Strassmeier, K. G.; Ilyin, I.; Keles, E.; Mallonn, M.; Järvinen, A.; Weber, M.; Mackebrandt, F.; Hill, J. M.: High-resolution spectroscopy and spectropolarimetry of the total lunar eclipse January 2019. Astronomy and Astrophysics 635, A156 (2020)
Mackebrandt, F.; Mallonn, M.; Ohlert, J. M.; Granzer, T.; Lalitha, S.; Muñoz, A. G.; Gibson, N. P.; Lee, J. W.; Sozzetti, A.; Turner, J. D.et al.; Vaňko, M.; Strassmeier, K. G.: Transmission spectroscopy of the hot Jupiter TrES-3 b: Disproof of an overly large Rayleigh-like feature. Astronomy and Astrophysics 608, A26 (2017)
Mackebrandt, F.: Phantastische Welten und wie sie zu finden sind. Max Planck geht zur Schule, Theodor-Heuss-Gymnasium und Felix-Klein-Gymnasium Göttingen, Göttingen (2021)
Mackebrandt, F.: The stellar pulsation timing method to detect sub-stellar companions. Virtual Annual Meeting of the Astronomische Gesellschaft 2021
, Online (2021)
Mackebrandt, F.; Schuh, S.; Silvotti, R.: The EXOTIME project: Using the stellar pulsation timing method to detect sub-stellar companions. Virtual Annual Meeting of the Astronomische Gesellschaft 2020
(2020)
Mackebrandt, F.; Schuh, S.; Silvotti, R.: The stellar pulsation timing method to detect substellar companions. Annual Meeting of the Astronomische Gesellschaft 2017 , Splinter HotStars, Göttingen, Germany (2017)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing method to detect substellar companions. Planets Days Workshop, IAU General Assembly 2018, Vienna, Austria (2018)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing detection method for substellar companions. The PLATO Mission Conference 2017: Exoplanetary systems in the PLATO era, Warwick, UK (2017)
Mackebrandt, F.: The stellar pulsation timing method to detect substellar companions. 2nd Advanced School on Exoplanetary Science, Vietri sul Mare, Italy (2017)
Mackebrandt, F.; Schuh, S.: The stellar pulsation timing detection method for substellar companions. Planetary Systems Beyond The Main Sequence II, Technion, Haifa, Israel (2017)
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, ...