Bhatia, T. S.; Cameron, R.; Peter, H.; Solanki, S.: Small-scale dynamo in cool stars. III. Changes in the photospheres of F3V to M0V stars. Astronomy and Astrophysics 681, p. A32 (2024)
Breu, C. A.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society (2024)
Breu, C.; Peter, H.; Solanki, S. K.; Cameron, R.; De Moortel, I.: Non-thermal broadening of coronal lines in a 3D MHD loop model. Monthly Notices of the Royal Astronomical Society 530, pp. 2361 - 2377 (2024)
Chen, Y.; Mandal, S.; Peter, H.; Chitta, L. P.: Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI. Astronomy and Astrophysics 692, p. A119 (2024)
Chitta, L. P.; Zhukov, A. N.; Berghmans, D.; Peter, H.; Parenti, S.; Mandal, S.; Aznar Cuadrado, R.; Schühle, U.; Teriaca, L.; Auchère, F.et al.; Barczynski, K.; Buchlin, É.; Harra, L.; Kraaikamp, E.; Long, D. M.; Rodriguez, L.; Schwanitz, C.; Smith, P. J.; Verbeeck, C.; Seaton, D. B.: Picoflare jets power the solar wind emerging from a coronal hole on the Sun. Science 38, pp. 867 - 872 (2023)
Baker, D.; Démoulin, P.; Yardley, S. L.; Mihailescu, T.; van Driel-Gesztelyi, L.; D'Amicis, R.; Long, D. M.; To, A. S. H.; Owen, C. J.; Horbury, T. S.et al.; Brooks, D. H.; Perrone, D.; French, R. J.; James, A. W.; Janvier, M.; Matthews, S.; Stangalini, M.; Valori, G.; Smith, P.; Aznar Cuadrado, R.; Peter, H.; Schühle, U.; Harra, L.; Barczynski, K.; Berghmans, D.; Zhukov, A. N.; Rodriguez, L.; Verbeeck, C.: Observational Evidence of S-web Source of the Slow Solar Wind. The Astrophysical Journal 950, p. 65 (2023)
Cheng, X.; Xing, C.; Aulanier, G.; Solanki, S. K.; Peter, H.; Ding, M. D.: Deciphering the Slow-rise Precursor of a Major Coronal Mass Ejection. The Astrophysical Journal 954, p. L47 (2023)
Li, Z.; Cheng, X.; Ding, M. D.; Chitta, L. P.; Peter, H.; Berghmans, D.; Smith, P. J.; Auchère, F.; Parenti, S.; Barczynski, K.et al.; Harra, L.; Schühle, U.; Buchlin, É.; Verbeeck, C.; Aznar Cuadrado, R.; Zhukov, A. N.; Long, D. M.; Teriaca, L.; Rodriguez, L.: Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUI. Astronomy and Astrophysics 673, p. A83 (2023)
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, ...