: Temperature of source regions of 3He-rich impulsive solar energetic particle events. ISEST/MiniMax 2017 Workshop, Jeju, Republic of Korea (2017)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Association of impulsive solar energetic particle events with large-scale coronal waves. AGU Fall Meeting, San Francisco, USA (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Large-scale Coronal Waves in 3He-rich Solar Energetic Particle Events. 15th Annual International Astrophysics Conference, The Science of Ed Stone: Celebrating his 80th Birthday, Cape Coral, USA (2016)
Bučík, R.: STEREOscopic observations of energetic particle sources in the inner heliosphere. NASA/Goddard Space Flight Center Seminar, Greenbelt, MD, USA (2015)
Bučík, R.: The origin of impulsive solar flare energetic ions. Meeting of the Evaluation Committee of the Marie Curie Program SASPRO, Bratislava, Slovakia (2015)
Bučík, R.; Innes, D. E.; Chen, N.-H.; Mason, G. M.; Gomez-Herrero, R.; Wiedenbeck, M. E.: Long-lived energetic ion sources on the Sun. STEREO/SOHO team meeting, Alcala de Henares, Spain (2015)
Bučík, R.; Innes, D. E.; Chen, N.-H.; Mason, G. M.; Gomez-Herrero, R.; Wiedenbeck, M. E.: Long-lived energetic particle source regions on the Sun. 14th Annual International Astrophysics Conference, Tampa, USA (2015)
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)
Kecskemety, K.; Zeldovich, M.; Logachev, Y.; Bučík, R.: Suprathermal ions 3He, 4He, C, O, Fe in solar wind particle fluxes at 1 AU in solar cycles 23 and 24. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Bučík, R.; Wiedenbeck, M.E.; Gómez-Herrero, R.; Mason, G.M.; Nitta, N.V.: 3He-rich Solar Energetic Particles from Sunspot Jets. AGU Fall Meeting, Washington D.C., USA (2018)
Heber, B.; Kuehl, P.; Wraase, S.; Böttcher, S.; Bučík, R.; Dresing, N.; Gómez-Herrero, R.; Klassen, A.; Müller-Mellin, R.: Interpretation of increased solar energetic particle ux measurements with SEPT aboard the STEREO spacecraft and contamination. Particle Acceleration and Transport: From the Sun to the Extragalactic sources, Universita della Calabria, Rende, Italy (2018)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".