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)
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)
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)
Guo, L.-J.; Huang, Y.-M.; Bhattacharjee, A.; Innes, D. E.: Rayleigh-Taylor Type Instabilities in the Reconnection Exhaust Jet as a Mechanism for Supra-Arcade Downflows in the Sun. Astrophysical Journal 796 (2), L29 (2014)
Innes, D. E.; Guo, L.-J.; Bhattacharjee, A.; Huang, Y.-M.; Schmit, D.: Observations of Supra-Arcade Fans: Instabilities at the Head of Reconnection Jets. Astrophysical Journal 796 (1), 27 (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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...