Bučík, R.; Innes, D.; Mason, G. M.; Wiedenbeck, M. E.; Gómez-Herrero, R.; Nitta, N. V.: 3He-rich Solar Energetic Particles in Helical Jets on the Sun. The Astrophysical Journal 852, 76 (2018)
Attie, R.; Innes, D. E.; Solanki, S. K.; Glassmeier, K.-H.: Relationship between supergranulation flows, magnetic cancellation and network flares. Astronomy and Astrophysics 596, A15 (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Energy spectra of 3He-rich solar energetic particles associated with coronal waves. J. Phys.: Conf. Ser. 767, 012002 (2016)
Bučík, R.; Innes, D. E.; Mason, G. M.; Wiedenbeck, M. E.: Association of 3He-rich solar energetic particles with large-scale coronal waves. Astrophysical Journal 833, 63 (2016)
Innes, D. E.; Bučík, R.; Guo, L.-J.; Nitta, N.: Observations of solar X-ray and EUV jets and their related phenomena. Astron. Nachrichten 337, pp. 1024 - 1032 (2016)
Innes, D. E.; Heinrich, P.; Inhester, B.; Guo, L.-J.: Analysis of UV and EUV emission from impacts on the Sun after 2011 June 7 eruptive flare. Astronomy and Astrophysics 592, A17 (2016)
Kumar, P.; Innes, D. E.; Cho, K.-S.: Flare-Generated Shock Wave Propagation Through Solar Coronal Arcade Loops and an Associated Type II Radio Burst. Astrophysical Journal 828 (1), 28 (2016)
Mason, G. M.; Nitta, N. V.; Wiedenbeck, M. E.; Innes, D. E.: Evidence for a Common Acceleration Mechanism for Enrichments of He-3 And Heavy Ions in Impulsive SEP Events. Astrophysical Journal 823 (2), 138 (2016)
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. Journal of Physics: Conference Series 642, 012002 (2015)
Bučík, R.; Innes, D. E.; Guo, L.; Mason, G. M.; Wiedenbeck, M. E.: Observations of EUV waves in 3He-rich solar energetic particle events. Astrophysical Journal 812 (1), 53 (2015)
Chen, N.-H.; Bučík, R.; Innes, D. E.; Mason, G. M.: Case studies of multi-day 3He-rich solar energetic particle periods. Astronomy and Astrophysics 580, A16 (2015)
Innes, D.; Guo, L.; Huang, Y.-M.; Bhattacharjee, A.: IRIS Si IV Line Profiles: An Indication for the Plasmoid Instability During Small-scale Magnetic Reconnection on the Sun. Astrophysical Journal 813, pp. 86 - 96 (2015)
Kumar, P.; Innes, D.: Partial Reflection and Trapping of a Fast-mode Wave in Solar Coronal Arcade Loops. Astrophysical Journal 803, pp. L23 - L29 (2015)
Panesar, N.; Sterling, A.; Innes, D.; Moore, R.: Destabilization of a Solar Prominence/Filament Field System by a Series of Eight Homologous Eruptive Flares Leading to a CME. Astrophysical Journal 811, pp. 5 - 15 (2015)
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".