Budde, G.; Tissot, F. L.H.; Kleine, T.; Marquez, R. T.: Spurious molybdenum isotope anomalies resulting from non-exponential mass fractionation. Geochemistry (2023)
Pape, J.; Zhang, B.; Spitzer, F.; Rubin, A. E.; Kleine, T.: Isotopic constraints on genetic relationships among group IIIF iron meteorites, Fitzwater Pass, and the Zinder pallasite. Meteoritics & Planetary Science, pp. 1 - 11 (2023)
Schneider, J. M.; Burkhardt, C.; Kleine, T.: Distribution of s-, r-, and p-process Nuclides in the Early Solar System Inferred from Sr Isotope Anomalies in Meteorites. The Astrophysical Journal 952, p. L25 (2023)
Windmill, R. J.; Franchi, I. A.; Hellmann, J. L.; Schneider, J. M.; Fridolin, S.; Kleine, T.; Greenwood, R. C.; Anand, M.: Isotopic evidence for pallasite formation by impact mixing of olivine and metal during the first 10 million years of the Solar System. PNAS Nexus 1 (1) (2022)
Budde, G.; Archer, G. J.; Tissot, F. L. H.; Kleine, T.; Tappe, S.: Origin of the analytical 183W effect and its implications for tungsten isotope analyses. Journal of Analytical Atomic Spectrometry (2022)
Burkhardt, C.; Spitzer, F.; Morbidelli, A.; Budde, G.; Render, J. H.; Kruijer, T. S.; Kleine, T.: Terrestrial planet formation from lost inner solar system material. Science Advances (2022)
Fridolin, S.; Burkhardt, C.; Pape, J.; Kleine, T.: Collisional mixing between inner and outer solar system planetesimals inferred from the Nedagolla iron meteorite. Meteoritics and Planetary Science 57, pp. 261 - 276 (2022)
Kruijer, T. S.; Burkhardt, C.; Borg, L. E.; Kleine, T.: Tungsten and molybdenum isotopic evidence for an impact origin of pallasites. Earth and Planetary Science Letters 584, p. 117440 (2022)
Morbidelli, A.; Baillié, K.; Batygin, K.; Charnoz, S.; Guillot, T.; Rubie, D. C.; Kleine, T.: Contemporary formation of early Solar System planetesimals at two distinct radial locations. Nature Astronomy 6, pp. 72 - 79 (2022)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".