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)
Schühle, U.; Halain, J.-P.; Meining, S.; Teriaca, L.: The Lyman-alpha telescope of the extreme ultraviolet imager on Solar Orbiter. Proceedings of the SPIE 8148, 81480K (2011)
Gupta, G. R.; Banerjee, D.; Teriaca, L.; Imada, S.; Solanki, S.: Accelerating Waves in Polar Coronal Holes as Seen by EIS and SUMER. Astrophysical Journal 718 (1), pp. 11 - 22 (2010)
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, ...