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Albert, K.; Hirzberger, J.; Busse, D.; Lange, T.; Kolleck, M.; Fiethe, B.; Suárez, D. O.; Woch, J.; Schou, J.; Rodriguez, J. B.et al.; Gandorfer, A. M.; Guan, Y.; Carrascosa, J. P. C.; Expósito, D. H.; Iniesta, J. C. d. T.; Solanki, S. K.; Michalik, H.: Autonomous on-board data processing and instrument calibration software for the SO/PHI. In: Proceedings Software and Cyberinfrastructure for Astronomy V, Vol. 10707, 107070O. SPIE Astronomical Telescopes + Instrumentation 2018, Austin, Texas, USA. (2018)
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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.
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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.