Matković, F.; Brajša, R.; Temmer, M.; Heinemann, S. G.; Ludwig, H.-G.; Saar, S. H.; Selhorst, C. L.; Skokić, I.; Sudar, D.: Differences in physical properties of coronal bright points and their ALMA counterparts within and outside coronal holes. Astronomy and Astrophysics 670, p. A146 (2023)
Milošić, D.; Temmer, M.; Heinemann, S. G.; Podladchikova, T.; Veronig, A.; Vršnak, B.: Improvements to the Empirical Solar Wind Forecast (ESWF) model. Solar Physics 298, p. 45 (2023)
Hofmeister, S. J.; Asvestari, E.; Guo, J.; Heidrich-Meisner, V.; Heinemann, S. G.; Magdalenic, J.; Poedts, S.; Samara, E.; Temmer, M.; Vennerstrom, S.et al.; Veronig, A.; Vršnak, B.; Wimmer-Schweingruber, R.: How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth: An analytical model. Astronomy and Astrophysics 659, p. A190 (2022)
Inceoglu, F.; Shprits, Y. Y.; Heinemann, S. G.; Bianco, S.: Identification of Coronal Holes on AIA/SDO Images Using Unsupervised Machine Learning. The Astrophysical Journal 930, p. 118 (2022)
Samara, E.; Magdalenić, J.; Rodriguez, L.; Heinemann, S. G.; Georgoulis, M. K.; Hofmeister, S. J.; Poedts, S.: Influence of coronal hole morphology on the solar wind speed at Earth. Astronomy and Astrophysics 662, p. A68 (2022)
Wagner, A.; Asvestari, E.; Temmer, M.; Heinemann, S. G.; Pomoell, J.: Validation scheme for solar coronal models: Constraints from multi-perspective observations in EUV and white light. Astronomy and Astrophysics 657, p. A117 (2022)
Geyer, P.; Temmer, M.; Guo, J.; Heinemann, S. G.: Properties of stream interaction regions at Earth and Mars during the declining phase of SC 24. Astronomy and Astrophysics 649, A80 (2021)
Heinemann, S. G.; Temmer, M.; Hofmeister, S. J.; Stojakovic, A.; Gizon, L.; Yang, D.: How to Estimate the Far-Side Open Flux Using STEREO Coronal Holes. Solar Physics 296, 141 (2021)
Jarolim, R.; Veronig, A. M.; Hofmeister, S.; Heinemann, S. G.; Temmer, M.; Podladchikova, T.; Dissauer, K.: Multi-channel coronal hole detection with convolutional neural networks. Astronomy and Astrophysics 652, A13 (2021)
Zhang, J.; Temmer, M.; Gopalswamy, N.; Malandraki, O.; Nitta, N. V.; Patsourakos, S.; Shen, F.; Vrsnak, B.; Wang, Y.; Webb, D.et al.; Desai, M. I.; Dissauer, K.; Dresing, N.; Dumbovic, M.; Feng, X.; Heinemann, S. G.; Laurenza, M.; Lugaz, N.; Zhuang, B.: Earth-affecting solar transients: a review of progresses in solar cycle 24. Progress in Earth and Planetary Science 8 (1), 56 (2021)
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, ...