Parenti, S.; del Zanna, G.; Petralia, A.; Reale, F.; Teriaca, L.; Testa, P.; Mason, H. E.: Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties. Astrophysical Journal 846 (1), 25 (2017)
Mandal, S.; Samanta, T.; Banerjee, D.; Krishna Prasad, S.; Teriaca, L.: Propagating disturbances along fan-like coronal loops in an active region. Research in Astronomy and Astrophysics 15 (11), pp. 1832 - 1842 (2015)
Pancrazzi, M.; Focardi, M.; Nicolini, G.; Andretta, V.; Uslenghi, M.; Magli, E.; Ricci, M.; Bemporad, A.; Spadaro, D.; Landini, F.et al.; Romoli, M.; Antonucci, E.; Fineschi, S.; Naletto, G.; Nicolosi, P.; Teriaca, L.: Hardware and software architecture on board solar orbiter/METIS: an update. Proceedings of the SPIE 9144, 91443F (2014)
Gupta, G. R.; Teriaca, L.; Marsch, E.; Solanki, S. K.; Banerjee, D.: Spectroscopic observations of propagating disturbances in a polar coronal hole: evidence of slow magneto-acoustic waves. Astronomy and Astrophysics 546, A93 (2012)
Kamio, S.; Curdt, W.; Teriaca, L.; Innes, D. E.: Evolution of microflares associated with bright points in coronal holes and in quiet regions. Astronomy and Astrophysics 529, A21 (2011)
Korendyke, C. M.; Teriaca, L.; Doschek, G. A.; Harra, L. K.; Schühle, U. H.; Shimizu, T.: LEMUR (Large European Module for solar Ultraviolet Research): a VUV imaging spectrograph for the JAXA Solar-C Mission. Proceedings of the SPIE 8148, p. 81480I-81480I-13 (2011)
The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.